{"paper_id": "prb10", "title": "Study of the doubly charmed tetraquark T_cc+", "text": "Study of the doubly charmed tetraquark \\( T_{cc}^+ \\)\n\nLHCb collaboration†\n\nAbstract\nAn exotic narrow state in the D\\( ^0 \\)D\\( ^0 \\)\\( \\pi^+ \\) mass spectrum just below the D\\( ^*+ \\)D\\( ^0 \\) mass threshold is studied using a data set corresponding to an integrated luminosity of 9\\( \\mathrm{fb}^{-1} \\) acquired with the LHCb detector in proton-proton collisions at centre-of-mass energies of 7, 8 and 13 TeV. The state is consistent with the ground isoscalar \\( T_{cc}^+ \\) tetraquark with a quark content of cc\\( \\overline{u} \\)d and spin-parity quantum numbers \\( J^P = 1^+ \\). Study of the DD mass spectra disfavours interpretation of the resonance as the isovector state. The decay structure via intermediate off-shell D\\( ^*+ \\) mesons is confirmed by the D\\( ^0 \\)\\( \\pi^+ \\) mass distribution. The mass of the resonance and its coupling to the D\\( ^* \\)D system are analysed. Resonance parameters including the pole position, scattering length, effective range and compositeness are measured to reveal important information about the nature of the \\( T_{cc}^+ \\) state. In addition, an unexpected dependence of the production rate on track multiplicity is observed.\n\n†Authors are listed at the end of this paper.\nIntroduction\n\nHadrons with quark content other than that seen in mesons (q_1\\bar{q}_2) and baryons (q_1q_2q_3) have been actively discussed since the birth of the quark model [1–5]. Since the discovery of the \\( \\chi_c(3872) \\) state [6] many tetraquark and pentaquark candidates listed in Table 1 have been observed. For all but the X_0(2900) and X_1(2900) states the minimal quark content implies the presence of either a c\\bar{c} or b\\bar{b} quark-antiquark pair. The masses of many tetra- and pentaquark states are close to mass thresholds, *e.g.* D^{(*)}\\overline{D}^{(*)} or B^{(*)}\\overline{B}^{(*)}, where D^{(*)} or B^{(*)} represents a hadron containing a charm or beauty quark, respectively. Therefore, these states are likely to be hadronic molecules [7–10] where colour-singlet hadrons are bound by residual nuclear forces, such as the exchange of a pion or \\( \\rho \\) meson [11], similar to electromagnetic van der Waals forces attracting electrically neutral atoms and molecules. These states are expected to have a spatial extension significantly larger than a typical compact hadron. Conversely, the only hadron currently observed that contains a pair of cc quarks is the \\( \\Xi_{cc}^{++} \\) (ccu) baryon, a long-lived, weakly-decaying compact object [12,13]. The recently observed X(6900) structure in the J/\\psiJ/\\psi mass spectrum [14] belongs to both categories simultaneously. Its proximity to the \\( \\chi_{c0}\\chi_{c1} \\) threshold could indicate a molecular structure [15,16]. Alternatively, it could be a compact object, where all four quarks are within one confinement volume and each quark interacts directly with the other three quarks via the strong force [17–20].\n\nThe existence and properties of Q_1Q_2\\bar{q}_1\\bar{q}_2 states with two heavy quarks and two light antiquarks have been widely discussed for a long time [45–50]. In the limit of large masses of the heavy quarks the corresponding ground state should be deeply bound. In this limit, the two heavy quarks Q_1Q_2 form a point-like color-antitriplet object,\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
StatesQuark content
X_0(2900), X_1(2900) [21,22]\\( \\bar{c}dus \\)
\\( \\chi_{c1}(3872) \\) [6]c\\bar{c}qq\\bar{q}
Z_c(3900) [23], Z_c(4020) [24,25], Z_c(4050) [26], X(4100) [27], Z_c(4200) [28], Z_c(4430) [29–32], R_{c0}(4240) [31]c\\bar{c}ud\\bar{d}
Z_{cs}(3985) [33], Z_{cs}(4000), Z_{cs}(4220) [34]c\\bar{c}u\\bar{s}
\\( \\chi_{c1}(4140) \\) [35–38], \\( \\chi_{c1}(4274) \\), \\( \\chi_{c0}(4500) \\), \\( \\chi_{c0}(4700) \\) [38], X(4630), X(4685) [34], X(4740) [39]c\\bar{c}s\\bar{s}
X(6900) [14]c\\bar{c}c\\bar{c}
Z_b(10610), Z_b(10650) [40]bbud
P_c(4312) [41], P_c(4380) [42], P_c(4440), P_c(4457) [41], P_c(4357) [43]ccuud
P_{cs}(4459) [44]c\\bar{c}uds
\n\nTable 1: Tetra- and pentaquark candidates and their plausible valence quark content.\nanalogous to an antiquark, and as a result the Q₁Q₂q₁q₂ system has similar degrees of freedom for its light quarks as an antibaryon with a single heavy quark, e.g. the \\( \\overline{\\Lambda}_c^0 \\) or \\( \\overline{\\Lambda}_b^0 \\) antibaryons. The beauty quark is considered heavy enough to sustain the existence of a bbūd state that is stable with respect to the strong and electromagnetic interactions with a mass of about 200 MeV below the BB* mass threshold. In the case of the bcūd and ccūd systems, there is currently no consensus in the literature whether such states exist and if their natural widths are narrow enough to allow for experimental observation. The theoretical predictions for the mass of the ccūd ground state with spin-parity quantum numbers J\\( ^P \\) = 1\\( ^+ \\) and isospin I = 0, denoted hereafter as T\\( _{cc}^+ \\), relative to the D*+D\\( ^0 \\) mass threshold\n\n\\[\n\\delta m \\equiv m_{T_{cc}^+} - (m_{D^{*+}} + m_{D^0})\n\\]\n\nlie in the range \\( -300 < \\delta m < 300 \\) MeV/\\( c^2 \\) [51–82], where \\( m_{D^{*+}} \\) and \\( m_{D^0} \\) denote the known masses of the D*+ and D\\( ^0 \\) mesons [83], with cūd and cū quark content, respectively. The observation of a narrow state in the D\\( ^0 \\)D\\( ^0 \\)π\\( ^+ \\) mass spectrum near the D*+D\\( ^0 \\) mass threshold, compatible with being a T\\( _{cc}^+ \\) tetraquark state with ccūd quark content is reported in Ref. [84]. In the work presented here, the properties of this state are studied by constructing a dedicated amplitude model that accounts for the D*+D\\( ^0 \\) and D*0D\\( ^+ \\) decay channels. In addition, the mass spectra of other DD(*) and opposite-sign DD(*) combinations are explored. Furthermore, production-related observables, such as the event multiplicity and transverse momentum (\\( p_T \\)) spectra that are sensitive to the internal structure of the state, are discussed. This analysis is based on proton-proton (pp) collision data, corresponding to integrated luminosity of 9 fb\\( ^{-1} \\), collected with the LHCb detector at centre-of-mass energies of 7, 8 and 13 TeV. The LHCb detector [85,86] is a single-arm forward spectrometer covering the pseudorapidity range 2 < \\( \\eta \\) < 5, designed for the study of particles containing b or c quarks and is further described in Methods.\n\n**T\\( _{cc}^+ \\) signal in the D\\( ^0 \\)D\\( ^0 \\)π\\( ^+ \\) mass spectrum**\n\nThe D\\( ^0 \\)D\\( ^0 \\)π\\( ^+ \\) final state is reconstructed using the D\\( ^0 \\) → K\\( ^- \\)π\\( ^+ \\) decay channel with two D\\( ^0 \\) mesons and a pion all produced promptly in the same pp collision. The selection criteria are similar to those used in Refs. [87–90] and described in detail in Methods. The background not originating from true D\\( ^0 \\) mesons is subtracted using an extended unbinned maximum-likelihood fit to the two-dimensional distribution of the masses of the two D\\( ^0 \\) candidates from selected D\\( ^0 \\)D\\( ^0 \\)π\\( ^+ \\) combinations, see Methods and Extended Data Fig. 1(a). The obtained D\\( ^0 \\)D\\( ^0 \\)π\\( ^+ \\) mass distribution for selected D\\( ^0 \\)D\\( ^0 \\)π\\( ^+ \\) combinations is shown in Fig. 1.\n\nAn extended unbinned maximum-likelihood fit to the D\\( ^0 \\)D\\( ^0 \\)π\\( ^+ \\) mass distribution is performed using a model consisting of signal and background components. The signal component corresponds to the T\\( _{cc}^+ \\)→ D\\( ^0 \\)D\\( ^0 \\)π\\( ^+ \\) decay and is described as the convolution of the natural resonance profile with the detector mass resolution function. A relativistic P-wave two-body Breit–Wigner function \\( \\mathcal{F}^{BW} \\) with a Blatt–Weisskopf form factor [91,92] is used in Ref. [84] as the natural resonance profile. That function, while sufficient to reveal the existence of the state, does not account for the resonance being in close vicinity of the D*D threshold. To assess the fundamental properties of resonances that are close to thresholds, advanced parametrisations ought to be used [93–103]. A unitarised Breit–Wigner profile \\( \\mathcal{F}^U \\), described in Methods Eq. (M9), is used in this analysis.\nFigure 1: Distribution of \\( D^0 D^0 \\pi^+ \\) mass. Distribution of \\( D^0 D^0 \\pi^+ \\) mass where the contribution of the non-D\\( ^0 \\) background has been statistically subtracted. The result of the fit described in the text is overlaid.\n\nThe function is built under two assumptions. Firstly, that the newly observed state has quantum numbers \\( J^P = 1^+ \\) and isospin \\( I = 0 \\) in accordance with the theoretical expectation for the \\( T_{cc}^+ \\) ground state. Secondly, that the \\( T_{cc}^+ \\) state is strongly coupled to the D*D channel. The derivation of \\( \\mathfrak{F}^U \\) relies on the isospin symmetry for \\( T_{cc}^+ \\to D^* D \\) decays and explicitly accounts for the energy dependency of the \\( T_{cc}^+ \\to D^0 D^0 \\pi^+ \\), \\( T_{cc}^+ \\to D^0 D^+ \\pi^0 \\) and \\( T_{cc}^+ \\to D^0 D^+ \\gamma \\) decay widths as required by unitarity. Similarly to the \\( \\mathfrak{F}^{BW} \\) profile, the \\( \\mathfrak{F}^U \\) function has two parameters: the peak location \\( m_U \\), defined as the mass value where the real part of the complex amplitude vanishes, and the absolute value of the coupling constant \\( g \\) for the \\( T_{cc}^+ \\to D^* D \\) decay.\n\nThe detector mass resolution, \\( \\mathcal{R} \\), is modelled with the sum of two Gaussian functions with a common mean, and parameters taken from simulation, see Methods. The widths of the Gaussian functions are corrected by a factor of 1.05, that accounts for a small residual difference between simulation and data [39, 104, 105]. The root mean square of the resolution function is around 400 keV/\\( c^2 \\).\n\nA study of the \\( D^0 \\pi^+ \\) mass distribution for selected \\( D^0 D^0 \\pi^+ \\) combinations in the region above the \\( D^{*0} D^+ \\) mass threshold and below 3.9 GeV/\\( c^2 \\) shows that approximately 90% of all\nTable 2: Signal yield, \\( N \\), and the resonance mass parameter with respect to the D*+D^0 mass threshold, \\( \\delta m_U \\), obtained from the fit with a model based on the \\( \\mathfrak{F}^U \\) signal profile. Uncertainties are statistical only.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
ParameterValue
\\( N \\)186 ± 24
\\( \\delta m_U \\)−359 ± 40 keV/\\( c^2 \\)
\\( |g| \\)\\( 3 \\times 10^4 \\) GeV (fixed)
\n\n\\( D^0 D^0 \\pi^+ \\) combinations contain a true D*+ meson. Therefore, the background component is parameterised with a product of the two-body phase space function \\( \\Phi_{D^*+D^0} \\) [106] and a positive polynomial function \\( P_n \\), convolved with the detector resolution function \\( \\mathcal{R} \\)\n\n\\[\nB_n = (\\Phi_{D^*+D^0} \\times P_n) * \\mathcal{R},\n\\]\n\nwhere \\( n \\) denotes the order of the polynomial function, \\( n = 2 \\) is used in the default fit.\n\nThe \\( D^0 D^0 \\pi^+ \\) mass spectrum with non-D^0 background subtracted is shown in Fig. 1 with the result of the fit using a model based on the \\( \\mathfrak{F}^U \\) signal profile overlaid. The signal yield, \\( N \\), and mass parameter relative to the D*+D^0 mass threshold, \\( \\delta m_U \\), are listed in Table 2. The statistical significances of the observed \\( T_{cc}^+ \\to D^0 D^0 \\pi^+ \\) signal and for the \\( \\delta m_U < 0 \\) hypothesis are determined using Wilks’ theorem to be 22 and 9 standard deviations, respectively.\n\nThe width of the resonance is determined by the coupling constant \\( g \\) for small values of \\( |g| \\). With increasing \\( |g| \\), the width increases to an asymptotic value determined by the width of the D*+ meson, see Methods and Extended Data Fig. 7. In this regime of large \\( |g| \\), the \\( \\mathfrak{F}^U \\) signal profile exhibits a scaling property similar to the Flatté function [104,107,108]. The parameter \\( |g| \\) effectively decouples from the fit model, and the model resembles the scattering-length approximation [94]. The likelihood profile for the parameter \\( |g| \\) is shown in Fig. 2, where one can see a plateau at large values. At small values of the \\( |g| \\) parameter, \\( |g| < 1 \\) GeV, the likelihood function is independent of \\( |g| \\) because the resonance is too narrow for the details of the \\( \\mathfrak{F}^U \\) signal profile to be resolved by the detector. The lower limits on the \\( |g| \\) parameter of \\( |g| > 7.7 \\) (6.2) GeV at 90 (95)% confidence level (CL) are obtained as the values where the difference in the negative log-likelihood \\( -\\Delta \\log \\mathcal{L} \\) is equal to 1.35 and 1.92, respectively. Smaller values for \\( |g| \\) are further used for systematic uncertainty evaluation.\n\nThe modes relative to the D*+D^0 mass threshold, \\( \\delta m \\), and the full widths at half maximum (FWHM), \\( \\Gamma \\), for the \\( \\mathfrak{F}^{BW} \\) and \\( \\mathfrak{F}^U \\) signal profiles are compared in Table 3 and appear to be rather different. To check the consistency of these seemingly contradictory results, pseudoexperiments are generated with a model based on the \\( \\mathfrak{F}^U \\) signal profile and analysed with a model based on the \\( \\mathfrak{F}^{BW} \\) signal profile. Each pseudoexperiment is generated using the parameters obtained from the fit to data and accounting for detector resolution and background. The obtained mean and root mean square (RMS) values for the parameters \\( \\delta m_{BW} \\) and \\( \\Gamma_{BW} \\) are shown in Table 4. In a similar way, an ensemble of pseudoexperiments generated with a model based on the \\( \\mathfrak{F}^{BW} \\) signal profile is analysed with a model based on the \\( \\mathfrak{F}^U \\) signal profile and the obtained mean and RMS values for the parameter \\( \\delta m_U \\) are reported in Table 4. The largest discrepancy between the values\n![Likelihood profile for the |g| parameter. Likelihood profile for the absolute value of the coupling constant g from the fit to the background-subtracted D^0D^0\\pi^+ mass spectrum with a model based on the \\( \\mathcal{F}^U \\) signal profile.](page_186_234_1207_654.png)\n\nFigure 2: Likelihood profile for the |g| parameter. Likelihood profile for the absolute value of the coupling constant g from the fit to the background-subtracted D^0D^0\\pi^+ mass spectrum with a model based on the \\( \\mathcal{F}^U \\) signal profile.\n\nTable 3: Mode relative to the D^{*+}D^0 mass threshold, \\( \\delta m \\), and FWHM, \\( \\mathfrak{w} \\), for the \\( \\mathcal{F}^U \\) and \\( \\mathcal{F}^{BW} \\) signal profiles. Uncertainties are statistical only.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
\\( \\delta m \\) [keV/c^2]\\( \\mathfrak{w} \\) [keV/c^2]
\\( \\mathcal{F}^{BW} \\)−279 ± 59409 ± 163
\\( \\mathcal{F}^U \\)−361 ± 4047.8 ± 1.9
\n\nin Table 4 and those from Table 2 and Ref. [84] is less than one standard deviation for the parameter \\( \\Gamma_{BW} \\). This demonstrates that the results obtained with the \\( \\mathcal{F}^{BW} \\) and \\( \\mathcal{F}^U \\) signal profiles are consistent, taking into account the detector resolution and background.\nTable 4: Mean and root mean square (RMS) values for the \\( \\delta m_{\\mathrm{BW}} \\), \\( \\Gamma_{\\mathrm{BW}} \\) and \\( \\delta m_{\\mathrm{U}} \\) parameters obtained from pseudoexperiments produced as a consistency check.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
ParameterPseudoexperimentsData
meanRMS
\\( \\delta m_{\\mathrm{BW}} \\)[keV/\\( c^2 \\)]−30150−273 ± 61 [84]
\\( \\Gamma_{\\mathrm{BW}} \\)[keV]222121410 ± 165
\\( \\delta m_{\\mathrm{U}} \\)[keV/\\( c^2 \\)]−37846−359 ± 40
\n\nSystematic uncertainties\n\nSystematic uncertainties for the \\( \\delta m_{\\mathrm{U}} \\) parameter are summarised in Table 5 and described in greater detail below. The systematic uncertainty related to the fit model is studied using pseudoexperiments with a set of alternative parameterisations. For each alternative model an ensemble of pseudoexperiments is performed with parameters obtained from a fit to data. A fit with the baseline model is performed to each pseudoexperiment, and the mean values of the parameters of interest are evaluated over the ensemble. The absolute values of the differences between these mean values and the corresponding parameter values obtained from the fit to data are used to assess the systematic uncertainty due to the choice of the fit model. The maximal value of such differences over the considered set of alternative models is taken as the corresponding systematic uncertainty. The following sources of systematic uncertainty related to the fit model are considered:\n\n• Imperfect knowledge of the detector resolution model. To estimate the associated systematic uncertainty a set of alternative resolution functions is tested: a symmetric variant of an Apollonios function [109], a modified Gaussian function with symmetric power-law tails on both sides of the distribution [110,111], a generalised symmetric Student’s \\( t \\)-distribution [112,113], a symmetric Johnson’s S_U distribution [114,115], and a modified Novosibirsk function [116].\n\n• A small difference in the detector resolution between data and simulation. A correction factor of 1.05 is applied to account for known discrepancies in modelling the detector resolution in simulation. This factor was studied for different decays [39,104,105,117–119] and found to lie between 1.0 and 1.1. For decays with relatively low momentum tracks, this factor is close to 1.05, which is the nominal value used in this analysis. This factor is also cross-checked using large samples of \\( D^{*+} \\rightarrow D^0 \\pi^+ \\) decays, where a value of 1.06 is obtained. To assess the systematic uncertainty related to this factor, detector resolution models with correction factors of 1.0 and 1.1 are studied as alternatives.\n\n• Parameterisation of the background component. To assess the associated systematic uncertainty, the order of the positive polynomial function of Eq. (2) is varied. In addition, to estimate the possible effect from a small contribution from three-body \\( D^0 D^0 \\pi^+ \\) combinations without an intermediate \\( D^{*+} \\) meson, a more general family of background models is tested\n\n\\[\nB'_{nm} = B_n + \\Phi_{D^0 D^0 \\pi^+} \\times P_m ,\n\\]\n\n(3)\nTable 5: Systematic uncertainties for the \\( \\delta m_U \\) parameter. The total uncertainty is calculated as the sum in quadrature of all components.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Source\\( \\sigma_{\\delta m_U} \\) [keV/\\( c^2 \\)]
Fit model
Resolution model2
Resolution correction factor2
Background model2
Coupling constants1
Unknown value of \\( |g| \\)\\(+7\\)
\\(-0\\)
Momentum scaling3
Energy loss1
D*+ – D0 mass difference2
Total\\(+9\\)
\\(-6\\)
\n\nwhere \\( \\Phi_{D^0D^0\\pi^+} \\) denotes the three-body phase-space function [120–122]. The functions \\( B_0, B_1, B_3 \\) and \\( B'_{nm} \\) with \\( n \\leq 2, m \\leq 1 \\) are used as alternative models for the estimation of the systematic uncertainty.\n\n• Values of the coupling constants for the D* → Dπ and D* → Dγ decays affecting the shape of the \\( \\mathcal{F}^U \\) signal profile. These coupling constants are calculated from the known branching fractions of the D* → Dπ and D* → Dγ decays [83], the measured natural width of the D*+ meson [83,123] and the derived value for the natural width of the D*0 meson [78,94,124]. To assess the associated systematic uncertainty, a set of alternative models built around the \\( \\mathcal{F}^U \\) profiles obtained with coupling constants varying within their calculated uncertainties is studied.\n\n• Unknown value of the \\( |g| \\) parameter. In the baseline fit the value of the \\( |g| \\) parameter is fixed to a large value. To assess the effect of this constraint the fit is repeated using the value of \\( |g| = 8.08 \\) GeV, that corresponds to \\( -2\\Delta \\log \\mathcal{L} = 1 \\) for the most conservative likelihood profile for \\( |g| \\) that accounts for the systematic uncertainty. The change of 7 keV/\\( c^2 \\) of the \\( \\delta m_U \\) parameter is assigned as the systematic uncertainty.\n\nThe calibration of the momentum scale of the tracking system is based upon large samples of B+ → J/ψK+ and J/ψ → μ+μ− decays [125]. The accuracy of the procedure has been checked using fully reconstructed B decays together with two-body Υ(nS) and K_S^0 decays and the largest deviation of the bias in the momentum scale of \\( \\delta \\alpha = 3 \\times 10^{-4} \\) is taken as the uncertainty [126]. This uncertainty is propagated to uncertainties for the parameters of interest using simulated samples, with momentum scale corrections of (1 ± \\( \\delta \\alpha \\)) applied. Half of the difference between the obtained peak locations is taken as an estimate of the systematic uncertainty.\n\nIn the reconstruction step, the momenta of the charged tracks are corrected for energy loss in the detector material using the Bethe–Bloch formula [127,128]. The amount of the material traversed in the tracking system by a charged particle is known to 10%\naccuracy [129]. To assess the corresponding uncertainty the magnitude of the calculated corrections is varied by ±10%. Half of the difference between the obtained peak locations is taken as an estimate of the systematic uncertainty due to energy loss corrections.\n\nThe mass of D^0D^0\\pi^+ combinations is calculated with the mass of each D^0 meson constrained to the known value of the D^0 mass [83]. This procedure produces negligible uncertainties for the \\( \\delta m_U \\) parameter due to imprecise knowledge of the D^0 mass. However, the small uncertainty of 2 keV/\\( c^2 \\) for the known D^{*+} – D^0 mass difference [83, 123, 130] directly affects the values of these parameters and is assigned as corresponding systematic uncertainty.\n\nFor the lower limit on the parameter \\( |g| \\), only systematic uncertainties related to the fit model are considered. For each alternative model the likelihood profile curves are built and corresponding 90 and 95 % CL lower limits are calculated using the procedure described above. The smallest of the resulting values is taken as the lower limit that accounts for the systematic uncertainty: \\( |g| > 5.1\\ (4.3)\\ \\mathrm{GeV} \\) at 90(95) % CL.\n\nDiscussion\n\nStudying the D^0\\pi^+ mass distribution for T_{cc}^+ \\rightarrow D^0D^0\\pi^+ decays allows testing the hypothesis that the T_{cc}^+ \\rightarrow D^0D^0\\pi^+ decay proceeds through an intermediate off-shell D^{*+} meson. The background-subtracted D^0\\pi^+ mass distribution for selected D^0D^0\\pi^+ candidates\\footnote{Both D^0\\pi^+ combinations are included. The two-dimensional distribution of the mass of one D^0\\pi^+ combination versus the mass of another D^0\\pi^+ combination is presented in Extended Data Fig. 10.} with the D^0D^0\\pi^+ mass with respect to the D^{*+}D^0 mass threshold, \\( \\delta m_{D^0D^0\\pi^+} \\), below zero is shown in Fig. 3. A fit is performed to this distribution with a model containing signal and background components. The signal component is derived from the \\( \\mathcal{A}_U \\) amplitude, see Methods Eq. (M9b), and is convolved with a detector resolution for the D^0\\pi^+ mass. This detector resolution function is modelled with a modified Gaussian function with power-law tails on both sides of the distribution [110,111] and parameters taken from simulation. Similarly to the correction used for the D^0D^0\\pi^+ mass resolution function \\( \\mathfrak{R} \\), the width of the Gaussian function is corrected by a factor of 1.06, which is determined by studying large samples of D^{*+} \\rightarrow D^0\\pi^+ decays. The shape of the background component is derived from data for \\( \\delta m_{D^0D^0\\pi^+} > 0.6\\ \\mathrm{MeV}/c^2 \\). The fit results are overlaid in Fig. 3. The background component vanishes in the fit, and the D^0\\pi^+ spectrum is consistent with the hypothesis that the T_{cc}^+ \\rightarrow D^0D^0\\pi^+ decay proceeds through an intermediate off-shell D^{*+} meson. This in turn favours the 1^+ assignment for the spin-parity of the state.\n\nDue to the proximity of the observed T_{cc}^+ signal to the D^{*+}D^0 mass threshold, and the small energy release in the D^{*+} \\rightarrow D^0\\pi^+ decay, the D^0D^0 mass distribution from the T_{cc}^+ \\rightarrow D^0D^0\\pi^+ decay forms a narrow peak just above the D^0D^0 mass threshold. In a similar way, a peaking structure in the D^+D^0 mass spectrum just above the D^+D^0 mass threshold is expected from T_{cc}^+ \\rightarrow D^+D^0\\pi^0 and T_{cc}^+ \\rightarrow D^+D^0\\gamma decays, both proceeding via off-shell intermediate D^{*+}D^0 and D^0D^+ states. The D^0D^0 and D^+D^0 final states are reconstructed and selected similarly to the D^0D^0\\pi^+ final state, where the D^+ \\rightarrow K^- \\pi^+ \\pi^- decay channel is used. The background-subtracted D^0D^0 and D^+D^0 mass distributions are shown in Fig. 4, where narrow structures are clearly visible just above the DD thresholds. Fits to these distributions are performed using models consisting of two components: a signal component \\( F_{DD} \\) described in Methods Eq. (M22) and obtained via integration of the matrix\n![Mass distribution for D^0\\pi^+ pairs.](page_184_232_1207_693.png)\n\nFigure 3: Mass distribution for D^0\\pi^+ pairs. Mass distribution for D^0\\pi^+ pairs from selected D^0D^0\\pi^+ candidates with a mass below the D^{*+}D^0 mass threshold with non-D^0 background subtracted. The overlaid fit result is described in the text.\n\nelements for the T_{cc}^+ \\rightarrow DD\\pi/\\gamma decays with the \\( \\mathcal{F}^U \\) profile, and a background component, parameterised as a product of the two-body phase space function \\( \\Phi_{DD} \\) and a positive linear function \\( P_1 \\). The fit results are overlaid in Fig. 4 and summarised in Table 6. The statistical significance of the observed T_{cc}^+ \\rightarrow D^0D^0X and T_{cc}^+ \\rightarrow D^+D^0X signals, where X stands for non-reconstructed pions or photons, is estimated using Wilks' theorem [131] and is found to be in excess of 20 and 10 standard deviations, respectively. The relative yields for the signals observed in the D^0D^0\\pi^+, D^0D^0 and D^0D^+ mass spectra agree with the expectations of the model described in Methods where the decay of an isoscalar T_{cc}^+ state via the D^*D channel with an intermediate off-shell D^* meson is assumed.\n\nThe observation of the near-threshold signals in the D^0D^0 and D^+D^0 mass spectra, along with the signal shapes and yields, all agree with the isoscalar T_{cc}^+ hypothesis for the narrow signal observed in the D^0D^0\\pi^+ mass spectrum. However, an alternative interpretation could be that this state is the I_3 = 0 component of a \\( \\hat{T}_{cc} \\) isotriplet (\\( \\hat{T}_{cc}^0, \\hat{T}_{cc}^+, \\hat{T}_{cc}^{++} \\)) with cc\\bar{u}\\bar{u}, cc\\bar{d}\\bar{d} and cccd quark content, respectively. Assuming that the observed peak corresponds to the \\( \\hat{T}_{cc}^+ \\) component and using the estimates for the \\( \\hat{T}_{cc} \\) mass splitting from Methods Eq. (M30), the masses of the \\( \\hat{T}_{cc}^0 \\) and \\( \\hat{T}_{cc}^{++} \\) states are estimated to be\nFigure 4: Mass distributions for selected D^0D^0 and D^+D^0 combinations. DD mass distributions for selected (left) D^0D^0 and (right) D^+D^0 candidates with the non-D background subtracted. The overlaid fit results are described in the text. For visibility the T_{cc}^{++} \\rightarrow D^+D^0\\pi^0 is stacked on top of the T_{cc}^{+} \\rightarrow D^+D^0\\gamma component.\n\nTable 6: Signal and background yields, \\( N_S \\) and \\( N_B \\), from the fits to DD mass spectra. The uncertainties are statistical only.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
N_SN_B
D^0D^0263 ± 23962 ± 45
D^+D^0171 ± 26763 ± 47
\n\nslightly below the D^0D^{*0} and slightly above the D^+D^{*+} mass thresholds, respectively:\n\n\\[\nm_{\\hat{T}_{cc}^0} - (m_{D^0} + m_{D^{*0}}) = -2.8 \\pm 1.5\\ \\mathrm{MeV}/c^2,\n\\]\n(4a)\n\n\\[\nm_{\\hat{T}_{cc}^{++}} - (m_{D^+} + m_{D^{*+}}) = 2.7 \\pm 1.3\\ \\mathrm{MeV}/c^2.\n\\]\n(4b)\n\nWith these mass assignments, assuming equal production of all three \\( \\hat{T}_{cc} \\) components, the \\( \\hat{T}_{cc}^0 \\) state would be an extra narrow state that decays into the D^0D^0\\pi^0 and D^0D^0\\gamma final states via an off-shell D^{*0} meson. These decays would contribute to the narrow near-threshold enhancement in the D^0D^0 spectrum, and increase the signal in the D^0D^0 mass spectrum by almost a factor of three. The \\( \\hat{T}_{cc}^{++} \\) state would decay via an on-shell D^{*+} meson \\( \\hat{T}_{cc}^{++} \\rightarrow D^+D^{*+} \\), therefore it could be a relatively wide state, with width up to a few MeV [132]. Therefore, it would manifest itself as a peak with a moderate width in the D^+D^0\\pi^+ mass spectrum with a yield comparable to that of the \\( \\hat{T}_{cc}^{+} \\rightarrow D^0D^0\\pi^+ \\) decays. In addition, it would contribute to the D^+D^0 mass spectrum, tripling the contribution from the \\( \\hat{T}_{cc}^{+} \\) decays. However, due to the larger mass of the \\( \\hat{T}_{cc}^{++} \\) state and its larger width, this contribution should be wider, making it more difficult to disentangle from the background. Finally, the \\( \\hat{T}_{cc}^{++} \\) state would make a contribution to the D^+D^+ spectrum with a yield similar to the contribution from \\( \\hat{T}_{cc}^{+} \\rightarrow D^0D^+\\pi^0/\\gamma \\) decays to the D^0D^+ spectrum, but wider. The mass spectra for D^+D^+ and D^+D^0\\pi^+ combinations are shown in Fig. 5. Neither distribution exhibits any\nFigure 5: Mass distributions for selected \\( \\mathrm{D}^+ \\mathrm{D}^+ \\) and \\( \\mathrm{D}^+ \\mathrm{D}^0 \\pi^+ \\) candidates. Mass distributions for selected (left) \\( \\mathrm{D}^+ \\mathrm{D}^+ \\) and (right) \\( \\mathrm{D}^+ \\mathrm{D}^0 \\pi^+ \\) candidates with the non-D background subtracted. The vertical coloured band indicates the expected mass for the hypothetical \\( \\tilde{T}_{cc}^{++} \\) state. The overlaid fit results with background-only functions are described in the text.\n\nnarrow signal-like structure. Fits to these spectra are performed using the following background-only functions:\n\n\\[\nB_{\\mathrm{D}^+ \\mathrm{D}^+} = \\Phi_{\\mathrm{D}^+ \\mathrm{D}^+} \\times P_1,\n\\]\n\\[\nB_{\\mathrm{D}^+ \\mathrm{D}^0 \\pi^+} = (\\Phi_{\\mathrm{D}^+ \\mathrm{D}^+} \\times P_1) * \\mathfrak{R} + \\Phi_{\\mathrm{D}^+ \\mathrm{D}^0 \\pi^+} \\times P_0 .\n\\]\n\nThe results of these fits are overlaid in Fig. 5. The absence of any signals in the \\( \\mathrm{D}^+ \\mathrm{D}^+ \\) and \\( \\mathrm{D}^+ \\mathrm{D}^0 \\pi^+ \\) mass spectra is therefore a strong argument in favour of the isoscalar nature of the observed peak in the \\( \\mathrm{D}^0 \\mathrm{D}^0 \\pi^+ \\) mass spectrum.\n\nThe interference between two virtual channels for the \\( \\mathrm{T}_{cc}^+ \\to \\mathrm{D}^0 \\mathrm{D}^0 \\pi^+ \\) decay, corresponding to two amplitude terms, see Methods Eq. (M4a), is studied by setting the term proportional to \\( C \\) in Methods Eq. (M6a) to be equal to zero. This causes a 43% reduction in the decay rate, pointing to a large interference. The same procedure applied to the \\( \\mathrm{T}_{cc}^+ \\to \\mathrm{D}^+ \\mathrm{D}^0 \\pi^0 \\) decays gives the contribution of 45% for the interference between the \\( (\\mathrm{D}^{*+} \\to \\mathrm{D}^+ \\pi^0) \\mathrm{D}^0 \\) and \\( (\\mathrm{D}^{*0} \\to \\mathrm{D}^0 \\pi^0) \\mathrm{D}^+ \\) channels. For \\( \\mathrm{T}_{cc}^+ \\to \\mathrm{D}^+ \\mathrm{D}^0 \\gamma \\) decays the role of the interference between the \\( (\\mathrm{D}^{*+} \\to \\mathrm{D}^+ \\gamma) \\mathrm{D}^0 \\) and \\( (\\mathrm{D}^{*0} \\to \\mathrm{D}^0 \\gamma) \\mathrm{D}^+ \\) channels is estimated by equating to zero the \\( \\mathfrak{F}_+ \\mathfrak{F}_0^* \\) and \\( \\mathfrak{F}_+^* \\mathfrak{F}_0 \\) terms in Methods Eq. (M8). The interference contribution is found to be 33%.\n\nA model-independent characteristic of the state is the position of the amplitude pole \\( \\hat{s} \\) in the complex plane, responsible for the appearance of the narrow structure in the \\( \\mathrm{D}^0 \\mathrm{D}^0 \\pi^+ \\) mass spectrum. The pole parameters, mass \\( m_{\\text{pole}} \\) and width \\( \\Gamma_{\\text{pole}} \\), are defined through the pole location \\( \\hat{s} \\) as\n\n\\[\n\\sqrt{\\hat{s}} \\equiv m_{\\text{pole}} - \\frac{i}{2} \\Gamma_{\\text{pole}} .\n\\]\n\nThe pole location \\( \\hat{s} \\) is a solution of the equation\n\n\\[\n\\frac{1}{\\mathcal{A}_U^H(\\hat{s})} = 0 ,\n\\]\nwhere \\( \\mathcal{A}_U^{\\prime\\prime}(s) \\) denotes the amplitude on the second Riemann sheet defined in Methods Eq. (M16). For large coupling \\( |g| \\) the position of the resonance pole is uniquely determined by the parameter \\( \\delta m_U \\), *i.e.* the binding energy and the width of the D*+ meson. Figure 6 shows the complex plane of the \\( \\delta \\sqrt{s} \\) variable, defined as\n\n\\[\n\\delta \\sqrt{s} \\equiv \\sqrt{s} - (m_{D^{*+}} + m_{D^0}) .\n\\]\n\nAll possible positions of the pole for \\( |g| \\gg m_{D^0} + m_{D^{*+}} \\) are located on a red dashed curve in Fig. 6. The behaviour of the curve can be understood as follows: with an increase of the binding energy (distance to the D*+D^0 mass threshold), the width gets narrower; and when the parameter \\( \\delta m_U \\) approaches zero, the pole touches the D^0D*+ cut and moves to the other complex sheet, *i.e.* the state becomes virtual. For smaller values of \\( |g| \\), the pole is located between the limiting curve and the \\( \\Re s = 0 \\) line. The pole parameters are found to be\n\n\\[\n\\begin{align*}\n\\delta m_{\\text{pole}} &= -360 \\pm 40^{+4}_{-0} \\text{ keV}/c^2 , \\\\\n\\Gamma_{\\text{pole}} &= 48 \\pm 2^{+0}_{-14} \\text{ keV} ,\n\\end{align*}\n\\]\n\nwhere the first uncertainty is due to the \\( \\delta m_U \\) parameter and the second is due to the unknown value of the \\( |g| \\) parameter The peak is well separated from the D*+D^0 threshold in the D^0D^0\\pi^+ mass spectrum. Hence, as for an isolated narrow resonance, the parameters of the pole are similar to the visible peak parameters, namely the mode \\( \\delta m \\) and FWHM \\( \\nu \\) from Table 3.\n\nA study of the behaviour of the \\( \\mathcal{A}_U(s) \\) amplitude in the vicinity of the D*+D^0 mass threshold leads to the determination of the low-energy scattering parameters, namely the scattering length, \\( a \\), and the effective range, \\( r \\). These parameters are defined via the coefficients of the first two terms of the Taylor expansion of the inverse non-relativistic amplitude [133], *i.e.*\n\n\\[\n\\mathcal{A}_{NR}^{-1} = \\frac{1}{a} + r \\frac{k^2}{2} - i k + \\mathcal{O}(k^4) ,\n\\]\n\nwhere \\( k \\) is the wave number. For \\( \\delta \\sqrt{s} \\lesssim -\\Gamma_{D^{*+}} \\) the inverse amplitude from Eq. (M9a) matches Eq. (10) up to a scale parameter obtained numerically, see Methods Eq. (M24). The value of the scattering length is found to be\n\n\\[\na = \\left[ -(7.16 \\pm 0.51) + i\\,(1.85 \\pm 0.28) \\right] \\text{ fm} .\n\\]\n\nTypically, a non-vanishing imaginary part of the scattering length indicates the presence of inelastic channels [134]; however, in this case the non-zero imaginary part is related to the lower threshold, \\( T_{cc}^{++} \\to D^0 D^0 \\pi^+ \\), and is determined by the width of the D*+ meson. The real part of the scattering length \\( a \\) is negative indicating attraction. This can be interpreted as the characteristic size of the state [8],\n\n\\[\nR_a \\equiv -\\Re a = 7.16 \\pm 0.51 \\text{ fm} .\n\\]\n\nFor the \\( \\mathcal{A}_U \\) amplitude the effective range \\( r \\) is non-positive and proportional to \\( |g|^{-2} \\), see Methods Eq. (M26). Its value is consistent with zero for the baseline fit. An upper limit on the \\( -r \\) value is set as\n\n\\[\n0 \\leq -r < 11.9\\,(16.9) \\text{ fm at } 90\\,(95)\\% \\text{ CL} .\n\\]\nFigure 6: Complex plane of the \\( \\delta \\sqrt{s} \\) variable. Complex plane of the \\( \\delta \\sqrt{s} \\) variable. The dashed red line shows the allowed region for large \\( |g| \\) values. The filled red circle indicates the best estimate for the pole location and the filled regions show 1\\( \\sigma \\) and 2\\( \\sigma \\) confidence regions. Open blue and green circles show the branch points corresponding to the D*+D0 and D*0D+ channels, respectively, and the corresponding blue and green lines indicate branch cuts. Three other branch points at \\( \\sqrt{s} \\) of \\( m_{D^0} + m_{D^+} \\), \\( m_{D^0} + m_{D^+} + m_{\\pi^0} \\) and \\( 2m_{D^0} + m_{\\pi^+} \\), corresponding to the openings of the D0D+γ, D0D+π0 and D0D0π+ decay channels, are outside of the displayed region.\n\nThe Weinberg compositeness criterion [135,136] makes use of the relation between the scattering length and the effective range to construct the compositeness variable \\( Z \\),\n\n\\[\nZ = 1 - \\sqrt{\\frac{1}{1 + 2|r/\\Re a|}} ,\n\\]\n\nfor which \\( Z = 1 \\) corresponds to a compact state that does not interact with the continuum, while \\( Z = 0 \\) indicates a composite state formed by compound interaction. Using the relation between \\( r \\) and \\( |g| \\) from Methods Eq. (M26), one finds \\( Z \\propto |g|^{-2} \\) for large values of \\( |g| \\). The default fit corresponds to large values of \\( |g| \\), and thus, \\( Z \\) approaching to zero. A non-zero value of \\( Z \\) would require a smaller value of \\( |g| \\), i.e. smaller resonance width, see Extended Data Fig. 7. The following upper limit of the compositeness parameter \\( Z \\) is\nset:\n\\[\nZ < 0.52\\,(0.58) \\text{ at } 90\\,(95)\\% \\text{ CL}.\n\\]\n\nAnother estimate of the characteristic size is obtained from the value of the binding energy \\( \\Delta E \\). Within the interpretation of the \\( T_{cc}^+ \\) state as a bound \\( D^{*+}D^0 \\) molecular-like state, the binding energy is \\( \\Delta E = -\\delta m_U \\). The characteristic momentum scale \\( \\gamma \\) [8] is estimated to be\n\\[\n\\gamma = \\sqrt{2 \\mu \\Delta E} = 26.4 \\pm 1.5\\,\\text{MeV}/c,\n\\]\nwhere \\( \\mu \\) is the reduced mass of the \\( D^{*+}D^0 \\) system. This value of the momentum scale in turn corresponds to a characteristic size \\( R_{\\Delta E} \\) of the molecular-like state,\n\\[\nR_{\\Delta E} \\equiv \\frac{1}{\\gamma} = 7.5 \\pm 0.4\\,\\text{fm},\n\\]\nwhich is consistent with the \\( R_a \\) estimate from the scattering length.\n\nFor high-energy hadroproduction of a state with such a large size, \\( R_a \\) or \\( R_{\\Delta E} \\), one expects a strong dependency of the production rate on event multiplicity, similar to that observed for the \\( \\chi_{c1}(3872) \\) state [137]. The background-subtracted distribution of the number of tracks reconstructed in the vertex detector, \\( N_{\\text{tracks}} \\), is shown in Fig. 7 together with the distributions for low-mass \\( D^0\\overline{D}^0 \\) pairs\\footnote{The chosen interval for \\( D^0\\overline{D}^0 \\) pairs includes the region populated by the \\( \\chi_{c1}(3872) \\rightarrow D^0\\overline{D}^0\\pi^0/\\gamma \\) decays;} with \\( m_{D^0\\overline{D}^0} < 3.87\\,\\text{GeV}/c^2 \\) and low-mass \\( D^0D^0 \\) pairs with mass \\( 3.75 < m_{D^0D^0} < 3.87\\,\\text{GeV}/c^2 \\). The former is dominated by \\( pp \\rightarrow c\\overline{c}X \\) production, while the latter is presumably dominated by the double parton scattering process [87, 138]. The \\( \\chi_{c1}(3872) \\) production cross-section is suppressed with respect to the conventional charmonium state \\( \\psi(2S) \\) at large track multiplicities [137]. It is noteworthy that the track multiplicity distribution for the \\( T_{cc}^+ \\) state differs from that of the low-mass \\( D^0\\overline{D}^0 \\) pairs, in particular no suppression at large multiplicity is observed. A \\( p \\)-value for the consistency of the track multiplicity distributions for \\( T_{cc}^+ \\) production and low-mass \\( D^0\\overline{D}^0 \\) pairs is found to be 0.1%. It is interesting to note that the multiplicity distribution for \\( T_{cc}^+ \\) production and the one for \\( D^0D^0 \\)-pairs with \\( 3.75 < m_{D^0D^0} < 3.87 \\) are consistent with a corresponding \\( p \\)-value of 12%. The similarity between \\( T_{cc}^+ \\) production, which is inherently a single parton scattering process, and the distribution for process dominated by a double parton scattering is surprising.\n\nThe transverse momentum spectrum for the \\( T_{cc}^+ \\) state is compared with those for the low-mass \\( D^0\\overline{D}^0 \\) and \\( D^0D^0 \\) pairs in Fig. 8. The \\( p \\)-values for the consistency of the \\( p_T \\) spectra for the \\( T_{cc}^+ \\) state and low-mass \\( D^0\\overline{D}^0 \\) pairs are 1.4%, and 0.02% for low-mass \\( D^0D^0 \\) pairs. More data are needed for further conclusions.\n\nThe background-subtracted \\( D^0D^0 \\) mass distribution in a wider mass range is shown in Fig. 9 together with a similar distribution for \\( D^0D^0 \\) pairs. In the \\( D^0D^0 \\) mass spectrum the near-threshold enhancement is due to \\( \\chi_{c1}(3872) \\rightarrow D^0\\overline{D}^0\\pi^0 \\) and \\( \\chi_{c1}(3872) \\rightarrow D^0\\overline{D}^0\\gamma \\) decays via intermediate \\( D^{*0} \\) mesons [90]. This structure is significantly wider than the structure in the \\( D^0D^0 \\) mass spectrum from \\( T_{cc}^+ \\rightarrow D^0D^0\\pi^+ \\) decays primarily due to the larger natural width and smaller binding energy for the \\( \\chi_{c1}(3872) \\) state [104, 105]. With more data, and with a better understanding of the dynamics of \\( \\chi_{c1}(3872) \\rightarrow D^0\\overline{D}^0\\pi^0/\\gamma \\) decays, and therefore of the corresponding shape in the \\( D^0\\overline{D}^0 \\) mass spectrum, it will be possible to estimate the relative production rates for the \\( T_{cc}^+ \\) and \\( \\chi_{c1}(3872) \\) states. Background-subtracted \\( D^0D^0\\pi^+ \\) and \\( D^0D^+ \\) mass distributions together with those for \\( \\overline{D}^0D^0\\pi^+ \\) and \\( D^0D^- \\) are shown in Extended Data Figs. 3 and 4.\n![Track multiplicity distributions. Background-subtracted distributions for the multiplicity of tracks reconstructed in the vertex detector for (red circles) \\( T_{cc}^+ \\to D^0 D^0 \\pi^+ \\) signal, low-mass (blue open squares) \\( D^0 \\overline{D}^0 \\) and (green filled diamonds) \\( D^0 D^0 \\) pairs. The binning scheme is chosen to have an approximately uniform distribution for \\( D^0 \\overline{D}^0 \\) pairs. The distributions for the \\( D^0 \\overline{D}^0 \\) and \\( D^0 D^0 \\) pairs are normalised to the same yields as the \\( T_{cc}^+ \\to D^0 D^0 \\pi^+ \\) signal. For better visualisation, the points are slightly displaced from the bin centres.](page_184_232_1207_693.png)\n\nFigure 7: **Track multiplicity distributions.** Background-subtracted distributions for the multiplicity of tracks reconstructed in the vertex detector for (red circles) \\( T_{cc}^+ \\to D^0 D^0 \\pi^+ \\) signal, low-mass (blue open squares) \\( D^0 \\overline{D}^0 \\) and (green filled diamonds) \\( D^0 D^0 \\) pairs. The binning scheme is chosen to have an approximately uniform distribution for \\( D^0 \\overline{D}^0 \\) pairs. The distributions for the \\( D^0 \\overline{D}^0 \\) and \\( D^0 D^0 \\) pairs are normalised to the same yields as the \\( T_{cc}^+ \\to D^0 D^0 \\pi^+ \\) signal. For better visualisation, the points are slightly displaced from the bin centres.\n\nSummary\n\nThe exotic narrow tetraquark state \\( T_{cc}^+ \\) observed in Ref. [84] is studied using a dataset corresponding to an integrated luminosity of 9\\( \\text{fb}^{-1} \\), collected by the LHCb experiment in pp collisions at centre-of-mass energies of 7, 8 and 13 TeV. The observed \\( D^0 \\pi^+ \\) mass distribution indicates that the \\( T_{cc}^+ \\to D^0 D^0 \\pi^+ \\) decay proceeds via an intermediate off-shell \\( D^{*+} \\) meson. Together with the proximity of the state to the \\( D^* D^0 \\) mass threshold this favours the spin-parity quantum numbers \\( J^P \\) to be \\( 1^+ \\). Narrow near-threshold structures are observed in the \\( D^0 D^0 \\) and \\( D^0 D^+ \\) mass spectra with high significance. They are found to be consistent with originating from off-shell \\( T_{cc}^+ \\to D^* D \\) decays followed by the \\( D^* \\to D \\pi \\) and \\( D^* \\to D \\gamma \\) decays. No signal is observed in the \\( D^+ D^0 \\pi^+ \\) mass spectrum, and no structure is observed in the \\( D^+ D^+ \\) mass spectrum. These non-observations provide\n\nhowever, this contribution is small, see Fig. 9.\nFigure 8: **Transverse momentum spectra**. Background-subtracted transverse momentum spectra for (red circles) \\( T_{c\\bar{c}}^+ \\to D^0 D^0 \\pi^+ \\) signal, (blue open squares) low-mass \\( D^0 \\overline{D}^0 \\) and (green filled diamonds) \\( D^0 D^0 \\), \\( 3.75 < m_{D^0 D^0} < 3.87 \\) GeV/\\( c^2 \\). The binning scheme is chosen to have an approximately uniform distribution for \\( D^0 \\overline{D}^0 \\) pairs. The distributions for the \\( D^0 \\overline{D}^0 \\) and \\( D^0 D^0 \\) pairs are normalised to the same yields as \\( T_{c\\bar{c}}^+ \\to D^0 D^0 \\pi^+ \\) signal. For better visualisation, the points are slightly displaced from the bin centres.\n\na strong argument in favour of the isoscalar nature for the observed state, supporting its interpretation as the isoscalar \\( J^P = 1^+ \\) cc\\( \\bar{u}\\bar{d} \\)-tetraquark ground state. Under this hypothesis the mass of the \\( T_{c\\bar{c}}^+ \\) state, relative to the \\( D^*+D^0 \\) mass threshold, is determined using a unitarised three-body Breit–Wigner amplitude model\n\n\\[\n\\delta m_U = -359 \\pm 40^{+9}_{-6} \\text{ keV}/c^2,\n\\]\n\nwhere the first uncertainty is statistic and the second systematic. The lower limit on the absolute value of the coupling constant of the \\( T_{c\\bar{c}}^+ \\) state to the \\( D^* D \\) system is\n\n\\[\n|g| > 5.1\\,(4.3)\\ \\text{GeV at } 90\\,(95)\\% \\text{ CL}.\n\\]\nFigure 9: Mass distributions for \\( D^0 \\overline{D}^0 \\) and \\( D^0 D^0 \\) candidates. Background-subtracted \\( D^0 D^0 \\) and \\( D^0 \\overline{D}^0 \\) mass distributions. The near-threshold enhancement in the \\( D^0 D^0 \\) channel corresponds to partially reconstructed \\( T_{cc}^+ \\to D^0 D^0 \\pi^+ \\) decays, while in the \\( D^0 \\overline{D}^0 \\) channel the threshold enhancement corresponds to partially reconstructed \\( \\chi_{c1}(3872) \\to D^0 \\overline{D}^0 \\pi^0 \\) decays.\n\nFrom the low-energy limit of the amplitude, the estimates for the scattering length \\( a \\), effective range \\( r \\), and the compositeness, \\( Z \\), are obtained\n\n\\[\na = \\left[ - (7.16 \\pm 0.51) + i \\ (1.85 \\pm 0.28) \\right] \\text{fm},\n\\]\n\\[\n-r < 11.9 \\ (16.9) \\ \\text{fm at } 90 \\ (95)\\% \\text{ CL},\n\\]\n\\[\nZ < 0.52 \\ (0.58) \\ \\text{at } 90 \\ (95)\\% \\text{ CL}.\n\\]\n\nThe characteristic size calculated from the binding energy is \\( R_{\\Delta E} = 7.49 \\pm 0.42 \\) fm. This value is consistent with the estimation from the scattering length, \\( R_a = 7.16 \\pm 0.51 \\) fm. Both \\( R_{\\Delta E} \\) and \\( R_a \\) correspond to a spatial extension significantly exceeding the typical scale for heavy-flavour hadrons.\n\nThe amplitude pole is found to be located on the second Riemann sheet with respect to the \\( D^0 D^0 \\pi^+ \\) threshold, at \\( \\hat{s} = m_{\\text{pole}} - \\frac{i}{2} \\Gamma_{\\text{pole}} \\), where\n\\[\n\\delta m_{\\text{pole}} = -360 \\pm 40^{+4}_{-0} \\ \\text{keV}/c^2,\n\\]\n\\[\n\\Gamma_{\\text{pole}} = 48 \\pm 2^{+0}_{-14} \\ \\text{keV},\n\\]\nwhere the first uncertainty accounts for statistical and systematic uncertainties for the \\( \\delta m_U \\) parameters, and the second is due to the unknown value of the \\( |g| \\) parameter. The pole position, scattering length, effective range and compositeness form a complete set of experimental observables related to the \\( T_{cc}^{++} \\to D^0 \\overline{D}^0 \\pi^+ \\) reaction amplitude, which is vital for inferring the nature of the \\( T_{cc}^{++} \\) tetraquark.\n\nUnlike the prompt production of the \\( \\chi_{c1}(3872) \\) state, no suppression of the \\( T_{cc}^{++} \\) state production at high track multiplicities is observed relative to the low-mass \\( D^0 \\overline{D}^0 \\) pairs. The observed similarity with the multiplicity distribution for the low-mass \\( D^0 \\overline{D}^0 \\) production process, that is presumably double-parton-scattering dominated, is unexpected. In the future with a larger dataset and including other decay modes, *e.g.* \\( D^0 \\to K^- \\pi^+ \\pi^+ \\pi^- \\), detailed studies of the properties of this new state and its production mechanisms could be possible.\n\nAcknowledgements\n\nThis paper is dedicated to the memory of our dear friend and colleague Simon Eidelman, whose contributions to improving the quality of our papers were greatly appreciated. We thank M. Karliner for inspiring and stimulating discussions. We express our gratitude to our colleagues in the CERN accelerator departments for the excellent performance of the LHC. We thank the technical and administrative staff at the LHCb institutes. We acknowledge support from CERN and from the national agencies: CAPES, CNPq, FAPERJ and FINEP (Brazil); MOST and NSFC (China); CNRS/IN2P3 (France); BMBF, DFG and MPG (Germany); INFN (Italy); NWO (Netherlands); MNiSW and NCN (Poland); MEN/IFA (Romania); MSHE (Russia); MICINN (Spain); SNSF and SER (Switzerland); NASU (Ukraine); STFC (United Kingdom); DOE NP and NSF (USA). We acknowledge the computing resources that are provided by CERN, IN2P3 (France), KIT and DESY (Germany), INFN (Italy), SURF (Netherlands), PIC (Spain), GridPP (United Kingdom), RRCKI and Yandex LLC (Russia), CSCS (Switzerland), IFIN-HH (Romania), CBPF (Brazil), PL-GRID (Poland) and NERSC (USA). We are indebted to the communities behind the multiple open-source software packages on which we depend. Individual groups or members have received support from ARC and ARDC (Australia); AvH Foundation (Germany); EPLANET, Marie Sklodowska-Curie Actions and ERC (European Union); A*MIDEX, ANR, IPhU and Labex P2IO, and Région Auvergne-Rhône-Alpes (France); Key Research Program of Frontier Sciences of CAS, CAS PIFI, CAS CCEPP, Fundamental Research Funds for the Central Universities, and Sci. & Tech. Program of Guangzhou (China); RFBR, RSF and Yandex LLC (Russia); GVA, XuntaGal and GENCAT (Spain); the Leverhulme Trust, the Royal Society and UKRI (United Kingdom).\nMethods\n\nExperimental setup\nThe LHCb detector [85, 86] is a single-arm forward spectrometer covering the pseudo-rapidity range \\(2 < \\eta < 5\\), designed for the study of particles containing b or c quarks. The detector includes a high-precision tracking system consisting of a silicon-strip vertex detector surrounding the pp interaction region, a large-area silicon-strip detector located upstream of a dipole magnet with a bending power of about 4 Tm, and three stations of silicon-strip detectors and straw drift tubes placed downstream of the magnet. The tracking system provides a measurement of the momentum, \\(p\\), of charged particles with a relative uncertainty that varies from 0.5% at low momentum to 1.0% at 200 GeV/\\(c\\). The minimum distance of a track to a primary pp collision vertex (PV), the impact parameter (IP), is measured with a resolution of \\((15 + 29/p_T)\\) \\(\\mu\\)m, where \\(p_T\\) is the component of the momentum transverse to the beam, in GeV/\\(c\\). Different types of charged hadrons are distinguished using information from two ring-imaging Cherenkov detectors [139]. Photons, electrons and hadrons are identified by a calorimeter system consisting of scintillating-pad and preshower detectors, an electromagnetic and a hadronic calorimeter. Muons are identified by a system composed of alternating layers of iron and multiwire proportional chambers. The online event selection is performed by a trigger, which consists of a hardware stage, based on information from the calorimeter and muon systems, followed by a software stage, which applies a full event reconstruction.\n\nSimulation\nSimulation is required to model the effects of the detector acceptance, resolution, and the efficiency of the imposed selection requirements. In the simulation, pp collisions are generated using PYTHIA [140] with a specific LHCb configuration [141]. Decays of unstable particles are described by EVTGEN [142], in which final-state radiation is generated using PHOTOS [143]. The interaction of the generated particles with the detector, and its response, are implemented using the GEANT4 toolkit [144] as described in Ref. [145].\n\nEvent selection\nThe D\\(^0\\)D\\(^0\\), D\\(^0\\)D\\(^{+}\\) and D\\(^0\\)D\\(^0\\pi^+\\) final states are reconstructed using the D\\(^0 \\to K^- \\pi^+\\) and D\\(^+ \\to K^- \\pi^+ \\pi^+\\) decay channels. The selection criteria are similar to those used in Refs. [87–90]. Kaons and pions are selected from well-reconstructed tracks within the acceptance of the spectrometer that are identified using information from the ring-imaging Cherenkov detectors. The kaon and pion candidates that have transverse momenta larger than 250 MeV/\\(c\\) and are inconsistent with being produced at a pp interaction vertex are combined together to form D\\(^0\\) and D\\(^+\\) candidates, referred to as D hereafter. The resulting D candidates are required to have good vertex quality, mass within \\( \\pm 65 \\) MeV/\\(c^2\\) and \\( \\pm 50 \\) MeV/\\(c^2\\) of the known D\\(^0\\) and D\\(^+\\) masses [83], respectively, transverse momentum larger than 1 GeV/\\(c\\), decay time larger than 100 \\(\\mu\\)m/\\(c\\) and a momentum direction that is consistent with the vector from the primary to secondary vertex. Selected D\\(^0\\) and D\\(^+\\) candidates consistent with originating from a common primary vertex are combined to form D\\(^0\\)D\\(^0\\) and D\\(^0\\)D\\(^+\\) candidates. The resulting D\\(^0\\)D\\(^0\\) candidates are combined with a pion\nto form \\( D^0 D^0 \\pi^+ \\) candidates. For those, at least one out of the two \\( D^0 \\pi^+ \\) combinations is required to have good vertex quality and mass not exceeding the known \\( D^{*+} \\) mass by more than 155 MeV/\\( c^2 \\). For each \\( D^0 D^0 \\), \\( D^0 D^+ \\) and \\( D^0 D^0 \\pi^+ \\) candidate a kinematic fit [146] is performed. This fit constrains the mass of the D candidates to their known values and requires both D mesons, and a pion in the case of \\( D^0 D^0 \\pi^+ \\), to originate from the same primary vertex. A requirement is applied to the quality of this fit to further suppress combinatorial background and reduce the background from D candidates produced in two independent pp interactions or in the decays of beauty hadrons [87]. To suppress background from kaon and pion candidates reconstructed from one common track, all track pairs of the same charge are required to have an opening angle inconsistent with being zero and the mass of the combination must be inconsistent with the sum of the masses of the two constituents. For cross-checks additional final states \\( D^+ D^+ \\), \\( D^+ D^0 \\pi^+ \\), \\( D^0 \\overline{D}^0 \\), \\( D^0 D^- \\) and \\( \\overline{D}^0 D^0 \\pi^+ \\) are reconstructed, selected and treated in the same way.\n\nNon-D background subtraction\n\nTwo-dimensional distributions of the mass of one D candidate versus the mass of the other D candidate from selected \\( D^0 D^0 \\pi^+ \\), \\( D^0 D^0 \\) and \\( D^0 D^+ \\) combinations are shown in Extended Data Fig. 1. These distributions illustrate the relatively small combinatorial background levels due to fake D candidates. This background is subtracted using the sPlot technique [147], which is based on an extended unbinned maximum-likelihood fit to these two-dimensional distributions with the function described in Ref. [87]. This function consists of four components:\n\n• a component corresponding to genuine \\( D_1 D_2 \\) pairs and described as a product of two signal functions, each parameterised with a modified Novosibirsk function [116];\n\n• two components corresponding to combinations of one of the D mesons with combinatorial background and described as products of the signal functions and background function in turn parameterised with a product of an exponential function and a positive first-order polynomial;\n\n• a component corresponding to pure background pairs and described by a product of exponential functions and a positive two-dimensional non-factorisable second-order polynomial function.\n\nBased on the results of the fit, each candidate is assigned a positive weight for being signal-like or a negative weight for being background-like, with the masses of the two \\( D^0 \\) candidates as discriminating variables. The \\( D^0 D^0 \\pi^+ \\) mass distributions for each of the subtracted background components are presented in Extended Data Fig. 2, where fit results with background-only functions \\( B'_{10} \\), defined in Eq. (3) are overlaid.\n\nResolution model for the \\( D^0 D^0 \\pi^+ \\) mass\n\nIn the vicinity of the \\( D^{*+} D^0 \\) mass threshold the resolution function \\( \\mathfrak{R} \\) for the \\( D^0 D^0 \\pi^+ \\) mass is parametrised with the sum of two Gaussian functions with a common mean. The widths of the Gaussian functions are \\( \\sigma_1 = 1.05 \\times 263 \\) keV/\\( c^2 \\) and \\( \\sigma_2 = 2.413 \\times \\sigma_1 \\) for the narrow and wide components, respectively, and the fraction of the narrow Gaussian is \\( \\alpha = 0.778 \\).\nThe parameters \\( \\alpha \\) and \\( \\sigma_{1,2} \\) are taken from simulation, and \\( \\sigma_{1,2} \\) are corrected with a factor of 1.05 that accounts for a small difference between simulation and data for the mass resolution [39, 104, 105]. The root mean square of the resolution function is around 400 keV/\\( c^2 \\).\n\nMatrix elements for \\( T_{cc}^+ \\to DD\\pi/\\gamma \\) decays\n\nAssuming isospin symmetry, the isoscalar vector state \\( T_{cc}^+ \\) that decays into the D*D final state can be expressed as\n\\[\n|T_{cc}^+\\rangle = \\frac{1}{\\sqrt{2}} \\left(|D^{*+}D^0\\rangle - |D^{*0}D^+\\rangle\\right).\n\\]\n(M1)\n\nTherefore, the S-wave amplitudes\\footnote{The S-wave (corresponds to orbital angular momentum equal to zero) approximation is valid for a near-threshold peak. For \\( T_{cc}^+ \\) masses significantly above the D*D threshold, higher-order waves also need to be considered.} for the \\( T_{cc}^+ \\to D^{*+}D^0 \\) and \\( T_{cc}^+ \\to D^{*0}D^+ \\) decays have different signs\n\\[\n\\mathcal{A}_{T_{cc}^+ \\to D^{*+}D^0}^{\\text{S-wave}} = + \\frac{g}{\\sqrt{2}} \\epsilon_{T_{cc}^+}^\\mu \\epsilon_{D^*}^{\\nu\\mu},\n\\]\n(M2a)\n\\[\n\\mathcal{A}_{T_{cc}^+ \\to D^{*0}D^+}^{\\text{S-wave}} = - \\frac{g}{\\sqrt{2}} \\epsilon_{T_{cc}^+}^\\mu \\epsilon_{D^*}^{\\nu\\mu},\n\\]\n(M2b)\nwhere \\( g \\) is a coupling constant, \\( \\epsilon_{T_{cc}^+} \\) is the polarisation vector of the \\( T_{cc}^+ \\) particle and \\( \\epsilon_{D^*} \\) is the polarisation vector of \\( D^* \\) meson, and the upper and lower Greek indices imply the summation in the Einstein notation. The amplitudes for the \\( D^* \\to D\\pi \\) decays are written as\n\\[\n\\mathcal{A}_{D^{*+} \\to D^0\\pi^+} = f \\epsilon_{D^*}^\\alpha p_{D\\alpha}\n\\]\n(M3a)\n\\[\n\\mathcal{A}_{D^{*+} \\to D^+\\pi^0} = - \\frac{f}{\\sqrt{2}} \\epsilon_{D^*}^\\alpha p_{D\\alpha}\n\\]\n(M3b)\n\\[\n\\mathcal{A}_{D^{*0} \\to D^0\\pi^0} = + \\frac{f}{\\sqrt{2}} \\epsilon_{D^*}^\\alpha p_{D\\alpha},\n\\]\n(M3c)\nwhere \\( f \\) denotes a coupling constant, and \\( p_D \\) stands for the momentum of the D meson. The amplitude for the \\( D^* \\to D\\gamma \\) decays is\n\\[\n\\mathcal{A}_{D^{*+} \\to D\\gamma} = i \\mu h \\epsilon_{\\alpha\\beta\\eta\\xi} \\epsilon_{D^*}^\\alpha p_{D^*}^\\beta \\epsilon_\\gamma^\\eta p_\\gamma^\\xi,\n\\]\n(M3d)\nwhere \\( h \\) denotes a coupling constant, \\( \\mu \\) stands for the magnetic moment for \\( D^* \\to D\\gamma \\) transitions, \\( p_{D^*} \\) and \\( p_\\gamma \\) are the the D*-meson and photon momenta, respectively, and \\( \\epsilon_\\gamma \\) is the polarisation vector of the photon. The three amplitudes for \\( T_{cc}^+ \\to \\pi DD \\) and \\( T_{cc}^+ \\to \\gamma DD \\) decays are\n\\[\n\\mathcal{A}_{\\pi^+D^0D^0} = \\frac{f g}{\\sqrt{2}} \\epsilon_{T_{cc}^+}^\\nu \\left[ \\mathfrak{F}_+(s_{12}) \\times \\left(-p_2' + \\frac{(p_2 p_{12}) p_{12}'}{s_{12}}\\right) + (p_2 \\leftrightarrow p_3) \\right],\n\\]\n(M4a)\n\\[\n\\mathcal{A}_{\\pi^0D^+D^0} = - \\frac{f g}{2} \\epsilon_{T_{cc}^+}^\\nu \\left[ \\mathfrak{F}_+(s_{12}) \\times \\left(-p_2' + \\frac{(p_2 p_{12}) p_{12}'}{s_{12}}\\right) + \\left(p_2 \\leftrightarrow p_3\\right) \\left(\\mathfrak{F}_+ \\leftrightarrow \\mathfrak{F}_0\\right) \\right],\n\\]\n(M4b)\n\\[\n\\mathcal{A}_{\\gamma D^+D^0} = i \\frac{h g}{\\sqrt{2}} \\epsilon_{\\alpha \\beta \\eta \\xi} \\epsilon_{T_{cc}^\\mu}^{\\eta} p_\\gamma^{\\xi} [\\mu_+ \\mathfrak{F}_+(s_{12}) p_{12}^\\alpha - \\mu_0 \\mathfrak{F}_0(s_{13}) p_{13}^\\alpha] ,\n\\]\nwhere \\( s_{ij} = p_{ij}^2 = (p_i + p_j)^2 \\) and \\( \\mathfrak{F} \\) functions that denote the Breit–Wigner amplitude for the D* mesons are\n\\[\n\\mathfrak{F}(s) = \\frac{1}{m_{D^*}^2 - s - i m_{D^*} \\Gamma_{D^*}} .\n\\]\nThe last terms in Eqs. (M4a) and (M4b) imply the same amplitudes with swapped momenta.\n\nThe T$_{cc}^+$ state is assumed to be produced unpolarized, therefore the squared absolute values of the decay amplitudes with pions in the final state, averaged over the initial spin-state are\n\\[\n|\\mathcal{M}_{\\pi^+D^0D^0}|^2 = \\frac{1}{3} \\frac{f^2 g^2}{2! \\cdot 2} [|\\mathfrak{F}_+(s_{12})|^2 A + |\\mathfrak{F}_+(s_{13})|^2 B + 2 \\Re \\{ \\mathfrak{F}_+(s_{12}) \\mathfrak{F}_+^*(s_{13}) \\} C] , \\tag{M6a}\n\\]\n\\[\n|\\mathcal{M}_{\\pi^0D^+D^0}|^2 = \\frac{1}{3} \\frac{f^2 g^2}{4} [|\\mathfrak{F}_+(s_{12})|^2 A + |\\mathfrak{F}_0(s_{13})|^2 B + 2 \\Re \\{ \\mathfrak{F}_+(s_{12}) \\mathfrak{F}_0^*(s_{13}) \\} C] , \\tag{M6b}\n\\]\nwhere\n\\[\nA = \\frac{\\lambda(s_{12}, m_1^2, m_2^2)}{4 s_{12}} + \\frac{1}{s} \\left( \\frac{(pp_{12})(p_2 p_{12})}{s_{12}} - pp_2 \\right)^2 , \\tag{M7a}\n\\]\n\\[\nB = \\frac{\\lambda(s_{13}, m_1^2, m_3^2)}{4 s_{13}} + \\frac{1}{s} \\left( \\frac{(pp_{13})(p_3 p_{13})}{s_{13}} - pp_3 \\right)^2 , \\tag{M7b}\n\\]\n\\[\nC = D + E\n\\]\n\\[\nD = \\frac{(p_3 p_{12})(p_2 p_{12})}{s_{12}} + \\frac{(p_2 p_{13})(p_3 p_{13})}{s_{13}} - \\frac{(p_{12} p_{13})(p_2 p_{12})(p_3 p_{13})}{s_{12} s_{13}} - p_2 p_3 , \\tag{M7c}\n\\]\n\\[\nE = \\frac{(pp_{12})(pp_{13})(p_2 p_{12})(p_3 p_{13})}{s s_{12} s_{13}} + \\frac{(pp_2)(pp_3)}{s}\n- \\frac{(pp_{12})(p_2 p_{12})(pp_3)}{s s_{12}} - \\frac{(pp_{13})(p_3 p_{13})(pp_2)}{s s_{13}} , \\tag{M7d}\n\\]\nand \\( \\lambda(x, y, z) \\) stands for the Källén function [106]. The additional factor of 2! in the denominator of Eq. (M6a) is due to the presence of two identical particles (D$^0$) in the final state. The squared absolute values of the decay amplitude with a photon in the final state, averaged over the initial spin state is\n\\[\n|\\mathcal{M}_{T_{cc}^+\\to\\gamma D^+D^0}|^2 = \\frac{1}{3} |g h|^2 |\\mu_+ \\mathfrak{F}_+(s_{12})(p_1 p_2) - \\mu_0 \\mathfrak{F}_0(s_{13})(p_1 p_3)|^2\n+ \\frac{1}{3} |g h|^2 |\\mu_+ \\mathfrak{F}_+(s_{12}) + \\mu_0 \\mathfrak{F}_0(s_{13})|^2 G , \\tag{M8a}\n\\]\n\\[\nG = \\frac{1}{2 s} [2(p_1 p_2)(p_1 p_3)(p_2 p_3) - m_2^2 (p_1 p_3)^2 - m_3^2 (p_1 p_2)^2] . \\tag{M8b}\n\\]\nThe coupling constants \\( f \\) and \\( h \\) for the D$^*\\to$ D$\\pi$ and D$^*\\to$ D$\\gamma$ decays are calculated using Eqs. (M3) from the known branching fractions of the D$^*\\to$ D$\\pi$ and D$^*\\to$ D$\\gamma$ decays [83], the measured natural width of the D$^{*+}$ meson [83,123] and the derived value for the natural width for the D$^{*0}$ meson [78,94,124]. The magnetic moment \\( \\mu_+ \\) is taken to be 1 and the ratio of magnetic moments \\( \\mu_0/\\mu_+ \\) is calculated according to Refs. [148–150].\nUnitarised Breit–Wigner shape\n\nA unitarised three-body Breit–Wigner function is defined as\n\\[\n\\mathfrak{F}_f^U(s) = \\varrho_f(s) |\\mathcal{A}_U(s)|^2 , \\tag{M9a}\n\\]\n\\[\n\\mathcal{A}_U(s) = \\frac{1}{m_U^2 - s - i m_U \\hat{\\Gamma}(s)} , \\tag{M9b}\n\\]\nwhere \\( f \\in \\{ D^0 D^0 \\pi^+, D^0 D^+ \\pi^0, D^0 D^+ \\gamma \\} \\) denotes the final state. The decay matrix element for each channel integrated over the three-body phase space is denoted by\n\\[\n\\varrho_f(s) = \\frac{1}{(2\\pi)^5 4s} \\int \\int ds_{12} ds_{23} \\frac{|\\mathfrak{M}_f(s, s_{12}, s_{23})|^2}{|g|^2} , \\tag{M10}\n\\]\nwhere \\( |\\mathfrak{M}_f|^2 \\) is defined by Eqs.(M6) and (M8), and the unknown coupling constant \\( g \\) is taken out of the expression for \\( |\\mathfrak{M}_f|^2 \\). For large values of \\( s \\), in excess of \\( s^* \\), such as \\( \\sqrt{s^*} - (m_{D^*} + m_D) \\gg \\Gamma_{D^*} \\), the functions \\( \\varrho_f(s) \\) are defined as\n\\[\n\\begin{align*}\n\\varrho_{D^0 D^0 \\pi^+}(s)|_{s > s^*} &= c_1 \\Phi_{D^* D^0}(s) , \\\\\n\\varrho_{D^0 D^+ \\pi^0}(s)|_{s > s^*} &= c_2 \\Phi_{D^* D^0}(s) , \\\\\n\\varrho_{D^0 D^+ \\gamma}(s)|_{s > s^*} &= c_3 \\Phi_{D^* D^0}(s) ,\n\\end{align*} \\tag{M11a, M11b, M11c}\n\\]\nwhere \\( \\Phi_{D^* D}(s) \\) denotes the two-body phase-space function, the constants \\( c_1, c_2 \\) and \\( c_3 \\) are chosen to ensure the continuity of the functions \\( \\varrho_f(s) \\), and a value of \\( \\sqrt{s^*} = 3.9 \\) GeV/\\( c^2 \\) is used. The functions \\( \\varrho_f(s) \\) are shown in Extended Data Fig. 5. The complex-valued width \\( \\hat{\\Gamma}(s) \\) is defined via the self-energy function \\( \\Sigma(s) \\) [151]\n\\[\ni m_U \\hat{\\Gamma}(s) \\equiv |g|^2 \\Sigma(s) , \\tag{M12}\n\\]\nwhere \\( |g|^2 \\) is again factored out for convenience. The imaginary part of \\( \\Sigma(s) \\) for real physical values of \\( s \\) is computed through the optical theorem as half of the sum of the decay probability to all available channels [152]:\n\\[\n\\Im \\Sigma(s)|_{s = 0^+} = \\frac{1}{2} \\varrho_{\\text{tot}}(s) , \\tag{M13a}\n\\]\n\\[\n\\varrho_{\\text{tot}}(s) \\equiv \\sum_f \\varrho_f(s) . \\tag{M13b}\n\\]\nThe real part of the self-energy function is computed using dispersion Kramers–Kronig relations with a single subtraction [153,154],\n\\[\n\\Re \\Sigma(s)|_{s = 0^+} = \\xi(s) - \\xi(m_f^2) , \\tag{M13c}\n\\]\n\\[\n\\xi(s) = \\frac{s}{2\\pi} \\text{p.v.} \\int_{s_{th}^*}^{+\\infty} \\frac{\\varrho_{\\text{tot}}(s')}{s'(s' - s)} ds' , \\tag{M13d}\n\\]\nwhere the Cauchy principal value (p.v.) integral over \\( \\varrho_{\\text{tot}}(s) \\) is understood as\n\\[\n\\text{p.v.} \\int_{s_{th}^*}^{+\\infty} ds \\, \\varrho_{\\text{tot}}(s) ... \\equiv \\sum_f \\text{p.v.} \\int_{s_f^*}^{+\\infty} ds \\, \\varrho_f(s) ... , \\tag{M14}\n\\]\nand \\( s_f \\) denotes the threshold value for the channel \\( f \\). The subtraction is needed since the integral \\( \\int \\varrho_{\\mathrm{tot}}(s)/s\\,ds \\) diverges. The term \\( \\xi(m_U^2) \\) in Eq. (M13c) corresponds to the choice of subtraction constant such that \\( \\Re \\mathcal{A}_U(m_U^2) = 0 \\). The function \\( \\xi(s) \\) is shown in Extended Data Fig. 6.\n\nSimilar to the Flatté function [107] for large values of the \\( |g| \\) parameter, the \\( \\mathfrak{F}^{\\mathrm{U}} \\) signal profile exhibits a scaling property [104,108]. For large values of the \\( |g| \\) parameter the width approaches asymptotic behaviour, see Extended Data Fig. 7. The unitarised three-body Breit–Wigner function \\( \\mathfrak{F}^{\\mathrm{U}} \\) for \\( \\mathrm{T}_{cc}^+ \\to D^0 D^0 \\pi^+ \\) decays with parameters \\( m_U \\) and \\( |g| \\) obtained from the fit to data is shown in Extended Data Fig. 8. The inset illustrates the similarity of the profile with the single-pole profile in the vicinity of the pole\n\n\\[\n\\sqrt{s} = m - \\frac{i}{2} \\mathfrak{w},\n\\]\n\nwhere \\( m \\) and \\( \\mathfrak{w} \\) are the mode and full width at half maximum, respectively.\n\nAnalytic continuation\n\nEquations (M13) define \\( \\Sigma(s) \\) and the amplitude \\( \\mathcal{A}_U(s) \\) for real values of \\( s \\). Analytic continuation to the whole first Riemann sheet is calculated as\n\n\\[\n\\Sigma(s) = \\frac{s}{2\\pi} \\int_{s_{\\mathrm{th}}}^{+\\infty} \\frac{\\varrho_{\\mathrm{tot}}(s')}{s'(s'-s)}\\,ds' - \\xi\\left(m_U^2\\right),\n\\]\n(M15)\n\nwhere the integral is understood as in Eq. (M14). The search for the resonance pole requires knowledge of the amplitude on the second Riemann sheet denoted by \\( \\mathcal{A}_U^H \\). According to the optical theorem [152], the discontinuity of the inverse amplitude across the unitarity cut is given by \\( i\\,|g|^2\\,\\varrho_{\\mathrm{tot}}(s) \\):\n\n\\[\n\\frac{1}{\\mathcal{A}_U^H(s)} = m_U^2 - s - |g|^2\\,\\Sigma(s) + i\\,|g|^2\\,\\varrho_{\\mathrm{tot}}(s).\n\\]\n(M16)\n\nFor the complex-values \\( s \\), the analytic continuation of \\( \\varrho_{\\mathrm{tot}}(s) \\) is needed: the phase space integral in Eq. (M10) is performed over a two-dimensional complex manifold \\( \\mathcal{D} \\) (see discussion on the continuation in Ref. [155]):\n\n\\[\n\\int_{\\mathcal{D}} |\\mathfrak{m}|^2\\,d\\Phi_3 = \\frac{1}{2\\pi(8\\pi)^2 s} \\int_{(m_2+m_3)^2}^{(\\sqrt{s}-m_1)^2} ds_{23} \\int_{s_{12}^-(s,s_{23})}^{s_{12}^+(s,s_{23})} |\\mathfrak{m}|^2\\,ds_{12},\n\\]\n(M17)\n\nwhere the limits of the second integral represent the Dalitz plot borders [120],\n\n\\[\ns_{12}^{\\pm}(s,s_{23}) = m_1^2 + m_2^2 - \\frac{(s_{23} - s + m_1^2)(s_{23} + m^2 + m_3^2)}{2s_{23}} \\\\\n\\pm \\frac{\\lambda^{1/2}(s_{23}, s, m_1^2)\\lambda^{1/2}(s_{23}, m_2^2, m_3^2)}{2s_{23}}.\n\\]\n(M18)\n\nThe integration is performed along straight lines connecting the end points in the complex plane.\nDD spectra from \\( \\mathrm{T}_{cc}^+ \\to \\mathrm{DD}\\pi/\\gamma \\) decays\n\nThe shapes of the D\\( ^0 \\)D\\( ^0 \\) and D\\( ^+ \\)D\\( ^- \\) mass spectra from \\( \\mathrm{T}_{cc}^+ \\to \\mathrm{DD}\\pi/\\gamma \\) decays are obtained via integration of the \\( |\\mathcal{M}_f|^2 \\) expressions from Eqs. (M6) and (M8) over the s and \\( s_{12} \\) variables with the \\( \\mathrm{T}_{cc}^+ \\) amplitude squared, \\( |\\mathcal{A}_U(s)|^2 \\), from Eq. (M9a):\n\n\\[\nR_f(s_{23}) \\equiv \\int_{(m_1+\\sqrt{s_{23}})^2}^{+\\infty} ds \\; |\\mathcal{A}_U(s)|^2 f_C(s) \\frac{1}{s} \\int_{s_{12}(s,s_{23})}^{s_{12}^+(s,s_{23})} ds_{12} \\; |\\mathcal{M}_f(s, s_{12}, s_{23})|^2 ,\n\\] (M19)\n\nwhere the lower and upper integration limits for \\( s_{12} \\) at fixed s and \\( s_{23} \\) are given in Eq. (M18). The function \\( f_C(s) \\) is introduced to perform a smooth cutoff of the long tail of the \\( \\mathrm{T}_{cc}^+ \\) profile. Cutoffs are chosen to suppress the profile for regions \\( |\\sqrt{s}-m| \\gg w \\), where m and w are the mode and FWHM for the \\( \\mathfrak{F}^U(s) \\) distribution from Table 3. Two cut-off functions \\( f_C(s) \\) are studied:\n\n1. A Gaussian cut-off \\( f_C^G(s) \\) defined as\n\n\\[\nf_C^G(s|x_c, \\sigma_c) = \\begin{cases}\n1 & \\text{for } \\sqrt{s} \\leq x_c ; \\\\\n\\mathrm{e}^{-\\frac{(\\sqrt{s}-x_c)^2}{2\\sigma_c^2}} & \\text{for } \\sqrt{s} > x_c .\n\\end{cases}\n\\] (M20)\n\n2. A power-law cut off \\( f_C^P(s) \\) defined as\n\n\\[\nf_C^P(s|x_c, \\sigma_c, \\nu_c) = \\begin{cases}\n1 & \\text{for } \\sqrt{s} \\leq x_c ; \\\\\n\\left( 1 + \\frac{1}{\\nu_c} \\frac{(\\sqrt{s}-x_c)^2}{\\sigma_c^2} \\right)^{-\\frac{\\nu_c+1}{2}} & \\text{for } \\sqrt{s} > x_c .\n\\end{cases}\n\\] (M21)\n\nFits to the background-subtracted D\\( ^0 \\)D\\( ^0 \\)\\( \\pi^+ \\) mass spectrum using a signal profile of the form \\( \\mathfrak{F}^U(s) \\times f_C(s) \\) show that the parameter \\( \\delta m_U \\) is insensitive to the choice of cut-off function when \\( x_c \\geq m_{D^0} + m_{D^+} \\) and \\( \\sigma_c \\geq 1 \\) MeV/\\( c^2 \\). The power-law cut-off function \\( f_C^P(s) \\) with parameters \\( x_c = m_{D^0} + m_{D^+} \\) and \\( \\sigma_c = 1 \\) MeV/\\( c^2 \\) is chosen. The shapes for the D\\( ^0 \\)D\\( ^0 \\) and D\\( ^+ \\)D\\( ^0 \\) mass distributions are defined as\n\n\\[\n\\begin{align*}\nF_{D^0D^0}(m) &= m R_{D^0D^0\\pi^+}(m^2) , \\\\\nF_{D^+D^0}(m) &= m R_{D^+D^0\\pi^+}(m^2) + m R_{D^+D^0\\gamma}(m^2) .\n\\end{align*}\n\\] (M22a)(M22b)\n\nLow-energy scattering amplitude\n\nThe unitarized Breit–Wigner amplitude is formally similar to the low-energy expansion given by Eq. (10) once the factor \\( \\frac{1}{2} |g|^2 \\) is divided out:\n\n\\[\n\\begin{align*}\n\\mathcal{A}_{NR}^{-1} &= \\frac{1}{a} + r \\frac{k^2}{2} - i k + \\mathcal{O}(k^4) , \\\\\n\\frac{2}{|g|^2} \\mathcal{A}_U^{-1} &= - [\\xi(s) - \\xi(m_U^2)] + 2 \\frac{m_U^2 - s}{|g|^2} - i \\varrho_{tot}(s) .\n\\end{align*}\n\\] (M23a)(M23b)\n\nThe function \\( i \\varrho_{tot}(s) \\) matches \\( i k \\) up to a slowly varying energy factor that can be approximated by a constant in the threshold region. The proportionality factor w has\nthe dimension of an inverse mass and is found by matching the decay probability to the two-body phase-space expression:\n\n\\[\nw = \\frac{24\\pi}{m_{D^{*+}} + m_{D^0}} \\frac{1}{c_1},\n\\]\n\nwhere \\( c_1 \\) is a coefficient computed in Eq. (M11). The comparison of \\( \\mathcal{A}_{NR}^{-1} \\) and \\( \\mathcal{A}_U^{-1} \\times 2w/|g|^2 \\) that validates the matching is shown in Extended Data Fig. 9.\n\nThe inverse scattering length is defined as the value of the amplitude in Eq. (M23a) at the D^{*+}D^0 threshold:\n\n\\[\n\\frac{1}{a} = -\\frac{1}{w} \\left\\{ [\\xi(s_{th}) - \\xi(m_U^2)] + i q_{tot}(s_{th}) \\right\\}.\n\\]\n\nThe imaginary part is fully determined by the available decay channels, while the real part depends on the constant \\( \\xi(m_U^2) \\) adjusted in the fit. The quadratic term, \\( k^2 \\) in Eq. (M23a), corresponds to the linear correction in \\( s \\) since \\( k^2 = (s - s_{th})/4 \\) for the non-relativistic case. Hence, the slope of the linear term in the \\( \\mathcal{A}_U^{-1} \\) amplitude is related to the effective range as follows:\n\n\\[\nr = -\\frac{1}{w} \\frac{16}{|g|^2}.\n\\]\n\nMass splitting for the \\( \\hat{T}_{cc} \\) isotriplet\n\nWhile the degrees of freedom of the light diquark for the isoscalar \\( T_{cc}^+ \\) state are similar to those for the \\( \\overline{\\Lambda}_c^- \\) state, for the \\( \\hat{T}_{cc} \\) isotriplet (\\( \\hat{T}_{cc}^0, \\hat{T}_{cc}^+, \\hat{T}_{cc}^{++} \\)) the light diquark degrees of freedom would be similar to those for the \\( \\Sigma_c \\) (anti)triplet. Assuming that the difference in the light quark masses, the Coulomb interaction of light quarks in the diquark, and the Coulomb interaction of the light diquark with the c-quark are responsible for the observed mass splitting in the \\( \\Sigma_c \\) isotriplet, the masses for the \\( \\Sigma_c \\) states can be written as\n\n\\[\n\\begin{align*}\nm_{\\Sigma_c^{++}} &= m_\\Sigma + m_u + m_u - a\\, q_u q_u - b\\, q_c (q_u + q_u) , \\\\\nm_{\\Sigma_c^+} &= m_\\Sigma + m_u + m_d - a\\, q_u q_d - b\\, q_c (q_u + q_d) , \\\\\nm_{\\Sigma_c^0} &= m_\\Sigma + m_d + m_d - a\\, q_d q_d - b\\, q_c (q_d + q_d) ,\n\\end{align*}\n\\]\n\nwhere \\( m_\\Sigma \\) is a common mass parameter; the second and third terms describe the contribution from the light quark masses, \\( m_u \\) and \\( m_d \\), into the mass splitting; terms proportional to \\( a \\) describe Coulomb interactions of light quarks in the diquark; terms proportional to \\( b \\) describe the Coulomb interactions of the diquark with the c-quark; and \\( q_q \\) denotes the charge of the q-quark. Similar expressions can be written for the \\( \\hat{T}_{cc} \\) isotriplet:\n\n\\[\n\\begin{align*}\nm_{\\hat{T}_{cc}^0} &= m_{\\hat{T}_{cc}} + m_u + m_u - a'\\, q_{\\pi q_{\\pi}} - b'\\, q_{cc} (q_{\\pi} + q_{\\pi}) , \\\\\nm_{\\hat{T}_{cc}^+} &= m_{\\hat{T}_{cc}} + m_u + m_d - a'\\, q_{\\pi q_{d}} - b'\\, q_{cc} (q_{\\pi} + q_{d}) , \\\\\nm_{\\hat{T}_{cc}^{++}} &= m_{\\hat{T}_{cc}} + m_d + m_d - a'\\, q_{d q_{d}} - b'\\, q_{cc} (q_{d} + q_{d}) ,\n\\end{align*}\n\\]\n\nwhere \\( m_{\\hat{T}_{cc}} \\) is the common mass parameter, \\( q_{\\pi} = -q_c \\) and \\( q_{cc} = 2q_c \\) is the charge of a cc diquark. Using the known masses of the light quarks and \\( \\Sigma_c \\) states [83] and taking \\( a' = a \\) and \\( b' = b \\), the mass splitting for the \\( \\hat{T}_{cc} \\) isotriplet is estimated to be\n\n\\[\nm_{\\hat{T}_{cc}^0} - m_{\\hat{T}_{cc}^+} = -5.9 \\pm 1.3\\ \\mathrm{MeV}/c^2 ,\n\\]\n\\[\nm_{\\tilde{\\Sigma}^{++}_{cc}} - m_{\\tilde{\\Sigma}^{+}_{cc}} = \\quad 7.9 \\pm 1.0\\ \\mathrm{MeV}/c^2 .\n\\] (M29b)\n\nThe validity of this approach is tested by comparing the calculated mass splitting between \\( \\Sigma_b^+ \\) and \\( \\Sigma_b^- \\) states of \\( -6.7 \\pm 0.7\\ \\mathrm{MeV}/c^2 \\) with the measured value of \\( -5.1 \\pm 0.2\\ \\mathrm{MeV}/c^2 \\) [83]. Based on the small observed difference, an addition uncertainty of \\( 0.8\\ \\mathrm{MeV}/c^2 \\) is added in quadrature to the results from Eq. (M29), and finally one gets\n\n\\[\nm_{\\tilde{\\Sigma}^{0}_{cc}} - m_{\\tilde{\\Sigma}^{+}_{cc}} = \\quad -5.9 \\pm 1.5\\ \\mathrm{MeV}/c^2 ,\n\\] (M30a)\n\n\\[\nm_{\\tilde{\\Sigma}^{++}_{cc}} - m_{\\tilde{\\Sigma}^{+}_{cc}} = \\quad 7.9 \\pm 1.3\\ \\mathrm{MeV}/c^2 .\n\\] (M30b)\n\nThese results agree within the assigned uncertainty with results based on a more advanced model from Ref. [156].\nExtended Data\n\n![Two-dimensional mass distributions for selected D^0D^0π^+, D^0D^0 and D^0D^+ combinations.](page_324_186_957_670.png)\n\nExtended Data Fig. 1: Two-dimensional mass distributions for selected \\( \\mathrm{D}^0\\mathrm{D}^0\\pi^+ \\), \\( \\mathrm{D}^0\\mathrm{D}^0 \\) and \\( \\mathrm{D}^0\\mathrm{D}^+ \\) combinations. Two-dimensional mass distributions for \\( \\mathrm{D}^0 \\) and \\( \\mathrm{D}^+ \\) candidates from selected (a) \\( \\mathrm{D}^0\\mathrm{D}^0\\pi^+ \\), (b) \\( \\mathrm{D}^0\\mathrm{D}^0 \\) and (c) \\( \\mathrm{D}^0\\mathrm{D}^+ \\) combinations. \\( K_{1/2} \\) and \\( \\pi_{1/2} \\) correspond to daughters of the first/second \\( \\mathrm{D}^0 \\) candidate in \\( \\mathrm{D}^0\\mathrm{D}^0 \\) and \\( \\mathrm{D}^0\\mathrm{D}^0\\pi^+ \\) final states.\nExtended Data Fig. 2: Mass distributions for \\( D^0 D^0 \\pi^+ \\) combinations with fake \\( D^0 \\) candidates. Mass distributions for \\( D^0 D^0 \\pi^+ \\) combinations with (a) one true and one fake \\( D^0 \\) candidate, (b) two fake \\( D^0 \\) candidates and (c) at least one fake \\( D^0 \\) candidate. Results of the fits with background-only functions are overlaid.\n\n![Mass distributions for D^0D^0π^+ combinations with fake D^0 candidates](page_312_670_968_482.png)\nExtended Data Fig. 3: Mass distributions for \\( D^0 \\overline{D}^0 \\pi^+ \\) and \\( D^0 \\overline{D}^0 \\pi^- \\) candidates. Background-subtracted \\( D^0 D^0 \\pi^+ \\) and \\( D^0 \\overline{D}^0 \\pi^- \\) mass distributions.\n\n![Mass distributions for D^0D^0\\pi^+ and D^0\\overline{D}^0\\pi^- candidates. Background-subtracted D^0D^0\\pi^+ and D^0\\overline{D}^0\\pi^- mass distributions.](page_374_629_1057_682.png)\nExtended Data Fig. 4: Mass distributions for D^0D^+ and D^0D^- candidates. Background-subtracted D^0D^+ and D^0D^- mass distributions.\n\n![Mass distributions for D^0D^+ and D^0D^- candidates. Background-subtracted D^0D^+ and D^0D^- mass distributions.](page_382_613_1097_563.png)\nExtended Data Fig. 5: Three-body phase-space functions \\( \\varrho_f(s) \\). Three-body phase-space functions \\( \\varrho_f(s) \\) with (left) linear and (right) logarithmic vertical-axis scale; (red) \\( T_{cc}^+ \\to D^0 D^0 \\pi^+ \\), (blue) \\( T_{cc}^+ \\to D^+ D^0 \\pi^0 \\) and (green) \\( T_{cc}^+ \\to D^+ D^0 \\gamma \\). The sum, \\( \\varrho_{tot}(s) \\), is shown with a black line. The two-body \\( D^* D \\) phase-space shapes are shown by the dashed lines and are different from the \\( \\varrho_f(s) \\) functions only in the vicinity of the thresholds or below them. Vertical dash-dotted line indicates \\( \\sqrt{s^*} = 3.9 \\) GeV.\n\nExtended Data Fig. 6: Function \\( \\xi(s) \\). Function \\( \\xi(s) \\) with (left) linear and (right) logarithmic vertical-axis scale is shown with a red line. The three-body phase-space function \\( \\varrho_{tot}(s) \\) is shown for comparison with a dashed line.\nExtended Data Fig. 7: Scaling behaviour of the \\( \\mathcal{F}^U \\) profile. The full width at half maximum \\( w \\) as a function of the \\( |g| \\) parameter for a fixed value of the \\( \\delta m_U \\) parameter \\( \\delta m_U = -359\\,\\mathrm{keV}/c^2 \\). The horizontal dashed blue line indicates the value of \\( w \\) corresponding to the best fit parameters.\n\n![Scaling behaviour of the \\( \\mathcal{F}^U \\) profile. The full width at half maximum \\( w \\) as a function of the \\( |g| \\) parameter for a fixed value of the \\( \\delta m_U \\) parameter \\( \\delta m_U = -359\\,\\mathrm{keV}/c^2 \\). The horizontal dashed blue line indicates the value of \\( w \\) corresponding to the best fit parameters.](page_312_682_1042_627.png)\nExtended Data Fig. 8: Unitarised three-body Breit–Wigner function \\( \\mathfrak{F}^U \\). Unitarised three-body Breit–Wigner function \\( \\mathfrak{F}^U \\) for \\( T_{cc}^+ \\to D^0 D^0 \\pi^+ \\) decays (red line) for a large value of the \\( |g| \\) parameter and \\( \\delta m_U = -359\\,\\mathrm{keV}/c^2 \\), normalized to unity for \\( \\delta m_{D^0 D^0 \\pi^+} = \\delta m_U \\). Top inset shows a zoomed region with overlaid (blue dashed line) *single-pole* profile with \\( \\sqrt{s} = m - \\frac{i}{2}\\Gamma \\), and (thin green line) three-body Breit–Wigner profile with \\( |g| = 5.1\\,\\mathrm{GeV} \\). Bottom inset shows the \\( \\mathfrak{F}^U \\) profile in log-scale. Vertical dashed lines indicate (left-to-right) \\( D^{*+} D^0 \\) and \\( D^* D^0 \\) mass thresholds.\n\n![Unitarised three-body Breit–Wigner function plot](page_246_670_1092_670.png)\nExtended Data Fig. 9: Comparison of the \\( \\mathcal{A}_U \\) and \\( \\mathcal{A}_{NR} \\) amplitudes. The real and imaginary parts of the inverse \\( \\mathcal{A}_U \\) and \\( \\mathcal{A}_{NR} \\) amplitudes. 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Congedo19,c, A. Contu27, N. Cooke53, G. Coombs39, I. Corredoira 46,\nG. Corti48, C.M. Costa Sobral56, B. Couturier48, D.C. Craik64, J. Crkovska67, M. Cruz Torres1,\nR. Curries58, C.L. Da Silva57, S. Dadabaevas3, L. Dai71, E. Dall’Occo15, J. Dalseno46,\nC. D’Ambrosio48, A. Danilina41, P. d’Argent48, J.E. Davies62, A. Davis62,\nO. De Aguilar Francisco62, K. De Bruyn79, S. De Capua62, M. De Cian49, J.M. De Miranda1,\nL. De Paula2, M. De Serio19,c, D. De Simone50, P. De Simone23, F. De Vellis15, J.A. de Vries80,\nC.T. Dean67, F. Debernardis19,c, D. Decamp8, V. Dediu10, L. Del Buono13, B. Delaney55,\nH.-P. Dembinski15, A. Dendek34, V. Denysenko50, D. Derkach82, O. Deschamps9, F. Desse11,\nF. Dettori27,e, B. Dey77, A. Di Cicco23, P. Di Nezza23, S. Didenko83, L. Dieste Maronas46,\nH. Dijkstra48, V. Dobishuk52, C. Dong3, A.M. Donohoe18, F. Dordei27, A.C. dos Reis1,\nL. Douglas59, A. Dovbnya51, A.G. Downes8, M.W. Dudek25, L. Dufour48, V. Duk78,\nP. Durante48, J.M. Durham67, D. Dutta62, A. Dziurda35, A. Dzyuba38, S. Easo57, U. Egede69,\nV. Egorychev41, S. Eidelman43,u,i, S. Eisenhardt58, S. Ek-In49, L. Eklund59,86, S. Ely68,\nA. Ene37, E. Epple67, S. Escher14, J. Eschle50, S. Esen13, T. Evans48, A. Falabella20, J. Fan3,\nY. Fan6, B. Fang73, S. Farry60, D. Fazzini26,j, M. Feó48, A. Fernandez Prieto46, A.D. Fernez66,\nF. Ferrari20,d, L. Ferreira Lopes49, F. Ferreira Rodrigues2, S. Ferreres Sole32, M. Ferrillo50,\nM. Ferro-Luzzi48, S. Filippov39, R.A. Fini19, M. Fiorini21,f, M. Firlej34, K.M. Fischer63,\nD.S. Fitzgerald87, C. Fitzpatrick62, T. Fiutowski34, A. Fkiaras48, F. Fleuret12, M. Fontana13, F. Fontanelli24,h, R. Forty48, D. Foulds-Holt55, V. Franco Lima60, M. Franco Sevilla66, M. Frank48, E. Franzoso21, G. Frau17, C. Frei48, D.A. Friday59, J. Fu6, Q. Fuhring15, E. Gabriel32, G. Galati19,e, A. Gallas Torreia46, D. Galli20,d, S. Gambetta58,48, Y. Gan3, M. Gandelman2, P. Gandini25, Y. Gao5, M. Garau27, L.M. Garcia Martin56, P. Garcia Moreno45, J. García Pardinas26,j, B. Garcia Plana46, F.A. Garcia Rosales12, L. Garrido45, C. Gaspar48, R.E. Geertsema32, D. Gerick17, L.L. Gerken15, E. Gersabeck62, M. Gersabeck62, T. Gershon56, D. Gerstel10, L. Giambastiani28, V. Gibson55, H.K. Giemza36, A.L. Gilman63, M. Giovannetti23,p, A. Gioventù46, P. Gironella Gironeil45, L. Giubega37, C. Giugliano21,f,48, K. Gizdov58, E.L. Gkougkousis48, V.V. Gligorov13, C. Göbel70, E. Golobarbes85, D. Golubkov41, A. Golutvin61,83, A. Gomes1,a, S. Gomez Fernandez45, F. Goncalves Abrantes63, M. Goncerz35, G. Gong3, P. Gorbounov41, I.V. Gorelov40, C. Gott126, E. Govorkova48, J.P. Grabowski17, T. Grammatico13, L.A. Granado Cardoso48, E. Graugès46, E. Graverini49, G. Graziani22, A. Greco37, L.M. Greeven32, N.A. Grieser48, L. Grillo62, S. Gromov83, B.R. Gruberg Cazon63, C. Gu3, M. Guarise21, M. Guittiere11, P. A. Günther17, E. Gushchin39, A. Guth14, Y. Guz44, T. Gys48, T. Hadavizadeh69, G. Haefeli49, C. Haen48, J. Hainberger48, T. Halewood-leagas60, P.M. Hamilton66, J.P. Hammerich60, Q. Han7, X. Han17, T.H. Hancock63, E.B. Hansen62, S. Hansmann-Menzemer17, N. Harnew63, T. Harrison60, C. Hasse48, M. Hatch48, J. He6,b, M. Hecker61, K. Heijhoff32, K. Heinicke15, A.M. Hennequin48, K. Hennessy60, L. Henry48, J. Heuel14, A. Hicheur2, D. Hill49, M. Hilton62, S.E. Hollitt15, R. Hou7, Y. Hou8, J. Hu17, J. Hu72, W. Hu7, X. Hu3, W. Huang6, X. Huang73, W. Hulsbergen32, R.J. Hunter56, M. Hushchyn82, D. Hutchcroft60, D. Hynds32, P. Ibis15, M. Idzik34, D. Ilin38, P. Ilten65, A. Inglessi38, A. Ishteev83, K. Ivshin38, R. Jacobsson48, H. Jage14, S. Jakobsen48, E. Jans32, B.K. Jashal47, A. Jawahery66, V. Jevtic15, F. Jiang3, M. John63, D. Johnson48, C.R. Jones55, T.P. Jones56, B. Jost48, N. Jurik48, S.H. Kalavan Kadavath34, S. Kandybei51, Y. Kang3, M. Karacson18, M. Karpov82, F. Keizer18, D.M. Keller68, M. Kenzie56, T. Ketel33, B. Khanji15, A. Kharisova84, S. Kholodenko44, T. Kirn14, V.S. Kirsebom49, O. Kitoumi64, S. Klaver32, N. Kleijn29, K. Klimaszewski36, M.R. Kmiec36, S. Koliev52, A. Kondybayeva83, A. Konoplyannikov41, P. Kopczewicz34, R. Kopecnak17, P. Koppenburg32, M. Korolev40, I. Kostiuk32,52, O. Kot52, S. Kotriakhova21,38, P. Kravchenko38, L. Kravchuk39, R.D. Krawczyk48, M. Kreps56, F. Kress61, S. Kretzschmar14, P. Krokovny43,u, W. Krupa34, W. Krzemien36, M. Kucharczyk35, V. Kudryavtsev43,u, H.S. Kuindersma32,33, G.J. Kunde67, T. Kvaratskheliya41, D. Lacarrere48, G. Lafferty62, A. Lat27, A. Lampis27, D. Lancieneris50, J.J. Lane52, R. Lane54, G. Lanfranchi23, C. Langenbruch14, J. Langer15, O. Lantwin83, T. Latham56, F. Lazzari29,q, R. Le Gac10, S.H. Lee87, R. Lefèvre9, A. Leflat40, S. Legotin83, O. Leroy10, T. Lesiak35, B. Leverington17, H. Li72, P. Li17, S. Li7, Y. Li4, Y. Li4, Z. Li68, X. Liang68, T. Lin61, R. Lindner48, V. Lisovskyi15, R. Litvinov27, G. Liu72, H. Liu6, Q. Liu6, S. Liu4, A. Lobo Salvia45, A. Loi27, J. Lomba Castro46, I. Longstaff50, J.H. Lopes2, S. Lopez Solino46, G.H. Lovell55, Y. Lu4, C. Lucarelli22,g, D. Lucchesi28,l, S. Luchuk39, M. Lucio Martinez32, V. Lukashenko32,52, Y. Luo3, A. Lupato02, E. Luppi21,f, O. Lupton56, A. Lusiani29,m, X. Lyu6, L. Ma4, R. Ma6, S. Maccolini20,d, F. Machefert11, F. Maciuc37, V. Macko49, P. Mackowiak15, S. Maddrell-Mander54, O. Madejczyk34, L.R. Madhan Mohan54, O. Maev38, A. Maevskiy82, D. Maisuzenko38, M.W. Majewski34, J.J. Malczewski35, S. Malde63, B. Malecki48, A. Malinin81, T. Maltsev43,u, H. Malygina17, G. Manca27,e, G. Mancinelli10, D. Manuzzi20,d, D. Marangotto25,i, J. Maratas9,s, J.F. Marchand8, U. Marconi20, S. Mariani22,g, C. Marin Benito48, M. Marinangeli49, J. Marks17, A.M. Marshall54, P.J. Marshall60, G. Martelli78, G. Martellotti30, L. Martinazzoli48,j, M. Martinelli26,j, D. Martinez Santos46, F. Martinez Vidal47, A. Massafferri1, M. Materok14, R. Matev48, A. Mathad50, V. Matiuin11, C. Matteuzzi26, K.R. Mattioli87, A. Mauri32, E. Maurice12, J. Mauricio45, M. Mazurek48, M. McCann61, L. McConnell18, T.H. McGrath02, N.T. Mchugh99, A. McNab02, R. McNulty18,\nJ.V. Mead60, B. Meadows65, G. Meier15, N. Meinert76, D. Melnychuk36, S. Meloni26,j, M. Merk32,80, A. Merli25, L. Meyer Garcia2, M. Mikhasenko48, D.A. Milanes74, E. Millard56, M. Milovanovic48, M.-N. Minard8, A. Minotti26,j, L. Minzioni21,f, S.E. Mitchell58, B. Mitreska62, D.S. Mitzel15, A. Mödden 15, R.A. Mohammed63, R.D. Moise61, S. Mokhnenko82, T. Mombächer46, I.A. Monroy74, S. Monteil9, M. Morandin28, G. Morello23, M.J. Moreno29,m, J. Moron34, A.B. Morris75, A.G. Morris56, R. Mountain68, H. Mu3, F. Muheim58,48, M. Mulder48, D. Müller48, K. Müller50, C.H. Murphy63, D. Murray62, P. Muzzetto27,48, P. Naik54, T. Nakada49, R. Nandakumar57, T. Nanut49, I. Nasteva2, M. Needham58, I. Neri21, N. Neri25,i, S. Neubert75, N. Neufeld48, R. Newcombe61, E.M. Niel11, S. Nieswand14, N. Nikitin40, N.S. Nolte64, C. Normand8, C. Nunez87, A. Oblakowska-Mucha34, V. Obraztsov44, T. Oeser14, D.P. O'Hanlon54, S. Okamura21, R. Oldeman27,e, F. Oliva58, M.E. Olivares68, C.J.G. Onderwater79, R.H. O'neil58, J.M. Otalora Goicochea2, T. Ovsiannikova41, P. Owen50, A. Oyanguren47, K.O. Paddeken75, B. Pagare56, P.R. Pais48, T. Pajero63, A. Palano19, M. Palutan23, Y. Pan62, G. Panshin84, A. Papaneistis57, M. Pappagallo19,c, L.L. Pappalardo21,f, C. Pappenheimer65, W. Parker66, C. Parkes62, B. Passalacqua21, G. Passaleva22, A. Pastore19, M. Patel91, C. Patrignani20,d, C.J. Pawley80, A. Pearce48, A. Pellegrino32, M. Pepe Altarelli48, S. Perazzini20, D. Pereina41, A. Pereiro Castro46, P. Perret9, M. Petric59,48, K. Petridis54, A. Petrolini24,h, A. Petrov81, S. Petruccii58, M. Petruzzo25, T.T.H. Pham68, L. Pica29,m, M. Piccini78, B. Pietrzyk8, G. Pietrzyk49, M. Pili63, D. Pinci30, F. Pisani48, M. Pizzichemi26,48,j, Resmi P.K10, V. Placinta37, J. Plews53, M. Plo Casasus46, F. Polci13, M. Poli Lener23, M. Poliakova68, A. Poluektov10, N. Polukhina83,t, I. Polyakov68, E. Polycarpo2, S. Ponce48, D. Popov6,48, S. Popov42, S. Poslavskii44, K. Prasanth35, L. Promberger48, C. Prouve46, V. Pugatch52, V. Puill11, H. Puller63, G. Punzi29,n, H. Qi3, W. Qian6, J. Qin6, N. Qin3, R. Quagliani49, B. Quintana8, N.V. Raab18, R.I. Rabadan Trejo6, B. Rachwal34, J.H. Rademacker54, M. Rama29, M. Ramos Pernas56, M.S. Rangel2, F. Ratnikov42,82, G. Raven33, M. Reboud8, F. Redi49, F. Reiss62, C. Remon Alepuz47, Z. Ren3, V. Renaudin63, R. Ribatti29, S. Ricciardi57, K. Rinnert60, P. Robbe11, G. Robertson58, A.B. Rodrigues49, E. Rodrigues60, J.A. Rodriguez Lopez74, E.R.R. Rodriguez Rodriguez46, A. Rollings63, P. Roloff88, V. Romanovsky44, M. Romero Lamas46, A. Romero Vidal46, J.D. Roth87, M. Rotondo23, M.S. Rudolph68, T. Ruf18, R.A. Ruiz Fernandez46, J. Ruiz Vidal47, A. Ryzhikov82, J. Ryzka34, J.J. Saborido Silva46, N. Sagidova38, N. Sahoo56, B. Saitta27,e, M. Salomoni48, C. Sanchez Gras32, R. Santacesaria30, C. Santamarina Rios46, M. Santimaria23, E. Santovetti31,p, D. Saranin83, G. Sarpis14, M. Sarpis75, A. Sarti30, C. Satriano30,o, A. Satta31, M. Saur15, D. Savrina41,40, H. Szak9, L.G. Scantlebury Smead63, A. Scarabotto13, S. Schael14, S. Scherf60, M. Schiller59, H. Schindler48, M. Schnelling16, B. Schmidt48, S. Schmitt14, O. Schneider49, A. Schopper48, M. Schubiger62, S. Schulze49, M.H. Schune11, R. Schwemmer48, B. Sciascia23,48, S. Sellam46, A. Semennikov41, M. Senghi Soares33, A. Sergi24,h, N. Serra50, L. Sestini28, A. Seuthe15, Y. Shang8, D.M. Shangase37, M. Shapkin44, I. Shechmerov83, L. Shchutska49, T. Shears60, L. Shekhtman43,u, Z. Shen5, V. Shevchenko81, E.B. Shields26,j, Y. Shimizu11, E. Shmanin83, J.D. Shupperd68, B.G. Siddi21, R. Silva Coutinho50, G. Simi28, S. Simonc19,c, N. Skidmore62, T. Skwarnicki68, M.W. Slater53, I. Slazyk21,f, J.C. Smallwood63, J.G. Smeaton55, A. Smetkina41, E. Smith50, M. Smith61, A. Snoch32, M. Soares20, L. Soares Lavra9, M.D. Sokoloff65, F.J.P. Soler59, A. Solovev38, I. Solovyev38, F.L. Souza De Almeida2, B. Souza De Paula2, B. Spaan15, E. Spadaro Norella25, P. Spradlin59, F. Stagni48, M. Stahl65, S. Stahl48, S. Stanislaus63, O. Steinkamp50,83, O. Stenyakin44, H. Stevens15, S. Stone68, M. Straticiuc37, D. Strekalina83, F. Suljik63, J. Sun27, L. Sun73, Y. Sun66, P. Svihra62, P.N. Swallow53, K. Swientek34, A. Szabelski36, T. Szumlak34, M. Szymanski48, S. Tancaja62, A.R. Tanner54, M.D. Tat63, A. Terentev83, F. Teubert48, E. Thomas48, D.J.D. Thompson53, K.A. Thomson60, V. Tisserand9, S. T'Jampens8, M. Tobin4, L. Tomassetti21,f, X. Tong5, D. Torres Machado4, D.Y. Tou13, E. Trifonova83, C. Tripli49,\nG. Tuci6, A. Tully49, N. Tuning32,48, A. Ukleja36, D.J. Unverzagt17, E. Ursov83, A. Usachov32, A. Ustyuzhanin42,82, U. Uwer17, A. Vagner84, V. Vagnon20, A. Valassi48, G. Valenti20, N. Valls Canudas85, M. van Beuzekom32, M. Van Dijk49, E. van Herwijnen83, C.B. Van Hulse18, M. van Veghel79, R. Vazquez Gomez45, P. Vazquez Regueiro46, C. Vázquez Sierra48, S. Vecchi21, J.J. Velthuis54, M. Veltri22,r, A. Venkateswaran68, M. Veronesi32, M. Vesterinen56, D. Vieira65, M. Vieites Diaz49, H. Viemann76, X. Vilasis-Cardona85, E. Vilella Figueras60, A. Villa20, P. Vincent13, F.C. Volle11, D. Vom Bruch10, A. Vorobyev38, V. Vorobyev43,u, N. Voropaev38, K. Vos80, R. Waldi17, J. Walsh29, C. Wang17, J. Wang5, J. Wang4, J. Wang3, J. Wang73, M. Wang3, R. Wang54, Y. Wang7, Z. Wang50, Z. Wang3, Z. Wang6, J.A. Ward56, N.K. Watson53, S.G. Weber13, D. Websdale61, C. Weisser64, B.D.C. Westhenry54, D.J. White62, M. Whitehead54, A.R. Wiederhold56, D. Wiedner15, G. Wilkinson63, M. Wilkinson68, I. Williams55, M. Williams64, M.R.J. Williams58, F.F. Wilson57, W. Wislicki36, M. Witek35, L. Witola17, G. Wormser11, S.A. Wotton55, H. Wu68, K. Wyllie48, Z. Xiang6, D. Xiao7, Y. Xie7, A. Xu5, J. Xu6, L. Xu3, M. Xu7, Q. Xu6, Z. Xu5, Z. Xu6, D. Yang3, S. Yang6, Y. Yang6, Z. Yang5, Z. Yang66, Y. Yao68, L.E. Yeomans60, H. Yin7, J. Yu71, X. Yuan68, O. Yushchenko44, E. Zaffaroni49, M. Zavertyaev16,t, M. Zdybal35, O. Zenaiev48, M. Zeng3, D. Zhang7, L. Zhang3, S. Zhang71, S. Zhang5, Y. Zhang5, Y. Zhang63, A. Zharkova83, A. Zhelezov17, Y. Zheng6, T. Zhou5, X. Zhou6, Y. Zhou6, V. Zhokhovska11, X. Zhu3, X. Zhu7, Z. Zhu6, V. Zhukov14,40, J.B. Zonneveld58, Q. Zou4, S. Zucchelli20,d, D. Zuliani28, G. Zunic62.\n\n1 Centro Brasileiro de Pesquisas Físicas (CBPF), Rio de Janeiro, Brazil\n2 Universidade Federal do Rio de Janeiro (UFRJ), Rio de Janeiro, Brazil\n3 Center for High Energy Physics, Tsinghua University, Beijing, China\n4 Institute Of High Energy Physics (IHEP), Beijing, China\n5 School of Physics State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing, China\n6 University of Chinese Academy of Sciences, Beijing, China\n7 Institute of Particle Physics, Central China Normal University, Wuhan, Hubei, China\n8 Univ. Savoie Mont Blanc, CNRS, IN2P3-LAPP, Annecy, France\n9 Université Clermont Auvergne, CNRS/IN2P3, LPC, Clermont-Ferrand, France\n10 Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France\n11 Université Paris-Saclay, CNRS/IN2P3, IJCLab, Orsay, France\n12 Laboratoire Leprince-Ringuet, CNRS/IN2P3, Ecole Polytechnique, Institut Polytechnique de Paris, Palaiseau, France\n13 LPNHE, Sorbonne Université, Paris Diderot Sorbonne Paris Cité, CNRS/IN2P3, Paris, France\n14 I. Physikalisches Institut, RWTH Aachen University, Aachen, Germany\n15 Fakultät Physik, Technische Universität Dortmund, Dortmund, Germany\n16 Max-Planck-Institut für Kernphysik (MPIK), Heidelberg, Germany\n17 Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany\n18 School of Physics, University College Dublin, Dublin, Ireland\n19 INFN Sezione di Bari, Bari, Italy\n20 INFN Sezione di Bologna, Bologna, Italy\n21 INFN Sezione di Ferrara, Ferrara, Italy\n22 INFN Sezione di Firenze, Firenze, Italy\n23 INFN Laboratori Nazionali di Frascati, Frascati, Italy\n24 INFN Sezione di Genova, Genova, Italy\n25 INFN Sezione di Milano, Milano, Italy\n26 INFN Sezione di Milano-Bicocca, Milano, Italy\n27 INFN Sezione di Cagliari, Monserrato, Italy\n28 Università degli Studi di Padova, Università e INFN, Padova, Padova, Italy\n29 INFN Sezione di Pisa, Pisa, Italy\n30 INFN Sezione di Roma La Sapienza, Roma, Italy\n31 INFN Sezione di Roma Tor Vergata, Roma, Italy\n32 Nikhef National Institute for Subatomic Physics, Amsterdam, Netherlands\n33 Nikhef National Institute for Subatomic Physics and VU University Amsterdam, Amsterdam, Netherlands\n34 AGH - University of Science and Technology, Faculty of Physics and Applied Computer Science, Kraków, Poland\n35 Henryk Niewodniczanski Institute of Nuclear Physics Polish Academy of Sciences, Kraków, Poland\n36 National Center for Nuclear Research (NCBJ), Warsaw, Poland\n37 Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest-Magurele, Romania\n38 Petersburg Nuclear Physics Institute NRC Kurchatov Institute (PNPI NRC KI), Gatchina, Russia\n39 Institute for Nuclear Research of the Russian Academy of Sciences (INR RAS), Moscow, Russia\n40 Institute of Nuclear Physics, Moscow State University (SINP MSU), Moscow, Russia\n41 Institute of Theoretical and Experimental Physics NRC Kurchatov Institute (ITEP NRC KI), Moscow, Russia\n42 Yandex School of Data Analysis, Moscow, Russia\n43 Budker Institute of Nuclear Physics (SB RAS), Novosibirsk, Russia\n44 Institute for High Energy Physics NRC Kurchatov Institute (IHEP NRC KI), Protvino, Russia, Protvino, Russia\n45 ICCUB, Universitat de Barcelona, Barcelona, Spain\n46 Instituto Galego de Física de Altas Enerxías (IGFAE), Universidade de Santiago de Compostela, Santiago de Compostela, Spain\n47 Instituto de Física Corpuscular, Centro Mixto Universidad de Valencia - CSIC, Valencia, Spain\n48 European Organization for Nuclear Research (CERN), Geneva, Switzerland\n49 Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland\n50 Physik-Institut, Universität Zürich, Zürich, Switzerland\n51 NSC Kharkiv Institute of Physics and Technology (NSC KIPT), Kharkiv, Ukraine\n52 Institute for Nuclear Research of the National Academy of Sciences (KINR), Kyiv, Ukraine\n53 University of Birmingham, Birmingham, United Kingdom\n54 H.H. Wills Physics Laboratory, University of Bristol, Bristol, United Kingdom\n55 Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom\n56 Department of Physics, University of Warwick, Coventry, United Kingdom\n57 STFC Rutherford Appleton Laboratory, Didcot, United Kingdom\n58 School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom\n59 School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom\n60 Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom\n61 Imperial College London, London, United Kingdom\n62 Department of Physics and Astronomy, University of Manchester, Manchester, United Kingdom\n63 Department of Physics, University of Oxford, Oxford, United Kingdom\n64 Massachusetts Institute of Technology, Cambridge, MA, United States\n65 University of Cincinnati, Cincinnati, OH, United States\n66 University of Maryland, College Park, MD, United States\n67 Los Alamos National Laboratory (LANL), Los Alamos, United States\n68 Syracuse University, Syracuse, NY, United States\n69 School of Physics and Astronomy, Monash University, Melbourne, Australia, associated to 56\n70 Pontifícia Universidade Católica do Rio de Janeiro (PUC-Rio), Rio de Janeiro, Brazil, associated to 2\n71 Physics and Micro Electronic College, Hunan University, Changsha City, China, associated to 7\n72 Guangdong Provincial Key Laboratory of Nuclear Science, Guangdong-Hong Kong Joint Laboratory of Quantum Matter, Institute of Quantum Matter, South China Normal University, Guangzhou, China, associated to 3\n73 School of Physics and Technology, Wuhan University, Wuhan, China, associated to 3\n74 Departamento de Física , Universidad Nacional de Colombia, Bogota, Colombia, associated to 13\n75 Universität Bonn - Helmholtz-Institut für Strahlen und Kernphysik, Bonn, Germany, associated to 17\n76 Institut für Physik, Universität Rostock, Rostock, Germany, associated to 17\n77 Eotvos Lorand University, Budapest, Hungary, associated to 48\n78 INFN Sezione di Perugia, Perugia, Italy, associated to 21\n79 Van Swinderen Institute, University of Groningen, Groningen, Netherlands, associated to 32\n80 Universiteit Maastricht, Maastricht, Netherlands, associated to 32\n81 National Research Centre Kurchatov Institute, Moscow, Russia, associated to 41\n82 National Research University Higher School of Economics, Moscow, Russia, associated to 42\n83 National University of Science and Technology “MISIS”, Moscow, Russia, associated to 41\n84 National Research Tomsk Polytechnic University, Tomsk, Russia, associated to 41\n85 DS4DS, La Salle, Universitat Ramon Llull, Barcelona, Spain, associated to 45\n86 Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden, associated to 59\n87 University of Michigan, Ann Arbor, United States, associated to 68\n\na Universidade Federal do Triângulo Mineiro (UFTM), Uberaba-MG, Brazil\nb Hangzhou Institute for Advanced Study, UCAS, Hangzhou, China\nc Università di Bari, Bari, Italy\nd Università di Bologna, Bologna, Italy\ne Università di Cagliari, Cagliari, Italy\nf Università di Ferrara, Ferrara, Italy\ng Università di Firenze, Firenze, Italy\nh Università di Genova, Genova, Italy\ni Università degli Studi di Milano, Milano, Italy\nj Università di Milano Bicocca, Milano, Italy\nk Università di Modena e Reggio Emilia, Modena, Italy\nl Università di Padova, Padova, Italy\nm Scuola Normale Superiore, Pisa, Italy\nn Università di Pisa, Pisa, Italy\no Università della Basilicata, Potenza, Italy\np Università di Roma Tor Vergata, Roma, Italy\nq Università di Siena, Siena, Italy\nr Università di Urbino, Urbino, Italy\ns MSU - Iligan Institute of Technology (MSU-IIT), Iligan, Philippines\nt P.N. Lebedev Physical Institute, Russian Academy of Science (LPI RAS), Moscow, Russia\nu Novosibirsk State University, Novosibirsk, Russia\n\n† Deceased\nLHCb collaboration\n\nR. Aaij32, A.S.W. Abdelmotteleb56, C. Abellán Beteta50, F.J. Abudinen Gallego56,\nT. Ackernley60, B. Adeva46, M. Adinolfi54, H. Afsharnia9, C. Agapopoulou13, C.A. Aidala87,\nS. Aiola25, Z. Ajaltouni9, S. Akar65, J. Albrecht15, F. Alessio48, M. Alexander59,\nA. Alfonso Albero45, Z. Aliouche62, G. Alkhazov38, P. Alvarez Cartelle55, S. Amato2,\nJ.L. Amey54, Y. Amhis11, L. An48, L. Anderlini22, A. Andreianov38, M. Andreotti21,\nF. Archilli17, A. Artamonov44, M. Artuso68, K. Arzimatov42, E. Aslanides10, M. Atzeni50,\nB. Audurier12, S. Bachmann17, M. Bachmayer49, J.J. Back56, P. Baladron Rodriguez16,\nV. Balagura12, W. Baldini21, J. Baptista Leite1, M. Barbetti22,g, R.J. Barlow62, S. Barsuk11,\nW. Bartesaghi61, M. Bartolini24,f, F. Baryshnikov83, J.M. Basels14, S. Bashir34, G. Bassi29,\nB. Batsukh68, A. Battig15, A. Bay49, A. Beck56, M. Becker15, F. Bedeschi29, I. Bediaga1,\nA. Beiter58, V. Belavin28, S. Belin27, V. Bellec50, K. Belous44, I. Below40, I. Belyaev41,\nG. Bencivenni23, E. Ben-Haim13, A. Berezhnoy40, R. Bernet50, D. Berninghoff17,\nH.C. Bernstein68, C. Bertella48, A. Bertolin28, C. Betancourt50, F. Bett148, Ia. Bezshyiko50,\nS. Bhasin54, J. Bhom35, L. Bian73, M.S. Bicker15, S. Bifani53, P. Billoir13, M. Birch61,\nF.C.R. Bishop55, A. Bitadze62, A. Bizzet122,k, M. Bjorn53, M.P. Blago48, T. Blake56, F. Blanc49,\nS. Blusk68, D. Bobulska59, J.A. Boelhauve15, O. Boente Garcia46, T. Boettcher65,\nA. Boldyrev82, A. Bondar43, N. Bondar38,48, S. Borghi62, M. Borisyak42, M. Borsato17,\nJ.T. Borsuk35, S.A. Bouchiba49, T.J.V. Bowcock60, A. Boyer48, C. Bozzi21, M.J. Bradley61,\nS. Braun66, A. Brea Rodriguez46, J. Brodzicka35, A. Brossa Gonzalez56, D. Brundu27,\nA. Buonaura50, L. Buonincontri28, A.T. Burke62, C. Bur48, A. Bursche72, A. Butkevich39,\nJ.S. Butler32, J. Buytaert48, W. Byczynski48, S. Cadeddu27, H. Cai73, R. Calabrese21,f,\nL. Calefice15,13, L. Calero Diaz23, S. Cali23, R. Calladine53, M. Calvi26,j, M. Calvo Gomez85,\nP. Camargo Magalhaes54, P. Campana23, A.F. Campoverde Quezada6, S. Capelli26,j,\nL. Capriotti20,d, A. Carbonne20,d, G. Carboni31, R. Cardinale24,h, A. Cardini27, I. Carli4,\nP. Carniti26,j, L. Carus14, K. Carvalho Akiba32, A. Casais Vidal46, G. Casse60, M. Cattaneo48,\nG. Cavallero48, S. Celani49, J. Cerasoli10, D. Cervenkov63, A.J. Chadwick60, M.G. Chapman54,\nM. Charles13, Ph. Charpentier48, G. Chatzikonstantinidis53, C.A. Chavez Barajas60,\nM. Chefdeville8, C. Chen3, S. Chen4, A. Chernov35, V. Chobanova46, S. Cholak49,\nM. Chrzaszcz35, A. Chubykin38, V. Chulikov38, P. Ciambrone23, M.F. Cicala56, X. Cid Vidal46,\nG. Ciezarek48, P.E.L. Clarke58, M. Clemente48, H.V. Cliff55, J. Cloisier48, J.L. Cobbledick62,\nV. Coco48, J.A.B. Coelho11, J. Cogan10, E. Cogneras9, L. Cojocariu37, P. Collins48,\nT. Colombo48, L. Congedo19,c, A. Contu27, N. Cooke53, G. Coombs39, I. Corredoira 46,\nG. Corti48, C.M. Costa Sobral56, B. Couturier48, D.C. Craik64, J. Crkovska67, M. Cruz Torres1,\nR. Currie58, C.L. Da Silva57, S. Dadabaevas3, L. Dai71, E. Dall’Occo15, J. Dalseno46,\nC. D’Ambrosio48, A. Danilina41, P. d’Argent48, J.E. Davies62, A. Davis62,\nO. De Aguilar Francisco62, K. De Bruyn79, S. De Capua62, M. De Cian49, J.M. De Miranda1,\nL. De Paula2, M. De Serio19,c, D. De Simone50, P. De Simone23, F. De Vellis15, J.A. de Vries80,\nC.T. Dean67, F. Deberardinis19,c, D. Decamps8, V. Dedu10, L. Del Buono13, B. Delaney55,\nH.-P. Dembinski15, A. Dendek34, V. Denysenko50, D. Derkach82, O. Deschamps9, F. Desse11,\nF. Dettori27,e, B. Dey77, A. Di Cicco23, P. Di Nezza23, S. Didenko83, L. Dieste Maronas46,\nH. Dijkstra48, V. Dobishuk52, C. Dong3, A.M. Donohoe18, F. Dordei27, A.C. dos Reis1,\nL. Douglas59, A. Dovbnya51, A.G. Downes8, M.W. Dudek25, L. Dufour48, V. Duk78,\nP. Durante48, J.M. Durham67, D. Dutta62, A. Dziurda35, A. Dzyuba38, S. Easo57, U. Egede69,\nV. Egorychev41, S. Eidelman43,u,i, S. Eisenhardt58, S. Ek-In49, L. Eklund59,86, S. Ely68,\nA. Ene37, E. Epple67, S. Escher14, J. Eschle50, S. Esen13, T. Evans48, A. Falabella20, J. Fan3,\nY. Fan6, B. Fang73, S. Farry60, D. Fazzini26,j, M. Feo48, A. Fernandez Prieto46, A.D. Fernez66,\nF. Ferrari20,d, L. Ferreira Lopes49, F. Ferreira Rodrigues2, S. Ferreres Sole32, M. Ferrari50,\nM. Ferro-Luzzi48, S. Filipov39, R.A. Fini19, M. Fiorini21,f, M. Firlej34, K.M. Fischer63,\nD.S. Fitzgerald87, C. Fitzpatrick62, T. Fiutowski34, A. Fkiaras48, F. Fleuret12, M. Fontana13, F. Fontanelli24,h, R. Forty48, D. Foulds-Holt55, V. Franco Lima60, M. Franco Sevilla66, M. Frank48, E. Franzoso21, G. Frau17, C. Frei48, D.A. Friday59, J. Fu6, Q. Fuhring15, E. Gabriel32, G. Galati19,e, A. Gallas Torreia46, D. Galli20,d, S. Gambetta58,48, Y. Gan3, M. Gandelman2, P. Gandini25, Y. Gao5, M. Garau27, L.M. Garcia Martin56, P. Garcia Moreno45, J. García Pardinas26,j, B. Garcia Plana46, F.A. Garcia Rosales12, L. Garrido45, C. Gaspar48, R.E. Geertsema32, D. Gerick17, L.L. Gerken15, E. Gersabeck62, M. Gersabeck62, T. Gershon56, D. Gerstel10, L. Giambastiani28, V. Gibson55, H.K. Giemza36, A.L. Gilman63, M. Giovannetti23,p, A. Gioventù46, P. Gironella Girone15, L. Giubega37, C. Giugliano21,f,48, K. Gizdov58, E.L. Gkougkousis48, V.V. Gligorov13, C. Göbel70, E. Golobarbes85, D. Golubkov41, A. Golutvin61,83, A. Gomes1,a, S. Gomez Fernandez45, F. Goncalves Abrantes63, M. Goncerz35, G. Gong3, P. Gorbounov41, I.V. Gorelov40, C. Gott126, E. Govorkova48, J.P. Grabowski17, T. Grammatico13, L.A. Granado Cardoso48, E. Graugès46, E. Graverini49, G. Graziani22, A. Greco37, L.M. Greeven32, N.A. Grieser4, L. Grillo62, S. Gromov83, B.R. Gruberg Cazon63, C. Gu3, M. Guarise21, M. Guittiere11, P. A. Günther17, E. Gushchin39, A. Guth14, Y. Guz44, T. Gys48, T. Hadavizadeh69, G. Haefeli49, C. Haen48, J. Hainberger48, T. Halewood-leagas60, P.M. Hamilton66, J.P. Hammerich60, Q. Han7, X. Han17, T.H. Hancock63, E.B. Hansen62, S. Hansmann-Menzemer17, N. Harnew63, T. Harrison60, C. Hasse48, M. Hatch48, J. He6,b, M. Hecker61, K. Heijhoff32, K. Heinicke15, A.M. Hennequin48, K. Hennessy60, L. Henry48, J. Heuel14, A. Hicheur2, D. Hill49, M. Hilton62, S.E. Hollitt15, R. Hou7, Y. Hou8, J. Hu17, J. Hu72, W. Hu7, X. Hu3, W. Huang6, X. Huang73, W. Hulsbergen32, R.J. Hunter56, M. Hushchyn82, D. Hutchcroft60, D. Hynds32, P. Ibis15, M. Idzik34, D. Ilin38, P. Ilten65, A. Inglessi38, A. Ishteev83, K. Ivshin38, R. Jacobsson48, H. Jage14, S. Jakobsen48, E. Jans32, B.K. Jashal47, A. Jawahery66, V. Jevtic15, F. Jiang3, M. John63, D. Johnson48, C.R. Jones55, T.P. Jones56, B. Jost48, N. Jurik48, S.H. Kalavan Kadavath34, S. Kandybei51, Y. Kang3, M. Karacson18, M. Karpov82, F. Keizer18, D.M. Keller68, M. Kenzie56, T. Ketel33, B. Khanji15, A. Kharisova84, S. Kholodenko44, T. Kirn14, V.S. Kirsebom49, O. Kitouni64, S. Klaver32, N. Kleijne29, K. Klimaszewski36, M.R. Kmiec36, S. Koliev52, A. Kondybayeva83, A. Konoplyannikov41, P. Kopciewicz34, R. Kopecnak17, P. Koppenburg32, M. Korolev40, I. Kostiuk32,52, O. Kot52, S. Kotriakhova21,38, P. Kravchenko38, L. Kravchuk39, R.D. Krawczyk48, M. Kreps56, F. Kress61, S. Kretzschmar14, P. Krokovny43,u, W. Krupa34, W. Krzemien36, M. Kucharczyk35, V. Kudryavtsev43,u, H.S. Kuindersma32,33, G.J. Kunde67, T. Kvaratskheliya41, D. Lacarrere48, G. Lafferty62, A. Lat27, A. Lampis27, D. Lancienerio50, J.J. Lane52, R. Lane54, G. Lanfranchi23, C. Langenbruch14, J. Langer15, O. Lantwin83, T. Latham56, F. Lazzari29,q, R. Le Gac10, S.H. Lee87, R. Lefèvre9, A. Leflat40, S. Legotin83, O. Leroy10, T. Lesiak35, B. Leverington17, H. Li72, P. Li17, S. Li7, Y. Li4, Y. Li4, Z. Li88, X. Liang68, T. Lin61, R. Lindner48, V. Lisovskyi15, R. Litvinov27, G. Liu72, H. Liu6, Q. Liu6, S. Liu4, A. Lobo Salvia45, A. Loi27, J. Lomba Castro46, I. Longstaff50, J.H. Lopes2, S. Lopez Solino46, G.H. Lovell55, Y. Lu4, C. Lucarelli22,g, D. Lucchesi28,l, S. Luchuk39, M. Lucio Martinez32, V. Lukashenko32,52, Y. Luo3, A. Lupato02, E. Luppi21,f, O. Lupton56, A. Lusiani29,m, X. Lyu6, L. Ma4, R. Ma6, S. Maccolini20,d, F. Machefert11, F. Maciuc37, V. Macko49, P. Mackowiak15, S. Maddrell-Mander54, O. Madejczyk34, L.R. Madhan Mohan54, O. Maev38, A. Maevskiy82, D. Maisuzenko38, M.W. Majewski34, J.J. Malczewski35, S. Malde63, B. Malecki48, A. Malinin81, T. Maltsev43,u, H. Malygina17, G. Manca27,e, G. Mancinelli10, D. Manuzzi20,d, D. Marangotto25,i, J. Maratas9,s, J.F. Marchand8, U. Marconi20, S. Mariani22,g, C. Marin Benito48, M. Marinangeli49, J. Marks17, A.M. Marshall54, P.J. Marshall60, G. Martelli78, G. Martellotti30, L. Martinazzoli48,j, M. Martinelli26,j, D. Martinez Santos46, F. Martinez Vidal47, A. Massafferri1, M. Materok14, R. Matev48, A. Mathad50, V. Matiuin11, C. Matteuzzi26, K.R. Mattioli87, A. Mauri32, E. Maurice12, J. Mauricio45, M. Mazurek48, M. McCann61, L. McConnell18, T.H. McGrath02, N.T. Mchugh99, A. McNab02, R. McNulty18,\nJ.V. Mead60, B. Meadows65, G. Meier15, N. Meinert76, D. Melnychuk36, S. Meloni26,j, M. Merk32,80, A. Merli25, L. Meyer Garcia2, M. Mikhasenko48, D.A. Milanes74, E. Millard56, M. Milovanovic48, M.-N. Minard8, A. Minotti26,j, L. Minzioni21,f, S.E. Mitchell58, B. Mitreska62, D.S. Mitzel15, A. Mödden 15, R.A. Mohammed63, R.D. Moise61, S. Mokhnenko82, T. Mombächer46, I.A. Monroy74, S. Monteil9, M. Morandin28, G. Morello23, M.J. Morello29,m, J. Moron34, A.B. Morris75, A.G. Morris56, R. Mountain68, H. Mu3, F. Muheim58,48, M. Mulder48, D. Müller48, K. Müller50, C.H. Murphy63, D. Murray62, P. Muzzetto27,48, P. Naik54, T. Nakada49, R. Nandakumar57, T. Nanut49, I. Nasteva2, M. Needham58, I. Neri21, N. Neri25,i, S. Neubert75, N. Neufeld48, R. Newcombe61, E.M. Niel11, S. Nieswand14, N. Nikitin40, N.S. Nolte64, C. Normand8, C. Nunez87, A. Oblakowska-Mucha34, V. Obraztsov44, T. Oeser14, D.P. O'Hanlon54, S. Okamura21, R. Oldeman27,e, F. Oliva58, M.E. Olivares68, C.J.G. Onderwater79, R.H. O'neil58, J.M. Otalora Goicochea2, T. Ovsiannikova41, P. Owen50, A. Oyanguren47, K.O. Paddeken75, B. Pagare56, P.R. Pais48, T. Pajero63, A. Palano19, M. Palutan23, Y. Pan62, G. Panshin84, A. Papaneistis57, M. Pappagallo19,c, L.L. Pappalardo21,f, C. Pappenheimer65, W. Parker66, C. Parkes62, B. Passalacqua21, G. Passaleva22, A. Pastore19, M. Patel91, C. Patrignani20,d, C.J. Pawley80, A. Pearce48, A. Pellegrino32, M. Pepe Altarelli48, S. Perazzini20, D. Pereina41, A. Pereiro Castro46, P. Perret9, M. Petric59,48, K. Petridis54, A. Petrolini24,h, A. Petrov81, S. Petruccis58, M. Petruzzo25, T.T.H. Pham68, L. Pica29,m, M. Piccini78, B. Pietrzyk8, G. Pietrzyk49, M. Pili63, D. Pinci30, F. Pisani48, M. Pizzichemi26,48,j, Resmi P.K10, V. Placinta37, J. Plews53, M. Plo Casasus46, F. Polci13, M. Poli Lener23, M. Poliakova68, A. Poluektov10, N. Polukhina83,t, I. Polyakov68, E. Polycarpo2, S. Ponce48, D. Popov6,48, S. Popov42, S. Poslavskii44, K. Prasanth35, L. Promberger48, C. Prouve46, V. Pugatch52, V. Puill11, H. Puller63, G. Punzi29,n, H. Qi3, W. Qian6, J. Qin6, N. Qin3, R. Quagliani49, B. Quintana8, N.V. Raab18, R.I. Rabadan Trejo6, B. Rachwal34, J.H. Rademacker54, M. Rama29, M. Ramos Pernas56, M.S. Rangel2, F. Ratnikov42,82, G. Raven33, M. Reboud8, F. Redi49, F. Reiss62, C. Remon Alepuz47, Z. Ren3, V. Renaudin63, R. Ribatti29, S. Ricciardi57, K. Rinnert60, P. Robbe11, G. Robertson58, A.B. Rodrigues49, E. Rodrigues60, J.A. Rodriguez Lopez74, E.R.R. Rodriguez Rodriguez46, A. Rollings63, P. Roloff88, V. Romanovsky44, M. Romero Lamas46, A. Romero Vidal46, J.D. Roth87, M. Rotondo23, M.S. Rudolph68, T. Ruf18, R.A. Ruiz Fernandez46, J. Ruiz Vidal47, A. Ryzhikov82, J. Ryzka34, J.J. Saborido Silva46, N. Sagidova38, N. Sahoo56, B. Saitta27,e, M. Salomoni48, C. Sanchez Gras32, R. Santacesaria30, C. Santamarina Rios46, M. Santimaria23, E. Santovetti31,p, D. Saranin83, G. Sarpis14, M. Sarpis75, A. Sarti30, C. Satriano30,o, A. Satta31, M. Saur15, D. Savrina41,40, H. Szak9, L.G. Scantlebury Smead63, A. Scarabotto13, S. Schael14, S. Scherf60, M. Schiller59, H. Schindler48, M. Schnelling16, B. Schmidt48, S. Schmitt14, O. Schneider49, A. Schopper48, M. Schubiger62, S. Schulze49, M.H. Schune11, R. Schwemmer48, B. Sciascia23,48, S. Sellam46, A. Semennikov41, M. Senghi Soares33, A. Sergi24,h, N. Serra50, L. Sestini28, A. Seuthe15, Y. Shang8, D.M. Shangase37, M. Shapkin44, I. Shchemerov83, L. Shchutska49, T. Shears60, L. Shekhtman43,u, Z. Shen5, V. Shevchenko81, E.B. Shields26,j, Y. Shimizu11, E. Shmumin83, J.D. Shupperd68, B.G. Siddi21, R. Silva Coutinho50, G. Simi28, S. Simonc19,c, N. Skidmore62, T. Skwarnicki68, M.W. Slater53, I. Slazyk21,f, J.C. Smallwood63, J.G. Smeaton55, A. Smetkina41, E. Smith50, M. Smith61, A. Snoch32, M. Soares20, L. Soares Lavra9, M.D. Sokoloff65, F.J.P. Soler59, A. Solovev38, I. Solovyev38, F.L. Souza De Almeida2, B. Souza De Paula2, B. Spaan15, E. Spadaro Norella25, P. Spradlin59, F. Stagni48, M. Stahl65, S. Stahl48, S. Stanislaus63, O. Steinkamp50,83, O. Stenyakin44, H. Stevens15, S. Stone68, M. Straticiuc37, D. Strekalina83, F. Suljik63, J. Sun27, L. Sun73, Y. Sun66, P. Svihra62, P.N. Swallow53, K. Swientek34, A. Szabelski36, T. Szumlak34, M. Szymanski48, S. Tancaja62, A.R. Tanner54, M.D. Tat63, A. Terentev83, F. Teubert48, E. Thomas48, D.J.D. Thompson53, K.A. Thomson60, V. Tisserand9, S. T'Jampens8, M. Tobin4, L. Tomassetti21,f, X. Tong5, D. Torres Machado1, D.Y. Tou13, E. Trifonova83, C. Tripli49,\nG. Tuci6, A. Tully49, N. Tuning32,48, A. Ukleja36, D.J. Unverzagt17, E. Ursov83, A. Usachov32, A. Ustyuzhanin42,82, U. Uwer17, A. Vagner84, V. Vagnon20, A. Valassi48, G. Valenti20, N. Valls Canudas85, M. van Beuzekom32, M. Van Dijk49, E. van Herwijnen83, C.B. Van Hulse18, M. van Veghel79, R. Vazquez Gomez45, P. Vazquez Regueiro46, C. Vázquez Sierra48, S. Vecchi21, J.J. Velthuis54, M. Veltri22,r, A. Venkateswaran68, M. Veronesi32, M. Vesterinen56, D. Vieira65, M. Vieites Diaz49, H. Viemann76, X. Vilasis-Cardona85, E. Vilella Figueras60, A. Villa20, P. Vincent13, F.C. Volle11, D. Vom Bruch10, A. Vorobyev38, V. Vorobyev43,u, N. Voropaev38, K. Vos80, R. Waldi17, J. Walsh29, C. Wang17, J. Wang5, J. Wang4, J. Wang3, J. Wang73, M. Wang3, R. Wang54, Y. Wang7, Z. Wang50, Z. Wang3, Z. Wang6, J.A. Ward56, N.K. Watson53, S.G. Weber13, D. Websdale61, C. Weisser64, B.D.C. Westhenry54, D.J. White62, M. Whitehead54, A.R. Wiederhold56, D. Wiedner15, G. Wilkinson63, M. Wilkinson68, I. Williams55, M. Williams64, M.R.J. Williams58, F.F. Wilson57, W. Wislicki36, M. Witek35, L. Witola17, G. Wormser11, S.A. Wotton55, H. Wu68, K. Wyllie48, Z. Xiang6, D. Xiao7, Y. Xie7, A. Xu5, J. Xu6, L. Xu3, M. Xu7, Q. Xu6, Z. Xu5, Z. Xu6, D. Yang3, S. Yang6, Y. Yang6, Z. Yang5, Z. Yang66, Y. Yao68, L.E. Yeomans60, H. Yin7, J. Yu71, X. Yuan68, O. Yushchenko44, E. Zaffaroni49, M. Zavertyaev16,t, M. Zdybal35, O. Zenaiev48, M. Zeng3, D. Zhang7, L. Zhang3, S. Zhang71, S. Zhang5, Y. Zhang5, Y. Zhang63, A. Zharkova83, A. Zhelezov17, Y. Zheng6, T. Zhou5, X. Zhou6, Y. Zhou6, V. Zhokhovska11, X. Zhu3, X. Zhu7, Z. Zhu6, V. Zhukov14,40, J.B. Zonneveld58, Q. Zou4, S. Zucchelli20,d, D. Zuliani28, G. Zunic62.\n\n1 Centro Brasileiro de Pesquisas Físicas (CBPF), Rio de Janeiro, Brazil\n2 Universidade Federal do Rio de Janeiro (UFRJ), Rio de Janeiro, Brazil\n3 Center for High Energy Physics, Tsinghua University, Beijing, China\n4 Institute Of High Energy Physics (IHEP), Beijing, China\n5 School of Physics State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing, China\n6 University of Chinese Academy of Sciences, Beijing, China\n7 Institute of Particle Physics, Central China Normal University, Wuhan, Hubei, China\n8 Univ. Savoie Mont Blanc, CNRS, IN2P3-LAPP, Annecy, France\n9 Université Clermont Auvergne, CNRS/IN2P3, LPC, Clermont-Ferrand, France\n10 Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France\n11 Université Paris-Saclay, CNRS/IN2P3, IJCLab, Orsay, France\n12 Laboratoire Leprince-Ringuet, CNRS/IN2P3, Ecole Polytechnique, Institut Polytechnique de Paris, Palaiseau, France\n13 LPNHE, Sorbonne Université, Paris Diderot Sorbonne Paris Cité, CNRS/IN2P3, Paris, France\n14 I. Physikalisches Institut, RWTH Aachen University, Aachen, Germany\n15 Fakultät Physik, Technische Universität Dortmund, Dortmund, Germany\n16 Max-Planck-Institut für Kernphysik (MPIK), Heidelberg, Germany\n17 Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany\n18 School of Physics, University College Dublin, Dublin, Ireland\n19 INFN Sezione di Bari, Bari, Italy\n20 INFN Sezione di Bologna, Bologna, Italy\n21 INFN Sezione di Ferrara, Ferrara, Italy\n22 INFN Sezione di Firenze, Firenze, Italy\n23 INFN Laboratori Nazionali di Frascati, Frascati, Italy\n24 INFN Sezione di Genova, Genova, Italy\n25 INFN Sezione di Milano, Milano, Italy\n26 INFN Sezione di Milano-Bicocca, Milano, Italy\n27 INFN Sezione di Cagliari, Monserrato, Italy\n28 Università degli Studi di Padova, Università e INFN, Padova, Padova, Italy\n29 INFN Sezione di Pisa, Pisa, Italy\n30 INFN Sezione di Roma La Sapienza, Roma, Italy\n31 INFN Sezione di Roma Tor Vergata, Roma, Italy\n32 Nikhef National Institute for Subatomic Physics, Amsterdam, Netherlands\n33 Nikhef National Institute for Subatomic Physics and VU University Amsterdam, Amsterdam, Netherlands\n34 AGH - University of Science and Technology, Faculty of Physics and Applied Computer Science, Kraków, Poland\n35 Henryk Niewodniczanski Institute of Nuclear Physics Polish Academy of Sciences, Kraków, Poland\n36 National Center for Nuclear Research (NCBJ), Warsaw, Poland\n37 Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest-Magurele, Romania\n38 Petersburg Nuclear Physics Institute NRC Kurchatov Institute (PNPI NRC KI), Gatchina, Russia\n39 Institute for Nuclear Research of the Russian Academy of Sciences (INR RAS), Moscow, Russia\n40 Institute of Nuclear Physics, Moscow State University (SINP MSU), Moscow, Russia\n41 Institute of Theoretical and Experimental Physics NRC Kurchatov Institute (ITEP NRC KI), Moscow, Russia\n42 Yandex School of Data Analysis, Moscow, Russia\n43 Budker Institute of Nuclear Physics (SB RAS), Novosibirsk, Russia\n44 Institute for High Energy Physics NRC Kurchatov Institute (IHEP NRC KI), Protvino, Russia, Protvino, Russia\n45 ICCUB, Universitat de Barcelona, Barcelona, Spain\n46 Instituto Galego de Física de Altas Enerxías (IGFAE), Universidade de Santiago de Compostela, Santiago de Compostela, Spain\n47 Instituto de Física Corpuscular, Centro Mixto Universidad de Valencia - CSIC, Valencia, Spain\n48 European Organization for Nuclear Research (CERN), Geneva, Switzerland\n49 Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland\n50 Physik-Institut, Universität Zürich, Zürich, Switzerland\n51 NSC Kharkiv Institute of Physics and Technology (NSC KIPT), Kharkiv, Ukraine\n52 Institute for Nuclear Research of the National Academy of Sciences (KINR), Kyiv, Ukraine\n53 University of Birmingham, Birmingham, United Kingdom\n54 H.H. Wills Physics Laboratory, University of Bristol, Bristol, United Kingdom\n55 Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom\n56 Department of Physics, University of Warwick, Coventry, United Kingdom\n57 STFC Rutherford Appleton Laboratory, Didcot, United Kingdom\n58 School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom\n59 School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom\n60 Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom\n61 Imperial College London, London, United Kingdom\n62 Department of Physics and Astronomy, University of Manchester, Manchester, United Kingdom\n63 Department of Physics, University of Oxford, Oxford, United Kingdom\n64 Massachusetts Institute of Technology, Cambridge, MA, United States\n65 University of Cincinnati, Cincinnati, OH, United States\n66 University of Maryland, College Park, MD, United States\n67 Los Alamos National Laboratory (LANL), Los Alamos, United States\n68 Syracuse University, Syracuse, NY, United States\n69 School of Physics and Astronomy, Monash University, Melbourne, Australia, associated to 56\n70 Pontifícia Universidade Católica do Rio de Janeiro (PUC-Rio), Rio de Janeiro, Brazil, associated to 2\n71 Physics and Micro Electronic College, Hunan University, Changsha City, China, associated to 7\n72 Guangdong Provincial Key Laboratory of Nuclear Science, Guangdong-Hong Kong Joint Laboratory of Quantum Matter, Institute of Quantum Matter, South China Normal University, Guangzhou, China, associated to 3\n73 School of Physics and Technology, Wuhan University, Wuhan, China, associated to 3\n74 Departamento de Física , Universidad Nacional de Colombia, Bogota, Colombia, associated to 13\n75 Universität Bonn - Helmholtz-Institut für Strahlen und Kernphysik, Bonn, Germany, associated to 17\n76 Institut für Physik, Universität Rostock, Rostock, Germany, associated to 17\n77 Eotvos Lorand University, Budapest, Hungary, associated to 48\n78 INFN Sezione di Perugia, Perugia, Italy, associated to 21\n79 Van Swinderen Institute, University of Groningen, Groningen, Netherlands, associated to 32\n80 Universiteit Maastricht, Maastricht, Netherlands, associated to 32\n81 National Research Centre Kurchatov Institute, Moscow, Russia, associated to 41\n82 National Research University Higher School of Economics, Moscow, Russia, associated to 42\n83 National University of Science and Technology “MISIS”, Moscow, Russia, associated to 41\n84 National Research Tomsk Polytechnic University, Tomsk, Russia, associated to 41\n85 DS4DS, La Salle, Universitat Ramon Llull, Barcelona, Spain, associated to 45\n86 Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden, associated to 59\n87 University of Michigan, Ann Arbor, United States, associated to 68\n\na Universidade Federal do Triângulo Mineiro (UFTM), Uberaba-MG, Brazil\nb Hangzhou Institute for Advanced Study, UCAS, Hangzhou, China\nc Università di Bari, Bari, Italy\nd Università di Bologna, Bologna, Italy\ne Università di Cagliari, Cagliari, Italy\nf Università di Ferrara, Ferrara, Italy\ng Università di Firenze, Firenze, Italy\nh Università di Genova, Genova, Italy\ni Università degli Studi di Milano, Milano, Italy\nj Università di Milano Bicocca, Milano, Italy\nk Università di Modena e Reggio Emilia, Modena, Italy\nl Università di Padova, Padova, Italy\nm Scuola Normale Superiore, Pisa, Italy\nn Università di Pisa, Pisa, Italy\no Università della Basilicata, Potenza, Italy\np Università di Roma Tor Vergata, Roma, Italy\nq Università di Siena, Siena, Italy\nr Università di Urbino, Urbino, Italy\ns MSU - Iligan Institute of Technology (MSU-IIT), Iligan, Philippines\nt P.N. Lebedev Physical Institute, Russian Academy of Science (LPI RAS), Moscow, Russia\nu Novosibirsk State University, Novosibirsk, Russia\n\n† Deceased"} {"paper_id": "prb12", "title": "Evolving parsec-scale radio structure in the most distant blazar known", "text": "Evolving parsec-scale radio structure in the most distant blazar known\n\nTao An1*, Prashanth Mohan1, Yingkang Zhang1,2, Sándor Frey3, Jun Yang4, Krisztina É. Gabányi5,3,6, Leonid I. Gurvits7,8, Zsolt Paragi7, Krisztina Perger6,3, Zhenya Zheng1\n\n1. Shanghai Astronomical Observatory, Key Laboratory of Radio Astronomy, 80 Nandan Road, 200030 Shanghai, China\n2. University of Chinese Academy of Sciences, 19A Yuquan Road, Shijingshan District, 100049 Beijing, China\n3. Konkoly Observatory, CSFK, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary\n4. Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala, Sweden\n5. MTA-ELTE Extragalactic Astrophysics Research Group, Pázmány Péter sétány 1/A, H-1117 Budapest, Hungary\n6. Department of Astronomy, Eötvös Loránd University, Pázmány Péter sétány 1/A, H-1117 Budapest, Hungary\n7. Joint Institute for VLBI ERIC (JIVE), Postbus 2, NL-7990 AA Dwingeloo, the Netherlands\n8. Department of Astrodynamics and Space Missions, Delft University of Technology, Kluyverweg 1, 2629 HS Delft, the Netherlands\n\n* antao@shao.ac.cn\n\nAbstract\nBlazars are a sub-class of quasars with Doppler boosted jets oriented close to the line of sight, and thus efficient probes of supermassive black hole growth and their environment, especially at high redshifts. Here we report on Very Long Baseline Interferometry observations of a blazar J0906+6930 at z = 5.47, which enabled the detection of polarised emission and measurement of jet proper motion at parsec scales. The observations suggest a less powerful jet compared with the general blazar population, including lower proper motion and bulk Lorentz factor. This coupled with a previously inferred high accretion rate indicate a transition from an accretion radiative power to a jet mechanical power based transfer of energy and momentum to the surrounding gas. While alternative scenarios could not be fully ruled out, our results indicate a possibly nascent jet embedded in and interacting with a dense medium resulting in a jet bending.\n\nIntroduction\nMechanisms for the formation and rapid growth of supermassive black holes (SMBHs) in the early Universe remain debatable1 and have a complex connection with the evolution of their host galaxies through feedback2. The discovery of quasars at redshift \\( \\gtrsim 6^{3,4} \\) indicates that SMBHs as heavy as \\( \\sim 10^9 \\) solar masses (\\( M_\\odot \\)) have already existed when the Universe was at about a tenth of its current age. Spectroscopic surveys have largely enabled the discovery of high-redshift galaxies and quasars3, paving the way for deeper optical, infrared and radio follow-up observations 5–8. Currently there are more than 200 quasars discovered above redshift of 5.7. High-redshift blazars are useful probes of the early Universe owing to their Doppler-beamed emission which makes them amongst the brightest sources. As their jet power scales with the mass of the SMBH9, blazars shed light on the cosmic evolution of massive black holes10,11. Jetted but misaligned quasars (i.e. larger inclination angle towards the observer’s LOS (line of sight); not strongly beamed) are expected to outnumber blazars at a given redshift by a factor \\( \\sim \\Gamma^2 \\) (where \\( \\Gamma \\) is the jet bulk Lorentz factor) rendering the occurrence of blazars rare at high redshifts9. An increasing sample size can help probe their expected number density and luminosity evolution over cosmic time12, essential inputs for planning future surveys. This information can help to study the formation of SMBHs in the early Universe11,13, active galactic nucleus (AGN) activity, the interaction of jets with the surrounding interstellar medium (ISM) and AGN feedback influencing the evolution of the host galaxy2.\n\nThe source J0906+6930 (\\( z = 5.47 \\)), identified as a blazar14 remains the farthest yet in its class of objects. Unravelling the jet structure of high-redshift blazars requires extremely high resolution. It has a prominent pc-scale core–jet structure, unraveled by Very Long Baseline Array (VLBA) observations at 15 GHz14,15. The archival 15 GHz and new 22 GHz data obtained with the Korean VLBI network and the Japanese VLBI Exploration of Radio Astrometry (KaVA) arrays confirm a core–jet structure with a projected size of \\( \\sim 5 \\) pc, extending to the south-west direction16.\nHere, we report the measurement of proper motion and linear polarisation in the parsec-scale jet of this high redshift blazar. We use new 15-GHz data observed with the VLBA in 2017 and 2018, archival VLBA data obtained in 2004–2005 (see details in Supplementary Table 1) and the flux densities reported by the 40 m telescope at the Owens Valley Radio Observatory (OVRO) to explore the evolution of the source morphology and infer its physical characteristics. The jet parameters (lower proper motion and bulk Lorentz factor) are inclined to support a less powerful jet, compared with the general blazar population. The jet interacts with the surrounding interstellar medium resulting in a jet bending and polarised emission.\n\nResults\n\nThe new 15-GHz VLBA images are shown in Figures 1 panels d and e and the archival images in panels a to c. The noise in the image from the 2017 observation is a factor of 7–16 lower than those obtained during 2004–2005. All image parameters (beam size, peak brightness and rms noise) are presented in Supplementary Table 2. The peak brightness of the 2017 and 2018 images is ~3 times lower than 13 years ago, consistent with the declining flux density as indicated from the long-term 15 GHz light curve based on single-dish monitoring at the OVRO (see Supplementary Figure 1 ).\n\nA compact core–jet structure is present in all images. The shape of the elliptical Gaussian model indicates that the core region (C) is a blend of the optically thick (at 15 GHz) jet base and an inner section of the optically-thin jet. The major to minor axis ratio of C ranges between 3.7 to 13.5 with a northeast–southwest elongation. The jet component J1 is ~ 0.9 mas away from the core at a position angle of ~ −138°. In the highest-resolution 2005 image16 and the new 2017 image, a sharp (> 90°) jet bending is seen from the southwest to the south at the location of J1. The fainter component J2 is at the end of the pc-scale jet, about 1 mas south of the core. The same bent jet morphology is seen at lower frequencies17, up to ~2 mas from C.\n\nApparently abrupt changes in jet direction on pc scales in blazars are frequently observed. In most cases this implies a slight change of direction in the jet which points very close to our line of sight (LOS). The jet bending itself may indicate a low-pitch angle helical motion18, like in the well-studied blazar, e.g., 1156+29519. Alternatively, the jet bending may also result from interaction with massive clouds in the ISM, e.g. dense clouds in the broad or narrow line regions20, 21. In the present case of J0906+6930, we find no indication for helical motion, for example, there is no noticeable variation in the core position angle or in the shape of the optically-thick jet base (i.e. the fitted core component in Table 1), and there are no significant periodic variations seen in the light curve (Supplementary Figure 1 ). There is however support for possible jet–ISM interaction, evidenced by the relatively high levels of linear polarization observed near the jet bending (see discussion below). The density contrast between the material in the jet and that external to it is > 9 (see Methods jet and ISM properties), thus suggesting a relatively lighter jet susceptible to interaction and bending owing to a relatively denser medium. Assuming a momentum balance across the jet–ISM interaction interface, the ISM number density is estimated to be \\( n_e \\geq 26.6 \\) cm\\(^{-3}\\).\n\nThe position of J1 (projected distance ~5.3 pc away from the core) is nearly stationary between 2004 and 2018, consistent with a jet beam encountering dense surrounding ISM. This is also supported by the increasing flux density at J1, which represents a standing shock where the material and magnetic fields near the jet head are substantially compressed, resulting in an increased synchrotron emission20. This is indeed manifested in the polarisation image obtained from the 2018 epoch shown in Figure 2. The polarised emission peaks at 0.8 mas south of the core and is aligned in the direction between J1 and J2. The maximum fractional polarisation is ~10%, and the peak polarised intensity is ~0.6 mJy beam\\(^{-1}\\) (about 10 times above the rms noise). This is the initial polarisation measurement in a jet of a radio-loud quasar at redshift > 5. In contrast, the core is weakly polarised (<3σ). This is similar to the blazar CTA 102 (\\( z = 1.037 \\)) observed at 43 GHz (rest frame frequency of ~ 88 GHz) which indicates a relatively low linear polarisation in the core with a remarkable increase of the polarisation intensity in the pc-scale jet, attributed to either a jet–ISM interaction or to preferential locations along a helical jet22. Statistical studies of radio polarisation in blazars indicate cores with relatively low polarisation fractions of 2–3 % amongst sub-samples consisting of low and high synchrotron peaked sources23. If the synchrotron peak is associated with emission from the region downstream of a transverse shock, the polarisation near the core should be high owing to the shock passage resulting in an ordered magnetic field24. However, the low or near absent polarisation in the core of J0906+6930 indicates that the magnetic field could be turbulent or tangled.\n\nA radio spectrum with a peak between 40 and 60 GHz (rest frame frequency)16, and a weakly polarised core are characteristic of high-frequency peakers25, where a higher peak frequency due to synchrotron self absorption is a consequence of a younger jet based on self-similar models of hot-spot expansion26, consistent with the above inference from polarisation. A revised black hole mass of \\( 4.4 \\times 10^7 M_\\odot \\) is obtained if we use\nscaling relations appropriate to a Doppler beamed jetted source. The mass is consistent with the expectation from a population of radio galaxies characterised with GHz peaked radio spectrum; together with the young AGN scenario, these are indicative of an ongoing transition in AGN feedback and an evolving black hole (see Methods black hole mass). Based on the location of the synchrotron peak frequency \\( v_s \\) in the spectral energy distribution, blazars are classified into low synchrotron peaked if \\( v_s < 10^{14} \\) Hz (in the infrared), intermediate synchrotron peaked if \\( 10^{14} \\) Hz \\( < v_s < 10^{15} \\) Hz (optical — ultra-violet) and high synchrotron peaked if \\( v_s > 10^{15} \\) Hz (in the X-rays). J0906+6930 is identified as a low synchrotron peaked blazar with \\( v_s \\sim 10^{12} \\) Hz\\(^{27}\\). Such sources are characterised by energetic jets with relatively highly superluminal (apparent) jet components. However, as this is not the case for J0906+6930 based on the low bulk Lorentz factor, slower component proper motion and a possible tangled or turbulent magnetic field, the jet is likely developing and nascent. Similarly, the recently discovered radio galaxy TGSS J1530+1049 at \\( z = 5.72 \\) also has a compact structure resembling a radio galaxy in an early evolutionary phase\\(^{28}\\). An alternative scenario of the J0906+6930 radio structure involving a re-started jet tracing a path swept by the past jet activity can not be fully ruled out from the present observation. The implications of AGN jet activity on SMBH growth in the early Universe, and additional alternative scenarios enabling the jet structure are discussed in Methods black hole mass. To check the latter picture, further high-sensitivity radio interferometric observations are necessary to search for relic emission structure on 100 mas scales.\n\nAt \\( z > 4.5 \\), about 50 quasars have been detected in radio bands with 30 of them being VLBI imaged\\(^{5}\\). As the sources are mostly dominated by compact single components with flux densities \\( < 20 \\) mJy (at GHz observing frequencies), proper motion measurements face challenges owing to the relative scarcity, faintness and a requirement for long time gaps between epochs for a definitive estimate due to cosmological time dilation. Successful measurements have been only made for two \\( z > 4 \\) blazars with the European VLBI Network (EVN) using only two epochs. These include J1026+2542 (\\( z = 5.27 \\)) with a proper motion of 3.3–14.0 c over 7 yr\\(^{29}\\) and J2134–0419 (\\( z = 4.33 \\)) with a proper motion of 4.1±2.7 c over 16 yr\\(^{30}\\). The compact and bright jet in J0906+6930 makes it suitable for the study of jet kinematics. Combining the archival and new data, the proper motion of J1 is \\( -0.006 \\pm 0.004 \\) mas yr\\(^{-1}\\) (–0.8±0.5 c, Figure 3), consistent with a scenario involving jet–ISM interaction and the subsequent jet bending. The separation of component J2 shows a visible increase from 1.27 mas in 2005 to 1.58 mas in 2017/2018. The apparent proper motion of J2 is 0.019 ± 0.006 mas yr\\(^{-1}\\) (2.5 ± 0.8 c, Figure 3). These are the preliminary measurements for a \\( z > 4.5 \\) blazar based on data spanning more than two epochs and are consistent with (much lower than) a maximal proper motion of 0.09 mas yr\\(^{-1}\\) expected in a highly beamed jet in an accelerated cosmological expansion (see Methods maximum proper motion). For a sample of 122 relatively lower-redshift (\\( z = 0.1–3 \\)) radio-loud AGN, the median jet proper motion peaks at \\( \\lesssim 5c \\)\\(^{31}\\), with the low synchrotron peaked sources indicating the fastest speeds (upto ~40 c) and high Doppler boosted Tera electron Volt (TeV) γ-ray emission. Although the estimate for J0906+6930 is consistent within the statistical expectation, the apparent jet speed is significantly lower than the expected value for a low synchrotron peaked blazar.\n\nDoppler beaming in the relativistic jet can cause the core brightness temperature (\\( T_B \\)) to exceed the theoretical limits set by equipartition between the kinetic and magnetic energy densities, assumed to be \\( T_{B,\\text{eq}} = 5 \\times 10^{10} \\) K\\(^{32}\\). The \\( T_B \\) of the J0906+6930 core is \\( (30.2 \\pm 4.0) \\times 10^{10} \\) K with a consequent Doppler factor \\( \\delta = T_B/T_{B,\\text{eq}} \\) of 6.1 ± 0.8 (see Methods Doppler boosting parameters). From the inferred apparent velocity and Doppler factor, the bulk Lorentz factor \\( \\Gamma = 3.6 \\pm 0.5 \\) and inclination angle towards the observer line of sight \\( \\theta = 6.^{\\circ}8 \\pm 2.^{\\circ}2 \\). These values are consistent with estimates from the parametric modeling of the spectral energy distribution\\(^{27}\\). The lower Lorentz factor and slower jet component are consistent with the less powerful nature of the J0906+6930 jet (jet/Eddington luminosity \\( \\sim 0.004 \\), see Methods jet and ISM properties). The relatively less powerful jet, in addition to clues from the radio spectrum and polarisation point to its possible nascent nature. A prominent disk emission is inferred from the modelling of the spectral energy distribution of this and three other high-z blazars\\(^{27}\\). This coupled with a relatively less powerful jet luminosity marks a possible transition in this source between the accretion or quasar mode and the onset of the jet or radio mode. In the former, the accretion energy can radiatively drive (momentum transfer) surrounding gas to galactic scales, and in the latter, a powerful jet can transfer mechanical energy acting to heat up the gas at galactic and cluster scales\\(^{2}\\).\n\nThe present VLBI data thus characterize J0906+6930 as a high-redshift blazar with a nascent jet embedded in a dense medium causing the pc-scale jet–ISM interaction and the consequent jet bending. These represent the initial results of ongoing investigations on high resolution imaging of a sample of high-redshift blazars. Further simultaneous multi-frequency VLBI observations can help constrain the magnetic field strength and electron density from Faraday rotation measurements. The next generation VLBI facilities (e.g. Square Kilometre Array VLBI programme\\(^{33}\\)) are more sensitive to detect much weaker high redshift blazars, thus advancing our\nunderstanding of the co-evolution of SMBHs and host galaxies in the early Universe.\n\nMethods\n\nVLBI Observations\n\nThe compact prominent jet and an elapsed time longer than 10 yr since the earlier observations make J0906+6930 a promising source for continued monitoring of the evolution of the jet structure. We additionally compiled and reduced archival VLBA data in this analysis. The observational setup for each observation is presented in Supplementary Table 1.\n\nWe conducted VLBA 15 GHz observations on 2017 September 11 and 2018 January 31. All ten VLBA telescopes were requested in the proposals BZ068 and BZ071. However, due to unfavourable weather conditions and maintenance time, the Saint Croix (SC) telescope did not participate in the observations, resulting in relatively lower resolution in east–west direction in the 2017 and 2018 images compared to those obtained from the full VLBA in 2004. To enable a complete analysis of the pc-scale jet evolution in J0906+6930, we obtained all available 15-GHz VLBA data from the NRAO Archive (https://archive.nrao.edu/).\n\nFor the BZ068 observation, the data were recorded in four baseband channels, each with 64 MHz bandwidth. Each of the left-handed circular polarisation (LCP) and right-handed circular polarisation (RCP) occupies two channels. A 2-bit sampling resulted in a total data rate of 1 gigabit per second (Gbps). Phase referencing was not required as the source J0906+6930 itself was bright and compact enough to be used for fringe fitting. Except for a few scans which were used on the fringe finder (NRAO 150 and 3C 84) in the beginning and end of the observation run, the on-source time was about 400 min. The BZ068 observation thus led to a vast improvement in image quality (lowest image noise) compared to previous VLBA observations.\n\nThe main goal of the subsequent BZ071 observation was the detection of the linear polarisation in J0906+6930. The observation was carried out in full polarisation mode. The radio galaxy 3C 84 was used for instrumental polarisation calibration, and the quasar NRAO 150 for fringe searching and bandpass calibration. The recording settings are similar to those of BZ068 except that four 128-MHz baseband channels were used, resulting in a total data rate of 2 Gbps, twice that of BZ068. After observation, both data sets were correlated at the National Radio Astronomy Observatory in Socorro, USA, using the DiFX software correlator34. The post calibration and imaging were carried out at the China SKA Regional Centre prototype35.\n\nData reduction\n\nThe correlated visibility data were imported into the NRAO Astronomical Image Processing System (AIPS) software package36 for amplitude and phase calibration. We applied the standard calibration procedure of AIPS. The AIPS task APCAL was performed to calibrate the visibility amplitudes, using the antenna gains and system temperatures measured at each station during the observation. The atmospheric opacity was estimated based on the weather information recorded at each station and accounted for. The instrumental delay and global phase errors were then calibrated using the FRING task. This included a manual fringe fitting using NRAO 150 (~10 Jy at this frequency in this epoch) as calibrator to determine the delay offsets and phase errors between different sub-bands, and for application the solutions to all antennas. This was followed by running the global fringe fitting including all data to calculate and remove the global phase errors. Over 98% good solutions were achieved for both datasets. Then, the antenna-based bandpass functions were solved from the NRAO 150 data by using the task BPASS and applied to the visibility data. The bandpass shape across the broad 128–256 MHz baseband is corrected resulting in an increased dynamic range (the ratio of image peak to noise).\n\nThe calibrated data were averaged in each subband (each 64 MHz wide) and in time (2 s) and exported to external FITS files using the task SPLIT. The resulting single-source data file was imported into the Caltech Difmap package37 to further calibrate residual phase errors. The hybrid mapping process consisted of several iterations of CLEAN and self-calibration. The final image was obtained after a few iterations of phase and amplitude self-calibrations, repeated by gradually reducing the solution intervals from 8 h to 1 min.\n\nThe raw correlated visibilities from the 2004 and 2005 observations were processed following the same procedure as discussed above using AIPS. The BG154B (2005 March 22) and BG154E (2005 May 15) data were combined owing to a close time separation after ensuring that there were no significant differences in the measured flux densities. This resulted in a high-resolution image with excellent (u,v) coverage in both N–S and E–W directions. This and the resulting improved sensitivity enabled the detection of the weak J2 jet component (see Figure 1 panel c), which was earlier not possible. All parameters including beam properties, peak brightness and noise rms for each image are presented in Supplementary Table 2.\n\nModel fitting and error estimation\n\nAfter self-calibration, the modelfit procedure (in Difmap) was used to fit the visibilities (at all epochs) with Gaussian\nbrightness distribution models. An elliptical Gaussian model is used to fit the core while circular ones are used for the jet. In order to avoid positional and intensity offsets between LL and RR polarisations (a possible tiny difference), for the model fitting we used only LL cross-correlation products.\n\nThe fitted Gaussian models are shown as elliptical or circular shapes in Figure 1. In the 2004 epochs, two components were detected: the core (C) and a southwest jet component (J1). Due to the improved sensitivity and better north–south (u,v) coverage, one more jet component J2 was detected at about 1.5 mas south of the core in the other three epochs. The core was unresolved on 2018 January 31, and its minor-axis size was estimated as an upper limit by considering the restoring beam size and signal-to-noise level\\(^{38}\\). In all five epochs, although the (u,v) coverages and observation time ranges were different, the core component was elongated along the same northeast–southwest direction, with the position angles ranging between 28.1° and 55.3°, roughly within three times \\( \\sigma \\) (rms). This is possibly a true feature or could arise as an artefact of the VLBA (u,v)-coverage pattern. It is worth noticing that the core component major axis always points towards J1 (see Table 1). These clues together indicate that the unresolved core region likely contains an opaque core (at this frequency) and an inner jet along the C–J1 direction. In the model fitting of the 2017 September 11 epoch (highest quality data), an emission component of ~0.6 mJy beam\\(^{-1}\\) peaks between C and J1 in the residual image after removing these components, adding weight to the possible emergence of a newly generated, yet unresolved jet component.\n\nThe statistical errors from the fitted Gaussian models are rough estimates based on the signal-to-noise levels in the images\\(^{39}\\). In addition to the statistical error \\( \\sigma_{S,\\text{sta}} \\), the true errors can comprise contributions from other factors resulting from the calibration error of flux density scale, incomplete (u,v) coverage of the interferometric array, and the complex jet structure. An extra 5 per cent of flux density calibration error, which is the typical value for the VLBA\\(^{40}\\), is added to account for the calibration error \\( \\sigma_{S,\\text{cal}} \\) of the visibility amplitude. Thus the uncertainty of the flux density is estimated as: \\( \\sigma_S = \\sqrt{\\sigma_{S,\\text{cal}}^2 + \\sigma_{S,\\text{sta}}^2} \\).\n\nThe uncertainty of the Gaussian component size is decomposed as the statistical error and the fitting error. The statistical error is \\( \\frac{\\theta_D}{\\text{SNR}} \\), where the SNR is the signal-to-noise ratio of the fitted Gaussian component, \\( \\theta_D \\) is the fitted Gaussian size \\( D_{\\text{maj}} \\) and \\( D_{\\text{min}} \\) listed in columns 4-5 of Table 1. The final size uncertainty is the quadratic mean of these two errors.\n\nThe positions of jet components are measured with respect to the core which is assumed to be stationary. The statistical error on the position is \\( \\sigma_{p,\\text{sta}} = \\frac{\\theta}{2 \\times \\text{SNR}} \\), where \\( \\theta \\) is taken as the synthesized beam size (the full width at half maximum, FWHM). As mentioned above, the core component is likely mixed with inner jet emission. In reality, the peak emission of the core can be affected by intrinsic changes of the emission structure (for example, the ejection of a new jet component or a passing shock) and the goodness of the intensity distribution being fitted with a Gaussian function. All these factors may introduce an additional uncertainty to the reference point. We have fitted the core with several different models: a single elliptical Gaussian; one circular Gaussian component (the core) plus a point source (to represent the residual emission from the unresolved inner jet); two circular Gaussian components; two point sources. The discrepancy between the fitted core positions is used as the systematic error of the reference point \\( \\sigma_{p,\\text{sys}} \\), which is added into the total error budget. The positional error of jet component can be expressed as \\( \\sigma_p = \\sqrt{\\sigma_{p,\\text{sta}}^2 + \\sigma_{p,\\text{sys}}^2} \\). We found that the positional error of the brighter component J1 is dominated by the systematic error, while the statistical error contributes a significant fraction to the positional error of J2. The positional errors of J1 and J2, as well as the derived proper motions are tabulated in Supplementary Tables 3–5.\n\nPolarisation calibration\n\nThe VLBA observing project BZ071 presented in this paper was designed primarily as the preliminary exploratory attempt to detect a pc-scale polarised emission from the source. As the observing period was only 2 hours, the primary focus was on inferring the intensity and the location of the polarised emission; calibration of absolute electric vector position angle (EVPA) was not attempted since it would decrease already short total exposition on the target source. The unpolarised source 3C 84 was used as the instrumental polarisation (so-called ‘D-term’) calibrator.\n\nThe correlated visibilities were then imported into AIPS to calibrate the amplitudes and phases of the data, with further details as described previously in Methods data reduction. Additional steps included calibration of the RCP–LCP phase and delay offsets, and determination of the D-term of each telescope. The broad bandwidth of 256 MHz makes it difficult to correct the delay offsets in the RL and LR polarisations using the task RLDLY. To deal with this issue, two 128-MHz intermediate frequency channels (IFs) were first divided into eight 32-MHz sub-IFs using the task MORIF. Then we run the CROSSPOL procedure to check and calibrate the RCP–LCP delay offsets. Additional details are presented in the NRAO AIPS memo 79\\(^{41}\\). The AIPS task LPCAL was then used to determine the D-terms using the self-calibrated source model of 3C 84.\n\nAfter the calibration of visibility phase, amplitude and instrumental polarisation, the J0906+6930 data were imported into the Caltech Diffmap package for self-calibration and imaging. Several iterations of self-calibration and deconvolution were carried out until the signal-to-noise ratio in the image was below 5\\( \\sigma \\). After self-calibration, the Stokes I, Q and U components were separately imaged. The Stokes Q and U images were then combined to create the polarised intensity image\nusing the AIPS task COMB, shown in Figure 2. The rms noise in the combined polarised intensity image approaches the thermal noise 50 μJy beam⁻¹ estimated based on the observing time and telescope sensitivities. A 3σ threshold was used to remove the contamination from fake noise features when combining the polarised intensity image. In order to highlight the distribution of the polarised emission in the jet, the image was restored with a higher resolution beam, same as of the 2017 image. The polarised emission peaks at 0.8 mas southwest of the core, aligned in the direction of J2 and is slightly eastward offset from J1. The fractional polarisation is ≈10%, peak intensity is ≈0.6 mJy beam⁻¹ (~12 times above the rms noise). This is the preliminary detection of linear polarisation from a z > 5 blazar, at a rest frame frequency ~100 GHz.\n\nAlthough, as stated above, our project was not designed to reconstruct the EVPA of the yet to be detected polarised emission, once the detection was achieved, we reconstructed uncalibrated EVPA distribution following a standard procedure. EVPAs are calculated by using Stokes U and Q values, \\( \\mathrm{EVPA} = \\frac{1}{2} \\tan^{-1} \\frac{U}{Q} \\). Supplementary Figure 2 represents the polarised emission image of J0906+6930 with uncalibrated distribution of EVPA. While specific orientation of the EVPA cannot be treated physically due to the absence of its calibration, the orderly distributed electric vectors are consistent with the shock-compressed magnetic field model.\n\nRadio light curve\n\nThe source has been monitored by the Owens Valley Radio Observatory 40-m telescope monitoring program⁶² at 15 GHz from 2009. This enabled the verification of the amplitude calibration of the 15-GHz VLBA data. In Supplementary Figure 1 we plot the light curve together with our VLBA measurements in the 2017 and 2018 epochs. The new VLBA measurements are consistent with the single-dish flux densities (the inset of Supplementary Figure 1). This indicates that the integrated radio emission is dominated by the pc-scale compact core–jet. The dimming of the core and the brightening of J1 in 2017 and 2018 (in comparison to 2004 and 2005) possibly originates from the propagating shock (post the 2011 flare) interacting with the ISM.\n\nDoppler boosting parameters\nThe brightness temperatures of the VLBI core\n\\[\nT_B = 1.22 \\times 10^{12} \\frac{S}{D_{maj} D_{min} v^2} (1 + z) \\ K\n\\]\n(1)\n\nwhere S is the flux density (Jy) at the observing frequency ν (GHz), Dmaj and Dmin are the major and minor axis sizes of a Gaussian model (mas), and z is the redshift. T_B ranges from 18.0–47.5 × 10¹⁰ K with a mean \\( T_B = (30.2 \\pm 4.0) \\times 10^{10} \\ K \\).\n\nThe inverse Compton catastrophe prevents the synchrotron brightness temperature from exceeding a threshold of \\( \\approx 10^{12} \\) K⁴³. An energy equipartition between magnetic fields and relativistic particles in a synchrotron radio source sets a lower maximum brightness temperature \\( T_{B,\\text{eq}} \\) of \\( 5 \\times 10^{10} \\) K ³² than that theoretically expected⁸⁸,⁴⁴. T_B in excess of T_B,eq can be attributed to Doppler boosting of the relativistic jet beam. Using\n\\[\nT_B = \\delta T_{B,\\text{eq}}\n\\]\n(2)\n\nwhere \\( \\delta \\equiv [\\Gamma(1 - \\beta \\cos \\theta)]^{-1} \\) is the Doppler factor, \\( \\Gamma \\) is the bulk Lorentz factor and \\( \\beta \\) is the jet bulk speed (in units of c), we obtain \\( \\delta = 6.1 \\pm 0.8 \\). The bulk Lorentz factor \\( \\Gamma \\) and the viewing angle of the jet with respect to the observer line of sight \\( \\theta \\) are\n\\[\n\\Gamma = \\frac{\\beta_{\\text{app}}^2 + \\delta^2 + 1}{2 \\delta}\n\\]\n(3)\n\\[\n\\tan \\theta = \\frac{2 \\beta_{\\text{app}}}{\\beta_{\\text{app}}^2 + \\delta^2 - 1}\n\\]\n(2)\nWith a jet apparent transverse speed \\( \\beta_{app} = (2.5 \\pm 0.8) \\) c and \\( \\delta = 6.1 \\pm 0.9 \\), we obtain \\( \\Gamma = 3.6 \\pm 0.5 \\) and \\( \\theta = 6.8 \\pm 2.2^\\circ \\). These values are consistent with the parametric fitting of the spectral energy distribution\\(^{27}\\), where \\( \\delta = 9^{+3.5}_{-3} \\) and \\( \\theta \\leq 9.\\)^{6} were obtained.\n\nWe also estimate the Doppler factor from the variability of radio flux density\\(^{45,46}\\). The monitoring data at 15 GHz from the OVRO 40-m telescope\\(^{12}\\) is used for calculating the variability brightness temperature (\\( T_{B,\\text{var}} \\)). We modelled the flare with a Gaussian function :\n\n\\[\nS(t) = A \\exp \\left( -\\frac{(t - t_p)}{2 \\tau^2} \\right) + B\n\\]\n\nwhere S(t) is the source flux density (Jy), t is the observation time (days), B is the constant noise background (Jy), tp is the peak time (days), and \\( \\tau \\) is the characteristic flare rise timescale (days). We used a least squares fit to estimate the Gaussian parameters, \\( t_p = 2012 \\) May 20, \\( \\tau = 847 \\) days, \\( A = 0.149 \\) Jy, \\( B = 0.061 \\) Jy. The fitted parameters give a variability brightness temperature, \\( T_{B,\\text{var}} = 5.7 \\times 10^{12} \\) K. The corresponding Doppler factor is \\( \\delta_{\\text{var}} = \\sqrt[3]{\\frac{T_{B,\\text{var}}}{T_{B,\\text{eq}}}} = 4.8 \\).\n\nThis value is consistent but marginally lower than that derived from the above VLBI model fitting.\n\n**Maximum proper motion**\n\nThe proper motion can be expressed as\n\n\\[\n\\mu = \\frac{\\beta_\\perp c}{D_A}\n\\]\n\nwhere \\( \\beta_\\perp \\) is the transverse jet speed, \\( a = (1 + z)^{-1} \\) and \\( D_A \\) is the angular size distance. This can be approximated in terms of the Hubble distance \\( c/H_0 \\) as\\(^{47}\\)\n\n\\[\nD_A = \\frac{c}{H_0} \\frac{a}{g(a)}\n\\]\n\nwhere\n\n\\[\ng(a) = \\left( \\frac{a}{1-a} + 0.2278 + \\frac{0.027(1-a)}{0.785+a} - \\frac{0.0158(1-a)}{(0.312+a)^2} \\right)\n\\]\n\nUsing equations (6), (7) and \\( \\beta_\\perp \\approx \\Gamma \\beta \\) (for an extremely beamed jet) in equation (5), the maximal proper motion\n\n\\[\n\\mu_{\\text{max.}} \\leq H_0 \\Gamma \\beta g(a)^{-1}\n\\]\n\\[\n\\mu_{\\text{max.}} = (0.1 \\text{ mas yr}^{-1}) \\left( \\frac{\\Gamma}{3.6} \\right) \\left( \\frac{H_0}{70 \\text{ km s}^{-1} \\text{ Mpc}^{-1}} \\right)\n\\]\n\nfor \\( z = 5.47 \\) and \\( \\beta = 1 \\).\n\n**Black hole mass and jet activity**\n\nThe previous black hole mass estimate of \\( M_{BH} = 4.2 \\times 10^9 M_\\odot \\)\\(^{27}\\) is in tension with the inferred observational signatures of the source resembling a high frequency peaker, which typically have moderately lower masses in the range \\( 10^{7.5} - 10^8 M_\\odot \\)\\(^{48}\\). The earlier estimates are based on scaling relations relevant to non-jetted quasars. However, the employed luminosity requires to be Doppler beaming corrected for a jetted quasar\\(^{49}\\). For the blazar J0906+6930, comparing the scaled broad line region (BLR) radius \\( r_{BLR} = (5.8 \\times 10^{16} \\text{ cm}) \\left[ \\frac{\\lambda L_\\lambda(1350 \\text{ \\AA})}{10^{44} \\text{erg s}^{-1}} \\right]^{0.61} \\)\\(^{49}\\) with \\( r_{BLR} = (9.54 \\times 10^{16} \\text{cm})(\\dot{m} m_9)^{0.5} \\) where \\( \\dot{m} \\) is the mass accretion rate scaled in Eddington units and \\( m_9 = \\frac{M_{BH}}{10^9 M_\\odot} \\)\\(^{50}\\), results in \\( \\left( \\lambda L_\\lambda (1350 \\text{ \\AA}) \\right) = (2.6 \\times 10^{44} \\text{ erg s}^{-1})(\\dot{m} m_9)^{0.82} \\). Using this in the revised scaling relation \\( m_9 = 3.26 \\times 10^{-3} \\left[ \\frac{\\lambda L_\\lambda(1350 \\text{ \\AA})}{10^{44} \\text{erg s}^{-1}} \\right]^{0.61} \\left[ \\frac{v}{10^3 \\text{km s}^{-1}} \\right]^2 \\) where \\( v \\) is the full-width at the half-maximum velocity as inferred from the emission line\\(^{49}\\), for \\( m \\leq 1 \\)\\(^{51}\\) and \\( v = 6000 \\) km s\\(^{-1}\\)\\(^{27}\\), we obtain \\( M_{BH} = 4.4 \\times 10^7 M_\\odot \\) which is consistent with the above expectation from the population of sources. The lower mass and a similarity to a young AGN indicate the ongoing evolution of the black hole\\(^{48}\\), with feedback transitioning from accretion dominated (radiative) to the onset of the jet (momentum) driving possibly resulting in a black hole – galaxy co-evolution.\n\nThe formation and rapid growth of SMBHs in the early Universe remains debatable. That can be enabled by a combination of accretion and fuelling, AGN feedback through radiation and jet interaction with the large-scale environment, and galaxy mergers. The accompanying jet activity includes a component ejection associated with a major flare with nearly constant amplitudes and lack of a time delay when observed at different frequencies\\(^{52}\\). The jet structure and kinematic evolution can result from scenarios alternative to the bending due to interaction. These include a helical trajectory\\(^{53}\\), instabilities in the jet\\(^{54,55}\\) possibly induced by the surrounding environment or through turbulent loading at the jet base\\(^{56,57}\\). In these cases, the jet is non-nascent and could either be an ongoing process or episodic. This would indicate a departure from the young AGN\nscenario, and point towards a relatively lower powered evolved blazar with possibly large-scale morphology. These can be addressed through the continued observation of this and similar sources at various physical scales (pc–kpc) and from an accumulated statistically viable sample.\n\nJet and ISM properties\nAssuming the convention \\( S_\\nu \\propto \\nu^\\alpha \\), a core spectral index of \\( \\alpha = 0 \\) is assumed based on the inference of a spectral turnover near 10 GHz\\(^{15,16}\\), also indicated by similar core flux densities at 8.4 GHz and 15 GHz during the 2004 epoch\\(^{15}\\). The average monochromatic radio power of the core-jet,\n\n\\[\n\\overline{P}_\\nu = 4 \\pi D_L^2 S_\\nu (1 + z)^{-1-\\alpha}\n\\]\n\n(9)\n\nWith a luminosity distance \\( D_L = 53.66 \\) Gpc (\\( z = 5.47 \\) for J0906+6930) obtained using CosmoCalc\\(^{58} \\), \\( \\overline{S}_{\\text{core},15\\,\\text{GHz}} = 90.94 \\pm 5.18 \\) mJy and the above \\( \\alpha = 0 \\), \\( L_{\\text{radio}} \\approx v_{15\\,\\text{GHz}} \\overline{P}_{\\text{core},15\\,\\text{GHz}} = (7.28 \\pm 0.42) \\times 10^{44} \\text{erg s}^{-1} \\). A standard \\( \\Lambda \\)CDM cosmological model with \\( H_0 = 70 \\) km s\\(^{-1}\\) Mpc , \\( \\Omega_\\Lambda = 0.73 \\) and \\( \\Omega_M = 0.27 \\) was used. The radiative and kinetic contributions to the jet luminosity \\( L_{\\text{jet}} \\) are related to the radio luminosity by the empirical relations\\(^{59}\\)\n\n\\[\n\\log L_{\\text{jet,rad}} = (12 \\pm 2) + (0.75 \\pm 0.04) \\log L_{\\text{radio}}\n\\]\n(10)\n\n\\[\n\\log L_{\\text{jet,kinetic}} = (6 \\pm 2) + (0.90 \\pm 0.04) \\log L_{\\text{radio}}\n\\]\n(11)\n\nThe jet luminosity is taken as the addition of the radiative and kinetic contributions and is \\( L_{\\text{jet}} = 2.8 \\times 10^{46} \\) erg s\\(^{-1}\\), and is \\( 2.2 \\times 10^{43} \\) erg s\\(^{-1}\\) using \\( \\delta = 6.0 \\) as inferred in Appendix F. This is ~0.02 \\( L_{\\text{edd}} \\), where \\( L_{\\text{edd}} = (1.3 \\times 10^{47} \\) erg s\\(^{-1}\\))\\( m_g \\) is the Eddington luminosity and using \\( m_g = 4.4 \\times 10^{-2} \\) as inferred from Appendix H. It must be noted that the empirical relations have a large scatter mainly due to the diversity in the sources constituting the inference, ranging from radio-loud AGN to X-ray binaries, and having to properly account for spectral state transitions, variability and systematics from comparison of data from different databases\\(^{59}\\). The uncertainty on the jet power may then be underestimated.\n\nUnder conditions of an ambient ISM (non-relativistic), the momentum flux balance between the jet and the ISM \\( ^{60} \\)\n\n\\[\n\\frac{L_{\\text{jet}}}{(\\beta_{\\text{jet}} - \\beta_h)c} = \\rho_{\\text{ISM}} \\beta_h^2 c^2 A_h\n\\]\n\n(12)\n\nwhere \\( L_{\\text{jet}} \\) is the jet luminosity, \\( \\beta_{\\text{jet}} \\) is the jet speed (in units of \\( c \\)), \\( \\rho_{\\text{ISM}} \\) is the ISM density, \\( \\beta_h \\) is the speed of the advancing jet head (in units of \\( c \\)) and \\( A_h \\) is the surface area of the jet head interacting with the ISM.\n\nThe average core separation from J1, \\( r_{1}/\\sin \\theta = 43.2 \\) pc from which, the circumferential radius in contact with the ISM \\( r_h = r_{1}/2 = 21.6 \\) pc and \\( A_h \\approx r_h^2 \\sin \\theta_0 = 82.9 \\) pc\\(^2\\) assuming an intrinsic jet half-opening angle \\( \\theta_0 = 10^\\circ \\)\\(^{61}\\). The relativistic transformation,\n\n\\[\n\\beta = \\frac{\\beta_{\\perp}}{\\sin \\theta + \\beta_{\\perp} \\cos \\theta}\n\\]\n\n(13)\n\nrelates the projected transverse speed (proper motion) \\( \\beta_{\\perp} \\) with the true speed \\( \\beta \\) through the inclination angle \\( \\theta \\). The jet speed \\( \\beta_{\\text{jet}} \\sim \\beta_{12} = 0.96 \\) \\( c \\) based on a \\( \\beta_{\\perp,2} = 2.5 \\) \\( c \\) and using the above relativistic transformation. The speed of the jet head \\( \\beta_h < \\beta_{12}/4 = 0.24 \\) \\( c \\) (upper limit on the speed of the shocked expanding gas at the jet head post interaction with the ISM), assuming a strong shock interaction which entails a post shock plasma with the above maximal speed. The density contrast between the ISM and jet\\(^{60} \\) is\n\n\\[\n\\frac{\\rho_{\\text{ISM}}}{\\rho_{\\text{jet}}} = \\left( \\frac{\\beta_{\\text{jet}}}{\\beta_h} - 1 \\right)^2\n\\]\n\n(14)\nusing which \\( \\rho_{ISM}/\\rho_{jet} > 9 \\), likely resulting in the lower density jet being susceptible to a deflection or bending upon interaction with the ISM, while being able to cause a compression of the material near the jet head. Employing the above calculated quantities and the simplifying assumptions in equation (12), \\( \\rho_{ISM} \\geq 2.4 \\times 10^{-26} \\) g cm\\(^{-3}\\) which corresponds to a number density \\( n_e \\geq 26.6 \\) cm\\(^{-3}\\).\n\nData Availability\nAll data used in this study are public and can be accessed through the different data archives of the various instruments. NRAO VLBA archive: https://archive.nrao.edu/archive/advquery.jsp, OVRO archive: http://www.astro.caltech.edu/ovroblazars/data.php?page=data_query. The authors can provide data supporting this study upon request.\n\nCode Availability\nUpon reasonable request the authors will provide all code supporting this study. Astronomical Image Processing System (AIPS) software can be found at http://www.aips.nrao.edu/index.shtml. Difmap software can be found at ftp://ftp.astro.caltech.edu/pub/difmap/.\n\nReferences\n1. Volonteri, M. The formation and evolution of massive black holes. Science, **337**, 544-547 (2012).\n2. Fabian, A. C. Observational evidence of active galactic nuclei feedback. Ann. Rev. Astron. Astrophys. **50**, 455-489 (2012).\n3. Fan, X. et al. The discovery of a luminous z=5.80 quasar from the Sloan Digital Sky Survey. Astron. J. **120**, 1167-1174 (2000).\n4. Fan, X. et al. A Survey of z>5.8 Quasars in the Sloan Digital Sky Survey. I. Discovery of three new quasars and the spatial density of luminous quasars at z~6. Astron. J. **122**, 2833-2849 (2001).\n5. Coppejans, R. et al. 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X-Ray Variability and the Inner Region in Active Galactic Nuclei. Astrophys. J. **791**, 74 (2014).\n52. Valtaoja, E. H. et al. Five years monitoring of extragalactic radio sources. III. Generalized shock models and the dependence of variability on frequency. Astron. Astrophys. **254**, 71-79 (1992).\n53. Mohan, P. & Mangalam, A. Kinematics of and Emission from Helically Orbiting Blobs in a Relativistic Magnetized Jet. Astrophys. J. **805**, 91 (2015).\n54. Hummel, C. A et al. MERLIN and VLBI observations of the quasar 0836+710 : morphology of a parsec-kiloparsec scale jet. Astron. Astrophys. **266**, 93-100 (1992).\n55. Zhao, W. et al. Radio structure of the blazar 1156 + 295 with sub-pc resolution. Astron. Astrophys. **529**, A113 (2011).\n56. Britzen, S. et al. A new view on the M 87 jet origin: Turbulent loading leading to large-scale episodic wiggling. Astron. Astrophys. **601**, A52 (2017).\n57. An, T. et al. Periodic radio variabilities in NRAO 530: a jet-disc connection? Mon. Not. R. Astron. Soc. **434**, 3487-3496 (2013).\n58. Wright, E. L. A Cosmology calculator for the World Wide Web. Publ. Astron. Soc. Pac. **118**, 1711 (2006).\n59. Foschini, L. The Unification of Relativistic Jets, International Journal of Modern Physics: Conference Series **28**, id. 1460188 (2014).\n60. Ferrari, A. Modeling extragalactic jets. Ann. Rev. Astron. Astrophys. **36**, 539-598 (1998).\n61. Pushkarev, A. B., et al. MOJAVE - XIV. Shapes and opening angles of AGN jets. Mon. Not. R. Astron. Soc., **468**, 4992-5003 (2017).\n\nAcknowledgements\n\nThis work is funded by the National Key R&D Programme of China (2018YFA0404603), the Chinese Academy of Sciences (CAS, 114231KYSB20170003), and the Hungarian National Research, Development and Innovation Office (2018-2.1.14-TET-CN-2018-00001). P.M. is supported by CAS-PIFI (2016PM024) post-doctoral fellowship and the NSFC grant (11650110438). K. É. G. was supported by the János Bolyai Research Scholarship of the Hungarian Academy of Sciences and by the ÚNKP-19-4 New National Excellence Program of the Ministry for Innovation and Technology. This research has made use of data observed with the Very Long Baseline Array of the National Radio Astronomy Observatory (project codes: BR093, BG154, BZ068, BZ071). The NRAO is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. We acknowledge the use of calibrated visibility data from the Astrogeo Center Database maintained by L. Petrov and the lightcurve data from the OVRO 40-m monitoring program which is supported in part by NASA grants NNX08AW31G, NNX11A043G, and NNX14AQ89G and NSF grants AST-0808050 and AST-1109911.\n\nSupplementary Information\nSupplementary Figures 1 and 2\nSupplementary Tables 1-5\nSupplementary Note\n\nFigures\nFig. 1 Radio morphology of J0906+6930 derived from VLBA observations at six epochs. The data of 2005 March 22 and 2005 May 15 are combined to create a single image (panel c). Symbols (elliptical and circular Gaussian) represent the model fitting of emission components. Detailed imaging parameters are listed in Supplementary Table 2. The noise rms is 0.18, 0.19 and 0.16 mJy beam^{-1} for the 2004 – 2005 epoch images (panels a, b and c respectively) and is much smaller at 0.034 mJy beam^{-1} and 0.057 mJy beam^{-1} for the 2017 and 2018 epoch images (panels d and e respectively). The core C is the brightest and most compact. Two jet components, marked as J1 and J2, are detected within 1.5 mas away from the core. The contours increase by a factor of 2. The grey ellipse at the bottom left corner of each panel represents the full width at half maximum (FWHM) of the restoring beam.\n\nFig. 2 Linear polarisation image (colored scale) of J0906+6930. The images are derived from the 15-GHz VLBA observation on 2018 January 31. The core is denoted by C and jet components by J1 and J2. The contours represent Stokes I intensity, same as Figure 1 panel e. The colored scale denotes the strength of the linear polarisation. The gray-shaded ellipse in the bottom left corner is the restoring beam. The peak of the polarised intensity, ~0.6 mJy beam^{-1}, is about 0.8 mas southwest of the total intensity core. The maximum fractional polarisation is ~10% appearing at the southernmost of the polarised component. The core region is weakly polarised. This is the only polarisation measurement in a radio-loud quasar at redshift > 5 so far.\nFig. 3 Radial distance of J1 and J2 as a function of observing time. The straight lines (blue line for J1 and red line for J2) represent a linear regression fit to infer the jet proper motion. The denoted error bars on each point are the 1σ errors (see Table 1). That gives \\( \\mu(J1) = -0.006 \\pm 0.004\\text{yr}^{-1} \\), and \\( \\mu(J2) = 0.019 \\pm 0.006 \\) mas.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Epoch (yyyy mm dd)Com pStotal (mJy)Dmaj (mas)Dmin (mas)φ (°)R (mas)PA (°)TB (\\( \\times 10^{10} \\) K)
(1)(2)(3)(4)(5)(6)(7)(8)(9)
2004 02 27C119.5±6.30.206±0.0050.041±0.00140.9±0.9--47.5±3.0
J17.2±0.70.396±0.051--0.825±0.068222.2±1.1-
2004 11 22C127.3±6.60.269±0.0020.065±0.00228.1±0.1--24.4±1.5
J18.7±0.80.279±0.027--0.906±0.064225.0±0.3-
2005 03 22 & 2005 05 15C122.7±6.40.209±0.0010.067±0.00255.3±0.1--31.0±1.8
J18.4±0.60.267±0.007--0.944±0.052224.7±0.2-
J21.9±0.30.321±0.053--1.290±0.061179.8±1.3-
2017 09 11C43.4±2.30.260±0.0010.032±0.00149.4±0.1--18.0±1.1
J120.4±1.10.291±0.001--0.814±0.049222.2±0.1-
J21.0±0.10.270±0.033--1.568±0.053184.6±0.1-
2018 01 31C41.8±2.20.249±0.004>0.03452.2±1.3-->17.1
J118.0±1.00.170±0.001--0.801±0.071222.8±0.1-
J21.4±0.20.444±0.079--1.435±0.076184.8±0.9-
\n\na Parameters are derived from modeled Stokes LL images. Column (1) presents the observation epoch. Column (2) gives the label of the VLBI components. Column (3) presents the integrated flux density of all VLBI components. Columns (4) to (5) give the major and (in case of ellipticals) the minor axis sizes (FWHM) of the fitted Gaussian models. Column (6) is the position angle of the major axis of Gaussian, measured from north to east. The data from 2005 March 22 and May 15 were combined before model fitting. Columns (7) and (8) give the radial distance R of components with respect to the core, and the position angle measured from north to east. Column (9) lists the calculated brightness temperature of the core. For the unresolved core, a maximum size is estimated, thus the lower limit of T_B is given.\nSupplementary Figures\n\n![Light curve plot showing OVRO and VLBA flux densities over time](page_184_232_1079_563.png)\n\nSupplementary Figure 1 The 15 GHz light curve of J0906+6930. The compiled and newly measured VLBA flux densities (shown as red points) are overlaid on the 15 GHz single dish flux densities (shown as blue points) from the Owens Valley Radio Observatory (OVRO). A prominent flare with a peak flux density of ~220 mJy occurs close to the end of 2011. The source flux density gradually decreases afterwards. The inset shows the latest epoch VLBI data points overlaid on the single-dish light curve, showing good consistency. The source flux density in 2017-2018 is at a minimum. Three earlier epoch VLBA data points are also plotted. The error bars on the OVRO data points are based on the reported flux densities, and those on the VLBA points are based on the 1σ errors on the total flux densities (core and jet, see Table 1 of the main article).\n\n![Polarisation image of J0906+6930](page_184_1012_1079_563.png)\n\nSupplementary Figure 2 The polarisation image of J0906+6930 (January 31, 2018). The color scale represents the linear polarisation, the unit of the colorbar is in mJy beam^{-1}. The Stokes I intensity image is shown as contours. The rms level in the image is 0.057 mJy beam^{-1}. The short blue-colored lines overlaid on the color gradients (dark\norange shaded area) represent the uncalibrated electric vector position angle (EVPA) orientations. The length of the blue line denotes the polarisation intensity, 1 mas = 1.25 mJy beam$^{-1}$. The ellipse in the bottom left corner is the restoring beam, which is 1.38 mas $\\times$ 0.53 mas, at a major axis position angle of 10.8$^\\circ$.\nSupplementary Tables\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
NO.Project codev (GHz)DateTimea (min)Participating antennabBandwidthc (MHz)ref.
1BR09315.42004 Feb 2775VLBA all 1016×2 (LCP+RCP)1,16
2BG154x15.42004 Nov 22120VLBA all 1016×2 (LCP+RCP)3
3BG154B14.42005 Mar 2240VLBA 8 (no PT, SC)64×1 (LCP+RCP)16
4BG154E15.42005 May 15120VLBA 9 (no Br)16×2 (LCP+RCP)16
5BZ06815.22017 Sep 11400VLBA 9 (no SC)128×2 (LCP+RCP)3
6BZ07115.22018 Jan 3180VLBA 9 (no SC)256×2 (LCP+RCP)3
\n\nSupplementary Table 1. Observation setup and logs. a: The total observation time spent on the target source, in minutes. b: General VLBA observations contain the following ten telescopes: Brewster (BR), Fort Davis (FD), Hancock (HN), Kitt Peak (KP), Los Alamos (LA), Mauna Kea (MK), North Liberty (NL), Owens Valley (OV), Pie Town (PT), and Saint Croix (SC). One or two telescopes did not participate in some observations because of technical problem or maintenance. c: Total bandwidth of the recording backends, in MHz. LCP — left-handed circular polarisation; RCP — right-handed circular polarisation.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Figure LabelProject CodeRestoring Beam (θmaj, θmin, PA)Speak (mJy beam-1)rms (mJy beam-1)
1aBR0931.46×0.48, −0.79121.40.180
1bBG154x1.36×0.45, 0.90119.00.190
1c*BG154B&E0.73×0.55, −15.5114.30.160
1dBZ0680.87×0.60, −14.240.00.034
1eBZ0711.38×0.53, 10.841.60.057
\n\nSupplementary Table 2. Image parameters. *: owing to their closeness in time, the data of BG154B and BG154E were combined to make a single image.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
EpochσR, staσR, sysσR
2004 02 270.0180.0550.058
2004 11 220.0120.0630.064
2005 comb0.0060.0520.052
2017 09 110.0010.0490.049
2018 01 310.0020.0710.071
\n\nSupplementary Table 3. Positional errors of component J1.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
EpochσR, staσR, sysσR
2005 comb0.0330.0550.061
2017 09 110.0190.0630.053
2018 01 310.0280.0520.076
\n\nSupplementary Table 4. Positional errors of component J2.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Comp.μ(RA)μ (Dec)μ (R)
J1−0.005±0.003−0.004±0.003−0.006±0.004
J20.010±0.0050.019±0.0050.019±0.006
\n\nSupplementary Table 5: Proper motion results (in unit of mas/yr). Note - the proper motion μ(R) is the square root of the sum of squares of μ(RA) and μ(Dec). The significance of μ(Dec, J2) is larger than 3σ , roughly along the C-J2 direction, indicating the jet expansion.\nSupplementary Note\n\nWe use new 15-GHz data observed with the VLBA in 2017 and 2018, archival VLBA data obtained in 2004–2005 (see details in Supplementary Table 1) and the flux densities reported by the 40 m telescope at the Owens Valley Radio Observatory (OVRO) to explore the evolution of the source morphology and infer its physical characteristics. The OVRO 15 GHz data enabled the verification of the amplitude calibration of the 15-GHz VLBA data. In Supplementary Figure 1 we plot the light curve together with our VLBA measurements in the 2017 and 2018 epochs. The new VLBA measurements are consistent with the single-dish flux densities (the inset of Supplementary Figure 1). This indicates that the integrated radio emission is dominated by the pc-scale compact core–jet. The dimming of the core and the brightening of J1 in 2017 and 2018 (in comparison to 2004 and 2005) possibly originates from the propagating shock (post the 2011 flare) interacting with the interstellar medium.\n\nAlthough, as stated in the main text, our project was not designed to reconstruct the electric vector position angle (EVPA) of the yet to be detected polarised emission, once the detection was achieved, we reconstructed uncalibrated EVPA distribution following a standard procedure. EVPAs are calculated by using Stokes U and Q values, \\( \\mathrm{EVPA} = \\frac{1}{2} \\tan^{-1} \\frac{U}{Q} \\). Supplementary Figure 2 represents the polarised emission image of J0906+6930 with uncalibrated distribution of EVPA. While specific orientation of the EVPA cannot be treated physically due to the absence of its calibration, the orderly distributed electric vectors are consistent with the shock-compressed magnetic field model.\n\nThe fitted Gaussian models are presented in Table 1. The positional errors of J1 and J2, as well as the derived proper motions are tabulated in Supplementary Tables 3–5.\n\nReferences\n1. Romani, R. W., Sowards-Emmerd, D., Greenhill, L. & Michelson, P. Q0906+6930: the highest redshift blazar. Astrophys. J. **610**, L9-L11 (2004).\n2. Zhang, Y. et al. J0906+6930: a radio-loud quasar in the early Universe. Mon. Not. R. Astron. Soc. **468**, 69-76 (2017).\n3. the present paper."} {"paper_id": "prb13", "title": "A Brain Connectome Biomarker for Sleep Health", "text": "# Abstract\n\nSleep health is both conceptually and operationally a composite concept containing multiple domains of sleep. In line with this, high dependence and interaction across different domains of sleep health encourage a transition in sleep health research from categorical to dimensional approaches that integrate neuroscience and sleep health. Here, we seek to identify the covariance patterns between multiple-sleep health domains and distributed intrinsic functional connectivity by applying a multivariate approach (partial least squares). This multivariate analysis revealed a composite sleep health dimension co-varying with connectivity patterns involving the attentional and thalamic networks and which appear relevant at the neuromolecular level. These findings were further replicated and generalized to several unseen independent datasets. Critically, the identified sleep-health related connectome showed diagnostic potential for insomnia disorder. These results together delineate a brain connectome biomarker for sleep health with high potential for clinical translation.\n\n- Biological sciences/Neuroscience/Cognitive neuroscience/Consciousness\n- Biological sciences/Neuroscience/Cognitive neuroscience\n- Sleep health\n- Dimensional approach\n- resting-state functional connectivity\n- Classification\n- Attentional and thalamus networks\n\n# Introduction\n\nJust as proper nutrition is not a unitary construct, sleep health (SH) is viewed as a multidimensional construct12. Sleep health has been defined as “a multidimensional pattern of sleep-wakefulness, adapted to individual, social, and environmental demands, that promotes physical and mental well-being”3. Resting on this theoretical consideration and previous researches examining associations between different sleep measures and health outcomes345, sleep health mainly consists of six domains of sleep and circadian functioning: Regularity in sleep, Satisfaction with sleep/sleep quality, Alertness during waking hours, Timing of sleep, Sleep Efficiency/Continuity, and Sleep Duration (Ru-SATED). Emerging studies also pointed out that there exist other domains that can be considered as relevant to the construction of sleep health, such as sleep quality6, insomnia symptoms7 and sleep medication use7.\n\nRecent studies have begun to construct a sleep health composite towards studying multiple domains of sleep18910. Indeed, previous research has mostly focused on single indicators of sleep health, making it difficult to provide a consistent guideline for research and practical settings6. A composite measure not only would provide a more comprehensive indicator of sleep health than any single standard measure111213 but also would be less prone to noise and hence could present a greater neurobiological validity14. For instance, Dalmases and colleagues reported that the Ru-SATED score was more strongly linked with self-rated health status than sleep duration alone15. Nonetheless, considerations of constructing a sleep health composite with multi-domains of sleep health rather than individual sleep metrics is still an emerging research area with many remaining gaps in the literature14. In particular, the neurobiological validity of a composite score could be importantly increased by capitalizing on its association with intrinsic functional connectivity in the population.\n\nResting-state networks are typically derived from the connectivity profile of spontaneous fluctuations in functional MRI (fMRI) signal and are thought to reflect the intrinsic brain functional connectivity1617. Converging research evidence across datasets, methods, and laboratories has agreed upon the principle resting-state networks such as the somatomotor, visual, default mode, and fronto-parietal control networks1819. In that context, resting-state functional connectivity (RSFC), such as the anti-correlations between the default mode network (DMN) and the task positive network (TPN) was found to be a reliable biomarker to classify different sleep stages [for a review, see20]. Also, RSFC was found to be influenced by sleep deprivation evidenced by the reduced connectivity within the DMN21, the dorsal attention network (DAN), and the auditory, visual, and motor networks [for a tabular overview, see16]. Moreover, abnormalities in functional network modules subserving hyperarousal, salience, sensory-motor, cognitive and self-referential processes, including the limbic, thalamus, sensory-motor, fronto-parietal control and default mode networks have been shown in insomnia disorder [for a review, see2223]. These lines of research together suggest RSFC contains crucial information underlying the neurobiological mechanisms of different aspects of sleep health.\n\nActually, RSFC has been shown to be associated to some domains of sleep health such as sleep duration24, sleep quality25 and timing of sleep (or chronotype)26. Despite this increasing interest in revealing the interplay between intrinsic brain functional connectivity and domains of sleep health, existing studies have been limited in several respects. First, most have adopted a categorical approach, or only examined a single domain of sleep health, and are therefore unable to capture the heterogeneity across different sleep health domains. Second, constructions of sleep health composite were mainly driven by the conceptual Ru-SATED model, rather than being guided by the intrinsic structure of brain and behavior features. Third, existing work in sleep health composite has often used relatively small samples (e.g., dozens of participants)27. While multivariate techniques allow the examination of both multiple brain systems and sleep health domains simultaneously, such techniques usually require large samples2829. Also in line with these considerations, the high dependence and interaction across different domains of sleep health encourages a transition in sleep health research14 from categorical to dimensional approaches that integrate intrinsic brain functional connectivity and sleep health.\n\nIn this study, we addressed this research gap by relating RSFC to a large set of sleep health measures in a single integrated analysis to identify a brain connectome biomarker for sleep health. More specifically, we addressed the following four research questions (Figure 1): 1) Can we identify a composite sleep health dimension that relates to RSFC patterns? 2) Can the obtained dimension be replicated and generalized to unseen independent datasets? 3) What is the neuromolecular relevance (based on neurotransmitter receptor maps30) of the brain connectome underlying interindividual differences in sleep phenotype? 4) Does the sleep-health related brain connectome have predictive utility for both health population and insomnia disorder?\n\nTo answer these questions, we first capitalized on a large sample of young adults from the Behavioral Brain Research Project to Chinese Personality (BBP) by applying a machine learning technique called partial least squares (PLS)313233. As a multivariate data-driven statistical technique, PLS is capable of discovering the latent dimensions that link interindividual variability in intrinsic functional organization to interindividual variability in behavioral measures spanning multiple domains of sleep health. To comprehensively assess this latter, we included measures suggested by the Ru-SATED model, but we also incorporated several additional metrics associated with sleep health defined broadly6, that are: 1) beliefs, attitudes, and habits about sleep, considering that individuals with more-positive beliefs and attitudes about sleep or who adopt sleep-protective behaviors are more likely to experience better sleep health34; 2) sleep deficiency which also incorporates insomnia symptoms, sleep disorders and sleep medication use, considering both sleep health and sleep deficiency can be regarded as the anchors at either end of a continuum3; 3) have one slept enough, whether one felt refreshed upon waking35, the necessity of nap and the needed nap time were also incorporated to evaluate the satisfaction with sleep/sleep quality6; 4) tendency to engage in spontaneous waking thought36, attention related deficiency37 and fatigue38 as supplements to assess the alertness during waking hours. To ensure that the latent dimensions linking sleep phenotype to RSFC uncovered by PLS were robust, multiple control analyses were performed. Furthermore, as multivariate approaches in high-dimensional data such as PLS are prone to overfitting, a 10-fold cross-validation was performed here to assess the generalization performance of the latent dimensions to unseen test data.\n\nAs described below, we uncovered one latent dimension of the RSFC that was highly correlated with one latent dimension of sleep health in a discovery dataset (n=687). This dimension was characterized by a specific spectrum of sleep health-related measures and by specific RSFC features. These latter appeared as a neurobiologically relevant connectome since the RSFC loadings were spatially correlated with the distribution of several neurotransmitter systems relevant for sleep health, including serotonin receptors, as well as metabotropic glutamate receptor 5 (mGluR5) and the γ-Aminobutyric acid type A (GABAA) receptor3940. Furthermore, the associative pattern was successfully replicated, and the model showed generalizability in an internal validation dataset (n = 628). Importantly, the identified connectome pattern shows predictive utility for sleep quality in an independent sample consisting of unrelated individuals from the Human Connectome Project (HCP) dataset (n=435). Finally, this connectome pattern critically shows diagnostic potential to distinguish insomnia patients (n=52) from sleep healthy subjects (n=49) with an accuracy of 79.12%. These results hence delineated a sleep health dimension whose associated functional connectome could serve as an objective neuroimaging biomarker in clinical translations, such as to assess sleep-based interventions for improving brain health.\n\n# Results\n\nPLS Model Reveals One Robust Dimension Linking Sleep Health and Resting-state Function Connectivity\n\nWe sought to delineate multivariate relationships between resting state functional connectivity and sleep health in a large discovery dataset (n=687). To this end, we applied PLS, an unsupervised machine learning technique that seeks to find covariance between two high-dimensional matrices, namely whole brain RSFC and 36 behavioral measures spanning multiple domains of sleep health. Following pre-processing using a validated pipeline that minimizes the impact of in-scanner motion (see Online Methods section), we constructed subject-level RSFC using a 246-node parcellation system that includes 210 cortical regions and 36 subcortical regions. Prior to analysis with PLS, we regressed age, sex, handedness, and head motion out of both the RSFC and behavior data to ensure that these potential confounders did not drive results. The input data thus consisted of 30,135 unique functional connections and 36 sleep health related variables. The selection of the sleep health measures was based on the consideration to select available variables in the BBP that 1) represent central domains of SH described in the Ru SATED as well as in the National Sleep Foundation (NSF)’s Sleep Health Index; 2) provide high consistency with previous SH studies; 3) draw a multifaceted picture of SH to a bigger extent based on its broader definition. On that basis, the chosen 36 variables were grouped into seven domains including 1) Satisfaction with sleep/Sleep quality; 2) Alertness during waking hours; 3) Timing of sleep; 4) Sleep efficiency/continuity; 5) Sleep duration; 6) Sleep deficiency; 7) Sleep beliefs, attitudes, and habits (see Online Methods and table S1 for the details).\n\nFigure 2a shows the amount of covariance explained by each latent variable (LV). Notably, only one LV (LV1) survived after permutation testing with FDR correction (q<0.05) (Figure 2b). Importantly, several control analyses were performed to ensure the robustness of the obtained LV1. See Tables S2 for details. First, 10-fold cross-validation was successful; PLS components estimated from 90% of the participants successfully generalized to the remaining 10% of participants, as indicated by significant correlation between RSFC and behavioral composite scores in the test folds (LV1, mean r = 0.17, permuted p <3.0x10−3). It should be noted that, to avoid data leakage issue, the adjustment for confounds and data standardization were performed within the cross-validation loop (i.e., at first, we estimated parameters of data standardization and confounds regression in the nine training folds and then applied the obtained parameters to the test fold). Second, PLS components were robust to global signal regression, total intracranial volume regression, the pre-scanning positive and negative affect regression, body mass index (BMI) regression and family income regression, as indicated by the high correlation (r > 0.93, Table S2) between saliences of original PLS and PLS with corresponding variable regression. Third, instead of regressing age, sex, handedness, and head motion from the data, these variables were added to the phenotypic data for the PLS analysis. The results were largely unchanged as indicated by the high correlation (r > 0.92, Table S2) between saliences of original PLS and PLS with adding age, sex, handedness and motion into the phenotypic data. Fourth, PLS components were not driven by the non-Gaussian distributions of the behavioral data and skewed behavioral distributions, as indicated by the high correlation (r > 0.98, Table S2) between saliences of original PLS and PLS with quantile normalization to improve the Gaussian distributions of the behavioral data. Fifth, the results remained largely unchanged when using a different Seitzman et al’ Atlas containing 300 regions for the RSFC construction, as indicated by the high correlation (r = 0.99 for behavior data; r = 0.78 for RSFC data) between loading scores of Brainconnectome Atlas and Seitzman et al’ Atlas, see details in Supplementary results, Figure S1 and S2.\n\nThis survived dimension (LV1) accounted for 28.6% of RSFC-behavior covariance (figure 2a), with significant association (r=0.50, permuted p = 9.9x10−4) between RSFC and behavioral composite scores (figure 2b). Figure 2c shows the top correlations between LV1’s behavioral composite/loading score and the 27 significant sleep health measures. Greater behavioral composite score was associated with poorer sleep health (e.g., poor sleep quality, insomnia, hyperarousal, dysfunctional beliefs and attitudes about sleep, physical fatigue, not get enough sleep). Correlations between LV1’s RSFC composite/loading scores and the RSFC data are shown in Figure 2d (unthresholded correlations) and figure 2e (significant correlations). The significant edges were widely distributed throughout the brain, contain a small portion of the total edges in the connectome (5982 edges total out of 30135 or 18.95%). A total of 2676 common edges (8.88% of the 30135 total edges) positively correlated with RSFC composite score and a total of 3306 common edges (10.97% of the 30315 total edges) negatively correlated with RSFC composite score.\n\nFigure 2f shows the significant RSFC correlations averaged within and between networks defined by Yeo et al’s seven network. Greater RSFC composite score was associated with increased RSFC within subcortical network (SubC) mainly thalamus (figure 3a, figure S3h), and increased RSFC between DMN and the dorsal attention network (DAN), between DMN and the ventral attention network (VAN), between the frontoparietal network (FPN) and DAN, between FPN and VAN (figure 2d, 2e, 2f, and figure S3c, figure S3d, figure S3f, figure S3g). Greater RSFC composite score was associated with decreased RSFC within the Somatomotor network (SMN) and the VAN (figure 2d, 2e, 2f, 3a, and figure S3b, figure S3d), and between the DAN and VAN, between the DAN and SMN, between the SubC and DMN, between the SubC and FPN (figure 2d, 2e, 2f, 3a, and figure S3c, figure S3c, figure S3b, figure S3h).\n\nFigure 3b further demonstrated the relative importance of the regions in the obtained significant RSFC pattern by showing the top five nodes with highest weighted degree in both the positive and negative networks (Table S3). Specifically, for the positive network, the top five nodes with the greatest number of edges were primarily located in the VAN, i.e., the dorsal insular cortex and precentral gyrus (figure 3b). For the negative network, the top five nodes with the greatest number of edges were primarily located in the Subcortical regions, i.e., the thalamus, and somatomotor cortex (e.g., postcentral gyrus and paracentral lobule) (figure 3b).\n\nCross-dataset replicability and generalizability\n\nThe robustness of the obtained LV1 was further ensured with a large replication sample (N=628) from the BBP (see Online Methods for the details). To do this, we replicated the PLS procedure conducted in the discovery dataset with the replication dataset (see Online Methods for the details). The LV1 accounted for 26.3% variance and still survived after permutation testing with FDR correction (q<0.05) in the replication dataset with significant association (r =0.44, permuted p = 0.004) between RSFC and behavioral composite scores (figure S4). Importantly, the obtained LV1 was largely replicated, evidenced by the high correlation between the behavioral salience scores in the discovery and replication dataset (r= 0.95, p~=0, figure 4a), between the behavioral loading scores in the discovery and replication dataset (r= 0.99, p~=0, figure 4c), between the RSFC salience scores in the discovery and replication dataset (r= 0.71, p~=0, figure 4b), between the RSFC loading scores in the discovery and replication dataset (r~= 0.95, p~=0, figure 4d).\n\nWe further tested the cross-dataset generalizability by projecting the dataset 2 onto the salience parameters learned by PLS in dataset 1. Then, we examined the correlation between the behavioral and RSFC composite score in dataset 2. We found the obtained LV1 from dataset 1 successfully generalized to dataset 2, as evidenced by a significant correlation between the obtained behavioral and RSFC composite score (r=0.25, permuted p<0.001, figure 4e).\n\nSpatial Correlation with Neurotransmitter Densities\n\nFurthermore, we answered question3 (figure 1) by testing whether the sleep-health related connectome (figure2e) was spatially correlated with the distribution of several neurotransmitter systems involved in the domains of sleep health, including serotonin receptors (5-HT1a, 5-HT1b, and 5-HT2a) and transporters (5-HTT), together with metabotropic glutamate receptor 5 (mGluR5) and the γ-Aminobutyric acid type A (GABAA) receptor. First, density values were derived from average group maps of healthy volunteers obtained in prior multitracer molecular imaging studies. These maps were resampled to an isotropic 2-mm spatial resolution as we did in the fMRI data. Then, we obtained the average value for each region of the Brainconnectome atlas for each Neurotransmitter density map. Next, we summed the positive and negative FC loadings (weighted) separately for each region of Brainconnectome atlas to represent the region importance scores in positive (figure 5a) and negative network (figure 5b). Finally, spearman correlation analysis between the region importance score and receptor/transporter densities were conducted. Please refer to the Online Methods and Supplementary Materials for the details. After permutation testing with FDR correction (q<0.05), significant associations were found between on the one hand, the summed positive network and the 5HT1a map (figure 6a), the 5HT2a map (figure 6b), the GABAA map (figure 6c) and the mGluR5 (figure 6d) and on the other hand, the summed negative network and the 5HT1a (figure 6e) map, and the mGluR5 (figure 6f) map. These results suggested the PLS pattern estimated from RSFC may be relevant at the neuromolecular level in line with sleep health.\n\nPredictive utility of the sleep-health related connectome: for sleep quality in healthy population\n\nNext, considering that the most contributing measure in the LV/dimension found in the discovery (r=0.79, figure2c) and replication (r=0.78, figureS4c) BBP samples was the PSQI total score, we further examine the predictive utility of the sleep-health related connectome features for individual PSQI scores in a completely independent dataset. We here used support vector regression (SVR) to predict the sleep quality measured by the PSQI total score (see Figure 7a) in the unrelated individuals of the Human Connectome Project (HCP) dataset (n=435), see Online Methods for the details. It turned out the significant edges of the sleep-health related connectome found in the discovery sample can predict the total score of PSQI in the HCP dataset as evidenced by a significant Pearson correlation between the predicted and original PSQI (r average=0.18, r range = 0.12-0.24 permuted p<0.001) after a 100 repeated 10-fold cross validation (figure 7b,7c). Notably, the predicted PSQI score did not show significant associations with demographic variables and head motion (Table S4), suggesting that the demographic variables and head motion did not significantly affect the prediction. Importantly, we also examined the prediction performance of models using the whole brain connectome. Our results here showed that models using the specific sleep-health related connectome yield slightly higher prediction performance than whole-brain connectome models (after a 100 repeated 10-fold cross validation, r average=0.16, r range = 0.10-0.22, permuted p=0.002 (the blue correlational graph in figure 7c)) hence demonstrating that the identified sleep-health related connectome captures sufficient and relevant information for individual prediction of sleep phenotype in the adult population.\n\nPredictive utility of the sleep-health related connectome: for sleep disorders\n\nFurthermore, we investigated the possibility of distinguishing the insomnia patients from sleep healthy controls based on the sleep-health related connectome. To accomplish this, we utilized a gaussian radial basis function (RBF) kernel support vector machine (SVM) classifier which was implemented using the LIBSVM toolbox on our classification dataset containing 52 insomnia patients and 49 sleep healthy subjects (see Online Methods and table S6 for the sample details). The classifier performance was validated using a 100 repeated 10-fold cross-validation strategy (see Online Methods for details). Classification performance that had an accuracy higher than 70% were considered to be meaningful. It turned out that the sleep-health related connectome also has diagnostic potential to distinguish insomnia patients from sleep healthy subjects with an average accuracy across 100 CV of 79.12% (permuted p < 0.0001) with 76.92% sensitivity, 83.67% specificity and area under the curve (AUC) = 0.80 (figure 8a, green receiver operating characteristic (ROC) curve in figure 8b). Importantly, we tested to which extend the sleep-health related connectome does as well or better than using the whole brain connectome for the classification performance. It turned out the whole brain connectome-based classification performance was lower as indicated an average accuracy across 100 CV of 72.62% (permuted p < 0.0001) with 78.85% sensitivity, 67.35% specificity and AUC = 0.73 (red ROC curve in figure 8b). This result further suggests that the sleep-health related connectome feature sets have specific classification power for sleep health phenotype at the individual level and could therefore be seen as useful biomarkers.\n\n# Discussion\n\nThere is growing interest toward using a conceptual framework that articulates sleep health as multi-facet 2145. Although the importance of RSFC in multi-facets of sleep health is increasingly recognized, the degree to which RSFC is associated with sleep health as a multi-variate dimension remains largely unknown. Leveraging a unique dataset including resting-state fMRI and behavioral assessments spanning multiple domains of sleep health, we found robust correlated patterns of RSFC and sleep health measures that could be represented in one dimension. The derived pattern estimated from RSFC shows neurobiological relevance and predictive utility for sleep phenotype in healthy population. Critically, the RSFC spatial pattern of this dimension additionally shows diagnostic potential to distinguish insomnia patients from sleep healthy subjects. Together these results delineate RSFC-guided dimension of sleep health, which could serve as a foundation to develop a reliable brain connectome biomarker for sleep health with high potential for clinical translation—and ultimately for the diagnosis, prognosis, treatment, and prevention of sleep health-related problems.\n\nIn the present study, the measurement of sleep health composite was guided by both behavior and brain functional connectivity. The obtained dimension of sleep health was associated with a unique cluster of 27 out of the 36 selected SH measures mainly including sleep quality, severity of insomnia, degree of hyperarousal, degree of dysfunctional beliefs and attitudes about sleep, degree of physical fatigue and degree of subjective sleep lack/deprivation etc. (figure 2c). This significant cluster of SH variables were still fallen within the proposed seven domains and largely overlapped with the domains of sleep health examined in previous studies 3617 but draw a multifaceted picture of SH to a bigger extend based on its broader definition 2. The present study thus can be regarded as a step forward in measuring and quantifying sleep health composite by incorporating whole brain resting state functional connectivity 3. To this end, the present study validated the theory that sleep health can be operated and constructed as a composite dimension and that sleep health domains do not exist in isolation 129.\n\nNotably, four out of six measures in the domain of beliefs, attitudes, and habits about sleep 46 were found to be important measurements in the significant latent dimension, with the measure of diminished control and predictability contributing the most. Existing evidence suggests that individuals with more-positive beliefs and attitudes about sleep are more likely to experience better sleep health 3447. On the other hand, previous studies have proposed that the dysfunctional beliefs about sleep (e.g., diminished control and predictability of sleep) can result in the misperception of sleep duration (e.g. underestimate of sleep duration) 48, especially in people who are suffering from insomnia 4923. One possible explanation is that dysfunctional beliefs may alter the constructive process involved in remembering the amount of sleep obtained, thereby contributing to misperception 49. Also recent theories claimed that people tend to gather evidence that confirms our beliefs rather than evidence that challenges them 50, so it is crucial to disprove the dysfunctional beliefs to improve sleep health. In correspondence, Cognitive Behavioral Therapy for Insomnia (CBT-I) emphasized the importance of cognitive restructuring and sleep hygiene to alter the dysfunctional beliefs, attitudes, and habits about sleep as its two main components 51. Taken together, future studies investigating sleep health should pay more attention to the domain of beliefs, attitudes, and habits about sleep.\n\nThe latent dimension of sleep health was associated with a unique spatial pattern of resting state functional connectivity, namely a positive and negative network pattern. For the positive network pattern, poorer sleep health was associated with hyper-connectivity between the network involved in internally oriented attention (DMN) and the network responsible for modulation of the goal-directed attention (DAN), between DMN and the network involved in processing of salience (VAN), between the network involved in external goal-directed regulation (FPN) and DAN, between FPN and VAN as well as hyper-connectivity within the subcortical network (SubC) mainly the thalamus. The heightened coupling between the higher-order and attentional networks may suggest a decreasing dedifferentiation of the high-order system to the middle attentional system 1952 while the increased FC mainly within the thalamus (a brain system responsible for gating information) further indicates sustained ascending arousal input from the thalamus 16 in poor sleep health individual phenotype. Notably, the positive network consisted of highest-degree nodes in the left dorsal insular cortex and precentral gyrus. As key hubs of the salience network, these brain regions plays a crucial role in cognitive and emotional processes 2353. Impaired connectivity patterns between these areas and other regions could underlie cognitive, vigilance, and perception dysfunctions, as well as subjective distress and sleep complaints 54.\n\nFor the negative network pattern, poorer sleep health was also associated with hypo-connectivity between the two attentional networks, between DMN and SubC mainly the thalamus, between FPN and SubC mainly the thalamus, between DAN and the network involved in sensory and motor perception (SMN), as well as hypo-connectivity within the VAN and SMN. The reduced coupling between and within the attentional networks and the SMN may mainly suggest the collapse of top-down orienting of attention, bottom-up salience processing 5556 and sensory and motor perception 22 while the reduced connectivity between the high-order networks and thalamus further reflects the reduction in the upward transmission of information to the higher-order networks by the thalamus as a relay station 57 in the condition of poor sleep health. Moreover, the negative network consisted of highest-degree nodes in the thalamus and somatomotor cortex. Both the thalamus 57 and the somatomotor cortex 22 play a crucial role in the sleep physiology. Impaired connectivity patterns between these areas and other regions could suggest the dysfunction of relaying sensory and motor signals to the cerebral cortex, and regulating sleep, alertness and consciousness.\n\nBoth the positive and negative network pattern were spatially correlated with the distribution of several neurotransmitter systems involved in sleep health, including the serotonin receptors, the glutamate receptor (mGluR5) and the GABAA receptor. Previous studies have proven that: 1) serotonin functions predominantly to promote wakefulness and to inhibit REM (rapid eye movement) sleep (REMS) 40; 2) γ-aminobutyric acid (GABA) is increasingly recognized as an important inhibitory neurotransmitter for the initiation and maintenance of sleep 5839; 3) glutamate is the primary excitatory neurotransmitter in the central nervous system, its altered levels were found in people who suffered from insomnia disorders 592360. Taken together, the linked distribution of these neurotransmitter systems and the RSFC spatial pattern found in the present study further suggest that the derived pattern estimated from RSFC is neurobiologically relevant with regards to neuromolecular systems engaged in sleep health.\n\nCritically, the RSFC spatial pattern of this dimension also has diagnostic potential to distinguish insomnia patients from sleep healthy subjects with an accuracy of 79.12%. These results demonstrated that the obtained brain connectome pattern also contained pathophysiological relevance for insomnia disorder. Insomnia is a common, distressing, and clinically complex symptom, which causes difficulty initiating sleep; frequent awakening; or early-morning awakening with daytime dysfunction 5923. Based on the RSFC spatial pattern-based support vector machine (SVM) classifier derived from the obtained sleep health dimension, we will be able to aid in the diagnosis of insomnia disorder. To this end, these findings may suggest that insomnia is a condition with a multifaceted pathophysiology spanning over deficits in multiple domains of sleep health. Ultimately, the present study can serve as a foundation to identify targets that may enable sleep-based interventions for improving both brain health and clinical outcomes.\n\nThe strength of the present study includes the utilization of a large sample, advanced multivariate methods, and replication of results in an independent sample. The component we identified with RSFC not only show macromolecular relevance, but also had diagnostic potential, generalized well to unrelated individuals in the HCP dataset and were robust across alternative methodological strategies. Nonetheless, our work has several limitations. First, here we sought to delineate linked dimensions of sleep health and intrinsic brain functional connectivity, uncovering dimension of sleep health that are guided by and linked to underlying brain connectome properties. Although we included the largest sleep health domains in the neuroimaging studies of sleep heath, to the best of our knowledge, this approach necessarily is limited by the available variables measuring sleep health in the BBP, which did not represent the full domains of sleep health. Future studies can incorporate more sleep-related variables (i.e., sleep regularity) to depict the sleep health dimension. Second, our current analysis only considered functional connectivity and behavioral measures of sleep health. Future research could incorporate rich multi-modal imaging data, objective sleep measurements with actigraphy and polysomnography, biochemics and genomics. Third, the sample mainly consisted in young adults in pattern recognition and middle-aged adults in the prediction and classification test, leaving the RSFC guided sleep health dimension in other age groups such as children, adolescents, and elderly unknown. Recently, the definition on what constitutes good sleep health was adapted to pediatrics 61 as well as the elderly 62. Hence, it is of great importance for future studies to also examine the RSFC-informed sleep health dimension in both younger and older populations.\n\nIn summary, in this study we discovered and replicated multivariate patterns of intrinsic functional connectivity that are highly correlated with dimension of sleep health in a large sample of young adults. This dimension was composed of a unique cluster of sleep health and unique features of resting state functional connectivity, namely a positive and negative network pattern. Both the positive and negative network pattern were spatially correlated with the distribution of several neurotransmitter systems involved in sleep health. Moreover, the obtained positive and negative network pattern also contained pathophysiological relevance for insomnia disorder. These results thus delineate connectivity-guided dimension of sleep health, which could serve as a foundation for developing brain connectome-based biomarkers in sleep symptomatology.\n\n# Online Methods\n\n## Participants\n\n**Discovery and replication datasets (dataset 1 and 2):** The main dataset comprises individuals from the Behavioral Brain Research Project of Chinese Personality (BBP), which was launched in September 2019 (still in progress) to recruit participants from that year’s freshmen at Southwest University, Chongqing, China. In total, 1369 participants completed the cross-sectional neuroimaging protocol as well as the behavioral measures of sleep health. To create two independent samples for discovery and replication analyses, we split the participants according to their data collection periods (September–December 2019 [discovery dataset]; September–December 2020 [replication dataset]). Specifically, a discovery dataset (n = 712) and a replication dataset (n = 657) were created. Of the discovery dataset, 25 participants were excluded due to excessive head motion during scanning (e.g., with a mean framewise displacement [FD] larger than 0.3 mm), resulting in a final sample of 687 participants (mean age 18.96, SD= 0.95; 233 males and 454 females). Applying the same exclusion criteria to the replication dataset produced 628 participants (mean age 19.16, SD= 1.03; 208 males and 420 females). See Table 1 for detailed demographics of each dataset. The two datasets were confirmed to also have similar basic demographic variables, i.e., age, sex, and race (Table 1), as well as head motion (Table 1). Full informed consent from each participant was obtained by BBP Consortium, and research procedures and ethical guidelines were followed in compliance with Southwest University (SWU) institutional review board approval.\n\n**HCP external validation dataset (dataset 3):** The dataset 3 was selected from the 1200 Subjects Release of the Human Connectome Project (HCP). This dataset provides high-quality behavioral/demographic and imaging data from healthy young adults (https://www.humanconnectome.org/) 64. From the original HCP dataset, we first included a group of participants (n = 1084) for which L-R resting-state fMRI data as well as PSQI scores were available. From this group, we further excluded data from 46 participants based on the exclusion criteria indicated as follows: (1) participants with missing values on demographic variables such as age, sex, education, BMI, and race or family information; (2) participants with a history of hyper/hypothyroidism or history of other endocrine problems; (3) women who had recently given birth; and (4) participants having a mean FD more than 0.3 mm. Importantly, to exclude the influence of shared genetic and environmental factors, we randomly kept one subject from each family 65, resulting in 435 final unrelated subjects. See Table S5 for detailed demographics of each sample. Full informed consent from each participant was obtained by the Washington University–University of Minnesota (WU–Minn) HCP Consortium, and research procedures and ethical guidelines were followed in compliance with WU institutional review board approval.\n\n**Classification dataset (dataset 4):** The classification dataset involved 109 participants, including 56 patients with insomnia disorder (ID) and 53 healthy controls (HC). Part of the dataset was collected from the Sleep Center, Department of Brain Disease of Chongqing Traditional Chinese Medicine Hospital (CTCMH), which included 25 ID and 36 HC participants (referred as CTCMH dataset) and the remaining part of the dataset is from the Sleep and Neuroimaging Center, Southwest University (referred as SNIC dataset). All the participants received the MRI scanning at the brain imaging center of Southwest University. Patients with insomnia disorder were diagnosed by experienced hospital psychiatrists (D.G. and CY.L.) according to the International Classification of Sleep Disorders: Diagnostic and Coding Manual, 3rd ed. and insomnia symptoms has lasted at least three nights a week for more than 3 months. All the health controls met the following criteria: a good sleep habit and a good sleep onset and/or maintenance; a regular dietary habit; no consumption of any stimulants, medications, alcohol, and cocaine for at least 3 months before the study; no history of neurological or psychological disorders; lower scores of Pittsburg Sleep Quality Index (PSQI) than 7 66. Participants with any findings of pathological brain MRI as well as ineligibility for MRI scanning (any type of metal implant) were excluded in the study. Eight participants were excluded due to excessive head motion during the scanning (e.g., with a mean FD larger than 0.3 mm), resulting in a final sample of 52 ID patients (mean age= 44.00 years old, SD= 12.39) and 49 HC (mean age=42.10 years old, SD= 15.93). The research projects were approved by the local institutional review boards, and written informed consent was obtained from each participant in accordance with the Declaration of Helsinki. The two groups were matched for age, sex, and head motion (Table S6). The participants’ demographic characteristics are summarized in Table S6.\n\n**Sleep health-related assessments in the discovery and replication dataset**\n\nA large set of sleep health measures (Table S1) were included in the current study based on the consideration to select available variables in the Behavioral Brain Research Project of Chinese Personality (BBP) that 1) represent central domains of SH descried in the Ru SATED 3 as well as in the National Sleep Foundation (NSF)’s Sleep Health Index 6; 2) provide high consistency with previous SH studies 7115; 3) draw a multifaceted picture of SH to a bigger extend based on its broader definition by including variables that are sleep deficiency related, nighttime- and daytime-related, quantitative and qualitative informed. On that basis, the chosen 36 variables were grouped into seven domains: (1) **Satisfaction with sleep/ Sleep quality** (e.g., PSQI total score, Not get enough sleep, Feelings from wake-up, Necessity of nap, Needed nap time, Subjective sleep quality); (2) **Alertness during waking hours** (e.g., Epworth sleepiness scale, Mind-wandering, Spontaneous mind wandering, Deliberate mind wandering, Frequency of daydream, Fatigue severity, Physical fatigue, Mental fatigue, Attention-related cognitive errors, Valid sleep cue reaction time(RT), Invalid sleep cue RT, Valid sleep cue accuracy (ACC), Invalid sleep cue ACC); (3) **Timing of sleep** (e.g., Morningness-eveningness questionnaire); (4) **Sleep efficiency/ continuity** (e.g., Sleep efficiency, Sleep latency, Wake-up times); (5) **Sleep duration** (e.g., Total sleep time); (6) **Sleep deficiency** (e.g., Insomnia severity index, Hyperarousal, Ford insomnia response to stress test, Sleep disturbances, Use of sleep medications, Daytime dysfunction); (7) **Sleep beliefs, attitudes, and habits** (e.g., Dysfunctional beliefs and attitudes about sleep scale (DBAS)-total score, Misconceptions about causes, Diminished control and predictability, Unrealistic sleep expectations, Misattribution of the consequences, Faulty beliefs about sleep promoting practices). For the specific descriptions about the chosen variables, see Supplementary table S1.\n\n## Data acquisition and image preprocessing\n\n### The discovery and replication sample\n\n#### Data acquisition\n\nAll MR Images were acquired using a 3T Siemens Primsa-fit scanner with a standard 32 channel head coil located at Southwest University. High-resolution T1-weighted structural image was obtained using a three-dimensional gradient sequence in order to facilitate alignment of individual subject images into a common space (repetition time (TR) = 2530 ms, time of echo (TE) = 2.98 ms, field of view (FOV) = 256 × 256 mm 2, thickness = 1 mm, voxel size = 0.5 × 0.5 × 1 mm 3, flip angle = 7°, resolution matrix = 256 × 256, slices = 192, slice oversampling = 33.3%, phase encoding direction = AC » PC). Approximately 8 minutes of rs-fMRI data containing 240 volumes were acquired for each subject using a blood oxygen level-dependent (BOLD-weighted) sequence (TR = 2000 ms; TE = 30 ms; slices = 62; slice thickness = 2 mm; FOV = 224 × 224 mm 2; flip angle = 90°; resolution matrix = 112 × 112; voxel size=2× 2 ×2 mm 3; phase encoding direction = PC » AC). In order to minimize motion, prior to data acquisition participants’ heads were stabilized in the head coil using one foam pad over each ear and a third over the top of the head. During the resting-state scanning, a fixation cross was displayed as images were acquired. Participants were instructed to stay awake, keep their eyes open, fixate on the displayed crosshair, and remain still.\n\n#### Image preprocessing\n\nThe preprocessing steps on all collected neuroimaging data were performed using the publicly available CONN functional connectivity toolbox (version 20.b; https://www.nitrc.org/projects/conn), together with SPM12 (Wellcome Department of Cognitive Neurology, London, UK; http://www.fil.ion.ucl.ac.uk/spm). Functional images were (1) slice time corrected, (2) underwent motion correction and susceptibility artifact correction based on field map, (3) warped into Montreal Neurological Institute(MNI) standard space using the diffeomorphic Anatomical Registration Through exponentiated Lie Algebra (Dartel) approach to realign the 3D anatomical data into Montreal Neurological Institute space 67, (4) smoothed spatially with a Gaussian kernel of 6 mm full width at half maximum (FWHM). Next, functional images further underwent denoising steps using the anatomical component-based correction (aCompCor) method 68. Specifically, noise signals, including signals from cerebrospinal fluid and white matter (WM) (five principal components), and movement parameters (six motion parameters, six temporal derivatives, and their squares) and linear trend were removed from the images as confounds 69. Subsequently, data scrubbing was implemented to address head motion concerns. The bad time points were regarded as regressors defined as volumes with FD power > 0.5 mm as well as the two succeeding volumes and one preceding volume to reduce the spillover effect of head motion 69. Finally, functional images were filtered using a bandpass filter (0.008– 0.09 Hz) to reduce the effects of very-low-frequency drifts and high-frequency noises.\n\n### HCP sample\n\n#### Data acquisition\n\nStructural (T1 and T2 images, required for preprocessing functional neuroimaging data) and functional MRI data were collected at Washington University on the Siemens 3T Connectome Skyra scanner using a multi-band sequence. The structural images were 0.7 mm isotropic. The rs-fMRI data were 2 mm isotropic with TR = 0.72s. Full details of the acquisition parameters for the HCP data can be found elsewhere 70. Two sessions of rs-fMRI data were collected in consecutive days for each subject, and each session consisted of one or two runs. The length of each rs-fMRI scan was 14.4 min (1200 frames). Here, the analyses were restricted to individuals for whom the left–right phase-encoding scans for the rs-fMRI session was completed and available. For rs-fMRI data acquisition, participants were asked to lie with eyes open, with “relaxed” fixation on a white cross (on a dark background), think of nothing in particular, and not to fall asleep. Details of the data collection can be found elsewhere 71. Details about behavioral measures including PSQI can be found in HCP S1200 Data Dictionary(https://db.humanconnectome.org/data/projects/HCP_1200) and 72.\n\n#### Image preprocessing\n\nWe adopted the pre-processed data provided by the Human Connectome Project (HCP S1200 release), for which also the spatial normalization to the MNI152 template had already been performed before download. Details of the structural and functional data preprocessing can be found in the HCP S1200 manual 73, and we used version 3.21 of the HCP preprocessing pipeline. Consistent with BBP dataset, the HCP downloaded functional images were further smoothed, underwent regression of motion and non-relevant signals, including linear trend, Friston 24 head motion parameters, white matter (CompCor, 5 principal components), and CSF signal (CompCor, 5 principal components), scrubbed and filtered.\n\n### Classification sample:\n\n#### Data acquisition\n\nAll MR Images in the SNIC dataset were acquired using a 3T scanner (Magnetom TIM- Trio, Siemens, Erlangen, Germany) with a standard head coil located at Southwest University. In order to minimize motion, prior to data acquisition participants’ heads were stabilized in the head coil using one foam pad over each ear and a third over the top of the head. High- resolution T1- weighted anatomical images were collected using 3D spoiled gradient recalled (3DSPGR) sequence (TR/TE = 8.5/3.4 ms, flip angle = 12°, resolution matrix = 512 × 512, FOV = 240 × 240 mm 2, with a voxel size of 1 ×1 ×1 mm 3, 176 slices, 1 mm thickness). Approximately 5 minutes of rs-fMRI data containing 204 volumes were acquired for each subject using an echo-planar imaging (EPI) sequence (TR/TE = 1500/29 ms, flip angle = 90°, resolution matrix = 64 × 64, voxel size = 3 ×3 ×3 mm 3, FOV = 192 × 192 mm 2, axial slices = 25, thickness/ gap = 5/0.5 mm). The first four volumes were discarded to ensure steady- state longitudinal magnetization. During the resting-state scanning ,participants were instructed to fix on a crosshair in the center of black background screen without thinking intentionally in the mind and keep as motionless as possible 74.\n\nAll MR Images in the CTCMH dataset were acquired by using the same scanner as the discovery and replication dataset. The scanning parameters are also the same. During the resting-state scanning, all participants were instructed to fix on a crosshair in the center of black background screen without thinking intentionally in the mind and keep as motionless as possible.\n\n#### Image preprocessing\n\nThe preprocessing steps on all collected neuroimaging data in the classification sample were performed using fMRIPrep 21.0.1 7576 (RRID:SCR_016216), which is based on Nipype 1.6.1 77 (RRID:SCR_002502). Details of the structural and functional data preprocessing can be found in the supplementary materials.\n\n## Resting-State Functional Connectivity Construction\n\nTo construct RSFC, the preprocessed data in the discovery and replication dataset were first parcellated using the Brainnetome Atlas 41, which includes 210 cortical regions and 36 subcortical regions. For each participant, the BOLD time course of each node was extracted by taking the mean across voxels. Pearson correlation coefficient (r) between the time courses of each pair of nodes was calculated. A Fisher’s r-to-z transformation was performed to improve the normality of the correlation coefficients, which resulted in a 246×246 symmetric functional connectivity matrix with 30,135 [(245 × 246)/2] edges for each participant.\n\n## Partial least squares analysis\n\nWe used PLS analysis to examine the relationship between resting-state functional connectivity (RSFC) and sleep health (SH) measures (figure 1) in the discovery dataset. PLS analysis is a multivariate statistical technique that derives latent variables (LVs), by finding weighted patterns of variables from two given data sets that maximally covary with each other 7879. In the present analysis, 1 variable set corresponded to RSFC and the other to behavioral measures spanning multiple domains of sleep health. The 2 variable sets were correlated with each other across participants, and the resulting covariance matrix was subjected to singular value decomposition to identify the latent brain-behavior dimensions. Specifically, each LV is comprised of a RSFC pattern at node level (“RSFC saliences”) and an SH profile (“SH saliences”). Individual-specific RSFC and SH composite scores for each LV were obtained by linearly projecting the RSFC and SH measures of each participant onto their respective saliences. See supplementary methods section “Partial least squares analysis” for mathematical details. Before the PLS analysis, we regressed out the confounding effects from both RSFC and behavior data including mean FD, age, handedness, and sex.\n\nInference and validation of the statistical model were performed using nonparametric methods including: (1) statistical significance of overall patterns was assessed by permutation tests using 1000 permutations for behavioral data; (2) the importance (measured as loading scores) of feature (RSFC, sleep health measures) was evaluated by bootstrap resampling; (3) the generalizability of each LV was assessed by 10-fold cross-validation with 200 repetitions. Mathematical details of the analysis and inferential methods are described in supplementary methods section “Partial least squares analysis” and results. False discovery rate (FDR) correction (q < 0.05) was applied to all analyses.\n\n## Control and Reliability Analyses\n\nWe further tested whether LVs obtained in the discovery dataset were robust to 1) global signal regression, 2) total intracranial volume (including gray matter, white matter, and cerebrospinal fluid) regression, 3) the pre-scanning positive and negative affect regression, 4) BMI regression, 5) family income regression, 6) adding confounding variables (age, sex, handedness and head motion) into the phenotypic data for the PLS analysis, 7) non-Gaussian distributions of the behavioral data with quantile normalization, as well as 8) using a different brain (Seitzman et al.’s) Atlas 42 containing 300 regions for the RSFC construction. To assess the robustness of each LV, we computed Pearson’s correlations between RSFC (or SH) saliences obtained in each of the eight-control analysis and RSFC (or SH) saliences from the original PLS analysis. Please refer to table S2 for the results.\n\n## Internal validation\n\nAs an internal validation of the obtained LVs or dimensions in the discovery dataset, we first replicated the PLS analysis described in section “Partial least squares analysis”, and “Control and Reliability Analyses” with the replication dataset. Then, Pearson’s correlation coefficient between the behavioral salience scores in the discovery and replication dataset, between the behavioral loading scores in the discovery and replication dataset, between the RSFC salience scores in the discovery and replication dataset, between the RSFC loading scores in the discovery and replication dataset were computed respectively.\n\nWe further tested the cross-dataset generalizability by projecting the dataset 2 onto the salience parameters learned by the PLS analysis in dataset 1. Then, we examined the correlation between the behavioral and RSFC composite score in dataset 2. The significance of the correlation value was further assessed by a permutation test (behavioral data of dataset 2 shuffled 1000 times).\n\n## External prediction validation\n\nConsidering that the PSQI total score contributes the most in the LV/dimension found in the discovery BBP sample (r=0.79), we further tested whether the RSFC spatial pattern of this dimension observed in the discovery dataset can predict the sleep quality of unrelated individuals in the HCP dataset as an external prediction validation (figure 1). In particular, we adopted the support vector regression (SVR), the most widely used algorithm in multivariate neuroimaging research, to examine the predictive performance of the significant RSFC pattern in the LV found in the discovery sample on sleep quality in the HCP dataset. Specifically, we used all the edges of the significant RSFC pattern as the features. The 10-fold cross-validation was used to determine the optimal parameter C for SVR. Specifically, the optimal parameter was finally selected according to the prediction performance after the inner 10-fold cross-validation was performed for each parameter ([0.1,1] with a step of 0.1) in turn and was further utilized in the outer loop to accomplish the final prediction. All subjects were divided into 10 subsets by 10-fold cross-validation (outer loop). Nine of them were used as training set and model fitting was performed. The fitted model parameters and the remaining one subset were used as the test set to generate predicted values. This process was repeated 10 times to generate predicted values for all subjects. In order to obtain stable predictive performance, we repeated the above prediction pipeline 100 times to generate 100 predicted scores for each participant and further averaged these predicted scores to obtain robust estimates. Pearson’s correlation coefficient between the predicted average and actual values was computed to provide final estimates of predictive performance. The significance was evaluated by randomly shuffling the PSQI values 1000 times and running the above prediction pipeline for each time to obtain a null distribution of correlation coefficients between the predicted and actual values.\n\n## Spatial Correlation with Neurotransmitter Densities\n\nWe further test whether the FC loadings from the PLS analysis were spatially correlated with the distribution of several neurotransmitter systems potentially involved in domains of sleep health. Based on the literature 4058605980, serotonin receptors (5-HT1A, 5-HT1B, and 5-HT2A) and transporters (serotonin reuptake transporter [5-HTT]), together with metabotropic glutamate receptor 5 (mGluR5) and the γ-Aminobutyric acid type A (GABAA) receptor were investigated. Density values were derived from average group maps of healthy volunteers (5-HT1a: n = 35; 5-HT1b: n = 36; 5-HT2a: n = 29; 5-HTT: n = 100; mGluR5: n = 22; GABAA: n = 11) obtained in prior multitracer molecular imaging studies 30 (details were provided in the Table S7). These maps were resampled to an isotropic 2-mm spatial resolution as we did in the fMRI data. Then, we obtained the average value of each region of Brainconnectome atlas for each Neurotransmitter density map, i.e., a 246x1 matrix. Further, we summed the positive and negative FC loadings separately for each region of Brainconnectome atlas to represent the region importance scores in positive (figure6a) and negative network (figure6b). Finally, we conducted a Spearman correlation analysis between the region importance score and receptor/transporter densities calculated for these regions 43. To establish the statistical significance of a spatial correlation against chance, we conducted spatial permutation tests to obtain a null distribution of correlation coefficients for region importance scores and neurotransmitter densities extracted from 5000 permutations while accounting for the spatial autocorrelation of brain regions 8182. The p-value was determined by empirically observed spatial similarity values compared to the null distribution. Significance level was set at FDR corrected p<0.05.\n\n## Clinical diagnosis validation\n\nWe further evaluated the possibility of distinguishing the insomnia patients (n=52) from sleep healthy controls (n=49) based on the RSFC spatial pattern of the found LV/dimension (details about the classification sample were given in the section of participants). Specifically, we used all the edges of the significant RSFC pattern as the features. To accomplish this, we utilized a gaussian radial basis function (RBF) kernel SVM classifier which was implemented using the LIBSVM toolbox 44. The classifier performance was validated using a 10-fold cross-validation strategy. Specifically, all subjects were divided into 10 subsets by 10-fold cross-validation. Nine of them were used as training set and model fitting was performed. The fitted model parameters and the remaining one subset were used as the test set to generate classified labels. This process was repeated 10 times in sequence to generate classified labels for all subjects, and then calculating the classification accuracy. Regarding the optimal values for the RBF kernel parameters C and γ, they were tuned based on the training set using grid search strategy based on a 10-fold cross-validation (inner loop). Then the SVM classifier was trained by applying the optimized parameters to the training set, based on which the testing set was finally classified. In order to obtain stable classification performance, we repeated the above pipeline 100 times to generate 100 classification performance value and further averaged these values to obtain robust estimates.\n\nStatistical significance was evaluated by using 1,000 permutation tests with a threshold of p<0.05. In Brief, labels of participants were randomly shuffled for 1,000 times and split into the training and testing sets. Classification performance that had an accuracy of higher than 70% were considered to be meaningful.\n\n## Data and code availability\n\nThe BBP and classification sample were available upon reasonable request. HCP consortium database was freely available at https://db.humanconnectome.org/. The significant FC weights from the discovery cohort are provided at GitHub (https://github.com/wangyulinatUGent/Sleep_Health_Dimension). PET/SPECT data from the prior vivo molecular imaging studies 30 were openly accessed at (https://github.com/netneurolab/hansen_receptors/tree/main). We used the Matlab code from https://github.com/danizoeller/myPLS 83, based on Krishnan and associates’ work 32 to implement the PLS calculation. The code for spatial permutation testing can be found at https://github.com/frantisekvasa/rotate_parcellation. The codes for SVR and SVM analysis are openly available at https://www.csie.ntu.edu.tw/~cjlin/libsvm/ 44. The brain maps were presented using MRIcroGL toolbox (https://www.nitrc.org/projects/mricrogl). The connectome maps were presented using code from (https://github.com/cocoanlab/cocoanCORE/tree/master/Visualization) 84.\n\n# References\n\n1. Chung, J., Goodman, M., Huang, T., Bertisch, S. & Redline, S. Multidimensional sleep health in a diverse, aging adult cohort: Concepts, advances, and implications for research and intervention. *Sleep Heal.* **7**, 699–707 (2021).\n\n2. 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Demographic characteristics of participants in the discovery and replication dataset\n\n| | Discovery dataset (N=678) | Replication dataset (N=628) |\n|--- | --- | ---|\n| Age, mean (SD), years | 18.96(0.95) | 19.16(1.03) |\n| Female | 454(66.08) | 420(66.88) |\n| Handedness-Right | 606(88.21) | 575(91.56) |\n| BMI, mean (SD) | 21.23(2.87) | 21.85(3.19) |\n| Race | | |\n| Han | 569(82.82) | 527(83.92) |\n| Other | 118(17.18) | 101(16.08) |\n| Framewise displacement (FD), mean (SD) | 0.10(0.05) | 0.10(0.05) |\n| Total brain volume, mean (SD), mm³ | 1541331.47(138185.45) | 1539323.87(158514.00) |\n| Family income per year (yuan, RMB) | | |\n| < 5000 | 125(18.20%) | 93(14.81%) |\n| 5001~25000 | 277(40.32%) | 262(41.72%) |\n| 25001~45000 | 108(15.72%) | 96(15.29%) |\n| 45001~65000 | 55(8.01%) | 66(10.51%) |\n| 65001~85000 | 39(5.68%) | 36(5.73%) |\n| 85001~105000 | 45(6.55%) | 31(4.94%) |\n| >105000 | 38(5.53%) | 44(7.01%) |\n| PANAS-P, mean (SD) | 28.96(6.12) | 29.45(6.20) |\n| PANAS-N, mean (SD) | 17.66(5.97) | 17.39(6.00) |\n\n**Note.** PANAS, Positive and Negative Affect Schedule. SD, standard deviation.\n\n# Supplementary Files\n\n- [Supplementarymaterialsfinalized12172022.docx](https://assets-eu.researchsquare.com/files/rs-2391772/v1/1afb3f4cecee0a5c75724955.docx) \n Supplementary file of the main manuscript\n\n- [NCOMMS2302175TrS.pdf](https://assets-eu.researchsquare.com/files/rs-2391772/v1/0576b29bf36c7ec417574ca0.pdf) \n Reporting Summary"} {"paper_id": "prb14", "title": "Chronic intracranial recordings in the basal ganglia reveal patient-specific circadian rhythms in Parkinson's disease", "text": "# Abstract\n\nAdaptive deep brain stimulation (aDBS) is a promising therapeutic approach for subjects with Parkinson’s disease (PD) using neural signals as feedback control to adjust the level of therapy. However, the circadian fluctuation of neural signals may alter these control signals and possibly result in suboptimal therapy. We report a large retrospective cohort including 119 subjects with PD (165 hemispheres) with globus pallidus internus (GPi) and subthalamic nucleus (STN) activity recorded chronically in the home environment. Both GPi and STN activity was significantly altered by circadian rhythms. The direction of the circadian rhythm (increase versus decrease at night) depended on the frequency band in both the GPi and STN. The use of long-acting extended released dopaminergic medications significantly impacted the circadian rhythms in the GPi target. These findings demonstrate the variability of chronic circadian rhythms and suggest that aDBS will likely need to account for these patient-specific fluctuations to ensure successful implementation in real-world environments.\n\nHealth sciences/Neurology/Neurological disorders/Parkinson's disease \nBiological sciences/Neuroscience/Circadian rhythms and sleep/Circadian regulation \nBiological sciences/Neuroscience/Circadian rhythms and sleep/Sleep \nParkinson’s disease \ndeep brain stimulation \nlocal field potential \ncircadian rhythm \nglobus pallidus\n\n# Introduction\n\nParkinson’s disease (PD) is a neurodegenerative movement disorder characterized by the loss of dopaminergic neurons that leads to the development of motor and nonmotor symptoms. Deep brain stimulation (DBS) is an established therapy to treat motor symptoms in selected subjects with medication-refractory PD1,2. This invasive neurosurgical procedure consists in delivering electrical stimulation to the deep brain nuclei through electrodes implanted in the basal ganglia nuclei. In PD, DBS is commonly targeted to either the globus pallidus internus (GPi) or the subthalamic nucleus (STN), two key nodes in the basal ganglia-thalamo-cortical networks underlying PD pathophysiology3.\n\nCurrently, DBS therapy for PD delivers stimulation continuously to disrupt pathological neural activity. However, recent research has increasingly focused on the development of adaptive DBS (aDBS) algorithms, which use neural signals as feedback control to increase or to decrease stimulation based on the presence of pathological activity4. The development of aDBS has been recently facilitated by advancements in DBS devices to support bidirectional sensing-stimulation devices, enabling simultaneous stimulation and recording of local field potential (LFP), both in the clinic and the home environment. LFP activity in the beta frequency band (13–30 Hz) has been most commonly used as the aDBS feedback control signal5,6. Use of this signal has been largely based on established evidence that beta activity in both the GPi and STN correlate with PD rigidity and bradykinesia7–10. Experimental use of aDBS has been shown to improve symptoms with less stimulation-induced side effects and has been shown to improve battery life5,6,11,12. Narrow band gamma activity (70–90 Hz) has been suggested as a marker of the ‘on medication PD state’ and the hyperkinetic state of dyskinesia13, and has also been successfully used as feedback signals for aDBS. Chronic use of such algorithms over weeks, in patients’ home environment, has been shown to potentially improve on-time state and quality of life in most subjects studied14. Therefore, aDBS is an approach to improve the efficacy and efficiency of DBS for PD.\n\nAlthough encouraging, implementation of aDBS has been found to be more challenging than expected. One factor that has added complexity to stimulation parameterization is the presence of natural fluctuation of biomarkers due to sleep/wake cycles. Indeed, chronic brain recordings have shed light on rhythmic activity, more specifically circadian rhythms, that could potentially alter the target of aDBS algorithms15. Circadian rhythms are endogenous fluctuations that orchestrate a wide range of complex physiological and behavioral processes across the ~24-hour sleep/wake cycle16. Dopamine contributes to sleep/wake cycle regulation17–19 via pathways from the hypothalamus to the mesolimbic pathways20–23. Circadian rhythms disturbances have been observed in PD, resulting in a broad range of symptoms, including as sleep-wake disorders, autonomic dysregulation, temperature imbalance, and motor fluctuations24.\n\nRecent studies have revealed that the neural activity in the GPi and STN in subjects with PD exhibited circadian patterns15 and these fluctuated during different stages of sleep25–33. A recent study evaluating chronic STN LFP recordings in the home environment has revealed beta power circadian fluctuations, with a consistent reduction of beta power during sleep25. This result supported prior findings from acute STN recordings, performed in-clinic using externalized electrodes over 1 night, and showing that, on average, beta (13–30 Hz) and gamma (30–60 Hz) power in the STN decreased, while delta (0–3 Hz), theta (3–7 Hz), and alpha (7–13 Hz) power increased during non-rapid-eye-movement (NREM) sleep when compared to wakefulness and rapid-eye-movement (REM) sleep. While studies investigating circadian rhythm via subcortical electrophysiological signals have largely focused on STN, two recent studies by Yin et al have focused on GPi recordings in PD. When compared to Huntington’s disease and dystonia Yin et al found that, similar to STN, pallidal beta and gamma activity was reduced in NREM compared to REM sleep and awake state, while delta, theta, and alpha power were increased during NREM sleep29,30. However, overall, most studies have been conducted in small cohorts, and have focused on STN activity, recorded in the off-medication state, through externalized electrodes, and performed in controlled environments. Therefore, how circadian rhythm could modulate basal ganglia activity, in particular in GPi, and in patient’s naturalistic environment remains largely unknown.\n\nThe objective of this study was to characterize circadian patterns of neural activity recorded in the GPi and STN in a large cohort of subjects with PD using longitudinal, at-home recordings via a chronically implanted neurostimulator. An increased understanding of neurophysiologic biomarkers of symptoms and their association with circadian patterns is required to develop future aDBS paradigms that may enhance the treatment of PD symptoms.\n\n# Results\n\nIn this retrospective study, 119 patients (165 unique hemispheres) were recruited from an IRB approved movement disorders database (UF INFORM). Subjects selected were diagnosed with PD and implanted with the Medtronic Percept PC neurostimulators attached to unilateral or bilateral DBS leads in either the GPi (96 subjects, 135 hemispheres) or the STN (23 patients, 30 hemispheres). A total of 88 males and 29 females were included in this study, with an average age at surgery of 67.8 ± 9.0 (mean ± std) years and an average disease duration of 13.8 ± 6.5 (mean ± std) years. Table 1 summarizes the subjects characteristics for the cohort.\n\nIn each subject, neural activity was recorded chronically in participants’ home environment while under both therapeutic chronic medication and stimulation conditions. Therefore, for each subject and each hemisphere, we selected the first chronic neural recording, following DBS implantation, lasting at least 5-consecutive-day worth of data and out stimulation settings through the recordings. The average recording duration was 17.8 ± 19.7 (mean ± std) consecutive days commencing at 13 ± 35 days after pulse generator device implantation, which happens 4 weeks after DBS lead implantation at our center. The bipolar contact pair used for sensing was determined by the contact(s) used for continuous stimulation therapy. The frequency of oscillatory activity sensed chronically was selected for each subject by the clinician during DBS programming sessions. The clinicians typically selected the most prominent peak on the power spectral density generated after a short survey recording. The neural frequency tracked ranged from 5.86 Hz to 67.38 Hz across this cohort. For analysis, frequencies were grouped in bands defined as theta/alpha ( ≤ 12 Hz), low-beta (> 12 and ≤ 20 Hz), high-beta (> 20 and ≤ 30 Hz), and gamma ( ≥ 31 Hz). In GPi subjects, the theta/alpha band and low-beta band were most commonly reordered (46.7% and 37.0% respectively), while in STN the low-beta band was most commonly recorded (63.3%). In some participants, the gamma band was tracked either due to the presence of a physiology peak or documentation of dyskinetic symptoms.\n\nIn addition to sensing configuration, stimulation settings were also extracted for the analysis since most patients were receiving continuous high-frequency stimulation therapy during the chronic recordings. Therapy settings varied across subjects, with stimulation pulse width ranging from 60 to 90 µsec, the stimulation frequency ranging from 110 Hz to 180 Hz, and stimulation amplitude ranging from 0 mA to 4.5 mA.\n\n## Beta power was usually reduced at night but could also be increased, especially in GPi\n\nFigure 1 A shows chronic GPi high beta (24.41 Hz ± 2.50 Hz) activity recorded in an individual subject over 5 consecutive days. Power fluctuations were observed with a consistent reduction during night-time. The reduction manifested around midnight. Vertical lines indicate the time of the events marked, and ranged from 7am to midnight (EDT), corresponding to a period of higher beta power during the daytime period. The polar plots illustrate the circadian rhythms, showing that beta power was higher during the day (when the events were marked). Interestingly, an increased power at night was also observed in other patients. Figure 1 B shows an example of beta (19.53Hz ± 2.50Hz) in a different patient with GPi recordings, consistently increased at night and decreased during the day when the subject marked events. The normalized power collected in each GPi (N = 135) plotted over 24h and sorted by highest power in daytime, is shown on the circadian heatmap (Fig. 1 C). Visual inspection shows the presence of a strong circadian rhythm in most recordings. We found a decreased power at night in 57.8% of the recordings (78 hemispheres) while an increased power was observed in 28.9% (39 hemispheres). In 18 hemispheres (13.3%), there was no statistically significant difference between day and night (see Methods).\n\nAs expected, STN power was more consistently reduced at night compared to daytime when compared to the GPi (76.7%, 23 hemispheres), with only 5 hemispheres (16.7%) showing increased power at night-time. Two hemispheres (6.7%) exhibited no statistically significant difference between day and night-time. Figure 2 shows individual examples of STN beta power which was reduced at night (A), as well as STN beta power increased at night (B). The STN power fluctuation of each recording (n = 30) is shown on the circadian heatmap (Fig. 2 C).\n\n## Basal ganglia circadian rhythm depends on the frequency band recorded\n\nGiven the variability in circadian rhythm (increase vs decrease power at night), especially in GPi, we investigate the effects of sensing frequency. For each recording, the change in power between day and night was calculated and plotted against the center of the sensing frequency (Fig. 3 A/D).\n\nIn GPi, non-parametric tests within each canonical spectral band (theta/alpha, low-beta, high-beta, and gamma) indicated that changes in neural signals between day and night were significantly different from 0 (no-change) in both high-beta (median = 1.29, p = 0.044, FDR corrected) and gamma (median = 1.43, p = 0.013, FDR corrected). The positive median values indicate that GPi power in high-beta and gamma bands were more likely to decrease at night. Alpha and Low-Beta power were either decreased or increased during night-time, as indicated by a median non-significantly different from 0 (alpha, p = 0.576 and Low-Beta p = 0.291, FDR corrected). A one-way ANOVA to compare across spectral bands revealed a significant effect of sensing frequency in GPi (F = 6.42, p < 0.001). Post-hoc analysis with Tukey’s HSD showed that the circadian rhythm in the theta/alpha band showed more increased in night-time than high-beta (q=-0.81, p = 0.023) and gamma (q=-1.31, p = 0.002), and low-beta showed more increased in night-time than gamma (q=-1.07, p = 0.019) (Fig. 3 B).\n\nIn STN, non-parametric tests showed that low-beta (median = 1.29, p = 0.033, FDR corrected) and high-beta (median = 1.29, p = 0.022, FDR corrected) were significantly different from 0. The positive median revealed that STN power in low- or high-beta bands was more likely to decrease at night, while theta/alpha power was either increased or decreased. A one-way ANOVA to compare across spectral bands indicated a significant effect of sensing frequency (F = 4.11, p = 0.014). Post-hoc analysis with Tukey’s HSD showed that the circadian rhythm in high-beta decreased more in night-time than theta/alpha (q=-1.71, p = 0.013) (Fig. 3 E).\n\nThese results suggest that different frequency bands of brain activity exhibited circadian rhythms of different magnitudes and directions. In both targets, high-beta power was more consistently reduced at night, while theta/alpha power was either increased or reduced at night. However, low-beta band, especially in the GPi, was more likely to increase at night (32.6%) than in STN (11.1%).\n\n## Extended-release medications modulate circadian rhythm\n\nMedications and stimulation are known to modulate basal ganglia activity in PD, especially the beta band. Therefore, a general linear model (GLM) was built to test the effects of stimulation parameters and medications on the direction of beta power (13-30Hz) circadian rhythms in GPi and STN. In particular, we investigated whether the change in beta power (dependent variable) during daytime versus night-time was significantly modulated by the following independent variables: the levodopa equivalent daily dose (LEDD), the use of medications (dopaminergic extended-release, benzodiazepines, and melatoninergic medications), the total energy delivered (TEED) (a measure of the amount of stimulation based on amplitude, pulse width, and frequency), the contact used for stimulation (dorsal/ventral), and the hemisphere recorded (left/right).\n\nTable 2 summarizes the results of the GLM. The model indicated a significant effect of extended-release dopaminergic medications on beta power circadian rhythm (z = 2.46, p = 0.016), while all other variables (stimulation parameters and other medications) did not significantly affect the change in beta power during daytime versus night-time. In GPi, the group of subjects using extended-release dopaminergic medication showed a statistically significant greater decrease in power at night compared those who were not taking extended-release medication (W = 112, p < 0.001) (Fig. 3 C). Interestingly, the GLM built for STN recordings did not reveal any independent variable that contributed significantly to the direction of circadian rhythm in STN. The use of extended-release dopaminergic medication did not influence the direction of circadian rhythm in STN (z = 0.61, p = 0.540).\n\nAlthough the TEED did not significantly affect beta power circadian rhythms at the group level, we observed that stimulation parameters could affect circadian rhythms within individual subjects. In particular, larger stimulation amplitude might reduce the range of neural signal fluctuations as shown in Figure S1A. However, the influence of stimulation varies considerably across patients.\n\n# Discussion\n\nThis retrospective study characterizes the effect of circadian rhythm on PD GPi and STN neurophysiology, using a commercially available device in a large sample size. The data revealed that 1) both GPi and STN power is significantly modulated by circadian rhythm in most PD subjects, 2) although power was mainly reduced at night, increased power was also found, especially in GPi (28%), 3) Both the frequency of the power band recorded, and the use of long-acting levodopa medications influenced the neurophysiological circadian rhythm.\n\nThe large chronically recorded dataset revealed that basal ganglia activity was strongly modulated by circadian rhythm, and that the frequency of subcortical power recorded could significantly affect the direction of the spectral power changes (increase or decrease) between day and night-time. Previous studies exploring circadian changes in STN LFP15, 25, 27, 28, 34, have shown that different canonical spectral bands behave differently during sleep with a general trend of slowing of brain oscillations, with increased low frequency oscillatory power (< 12Hz) and decreased beta and gamma power (> 13Hz) at night. Although our STN sub-analysis largely matches these previous STN findings, the GPi findings indicate more variability in pallidal circadian rhythm, especially in the low beta band which was increased at night in ~ 1/3 of the recordings. The increase in power at night, especially in low beta power, could be explained by the large spectral window of the recording. Indeed, the neuronal signal recorded chronically is set at a preselected frequency with a 5Hz window (± 2Hz). Therefore, it is possible that alpha power (~ 10Hz) contaminated recordings at 13Hz. However, our results showed increased power at night even in frequencies above 14Hz, which are unlikely to be contaminated by alpha power (Figs.1 and 2).\n\nContrary to most studies on sleep in PD, in our study, the brain activity was collected chronically while the subjects were on typical medication dosages and on stimulation. Thus, to further understand this intriguing result, especially in the beta band, we investigated the effect of both medication and stimulation on circadian beta power. We found that, in GPi, the use of extended-release levodopa modulated the direction of power changes. In particular, a decrease in beta power at night was more likely observed in subjects treated with long-acting levodopa medications when compared to those who were not taking extended-released medication. The use of long-acting levodopa medications could suppress beta power at night-time similar to the daytime35–37, thus masking the emergence of pathological beta power at night as seen in patients who were not taking extended released medication. Interestingly, the effect of long-acting levodopa was not significant in STN, although this is likely due to lack of power in this subgroup.\n\nOur observations on impact of circadian rhythm on basal ganglia activity has important potential implications for the implementation of aDBS therapy in PD. Currently, aDBS algorithms utilize a single or double threshold approach which is centered around the pathological beta signal in basal ganglia circuitry. The aDBS control system will increase the therapy level when the tracked signal is high and reduce therapy level when the tracked signal is low. Our study has revealed that neural signals in basal ganglia, specifically in the beta-band, had different trends in different subjects. The aDBS therapy may be set to stay at higher duty cycle if the threshold is built on daytime recordings for patients who have significant increase of power at night-time and vice versa. This challenge may result in either unintended additional battery drains or suboptimal therapy in the night-time. In addition, our analysis also indicated that the medication usages may contribute to changes in circadian rhythm, meaning that aDBS algorithm may need re-calibration for night-time therapy when medications, specifically the long-acting levodopa medications, changed. Thus, we caution that while aDBS can improve the responsiveness of neuromodulatory therapy in PD to adapt to activities of daily life, it should not be implemented as a one-size-fits-all approach. We would argue that neuromodulation will need to be tailored to each individual’s neural signature for optimal therapeutic benefit and that circadian patterns are an important consideration given that many people spend ~ 1/3 of their time in a sleep state.\n\nIt is important to highlight several limitations of our study. As a retrospective study, we did not have wearable sleep data or formal sleep diaries to confirm the sleep/wake states in all subjects and instead we developed a novel automated circadian detection algorithm based on the chronic neural recordings. However, several previous studies have demonstrated the feasibility of characterizing sleep based on subthalamic and pallidal signals29, 34, 38–40. We validated our algorithm in subjects who had marked event that we used as a surrogate for wakefulness. Additionally, we did not have real-time measurements of the patients’ symptoms, disease states, and sleep stages at the time of recordings. However, future studies could incorporate such measurements to better understand the circadian modulation of pallidal signals in greater detail. Similarly, since the recordings were collected from subjects receiving continuous high-frequency DBS and effective DBS therapy has been demonstrated to change LFP signals including during sleep15, the effect of circadian rhythm could also have been influenced by the impact of the therapeutic stimulation. Although the total electrical energy delivered (TEED) did not significantly explain the variability of GPi beta oscillation circadian rhythm in patients with PD, we observed within-subject effects of changing stimulation parameters on circadian rhythms (Figure S1A). It is thus possible that an important factor is the therapeutic effect of each stimulation parameter, which unfortunately is not available in the current retrospective dataset, as opposed to the simple TEED measurements.\n\nFuture clinical studies will need to better characterize the awake/asleep states, sleep stages, PD symptoms, and related parasomnias. These findings could be used to help guide the use of circadian rhythmicity in aDBS strategies.\n\nWe conclude that there is a circadian rhythm in neural signals recorded chronically from both GPi and STN in PD, and that the directionality and amplitude of the changes depend on the frequency tracked and the use of long-acting levodopa medications. Application of aDBS will need to account for circadian rhythms and factor them into the algorithms to ensure successful implementation in real world environments.\n\n# Methods\n\n## Study Participants and Data Collection:\n\nThis retrospective study was performed at the Norman Fixel Institute for Neurological Diseases at the University of Florida (UF). All subjects included (117) provided informed consent, in accordance with the Declaration of Helsinki, to participate in the UF INFORM Database, a clinical-research database that hosts subjects’ clinical records and neural recordings41. The study was approved by UF Institutional Review Board (IRB) to request and process data from UF INFORM Database. The inclusion criteria were individuals diagnosed with PD by a movement disorders-trained neurologist and who received DBS therapy with the sensing-enabled Medtronic Percept PC neurostimulator with unilateral or bilateral electrode implanted in the GPi or STN.\n\nRetrospective data were extracted from the UF INFORM Database, including brain recording (average power every 10min), therapy settings at recording, medications, and preoperative symptom assessments. Chronic sensing was usually enabled if therapy configuration was one of the sensing-available configurations, and the neural signal recorded was usually selected based on the most prominent spectral peak shown during baseline surveys42. As a retrospective study, wearable devices and sleep diaries were not available. However, the Percept DBS device allows subjects to indicate specific ‘events’ or symptoms (i.e ‘medication intake, ‘presence of dyskinesia’) that might be relevant for their clinical care. Therefore, the time of each event marked during each recording was extracted and used as a proxy for wakefulness. For each patient, the medications dose and schedule, were used to calculate the total Levodopa Equivalent Daily Dose (LEDD) and classified into common medication classes, namely the immediate release dopaminergic medication, the extended-release dopaminergic medication, melatoninergic medication, and Benzodiazepines. A total of 165 recordings were included in this study.\n\n## Data Processing\n\nAll clinical DBS programming session files retrieved from the UF INFORM Database were imported into the Brain Recording Analysis and Visualization Online (BRAVO) Platform43. Therapy configurations and available neural recordings were sorted chronologically. Some subjects have significantly more recordings than others, so only one recording from each unique hemisphere was included in final analysis to ensure all subjects contributed equally. For each patient, the first chronic neural recording with more than 5 days of data for each available hemisphere was extracted. All neural signals were z-score normalized using ±12 hours of recordings to eliminate non-stationary slow-wave drifts and allow group analysis. All neural recordings were time-aligned on a 24-hour clock based on Eastern Daylight-saving Time (EDT, GMT-04:00). An automated circadian detection algorithm was then implemented to detect day vs night period. First, neural recordings were binned into 2-hour windows with 90-minute overlap to calculate the mean and 99.9% confidence interval of neural signals at each 30-minute mark for each patient. Second, the bins with maximum average neural signal and minimum neural signal were extracted. All bins that overlap with the 99.9% confidence interval of the maximum bin were considered as the “High Neural Signal” period and all bins that overlap with the 99.9% confidence interval of the minimum bin were considered as the “Low Neural Signal” period. The time of ‘low’ and ‘high’ neuronal signal periods was used to determine when each period occurred (day vs night). Finally, in a subset of recordings in which events were marked (61%), the time of each event marked by the subjects during those 2 periods was extracted, and used to confirm that patient was awake during the day. The effect of circadian rhythm was calculated as the mean normalized power during day period across all recorded days subtracted by mean normalized power during night period across all recorded days.\n\n## Statistical Methods\n\nThe circadian rhythm was measured as the normalized difference between the Awake period and Asleep period by subtracting the mean asleep period neural signals from mean awake period neural signals. For each patient, the spectral bands recorded by the neurostimulator were extracted and categorized into “Theta/Alpha” (0-12Hz), “Low Beta” (13-20Hz), “High Beta” (21-30Hz), and “Gamma” (>31Hz) groups. One-way ANOVA was used to examine the effect of sensing frequency on circadian rhythm. Post-hoc pairwise comparison between each group were performed using Tukey’s test if a significant effect was found from the ANOVA. Non-parametric Mann-Whitney U test, with multiple comparison corrected with false-discovery rate (FDR), was applied within each canonical sensing frequency group to identify if the trend of circadian rhythm is increasing in daytime or decreasing in daytime by testing against 0. In addition, other therapeutic variables such as therapy frequency, therapy pulse width, and therapy amplitude were extracted for the corresponding chronic neural recordings. Medication classes such as dopaminergic and nondopaminergic medication were included along with the therapeutic configurations and sensing frequency in a generalized linear model (GLM) to identify the variables that significantly contributed to the circadian rhythm. The GLM was designed with the change in Beta band (13-30Hz) neural signals as the dependent variable. Independent variables for the GLM included the therapy hemisphere (left/right), therapy contact (dorsal/ventral), TEED44, LEDD, levodopa extended-release, benzodiazepines, and melatoninergic medications (yes = 1, no = 0).\n\n# References\n\n1. Benabid, A. L. Deep brain stimulation for Parkinson’s disease. Current Opinion in Neurobiology 13, 696–706 (2003).\n2. Volkmann, J. Deep Brain Stimulation for the Treatment of Parkinson’s Disease. Journal of Clinical Neurophysiology 21, 6 (2004).\n3. Eisinger, R. S., Cernera, S., Gittis, A., Gunduz, A. & Okun, M. S. A review of basal ganglia circuits and physiology: Application to deep brain stimulation. Parkinsonism & Related Disorders 59, 9–20 (2019).\n4. Beudel, M. & Brown, P. Adaptive deep brain stimulation in Parkinson’s disease. Parkinsonism & Related Disorders 22, S123–S126 (2016).\n5. Little, S. et al. Adaptive deep brain stimulation in advanced Parkinson disease. Ann Neurol. 74, 449–457 (2013).\n6. Little, S. et al. Adaptive deep brain stimulation for Parkinson’s disease demonstrates reduced speech side effects compared to conventional stimulation in the acute setting. J Neurol Neurosurg Psychiatry 87, 1388–1389 (2016).\n7. Ray, N. J. et al. Local field potential beta activity in the subthalamic nucleus of patients with Parkinson’s disease is associated with improvements in bradykinesia after dopamine and deep brain stimulation. Experimental Neurology 213, 108–113 (2008).\n8. Cagle, J. N. et al. Suppression and rebound of pallidal beta power: observation using a chronic sensing DBS device. Frontiers in Human Neuroscience 15, 749567 (2021).\n9. Eisinger, R. S. et al. Parkinsonian Beta Dynamics during Rest and Movement in the Dorsal Pallidum and Subthalamic Nucleus. J. Neurosci. 40, 2859–2867 (2020).\n10. Feldmann, L. K. et al. Subthalamic beta band suppression reflects effective neuromodulation in chronic recordings. European Journal of Neurology n/a, (2021).\n11. Nakajima, A. et al. Case Report: Chronic Adaptive Deep Brain Stimulation Personalizing Therapy Based on Parkinsonian State. Front Hum Neurosci 15, 702961 (2021).\n12. Neumann, W.-J. et al. Toward Electrophysiology-Based Intelligent Adaptive Deep Brain Stimulation for Movement Disorders. Neurotherapeutics 16, 105–118 (2019).\n13. Swann, N. C. et al. Adaptive deep brain stimulation for Parkinson’s disease using motor cortex sensing. J Neural Eng 15, 046006 (2018).\n14. Oehrn, C. R. et al. Personalized chronic adaptive deep brain stimulation outperforms conventional stimulation in Parkinson’s disease. medRxiv 2023.08.03.23293450 (2023) doi: 10.1101/2023.08.03.23293450.\n15. Gilron, R. et al. Sleep-Aware Adaptive Deep Brain Stimulation Control: Chronic Use at Home With Dual Independent Linear Discriminate Detectors. Front Neurosci 15, 732499 (2021).\n16. Vitaterna, M. H., Takahashi, J. S. & Turek, F. W. Overview of Circadian Rhythms. Alcohol Res Health 25, 85–93 (2001).\n17. Parekh, P. K., Ozburn, A. R. & McClung, C. A. Circadian clock genes: Effects on dopamine, reward and addiction. Alcohol 49, 341–349 (2015).\n18. Radwan, B., Liu, H. & Chaudhury, D. The role of dopamine in mood disorders and the associated changes in circadian rhythms and sleep-wake cycle. Brain Research 1713, 42–51 (2019).\n19. Castañeda, T. R., de Prado, B. M., Prieto, D. & Mora, F. Circadian rhythms of dopamine, glutamate and GABA in the striatum and nucleus accumbens of the awake rat: modulation by light. Journal of Pineal Research 36, 177–185 (2004).\n20. Luo, A. H. & Aston-Jones, G. Circuit projection from suprachiasmatic nucleus to ventral tegmental area: a novel circadian output pathway. European Journal of Neuroscience 29, 748–760 (2009).\n21. Van Drunen, R. & Eckel-Mahan, K. Circadian Rhythms of the Hypothalamus: From Function to Physiology. Clocks & Sleep 3, 189–226 (2021).\n22. Seney, M. L. et al. Diurnal rhythms in gene expression in the prefrontal cortex in schizophrenia. Nat Commun 10, 3355 (2019).\n23. Oishi, Y. & Lazarus, M. The control of sleep and wakefulness by mesolimbic dopamine systems. Neuroscience Research 118, 66–73 (2017).\n24. Li, S., Wang, Y., Wang, F., Hu, L.-F. & Liu, C.-F. A New Perspective for Parkinson’s Disease: Circadian Rhythm. Neurosci Bull 33, 62–72 (2017).\n25. van Rheede, J. J. et al. Diurnal modulation of subthalamic beta oscillatory power in Parkinson’s disease patients during deep brain stimulation. npj Parkinsons Dis. 8, 1–12 (2022).\n26. Baumgartner, A. J. et al. Basal Ganglia Local Field Potentials as a Potential Biomarker for Sleep Disturbance in Parkinson’s Disease. Frontiers in Neurology 12, (2021).\n27. Thompson, J. A. et al. Sleep patterns in Parkinson’s disease: direct recordings from the subthalamic nucleus. J Neurol Neurosurg Psychiatry 89, 95–104 (2018).\n28. Urrestarazu, E. et al. Beta activity in the subthalamic nucleus during sleep in patients with Parkinson’s disease. Movement Disorders 24, 254–260 (2009).\n29. Yin, Z. et al. Pallidal activities during sleep and sleep decoding in dystonia, Huntington’s, and Parkinson’s disease. Neurobiology of Disease 182, 106143 (2023).\n30. Yin, Z. et al. Pathological pallidal beta activity in Parkinson’s disease is sustained during sleep and associated with sleep disturbance. Nat Commun 14, 5434 (2023).\n31. Anjum, M. F. et al. Multi-night naturalistic cortico-basal recordings reveal mechanisms of NREM slow wave suppression and spontaneous awakenings in Parkinson’s disease. 2023.06.23.546302 Preprint at https://doi.org/10.1101/2023.06.23.546302 (2023).\n32. Smyth, C. et al. Adaptive Deep Brain Stimulation for sleep stage targeting in Parkinson’s disease. Brain Stimulation 16, 1292–1296 (2023).\n33. Zahed, H. et al. The Neurophysiology of Sleep in Parkinson’s Disease. Movement Disorders 36, 1526–1542 (2021).\n34. Chen, Y. et al. Automatic Sleep Stage Classification Based on Subthalamic Local Field Potentials. IEEE Transactions on Neural Systems and Rehabilitation Engineering 27, 118–128 (2019).\n35. Schapira, A. H. V., Emre, M., Jenner, P. & Poewe, W. Levodopa in the treatment of Parkinson’s disease. European Journal of Neurology 16, 982–989 (2009).\n36. Gaudreau, H., Carrier, J. & Montplaisir, J. Age-related modifications of NREM sleep EEG: from childhood to middle age. Journal of Sleep Research 10, 165–172 (2001).\n37. Giannicola, G. et al. The effects of levodopa and ongoing deep brain stimulation on subthalamic beta oscillations in Parkinson’s disease. Experimental Neurology 226, 120–127 (2010).\n38. Verma, A. K. et al. Basal ganglia engagement during REM sleep movements in Parkinson’s disease. npj Parkinsons Dis. 8, 1–6 (2022).\n39. Christensen, E., Abosch, A., Thompson, J. A. & Zylberberg, J. Inferring sleep stage from local field potentials recorded in the subthalamic nucleus of Parkinson’s patients. Journal of Sleep Research 28, e12806 (2019).\n40. Verma, A. K. et al. Parkinsonian daytime sleep-wake classification using deep brain stimulation lead recordings. Neurobiology of Disease 176, 105963 (2023).\n41. Eisinger, R. S. et al. Parkinson’s disease motor subtype changes during 20 years of follow-up. Parkinsonism & Related Disorders 76, 104–107 (2020).\n42. Jimenez-Shahed, J. Device profile of the percept PC deep brain stimulation system for the treatment of Parkinson’s disease and related disorders. Expert Review of Medical Devices 18, 319–332 (2021).\n43. Cagle, J. N. et al. Brain Recording Analysis and Visualization Online (BRAVO): An open-source visualization tool for deep brain stimulation data. Brain Stimulation 16, 793–797 (2023).\n44. Koss, A. M., Alterman, R. L., Tagliati, M. & Shils, J. L. Calculating total electrical energy delivered by deep brain stimulation systems. Annals of Neurology 58, 168–168 (2005).\n\n# Tables\n\n## Table 1\nPatient demographic, clinical characterization and recording settings.\n\n| | GPi | STN | Total | P-value GPi vs STN |\n|---|---|---|---|---|\n| **Demography** | | | | |\n| total participants | 96
(135 hemispheres) | 23
(30 hemispheres) | 119
(165 hemispheres) | |\n| gender | M: 73 (76%)
F: 23 (24%) | M: 16 (70%)
F: 7 (30%) | M: 89 (75%)
F: 30 (25%) | |\n| age at surgery (year) | 67.9 ± 9.4 | 67.8 ± 6.9 | 67.9 ± 8.9 | 0.563 |\n| disease duration (year) | 13.7 ± 5.8 | 14.2 ± 9.0 | 13.7 ± 6.4 | 0.513 |\n| **Symptoms and Therapy Characteristics** | | | | |\n| Preoperative UPDRS | 35.4 ± 12.5 | 37.6 ± 13.5 | 35.8 ± 12.7 | 0.492 |\n| TEED (µj) | 129 ± 111 | 60 ± 74 | 118 ± 105 | 0.037 |\n| LEED (mg) | 1282 ± 686 | 1033 ± 486 | 1234 ± 658 | 0.176 |\n| **Recording Settings** | | | | |\n| recording durations (day) | 17.1 ± 20.5 | 20.9 ± 15.4 | 17.8 ± 19.7 | 0.036 |\n| time since implant (day) | 12 ± 34 | 18 ± 40 | 13 ± 35 | 0.792 |\n| sensing frequency (Hz) | 17.2 ± 13.0 | 16.4 ± 3.9 | 17.1 ± 11.9 | 0.018 |\n\nM: Male, F: Female, TEED: total electrical energy delivered, LEDD: levodopa equivalent daily dosage\n\n## Table 2\nGeneralized Linear Model for effect of stimulation therapy and medications in Beta-band (13-30Hz) subgroup.\n\n| | Coefficient | Std. Err. | z | P>|z| | [0.025 | 0.975] |\n|---|---|---|---|---|---|---|\n| const | 0.8452 | 0.537 | 1.575 | 0.115 | -0.207 | 1.897 |\n| hemisphere | 0.1552 | 0.245 | 0.633 | 0.526 | -0.325 | 0.635 |\n| channel | -0.4221 | 0.28 | -1.508 | 0.132 | -0.971 | 0.126 |\n| LEDD | -0.0004 | 0 | -1.78 | 0.075 | -0.001 | 4.42E-05 |\n| levodopa ER | 0.76 | 0.269 | 2.825 | **0.005** | 0.233 | 1.287 |\n| benzo | -0.1727 | 0.257 | -0.673 | 0.501 | -0.676 | 0.33 |\n| melatonin | -0.113 | 0.272 | -0.416 | 0.678 | -0.646 | 0.42 |\n| TEED | -0.0307 | 1.154 | -0.027 | 0.979 | -2.293 | 2.232 |\n\nTEED: total electrical energy delivered, LEDD: levodopa equivalent daily dosage\n\n# Supplementary Files\n\n- [SupplementaryFigure1.docx](https://assets-eu.researchsquare.com/files/rs-3467647/v1/4160f7db75d3f3a8be9d805c.docx)\n- [NCOMMS2350065rs.pdf](https://assets-eu.researchsquare.com/files/rs-3467647/v1/0d856a36d273f6d162646898.pdf) \n Reporting Summary"} {"paper_id": "prb15", "title": "Diminished circadian and ultradian rhythms in pathological brain tissue in human in vivo", "text": "Diminished circadian and ultradian rhythms in pathological brain tissue in human in vivo\n\nYujiang Wang\nCnnplab@newcastle.ac.uk\n\nNewcastle University https://orcid.org/0000-0002-4847-6273\n\nMariella Panagiotopoulou\nNewcastle University\n\nChristopher Thornton\nNewcastle University\n\nFahmida Chowdhury\nUniversity College London Hospitals NHS Foundation Trust\n\nJohn Duncan\nUCL Insitute of Neurology https://orcid.org/0000-0002-1373-0681\n\nAndrew McEvoy\nUK NIHR University College London Hospitals Biomedical Research Centre, Department of Clinical and Experimental Epilepsy, UCL Institute of Neurology, Queen Square, London\n\nJane de Tisi\nUniversity College London Hospitals NHS Foundation Trust\n\nPeter Taylor\nNewcastle University\n\nSarah Gascoigne\nNewcastle University\n\nBilly Smith\nNewcastle University\n\nBeate Diehl\nUniversity College London\n\nAnna Miserocchi\nUniversity College London\n\nArticle\n\nKeywords:\n\nPosted Date: September 18th, 2023\nDOI: https://doi.org/10.21203/rs.3.rs-3335487/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: There is NO Competing Interest.\n\nVersion of Record: A version of this preprint was published at Nature Communications on October 2nd, 2024. See the published version at https://doi.org/10.1038/s41467-024-52769-6.\nDiminished circadian and ultradian rhythms in pathological brain tissue in human *in vivo*\n\nMariella Panagiotopoulou$^{1,o}$, Christopher Thornton$^{1,o}$,\nFahmida A Chowdhury$^3$, Beate Diehl$^3$, John S Duncan$^3$,\nSarah J Gascoigne$^1$, Andrew W McEvoy$^3$, Anna Miserocchi$^3$,\nBilly C Smith$^1$, Jane de Tisi$^3$, Peter N Taylor$^{1,2,3}$,\nYujiang Wang$^{1,2,3,*}$\n\nSeptember 7, 2023\n\n1. CNNP Lab (www.cnnp-lab.com), Interdisciplinary Computing and Complex BioSystems Group, School of Computing, Newcastle University, Newcastle upon Tyne, United Kingdom\n\n2. Faculty of Medical Sciences, Newcastle University, Newcastle upon Tyne, United Kingdom\n\n3. UCL Queen Square Institute of Neurology, Queen Square, London, United Kingdom\n\n* Yujiang.Wang@newcastle.ac.uk\no Joint first authors\nAbstract\n\nChronobiological rhythms, such as the circadian rhythm, have long been linked to neurological disorders, but it is currently unknown how pathological processes affect the expression of biological rhythms in the brain.\n\nHere, we use the unique opportunity of long-term, continuous intracranially recorded EEG from 38 patients (totalling 6338 hours) to delineate circadian and ultradian rhythms in different brain regions. We show that functional circadian and ultradian rhythms are diminished in pathological tissue, independent of regional variations. We further demonstrate that these diminished rhythms are persistent in time, regardless of load or occurrence of pathological events.\n\nThese findings provide the first evidence that brain pathology is functionally associated with persistently diminished chronobiological rhythms *in vivo* in humans, independent of regional variations or pathological events. Future work interacting with, and restoring, these modulatory chronobiological rhythms may allow for novel therapies.\n1 Introduction\n\nPhysiological processes are often modulated and structured by chronobiological rhythms. The circadian rhythm is perhaps the most pertinent and well-studied rhythm with a central pacemaker in the suprachiasmatic nucleus. Such rhythms are also differentially expressed in a range of tissues and organs, entrained by the central pacemaker. For example, multiple organs have been shown to display their own circadian rhythm in terms of gene expression and translation even in the absence of the pacemaker (20). Even within a single organ, such as the brain, circadian regulation of gene expression is tissue-specific (32, 29). This local, or tissue-level, autonomous rhythmicity allows tissue-specific adaptations in phase or magnitude (46), whilst being coordinated by a central pacemaker. Other chronobiological rhythms also exist on longer and shorter timescales, termed infradian and ultradian rhythms, respectively. However, these are far less well-studied, appear to differ in magnitude and period between individuals, organs, and tissues, and their biological mechanisms are elusive. So far, candidate drivers of some ultradian rhythms have been proposed, such as the pulsatile cortisol secretion in mammals every 1-3 hours (18, 17), where various organs and tissues may react differently (12, 39). Taken together, there is evidence that, with or without a central pacemaker, circadian and ultradian rhythms are differentially expressed at the tissue level to temporally structure and modulate local physiological processes.\n\nDisrupted chronobiological rhythms are often associated with dysfunction and disease. Associations between altered circadian rhythms and neurodevelopmental disorders, mood disorders, epilepsy, Parkinson’s, and dementia are reported (24, 17). Similarly, disrupted ultradian rhythms may also be associated with neurological disorders, although their underpinning mechanisms are only beginning to be explored in animal models (28, 2). Many of the reported associations are linked to behavioural disruptions on circadian and ultradian timescales (e.g. sleep, levels of physical activity). However, tissue level regulation and expression of chronobiological rhythms in brain activity is less well-studied. One ex-vivo study with 16 patients with drug-refractory temporal lobe epilepsy showed that the expression of the circadian clock gene Bmal1 is reduced in surgically resected pathological tissue compared to healthy tissue (45). Similarly, tissue-level disruption to clock gene transcription and translation are found in various animal models of epilepsy (5). Thus,\nemerging evidence hints at tissue-level alteration of chronobiological rhythms in pathological tissue in brain disorders. However, to date, it is completely unknown if pathological tissue shows different expression of chronobiological rhythms in brain activity and electrophysiology *in vivo* in humans.\n\nHere, we therefore investigate the rhythmicity of human brain activity *in vivo*. EEG is a commonly used method to measure brain activity patterns and multiple studies have shown that circadian and multiple ultradian rhythms can also be captured as the rhythmic modulation of particular signal properties (e.g. (\\(37, 38, 56, 55, 54, 31\\))). In this study, we will use intracranially recorded continuous EEG (iEEG) over multiple days to measure circadian and ultradian rhythms in humans *in vivo*. Intracranial recordings have the advantage of a high signal-to-noise ratio, and provide excellent spatial resolution, as the electrodes directly sample from the target brain tissue without interference. This allows us to delineate functional chronobiological rhythms in specific locations.\n\n2 Results\n\n2.1 Overview of data and analysis\n\nWe analysed long-term iEEG recordings from 38 individuals with refractory focal epilepsy from the National Hospital for Neurology and Neurosurgery (Table 1). From the iEEG recordings of each patient, we localised each recording contact to an anatomical region of interest (ROI) and calculated the relative band power in the delta range (1 - 4 Hz) and the other four frequency bands ( theta : 4 - 8 Hz, alpha : 8 - 13 Hz, beta : 13 - 30 Hz and gamma : 30 - 47.5 Hz, 52.5 - 57.5 Hz, 62.5 - 77.5 Hz) using a non-overlapping 30 second window over the continuous recording in all patients (recording duration between 2-21 days). Circadian (a period of 19 - 31 hours) and ultradian (1-3h, 3-6h, 6-9h, 9-12h, 12-19h periods) rhythms were then isolated by applying band pass filters to the signal of relative band power over days in each ROI.\n\nWe used the clinically identified regions where seizures originate (seizure onset zone, or SOZ) as a proxy for pathological tissue. To ensure robustness of our results, we also used the alternative definition of the tissue that was subsequently surgically removed, as it was deemed central to\ngenerating epileptic seizures. We obtained similar results (Suppl. S5) with either definition, and will use the broad term of “pathological tissue” throughout the paper to refer to tissue that is most likely functionally (causing seizures) and/or structurally pathological.\n\nTable 1: Table 1: Summary of patient data used in the analysis.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
N38
Age (mean,SD)32.1 (8.5)
Sex (M,F)17,21
Temporal, extratemporal17,21
Side (Left, Right)22,16
Num contacts (mean, sd)72.8 (25.2)
Recording Duration in hours (mean, sd)111.5 (58.1 )
\n\n2.2 Circadian rhythms are diminished in pathological brain tissue\n\nFigure 1(a) shows the power of the delta EEG band over seven days for an example patient, filtered to isolate only the circadian rhythm (19h-31h). In this patient the regions with the weakest circadian rhythm are within the left inferior parietal lobe, visualized in Figure 1(b). These comprise two out of the three pathological regions. Figure 1(c) compares the power of the delta circadian rhythm in regions with pathology against the remaining regions. We quantify this difference using the non-parametric Area Under the Curve (AUC) of a Receiver Operating Characteristics analysis (7). Here, AUC values greater than 0.5 imply diminished power in pathological tissue and the example patient yielded an AUC=0.92. Figure 1(d) shows the AUC values across all 38 patients - the distribution is substantially greater than 0.5 (median AUC=0.62, p=0.005) implying a diminished circadian rhythm in delta power in the pathological tissue across a majority of patients (66% of subjects with AUC>0.5).\n\n2.3 Multiple ultradian rhythms are diminished in pathological brain tissue\n\nFigure 2(a) shows the delta band power, filtered to isolate the 3 - 6 hour ultradian rhythm, across regions for the same example patient. As with the circadian rhythm, there was a diminished power in the three pathological regions, quantified with an AUC of 0.96 for this patient and visualized in\nFigure 1: Circadian rhythm of delta power is diminished in brain areas with pathology. a-c) From subject A: (a) The circadian rhythm of delta power, obtained by applying a band-pass filter to isolate the power of the signal with a period between 19 and 31 hours. Pathological tissue is shown in red. Bars indicate the relative power of the signal in each ROI. (b) The relative power in each brain area, pathological tissue is outlined in red. (c) The relative power of the circadian rhythm in pathological tissue compared to other tissue. An AUC of 0.92 is calculated when using this relative power to predict pathology. (d) The AUC of each subject for the same prediction. An AUC>0.5 indicates that the rhythm is diminished in pathological tissue.\nFigure 2(b). Diminished ultradian rhythms are present across the cohort, with a median AUC of 0.69 for the 3 - 6 hour rhythm, and median AUC values above 0.5 for all rhythm periods - shown in Figure 2(c), p<0.05 for all.\n\nIn Suppl. S4 we further show that these effects in circadian and ultradian rhythms are not simply due to a dimished magnitude of the raw EEG signal in the pathological tissue.\n\n2.4 Pathology is independently associated with diminished chronobiological rhythms\n\nTo investigate if our observed effects are potentially explained by the spatial location, or the broad brain lobe (or subcortical region) of the observations, we plotted the power of an example ultradian rhythm in delta grouped by lobe across patients (Figure 3(a)). While there is some variation of power of this ultradian rhythm across lobes, the power in the pathological tissue in each area appears consistently diminished.\n\nTo show that pathology is independently associated with diminished chronobiological rhythms, we tested the association in a mixed effects regression with the lobe (those shown in figure 3(a)) as a covariate. This model took the power of the rhythm in each ROI as the dependent variable, the lobe of the ROI and whether the ROI has pathology (is within the SOZ) as independent variables, and grouped by patient. Figure 3(b) shows the partially standardized fixed effect for pathology (\\( \\beta_1 \\)) for each ultradian/circadian rhythm in delta band power. All coefficients are below zero, indicating that ultradian/circadian rhythms are diminished in pathological tissue. Applying a likelihood ratio test to compare a model with pathology and brain area to a model with brain area only, we find that the effect of pathology explains the power of cycles significantly better for almost all EEG bands and ultradian/circadian rhythms (see Suppl S2 for details).\n\nFinally, we also checked if any particular type of pathology was associated with diminished rhythmicity, and found that most subjects showed this effect without evidence for the influence of the type of pathology (Suppl. S6).\nFigure 2: Ultradian rhythm of delta power is diminished in brain areas with pathology. a-c) From subject A: (a) An ultradian rhythm of delta power, obtained by applying a band-pass filter to isolate the power of the signal with a period between 3 and 6 hours. Pathological tissue is shown in red. Bars indicate the relative power of the signal in each ROI. (b) The relative power of the ultradian rhythm (3-6h) in each brain area, pathological tissue is outlined in red, no recording was performed in gray areas. (c) The AUC of each subject when predicting pathology from the power of each ultradian rhythm. An AUC>0.5 indicates that the rhythm is diminished in pathological tissue.\n\nFigure 3: Tissue pathology is associated with diminished rhythms while controlling for brain region. (a) The power of the delta ultradian rhythm (3h-6h) in each lobe or region for all patients, with each dot showing the power of the rhythm recorded by an electrode located in that region - some patients have multiple electrode per region. Red dots indicate electrodes recording from pathological tissue, blue from other tissue. The lines indicate median and inter-quartile range, calculated on the medians for each individual. (b) The effect size (partially standardized coefficient and 95 % confidence interval) for tissue pathology in a mixed effects regression relating brain region and tissue pathology to rhythm power. Shows the expected difference in rhythm power (in standard deviations) for pathological tissue.\n2.5 Diminished rhythms are persistent in time and independent of seizure occurrence\n\nTo assess whether the rhythms remained diminished in pathological tissue consistently over time and not only during the period around epileptic seizures (peri-ictal period), we calculated a rolling median of the AUC using a window proportional to the rhythm period (36 hours for the circadian rhythm). We illustrate the circadian rhythm of delta power in our sample patient in figure 4(a), the rolling AUC is shown in figure 4(b) along with a histogram showing that the distributions of AUC values are similar during inter-ictal and peri-ictal periods. Figure 4(c) aggregates results across subjects and rhythms, showing no difference in the AUC distributions of inter-ictal and peri-ictal periods. The overall seizure load (average number of seizures per hour) was also not correlated with the AUC for the circadian rhythm of delta (\\( r = -0.04 \\)) and no strong correlation was found for any other rhythm (\\( r < 0.3 \\), see Suppl. S3).\nFigure 4: Rhythms remain diminished in pathological tissue across time and independent of seizure occurrence. a-e) Example subject A: (a) The power of the circadian rhythm of delta across ROIs. Each cell represents the power of the circadian rhythm in the corresponding ROI and 30 second time segment. ROIs in red are deemed pathological. (b) The median AUC of the circadian rhythm captured using a rolling window of 36 hours. The peri-ictal period (1 hour before seizure start to 1 hour after its end) is shown in orange. The histogram shows the distribution of AUC values calculated during peri-ictal and inter-ictal periods. (c) Compares rolling AUC values calculated during inter-ictal and peri-ictal periods for each circadian and ultradian rhythm of delta power. A paired t-test indicates no difference between periods for each rhythm.\n3 Discussion\n\nAnalysing long-term iEEG recordings from 38 subjects with refractory focal epilepsy, we identified rhythms in the power of canonical EEG bands at circadian and ultradian timescales. We found that these rhythms were diminished in pathological tissue, and that this association remained when we controlled for brain area. We also found that these rhythms remain diminished persistently across time, without dependence on seizure occurrence. Our work provides initial evidence of a link between the strength of chronobiological rhythms and the healthy functioning of brain tissue in humans *in vivo*.\n\nCircadian clock gene dysfunction has been seen in pathological tissue in multiple animal models (5) and human tissue (45), but a key advance in our study is to also demonstrate a *functional* abnormality in pathological tissue in terms of electrophysiological function in humans. From animal models we have learned that circadian gene oscillation pattern do not necessarily translate to similar changes in mRNA or protein level (5). It was therefore also unclear if disruptions in these patterns translate to electrophysiological dysfunction, particularly in humans. Although numerous studies have reported circadian and ultradian rhythms in a range of signal properties in human EEG, these have been reported both in healthy participants (1, 41, 6), as well as in e.g. epilepsy patients (27, 31). It was therefore unknown if (i) there was a dysfunction in circadian and ultradian rhythms in electrophysiology associated with pathology in humans and (ii) if so, how the dysfunction would be expressed. Our work therefore serves as crucial evidence that (i) dysfunction is seen in pathology in circadian and ultradian rhythms in electrophysiological function, and (ii) dysfunction is expressed as a persistently diminished rhythm.\n\nElectrophysiological function is, of course, not limited to the signal features of relative band power that we analyzed. Indeed, there is evidence that other EEG signal features may display different rhythms (27). Future work should investigate a fuller range of signal features and seek to answer questions such as whether different pathologies display different profiles of disruption in rhythms. Nevertheless, relative band power is a primary set of features that is both widely accepted and used in neuroscience, making it easier to compare and put our results into context. We are also encouraged that our main results replicate over all frequency bands. Finally, our results are\nin agreement with a wider literature: diminished rhythmicity appears to be consistently observed in multiple modalities and organs in ageing and pathology (22, 4).\n\nAnother open question is if the electrophysiological circadian disruptions are a cause or consequence of the epileptogenic pathology. In our data, we observed no correlation between the resection of diminished rhythms and subsequent surgical outcome. This observation would suggest that sparing regions with diminished rhythms does not cause recurrent seizures after surgery per se. Similarly, we observed no temporal correlation between the magnitude of diminished rhythms and seizure occurrence. These observations should be validated in a larger cohort in future, ideally with more complete spatial sampling. We can nevertheless conclude that we see no evidence of disrupted rhythms causing seizures in our cohort.\n\nInterestingly, circadian and multi-day rhythms have attracted great interest recently: Various EEG and physiological signals display circadian and multi-day rhythms, and seizures occurrence(21, 23, 14), as well as other seizure features(40, 31, 10) couple to the phase of these rhythms in most patients. However, the mechanism of this coupling remains elusive, and the key question is how the seizure-generating process was modulated. Our recordings were too short for most patients to investigate multi-day rhythms, but our work can contribute towards the circadian aspect of the question. Our data suggests the epileptogenic pathology actually experiences a persistently diminished circadian modulation, most likely caused by the pathology itself. Therefore, we suggest that the circadian modulation of seizure occurrence and other seizure features is most likely mediated as a network phenomenon with other non-pathological regions, rather than arising locally within the pathological tissue itself. This supposition is also supported by recent observations that interictal markers of epilepsy are also more persistent, and less rhythmic in pathological tissue, possibly independent of seizure occurrence (33, 44). Future work will investigate if direct evidence of this network modulation can be found.\n\nIn general, a bi-directional relationship is often highlighted between circadian rhythmicity and neurological conditions(24), particularly epilepsy(26). A vicious circle is often described, where pathology or pathological events may erode or disrupt circadian rhythms, and disrupted rhythms may in turn exacerbate disease symptoms or even support disease progression. A key component in\nthis vicious circle is sleep, which we have not investigated explicitly in our study. However, future work should consider if alterations in both ultradian and circadian rhythms may reflect a loss of healthy sleep physiology regionally and behaviorally. Much of this complex interplay between rhythms, sleep, and disease is still unknown; nevertheless, our work provides initial evidence for a vital part of this vicious circle: circadian modulation of electrophysiology is indeed impaired in pathological tissue.\n\nA limitation of our study is the coverage of electrodes in each patient. As the implantation of the iEEG is to inform surgery, electrodes are typically confined to a single hemisphere or a series of neighboring or connected regions. This means that each patient does not have complete data across all brain areas, and the AUC values calculated are based only implanted regions. A related limitation is that pathology might be present more broadly across the brain than the implanted region or SOZ (19 30 11). It is also possible that the typical chronobiological rhythms of patients could be disrupted by surgery and implantation of the iEEG electrodes, their stay in the epilepsy monitoring unit, and changes to anti-epileptic medication.\n\nFuture work will seek to establish a normative map (15 9 43, 3) of the expected power of each ultradian and circadian rhythms in healthy tissue. Such a map would allow a better estimation if any particular observed rhythm was abnormal in a given brain region. To create such a normative map, we need to draw on a large and diverse cohort of subjects and assess their healthy tissue to estimate the expected power. This approach has previously shown success in the context of intracranial EEG and epilepsy (43, 3), but was limited to assess short-term signal properties. Future work should extend this line of work into ultradian and circadian rhythms.\n\nFinally, a key limitation was our analysis of the ultradian rhythms. Due to the lack of a central pacemaker, ultradian rhythms are extremely variable between subjects, and possibly also over longer time periods. Our coarse grouping of these rhythms is inspired by literature, but not data-driven. Our results in this context should thus be interpreted as a lack of fluctuations on timescales below one day in pathological tissue, rather than any specific rhythmic activity being diminished. Future work should investigate these fluctuations from the perspective of episodic, but most likely not strictly rhythmic events (13).\nIn summary, pathological brain regions show weakened chronobiological rhythms. At present, the causal direction of this association is not clear, but the effect is independent of seizure occurrence and brain region. These findings encourage future research to consider chronobiological rhythms in the development of disease models and treatments.\n4 Methods\n\n4.1 Preprocessing of long-term iEEG recordings\n\nWe analysed long-term iEEG recordings from 38 subjects with refractory focal epilepsy from the National Hospital for Neurology and Neurosurgery (Table 1). For each subject we processed their entire available iEEG recordings. Firstly, we divided each subject’s iEEG data into 30 s non-overlapping, consecutive time segments. All channels in each time segment were re-referenced to a common average reference. In each time segment, we excluded any noisy channels (with outlier amplitude ranges) from the computed common average. To remove power line noise, each time segment was notch filtered at 50 Hz. Finally, segments were band-pass filtered from \\(0.5 - 80\\) Hz using a 4\\textsuperscript{th} order zero-phase Butterworth filter (second order forward and backward filter applied) and further downsampled to 200 Hz. Missing data were not tolerated in any time segment and denoted as missing for the downstream analysis.\n\nWe then calculated the iEEG band power for each 30 s time segment for all channels. We extracted iEEG band power from 30 s non-overlapping iEEG segments in five frequency bands (\\(\\delta : 1 - 4\\) Hz, \\(\\theta : 4 - 8\\) Hz, \\(\\alpha : 8 - 13\\) Hz, \\(\\beta : 13 - 30\\) Hz and \\(\\gamma : 30 - 47.5\\) Hz, \\(52.5 - 57.5\\) Hz, \\(62.5 - 77.5\\) Hz) using Welch’s method with 3 s non-overlapping windows. In detail, for each channel in every 2 s window we calculated the power spectral density (PSD) and used Simpson’s rule to obtain the band power values which then averaged over all time windows within a 30 s segment to get the final band power values. In order to remove electrical noise, we selected custom range limits for the gamma frequency band. We \\(log_{10}\\)-transformed and normalised the band power values to sum to one for each 30 s segment. We then averaged over the relative log band power of all electrodes included in each ROI, thus obtaining, for each subject, one matrix of relative log band power at the ROI level for each frequency band (of size number of ROIs by number of 30 s segments).\n\nIn the majority of resulting relative band power matrices had missing data, which we imputed (Suppl. S1) to enable extraction of rhythms and their time-varying characteristics, such as instantaneous frequency and amplitude. Imputed data were not used for subsequent analysis, and\nsegments with imputed data were blanked after extraction of rhythms.\n\n4.2 Extracting chronobiological rhythms using bandpass filter\n\nTo extract rhythms of various timescales from the relative log band power, we performed a 4th order zero-phase Butterworth filter (second order forward and backward). Within each subject, we extracted ultradian rhythms in different period bands (1h-3h, 3h-6h, 6h-9h, 9h-12h, 12h-9h). Finally, we denoted a circadian rhythm with period length of 19h-1.3d.\n\n4.3 MRI processing for identifying regions and resected tissue\n\nTo map electrode coordinates to brain regions we used the same methods as described previously (44). In brief, we assigned electrodes to one of 128 regions from the Lausanne scale60 atlas (16). We used FreeSurfer to generate volumetric parcellations of each patient’s pre-operative MRI (16, 8). Each electrode contact was assigned to the closest grey matter volumetric region within 5 mm. If the closest grey matter region was >5mm away then the contact was excluded from further analysis.\n\nTo identify which regions were later resected, we used previously described methods (42, 43). We registered post-operative MRI to the pre-operative MRI and manually delineated the resection cavity. This manual delineation accounted for post-operative brain shift and sagging into the resection cavity. Electrode contacts within 5mm of the resection were assigned as resected. Regions with >25% of their electrode contacts removed were considered as resected for downstream analysis.\n\n4.4 Determining if chronobiological rhythms are diminished in pathological tissue\n\nIn order to quantify the strength of each band power chronobiological rhythm at the ROI level for each subject, we computed the average power of each rhythm obtained from the bandpass filtered signal. In order to compare the strength of each rhythm between pathological and healthy tissue, we computed the area under the curve (AUC). AUC values higher than 0.5 indicate diminished band\npower rhythms in pathological tissue, while AUCs lower than 0.5 indicate diminished band power rhythms in spared ROIs and finally \\( \\mathrm{AUC} = 0.5 \\) indicates no discrimination between pathological and healthy tissue.\n\nWe used the clinically identified regions where seizures originate (seizure onset zone, or SOZ) as a proxy for pathological tissue. To ensure robustness of our results, we also used the alternative definition of the tissue that was subsequently surgically removed, as it was deemed central to generating epileptic seizures. We obtained similar results (Suppl S5) with either definition, and will use the broad term of “pathological tissue” throughout the paper to refer to tissue that is most likely functionally (causing seizures) and/or structurally pathological.\n\n4.5 Fitting a mixed effects model to control for brain area\n\nTo show that pathological tissue predicted diminished rhythms above any brain area specific effect, we fit a mixed effects model predicting the rhythm power in a given ROI from a categorical variable representing lobe within which the ROI resides, and whether that ROI was pathological, grouping by a random patient offset. Equation 1 describes the model, where \\( RhythmPower_{i,j} \\) is the power of the rhythm for patient \\( i \\) in ROI \\( j \\), \\( \\beta_0 \\) is the fixed intercept, \\( \\beta_1 \\) is the fixed effect for pathological ROI, \\( Path_{i,j} \\) is a binary variable indicating that ROI \\( j \\) of patient \\( i \\) is pathological, \\( \\beta_{2..7} \\) is the fixed effect of the region being in each lobe - a categorical variable with 7 levels corresponding to the x axis of figure 3 (a), \\( Lobe_{i,j} \\) indicates whether ROI \\( j \\) of patient \\( i \\) is in each lobe, \\( u_i \\) is the random intercept for patient \\( i \\), and \\( \\varepsilon_{i,j} \\) is the error. Regions were grouped into 7 possible lobes/areas: frontal, temporal, parietal, occipital, cingulate, hippocampus, amygdala. The dependent variable (rhythm power) was standardized before fitting to give partially standardized coefficients, allowing us to interpret \\( \\beta_1 \\) as the expected effect of pathology on rhythm power (in standard deviations) (25). A likelihood ratio test was used to assess whether the effect of pathology was statistically significant - comparing to a reduced model without pathology as a variable. Maximum likelihood estimation was used in the fitting of models, with Python (3.8.10) alongside the statsmodels library (0.14.0) and its MixedLM function providing the software.\n\\[\nrhythmPower_{i,j} = \\beta_0 + \\beta_1 hasPath_{i,j} + \\beta_{2..7} Lobe_{i,j} + u_i + \\mathcal{E}_{i,j}\n\\] (1)\n\n4.6 Code and data availability\n\nAll analysis was performed using Python (version 3.8) and MATLAB (version R2023a).\n\nCode used in analysis is available at: https://github.com/cnnp-lab/DiminishedRhythmsPathology\n\nData used in analysis is available at: https://zenodo.org/record/8289342\n\n5 Acknowledgements\n\nWe thank members of the Computational Neurology, Neuroscience & Psychiatry Lab (www.cnnp-lab.com) for discussions on the analysis and manuscript; P.N.T. and Y.W. are both supported by UKRI Future Leaders Fellowships (MR/T04294X/1, MR/V026569/1). 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Intrinsic brain dynamics in the Default Mode Network predict involuntary fluctuations of visual awareness\n\nDian Lu\nUniversity of Cambridge\nEmmanuel Stamatakis (eas46@cam.ac.uk)\nUniversity of Cambridge https://orcid.org/0000-0001-6955-9601\nShruti Naik\nCognitive Neuroimaging Unit, INSERM, CEA, Universite' Paris-Saclay\nDavid Menon\nUniversity of Cambridge https://orcid.org/0000-0002-3228-9692\n\nArticle\n\nKeywords: cognition, brain activity, consciousness\n\nPosted Date: July 13th, 2021\n\nDOI: https://doi.org/10.21203/rs.3.rs-646785/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: There is NO Competing Interest.\n\nVersion of Record: A version of this preprint was published at Nature Communications on November 14th, 2022. See the published version at https://doi.org/10.1038/s41467-022-34410-6.\nPerturbation or Function? Intrinsic brain dynamics in the Default Mode Network predict involuntary fluctuations of visual awareness\n\nDian Lyu1,2, Shruti Naik4, David K. Menon1,3, Emmanuel A. Stamatakis1,2*\n\n1University Division of Anaesthesia, University of Cambridge, Addenbrooke’s Hospital, Hills Rd, CB2 0SP Cambridge, UK\n2Department of Clinical Neuroscience, University of Cambridge, Addenbrooke’s Hospital, Hills Rd, CB2 0SP Cambridge, UK\n3Wolfson Brain Imaging Centre, University of Cambridge, Cambridge Biomedical Campus (Box 65), CB2 0QQ, Cambridge, UK\n4Cognitive Neuroimaging Unit, INSERM, CEA, Universite’ Paris-Saclay, NeuroSpin centre, 91191 Gif/Yvette, France\n\n*To whom correspondence should be addressed; E-mail: eas46@cam.ac.uk\n\nAbstract\n\nBrain activity is intrinsically organised into spatiotemporal patterns, but it is still not clear whether the intrinsic dynamical patterns are functional or epiphenomenal. Using a simultaneous fMRI-EEG implementation of a well-known bi-stable visual task, we showed that the latent transient states (~100-ms) in the intrinsic EEG oscillations can predict the upcoming involuntarily perceptual transitions. The critical state predicting a dominant perceptual transition was characterised by the phase coupling between the precuneus (PCU), a key node of the Default Mode Network (DMN), and the primary visual cortex (V1). The interaction between the lifetime of this state and the PCU->V1 causal effect is correlated with the rate of perceptual fluctuation. Our study suggests that the brain’s endogenous dynamics are phenomenologically relevant, as they can trigger a diversion between potential visual processing pathways, while external stimuli remain the same. In this sense, the intrinsic DMN dynamics pre-empt the content of consciousness.\nIntroduction\n\nBeing aware is believed to be a globally “illuminated” inner state when locally encoded information gets propagated through downstream pathways and becomes accessible to other processing streams in the brain (1). However, the mechanism of the propagation process is largely unknown. Recent theoretical developments in brain dynamics suggest that the spontaneous information propagation may be empowered by the intrinsic ignition of neural activity (2). Empirically, intrinsic brain activity has been extensively studied during resting state when no external stimuli are presented to participants. At rest, neural activity from certain distant regions is correlated forming what are known as large-scale networks (3). We know that external perturbations can interrupt or bias the global cascades of information propagation (e.g. visual masking and priming). One untested hypothesis is that this process can also be influenced by intrinsic perturbations that originate from “background” dynamics of large-scale brain networks (2). To test this hypothesis, we used a simultaneous fMRI-EEG implementation of the well-known Binocular rivalry (BR) paradigm to investigate whether and how intrinsic brain activity of a large-scale brain network influences the involuntary perceptual fluctuations during bi-stable visual awareness.\n\nBR is a robust visual phenomenon where the participant perceives continuously alternating images even though the visual stimuli presented to the viewer, remain the same. To successfully trigger this phenomenon, dissimilar images need to be presented to the two eyes (one eye’s view is blocked from the other); and to ensure balanced representations of the two images (or “percepts” as we shall call them in this paper), the two images should be distinguishable but of comparable cognitive load. Behavioural studies have established that the alternation of the two percepts is stochastic and beyond the participant’s volitional control, but it is not random: duration of each percept follows a log-normal probability distribution (4) and on average differs notably from person to person (5). BR has been a popular paradigm for researchers aiming to study visual awareness as well as the neural correlates of consciousness (NCCs) (6–8). The classical model for explaining this phenomenon is called the (general) mutual inhibition model (MIM), which takes the form of a non-linear dynamic system (9). Although the model can have many variations in terms of the configurations of the local neural circuitry for inducing the counterbalancing mutual inhibition (9), it generally requires mutually inhibitory neurons encoding the representations of the two images (which exist as attractors in the model), and\npossible sources of perturbations, i.e., global and/or local adaptation of the neuronal populations as well as neuronal noise (10–13). A dominant percept during BR can be considered as a stable state/equilibrium achieved by the neuronal activity settling in one of the two possible attractors (13), while the state can escape from the current attractor under the influence of noise or habituation processes (such as spike frequency adaptation and synaptic fatigue) (9, 11, 13). The MIM has been successful in fitting behavioural data measured during experiments, but empirical neural evidence to support the model is still lacking (14). In fact, this explanatory framework only focuses on the dynamics of the local neural circuitry, but totally ignores the background neural dynamics. However, the intrinsic dynamics of brain networks may have a lot of interactions with, and by which modulate, the activity of the local sensory region (1, 15).\n\nIntrinsic brain activity is not random, instead, it is spatiotemporally organised into specific reproducible states (16–19). Although the spatial patterns of large-scale networks are mostly derived from unconstrained resting state, they can be identified across different tasks as well, possibly serving as a scaffold for various brain processes (3, 20). One of the large-scale networks that has achieved a prominent position in recent literature is the default mode network (DMN) (21). The DMN encompasses a wide range of associative regions across the prefrontal, temporal and parietal lobes, and consumes a major part of the brain’s energy budget (22). A functional gradient analysis suggested that the DMN is situated at the top of the brain’s information processing hierarchy, where multi-modal sensory information is integrated and highly abstract information (such as a concept of “self”) is formed (23). Dynamic neural state studies using Hidden Markov models have shown that DMN activity dominates the latent brain states which are characterised by the synchronisation of high-order cognitive networks; where latent states are defined as recurring transient states that are assumed to drive the observed global neural dynamics (16, 19). Using control theory, it was also suggested that the DMN regions have the highest capability of steering the whole brain from one state to another, given the structural architecture of the brain (24).\n\nClinical studies have already highlighted the significance of the DMN in consciousness (25–27), but little work has been done to investigate the role of the DMN in visual awareness, even though the bi-stable visual phenomenon is a classic experimental paradigm for investigating the NCCs (6–8). There has been some suggestion in the literature that the DMN may play a role in BR. In many fMRI/EEG studies utilising the BR paradigm, frontal and parietal regions have been reported to be\nengaged (28–31), some of which may overlap with DMN subregions, especially in the parietal cortex where high-level cognitive networks mostly converge (32). A hypothesis of the DMN’s involvement in the BR task seems to be contradictory to its frequently attributed role of “task-negative”, a characterisation that originated from its discovery where its activity at rest was found to be higher compared to a cognitively demanding task conditions (22). However, the perceptual experience during BR is no more cognitively demanding than the control condition which is usually a normal viewing condition. In addition, there has been substantial evidence showing DMN engagement in tasks, suggesting that contribution to cognitive function from areas that make up the DMN is still not well understood (33–35). Therefore, here we aim to confirm the DMN’s involvement during BR before answering how it exerts an influence; this constitutes the first part of the study. In fact, a recent fMRI study using ambiguous images as stimuli to study pattern disambiguation has established a role for the DMN in prior-guided visual perception (36), which suggests that the DMN is involved in the online modulation of visual processing and its function may perhaps be associated with perceptual disambiguation.\n\nGiven the DMN’s role in global cortical dynamics and conscious representation, we hypothesised that the intrinsic DMN dynamics may have some influence on the involuntary perceptual fluctuations during BR, possibly by causing perturbation to the equilibrium of the current dominant percept.\n\nResults\n\nBehavioural analyses\n\nFor maximally eliciting BR perception, the experiment used stimuli of rotating green and red checkerboard images, which were presented to each eye simultaneously with the order counterbalanced across individuals. In a perceptually matched Replay (RPL) condition where no BR is elicited, the same rotating images of the red or green checkerboard were presented to both eyes at the same time, but they alternated in time (Fig. 1a, d). Participants were asked to instantaneously report their percept by using three different buttons, respectively for the (dominant) red or green percept, and the mixed percept i.e. a transitional phase between the red and green percept. Therefore, this paradigm had a 2×2 factorial design of dominant and mixed perception types for the BR and RPL conditions.\nIndividual difference of the percept duration during BR was significant (Fig. 1b) (reduced-RSS=1490, p = 0.00 by a \\( \\chi^2 \\) test; we also adopted the Akaike Information Criterion/AIC for statistical inference, which was decreased by 1057.5, suggesting stronger model evidence for a model considering individual differences compared to the one without it). The duration of (dominant/mixed) percept formed a heavy-tailed distribution (skewness=1.29, kurtosis=2.89 for dominant percept; 3.15 and 17.82 for mixed percept), and the dominant percept (median=2.22 seconds for the red and 2.04 for the green) was significantly longer (decreased AIC/dAIC = 7985) than the mixed percept (median=0.33) (Fig. 1c). Although stimulus colour seemed to be able to slightly influence perceptual duration according to the statistics, we do not explore this effect further and refer to the stable perception for both colours as the dominant percept. In fact, a subsequent fMRI contrast did not reveal significant activation difference between red and green percept.\nFig. 1. Experimental design with 2-by-2 conditions of different percepts and ways of percept generation (a) Experimental schema adapted from the original study (37) from which the data was shared. During the binocular rivalry (BR) blocks (left), the participants were presented with different images, each for one eye, in the centre of the visual field. During the replay (RPL) blocks (right), the participants were presented with the same image for both eyes, but this image alternates over time between red, green via a short superimposition, in order to simulate the experience in the BR condition. Both conditions can generate alternating percept of the dominant (red or green) and the transitional mixed images, however the perceptual alternation was generated endogenously in the BR condition while it was exogenously elicited in the RPL condition. (b) Individual difference in percept duration (s) for different percept types in the BR condition.\n(c) Distributions of percept duration in the BR condition. (d) Percept duration for different percepts in the RPL and BR condition.\n\nFMRI activation study\n\nIn agreement with the previous literature (30, 31), we found significantly activated regions in the cuneus, the intraparietal sulcus/inferior parietal lobule (BA40), angular gyrus (BA39) and inferior frontal gyrus (BA47), for the contrast of BR (dominant) > RPL (dominant). We also replicated the finding of the deactivation in the posterior (mid-) cingulate cortex (BA31) upon a report of mixed percept during BR, which was referred to as “perceptual transition” in the original paper where the data was shared from (37). As suggested by the meta-analysis driven BrainMap network atlases, a large portion of the significantly activated regions over- lapped with the DMN, supporting our hypothesis about the DMN’s involvement in the task (see a full report of significant clusters in the Supplementary Materials). Here we highlight an F- contrast for the 2-by-2 interaction effect: 2 perception types (dominant vs. mixed) × 2 ways of perception generation (BR vs. RPL), which revealed the DMN and visual cortex having the most variable activation patterns among the four conditions (Fig. 2). Our subsequent dynamic analysis will mostly focus on these regions.\nFig. 2. ICN affiliation of the fMRI activated regions as revealed by the interaction effect. The interaction analysis reveals the regions whose activity is most sensitive to the four conditions, i.e. the regions mostly engaged by the experiment paradigm. The brain activation maps indicate the significant regions that showed an interaction effect among the 4 conditions, passing the cluster-level threshold of 0.05 (family-wise error corrected/FWE-corr) upon an F test (two-tailed). ICN involvement is a measure of correspondence between an activation map and large-scale networks with well-established cognitive function. The spatial correspondence is supported by the BrainMap meta-analysis database (38).\n\nEEG evoked responses and source reconstruction\n\nThe EEG recording with its excellent temporal resolution gave us the opportunity to better locate the neuronal cause of a perceptual change by looking into a short time interval right before the perceptual change. Permutation cluster tests on the Global Field Power (GFP) of the perceptual conditions revealed that the most eventful epoch was between [-400-200] ms, which was when the EEG sensor voltages differed the most between the endogenously (BR) and exogenously (RPL) generated dominant percept (permutation cluster test on the time-window [-500, 0] ms, p<0.05) (Fig. 3a). We observed no significant difference for mixed percept between the BR and RPL conditions during the same temporal window (Fig. 3b). Further 2-way ANOVA analysis in this time-window revealed a significant main effect of the source of perceptual transitions (F(1, 19) = 4.70, p = 0.04), but no significant main effect of perceptual types\n(mixed or dominant) was found (F(1, 19) = 0.29; p = 0.59). Although there was a noticeable trend of interaction effect between the source of perceptual transitions and the perceptual type, the test was not significant (F(1, 19) = 2.63; p = 0.12) (Fig. 3c). The event-related potential (ERP) topographies during the [-400 -200] ms time window for the dominant percept in both conditions are shown in the Fig. 3d.\n\nTo discover the brain location of the signals that generated this scalp topological difference, we then conducted source reconstruction for the ERPs during this time window. The source reconstruction indicated that the topology was driven by a deactivation in the posterior cingulate cortex (PCC; BA23/24), precuneus (PCU; BA31/7m), thalamus, insula, caudate, claustrum and the fusiform gyrus (BA20) during BR (dominant) vs. RPL (dominant) condition (full results presented in the Supplementary Materials). An F contrast during this time window for the interaction effect of the 4 conditions revealed the following regions: insula (BA 13), postcentral gyrus (BA 43), thalamus, parahippocampal gyrus (BA 34), PCC (BA30), inferior frontal gyrus (BA 47) and anterior cingulate cortex (ACC) (Fig. 3e). See supplementary materials for a full report of significant regions, including relevant statistics and the results for other contrasts, which were classified into finer grained frequency bands and time windows.\nFig. 3. Event-Related Potentials for different perceptual conditions. (a) Event-Related Potentials for different perceptual conditions at the sensor level. The global field power (GFP) in the replay condition was significantly higher than that in BR condition from 400-200 ms before the report (at the 0 s) of change in percept (black line: p < 0.05 significant clusters, 1-sample permutation cluster t-test). (b) No significant difference in the overall GFP during mixed percept between the BR and RPL conditions. (c) GFP difference across sources of perceptual transitions and types of percept. There was a significant main effect of the source of perceptual transitions (BR/RPL) (2-way ANOVA, p <0.05). (d) ERP topographies for dominant percept in both of the BR and RPL conditions, and the contrast between them. (e) The localisation of (relative) evoked responses at the source level, contrasted between BR (dominant) and RPL (dominant) conditions, and for the interaction effect of the two variables.\n\nThe EEG evoked response and the BOLD response for the interaction effect with the experimental conditions largely overlap in the ACC, PCC, inferior frontal gyrus and the precentral gyrus. However, cuneus (BA18), extrastriate cortex (BA19) and posterior parietal cortices (PPC; BA39/40) only showed an interaction effect in the BOLD response but not in the EEG evoked response. This might be due to the fact that the EEG evoked response captured the moment before the participant’s explicit response for a perceptual change, while the fMRI activation should be mainly driven by the effect after the perceptual change. During the pre-response window for an immediate perceptual change, the visual\npercept might not have actually changed, so no significant cross-condition difference in the EEG evoked response was found in the visual areas, nor should there be a change of attention level (as indicated by the PPC BOLD activity) yet in this time. But an elevated level of attention could be caused by a change of perception by the time the participants already reported a perceptual change, and this might be what the fMRI activation in the occipital and posterior parietal cortices represented.\n\nHidden neural states within DMN can predict upcoming perceptual transitions\n\nThe previous evoked-response analysis showed that the biggest difference between BR and RPL conditions happened right before (~1 second) perceptual transitions. However, the evoked response of the GFP is a crude measure as it is a grand average across all trials and all channels. To uncover the dynamic patterns embedded in the EEG signals on a trial-by-trial basis, we adopted the embedded-lag HMM method (https://github.com/OHBA-analysis/HMM-MAR) which takes advantage of the excellent temporal resolution and rich spectral profiles of the EEG data. If the intrinsic fluctuation of the DMN regional activity influences the perceptual transitions during BR, we should expect to find a correspondence between the temporal dynamics of DMN regions and the upcoming perceptual transitions. To increase the sensitivity of the method as well as to avoid overfitting, we constrained our regions of interest to those which were shown to be significantly engaged in the experiment by the source-level evoked EEG activation contrasts between experimental conditions. These regions were DMN key regions, including bilateral parahippocampal gyri (HP), bilateral inferior parietal lobules (IPL), ACC, PCC, PCU, and the primary visual cortex (V1) (a full list of the regional coordinates where the signals were extracted is presented in the Supplementary Table 1). We targeted our dynamic analyses at the temporal window of the second (with 0.1-s post-response padding) before every perceptual transition as a trade-off between having enough sample points and having enough specificity for the targeted events.\n\nWe set the HMM algorithm to extract 4 states from the data, which are the concatenated regional signals of all trials from all conditions and subjects (Fig. 4). We chose 4 states because firstly we were interested in the differences of the neural activity among the four experimental conditions, supposing that the differences can be captured by the most salient four components in the variance of the data;\nand secondly, 4 components have often been chosen for discovering the EEG microstates in existing literature (39), and were shown to have correspondence with the ICN dynamics measured from the BOLD signals (40). These data-driven states were then examined and compared between the four experiment conditions. The resulting auto-covariance patterns of the 4 states are presented in the supplementary materials (sFig. 5). All of the comparisons were carried out within subjects and the difference was then grouped together for the population-level inference.\nFig. 4. Schematic illustration of the procedures for HMM. The one-second EEG epochs/trials were taken right before every perceptual change (“dominant” in red or green, “mixed” in black). To ensure experimental sensitivity, we select our regions of interest (ROI) from the significant results of the sensor-level evoked response in our previous analyses. Also because of our theoretical interest, we further constrained our selection of ROIs by choosing only the V1 and DMN regions to construct the HMM. Across all the experimental conditions, signals from significant peak voxels within the same ROIs were averaged for being used as the regional signal. The anatomical labels for the peak coordinates were identified with the Talairach Atlas (http://www.talairach.org/daemon.html), upon a conversion to the Talairach space. Full lists of the peak voxel coordinates used for this purpose are presented in the supplementary material.\n\nWe firstly compared the states’ dynamics features, such as the switching rate (SR), i.e. the rate of state switches which can be understood as a measure of state stability, and the fractional occupancy (FO), i.e. the proportion of dwelling time on a certain state given a period of time. The SRs were not different across conditions, except that the RPL (mixed) had significantly higher SR than the rest (t=3.57, p-adj=0.00 vs. BR (dominant); t=3.30, p-adj=0.00 vs. BR (mixed), and t=3.00, p-adj = 0.01 vs. RPL (dominant)). The fact that the SRs were about a quarter each suggested that there was a good mix of the presence of the 4 states, meaning the 4 states had been separated well for capturing the multi-dimensional variance in the data.\n\nImportantly, we found that the four states’ FO was significantly different among the conditions (p=0.00, dAIC=147.45). To establish exactly how the states’ FO differed (Fig. 5a), permutation tests\nwere conducted within each experimental condition for state-wise comparisons (with 2000 permutations for simulating a null distribution of the state-wise differences). It turned out that the states can discriminate conditions, in a way that a unique state was always visited mostly during one specific condition (Fig. 4b). This pattern was most noticeable in the BR (dominant) and RPL (mixed) conditions, where respectively *State 4* and *State 1* clearly stood out, with significant median differences of 0.44 (p-*adj*=0.00), and 0.36 (p-*adj*=0.00) to the second most prominent state in their respective conditions. Similarly, in the RPL (dominant) and the BR (mixed) condition, *State 2* and *State 3* were respectively visited the most, nevertheless they were not visited significantly more often than the second most prominent state.\n\nWe reflected on the reason why the RPL (dominant) and BR (mixed) conditions did not generate a single state as significantly dominant as was the case in the other two conditions. This might be explained by the idiosyncrasies of the perceptual compositions in some of the trials, given the nature of the experiment. In this experiment, the mixed percept can be seen as an ending phase of the last dominant percept, and a starting phase of the next one, and it is much shorter (~0.5 s on average) than its adjacent dominant percept (~2 s) (Fig. 1c,d). For data analyses, we extracted uniformly 1-s time windows before any perceptual switches to ensure equal (in terms of duration) data-points for the analysis. Therefore, the 1-s window before a dominant percept may cover periods of perceptual fluctuation, including the transitional mixed percept that is meant to be captured, and the residual of dominant percept from the last trial. The potential perceptual fluctuation in these trials could have confounded the RPL (dominant) condition, but it may not be a problem for the BR (dominant) condition. Because in RPL (dominant) condition, a perceptual switch was controlled by an external cause, as the images were designed to alter stochastically by the experimenters. By comparison, perceptual alternations in the BR conditions were generated endogenously, so the transient perceptual instability before may be considered as leading to a next dominant transition. Therefore, despite the BR (dominant) trials could contain perceptual fluctuation, the fluctuating percepts may be driven by same neural causal power and thus can be treated as common factors.\n\nTo validate the point that the continuity of the causal power in the neural activity is what sets the BR condition apart from the RPL condition, we further conducted a cross validation (CV), using the trial-by-trial FOs of the hidden neural states to predict the type (mixed or dominant) of the upcoming transition. This was done respectively for the BR (endogenous) and RPL (exogenous)\nconditions. As a result, the accuracy score for the BR condition was 92.01% (SD = 4.68%), which was higher than the score of 82.16% (SD = 9.14%) for the RPL condition (see the Supplementary Material sFig. 15 for more details). This suggests that these neural states we found in a purely data-driven way, actually contain the causal power for predicting the endogenously driven perceptual changes. In addition, according to the state FOs for each of the conditions, there was a mirrored difference between the BR and RPL conditions. Namely, *State 4* was visited distinctively the most in the BR (dominant) condition, but it was visited the least in the RPL (dominant) condition. Therefore, *State 4* seems to be key to the intrinsic neural cause of the spontaneous perceptual fluctuation during BR.\nFig. 5. Correspondence between states and conditions (a) Different fractional occupancy (FO) of the four states across conditions. Plotted data are the mean FO values averaged across trials for each individual, grouped by the two categorical variables: conditions and states. FDR-adjusted p-values of pair-wise permutation tests are presented on the significance bar on top of the compared groups. The distributions of non-averaged FO for all trials/epochs of all participants are presented in supplementary materials (sFig. 8). For the box plots, the white mark on each box indicates the mean, while the length of the box indicates quantiles with the middle bar showing the median. (b) Radar chart showing the correspondence between conditions and states. Scales on the radar chart indicate the median values of the state FO in the corresponding condition. (c) Spectral information of the states in the Alpha band. Diagonal and off-diagonal values of the upper-triangle heatmaps respectively indicate the power and phase coherence of the ROIs. The asterisk on the heatmap indicates that the phase coherence (or power) in this state is significantly higher (yellow) or lower (blue) compared with the other states (one-tailed test with the 95% confidence interval by permutation). The circular bundle plots below highlight the significant connectivities, with red and blue respectively signifying higher and lower significance for the connectivity. All of the connectivities (whether significant or not) are also mapped onto standardised brain anatomy from the left, right, back and top views (clock-wise), where the colour intensity of the connectivity has been normalised across all states, thus being suitable for visual state-wise comparisons. Coordinates of the nodes were selected based on significant peaks from the previous evoked-response analyses (See the Supplementary Table 1 for all of the peak coordinates).\nPCU-V1 phase coherence and Granger Causality predicts stable percepts\n\nTo unravel the neuronal signatures encapsulated in the states, we then extracted the spectral information (power and phase coherence) from the multivariate auto-covariance matrix of each state. Once we had estimated the power and coherence for each state, we factorised the frequencies into a few dominating components so as to facilitate interpretation with conventionally defined frequency bands. For that, we applied a non-negative matrix factorisation (NNMF) algorithm on the coherence matrix, concatenated across all states and ROIs and confined it to four components. The four components turned out to match traditional frequency bands: Theta (peak at 4 Hz, half- maximum at 1, 12 Hz), Alpha (peak at 11 Hz, half-maximum at 7, 15 Hz), Beta (peak at 20 Hz, half-maximum at 15, 34 Hz) and Gamma (peak at 34 Hz, half-maximum at 26 Hz) (sFig. 7 in supplementary materials). Therefore, we next focused into state-wise frequency- specific spectral information. As stated already, the data-driven states were indicative of the 4 experimental conditions (representing 4 kinds of perceptual experiences). We then looked into how each state is represented by the spectral features of the neural signals. To identify the characteristics of each state that stand out, we performed permutation tests for each power and coherence values, comparing across all 4 states (5000 permutations for each null distribution simulation; significance level is p<0.01) (Fig. 5c).\n\nFor a clear narrative, here we only focus on the Alpha band (peak at 11 Hz, FWHM = 8 Hz) of the states. Previous studies have shown that pre-stimuli alpha oscillations at posterior sensors can modulate subsequent processing and perception (41). In our study, the alpha band of the states also demonstrated an interesting pattern in the state-wise comparisons. Comparing the phase coherence among the ROIs across the four states (Fig. 5c), the one between PCU and V1 clearly stood out, as the PCU-V1 phase coherence was highest in State 4, an indicative state for the BR (dominant); and it was the lowest in State 2, an indicative state for the RPL (dominant) condition. This made us hypothesise that the PCU-V1 coherence may underlie the spontaneous transition to a stable percept.\n\nWe have presented the full results of other frequencies in the supplementary materials (sFig. 10-12). For the other frequencies, we would like to only point out the general increase of the theta coherences among DMN regions in the BR (mixed) condition (i.e. during a dominant percept because the trial is extracted before a perceptual change), especially the increased theta coherence between\nACC and PCC, which is unseen in other frequencies. This corresponds to previous MEG literature where intrahemispheric and interhemispheric theta coherences were found to be increased during periods of perceptual dominance in BR (42). The strong ACC-PCC coherence that we only observed in the theta oscillations also corresponds to an earlier study using the same HMM method which showed that the mPFC/ACC-PCC coherence in the delta/theta model characterises the anterior higher-order cognitive state during resting state (19).\n\nPCU-V1 phase coherence and Granger Causality predicts stable percepts\n\nWe then investigated the behavioural relevance of the critical state we found: State 4. State lifetime (also known as dwell-time) was used as an intuitive index for the state presence, estimated as the time that elapsed between entering and exiting a state according to the HMM (43). We correlated it with the reaction time (RT) which was defined as the interval of the participant’s adjacent reports to perceptual changes. When the correlation is examined on the individual level (i.e., when the variance is provided by different performances across trials), the RT was the perceptual duration of the last percept; but when examined on the group level (i.e., variance provided by different average performances of the individuals), the individual- averaged RT reflected the alternation rate for that participant. We found that longer State 4’s lifetime could predict faster perceptual transitions (b = -0.38, t = -2.27, p = 0.03; dAIC = 35.03) at the group level.\n\nTo better understand the cognitive implication of the PCU-V1 coupling, which was a main feature of State 4, we further investigated the causal effect of the PCU to V1 and its relationship with behavioural measures. As we were agnostic to the nature of this hypothetical causal relationship, we adopted a simple form of causality to perform this analysis, namely, Granger Causality, which basically searches for a time-lagged linear relationship between x_1 and x_2 that can predict x_1 better than what x_1’s own auto-regression can predict (i.e., x_2 granger-causes x_1). In the BR literature, it is commonly believed that a switch of perception is caused by a slip of equilibrium due to neuronal noise, and/or the constant decay of suppression that one neural population has over the other, due to habituation effects (10, 11, 44). Apart from these, attention effects have also been shown to play a role (10, 45). Therefore, the PCU→V1 top-down modulation could reflect either an intrinsically evoked attention effect, or an effect of the global adaptation/perceptual habituation. These two possibilities would lead\nto opposite trial-by-trial predictions. The attention effect has been shown to speed up BR transitions, possibly by increasing the visual contrast of the percept (46). If the PCU→V1 modulation represents the attention effect, we can predict that the stronger the causal effect is, the quicker the transition becomes. Whereas, if the PCU→V1 modulation reflects the adaptation/habituation effect, longer duration of the last stable percept should cause a stronger adaptation (i.e. stronger PCU→V1 modulation) in the following trial.\n\nWe constructed statistical models according to the above hypotheses, but we did not find a trial-by-trial relationship between the GC(PCU→V1) and the perceptual duration. However, the two variables were correlated on the group level. Specifically, we found an interaction effect between the individual-averaged state lifetime (K=4) and GC(PCU→V1) for predicting the individual-averaged perceptual duration. In other words, the GC becomes more relevant to quicker perceptual transitions when the trial is visited by State 4 more (b=-0.39, t=-3.01, p=0.00 fitted with a generalised linear model; dAIC = 4.54 compared to a multiple regression model with no interaction). When State 4 dwells for the majority (>95%) of the trial time(i.e., >0.95s), the negative correlation between the GC and the perceptual duration was significant (b=-0.931, t=-2.821, p=0.017; dAIC=29.56) (All statistical models have been presented in the Supplemental Materials).\n\nThe GC(PCU→V1) may be interpreted as an averaged modulation effect of the PCU to V1during the 1-second window of concern. That only its interaction with the lifetime of State 4 is significant for predicting perceptual fluctuations suggests that: 1. The modulation effect of the PCU to V1 is perceptually relevant, but it alone is not sufficient for leading to a perceptual transition. A perceptual transition also depends on the presence of State 4, which consists of many other features over and above the PCU-V1 relationship (e.g. the phase coherence between PCC and V1 in the theta and beta band) which were not discussed in this paper and were presented in the supplementary materials sFig. 10-12); 2. The modulation effect of the PCU to V1 seems to be temporally accumulative along with the lifetime of State 4, suggesting that it needs to be built up and pass a certain threshold to take effect.\nFig. 6. (a) Lifetime of *State 4* can predict the length of intervals between perceptual changes during BR (for both dominant and mixed transitions). The longer *State 4* persists, the shorter the transitional period lasts, i.e. the quicker the rivalry is resolved. (b) shows that the duration of the last stable percept is correlated with the Granger causality (GC) effect from PCU to V1 on the group level. Their relationship is also dependent on the lifetime of *State 4*. The GC effect size was approximated by the improvement of model evidence (dBIC).\nDiscussion\n\nAwareness is suggested to emerge through the interactions between local processing triggered by external stimuli, and global broadcasting afforded by the brain’s intrinsic spatiotemporal states (1). Resting-state whole-brain signals are shown to be spatiotemporally organised (16), but it is still not clear whether this intrinsic architecture is epiphenomenal or functional. By using simultaneously recorded EEG-fMRI data, we showed that the brain’s spatiotemporal patterns or states found in this study, characterised by EEG oscillation patterns in the DMN regions, are phenomenologically relevant. We found that the four data-driven states are associated with the four perceptual experiences corresponding to the experimental conditions. The state indicating a dominant perceptual transition during the BR task was characterised by phase coupling between the precuneus (PCU) and the primary visual cortex (V1). We further found that the causal effect from the PCU to the V1 is a temporally cumulative effect along with the state lifetime of *State 4*; namely, the interaction of them is associated with the rate of perceptual transitions. Taken together, our results suggest that the brain’s intrinsic dynamics can influence visual awareness, possibly by triggering a diversion of the whole visual processing pathway.\n\nThere are a lot of controversies in existing literature regarding the sources of perceptual fluctuations during BR. Many advocate that the rivalry is resolved at the early visual stage, for example in the lateral geniculate nucleus or the primary visual cortex, probably due to sensory bottlenecks (47–49). But the contradictory argument is also convincing. Tong et al. (1998) using “face vs. house” binocular stimuli suggested that the rivalry continues from the retina, V1, V4 and MT, until it reaches the object-based processing step, i.e., the human fusiform face area and parahippocampal place area as exemplified in their study (50). It is also a well-known phenomenon that the BR alternation rate can be modulated by object features, emotional or semantic loading embedded in the stimuli as well as higher-level cognition such as working memory and attentional control (51). Therefore, many supported a top-down control hypothesis, which suggests that the observed activity in the early visual pathway is but an outcome of the feedback projections from higher-level areas, while those higher-level areas are where the NCCs actually lie (52, 53). According to them, the higher-level regions suppress unfavourable stimuli representation in the early visual pathway in order to maintain a congruent conscious experience (14). These high-level regions have been localised to frontoparietal\nregions by previous functional and structural MRI studies, including the frontal eye field, superior/middle/inferior frontal gyrus and superior/inferior parietal lobule (SPL/IPL) (54–56). Especially the right-lateralised SPL was suggested to play a causal role in the BR transition by a TMS study (54).\n\nDespite its plausibility, the top-down control hypothesis cannot explain the BR phenomenon fully. Firstly, it is difficult to dissociate the cause and effect of the BR perception in practice. Given the poor temporal resolution of fMRI, the frontoparietal regions revealed by fMRI activation studies might reflect an elevated level of attention drawn by a perceptual change during BR. The right lateralisation of the SPL, as often reported in the BR literature, suggests that it may get involved by association with attention (56). In a more recent BR study, when more accurate temporal information of perceptual transitions was provided, the significance of SPL disappeared (37). This also suggested that the SPL activity may be secondary to BR transitions, and that it might get involved via an attention effect which inevitably intertwines with involuntary perceptual change. Similarly, it has been argued that the involvement of the frontal regions during BR may also reflect introspection and action to perceptual transitions, rather than being a real cause (57, 58). Even if the involvement of the frontoparietal regions represents the endogenous attention which is necessary for gating visual awareness, it has been shown that attention is a dissociable factor to visual awareness; therefore, it is still arguable whether the frontoparietal regions associated with an attentional effect can be considered as a true NCC (6, 31, 59). Secondly, the top-down control hypothesis cannot explain why the perceptual transition keeps occurring when a stable percept has been reached. According to this hypothesis, the rival signal is suppressed in the early visual pathway so that the higher-level regions can maintain a meaningful representation of the environment; then under the condition of a stable percept already being achieved, it would not make sense for the neural activity to suddenly revolt and take another route.\n\nOur study provides a novel perspective as to why regular perceptual transitions may occur during BR. We highlight the possible influence of the temporal unfolding of the intrinsic large-scale cortical dynamics, which could bias the binocular signalling gains, perturb the current equilibrium, and eventually lead to a diversion of visual stream. Vidaurre et al. (2018) found that the intrinsic transient states exhibited in the posterior subdivisions of the DMN were characterised by high power and total coherence in the alpha (8-12 Hz) range (19). It was also suggested that pre-stimulus posterior\nalpha power can modulate primary visual processing, likely by re-shaping the functional architecture of the brain network when preparing for upcoming processing (41). These findings support our hypothesis that the DMN’s activity may serve as a source of “perturbation” to a bi-stable visual system during BR, thus introducing a bias towards what external information gets released from the overloaded visual channel. In our study, we revealed 4 states in the EEG signals from the DMN nodes and V1, during the one-second time window before a perceptual alternation. The 4 brain states, found in a data-driven way, turned out to be phenomenologically meaningful, for their differential presence during the “pre-onset” window could predict the different types of the upcoming perceptual transitions; and the lifetime of the critical state (*State 4*) correlates with the perceptual-alternation rate on the group level. The critical state we found also exhibits important features regarding the brain connectivity. One of the dominant features we followed up in this study is the phase coherence between PCU and V1 in alpha oscillations, as it seems to underlie the dominant perceptual transition in BR. Phase coherence measures the consistency of the phase differences between two waves across trials. If there are consistent phase differences between two sources across many trials, it means the two neuronal populations always discharge in a temporally coordinated manner, i.e. a signal coupling (60).\n\nAlthough the DMN and V1 are situated at the two opposite ends of the brain’s functional gradient (23), our result suggests that they may achieve signal coupling via the PCU. To further understand this signal coupling, we have also derived a Granger-causal effect of the PCU to V1 from their EEG signals at the same time windows. We found that, during the critical state, the stronger the top-down effect from the PCU to V1, the quicker the individual’s perception alternated. However, this relationship only existed on the group level, but not for trial-by-trial prediction; therefore, it only establishes the behavioural relevance of the causal effect of PCU to V1, but did not provide enough evidence for us to claim that the causal effect from PCU to V1 means either signal adaptation or suppression, as both could potentially lead to a trial-by-trial prediction. That neither state properties nor Granger-causality from PCU to V1 could predict trial-by-trial performance may just be due to a lack of statistical power; however, it could also be a true negative. Namely, the intrinsic brain dynamics may reflect more of individual-specific biological regularities, rather than “on-line” cognitive control. In fact, the influence of voluntary top-down control over BR is known to be limited (45, 61, 62); and BR has been reported to have notable inter-individual differences, depending on the individual’s gender, psychological predispositions, neurotransmitter levels and even handedness (5, 51). Twins and genome-wide association studies have showed that the individual differences in BR can be attributed to genetic\nfactors (63, 64). These suggest that BR may be bound to certain biological constraints of the brain’s general state, while participants’ involuntary top-down control over the BR rate as exemplified in previous studies (such as more intrinsic attention evoked by higher contrast of the image) might have exerted influence rather indirectly by altering the general state of the brain. Therefore, in spite of the PCU’s well-known cognitive relevance to visual-spatial imagery (65), we suggest that its role in BR transition does not necessarily correspond to voluntary cognitive processes, either attentional control or memory retrieval (62,66). Rather, the PCU-V1 coupling demonstrated in this study could be an indication of the intrinsic dynamics making “ripples” onto the primary visual cortex.\n\nFinally, we would also like to comment on the correspondence between the brain’s spatiotemporal dynamics and the phenomenological mental dynamics. With abundant empirical evidence and theoretical arguments, it has been suggested that the spatiotemporal patterns of neural dynamics are the instantiation of mental dynamics (17, 67). We also believe that the subjective experience is nothing more and nothing less than neural activities which are manifested at the mental level. But this does not necessitate the case that the emerged patterns in the physical domain (e.g. the spatiotemporal dynamics in neural signals) and those in our mental domain (e.g. human cognition) should have a linear mapping. Take our BR results for example, the transient states (short-lasting for 100 ms) we found in the 1-second period before a subjective report were the spatiotemporal patterns corresponding to the upcoming perceptual changes, but participants were typically not aware of any change before its sudden occurrence. This further made us reflect on the function of the DMN. Evidence has suggested that DMN is important for self-representation and consciousness (26, 68, 69), but its dynamical patterns of activity may not necessarily correspond to the person’s stream of consciousness in a simultaneous and linear fashion. 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All data needed to evaluate the conclusions in the paper are publicly available in the repository: (https://datadryad.org/stash/dataset/doi:10.5061/dryad.bflb1). Acknowledgements are given to the research team led by Bin He from the Department of Biomedical Engineering and Department of Psychology in the University of Minnesota for data collection and deposition; and Abhrajeeet V. Roy for the correspondence regarding to data clarification.\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• BinocularRivalrySI2.pdf\n• NCOMMS2124200rs.pdf"} {"paper_id": "prb17", "title": "Collisionless Relaxation of a Disequilibrated Current Sheet and Implications for Bifurcated Structures", "text": "Collisionless Relaxation of a Disequilibrated Current Sheet and Implications for Bifurcated Structures\n\nYoung Dae Yoon ( yyoon11@postech.ac.kr )\nPohang Accelerator Laboratory https://orcid.org/0000-0001-8394-2076\nGunSu Yun\nPohang University of Science and Technology (POSTECH) https://orcid.org/0000-0002-1880-5865\nJames Burch\nSouthwest Research Institute https://orcid.org/0000-0003-0452-8403\nDeirdre Wendel\nNASA Goddard Space Flight Center https://orcid.org/0000-0002-1925-9413\n\nArticle\n\nKeywords: Magnetic Phenomena, Phase-space Distributions, Single-particle Orbit Classes, Particle-in-cell Simulations, Bifurcated Current Sheets\n\nPosted Date: March 25th, 2021\n\nDOI: https://doi.org/10.21203/rs.3.rs-343769/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nVersion of Record: A version of this preprint was published at Nature Communications on June 18th, 2021. See the published version at https://doi.org/10.1038/s41467-021-24006-x.\nCollisionless Relaxation of a Disequilibrated Current Sheet and Implications for Bifurcated Structures\n\nYoung Dae Yoon*\nPohang Accelerator Laboratory, POSTECH, Pohang, Republic of Korea\n\nGunsu S. Yun*\nDepartment of Physics, POSTECH, Pohang, Republic of Korea\n\nDeirdre E. Wendel\nNASA Goddard Space Flight Center, Greenbelt, MD, USA\n\nJames L. Burch\nSouthwest Research Institute, San Antonio, TX, USA\n\nAbstract\nCurrent sheets are ubiquitous plasma structures that play the crucial role of being energy sources for various magnetic phenomena. Although a plethora of current sheet equilibrium solutions have been found, the collisionless process through which a disequilibrated current sheet relaxes or equilibrates remains largely unknown. Here we show, through analyses of phase-space distributions of single-particle orbit classes and particle-in-cell simulations, that collisionless transitions among the orbit classes are responsible for this process. Bifurcated current sheets, which are readily observed in geospace but whose origins remain controversial, are shown to naturally arise from the equilibration process and thus are likely to be the underlying structures in various phenomena; comparisons of spacecraft observations to particle-in-cell simulations support this fact. The bearing of this result on previous explanations of bifurcated structures is also discussed.\nI. INTRODUCTION\n\nCurrent sheets are structures generated by opposing magnetic fields and are ubiquitous in magnetized plasmas such as solar flares[1], the solar wind[2], the heliosphere[3, 4], and planetary magnetospheres[5, 6]. It is also deeply related to magnetic reconnection[7, 8], a process in which the energy stored in magnetic fields is converted to particle kinetic energies. Current sheets have thus been subject to extensive research, and a plethora of equilibrium solutions have been found both analytically[9–16] and numerically[17–20].\n\nHowever, there remains an important outstanding question regarding current sheet equilibria. Although various equilibrium solutions have been found, the collisionless process through which a disequilibrated current sheet equilibrates remains largely unknown. Such knowledge is crucial because plasmas in general do not start from equilibria, and also because it elucidates how a given system “wants” to evolve in time, even if it does not eventually equilibrate. In addition, the equilibria that have been found are specific solutions; a comprehensive understanding of the equilibration or relaxation process is necessary in order to place current sheets in a general context.\n\nA commonly observed form of current sheets is a bifurcated current sheet, which has two current density peaks on either side of the symmetry plane. These were first observed in the Earth’s magnetotail by Cluster spacecraft measurements[21, 22] and were initially deemed atypical. Later analyses, however, showed that bifurcated current sheets are actually extremely common, and that they were detected ~25% of the time Cluster was in the magnetotail current sheet[23, 24]. Since then, various explanations have been put forth, including flapping motion[25], magnetic reconnection[26, 27], temperature anisotropy[28, 29], Speiser motion[30], and non-adiabatic scattering of particles in a strongly curved magnetic field[16]. However, there is no consensus on the origin of bifurcated current sheets, which largely remains a mystery despite being readily observed even to this day[31–33].\n\nIn this paper, the collisionless relaxation process of an initially disequilibrated current sheet is studied. The process is shown in three steps. First, particle orbits in a magnetic field reversal are comprehensively categorized into four orbit classes. Second, the phase-space distribution of each orbit class and the role each class plays with respect to current sheet density, temperature, and strength are examined. Finally, with the aid of particle-in-cell simulations, it is shown that transitions among the orbit classes are responsible for\ncollisionless current sheet relaxation. The final equilibrium is most naturally understood in terms of the relative population of the phase-space distributions of the four orbit classes, instead of closed-form functions such as a Maxwellian.\n\nThe bearing of this process on the origin of bifurcated current sheets is then discussed. Two of the orbit classes necessarily exhibit spatially bifurcated structures, and so such structures naturally arise as a current sheet evolves towards equilibrium via orbit class transitions. An exemplary equilibrium from particle-in-cell simulations is compared with Magnetospheric Multiscale (MMS) measurements of an electron-scale current sheet, and their profiles are shown to agree well. The relevance of the relaxation process to previous explanations of bifurcated current sheets is also discussed.\n\nII. RESULTS\n\nParticle Orbit Classes Let us first examine single-particle dynamics in the renowned Harris current sheet[9], which is chosen as the system of scrutiny in the present study. It is described by the following magnetic field profile and distribution function \\( f_\\sigma \\) for species \\( \\sigma \\) (\\( i \\) for ions and \\( e \\) for electrons):\n\n\\[\n\\mathbf{B}(x) = \\hat{y} B_0 \\tanh \\frac{x}{\\lambda}.\n\\]\n\\[\nf_\\sigma(x, \\mathbf{v}, t) = \\left( \\frac{1}{2 \\pi v_{T\\sigma}^2} \\right)^{3/2} \\frac{n_0}{\\cosh^2(x/\\lambda)} \n\\times \\exp \\left[ -\\frac{1}{2 v_{T\\sigma}^2} (v_x^2 + v_y^2 + (v_z - V_\\sigma)^2) \\right],\n\\]\n\nwhere \\( B_0 \\) is the asymptotic value of the magnetic field, \\( \\lambda \\) is the sheath thickness, \\( n_0 \\) is the sheath peak density, and \\( v_{T\\sigma} = \\sqrt{k_B T_\\sigma / m_\\sigma} \\) is the species thermal velocity where \\( T_\\sigma \\) and \\( m_\\sigma \\) are respectively the species temperature and mass. \\( V_\\sigma \\) is the species’ mean velocity in the \\( z \\)-direction, i.e., its drift velocity. It is also assumed that \\( T_i = T_e := T \\) and \\( V_i = -V_e := V \\); the latter can always be made true by choosing a frame of reference where the electrostatic potential \\( \\phi = 0 \\). Two conditions must be true in order for this system to be an exact solution of the stationary Vlasov equation: (i) \\( B_0 = 2 \\sqrt{\\mu_0 n_0 k_B T} \\), which describes the balance between the peak magnetic pressure \\( B_0^2 / 2 \\mu_0 \\) and the peak thermal pressure \\( n_0 k_B (T_i + T_e) = 2 n_0 k_B T \\), and (ii) \\( \\lambda = \\lambda_D c / V \\) where \\( \\lambda_D = \\sqrt{\\epsilon_0 k_B T / n_0 e^2} \\) is the Debye\nlength and \\( c \\) is speed of light, which determines the equilibrium sheath thickness.\n\nThe vector potential is chosen to be \\( \\mathbf{A} = -\\hat{z}\\lambda B_0 \\ln \\cosh x/\\lambda \\). Normalizing length by \\( \\lambda \\), mass by the species mass \\( m_\\sigma \\), and time by \\( \\omega_{c\\sigma} = q_\\sigma B_0/m_\\sigma \\) where \\( q_\\sigma \\) is the species charge, then a particle obeys Lagrangian dynamics with the normalized Lagrangian \\( \\bar{L} = (\\bar{v}_x^2 + \\bar{v}_y^2 + \\bar{v}_z^2)/2 - \\bar{v}_z \\ln \\cosh \\bar{x} \\), where barred quantities are normalized to their respective reference units, i.e., \\( \\bar{L} = L/m_\\sigma \\lambda^2 \\omega_{c\\sigma}^2 \\), \\( \\bar{v}_x = v_x/\\lambda \\omega_{c\\sigma} \\), and \\( \\bar{x} = x/\\lambda \\). Because \\( y \\) and \\( z \\) are ignorable coordinates, there are three constants of motion, namely the canonical momenta \\( \\bar{p}_y = \\partial \\bar{L}/\\partial \\bar{v}_y = \\bar{v}_y \\) and \\( \\bar{p}_z = \\partial \\bar{L}/\\partial \\bar{v}_z = \\bar{v}_z - \\ln \\cosh \\bar{x} \\), and the total energy of the particle (recall that \\( \\phi = 0 \\)), \\( \\bar{H} = (\\bar{v}_x^2 + \\bar{v}_y^2 + \\bar{v}_z^2)/2 = \\bar{v}_x^2/2 + [\\bar{p}_y^2 + (\\bar{p}_z + \\ln \\cosh \\bar{x})^2]/2 \\). The normalized effective potential \\( \\chi(\\bar{x}) \\) of the motion in the \\( x \\)-direction is therefore \\( \\chi(\\bar{x}) = [\\bar{p}_y^2 + (\\bar{p}_z + \\ln \\cosh \\bar{x})^2]/2 \\).\n\nAnalyzing the extrema of \\( \\chi(\\bar{x}) \\) shows that it exhibits two shapes depending on the sign of \\( \\bar{p}_z \\): (i) a single-well if \\( \\bar{p}_z > 0 \\) (e.g., black line in Fig. 1d), and (ii) a double-well with a local hill at \\( \\bar{x} = 0 \\) if \\( \\bar{p}_z < 0 \\) (e.g., black line in Fig. 1a). In case (ii), if a particle does not have enough energy to overcome the local hill, i.e., \\( \\bar{H} < \\chi(0) \\) or equivalently \\( \\sqrt{\\bar{v}_x^2 + \\bar{v}_z^2} = \\bar{v}_\\perp < -\\bar{p}_z \\), it oscillates within one of the two wells and does not cross \\( \\bar{x} = 0 \\). In the opposite case where \\( \\bar{v}_\\perp > -\\bar{p}_z \\), the particle has enough energy to overcome the hill and thus undergoes a full double-well orbit while crossing \\( \\bar{x} = 0 \\). This double-well orbit class can be further divided into two sub-classes depending on the particle’s bounce-period-averaged velocity in the \\( z \\)-direction \\( \\langle \\bar{v}_z \\rangle \\). Because \\( \\langle \\bar{v}_z \\rangle = \\langle \\bar{p}_z \\rangle + \\langle \\ln \\cosh \\bar{x} \\rangle \\) while \\( \\bar{p}_z < 0 \\) is a constant in the case of a double-well \\( \\chi \\), a particle can have either a positive or negative \\( \\langle \\bar{v}_z \\rangle \\) depending on its oscillation amplitude in the \\( x \\)-direction; particles with higher energies have higher values of \\( \\langle \\ln \\cosh \\bar{x} \\rangle \\) and thus can have positive values of \\( \\langle \\bar{v}_z \\rangle \\).\n\nFigure 1 summarizes the four classes of particle orbits. The black lines in Figs. 1a-d show the effective potential \\( \\chi \\) of each class, and the three dashed lines in each panel represent the energies of three particles with differing values of initial \\( \\bar{v}_x \\) and thus of \\( \\bar{H} \\). Each particle is distinguished by its respective color (blue, red, or cyan). The three lines in Figs. 1e-h show the motion of the three particles in the left panels in the \\( x - z \\) plane, and the black dots represent their starting positions.\n\nFigure 1e represents the non-crossing orbit class[34], hereafter denoted NC, where the particles are simply \\( \\nabla B \\) drifting with \\( \\langle \\bar{v}_z \\rangle < 0 \\). Figure 1f represents the class where particles undergo full double-well motion with \\( \\langle \\bar{v}_z \\rangle < 0 \\), hereafter denoted DW–. The blue particle in\nFIG. 1. Four classes of particle orbits and their effective potentials. Effective potentials \\( \\chi \\) of the **a** non-crossing (NC) orbit class, **b** double-well orbit class with a negative time-averaged velocity (\\( \\langle \\bar{v}_z \\rangle < 0 \\); DW−), **c** double-well orbit class with a positive time-averaged velocity (\\( \\langle \\bar{v}_z \\rangle > 0 \\); DW+), and **d** meandering (M) orbit class. **e-h** Particle orbits in the \\( \\bar{x} - \\bar{z} \\) plane respectively belong to the four classes in **a-d**. Three particles are plotted for each class and are labelled by the blue, cyan, and red colors. Each particle’s energy is represented by its corresponding color in **a-d**. The blue particles in **f** and **g** respectively belong to NC and DW− but are plotted to show the NC → DW− and DW− → DW+ transitions.\n\n![Four panels showing effective potentials and particle orbits for different orbit classes](page_186_120_1217_1042.png)\nFigure 1f belongs to NC but is plotted to show the transition from NC to DW−. Figure 1g represents the other class where \\( \\langle \\vec{v}_z \\rangle > 0 \\), hereafter denoted DW+. Again, the blue particle belongs to the DW− class but is plotted to show the transition from DW− to DW+. Figure 1h represents the meandering or Speiser orbit class[35] with \\( \\langle \\vec{v}_z \\rangle > 0 \\), hereafter denoted M.\n\nThe DW+ class was previously identified in a context with curved magnetic fields as “cucumber orbits[36, 37]” due to its cucumber shape. Here we have re-identified the class to clarify the physical origin of such motion and to distinguish more clearly between DW+ and DW−, the latter of which does not exhibit cucumber shapes.\n\nPhase-Space Distributions Now let us examine how each orbit class is represented in phase space. \\( 10^8 \\) particles were randomly sampled from Eq. 2 with \\( \\bar{V}_\\sigma = 0.005 \\) and \\( \\bar{v}_{T\\sigma} = 0.05 \\) — these specific values satisfy the equilibrium condition for the Harris sheet. Figure 2 shows the phase space distributions (a-c) and velocity space histograms (d-f) in each velocity direction, and Fig. 2g shows the spatial histograms. The orbit classes are distinguished by the black, red, green, and blue colors. The dotted lines and the arrows in the right panels correspond to the mean velocity and the velocity spread (two standard deviations) of each orbit class.\n\nThe phase-space distribution of each orbit class has its own contribution to current sheet density, temperature, and strength. The spatial distribution in Fig. 2g is related to the density, and the spreads and means of the velocity distributions in Figs. 2d-f are respectively related to the temperature and current strength of each orbit class.\n\nFigure 2d shows that the velocity spread and hence the temperature in the x-direction, \\( T_{xx} \\), has the following hierarchy: NC < DW− < DW+. This is because the transition from NC to DW necessarily involves a passage through the unstable equilibrium as in Fig. 1b, which in turn involves a breakdown of adiabatic invariance and phase-mixing[38]. \\( T_{xx} \\) of the M class is equal to the overall equilibrium temperature. The mean velocity in the x-direction is befittingly zero for all classes due to symmetry.\n\nFigure 2e shows that all classes have the same temperatures and zero mean velocities in the y-direction, since \\( \\bar{v}_y \\) is a constant of motion.\n\nFigure 2f shows that the temperature in the z-direction has the hierarchy M < DW+ < NC < DW−. The NC and DW− classes have negative mean velocities and the other two have positive mean velocities.\n\nFigure 2g shows that the three non-NC classes are spatially concentrated near the center.\nFIG. 2. **Particle distribution in phase space, velocity space, and physical space.** Phase space distributions of the four orbit classes distinguished by the blue, green, red, and black colors in **a** \\( \\bar{x} - \\bar{v}_x \\) space, **b** \\( \\bar{x} - \\bar{v}_y \\) space, and **c** \\( \\bar{x} - \\bar{v}_z \\) space. Particle histograms in **d** \\( \\bar{v}_x \\), **e** \\( \\bar{v}_y \\), and **f** \\( \\bar{v}_z \\). The dotted lines and arrows are respectively the average velocities and two standard deviations of each distribution. **g** Particle histogram in \\( \\bar{x} \\).\n\nNon-crossing\nMeandering\nDouble-well +\nDouble-well –\nAlso, the DW classes have relatively flat-top density profiles compared to the M class, a trait which will be revisited later.\n\nEquilibration Process We now have all the ingredients to understand how an initially disequilibrated current sheet equilibrates. Let us consider an under-heated Harris current sheet with a temperature lower than its equilibrium value. In this case, because the thermal pressure at the center is lower than the magnetic pressure at the outskirts, one expects heating and pinching (increase of current density) of the current sheet that lead to a new equilibrium.\n\nLet us first predict how the heating and pinching will happen. Inserting Eqs. 1 and 2 in the Vlasov equation yields\n\n\\[\n\\frac{\\partial \\ln f_{\\sigma}}{\\partial t} = -2 \\left( \\frac{\\bar{V}_{\\sigma}}{2 \\bar{v}_{T\\sigma}^2} - 1 \\right) \\bar{v}_x \\tanh \\bar{x}.\n\\] (3)\n\nAt equilibrium, the Harris sheet has \\( \\bar{V}_{\\sigma} = 2 \\bar{v}_{T\\sigma}^2 \\), which can be confirmed by matching the current density obtained by \\( \\mathbf{J} = \\nabla \\times \\mathbf{B}/\\mu_0 \\) and that obtained by \\( \\mathbf{J} = \\sum_{\\sigma} q_{\\sigma} \\int \\mathbf{v} f_{\\sigma} d^3 \\mathbf{v} \\). However, if the sheet is under-heated so that \\( 2 \\bar{v}_{T\\sigma}^2 < \\bar{V}_{\\sigma} \\), then the quantity \\( \\xi := \\bar{V}_{\\sigma} - 2 \\bar{v}_{T\\sigma}^2 \\) is positive and Eq. 3 yields a solution linear in a small time interval \\( \\Delta \\bar{t} \\):\n\n\\[\nf_{\\sigma} \\propto \\exp \\left[ -\\frac{1}{2 \\bar{v}_{T\\sigma}^2} (\\bar{v}_x + \\xi \\Delta \\bar{t} \\tanh \\bar{x})^2 \\right].\n\\] (4)\n\nThe mean velocity in the \\( x \\)-direction is thus \\( \\bar{V}_x(\\bar{x}) = -\\xi \\Delta \\bar{t} \\tanh \\bar{x} \\). At positive \\( \\bar{x} \\), particles gain negative \\( \\bar{v}_x \\) and vice-versa; therefore, the initial linear response of an under-heated Harris sheet is to bring particles closer to the center by increasing their \\( |\\bar{v}_x| \\).\n\nThis response induces transitions among particle classes. It is apparent from Fig. 1a-c that an increase in \\( |\\bar{v}_x| \\) moves NC particles to DW– and DW– particles to DW+. Applying the analysis of the phase-space distributions of the four classes in Fig. 2, these class transitions explain (i) current sheet heating in the \\( x \\)-direction, and (ii) current sheet pinching due to increases in both density and mean velocity at the center (note that the velocity decrease from the NC \\( \\rightarrow \\) DW– transition is more than compensated for in the DW– \\( \\rightarrow \\) DW+ transition). Also, there is no transition to or from the M class because the shape of \\( \\chi \\) is such that a change in \\( \\bar{v}_x \\) does not induce orbit class transitions.\n\nThe above analysis only considers linear dynamics assuming that the current sheet profile remains stationary. It is therefore not valid in the nonlinear regime where the profile self-consistently changes along with orbit class transitions. However, we may infer from the\nFIG. 3. Streak plots of variables from the particle-in-cell simulation. Streak plots of a the sheared magnetic field \\( B_y \\), b the current density \\( J_z \\), c the ion temperature \\( T_i \\), and d the ion density \\( n_i \\) from \\( t = 0 \\) to \\( 1000 \\omega_{ci}^{-1} \\).\n\nanalysis the primary mechanism—at least in the linear regime—underlying current sheet heating and pinching: transitions from the NC class to the DW classes and no transitions to or from the M class.\n\nThese predictions will now be verified with a one-dimensional particle-in-cell simulation. The initial condition was an under-heated Harris current sheet with a temperature \\( T = 0.2 T_{eq} \\) where \\( T_{eq} = B_0^2 / (4 \\mu_0 n_0 k_B) \\) is the Harris equilibrium temperature. The initial sheet thickness was \\( \\lambda = 10 d_i \\) where \\( d_i \\) is the collisionless ion skin depth. Figure 3 shows streak plots of \\( B_y \\), \\( J_z \\), the ion temperature \\( T_i \\), and the ion density \\( n_i \\). The current sheet pinches and heats up until \\( \\sim 30 \\omega_{ci}^{-1} \\), after which it remains steady and thus reaches equilibrium.\n\nFigures 4a-c show \\( f_i \\) in \\( x - v_x \\) space at \\( t = 0, 10, 100 \\omega_{ci}^{-1} \\), respectively. Figure 4b confirms the initial response of the under-heated current sheet as predicted by Eq. 4, namely the focussing of the particles towards the center. Figure 4c shows the equilibrium reached by \\( f_i \\), and Fig. 4d shows the difference (\\( \\Delta f_i \\)) between the initial state (Fig. 4a) and the equilibrium state (Fig. 4c). Comparing Fig. 4d to Fig. 2a, it is apparent that the NC class de-populates and migrates to the DW classes. The dynamics in the simulation is fully nonlinear, so transition to the M class also occurs, albeit less significantly than the main NC \\( \\rightarrow \\) DW transition.\n\nFigures 4e-g and 4i are the same as Figs. 4a-d except that they are in \\( x - v_z \\) space. Again, the NC \\( \\rightarrow \\) DW transition is evident from a comparison to the pronounced Y-shape\nFIG. 4. **Time evolution of the ion distribution function from the particle-in-cell simulation.** Ion distribution function \\( f_i \\) in \\( x - v_x \\) space at **a** \\( t = 0 \\), **b** \\( t = 10\\omega_{ci}^{-1} \\), and **c** \\( t = 100\\omega_{ci}^{-1} \\). **d** The difference (\\( \\Delta f_i \\)) between \\( f_i \\) in **c** and **a**. **e-g** and **i** are respectively the same as **a-c** and **d**, except in \\( x - v_z \\) space. **h** A slice through the dotted line in **g**. **j-l** The ion current density \\( J_{iz} \\) obtained by taking the first velocity moment of **e-g**. **m** The difference between **j** and **l**.\n\nof the phase-space distribution of the DW classes (Fig. 2c). Therefore, we have confirmed that collisionless equilibration of an under-heated Harris current sheet is mainly due to orbit class transitions from NC to DW.\n\nIt is clear from Figs. 4c and 4g that the final equilibrium is most naturally described by the relative population in each orbit class, rather than, e.g., Maxwellian or kappa distributions. Figure 4h shows the distribution in \\( v_z \\) at \\( x = 0.2\\lambda \\), whose profile is clearly non-Maxwellian. Note that electrons also mainly transition from NC to DW in this process because the orbit classes apply generally for any species. Figure 4 is therefore qualitatively applicable to electrons, except that their velocities change signs due to their negative charge.\n\n**Origin of Bifurcated Current Sheets** Figures 4j-l show the time evolution of the ion current density in the z-direction, \\( J_{iz} \\), and Fig. 4m shows the difference between the initial and final \\( J_{iz} \\). The bifurcated structure is evident, which naturally arises from the pronounced Y-shape of the phase-space distribution of the DW classes to which particles\nmigrate from the NC class. The total current density—mainly carried by the electrons—is also bifurcated, as shown in Fig. 3b. Bifurcated current structures are thus natural by-products of the collisionless equilibration process of a current sheet.\n\nLet us compare the simulation results with a current sheet detected by the Magnetospheric Multiscale (MMS) mission[39] from 20:24:00 to 20:24:15 UT on 17 June 2017, when the spacecraft was located at (−19.4, −10.4, 5.5) \\( R_e \\) in Geocentric Solar Ecliptic (GSE) coordinates while crossing the magnetotail plasma sheet from the southern to the northern hemisphere. This sheet has also been examined in previous studies under different contexts[33, 40, 41]. The focus will now be on electrons instead of ions because the observed current sheet has an electron scale thickness (\\( < 10d_e \\)), and as a confirmation that electrons have similar orbit class transition dynamics to that of ions.\n\nFigure 5 shows a side-by-side comparison of the current sheet detected by MMS and that from the particle-in-cell simulations. The data are presented using a local coordinate system, \\( LMN \\). The sheared magnetic field is in the \\( L \\)-direction, and \\( M \\) and \\( N \\) are respectively parallel and normal to the current sheet. The current is carried mainly by the electrons in both the observation and the simulation. The finite electron outflow \\( v_{eL} \\) in Fig. 5b indicates that the observed current sheet is undergoing magnetic reconnection, whereas the simulated current sheet, being one-dimensional, is not. Reconnection induces perpendicular electron heating at the sheet center[42], which explains the central increase of \\( T_{eMM} \\) in Fig. 5d relative to Fig. 5j. The relative increase of \\( T_{eLL} \\) at the outskirts in Fig. 5d is also attributed to reconnection-induced parallel electron heating[42].\n\nApart from such reconnection-related dissimilarities, the observed and simulated profiles agree strikingly well, including the bifurcated current structure. In particular, the simulated equilibrium explains the central dip and increased outskirts of the electron temperature tensor element \\( T_{eMM} \\) relative to \\( T_{eNN} \\), as shown in Figs. 5d and 5j. The profile of \\( T_{eNN} - T_{eMM} \\) in Fig. 5e is remarkably reproduced by Fig. 5k, except for the relative central dip in Fig. 5e due to the reconnection-induced increase of \\( T_{eMM} \\). Same goes for the pressure tensor elements \\( P_{eMM}, P_{eNN} \\), and \\( P_{eNN} - P_{eMM} \\) (Figs. 5f and 5l).\n\nThe increased amount of electron population in the DW classes is shown not only by the current, temperature, and pressure structures, but also by the density plateau in Fig. 5c and 5i which is due to migrations to the DW classes (see Fig. 2g). This density plateau was also observed in Cluster measurements[25].\nFIG. 5. Comparison of a current sheet detected by MMS to that from the particle-in-cell simulation. a-f Sequentially, the magnetic field \\( \\mathbf{B} \\), electron velocity \\( \\mathbf{v}_e \\), electron density \\( n_e \\), diagonal elements of the electron temperature tensor \\( \\mathbf{T}_e \\), the difference between the temperature tensor elements \\( T_{eNN} - T_{eMM} \\), and diagonal elements of the electron pressure tensor \\( \\mathbf{P}_e \\) and \\( P_{eNN} - P_{eMM} \\) (shifted up by 0.04) detected by the Magnetospheric Multiscale spacecraft from 20:24:00 to 20:24:15 UT on 17 June 2017. The x-axis is seconds from 20:24:00 UT. g-l Quantities from the particle-in-cell simulation respectively corresponding to a-f.\n\nIII. DISCUSSION\n\nAlthough the new kinetic equilibrium has been presented as an example of bifurcated current sheets, we are not claiming that all such sheets are in equilibrium states. Instead,\nthe claim is that bifurcated structures are natural repercussions of the collisionless current sheet equilibration process and so are likely to be observed in a variety of phenomena as the underlying structure. As mentioned in the Introduction, numerous explanations for bifurcated current sheets have been put forth; these explanations will now be unravelled in relation to the relaxation process.\n\nMagnetic reconnection has been one of the proposed causes of bifurcated current sheets[26, 43], but many such sheets were also observed without any fast flows[25, 44] which are sig- natures of reconnection. Nevertheless, a statistical study indicated that the thinner the structures are, the more likely they are to be bifurcated[24]. These observations can be unified by the fact that thinner current sheets are more likely to involve sub-skin-depth collisionless dynamics, which is favorable for the occurrence of both collisionless reconnec- tion and the present collisionless relaxation process. A possible scenario is one where an initially thick, under-heated current sheet equilibrates to a thin, sub-skin-depth bifurcated structure, which then undergoes collisionless reconnection. It fact, the initial condition for reconnection in collisionless situations is more likely to be the equilibrium presented here than widely-used specific solutions such as the Harris sheet[45]. If the sheet does not thin enough for reconnection to occur, then it may remain bifurcated and steady.\n\nFlapping motion was also observed in conjunction with bifurcated current sheets[25, 27]. This motion involves fast thinning and thickening of the sheet[27]. Such fast motion will naturally induce bifurcation via two possible scenarios: (i) disequilibration of current sheets, followed by relaxation via spontaneous orbit classes transitions, or (ii) unspontaneous transitions driven by the external source that thins the sheet.\n\nEquilibria involving anisotropic temperatures have also been shown to exhibit bifurcated structures[13, 28, 29], but the source of the anisotropy was not clear so the amount of anisotropy had been set ad-hoc. The present collisionless relaxation process naturally induces temperature anisotropy, which is thus an innate result of the equilibration process rather than a cause of bifurcated structures.\n\nSpeiser motion (M class) was also attributed to bifurcated structures[17, 30]. However, it is clear from Fig. 2 that the M class cannot contribute to bifurcated structures if the density is peaked near the center, unless the density itself is bifurcated[17] and/or heavier species are taken into account[30].\n\nSome studies[16, 36, 37] invoke non-adiabatic scattering of particles from M to DW+ via\na slow diffusive process in current sheet equilibria. However, the diffusion coefficient of such process is zero for \\( B_x = 0 \\) because it scales with the curvature parameter \\( \\kappa \\) (cf. equation 7 of Zelenyi et al.[37]). We have shown here that neither curved magnetic fields nor diffusive processes are necessary; simply choosing a disequilibrated initial state is sufficient for the development of bifurcated structures, although diffusion due to field curvature may aid the process.\n\nIn summary, the collisionless relaxation process of a disequilibrated current sheet was studied. The process is most naturally understood by orbit class transitions, which were analytically predicted and numerically verified. The relaxation mechanism was identified as the origin of bifurcated current sheets, and the significance of this identification in regards to previous explanations of bifurcated structures was discussed.\n\nIV. METHODS\n\nSampling from and categorization of the Harris distribution function Particle positions and velocities were sampled from Eq. 2 using the numpy.random package in Python 3.8. Particles with \\( \\bar{p}_z > 0 \\) and \\( \\bar{p}_z < -\\bar{v}_\\perp \\) were categorized into M and NC, respectively. For the rest of the particles that belong to the DW classes, the following steps were taken to further categorize them.\n\nFirst, a simple analysis of the Hamiltonian of each particle shows that its oscillation amplitude in the \\( x \\)-direction is given by \\( \\bar{x}_{\\text{max}} = \\operatorname{arccosh} (\\exp [\\bar{v}_\\perp - \\bar{p}_z]) \\). The bounce-period-averaged \\( \\bar{v}_z \\) of the particle is then given by\n\n\\[\n\\langle \\bar{v}_z \\rangle = \\frac{2}{T_0} \\int_{-\\bar{x}_{\\text{max}}}^{\\bar{x}_{\\text{max}}} \\frac{\\bar{v}_z}{\\bar{v}_x} d\\bar{x},\n\\]\n(5)\n\n\\[\n= \\frac{2}{T_0} \\int_{-\\bar{x}_{\\text{max}}}^{\\bar{x}_{\\text{max}}} \\frac{\\bar{p}_z + \\ln \\cosh \\bar{x}}{\\sqrt{(\\bar{p}_z + \\ln \\cosh \\bar{x}_{\\text{max}})^2 - (\\bar{p}_z + \\ln \\cosh \\bar{x})^2}} d\\bar{x},\n\\]\n(6)\n\nwhere \\( T_0 = 2 \\int_{-\\bar{x}_{\\text{max}}}^{\\bar{x}_{\\text{max}}} d\\bar{x}/\\bar{v}_x \\) is the bounce period. Only the sign of \\( \\langle \\bar{v}_z \\rangle \\) matters here, so the integral in Eq. 6 was evaluated numerically for each particle using the scipy.integrate.quad package in Python 3.8. Particles with positive \\( \\langle \\bar{v}_z \\rangle \\) were categorized into DW+, and the rest into DW−.\n\nParticle-in-cell simulation The open-source, fully-relativistic particle-in-cell code,\nSMILEI[46], was used. The 1D simulation domain was \\(10\\lambda = 100d_i\\) long and was divided into \\(2^{15} = 32,768\\) grid points. Open boundary conditions (Silver-Müller) were employed for the electromagnetic fields in the \\(x\\)-direction, and periodic boundary conditions were imposed for the fields in the \\(y\\)-direction and for the particles. 10,000 particles were placed per cell per species, so about \\(6 \\times 10^8\\) particles were simulated with a mass ratio \\(m_i/m_e = 100\\). The simulation run with a frequency ratio of \\(\\omega_{ce}/\\omega_{pe} = 5\\) is shown in this paper for clarity of presentation; ratios as low as \\(\\omega_{ce}/\\omega_{pe} = 0.2\\) were also tried, but lower ratios simply increased the duration of plasma oscillations that either damp or travel away from the center without any noticeable effect on the core relaxation mechanism. The initial conditions were Eqs. 1 and 2, and the electrostatic potential \\(\\phi = 0\\). The initial temperature was set as one-fifth of the Harris equilibrium temperature, i.e., \\(T = 0.2T_{eq}\\) where \\(T_{eq} = B_0^2/(4\\mu_0 n_0 k_B)\\) is the temperature that yields the Harris equilibrium. The simulation time was \\(t_{max} = 100\\omega_{ci}^{-1}\\) with a time step \\(\\Delta t = 7.63 \\times 10^{-4}\\omega_{ci}^{-1}\\).\n\nThe simulations were run on the KAIROS computer cluster at Korea Institute of Fusion Energy.\n\nMMS data and local LMN coordinates Data from MMS2, MMS3, and MMS4 from 20:24:00 to 20:24:15 UT on June 17, 2017 were averaged to yield the profiles shown in Figs. 5a-e. MMS1 data were omitted because the current density did not exhibit an obvious bifurcated structure. The magnetic field data were collected by the Fluxgate Magnetometer instrument[47] and the plasma data by the Fast Plasma Investigation instrument[48]. The local LMN coordinate system is obtained from a minimum variance analysis[49] of the averaged raw data which are in Geocentric Solar Ecliptic (GSE) coordinates. The values of the unit vectors in GSE coordinates are \\(L = (0.942, 0.308, -0.130)\\), \\(M = (0.194, -0.189, 0.963)\\), and \\(N = (0.272, -0.932, -0.238)\\) in GSE coordinates. \\(L\\) is the direction of the sheared magnetic field, \\(N\\) is the direction normal to the current sheet, and \\(LMN\\) form a right-handed coordinate system.\n\nDATA AVAILABILITY\n\nMMS data are publicly available from https://lasp.colorado.edu/mms/sdc/public. The data from the PIC simulations are available from https://doi.org/10.5281/zenodo.4607112.\nCODE AVAILABILITY\n\nSMILEI[46] is an open-source PIC code available from https://smileipic.github.io/Smilei.\nMMS data were analyzed using the pySPEDAS package, available from https://github.com/spedas/pyspedas.\nThe codes used in the data analyses are available from Y.D.Y. upon reasonable request.\n\n[1] Linhui Sui and Gordon D. Holman. Evidence for the Formation of a Large-Scale Current Sheet in a Solar Flare. 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LeCompte, A. Lukemire, E. MacDonald, A. Mariano, T. Mukai, K. Narayanan, Q. Nguyen, M. Onizuka, W. Paterson, S. Persyn, B. Piepgrass, F. Cheney, A. Rager, T. Raghu-ram, A. Ramil, L. Reichenthal, H. Rodriguez, J. Rouzaud, A. Rucker, Y. Saito, M. Samara, J.-A. Sauvaud, D. Schuster, M. Shappirio, K. Shelton, D. Sher, D. Smith, K. Smith, S. Smith, D. Steinfeld, R. Szymkiewicz, K. Tanimoto, J. Taylor, C. Tucker, K. Tull, A. Uhl, J. Vloet, P. Walpole, S. Weidner, D. White, G. Winkert, P.-S. Yeh, and M. Zeuch. Fast Plasma Investigation for Magnetospheric Multiscale. Space Science Reviews, 199(1-4):331–406, mar 2016.\n\n[49] Buo Sonnerup and Maureen Scheible. Minimum and maximum variance analysis. In Analysis methods for multi-spacecraft data, volume 001, pages 185–220. 1998.\nACKNOWLEDGMENTS\n\nThis work was supported by the National Research Foundation of Korea under grant nos. NRF-2019R1C1C1003412, NRF-2019R1A2C1004862, and 2019M1A7A1A03088456. We thank the entire MMS team and MMS Science Data Center for providing the high-quality data for this study. We also thank J. M. Kwon, J. H. Kim, and Korea Institute of Fusion Energy for providing the computer resources.\n\nAUTHOR CONTRIBUTIONS\n\nY.D.Y. conceived the central idea, performed the simulations and theoretical analysis, analyzed the spacecraft data, and wrote the manuscript based on extensive discussions with G.S.Y. D.E.W. contributed to the interpretation of the simulation and observation results, as well as to the revision of the draft. J.L.B. oversaw the MMS project and provided general guidance.\n\nCorrespondence and requests for materials should be addressed to Y.D.Y or G.S.Y.\n\nCOMPETING INTERESTS\n\nThe authors declare no competing interests.\nFigures\n\nFigure 1\n\nFour classes of particle orbits and their effective potentials. Please see manuscript .pdf for full caption.\nFigure 2\n\nParticle distribution in phase space, velocity space, and physical space. Please see manuscript .pdf for full caption.\nFigure 3\n\nStreak plots of variables from the particle-in-cell simulation. Please see manuscript .pdf for full caption.\n\nFigure 4\n\nTime evolution of the ion distribution function from the particle-in-cell simulation. Please see manuscript .pdf for full caption.\nFigure 5\n\nComparison of a current sheet detected by MMS to that from the particle-in-cell simulation. Please see manuscript .pdf for full caption."} {"paper_id": "prb18", "title": "Equilibrium selection via current sheet relaxation and guide field amplification", "text": "Equilibrium selection via current sheet relaxation and guide field amplification\n\nYoung Dae Yoon (yyoon11@postech.ac.kr)\nPohang Accelerator Laboratory https://orcid.org/0000-0001-8394-2076\n\nDeirdre Wendel\nNASA Goddard Space Flight Center https://orcid.org/0000-0002-1925-9413\n\nGunSu Yun\nPohang University of Science and Technology https://orcid.org/0000-0002-1880-5865\n\nPhysics Article\n\nKeywords:\n\nPosted Date: April 28th, 2022\n\nDOI: https://doi.org/10.21203/rs.3.rs-1423536/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\nEquilibrium selection via current sheet relaxation and guide field amplification\n\nYoung Dae Yoon*\nPohang Accelerator Laboratory, POSTECH, Pohang, Republic of Korea\n\nDeirdre E. Wendel\nNASA Goddard Space Flight Center, Greenbelt, USA\n\nGunSu S. Yun†\nDepartment of Physics and Division of Advanced Nuclear Engineering,\nPOSTECH, Pohang, Republic of Korea and\nCenter for Attosecond Science, Max Planck POSTECH/Korea Research Initiative, Pohang, Republic of Korea\nAbstract\n\nAlthough there is a continuous spectrum of current sheet equilibria, how a particular equilibrium is selected by a given system remains a mystery. Yet, only a limited number of equilibrium solutions are used for analyses of magnetized plasma phenomena. Here we present the exact process of equilibrium selection, by analyzing the relaxation process of a disequilibrated current sheet under a finite guide field. It is shown via phase-space analyses and particle-in-cell simulations that the current sheet relaxes in such a way that the guide field is locally amplified, yielding a mixed equilibrium from the spectrum. The universality of such equilibria is delineated by comparing the simulated current sheet to that observed in space.\n\nCurrent sheets are structures that are ubiquitous in space and laboratory plasmas [1–6]. Sandwiched by two regions of opposing magnetic fields, current sheets act as magnetic batteries which store magnetic free energy that can be converted to other forms of energy. Examples of such conversion processes include important phenomena such as magnetic reconnection [7, 8], drift kink instability [9], ideal tearing instability [10], and plasmoid instability [11, 12]. Current sheets have thus been subject to extensive research over the past few decades.\n\nA subject that has accrued much interest in particular is current sheet equilibria, which determine the stationary profiles of various plasma parameters such as magnetic field and temperature. A plethora of analytical and numerical equilibria have been found [13–24], and these are readily used as initial conditions for analyses of various plasma phenomena. For instance, two current sheet equilibrium solutions—the Harris equilibrium [13] and the force-free equilibrium [22]—are notably and almost exclusively used for magnetic reconnection analyses [25–28].\n\nA relatively less explored subject is how initially disequilibrated current sheets relax to equilibrium states. Such knowledge is important because plasma systems in general start from disequilibrated states and so it reveals how such systems tend to dynamically evolve in time. Also, the relaxation process manifests the general solution of current sheet equilibria, providing a more profound insight than the multitude of specific solutions that have been found so far. For instance, Ref. [29] showed that current sheet equilibration—heating and pinching—is achieved via particle orbit class transitions, or, in other words, that a particular equilibrium solution can be represented by the fractional population in each orbit\nclass. A useful by-product of this analysis was the prediction of bifurcated current sheets [30], whose origins had remained controversial for over a decade. The ubiquity of bifurcated structures was explained by showing that they are natural outcomes of the relaxation process of disequilibrated states, from which current sheets most likely start their dynamics.\n\nA crucial limitation to the analysis in Ref. [29] was that it did not include effects due to the magnetic field component parallel to the main current direction, i.e., the guide field. Guide field effects, however, are of paramount importance because zero-guide-field current sheets rarely exist in reality, and the presence of even the smallest guide fields significantly alter ensuing dynamics, e.g., in guide field reconnection [31, 32]. In fact, spacecraft observations seem to indicate that finite guide fields deter the formation of bifurcated current sheets [33–37]; the origin of this dissimilarity with the zero-guide-field case is unclear. As such, current sheet relaxation under guide fields is a different matter to deal with and must therefore be thoroughly investigated in comparison to the zero-guide-field case.\n\nFinite guide fields are also important in regards to equilibrium selection. Although the two aforementioned equilibrium solutions—Harris and force-free—are usually employed for many practical purposes, there is actually a continuous spectrum of solutions which can be represented by combinations of the two equilibria, which are respectively at each end of the spectrum [22, 38–41]. The frequent usage of only the two extremes is therefore not justified. In fact, it is not even clear how a particular equilibrium out of the spectrum is selected or generated by a given system, e.g., how a zero-guide-field Harris sheet transitions to a sheet with a locally-amplified guide field such as the force-free sheet.\n\nHere we present, via an analysis of the collisionless relaxation mechanism of a current sheet under a finite guide field, the comprehensive process in which a particular equilibrium is selected by a given plasma system. This is shown in the following steps; first, particle orbits in a magnetic field reversal under a finite guide field are exhaustively classified into three distinct orbit classes. The guide field induces an anti-symmetry in the particle phase space distribution. Second, it is then shown via comparisons to particle-in-cell (PIC) simulations that a disequilibrated (under-heated) Harris sheet with a small seed guide field relaxes via orbit class transitions. Ions are responsible for sheet heating and electrons are responsible for sheet pinching and shearing. The transitions are in such a way that the seed guide field is locally amplified at the center, yielding one of the equilibria within the spectrum, i.e., a mixture of Harris and force-free equilibria. The distribution anti-symmetry is responsible\nfor guide field amplification, but the phenomenon can also be intuitively understood in the magneto-hydrodynamic (MHD) picture. The reduction of bifurcation under finite guide fields is naturally explained by the type of orbit class transitions that take place. Finally, the equilibrium current sheet from the PIC simulation is compared with a current sheet observed by the Magnetospheric Multiscale (MMS) mission, thereby confirming the theoretical and numerical analyses and demonstrating the universality of mixed equilibria.\n\nEquilibrium spectrum The spectrum of one-dimensional equilibria represented by a mixture of Harris and force-free current sheets can be expressed by the electrostatic potential \\( \\phi = 0 \\) and the following values of the magnetic field \\( \\mathbf{B} \\), the plasma pressure tensor component \\( P_{xx} \\), and the current density \\( \\mathbf{J} \\) in Cartesian coordinates [22]:\n\n\\[\n\\mathbf{B} = B_0 \\left[ \\hat{y} \\tanh \\left( \\frac{x}{\\lambda} \\right) + \\hat{z} \\frac{b_g}{\\cosh (x/\\lambda)} \\right], \\tag{1}\n\\]\n\\[\nP_{xx} = \\frac{B_0^2}{2\\mu_0} \\left( 1 - b_g^2 \\right) \\frac{1}{\\cosh^2 (x/\\lambda)}, \\tag{2}\n\\]\n\\[\n\\mathbf{J} = \\frac{B_0}{\\mu_0 \\lambda} \\left[ \\hat{y} b_g \\frac{\\sinh (x/\\lambda)}{\\cosh^2 (x/\\lambda)} + \\hat{z} \\frac{1}{\\cosh^2 (x/\\lambda)} \\right], \\tag{3}\n\\]\n\nwhere \\( B_0 \\) is the asymptotic magnetic field strength, \\( b_g \\) is the guide field strength relative to \\( B_0 \\), \\( \\lambda \\) is the sheet half-thickness, and \\( x \\) is the direction normal to the current sheet. Taking \\( b_g = 0 \\) yields the Harris equilibrium where the asymptotic magnetic pressure \\( B_0^2/2\\mu_0 \\) is balanced by the thermal pressure at the center (\\( x = 0 \\)), and taking \\( b_g = 1 \\) yields the force-free equilibrium where \\( |\\mathbf{B}| = B_0 \\) everywhere and so \\( \\mathbf{J} \\times \\mathbf{B} = 0 \\). The two equilibria are therefore limiting cases of a continuous spectrum from which a particular equilibrium is determined by the value of \\( b_g \\). Figures 1a and 1b show graphical illustrations of Harris and force-free equilibrium current sheets, respectively. A combination of the two profiles yields a mixed equilibrium, as shown in Fig. 1c.\n\nWe now argue that a particular equilibrium from the spectrum is attained in the following relaxation process, as illustrated in Fig. 1d. Consider an initially disequilibrated collisionless current sheet whose plasma thermal pressure at the center is lower than the magnetic pressure at the outskirts and which is under a small but finite, uniform seed guide field. As the current sheet pinches to achieve equilibrium, the frozen-in guide field is amplified at the center. The final state is a mixture of a Harris current sheet (with a small uniform guide field) and a force-free current sheet, i.e., mixed equilibrium.\n\nThrough this relaxation process, any particular equilibrium can be attained given the\nFIG. 1: Current sheet types. Graphical illustrations of the a Harris equilibrium, b force-free equilibrium, and c mixed equilibrium. d The proposed process in which a disequilibrated Harris current sheet with a small seed guide field relaxes and locally amplifies the guide field in the process, thereby creating a mixed equilibrium. The arrow widths and color intensities represent the strengths of the magnetic field and plasma pressure, respectively.\n\nappropriate initial conditions, that is, the seed guide field strength and the initial difference between the thermal and magnetic pressures. The details of this process, however, are still unclear. For example, the final state in Fig. 1d exhibits a finite \\( \\partial B_z / \\partial x \\) that does not exist in the initial state; this corresponds to the development of a finite \\( J_y \\) shear, whose origins are puzzling at this point. This macroscopic alteration must originate from microscopic, single-particle transitions. Therefore, in order to fathom the equilibrium selection process, single-particle dynamics in a current sheet with a finite guide field will now be examined.\n\nParticle orbit classes For the magnetic field profile \\( \\mathbf{B} = B_0 [\\hat{y} \\tanh (x/\\lambda) + \\hat{z} b_g] \\), one may choose the vector potential \\( \\mathbf{A} = B_0 [\\hat{y} b_g x - \\hat{z} \\lambda \\ln \\cosh (x/\\lambda)] \\). Because the system is symmetric in the y and z directions, the canonical momenta \\( p_y = m v_y + q b_g B_0 x \\) and \\( p_z = m v_z - q \\lambda B_0 \\ln \\cosh (x/\\lambda) \\) are conserved quantities, where \\( m, q, \\) and \\( \\mathbf{v} \\) are the particle mass, charge, and velocity, respectively. The normalized total energy of the particle \\( \\bar{H} = H / (m \\lambda^2 \\omega_c^2) \\) where \\( \\omega_c = q B_0 / m \\) is then \\( \\bar{H} = \\bar{v}_x^2 / 2 + \\chi (\\bar{x}) \\), where\n\n\\[\n\\chi (\\bar{x}) = \\frac{1}{2} (\\bar{p}_y - b_g \\bar{x})^2 + \\frac{1}{2} (\\bar{p}_z + \\ln \\cosh \\bar{x})^2\n\\]\n\n(4)\nFIG. 2: Three classes of particle orbits and their effective potentials. Effective potentials \\( \\chi \\) of the **a** non-crossing (NC) orbit class, **b** double-well (DW) orbit class, **c** and meandering (M) orbit class. The blue particle in **b** belongs to NC but is plotted to show the NC \\( \\rightarrow \\) DW transition. **d-f** Particle orbits in the \\( \\bar{x} - \\bar{z} \\) plane respectively belonging to the three classes in **a-c**. The strength of the out-of-plane magnetic field \\( B_y \\) is represented by the magenta and green colors. Three particles are plotted for each class and are labeled by the blue, cyan, and red colors. Each particle’s energy is represented by its corresponding color in **a-c**. **g-i** Particle orbits in the \\( \\bar{x} - \\bar{y} \\) plane.\n\nis the normalized effective potential of the particle motion in the \\( x \\) direction. Here, the barred quantities are normalized, i.e., \\( \\bar{x} = x/\\lambda \\), \\( \\bar{\\mathbf{v}} = \\mathbf{v}/(\\lambda \\omega_c) \\), and \\( \\bar{\\mathbf{p}} = \\mathbf{p}/(m \\lambda \\omega_c) \\).\n\nWhen \\( b_g = 0 \\), i.e., there is no guide field, \\( \\chi \\) can have either a single-well shape (for \\( \\bar{p}_z \\geq 0 \\)) or a double-well shape (for \\( \\bar{p}_z < 0 \\)). Particle orbits can then be classified into four distinct classes, and current sheet relaxation can be characterized by transitions among the orbit classes [29]. When \\( b_g \\) is finite, however, \\( \\chi \\) is asymmetric and is necessarily single-welled when \\( \\bar{p}_z \\geq -b_g^2 \\); but the exact condition for double-welled \\( \\chi \\) becomes more complicated (see Methods). Nonetheless, particle orbits can still be classified into three distinct classes, as shown in Fig. 2. Figures 2a-c show examples of \\( \\chi (\\bar{x}) \\) for the three classes. Figures 2d-f\nshow the motion of three particles (red, blue, and cyan) in the \\((\\bar{x}, \\bar{z})\\) plane for each orbit class; the kinetic energy of each particle is shown as dashed lines with matching colors in Figs. 2a-c. Figures 2g-i are the same as Figs. 2d-f except that they are in the \\((\\bar{x}, \\bar{y})\\) plane.\n\nIf \\( \\chi \\) is double-welled, a particle may be in one of two orbit classes. The first one is the non-crossing (NC) class, where the particle is trapped in one of the two wells and does not cross \\( \\bar{x} = 0 \\) (Figs. 2a, d, and g). The second one is the double-well (DW) class, where the particle has enough energy to undergo a full double-well motion (Figs. 2b, e, and h). The blue particle in Figs. 2b belongs to NC, but is plotted to show the NC \\(\\rightarrow\\) DW transition as the particle gains energy. If \\( \\chi \\) is single-welled, a particle is in the meandering (M) orbit class (Figs. 2c, f, and i). For the DW and M classes, it can be seen that a particle’s average \\( \\bar{v}_z \\) or \\( \\langle \\bar{v}_z \\rangle \\) changes from negative to positive as the particle gains energy.\n\nOur classification of particle orbits in the finite \\( b_g \\) case is different from that in the \\( b_g = 0 \\) case [29] in the following aspects. First, the DW is not divided further into two subclasses based on their \\( \\langle \\bar{v}_z \\rangle \\). This is because for \\( b_g = 0 \\), only DW particles may have either \\( \\langle \\bar{v}_z \\rangle > 0 \\) or \\( \\langle \\bar{v}_z \\rangle < 0 \\) since \\( \\langle \\bar{v}_z \\rangle > 0 \\) for all M particles and \\( \\langle \\bar{v}_z \\rangle < 0 \\) for all NC particles. For finite \\( b_g \\), however, both DW and M classes may have either positive or negative \\( \\langle \\bar{v}_z \\rangle \\), so a further division of the DW class is not warranted. Second, \\( \\chi \\) is asymmetric and so is particle motion in the \\( \\bar{x} \\) direction. Third, in contrast to the \\( b_g = 0 \\) case, \\( \\bar{v}_y \\) is not a constant of motion anymore and changes in time for finite \\( b_g \\); in other words, the distributions of \\( \\bar{v}_y \\) are not the same for each class.\n\n*Phase-space distributions* Let us now examine how each orbit class is represented in phase space. \\( 8 \\times 10^7 \\) particles were randomly sampled from the Harris distribution,\n\n\\[\nf(\\bar{x}, \\bar{v}) \\propto \\exp \\left( \\frac{\\bar{v}_x^2 + \\bar{v}_y^2 + [\\bar{v}_z - \\bar{V}]^2}{2 \\bar{v}_T^2} \\right) \\frac{1}{\\cosh^2 \\bar{x}},\n\\]\n\nwhere \\( \\bar{V} \\) and \\( \\bar{v}_T \\) are the mean drift and thermal velocities normalized by \\( \\lambda \\omega_c \\), respectively. \\( \\bar{V} = 0.005 \\) and \\( \\bar{v}_T = 0.05 \\) were chosen, which satisfy the \\( \\bar{V}_\\sigma = 2 \\bar{v}_T^2 \\sigma \\) condition for equilibrium.\n\nFigures 3a-c show particle distributions in \\((\\bar{x}, \\bar{v}_x)\\), \\((\\bar{x}, \\bar{v}_y)\\), and \\((\\bar{x}, \\bar{v}_z)\\) phase spaces, respectively, where each orbit class is represented by one of three—black, blue, and red—colors. Figures 3d-f show the current density components \\( \\bar{J}_i = \\int \\bar{v}_i f_i d\\bar{v}_i \\) for \\( i = x, y, z \\), respectively, where \\( f_i \\) is normalized so that \\( \\int \\int f_i d\\bar{v}_i d\\bar{x} = 1 \\). Figures 3g-i show the diagonal elements of the temperature tensor \\( \\bar{T}_{ii} = \\int (\\bar{v}_i - \\langle \\bar{v}_i \\rangle)^2 f_i d\\bar{v}_i / \\int f_i d\\bar{v}_i \\) for \\( i = x, y, z \\), respectively.\nFIG. 3: Particle distribution in phase space, velocity space, and physical space.\nPhase space distributions of the three orbit classes distinguished by the black (non-crossing), red (double-well), and blue (meandering) colors in a \\( (\\tilde{x}, \\tilde{v}_x) \\), b \\( (\\tilde{x}, \\tilde{v}_y) \\), and c \\( (\\tilde{x}, \\tilde{v}_z) \\) spaces for uniform \\( b_g = 0.15 \\). Current density components d \\( \\bar{J}_x \\), e \\( \\bar{J}_y \\), and f \\( \\bar{J}_z \\), and diagonal components of the temperature tensor g \\( \\bar{T}_{xx} \\), h \\( \\bar{T}_{yy} \\), and i \\( \\bar{T}_{zz} \\) of the three orbit classes.\n\nRegarding current sheet equilibration, equilibration of an under-heated current sheet requires sheet pinching and heating, i.e., increase of \\( J_z \\) and ion/electron temperatures \\( T_{i,e} \\). For \\( b_g = 0 \\), these are achieved by NC \\( \\rightarrow \\) DW transitions induced by particle energization [29], because the DW class has a higher temperature and a higher \\( \\langle \\tilde{v}_z \\rangle \\) in comparison to NC. The heating occurs because the NC \\( \\rightarrow \\) DW transition necessarily involves a passage through the unstable equilibrium as in Fig. 2b, which in turn involves a breakdown of adiabatic invariance and phase-mixing [42]. The pinching occurs due to the sign reversal of \\( \\langle \\tilde{v}_z \\rangle \\). For finite \\( b_g \\), sheet equilibration is expected to be similarly achieved by orbit class transitions, but it will be shown later that NC \\( \\rightarrow \\) DW transitions of ions are responsible for heating and NC \\( \\rightarrow \\) M transitions of electrons are responsible for pinching. As a sidenote, the DW and M classes may be further divided based on the sign of \\( \\langle \\tilde{v}_z \\rangle \\) into two subclasses each (DW\\( \\pm \\) and M\\( \\pm \\)). The phase space distributions of each class and their respective contributions to density, temperature, and current density are shown in Extedend Data Fig. 2.\nRegarding equilibrium selection, the anti-symmetry in Fig. 3b is important in the transformation from the Harris current sheet with a seed guide field to a mixed current sheet. Recall that our proposed mechanism for the transformation involves the amplification of the seed \\( B_z \\), which is equivalent to the development of a \\( J_y \\) shear. Of the three classes, only the M class provides the correct shear direction that amplifies \\( B_z \\) because \\( B_z \\sim -\\int \\bar{J}_y d\\bar{x} \\) by Ampère’s law. For the M class, \\( \\bar{J}_y \\sim \\bar{x} \\) near \\( \\bar{x} = 0 \\), so \\( B_z \\sim c_0 - \\bar{x}^2 \\) where \\( c_0 \\) is a constant, which is a center-peaked profile. The other classes have \\( \\bar{J}_y \\sim -\\bar{x} \\) near \\( \\bar{x} = 0 \\), so \\( B_z \\sim c_0 + \\bar{x}^2 \\) which is a center-dipped profile. Therefore, the main current-carrying species must mainly undergo transitions to the M class.\n\nCombining these two observations gives conjectural answers to the aforesaid two main questions. An initially disequilibrated Harris-type current sheet under a small finite guide field equilibrates through NC \\( \\rightarrow \\) DW & M transitions. Ions undergo NC \\( \\rightarrow \\) DW transitions, being mainly responsible for heating, and electrons undergo NC \\( \\rightarrow \\) M transitions, being responsible for pinching. The latter transitions also induce \\( J_y \\) shear, i.e., a current sheet shear, which corresponds to a local increase of \\( B_z \\), leading to a locally-amplified guide field and a mixture of Harris and force-free equilibria.\n\n*Particle-in-cell verification* In order to verify the conjectural answers, one-dimensional particle-in-cell simulation were conducted. The initial condition was an under-heated Harris current sheet with temperatures \\( T_i = T_e = 0.2T_{eq} \\) where \\( T_{eq} = B_0^2/(4\\mu_0 n_0 k_B) \\) is the Harris equilibrium temperature. The sheet was initially immersed in a uniform seed guide field with strength \\( b_g = 0.15 \\). The initial sheet thickness was \\( \\lambda = 10d_i \\) where \\( d_i \\) is the collisionless ion skin depth, and the mass ratio \\( m_i/m_e = 100 \\). A simulation run with \\( c/v_\\Lambda = 2 \\) where \\( v_\\Lambda = B_0/\\sqrt{\\mu_0 n_0 m_i} \\) (Extended Data Fig. 3) will mainly be referred to in this paper for clarity of presentation; another run with \\( c/v_\\Lambda = 20 \\) was conducted (Extended Data Fig. 4), which exhibits plasma oscillations that damp away without affecting the core relaxation mechanism that is orbit class transitions. The current sheet pinches (Extended Data Fig. 3d) and heats up (Extended Data Fig. 3e-f) until \\( t = 30\\omega_{ci}^{-1} \\) after which it achieves equilibrium and remains steady. The resultant \\( J_z \\) is not bifurcated, in contrast to the \\( b_g = 0 \\) case [29]. The sheet also develops a finite \\( J_y \\) shear (Extended Data Fig. 3c) which strongly amplifies \\( B_z \\) at the center up to \\( 0.4B_0 \\) (Extended Data Fig. 3b).\n\nExamining the time evolution of ion and electron distribution functions reveals the origin of current sheet heating, pinching, and shearing. It will be shown that ions and electrons\nFIG. 4: Time evolution of \\( f_i \\) from the particle-in-cell simulation. Ion distribution function \\( f_i \\) in \\( (\\bar{x}, \\bar{v}_x) \\) space at **a** \\( t = 0 \\), **b** \\( t = 10\\omega_{ci}^{-1} \\), and **c** \\( t = 100\\omega_{ci}^{-1} \\). **d** The difference (\\( \\Delta f_i \\)) between \\( f_i \\) in **c** and **a**. **e-h (m-p)** are respectively the same as **a-d**, except in \\( (\\bar{x}, \\bar{v}_y) \\) (\\( (\\bar{x}, \\bar{v}_z) \\)) spaces. In each row, the color represents \\( f_i \\) normalized by the maximum value in the third column (**e, g, and o**). **i-l (q-t)** Ion current density \\( J_{iy} \\) (\\( J_{iz} \\)) obtained by taking the first velocity moment of **e-h (m-p)**.\n\nundergo different orbit class transitions in the presence of a guide field, making ions mainly responsible for heating and electrons mainly for pinching and shearing.\n\nFigure 4 shows the time evolution of the ion distribution function in \\( (\\bar{x}, \\bar{v}_x) \\) (**a-c**), \\( (\\bar{x}, \\bar{v}_y) \\) (**e-g**), and \\( (\\bar{x}, \\bar{v}_z) \\) (**m-o**) spaces and of the ion current densities \\( J_{iy} \\) (**i-k**) and \\( J_{iz} \\) (**q-s**). Figures 4d, h, and p show the difference between the initial and the final states, so the red (blue) color indicates the region to (from) which ions migrate during equilibration. In respective comparisons to Figs. 3a-c, it can clearly be seen that ions mostly undergo NC \\( \\rightarrow \\) DW\nFIG. 5: **Time evolution of \\( f_e \\) from the particle-in-cell simulation.** Same as Fig. 4, but for electrons.\n\ntransitions. Two obvious features indicating this fact are (i) the pronounced slope that goes like \\( \\bar{v}_y \\sim -\\bar{x} \\) in Fig. 4g that produces \\( \\bar{J}_{1y} \\sim -\\bar{x} \\) near \\( \\bar{x} = 0 \\) (Fig. 4k), and (ii) the pronounced V-shape in Fig. 4o and the resultant bifurcated \\( \\bar{J}_{1z} \\). Ions are heated as a result of this transition because of the aforesaid breakdown of adiabatic invariance and phase-mixing. Therefore, ions are responsible for sheet heating during equilibration, much more so than electrons (compare Extended Data Fig. 3e to 3f) because electrons do not mainly undergo NC \\( \\rightarrow \\) DW transitions, as we will see shortly.\n\nFigure 5 is the same as Fig. 4, except that it pertains to electrons. It can be seen from the pronounced void in Fig. 5g and h crossing \\( (\\bar{x}, \\bar{v}_y) = (0, 0) \\)—corresponding to the slope that is present in Fig. 4g and h—that electrons do not transition to the DW class, but to the M class. The development of \\( \\bar{J}_{ey} \\sim \\bar{x} \\) near \\( \\bar{x} = 0 \\) (Fig. 5k) also indicates this\nfact. In particular, the enhanced localized current density in Fig. 5s indicates that electrons are responsible for sheet pinching. Electrons are the main current carriers, because the \\( J_{ez} \\) peak in Fig. 5s is about five times larger than the \\( J_{iz} \\) peaks in Fig. 4s (note that \\( J_z/n_0 q_e \\lambda \\omega_{ce} = m_e/m_i \\times J_z/n_0 q_i \\lambda \\omega_{ci} \\) and \\( m_i/m_e = 100 \\) here). One can also see from Fig. 5S that the electrons transition in such a way that the current density is less bifurcated, as opposed to the \\( b_g = 0 \\) case.\n\nNC \\( \\rightarrow \\) M transitions correspond to a local amplification of the seed guide field near \\( \\bar{x} = 0 \\) (cf. Fig. 3e). Although the ions’ NC \\( \\rightarrow \\) DW transitions induce \\( J_y \\) of the opposite polarity (Fig. 4k), the magnitude of \\( J_{iy} \\) is only half of that of \\( J_{ey} \\). Therefore, the electrons’ NC \\( \\rightarrow \\) M transitions are responsible for sheet shearing and guide field amplification.\n\nThe difference in the transition types of ions and electrons arises because the single-well condition (\\( \\bar{p}_{z\\sigma} = \\bar{v}_{z\\sigma}|_{\\bar{x}=0} > -b_g^2 \\)) is more sensitive to changes in \\( b_g \\) for electrons than for ions. For \\( T_i = T_e \\), the order of magnitude of \\( \\bar{v}_{zi} \\) is much larger than that of \\( \\bar{v}_{ze} \\) (compare the scale of Fig. 4o to that of Fig. 5o), and so as \\( b_g \\) increases due to current sheet shearing, the condition \\( \\bar{v}_{ze}|_{\\bar{x}=0} > -b_g^2 \\) is more easily satisfied. This is not the case for \\( b_g = 0 \\), so both ions and electrons mainly undergo NC \\( \\rightarrow \\) DW transitions [29] in contrast to the finite \\( b_g \\) case presented here.\n\n*Comparison to spacecraft observations* In order to show the universality of mixed equilibria, we now compare the final equilibrium obtained in the PIC simulation at \\( t = 100 \\omega_{ci}^{-1} \\) to a reconnecting current sheet measured by the MMS spacecraft from 05:26:41.7 to 05:26:43.7 UT on 3 July 2017, when it was located at \\((-17.6, 3.3, 1.7)\\) \\( R_E \\)—where \\( R_E \\) is the Earth’s radius—in Geocentric Solar Ecliptic (GSE) coordinates while crossing the magnetotail plasma sheet. This current sheet was undergoing magnetic reconnection, whose details were scrupulously examined in [43].\n\nFigure 6 shows the side-by-side comparison of various quantities between the measured sheet (Figs. 6a-f) and the simulated sheet (Figs. 6g-l). The data are presented in *LMN* coordinates, where \\( L \\) is the sheared magnetic field direction, \\( M \\) is the guide field direction, and \\( N \\) is the direction normal to the current sheet. The measurement time window translates to 2 s \\( \\simeq 200 \\) km [43], which, using the measured electron density \\( n_e = 0.45 \\) cm\\(^{-3}\\), translates to \\( \\sim 25 d_e \\). In the simulation, \\( \\lambda = 10 d_i = 100 d_e \\), so the window in Figs. 6g-l is \\( 0.5 \\lambda = 50 d_e \\). The measured electron diffusion region was estimated to be \\( \\sim 6 d_e \\), and the corresponding region in the simulation is \\( \\sim 12 d_e \\). Also, \\( b_g \\simeq 0.4 \\) for both sheets. Therefore, the two sheets\nFIG. 6: Comparison of MMS data to the PIC simulation. a-f Sequentially, the magnetic field \\( \\mathbf{B} \\), electron velocity \\( \\mathbf{v}_e \\) (note that the sign is reversed), electron density \\( n_e \\), diagonal elements of the electron temperature tensor \\( T_e \\), the parallel and perpendicular electron temperatures \\( T_{e\\parallel} \\) and \\( T_{e\\perp} \\), and diagonal elements of the electron pressure tensor \\( P_e \\) detected by the Magnetospheric Multiscale spacecraft from 05:26:41.7 to 05:26:43.7 UT on 3 July 2017. The \\( x \\)-axis is seconds from 05:26:00 UT, and 1 s corresponds to about \\( 12.5 d_e \\). g-l Quantities from the particle-in-cell simulation respectively corresponding to a-f. The \\( x \\)-axis is in units of \\( \\lambda = 10 d_i = 100 d_e \\). The dashed lines in g and l are analytically calculated profiles from Eqs. 1 and 2.\n\nare similar in that their length scales \\( L \\) satisfy \\( d_e \\ll L \\lesssim d_i \\), so their dynamics are mainly controlled by electrons, and in that the guide field strengths are the same.\n\nThe dashed lines in Figs. 6g and 6l show analytical solutions that are slightly modified from Eqs. 1 and 2. Because, in the simulation, a seed guide field of strength 0.15 exists and the current sheet pinches down to a length scale \\( \\lambda' \\simeq 0.2 \\lambda \\), \\( B_M = 0.15 + 0.2 / \\cosh(x/\\lambda') \\) is plotted (purple dashed line in Fig. 6g). The analytical pressure tensor component \\( P_{xx} \\)\n\n![Comparison of MMS data to the PIC simulation.](page_180_120_1208_1012.png)\nwas re-calculated accordingly and it was also assumed that \\( P_{xx} \\) is distributed equally among all three components, and therefore \\( P_{xx}/3 \\) is plotted (cyan dashed line in Fig. 6l). The agreement between the analytical and numerical solution is evident, save some details in the pressure tensor; strictly speaking, this means that even Eqs. 1 and 2 do not capture the whole spectrum and detailed phase-space analyses are necessary.\n\nOne obvious discrepancy is the central \\( v_{eL} \\) reversal (yellow arrows in Fig. 6b) in the measured sheet that is not present in the simulated sheet (Fig. 6h). This is because of the localized dip in \\( B_M \\) (purple arrow in Fig. 6a; note that \\( -v_{eL} \\sim J_{eL} \\sim -\\partial B_M/\\partial N \\)), which likely exists due to an initially non-uniform seed guide field with said dip. A PIC simulation run with a center-dipped initial guide field was conducted, and its results reproduce the central \\( v_{eL} \\) reversal (Extended Data Fig. 5h). Another discrepancy is the rather flat nature of the measured \\( T_{eLL} \\) (Fig. 6d) compared to the simulated \\( T_{eLL} \\) (Fig. 6j). However, this can be explained by the fact that reconnection induces an increase of \\( T_{eLL} \\) at the outskirts [29, 44], rendering the profile flat.\n\nAside from these particulars, the profiles of the measured and simulated sheets agree very well. The global reversal of \\( v_{eL} \\) in Fig. 6h is well reproduced in Fig. 6b, corresponding to the overall center-peaked \\( B_M \\) in Figs. 6a and 6g. A noteworthy feature is the presence of a double-peak \\( T_{eMM} \\) (arrows in Fig. 6d) and a single-peak \\( T_{eNN} \\) profile, which is reproduced in Fig. 6j. The agreement is much clearer in Figs. 6e and K, where the parallel temperature is double-peaked and the perpendicular temperature is single-peaked in both sheets. Note that the relative amplitudes between \\( T_\\perp \\) and \\( T_\\parallel \\) are different in the two cases because the background (upstream) plasma temperature is anisotropic in the measured sheet but is isotropic in the simulated sheet. From the agreement between the two sheets, one can see that the measured current sheet arose from an initially disequilibrated state.\n\nDiscussion and outlook Because the measured sheet is reconnecting, it is not in such static equilibrium as the simulated sheet. However, it is evident from our results that many features of 1D current sheet equilibration apply to 2D reconnecting sheets as well. It is therefore important to distinguish effects due to current sheet thinning from those due to reconnection itself. For instance, while the global \\( v_{eL} \\) reversal in Fig. 6b would most likely be interpreted according to the status quo as electron outflows during reconnection, it can also be interpreted as the result of current sheet relaxation leading to guide field amplification as in the present study. Considering that a popular method of identifying reconnection sites\nis by identifying jet reversals, the ambiguity of the origin of such reversals has important implications.\n\nThe relaxation time scale is an important factor in determining whether mixed equilibria are ubiquitous, because if the time scale is too long, then other faster phenomena become dominant before equilibration. One obvious indicator is the time it takes for the sheet to completely equilibrate. For the simulation run with \\( c/v_A = 2 \\), it takes \\( \\sim 30\\omega_{ci}^{-1} \\) (Extended Data Fig. 3), and for the run with \\( c/v_A = 20 \\), it takes \\( \\sim 200\\omega_{ci}^{-1} \\) to settle to a new equilibrium (Extended Data Fig. 4). Another indicator is the inductive electric field \\( E_z \\), which is equal to the rate of change of magnetic flux per unit length. For \\( c/v_A = 2 \\), it was found that the peak value of \\( E_z/v_A B_0 \\simeq 0.32 \\) (Extended Data Fig. 6a), and for \\( c/v_A = 20 \\), \\( E_z/v_A B_0 \\simeq 0.6 \\) (Extended Data Fig. 6b). Note that there is no \\( E_z \\) after the sheet equilibrates because \\( \\partial \\mathbf{B}/\\partial t = 0 \\) and that there is no parallel electric field at the center, so its peak value along flux loops at the outskirts is noted. For comparison, it is widely known that, during collisionless Hall reconnection, \\( E_z/v_A B_0 \\simeq 0.15 \\) and that it takes around tens to hundreds of \\( \\omega_{ci}^{-1} \\) for \\( E_z \\) to reach this value depending on the initial sheet and plasma parameters [25, 45]. Therefore, 1D current sheet relaxation is at least as fast as fast reconnection, and so mixed equilibria are expected to be ubiquitous.\n\nThe rapidity of sheet equilibration begs the question of how mixed equilibria change the 2D/3D reconnection dynamics. As mentioned before, reconnection simulations have almost exclusively used as initial conditions the Harris equilibrium (with or without a uniform guide field) and the force-free equilibrium, but mixed equilibria are more likely to be the underlying current sheet in many situations. Also, preliminary 2D simulations of a large-scale disequilibrated current sheet indicate that, after it rapidly equilibrates down to kinetic scales, reconnection proceeds spontaneously in various places within the sheet without any external perturbations. This is related to the multiple scale problem and/or the onset problem, both of which are important challenges for reconnection research [46].\n\nIn summary, the relaxation process of an initially disequilibrated current sheet under finite guide fields was studied. The process involves orbit class transitions similar to the zero-guide-field case, but their details and effects significantly differ. In particular, the transitions reveal the process in which a given plasma system “chooses” one equilibrium from the spectrum represented by mixtures of the Harris and force-free equilibria. The process was verified by PIC simulations through phase-space analysis and the resultant equilibrium\nwas compared to MMS observations, demonstrating solid mutual agreement and thus the universality of mixed equilibria. Important implications for magnetic reconnection analyses were also discussed.\n\nMETHODS\n\nParticle Orbit Classification\n\nThe condition for double-well motion must first be derived. Differentiating Eq. 4 to find its extrema yields\n\\[\n\\frac{d\\chi}{d\\bar{x}} = -b_g (\\bar{p}_y - b_g \\bar{x}) + (\\bar{p}_z + \\ln \\cosh \\bar{x}) \\tanh \\bar{x}.\n\\]\n(S1)\n\nThe solutions to \\( d\\chi/d\\bar{x} = 0 \\) are the intercepts between the functions \\( f_1(\\bar{x}) = b_g (\\bar{p}_y - b_g \\bar{x}) \\) and \\( f_2(\\bar{x}) = (\\bar{p}_z + \\ln \\cosh \\bar{x}) \\tanh \\bar{x} \\). In order for \\( \\chi \\) to be double-welled, there must be three intercepts, one for a local maximum and two for local minima.\n\nExtended Data Fig. 1 shows an example of the two functions. It can be seen seen that for there to be three intercepts, two conditions must be true. (i) The slope of \\( f_1 \\) at \\( \\bar{x} = 0 \\), which is \\( \\bar{p}_z \\), must be steeper than the slope of \\( f_2 \\), which is \\( -b_g^2 \\). This yields the first condition, which is\n\\[\n\\bar{p}_z < -b_g^2.\n\\]\n(S2)\n\n(ii) At the points where the slope of the two functions are the same, the absolute value of the linear function must be less than that of the nonlinear function at those points. The condition for the slope of \\( f_2 \\) to be \\( -b_g^2 \\) is\n\\[\n(\\bar{p}_z + \\ln \\cosh \\bar{x}) = 1 - (1 + b_g^2) \\cosh^2 \\bar{x},\n\\]\n(S3)\n\nwhich cannot be solved in closed form. Instead, we can make approximations for small \\( \\bar{x} \\), \\( \\ln \\cosh \\bar{x} \\simeq \\bar{x}^2/2 \\) and \\( \\cosh^2 \\bar{x} \\simeq 1 + \\bar{x}^2 \\). Equation S3 then becomes\n\\[\n\\bar{p}_z + \\frac{\\bar{x}^2}{2} = 1 - (1 + b_g^2) \\left(1 + \\bar{x}^2\\right),\n\\]\n(S4)\n\nFor which the solutions are\n\\[\n\\bar{x}_{\\pm} = \\pm \\sqrt{\\frac{-b_g^2 - \\bar{p}_z}{3/2 + b_g^2}}.\n\\]\n(S5)\nCondition (ii) now becomes simultaneously satisfying \\( f_1(\\bar{x}_+) > f_2(\\bar{x}_+) \\) and \\( f_1(\\bar{x}_-) < f_2(\\bar{x}_-) \\), which is for small \\( \\bar{x}_\\pm \\),\n\n\\[\nb_g (\\bar{p}_y - b_g \\bar{x}_\\pm) \\gtrsim \\bar{p}_z \\bar{x}_\\pm.\n\\] (S6)\n\nInserting Eq. S5 and solving yields the condition for \\( \\chi \\) to be double-welled:\n\n\\[\n\\bar{p}_y^2 < \\frac{(-b_g^2 - \\bar{p}_z)^3}{b_g^2 (3/2 + b_g^2)}.\n\\] (S7)\n\nNote that Eq. S2 is a necessary condition for there to be a solution for \\( \\bar{p}_y \\) in Eq. S7. If a particle does not satisfy Eq. S7, it belongs to the M class.\n\nEven if \\( \\chi \\) is double-welled, a particle still needs to have enough energy to overcome the local hill near \\( \\bar{x} = 0 \\) in order to undergo full double-well motion. Approximating \\( f_2 \\) as \\( \\bar{p}_z \\bar{x} \\), the location of the local hill is at \\( \\bar{x}_{lh} \\simeq b_g \\bar{p}_y / (\\bar{p}_z + b_g^2) \\). The value of the effective potential at this point is, approximately,\n\n\\[\n\\chi(\\bar{x}_{lh}) \\simeq \\frac{1}{2} \\bar{p}_y^2 \\left( 1 - \\frac{b_g^2}{\\bar{p}_z + b_g^2} \\right) + \\frac{1}{2} \\bar{p}_z^2,\n\\] (S8)\n\nwhere terms up to \\( O(\\bar{x}_{lh}^2) \\) are kept. If the particle energy is bigger than \\( \\chi(\\bar{x}_{lh}) \\), it belongs to the DW class, and if not, it belongs to the NC class.\n\nFinally, the sign of \\( \\langle \\bar{v}_z \\rangle \\) must be determined if one wants to further classify the DW and M classes. The bounce-period-averaged \\( \\bar{v}_{z\\sigma} \\) is given by\n\n\\[\n\\langle \\bar{v}_z \\rangle = \\frac{2}{T_0} \\int_{\\bar{x}_{min}}^{\\bar{x}_{max}} \\frac{\\bar{v}_z}{\\bar{v}_x} d\\bar{x},\n\\] (S9)\n\n\\[\n= \\frac{2}{T_0} \\int_{\\bar{x}_{min}}^{\\bar{x}_{max}} \\frac{\\bar{p}_z + \\ln \\cosh \\bar{x}}{\\sqrt{2H - (\\bar{p}_z + \\ln \\cosh \\bar{x})^2 - (\\bar{p}_y - b_g \\bar{x})^2}} d\\bar{x},\n\\] (S10)\n\nwhere \\( T_0 = 2 \\int_{\\bar{x}_{min}}^{\\bar{x}_{max}} d\\bar{x}/\\bar{v}_x \\) is the bounce period, and \\( \\bar{x}_{min} \\) and \\( \\bar{x}_{max} \\) are solutions to\n\n\\[\n\\frac{1}{2} (\\bar{p}_z + \\ln \\cosh \\bar{x})^2 + \\frac{1}{2} (\\bar{p}_y - b_g \\bar{x})^2 = 0.\n\\] (S11)\n\nIf \\( \\langle \\bar{v}_z \\rangle > 0 \\), the particle belongs to the \\( + \\) class, and to the \\( - \\) class otherwise.\n\nIf the DW and M classes are further divided into DW± and M± classes based on the sign of \\( \\langle \\bar{v}_z \\rangle \\), there are a total of five orbit classes for a current sheet under a finite guide field. Figure 2 shows the distribution classification of the five orbit classes. Extended Data Figs. 2a-c should be compared with Figs. 3a-c.\nParticle-in-cell simulation\n\nThe open-source, fully-relativistic particle-in-cell code, SMILEI [47], was used. The simulation domain was \\(10\\lambda = 100d_i\\), which was divided into \\(2^{15} = 32,768\\) grid points. The boundary conditions for the electromagnetic fields and particles were Silver-Müller and periodic, respectively. Two simulations were conducted, one with (i) \\(c/v_A = 2\\) (Extended Data Fig. 3) and another with (ii) \\(c/v_A = 20\\) (Extended Data Fig. 4). For case (i), 10,000 particles were placed per cell and the simulation was run for \\(100\\omega_{ci}^{-1}\\) with timestep \\(\\Delta t = 7.63 \\times 10^{-4}\\omega_{ci}^{-1}\\), and for case (ii) 100 particles were placed per cell and the simulation was run for \\(250\\omega_{ci}^{-1}\\) with timestep \\(\\Delta t = 7.63 \\times 10^{-5}\\omega_{ci}^{-1}\\). In both cases, the initial condition was a Harris sheet with the ion and electron temperatures set as one-fifth of the equilibrium temperature, i.e., \\(T_{i,e} = 0.2T_{eq}\\) where \\(T_{eq} = B_0^2/(4\\mu_0 n_0 k_B)\\), and with a uniform seed guide field of strength \\(0.15B_0\\). Streak plots of the out-of-plane inductive electric field \\(E_z\\) are shown for (i) \\(c/v_A = 2\\) (Extended Data Fig. 6a) and (ii) \\(c/v_A = 20\\) (Extended Data Fig. 6b). The peak values of \\(E_z\\) are around 0.3 and 0.6, respectively.\n\nThe simulations were run on the KAiros computer cluster at Korea Institute of Fusion Energy.\n\nMMS data and LMN coordinate system\n\nMMS1, MMS2, and MMS3 data from 05:26:41.7 to 05:26:43.7 UT on 3 July 2017 were averaged to yield the profiles in Figs. 6a-f. MMS4 data were omitted because it was not available from the import method provided by the pySPEDAS package [48], which was used for extracting the data. 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Wendel was supported by the NASA Magnetospheric Multi-Scale Mission in association with NASA contract NNG04EB99C. Y. D. Yoon was supported by the PIURI fellowship of POSTECH and the POSCO Science Fellowship of POSCO TJ Park Foundation. The particle-in-cell simulations presented here were conducted on the KAIROS computing cluster at Korea Institute of Fusion Energy.\n\nEXTENDED DATA FIGURES\nExtended Data FIG. 1. Two functions that contribute to \\( d\\chi/d\\bar{x} \\) for \\( \\bar{p}_y = 0.1, \\bar{p}_z = -0.1, \\) and \\( b_g = 0.2 \\).\n\n![Two curves labeled \\( b_g(\\bar{p}_y - b_g x) \\) and \\( (\\bar{p}_z + \\ln \\cosh x) \\tanh x \\) plotted against \\( x \\)](page_374_186_591_377.png)\nExtended Data FIG. 2. **Particle distribution in phase space, velocity space, and physical space.** Phase space distributions of the five orbit classes distinguished by the blue, magenta, green, red, black colors in **a** (\\( \\bar{x}, \\bar{v}_x \\)), **b** (\\( \\bar{x}, \\bar{v}_y \\)), and **c** (\\( \\bar{x}, \\bar{v}_z \\)) spaces. Histograms of particles satisfying \\( \\bar{x} > 0 \\) in **d** \\( \\bar{v}_x \\), **e** \\( \\bar{v}_y \\), and **f** \\( \\bar{v}_z \\) spaces. The dotted lines and arrows are respectively the average velocities and two standard deviations of each distribution. **g** Particle histogram in \\( \\bar{x} \\). The red and green lines in **d-g** are amplified five and ten times, respectively, so that they are visible on the same plot.\nExtended Data FIG. 3. Streak plots of variables from the particle-in-cell simulation with \\( c/v_A = 2 \\). Streak plots of the magnetic fields a \\( B_y \\) (sheared field), b \\( B_z \\) (out-of-plane field), the current densities c \\( J_y \\) (sheared current), d \\( J_z \\) (out-of-plane current), e ion temperature \\( T_i \\), and f electron temperature \\( T_e \\) from \\( t = 0 \\) to \\( 100\\omega_{ci}^{-1} \\).\n\n![Streak plots of variables from the particle-in-cell simulation](page_184_120_1207_670.png)\nExtended Data FIG. 4. Streak plots of variables from the particle-in-cell simulation with \\( c/v_A = 20 \\). Same as Fig. 3, but for \\( c/v_A = 20 \\).\n\n![Streak plots of variables from the particle-in-cell simulation with c/v_A = 20](page_186_153_1217_693.png)\nExtended Data FIG. 5. Comparison of a simulated sheet with an initial dip in the guide field with MMS spacecraft observations. Same as Fig. 6, but the simulated current sheet in the right panels had an initial dip in the guide field that carries over to the final configuration (inset in g).\n\nExtended Data FIG. 6. Streak plots of \\( E_z \\). Streak plots of the inductive out-of-plane electric field \\( E_z \\), for **a** \\( c/v_A = 2 \\) and **b** \\( c/v_A = 20 \\).\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• GUIDEDOA2200435reportingsummary.pdf"} {"paper_id": "prb19", "title": "Polarisation of Decayless Kink Oscillations of Solar Coronal Loops", "text": "Polarisation of Decayless Kink Oscillations of Solar Coronal Loops\n\nSihui Zhong\nUniversity of Warwick https://orcid.org/0000-0002-5606-0411\nValery Nakariakov (V.Nakariakov@warwick.ac.uk)\nUniversity of Warwick https://orcid.org/0000-0001-6423-8286\nDmitrii Kolotkov\nUniversity of Warwick https://orcid.org/0000-0002-0687-6172\nLakshmi Pradeep Chitta\nMax Planck Institute for Solar System Research https://orcid.org/0000-0002-9270-6785\nPatrick Antolin\nNorthumbria University https://orcid.org/0000-0003-1529-4681\nCis Verbeeck\nRoyal Observatory of Belgium\nDavid Berghmans\nRoyal Observatory of Belgium\n\nArticle\n\nKeywords:\n\nPosted Date: March 16th, 2023\n\nDOI: https://doi.org/10.21203/rs.3.rs-2648489/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nAdditional Declarations: There is NO Competing Interest.\n\nVersion of Record: A version of this preprint was published at Nature Communications on September 12th, 2023. See the published version at https://doi.org/10.1038/s41467-023-41029-8.\nPolarisation of decayless kink oscillations of solar coronal loops\n\nSihui Zhong1, Valery M. Nakariakov4,2, Dmitrii Y. Kolotkov1,\nLakshmi Pradeep Chitta3, Patrick Antolin4, Cis Verbeeck5 David Berghmans5\n\n1Centre for Fusion, Space and Astrophysics, Physics Department, University of Warwick,\nCoventry CV4 7AL, UK\n2Centro de Investigacion en Astronomia, Universidad Bernardo O'Higgins,\nAvenida Viel 1497, Santiago, Chile\n3Max Planck Institute for Solar System Research, D-37077 Göttingen, Germany\n4Department of Mathematics, Physics and Electrical Engineering, Northumbria University,\nNewcastle Upon Tyne, NE1 8ST, UK\n5Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium,\nRinglaan -3- Av. Circulaire, Brussels, 1180, Belgium\n\nAbstract\nDecayless kink oscillations of plasma loops in the solar corona may contain an answer to the enigmatic problem of solar and stellar coronal heating. The polarisation of the oscillations gives us a unique information about their excitation mechanisms and energy supply. However, unambiguous determination of the polarisation has remained elusive. Simultaneous detection of a 4-min decayless kink oscillation from two non-parallel lines-of-sights, separated by about 104 degrees, provided by unique combination of the High Resolution Imager on Solar Orbiter and the Atmospheric Imaging Assembly on Solar Dynamics Observatory, reveals, for the first time, a horizontal or weakly oblique linear polarisation of the oscillation. This conclusion is based on the comparison of observational results with forward modelling of the observational manifestation of various kinds of polarisation of kink oscillations. The revealed polarisation favours the sustainability of these oscillations by quasi-steady flows which may hence supply the energy for coronal heating.\n\n1 Introduction\nThe outermost, fully-ionised and magnetically-dominated part of the atmosphere of the Sun, the corona, attracts our attention as the birthplace of extreme events of space weather, such as flares and coronal mass ejections[1]. The corona is a natural plasma physics laboratory allowing for high-resolution study of basic phenomena which are of interest for various astrophysical, geophysical and laboratory plasma physics applications. The corona offers us several enigmatic puzzles, such as the rapid release of the magnetic energy, and heating of the plasma to temperatures about three orders of magnitude higher than the surface temperature.\nOne of the most rapidly developing avenues of modern coronal physics is the study of magnetohydrodynamic (MHD) wave phenomena, see, e.g.[2]. Coronal waves are of specific interest as possible agents of coronal heating, see, e.g.[3] seismological probes of the coronal plasma structures e.g.[4,6,7] and an important element of flaring energy releases, e.g.,[5]. A ubiquitous phenomenon are transverse, or kink, oscillations of coronal plasma loops[8], which appear in two different regimes. Large-amplitude rapidly-decaying kink oscillations are normally excited by displacements of the loops from the equilibrium, caused by low-coronal eruption,[10] and decay by resonant absorption (e.g.,[1]) and/or by Kelvin–Helmholtz instability (e.g.,[12,13]). The nature of another type, low-amplitude decayless kink oscillations,[14,15,16,17] is subject to intensive ongoing studies. The mechanisms which could counteract the oscillation damping are random footpoint movements, e.g.[18,19,20] and quasi-stationary coronal, chromospheric or photospheric flows, e.g.[21,22,23], or their combination[24]. Alternative mechanisms for the apparent decayless behaviour are the Kelvin–Helmholtz instability[25] and a\npattern of interference fringes[26]. In addition, field-aligned flows such as coronal rain could be accompanied by decayless kink oscillations[27,28].\n\nIn contrast with large-amplitude decaying kink oscillations which are relatively rare and therefore cannot contribute to coronal heating, the ubiquity of decayless kink oscillations makes them an important process for the coronal energy balance[29]. As it has been shown in[29], decayless kink oscillations can represent a significant energy input in the loop. In other words, their relatively low amplitudes are not representative of the total amount of energy converted by this process. In this context, a crucial question is the mechanism which counteracts the oscillation damping and hence is responsible for the energy supply to the corona. One of the key indicators of the oscillation excitation mechanism and hence of such an energy supply mechanism is the oscillation polarisation. For example, decaying kink oscillations polarised in the horizontal and vertical directions have been observed to be excited by a non-radial eruption of a magnetic flux rope[30]. Likewise, the coronal rain has been shown to lead to vertically polarised transverse oscillations of a loop in 2.5D MHD simulations[28].\n\nIn a few very rare cases when the top segments of the oscillating loops were parallel to the line-of-sight (LOS), the polarisation of large-amplitude decaying kink oscillations could be determined[11,12]. Another potential opportunity appears if imaging observations are supplemented with spectroscopic observations[31]. However, only stereoscopy, i.e., observations from different vantage points would allow one to study 3D geometry of kink oscillations properly. So far, there has been only one attempt to estimate the polarisation plane stereoscopically, for a large-amplitude decaying regime[4]. The oscillation with a period about 10.5 min, damping time about 17 min, and initial amplitude of about 4 Mm was detected with the Extreme Ultraviolet Imager (EUVI) instruments on board the two Solar TErrestrial RElations Observatories (STEREO). The instruments had a temporal resolution of 2.5 minutes, and the pixel sizes 1100 km and 1240 km, respectively. The two STEREO spacecraft were separated by 15.4 degrees. Unfortunately, in that observation the footpoints of the oscillating loop were behind the limb for both vantage points. Thus, the stereoscopic reconstruction was based on the observations of footpoints three days later than the oscillation event, when the loop was not visible. An additional information used in this study was the perturbation of the emission intensity in the loop, caused by the variation of the column depth in the optically thin regime. Assuming that the oscillation was linearly polarised, it was deduced that the oscillation was polarised rather horizontally. This result is consistent with the excitation of a large-amplitude decaying kink oscillation by an impulsive displacement[10].\n\nFor decayless oscillations, until the commissioning of high-resolution EUV imagers of the new generation, it has not been possible to determine the polarisation sense and constrain the mechanism by which the energy is transferred to the corona to sustain the oscillation. In particular, one would expect that random footpoint motions result in a randomly varying polarisation. Simultaneous observations of a decayless kink oscillation with the Atmospheric Imaging Assembly (AIA)[32] on board the Solar Dynamics Observatory (SDO)[33], and the Extreme Ultraviolet Imager (EUI)[34] on board the recently launched Solar Orbiter (SolO,[35]) allow us to determine, for the first time, polarisation properties of this phenomenon. Here, we report simultaneous high-resolution detection of decayless kink oscillations of a coronal loop with two non-parallel LoS, identify the type of polarisation of the observed mode, and draw important conclusions concerning the driving mechanism.\n\n2 Results\n\n2.1 Spacecraft constellation\n\nDuring 09:19 to 10:34 UT on April 1st 2022, when the Solar Orbiter (SolO) was near the perihelion of its orbit, HRIEUv (EUI’s High Resolution Imager which observes the Sun in the 174 Å passband[37]), detected decayless kink oscillations in a bundle of loops on the solar disk near the limb. The oscillating loops were situated at the outskirt of NOAA active region (AR) 12976 (Fig. 1) of the β Hale class. Thanks to its unprecedentedly high spatial resolution, 123 km for each pixel, the oscillations can be well seen by eye in the movie constructed by a sequence of images (see Supplementary Movie 1, left). Meanwhile, AIA took images of the same bundle of loops from a different LoS, see the left panel in Fig. 1. As the spatial resolution of AIA images (435 km/pixel) is about 3.5 times HRIEUv’s, the low-amplitude oscillations recorded by AIA are not resolvable by naked eye in the movie. However, the oscillations were clearly detected in a movie\nprocessed with the motion magnification technique (Supplementary Movie 1, right). No flares or CMEs are reported in this AR during the observations. During the observation, the distance from the Sun for SoIO is 0.350 a.u., and that for SDO is 0.999 a.u. Therefore, the light travel time difference between two spacecrafts was 325.5 second (5.4 min). The Carrington longitude and latitude of centers of the field-of-view (FoV) for HRIEUV and full-disk SDO/AIA data roughly [135.5 degrees, 2.3 degrees] and [31.8 degrees, -6.5 degrees] respectively. The angle separation between the two LoS was 103.95 degrees.\n\n2.2 Oscillation properties\n\nAs shown in Supplementary Movie 1, the oscillating loop bundle consists of multiple strands which perform a collective transverse oscillation. Therefore, rather than analysing a specific strand, we treat the bundle as a single entity. From HRIEUV’s view (Fig. 2b and Supplementary Movie 1, left), only one leg and the apparent apex of the oscillating loop bundle can be clearly identified. The footpoints are not clearly seen, and the other leg is overlaid by another loop coming into LoS in the second half of the analysed time interval. In AIA images (Fig. 2c and Supplementary Movie 1, middle), the footpoints and one leg are well visible, but some segments of the oscillating bundle are overlapped with bright plasma flows in the background most of the time. The HMI LoS magnetogram shows that the loops forming the bundle connect a pair of photospheric magnetic patches of opposite polarities, see the red and blue contours overlaid on a coronal AIA EUV image in Fig. 2f. Time–distance maps were constructed for some particular loop segments whose transverse oscillations were well resolvable, with slits put across the loop (Fig. 2b1–b3 and d1–d3). Both HRIEUV and AIA time–distance maps demonstrate transverse oscillatory patterns. The oscillations appear to be almost monochromatic, and last for tens of cycles. The oscillation amplitudes do not show systematic decay or growth, which is typical for the decayless regime (e.g., [11]).\n\nThe oscillatory patterns are clearly evidenced in time–distance maps constructed for various perpendicular slits. To make the narrative easier, the loop bundle is divided into three segments – Leg 1, (apparent) Apex, and Leg 2. For oscillations detected by HRIEUV (Fig. 2b1-b3), the apparent displacement amplitude is seen to increase towards the apex. Moreover, detrended oscillations of different segments of the loop appear to be in phase with each other (Fig. 3a). This behaviour is consistent with the fundamental kink mode (see [12]). This conclusion is also confirmed by the in-phase oscillatory patterns detected with AIA in Leg 1, Apex, and Leg 2 (Fig. 3d). Note that oscillations in AIA data set are less clear due to the lower resolution and the abrupt interruption of the background evolution during the observation. In particular, slits 13, 28, and 41 show the most clear oscillation examples in the corresponding loop segments. Only those slits which do not show significant deviations from a quasi-oscillatory pattern are accepted for further analysis. Fig. 3b displays Fourier power spectra of the oscillatory patterns made for different slits with the use of HRIEUV. As the analysed oscillation is the fundamental mode, i.e., all segments of the loop oscillate in phase, we may improve the signal-to-noise ratio by averaging the spectra over a particular segment, see Fig. 3c. The oscillations detected in legs and at the apex have the same power peak at about 4 min, which further corroborates the detection of the fundamental mode. Likewise, the AIA data demonstrate the domination of 4-min oscillations in all segments of the loop (Fig. 3e and f). The nature of the minor peaks at about 8–9 min (HRIEUV) or 6–12 min (AIA) is not clear, but it is not relevant to the analysis of 4-min oscillations.\n\nThe determination of the oscillation polarisation is based on the estimation of the phase difference between oscillations detected with HRIEUV and AIA, i.e., from two different vantage points (see Section I.2). As the phase comparison requires the adjustment of the time scales, the light travel time correction is applied to the AIA signal, allowing us to account for the difference in the distances from the Sun to the spacecraft. In addition, the instantaneous amplitudes are normalized by their envelope, to remove the amplitude modulation. In order to minimize the effect of background noise, the transverse displacements are averaged over five neighbouring slits (around 10 Mm wide segment) near the apparent apex in both data sets. Eleven oscillation cycles were detected in the common time interval. As shown in Fig. 4a1, original signal-pairs seem to be approximately in anti-phase. The cross-correlation coefficient calculated with different time lags peaks at a time lag of 120 s, almost exactly at half of the oscillation period (4 min). Thus, the phase shift is about 180 degrees. Also, we constructed a phase portrait (also called a hodogram, Fig. 4b2) of the normalised oscillatory patterns detected with AIA and HRIEUV (see [4]). The hodogram demonstrates that, in general, the shape of most of the mutual oscillation cycles is approximately elliptical with a high eccentricity and negative inclination. Given that the amplitudes are normalised, the eccentricity\nFigure 1: Left: The location of SDO and the Solar Orbiter during the observations. Right: An AIA 171 Å image indicating the region of interest (the red box). Oscillating loops are denoted by the white arrow. The blue quadrilateral indicates the field of view of HRIEUV, projected onto the AIA image plane.\n\nof the ellipse coincides with the length of its minor axis. To simplify the measurement, the pattern is rotated clockwise with 45 degrees so that the minor axes of the ellipses related to various oscillation cycles appear in the horizontal direction, as displayed in panel a3. The histogram of the distribution of the minor axis lengths approaches a Gaussian. The average length of the minor axes, \\( \\sigma \\), is estimated by the width (standard deviation) of the best fitted Gaussian, resulting in \\( \\sigma = 0.19 \\). Thus the ratio of the major and minor axes of the hodogram ellipses is \\( 0.19/0.7 = 0.27 \\), where 0.7 is the half width of the major axis.\n\nTo get rid of the undesired noisy fluctuations beside the 4-min oscillation, we filter out the time-series data with peak frequency with a 30-s window, resulting in cleaner oscillatory signals, as displayed in Fig. 4b. Similar to the original signals, the filtered oscillatory signals detected with AIA and HRIEUV appear to be out of phase with each other. The cross-correlation coefficient peaks at a time lag of -0.48 periods, indicating a phase shift of 174 degrees. As shown in Fig. 2b2-b3, the hodogram trajectory of each cycle is a narrow ellipse with \\( \\sigma = 0.08 \\) and an elongation ratio of 0.11. Repeating the above analysis with the signals averaged over 7 slits near the apex, similar results are obtained: the oscillatory signal detected with AIA and HRIEUV are in anti-phase, and the hodogram trajectories are highly elliptical, with \\( \\sigma = 0.05 \\) in the minor axis.\n\n2.3 Polarisation signatures in forward modelling\n\nWith the analytical model detailed in Sec. 4.2 we reproduce kink oscillations of a 3D loop with different types of polarisation, as seen in the LoS of HRIEUV and AIA (see Figs. 5,6). Projecting the modelled loop onto the planes-of-sky (PoS) of HRIEUV and AIA (Fig. 5), the simulated 2D images are seen to reproduce well the observed geometry. The dynamics of the modelled loop, manifesting harmonic kink oscillations of different polarisation (i.e. horizontal, vertical and oblique linear with respect to the loop’s plane, and also circular, and elliptical) in the HRIEUV (left) and AIA (right) LoS, is shown by Supplementary Movie 2. For all types of polarisation seen in the simulated AIA LoS, oscillations of all loop segments are in phase, as it is expected for the fundamental kink mode and is consistent with observations (see Fig. 3). Likewise, kink oscillations seen in the modelled HRIEUV LoS in Leg 2 and near the loop apex are also in phase for all types of the polarisation (Leg 1 is not well seen in HRIEUV observations, hence cannot be used for comparison).\n\nOn the other hand, each type of polarisation is expected to have its own characteristic signatures, specific for the considered combination of AIA and HRIEUV observations. To reveal these distinct signatures, we apply the same time–distance analysis to the synthetic data sets as it has been done for revealing the observed\nFigure 2: Decayless kink oscillations of the analysed loop bundle. The oscillating loop shown in HRIEUV (panel a) and AIA (panel c) images is best-fitted with truncated ellipses (white dashed curves). The loop legs are indicated by labels, Leg1 and Leg2. In panel a, the small inset window on the top right displays the full range of the HRIEUV image (2048 × 2048 pixel) and the dark blue box indicates the region shown in panel a. In panel c, the LoS magnetogram is over-plotted to show the magnetic connectivity (positive in red and negative in blue). The slits across the loop are used to make time–distance plots shown on the right (panels b1-b3, d1-d3 for HRIEUV and AIA, respectively). In the time–distance plots, the corresponding slit index numbers are denoted, and the displacements of loop centre/boundary are marked by the red curves. For the AIA data set, the time–distance plots were made with the data processed with the motion magnification coefficient 5.\nFigure 3: Oscillatory transverse displacements of different segments along the analysed loop (panels a and d, for HR1EUV and AIA, respectively), and their Fourier power spectra (panels b and e). Panels a and d show the detrended oscillations signals, obtained by subtracting the trend from original displacements determined by the time–distance maps. The trend is obtained by smoothing the original signals with a window longer than the oscillation period. The colour scheme indicates the slit index numbers, with the dark blue corresponding to smaller numbers. Panels b and e: Fourier power spectra of the transverse displacements of different slits, with the colour scheme showing the spectral power normalised to the maximum. Panels c and f: Spectral power averaged over a particular segment of the oscillating loop.\nFigure 4: Phase shifts between the kink oscillations detected with HRIEUV and AIA. The signals are averaged over 5 slits near the apex. Panels **a** show original signals. Panels **b** show the signals filtered out in the vicinity of the 4-min period with a spectral window of 30 s. The AIA signals are shifted forwards in time by 325.5 s to compensate the light travel time difference. In panels **a1** and **b1**, the signals are shown as a function of time. Panels **a2** and **b2**, display hodograms of the oscillatory signals. The colour code indicates different oscillation cycles. Panels **a3** and **b3** demonstrate the estimation of the elongation ratio \\( \\sigma \\).\noscillation properties in Sec. [2.2]. Namely, we select segments of the modelled loop projected on the planes-of-sky (PoS), similar to those used in the observations (see Fig. 2 and the green and red slits in Fig. 5). In particular, Fig. 6 shows synthetic time–distance maps with the modelled kink oscillatory patterns of different polarisation seen with two LoS, taken at the slit situated near the loop apex (i.e., near the location of the maximum oscillation amplitude).\n\nExtracting the loop boundary displacements obtained in two LoS from the modelled time–distance maps (see Fig. 6 c1–c5), we calculate their phase difference and simulate hodograms (see Fig. 6 d1–d5). In the case of horizontal and oblique polarisations, the oscillatory AIA and HRIEUV signals appear to be in anti-phase, and the resulting phase portrait shows a narrow structure with a negative gradient (panels d1 and d3). For vertical polarisation, the AIA and HRIEUV signals are in phase, also resulting in a narrow phase trajectory but with a positive gradient (panel d2). For the circular polarisation, oscillations taken in two LoS are about −120 degrees out of phase with each other, leading to an elliptical trajectory in the hodogram, with the ratio of the major to minor axes about 0.6 (panel d4). Similarly, in the case of the elliptical polarisation, oscillations are about −144 degrees out of phase, making a narrower ellipse with the axes ratio of 0.45 in the phase portrait. Thus, we consider the time phase difference between AIA and HRIEUV oscillatory signals and the corresponding hodogram shapes as distinct characteristic signatures of different kink polarisation types, to be compared with observations.\n\nIn addition, for the oblique and elliptical polarisations in the AIA LoS, oscillation profiles manifest distortions from a harmonic shape, so that the waveforms of the AIA signals in panels c3 and c5 are asymmetric with respect to the horizontal and vertical axes, respectively. This, in turn, leads to the skewness of the corresponding phase trajectories in hodograms (panels d3 and d5), which however remains small. As the kink oscillations are assumed to be linear in the model (see Eqs. 4 and 5), these waveform distortions are attributed to projection effects only. Similar skewed waveforms have been observed in, e.g., decaying kink oscillations of a flux rope[32].\n\n2.4 Determination of polarisation\n\nComparison of Figs. 4 and 6 allows us to exclude the possibility of the vertical polarisation in the observed decayless event, as the in-phase behaviour of the simulated AIA and HRIEUV signals and the phase portrait with a positive gradient are not consistent with observations. The other four types of polarisation result in the phase portraits of the AIA and HRIEUV signals with a negative gradient, and thus are in general agreement with the observed oscillation properties. Moreover, the observed phase delay of 174 degrees between oscillations in two LoS is broadly consistent with the horizontally, obliquely, and elliptically polarised oscillation models, taking the observational and data analysis uncertainties into account. However, only models with horizontal and oblique linear polarisations successfully reproduce the localisation of the majority of phase trajectories near the major axis in the observed elliptical hodogram in Fig. 4. In other words, the observed Gaussian distribution of the minor axes in the right column of Fig. 4 can be caused by the horizontal or oblique linear polarisation of oscillations only, whereas the finite width of the obtained Gaussian peak can be attributed to noise of the instrumental or another origin.\n\nThe further discrimination between horizontal and oblique linear polarisations can be based on a skewed hodogram shape of the latter, caused by the distortion of the oscillation profiles from a harmonic shape due to projection effects as discussed in Sec. 2.3. However, as this effect is found to be rather minor in modelling, it is most likely to be obscured by noise in the top panels of Fig. 4. Suppression of noise by narrow-band Fourier filtering (bottom panels in Fig. 4), described in Sec. 2.2 cannot account for this skewness due to the essentially harmonic nature of the Fourier transform. Hence, we conclude that the horizontal and oblique linear polarisations of decayless kink oscillations are equally possible in the observed event.\n\n3 Discussion\n\nThe paper presents unprecedented high-resolution detection of a decayless kink oscillation of a coronal loop, observed simultaneously from two vantage points by the spaceborne EUI/HRIEUV and AIA EUV imagers onboard the Solar Orbiter and Solar Dynamics Observatory missions, respectively. The oscillatory signals detected by HRIEUV and AIA, i.e., projected on differently oriented PoS, are found to be nearly anti-phase. The mutual hodograms of the signals are highly elliptical, with a ratio of the major and minor axes\nFigure 5: Modelling an oscillating coronal loop observed in two non-parallel LoS mimicking that of the HRIEUV and AIA observations. The first row: the modelled loop, LoS, and plane-of-sky (PoS), seen in different views. The green and red normal vector and the plane indicate the LoS and corresponding PoS of HRIEUV and AIA images, respectively. The second and third rows: Projection of the 3D loop onto a particular PoS (left) and the resulting simulated image (middle), with the observational image (right) for comparison. The second row is for the modelled HRIEUV LoS, and the third is for AIA. The slits cover the segments similar to those analysed in the observations. The stars denoted the slits which are used to make TD maps in Figure 6\nFigure 6: Simulated oscillatory patterns seen in two LoS similar to that of observations, considering different types of polarisation indicated in the left column. Representative time-distance maps revealing oscillations viewed in LoS mimicking HRI’s (a1–a5) and AIA’s (b1–b5) view. The TD maps are made using slits marked by the stars in Fig. 3. The oscillatory signals from two LoS are combined to reveal their correlation (c1–c5). Panels (d1–d5) show the mutual hodograms of the oscillatory signals.\nof the ellipses of 0.11. To interpret the observations and determine the type and sense of the oscillation polarisation, we designed an analytical model which mimics the manifestation of the oscillations of certain polarisation, e.g., the linear polarisation with different orientations of the oscillation plane, and elliptical and circular polarisations, in the PoS of HRIEUV and AIA. We conclude that the detected kink mode is linearly polarised with the polarisation plane being highly horizontal, i.e., it is either horizontal or oblique with a strong horizontal component.\n\nThis finding has important implications for the problem of the energy balance in the solar corona. The ubiquitous nature of decayless oscillatory transverse displacements of coronal plasma loops requires a persistently operating mechanism which counteracts processes responsible for the oscillation decay. In particular, in the other, large-amplitude decaying regime, kink oscillations of coronal loops are seen to damp in a few oscillation cycles, i.e., the damping mechanism is very effective. The mechanism is linked with the effect of resonant absorption. Essentially, this effect is linear, and hence should work in low-amplitude oscillations too. The mechanisms proposed to compensate the energy losses in a loop which is not excited by any flare or eruption, are the random movements of footpoints or the interaction of the loop with quasi-steady flows. The mechanism based on KHI requires the oscillation to be excited somehow, which often is not observed. The mechanism based on existence of a periodic driver, e.g., the leakage of 5-min or 3-min oscillations typical for the lower atmospheric layers is excluded because of the established dependence of the decayless oscillation period on the length of the oscillating loop[17] and the lack of resonant peaks in the distribution of the detected oscillation periods.\n\nIf the decayless oscillation is sustained by random footpoint movements, the movements are likely to be randomly directed in the horizontal plane. In other words, the horizontal motions are not likely to have a prescribed direction which could be anyhow connected with the orientation of the plane of the loop. Thus, we expect that random, in the horizontal direction, motions of footpoints should result in randomly polarised oscillatory motions of the loop. This picture is inconsistent with the observed behaviour. Vertical random motions, i.e., random upflows or downflows, may sustain only vertically polarised kink oscillations as the centrifugal force is directed along the major radius of the loop, e.g.[4], which does not match the observations either. On the other hand, the self-oscillatory scenario based on the interaction of the loop with steady flows[22][23] that are perpendicular to the loop plane can readily explain the observed stable horizontal (or an oblique, but with a large horizontal component) polarisation. It can be illustrated by transverse self-oscillations of a violin string, excited and sustained by a steady motion of a bow. The oscillations loose energy to sound waves, while their amplitude, i.e., the sound volume, could remain at the same level for a number of oscillation periods. The energy lost by the sound wave radiation, aerodynamic friction, and friction at the pegbox and bridge, is compensated by the negative friction between the string and the bow. Importantly, the oscillation is essentially linearly polarised in the direction along the bow motion.\n\nThe self-oscillatory scenario implies that the external plasma motions responsible for the decayless regime change at a characteristic time scale much longer than the oscillation period. In other words, the main energy is in the low-frequency part of the spectrum, such as, in particular, in the case of red or pink noise. Dynamic processes of this kind are typical for the solar atmosphere[45][46]. In addition, in 3D MHD simulations of the quiet Sun and coronal arcade, the time scale of coronal energy transport and release is expected to be 20–50 min[17], i.e. about an order of magnitude longer than typical oscillation periods. In the context of the coronal energy balance, this finding indicates that coronal loops can readily obtain the energy from the low-frequency, high-energy spectral band of the solar atmospheric dynamics, well outside the resonant kink frequencies of the loops. As kink oscillations are not leaky, the energy remains inside the loops until it is converted into the internal energy of the coronal plasma. The total energy budget of an oscillating loop could be inferred from the combination of the kinetic energy of kink oscillations counteracted by damping, free magnetic energy, non-thermal energy of accelerated particles, etc. From the current observation, we estimate the kinetic energy of the observed decayless kink oscillations to be as tiny as \\(10^{22} - 10^{23}\\) ergs. However, this figure does not correspond to the energy going into heat, as it is rather a surplus between total energy gains and resonant damping losses in the loop. The dependence of the estimated energy on the oscillation properties such as velocity amplitude could be more complicated, as in the violin scenario, for example, the friction between the string and the bow depends not only on the bowing velocity[45][46]. According to the findings of[29], this estimation is a very low limit of the actual energy converted into heat by this phenomenon.\n4 Methods\n\n4.1 Data processing and analysis\n\nThe imaging data from HRIEUV have a time cadence of 10 s, pixel size of 0.492 arcsec, and FoV of 2048 × 2048 pixels. The HRIEUV data is internally aligned using a cross correlation technique[50] to remove the spacecraft jitters. The co-temporal AIA images in 171 Å have a time cadence of 12 s and pixel size of 0.6 arcsec. The HMI LoS magnetograms have spatial resolution of 0.5 arcsec/pixel. The location map of SDO and SolO is created using the propagation tool (http://propagationtool.cdpp.eu/).\n\nThe same oscillating loop in two data sets is identified based on the surrounding common features including the magnetic connectivity. Additionally, scc_measure.pro, a tie-pointing SolarSoft procedure is implemented to double-confirm the identity. With the help of it, the leg ahead in the HRIEUV images is found to be the right leg in the AIA images.\n\nThe motion magnification technique is a robust tool to help detecting low-amplitude quasi-periodic transverse movements in the PoS in imaging data whose spatial resolution does not allow visual inspection by naked eye. The technique we employed is based on the 2D dual-tree complex wavelet transform. The method magnifies the displacement amplitude linearly by a user-defined factor, without changing the oscillation period.[59] The algorithm is briefly summarised as follow. First, the input images are decomposed by the dual-tree complex wavelet transform into different scales of high-pass images and low-pass images, and the relative phases of each pixel of high-pass images are calculated. Then the phase trend is smoothed over a user-defined width which is expected to be longer than the movement period. After that, the detrended phase, i.e., the phase with the trend subtracted, is multiplied by the magnification factor. Finally, the sum of the phase trend and magnified detrended phase are delivered to synthesize the magnified image sequence via the inverse dual-tree complex wavelet transform. For AIA data sets, we apply this technique to magnify the tiny transverse periodic motions. The magnification factor is within 5-10 depending on the original and desired amplitude.\n\nTo analyse the oscillations, a time–distance (TD) analysis routine is applied. In each data set, the oscillating loop is first best-fitted with a truncated ellipse. Then several slits perpendicular to the loop segments are put evenly along the ellipse to record the transverse profile at each time frame, and then time-varying profiles are tiled into a TD map. The slit is of 5 pixels in width, and in each frame, the profile is averaged over 5 pixels to reduce noise. In TD maps, the oscillatory patterns at a particular location are revealed. To track the oscillations, a transverse intensity profile of the oscillating loop (or its derivative) at each instance of time is best fitted with a Gaussian to obtain the location of the loop centre (or boundary). In this way, the time variation of the displacement of a certain loop segment is obtained. Further, the background trend is obtained by smoothing the original time series of the oscillatory displacement with a window slightly longer than the period. Then the trends are subtracted from the original signals. Oscillation periods are estimated via the Fast Fourier transform.\n\nAs mentioned in Sec. 2.1, the angle separation between SolO and SDO is 103.95 degrees, constructing a quasi-quadrature configuration. Thus, oscillations from these two data sets can be treated as two almost perpendicular components, whose trajectories in the phase plane construct a phase portrait (also known as hodogram) to reveal their phase and frequency differences. Similar to a Lissajous figure, the shape of such a hodogram carries information about the polarisation of the observed oscillations. Generally, a line, a circle, and an ellipse, is expected for linear, circular, and elliptical polarisation, respectively. In our work, we assign the normalized displacement amplitude of AIA and HRIEUV as \\( x \\) and \\( y \\) component respectively, and make a plot of \\( y \\) as a function of \\( x \\), see Fig. 4.2–b2.\n\n4.2 The geometrical model\n\nTo interpret the observed oscillation properties, we set up a geometrical model for a 3D coronal loop exhibiting fundamental kink oscillations with different types of polarisation.\nThe loop is described as a semi-torus in 3D space with Cartesian coordinates[51],\n\n\\[\nx = (R + r \\cos \\phi) \\cos \\theta,\n\\]\n\\[\ny = (R + r \\cos \\phi) \\sin \\theta,\n\\]\n\\[\nz = r \\sin \\phi,\n\\]\n\nwhere \\( R = 15 \\) and \\( r = 1 \\) are the normalised major and minor radii of the loop, \\( \\theta \\in [0, \\pi] \\) is the angle along the loop axis, and \\( \\phi \\in [0, 2\\pi] \\) is the angle in the azimuthal direction.\n\nIn this work, five types of polarisation with respect to the loop’s plane (\\( x, y \\)) are considered: horizontal polarisation, vertical polarisation, their linear in-phase combination with the same amplitudes as oblique polarisation, the same amplitudes but 90 degrees out of phase as circular polarisation, 90 degrees out of phase but with different amplitudes as elliptical polarisation. The periodic transverse displacements of the loop boundaries by kink oscillations are implemented by modulating the minor radius as\n\n\\[\nr = 1 + A_0 \\sin \\theta \\sin(m \\phi) \\sin \\omega t\n\\]\n\nfor horizontally polarised oscillations, and\n\n\\[\nr = 1 + A_0 \\sin \\theta \\cos(m \\phi) \\sin \\omega t\n\\]\n\nfor vertically polarised oscillations, where \\( A_0 \\) is the perturbation amplitude which is kept low (\\(< 0.4\\)) for the linear regime, \\( m = 1 \\) indicates the kink symmetry of the perturbation, and \\( \\omega t \\) is the oscillation phase in radians. All other polarisation types are obtained as combinations of Eqs. [4] and [5], described above (see Supplementary Movie 2).\n\nThe modelled kink-oscillating loop is viewed in two particular LoS mimicking those of the HRIEUV and AIA observations considered in this work (see Fig. 5, top row). The LoS is defined by the angle \\( \\alpha \\) with respect to the loop’s plane (\\( x, y \\)), and by the angle \\( \\beta \\) to the footpoints plane (\\( y, z \\)). Thus, for HRIEUV LoS, we use \\( \\alpha = 1.92\\pi \\) and \\( \\beta = -0.06\\pi \\). For AIA LoS, we use \\( \\alpha = 0.56\\pi \\) and \\( \\beta = 0.36\\pi \\). The angle separation between these two synthetic LoS is 109 degrees, which is about the observational one (104 degrees).\n\nBeing normal to the LoS, the planes of sky (PoS) of the HRIEUV and AIA instruments are defined by the normal vector and a fixed point (we select the midpoint between the footpoints here). Then the projections of a 3D loop onto the two PoS are obtained with standard linear algebra transformations. The 2D synthetic images of the kink-oscillating loop are thus created, with the local coordinate system redefined, so that the abscissa/ordinate is parallel/perpendicular to the line connecting the loop footpoints, respectively.\n\nIn the model described, the effects of optical depth are omitted, as we focus on the transverse displacements of the loop boundaries only (as kink oscillations are usually observed).\n\n5 Data Availability\n\nThe data analysed during the current study are obtained from EUI Data Release 5.0 https://doi.org/10.24414/2qfw-tr95 and from the Joint Science Operations Center (JSOC) database http://jsoc.stanford.edu/. The artificial images are available from the authors upon request.\n\n6 Acknowledgements\n\nS.Z. acknowledge support from China Schorlarship Council-University of Warwick joint scholarship. D.Y.K. and V.M.N. acknowledge support from the STFC consolidated grants ST/T000252/1. P.A. acknowledges funding from his STFC Ernest Rutherford Fellowship (No. ST/R004285/2). L.P.C. gratefully acknowledges funding by the European Union (ERC, ORIGIN, 101039844). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them. Solar Orbiter is a space mission of international collaboration between ESA and NASA, operated by ESA. The EUI instrument was built by CSL, IAS, MPS, MSSL/UCL, PMOD/WRC, ROB, LCF/IO with funding from the Belgian Federal Science Policy Office (BELSPO/PRODEX PEA 4000134088, 4000112292, 4000117262,\nand 4000134474), the Centre National d’Etudes Spatiales (CNES); the UK Space Agency (UKSA); the Bundesministerium für Wirtschaft und Energie (BMWi) through the Deutsches Zentrum für Luft- und Raumfahrt (DLR); and the Swiss Space Office (SSO).\n\n7 Author contributions\n\nS.Z. performed the data analysis (both observational and modelling), produced figures, and wrote the Results and Methods sections. V.M.N. proposed the concept of the research, supervised the data analysis and modelling, and wrote the Introduction section. D.Y.K. proposed and developed the model, contributed to forward modelling and interpretation of observations. L.P.C. implemented the internal alignment for HRI data. A.P. identified the analysed event in preliminary observational data. 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Mathews7,8,9, Rohan P. Naidu12, Erica J. Nelson6, Sandro Tacchella10,11, Bryan A. Terrazas13, Rainer Weinberger14\n\n1Dipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy.\n2Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA.\n3Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria, Australia.\n4ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia.\n5Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT, Australia.\n6Department for Astrophysical and Planetary Science, University of Colorado, Boulder, CO, USA.\n7Department of Astronomy & Astrophysics, The Pennsylvania State University, University Park, PA, USA.\n8Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA, USA.\n9Institute for Computational & Data Sciences, The Pennsylvania State University, University Park, PA, USA.\n10Kavli Institute for Cosmology, University of Cambridge, Cambridge, UK.\n11Cavendish Laboratory, University of Cambridge, Cambridge, UK.\n12MIT Kavli Institute for Astrophysics and Space Research, Cambridge, MA, USA.\n13Columbia Astrophysics Laboratory, Columbia University, New York, NY, USA.\n14Leibniz Institute for Astrophysics, Potsdam, Germany.\n\nAbstract\n\nLarge-scale outflows driven by supermassive black holes are thought to play a fundamental role in suppressing star formation in massive galaxies. However, direct observational evidence for this hypothesis is still lacking, particularly in the young universe where star formation quenching is remarkably rapid [1–3], thus requiring effective removal of gas [4] as opposed to slow gas heating [5, 6]. While outflows of ionized gas are commonly detected in massive distant galaxies [7], the amount of ejected mass is too small to be able to suppress star formation [8, 9]. Gas ejection is expected to be more efficient in the neutral and molecular phases [10], but at high redshift these have only been observed in starbursts and quasars [11, 12]. Using deep spectroscopy from JWST, here we show the presence of an outflow of neutral and ionized gas in a massive galaxy observed during the rapid quenching of its star formation, at a redshift of \\( z = 2.445 \\). The outflowing mass is mostly in the neutral phase, and the mass outflow rate is larger than the residual star formation rate, indicating that the gas ejection is likely to have a strong impact on the evolution of the galaxy. We do not detect X-ray or radio activity; however the presence of a supermassive black hole is suggested by the properties of the ionized gas emission lines. We thus conclude that supermassive black holes are able to rapidly suppress star formation in massive galaxies by efficiently ejecting neutral gas.\nWe observed the galaxy COSMOS-11142 as part of the Blue Jay survey, a Cycle-1 JWST program that targeted about 150 galaxies uniformly distributed in redshift \\( z \\) (1.7 < \\( z \\) < 3.5) and stellar mass \\( M_* \\) (\\( \\log M_*/M_\\odot > 9 \\)). COSMOS-11142 is among the most massive targets, with \\( \\log M_*/M_\\odot = 10.9 \\), and is one of the 17 objects that are classified as quiescent according to the rest-frame \\( UVJ \\) colors [13]. This is confirmed by the JWST/NIRSpec spectrum, shown in Figure 1, which covers the rest-frame range from 3000 Å to 1.4 µm and features several stellar absorption lines and relatively weak emission lines from ionized gas. The presence of deep Balmer absorption lines clearly indicates that the galaxy is in the “post-starburst” phase immediately following the rapid quenching of a star formation episode.\n\nWe fit stellar population models to the observed spectroscopy together with the photometry, which covers a wider wavelength range from the ultraviolet to the mid-infrared. The best-fit spectral model is shown in red in Figure 1, and includes stellar light, absorption by dust, and re-emission by dust at longer wavelengths, but does not include the contribution of gas. By analyzing the difference between the data and the model we detect several emission lines due to warm ionized gas: [O II], [Ne III], H\\( \\beta \\), [O III], H\\( \\alpha \\), [N II], [S II], [S III], He I. We also detect three absorption lines, Ca II K, Ca II H, Na I D, which are not correctly reproduced by the stellar model. Unlike the other absorption lines visible in the spectrum, these three are resonant lines, meaning that they can be produced both by stars and by intervening gas, because they involve transitions out of the atomic ground level. The detection of extra absorption in these lines is thus revealing the presence of cold gas. Since the energy required to ionize Na I and Ca II (5.1 and 11.9 eV respectively) is smaller than that required to ionize hydrogen (13.6 eV), these lines probe gas in the neutral atomic phase (i.e., where hydrogen atoms are neutral).\n\nWe fit a Gaussian profile to each gas emission and absorption line, obtaining a measure of their flux, line width \\( \\sigma \\), and velocity offset \\( \\Delta v \\) with respect to the systemic velocity of the galaxy. We show a selection of lines in the left column of Figure 2: a remarkable diversity of kinematics is apparent, with a wide range of measured line widths and velocity offsets. The presence of blueshifted lines, both in absorption and in emission, with velocity offsets of hundreds of km/s is the unmistakable sign of a gas outflow.\n\nWe use a simple model of a biconical outflow, shown in the right column of Figure 2, to qualitatively explain the kinematics of all the observed lines. The five rows of the figure illustrate five different types of lines, classified according to their kinematics, which we discuss here from top to bottom. 1) Low-ionization lines such as [O II] and [S II] have kinematics in agreement with those of the stellar population (i.e., \\( \\Delta v \\sim 0 \\) km/s and \\( \\sigma \\sim 300 \\) km/s), suggesting that they originate in the galaxy and not in the outflow. 2) The neutral absorption lines Na I D and Ca II K are significantly blueshifted with \\( \\Delta v \\sim -200 \\) km/s, and are therefore tracing the foreground gas that is in the approaching side of the outflow. 3) Emission lines with a relatively high ionization energy, such as [O III] and [Ne III], are also blueshifted (\\( \\Delta v \\sim -200 \\) to \\(-400\\) km/s), and are thus likely to originate in the approaching side of the outflow. 4) A special case is [S III], which is also a high-ionization emission line but is observed to be at roughly systemic velocity (\\( \\Delta v \\sim 0 \\) km/s) and with a line width that is too broad to be produced by the gas in the galaxy (\\( \\sigma \\sim 600 \\) km/s); this emission is likely tracing both the approaching and the receding side of the outflow. The difference with the other high-ionization emission lines is due to the redder rest-frame wavelength of [S III], which makes it less prone to dust attenuation and allows us to see the full velocity distribution. The [O III] emission is thus blueshifted not because the outflow is asymmetric, but because its far, redshifted side is hidden by dust attenuation. 5) Finally, He I is the only emission line that is redshifted (\\( \\Delta v \\sim +400 \\) km/s) compared to the systemic velocity of the galaxy, implying that we are seeing the receding side of the outflow but not the approaching side. This behavior is often found in observations of the Ly\\( \\alpha \\) line, which experiences resonant scattering, where the photons emitted in the outflow are re-absorbed by the neutral hydrogen unless they are substantially redshifted. Since the He I transition involves a meta-stable level of the helium atom, it can give rise to a similar resonant scattering (with the difference that the meta-stable level can only be populated via recombination, meaning that the He I line, unlike Ly\\( \\alpha \\), traces gas that is ionized). Its velocity offset and line width are consistent with the values measured for blueshifted emission lines, thus qualitatively confirming the outflow geometry shown in Figure 2. The overall picture emerging from the observations is that of an outflow that is present both on the foreground and on the background of\nFig. 1 JWST/NIRSpec spectrum of COSMOS-11142. The best-fit model, which includes the contribution of stars and dust, is shown in red. Data and model are inverse-variance smoothed using a 2-pixel window. Important absorption lines due to hydrogen (violet) and metals (black), and emission lines due to ionized gas (blue) are marked. The discrepancy between the stellar model and the data reveals the presence of substantial neutral gas (absorption by Ca II and Na I) and ionized gas (emission by O II, O III, N II, and other species).\n\nthe galaxy: this could be either a biconical or a spherical outflow.\n\nAssuming that the observed line profile is mostly due to projection effects, the outflow velocity can be estimated as \\( v_{\\text{out}} = |\\Delta v| + 2\\sigma \\) [10, 14]. We derive high outflow velocities for the ionized lines, up to \\( \\sim 1700 \\) km/s in the case of [O III], which strongly suggests the outflow is driven by an active galactic nucleus (AGN). The presence of an AGN is confirmed by the high [N II]/Hα and [O III]/Hβ line ratios [15].\n\nFollowing standard modeling for the ionized [16, 17] and neutral [14] phases we measure \\( M_{\\text{out}} \\), the mass of gas in the outflow. The derived outflow masses are particularly sensitive to the assumptions made in the derivation, such as the electron number density (for the ionized phase) and the dust depletion together with the opening angle (for the neutral phase; see Methods for details).\n\nThe uncertainties are therefore dominated by systematics, which we estimate to be about 0.7 dex for both the ionized and the neutral outflow mass. Dust depletion is particularly uncertain for calcium, and so we can use the Ca II K line only to derive a lower limit on the outflow mass. The resulting outflow velocities and masses are shown in the left panel of Figure 3. The ionized outflow masses derived from four different emission lines are in remarkable agreement, which validates some of the assumptions made in the modeling. Moreover, we find that the neutral outflow is slower but has a substantially larger mass, in qualitative agreement with observations of local galaxies [18].\n\nKnowing the outflow mass and velocity allows us to calculate the mass outflow rate, \\( \\dot{M}_{\\text{out}} = M_{\\text{out}} \\cdot v_{\\text{out}} / R_{\\text{out}} \\), where \\( R_{\\text{out}} \\) is the size of the outflow. We estimate \\( R_{\\text{out}} \\sim 3 \\) kpc from the NIRSpec data, in which we are able to spatially resolve\n1) Narrow emission\nIonized gas in the galaxy\n\n2) Blueshifted absorption\nNeutral gas in the foreground\n\n3) Blueshifted emission\nIonized gas in the foreground (strong dust attenuation)\n\n4) Broad emission\nIonized gas in the foreground and background (weak dust attenuation)\n\n5) Redshifted emission\nIonized gas in the background (resonant scattering)\n\nFig. 2 Kinematics of gas emission and absorption lines. Each row illustrates a different kinematic component of the gas, with the observations on the left and a cartoon on the right showing which spatial regions (highlighted in color) are probed by the observations. In the left panels, Gaussian fits are shown in purple, with fits to the individual lines in doublets ([O II] and Na I D) shown in a lighter color. For the emission lines, the difference between the observed flux and the best-fit stellar model is shown, while for the absorption line the ratio of the observed flux and the best-fit stellar model is shown. The zero of the velocity scale corresponds to the redshift of the stellar component measured from spectral fitting, and the dashed vertical lines mark the expected rest-frame location of the emission or absorption lines.\nFig. 3 Physical properties of the outflow and comparison to the star formation history. Left: outflow mass versus velocity derived for individual lines, probing neutral and ionized gas. The vertical error bars show the 0.7 dex systematic uncertainty on the outflow mass measurements. The Ca II K outflow mass is derived assuming no depletion onto dust, and is therefore a lower limit. The diagonal lines are at constant mass outflow rate assuming \\( \\dot{M}_{\\text{out}} = M_{\\text{out}} v_{\\text{out}} / R_{\\text{out}} \\).\nRight: Star formation history (red line) and 95% credible region (shaded area) derived from fitting the spectroscopic and photometric data. The mass outflow rate is shown for neutral and ionized gas at a lookback time of zero (i.e., the epoch at which the galaxy is observed). The mass outflow rate for the neutral gas is substantially higher than the residual star formation rate, implying that the outflow is able to strongly suppress the star formation activity.\n\nthe blueshifted [O III] emission. We then find \\( \\dot{M}_{\\text{out}} \\sim 100 \\, M_\\odot/\\text{yr} \\) for the neutral outflow and \\( \\dot{M}_{\\text{out}} \\sim 1 \\, M_\\odot/\\text{yr} \\) for the ionized outflow. The ratio between the two phases is large, but within the range measured in local outflows [18–22]. However, the mass outflow rate of COSMOS-11142 is an order of magnitude larger than the typical values measured in local star-forming galaxies [23, 24]; this is mostly a reflection of the much stronger Na I D absorption line observed in COSMOS-11142. At high redshift, measurements of neutral outflows from Na I D absorption have only been obtained for a few quasars [25, 26], but observations of UV or sub-millimeter lines tracing neutral gas reveal high mass outflow rates in star-forming galaxies and AGN systems [11].\n\nTo understand the role of the outflow in the evolution of COSMOS-11142, in the right panel of Figure 3 we show the star formation history of the galaxy, derived from our spectro-photometric fit. We confirm that the system is a post-starburst galaxy: it formed most of its stellar mass in a rapid and powerful starburst \\( \\sim 300 \\) Myr before the observations, and then experienced a rapid quenching of the star formation rate by two orders of magnitude. These remarkably rapid formation and quenching timescales are not seen in the local universe, but are common among massive systems at \\( z \\sim 1-2 \\) [1–3], and represent the only way to form quiescent galaxies at even higher redshift [27] due to the younger age of the universe. According to the star formation history, the rate at which COSMOS-11142 is currently forming stars is between 1 and 10 \\( M_\\odot/\\text{yr} \\); we obtain consistent estimates from ionized emission lines and infrared emission. The system is therefore in the middle of quenching, about 1 dex below the main sequence of star formation [28], but still above the bulk of the quiescent population [29, 30]. By comparing the mass outflow rate to the current star formation rate, we conclude that the ionized outflow is weak, while the neutral outflow is very strong. This comparison shows that the ionized outflow is irrelevant in terms of gas budget, whereas the neutral outflow is able to substantially affect the star formation rate by ejecting cold gas before it can be transformed into stars. We thus conclude that the observed outflow likely plays a key role in the rapid quenching of COSMOS-11142; this conclusion is further strengthened when considering that the molecular phase (not probed by our observations) is expected to be equally effective as the neutral phase at ejecting gas [20]. Given the relatively low outflow velocity, \\( v_{\\text{out}} \\sim 600 \\) km/s, it is possible that most of the cold gas is not able to escape the galaxy. In this case, heating of the halo gas by radio-mode AGN feedback is likely required to maintain this galaxy quiescent over a Hubble timescale. However, this does not change our main conclusion, since radio-mode AGN feedback alone is unable to explain the observed rapidity of quenching.\nDespite the highly effective feedback in action, COSMOS-11142 is not detected in publicly available X-ray or radio observations. This suggests that AGN samples selected at those wavelengths do not necessarily probe the galaxy population in which feedback is being most effective. Such samples are usually biased towards powerful AGNs, which tend to live in gas-rich, star-forming galaxies [31, 32]. Strong neutral outflows similar to the one detected in COSMOS-11142 may in fact be present in the majority of massive galaxies, which often have emission line ratios consistent with AGN activity despite the lack of X-ray emission [7, 33]. Among massive galaxies, AGN-driven outflows may be particularly important for the post-starburst population, which is very likely to host emission lines with high [NII]/Hα ratio [3, 30]. Moreover, the detection of blueshifted neutral gas absorption in post-starburst galaxies at \\( z \\sim 1 \\) [34, 35] suggests that neutral outflows are frequent during this specific evolutionary phase. The rapid quenching of massive galaxies at \\( z > 1 \\) may thus be fully explained by the AGN-driven ejection of cold gas.\n\nMethods\n\nJWST Spectroscopy\n\nThe Blue Jay survey is a Cycle-1 JWST program (GO 1810) that observed about 150 galaxies at \\( 1.7 < z < 3.5 \\) in the COSMOS field with the NIRSpec Micro-Shutter Assembly (MSA). Each galaxy was observed with the three medium-resolution gratings, covering the 1 - 5 μm wavelength range at a spectral resolution of \\( R \\sim 1000 \\). The target sample was drawn from a catalog [36] based on Hubble Space Telescope (HST) data. The selection was designed in a way to obtain a roughly uniform coverage in redshift and mass, and the sample is unbiased above a redshift-dependent stellar mass of \\( 10^{8.7} - 10^{9.3} \\ M_\\odot \\). COSMOS-11142 (the ID is from ref. [36]) was observed in December 2022 for a total of 13 hours in G140M, 3.2 hours in G235M, and 1.6 hours in G395M. A slitlet made of four MSA shutters (shown in Figure 4) was placed on the target and the observations employed a 2-point A-B nodding pattern along the slit. We reduced the NIRSpec data using a modified version of the JWST Science Calibration Pipeline v1.10.1, using version 1093 of the Calibration Reference Data System. Prior to combining the data we visually inspected and excluded any remaining artefacts in the individual exposures. The galaxy ID spectrum was then optimally extracted. For more details on the Blue Jay survey and the data reduction, see Belli et al. (in preparation).\n\nJWST Imaging\n\nJWST imaging of COSMOS-11142 is available from the PRIMER survey (GO 1837, PI: J. Dunlop) in several bands: F090W, F115W, F150W, F200W, F277W, F356W, F410M, and F444W with NIRCam; and F770W and F1800W with MIRI. We performed aperture photometry on the MIRI data and applied a point-source correction derived from WebbPSF [37]. For the NIRCam data, which have a higher resolution and sensitivity, we fit the surface brightness profile of COSMOS-11142, independently in each band, using Forcepho (Johnson et al., in preparation). We model the galaxy using a single Sersic profile, convolved with the point spread function, and explore the posterior distribution via Markov Chain Monte Carlo (MCMC). This yields a multi-band set of photometric and structural measurements. Figure 4 shows the data and the model for F200W, which is the short-channel band with the highest signal-to-noise ratio (SNR=212), where we measure an effective (half-light) radius \\( R_e = 0.075'' \\), corresponding to 0.6 kpc, a Sersic index \\( n = 2.6 \\), and an axis ratio \\( q = 0.5 \\). While the formal errors are small, and the measurements are likely dominated by systematic uncertainties, we can robustly conclude that the galaxy is compact (yet well resolved in the NIRCam data) and elongated. These results are qualitatively unchanged when considering the other NIRCam bands. The residuals are small, implying that a single Sersic profile is a good description of the galaxy morphology and ruling out the presence of a major merger, a close companion, or bright point-source emission from a Type-1 AGN.\n\nSpectral Fitting\n\nWe characterize the stellar population and dust properties of COSMOS-11142 by fitting models to the observed spectroscopic and photometric data. We use the Bayesian code Prospector [38] and follow the approach explained in ref. [3, 39]. We adopt the synthetic stellar population library FSPS [40, 41], the MIST isochrones [42], the C3K spectral library [43], and the Chabrier initial mass function [44]. The galaxy stellar population is described by stellar mass, redshift, velocity dispersion, metallicity, and a non-parametric star formation history\nFig. 4 Observed and modeled surface brightness distribution. The first panel shows the HST F160W data used for designing the observations, with the footprint of the four open MSA microshutters. The other three panels show, respectively, the data, model, and residual for the F200W NIRCam observations. The model is a single Sersic profile obtained with ForcePho, and is able to reproduce the data well.\n\n![Observed and modeled surface brightness distribution](page_184_97_1080_232.png)\n\nFig. 5 Spectral energy distribution. Points show the observed photometry from the ACS and WFC3 instruments onboard HST (circles), and from the NIRCam and MIRI instruments onboard JWST (pentagons). The observed NIRSpec spectrum is shown in blue, and the red line represents the best-fit model from Prospector, with the shaded red region marking the central 95% confidence interval.\n\n![Spectral energy distribution](page_184_370_1080_464.png)\n\nwith 14 bins. The bins are logarithmically spaced except for the two youngest ones (0–30 Myr and 30–100 Myr), and the oldest, which is a narrow bin placed at the age of the universe, providing the possibility of a maximally old population. We adopt a continuity prior that disfavors abrupt changes in the star formation history (see [45] for details). The model also includes attenuation by dust, described by three parameters (\\(A_V\\), dust index, and extra attenuation towards young stars; [46, 47]), and dust emission, implemented with three free parameters describing the infrared emission spectrum [48]. We assume that the total amount of energy absorbed by dust is then re-emitted in the infrared. We do not include the contribution from gas or AGN.\n\nIn order to fit a single model to both the JWST spectroscopy and the multi-wavelength photometry, it is necessary to include important systematic effects, as described in [38]. We add one parameter describing the fraction of spectral pixels that are outliers, and one “jitter” parameter that can rescale the spectroscopic uncertainties when necessary to obtain a good fit. The best-fit value for the jitter parameter is 2.05, suggesting that the NIRSpec data reduction pipeline underestimates the spectral uncertainties. In our subsequent analysis of the emission and absorption lines, we\nTable 1 Measured properties of absorption and emission lines. Quantities marked with † have been fixed during the fit. Missing entries are tied to the entry above them.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Line\\( \\lambda_{rest} \\) (Å)\\( \\Delta v \\) (km/s)\\( \\sigma \\) (km/s)Flux (\\( 10^{-18} \\) erg s\\(^{-1}\\) cm\\(^{-2}\\))EW (Å)
Absorption
Ca II K3935−212 ± 21191 ± 253.4 ± 0.3
Ca II H3970——1.3 ± 0.3
Na I D5892, 5898−212 ± 23187 ± 356.5 ± 0.5
Emission
[O II]3727, 373067 ± 22292 ± 264.2 ± 0.2
[Ne III]3870−190 ± 71168 ± 900.8 ± 0.2
H\\( \\beta \\)4863−226 ± 98314 ± 1021.2 ± 0.3
[O III]5008−438 ± 32632 ± 3314.3 ± 0.6
H\\( \\alpha \\)6565−226†314†5.3 ± 0.7
[N II]6585−62 ± 20493 ± 2030.2 ± 16.0
[S II]6718, 67335 ± 88292†4.8 ± 0.6
[S III]9533−61 ± 90591 ± 925.5 ± 0.7
He I10833386 ± 63531 ± 647.4 ± 0.7
\n\napply this jitter term to the error spectrum, in order to obtain a more accurate estimate of the uncertainties on our results.\n\nWe also adopt a polynomial distortion of the spectrum to match the spectral shape of the template, to allow for imperfect flux calibration and slit loss corrections (particularly important in this case since the shutter covers only a fraction of the galaxy). In practice, this is equivalent to normalizing the continuum and only considering the small-scale spectral features such as breaks and absorption lines. In turn, this procedure yields an accurate flux calibration for the JWST spectrum, if we assume that the emission probed by the MSA shutter is just a rescaling of the emission probed by the photometry (i.e., we are neglecting strong color gradients). This yields a slit-loss correction of \\( \\sim 2 \\), with a small dependence on wavelength. The spectrum shown in Figure 1 has been calibrated in this way, and we adopt this calibration also in subsequent analysis of absorption and emission lines.\n\nThe model has a total of 25 free parameters, and to fully explore the posterior distribution we employ the nested sampling package dynesty [49]. We fit the model to the observed NIRSpec spectroscopy and to the broadband data (shown in Figure 5). In the spectrum we mask ionized gas emission lines, including H\\( \\alpha \\) and H\\( \\beta \\), and the resonant absorption lines Na I D, Ca II H, and Ca II K. For the photometry we make use of our measurements from MIRI and NIRCam data (excluding F356W and F410M because the data reduction pipeline flagged most of the galaxy pixels as outliers). We also adopt archival photometry from HST, measured from data taken with the ACS and WFC3 instruments [36]. These measurements are clearly offset from the JWST NIRCam photometry, likely because they have been measured using a different method (photometry within a fixed aperture). From comparing the HST F160W and the JWST F150W bands, which cover a very similar wavelength range, we estimate that the HST fluxes are overestimated by 26%. We correct all the HST points for this offset, and add in quadrature a 26% relative error to the HST uncertainties.\n\nThe best-fit model is shown in red in Figure 1 and Figure 5: the same model is able to simultaneously reproduce the spectroscopy and the photometry. The fit yields a stellar mass \\( \\log M_*/M_\\odot = 10.9 \\), a stellar velocity dispersion \\( \\sigma = 273 \\pm 13 \\) km/s, and a metallicity \\( [\\mathrm{Fe}/\\mathrm{H}] = 0.16 \\pm 0.05 \\): the resulting star formation history is shown in Figure 3. The galaxy is relatively dusty, with \\( A_V = 1.5 \\pm 0.1 \\), which is higher than what found in quiescent systems and may be related to the rapid quenching phase in which it is observed. We find that the main results of our analysis do not change when excluding the HST photometry, using a smaller wavelength range for the spectroscopic data, or changing the order of the polynomial distortion.\n\nCombining the stellar velocity dispersion with the major axis measured from NIRCam we estimate [50] a dynamical mass \\( M_{dyn} \\sim 7 \\cdot 10^{10} \\ M_\\odot \\),\nFig. 6 Absorption lines from neutral gas. Top: observed spectrum, with the best-fit stellar model (red). Bottom: ratio of the observed spectrum to the stellar model, with the best-fit Gaussian components describing absorption by neutral gas (purple). The expected position of the resonant lines (at the systemic velocity of the galaxy) are shown in gray, while the position of the Balmer lines, which are only present in the stellar spectrum, are shown in green. The absorption by neutral gas is clearly blueshifted.\n\nwhich is slightly smaller than the stellar mass. This could imply issues with the stellar mass measurement, but could also be due to the presence of rotation in the galaxy (suggested by the elongated axis ratio) and/or to the limited sampling of stellar velocities by the small footprint of the MSA shutters. It is intriguing that a similar discrepancy has been found in the only other quiescent galaxy at high redshift for which precise kinematic and structural measurements based on JWST are available [27].\n\nAbsorption and Emission Lines\n\nTo analyze the gas emission and absorption lines, we first mask these features when running Prospector, and then fit the residuals using Gaussian profiles convolved with the instrumental resolution. The results of the Gaussian fits are listed in Table 1.\n\nWe show the resonant absorption lines Ca II H, K and Na I D in Figure 6. These lines are also present in the best-fit stellar model, but the observed absorption is both much stronger and clearly blueshifted, making it easier to study the neutral gas. We also note that the Ca II H line lies on top of the Balmer He absorption line, which however is not resonant and is therefore present only in the stellar spectrum.\n\nSince the effect of neutral gas absorption is multiplicative, when fitting Gaussian profiles we consider the ratio of the observed spectrum to the stellar model. We model Ca II H and Ca II K with a Gaussian profile each, assuming the same width and velocity offset. The ratio of their equivalent widths is noisy due to the faintness of Ca II H, but is consistent with 2, which is the value expected for optically thin gas [51]. We independently fit the Na I D doublet, which is unresolved, using two Gaussians with the same width and velocity offset, and fixing their equivalent width ratio to 2, the value appropriate for optically thin gas. We verified that the results do not change in a substantial way when leaving the doublet ratio free.\n\nThe observed line profiles do not warrant the modeling of multiple kinematic components; however, we consider the possibility that the observed absorption consists of the sum of a blueshifted and a systemic component. For example, this could be the case if our model underestimates the stellar absorption. We use the Alf stellar population synthesis code [52, 53] to assess how\nFig. 7 Emission lines from ionized gas. The spectra shown are obtained by subtracting the best-fit stellar model obtained with Prospector from the observed spectrum. Gaussian fits are shown in purple, with lighter lines showing fits to the individual lines when multiple components are fit simultaneously. The dashed vertical lines mark the expected rest-frame location of the emission lines. Other emission lines are shown in Figure 2.\n\nthe observed absorption lines vary when changing the abundance of individual elements in the stellar populations. We conclude that this effect is negligible: for a Na abundance that is twice the solar value, the extra absorption in Na I D would be only 8% of the equivalent width we observe in COSMOS-11142. A systemic component could also arise from neutral gas that is in the galaxy and not in the outflow. We find this unlikely because of the increased importance of the molecular phase, at the expense of the neutral phase, for the gas reservoir of galaxies at high redshift [54]; and also based on a study of Na I D absorption in the Blue Jay survey, where neutral gas is mostly associated with outflows and not with the gas reservoir, even in star-forming galaxies (Davies et al., in preparation). Nonetheless, we repeat the fit for Ca II K, which is well detected and not blended, adding a Gaussian component fixed at systemic velocity. In this case we find that the equivalent width of the blueshifted component would be reduced by (41 ± 9)%.\n\nSimilarly to what was done for the absorption lines, we fit Gaussian profiles to all the detected emission lines, which are shown in Figure 2 and Figure 7. Given the additive nature of the emission, here we consider the difference between the observed spectrum and the stellar model. We fit each isolated line independently, assuming a single Gaussian profile. For the unresolved [O II] doublet we assume two Gaussian profiles with same width and velocity offset and a fixed ratio of 1:1, which is in the middle of the allowed range. We use the same model also to fit the unresolved [S II] doublet, but due to the lower signal-to-noise ratio we also need to fix the velocity dispersion, adopting the value measured for [O II] (given the similar ionization energy). The [N II] doublet and Hα line are also blended, and we need to model all three lines simultaneously. In this case we find that in order to correctly reproduce the observed profile, the Hα line must be slightly blueshifted compared to the [N II] lines; a possible interpretation for this is that Hα mostly comes from the outflow while [N II] originates in the galaxy. We thus fix the velocity offset and dispersion of Hα to the values measured for Hβ, letting free the [N II] kinematics, and fixing the [N II] doublet ratio to the theoretical value of 3:1. The resulting line width for [N II] is relatively high, suggesting the presence of a broad component. We test a different model with a broad and a narrow component for each emission line, finding qualitatively similar results. We do not use the results of this more complex model for consistency with the other emission lines, most of which have a signal-to-noise ratio that is too\nlow to perform a decomposition into broad and narrow components.\n\nStar Formation Rate\n\nThe star formation rate of COSMOS-11142 is a key physical quantity, since it is used both to confirm the quiescent nature of the system and as a comparison to the mass outflow rate. We employ several methods to estimate the star formation rate, obtaining consistent results. The Prospector fit gives a star formation rate of \\( \\sim 3\\ M_\\odot/\\text{yr} \\) in the youngest bin (0-30 Myr), with an uncertainty of a factor of 3; considering the average star formation over the last 100 Myr we obtain an upper limit of \\( 10\\ M_\\odot/\\text{yr} \\). An alternative, independent method relies on the hydrogen recombination emission lines; because of the contribution from the outflow to the observed flux, this method can only yield an upper limit on the star formation rate. We first correct the measured emission line fluxes for dust attenuation using the result of the Prospector fitting (including the extra attenuation towards young stars); we then use the standard conversion [55] applied to the measured H\\(\\alpha\\) flux, obtaining an upper limit of \\( 10\\ M_\\odot/\\text{yr} \\). A similar upper limit is obtained using the observed H\\(\\beta\\) flux. It is possible that this method misses heavily dust-obscured regions hosting a starburst, as it is sometimes found in local post-starburst galaxies [56]. We check for this possibility by using redder hydrogen emission lines, which can be used to probe deeper into the dust: while we do not detect any of the Paschen lines in emission, we can place a 3-\\(\\sigma\\) upper limit to the Pa\\(\\gamma\\) flux of \\( 2.2 \\times 10^{-18}\\ \\text{erg s}^{-1}\\ \\text{cm}^{-2} \\), yielding an upper limit on the star formation of \\( 28\\ M_\\odot/\\text{yr} \\). The absence of substantial star formation in dust-obscured regions is also confirmed by the lack of strong mid-infrared emission. COSMOS-11142 is not detected in the *Spitzer* 24-\\(\\mu\\)m observations from the S-COSMOS survey [57], yielding a 3-\\(\\sigma\\) upper limit of \\( 38\\ M_\\odot/\\text{yr} \\), according to the measurements and assumptions detailed in [58]. However this estimate assumes that dust is heated exclusively by young stars – a bias known to lead to an overestimate of the star formation rate for quiescent galaxies, in which most of the heating is due to older stars [59]. The more sensitive JWST/MIRI observations detect the galaxy at 18 \\(\\mu\\)m, and the measured flux is fully consistent with the best-fit Prospector model, as shown in Figure 5, thus confirming the lack of substantial star formation hidden by dust.\n\nIonized Outflow\n\nWe detect clear signs of ionized outflow as blueshifted emission in [O III], [Ne III], and H\\(\\beta\\), and as a broad emission in [S III]. We can independently estimate the outflow properties using each of these emission lines. For a generic element X, the outflow mass can be written as a function of the observed line luminosity \\( L \\) [16, 17]:\n\n\\[\nM_{\\text{out}} = \\frac{1.4\\ m_p\\ L}{n_e\\ 10^{[X/H]} (n_X/n_H)_\\odot\\ j} ,\n\\]\n\nwhere \\( m_p \\) is the proton mass, \\( n_e \\) is the electron density, [X/H] is the logarithmic elemental abundance in the gas relative to the solar value (\\( n_X/n_H \\)_\\(\\odot\\) (which we take from ref. [60]), and \\( j \\) is the line emissivity. In this relation we neglect a factor \\( \\langle n_e^2 \\rangle / \\langle n_e \\rangle^2 \\), and we assume that all the atoms of the element X are found in the ionization stage responsible for the observed line (this is consistent with the observation of strong [O III] emission in the outflow but nearly absent [O II]; the other outflow-tracing emission lines have comparable excitation energy). We calculate the emissivity for each line using pyNeb [61] with standard assumptions (density 500 cm\\(^{-3}\\) and temperature 10\\(^4\\) K). We further assume that the gas in the outflow has solar metallicity, given the high stellar mass of the galaxy and the result of the Prospector fit. The electron density cannot be reliably derived from the flux ratio of the poorly resolved [S II] and [O II] doublets. We make the standard assumption of \\( n_e = 500\\ \\text{cm}^{-3} \\) [17], however we note that this value is highly uncertain. Since local studies using different methods find a wide range of values, \\( \\log n_e \\sim 2 - 3.5 \\) [62], we assign a systematic uncertainty of 0.7 dex (a factor of 5 in each direction) to the assumed value of \\( n_e \\). For the blueshifted lines we multiply the observed luminosity by two to account for the receding side hidden by dust. The resulting outflow masses are listed in Table 2 (see also Figure 3) and are in agreement with each other to better than 30%. This is remarkable given that the mass derived from H\\(\\beta\\) does not depend on assumptions on the ionization stage and the gas metallicity. However, all four lines depend in the same way on \\( n_e \\). The uncertainty on the outflow mass measurement is therefore dominated by the assumed \\( n_e \\).\n\nIn order to calculate the mass outflow rate we assume that the ionized gas is distributed, on each side of the outflow, in a mass-conserving cone that is expanding with velocity \\( v_{\\text{out}} \\), independent of radius [14]. In this case the mass outflow rate can\nFig. 8 Two-dimensional JWST/NIRSpec spectrum centered on the [O III]λ5008 emission line. The observed trace is mostly due to stellar emission (left panel); the spatially resolved [O III] emission becomes clear after subtracting the median stellar continuum (right panel). The vertical dashed line marks the expected position of [O III] at the systemic velocity.\n\nTable 2 Outflow properties measured from different lines\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
vout (103 km/s)Mout (106 M☉)˙Mout (M☉/yr)
Neutral outflow
Na I D0.5948897
Ca II K0.59> 9> 1.9
Ionized outflow
[Ne III]0.531.440.26
Hβ0.852.250.66
[O III]1.701.981.15
[S III]1.242.461.04
\n\nbe easily derived to be \\( \\dot{M}_{\\text{out}} = M_{\\text{out}} \\ v_{\\text{out}} / R_{\\text{out}} \\). We estimate the outflow velocity from the Gaussian fit as \\( v_{\\text{out}} = |\\Delta v| + 2\\sigma \\), and analyze the 2-D NIRSpec spectrum around the location of the [O III]λ5008 line to constrain the outflow size. We first construct the spatial profile by taking the median flux along each spatial pixel row; then we subtract this profile, representing the stellar continuum, from the data, revealing a clearly resolved [O III] line (see Figure 8). The emission line morphology is complex, and includes two components extending several pixels in the spatial directions. Both components are blueshifted, and are therefore not associated with a large-scale rotating disk. We measure the extent of each of these components to be approximately 4 spatial pixels, i.e. 0.4\", corresponding to \\( R_{\\text{out}} \\sim 3 \\) kpc. This allows us to derive ionized outflow masses, which are in the range 0.3 – 1.2 \\( M_{\\odot} \\)/yr.\n\nNeutral Outflow\n\nWe use the measured properties of the Na I D and Ca II K lines to constrain the properties of the neutral outflow. The first step is to derive the Na I and Ca II column density from the observed equivalent widths (listed in Table 1), which can be done easily in the optically thin case [51], yielding \\( N_{\\text{Na I}} = 2.2 \\times 10^{13} \\) cm\\(^{-2}\\) and \\( N_{\\text{Ca II}} = 3.7 \\times 10^{13} \\) cm\\(^{-2}\\). These should be considered lower limits, as even small deviations from the optically thin case can substantially increase the column density corresponding to the observed equivalent width. If the outflow is clumpy, and its covering fraction is less than unity, then the true equivalent width would be larger than the observed one.\nIn our case, the observed maximum depth of the absorption lines implies that the covering fraction must be larger than 50%. The column density may then be up to a factor of two larger than the value we derive. Unless one can constrain the Ca II or Na I doublet ratio [63], it is only possible to measure the product of the covering fraction and the column density. However, the mass outflow rate only depends on this product, thus making this decomposition unimportant for our analysis. For simplicity, here we assume a covering fraction of unity.\n\nThe next step consists in inferring the hydrogen column density. For Na I we can write [19, 63]:\n\n\\[\nN_{\\mathrm{H}} = \\frac{N_{\\mathrm{Na}\\,\\mathrm{I}}}{(1-y)\\ 10^{[\\mathrm{Na}/\\mathrm{H}]} (n_{\\mathrm{Na}}/n_{\\mathrm{H}})_{\\odot}\\ 10^6},\n\\]\n\nwhere \\( y \\) is the sodium ionization fraction, and \\( 10^6 \\) represents the depletion of sodium onto dust. For consistency with local studies we make the standard assumption \\( 1-y = 0.1 \\) [63], meaning that only 10% of the sodium is in the neutral phase; it is likely that the true value is even lower [19], which would increase the derived column density and therefore the outflow mass. We also assume solar metallicity for the gas, and take the canonical values [64] for solar abundance, \\( \\log(n_{\\mathrm{Na}}/n_{\\mathrm{H}})_{\\odot} = -5.69 \\), and dust depletion, \\( b = -0.95 \\). We obtain a hydrogen column density \\( N_{\\mathrm{H}} = 9.6 \\times 10^{20} \\) cm\\(^{-2}\\). The systematic uncertainty on this result is dominated by the observed scatter in the dust depletion value, which is 0.5 dex [65].\n\nThe calcium column density is more difficult to interpret because calcium, unlike sodium, presents a highly variable depletion onto dust as a function of the environment [66, 67]. Observations of Milky Way clouds show very high dust depletion (up to 4 dex) for calcium at the high column density that we measure, which would imply a hydrogen column density that is \\( \\sim 20\\times \\) higher than what measured from Na I D. This discrepancy is probably caused by the presence of shocks in the outflow, which can destroy dust grains and decrease the depletion of calcium. Thus, we can only derive a lower limit on the hydrogen column density by assuming that calcium is not depleted at all, and we obtain \\( N_{\\mathrm{H}} > 1.8 \\times 10^{19} \\) cm\\(^{-2}\\). We have neglected the ionization correction since most of the calcium in the neutral gas is expected to be in the form of Ca II [68].\n\nIn order to derive the outflow mass we assume that the neutral gas forms an expanding shell outside the ionized outflow. This is consistent with local observations [19] and with the idea that the neutral gas must be further out from the ionizing source. For a shell geometry, the outflow mass and mass rate are [14]:\n\n\\[\nM_{\\mathrm{out}} = 1.4\\ m_p\\ \\Omega\\ N_{\\mathrm{H}}\\ R_{\\mathrm{out}}^2 ,\n\\]\n\\[\n\\dot{M}_{\\mathrm{out}} = 1.4\\ m_p\\ \\Omega\\ N_{\\mathrm{H}}\\ R_{\\mathrm{out}}\\ v_{\\mathrm{out}},\n\\]\n\nwhere \\( \\Omega \\) is the solid angle subtended by the outflow. Based on the results of local studies [14] and on the incidence of neutral outflows in the Blue Jay sample (Davies et al., in preparation), we assume an opening angle of 40% of the solid sphere, i.e. \\( \\Omega/4\\pi = 0.4 \\). We consider the systematic uncertainty on \\( \\Omega \\) to be a factor of 2.5 in each direction, ranging from a narrow opening to a spherical and homogeneous outflow. Combined with the uncertainty on the calcium dust depletion, this gives a total uncertainty on the outflow mass of \\( \\sim 0.7 \\) dex, similar to that on the ionized outflow mass (but due to a different set of assumptions).\n\nThe neutral mass outflow rate estimated from the Na I D line is 97 \\( M_\\odot/\\mathrm{yr} \\), about two orders of magnitude larger than what measured for the ionized phase. In addition to the 0.7 dex uncertainty due to the opening angle and the dust depletion, there are two additional assumptions that could influence this result. First, we ignored a possible contribution to Na I D from a systemic component of neutral gas not associated with the outflow, which would decrease the measured column density by 41% (adopting the value derived for Ca II K). Second, we assumed that the radius of the neutral outflow coincides with that of the ionized outflow; in principle, the neutral outflow radius could be as small as the galaxy effective radius, which is 0.6 kpc (it cannot be smaller than this because the observed depth of the gas absorption reaches \\( \\sim 50\\% \\) of the stellar continuum, meaning that the neutral gas must be in front of at least 50% of the stars in the galaxy). If we make the most conservative choice on the systemic component of Na I D and on the outflow radius we obtain a mass outflow rate for the neutral phase that is 8.5 times lower compared to our default assumptions, i.e., \\( \\dot{M}_{\\mathrm{out}} = 11\\ M_\\odot/\\mathrm{yr} \\). This is still one order of magnitude larger than the ionized mass outflow rate.\nFig. 9 Emission line diagnostics. BPT diagrams [15] showing the line flux ratios for local galaxies [69] (black) and for COSMOS-11142 (red). Blue curved lines represent the theoretical maximum starburst locus [70], while the blue straight line in the right panel shows an empirical separation between Seyferts and LINERS [71].\n\nPhysical Nature of the Outflow and Properties of the AGN\n\nDue to the low star formation rate of COSMOS-11142, it is unlikely that the outflow is driven by star formation activity. We can also rule out a star-formation driven fossil outflow: the travel time to reach a distance of \\( R_{\\text{out}} \\sim 3 \\) kpc at the observed velocity is less than 10 Myr, which is much smaller than the time elapsed since the starburst phase, according to the inferred star formation history. Moreover, the ionized gas velocity we measure is substantially higher than what observed in the most powerful star-formation driven outflows at \\( z \\sim 2 \\) [72]. Another possibility could be that the outflowing material actually consists of tidally ejected gas due to a major merger [73, 74]. However, the lack of tidal features or asymmetries in the near-infrared imaging, together with the high velocity of the ionized gas, rule out this scenario.\n\nThe only reasonable explanation is therefore that the observed outflow is driven by AGN feedback. This is confirmed by the emission line flux ratios, which we compare to those of the local galaxy population [69] in Figure 9. COSMOS-11142 occupies a region on these Baldwin-Phillips-Terlevich (BPT) diagrams [15] which is exclusively populated by AGN systems. We note that some of the measured emission lines (notably [O III] and H\\( \\beta \\)) trace the outflow rather than the galaxy, which may complicate the interpretation of the position on the BPT diagram. Nonetheless, the line ratios measured in COSMOS-11142 are fully consistent with those measured in the outflows of high-redshift quasars [25, 75].\n\nDespite the rather extreme line ratios, the AGN activity in 11142 is relatively weak, leaving no trace other than the ionized gas emission lines. We do not detect AGN emission in the UV-to-IR broadband photometry (which is well fit by a model without AGN contribution), in the mid-infrared IRAC colors (using the criterion proposed by ref. [76]), in the rest-frame optical morphology (no evidence for a point source in the NIRCam imaging), in X-ray observations [77], or in radio observations [78]. We estimate the bolometric luminosity of the AGN from the [O III] luminosity [79], obtaining \\( \\log L_{\\text{bol}} \\sim 45.3 \\); this is however an upper limit since part of the observed line luminosity may come from shock excitation. The actual bolometric luminosity may be an order of magnitude lower; in this case our measured mass outflow rates for the ionized and neutral phase would not be substantially off from the known AGN scaling relations [10], assuming that the neutral phase is comparable to the molecular phase. What sets COSMOS-11142 apart from known systems, however, is its gas-poor and quiescent nature.\n\nAcknowledgments\n\nWe acknowledge discussions with Marcella Brusa, Karl Glazebrook, Shri Kulkarni, Luca Ciotti, and Andrea Ferrara. SB is supported by the the ERC Starting Grant “Red Cardinal”, GA 101076080. RD is supported by the Australian Research\nCouncil Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. RE acknowledges the support from grant numbers 21-atp21-0077, NSF AST-1816420, and HST-GO-16173.001-A as well as the Institute for Theory and Computation at the Center for Astrophysics. 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ApJ 613, 109–118 (2004)."} {"paper_id": "prb23", "title": "A computational approach to evaluate how molecular mechanisms impact large-scale brain activity", "text": "A computational approach to evaluate how molecular mechanisms impact large-scale brain activity\n\nAlain Destexhe\nAlain.Destexhe@cnrs.fr\n\nCNRS, Paris-Saclay University https://orcid.org/0000-0001-7405-0455\n\nMaria Sacha\nCNRS, Paris-Saclay University\n\nFederico Tesler\nCNRS, Paris-Saclay University\n\nRodrigo Cofre\nInstitute of Neuroscience (NeuroPSI), Paris-Saclay University, Centre National de la Recherche Scientifique (CNRS), Gif-sur-Yvette, France https://orcid.org/0000-0002-7498-7122\n\nArticle\n\nKeywords:\n\nPosted Date: October 1st, 2024\n\nDOI: https://doi.org/10.21203/rs.3.rs-4610184/v1\n\nLicense: © This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nAdditional Declarations: There is NO Competing Interest.\n\nVersion of Record: A version of this preprint was published at Nature Computational Science on May 28th, 2025. See the published version at https://doi.org/10.1038/s43588-025-00796-8.\nA computational approach to evaluate how molecular mechanisms impact large-scale brain activity\n\nMaria Sacha1, Federico Tesler1, Rodrigo Cofre1, Alain Destexhe1*\n\n1 Paris-Saclay University, CNRS, Paris-Saclay Institute of Neuroscience (NeuroPSI), 91400 Saclay, France\n\nAbstract\nAssessing the impact of pharmaceutical compounds on brain activity is a critical issue in contemporary neuroscience. Currently, no systematic approach exists for evaluating these effects in whole-brain models, which typically focus on macroscopic phenomena, while pharmaceutical interventions operate at the molecular scale. Here, we address this issue by presenting a computational approach for brain simulations using biophysically grounded mean-field models that integrate membrane conductances and synaptic receptors, showcased in the example of anesthesia. We show that anesthetics targeting GABA_A and NMDA receptors can switch brain activity to generalized slow-wave patterns, as observed experimentally in deep anesthesia. To validate our models, we demonstrate that these slow-wave states exhibit reduced responsiveness to external stimuli and functional connectivity constrained by anatomical connectivity, mirroring experimental findings in anesthetized states across species. Our approach, founded on mean-field models that incorporate molecular realism, provides a robust framework for understanding how molecular-level drug actions impact whole-brain dynamics.\n\n1 Introduction\nRecent advances in neuroimaging techniques have made it possible to build detailed brain atlases and generate personalized connectomes of the human brain through cutting-edge tools such as diffusion MRI, MEG, and fMRI. These advancements have catalyzed the conceptualization within the scientific community of highly detailed, personalized whole-brain models, colloquially termed \"Digital Twins,\" poised to revolutionize the exploration, diagnosis, and therapeutic interventions for various neurological conditions such as disorders of consciousness, epilepsy, Alzheimer’s disease, and schizophrenia (Arababayzad et al., 2021; Stefanovski et al., 2021; Jirsa et al., 2023; Luppi et al., 2023; Amunts et al., 2024).\nDespite significant advances in this domain, a primary challenge faced by these models lies in effectively addressing the diverse spatial and temporal scales inherent to brain activity. Numerous diseases or alterations in brain states emerge at the molecular or cellular level, requiring comprehensive descriptions within whole-brain models to ensure accuracy. Thus, integrating cellular-scale details is imperative for these models to capture the intricacies of neurological phenomena. However, the human brain comprises approximately 85 billion neurons and an estimated \\(10^{15}\\) synaptic connections. Consequently, creating a large-scale model of the brain (macro-scale) with single-cell resolution (micro-scale) remains an insurmountable challenge. Establishing a seamless interface between these disparate scales is, therefore, a pivotal challenge for enhancing the utility and precision of digital twins and whole-brain simulations.\nThis article introduces a novel framework aimed at addressing this challenge, offering an efficient pathway for transitioning from the cellular scale to the whole-brain level. Central to our methodology is the integration of a biophysically grounded mean-field model, encompassing cellular and molecular properties. This model effectively reduces system dimensionality while capturing emergent properties observed at the meso and macro scale due to cellular-level changes. Our methodology comprises four parts: i) Single-cell models (microscale); ii) Networks of spiking neurons (mesoscale); iii) a mean-field model elucidating the activity and dynamics of the network (mesoscale, low-dimensional); and iv) a Whole-brain model leveraging the mean-field model for generating large-scale simulations (macroscale). To facilitate the execution of these simulations, we utilize The Virtual Brain (TVB) platform (Sanz-Leon et al., 2015), a versatile tool enabling the execution of large-scale simulations with customizable brain connectomes.\nTo illustrate our approach, we simulate the molecular actions leading to general anesthesia, specifically with anesthetics such as ketamine and propofol, and investigate their effects at the mesoscale and whole-brain levels. Our focus includes the generation of slow-wave activity, reduced responsiveness to external stimuli, and increased anatomical-functional correlations, as measured experimentally for anes-\n2 Results\n\nThe components of our method are introduced sequentially, following the bottom-up approach of the model construction. As a benchmark, we apply this model within the context of general anesthesia, which serves as an example of how molecular changes at the synaptic level can significantly impact whole-brain dynamics. The diagram of the framework is presented in Fig. 1.\n\n2.1 Single-Cell Model\n\nThe first step of our framework consists of selecting a spiking neuron model. Here, we used the Adaptive Exponential integrate-and-fire model (AdEx), recognized for its capacity to capture a wide range of neuronal firing patterns, while also providing biophysically realistic representations of neuronal behavior and mathematical simplicity (Brette and Gerstner, 2005; Naud et al., 2008). Nevertheless, our methodology remains adaptable to a variety of neuronal models, such as quadratic Integrate-and-Fire or Hodgkin-Huxley (Carlu et al., 2020; Alexandersen et al., 2024; Lorenzi et al., 2023), thereby showcasing the broad applicability of our approach.\n\nThe AdEx model consists of two differential equations. The first equation (Eq. 1) describes the membrane potential dynamics and the second (Eq. 2), a slow adaptation current (see Methods section for details). This adaptation current varies over time in response to spiking activity, modulating the excitability of the neuron (Brette and Gerstner, 2005).\n\nWe consider two types of cells: pyramidal (excitatory) neurons and fast-spiking (inhibitory) interneurons. Each type of cell is characterized by a different set of parameters in the AdEx model. The baseline parameters used for each neuron type are extracted from fits on experimental data of cortical neurons (Di Volo et al., 2019). However, the method we present can be equally applied to simulate the dynamics of neurons in other brain areas such as the thalamus (Overwiening et al., 2023), basal ganglia (Tesler et al., 2023a), or cerebellum (Lorenzi et al., 2023).\n\n2.2 Network of Spiking Neurons\n\nThe second step of our framework consists of the construction of networks of spiking neurons representing local circuits or specific brain structures. The networks are characterized by the type and number of neurons, their connectivity patterns (probability of connections between neurons), and the synaptic model used. In terms of the number of neurons and the connectivity pattern, the example presented in this article adopts values representative of prototypical cortical circuits, specifically modeling a single cortical column. We consider a network made of 10000 neurons, with 80% of pyramidal cells and 20% of interneurons, connected randomly with probability \\( p = 0.05 \\). Different connectivity patterns can be considered and are compatible with our method, which can be used to represent different brain structures (Tesler et al., 2022; Lorenzi et al., 2023; Overwiening et al., 2023; Tesler et al., 2024). Regarding the synaptic model, we consider conductance-based synapses through glutamate (AMPA-NMDA) and GABA\\(_A\\) receptors, but current-based synapses are also compatible with our framework (El Boustani and Destexhe, 2009). The equation for the synaptic model is presented in the Methods section, Eq. 4.\n\n2.3 Mean-Field Model\n\nThe central component of our framework is the integration of a recently developed mean-field formalism, which enables an efficient transition between scales while preserving the characteristics and relevant parameters of both the cellular and network levels. The derivation of the mean-field model used here follows a bottom-up approach based on a second-order Master Equation formalism, that describes the average activity (mean firing rate, membrane potential, conductance) and covariance of networks of spiking neurons (El Boustani and Destexhe, 2009). A key component of these equations is the transfer function, which relates a neuron’s output (firing rate) to its presynaptic input. This function cannot be expressed analytically for complex neurons, particularly those interacting through conductance-based synapses. However, a semi-analytic approach can be followed. First, numerical simulations of the desired neuron model are realized and used to fit an analytically derived mathematical template of the transfer function. This approach has been applied previously to the AdEx model (Zerlaut et al., 2018; Di Volo et al., 2019), but it has been extended to more complex models, such as the quadratic integrate-and-fire neuron (Alexandersen et al., 2024), the Morris-Lecar and Hodgkin-Huxley model (Carlu et al., 2020)\n\nThrough this semi-analytical approach, population models that preserve biological relevance can be constructed. This novel formulation allows us to study the effects of changes in molecular and network parameters at the mesoscale level, trace the mechanisms behind dynamical transitions in large populations (facilitated by the low dimension of the mean-field model), and to construct finally whole-brain simu-\nFigure 1: Schematic diagram of the bottom-up construction of the whole-brain modelling framework (top row) and the corresponding signals simulated across the various scales (bottom row). Microscale: a point neuron model is selected to describe the activity of individual neurons, representing different cellular types with specific neuroreceptors and characterized by distinct firing patterns—ranging from regular spiking cells with adaptive firing rates to fast-spiking cells. Mesoscale: based on experimental data of brain microcircuits, we connect the single neurons to build spiking neural networks (high-dimensional mesoscale) from which biologically grounded mean-field models are derived to describe collective dynamics (low-dimensional mesoscale). Macroscale: structural connectivity data are integrated into the framework to build large-scale networks of mean-field models to perform whole-brain simulations, allowing the exploration of emergent properties at this scale (e.g. responsiveness to external stimulation).\n\nFigure 2: Synaptic targets of general anesthesia and its effect at the cellular scale, in experiments and modeling. A. General anesthesia that targets GABA_A receptors (e.g., propofol) prolongs inhibitory post-synaptic potentials (IPSPs) by increasing the opening duration of the chloride channels. We model this effect as an increase in the inhibitory synaptic decay time constant (\\( \\tau_i \\)). We illustrate the comparison of the model with whole-cell patch clamp recordings demonstrating the prolongation of IPSP caused by halothane (top row in A.II, modified from Maciver et al. (1991). B. NMDA blockers (e.g. ketamine, xenon) decrease the duration of excitatory post-synaptic potentials (EPSPs), as shown by patch-clamp recordings of AMPA and NMDA currents under the effect of ketamine (top row in B.II modified from Destexhe et al. (1998)). This effect can be modeled as a decrease of the excitatory synaptic decay time constant (\\( \\tau_e \\)).\n2.4 Whole-brain model\n\nWe move to the last scale of our formalism, i.e. the whole brain scale, which is essential for examining properties that manifest exclusively at a macroscale. The whole-brain model is described by a network of mean-fields interconnected based on experimental data (connectome). First, a parcellation of the brain is selected, that divides the cortex into distinct regions. The granularity of the parcellation can vary from tens to thousands of regions. Information on the connection between these regions is available through various anatomical connectivity studies, obtained using diffusion weight imaging, tracer studies (in non-human species), or a combination of both. The output of these studies relevant to our method is a connectivity matrix that provides information on the connection strength and the distance between each pair of regions.\n\nThe activity of each region can be described using the developed mean-field model, forming a node in the whole-brain model. Each node’s input consists of an external noise, described by an Ornstein-Uhlenbeck process, and the output firing rate of its connected nodes. The input of the connected nodes is weighted according to the connection strength and received with a delay based on the distance between the two nodes.\n\nWe employed a parcellation scheme of a human brain comprising 68 brain regions (Anatomical Desikan-Killiany Atlas (Desikan et al., 2006)), giving rise to a network of interconnected mean fields. The implementation of the model was realized in the TVB platform.\n\n2.5 The case of general anesthesia\n\nTo provide an example of the use of our framework, we consider the case of general anesthesia. General anesthesia directly impact various cortical receptors (Moody et al., 2021), primarily GABA_A and NMDA receptors (Hemmings et al., 2005), influencing the activity of both inhibitory and excitatory synapses. GABAergic anesthetics (propofol, volatile anesthetics) act as a positive allosteric modulator of the GABA_A receptor, potentiating GABA-mediated inhibition (Vanlersberghe and Camu, 2008). They increase the opening duration of the chloride channel, increasing the Cl⁻ conductance and prolonging the duration of inhibitory post-synaptic potentials (IPSPs) (Forman SA, 2008; Franks, 2008; Nguyen and Postnova, 2021). Conversely, NMDA receptor antagonism (ketamine, xenon), leads to a shortening of the kinetics of the conductance of AMPA/NMDA excitatory synaptic input (Orser et al., 1997; Dilger, 2002; Mion and Villevieille, 2013). Thus, the main effect of these anesthetics on cortical synapses can be described as an increase in the time constant of inhibitory synaptic decay (\\( \\tau_i \\) in Eq. 4) to account for the IPSP prolongation caused by GABAergic anesthetics, while a decrease in the excitatory synaptic decay time (\\( \\tau_e \\) in Eq. 4) corresponds to NMDA-antagonism.\n\nDespite these seemingly small changes at the cellular scale, at the meso- and macro-scale, general anesthesia is characterized by a qualitative transition in the global neuronal dynamics. While the awake state is characterized by asynchronous and irregular dynamics, one of the hallmarks of general-anesthesia states is the appearance of high-amplitude, low-frequency (<4 Hz) oscillations in neuronal activity, correlated with synchronized transitions of neocortical neurons between hyperpolarized and depolarized states (Steriade et al., 1993a; Contreras and Steriade, 1995; Steriade et al., 2001). These transitions manifest as alternating periods of intense neuronal firing (UP states) and periods of quiescence (DOWN states).\n\nThis type of activity is also found in NREM sleep (Steriade et al., 1993a,b; Timofeev et al., 2001; McCormick, 1993), where the low levels of acetylcholine lead to the activation of leak K⁺ channels and the increase of neuronal spike-frequency adaptation (described by the parameter \\( b \\) in the AdEx model), as shown in previous modelling works (Di Volo et al., 2019; Goldman et al., 2022). Variations in the level of acetylcholine are also observed for anesthetics such as propofol (Huang et al., 2024), but it does not constitute its main pharmacological effect. Thus, how this global transition in neuronal dynamics occurs during anesthesia and how it is related to the molecular changes described before is still an open question. Furthermore, how the molecular changes occurring during NREM sleep lead to the same kind of global transition as in anesthesia is yet not well understood. We show in the next sections how our framework can capture this transition at multiple scales and how the mechanisms and interplay between the different molecular mechanisms acting during anesthesia and sleep can be understood using our framework.\n\n2.6 Emergence of UP-and-DOWN states in anesthesia and NREM sleep\n\nIn this section, we present an analysis of the mechanisms behind the emergence of UP-and-Down states in general anesthesia and its relation to slow waves in NREM sleep. Previous modeling work has shown that the emergence of Up-and-Down states during NREM sleep can be associated with the periodic destabilization of a self-sustained state due to the action of a slow adaptation current (Di Volo et al., 2019; Cakan et al., 2022). For a large enough strength of\nFigure 3: Emergence of UP-and-DOWN states in simulated anesthesia and NREM sleep: effects of molecular mechanisms at the mesoscale level. A. Loss of self-sustain activity states in the spiking network as a consequence of changes in GABA-ergic receptors under general anesthesia (for GABA-targeting case). An external input (depicted in green) stimulates the network, resulting in a high firing rate. In the case of higher \\( \\tau_i \\) (general anesthesia state, right panel), the system’s activity is suppressed after the end of the stimulus, in contrast to the reference case (lower values of \\( \\tau_i \\), left panel) where a self-sustained state is obtained. B. Graphical solution of the first-order mean-field equations for stationary points, predicting the destabilization of self-sustain states and the emergence of the UP-and-DOWN states in NREM sleep and general anesthesia. The function \\( H(v_c) \\) corresponds to the Transfer Function of pyramidal cells evaluated at the corresponding stationary solution for FS cells and the black dashed line corresponds to the bisector (see methods and ref. Di Volo et al. (2019) for details). Stable fixed points are marked with filled circles and unstable ones with empty circles. The destabilization of the high-rate (self-sustained) stationary point is promoted by the increase of the synaptic decay time \\( \\tau_i \\) (left panel) and due to the increase of spike-triggered adaptation (\\( b_e \\), right panel). C,D. Decay time of the spiking network activity after the end of an external stimulus (survival time of the spiking network) as a function of synaptic decay times and spike-triggered adaptation parameters. For each value of \\( \\tau_{e,i} \\) a critical value of \\( b_e \\) exists (\\( b_{crit} \\)) for which the sustained network activity is suppressed. For each combination of \\( b_e \\) and \\( \\tau_{e,i} \\), 20 different trials with different noise realizations were conducted. The final survival time is reported as the average across these trials. The yellow lines describe the superimposed mean-field predictions of \\( b_{crit} \\) (see text for details), demonstrating the capacity of the mean-field to explain the transition in dynamics at the mesoscale level.\n\nthe spike-triggered adaptation current, determined by the parameter \\( b \\) in Eq. 2, a transition from an asynchronous irregular state to a UP-and-DOWN state is obtained. Here we extend this analysis and show by combining the mean-field and network simulations (mesoscale level) that this destabilization is promoted by the variations in the synaptic decay times (induced by general anesthesia) and, furthermore, that the transition to UP-and-DOWN states in general anesthesia can be explained as a result of an interplay between the values of synaptic decay \\( \\tau_{e,i} \\) and the spike frequency adaptation of excitatory cells \\( b_e \\) (related to neuromodulatory currents that affect neuronal excitability).\n\nWe start by examining the self-sustainability of the AdEx spiking networks as a function of the parameters \\( b_e \\) and \\( \\tau_{e,i} \\) (\\( \\tau_e \\) or \\( \\tau_i \\)). To investigate the existence of self-sustained states in the network we apply a short initial stimulus of 1Hz of amplitude and a total duration of 120ms. In the cases where the system exhibits a self-sustained state, the network maintains its activity after the end of the stimulus, otherwise, it decays fast to zero (Fig. 3.A). An extensive scan along these variables was performed and the survival time of the activity after the end of the stimulus was calculated. Two parameter scans were performed, one for varied \\( b_e \\) and \\( \\tau_i \\) (Fig.3.C) and one for varied \\( b_e \\) and \\( \\tau_e \\) (Fig.3.D).\n\nAs seen in the Fig. 3.C,D, for both cases there is a region of the parameter space where the network sustains its activity beyond the removal of the external input (white area), followed by a transition zone where the survival time decreases progressively until it reaches an area where the network no longer\nis able to sustain its activity (in black). It becomes evident that the loss of the stable high state of the system depends on the interaction between the synaptic parameters \\( \\tau_{e,i} \\) and the adaptation \\( b_e \\).\n\nTo better understand the interplay of the different parameters (\\( b_e, \\tau_e \\) and \\( \\tau_i \\)), and the mechanism behind the emergence of UP-and-DOWN states, we turn now to the mean-field model. An analysis of the stable solutions of the system is performed. We show in Fig. 3.B a graphical solution for the calculation of the fixed points of the excitatory firing rate (\\( v_e \\)). We continue with the exploration of the bistability of the system as predicted by the AdEx mean-field, seeking to identify the critical value of \\( b_e \\) (defined as the value of \\( b_e \\) where the high-rate fixed point of the system is lost). To obtain this solution a scan is performed for different values of the \\( v_e \\) and the corresponding function \\( H(v_e) = F_e(v_e, \\bar{v}_i) \\) is calculated, where \\( \\bar{v}_i = F_i(v_e, \\bar{v}_i) \\) (first-order mean-field \\( \\bar{v}_i = 0 \\)). The fixed point of the system is obtained when \\( H(v_e) = v_e \\), therefore the graphical solution corresponds to the intersection point of the plotted function \\( H \\) and the bisector.\n\nTo explore the effects of the parameters \\( b_e \\) and \\( \\tau_{e,i} \\) on the stable points of the system we fix the value of \\( \\tau_{e,i} \\) and we progressively increase the value of \\( b_e \\) starting from zero. As observed in the plot, as the magnitude of \\( b_e \\) increases there is a critical value (\\( b_{crit} \\)) for which the system transitions from two fixed-points to only one fixed point located at zero. However, this critical value depends on the respective value of \\( \\tau_{e,i} \\): variations in \\( \\tau_{e,i} \\) modify the global excitability of the system, facilitating or hindering the suppression of the self-sustained state due to \\( b_e \\) (or even completely eliminating the self-sustained state independently of the adaptation). We present the predicted \\( b_{crit} \\) as a function of \\( \\tau_i \\) and \\( \\tau_e \\) in Fig. 3.C and D respectively superimposed to the predictions of the survival time of the spiking networks (yellow lines in Fig. 3.C and D). As expected, the \\( b_{crit} \\) is lower for higher values of \\( \\tau_i \\), with the opposite behavior observed in the case of \\( \\tau_e \\). A good agreement is observed between the predictions of the mean-field and the spiking network, with the mean-field predictions delimiting the area after which the values of the survival time are uniformly zero. Notice that for spiking-networks the intrinsic fluctuations due to limit-size effects induce a gradual transition in the survival time which is not captured by the mean-field model.\n\nIn Fig.4 we demonstrate the transition of states (from asynchronous irregular to UP-and-DOWN dynamics) at the different scales obtained within our framework. In conclusion, in this section we have shown how we can capture the emergence of UP-and-DOWN states in general anesthesia at the different scales by modeling molecular changes, and how our framework (network-simulations in combination with the mean-field formalism) can be used to explain the mechanisms behind the transition between states.\n\n2.7 Emergent whole-brain effects of microscopic changes\n\nWe advance to the next stage by using our framework to assess emergent changes at the whole-brain scale. We analyze changes occurring at the functional and behavioral level between the awake and anesthetized states and compare our model with experimental data of both resting state and stimulus-response paradigms.\n\nState-dependent Resting State Dynamics: Correlation between Structural and Functional Connectivity\nAn increase of similarity between the structural and functional connectivity (SC and FC respectively) during anesthesia has been reported in experimental data (Barttfeld et al., 2015) and is considered one of the neural signatures of unconsciousness. This property can only be studied using a whole brain model capable of describing the activity of distinct brain regions (functional component) while incorporating tractographic information on their connections (structural component). Our approach offers the possibility of studying such emergent properties while allowing the mapping of macroscale observations to microscopic factors.\n\nWe used resting state fMRI experimental data from humans in the awake state and under propofol anesthesia to reveal differences in SC-FC correlation between the two states. We followed the same analysis on simulated data, by generating BOLD signals based on the nodes’ firing rates of the whole-brain model, and compared the experimental results to the model’s predictions.\n\nFigure 5 presents the Pearson correlation between functional and structural connectivity for both experimental and simulated data in humans (Fig. 5). Resting-state fMRI data from 26 individuals during wakefulness and under propofol anesthesia were analysed. From these signals, the FC matrix was computed for each participant and correlated with a reference SC. The Pearson correlation between SC and FC was significantly higher during anesthesia compared to wakefulness.\n\nWe used our framework to simulate wakefulness and propofol anesthesia, modeled as GABA\\(_A\\) receptor potentiation. The firing rates were convolved with a canonical hemodynamic response function to generate simulated BOLD signals (done with the BOLD-monitor integrated in the TVB platform). The\nFigure 4: Transition from asynchronous irregular to UP-and-DOWN dynamics across the different components and scales of our framework: spiking network (single-cell models), mean-field and whole-brain model. Raster plots (A–C_I, v) and average firing rate (A–C_II, VI) of the excitatory (blue) and inhibitory (red) AdEx neurons in the spiking network, with the corresponding mean-field dynamics (A–C_III, VII) and whole-brain model (A–C_IV, VIII). For each of the A,B,C cases, a different microscopic parameter (\\( b_e, \\tau_e, \\tau_i \\) respectively) is changed to produce synchronous dynamics. A. Increased spike-frequency adaptation current \\( b_e \\) simulating NREM sleep, \\( b_e =5\\)pA in AI and 120pA in UD, \\( \\tau_e = \\tau_i =5\\)ms in both conditions, \\( v_{drive} =0.4\\)Hz. In the whole-brain model, \\( v_{drive} =0.315\\)Hz for both AI and slow-wave state. B. Decreased excitatory synaptic decay, \\( \\tau_e \\), mimicking the action of NMDA-blockers( \\( \\tau_e =5\\)ms in AI and 3.75ms in UD, \\( b_e =20\\)pA in both conditions\\( v_{drive} =0.55\\)Hz). In the whole-brain model, \\( b_e =5\\)pA and \\( \\tau_e =5\\)ms in AI, \\( b_e =30\\)pA and \\( \\tau_e =3.75\\)ms in synchronous state and \\( v_{drive} =0.315\\)Hz in both states C. Increased inhibitory synaptic decay, \\( \\tau_i \\), mimicking the action of GABA-ergic agents( \\( \\tau_i =5\\)ms in AI and 7.0ms in UD, \\( b_e =10\\)pA in both conditions,\\( v_{drive} =0.345\\)Hz). In the whole-brain model, \\( b_e =5\\)pA and \\( \\tau_e =5\\)ms in AI, \\( b_e =30\\)pA and \\( \\tau_i =7\\)ms in synchronous state and \\( v_{drive} =0.315\\)Hz in both states\n\ncalculated FC matrices were correlated with the same reference SC used for the experimental data. Different seeds (n=16) for noise realizations were implemented to address inter-subject variability. The whole-brain model successfully captures the same transition between the simulated data for wakefulness and propofol anesthesia. Despite a larger increase of SC-FC correlation in the case of simulated general anesthesia, the model qualitatively reproduced their relative difference.\n\nState-dependent Evoked Dynamics: Perturbational Complexity Index Conscious and unconscious states exhibit distinct brain responses to external stimuli, with a longer and more widespread propagation of brain activity across the brain during conscious states (Massimini et al., 2005). This state-dependent response is quantified and clinically study with the Perturbational Complexity Index (PCI), which can distinguish different states of consciousness by quantifying the complexity of EEG responses after a TMS-induced direct cortical perturbation (Casali et al., 2013; Massimini et al., 2005). Conscious individuals typically demonstrate higher PCI values compared to those during NREM sleep or under general anesthesia (Fig. 6.B).\n\nHere, we adopt a similar approach to explore how perturbations propagate through a network of mean-fields in the whole-brain model. Goldman et al. (2022) demonstrated that simulated NREM sleep, modeled with increased spike-triggered adaptation in the whole-brain model, was characterized by lower PCI values compared to wake-like states. In this study, we extend this analysis to simulated anesthesia, comparing it with both simulated NREM sleep and wakefulness.\n\nThe perturbation was introduced in the whole brain model as a square wave of amplitude 1 Hz and a duration of 50 ms, applied to the excitatory population of the caudal part of the right middle\nFigure 5: Structure-function correlation is increased under anesthesia. A) Resting-state fMRI BOLD signals from 26 individuals were obtained during wakefulness and under propofol anesthesia and were used to compute the functional connectivity matrix (FC) for each participant. We observe a significantly higher correlation between the structural connectivity (SC) and FC for the case of propofol anesthesia. B) The whole-brain model was used to simulate BOLD signals for the wake-like (\\( b_r = 30\\mu A,\\ \\tau_r = 5ms \\)) and propofol anesthesia (\\( b_r = 30\\mu A,\\ \\tau_r = 7ms \\)) conditions (16 different noise realizations). An increased correlation between SC-FC was observed, similar to the experimental data. *** p < 0.001 from Mann-Whitney U test. Middle white line: median; white dot: mean; box limits: first quartile (Q1) and third quartile (Q3) of the data; whiskers: 1.5x inter-quartile range (IQR); Black dots show the SC-FC correlation per subject or noise realization.\n\nfrontal gyrus. In Figure 6.C, we provide a graphical representation of the spatiotemporal aspects of the signal propagation. The plot illustrates the time each region exceeded the significance activation threshold. The results indicate that, in the case of simulated wakefulness, the signal propagated extensively across the cortex, with regions becoming activated late (depicted in blue). In contrast, during simulated unconscious states, only a few regions surpassed the significance threshold, and these activations occurred primarily shortly after the initial stimulus.\n\nIn Figure 6.A we show the PCI values calculated across 60 trials (using different noise seeds) per condition. We observe that simulated wakefulness is associated with higher PCI values compared to all other unconscious states, namely NREM sleep , NMDA-blocker anesthesia , and GABA_A-potentiators anesthesia.\n\nWhile PCI values in wake-like condition were significantly higher than the unconscious states (p<0.001), a high degree of overlap was found among the unconscious, with no significant differences detected between the different simulated mechanisms of general anesthesia, although both were lower than NREM sleep.\n\n3 Discussion\n\nWe present a new computational framework to simulate emergent dynamics and brain states arising from changes at the molecular scale. Our approach utilizes a multiscale model that begins at the cellular level and follows a bottom-up methodology to reach the whole-brain scale. A key aspect of our approach is\nFigure 6: Reduced responsiveness to external stimulus in unconscious states (simulated (A,C) and empirical (B)). A. Perturbational Complexity Index (PCI) values for the cases of simulated wakefulness (\\( b_c = 5\\mu A \\), \\( \\tau_c = \\tau_i = 5.0\\text{ms} \\)), anesthesia (NMDA-blockers (\\( \\tau_c = 3.75\\text{ ms}, b_c = 30\\mu A \\)), GABA_A receptors potentiation(\\( \\tau_i = 8.0\\text{ms}, b_c = 30\\mu A \\))) and NREM sleep (\\( b_c = 120\\mu A, \\tau_c = \\tau_i = 5.0\\text{ms} \\)). Each point corresponds to a different noise realization of the model (in total 60 trials per condition). The horizontal axis corresponds to the noise seed used for the specific simulation, so that each pair of wakefulness-unconscious state is plotted on the same vertical axis; in the most right panel the raw jittered data are collapsed to the same vertical axis for each condition; the limits of boxplots include the first quartile (Q1) and third quartile (Q3) of the data, the middle horizontal lines correspond to the median values; the half violin plots describe the probability density function; Post-hoc Conover tests were performed to assess statistical significance of the difference in PCI values between the conditions, and the Holm-Bonferroni method was used to control for multiple comparisons (*: p<0.05, **: p<0.01, ***: p<0.001). B. Modified from Casali et al. (2013): Empirical PCI data from human subjects showing a clear distinction between awake and unconscious individuals. C. Spatiotemporal dynamics of applied perturbation propagation. Following stimulation, applied at t = 0ms, all regions were evaluated to determine if they surpassed the significance threshold, as defined by the PCI calculation algorithm. The time each region exceeded this threshold is color-coded showcasing a widespread and temporally sustained signal propagation during wakefulness. The yellow cross denotes the stimulated region, corresponding to the caudal part of the right middle frontal gyrus.\n\nthe use of biophysically grounded mean-field models to bridge the gap between the micro and macro scales, enhancing computational efficiency by reducing the system dimensionality. Additionally, the bottom-up mean-field models developed and implemented in our framework incorporate all cellular parameters, which allows us to capture the emergence of different brain states and brain dynamics generated by changes at the cellular level and to understand the mechanisms behind these transitions.\n\nTo demonstrate the application of our framework, we study the effects of common anesthetics at the whole brain level. Our approach successfully captures the different mechanisms leading to changes in brain states (between conscious and unconscious states) in sleep and anesthesia, highlighting the generality of our approach. Furthermore, we illustrate how our model can explain the transition between dynamical states and the complex interplay between different molecular parameters and mechanisms underlying these transitions. These characteristics make our model suitable for modeling anesthetics in biologically realistic scenarios. Previous studies have used the mean-field approach to model the macroscopic effects of general anesthesia on the brain at the macroscale (Luppi et al., 2022), and the action of psychedelic compounds on the brain (Deco et al., 2018; Herzog et al., 2023), however, without explicitly considering the biophysical details of the molecular action.\n\nOur model holds great potential for clinical applications, where it could be used to predict particular activity patterns as a function of anesthesia depth, such as the level of diminished responsiveness, which may be interesting to explore for intermediate anesthesia levels.\n\nTo yield more precise models providing a quantitative comparison with experimental data, it is crucial to accurately reconstruct brain signals (such as EEG, MEG or MRI) from mean-field models, as proposed recently (Tesler et al., 2022, 2023b), which will allow a more direct comparison with experiments. In addition, it is of great importance to include regional variations, by designing specific models for each\nbrain area, as done recently for non-cortical structures (Overwiening et al., 2023; Tesler et al., 2023a, 2024). We hope that this level of biophysical accuracy will bring the model closer to a quantitative account of the fine details of the experimental data, and be more precise and specific to investigate their underlying mechanisms.\n\n4 Methods\n\nWe describe here the details of the multiscale whole-brain model: we start at the cellular level with the introduction of the single-cell model, then we move to the mesoscale with the construction of a neuronal network and the formulation of a mean-field model describing the mesoscopic network activity, and we end at the whole brain scale using a large network of mean-fields interconnected using the anatomical connectome, step realized through the integration in The Virtual Brain simulator (Fig. 1).\n\n4.1 Single cell model\n\nThe dynamics of the single neuron are based on the adaptive exponential integrate-and-fire model (AdEx) and are described by the following equations (Brette and Gerstner, 2005):\n\n\\[\nc_m \\frac{dv}{dt} = g_L(E_L - v) + g_L \\Delta e^{\\frac{v-v_{thr}}{\\Delta}} - w + I_{syn}\n\\]\n(1)\n\\[\n\\frac{dw}{dt} = -\\frac{1}{\\tau_w}(a(v-E_L)-w) + b \\sum_{t_{sp}} \\delta(t-t_{sp})\n\\]\n(2)\n\nwhere \\( v \\) is the membrane potential, \\( c_m = 200 \\) pF is the membrane capacitance and \\( g_L = 10 \\) nS is the leak conductance. The leakage reversal potential \\( E_L \\) equals -65 mV and -64 mV for inhibitory and excitatory cells respectively. The exponential term \\( \\Delta \\) has a different strength for the two types of cells (2 mV for excitatory and 0.5 mV for inhibitory cells). \\( W \\) and \\( I_{syn} \\) describe the adaptation and synaptic current respectively. Parameter \\( a \\) describes the sub-threshold adaptation and \\( b \\) describes the spike-triggered adaptation. A spike is generated when the membrane potential exceeds a voltage threshold \\( v_{thr} = -50 \\) mV at time \\( t_{sp} \\). The neuron’s membrane potential is subsequently reset to a resting voltage \\( v_{rest} = -65 \\) mV and fixed to that value for a refractory period \\( T_{refr} = 5 \\) ms. The Dirac \\( \\delta \\)-function indicates that whenever a neuron fires at time \\( t_{sp}(k) \\), the adaptation current \\( W \\) is incremented by an amount \\( b \\). Based on physiological characteristics (Destexhe, 2009), the inhibitory cells are modelled as fast-spiking (FS) neurons, exhibiting no adaptation (\\( a_i = b_i = 0 \\)). Excitatory neurons are modelled as regular spiking (RS) cells, characterised by lower excitability due to the presence of spiking frequency adaptation (\\( b_e \\) varies in our simulations, \\( a_e = 0 \\)nS, and the adaptation time constant \\( \\tau_w = 500 \\)ms).\n\n4.2 Synaptic model\n\nEach neuron \\( k \\) receives a synaptic current \\( I_{syn} \\), which corresponds to the spiking activity of all presynaptic neurons \\( j \\in \\text{pre}(k) \\) of neuron \\( k \\). \\( I_{syn} \\) can be decomposed to the input received from excitatory (E) and inhibitory (I) presynaptic spikes, so as\n\n\\[\nI_{syn} = G_{syn}^e (E_e - v) + G_{syn}^i (E_i - v),\n\\]\n(3)\n\nwhere \\( E_e = 0 \\)mV (\\( E_i = -80 \\)mV) is the excitatory (inhibitory) reversal potential and \\( G_{syn}^e \\) (\\( G_{syn}^i \\)) the excitatory (inhibitory) synaptic conductance. Synaptic conductances were modeled by a decaying exponential function that sharply increases by a fixed amount \\( Q_x \\) , at each spiking time (\\( t_{sp,j_x} \\)) of a presynaptic neuron \\( j_x \\):\n\n\\[\nG_{syn}^x(t) = Q_x \\sum_{t_{sp,j_x}} \\Theta(t - t_{sp,j_x}) \\ e^{-\\frac{t-t_{sp,j_x}}{\\tau_x}},\n\\]\n(4)\n\nwhere x corresponds to the population type (\\( x \\in \\{e, i\\} \\)), \\( \\Theta \\) is the Heaviside function, \\( \\tau_x \\) is the characteristic decay time of synaptic conductances (varied in our simulations), and \\( Q_x \\) is the quantal conductance (\\( Q_e = 1.5 \\)nS , \\( Q_i = 5 \\)nS). The sum runs over all the spiking times of excitatory (\\( t_{sp,j_e} \\)) or inhibitory (\\( t_{sp,j_i} \\)) presynaptic neurons \\( j_e \\) or \\( j_i \\) of neuron \\( k \\).\n\n4.3 Spiking network model\n\nWe studied a network of \\( N = 10^4 \\) integrate-and-fire neurons that displayed spike-frequency adaptation (Destexhe, 2009; Zerlaut et al., 2018). The neurons were connected over a topologically random network with a probability of connection between two neurons equal to \\( p = 5\\% \\). The network was composed of two populations of inhibitory and excitatory neurons, with the inhibitory neurons consisting the 20% of the whole network size.\n\n4.4 Mean-field model\n\nThe mean-field used here is based on a bottom-up formalism derived from a Master Equation (El Boustani and Destexhe, 2009), and which has recently been extended to include the effects of adaptation (Zerlaut et al., 2018; Di Volo et al., 2019). The mean-field equations of the system can be written as :\n\\[\nT \\frac{\\partial v_{\\mu}}{\\partial t} = (F_{\\mu} - v_{\\mu}) + \\frac{1}{2} c_{\\lambda \\eta} \\frac{\\partial^2 F_{\\mu}}{\\partial v_{\\lambda} \\partial v_{\\eta}}\n\\]\n\\[\nT \\frac{\\partial c_{\\lambda \\eta}}{\\partial t} = \\delta_{\\lambda \\eta} \\frac{F_{\\lambda}(1/T - F_{\\eta})}{N_{\\lambda}} + (F_{\\lambda} - v_{\\lambda})(F_{\\eta} - v_{\\eta})\n+ \\frac{\\partial F_{\\lambda}}{\\partial v_{\\mu}} c_{\\eta \\mu} + \\frac{\\partial F_{\\eta}}{\\partial v_{\\mu}} c_{\\lambda \\mu} - 2c_{\\lambda \\eta}\n\\]\n\\[\n\\frac{\\partial W}{\\partial t} = \\frac{1}{\\tau_w}(a(\\mu_V(v_e, v_i, W) - E_L) - W) + b v_e ,\n\\]\nwhere \\( \\mu = \\{e, i\\} \\) is the neural population index (excitatory or inhibitory), \\( v_{\\mu} \\) the mean firing rate of the corresponding population, \\( c_{\\lambda \\eta} \\) the covariance between populations (\\( \\lambda \\) and \\( \\eta \\)), \\( W \\) is the mean adaptation, and \\( T \\) is the mean-field characteristic time constant.\n\nThe function \\( F_{\\mu} = F_{\\mu}(v_e, v_i, W) \\) is the transfer function (TF) of a neuron of type \\( \\mu \\), i.e. its output firing rate when receiving inhibitory and excitatory inputs with rates \\( v_e \\) and \\( v_i \\), and adaptation level \\( W \\). The TF can be derived following a semi-analytic approach (Zerlaut et al. (2018)), where the output firing rate of a neuron can be written as a function of its mean subthreshold membrane voltage \\( \\mu_V \\), its standard deviation \\( \\sigma_V \\), and its time correlation decay time \\( \\tau_V \\):\n\n\\[\nF = v_{out} = \\frac{1}{2\\tau_V} \\cdot \\mathrm{Erfc} \\left( \\frac{V_{thr}^{\\mathrm{eff}} - \\mu_V}{\\sqrt{2}\\sigma_V} \\right).\n\\]\n\nwhere \\( (\\mu_V, \\sigma_V, \\tau_V) \\) are calculated as a function of the input firing rates (\\( v_E, v_I \\)) and the adaptation intensity \\( W \\) following the equations described in Di Volo et al. (2019). The \\( V_{thr}^{\\mathrm{eff}} \\) is the phenomenological spike threshold voltage taken as a second-order polynomial:\n\n\\[\nV_{thr}^{\\mathrm{eff}}(\\mu_V, \\sigma_V, \\tau_V^N) = P_0 + \\sum_{x \\in [\\mu_V, \\sigma_V, \\tau_V^N]} P_x \\left( \\frac{x - x_0}{\\delta x_0} \\right)\n+ \\sum_{x,y \\in [\\mu_V, \\sigma_V, \\tau_V^N]^2} P_{xy} \\left( \\frac{x - x_0}{\\delta x_0} \\right) \\left( \\frac{y - y_0}{\\delta y_0} \\right),\n\\]\n\nwhere \\( \\tau_V^N = \\frac{\\tau_V G_e}{C_m} \\) a non-dimensional quality. The polynomial coefficients of \\( P \\) are determined through a fitting of the TF template to the output firing rate of individual neuron simulations, varying both inhibitory and excitatory inputs. The values for the normalization of the fluctuation regime were set following previous work (Zerlaut et al., 2018; Di Volo et al., 2019): \\( \\mu_V^0 = -60 \\) mV, \\( \\sigma_V^0 = 0.004 \\) mV, \\( (\\tau_V^N)^0 = 0.5 \\), \\( \\delta \\tau_V^0 = 0.001 \\) mV, \\( \\delta \\sigma_V^0 = 0.006 \\) mV and \\( \\delta (\\tau_V^N)^0 = 1 \\). The fit is performed for each of the cell types included in the network, so in our case for fast and regular spiking cells. As shown in Di Volo et al. (2019) the mean-field predictions work even far from the fitting point of the TF, so in all the examples showcased in this work we used previously calculated \\( P \\), fitted for similar parameterizations of the two types of cells (see Table 1).\n\nTaking the first-order equations by disregarding the covariance term dynamics in Equation 5, the mean-field model for the excitatory and inhibitory populations representing a cortical volume can be written as:\n\n\\[\nT \\frac{dv_e}{dt} = \\mathcal{F}_e(v_e + v_{auff}, v_i, W) - v_e\n\\]\n\\[\nT \\frac{dv_i}{dt} = \\mathcal{F}_i(v_e + v_{auff}, v_i, W) - v_i\n\\]\n\\[\n\\frac{dW}{dt} = -\\frac{W}{\\tau_w} + b v_e + \\frac{a}{\\tau_w}(\\mu_V(v_e, v_i, W) - E_L) ,\n\\]\n\nwhere \\( v_{auff} \\) denotes an afferent input to both type of populations which we write as:\n\n\\[\nv_{auff}(t) = v_{drive} + \\sigma \\xi(t),\n\\]\n\nwhere \\( \\sigma = 3.5 \\) and \\( \\xi(t) \\) denotes an Ornstein-Uhlenbeck (OU) process, of the form:\n\n\\[\nd\\xi(t) = -\\xi(t) \\frac{dt}{\\tau_{OU}} + dW_t\n\\]\n\nwhere \\( \\tau_{OU} = 5 \\)ms is the timescale of the OU process and \\( dW_t \\) is a Wiener process of amplitude one and zero average. The \\( v_{drive} \\) received different values in our simulations depending on the microscopic parameter that was selectively changed.\n\n4.5 Networks of mean-field models\n\nTo model whole-brain dynamics, a network of mean-fields is defined, where each mean-field describes the activity of a brain region. The interactions between the mean-fields are excitatory while the inhibitory connections are preserved solely on the regional level. Extending on the single mean-field equations (Eq. 7), now the population activity of each region is given by the following equations:\n\n\\[\nT \\frac{dv_{e(k)}}{dt} = \\mathcal{F}_e[v_{e(input)}(k), v_{i(k)}, W(k)] - v_{e(k)}\n\\]\n\\[\nT \\frac{dv_{i(k)}}{dt} = \\mathcal{F}_i[v_{e(input)}(k), v_{i(k)}, W(k)] - v_{i(k)}\n\\]\n\\[\n\\frac{dW(k)}{dt} = -W(k) + b \\tau_w v_{e(k)}\n+ a(\\mu_V(v_{e(k)}, v_{i(k)}, W(k)) - E_L) ,\n\\]\n\nwhere \\( v_{e(k)} \\) (\\( v_{i(k)} \\)) describes the firing rates of the excitatory (inhibitory) population of the region (\\( k \\)), \\( W(k) \\) the adaptation of the population, and \\( v_{e(input)}(k) \\) is the total excitatory synaptic input that the region\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Cell Type\\( P_0 \\)\\( P_{\\mu V} \\)\\( P_{rV} \\)\\( P_{rN}^V \\)\\( P_{\\mu V}^2 \\)\\( P_{rV}^2 \\)\\( (P_{rN}^V)^2 \\)\\( P_{\\mu V}\\sigma V \\)\\( P_{\\mu V}\\tau N^V \\)\\( P_{rV}\\tau N \\)
RS-cell-50.174.52-7.94-2.08-0.553.42-11.561.952.74-10.67
FS-cell-51.856.16-14.041.67-2.063.18-31.136.571.72-45.16
\n\nTable 1: Fitting parameters expressed in mV\n\nreceives from the rest of the nodes of the network, given by the following equation:\n\n\\[\nv_e^{input}(k) = v_e(k) + v_{aff}(k) \\\\\n+ G \\sum_j C_{jk} v_e(j,t - \\|j-k\\|/v_c)\n\\]\n\nwhere the sum runs over all nodes \\( j \\) connected to node \\( k \\), and \\( C_{jk} \\) the connection strength between \\( j \\) and \\( k \\) (and is equal to 1 for \\( j = k \\)), and the global coupling factor \\( G \\) rescales the connection strength while maintaining the ratio between different values. The term \\( \\|j-k\\| \\) is the distance between the nodes \\( j \\) and \\( k \\), while \\( v_c \\) is the speed with which the signal propagates along the axis so that the model accounts for the delay of axonal propagation. Here \\( v_{aff} \\) is defined as in Eq. 8.\n\nA cortical parcellation of 68 regions was used. The connection strengths and tract lengths between the nodes were provided by the Berlin empirical data processing pipeline, based on human tractography methods (Schriner et al., 2015). We performed the simulations using The Virtual Brain (TVB) platform, leveraging its capabilities to model and simulate large-scale brain networks. TVB offers a useful tool to study the dynamics of the entire brain through the construction of a network defined by its large-scale structural connectivity and the mesoscopic models that describe each node’s intrinsic dynamics. This approach allows us to simulate and analyze the complex interactions and emergent properties of the brain’s functional dynamics at both the mesoscopic and macroscopic levels.\n\n4.6 Data for Structural-Functional Connectivity Analysis\n\nSimulated BOLD signals The simulated BOLD signal was generated through the dedicated BOLD monitor provided by The Virtual Brain software. The simulated mean field time series of the excitatory population (down-sampled at 250Hz) of each node were convolved with the hemodynamic response function (described by the first order Volterra kernel of the Ballon Windekessel model (Friston et al., 2000)). This signal was finally down-sampled to the frequency matching the repetition time (TR) of the fMRI series. For the simulations of the human brain, the human connectome described in 4.5 was used.\n\nHuman fMRI Data Details can be found in (Huang et al., 2021).\n\n4.7 Evoked activity and PCI calculation\n\nThe Perturbational Complexity Index (PCI), as proposed by Casali et al. (Casali et al., 2013) is the normalized Lempel-Ziv complexity of the evoked spatiotemporal patterns of cortical activation \\( SS(x,t) \\) and was computed to capture the complexity of the signal propagation after a stimulation. Evoked potentials were generated using the whole-brain model, where a square wave stimulus was applied on the firing rates of the excitatory population on a single node (corresponding to the right premotor cortex). 60 different trials, each with a different stimulus onset and noise realization, were performed where the analysis concerns an interval of 300 ms pre- and post-stimulus. The firing rates of the excitatory populations were firstly binarized to extract significant vectors \\( s(t) \\) per trial, and the Lempel-Ziv complexity \\( LZ(S) \\) was calculated for each of these vectors (Goldman et al., 2022). Finally the PCI is expressed as the ratio of \\( \\frac{LZ(S)}{H(S)} \\) where \\( H(S) \\) is the spatial source entropy:\n\n\\[\nH(S) = -p(S=0)\\log_2(p(S=0)) \\\\\n- p(S=1)\\log_2(p(S=1))\n\\]\n\n(10)\n\n4.8 Data availability\n\nData used in this article can be found in https://zenodo.org/records/6955280\n\n4.9 Code availability\n\nThe code source of all simulations shown in this article is available online in https://github.com/mariasacha/paper_pipeline_hub/.\n\nAcknowledgments\n\nResearch supported by the CNRS and the European Union (Human Brain Project H2020-785907, H2020-945539, Virtual Brain Twin project 101137289).\nReferences\n\nAlexandersen, C.G., Duprat, C., Ezzati, A., Houzelstein, P., Ledoux, A., Liu, Y., Saghir, S., Destexhe, A., Tesler, F., Depannemaeker, D., 2024. A mean field to capture asynchronous irregular dynamics of conductance-based networks of adaptive quadratic integrate-and-fire neuron models. 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Modeling mesoscopic cortical dynamics using a mean-field model of conductance-based networks of adaptive exponential integrate-and-fire neurons. Journal of Computational Neuroscience 44, 45–61."} {"paper_id": "prb24", "title": "Developmental atlas of phase-amplitude coupling between physiologic high-frequency oscillations and slow waves", "text": "# Abstract\n\nThe cortex generates high-frequency oscillations (HFO) nested in slow waves during sleep, and these signals are especially elevated in the seizure onset zone. Thus, HFO occurrence rate and Modulation Index (MI), which quantifies the strength of coupling between HFO amplitude and slow-wave phase, represent promising epilepsy biomarkers. However, their diagnostic utility may be suboptimal because the endogenous developmental distributions are unknown. To improve age-appropriate localization of the epileptogenic zone, we hence constructed normative brain atlases demonstrating the developmental changes in MI and HFO rate.\n\nOur study investigated extraoperative, intracranial EEG data from 114 patients with focal epilepsy (ages 1.0 to 41.5 years) who achieved International League Against Epilepsy class I outcomes following resective surgery. We analyzed 20-minute slow-wave sleep epochs at 8,251 nonepileptic electrode sites (those outside the seizure onset zone, interictal spike zone, or MRI-visible lesions). Each electrode was transposed onto a standard brain template, and we then calculated its MI and HFO occurrence rate using four different detector toolboxes. Linear and nonlinear regression models determined the developmental slope of MI and HFO rate at each cortical mesh point. Mixed model analysis established the significance of MI and HFO rate developmental changes in each region of interest, while accounting for the independent effects of patient and epilepsy profiles. Finally, we created a dynamic tractography movie visualizing white matter pathways connecting cortical regions showing developmental co-growth in MI.\n\nWe found that the occipital lobe exhibited enhanced MI compared to other lobes in both children and adults. Increased age, square root of age, and log base 10 of age were independently associated with elevated MI exclusively in the occipital lobe. The cortical regions showing developmental co-growth in MI were connected via the vertical occipital fasciculi and posterior callosal fibers. In contrast, we did not observe any significant association between age measures and HFO rate in the occipital lobe, but rather noted an inverse relationship between age and HFO rate in the temporal, frontal, and parietal lobes.\n\nOur study suggests that phase-amplitude coupling between physiologic HFO and delta waves, as rated by MI, is strengthened during development, in the occipital lobe particularly during toddlerhood and preschool. Given that occipital delta-nested HFO are believed to support visual memory consolidation, our observations imply that process may be significantly strengthened during early childhood. The data is publicly available to provide investigators with a crucial reference for MI and HFO-based presurgical evaluation of the epileptogenic zone.\n\nHealth sciences/Diseases/Neurological disorders/Epilepsy \nBiological sciences/Neuroscience/Diseases of the nervous system/Epilepsy\n\n# Introduction\n\nIn patients with drug-resistant focal epilepsy, surgical resection of the epileptogenic zone results in long-term seizure control, and clinicians employ intracranial EEG (iEEG) recording via subdural and/or depth electrodes to localize such areas. The occurrence rate of spontaneous interictal high-frequency oscillations (HFO) - defined as transient bursts of ≥ 80 Hz activity (Zweiphenning et al., 2022 a) - has garnered significant attention as an iEEG-based epilepsy biomarker, since it is generally increased in the seizure onset zone (SOZ) (Gloss et al., 2014; Höller et al., 2015; Frauscher et al., 2017; Remakanthakurup Sindhu et al., 2020). Furthermore, a randomized clinical trial involving 78 patients with extratemporal lobe epilepsy recently reported that the efficacy of HFO-guided resection in controlling seizures was non-inferior to that of conventional resection guided by interictal spike discharges (Zweiphenning et al., 2022 a).\n\nIn addition, HFO are generally nested within slow waves during sleep, and modulation index (MI) is a quantitative measure of the coupling strength between HFO amplitude and slow-wave phase (Canolty et al., 2006; Miyakoshi et al., 2013). MI represents a potentially valuable iEEG-based epilepsy biomarker; in particular, it is an effective proxy measure for epileptiform spike-and-wave discharges, since each spike component is associated with a transient increase in HFO that is stereotypically coupled with a delta wave (Motoi et al., 2018; Kural et al., 2020). Retrospective analysis of iEEG recordings from human epilepsy patients demonstrated that MI is elevated in the SOZ, and complete resection of high-value MI sites was associated with better postoperative seizure outcomes (Nonoda et al., 2016; Iimura et al., 2018; Motoi et al., 2018; Kural et al., 2020; Kuroda et al., 2021; Ma et al., 2021). Notably, MI has advantages over HFO rate as a biomarker that include being a continuous measure and requiring significantly less computational time (Kuroda et al., 2021).\n\nIn clinical practice, caution is required when using MI and HFO rate as iEEG biomarkers because these signals are endogenously present and exhibit topographical variation across the cortex (Guragain et al., 2018; Bernabei et al., 2022; Taylor et al., 2022). The occipital lobe is an area that naturally exhibits elevated MI and HFO rate, regardless of epileptogenicity (Nagasawa et al., 2012; Alkawadri et al., 2014; Frauscher et al., 2018; Kuroda et al., 2021). However, the developmental implications of these physiologic distributions remain unknown, and gleaning this knowledge is expected to significantly improve interpretation of iEEG biomarker clinical significance, in the pediatric brain.\n\nThe aim of the present study was to create a novel normative atlas that visualizes developmental changes in MI and HFO rate across artifact-free nonepileptic iEEG electrode sites (defined as those outside the SOZ, interictal spike zone, and MRI-visible lesions; Frauscher et al., 2018; Kuroda et al., 2021; Bernabei et al., 2022; Taylor et al., 2022). To optimize the generalizability of our observations, we employed four different detector toolboxes to calculate HFO rate (Staba et al., 2002; Gardner et al., 2007; Crépon et al., 2010; Zelmann et al., 2010) and used mixed model analysis to determine whether the observed developmental slope of iEEG biomarkers remained significant after accounting for the independent effects of patient and epilepsy profiles (Sakakura et al., 2022).\n\nInvasive studies of healthy cortices in animal models and nonepileptic cortices of patients with focal epilepsy have reported that spontaneous HFO are nested in delta waves and involve large-scale cortical networks during slow-wave sleep (Steriade et al., 1993; Contreras et al., 1996; Sanchez-Vives and McCormick, 2000; Csercsa et al., 2010; Hangya et al., 2011; Nagasawa et al., 2012; Arnulfo et al., 2020). This nested HFO during slow-wave sleep is believed to replay sensory-related neural communications across two regions occurring during wakefulness and facilitate the consolidation of long-term memory related to given sensory representations. For example, spontaneous HFO ≥ 80 Hz nested in delta waves 0.5−1 Hz in the primary visual cortex during slow-wave sleep are thought to be involved in the consolidation of visual memory (Ji and Wilson, 2007; Mehta, 2007; Sasaki et al., 2010; Buzsáki and da Silva, 2012; Nagasawa et al., 2012).\n\nGiven that preverbal infants are known to encode and retain visual information (Werner and Perlmutter, 1979) and this process likely involves HFO-delta phase-amplitude coupling, we hypothesized that young children would have already developed the spatial profile of MI ≥ 80 Hz & 0.5−1 Hz: namely physiological enhancement in the nonepileptic occipital lobe, as seen in older children and adults. In addition, since pattern recognition memory is known to improve most rapidly before six years of age (Toornstra et al., 2019), we further hypothesized that the developmental slope of MI ≥ 80 Hz & 0.5−1 Hz would be steepest during young childhood. Here, MI ≥ 80 Hz & 0.5−1 Hz denotes the strength of coupling between the amplitude of HFO ≥ 80 Hz and the phase of slow-wave 0.5−1 Hz.\n\nIn addition to modeling cortical ontogenic changes, the present study also visualized white matter pathways supporting the development of neural communications via delta-nested HFO (as rated by MI ≥ 80 Hz & 0.5−1 Hz), during slow-wave sleep. To accomplish this, we utilized our novel imaging technique, dynamic tractography, which combines iEEG signals with MRI tractography (Sonoda et al., 2021; Kitazawa et al., 2023; Ono et al., 2023). Previous studies in animal models and patients with focal epilepsy have demonstrated that neural circuits engaging in high-frequency communication are susceptible to use-dependent modifications of synaptic transmission that enhance effective connectivity via monosynaptic white matter tracts in the developing brain (Buonomano and Merzenich, 1998; Singer, 2018; Sonoda et al., 2021). Additionally, white matter development, as rated by MRI tractography, is generally drastic during early childhood and modest during late adolescence (Asato et al., 2010; Lebel et al., 2018; Baum et al., 2022). Using the dynamic tractography method, we visualized intra- and inter-hemispheric, monosynaptic white matter tracts that connect cortical regions exhibiting significant developmental co-growth of MI ≥ 80 Hz & 0.5−1 Hz.\n\n# Materials And Methods\n\n## Patients\n\nWe studied a consecutive series of 114 patients with focal epilepsy (ages 1.0 to 41.5 years) who met the following eligibility criteria (Table 1; Figure S1). Inclusion criteria consisted of: [a] simultaneous video-iEEG recording between January 2007 and November 2020, as part of presurgical assessment at Children's Hospital of Michigan or Harper University Hospital, Detroit Medical Center, [b] iEEG sampling rate of 1,000 Hz (Davis et al., 2018), [c] iEEG contained an artifact-free 20-minute slow-wave sleep epoch at least two hours apart from clinical seizure events (Bagshaw et al., 2009; Nagasawa et al., 2012), and [d] International League Against Epilepsy (ILAE) class 1 outcome in the last follow-up after focal resection (Kuroda et al., 2021). Exclusion criteria included [a] a history of previous resective epilepsy surgery, [b] undergoing hemispherotomy or hemispherectomy, and [c] lacking artifact-free, nonepileptic electrode sites (defined as those outside the SOZ [Asano et al., 2009], interictal spike zone [Kural et al., 2020], and MRI-visible lesions [van Klink et al., 2021]). The Institutional Review Board of Wayne State University approved the current study, and we obtained written informed consent from the patients' legal guardians and written assent from pediatric patients aged 13 years or older.\n\n**Table 1** \nPatient Profile. In Figure S1, we have provided the distribution of patient ages.\n\n| Number of patients | 114 |\n|--------------------|-----|\n| Mean age in years (range) | 11.4 (1.0–41.5) |\n| Proportion of female (%) | 47.4 |\n| Sampled hemisphere (%) | |\n| Left | 45.6 |\n| Right | 43.0 |\n| Both | 11.4 |\n| Seizure onset zone (%) | |\n| Frontal | 24.6 |\n| Temporal | 47.4 |\n| Parietal | 27.2 |\n| Occipital | 19.3 |\n| MRI-visible structural lesion (%) | 66.7 |\n| Mean number of antiseizure medications (range) | 2.0 (1–5) |\n\n## Extraoperative video-iEEG\n\nWe acquired extraoperative video-iEEG data using the same protocols as reported in our previous studies (Nagasawa et al., 2012; Kuroda et al., 2021; Sakakura et al., 2022). A licensed neurosurgeon surgically implanted platinum subdural disk electrodes (3 mm diameter and 10 mm center-to-center distance) on the hemisphere suspected to contain the epileptogenic zone, followed by the placement of surface electromyographic electrodes on the deltoid muscles and electrooculographic electrodes (2.5 cm below and 2.5 cm lateral to the outer canthi) to assess body movements during iEEG recording (Nariai et al., 2011; Nagasawa et al., 2012). Intracranial EEG recording aimed to determine the boundaries of the presumed epileptogenic zone, as well as functionally important cortices, and the spatial extent and duration of iEEG sampling were solely determined by clinical needs specific to each patient. Following implantation, iEEG data was continuously recorded at the bedside with a sampling rate of 1,000 Hz, for 2–7 days. To ensure the accuracy of the developmental iEEG atlases, we only included artifact-free iEEG segments from 8,251 nonepileptic electrode sites (mean: 72.4 per patient; range: 12 to 121; Fig. 1 A). This approach minimized the unwanted effects of pathological HFO events (Guth et al., 2021; Dimakopoulos et al., 2022).\n\n## MRI\n\nWe obtained preoperative 3-tesla MRI data, including T1-weighted spoiled gradient-echo volumetric and fluid-attenuated inversion recovery images (Nakai et al., 2017; Sakakura et al., 2022). The FreeSurfer software package was used to reconstruct the MRI surface image of patients aged two and above (http://surfer.nmr.mgh.harvard.edu; Desikan et al., 2006; Ghosh et al., 2010). In cases where the software failed to detect the pial surface accurately due to insufficient cerebral myelination, a board-certified neurosurgeon (K.S.) manually delineated the pial surface using the Control Point function (https://surfer.nmr.mgh.harvard.edu/fswiki/FsTutorial/ControlPoints_freeview/; Deoni et al., 2015; Croteau-Chonka et al., 2016; Remer et al., 2017; Sakakura et al., 2022). For patients younger than two, we used the Infant FreeSurfer software package to reconstruct the surface image (https://surfer.nmr.mgh.harvard.edu/fswiki/infantFS; Zöllei et al., 2020; Sakakura et al., 2022).\n\nWe displayed electrode sites on the pial surface of the brain using preoperative MRI and a post-implant CT image (Stolk et al., 2018; Sakakura et al., 2022). Two board-certified neurosurgeons (K.S. and N.K.) visually assessed intraoperative photographs to confirm the spatial accuracy of electrode locations co-registered to the MRI surface image (Pieters et al., 2013). In order to pool sites from all patients, it was necessary to normalize the electrode locations to the standardized FSaverage brain surface (http://surfer.nmr.mgh.harvard.edu). In a previous iEEG study of 32 patients, we found that the mean coregistration error ranged below 0.4 mm, and there was no significant correlation between patient age and the severity of coregistration error (Sakakura et al., 2022).\n\n## Focal resection and postoperative seizure outcome\n\nIn our previous studies (Asano et al., 2009; Sonoda et al., 2022), we described the guiding principle for determining the boundary of cortical resection. Our aim was to remove the SOZ and any adjacent MRI lesions, while preserving functionally-important cortex; this procedure is intended to maximize seizure control and minimize development of cognitive and/or sensorimotor deficits. Importantly, none of the data from this study was available to inform clinical decision making. Consistent with the study design, all 114 patients achieved ILAE Class-1 outcome at the last follow-up, which occurred at least one year after surgery.\n\n## Modulation index (MI)\n\nWe identified artifact-free, 20-minute slow-wave sleep iEEG recordings that were at least 2 hours apart from ictal events using visual assessment (Bagshaw et al., 2009; Motoi et al., 2018; Kuroda et al., 2021). At each artifact-free nonepileptic site, we used the EEGLAB winPACT toolbox (https://sccn.ucsd.edu/wiki/WinPACT; Miyakoshi et al., 2013) to automatically compute MI; this program transforms all iEEG data points into Hilbert spectra and quantifies the strength of coupling between HFO amplitude and the instantaneous phase of slow waves. In the notation MI≥f Hz & s Hz denotes the strength of coupling between the amplitude of HFO≥f Hz and the phase of slow-wave s Hz.\n\nBelow, we report the normative developmental changes primarily in MI≥80 Hz & 0.5−1 Hz (Fig. 2), which is considered a surrogate marker of the delta-nested HFO that are believed to underly consolidation of long-term memory related to given sensory representations (Ji and Wilson, 2007; Mehta, 2007; Sasaki et al., 2010; Buzsáki and da Silva, 2012; Nagasawa et al., 2012; Nonoda et al., 2016). We also report the normative developmental changes in MI≥80 Hz & 3−4 Hz, which are suggested to be increased in iEEG traces showing frequent interictal spike-and-wave discharges (Motoi et al., 2018; Kural et al., 2020). The normative spatial variability of this biomarker value could be a valuable reference in epilepsy presurgical evaluation.\n\n## High-frequency oscillation (HFO)\n\nDuring the same 20-minute slow-wave sleep iEEG epochs described above, we used the RIPPLELAB software (https://github.com/BSP-Uniandes/RIPPLELAB/; Navarrete et al., 2016) to compute the HFO rate at each artifact-free nonepileptic site, using four different detection algorithms: [1] Short Time Energy (STE) method (Staba et al., 2002), [2] Short Line Length (SLL) method (Gardner et al., 2007), [3] Hilbert (HIL) method (Crépon et al., 2010), and [4] Montreal Neurological Institute (MNI) method (Zelmann et al., 2010). The STE method defines a HFOSTE≥f Hz event as an iEEG segment presenting successive root mean square values greater than five standard deviations above the overall mean of root mean squares and containing more than six peaks greater than three standard deviations on the f-Hz high-pass filtered iEEG trace. The SLL method defines a HFOSLL≥f Hz as an iEEG segment presenting SLL amplitude augmentation greater than the 97.5th percentile of the empirical cumulative distribution function computed on the f-Hz high-pass filtered iEEG trace. The HIL method defines a HFOHIL≥f Hz as an iEEG segment presenting Hilbert transform-based envelope augmentation greater than five standard deviations on the f-Hz high-pass filtered iEEG trace. The MNI method defines a HFOMNI≥f Hz as an iEEG segment presenting root mean square energy above the 99.9999th percentile compared to the baseline. If the baseline was absent due to persistent high-frequency activity, the MNI method treated an iEEG segment presenting the ≥95th percentile of the cumulative distribution function as computed on the 1-minute f-Hz high-pass filtered iEEG trace. We used the default parameter settings in the RIPPLELAB software, as reported previously (Kuroda et al., 2021). In the present study, we focused on reporting the developmental changes in the occurrence rate of HFOHIL≥80 Hz (/min) as HFO event was defined commonly on Hilbert transformed iEEG traces when quantifying the HFOHIL occurrence rate and computing MI.\n\nAn ancillary analysis was performed on the rates of HFO≥150 Hz and HFO≥250 Hz for interested readers.\n\n### Statistical analysis to confirm physiological enhancement of MI and HFO in the occipital lobe during young childhood\n\nIn a previous study, we created normative atlases of MI and HFO based on data from 47 patients aged between 4 and 19 years, which revealed a general enhancement of these measures in the occipital lobe (Kuroda et al., 2021). In the current study, we aimed to replicate this finding in a cohort of 14 children aged between 1.0 and 3.9 years and 100 individuals aged 4 years or older. We used mixed model analysis with electrode location in the occipital lobe (yes = 1) as the fixed effect predictor variable and either MI≥80 Hz & 0.5−1 Hz, MI≥80 Hz & 3−4 Hz, HFOSTE≥80 Hz, HFOSLL≥80 Hz, HFOHIL≥80 Hz, or HFOMNI≥80 Hz as the dependent variable. The random effect factors included intercept and patient. We considered an FDR-corrected p-value of less than 0.05 as significant, for comparisons of six iEEG measures. We reported the mixed model effect and 95% confidence interval (95% CI) to highlight the impact of topography on normative iEEG biomarker measures. All statistical analyses were performed using Matlab R2020a (MathWorks Inc., Natick, MA).\n\n### Statistical analysis to visualize the developmental slope of cortical MI and HFO at given mesh points\n\nWe presented iEEG biomarker measures at each nonepileptic electrode site on a standardized brain surface image using FreeSurfer and interpolation within 10 mm from the electrode center at the individual patient level (Sakakura et al., 2022, Ono et al., 2023). Using linear and nonlinear univariate regression models at cortical surface mesh points consisting of 20 neighboring FreeSurfer vertex finite elements (Desikan et al., 2006; Sakakura et al., 2022), we then determined the developmental slope of the iEEG biomarker, at the whole brain level. We used age, square root of age (√age), and log10 age as an independent variable, and MI≥80 Hz & 0.5−1 Hz, MI≥80 Hz & 3−4 Hz, HFOSTE≥80 Hz, HFOSLL≥80 Hz, HFOHIL≥80 Hz, or HFOMNI≥80 Hz as dependent variables. We evaluated the goodness of fit of each regression model using Akaike Information Criterion (AIC). A biomarker value was considered to increase with age if the regression slope was significantly greater than zero. We identified the mesh points where the developmental change (enhancement or diminution) of a given iEEG biomarker measure survived an FDR correction (for 18 comparisons: six iEEG measures × three types of age measures) in the resulting normative atlas. We also created video atlases, each displaying MI≥80 Hz & 0.5−1 Hz, MI≥80 Hz & 3−4 Hz, or HFOHIL≥80 Hz values predicted by a given regression model at cortical mesh points (Fig. 3; Videos S1-S3).\n\n### Statistical analysis to determine the independent effects of development on cortical MI and HFO in each lobe\n\nWe used mixed model analysis (Sonoda et al., 2021; Sakakura et al., 2022) to determine the lobe where a developmental change of a given iEEG biomarker remained significant, after controlling for the independent effects of clinical profile and epilepsy-related variables. The aim was to account for potential confounders that could affect MI and HFO measures.\n\nTo assess the developmental change of MI at each lobe, we utilized the MATLAB fitlme command (https://www.mathworks.com/help/stats/fitlme.html) to fit a mixed model specified by the following formula: 'MI ~ 1 + age + sex + SOZ + MRI + hemisphere + number of antiseizure medications + (1|patient)'. Here, the dependent variable was MI at a given analysis mesh point, and the fixed effect predictors included [1] age at surgery (e.g., √year), [2] sex (female = 1), [3] presence of SOZ in a given lobe (yes = 1), [4] presence of MRI-visible structural lesion (yes = 1), [5] sampled hemisphere (left = 1), and [6] number of oral antiseizure medications taken immediately before the initiation of iEEG recording. We considered a larger number of antiseizure medications as a surrogate of a more severe seizure-related cognitive burden since polytherapy is associated with more disabling seizures and seizure-related cognitive impairment (Kwan and Brodie, 2001; Kuroda et al., 2021). We employed this approach since no single neuropsychological assessment can quantify the severity of cognitive impairment across all age ranges. Our random effect factors included the intercept and patient. We deemed an FDR-corrected p-value of 0.05 (for 18 comparisons: six iEEG measures × three types of age measures) as the significance threshold.\n\n### Statistical analysis to determine if the spectral frequency band of slow waves nesting HFO would change with development\n\nSome might hypothesize that slow waves with a higher spectral frequency band would facilitate a higher rate of spontaneous neural communication through nested HFO. As an ancillary analysis, we, therefore, sought to determine whether the spectral frequency band of slow waves nesting HFO would change with development. To accomplish this, we measured MI≥80 Hz & s Hz, where s was 0.5-1, 1–2, 2–3, 3–4, 4–5, 5–6, 6–7, or 7–8 (Fig. 4) and calculated the regression slope of MI≥80 Hz & s Hz with respect to s Hz, in each lobe. We then assessed whether this regression slope was dependent on patient age in each lobe using the Spearman correlation. A higher regression slope in older individuals, compared to younger individuals, would suggest that HFO≥80 Hz in older individuals were preferentially coupled with slow waves of higher spectral frequency bands. We set an FDR-corrected p-value of 0.05 (for testing at four lobes) as the significance threshold.\n\n## Statistical analysis: white matter tracts between cortices showing developmental MI co-growth\n\nWe visualized white matter tracts directly connecting cortical mesh points that showed significant developmental co-growth (or co-reduction) of MI≥80 Hz & 0.5−1 Hz. To this end, we used the regression slope of MI≥80 Hz & 0.5−1 Hz as a function of √age at each cortical mesh point, as computed in a regression analysis mentioned above. We declared that the developmental enhancement (or reduction) of nested HFO-based neural communications took place between two cortical mesh points only if [1] two distinct mesh points showed significantly positive (or negative) regression slopes, and [2] these mesh points were accompanied by direct tractography streamlines on diffusion-weighted imaging (DWI) analysis (Kitazawa et al., 2023; Ono et al., 2023).\n\nWe delineated white matter DWI streamlines using open-source data from 1,065 healthy participants (http://brain.labsolver.org/diffusion-mri-templates/hcp-842-hcp-1021; Yeh et al., 2018), as previously reported (Mitsuhashi et al., 2021, 2022; Sonoda et al., 2021; Kitazawa et al., 2023; Ono et al., 2023). Our group validated the use of open-source DWI data by demonstrating that the inferred velocity of neural propagations induced by single-pulse electrical stimulation was similar whether using open-source or individual patient DWI data (Sonoda et al., 2021). We placed seeds (4-mm radius) at cortical mesh points demonstrating significant developmental enhancement (or reduction) of nested HFO-based neural communications (as rated by MI≥80 Hz & 0.5−1 Hz). Using DSI Studio (http://dsi-studio.labsolver.org/), we visualized DWI streamlines directly connecting the mesh points within Montreal Neurological Institute standard space. For fiber tracking, we utilized the following parameters: a quantitative anisotropy threshold of 0.05, a maximum turning angle of 70°, and a streamline length of 20 to 250 mm. In this investigation, we exclusively visualized DWI streamlines with at least 50% of their coordinates in one of the following white matter tracts: arcuate fasciculus, cingulum, corpus callosum, extreme capsule, frontal aslant tract, inferior fronto-occipital fasciculus, inferior longitudinal fasciculus, middle longitudinal fasciculus, superior longitudinal fasciculus, uncinate fasciculus, or vertical occipital fasciculus, as defined in DSI Studio (as previously performed in Sonoda et al., 2021). We excluded streamlines involving the brainstem, basal ganglia, thalamus, or cerebrospinal fluid space.\n\nThe resulting dynamic tractography video atlases highlighted the intensity of MI≥80 Hz & 0.5−1 Hz developmental co-growth (or co-reduction) via given tractography streamlines for every 0.1 years; thereby, the intensity was defined as (√│regression slope at a mesh point│ × √│regression slope at another mesh point│), at a given streamline connecting a pair of mesh points (Fig. 5).\n\n## Data and code availability statement\n\nThe iEEG data are available at https://openneuro.org/ (doi: 10.18112/openneuro.ds004551.v1.0.2) and https://nemar.org/. The analysis codes are available at https://github.com/kaz1126/flatten_map_and_tractography.\n\n# Results\n\n## Developmental atlas of cortical MI\n\nFigure 2A illustrates the developmental changes in cortical MI ≥80 Hz & 0.5-1 Hz at specific lobes using dot plots. The regression slope, uncorrected p-value, regression t-value, and degrees of freedom (DF) are also shown. Video S1 provides a comprehensive summary of normative development of MI ≥80 Hz & 0.5-1 Hz, estimated by univariate regression models with age, √age, or log₁₀ age as independent variables. Linear and nonlinear regression models consistently indicate significant developmental growth in MI ≥80 Hz & 0.5-1 Hz prominently in the occipital lobe during young childhood and beyond. The assessment of AIC suggests that the developmental growth in occipital MI ≥80 Hz & 0.5-1 Hz was drastic during young childhood and modest during older childhood. The mean regression slope was +0.0072 /year (95%CI: +0.0050 to +0.0093; AIC: -368.0) in the linear regression model, +0.047 /√year (95%CI: +0.034 to +0.060; AIC: -374.3) and +0.14 /log₁₀ year (95%CI: +0.10 to +0.18; AIC: -376.6) in the nonlinear models. The regression slopes of MI ≥80 Hz & 0.5-1 Hz in the parietal, temporal, and frontal lobes were much flatter, compared to the occipital lobe (Figure 2 and Video S1).\n\nAs detailed in Figure S2 and Video S2, the developmental changes of MI ≥80 Hz & 0.5-1 Hz and MI ≥80 Hz & 3-4 Hz were qualitatively similar. The developmental growth of MI ≥80 Hz & 3-4 Hz was highest in the occipital lobe. The mean regression slope was +0.019 /√year (95%CI: +0.014 to +0.023) in the occipital lobe but not significantly different from zero in the remaining lobes.\n\nFigure 3A displays snapshots of normative developmental atlases for MI ≥80 Hz & 0.5-1 Hz at the whole brain level, emphasizing the increased values in cortical regions near the calcarine sulcus.\n\n## Developmental atlas of cortical HFO rate\n\nThe regression models, applied to all 114 patients, did not demonstrate any significant developmental growth or diminution of occipital HFO ≥80 Hz as defined by any detector (uncorrected p-value > 0.05; Figure 2B; Figure S2). In contrast, the rate of extra-occipital HFO ≥80 Hz generally showed significant developmental diminution (uncorrected p-value < 0.001). Such developmental diminution of extra-occipital HFO resulted in a relatively maintained HFO occurrence rate in the occipital lobes, particularly those adjacent to the calcarine cortex, during adolescence and beyond (Figure 3B). Below, we describe the findings of HFO HIL ≥80 Hz in detail.\n\nVideo S3 provides a comprehensive summary of normative development of HFO HIL≥80 Hz rate. Occipital HFO HIL ≥80 Hz rate failed to show significant developmental change (uncorrected p-value > 0.05; Figure 2B). In contrast, extra-occipital HFO HIL ≥80 Hz rate showed significant developmental diminution (uncorrected p-value < 0.001; Figure 2B). The assessment of AIC suggested that the developmental diminution in extra-occipital HFO HIL ≥80 Hz was comparable during young and older childhood (AIC in extra-occipital lobes: 2.60 x 10⁴ in age-incorporated model; 2.59 x 10⁴ in √age model; 2.59 x 10⁴ in log₁₀ age model). The regression slope was -0.41/√year (95%CI: -0.46 to -0.36) in the frontal lobe, -0.30/√year (95%CI: -0.36 to -0.25) in the temporal lobe, -0.33/√year (95%CI: -0.40 to -0.26) in the parietal lobe, and +0.081/√year (95%CI: -0.075 to +0.24) in the occipital lobe.\n\nDue to the infrequent occurrence of events, regression models failed to fit the data of HFO ≥150 Hz and HFO ≥250 Hz rates in a meaningful manner.\n\n## MI enhancement in the occipital lobe during young childhood and after\n\nThe mixed model analysis of iEEG data of 14 children aged from 1.0 and 3.9 suggested that, as compared to the other lobes, the occipital lobe showed higher MI ≥80 Hz & 0.5-1 Hz (mixed model effect: +0.087 [95%CI: +0.078 to +0.097]; uncorrected p-value: < 0.001) and MI ≥80 Hz & 3-4 Hz (mixed model effect: +0.033 [95%CI: +0.028 to +0.038]; uncorrected p-value: < 0.001).\n\nAn ancillary mixed model analysis of iEEG data of 100 individuals aged from 4.0 and 41.5 suggested that, as compared to the other lobes, the occipital lobe likewise showed higher MI ≥80 Hz & 0.5-1 Hz (mixed model effect: +0.17 [95%CI: +0.17 to +0.18]; uncorrected p-value: < 0.001) and MI ≥80 Hz & 3-4 Hz (mixed model effect: +0.063 [95%CI: +0.061 to +0.066]; uncorrected p-value: < 0.001). These findings indicate that the nonepileptic occipital lobe exhibits higher MI in comparison to the other regions, across all age groups (Figure 3A). Moreover, the difference in MI between the occipital and extra-occipital lobe regions was found to be approximately two times greater in older individuals.\n\n## Topographical variations of HFO rate during young childhood and after\n\nThe mixed-model analysis of iEEG data from 14 children between the ages of 1.0 and 3.9 did not show a higher HFO rate in the occipital lobe compared to extra-occipital lobes, except when considering the HFO rate defined by the Hilbert method (HFO STE ≥80 Hz mixed model effect: +0.022 [95%CI: -0.039 to +0.082]; uncorrected p-value: 0.48; HFO SLL ≥80 Hz mixed model effect: +0.036 [95%CI: -0.46 to +0.53]; uncorrected p-value: 0.89; HFO HIL ≥80 Hz mixed model effect: +0.84 [95%CI: +0.57 to +1.1]; uncorrected p-value: < 0.001; HFO MNI ≥80 Hz mixed model effect: -0.044 [95%CI: -0.90 to +3.0 x 10⁻³]; uncorrected p-value: 0.067). The model suggests that the nonepileptic occipital lobe of children under four years old generates Hilbert method-defined HFO ≥80 Hz occurrences at a rate of 0.84/min more frequently than extra-occipital lobe regions.\n\nAnother mixed-model analysis of iEEG data from 100 individuals between the ages of 4.0 and 41.5 demonstrated that the occipital lobe had a higher HFO rate compared to the extra-occipital lobes, except when considering the HFO rate defined by the MNI method (HFO STE ≥80 Hz mixed model effect: +0.14 [95%CI: +0.12 to +0.16]; uncorrected p-value: < 0.001; HFO SLL ≥80 Hz mixed model effect: +0.59 [95%CI: +0.43 to +0.75]; uncorrected p-value: < 0.001; HFO HIL ≥80 Hz mixed model effect: +1.8 [95%CI: +1.7 to +1.9]; uncorrected p-value: < 0.001; HFO MNI ≥80 Hz mixed model effect: +0.043 [95%CI: -0.014 to +0.099]; uncorrected p-value: 0.14). The model suggests that the non-epileptic occipital lobe of individuals of four years old or above generates Hilbert method-defined HFO ≥80 Hz occurrences at a rate of 1.8/min more frequently than extra-occipital lobe regions (Figure 3B).\n\n## Independent effects of development on cortical MI in each lobe\n\nThe mixed model analysis, employed to all 114 patients, confirmed that an increase in √age was associated with an increase in occipital MI ≥80 Hz & 0.5-1 Hz (mixed model effect: +0.046 [95%CI: +0.019 to +0.072]; uncorrected p-value: 7.43 x 10⁻⁴; t-value: +3.39; DF: 868) and MI ≥80 Hz & 3-4 Hz (mixed model effect: +0.019 [95%CI: +0.0090 to +0.029]; uncorrected p-value: 1.22 x 10⁻⁴; t-value: +3.86; DF: 868), independent of patient and epilepsy profiles. In contrast, mixed model analysis failed to confirm that an increase in √age was associated with an increase in extra-occipital MI ≥80 Hz & 0.5-1 Hz or MI ≥80 Hz & 3-4 Hz (uncorrected p-value: >0.05).\n\n## Independent effects of development on cortical HFO rate in each lobe\n\nThe mixed model analysis confirmed that an increase in √age was independently associated with a diminution of HFO HIL≥80 Hz rate in the frontal (mixed model effect: -0.53; uncorrected p-value: 5.68 x 10⁻⁷; t-value: -4.97; DF: 2973), temporal (mixed model effect: -0.34; uncorrected p-value: 2.0 x 10⁻³; t-value: -3.09; DF: 2388), and parietal lobes (mixed model effect: -0.38; uncorrected p-value: 5.43 x 10⁻⁴; t-value: -3.46; DF: 1994). However, this phenomenon was not observed in the occipital lobe (mixed model effect: +0.069; uncorrected p-value: 0.69; t-value: +0.40; DF: 868).\n\n## Developmental changes of the spectral frequency band of slow waves nesting HFO\n\nLooking at MI ≥80 Hz & varying slow waves, we failed to find a significant developmental change of the frequency band of slow waves nesting HFO (Figure 4). On average, the regression slope of MI ≥80 Hz & s Hz as a function of slow waves (s Hz) was -0.014 /Hz in the frontal lobe, -0.013 /Hz in the parietal lobe, -0.010 /Hz in the temporal lobe, and -0.027 /Hz in the occipital lobe. In other words, MI ≥80 Hz values were generally higher when using lower frequency slow waves. The Spearman correlation failed to demonstrate a significant correlation between this regression slope and patient age in any lobe (uncorrected p-value: >0.05). Thus, the present study failed to demonstrate that the spectral frequency band of slow waves nesting HFO would change with development.\n\n## White matter tracts connecting cortices with developmental MI co-growth\n\nUnivariate regression models, incorporating √age as an independent variable, found that 159 out of the 9464 cortical mesh points (1.7%) showed significantly positive regression slopes, whereas no cortical mesh points showed significantly negative regression slopes. DWI analysis revealed that the vertical occipital fasciculi and posterior callosal fibers directly connected mesh point pairs showing significant developmental co-growth of MI ≥80 Hz & 0.5-1 Hz (Figure 5A and Video S4).\n\n## White matter tracts connecting cortices with developmental HFO co-diminution\n\nUnivariate regression models incorporating √age as an independent variable found that 902 out of the 9464 cortical mesh points (9.5%) showed significantly negative regression slopes, whereas no cortical mesh points showed significantly positive regression slopes. DWI analysis revealed that the arcuate fasciculus, corpus callosum, extreme capsule, frontal aslant tract, inferior fronto-occipital fasciculus, inferior longitudinal fasciculus, middle longitudinal fasciculus, and superior longitudinal fasciculus directly connected mesh point pairs showing significant developmental co-diminution of HFO HIL≥80 Hz rate (Figure 5B and Video S5).\n\n# Discussion\n\n## Clinical significance of enhanced MI in the occipital lobe in epilepsy presurgical evaluation\n\nFor the first time, the current study created a developmental atlas of MI at the whole brain level, including the medial and inferior surfaces of the cerebral cortex. It demonstrated physiologically enhanced MI in the nonepileptic occipital lobe of children younger than 4 years and in the older patient group. The occipital lobe showed higher MI ≥ 80 Hz & 3−4 Hz than the other lobes by 0.033 on average in children younger than 4 years and by 0.063 on average in older patients. Although MI ≥ 80 Hz & 3−4 Hz is an excellent surrogate marker of interictal spike-and-wave discharges (Motoi et al., 2018; Kural et al., 2020), the occurrence of physiological HFO nested in slow-wave background activity (Steriade et al., 1993; Contreras et al., 1996; Sanchez-Vives and McCormick, 2000, Nagasawa et al., 2012; Nonoda et al., 2016) inflates MI ≥ 80 Hz & 3−4 Hz in the nonepileptic occipital lobe. Therefore, iEEG investigators should cautiously interpret the significance of high-value, occipital MI in presurgical evaluation for young and older patients with drug-resistant focal epilepsy. Nonepileptic occipital lobe sites, especially those proximal to the calcarine sulcus, are expected to show MI values higher than nonepileptic extra-occipital lobe sites (Video S1 and Fig. 3 A). With awareness of such topographic variations of MI, iEEG investigators can reduce the risk of incorrect localization of the epileptogenic zone.\n\nInvestigators previously reported the utility of normative atlases of MI, HFO, and other spectral frequency bands, in the presurgical evaluation of patients with the mean age ranging between adolescence and adulthood (Frauscher et al., 2018; Guragain et al., 2018; Kuroda et al., 2021; Bernabei et al., 2022; Taylor et al., 2022; Zweiphenning et al., 2022 b). A prospective study is warranted to investigate whether a more inclusive resection of cortical sites, whose MI values deviate from the age-specific normal range, would predict better postoperative seizure control in young children.\n\n## Clinical significance of HFO atlases in epilepsy presurgical evaluation\n\nFor the first time, the current study investigated the developmental changes of HFO occurrence rate defined by four open-source detectors (Fig. 2; Figure S2). Commonly across detectors, the HFO rate diminished in the frontal, parietal, and temporal lobes with development. Thus, clinicians need to be aware that young children may show nonepileptic HFO in the extra-occipital lobe regions more frequently than adults. As best demonstrated in Video S3, HFO HIL ≥80 Hz rate was physiologically enhanced in the occipital regions proximal to the calcarine cortex, but such occipital HFO enhancement was only evident during adolescence and adulthood and not during infancy or toddlerhood.\n\nHFO MNI ≥80 Hz rate was very low in the occipital lobes throughout all ages; this MNI method-specific observation can be attributed to its detector being designed to be agnostic to persistent forms of high-frequency activity (Zelmann et al., 2010), as often seen in the nonepileptic occipital lobe (Nagasawa et al., 2012).\n\n## Mechanistic significance of developmental changes of MI and HFO\n\nWhat is responsible for the developmental enhancement of MI in the occipital lobe? The current study found that MI ≥ 80 Hz & 0.5−1 Hz increases rapidly during early childhood and modestly thereafter. However, the occipital HFO rate did not increase significantly with development, suggesting that rate changes may not sufficiently account for the developmental enhancement of MI (Fig. 2 B). Furthermore, an assessment of the spectral frequency bands of slow-waves nesting HFO (Fig. 4) did not provide evidence that such nesting slow rhythms become faster with development. In contrast, our white matter connectivity assessment revealed that occipital regions exhibiting a developmental enhancement of MI were accompanied by monosynaptic white matter streamlines, including the vertical occipital fasciculi and posterior callosal fibers (Fig. 5 A). These white matter structures are essential for object recognition (Baynes et al., 1998; Schulte et al., 2010; Yeatman et al., 2014; Herbet et al., 2018); thus, one possible explanation for the developmental enhancement of occipital MI is that the cerebral cortex learns to generate HFO at a preferred phase of background rhythms in an experience-dependent manner, optimizing visual memory consolidation during slow-wave sleep (Ji and Wilson, 2007; Mehta, 2007; Sasaki et al., 2010; Buzsáki and da Silva, 2012; Nagasawa et al., 2012). This notion is supported by the observation that monocular sight deprivation during a critical period altered delta-gamma phase-amplitude coupling in the mouse visual cortex (Malik et al., 2022).\n\n## Innovation\n\nThe methodological innovations in the current study include the generation of developmental atlases based on iEEG signals from 114 patients, including infants and toddlers. We previously validated our group-level analysis of iEEG across generations from infancy to adulthood (Sakakura et al., 2022). A pivotal procedure to ensure the spatial accuracy of electrode-brain surface coregistration was a manual delineation of the pial surface in the temporal lobe regions that are frequently unmyelinated in young children (Sakakura et al., 2022).\n\nVisualization of the direct white matter streamlines connecting cortical regions with a developmental enhancement of MI is an innovative application of dynamic tractography technology (Sonoda et al., 2021; Kitazawa et al., 2023; Ono et al., 2023). We interpret the visualized streamlines, including vertical occipital fasciculi and posterior callosal fibers, to reflect the ongoing development of large-scale neural communications based on slow wave-nested HFO before reaching the adult level.\n\n## Methodological considerations\n\nInevitable limitations in the present study include limited spatial sampling, though 8,251 nonepileptic electrode sites were available for analysis. We are only able to place electrodes that are clinically indicated. Neither Heschl nor insular gyri were analyzed in the present study using subdural electrodes. Thus, our study was not designed to assess the developmental enhancement of MI or HFO in much of the primary auditory cortex. We did not sample iEEG signals from the thalamus either because there was no clinical indication. Since stereotactic-EEG depth electrodes are used to assess the thalamic nuclei to determine the optimal target for deep brain stimulation and responsive neurostimulation therapy, further studies are expected to determine the developmental changes of MI and HFO in such deep brain structures in the future.\n\nAnother limitation included cross-sectional measurement due to the invasive nature of iEEG recording. Chronic iEEG recording is available through eight intracranial electrode contacts in patients undergoing responsive neurostimulation. Yet, longitudinal assessment of nonepileptic iEEG signals using these contacts may not be feasible because these electrodes are implanted in the area proximal to the epileptogenic zone.\n\nOur ancillary analysis on the rates of HFO ≥ 150 Hz and HFO ≥ 250 Hz revealed that the infrequent occurrence of these events made it impossible for regression models to meaningfully fit the data. To detect sufficient numbers of HFO ≥ 150 Hz and HFO ≥ 250 Hz events for analysis of developmental changes, interictal slow-wave sleep epochs much longer than 20 minutes would be necessary. However, the duration of iEEG recording is determined solely by clinical needs, making it unrealistic to expect that all study participants would have prolonged iEEG epochs that meet the eligibility criteria employed in this study. Although the spatial distribution of the rates of HFO ≥ 80 Hz, HFO ≥ 150 Hz, and HFO ≥ 250 Hz are generally similar to each other, some studies suggest that HFO ≥ 250 Hz may be more specific than HFO ≥ 80 Hz in localizing the epileptogenic zone; however, others imply that HFO ≥ 250 Hz may not be as practical as HFO ≥ 80 Hz due to its rarity and its presence in the nonepileptic eloquent cortex (Gloss et al., 2014; Höller et al., 2015; Frauscher et al., 2017; Roehri et al., 2018; Kuroda et al., 2021; Zweiphenning et al., 2022 a).\n\nOne drawback of using iEEG is that we are unable to include healthy controls, because it is unethical to implant subdural electrodes without clinical indication. Thus, we excluded electrode sites affected by either SOZ, interictal spike zone, and MRI-visible lesions from the analysis. 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Neuroimage. 2009;46(3):708–716.\n\n# Supplementary Files\n\n- [HFOsakakuradevelopmentsupplementarydocumentea7ks5.docx](https://assets-eu.researchsquare.com/files/rs-2799931/v1/dd697e8fe978096340b9f1f3.docx)\n- [nreditorialpolicychecklistks1.pdf](https://assets-eu.researchsquare.com/files/rs-2799931/v1/ac68728689e21d5e133063c8.pdf)\n- [nrreportingsummaryks2ea1.pdf](https://assets-eu.researchsquare.com/files/rs-2799931/v1/4e998922f8723d862b1b3d6f.pdf)\n- [NCOMMS2315354rs.pdf](https://assets-eu.researchsquare.com/files/rs-2799931/v1/4bb0c80e0d830136fa423d75.pdf) \n Reporting Summary\n- [VideoS1MI800.5ks2.mp4](https://assets-eu.researchsquare.com/files/rs-2799931/v1/61cdc36570b7c71308e9f23d.mp4) \n Video S1\n- [VideoS2MI803ks1.mp4](https://assets-eu.researchsquare.com/files/rs-2799931/v1/f8c6658e05433ccc8600c928.mp4) \n Video S2\n- [VideoS3HIL80ks2.mp4](https://assets-eu.researchsquare.com/files/rs-2799931/v1/8de032ac2b6b2c536b9e0546.mp4) \n Video S3\n- [VideoS4MI800.5tractks1.mp4](https://assets-eu.researchsquare.com/files/rs-2799931/v1/6519361a5ca10e1a370b3c9e.mp4) \n Video S4\n- [VideoS5HIL80tractks3.mp4](https://assets-eu.researchsquare.com/files/rs-2799931/v1/ffb25194e2a1a637ea20a836.mp4) \n Video S5\n- [nrreportingsummaryea2.pdf](https://assets-eu.researchsquare.com/files/rs-2799931/v1/9c6222be14f542eeb082f121.pdf) \n Reporting Summary"} {"paper_id": "prb25", "title": "Spontaneous traveling waves naturally emerge from horizontal fiber time delays and travel through locally asynchronous-irregular states", "text": "Spontaneous traveling waves naturally emerge from horizontal fiber time delays and travel through locally asynchronous-irregular states\n\nZachary Davis (zdavis@salk.edu)\nSalk Institute for Biological Studies https://orcid.org/0000-0003-4440-9011\nGabriel Benigno\nWestern University\nCharlee Fletterman\nSalk Institute for Biological Studies\nTheo Desbordes\nSalk Institute for Biological Studies\nTerrence Sejnowski\nSalk Institute for Biological Studies https://orcid.org/0000-0002-0622-7391\nJohn Reynolds\nThe Salk Institute for Biological Studies\nLyle Muller\nWestern University\n\nArticle\n\nKeywords: sensory neuroscience, spontaneous fluctuations, cortical fibers\n\nPosted Date: December 2nd, 2020\n\nDOI: https://doi.org/10.21203/rs.3.rs-113978/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nVersion of Record: A version of this preprint was published at Nature Communications on October 18th, 2021. See the published version at https://doi.org/10.1038/s41467-021-26175-1.\nSpontaneous traveling waves naturally emerge from horizontal fiber time delays and travel through locally asynchronous-irregular states\n\nAuthors: Zachary W. Davis1*, Gabriel B. Benigno2,3,*; Charlee Fletterman1†; Theo Desbordes1, Terrence J. Sejnowski1,†, John Reynolds1,†, Lyle Muller2,3,†\n\nAffiliations:\n1The Salk Institute for Biological Studies, La Jolla, CA, USA.\n2Department of Applied Mathematics, Western University, London, ON, Canada.\n3Brain and Mind Institute, Western University, London, ON, Canada.\n* Authors contributed equally, † Co-senior authors\n* Corresponding authors J.H.R. and L.M., emails: reynolds@salk.edu and lmuller2@uwo.ca\n\nAbstract\n\nSensory neuroscience has focused a great deal of its attention on characterizing the mean firing rate that is evoked by a stimulus, and while it has long been recognized that the firing rates of individual neurons fluctuate around the mean, these fluctuations are often treated as a form of internally generated noise1. There is, however, evidence that these “ongoing” fluctuations of activity in sensory cortex during normal, waking function shape neuronal excitability and responses to external input2,3. We have recently found that spontaneous fluctuations are organized into waves traveling at speeds consistent with the speed of action potentials traversing unmyelinated horizontal cortical fibers (0.1-0.6 m/s)4 across the cortical surface5. These waves systematically modulate excitability across the retinotopic map, strongly affecting perceptual sensitivity as measured in a visual detection task. The underlying mechanism for these waves, however, is unknown. Further, it is unclear whether waves are consistent with the low rate, highly irregular, and weakly correlated “asynchronous-irregular” dynamics observed in computational models6 and cortical recordings in vivo7. Here, we study a large-scale computational model of a cortical sheet, with connections ranging up to biological scales. Using an efficient custom simulation framework, we study networks with topographically-organized connectivity and distance-dependent axonal conduction delays from several thousand up to one million neurons. We find that spontaneous traveling waves are a general property of these networks and are consistent with the asynchronous-irregular regime. These waves are well matched to spontaneous waves recorded in the neocortex of awake monkeys. Further, individual neurons\nsparsely participate in waves, yielding a sparse-wave regime that offers a unique operating mode, where traveling waves coexist with locally asynchronous-irregular dynamics, without inducing deleterious neuronal correlations8.\n\nIntroduction\n\nVisual cortical neurons exhibit variable fluctuations in their spontaneous activity and stimulus-evoked responses. Rather than being due to noise intrinsic to the neural spiking mechanism9, which is highly reliable10, variability is thought to emerge from ongoing synaptic activity in the dense recurrent connectivity of cortical networks1,2. When observed from a single point in the cortex, spontaneous fluctuations resemble a broadband temporal noise process1,11. Multisite recordings have revealed that these temporal fluctuations can be part of waves traveling across a cortical area12–16. Spontaneous traveling waves had largely been observed in slow-wave fluctuations associated with anesthesia, sleep, or low arousal. While traveling waves had been theorized to have an impact on cortical computation, it was difficult to identify their role since active cortical states exhibit fluctuations that are more complex, dominated by higher-frequency and lower-amplitude activity17, making these waves harder to detect. Further, driving input is believed to quench variability in ongoing dynamics,18 calling into question the potential impact of traveling waves on evoked activity19.\n\nRecent work has shown that spontaneous traveling waves are present in the awake state, that they influence the magnitude of sensory-evoked activity, and that—depending on their retinotopic alignment with sensory input—they can improve perceptual sensitivity5. However, the mechanisms that generate them, and whether they are consistent with the asynchronous-irregular spiking dynamics characteristic of awake cortex20, is unknown. Based on their speed of propagation, we hypothesize these waves result from action potentials propagating along unmyelinated horizontal fibers. To test this hypothesis, we studied a spiking network model across a range of biologically realistic neuronal densities, distance-dependent connection probabilities, excitatory/inhibitory balances, and synaptic conductance states. Importantly, this model incorporated axonal time delays from conduction along unmyelinated horizontal fibers, which shaped ongoing activity patterns into traveling waves consistent with those observed in vivo. Spontaneous traveling waves were apparent in this network model and occurred consistently across a wide parameter range that produced asynchronous-irregular dynamics.\nOne might wonder whether the occurrence of these traveling waves induces correlated variability, which has been found to impair perception\\(^8\\). Results from the spiking network model show this need not be the case. In both the computational model and multielectrode recordings in the marmoset visual system, we found neuronal participation in these waves was sparse, meaning that the probability of any individual neuron contributing to an individual traveling wave was low. We thus refer to the model as the sparse-wave model and this regime as the sparse-wave regime. Therefore, spontaneous waves can emerge at mesoscopic scales in subthreshold synaptic fluctuations, carried by sparse spiking activity along horizontal fibers, without inducing changes in pairwise correlations in the activity of individual neurons. Traveling waves can thus co-exist with a locally asynchronous-irregular state, conferring their benefits while maintaining the computational advantages of this dynamical regime\\(^{7,21}\\).\n\nResults\n\nSpontaneous synaptic fluctuations are comparable to those during stimulus-evoked responses\n\nPrevious work has shown that moment-by-moment fluctuations in synaptic input in the cortex can be on the same order of magnitude as during the sustained period of stimulus-evoked responses\\(^{12,22-24}\\). Fluctuating synaptic inputs can have a significant impact on neural excitability\\(^{25}\\), gain modulation\\(^{26}\\), and readout of sensory information\\(^{13}\\). To understand the impact of the spontaneous network state on evoked responses in the awake visual cortex, we recorded spontaneous and stimulus-evoked activity from chronically implanted multi-electrode Utah arrays (Blackrock Microsystems) in area MT of two common marmosets (\\emph{Callithrix jacchus}; data previously reported in Davis et al., 2020). Spontaneous multiunit activity recorded from a single electrode while a marmoset fixated a fixation point was characterized by a low, irregular firing rate. The appearance of a highly salient stimulus (10% Michelson contrast drifting Gabor) within the multiunit receptive field evoked a robust response (Figure 1a). When measured over many repeated presentations of the stimulus, the mean multiunit firing rate rose from \\(13 \\pm 1.6\\) sp/sec during fixation, to \\(97 \\pm 5.7\\) sp/sec in response to the stimulus (N = 40 trials over 3 recording sessions). These evoked spiking responses were variable from trial to trial (mean fano factor = \\(1.01 \\pm 0.01\\) SEM, 40 to 240 ms after stimulus onset), consistent with previous observations\\(^{18,27,28}\\).\n\nThis variability is partly the result of ongoing spontaneous fluctuations in synaptic activity in the local population at the time of the evoked spiking response\\(^{12,13}\\). These fluctuating synaptic inputs, in turn, contribute to the local field potential (LFP)\\(^{29,30}\\). When averaged across high-contrast trials,\nthe LFP had a robust negative deflection aligned to the stimulus-evoked spiking response, while the pre-stimulus period was flat (black line, Figure 1a). However, at the single-trial level, the stimulus-evoked LFP response was similar in magnitude to the spontaneous fluctuations occurring during fixation (right panel, Figure 1a). The relative power between the LFP just prior to the stimulus (-200 to 0 ms) and following stimulus onset (0 to +200 ms) across single trials had a small but significant difference from 0 dB, which represents parity between spontaneous and stimulus-evoked fluctuations (median 1.98 dB, p < 0.001 Wilcoxon signed-rank test).\n\nWhile strong, high-contrast visual stimulation evoked slightly stronger LFP fluctuations than intrinsic network fluctuations, the distinction disappears in the context of weak visual inputs (Figure 1b). When the marmoset was presented a faint stimulus that was detected approximately 50% of the time (<2% Michelson contrast), the evoked spiking response was significantly weaker and more variable (mean = 68 ± 4.4 sp/sec, p < 0.001; fano factor = 1.55 ± 0.09, p < 0.01, Wilcoxon rank-sum test). This corresponded to a weaker average LFP response, and the trial-by-trial relative power between spontaneous and evoked fluctuations was not significantly different from 0 dB (median = 0.18 dB, p= 0.55 Wilcoxon ranked-sum test).\n\nGiven the relative magnitude of spontaneous fluctuations to responses evoked by weak sensory inputs, we hypothesized that much of the variability in neuronal spiking responses could be explained by the state of the local network. We recently reported that spontaneous LFP fluctuations in awake cortex are organized into waves that travel across an entire cortical area (Figure 1c). They modulate spontaneous spiking probability (Figure 1d), and they directly impact the magnitude of stimulus-evoked responses depending on their alignment with neuronal receptive fields (Figure 1e). We found that, rather than acting as a source of noise that impairs perception, spontaneous waves can—depending on their spatiotemporal alignment with a visual stimulus—improve the monkeys’ ability to detect the stimulus. We thus sought to understand what mechanisms might generate traveling waves in cortex and test whether they represent an operating regime either consistent with or distinct from the irregular, asynchronous activity patterns classically observed *in silico*\\( ^{6,31} \\) and *in vivo*\\( ^{7,32} \\).\n\n*Spontaneous traveling waves can emerge in network models without altering individual neuron spiking statistics*\nTo address this question, we studied large-scale spiking network models composed of leaky integrate-and-fire neurons with balanced excitation and inhibition and conductance-based synapses. When neuronal interactions are modeled as conductances, taking into account the time-dependent driving forces and channel activations at the synapse, spiking network models can enter into states of self-sustained activity\\(^{33,34}\\). Asynchronous-irregular activity\\(^6\\) in these self-sustained states, generated without external drive, results naturally from the recurrently generated fluctuations intrinsic to the dynamics of the system\\(^{33,34}\\). These dynamics are characterized by low, variable firing rates, weak pairwise correlations, and coefficients of variation (C.V.) near unity. These self-sustained states provide an opportunity to study spiking network dynamics that are structured by the recurrent activity of the network itself, rather than dominated by random external Poisson synaptic input\\(^{21}\\), and are well suited to model the spontaneous background activity observed in cortex during active perception.\n\nWe first studied a two-dimensional conductance-based spiking network model with over 1,000,000 neurons distributed over a 6x6 mm area consisting of 80 percent excitatory and 20 percent inhibitory neurons, randomly connected with 3,000 synapses per cell, yielding a sparsely connected network. We eliminated the outer millimeter from analysis, yielding a 4x4 mm area with 450,000 neurons. These values were selected to approximate the density and connectivity of neurons in cortical layer 2/3 of area MT in the common marmoset\\(^{35,36}\\). This randomly-connected network generated self-sustained activity with spontaneous spiking fluctuations consistent with the asynchronous-irregular regime\\(^{6,37}\\) and lacked any spatiotemporal structure (Fig. 2b). A simulated LFP was calculated from summed excitatory and inhibitory synaptic activity over 10 x 10 adjacent, non-overlapping pools of neurons (corresponding to 67.8 x 67.8 \\( \\mu \\)M)\\(^{38}\\) and was used to estimate the local excitability state at each point in the network for comparison to the electrophysiological recordings. The LFP was homogeneous across the network, as would be expected from pools of neurons receiving synaptic input from random positions in the network (Fig. 2c).\n\nTo test whether topographic connections with transmission delays were sufficient to generate spontaneous traveling waves in the network, as a refinement to the model described in Figure 2a, two key elements were introduced: 1) connection probability decayed as a Gaussian with distance between neurons (\\( \\sigma = 400 \\) \\( \\mu \\)M)\\(^{39,40}\\) to mimic the topographic connectivity in cortex and 2) action potentials activated synaptic currents after a time delay determined by the distance of the connection to simulate the conduction velocity of horizontal fibers in cortex (\\( v_c = 0.2 \\) m/s,\\(^4\\)\nFig. 2d). This network also produced self-sustained, spontaneous fluctuations, but spiking activity was sparsely organized into bands that moved across the network as waves (rasters, Fig. 2e). LFP fluctuations were heterogeneous across the network and exhibited organized spatial structure with localized regions coordinated in amplitude (Fig. 2f).\n\nTo test whether the presence of these organized topographic fluctuations altered the asynchronous-irregular dynamics of individual neurons in the network, we compared the firing rates and C.V. across a randomly selected population of excitatory neurons (N = 5000). There was no difference in the distribution of firing rates across the networks (p = 0.68, Kolmogorov-Smirnov test; Fig. 2g) or in the distribution of C.V. (p = 0.79, Kolmogorov-Smirnov test; Fig. 2h). Therefore, individual neurons maintained their asynchronous and irregular firing states while the topographically-connected network produced spontaneous traveling waves.\n\nWhile one might expect the organized bands of spiking activity would result in increased correlations across neurons, we found no evidence that this was the case. The introduction of topographic connections did not affect pairwise correlations, as the degree of spike-spike coherence between the randomly- and topographically-connected networks was indistinguishable (N = 1000 random pairs; CI test, α = 0.05; Fig. 2i). Spatiotemporal structure can exist in these networks without disrupting C.V. or pairwise coherence because spikes are sparsely organized into waves, with only a small fraction of neurons spiking in any given wave. We therefore refer to this as the “sparse-wave” network regime. If it were the case that neurons strongly participated in these fluctuations, then they would show a degree of coherence in the range of frequencies dominated by those fluctuations. To demonstrate this, we simulated a smaller network with fewer neurons and denser connections which generated spontaneous fluctuations that strongly regulated spiking activity. This “dense-wave” network did exhibit strong spike-spike coherence in the frequency band dominated by fluctuations in the LFP (Fig. S1, model parameters table S1). Therefore, unlike in the dense-wave network, traveling waves in the sparse-wave regime do not necessarily induce pairwise correlation across the network.\n\nAs hypothesized, the addition of topographic connections and conduction delays was sufficient to produce clear spatiotemporal organization in the network activity (Fig. 3a). To classify these activity patterns as traveling waves and quantify their properties relative to cortical recordings from marmoset cortex, we applied the same analysis technique developed for the experimental recordings (Generalized Phase, GP⁵) to the simulated LFP in each 10 x 10 neuronal pool. We\nthen adapted a technique previously developed for detecting traveling waves in noisy multielectrode recordings\\(^{41,42}\\). We estimated the gradient of phase at each moment in time and calculated putative wavelengths and propagation speeds (Fig. 3b and d). We then identified places and times in the network where the organization of activity into traveling waves was significant. Significance was determined by comparing the observed wavelengths to the wavelength distribution after a spatial shuffle of electrode positions, with the 99th percentile of the shuffle distribution taken as the threshold criterion (Fig. 3c-d). This approach provides a sensitive and robust means to detect traveling waves from moment to moment\\(^{41,42}\\). We found significant wave activity in the topographically-connected network approximately 50 percent of the time, whereas the presence of significantly structured wave organization was absent from networks with random connections and no delays (Fig. 3e) as the distribution of putative wavelengths was similar to the shuffled distribution (Fig. 3f).\n\n*Spontaneous waves occur throughout the asynchronous-irregular regime*\n\nIn the example network, topographic connections were sufficient to induce large-scale waves of activity without disrupting the fine scale asynchronous-irregular dynamics of individual neurons. Does the presence of traveling waves generalize across all networks with asynchronous-irregular activity, topographic connections, and axonal conduction delays\\(^{34,37}\\)? We scanned across 2,500 combinations of different excitatory and inhibitory (E/I) conductances in the topographically-connected model and found 654 combinations that produced self-sustained spiking activity. We then identified networks with asynchronous-irregular spiking dynamics, defined as networks with mean excitatory firing rates between 1 and 25 sp/sec, mean C.V. between 0.7 and 1.4, and mean pairwise correlations between -0.1 and 0.1\\(^{37}\\). Approximately 98 percent (646 out of 654) of the self-sustained networks were classified as asynchronous-irregular. We then measured the percentage of time each network’s activity was significantly organized into traveling waves. Waves were present across the entire range of asynchronous-irregular networks (Fig. 4a). The strength of wave activity was negatively correlated with the magnitude of E/I conductance (Pearsons’s r = -0.35 ± 0.07, 95% CI; Fig. 4a) indicating weaker synapses led to stronger wave activity. The average wavelength was also negatively correlated with synaptic strength (Pearsons’s r = -0.41 ± 0.07; Fig. 4b), with weaker excitatory conductances particularly leading to longer wavelengths (Pearson’s r = -0.61 ± 0.05 for \\( g_e \\) vs. r = -0.21 ± 0.07 for \\( g_i \\)). These results demonstrate that spontaneous traveling waves are a general property of topographic connectivity and are entirely consistent with locally asynchronous-irregular states.\nHow important is network scale in generating traveling waves? To answer this question, we simulated networks ranging from 0.5 mm to 4 mm, holding neuronal and connection density constant. For small networks (~0.5 mm), a very limited range of the E/I space produced self-sustained and asynchronous network dynamics. As network size grew, the asynchronous-irregular parameter space grew as well, extending to include smaller and smaller combinations of E/I synaptic strength\\(^{20}\\) (Fig. 4c). It was thus necessary to simulate spiking network models at sufficient spatial scales (> 1 mm) to generate asynchronous-irregular activity in networks with conductances resembling those estimated *in vivo*\\(^{20}\\). At small network scales, wavelength distributions during asynchronous-irregular dynamics were not distinct from the spatial shuffle, and the parameters that favored longer wavelengths did not produce asynchronous-irregular activity. Only at larger network scales did wave activity become strongly apparent (Fig. 4d).\n\n*Network connectivity determines wave properties*\n\nWhat effect did our chosen parameters for connection distance and conduction velocity have on wave properties? We hypothesized the spatial extent of connections and the conduction speed of spikes directly control the wavelength and propagation speed, respectively, of traveling waves in the model. To test these predictions we simulated networks with various values of standard deviation (\\( \\sigma_s \\)) for the Gaussian connection probability distribution. Consistent with our hypotheses, the distribution of wavelengths increased with larger connection distances (Fig. 5a) and increasing the conduction velocity led to increased average wave speeds (Fig. 5b). Thus, the macroscopic features of spontaneous traveling waves were directly related to specific network structures in the model.\n\nAre these waves only possible with perfectly Gaussian connection profiles and uniform conduction velocity, or can they tolerate a broad range of values similar to those observed *in vivo*? To test this, we simulated the example model in Figure 2, with 10 percent of the connections randomly rewired with uniform probability across the network, generating long range connections\\(^{43,44}\\). The conduction velocity along each connection was drawn from the range of conduction speeds observed for unmyelinated horizontal fibers in cortex (0.1 to 0.6 m/s\\(^{4,45,46}\\)). Spontaneous traveling waves persisted under these network conditions (Fig. 5c, d), indicating the presence of waves was not limited to a fixed or limited set of homogeneous network properties, but instead also occurred in networks with large heterogeneity, as in cortex.\nNetwork simulations are consistent with traveling waves in vivo\n\nHow well do the dynamics observed in our simulations match the dynamics observed in electrophysiological recordings of the cortex? To test this we compared the model results to the data recorded from marmoset MT while monkeys fixated a spot at the center of an otherwise grey computer screen. We measured the mean firing rates (Fig. 6a) and C.V. (Fig. 6b) across the population of single- and multi-unit activity over multiple recording sessions. The distributions of firing rates and C.V. were qualitatively similar between the recorded data and the sparse-wave model, suggesting the spontaneous dynamics in the cortical recordings are also consistent with the asynchronous-irregular regime.\n\nWe next measured the distribution of estimated wavelengths in the data and compared this to the wavelength distribution in the model. LFP data in the cortex is not independent across electrodes (as it is in our simulation), but rather pools signals from a cortical volume of approximately 250 μM in radius around the electrode tip\\(^{29,30}\\) and has correlations that fall off with distance\\(^{17}\\). To emulate these properties of cortical LFP recordings, we applied a smoothing kernel that expanded the area of integration from each simulated LFP point and reduced the independence of the signal. After smoothing our simulated LFP and quantifying wave properties, the distribution of simulated wavelengths closely approximated the distribution observed in cortex (dotted gray and red lines, Fig. 6c). Similarly, the distribution of observed speeds in both the network simulation and the data covered the range of conduction velocities in the horizontal fibers, peaking at approximately 0.2 m/s (Fig. 6d). Thus, across four different measures (spike-rate, spike-variability, wave-size, wave-velocity), the distributions characterizing activity in the network model were in close alignment with experimental recordings.\n\nNeurons sparsely participate in waves due to weak coupling to synaptic fluctuations\n\nWhat is the conductance state of spontaneous fluctuations in the sparse-wave network simulation? Membrane potential fluctuations were consistent with high conductance states, with a Gaussian distribution whose mean was close to the spiking threshold (black line, Fig. 7a). This contrasted with the skewed distribution of membrane potentials in the dense wave network, which was consistent with a low conductance state transitioning between quiescent-hyperpolarized and bursting-depolarized membrane potentials (purple line, Fig. 7a). In the\nsparse-wave network model, stochastic fluctuations in the membrane potential produced sparse and irregular spiking activity. These fluctuations were driven by shifts in excitatory-inhibitory balance across the local population which, due to the topographic network connections, were shared by adjacent populations and carried by spikes across horizontal connections. These summed currents in our estimate of the LFP exhibited a counterphase relationship with the relative E/I balance: the inhibition-dominated E/I regime produced positive LFP potentials, and the excitation-dominated E/I regime produced negative LFP potentials (Fig. 7b, c).\n\nTo demonstrate that simulated neurons are sparsely modulated by traveling waves, we measured the LFP phase at which each spike occurred (10 bins from -π to π; z-scored to normalize across variable firing rates in each network; Fig. 7d) for E/I conductances that yielded asynchronous-irregular dynamics. The degree of spike-phase modulation was significant across the entire parameter space, with spikes more likely during phases closer to ±π. The magnitude of this modulation was inversely correlated with the magnitude of E/I conductances (Pearson’s r = -0.44 ± 0.09, 95% CI; N = 646 simulations), with the largest modulations in the range of the smallest conductance values that supported asynchronous-irregular activity in our simulations (where traveling waves were most frequent and also had the longest wavelengths; Fig. 4a and 4b, respectively). We chose a point among these small conductance values (1 nS g_e, 10 nS g_i), to compare the degree of coupling between the model and the cortical recordings. There was no difference between the spike-phase modulation observed in the sparse-wave network model and the recorded data (N = 22 matched resamplings; model circular-resultant = 0.15 ± 0.001 S.E.M.; data circular-resultant = 0.16 ± 0.005; p = 0.28, Wilcoxon signed-rank test), although the preferred phase-angle differed slightly between the data and model (data-preferred phase = 3.05 rad, model-preferred phase = -1.96 rad).\n\nWhile there was a similar degree of spike-phase modulation between the cortical data and the sparse-wave model, the modulation was significantly stronger in the dense-wave model (N = 10 resamples; circular-resultant = 0.43 ± 0.006, p < 0.00001, Wilcoxon rank-sum test; Fig. 7g). The phase distribution follows this pattern as well, with both the cortical data and sparse-wave model spiking more near ±π phases, whereas the dense-wave model spiking is minimal at these phases. Additionally, the randomly-connected network showed the weakest spike-phase relationship (N = 22 resamples; circular-resultant = 0.07 ± 0.001; p < 0.0001 Wilcoxon signed-rank test; Fig. S2), as expected from a network where the neurons in the LFP pool draw from inputs distributed throughout the entire network. These results demonstrate that—in the\nsimulated large-scale spiking networks—waves exist primarily in subthreshold synaptic fluctuations that are carried through sparse, phase-modulated spiking activity traveling along topographically distributed horizontal fibers. The presence of a similar spike-phase relationship *in vivo*, particularly for model conductance states which corresponded to experimental estimates of neuronal conductance states\\(^{20}\\), demonstrates that the sparse-wave regime in the model is consistent with the properties of waves observed in the experimental recordings.\n\n*Spontaneous traveling waves modulate responses to inputs*\n\nFinally, we hypothesized the state of network fluctuations in the sparse-wave network model would modulate the magnitude of responses evoked by feed-forward inputs. To test this, we stimulated one 10x10 neuron pool in the sparse-wave network with a 50 Hz Poisson spike train on 100 afferent synapses to each neuron to mimic feed-forward stimulus input to the network. We stimulated for 10 ms, aligned either to the depolarized or hyperpolarized state of network fluctuations defined, respectively, by the most and least probable phases for spikes to occur according to the network’s spontaneous spike-phase distribution. When spiking inputs were aligned to the depolarized state, the evoked spiking responses were boosted (blue lines, Fig. 8a) relative to weaker responses when inputs were aligned to the hyperpolarized state (red lines, Fig. 8a). These effects were consistent with wave-modulated visual responses to motion stimuli observed in area MT *in vivo* (cf. Fig. 1e). In contrast, stimulation in the depolarized state was wholly suppressed in the smaller, dense-wave network and the hyperpolarized state yielded higher responses (red and blue lines, Fig. 8b).\n\nTo quantify the effect of the traveling waves on evoked responses in each network, we then calculated the gain modulation, which is the ratio between the maximum stimulus-evoked response and the spontaneous spiking rate when no stimulus was applied (Fig. 8c). Across repeated input stimulations, input gain was much stronger for the depolarized state relative to the hyperpolarized state in the sparse-wave network (N = 20 stimulations; depolarized state = 4.25 ± 0.11; hyperpolarized state = 1.74 ± 0.08). In contrast, in the dense-wave network the strong spontaneous fluctuations shunted the incoming spikes, resulting in larger gain for the hyperpolarized state relative to the depolarized state (depolarized state = 1.11 ± 0.01; hyperpolarized state = 1.74 ± 0.07). The highest gain in the dense-wave model was significantly weaker than the depolarized gain in the sparse-wave network (p < 1x10\\(^{-7}\\), Wilcoxon ranked-sum test). The increase in gain that occurs in the sparse-wave network mirrors our observations of\nwave-dependent sensitivity in awake monkeys performing a threshold detection task\\(^5\\). Thus the sparse-wave model offers a mechanistic account for observed phase-dependent modulations of weak sensory responses by traveling waves measured *in vivo* that a network characterized by dense-wave dynamics fails to replicate.\n\n**Discussion**\n\nThe present work builds on and seeks to explain our recent finding that spontaneous fluctuations in cortical activity modulate the moment-to-moment processing of sensory information in a manner that affects perceptual sensitivity. These fluctuations are neither synchronous across the cortical surface nor independent noise processes. Rather, they are structured as traveling waves. The model presented here shows that distance-dependent conduction delays in topographic, conductance-based spiking network models are sufficient to account for our results *in vivo*. Waves occur spontaneously, without requiring a driving input, and they occur robustly, in the sense that they are generated across a wide parameter space and in the sense that they occur across the entire space of E/I conductances that gives rise to asynchronous-irregular activity dynamics. The properties of these waves depend systematically on the scales of distance-dependant connections and the speeds of action-potential propagation. The waves were well matched to those observed in cortical recordings from behaving marmosets\\(^5\\) for speeds consistent with the conduction velocity of unmyelinated horizontal fibers. Neurons sparsely participated in these waves at the scales of neuronal density and connectivity found in cortex. The sparseness of the waves allowed them to occur without disturbing the asynchronous-irregular dynamics that are observed in cortical activity and have advantages for neural computation\\(^{2,7,21,47,48}\\). These sparse-wave networks remain sensitive to spiking inputs, producing evoked responses modulated in a phase-dependent manner, as observed *in vivo*. This is in contrast to smaller scale networks that exhibit dense-waves that drive correlated fluctuations across the population and render the network insensitive to spiking inputs.\n\nThese results demonstrate the importance of considering distance-dependent time delays in neural systems. When considered at the scales of entire cortical areas, individual horizontal fibers can span distances ranging from hundreds of microns to several millimeters\\(^{43,44}\\), with axonal conduction delays on the order of tens of milliseconds\\(^{4,45}\\). While previous computational models held that the contribution of axonal delays was negligible in their effects on the temporal properties of spiking networks\\(^{49}\\), and they are rarely considered, others have found delays to be\nimportant in shaping neural dynamics\\(^{50,51}\\). Traveling waves have been described in topographic spiking network models that lack distance-dependent delays, but only in restricted parameter ranges\\(^{52-54}\\). With distance-dependent delays, however, we find that traveling waves occur across the whole asynchronous-irregular regime, in models that are sufficiently large in scale. Thus, not only are spontaneous traveling waves consistent with the asynchronous-irregular regime, they are a necessary consequence of topographic connectivity and time delays in cortex across conditions that yield asynchronous-irregular spiking.\n\nCritically, the waves we observe sparsely modulate the background spiking probability of neurons in the network, allowing them to maintain locally asynchronous-irregular dynamics. These sparse-wave dynamics only become apparent when networks are modeled at sufficient scales, in particular hundreds of thousands of neurons over an area a few millimeters across (Fig 4B). Our custom software implementation allowed for the simulation of networks with approximately 100,000 to 1,000,000 neurons, each with 3,000 synapses per cell, addressing in the largest networks over 60 GB of RAM. Importantly, while the cells in our network models have a large number of synapses per cell, the number of possible connection partners is high such that the network connectivity remains sparse. In these networks, the large number of synapses per cell allows the network to achieve self-sustained asynchronous-irregular activity when synaptic conductances are on the order observed in cortex\\(^{34,55}\\).\n\nUnlike the outsized conductances typically used in smaller network simulations, the large scale networks simulated here enabled us to incorporate E/I synaptic strengths that were similar to those observed experimentally, leading to total E/I conductances on the order of the leak conductance\\(^{20,56}\\). This is advantageous because the larger conductances needed in smaller networks yield unrealistic coupling of spiking activity to synaptic fluctuations and shunt driving inputs\\(^{57}\\), as illustrated in the dense-wave model. By scaling our model to realistic neuronal densities on a spatial scale over several millimeters of cortex (450,000 neurons over 16 mm\\(^2\\) in the case studied here), the sparse wave model sustains irregular activity, with strengths of individual synaptic inputs down to 0.5 nS and 4 nS for excitatory connections and inhibitory connections respectively. At these spatial scales and synaptic conductances, waves are present about 50% of the time, similar to what we find in neocortex, and the wavelengths closely approximate those we find *in vivo*.\nTraveling waves of neural activity in awake cortex have been observed under stimulus-evoked\\(^{41,58,59}\\), behavior-evoked\\(^{60-62}\\), and spontaneous conditions\\(^{5}\\). The fundamental neural circuit mechanism for these waves, however, had remained unclear. Our modeling results suggest that the spontaneous LFP fluctuations we observe traveling as waves in the cortex during active vision result from sparse waves of spiking activity traveling unmyelinated horizontal fibers. The sparse-wave model, which produces activity patterns consistent with the spiking activity observed *in vivo*, posits that these waves arise from the time delays inherent in communicating spikes across topographic connections within a cortical area. Further, observations from the model suggest that as these sparse waves traverse the massive recurrent connectivity within cortical areas\\(^{2,35,63,64}\\), they produce subthreshold shifts in the local E-I balance that, collectively, modulate cortical excitability. Thus, the model offers an explanation for our empirical finding that perceptual sensitivity varies over space and time depending on the alignment of wave phase\\(^{5}\\). Importantly, these traveling waves need not introduce correlated variability believed to harm perceptual sensitivity; instead, the sparse-wave state weakly modulates the background spiking probability in locally asynchronous-irregular neuron pools. Rather than a source of noise, as would be predicted if waves modulated activity akin to the dense-wave regime, the presence of these sparse waves can boost weak inputs that would otherwise have been imperceptible. These results indicate these traveling waves may be a network mechanism that can improve perceptual processing when aligned to the source of feed-forward signals, without disrupting the computational benefits of the irregular spiking dynamics of individual neurons.\n\nFigures\n\n**Figure 1. Spontaneous network fluctuations are of similar magnitude to stimulus-evoked responses.** (a) Spike raster for repeated presentations (N = 40) of a high contrast (10% Michelson contrast) drifting Gabor recorded from area MT of a fixating marmoset (stimulus-onset, red line; mean response, blue line). A single trial LFP trace is plotted in gray, and the average LFP response is plotted in black. The relative power between baseline (-100 ms to stimulus-onset) and evoked fluctuations (stimulus-onset to 100 ms) significantly favored the evoked response (right panel; N = 110 trials; median = 2.78 dB, p < 1x10\\(^{-6}\\), Wilcoxon ranked-sum test). (b) Same as in (a), but for a low contrast stimulus (< 2% Michelson contrast). The relative power between baseline and evoked LFP fluctuations was not statistically different from parity (median = 0.18 dB, p = 0.55 Wilcoxon ranked-sum test). (c) Spontaneous LFP fluctuations\nrecorded simultaneously from a spatially distributed multielectrode array were structured as traveling waves. (d) Histogram of spontaneous spike probability as a function of the Generalized Phase of the LFP during fixation. (e) The average evoked response to low contrast stimuli was stronger when a more excitable phase (\\( \\pm \\pi \\) rad) of a spontaneous traveling wave aligned with the retinotopic location of the target (green line) as compared to when a less excitable phase (0 rad) was aligned (purple line; shaded region S.E.M.; \\( p < 0.01 \\) Wilcoxon ranked-sum test). Data for panels c-e modified from Davis et al. 2020 with permission.\n\nFigure 2. Topographically-connected networks produce structured fluctuations without altering neuronal spiking dynamics. (a) Schematic diagram of a 2-D spiking network model with 80 percent excitatory (gray) and 20 percent inhibitory (blue) neurons wired with a random connection probability. (b) Spike rasters from 10000 excitatory neurons arranged by linear distance in the network. LFP fluctuations calculated from summed synaptic currents for a single 10x10 neuron pool is plotted in red. The mean spike rate across the same pool is shown in black. (c) Spatial organization of LFP amplitude for each neuron pool in the network plotted at one time. (d) Network schematic as in (a), but the network was topographically-connected with probabilities drawn from a Gaussian (\\( \\sigma = 400 \\) \\( \\mu \\)M), and activity had a distance dependent transmission delay (0.2 m/s). (e) Spike rasters as in (b), but sparse fluctuations were apparent across the network. (f) Spatial LFP amplitude as in (c), but the LFP was heterogeneous across the network with topographic structure. (g) The distribution of single unit mean firing rates did not differ between the random (blue line) and topographic networks (purple line; N= 5000 neurons; \\( p = 0.68 \\), Kolmogorov-Smirnov test). (h) The distribution of single unit C.V. did not differ between the random and topographic networks (\\( p = 0.79 \\), Kolmogorov-Smirnov test). (i) Pairwise spike coherence did not differ between the random and topographic networks (N = 1000 random pairs; CI test, \\( \\alpha = 0.05 \\); dotted lines 95% CI).\n\nFigure 3. Spontaneous topographic network fluctuations travel as waves. (a) Time series of simulated LFP activity from the topographically-connected network in Figure 2. Regional peaks and troughs moved coherently across the network as traveling waves. (b) Distribution of speeds for putative waves observed in the network. (c) Significant (white) and non-significant (black) wave values were defined as estimated wavelengths that exceeded the 99th percentile of the spatially shuffled wavelength distribution (47.67% of network activity). (d) Cumulative distribution functions (CDFs) of the estimated LFP wavelengths (blue) and shuffle wavelengths (red, 99th percentile, red dashed line). (e) The randomly-connected network had few points that\nclassify as traveling waves (1.12% of network activity). (f). Wavelength CDFs for the randomly-connected network and its shuffle.\n\nFigure 4. Spontaneous traveling waves emerge in network regimes consistent with asynchronous-irregular dynamics. (a) The percentage of wave-like activity across ranges of excitatory and inhibitory conductances. Each pixel is one simulation of a network as described in figure 2, but with the excitatory and inhibitory conductances corresponding to its x and y coordinate, respectively. Networks consistent with asynchronous-irregular spiking dynamics fall within the black border. White pixels are networks that did not self sustain or had extremely low/high mean firing rates (FR < 1 or FR > 25 sp/sec). (b) Same as a, but the mean of the wavelength distribution is plotted. (c) The region of the parameter space that exhibited asynchronous-irregular activity grew with the size of the network (width 0.5 mm to 4 mm). (d) The fraction of wave activity present across all self-sustained networks grew with the size of the simulated network (mean ± SEM).\n\nFigure 5. Wavelength and speed distributions change with connection distance and conduction velocity parameters. (a) CDFs for networks simulated across a range of Gaussian sigma values for the topographic connection probability. (b) Distributions of wave speeds across a range of networks simulated with different conduction velocities (0.1 to 0.6 m/s). (insert) The mean network speed plotted as a function of the simulated conduction velocity. (c) Waves (white pixels) were strongly present in a network with a mix of topographically (90%) and randomly (10%) connected projections and a range of conduction velocities (0.1 to 0.6 m/s). (d) CDFs for the simulation in (c) and its shuffle (blue and red respectively).\n\nFigure 6. Simulated network dynamics approximate dynamics observed in cortical recordings of area MT. (a) Distribution of mean firing rates across simulated neurons in figure 2 (blue) and the distribution observed across single and multiunits recorded from area MT of awake, behaving marmosets (red). (b) The distributions of C.V. for simulated (blue) and recorded cortical data (red). (c) CDFs of wavelengths for the simulation in figure 5c (blue), its shuffle (yellow), and the observed distribution recorded in the cortex (red). Simulated wavelengths were similar to observed wavelengths *in vivo* after applying a smoothing kernel to approximate the estimated spatial integration of the LFP in electrophysiological recordings (250 μM, gray dashed line). (d) Wave speed distributions for the simulation in figure 5c (blue), and recorded cortical data (red) covered a range consistent with axonal conduction velocities (0.1 to 0.6 m/s).\nFigure 7. Spontaneous waves reflect structured fluctuations in E/I balance that sparsely modulate spike probability. (a) Membrane voltage for a simulated neuron in either the sparse-wave network (black line) or dense-wave network (purple-line) calculated from the summed excitatory and inhibitory synaptic currents received by that neuron. Spiking activity occured when the voltage crosses the threshold (\\( V_{th} \\) red line). The distribution of membrane potentials over the interval for the sparse and dense networks is plotted on the right. (b) The amplitude of the simulated LFP (blue line) and the relative level of excitatory and inhibitory currents (red line) over a 10x10 neuron pool were counterphase. (c) Scatter plot of LFP and E-I difference revealed a significant negative correlation (N = 50000 time points; Pearson’s r = -0.83; CI test, \\( \\alpha = 0.01 \\)). (d) Spike-phase coupling was significant across networks in the asynchronous-irregular regime, and the degree of coupling was negatively correlated with the magnitude of synaptic conductances (N = 646 simulations; Pearson’s \\( r = -0.45 \\pm 0.06 \\), CI test, \\( \\alpha = 0.05 \\)). (e) Histogram showing the fraction of spikes that occurred during each phase of the simulated LFP in the topographically-connected network. Spike probability was significantly modulated by LFP phase (N = 22 resamples versus shuffle; circular-resultant = 0.15, p < 1x10\\(^{-4}\\), Wilcoxon signed-rank test). (f) Same as in (e), but for recorded cortical data. Spike probability was similarly significantly modulated (circular-resultant = 0.16; N = 22 recording sessions versus shuffle; p < 1x10\\(^{-4}\\), Wilcoxon signed-rank test). (g) The dense-wave network simulation had a significantly stronger spike-phase relationship (N = 10 resamples; circular-resultant = 0.43, p < 1x10\\(^{-4}\\), Wilcoxon ranked-sum test).\n\nFigure 8. The sparse-wave network regime boosts spike inputs while the dense-wave network shunts. (a) The average firing rate across a neuron pool in the sparse-wave network model received a 50 Hz Poisson spike train input for 10 ms aligned either to a period of depolarization (blue shaded region) or hyperpolarization (red shaded region) as defined by the spike-LFP phase relationship. The blue and red lines are the mean evoked firing rate after receiving the spiking input in either the depolarized or hyperpolarized phase respectively (faint blue and red lines represent 20 individual trials). The black line is the firing rate of the neuron pool when no input was given. (b) Same as (a), but the inputs were delivered to the dense-wave network. The evoked responses were much weaker as the network shunted the currents evoked by the incoming spikes. (c) The response gain between the distributions of spontaneous and evoked activity across 20 presentations of spiking input. In the sparse-wave network (left bars), inputs during the depolarized state had larger relative responses as compared to inputs during\nthe hyperpolarized state. Conversely, the dense-wave network (right bars) responses had higher gain during the hyperpolarized state, which was still significantly weaker than the depolarized state in the sparse-wave network (4.25 ± 0.11 v. 1.74 ± 0.07; p < 1×10^{-7}, Wilcoxon ranked-sum test).\n\nSupplemental Figures\n\nFigure S1. Dense spiking waves induce pairwise correlation while sparse spiking waves do not. (a) Spike raster for a 10000 neuron network simulation with topographic connections and delays. Dense spike participation in traveling waves produces large fluctuations in spiking activity (black line, pooled LFP example red line). (b) The spike-spike coherence for 1000 randomly selected pairs of neurons has a strong peak between 20-30 Hz (black line, dotted lines 95% CI) corresponding to the peak of the PSD for the example LFP (red line). (c) Spike probability is strongly coupled to the phase of the LFP.\n\nFigure S2. Randomly-connected spiking network model has weak spike-LFP phase coupling. (a) Histogram showing the fraction of spikes that occurred during each phase of the LFP in the randomly connected network shown in Figure 2 (circular-resultant = 0.07).\n\nTable S1. Parameters for random, sparse-wave, and dense-wave network simulations\n\nTable S2. Parameters for networks of various sizes\n\nMethods\n\nIn vivo cortical recordings\n\nOne male (monkey W) and one female (monkey T) marmoset monkey (*Callithrix jacchus*) was surgically implanted with a headpost for head stabilization and eye tracking. The headpost contained a hollow chamber housing an Omnetics connector for a Utah array (Blackrock Microsystems), which was implanted in a 7×10 mm craniotomy over area MT (stereotaxic coordinates 2 mm anterior, 12 mm dorsal). An 8×8 (64 channel, monkey W) and 9×9 with alternating channels removed (40 channel, monkey T) Utah array was chronically implanted over area MT using a pneumatic inserter wand. The electrodes spacing was 400 μM with a pitch depth\nof 1.5 mm. The craniotomy was closed with Duraseal (Integra Life Sciences, monkey W) or Duragen (Integra Life Sciences, monkey T), and covered with a titanium mesh embedded in dental acrylic. All surgical procedures were performed with the monkeys under general anesthesia in an aseptic environment in compliance with NIH guidelines. All experimental methods were approved by the Institutional Animal Care and Use Committee (IACUC) of the Salk Institute for Biological Studies and conformed with NIH guidelines.\n\nMarmosets were trained to enter a custom-built marmoset chair that was placed inside a faraday box with an LCD monitor (ASUS VG248QE) at a distance of 40 cm. The monitor was set to a refresh rate of 100 Hz and gamma corrected with a mean gray luminance of 75 candelas/m\\(^2\\). Electrode voltages were recorded from the Utah arrays using two Intan RHD2132 amplifiers connected to an Intan RHD2000 USB interface board. Data were sampled at 30 kHz from all channels. The marmosets were headfixed by a headpost for all recordings. Eye position was measured with an IScan CCD infrared camera sampling eye position at 500 Hz. Stimulus presentation and behavioral control was managed through MonkeyLogic in Matlab. Digital and analog signals were coordinated through National Instrument DAQ cards (NI PCI6621) and BNC breakout boxes (NI BNC2090A). Neural data was broken into two streams for offline processing of spikes (single-unit and multi-unit activity) and LFPs. Spike data was high-pass filtered at 500 Hz and candidate spike waveforms were defined as exceeding 4 standard deviations of a sliding 1 second window of ongoing voltage fluctuations. Artifacts were rejected if appearing synchronously (within 0.5 ms) on over a quarter of all recorded channels. Segments of data (1.5 ms) around the time of candidate spikes were selected for spike sorting using principal component analysis through the open source spike sorting software MClust in Matlab (A. David Redish, University of Minnesota). Sorted units were classified as single- or multi-units and single units were validated by the presence of a clear refractory period in the autocorrelogram. LFP data was low-pass filtered at 300 Hz and down-sampled to 1000 Hz.\n\nReceptive Field Mapping\n\nReceptive fields were mapped through reverse correlation. The marmoset was trained to hold fixation on an image (marmoset face, 1 degree of visual angle (DVA) square) presented to the center of the LCD monitor. A drifting Gabor (2 degrees diameter, spatial frequency: 0.5 cycles per degree, temporal frequency 10 cycles per second) was presented at a random position on the monitor between 0-18 degrees in azimuth and -15 to 15 degrees in elevation, drifting in one of 8 possible directions for 200 ms, after which it disappeared. After a random delay drawn from\nan exponential distribution (mean 40 ms), a new probe appeared and the pattern repeated until the marmoset broke fixation (defined as an excursion of 1.5 degrees from fixation) or viewed 16 probes. The marmoset was given a juice reward proportional to the number of probes presented. The receptive field for each unit recorded on the array was estimated by calculating the spike-triggered average (STA) stimulus that evoked the maximal response:\n\n\\[\nSTA = \\frac{1}{N} \\sum_i^N x_i y_i\n\\]\n\nThe STA is the sum of probe location \\( x_i \\) weighted by the spike count \\( y_i \\) within the time bin 40 to 200 ms after probe onset, normalized by the number of all recorded spikes \\( N \\). From the location of estimated receptive fields on each spiking channel, and the known topography of area MT in the marmoset\\(^{65}\\), we estimated the relative position of each recording array in marmoset cortex (Fig. 1a). We excluded from the analysis the upper half of monkey W’s array as the recordings did not appear to be in area MT.\n\n*Behavioral Task*\n\nThe marmosets were trained to saccade to a marmoset face to initiate each trial, after which the face turned into a fixation point (0.15 DVA). The marmosets held fixation on the fixation point (1.5 degree tolerance) for a minimum duration (400 ms monkey W, 300 ms monkey T) awaiting the appearance of a drifting Gabor (4 DVA diameter which reliably produced evoked responses on 1-2 electrodes; spatial frequency, 0.5 cycles per degree; temporal frequency, 10 cycles per second, drifting in one of up to 8 possible directions). Spontaneous data were analyzed from the period of fixation preceding the appearance of a target. Early fixation breaks (defined by the excursion of the eye position from the fixation window) were excluded from analysis. The target only appeared if fixation was held for an additional random duration drawn from an exponential distribution (mean 200 ms) to generate a flat hazard function.\n\n*Computational Simulations*\n\nThe model consists of \\( N \\) leaky integrate-and-fire (LIF) neurons, with \\( N_e = 0.8N \\) excitatory units and \\( N_i = 0.2N \\) inhibitory. The membrane potential \\( V \\) of the \\( i \\)th unit evolves in time according to the equation:\n\\[\nC_m \\dot{V}_i = g_L (E_L - V_i) + g_e (E_e - V_i) + g_i (E_i - V_i)\n\\]\nwhere \\( C_m \\) is the membrane capacitance, \\( g_L \\) is the leak conductance, \\( E_L \\) is the resting membrane potential, \\( g_{\\{e,i\\}} \\) are the time-dependent synaptic conductances, respectively, and \\( E_{\\{e,i\\}} \\) are the reversal potentials for excitatory and inhibitory synaptic transmission. When the membrane potential \\( V_i \\) exceeds threshold \\( V_t \\), the model obeys the following spike and reset conditions:\n\n\\[\nV_i \\rightarrow V_r \\\\\ng_{\\{e,i\\},j} \\rightarrow g_{\\{e,i\\},j} + w_{\\{e,i\\}} \\quad \\forall j \\in [1, K]\n\\]\n\nwhere \\( V_r \\) is the reset potential, \\( w_{\\{e,i\\}} \\) are the excitatory and inhibitory synaptic weights, respectively, and \\( K \\) is the number of postsynaptic targets of neuron \\( i \\). Following the initial conductance increase caused by an incoming spike, the excitatory and inhibitory synaptic conductances follow exponential decay:\n\n\\[\n\\tau_{\\{e,i\\}} \\; \\dot{g}_{\\{e,i\\}} = -g_{\\{e,i\\}}\n\\]\n\nwhere \\( \\tau_{\\{e,i\\}} \\) are the excitatory and inhibitory synaptic time constants.\n\nNetwork connectivity and axonal conduction delays\n\nWe studied either spiking network models with unstructured, random connectivity (random networks, Fig. 2a) or topographic, locally random connectivity (topographic networks, Fig. 2d, for parameters see Table S1). Neurons in the random network were connected to \\( K \\) post-synaptic targets chosen with uniform probability. Axonal delays (\\( \\tau \\)) in the random network were short and homogeneous (300 \\( \\mu \\)s). In the topographic network, connections were chosen to \\( K \\) post-synaptic targets with probability decaying as a Gaussian with distance from the sending neuron, with spatial width \\( \\sigma_s \\) of 400 \\( \\mu \\)m (except where the effect of this parameter is studied systematically in Fig. 6a). Axonal conduction delays in the topographic network increased linearly with distance between pre- and post-synaptic cells:\n\n\\[\n\\tau_{ij} = \\tau_s + \\frac{d_{ij}}{v_c}\n\\]\nwhere \\( \\tau_{ij} \\) is the delay from neuron \\( i \\) to neuron \\( j \\), \\( \\tau_s \\) is the delay caused by synaptic vesicle release, \\( d_{ij} \\) is the Euclidean distance between \\( i \\) and \\( j \\), and \\( v_c \\) is the axonal conduction speed. All distances were calculated taking 2D periodic boundary conditions into account, effectively wrapping the network onto a toroidal topology\\(^{55,66}\\).\n\nSelf-sustained activity\n\nInstead of initializing self-sustained activity through a “kick” of external Poisson input spikes\\(^{33,34,37}\\), which may induce trace activity correlations, we recorded the state variables of a self-sustained network, including membrane potential (\\( V \\)) and conductance (\\( g_{\\{e,i\\}} \\)), after a long period (10 seconds) of simulated self-sustained activity. Taking these distributions as a steady state, we then used the Gaussian approximation (mean and variance) to initialize the membrane potentials and conductances with randomly drawn values in the simulations thereafter. After starting the simulation with these initial conditions, networks with approximately balanced excitation and inhibition exhibit self-sustained, irregular spiking activity. Each simulation ran for 1.2 seconds, from which we eliminated the first 200 ms from our analysis in case of residual initialization artifacts.\n\nSpike train statistics and the asynchronous-irregular regime\n\nTo characterize basic spike train statistics, we randomly selected 5,000 neurons in the simulation and measured the mean firing rate, coefficient of variation (C.V., defined as the ratio of the standard variation of the interspike interval to the mean for each neuron that has a minimum of 3 spikes over the simulation window), and the average pairwise correlation (average Pearson correlation between spike trains smoothed with a 100 ms window for 1,000 randomly selected pairs). To prevent longer simulations with high firing rate during our parallel runs, networks that produced mean firing rates over 50 sp/s had an early exit condition. Simulations were classified as asynchronous-irregular if the mean firing rate across all simulated units was greater than 1 and less than 25 sp/s; the mean C.V. across all units was greater than 0.7 and less than 1.4, and the average pairwise cross-correlation was greater than -0.1 and less than 0.1.\n\nPairwise Spike Coherence\nPairwise spike coherence was calculated using multitaper methods as described previously67. The 1000 ms of simulation time was broken into 500 ms epochs, stepping 125 ms to cover the full period. The DC component of each unit’s spike train was removed, and tapered with a single Slepian taper, giving an effective smoothing of 2.5 Hz for the 500ms data windows (NW = 1, K = 1). To control for differences in firing rate among units, randomly chosen spikes were eliminated in order to equate the total number of spikes in each paired spike train. This procedure was repeated 10 times and the results were averaged to produce the single paired coherence. Coherence was then computed across 1000 randomly selected pairs of units, and normalized by the pooled power spectrum. Confidence intervals were evaluated using a jack knife procedure leaving out individual pairs of units.\n\nNETSIM software\n\nSimulations were generated using a specialized program called NETSIM, which is approximately 1,500 lines of C code (available at http://mullerlab.github.io). Equations in the model were integrated using the forward Euler method with a timestep of 0.1 ms. Simulation results were additionally point-checked with shorter timesteps throughout. Random numbers were generated using a C implementation of the ISAAC algorithm68 (Tom Bartol, personal communication). To verify the numerical integration in this program, we confirmed the network displayed the correct firing rate for unconnected LIF neurons with varying DC-current injections. We also verified simulations under a simple feed-forward network topology to confirm the accuracy of the simulations. Additionally, to ensure reproducibility of our computational simulations69, we compared results from NETSIM and Brian2 at specific points in the \\((g_e, g_i)\\) parameter space for the balanced random network model, verifying that the mean firing rate, C.V., and cross-correlation were in agreement between the two simulators.\n\nNetwork Parameter Scans\n\nIn order to identify the excitatory and inhibitory synaptic conductance weights that produced self sustained and asynchronous-irregular activity, we simulated networks with 50 values of \\(g_e\\) ranging from 0.1 to 5 nS and \\(g_i\\) ranging from 1 to 50 nS for a total of 2,500 simulations (Table S2). In order to determine the effect of network scale on the range of these 2,500 simulations that produced self sustained and asynchronous-irregular activity, we repeated these simulations 5 times with varying parameters of network size, neuron number, and connections per neuron\n(Table S2). The number of neurons per network size was chosen to maintain a density of 28,125 neurons per mm². The number of connections was chosen to maintain the density of connections within the Gaussian used to assign connections across network sizes. For larger networks (> 2 mm) the connection number did not grow with the size of the network, as 99 percent of the connections occur within 3 S.D. of the Gaussian (\\( \\sigma = 400 \\mu\\mathrm{M} \\)). In order to run these simulations across all combinations of network size and conductance parameters, we utilized the Extreme Science Engineering Discovery Environment (XSEDE) Comet cluster at the San Diego SuperComputer (SDSC) center at UC San Diego. Data analysis for these simulations was also performed on the Comet cluster running MATLAB. Circular variables were analyzed using the Circular Statistics Toolbox.\n\nCalculation of LFP estimate\n\nWe utilized a previously developed proxy for the LFP generated by a network of point LIF neurons, which was systematically developed from a spatially extended model[38]. The LFP estimate \\( \\lambda(t) \\) is computed as a weighted sum of the excitatory and inhibitory synaptic currents \\( I_e \\) and \\( I_i \\) across \\( m \\) excitatory cells in each 10 x 10 neuron pool:\n\n\\[\n\\lambda(t) = \\sum_j^m I_{e,j}(t - \\tau) - \\alpha \\sum_j^m I_{i,j}(t)\n\\]\n\nwhere \\( \\tau = 6 \\) ms and \\( \\alpha = 1.65 \\). This LFP proxy is then computed for each 10 x 10 neuron pool across the two-dimensional network. This proxy was initially computed independently for each neuron pool, excluding effects from mixing of the LFP signal across space. We note that excluding these effects is a conservative step, as the addition of the mixing across space would only increase traveling waves in the LFP. Further, we note that our results do not depend critically on the choice of LFP proxy and our conclusions are unchanged when analyzing the mean membrane potentials or excitatory synaptic conductances.\n\nIn order to compare the properties of waves in our model, where LFP signals are independent across space, from waves recorded from the cortex, where electrodes pool signals across a volume approximately 250 \\( \\mu\\mathrm{M} \\) in radius[29,70], we convolved the LFP with a 2D Gaussian kernel (with a spatial standard deviation of 4 LFP bins, corresponding to a radius of 272 \\( \\mu\\mathrm{M} \\)) before further analysis.\nAnalysis of spatiotemporal dynamics\n\nTo analyze spatiotemporal dynamics in the population activity produced by the spiking network model, we used a technique we recently developed for wideband analysis of non-stationary data. Briefly, for each real-valued time series \\( \\lambda_{x,y}(t) \\) \\( \\forall x \\in [1, N_c], y \\in [1, N_r] \\), where \\( N_c \\) and \\( N_r \\) are the number of columns and rows, respectively, we compute the generalized phase (GP) \\( \\phi_{x,y} \\) at each point using the corrected analytic signal representation introduced in recent work\\(^5\\). We next calculated the gradient of GP \\( \\vec{g}_{x,y}(t) \\) at each moment in time:\n\n\\[\n\\vec{g}_{x,y}(t) = -\\nabla \\phi_{x,y}(t)\n\\]\n\nFor the spatial gradient, derivatives are taken across the two dimensions of space and are approximated by the appropriate forward and centered finite differences. As in previous work, phase derivatives were implemented as multiplications in the complex plane\\(^{41,71}\\), so that unwrapping phase across the two dimensions of the network was not necessary. Wavelength is the reciprocal of the phase gradient magnitude at each point in space and time. Wave speed was computed as the ratio of instantaneous frequency to phase gradient magnitude, as in previous work\\(^{60}\\).\n\nCalculation of response gain\n\nIn order to quantify the sensitivity of the sparse and dense-wave network regimes to incoming stimulation, we first identified depolarized and hyperpolarized states from the LFP of a 10 x 10 neuron pool defined by the spike-phase bins that generated the maximum or minimum spiking probability respectively for each network regime. We then applied feed-forward stimulation of 50 Hz Poisson spiking input to 100 synapses for each neuron within the 10 x 10 neuron pool for 10 ms, aligned to the depolarized or hyperpolarized phase in the network. This process was repeated across 20 trials, yielding a distribution of evoked responses. The same random seed was used to construct the networks across each trial, so that the simulations were identical up to the point of stimulation. We calculated the ratio of the evoked responses to the spontaneous response in the absence of any stimulation at the defined time point.\n\nAcknowledgments: The authors would like to thank Katie Williams, Sean Adams, and Mat LeBlanc for their contributions to this project, in addition to the San Diego Supercomputer Center for their support for this project. The authors would also like to thank Tom Bartol for discussions\non the software implementation. Funding: Gatsby Charitable Foundation, the Fiona and Sanjay Jha Chair in Neuroscience, the Canadian Institute for Health Research, the Swartz Foundation, NIH grants R01-EY028723, T32 EY020503-06, T32 MH020002-16A, and BrainsCAN at Western University through the Canada First Research Excellence Fund (CFREF).\n\nAuthor Contributions: Conceptualization, Z.W.D., G.B.B., C.F., T.D., T.J.S., J.H.R., L.M.; Data Curation, Z.W.D., G.B.B. C.F., T.D., L.M.; Formal Analysis, Z.W.D., G.B.B., C.F., T.D., L.M.; Funding Acquisition, Z.W.D., T.J.S., J.H.R., L.M.; Investigation, Z.W.D., G.B.B., L.M.; Methodology, Z.W.D., G.B.B., C.F., T.S., J.H.R., L.M.; Supervision, T.J.S., J.H.R., L.M.; Visualization, Z.W.D., G.B.B., L.M.; Writing - original draft, Z.W.D., G.B.B., C.F., T.D. J.H.R., L.M.; Writing - review and editing, Z.W.D., G.B.B., T.J.S., J.H.R., L.M.\n\nCompeting Interests: Authors declare no competing interests.\n\nMaterials & Correspondence: Correspondence and requests for material should be addressed to J.H.R and L.M.\n\nData Availability: The data that support the findings of this study are available from the corresponding author upon reasonable request.\n\nCode Availability: An open-source code repository for all methods is available on http://mullerlab.github.io.\n\nReferences\n\n1. Destexhe, A. & Rudolph-Lilith, M. Neuronal Noise: (Springer US, 2012).\n2. Destexhe, A., Rudolph, M. & Paré, D. 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Signal Process. **25**, 735–802 (2011/4).\nFigures\n\n![Panel a: High Contrast Target (10%) showing single-trial LFP, mean LFP, and mean spike rate traces; panel b: Low Contrast Target (<2%) showing similar traces; panel c: Detected Spontaneous Traveling LFP Wave heatmaps; panel d: Spontaneous Spike-Phase Coupling histogram; panel e: Wave-Dependent Evoked Modulation line graph](page_68_120_1447_1042.png)\n\nFigure 1\n\n[Please see the manuscript file to view the figure caption.]\nFigure 2\n\n[Please see the manuscript file to view the figure caption.]\nFigure 3\n\n[Please see the manuscript file to view the figure caption.]\nFigure 4\n\n[Please see the manuscript file to view the figure caption.]\nFigure 5\n\n[Please see the manuscript file to view the figure caption.]\nFigure 6\n\n[Please see the manuscript file to view the figure caption.]\nFigure 7\n\n[Please see the manuscript file to view the figure caption.]\nFigure 8\n\n[Please see the manuscript file to view the figure caption.]\n\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• tableS1.pdf\n• tableS2.pdf\n• figureS2.pdf\n• FigureS1.pdf"} {"paper_id": "prb26", "title": "Virtual brain twins for stimulation in epilepsy", "text": "Virtual brain twins for stimulation in epilepsy\n\nHuifang Wang\nhuifang.wang@univ-amu.fr\n\nAix Marseille Univ, INSERM https://orcid.org/0000-0002-4060-8649\nBorana Dollomaja\nAix Marseille Univ, INSERM\nPaul Triebkorn\nAix-Marseille University https://orcid.org/0000-0002-0371-8400\nGian Marco Duma\nAix Marseille Univ, INSERM\nAdam Williamson\nAix Marseille Univ, INSERM\nJulia Makhalova\nAix Marseille Univ, CNRS, CRMBM;\nJean-Didier Lemarecha\nAix Marseille Univ, INSERM\nFabrice Bartolomei\nAix Marseille Univ, INSERM\nViktor Jirsa\nAix-Marseille University https://orcid.org/0000-0002-8251-8860\n\nArticle\n\nKeywords: Personalized medicine, Brain modelling, Epilepsy, Stimulation, Stereo-EEG, Temporal interference, Diagnosis and treatment\n\nPosted Date: September 4th, 2024\n\nDOI: https://doi.org/10.21203/rs.3.rs-4908955/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nAdditional Declarations: There is NO Competing Interest.\nVersion of Record: A version of this preprint was published at Nature Computational Science on August 5th, 2025. See the published version at https://doi.org/10.1038/s43588-025-00841-6.\nVirtual brain twins for stimulation in epilepsy\n\nHuifang E. Wang1*, Borana Dollomaja1, Paul Triebkorn1, Gian Marco Duma1,5, Adam Williamson1, Julia Makhalova2,3,4, Jean-Didier Lemarecha1, Fabrice Bartolomei1,2, Viktor Jirsa1*\n\n1* Aix Marseille Univ, INSERM, INS, Inst Neurosci Syst, Marseille, 13005, France.\n2 APHM, Epileptology and Clinical Neurophysiology Department, Timone Hospital; Marseille, 13005, France.\n3 Aix Marseille Univ, CNRS, CRMBM ; Marseille, 13005, France.\n4 APHM, Timone University Hospital, CEMEREM ; Marseille, 13005, France.\n5 Epilepsy Unit, IRCCS E. Medea Scientific Institute, Via Costa Alta 37, Conegliano, Treviso 31015, Italy.\n\n*Corresponding author(s). E-mail(s): huyfang.wang@univ-amu.fr;\nviktor.jirsa@univ-amu.fr;\nContributing authors: borana.DOLLOMAJA@univ-amu.fr; jan-paul.TRIEBKORN@univ-amu.fr; giannmarco.duma@lanostrafamiglia.it; adam.WILLIAMSON@univ-amu.fr; Julia.SCHOLLY@ap-hm.fr; jean-didier.LEMARECHAL@univ-amu.fr; Fabrice.BARTOLOMEI@ap-hm.fr;\n\nAbstract\nEstimating the epileptogenic zone network (EZN) is an important part of the diagnosis of drug-resistant focal epilepsy and plays a pivotal role in treatment and intervention. Virtual brain twins, based on personalized whole brain modeling, provide a formal method for personalized diagnosis and treatment. They integrate patient-specific brain topography with structural connectivity from anatomical neuroimaging such as MRI, and dynamic activity from functional recordings such as EEG and stereo-EEG (SEEG). Seizures demonstrate rich spatial and temporal features in functional recordings, which can be exploited to estimate the EZN. Stimulation-induced seizures can provide important and complementary information. We consider invasive SEEG stimulation as the most practical current approach, and temporal interference (TI) stimulation as a potential future approach for non-invasive diagnosis and treatment. This paper offers a virtual brain twin framework for EZN diagnosis based on stimulation-induced seizures. This framework estimates the EZN and validated the results on synthetic data with ground-truth. It provides an important methodological and conceptual basis for a series of ongoing scientific studies and clinical usage, which are specified in this paper. This framework also provides the necessary step to go from invasive to non-invasive diagnosis and treatment of drug-resistant focal epilepsy.\n1 Introduction\n\nIn the most complex cases of drug-resistant focal epilepsy, accurate diagnosis requires invasive stereo-EEG (SEEG) implantation. This procedure is crucial for estimating the epileptogenic zone network (EZN), a key element for successful treatment [1, 2]. SEEG has become one of the principal techniques for delineating EZNs [3, 4]. In the past 15 years, several data analysis methods for quantifying EZNs were proposed based on the spectral analysis of SEEG signals [5, 6]. Beyond pure data-driven analysis approaches, several methods linking mechanistic models and data analysis have been developed [7–12], formally exploiting causal hypotheses within an inference framework. We developed a workflow for the estimation of a patient’s EZN using personalized whole brain models, called the virtual epileptic patient (VEP), [13–16]. The VEP workflow was evaluated retrospectively using 53 patients with 187 spontaneous seizures and is now being evaluated in an ongoing clinical trial (EPINOV) with an expected 356 prospective patients with epilepsy [14, 15]. The virtual brain twin concept has been proposed based on the VEP workflow and was extended to various brain disorders [17]. Virtual brain twins are personalized, generative and adaptive brain models based on data from an individual’s brain for scientific and clinical use. In this study, we introduce the first high-resolution virtual brain twin workflow, specifically designed for estimating the EZN using a stimulation paradigm.\n\nSEEG stimulation, involving direct electrical stimulation through SEEG electrodes, can be used to map brain function, as well as to provoke seizures for better EZN diagnosis, especially when spontaneous seizures are not obtained. SEEG stimulation-induced seizures (at 1 Hz or 50 Hz, usually with pulses of 1 ms at 1-3 mA) are an important tool for localizing the EZ and are also associated with a better post-surgical outcome [18–20]. First, we propose a personalized whole brain model, i.e a virtual brain twin, dedicated to assessing stimulations performed through SEEG electrodes. We build a high-resolution brain model for an individual patient and compute the electric fields induced by SEEG stimulation. We simulate the brain responses induced by SEEG stimulation and estimate the EZN based on the induced seizures. As the ground truth is known for the simulated data, we can formally validate the EZN estimation. Then, we evaluate the capacity of our approach to translate from invasive stimulation and recording via SEEG to non-invasive procedures using scalp-EEG recordings and\ntranscranial electrical stimulation techniques, notably temporal interference (TI). The recently developed TI has the capacity of reaching deeper structures than conventional transcranial direct/alternating current stimulation (tDCS/tACS) [21, 22]. Thus combining the advantages of tDCS and DBS [23], TI stimulation [24] is both non-invasive and focal and can stimulate deep structures of the brain. TI exploits the insensitivity of brain tissue to electric stimulation at high frequencies (above 500 Hz) [24]. When two slightly detuned high frequency electric fields are applied at different locations, their interference provides an envelope modulation at a lower frequency, equal to the difference between the two electric field frequencies \\( \\Delta f \\) (normally below 150 Hz), and acts as an effective stimulation at a desired targeted location. Thus the obtained low frequency modulation is relevant to functional dynamics of the brain.\n\nIn summary, this study presents a workflow for estimating the EZN using personalized high-resolution virtual brain twin under a stimulation paradigm. We develop a pipeline that can 1) build a personalized high-resolution brain model for either SEEG or TI stimulation; 2) estimate the EZN from stimulation-induced seizures, and validate it by simulated data; and 3) refine the estimation of EZN by integrating multiple recording modalities, such as by combining scalp-EEG and SEEG. This research provides a necessary step for 1) a series of scientific and clinical studies, such as optimization of stimulation parameters for diagnosis and treatment; 2) moving from invasive to non-invasive diagnosis and treatment of drug-resistant focal epilepsy; 3) natural integration of multiple functional data modules.\n\n2 Results\n\n2.1 VEP-stimulation workflow\n\nWe built a high-resolution virtual brain twin workflow to estimate the EZN using stimulation techniques. First, we built a virtual brain twin based on available data before stimulation. An EZN is defined as the tissue responsible for generating seizures and may involve distant brain areas characterized by altered excitability [1]. Our model-based high-resolution workflow using perturbation techniques for diagnostic EZ mapping is shown in Fig. 1 and the detailed flowchart is shown in supplementary Fig. A1. First, high-resolution full brain network models (Fig. 1 A) were established using patient-specific data from patients with epilepsy. The structure of the model was defined by the detailed surface of the cortex and the subcortical volumes. The heterogeneous structural connectivity between brain regions through white matter fibers was estimated from diffusion-weighted MRI. The cortical surface data was generated from\nFig. 1 The workflow of the virtual brain twin for estimating the epileptogenic zone network (EZN) using stimulation techniques. A personalized high-resolution model (A) is based on individual brain geometry extracted from T1-weighted MRI and structural connectivity from tractography on diffusion-weighted MRI data (B). High resolution virtual brain models simulate neural source activity with spatial resolutions of about 10 \\( mm^2 \\). The modelling parameters are inferred from the spontaneous SEEG recordings (B). We illustrated two types of stimulation: SEEG and Temporal interference (TI), to induce seizure activity. SEEG stimulation (C) uses bipolar stimulation in which two electrodes are used: one serves as the cathode and the other as the anode. The electric current flows between two electrodes, which is parameterized by current amplitude, pulse width and frequency. TI stimulation (D) applies two current sources simultaneously via electrically isolated pairs of scalp electrodes (green and pink) at kHz frequencies \\( f \\) and \\( f + \\Delta f \\). The currents generate oscillating electric fields which results in an envelope amplitude that is modulated periodically at \\( \\Delta f \\). The electric field influences the brain activity which can be generated by the high-resolution personalized whole-brain model (A). The red and blue dots represent SEEG and scalp-EEG electrodes, respectively. The simulated source activity can be mapped onto the corresponding SEEG and scalp-EEG signals (E), through the gain matrices, which are constructed based on the locations of SEEG/scalp-EEG electrodes relative to the source vertices. The red curves on the scalp-EEG recordings are plotted using a different scale to visualize the signals following the high-amplitude signals induced by TI stimulation. By utilizing data features extracted from SEEG and scalp-EEG signals, Bayesian inference methods can estimate a posterior distribution of epileptogenic values, suggesting the potential EZN (F).\n\nT1-weighted MRI using the Freesurfer software package, resulting in surfaces with 20284 vertices with a vertex area of about 10 \\( mm^2 \\). We simulated the time series on the patient’s specific structural scaffold using the phenomenological Epiletor model [25], a system of differential equations that can describe seizure initiation, propagation, and termination, resulting in electrophysiological seizure like events. The spatial domain of the Epiletor is given by the high-resolution network of neural masses, thus seizures can propagate locally across neighboring vertices of the cortex and globally\nthrough white matter fiber connections [7]. The personalized modelling parameters can be inferred from the spontaneous seizure recording [15].\n\nThen, we developed the first high-resolution virtual brain twin designed for stimulation. First, we calculated the electric fields induced by both stimulation methods (Fig. 1 C,D). For the SEEG stimulation, two SEEG electrodes serve as cathode and anode to generate bipolar stimulation and electric current flow is parameterized by current amplitude, pulse width and frequency (Fig. 1 C). The perturbation effect was applied to the vertices of the high-resolution surface through the SEEG-to-source mapping, with perturbation strength decaying as the distance between vertices and electrodes increased. For the TI stimulation, we calculated the envelope amplitude of the TI electric field for each vertex whose envelope is modulated at the frequency \\( \\Delta f \\) (Fig. 1 D). Both types of stimulation generated an accumulative increase in the state variable \\( m \\) of the Epileptor-Stimulation model (eq. 1). The slowly evolving state variable captures changing tissue properties under electric stimulation. When \\( m \\) reaches a given threshold, the model undergoes a transition into the seizure state. A post-SEEG implantation CT scan is used to localize SEEG contacts and co-register them with the structural scaffold. Scalp-EEG electrodes were placed on the scalp using the standard international 10-5 system to place scalp-EEG electrodes. This high-resolution model allows us to consider detailed electric dipoles, generated by neural activity, for building high-fidelity forward solutions. The gain matrix maps the activity from the neural sources (located at vertices of the surface and subcortex) to the electrodes (SEEG/scalp-EEG), based on their orientation and distance.\n\nModel inversion estimates patient-specific brain model parameters, especially epileptogenicity and global network scaling using Hamiltonian Monte Carlo (HMC) sampling techniques from Bayesian inference methods [10, 15]. The estimation is based on the structural brain scaffold, modelled seizure dynamics, and the data feature extracted from scalp-EEG and/or SEEG seizure recordings (Fig. 1 E). The model inversion uses a noninformative prior where all the brain regions have the same prior distribution (the prior assumption is that all regions are healthy). The result is the posterior probability from which the EZN is identified. We also introduced multimodal inference for simultaneous SEEG/scalp-EEG to infer the EZN (Fig. 1 F).\n\n2.2 Virtual brain twins for SEEG stimulation\n\nWe used the data from a right-handed 23 years old female patient diagnosed with left occipital lobe epilepsy to illustrate how to use our workflow. We first extracted the brain geometry, the structural connectivity matrix and the source-to-sensor mapping\nFig. 2 VEP diagnostic mapping for spontaneous seizures. (A) Selected SEEG recordings from one seizure in a 23-year-old female patient. (B) Posterior distribution of the epileptogenic values (EV) (higher value indicates higher probability of seizure) for ten selected regions obtained from the HMC pipeline. (C) Heatmap of the left O2 identified by VEP (in red) shown in a preoperative T1-MRI. (D) Heatmap of the left O2 identified by VEP (in red) shown in a postoperative T1-MRI. (E) The left O2 (in red) was projected on the patient’s 3D meshes.\n\nfrom the T1-MRI, diffusion-weighted MRI, and post-SEEG-implantation CT scans for this patient. We built the whole brain neural mass model based on this anatomical information. Then we ran the HMC algorithms for three spontaneous seizures recorded from this patient (one of the three seizures is shown in Fig. 2 (A)). We pooled the posterior distribution from the three seizures, in which the left lateral occipital cortex (region O2 (in VEP atlas [26]) was consistently identified as part of the EZ. Then we projected the left O2 onto both preoperative and postoperative T1-MRI slides and 3D brain meshes (in Fig. 2(C-E)) to compare its extent with the size of the surgical resection. The patient underwent resective surgery, in which a large portion of the left O2 was removed, and was almost seizure free after surgery (surgery outcome class of Engel II [27]). Based on this result, we built the high-resolution whole brain model for SEEG- and TI-stimulation with the hypothesis that the left O2 was the EZ of the patient.\n\nTo model direct electrical stimulation by SEEG electrodes in the brain, we first mapped the contribution of SEEG stimulation current to brain source activity. We\nFig. 3 Estimating EZN from a SEEG stimulation induced seizure. (A) GL’5-6 (large blue/red sphere) is the stimulated contact in the left occipital lobe, using a bipolar pulse stimulation (50 Hz for a duration of 3.5 s with pulse duration 1 ms) (Top). The spatial mapping of the maximum of stimulation values for each vertex of the brain from contact pair GL’5-6 (bottom). (B) Neural source activity is shown on the cortical mesh at 5 different time points. The seizures are located around the left O2 region of the VEP atlas. (C) Selected simulated SEEG time-series from a SEEG stimulation-induced seizure. (D) Posterior distribution of the EV (higher value indicates higher chance for seizure) of 9 selected regions obtained from HMC sampling. Red regions indicate highest chance of being the EZ, other areas are in green. The region of the highest EV posterior distribution is the left O2 in red shown in T1-MRI (E) and 3D brain in (F). The two regions (the left lingual gyrus and the left occipital pole) are shown in yellow in (E, F).\n\nretrieved the contribution from a pair of electrodes, in which the perturbation is applied to the brain regions based on the sensor-to-source mapping matrix [15]. Then we calculated the effect of the bipolar pulse stimulation (50 Hz for a duration of 3.5 s on bipolar GL’5-6 electrode leads) on each vertex of the cortex mesh (Fig. 3A). We used the Epileptor-Stimulation model on each of the 20,284 vertices. The stimulation of the Epileptor leads to an accumulation in a state variable \\( m \\) that pushes the brain to seize (supplementary Fig. A2). The seizures were located around the left O2 regions. From these simulated neural source signals (Fig. 3B and Movie S1), we obtained\nSEEG signals (Fig. 3C) using the source-to-sensor gain matrix while considering the orientation of dipoles.\n\nThese synthetic SEEG recordings (Fig. 3C) were used for model inversion, to estimate the EZN. We obtained the left O2 with the highest EVs out of all the samples according to the posterior distribution from the HMC algorithm (Fig. 3D). The two neighboring regions (the left-lingual-gyrus and the left-occipital-pole) were the second-group of candidates that could belong to the EZN. The heatmap projected on the patient’s T1-MRI revealed the spatial mapping of the EZN (sagittal, axial and coronal view images shown in Fig. 3E). The spatial mapping of these three regions in 3D brain is highlighted in red and yellow in Fig. 3F.\n\n2.3 Virtual brain twins for TI stimulation\n\nWe demonstrate now how the pipeline works on TI stimulation. First, we used high resolution modeling for TI stimulation. We calculated the TI electric field, which is projected onto the cortical surface by stimulating two pairs of scalp-EEG electrodes PPO3-P5h and PPO5-PO5h [28] in Fig. 4A) at the frequencies of 1000 Hz and 1005 Hz, respectively. The stimulation amplitude is determined based on the assumption that the components of the field that have the greatest impact are those that are parallel to the neurons’ axons [29]. We used the amplitude of the TI electric field as input to the Epileptor model on each vertex of the cortical mesh (supplementary Fig. A3). We simulated the brain source signals on each vertex of the whole brain by considering both global and local connectivity (Fig. 4B and Movie S2). We then mapped the activities from the vertices of the cortical surface onto the scalp-EEG signals (Fig. 4C) using the source-to-sensor mapping matrix.\n\nWe extracted the data features from these synthetic scalp-EEG recordings (Fig. 4C) as input to the HMC model inversion to estimate the epileptogenic zone. From the posterior distribution of EVs, we obtained the left O2 as first and the left O1 as the second candidate belonging to the EZN (Fig. 4D). The heatmap of these two regions projected on the patient’s T1-MRI shows the spatial mapping of the EZN (sagittal, axial and coronal view images shown in Fig. 4E) and the 3D brain in Fig. 4F, where the left O2 is in red and the left O1 in yellow.\n\n2.4 Multimodal inference\n\nFor patients with multiple seizure recordings or simultaneous multiple modality recordings (here we used SEEG and scalp-EEG as examples), we integrate both modalities into the model inversion algorithm to combine their information in the parameter\nFig. 4 Estimating EZN from TI stimulation induced seizure. (A) The electric field of TI stimulation by two pairs of scalp-EEG electrodes (shown in red and orange) based on the 10-5 international reference system, using an extended scalp-EEG cap from SIMNIBS [28]. We applied a frequency of 1000 and 1005 Hz for the first and second electrode pairs, respectively. The spatial distribution of the peak activity of the TI envelope is colored in the 3D brain. (B) Seizure dynamics were simulated using the Epileptor-Stimulation model through the TI stimulation. Neural activity is shown on the cortical mesh at 6 different time points. The seizures are located around the left O2 regions of the VEP atlas. (C) Selected simulated scalp-EEG time-series from TI stimulation-induced seizure. The scaled-up time series during the seizure period is shown in red. (D) Posterior distribution of the EV (higher value indicates higher chance for seizure) for 10 selected regions obtained from the HMC sampling. Red regions indicate highest chance of being the EZN; the others are in green. The region of the highest EV posterior distribution is the left O2 in red shown in T1-MRI (E) and 3D brain in (F). The second region (Left O1) is shown in yellow in (E, F).\n\nestimation process and potentially improve clinical decision making. Here we demonstrated two cases in which the EZN estimation from multimodal functional recordings were integrated. The first case estimated the EZN from simultaneous scalp-EEG and SEEG recordings under SEEG stimulation (Fig. 5A and supplementary Fig. A4A). Here we mapped the same source signals to both the SEEG and scalp-EEG sensors in both the simulation and during model inversion. Two added values come about as a result of doing simultaneous SEEG and scalp-EEG. First, the scalp-EEG provides\nFig. 5 Multimodal inference for EZN estimation from simultaneous SEEG and scalp-EEG recordings. (A) We combined ictal recordings from SEEG (middle top) and scalp-EEG (middle bottom) induced by SEEG stimulation (left), using multimodal inference to obtain the distribution of EVs (right top). The results were mapped in 3D. In this case, we obtained the ground-truth left O2 in red. (B) We combined ictal recordings from SEEG (middle top) and scalp-EEG (middle bottom) induced by TI stimulation (left), using multimodal inference to obtain the distribution of EVs (right top). The results were mapped in 3D. In this case, we obtained the ground-truth left O2 in red and additional brain region as left STS-posterior in yellow.\n\na whole brain sampling although it mainly measures weak cortical surface signals in contrast to the SEEG, which only samples partial brain space with relatively strong signals from deep structures as well. Second, this pipeline provides a way to evaluate the roles of the scalp-EEG so that we could design a less invasive SEEG implantation in the future. The posterior of the EVs from a simultaneous model inversion showed the left O2 as the EZ (Fig. 5A). The second case estimated the EZN from simultaneous scalp-EEG and SEEG recordings under TI stimulation (Fig. 5B and supplementary Fig. A1B). The posterior of the EVs from the multimodal model inversion showed the left O2 as the EZ and the left STS-posterior as a second candidate.\n\nFor complement of the cases, we utilized the multimodal model inversion module on SEEG recordings from SEEG stimulation (Fig. 5A) and scalp-EEG recording from\nTI stimulation (Fig. 5B) in the supplementary material. The posterior of the EVs from the multimodal model inversion showed the left O2 as the EZ (supplementary Fig. A4C). Notice that, in this case, the functional SEEG and scalp-EEG data here were not simultaneous recorded. The SEEG and TI stimulation generated the seizures with different initial conditions. Then results would be valid only with an assumption that the HMC sampled all feasible initial conditions. For comparison, in the forth case, we pooled the posterior distributions of the EVs from the SEEG (in Fig. 3D under SEEG stimulation) with the EVs from the scalp-EEG (in Fig. 4D under TI stimulation). We obtained the left O2 as the intersection of the two distributions to be the only brain region in the EZN (supplementary Fig. A4D).\n\n2.5 Validation of the pipeline\n\nTo validate that the pipeline can be easily used in other patients, we added the results of a second patient with left frontal lobe epilepsy. The patient underwent resective surgery resulting in seizure freedom (surgery outcome class of Engel I [27]). Eight brain regions including the orbito frontal, anterior-cingulate, F1 lateral prefrontal, F2 rostral, SFS rostral, frontal pole and F1-mesial-prefrontal cortex in the left hemisphere were resected. We built the high-resolution whole-brain model for two types of perturbations under the hypothesis that the left F1 lateral prefrontal is the EZ. To model direct electrical stimulation by SEEG electrodes in the brain, we calculated the effect of the bipolar pulse perturbation (50 Hz, for a duration of 3 s on bipolar PM’3-4 electrode leads) (Fig. 6A). The seizure was induced around the left F1 lateral prefrontal cortex. From the simulated neural source signals (Fig. 6B and Movie S3), we obtained simultaneous SEEG and scalp-EEG signals (Fig. 6C) using the source-to-sensor gain matrix. These synthetic SEEG and scalp-EEG signals during ictal period served as input for multimodal inference to estimate the EZN. We obtained the left-F1-lateral-prefrontal cortex as the region with the highest EV from the HMC algorithm (Fig. 6D,E). The two neighboring regions (the left-F1-mesial-prefrontal and the left-middle-frontal-sulcus) were identified as secondary candidates that could belong to the EZN (Fig. 6D,E).\n\nWe also illustrated the results of this frontal lobe epilepsy patient with TI stimulation in Fig. 7. First, we used high resolution modeling to simulate TI stimulation. We calculated the TI electric field, which is projected onto the cortical surface by stimulating two pairs of scalp-EEG electrodes FPz-AF3 and AFz-Fp1 in Fig. 7A) at the frequencies of 1000 Hz and 1005 Hz, respectively. The brain source signals on each vertex of the whole brain is shown in (Fig. 7B and Movie S4). We then mapped the\nFig. 6 Estimating EZN from SEEG stimulation for a second patient with frontal lobe epilepsy. (A) PM’3-4 (large blue/red sphere) is the stimulated contact in the left frontal lobe, using a bipolar pulse stimulation (50 Hz for a duration of 3 s with pulse duration 1ms) (Top). The spatial mapping of the maximum of stimulation values (shown in the colorbar from low (left) to high (right) values) for each vertex of the brain from sensor PM’3-4 (bottom). (B) Seizure dynamics were simulated using the Epileptor-Stimulation model and induced through SEEG stimulation. Neural activity is shown on the cortical mesh at 5 different time points. (C) Selected simulated SEEG time-series (top) and EEG time-series (bottom) from SEEG stimulation-induced seizure. The scaled-up time series during the seizure period is shown in red. (D) Posterior distribution of EVs (higher value indicates higher chance for seizure) for 8 selected regions obtained from the HMC sampling when analyzing simultaneously SEEG and scalp-EEG. (E) The highest chance of being the EZN as left-F1-lateral-prefrontal in red mapped in 3D brain and left-F1-mesial-prefrontal cortex and left-middle-frontal-sulcus in yellow.\n\nneural activity from the cortical surface onto the SEEG and scalp-EEG electrodes (Fig. 7C) using the source-to-sensor mapping matrix. We extracted the data features from simultaneous ictal synthetic SEEG and scalp-EEG recordings (Fig. 7C) which served as the input to the multimodal inference to estimate the EZN. We obtained the left middle frontal cortex as the region with highest EVs from all samples (Fig. 7D),\nFig. 7 Estimating EZN from TI stimulation for a second patient with frontal lobe epilepsy. (A) The electric field of TI stimulation by two pairs of scalp-EEG electrodes (shown in red and orange). We applied a frequency of 1000 and 1005 Hz for the first and second electrode pairs, respectively. The Spatial distribution of the peak activity of the TI envelope is colored in the 3D brain. (B) Seizure dynamics were simulated using the Epileptor-Stimulation model through the TI stimulation. Neural activity is shown on the cortical mesh at 4 different time points. (C) Selected synthetic SEEG time-series (top) and scalp-EEG time-series (bottom) from TI stimulation-induced seizure. The scaled-up time series during the seizure period is shown in red. (D) Posterior distribution of the EV (higher value indicates higher chance for seizure) for 8 selected regions the same as Fig. 6 D. (E) The highest chance of being the EZN as left-middle-frontal-sulcus in red mapped in 3D brain and left-F1-lateral-prefrontal and left-orbito-frontal-cortex in yellow.\n\nshown in red in 3D in Fig. 7E). The left F1-lateral prefrontal and left-Orbito-frontal-sulcus were identified as the second candidates belonging to the EZN (Fig. 7D) and are shown in yellow in Fig. 7E.\n3 Discussion\n\n3.1 Summary\n\nWe developed a virtual brain twins pipeline tailored for stimulation based on personalized whole brain network modeling in epilepsy. This pipeline integrates empirical patient data and undergoes validation using simulated data generated from high-resolution network models. They are able to explore stimulation effects. Moreover, the proposed pipeline employs model inversion through HMC and Bayesian inference to estimates EZNs. We demonstrated the estimation of the EZN from SEEG and scalp-EEG signals during seizure activity triggered by direct electrical SEEG or TI stimulation. We introduced multimodal inference integrating multiple, potentially simultaneous, modalities as well. The virtual brain twins pipeline for stimulation provides a directly applicable methodological and conceptual basis for a series of scientific studies and clinical translations. The concept of virtual brain twins from this pipeline can be extended to other brain disorders, such as Alzheimer’s and psychiatric disorder, among others [17]. In the subsequent discussion, we will delve into its methodological and conceptual implications for practical applications.\n\n3.2 Application: Ongoing scientific studies\n\nThe first application of this pipeline can help us answering a crucial diagnostic question: How to infer the underlying EZNs from stimulated seizures? To answer this question, it is necessary to investigate the following problems, illustrated in supplementary Fig. A5. First, what is the proper range of stimulation parameters to induce seizures for diagnosis? Currently, no standardized stimulation protocols exist [20]. The French guidelines suggest parameters for both low-frequency (1 Hz) and high-frequency (50 Hz) stimulation with specified ranges on pulse width, pulse intensity and stimulation duration [3]. Our personalized whole brain model has the ability to predict the stimulation effect for individual patients given specified stimulation parameters and should be validated in future empirical studies. On the patient-specific level, among the proper range of stimulation parameters, then what are the optimal stimulation parameters for inducing seizures for diagnosis? Second, what is the relationship between the EZN triggered by stimulation and the one occurring during spontaneous seizures? More specifically, we want to investigate whether the EZN estimated from stimulation induced seizures equals the EZN of spontaneous seizures. It could be possible that stimulation forces seizures in brain regions that would not be epileptogenic otherwise, or that stimulation uncovers only a subset of epileptogenic regions. Even\nfor spontaneous seizures, we have to remember that the limited observations of recordings of spontaneous seizures may also only tell part of the story. Third, how many induced seizures by SEEG stimulation are sufficient for identifying the full underlying EZN? We can investigate this question by systematically evaluating the EZNs on SEEG stimulated induced seizures generated by virtual brain twin models with given EZNs. The proposed VEP stimulation pipeline with high-resolution modeling provides a reasonable framework as a useful tool to address all these questions.\n\nThe proposed virtual epilepsy patient pipeline has the capability to integrate multimodal neuroimaging data, including anatomical recordings, such as T1-weighted MRI, diffusion-weighted MRI, and CT; as well as functional ones, such as scalp-EEG, MEG, SEEG, subdural grid, PET and fMRI. The framework that we introduced here takes this process further and the multimodal inference demonstrates possible approaches to integrate information from scalp-EEG and SEEG. This process can be easily extended to other recordings, such as MEG, fMRI, and subdural grid electrodes, depending on the available data. The only difference between the different functional measures is the forward solution matrix. We designed an multimodal inference version of the HMC algorithm, which can be directly used for simultaneous functional recordings, such as SEEG/scalp-EEG [30] or MEG/scalp-EEG [31] or SEEG/MEG [32]. The proposed pipeline also provides a basic structure for estimating the EZN using interictal spikes as a datafeature from interictal SEEG/MEG recordings. The usage of this multimodal inference is also valid in cases where different recordings start with the same brain states, or when the sampling algorithms can cover all possible initial conditions.\n\nThe diagnostic pipeline for TI stimulation can provide a theoretical basis for non-invasive diagnosis and treatment of epilepsy. TI stimulation is a good candidate for both diagnosis and treatment in epilepsy within the non-invasive stimulation family. Other non-invasive stimulation techniques, such as tDCS [33], are mostly used for treatment only in epilepsy. The key feature of TI stimulation is that it enables a focused stimulation which can reach deep brain structures non-invasively [24, 34], such as the hippocampus, which quite often is involved in the EZN in temporal lobe epilepsy. Studies have demonstrated the safety of TI in human participants [35]. Literature and seminars with preliminary results have started to discuss the application of TI stimulation to brain disorders, such as epilepsy [23, 36], Alzheimer’s [37], Parkinson’s [38] and essential tremor [39]. TI stimulation has evoked seizure-like events in the mouse hippocampus that have been experimentally well controlled [40]. Our study provides a pipeline for predicting the use of TI for the diagnosis of the EZN in human epilepsy, and is a basis for an optimization strategy for TI stimulation. Based on\nthis proposed framework, we can further build high resolution models for individual patients in future therapeutic interventions. Although we obtained a good estimate of the EZN from non-invasive scalp-EEG signals for patient examples whose EZNs were in cortical regions, for in deep structures, we are exploring the non-invasive measure approach that can record useful data features from these deep brain structures.\n\n3.3 Limitations\n\nThe current pipeline has several limitations. Model-based approaches are usually computationally expensive and parameter sensitive, which may pose challenges for real-time use in clinical routine, such as the optimization of stimulation parameters. The current pipeline does not consider the dynamics of the epileptic disorders over long timescales nor the long-term effects of the stimulation. Ongoing systematic evaluations and studies will also improve the current pipeline in the following ways. High-resolution modeling of the subcortical structure and a more realistic forward resolution may improve the whole brain modeling. The introduction of regional variations (such as cell density and receptor density) [41, 42] may provide a fundamental way to improve the current pipeline.\n\n4 Methods and Materials\n\n4.1 Patient data\n\nWe used the data from two patients who underwent a standard presurgical protocol at La Timone Hospital in Marseille. Informed written consent was obtained in compliance with the ethical requirements of the Declaration of Helsinki and the study protocol was approved by the local Ethics Committee (Comité de Protection des Personnes sud Méditerranée 1). This patient underwent a comprehensive presurgical assessment, which included medical history, neuropsychological assessment, neurological examination, fluorodeoxyglucose positron emission tomography, high-resolution 3T MRI, long-term scalp-EEG and invasive SEEG recordings. The patient received non-invasive T1-weighted imaging (MPRAGE sequence, repetition time = 1.9 s, echo time = 2.19 ms, voxel size \\(1.0 \\times 1.0 \\times 1.0\\ mm^3\\)) and diffusion-weighted MRI images (with an angular gradient set of 64 directions, repetition time = 10.7 s, echo time = 95 ms, voxel size \\(1.95 \\times 1.95 \\times 2.0\\ mm^3\\), b-weighting of 1000 \\(s/mm^2\\)). The images were acquired on a Siemens Magnetom Verio 3T MR-scanner. The patient had invasive SEEG recordings obtained by implanting multiple depth electrodes, each containing 10–18 contacts 2 \\(mm\\) long and separated by 1.5 or 5 \\(mm\\) gaps. The SEEG signals were\nacquired on a 128 channel Deltamed/Natus system. After the electrode implantation, a cranial CT scan was performed to obtain the location of the implanted electrodes.\n\n4.2 Data processing\n\nTo construct the individual brain network models, we first preprocessed the T1-MRI and diffusion-weighted MRI data. Volumetric segmentation and cortical surface reconstruction were from the patient-specific T1-MRI data using the recon-all pipeline of the FreeSurfer software package http://surfer.nmr.mgh.harvard.edu. The cortical surface was parcellated according to the VEP atlas [26], the code for which is available at https://github.com/HuifangWang/VEP_atlas_shared.git. We utilized the MRtrix software package to process the diffusion-weighted MRI [43], employing the iterative algorithm described in [44] to estimate the response functions and subsequently used constrained spherical deconvolution [45] to derive the fiber orientation distribution functions. The iFOD2 algorithm [46] was used to sample 15 million tracts. The structural connectome was constructed by assigning and counting the streamlines to and from each VEP brain region. The diagonal entries of the connectome matrix were set to 0 to exclude self-connections within areas and the matrix was normalized so that the maximum value was equal to one. We obtained the location of the SEEG contacts from post-implantation CT scans using GARDEL (Graphical user interface for Automatic Registration and Depth Electrodes Localization), which is part of the EpiTools software package [47]. Then we coregistered the contact positions from the CT scan space to the T1-MRI scan space for this patient.\n\n4.3 High resolution simulation of the Epiletor-Stimulation model\n\nWe modeled epileptic seizures on a patient-specific high-resolution brain model. Although there is no consensus about the precise biophysical mechanism of ion exchanges that leads to seizure onset. Previous studies demonstrated an increase in excitability, spike frequency and oscillation power [48–51] when an external perturbation was applied. Experimental studies have linked seizure onset to specific changes in ion dynamics such as extracellular potassium or intracellular chloride [52–54]. We hypothesized that exposure of repetitive stimulation/pertubation generates a slow accumulation effect, which can push the system to the seizure state when a seizure threshold is reached.\n\nWe model this accumulation effect phenomenologically via the parameter \\( m \\), which influences the oscillatory dynamics in the seizure onset state in the Epiletor model\n[55, 56]. We render \\( m \\) time dependent, \\( m = m(t) \\), and introduce an exponentially decaying memory kernel of length \\( r \\) through a linear ordinary differential equation, which slowly builds up when an external stimulus is applied until the seizure threshold is reached. In the absence of a stimulus, \\( m(t) \\) slowly returns back to baseline. \\( H \\) is the Heaviside function. When \\( m \\) is greater than the seizure threshold \\( m_{thresh} \\), the \\( H \\) function equals 1, which kicks the system into the seizure-like state. Otherwise, the \\( H \\) function equals 0.\n\nThe pial surfaces of both hemispheres define the spatial domain along which the network activity can unfold. Neural dynamics are governed by an extension of the original Epiletor model [25]. The extended Epiletor-Stimulation model includes a stimulation-accumulating state variable \\( m \\) that can destabilize the system and produce a seizure. The neural activity at every vertex \\( i = 1, ..., N \\) of the network is governed by the following equations:\n\n\\[\n\\dot{x}_i = y_i - f_1(x_i) - z_i + I_{ext} + I_{stim} +\n\\gamma_{hom} \\sum_{j=1}^N S(g_{i,j})H(x_j, \\theta_{hom}) + \\gamma_{het} \\sum_{l=1}^L W_{k,l}H(X_l, \\theta_{het})\n\\]\n\\[\n\\dot{y}_i = c - dx_i^2 - y_i\n\\]\n\\[\n\\dot{z}_i = r(4(x_i - x_0 + nH(m_i - m_{thresh})) - z_i) + f_2(z_i)\n\\]\n\\[\n\\dot{m}_i = r(I_{stim} - m_i)\n\\]\n\nwhere:\n\n\\[\nf_1(x) = \\begin{cases}\nax^3 - bx^2 & \\text{if } x < 0 \\\\\n-(m + 0.6(z - 4)^2)x & \\text{if } x \\geq 0\n\\end{cases}\n\\]\n\\[\nf_2(z) = \\begin{cases}\n-0.1z^7 & \\text{if } z < 0 \\\\\n0 & \\text{if } z \\geq 0\n\\end{cases}\n\\]\n\\[\nH(x, \\theta) = \\begin{cases}\n1 & \\text{if } x \\geq \\theta \\\\\n0, & \\text{if } x < 0\n\\end{cases}\n\\]\n\\[\nS(x) = \\frac{1}{2}e^{-|x|}\n\\]\n\nThe state variables \\( x \\) and \\( y \\) describe the activity of neural populations on a fast time scale and can model fast discharges. The oscillation of the slow permittivity variable \\( z \\) drives the system autonomously between ictal and interictal states. The parameter\n\\( x_0 \\) indicates the degree of excitability and directly controls the dynamics of the neural population to produce seizures or not. Each vertex \\( i \\) is connected locally through homogeneous connections and globally through heterogeneous connections to other parts of the brain. Although local connections are actually heterogeneous with a complex variability of interneurons and dendritic arborization, due to lack of personalized measurement in clinical routines, we made an assumption of homogeneity in the local connections while considering only geometric features of the cortical surface. Local connections, parameters with the subscript \\( hom \\), are described by a translationally invariant Laplacian coupling kernel \\( S(g_{i,j}) \\) where \\( g_{i,j} \\) denotes the geodesic distance along the cortical mesh between vertices \\( i \\) and \\( j \\). Additionally, global connections, parameters with the subscript \\( het \\), along white matter fibers, are accounted for by the connectome matrix, where \\( W_{k,l} \\) is the connection strength between brain areas \\( k \\) and \\( l \\). Each vertex \\( i \\) is assigned to a brain area \\( k = 1,...,L \\) according to a cortical parcellation. For this study we used the VEP parcellation. The average neural activity \\( X_l \\) of all vertices belonging to area \\( l \\) is coupled throughout the network and projected uniformly to all vertices of area \\( k \\). The default parameters of the system are \\( I_{ext} = 3.1, c = 1, d = 5, r = 1, a = 1, n = 1, m_{thresh} = 1.8, \\gamma_{het} = 0.1, \\gamma_{hom} = 0.8, \\theta_{het} = -1, \\theta_{hom} = -1 \\). The time varying input \\( I_{stim} \\) describes the perturbation signal in each time step depending on stimulation parameters. To accomplish this, we computed the generated electric field from the two types of perturbation a) an invasive SEEG stimulation, and b) a non-invasive TI stimulation. These are described in two separate subsections below.\n\n4.4 Calculation of the electric field of SEEG stimulation\n\nThe SEEG stimulation is applied to a pair of neighboring sensors, in which one acts as a cathode and the other one as an anode. This generates a bipolar pulse perturbation in the area where the electrodes are located. However, the effects of the stimuli are not only local, because they can propagate through short-range and long-range connections towards other brain areas. The parameters used clinically are restricted to frequencies of either 1 Hz or 50 Hz, weak amplitudes ranging from 0.1 to 3 mA, and pulse widths of 500 – 2000 microseconds. We modeled the same stimulus as had been applied clinically on a personalized digital brain model of the patient. Using the reconstructed brain structure and the overlayed SEEG electrodes, we generated a biphasic signal using the stimulation parameters for the pair of electrodes chosen by the clinician. We then mapped the stimulus signal onto the parcelated brain areas based on the distance, which resulted in an estimated electric field across the brain regions. We used this\nestimated field as an input to the \\( I_{stim} \\) parameter and simulated the time series on selected vertices from the EZ.\n\n4.5 Calculation of the electric field of the TI stimulation\n\nNon-invasive stimulation with TI is a recent method that aims to mimic DBS’s capabilities to be both focal and sub-cortical without being invasive. This is done using the assumption that high frequencies (above 500 Hz) have an ignorable effect on neuronal activity [24, 34]. By combining multiple fields of very high-frequency tACS stimulations, such that they interfere maximally in the target of choice, a new electric field can be generated, which modulates at much lower frequencies (e.g. two fields of 1000 and 1050 Hz modulate at 50 Hz at the target of choice). The generated electric field was computed using SimNIBS, as described previously, to compute the generated tACS fields. Then, the vectorial tACS fields are added together, resulting in a TI field estimate for the brain regions. We used this estimated field as an input to the \\( I_{stim} \\) parameter and simulated the time series on one selected vertex from the EZ.\n\nTo obtain the distribution of the TI field in the gray matter, we started by computing the electric field distribution from the simulation of a transcranial direct current stimulation (tDCS) via SimNIBS [57]. First, we reprocessed the individual T1-weighted MRI via the SimNIBS process “mri2mesh”, which resulted in the segmentation into five head tissues: white and grey matters, cerebrospinal fluid, skull and scalp. This process creates the tetrahedral meshes necessary for the finite element method (FEM) for the simulation of the electric field distribution. We computed the tDCS field for each pair of electrodes positioned based on the location of the coregistered 128 electrodes scalp-EEG cap, using the 10-5 system. Circular electrodes with a diameter of 10 mm and a thickness of 5 mm were directly applied on the head. Then, we projected these electric fields onto the resampled Freesurfer surface (20484 vertices). We extracted the amplitude of the electric field at each vertex of the cortex surface. These fields derived from the coupled electrodes pairs were then modulated by multiplying them with two sinusoids with the frequency of 1000 Hz and 1005 Hz, respectively, for 1 second. Two oscillatory electric fields, which were linearly summed, provided an interference field. To obtain a correct representation of the high frequency activity, the sampling rate was 30 kHz. We extracted the 5 Hz peak envelope by using spline interpolation. Finally, we included this envelope in the virtual brain model as the source of external simulation for the cortex vertices (20484). For this patient, we targeted the highest TI stimulation effect on the left O2 in the VEP atlas [26]. We used the optimization process in SimNIBS to identify the best 4 electrodes configurations (10-5 scalp-EEG\nmontage), which maximized the electric field in the left O2. This procedure allowed us to identify, in our case, PPO3-PPO5 and P5h-PO5h ([28]) as the best electrodes couple for the left-O2 stimulation.\n\n4.6 Forward solution for SEEG signals\n\nThe forward solution for the SEEG signals maps the neural activity from the sources to the sensors (SEEG contacts), represented by a source-to-sensor matrix (gain matrix). As sources for our model, we used the vertices of the pial surface for the cortical regions, and each subcortical region as a single node as in the neural mass model (NMM). Surfaces are represented as triangular meshes. For the NMM, we defined the mapping \\( g_{j,k} \\) from the source brain region \\( j \\) to the sensor \\( k \\) as the sum of the inverse of the squared Euclidean distance \\( d_{i,k} \\) from vertex \\( i \\) to sensor \\( k \\), weighted by the area \\( a_i \\) of the vertex on the surface.\n\n\\[\ng_{j,k} = \\sum_{i=0}^{N_j} a_i / d_{i,k}^2\n\\]\n\nHere vertex \\( i \\) belongs to region \\( j \\) which has \\( N_j \\) vertices in total. The area \\( a_i \\) of vertex \\( i \\) was obtained by summing up one third of the area of all the neighboring triangles. Vertices belonging to the same brain region were summed to obtain the gain for a single region of our brain network model. The resulting gain matrix has dimensions \\( M \\times N \\), with \\( M \\) being the number of regions and \\( N \\) the number of sensors.\n\nMatrix multiplication of the simulated source activity with the gain matrix yielded the simulated SEEG signals, i.e., \\( SEEG_k(t) = \\sum_j g_{j,k} x_j(t) \\), where \\( x_j(t) \\) is the time series of the source level signals. This distance-based approach and the summation of all the vertices within each region neglect the orientation of the underlying current dipoles. Pyramidal neurons, which are oriented normal to the cortical surface, are assumed to be the physiological source of any electric signal recorded with SEEG, scalp-EEG, or MEG [58]. The direction of the NMM is ill defined at typical spatial resolutions of 10-20 \\( cm^2 \\) in virtual brain networks of 100-200 nodes [26]. However, approaches that use high resolution representation of the network, allowing to compute an surface orthogonal, have this ability. To solve the forward problem we followed the analytical solution proposed in [59] for electric fields in an unbounded homogeneous medium. This choice of forward model assumes no boundary effects of changes of conductivity at tissue boundaries. A previous study has shown that the error of an unbounded homogeneous conductivity model compared to a more accurate finite element method model with changes in conductivity is relatively small for electric\nfields generated by dipoles deep in the brain and electrodes close to the source [60]. Therefore, we can estimate the gain matrix elements \\( g_{i,k} \\) for the NMM approach by\n\n\\[\ng_{i,k} = a_i / 4\\pi \\sigma Q * (r_k - r_i) / (|r_k - r_i|^3)\n\\]\n\nwhere \\( r_k \\) and \\( r_i \\) are the position vectors of sensor \\( k \\) and source vertex \\( i \\), respectively. \\( |v| \\) represents the L2 norm of a vector \\( v \\). \\( Q \\) is the dipole orientation vector, and \\( \\sigma \\) is the electric conductivity. Since we assume constant conductivity across the brain, it becomes merely a scaling factor, which we set to \\( \\sigma = 1 \\).\n\n4.7 Forward solution for scalp-EEG signals\n\nTo compute the forward solution of scalp-EEG signals, we first reconstructed three individual surfaces (inner skull, outer skull, and head) of the patient based on boundary element models (BEM) using Brainstorm [61]. Then in Brainstorm, we coregistered the scalp-EEG electrodes positions (of the Hydrocel E1 128 channels electrode cap) onto the head surface, according to the fiducial points of the patient’s T1-MRI. We applied a slight manual correction to better orient the scalp-EEG cap to the individual anatomy. Finally, we derived an scalp-EEG forward model using a 3-shell BEM model (conductivity: 0.33, 0.165, 0.33 S/m; ratio: 1/20) [62] and the OpenMEEG method implemented in Brainstorm [63, 64], to provide a realistic head model. Then we obtained a gain value for each dipole (20484 vertices), with the constrained direction normal to the cortex surface, for each scalp-EEG electrode. Finally, the gain matrix derived from the head model was multiplied by the simulated time series of the brain sources to obtain the scalp-EEG activity, i.e. \\( EEG_l(t) = \\sum_j g_{j,l}^{EEG} x_j(t) \\), \\( g_{j,l}^{EEG} \\) from the source signal on brain region \\( j \\) to the \\( EEG \\) signal on channel \\( l \\).\n\n4.8 Calculation of the SEEG/scalp-EEG data features\n\nWe extracted the data features from the SEEG and scalp-EEG signal to be the input of the model inversion modules. The SEEG data was re-referenced using a bipolar montage, which was obtained using the difference between 2 neighboring contacts on one electrode. The 2D Epileptor model, introduced below, is suitable for fitting the envelope of the seizure time series. Ideally, the envelope follows a slightly smoothed rectangular function from the onset until the offset of the seizure. To get a well-formed target that our model should fit, we extracted the bipolarized SEEG signal from 10s before the seizure onset until 10s after the seizure offset. We identified the outlier time points that were greater than 2-times the standard deviation of the extracted signal and replaced them with the mean of the extracted signal. The signal was then\nhigh-pass filtered with a cut-off at 10 Hz to remove slow signal drifts. The envelope was calculated using a sliding-window approach with a window length of 100 time points. The signal inside the window was squared, averaged and log transformed. From the resulting envelope, we again identified and removed outliers, as described above. Finally, the envelope was smoothed using a lowpass filter with a cut-off of 0.05 Hz. The mean across the first few seconds of the envelope was used to calculate a baseline, which was then subtracted from the envelope. The same procedure was used for the EEG data, the only difference being that we used absolute values for the gain matrix, in order to get the accumulated effect on each EEG electrode throughout the entire seizure.\n\n4.9 The HMC model inversion\n\nBy taking advantage of time scale separation and using averaging methods, the Epileptor can be reduced to a 2D system [65]:\n\n\\[\n\\dot{x}_i = I_1 - x_i^3 - 2x_i^2 - z_i \\\\\n\\dot{z}_i = (1/\\tau_0)(4(x_i - x_{i,0}) - z_i + K \\sum_{j=1}^{N} C_{i,j}(x_j - x_i))\n\\]\n\nwhere \\( \\tau_0 \\) scales the length of the seizure. The external input is defined as \\( I_1 = 3.1 \\).\n\nWe used the 2D Epileptor for the model inversion, i.e. the parameter estimate of the model, from the scalp-EEG and SEEG recordings.\n\nFor the individual SEEG model inversion, the forward solution is: \\( SEEK_k(t) = \\sum_j g_{j,k} x_j(t) \\). For the individual scalp-EEG model inversion, the forward solution is: \\( EEG_l(t) = \\sum_j g_{j,l}^{EEG} x_j(t) \\).\n\nFor the multimodal model inversion, we projected the same source signals to the scalp-EEG and SEEG at the same time while we calculated the likelihood according to the HMC algorithm, i.e. \\( SEEK_k(t) = \\sum_j g_{j,k} x_j(t); EEG_l(t) = \\sum_j g_{j,l}^{EEG} x_j(t) \\).\n\nFor the model inversion, we applied the No-U-Turn Sampler (NUTS), an adaptive variant of the HMC algorithm to sample the posterior density of the model parameters. The performance of the HMC is highly sensitive to the step size and number of steps in the leapfrog integrator for updating the position and momentum variables in a Hamiltonian dynamic simulation [66]. We used NUTS, which is implemented in Stan and extends HMC with adaptive tuning of both the step size and the number of steps in a leapfrog integration to sample efficiently from the posterior distributions [66, 67]. To overcome the inefficiency in the exploration of the posterior distribution of the model parameters, we used a reparameterization of the model parameters based on the map\nfunction from the model configuration space to the observed measurements [10]. Our reparameterization-based approach reduces the computation time by providing more effective sample sizes and removing divergences by exploring the posterior distributions of the linear combinations of regional parameters that represent the eigenvectors obtained from the singular value decomposition of the gain matrix. We denote the matrix of the eigenvectors of \\( G^T G \\) as \\( V \\) and the new parameters as \\( x_{i,0}^* = V^T x_{i,0} \\) and \\( z_i(t_0)^* = V^T z_i(t_0) \\). We ran the model inversion on both empirical and simulated seizures with 16 chains starting from eight optimized initial conditions. The eight optimized initial conditions are the output of maximum a posterior estimation algorithm [15]. We ran the maximum a posterior estimation algorithm 50 times and selected the best eight results in terms of the likelihood. We assessed model identifiability based on an analysis of posterior samples, which demonstrated that the sampler explores all the modes in the parameter space efficiently. The analysis includes trace-plots (evolution of parameter estimates from draws over the iterations), pair plots (to identify collinearity between variables), and autocorrelation plots (to measure the degree of correlation between draws of samples). 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Biomedical engineering online **9**, 45 (2010).\n\n[64] Kybic, J. *et al.* A common formalism for the integral formulations of the forward eeg problem. IEEE Transactions on Medical Imaging **24**, 12–28 (2005). URL http://ieeexplore.ieee.org/document/1375158/.\n\n[65] Proix, T., Bartolomei, F., Chauvel, P., Bernard, C. & Jirsa, V. K. Permittivity coupling across brain regions determines seizure recruitment in partial epilepsy. Journal of Neuroscience **34**, 15009–15021 (2014). URL http://www.jneurosci.org/cgi/doi/10.1523/JNEUROSCI.1570-14.2014.\n\n[66] Hoffman, M. D. & Gelman, A. The no-u-turn sampler: Adaptively setting path lengths in hamiltonian monte carloo title. Journal of Machine Learning Research **15**, 1593–1623 (2014).\n\n[67] Betancourt, M. A conceptual introduction to hamiltonian monte carlo. arXiv (2017). URL http://arxiv.org/abs/1701.02434.\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• ResultsFiles.zip\n• VEPstimulationsupplementary.pdf\n• videos.zip"} {"paper_id": "prb27", "title": "Wake slow waves in focal human epilepsy impact network activity and cognition", "text": "# Abstract\n\nSlow waves of neuronal activity are a fundamental component of sleep that are proposed to have homeostatic and restorative functions. Despite this, their interaction with pathology is unclear and there is only indirect evidence of their presence during wakefulness. Using intracortical recordings from the temporal lobe of 25 patients with epilepsy, we demonstrate the existence of local wake slow waves (LoWS) with key features of sleep slow waves, including the down-state of neuronal firing. LoWS were distinct from slow waves recorded in people without epilepsy and showed evidence of adaptation during periods of increased normal (cognitive task) and abnormal (interictal epileptiform discharges, IEDs) activity. Importantly, we also provide evidence that LoWS reduce increases in network excitability during IEDs but are associated with poorer memory. We therefore propose an “epilepsy homeostasis hypothesis”: that slow waves are activated in epilepsy to reduce aberrant activity at the price of transient cognitive impairment.\n\nHealth sciences/Neurology/Neurological disorders/Epilepsy \nBiological sciences/Neuroscience/Learning and memory/Hippocampus \nBiological sciences/Neuroscience/Diseases of the nervous system/Epilepsy\n\n# Introduction\n\nDuring non-rapid eye movement (NREM) sleep, neurons undergo slow fluctuations of membrane potential, producing a burst firing mode (up-state) and a suppression of their activity (down-state). This fluctuation is reflected by slow oscillations (0.5-4 Hz) of the local field potential (LFP) termed slow wave activity (SWA, Fig. 1a). SWA is a canonical component of sleep¹,² and has been proposed to be critical for sleep homeostasis³–⁷ (specifically, the normalization of synaptic strength⁶,⁸), metabolic regulation⁹, and metabolic waste clearance in general¹⁰. Elevated sleep pressure, as occurs after a wake period, is reflected by an increased rate, slope and amplitude of sleep slow waves (SWs), which decrease over the course of the night⁴,¹¹–¹⁶ (Fig. 1b). Furthermore, evidence suggests that neuronal synchrony, i.e., the concentration of neuronal firing during the up-state and neuronal silence during the down-state of sleep SWs, favours synaptic normalization⁸,¹¹,¹⁷, and is homeostatically modulated (high after a wake period, low after a sleep period, Fig. 1a)¹².\n\nAs occurs with wakefulness⁴ and cognitive processing³,¹⁸, epileptic activity results in increased synaptic connectivity¹⁹–²¹ and metabolic need²². Consequently, the increased SWA observed during sleep after repetitive seizures has been interpreted as a compensatory mechanism²³–²⁵ which counteracts the increased local metabolic demand, although there is currently no evidence for SW having a beneficial impact on epileptic activity. Furthermore, it is unclear whether such SWA might also appear during wakefulness, although this could constitute a mechanism to offset pathological activity, such as epileptiform discharges and seizures.\n\nHere, using macro- and micro-electrode intracranial recordings from the temporal lobe of people with focal, pharmacoresistant epilepsy, we demonstrate the presence of highly local wake slow waves (LoWS) that recapitulate the core features of sleep slow waves, including the associated down-state of neuronal spiking activity. We hypothesized that these LoWS could serve a homeostatic purpose by normalizing neuronal activity to prevent epileptic discharges, mirroring the function of sleep SWs which correct the excessive neuronal excitability accumulated during wakefulness that translates into high sleep pressure (i.e., sleep homeostasis⁶). If LoWS do serve a homeostatic function, then they should exhibit two key features: first, responding to increases in network activity associated with interictal epileptiform discharges (IEDs); and second, reducing abnormal activity linked with IEDs. In line with this hypothesis, we observed that progressive increases in neuronal activity (estimated by high-gamma (HG) power) before IEDs is paralleled by an adaptation of the slope and amplitude of LoWS, analogous to that observed in the response of sleep SW to increased sleep pressure, i.e., enhanced slope and amplitude¹³,¹⁶. Moreover, the longer the delay since the last LoWS, the higher the HG power during IEDs, suggesting that any protective function of LoWS dissipates with time. Lastly, we found that the higher rate of LoWS during an associative memory task was associated with longer reaction times (RT), supporting the prediction⁵ that the substantial modulation of neuronal activity during SWs¹²,²⁶ impacts cognitive processing. Together, our findings indicate that LoWS with key features of sleep SW dynamically respond to changes in network excitability, reduce aberrant activity associated with IEDs, and impact on cognition. We therefore propose that LoWS represent a homeostatic process that comes at the cost of transient cognitive impairment.\n\n# Results\n\n## Identification of slow waves during wakefulness in patients with epilepsy\n\nWe first asked if we could reliably detect local slow waves during wakefulness in a cohort of people with focal epilepsy (n=17) undergoing intracranial EEG recordings, and then whether such slow waves had key features of sleep slow waves (Fig. 1). We used a validated algorithm for slow wave detection13,26–28 to track their presence in the human hippocampus (mean ± SD of hippocampal contacts = 3.4 ± 1.8, see Extended Data Table 1), while people with focal epilepsy were performing an associative memory task. We excluded any slow waves associated with (i.e., within 1 s of) an IED and took several confirmatory steps to ensure that the identified slow waves were not mislabeled IEDs (see Online Methods).\n\nThe negative and positive components of slow waves, i.e., negative and positive slow waves, were identified (nSW and pSW respectively, Fig. 1c-d). To note, traces are inverted during acquisition, such that negative deflection (nSW) corresponds to positive extracellular potential, and vice versa. Rates of nSW and pSW were similar (effect size [ES] across electrodes expressed as mean difference, 95% CI: 0.002/s/electrode, -0.001 to 0.009, p=0.464, n=17 patients, Extended Data Fig. 1a) and were highly correlated across patients (Pearson correlation, r2=0.79, p<0.0001, n=17, Extended Data Fig. 1b). nSW had a peak (extracellular) positive potential (Fig. 1c-d), which corresponds to a hyperpolarization of neurons. This inactive state is a core feature of, and defines, sleep SW5,26,29. For this reason, we subsequently focus only on the negative component of this slow wave activity (i.e., nSW), except where stated otherwise. nSW occurred at a mean ± SD rate of 0.06/s/electrode ± 0.02 (Extended Data Fig. 1a), well below the rate described during sleep13,27,28. The median oscillatory frequency of nSW, estimated by the delay between the two 0-crossings, was 1.4 Hz (interquartile range, IQR: 1.1-1.7 Hz, n=17,712 hippocampal nSW identified across patients).\n\n## Negative slow waves during wakefulness share key characteristics with sleep slow waves\n\nNext, we determined whether identified slow waves had key characteristics of sleep SW (Fig. 1). Analogous to sleep SW26, nSW were associated with a down-state, as revealed by decreased high-gamma (HG, 45-130 Hz) power averaged between the two 0-crossings of the grand average nSW (-0.15 to 0.165 s around the trough of nSW versus baseline: ES, 95% CI: -0.137, -0.236 to -0.0884, p=0.0004, n=17, Fig. 1e). Using a time-resolved frequency analysis, we confirmed that the decrease in HG power was localized to the nSW trough (Fig. 1f). This was further confirmed through the observation of a decrease in HG power before the peak of pSW (from -0.42 to -0.13 s, Fig. 1g), the timing of which matched the peak of nSW occurrence before pSW in our data (around -0.36 s, Fig. 1g, i). Importantly, the peak of HG associated with IEDs was significantly higher than that during pSW (ES, 95% CI: 4,490 µV2, 2,680-7,250, p=0.0008, Extended Data Fig. 2a), arguing against a mislabeling of the two events (see Online Methods for further confirmation analyses).\n\nIn the time domain, identified nSW occurred mainly as isolated events, with only 9-10% of nSW being preceded or followed by a pSW (with a delay of ± 0.37 s, Fig. 1h). The same analysis for pSW gave, as expected, a similar result (Fig. 1i). This suggests that nSW were mainly preceded and followed by positive deflections that either did not reach the amplitude or the frequency criteria for pSW (see Online Methods), and vice versa. In the spatial domain, nSW were mainly focal since the presence of a slow wave on one hippocampal contact was accompanied by a slow wave on only 27% of the other hippocampal contacts (Extended Data Fig. 3a). This microfocality was less pronounced in the amygdala (49%, Extended Data Fig. 3b) and more pronounced in the temporal neocortex (18%, Extended Data Fig. 3c), which could reflect differences in the volume and coverage of these brain regions. Similarly, the detection of a slow wave in the hippocampus, amygdala or temporal neocortex was accompanied, on average, by the detection of a slow wave in at least one of the other regions in only 24% of cases (Extended Data Fig. 3d), remarkably close to the percentage observed for sleep SW26. Slow wave incidence rates were similar in the hippocampus, amygdala, and temporal neocortex (Extended Data Fig. 3e). Given the highly focal nature of detected nSW, we subsequently refer to them as local wake slow waves (LoWS).\n\n## LoWS are associated with a down-state of neuronal firing, capturing a core feature of sleep slow waves\n\nTo confirm that the decrease in HG power during the LoWS trough corresponds to decreased neuronal activity, we examined LoWS in a separate cohort of patients who underwent hippocampal microelectrode implantation (n=8 patients) and identified unit spiking activity (see Online Methods and Fig. 2a). We observed a significant decrease in unit activity locked to the trough of LoWS (paired bootstrap statistic followed by false discovery rate correction across time bins, p<0.05 from -0.049 to 0.147 s, Fig. 2b). The maximal decrease of neuronal firing occurred just after the trough (Fig. 2a-d), as previously described for sleep slow waves in the hippocampus26. At this time point, > 50% of identified units in all 8 patients showed a decrease in firing rate (mean ± SD = 78 ± 17%, one sample t-test, p=0.0024, Fig. 2c, n=8). Similarly, a comparison of normalized mean firing rates between the two 0-crossings of the grand average LoWS versus baseline confirmed that the decrease was significant (ES, 95% CI: -0.273, -0.455 to -0.0795, p=0.0368, n=8, Fig. 2e blue lines). Conversely, we found only non-significant trends in the modulation of neuronal activity around pSW (red lines in Fig. 2e) and IEDs (Extended Data Fig. 2b). In sum, neuronal activity shows a significant decrease shortly after the trough of LoWS during wakefulness, confirming the presence of this core feature of sleep slow waves in LoWS.\n\n## LoWS that occur in focal epilepsy are distinct from those in non-epileptic patients\n\nWe next determined if LoWS were unique to our cohort or also present in other cohorts of patients with focal epilepsy. We took advantage of an independent, publicly available dataset from patients with focal epilepsy undergoing intracranial recordings30 (from Boran et al., 2020, referred to as the “Boran dataset” below) and detected similar wake slow waves in the hippocampus (see Online Methods), although they occurred less frequently (Boran dataset versus UCL dataset, ES, 95% CI: 0.0294/s/electrode, 0.0164-0.0398, p=0.0004, n=9 and 17 patients respectively, Extended Data Fig. 4a, c).\n\nWe further asked whether such LoWS were a feature of focal epilepsy or a ubiquitous phenomenon. Since it was not possible to obtain intracortical, mesial temporal lobe recording in healthy subjects, we examined a dataset of neocortical, electrocorticographic (ECoG) recordings in awake patients with Parkinson’s disease31 using the same detection algorithm. Slow waves in wakefulness were also detected in the Parkinson’s disease patients but were rarer than in either epilepsy cohort (UCL dataset versus Parkinson’s dataset, ES, 95% CI: 0.04/s/electrode, 0.03-0.05, p<0.0001, n=17 and n=16 patients respectively; Boran dataset versus Parkinson’s dataset, ES, 95% CI: 0.01/s/electrode, 0.005-0.02, p=0.0138, n=9 and 16 patients respectively, Extended Data Fig. 4b-c).\n\nMoreover, LoWS in the Parkinson’s dataset were less easily detectable from background LFP (i.e., had a significantly lower signal to noise ratio) than those in either epilepsy cohort (Parkinson’s dataset versus Boran dataset, ES, 95% CI: 1.05, 0.761-1.31, p<0.0001; Parkinson’s dataset versus UCL dataset, ES, 95% CI: 1.15, 0.862-1.43, p<0.0001; Boran dataset versus UCL dataset, ES, 95% CI: 0.0988, -0.148 to 0.356, p=0.537, Extended Data Fig. 4d). Since slope and the associated down-state (i.e., mean HG power between the two 0-crossings of LoWS at -0.15 and 0.165 s) clearly distinguish LoWS from background noise, we used these intrinsic features to further characterize slow waves. When plotting all patients in a 2-dimensional space defined by these features, we observed that patients with Parkinson’s disease constituted an isolated cluster with low slope and absent down-state. This was confirmed by statistical analysis of the inter-patient Euclidean distance within this 2-D space (see Extended Data Fig. 4e-f and Online Methods for further details and statistical analyses).\n\n## LoWS and interictal epileptiform discharges\n\nThere is burgeoning evidence of a complex interplay between epileptic and sleep-related network activity23,27,32,33. We thus examined the interaction between LoWS and interictal epileptiform discharges (IEDs). We identified IEDs in all but one patient (mean rate ± SD across patients and electrodes: 0.01/s/electrode ± 0.01, n=16, Fig. 3a-c).\n\nWe next determined the rate of LoWS against that of IEDs. We observed a significant negative correlation across patients (Pearson correlation, r2=0.51, p=0.002, n=16, Fig. 3d, see Supplementary Information for further discussion). We explored this further by determining whether this could explain why we found more LoWS in our dataset than in the other dataset of patients with epilepsy. After correcting the rate of LoWS by that of IEDs (see Online Methods), we indeed found a similar normalized rate of LoWS between both datasets of patients with epilepsy (Boran dataset versus UCL dataset, ES, 95% CI: -0.0004, -0.001 to 0.0001, p=0.22, Extended Data Fig. 4c, two last columns). Besides LoWS rate, neither the slope (Pearson correlation, r2<0.001, p>0.99, n=16, Extended Data Fig. 5a), nor the amplitude (Pearson correlation, r2<0.001, p=0.96, n=16, Extended Data Fig. 5b) of LoWS correlated with the IED rate.\n\nSome evidence suggests that IEDs are preceded by a progressive increase in excitability34,35. In line with this, we observed a progressive increase in HG power prior to IEDs (β-estimate ± SD: increase of 1 log(µV2) in HG power each 66.5 s ± 25.4, p=0.009, Fig. 3e). Thus, in parallel to this progressive increase in excitability before IEDs, we next asked whether LoWS undergo key electrophysiological changes similar to those of sleep SW in response to increased excitability after a period of wakefulness. Under high homeostatic sleep pressure, sleep SW present with high incidence rate, slope and amplitude16 (see Fig. 1a-b). Using these features as covariates in a linear mixed model with time to the next IED as the dependent variable, we found that the slope (β-estimate ± SD: slope increases by 1% each 347 s ± 114, adj. p=0.0026, n=16, Fig. 4a, b) and amplitude (β-estimate ± SD: amplitude increases by 1% each 285 s ± 101, adj. p=0.01, n=16, Fig. 4a, c) but not the rate (β-estimate ± SD: rate changes by -1% each 55 s ± 96, adj. p=0.57, n=16) of LoWS increase significantly across time leading up to the next IED. Importantly, although these rates of change may appear small, they are more than double that reported in sleep SW across a whole night (at least for SW slope: change of 20-30% across 381 min of sleep)13. Thus, two classical markers of synaptic strength (the slope and amplitude of LoWS)6 change in parallel to progressive increases in HG power prior to IEDs. This indicates that LoWS exhibit a key condition associated with homeostatic activity: they show adaptation in parallel to excitability, similar to the response of sleep SW to increased activity during wakefulness.\n\n## Effects of LoWS on IEDs\n\nThe results above indicate a response of LoWS to increases in network activity leading up to IEDs, but do LoWS also represent a mechanism to reduce these aberrant increases in network activity? IEDs are proposed to represent cellular depolarization36 and can be generated locally or propagate from more distant sites. It has been suggested that the local or distal nature of IEDs can be determined by the presence or absence of an increase in gamma activity prior to the IED, respectively34. Moreover, high-gamma activity can further distinguish IEDs that are associated with increases in neuronal firing from those that are not37,38.\n\nTo investigate the negative feed-back of LoWS on IEDs, we used a linear mixed model with delay since the last LoWS and the rate of LoWS in-between two successive IEDs as covariates and HG power during IEDs (from -0.05 to 0.05 s around peak amplitude) as the dependent variable. In addition, since we observed increases in HG prior to IEDs, we used the increase rate of baseline HG (ratio of HG power between -6 to -1 s before IEDs divided by -250 to -245 s) as a third covariate to identify any effects that might be specific to locally generated IEDs (i.e., those preceded by increases in HG), or that reflect an interaction between LoWS and background excitability. We hypothesized that LoWS would reduce increased excitability associated with IEDs (i.e., would impact the HG burst associated with IEDs) and would have greater effect on IEDs that are generated locally (i.e., the impact would be dependent on the level of baseline change in HG power). We found a significant effect of the delay since the last LoWS on HG power during IEDs (β-estimate ± SD: 7.7∙10-5 ± 1.2∙10-5 log(µV2/ µV2)/s, p=8∙10-11, blank red bar in Fig. 4d) and a significant interaction between baseline increases in HG power and delay since the last LoWS on HG power during IEDs (β-estimate ± SD: 1.8∙10-5 ± 8.4∙10-6/s, p=0.031, filled red bar in Fig. 4d). No significant association was found for LoWS rate prior to IEDs (Fig. 4d). Thus, a longer delay since the last LoWS is associated with high network excitability during IEDs (and vice versa), and this effect is more pronounced for IEDs that may be locally generated and / or associated with large preceding increases in background excitability. This suggests that LoWS also exhibit the second property expected of a homeostatic process: they reduce network excitability, similar to the proposed function of sleep SW.\n\n## Phasic modulation of LoWS during a cognitive task\n\nCognitive tasks are known to increase the brain’s metabolic demand39. We therefore asked whether this increased demand also changed features of LoWS, consistent with a putative homeostatic role. To do so, we examined the properties of LoWS during the encoding and retrieval phases of a temporal lobe dependent associative memory task (see Online Methods). We found that the rate of LoWS increased during encoding (ES, 95% CI: 0.0116/s/electrode, 0.0038-0.026, p=0.023, n=17, Fig. 5a) but not retrieval (ES, 95% CI: 0.00446/s/electrode, -0.00343 to 0.0136, p=0.348, n=17, Fig. 5a). Furthermore, we observed that the slope of LoWS was steeper during both the encoding (ES, 95% CI: 0.06, 0.03-0.09, p=0.002, n=17, Fig. 5b) and retrieval (ES, 95% CI: 0.05, 0.02-0.08, p=0.007, n=17, Fig. 5b) phases of the memory task, while LoWS amplitude was higher during encoding (ES, 95% CI: 0.108 µV, 0.07-0.15, p=0.0002, n=17, Fig. 5c) but not retrieval (ES, 95% CI: -0.00104 µV, -0.0555 to 0.0459, p=0.972, n=17, Fig. 5c) phase. Together, these results support an adaptative modulation of LoWS by cognitive processes.\n\n## LoWS are associated with transient cognitive impairment\n\nOne reason why SW are believed to be restricted to sleep is their impact on neuronal activity, which might be expected to have a detrimental effect on cognition5. We tested this prediction by analyzing the relationship between LoWS and performance on the associative memory task. We found that the rate of LoWS during retrieval was significantly lower during trials with fast versus slow reaction times (RTs; ES, 95% CI: -0.11/s, -0.22 to -0.05, p=0.0114, n=17, Fig. 6a), suggesting that the occurrence of LoWS during retrieval impacts task performance. In contrast, the rate of LoWS was similar during good and bad accuracy trials (Fig. 6b). Performing the same analysis on IEDs revealed no significant difference in the incidence rate between trials with fast versus slow RTs (Fig. 6c). However, the rate of IEDs was significantly lower during good versus bad accuracy trials in both the encoding and retrieval phases (ES, 95% CI during encoding: -0.04/s, -0.12 to -0.01, p=0.0114, n=15 subjects with ≥ 1 IED and ≥ 1 trial with bad and good accuracy; ES, 95% CI during retrieval: -0.02/s, -0.03 to -0.01, p=0.0032, n=16 subjects with ≥ 1 IED, Fig. 6d), consistent with previous studies40. Altogether, these results indicate that LoWS and IEDs are associated with distinct cognitive impairment: the former with increased RT and the latter with decreased accuracy.\n\n# Discussion\n\nIn sum, these findings reveal the existence of SW during wakefulness that recapitulate the distinctive features of sleep SW, including the down-state of neuronal activity. Although evidence supports a restorative function of SW during sleep10,11, it was previously unknown whether such beneficial activity could also be activated during wakefulness in pathological conditions. Here, we provide evidence of changes in LoWS properties (slope and amplitude) before IEDs that reproduce the changes of sleep SW under high homeostatic sleep pressure13,16. We further show that LoWS occurring during this vulnerable period oppose the effect of baseline HG power in generating the burst of increased excitability associated with IEDs (i.e., elevated HG power during IEDs), suggesting that LoWS could operate as key components of epilepsy homeostasis41, mirroring the well-known sleep homeostasis regulated by sleep SWs6. This is further supported by the negative correlation between LoWS rate and IED rate, which suggests that IEDs occur more frequently in patients with fewer protective LoWS. Last, we observed that these beneficial effects place a burden on cognitive processing, slowing reactions times in an associative memory task, consistent with their impact on neuronal activity5.\n\nWhile the finding of slow waves during wakefulness in an independent cohort of patients with Parkinson’s disease suggests that they are not strictly specific to epilepsy, our work shows that they are more frequent and more readily distinguished from background in patients with epilepsy. Moreover, the wake slow waves in Parkinson’s disease were distinct from LoWS in epilepsy as they had a reduced slope and were not clearly associated with a down state. It is worth noting, however, that the Parkinson’s disease data31 were obtained from neocortical surface recordings, as opposed to the mesial temporal, depth electrode recordings in both epilepsy cohorts. However, placing depth electrodes in the mesial temporal lobe of healthy subjects is not clinically justifiable.\n\nSleep SW have long been recognized and extensively investigated4,6,10,12,16,18,28,29,42–44 whilst suggestive evidence of slow wave activity during wakefulness has only recently been described45,46. Previous studies of wake slow waves have made use of sleep-deprived animals24, humans under sleep pressure undergoing scalp EEG recordings45, or stimulation of cortical regions surrounding focal brain injury25. However, typical slow waves with an associated neuronal down-state have not previously been described in awake humans, and it was unknown whether this core feature of sleep SW occurred during wakefulness. Indeed, the identification of neuronal down-states has been recognized as particularly challenging in awake humans, since these periods are expected to be very short47. However, by applying stringent criteria for selecting waves within the delta range, we have been able to characterize neuronal down-states during wakefulness in humans.\n\nIn the search for slow waves, some studies have included oscillatory activity up to 7-9 Hz45,47–49, which increases the risk of incorporating theta oscillations that are typically enhanced by cognitive processes50 or benign variants associated with drowsiness51. This is a concern, given our observation that the rate of LoWS increased with cognitive demand. This emphasises the importance of identifying neuronal down-states, in order to differentiate delta and theta oscillations from wake slow waves. The lower signal-to-noise ratio of scalp EEG also increases the difficulty of identifying wake slow waves, and the lower spatial resolution complicates the study of focal slow waves and their interaction with other local activity patterns, such as epileptiform discharges. Here, intracranial recordings allowed us to describe a local interplay between interictal epileptiform discharges and LoWS.\n\nOn a complementary note, many previous intracranial EEG studies describe separate “low” and “high” theta bands that are independently modulated by various cognitive processes52–54. However, the results presented here raise the possibility that changes in “low” theta power instead reflect an increased incidence of LoWS associated with cognitive effort. This would also explain why “low” theta is rarely observed in EEG or MEG recordings from healthy participants performing similar tasks55 and incites further characterization of LoWS to clarify their interplay with cognitive processes.\n\nThe LoWS we observed in epilepsy resulted in decreased HG activity and neuronal firing akin to an interruption of network function, so it is not surprising that LoWS were also associated with slower memory retrieval. Importantly, this impact on cognition is distinct from the impaired accuracy associated with IEDs, which has been previously described40. The impact of LoWS on neuronal activity in the hippocampus could be less pronounced than that observed in other brain regions, as changes in the activity of hippocampal neurons during down- to up-state transitions are less evident than in neocortex and parahippocampus56, despite similar phase locking to slow oscillations26. Furthermore, the normalization of neuronal excitability during sleep involves a complex dynamic affecting differentially neocortical cells with high- and low-firing rates57, and further work is needed to clarify the effect of LoWS on neuronal subpopulations. It is also important to note that despite this negative short-term impact on cognition, the homeostatic role of LoWS is likely to be beneficial for longer-term brain function, similar to sleep slow waves10,23. In this context, the specificity of low-frequency (1-3 Hz) stimulation to elicit synaptic depressionin vitro58 and to decrease cortical excitability in humans59 as well as its antiepileptogenic effect in a rodent model of epilepsy60 fits well with the hypothetical antiepileptic property of LoWS. Our work proposes that the same pattern of activity is naturally employed by the brain in patients with epilepsy, and a failure to express LoWS could be detrimental. Modulating LoWS could thus represent an efficient neurostimulation protocol that enhances their protective activity to increase the epileptic threshold. Since preliminary works have shown that it is possible to experimentally amplify sleep SW61, the application or improvement62 of such devices to the field of epilepsy could be within reach in the near future.\n\nWe observed changes in the properties of LoWS in the order of seconds to minutes before IEDs, suggesting that the time-scale for homeostatic control during wakefulness is shorter and more dynamic than that during sleep23, as predicted by Vyazovskiy and Harris5. Consistent with this, our results argue in favor of discrete, isolated waves during wakefulness. Thisphasic homeostatic control, intimately linked to the occurrence of IEDs, could be explained by a temporal and spatial constrain on the generation of LoWS to minimize the deleterious effect of LoWS on cognitive functions5. Indeed, our data indicate that LoWS are a very local phenomenon that seems to affect mainly locally generated IEDs.\n\nTo summarize, our study provides evidence of “micro-sleep” modules activated during wakefulness in epilepsy that present with clear homeostatic features, showing not only adaptation in association with increases in network excitability before IEDs, but also negative feed-back on IEDs, and comes at the cost of cognitive lapses. Our work highlights the compromise made by a brain that is affected by transient pathological activity and calls for the development of interventional strategies aiming at promoting LoWS to test their direct therapeutic ability in epilepsy.\n\n# Online Methods\n\n## Patients\n\nA total of 25 patients with medically refractory epilepsy (11 female, 23 right-handed, mean age of 38.5 yrs, 17 with macroelectrode recordings and 8 with microelectrode recordings, Extended Data Table 1) undergoing intracranial EEG monitoring for clinical purposes at the National Hospital for Neurology and Neurosurgery, London were included in this study. One supplementary patient with microelectrode recording was excluded because of high epileptic activity that would have impeded a reliable analysis of slow wave activity. Prior approval was granted by the NHS Research Ethics Committee (15/LO/1783), and informed written consent was obtained from each patient. Patients were recruited if the research protocol did not impact negatively on their clinical care, and if intracranial electrodes were targeted at mesial temporal lobe structures. Sex and gender were not considered in the study design, given the rarity of the data. Some of these patients participated in other research projects that have been published elsewhere63,64. Two publicly available datasets30,31 relating to complementary cohorts from other centers (16 patients with Parkinson’s disease and 9 patients with epilepsy), were also included for control purposes. The Parkinson’s disease dataset31 was published under a CC0 1.0 license (without copyright) and is available here: doi.org/10.7910/DVN/IO2FLM. The dataset of patients with epilepsy30 was published under a CC BY-SA 4.0 license (https://creativecommons.org/licenses/by/4.0/) and is available here: https://doi.org/10.12751/g-node.d76994.\n\n## Task\n\nA description of the associative memory task is provided in more detail elsewhere63,64. Briefly, the task was divided into encoding and retrieval phases. During encoding, participants were presented with 27 pairs of images that remained on screen for 6 s, preceded by a 2 s fixation cross and followed by a 2 s blank screen. Unbeknownst to participants, each pair was drawn from one of 9 discrete “events” comprised of a person, place and object. As such, each item (person, place, object) was paired with two other items over the course of encoding. During retrieval, participants were first presented with a single cue image for 3 s, drawn either from one of the 9 events viewed during encoding or an equal number of ‘New’ events, comprised of person, place and object images that had not been viewed during encoding. Next, participants were asked whether the cue image was “Old or New?” – i.e., whether that image had formed part of a pair viewed during encoding or not. If the cue image was ‘Old’, whether or not the participant correctly identified it as such, they were then successively asked to indicate which two images it had been paired with, from two groups of four alternative choices drawn from the same image category across all ‘Old’ events (i.e. if cued with a person, they were first asked which place and then which object it had been paired with during encoding). In each case, participants had unlimited time to indicate their response with a key press, and reaction times (RTs) were recorded.\n\nTo test if the rate of IEDs or LoWS during encoding was associated with changes in accuracy or RTs, the mean incidence rate across the two 6 s encoding trials where each image was presented was measured. To test if the rate of IEDs or LoWS during retrieval was associated with changes in accuracy or RTs, the incidence rate during the time taken to make an associative memory response was measured.\n\n## Data acquisition\n\nMacroelectrode EEG data were recorded continuously at a sample rate of 2048 Hz (Patients 12 and 13), 512 Hz (Patients 1 and 16), or 1024 Hz (all other patients) using a Micromed SD long-term monitoring system (Micromed). Recordings made at a higher sampling rate were downsampled to 512 Hz before any analyses were performed. Microwire EEG data were recorded continuously at a sample rate of 30 kHz using a Blackrock Neuroport system (Blackrock Neurotech LLC).\n\n## Data analysis\n\n### Code and software used for analyses\n\nAnalyses were performed using custom Matlab (The MathWorks, v. 2022a) code and the Fieldtrip toolbox65. Statistical analyses were performed using the web application EstimationStats66, Graphpad Prism (v. 9.5.0), SPSS (v. 29.0.0.0) and Matlab (v. 2022a). Figures were designed in Matlab, Graphpad Prism and Adobe Illustrator.\n\n### Identification of IEDs\n\nIEDs were identified in a semi-automated manner. First, the data were screened using a published algorithm for rodent models of epilepsy32 that was adapted to human recordings. Briefly, data were filtered between 20-80 Hz (using a second order Butterworth filter) and the amplitude of the filtered signal estimated using the absolute value of the Hilbert transform. Candidate IEDs were then defined as periods where both the amplitude of the filtered signal exceeded 3.5 times the mean envelope and the amplitude of the unfiltered signal exceeded 4 times the mean envelope. A refractory period of 1 s after each candidate IED was added, during which no other IED could be detected. Next, if >1 recording contact in any single region of interest (hippocampus, amygdala, temporal neocortex) exhibited a candidate IED within a window of ±0.3 s, only the candidate IED with the highest amplitude was retained. Finally, all candidate IEDs were curated by visual inspection and missed IEDs were manually added.\n\n### Identification of slow waves\n\nSlow waves were detected using a standard algorithm13,26–28. First, the LFP signal was filtered between 0.5-4 Hz (using a second order Butterworth filter), all positive-to-negative zero-crossings and negative-to-positive zero-crossings in the filtered signal were detected, and events with a duration of 0.25 to 1 s were selected as candidate slow waves. Next, any candidate slow waves that occurred ≤1 s after a detected IED on any of the recording contacts in the same brain region were discarded. Finally, only the remaining candidate slow waves whose amplitude exceeded the 90th percentile were retained. Those slow waves were then visually inspected, and any that appeared artifactual or had an apparent IED occurring shortly beforehand were discarded. We were concerned by the fact that IEDs are typically followed by a slow wave, but it was not possible to visually inspect all slow waves, due to the large number detected. In addition to the precautionary measures taken above, we thus undertook several verification steps to ensure that detected slow waves were not mislabeled IEDs:\n\n1. Detected slow waves were visually similar to those described in other publications (Fig. 1c-d)13,28.\n2. Detected slow waves and IEDs had a different spectral signature (Fig. 1f-g and Fig. 3c).\n3. 45-130 Hz high-gamma (HG) power during IEDs (measured either during the time window used for down-state analysis, -0.15 to 0.165 s; or during the time window of IED peak, -0.05 to 0.05 s; was significantly higher than during pSW (ES, 95% CI: 4.49∙103 µV2, 2.68∙103-7.25∙103; and ES, 95% CI: 2.24∙104 µV2, 1.29∙104-3.71∙104, p=0.0008 for both, Extended Data Fig. 2a). Note that since HG power is decreased during LoWS, we did not compare it with HG increases during IEDs.\n4. If slow waves were mislabeled IEDs, then variability in the rate of slow waves across electrodes should follow variability in the rate of IEDs rate across the same electrodes. To test this, we defined an index of ‘parallel rate variability’ (PRV) that records the ratio of IED rate to slow wave rate for each electrode minus the ratio of the sum of IED rate and slow wave rate across all electrodes for each participant. As such, the median PRV value is expected to be significantly different from 0 if the rates of IEDs and slow waves do not follow the same pattern across electrodes. The PRV is defined by:\n [IMAGE_ONLINE_METHODS_1]\n Where n=1 to N indexes the electrodes in a specific patient. Across participants, the median PRV was significantly different from 0 (median, 25-75th percentile: 0.06, 0.001-1.62, one sample Wilcoxon test, p<0.0001, Extended Data Fig. 6), indicating that variability in the rate of IEDs rate is not paralleled by variability in the rate of slow waves across electrodes. We calculated the PRV only in the hippocampus, where all main analyses were performed.\n5. If LoWS were mislabeled IEDs, then electrodes that exhibit the greatest number of IEDs should also record the greatest number of slow waves. However, there was no difference in the rate of slow waves rate between all electrodes but the one with the highest rate of IEDs rate and that with the highest rate of IEDs (dES, 95% CI: -0.002/s, -0.01 to 0.003, p=0.595, Extended Data Fig. 7).\n6. LoWS and IEDs have differential impacts on memory processing (Fig. 6).\n7. LoWS and IEDs rates are negatively correlated (Fig. 3d). If LoWS were a subpopulation of mislabeled IEDs, and since LoWS detection is semi-automatic (except for the visual removal of artefacts and post-IED waves), then the proportion of mislabeled IEDs as LoWS should be constant across participants, resulting in a positive correlation (we provide further discussion of this point, as well as statistical confirmation, in the Supplementary Information).\n8. Finally, we also wished to address the possibility that the slow waves we identified corresponded to low frequency post-IED waves that propagate more readily across electrode contacts than the sharp component of the IED. To test this, we measured the absolute amplitude of the raw LFP signal at the peak of each IED (i.e., the amplitude of the sharp component) across all hippocampal electrodes and the maximum absolute amplitude in the 0 to 0.5 s window after that peak (i.e., the amplitude of the subsequent slow wave) and then quantified the relative reduction in amplitude of each with distance from the focus. Across 7 adjacent recording contacts (the maximum number available on each depth electrode), there was no significant difference in these normalized amplitudes (Extended Data Fig. 8a-b). Since our main focus was on the deepest (i.e., most medial) recording contacts (located in the hippocampus), we also compared the ratio of amplitudes on the 1st electrode (electrode of interest) and 2nd (adjacent electrode contact) and did not find a significant difference (dES, 95% CI: 0.0391, -0.0513 to 0.153, p=0.49, Extended Data Fig. 8c). In sum, this indicates that the amplitude of post-IED slow waves decreases with distance from the focus at the same rate as the sharp component, arguing against the wider propagation of post-IED slow waves compared to the sharp component which could make post-IED waves appear as LoWS (i.e., without the sharp component).\n\n### Corrected rate of slow waves.\n\nSince we observed a negative correlation between the rate of LoWS and IEDs (Fig. 3d), we computed the rate of LoWS corrected for the rate of IEDs to verify whether variability in the rate of IEDs could explain discrepancies between our dataset and the Boran dataset (Extended Data Fig. 4c, 3 first columns). The corrected rate was calculated by multiplying the LoWS rate by the IED rate (Extended Data Fig. 4c, 2 last columns), to account for the negative correlation between these variables.\n\n### Signal-to-noise ratio of slow waves.\n\nBefore calculating the signal-to-noise ratio and to approximately match our dataset, data from the Parkinson’s and Boran datasets were downsampled to 500 Hz from their original sampling frequency of 1000 Hz and 2000 Hz, respectively. For each dataset, we then normalized the amplitude of the signal in a ± 3 s around each slow wave to the maximal amplitude in the same time window. The signal-to-noise ratio was then measured as the ratio of the peak amplitude of the wave to the standard deviation across the entire window.\n\n### Identification of slow waves in the Boran dataset.\n\nWe used another dataset of patients with epilepsy recorded with intracortical electrodes30 to assess the reproducibility of slow waves detection. To identify hippocampal slow waves, we used the Juelich Histological Atlas, which computes a probability that each contact is located in a subset of brain regions. We considered a contact to locate in the hippocampus if the hippocampus was the most probable region and the probability was ≥ 25%. We used the Matlab mni2atlas.m function for that purpose (https://github.com/dmascali/mni2atlas/releases/tag/1.1).\n\n### Identification of slow waves in patients with Parkinson’s disease.\n\nWe followed the same procedure as the one described for the detection of slow waves in our dataset, except that we did not identify IEDs. None of the 16 patients were suffering from epilepsy (personal communication with Dr. Merk). Data were converted into µV for display. We only used the signal from neocortical contacts.\n\n### Interactions between IEDs and LoWS\n\n#### LoWS-rate around IEDs.\n\nTo measure variability in the incidence rate of LoWS around IEDs, we calculated the mean rate of LoWS across electrodes in a series of non-overlapping 5 s time windows relative to the closest IED (up to 250 s before IEDs). These values were then normalized by the maximal LoWS rate for each patient. We then used the software SPSS to compute linear mixed models using time as the dependent variable and rate, slope and amplitude of LoWS as covariates (see below). The y-intercept was specific to each subject.\n\n#### LoWS-slope around IEDs.\n\nTo measure variability in the slope of LoWS around IEDs, we computed the average slope of all LoWS in each 5 s time window relative to the closest IED (up to 250 s before IEDs). To do so, we identified the minimum of the 0.5-4 Hz filtered signal in a 1 s window following LoWS onset and defined LoWS slope as the ratio between the amplitude and post-onset time of this minima. Each slope was normalized by the value of the highest absolute slope for that patient, so that all values lay in the range of 0 to 1. These values were then used as covariate in the linear mixed model, as indicated above.\n\n#### Amplitude of LoWS around IEDs.\n\nTo measure variability in the amplitude of LoWS around IEDs, we followed the same procedure described above but using the absolute minima of the 0.5-4 Hz filtered signal in a 1 s window following LoWS onset, in place of the estimate of LoWS slope.\n\n#### HG power before IEDs.\n\nWe used the Fieldtrip65 function ft_freqanalysis.m to calculate the HG power (45-130 Hz) during non-overlapping windows of 1 s before IEDs (multitaper frequency transformation) and log-transformed the result. Each IED presented with a different pre-IED time-window, which length depended on the delay since the last IED. Since frequency power is exponentially distributed, it was important to include as many trials in each non-overlapping time-bin before IEDs, to avoid that very low, or very high, values of HG power affect differentially time-bins with only a few or many trials. Hence, we selected the same number of trials for each time-bin prior to IEDs by identifying for each participant the maximal pre-IED duration that would encompass at least 50% of all IEDs. HG power was then used as a covariate and time to the next IED as the dependent variable in a mixed linear model.\n\n### Interaction between LoWS, baseline HG and HG power during IEDs\n\nTo calculate the increase rate of HG power before IEDs, we measured the ratio of HG power (45-130 Hz) before IEDs (-6 to -1 s before IEDs) to a period away from IEDs (-250 to -245 s) using ft_freqanalysis.m (multitaper frequency transformation) and log-transformed the result. The period (-250 to -245 s) and the size of the time-windows (5 s) were chosen for homogeneity with the analysis of rate, slope and amplitude before IEDs. To calculate HG power during IEDs, we measured the HG power during IEDs (-0.05 to 0.05 s around IEDs, thus not overlapping the window for increase rate of baseline HG) and normalized it against HG power sampled randomly during artefact-free periods. The delay since the last LoWS was recorded in seconds. The rate of LoWS was calculated as the number of LoWS between the last IED and the IED of interest, divided by the duration of that interval (in seconds). Then, we used a linear mixed model with HG power during the IED as the dependent variable and delay since the last LoWS, rate of LoWS, interaction [baseline increases in HG*delay] and [baseline increases HG*rate] as covariates. We did not include “baseline increases in HG” as an independent covariate, since it can be expected that an increase in HG power will be followed by high values of HG, and vice versa. We selected HG power during IEDs, rather than the peak amplitude of IED, because the peak amplitude is sampled at only one timeframe, which would not reliably represent the relatively long duration of IEDs (see Fig. 3b), and because the peak amplitude can vary with shifts in the ongoing baseline activity. Furthermore, HG activity is typically considered a reliable proxy of neuronal activity38.\n\n### Time-frequency analyses\n\nTo measure changes in 45-130 Hz HG power associated with LoWS (Fig. 1e), we used Fieldtrip65 function ft_freqanalysis.m (multitaper frequency transformation) for the time window between the two zero-crossings of the grand average LoWS (-0.15 to 0.165 s around the LoWS trough). Power values were baseline corrected using average power at each frequency across the -2.9 to -0.2 s and 0.2 to 2.9 s time windows relative to the LoWS trough. As a control, the same analysis was performed relative to a randomly sampled set of time bins (as opposed to the occurrence of genuine LoWS). Importantly, changes in HG power associated with pSW and IEDs were not baseline corrected, because changes in HG power were observed within the baseline time windows (e.g., during the down-state before pSW [Fig. 1g] and following IEDs [Fig. 3c]). For the time-frequency decompositions in Fig. 1f,g (LoWS) and 3c (IEDs), dynamic changes in oscillatory power were estimated using a seven-cycle Morlet wavelet transform (implemented using the Fieldtrip function ft_freqanalysis.m) in ± 3 s time windows around IEDs and LoWS across a 1.5 to 130 Hz frequency range. For control purposes, we used the functions randsample.m or datasample.m to randomly generate twice as many time bins (for LoWS) or the same number of time bins (for IEDs), excluding artefactual periods and time windows of ± 3 s around another IED or LoWS (for LoWS) or time windows of ± 3 s around another IED (for IEDs).\n\n### Micro-electrode recordings\n\nSingle and multi-unit activity was identified using the wave_clus toolbox67. Briefly, data were filtered in the 300-3000 Hz range and events whose amplitude was within 4-50 standard deviations of the median noise identified as candidate spikes. Spikes were then clustered automatically based on wavelet features of the waveform before single- and multi-unit activity clusters (denoted together as unit spiking activity or “units” in the manuscript) were manually identified based on the inter-spike interval distribution and average waveform. The firing rate of each unit was then convolved with a 0.2 s Gaussian window and normalized to the mean firing rate across epochs (± 3 s around individual LoWS). Finally, units with a mean firing rate < 2 Hz across the entire recording session were discarded, following26. The statistical analysis in Fig. 2c was performed with units that had a mean firing rate > 2 Hz across the entire EEG and with units that had a mean firing rate > 2 Hz during the surrounding baseline (-2.9 to -0.2 and 0.2 to 2.9) and both came out as significant after Bonferroni-Holm correction. For display (Fig. 2d) we used units with mean firing > 2 Hz during the surrounding baseline.\n\nTo obtain a time-resolved evaluation of the firing rate around LoWS, we first obtained the mean firing rate per patient (n=8) and downsampled these time series to 10 Hz, thus obtaining a resolution of 0.1 s for statistical analysis. We then used a bootstrapping approach as follows: for each time bin from -1 to 1 s around the LoWS trough, the difference between the mean firing rate around LoWS and five times as many randomly sampled time bins was calculated. Across 5000 bootstraps, the identity of these conditions was then randomly switched to obtain a null distribution of paired firing rate differences. We then identified where the actual firing rate difference lay on the bootstrapped distribution and recorded the percentile to calculate a two-tailed p-value. We chose more control markers to increase the reliability of baseline estimation. Finally, p-values were adjusted by the false-discovery rate (function fdr_bh.m68).\n\nMean firing rates during the down-state were computed between the two zero-crossings of the mean LoWS (from -0.15 to 0.165 s around the LoWS trough) and normalized by the mean firing rate during the surrounding baseline window (-2.9 to -0.2 and 0.2 to 2.9 s around the LoWS trough). For statistical analysis, these values were compared against the firing rate occurring around nSW and pSW, which occurrence had been shuffled (left end of each line in Fig. 2e).\n\n### Analysis of IEDs, LoWS and memory performance\n\nTo assess the effect of IEDs and LoWS on memory performance, we tested whether mean incidence rates during encoding (i.e., during the 6 s of image presentation) and retrieval (i.e., during the variable duration period between the associative memory question appearing and participant’s response) differed between good and bad accuracy trials (i.e. those with correct versus incorrect responses) and fast vs slow RT trials (i.e. those with RTs below the 20th percentile and above the 80th percentile across all trials).\n\n## Statistical analyses\n\nUsing the web application estimationstats.com66, we performed estimation statistics rather than significance testing for most statistical analyses. Estimation statistics provide numerous advantages69, one of them being that the statistical analyses relies on an evaluation of the effect size. For these analyses, the p-values displayed represent the probability to obtain the same effect size if the mean paired difference is equal to 0. We indicate the mean paired difference (effect size, ES) as well as the 95% confidence interval (95% CI). P-values are obtained through two-sided permutation t-tests using 5000 bootstraps. Since estimation statistics are not null-hypothesis testing, they do not require correction for multiple comparisons. Even so, we checked whether p-values resisted a Bonferroni-Holm correction when multiple comparisons were applied: % of unit spiking activity showing a decrease during down-state; LoWS rate across 3 datasets; LoWS signal-to-noise ratio; analysis of cluster (Extended Data Fig. 4f); LoWS effect on behavior; IEDs effect on behavior; LoWS slope during encoding and retrieval; LoWS amplitude during encoding and retrieval; LoWS rate during encoding and retrieval. We found that all p-values remained significant. When multiple comparisons were applied on null-hypothesis statistics, we also applied a Bonferroni-Holm correction. For most plots, we display the effect size on the right of the respective panel.\n\nTo test whether the waves identified in patients with Parkinson’s disease31, in another dataset of patients with epilepsy30, and in our dataset, were similar or constituted separate clusters, we plotted all participants’ average slow wave in a 2-dimensional space defined by slow waves slope and down-state (estimated by HG power). We then measured the Euclidean distance between two points (slow waves in the 2D space defined above) of the group of interest, which we call distance “a”. We then calculated the Euclidean distance between one point of the group of interest and one point sampled across all points (for patients with Parkinson’s disease) and one point of the group of interest and one point sampled across all patients with epilepsy (for patients with epilepsy), which we call distance “b”. Each of these points was randomly sampled 1000 times. We then calculated the difference between distance “a” and distance “b” across these 1000 samples. Across these 1000 differences, we then calculated the z-value of a one-sample Wilcoxon signed rank test (signrank.m) and the median of the difference, the null hypothesis being a median equal to 0 (the distance between two points within one group is equal to the distance across groups). We repeated this operation 1000 times to obtain 1000 z-values and 1000 medians. We then calculated the corresponding two-tailed p-value and the mean median of the distance difference. We used two sets of 1000 repetitions as the one-sample Wilcoxon signed rank test tends to virtually always gives a significant p-value for large datasets, even for very small differences that cast doubt on the meaning of the observed effect (risk of type I error). On the other hand, datasets that are too small fail to reliably assess a potential effect (risk of type II error). Hence, by extracting one z-value based on 1000 repetitions, we mitigate the risk of type I error and by calculating the mean z-value across 1000 repetitions, we mitigate the risk of type II error. To test whether the subset of patients with Parkinson’s disease formed an isolated dataset, we followed this strategy:\n\n1. We tested whether patients with epilepsy from the Boran dataset30 presented with waves that were closer to themselves than to a group composed of waves from the Boran dataset and ours. This analysis revealed a significant positive difference of distance (median of the difference, 25-75th percentile: 0.04, 0.03-0.06, adj. p<0.0001, Extended Data Fig. 4f), indicating that patients from the Boran dataset are more distributed than all patients with epilepsy taken together. The inverse, i.e., whether our cohort was isolated from the Boran dataset, showed no significantly different distance (median, 25-75th percentile: -0.008, -0.01 to -0.0002, adj. p=0.1165, Extended Data Fig. 4f). Altogether, this shows that patients with epilepsy from the Boran dataset and ours are intermingled.\n2. We then tested whether patients with Parkinson’s disease31 presented with waves that are closer to themselves than to a group composed of all patients together. This revealed a significantly negative difference (median, 25-75th percentile: -0.04, -0.05 to -0.04, adj. p=0.0004), indicating that slow waves from patients with Parkinson’s disease indeed constitute a separate population.\n\nThus, slow waves identified in patients with Parkinson’s disease constitute a separate population from those identified in two independent datasets of patients with epilepsy.\n\n# Abbreviations\n\nHG:     high-gamma \nIEDs:     interictal epileptiform discharges \nLoWS:     local wake slow wave \nNREM:     non-rapid eye movement (sleep) \nnSW:     negative slow wave, i.e., associated with down-state of neuronal activity \npSW:     positive slow wave, i.e., associated with up-state of neuronal activity \nSW:       sleep slow wave \nSWA:     slow-wave activity (power between 0.5-4 Hz)\n\n# References\n\n1. Fiorillo, L. et al. Automated sleep scoring: A review of the latest approaches. *Sleep Medicine Reviews* **48**, 101204 (2019).\n2. 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Estimation statistics should replace significance testing. *Nat Methods* **13**, 108–109 (2016).\n\n# Supplementary Files\n\n- [SheybaniSupplementaryInformation.docx](https://assets-eu.researchsquare.com/files/rs-2693418/v1/a839840137356a6e98e91f98.docx) \n Supplementary Information\n\n- [Sheybanisupplementarytablesandfigures.docx](https://assets-eu.researchsquare.com/files/rs-2693418/v1/4bb33731a31d7661d0924beb.docx)"} {"paper_id": "prb28", "title": "Collective dynamical regimes predict invasion success and impacts in microbial communities", "text": "Collective dynamical regimes predict invasion success and impacts in microbial communities\n\nJeff Gore\ngore@mit.edu\n\nMassachusetts Institute of Technology https://orcid.org/0000-0003-4583-8555\nJiliang hu\nMassachusetts Institute of Technology\nMatthieu Barbier\nCNRS\nGuy Bunin\nIsrael Institute of Technology\n\nArticle\n\nKeywords:\n\nPosted Date: March 1st, 2024\n\nDOI: https://doi.org/10.21203/rs.3.rs-3979841/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nAdditional Declarations: There is NO Competing Interest.\n\nVersion of Record: A version of this preprint was published at Nature Ecology & Evolution on January 6th, 2025. See the published version at https://doi.org/10.1038/s41559-024-02618-y.\nCollective dynamical regimes predict invasion success and impacts in microbial communities\n\nAuthors:\nJiliang Hu1,2, Matthieu Barbier3,4, Guy Bunin5, Jeff Gore1*\n\nAffiliations:\n1 Physics of Living Systems, Department of Physics, Massachusetts Institute of Technology; Cambridge, MA 02139, USA.\n2 Department of Mechanical Engineering, Massachusetts Institute of Technology; Cambridge, MA 02139, USA.\n3 CIRAD, UMR PHIM, 34090, Montpellier, France\n4 PHIM Plant Health Institute, Univ Montpellier, CIRAD, INRAE, Institut Agro, IRD, 34090 Montpellier, France\n5 Department of Physics, Technion—Israel Institute of Technology; Haifa 3200003, Israel\n\nAbstract\nInvasions of microbial communities by species such as pathogens can have significant impacts on ecosystem services and human health. Predicting the outcomes of these invasions, however, remains a challenge. Various theories propose that these outcomes depend on either characteristics of the invading species or attributes of the resident community, including its composition and biodiversity. Here we used a combination of experiments and theory to show that the interplay between dynamics, interaction strength, and diversity determine the invasion outcome in microbial communities. We found that the communities with fluctuations in species abundance are both more invasible and more diverse than stable communities, leading to a positive diversity-invasibility relationship among communities assembled in the same environment. As predicted by theory, increasing interspecies interaction strength and species pool size leads to a decrease of invasion probability in our experiment. Although diversity-invasibility relationships are qualitatively different depending upon how the diversity is changed, we provide a unified perspective on the diversity-invasibility debate by showing a universal positive correspondence between invasibility and survival fraction of resident species across all conditions. Communities composed of strongly interacting species can exhibit an emergent priority effect in which invader species are less likely to colonize than species in the original pool. However, in this regime of strong interspecies interactions, if an invasion is successful, it causes larger ecological effects on the resident community than when interactions are weak. Our results demonstrate that the invasibility and invasion effect are emergent properties of interacting species, which can be predicted by simple community-level features.\nIntroduction\n\nEcological invasions, characterized by the spread of non-native species into novel environments, have significant consequences for biodiversity, ecosystem function, and habitat resilience \\( ^1 \\). Over decades, ecologists have sought to unravel the myriad factors influencing why some species invade successfully, and why some of those have large impacts on resident species communities, while others do not. Ecologists have posited a range of determinants, from the fitness and adaptability of the invaders to the resilience and composition of native communities \\( ^{2-4} \\). Among studies focusing on the invader species, many have sought to identify traits, such as growth and dispersal strategies, that may shape invasion outcomes\\( ^5 \\). Others have emphasized the role of the invaders' initial population size in the likelihood of establishment and spread\\( ^{6,7} \\). Yet others have emphasized interactions with resident species, e.g. the enemy release hypothesis suggesting that invasive species often succeed in new environments because they lack consumers or pathogens\\( ^8 \\). This has led to research on how properties of resident communities as a whole can determine the invasion outcome. For instance, the biotic resistance hypothesis suggests that communities with high native biodiversity are more resistant to invasion than less diverse communities, due to more efficient resource use or presence of natural enemies, but it is not consistently supported by empirical results\\( ^{9-12} \\). Beyond the characteristics of invader species and resident communities, environmental conditions have been shown to play a crucial role in shaping the invasion outcome\\( ^1 \\). Theories such as the storage effect and the fluctuating resource availability hypothesis posit that environmental disturbances and fluctuations might favor invader species in specific periods\\( ^{13-15} \\).\n\nMore recently, the issue of ecological invasion has become salient in the study of microbial communities, ranging from soil and aquatic ecosystems to the human body\\( ^{16-22} \\). These invasions can have profound impacts on ecosystem services and human health\\( ^{16,17,19,20} \\). Pathogenic microbes can invade host-associated microbial communities, leading to infections and diseases\\( ^{19,23,24} \\). For example, the invasion of pathogenic microbes \\( C. difficile \\) into the gut microbiota can lead to severe diseases including diarrhea and colitis\\( ^{23,25} \\). Understanding the mechanisms underlying invasion success and ecological consequences can help inform strategies for disease prevention, as well as the development of targeted therapies to control invasive pathogens\\( ^{25,26} \\). Similar to larger-scale ecological systems, it has been suggested that microbial communities with higher diversity are less likely to be invaded because diverse resident species may occupy all available niches and resources, leaving less room for invaders\\( ^{18,27-29} \\). Furthermore, it was shown that facilitative and competitive interactions between microbes can favor and prevent successful invasions, respectively\\( ^{27,30-32} \\). Parallel to observations in macro-organisms, external disruptions such as antibiotic interventions or nutrient level shifts can heighten the vulnerability of microbial communities to invasions\\( ^{16,33-35} \\).\n\nWhile research in microbial invasions has made significant strides, it remains unclear what characteristics of resident communities determine the success and impacts of an invasion\\( ^{17,18,36,37} \\). Species diversity is an easily measured indicator, but its relationship to invasibility may not be straightforward, whereas species interactions are likely important but often difficult to quantify. A more rarely emphasized property is the residents' dynamics: are they at equilibrium or fluctuating? It is not obvious that we can characterize dynamics at the level of the community; yet, building upon the groundbreaking work of Robert May, ecologists have explored the possibility of community-wide emergent dynamics, that can be classified into only a few qualitatively distinct regimes. and predicted from a few macroscopic parameters\\( ^{10,38-43} \\). In a recent study\\( ^{30} \\), we\nexperimentally assembled communities from various pools of microbial species in different conditions, and confirmed that simple community-level features, including species pool size and interaction strength, determined distinct dynamical regimes, characterized by the fraction of surviving species and the emergence of persistent abundance fluctuations over time.\n\nHere, we perform invasion experiments in diverse assembled microbial communities, and first observe that the foremost predictor of invasion outcomes appears to be the dynamical state of the resident community. We then use a combination of experiments and theory, exploring several dynamical regimes and spanning their control parameters (species pool size and interaction strength) to show that, taken together, they explain many features of invasibility and invasion effects. Communities of weakly interacting species reach a stable composition, where a fraction of the initial species pool survives, and further invasions display the same fraction of successes, only weakly perturbing resident species. Richer species pools and stronger interactions can give rise to fluctuating states, where species abundances fluctuate over time. We found that these fluctuating communities are more invasible and diverse than stable communities, leading to a positive diversity-invasibility relationship among communities assembled in the same environment. Finally, communities with strong interactions may also reach stable states with lower diversity, whose experimental phenomenology evokes the presence of alternative stable states: invasions succeed more rarely than predicted by survival fraction, but strongly impact the resident community when they do. The lower probability of invasion suggests a priority effect, whereby earlier invaders preclude later ones from growing from small abundances, leading to situations where the sequence and timing of species introduction can influence invasion success\\(^{10,44,45}\\).\n\nStudying invasions through the prism of community-wide dynamical regimes allows us to connect several strands of ecological thinking, regarding what counts as a successful invasion, when factors such as population size and history matter, and what consequences invasions have on resident community structure and functioning\\(^{46,47}\\). Furthermore, it helps clarify the hypothesis that increased community diversity results in reduced invasion probability due to fewer available niches\\(^{18,27-29}\\). Within fixed conditions (given the same initial species pool size and environment), more diverse communities tend to be found in fluctuating states, and are actually more likely to be invaded. Depending on how we change conditions, e.g. increasing species pool or reducing interaction strength, diversity may positively or negatively correlate with invasibility, providing one explanation for inconsistent observations\\(^{48-50}\\). Throughout, the fraction of surviving species remains a better predictor, displaying a universal positive correspondence with invasibility across all conditions, modulated by the presence of priority effects. Our results demonstrate that both invasibility and invasion effects are emergent properties, shaped by the interactions of resident species, which can be predicted by simple community-level features.\nResults and discussion\n\nTo experimentally characterize invasions in microbial communities, we built 17 different synthetic communities of size \\( S = 20 \\) using a library of 80 bacterial isolates from river and terrestrial environments (Fig. 1a and Supplementary Fig. 1). We exposed each community to daily cycles of growth and dilution into fresh media, with dispersal from the species pool (\\( S = 20 \\)) to mimic species dispersal in natural habitats (Fig. 1a). After six days of culturing, each community was exposed to an invader species (Fig. 1a) and we continued to culture the communities for another 6 days with dispersal of all species on each dilution cycle (Fig. 1a, b). For each resident community, we performed 7-9 independent invasion tests with different invader species on day 6, and monitored the growth of the invader and resident species (Fig. 1b). Analyzing species abundances through 16S sequencing, we found that 7% ± 2% of invasion tests were successful (relative invader abundance exceed extinction threshold \\( 8 \\times 10^{-4} \\) on the last day 12) (Fig. 1c and Supplementary Fig. 2). Although diverse ecosystems are typically thought to be more resistant to invaders\\(^{18,27-29}\\), our experimental results display a significant (\\( p=0.036 \\)) positive correlation between invasion probability and community diversity (correlation coefficient=0.51, Fig. 1c). Among communities of low diversity (2 – 5 surviving species) only 3% ± 2% of invasions were successful, whereas among communities of high diversity (6 – 9 surviving species) 13% ± 5% of invasions were successful. We therefore find that less diverse communities may resist invasions better than highly diverse ones under the same initial species pool size and nutrient conditions.\n\nTo better understand why the more diverse communities were more invasible, we next quantified the dynamics of the resident communities before invasion. We found that just under half (8 / 17) of the resident communities displayed persistent fluctuations in biomass and species composition, with the remainder reaching stable community states (Fig. 1d-f and Supplementary Fig. 3-12). We found that biomass fluctuations were highly correlated with species abundance fluctuations (Supplementary Fig. 12) and the classification of stable and fluctuating communities was robust to different methods (Supplementary Fig. 12). Consistent with our previous results, we found that the diversity of fluctuating communities is approximately twice the diversity in stable communities (Fig. 1e)\\(^{40}\\). Given this higher diversity in fluctuating communities, we next analyzed the invasibility of communities separately for the stable and fluctuating communities to determine if this could be driving the positive diversity-invasibility relationship that we observed. Indeed, we detected 8 successful invasions out of 61 invasion tests to fluctuating communities, while there was only one single successful invasion out of 60 invasion tests to stable communities (Supplementary Fig. 2). Our results therefore show that the probability to successfully invade fluctuating communities (13% ± 4%) is statistically ~8 fold larger than the probability of invading stable communities (1.7% ± 1.7%) (Fig. 1g). Our experimental tests of invasion demonstrate that, for fixed species pool size and conditions (including species interaction strength), more diverse communities are more invasible because fluctuating communities are both more diverse and more susceptible to invasion.\nTo gain insight into these surprising relationships between diversity, stability, and invasibility, we next studied invasions in the well-known generalized Lotka-Volterra (gLV) model, modified to include dispersal from a species pool:\n\n\\[\n\\frac{dN_i}{dt} = N_i \\left(1 - \\sum_{j=1}^S \\alpha_{ij} N_j \\right) + D\n\\]\n\nwhere \\( N_i \\) is the abundance of species \\( i \\) (normalized to its carrying capacity), \\( \\alpha_{ij} \\) is the interaction strength that captures how strongly species \\( j \\) inhibits species \\( i \\) (with self-regulation \\( \\alpha_{ii} = 1 \\)), and \\( D \\) is the dispersal rate. We simulated the dynamics of communities with different species pool sizes \\( S \\) and interaction matrices. We sampled the interaction strength from a uniform distribution \\( U [0, 2<\\alpha_{ij}>] \\), where \\( <\\alpha_{ij}> \\) is the mean interaction strength between species (predictions of this model are insensitive to the particular distribution chosen\\(^{40}\\)). Modeling species interactions as a random interaction network captures species heterogeneity without assuming any particular community structure \\(^{10,38-40}\\). We introduced invaders into resident communities at \\( t=10^3 \\) and continued to simulate the dynamics until \\( t=2\\times10^3 \\) to determine to invasion outcome.\n\nOur simulations revealed rich dynamics and invasion outcomes under strong interaction strength between species (Fig. 2a). Some successful invasions cause dramatic effect on the structures of resident communities, whereas other invasions only yield weak change in communities (Fig. 2a). Consistent with our experimental results (Fig. 1c and 1g), we found a positive correlation between invasion probability and richness (Fig. 2b), which is because fluctuating communities exhibit larger invasion probability than stable communities under the same conditions (Fig. 2c). Our simulation results with the Lotka-Volterra model also predict that the invasion probability decreases when interaction strength \\( <\\alpha_{ij}> \\) and the species pool size \\( S \\) increase (Fig. 2d-f). It is important to note that although fluctuating communities exhibit smaller invasion resistance than stable communities under the same conditions, stable communities can still yield smaller invasion resistance under weaker interaction strength \\( <\\alpha_{ij}> \\) or smaller species pool size \\( S \\) (Fig. 2d-f). The Lotka-Volterra model therefore explains why our diverse and fluctuating communities are susceptible to species invasion and makes new predictions regarding how invasibility would change with the size of the species pool and the strength of interspecies interactions (Fig. 2d-f).\n\nTo experimentally test the predicted dependence of invasion resistance on interaction strength and species pool size, we tuned the inter-species interaction strength by tuning the concentration of supplemented glucose and urea in the culture medium \\(^{40,51,52}\\). As discussed in our previous work \\(^{40,51,52}\\), increasing the concentration of supplemented glucose and urea leads to stronger strength of competitive interactions between bacterial species due to extensive modification of the media (e.g. pH). We measured the invasion of ~9 invader species to 15 synthetic resident communities under low nutrient (weak interaction) and 25 communities under high nutrient (strong interaction) conditions. Consistent with our theoretical predictions, we found that increasing interaction strength leads to an increase of invasion resistance in resident communities (Fig. 3a). Specifically, the invasion probability was \\( 7\\% \\pm 2\\% \\) in high nutrient conditions (strong interaction), 8 fold lower than the invasion probability of \\( 56\\% \\pm 8\\% \\) observed in low nutrient conditions (weak interaction) (Fig. 3a). We also decreased the species pool size from \\( S=20 \\) to \\( S=12 \\) and found that invasion probability increased to \\( 85\\% \\pm 6\\% \\) from \\( 56\\% \\pm 8\\% \\) in low nutrient conditions (Fig. 3b), consistent with our theoretical predictions. Our theory and\nexperiment both indicate that increasing either interaction strength or species pool size leads to a decrease in community invasibility \\(^{10,18,27-29}\\).\n\nTo unify different invasibility-richness relationships in the experiments depending upon how the richness is changed (by varying interaction strength, species pool size, or dynamical regime) (Supplementary Fig. 13), we next analyzed the dependence of invasion probability on the survival fraction of species in resident communities, defined as the fraction of species in the initial pool which survive the assembly process (on day 6 before invasion). The results show a strongly positive correlation of invasibility on survival fraction, where the correlation coefficient is 0.82 (Fig. 3c). Microbial communities cultured in low nutrient (weak interaction) media display both a larger invasion probability and larger survival fraction than communities under high nutrient (strong interaction) (Fig. 3c). Furthermore, fluctuating communities which are easier to be successfully invaded also exhibit larger survival fraction than stable communities under the same conditions (Fig. 3c and 1c). These results demonstrate that the survival fraction can serve as a unifying predictor of the invasibility of a resident community. Although it has been suggested that microbial communities with higher diversity are less likely to be invaded because they leave less available niches and resources for invaders\\(^{18,27-29}\\), our results indicate that this is only true when the diversity is increased by increasing the size of the species pool (Fig. 3c and 1c). However, if diversity is modulated by a change in interaction strength or stability then more diverse communities are instead more invasible.\n\nDespite our experimentally observed correspondence between invasion probability and survival fraction, we noted that the invasion probability for communities under high nutrient are usually lower than their survival fraction (majority of points on the bottom left (high nutrient) are below the diagonal line on Fig. 3c). In ecology, the priority effect refers to the phenomenon in which the community structure is influenced by the order and timing of species’ arrival in a community\\(^{44,45}\\). We interpret the mismatch between invasion probability and survival fraction under high nutrient as evidence of priority effects in the community assembly under strong interactions in our experiment. Under weak interactions, the colonization probability of invader species is similar with the probability of a species in the initial pool surviving the process of community assembly, whereas invader species are statistically less likely to survive in the communities than the species in the initial pool under strong interactions (Fig. 3c)\\(^{10}\\). The emergent priority effect in communities composed of strongly interacting species could be explained by alternative stable states tending to inhibit the growth of invaders at low abundance\\(^{10,40}\\).\n\nTo understand the reason for different diversity-invasibility relationships when varying interaction strength, species pool size or dynamical regime (Fig. 1c, Fig. 2 and Fig. 3), we sampled resident communities along different paths on the phase diagram (Fig. 2f). We simulated invasions to these resident communities and found different diversity-invasibility relationship along different paths (Fig. 4a). The results show a positive diversity-invasibility relationship when only varying interaction strength while fixing species pool size, or randomly sampling communities under the same parameters of species pool size and interactions (Fig. 4a). On the contrary, a reversed negative or non-monotonic diversity-invasibility relationship was observed when varying species pool size while fixing interaction strength (Fig. 4a). Despite these conflicting diversity-invasibility relationships, after scaling richness with species pool size to get the survival fraction, we found that all communities collapsed to a universal line in which the invasion probability is approximately equal to the survival fraction (Fig. 4b). The deviation from the exact collapse in small survival fraction regime (bottom left of Fig. 4b) indicates priority effect under strong\ninteraction. Our results indicate that survival fraction determines invasibility, whereas diversity-invasibility relationship can be qualitatively different depending upon the origin of different diversity in different communities.\n\nThe emergence of the priority effect in experiments (Fig. 3c) was also found in the Lotka-Volterra model under different regimes of interaction strength and species pool size. We quantified the priority effect by calculating the difference between survival fraction of resident species and the invasion probability of species that invade after the resident communities have assembled, where the difference was normalized by survival fraction (Fig. 4c). We found there is no clear priority effect in the small species pool size and weak interaction regime, where species in the initial pool and invader species display similar probability of colonizing in the communities (Fig. 4c). Consistent with our experimental results, increasing species pool size and interaction strength in the model leads to the emergence of priority effect in the phase where communities reach fluctuation or alternative stable states (Fig, 4c). We found the priority effect originated from alternative stable states or limit cycle oscillations in the strongly interacting phase, whereas chaotic fluctuations display no significant priority effect in simulation (Supplementary Fig. 14), which can be explained by its ergodicity\\(^{41,43}\\).\n\nWe also investigated the idea that successful invasions can cause strong or weak effects on resident community structure depending on how invaders interact with resident species\\(^{10,30,31}\\). Our simulations show that invasions cause stronger change on structure of resident communities under stronger interactions, where the invasion effect is measured as the proportion of change in surviving species before and after the invasion, calculated as 1 minus the ratio of overlapping species to total species (1 - (number of overlapping species / total number of species)). (Fig. 4d). To understand the effect of a successful invasion in the experiment, we analyzed the change of biomass and species composition before and after the invasions (Fig. 5). The community biomass displays relatively small changes after invasion under weak interactions (low nutrient regime, inset of Fig. 5a and Supplementary Fig. 6-7). In the strong interaction regime (high nutrient), we found that stable communities typically transitioned from low biomass states to high biomass states after successful invasions, whereas the biomass of fluctuating communities continued to fluctuate over a similar range (Fig. 5a-c and Supplementary Fig. 3-5). Averaging across both stable and fluctuating communities, we found that community biomass under strong interaction displayed a larger fold change (2.9 ± 0.8) after successful invasion than those under weak interaction (1.15 ± 0.03) (Fig. 5c). We defined the invasion effect as the fraction of surviving species that change before and after invasion. We compared the change of relative species abundance between invaded communities and control communities without adding invaders (Supplementary Fig. 15-18). This analysis on species abundances through 16S sequencing further indicated that successful invasions cause stronger change in the species compositions under strong interaction (53 % ± 6%) than weak interaction (39% ± 2%) (Fig. 5d), which is consistent with the simulation results with Lotka-Volterra model (Fig. 4d). The growth of invader species influences the community structure more dramatically when it has stronger interaction with other resident species, and the strong interplay between resident species can also cause stronger secondary effect on other resident species when their abundance change\\(^{10,47}\\).\n\nAlthough our study was primarily focused on community-level properties that determine invasibility and invasion effect, we also analyzed properties of the invader species that correlated with invasibility and invasion effect. Perhaps surprisingly, we did not observe a significant correlation between a species’ ability to invade and that species growth in monoculture\n(Supplementary Fig. 19). For example, Pseudomonas (invader 4) and Enterobacterales (invader 7) were the two most successful invader species (16/35 and 6/11 invasions, respectively), yet displayed growth in monoculture that was typical of the group of nine invaders that were tested. Bacillus (invader 6) with the highest growth rate among all invaders under both high and low nutrients, only display a small fraction of invasion success (2/37). Moreover, we also observed that Pseudomonas (invader 2) and Pedobacter (invader 3) could occasionally invade communities despite being subject to a strong Allee effect that prevented the species from growing from an initially small inoculum (Supplementary Fig. 17). Furthermore, we did not observe significant correlation between the invasion effect and invader properties either (Supplementary Fig. 20). Whether for the invasion probability of resident communities or different invaders, we found an absence of correlation between invasion probability and invasion effect (Supplementary Fig. 21). Taking these together, we therefore found that monoculture growth properties were surprisingly ineffective at predicting the success of a species as an invader, while resident community properties are the primary factors determining the invasion outcome.\n\nOur findings show that invasibility and invasion effects can be statistically predicted by simple community-level features including the community's dynamical regime, species pool size, and interaction strength. As predicted by our theory, increasing community diversity leads to stronger resistance to invaders only when varying species pool size and fixing community stability and environmental conditions (including interaction strength), which is consistent with the biotic resistance hypothesis9–11. We demonstrated that, when diversity is tied to increased dynamic fluctuations or reduced interaction strength, more diverse communities might instead exhibit decreased resistance to invasion (Fig. 1c and 3e). Our results emphasize that only by concurrently considering the effects of interaction strength and stability can the diversity of native communities be used to predict invasion resistance; diversity alone is insufficient for such predictions. By normalizing richness with species pool size, we obtained the survival fraction, a unified predictor that closely approximates invasion probability across different conditions (Fig. 3c and Fig. 4b). This survival fraction is influenced by factors such as species pool size, interaction strength, and stability (Fig. 2b, cand 3c).\n\nApplying the insights developed here to natural communities requires that we draw a parallel between the three recognized types of diversity in ecology—alpha, beta, and gamma diversity—and the three species number variables we've investigated in our study: richness, survival fraction, and species pool size53. Specifically, richness and species pool size can be seen as analogs for alpha (local diversity) and gamma (regional diversity) diversities, respectively. Beta diversity, defined as the ratio between regional and local diversity, is the reciprocal of the survival fraction. Consequently, our discovery of a universal positive relationship between invasibility and survival fraction suggests an overarching negative correlation between invasibility and beta diversity. While directly measuring the survival fraction in natural communities can be challenging, the ratio of local richness to regional richness in natural habitats may serve as a reliable approximation of survival fraction9,12,48,53, acting as a singular predictor for invasion probability. That prediction is nevertheless affected by the presence or absence of priority effects. Building upon our earlier discoveries regarding emergent phases in communities40, our current work suggests that priority effects are most pronounced in the theoretically-predicted phase of alternative stable states,\nmatching our empirical observations of stable states found under conditions of strong interactions and a large species pool (Fig. 2e and 3c).\n\nOur invasion experiments in synthetic microbial communities under controlled conditions have shown that, prior to any other feature of invader or resident species, the qualitative dynamical regime of the resident community is a central factor that informs all other predictions. The distinct regimes that we found, and the relationships between various predictions, were all compatible with a theory governed only by a few community-level parameters of (pool) diversity and interaction strength. Future work is necessary to determine whether these community-level features can predict invasion outcomes across spatiotemporal scales, environmental conditions, and organism types.\n\n![Diagram showing experimental setup for synthetic microbial communities, including steps such as dispersal, dilution, inoculation, growth, invasion, and measurement techniques.](page_186_495_1207_312.png)\n\n![Diagram showing a phylogenetic tree of resident communities and invader species.](page_186_819_377_181.png)\n\n![Scatter plot showing invasion probability vs. richness of resident community.](page_563_819_377_181.png)\n\n![Line graph showing biomass over time for fluctuation and stable communities.](page_940_819_377_181.png)\n\n![Line graphs showing relative species abundance before and after invasion for stable and fluctuating communities.](page_186_1143_377_181.png)\n\n![Line graph showing relative species abundance before and after invasion for fluctuating community.](page_563_1143_377_181.png)\n\n![Bar chart comparing invasion probability between stable and fluctuation communities.](page_940_1143_377_181.png)\n\nFig 1. Experiments using synthetic microbial communities show that the invasion probability in fluctuating communities is higher than stable ones, leading to a positive diversity-invasibility relationship. a, We used a library of bacteria to generate different synthetic communities with S=20 species in the pool (under “high” nutrient conditions; see supplement).\nCommunities underwent serial daily dilutions with additional dispersal from the pool. We introduced invader species to the resident communities on day 6 and continued to apply daily dispersal of invaders. Community composition and total biomass were monitored via 16S sequencing and optical density (OD). b, We formed 17 resident communities with different sets of species (S=20). We added invader species outside the pool into the resident communities on day 6, and then measured the community compositions and biomass on day 12 to determine the outcome and effect of the invasions. c, The invasion probability of resident communities positively correlate with their richness (correlation coefficient=0.51). d, 8 out of the 17 resident communities reach fluctuation in biomass (orange) and the rest 9 communities reach stable states (purple). e, Representative time course of relative species abundance via 16S sequencing show the stable community was not invaded. f, Representative time course of relative species abundance shows the invader successfully invade and grow in the fluctuating community. g, The invasion probability to fluctuating resident communities is statistically higher than that to stable communities (p=0.016, the number of invasion tests is n=61 (60) for fluctuating (stable) communities. Error bars represent s.e.m..\n\n![Representative time series of species abundance in simulation showing diverse invasion dynamics and outcome](page_184_370_1012_1012.png)\n\nFig 2. The Lotka-Volterra model predicts a decrease of invasion probability when stability, interaction strength and species pool size of resident communities increase. a, Representative time series of species abundance in simulation show diverse invasion dynamics and outcome: invader species failed to grow in the community (top left panel, the black curve represents invader);\ninvader grow and only cause small effect on community composition (top right panel); invader successfully invade and cause large change on community composition (bottom left panel); invasion to a fluctuating resident community (bottom right panel) (\\( = 0.6, S=32 \\)). **b**, Consistent with experiments (Fig. 1c), the invasion probability of simulated resident communities positively correlates with their richness, which arises because fluctuating communities are more diverse and more invasible. **c**, The invasion probability to fluctuating resident communities is statistically higher than that to stable communities (p < 0.001). **d**, Increasing species pool size leads to a decrease in invasion probability. Fluctuating communities (orange points) exhibit higher invasion probability than stable communities (purple points). **e**, Increasing interaction strength leads to a decrease in invasion probability. **f**, Increasing species pool size and interaction strength leads to a decrease in invasion probability. The curves and color maps depict the mean value over 1000 simulations.\n\n![Three panels showing invasion probability vs. nutrient fluctuation, species pool size, and survival fraction](page_489_728_654_496.png)\n\nFig 3. Increasing interaction strength and species pool size leads to higher invasion resistance of resident communities in experiment. **a**, The invasions to resident communities under low nutrient (weak interaction) exhibit statistically higher invasion probability than communities under high nutrient (strong interaction) (p < 0.001, the number of invasion tests is n=120 (39) for high (low) nutrient). **b**, The invasions to resident communities under smaller species pool size (S=12) exhibit statistically higher invasion probability than communities under larger species pool size (S=20) (p = 0.007, the number of invasion tests is n=39 (34) for S=20 (12), all communities were cultured under low nutrient). Error bars represent s.e.m.. **c**, The invasion probability positively\ncorrelates with survival fraction (before invasion) across different communities and nutrient conditions (each point represents one community; correlation coefficient is 0.82). The points corresponding to communities under high nutrient are below the diagonal line, showing the invasion probability of communities under high nutrient are generally smaller than their survival fraction, which indicates the priority effect under strong interaction strength.\n\n![Four panels showing invasion probability vs richness, invasion probability vs survival fraction, priority effect, and effect on resident community](page_312_495_1067_627.png)\n\nFig 4. The Lotka-Volterra model predicts a universal correspondence between invasion probability and survival fraction, the emergence of priority effects and stronger invasion effects when increasing interaction strength. **a**, The dependence of invasion probability on final richness of resident communities is qualitatively different depending upon how the richness is changed. Invasion probability positively correlates with richness when varying interaction strength or when randomly sampling communities with a fixed species pool size and interaction strength distribution. Invasion probability can decrease with community diversity when varying species pool size. **b**, Invasion probability is approximately equal to the survival fraction of species in the resident communities, no matter how we change richness, species pool or interaction strength. **c**, Increasing species pool size and interaction strength leads to the emergence of priority effect, where the invasion probability of resident communities is smaller than their species survival fraction. **d**, Successful invasions cause larger effect on species composition in the resident communities under stronger interaction strength. The curves depict the mean value over 1000 simulations.\nFig 5. Increasing interaction strength leads to a stronger effect on resident communities under invasion success. a, The stable communities under high nutrient experienced a large increase in biomass after successful invasions (dark purple curves). Inset shows the invasions under low nutrient only cause weak effect on community biomass as compared with high nutrient. b, The time course of fluctuating community biomass under high nutrient before invasion and after invasion, where dark and light orange curves represent successful and failed invasions, respectively. c, The invasions to resident communities under low nutrient (weak interaction) cause statistically lower fold change of biomass than communities under high nutrient (strong interaction) (p < 0.001, the number of successful invasions is n=51 (11) for low (high) nutrient). 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Click to download.\n\n• SupplementaryMaterials.pdf"} {"paper_id": "prb29", "title": "Data-driven prediction of colonization outcomes for complex microbial communities", "text": "Data-driven prediction of colonization outcomes for complex microbial communities\n\nLu Wu\nShenzhen Institute of Advanced Technology, Chinese Academy of Sciences\n\nXu-Wen Wang\nHarvard Medical School https://orcid.org/0000-0001-7670-3544\n\nZining Tao\nShenzhen Institute of Advanced Technology, Chinese Academy of Sciences\n\nTong Wang\nBrigham and Women’s Hospital and Harvard Medical School\n\nWenlong Zuo\nShenzhen Institutes of Advanced Technology, Chinese Academy of Sciences https://orcid.org/0000-0001-6557-410X\n\nYu Zeng\nShenzhen Institute of Advanced Technology, Chinese Academy of Sciences\n\nYang-Yu Liu\nHarvard Medical School https://orcid.org/0000-0003-2728-4907\n\nLei Dai\nlei.dai@siat.ac.cn\n\nShenzhen Institute of Advanced Technology, Chinese Academy of Sciences https://orcid.org/0000-0002-5598-5308\n\nBiological Sciences - Article\n\nKeywords:\n\nPosted Date: August 24th, 2023\n\nDOI: https://doi.org/10.21203/rs.3.rs-2864317/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: There is NO Competing Interest.\nVersion of Record: A version of this preprint was published at Nature Communications on March 16th, 2024. See the published version at https://doi.org/10.1038/s41467-024-46766-y.\nData-driven prediction of colonization outcomes for complex microbial communities\n\nLu Wu1,*, Xu-Wen Wang2,*, Zining Tao1,3, Tong Wang2, Wenlong Zuo1, Yu Zeng1, Yang-Yu Liu2,4,#, Lei Dai1,5,#\n\n1CAS Key Laboratory of Quantitative Engineering Biology, Shenzhen Institute of Synthetic Biology, Shenzhen Institute of Advanced Technology, Chinese Academy of Sciences, Shenzhen 518055, China.\n2Channing Division of Network Medicine, Department of Medicine, Brigham and Women’s Hospital and Harvard Medical School, Boston, MA, 02115, USA.\n3Shandong Agricultural University, Tai’an 271000, China.\n4Center for Artificial Intelligence and Modeling, The Carl R. Woese Institute for Genomic Biology, University of Illinois at Urbana-Champaign, Champaign, IL 61820, USA\n5University of Chinese Academy of Sciences, Beijing 100049, China.\n\n*These authors contributed equally to this work\n#Corresponding author: yy1@channing.harvard.edu (Y.Y.L.), lei.dai@siat.ac.cn (L.D.)\nAbstract\n\nComplex microbial interactions can lead to different colonization outcomes of exogenous species, be they pathogenic or beneficial in nature. Predicting the colonization of exogenous species in complex communities remains a fundamental challenge in microbial ecology, mainly due to our limited knowledge of the diverse physical, biochemical, and ecological processes governing microbial dynamics. Here, we proposed a data-driven approach independent of any dynamics model to predict colonization outcomes of exogenous species from the baseline compositions of microbial communities. We systematically validated this approach using synthetic data, finding that machine learning models (including Random Forest and neural ODE) can predict not only the binary colonization outcome but also the post-invasion steady-state abundance of the invading species. Then we conducted colonization experiments for two commensal gut bacteria species Enterococcus faecium and Akkermansia muciniphila in hundreds of human stool-derived in vitro microbial communities, confirming that the data-driven approach can successfully predict the colonization outcomes. Furthermore, we found that while most resident species were predicted to have a weak negative impact on the colonization of exogenous species, strongly interacting species could significantly alter the colonization outcomes, e.g., the presence of Enterococcus faecalis inhibits the invasion of E. faecium. The presented results suggest that the data-driven approach is a powerful tool to inform the ecology and management of complex microbial communities.\nIntroduction\n\nMicrobial communities are constantly exposed to the invasion of exogenous species, which can significantly alter their composition and function (1-4). The capacity of a microbial community to resist invasion is regarded as an emergent property (i.e., from individual parts to a holistic function) arising from the complex interactions among its constituent species (5). Theoretical studies have found that communities with higher diversity or stronger interaction strengths among species are more resistant to potential invaders (6-8), attributed to the fact that communities with higher diversity can occupy more niches and provide functional redundancy, making it more difficult for an invading species to establish and thrive.\n\nThe role of host-associated microbiota in defending against pathogens has been extensively studied (9-12), particularly in the context of the human gut microbiome. For the human gut microbiome, invasion of resident microbial communities can occur when non-resident bacteria from foods and the upper gastrointestinal tract reach the gut ecosystem (13, 14). The resident microbes in the gut ecosystem outcompete and exclude invaders through a combination of mechanisms, such as producing antimicrobial compounds (15, 16), competing for nutrients and space (17-20), and modulating the host's immune response (21, 22). However, the composition of the human gut microbiota can vary significantly across individuals (23, 24) and over time (25, 26). Dietary shifts, medication, and other environmental factors can greatly alter the composition of the gut microbial community (27, 28). These interpersonal and dynamic variations in the gut microbiome can lead to significantly different colonization outcomes, such as resistance to pathogens (29, 30) and probiotics (31, 32). For example, antibiotics treatment often leads to a loss of diversity and promotes the invasion of exogenous species (30, 33). The ability to predict and alter the colonization outcomes (i.e., prevent the engraftment of pathogens and promote the engraftment of probiotics) is critical for personalized microbiota-based interventions in nutrition and medicine.\n\nDespite the accumulating empirical studies, predicting the colonization outcomes in complex communities, such as the human gut microbiome, remains a fundamental challenge due to limited knowledge of interspecies interactions. For a meta-community of \\( N \\) species (\\( N \\) ranges from hundreds to thousands for the human gut microbiome), we would need to isolate and culture all these species (which is already a formidable task) and conduct a considerable number of experiments to map pairwise interactions (on the order of \\( \\sim O(N^2) \\)), not to mention higher-order interactions. Thus, novel approaches are needed to study the ecology of highly complex communities.\n\nThe key question is: can we achieve system-level predictions for complex ecological systems\nwithout requiring detailed mechanistic information? Colonization outcome can be viewed as a mapping from the community structure of a complex ecological system (i.e., the pre-invasion community profile) to its function (i.e., the post-invasion abundance of the invading species). Recently, the application of data-driven models (machine learning and deep learning) has shown great promise in predicting the emergent properties of complex biomolecules, such as protein structure (mapping from protein sequence to structure) (34), promoter strength (mapping from DNA sequence to function) (35). In contrast, this paradigm shift to data-driven approaches has received much less attention in ecology (36).\n\nHere, we proposed a data-driven approach to predict colonization outcomes of exogenous species in complex microbial communities. First, we systematically evaluated the approach using synthetic data generated by classical ecological dynamical models. We found that, with sufficient sample size in training data (on the order of \\( \\sim O(N) \\)), the colonization outcomes (i.e., whether an exogenous species can engraft and what its abundance would be if it can engraft) can be accurately predicted by machine learning models. Then, we generated large-scale datasets with *in-vitro* experimental outcomes of two representative species (*E. faecium* and *A. muciniphila*) colonizing human stool-derived microbial communities. We validated that machine-learning models, including Random Forest and neural ODE, can accurately predict the colonization outcomes in experiments. Finally, we used the machine learning models to infer species with large colonization impacts and experimentally demonstrated that the introduction of strongly interacting species can significantly alter the colonization outcomes. Our results suggest that the function of complex microbial communities is predictable and tunable via the data-driven approach.\n\n**Results**\n\n**The data-driven approach of predicting colonization outcomes for complex microbial communities**\n\nLet’s consider a meta-community with a pool of \\( N \\) microbial species, denoted as \\( \\Omega = \\{1, \\cdots, N\\} \\). Consider a large set of \\( M \\) microbiome samples, denoted as \\( \\mathcal{S} = \\{1, ..., M\\} \\), collected from this meta-community. A microbiome sample \\( s \\in \\mathcal{S} \\) can be considered as a local community of the meta-community with a subset of coexisting species (**Fig.1A**). For a local community \\( s \\), if an exogenous species-*i* (still in the species pool \\( \\Omega \\), but not in \\( s \\)) is introduced to \\( s \\), whether it can successfully colonize the community or not, as well as its post-invasion abundance \\( x_i \\), will depend on the baseline composition of \\( s \\). For example, it is easier (or harder) for species-*i* to colonize \\( s \\) if some resident species strongly promote (or inhibit) its growth of species-*i*, respectively. Hereafter, we call the community \\( s \\) *permissive* (or *resistant*) to species-*i* if species-*i* can (or cannot) successfully colonize \\( s \\), respectively. If we only have the information about species-*i* and a\ncommunity \\( s \\), it may seem impossible to accurately predict the colonization outcome without detailed knowledge about microbial interactions. However, if we have access to the data from colonization experiments of many local communities, then, in principle, we can formalize the colonization outcome prediction problem as a machine-learning task that can be solved in a data-driven fashion. To ensure the problem is mathematically well-defined, we must assume that the different local communities in this meta-community share identical assembly rules and microbial interactions (37). This way, the colonization outcomes of some local communities can be used to train a machine-learning model to predict the colonization outcomes of other local communities.\n\nConsider species-\\( i \\) as the exogenous species to a local community \\( s \\). Note that the baseline abundance of species-\\( i \\) is zero (i.e., \\( x_i^{(0)} = 0 \\)) in \\( s \\) before the invasion. With some initial abundance, the exogenous species will interact with the resident species in \\( s \\), and its post-invasion steady-state abundance is denoted as \\( x_i^{(1)} \\). We propose to solve the Colonization Outcome Prediction (COP) problem using machine-learning models that treat the baseline (i.e., pre-invasion) taxonomic profile \\( \\mathbf{x}^{(0)} \\) as inputs and the steady state abundance of the invasive species \\( x_i^{(1)} \\) as output (**Fig.1B**). Mathematically, we intend to learn the mapping from the baseline taxonomic profile of a community \\( \\mathbf{x}^{(0)} \\) to the steady state abundance of the invading species \\( x_i^{(1)} \\), i.e., \\( \\varphi : \\mathbf{x}^{(0)} \\mapsto x_i^{(1)} \\). In addition, this mapping could help us infer the impact of each resident species on the colonization of the exogenous species.\n\nWe conducted *in silico* simulations to validate the feasibility of our approach. We generated synthetic data of colonization outcomes using the Generalized Lotka-Volterra (GLV) model with \\( N = 100 \\) species in the meta-community (see **Methods**). The initial species collection of each sample (i.e., a local community) consists of 30 species randomly drawn from the (\\( N - 1 \\)) species pool (the exogenous species is absent in all the local communities). We generated the baseline profiles of local communities by running the GLV dynamics to a steady state. The exogenous species was then added to each local community, and its post-invasion abundance was obtained by running the GLV dynamics to a new steady state.\n\nWe can formalize COP as two sub-problems: (1) *Classification*: predict whether an exogenous species can colonize a local community; (2) *Regression*: predict the steady-state abundance of an exogenous species after colonization. Using the synthetic data generated by the GLV model, we first addressed the *classification* problem, i.e., predicting whether the invading species can colonize a community. We employed three models covering representative categories of machine learning: Logistic Regression, Random Forest classifier, and COP-Neural Ordinary Differential Equations (COP-NODE) classifier (see **Methods**). We tuned the complexity of the ecological network (i.e., network connectivity) and evaluated the performance of different models at varying\nlevels of the training sample size (**Fig.1C-E**). Here, the network connectivity represents the probability of two species in the species pool interacting with each other. As expected, we observed that the predictive performance of machine learning models improved with the number of training samples. For network connectivity \\( C = 0.3 \\), we found that the Area Under the Receiver Operating Characteristic curve (AUROC) of three machine learning models was above 0.9 with training sample size \\( S_{\\text{train}} = N \\). For higher network connectivity (e.g., \\( C = 0.4 \\) and 0.5), the increased complexity in inter-species interactions rendered the binary prediction of colonization outcomes more difficult. Nevertheless, with a sample size on the order of \\( \\sim O(N) \\)), machine learning models were able to achieve accurate classification of colonization outcomes in synthetic data (AUROC > 0.8).\n\nNext, we addressed the *regression* problem, i.e., predicting the steady-state abundance of the exogenous species. For the GLV model, our analytical derivations discovered a surprisingly simple linear relation between the post-invasion abundance of the exogenous species and the pre-invasion abundance of resident species (Supplementary Text, **Fig.S1**). Although the linear relation doesn’t hold for other dynamical models, it suggests that learning the mapping for COP is feasible by the data-driven approach, and the number of parameters required for fitting the relation is on the order of \\( \\sim O(N) \\). We employed three machine learning models: Elastic Net Linear Regression, Random Forest regressor, and COP-NODE regressor (**Fig.1F-H**). The predictive performance was evaluated with Pearson’s correlation coefficient between the predicted and true abundance (log-transformed). We systematically examined the predictive performance of three models at varying levels of network connectivity and training sample size. Similar to the classification problem, we found that increasing network connectivity \\( C \\) rendered the regression problem more difficult. For training sample size \\( S_{\\text{train}} = 2N \\) or higher, there was a substantial improvement in the quantitative prediction of the post-invasion abundance.\n\n**Generation of human stool-derived *in vitro* microbial communities with diverse compositional profiles**\n\nTo systematically study colonization outcomes in complex microbial communities, we established large-scale cultivation of human stool-derived *in vitro* communities in multi-well plates (38-41) (**Fig.2A**, *Methods*). Briefly, we cultured gut microbial communities derived from 24 donors to reach steady states after five rounds of serial passaging *in vitro*. To increase the diversity in baseline communities, we treated each donor’s sample with 12 antibiotics from different classes (**Table S1**). Overall, we obtained more than 300 baseline communities with substantial variation in the compositional profiles at the species level (**Fig.2B**, **Fig.S2-S3**). The compositional profiles of the baseline communities were stable, with around 40 to 120 co-existing species in each community (**Fig.S4**).\nFor the invasion experiments, we would introduce an exogenous species into the baseline communities and determine its colonization outcome after 8-10 rounds of serial passaging (Fig.2C). We conducted a preliminary experiment to investigate the colonization outcome of different exogenous species (Fig.S5). We found that E. faecium, A. muciniphila, and F. nucleatum could successfully colonize in some communities at varying levels of post-invasion abundance. In contrast, S. salivarius, B. breve, and Lactobacillus spp. could not colonize in nearly all the communities we tested. Moreover, vancomycin treatment significantly altered the colonization outcomes, rendering the gut microbial communities more susceptible to invasion (Fig.S5C). Overall, our results support the use of human stool-derived in vitro communities as a model experimental system for studying colonization outcomes.\n\nColonization outcome of E. faecium in human stool-derived in vitro communities is baseline-dependent and predictable\n\nWe selected E. faecium as a representative species for colonization experiments in human stool-derived in vitro communities. E. faecium is a Gram-positive bacterium that inhabits the gut of humans and other animals. Some E. faecium strains have probiotic potential (42), and recent studies suggest that it plays a positive role in cancer immunotherapy (43, 44). On the other hand, some E. faecium strains cause opportunistic infections in hospitalized patients with disrupted gut microbiota (45).\n\nWe introduced E. faecium to ~300 baseline communities (Fig.S2) at a dose of 5% relative to the total abundance of resident species. We passaged all communities for ten rounds to reach the post-invasion steady state (Methods). We observed that the colonization outcome of E. faecium in different communities was persistent during serial passaging (Fig.S6). In addition, the composition of in vitro communities before and after E. faecium invasion is highly reproducible across three replicates (Fig.S7).\n\nWe found that E. faecium was able to colonize 32% of baseline communities (i.e., permissive), with its post-invasion abundance in permissive communities varying over two orders of magnitude (Fig.3A). Previous studies suggested that community biomass and diversity are important factors underlying the colonization resistance to exogenous species (46, 47). For example, reduced diversity of the resident community is often linked to pathogen infection in the human gut or other ecosystems (48). Indeed, we found that the biomass and species richness of the baseline communities exhibited a clear negative correlation with the post-colonization abundances of E. faecium (Fig.S8). The diversity of the E. faecium permissive communities was significantly lower than the resistant communities (Fig.3B-C). Furthermore, we observed a significant difference\nbetween the composition of *E. faecium* permissive communities and resistant communities (**Fig.3D**). The colonization success of *E. faecium* was highly baseline-dependent, with substantial variations across different donors and antibiotics treatments (**Fig.S9**).\n\nTo predict the binary colonization outcomes (permissive vs. resistant) of *E. faecium*, we employed three machine learning models, including Logistic Regression, COP-NODE classifier, and Random Forest classifier (**Fig.3E-G**, **Fig.S10**). For 6-fold cross-validation, we used the communities derived from 20 donors (~240 samples) to train the model and the communities derived from the remaining 4 donors (~60 samples) to evaluate the model. Random Forest classifier displayed the best performance in predicting whether *E. faecium* could successfully colonize based on the species-level community composition (AUROC=0.86), followed by COP-NODE classifier (AUROC=0.81) and Logistic Regression (AUROC=0.71). Thus, our colonization experiments of *E. faecium* in complex human gut microbial communities validated that the data-driven approach can solve the classification problem of COP.\n\n**Colonization outcome of *A. muciniphila* is quantitatively predictable**\n\nTo investigate the generality of our approach, we selected *A. muciniphila* as a second representative species for colonization experiments in human stool-derived *in vitro* communities. *A. muciniphila* is a Gram-negative mucin-degrading bacterium that inhabits the human gut. Due to its potential beneficial effects on human health (49-51), *A. muciniphila* is considered a promising probiotic candidate (52). *A. muciniphila* is found in the gut microbiome of around 30% of adults, and its abundance varies substantially across individuals (53). Similar to the experimental design of *E. faecium*, we introduced *A. muciniphila* to ~300 baseline communities at a dose of 5% relative to the total abundance of resident species and passaged all communities for eight rounds to reach the post-invasion steady state. The colonization outcome of *A. muciniphila* in different communities was persistent during serial passaging (**Fig.S11**), and the composition of *in vitro* communities post *A. muciniphila* invasion is highly reproducible across three replicates (**Fig.S12**).\n\nOverall, we found substantial variations in the post-invasion steady-state abundance of *A. muciniphila* across different donors and antibiotics treatments (**Fig.S13**). *A. muciniphila* could colonize in 93.6% of baseline communities (i.e., permissive). For permissive communities, the post-invasion abundance of *A. muciniphila* displayed a bimodal distribution (**Fig.4A**). We classified the permissive communities into two subgroups (high vs. low), depending on the post-invasion abundance of *A. muciniphila* (abundance threshold at \\(10^{-2}\\)). The Shannon diversity (**Fig.4B**) and species richness (**Fig.4C**) of the *A. muciniphila* high permissive communities were significantly lower than those of the low permissive communities, and there was a significant difference between the community composition of the two groups (**Fig.4D**).\nWe evaluated the performance of machine learning models in predicting the colonization outcome of *A. muciniphila*, both qualitatively (classification) and quantitatively (regression). Random Forest classifier displayed the best performance in binary classification (high permissive vs. low permissive of *A. muciniphila*) based on the species-level community composition (AUROC=0.84), followed by COP-NODE classifier (AUROC=0.79) and Logistic Regression (AUROC=0.74) (**Fig.4E-G**). To quantitatively predict the post-invasion abundance of *A. muciniphila*, we employed three machine learning models: Elastic Net Linear Regression, COP-NODE regressor, and Random Forest regressor (**Fig.4H-J**, **Fig.S14**). In comparison to the other two methods, the Random Forest regressor achieved the highest accuracy in quantitative prediction (Pearson’s correlation coefficient between the predicted and true abundances \\( R = 0.74, p < 2.2 \\times 10^{-16} \\)) and successfully recapitulated the bimodal distribution in the abundance of *A. muciniphila*. Taken together, we demonstrated the generality of the data-driven approach in predicting baseline-dependent colonization outcomes for complex microbial communities.\n\n**Colonization impact in simulated and experimental communities**\n\nLearning the mapping from the baseline taxonomic profile to colonization outcomes can help us infer the impact of each resident species on the colonization of the exogenous species (**Fig.1B**). To compute the colonization impact of regression (classification), we can perform a thought experiment by introducing a perturbation in the abundance of the resident species, and use the trained machine learning model to predict the new colonization outcome of invading species after the perturbation (**Fig.5A**). Negative colonization impact means that a resident species inhibits the colonization of the exogenous species in a given local community. In GLV simulations, while the colonization impact of resident species was randomly distributed (**Fig.5B**), we found that the median colonization impact of a resident species across different local communities was positively correlated to its interaction strength on the exogenous species (Spearman correlation coefficient \\( \\rho = 0.73, p < 2.2 \\times 10^{-16} \\), **Fig.5C**), suggesting that we may use colonization impact to identify strongly interacting species.\n\nWe used the Random Forest model to evaluate the colonization impact of all species in human stool-derived *in vitro* communities on *E. faecium* and *A. muciniphila* (**Fig.5D-G**). We inferred that most resident species had a weak negative colonization impact (**Fig.5D and 5F**). Based on the median colonization impact of a certain resident species across different local communities, we identified the top-ranking species with negative colonization impact (**Fig.5E and 5G**). Colonization impact on *A. muciniphila* was overall less negative than *E. faecium*, consistent with our observation that human gut microbial communities were more permissive to *A. muciniphila* colonization.\nThe impact of strongly interacting species on colonization outcomes\nTo understand the role of strongly interacting species on colonization outcomes, we systematically studied the impact of E. faecalis on the colonization of E. faecium. E. faecalis was inferred to have the strongest colonization impact on E. faecium across different baseline communities (Fig.5E). We observed a statistically significant negative correlation between the abundance of E. faecalis in baseline communities and the post-invasion abundance of E. faecium (Kendall’s \\( \\tau = -0.37, p = 5.29 \\times 10^{-16} \\)). In particular, baseline communities derived from some donors (e.g., S10, S07) had a high abundance of E. faecalis and were resistant to E. faecium colonization (Fig.6A).\n\nWe found that E. faecalis inhibited the growth of E. faecium in pairwise co-culture, either in liquid culture or on agar plates (Fig.S15). Then, we introduced E. faecalis into eight human stool-derived in vitro communities that were permissive to E. faecium invasion, using three different types of interventions (Fig.6B-D, Fig.S16A): 1) add E. faecalis into the baseline community, followed by E. faecium on the next day; 2) add E. faecalis and E. faecium on the same day; 3) add E. faecium into the baseline community, followed by E. faecalis on the next day. In the control group, we only added E. faecium. In all three intervention groups, the colonization of E. faecium was significantly inhibited by E. faecalis across different baseline communities. Also, the inhibitory effect was consistent for two different E. faecalis strains isolated from human stool samples (Methods). In comparison, Clostridium symbiosum, a species predicted to have a neutral impact, did not alter the colonization of E. faecium (Fig.S16B).\n\nFinally, we explored if the strong inhibition of E. faecalis on E. faecium could be shaping their distribution in the human gut via priority effects, i.e., the gut microbiome colonized with E. faecalis becomes resistant to E. faecium. We performed metagenomic sequencing of ~120 healthy volunteers in the SIAT cohort (Methods), whose samples were used to derive the in vitro communities and isolate the Enterococcus strains in this study. Indeed, there was a statistically significant negative correlation between the relative abundance of E. faecalis and E. faecium in the SIAT cohort (Kendall correlation \\( \\tau = -0.36, p = 0.0044 \\), Fig. S17A). A similar pattern was observed in gut metagenomic samples of four independent cohorts (Kendall correlation \\( \\tau = -0.36, p = 5.439 \\times 10^{-15} \\)), Fig. S17B).\n\nOverall, our experimental validations and analysis suggest that data-driven models can infer species with strong colonization impact and guide the modulation of resident communities to alter the colonization outcomes of exogenous species.\nDiscussion\n\nHere we proposed and systematically validated a data-driven approach to predict colonization outcomes of exogenous species, providing a powerful tool to inform the management of complex ecosystems. Pairwise co-culture (47, 54-56) and synthetic communities (17, 57, 58) have been widely used to study the ecology and function of microbial communities. These experiments require the isolation and cultivation of individual species, thus are often limited to simple communities. In comparison, our approach is based on sampling an ensemble of complex communities (~100 species, Fig.S4) and using the sampled communities to infer the mapping between community composition and colonization outcomes (59). We demonstrate that the data-driven approach enables accurate function prediction and system-level understanding of complex microbial communities.\n\nUnderstanding the colonization resistance of complex communities is a fundamental question in ecology. In our large-scale invasion experiments (~300 local communities and two different exogenous species), we found that resistance to exogenous species was positively correlated to community diversity, supporting the view that colonization resistance is an emergent property of complex communities (8). While most resident species had a weak negative impact on the colonization of exogenous species, we identified E. faecalis as a strong inhibitor of E. faecium. We validated that introducing strongly interacting species into baseline communities can alter the colonization outcomes. It should be noted that the colonization impact is dependent on the community context (Fig.5), because it takes into account both direct and indirect effects on the invading species (60), as well as potential higher-order interactions (61, 62). Previous studies have shown that strongly interacting species can lead to priority effects (63), with important implications for community assembly in the infant gut microbiome and the formation of community types (64, 65). Moreover, strongly interacting species can be used to modulate the resident communities to prevent the colonization of pathogens (16) or facilitate the colonization of beneficial microbes (e.g., probiotics, crop fertilizers) (66).\n\nOur results suggest that the colonization resistance of microbial communities is predictable and tunable via the data-driven approach, given that training data size is sufficient (on the order of ~\\( O(N) \\)). The high-throughput cultivation of gut microbial communities *in vitro* provides a powerful approach to studying the human gut microbiome (67, 68). In our experiments, the number of species in the meta-community was ~160, and we profiled ~300 baseline communities for proof-of-concept validation. Meeting the sample size requirement for gnotobiotic plants is feasible (69, 70). However, it could be challenging to gather sufficient training data for gnotobiotic animals and human cohort studies, depending on the complexity of the meta-community. In addition to data\nsize, another critical concern is the technical variability in large-scale experiments (71). In future studies, experimental workflows can be automated to minimize technical variability and ensure data quality for training machine learning models.\n\nOur study has several limitations. First, we did not account for potential variations at the strain level (72). Previous studies have shown that the strength of interspecies interactions can vary across different strains, such as the inhibition of Klebsiella pneumoniae by Klebsiella oxytoca (16, 73). We also observed strain-level variations in the inhibition of E. faecium by E. faecalis (Fig.6), and the underlying mechanism remains to be elucidated. Second, our invasion experiments in vitro did not reflect host-mediated interactions, which also contribute to colonization resistance in vivo (22). Nevertheless, the higher permissiveness to A. muciniphila than E. faecium in human gut microbial communities in vitro is consistent with the higher prevalence of A. muciniphila in metagenomic samples (53, 74). Third, we assumed that there was a single post-invasion steady state in simulated and experimental communities. The colonization outcomes may be influenced by multi-stability in microbial communities, e.g., successful colonization depends on the initial abundance of the invading species (75, 76).\n\nOur data-driven approach is independent of any dynamics model to predict colonization outcomes of exogenous species for complex microbial communities without detailed knowledge of the underlying ecological and biochemical process. We anticipate that the data-driven approach can be generalized to predict and engineer the function of microbial communities (i.e. mapping from community composition to function) (36, 77-79). 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Schloss, Antibiotic-Induced Alterations of the Murine Gut Microbiota and Subsequent Effects on Colonization Resistance against Clostridium difficile. mBio 6, e00974 (2015).\n78. A. Sanchez et al., The community-function landscape of microbial consortia. Cell Syst 14, 122-134 (2023).\n79. R. L. Clark et al., Design of synthetic human gut microbiome assembly and butyrate production. Nat Commun 12, 3254 (2021).\n80. N. T. Baxter et al., Dynamics of Human Gut Microbiota and Short-Chain Fatty Acids in Response to Dietary Interventions with Three Fermentable Fibers. mBio 10, (2019).\n81. J. Suez et al., Personalized microbiome-driven effects of non-nutritive sweeteners on human glucose tolerance. Cell 185, 3307-3328 e3319 (2022).\nAcknowledgments\nWe thank Na Li and volunteers at Shenzhen Institute of Advanced Technology (SIAT) for stool sample collection. We thank Zepeng Qu and Zhenkun Zhang for isolating human gut bacterial strains. We thank Prof. Jiachao Zhang at Hainan University for providing probiotic strains. We thank Huaijie Hao and Yan Tan at Xbiome for providing help with the anaerobic workstation. We thank Shenzhen Infrastructure for Synthetic Biology and Chaobi Lei for providing support in DNA extraction. We thank Zheng Sun, Chen Liao, Hongbin Liu, Lanxiang Wang, and colleagues at SIAT for valuable discussions.\n\nFunding\nL.D. acknowledges support from the National Key R&D Program of China (2019YFA0906700), the National Natural Science Foundation of China (31971513), and Shenzhen Key Laboratory for the Intelligent Microbial Manufacturing of Medicines (ZDSYS20210623091810032). Y.Y.L. acknowledges grants from the National Institutes of Health (R01AI141529, R01HD093761, RF1AG067744, UH3OD023268, U19AI095219, and U01HL089856). L.W. acknowledges support from the National Natural Science Foundation of China (32100089).\n\nAuthor contributions\nL.D., Y.Y.L., L.W., and X.W.W. conceived the presented idea, designed the project, interpreted the results, and wrote the manuscript. X.W.W. implemented in silico simulations, machine learning models, and analytical derivations. L.W. and Z.T. performed the in vitro experiments. Y.Z. assisted in experiments. L.W. analyzed the experimental data. T.W. discussed the results and revised the manuscript. W.Z. assisted in data analysis and interpretation. All authors approved the final manuscript. L.D. and Y.Y.L. provided supervision and resources for this study.\n\nCompeting interests\nAll authors declare no competing interests.\n\nData availability\nAll sequencing data generated in this study are available from European Nucleotide Archive (ENA) under study accession number PRJEB60398.\n\nCode availability\nThe code for simulations and data analysis is available at https://github.com/spxuw/COP.\nFigure 1. Prediction of colonization outcomes for complex microbial communities via the data-driven approach. (A) Each individual’s microbiome can be viewed as a local community, a subset of the meta-community of microbial species. For an exogenous species that invades the local communities, its colonization outcome (e.g., permissive or resistant) can be highly personalized, depending on the composition of local communities. (B) Colonization outcome prediction (COP) can be solved by learning the mapping from the baseline taxonomic profile to the post-invasion abundance of the exogenous species (i.e., \\( \\varphi : x^0 \\mapsto x^1 \\)). (C-E) Evaluation of the data-driven approach in solving the classification task of COP. AUROC of three machine learning models, including Logistic Regression (LR), COP-Neural Ordinary Differential Equations\nclassifier (NODE), and Random Forest classifier (RF). **(F-H)** Evaluation of the data-driven approach in solving the regression task of COP. Pearson correlation between the true abundance and the abundance predicted by three machine learning models, including Elastic Net Linear Regression (ENET), COP-NODE regressor (NODE), and Random Forest regressor (RF).\nFigure 2. Large-scale invasion experiments in human stool-derived in vitro microbial communities. (A) Schematic representation of in vitro culture of human stool-derived microbial communities in 96-well plates (Methods). Stool samples from 24 donors were treated with 12 different antibiotics for 24 h. The control group was not treated with antibiotics. All communities were passaged five times to reach a stable state, i.e., baseline community profiles (green dot) (B). Exogenous species was introduced on Day 6. After 8-10 times of passaging, the end-point community profiles (red dot) were sequenced to determine the colonization outcome (C).\nFigure 3. The colonization outcome of E. faecium in human stool-derived in vitro microbial communities is baseline-dependent and predictable. (A) The distribution of E. faecium colonization outcomes across permissive communities (colored in red). The abundance of E. faecium in resistant communities is below the detection threshold and not shown. Inset: Percentage of permissive (red) and resistant communities (gray) based on E. faecium colonization outcomes. (B-C) Shannon diversity and species richness of E. faecium resistant and permissive communities (****p < 0.0001, Mann-Whitney U-tests). (D) Principal component analysis (PCoA) based on the Bray-Curtis dissimilarity of the compositional profiles of baseline communities. The difference between permissive and resistant communities was significant (PERMANOVA Adonis test, \\( R^2 = 0.03, p < 0.0001 \\)). (E-G) ROC curve of machine learning models in binary classification (permissive vs. resistant) of the colonization outcomes of E. faecium. For each 6-fold cross-validation (ROC curves shown in a light color), we used the samples from 20 subjects to train each model and the samples from the remaining four subjects to evaluate the model. The mean ROC curve is shown in dark color. LR: Logistic Regression, NODE: COP-Neural Ordinary Differential Equations classifier, RF: Random Forest classifier.\nFigure 4. The colonization outcome of A. muciniphila in human stool-derived in vitro microbial communities is quantitatively predictable. (A) The distribution of A. muciniphila colonization outcomes across permissive communities. The abundance of A. muciniphila in resistant communities is below the detection threshold and not shown. Inset: Percentage of high permissive (dark blue color), low permissive (light blue), and resistant communities (gray) based on A. muciniphila colonization outcomes. (B-C) Shannon diversity and species richness of A. muciniphila resistant, permissive (low), and permissive (high) communities (ns, not significant, **p < 0.01, ****p < 0.0001, Mann-Whitney U-tests). (D) Principal component analysis (PCoA) plots based on the Bray-Curtis dissimilarity of the compositional profiles of baseline communities. Color of the point showing the abundance of A. muciniphila in communities. The difference between highly permissive and lowly permissive communities was significant (PERMANOVA Adonis test, \\( R^2 = 0.022, p < 0.001 \\)). (E-G) ROC curve of machine learning models in binary classification (high permissive vs. low permissive) of the colonization outcomes of A. muciniphila. For each 6-fold cross-validation (ROC curves shown in a light color), we used the samples from 20 subjects to train each model and the samples from the remaining four subjects to evaluate the\nmodel. The mean ROC curve is shown in dark color. ENET: Elastic Net Linear Regression, NODE: COP-Neural Ordinary Differential Equations regressor, RF: Random Forest regressor. (H-J) Pearson’s correlation coefficient between the predicted abundance and the true abundance of A. muciniphila.\nFigure 5. Colonization impact in simulated and experimental communities. (A) To compute the colonization impact, i.e., the impact of a resident species on the colonization outcome of the invading species, we first trained the prediction models using all the samples. Then, we performed a thought experiment by introducing a perturbation in the abundance of the resident species and used the trained machine learning model to predict the new steady state abundance of invading species after the perturbation. A negative colonization impact indicates that a resident species inhibits the colonization of the invading species. (B–C) In simulated data, the colonization impact is randomly distributed. The median colonization impact of a resident species across different local communities is positively correlated to its interaction strength on the exogenous species (Spearman\ncorrelation \\( \\rho = 0.73, p < 2.2 \\times 10^{-16} \\). ). Network connectivity \\( C = 0.3, S_{\\text{trian}}/N = 5 \\). COP-NODE regressor is used. **(D-E)** The distribution of colonization impact on *E. faecium*, and the top ranking species with negative colonization impact (median across different communities, RF classifier). **(F-G)** The distribution of colonization impact on *A. muciniphila* and the top-ranking species with negative colonization impact (median across different communities, RF regressor).\nFigure 6. The presence of E. faecalis in baseline communities inhibits the invasion of E. faecium. (A) The post-invasion relative abundance of E. faecium (aqua) is negatively associated with the relative abundance of E. faecalis (red) across baseline communities derived from different human subjects (labeled as S01 to S24). (B-D) The colonization of E. faecium is significantly inhibited by E. faecalis across different baseline communities (labeled as B1 to B8). There were three different intervention groups: 1) add E. faecalis (or C. symbiosum) into the baseline community, followed by E. faecium on the next day (B); 2) add E. faecalis and E. faecium on the same day (C); 3) add E. faecium into the baseline community, followed by E. faecalis on the next day (D). In the control group, we only added E. faecium. After five passages, the end-point abundance of E. faecium was measured by qPCR. The fold change in the end-point abundance of E. faecium (the intervention group divided by the control group) is lower than 1 (dashed line), indicating that E. faecalis inhibits the colonization of E. faecium. Two different E. faecalis strains, DA462 and DA894, were used. n=3 replicates, the error bars are SEMs.\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• SupplementaryMaterials0419final.pdf"} {"paper_id": "prb3", "title": "On the impact of nuclear quantum effects on zeolite proton hopping kinetics through machine learning potentials and path integral molecular dynamics simulations", "text": "On the impact of nuclear quantum effects on zeolite proton hopping kinetics through machine learning potentials and path integral molecular dynamics simulations\n\nMassimo Bocus\nGhent University https://orcid.org/0000-0001-9474-6644\nRuben Goeminne\nGhent University\nAran Lamaire\nGhent University https://orcid.org/0000-0003-0093-5490\nMaarten Cools-Ceuppens\nGhent University\nToon Verstraelen\nGhent University\nVeronique Van Speybroeck (Veronique.VanSpeybroeck@ugent.be)\nGhent University https://orcid.org/0000-0003-2206-178X\n\nArticle\n\nKeywords:\n\nPosted Date: October 4th, 2022\n\nDOI: https://doi.org/10.21203/rs.3.rs-1898388/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\nOn the impact of nuclear quantum effects on zeolite proton hopping kinetics through machine learning potentials and path integral molecular dynamics simulations\n\nMassimo Bocus†, Ruben Goeminne†, Aran Lamaire, Maarten Cools-Ceuppens, Toon Verstraelen and Veronique Van Speybroeck*\n\nCenter for Molecular Modeling, Ghent University, Technologiepark 46, 9052 Zwijnaarde (Belgium)\n\n* Corresponding author: Veronique.Vanspeybroeck@Ugent.be\n† These authors contributed equally\nAbstract\n\nProton hopping is a key reactive process within zeolite catalysis, however the accurate determination of its kinetics poses major challenges both for theoreticians and experimentalists. Nuclear quantum effects (NQEs) are known to influence the structure and dynamics of protons, but their inclusion in a rigorous way through the path integral molecular dynamics (PIMD) formalism was so far beyond reach for zeolite catalyzed processes due to the excessive computational cost of evaluating all forces and energies at the Density Functional Theory (DFT) level. Herein, we overcome this limitation, by training first a reactive machine learning potential (MLP) that can reproduce with high fidelity the DFT potential energy surface of proton hopping around the first Al coordination sphere in the H-CHA zeolite. The MLP offers an immense computational speedup, which enabled us to derive accurate reaction kinetics for the proton hopping reaction. NQEs are explicitly accounted for through PIMD simulations, and the kinetics is derived using the reactive flux formalism allowing also barrier recrossings, thus going beyond standard transition state theory. More than 0.6 \\( \\mu \\)s of simulation time was necessary, which is far beyond reach of any standard DFT approach. NQEs are found to significantly impact the proton hopping kinetics up to ~473 K. These proof-of-concept results open the window to include in a more systematic way NQEs for heterogeneous catalyzed processes.\n\nGraphical abstract\n\nProton hopping in zeolites\nPES exploration via machine learning potentials\nEnhanced sampling\nnuclear quantum effects\nThermodynamics\nKinetics\nIntroduction\n\nBrønsted-acidic zeolites are versatile, resistant catalysts that for decades have been recognized as the workhorse of the petrochemical industry.\\(^1\\) Furthermore, they are also expected to play a vital role in next-generation biorefineries for the conversion of non-fossil feedstocks.\\(^2\\) From a theoretical point of view, zeolites belong to the most studied materials in the field of heterogeneous computational catalysis.\\(^3\\) In their ideal, defect-free crystalline form, Brønsted-acidic zeolites are composed of interconnected SiO\\(_4\\) tetrahedra, where a fraction of the Si\\(^{4+}\\) ions is substituted by Al\\(^{3+}\\). The excess of negative charge is compensated by the addition of a proton – the Brønsted Acid Site (BAS) – on one of the oxygens in the first coordination sphere of the Al substitution. Interestingly, the BAS is not confined to a specific oxygen of the Al tetrahedron, but it can jump from one oxygen atom to another in what is commonly known as the ‘proton hopping’ reaction. This process is one of the most fundamental activated events within zeolite chemistry (\\( \\textbf{Figure 1a} \\)) and represents the archetypal proton transfer reaction which is at the base of any Brønsted acid-catalyzed reaction.\n\nBecause of its apparent simplicity, proton hopping is an ideal case study for both experiment and theory, hence various methods have been used to investigate the process kinetics. Experimentally, Nuclear Magnetic Resonance (NMR),\\(^{4-6}\\) Impedance Spectroscopy (IS)\\(^7\\) and InfraRed spectroscopy (IR)\\(^8\\) have been employed to retrieve the activation energies for the proton hopping process. From the theoretical side, the reaction has been tackled with various methodologies ranging from static simulations\\(^9-15\\) to enhanced-sampling techniques based on molecular dynamics.\\(^16\\) Given this plethora of scientific reports, it would be tempting to assume that every detail of the proton hopping reaction is now revealed. However, when surveying the available literature, a huge spread in both the theoretically and experimentally obtained activation energies for proton hopping barriers can be found (\\( \\textbf{Figure 1b} \\)).\n\n![Schematic depiction of the proton hopping reaction, activation energy plots for multiple zeolites, and part of the H-CHA unit cell](page_184_682_1080_482.png)\n\nFigure 1. Poor agreement is found in the available literature for the activation energy of the proton hopping reaction.\n\\( a. \\) Schematic depiction of the proton hopping reaction. \\( b. \\) Activation energy for the proton hopping process as function of the Si/Al ratio for multiple zeolites, as derived from the available literature.\\(^{17}\\) The data was obtained from \\( ab \\) \\( initio \\) calculations, InfraRed spectroscopy (IR), Nuclear Magnetic Resonance (NMR) and Impedance Spectroscopy (IS). If more values are available for different temperatures, they are reported with diamonds interconnected by a dotted line. Error bars are shown where available. For more details about the reported values and a full list of references, the interested reader is referred to Section S1 of the Supplementary Information. \\( c. \\) Part of the H-CHA unit cell, showing the conventional nomenclature of the oxygen atoms in the first coordination sphere of the Al defect adopted herein.\n\nIn general, activation energies derived from NMR spectroscopy are lower than the theoretical ones. From IR experiments, two different activation energies were obtained for two different temperature ranges (398-548 and 573-773 K, see green diamonds in \\( \\textbf{Figure 1} \\)), a fact that was attributed to the\nswitch from intra-site hopping to inter-site hopping.\\(^8\\) However, a more recent investigation has disproven such interpretation and indicated active site proximity effects as the main cause for the observed change in activation energy.\\(^18\\) Inter-site hopping was also suggested to be responsible for the high activation energies retrieved with IS.\\(^7\\)\n\nTo understand this lack of consistency, it is important to consider the main possible sources of discrepancy between the proton hopping barriers from literature. First, the residual presence of water in the catalyst is often indicated as the main source for the – in general – low experimental barriers,\\(^10\\) as it is almost impossible to achieve a completely dry material with routine drying procedures.\\(^19\\) Moreover, the presence of defective sites like extra-framework aluminum species is known to alter the BAS’ acidity compared to the pristine material.\\(^20\\) On the theoretical side, most of the calculations performed so far did not explicitly account for the quantum nature of the hydrogen nucleus. Instead, the nuclei in the system are treated as classical particles moving on an underlying Potential Energy Surface (PES), which is obtained by solving the electronic many-body problem using quantum many body techniques. This is normally done using DFT for the sake of computational efficiency. In what follows, the terminology ‘classical DFT PES’ will be used to refer to nuclei that are treated as classical particles on a DFT-determined PES, thus the electronic degrees of freedom are treated quantum mechanically whereas the nuclei are treated as classical particles. To include Nuclear Quantum Effects (NQEs), approximative methods have been used, for example tunneling corrections have sometimes been applied to account for NQEs.\\(^12\\) To more rigorously account for NQEs, one should resort to computationally more expensive methods such as the Path Integral Molecular Dynamics (PIMD) approach, which relies on Feynman’s path integral formulation of quantum mechanics. Within PIMD simulations, the statistics of quantum particles are retrieved using a classical ring polymer consisting of \\(P\\) replicas of the system.\\(^21\\) Each replica runs on the classical DFT PES, making PIMD \\(P\\) times more expensive than a standard MD simulation. This is because an independent DFT-level energy and force evaluation must be performed every MD step for each replica. Within the field of heterogeneous-catalyzed reactions such simulations have so far been mostly unfeasible due to the extremely high computational cost of each PIMD step, as at least 10 replicas are usually required to achieve converged results, making the simulations prohibitively expensive.\\(^22\\) Nonetheless, there is clear evidence that NQEs may have a significant impact on the physicochemical properties of systems containing light atoms.\\(^{21,23-25}\\) For example, it is well-known that they can significantly affect the strength of hydrogen bonds in a variety of systems.\\(^{26,27}\\) To the best of our knowledge, NQEs have never been explicitly included in zeolite-related reactions and thus it remains unclear to what extent they would affect the rate of proton hopping and by extension any proton transfer reactions within the field of zeolite catalysis.\n\nTo fill this gap of knowledge, we present in the current contribution a methodology that may allow to systematically include NQEs when investigating activated hydrogen transfer events. To this end, proton hopping in H-CHA with isolated active sites is used as a case study (\\textbf{Figure 1c}), for which we first trained an accurate Machine Learning Potential (MLP) based on an underlying set of high temperature DFT Umbrella Sampling (US) simulations. The use of an enhanced sampling simulations is essential to also explore in an efficient way the less less-probable highly-energetic regions of the PES, which are typically associated with reactive events. The underlying DFT simulations at finite temperatures, serve as input to train a deep neural network MLP (\\textbf{Figure 2}). Once an accurate MLP is constructed, an enormous computational speedup can be achieved, which allowed to : (i) compute the Free Energy Surfaces (FESs) of all possible hoppings around an isolated Al defect in the temperature range 273-873 K, (ii) explicitly include NQEs through the PIMD approach and (iii) derive accurate kinetic constants beyond the Transition State Theory (TST) approximation, taking barrier recrossing into account \\emph{via} the reactive flux formalism.\\(^{28}\\)\n\nWe show that even at catalytically relevant temperatures (>400K) NQEs may still be important to consider when computing reaction kinetics and their relevance is not restricted to the absolute low temperature regime. While the work performed here is illustrative for the most basic proton hopping\nreaction in zeolites, it paves the way towards a routine inclusion of NQEs when studying any proton transfer events in heterogeneous catalysis.\n\n![Schematic showing enhanced sampling DFT and PIMD simulations on classical and MLP PES](page_186_324_1077_393.png)\n\nFigure 2. Kinetic and thermodynamic properties with and without NQEs over a wide range of temperatures can be computed using an MLP trained on high-temperature enhanced sampling DFT simulations. The pictures show a simplified schematic representation of the potential energy surface experienced by the proton when hopping between two oxygens around the Al site (red and blue spheres, respectively). On the right side, a schematic view of the hydrogen ring polymer with \\( P \\) replicas running on the classical MLP PES is shown.\n\nResults\n\nConstruction of a reactive MLP with DFT accuracy for proton hopping\nTo train an accurate MLP, a sufficiently large set of DFT datapoints is required, which should cover the relevant regions of the reaction phase space. To this end, high-temperature (873 K) DFT US simulations were performed on a CHA conventional cell containing 36T Si atoms, where 1 silicon is replaced by Al to give a final Si/Al ratio of 35. In the CHA topology, all T atoms are equivalent. However, the four O atoms in the first coordination sphere of the Al defect are not (Figure 1c). This leads to 6 distinct hopping paths, which are all considered in this work. To assess whether any path could be significantly disfavored, activation free energies were initially screened with static calculations. The results suggest that all 6 possible hopping paths have relatively similar activation free energies (within ~20 kJ·mol\\(^{-1}\\)) and no single one is strongly (dis)favored (Section S2 of the Supplementary Information). Therefore, 6 separate DFT US simulations at 873 K were performed to sample all the possible hoppings. A difference in coordination numbers between the proton and the two oxygen atoms involved in the hopping was used as main collective variable to bias the system (see Methods section and Section S3 of the Supplementary Information). One-dimensional umbrellas were used to sample the reaction path and, if needed, additional two-dimensional umbrellas were added to improve the sampling of scarcely visited regions of the phase space (more details are reported in Section S3.2 of the Supplementary Information). A full overview of the DFT US results is reported in Section S4 of the Supplementary Information.\n\nEnergies and forces were extracted every 5 fs from the DFT US trajectories, yielding a total of ~1,200,000 training structures which were used to train an MLP with the SchNetPack package (see Methods section and Figure 2). Performing MD simulations with the MLP provides a dramatic speedup in computational time, going from ~8.3 s/step on 56 Xeon E5-2680v4 CPUs@2.4GHz cores to ~0.01 s/step on a single NVIDIA Volta V100 GPU. As part of the MLP validation, well-converged\n873 K DFT FESs needed to be generated in order to compare them with the MLP-derived ones within a reasonably small uncertainty. To this end, about 50 ps of simulation time was required in each DFT umbrella. Considering that 19 umbrellas are needed to sample each of the 6 hoppings, this was a computationally demanding task. On the other hand, it also provided us with a very large number of DFT datapoints, hence the large number of structures used to train the MLP. With the acquired knowledge that a mean absolute error on the force of about 40 meV·Å⁻¹ is sufficient to obtain very accurate FESs (vide infra), we also tested the performance of newer and more data efficient equivariant neural networks,³¹ where preliminary results indicate that a few hundred fs per umbrella are sufficient to achieve converged results (Section S10 of the Supplementary Information), providing an enormous computational saving in the DFT data generation.\n\nTo further validate the trained MLP, we also tested whether it could reproduce free energy surfaces at lower temperatures than the training one. To this end, two additional sets of DFT US simulations for the 2-3 hopping were performed at 273 and 573 K. The 2-3 hopping was chosen for most of the benchmarks reported herein, as it is one of the lower activated paths. As shown in Figure 3, the DFT and MLP FESs exhibit an almost perfect overlap, with most variations contained well within the error bars. The 573 K DFT profile contains a moderate spike around the transition state, which is not present in the MLP profile. Given the FES’ shape at the other two temperatures, this spike can likely be attributed to a limited sampling of the region during the DFT simulations, rather than to a true physical phenomenon. Thanks to the large computational speedup enabled by the MLP, on the other hand, longer simulation times (100 ps vs. 50 ps per umbrella) and a larger number of umbrellas (39 vs. 19 per hopping) were easily achievable. This led to a vastly improved sampling of the reaction PES, thereby obtaining much better converged FESs. Moreover, all MLP simulations were repeated three separate times starting from different initial velocities and the associated results and uncertainties were obtained by averaging over these three independent runs. The results show that (i) the trained MLP is effectively capable of encoding chemical reactivity and (ii) high accuracy on the computed FESs is retained also for temperatures lower than the training one, offering thermodynamic transferability in terms of operating conditions.\n\n![The trained MLP can reproduce DFT FESs with high accuracy. The MLP and DFT FESs of the 2-3 hopping at 273, 573 and 873K are almost perfectly superimposable, even though the MLP model is only trained on snapshots at the highest temperature. A comparison of the FESs for the other hoppings at 873 K is shown in Figure S10. For a more detailed definition of the collective variable (q) used to build the FESs, the interested reader is referred to the Methods section. Uncertainties on the MLP FESs are obtained by averaging over 3 independent runs while for DFT they are estimated according to the procedure summarized in Section S3.1.3 of the Supplementary Information.](page_180_1012_1087_340.png)\n\nFigure 3. The trained MLP can reproduce DFT FESs with high accuracy. The MLP and DFT FESs of the 2-3 hopping at 273, 573 and 873K are almost perfectly superimposable, even though the MLP model is only trained on snapshots at the highest temperature. A comparison of the FESs for the other hoppings at 873 K is shown in Figure S10. For a more detailed definition of the collective variable (q) used to build the FESs, the interested reader is referred to the Methods section. Uncertainties on the MLP FESs are obtained by averaging over 3 independent runs while for DFT they are estimated according to the procedure summarized in Section S3.1.3 of the Supplementary Information.\n\nWhile directly superimposing FESs provides an intuitive visual means of comparison, the FES itself is not experimentally measurable. The final macroscopic quantity of interest is the kinetic constant of the reaction, which does not depend on the choice of the collective variable used to represent the FES.³²,³³ By means of classical transition state theory (TST), the forward and backward kinetic constants for the 6 high-temperature hoppings and the 2-3 hopping at lower temperatures were retrieved (see Methods\nsection). Figure 4 reports a graphical comparison between the DFT and MLP rates, where the computed kinetic constants are converted to a corresponding phenomenological barrier using Eyring’s equation.\\(^{33}\\) The sole purpose of the latter is to provide a more tangible equivalent to the kinetic constant, without comparing values that can span multiple orders of magnitude (more details are provided in the Methods section). None of the computed barriers differ more than ~5 kJ·mol\\(^{-1}\\) and, for most of the hoppings, the MLP values lie within the error bars of the DFT ones. These results indicate that the MLP accurately reproduces the DFT potential energy surface underlying the proton hopping reaction in H-CHA and can therefore be used to compute reaction rates at any temperature of interest and to explicitly introduce NQEs through the PIMD approach (Figure 2).\n\n![Graphical comparison between DFT and MLP phenomenological barriers](page_370_682_708_393.png)\n\nFigure 4. The DFT and MLP phenomenological barriers are in excellent agreement. The available DFT phenomenological barriers (12 forward and backward barriers for the 873 K hoppings and the forward and backward barriers for the 2-3 hopping at 273 and 573 K) are all within about ±5 kJ·mol\\(^{-1}\\) from the MLP ones, as highlighted by the grey shaded area. The phenomenological barriers of the 2-3 hopping at various temperatures, corresponding with the free energy profiles of Figure 3, are highlighted in different colors. Uncertainties on the MLP barriers are obtained by averaging over 3 independent runs (although their magnitude is so low that they are barely visible in the figure) while for DFT they are estimated according to the procedure summarized in Section S3.3 of the Supplementary Information.\n\nFull characterization of the hopping kinetics\nHaving validated the MLP to faithfully reproduce the proton hopping FESs over a broad temperature range (273-873 K), additional US simulations were performed to retrieve the full reaction kinetics considering all hopping paths. Moreover, NQEs can be systematically included in the reaction investigation as the PIMD formalism becomes accessible, thanks to the large computational efficiency of the MLP. To obtain well-converged FESs, at least 16 system replicas (also referred to as beads) are required in the ring polymer (Section S7.1 of the Supplementary Information). A graphical visualization of the spread of the beads around the transition state region compared with the classical case is shown in Figure 5, where it becomes clear that quite some uncertainty is present on the proton’s position compared to the classical deterministic trajectories. A full overview of the classical and quantum FESs is reported in Sections S6.1 and S7.3 of the Supplementary Information, respectively. Introducing NQEs leads to a general decrease of the free energy barriers compared to the case where nuclei are treated classically. This effect tends to lessen with increasing temperatures, in accordance with the expected convergence between the quantum and classical behavior for high temperatures. Not only does the MLP allow to include in a reliable – yet computationally feasible – way NQEs, but it also allows to determine reaction kinetics beyond classical TST and explicitly include barrier recrossing through the reactive flux formalism (obtaining the true kinetic constant of the reaction),\\(^{28,34}\\) which is in its turn part of the Bennett-Chandler reaction rate theory.\\(^{35,36}\\) In this approach, multiple unbiased simulations (5000 in this case) are initialized atop the transition state and monitored through\ntime, to retrieve whether they end up in the product basin or whether they recross the barrier towards the reactant basin (see Methods section). This approach is most appropriate when NQEs are included, as quantum TST approximations such as ring polymer molecular dynamics (RPMD) TST do not yield a strict upper bound for the quantum rate (more details can be found in Section S7.4 of the Supplementary Information).37 Overall, the MLP US simulations allowed to compute three different kinetic constants for all hopping paths and all temperatures: a classical TST-based one (\\( k_{TST}^c \\)), derived from classical MD and the TST approximation, a classical Bennett-Chandler one (\\( k_{BC}^c \\)), where barrier recrossing is now explicitly taken into account and, finally, a quantum Bennett-Chandler one (\\( k_{BC}^q \\)), analogous to \\( k_{BC}^c \\) but derived from the PIMD simulations and thus including NQEs. Remark that the amount of data used to obtain them is well beyond the reach of any pure ab initio methodology where all single energy and force simulations are performed at the DFT level. Even when excluding the thousands of short trajectories required to obtain well-converged \\( k_{BC} \\) values, computing the quantum FESs requires 42 sets of US simulations (6 hopping paths at 7 different temperatures), each consisting of 39 umbrellas simulated with 16 parallel beads – for a total of more than 0.6 μs of simulation time. Such simulation lengths are clearly beyond the limit of any DFT-based MD simulation.\n\n![Two snapshots extracted from transition state umbrella of the 2-3 hopping, highlighting the spread in proton location between classical and quantum cases](page_384_573_1012_246.png)\n\nFigure 5. The use of PIMD leads to a significant spread in the proton location. These two snapshots, arbitrarily extracted from the transition state umbrella of the 2-3 hopping, highlight how the system beads in PIMD (b) can be spread quite significantly in space with respect to the classical case (a). For the sake of clarity, only the H-SSZ-13 atoms up to the second coordination sphere around the Al site are shown and in b a superposition of all beads is only present for the proton.\n\nUsing the computed kinetic constants, the equilibrium coverage of the 4 oxygen sites (\\( \\theta_i,\\ i = 1 - 4 \\)) was determined as a function of temperature (more details can be found in Section S8 of the Supplementary Information). The results are shown in Figure 6a-c. When considering the \\( k_{TST}^c \\) and \\( k_{BC}^c \\) kinetic constants, similar equilibrium populations are obtained within the limits of uncertainty (Figure 6a, b), which is a consequence of the similar recrossing rate between the forward and backward barriers. In general, O1 and O3 are the most populated sites at any temperature, followed by O2 and O4. In the classical case, O3 has the largest population up to 373 K, while at higher temperatures its population becomes nearly identical to O1. Significantly different results are obtained when the quantum kinetic constants (\\( k_{BC}^q \\), Figure 6c) are considered, where \\( \\theta_3 \\) remains significantly larger than \\( \\theta_1 \\) at all temperatures. When the proton is on O3, it finds itself oriented towards the center of the 6 T atoms ring (Figure 6d) and can, therefore, interact with the oxygens on the opposite side. To understand more profoundly the impact of these intra-framework interactions, we performed a 273 K classical MD and PIMD simulations of the zeolite with the proton located on O3. We then analyzed the radial distribution functions (RDFs) of the proton with the 6 oxygens sharing the Si and Al with O3 ('adjacent' in Figure 6e) and all the other oxygens in the unit cell ('others'). We found that – as expected – the BAS lies within 2-3 Å from the oxygens on the other side of the 6-Si ring and will therefore interact with them. By comparing the classical and quantum RDFs (Figure 6e), it can be seen how the maximum in the RDF H-O (others) occurs at slightly shorter distances in the quantum case and, moreover, shorter distances – in the order of ~2Å – are explored more often. Based on these findings, it appears that when the quantum nature of the hydrogen nucleus is considered the weak interaction between the non-\nadjacent framework oxygens and the proton becomes stronger and, as a result, O$_3$ becomes further stabilized with an increase in \\( \\theta_3 \\). No other site interacts with other framework oxygens within 3Å (Figure S18). Previous reports in the literature, based on geometrical considerations concerning the crystallographic zeolite unit cell, suggested that none of the four BAS locations are suited to form H-bonds with other oxygens in the framework.\\textsuperscript{38} This no longer seems to be the case when temperature effects and NQEs are explicitly taken into account. The number of zeolite frameworks presenting this type of intra-framework interaction could thus be higher than previously thought\\textsuperscript{38} at realistic *operando* conditions.\n\n![Three line graphs showing equilibrium coverages of the 4 oxygen sites around the Al defect as function of temperature, computed from the kinetic constants k_{TSR}, k_{BC}^q, and k_{BC}^q. Below, a schematic drawing of the H-CHA framework and RDFs between the BAS lying on O3 and the 6 oxygens sharing the same Si and Al as O3.](page_256_370_1047_496.png)\n\nFigure 6. Including NQEs can change the computed equilibrium proton coverages. *a-c*, Equilibrium coverages of the 4 oxygen sites around the Al defect as function of temperature, computed from the \\( k_{TSR}^q \\), \\( k_{BC}^q \\) and \\( k_{BC}^q \\) kinetic constants. *d*. Portion of the H-CHA framework as seen along the c cell vector, showing the optimized structure of the BAS on O$_3$. *e*. RDFs between the BAS lying on O$_3$ and the 6 oxygens sharing the same Si and Al as O$_3$ (green line) and the BAS and all other oxygens in the unit cell (red line), from classical and NQE simulations. The schematic drawing is seen from the same perspective as *d* and highlights some of the oxygens belonging to 'adjacent' and 'others'.\n\nOnce all the equilibrium coverages as a function of temperature are known, the overall hopping rate can be computed using the formula:\n\n\\[\nr = \\sum_{i=1}^{4} \\sum_{j \\neq i}^{4} k_{ij} \\theta_i,\n\\]\n\nWhere \\( k_{ij} \\) is the kinetic constant of the hopping from O$_i$ to O$_j$ and \\( \\theta_i \\) the coverage of O$_i$. From this, an Arrhenius plot for the hopping rate as a function of the temperature is computed (**Figure 7a**), whose activation energy should be comparable with experiment. Firstly, we analyzed in how far each of the hoppings is contributing to the overall rate. In all cases, only two hopping paths dominate the rate kinetics (**Figure 7b**), namely the 1→4 and 2→3 paths, as one could expect based on their low free energy barriers. Note that the forward and backward rates have similar contributions, as a higher free energy of the minimum corresponds to both a lower coverage and a lower free energy barrier to hop towards a stabler minimum. These two factors tend to cancel each other when computing \\( k_{ij} \\theta_i \\). Minor contributions are given by the 1→2 and 2→4 paths, while the remaining two paths (1→3 and 3→4)\nonly have noticeable contributions at the highest temperatures. By considering the slope of the best fit lines in the Arrhenius plots (Figure 7a) it is possible to retrieve an effective activation energy for the proton hopping reaction. The \\( k_{TST}^q \\) results yield an activation energy of 67.1 kJ·mol\\(^{-1}\\). Going beyond the TST approximation and explicitly including recrossing (\\( k_{BC}^c \\)) does not significantly change the results, with a consistent – but almost negligible – decrease in the rate across the whole temperature range. When NQEs are included (\\( k_{BC}^q \\)), in contrast, the activation energy decreases with about 11 kJ·mol\\(^{-1}\\) due to the possibility of the proton to tunnel through the potential energy barriers. When analyzing the rates related to a specific hopping (Figure S17), it was noticed that this effect is not constant, and becomes more prominent in the hopping paths with a more sharply peaked FES around the transition state region (Figure S15-S16). This is because a narrower barrier increases the probability of tunneling, which in practice means that the beads of the ring polymer are easily located on both sides of the potential energy barrier experiencing on average a lower free energy. These results show that the impact of NQEs is not systematic in nature and can therefore be challenging to capture with *ad hoc* corrections. Indeed, previous investigations which included NQEs through an *a posteriori* tunneling correction suggested that above room temperature no significant effect should be observed.\\(^{12}\\) Our results, on the other hand, show that the reaction proceeds 65 times faster at 273 K if NQEs are included and, even at 373 K, a 16-fold increase in the computed rate is still present (Figure 7c). At 473 K, the reaction remains 7 times faster while the speedup, as expected, tends to become negligible at higher temperatures. It appears therefore that for zeolite-catalyzed processes conducted at milder conditions, among which the ones related to biomass conversion are a predominant example,\\(^{2}\\) NQEs might be non-negligible when computing the kinetics of proton-transfer steps.\n\n![Arrhenius plot showing overall hopping rate and rate contributions from different mechanisms](page_184_693_563_377.png)\n\nFigure 7. NQEs have a significant effect on the computed hopping rate. *a.* Arrhenius plot showing the overall hopping rate as function of 1/RT. *b.* Contributions to the overall rate from the different hopping paths, as function of temperature and methodology used. *c.* Speedup in the rate due to the inclusion of the NQEs.\n\nSo far, the study focused on H-CHA, which has a single indistinguishable T-site and a small unit cell. To broaden our scope, it is important to assess the MLP capability of describing other zeolite frameworks on which the MLP was not trained. To this end, the transferability of the MLP to other zeolite topologies was investigated. More specifically, we selected five all-silica frameworks from the international zeolite (IZA) database\\(^{39}\\) that are of interest for catalytic applications\\(^{3}\\) (AFX, CHA, FER, MFI and MOR) and performed a 100 ps NVT DFT MD simulation using the crystallographic unit cell parameters reported in the IZA database (see *Section S9* of the *Supplementary Information*). The CHA topology was included as a control system, to ensure that the MLP is robust with respect to changes in the unit cell volume. Surprisingly, not only did none of the MLP simulations presented obvious instabilities, but the error on the forces also remains moderate for frameworks that do not share\nany secondary building unit with CHA, varying between 196 meV·Å^{-1} for MOR and 258 meV·Å^{-1} for MFI. The quality of the zeolite trajectories, monitored through the Si-O and Si-Si RDFs, remains very high with only small long-range differences for MFI (Figure S19). Testing the proton hopping reactivity in a systematic way for more frameworks would require a further set of expensive *ab initio* US simulations and, therefore, is outside the scope of this work. The results obtained on the all-silica frameworks, nonetheless, still indicate that the MLP can capture in a large extent the chemistry of Si-O-Si bonds and, therefore, we expect that not many additional DFT simulations would be needed to retrain it and extend its accuracy to new zeolite frameworks.\n\nDiscussion\n\nProton transfer reactions are of primordial importance within zeolite catalysis. Thus far, it was unclear in how far NQEs affect the barriers and rates of proton hopping processes at realistic operating conditions, as their explicit inclusion through PIMD was so far prohibitively expensive if the underlying classical PES is evaluated at a DFT level of theory. Herein, we showed that a reactive MLP can be trained based on underlying high-temperature (873 K) US simulations at the DFT level, that provides kinetic results with similar accuracy than the underlying DFT data. However, thanks to the enormous computational speedup gained by describing the PES based on the MLP compared to the original DFT energy and force calculations, the MLP can be used to perform virtually any type of simulation that relies on the classical PES of the considered reaction(s) over a broad range of temperatures. The proposed methodology thus not only succeeds in reproducing the underlying DFT simulations but comes with a series of advantages which we were so far unreachable due to the prohibitively excessive computational cost.\n\nFirstly, the convergence of the free energy surfaces obtained from enhanced sampling techniques can be improved by using many more umbrellas and by simulating for a longer time. Secondly, PIMD can be employed to explicitly account for the quantum nature of the nuclei in the system. While the inclusion of NQEs through MLPs has already been explored in the literature,\\(^{22,40,41}\\) this work consists of the first application of PIMD/MLP to an activated event in heterogenous catalysis – to the best of our knowledge. Thirdly, it also becomes possible to go beyond the TST approximation and explicitly include barrier recrossing via the reactive flux formalism, thereby obtaining the true kinetic constant of the reaction. Because of the thousands of short MD trajectories that have to be initialized atop the transition state, this type of calculation was so far too expensive to be performed at a DFT level of theory. The more efficient methodology for describing the forces and energies, may not also open the window to use methods like transition path sampling within the field of zeolite catalysis, which were thus far not truly accessible due to the large number of paths to be sampled at the DFT level.\\(^{42}\\)\n\nOur results show that the expected Arrhenius activation energy for the hopping process, considering all six hoppings and the coverages of the four oxygen sites, is 67.1 kJ·mol^{-1} in the absence of NQEs, whereas including the quantum nature of the proton brings the activation energy down to 55.8 kJ·mol^{-1}. When quantitively comparing this activation energy to experimental results, it is important to note that this study makes use of the revPBE-D3 level of theory, which is known to underestimate the activation energies of chemical reactions.\\(^{16,43,44}\\) In this sense, our barriers will present a lower boundary for the chemically accurate activation energy. Because of the large improvement in data efficiency of newer MLP architectures (*Section S10* of the Supplementary Information), we believe that training an accurate model based on a more expensive albeit more reliable exchange-correlation functionals should become feasible. Lower experimental barriers than the one reported in this work are most likely related to the fact that zeolites are fundamentally never completely dry at experimental conditions and other active sites, like EFAL species, will most likely be present aside pristine BASSs. Both these factors are known to change the proton acidity and potentially speed up proton transfer reactions.\\(^{20,45}\\) With the presented proof-of-concept study presented, it becomes possible to train more MLPs for other acidic\nmore realistic environments and eventually simulate in a more realistic way proton hoppings and activated processes in zeolite catalysis.\n\nMethods\n\nUmbrella sampling simulations\nThe hopping of the H-CHA BAS between the oxygens in the first coordination sphere of the Al defect was studied by means of umbrella sampling simulations.\\(^{46,47}\\) In this approach, quadratic bias potentials (the ‘umbrellas’) are placed along a certain collective variable (\\(q\\)) which should smoothly vary between reactants and products. The bias has the form \\(V_i(q) = \\frac{1}{2} K_i (q - q_{0,i})^2\\), where \\(K_i\\) is the force constant of the \\(i\\)th umbrella and \\(q_{0,i}\\) its center. An MD simulation is then performed within each umbrella. To study the proton hopping, the chosen collective variable is a difference of coordination numbers (CNs) between the BAS and the two oxygens involved in the hopping:\n\n\\[\nq = CN(O_i; H) - CN(O_j; H) = \\frac{1 - \\left(\\frac{\\gamma_{O_iH}}{r_0}\\right)^N}{1 - \\left(\\frac{\\gamma_{O_iH}}{r_0}\\right)^{2N}} - \\frac{1 - \\left(\\frac{\\gamma_{O_jH}}{r_0}\\right)^N}{1 - \\left(\\frac{\\gamma_{O_jH}}{r_0}\\right)^{2N}}\n\\]\n\nThe specific values of the N and \\(r_0\\) parameters were adapted based on the reaction conditions, more information can be found in the Supplementary Information, Section S5.2. The bias potential was applied using PLUMED\\(^{48,49}\\) and the final statistical analysis of the data was performed with our in-house developed ThermoLIB library.\\(^{50}\\) For some of the hoppings, additional wall potentials were required to prevent undesired side reactions; further details are reported in Section S3.1.4 of the Supplementary Information.\n\nDFT molecular dynamics\nTo perform the DFT MD simulations, the CP2K software package (version 7.1)\\(^{51,52}\\) was employed to compute energies and forces at a revPBE-D3/TZVP\\(^{53-55}\\) level of theory. Because of the mixed plane waves – atom-centered orbitals approach\\(^{56}\\) used by CP2K, the plane waves energy cutoff was set to 350 Ry and GTH pseudopotentials\\(^{57}\\) were used to smooth the electron density in the proximity of the nuclei. A significant dependency of the forces on the plane waves cutoff was found, but this was shown to have a negligible impact on the final FESs when much higher settings are used (Section S3.1.5 of the Supplementary Information). The time step for the integration of the equations of motion was set to 0.5 fs. After equilibration of the unit cell (Section S3.3.1 of the Supplementary Information), production runs were performed in the NVT ensemble using a Nosé-Hoover thermostat with a chain consisting of five beads\\(^{58,59}\\) to control the temperature.\n\nMLP training and usage\nA SchNet MLP was trained with the SchNetPack package on the DFT energies and forces which were extracted every 5 fs from the DFT US simulations at 873 K.\\(^{29,30}\\) First, the energies and forces were unbiased by subtracting the bias potential applied in the US simulations with PLUMED.\\(^{48,49}\\) Subsequently, the MLP was trained with a cutoff of 6 Å, 128 features, 50 gaussians and 6 interaction blocks. The resulting MAE on the validation set is 41.9 meV/Å. More details on the training are provided in Section S5.1 of the Supplementary Information. Classical unbiased and US simulations with the trained MLP were performed with our in-house code YAFF\\(^{60}\\) using a time step of 0.5 fs and a Nosé-Hoover thermostat with three beads for temperature control.\\(^{58,59}\\) PIMD simulations were performed with the i-PI driver\\(^{61}\\) using a time step of 0.25 fs and a PILE thermostat\\(^{62}\\) with a time constant of 100 fs for temperature control. Because of the harmonic repulsion between the beads, some of them might explore regions of the phase space that are not necessarily well-sampled in classical DFT US. Therefore, we also performed an extra DFT PIMD US simulation for the 2-3 hopping (Section S7.2 of\nthe Supplementary Information) and the resulting FES shows an excellent agreement with the MLP one. In both the classical and PIMD US simulations, PLUMED was used to apply the bias.\n\nKinetic rate constant calculation\nAs demonstrated in previous work,\\(^{32,33}\\) the plain activation free energy obtained from a FES is largely dependent on the choice of collective variable. To remove such dependency, it is necessary to move towards a more general macroscopic property of the process under study, namely the kinetic rate constant. In the Bennett-Chandler approach to transition state theory,\\(^{35,36}\\) the rate constant of a reaction can be written as:\\(^{63}\\)\n\n\\[\nk_{BC}(t) = \\langle \\dot{q}(0)\\theta(q(t) - q^*)|_{q(0)=q^*} \\frac{e^{-\\beta F(q^*)}}{\\int_{-\\infty}^{q^*} e^{-\\beta F(q)}dq},\n\\]\n\nwhere the first term is the ensemble average of the time derivatives of \\(q\\) for trajectories that, starting atop the transition state (\\(q(0) = q^*\\)), end up in the product basin (as imposed by the Heavyside function \\(\\theta(q(t) - q^*)\\)). With the MLP, it is possible to explicitly compute the first term by performing a large number of unbiased MD simulations (5000 in this case) starting on the transition state and monitor how many of them effectively end up in the product basin.\\(^{28,34}\\) The true rate constant is, in principle, given by \\(k_{BC} = \\lim_{t \\to +\\infty} k_{BC}(t)\\). Luckily, its value quickly reaches a plateau and 50 fs of simulation were sufficient to obtain well-converged results (Section S6.2 of the Supplementary Information). The rate constant calculated in this manner is referred to as the Bennett-Chandler one (\\(k_{BC}\\)).\nIn general, this approach is too expensive, especially for the DFT case, so that only the approximate transition state theory constant (\\(k_{TST} = \\lim_{t \\to 0^+} k_{BC}(t)\\)) can be computed from the US trajectories, thereby avoiding the need for additional simulations. While \\(k_{TST}\\) represents an upper limit of the true kinetic constant, assuming a recrossing probability equal to zero, it can be used to compare the DFT and MLP results. Further details are reported in Section S3.3 of the Supplementary Information.\nAs the kinetic constant values can span several orders of magnitude, we often make use of Eyring’s equation to convert them into *phenomenological barriers*, which encode the same information while being – in our opinion – more tangible than a reaction rate.\n\n\\[\n\\Delta F_{phen}^\\ddagger = -\\frac{1}{\\beta} \\ln(\\beta h k)\n\\]\n\nData availability\n\nRelevant atomic coordinates, example of input files and the trained MLP can be found in the Supplementary Data. Any other data is available from the authors upon reasonable request. An extended discussion of the results can be found in the Supplementary Information.\n\nReferences\n\n1. Weissermel, K. & Arpe, H.-J. *Industrial Organic Chemistry*. 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Yaff, Yet Another Force Field. http://molmod.github.io/yaff/index.html.\n61. Kapil, V. *et al.* i-PI 2.0: A universal force engine for advanced molecular simulations. Computer Physics Communications **236**, 214–223 (2019).\n62. Ceriotti, M., Parrinello, M., Markland, T. E. & Manolopoulos, D. E. Efficient stochastic thermostatting of path integral molecular dynamics. Journal of Chemical Physics **133**, 124104 (2010).\n63. Frenkel, D. & Smit, B. Rare Events. in *Understanding Molecular Simulation* 431–464 (Academic Press, 2002). doi:10.1016/b978-012267351-1/50018-3.\n\nAcknowledgments\n\nThis work was supported by the Fund for Scientific Research Flanders (FWO) and the Research Board of Ghent University (BOF). The computational resources (Stevin Super-computer Infrastructure) and services used in this work were provided by the VSC (Flemish Supercomputer Center), funded by Ghent University, FWO, and the Flemish Government – department EWI.\nAuthor contribution\n\nM.B. and V.V.S. initiated the discussion and designed the scope of the project. M.B. performed the classical DFT simulations. A.L. provided technical support for the PIMD simulations and performed the PIMD DFT simulations. Under the supervision of T.V., R.G. trained the MLP and performed the related simulations, with support from M.C.C. M.B., R.G. and A.L. analyzed the results, which were discussed among all authors. M.B. and V.V.S. wrote the manuscript, with contributions from all authors.\n\nCompeting interests\n\nThe authors declare no competing interests.\n\nMaterials and Correspondence\n\nCorrespondence and request for material should be addressed to veronique.vanspeybroeck@ugent.be\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• ProtonHoppingSlv4.pdf"} {"paper_id": "prb31", "title": "Reconstruction of a catalogue of genome-scale metabolic models with enzymatic constraints using GECKO 2.0", "text": "Reconstruction of a catalogue of genome-scale metabolic models with enzymatic constraints using GECKO 2.0\n\nIván Domenzain\nChalmers University of Technology https://orcid.org/0000-0002-5322-2040\nBenjamín Sánchez\nTechnical University of Denmark https://orcid.org/0000-0001-6093-4110\nMihail Anton\nChalmers University of Technology https://orcid.org/0000-0002-7753-9042\nEduard J Kerkhoven\nChalmers University of Technology https://orcid.org/0000-0002-3593-5792\nAarón Millán-Oropeza\nINRAE, Micalis Institute\nCéline Henry\nINRA https://orcid.org/0000-0002-2355-1791\nVerena Siewers\nChalmers University of Technology https://orcid.org/0000-0002-9502-9804\nJohn Morrissey\nUCC https://orcid.org/0000-0001-7960-2001\nNikolaus Sonnenschein\nTechnical University of Denmark\nJens Nielsen (nielsenj@chalmers.se)\nChalmers University of Technology https://orcid.org/0000-0002-9955-6003\n\nArticle\n\nKeywords: genome-scale metabolic models, GECKO, enzyme constraints\n\nPosted Date: April 1st, 2021\n\nDOI: https://doi.org/10.21203/rs.3.rs-351350/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\nVersion of Record: A version of this preprint was published at Nature Communications on June 30th, 2022. See the published version at https://doi.org/10.1038/s41467-022-31421-1.\nAbstract\n\nGenome-scale metabolic models (GEMs) have been widely used for quantitative exploration of the relation between genotype and phenotype. Streamlined integration of enzyme constraints and proteomics data into GEMs was first enabled by the GECKO method, allowing the study of phenotypes constrained by protein limitations. Here, we upgraded the GECKO toolbox in order to enhance models with enzyme and proteomics constraints for any organism with an available GEM reconstruction. With this, enzyme-constrained models (ecModels) for the budding yeasts Saccharomyces cerevisiae, Yarrowia lipolytica and Kluyveromyces marxianus were generated, aiming to study their long-term adaptation to several stress factors by incorporation of proteomics data. Predictions revealed that upregulation and high saturation of enzymes in amino acid metabolism were found to be common across organisms and conditions, suggesting the relevance of metabolic robustness in contrast to optimal protein utilization as a cellular objective for microbial growth under stress and nutrient-limited conditions. The functionality of GECKO was further developed by the implementation of an automated framework for continuous and version-controlled update of ecModels, which was validated by producing additional high-quality ecModels for Escherichia coli and Homo sapiens. These efforts aim to facilitate the utilization of ecModels in basic science, metabolic engineering and synthetic biology purposes.\n\nIntroduction\n\nGenome-scale metabolic models (GEMs) have become an established tool for systematic analyses of metabolism for a wide variety of organisms\\( ^{1-6} \\). Their myriads of applications span from model-driven development of efficient cell factories\\( ^{3,7-9} \\), to their utilization for understanding mechanisms underlying complex human diseases\\( ^{10-12} \\). One of the most common simulation techniques for enabling phenotype predictions with these models is flux balance analysis (FBA), which assumes that there is balancing of fluxes around each metabolite in the metabolic network. This means that fluxes are constrained by stoichiometries of the biochemical reactions in the network, and that cells have evolved in order to operate their metabolism according to optimality principles\\( ^{13,14} \\). Quantitative determination of biologically meaningful flux distribution profiles is a major challenge for constraint-based methods, as optimal phenotypes can be attained by alternate flux distribution profiles\\( ^{15} \\), caused by the presence of network redundancies that provide organisms with robustness to environmental and genetic perturbations. This limitation is often addressed by incorporation of experimental measurements of exchange fluxes (secretion of byproducts and uptake of substrates) as numerical flux constraints for the FBA problem. However, such measurements are not readily available for a wide variety of conditions and organisms.\n\nIn order to overcome these limitations, the concept of enzymatic limitations on metabolic reactions has been explored and incorporated by several constraint-based methods. Some of these have modelled enzyme demands of metabolic reactions by constraining metabolic networks with kinetic parameters and physiological limitations of cells, such as a crowded intracellular volume\\( ^{16-18} \\), a finite membrane surface\narea for expression of transporter proteins\\(^{19}\\) and a bounded total protein mass available for metabolic enzymes\\(^{20-25}\\). All of these modelling frameworks have been successful at expanding the range of predictions of classical FBA, providing explanations for overflow metabolism and cellular growth on diverse environments for *Escherichia coli*\\(^{16-19,21,23,25}\\), *Saccharomyces cerevisiae*\\(^{22,25,26}\\), *Lactococcus lactis*\\(^{27}\\) and even human cells\\(^{20,24}\\). However, these modelling approaches were applied to metabolic networks of extensively studied model organisms, which are usually well represented in specialized resources for kinetic parameters such as the BRENDAd\\(^{28}\\) and SABIO RK\\(^{29}\\) databases. Furthermore, collecting the necessary parameters for the aforementioned models was mostly done manually; therefore, no generalized model parameterization procedure was provided as an integral part of these methods.\n\nEnzyme limitations have also been introduced into models of metabolism by other formalisms, for instance, Metabolic and gene Expression models (ME-models), implemented on reconstructions for *E. coli*\\(^{30-33}\\), *Thermotoga maritima*\\(^{34}\\) and *Lactococcus lactis*\\(^{35}\\); and resource balance analysis models (RBA), on reconstructions for *E. coli*\\(^{36}\\) and *Bacillus subtilis*\\(^{36,37}\\). These formalisms succeeded at merging genome-scale metabolic networks together with comprehensive representations of macromolecular expression processes, enabling detailed exploration of the constraints that govern cellular growth on diverse environments. Despite the great advances for understanding cell physiology, provided by these modelling formalisms, accuracy on phenotype predictions is compromised by the large number of parameters that are required (rate constants for transcriptional, translational, protein folding and degradation processes), with most of these not being readily available in the literature. Moreover, these models encompass processes that differ radically in their temporal scales (e.g., protein synthesis vs. metabolic rates) and their mathematical representation (presence of non-linear expressions in ME-models), requiring the implementation of more elaborate techniques for numerical simulation.\n\nGECKO, a method for enhancement of GEMs with Enzymatic Constraints using Kinetic and Omics data, was developed in 2017 and applied to the consensus GEM for *S. cerevisiae*, Yeast\\(^{738}\\). This method extends the classical FBA approach by incorporating a detailed description of the enzyme demands for the metabolic reactions in a network, accounting for all types of enzyme-reaction relations, including isoenzymes, promiscuous enzymes and enzymatic complexes. Moreover, GECKO enables direct integration of proteomics abundance data, if available, as constraints for individual protein demands, represented as enzyme usage pseudo-reactions, whilst all of the unmeasured enzymes in the network are constrained by a pool of remaining protein mass. Additionally, this method incorporates a hierarchical and automated procedure for retrieval of kinetic parameters from the BRENDAd database, which yielded a high coverage of kinetic constraints for the *S. cerevisiae* network. The resulting enzyme-constrained model, ecYeast7, was used for successful prediction of the Crabtree effect in wild-type and mutant strains of *S. cerevisiae* and cellular growth on diverse environments and genetic backgrounds, but also provided a simple framework for prediction of protein allocation profiles and study of proteomics data in a metabolic context. Furthermore, the model formed the basis for modeling yeast growth at different temperatures\\(^{39}\\).\nSince the first implementation of the GECKO method\\(^{38}\\), its principles of enzyme constraints have been incorporated into GEMs for *B. subtilis*\\(^{40}\\), *E. coli*\\(^{41}\\), *B. coagulans*\\(^{42}\\), *Streptomyces coelicolor*\\(^{43}\\) and even for diverse human cancer cell-lines\\(^{2}\\), showing the applicability of the method even for non-model organisms. Despite the rapid adoption of the method by the constraint-based modelling community, there is still a need for automating the model generation and enabling identification of kinetic parameters for less studied organisms. Here we wanted to build GECKO models for several organisms, and we therefore updated the GECKO toolbox to its 2.0 version. Among other improvements, we generalized its structure to facilitate its applicability to a wide variety of GEMs, and we improved its parameterization procedure to ensure high coverage of kinetic constraints, even for poorly studied organisms. Additionally, we incorporated simulation utility functions, and developed an automated virtual pipeline for update of enzyme-constrained models (ecModels), named ecModels container. This container is directly connected to the original sources of version-controlled GEMs and the GECKO toolbox, offering a continuously updated catalogue of diverse ecModels.\n\nResults\n\nCommunity development of GECKO\nTo ensure wide application and enable future development by the research community, we established the GECKO toolbox as open-source software, mostly encoded in MATLAB. It integrates modules for enhancement of GEMs with kinetic and proteomics constraints, automated retrieval of kinetic parameters from the BRENDA database (python module), as well as simulation utilities and export of ecModel files compatible with both the COBRA toolbox\\(^{44}\\) and the COBRAPy package\\(^{45}\\). The development of GECKO has been continuously tracked in a public repository (\\(https://github.com/SysBioChalmers/GECKO\\)) since 2017, providing a platform for open and collaborative development. The generation of output model files in .txt and SBML L3V1 FBC2\\(^{46}\\) formats enabled the utilization of ecYeastGEM\\(^{1}\\) structure as a standard test to track the effects of any modifications in the toolbox algorithm through the use of the Git version control system, contributing to reproducibility of results and backwards compatibility of code.\n\nInteraction with users of the GECKO toolbox and the ecYeastGEM model has also been facilitated through the use of the GECKO repository, allowing users to raise issues related with the programming of the toolbox or even about conceptual assumptions of the method, which has guided cumulative enhancements. Additionally, technical support for installation and utilization of the toolbox and ecYeastGEM is now provided through an open community chat room (available at: \\(https://gitter.im/SysBioChalmers/GECKO\\)), reinforcing transparent and continuous communication between users and developers.\n\nNew additions to the GECKO toolbox\nThe first implementation of the GECKO method significantly improved phenotype predictions for S. cerevisiae’s metabolism under a wide variety of genetic and environmental perturbations\\(^{38}\\). However, its development underscored some issues, in particular that quantitative prediction of the critical dilution rate and exchange fluxes at fermentative conditions are highly sensitive to the distribution of incorporated kinetic parameters. Although S. cerevisiae is one of the most studied eukaryal organisms, not all reactions included in its model have been kinetically characterized. Therefore, a large number of \\( k_{cat} \\) numbers measured for other organisms (48.35%), or even non-specific to their reaction mechanism (56.03% of \\( k_{cat} \\) values found by introduction of wild cards into E.C. numbers) were needed to be incorporated, in order to fill the gaps in the available data for the reconstruction of the first S. cerevisiae ecModel, ecYeast7. Moreover, detailed manual curation of \\( k_{cat} \\) numbers was needed for several key enzymes in order to achieve biologically meaningful predictions.\n\nAs the BRENDA database\\(^{47}\\) is the main source of kinetic parameters for GECKO, all of the available \\( k_{cat} \\) and specific activity entries for non-mutant enzymes were retrieved. In total, 38,280 entries for 4,130 unique E.C. numbers were obtained and classified according to biochemical mechanisms, phylogeny of host organisms and metabolic context (\\( \\textbf{Supp. file 1} \\)), in order to assess significant differences in distributions of kinetic parameters. This analysis showed that not all organisms have been equally studied. Whilst entries for H. sapiens, E. coli, R. norvegicus and S. cerevisiae account for 24.02% of the total, very few kinetic parameters are available for most of the thousands of organisms present in the database, showing a median of 2 entries per organism (\\( \\textbf{Fig. 1A, Supp. file 1} \\)). The analysis also showed that kinetic activity can differ drastically, spanning several orders of magnitude even for families of enzymes with closely related biochemical mechanisms (\\( \\textbf{Fig. 1B} \\)). Finally, it was also observed that \\( k_{cat} \\) distributions for enzymes in the central carbon and energy metabolism differ significantly from those in other metabolic contexts across phylogenetic groups of host organisms (life kingdoms, according to the KEGG phylogenetic tree\\(^{48}\\)), even without filtering the dataset for entries reported exclusively for natural substrates, as previously done by other studies\\(^{49} \\) (\\( \\textbf{Fig. 1C} \\)).\n\nAs \\( k_{cat} \\) numbers depend on biochemical mechanisms, metabolic context and phylogeny of host organisms, a modified set of hierarchical \\( k_{cat} \\) matching criteria was implemented as part of GECKO 2.0. The modified parameterization procedure enables the incorporation of kinetic parameters that have been reported as *specific activities* in BRENDA when no \\( k_{cat} \\) is found for a given query (as the specific activity of an enzyme is defined as its \\( k_{cat} \\) over its molecular weight), adding 8,118 new entries to the catalogue of kinetic parameters in the toolbox. A phylogenetic distance-based criterion, based on the phylogenetic tree available in the KEGG database\\(^{48}\\), was introduced for cases in which no organism-specific entries are available for a\ngiven query in the kinetic parameters dataset. A comparison of the new \\( k_{cat} \\) matching criteria with their predecessor set is shown in **Supp. file 2**.\n\nIn order to assess the impact of the modified \\( k_{cat} \\) assignment algorithm on an ecModel, ecYeast7 was reconstructed using both the first and the new version of the GECKO toolbox (GECKO 2.0). A classification of the matched \\( k_{cat} \\) numbers according to the different levels of the new matching algorithm is provided in **Fig. 1D**. The incorporation of specific activity values in the parameter catalogue increased the number of kinetic parameters matched to complete E.C. numbers (no added wild cards) from 1432 to 2696 (**Fig. 1E**). Moreover, the implementation of the phylogenetic distance-based criterion yielded a distribution of kinetic parameters that showed no significant differences when compared to the values reported in BRENDA for all fungi species, in contrast to the kinetic profile matched by the previous algorithm (\\( p\\)-values <\\( 10^{-10} \\) and <\\( 10^{-7} \\), when compared to the BRENDA fungi and S. cerevisiae distributions, respectively, under a Kolmogorov-Smirnov test) (**Fig. 1F**). The quality of phenotype predictions for the ecYeast7 model enhanced by GECKO2.0 was evaluated by simulation of batch growth in 19 different environments, with an average relative error of 23.97% when compared to experimental data (**Fig. 1G**), in contrast, its GECKO1.0 counterpart yielded an average relative error of 32.07%.\n\nThe introduction of manually curated \\( k_{cat} \\) numbers in a metabolic network has been proven to increase the quality of phenotype predictions for *S. cerevisiae*\\( ^{22,25,38} \\); nevertheless, this is an intensive and time consuming procedure that is hard to ensure for a large number of models subject to continuous modifications. In order to ensure applicability of the GECKO method to any standard GEM, a unified procedure for curation of kinetic parameters was developed based on parameter sensitivity analysis. For automatically generated ecModels that are not able to reach the provided experimental value for maximum batch growth rate, an automatic module performs a series of steps in which the top enzymatic limitation on growth rate is identified through the quantification of enzyme control coefficients. For such enzymes, the E.C. number is obtained and then its correspondent \\( k_{cat} \\) value is substituted by the highest one available in BRENDA for the given enzyme class. This procedure iterates until the specific growth rate predicted by the model reaches the provided experimental value.\n\nFinally, as the first version of the toolbox relied on the structure and nomenclature of the model Yeast7, its applicability to other reconstructions was not possible in a straightforward way. In order to provide compatibility with any other GEM, based on COBRA\\( ^{44} \\) or RAVEN\\( ^{50} \\) formats, all of the organism-specific parameters required by the method (experimental growth rate, total protein content, organism name, names and identifiers for\nsome key reactions, etc.) can be provided in a single MATLAB initialization script, minimizing the modifications needed for the generation of a new ecModel.\n\necModels container: an automatically updated repository\nSeveral GEMs that have been published are still subject to continuous development and maintenance\\( ^{1-3,5,6} \\), this renders GEMs to be dynamic structures that can change rapidly. In order to integrate such continuous updates into the enzyme constrained version of a model in an organized way, an automated pipeline named **ecModels container** was developed.\n\nThe ecModels container is a continuous integration implementation whose main functionality is to provide a catalogue of ecModels for several relevant organisms that are automatically updated every time a modification is detected either in the original GEM source repository or in the GECKO toolbox, i.e. new releases in their respective repositories. The pipeline generates ecModels in different formats, including the standard SBML and MATLAB files, and stores them in a container repository (https://github.com/SysBioChalmers/ecModels) in a version controlled way, requiring minimal human interaction and maintenance. The GECKO toolbox ensures the creation of functional and calibrated ecModels that are compatible with the provided experimental data (maximum batch growth rate, total protein content of cells and exchange fluxes at different dilution rates as an optional input). This whole computational pipeline is illustrated in **Fig. 2**. Further description of the ecModels container pipeline functioning is included in in the **Materials and Methods** section.\n\nA catalogue of new ecModels\nFollowing the aforementioned additions to the GECKO toolbox, that have allowed its generalization, we used the toolbox for the reconstruction of four new ecModels from previously existing high-quality metabolic network reconstructions: *iYali4*, for the oleaginous yeast *Yarrowia lipolytica*\\(^5\\); *iSM996*, for the thermotolerant yeast *Kluyveromyces marxianus*\\(^6\\); *iML1515*, for the widely studied bacterium *E. coli*\\(^A\\); and Human1, being the latest and largest network reconstruction available for studying *H. sapiens* metabolism\\(^2\\). For the microbial models, all model parameters were calibrated according to the provided experimental data, generated by independent studies\\(^{4,51-53}\\), yielding functional ecModels ready for simulations. Size metrics for these models can be seen in **Table 1**.\n\nThese ecModels, together with ecYeastGEM, are hosted in the ecModels container repository for their continuous and automated update every time that a version change is detected either in the original model source or in the GECKO repository. In the case of microbial species, two different model structures are provided: **ecModel**, which has unbounded individual enzyme usage reactions ready for incorporation of proteomics data; and **ecModel_batch** in which all enzyme usage reactions are connected to a shared protein pool. This pool is then constrained\nby experimental values of total protein content, and calibrated for batch simulations using experimental measurements of maximum batch growth rates on minimal glucose media, thus providing a functional ecModel structure ready for simulations.\n\nFor ecHumanGEM just the unbounded ecModel files are provided, as this is a general network of human metabolism, containing all reactions from any kind of human tissue or cell type for which evidence is available, and therefore not suitable for numerical simulation. As *H. sapiens* is the most represented organism in the BRENDA database, accounting for 11% of the total number of available \\( k_{cat} \\) values (**Supp. file 1**), kinetic parameters from other organisms were not taken into account for its enhancement with enzyme constraints. ecHuman1 provides the research community with an extensive knowledge base that represents a complete and direct link between genes, proteins, kinetic parameters, reactions and metabolites for human cells in a single model structure, subject to automated continuous update by the **ecModels container** pipeline.\n\n**Table 1.-** Size metrics summary for the ecModels catalogue.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Original GEMs
OrganismS. cerevisiaeY. lipolyticaK. marxianusE. coliH. sapiens
Model IDyeastGEM_8.3.3rYali4iSM996iML1515Human1
Reactions396319241913271113101
Metabolites26911671153118778400
Genes113984799615163628
Enzyme constrained GEMs
Model IDecYeastGEMecYalieciSM996eciML1515ecHumanGEM
Reactions802838815334608446259
Metabolites415318802064233412191
Enzymes96564771612593224
Enzyme coverage84.72%76.39%71.89%83.05%88.86%
Reactions w/ \\( k_{cat} \\)377115862891256227014
Reactions w/ Isoenzymes5042055324563791
Promiscuous Enzymes5723244696732184
Enzyme complexes2527527383756
\n\n**Visualization of GECKO simulations in the Caffeine platform**\nWe implemented simulations with ecModels in Caffeine, an open-source software platform for cell factory design. Caffeine, publicly available at http://caffeine.dd-decaf.eu, allows user-friendly simulation and visualization of flux predictions made by genome-scale metabolic models. Several standard modelling methods are already included in the platform, such as \\( ^{13}\\mathrm{C} \\) fluxomics data integration, and simulation of gene deletion and/or overexpression, to interactively explore strain engineering strategies. In order to allow for GECKO simulations, we\nadded a new feature to the platform for uploading enzyme-constrained models and absolute proteomics data. Additionally, we added a simulation algorithm that recognizes said models, and overlays the selected proteomics data on them, leaving out data that makes the model unable to grow at a pre-specified growth rate. After these inclusions to the platform, enzyme usage can now be computed on the fly and visualized on metabolic maps (Fig. 2B), to identify potential metabolic bottlenecks in a given condition. The original proteomics data can be visualized as well, to identify if the specific bottleneck is due to a lack of enzyme availability, or instead due to an inefficient kinetic property. This will suggest different metabolic engineering strategies to the user: if the problem lies in the intracellular enzyme levels, the user can interpret this as a recommendation for overexpressing the corresponding gene, whereas if the problem lies in the enzyme efficiency, the user could assess introducing a heterologous enzyme as an alternative.\n\nGECKO simulation utilities\nAs ecModels are defined in an irreversible format and incorporate additional elements such as enzymes (as new pseudo-metabolites) and their usages (represented as pseudo-reactions), they might sometimes not be directly compatible with all of the functionalities offered by currently available constraint-based simulation software\\(^{44,45,50,54,55}\\). We therefore added several new features to the GECKO toolbox that allow the exploration and exploitation of ecModels. These include utilities for: 1) basic simulation and analysis purposes, 2) accessible retrieval of kinetic parameters, 3) automated generation of condition-dependent ecModels with proteomic abundance constraints, 4) comparative flux variability analysis between a GEM and its ecModel counterpart, and 5) prediction of metabolic engineering targets for enhanced production with an implementation of the FSEOF method\\(^{56}\\) for ecModels. Detailed information about the inputs and outputs for each utility can be found on their respective documentation, available at: https://github.com/SysBioChalmers/GECKO/tree/master/geckomat/utilities. All of these utilities were developed in MATLAB due to their dependency on some RAVEN toolbox functions\\(^{50}\\).\n\nPredicting microbial proteome allocation in multiple environments\nIn order to test the quality of the phenotype predictions of an ecModel automatically generated by the *ecModels container* pipeline, batch growth under 11 different carbon sources was simulated with eciML1515 for *E. coli*. **Figure 3A** shows that, for all carbon sources, growth rates were predicted at the same order of magnitude as their corresponding experimental measurements, with the most accurate predictions obtained for growth on D-glucose, mannose and D-glucosamine. Furthermore, batch growth rate and protein allocation predictions, using no exchange flux constraints, were compared between eciML1515 and the jL1678 ME-model\\(^{32}\\), the latter accounting for both metabolism and macromolecular expression processes. The sum squared error (SSE) for batch growth rate predictions across the 11 carbon sources\nusing eciML1515 was 0.27, a drastic improvement when compared to the 1.21 SSE of iJL1678 ME-model predictions32. Figure 3B shows the predicted total proteome needed by cells to sustain the provided experimental growth rates for the same 11 environments. Notably eciML1515 predicts values that lie within the range of predictions of the iJL1678 ME-model (from the optimal to the generalist case) for 10 out of the 11 carbon sources (see Materiales and Methods for simulation details). This shows that the new version of the GECKO toolbox ensures the generation of functional ecModels that can be readily used for simulation of metabolism, due to its systematic parameter flexibilization step which reduces the need of extensive manual curation for new ecModels. Furthermore, iML1515 is a model available as a static file at the BiGG models repository57; therefore, its integration to the ecModels container for continuous update demonstrates the flexibility of our pipeline, regarding compatibility with original GEM sources, which can be provided as a link to their git-based repositories or even as static URLs.\n\nProteomics constraints refine phenotype predictions for multiple organisms and conditions\nThe previously mentioned module for integration of proteomics data generates a condition-dependent ecModel with proteomics constraints for each condition/replicate in a provided dataset of absolute protein abundances [mmol/gDw]. Even though absolute quantification of proteins is becoming more accessible and integrated into systems biology studies58-62, a major caveat of using proteomics data as constraints for quantitative models is their intrinsic high biological and technical variability63, therefore some of the incorporated data constraints need to be loosened in order to obtain functional ecModels. When needed, additional condition-dependent exchange fluxes of byproducts can also be used as constraints in order to limit the feasible solution space. A detailed description of the proteomics integration algorithm implemented in GECKO is given in Supp. file 2.\n\nThe new proteomics integration module was tested on the three ecModels for budding yeasts available in ecModels container (ecYeastGEM, ecYali, eciSM996). We measured absolute protein abundances for S. cerevisiae, Y. lipolytica and K. marxianus, grown in chemostats at 0.1 h^{-1} dilution rate and subject to several experimental conditions (high temperature, low pH and osmotic stress with KCl)64, and incorporated these data into the ecModels as upper bounds for individual enzyme usage pseudo-reactions. Then, exchange fluxes for CO_2 and oxygen corresponding to the same chemostat experiments were used as a comparison basis to evaluate quality of phenotype predictions. For each organism-condition pair, 3 models were generated and compared in terms of predictions: a pure stoichiometric metabolic model, an enzyme-constrained model with a limited shared protein pool, and an enzyme-constrained model with proteomics constraints. It was found that the addition of the enzyme pool constraint enables major reduction of the relative error in prediction of gaseous exchange fluxes in some of the studied conditions. Additionally, the incorporation of individual protein abundance constraints\nimproves even further the predictive accuracy of gaseous exchanges, for 10 out of the 11 evaluated cases (Fig. 4A-C).\n\nThe impact of incorporating enzyme and proteomics constraints on intracellular flux predictions was further assessed by mapping all condition-dependent flux distributions from the tested ecModels to their corresponding reactions in the original GEMs. In general, metabolic flux distributions showed high similarity when comparing ecModel to GEM predictions (Fig. S1), as 70-90% of the active fluxes were predicted within the interval of \\(0.5 < \\left( FC = \\frac{v_i^{ecModel}}{v_i^{GEM}} \\right) < 2\\) across all conditions (Fig. S2 A-C, Supp. file 3). In addition, principal component analysis on absolute enzyme usage profiles predicted by ecModels revealed that, at low dilution rates, predictions of enzyme demands are mostly defined by the selected set of imposed constraints (shared protein pool vs. proteomics constraints) rather than by environmental condition, i.e. exchange fluxes (Fig. S2 D-F). However, more straightforward comparison of the models’ predictions, by pairwise comparison of predicted absolute enzyme usage profiles, showed that 60 - 80% of the predicted enzyme usages lie within a range of \\(0.5 < \\text{fold-change} < 2\\), when comparing ecModels predictions with and without proteomics constraints, across organisms and conditions (Fig. 4D, Fig. S2 G-I and Supp. file 3). It was observed that the incorporation of proteomics constraints induces a drastic differential use for a considerable amount of enzymes, as 12-21% of enzyme usages were predicted as either enabled or disabled by these constraints across all the simulated conditions, showing slight enrichment for enabled alternative isoenzymes for already active reactions (Supp. file 3). This suggests that upper bounds on enzyme usages induce differentiated utilization of isoenzymes, reflecting well why isoenzymes have been maintained throughout evolution.\n\nThe explicit inclusion of enzymes into GEMs by the GECKO method enables prediction of enzyme demands at the protein, reaction and pathway levels. Total protein burden values predicted by ecModels for several relevant metabolic superpathways (central carbon and energy metabolism, amino acid metabolism, lipid and fatty acid metabolism, cofactor and vitamin metabolism and nucleotide metabolism, according to the KEGG metabolic subsystems\\(^{48}\\)), showed that central carbon and energy metabolism is the most affected sector in the ecYeastGEM network by integration of proteomics constraints, as protein burden predictions were higher, at least by 20%, for 3 out the 4 simulated conditions when compared with predictions of the ecYeastGEM without proteomics data (Fig. 4E).\n\nRelative enzyme usages, estimated as predicted absolute enzyme usage over enzyme abundance for all of the measured enzymes in an ecModel \\( \\left( \\frac{e_i}{[E_i]} \\right) \\), can be understood as the saturation level of enzymes in a given condition. In order to analyze the metabolic mechanisms underlying long-term adaptation to stress in budding yeasts, relative enzyme usage profiles were computed from all the previous simulations of ecModels with proteomics constraints.\nEnzymes that display fold-changes higher than 1 for both absolute abundance and their saturation level, when comparing predicted usage profiles between stress and reference conditions, suggest regulatory mechanisms on individual proteins that contribute to cell growth on the analyzed stress condition. **Figure 4F** shows all of the enzymes that were identified as responsive to environmental stress in this study, displaying enrichment for enzymes involved in biosynthesis of diverse amino acids and folate metabolism.\n\nA further mapping of all enzymes in these ecModels to a list of 2,959 single copy protein-coding gene orthologs across the three yeast species\\(^{64}\\) found 310 core proteins across these ecModels. Principal component analysis revealed that variance on absolute enzyme usages and abundance profiles for these core proteins is mostly explained by differences in the metabolic networks of the different species rather than by environmental conditions (**Fig. S3 B-C**), reinforcing previous results suggesting that, despite being phylogenetically related, their long-term stress responses at the molecular level have evolved independently after their divergence in evolutionary history\\(^{64}\\).\n\n**Exploring the solution space reduction**\nA major limitation in the use of GEMs is the high variability of flux distributions for a given cellular objective when implementing flux balance analysis, as this requires solving largely underdetermined linear systems through optimization algorithms\\(^{15,65}\\). This limitation has usually been overcome with incorporation of measured exchange fluxes as constraints. However, these data are typically sparse in the literature. Previous studies explored the drastic reduction in flux variability ranges of ecModels for *S. cerevisiae* and 11 human cell-lines when compared to their original GEMs due to the addition of enzyme constraints\\(^{1,2,38}\\). However, the irreversible format of ecModels (forward and backwards reactions are split in order to account for enzyme demands of both directions) hinders their compatibility with the flux variability analysis (FVA) functions already available in COBRA\\(^{44}\\) and RAVEN\\(^{50}\\) toolboxes. As a solution to this, an FVA module was integrated to the utilities repertoire in GECKO, whose applicability has been previously tested on studies with ecModels for *S. cerevisiae*\\(^1\\) and human cell lines\\(^2\\). This module contains the necessary functions to perform FVA on any set of reactions of an ecModel, enabling also a direct comparison of flux variability ranges between an ecModel and its GEM counterpart in a consistent way (see **Supp. file 2**).\n\nThe FVA utility was applied on three different ecModels of microbial metabolism and their correspondent GEMs (*iML1515*, *iYali4* and *iSM996*). In all cases the FVA comparisons were carried out for both chemostat and batch growth conditions in order to span different degrees of constraining of the metabolic networks (0.1 h\\(^{-1}\\) dilution rate and minimal glucose uptake rate fixed for chemostat conditions; biomass production fixed to experimental measurements of and unconstrained uptake of minimal media components, for batch conditions). Cumulative distributions for flux variability ranges for all explored ecModels and GEMs are shown\nin **Figure 5**, in which it can be seen that median flux variability ranges are much reduced for all ecModels and conditions, especially at high growth rates where enzyme constraints reduce the variability range 5-6 orders of magnitude when compared to pure GEMs. The cumulative distributions also show a major reduction in the amount of totally variable fluxes (reactions that can carry any flux between -1000 to 1000 mmol/gDw h), which are an indicator of undesirable futile cycles present in the network due to lack of thermodynamic and enzyme cost information\\(^{66-68}\\). For high growth rates, the amount of totally variable fluxes accounts for 3-12% of the active reactions in the analysed GEMs, in contrast to their corresponding ecModels in which such extreme variability ranges are completely absent.\n\nFurther analysis of the FVA results revealed that a reduction of at least 95% of the variability range was achieved for more than 90% of all active fluxes at high growth rates in all ecModel. Interestingly, the aforementioned flux variability metrics were overall improved even for the chemostat conditions, despite a higher degree of constraining (fixed low growth rate and optimal uptake rate), which restrains these models to an energy efficient respiratory mode (**Supp. file 4**).\n\n**Discussion**\n\nHere we demonstrated how enzyme constrained models for diverse species significantly improve simulation performance compared to traditional GEMs. Furthermore, to enable the community to easily adapt this modelling approach, we upgraded the GECKO toolbox for enhancement of genome-scale models with enzyme and omics constraints to its version 2.0. Major improvements on the \\( k_{cat} \\) matching algorithm were incorporated into the toolbox, based on phylogenetic distance between the modeled organism and the host organisms for data queries, and an automated curation of \\( k_{cat} \\) numbers for over-constrained models were incorporated into the toolbox. Major refactoring of the GECKO toolbox enabled a generalization of the method, allowing the creation of high-quality ecModels for any provided functional GEM with minimal need for case-specific introduction of new code. Additionally, several utility functions were integrated into the toolbox in order to enable basic simulation purposes, accessible retrieval of enzyme parameters, integration of proteomics data as constraints, flux variability analysis and prediction of gene targets for enhanced production of metabolites. Overall, it was shown that these enhancements to the GECKO toolbox improve the incorporation of kinetic parameters into a metabolic model, yielding ecModels with biologically meaningful kinetic profiles without compromising accuracy on phenotype predictions.\n\nTwo major limitations of the first version of the GECKO toolbox were its specific customization to the *S. cerevisiae* model, Yeast7, and the need of extensive manual curation for generating an ecModel suited for FBA simulations; thus, its applicability to other GEMs was not a straightforward procedure. To overcome these limitations, we generalized the code with the aim of making GECKO a model-agnostic tool. The development of a procedure for automatic curation of kinetic parameters enabled the generation of\nfunctional ecModels with minimal requirements for experimental data. Recently, ecModels for 11 human cancer cell-lines were generated with this automated procedure, using Human1 as a model input and RNAseq datasets together with the tINIT algorithm\\(^{10}\\) to generate cell-line specific networks\\(^2\\). These ecModels were used for the prediction of cellular growth and metabolite exchange rates at different levels of added constraints, resulting in remarkable improvements in accuracy when compared with predictions of their original GEMs. This highlights one of the main advantages of ecModels: their capability of yielding biologically meaningful phenotype predictions without an excessive dependency on exchange fluxes as constraints.\n\nIn order to further showcase the functionality of the GECKO toolbox 2.0, a family of new high-quality ecModels were generated for *E. coli*, *Y. lipolytica*, *K. marxianus* and *H. sapiens*, based on the original GEMs *iML1515*, *iYali4*, *iSM996* and Human1, respectively. Furthermore, we generated a self-hosted pipeline for continuous and automated generation and update of ecModels, ecModels container, so that each of the currently available ecModels (ecYeastGEM, ec/iML1515, ec/Yali, ec/SM996 and ecHuman1) are integrated to it, providing a version-controlled and continuously updated repository for high-quality ecModels.\n\nAbsolute proteomics measurements for the budding yeasts *S. cerevisiae*, *K. marxianus* and *Y. lipolytica* grown under multiple environmental conditions, were incorporated as constraints into their ecModels by using the proteomics integration module added to the GECKO toolbox. Analysis of metabolic flux distributions revealed that net reaction fluxes predicted by GEMs are not significantly affected by the incorporation of kinetic and proteomics constraints, however the explicit integration of enzymes into ecModels extends the range of predictions of classical FBA and enables computation of enzyme demands at the reaction and pathway levels. It was found that incorporation of proteomics constraints does not affect enzyme demand predictions significantly for most of the active enzymes at low dilution rates across the simulated conditions. However, we observed that a diversified utilization of isoenzymes, enforced by proteomics constraints, increases the predicted total protein mass allocated to central carbon and energy metabolism, in comparison to optimal enzyme allocation profiles. This result suggests the relevance of metabolic robustness in contrast to optimal protein utilization for microbial growth under environmental stress and nutrient-limited conditions.\n\nIncorporation of proteomics data allows the use of ecModels as scaffolds for systems-level studies of metabolism, providing a tool for uncovering metabolic readjustments induced by genetic and environmental perturbations, which might be difficult to elucidate by purely data-driven approaches, specially at conditions of relatively low changes at the transcript\\(^{69}\\) and protein levels\\(^{64}\\). For all studied stress conditions in this study, we identified upregulated proteins (increased abundance) that are needed to operate at high saturation levels in stress conditions, while showing low usage at reference conditions, creating lists of potential gene amplification targets for enhancing stress tolerance in three industrially relevant yeast species (**Supp. file 3**). Upregulation and high saturation of enzymes in amino acid and folate metabolism were found to be common across the studied organisms and stress conditions (**Fig. S3 D** and **Supp. file 3**). These results suggests that yeast cells display enzyme expression profiles that\nprovide them with metabolic robustness for microbial growth under stress and nutrient-limited conditions, in contrast to an optimal protein allocation strategy that prioritizes expression of the most efficient and non-redundant enzymes.\n\nOur results on drastic reduction of median flux variability ranges and the number of totally unbounded fluxes for ecYali, ecSM996 and ecML1515, together with previous studies^{1,2,38}, suggest that a major reduction of the solution space of metabolic models to a more biologically meaningful subspace is a general property of ecModels. However, flux variability is an intrinsic characteristic of metabolism; therefore, metabolic models with highly constrained solution spaces may exclude some biological capabilities of organisms, which are not compatible with the set of constraints used for the analysis (exchange fluxes, growth rates and even profiles of kinetic parameters, considered as condition-independent in ecModels).\n\nHere, the predictive capabilities of ecML1515 and iJL1678 ME-model (both for *E. coli*) for cellular growth and global protein demands on diverse environments were compared. The major improvement in predicted maximum growth rates, together with a comparable performance on quantification of protein demands, shown by ecML1515 suggest that, despite its mathematical and conceptual simplicity, the GECKO formalism is a suitable framework for quantitative probing of metabolic capabilities, compatible with the widely used FBA method and without the need of excessive complexity or computational power. Nevertheless, ME-models provide a much wider range of predictions that explore additional processes in cell physiology with great detail. Direct comparison between the predictions of these modelling formalisms, suggest that ME-models performance can be improved by incorporation of either curated or systematically retrieved kinetic parameters that are suitable for the modelled organisms.\n\nSimpler modelling frameworks that account for protein or enzyme constraints in metabolism, such as flux balance analysis with molecular crowding (FBAwMC)^{16,17}, metabolic modelling with enzyme kinetics (MOMENT)^{23} and constrained allocation flux balance analysis (CAFBA)^{21}, have also been developed and used to explore microbial cellular growth^{16,17,21} and overflow metabolism^{16,23}. These methods have overcome the lack of reported parameters for some specific reactions either by incorporation of proteomics measurements and prior flux distributions^{23}, manual curation and sampling procedures^{16,17} or even by lumping protein demands by functionally related proteome groups. In contrast, the new version of the GECKO toolbox provides a systematic and robust parameterization procedure, leveraging the vastly accumulated knowledge of biochemistry research stored in public databases, ensuring the incorporation of biologically meaningful kinetic parameters even for poorly studied reactions and organisms.\n\nThe applicability of these other simple modelling formalisms to models for diverse species is limited as none of these methods has been provided as part of a generalized model-agnostic software implementation. Recently, a simplified variant of the MOMENT method (sMOMENT) was developed and embedded into an automated pipeline for generation and calibration of enzyme-constrained models of metabolism (AutoPACMEN)^{70}. The pipeline was tested on the generation of an enzyme-constrained version of the *iJO1366* metabolic reconstruction for *E. coli*, which also showed consistency with\nexperimental data. This work represented a step forward in the field of constrain-based metabolic modelling, as it contributed to standardization of model generation and facilitating their utilization and applicability to other cases. However, due to the intrinsic trade-off between model simplicity and descriptive representation, a limitation of the sMOMENT method is its simplification of redundancies in metabolism, which just accounts for the optimal way of catalysing a given biochemical reaction, discarding the representation of alternative isoforms that might be relevant under certain conditions. In GECKO ecModels, all enzymes for which a gene-E.C. number relationship exists are included in the model structure. As traditional FBA simulations rely on optimality principles one could, in principle, expect the same predicted flux distributions by sMOMENT and GECKO ecModels. Nonetheless, the explicit incorporation of all enzymes in a metabolic network enables explanation of protein expression profiles that deviate from optimality in order to gain robustness to changes in the environment, as it has been recently shown by the integration of a regulatory nutrient-signalling Boolean network together with an ecModel for S. cerevisiae’s central carbon metabolism\\(^{71}\\).\n\nIn conclusion, GECKO2.0 together with the development of the automated pipeline ecModels container facilitates the generation, standardization, utilization, exchange and community development of ecModels through a transparent version-controlled environment. This tool provides a dynamic, and potentially increasing, catalogue of updated ecModels trying to close the gap between model developers and final users and reduce the time-consuming tasks of model maintenance. We are confident that this will enable wide use of ecModels in basic science for obtaining novel insight into the function of metabolism as well as in synthetic biology and metabolic engineering for design of strains with improved functionalities, e.g., for high-level production of valuable chemicals.\n\nMaterial And Methods\n\nAutomation pipeline and version-controlled hosting of the ecModels container\n\nThe ecModels repository is used to version-control the pipeline code and the resulting models. The pipeline is restricted to 2 short Python files, whose role is to decide when models need to be updated based on a configuration file **config.ini**, and to consequently invoke the use of GECKO for each model. Updates are deemed necessary when either the underlying dependencies (i.e., GECKO, RAVEN and COBRA toolboxes, the Gurobi solver, and libSMBL) or the source GEMs are independently updated to a new version (release) in their respective repositories.\n\nThe pipeline is designed be automatic and to not require supervision. It was developed to work with both version-controlled GEMs and GEMs downloadable from a URL, updating the version in the configuration after a new ecModel is obtained. For easy review, the pipeline log is publicly available under the *Actions* tab of the GitHub repository. The computation is performed through a self-hosted GitHub runner, further leveraging the transparent nature of the GitHub platform and the *git* version-control system. The resulting ecModel and updated configuration are committed to the repository, with the changes being made available for review through a pull request. Additionally, the GECKO output is also replicated in the pull\nQuantification of absolute protein concentrations for S. cerevisiae, Y. lipolytica and K. marxianus\n\nTotal protein extraction for the strains Saccharomyces cerevisiae CEN.PK113-7D (standard, low pH, high temperature, osmotic stress), Kluyveromyces marxianus CBS6556 (standard, low pH, high temperature, osmotic stress) and Yarrowia lipolytica W29 (standard, low pH, high temperature) was conducted as described in Supp. file 2. Three reference samples (hereafter, 'bulk' samples), one per strain, were constructed by pooling 5 µg of each experimental sample. Aliquots of 15 µg of total protein extract from each sample (3 strains x 4 conditions x 3 replicates) and the three bulks were separated on one-dimensional SDS-PAGE short-migration gels (1x1 cm lanes, Invitrogen, NP321BOX). Yeast proteins digestion was performed on excised bands from gel gradient and digested peptides of UPS2 (Sigma) were used as external standards for absolute protein quantification (more details in Supp. file 2). Four µl of the different peptide mixtures (800 ng for yeast peptides and 949 ng for bulks) were analyzed using an Orbitrap Fusion™ Lumos™ Tribrid™ mass spectrometer (Thermo Fisher Scientific).\n\nProtein identification was performed using the open-source search engine X!Tandem pipeline 3.4.472. Data filtering was set to peptide E-value < 0.01 and protein log(E-value) < −3. Relative quantification of protein abundances was carried out using the Normalized Spectral Abundance Factor (NSAF)73 and the NSAF values obtained from UPS2 proteins in bulk samples were used to determine the suitable regression curves that allowed the conversion from relative protein abundance into absolute terms. The regression curves parameters for protein abundance quantification are shown in Supp. file 2. MS data is available online on public databases via the PRIDE repository74 with the dataset identifier PXD012836.\n\nSimulation of condition-dependent flux distributions\n\nSimulation of cellular phenotypes for conditions of environmental stress at low dilution rates with GEMs were performed by first setting bounds on measured glucose uptake and byproduct secretion rates according to experimental data from previous studies on chemostats64. Then the biomass production rate was constrained (both upper and lower bounds) with the experimental dilution rate (0.1 h⁻¹). Maximization of the non-growth associated maintenance pseudo-reaction was set as an objective function for the parsimonious FBA problem as a representation of the additional energy demands for regulation of cellular growth at non-optimal conditions. The same procedure was followed for simulations with ecModels constrained by a total protein pool. For the case of ecModels with proteomics constraints, the same set of constraints was used but the objective function was set as minimization of the total usage of unmeasured proteins, assuming that the regulatory machinery for stress tolerance is represented by the condition-specific protein expression profile.\nPrediction of microbial batch growth rates\n\nBatch cellular growth was simulated by allowing unconstrained uptake of all nutrients present in minimal mineral media, enabling a specific carbon source uptake reaction for each case while blocking the rest of the uptake reactions and allowing unconstrained secretion rates for all exchangeable metabolites. Maximization of the biomass production rate was used as an objective function for the resulting FBA problem. For prediction of total protein demands on unlimited nutrient conditions, media constraints were set as expressed above and experimental batch growth rate values were fixed as both lower and upper bounds for the biomass production pseudo-reaction. The total protein pool exchange pseudo-reaction was then unconstrained and set as an objective function to minimize, assuming that when exposed to unlimited availability of nutrients the total mass of protein available for catalyzing metabolic reactions becomes the limiting resource for cells. The solveLP function, available in the RAVEN toolbox, was used for solving all FBA problems in this study.\n\nDeclarations\n\nCode availability\n\nThe source code of the updated GECKO toolbox is available at: https://github.com/SysBioChalmers/GECKO. The code for ecModels container and the whole catalogue of updated ecModel files can be accessed at: https://github.com/SysBioChalmers/ecModels. All custom scripts for simulations included in this study can be found at: https://github.com/SysBioChalmers/GECKO2_simulations. All the necessary scripts for reproducing the \\( k_{cat} \\) parameters analysis in Supplementary file 2 are available at: https://github.com/SysBioChalmers/Enzyme-parameters-analysis. All of these repositories are public and open to collaborative continuous development.\n\nAcknowledgements\n\nWe are grateful to Feiran Li, Raphaël Ferreira, Jonathan Robinson and all the GECKO users that have provided feedback for improving our toolbox and extending its range of applications and to the CHASSY project consortium for having motivated and supported this work. This project has received funding from the European Union’s Horizon 2020 Framework Programme for Research and Innovation – Grant Agreements No. 720824 and 686070. This work was also supported by the Knut and Alice Wallenberg Foundation and The Novo Nordisk Foundation - Grant no NNF10CC1016517.\n\nReferences\n1. Lu, H. et al. A consensus S. cerevisiae metabolic model Yeast8 and its ecosystem for comprehensively probing cellular metabolism. Nat. Commun. (2019). doi:10.1038/s41467-019-11581-3\n2. Robinson, J. L. et al. An atlas of human metabolism. Sci. Signal. (2020). doi:10.1126/scisignal.aaz1482\n3. Tiukova, I. A., Prigent, S., Nielsen, J., Sandgren, M. & Kerkhoven, E. J. Genome-scale model of Rhodotorula toruloides metabolism. Biotechnol. Bioeng. (2019). doi:10.1002/bit.27162\n4. Monk, J. M. et al. iML1515, a knowledgebase that computes Escherichia coli traits. Nature Biotechnology **35**, 904–908 (2017).\n5. Kerkhoven, E. J., Pomraning, K. R., Baker, S. E. & Nielsen, J. Regulation of amino-acid metabolism controls flux to lipid accumulation in Yarrowia lipolytica. npj Syst. Biol. Appl. **2**, 16005 (2016).\n6. 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Nucleic Acids Res. 44, (2016).\n\nFigures\n\n![A set of seven panels showing various data visualizations and plots related to enzyme kinetics and proteomics, including histograms, density plots, boxplots, and scatter plots.](page_186_682_1207_496.png)\n\nFigure 1\nkcat distributions in BRENDA and ecYeast7. A) Number of kcat entries in BRENDA per organism. B) kcat distributions for closely related enzyme families. Sample size and median values (in s-1) are shown after each family identifier. C) kcat distributions for enzymes in BRENDA by metabolic context and life kingdoms. Median values are indicated by red dots in each distribution, statistical significance (under a Kolmogorov-Smirnov test) is indicated by red stars for each pair of distributions for a given kingdom. CEM – central carbon and energy metabolism; ALM – Amino acid and lipid metabolism; ISM – Intermediate and secondary metabolism. D) Number of kcat matches in ecYeast7 per assignment category (GECKO 2.0). E) Comparison of the number of kcat matches for E.C. numbers with 0, 1, 2 and 3 introduced wild-cards by GECKO 2.0 and GECKO kcat matching algorithms. F) Cumulative kcat distributions for: all S. cerevisiae entries in BRENDA, all entries for fungi in BRENDA, ecYeast7 enhanced by GECKO and ecYeast7 enhanced by GECKO 2.0. Colored points and vertical dashed lines indicate the value for the median value for each distribution. Statistical significance under a Kolmogorov-Smirnov test of the matched kcat distributions when compared to all entries for S. cerevisiae and fungi, is shown with red circles and stars, respectively. p-values below 1x10-2 are indicated with red. G) Prediction of batch maximum growth rates on diverse media with ecYeast7 enhanced by GECKO 2.0. Glu – glucose, Fru – fructose, Suc – sucrose, Raf – raffinose, Mal – maltose, Gal – galactose, Tre – trehalose, Gly – glycerol, Ace – acetate, Eth – ethanol.\nFigure 2\n\nExtending utilization of ecModels. A) ecModels container: Integrated pipeline for continuous and automated update of ecModels. B) Implementation of GECKO simulations in the Caffeine platform (https://caffeine.dd-decaf.eu/) for visualization of enzyme usage. The color of the arrows corresponds to the value of the corresponding fluxes. Genes or reactions connected to enzymes with a usage above 90%\nare highlighted with a glow around the corresponding text or arrow, respectively. The chosen usage threshold to highlight can be tuned with the slider on the right.\n\n![Batch growth predictions and Total protein content prediction](page_186_324_1207_495.png)\n\nFigure 3\n\nComparison of predictive capabilities between eciML1515 and ME-iJL1678 for E. coli. A) Maximum batch growth rate predictions on minimal media with diverse carbon sources. Squared-sum errors when compared to experimental values are shown for both eciML1515 and ME-iJL1678. B) Prediction of total protein content in the cell by eciML1515 and ME-iJL1678 using the optimal and generalist approaches.\nFigure 4\n\nEvaluation of proteomics-constrained ecModels. Comparison of median relative error in prediction of exchange fluxes for O2 and CO2 by GEMs, ecModels and proteomics-constrained ecModels across diverse conditions (chemostat cultures at 0.1 h-1 dilution rate) for A) S. cerevisiae B) K. marxianus C) Y. lipolytica. D) Comparison of absolute enzyme usage profiles [mmol/gDw] predicted by ecYeastGEM (ecM) and ecYeastGEM with proteomics constraints (ecP) for several experimental conditions. The region between the two dashed grey lines indicates enzyme usages predicted in the interval 0.5≤E_i^ecP/E_i^ecM≤2, the region between the two dashed black lines indicates enzyme usages predicted in the interval 0.1≤E_i^ecP/E_i^ecM≤10 when comparing the two ecModels. E) Protein burden for different superpathways predicted by ecYeastGEM (ecM) and ecYeastGEM with proteomics constraints (ecP). F) Highly saturated enzymes at different stress conditions for S. cerevisiae, K. marxianus and Y. lipolytica predicted by their corresponding ecModels constrained with proteomics data. Yellow cells indicate condition-responsive enzymes (relative usage ≥0.95). Red asterisks indicate enzymes conserved as single copy orthologs across the three yeast species. Std – Reference condition, HiT – High temperature condition, LpH – Low pH condition, Osm – Osmotic stress condition, AA – amino acid metabolism, NUC – nucleotide metabolism, CEM - central carbon and energy metabolism, CofVit – cofactor and vitamin metabolism, Lip – lipid and fatty acid metabolism.\nFigure 5\n\nCumulative distributions of flux variability ranges for iSM996, iYali4 and iML1515 compared to their respective enzyme-constrained versions at low and high growth rates.\n\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• Kcatanalysis.pdf\n• suppfile2.docx\n• suppfile3.xlsx\n• suppfile4.xlsx\n• SFigures.docx"} {"paper_id": "prb32", "title": "Data-driven Design of Electrolyte Additives for High-Performance 5 V LiNi0.5Mn1.5O4 Cathodes", "text": "# Abstract\n\nLiNi0.5Mn1.5O4 (LNMO) is a high-capacity spinel-structured material with an average lithiation/de-lithiation potential at ca. 4.6–4.7 V, far exceeding the stability limits of electrolytes. An efficient way to enable LNMO in lithium-ion batteries is to reformulate an electrolyte composition that stabilizes both graphitic (Gr) anode with solid-electrolyte-interphase (SEI) and LNMO with cathode-electrolyte-interphase (CEI). In this study, we selected and tested a diverse collection of 28 single and dual additives for the LNMO||Gr system. Subsequently, we trained machine learning (ML) models using this dataset and employed these models to identify 6 optimal binary compositions out of 125, based on their predicted final area-specific-impedance, impedance-rise, and final specific-capacity. The additives generated through this ML approach demonstrated superior performance compared to those in the initial dataset. This finding not only underscores the efficacy of ML in identifying new materials in a highly complicated application space, but also showcases an accelerated material discovery workflow that directly integrates data-driven methods with battery testing experiments.\n\nPhysical sciences/Energy science and technology \nPhysical sciences/Chemistry/Energy \nadditives \nspinel \nimpedance rise \ntransesterification \nand transition metal dissolution\n\n# 1. Introduction\n\nThe spinel-structured LiNi0.5Mn1.5O4 exhibits an average lithiation/de-lithiation voltage at ~4.7 V with a high specific capacity and excellent rate capability, making it a promising candidate as cathode material for high-energy lithium-ion batteries (LIBs), while the absence of cobalt (Co) in it brings additional advantage considering the geopolitical as well as ethical risks associated with mining of Co. However, serious challenges also arise from the high operating voltage of LNMO, which far exceeds the stability limit of any known electrolyte. One typical example of the reaction between electrolyte and LNMO is the oxidative decomposition of ethylene carbonate (EC), a prevalent electrolyte solvent in mainstream LIB industry, which forms glycolic acid and difluorophosphoric acid (HPO2F2) accompanied with the reduction of transition metal cores and their concomitant dissolution. The dissolved species such as Mn(II) further engage in the cross-talk between cathode and anode, where it deposits on anode surface in either metallic or ionic form, resulting in additional capacity loss as well as cell impedance rise.1, 2 To make LNMO chemistry reversible, utilization of the electrolyte additives is the most efficient and economical approach, which, without significantly changing in the mainstream electrolyte formulation and supply chain, offers several advantages. Among them are low cost, direct interphasial engineering, and minimized side effects on other important properties of electrolytes such as ion transport, chemical compatibility with other cell parts, as well as the viscosity and rheology that are already integrated as part of the mature LIB manufacturing protocol. However, the massive chemical space of electrolyte additives together with long cycling experiments often render any large-scale screening effort practically impossible.\n\nMachine learning (ML) has rapidly become a new paradigm in the field of materials science, offering unprecedented acceleration in materials discovery and optimization.3 ML techniques enable the prediction of material properties, design of material structures with desired functionality, and identification of novel material candidates through the analysis of extensive and multifaceted datasets.4 This approach has significantly reduced the time and cost associated with traditional experimental approaches, particularly in domains critical to technological progress such as energy storage5 and catalysis.6 In the realm of battery technology, the impact of ML has been profound for accelerated screening of liquid7, 8, 9 and solid electrolytes.10, 11, 12 Specifically, ML algorithms have been used to predict the redox potentials of electrolyte additives,13, 14 as well as coulombic efficiency15 and cycle life16 of LIBs as a function of additive formulas, facilitating the identification of compounds that could lead to superior battery performance.\n\nIn this study, we proposed employing machine learning predictions of key battery’s performance metrics to accelerate the discovery of optimal electrolyte additives. The overall ML-guided experimental workflow is illustrated in Fig. 1 a, and stepwise ML tasks are shown in Fig. 1 b. We initially compiled a diverse collection of electrolyte additives and examined their impact on the performance of LNMO||Gr cells, accompanied by extensive characterizations (Fig. 1 b, Step 1). This dataset allowed us to explore the structure-property relationship between additives and three key performance indicators of the battery, namely the final area specific impedance (ASI), impedance rise (∆ASI), and final specific capacity (Q). Among these, lower ASI and ∆ASI indicate higher power density, improved charging/discharging rate, and enhanced efficiency, whereas a higher Q represents higher energy density for a given weight of the battery. We then trained and evaluated ML models with the dataset so that they can predict ASI, ∆ASI, and Q (Fig. 1 b, Step 3) based on the chemical formulas and compositions of additives. Finally, we applied the trained models on an unknown set of 125 dual additives, of which the predicted metrics were utilized to determine the most promising candidates for experimental validation (Fig. 1 b, Step 4 & 5).\n\n# 2. Result and Discussion\n\n## 2.1. Electrochemical Performance\n\nOur approach started with collecting a diverse set of additives that have been reported in the literature. These additives have been shown to contribute to the improved performance of either cathode or anode by reducing impedance, preventing lithium inventory loss, and mitigating electrolyte hydrolysis. In this paper, the beneficial additives for cathodes are referred to as cathode additives, while those benefitting anode are referred to as anode additives. The baseline solvent is 1.0 M LiPF₆ in EC/EMC at 1/9 volumetric ratio, whose performance will be used as a reference. In our list, there are 14 cathode additives and 10 anode additives (Fig. 2). The most commonly used cathode additives include lithium difluorophosphate (LDF),17 *in situ* generated lithium malonato tetrafluorophosphates (MS),18 and aged trimethylsilyl phosphite (TMSPi) (Scheme S1).19 Similarly, anode additives comprises of several typical choices including lithium difluorooxalato borate (LiDFOB),20 vinylene carbonate (VC),21 phenylboronic acid 1,3-propanediol ester (PBE),22 trivinylcyclotriboroxane pyridine complex (tVCBO), etc.23 Overall, their chemical structures consist of up to seven different elements, namely C, H, Li, P, F, O, and Si. In addition, various functional groups are present in these additives, including phenyl (C₆H₅), phosphine oxide (X₃P=O), P-F, malonato (-O-C(=O)-CH₂-C(=O)-O-), trimethylsilyl (-Si(OCH₃)₃), carboxyl (-C(=O)-O-), B-F, B-O, B-C, and alkene (-C=C-).\n\nFrom our collection of anode and cathode additives, we further curated and tested 10 single and 18 dual additive systems of various weight percentages (wt%). In this work, the dual additives always consist of a cathode and an anode additive each, as we hypothesized that their co-existence in the electrolyte and the synergistic effects would be critical to stabilize the two electrodes at their respective extreme potentials simultaneously. The distributions of ASI, ∆ASI, and Q corresponding to 28 additives, as well as the baseline electrolyte solvent are shown in Fig. 3 (tabulated data in Table S1). In general, these distributions were found to have non-normal trends, skewing either to the left (ASI and ∆ASI) or to the right (Q) of their respective range of values. Although multiple additives contribute to improvement over the baseline in one or two performance metrics, only two dual additives, specifically tVCBO at 0.25 wt% and MS at 1.0 wt%, and LiDFOB at 1.0 wt% and TMSPi at 1.0 wt%, surpass the baseline across all three evaluated metrics, achieving lower ASI and ∆ASI, as well as a higher specific capacity. It is also noted that many additives containing tVCBO or LiDFOB show enhanced capacity retention compared to the baseline system (Fig. S2)\n\n## 2.2. Structure-property relationship\n\nIdentifying the structure-property relationships of additives is critical for identifying the impacts (whether positive or negative) of structural features/descriptors on certain targeted properties. The assignment of the descriptors/features for additives here is inspired by the previous work of Okamoto et al,14 wherein the frequency/count of each atom and its coordination in the structure was tabulated. To further distinguish atoms beyond their coordinations, we also incorporated additional physicochemical properties such as formal charge and whether the atom is part of a ring (Fig. 4a). For example, the feature B[-1]_4_inRing can be expalined as follows: B represents the element Boron, [-1] indicates the formal charge of -1, the number 4 after the underscore is the coordination (number of neighboring atoms except for H), and “inRing” indicates that the atom B is part of a ring. Note that the descriptor values, or the counts of distinct atomic features, were normalized to account for various concentrations of the additives. A full list of generated features and their calcuated values corresponding to 28 electrolyte addtives in the initial dataset is provided in the SI (Spreadsheet titled “Feature table for SI.xlsx”).\n\nBy analyzing the correlations between descriptors and performance metrics, we can extract the influence of each descriptor systematically. In this work, we utilized Spearman correlation analysis which describes how well the relationship between feature and performance metric can be describe as a monotonic function. The most relevant features, based on Spearman correlation cofficients, with respect to ASI, ∆ASI, and Q are shown in Fig. 4b, 4c, and 4d, respectively. In these plots, positive and negative monotonic trend between each feature and the performance metrics are indicated by positive and negative values. Notably, among the most negatively correlated features (Spearman correlation coefficient < -0.2) of additives with respect to impedance include B[-1]_4_inRing, P[-1]_6_inRing, Si_4, and N_2_inRing, respectively. Indeed, the additive combination of 1% LiDFOB and 1% MS (Fig. 4a), where both B[-1]_4_inRing and P[-1]_6_inRing features are present, has the lowest measured impedance (44.21 Ωcm2). Furthermore, these findings align remarkably well with our current knowledge of addive effects on battery performance: 1) B[-1]_4_inRing implies that the chemical structures of lithium bisoxolatoborate (LiBOB) and lithium difluorobisoxolatoborate (LiDFOB) serve as beneficial cathode electrolyte interphase (CEI) agents.33 2) P[-1]_6_inRing suggests that oxyfluorophosphate-based cathodes are favorable for low resistance and robust CEI formation;34, 35 3) Si_4 indicates that the presence of a scavenging group, such as trimethylsilyl, effectively reduces impedance;34, 36 4) N_2_inRing suggests that a basic group like pyrrole or morpholine behaves as an HF scavenger, reducing transition metal (TM) dissolution.34, 35 These empirical results further reinforce our design principles for cathode additive, demonstrating the consistency between the observed correlations in this work and the previous research findings.\n\nAs illustrated in Fig. 4c, a similar trend was observed in the Spearman correlation of the descriptors with impedance rise, with slight diferrence observed in some new features of P[-1]_4, and O_2_inRing. The P[-1]_4 feature is associated with oxyfluorophosphate such as LiPO₂F₂ and LiPO₃F, while O_2_inRing in this case is associated with boroxane structure such as in tVCBO and PBE. The correlation between the features and final specific capacity (Fig. 4d) is less insightful, as it is influenced by vairous interplaying factors of transition metal dissolution, lithium inventories loss, impedance, and SEI robustness. Nevertheless, we still can obtain some general features that carry certain chemistry significance, for example, the features that are most positively related to final specific capacity coincide with those that are inversely related to final impedance, such as P[-1]_6_inRing, B[-1]_4_inRing, and N_2_inRing. This suggests that these features are desired as they lead to both specific capacity improvement and reduction in impedance rise.\n\n## 2.3. Machine Learning Models\n\nTo accelerate the search for new additives, it is essential to develop predictive capability ahead of tedious experiments, which typically require several months to complete. Hence, we utilized the above initial dataset to train ML models to predict potential chemical structures and compositions that could lead to improvements in ASI, ∆ASI, and Q metrics. Specifically, Gaussian Process Regression (GPR) is the ML model of choice as it has been shown to be one of the most reliable algorithms for low-dimensional and small datasets,37 which is the case in this work. In addition, GPR also produces uncertainty quantification for every prediction, allowing for quality evaluation of the prediction (see Machine Learning methods in the SI). To further enhance the assessment of our models' reliability, we implemented 10-fold cross-validation (CV), in which the dataset is partitioned into 10 equal segments. During each iteration, one segment is reserved for testing while the remaining nine are utilized for training. This procedure is conducted ten times, with each iteration featuring a distinct test set. The overall error is determined by averaging the errors across all ten models. For all models, mean absolute error (MAE) is employed as the evaluation metric. The parity plots comparing GPR predictions with experimental measurements of 28 additives and the baseline systems are shown in Fig. 5. Based on the results, the highest prediction accuracy is observed for final specific capacity model (Test MAE10−fold CV = 10.7 ± 4.6 mAhg⁻¹), followed by impedance rise model (Test MAE10−fold CV = 15.3 ± 7.8 Ωcm²) and final area specific impedance model (Test MAE10−fold CV = 20.0 ± 10.6 Ωcm²). Overall, we believe that our ML models are reasonably accurate given the size of the current training dataset.\n\n## 2.4. Prediction and validation\n\nTo identify new additives with improved performance, we systematically examined every possible combination of dual additives, totaling 140 pairs, by mixing 14 cathode and 10 anode additives in equal weight percentages of 1%. Among these, 15 have already been tested and included in the initial dataset, which leaves 125 additive combinations yet to be explored. Using our trained GPR models, we performed prediction of ASI, ∆ASI, and Q for 125 unknown additive candidates. The results were tabulated in as shown the SI (Spreadsheet titled “LNMO_wSingle_additive_customFeats_Highlighted.xlxs”). Furthermore, as the accuracy of GPR models has been shown to be more reliable for the prediction of ∆ASI and Q with lower MAEs and uncertainty (Fig. 5), we employed those as the ranking criteria for selecting new additive combinations for experimental validation. The experimental measurements for the top 6 dual additives candidates are reported in Table 1, where we identified three out of six dual additives with desirable measured performance metrics (No. 29, 31, and 32). Among these, the dual system comprising of LiDFOB at 1.0 wt% and SA at 1.0 wt% shows similar Q but improved (lower) ASI and ∆ASI compared to the baseline solvent. More importantly, the addition of either MS or SA to LiBOB show notable enhancement in all three considered metrics, with the combination of LiBOB at 1.0 wt% and SA at 1.0 wt% achieving the highest final specific capacity (95.49 mAhg⁻¹) among all additives in this work.\n\nTo gain further insights into additive performance, we carried out an array of experimental and post-test analysis of the cycled cells of the top four additive compositions and the baseline in this study, particularly focusing on the degradation mechanisms, including the regular checkup on the cycled anodes for the TM cross walked from the cathodes (see SI for details).1 H nuclear magnetic resonance spectroscopy (NMR) clearly shows the inhibition of transesterification in presence of the designed additive combinations (Fig. S8). X-ray photoelectron spectroscopy (XPS) confirms the formation of oxyfluorophosphates in some additives that improves CEI (Fig. S9). Inductive coupled plasma mass spectrometry (ICP-MS) confirms the beneficial effects of additives in reducing transition metal dissolution/deposition on the anode side (Fig. S10). SEM confirms the presence of TM aggregates in cells with additives, thereby reducing their detrimental effects on SEI rejuvenation and lithium inventory consumption (Fig. S11 – S15). The online electrochemical mass spectrometry (OEMS) experiments have shown that these additives can also inhibit the consecutive breakdown and reformation of SEI, a process that leads to lithium inventory consumption (Fig. S16). The experiments on harvested cell components clearly identify the lithium inventory loss as the main degradation mechanism, associated with TM dissolution and high impedance rise (Table S2 and Fig. S7). All these point to the effective mitigation of degradation by these ML-predicted additive formulations.\n\n| No. | Additive | ASI (Ωcm²)^ | ∆ASI (Ωcm²)* | Q (mAhg⁻¹)% |\n|-----|----------|------------------------|------------------------|------------------------|\n| 29 | LiDFOB 1.0 wt% + SA 1.0 wt% | 41.19 | 16.26 | 91.79 |\n| 30 | LiDFOB 1.0 wt% + MS 1.0 wt% | 104.76 | 65.57 | 69.80 |\n| 31 | LiDFOB 1.0 wt% + SA 1.0 wt% | 50.13 | 16.77 | 92.17 |\n| 32 | LiBOB 1.0 wt% + SA 1.0 wt% | 46.79 | 10.19 | 95.49 |\n| 32 | LiBOB 1.0 wt% + MS 1.0 wt% | 123.53 | 85.94 | 47.07 |\n| 33 | LiDFOB 1.0 wt% + MS 1.0 wt% | 203.43 | 110.36 | 80.06 |\n| | Baseline | 54.47 | 19.35 | 91.94 |\n\n^: Area specific impedance; *: Impedance rise; %: Final specific capacity\n\n# 3. Conclusion\n\nIn summary, we successfully showcased a data-driven experimental framework aimed at fast and efficient identification of electrolyte additives for LIBs based on LNMO cathodes. This method utilized a limited set of initial experimental data to develop reliable machine learning models that directed subsequent experimental efforts. We began by creating an initial dataset from performance metrics including final area specific impedance, impedance rise, and final specific capacity, gathered from 28 additives and the baseline solvent. Utilizing this data, we employed ML models to evaluate these performance metrics for an expanded, untested group of 125 dual electrolyte additives. Remarkably, by experimentally validating only the top 6 candidates identified through ML predictions, we discovered a new binary formulation, namely LiBOB at 1wt% and SA at 1wt%, that outperformed all additives in the initial dataset. Future research will explore a broader array of additives, including ternary compositions, via closed-loop experiments guided by Bayesian optimization. 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Yang J, et al. 4-(Trimethylsilyl) Morpholine as a Multifunctional Electrolyte Additive in High Voltage Lithium Ion Batteries. *J Electrochem Soc* **167**, 070533 (2020).\n\n35. Yang J, et al. Design of a Scavenging Pyrrole Additive for High Voltage Lithium-Ion Batteries. *J Electrochem Soc*, (2022).\n\n36. Peebles C, et al. Chemical “Pickling” of Phosphite Additives Mitigates Impedance Rise in Li Ion Batteries. *J Phys Chem C* **122**, 9811–9824 (2018).\n\n37. Xu P, Ji X, Li M, Lu W. Small data machine learning in materials science. *Npj Comput Mater* **9**, 42 (2023).\n\n# Supplementary Files\n\n- [SILNMOML3.3.docx](https://assets-eu.researchsquare.com/files/rs-4420883/v1/958f7ea7469403d75041dd17.docx)\n- [LNMOwSingleadditivecustomFeatsHighlighted.xlsx](https://assets-eu.researchsquare.com/files/rs-4420883/v1/63350ca800400fff74f9bbb8.xlsx) \n Supplementary Dataset 2\n- [FeaturetableforSI.xlsx](https://assets-eu.researchsquare.com/files/rs-4420883/v1/2a7dec1d03f75de48aa62f8d.xlsx) \n Supplementary Dataset 1\n- [TOC.png](https://assets-eu.researchsquare.com/files/rs-4420883/v1/c59c2011534bc289b1ded58a.png) \n For Table of Contents Only"} {"paper_id": "prb33", "title": "Machine learning-guided discovery of ionic polymer electrolytes for lithium metal batteries", "text": "# Abstract\n\nDevelopment of ionic polymer electrolytes (IPEs) without flammable organics is a critical strategy to enable safe and high-energy lithium metal batteries (LMBs). As critical components in IPEs, ionic liquids (ILs) with high ionic conductivity and wide electrochemical window are promising candidates to enable LMBs. Here, we describe a fast and robust machine learning workflow embedded with quantum chemistry calculation and graph convolutional neural network to discover promising ILs for IPEs. By selecting subsets of the recommended ILs, combining with a rigid-rod polyelectrolyte and a predetermined lithium salt, we develop a class of large area and mechanically strong IPE membranes with thickness ~ 50 μm. The symmetric cells exhibit stable cycling performance at 1 mA cm⁻¹ (0.5 mAh cm⁻²) up to 800 h at room temperature (RT) and excellent reversibility at 6 mA cm⁻² (3 mAh cm⁻²) at 80 °C. With LiFePO₄ loading ~ 10.3 mg cm⁻², the full cells deliver outstanding capacity retention for > 350 cycles (> 96% with 0.5 C at RT; > 80% with 2 C at 50 °C), fast charge/discharge capability (146 mAh g⁻¹ with 5 C at 80 °C) and ultrahigh coulombic efficiency (> 99.92%). This performance is rarely reported by any single-layer polymer electrolytes without any organic plasticizers/oligomers for LMBs.\n\nPhysical sciences/Energy science and technology/Energy storage/Batteries \nPhysical sciences/Materials science/Materials for energy and catalysis/Batteries \nPhysical sciences/Materials science/Soft materials/Polymers \nPhysical sciences/Materials science/Soft materials/Liquid crystals \nPhysical sciences/Materials science/Theory and computation\n\n# Full Text\n\nIonic polymer electrolytes (IPEs) containing the non-flammable ions embedded with the mechanically supporting polymers with predetermined ionic pathway have received considerable attention toward reviving clean energy storage and conversion devices, such as batteries, \n1-6 fuel cells, \n7 supercapacitors, \n8 mechanical actuators \n9 and reverse osmosis membranes. \n10 As promising candidates for safe and environmentally friendly electrolyte materials, ionic liquids (ILs) are room temperature (RT) molten salts with low vapor pressure, high thermal stability, wide electrochemical window and high ionic conductivity. \n1,5,11 In recent years, liquid crystalline polymers have shown the capability to effectively reduce the interfacial resistance, meanwhile raising unique ion conduction mechanisms in lithium metal batteries (LMBs). \n1,12 Li metal anode coupled with high-energy-density cathodes, for example Li-air and Li-sulfur batteries, usually require highly conductive, thermal-stable and electrochemical-stable electrolytes to suppress inhomogeneous Li dendrites, overcome the side reactions and break the tradeoff between conductivity and modulus in the composite electrolytes. \n13,14 To alleviate these issues synergistically, IPEs have shown the capability to block dendrites through the robust polymer matrix, meanwhile guarantee the extreme safety by avoiding organic plasticizer in LMBs. \n13,15-17\n\nAs critical components in IPEs, it is desirable to develop a method to screen suitable ILs from a large population of ion pairs to develop successful IPEs for LMBs. ML has been widely discussed to predict properties and learn the rules underlying datasets, thus efficiently simplifying the material-discovery process. \n18-23 Here, we describe a machine learning (ML) workflow embedded with the quantum chemistry calculation and graph convolutional neural network (GCN) to discover potential ILs with high ionic conductivity and sufficient electrochemical window. Driven by the structure-property relationships, previous researchers have developed diverse statistical methods and regression models to predict physical properties, for example, melting point \n24, viscosity \n25 and ionic conductivity \n26 based on the structure descriptors of the ILs. \n27 However, the reported high accuracy usually originates from the overfitting of the dataset. \n28,29 Among the training datasets, the sample size of unique ILs is extremely limited. \n27,28 The investigated datasets usually contain the datapoints of the same ILs at varying temperatures, these replicated datapoints will increase the appeal accuracy of the reported models artificially. \n25,30 Thus, it is still challenging to predict the accurate properties of new ILs without enough labeled datapoints and preparation of featured factors for the explanatory variables. However, to overcome the data scarcity issue, we can specifically focus on the design of statistical regression and classification workflow to discover new applicable ILs instead of predicting the absolute physical properties of the IL pairs, thus will relief the issue of data scarcity in practical application of ML in material science. In addition, this work also demonstrates the efficiency to use GCN for the graph classification task based on the graph-to-property relationship of ILs.\n\nBased on the screening results from ML, we experimentally investigate some of the filtered ILs combined with a liquid crystalline polyelectrolyte Poly 2,2′-disulfonyl-4,4′-benzidine terephthalamide (PBDT) and a predetermined Li salt to develop a series of IPEs. As reported previously, Li metal anode shows highly reversible cycling-performance with a stable solid-electrolyte interphase (SEI) formed by electrochemically reduction of the bis(fluorosulfonyl)imide (FSI \n−) anion. \n31,32 Thus, we employ LiFSI dissolved in ILs as an ion exchange medium to load Li ions in the IPEs. By incorporating these IPEs into batteries with Li metal as an anode, we can experimentally confirm the properties of these developed IPEs, including thermal stability, ionic conductivity, Li \n+ transference number, electrochemical window and Li dendrite suppression.\n\n## Machine Learning-guided Screening Of Ionic Liquids\n\nThis machine learning workflow requires two main steps: (1) Unsupervised learning, followed by (2) Supervised learning to target promising ILs. As shown in Fig. \n1, we obtain 76 cations and 31 anions from the web scrapping of IoLiTech website. The permutation of cations and anions forms an ionic liquid pool containing 2356 unique ILs, but only less than 13% of the ILs showing measured properties, for example melting point, viscosity, conductivity and electrochemical window. Three open-source platforms, including RDKit, Psi4 and Pytorch Geometrics (PyG), have been employed to generate the molecular descriptors of the raw dataset. RDKit is a powerful tool to calculate the molecular structure and three dimensional (3D) descriptors of the molecules. \n33 Psi4 is an open-source ab initio electronic structure program for high-throughput quantum chemistry. \n34 We employ the self-consistence field (SCF) method along with the basis set of 6-311 + G** to optimize the geometric structure and then calcualte the energy, the highest occupied molecular orbital energy (E \nHOMO), the lowest unoccupied molecular orbital energy (E \nLUMO) and the molecular dipole moment for the cations and anions seperately. In this work, we combine 60 molecular structure descriptors from RDKit and 14 calculated variables from Psi4 for cations, anions in the final dataset. PyG is a library based on Pytorch to build and train Graph Neural Networks (GNN) for a wide range of prediction tasks. For the unsupervised learning, we employ boxplots, pair plots and hierarchical clustering to summarize the basic rules underlying the dataset. In terms of the supervised learning, we employ both statistical regression and classification to promote the screening efficiency. Among the 2356 ILs, we initially use the classification method to predict the state (solid/liquid) of the ion pairs at RT. Then we employ both statistical regression and classification to evaluate the conductivity of the obtained 1240 ILs (liquid at RT). As we expected, it is particularly challenging to obtain the absolute conductivity of the ILs with high accuracy through regression, especially for the ions with small samples in the training model. To improve the screening efficiency, we utilize a complementary classification method, which will classify the ILs into two categories, based on predetermined and tunable threshold of conductivity, thus will alleviate the low accuracy arises from the limited datapoints. The ensemble learning is based on the combination of algorithms including support vector machine (SVM), random forest (RF), XGBoosting (XGB) and GCN. The last screening step is determined by the computed electrochemical window value (ECW) according to Eq. 1–3 through Psi4. The ECW of an IL is determined by both cations and anions. The cathodic limit (V \nCL) is the maximum value of the cathodic potential determined by the E \nLUMO for cations and anions. Similarly, the anodic limit (V \nAL) is the minimum value of the anodic potential determined by the E \nHOMO for cations and anions. \n35 According to this machine learning workflow shown in Fig. \n1, we finally obtain 40 ILs in the recommendation list. We will expand the discussion of the unsupervised learning and the supervised learning in the following sections.\n\n$$\n{V}_{CL}=\\text{max}\\left(-\\frac{{E}_{LUMO}[+]}{e},-\\frac{{E}_{LUMO}[-]}{e}\\right)\n$$\nEq. (1)\n\n$$\n{V}_{AL}=\\text{min}\\left(-\\frac{{E}_{HOMO}[+]}{e},-\\frac{{E}_{HOMO}[-]}{e}\\right)\n$$\nEquation (2)\n\n$$\n\\text{E}\\text{C}\\text{W}= {V}_{AL}- {V}_{CL}\n$$\nEq. (3)\n\n## Unsupervised Learning\n\nTo investigate the features and the underlying correlations in the dataset, we employ the unsupervised learning as a feature detector. Figure \n2 a,b display the boxplots of the ILs with known σ in the dataset, which are classified by the cation and anion types correspondingly. In terms of the cations, the average σ follows the order of ammonium > sulfonium > pyrrolidinium > imidazolium > pyridinium > piperidinium > phosphonium. Accordingly, the rule for the anions is nitrate > thiocyanate > DCA > BF \n4 > triflate > sulfate > imide > sulfonate > acetate > halogen > phosph. Figure \n2 c,d display the rankings for the measured ECW of the ILs correspondingly. We observe that the ECW boxplots showing large variations, but the ammonium-based cations and imide-based anions commonly displaying promissing ECWs. In order to understand the corelations between different features, as shown in Fig. \n2 e, we observe that the σ is highly corelated with the viscosity of ILs, which can be elucidated by Nernst-Einstein equation and Stokes-Einstein equation included in Supplementary Note 1. \n36 However, as shown in Fig. \n2 f, there is no strong corelation between σ and ECW. Thus, we can conclude that σ and ECW of ILs are two independent features. As we familar, both σ and ECW are essential properties for electrolytes applied for LMBs. Zhang \n30 has employed hierachical clustering to predict fast inorganic Li ion conductors. Here, we also employ this algorithm to detect the clusters of ILs with high conductivity and wide ECW. The key features used for the hierachical clustering include the computed ECW and the top 10 factors obtained from the XGBoosting model for conductivity classification (Supplementary Note 2). The clustering criterior is a combination of the σ and the ECW of the ILs. The final results are shown in Fig. \n2 g. Additionally, in order to validate the effectiveness of the clustering, we also plot the finally screened ILs based on the supervised learning in Fig. \n2 h, we can clearly observe that the results based on the two learning protocols are highly overlaped, which indicates the high efficiency of the unsupervised learning as compared to the supervised learning introduced in the following section.\n\n## Supervised Learning\n\nBuilding on the unsupervised learning, we initially propose a complementary supervised learning to filter ILs with liquid phase at RT based on the ensemble learning of SVM, RF, XGB and GCN. The classification results are shown in the Supplementary Note 3. Figure \n3 a indicates the corelation between the radius of gyration for anion and the heavy atom molecular weight for the classified solid and liquid groups, we observe that the ILs with high sphericity tend to be in solid state, whereras those with high asymmetry of anions will usually turn to be liquid state. We also include the top 10 importance features of XGB model in Fig. \n3 b. As we expected, the phase of ILs are highly dependent on the gyometic strucutres of anions. To further validate the predicted results, we employ quantum chemistry calculation to calculate the interaction energy between cations and anions. We randomly select 20 ILs from the predicted solid and liquid groups, seperately. The interaction energies of the selected ion pairs are calculated based on Eq. 4. As shown in Fig. \n3 c, the interaction energies for the solid ILs are generally lower compared to the liquid ILs. The detailed calculation results are included in Supplementary Table 1. As we know, the interaction energy of the cation and anion is the energy required to combine cation and anion. The lower of the interaction energies means easier for the cations and anions to stay in tightly associated pairs. In addition, we also employ GCN model to investigate this classification. The workflow of the GCN model is shown in Fig. \n3 d. The details about the GCN model used in this work are also included in the Supplementary Note 4. The efficiencies of employed models are included in Table \n1. We observe that the GCN model offers similar performance only based on the chemcial geometric descriptors without any additional calculation results, which shows high promise for this algotihrm for future materials genome projects. Additionally, we also apply the other three models to predict the absolute σ of the liquid (1084) ILs pairs at RT. The boxplots shown in Fig. \n3 e further indicate the consistency between the regression and the classification results. The median value of the predicted conductivity for cluster with σ < 5 is 1.9 mS cm \n− 1. Meanwhile, the median value for cluster with σ ≥ 5 is 8.9 mS cm \n− 1. Finally, we propose 40 ILs with σ ≥ 5 mS cm \n− 1 along with an satisfactory ECW > 3.5 V in the final recommendation list for development of IPE in LMBs. The full list is included in Supplementary Table 2. The bubble plots shown in Fig. \n3 f, g indicate the distribution of the filtered ILs based on the cation and anion types, correspondingly. In terms of the cations, we observe that the imidazolium cations display the highest average ionic conductivity. In terms of the anions, BF \n4, sulfate and triflate show both promising ECW and σ. Base on this prliminary rules, we select four widely discussed ILs from the bubbles and conduct experimetanl validation in the following section.\n\n$$\n{\\text{E}}_{interaction energy}= {\\text{E}}_{\\left[+\\right]\\left[-\\right]}- {\\text{E}}_{[+]}-{\\text{E}}_{[-]}\n$$\nEq. (4)\n\n| Algorithm | R2 (Solid or Liquid) | R2 (σ ≥ 5 or σ < 5) |\n|---------|-------------------------------|-------------------------------|\n| Support Vector Machine (SVM) | 0.80 | 0.82 |\n| Random Forest (RF) | 0.85 | 0.81 |\n| XGBoosting (XGB) | 0.86 | 0.81 |\n| Graph Convolutional Neural Network (GCN) | 0.83 | NA |\n\n*The R2 for SVM, RF and XGB algorithms are the avergae of the 5-fold cross-validation accuracy results.\n\n## Electrochemical Performance Of Ipes Based On The Filtered Il\n\nTo verify the efficiency of this screening process, we develop a series of IPEs based on 4 hydrophilic ILs on the final recommendation list and validate the cycling behavior and electrochemical performance of the developed IPEs coupled with the Li metal anodes. The selected ILs include 1-ethyl-3-methylimidazolium triflate (C \n2 mimTFO), 1-ethyl-3-methylimidazolium tetrafluoroborate (C \n2 mimBF \n4), 1-ethyl-3-methylimidazolium ethyl sulfate (C \n2 mimEthylSulfate) and diethylmethylammonium triflate (DemaTFO). All these ILs are hydrophilic and showing high ionic conductivity at RT, we can use solvent-casting method to prepare ultrathin (~ 50 µm) polymer electrolytes as reported previously. \n1, 6, 37 The fabricated films are transparent and mechanically strong with 5/10wt% of PBDT. After ion exchange with the ionic liquid electrolyte (ILE) with LiFSI dissolved in N-propyl-N-methylpyrrolidinium bis(fluorosulfonyl)imide (C \n3 mpyrFSI), we obtain large area and flexible IPE membranes. The solid-state membrane electrolytes with diameter of 9 mm shown as insets in Fig. \n4 a-c are assembled in LMBs. Initially, we perform cyclic voltammetry (CV) on Li|IPEs|SUS to evaluate the Li plating (negative scan) and stripping (positive scan) behavior of the selected ILs combined with PBDT. We observe that upon scanning in the negative direction, this electrolyte displays excellent cathodic stability for Li-metal cycling. The achieved high current density offers promise for these IPEs as conductive electrolytes in LMBs. Among the four ILs, only DemaTFO displays no Li deposition in the cathodic deposition, which indicates that the ion exchange protocol fails to incorporate Li ions in DemaTFO based IPEs. Thus, we conclude that the ion association behavior and varying interaction energies are essential factors to determine the final chemical composition in the IPEs. In the following discussion, we will only focus on the other three IPEs. For the positive direction, as shown in the enlarged curves in the insets, we observe that C \n2 mimTFO based IPEs show the highest anodic stability up to 5 V vs Li|Li \n+, which confirms the high electrochemical stability of IPEs based on C \n2 mimTFO. However, both BF \n4 \n− and Ethyl Sulfate display fluctuate current starting from 4V for BF \n4 and 3.5V for Ethyl Sulfate, which are lower compared to the computed ECWs. As reported previously, the calculated anodic limits for BF \n4 \n− are usually overestimated using the vacuum calculation model compared to the experimental results. \n35 The reasons for the inconsistency originate from many factors, for example the assumption of the calculation model and the complicated ion association in the real system. For comparison, we include the CV results for the three neat ILs in Supplementary Note 5. Surprisingly, the cathodic limits for the neat ILs are much lower compared to the IPEs. We propose that the high Li \n+ concentration and PBDT in the IPEs can improve the cathodic stability of the composite electrolytes, which is analogy to the “water in salt” electrolytes proposed by Suo et al. \n38 The solvation of the Li \n+, cations and anions will change dramatically with the adjustment of the relative ion concentrations. We have demonstrated that the rigid-rod polyelectrolyte PBDT backbone will selectively absorb cations and anions during the ion exchange process, which will promote the Li transference number ( \nt \nLi \n+) of the system. Here, we estimate the \nt \nLi \n+ based on the steady-state current of the Li symmetric cell assembled with IPEs as electrolyte and separator in Fig. \n4 d. The insets show the corresponding impedance spectra of the cells before and after the polarization. The \nt \nLi \n+ of Bruce-Vincent analysis is defined in Supplementary Note 6. \n39 The determined \nt \nLi \n+ in these IPEs (0.4–0.5) are much higher compared to the pure ILE with LiFSI|C \n3 mpyrFSI ( \nt \nLi \n+ = 0.18) \n40. Among these three IPEs, C \n2 mimTFO based IPEs show higher \nt \nLi \n+ = 0.5 compared to C \n2 mimBF \n4 (0.4) and Dema Ethyl Sulfate (0.4) for the varying interaction between PBDT chains and the anions in ILs. We are conducting in depth quantum chemistry calculations to measure the interaction energies between anions and PBDT polymer chains, thus will offer more clear idea about the determining factors in the ion exchange process. Figure \n4 e shows ionic conductivities of the IPEs as a function of temperature. The exceedingly high σ at RT (> 1 mS cm \n- 1) originates from the fibrillar and nanocrystalline conducting phase formed in the composite structure of IL and liquid-crystalline polymers reported previously. \n1, 6 Meanwhile, all samples show stable Li stripping and plating at varying current grades in the Li||Li cell cycling process. As shown in Fig. \n4 f, C \n2 mimTFO and C \n2 mim Ethyl Sulfate display stable cycling at high current density ( \nJ) at 6 mA cm \n- 2 at 80°C, which is promising, since most organic cells reported cannot sustain any stable performance at this high temperature without any safety concerns.\n\nIn this section, we mainly extend the investigation of IPEs based on C \n2 mimTFO at varying temperature and cell configurations. In Fig. \n5 a, we initially test the symmetric cell performance at varying \nJ at RT. The critical \nJ is 2.0 mA cm \n− 2 at RT. As shown in Fig. \n5 b, the cells can maintain at least 800 hours at 1 mA cm \n− 2 at RT, which is rarely seen by other single-layer polymer electrolytes without any supporting separators or organic plastiziers. \n41 In addition, we prepare the Li|IPEs|Cu cell to investigate the plating and striping of Li at the Cu anode based on these IPEs. Figure \n5 b shows the voltage-cycle profile for the cells at RT. The secondary axis shows the corresponding columbic efficiency (CE) values, the average value of which is > 98%. The reported average CE for Li||Cu cell using regular organic electrolytes is ~ 90%, which indicates the highly reversible Li deposition on Cu surface of these IPEs. \n42–44 The SEM images of the deposited Li on current collector is included in the Supplementary Note 7. We observe no Li dendrites formed using these IPEs coupled with Li metal anodes.\n\nFor practical application, we also report the full cell performance based on the commercial LiFePO \n4 cathode with high loading (10.3 mg cm \n− 2). Figure \n6 a shows the long-term cycling of the full cell at RT at 0.5 C rate, the cell shows 96% capacity retention at 350 cycle. The voltage capacity files for the selected main cycles are shown in Fig. \n6 b. The major population of the CE is between 100.1% – 100.2%, which is slightly higher than the theoretical maximum value (100%) because of the thermal fluctuation at the ambient temperature. Thus indicates the high reversibility of the Li metal cells based on this IPEs at RT. Figure \n6 c shows the long-term cycling of the full cell at 50°C at 2 C rate, the cell shows not only high average CE (> 99.9), but also 80% capacity retention at 350th cycle, which is promising to satisfy the fast charge/discharge requirements for widely used portable devices. The voltage capacity files for the selected main cycles are shown in Fig. \n6 d. At last, we also investigate the fast charge/discharge capability and thermal stability of this IPEs at 80°C, which is a dangerous temperature for regular organic cells. Figure \n6 e shows the cycling performance of the IPE at increasing C rate from 0.5 C (0.53mA/cm2) to 5 C (5.3 mA cm- \n2)) at 80°C. Here, we observe that the cell can cycle without short circuit at super high \nJ up to 5C (8.3 mA cm \n− 2), which show promise for this IPEs as next-generation solid-state electrolytes for fast charge LMBs at mid-high temperatures. The corresponding voltage capacity curves for the selected cycles are shown in Fig. \n6 f.\n\nIn summary, we have described a machine learning-guided screening protocol to filter promising ILs with high ionic conductivity and wide electrochemical window for preparation of IPEs in LMBs. In addition, we further confirm the rigid-rod liquid crystalline polyelectrolyte PBDT as an essential polymer matrix to develop a series of solid-state polymer electrolytes with extremely high CE and excellent fast charge and discharge performance at high temperature. This platform shows immense potential to serve as an efficient method to quickly focus on the essential ionic liquids for specific applications. More importantly, this work provides novel insights into strategies to overcome the data scarcity issues and realize the efficient utilization of ML in material design and optimization. Through investigation of the golden rules, we could fabricate IPEs with tunable variations in mechanical, structural and transport properties for a large array of applications in versatile functional devices, including capacitors, mechanical actuators, water reverse osmosis membranes and so on.\n\n# Methods\n\n## Machine Learning\nPython programming language was used to conduct the machine learning workflow. For the unsupervised learning, Dendrogram function from the SciPy package was used to perform the agglomerative hierarchical clustering. For the supervised learning, three main algorithms, including support vector machine, random forest and XGBoosting from the Scikit-learn package were used for the regression and classification. Graph convolutional neural network (GCN) has been employed to conduct the classification in the supervised learning according to the RDkit and PyTorch Geometic (PyG) library. The machine learning workflow mainly consists of 8 sections, the code for each section were packaged in a Class object and the description of the codes are available at the GitHub website.\n\n## Quantum chemistry calculation\nAll quantum chemistry calculation were performed using Psi4 based on self-consistence field method with basis set of 6-311 + g**. The Psikit module, which is an ensemble of RDkit and Psi4, has been used to connect and perform the calculation of the energy, the HOMO, the LUMO, the total dipole moment and the individual dipole moments along the three main directions for the cations and anions in the IL permutation table.\n\n## Materials\nPoly 2,2′-disulfonyl-4,4′-benzidine terephthalamide (PBDT) was synthesized by interfacial condensation polymerization as described previously. 45, 46 1-ethyl-3-methylimidazolium triflate, 1-ethyl-3-methylimidazolium tetrafluoroborate, 1-ethyl-3-methylimidazolium ethyl sulfate and diethylmethylammonium triflate were purchased from IoliTech. N-propyl-N-methylpyrrolidinium bis(fluorosulfonyl)imide (C3mpyrFSI, purity > 99.9%) and Lithium bis(fluorosulfonyl)imide (LiFSI, purity > 99.5%) were purchased from Solvionic. Lithium metal (Li-metal) foil with thickness of 180 µm was sourced from Hongwei Lithium Co. Ltd. (purity > 99.9%). The LiFePO4 cathode with area loading of 10.3 mg cm− 2 and Cu foil were sourced from Canrd.\n\n## Preparation of the ionic polymer electrolytes (IPEs)\n0.45 g ILs and 0.05 g PBDT were dissolved in 5 g distilled water separately. The two aqueous solutions were mixed while heated up to 50 ̊C. Then the mixture solutions were poured into a 80mm × 60 mm PTFE mode. The water solvent was slowly evaporated at RT and followed with vacuum drying at 80 ̊C for at least 24 h before transferring to the glove box. The membrane was then cut to round disks with a diameter of 9 mm and then immersed in the ionic liquid electrolytes (ILEs) for > 24 h at RT. The ILEs were prepared by adding the prescribed amounts of LiFSI to C3mpyrFSI IL at RT in an Ar-filled glove box (< 0.01 ppm O2 and < 0.01 ppm H2O). The concentration of LiFSI in the ILEs employed in this work is 3.2 mol kg−1.\n\n## Symmetric and full cells\nThe Li-metal symmetric coin cells were prepared with CR2032 cases with two 5 mm diameter Li-metal electrodes and 9 mm diameter IPEs (~ 50 µm) between them in an Ar-filled glove box. The Li|IPEs|Li symmetric coin cells were used for polarization, impedance spectroscopy and cycling measurements. The Li|IPEs|LiFePO4 and Li|IPEs|Cu coin cells were also prepared for investigation of the electrochemical cycling performance, correspondingly. A Neware system were used for battery testing.\n\n## Cyclic voltammetry\nA stainless steel working electrode and a Li-metal foil counter electrode were employed for cyclic voltammetry. The CV measurements were performed against Li|Li+ redox potential. All scans were performed at RT with 10 mV s− 1 scan rate using a Biologic VMP 3e controlled by EC-Lab (ver. 10.40) software.\n\n## Ionic conductivity\nThe ionic conductivity was measured via dielectric response over a 100 mHz – 1 MHz frequency range for the assemble coin cells with stainless steel as the electrodes. A temperature scan range − 50°C to 150°C was selected, and the temperature was controlled by an oven. The ionic conductivities of the IPEs were obtained by fitting the electrochemical impedance spectra to an equivalent circuit model using EC-Lab (ver. 13.40) software®.\n\nLi Transference Number (tLi+): The transference number was determined by direct current (DC) polarization. An AC impedance test was firstly performed over a 100 mHz to 1 MHz range to obtain the interfacial resistance before and after the polarization. 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Molecular Alignment and Ion Transport in Rigid Rod Polyelectrolyte Solutions. *Macromolecules* **47**, 2984–2992, doi: 10.1021/ma500364t (2014).\n\n# Supplementary Files\n\n- [WangMLPolymerElectrolytesupporting20221031.docx](https://assets-eu.researchsquare.com/files/rs-2220925/v1/bcee1c08f62190e8e958ce12.docx) \n Supplementary Note 1-7 and Supplementary Table 1-2"} {"paper_id": "prb34", "title": "Theoretical and Experimental Studies of ion Transport in Mixed Polyanion Solid Electrolytes", "text": "Theoretical and Experimental Studies of ion Transport in Mixed Polyanion Solid Electrolytes\n\nZeyu Deng\nNational University of Singapore https://orcid.org/0000-0003-0109-9367\n\nTara Mishra\nNational University of Singapore\n\nEunike Mahayoni\nUniversité de Picardie Jules Verne\n\nQianli Ma\nForschungszentrum Jülich https://orcid.org/0000-0002-4709-4927\n\nOlivier Guillon\nForschungszentrum Juelich GmbH, Institute of Energy and Climate Research IEK-1\n\nJean-Noel Chotard\nUniversity of Picardie Jules Verne https://orcid.org/0000-0002-9867-7954\n\nVincent Seznec\nhttps://orcid.org/0000-0001-5233-5943\n\nAnthony K. Cheetham\nUniversity of Cambridge https://orcid.org/0000-0003-1518-4845\n\nChristian Masquelier\nUniv. Picardie Jules Verne\n\nGopalakrishnan Sai Gautam\nMassachusetts Institute of Technology https://orcid.org/0000-0002-1303-0976\n\nPieremanuele Canepa (pcanepa@nus.edu.sg)\nNational University of Singapore https://orcid.org/0000-0002-5168-9253\n\nArticle\n\nKeywords: ion transport, polyanion mixing, NASICON\n\nPosted Date: December 1st, 2021\n\nDOI: https://doi.org/10.21203/rs.3.rs-1102507/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\nVersion of Record: A version of this preprint was published at Nature Communications on August 2nd, 2022. See the published version at https://doi.org/10.1038/s41467-022-32190-7.\nTheoretical and Experimental Studies of ion Transport in Mixed Polyanion Solid Electrolytes\n\nZeyu Deng,1* Tara P. Mishra,1,2 Eunike Mahayoni,3,4,5 Qianli Ma,6 Olivier Guillon,6,7 Jean-Noël Chotard,3,4,5 Vincent Seznec,3,4,5 Anthony K. Cheetham,1 Christian Masquelier3,4,5 Gopalakrishnan Sai Gautam,8 and Pieremanuele Canepa1,2,9 #\n\n1Department of Materials Science and Engineering, National University of Singapore, Singapore 117575, Singapore\n2Singapore-MIT Alliance for Research and Technology, 1 CREATE Way, 10-01 CREATE Tower, Singapore 138602, Singapore\n3Laboratoire de Réactivité et de Chimie des Solides (LRCS), CNRS UMR 7314, Université de Picardie Jules Verne, 80039 Amiens Cedex, France.\n4RS2E, Réseau Français sur le Stockage Electrochimique de l’Energie, FR CNRS 3459, F-80039 Amiens Cedex 1, France.\n5ALISTORE-ERI European Research Institute, FR CNRS 3104, Amiens, F-80039 Cedex 1, France.\n6Forschungszentrum Jülich GmbH, Institute of Energy and Climate Research, Materials Synthesis and Processing (IEK-1), 52425 Jülich, Germany\n7Helmholtz-Institute Münster, c/o Forschungszentrum Jülich GmbH, 52425 Jülich, Germany\n8Department of Materials Engineering, Indian Institute of Science, Bengaluru, 560012, Karnataka, India\n9Chemical and Biomolecular Engineering, National University of Singapore, 4 Engineering Drive 4, Singapore, 117585, Singapore.\n\nCorresponding authors: *msedz@nus.edu.sg and #pcanepa@nus.edu.sg\nAbstract\nLithium and sodium (Na) mixed polyanion solid electrolytes for all-solid-state batteries display some of the highest ionic conductivities reported to date. However, the effect of polyanion mixing on ion transport properties is still debated. Here, we focus on Na_{1+x}Zr_2Si_xP_{3-x}O_{12} (0 \\leq x \\leq 3) NASICON electrolyte to elucidate the role of polyanion mixing on Na-transport properties. Although there is a large body of data available on this NASICON system, transport properties extracted from experiments or theory vary by orders of magnitude, signifying the need to bridge the gap between different studies. Here, more than 2,000 distinct ab initio-based kinetic Monte Carlo simulations have been used to map the statistically vast compositional space of NASICON over an unprecedented time range and spatial resolution and across a range of temperatures. We performed impedance spectroscopy of samples with varying Na compositions revealing that the highest ionic conductivity (\\(~0.1\\ S\\ cm^{-1}\\)) is achieved in Na_{3.4}Zr_2Si_{2.4}P_{0.6}O_{12}, in line with our predictions (\\(~0.2\\ S\\ cm^{-1}\\)). Our predictions indicate that suitably doped NASICON compositions, especially with high silicon content, can achieve high Na^+ mobilities. Our findings are relevant for the optimization of mixed polyanion solid electrolytes and electrodes, including sulfide-based polyanion frameworks, which are known for their superior ionic conductivities.\nIntroduction\n\nThe reliability of rechargeable batteries and other energy storage devices depends on the fast delivery of ions between electrodes.\\(^{1-4}\\) In rechargeable batteries, the safety and performance of electrolytes are as important as other battery components, such as electrodes. Solid-state batteries, where liquid electrolytes are replaced by solid fast-ion conductors, offer a promising pathway for safer commercial lithium-ion and prototypical sodium (Na)-ion batteries.\\(^{4-6}\\) Several solid electrolytes, such as the LiSiCON-type Li\\(_{4±x}\\)Si\\(_{1-x}\\)Z\\(_x\\)O\\(_4\\) (Z = P\\(^{5+}\\), Al\\(^{3+}\\), Sn\\(^{4+}\\) and/or Ge\\(^{4+}\\)),\\(^{7,8}\\) Li\\(_{10}\\)MP\\(_2\\)S\\(_{12}\\) made from Li\\(_4\\)MS\\(_4\\):Li\\(_3\\)PS\\(_4\\) (M = Ge\\(^{4+}\\), Sn\\(^{4+}\\), and Si\\(^{4+}\\)),\\(^{9-16}\\) and Na\\(_{1+x}\\)Zr\\(_2\\)Si\\(_x\\)P\\(_{3-x}\\)O\\(_{12}\\) (hereafter referred as NASICON),\\(^{17-19}\\) leverage mixed polyanion frameworks to attain some of the highest ionic conductivities (\\(\\approx 10\\) mS/cm) reported so far.\\(^4\\)\n\nIon transport in mixed polyanion solid electrolytes has been investigated using both computation and experiments before.\\(^{4,9,18,7,11}\\) Yet transport properties measured from different techniques typically vary by orders of magnitude.\\(^{20}\\) On one hand, averaged transport properties obtained from experiments, such as impedance spectroscopy, solid-state nuclear magnetic resonance, and quasi-elastic neutron scattering,\\(^{4,6,16,21}\\) may incorporate effects arising from defects and grain boundaries.\\(^{22}\\) On the other hand, classical or *ab initio* molecular dynamics (MD) studies perform “one shot” simulations on selected bulk structures, which may not be sufficiently representative in terms of longer time-scale transport processes as well as in the number of possible arrangements of different polyanions.\\(^{2,3,23-25}\\) Thus, there is a need to reconcile the measurements and simulations to guide the development and manufacturing of the next generation of solid electrolytes and their batteries.\n\nIn this study, we have selected the NASICON Na\\(_{1+x}\\)Zr\\(_2\\)Si\\(_x\\)P\\(_{3-x}\\)O\\(_{12}\\) (\\(0 \\leq x \\leq 3\\)) electrolyte as an example to elucidate the role of polyanion mixing on the macroscopic\ntransport properties, including ionic diffusivity and conductivity. The choice of NASICON is justified by the large body of data available on this system since its discovery more than 40 years ago,\\(^{17,18,26-29}\\) making it easier to reconcile previous experimental and computational studies.\n\nTo capture the large statistical variance in transport properties introduced by mixed polyanions in NASICON samples, we developed a high-fidelity kinetic Monte Carlo (kMC) model bearing the accuracy of density functional theory (DFT) calculations. More than 2,000 distinct kMC simulations served to map the statistically vast compositional space of Na\\(_{1+x}\\)Zr\\(_2\\)Si\\(_x\\)P\\(_{3-x}\\)O\\(_{12}\\) over an unprecedented time range – in the realm of milliseconds – and spatial resolution, with varying temperature.\n\nFirst of all, our model reproduces existing measurements of Na-transport properties in NASICON, suggesting that a robust sampling of both the spatial and temporal axes is required in computations to accurately estimate these properties. The reproduction of measured Na-transport properties in NASICON also implies that our model correctly captures the collective nature of Na-transport, which is responsible for the high ionic conductivity observed in NASICON. Second, our simulations elucidate the impact of the thermodynamic forces driving the random distribution of PO\\(_4^{3-}\\) and SiO\\(_4^{4-}\\) groups in NASICON during synthesis (and subsequent thermal treatment) on the Na-ion transport. Third, our statistical insights can guide the selection of optimal doping and thermal treatment strategies to further improve the properties of NASICON electrolytes. For example, our analysis suggests that higher Na\\(^+\\) conductivity in NASICON can be achieved by increasing the content of SiO\\(_4^{4-}\\) units in place of PO\\(_4^{3-}\\) moieties, while maintaining high Na content in the structure. Motivated by our computational findings, we have also synthesized and characterized selected compositions of the NASICON, which validates our predictions. These findings,\nelaborated on NASICON electrolytes, are general and transferable to the study of ionic transport in other topical mixed-polyanion Li and Na solid electrolytes.\nResults\n\nFigure 1a depicts the crystal structure of NASICON, where red SiO4/PO4 tetrahedra share corners with two blue ZrO6 octahedra forming the so-called “lantern units”. In the rhombohedral high-temperature NASICON structure (\\( R\\overline{3}c \\)), there are two independent and partially occupied sodium sites, Na(1) and Na(2). The partial occupancy of these sites gives rise to the well-known high ionic conductivity in NASICON. A third interstitial Na site, known as Na(3), adjacent to Na(1) and Na(2) has been previously considered.\\(^{30,31}\\) However, Zhang et al.\\(^{32}\\) showed that Na(3) is negligibly occupied over a wide range of temperatures (200 < T < 800 \\(^\\circ\\)C) and less relevant for Na-transport in NASICON. The structural images in Figure 1b and c emphasize the Na(1) sites, with their neighboring Na(2) (orange spheres) and Si/P (red spheres) sites, resulting in distorted hexagonal prisms (silver). For visualization purposes, Figure 1b and c omit the Zr and O atoms.\nFigure 1 | Characteristics of sodium ion transport in NASICON. Structural models of Na_{1+x}Zr_2Si_xP_{3-x}O_{12} (a, b, c, and d) and Na-migration barriers (e). In a, b, c and d, the Na(1) sites are indicated by silver spheres, the Na(2) by orange spheres, the (Si/P)O_4 groups by red tetrahedra, Si/P atoms by red spheres, and ZrO_6 units by blue octahedra. b and c depict the local environment of Na(1), with each Na(1) surrounded by six neighboring Na(2) atoms (orange spheres) and six Si/P (red spheres) atoms. For simplicity, O and Zr atoms are not shown in b, c, and d. Each silver hexagonal prism in b or c represents the first coordination shell of a Na(1) site. Panel d is the migration unit used to study Na-migration in NASICON, and Na must hop across several different migration units to ensure Na diffusion. Red triangles in d indicate the bottlenecks caused by Si/PO_4 tetrahedra (oxygen atoms are not shown). e shows the averaged kinetically resolved activation (KRA) barriers for Na(2)→Na(1) hops, with varying Na(2) site occupation and Si/P content per migration unit. The barriers were extracted from a local cluster expansion model, which was fitted to the calculated nudged elastic band (NEB) barriers. The diagonal line in e shows locally charge neutral Si/P configurations. The computed NEB barriers used for fitting to generate the heatmap in e are available in the supporting information (SI).\nFigure 1d shows the smallest relevant unit –the migration unit– encompassing all possible migration events for Na-ions in NASICON. The migration unit centered around Na(1) highlights the connectivity between the Na(1) site and its closest six Na(2) neighbor sites, as well as the neighboring Si(P) atoms. Each migration unit (see Figure 1b and c) is edge-shared with six neighboring migration units, where each unit can exhibit its own distribution of Na/vacancies and Si/P. In the NASICON structure, Na-transport must always involve both Na(1) and Na(2) sites,\\(^{18,30,33,34}\\) giving rise to migration pathways of the kind Na(1) \\( \\leftrightarrow \\) Na(2). The specific Na-migration pathway depends entirely on the Na and Si/P content within the structure,\\(^{19,30,31}\\) which sets the occupation and the relative stability of Na(1) and Na(2) sites. For example, at low Na content (\\( x = 0 \\)), Na ions reside only in Na(1) sites, favoring a Na(1) \\( \\leftrightarrow \\) Na(2) \\( \\leftrightarrow \\) Na(1) pathway.\\(^{17,30,32}\\) At higher Na content (\\( x \\geq 2 \\)), both Na(1) and Na(2) sites are occupied to varying degrees (see later Figure 2), and any of the two migration pathways can be active.\\(^{19,30}\\) Importantly, for macroscopic Na diffusion to occur in NASICON, several successful migration hopping events, between adjacent migration units, need to happen, for which it is critical that Na atoms can hop from Na(1) to Na(2) sites (or vice-versa) within each unit. Thus, we considered a single migration event to be Na(1) \\( \\leftrightarrow \\) Na(2) within a single migration unit, in the presence of varying Na and Si/P content.\n\nFor any Na composition in the range \\( 0 \\leq x \\leq 3 \\), the concentrations of Si, and P are set by the NASICON stoichiometry, such that the composition guarantees global charge neutrality (i.e., the NASICON cell is electrostatically neutral). However, each migration unit can exhibit random occupancies of Si/P in Si/P sites, and Na/vacancies in the Na(2) sites (panels b, c and d of Figure 1). Consequently, the migration of Na-ions may occur through migration units that are not locally charge neutral, i.e., a given unit by itself may not be electrostatically neutral. In our work, we consider all possible\nNa(1)↔Na(2) hopping events within a given migration unit, including scenarios with and without local charge neutrality.\n\nWe evaluated all the unique Na-ion migration pathways that are possible within a migration unit of Figure 1d using the nudged elastic band method (NEB)\\(^{35}\\) together with density functional theory (DFT), and using the strongly constrained and appropriately normed (SCAN) meta-generalized gradient approximation.\\(^{36}\\) The NEB method is designed to calculate migration barriers in solid electrolytes, as highlighted by prior studies.\\(^{2,3,37,38}\\) We identified 32 unique Na-hops, given the migration unit of Figure 1d, which included barriers computed at different Si and P compositions and Na/vacancy contents (Section S2 of the Supporting Information, SI). The calculated migration barriers at 0 K are defined as the difference between the highest energy state and the configuration with the lowest energy —the initial and/or final end point.\\(^{37}\\) The accuracy of our computed barriers is validated by the excellent agreement with existing data. For example, our calculated barrier at NaZr\\(_2\\)PO\\(_4\\)\\(_3\\) (\\(~ 458\\) meV, Table S1) agrees well with existing experimental values (\\(~ 470\\) meV)\\(^{26}\\) and *ab initio* MD (\\(~ 472\\) meV).\\(^{32}\\)\n\nTypically, migration events have an intrinsic directional dependence if the initial and final states are not equivalent, i.e., a Na(1) → Na(2) hop may exhibit a different migration barrier compared to the reverse hop, Na(2) → Na(1), due to energy differences between the end points, namely, Na(1) and Na(2). Van der Ven et al.\\(^{39}\\) introduced the kinetically resolved activation (KRA) barrier, or \\( E_{KRA} \\) (see Equation 2 in the Methods section) that removes the directional dependence of the migration barriers. Note that low values of \\( E_{KRA} \\) correspond to low values of migration barriers and vice versa. Furthermore, we trained a local cluster expansion (LCE) Hamiltonian\\(^{40}\\) on the computed \\( E_{KRA} \\) values (listed in Table S1 of the SI), which assigns a single\n\\( E_{KRA} \\) value per migration unit and enables simulating large supercells of NASICON over long time-scales within our in-house kinetic Monte Carlo (kMC) package (Methods section and Section S3 and S4 of SI). The main advantage of the LCE over computationally expensive NEB calculations at all possible configurations, is that it enables the rapid estimation of \\( E_{KRA} \\) (and the corresponding migration barriers) at all Na(2), Si and P compositions in a given migration unit.\n\nThe average \\( E_{KRA} \\) values obtained by the LCE model are plotted in Figure 1e, with the dashed black diagonal indicating migration units that are locally charge neutral. Off-diagonal barriers are for locally charged situations and reflect multiple Na and Si/P configurations. For example, there are 400 possible configurations for a migration unit with 3 Na and 3 Si, and the \\( E_{KRA} \\) of \\( \\sim 410 \\) meV (Figure 1e) is obtained by averaging the barriers across all the configurations. A similar averaging procedure is used for all scenarios where multiple Na/vacancy and Si/P configurations can exist within the same migration unit.\n\nDepending on the Si/P environments, two distinct regions of high and low average \\( E_{KRA} \\) are inferred from Figure 1e. At lower Si or higher P content (bottom rows of Figure 1e), high average \\( E_{KRA} \\) (\\( \\sim 500 \\) meV or similar) are observed. In contrast, increasing the Si content or decreasing the P content (top rows of Figure 1e) lowers the average \\( E_{KRA} \\) (values as low as \\( \\sim 50 \\) meV). Importantly, an increase in Si concentration in NASICON lowers the average \\( E_{KRA} \\). The monotonic decrease in \\( E_{KRA} \\) (and migration barriers) with Si content can be attributed to lower Si\\(^{4+}\\)-Na\\(^+\\) electrostatic repulsion compared to P\\(^{5+}\\)-Na\\(^+\\) repulsion during Na-migration.\n\nChanging the Na concentration at a given Si/P content within the migration unit does not result in a monotonic increase or decrease in average \\( E_{KRA} \\). For instance, at\n4/6 Si @ Si/P site in Figure 1e, the average \\( E_{KRA} \\) is low at both 0/6 Na @ Na(2) site and at 6/6 Na @ Na(2) site, with the average \\( E_{KRA} \\) reaching a maximum at 3/6 Na @ Na(2) site. This non-monotonic behavior is likely due to a combination of local electrostatic repulsions and local charge imbalance within the migration unit. For example, at 6/6 Na @ Na(2) site and 0/6 Si @ Si/P site (bottom right corner of Figure 1e), a high \\( E_{KRA} \\) can be attributed to the higher electrostatic repulsion between the Na\\(^+\\) and P\\(^{5+}\\) ions. In contrast, low barriers at both 0/6 Na @ Na(2) and 6/6 Na @ Na(2) along 4/6 Si @ Si/P are likely because of high local charge imbalance that destabilizes the initial/final Na(1) and Na(2) configurations along the pathway. Eventually, high Na content in the migration unit contributes to low \\( E_{KRA} \\), particularly at high Si content, as indicated by the blue squares towards the top right corner of Figure 1e. Indeed, the lowest values of \\( E_{KRA} \\) are observed at both high Na and high Si contents.\n\nCombining the LCE and kMC, we investigated the relevant Na-transport properties in NASICON, such as ionic diffusivity and conductivity. The main advantage of using a kMC framework is the access to statistically significant amounts of data over large length and time scales, as well as the ability to sample a wide variety of configurations. By comparison, a classical or *ab initio* MD simulation\\(^{3,23-25}\\) performs a “one shot” representative calculation of a system at a given atomic configuration and composition, over smaller length and orders of magnitude shorter time scales.\n\nIn total, more than 2,000 kMC simulations were performed to predict the Na\\(^+\\) diffusivities and conductivities at selected temperatures of 373, 473 and 573 K of 50 NASICON models (with varying Si/P configurations) at 11 distinct Na concentrations. Using canonical Monte Carlo simulations from our previous work,\\(^{19}\\) 550 starting NASICON configurations (50 configurations × 11 concentrations) were generated at high temperature (~1500 K), which mimics the typical synthesis conditions and thermal\ntreatments of \\( \\mathrm{Na}_{1+x}\\mathrm{Zr}_2\\mathrm{Si}_x\\mathrm{P}_{3-x}\\mathrm{O}_{12} \\) and other NASICON-based electrodes.\\(^{17,28,30,41}\\)\n\nUsing high-temperature structures as starting configurations in our kMC guarantees a random distribution of PO\\(_4\\) and SiO\\(_4\\) tetrahedra in the NASICON structures, as observed in reports.\\(^{17,30,32,41}\\) The choice of temperatures for the study of Na-transport in our work (measured at 373 – 573 K) is largely motivated by the availability of experimental measurements to compare, but our framework can be easily extended to other temperatures as well. The comprehensive statistical analysis of this study, which addresses the role played by the PO\\(_4\\) and SiO\\(_4\\) distributions on overall Na-ion transport in \\( \\mathrm{Na}_{1+x}\\mathrm{Zr}_2\\mathrm{Si}_x\\mathrm{P}_{3-x}\\mathrm{O}_{12} \\), is essential to capture differences occurring during the sample preparation.\\(^{19}\\)\n\n![Four plots showing Na+ diffusivity, conductivity, Haven ratio, and correlation factor as a function of x in Na_{1+x}Zr_2Si_xP_{3-x}O_{12} for different temperatures.](page_362_682_1042_627.png)\nFigure 2 | Computed Na-ion transport properties of Na_{1+x}Zr_2Si_xP_{3-x}O_{12} bulk based on kinetic Monte Carlo simulations. Calculated Na^+ diffusivity (a), conductivity (b), Haven’s ratio (c) and averaged correlation factor (d) of Na_{1+x}Zr_2Si_xP_{3-x}O_{12} at several temperatures: 373 (dark blue circles), 473 (orange squares) and 573 (red triangles) K, respectively. In panel b, the computed ionic conductivities are compared with the experimental values of this work (see Figure 4 and Figure S6 of the SI) at selected temperatures. Experimental values in b are depicted with larger light blue circles (373 K), yellow squares (473 K), and red triangles (573 K). An exhaustive comparison with previous experimental values of ionic conductivities is shown in the Supporting Information (Figure S6). The grey band in panel b shows the interval of confidence of our predictions at 573 K, which is lower in magnitude than the variance of Na-ion conductivities observed experimentally (Figure S6).\n\nFigure 2 shows the computed Na^+ diffusivity (D, panel a), the conductivity (\\( \\sigma \\), panel b), Haven’s ratio (H_R, panel c) and averaged correlation factor (f, panel d) at relevant temperatures of 373, 473, and 573 K, from kMC simulations of Na_{1+x}Zr_2Si_xP_{3-x}O_{12} as the Na content (x) is varied. Note that the conductivity values (\\( \\sigma \\)) in Figure 2b were calculated using the Nernst-Einstein equation, as expressed in terms of diffusivity D in Equation 1.\\(^{3,23,24,39,40}\\)\n\n\\[\n\\sigma = \\frac{e^2 C}{k_B T} D\n\\]\n\nwhere \\( e \\) is the elemental charge, \\( C \\) is the concentration of Na-ions, \\( k_B \\) is the Boltzmann constant and \\( T \\) is the temperature. Importantly, in Equation 1, D is the diffusivity of the center-of-mass of Na-ions in the NASICON structure, which includes cross-correlations of the migrations of different Na-ions (see Section S4 of SI) and not the tracer diffusivity, as often used in many studies.\\(^{23,39,40}\\)\nAs confirmed by Figure 2a and Figure 2b, a temperature increase can significantly boost both Na\\(^+\\) diffusivities and conductivities across the full Na concentration. Interestingly, Na diffusivity and conductivity increase for increasing Na (and Si) concentrations up to x ~ 2.4, beyond which there is a drop in both diffusivity and conductivity. Thus, we conclude that Na-ion transport in Na\\(_{1+x}\\)Zr\\(_2\\)Si\\(_x\\)P\\(_3-x\\)O\\(_{12}\\) is fastest at x ~ 2.4, at all temperatures considered in this work, which agrees with our experimental observations presented below.\n\nFigure S6 reveals a significant spread of experimentally measured ionic conductivities from different reports,\\(^{18,27,33,42-45}\\) which is indicative of the difficulties in performing accurate measurements as well as the large variability in sample preparation. Nonetheless, for Na\\(_3\\)Zr\\(_2\\)Si\\(_2\\)P\\(_1\\)O\\(_{12}\\) our measured experimental conductivity (see Figure 4b) of ~ 0.1 S cm\\(^{-1}\\) at 573 K is in excellent agreement with our computed value of ~ 0.2 S cm\\(^{-1}\\). Our model also agrees with previous measurements\\(^{18,19,30,32}\\) which report a low conductivity and diffusivity in Na\\(_1\\)Zr\\(_2\\)P\\(_3\\)O\\(_{12}\\).\n\nPrevious studies have shown that correlated ion-migration can contribute to high diffusivity and conductivity in ionic conductors.\\(^{3,4,7,23,32,40,46,47}\\) In regimes of non-dilute diffusion carriers, the Haven’s ratio (H\\(_R\\)) of Figure 2c quantifies the degree of cross-correlation between migrating Na\\(^+\\) ions, i.e., the extent to which individual Na\\(^+\\) hops contribute to the overall motion of the Na\\(^+\\) center-of-mass (Equation S8 of SI). H\\(_R\\) varies between 1 (no cross-correlation or a random movement of individual Na\\(^+\\) ions) and 0 (fully correlated transport or non-random movement). While we observe small values of H\\(_R\\) (0.01 – 0.2) throughout the Na concentration range in the NASICON, indicating significant cross-correlation between Na ions, H\\(_R\\) at low Na concentrations (x ~ 0) is moderately high (~ 0.2) compared to high Na concentrations (H\\(_R\\) ~ 0.01 at x ~ 3). The variation in H\\(_R\\) with Na composition (x) can be partly attributed\nto the occupancy of Na across the Na(1) and Na(2) sites in the NASICON. For example, at x ~ 0, Na^+ mostly resides in the Na(1) sites, which are separated from each other by large distances (~ 6.47 Å), suggesting lower degrees of cross-correlations between migrating Na^+ ions. At x ~ 3, Na^+ ions populate both Na(1) and Na(2),\\(^{30}\\) which are separated by shorter distances (~ 3.48 Å) than Na(1)-Na(1), possibly facilitating correlated migration of Na^+ ions. Interestingly, cross-correlation between Na^+ ions shows an increase with increasing temperature, as indicated by the drop in H_R with rising temperature at all x (Figure 2c); this trend also coincides with increasing of D and \\( \\sigma \\), highlighting the positive impact of correlated motion on the overall Na-ion transport.\n\nAnother type of correlation, specifically between successive jumps of the same Na^+ ion, is to estimate the average correlation factor, \\( f \\), of Figure 2d (see Equation S10 of the SI). \\( f \\) measures the variation in local environments (resulting in a change of migration barriers) as experienced by individual Na^+ ions as they migrate through NASICON. \\( f \\) captures the deviation away from a truly random walk of a given Na^+ ion within the structure, with \\( f = 1 \\) indicating a true random walk and \\( f = 0 \\) signifying truly non-random walk. Thus, \\( f \\) is different from H_R, which describes the correlation between the motions of different Na^+ ions. Similarly, to our observations with H_R, we find that correlation effects, as measured by \\( f \\), are quite pronounced at all Na concentrations in NASICON (Figure 2d). For example, \\( f \\) decreases progressively from 0.2 to 0.01 as x varies from 1 to 2. Notably, \\( f \\) exhibits more significant non-monotonic behavior compared to H_R in the range 0 < x < 3.\n\nOne of the main reasons behind the high degree of correlation (as indicated by H_R and f) in NASICON is the high sensitivity of the E_{KRAS} to the local Si/P environment (Figure 1e). Indeed, one may observe large variations in the local migration units,\nwhich leads to significant changes in \\( E_{KRA} \\), at a given Na concentration. This is clearly shown in **Figure S2**, where the migration barrier varies between ~ 300 meV and ~ 800 meV at x ~ 2. Every Na\\(^+\\) migration event leads to a dynamic change in local environment by creating new vacancies and eliminating existing ones, which can have sizeable effects on the migration barriers (and hence \\( E_{KRA} \\)), eventually resulting in highly correlated motion.\n\n![Panel a shows sodium occupancies as a function of Na content, panel b shows N(Na+) × N(Vacancy) as a function of Na content](page_184_670_1082_393.png)\n\n**Figure 3 | Sodium occupancies and concentrations as a function of Na content.** Panel **a** shows the averaged Na site occupancy at Na(1) site (blue circles) and Na(2) site (blue triangles) from kMC simulations at 443 K, and compared with previous Grand Canonical Monte Carlo simulations\\(^{19}\\) (red circles and triangles) at the same temperature, and existing experimental data\\(^{30}\\) (in orange circle and triangles). Dashed lines are used as guide for the eye. Panel **b** shows \\( N(\\mathrm{Na^+}) \\times N(\\mathrm{Vacancy}) \\) (solid blue curve, per f.u.) at 443 K from kMC simulations. The contributions to \\( N(\\mathrm{Na^+}) \\times N(\\mathrm{Vacancy}) \\) from individual sodium sites, Na(1) and Na(2), are shown as blue dashed lines. In panel **b**, the shaded regions mark areas where Na\\(^+\\)-ion conductivity is highly (red) or slightly (blue) impacted by the charge carrier concentration.\n\nIt is worth analyzing how the distribution of Na-ions, across the Na(1) and Na(2) sites controls the Na diffusivity (and conductivity) of NASICON. **Figure 3a** shows the\naveraged Na occupancy of the Na(1) and Na(2) sites, as extracted from our kMC simulations. We compare these values with single-crystal X-ray diffraction experiments by Boilot et al.\\(^{30}\\) at specific compositions, and our previous grand-canonical Monte Carlo simulations,\\(^{19}\\) which do not account for the dynamics of the Na\\(^+\\) ions.\n\nIn NASICONs,\\(^{18,48}\\) Na-transport can only occur if multiple exchanges between Na(2)\\(\\leftrightarrow\\) Na(1) sites occur.\\(^{18,30,31}\\) This implies that both Na(1) and Na(2) must be occupied to some degree\\(^{18,30,31}\\) for facile transport. The Na site occupancies derived from our kMC data which includes possible Na-migration events, at 443 K (170 °C, blue shapes in **Figure 3a**) show that both Na(1) and Na(2) are partially occupied at compositions \\(1 < x < 3\\). The kMC results are in qualitative agreement with X-ray measurements at 443 K of Ref. 30 (orange shapes in **Figure 3a**). In contrast, occupations generated by the grand-canonical Monte Carlo model (red filled shapes in **Figure 3a**) indicate the equilibrium Na occupancies, which are distinctly different from the kMC simulations (and experiments) that include the impact of Na movement.\n\nImportantly, both our kMC and grand-canonical Monte Carlo simulations indicate that at Na\\(_1\\)Zr\\(_2\\)P\\(_3\\)O\\(_{12}\\), Na\\(^+\\) ions will be almost exclusively located at Na(1), even after including Na\\(^+\\) dynamics at 443 K (**Figure 3a**).\\(^{32}\\) In Na\\(_1\\)Zr\\(_2\\)P\\(_3\\)O\\(_{12}\\), the Na(2) sites are empty because they are not thermodynamically stable at this composition.\\(^{32,41}\\) Thus, the lack of Na atoms present in Na(2) sites that can act as diffusion carriers, contributes significantly to the low D (and \\(\\sigma\\)) observed at low Na content (\\(x \\sim 0\\), **Figure 2**), in addition to the high \\(E_{KRA}\\) observed (i.e., at low values of Na@ Na(2) and Si@ Si/P in **Figure 1e**).\n\nBy contrast, at high Na contents (\\(x \\sim 3\\), Na\\(_4\\)Zr\\(_2\\)Si\\(_3\\)O\\(_{12}\\)), Na\\(^+\\) diffusion is mostly limited by a lack of Na vacancies (either on Na(1) or Na(2) sites), which contributes to\nthe moderately low computed D and \\( \\sigma \\). Note that the computed \\( E_{KRA} \\) barriers achieve their lowest values corresponding to high Na and Si content (**Figure 1e**), which is similar to the local migration units that will be observed at \\( x \\sim 3 \\), and should, in principle, contribute to increase D and \\( \\sigma \\). However, the sharp decrease in the number of available vacancies prevails over the decrease in \\( E_{KRA} \\), eventually lowering D and \\( \\sigma \\). While we only consider vacancy-based migration mechanisms in our work, a recent study has also explored interstitial-based migration mechanisms in various solid electrolytes.\\(^{49}\\) Given the robust agreement between our predictions and measurements, we believe that an interstitial-based mechanism is not active within NASICON structures.\n\n**Figure 3b** further quantifies the extent of diffusion carrier availability within the NASICON structure. For example, the solid blue curve of **Figure 3b** shows the product of the number of Na ions and vacancies in the structure \\([N(\\mathrm{Na}^+) \\times N(\\mathrm{Vacancy})]\\), which is a proxy for the availability of diffusion carriers in the structure, as a function of Na content. **Figure 3b** also splits the concentration of Na ions, \\( N(\\mathrm{Na}^+) \\), into site-specific quantities, \\( N(\\mathrm{Na}(1)) \\) and \\( N(\\mathrm{Na}(2)) \\), as indicated by the dashed blue curves.\n\nIn the blue-shaded region of **Figure 3b** in the range \\( 0 < x < 2 \\), \\( N(\\mathrm{Na}^+) \\times N(\\mathrm{Vacancy}) \\) is extended, signifying high availability of diffusion carriers, but the barriers for Na motion are large as well (bottom half of **Figure 1e**). In striking contrast, for \\( x > 2 \\), \\( N(\\mathrm{Na}^+) \\times N(\\mathrm{Vacancy}) \\) decreases sharply, along with a decrease in \\( E_{KRA} \\) as well (top half of **Figure 1e**), signifying an increase in D and \\( \\sigma \\) up to \\( x \\sim 2.4 \\) followed by an eventual decline of both quantities as \\( x \\to 3 \\). In **Figure 3a**, at \\( x = 3 \\), both Na(1) and Na(2) sites are filled and no free charge carriers are available.\nExperimentally and theoretically,\\(^{17-19,30}\\) at \\(x \\sim 2.4\\) both Na(1) sites and Na(2) sites are expected to be occupied to some degree and the Na\\(^+\\) has enough vacancies to migrate. Furthermore, we expect the overall migration barriers to be low at \\(x \\sim 2.4\\) compared to \\(x < 2\\), as quantified by trends in \\(E_{KRA}\\) in **Figure 1e**. Therefore, **Na\\(_{3.4}Zr_2Si_{2.4}P_{0.6}O_{12}\\)** strikes the optimal combination of density of diffusion carriers (i.e., availability of Na ions and vacancies in both Na(1) and Na(2) sites), and low migration barriers to achieve the fastest Na-transport in the NASICON electrolyte.\n\nWe have synthesized different compositions of the NASICON, namely, **Na\\(_{2.5}Zr_2Si_{1.5}P_{1.5}O_{12}\\)**, **Na\\(_3Zr_2Si_2P_1O_{12}\\)**, and **Na\\(_{3.4}Zr_2Si_{2.4}P_{0.6}O_{12}\\)** and tested their Na-ion transport characteristics. **Figure 4a** shows the powder X-ray diffractions (PXRD) measured at room temperature, with the PXRD profiles matching the rhombohedral (\\(R\\overline{3}c\\)) **Na\\(_{2.5}Zr_2Si_{1.5}P_{1.5}O_{12}\\)**, the monoclinic (\\(C2/c\\)) **Na\\(_3Zr_2Si_2P_1O_{12}\\)**, and \\(C2/c\\) - **Na\\(_{3.4}Zr_2Si_{2.4}P_{0.6}O_{12}\\)** structures, respectively. Information about the synthesis of these NASICON compositions are discussed in the **Methods** section.\nFigure 4 | Room temperature powder X-ray diffraction of selected NASICON compounds and their ionic conductivities measured using the pellets formed by these powders. In panel a, X-Ray diffraction pattern (dark blue, orange, and red circles), and Le Bail fitting (solid lines in cyan, dark brown and dark red) for synthesized Na_{1+x}Zr_2Si_xP_{3-x}O_{12} (x = 1.5, 2.0, and 2.4). b Arrhenius plot from AC impedance measurements of synthesized samples (x = 1.5 in dark blue, x = 2.0 in orange, x = 2.4 in red). c Representative Nyquist plot for Na_3Zr_2Si_2P_1O_{12} at variable measured at 373 (blue), 473 (purple) and 573 K (green). Other Nyquist plots are Figure S9 in the SI.\n\nThe refined lattice parameters of Na_{2.5}Zr_2Si_{1.5}P_{1.5}O_{12}, Na_3Zr_2Si_2P_1O_{12} and Na_{3.4}Zr_2Si_{2.4}P_{0.6}O_{12} are listed in Table 1 and are in agreement with existing reports.\\(^{17,50}\\)\n\nThe phase purity of these compounds enables us to characterize their variable temperature Na ionic conductivities, as reported in the Arrhenius plots of Figure 4b.\nImpedance spectra at variable temperatures and their fitting details are also provided in Figure S9 and related text in the SI.\n\nTable 1 | Lattice parameters of selected NASICON samples obtained from room temperature PXRD. Lattice constants, angles and volumes are in Å, °, and ų, respectively. Z is the number of formula units.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Na2.5Zr2Si1.5P1.5O12Na3Zr2Si2P1O12Na3.4Zr2Si2.4P0.6O12
Space groupR3cC2/cC2/c
a8.9864(13)15.6565(16)15.7571(15)
b8.9864(13)9.0634(7)9.0835(7)
c22.960(5)9.2216(15)9.2549(8)
β–124.255(8)124.963(5)
Volume1605.7(5)1081.6(2)1085.58(16)
Z644
Volume/Z267.6270.4271.40
\n\nThe ionic conductivities of the synthesized Na1+xZr2SixP3-xO12 phases at variable temperature were fitted with appropriate equivalent circuits (see Methods section). The extracted activation energies for all three NASICON compositions were obtained from the Arrhenius plots (ln(σT) vs. 1000/T) of Figure 4b. For the composition x = 1.5, the extracted activation energy is ~ 0.37 eV, and no phase transition is observed due to the stability of the rhombohedral phase at room and higher temperatures. Both compositions at x = 2.0 and x = 2.4 show two linear domains with different activation energies displayed in Figure 4b. Thus, the Arrhenius plots of Figure 4b reproduce the documented monoclinic-to-rhombohedral phase transition upon heating for the compositions Na3Zr2Si2P1O12, and Na3.4Zr2Si2.4P0.6O12 at ~ 433 ± 15 K.\\(^{51-53}\\) Heating and cooling responses of ionic conductivity vs. temperature for the three compositions are discussed in Figure S10 of the SI. The activation energies for x = 2.0 are 0.38 eV (below the phase transition ~ 433 K) and 0.22 eV (above ~ 433 K), which are in good agreement with previous works.\\(^{41,54-60}\\) Na3.4Zr2Si2.4P0.6O12 shows similar activation\nenergies, with values of 0.38 eV (below ~ 433 K) and 0.22 eV (above ~ 433 K) at x = 2.4, in agreement with Ref. 54.\n\nAn example of a Nyquist plot used to extract the total ionic conductivity from the sintered pellets of the NASICON compositions at variable temperatures (373 K, 473 K, and 573 K) is given in Figure 4c. The composition with x = 1.5 has the lowest ionic conductivity for all temperatures compared to structures with x = 2.0 and 2.4. Note, low-temperature impedance measurements of the monoclinic Na_{3.4}Zr_2Si_{2.4}P_{0.6}O_{12} phase do indicate high Na-conductivity.58 The ionic conductivity of x = 2.0 showed that the measured values of this work are within the range of reported values.41,61,43,44,18,45,27\n\nDiscussion\n\nExperimentally, ionic diffusivity can be measured by a number of techniques, such as solid-state nuclear magnetic resonance, quasi elastic neutron scattering and secondary-ion mass spectroscopy,20,62 while AC impedance spectroscopy is the method of choice for determining ionic conductivity in solid electrolytes.63 Indeed, we have used AC impedance spectroscopy in this study. Although classical and ab initio molecular dynamics simulations have proved invaluable in the prediction of ionic conductivities in solid electrolytes,2,3,7,20,22,24,40,46,64–67 we have demonstrated that first-principles-based kMC can access significantly longer time scales in the millisecond range and larger length scales (a total of 21,504 atom supercells in the present work), enabling us to approach experimental time and space resolutions and establish a robust link between measurements and theory. To the best of our knowledge, this is\nthe first study to use a LCE+kMC approach, bearing the accuracy of DFT calculations, to probe the ion-dynamics in solid electrolytes.\n\nOur kMC simulations provide the hopping frequencies of Na\\(^+\\) migration, of different Na concentrations and temperatures, which can be efficiently evaluated and mapped in large supercell models. The hopping frequency is defined in Equation S4 in the SI and includes the attempt frequency and the migration barrier. From our kMC data, we plot heatmaps indicating the spatial migration of Na-ions in Figure 5, along with the frequency associated with each Na migration event. Figure 5 shows the hopping frequency of three representative NASICON compositions, i.e., x = 0.3, 2.4, and 2.97, capturing Na-ion transport in low, intermediate, and high sodium concentrations. Each panel in Figure 5 contains 1,024 migration units (Figure 1e), where each migration unit is represented by a distinct colored hexagonal prism. In Figure 5, the migration units with high hopping frequencies, shown by red prisms, imply that Na-ions have a high probability of migrating beyond the migration unit, thus contributing actively to macroscopic diffusion (the inference is vice versa for blue/purple prisms corresponding to low hopping frequencies). Expectedly, as discussed in Figure 2, x = 2.4 shows significantly higher hopping frequency compared to compositions x = 0.3, and 2.97.\nFigure 5 | Sodium hopping frequencies in NASICON materials. Heatmap representation of the frequency (in Hz) of Na-ion migration from selected kMC simulation supercells (8×8×8 of the primitive cell, including 1,024 migration units) at Na contents of x = 0.3, 2.4 and 2.97. The temperature in all panels is 573 K. Each colored hexagonal prism represents a migration unit, as exemplified in Figure 1d. The hopping frequency of each migration unit is taken by averaging the probability of the six possible migrations of Na+ between the central Na(1) site and the six Na(2) sites in each unit. The top and bottom panels show views along the c-axis from above and below the supercells.\n\nThe direct visualization of the hopping frequency of Na+ migration is insightful for unravelling the respective effects played by PO4 and SiO4 moieties on the overall Na+ transport. In Figure 5, at low Na concentrations, e.g., x = 0.3, most migration units\nappear purple (low frequency) signifying low diffusivity/conductivity, whereas these blue regions turn progressively to yellow and eventually red for increasing values of x. At x ~ 2, most Na-ions are actively engaged in ion transport as most migration units are red (**Figure 5**), highlighting facile ionic transport, consistent with the highest values of observed D and \\( \\sigma \\) at \\( x \\sim 2.4 \\) (**Figure 2**). As x approaches 3 (\\( x \\sim 2.97 \\) shown in **Figure 5**), the color of the migration units eventually become purple, coinciding with the drop in D/\\( \\sigma \\) at high Na-contents (**Figure 2**) due to the low availability of Na-vacancies. This informative analysis can be extended to other topical solid electrolytes with mixed polyanion sulfides, such as, GeS\\(_4\\), PS\\(_4\\), SiS\\(_4\\), etc.\\(^{8,9,12-14}\\)\n\nThe underlying structural models to generate the data in **Figure 5** are based on disordered NASICON structures, where at a given Na concertation the SiO\\(_4\\) and PO\\(_4\\) units are randomly distributed. This is also the case of the most researched sulfide electrolytes for Li-ion solid-state batteries with various degree of mixing of GeS\\(_4\\), SiS\\(_4\\), SiS\\(_4\\) and SnS\\(_4\\) moieties.\\(^{9,11-14}\\) Thus, these NASICON structures truly mimic the experimental synthesis conditions (~ 1200 °C for solid-state synthesis\\(^{18,33}\\)) and/or heat treatments (e.g., low-temperature sol-gel synthesis\\(^{27,68}\\) followed by sintering at ~1200 °C for densification\\(^{18,33,68}\\)), which quench the disorder of the phosphate and silicate units accessed at high temperatures. Previously we have shown that under equilibrium conditions NASICON should phase separate into P-rich and Si-rich domains, particularly across Na concentrations from \\( x = 0 \\) to 2.\\(^{19}\\) It is also important to understand the impact of phase separation (or lack thereof) on Na-diffusivity and conductivity.\n\nWe have extended our kMC model to structures produced in regimes of complete phase separation in **Figure S7** of the SI. Notably, the computed ionic conductivity and other related quantities predicted in regimes of phase separation look\nsimilar to those reported in Figure 2, with the exception of a dip in D and \\( \\sigma \\) around x ~ 1.8 – 2 compared to the scenario of fully disordered system (non-phase separated). However, this dip in ion transport properties approximately accounts for one order of magnitude, well within the error of the available experiments and our calculations, thus making it challenging to detect the signature of phase separation via diffusivity/conductivity measurements or calculations. Our calculations suggest that Na diffusivity and conductivity cannot be used to identify the underlying phases within the NASICON electrolyte. We believe this conclusion may also be valid for other solid electrolytes and electrodes of interest, particularly those adopting the NASICON structure, which can also thermodynamically favor phase separation.\\(^{69,70}\\) Notably, heatmaps produced in structures with phase separation (**Figure S8**) do clearly depict the presence of phase boundaries (differentiating Si-rich and P-rich domains), indicating that robust structural characterizations are still the best way of detecting phase separation.\n\nOur computed barriers and kMC simulations suggest that higher Na\\(^+\\) conductivity in NASICON can simply be achieved by increasing the SiO\\(_4\\) to PO\\(_4\\) ratio. There are two reasons for this: (i) higher Si\\(^{4+}\\) content decreases that of P\\(^{5+}\\) cations in the system, thereby reducing the electrostatic repulsion between the Na\\(^+\\) and P\\(^{5+}\\) cations during Na migration, and (ii) due to the longer Si-O bonds in SiO\\(_4\\) compared to the P-O bonds in PO\\(_4\\), Si-rich migration units will be larger, facilitating migration of large ions, such as Na\\(^+\\). Thus, tuning the Si concentration (or, equivalently, increasing the number of 4+ instead of 5+ cations within the polyanion groups) in the NASICON structure (via aliovalent doping, for example), clearly provides a new way for optimizing ionic transport in this class of ionic conductors.\nIndeed, the last ~40 years of research on NASICON materials has investigated aliovalent doping as a way to improve the Na-ion conductivity of this material. An increase of Na ions is typically achieved by subvalent doping of the Zr^{4+} with trivalent Al^{3+}, Cr^{3+}, Dy^{3+}, Er^{3+}, Fe^{3+}, Gd^{3+}, In^{3+}, Sc^{3+}, Tb^{3+}, Y^{3+} and Yb^{3+}, and/or divalent Co^{2+}, Mg^{2+}, Ni^{2+} and Zn^{2+} species.\\(^{32,26,28,71–73,41}\\) Combining a high Si content in the structure with trivalent doping on Zr^{4+} can potentially improve Na transport at high Na concentrations in NASICONs (x→3). Alternatively, supervalent doping on the Zr^{4+} site with V^{5+}, Bi^{5+}, Sb^{5+}, Nb^{5+} and Ta^{5+} cations is used to increase the number of Na vacancies, and also to reduce (by ~ 30 K) the temperature of the monoclinic-to-rhombohedral phase transition.\\(^{74}\\) Supervalent doping is also a viable strategy for increasing the Si content in the NASICON structure while preserving the stoichiometric ratio of Na-ions and vacancies. Specifically, the ionic radii of Sb^{5+} (~ 0.60 Å), Nb^{5+} (~ 0.64 Å) and Ta^{5+} (~ 0.64 Å) in octahedral environments appear compatible with that of Zr^{4+} (~ 0.72 Å).\\(^{75}\\) The higher stability of the 5+ oxidation state of the three candidates represents the most viable choice for incorporating more Si into the NASICON structure. Furthermore, it has been shown that isovalent doping of Ge^{4+} on Si^{4+} can also increase the size of the migration unit,\\(^{76}\\) potentially facilitating Na-diffusion.\nConclusions\n\nWe have used a combination of state-of-the-art computational tools to explain the influence of polyanion mixing, composition and temperature on ionic transport in Na_{1+x}Zr_2Si_xP_{3-x}O_{12}, as an example ionic conductor. This was achieved by using a combination of density functional theory-based nudged elastic band calculations, a local cluster expansion Hamiltonian, and kinetic Monte Carlo simulations over millisecond timescales and nanometer length scales. Our study has demonstrated that low migration barriers for Na^{+}-ions can be achieved by having local environments that are rich in Si and Na, which can be attributed to the lower electrostatic repulsion between Si^{4+} and Na^{+} (vs. P^{5+} and Na^{+}) during Na migration. A further increase of Si content in Na_{1+x}Zr_2Si_xP_{3-x}O_{12} can be achieved by doping Zr with stable 5+ cations, such as Ta, Nb, Sb, while maintaining an optimal Na composition. Importantly, we discovered a complex interplay between migration barriers and diffusion carrier availability in determining the overall ionic diffusivity/conductivity. For example, at low Na concentrations (0 < x < 2), high migration barriers dominate, resulting in a gradual increase in diffusivity/conductivity with increasing x. At high Na concentrations (x > 2.5), the lack of diffusion carriers dominates (despite low migration barriers), resulting in a drop in diffusivity/conductivity. Thus, we observe that a Na composition of x ~ 2.4 is optimal in terms of combining enough diffusion carriers with low migration barriers, resulting in the highest diffusivity/conductivity. Through synthesis and characterization of the Na_{3.4}Zr_2Si_{2.4}P_{0.6}O_{12}, we have confirmed its high Na-conductivity, as predicted by our simulations. Using Na_{1+x}Zr_2Si_xP_{3-x}O_{12} as a model system, we demonstrated the importance of sampling statistically vast composition, length, and time scales to capture the highly correlated ionic motion that can be observed in mixed polyanion systems. Our findings are significant for the optimization of mixed polyanion solid\nelectrolytes, such as sulfide-based systems which can achieve regimes of super-ionic conductivity.\n\nMethods\nSodium Migration Barriers from Density Functional Theory\n\nNa migration barriers were calculated using the nudged elastic band (NEB) method\\(^{35}\\) through density functional theory (DFT) simulations as implemented in the Vienna ab initio simulation package (VASP).\\(^{77,78}\\) All the calculation parameters used in the DFT simulations can be found in Section S2 of the SI. The NEB barriers were modeled at 3 representative Na concentrations, at x = 0, 2, and 3 as in Na\\(_{1+x}\\)Zr\\(_2\\)Si\\(_x\\)P\\(_{3-x}\\)O\\(_{12}\\). This selection is motivated by our previous knowledge on the compositional phase diagram of Na\\(_{1+x}\\)Zr\\(_2\\)Si\\(_x\\)P\\(_{3-x}\\)O\\(_{12}\\),\\(^{19}\\) where NASICON exhibits three distinct ground states at 0 K.\n\nSpecial care is required for the NEB barrier calculations of NaZr\\(_2\\)(PO\\(_4\\))\\(_3\\) (x = 0) which follows a pathway Na(1)\\(\\rightarrow\\)Na(2)\\(\\rightarrow\\)Na(1). In NaZr\\(_2\\)(PO\\(_4\\))\\(_3\\) all the Na(1) sites are occupied and Na migration is only possible if vacancies in Na(1) are introduced. For this specific case the energy required for Na\\(^+\\) migration should also include the formation energy of Na vacancy, which we computed using the method of Ref.\\(^{79}\\). We found that the Na vacancy formation energy in NaZr\\(_2\\)(PO\\(_4\\))\\(_3\\) is \\(\\sim 474\\) meV, which we added in our model (see SI). Whereas the Na vacancy formation energy at x = 2 and 3 is negligible (\\(\\sim 13\\) meV). Note that at x = 2, Na(1) and Na(2) are only partially occupied which guarantees facile Na transport.\n\nTo remove the directional dependence of migration barriers, we define the kinetically resolved activation (KRA) barrier, \\(E_{KRA}\\) of Equation 2,\n\\[\nE_{KRA} = E_{\\text{barrier}}[\\text{Na}(1) \\leftrightarrow \\text{Na}(2)] - \\frac{1}{2}(\\Delta E_{\\text{end}})\n\\] (2)\n\nwhere the \\( E_{\\text{barrier}}[\\text{Na}(1) \\leftrightarrow \\text{Na}(2)] \\) is the NEB barrier,\\(^{39,40}\\) and \\( \\Delta E_{\\text{end}} \\) is the absolute difference between the computed energies of the initial and final end point structures. The distribution of \\( E_{KRA} \\) at different configurations of Na and Si/P environments is shown in **Figure S1**, **S2**, **S3**, and **Table S1** of the SI.\n\n**Local Cluster Expansion Hamiltonian**\n\nThe calculated \\( E_{KRA} \\) are fitted to a local cluster expansion (LCE) Hamiltonian built around a migration unit (see **Figure 1d**) centered on the Na(1) site and using a cut-off radius of 5 Å. Details of the LCE model and the fitting strategy are given in the SI. The fitted Hamiltonian can be used efficiently to compute migration barriers inside the migration unit at any given Na/vacancy and Si/P content/configuration. The LCE Hamiltonian includes 1 point, 5 pair, and 1 triplet terms (see **Table S3** and **Table S4**), respectively. The LCE Hamiltonian can reproduce the migration barriers with a RMS error of \\( \\sim \\pm 38 \\) meV. The robustness of the LCE Hamiltonian was cross-validated using the leave-one out method. Notably, a variability of \\( \\sim \\pm 38 \\) meV corresponds to a less than an order of magnitude in diffusivity (\\( \\pm 60 \\) meV),\\(^{80}\\) which is the typical uncertainty of experimental measurements and theoretical calculations for electrode materials.\\(^{40}\\)\n\n**Kinetic Monte Carlo Simulations**\n\nWe implemented a rejection-free kinetic Monte Carlo (kMC) simulation scheme in an in-house-code, as described in Refs.\\(^{39,40}\\). The initial configurations for the kMC were\ngenerated using the canonical Monte Carlo simulation (based on our previous work where we constructed a global cluster expansion model on the NASICON)19 in an 8×8×8 supercell at 0 ≤ x ≤ 3 containing 4,096 distinct Na sites and 3,072 Si/P sites. These structures were generated at 1500 K, and close to the experimental synthesis temperature.17,34,28,41 For each of the 11 compositions sampled (x = 0.03, 0.3, 0.6, 0.9, 1.2, 1.5, 1.8, 2.1, 2.4, 2.7, 2.97), 50 structural models were generated using the canonical Monte Carlo approach.19\n\nWe used kMC to evaluate the transport properties of NASICON crystals, including Na+ diffusivity, bulk conductivity, Haven's ratio, and correlation factor. These physical quantities are averaged for each of the 50 initial configurations per Na composition. During the kMC simulation, only Na ions can hop while the remaining atoms are frozen. Each kMC simulation included 2,048,000 equilibration steps, followed by 12,288,000 sampling steps for statistical analysis at 373, 473 and 573 K, respectively. In total, we have run 1650 independent kMC simulations (11 compositions×50 initial configurations ×3 temperatures) with a total of ~14 million steps per configuration, which totals to approximately 23 billion kMC steps. For investigating the impact of phase separation on ionic transport, we followed the same procedure as above, except the canonical Monte Carlo, equilibrated structures were generated at 573 K, instead of at 1500 K.\n\nSynthesis and X-ray Characterization of Na1+xZr2SiₓP3−ₓO₁₂ Compositions\n\nSynthesis of Na1+xZr2SiₓP3−ₓO₁₂ for x = 1.5 and x = 2.0 were carried out using a sol-gel method with NaNO₃, NH₄H₂PO₄, ZrO(NO₃)₂.xH₂O, Si(OC₂H₅)₄ (Tetraethyl orthosilicate/TEOS) and citric acid as precursors followed by carefully optimized\nthermal treatments. Citric acid was first mixed with 300 mL of ethanol:deionized water (1:1), at 343 K for 1 hour. Then a stoichiometric amount of the precursors was introduced to the solution and the temperature was raised to 363 K for 1.5 hours. The resulting gel was then dried for 8 hours, at 453 K. A first calcination was carried out at 873 K for 8 hours, followed by second calcination at 1373 K for 18 hours. For the composition \\( x = 2.4 \\), a solvent-assisted solid-state reaction method was applied.\\(^{54}\\) Corresponding amounts of NaNO\\(_3\\), and ZrO(NO\\(_3\\))\\(_2\\) were dissolved into deionized water. A stoichiometric amount of Si(OC\\(_2\\)H\\(_5\\))\\(_4\\) was also added to the solution while stirring. When Si(OC\\(_2\\)H\\(_5\\))\\(_4\\) was hydrolyzed, the corresponding amount of NH\\(_4\\)H\\(_2\\)PO\\(_4\\) was added to the system while stirring. The homogeneous aqueous system then changed to a mixture of a colloidal sol and precipitates of complex zirconium oxyphosphate compounds. The whole mixture was dried at \\( \\sim 85 \\ ^\\circ \\mathrm{C} \\). The dried powder was calcined at \\( \\sim 800 \\ ^\\circ \\mathrm{C} \\) for 3 hours. After calcination, a white powder was obtained. The calcined powder was then milled in ethanol with zirconia balls on a milling bench for 48 hours and dried at \\( \\sim 70 \\ ^\\circ \\mathrm{C} \\) for 12 hours. The as-prepared powder (which was just calcinated at 1073 K) was then sintered at \\( \\sim 1373 \\ \\mathrm{K} \\) for 18 hours to crystallize the phase.\n\nX-Ray diffraction patterns of the obtained white powders were then measured at room temperature using a Bruker D8 diffractometer with copper source, (\\( K_{\\alpha 1} = 1.54056 \\ \\text{\\AA} \\) and \\( K_{\\alpha 2} = 1.54439 \\ \\text{\\AA} \\)), and a step size of 0.021°. Profile matchings were done using WinPLOTR and FullProf software.\\(^{41}\\) For \\( x = 1.5 \\) the pattern was fitted using the \\( R3c \\) space group,\\(^{18,76,81,82}\\) while \\( x = 2.0 \\) and \\( x = 2.4 \\) were fitted using the \\( C2/c \\) space group.\\(^{41,83}\\)\nFor the preparation of impedance measurements, the three samples were cold pressed into 6 mm pellets and sintered at ~ 1373 K for 12 hours. The sintered pellets were then gold-sputtered (~ 75 nm), and carbon paper (papyex) was added on each side of the pellet to ensure good contacts for the impedance measurements in the high temperature impedance cell BioLogic HTSH-100. The latter was inserted in high temperature furnace BioLogic HTF-1100 and connected to impedance analyzer BioLogic MTZ-35 with a two-point connection. The frequency range used was from 0.1 Hz to 30 MHz, with an amplitude of 0.02 V. Measurements were recorded every 50 K from 323 K to 623 K (15 minutes soaking each time), and then cooled down every 50 K from 623 K to 323 K.\n\nThe fitting of Nyquist plot was carried out using ZView software. For x = 1.5, the equivalent circuit used was based on semicircle phenomena as seen in other reports,\\(^{28,59,84-86}\\) with R1 representing the contact resistance, parallel of CPE1 and R2 representing the semi-circle, and initially a CPE2 for the diffusion tail. Since CPE2 has an n-value close to 0.5, a Warburg element is used to better fit the diffusion tail. Applying the same equivalent circuit for other samples (x = 2.0 and x = 2.4) was not satisfactory, thus a one-phenomena Debye Model for solid electrolyte between two ionically blocking electrodes is used instead.\\(^{87}\\) Schematics of the equivalent circuits are shown in Figure S9 of SI.\n\nAcknowledgments\nP.C., C.M., A.K.C., E.M., V.S., and J.-N. C. are grateful to the ANR-NRF for the funding of the NRF2019-NRF-ANR073 Na-MASTER project. P.C. and Z.D. acknowledge funding from the National Research Foundation under NRF Fellowship NRFF12-2020-\n0012. T. P. M. was supported by the National Research Foundation (NRF) Singapore through Singapore MIT Alliance for Research and Technology (SMART)'s Low Energy Electronic Systems (LEES) IRG. The computational work was performed on resources of the National Supercomputing Centre, Singapore (https://www.nscc.sg). We thank Dr. Theodosios Famprikis at TUDelft for fruitful discussion.\n\nAuthors Contributions\nP.C. designed and supervised the project. Z.D., T.P.M., and P.C. performed the NEB simulations and fitted the local cluster expansion Hamiltonian with discussions with G.S.G. Z.D. developed all the tools for constructing models, Hamiltonian fitting, kinetic Monte Carlo and data analysis. Q.M. and E.M. carried out the synthesis of the NASICON phases, E.M. performed the PXRD, and the impedance measurements. E.M. performed the data analysis of the experimental data under the supervision of J.-N. C., V.S. and C. M. Z.D., T.P.M. and P.C. wrote the first draft. Z.D., P.C., G.S.G. and A.K.C. contributed to the initial data analysis of the computed data. All the authors contributed to the discussion and final version of this manuscript.\n\nConflicts of Interests\nThere are no conflicts to declare.\n\nSupplementary information\nThe supplementary Information contains details of the density functional theory simulations, nudged elastic band results, kinetic Monte Carlo simulations, AC impedance measurements, equivalent circuits for the analysis of the AC-impedance\ndata, and the Arrhenius plot of conductivities vs 1/temperatures of selected NASICON compositions.\n\nCode and Data Availability\n\nAll the computational data associated with this study are freely available at the Git repository https://github.com/caneparesearch/NASICON_KMC_paper_data\n\nReferences\n\n1. Goodenough, J. B. & Park, K.-S. The Li-Ion Rechargeable Battery: A Perspective. J. Am. Chem. Soc. **135**, 1167–1176 (2013).\n2. Wang, Y. *et al.* Design principles for solid-state lithium superionic conductors. *Nat. Mater.* **14**, 1026–1031 (2015).\n3. 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Click to download.\n\n• nasiconkmcSlforsubmission.pdf"} {"paper_id": "prb35", "title": "A Variational Expectation-Maximization Framework for Balanced Multi-scale Learning of Protein and Drug Interactions", "text": "A Variational Expectation-Maximization Framework for Balanced Multi-scale Learning of Protein and Drug Interactions\n\nYuedong Yang\nyangyd25@mail.sysu.edu.cn\n\nSun Yat-sen University https://orcid.org/0000-0002-6782-2813\nJiahua Rao\nSun Yat-sen University https://orcid.org/0000-0002-6840-8198\nJiancong Xie\nSun Yat-sen University\nQianmu Yuan\nSun Yat-sen University https://orcid.org/0000-0001-6098-9103\nDeqin Liu\nSun Yat-sen University\nZhen Wang\nSun Yat-sen University\nYutong Lu\nSun Yat-sen University\nShuangjia Zheng\nShanghai Jiao Tong University https://orcid.org/0000-0001-9747-4285\n\nArticle\n\nKeywords: Multi-scale Learning, Expectation-Maximization, Protein-Protein Interactions, Drug-Protein Interactions, Protein Interface Prediction\n\nPosted Date: March 20th, 2024\n\nDOI: https://doi.org/10.21203/rs.3.rs-3620776/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: There is NO Competing Interest.\nVersion of Record: A version of this preprint was published at Nature Communications on May 25th, 2024. See the published version at https://doi.org/10.1038/s41467-024-48801-4.\nA Variational Expectation-Maximization Framework for Balanced Multi-scale Learning of Protein and Drug Interactions\n\nJiahua Rao$^{1}$, Jiancong Xie$^{1}$, Qianmu Yuan$^{1}$, Deqin Liu$^{1}$, Zhen Wang$^{1}$, Yutong Lu$^{1*}$, Shuangjia Zheng$^{2*}$ and Yuedong Yang$^{1,3,4*}$\n\n$^{1}$School of Computer Science and Engineering, Sun Yat-sen University, Guangzhou, China.\n$^{2}$Shanghai Jiao Tong University, Shanghai, China.\n$^{3}$Key Laboratory of Machine Intelligence and Advanced Computing, Sun Yat-sen University, Guangzhou, China.\n$^{4}$State Key Laboratory of Oncology in South China, Sun Yat-sen University, Guangzhou, China.\n\n*Corresponding author(s). E-mail(s):\nshuangjia.zheng@sjtu.edu.cn; yangvd25@mail.sysu.edu.cn;\nContributing authors: raojh6@mail2.sysu.edu.cn;\n\nAbstract\nProtein functions are characterized by interactions with proteins, drugs, and other biomolecules. Understanding these interactions is essential for deciphering the molecular mechanisms underlying biological processes and developing new therapeutic strategies. Current computational methods mostly predict interactions based on either molecular network or structural information, without integrating them within a unified multi-scale framework. While a few multi-view learning methods are devoted to fusing the multi-scale information, these methods tend to rely intensively on a single scale and under-fitting the others, likely attributed to the imbalanced nature and inherent greediness of multi-scale learning. To alleviate the optimization imbalance, we present MUSE, a multi-scale representation learning framework based on a variant expectation maximization to optimize different scales in an alternating procedure over multiple iterations. This strategy efficiently\nfuses multi-scale information between atomic structure and molecular network scale through mutual supervision and iterative optimization. MUSE outperforms the current state-of-the-art models not only in molecular interaction (protein-protein, drug-protein, and drug-drug) tasks but also in protein interface prediction at the atomic structure scale. More importantly, the multi-scale learning framework shows potential for extension to other scales of computational drug discovery.\n\nKeywords: Multi-scale Learning, Expectation-Maximization, Protein-Protein Interactions, Drug-Protein Interactions, Protein Interface Prediction\n\n1 Introduction\n\nInteractions between proteins, drugs, and other biomolecules play a crucial role in various biological processes [1–3]. Understanding these interactions is essential for deciphering the molecular mechanisms underlying biological processes and developing new therapeutic strategies [4]. However, the massive growth in demand and cost associated with experimental interactions calls for computational tools for automated prediction and understanding of interactions between biomolecules [5].\n\nMany computational methods have been developed for studying the interactions between biomolecules [6–9]. Predicting these interactions purely from structures is one of the most important challenges in structural biology [10, 11]. The structural-based methods aim to promote our understanding of the patterns of interactions among residues/atoms at the atomic structural scale (intra-molecular scale). Unfortunately, these methods often lead to inferior performance when high-quality molecular structural features are not available [9]. On the other hand, network-based methods analyzed the topology of the molecular networks to infer potential new interactions [12, 13]. Similarly, these methods don’t perform well due to ignorance of protein structures. Thus, accurate predictions need to capture multi-scale hierarchical and complementary information.\n\nTo model the joint distribution over the multi-scale of protein and drug interactions, a few attempts have been developed [14, 15]. An intuitive approach for learning multi-scale representations is to combine the molecular graph with an interaction network and optimize them jointly. For example, HIGH-PPI [15] is the first to jointly optimize a hierarchical graph including the PPI network (outside-of-protein view) and the protein graph (inside-of-protein view) for protein-protein interactions. MIRACLE [14] proposed a contrastive learning strategy to integrate the multi-view information of drug-drug interactions. ScanNet [16] also integrates information from multiple scales (atom, amino acid) to improve the prediction of protein-protein binding sites. However, due to the imbalanced nature and inherent greediness of multi-scale learning [17–19], these models often intensively rely on a single scale and\nunder-fitting the others. This imbalanced nature prevents these approaches from effectively leveraging all informative scale-related information and often results in worse generalization. Furthermore, an effective multi-scale framework needs not only capture the rich information within different scales but also faithfully preserve the underlying relation in between.\n\nIn this study, we present MUSE, a multi-scale representation learning framework based on a variant expectation maximization [20]. In contrast to existing methods that rely intensively on single-scale information, MUSE efficiently incorporates multi-scale information through a variant expectation maximization framework. The framework effectively addresses the optimization imbalance in multi-scale learning through mutual supervision and iterative optimization. The method was shown effective not only for predicting molecular interactions (including protein-protein, drug-protein, and drug-drug interactions) but also for predicting molecular binding interfaces. Such a multi-scale framework has the potential for applications with more scales including atom and amino acid scale.\n\n2 Results\n\n2.1 MUSE: A balanced expectation-maximization learning framework to learn protein and drug multi-scale information.\n\nAs shown in Fig. 1, MUSE is a multi-scale learning method that integrates both molecular structure modeling and interaction network learning of proteins through a variational expectation-maximization (EM) framework. The EM framework optimizes two modules, the expectation step (E-step) and the maximization step (M-step), in an alternating procedure over multiple iterations [18, 21]. During the E-step, MUSE utilizes the structural information of each biomolecule to learn an effective structural representation for training with known interactions and augmented samples in the M-step. It takes the pair of protein and drug with their atom-level structural information as input and augments with the predicted interactions from the M-step. The M-step takes the molecule-level interaction network and the structural embeddings and predicted interactions from the E-step as the input and also outputs the predicted interactions. This iterative optimization between the E-step and the M-step ensures the capturing of both the molecular structures and network information interactively, with different learning rates at two scales. The mutual supervision ensures that each scale model learns in an appropriate manner, enabling the utilization of effective information at different scales. This framework will be demonstrated on several multi-scale tasks for interactions between proteins and drugs. We additionally analyzed that MUSE mitigates the imbalanced characteristics in multi-scale learning and effectively integrates the hierarchical and complementary information from different scales.\n2.2 Leveraging atomic structure information for improving predictions at the molecular network scale.\n\nTo evaluate our method, we first utilized MUSE to integrate atomic structural information to improve molecular network scale predictions. As shown in Fig. 2a, MUSE achieved state-of-the-art performance consistently on the three multi-scale interaction predictions tasks, including protein-protein interactions (PPI) [15, 22], drug-protein interactions (DPI) [11, 23], and drug-drug interactions (DDI) [14, 24].\n\nSpecifically, on the PPI dataset, MUSE outperformed all existing models including single-scale (DrugVQA [8] and TAG-PPI [25]), and multi-view methods (GNN-PPI [22] and HIGH-PPI [15]). TAG-PPI and DrugVQA, which solely focus on the atomic structure scale, achieved the poorest performance as they neglected the molecular network scale information. Our model showed substantial improvements over the strongest baseline HIGH-PPI, which also incorporates multi-scale information for enhanced predictions, with an increase of 8.41% in the BFS split, 13.04% in the DFS split, 7.69% in the Random split, (Fig. 2c and Fig. S1). Furthermore, our model also showed improvements over the ablation study MUSE-Joint, which integrates two scale models and optimizes them jointly with multiple iterations, attributed to the efficient utilization of the EM framework. The MUSE-Joint is also slightly better than HIGH-PPI, as HIGH-PPI does not optimize the structural information jointly for predictions.\n\nSimilar results have been shown on the DPI and DDI datasets. MUSE achieved the AUPRC of 0.998 and 0.922 and the AUROC of 0.993 and 0.915 respectively on the DDI and DPI datasets (Supplementary Table S2-S3). When compared with state-of-the-art methods, MUSE showed improvements of 5.05% on the DDI dataset (over CGIB [26]) and 2.67% on the DPI dataset (over ConPlex [11]). Interestingly, the baseline method (MIRACLE[14]), which directly combines information from different scales in GNN, underperforms the recent structure-based baseline method CGIB on most metrics. These results indicated the importance of the multi-scale integration strategy, and a sub-optimal strategy might even lead to worse performance than single-scale models.\n\n2.3 Improving predictions at the atomic structure scale from the molecular network scale.\n\nIn addition to leveraging atomic structural information to improve molecular network scale prediction, we further investigated the ability of MUSE on the learning and prediction of structural properties at the atomic structural scale, including the prediction of interface contacts [28–30] and binding sites [16, 31, 32] related to protein-protein interactions (PPI).\n\nTo evaluate the prediction of protein inter-chain contact, MUSE was compared with the state-of-the-art methods on the DIPS-Plus benchmark [33]. As\nshown in Fig. 3a, MUSE consistently outperformed all other methods [30, 34–36], validating its effectiveness and adaptability in the atomic structural predictions. To be specific, our model achieved the AUROC of 0.92 and the highest precision of 0.26, 0.25, and 0.23 for P@10, P@L/10, and P@L/5, respectively, significantly outperforming the best method, DeepInteract, with AUROC of 0.90 and precision values of 0.20, 0.19, and 0.17. This improvement could likely be attributed to the EM training paradigm in MUSE, which is capable of learning geometric representations (E-step) and interaction patterns (M-step) of proteins in an iterative optimization process. We also highlighted the capabilities of MUSE by examining three examples from the testing set. As shown in Fig. 3b (and Supplementary Fig. S2), MUSE accurately predicted contact interfaces with an average precision of 0.711, which is significantly better than DeepInteract’s 0.592 and GLINTER’s 0.019. Furthermore, the predicted contact map of MUSE leads to better docking results upon integration of the Kabsch algorithm (RMSD: 4.33). In contrast, alternative methods struggle to generate accurate binding structures, resulting in a relatively high RMSD (DeepInteract: 8.15 and GLINTER: 19.90).\n\nMUSE was further evaluated for predicting whether the residues are directly involved in protein-protein interactions [16, 32]. As shown in Fig. 3c and Supplementary Table S3, on the ScanNet [16] benchmark, MUSE achieved a Median AUPRC of 0.811 and a Median AUROC of 0.938 for the full test set, 1.76% and 0.969% better than the second best method PeSTo [32]. The improvements demonstrate that the learning of molecular network scale in MUSE could provide valuable insights into the predictions at the atomic structural scale. MUSE also performed best on another benchmark dataset developed by Masif-site [10], 2.23% and 1.40% better than PeSTo and MUSE-Joint respectively. These improvements are in line with our expectation as the effective integration of multiple scales (atom, amino acid, molecule) could efficiently detect protein–protein binding sites. Visualizations of MUSE predictions for representative examples (Supplementary Fig. S3) illustrate that the binding sites are correctly identified (0.978 and 0.977 accuracy).\n\n2.4 Mitigating the imbalanced characteristics of multi-scale learning through iterative optimization.\n\nTo investigate why MUSE achieved the superior performance of multi-scale representations, we analyzed the learning ability of MUSE for the imbalanced characteristics of multi-scale learning. We hypothesized that the slow-learning scale’s updating direction is severely disturbed by the dominant one, making it hard to exploit its features for accurate predictions [17, 37].\n\nTo indicate the information utilization at different scales, we defined the information utilization rate as the proportion of accuracy changes achieved by single-scale models relative to the final multi-scale model, similar to previous studies [17, 37]. As shown in Fig. 4a, for HIGH-PPI, the utilization rate is 0.009 for the atomic structure scale and 0.191 for the molecular network scale, leading to a ratio of 21.22. These indicated that HIGH-PPI was dominated\nby the molecular network scale. Similarly, MIRACLE and other methods were also harmed by molecular network scale information. In contrast, the utilization rates of MUSE for the atomic structure and molecular network scales rose to 0.103 and 0.318, with a ratio of 3.08. These results indicated that MUSE efficiently alleviates the inhibition on the molecular network scale and fully exploits the structural properties in multi-scale learning. The different contributions of different scales to the learning objective are due to the natural imbalance that exists in the current dataset.\n\nTo explore the contribution of iterative optimization, we could see that MUSE did not perform as well as other baseline methods in the beginning but outperformed them after iterations (Fig. 4b). The continuous increase in accuracy (red curve) shows how MUSE continuously alleviates the imbalance characteristics of multi-scale learning and improves its multi-scale utilization. The learned representations by MUSE classify the interaction type between protein and protein while both the molecular network model (Fig. 4c) and MUSE without iterative optimization (MUSE-Joint) have a small number of samples mixed. Specifically, case (#1) demonstrates that MUSE-Joint inhibits the utilization of structural information for predictions, while MUSE alleviates this inhibition and fully utilizes these structural features. On the other hand, case (#2) illustrated that MUSE-Joint is disturbed by the other scale during training, whereas MUSE does not encounter this issue.\n\nIn summary, MUSE effectively mitigates the imbalance characteristics and greedy learning in multi-scale learning, ensuring the comprehensive utilization of information at different scales during training. Furthermore, the experiment of utilization rate analysis enables us to have a concrete look at what the model has learned and demonstrate that using MUSE to balance the models’ learning from different scales enhances generalization.\n\n2.5 Visualization and interpretation of the learned multi-scale representations.\n\nTo better understand the learned multi-scale representations, we investigated the learned multi-scale representation by MUSE from different perspectives, including (1) the capability of MUSE to capture the atomic structure information (i.e. structural motifs and embeddings) involved in PPI, and (2) the mutual supervision between the learned atomic structure and molecular network representations.\n\nAs an example of binding site prediction (PDB id: 3CQQ-A), MUSE can accurately identify the residues belonging to the binding sites (Fig. 5a) (97.7% accuracy). This demonstrated that the mutual supervision in MUSE helps the atomic structure scale model to learn key substructures related to interactions. The learned atomic structural representations (Fig. 5b) confirmed that our learned representation aids in discriminating the interaction types while HIGH-PPI showed a distribution close to the random. This agreed that HIGH-PPI didn’t well utilize the structural information with a low atomic structure information utilization rate (0.009).\nTo illustrate the role of mutual supervision, we conducted an ablation study to investigate the effect of the pseudo-labels predicted by the atomic structure scale on the molecular network scale. We computed the best-F1 scores at different thresholds for pseudo-labeling on the PPI dataset (box plots, Fig. 5c). Without implementing mutual supervision (\\( t = 0 \\)), the model achieved a best-F1 of 0.908, only marginally outperforming the baseline method (0.886, HIGH-PPI). As the threshold value of \\( t \\) increases, the Best-F1 score of MUSE improves rapidly. This improvement is attributed to the addition of more pseudo interactions to the PPI network, mitigating the incompleteness of the network [38]. Subsequently, the performance gradually decreases as the threshold \\( t \\) increases, indicating that the predicted pseudo interactions become increasingly noisy when \\( t > 0.4 \\).\n\n3 Discussion\n\nMUSE unifies two scales of biomolecules, **atomic structure scale and molecular network scale**, into a multi-scale framework. The iterative optimization and mutual supervision process partially overcome the greedy nature of multi-scale learning, and thus significantly improve the multi-scale representation learning. These advantages uniquely empower MUSE for the multi-scale learning of proteins and drugs that could be extended to other multi-scale tasks.\n\nWith the continuously growing of multi-scale data, the integration of data across different scales is becoming increasingly critical. Unfortunately, achieving this integration is challenging, as the straightforward approaches are often dominated by individual scale due to the **imbalanced nature** for different scales and the inherent greediness of deep neural networks. Our approach offers a novel perspective for integrating multiple scales of data. We show the efficacy of MUSE across various interaction prediction tasks, highlighting the superiority of integrating atomic structure scale information into molecular interaction predictions. Furthermore, the molecular network scale learning within MUSE offers valuable insights for further optimizing the atomic structure scale model to enhance protein representations, as indicated by the improvements in the atomic structure scale tasks.\n\nWhile MUSE has demonstrated state-of-the-art performance in our benchmarks, there remains potential for enhancing its ability to handle noisy and incomplete multi-scale downstream tasks. This might be combined to incorporate prior knowledge through a knowledge graph and explainable AI techniques. On the other hand, our conceptual multi-scale framework also exhibits potential for extension to other scales of computational drug discovery. For example, MUSE could be applied to the atom and amino acid scale in protein representation learning, deepening our understanding of the multiple structural scales of protein. We hope that its broad applicability and scalability to other scales will contribute to the drug discovery of effective therapeutics.\n4 Methods\n\n4.1 Datasets with Multi-Scale Learning\n\nWe have evaluated our framework on three multi-scale interaction prediction benchmarks, the protein inter-chain benchmark (DIPS-Plus) and the protein binding sites benchmark (Scannet). The statistics of these datasets are presented in Supplementary Information B.\n\nFirstly, we evaluated our framework on three multi-scale interaction prediction benchmarks, i.e., protein-protein interaction predictions (SHS27K), drug-protein interaction predictions (BioSNAP), and drug-drug interaction predictions (DeepDDI). The SHS27K PPI dataset contains SHS27k (subdataset of STRING [39]) with 6660 protein-protein pairs (PPIs) and 1533 human proteins with native protein structures. These PPIs are divided into 7 types, namely reaction, binding, post-translational modifications (ptmod) activation, inhibition, catalysis, and expression, which contain 15,056 positive interaction types and 31,564 negative interaction types. The native protein structures are obtained from PDB (https://www.rcsb.org/), in line with previous works [15]. The BioSNAP dataset, obtained from [23], consists of only positive drug-target interactions. The negative drug-protein interactions were generated by randomly selecting an equal number of protein–drug pairs [14, 26]. We ensure that our data splits and sampling methods align with those used in previous work [11]. Herein, we used the molecular 2D graph for drugs and the protein structures are obtained from the pre-trained language model ESMFold [40]. For the DeepDDI dataset, we used 192,284 pairwise drug-drug interactions and their polypharmacy side-effect information extracted from DrugBank [41].\n\nWhen predicting the protein interface contacts at the structural scale, we chose to use DIPS-Plus [33], a large protein complex structures dataset mined from the Protein Data Bank and tailored for rigid body docking. Following Morehead et al [30], we select 32 homodimers and heterodimers to evaluate the performance of our model in predicting interface contacts. After removing proteins with \\( \\geq 30\\% \\) sequence identity with the test datasets, 15,618 and 3,548 binary complexes are left for training and validation.\n\nFor the prediction of protein–protein binding sites (PPBS), we obtained 41,466 distinct PDB files, involved in 240,506 protein–protein interfaces from the Dockground database [42]. Following Tubiana et al. [16], we investigated the impact of homology between train and test set examples on generalization of our framework and baseline models and therefore grouped validation and test examples into four subgroups based on their degrees of homology: (1) Val/Test 70% (at least 70% sequence identity with at least one train set example), (2) Val/Test homology (at most 70% sequence identity with any train set example), (3) Val/Test topology (at least one train set example with similar protein topology), and (4) Val/Test none (none of the above). The additional independent testing set is composed of clusters containing any of the 53 subunits from the MaSIF-site benchmark dataset.\n4.2 Notations and Problem Formulation\n\nSuppose that we have a multi-scale network \\( \\mathcal{N} \\) which is presented by \\( \\mathcal{N} = \\{\\mathcal{G}, \\mathcal{L}\\} \\) where \\( \\mathcal{G} := \\{G_i\\}_{i=1}^N \\) is the set of the biomolecular graph \\( G \\) and \\( \\mathcal{L} := \\{L_{i,j}\\}_{(i,j)}^M \\) is the set of the known interaction link \\( L \\) between biomolecules. For each node \\( G \\) in \\( \\mathcal{N} \\), we denote the biomolecular structural graph \\( G = \\{\\mathcal{V}, \\mathcal{E}\\} \\), where \\( \\mathcal{V} \\) is the set of atoms \\( v \\in \\mathcal{V} \\) and \\( \\mathcal{E} \\) is the set of edges/bonds \\( e \\in \\mathcal{E} \\), so the known interaction links between biomolecules also can be denoted as the pairs of molecular atomic structural graphs: \\( \\mathcal{D} := \\{(G_i, G_j)\\}_{(i,j)}^M \\). Herein, we study the problem of link prediction on \\( \\mathcal{N} \\), for predicting the labels \\( y_{\\mathcal{L}_U} \\) of the unobserved (test-set) interactions \\( \\mathcal{L}_U \\) with a few observed labels \\( y_{\\mathcal{L}_V} \\), \\( \\mathcal{L} = \\mathcal{L}_V \\cup \\mathcal{L}_U \\). We also defined the adjacency matrix in the network \\( \\mathcal{N} \\) as \\( A \\in \\mathbb{R}^{(N \\times N)} \\) where \\( A_{i,j} = 1 \\) if \\( (i, j) \\in \\mathcal{L}_V \\) and \\( A_{i,j} = 0 \\) otherwise.\n\n4.3 Variational Expectation-Maximization (EM) Framework\n\nAt the core of our method is combining the atomic structure scale and molecular network scale models for link prediction learning on multi-scale networks with a variational EM framework. Given the observed variables \\( y_{\\mathcal{L}_V} \\), unobserved variables \\( y_{\\mathcal{L}_U} \\), and model parameters \\( \\theta, \\phi \\), our framework tries to maximize the log-likelihood function of the observed interaction labels, i.e. \\( \\log p_\\theta(y_{\\mathcal{L}_V}|\\mathcal{G}, A) \\). It is computationally intractable to compute this log-likelihood as it requires integration over all combinations of object labels, i.e. \\( \\log \\prod_{l \\in \\mathcal{L}_V} p_\\theta(y_l|\\mathcal{G}, A) \\). Thus we instead optimize the evidence lower bound (ELBO) of the log-likelihood function:\n\n\\[\n\\mathcal{O}(\\theta) = \\log p_\\theta(y_{\\mathcal{L}_V}|\\mathcal{G}, A) \\geq \\mathbb{E}_{q_\\phi(y_{\\mathcal{L}_U}|\\mathcal{G}, A)}[\\log p_\\theta(y_{\\mathcal{L}_V}, y_{\\mathcal{L}_U}|\\mathcal{G}, A)] - \\log q_\\phi(y_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D}),\n\\]\n\nwhere \\( q_\\phi(y_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D}) \\) can by any variation distributions over \\( y_{\\mathcal{L}_U} \\), and the equation holds when \\( q_\\phi(y_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D}) = p_\\theta(y_{\\mathcal{L}_U}|y_{\\mathcal{L}_V}, \\mathcal{G}, A) \\). The ELBO is also challenging to directly derive the maximum likelihood estimator via the EM algorithm. Therefore, we use a variational approximation of the EM algorithm to optimize the lower bound by iteratively alternating between optimizing the distribution \\( q \\) (i.e., E-step) and the distribution \\( p \\) (i.e., M-step).\n\nIn the variational E-step, the goal is to fix \\( p_\\theta \\) and update \\( q_\\phi \\) to minimize the KL divergence between \\( q_\\phi(y_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D}) \\) and \\( p_\\theta(y_{\\mathcal{L}_U}|y_{\\mathcal{L}_V}, \\mathcal{G}, A) \\).\n\nIn the M-step, we aim to update \\( p_\\theta \\) to maximize the below likelihood function:\n\n\\[\n\\mathcal{O}(\\theta) = \\mathbb{E}_{q_\\phi(y_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D})}[p_\\theta(y_{\\mathcal{L}_V}, y_{\\mathcal{L}_U}|\\mathcal{G}, A)]\n\\]\n\nTo prevent a computational complexity of \\( p_\\theta \\) in the EM algorithm, we utilized the following pseudo-likelihood function:\n\\[\n\\mathcal{O}_{PL}(\\theta) \\triangleq \\mathbb{E}_{q_{\\phi}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D})}[\\sum_{L_{ij} \\in \\mathcal{L}_V} \\log p_{\\theta}(\\mathbf{y}_{L_{ij}}|\\mathcal{G}, A, \\mathbf{y}_{\\mathcal{L}\\setminus L_{ij}})]\n\\]\n\\[\n\\triangleq \\mathbb{E}_{q_{\\phi}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D})}[\\sum_{L_{ij} \\in \\mathcal{L}_V} \\log p_{\\theta}(\\mathbf{y}_{L_{ij}}|\\mathcal{G}, A, \\mathbf{y}_{NB(L_{ij})})],\n\\]\nwhere \\(NB(L_{ij})\\) is the neighborhood information around interactions \\(L_{ij}\\). Next, we introduce how we apply the framework to link prediction in the multi-scale network by instantiating the \\(p\\) and \\(q\\) distributions with atomic structure scale \\(q_{\\phi}\\) and molecular network scale \\(p_{\\theta}\\) models respectively.\n\n4.4 E-Step: Atomic structure scale Modeling\n\nThe variational E-step aims to update the variational distribution \\(q_{\\phi}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D})\\) to approximate the true posterior distribution \\(p_{\\theta}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A)\\).\n\nTherefore, we could minimize the KL divergence between the posterior distribution and the variational distribution:\n\n\\[\n\\mathrm{KL}(q_{\\phi}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D}) \\| p_{\\theta}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A)).\n\\]\n\nWe followed the idea of [18, 21] to utilize the wake-sleep algorithm [43] for minimizing the reverse KL divergence (refer to Supplementary information A.2 for detailed proofs):\n\n\\[\n\\mathcal{O}(q_{\\phi}(\\mathbf{y}_{\\mathcal{L}_U})|\\mathcal{G}, \\mathcal{D}) = -\\mathrm{KL}(q_{\\phi}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D}) \\| p_{\\theta}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A))\n\\]\n\\[\n= \\sum_{\\mathbf{y}_{\\mathcal{L}_U}} q_{\\phi}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D}) \\left[ \\log p_{\\theta}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A) - \\log q_{\\phi}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D}) \\right]\n\\]\n\\[\n= -\\mathrm{KL} \\left( q_{\\phi}(\\mathbf{y}_{\\mathcal{L}'_U}|\\mathcal{G}, \\mathcal{D}) \\| \\frac{\\mathcal{F}(\\mathbf{y}_{\\mathcal{L}'_U})}{Z} \\right) + \\text{const}\n\\]\nwhere \\(Z\\) is a normalization term and \\(\\mathcal{F}(\\mathbf{y}_{\\mathcal{L}'_U})\\) is the distribution on \\(\\mathbf{y}_{\\mathcal{L}'_U}\\):\n\\[\n\\mathcal{F}(\\mathbf{y}_{\\mathcal{L}'_U}) = \\mathbb{E}_{q_{\\phi}(\\mathbf{y}_{\\mathcal{L}_U \\setminus L_{ij}}|\\mathcal{G}, \\mathcal{D})} [\\log p_{\\theta}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A)]\n\\]\n\nTherefore, we no longer need to consider the entropy of \\(p_{\\theta}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A)\\). Thus, the KL divergence could be formulated as:\n\n\\[\n\\mathrm{KL}(q_{\\phi}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathcal{G}, \\mathcal{D}) \\| p_{\\theta}(\\mathbf{y}_{\\mathcal{L}_U}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A)) =\n-\\sum_{L_{ij} \\in \\mathcal{L}_U} \\mathbb{E}_{q_{\\phi}(\\mathbf{y}_{L_{ij}}|\\mathcal{G}, \\mathcal{D})} [\\log p_{\\theta}(\\mathbf{y}_{L_{ij}}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A)] + \\text{const}.\n\\]\n\nHerein, to model the distribution of each interaction, we parameterize \\(q_{\\phi}(\\mathbf{y}_{L_{ij}}|\\mathcal{G}, \\mathcal{D})\\) with a molecular network scale GNN\\(_{\\phi}\\) for predicting the\ninteraction labels:\n\n\\[\nq_{\\phi}(\\mathbf{y}_{L_{ij}}|G,\\mathcal{E},\\mathbf{y}_{NB(L_{ij})}) = q(\\mathbf{y}_{L_{ij}}|\\sigma(W_{\\phi} \\cdot F(h_i, h_j))),\n\\]\n\nwhere the probability of each interaction class is calculated by a softmax/sigmoid classifier \\( \\sigma \\) based on the interaction representation \\( F(h_i, h_j) \\). \\( F \\) is the concatenation function to concatenate the node representations of the linking nodes \\( i, j \\) (i.e., \\( F = \\text{MLP};\\ h_{ij} = \\text{MLP}(h_i \\odot h_j) \\)), and the node representation \\( h_i \\) is learned by an atomic structure scale GNN model, which is denoted as \\( \\text{GNN}_\\phi \\).\n\nTo model the \\( \\text{GNN}_\\phi \\), we use the structural graph \\( G \\) of the biomolecules, where we represent \\( h_i^{(0)} = X_i \\in \\mathbb{R}^{n \\times d_n} \\) for the atom attributes with \\( d_n \\) as the feature dimension of atoms and \\( E_{ij} \\in \\mathbb{R}^{m \\times d_e} \\) for the edge/bond attributes with \\( d_e \\) as the feature dimension of edge. Therefore, the molecular structural representation can be denoted as:\n\n\\[\nh_i^{(l)} = f(h_i^{(l)}, f_{AGG}\\{(h_i^{(l-1)}, h_j^{(l-1)}, X) : j \\in \\text{neighbors}(i)\\}),\n\\]\n\nwhere \\( f \\) and \\( f_{AGG} \\) stand for the message and aggregation functions in the \\( l \\)-th layer respectively, \\( X \\) is the transformed node embeddings from the atomic structural graph, and neighbors(i) denote the neighbor nodes of \\( i \\).\n\nNow, the sole difficulty lies in computing the distribution \\( p_\\theta(\\mathbf{y}_{L_{ij} \\in \\mathcal{L}_U}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A)) \\), which aims to predict the label distribution of an interaction \\( L_{ij} \\in \\mathcal{L}_U \\) based on the surrounding node features and edge information. However, the labels of the unobserved interactions are not specified. Therefore, we propose to annotate the unobserved interactions with the pseudo-labels predicted by the molecular network scale model \\( \\text{GNN}_\\theta \\), so that we can approximate the distribution as follows:\n\n\\[\np_\\theta(\\mathbf{y}_{L_{ij}}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A)) = p_\\theta(\\mathbf{y}_{L_{ij}}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A, \\hat{\\mathbf{y}}_{\\mathcal{L}_U \\setminus L_{ij}}),\n\\]\n\nwhere \\( \\hat{\\mathbf{y}}_{\\mathcal{L}_U \\setminus L_{ij}} \\) denote the predicted pseudo interaction labels.\n\nCombining them with the above objective function, we could obtain the final objective function for training the GNN model of atomic structure scale:\n\n\\[\n\\begin{align*}\n\\mathcal{O}_{q_\\phi} &= \\alpha \\sum_{L_{ij} \\in \\mathcal{L}_U} \\mathbb{E}_{p(\\mathbf{y}_{L_{ij}}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A, \\hat{\\mathbf{y}}_{\\mathcal{L}_U \\setminus L_{ij}})}[\\log q(\\mathbf{y}_{L_{ij}}|\\mathcal{G}, \\mathcal{D})] \\\\\n&+ (1-\\alpha) \\sum_{L_{ij} \\in \\mathcal{L}_V} \\log q(\\mathbf{y}_{L_{ij}}|\\mathcal{G}, \\mathcal{D}),\n\\end{align*}\n\\]\n\nwhere \\( \\alpha \\) is a hyperparameter. Intuitively, the first term could be viewed as a knowledge-distilling process that teaches the model of atomic structure scale GNN_\\phi by forcing it to predict the label distribution based on the predicted pseudo interaction from the molecular network model GNN_\\theta. The second term is a supervised objective which uses the given labeled interactions for training.\n4.5 M-step: Molecular Network scale Modeling\n\nDuring the M-step, we seek to learn the parameter \\( \\theta \\) and update \\( p_\\theta \\) to maximize the objective function Eq. 3, which aims to optimize the molecular network model.\n\nHere, we parameterize the conditional distribution \\( p_\\theta \\) with another graph neural network (GNN) model on molecular network \\( \\mathcal{N} \\) because of its effectiveness:\n\n\\[\np_\\theta(\\mathbf{y}_{L_{ij} \\in \\mathcal{L}_U}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A) = p(\\mathbf{y}_{L_{ij} \\in \\mathcal{L}_U}|\\sigma(W_\\phi \\cdot g_{ij})),\n\\]\nwhere \\( p_\\theta \\) is formulated as a categorical distribution, and the probability of each interaction class is calculated by a softmax/sigmoid classifier \\( \\sigma \\) based on the interaction representation \\( g_{ij} \\). The interaction representation \\( g_{ij} \\) is derived from the hidden representation in the node level (i.e., nodes \\( g_i, g_j \\)) with a concatenation function \\( F \\). The node representation \\( g_i, g_j \\) is learned by a molecular network scale GNN model (\\( \\mathrm{GNN}_\\phi \\)), which is used to learn the molecular network information with a message-passing mechanism:\n\n\\[\ng_i^{(l)} = f(g_i^{(l)}, f_{AGG}\\{(g_i^{(l-1)}, g_j^{(l-1)}) : j \\in \\text{neighbors}(i)\\}),\n\\]\nwhere \\( f \\) and \\( f_{AGG} \\) stand for the message and aggregation functions in the \\( l \\)-th layer respectively, and neighbors(\\( i \\)) denote the neighbor nodes of \\( i \\).\n\nTo be more specific, we use the \\( \\mathrm{GNN}_\\phi \\) to generate structural representations \\( g^{(0)} \\) as node initial features and feed them into the molecular network model for message passing.\n\nWe notice that the objective function Eq. 3 also relies on the expectation with respect to \\( p_\\theta \\), which can be approximated by drawing a sample \\( \\hat{\\mathbf{y}}_{\\mathcal{L}_U} \\) from \\( p_\\theta(\\mathbf{y}_{\\mathcal{L}_U}|\\mathbf{y}_{\\mathcal{L}_V}, \\mathcal{G}, A) \\). In other words, we need the atomic structure scale model \\( \\mathrm{GNN}_\\phi \\) to predict a pseudo-label \\( \\hat{\\mathbf{y}}_{L_{ij}} \\) for each unobserved interaction \\( L_{ij} \\in \\mathcal{L}_U \\) and combine all the labels \\( \\{\\hat{\\mathbf{y}}_L\\}_{L \\in \\mathcal{L}_U} \\) into \\( \\hat{\\mathbf{y}}_{\\mathcal{L}_U} \\). Therefore, the pseudo-likelihood can be rewritten as follows:\n\n\\[\n\\begin{align*}\n\\mathcal{O}_\\theta &= \\beta \\sum_{L_{ij} \\in \\mathcal{L}_U} \\log p_\\theta(\\hat{\\mathbf{y}}_{L_{ij}}|\\mathcal{G}, A, \\mathbf{y}_{\\mathcal{L}_V}; \\hat{\\mathbf{y}}_{\\mathcal{L}_U \\setminus L_{ij}}) \\\\\n&\\quad + (1 - \\beta) \\sum_{L_{ij} \\in \\mathcal{L}_V} \\log p_\\theta(\\mathbf{y}_{L_{ij}}|\\mathcal{G}, A, \\mathbf{y}_{\\mathcal{L}_V \\setminus L_{ij}}, \\hat{\\mathbf{y}}_{\\mathcal{L}_U}),\n\\end{align*}\n\\]\nwhere \\( \\beta \\) is a hyperparameter that is added to balance the weight of the two terms. Again, the first term can be viewed as a knowledge distillation process that injects the knowledge captured by the model of atomic structure scale \\( \\mathrm{GNN}_\\phi \\) into the molecular network scale model \\( \\mathrm{GNN}_\\theta \\) via all the pseudo-labels. The second term is simply a supervised loss, where we use observed interaction labels for model training.\n4.6 Iterative Optimization\n\nAs illustrated in Fig. 1 (and Supplementary Method A.1), during each iteration, MUSE first performs the E-step, where it constructs structural graphs for each interaction pair, represented as structural graphs \\( g_1 \\) and \\( g_2 \\). Structural graph encoders (\\( f_g \\) or \\( f_d \\)) are then employed to generate representations of the protein/drug graphs and an interaction predictor is utilized to predict the interaction for the given biomolecule pair. This atomic structure scale model pulls the interacted graph pairs together and models label distributions conditioned on structural attributes. After optimization in E-step, the structural representations and interaction graph are fed into a molecular network scale message passing module. In M-step, information is propagated along interactions in the network for learning network topology and neighbor information. Consequently, MUSE iteratively updates the two modules in the E-step and M-step until the model converges. More importantly, the one-step model provides the interacting pseudo-labels for training the other, as part of mutual supervision. The pseudo-labels generated at the molecular network scale are also used as data augmentation for the atomic structure scale model while those from the atomic structure scale can be used for training the molecular network scale model by adding pseudo edges.\n\nAccording to the greedy learner hypothesis [17], it is the different speeds at which a neural network learns from different scales that lead to a utilization imbalance. The iterative optimization of the atomic structure and molecular network scale in MUSE enables us to mitigate the hurtful imbalance and achieve stronger generalization on multi-scale representations. Mutual supervision ensures that each scale model learns in the appropriate manner, thereby facilitating the utilization of effective information at different scales.\n\n4.7 Graph Neural Network for Learning Protein Representations\n\nTo evaluate the effectiveness of our EM training paradigm in interaction prediction tasks, we first use a general graph neural network (GNN)to learn graph representations of proteins, consistent with competing methods [15].\n\nRecalling our definition in Sec. 4.2, we denote the protein structural graph \\( G = \\{ \\mathcal{V}, \\mathcal{E} \\} \\) where \\( \\mathcal{V} \\) is the set of atoms \\( v \\in \\mathcal{V} \\) and \\( \\mathcal{E} \\) is the set of edges \\( e \\in \\mathcal{E} \\). Herein, \\( \\mathcal{V} \\) is a set of amino acid residues in a protein and the \\( \\mathcal{E} \\) are obtained from the protein contact map with atomic level 3D coordinates of proteins. Following Gao et al. [15], we choose the optimal cutoff distance of 10 \\( \\AA \\) for the presence or the absence of contact between a pair of residues, constructing the adjacency matrix \\( A_p \\). For the feature matrix \\( h_p^{(0)} \\), we use the protein features based on amino acid sequence, refer to [22, 44]. Each embedding vector represents a set of properties for one amino acid residue, including isoelectric point, polarity, acidity and alkalinity, hydrogen bond acceptor, hydrogen bond donor, octanol-water partition coefficient, and topological polar surface area.\nTherefore, GNN outputs the residue-level representations in each block:\n\n\\[\nh_p^{(l)} = \\text{BatchNorm} \\left( \\text{ReLU}(\\hat{A} h_p^{(l-1)} W^{(l)}) \\right),\n\\]\n\nwhere \\( \\hat{A} = \\tilde{D}^{-1/2} A_p \\tilde{D}^{-1/2} \\), \\( \\tilde{D} \\) is the diagonal degree matrix, \\( W^{(l)} \\) is a learnable weight matrix for the \\( l \\)-th GCN layer, ReLU, BatchNorm denotes the ReLU activation function and batch normalization, respectively.\n\nFurthermore, we also implemented a geometric graph neural network for learning the effective protein structural information within our EM framework. In this setting, we denote each protein chain as a graph \\( G \\) with edges \\( \\mathcal{E} \\) between the \\( k \\)-nearest neighbors of its nodes \\( \\mathcal{V} \\), with nodes corresponding to the chain’s amino acid residues represented by their \\( C\\alpha \\) atoms.\n\nInspired by GVP-GNN [45, 46], we leveraged message passing over geometric vectors and scalars, in which messages from neighboring nodes and edges are used to update node embeddings at each graph propagation step as:\n\n\\[\nh_p^{j \\rightarrow i} = \\text{MPNN} \\left( \\text{concat} \\left( h_v^{(j)}, h_e^{(j \\rightarrow i)} \\right) \\right),\n\\]\n\n\\[\nh_v^{(i)} = \\text{LayerNorm} \\left( h_v^{(i)} + \\text{Dropout} \\left( \\sum_{j : e_{j \\rightarrow i} \\in \\mathcal{E}} h_p^{(j \\rightarrow i)} \\right) \\right).\n\\]\n\nHere, \\( h_v^{(i)} \\) and \\( h_e^{(j \\rightarrow i)} \\) are the embeddings of the node \\( i \\) and edge \\( j \\rightarrow i \\), and \\( h_p^{j \\rightarrow i} \\) represents the message passed from node \\( j \\) to node \\( i \\) of proteins. For the initial geometric features, we calculate distance, direction, and angle features for each residue as node features, and construct geometric edge features between neighboring residues including distance, direction and orientation.\n\nFinally, we perform the readout operation to obtain the entire graph representation of proteins \\( H_p \\).\n\n\\[\nH_p = \\sum_{v \\in \\mathcal{V}} \\text{Readout}(h_v^{(l)}).\n\\]\n\n4.8 Graph Neural Network for Learning Drug Representations\n\nA drug structural graph also can be represented as an attributed graph \\( G = (\\mathcal{V}, \\mathcal{E}) \\), where \\( |\\mathcal{V}| = n \\) denotes a set of \\( n \\) atoms (nodes) and \\( |\\mathcal{E}| = m \\) denotes a set of \\( m \\) bonds (edges). We represent \\( X_v \\in \\mathbb{R} \\) for the node attributes and \\( E_{uv} \\in \\mathbb{R} \\) for the edge attributes. A graph neural network (GNN) \\( f^d \\) learns to embed an attributed graph \\( G \\) into a feature vector \\( h_d \\). We adopt the Graph Isomorphism Network (GIN) from [47], where the node and edge attributes are propagated at each iteration. Formally, the \\( l \\)-th iteration of a GNN is:\n\n\\[\nh_v^{(l)} = g_U^{(l)} \\left( h_v^{(l-1)}, g_{AGG}^{(l)} \\{ (h_v^{(l-1)}, h_u^{(l-1)}, X_{uv}) : u \\in \\mathcal{N}(v) \\} \\right),\n\\]\nwhere \\( h_v^{(l)} \\) are the representation of node \\( v \\) at the \\( l \\)-th layer, \\( \\mathcal{N}(v) \\) is the neighbourhood set of node \\( v \\), \\( h_v^{(0)} \\) is initialised with \\( X_v \\) encoding its atom properties. \\( g_{AGG}^{(l)} \\) stands for the aggregation function and \\( g_U^{(l)} \\) stands for the update function.\n\nAfter \\( l \\) graph convolutions, \\( h^{(l)} \\) have captured their \\( l \\)-hop neighborhood information. Finally, a readout function is used to aggregate all node representations output by the \\( l \\)-th GNN layer to obtain the entire molecule’s representation \\( H_d \\):\n\n\\[\nH_d = \\sum_{v \\in \\mathcal{V}} Readout(h_v^{(l)}).\n\\] (20)\n\n4.9 Graph Neural Network for Interaction Network Message Passing\n\nwe use the graph isomorphism networks (GIN [47]), which has the super-expressive power to capture graph structures and to learn molecular network information. Formally, the interaction network \\( \\mathcal{N} \\) is presented as \\( \\mathcal{N} = \\{ \\mathcal{G}, \\mathcal{L} \\} \\), where \\( \\mathcal{G} := \\{ G_i \\}_i^N \\) is the set of the biomolecular graph \\( G \\) and \\( \\mathcal{L} := \\{ L_{i,j} \\}_{(i,j)}^M \\) is the set of the known interaction links \\( L \\) between biomolecules, which also could be represented as the adjacency matrix \\( A \\). The initial node attributes are obtained from the model of atomic structure scale \\( H_G^{(0)} = (H_p, H_d) \\). Therefore, the molecular network scale model updates the representation of biomolecules in the \\( l \\)-th GIN block \\( \\mathrm{GNN}_\\theta \\):\n\n\\[\n\\begin{align*}\nH_v^{(l)} &= \\mathrm{GNN}_\\theta \\left( v, A, H_G^{(l-1)} \\right) \\\\\n&= \\mathrm{BatchNorm} \\left( \\mathrm{ReLU} \\left( H_v^{(l-1)} + \\sum_{u \\in \\mathcal{N}(v)} \\left( H_u^{(l-1)} \\right) \\right) \\right),\n\\end{align*}\n\\] (21)\n\nwhere \\( H_v^{(l)} \\) denotes the representation of biomolecule \\( v \\) after the \\( l \\)-th GIN block, \\( \\mathcal{N}(v) \\) is a set of biomolecules adjacent to \\( v \\).\n\nAfter stacking \\( l \\) GIN layers, node representations \\( H_G \\) are then used to predict existence of each link \\( (i, j) \\):\n\n\\[\n\\hat{Y}_{L_{ij}} = \\sigma(\\mathrm{NCN}(h_i^{(l)}, h_j^{(l)})),\n\\] (22)\n\nwhere NCN is a simple but powerful model to capture pairwise features [38], and \\( h_i^{(l)} \\) is the representation of the node \\( i \\) from \\( H_G \\).\n\nWhen applying the NCN model for pairwise predictions, we choose to keep the first-order neighbor and set the operator only to intersection:\n\n\\[\n\\mathrm{NCN}(h_i^{(l)}, h_j^{(l)}) = \\sum_{C \\in N_{(i)} \\cap N_{(j)}} \\mathrm{GNN}_\\theta^{(l)} \\left( C, A, H_G^{(l)} \\right),\n\\] (23)\nwhere GNN\\(_\\theta\\) is the powerful GIN block in molecular network scale to output the final node representations of the last message passing layer, \\(N_{(i)}, N_{(j)}\\) denote the sets of neighboring nodes for biomolecules \\(i\\) and \\(j\\), respectively, and \\(C\\) is the set of common neighbor nodes between biomolecule \\(i\\) and \\(j\\).\n\n4.10 Pseudo Likelihood Learning in the Molecular Network Scale\n\nThe limitation in the performance of link prediction tasks is from the incompleteness of the graph [38]. To alleviate this incompleteness, we adopted the pseudo-likelihood learning in our variational expectation-maximization framework, augmenting the molecular network graph \\(\\mathcal{N}\\) with pseudo interactions predicted by the atomic structure scale model GNN\\(_\\phi\\).\n\nFormally, when predicting the interaction \\(L_{ij}\\), we aim to utilize the edges \\((i, u)\\) and \\((j, u)\\) in the complete graph to compute the common neighbor \\(C_u\\). However, since \\(L_{iu}\\) and \\(L_{ju}\\) are unknown, we let the model of atomic structure scale GNN\\(_\\phi\\) output the probability of the existence for \\(L_{iu}\\) and \\(L_{ju}\\) as follows:\n\n\\[\n\\left\\{\n\\begin{array}{ll}\n\\hat{y}_{L_{iu}} = \\sigma\\left(\\mathrm{GNN}_\\phi(i, u)\\right), & \\text{if } u \\in N_{(j)} - N_{(i)} \\\\\n\\hat{y}_{L_{ju}} = \\sigma\\left(\\mathrm{GNN}_\\phi(j, u)\\right), & \\text{if } u \\in N_{(i)} - N_{(j)}\n\\end{array}\n\\right.\n\\]\n\nwhere GNN\\(_\\phi\\) represents the GNN model of atomic structure scale, \\(\\hat{y}_{L_{iu}}\\) and \\(\\hat{y}_{L_{ju}}\\) denote the probabilities of the existence of interactions \\(i \\to u\\) and \\(j \\to u\\), respectively. When the probability exceeds the threshold \\(1-t\\), the predicted interaction is incorporated into the interaction network graph.\n\nTherefore, the interaction network graph \\(\\mathcal{N}\\) has been complemented softly, and then the molecular network model GNN\\(_\\theta\\) on the more complete graph to give final predictions.\n\nFurthermore, this strategy has been extended to our iterative optimization process. Starting from the original network \\(\\mathcal{N}^{(0)} = \\mathcal{N}\\), we iteratively complete the graph to get the \\(\\mathcal{N}^{(k)}\\) from \\(\\mathcal{N}^{(k-1)}\\) with the help of the prediction of other scale model (i.e. atomic structure scale model) until the final iteration \\(k\\).\n\n4.11 Utilization Rate Estimation\n\nFor a multi-scale model \\(M\\), taking two scales \\(s_0\\) (atomic structure scale) and \\(s_1\\) (molecular network scale) as inputs, its utilization rates for \\(s_0\\) and \\(s_1\\) are defined as\n\\[\nu(s_0|s) = \\frac{f(M) - f(M_1)}{f(M_1)},\n\\]\nand\n\\[\nu(s_1|s) = \\frac{f(M) - f(M_0)}{f(M_0)}\n\\]\nHere, \\(M_0\\) and \\(M_1\\) represent single-scale models obtained from the multi-scale model \\(M\\), while \\(f\\) denotes the predicted evaluation function. The utilization rate is the relative change in accuracy between the two models within each pair.\nFor example, \\( u(s_0|s) \\) measures the incremental impact of the atomic structure scale \\( s_0 \\) on improving the accuracy of label predictions. It is constrained within the range of -1 to 1. A higher utilization rate indicates that the multi-scale model can benefit from incorporating this scale.\n\n4.12 Evaluation Metrics\n\nFor the three multi-scale interaction prediction benchmarks, i.e. SHS27K, BioSNAP, and DeepDDI, we evaluated their performance using micro-F1 (Best-F1), Area Under the Receiver Operating Characteristic curve (AUROC) and Area Under Precision-Recall Curve (AUPRC). In particular, for the multi-label PPI prediction, the different PPI types in the datasets we used are very imbalanced, so micro-F1 may be preferred.\n\nTo evaluate the prediction of protein inter-chain contact, we follow the setting established by [30], where a positive label is assigned to each inter-chain residue pair found within 6 Å of each other in the complex’s bound (i.e., structurally-conformed) state. We use Average top-k precision (P@k), Recall (R@k), and Area Under the Receiver Operating Characteristic curve (AUROC) to assess our method in predicting protein-protein interactions and the quality of the generated docking results.\n\nFollowing the previous studies [16], we use Area Under the Receiver Operating Characteristic curve (AUROC), and Area Under the Precision-Recall Curve (AUPRC) to evaluate the binding-sites prediction performance.\n\n4.13 Implementation details\n\nWe trained the model by using the AdamW optimizer with Pytorch (v2.0.1), pytorch geometric (v2.3.0), and Python (v3.9.16). The experiments of protein and drug interaction predictions and protein binding site predictions were performed five times on an NVIDIA GeForce RTX 4090 GPU, and the experiments on protein contact interface predictions were performed on A800 GPU with a large GPU memory. The iteration k of the EM framework was usually converged in 5-8 iterations. The hyper-parameters on each task and additional ablation study are presented in Supplementary information B.\n\nData Availability\n\nThe PPI and protein data used in this study are obtained from the previous study (HIGH-PPI), which are available in the Zenodo database under accession code https://doi.org/10.5281/zenodo.7213401. The native protein structures are obtained from PDB: https://www.rcsb.org/. The DPI data are obtained from the previous study (ConPLex), which are available on GitHub (https://github.com/samsledje/ConPLex_dev/tree/main/dataset/BIOSNAP). The DDI data are obtained from the previous study (MIRACLE), which are available on GitHub (https://github.com/isjakewong/MIRACLE/tree/main/MIRACLE/datachem). The DIPS-Plus are obtained from the\nprevious study (DeepInteract), which is available in https://github.com/BioinfoMachineLearning/DIPS-Plus. The protein-protein binding sites dataset is obtained from https://github.com/jertubiana/ScanNet/tree/main/datasets.\n\nCode availability\n\nThe source code of MUSE is available at https://github.com/biomed-AI/MUSE.\n\nFunding and Acknowledgements\n\nThis study has been supported by the National Key R&D Program of China (2022YFF1203100), the National Natural Science Foundation of China (T2394502), and the Fundamental Research Funds for the Central Universities (Sun Yat-sen University, 22lglj08).\n\nConflict of interest\n\nThe authors declare that no competing interests exist.\n\nInclusion and Ethics statement\n\nAll collaborators of this study have fulfilled the criteria for authorship required by Nature Portfolio journals.\n\nAuthors’ contributions\n\nJ.R. and Y.Y. conceived and supervised the project. J.R., J.X., and S.Z. contributed to the algorithm implementation. J.R., Y.L., S.Z., and Y.Y. wrote the manuscript. Q.Y, D.L., Z.W. Y.L, S.Z., and Y.Y. were involved in the discussion and proofreading.\n(a) Multi-scale Vanilla Learning\n\nAtomic Structure Scale\nMolecular Network Scale\n\nVanilla Learning:\n\\( \\mathcal{L} = \\mathcal{L}_{network} + \\mathcal{L}_{structure} \\)\n\n(b) Multi-scale EM Framework (MUSE)\n\nExpectation step (Atomic Structure Scale)\nMaximization step (Molecular Network Scale)\n\nIterative optimization\n\n(c) Applications\n\nMolecular Network Tasks\nAtomic Structure Tasks\n\nInteraction Prediction\nProtein Interface Contact\nProtein Binding Sites\n\nWhether to interact\nHow to interact\n\nFig. 1: Illustration of the MUSE framework and its applications. (a) The vanilla approach for learning multi-scale representations is to combine the two single-scale models and optimize them jointly. (b) The EM framework (MUSE) for Multi-scale Learning. The Expectation step trains a model with structural information of protein and drug as input to fit the known and pseudo interactions (the predicted interactions from the M-step except the first iteration). The updated interactions and structural embeddings were input to the M-step, where the molecular network was constructed to maximize the known interactions and the predicted interactions from the E-step. The updated interactions were sent to E-step for new iterations. (c) MUSE is generalizable and applicable to multiple prediction tasks: predicting different types of molecular interactions and molecular binding interfaces.\nFig. 2: (a) Precision-recall curves of PPI prediction on SHS27k, DPI prediction on BioSNAP, and DDI prediction on DeepDDI, showing the performance of MUSE compared to state-of-the-art baselines. (b) Receiver Operator characteristic curves of PPI prediction on SHS27k, DPI prediction on BioSNAP, and DDI prediction on DeepDDI, showing the performance of MUSE compared to state-of-the-art baselines. (c) Barplot shows the best micro-F1 scores (Best-F1) or ROC-AUC of baseline, ablation study MUSE-Joint and MUSE predictions respectively on PPI predictions (Random, BFS and DFS splits), DPI predictions (Unseen Protein or Drugs) and DDI predictions.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
MethodDIPS-Plus
AUCP@10P@L/10P@L/5R@LR@L/2R@L/5
BI-0.010.010.010.010.0040.003
CDPred0.8600.150.150.130.090.060.03
DeepInteract0.9020.200.190.170.150.090.04
GLINTER0.8780.230.220.190.150.100.06
MUSE0.9200.260.250.230.200.120.09
\n\nFig. 3: (a) The average top-k precision, recall, and AUROC metrics for different protein-protein interaction prediction methods on the DIPS-Plus benchmark. Five predictors are compared: BIPSPI, DeepInteract, GLINTER, CDPred, and MUSE. (b) The ground truth and predictions for PDB entry 1UZN are presented. For each method, we display the surface of the predicted and ground truth ligand relative to the ground truth receptor. Following previous work [27], we employed the Kabsch algorithm to dock the two proteins based on the contact map predicted by each method and calculated the Root Mean Square Deviation (RMSD) for the ground truth. (c) MUSE achieves state-of-the-art performance on a broad range of test sets in the PPBS dataset compared with state-of-the-art baselines and an ablation study MUSE-Joint.\nFig. 4: (a) The boxplot of utilization rate in each scale for different multi-scale models, demonstrating that MUSE efficiently alleviates the inhibition on molecular network scale and fully exploits the atomic structural properties in multi-scale learning. (b) The convergence curves of MUSE and MUSE-Joint on the PPI dataset during the EM optimization iteration steps. The red curve in iterative optimization shows how MUSE continuously alleviates the imbalance characteristics of multi-scale learning and improves its multi-scale utilization. (c) Visualization and Case Study on the interaction predictions of molecular network model, MUSE-Joint and MUSE. Case (#1) represents the examples in which MUSE-Joint cannot utilize other scale information for prediction, and case (#2) represents the examples in which MUSE-Joint is disturbed by other scale learning. MUSE classifies these interaction types between protein and protein clearly.\nFig. 5: (a) Left: Depiction of a complex protein (protein, PDB id: 3CQQ-A). Right: Residue importance of the query protein learned from MUSE with coloring ranging from low (red) to high (red). (b) Two-dimensional projection of the learned atomic structure scale representation using t-SNE. Each point corresponds to an interaction. Coloring is based on the interaction types. The learned atomic structural representation of MUSE is effective for label prediction while the representation learned by HIGH-PPI is quite close to the random initialization. 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Click to download.\n\n• MUSEsupprevised.pdf\n• NCOMMS2358788ARS.pdf"} {"paper_id": "prb36", "title": "Data-driven identification of predictive risk biomarkers for subgroups of osteoarthritis using an interpretable machine learning framework: a UK biobank study", "text": "# Abstract\n\nOsteoarthritis (OA) is increasing in prevalence and has a severe impact on patients’ lives. However, our understanding of biomarkers driving OA risk remains limited. We developed a model predicting the five-year risk of OA, integrating clinical, lifestyle and biomarker data from the UK Biobank (19,120 patients with OA, ROC-AUC:0.72 95%CI (0.71 – 0.73)). Higher age, BMI, and prescription of non-steroidal anti-inflammatory drugs contributed most to increased OA risk prediction. 14 sub-groups of OA risk profiles were identified, and validated in an independent set of patients evaluating the 11-year OA risk, with 88% of patients uniquely assigned to one of the sub-groups. Individual OA risk profiles were characterised by personalised biomarkers. Omics integration demonstrated the predictive importance of key OA genes and pathways (e.g. *GDF5* and TGF-β signalling) and identified OA-specific biomarkers (e.g. CRTAC1 and COL9A1). In summary, this work identified opportunities for personalised OA prevention and insights into its underlying pathogenesis.\n\n- Health sciences/Risk factors\n- Biological sciences/Computational biology and bioinformatics/Machine learning\n- Biological sciences/Computational biology and bioinformatics/Predictive medicine\n\n# Introduction\n\nOsteoarthritis (OA) is a chronic degenerative joint disease, that results in decreased quality of life and a high economic health-care burden. Globally, 528 million people are living with OA1. The global prevalence has increased by 48% from 1990 to 2019, with further increases expected due to ageing populations and the increasing prevalence of obesity1,2. OA has a high impact on health care expenditure and social care cost3, with the economic impact ranging from 1 to 2.5% of gross national product (GNP) in some countries. The average annual cost of OA for an individual is estimated to be between $700-$15,600 (2019)1. Patients are often diagnosed with late-stage disease when irreversible joint damage has already occurred4. There are currently no approved treatments that can prevent OA development and progression or cure the disease4. The main treatments remain symptomatic, with some patients ultimately needing joint replacement surgery5. Hence, there is a need to identify strategies that aid disease prevention and early diagnosis, to facilitate the development of disease modifying therapies.\n\nAn improved understanding of OA pathogenesis is necessary to develop new approaches to early diagnosis, prevention and treatment of OA5,6. OA is a complex and heterogenous disease, spanning multiple biological mechanisms. These range from cartilage degeneration to systemic and synovial inflammation5,6. It has been proposed that OA would benefit from the use of data-driven and machine learning approaches for patient-specific prediction models to dissect the complex relationship between susceptibility biomarkers4,7–9.\n\nPrevious disease predictions of OA have been limited by a focus on knee OA, small sample sizes, restricted sets of input features and more traditional statistical analysis methods4,8,9. Additionally, multiple studies focus on disease classification or the prediction of disease progression rather than prediction of disease incidence4.\n\nKnown OA risk biomarkers include age, female sex, BMI/obesity10, genetic predisposition, as well as joint-specific risk biomarkers such as injuries11. However, the complex interplay between risk biomarkers, and to what extent combinations of risk biomarkers can predict individual OA risk, remains to be determined.\n\nDespite efforts to predict individual risk of OA, the majority of these have lacked comprehensive incorporation of genetics, clinical biomarkers and other environmental factors to guide preventative strategies and precision medicine4,8,12. Additionally, further work is required to study the impact of changes in modifiable risk biomarkers on the individual risk of OA9. Machine learning methods have the unique potential to integrate diverse patient data for the prediction of disease outcomes13. In this study, we developed a machine learning model to predict individual five-year risk of OA and identify risk biomarkers. Through the integration of multi-modal patient data, we identified sub-groups of OA with differing risk biomarker profiles. The model captured the broad patient landscape in a UK cohort of ~20,000 people diagnosed with OA, capturing electronic health records (EHR), clinical biomarkers, self-reported questionnaire data, genomics, proteomics, and metabolomics on available subsets of individuals. The model quantified the impact of risk biomarkers on the predicted OA risk at the population and individual level, enabling detailed estimation of the contribution of these biomarkers for OA risk.\n\n# Results\n\n## OA study population and risk modelling\n\n103,086 patients with OA were identified from primary and secondary EHR data (~21% of all UK biobank study participants, Sup File 1). The UK biobank contains detailed phenotyping of individuals at the recruitment assessment centre between 2006 – 2010. Primary care data enabled the capture of longitudinal OA progression data but was only available for a subset of patients with OA (N = 67,772). An equal number of control participants who never developed OA were identified (N = 67,772). Controls were randomly selected and date-matched with the OA diagnosis dates for case patients. Cases and controls were then filtered for those with an OA diagnosis/matched index date a maximum of five years after the recruitment assessment centre. Controls were required to have observational data and no death registered during the five years prior to the index date (study period: 06/2006 – 09/2015). This resulted in a total of 19,120 patients with OA and 19,252 controls included in the analysis (Fig. 1A left, Sup Fig. 1). The cases and controls were well-matched based on comparison of baseline distribution for known OA risk biomarkers (Fig. 1B). For the patients with OA, the specific joints affected were mapped to the following groups: foot (4%), spine (10%), arm (11%), hip (13%), and knee (28%) (Fig. 1C). In addition to the OA study population, an independent hold-out validation cohort was generated following the same procedure as above. However, for this validation cohort, the time between data collection at the assessment centre and OA diagnosis was more than five years. (Fig. 1A left, 1B, study period: 09/2011 – 09/2017).\n\nBased on the identified cases and controls in the OA study population, an eXtreme Gradient Boosting (XGBoost) machine learning model was trained to predict the five-year risk of developing OA using multi-model longitudinal data. Performance was evaluated in the test set in a 5*5 cross-validation (Fig. 1A right). The XGBoost model integrated clinical, sociodemographic, diet, physical activity and lifestyle data from the recruitment assessment centre, with clinical data from the five-year longitudinal EHR data (Fig.1A left). The EHR data captured diagnosis of previous post-traumatic OA diagnosis, longitudinal blood and urine biomarkers, clinical measurements, as well as medication data for obesity, OA, and type 2 diabetes. Longitudinal data was captured in the five years prior to OA diagnosis/index date using yearly data bins (Sup Fig. 2). Missingness estimation for each feature included in the machine learning models is presented in Sup File2.\n\n## Prediction of OA from five-year multi-modal clinical data\n\nLongitudinal clinical data were integrated in a XGBoost model predicting the five-year risk of OA (Clin model), achieving a cross-validated ROC-AUC performance of 0.72 (95% CI: 0.71 – 0.73, Fig. 2A, 2B and 2C). The Clin model was able to predict 7 in 10 patients who developed OA, and out of all the OA case predictions made by the model, 66% of these were true-positive OA cases (Fig. 2C). Conversely, we were able to predict 6 in 10 patients who did not develop OA, with 67% of the predicted controls being true-negative controls (Fig. 2C). Clin model’s predictive performance was robust across random model initialisations and performed significantly better than models trained on permuted OA status labels (Sup Table 1). We assessed if the Clin model had a stronger predictive performance when predicting specific subgroups of OA across different affected joints, specified for some of the OA diagnoses, including arm, foot, hip, knee, or spine. Performance ranged with ROC-AUC: 0.67 – 0.73 (Fig. 2A) and was highest for weight-bearing joints (ROC-AUC: 0.73 for knee OA prediction, and 0.72 for hip OA prediction).\n\n## Population risk biomarkers predictive of OA risk\n\nTo interpret which risk biomarkers were most important for OA prediction, Shapley additive explanations (SHAP) values were calculated. SHAP values estimate the marginal conditional impact of a feature on the model’s prediction in relation to all other features included in the model. The top three predictors of increased OA risk included higher age, prescription of non-steroidal anti-inflammatory drugs (NSAIDs) during the year prior to OA diagnosis, and higher BMI compared to individuals that did not develop OA (Fig. 2D). Following these three risk biomarkers, predictive contributions were made by a variety of features across individuals. Participants who rated their own health as excellent and had a faster walking pace, had a lower risk of OA. Higher levels of vitamin D were predictive of increased OA risk, and individuals that reported taking vitamin D supplements typically had a higher age and higher levels of vitamin D (Sup Fig. 3). Additionally, a higher hand grip strength, and a lower ratio of fat mass to fat free mass were also predictive of lower OA risk. Individuals that had a higher socioeconomic status, as indicated by having a college or university degree and higher income, had a lower risk of OA. In contrast, people working heavy manual or physical jobs, or doing shift work, had increased risk of OA.\n\n## Precision sub-groups of OA\n\nThe Clin model confirmed that the biological and environmental risk factors underlying OA are heterogenous across individuals. We attempted to capture this heterogeneity and categorise patients into sub-groups with differing risk biomarker profiles. Hence, we clustered the SHAP values, as estimated by the Clin model, for all risk biomarkers across all individuals. The clustering resolution was optimised based on silhouette scores and prediction metrics (Sup Fig. 4) identifying 14 clusters of individuals (Fig. 3A). The clustering allowed us to uncover sub-groups of individuals predicted to have high risk of OA (cf. prediction probabilities shown in Fig. 3B). Furthermore, by using SHAP values, rather than the original input values, we were able to account for the relative importance of features for OA prediction (Fig. 3C). Finally, all identified clusters were described using the average values of the top 6 features in our model, using the original input values to characterise the differences between clusters. This generated an overview of the most defining characteristics of each OA sub-group, capturing predicted archetypes of OA risk with distinct biomarker profiles (Fig. 3D).\n\nTo identify clusters with high predicted OA risk and understand sub-group characteristics, we defined the prediction performance of the XGBoost model within each cluster (F1/PPV/Sensitivity) the cluster case/control ratios and average prediction probability (Fig. 4). The top 3 clusters (12, 11 and 0), representing 23% of all individuals, were the clusters for which individuals were best predicted as OA cases, with F1 > 0.83. Another group of 6 clusters (10, 5, 9, 1, 13 and 8; ~35% of all individuals) had more modest values, but were still predictive for OA (0.73 > F1 > 0.61). The last 5 clusters (6, 7, 3, 4 and 2; ~ 41% of all individuals) were the least predictive for OA (F1 < 0.35).\n\nWe used a decision tree-based algorithm (SkopeRules) to define sets of rules, per cluster, based on the input values of the XGBoost model. These rules allowed us to “scope” each predicted OA archetype by identifying the most distinctive variables and values that determined an individual’s cluster allocation with high PPV (Fig. 4, Sup Fig. 5). The rules that defined the top 3 high-risk patient groups included: age, prescription of NSAIDs within the last year, hand grip strength, self-reported walking pace and health rating, Townsend deprivation index and IGF-1 levels (Fig. 4). To validate the potential clinical value of these rules, we applied them to an independent hold-out population (with similar case/control definitions, and with cases being diagnosed more than five years after the assessment center visit; 7,341 cases and 5,999 controls). While 4% of individuals could not be accurately mapped to any sub-group based on these sets of rules, we were able to uniquely assign 88.2% of individuals to a cluster, and 7.8% to two possible clusters. In the latter case, we selected the cluster with the highest case/control ratio in the OA study population in order to minimise the risk of false negatives (Fig. 4 shows cluster attribution). We observed a high correlation of case/control ratios between clusters of the OA study and hold-out populations (R² = 0.90), as well as a strong correlation in the proportion of individuals in each cluster (R² = 0.68) (Sup Fig. 6).\n\n## Personalised risk biomarkers of OA\n\nInterpretation using SHAP values from the XGBoost models enabled us to quantify the impact an individual’s patient data had on their predicted risk of OA. We extracted and visualised individual OA risk profiles using waterfall plots, demonstrating the predicted positive and negative impact of personal OA risk biomarkers (Fig. 5). For example, a patient who developed OA from Cluster 1 had a predicted risk of 64% for OA. This predicted risk was predominantly driven by a BMI in the obesity range and age of 65 years (Fig. 5A). However, this patient had not taken NSAIDs 1 year prior to OA diagnosis, and this decreased the predicted risk for OA. Other risk biomarkers had more minor contributions to increasing the predicted OA risk, including a lower muscle strength (indicated by hand grip strength), and lower socioeconomic status (indicated by lower average income and level of education). For this patient, if the BMI was not considered, the predicted OA risk would have decreased to 57%. Our results are suggestive of potential intervention opportunities on high impact modifiable risk biomarkers that may be driving OA risk.\n\nAdditional individual OA risk profiles were examined, including an individual from cluster 2 with very low predicted OA risk (Fig. 5B), patient with OA from cluster 12 with multiple signs of poor metabolic health (Fig. 5C), and an individual profile impacted by lifestyle factors such as heavy manual/physical work and shift work from cluster 9 (Fig. 5D).\n\n## Multi-omics OA risk biomarkers\n\nTo explore molecular risk biomarkers of OA in the context of the clinical prediction model (Clin model), we integrated various types of omics data with the clinical features including OA genetics (ClinSNP, ClinGRS and ClinPath models), metabolomics (ClinMet model) and proteomics data (ClinPro model) for subsets of individuals where this data were available (Fig. 6A). The predictive performance remained unchanged compared to the Clin model (ROC-AUC: 0.70 – 0.72, Fig. 6A, sensitivity analysis of the Clin model on these specific subsets in Sup Table 2). However, the inclusion of OA omics signatures influenced the rankings of OA risk biomarkers in the model (Fig. 6A and 6B).\n\nFirstly, when including a whole-genome polygenic risk score (WGPRS) for OA in our models (ClinWGPRS), it was the sixth most predictive risk feature for OA risk (data not shown). At the population level, the OA WGPRS did not affect the overall performance of the model (ROC-AUC: 0.72) compared to Clin model. However, the predictive performance for the model (F1 and sensitivity) were higher for a population with higher OA WGPRS (Sup Fig. 7). Therefore, although the OA WGPRS provided minimal additional benefit when predicting OA at the population level, it did provide additional value for sub-groups with more extreme genetic risk.\n\nAt the gene locus level, the highest ranked gene-level genetic risk scores (gene-GRS) by the OA prediction model were *TGFB1*, *GDF5*, *PTCH1* and *FAM53A*. The relevance of *TGFB1* to OA was further supported by the TGF beta signalling pathway being the top ranked pathway-level polygenic risk score (pathway-PRS). Other pathways identified as being predictive of OA, in the context of clinical features, included glycosphingolipid biosynthesis, adipocytokine signalling and cytokine-cytokine receptor interactions. No strong predictive signal was identified for previously reported OA-associated single nucleotide variants. Blood plasma metabolites that were identified as being important for the prediction of OA included acetate, valine, 3-hydroxybutyrate, citrate and the percentage of saturated fatty acids to total fatty acids. Strong predictive proteomics signatures were identified where CRTAC1, COL9A1, ACTA2, EDA2R and TACSTD2 were the most predictive of OA risk together with higher age, prescription of NSAIDs during the year prior to OA diagnosis, and higher BMI as seen in the Clin model (Sup Fig. 8). There were significant differences in the normalised expression levels of all five proteins between OA cases and controls. Higher levels of CRTAC1, COL9A1, ACTA2, EDA2R were observed in patients with OA, whereas lower levels of TACSTD2 were observed in patients with OA (Fig. 6B). Interaction dependencies in the XGBoost model between these top five proteins and the most predictive clinical features of OA risk (age, NSAIDs prescriptions one year before diagnosis and BMI) were tested. Significant interactions were identified between age and CRTAC1, COL9A1, EDA2R and TACSTD2 (Sup Fig. 9). Protein levels of COL9A1 were more important for OA prediction in people with an age above 55. EDA2R was generally seen in lower protein levels for individuals under 60 years old, while increased importance of EDA2R as an OA risk biomarker was seen in older individuals.\n\n# Discussion\n\nWe present a large-scale study of OA, in a UK cohort of ~20,000 patients with OA and ~20,000 controls, encompassing a broad set of OA risk biomarkers. Using interpretable machine learning, we developed a model predictive of an individual’s five-year risk of progression to OA. We mapped the complex landscape of risk biomarkers using both multi-modal clinical data and molecular signatures of OA. We identified sub-groups of OA, characterised by distinct profiles of risk biomarkers. Furthermore, our clustering approach enabled us to derive simple clinical association rules for these sub-groups. Finally, we demonstrated how individual patient journeys can be dissected to identify risk biomarkers for OA, which might allow the development of personalised preventative strategies.\n\nOA has significant health consequences with links to frailty and multimorbidity, highlighting the need for OA prevention strategies2. However, to develop appropriate preventative strategies, there is a need for reliable predictive models with robust performance. Previous OA risk studies have either focussed on a specific joint (such as knee OA)2,27, included relatively small sample sizes, used only questionnaire-based data, incorporated a small set of risk biomarkers, or did not dissect clusters of patients with varying OA risk profiles4,9,12,16,17. To realise the full potential of machine learning to advance our understanding of OA risk, there is a need for more diverse studies of OA, encompassing multiple OA subtypes and diverse patient cohorts9. The OA risk models described in this paper were built using a large sample size of approximately 20,000 patients with OA, utilising a large set of longitudinal clinical, biochemical, and omics-based risk biomarkers, and identified patient clusters which varied in OA risk profiles. We demonstrated the strong and robust predictive performance of our model, with the model able to correctly predict 7 in 10 patients who developed OA, with 66% of these being true-positive OA cases. The model identified and estimated the predictive impact for a range of risk biomarkers. Some of these were recognised as OA risk biomarkers (e.g. age and BMI)11, while others were not traditionally considered OA risk biomarkers (e.g. personal health rating, hand grip strength, body composition, and walking pace). This highlights the heterogeneity in OA pathogenesis and the novelty of the OA risk models in our study. Preventative interventions may need to target multiple risk biomarkers to reduce OA incidence. Most of the predictors included in the model are easy to obtain in clinical practice, although some may require specific testing, such as hand grip strength. Risk biomarkers that are easy to obtain clinically may enable preventative strategies that prioritise interventions to those with the highest risk.\n\nAge and BMI were the top and 3rd predictor of OA in the model respectively, both of which are established risk biomarkers for OA10. The impact of BMI on the risk of OA was present even in those who did not have BMI ≥ 30 kg2, with lower BMI levels reducing OA risk. This is unsurprising since increases in BMI levels, regardless of the BMI category in which the increase occurs, can increase the risk of obesity-related complications (as seen in type 2 diabetes18). NSAID prescription one year prior to OA diagnosis was the second most important predictor. This likely reflects the delay or clinical inertia in the diagnosis of OA, reflecting several barriers to OA management in primary care that have been described previously19,20.\n\nHigher vitamin D levels were also identified as a predictor of increased OA risk in this model. It was observed that individuals taking vitamin D supplements typically had higher vitamin D levels and a higher age. Therefore, vitamin D levels in the Clin model may be capturing an older population who take vitamin supplements. Vitamin D may affect progression and pain associated with OA21–23, but the levels of vitamin D and use of supplements may vary across different global societies24. Additionally, it was seen that a lower socioeconomic status, as indicated by a lower income and level of education, was predictive of an increased OA risk. This agrees with previous work, that demonstrated that social deprivation, including lower education, was associated with increased OA risk25,26. Additionally, lower social deprivation and increased OA risk were previously linked to obesity25.\n\nThere have been efforts to identify sub-groups of OA to enable targeted treatment and management of patients. Sub-groups of OA have been proposed based on a shortlist of blood and urine biomarkers; however, these did not incorporate additional types of patient data6. Sub-groups based on comorbid symptoms have also been identified, but this was restricted to older individuals with knee or hip OA27. Both studies are limited by identifying sub-groups of established disease, which does not contribute to the understanding of the impact of risk biomarkers on developing OA. By modelling OA risk biomarkers ahead of diagnosis, we were able to identify opportunities for early intervention and prevention of disease progression.\n\nOur data-driven approach allowed identification of distinct sub-groups of OA risk profiles. These results suggest that simple sets of rules may be used to assign most individuals to specific sub-groups, which differ in their predicted OA risk and risk biomarkers. This approach may help inform both clinicians and patients to simply assess the potential for belonging to high-risk groups for OA risk, and the need for an OA diagnostic assessment. The interpretable machine learning approach also provided an understanding of the contributing factors to the predicted OA risk for specific individuals. This explainability generates trust in the predictions and enables identification of high-risk individuals to target for prevention of disease progression. OA Risk C (calculator.oarisk.org)28 is an online tool that estimates the risk of an individual developing knee OA. However, it is limited by its restricted set of risk biomarkers. We present a more complex OA risk model, encompassing a wider range of OA risk biomarkers. Our study could contribute to the prioritisation of relevant input data for future, more comprehensive OA risk tools. In addition, our incorporation of modifiable risk biomarkers may inform potential interventions targeting the risk biomarkers. Based on machine learning predictions of OA risk, it cannot be fully assessed whether intervention on risk biomarkers would decrease OA risk, and the extent of this decrease. However, it has previously been shown that reduction in modifiable risk biomarkers corresponded with a reduced individual probability of developing knee OA12.\n\nAlthough the integration of omics in our models did not improve the overall performance, it did change the ranking of the risk biomarkers. Some omics biomarkers replaced clinical risk biomarkers, with some being more predictive of OA risk than BMI (CRTAC1 and COL9A1). CRTAC1 was the most predictive protein and has previously been proposed as an OA risk biomarker29–31. CRTAC1 is associated with OA diagnosis across multiple joints, and with the severity of OA, including progression to total joint replacement29–31. These findings are across multiple cohorts (including the UK Biobank), proteomics technologies, and methods. It has been suggested that CRTAC1 is upregulated in joints in OA by pro-inflammatory cytokines, and there may be a sex specific role for CRTAC1 in OA progression32. COL9A1 is both genetically and epigenetically linked to OA with its hypermethylation linked to decreased anabolism in OA33–37. Additionally, mutations in COL9A1 are associated with multiple epiphyseal dysplasia, a hereditary condition characterised by early onset OA36.\n\nThe integration of multiple omics biomarkers highlighted relevant biological pathways important for OA disease prediction. An improved understanding of predictive OA molecular risk biomarkers may help guide more OA-specific prevention strategies. In contrast, other clinical risk biomarkers, such as BMI, may reflect a more general risk of obesity-related complications12. Proteomics biomarkers were highly important in the prediction of OA risk and other identified proteins included ACTA2 and EDA2R. The smooth muscle cell protein ACTA2 has previously been associated with sub-groups of OA38, and is associated with clusters of smooth muscle cells in the OA synovium39. Lastly, EDA2R has previously been associated with TNF mediated inflammation, in the context of rheumatoid arthritis40.\n\nIt has been demonstrated that multiple genetic risk variants are associated with OA5. Although the OA WGPRS had limited predictive value across the general population, we found it may be informative for those with more extreme genetic risk. It has previously been seen that only a small proportion of variance in OA can be explained by genetics5, and that genetics had a limited ability to predict OA16,41. This highlights the importance of including additional clinical and biological data in prediction models, to provide contextual disease information.\n\nOur GRS approach enabled us to estimate the contribution to predicted OA risk from genes previously associated with OA. The GRS for the TGFB1 locus was the top ranked GRS in the ClinGRS model. TGF-β signalling affects chondrocytes, mesenchymal stem cells and synovial lining cells in OA development and progression42. Multiple components of the TGF-β pathway have been genetically associated with OA, including SMAD3, a regulator of TGFB1 expression that impacts chondrogenic differentiation42,43. In phase 3 clinical trials, TGFB1 cell and gene therapy improved function and pain in knee OA44. The GDF5 GRS was predictive for OA and GDF5 has a role in chondrogenesis, a critical process for cartilage and bone development45. Higher levels of GDF5 were seen in OA with advanced cartilage damage46, and GDF5 is currently a target in clinical development for cartilage regeneration indications43. Lastly, the PTCH1 GRS was predictive of OA, and PTCH1 encodes a transmembrane receptor for Hedgehog ligands. Hedgehog signalling is associated with chondrocyte proliferation, osteogenesis, cartilage degeneration and disease severity in OA5,47,48. Loss of PTCH1 induces OA-like phenotypes48,49 and PTCH1 is genetically associated with total hip, knee and joint replacements5. Therefore, PTCH1 may be particularly relevant for OA disease progression, and targeting the Hedgehog pathway may be a therapeutic opportunity for OA47.\n\nMultiple metabolites were relevant for predicting OA and have previous associations with the complex metabolism underlying OA. Acetate was the most predictive metabolite for OA. ACOT12 breaks down acetyl-CoA into acetate and CoA, and is a novel regulator of de novo lipogenesis (DNL) associated cartilage degradation in OA50. Valine was also predictive for OA and is an essential branched chain amino acid (BCAA). Valine has previously been associated with the severity of inflammation in synovial tissue51. BCAAs may play a role in increased inflammation, reduced autophagy, and increased insulin resistance in OA52. The ketone body 3-hydroxybutarate (βHB, β-hydroxybutarate) may have anti-senescence effects which delay OA progression53. Finally, citrate levels in synovial fluid have conflicting associations with knee OA54, and may be linked to altered energy metabolism55.\n\nThere is a complex relationship between fatty acids and OA, that may be impacted by sex, obesity, OA joint and whether measured in the fasted or postprandial state56,57. Different fatty acids have distinct effects on OA58. Previous work has shown that longer chain saturated fatty acids induced metabolic syndrome and OA-like cartilage degradation59,60, and induced systemic inflammation, independent of weight-gain in obesity related OA61.\n\nCurrently, omics data may not be easily available in routine clinical practice, although this may change in the future as the utility of omics biomarkers matures. However, even without the inclusion of omics data, our Clin model provided a significant advance in predicting the risk of OA across subgroups and at the individual level, encompassing a broad set of clinical risk biomarkers. The availability of some of the clinical risk biomarkers, such as hand grip strength and regional body composition, might be challenging depending on the health care system and the setting (for example primary vs secondary care). Nonetheless, the top 6 predictors in the Clin model were all easily obtainable. Our study incorporated a diversity of risk biomarkers, including genetics, proteomics, and metabolomics. Future work would benefit from the incorporation of joint imaging data, WOMAC pain scores, and transcriptomic data, which may contribute to the prediction of OA and a better understanding of biological pathways associated with (progression of) OA62–64. It should also be noted that the timing of biological sampling, whether in the UK Biobank or clinical practice, may have an impact on risk biomarker levels and estimated OA risk.\n\nIn summary, we present large-scale predictive models for incident OA risk, incorporating a broad range of risk biomarkers. The use of interpretable machine learning for individual patients enabled the identification of personalised modifiable risk biomarkers, opening up the opportunity for tailored OA preventative strategies. Our integration of omics features identified OA-specific risk biomarkers and highlighted the predictive importance of underlying OA disease biology. Taken together, these findings may advance early screening, prevention and treatment of OA, reducing both disease incidence and progression.\n\n# Online Methods\n\nUK biobank \nThe UK Biobank is a human cohort comprising ~ 500,000 individuals, aged between 40 and 69 years at recruitment, from 2006 to 201014. At a recruitment assessment centre, participants contributed to in-depth data collection and banking of biological samples. Biological samples were subsequently used for the generation of various omics data and biomarker measurements. Clinical outcomes for participants can be followed-up through linkage to secondary care data and for ~ 45% of participants primary care data (available data until 31/12 2020). The machine learning models integrated both clinical, metabolomics, proteomics and genetic data from the recruitment assessment centre as well as longitudinal information captured from the EHR data.\n\n## Pre-processing of assessment centre data\n\n### Clinical assessment centre data \nDiverse participant data from the recruitment assessment centre was processed for input into machine learning models to integrate multi-modal signals in the models (Sup File 3). This included data on socio-demographics (including Townsend deprivation index), lifestyle, diet, and physical activity. Additionally, a panel of blood and urine biomarkers were measured at recruitment (Sup File 3) and included as input features. Biomarker data from recruitment was processed to assign outliers outside the 1st and 99th percentiles to the value of the 1st and 99th percentile. Body impedance data reflecting body composition was taken from the first assessment instance and included derived measurement of the fat mass (Kg) to fat-free mass (Kg) ratio across whole body, and specific body areas including trunk area, leg and arms (legs and arms indicated by differences in right and left side of an individual’s body composition).\n\n### Genetic data \nThe imputed genetics data was generated and provided by the UK BioBank and processed using PLINK (v2.00a3LM)65,66. Single nucleotide polymorphisms (SNPs) were subsequently removed if they had a minor allele frequency (MAF) < 1%, a missingness > 1%, an imputation score (INFO) < 0.8 or with a Hardy-Weinberg Equilibrium exact p-value < 0.00001. This resulted in a set of around 9.4M high quality imputed common genetic variants that were used to generate genetic risk scores (GRS).\n\nGenetic information was integrated into the machine learning models through several representations of the genetic information by i) individual SNPs, ii) whole genome polygenic risk score of OA (WGPRS) as well as genetic risk scores for either iii) specific gene-level genetic risk scores (gene-GRS) or iv) pathway-level polygenic risk scores (pathway-PRS).\n\nGenetic risk scores were generated using the software PRSice (v.2.3.3)67 and the weights of variants associated with OA from a recent meta-analysis5 (summary statistics of a sub-analysis excluding the UK Biobank samples).\n\nFor gene-GRS, SNPs within 5kb upstream and 1.5kb downstream of a gene were used for scoring after clumping. Furthermore, analyses were run with and without a linkage disequilibrium proxy (LD proxy): including SNPs in LD with the clumped region, with R^2 > 0.8. The gene regions were defined using GENCODE annotations (V43lift37); only protein-coding genes were considered for analyses.\n\nFor pathway-PRS, SNPs within genes (as described above) belonging to specific gene-sets were aggregated together into a score (with and without LD proxy). The gene-sets used for the pathway-PRS were generated using KEGG pathways obtained via the Molecular Signature Database (MsigDB; v2022.1).\n\nThe default PRSice clumping parameters were used. For WGPRS and gene-GRS/pathway-PRS, no p-value based thresholding was applied to maximise the number of SNPs included in the analyses; however multiple thresholds were tested for WGPRS, with no significant impact on the results (data not shown).\n\nSNPs and genes to be included in the models were guided by using previously identified variants and loci associated with OA risk genes from two recent large GWAS-based studies5,68. Indels were removed from individual genetic variants, resulting in a set of 85 SNPs. Specific gene-GRS features to include were prioritised based on the genes annotated to the GWAS significant loci. This included 77 high effector OA genes identified by Boer *et al*5 and 134 OA genes annotated to genome-wide significant SNPs by McDonald *et al*68. In total, 204 unique genes associated to OA risk were identified, where 193 genes were protein-encoding and prioritised for the list of gene-GRS used. All pathways from KEGG were tested for pathway-GRS (n = 186).\n\n### Metabolomics data \nCirculating metabolite biomarkers from blood EDTA plasma samples were quantified from a subset of UK biobank participants (N = 118,021) using Nightingale’s high-throughput proton NMR metabolomics platform69–71. A total of 249 metabolites were quantified (168 metabolites given in absolute molar concentration units (differs per biomarker, see details: https://research.nightingalehealth.com) and 81 ratios of these) spanning amino acids, (apo-)lipoproteins (incl subclasses), cholesterol, cholesteryl esters, fatty acids, biomarkers of fluid balance, glycolysis related metabolites, inflammation biomarkers, ketone bodies, phosphor- and/or other lipids. Metabolites that were measured by absolute concentrations were normalised by square root. Metabolites given as ratio or percentages were not processed further before including in the machine learning models.\n\n### Proteomics data \nA subset of UK biobank participants (as previously described72) had biomarkers measured from plasma blood samples by Olink Proximity Extension assays across 58,634 samples for 54,308 individuals. The data was filtered to only include individuals with samples obtained from the first assessment centre, samples were processed and no withdrawn consent as per reported by UK Biobank (48,040 samples and 46,673 individuals). In total, 1,472 proteomics markers were measured across four Olink panels (cardiometabolic panel: 369, inflammation: 368, neurology: 367, oncology: 368). The quality of the assay and sample quality was checked by Olink’s built-in quality control. Sample with < 85% of assays not completely passing Olink’s built-in quality control were excluded for analysis. The protein expression was normalised into Normalized Protein eXpression (NPX), which is Olink’s arbitrary unit (Log2 scale). NPX values were compared across individuals and extreme outliers were removed if the mean NPX for an individual was < 0.2% or > 99.8% percentile of the overall cohort mean NPX values. Proteins that were identified by non-normal / bimodal residuals from age, sex, BMI were removed from the analysis. CXCL8, IL6, and TNF were measured across all four Olink assays and an average NPX value was calculated. Furthermore, some samples were assayed twice for replication and for machine learning analyses, an average NPX value was calculated.\n\n## Pre-processing of longitudinal primary and secondary care data (biomarker & medication) during the 5 years pre-index date \nLongitudinal data was captured 5-years prior to OA diagnosis/matched index date from the primary and secondary health care data (Fig. 1 and Sup Fig. 1–2). \n\nPrimary care data was used as a source of longitudinal biomarkers, clinical measurements, and prescription data. Biomarkers and clinical measurements included haematological measurements, liver biomarkers, anthropometric measurements, cardiovascular biomarkers, renal biomarkers, bone & joint biomarkers, lifestyle measurements, hormonal measurements, and diabetes biomarkers (Sup File 4). Where appropriate, data was processed to align units and outliers. Medication for type 2 diabetes, obesity and OA was extracted from prescription data (Sup File 5).\n\nLongitudinal data was captured in yearly snapshots 5 years prior to OA diagnosis. For continuous data, this was represented as the median value across an 11-month period in the year. For medication data, prescriptions were grouped into medication classes and a binary value indicated whether the patient had a prescription for the medication class during the year.\n\nFinally, primary and secondary health care data was used to indicate if OA patients had a diagnosis of posttraumatic OA before onset of their OA diagnosis, as this has been shown to increase individual OA risk73. Diagnoses of post-traumatic OA were identified and annotated if any codes were given ahead of the OA date / control proxy day.\n\n## OA study and validation populations \nOA diagnoses were identified from primary and secondary health care data linked to individual participants (> 18 years old) using read2, read3, ICD-9 and ICD-10 clinical codes (Sup File 1). Further inclusion criteria for the study included filtering of patients with available primary care data in the UK Biobank. An equal number of control participants, who never developed OA and had observational data during the entire study period (e.g., due to death), were identified. Controls were date-matched with the OA diagnosis dates for case patients to enable retrospective capture of longitudinal data five year before OA diagnosis or OA proxy date. Cases and controls were then filtered for those with an OA diagnosis/matched index date after the date of the recruitment assessment centre, and maximum five years between the OA diagnosis and assessment centre, allowing the use of this recruitment data in predictive models to estimate the five-year risk (Fig. 1A).\n\n## Machine learning models \nExtreme Gradient Boosting (XGBoost) models with decision-tree based learners were implemented by R version 4.2.0 using the publicly available R libraries; xgboost (v 1.6.0.1), pROC (v 1.18) and caret (v6.0-93). XGboost models were trained using a nested two-level five-fold case-control stratified cross-validation. Missing values were handled by imputation within each cross-validation fold based on the median value available across cases and controls in the training dataset. Features with > 50% missing data were excluded from analysis. Additionally, near zero variance features were excluded using ‘near0var’ from the caret library. Hyperparameters for the cross-validated models were optimised via a cross-validation grid search, where optimal parameters were selected based on highest cross-validated ROC-AUC in the inner cross-validation fold. The grid optimised for the following parameters eta: (0.05, 0.10, 0.15, 0.20, 0.25,0.30) and nrounds: (50, 100, 200, 300, 500, 700, 1000) with the following other parameters fixed in the XGBoost model; booster: gbtree, max depth: 10, eval_metric: logloss, objective: binary:logistic, subsample = 0.8, sample:method = uniform and min_child_weight = 50. For models where omics data (genomics, metabolomics or proteomics) were integrated the XGBoost model also had colsample_bytree = 0.8. The short depth of each decision tree was set to help guide feature selection and reduce risk of overfitting. The selected hyperparameters were selected for re-training of one model in the outer cross-validation level. The model performance was validated on the outer test set that has been held out from any model training. Model performance was estimated by evaluating classification of true positive (TP), false positive (FP), true negative (TN) and false negative (FN) classifications done by the machine learning model. To account for variance between the five cross-validation sets, both the average and 95% confidence interval (CI) across the five validation datasets were reported. The classification performance is reported by the area under the receiver operating characteristic curve (ROC-AUC), sensitivity (recall, (\\\\(\\\\frac{TP}{TP+FN}\\\\))), positive predictive value (PPV, precision, (\\\\(\\\\frac{TP}{TP+FP}\\\\))), specificity (\\\\(\\\\frac{TN}{TN+FP}\\\\)) and negative predictive value (NPV, \\\\(\\\\frac{TN}{TN+FP}\\\\)). ROC and precision-recall curves were generated using the R library yardstick (v 1.1.0). The robustness and stability of the machine learning models was evaluated across 100 random model initialisation and against 100 random model initialisations with a permuted prediction outcome of OA cases and controls that both accessed impact on predictive performance. Transparent reporting of a multivariate prediction model for individual prognosis or diagnosis (TRIPOD) checklist for prediction model development were followed to ensure clarity and reproducibility of the multivariate prediction model of individual OA risk (Sup File 6).\n\n## Model interpretation \nTo explore how each individual features contribute to the risk prediction of OA, Shapley Additive explanation (SHAP) values were calculated from the XGBoost models using Tree SHAP74. The SHAP values were given as the log-odds of the individual contributions and were visualised using the R libraries SHAPforxgboost (v 0.1.1) and shapviz (v 0.4.1). For global estimation of feature importance across the five outer test datasets, the mean absolute SHAP values were calculated, which quantifies, on average, the magnitude of a feature’s ability to predict individual risk of osteoarthritis.\n\n## Cluster analyses \nTo explore differences in feature importance in the prediction model between subgroups of individuals, clustering was performed on the SHAP values. For this, the Seurat75 (v.4.3.0) implementation of the Louvain clustering algorithm76 was used after reducing the data to 10 dimensions by principal component analysis (PCA). A three-steps approach was used to determine the number of clusters. First, the package chooseR77 was used to perform a subsampling-based approach to generate silhouette scores (as a measure of cluster robustness) for various resolutions (number of clusters). Secondly, the PPV, sensitivity and F1 (a balanced metric evaluating accuracy of case classification, \\\\(\\\\frac{2}{sensitivit{y}^{-1}+PP{V}^{-1}}\\\\)) values of each cluster were calculated, based on the prediction results of the XGBoost model. Finally, these two steps were integrated by looking at the cluster resolutions leading to the best combination of these metrics with the formula: \\\\(cluster score=\\\\frac{weighted mean \\\\left(silhouette scores\\\\right)}{1-weighted median \\\\left(prediction values\\\\right)}\\\\).\n\nAfter manually selecting the optimal resolution parameter to maximise cluster robustness, number of clusters and per-cluster F1 values (resolution = 0.5, n = 14 clusters), each cluster was first characterised by averaging the values of the top 6 predictive features to plot as a heatmap using the ComplexHeatmap78 R package(v.2.13.1). 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Bioinformatics 32, 2847–2849 (2016).\n\n# Supplementary Files\n\n- [SupplFile1OAclinicalcodes.xlsx](https://assets-eu.researchsquare.com/files/rs-3230959/v1/40df3fd08285aebde1f2e68e.xlsx)\n- [SupplFile2missingclinicaldata.xlsx](https://assets-eu.researchsquare.com/files/rs-3230959/v1/c5891e8aea9f9e7885ebde5f.xlsx)\n- [SupplFile3InputFeaturesAC.xlsx](https://assets-eu.researchsquare.com/files/rs-3230959/v1/f9ff8767cf8cf0acf0349beb.xlsx)\n- [SupplFile4BiomarkerReadCodes.xlsx](https://assets-eu.researchsquare.com/files/rs-3230959/v1/e25f343959d28c6cd3fb6b3b.xlsx)\n- [SupplFile5PrimaryMedicationCodes.xlsx](https://assets-eu.researchsquare.com/files/rs-3230959/v1/4502a92d5a879fe9af531cd9.xlsx)\n- [SupplFile6TripodCheclistPredictionModelDevelopment.pdf](https://assets-eu.researchsquare.com/files/rs-3230959/v1/f67b08b9fd193b3fd56da25a.pdf)\n- [OAsupplv27.docx](https://assets-eu.researchsquare.com/files/rs-3230959/v1/e3c023443548fd95fe5cc6a9.docx)"} {"paper_id": "prb37", "title": "Enformer: An encoder-decoder generative model to enhance prediction of disease outcomes using electronic health records", "text": "# Abstract\n\nDeep learning transformer-based models using longitudinal electronic health records (EHRs) have shown a great success in prediction of clinical diseases or outcomes. Pretraining on a large dataset can help such models map the input space better and boost their performance on relevant tasks through finetuning with limited data. In this study, we present Enformer, a generative encoder-decoder model with transformer that was pretrained using a new pretraining objective - predicting all diseases and outcomes of a patient at a future visit from previous visits. Enformer’s encoder-decoder framework, paired with the novel pretraining objective, helped it achieve the new state-of-the-art (SOTA) performance on multiple clinical prediction tasks. Comparing with the previous SOTA model, Enformer improved area under the precision–recall curve (AUPRC) by 2% (p<0.001) for pancreatic cancer onset and by 24% (p<0.001) for intentional self-harm in patients with PTSD. The high performance in predicting intentional self-harm shows the potential of Enformer in building effective clinical intervention systems. Enformer is also generalizable and can be easily finetuned for clinical prediction tasks with limited data.\n\nHealth sciences/Medical research/Experimental models of disease \nHealth sciences/Health care/Disease prevention\n\n# Introduction\n\nThe widespread adoption of electronic health records (EHRs) across US hospitals has led to the development and adoption of numerous data mining and statistical techniques for EHRs. Longitudinal EHRs have been successfully used to predict clinical diseases or outcomes. \n1–3 Early work applied regression and traditional machine learning (ML) based models (e.g., support vectors machines, random forest, and gradient boosting) to predict single disease or outcome. Examples include congestive heart failure, \n4 sepsis mortality, \n5 mechanical ventilation, \n5 septic shock, \n6 type 2 diabetes, \n7 and development of post-traumatic stress disorder (PTSD) \n8 , among others.\n\nWith the availability of large cohorts and computational resources, deep learning based models can outperform traditional ML models \n9–15 . State-of-the-art (SOTA) models in EHR-based predictive modeling achieved this through the pretrain-finetune paradigm - a two-step process where the model is first trained on large-scale longitudinal EHRs to learn the representations of clinical features such as, International Classification of Diseases (ICD) codes (pretrain) and then further trained to adapt to specific tasks e.g., outcome prediction (finetune). Models such as Med-BERT \n12 , BEHRT \n13 , and BRLTM \n14 fall in this category. However, their pretraining objectives were limited in predicting a fraction of ICD codes within each visit. In reality, most patients have multiple diseases or outcomes at once, \n16 many of which are highly correlated (such as obesity, diabetes, and hypertension \n17–19) and thus collectively contribute to the disease or outcome trajectories. Therefore, a novel pretraining strategy, which predicts the complete set of diseases and outcomes within a visit, might improve clinical predictive modeling.\n\nIn this study, we propose Enformer, an innovative denoising sequence to sequence transformer \n20 model that was pretrained on 6.5 million patients’ EHRs to predict complete ICD codes of a visit. Enformer can be further finetuned for single disease or outcome predictions. Unlike previous EHR-based models \n12–15 which rely on the bidirectional (left-to-right and right-to-left) encoder representation from transformers (BERT) framework, \n21 Enformer used a transformer-based encoder-decoder generative framework to predict future ICD codes during pretraining. The unidirectional (left-to-right) decoder in such an encoder-decoder framework is more similar to the use case of future disease or outcome predictions based on history of past diseases or outcomes (past-to-future) compared to the bidirectional encoder-only framework.\n\nAlthough the encoder-decoder framework was originally designed to generate next sentence given previous sentences as context, \n22,23 we repurposed the framework for Enformer to generate the ICD codes of the next visit given previous EHRs (context). Enformer can utilize cross-attention \n20 by identifying relevant ICD codes from previous visits to predict future ICD codes. The decoder then predicts ICD codes one after another by using already predicted diagnostic ICD codes to predict next ICD codes. Furthermore, Enformer includes date of each visit to integrate temporal information, whereas previous transformer-based predictive models only included their sequential order. \n12–15 Specific date of each visit is an important feature in predictive modeling as importance of predictor in a visit can vary over time. \n1,24,25\n\nWe evaluated Enformer for a broad range of disease and outcome predictions. In addition to predictions of ICD codes, we evaluated Enformer on two challenging and clinically important disease and outcome prediction tasks: pancreatic cancer prediction and intentional self-harm prediction among PTSD patients. In summary, our key contributions are as follows:\n\n1. We propose a new pretraining objective that predicts all diseases or outcomes of a future visit using longitudinal information from the previous visits. Such pretraining objective can leverage the clinical relations among diseases and outcomes.\n2. This is the first study that explores a generative encoder-decoder framework to predict patients’ ICD codes using their longitudinal EHRs. Our encoder-decoder framework outperformed the encoder-based models in part due to the decoder self-attention and cross-attention mechanisms. Enformer outperformed SOTA BERT models on both common and uncommon ICD code predictions. In particular, the improvements for uncommon were substantial.\n3. Enformer achieved a positive predictive value (PPV) of 8.45% for prediction of intentional self-harm among the top 10% PTSD patients at high predicted risk. A recent study has shown that a practical suicide prevention tool must achieve above 1.7% PPV to minimize the resource cost and intrusion directed at patients who will never attempt self-harm. \n26 This shows the potential of deploying Enformer for clinical screening and interventions.\n4. We validated the generalizability of Enformer using both internal and external datasets. Internally, we evaluated Enformer on “never-seen” in-domain EHR data from VHA facilities. Externally, we evaluated Enformer on out-of-domain data from a non-VHA hospital. Our results demonstrated a strong transfer learning \n27 capability of Enformer, which can greatly benefit hospitals with limited data and computing resources.\n\n# Results\n\n## Data\n\nOur pretraining cohort comprises 6,475,218 patients who received care from more than 1,200 health care facilities of the US Veterans Health Administrations (VHA) from 1/1/2016 to 12/31/2019. To evaluate pretrained models, we created two disease/outcome agnostic prediction (DOAP) datasets – one for common and one for uncommon diseases/outcomes. We selected 10 ICD-10 codes with the highest prevalence (prevalence ratio > 2%) in our pretraining cohort for our common disease/outcome DOAP dataset. As for the set of uncommon diseases/outcomes, we followed the FDA guidelines28 to randomly select 10 ICD-10 codes with a prevalence ratio ranging from 0.04% to 0.05% in our pretraining cohort. The lists of common and uncommon diseases/outcomes are shown in Table 1.\n\nTo evaluate finetuned models for single disease and outcome predictions with low prevalence ratio, we created two EHR datasets for two important prediction tasks: pancreatic cancer (single disease) and intentional self-harm among patients with PTSD (single outcome). Early screening, early diagnosis and early treatment of pancreatic cancer are critical for this deadly disease.29,30 Med-BERT12 has been used to predict pancreatic cancer. Intentional self-harm is common among the US military Veterans with PTSD.31 The detailed pretraining and finetuning cohort definitions are presented in Methods section. We compare these cohorts in Supplementary Table 1.\n\nTo assess the generalizability, we evaluated Enformer on both “unseen” in-domain EHR data and out-of-domain non-VHA EHR data. The unseen in-domain EHR data were collected from VHA facilities not included in the pretraining cohort and we created a dataset for the intentional self-harm prediction task among PTSD patients. As the out-of-domain non-VHA EHR data, we used the MIMIC-IV dataset32 to build a non-VHA DOAP dataset. The MIMIC-IV dataset includes intensive care unit patients admitted to the Beth Israel Deaconess Medical Center in Boston, Massachusetts. Since the dataset contains information from 2008 to 2019 but the implementation of ICD-10 started from October 2015, we only selected patients with the ICD-10 records to match our implementation for the cohorts from VHA, resulting in a dataset of 29,482 patients.\n\n## Longitudinal EHRs\n\nAs shown in Figure 1, Enformer takes longitudinal EHRs as input. To compare Enformer with the previous SOTA EHR-based models using BERT,12,14 we included demographic information and ICD-10 codes as predictors. Demographic information includes gender, age, race, and marital status. The attributes (e.g., male) of each category (e.g., gender) were appended as individual predictors. Following previous work,12 we grouped ICD codes at visit level. Within a visit, we ordered ICD codes from high to low priority, as assigned by health care providers, where the primary diagnosis is typically given the highest priority, followed by the secondary diagnosis and so on.\n\nMultiple visits of each patient formed a time-stamped (by date of visit) input of a sequence of ICD-10 code groups (Figure 2). We used multi-level embeddings.12 Embeddings are trainable fixed-dimensional vectors that were used to represent predictors in a continuous vector space and were learned during the pretraining process (details in the next section). We represented each visit in an input sequence using a visit embedding and each ICD code using a code embedding. To embed the specific date of each visit, we applied sinusoidal position embedding20 to the numerical format of date. Finally, each input embedding was constructed by summing up the corresponding code embedding, visit embedding, and date embedding (Figure 2a).\n\n## Pretrain-Finetune Paradigm\n\nWith longitudinal EHRs as input, we first pretrained models on the pretraining cohort of 6,475,218 patients and then finetuned the model for single disease or outcome prediction, as shown in Figure 3. During the pretraining, the model was trained to recover the original longitudinal EHRs from corrupted (masked) longitudinal EHRs.\n\nPrevious EHR-based BERT models corrupted longitudinal EHRs by randomly sampling 25% ICD codes and replacing them with mask (code masking).12–14 Enformer, on the other hand, masked all ICD codes in a single visit (visit masking). A comparative example is illustrated in Figure 2b. In other words, Enformer was pretrained to predict the complete set of ICD codes of a patient’s future visit, given demographic information and longitudinal ICD codes up to the current visit.\n\n## Enformer Architecture\n\nEnformer uses an encoder–decoder transformer architecture.22,23 The encoder processes the input embeddings and generates a set of hidden representations for each predictor. Unlike the encoder-only transformer architecture used by existing EHR-based BERT models,12–14 Enformer performs cross-attention over the hidden representations from the encoder and assigns an attention weight for each representation. These weighted representations are then fed to the decoder, which generates ICD codes of the future visit as illustrated in Figure 3. The decoder generates ICD codes following the sequential order of code priority within a visit. In other words, it first generates primary diagnosis, and then generates secondary diagnosis based on primary diagnosis. This step is repeated until all diagnoses of a future visit are completed. Our results showed that the Enformer architecture outperformed the encoder-only architecture.\n\n## Evaluation Metrics\n\nWe used Jaccard similarity score to measure model performance on the DOAP task. Jaccard similarity score measures the similarity between ground truth and model predictions as the size of the intersection of ground truth codes and the prediction codes divided by the size of their union. A higher score indicates better model performance. We also reported positive predictive value (PPV or precision), area under the receiver operating characteristic curve (AUROC), and area under the precision recall curve (AUPRC) to measure models’ performance on single disease or outcome predictions. PPV is the fraction of true positives from all predicted positives. AUROC is the area under sensitivity and false positive rate curve. Sensitivity (or recall) is the number of true positives divided by the number of ground truth positives. False positive rate is the number of false positives divided by total number of negatives. AUPRC is the area under PPV and sensitivity curve, and it has shown to be an effective measure for highly imbalanced binary classification problems, which include self-harm prediction.33,34\n\nWe compared Enformer with four strong baseline models: copy, logistic regression, long short-term memory (LSTM),35 and BERT21 pretrained on VHA cohort. The copy baseline is essentially making predictions by simply copying the ICD codes from the previous visit. Although simple, this is a strong baseline since it is well known that physicians copy and paste note content.36,37\n\n## Pretraining Evaluation: Disease or Outcome Agnostic Prediction\n\nDOAP is the task of predicting the ICD codes of a patient’s future visit based on patient’s demographic information and longitudinal ICD codes up to the current visit. Supplementary Table 2 showed that pretraining substantially improved predictions of both common and uncommon diseases/outcomes. Compared to the copy baseline, Enformer improved the Jaccard similarity scores for recurrent common diseases/outcomes by 64% (average 30.41, from 45.49 to 74.85) and for uncommon diseases/outcomes by 83% (average 22.04, from 26.54 to 48.58). Compared to BERT, Enformer also improved performance by 37% in Jaccard similarity in all prediction subtasks, regardless of disease/outcome category (common or uncommon) and occurrence type (new or recurrent). We found a 15% improvement in Jaccard similarity score on common disease/outcome predictions and 45% improvement on uncommon disease/outcome predictions.\n\nOur Enformer contains three unique components compared to previous medical BERT-based models: 1) visit masking, 2) encoder-decoder architecture, and 3) date embedding. We performed ablation analysis to evaluate the effectiveness of each component. First, we compared an encoder-decoder model that uses visit masking, i.e., masking all ICD codes of a visit, to another encoder-decoder model that uses code masking, i.e., masking a randomly selected fragment of ICD codes of a visit. Our findings revealed that the visit masking performed better (showing an average improvement of 23% in Jaccard similarity score) compared to code masking for all diseases/outcomes tested as shown in Supplementary Table 3. These results demonstrated that pretraining for prediction of all diseases and outcomes outperform traditional pretraining objectives.\n\nNext, we compared encoder-decoder model with encoder-only model (BERT) on DOAP. Our findings showed that the encoder-decoder model outperformed the encoder-only model (with an average improvement of 9% in Jaccard similarity score) across all diseases/outcomes tested (Supplementary Table 2 and 3).\n\nFinally, we conducted an experiment by excluding date embedding from the implementation of Enformer. Data embedding allows Enformer to capture the temporal information of prior visits. Our results indicated that Enformer with date embedding exhibits a moderate improvement (with an average increase of 1% in Jaccard similarity score) than Enformer without date embedding across most diseases/outcomes (Supplementary Table 3).\n\n## Finetuning Evaluation: Single Disease or Outcome Prediction\n\n### Pancreatic Cancer\n\nResults of pancreatic cancer onset prediction are shown in Table 2. Enformer achieved AUPRC of 82.73 (95% CI: 81.81, 83.65), outperforming both the logistic regression model (63.81; 95% CI: 61.47, 66.15, p<0.001), LSTM (78.46; 95% CI: 77.60, 79.32, p<0.001) and BERT (81.11; 95% CI: 80.53, 81.69, P=0.01).\n\n### Intentional Self-Harm in Patients with PTSD\n\nThis task is challenging because of its low prevalence (1.9%). As shown in Table 3, AUPRC of Enformer was 16.38 (95% CI, 15.25, 17.52), outperforming BERT (13.17; 95% CI: 11.72, 14.61), LSTM (8.32; 95% CI: 7.02, 9.61), and logistic regression (2.8; 95% CI: 0.49, 5.13) by 24.3%, 55.4%, 96.9%, and 482.9% respectively. We also calculated sensitivity and PPV for a variety of thresholds. As shown in Supplementary Table 4, The PPV of Enformer ranges from 3.11 to 8.45 for 10% to 60% threshold.\n\n#### Subgroup analyses among different demographics:\n\nThe results of the subgroup analyses are shown in Supplementary Table 5. AUPRC was consistent among different genders, ages, races, and marital status. For example, the AUPRC of patients who were more than 80-year-old (4.86% of the cohort) was 17.97 (95% CI, 16.43, 19.51), which was not statistically different from the AUPRC of patients whose ages range from 30 to 39 (19.58% of the cohort): 16.29 (95% CI, 14.41, 18.17).\n\n#### Effect of historical EHR length on performance:\n\nTo examine the impact of how patients’ prior history impacts model predictions, we conducted two experiments - \"self-harm with short history\" (included only the 5 most recent visits) and \"self-harm\" included all visits). As shown in Table 3, The AUPRC of Enformer using only the 5 prior visits was 13.82. Using all visits, the AUPRC improved by 18% to 16.38.\n\n## Generalizability Evaluation\n\nWe validated the generalizability of Enformer both internally and externally. Out of 1,239 VHA health care facilities, we found that EHR data from 121 facilities were not included in the pretraining cohort. We created an internal generalizability evaluation dataset using this subset of EHR data for the intentional self-harm prediction task among PTSD patients. Upon evaluating Enformer on this dataset, our results showed no statistical difference in AUPRC between data from unseen facilities (1st bar on the left of Supplementary Figure 1) and data from facilities where at least some of the data were included in the pretraining cohort (other bars of Supplementary Figure 1).\n\nTo evaluate Enformer’s generalizability on the external dataset, we further finetuned the pretrained Enformer and BERT on the training set of a non-VHA DOAP dataset and evaluated them on the testing set. Enformer outperformed BERT by 8% with a Jaccard similarity score of 24.35, whereas BERT obtained a score of 22.51.\n\n# Discussion\n\nIn this study we introduced Enformer, a novel generative deep neural network model for the prediction of diseases and outcomes using patients’ longitudinal EHRs. By first pretraining Enformer on a large collection of EHRs (255 million visits from 6.5 million patients between 2016 and 2019) and then finetuning for specific clinical applications, we found that Enformer outperformed existing SOTA models on a wide range of disease or outcome predictions. The performance gain was substantial on intentional self-harm prediction among PTSD patients. As shown in Table 3, Enformer was the best-performing model and outperformed BERT, LSTM, and logistic regression models by 24.3%, 96.9%, and 482.9%, respectively. The aforementioned results were not surprising, as deep-learning-based models are known to capture the salient information of EHR data to create powerful feature representations.38 In addition, pretraining on large data and using the encoder-decoder framework have both been shown to be SOTA strategies for sequence-to-sequence applications.22\n\nEnformer outperformed BERT for prediction of both single and multiple diseases/outcomes, as shown in Tables 2, 3, and Supplementary Table 2. In contrast to BERT, Enformer learned the representation of each clinical variable by predicting the complete diseases and outcomes with the help of cross-attention and decoder self-attention. Cross-attention allowed Enformer to selectively focus on sections of past visit ICD codes that were most relevant to predicting each ICD code in the future visit, and the decoder self-attention helped Enformer in predicting complete diseases and outcomes by leveraging already predicted primary diagnostic ICD codes to predict secondary codes that are less common. Thus, the performance gains were the highest among uncommon disease predictions. As shown in Table 2, compared with the BERT model, Enformer improved the Jaccard similarity score by an average of 15% in predicting 10 common diseases, and by an average of 45% in predicting 10 uncommon diseases. Enformer also substantially improved prediction for intentional self-harm prediction (AUPRC from 13.17 to 16.38, p<0.001) and pancreatic cancer prediction (AUPRC from 81.11 to 82.73, p<0.001).\n\nPretraining played a key role in improving the performance of our deep-learning-based models. To demonstrate, we chose intentional self-harm prediction and compared the performance between a BERT model pretrained on our pretraining cohort (as described in the Data section) and a BERT model with no pretraining (parameters were randomly initialized before fine-tuning). Pretrained BERT substantially outperformed the non-pretrained BERT (19.51% higher AUPRC and 29.55% higher PPV), as shown in Table 3. In particular, pretraining helps improve the latent representations of EHR data compared to non-pretrained models. This helped improve the probability distribution of candidate diseases or outcomes. As shown in Figure 3, after pretraining on a large EHR cohort, the probability distribution for the next visit ICD code changed from a random distribution to a learned representation of clinically relevant diseases or outcomes. While a pretrained model can capture the probability distribution at a large cohort level, finetuning it further can improve the performance for a specific application.\n\nAttention-based models benefit from longitudinal EHRs with long histories (approximately 10 prior visits). As shown in Table 3, of the attention-based models (Enformer and BERT) finetuned on more than 5 visits, the AUPRC scores improved by 18% and 27%, respectively, in comparison with models finetuned on only 5 most recent visits. However, with the same experimental setup, the AUPRC scores of non-attention-based models such as LSTM and logistic regression decreased by 8% and 58%, respectively, when finetuned on more than 5 prior visits (on average 10) compared with the models finetuned on only the 5 most recent visits. These findings were consistent with previous research,39 which showed that LSTM, although good at mitigating the vanishing gradient challenge of RNN, remains suboptimal with long-time dependencies.\n\nOur work is also related to predictive model studies focused on intentional self-harm.40–44 Typically, these approaches sample thousands of patients and use probability tables, decision trees, and logistic regression to predict intentional self-harm. PPV plays a crucial role here in estimating the potential benefit of any intensive case management intervention, if one were to be implemented based on any such approach. PPV indicates the percentage of patients receiving an intervention who would otherwise attempt self-harm. Hartl et al.42 predicted intentional self-harm among PTSD patients (prevalence ratio 5%, PPV 0%). Simon et al.44 integrated EHR data and questionnaires for 2,960,929 patients to predict suicide attempts (prevalence ratio 1%) within 90 days of a mental health visit. The most successful model demonstrated a PPV of 5%. Enformer, on the other hand, achieved a PPV of 8.45% at 10% threshold for prediction of intentional self-harm among PTSD patients, which substantially outperformed the baselines (Table 3). In other words, out of the 100 highest-predicted-risk patients from 1,000 previously diagnosed PTSD patients, almost 8 patients would attempt intentional self-harm for the first time before the next visit. In comparison, for logistic regression the PPV at the 10% threshold was 2.17%. A practical suicide prevention tool must have a relatively high PPV to minimize the resource cost and intrusion directed at patients who will never attempt self-harm.45 Therefore, Enformer may be a reliable and feasible option for designing an effective suicide prevention system.\n\nIn conclusion, our results have multiple clinical implications. First, existing predictive models tend to focus on single diseases. Yet the focus in clinical care, particularly in older people, is often on managing comorbidities.16 A predictive model that can predict multiple diseases or outcomes may be useful in designing complex treatment plans. Second, a disease-specific approach could require building hundreds of different predictive models, an inefficient and costly use of resources whereas Enformer’s unique pretraining objective enables it to predict all diseases and outcomes of a visit, immediately after the pretraining. Third, Enformer outperformed existing SOTA predictive models with a substantial performance gain, especially for uncommon disease/outcome predictions. Thus, our approach could assist in the development of screening algorithms to detect uncommon conditions. Fourth, Enformer can be easily generalized on an out-of-domain dataset with a significantly smaller training data. Enformer’s strong transfer learning capability makes it a good fit for hospital settings with limited data and computing resources.\n\nDespite the merits of this study, there are several limitations that provide opportunities for future improvements. First, we followed previous work on model pretraining and included only diagnostic ICD codes and demographic information.12 However, other information such as procedure codes, medications, lab results, and phenotypical information extracted from notes can be added to further improve the performance.46 Second, our prediction of single disease was limited to pancreatic cancer and single outcome was limited to intentional self-harm with PTSD. Future works would expand the set of diseases and outcomes.\n\n# Methods\n\n## Cohort and Use Case Definitions\n\n**VHA Cohort**: Using the Veterans Health Administrations (VHA) Clinical Data Warehouse (CDW), we first identified a total of 8,308,742 patients who received care from more than 1,200 health care facilities of the US VHA from 1/1/2016 to 12/31/2019. For inclusion, we required each patient to have at least two visits: one outcome visit and at least one prior visit to be used for prediction of the outcome. This resulted in a total of 6,829,064 patients.\n\n**Pretraining and Finetuning Cohorts**: Following the standard 95-5 split12,21, we randomly took 95% of the patients (6,475,218) to create our pretraining cohort and used the remaining 5% (353,846) to create other datasets to finetune for DOAP and single disease or outcome predictions. The detailed patient cohort selections and diseases or outcomes for this study are shown in Figure 2 in the Supplement. The study protocol was approved by the Institutional Review Board at the VA Bedford Healthcare System.\n\nWe identified two use cases to evaluate Enformer.\n\n**Pancreatic Cancer**: Although pancreatic cancer is relatively uncommon, it is deadly, projecting to become the second leading cause of cancer-related mortality by 203029. Since effective screening is not available for pancreatic cancer, most patients can seek medical attention only after being diagnosed with locally advanced or metastatic cancer. Therefore, accurate prediction of pancreatic cancer can help early detection of pancreatic cancer. Previous research12 has evaluated BERT for pancreatic cancer prediction. Following the same criteria in a previous study12, we defined pancreatic cancer with the first 3 digit ICD-10 codes as C25. 10,287 patients of 45 years or older with no report of any other cancer disease before their first pancreatic cancer diagnosis were included as cases, and 11,522 patients of 45 years or older without any cancer diagnosis were selected as controls.\n\n**Prediction of intentional self-harm**: PTSD is considered as a hallmark injury of US Post-9/11 Veterans, with a prevalence estimated to be up to 23%47. Individuals with PTSD also have co-occurring physical health (e.g., chronic pain48), mental health (e.g., depression and anxiety49,50), and behavioral conditions (e.g., substance use disorder51,52). People with PTSD have 5.3-13 times the rate of suicide than people without PTSD53. Hence, we also evaluated Enformer for prediction of intentional self-harm for patients with PTSD. Out of 70,967 the patients who had been diagnosed with PTSD from 353,846 patients not in the pretraining cohort, 1,342 patients who would attempt self-harm for the first-time (from VHA CDW and Suicide Prevention Applications Network) were collected as cases. Following previous research that used the ICD-9 codes for intentional self-harm54, we converted those ICD-9 into ICD-10 and defined intentional self-harm using ICD-10 codes as in Supplementary Table 6. Another 281 patients were considered as controls who were diagnosed with PTSD but would not attempt self-harm in six months after their last visit. The observed self-harm rate was 1.9% among PTSD patients. Further details of the cohort definition are available in Supplementary Figure 3. All inpatient and outpatient ICD codes were included in our data.\n\n## Implementation Details\n\nExperiments were conducted using Python version 3.8 and Transformer library version 4.16.2. For pretraining, we tasked Enformer to predict the next visit ICD codes recursively. Specifically, for each patient’s input sequence, we used the first visit to predict the second visit, and then used the first two visits to predict the third visit, and so on. This process was repeated until the last visit as recorded in the input sequence was predicted. ICD codes were ordered by their priorities within a visit. We set the maximum sequence length (number of ICD codes) to be 512. To prevent the model from simply memorizing the pretraining data, we randomly drop 15% of visits from each input during pretraining. Other hyperparameters include a warmup ratio of 0.1, a learning rate of 1e−3, a dropout rate of 0.1, and an L2 weight decay of 1e−3 with fp16. To make a fair comparison, we pretrained the baseline BERT model on the same pretraining cohort, instead of using existing models pretrained on other cohorts. Other hyperparameters were the same as Enformer’s. We used 4 Nvidia Tesla P40 GPU of 22 GB graphics memory capacity and trained each model for 6 days with more than 280k steps and batch size of 48.\n\nDuring finetuning, we added a task-specific classifier layer (a linear layer) on top of Enformer and BERT to predict disease or outcome as a binary classification task. For a fair comparison with other medical BERT models12–14, Enformer used 6 layers in both encoder and decoder modules to best match the amount of parameters. All models were finetuned with 5 random seeds and statistical tests were carried out among these models. To ensure a fair comparison, the same feature transformation, L2 regularization, and hyperparameter tuning strategies, were used to finetune Enformer and all baseline models. For each outcome prediction, we built training, validation, and test datasets by the ratio of 7:1:2. One sided student's t-test was used to determine if Enformer outperforms baseline models. All finetuning experiments were conducted with Nvidia Tesla P40 GPU, and each single disease or outcome prediction was finetuned within 12 hours.\n\n# References\n\n1. Kessler RC, Bauer MS, Bishop TM, et al. Using Administrative Data to Predict Suicide After Psychiatric Hospitalization in the Veterans Health Administration System. *Front Psychiatry*. 2020;11:390. doi:10.3389/fpsyt.2020.00390\n2. Zhao W, Jiang W, Qiu X. Deep learning for COVID-19 detection based on CT images. *Sci Rep*. 2021;11.\n3. Goh KH, Wang L, Yeow AYK, et al. Artificial intelligence in sepsis early prediction and diagnosis using unstructured data in healthcare. *Nat Commun*. 2021;12.\n4. Choi E, Bahadori MT, Sun J, Kulas J, Schuetz A, Stewart W. RETAIN: An Interpretable Predictive Model for Healthcare using Reverse Time Attention Mechanism. In: *Advances in Neural Information Processing Systems*. ; 2016:3504-3512. 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Published online 2020.\n33. Saito T, Rehmsmeier M. The Precision-Recall Plot Is More Informative than the ROC Plot When Evaluating Binary Classifiers on Imbalanced Datasets. *PLoS ONE*. 2015;10.\n34. Walsh CG, Ribeiro JD, Franklin JC. Predicting Risk of Suicide Attempts Over Time Through Machine Learning. *Clin Psychol Sci*. 2017;5(3):457-469. doi:10.1177/2167702617691560\n35. Hochreiter S, Schmidhuber J. Long Short-Term Memory. *Neural Comput*. 1997;9(8):1735-1780. doi:10.1162/neco.1997.9.8.1735\n36. Tang KL, Lucyk K, Quan H. Coder perspectives on physician-related barriers to producing high-quality administrative data: a qualitative study. *CMAJ Open*. 2017;5 3:E617-E622.\n37. Wang MD, Khanna RR, Najafi N. Characterizing the Source of Text in Electronic Health Record Progress Notes. *JAMA Intern Med*. 2017;177:1212-1213.\n38. Miotto R, Li L, Kidd BA, Dudley JT. Deep Patient: An Unsupervised Representation to Predict the Future of Patients from the Electronic Health Records. *Sci Rep*. 2016;6. doi:10.1038/srep26094\n39. Pascanu R, Mikolov T, Bengio Y. On the difficulty of training recurrent neural networks. In: *International Conference on Machine Learning*. ; 2013:1310-1318. http://www.jmlr.org/proceedings/papers/v28/pascanu13.pdf\n40. Tsui FR, Shi L, Ruiz VM, et al. Natural language processing and machine learning of electronic health records for prediction of first-time suicide attempts. *JAMIA Open*. 2021;4.\n41. Galfalvy HC, Oquendo MA, Mann JJ. Evaluation of clinical prognostic models for suicide attempts after a major depressive episode. *Acta Psychiatr Scand*. 2008;117.\n42. Hartl TL, Rosen C, Drescher K, Lee TT, Gusman F. Predicting High-Risk Behaviors in Veterans With Posttraumatic Stress Disorder. *J Nerv Ment Dis*. 2005;193(7). https://journals.lww.com/jonmd/Fulltext/2005/07000/Predicting_High_Risk_Behaviors_in_Veterans_With.6.aspx\n43. Nock MK, Millner AJ, Joiner TE, et al. Risk Factors for the Transition from Suicide Ideation to Suicide Attempt: Results from the Army Study to Assess Risk and Resilience in Servicemembers (Army STARRS). *J Abnorm Psychol*. 2018;127:139-149.\n44. Simon GE, Johnson E, Lawrence JM, et al. Predicting Suicide Attempts and Suicide Deaths Following Outpatient Visits Using Electronic Health Records. *Am J Psychiatry*. 2018;175(10):951-960. doi:10.1176/appi.ajp.2018.17101167\n45. Large M, Myles N, Myles H, et al. Suicide risk assessment among psychiatric inpatients: a systematic review and meta-analysis of high-risk categories. *Psychol Med*. 2017;48:1119-1127.\n46. Rongali S, Rose AJ, McManus DD, et al. Learning Latent Space Representations to Predict Patient Outcomes: Model Development and Validation. *J Med Internet Res*. 2020;22(3):e16374. doi:10.2196/16374\n47. Fulton JJ, Calhoun PS, Wagner HR, et al. The prevalence of posttraumatic stress disorder in Operation Enduring Freedom/Operation Iraqi Freedom (OEF/OIF) Veterans: a meta-analysis. *J Anxiety Disord*. 2015;31:98-107. doi:10.1016/j.janxdis.2015.02.003\n48. Seal KH, Bertenthal D, Barnes DE, et al. Association of Traumatic Brain Injury With Chronic Pain in Iraq and Afghanistan Veterans: Effect of Comorbid Mental Health Conditions. *Arch Phys Med Rehabil*. 2017;98(8):1636-1645. doi:10.1016/j.apmr.2017.03.026\n49. Pugh MJ, Swan AA, Carlson KF, et al. Traumatic Brain Injury Severity, Comorbidity, Social Support, Family Functioning, and Community Reintegration Among Veterans of the Afghanistan and Iraq Wars. *Arch Phys Med Rehabil*. 2018;99(2S):S40-S49. doi:10.1016/j.apmr.2017.05.021\n50. Dismuke-Greer CE, Gebregziabher M, Byers AL, et al. Comorbid TBI-depression costs in veterans: a chronic effect of neurotrauma consortium (CENC) study. *Brain Inj*. Published online November 7, 2018:1-7. doi:10.1080/02699052.2018.1542508\n51. Greer N, Ackland P, Sayer N, et al. *Relationship of Deployment-Related Mild Traumatic Brain Injury to Posttraumatic Stress Disorder, Depressive Disorders, Substance Use Disorders, Suicidal Ideation, and Anxiety Disorders: A Systematic Review*. Department of Veterans Affairs (US); 2019. Accessed January 28, 2020. http://www.ncbi.nlm.nih.gov/books/NBK541421/\n52. McHugo GJ, Krassenbaum S, Donley S, Corrigan JD, Bogner J, Drake RE. The prevalence of traumatic brain injury among people with co-occurring mental health and substance use disorders. *J Head Trauma Rehabil*. 2017;32(3):E65-E74.\n53. Gradus J. PTSD and Death from Suicide. *Natl Cent Posttraumatic Stress Disord*. 2017;28(4):1050-1835.\n54. Patrick AR, Miller M, Barber CW, Wang PS, Canning CF, Schneeweiss S. Identification of Hospitalizations for Intentional Self-Harm when E-Codes are Incompletely Recorded. *Pharmacoepidemiol Drug Saf*. 2010;19(12):1263-1275. doi:10.1002/pds.2037\n\n# Tables\n\n**Table 1.** Disease or outcome definitions in this study.\n\n[IMAGE_TABLES_1]\n\n**Table 2.** Performance of models for pancreatic cancer prediction. Result is calculated from best hyperparameters with 10 randomized seeds each.\n\n| | | AUROC | AUPRC |\n|---|---|---|---|\n| | | Mean (95% CI) | Mean (95% CI) |\n| Without Pretraining | Logistic regression | 77.71 (75.03-80.39) | 63.81 (61.47-66.15) |\n| | LSTM | 81.34 (80.88-81.80) | 78.46 (77.60-79.32) |\n| | BERT without pretraining | 81.35 (80.90-81.80) | 78.65(77.87-79.43) |\n| With Pretraining | BERT | 83.42 (82.98-83.86) | 81.11 (80.53-81.69) |\n| | Enformer (ours) | 85.35 (83.93-86.77) | 82.73 (81.81-83.65) |\n\n**Table 3.** Performance (and standard deviation) of predictive models for intentional self-harm. Result is calculated from best hyperparameters with 10 randomized seeds each. \"Self-Harm w/ Full History\" refers to cases where the prediction is based on the original EHR (mean: 10.1 visits, st.dev.: 3.3 visits) prior to predicting intentional self-harm. \"Self-Harm w/ Short History\" includes only the 5 most recent visits.\n\n| | Models | Self-Harm w/ Short History | | | Self-Harm w/ Full History | | |\n|---|---|---|---|---|---|---|---|\n| | | AUPRC | PPV | F1 | AUPRC | PPV | F1 |\n| | | % | % | % | % | % | % |\n| Without Pretraining | Logistic regression | 6.89 | 3.37 | 6.28 | 2.81 | 2.96 | 5.67 |\n| | | (1.57) | (0.04) | (0.07) | (1.16) | (0.87) | (1.61) |\n| | LSTM | 9.14 | 3.92 | 7.30 | 8.32 | 3.71 | 6.88 |\n| | | (0.56) | (0.25) | (0.43) | (0.65) | (0.13) | (0.29) |\n| | BERT without pretraining | 9.42 | 5.41 | 8.99 | 11.02 | 6.1 | 9.28 |\n| | | (0.62) | (0.46) | (0.87) | (0.75) | (1.29) | (0.77) |\n| With Pretraining | BERT | 10.31 | 5.78 | 9.49 | 13.17 | 7.14 | 10.47 |\n| | | (0.89) | (1.50) | (1.78) | (0.72) | (1.11) | (0.99) |\n| | Enformer | 13.82 | 6.11 | 10.83 | 16.38 | 8.67 | 14.42 |\n| | | (0.79) | (0.71) | (0.98) | (0.57) | (0.21) | (0.43) |\n\n# Supplementary Files\n\n- [Supplement.docx](https://assets-eu.researchsquare.com/files/rs-2922823/v1/f744650e08915fa66e0205f1.docx)"} {"paper_id": "prb38", "title": "", "text": "Autocharacterization: Automated and Scalable Semiconductor Property Estimation from High-throughput Experiments using Computer Vision\n\nAlexander Siemenn\nasiemenn@mit.edu\n\nMassachusetts Institute of Technology https://orcid.org/0000-0001-8841-7887\nEunice Aissi\nMassachusetts Institute of Technology\nFang Sheng\nMassachusetts Institute of Technology\nArmi Tiihonen\nMassachusetts Institute of Technology\nHamide Kavak\nMassachusetts Institute of Technology https://orcid.org/0000-0002-9810-2640\nBasita Das\nMassachusetts Institute of Technology\nTonio Buonassisi\nMassachusetts Institute of Technology\n\nArticle\n\nKeywords: high-throughput laboratory automation, scalable computer vision segmentation, perovskite composition engineering, optical band gap, stability measurement\n\nPosted Date: October 31st, 2023\n\nDOI: https://doi.org/10.21203/rs.3.rs-3352833/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: Yes there is potential Competing Interest. Although our laboratory has IP filed covering photovoltaic technologies and materials informatics broadly, we do not envision a direct COI\nwith this study, the content of which is open-sourced. T.B. owns equity in Xinterra Pte Ltd, which applies machine learning to accelerate novel materials development.\n\nVersion of Record: A version of this preprint was published at Nature Communications on June 11th, 2024. See the published version at https://doi.org/10.1038/s41467-024-48768-2.\nAutocharacterization: Automated and Scalable Semiconductor Property Estimation from High-throughput Experiments using Computer Vision\n\nAlexander E. Siemenn1*†, Eunice Aissi1*†, Fang Sheng1, Armi Tiihonen1,2, Hamide Kavak1,3, Basita Das1, Tonio Buonassisi1\n\n1Department of Mechanical Engineering, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, 02139, Massachusetts, USA.\n2Department of Applied Physics, Aalto University, Otakaari 24, Espoo, 02150, Finland.\n3Department of Physics, Cukurova University, Adana, 01330, Turkiye.\n\n*Corresponding author(s). E-mail(s): asiemenn@mit.edu; eunicea@mit.edu;\nContributing authors: shengf22@mit.edu; armi.tiihonen@gmail.com; hkavak@mit.edu; dasb@mit.edu; buonassisi@mit.edu;\n†These authors contributed equally to this work.\n\nAbstract\nHigh-throughput materials synthesis methods have risen in popularity due to their potential to accelerate the design and discovery of novel functional materials, such as solution-processed semiconductors. After synthesis, key material properties must be measured and characterized to validate discovery and provide feedback to optimization cycles. However, with the boom in development of high-throughput synthesis tools that champion production rates up to \\(10^4\\) samples per hour with flexible form factors, most sample characterization methods are either slow (conventional rates of \\(10^1\\) samples per hour, approximately 1000x slower) or rigid (\\emph{e.g.}, designed for standard-size microplates), resulting in a bottleneck that impedes the materials-design process. To overcome this challenge,\nwe propose a set of automated material property characterization (autocharacterization) tools that leverage the adaptive, parallelizable, and scalable nature of computer vision to accelerate the throughput of characterization by 85x compared to the non-automated workflow. We demonstrate a generalizable composition mapping tool for high-throughput synthesized binary material systems as well as two scalable autocharacterization algorithms that (1) autonomously compute the band gap of 200 unique compositions in 6 minutes and (2) autonomously compute the degree of degradation in 200 unique compositions in 20 minutes, generating ultra-high compositional resolution trends of band gap and stability. We demonstrate that the developed band gap and degradation detection autocharacterization methods achieve 98.5% accuracy and 96.9% accuracy, respectively, on the FA1−xMAxPbI3, \\( 0 \\leq x \\leq 1 \\) perovskite semiconductor system.\n\nKeywords: high-throughput laboratory automation, scalable computer vision segmentation, perovskite composition engineering, optical band gap, stability measurement\n\nIntroduction\n\nTo discover commercially relevant semiconductor materials, *e.g.*, for solar applications [1–3], vast compositional search spaces must be rapidly synthesized and characterized, *e.g.*, for band gap [4–6] and stability [7, 8]. Recently, several new methods have been developed for high-throughput (HT) combinatorial synthesis across a wide range of material domains including perovskites, nanomaterials, porous media, aerosols, and lithium-ion batteries [9–18]. Although these HT manufacturing methods have shown great progress in driving the rapid screening of large material search spaces in an automated fashion, much of the materials characterization process is still hindered due to its manual nature [14, 19] or rigid microplate-based form factors [9, 10, 20, 21]. This results in a significant bottleneck in which the rate of synthesis can achieve throughputs over 800x faster than those of characterization (*e.g.*, Supplementary Figure S-1). The importance of developing rapid and accurate methods of characterization for HT materials discovery and optimization derives from the intractable nature of exhaustively testing every material within a functional material’s search space using these conventional tools [14].\n\nThe metal halide perovskite material search space is both highly dimensional and vast, hence, as a result, it is intractable to map using conventional synthesis or characterization methods. The common metal halide perovskite subspace explored in literature consists of an eight-component system: (FAxMAyCs1−x−y)(PbzSn1−z)(BrαClβI1−α−β)3 [7, 9, 14, 22–24]. For one to exhaustively search this subspace at 1% compositional steps would require synthesizing and characterizing \\( 7 \\times 10^{12} \\) unique material samples (Supplementary Figure S-14). Thus, only small regions of this search space can be explored experimentally with current methods, given the large discrepancy between search space size and characterization throughput. For example, Escobedo *et al.* [25] develop automated programs to compute the band gap of semiconductor materials, however, the throughput of the\nFig. 1: a-c, Overview of the synthesis and characterization of perovskite semiconductors. a, High-throughput combinatorial synthesis of FA_{1-x}MA_xPbI_3 perovskites attain throughputs of \\(10^4\\) samples/hr. b, Manual characterization of the high-throughput-manufactured materials using UV-Vis spectroscopy and manual determination of band gap and degradation bottlenecks the pipeline down to a throughput of \\(10^1\\) samples/hr. c, Autocharacterization, developed in this paper, of the high-throughput-manufactured material’s band gaps and degradation attain throughputs of \\(10^3\\) samples/hr using scalable and parallelizable computer vision measurement. Band gap is determined by automatically segmenting and fitting the material reflectance spectra while the degradation pathway is detected by the material yellowing, in the case depicted above due to a phase change from \\(α\\)-FAPbI_3 to \\(δ\\)-FAPbI_3. The widths of the gray backgrounds visualize the process throughputs.\nsoftware is insufficient for HT combinatorial synthesis applications as it can only compute the band gap of one sample at a time using pre-collected optical data. Surmiak et al. [20] and Reinhardt et al. [21] expand on these methods by employing HT optical characterization of perovskites for up to 24 unique samples per batch, however, their measurements occur in serial and are rigidly hard-coded to measure only specified locations, in turn, lacking scalability and generalizability. Similarly, Langner et al. [10] and Wang et al. [9] develop significantly higher throughput drop casting tools capable of synthesizing and characterizing up to 6048 organic photovoltaic films per day, however, their characterization measurements are also fixed, locking the characterization method to their specific system architecture. Unlike the aforementioned literature, Wu et al. [26] develop a HT and scalable tool, automated from end-to-end, to characterize the optical properties of organic molecules. However, their developed tool is designed to only characterize organic molecules actively suspended in solution [26], thus, leaving the task of rapidly and automatically characterizing semiconductors deposited with flexible form factors onto a substrate as an open research gap.\n\nDebottlenecking the materials screening pipeline is not only a matter of accelerating the characterization time per sample [27, 28] but also a matter of scaling the characterization procedure to many samples in parallel [29, 30]. Computer vision methods have the capacity to scale a measurement to arbitrarily many samples, each with differing form factor geometries, without significantly slowing characterization time [31–33]. Material science applications of computer vision are gaining traction in current literature, specifically in the use case of rapid morphological analysis of large microscopy datasets [33]. In turn, several analytical computer vision tools have been developed to access and characterize this morphological information, often focused on identifying microstructures. For example, Park et al. [34] create a semi-automated image segmentation and analysis algorithm to classify the morphology of nanoparticles from image data. Likewise, Chowdhury et al. [35] utilize computer vision and machine learning to detect dendritic microstructures from a database of solder alloy micrographs. There is also extensive work surrounding materials recognition in non-micrographic images using computer vision [27, 36–38]. In order to support the growing need for the analysis of micrographs and other experimental images, advances like those made by Li et al. [32], Wang et al. [39], Neshatavar et al. [40], Tung et al. [29], and Jain et al. [30] on object segmentation, denoising, and scalability allow for further use cases of computer vision in scientific research. The throughput dichotomy between characterization and HT synthesis motivates the integration of computer vision into the semiconductor characterization pipeline to parallelize measurements and, in turn, match or exceed the rate of synthesis while achieving accuracies comparable to those attained by domain expert evaluation.\n\nIn this paper, we address the unresolved challenge of characterizing deposited materials quickly and automatically in parallel by developing a suite of computer vision-based automated characterization (autocharacterization) tools that enable the quantification of three key properties within minutes: composition [41, 42], optical band gap [4–6], and environmental degradation [7–9]. We propose the following in this contribution: (1) sample detection by a scalable computer vision tool that segments arbitrarily many, spatially non-uniform material samples, (2) a tool to map the\nelemental composition of HT-manufactured material arrays, (3) a scalable autocharacterization algorithm for the computation of direct band gaps from hyperspectral reflectance data, and (4) a scalable autocharacterization algorithm for quantifying the environmental stability of perovskite samples from optical degradation data. The performances of the developed autocharacterization methods are demonstrated on 200 unique HT-manufactured FA_{1-x}MA_xPbI_3 perovskite semiconductor samples, generating ultra-high compositional resolution trends of band gap and stability, and are benchmarked against X-ray diffraction [43, 44], X-ray photoelectron spectroscopy [45, 46], and domain expert evaluation.\n\nResults\n\nComputer Vision Parallelization\n\n![Raw hyperspectral datacube and computer-vision segmented datacube diagrams](page_370_682_708_246.png)\n\nFig. 2: a, Raw hyperspectral datacube, \\( \\Omega = (X, Y, R(\\lambda)) \\), captured using a hyperspectral imager (Resonon, Pika L) of HT-deposited FA_{1-x}MA_xPbI_3 perovskites. (\\( X, Y \\)) represents the pixel coordinates, and \\( R(\\lambda) \\) represents the reflectance spectra for each pixel. Each sample is deposited onto the glass substrate with a unique composition \\( 0 \\leq x \\leq 1 \\) and flexible form factor geometry. b, Computer-vision segmented datacube, \\( \\Phi = (\\hat{X}, \\hat{Y}, R(\\lambda)) \\), that pairs each unique sample’s pixels, \\( (\\hat{X}, \\hat{Y})_n \\in N \\), to its reflectance spectra, \\( R(\\lambda) \\). The gray hatched region indicates the discarded background pixels.\n\nWith the integration of computer vision into the materials characterization workflow, data across many samples can be captured and analyzed in parallel as a fast and scalable process [29–33]. Computer vision can be applied to both standard RGB and hyperspectral image data types. Figure 2 illustrates the segmentation of a hyperspectral datacube, taken for one batch of HT-manufactured perovskite samples [27]. In this study, we synthesize three batches of samples, amounting to a total of \\( N = 201 \\) unique semiconductors along the FA_{1-x}MA_xPbI_3 compositional series with \\( 0 \\leq x \\leq 1 \\).\nUsing Algorithm 1, we generate unique pairings for each discrete semiconductor sample, \\( (\\tilde{X}, \\tilde{Y})_n \\in N \\), and its corresponding reflectance spectra, \\( R(\\lambda) \\), via parallel image segmentation and mapping, shown in Figure 2b.\n\nThe process of parallel segmentation uses a sequence of edge-detection filters [47] to first identify each island of material and then uniquely index each island based on its position within a graph connectivity network [48, 49]. The pixel coordinates of each segmented sample are then spatially mapped to their corresponding reflectance spectra, in turn, generating the segmented datacube \\( \\Phi = (\\tilde{X}, \\tilde{Y}, R(\\lambda)) \\). Parallel segmentation and mapping of these reflectance spectra accelerate a once point-by-point measurement process [14, 19], to a rapid and scalable process that can rate-match the throughput of HT synthesis (Supplementary Figure S-1). Furthermore, this segmentation process is shown to scale to more than 80 unique samples in parallel (Supplementary Figure S-4). Algorithm 1 illustrates the sample size-agnostic nature of the method, highlighting its further scalable potential. This segmented reflectance data serves as the starting point for automating the mapping of composition as well as the automating the computation of optical band gap and degradation for all \\( N = 201 \\) unique semiconductors.\n\nComposition Mapping\n\nSemiconductor properties, such as band gap and stability, are largely governed by the chemical composition of the material [7, 8, 41]. Thus, determining the composition accurately enough and mapping the composition to a correct sample is essential for scalable HT setups that deposit variable sample geometries. In this work, we use HT deposition of solution-processed precursors to synthesize perovskite semiconductor samples. The variable rotational velocities of two pumps, \\( \\omega_{\\text{FA}} \\) and \\( \\omega_{\\text{MA}} \\), determine the output sample composition by combining the liquid-based FAPbI$_3$ and MAPbI$_3$ precursors. Figure 3a illustrates this printing process as a function of both space and time. The FA-rich materials are printed first and then proportions of MA are added gradually as the print head rasters in a serpentine pattern. Thus, to determine the composition of each material deposit, \\( \\omega_{\\text{FA}} \\) and \\( \\omega_{\\text{MA}} \\) are spatially and temporally mapped onto the computer vision-segmented samples, \\( (\\tilde{X}, \\tilde{Y})_n \\in N \\), and then integrated over time to determine each sample’s computed FA$_{1-x}$MA$_x$PbI$_3$ composition:\n\n\\[\nx(t) \\approx \\int_{t_a}^{t_b} \\frac{\\omega_{\\text{MA}}(t)}{(\\omega_{\\text{MA}}(t) + \\omega_{\\text{FA}}(t))} dt,\n\\]\n\nwhere \\( x \\) is the proportion of MA, \\( t_a \\) and \\( t_b \\) are the starting and ending timesteps for the deposition of a single sample, and \\( \\omega_{\\text{FA}}(t) \\) and \\( \\omega_{\\text{MA}}(t) \\) are the pump velocities at a given timestep for the FAPbI$_3$ and MAPbI$_3$ precursors, respectively.\n\nFigure 3b-c illustrates the composition validation results using X-ray diffraction (XRD) and X-ray photoelectron spectroscopy (XPS). XRD is used to validate the crystalline structure [43, 44] while XPS is used to validate the elemental composition of the manufactured perovskite deposits [45, 46]. By assessing the gradated shifts in both XRD and XPS peaks, the composition mapping can be validated. For crystal structure validation, the crystal lattice size of MAPbI$_3$ is smaller than that of FAPbI$_3$\nFig. 3: a, High-throughput combinatorial synthesis of one batch of perovskite samples illustrated with its corresponding computer vision-segmented composition map. The print head rasters in a serpentine pattern (black connecting lines) to print a gradient of FA_{1-x}MA_xPbI_3 deposits onto a glass substrate, where the purple labels indicate FA-rich deposits, and the yellow labels indicate MA-rich deposits. Integrating the pump speeds over time determines the proportion of MA, x, in the composition. b, XRD peak traces at the (012) crystallographic plane measured at uniformly spaced compositions in the batch print. The peak shifts towards a higher \\(2\\theta\\) angle gradually as the proportion of MA increases in the composition. c, XPS traces of the C=N bond peak (red area under the curve) and C-N bond peak (gray area under the curve) measured at uniformly spaced compositions in the batch print. The C=N peak intensity decreases as the proportion of MA increases. Purple-labeled traces are FA-rich while yellow-labeled traces are MA-rich.\n\n[42], thus, we expect the XRD peaks of the MA-rich deposits to shift toward higher angles [50]. In Figure 3b, the (012) crystallographic plane at \\(2\\theta \\approx 31.5^\\circ\\) [51, 52] is shown, for uniformly-spaced samples across the batch print, to gradually increase in angle from the FA-rich to the MA-rich compositions of FA_{1-x}MA_xPbI_3, amounting to a total shift of approximately 0.16° (quantitative shifts shown in Supplementary Figure S-13a). For elemental validation, the A-site MA and FA cations are distinguished by the presence of a carbon-nitrogen double bond (C=N), where FA contains a C=N bond while MA contains only a C-N single bond [50]. In the high-resolution XPS scans, shown in Figure 3c, the C=N bond peak appears at approximately 400eV [53]. This C=N bond peak is shown, for uniformly-spaced samples across the batch print, to gradually decrease in intensity from the FA-rich to the MA-rich compositions of FA_{1-x}MA_xPbI_3 (quantitative shifts shown in Supplementary Figure S-13b). These results validate both the structural and elemental composition gradients synthesized and mapped using computer vision. With the developed composition map, we can now automatically compute the band gap and detect degradation across the 201 uniquely synthesized compositions.\nAutomated Band Gap Extraction\n\n![Automatic band gap computation shown for two unique, computer vision-segmented perovskite deposits. The reflectance intensities, R(λ), are acquired for each sample from a, the vision-segmented hypercube, Φ. The Tauc curves are computed from the median reflectance spectra for each deposit, recursively segmented into line segments, and then iteratively fit with linear regression lines. The best-fit regression line that minimizes the RMSE between the detected Tauc peaks is illustrated by the thick red line, which determines the band gap, E_g, from the x-intercept.](page_184_232_1079_563.png)\n\nFig. 4: a-c, Automatic band gap computation shown for two unique, computer vision-segmented perovskite deposits. b, The reflectance intensities, \\( R(\\lambda) \\), are acquired for each sample from a, the vision-segmented hypercube, \\( \\Phi \\). c, The Tauc curves are computed from the median reflectance spectra for each deposit, recursively segmented into line segments, and then iteratively fit with linear regression lines. The best-fit regression line that minimizes the RMSE between the detected Tauc peaks is illustrated by the thick red line, which determines the band gap, \\( E_g \\), from the x-intercept.\n\nBand gap is essential in defining the light-harvesting potential of a semiconductor material [4, 42]. However, conventionally computing the band gap of a material is a laborious process, requiring a user to manually curve-fit the Tauc-transformed UV-Vis spectra [19, 54]. In this paper, we automate and accelerate the computation of band gap across 201 unique semiconductor samples by leveraging hyperspectral imaging and computer vision segmentation, such that the characterization process is parallelized across batches of HT-manufactured semiconductor samples.\n\nFigure 4 illustrates the autocharacterization process of band gap by first, (a) extracting the reflectance spectra from each computer vision-segmented sample within the hyperspectral datacube, then, (b) transforming each reflectance spectra to its Tauc curve, and finally, (c) recursively segmenting the Tauc curves into linear segments (\\( R^2 \\geq 0.990 \\)) to find the regression line of best fit between peaks, which determines band gap. The Tauc curves are obtained from a hyperspectral reflectance datacube using the following transformation [19]:\n\n\\[\nF(R(\\lambda) \\cdot h \\nu)^{1/\\gamma} = B(h \\nu - E_g),\n\\]\n\n(2)\nwhere \\( F(R(\\lambda)) \\) is the Kubelka-Munk function [55] applied to reflectance spectra, \\( R(\\lambda) \\), for each wavelength, \\( \\lambda \\), with \\( h \\) as the Planck constant, \\( \\nu \\) as the photon frequency, \\( B \\) as a constant, and \\( \\gamma = \\frac{1}{2} \\) for direct band gap and \\( \\gamma = 2 \\) for indirect band gap.\n\n![Scatter plot comparing automated and expert band gaps, with regression fit and color bar indicating proportion of MA.](page_374_682_693_377.png)\n\nFig. 5: Performance of the autocharacterization of band gap relative to the domain expert-compute band gap for \\( N = 201 \\) unique perovskite samples across 3 independent trials. The solid black line is the regression fit to the band gap data and the dashed black line is the \\( y = x \\) line. Histogram distributions of both autocharacterization and domain expert band gaps are shown on the right and top of the plot area, respectively. The color of the scatter points corresponds to the proportion of MA, \\( x \\), in the composition \\( \\mathrm{FA}_{1-x}\\mathrm{MA}_x\\mathrm{PbI}_3 \\).\n\nTo demonstrate the performance of the band gap autocharacterization developed in this paper, the algorithm’s output band gaps are compared with those calculated by a domain expert using the manual fitting process described in Makula et al. [19]. The autocharacterization output was withheld from the domain expert. Figure 5 illustrates the performance of the autocharacterization-calculated band gaps relative to the expert-calculated band gaps for \\( N = 201 \\) \\( \\mathrm{FA}_{1-x}\\mathrm{MA}_x\\mathrm{PbI}_3 \\) compositions across three independent batches of samples. The autocharacterization output achieves a strong linear fit of \\( R^2 = 0.975 \\) with the expert-calculated results, however, a systematic underprediction of the autocharacterization algorithm is noted. Relative to the expert-computed band gap, the autocharacterization method achieves 98.5% accuracy within a 0.02eV range on the \\( \\mathrm{FA}_{1-x}\\mathrm{MA}_x\\mathrm{PbI}_3 \\) system (Supplementary Figure S-6). In addition to the autocharacterization achieving high similitude with the domain expert, it also provides significant speedups in band gap determination. The domain expert takes approximately 510 minutes to compute the band gap of 200 unique samples while the autocharacterization takes 6 minutes to compute the band gap of 200 samples, resulting in the developed autocharacterization tool achieving 85x faster throughput via the parallel-processing power of computer vision.\nUsing the fast and accurate band gap autocharacterization tool developed in this paper, we tractably generate an ultra-high resolution band gap trend for the FA_{1-x}MA_xPbI_3, 0 \\leq x \\leq 1 series, shown in Figure 5, where 120 of the 201 compositions are unique, a resolution that has not yet been reported in literature. Prior literature reports band gap compositional resolutions from 0 \\leq x \\leq 1 for 9 compositions [56], 7 compositions [57, 58], 6 compositions [59], and 5 compositions [7] using conventional characterization methods. Thus, with autocharacterization, we achieve over a 13x increase in the compositional resolution of FA_{1-x}MA_xPbI_3 band gap, to our knowledge.\n\nAutomated Degradation Detection\n\n![Automatic degradation testing and measurement of computer vision-segmented perovskite deposits.](page_184_370_1082_370.png)\n\nFig. 6: a-c Automatic degradation testing and measurement of computer vision-segmented perovskite deposits. a, The samples are placed in the degradation chamber with specified environmental conditions for a total of two hours. b, RGB images of the samples are taken every 30 seconds for two hours to resolve the time-dependent color change in material. c, Computer vision is used to segment each deposited sample over time, \\( \\Phi(t) \\), to compute the degradation intensity metric, \\( I_c \\).\n\nSufficient stability of perovskite semiconductors is required for the material to be utilized in solar cell applications [1–3, 60]. As a lead halide perovskite degrades, it changes color from black to yellow, a result of a phase change and/or decomposition of the structure [7, 61, 62]. We leverage this RGB-detectable degradation mechanism [8] and use parallelized computer vision segmentation to automate the detection of degradation within perovskites, as shown in Figure 6c. Three independent degradation experiments are conducted across the \\( N = 201 \\) samples by placing each batch of samples within a degradation chamber, shown in Figure 6a, for 2 hours at an illumination of 0.5 suns, temperature of 34.5°C ± 0.5°C, and relative humidity of 40% ± 1%\n(Supplementary Figure S-7). We compute the degradation intensity, \\( I_c \\), of each HT-manufactured perovskite composition by integrating the change in color, \\( R \\), for each sample over time, \\( t \\) [7]:\n\n\\[\nI_c(\\hat{X}, \\hat{Y}) = \\sum_{R=\\{r,g,b\\}} \\int_0^T |R(t; \\hat{X}, \\hat{Y}) - R(0; \\hat{X}, \\hat{Y})| dt,\n\\]\n\nwhere \\( T \\) is the duration of the degradation and the three reflectance color channels are red, \\( r \\), green, \\( g \\), and blue, \\( b \\), for each sample, \\( (\\hat{X}, \\hat{Y})_n \\in N \\). High \\( I_c \\) indicates high color change, corresponding to high degradation; \\( I_c \\) close to zero indicates low color change and low degradation.\n\n![Scatter plot showing degradation intensity vs composition and images of three batches of FA1-xMAxPbI3 gradient samples](page_246_563_956_388.png)\n\nFig. 7: a, Performance of the autocharacterization of degradation intensity, \\( I_c \\), relative to the ground truth degradation determined by a domain expert (yellow scatter points) on \\( N = 201 \\) unique perovskite samples across 3 independent trials. The black dashed line indicates the split between high and low \\( I_c \\) values, corresponding to high and low degrees of degradation, respectively. b, Images of the three batches of FA1-xMAxPbI3 gradient samples after the 2-hour controlled degradation. The leftmost samples are FA-rich and the rightmost samples are MA-rich. The yellowed FA-rich compounds have undergone a phase transition from \\( \\alpha \\)-FAPbI3 to \\( \\delta \\)-FAPbI3 and are considered as “ground truth” degradation samples if they exhibit a deviation of > 0.02eV in band gap from pre- to post-degradation, evaluated by a domain expert.\n\nThe performance of the degradation autocharacterization is demonstrated by comparing the output \\( I_c \\) to the ground truth degradation, obtained from the pre- and post-band gap deviation [7, 63] (Supplementary Figure S-10a). Figure 7a illustrates the output of the autocharacterization where high computed \\( I_c \\) values strongly correspond to the occurrence of the ground truth degradation in the samples (yellow\nscatter points). The determination of ground truth degradation is conducted by a human domain expert, further described in Supplementary Figure S-10a. This classification performance of the autocharacterization algorithm achieves a precision-recall AUC (area under the curve) of 0.853 (Supplementary Figure S-10c), and a maximal accuracy of 96.9%, relative to the ground truth (Supplementary Figure S-10d). The yellowing pattern of the FA-rich samples is shown in Figure 7b as a result of the phase change from favorable cubic phase \\( \\alpha \\)-FAPbI\\(_3\\) to the non-perovskite hexagonal phase \\( \\delta \\)-FAPbI\\(_3\\) [61] (Supplementary Figure S-11). Furthermore, running a full degradation detection computation using autocharacterization takes only 20 minutes per 200 samples, given 48000 total degradation images over the 2-hour degradation experiment. This is a significant speedup from the standard microscopy or XRD methods of determining degradation, which can take hours or days to identify the degradation of an equivalent number of samples.\n\nUsing the fast and accurate stability autocharacterization tool developed in this paper, we tractably generate an ultra-high resolution stability trend for the FA\\(_{1-x}\\)MA\\(_x\\)PbI\\(_3\\) series, shown in Figure 7a where, similar to band gap, this trend has not been reported at such a high resolution yet in literature. Prior literature reports stability compositional resolutions from \\( 0 \\leq x \\leq 1 \\) for 11 compositions [64], 9 compositions [56], and 7 compositions [65] using conventional characterization methods. Moreover, Charles et al. [64] reports the stability at \\( x \\approx 0.1 \\) compositional increments from \\( 0 \\leq x \\leq 1 \\) using 6 timesteps, amounting to a total of 66 temporal data points. Comparatively, this study reports the stability at \\( x \\approx 0.008 \\) unique compositional increments from \\( 0 \\leq x \\leq 1 \\) using 240 timesteps, amounting to 28800 unique temporal data points (with 48000 total temporal data points). Thus, with autocharacterization, we achieve over a 10x increase in the compositional resolution and a 40x increase in the temporal resolution for a total of a 436x increase in the number of unique data points reported for the FA\\(_{1-x}\\)MA\\(_x\\)PbI\\(_3\\) stability series, to our knowledge. Furthermore, with this high-resolution stability trend, we note the same regions of high-degradation appear in Figure 7a as do in the literature for the \\( \\alpha \\)-FAPbI\\(_3 \\rightarrow \\delta \\)-FAPbI\\(_3\\) degradation pathway at \\( 0.0 \\leq x \\leq 0.15 \\), with the optimal low-degradation region occurring at \\( x \\approx 0.40 \\) [64, 66]. Through the generation of ultra-high resolution trends, we may achieve a better understanding of complex semiconductor composition-property relationships to enable higher-performance design of materials in the future.\n\nConclusion\n\nAccelerating the characterization of key material properties relevant to semiconductor engineering, such as band gap and stability, is a necessary step to enable the high-throughput discovery and optimization of perovskite materials. Conventional methods of characterization bottleneck the materials screening pipeline when high-throughput synthesis is utilized, inhibiting optimally efficient high-throughput experimentation. For example, computing the band gap of 200 unique halide perovskite samples takes a domain expert over 8 hours to complete. In this work, we demonstrate the fast and accurate characterization of band gap and detection of degradation within the\nFA_{1-x}MA_xPbI_3, \\ 0 \\leq x \\leq 1 perovskite system using parallelized, scalable computer vision segmentation. From the segmented data, the band gaps and degrees of degradation are automatically computed using the developed autocharacterization algorithms, and ultra-high compositional resolution trends are generated. The band gaps of 200 unique perovskite samples are determined in 6 minutes at 98.5% accuracy within a 0.02eV range using the band gap autocharacterization tool. The degrees of degradation of 200 unique perovskite samples are determined within 20 minutes at 96.9% accuracy using the degradation autocharacterization tool. Overall, the developed autocharacterization methods achieve 85x faster throughputs than conventional domain expert evaluation, in turn, contributing to the debottlenecking of high-throughput and autonomous materials discovery and optimization workflows. Therefore, through the wider application of autocharacterization methods, the ability to scan through larger material search spaces is unlocked, in turn, enabling the tractable design of higher-performance functional materials\n\nMethods\n\nMaterials\n\n3\"×2\"×1mm glass slides (C&A Scientific) are cleaned using deionized water (DI, < 1.0μS/cm, VWR), Hellmanex III (VWR), and isopropyl alcohol (IPA, ≥ 99.5%, VWR) to be used as substrates. Lead iodide powder (PbI_2, 99.999% trace metal basis, Sigma-Aldrich), formamidinium iodide powder (FAI, >99.9%, Greatcell Solar Materials), methylammonium iodide (MAI, >99.9%, Greatcell Solar Materials), dimethylformamide (DMF, ≥99.8%, Sigma-Aldrich), and dimethylsulfoxide (DMSO, ≥99.9%, Sigma-Aldrich) are used to prepare the perovskites.\n\nComputer Vision Segmentation of Hyperspectral Datacubes\n\nA hyperspectral datacube of size \\( X \\times Y \\times R(\\lambda) \\rightarrow 900\\text{px} \\times 800\\text{px} \\times 300 \\), where 300 is the number of wavelengths, \\( \\lambda \\), is captured as a raw image, \\( \\Omega = (X,Y,R(\\lambda)) \\), from the hyperspectral camera (Resonon, Pika L). This datacube is passed through several filters to find the edges and segment each material deposit sample \\( (\\tilde{X}, \\tilde{Y})_n \\in N \\) and then index the features appropriately, such that each pixel is mapped to its reflectance spectra, \\( R(\\lambda) \\). Once segmented, each deposited material contains an area of approximately 1000px worth of spatial spectral data. Inputting images or features of different sizes may require tuning the kernel sizes, \\( \\kappa \\), of the filters.\n\nAlgorithm 1 describes this segmentation process of \\( (X,Y,R(\\lambda)) \\rightarrow (\\tilde{X},\\tilde{Y},R(\\lambda)) \\). First, the input image is cropped and converted to greyscale, then it is passed through several layers of thresholding and smoothing. By thresholding, eroding, blurring, and then thresholding again, we capture the edges of each feature while removing edge effects. The background is indexed as zeros, hence, all features split by zeros are assigned a unique index using island-finding graph network methods from the OpenCV Python library [47]: LabelFeatures(:) and Watershed(:) [48, 49]. Once segmented, the features are smoothed, and any improperly segmented aberrations are pruned with the user-selected variables \\( \\Theta_{\\min}, \\Theta_{\\max} \\), where features of size \\( s < \\Theta_{\\min} \\) or \\( s > \\Theta_{\\max} \\)\nare removed. Finally, a boolean mask is created for all pixels encoded with non-zero values to output \\( \\Phi \\), where each uniquely indexed material deposit is directly mappable to the \\( R(\\lambda) \\) measured for that deposit.\n\nAlgorithm 1: Scalable Computer Vision Segmentation\n\nInput : \\((X, Y, R(\\lambda))\\): All image pixels and reflectance\n \\( \\Theta_{\\min} \\): Minimum segmented feature size\n \\( \\Theta_{\\max} \\): Maximum segmented feature size\nOutput : \\((\\hat{X}, \\hat{Y}, R(\\lambda))\\): Segmented pixels and reflectance\n Let \\( \\kappa \\) be kernel size\n 1 img \\( \\leftarrow (X, Y, R(\\lambda)) \\)\n 2 img \\( \\leftarrow \\text{Crop(img)} \\)\n 3 img \\( \\leftarrow \\text{Grayscale(img)} \\)\n 4 img \\( \\leftarrow 255 - \\text{img} \\)\n 5 mask \\( \\leftarrow \\text{Binarize(img)} \\)\n 6 mask \\( \\leftarrow \\text{MorphGradient(mask, } \\kappa = 12 \\text{)} \\)\n 7 mask \\( \\leftarrow \\text{Erode(mask, } \\kappa = 3 \\text{)} \\)\n 8 mask \\( \\leftarrow \\text{MedianBlur(mask, } \\kappa = 7 \\text{)} \\)\n 9 mask \\( \\leftarrow \\text{DistTransform(mask, } \\kappa = 3 \\text{)} \\)\n 10 mask \\( \\leftarrow \\text{LabelFeatures(mask)} \\)\n 11 \\((\\hat{X}, \\hat{Y}) \\leftarrow \\text{Watershed(img, mask)} \\)\n 12 \\((\\hat{X}, \\hat{Y}) \\leftarrow \\text{Dilate}((\\hat{X}, \\hat{Y}), \\kappa = 5) \\)\n 13 \\((\\hat{X}, \\hat{Y}) \\leftarrow \\text{MedianBlur}((\\hat{X}, \\hat{Y}), \\kappa = 7) \\)\n 14 for \\( \\phi \\) in \\( \\text{Feature}((\\hat{X}, \\hat{Y})) \\) do\n 15 if \\( \\text{Size}(\\phi) < \\Theta_{\\min} \\) or \\( \\text{Size}(\\phi) > \\Theta_{\\max} \\) then\n 16 \\((\\hat{X}, \\hat{Y})\\).Prune(\\( \\phi \\))\n end\n end\n 19 bool \\( \\leftarrow \\text{Boolean}((\\hat{X}, \\hat{Y})) \\)\n 20 \\((\\hat{X}, \\hat{Y}, R(\\lambda)) \\leftarrow (X, Y, R(\\lambda)).\\text{Mask}(bool)\\)\n Return \\((\\hat{X}, \\hat{Y}, R(\\lambda))\\)\n\nPerovskite Elemental Composition Mapping onto Computer Vision Segmented Data\n\nThe composition for each segmented deposit, \\((\\hat{X}, \\hat{Y})_n \\in N\\) is determined by mapping the encoded pump speeds of the high-throughput combinatorial printer to the time step, \\( \\Delta t = [t_a, t_b] \\), at which each deposit is printed. This is done by mapping the segmented image \\( \\Phi \\) to the printer head raster path, acquired from the G-code controlling the printer motion. Hence, each deposited material now has its pixel coordinates \\((\\hat{X}, \\hat{Y})\\) mapped to a timestamp along the raster path. Then, this positional timestamp is mapped to its corresponding pump speed timestamp, \\( t(\\hat{X}, \\hat{Y}) \\rightarrow t(\\omega_{FA}, \\omega_{MA}) \\). Since these variable pump speeds \\( \\omega_{FA} \\) and \\( \\omega_{MA} \\) are both monotonic along the time series,\nthey are deterministic of the proportion of FA and MA within the FA_{1-x}MA_xPbI_3 compositional structure by integrating pump speed over the \\( \\Delta t \\) for each material deposit *via* Equation 1.\n\n**Automating Band Gap Computation using Hyperspectral Reflectance Data**\n\nThe direct band gap for all \\( N = 201 \\) FA_{1-x}MA_xPbI_3 perovskite compositions is computed from the vision-segmented reflectance data, \\( \\Phi = (\\hat{X}, \\hat{Y}, R(\\lambda)) \\), since all the FA_{1-x}MA_xPbI_3 compositions are direct band gap materials at atmospheric pressure [67, 68]. For every segmented sample, \\( (\\hat{X}_i, \\hat{Y}_i) \\in N \\), the spatial median \\( R(\\lambda) \\) spectra is used for computing the band gap. \\( R(\\lambda) \\) spans across wavelengths, \\( \\lambda \\), where \\( \\{\\lambda \\in \\mathbb{Z} : 380\\text{nm} \\leq \\lambda \\leq 1020\\text{nm}\\} \\) for hyperspectral imaging and \\( \\lambda = \\{r, g, b\\} \\) for the red, green, and blue color channels of RGB imaging. First, the median \\( R(\\lambda) \\) spectra are transformed into a Tauc curve using Equation 2, with \\( \\gamma = \\frac{1}{2} \\) for direct band gap. Then, transformed Tauc curves are recursively segmented in half until each segment achieves a fit of \\( R^2 \\geq 0.990 \\), indicating that each segment is near-linear:\n\n\\[\nR^2 = 1 - \\frac{\\sum_i^N (y_i - \\hat{y}_i)^2}{\\sum_i (y_i - \\overline{y})^2},\n\\]\n\nwhere \\( \\hat{y} \\) is the predicted value and \\( \\overline{y} \\) is the average value of the set. Once the recursion is complete, each pair of adjacent line segments is iteratively fit to a linear regression line, generating a set of candidate fit lines to use for computing band gap. To determine the best candidate fitted line, RMSE is used rather than using the inclination angles of Tauc curves [25] to improve generalizability across different materials, *e.g.* FAPbI_3 and MAPbI_3:\n\n\\[\n\\text{RMSE} = \\sqrt{\\frac{\\sum_i^N (y_i - \\hat{y}_i)^2}{N}}.\n\\]\n\nWe implement an iterative root-mean-square error (RMSE) minimization routine that automatically identifies the Tauc curve peaks to fit between. Then, the RMSE is computed between each regression line and the Tauc curve within the lower bound of the regression x-intercept and the upper bound of the Tauc peak location minus one-half of the peak width. Enforcing the RMSE computation to occur within these bounds was shown to increase fitting accuracy with the Tauc slope. The band gap, \\( E_g \\), is then extracted from x-intercept point of the regression line that achieves the minimum RMSE.\n\n**Detecting Perovskite Degradation from RGB Time Series Data**\n\nIn order to use color as a reproducible and repeatable quantitative proxy for degradation, color calibration needs to be applied because the illumination conditions in the aging test chamber may create distortions to the true sample color. At the beginning of the degradation study, an image of a reference color chart (X-Rite Colour Checker Passport; 28 reference color patches), \\( I_{R_i} \\), is taken under the same illumination conditions as the perovskite semiconductor samples. Images at each time step, \\( \\Omega(\\Delta t) \\), are\ntransformed into CIELAB colorspace and subsequently into a stable reference color space, CIE 1931 color space with a 2-degree standard observer and standard illuminant D50, by applying a 3D-thin plate spline distortion matrix \\( D \\) [7, 69] defined by \\( I_R \\) and known colors of the reference color chart:\n\n\\[\nD = \\begin{bmatrix} V \\\\ O(4,3) \\end{bmatrix} \\begin{bmatrix} K & P \\\\ P^T & O(4,4) \\end{bmatrix}^{-1}\n\\]\n\nHere, \\( O(n,m) \\) is an \\( n \\times m \\) zero matrix, \\( V \\) is a matrix of the color checker reference colors in the stable reference color space, \\( P \\) is a matrix of the color checker RGB colors obtained from \\( I_R \\), and \\( K \\) is a distortion matrix between the color checker colors in the reference space and in \\( I_R \\). Using the color-calibrated images and droplet pixel locations given by \\( \\Phi \\), a final array, \\( R(t;\\vec{X},\\vec{Y}) \\) of the average color at time \\( t \\) for perovskite semiconductor of composition \\( \\mathrm{FA}_{1-x}\\mathrm{MA}_x\\mathrm{PbI}_3 \\) is created. The color of each droplet is measured to determine the stability metric \\( I_c \\) [7], calculated using Equation 3.\n\nExperimental Section\n\nSubstrate Preparation\n\nGlass slide substrates are prepared for printing the perovskite samples using a three-step cleaning process: (1) ultrasonication for 5 minutes in DI water with 2%vol. Hellmanex III solution, (2) ultrasonication for 5 minutes in DI water only, and (3) ultrasonication for 5 minutes in IPA. Once cleaned, the substrates are transferred to an inert nitrogen environment glovebox with moisture levels < 10ppm.\n\nPerovskite Preparation\n\nFAPbI$_3$ (formamidinium lead iodide) and MAPbI$_3$ (methylammonium lead iodide) are prepared as 0.6M liquid-based precursors for high-throughput printing. For printing, 2mL of each precursor is prepared in an inert nitrogen environment glovebox with moisture levels < 10ppm. First, 3.2mL DMF is mixed with 0.8mL of DMSO to make 4mL of 4 : 1 DMF:DMSO solution. Then, 1.106g of PbI$_2$ powder is dissolved into the 4mL of 4 : 1 DMF:DMSO to make a PbI$_2$ stock. Next, the 4mL PbI$_2$ stock is split in half, pipetting 2mL of stock per vial. Lastly, 0.206g of FAI powder is dissolved into one of the 2mL PbI$_2$ stock vials and 0.191g of MAI powder is dissolved into the other making 0.6M FAPbI$_3$ and 0.6M MAPbI$_3$, respectively.\n\nHigh-throughput Perovskite Synthesis\n\nThe liquid-based FAPbI$_3$ and MAPbI$_3$ precursor solutions are used in the high-throughput combinatorial printer to synthesize \\( N = 201 \\) unique \\( \\mathrm{FA}_{1-x}\\mathrm{MA}_x\\mathrm{PbI}_3 \\) composition samples. The high-throughput printer is custom-made, and parts of its construction are documented in Siemenn et al. [27]. To begin printing, first, all printer plumbing lines are flushed twice with the 4 : 1 ratio DMF:DMSO solution. Then, the FAPbI$_3$ and MAPbI$_3$ precursors are extracted into syringes using a microcontroller to communicate with the pumps. These syringes contain prismatic motion plungers that use positive displacement to fill and eject solution. Next, all plumbing lines are\nprimed with the precursor solution. After priming, the precursors are purged at equal rates from both syringes for 50 seconds to remove air bubbles. Finally, motor encoders pump the precursors out of the syringes at pre-programmed rates, illustrated in Supplementary Figure S-3, and enter a mixing chamber prior to deposition. A pinch valve breaks up the fluid flow within a 1/32”ID × 3/32”OD silicone tube, actuating at 11Hz frequency and 5% duty cycle to deposit each sample as a discrete droplet onto the cleaned glass slide. The print head translates at a speed of 38mm/s over the 3”×2” glass slide in a serpentine pattern, depositing approximately 70-80 unique composition samples per batch in 16.5 seconds. Approximately 0.15mL of total precursor volume is consumed per print, which includes the volume required for purging and priming the plumbing lines. After the droplets have been deposited onto the substrate, the substrate is transferred to a hotplate to anneal for 15 minutes at 150°C.\n\nData Availability\n\nThe raw experimental data that support the findings and plots of this study are available publicly. The band gap data (https://osf.io/qe9ax) and the degradation data (https://osf.io/y2xds) are available from OSF.\n\nCode Availability\n\nAll code used to develop the autocharacterization and computer vision algorithms are available publicly with complete working examples. The band gap autocharacterization code (https://github.com/PV-Lab/Autocharacterization-Bandgap) and the degradation detection autocharacterization code (https://github.com/PV-Lab/Autocharacterization-Stability) are available from GitHub.\nAcknowledgements\n\nWe thank First Solar for support and fruitful discussions. The automation portion of this work was undertaken thanks in part to funding provided to the University of Toronto’s Acceleration Consortium. This material is partially based upon work supported by the U.S. Department of Energy’s Office of Energy Efficiency and Renewable Energy (EERE) under the Advanced Manufacturing Office (AMO) Award Number DE-EE0009096. B.D. acknowledges the support of the Simons Foundation. A.T. was supported by the Research Council of Finland Flagship programme: Finnish Center for Artificial Intelligence FCAI. H.K. received financial support from the Scientific and Technological Research Council of Turkey (TUBITAK) BIDEB-2219 (Project No: 1059B192100703) during this study. This work made use of the MRSEC Shared Experimental Facilities at MIT, supported by the National Science Foundation under award number DMR-1419807.\n\nAuthor Contributions\n\nA.E.S. and E.A. conceptualized the work. A.E.S., E.A., A.T., B.D., and T.B. designed the methodology. A.E.S., E.A., and A.T. wrote the software. F.S. and H.K. prepared the experimental materials. A.E.S., E.A., F.S., and B.D. conducted experiments. 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Click to download.\n\n• AutocharacterizationSI.pdf"} {"paper_id": "prb39", "title": "Autonomous Microscopy Experiments through Large Language Model Agents", "text": "Autonomous Microscopy Experiments through Large Language Model Agents\n\nN M Anoop Krishnan\nkrishnan@iitd.ac.in\n\nIndian Institute of Technology Delhi https://orcid.org/0000-0003-1500-4947\nIndrajeet Mandal\nIndian Institute of Technology Delhi\nJitendra Soni\nIndian Institute of Technology Delhi\nMohd Zaki\nIndian Institute of Technology Delhi https://orcid.org/0000-0002-4551-3470\nMorten Smedskjaer\nAalborg University https://orcid.org/0000-0003-0476-2021\nKatrin Wondraczek\nLeibniz Institute of Photonic Technology\nLothar Wondraczek\nUniversity of Jena\nNitya Nand Gosvami\nIndian Institute of Technology Delhi\n\nArticle\n\nKeywords: self-driving laboratory, atomic force microscopy, benchmarking, AI agents\n\nPosted Date: December 19th, 2024\n\nDOI: https://doi.org/10.21203/rs.3.rs-5600537/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nAdditional Declarations: There is NO Competing Interest.\nVersion of Record: A version of this preprint was published at Nature Communications on October 14th, 2025. See the published version at https://doi.org/10.1038/s41467-025-64105-7.\nAutonomous Microscopy Experiments through Large Language Model Agents\n\nIndrajeet Mandal1, Jitendra Soni2, Mohd Zaki3, Morten M. Smedskjaer4, Katrin Wondraczek5, Lothar Wondraczek6, Nitya Nand Gosvami1,2,7*, N. M. Anoop Krishnan1,3,7,*\n\n1School of Interdisciplinary Research, Indian Institute of Technology Delhi, Hauz Khas, New Delhi 110016, India.\n2Department of Materials Science and Engineering, Indian Institute of Technology Delhi, Hauz Khas, New Delhi 110016, India\n3Department of Civil Engineering, Indian Institute of Technology Delhi, Hauz Khas, New Delhi 110016, India.\n4Department of Chemistry and Bioscience, Aalborg University, Aalborg, Denmark\n5Leibniz Institute of Photonic Technology, 07745 Jena, Germany\n6Otto Schott Institute of Materials Research, University of Jena, 07743 Jena, Germany\n7Yardi School of Artificial Intelligence, Indian Institute of Technology Delhi, Hauz Khas, New Delhi 110016, India\n\n*Corresponding Authors: ngosvami@iitd.ac.in (N. N. G.); krishnan@iitd.ac.in (N. M. A. K.)\nFax: +91-11-2658-1117; Tel: +91-11-2659-1223\n\nKeywords: self-driving laboratory, atomic force microscopy, benchmarking, AI agents\n\nAbstract\nThe emergence of large language models (LLMs) has accelerated the development of self-driving laboratories (SDLs) for materials research. Despite their transformative potential, current SDL implementations rely on rigid, predefined protocols that limit their adaptability to dynamic experimental scenarios across different labs. A significant challenge persists in measuring how effectively AI agents can replicate the adaptive decision-making and experimental intuition of expert scientists. Here, we introduce AILA (Artificially Intelligent Lab Assistant), a framework that automates atomic force microscopy (AFM) through LLM-driven agents. Using AFM as an experimental testbed, we develop AFMBench—a comprehensive evaluation suite that challenges AI agents based on language models like GPT-4o and GPT-3.5 to perform tasks spanning the scientific workflow: from experimental design to results analysis. Our systematic assessment shows that state-of-the-art language models struggle even with basic tasks such as documentation retrieval, leading to a significant decline in performance in multi-agent coordination scenarios. Further, we observe that LLMs exhibit a tendency to not adhere to instructions or even divagate to additional tasks beyond the original request, raising serious concerns regarding safety alignment aspects of AI agents for SDLs. Finally, we demonstrate the application of AILA on increasingly complex experiments open-ended experiments: automated AFM calibration, high-resolution feature detection, and mechanical property measurement. Our findings emphasize the necessity for stringent\nbenchmarking protocols before deploying AI agents as laboratory assistants across scientific disciplines.\n\n1. Introduction\nScientific experimentation demands exceptional domain expertise, from exploration or hypothesis-driven experimental design to precision execution and rigorous data analysis. This complexity creates bottlenecks in scientific discovery, particularly as experimental techniques grow increasingly sophisticated. The advent of large language models (LLMs) has propelled the development of self-driving laboratories (SDLs) that integrate diverse information sources for automated planning\\(^1\\) and experimentation. AI-agents\\(^2,3\\) and SDLs have already achieved several feats in materials or molecular discovery\\(^4–6\\), chemistry research\\(^7\\), and inorganic materials synthesis. The promise of SDLs toward achieving sustainable development\\(^8\\) has resulted in enormous efforts to harness their potential in high-throughput experimentation and discovery\\(^9\\). Efforts to streamline SDLs have resulted in orchestration architectures such as ChemOS\\(^10\\). Additionally, it has been demonstrated that the capability of SDLs can be enhanced by a human-in-the-loop framework that handles disambiguation, thereby enabling better planning and execution\\(^11\\). While early demonstrations of LLM-based lab assistants showed promise in chemistry and materials science\\(^1–3\\), their operational reliability remains largely uncharacterized beyond specific applications or repetitive use cases with predetermined protocols\\(^15–19\\).\n\nCurrent research predominantly addresses well-documented or predefined protocols and single-objective tasks, failing to capture the intricate interplay between experimental planning, multi-tool coordination, and result interpretation or online intervention\\(^10\\). While recent investigations incorporating planning elements have demonstrated success in achieving specific experimental objectives, they have not systematically evaluated SDL reliability across the broader spectrum of laboratory automation tasks\\(^15,16\\). Although several studies have benchmarked LLMs\\(^17,18,20–23\\) and vision language models (VLMs)\\(^13–16\\) through question-answer protocols to assess their potential as materials research co-pilots, a crucial knowledge gap persists: understanding how these AI systems handle novel experimental scenarios and their fundamental limitations.\n\nTo address this challenge, we here introduce AILA (Artificially Intelligent Lab Assistant), an LLM-powered framework augmented with specialized tools. We selected scanning probe microscopy\\(^20\\), specifically atomic force microscopy (AFM), as our experimental testbed, given its inherent complexity and broad applicability in materials research. There have been several efforts to automate microscopy techniques using AI and human-in-the-loop approaches due to their extensive applications in materials characterization\\(^28–30,30,31,31–35\\). These efforts focus exclusively on advancing specific operational aspects, such as analysing moving objects or optimizing illumination conditions, with an emphasis on improving individual steps within the broader experimental protocol\\(^30,32,35\\). AFM operation demands expertise across multiple domains—from probe calibration to parameter optimization and data interpretation—making\nit an ideal platform for evaluating AI agents’ ability to manage sophisticated experimental workflows.\n\nUsing AFM as the model system, we probe AILA’s capabilities through AFMBench on five critical aspects of scientific automation: experimental workflow design, multi-tool coordination, decision-making, execution of open-ended experiments, and data analysis. Our systematic evaluation reveals key failure modes and areas requiring enhancement. We demonstrate AILA’s practical utility through three increasingly complex case studies: automated microscope calibration, high-resolution graphene step-edge imaging, and load-dependent roughness analysis on highly oriented pyrolytic graphite (HOPG).\n\n2. Results\n2.1 AILA framework\nAILA’s architecture prioritizes modularity, enabling seamless integration with diverse experimental and analytical platforms. At its core lies an LLM-powered planner—the framework’s cognitive centre—which orchestrates user interactions and coordinates specialized agents (Fig. 1a). For AFM operations, AILA deploys two agents: the AFM Handler Agent (AFM-HA) for experimental control and the Data Handler Agent (DHA) for analysis. The AFM-HA interfaces with a document retrieval system comprising AFM software documentation and a code execution engine that translates Python commands into experimental actions. A Python-based API establishes the hardware-software interface, enabling direct control of the AFM system through vendor-specific protocols (Fig. 1b). The DHA manages image optimization and analysis through dedicated tools: an Image Optimizer that fine-tunes PID parameters for high-fidelity imaging and an Image Analyzer that extracts targeted features from experimental data. For queries beyond agent capabilities, the planner generates alternative approaches or recommended actions. The technical specifications and implementation details of each module are explained in the Methods section.\n\nTo demonstrate AILA’s operational workflow, we present a multi-step experiment: acquiring an AFM image of HOPG and extracting its friction and roughness parameters (Fig. 1c). This open-ended task exemplifies real-world complexity, offering multiple solution pathways. Upon receiving the query, AILA dissects it into sequential objectives: image acquisition via AFM-HA followed by DHA-led analysis. AFM-HA retrieves relevant documentation, generates executable code, and captures the image. Following successful acquisition, AILA transitions control to DHA, which directs the Image Analyzer to compute the specified parameters. This orchestrated sequence exemplifies AILA’s core strengths: the ability to parse complex natural language queries, develop strategic workflows, and coordinate multiple agents toward achieving experimental objectives.\nFigure 1. AILA Framework and Implementation. (A) System Architecture of the Artificially Intelligent Laboratory Assistant (AILA). Dotted lines indicate adaptive information flow governed by AILA’s decision-making, and solid lines represent deterministic information pathways with predefined routing protocols. (B) Image of the atomic force microscope (AFM) experimental setup showing key hardware components and control interfaces. (C) Representative demonstration of AILA’s operation: raw transcript of a user query and AILA’s unedited response sequence, showing the system’s query interpretation, task planning, and execution capabilities.\n2.2 AFMBench: tasks for evaluating the AILA framework\n\nA Tool requirement\nAgent requirement\nB Operation type\nC\nD Documentation\nE\nTool Requirement: Single tool Operation Type: Basic\nAgent Requirement: Single agents Require: Analysis\nTool Requirement: Multiple tools Operation Type: Advanced\nAgent Requirement: Multiple agents Require: All\n\nFigure 2. Task Distribution and Module Utilization in AFMBench. A. Pie charts showing the distribution of tool requirements (left, single vs. multiple) and agent requirements (right, single vs. multiple) across benchmark tasks. B. Operation complexity categorization showing the proportion of basic versus advanced tasks. C. Horizontal bar chart quantifying module engagement frequency across all tasks, demonstrating utilization patterns of each tool and agent. D. Venn diagram illustrating the overlap between documentation, analysis, and calculation tasks. E. Representative examples of basic (left) and advanced (right) tasks, demonstrating increasing complexity in experimental workflows.\n\nAFMBench comprises 100 expertly curated experimental tasks (see S3.1 in Supplementary Information for a few examples of tasks; all the tasks are available in the GitHub repo) manually designed to rigorously evaluate autonomous AFM operations across multiple dimensions of complexity. Unlike conventional LLM benchmarks or simulation-based evaluations, each AFMBench task demands physical execution on AFM hardware, introducing real-world temporal constraints and experimental variability. Analysis of the task architecture reveals distinct patterns in resource utilization and operational complexity. In Figure 2A, tool coordination requirements highlight a systematic preference for sophisticated workflows, with\n69% of tasks demanding multi-tool integration, while 31% operate through single-tool protocols. Agent deployment analysis reveals a distribution: 83% of operations utilize single-agent protocols, while 17% require multi-agent coordination—enabling evaluation of both targeted expertise and system-wide integration capabilities.\n\nIn Figure 2B, the operational landscape is divided into two primary complexity tiers: basic operations (56%) encompassing fundamental microscopy tasks and advanced procedures (44%) requiring more sophisticated experimental workflows (for example questions see Figure 2E). Core system components—the AFM Handler, Document Retriever, and Code Executor—demonstrate maximum engagement, each activating in 66 distinct tasks. The Data Handler Agent and Image Analyzer exhibit selective activation patterns (52 and 48 tasks, respectively), while the Image Optimizer engages exclusively in critical parameter optimization scenarios (4 tasks).\n\nTask distribution across functional domains reveals three primary clusters: documentation (50 standalone tasks), analysis (14 tasks), and calculation (10 tasks) (see Figure 2D). A significant overlap between these domains emerges through integrated tasks that combine multiple functional requirements, reflecting the interconnected nature of experimental workflows. This carefully constructed distribution enables systematic evaluation of AI systems across a spectrum of experimental complexity—from basic instrument control to advanced multi-step procedures requiring mathematical reasoning and dynamic decision-making—effectively mirroring the cognitive hierarchy of expert atomic force microscopists.\n\n2.3 Performance of AI Agents\nSystematic evaluation of AILA using two advanced closed source language models—GPT-4o and GPT-3.5-turbo-0125—unveils distinctive execution patterns and operational efficacies. GPT-4o exhibits exceptional proficiency in documentation-centric operations, achieving a 92% success rate, complemented by robust execution in analysis (71%) and computational tasks (70%). The model’s strength lies in its ability to navigate interconnected workflows: 80% success in merged documentation-analysis procedures and 60% in documentation-computation sequences. These metrics highlight GPT-4o’s capacity to replicate the integrative reasoning characteristic of expert microscopists.\nFigure 3. Comparative Performance Analysis of Language Models on AFMBench. A. Venn diagrams showing accuracy (left) and efficiency (right) metrics for GPT-4o across documentation, analysis, and calculation tasks. Numbers indicate percentage accuracy and processing time in seconds. B. Corresponding performance metrics for GPT-3.5-turbo-0125, highlighting domain-specific competencies and processing speeds. C. A horizontal bar chart comparing tool and agent utilization efficiency between models is expressed as a percentage of successful engagements.\n\nIn marked contrast, GPT-3.5-turbo-0125 displays compartmentalized strengths: substantial accuracy in standalone documentation (72%), analytical interpretation (71%), and mathematical operations (40%). However, its performance degrades significantly when confronted with multi-domain challenges, registering null success rates in tasks demanding simultaneous expertise across domains. This limitation suggests insufficient development of cross-functional reasoning capabilities essential for autonomous experimentation.\n\nTemporal efficiency metrics augment these distinctions. GPT-4o maintains steady execution speeds: documentation tasks took an average of 12.23 seconds, analytical procedures 9.25\nseconds, and computational operations 11.06 seconds. GPT-3.5-turbo-0125 demonstrates irregular processing intervals: 8.88 seconds for documentation, 13.48 seconds for analysis, and 3.26 seconds for calculations. This temporal variability indicates underlying differences in task comprehension and execution strategies between the models.\n\nComponent utilization analysis reinforces these observations. GPT-4o achieves consistently elevated engagement across system modules, particularly excelling in AFM operation control and document interpretation. These results highlight the fundamental importance of model architecture in autonomous experimental platforms, with GPT-4o’s advanced integrative capabilities positioning it as the superior choice for sophisticated experimental automation.\n\n2.4 Error Analysis Reveals Model-Specific Limitations\nDetailed examination of failure cases revealed distinctive error patterns between the two language models, offering insights into their operational limitations. GPT-4o exhibits a total error rate of 20%, with errors distributed across three primary categories: code generation (60%), agent/tool selection (25%), and instruction adherence (15%). The predominance of code generation errors suggests challenges in translating conceptual understanding into executable commands despite the model’s strong performance in task comprehension.\n\nGPT-3.5-turbo-0125 demonstrates a markedly higher total error rate of 45%, with errors concentrated in two categories: code generation (66.7%) and agent/tool selection (33.3%). Notably, the model shows no fundamental query interpretation errors, indicating robust natural language processing capabilities. However, the elevated frequency of code generation errors, coupled with significant agent/tool selection failures, points to underlying deficiencies in translating comprehension into actionable experimental protocols.\n\nA critical finding emerged regarding GPT4o’s instruction adherence. In one of the three recorded errors, GPT-4o exceeded its designated operational limits, performing actions that were not authorized by the provided guidelines. For instance, it carried out potentially risky tip movements while it was only instructed to scan the surface (see S2.3 in the Supplementary Information). In another case, GPT-4o was instructed to capture an image and calculate surface friction. While the image was captured correctly, the system failed to analyse it and switches the AFM to the lateral force mode instead of following clear instructions for a specific task (see S2.3 in the Supplementary Information). Instead of staying within the scope of the task, it performed additional actions. Although sometimes the final result may have been correct, the failure to follow instructions highlights concerns about AI-agent behaviour and raises safety risks in automated lab environments. Similar to the observation of “hallucination” in LLMs\\(^{36}\\), these results present a unique challenge—SDLs tend to take arbitrary actions potentially based on memory rather than following the instructions, referred to hereafter as “sleepwalking”. These issues are especially critical in sensitive experimental settings, where strict protocol adherence is essential to ensure both equipment safety and the validity of results.\n\nThis error distribution illuminates critical areas for framework enhancement. While GPT-4o’s balanced error profile suggests the need for targeted improvements across multiple domains,\nGPT-3.5-turbo-0125’s concentrated error patterns indicate fundamental limitations in experimental execution capabilities. These findings underscore the necessity for specialized training in automated experimental systems, particularly focusing on the translation of scientific protocols into executable code sequences.\n\n2.5 Safety Alignment in SDLs\nTo understand the safety challenges37 of AI agents, we evaluate the effectiveness of implementing a safety framework in AILA. First, we establish restricted access protocols for critical AFM functions, coupled with ethical system prompts (see S2.1 in Supplementary Information) that constrain code generation to predefined documentation38. Second, we develop strict operational boundaries that permit dynamic code generation solely for image analysis while preventing external software installation or system modifications. Evaluation of the improved protocol demonstrates the effectiveness of these safeguards—AILA appropriately failed when prompted to install external Python libraries. (see S3.3 in Supplementary Information for complete validation logs). These findings underscore the critical importance of robust safety protocols in SDLs, emphasizing the necessity of comprehensive benchmarking and operational guardrails.\n\n![Pie charts comparing error mode distribution between GPT-4o and GPT-3.5-turbo-0125](page_682_1042_496_384.png)\n\nFigure 4. Error Mode Distribution in Model Performance. Error patterns between GPT-4o (top) and GPT-3.5-turbo-0125 (bottom). Segments represent a proportional distribution of error types: Instruction adherence (dark blue), agent/tool selection (gray), and code generation (light\ngreen). Central numbers indicate total error counts for each model, demonstrating significant differences in overall error rates (20 versus 45 errors, respectively).\n\n2.6 Pushing the Limits of Autonomous Experimentation\nFinally, to demonstrate AILA’s capabilities in real-world scenarios, we demonstrate three increasingly complex experimental tasks that typically require expert intervention: automated AFM calibration, high-resolution feature detection, and mechanical property measurement.\n\n2.6.1 AFM Parameter Optimization\nAFM imaging requires precise calibration of Proportional-Integral-Derivative (PID) gain values, which traditionally demand expert intervention due to the continuous nature of these parameters. This dependency on skilled operators presents a significant barrier to broader AFM adoption. We demonstrate AILA’s capability to autonomously optimize these parameters by minimizing the forward-backward scan differential on standard calibration grids. To this end, after loading the calibration sample, AILA was prompted to optimize the imaging parameters (see S4 in Supplementary Information for the complete prompt and output log). A total of 45 images are generated, with 3 images produced in each of the 15 generations. Figure 5A presents experimental AFM data acquired by AILA for the 1st and 15th generation of variable PID configurations, with corresponding line scan analyses that quantify trace-retrace symmetry. Initial scans with suboptimal parameters (P: 93-208, I: 1747-6623, D: 0-39) exhibit poor SSIM scores (0.392-0.768), manifesting as visible distortions in topographic data. Note that a higher SSIM value, closer to 1, indicates a perfect match, while a value of 0 represents no similarity. Through iterative optimization, AILA achieves superior scan quality (SSIM > 0.81) with optimized parameters (P: 246-249, I: 8676-8957, D: 17-30; see Figure 5A).\n\nThe genetic algorithm’s convergence efficiency is demonstrated in Figure 5C, where optimal PID configurations are achieved within 15 generations. Both maximum and mean SSIM values show rapid improvement, stabilizing above 0.8, indicating robust parameter optimization. Figure 5B validates the optimized parameters (P:249, I:8957, D:26) across a larger scan area, maintaining high-quality imaging across multiple grid features.\nFigure 5. Autonomous AFM experiments. A. Evolution of AFM image quality under varying PID parameters. The left panels show topographic images of the calibration grid; the right panels display corresponding line scan profiles (solid: trace, dashed: retrace). SSIM scores quantify trace-retrace correlation, with higher values indicating superior imaging quality. Optimal parameters (P: 249, I: 8957, D: 26) achieve SSIM = 0.818. B. Large-area scan demonstrating consistent imaging quality using optimized parameters across multiple grid features. C. Convergence plot showing genetic algorithm optimization efficiency. Red circles: maximum SSIM; black circles: mean SSIM per generation.\n\n2.6.2 High-Resolution Step-Edge Detection\nSurface characterization through AFM is challenged by noise sources such as thermal drift, mechanical vibrations, and electronic interference39–41, which can obscure subtle topographic features like graphene step edges. In this study, we leverage the advanced analytical capabilities of AILA to address these challenges using highly ordered pyrolytic graphite (HOPG) as a model system. AILA autonomously determines the necessity for baseline correction based on feature size, recognizing that baseline artifacts predominantly affect smaller features. For instance, in the raw image (Figure 6A), the graphene step edge remains indiscernible due to\nbaseline distortions. AILA applies a fifth-order polynomial baseline correction to generate the 1st generation image (Figure 6A), which serves as the foundation for PID gain optimization. Following a process similar to the calibration grid optimization, the image is refined through iterative PID adjustments, resulting in the final optimized image in the 10th generation, where atomic steps become distinctly visible. The automated optimization process surpasses conventional manual adjustments, offering an enhanced resolution of nanoscale features. Additionally, further analysis of the processed data, including the determination of graphene step height, was facilitated through specific prompts, with the prompts and results detailed in the Supplementary Information S4.\n\n![High-resolution HOPG imaging demonstrating baseline artifact challenges. Top panels: topographic images at different Z ranges; bottom panels: corresponding line profiles revealing surface features. Left: HOPG images obtained using setpoints of 0.2 V and 0.4 V, both manually captured and taken by AILA with GPT-4o. Right: Plot showing the relationship between setpoint and average friction.](page_184_370_1080_563.png)\n\nFigure 6. Autonomous AFM experiments. **A.** High-resolution HOPG imaging demonstrating baseline artifact challenges. Top panels: topographic images at different Z ranges; bottom panels: corresponding line profiles revealing surface features. **B.** Left: HOPG images obtained using setpoints of 0.2 V and 0.4 V, both manually captured and taken by AILA with GPT-4o. Right: Plot showing the relationship between setpoint and average friction.\n\n**2.6.3 Load-dependent roughness measurement**\nWe conduct a comprehensive load-dependent roughness analysis of HOPG. The experiment requires iterative adjustments of AFM parameters, including setting a range of setpoints, capturing images, and analyzing the corresponding friction data. Manually performing this\nprocedure is time-intensive, involving parameter modifications, image acquisition, data extraction, and result plotting. To streamline this process, we utilize AILA to automate the experiment.\n\nAILA was instructed (see S4 in Supplementary materials for the complete prompt and output log) to vary the setpoint voltage from 0.2 V to 1.2 V in increments of 0.2 V. At each setpoint, AILA independently captured the AFM image, calculated the average friction value, and generated the corresponding plot. Figure 6B presents the graph of average friction versus setpoint voltage for both manually obtained and AILA-captured images using the GPT-4o model. The raw images generated by AILA can be found in the Supplementary Information Figure S2. The entire process was conducted without additional user input regarding figure formatting or parameter settings. Remarkably, AILA autonomously develops the required Python script, executes the experimental protocol, and generates the output, including raw, unedited plots. This automation significantly reduces the time and effort compared to manual execution. The results not only validate the capability of AILA in handling complex AFM experiments but also demonstrate its efficiency in generating reproducible and high-quality outputs for scientific analyses.\n\n3. Discussion\nAILA’s evaluation of AFMBench reveals quantifiable distinctions between LLM capabilities in experimental automation. The performance gap between GPT-4o and GPT-3.5-turbo-0125 in cross-domain operations (80% versus 0% success in hybrid tasks) quantifies a key requirement for autonomous laboratories: integrated experimental reasoning. Single-domain competence, while necessary, proves insufficient for replicating expert-level experimental workflows. This disparity in cross-domain integration particularly manifests in complex scenarios, requiring simultaneous optimization of imaging parameters and data analysis—tasks routinely performed by experienced microscopists.\n\nError pattern analysis identifies a persistent challenge: protocol-to-execution translation. Code generation errors dominate failure modes (60-67%) across both architectures, establishing a primary bottleneck in experimental automation. This systematic limitation persists even in advanced models, suggesting architectural constraints beyond mere computational capability. The distribution of error types—particularly the presence of instruction adherence errors (15%) in GPT-4o versus their absence in GPT-3.5-turbo-0125—reveals nuanced differences in model behavior that warrant further investigation regarding the safety and alignment issues associated with the LLMs. It is worth noting that AI-agent based on GPT-4o, a model known for its reasoning capabilities, exhibit tendencies to perform actions beyond what is instructed, termed as “sleepwalking”. Note that depending on the nature of the LLM, “sleepwalking” could result in potentially harmful outcomes in SDLs when dealing with highly dangerous chemicals or conditions such as high temperature pressure to name a few.\n\nAILA’s modular design establishes quantifiable metrics for autonomous system development. The successful automation of AFM operations validates this architecture for complex\ninstrumentation control, demonstrating efficacy in parameter optimization and feature extraction tasks. The measured limitations in tool coordination depending on the LLMs define specific thresholds for improving inter-module communication protocols. Notably, the agent deployment ratio (83:17 single-to-multi-agent) establishes an empirical baseline for balancing specialized and integrated operations—a metric applicable to automation across analytical platforms, from mass spectrometers to X-ray diffractometers.\n\nThese findings suggest specific architectural improvements for next-generation autonomous laboratories. Enhanced integration protocols between specialized agents could address the observed limitations in multi-tool coordination. Similarly, dedicated code generation modules might mitigate the predominant error mode, potentially incorporating specialized scientific programming frameworks.\n\n4. Outlook\nAltogether, AILA demonstrates quantifiable advances in experimental automation through systematic benchmarking. The framework’s comprehensive performance metrics in AFM operations establish standards for autonomous laboratory evaluation, while AFMBench introduces reproducible protocols for systematic assessment across experimental domains. Successful execution of complex tasks—from automated image optimization to nanomechanical measurements—validates the framework's capabilities for sophisticated materials characterization. However, the observed tendencies of LLM agents to exceed operational boundaries and perform “sleepwalking” while carrying out the experiments raise significant safety concerns. This behavior, reported for the first time to the best of that authors’ knowledge, emphasize critical areas for development in instruction alignment and operational safety.\n\nThis work’s implications transcend materials characterization. The empirically validated principles—modular architecture (69% multi-tool efficiency), strategic agent deployment (83:17 ratio), and cross-domain integration (80% hybrid task success)—establish design parameters for autonomous laboratories across disciplines. Applications span pharmaceutical screening, environmental monitoring, and process optimization. For instance, the documented success in parameter optimization could translate directly to automated high-throughput drug screening or catalyst discovery platforms. While current limitations in code generation (60% error rate) and tool coordination (31% efficiency) define immediate development targets, these metrics provide clear objectives for advancing autonomous scientific platforms. The path forward requires focused development in three key areas: enhanced cross-domain reasoning capabilities, robust code generation protocols, and sophisticated multi-agent coordination mechanisms. Success in these domains would enable truly autonomous scientific platforms capable of accelerating discovery across the scientific landscape.\nMethodology\nAILA\nAILA is constructed utilizing the LangChain software framework, incorporating components such as prompts, LLMs, memory, agents, and tools. AILA uses two categories of prompts: system prompts (see S2.1 in Supplementary Information for the system prompts) and user prompts. System prompts define ethical rules for AILA’s interactions and describe the responsibilities assigned to each agent, whereas user prompts are variable inputs provided by end-users. AILA’s backbone consists of LLMs, namely GPT-4o and GPT-3.5-turbo-0125, which process user input as strings and provide string-based outputs. These LLMs are stateless, indicating that they do not save conversational context. Here, all interactions and agent states are stored in a Python dictionary and can be accessed by other agents. AILA consists of two specialized agents: the AFM Handler Agent and the Data Handler Agent, both equipped with unique tools to do specific tasks. These agents possess individual prompts, LLMs, and tools; however, they utilize a shared memory to store and access states, facilitating smooth interaction. The system prompts within the agents offer instructions for tool utilization and ethical guidelines, whereas the outputs from other tools or agents serve as user prompts. The framework utilizes LangGraph, a library that allows the construction of an effective multi-agent workflow, integrating all agents and tools seamlessly.\n\nThe architecture for AILA’s decision-making process is carefully designed to ensure precise information routing. AILA can dynamically select among three primary options: AFM Handler, Data Handler, or FINISH. When AILA identifies the appropriate agent to handle a query, it routes the information to the selected option. In cases where AILA determines that none of the available agents can sufficiently address the question, it generates a well-structured response and selects the FINISH option to conclude the session effectively. The agents within this system are equipped with three distinct operational choices: utilizing their respective tools, transferring information to the next agent, or terminating the session. A system prompt has been integrated to streamline these decisions. Agents append the prefix NEED HELP to their response when transferring information to another agent. Alternatively, if they believe the query has been adequately addressed, they use the prefix FINAL ANSWER to signal the session’s conclusion. By analyzing the output for these keywords, the system seamlessly routes the response to the designated agent or tool or finalizes the session. This structured approach enables efficient multi-agent collaboration, ensuring clarity, accuracy, and optimal performance across tasks while maintaining a robust and adaptive framework.\n\nAFM Handler Agent\nAtomic Force Microscopy demands precise sequential execution of multiple experimental stages. Image acquisition requires optimization across three critical parameters: imaging conditions, probe selection, and operational mode configuration (tapping/contact). The experimental sequence encompasses surface approach protocols, scanning procedures, and standardized data acquisition—with procedural deviations potentially resulting in equipment damage or data corruption. Our implementation utilizes the DriveAFM instrument (Nanosurf), which is accessed through a Python-based API architecture and designed for universal compatibility with API-enabled AFM systems. To facilitate AFM imaging experiments, we\nhave created the AFM Handler agent, which is integrated with two specialized tools: the Document Retrieval Tool and the Code Executor Tool. Every tool has an individual role, and the AFM Handler agent can dynamically assign tasks to these tools. The agent will assign the responsibility to the Data Handler agent if it finds that neither tool can handle the task.\n\nDocument Retrieval tool\nThe documentation for the instrument offers detailed instructions on how to handle and calibrate it. However, providing full access to the documentation to an LLM entails risks, such as inadvertent alterations to factory settings or calibration data, which could potentially result in damage or malfunction of the instrument. To address this concern, we manually extracted the essential information from the AFM documentation necessary for conducting experiments while safeguarding the instrument’s integrity. We consolidated all the crucial codes for regulating each parameter of the instrument into a comprehensive Python script. Since Python code relies heavily on precise indentation and line structure, we utilized the Recursive Character Text Splitter from the LangChain library, specifically designed for Python, to divide the script into manageable chunks. The chunk size was set to a maximum of 1000 characters without overlap, adhering to the token limit for embedding models. Each code chunk comprises three sections: the first includes the necessary Python libraries, the second contains the code required to load the application, and the third section features unique Python code specific to the given task. The first two sections are consistent across all chunks (see S2.2 in the Supplementary Information file for more details). These chunks were then combined to generate a document, embedded using OpenAI’s text-embedding-3-large model. This model, with the capability of producing embeddings of size up to 3072 dimensions, delivers exceptional performance compared to other OpenAI embedding models, especially in multi-language retrieval benchmarks like MIRACL\\(^{42}\\). To store the embeddings, we opted for Chroma, an open-source vector database known for its reliability and efficiency in managing large-scale embedding data. We use a vector store retriever to retrieve the data from the vector store.\n\nCode Executor tool\nA code executor tool has been developed to execute Python scripts generated by the AFM Handler Agent to control the AFM software. This tool is intended to run Python code, provided as a text string, directly on the local system to allow for smooth integration with the workflow of the AFM Handler Agent. The utility executes the code and sends back a success message or a detailed description of the error that occurred. If there is an error, the error message is returned to the AFM Handler agent so it can correct the error and retry executing. Otherwise, if the script runs without errors, it is considered the final result. This iterative process ensures precise control of the AFM system while systematically addressing any issues in the script.\n\nData Handler Agent\nSurface tracking optimization in AFM requires precise calibration of three fundamental parameters: Proportional (P), Integral (I), and Derivative (D) gains. Optimal calibration manifests as convergence between trace and retrace signals, indicating stable scanning conditions. The Data Handler agent interfaces with specialized optimization and analysis\nmodules; these models can access AFM image data stored in local storage systems. The agent can optimize P, I, and D gains or calculate various surface properties, such as average friction and surface roughness, using the help of modules and image files stored locally.\n\nImage Optimization Tool\nThe feedback system in an Atomic Force Microscope (AFM) plays a crucial role in maintaining control over the interaction between the cantilever tip and the sample surface. During scanning, variations in surface features alter the interaction forces between the tip and the sample, leading to deflections in the cantilever. These deflections are detected by a photodetector. To ensure that these deflections stay within a specified range, the feedback mechanism continuously adjusts the height of either the tip or the sample stage in real time. This process is managed by a PID (Proportional-Integral-Derivative) controller, which regulates the position of the z-piezo actuator. By moving the cantilever probe up or down, the controller maintains a steady interaction force or adheres to a predefined setpoint, depending on the chosen mode of operation.\n\nFine-tuning the P, I, and D gain values of the controller is vital for achieving accurate control of the setpoint in AFM imaging. The integral gain is especially important for enhancing image clarity by mitigating drift and reducing steady-state errors. Once the integral gain is optimized, adjusting the proportional gain can provide further refinement. The derivative gain, on the other hand, is particularly beneficial for imaging samples with pronounced edge features. If the gains are set too low, the PID loop may fail to maintain the setpoint effectively, while excessively high gain values can introduce electrical noise into the image due to amplified feedback or overcompensation for deviations. Properly optimized PID parameters ensure that the feedback loop remains stable and responsive, enabling the AFM to accurately track surface topography, even at higher scanning speeds. This balance is especially critical when imaging delicate, irregular, or soft materials, as it preserves the integrity of tip-sample interactions.\n\nA genetic algorithm (GA) was employed for PID gain optimization. The GA parameters included a fixed population size of three and a total of 15 generations, enabling efficient tuning of the gains. Although these parameters can be manually adjusted, but excessive image scanning may degrade the AFM tip. The optimized gains ensure effective feedback control, producing comparable forward and backward images. This can be achieved by calculating the mean squared error (MSE) between forward and backward z-axis images for various PID gain settings. However, this method is sensitive to drift during scanning, and this method also depends on previously acquired images. To address this, the structural similarity index (SSIM) was adopted as the fitness function in the genetic algorithm, providing a robust measure of image similarity between the z-axis forward and backward image independent of prior image data.\n\nThis metric offers advantages over traditional Mean Square Error (MSE) approaches by (i) addressing tip degradation challenges in contact-mode AFM by minimizing required scan cycles and enabling optimization using low-resolution images, (ii) maintaining accuracy under drift conditions, (iii) incorporating structural, brightness, and contrast variations in\noptimization, and (iv) providing normalized scores between 0 and 1, where 1 indicates perfect similarity.\n\nThe SSIM is defined as:\n\\[\nSSIM(x, y) = [l(x, y)]^\\alpha \\times [c(x, y)]^\\beta \\times [s(x, y)]^\\gamma\n\\]\nwhere, \\( l(x, y) \\) is the luminance comparison, \\( c(x, y) \\) is the contrast comparison, and \\( s(x, y) \\) is the structure comparison with \\( \\alpha, \\beta, \\gamma \\) being the weighting parameters. Note that the individual components are defined as:\n\\[\nl(x, y) = (2\\mu_x \\mu_y + C_1)/(\\mu x^2 + \\mu y^2 + C_1)\n\\]\n\\[\nc(x, y) = (2\\sigma_x \\sigma_y + C_2)/(\\sigma_x^2 + \\sigma_y^2 + C_2)\n\\]\n\\[\ns(x, y) = (\\sigma_{xy} + C_3)/(\\sigma_x \\sigma_y + C_3)\n\\]\nwhere, \\( \\mu_x, \\mu_y \\) represent the mean intensities of images \\( x \\) and \\( y \\), \\( \\sigma_x, \\sigma_y \\) is the standard deviations of images \\( x \\) and \\( y \\), \\( \\sigma_{xy} \\) is the cross-covariance between images \\( x \\) and \\( y \\), and \\( C_1, C_2, C_3 \\) are constants to avoid instability with (\\( C_1 = (k_1 L)^2, C_2 = (k_2 L)^2, C_3 = C_2 / 2 \\)) and \\( L \\) being the dynamic range of pixel values and \\( k_1 = 0.01 \\) and \\( k_2 = 0.03 \\).\n\nBaseline correction\nThe adaptive baseline correction employed in the step-edge detection of graphene is given by\n\\[\nB(x, y) = \\Sigma_{i,j} a_{ij} x^i y^j\n\\]\nWhere, \\( B(x, y) \\) is the baseline function, \\( a_{ij} \\) are the polynomial coefficients, \\( i \\) and \\( j \\) are the polynomial degrees (\\( 0 \\leq i, j \\leq n \\)) with \\( n \\) being the maximum polynomial degree.\n\nImage Analysis tool\nAFM instrument stores the image data as a *.nid file in the local system. This *.nid file contains deflection, friction force, and z-axis images for both backward and forward scans. To further process any image from the file, exact data must be extracted from the file. To conduct this, we have used the NSFopen python library in the Image Analysis tool, which takes the query from the data handler agent regarding the specific image data and its location and returns the image data in an array to the data handler tool. To conduct further processing of the images, any Python script generated by the data handler tool can be executed in the Image Analysis tool, and the result can be returned to the data handler agent. Note that there is no database available to guide the LLM model in generating the Python script. It can generate the Python script by itself. There is a total of 6 input parameters for this tool:\n(1) path (str): Directory path to search for the latest file (default: None).\n(2) filename (str): Specific image file to display (default: None).\n(3) dynamic_code (str): Python code for processing image data (default: None).\n(4) calculate_friction (bool): Option to compute average friction (default: False).\n(5) calculate_mean_roughness (bool): Option to compute mean roughness (default: False).\n(6) calculate_rms_roughness (bool): Option to compute RMS roughness (default: False).\nReturns: A dictionary with the status, image data, or error details.\nAverage friction was calculated using the following formula:\n\\[\nF_{ave} = \\frac{1}{2} \\times (f_{ij} - b_{ij})\n\\]\nWhere \\( f_{ij} \\) and \\( b_{ij} \\) are the element at position \\((i,j)\\) in the array of the forward and backward friction image data. We have used the formula in this tool to calculate the mean roughness and RMS roughness values\n\n\\[\nR_{mean} = \\frac{1}{M.N} \\sum_{i=1}^{M} \\sum_{j=1}^{N} |z_{ij} - \\bar{z}|\n\\]\n\n\\[\nR_{rms} = \\frac{1}{M.N} \\sum_{i=1}^{M} \\sum_{j=1}^{N} (z_{ij} - \\bar{z})^2\n\\]\n\nwhere \\( z_{ij} \\) is the element at position \\((i,j)\\) in the array, \\( \\bar{z} \\) is the mean of all elements in the array, \\( M \\) is the number of rows in the array, N is the number of columns in the array of the z-axis forward image data.\n\nAFMBench\nDataset preparation. To evaluate the performance of the AILA, we have manually created a set of 100 questions, carefully categorized into three distinct groups. The first classification is based on whether a question requires one or multiple tools/agents to be solved. The second category assesses the complexity of the questions, distinguishing between basic and advanced levels. Lastly, the questions are grouped by their requirements, such as documentation analysis or calculations. The complexity of each question is determined by the number of agents involved and the steps required to achieve the solution. For instance, modifying a parameter in an AFM system typically requires documentation review and the use of a single agent, categorizing it as a basic task. Conversely, capturing an AFM image and analyzing its surface roughness involves multiple agents, documentation analysis, and calculations, making it an advanced task. A comprehensive JSON file has been created, encapsulating detailed metadata about each question, including its respective category, for streamlined analysis and evaluation. This file serves as a structured resource for further investigations and testing. All questions, along with their relevant classifications and details, have been made accessible on GitHub (https://github.com/M3RG-IITD/AILA) to support transparency and reproducibility in research.\n\nEvaluation\nWe developed a graphical user interface (GUI) using Streamlit, an open-source Python framework, to streamline user interaction with AILA. The GUI allows users to input text-based queries, select the desired LLM model, and specify a log file name. It then executes AILA in the backend, saving the output log file locally and enabling users to observe results directly within the AFM software. Any output images or figures generated by AILA are also stored in the local system for further analysis. To ensure robustness, we manually evaluated all questions using GPT-4o and GPT-3.5-turbo-0125, verifying the output log files and AFM software results multiple times in collaboration with different researchers to eliminate potential human errors. The evaluation of AILA’s performance was categorized into two metrics: accuracy and\nefficiency. For accuracy, questions were divided into categories based on complexity and tool/agent usage, with a percentage of correct answers calculated for each category. For efficiency, uniform parameters were maintained across models in the AFM software, including default settings of 0.1 seconds for time per line and 128 points per line and frame when not specified by the user. To ensure precise efficiency measurements, scanning time for images and the time taken by questions with incorrect answers were excluded from the analysis. Average response times were computed for each category to assess AILA’s overall efficiency.\n\nEvaluation Metric\nTo assess the evaluation of questions in terms of accuracy, we classified the answers provided by AILA into two categories: fully correct answers and incorrect or partially correct answers. A fully correct answer was considered accurate, while any incorrect or incomplete response was deemed incorrect. Given that some questions require manual inspection of the AFM software to verify whether specific parameters are set correctly and whether the AFM image is captured as intended, multiple researchers were involved in verifying the results. They carefully checked the outcomes to ensure error-free results. For measurements of different properties, such as average friction, roughness, and RMS value of roughness, we used the Gwydion software to verify the accuracy of the results. Subsequently, the questions were clustered into appropriate groups, and the corresponding average percentage of correct answers was calculated.\n\nData and Code Availability\nAll the tasks in AFMBench, along with the complete log files of the responses for each of the tasks from GPT-4o and GPT-3.5 are available at: https://github.com/M3RG-IITD/AILA\n\nAcknowledgement\nN.M.A.K. acknowledges the funding support from Google Research Scholar Award, and the Alexander von Humboldt Foundation. I.M. thanks University Grants Commission (UGC), Government of India for the NET-JRF fellowship (221610021768). The authors thank IIT Delhi HPC facility for computational and storage resources.\n\nReferences\n\n1. Zhao, Z., Lee, W. S. & Hsu, D. Large language models as commonsense knowledge for large-scale task planning. Advances in Neural Information Processing Systems **36**, (2024).\n\n2. 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Click to download.\n\n• SupplementaryMaterials.pdf"} {"paper_id": "prb4", "title": "Prediction of Transition State Structures of General Chemical Reactions via Machine Learning", "text": "Prediction of Transition State Structures of General Chemical Reactions via Machine Learning\n\nSunghwan Choi (sunghwanchoi@kisti.re.kr)\nKorea Institute of Science and Technology Information https://orcid.org/0000-0002-4330-7710\n\nArticle\n\nKeywords: Transition state, Machine learning, Reaction path, Chemical reaction\n\nPosted Date: September 29th, 2022\n\nDOI: https://doi.org/10.21203/rs.3.rs-2082595/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\nPrediction of Transition State Structures of General Chemical Reactions via Machine Learning\n\nSunghwan Choi1*\n\n1*Division of National Supercomputing, Korea Institute of Science and Technology Information, 245 Daehak-ro, Yuseong-gu, 34141, Daejeon, Republic of Korea.\n\nCorresponding author(s). E-mail(s): sunghwanchoi@kisti.re.kr;\n\nAbstract\nThe elucidation of transition state (TS) structures is essential for understanding the mechanisms of chemical reactions and exploring reaction networks. Despite advances in computational approaches, TS searches remain still a challenging problem due to the difficulty of constructing an initial structure and heavy computational costs. Herein, a novel machine learning (ML) model for predicting TS structures of general organic reactions is proposed. The proposed model derives interatomic distances of a TS structure from atomic pair features reflecting reactant, product, and linearly interpolated structures. The model shows excellent accuracy, particularly for the atomic pairs where bond formation or breakage occurs. The predicted TS structures result in a high success ratio (93.8%) of quantum chemical saddle-point optimizations, and 88.8% of the optimization results have energy errors of less than 0.1 kcal/mol. Additionally, as a proof-of-concept, exploring multiple reaction paths of an organic reaction is demonstrated with the ML inferences. I envision that the proposed approach will aid the construction of initial geometry for TS optimization and reaction path explorations.\n\nKeywords: Transition state, Machine learning, Reaction path, Chemical reaction\n1 Introduction\n\nA transition state(TS) is essential to understanding chemical reactions and reaction networks.[1–3] In principle, the characteristics of chemical reactions are determined not by a specific molecular conformation, but by molecular trajectories that are affected by the entire potential energy surface (PES). Various advanced computational methods have been proposed to effectively simulate the molecular trajectories of chemical reactions.[4–8] However, because of the tremendous computation costs of obtaining accurate PESs and trajectories, elucidations of chemical reactions still rely heavily on classical TS theory.[9, 10] The TS theory is used to derive many reaction properties from a TS, a saddle-point on PES.[11, 12]\n\nExperimentally capturing TS structures is hardly accessible owing to their transient nature. In contrast, they can be accurately determined by computational methods. Over the last five decades, various quantum chemical methods using the first and second derivatives of energy with respect to atomic coordinates have been proposed to accurately capture a saddle-point in PES.[13–16] These methods can be used to reliably determine the TS of target reaction based on a given initial structure. However, they demand precise chemical knowledge on a target reaction to build an initial conformation. Because of the high complexity of PESs and the high sensitivity of quantum chemical calculations to the initial structures, dozens of numerical experiments may be required to design an appropriate initial structure, even for trained chemists. This repetitive trial and error is one of the hurdles to calculate TS structures, along with the high computational cost of quantum chemical methods.\n\nOn the other hand, machine learning (ML) techniques are broadly applied in many contexts of chemistry to build chemical knowledge from a wide database.[17–19] By the introduction of various neural network architectures, many molecular and reaction properties (e.g. molecular energy and activation barrier) are accurately predicted.[20–23] Despite those advances of ML techniques, a prediction of 3-dimensional(D) molecular structure is not easily achievable because the inferred 3D structures need to satisfy not only the permutation invariance with respect to the atom order but also physical (rotational and translational invariances) and Euclidean (triangle inequality) constraints.\n\nRecently, researchers have developed ML architectures that can predict TS structures while preserving these conditions. Pattanaik et al.[24] used a graph neural network to generate the initial interatomic distance and weight matrix from interatomic distances of reactant and product structures. This model, referred to as TSGen hereinafter, adopt internal nonlinear optimization to fine the atomic positions with the closet interatomic distance matrix to the initial one. A second model, TSNet was released by Jackson et al.[25] This model is based on a tensor-field network that applies spherical harmonics as convolution filters to distinguish relative atomic positions and directly predicts the atomic positions of TS structures.[26] These ML architectures mathematically preserve the conditions for determining TS structures. To achieve further\nimprovements on quality of prediction, a specialized ML model for a specific reaction type can be introduced.[27] However, the applicable range of specialized ML models are limited to the reaction with the same mechanism. Hence, these models cannot be suitable approach for exploring the chemical reaction space.\n\nHere, a novel ML model that infers TS structures of general single-step reactions is proposed and it is used to find multiple TSs that yield the target reactant and product. Using two organic reaction databases, it is confirmed that the proposed model outperforms existing models particularly for predicting the rarely distributed cases (e.g. bond formation or breakage). In addition to estimating the error of predicted distances, the quantum chemical calculations are performed to measure the chemical validity of the predicted TS structures. The most predicted TS structures converge to saddle-points, and their energies have high agreement with the reference energy. Additionally, by utilizing ML predictions of TS structures, a fast TS finder is implemented.\n\n2 Results\n\n2.1 Prediction accuracy\n\nSchematic representations of the proposed model architecture and its inference procedure are present in Fig. 1. The model is designed to predict the interatomic distances of TS structures from three molecular structures: reactant, product and their linear interpolation. Each structure is featurized as a set of atomic pair features. The pair features of three structures are constructed by concatenating features from two atomic numbers and an interatomic distance (\\( d_{ij} \\)). The sets of pair features from reactant, product and linearly interpolated structures are marked with green, red and purple round boxes. These sets of pair features are updated by pair sequence interaction (PSI) layers without loss of permutation-invariance and size-extensivity. Figure 1 (b) represents PSI layer which consists of two different components; transformer encoder and bidirectional gated recurrent unit (GRU) layers. The transformer encoder updates the pair features by reflecting only a set of pair features belonging to one structure whereas the following bidirectional GRU updates the feature by considering the same pairs in different structures. From the updated features of the interpolated structures(\\( f^{l,\\text{pair}}_{ij} \\)), the model predicts the normalized distances of TS structures by those of the interpolated structure (\\( d^{TS}_{ij}/d^{l}_{ij} \\)). Further details of the model architecture and training are provided in Section 4.2.\n\nThe model outputs are then converted to the predicted interatomic distances (\\( d^{TS}_{ij} \\)) and used to generate the atomic positions in the TS structures (\\( X^* \\)) by nonlinear optimization. As shown in Fig. 1 (c), the nonlinear optimization determines the atomic positions by minimizing the difference between the predicted and reconstructed interatomic distances. To mitigate the effects of prediction errors on the results of nonlinear optimization, the inferences from the trained ML models can be utilized, which named ensemble method. Here,\nFig. 1 Schematic representations of machine learning model. (a) Overall machine learning procedure utilizing reactant, product and linearly interpolated structures. (b) Illustration of pair sequence interaction layer. (c) The predicted interatomic distances are used to reconstruct three-dimensional atomic positions by nonlinear optimization. For ensemble predictions, results from multiple models can be utilized in a single nonlinear optimization.\n\n90 trained models are employed for ensemble predictions. For both single-model and ensemble cases, the linearly interpolated structure is used for a initial geometry of the nonlinear optimization. The details of the ensemble predictions are explained in Section 4.5.\n\nThe proposed model is trained and validated using the organic reaction database released by Grambow et al.[28] Figure 2 plots the test errors of the single-model and ensemble prediction results in terms of two metrics: molecular mean absolute error (MAE) and molecular mean absolute percentage error(MAPE). Molecular MAE is appropriate for estimating overall deviations of bond distances. However, in terms of chemical aspects, errors in interatomic distances are not fairly important; while relatively large errors can be tolerated at sufficiently long interatomic distances, even small errors can be critical to the TS structure if they occur in the chemical bonding region. Therefore, to sensitively reflect errors at small distances, a new metric, molecular MAPE, is introduced. The mathematical definitions of both metrics are present in Section 4.3.\n\nThe error of the outputs of the single-model and ensemble include 3.681% and 3.407% (molecular MAPE), respectively, and 11.56pm and 10.70pm\nFig. 2 Accuracy of trained models for predicting interatomic distances. (a) Molecular mean absolute error (MAE) and (b) molecular mean absolute percentage error (MAPE) of single-model, ensemble, and comparison model results. The red, orange, and yellow bars represent the magnitudes of errors from direct inferences, test-time augmentation(TTA), and TTA with nonlinear optimization (NLOpt). The last row in each table lists the test errors of ML models proposed by other groups. Both comparison models are trained with the same database as the database used for training of the proposed model.\n\n(molecular MAE), respectively. The error is reduced further by test-time augmentation (TTA), which is a useful ML technique for mitigating the variance of inference without additional training costs.[29, 30] In this study, the augmentation of chemical reactions is performed by reversing the their direction, and the inference results from the forward and backward reactions are averaged. This equates to averaging the TS structures of the forward and backward reactions, which should be identical from a chemical perspective. Thus, in addition to the improvement of prediction accuracy, TTA eliminates order-dependence of outputs according to the direction of a chemical reaction.\n\nThe interatomic distances obtained from ML inferences are highly accurate; however, they do not directly correspond to reliable 3D TS structures. Fortunately, by nonlinear optimization using the results of inferences, accurate molecular geometries whose errors in the interatomic distances are less than those of both single-model and ensemble results are obtained. This indicates that the remaining error on the predicted distances can be mitigated by constraining a set of interatomic distances to satisfy the Euclidean condition.\n\nTo compare the performances against the other ML models, two existing models, TSGen and TSNet, are trained with the same train dataset.[24, 25]. TSGen exhibited slightly better performance than TSNet. However, both models showed more than two-fold greater errors (for both error metrics) compared with the proposed model.\nFig. 3 Error analysis of machine learning predictions. (a) Average values of absolute percentage errors of four interatomic pairs depending on bond change types during a reaction. Blue, green, and black bars represent the prediction errors from TSNet, TSGen and the ensemble approach, respectively. The percentages in parentheses represent the ratio of the type of interatomic pair in the entire training set. The presence and absence of chemical bond in reactant and product is simplified as whether an interatomic distance is less than 156.6pm or not. (b) Absolute percentage errors and numbers of atomic pairs with different element sets according to a length of interatomic distance. The dotted, dashed, and solid lines show the average error of TSNet, TSGen and the ensemble predictions, respectively. The bars represent the frequencies of distances in the training set by atomic numbers. The red line indicates 156.6pm, which is criteria for the presence of a chemical bond.\n\nFor detailed error analysis, Fig. 3 (a) plots the averages of the absolute percentage error for four different categories of atomic pairs. The first category, which is the most common in the database, corresponds to atomic pairs that are not bonded in either the reactant or product. The second and third categories correspond to atomic pairs that undergo bond formation and bond breakage, respectively. The last category corresponds to the atomic pairs that are bonded in both the reactant and product. Because only a limited number of bond changes occurs in single-step reactions, the second and third cases are relatively rare (1.27% and 1.96% of all interatomic pairs in the training set, respectively). Despite the limited number of the pairs belonging to the second and third categories, the ensemble predictions achieve ~5% errors on the both categories while two comparison models record more than 15% errors. In the prediction of TS structures, determining interatomic distances that induce\nchemical bond formation and breakage are essential. The comparison models failed significantly in these cases.\n\nTo observe the dependency of the model accuracy on the size of the interatomic distances and atomic numbers, changes of absolute percentage errors and frequencies of atomic pairs in the database are shown in Fig. 3 (b). The colored bars represent the distributions of ten different combinations of atomic pairs at intervals of 4.125pm. The dotted, dashed, and solid black lines show the absolute percentage errors of the interatomic distances using TSNet, TSGen, and the ensemble approach. The points at the shown lines are obtained by averaging the percentage errors of all training interatomic distances belonging to the same interval to the bars. The red line represents the criteria for chemical bond, 156.6pm, which is used for determining the category of each atomic pair.\n\nIn Fig. 3 (b), large absolute percentage errors are commonly observed in the three ML predictions where interatomic distance are rarely distributed. Especially, in the bonding region, all models record relatively high error except around 105pm and 150pm regions in which a large number of C–H and C–C bonds are distributed. Despite this common trend, the proposed model outperforms both TSNet and TSGen throughout the entire distance range. Even for the atomic pairs in the bonding region, at most 6% of errors are observed in the ensemble prediction while the comparison models record up to 15% or more errors. This analysis confirms that the proposed model provides reliable predictions for all types of atomic pairs, particularly for those atomic pairs that have chemical bond bonding and participate reactions. In addition, it has a high accuracy for atomic pairs consisting of infrequently distributed elements.\n\nTo investigate the applicability of the proposed approach, the model is trained using the S_{N}2 database, which was published by the authors of TSNet.[25] For S_{N}2 reactions, the proposed ensemble approach recorded 4.54pm (molecular MAE) and 1.738% (molecular MAPE). For the S_{N}2 reaction database, the best-reported MAE is 18.31 pm using the TSNet model.[25] Because the used definition of error is slightly different from the molecular MAE, if the same definition is applied, the error of the ensemble results becomes 4.97pm. Consequently, the proposed model shows is more than three times as accurate as the TSNet model. In fact, the model based on PSI layers achieved overwhelming accuracy in both experiments. The proposed model utilize linearly interpolated structure in two aspects; normalization of interatomic distances for output values and construction of input features. As aforementioned, the interpolated structure provides reliable interatomic distances for rarely distributed cases so that the proposed model can result in the refined interatomic distances for those rare atomic pairs.\n\nTo estimate chemical validity of the predicted TS structures, quantum chemical simulations are performed. Although the S_{N}2 database includes many realistic chemical reactions, the validation based on quantum chemical calculations is only conducted for only the database released by Grambow et al.[28] because of the small size of S_{N}2 database.\n2.2 Quantum chemical validation\n\n![Quantum chemical validation results of predicted transition state structures](page_184_370_1062_563.png)\n\nFig. 4 Quantum chemical validation results of predicted transition state structures (a) Distributions of molecular MAPE of inferred and quantum chemically optimized TS structures. Orange and blue bars indicate the molecular MAPE of the structures that yielded successful and unsuccessful convergence in the saddle-point optimizations, respectively. Green bars indicate molecular MAPE of optimized structures. (b) Distributions of absolute energy error of inferred and optimized structures. The red line indicates an absolute energy error of 0.1kcal/mol. Intrinsic reaction coordinate (IRC) calculations are performed for the structures on right side of the red bar (126 cases). (c) Distributions of absolute energy errors of structures whose reference product and reactant structures are acquired (orange) or not acquired (blue) by IRC calculations.\n\nTo validate the ML results, saddle-point optimizations are performed using the predicted TS structures as the initial structures. Among the 1196 test molecules, 1122 (93.8%) of the molecular structures are successfully converged. This high success ratio implies that the model inferences provide structures close to the reference ones. Of the failed saddle-point optimizations, 60 failed because the maximum number of iterations for geometry relaxation is exceeded; six failed because self-consistent field failed to converge; and eight failed for other reasons.\n\nThe effect of saddle-point optimization on TS structures is evaluated by plotting the distributions of molecular MAPE before and after the saddle-point optimization, as shown by the orange and green bars in Fig. 4 (a), respectively. The MAPE distribution shifted to the left after saddle-point optimization, which corresponds to a reduction of the error. However, a considerable portion of the structures remained on around 8% molecular MAPE, creating a bimodal distribution. The splitting of distribution due to quantum chemical refinements is also observed in the energy error. Figure 4 (b) shows the distribution of the absolute energy error in the optimization results. The absolute energy errors of the predicted structures are broadly distributed at 0.1–100 kcal/mol.\nHowever, for the optimized structures, the absolute energy errors of most of the structures (996 cases) are reduced to below 0.1 kcal/mol, and only a small number of cases remained within the original error range. This implies two things. First, the energy of the inferred structure is not sufficiently accurate, even if the inferred interatomic distances have an error of only few percentage on average. Second, quantum chemical optimization reduces energy errors and yields reliable energy in most cases; however, in some cases, the results of saddle-point optimization are still far from the reference TS.\n\nIntrinsic reaction coordination (IRC) calculations are performed to verify whether the reaction paths with the optimized TS structures are appropriately connected to the reference reactant and product structures. The structures with errors greater than 0.1kcal/mol (shown on the right-hand side of the red line in Fig. 4 (b) ) are selected for testing (126 cases). If the reference reactant and product structures are obtained by IRC calculations, the cases are classified into the IRC success group, otherwise, they are classified into the IRC failure group. The orange and blue bars in Fig. 4(c) represent the energy error (\\(|E^{\\text{Opt}} - E^{\\text{Ref}}|\\)) distribution of the IRC success and IRC fail groups, respectively. Generally, the IRC success cases (79 structures) have lower \\(|E^{\\text{Opt}} - E^{\\text{Ref}}|\\) values than the IRC failure cases. In particular, in the range below 0.5kcal/mol, only one structure failed to reproduce the reactant and product structures. Conversely, even some structures with a difference of more than 10kcal/mol successfully yielded the correct reactants and products. An energy difference over 10kcal/mol indicates that the optimized TS structure has a significantly different conformation from the reference structure. Despite this large discordance, these cases can be included in the IRC success group because of the nonuniqueness of reaction paths.\n\nFigure 5 visualizes two extreme IRC success cases with respect to the energy error. The upper and lower subplots show the reference, predicted, and optimized TS structures for the cases with the most positive and most negative energy errors, respectively. In both positive and negative error cases, it is observed that the predicted TS structures are not significantly changed by the saddle-point optimization while the reference TS structures are noticeably different from both the predicted and optimized TS structures. This means that the proposed model predicts one of the TS structures, and it is well optimized to the closest TS structure, but it is not the same as the reference one. In the positive error case, the activation energy of the reaction passing through reference TS (\\(E_a^{\\text{ref}}\\)) is lower than that of the optimized TS (\\(E_a^{\\text{opt}}\\)) because the energy of optimized structure is higher than that of reference one. In contrast, the negative error indicates that \\(E_a^{\\text{opt}}\\) is less than \\(E_a^{\\text{ref}}\\) which means that the ML method predicts energetically more favorable TS structure than reference one.\n\nMultiple TSs for a chemical reaction are frequently observed in general polyatomic systems. In a strict sense, it is extremely difficult to precisely target the most stable TS structure; however, practically, the most stable TS structure can be found by exploring multiple TSs. Therefore, the generation\nFig. 5 Molecular structures and activation barriers for extreme cases Reactant, product and transition states having (a) the most positive and (b) the most negative energy errors among the inferred structures that yielded correct reactant and product structures through intrinsic reaction coordinate calculations. A positive (or negative) error indicates that the obtained TS structure is energetically less (or more) probable than the corresponding reference transition state.\n\nof multiple reaction pathways is essential for many applications. Furthermore, to design catalysts or retrosynthetic pathways, acquiring information on competitive reaction mechanisms is a challenging but demanding work.[31–33] To tackle this problem, generation of multiple TS structures using the fast and accurate ML inferences is demonstrated with the aid of reactant and product sampling.\n\n2.3 Exploring multiple reaction paths\n\nFor the reaction in which the ML model fails the most (Fig. 5 (a)), multiple TS structures are found by using the ensemble approach with normal mode sampling (NMS) of reactant and product. NMS can quickly sample a large number of thermally activated structures because it perturbs atomic positions along the normal modes of the equilibrium structure instead of heavy molecular dynamic simulations.[34] From the 2000 sets of sampled reactants and products, the same number of TS structures are generated by the ensemble method.\nFig. 6 Relative energies from transition state exploration The TS exploration is performed for the reaction shown in Fig. 5 (a) using quantum chemical saddle-point optimization and the proposed machine learning approach with off-equilibrium samplings of reactant and product. The relative energy of 24 TS structures from the exploration are plotted, in descending order, with respect to the energy of reference TS structure, \\( E^{\\mathrm{TS,\\text{opt}}} - E^{\\mathrm{TS,\\text{ref}}} \\). The energies with the same color share the same conformation. The representative structures are shown in boxes of the same color.\n\nGenerating 2000 TS structures typically requires considerable human labor or computational cost, even if an automatic reaction path finder is applied. In contrast, only 1 minute is spent for inferring 2000 TS structures with NVIDIA Titan RTX graphic card. Although 90 ML models are used for the ensemble predictions, these inferences can be performed independently. Therefore, the computational expense of even ensemble inferences is manageable. To reduce computational costs of quantum chemical refinement, instead of simulating all generated TS structures, 117 representative TS structures are selected by clustering and they are used for saddle-point calculations as initial geometries. (See Section 4.6 for details the NMS and clustering procedures) Among the 117 calculations, 24 calculations successfully converged.\n\nFigure 6 shows the relative energies (\\( |E^{\\mathrm{TS,\\text{opt}}} - E^{\\mathrm{TS,\\text{ref}}}| \\)) of the 24 successfully converged TS structures relative to the reference structures. Among 24 structures, four conformations are observed. The energy deviations among structures with the same conformations are less than 0.05kcal/mol. The energies of each conformations and its corresponding structure are shown with the same color. The conformation with the lowest energy (shown in the red box) is the same as that of the reference TS. The conformations within blue and pink boxes share most structural characteristics, except for the direction of the –OH group. In contrast, the conformation shown in the green box has a completely different structure even though its energy is close to those of other two conformations. By utilizing ensemble inferences with NMS, four different TS structures are obtained within a reasonable number of quantum chemical calculations.\n\nTo validate the TS structures, IRC calculations are performed to the obtained four conformers shown in Fig. 6. It is confirmed that reference reactant and product are obtained from IRC calculations using the structures shown in green, blue, and pink boxes as an initial geometry. In contrast, the\nstructure in the red box, which has the same conformation to the reference TS, does not yield the correct product structure. Instead of the reference product, the IRC calculation generates the conformation consisting of three molecules (C2H5, H2O, and C2OH3). Interestingly, this same products are generated by IRC validation of the reference TS structure. Because the reference TS structures are generated from the single-ended growing string method followed by refinement with saddle-point optimization, the obtained TS can be transformed into the TS of unwanted reaction during the saddle-point optimization. Although one of the obtained TS is not a correct TS of target reaction, these results confirm that the proposed method can generate reliable TS structures, even with off-equilibrium reactant and product structures. Additionally, the effectiveness of the proposed approach for tackling multiple reaction paths is also demonstrated.\n\nThe IRC validations of the obtained TS conformations reveals that the large energy errors of the originally predicted TS structures may not be actual errors of the model, but the reference database. To systematically evaluate data errors in the TS database, a large number of IRC calculations are required, which is not viable using current computing resources. Despite some potential faults in the reference structures, the proposed ML model is stably trained and can be applied to exploring multiple reaction paths which is a challenging problem in many contexts of chemistry.\n\n3 Discussion\n\nIn this study, a novel ML model for fast and accurate prediction of TS structures is proposed and validated using general organic chemical reactions. To achieve high accuracy with the satisfaction of various necessary invariances, the ML model contained PSI layers designed to handle any size of molecules and any type of element. This layer relies not on any prior knowledge of chemical reaction type but on reactant and product structures, thus can be extended to all types of chemical reactions without modifications. Despite the lack of reliable TS data, the proposed ML model shows high accuracy for general organic reactions. In particular, for atomic pairs that undergo bond formation or breakage during the reaction, the proposed model noticeably outperforms existing models. Additionally, when the inferred TS structures are used as inputs for quantum chemical saddle-point optimizations, a high convergence ratio is achieved, which demonstrates that this ML method can be an attractive solution for initializing a starting structure for saddle-point optimizations.\n\nTo demonstrate the potential usage of the model in searching multiple reaction paths, an autonomous reaction path finder is implemented and tested on a polyatomic reaction. By performing ML inference from the off-equilibrium conformations of reactant and the product and further refinement by saddle-point calculations, various chemically meaningful TS structures are identified. This automated TS finder has huge potential to leverage ML applications for chemical reactions because it can be directly utilized for not only chemical\napplications (e.g. design of synthetic routes and catalysts), but also various ML applications for chemical reactions (e.g. active learning). Hopefully, the proposed ML approach as well as its components (such as TTA, and ensemble) will be utilized to construct powerful artificial intelligence in the field of chemical reactions.\n\n4 Methods\n\n4.1 Data preparation and quantum chemical validation\n\nIn this study, two publicly available reaction databases are used. The first was released by Grambow et al.[28] This database is consist of density functional theory (DFT) results with two different options, B97-D3/def2-mSVP and ωB97X-D3/def2-TZVP. Here, ωB97X-D3/def2-TZVP results (11961 reactions) are employed because of its reliable accuracy. To extract atomic positions and molecular properties from the DFT results, ard_gsm package provided by the authors of the database is utilized. (www.github.com/cgrambow/ard_gsm) The database, is split randomly into training, validation, and test sets with an 80-10-10 ratio. The second database includes 53 S_N2 reactions which was released by the author of TSNet.[25] This database includes five validation and 48 training data. The same splitting result is adopted.\n\nSaddle-point optimization and IRC calculations are performed for the test reactions in the first database using the same DFT functional(ωB97X-D3) and basis set (def2-TZVP). Saddle-point optimization is performed with TS optimization implemented in QChem while pysisyphus program is utilized for IRC calculations.[35] The pysisyphus program provides various methods of exploring PESs based on the results (mainly, gradients and Hessian) of a quantum chemical package. To run IRC calculations with pysisyphus, Psi4 package is employed because it is seamlessly coupled to pysisyphus and supports ωB97X-D3 and def2-TZVP.[36]\n\n4.2 Model Architecture and Training\n\nLinear interpolated geometries are frequently used for TS search algorithms because of their reliable structures and low costs. [13, 37] The proposed model predicts the interatomic distances of the true TS from the reactant, product, and linearly interpolated structures. These three structures are featurized as a sequence of atomic pair sets. The pair features are constructed by concatenating one distance and two atomic features. For atomic and distance features, entity embedding of atomic numbers and Gaussian kernel are employed, respectively. For centers of Gaussian functions, points on an equidistant grid are used. The information on the grid is present in Table S1. Each structure includes a set of pair features (\\( f_{ij} \\)) and reactions are featurized as a sequence of structure feature sets whose dimension is \\( \\left( \\frac{N_{\\text{atom}} \\times (N_{\\text{atom}} + 1)}{2}, 3, N_f \\right) \\) where \\( N_{\\text{atom}} \\) and \\( N_f \\) are number of atoms and feature size for the pairs, respectively. For convenience, in Fig. 1, two atomic indices (\\( i, j \\)) are introduced; however, only one index is\nused for atomic pairs in the actual implementation. The pair features satisfy the translational and rotational invariances because neither atomic numbers nor distances are changed by translation or rotation.\n\nBecause the number of atoms participating in a reaction is not fixed, and because their order is not chemically meaningful, operations on the first dimension of pair features need to be size-extensive and permutation-invariant, whereas the size of the second dimension is always fixed and the order is not interchangeable. To preserve the nature of data structure, the novel layer named pair sequence interaction (PSI) layer is introduced.\n\nInitially, the PSI layer updates the pair features by reflecting other pairs in the same structure. This procedure consists of a transformer encoder, which is a permutation-invariant and size-extensive operation. This first update is not affected by the pair features of other structures. Subsequently, the atomic features are updated again to reflect the information from other structures. Because this second update proceeds only among only atomic pairs sharing the same index, the permutation invariance and size-extensivity of the first dimension are still preserved. For the second update, a GRU is used. Figure 1(b) illustrates the two updates of the PSI layer using different colors. The yellow operation operates only on pair features in the same structure, whereas the following blue operation updates pair features by reflecting pairs with the same index but in other structures. By stacking multiple PSI layers, the effects of all the atomic pairs of the reactant, product, and linearly interpolated structures participate in determining every one of the final atomic pair features. In the proposed model, two PSI layers are stacked and the initial feature size of atomic pair feature (128) is changed to 512 at the end of the two stacked PSI layers because each bidirectional GRU doubles the feature size.\n\nTo compute the reaction properties from the updated atomic pair features, two readout layers are used. The first of these readout layers, represented as the purple box in Fig. 1 (a), is applied to compute the ratios of the interatomic distances between the TS structure and linearly interpolated structure. The second readout layer computes the contribution of each atom to total energy, rotational entropy, and translational entropy. (\\( E_{i}, S_{(vib,i)} \\) and, \\( S_{(rot,i)} \\)) The atomic features for the second layer is computed using the following equation:\n\n\\[\nf_{i}^{\\text{atom}} = \\sum_{j} f_{ij}^{\\text{pair}}\n\\]\n\nwhere \\( f_{i}^{\\text{atom}} \\), and \\( f_{ij}^{\\text{pair}} \\) are the atomic and pair features. Because the model only computes \\( f_{ij}^{\\text{pair}} \\) when \\( i \\geq j \\), the omitted pair features are recovered using symmetric approximation, \\( f_{ij}^{\\text{pair}} = f_{ji}^{\\text{pair}} \\). The predicted values from the second readout layers are utilized for multi-label learning which is frequently used to improve the quality of ML inferences by leveraging the information from the related information.[38, 39]\n\nImplementation and training of the proposed model are performed with PyTorch Lightning, which supports a high-level interface of PyTorch and\nis freely available at https://github.com/Lightning-AI/lightning. The implemented model and scripts for training and inference are uploaded at https://gitlab.com/sunghwan.choi/learnts. All hyperparameters used to train the model are summarized in Table S1.\n\n4.3 Metrics\n\nMolecular MAE and molecular MAPE are defined as follows:\n\n\\[\n\\text{(Molecular MAE)} = \\frac{1}{M} \\sum_t^M \\frac{2}{N_{\\text{atom},t}(N_{\\text{atom},t}-1)} \\sum_{i400 conductive aerogels (3–4 replicates for each data point) were evaluated using the autonomous testing platform, and the total operation time was estimated to be 81 hours, averaging about 12 minutes to test one aerogel sample.\n\nFrom the stress–strain curve of each conductive aerogel, the compressive stress at 30% strain (abbreviated as \\( \\sigma_{30} \\)) was characterized, and the average \\( \\sigma_{30} \\) value from 3–4 aerogel replicates was designated as the “mechanical” label. Next, by using a two-electrode system (with a 1-cm gap between electrodes), the initial electrical resistance of each conductive aerogel (abbreviated as \\( R_0 \\)) was measured, and the average \\( R_0 \\) value from 3–4 aerogel replicates was recorded as the “electrical” label. In short, each kind of conductive aerogel resulted in one data point, which included four “composition” labels, one “loading” label, one “mechanical” label, and one “electrical” label (see Table S3). For one active learning loop, 20 new kinds of conductive aerogels were produced, therefore adding 20 data points to the database.\n\nTo improve model training efficiency and counteract potential overfitting, the User Input Principle (UIP) method was adopted to synthesize virtual data points (refer to Note S6 for detailed description). The creation of virtual data points took place in the vicinity of collected real data points. For instance, Fig. S7a,b demonstrate that, with slight variations in the MXene/CNF/gelatin/GA ratios (e.g., 64/24/12/+ vs. 62/26/12/+), led to the conductive aerogels with similar \\( \\sigma_{30} \\) (10.58 kPa vs. 10.63 kPa) and \\( R_0 \\) values (8.9 \\( \\Omega \\) vs. 10.1 \\( \\Omega \\)). Meanwhile, when the replicates of conductive aerogels were characterized, Fig. S7c indicates that there were slight measurement variations in \\( \\sigma_{30} \\) and \\( R_0 \\). To synthesize virtual data points, Gaussian noises were\nintroduced in the proximity of the composition, mechanical, and electrical labels based on our experimental observations. Afterward, both real and virtual data points were utilized as training data points for an ANN-based model using 4-fold cross-validation.\\(^{70}\\)\n\nTo collect more data points in the next active learning loop, the ANN model assessed the unfamiliarity level of each data point within the feasible parameter space using a hybrid acquisition function termed *A Score*, represented by **Equation 1**,\\(^{71}\\)\n\n\\[\nA\\ Score = \\hat{L} \\cdot \\hat{\\sigma}\n\\]\n\n(1)\n\n, where \\( \\hat{L} \\) denotes the Euclidean distance between in-model and model-targeted data points and \\( \\hat{\\sigma} \\) denotes the ANN model’s prediction variance (as detailed in **Note S7**). The data points with the highest *A Scores* were the least familiar to the model and pinpointed for experimental validation in the next loop. By extracting the composition and loading labels of pinpointed data points, the OT-2 robot was activated to prepare a new set of MXene/CNF/gelatin/GA mixtures. Once vortexed, cast, and freeze-dried, a new batch of conductive aerogels was produced. Similarly, the \\( \\sigma_{30} \\) and \\( R_0 \\) values of these conductive aerogels were characterized *via* the autonomous testing platform and the two-electrode system, respectively. Based on these real data points, virtual data points were synthesized using the UIP method. Upon inputting the real and virtual data points, the ANN model was retrained, re-assessed *A Scores*, and suggested another set of fabrication parameters for the next active learning cycle. With the operation of two collaborative robots, the active learning loops were largely facilitated. Each loop took an average of 2.5 days: 2 hours dedicated to OT-2 pipetting, 48 hours for freeze-drying, 4 hours allocated to autonomous testing, and another 4 hours for model training. In total, 8 active learning loops were carried out, and 162 kinds of conductive aerogels were stagewise produced (refer to **Table S3**). Finally, the database contained approximately 160,000 data points, including both actual and virtual ones.\nDuring the active learning loops, the ANN model continued to evolve and was evaluated from two perspectives: (1) the distribution of collected data points and (2) the accuracy of multi-property predictions. First, as shown in Fig. 2c,d and S8, 2D Voronoi tessellation diagrams were plotted to visualize how data points were sequentially collected and distributed within the feasible parameter space. During active learning loops, the ANN model efficiently explored the feasible parameter space and guided experiments towards the unfamiliar regions, effectively mitigating the rise of redundant data clusters.\n\nSecond, the accuracy of multi-property predictions was assessed using a set of testing data points, which were never input into the model (see Table S4). For each testing data point, the ANN model provided the predicted \\( \\sigma_{30} \\) and \\( R_0 \\) values based on the “composition” and “loading” labels. Then, the model-predicted \\( \\sigma_{30} \\) and \\( R_0 \\) values were compared with the actual \\( \\sigma_{30} \\) and \\( R_0 \\) values of the testing data point. The deviation between model-predicted and actual \\( \\sigma_{30} \\) values was evaluated using the mean absolute error (MAE), as detailed in Equation 2,\n\n\\[\nMAE = \\frac{1}{N} \\sum_{i=1}^{N} |predicted\\ \\sigma_{30}^i - \\sigma_{30}^i|\n\\]\n\n(2)\n\n, where \\( N \\) is the cumulative number of testing data points, \\( predicted\\ \\sigma_{30}^i \\) is the model-predicted \\( \\sigma_{30} \\) value based on a testing data point (\\( i \\)), \\( \\sigma_{30}^i \\) is the actual \\( \\sigma_{30} \\) value of a testing data point (\\( i \\)). On the other hand, the deviation between model-predicted and actual \\( R_0 \\) values were assessed using the mean relative error (MRE), as detailed in Equation 3,\n\n\\[\nMRE = \\frac{1}{N} \\sum_{i=1}^{N} \\left| \\frac{\\log(predicted\\ R_0^i) - \\log(R_0^i)}{\\log(R_0^i)} \\right|\n\\]\n\n(3)\n\n, where \\( N \\) is the cumulative number of testing data points, \\( predicted\\ R_0^i \\) is the model-predicted \\( R_0 \\) value based on a testing data point (\\( i \\)), \\( R_0^i \\) is the actual \\( R_0 \\) value of a testing data point (\\( i \\)). Smaller MAE and MRE values indicated higher prediction accuracy, while larger values indicated\nlower accuracy. By evaluating MAEs and MREs, we were able to assess the model’s prediction accuracy in predicting the mechanical and electrical properties of conductive aerogels from their fabrication parameters.\n\nThroughout 8 active learning loops, the MAE (that assessed the accuracy of \\( \\sigma_{30} \\) prediction) continually decreased from 2.5 to 1.5 kPa (**Fig. 2e**, top), and the MRE (that assessed the accuracy of \\( R_0 \\) prediction) decreased from 49.0% to 18.4% (**Fig. 2e**, bottom). Towards the end of active learning loops, both MAE and MRE values were stabilized and gradually approached toward the measurement variations of \\( \\sigma_{30} \\) (~1.1 kPa) and \\( R_0 \\) (~10.1%). Among other models based on linear regression, decision tree, gradient-boosted decision tree, random forest algorithms, the ANN model demonstrated the lowest MAE and MRE values (**Fig. 2e**). Furthermore, without conducting data augmentation, the ANN model presented a higher MAE of >1.9 kPa (for \\( \\sigma_{30} \\) prediction) and a higher MRE of >37% (for \\( R_0 \\) prediction), due to the model overfitting upon the use of a small database (**Fig. 2f**). As the virtual-to-real data ratio increased to 100 and 1,000, the MAE values decreased to 1.8 kPa and 1.5 kPa, and the MRE values decreased to 21.5% and 18.4%, respectively. In this work, the optimal virtual-to-real data ratio was set to be 1,000, which enabled high learning efficiency and still kept the model training time below 4 hours. On the other hand, when the virtual-to-real data ratio increased to 5,000 and 10,000, the model training time increased to >1 and >2 days, respectively. Finally, the ANN model that demonstrated the lowest MAE and MRE values was selected as “the champion model”, which was deployed the next to automate the design of conductive aerogels with programmable mechanical and electrical properties.\nFig. 2. Constructing a prediction model via active learning loops, data augmentation, and collaborative robots. (a) Schematic illustration of a multi-stage AI/ML framework for constructing a prediction model via active learning loops, data augmentation, and robot–human teaming. (b) An autonomous testing platform integrated with a UR5e robotic arm and an Instron\ncompression tester. 2D Voronoi tessellation diagrams (c) without and (d) with the GA incorporation after 8 active learning loops. (e) MAE (top) and MRE (bottom) values of various prediction models based on linear regression, decision tree, gradient-boosted decision tree, random forest, and ANN algorithms. (f) MAE (top) and MRE (bottom) values of various ANN models based on different virtual-to-real data ratios.\n\nPredicting compressive strengths and electrical resistances of conductive aerogels\n\nBy leveraging the champion model’s prediction capabilities, two-way design tasks were successfully demonstrated, involving (1) predicting the \\( \\sigma_{30} \\) and \\( R_0 \\) values of a conductive aerogel from its fabrication parameters and (2) suggesting an ideal set of MXene/CNF/gelatin/GA ratio and mixture loading to produce a conductive aerogel with user-designated characteristics.\n\nFirst, by selecting different sets of fabrication parameters, various conductive aerogels were fabricated and characterized (recipes #1–#8 in Table S5). As evidenced in Fig. 3a,b, the champion model predicted the \\( \\sigma_{30} \\) and \\( R_0 \\) values of these conductive aerogels accurately based on their “composition” and “loading” labels, and the predicted values were close to the experimentally characterized results. Second, the inverse design of conductive aerogels was automated by the champion model, without the need for iterative optimization experiments. As illustrated in Fig. 3c, two conductive aerogels were targeted with specific property requirements, including (1) high-strength aerogels (\\( \\sigma_{30} > 10 \\) kPa) and (2) high-strength, conductive aerogels (\\( \\sigma_{30} > 10 \\) kPa and \\( R_0 < 10 \\Omega \\)). By inputting these design requests, the champion model performed clustering analyses to pinpoint the most suitable sets of fabrication parameters. By following the model-suggested fabrication parameters, two kinds of conductive aerogels were produced. As demonstrated in Fig.\n3d, for the design request #1, the champion model suggested two aerogels (recipes #9–#10 in Table S6), both of which demonstrated the \\( \\sigma_{30} \\) values that were higher than the input requirement of 10 kPa. For the design request #2, the champion model suggested four aerogels (recipes #11–#14 in Table S6), showing the average \\( \\sigma_{30} \\) and \\( R_0 \\) values >10 kPa and <10 \\( \\Omega \\), respectively. The inset of Fig. 3c and Fig. S9 show the SEM images of the model-suggested aerogels (recipes #9 and #14). As displayed in the violin plots (Fig. 3e), the achievable \\( \\sigma_{30} \\) and \\( R_0 \\) values of conductive aerogels spanned widely between \\( 0.1 < \\sigma_{30} < 16.0 \\) kPa and \\( 10^0 < R_0 < 10^{10} \\) \\( \\Omega \\), through navigating the DOFs of MXene/CNF/gelatin/GA ratios and mixture loadings. Compared with the state-of-the-art works of conductive aerogels (Table S7),\\(^{2,8,19,20,29,33,72-80}\\) our AI/ML integrated approach proved to be efficient in discovering the conductive aerogels with programmable mechanical and electrical properties, without the need for iterative optimization experiments.\nFig. 3. Predicting compressive strengths and electrical resistances of conductive aerogels. (a) Comparison between the actual stress–strain curves of conductive aerogels (recipes #1–#8) and the model-predicted \\( \\sigma_{30} \\) values. (b) Comparison between the actual initial electrical resistances of conductive aerogels (recipes #1–#8) and model-predicted \\( R_0 \\) values. (c) By inputting specific\ndesign requests, the champion model was able to automate the inverse design processes of conductive aerogels by directly suggesting suitable sets of fabrication parameters, without the need for iterative optimization experiments. Inset shows the SEM images of two model-suggested conductive aerogels. (d) Comparison between actual and model-predicted \\( \\sigma_{30} \\) (left) and \\( R_0 \\) (right) values of conductive aerogels (recipes #9–#14). (e) Violin plots of achievable \\( \\sigma_{30} \\) and \\( R_0 \\) values of conductive aerogels.\n\nSHAP model interpretation and FE simulations to uncover complex fabrication–structure–property correlations\n\nTo address the “black box” nature of the champion model, the SHAP model interpretation method was applied to 162 data points collected during active learning loops. SHAP relies on a game theoretic approach and contains a permutation explainer program to explain the output of any AI/ML model.\\(^{81}\\) By iterating over complete permutations of the features, the SHAP values are calculated to approximate the contribution of each fabrication parameter to a specific property. A positive SHAP value indicates a positive correlation, and *vice versa* (see **Note S8** and **Fig. S10** for further details). In this study, the SHAP values of MXene, CNF, gelatin, GA loadings, and mixture loading on the \\( \\sigma_{30} \\) and \\( R_0 \\) values of conductive aerogels were calculated. As shown in **Fig. S11**, the SHAP value of MXene loading on \\( R_0 \\) ranged from –0.94 to +0.97, showing the widest range compared to the other SHAP values (e.g., CNF loading from –0.41 to +0.65, gelatin loading from –0.83 to +0.94, GA loading from –0.24 to +0.36, and mixture loading from –0.35 to +1.00). The SHAP results clearly indicate that the \\( R_0 \\) values of conductive aerogels were primarily influenced by the amount of MXene nanosheets incorporated. On the other hand, **Fig. 4a** shows that the SHAP\nvalue of mixture loading on ranged the widest from –1.00 to +0.97 among the others (e.g., MXene loading from –0.28 to +0.28, CNF loading from –0.41 to +0.32, gelatin loading from –0.71 to +0.56, and GA loading from –0.23 to +0.19). The above SHAP results suggest that the mixture loading of aqueous mixture (that affected the density of a conductive aerogel) presented the most significant impact on the mechanical properties.\n\nNext, to investigate strong correlations between mixture loading and \\( \\sigma_{30} \\) value, four conductive aerogels were fabricated at the same MXene/CNF/gelatin/GA ratio of 80/20/0/– but at different mixture loadings (from 2.5 to 10.0 mg mL\\(^{-1}\\)). As shown in Fig. 4b, as the mixture loadings increased, the \\( \\sigma_{30} \\) values of conductive aerogels rose significantly from 0.2 kPa to 5.9 kPa. Four other conductive aerogels were produced at the same mixture loading of 10.0 mg mL\\(^{-1}\\) but with various MXene/CNF/gelatin/GA ratios (from 80/20/0/– to 20/80/0/–). Despite the difference in aerogel composition, the \\( \\sigma_{30} \\) values exhibited only a minor shift from 7.5 kPa to 5.9 kPa. Supported by SHAP analyses and experimental results, it was determined that adjusting the mixture loading level was a more effective method for tuning the compression resilience of a conductive aerogel (e.g., \\( \\sigma_{30} \\)).\n\nTo delve deeper into the mechanistic effects of mixture loadings on the mechanical properties of conductive aerogels, three FE models were constructed. These FE models represented the conductive aerogels at the same MXene/CNF/gelatin/GA ratio (80.0/20.0/0.0/–) yet at different mixture loadings (10.0, 7.5, 5.0 mg mL\\(^{-1}\\)). These FE models were named as high-, medium-, and low-density aerogel models. Extracted from the SEM images in Fig. 4c and summarized in Table S8, several structural features of conductive aerogels, such as pore dimensions, wall thicknesses, and fracture densities, were input to construct these FE models using a commercial package of ABAQUS/CAE 2020. In the FE simulations, the microstructures of conductive aerogels were\nrepresented as the \\(4 \\times 4\\) supercells containing two-dimensional staggered lattices using second-order plane strain elements, and the periodic boundary conditions were imposed. Then, wall discontinuities were randomly introduced into the FE models to account for the structural imperfections of conductive aerogels. **Note S9**, **Fig. S12**, and **S13** provide further details regarding the construction of FE models. Next, by exerting a vertical compressive strain of 30%, the \\( \\sigma_{30} \\) values of three FE models were simulated in **Fig. 4b**, showing good agreement with the experimentally characterized \\( \\sigma_{30} \\) values. **Fig. 4d** showcases the FE models of conductive aerogels under 30% compression to provide insights regarding internal displacements and localized stress distributions. As compared in **Fig. 4e**, the FE models under 30% compression cohered with the SEM observations of conductive aerogels at their compressed states.\n\nThe high-density aerogel exhibited small, closely packed pores (with the average size of \\(18.2 \\times 6.4\\ \\mu\\mathrm{m}^2\\)) and thus allowed for uniform stress distributions upon compression, largely suppressing internal displacements of compartments. In the high-density aerogel, the localized stress tended to concentrate at the corners of each compartment, while the MXene-based walls were robust enough (with Young’s modulus at 3.4 GPa) to prevent significant deformation toward cracking. On the other hand, as the mixture loading decreased, the medium- and low-density aerogels had larger and wider pores (\\(28.3 \\times 17.8\\) and \\(39.1 \\times 19.0\\ \\mu\\mathrm{m}^2\\)), which were less efficient to transmit vertical stresses to neighboring compartments. As a result, the pores were likely to deform and distort upon the localized stress, resulting in significant internal displacements of compartments. Through the combined use of SHAP analyses, experimental validation, and FE simulations, we provided a promising solution to the “black box” challenges often associated with AI/ML predictions, enhancing the champion model’s interpretability.\nFig. 4 SHAP model interpretation and FE simulations to uncover complex fabrication–structure–property correlations. (a) Normalized SHAP values of MXene, CNF, gelatin, GA loadings, and mixture loading on the \\( \\sigma_{30} \\) values of conductive aerogels. (b) Comparison between\nthe FE-simulated and experimentally characterized \\( \\sigma_{30} \\) values of conductive aerogels at the same MXene/CNF/gelatin/GA ratio yet at different mixture loadings. (c) SEM images of high-, medium-, and low-density conductive aerogels at their uncompressed states. (d) Localized stress distribution profiles of high-, medium-, and low-density aerogel models (from FE simulations) under 30% compression. (e) SEM images of high-, medium-, and low-density conductive aerogels at their compressed states.\n\nMachine intelligence accelerated discovery of strain-insensitive conductive aerogels for wearable thermal management\n\nConductive aerogels offer promising applications in personal thermal management, owing to their lightweight feature, high electrical conductivity, and thermal insulation properties.\\(^{14}\\) **Fig. 5a** outlines the machine intelligence accelerated design process to fabricate a strain-insensitive conductive aerogel suitable for wearable heating applications. First, two property requirements were considered: (*I*) compatible compressive strength with current filling materials (\\( \\sigma_{30} \\sim 4-8 \\) kPa) and (2) high electrical conductivity for efficient Joule heating (\\( R_0 < 20 \\) \\( \\Omega \\)). Upon inputting these design requests, the champion model was able to suggest multiple sets of fabrication parameters, and various conductive aerogels that met two property requirements were fabricated (see **Table S9**).\n\nNext, an additional criterion of low pressure sensitivity was set to discover a strain-insensitive conductive aerogel, ensuring strain-stable Joule heating performance under repetitive compression. The definition of pressure sensitivity is provided in **Equation 4**,\nPressure Sensitivity (\\( S \\)) = \\( \\frac{|(R - R_0)/R_0|}{\\sigma_{30}} \\) (4)\n\nAs demonstrated in the \\( R_0 \\)-sensitivity profiles (**Fig. 5b**), the conductive aerogel based on recipe #16 was selected (at the MXene/CNF/gelatin/GA ratio of 78/13/9/– and at the mixture loading of 7.5 mg mL\\(^{-1}\\)). The model-suggested conductive aerogel exhibited a \\( \\sigma_{30} \\) value of 4.0 kPa, a low \\( R_0 \\) value of 1.7, and an ultralow pressure sensitivity of 0.02 kPa\\(^{-1}\\). **Fig. 5c** demonstrates that the relative resistance changes of the strain-insensitive conductive aerogel was only 0.9% under 100 cycles of 20% compression. Next, the Joule heating performance of the strain-insensitive conductive aerogel was investigated by applying various voltages, as evidenced in the measured temperature–time profiles (**Fig. 5d**). At the applied voltages of 0.5, 1.0, 1.5, and 2.0 V, the strain-insensitive conductive aerogel demonstrated sharp temperature increases up to 29, 37, 51, and 70 °C, respectively, within 300 seconds. As shown in **Fig. S14**, the strain-insensitive conductive aerogel displayed a linear relationship between the maximum temperature and the square of the applied voltage, well adhering to Joule’s law.\n\nTo further assess the Joule heating performance under compression, the strain-insensitive conductive aerogel at both relaxed and 20% compressed states was subject to 100 heating cycles at 1.0 and 1.5 V. As shown in **Fig. 5e**, the conductive aerogels demonstrated strain-unresponsive heating/cooling profiles, with stable average temperature variations for 100 heating cycles. Such efficient and strain-stable Joule heating performance was well-suited for wearable heating applications. Additionally, we conducted thermal conductivity measurements to assess the thermal insulation properties of the strain-insensitive conductive aerogel. The density and thermal insulation performance of the strain-insensitive conductive aerogel were characterized as 10.1 mg cm\\(^{-3}\\) and 0.034 W mK\\(^{-1}\\), respectively. Compared with other thermal insulation materials in **Fig. S15**, the strain-insensitive conductive aerogel offered lightweight features, competitive thermal\ninsulation properties, and efficient Joule heating performance. To demonstrate its practical exploitation, multiple strain-insensitive conductive aerogels with the dimensions of \\(5.0 \\times 5.0 \\times 1.0\\) cm\\(^3\\) were inserted into a commercial jacket. Powered by a portable battery system (at 1.5 V), the aerogel-incorporated jacket was heated on demand to warm the subregion of a volunteer (thermal images in **Fig. 5f**).\nFig 5. Machine intelligence accelerated discovery of strain-insensitive conductive aerogels for wearable thermal management. (a) Schematic illustration of machine intelligence design process of strain-insensitive conductive aerogels. (b) \\( R_0 \\)-sensitivity profile of model-suggested conductive aerogels. (c) Time-resolved relative resistance changes of a strain-insensitive conductive aerogel under 100 cycles of 20% compression. (d) Temperature–time profiles of a\nstrain-insensitive conductive aerogel at different applied voltages. (e) Time-resolved temperature profiles of a strain-insensitive conductive aerogel at its relaxed and 20% compressed states under Joule heating (at 1.0 and 1.5 V). (f) Thermal images of the aerogel-incorporated jacket under Joule heating at 1.5 V.\nConclusion\n\nIn conclusion, an integrated platform that combined automated robotic experiments with an AI/ML framework was realized to automate the inverse design of conductive aerogels with programmable mechanical and electrical properties. Through an AI/ML framework comprising SVM classifier, active learning loops, and data augmentation, the champion model demonstrated exceptional prediction capabilities and allowed for two-way design tasks, including accurately predicting the \\( \\sigma_{30} \\) and \\( R_0 \\) values of a conductive aerogel and suggesting suitable fabrication parameters to produce conductive aerogels that met specific property requirements. Compared with conventional design of experiment, this hybrid approach was efficient to discover the conductive MXene aerogels with achievable \\( \\sigma_{30} \\) and \\( R_0 \\) values spanning between \\( 0.1 < \\sigma_{30} < 16.0 \\) kPa and \\( 10^0 < R_0 < 10^{10} \\) \\( \\Omega \\). The SHAP analyses and FE simulations further provided mechanistic insights into the impacts of fabrication parameters on the properties of conductive aerogels, enhancing our understanding of the aerogels’ mechanical behaviors. Moreover, the predictive power of the champion model was harnessed to discover a strain-insensitive conductive aerogel with compatible mechanical strength, high electrical conductivity, and ultralow pressure sensitivity suitable for wearable heating applications.\n\nThe successful integration of robotic experiments, AI/ML predictions, and FE simulations has demonstrated a synergistic approach, with potential applications beyond conductive aerogels, such as tactile sensors,\\(^{82,83}\\) stretchable conductors,\\(^{84,85}\\) catalysts,\\(^{59,60}\\) and electrochemical electrolyte optimization.\\(^{57,58}\\) Our findings contribute to advancing the understanding of vital correlations between fabrication parameters and physicochemical properties, enabling the rational design of functional materials for scalable production.\nMaterials\n\nLithium fluoride (LiF, BioUltra, ≥99.0%), hydrochloric acid (HCl, 37%), northern bleached softwood kraft (NBSK) pulp (NIST® RM 8495), TEMPO (99%), sodium bromide (NaBr, ≥99.5%), sodium bicarbonate (NaHCO₃, ≥99.7%), sodium hydroxide (NaOH, ≥98%), and gelatin (from porcine skin, Type A) were purchased from Sigma-Aldrich. Ti₃AlC₂ MAX powders were purchased from Lai Zhou Kai Kai, China. Silicone molds were purchased from Amazon. Deionized water (18.2 MΩ) was obtained from a Milli-Q water purification system (Millipore Corp., Bedford, MA, USA) and used as the water source in this work.\n\nMethods\n\nPreparation of Ti₃C₂Tₓ MXene nanosheets. Ti₃C₂Tₓ MXene nanosheets were prepared according to the literature.⁸⁶ First, 3.0 g of LiF was dissolved in 6.0 M HCl at 35 °C under vigorous stirring. After the dissolution of LiF, 1.0 g of Ti₃AlC₂ MAX powder was slowly added into the HF-containing solution. The mixture was kept at 35 °C for 24 hours. Afterward, the solid residue was washed with 2.0 M HCl and DI water sequentially until the pH value increased to 6. Subsequently, the washed residue was added into 100 mL of DI water, ultrasonicated for 1 hour, and centrifuged at 3,000 r.p.m. for 30 minutes. The supernatant was collected as the final suspension of MXene nanosheets with the concentration of 10–12 mg mL⁻¹.\n\nPreparation of CNF dispersion. The CNF dispersion was prepared according to the literature.⁸⁷ First, 20 g of NBSK pulp was suspended in 1.0 L of DI water, and then TEMPO (2 × 10⁻³ mole) and NaBr (0.02 mole) were added into the pulp. The TEMPO-mediated oxidation was initiated by\nadding 0.2 mole of NaClO, and the oxidation process was maintained for 5–6 hours under continuous stirring, during which the pH was controlled at 10.0 by adding NaOH solution. The TEMPO-oxidized pulp was repeatedly washed with DI water until the pH returned back to 7.0. Afterward, the pulp was disassembled in a microfluidizer processor (Microfluidics M-110EH), and the concentration of CNF dispersion was about 10 mg mL\\(^{-1}\\).\n\n*Preparation of gelatin solution.* 8.0 g of gelatin was dissolved in 1.0 L of DI water followed by continuous stirring for 48 hours, and the concentration of gelatin solution was 8.0 mg mL\\(^{-1}\\).\n\n*Robot-assisted fabrication of conductive aerogels.* An automated pipetting robot (OT-2, Opentrons) was operated to prepare different mixtures with varying MXene/CNF/gelatin ratios. For each mixture, the dispersions of MXene nanosheets and CNFs as well as the gelatin solution were mixed at different volumes. The mixture loadings of MXene/CNF/gelatin mixtures were controlled to be 10.0, 7.5, 5.0, and 2.5 mg mL\\(^{-1}\\). The solution containing 25 wt.% of GA was optionally added into the MXene/CNF/gelatin mixtures at a consistent ratio of 35 \\( \\mu \\)L for every 100 mg of solid content. Afterward, the robot-prepared MXene/CNF/gelatin/GA mixtures were vortexed at 2,000 r.p.m. for 30 seconds and poured into silicone molds. Silicone molds with cavities of 15 \\( \\times \\) 15 mm and a height of 12 mm were used to prepare cuboid aerogel samples. The slurry-like mixtures were refrigerated overnight at 4.0 °C and then frozen using liquid nitrogen followed by a freeze-drying process (at –85 °C and \\( 10^{-3} \\) atm, Labconco FreeZone), allowing for the production of conductive aerogels.\nCompression tests of conductive aerogels. The stress–strain curves of conductive aerogels (with average dimensions of \\(1.5 \\times 1.5 \\times 1.0\\ \\mathrm{cm}^3\\)) were measured by a mechanical testing machine (Instron 68SC-05) with a 500 N load cell for 5 cycles of loading and unloading (at 5 mm s\\(^{-1}\\) for 30% compression). A collaborative robotic arm (UR5e, Universal Robots) was integrated into a universal testing system to automate the compression tests.\n\nElectrical resistance measurements of conductive aerogels. The initial electrical resistance, \\(R_0\\), of the conductive aerogels were measured using a two-electrode system connected with an electrochemical workstation (Autolab PGSTAT302N, Metrohm) or an Industrial Multimeter (Fluke 87V). The gap between two electrodes was fixed at 1 cm.\n\nPressure sensitivity measurements of conductive aerogels. The conductive aerogels were initially set up on a two-electrode system and linked to an electrochemical workstation (Autolab PGSTAT302N, Metrohm). To determine the pressure sensitivity (\\(S\\)) of conductive aerogels, they were subjected to a continuous compression process using the Instron compression tester, reaching up to 30% strain at a rate of 0.02 mm s\\(^{-1}\\). Throughout this compression testing, the relative resistance changes of conductive aerogels were consistently monitored. Additionally, their stress–strain curves and \\(\\sigma_{30}\\) values were characterized. The \\(S\\) of the aerogel was subsequently calculated using Equation 4.\n\nJoule heating of strain-insensitive conductive aerogels. To evaluate the Joule heating performance, the strain-insensitive conductive aerogels were first positioned on a two-electrode system. This system was then linked to either an electrochemical workstation (Autolab\nPGSTAT302N, Metrohm) or a portable battery setup. To measure the surface temperature, thermocouple probes (K Type Thermometer, Gain Express AZ Instruments) were attached to the sides of the aerogels. The electrochemical workstation enabled the application of varying voltages, ranging from 0.0 to 5.0 V. During cycling tests, the conductive aerogel was subjected to constant voltages of 1.0 and 1.5 V for 100-second intervals, followed by a 100-second pause.\n\n*Thermal conductivity measurements of strain-insensitive conductive aerogels.* Thermal conductivity measurements were carried out at room temperature using a heat flow meter (HFM-25, Thermttest Instruments). The temperature differentials were set at 17.5 °C and 32.0 °C. For these tests, the strain-insensitive conductive aerogel with the dimensions of \\( 5.0 \\times 5.0 \\times 2.0 \\ \\mathrm{cm}^3 \\) was utilized.\n\n*Characterization.* The microstructures of conductive aerogels were investigated using a field emission scanning electron microscope (FESEM, Hitachi SU-70) operating at 1.0–2.0 kV for low, medium, and high-resolution imaging, equipped with an energy dispersive spectroscopy (EDS) for elemental analyses. All of the SEM samples were sputtered with a layer of AuPd (~1.0 nm) prior imaging. XPS were obtained by an X-ray photoelectron spectrometer (Kratos AXXIS UltraDLD) using a microfocused Al X-ray beam (100 μm, 25 W) with a photoelectron take-off angle of 90°.\n\n*Construction of finite element (FE) models.* The FE models of conductive aerogels were created using the commercial package ABAQUS/CAB 2020. The microstructures of high-, medium-, and low-density aerogels (at the same MXene/CNF/gelatin/GA ratio of 80/20/0/--) were represented as\ntwo-dimensional periodic cellular structures with rectangular unit cells. The pore dimensions were approximated from the SEM images of experimental samples (Fig. 4c). The FE model structure was represented using plane strain elements within a \\(4 \\times 4\\) supercell, onto which periodic boundary conditions were imposed by relating the displacements of nodes on opposing sides of the structure. To simulate the effects of the random imperfections observed in the SEM images of experimental samples, a constant number of wall discontinuities was seeded for all three FEA models, with the exact number chosen as a tuning parameter. By imposing 30% vertical compression on the supercells, the \\( \\sigma_{30} \\) values were extracted from 10 successive runs with differently seeded discontinuities. The localized stress profiles across the aerogel structures were extracted at both relaxed and compressed states.\n\n**Code availability**\n\nThe Python code to implement the machine learning tasks within this study are available from GitHub (https://github.com/oshin71/Programmable-MXene-Aerogel).\n\n**Data availability**\n\nThe data that support the plots within this paper and other findings of this study are available from the corresponding authors upon reasonable request.\n\n**Acknowledgments**\n\nThe authors acknowledge the financial support provided by the Start-Up Fund of University of Maryland, College Park (KFS No.: 2957431 to P.-Y. Chen). Fundings for this research were\nprovided by MOST-AFOSR Taiwan Topological and Nanostructured Materials Grant under Grant No. FA2386-21-1-4065 (KFS No.: 5284212 to P.-Y. Chen), and Energy Innovation Seed Grant from Maryland Energy Innovation Institute (MEI^2) (KFS No.: 2957597 to P.-Y. Chen).\n\nAuthor contributions\n\nP.-Y.C. and S.S. conceived the project ideas and designed the experiments. T.C., S.S., Y.L., and J.M.L. carried out the synthesis and characterization of MXene nanosheets and CNF. T.C. and H.Y. designed the ML framework and implemented the ML tasks in Python. S.S. and M.M.K. collected the experimental data. K.J.B. and E.T. performed FE simulations and constructed FE models of conductive aerogels. P.-Y.C. and S.S. interpreted the results and co-wrote the manuscript. P.-Y.C., E.T., S.S., K.J.B., Y.L., T.C., J.M.L., H.Y., and M.M.K. were involved in the discussion. P.-Y.C. and E.T. supervised this project.\n\nCompeting interests\n\nAuthors declare no competing interests.\n\nCorrespondence and requests for materials should be addressed to E.T. and P.-Y.C.\nReferences\n\n1 Xue, T. et al. 3D Printed Integrated Gradient-Conductive MXene/CNT/Polyimide Aerogel Frames for Electromagnetic Interference Shielding with Ultra-Low Reflection. 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Click to download.\n\n• SIFinalRef.pdf\n• MovieS1.mp4\n• MovieS2.mp4"} {"paper_id": "prb41", "title": "Biome type and availability of natural vegetation dictate whether farmland intensification or expansion is worse for biodiversity", "text": "# Abstract\n\nTo reduce the biodiversity impact of agriculture, increasing yields on existing farmland has been proposed as an alternative to farmland expansion. However, the relative effects of yield increases versus agricultural expansion have mostly been examined regionally, and measured in terms of species persistence—a metric relevant to extinction risk but limited in describing ecological communities and their support for ecosystem services. Without a thorough analysis, the lower biodiversity impacts of agricultural intensification remain largely speculative. This study provides a global assessment of biodiversity responses to land conversion and yield increases, including closing yield gaps. We also compare the biodiversity impacts of expanding farmland versus intensifying yields in agricultural landscapes to achieve a 1% increase in total production. Utilizing a large biodiversity database, natural vegetation data, and agricultural yield estimates at the landscape scale, we assess three biodiversity metrics: species richness, total abundance, and relative community abundance-weighted average range-size (RCAR), which provides a proxy for biotic homogenisation. Our models highlight that land conversion is associated with significant biodiversity loss at both local and landscape scales, emphasizing the importance of avoiding farmland expansion into new landscapes. However, yield also lead to significant biodiversity loss; closing yield gaps is associated with a median species loss of nearly 11%, and median abundance loss of almost 13%, with some agricultural landscapes losing almost 90% of species and more than 90% in abundance. Additionally, 30% of global agricultural landscapes, predominantly in the tropics, are likely to experience increased biotic homogenization. Neither expansion nor intensification is consistently better for biodiversity, with biome type, crop, biodiversity metric, and percentage of natural vegetation influencing which approach is less harmful. Our results suggest that minimising the biodiversity cost of agriculture requires a context-dependent balance between intensification and expansion in agricultural landscapes.\n\nEarth and environmental sciences/Ecology/Conservation biology \nEarth and environmental sciences/Ecology/Biodiversity \nEarth and environmental sciences/Ecology/Agroecology \nEarth and environmental sciences/Ecology/Macroecology\n\n# Introduction\n\nAgriculture is one of the major drivers of biodiversity loss (Maxwell et al. 2016; Uhler et al. 2021) and many projections suggest that biodiversity loss due to agriculture may continue to occur locally, even under ambitious scenarios that include efforts to limit future demand for agricultural products (Kok et al. 2023; Leclère et al. 2020; Williams et al. 2021). Policies attempting to reduce the biodiversity cost of agriculture often aim to reduce farmland expansion by increasing yields on existing agricultural land (Mueller et al. 2012; Phalan et al. 2014). To understand the effectiveness of this strategy we need to fully quantify the biodiversity impact of yield increases and compare it to the impact of farmland expansion. The intensification-expansion options are often discussed within the land-sparing/sharing framework, in which the two extreme options are land sparing, when production is concentrated on the smallest possible area by intensifying agriculture, and land-sharing, when production is spread with the lowest possible local impact through the use of biodiversity-friendly practices (Balmford 2021). The land-sparing/sharing studies often rely on models of population density in relation to yield at regional scales as a measure of likelihood of species persistence, aimed at understanding extinction risk. Most of these studies conclude that more species would benefit from land sparing than from land sharing when aiming to reach a given production target (Balmford 2021; Dotta et al. 2016; Kamp et al. 2015; Phalan et al. 2014; Williams et al. 2017) whereas other studies show that species responses are mediated by surrounding natural habitat (Gilroy et al. 2014; Karp et al. 2019; Macchi et al. 2020) and land-use history (Feniuk et al. 2019; Finch et al. 2019; Simons & Weisser 2017). Studies of local community metrics in relation to yield, which is important to understand ecosystem service supply (Winfree et al. 2015), and stability of ecological communities (Hatton et al. 2024) are rarer, and show mixed responses of biodiversity to yield increases (Clough et al. 2011; Guerrero et al. 2012; Winqvist et al. 2014; Wurz et al. 2022). Neither species persistence or community metrics response to yield increases were assessed globally so our understanding of the comparative biodiversity impacts of agricultural intensification and expansion is far from complete.\n\nTo quantify the biodiversity impacts of agricultural management, previous large-scale studies have either used broad categories of land-use intensity (which typically consider both agricultural inputs and outputs) (Beckmann et al. 2019; Newbold et al. 2015), modelled proxies such as human-appropriated net primary productivity (Semenchuk et al. 2022), or agricultural inputs such as fertilisers (Semenchuk et al. 2022). As agricultural management is only a means to obtaining a certain level of yield, focusing instead on the biodiversity impact of yield will provide a more direct relationship to consumption patterns, which foregrounds the importance of the demand-side measures to reducing biodiversity impacts of agriculture (Leclère et al. 2020). This approach also provides a more direct relationship to agricultural production as higher agricultural inputs do not always translate into higher yield, and degraded farmland might actually require higher inputs for the same yield level (Ray et al. 2012). Similarly, yields can be increased with lower biodiversity impacts when relying on ecosystem services (Kleijn et al. 2019; Rockström et al. 2017) or using technological improvements benign for biodiversity (Sajjad et al. 2022).\n\nTo fully quantify the biodiversity impact of yield increases, we have to look beyond the most frequently-used metrics of species richness (Attwood et al. 2008; Beckmann et al. 2019; Newbold et al. 2015) and total abundance (Attwood et al. 2008; Newbold et al. 2015), which can obscure changes in community composition. Biotic homogenisation, which happens when ecological communities become increasingly similar across space (Baiser et al. 2012), is often a consequence of human impact even when other biodiversity metrics appear unchanged (Dornelas et al. 2014). One metric capturing biotic homogenisation of ecological communities is the community-average range size, often weighted by the abundance of the component species, because more widely-distributed species are part of more ecological communities, making them more similar (Newbold et al. 2018). Apart from Phalan et al. (2011, 2014) who report how global ranges of birds and trees in Ghana and India relate to species’ ability to persist in agricultural landscapes at different yield levels, few studies report how biotic homogenisation relates to agricultural management (Newbold et al. 2018) and none to different yield levels at global scale.\n\nHere, we provide a large-scale assessment of the biodiversity consequences of yield increases and land conversion in landscapes producing four crops (maize, soybean, wheat and rice). We also compare the potential biodiversity impacts globally of pursuing these two options to achieve a 1% increase in production. We achieve this in three stages, each focused on a related question: 1) what is the biodiversity impact of land conversion in the absence of any yield considerations, considering both local and landscape-level effects of land conversion; 2) within agricultural landscapes, what is the biodiversity impact of increasing yields and closing yield gaps in the absence of land conversion; and 3) using the models developed in step 2, how do the potential impacts of land conversion and yield increases compare across global agricultural landscapes for a hypothetical 1% increase in production? For our purposes, we define landscape scale as the extent of one raster cells in our spatial data. We analyse four crops separately to capture potential differences in landscape types and landscape effects of different management approaches. We use a space-for-time substitution to model three biodiversity metrics: sampled species richness, sampled total abundance, and relative community abundance-weighted average range-size (RCAR). Firstly, we model how biodiversity reacts to land-use conversion locally (farmland versus primary vegetation), and at landscape scale (modified landscapes with less than 30% natural habitat versus natural landscapes with more than 70% natural habitat). Secondly, we model biodiversity impacts of yield increases in cropland, and in primary vegetation in the farmed landscape, accounting also for amount of natural vegetation in the landscape (Hoskins et al. 2016), among other factors, in preparation for answering the third question of this study. To illustrate the potential upper bounds of biodiversity effects of yield increases, we use the selected models to calculate biodiversity change weighted by cropland and primary vegetation proportions in the landscape when closing yield gaps as identified based on agricultural estimates for the year 2000. Thirdly, we compare the impact of conversion against yield increases by using the models produced in step 2 to project biodiversity change in two scenarios: one in which farmland cultivated with the respective crop expands by 1% at the cost of primary vegetation in cultivated landscapes, and one in which the agricultural yield increases by 1% on already existing farmland, leading to identical total production increases.\n\n# Methods\n\nFor biodiversity data, we used the 2016 release of the PREDICTS database, which contains 3,250,404 biodiversity records, mostly sampled from 2000 to 2012, from 666 published studies (Hudson et al. 2017). Each study within the PREDICTS database contains data sampled with the same method across a gradient of land use or land-use intensity. The data in each study are grouped into one or more spatial blocks, each containing data from one or more sites. Each site is attributed one of 6 predominant land-use classes based on the information provided in the original papers, or by the authors of those papers. For our purposes, we selected only those sites located in cropland (i.e., land used for cultivation of herbaceous crops) or primary vegetation (i.e., land showing no evidence of prior destruction of vegetation, either by human actions or extreme natural events), resulting in 1,318,867 records from 10,094 sites from 489 studies. The dataset included 18,853 species of which there were 3,994 vertebrates, 6,693 invertebrates, 7,269 plants, 894 fungi, and three protists. For each of the statistical analyses on relative biodiversity of human-modified and natural landscapes, henceforth land-conversion models, and biodiversity impact of yield, henceforth yield-biodiversity models, we used subsets of these data (Tables S4-S8, Figures S1 – S4), which we selected based on the methods described in ‘Data processing for statistical analysis’, below.\n\nWe used three biodiversity metrics: sampled species richness, total sampled relative abundance, and relative abundance-weighted community-average range size (RCAR). Sampled species richness represented the count of all species sampled at a site, as identified by the authors of the original study (not necessarily always resolving taxonomic synonymy). Total sampled relative abundance was calculated as the sum of abundance measures for all taxa at a site. Abundance was reported in a variety of measures, some of them sensitive to sampling effort. For measures sensitive to sampling effort, and where that effort differed among sampled sites within a study (~1% of records), we corrected the raw abundance measure by dividing it by its relative effort as a proportion of the effort of the most sampled site within a study (Newbold et al. 2015). RCAR is a measure of how widely or narrowly distributed are the species in a community, on average. An increase in RCAR metrics indicates a shift towards more widely distributed species on average, which could be caused either by increases in the number or relative abundance of wide-ranging species and/or by decreases in narrow-ranging species. Similarly, a decrease in RCAR indicates a change toward more narrow-ranged species, on average, which could be caused by increases in narrow-ranged species and/or decreases in wide-ranging species. We used a RCAR metric as calculated in Newbold et al (2018) based on occurrence data from the GBIF database (GBIF.org 2015). The estimated area of occupancy of each species, computed as the sum of the total area of grid cells containing GBIF records of the respective species, was extracted at 55 km × 55 km resolution. Modelled responses of RCAR to land use and land-use intensity have previously been shown to be robust to using different grid resolutions to calculate area or occupancy from GBIF records, and also to using alternative measures of range size, including extent rather than area of occupancy (Newbold et al. 2018). Further details of the methodology for calculating RCAR are detailed in Newbold et al (2018).\n\nFor the yield-biodiversity models, we used global agricultural estimates based on national and sub-national statistics whose spatial allocation to pixel level was modelled following certain assumptions. Different authors will often use the same reported statistics for the same time periods, but present different spatial patterns due to different modelling choices. To account for the influence that different modelling approaches can have on our results, we use here two global agricultural datasets, EarthStat (Monfreda et al. 2008) and MapSPAM (You et al. 2014), but focus on EarthStat for model selection and visualisations and use MapSPAM for robustness testing. Although MapSPAM has the advantage that it covers three years (2000, 2005 and 2010) instead of only one year (2000 for EarthStat), EarthStat provides information on the resolution (i.e., administrative level of reporting) of the reported agricultural data that influences the quality of the spatial modelling (Monfreda et al. 2008), and which we used to discard spatial estimates based on statistics of lower quality. MapSPAM also has the disadvantage that it includes biophysical potential of crops as one of the assumptions used for the spatial disaggregation of agricultural data, which risked creating circularity in our statistical models, because we control for agricultural suitability (see Subsistence yield as proxy for agricultural suitability subsection).\n\nEarthStat agricultural estimates include global estimates of yield and harvested areas for 175 crops in 206 countries around the year 2000 at a spatial resolution of 5’ × 5’ (~10 km × 10 km at equator) (Monfreda et al. 2008). The EarthStat authors preferentially collected subnational agricultural statistics at one (state or province) or two administrative levels (county or district) below the national level, where available. Consequently, data were collected from 2,299 administrative units one level below national from 150 countries (72.8% of the total) and 19,751 units two levels below national from 73 countries (35.4% of the total), with data sometimes available at different subnational levels for different areas of the same country. The largest data source of subnational agricultural statistics was Agro-MAPS (George 2004). Other data sources were national census agencies and agricultural surveys for the largest countries such as United States, Brazil and China (Monfreda et al. 2008). In the absence of subnational statistics, Monfreda et al. (2008) used national-level data from the Food and Agricultural Organisation (FAO, 2006), and independent national level data from Afghanistan, Iraq, Somalia, and Taiwan that were not present in the FAO database. A single value for the lowest available administrative unit was calculated by averaging all the information available for the years between 1997 and 2003. The average reported statistics were then disaggregated spatially onto a gridded map according to the fraction of each cell covered by cropland. Further information regarding the methodology for generating the EarthStat estimates can be found in Monfreda et al. (2008) and Ramankutty et al. (2008).\n\nEarthStat data include spatial layers on yield in tons per hectare, data quality for yield information, total production in tons, fractional harvested area, harvested area in hectares, and data quality for harvested area for each crop in each grid cell. For our analysis, we used yield, data quality for yield information, and the harvested area in hectares layers. Given the widely variable data quality and availability across crops and countries, we selected four of the major crops for which estimates are likely to be more reliable (Monfreda et al. 2008): maize, soybean, wheat and rice, which together represent over 60% of total global calorie production (Tilman et al. 2011). The crops were selected also based on availability of subsistence yield data to be used as a proxy for agricultural suitability. We selected for our analysis the EarthStat estimates that relied on subnational level data at one and two administrative levels below national level (top two data quality scores in the yield data quality spatial layer), disregarding estimates based on national-level and FAO statistics.\n\nMapSPAM agricultural estimates were created with the Spatial Production Allocation Model (SPAM), a model produced by the International Food Policy Research Institute. SPAM uses a range of variables to guide spatial allocation (e.g., probability of crop existence in a spatial unit, biophysical potential, area constraints, management constraints) to guide the spatial allocation of agricultural data into a global 5’ x 5’ (~10 km x 10 km at equator) gridded representation of cultivated area, production quantity and yield under different management regimes for the years 2000, 2005 and 2010 (You et al. 2014). Similarly to EarthStat data, MapSPAM relies on sub-national reported statistics sourced from Agro-MAPS and on additional data collected by authors through research partnerships. The sub-national crop data of MapSPAM were collected from 2,758 administrative units one level below national (compared to 2,299 for EarthStat) and 21,498 units two levels below national (compared to 19,751 for EarthStat). Where in disagreement, the sub-national data were calibrated to agree with the national FAO data (You & Wood 2006). For the rest of the area, FAO national statistics were used. MapSPAM estimates do not include spatial information on resolution of the underlying agricultural data and therefore, it was not possible to select spatial estimates based on the highest resolutions. For the year 2000, estimates were available for 20 crops, while all other crops were included in an additional catch-all group. For the years 2005 and 2010, the estimates include 42 crop categories including the catch-all group. The reported statistics used for each time step were averaged over the three years around the reference year (for example, 1999–2001 for year 2000) (Wood-Sichra et al. 2016). Through a combination of data and expert opinion, MapSPAM authors further disaggregate agricultural estimates into four levels according to farming technology and crop management systems: irrigated, rainfed high inputs, rainfed low inputs and rainfed subsistence. We used MapSPAM subsistence estimates, which assumes rainfed conditions and no inputs, to check for the robustness of models to choice of subsistence yield.\n\nThe SPAM modelling approach combines several types of data (e.g., revenue, market access models, evidence of existing crop distribution, biophysical suitability, information on agricultural management) to create an informed spatial prior covering the territory over which the agricultural statistics are disaggregated (You et al. 2014). While the EarthStat approach uses only land cover information to allocate the reported statistics, the MapSPAM model uses this informed spatial prior together with land cover to allocate agricultural area and production.\n\nWe included percentage of natural habitat in our models because of previous studies indicating the importance of this landscape characteristic on its own (Outhwaite et al. 2022) and in interaction with yield (Macchi et al. 2020) for determining biodiversity patterns. We extracted for each data point the percentage of natural habitat at that location by using a modified version of the land-use estimates from Hoskins et al. (2016). The original dataset at 30-arc-second resolution includes estimates of proportional cover for five land-use classes (urban, cropland, pasture, secondary habitat and primary habitat). These estimates were obtained by downscaling the Land-use Harmonization dataset (Hurtt et al. 2011), a global time series of land use at a resolution of 0.5° that covers the time period 1500–2100. Hoskins et al. (2016) downscale estimates for 2005, based on statistical relationships with fine-scale data on climate, land cover, landform, human population density and accessibility defined at the level of 61 unique combinations of biomes and biogeographical realms. The year 2005 is within the sampling timespan of the PREDICTS data and therefore, a suitable data source. We projected primary and secondary vegetation proportional cover estimates onto a Behrmann equal-area projection, with 1-km spatial resolution, using the projectRaster function with bilinear interpolation in the raster R package, and then summed them to obtain an estimate for natural habitat cover. We then calculated the average percentage cover of natural habitat within 5-km × 5-km grid cells using the ‘zonal’ function in the raster package.\n\nFor the yield-biodiversity models, we used percentage of natural habitat as a continuous variable and interaction term with yield, land use, biome type and subsistence yield, to account for potentially different biodiversity responses to these variables at different levels of natural habitat (Macchi et al. 2020; Outhwaite et al. 2022). For the land-conversion models, we used percentage of natural habitat to select sites that were located in pixels with less than 30% natural vegetation (‘human-modified landscapes’), and pixels with more than 70% natural vegetation (‘natural landscapes’) (Table S4). We chose this threshold of natural habitat based on previous literature showing that biodiversity loss becomes steeper as landscapes lose more than 30% of suitable habitat (Andren 1994). We then combined this landscape classification based on natural vegetation with the PREDICTS land-use classification to create a combined variable describing landscape modification and local land use in four groups: primary vegetation in natural landscapes, primary vegetation in human-modified landscapes, cropland in natural landscapes, cropland in human-modified landscapes.\n\nPrimary vegetation is the land-cover type that preserves best the biodiversity in a landscape and often represents a source of biodiversity-based ecosystem services in agricultural landscapes (Karp et al. 2013), but it is also impacted by neighbouring agricultural expansion and management (Rand et al. 2006). To capture potential differences in the impact of yield increases on cropland and primary vegetation within the same landscape, we included the PREDICTS land-use classification as a variable in the models. For the yield-biodiversity models, we used the original land-use classification from the PREDICTS database and interaction terms between land use, and yield and percentage of natural vegetation as we expect that these effects will differ depending on local land use (Outhwaite et al. 2022). For the land-conversion models, we used the land-use classification in combination with percentage of natural habitat, as detailed above.\n\nWe included a classification of biome type in our models because the different biodiversity patterns and socioeconomic conditions across world biomes is likely to impact the biodiversity response to land use and agricultural management (Newbold et al. 2020). To improve the tractability of statistical models compared to using the usual 14 biomes classification (The Nature Conservancy 2009), we assigned each data point a tropical/non-tropical classification based on their latitude. Data points located between 23.5°N and 23.5°S were identified as tropical, and otherwise as non-tropical. For the yield-biodiversity models, we also included interaction terms between biome type and both yield and percentage of natural vegetation, because these two variables could have different biodiversity impacts depending on the environmental and socioeconomic differences captured by the tropical/non-tropical classification.\n\nThe suitability of different areas for growing crops varies widely, resulting in wide variation in the inputs required to achieve similar yield levels, which might affect biodiversity for a given level of achieved yield. For example, yields reached with irrigation in water limited regions could be comparable to rainfed yields reached in similar but not water limited regions: however, the management footprints – and therefore the biodiversity impacts – could differ. Moreover, agricultural suitability can correlate positively with different biodiversity metrics because often conditions that are favourable for crops are also favourable for many other species (Chown et al. 2003; Luck et al. 2010), distorting the relationship between biodiversity and yield. We used yields in the absence of inputs, irrigation and most human management, i.e., subsistence yields, as a proxy for agricultural suitability for each crop. We used subsistence yields modelled by a version of the Environmental Policy Integrated Climate (EPIC) model, which was initially developed in the United States to model how soil productivity is affected by agricultural management (Williams et al. 1989). Since then, it has been expanded to allow the simulation of yields and agricultural processes at global and regional scales, and their interactions with agricultural management (Balkovič et al. 2013; Izaurralde et al. 2006; Müller et al. 2019). EPIC uses a daily time step and includes components on crop growth, weather simulation, competition, water, carbon and nutrient cycling, and soil processes. Simulated potential plant growth depends on conversion of CO₂ to biomass, intercepted solar radiation and vapour pressure deficit, while stresses from temperature, nutrient deficit, salinity and other soil factors lead to decreased plant growth. We used here a version of the EPIC model developed at University of Natural Resources and Life Sciences (BOKU) in Vienna, Austria, referred to in the literature as EPIC-BOKU (Müller et al. 2018), which was specifically created to estimate yields at different management intensities (Frank et al. 2015; Havlík et al. 2011; Skalskỳ et al. 2008). We used yield simulated with EPIC-BOKU under a subsistence management system without fertilisation or irrigation at 0.5° x 0.5° resolution. The simulation used the WFDEI meteorological forcing data, which represents historical daily-resolution climate data on land at 0.5° × 0.5° resolution based on ERA-Interim reanalysis data (Weedon et al 2014). For analysis with the EarthStat yield estimates for the year 2000, we averaged EPIC-BOKU subsistence yield estimates between the years 1997–2003. Considering that agricultural suitability could have different relationships to biodiversity at different landscape compositions and yield levels, we added in our models interaction terms between subsistence yield and both yield and percentage of natural habitat. For models with MapSPAM, we averaged EPIC-BOKU subsistence yield estimates between the years 1997–2003 for the 2000 yields, 2002–2008 for the 2005 yields, and 2007–2013 for the 2010 yields. We used a five-year averaging window for MapSPAM as we did for EarthStat in order to have subsistence yield values consistent with those in the Earthstat models when performing the robustness tests described below.\n\nWe tested for the robustness of our statistical models to choice of subsistence yield by replacing EPIC-BOKU subsistence yield with MapSPAM estimates of subsistence yield in both the Earthstat-based and MapSPAM-based yield-biodiversity models. MapSPAM estimates of subsistence yield were obtained through a combination of data and expert opinion that allowed authors to disaggregate reported agricultural statistics into four levels according to farming technology and crop management systems: irrigated, rainfed high inputs, rainfed low inputs and rainfed subsistence. For a few large countries management information was collected at the level of the first subnational administrative level below national (You et al. 2014). The authors collected information at national level on the ratios of yields under irrigated and rainfed conditions, and under high-input rainfed and low-input rainfed conditions for each crop. They then use these two ratios and areas under different production systems to calculate estimates of yield under different management systems, using reported yields as average yields across all the production systems within a pixel.\n\nTo control for additional factors that could influence biodiversity outcomes in the yield-biodiversity models, we extracted a number of spatial variables at the locations of our biodiversity data to be included in the statistical models. Crop diversity has been found to sometimes have a positive effect on local biodiversity (Palmu et al. 2014). We therefore calculated a Shannon crop diversity index based on all EarthStat estimates for all 175 crops:\n$$\n{H}^{\\prime }=-\\sum _{i=1}^{n}{p}_{i}\\text{ln}{p}_{i}\n$$\n, where H’ is the Shannon index, pi is the proportion of cropland covered by crop i out of the total cropland for all n crops in the pixel. The EarthStat estimates were more appropriate for this calculation as Earthstat data covers a greater number of crops than MapSPAM.\n\nTo account for potential effects of agricultural management and expansion at a larger scale than the pixel scale, we used percentage of natural habitat, as well as yield data from EarthStat and MapSPAM, to calculate an average percentage of natural habitat and yield in a one-pixel buffer (~10-km radius) around the focal pixel where the PREDICTS site was located. Because the average yield/percentage of natural habitat in the buffer was highly correlated with the value in the focal pixel, we calculated and used in the statistical models the difference between the buffer and the focal pixel value (buffer-focal difference). The yield buffer-focal difference calculated with EarthStat was used in the yield-biodiversity models with EarthStat data and the yield buffer-focal difference calculated with MapSPAM was used in the robustness checks with MapSPAM data.\n\nTo account for the duration of substantial human landscape modification, we used the HYDE model (Klein Goldewijk et al. 2011) to calculate the number of years since 30% of a grid cell (0.5° × 0.5° resolution) is estimated to have become covered by human land uses. We then extracted this information at the location of the biodiversity data. Finally, we also extracted climate information at the location of the biodiversity data, based on the WorldClim estimates of historical annual mean temperature and annual precipitation for the period 1970–2000 (Fick & Hijmans 2017). We added climate variables in our models because climate is an important determinant of biodiversity levels. However, climate might also correlate strongly with some of our models variables (e.g, yield, subsistence yield), in which case the respective climate variable was removed.\n\nWe loge-transformed variables with right-skewed distributions: annual precipitation, MapSPAM yield, and MapSPAM subsistence for all crops, EPIC-BOKU subsistence for maize and wheat, and EarthStat yield for rice. We added a value of 0.01 (less than 1% of the highest value) to deal with 0 values for MapSPAM subsistence yields for all crops, and for EPIC-BOKU subsistence-yield estimates for maize. Variables with left-skewed distributions were transformed with the formula:\n$$\n{V}_{t}={log}_{e}(C-V)\n$$\n, where Vt is the transformed variable, C is a constant used to avoid negative values, and determined by adding a small number to the highest value of the respective variable and rounding it up. Variables with a left tail distribution were duration of substantial human landscape modification for all crops (with C = 2005, obtained by rounding up the sum between maximum value 1981.6 and 20) and annual mean temperature for rice (with C = 30, obtained by rounding up the sum between maximum value 28.5° and 1°). We then scaled all continuous variables to have a mean of 0 and a standard deviation of 1.\n\nAll spatial estimates were transformed to the Behrman equal-area projection and resampled to the EarthStat resolution and extent in R (R Core Team 2022) with the projectRaster and resample functions, respectively, from the raster package, version 3.6–23 (Hijmans 2023). We used bilinear interpolation for spatial averaging. We then extracted the values within spatial layers at the locations of the PREDICTS sites based on geographical coordinates. For the yield-biodiversity models for each crop, we selected all PREDICTS sites in primary vegetation or cropland that fell within pixels that contained cultivated areas of the respective crop according to EarthStat estimates (at the highest or second-highest data quality level; see Global Agricultural Estimates subsection). The PREDICTS cropland classification does not differentiate according to the crop cultivated at the precise sampling location. Therefore, the biodiversity data were sampled in landscapes used to grow the focal crops (according to EarthStat estimates), even if the actual sample may have been taken in a different crop. In doing so, we assume that intensification levels tend to be similar across cropping systems within an agricultural landscape.\n\nFor the MapSPAM yield, we chose either the 2000, 2005 or 2010 estimates based on which of the three years was closest to the year of the midpoint of the collection dates for each PREDICTS site. If a midpoint year was equally close to two MapSPAM years, we chose the earlier year because that would be more likely to represent the agricultural management impacting biodiversity by virtue of preceding in time.\n\nFor the land-conversion models, we used sites that were either in natural landscapes (> 70% natural vegetation) or human-modified landscapes (< 30% natural vegetation), a total of 5,328 sites (Table S1). For yield-biodiversity models, the spatial intersection between PREDICTS data and EarthStat estimates resulted in 4,862 sites for maize; 2,404 sites for soybean; 3,227 sites for wheat; and 2,810 sites for rice (Tables S5 - S8) with at least species richness data.\n\nWe tested for correlations among all explanatory variables for both the yield-biodiversity and land-conversion models. Collinearity among variables was generally low with most correlations between variables being very weak (0 to 0.2) or weak (0.2 to 0.4). A few pairs of variables were moderately correlated (0.4 to 0.6) and a maximum of one pair of variables were strongly correlated (0.6 to 0.8) for some of our statistical models (Table S6). When a pair of variables was strongly correlated, we eliminated one of them (Table S6), prioritising yield, percentage of natural habitat and subsistence yield measures (in this order) to be kept for modelling. In all cases, it was climate variables (annual mean temperature and annual precipitation) that had to be removed due to high correlations with EarthStat yield, Epic-BOKU subsistence yield or, in the case of the yield-biodiversity model for rice, with percentage natural habitat.\n\nWe modelled separately the three biodiversity metrics – species richness, abundance and RCAR – using mixed-effects models with random effects for study identity and spatial block nested within study, to account for non-independence of sites. The random effect for study accounted for differences in sampling methods, sampling effort, focal taxonomic group and broad geographic regions among the different studies in PREDICTS. The random effect for spatial block accounted for the spatial structuring of sampling within a study. To account for overdispersion, we included a random effect for site in the models for species richness (Rigby et al. 2008). To reduce the right skew in the abundance data due to measurements across many taxonomic groups and with a variety of methods, we scaled total abundance by dividing values by the maximum abundance within each study (Outhwaite et al. 2022 a). We then loge-transformed the rescaled values to further reduce the skew of the distribution adding 0.01 to deal with 0 values.\n\nFor the yield-biodiversity models, each data point/site was weighted in the statistical analysis by the area of the respective crop as a fraction of all crops grown in the pixel to account for the differences in crop composition of agricultural landscapes according to the formula:\n$$\n{RA}_{C}= \\frac{{A}_{C}}{{\\sum }_{i=1}^{175}{A}_{i}}\n$$\nwhere RAC is relative area for crop C, where C is maize, soybean, wheat or rice, AC is the harvested area in hectares for crop C, and Ai is the harvested area for each of the 175 crops available in the EarthStat dataset. We rescaled the area fractions such that the average weight is equal to 1, to avoid an apparent reduction in total sample size, which would have an adverse influence on some statistical properties:\n$$\n{Rescaled\\_RA}_{C}= {N}_{Sites}\\frac{{RA}_{C}}{\\sum _{j=1}^{{N}_{Sites}}{RA}_{j}}\n$$\nwhere NSites is the total number of sites resulting from combining the biodiversity and agricultural data for each crop. We rescaled the area fractions again for each crop and biodiversity metric because the rescaled weights are dependent on the total sum of relative areas, which changes with number of data points.\n\nThe default set of initial variables for the land-conversion models was: annual mean temperature, annual precipitation, biome type, and the combination of landscape conversion and local land use. The default set of initial variables for the yield-biodiversity models was: EarthStat yield, yield buffer-focal difference, percentage of natural habitat, percentage of natural habitat buffer-focal difference, EPIC-BOKU subsistence yield, duration of substantial human landscape modification, crop diversity, annual mean temperature, annual precipitation, biome type (tropical/non-tropical), and land use as identified in the PREDICTS database. This set of variables was modified by removing correlated variables for both type of models, as described above (Table S6). For all yield-biodiversity models, we initially included six 2-way interactions: between EarthStat yield and each of the variables EPIC-BOKU subsistence yield, percentage of natural habitat, land use and biome type; and between percentage natural habitat and each of the variables EPIC-BOKU subsistence yield measure, land use and biome type (justifications for considering these interactions were described above). For the soy RCAR model, due to model convergence issues we had to remove 3 of the 6 interactions: EPIC-BOKU subsistence yield interactions with yield and percentage of natural vegetation, and the interactions between biome type and percentage of natural vegetation, which we considered having less support in the literature. Annual mean temperature was also removed as a main effect from the initial model structure, in addition to annual precipitation, which was removed due to a high correlation with EPIC-BOKU subsistence yield. The convergence issues were probably triggered by a reduction in data points (1,482 RCAR data points compared to 2,404 for species richness).\n\nFor both yield-biodiversity and land conversion models, we modelled species richness using generalised linear mixed-effects models with a Poisson distribution, while for (loge-transformed) abundance and (log10-transformed) RCAR we used linear mixed-effects models. We performed backward stepwise selection based on likelihood-ratio tests with a p-value threshold of 0.05 to select the fixed-effects structure for each model. The selected model structures are presented in Table S7. As an alternative way to deal with overdispersion, we reran the species richness models substituting the Poisson distribution with a negative binomial distribution and dropping the random effect for site (Table S20). To test the consistency of our results, we also ran the final model structures using a Bayesian modelling framework (Table S21). These models using uninformative priors used 4 Markov chains and 5000 iterations with 2500 warmup iterations. We considered that the models converged if Rhat convergence diagnostic was ≤ 1.01 and rank-normalized effective sample size was ≥ 400, which represents 100 times the number of chains (Stan Development Team 2024).\n\nWe conducted all statistical analyses and projections of biodiversity impacts of yield increases in R 3.6.3 (R Core Team 2022). For the mixed-effects modelling, we used the glmmTMB package, version 1.1.5 (Brooks et al. 2017). For model selection, we adapted several functions from the packages associated with the PREDICTS data (Newbold 2018). For checks of the models assuming a Poisson distribution we used DHARMa package (Hartig 2022), and for the Bayesian models we used the brms package (Bürkner 2021).\n\nWe used the best EarthStat–EPIC-BOKU models to project biodiversity change when closing yield gaps for the global areas occupied by the four crops in the year 2000. Yield gaps where defined by Mueller et al. (2012) as the difference between attainable yields, which are the area-weighted 95th percentiles of observed yields within zones of similar annual precipitation and growing-degree days, and yields given by the EarthStat estimates for the year 2000 that are below attainable yield values for the area. We first projected biodiversity levels in cropland and primary vegetation for yield levels in the year 2000. We then used the same models to project biodiversity levels in cropland and primary vegetation at yields equal to those necessary to close yield gaps. We then calculated an aggregated estimated biodiversity value across all four crops for each pixel, for each metric at each of the two yield levels, using the following formula:\n$$\nBD= \\sum _{i}^{n=4}{p}_{i}({BD}_{Cropland}{p}_{Cropland}+ {BD}_{PV}{p}_{PV})\n$$\nwhere BD is the biodiversity metric in the respective pixel, pi is the proportion of crop i in the total cropland of the respective pixel, BDCropland and BDPV are values of the biodiversity metric estimated by the yield-biodiversity model for cropland and primary vegetation, respectively, and pCropland and pPV are proportion of each land use type out of the total area of the pixel. Where land use was not selected in the fixed structure of the best models, BD was identical for both primary vegetation and cropland. We calculated the percentage change in biodiversity relative to the biodiversity corresponding to the year 2000 yields by subtracting in each pixel the biodiversity metric at gap-closing yields from the biodiversity metric corresponding to year 2000 yield and dividing the difference by the biodiversity metric corresponding to year 2000 yields. The biodiversity contribution of the other land uses in the pixel are assumed to be constant at the two time steps and therefore, it does not influence percentage change in biodiversity.\n\nCropland expansion can take place at the cost of most land-uses present in a landscape at a given time. Cropland expansion into other land-uses than primary vegetation (e.g., pastureland) is likely to lead to lower biodiversity impacts. We consider here cropland expansion at the cost of primary vegetation to establish a “worst-case scenario” against which to compare intensification. It is important to note that our scenarios for achieving a 1% increase in production exclusively through either intensification or cropland expansion into primary vegetation are not realistic projections for the future but rather extreme cases of a range of possible strategies. However, this scenario exercise allows us to contrast the biodiversity outcomes of intensification and expansion as two extreme approaches to increasing agricultural production.\n\nTo compare cropland expansion into primary vegetation to intensification within cropland, we used the EarthStat–EPIC-BOKU models to project biodiversity metrics for two scenarios that would yield identical increases of total production in each pixel for each crop. We then aggregated the biodiversity metric in each pixel for each crop according to the formula:\n$$\nBD=({BD}_{Cropland}{p}_{Cropland}+ {BD}_{PV}{p}_{PV})\n$$\nwhere BD is the biodiversity metric in the respective pixel, BDCropland and BDPV are the model-estimated values of the biodiversity metric for cropland and primary vegetation, respectively, and pCropland and pPV are proportion of each land-use type out of the total area of the pixel.\n\nFor the expansion scenario, we kept the yield equal to the year 2000 yield but increased the area cultivated with the respective crop by 1% at the cost of primary vegetation in the pixel, thus changing pCropland and pPV in favour of a larger pCropland. This meant also a decrease by the equivalent area in the total percentage of natural habitat variable in the respective yield-biodiversity model. For the intensification scenario, the only variable that changed was the yield for each crop, which increased by 1%. We then calculated a percentage change in biodiversity by extracting the biodiversity calculated for the intensification scenario from the biodiversity calculated for the expansion scenario and dividing the difference by the biodiversity metric corresponding to year 2000 yields and landscape composition. The biodiversity contribution of the other land uses in the pixel are assumed to be constant between the two scenarios and equal to the biodiversity of these land uses corresponding to the year 2000 yield and landscape composition.\n\n# Results\n\nRelative to primary vegetation in natural landscapes, all other habitat-landscape categories showed reductions in species richness (Fig. 2 a.) and abundance (Fig. 2 b.), and increases in relative abundance-weighted community-average range size (RCAR) (Fig. 2 c.). Species richness is estimated to decrease by -19.3% [95% CI: -26.8%, -11%] in primary vegetation in modified landscapes, by -26.6% [95% CI: -32.2%, -20.5%] in cropland in natural landscapes, and by -31.8% [95% CI: -39.1%, -23.7%] in cropland in modified landscapes, relative to primary vegetation in natural landscapes. Abundance is estimated to decrease by -37.5% [95% CI: -48.2%, -24.6%] in primary vegetation in modified landscapes, by -30.5% [95% CI: -41%, -18.3%] in cropland in natural landscapes, and by -56.7% [95% CI: -64.9%, -46.7%] in cropland in modified landscapes. RCAR is estimated to increase by 33.9% [95% CI: 9%, 64.6%] in primary vegetation in modified landscapes by 90.1% [95% CI: 65.4%, 118.5%], in cropland in natural landscapes, and by 102.4% [95% CI: 59.3%, 157.2%] in cropland in modified landscapes.\n\nBiodiversity change with yield increases is mediated by land use, biome type and percentage of natural habitat in the landscape. Yield increases were associated most often with decreases in species richness (Fig. 3 a, c, d), except in landscapes used to grow soybeans, where soybean yield increases were not associated with any changes in species richness (Fig. 3 b), and in landscapes used to grow rice in which there is a high percentage of natural vegetation, where rice yield increases were associated with increases in species richness (Fig. 3 d). The association between yield increases and total abundance is more complex (Fig. 3 e, f, g, h), the interaction with biome type becoming important to explain abundance patterns within landscapes with maize, soybean and rice cultivation (Figure e, f, h, respectively). The general pattern is that total abundance increases with yield in tropical landscapes and decreases in temperate landscapes, while high levels of natural vegetation accelerate increases and dampen decreases in tropical and non-tropical landscapes, respectively. In landscapes used to grow wheat, total abundance decreases with increases in yield, most strongly in landscapes with a high percentage of natural vegetation (Fig. 3 g). Biome type impacts the effects of maize and soybean yield on RCAR, with tropical landscapes experiencing strong negative biodiversity impacts of increasing yields (i.e., steep increases in RCAR), and non-tropical landscapes showing smaller impacts or even decreasing RCAR with increasing yields (Fig. 3 i, j). In landscapes with rice cultivation, RCAR decreases with increasing yield where the percentage of natural vegetation is high, but increases in landscapes with a low percentage of natural vegetation (Fig. 3 l). Wheat yield was not associated with any change in RCAR. The models were robust to the choice of subsistence yield and fairly robust to the choice of yield data (Tables S10-S19). Most models using yields from MapSPAM agreed with the models that used yields from EarthStat in direction, or in both direction and magnitude of biodiversity change (Table S9). The only MapSPAM yield models that did not agree on the direction of the effect of yield on biodiversity were rice-total abundance and maize-RCAR models (Tables S16-S17).\n\nAmong the other variables, subsistence yield was selected in 7 of the 12 models (4 crops X 3 biodiversity metrics), had both positive and negative effects on biodiversity, and interacted with yield and percentage of natural habitat, especially in the total abundance models. All the other variables were selected in 4 or less of the 12 models. Crop diversity had a negative effect on species richness and abundance in maize landscapes but it had a positive effect on abundance in soy landscapes. Duration of substantial human landscape modification had a positive impact on total abundance in maize and rice landscapes.\n\nThe variance explained by fixed effects (marginal pseudo-R²) for all models varied between 0.05 and 0.36, whereas the variance explained by fixed and random effects together (conditional pseudo-R²) varied between 0.52 and 0.98 (Nakagawa & Schielzeth 2013). These levels of pseudo-R² are typical for models based on datasets collected from multiple source, in which most of the variation is explained by the random effects (Williams et al. 2022). The model diagnostic plots suggest that our models do not fully fit model assumptions (Figure S5 – S21). The use of the negative binomial instead of the Poisson distribution for the species richness models did not substantially improve model behaviour (Figure S5-S12). The estimated effects were similar to the Poisson models, with weaker negative effects for the negative binomial land conversion model for species richness (Figure S13, Table S20). The Bayesian models produced very similar results to the original models (Table S21).\n\nWhen closing yield gaps for all four crops, as estimated for the year 2000, 83% of all grid cells would experience a decrease in species richness. Mean species richness change per pixel globally was −11.8% and the median was −10.8%. The decrease in species richness is spread across both tropical and non-tropical areas (Fig. 4 a). The small areas of species richness increases are likely due to positive rice yield effects in landscapes with a high percentage of natural habitat and wheat yield effects in landscapes with very low percentage of natural habitat (Figure S24). 63% of all grid cells will experience a decrease in total abundance with an average of +62.6% change driven by high abundance increases for maize and soybean in tropical areas (Figure S25), and a median of -12.7%. Non-tropical areas are almost all characterised by decreases in abundances (Fig. 4 b). For RCAR, 34% of grid cells will experience a negative biodiversity impact and almost all of them are in tropical areas (Fig. 4 c). The difference in biomes type patterns are most likely driven by soybean and maize yield RCAR effects (Fig. 3 I, j). The average projected RCAR change across all grid cells was +61.6% with a median of 0%. Almost 20% (19.8%) of grid cells had a 0% change in RCAR, these likely representing non-tropical landscapes with wheat cultivation (Figure S26).\n\nWhen comparing hypothetical options for increasing total production by 1% in existing agricultural landscapes, neither expansion, nor intensification had uniformly better estimated biodiversity outcomes in all locations. Intensification was associated with better biodiversity outcomes in terms of species richness than farmland expansion on 0.4%, 67.3%, 10.9% and 47.4% of the cultivated areas for maize, soybean, wheat and rice respectively (Fig. 5 a, b, c, d). Farmland expansion was associated with higher species richness on the rest of the cultivated areas, i.e., the majority of land cultivated with maize, wheat and rice, especially in non-tropical areas (Fig. 5 a, b, c, d). In terms of total abundance, modelled intensification was associated with more positive outcomes on 37.9%, 34.6%, 5.8% and 55.5% of the cultivated areas for maize, soybean, wheat and rice respectively. Thus, farmland expansion was associated with higher total abundances on most of the land cultivated with maize, soybean and wheat, but intensification was estimated to be better across much of the tropics (Fig. 5 e, f, g, h). For RCAR, farmland intensification resulted in better modelled outcomes on 62.3%, 60.5%, 60.4% and 40.2% of the cultivated areas for maize, soybean, wheat and rice respectively. In this case, intensification was the better production-growing strategy compared to farmland expansion for three of the four crops: maize, soybean and wheat. However, farmland expansion resulted in better modelled outcomes in the tropics, especially for maize and soybean (Fig. 5 I, j, k, l).\n\n# Discussion\n\nWhen looking at the biodiversity impact of land conversion separately from yield considerations, impacts of both local land use and landscape composition are uniformly negative and relatively strong across species richness, total abundance and relative abundance-weighted community-average range size (RCAR). Our results are consistent with previous studies on local land-use change (Gibson et al. 2011; Murphy & Romanuk 2014; Newbold et al. 2015) and landscape composition effects (Outhwaite et al. 2022). More specifically, our results highlight the importance of considering the landscape context when designing and implementing conservation management. For instance, biodiversity in primary vegetation in agricultural landscapes changes compared to primary vegetation in natural landscapes across all three metrics. This suggests that primary vegetation in human-modified landscapes has less conservation value than primary vegetation in natural landscapes (Chase et al. 2020; Venter et al. 2016) and highlights the high biodiversity costs of expanding agriculture in previously unfarmed landscapes. However, primary vegetation in modified landscapes likely represents an important source of biodiversity and ecosystem services for the surrounding farmland (Karp et al. 2013; Outhwaite et al. 2022).\n\nWhen looking at the biodiversity impacts of yield or agricultural management, large-scale studies of biodiversity impacts rarely assess how the direction of these effects might differ in different biomes. In our results, tropical landscapes cultivated with maize and soybean show an increase in total abundance and an increase in biotic homogenisation, as measured by RCAR (Fig. 3), suggesting that abundance increases are driven by widespread species (Newbold et al. 2018). Indeed, previous research in tropical areas showed that species with large global ranges are more likely to persist and thrive in agricultural landscapes (Phalan et al. 2011, 2014). In non-tropical soy and maize landscapes, both total abundance and biotic homogenisation generally decrease, suggesting that abundance decreases in these landscapes are also driven by changes in the abundance of widespread species, this time decreases. Supporting evidence for this pattern comes from abundance decreases in common European birds (Inger et al. 2015), often attributed to agricultural intensification (Rigal et al. 2023). There are two considerations that can help interpret these opposing responses of widespread species to yield increases. Firstly, most tropical yields in our data are at the lower end of the yield range whereas non-tropical yields are more equally distributed (Fig. 3, data distribution rugs at the bottom of all panels). Therefore, the tropical trends in our data are likely to be representative of lower yields, whereas the non-tropical trends likely capture biodiversity trends across a wider yield range. Secondly, non-tropical areas, especially temperate regions, tend to have a longer history of human occupation, and smaller areas of natural habitats than tropical landscapes (Venter et al. 2016). This probably led to farmland-intolerant species being filtered out (Balmford 1996) and farmland-tolerant species increasing in abundance well before the accelerated intensification of the last decades. These ecological communities dominated by farmland-tolerant species in lower intensity agriculture still persist in Eastern European traditional landscapes (Sutcliffe et al. 2015). We speculate that the tropical biodiversity trends in our results capture the type of community change that had happened in the past in non-tropical agricultural landscapes, whereas the non-tropical trends capture mainly the response of farmland tolerant species to the recent high levels of intensification in non-tropical areas.\n\nPrevious research has shown the importance of natural habitat in buffering the effects of human activity on biodiversity (Macchi et al. 2020; Outhwaite et al. 2022) but our results suggest nuanced effects depending on crop. In landscapes with wheat cultivation, areas with higher percentage of natural habitat experience steeper decreases in species richness and abundance with yield, likely from higher initial biodiversity as natural habitat is positively related to species richness and abundance in wheat landscapes (Table S20). This suggests that aspects of wheat landscapes or their management might undermine the ability of natural habitat patches to buffer the impact of yield increases, in accordance with research highlighting the importance of landscape context for the biodiversity value of natural habitat patches (Bennett et al. 2004). In maize and soybean landscapes, higher percentage of natural habitat has a positive impact on the effect of yield on total abundance, accelerating increases in tropical and dampening decreases in non-tropical biomes, but a negative biodiversity impact in terms of biotic homogenisation, accelerating RCAR increases in tropical and dampening decreases in RCAR in non-tropical biomes. These results suggest that natural habitat in these landscapes is beneficial mostly to widespread species, that are able to use natural habitat to either benefit or avoid the most serious losses caused by increases in yield (Tscharntke et al. 2002). In landscapes with rice cultivation, higher percentage of natural habitat has a positive impact on the effect of yield on biodiversity as measured by all three metrics. This suggests that species richness and abundance increases with rice yield in landscapes with high percentage of natural habitat is driven by narrow-ranged species. This could be due to the specific requirements of rice cultivation that often involves a period of water submergence (Bambaradeniya & Amerasinghe 2004), which creates temporary wetlands that can be functionally equivalent to more natural wetlands (Elphick 2000). Given that wetland represent only 5–10% of the global land surface and that more than half of the global wetland area has been destroyed or modified (Kingsford et al. 2016), species that are likely to benefit from anthropogenic wetlands created by agriculture are likely to be relatively narrow-ranged (Dudgeon et al. 2006). Our results suggest that a certain amount of natural habitat is necessary for this to happen, as suggested by research that shows the importance of natural habitat for connecting populations of wetland species (Quesnelle et al. 2013).\n\nAlthough closing yield gaps was proposed over a decade ago as a solution to the challenge of producing food while protecting biodiversity (Foley et al. 2011), there are surprisingly few quantitative assessments of its biodiversity impacts. Compared to existing assessments, our results suggest more severe losses in local biodiversity when closing yield gaps. Kehoe et al. (2017), who analyse the biodiversity impact of maximising agricultural intensity on all existing farmland, estimate a maximum of 7% loss in species richness, which contrasts with our maximum of 89.1% species loss, and 13% loss is abundance, which contrasts with our maximum 99.7% loss in abundance from closing yield gaps. In their analysis, intensification on all existing cropland leads to little change in species richness and abundance in many areas, compared to our analysis, in which closing yield gaps leads to decreases in species richness on over 80%, and in abundance on over 60% of the global agricultural landscapes. Kehoe et al. (2017) used modelled estimates of biodiversity loss from a global study of land use impact on biodiversity using the same dataset from which we derived our data (Newbold et al. 2015). The difference in results is likely due to the focus of Newbold et al. (2015) on agriculture in general rather than crop type, and absence of interactions between intensity, and natural habitat or biome type in their statistical models (Newbold et al. 2015). As indicated by our analysis, these elements can have opposing effects on biodiversity, and therefore, the negative impacts can be obscured in simpler models. Comparisons with existing assessments of the biodiversity costs of closing yield gaps is complicated further by the use of different biodiversity metrics. For example, Egli et al. (2018) use a metric capturing the value of each pixel with any amount of farmland for the global survival of terrestrial mammals, birds and amphibians. Based on assumed responses of species persistence to agricultural intensification based on habitat preferences, the authors estimate a decrease of 11.1% in the global biodiversity value of agricultural lands due to closing yield gaps. Although the biodiversity metric used by Egli et al. (2018) is not directly comparable to our metrics, the spatial patterns of high biodiversity loss tend to agree, especially with our RCAR patterns in the tropics.\n\nConsidering the reduced biodiversity in primary vegetation in modified landscapes (Fig. 2) and the strong association between yield and negative biodiversity outcomes in some landscapes (Fig. 3), it is not surprising that agricultural intensification is not always the best solution for increasing agricultural production in terms of local biodiversity outcomes (Fig. 5). Land-sparing/sharing studies at regional scale usually conclude that land sparing, i.e. intensification, results in better outcomes in terms of reducing extinction risks (Balmford 2021). To the extent that biotic homogenisation of communities as measured here does lead to higher extinction risks, our results disagree with the land-sparing/sharing research as many tropical areas in our results experience higher biotic homogenisation when raising yields by 1% than by expanding cropland by 1% at the expense of primary vegetation. However, our models do not account for the configuration of cropland and primary vegetation areas in our pixels, which is an important aspect of the land-sparing/sharing framework that recommends sharing or sparing of patches of at least 1–10 km² (Balmford 2021). Moreover, it is important to emphasise that we are comparing intensification and expansion within existing agricultural landscapes, and that expanding agriculture into new landscapes will lead to significant decreases in biodiversity (Fig. 2).\n\nOur study has several limitations that need to be considered when interpreting the results. First, our focus on the direct association between biodiversity metrics and yields means that relationships may change if agricultural management practices differ from those used at the sampled locations. As a consequence, our results are most representative of the time window represented by the EathStat and PREDICTS data, which is the time period between 2000 and 2005. Although it is reasonable to assume that agricultural practices have not changed dramatically since then, closing yield gaps would probably result in considerable changes in management practices in some areas, which might change the biodiversity trends presented here. Second, our cropland data were not sampled necessarily within cropland cultivated with the particular crops for which we are using landscape-scale yield estimates. Therefore, our models capture landscape-scale but not local-scale impacts of crop-specific management. Third, our choice of classifying sites into tropical or non-tropical biome types based on latitude, although it avoids other limitations (see Methods), leads to unnatural artefacts in our figures where the border between positive and negative impacts is often a straight line (e.g., Figs. 4 and 5), whereas any changes in the relationship between biodiversity and yield in real landscapes would be more gradual. Fourth, all the limitations inherent to the datasets we use, such as geographical and taxonomical biases in PREDICTS (Hudson et al. 2017), and data and downscaling uncertainties in EarthStat (Monfreda et al. 2008) are carried over to our own study. Fifth, there are several limitations of using spatial biodiversity data to infer changes through time, most importantly an inability to consider time lags in biotic changes and responses to environmental changes (Wearn et al. 2012). Finally, some of our more models were less robust to the choice of yield data source (Table S9) and their results should be interpreted with caution.\n\nBoth land conversion and increasing agricultural yields have significant biodiversity impacts. In particular, closing yield gaps will likely lead to at a much higher biodiversity cost than previously estimated (Kehoe et al. 2017) and the increase in biotic homogenisation with agricultural yields in the tropics is particularly worrying from a global biodiversity perspective. Given the mostly positive impact of natural habitat on biodiversity and ecosystem services, there is likely a balance that can be struck between intensification and expansion in agricultural landscapes but this balance might change depending on biome, crop, conservation goals and remaining natural vegetation in the landscape. 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Generating global crop distribution maps: From census to grid. *Agricultural Systems*, 127, 53–60."} {"paper_id": "prb42", "title": "Matrix condition mitigates the effects of habitat fragmentation on species extinction risk", "text": "Matrix condition mitigates the effects of habitat fragmentation on species extinction risk\n\nJuan Ramírez-Delgado (delgado@unbc.ca)\nUniversity of Northern British Columbia https://orcid.org/0000-0003-2673-0741\nMoreno Di Marco\nSapienza University of Rome\nJames Watson\nUniversity of Queensland\nChris Johnson\nUniversity of Northern British Columbia\nCarlo Rondinini\nSapienza University of Rome https://orcid.org/0000-0002-6617-018X\nXavier Corredor Llano\nUniversity of Northern British Columbia\nMiguel Arias\nUniversity of Northern British Columbia\nOscar Venter\nUniversity of Northern British Columbia\n\nArticle\n\nKeywords: Habitat Loss, Global Biodiversity Decline, Human Footprint Levels, Conservation Action\n\nPosted Date: March 18th, 2021\n\nDOI: https://doi.org/10.21203/rs.3.rs-340760/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nVersion of Record: A version of this preprint was published at Nature Communications on February 1st, 2022. See the published version at https://doi.org/10.1038/s41467-022-28270-3.\nTitle\nMatrix condition mitigates the effects of habitat fragmentation on species extinction risk\n\nAuthors\nJuan Pablo Ramírez-Delgado*1, Moreno Di Marco2,3, James E.M. Watson3,4,5, Chris J. Johnson1, Carlo Rondinini6, Xavier Corredor Llano1, Miguel Arias1, Oscar Venter1\n\nAffiliations\n1Natural Resources and Environmental Studies Institute, University of Northern British Columbia, Prince George V2N 4Z9, Canada.\n2Department of Biology and Biotechnologies, Sapienza University of Rome, Rome 00185, Italy.\n3School of Earth and Environmental Sciences, University of Queensland, St Lucia 4072, Australia.\n4Centre for Biodiversity and Conservation Science, School of Biological Sciences, The University of Queensland, Brisbane 4072, Queensland, Australia.\n5Wildlife Conservation Society, Global Conservation Program, Bronx, NY 20460, USA.\n6Global Mammal Assessment Program, Department of Biology and Biotechnologies, Sapienza University of Rome, Rome 00185, Italy.\n\n*Correspondence and request for materials should be addressed to J.P.R.-D. (delgado@unbc.ca)\nAbstract\n\nHabitat loss is the leading cause of global biodiversity decline, but the influence of human pressure within the matrix surrounding habitat fragments remains poorly understood. Here we measure the relationship between fragmentation, matrix condition (measured as the extent of high human footprint levels), and the change in extinction risk of 4,327 terrestrial mammals. We find that the matrix condition and the fragmentation of habitat are strongly associated with changes in species extinction risk. Importantly, we discover that fragmentation is a stronger predictor of risk than species life-history traits, habitat loss, and habitat amount. Moreover, the importance of fragmentation increases with an increasing deterioration of the matrix condition, highlighting the critical influence matrix quality plays on the effects of fragmentation. These findings suggest that restoration measures in habitat matrices may be an important conservation action for mitigating the effects of fragmentation relative to extinction risk of terrestrial mammals.\n\nMain\n\nAlthough habitat loss is the leading cause of ongoing biodiversity loss\\( ^{1-4} \\), the degree to which habitat fragmentation, defined as the spatial arrangement of remaining habitat for a given amount of habitat loss, influences the loss of biodiversity has remained the focus of considerable debate\\( ^{5-10} \\). Central to the debate has been a persistent uncertainty in disentangling the effects of habitat loss on biodiversity from the effects of fragmentation \\( per se \\), especially relative to the reduction in patch size and the increase in patch isolation\\( ^{8,11} \\). Whereas some studies have challenged the assumption of the impacts of fragmentation\\( ^{6,8,9,12} \\), others have demonstrated that the effects of fragmentation are negative and stronger for local species\\( ^{5,7,13,14} \\), particularly in the tropics\\( ^{15} \\) and\nat intermediate (30–60%) levels of habitat amount\\(^{16,17}\\). Resolving this debate is critical to not just informing efforts to prioritize the protection and management of intact and fragmented landscapes with the same total amount of habitat, but also to better understand the role of the areas surrounding patches of habitat, commonly referred to as the ‘matrix’, in maintaining biodiversity\\(^{10,18,19}\\).\n\nThe traditional characterization of landscapes, which views patches of habitat as islands embedded in a matrix of non-habitat, as assumed in classical theoretical models\\(^{20,21}\\), has been strongly criticized\\(^{18,22–24}\\). This characterization has progressively been relaxed with approaches based on the premise that the matrix should in fact be treated as a heterogeneous mosaic of different land covers (e.g. ‘countryside biogeography’\\(^{25}\\), and the ‘land-sharing’ and ‘land-sparing’ approaches\\(^{26–30}\\)), as it is recognized that species use different matrices for foraging, dispersing, and reproduction purposes\\(^{31,32}\\). While high-contrast matrices (e.g. intensive agricultural or built environments) act as movement barriers or ecological traps for many species, with an elevated risk of mortality\\(^{33}\\), low-contrast matrices (e.g. secondary forests or shade-grown low-intensive agriculture in forested regions) may act as permeable barriers with a reduced risk of mortality, even for those species typically considered habitat specialists\\(^{25,27}\\). To date, however, conservation and management assessments across different scales have focused mainly on species’ primary habitat\\(^{34,35}\\), thus limiting our understanding of their response to the matrix, which may have direct implications for the design of functional landscapes\\(^{36}\\) and the prioritization of different conservation actions in fragmented landscapes\\(^{37}\\).\nComparative extinction risk modelling is an approach for assessing the drivers of extinction risk and its change over time, based on the relationship between species’ life histories, the pressure within species geographic ranges, and their threat status^{38-43}. Built with readily available data, this approach allows for the prediction of the risk of extinction of a larger number of species compared with that provided by expert-based assessments. This more rapid approach can substantially reduce resource requirements, as well as proactively inform conservation and management strategies^{44,45}. Although the loss^{3,43} and fragmentation^{46,47} of habitat are among the main determinants of species extinction risk, the influence of the matrix condition on the effects of fragmentation and its relationship with species extinction risk has not been well evaluated for any animal taxon at a global scale.\n\nHere, we quantify the relationship between changes in the extinction risk of 4,327 terrestrial mammals over a 24-year period (1996-2020), the degree of fragmentation of their suitable habitat, and the levels of human pressure within the associated habitat matrix. Our goal is to test the influence of human pressure within the matrix on the effects of fragmentation for determining changes in species extinction risk globally. We focus on terrestrial mammals as they have been used as a focal taxon in previous extinction risk analyses^{48}, they are known to be sensitive to fragmentation^{46}, and data are available to delineate levels of suitable habitat and ‘unsuitable’ (i.e. matrix) habitat within their ranges^{49}. For each species, we quantify the degree of fragmentation as the average Euclidean distance within patches of suitable habitat from the nearest patch edge, and matrix condition as the extent and change over time of high human pressure levels overlapping with the surrounding matrix. Spatial data representing the condition of the matrix were obtained from the most comprehensive global maps of changing human\npressure on the environment\\(^{50}\\), the recently updated human footprint maps\\(^{51}\\), which provide a single metric that combines data on human activities, all of which are driving the current biodiversity crisis\\(^3\\). We define a human footprint threshold of \\( \\geq 3 \\) out of 50 to represent the extent of human-modified habitat within the matrix. This threshold was used as it has shown to be the strongest predictor of transitions in extinction risk for terrestrial mammals\\(^{43}\\). Furthermore, this human footprint threshold is associated with the highest declines in mammalian movements\\(^{52}\\) and chimpanzee behavioral diversity\\(^{53}\\). Following previous studies\\(^{42,43,54}\\), we classify species into two groups of extinction risk, low-risk transitions and high-risk transitions (Fig. 1), based on the initial and final Red List category registered between 1996 and 2020. In combination with other predictors of extinction risk (see Table 2 for a description), we quantify the relative predictive importance of habitat fragmentation and the condition of the matrix for determining extinction risk transitions in terrestrial mammals.\n\nOur analyses reveal that the condition of the matrix plays a major role on the effects of fragmentation for predicting extinction risk transitions in terrestrial mammals. Our results suggest that the negative effects of habitat fragmentation may be somewhat mitigated when the matrix is associated with lower levels of human pressure.\n\nResults\n\nChanges in species extinction risk\n\nWhen classifying extinction risk transitions with the initial and final Red List categories registered between 1996 and 2020, we found that 2,907 (67.2%) species faced a low-risk transition and 1,420 (32.8%) a high-risk transition (Fig. 1). The proportions of low-risk and high-\nrisk transitions were almost unchanged when applying a different classification routine (Supplementary Fig. 1; Supplementary Note 1).\n\n![Classification of species extinction risk transitions based on past and present IUCN Red List categories. a Represents low-risk transitions, which included species that retained a category of least concern, together with those species that moved from any higher category of threat to a lower category between 1996 and 2020. b Represents high-risk transitions, which included all species that retained a category of threatened or near threatened, together with those species that moved from any lower category of threat to a higher category between 1996 and 2020. *Acronyms refer to the IUCN Red List categories, including Least Concern (LC), Near Threatened (NT), Vulnerable (VU), Endangered (EN), and Critically Endangered (CR) (figure adapted from Di Marco et al.43).](page_256_370_1087_312.png)\n\nFigure 1. Classification of species extinction risk transitions based on past and present IUCN Red List categories*. a Represents low-risk transitions, which included species that retained a category of least concern, together with those species that moved from any higher category of threat to a lower category between 1996 and 2020. b Represents high-risk transitions, which included all species that retained a category of threatened or near threatened, together with those species that moved from any lower category of threat to a higher category between 1996 and 2020. *Acronyms refer to the IUCN Red List categories, including Least Concern (LC), Near Threatened (NT), Vulnerable (VU), Endangered (EN), and Critically Endangered (CR) (figure adapted from Di Marco et al.43).\n\nPredicting transitions in species extinction risk\n\nUsing a Random Forest model for classification55, we measured the performance of an array of life-history, environmental and pressure variables for the prediction of extinction risk transitions (see Table 2 for a description). We found that the extent of high human footprint values in the\nmatrix and the degree of fragmentation of suitable habitat had higher predictive performance than life-history traits and other pressure and environmental variables (Fig. 2). When employing a different classification routine of extinction risk transitions (i.e. when transitions were classified using the second last and last Red List category instead of the initial and final Red List categories between 1996 and 2020), these two variables remained as the most important predictors of extinction risk (Supplementary Fig. 2a), suggesting that these results are robust to changes in species threat status.\n\n![Bar chart showing variable importance for selected variables in predicting extinction risk transitions in terrestrial mammals, color-coded by Life-history, Environment, and Pressure](page_484_573_1017_312.png)\n\nFig. 2. Relative importance of selected variables for the prediction of extinction risk transitions in terrestrial mammals. Variables are colour-coded according to their broad class (life-history, environment, and human pressure). The description of each variable can be found in Table 2. High levels of the human footprint (HFP) included values of 3 or above.\n\nInterestingly, our results show that the degree of fragmentation of suitable habitat had higher predictive performance than the change in high human footprint values (as defined by increases in high human footprint values through time) within suitable habitat and the proportion of\nsuitable habitat (Fig. 2). This result is supported by a sensitivity analysis where a different classification routine of extinction risk transitions and a different combination of the levels of habitat suitability were applied (Supplementary Fig. 2a and 2b). This suggests that habitat fragmentation better predicts changes in species extinction risk than habitat loss and habitat amount at a global scale.\n\nOur results also show that the predictive importance of the change in high human footprint values within the extent of suitable habitat is greater than that within the extent of the matrix (Fig. 2). This result was confirmed when employing a different classification routine of extinction risk transitions and a different combination of the levels of habitat suitability (Supplementary Fig. 2a and 2b), highlighting the key influence of the extent and change over time of high human pressure levels within species’ ranges43.\n\nWhen looking at the interaction between the degree of fragmentation of suitable habitat and the condition of the matrix on the probability of changes in species extinction risk (Fig. 3), we found that the probability of high-risk transitions increased with an increasing degree of habitat fragmentation and an increasing extent of high human pressure levels within the matrix. This trend was reversed to an increased probability of low-risk transitions.\nFig. 3. Interaction of the degree of habitat fragmentation with the matrix condition on extinction risk transitions in terrestrial mammals. The plot represents the positive interaction between the degree of fragmentation of suitable habitat and the matrix condition for high-risk transition. The interaction between the degree of fragmentation of suitable habitat and the matrix condition for low-risk species is represented when the plot is inverted. The fragmentation metric was inverse-coded so high values represent high degree of fragmentation. The extent of high human footprint values in the matrix was arcsine square-root-transformed to avoid variance instability when handling proportions close to zero. The description of each variable is given in Table 2. High levels of the human footprint (HFP) included values of 3 or above.\n\nOur model showed good overall classification ability during cross-validation, with 82% of species correctly classified. The accuracy in predicting high-risk transitions (sensitivity = 61.7%) was lower than the accuracy in predicting low-risk transitions (specificity = 84.4%), with a true skill statistic of 0.5.\n\nThe predictive performance of our model did not markedly change compared to the models built based on a different classification routine of extinction risk transitions and a different\ncombination of the levels of habitat suitability (Supplementary Table 1). Thus, the model is robust to changes in species threat status and in the levels of habitat suitability.\n\nThe influence of the matrix condition on the importance of habitat fragmentation for predicting extinction risk transitions\n\nIn order to measure the influence of the matrix on the importance of fragmentation for the prediction of extinction risk transitions, we first discretized the extent of high human footprint values within the matrix into two broad levels as a proxy for matrix quality: 'low-quality matrix', representing species with \\( \\geq 50\\% \\) of the extent of their matrix overlapping with high human footprint values (\\( n = 2,529 \\) low-risk species and 1,250 high-risk species); and ‘high-quality matrix’, representing species with \\( < 50\\% \\) of the extent of their matrix overlapping with high human footprint values (\\( n = 341 \\) low-risk species and 111 high-risk species). We then built separate Random Forest models for each level of quality of the matrix in order to compare the predictive performance of the degree of fragmentation of suitable habitat between the defined levels of quality of the matrix. We found that the degree of fragmentation had a higher relative predictive performance for species with low-quality matrix (Fig. 4a) than that observed for species with low-quality matrix (Fig. 4b), with a decrease of 30.1%. Notably, the relative predictive importance of the extent of high human footprint values in the matrix was markedly higher for the low-quality matrix model compared with the high-quality matrix model, suggesting that the lower the quality of the matrix, the higher the predictive importance of the matrix.\nFig. 4. Influence of the matrix condition on the relative importance of selected variables for the prediction of extinction risk transitions in terrestrial mammals. a Shows the relative importance of each predictor with low-quality matrix, which included species with proportions \\( \\geq 50\\% \\) of the extent of their matrix overlapping with high human footprint values (\\( n = 2,529 \\) low-risk species and 1,250 high-risk species). b Shows the relative importance of each predictor with high-quality matrix, which included species with proportions < 50% of the extent of their matrix overlapping with high human footprint values (\\( n = 341 \\) low-risk species and 111 high-risk species). Variables are colour-coded according to their broad class (life-history, environment, and\nhuman pressure). The description of each variable is given in Table 2. High levels of the human footprint (HFP) included values of 3 or above.\n\nWhen looking at the difference in the degree of fragmentation for low-risk and high-risk species, we found that those classified as high-risk had higher degrees of fragmentation, with a difference that was significant for each of the levels of quality of the matrix (\\( p \\)-values < 0.001; Wilcoxon signed rank test, one-sided). When it comes to the effect size of the degree of fragmentation between low-risk and high-risk species, we found that such an effect was slightly lower for those species with matrices of high-quality habitat (Cohen’s d = 0.15; Supplementary Fig. 3a) compared to those with matrices of low-quality habitat (Cohen’s d = 0.16; Supplementary Fig. 3b).\n\nOur results show that the model for species with matrices of low-quality habitat had higher predictive performance than the model for species with matrices of high-quality habitat (Table 1). However, it is important to note that this result is related to the fact that the latter showed a larger imbalance between low-risk and high-risk species than that showed by the former.\n\nTable 1. Cross-validation results of the Random Forest models for the prediction of extinction risk transitions in terrestrial mammals with low- and high-quality matrix. The cross-validation was performed in terms of proportion of correctly classified species (accuracy), proportion of correctly classified high-risk species (sensitivity), proportion of correctly classified low-risk species (specificity), and the true skill statistic (TSS = sensitivity + specificity – 1).\n\nLow-quality matrix included species with proportions \\( \\geq 50\\% \\) of the extent of their matrix\noverlapping with high human footprint values (\\( n = 2,529 \\) low-risk species and \\( 1,250 \\) high-risk species). High-quality matrix included species with proportions < 50% of the extent of their matrix overlapping with high human footprint values (\\( n = 341 \\) low-risk species and \\( 111 \\) high-risk species). High human footprint included values of 3 or above.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
ModelAccuracy (%)Sensitivity (%)Specificity (%)TSS
Extinction risk transitions ~ Low-quality matrix81.562.884.10.5
Extinction risk transitions ~ High-quality matrix81.734.883.70.2
\n\nDiscussion\n\nUnderstanding the external conditions under which a species is likely to face an increased risk of extinction are necessary to inform conservation policies and management strategies\\(^{42}\\). We found that the condition of the matrix, as defined by the extent of high human footprint values between patches of suitable habitat, strongly influenced the effects of fragmentation on extinction risk transitions of terrestrial mammals. Specifically, we found that when predicting changes in the risk of extinction of terrestrial mammals, matrices of high-quality habitat decreased the relative predictive importance of the degree of habitat fragmentation by ~30% compared with low-quality matrices. To the best of our knowledge, this finding is the first to demonstrate consistently whether and how much human pressure within the matrix alters the importance of habitat fragmentation as a predictor of extinction risk change. This finding is consistent with previous studies showing that the use of the matrix is among the main determinants of the\nvulnerability of mammalian populations to local extinction in fragmented landscapes^{25,56,57}, and supports recent findings demonstrating that species living in forested landscapes with a low-quality matrix (in terms of plant biomass) are more vulnerable to extinction than those living in forested landscapes with a higher quality matrix^{58}.\n\nOur results showed that species with greater fragmentation and lower quality matrix within their ranges tended to be at greater risk of extinction. As reported by others^{48}, this might indicate that species at a lower risk of extinction are able to exploit a greater number of habitats and resources compared to species in the high-risk group. This result might be related to the fact that species occurring in regions with low rates of historical disturbance are more likely to be sensitive to fragmentation^{15}, and thus more likely to face an increased risk of extinction. That would suggest that those species within the high-risk group are mainly concentrated in the tropics, particularly in forested landscapes, where deforestation continues at a rapid rate^{59,60}. In fact, ~33%, ~34%, and ~45% of all species restricted to the Neotropical, Afrotropical, and Indo-Malay biogeographic realms, respectively, were facing an increased risk of extinction between 1996 and 2020, which is consistent with these findings.\n\nIn our extinction risk model, some variables had higher predictive performance than others. For example, the extent of high human footprint values in the matrix was the most important predictor of changes in species extinction risk. This result contrasts with the findings from previous extinction risk modelling exercises for mammals, where the predictive importance of human pressure was found to be lower than life-history traits or environmental conditions^{48,61,62}. However, it helps confirms the findings of one recent extinction risk modelling exercise for\nmammals\\(^{43}\\), where the extent of high human footprint values within species’ ranges had higher predictive importance than environmental conditions, life-history traits, and other measures of human pressure. This result may, in part, be explained by the fact that species are increasingly exposed to anthropogenic land covers\\(^{63,64}\\), especially in the matrix where higher contrast (i.e. lower quality habitat) likely prevents their movement\\(^{52}\\) and elevates their mortality\\(^{33}\\) (e.g. by roadkill\\(^{65}\\) or increasing predation by feral animals\\(^{66}\\)).\n\nThe degree of fragmentation of suitable habitat was also found to be a key correlate of change in extinction risk. This finding is in line with previous extinction risk modelling showing that the inclusion of habitat fragmentation as a predictor increases the explanatory power of the models\\(^{46,47}\\). In particular, this result supports previous findings showing that terrestrial mammals with higher fragmentation have smaller ranges, lower proportions of suitable habitat and are at greater risk of extinction\\(^{46}\\).\n\nConflicting results on the effects of fragmentation *per se* on biodiversity have arisen from studies attempting to separate ‘independent’ effects of habitat loss from those of habitat fragmentation\\(^{11}\\). Some studies have argued that the effects of habitat loss are greater and more negative (e.g.\\(^{6,8,9,12}\\)), while others have demonstrated that the effects due to fragmentation, such as declining patch size, increasing habitat isolation, and increasing edge effects, are essentially negative and lasting (e.g.\\(^{5,7,13,14}\\)). However, in real landscapes, habitat loss inevitably causes habitat fragmentation, and both act in synergy with other threats to biodiversity\\(^{67,68}\\). Thus, there is little practical value in attempting to separate the effects of habitat loss and fragmentation\\(^{7,69–71}\\). Our study does not attempt to resolve the current debate as to whether and how habitat\nfragmentation per se (i.e. the spatial arrangement of remaining habitat for a given amount of habitat loss) influences biodiversity\\(^{5-10}\\), but the results showed that the degree of fragmentation of suitable habitat was more important than the change in high human footprint values (as represented by increases in high human pressure levels over time) within suitable habitat and the proportion of suitable habitat. This suggests that changes in species extinction risk are primarily determined by the fragmentation of habitat, and secondarily by the loss and the amount of habitat within species’ ranges. However, there is also the possibility that the loss of most suitable habitat patches had already occurred before the beginning of the study period, resulting in fragmentation being a more important predictor of extinction risk than habitat loss and habitat amount.\n\nOur models were better at correctly classifying low-risk transitions than high-risk transitions. This suggests that the external conditions leading to a high-risk transition might be more difficult to identify than those leading to a low-risk transition, as also indicated in previous studies\\(^{41-43,62,72}\\). However, it is important to acknowledge that the exclusion of other variables associated with pressure (such as overhunting, disease, invasive species, and climate change) and life-history traits (such as rarity, dispersal mode, and ranging behavior) could have increased the uncertainty of our predictions, and thus influenced the ability of our models to correctly classify high-risk transitions.\n\nOur modelling framework can be used to proactively inform conservation and management strategies seeking to minimize the number of species that are facing or will face an increased risk of extinction. This includes species that are currently classified as threatened and those that are likely to become so if human activities continue to expand and intensify into the future. An\nimportant next step will be to create a global map that captures the matrix condition for the world’s terrestrial mammals. This will require weighting the extent of the matrix of all terrestrial mammals with the human footprint as a proxy for matrix quality within species’ geographic distributions. If species threat statuses are considered, this could have the potential to identify where conservation actions are needed to be improved. For example, in those locations where species with an increased risk of extinction show a low-quality habitat within their matrix, a land-sparing approach could be effective as it maximizes conservation actions on the remaining patches of suitable habitat while concentrating agriculture production elsewhere\\(^{26,28-30}\\).\n\nAlternatively, in those locations where species with an increased risk of extinction show a high-quality habitat within their matrix, a land-sharing approach would work better as it minimizes the impact of agriculture production by maintaining or restoring the conservation value of the land already farmed\\(^{27-30}\\).\n\nOur results indicate that species suffering from greater pressure in their matrix require particular conservation attention. Among these species, those with smaller ranges require careful management of the areas surrounding their suitable habitat, especially in light of the current and future effects of climate and land-use change\\(^{73}\\). Our results also highlight the potential of high-quality matrices to mitigate the effects of fragmentation on species extinction risk, thus suggesting that in addition to efforts to maintain remaining suitable habitat\\(^{32,35,74}\\), there is a need for restoration of habitats in the matrix.\nMethods\n\nHabitat suitability models\n\nWe used habitat suitability models developed by Rondinini et al.49 to represent the extent of suitable habitat patches and the extent of the matrix of 4,327 out of 5,722 extant terrestrial mammals, corresponding to 76% of all species in the group75. These models were built for the year 2000 at a spatial resolution of 300 m, based on species’ elevation range and other habitat affinities, including preferred land cover types and relationship to water bodies. Data for each species were extracted from the International Union for Conservation of Nature (IUCN) datasets, and using expert information combined with spatial data on habitat variables. The models include three levels of habitat suitability: (i) high, representing primary habitat or preferred habitat where the species can persist; (ii) medium, representing secondary habitat where the species can occur but not persist without nearby high suitable habitat; and (iii) ‘unsuitable’, representing locations where the species is expected to occasionally or never be found.\n\nWhen delineating the levels of habitat suitability for each species, small contiguous groups of pixels ( < 4 adjacent pixels of the same level of habitat suitability) were removed and replaced with the pixel value of the largest neighbor of the contiguous groups of pixels, setting eight neighboring pixels. This reduced the influence of isolated groups of pixels of the same level of habitat suitability, and improved the computational efficiency of the analysis, as also reported in other studies46,76.\n\nIn this analysis, we combined high and medium habitat suitability to represent the extent of suitable habitat patches, and use the level of ‘unsuitable’ habitat to represent the extent of the\nmatrix of each species. We also applied a different combination of the levels of habitat suitability when representing the extent of suitable habitat patches (high suitability instead of high and medium suitability combined) and the extent of the matrix (medium suitability and ‘unsuitable’ combined instead of ‘unsuitable’ habitat) of each species.\n\nHabitat fragmentation as a predictor of extinction risk transitions\n\nFor each species, we measured the degree of habitat fragmentation by quantifying the average Euclidean distance of all the pixels within patches of suitable habitat from the nearest patch edge\\(^{77}\\). Large values of the average Euclidean distance represented low degrees of habitat fragmentation, whereas small values represented high degrees of habitat fragmentation.\n\nAdditionally, we calculated the average Euclidean distance between patches of suitable habitat through the surrounding matrix (i.e., the average Euclidean distance of all the pixels within ‘unsuitable’ habitat from the nearest edge) to account for patch isolation (after\\(^{46}\\)). Here, large values of the average Euclidean distance represented low degrees of patch isolation, and small values represented high degrees of patch isolation. The average Euclidean distance was considered because this metric does not require a predetermined distance threshold of what constitutes an edge, accounts for different shapes of fragments and landscapes patterns and arrangements, accounts for the distribution of habitat area\\(^{78}\\), is comparable across landscapes of different extents, and provides stable and readily interpretable information\\(^{76}\\). Moreover, average Euclidean distance has been shown to be singularly valuable in quantifying the relationship between habitat fragmentation and extinction risk of the world’s terrestrial mammals\\(^{46}\\), which made it highly suitable for our analyses.\nThe matrix condition as a predictor of extinction risk transitions\n\nSpatially explicit data on the condition of the matrix, as represented by the extent and change over time of high human pressure levels overlapping with the area of ‘unsuitable’ habitat surrounding patches of suitable habitat (after43), was obtained from the recently updated global human footprint maps51. These maps represent the most comprehensive global distribution of changing human pressure on the environment at 1 km resolution between 2000 and 2013, based on eight pressure layers50: (i) built environments; (ii) intensive agriculture; (iii) pasture land; (iv) human population density; (v) night-time lights; (vi) roads; (vii) railways; and (viii) navigable waterways, all of which are driving the current extinction crisis3. Each human footprint map provides a single pressure metric ranging from 0 to 50, where a value of 0 represents areas free of any human influence (e.g., terrestrial remaining wilderness), values of 4 or below represent areas of low human pressure (e.g., pasture lands), and values above 20 represent areas with very high pressure levels (e.g., densely populated semi-urban and urban environments).\n\nIn this analysis, we measured the current extent of high human footprint values and their change over time (between 2000 and 2013) in areas of ‘unsuitable’ habitat, using a defined human footprint threshold of 3 or above. This threshold was used as it is the strongest predictor of extinction risk transitions in terrestrial mammals43, and is associated with the highest declines in mammalian movements52 and chimpanzee behavioral diversity53. Based on previous studies43,79, we considered high human footprint values as the extent and change over time of high pressure levels within species’ ranges have shown to be more sensitive to predict extinction risk than using mean pressure levels. We also considered the changes in the extent of high human footprint values after discarding areas where the human footprint was lower in 2013 than in 2000\n(assuming no change in these particular areas), as decreases in human pressure levels are likely to take time before having a measurable effect on species threat status, particularly for species with a long generation time period43.\n\nChanges in species extinction risk\n\nWe used the IUCN Red List of Threatened Species75,80, the retrospective Red List Assessments published in Hoffman et al.54, and the IUCN list of genuine changes in the conservation status of mammal species (https://www.iucnredlist.org/resources/summary-statistics) to represent trends in extinction risk of terrestrial mammals. Following the classification of extinction risk transitions developed by Di Marco et al.42,43, we classified the species into two main groups, low-risk transitions and high-risk transitions (Fig. 1). The low-risk group includes species that retain a category of least concern, together with those species that move from any higher category of threat to a lower category assessment period. The high-risk group includes all species that retain a category of threatened or near threatened, together with those species that move from any lower category of threat to a higher category over time.\n\nIn this analysis, we classified species into the two extinction risk groups (low-risk transitions and high-risk transitions) based on the initial and final Red List category registered between 1996 and 2020. In order to test the sensitivity of this classification, we also classified all species into the two extinction risk groups based on the last two Red List assessments registered between 1996 and 2020 (i.e. the second last and last Red List categories registered between 1996 and 2020). We excluded species without a defined threat status (Data Deficient), and those already extinct at the beginning of the study period.\nPredicting extinction risk transitions\n\nWe used a multivariate Random Forest model to predict extinction risk transitions of terrestrial mammals (Fig. 1). Random Forest is a non-parametric, tree based, machine-learning technique that produces multiple decision tress using a randomly selected subset of training samples and variables to make a prediction\\(^{55,81}\\). Due to its limited assumptions on data distributions, its high classification stability and performance, and its ability to cope well with a large number of potentially correlated predictors and non-linear responses, Random Forest is a highly suitable technique for species threat status classification\\(^{62}\\). Furthermore, Random Forest modelling has shown to have the highest performance among several machine learning techniques tested for the prediction of global extinction risk of terrestrial mammals\\(^{72}\\).\n\nIn combination with previously identified variables (Table 2), predictors included the degree of fragmentation of suitable habitat and the extent and change over time of high human footprint values in the matrix within species’ ranges. Because mammals of greater body size usually move farther\\(^{82}\\), and diet may influence their movements as a result of differences in availability of resource types and foraging cost\\(^{83,84}\\), we decided to include body size and dietary breadth as life-history predictors. We also included the reproductive traits weaning age and the gestation length. Other life-history traits were broadly captured by representing taxonomic orders of each species. To avoid potential circularity in the estimation of changes in extinction risk, we did not include species’ range size as a predictor\\(^{38}\\).\nTable 2. Description of the selected variables to predict extinction risk transitions in terrestrial mammals.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
ClassVariableDescriptionSource
PressureHigh human footprint extent in the matrixProportion of the area of ‘unsuitable’ habitat overlapping with high human footprint values in 2000.49,51
High human footprint extent in patches of suitable habitatProportion of suitable habitat overlapping with high human footprint values in 2000.49,51
High human footprint change in the matrixDifference in the proportion overlap between the area of ‘unsuitable’ habitat and high human footprint values during 2000 and 2013.49,51
High human footprint change in patches of suitable habitatDifference in the proportion overlap between the area of suitable habitat and high human footprint values during 2000 and 2013.49,51
EnvironmentHabitat fragmentationAverage Euclidean distance within patches of suitable habitat from the nearest patch edge.49,77
\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Patch isolationAverage Euclidean distance within the area of ‘unsuitable’ habitat from the nearest edge.After46
Proportion of suitable habitatProportion of suitable habitat within species’ ranges.49
RealmBiogeographic realm.75,80
Life-historyBody massA generic proxy of species life history and energetic requirements.85–89
DietDietary categories: vertebrate carnivore ( > 90% vertebrate matter ingested), invertebrate carnivore ( > 90% invertebrate matter ingested), omnivore (10-90% animal matter ingested or 10-90% plant matter ingested), herbivore ( > 90% plant matter ingested).89–91
Weaning ageA proxy of species reproductive timing.86,87
Gestation lengthA proxy of species reproductive output.86,87
OrderSpecies taxonomic order.80
\nWe measured the predictive importance of each variable using the Actual Impurity Reduction Importance metric\\(^{92}\\). This metric is unbiased with regard to the number of categories in the variables, and it computes reliable importance estimates without the extra computing cost of permutations. We then calculated the relative predictive importance of each variable using the model improvement ratio (MIR) metric\\(^{93}\\). Unlike the raw importance scores, the MIR metric is comparable among models. MIR is calculated as \\([I_n/I_{max}]\\), where \\(I_n\\) is the importance of a given variable, and \\(I_{max}\\) is the maximum model improvement score. We reported the overall performance of the Random Forest model through cross-validation in terms of proportion of correctly classified species, proportion of correctly classified high-risk species (sensitivity), proportion of correctly classified low-risk species (specificity), and the true skill statistic (TSS = sensitivity + specificity – 1)\\(^{94}\\).\n\n**Assessing the influence of the matrix on the importance of fragmentation for predicting extinction risk transitions**\n\nTo measure the influence of the matrix on the importance of fragmentation for the prediction of extinction risk transitions, we first defined two broad levels of quality of the matrix (low and high), and then built separate Random Forest models for species restricted to such levels based on the proportion of high human footprint values in the matrix of each species. When defining the two levels of quality of the matrix, the extent of high human footprint values in the matrix of each species was discretized into two intervals using an equal width discretization method. Using the Actual Impurity Reduction Importance metric\\(^{92}\\) and the MIR metric\\(^{93}\\), we measured the relative predictive performance of fragmentation, including the other selected variables (Table 2), from the built Random Forest models. We used cross-validated measures of sensitivity,\nspecificity, and the true skill statistic to evaluate the overall performance of the models94. We also used Wilcoxon rank sum tests to test for statistical differences in the degree of fragmentation between low-risk and high-risk species restricted to the defined levels of quality of the matrix. To determine the effect size of the degree of habitat fragmentation between low-risk and high-risk species for each of the levels of quality of the matrix, we used Cohen’s d statistic95.\n\nSensitivity testing\n\nTo test the sensitivity of our model, we built additional Random Forest models based on the last two Red List assessments registered between 1996 and 2020 (i.e. the second last and last Red List categories registered during this period), and a different combination of the levels of habitat suitability to represent the extent of suitable habitat patches (high suitability instead of high and medium suitability combined) and the extent of the matrix (medium suitability and ‘unsuitable’ combined instead of ‘unsuitable’ habitat). From these models, the relative importance of each variable was quantified using the Actual Impurity Reduction Importance metric92 and the MIR metric93. The overall performance of these models was reported through cross-validation in terms of sensitivity, specificity, and the true skill statistic94.\n\nAll spatial analyses were performed in python using the ArcPy processing module from ArcGIS Pro 2.5.096. Statistical analyses were performed in R97, using the packages ‘randomforest’98, ‘caret’99, ‘ranger’100, ‘plotmo’101, and ‘effsize’102.\nData availability\n\nThe Human Footprint dataset used in this study is available for download at https://doi.org/10.5061/dryad.3tx95x6d9. Habitat suitability models for the world’s terrestrial mammals are available upon request from the model developers (see https://globalmammal.org/habitat-suitability-models-for-terrestrial-mammals/). The raw data on extinction risk categories is available in R97, using the package ‘rredlist’103. 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R package version 0.5.0, https://CRAN.R-project.org/package=rredlist (2018).\nAcknowledgements\n\nWe thank Michelle Venter, Kristen Kieta and Rajeev Pillay for comments on earlier drafts of this manuscript.\n\nAuthor contributions\n\nJ.P.R.-D. and O.V. conceived the study; J.P.R.-D. collected and analyzed all the data under advice of O.V., M.D., C.R., X.C.Ll., and M.A.; J.P.R.-D. led the writing of the manuscript with input from O.V., M.D., C.J.J., and C.R.\n\nAdditional information\n\nSupplementary information accompanies this paper as a separate file.\n\nCompeting interest: The authors declare not competing interest.\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• RamirezDelgadoetal2021Supplementaryinformationjp.pdf"} {"paper_id": "prb43", "title": "Federated Learning Enables Big Data for Rare Cancer Boundary Detection", "text": "Federated Learning Enables Big Data for Rare Cancer Boundary Detection\n\nSarthak Pati1,2,3,4,*●, Ujjwal Baid1,2,3,*●, Brandon Edwards5,*●, Micah Sheller5,*●, Shih-Han Wang5,*●, G Anthony Reina5,*●, Patrick Foley5,*●, Alexey Gruzdev5,*●, Deepthi Karkada5,*●, Christos Davatzikos1,2,*●, Chiharu Sako1,2,*●, Satyam Ghodasara2,*●, Michel Bilello1,2,*●, Suyash Mohan1,2,*●, Philipp Vollmuth7,*●, Gianluca Brugnara7,*●, Chandrakanth J Preetha7, Felix Sahm8,9, Klaus Maier-Hein10,143,*●, Maximilian Zenk10, Martin Bendszus7, Wolfgang Wick8,11,*●, Evan Calabrese12,*●, Jeffrey Rudie12,*●, Javier Villanueva-Meyer12,*●, Soomnee Cha12,*●, Madhura Ingalkhalikar13,*●, Manali JadHAV13,*●, Umang Pandey13,*●, Jitender Saini14,*●, John Garrett15,16, Matthew Larson15, Robert Jera15,16, Stuart Currie18, Russell Frood18, Kavi Fatania18, Raymond Y Huang19,*●, Ken Chang20,*●, Carmen Balana Quintero21, Jaume Capellades22, Josep Puig23, Johannes Trenkler24,*●, Josef Pichler25, Georg Necker24, Andreas Haunschmidt24, Stephan Meckel24,147,*●, Gaurav Shukla1,26, Spencer Liem27, Gregory S Alexander28, Joseph Lombardo27,29, Joshua D Palmer30, Adam E Flanders31, Adam P Dicker29, Haris I Sair32,33,*●, Craig K Jones33,*●, Archana Venkataraman34,*●, Meirui Jiang35,*●, Tiffany Y So35,*●, Cheng Chen35,*●, Pheng Ann Heng35,*●, Qi Dou35,*●, Michal Kozubek36,*●, Filip Lux36,*●, Jan Michálek36,*●, Petr Matula36,*●, Milos Kerkovsky37,*●, Tereza Kopřivová37,*●, Marek Dostál37,38,*●, Václav Vybíral39,*●, Michael A Vogelbaum40,*●, J Ross Mitchell87,88,*●, Joaquim Farinas42,*●, Joseph A Maldjian43, Chandan Ganesh Bangalore Yogananda43, Marco C Pinho43,*●, Divya Reddy43, James Holcomb43, Benjamin C Wagner43, Benjamin M Ellingson44,45,*●, Timothy F Cloughesy45,*●, Catalina Raymond44,*●, Talha Oughourlian44,46,*●, Akifumi 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Morón73,*●, Jacob Mandel74,*●, Konstantinos Kamnitsas74,75,*●, Ben Glocker74,*●, Luke V M Dixon76,*●, Matthew Williams77,*●, Peter Zampakias78,*●, Vasileios Panagiotopoulos79,*●, Panagiotis Tsiganas80,*●, Sotiris Alexiou81,*●, Ilias Haliasos82,*●, Evangelia I Zacharaki81,*●, Konstantinos Moustakas81,*●, Christina Kalogeropoulou81,*●, Dimitrios M Kardamakis150,*●, Yoon Seong Choi83,*●, Seung-Koo Lee83,*●, Jong Hee Chang83,*●, Sung Soo Ahn83,*●, Bing Luo84,*●, Laila Poisson85,*●, Ning Wen84,148,*●, Pallavi Tiwari86,*●, Ruchika Verma86,88,*●, Rohan Bareja86,*●, Ipsa Yadav86,*●, Jonathan Chen86,*●, Neeraj Kumar87,88,*●, Marion Smits89,*●, Sebastian R van der Voort89,*●, Ahmed Alafandi89,*●, Fatih Incekara89,90,*●, Maarten MJ Wijnenga91,*●, Georgios Kapsas89,*●, Renske Gahrmann89,*●, Joost W Schouten90,*●, Hendrikus J Dubbink93,*●, Arnaud JPE Vincent90,*●, Martin J van den Bent91,*●, Pim J French91,*●, Stefan Klein94,*●, Yading Yuan95,*●, Sonam Sharma95,*●, Tzu-Chi Tseng95,*●, Saba Adabi95,*●, Simone P Niclou96,*●, Olivier Keumen97,*●, Ann-Christin Hau96,98,*●, Martin Vallières99,145,*●, David Fortin100,145,*●, Martin Lepage101,145,*●, Bennett Landman102,*●, Karthik Ramadas102,*●, Kaiwen Xu103,*●, Silky Chotal104,*●, Lola B Chambless104,*●, Akshikumar Mistry104,*●, Reid C Thompson104,*●, Yuriy Gusev105,*●, Krithika Bhuvaneswara105,*●, Anousheh Sayah106,*●, Camelia Benchegroun105,*●, Anas Belouali105,*●, Subha Madhavan105,*●, Thomas C Booth107,108,*●, Alysha Chealliah107,*●, Marc Modat107,*●, Haris Shuaib109,110,*●, Carmen Dragos109,*●, Aly Abayazed111,*●, Kenneth Kolodziej111,*●, Michael Hill111,*●, Ahmed Abbassy112,*●, Shady Gamal112,*●, Mahmoud Mekhaimar112,*●, Mohamed Qayati112,*●, Mauricio Reyes113,*●, Ji Eun Park114,*●, Jihye Yun114,*●, Ho Sung Kim114,*●, Abhishek Mahajan115,*●, Mark Muzi116,*●, Sean Benson117,*●, Regina G H Beets-Tan152,153,*●, Jonas Teuwen117,*●, Alejandro Herrera-Trujillo118,119,*●, Maria Trujillo119,*●, William Escobar118,119,*●, Ana Abello119,*●, Jose Bernal119,120,*●, Jhon Gómez119,*●, Joseph Choi121,*●, Stephen Baek122,*●, Yusung Kim123,*●, Heba Ismael123,*●, Bryan Allen123,*●, John M Buatti123,*●, Aikaterini Kotrotsou126,*●, Hongwei Li6,*●, Tobias Weiss41,*●, Michael Weller41,*●, Andrea Bink17,*●, Bertrand Pouymayou17,*●, Hassan F Shaykh127,*●, Joel Saltz128,*●, Prateek Prasanna128,*●, Sampurna Shrestha128,*●, Kartik M Mami128,141,*●, David Payne142,*●, Tahnis Kurc128,129,*●, Enrique Pelaez130,*●, Heydy Franco-Maldonado144,*●, Francis Loayza130,*●, Sebastian Quevedo131,*●, Pamela Guevara132,*●, Esteban Torche132,*●, Cristobal Mendoza132,*●, Franco Vera132,*●, Elvis Rios132,*●, Eduardo López132,*●, Sergio A Velastin133,*●, Godwin Ogbole134,*●, Dotun Oyekunle134,*●, Olubunmi Odafe-Oyibotha135,*●, Babatunde Osobo134,*●, Mustapha Shu’aibu136,*●, Adeleye Dorcas137,*●, Mayowa Soneye134,*●, Farouk Dako2,124,*●, Amber L Simpson110,138,*●, Mohammad Hamghalam138,149,*●, Jacob J Peoples138,*●, Ricky Hu138,*●, Anh Tran138,*●, Danielle Cutler146,*●, Fabio Y Moraes151,*●, Michael A Boss139,*●, James Gimpel139,*●, Deepak Kattil Veettil139,*●\nKendall Schmidt92, Brian Bialecki92, Sailaja Marella139, Cynthia Price139, Lisa Cimino139, Charles Apgar139, Prashant Shah5, Bjoern Menze4,6, Jill S Barnholtz-Sloan68,140, Jason Martin5, and Spyridon Bakas1,2,3,8\n\n1 Center for Biomedical Image Computing and Analytics (CBICA), University of Pennsylvania, Philadelphia, Pennsylvania, USA.\n2 Department of Radiology, Perelman School of Medicine, University of Pennsylvania, Philadelphia, Pennsylvania, USA.\n3 Department of Pathology and Laboratory Medicine, Perelman School of Medicine, University of Pennsylvania, Philadelphia, Pennsylvania, USA.\n4 Department of Informatics, Technical University of Munich, Munich, Bavaria, Germany.\n5 Intel Corporation, Santa Clara, California, USA.\n6 Department of Quantitative Biomedicine, University of Zurich, Zurich, Switzerland.\n7 Department of Neuroradiology, Heidelberg University Hospital, Heidelberg, Germany.\n8 Clinical Cooperation Unit Neuropathology, German Cancer Consortium (DKTK) within the German Cancer Research Center (DKFZ), Heidelberg, Germany.\n9 Department of Neuropathology, Heidelberg University Hospital, Heidelberg, Germany.\n10 Division of Medical Image Computing, German Cancer Research Center, Heidelberg, Germany.\n11 Neurology Clinic, Heidelberg University Hospital, Heidelberg, Germany.\n12 Department of Radiology & Biomedical Imaging, University of California San Francisco, San Francisco, California, USA.\n13 Symbiosis Center for Medical Image Analysis, Symbiosis International University, Pune, Maharashtra, India.\n14 Department of Neuroimaging and Interventional Radiology, National Institute of Mental Health and Neurosciences, Bangalore, Karnataka, India.\n15 Department of Radiology, School of Medicine and Public Health, University of Wisconsin, Madison, Wisconsin, USA.\n16 Department of Medical Physics, School of Medicine and Public Health, University of Wisconsin, Madison, Wisconsin, USA.\n17 Department of Neuroradiology, Clinical Neuroscience Center, University Hospital Zurich and University of Zurich, Zurich, Switzerland.\n18 Leeds Teaching Hospitals Trust, Department of Radiology, Leeds, United Kingdom.\n19 Department of Radiology, Brigham and Women’s Hospital, Harvard Medical School, Boston, Massachusetts, USA.\n20 Athinoula A. Martinos Center for Biomedical Imaging, Massachusetts General Hospital, Charlestown, Massachusetts, USA.\n21 Catalan Institute of Oncology, Badalona, Spain.\n22 Consorci MAR Parc de Salut de Barcelona, Catalonia, Spain.\n23 Department of Radiology (IDI), Girona Biomedical Research Institute (IdIBGi), Josep Trueta University Hospital, Girona, Spain.\n24 Institute of Neuroradiology, Neumod Campus (NMC), Kepler University Hospital Linz, Linz, Austria.\n25 Department of Neurooncology, Neumod Campus (NMC), Kepler University Hospital Linz, Linz, Austria.\n26 Department of Radiation Oncology, Christiana Care Health System, Philadelphia, Pennsylvania, USA.\n27 Sidney Kimmel Medical College, Thomas Jefferson University, Philadelphia, Pennsylvania, USA.\n28 Department of Radiation Oncology, University of Maryland, Baltimore, Maryland, USA.\n29 Department of Radiation Oncology, Sidney Kimmel Cancer Center, Thomas Jefferson University, Philadelphia, Pennsylvania, USA.\n30 Department of Radiation Oncology, The James Cancer Hospital and Solove Research Institute, The Ohio State University Comprehensive Cancer Center, Columbus, Ohio, USA.\n31 Department of Radiology, Sidney Kimmel Cancer Center, Thomas Jefferson University, Philadelphia, Pennsylvania, USA.\n32 The Russell H. Morgan Department of Radiology and Radiological Science, Johns Hopkins University School of Medicine, Baltimore, Maryland, USA.\n33 The Malone Center for Engineering in Healthcare, The Whiting School of Engineering, Johns Hopkins University, Baltimore, Maryland, USA.\n34 Department of Electrical and Computer Engineering, Whiting School of Engineering, Johns Hopkins University, Baltimore, Maryland, USA.\n35 The Chinese University of Hong Kong, Hong Kong, China.\n36 Centre for Biomedical Image Analysis, Faculty of Informatics, Masaryk University, Brno, Czech Republic.\n37 Department of Radiology and Nuclear Medicine, Faculty of Medicine, Masaryk University, Brno and University Hospital Brno, Czech Republic.\n38 Department of Biophysics, Faculty of Medicine, Masaryk University, Brno, Czech Republic.\n39 Department of Neurosurgery, Faculty of Medicine, Masaryk University, Brno, and University Hospital and Czech Republic.\n40 Department of Neuro Oncology, H. Lee Moffitt Cancer Center and Research Institute, Tampa, Florida, USA.\n41 Department of Neurology, Clinical Neuroscience Center, University Hospital Zurich and University of Zurich, Zurich, Switzerland.\n42 Department of Radiology, H. Lee Moffitt Cancer Center and Research Institute, Tampa, Florida, USA.\n43 University of Texas Southwestern Medical Center, Dallas, Texas, USA.\n44 UCLA Brain Tumor Imaging Laboratory (BTIL), Center for Computer Vision and Imaging Biomarkers, Department of Radiological Sciences, David Geffen School of Medicine, University of California Los Angeles, Los Angeles, California, USA.\n45 UCLA Neuro-Oncology Program, Department of Neurology, David Geffen School of Medicine, University of California Los Angeles, Los Angeles, California, USA.\n46 Department of Radiological Sciences, David Geffen School of Medicine, University of California Los Angeles, Los Angeles, California, USA.\n47 College of Medicine and Public Health, Flinders University, Bedford Park, South Australia, Australia.\n48 Division of Surgery and Perioperative Medicine, Flinders Medical Centre, Bedford Park, South Australia, Australia.\n49 Department of Neurology, Baylor College of Medicine, Houston, Texas, USA.\n50 South Australia Medical Imaging, Flinders Medical Centre, Bedford Park, South Australia.\n51 Institute of Computing, University of Campinas, Campinas, São Paulo, Brazil.\n52 Federal Institute of São Paulo, Campinas, São Paulo, Brazil.\n53 Instituto de Neurologia de Curitiba, Curitiba, Paraná, Brazil.\n54 Department of Radiology, Hospital de Clínicas da Universidade Federal do Paraná, Curitiba, Paraná, Brazil.\n55 Department of Informatics, Universidade Federal do Paraná, Curitiba, Paraná, Brazil.\n56 Department of Radiology, Washington University in St. Louis, St. Louis, Missouri, USA.\n57 Department of Diagnostic and Interventional Neuroradiology, School of Medicine, Klinikum rechts der Isar, Technical University of Munich, Germany.\n58 TranslaTUM (Zentralinstitut für translationale Krebsforschung der Technischen Universität München), Klinikum rechts der Isar, Munich, Germany.\n59 Image-Based Biomedical Modeling, Department of Informatics, Technical University of Munich, Munich, Germany.\n60 Department of Radiology, NYU Grossman School of Medicine, New York, New York, USA.\n61 Department of Neurosurgery, NYU Grossman School of Medicine, New York, New York, USA.\n62 Support Center for Advanced Neuroimaging, University Institute of Diagnostic and Interventional Neuroradiology, University Hospital Bern, Inselspital, University of Bern, Bern, Switzerland.\n63 Department of Neurosurgery, Anschutz Medical Campus, University of Colorado, Aurora, Colorado, USA.\n64 Department of Radiology, University Hospitals Cleveland, Cleveland, Ohio, USA.\n65 Department of Neurological Surgery, University Hospitals-Seidman Cancer Center, Cleveland, Ohio, USA.\n66 Case Comprehensive Cancer Center, Cleveland, Ohio, USA.\n67 Department of Neurosurgery, Case Western Reserve University School of Medicine, Cleveland, Ohio, USA.\n68 National Cancer Institute, National Institute of Health, Division of Cancer Epidemiology and Genetics, Bethesda, Maryland, USA.\n69 Department of Radiology, Neuroradiology Division, University of Pittsburgh, Pittsburgh, Pennsylvania, USA.\n70 University of Pittsburgh Medical Center, Pittsburgh, Pennsylvania, USA.\n71 Department of Neuroradiology, University of Michigan, Ann Arbor, Michigan, USA.\n72 Department of Computational Medicine and Bioinformatics, University of Michigan, Ann Arbor, Michigan, USA.\n73 Department of Radiology, Baylor College of Medicine, Houston, Texas, USA.\n74 Department of Computing, Imperial College London, London, United Kingdom.\n75 Institute of Biomedical Engineering, Department of Engineering Science, University of Oxford, Oxford, United Kingdom.\n76 Department of Radiology, Imperial College NHS Healthcare Trust, London, United Kingdom.\n77 Computational Oncology Group, Institute for Global Health Innovation, Imperial College London, London, United Kingdom.\n78 Department of NeuroRadiology, University of Patras, Patras, Greece.\n79 Department of Neurosurgery, University of Patras, Patras, Greece.\n80 Clinical Radiology Laboratory, Department of Medicine, University of Patras, Patras, Greece.\n81 Department of Electrical and Computer Engineering, University of Patras, Patras, Greece.\n82 Department of Neuro-Oncology, University of Patras, Patras, Greece.\n83 Yonsei University College of Medicine, Seoul, Korea.\n84 Department of Radiation Oncology, Henry Ford Health System, Detroit, Michigan, USA.\n85 Public Health Sciences, Henry Ford Health System, Detroit, Michigan, USA.\n86 Case Western Reserve University, Cleveland, Ohio, USA.\n87 University of Alberta, Edmonton, Alberta, Canada.\n88 Alberta Machine Intelligence Institute, Edmonton, Alberta, Canada.\n89 Department of Radiology and Nuclear Medicine, Erasmus MC University Medical Centre Rotterdam, Rotterdam, Netherlands.\n90 Department of Neurosurgery, Brain Tumor Center, Erasmus MC University Medical Centre Rotterdam, Rotterdam, Netherlands.\n91 Department of Neurology, Brain Tumor Center, Erasmus MC Cancer Institute, Rotterdam, Netherlands.\n92 Data Science Institute, American College of Radiology, Reston, VA, USA.\n93 Department of Pathology, Brain Tumor Center, Erasmus MC Cancer Institute, Rotterdam, Netherlands.\n94 Biomedical Imaging Group Rotterdam, Department of Radiology and Nuclear Medicine, Erasmus MC University Medical Centre Rotterdam, Rotterdam, Netherlands.\n95 Department of Radiation Oncology, Icahn School of Medicine at Mount Sinai, New York, New York, USA.\n96 NORLUX Neuro-Oncology Laboratory, Department of Cancer Research, Luxembourg Institute of Health, Luxembourg, Luxembourg.\n97 Translation Radiomics, Department of Cancer Research, Luxembourg Institute of Health, Luxembourg.\n98 Luxembourg Center of Neuropathology, Laboratoire National De Santé, Luxembourg.\n99 Department of Computer Science, Université de Sherbrooke, Sherbrooke, Quebec, Canada.\n100 Division of Neurosurgery and Neuro-Oncology, Faculty of Medicine and Health Science, Université de Sherbrooke, Sherbrooke, Quebec, Canada.\n101 Department of Nuclear Medicine and Radiobiology, Sherbrooke Molecular Imaging Centre, Université de Sherbrooke, Sherbrooke, Quebec, Canada.\n102 Electrical and Computer Engineering, Vanderbilt University, Nashville, Tennessee, USA.\n103 Department of Computer Science, Vanderbilt University, Nashville, Tennessee, USA.\n104 Department of Neurosurgery, Vanderbilt University Medical Center, Nashville, Tennessee, USA.\n105 Innovation Center for Biomedical Informatics (ICBI), Georgetown University, Washington, District of Columbia, USA.\n106 Division of Neuroradiology & Neurointerventional Radiology, MedStar Georgetown University Hospital, Department of Radiology, Washington, DC, USA.\n107 School of Biomedical Engineering & Imaging Sciences, King’s College London, London, United Kingdom.\n108 Department of Neuroradiology; Ruskin Wing, King’s College Hospital NHS Foundation Trust, London, United Kingdom.\n109 Stoke Mandeville Hospital, Mandeville Road, Aylesbury, United Kingdom.\n110 Department of Biomedical and Molecular Sciences, Queen’s University, Kingston, ON, Canada.\n111 Neosoma Inc., Groton, Massachusetts, USA.\n112 University of Cairo School of Medicine, Giza, Egypt.\n113 University of Bern, Switzerland.\n114 Department of Radiology, Asan Medical Center, Seoul, South Korea.\n115 The Clatterbridge Cancer Centre NHS Foundation Trust Penbrooke Place, Liverpool, United Kingdom\n116 Department of Radiology, University of Washington, Seattle, Washington, USA.\n117 Netherlands Cancer Institute, Amsterdam, Netherlands.\n118 Clínica Imbanaco Grupo Quirón Salud, Cali, Colombia.\n119 Universidad del Valle, Cali, Colombia.\n120 The University of Edinburgh, Edinburgh, United Kingdom.\n121 Department of Industrial and Systems Engineering, University of Iowa, Iowa, USA.\n122 Department of Industrial and Systems Engineering, Department of Radiation Oncology, University of Iowa, Iowa, USA.\n123 Department of Radiation Oncology, University of Iowa, Iowa, USA.\n124 Center for Global Health, Perelman School of Medicine, University of Pennsylvania, Philadelphia, Pennsylvania, USA.\n125 Department of Diagnostic Radiology, University of Texas MD Anderson Cancer Center, Houston, Texas, USA.\n126 MD Anderson Cancer Center, University of Texas, Houston, Texas, USA.\n127 University of Alabama in Birmingham, Birmingham, Alabama, USA.\n128 Department of Biomedical Informatics, Stony Brook University, Stony Brook, New York, USA.\n129 Scientific Data Group, Oak Ridge National Laboratory, Oak Ridge, Tennessee, USA.\n130 Escuela Superior Politecnica del Litoral, Guayaquil, Guayas, Ecuador.\n131 Universidad Católica de Cuenca, Cuenca, Ecuador.\n132 Universidad de Concepción, Concepción, Biobío, Chile.\n133 School of Electronic Engineering and Computer Science, Queen Mary University of London, London, United Kingdom.\n134 Department of Radiology, University College Hospital Ibadan, Oyo, Nigeria.\n135 Clinic Healthcare, Lagos, Lagos, Nigeria.\n136 Department of Radiology, Muhammad Abdullahi Wase Teaching Hospital, Kano, Nigeria.\n137 Department of Radiology, Obafemi Awolowo University Ile-Ife, Ile-Ife, Osun, Nigeria.\n138 School of Computing, Queen’s University, Kingston, Ontario, Canada.\n139 Center for Research and Innovation, American College of Radiology, Philadelphia, Pennsylvania, USA.\n140 Center for Biomedical Informatics and Information Technology, National Cancer Institute (NCI), National Institute of Health, Bethesda, Maryland, USA.\n141 Department of Radiation Oncology, Stony Brook University, Stony Brook, New York, USA.\n142 Department of Radiology, Stony Brook University, Stony Brook, New York, USA.\n143 Pattern Analysis and Learning Group, Department of Radiation Oncology, Heidelberg University Hospital, Heidelberg, Germany.\n144 Sociedad de Lucha Contra el Cancer - SOLCA, Guayaquil Ecuador.\n145 Centre de Recherche du Centre Hospitalier Universitaire de Sherbrooke, Sherbrooke, Quebec, Canada.\n146 The Faculty of Arts & Sciences, Queen’s University, Kingston, Ontario, Canada.\n147 Institute of Diagnostic and Interventional Neuroradiology, RKH Klinikum Ludwigsburg, Ludwigsburg, Germany.\n148 SJTU-Ruijing-UIH Institute for Medical Imaging Technology, Ruijin Hospital, Shanghai Jiao Tong University School of Medicine, No. 197, Rui Jin 2nd Road, Shanghai 200025, China.\n149 Department of Electrical Engineering, Qazvin Branch, Islamic Azad University, Qazvin, Iran.\n150 Department of Radiation Oncology, University of Patras, Patras, Greece.\n151 Department of Oncology, Queen’s University, Kingston, Ontario, Canada.\n152 Department of Radiology, Netherlands Cancer Institute, Amsterdam, Netherlands.\n153 GROW School of Oncology and Developmental Biology, Maastricht, Netherlands.\nThese authors contributed equally to this work.\n$ Corresponding author: {sbakas@upenn.edu}\nAbstract. Although machine learning (ML) has shown promise in numerous domains, there are concerns about generalizability to out-of-sample data. This is currently addressed by centrally sharing ample, and importantly diverse, data from multiple sites. However, such centralization is challenging to scale (or even not feasible) due to various limitations. Federated ML (FL) provides an alternative to train accurate and generalizable ML models, by only sharing numerical model updates. Here we present findings from the largest FL study to-date, involving data from 71 healthcare institutions across 6 continents, to generate an automatic tumor boundary detector for the rare disease of glioblastoma, utilizing the largest dataset of such patients ever used in the literature (25,256 MRI scans from 6,314 patients). We demonstrate a 33% improvement over a publicly trained model to delineate the surgically targetable tumor, and 23% improvement over the tumor’s entire extent. We anticipate our study to: 1) enable more studies in healthcare informed by large and diverse data, ensuring meaningful results for rare diseases and underrepresented populations, 2) facilitate further quantitative analyses for glioblastoma via performance optimization of our consensus model for eventual public release, and 3) demonstrate the effectiveness of FL at such scale and task complexity as a paradigm shift for multi-site collaborations, alleviating the need for data sharing.\n\nKeywords: federated learning, deep learning, convolutional neural network, segmentation, brain tumor, glioma, glioblastoma, FeTS, BraTS\n\nAdvances in machine learning (\\( ML \\)), and particularly deep learning (\\( DL \\)), have shown promise in addressing complex healthcare problems\\(^{1-14}\\). However, there are concerns about generalizability on data from sources that did not participate in model training, i.e., “out-of-sample” data\\(^{15,16}\\). Literature indicates that training robust and accurate models requires large amounts of data\\(^{17-19}\\), the diversity of which affects model generalizability to “out-of-sample” cases\\(^{20}\\). To address these concerns, models need to be trained on data originating from numerous sites representing diverse population samples. The current paradigm for such multi-site collaborations is “centralized learning” (\\( CL \\)), in which data from different sites are shared to a centralized location following inter-site agreements\\(^{20-23}\\). However, such data centralization is difficult to scale (and might not even be feasible), especially at a global scale, due to concerns\\(^{24,25}\\) relating to privacy, data-ownership, intellectual property, technical challenges (e.g., network and storage limitations), as well as compliance with varying regulatory policies (e.g., Health Insurance Portability and Accountability Act (HIPAA) of the United States\\(^{26}\\) and the General Data Protection Regulation (GDPR) of the European Union\\(^{27}\\)). In contrast to this centralized paradigm, “federated learning” (\\( FL \\)) describes an approach where models are trained by only sharing model parameter updates from decentralized data (i.e., each site retains its data locally)\\(^{24,25,28-30}\\), without sacrificing performance when compared to CL-trained models\\(^{25,29,31-35}\\). Thus, FL can offer an alternative to CL, potentially creating a paradigm shift that alleviates the need for data sharing, and hence increase access to geographically-distinct collaborators, thereby increasing the size and diversity of data used to train ML models.\n\nFL has tremendous potential in healthcare\\(^{36,37}\\), particularly towards addressing health disparities, under-served populations, and “rare” diseases\\(^{38}\\), by enabling ML models to gain knowledge from ample and diverse data that would otherwise not be available. With that in mind, here we focus on the “rare” disease of glioblastoma, and particularly on the detection of its extent using multi-parametric magnetic resonance imaging (mpMRI) scans\\(^{39}\\). While glioblastoma is the most common malignant primary brain tumor\\(^{40-42}\\), it is still classified as a “rare” disease, as its incidence rate (i.e., 3/100,000 people) is substantially lower than\nthe rare disease definition rate (i.e., < 10/100,000 people)\\(^{38}\\). This means that single sites cannot collect large and diverse datasets to train robust and generalizable ML models, and necessitates collaboration between geographically distinct sites. Despite extensive efforts to improve prognosis of glioblastoma patients with intense multimodal therapy, their median overall survival is only 14.6 months after standard-of-care treatment, and 4 months without treatment\\(^{43}\\). Although the subtyping of glioblastoma has been improved\\(^{44}\\) and the standard-of-care treatment options have expanded during the last twenty years, there have been no substantial improvements in overall survival\\(^{45}\\). This reflects the major obstacle in treating these tumors that is their intrinsic heterogeneity\\(^{40,42}\\), and the need for analyses of larger and more diverse data towards better understanding the disease. In terms of radiologic appearance, glioblastomas comprise 3 main sub-compartments, defined as i) the “enhancing tumor” (ET), representing the vascular blood-brain barrier breakdown within the tumor, ii) the “tumor core” (TC), which includes the ET and the necrotic (NCR) part, and represents the surgically relevant part of the tumor, and iii) the “whole tumor” (WT), which is defined by the union of the TC and the peritumoral edematous/infiltrated tissue (ED), and represents the complete tumor extent relevant to radiotherapy (Fig. 1.b). Detecting these sub-compartment boundaries therefore defines a multi-parametric multi-class learning problem\\(^{46-50}\\), and is a critical first step towards further quantifying and assessing this heterogeneous rare disease and ultimately influencing clinical decision-making.\n\nCo-authors in this study have previously introduced FL in healthcare in a simulated setting\\(^{29}\\) and evaluated different FL approaches\\(^{25}\\) for the same use case as the present study, i.e., detecting the boundaries of glioblastoma sub-compartments. Findings from these studies supported the superiority of the FL approach used in the present study (i.e., based on an aggregation server\\(^{24,28}\\)), which had almost identical performance to CL. The present study describes the largest to-date global FL effort to develop an accurate and generalizable ML model for detecting glioblastoma sub-compartment boundaries, based on 25,256 MRI scans (over 5TB) of 6,314 glioblastoma patients from 71 geographically distinct sites, across 6 continents (Fig. 1.a). Notably, this describes the largest and most diverse dataset of glioblastoma patients ever considered in the literature. It was the use of FL that successfully enabled our ML model to gain knowledge from such an unprecedented dataset. The extended global footprint and the task complexity is what sets this study apart from current literature, since it dealt with a multi-parametric multi-class problem with reference standards that require expert clinicians following an involved manual annotation protocol, rather than recording a categorical entry from medical records\\(^{30,51}\\). Moreover, varying characteristics of the mpMRI data due to scanner hardware and acquisition protocol differences\\(^{52,53}\\) were handled at each collaborating site via established harmonized preprocessing pipelines\\(^{54-57}\\).\n\nThe scientific contributions of this manuscript can be summarized by i) the insights garnered during this work that can pave the way for more successful FL studies of increased scale and task complexity, ii) making a potential impact for the treatment of the rare disease of glioblastoma, by eventually publicly releasing an optimized trained consensus model for use in resource-constrained clinical settings, and iii) demonstrating the effectiveness of FL at such scale and task complexity as a paradigm shift redefining multi-site collaborations, while alleviating the need for data sharing.\nFig. 1: Representation of the study’s global scale, diversity, and complexity. a, The map of all sites involved in the development of FL consensus model. b, example of a glioblastoma mpMRI scan with corresponding reference annotations of the tumor sub-compartments. c-d, comparative performance evaluation of the final consensus model with the public initial model on the collaborators’ local validation data (in c) and on the complete out-of-sample data (in d), per tumor sub-compartment. Note the box and whiskers inside each violin plot, represent the true min and max values. The top and bottom of each “box” depict the 3rd and 1st quartile of each measure. The white line and the red ×, within each box, indicate the median and mean values, respectively. The fact that these are not necessarily at the centre of each box indicates the skewness of the distribution over different cases. The “whiskers” drawn above and below each box depict the extremal observations still within 1.5 times the interquartile range, above the 3rd or below the 1st quartile. e, number of contributed cases per collaborating site.\nMethods\n\nData\n\nThe data considered in this study described patient populations with adult-type diffuse glioma\\(^{44}\\), and specifically displaying the radiological features of glioblastoma, scanned with mpMRI to characterize the anatomical tissue structure\\(^{39}\\). Each case is specifically described by i) native T1-weighted (T1), ii) Gadolinium-enhanced T1-weighted (T1Gd), iii) T2-weighted (T2), and iv) T2-weighted-Fluid-Attenuated-Inversion-Recovery (T2-FLAIR) MRI scans. Cases with any of these sequences missing were not included in the study. Note that no inclusion/exclusion criterion applied relating to the type of acquisition (i.e., both 2D axial and 3D acquisitions were included, with a preference for 3D if available), or the exact type of sequence (e.g., MP-RAGE vs SPGR). The only exclusion criterion was for T1-FLAIR scans that were intentionally excluded to avoid mixing varying tissue appearance due to the type of sequence, across native T1-weighted scans.\n\nThe eligibility of collaborating sites to participate in the federation was determined based on data availability, and approval by their respective institutional review board. 55 sites participated as independent collaborators in the study defining a dataset of 6,083 cases. The MRI scanners used for data acquisition were from multiple vendors (i.e., Siemens, GE, Philips, Hitachi, Toshiba), with magnetic field strength ranging from 1T to 3T. The data from all 55 collaborating sites followed a male:female ratio of 1.47 : 1 with age ranging between 7 and 94 years.\n\nFrom all 55 collaborating sites, 49 were chosen to be part of the training phase, and 6 sites were categorized as “out-of-sample”, i.e., none of these were part of the training stage. These specific 6 out-of-sample sites (Site IDs: 8, 11, 19, 20, 21, 43) were allocated based on their availability, i.e., they have indicated an expected delayed participation rendering them optimal for model generalizability validation. One of these 6 out-of-sample sites (Site 11) contributed aggregated *a priori* data from a multi-site randomized clinical trial for newly diagnosed glioblastoma (ClinicalTrials.gov Identifier: NCT00884741, RTOG0825\\(^{58,59}\\), ACRIN6686\\(^{60,61}\\)), with inherent diversity benefiting the intended generalizability validation purpose. The American College of Radiology (ACR - Site 11) serves as the custodian of this trial’s imaging data on behalf of ECOG-ACRIN, who made the data available for this study. Following screening for availability of the 4 required mpMRI scans with sufficient signal-to-noise ratio judged by visual observation, a subset of 362 cases from the original trial data were included in this study. The out-of-sample data totaled 590 cases intentionally held-out of the federation, with the intention of validating the consensus model in completely unseen cases. To facilitate further such generalizability evaluation without burdening the collaborating sites, a subset consisting of 332 cases (including the multi-site clinical data provided by ACR) from this out-of-sample data was aggregated, to serve as the “*centralized out-of-sample*” dataset. Furthermore, the 49 sites participating in the training phase define a collective dataset of 5,493 cases. The exact 49 site IDs are: 1, 2, 3, 4, 5, 6, 7, 9, 10, 12, 13, 14, 15, 16, 17, 18, 22, 23, 24, 25, 26, 27, 28, 29, 30, 31, 32, 33, 34, 35, 36, 37, 38, 39, 40, 41, 42, 44, 45, 46, 48, 49, 50, 52, 53, 54, 56, 59, 60. These cases were automatically split at each site following a 4 : 1 ratio between cases for training and local validation. During the federated training phase the data used for the public initial model were also included as a dataset from a separate node, such that the contribution of sites providing the publicly available data is not forgotten within the global consensus model. This\nresults in the final consensus model being developed based on data from 71 sites over a total dataset of 6,314 cases.\n\nHarmonized Data Preprocessing\n\nOnce each collaborating site identified their local data, they were asked to use the preprocessing functionality of the software platform we provided. This functionality follows the harmonized data preprocessing protocol defined by the BraTS challenge\\(^{54-57}\\), to account for inter-site acquisition protocol variations, e.g., 3D vs 2D axial plane acquisitions.\n\nThe neural network architecture\n\nThe trained model to delineate the different tumor sub-compartments was based on the popular 3D U-Net with residual connections (3D-ResUNet)\\(^{62-66}\\). The network had 30 base filters, with a learning rate of \\(lr = 5 \\times 10^{-5}\\) optimized using the Adam optimizer\\(^{67}\\). For the loss function used in training, we used the generalized \\(DSC\\) score\\(^{68,69}\\) (represented mathematically in Eq. 1) on the absolute complement of each tumor sub-compartment independently. Such mirrored \\(DSC\\) loss has been shown to capture variations in smaller regions better\\(^{70}\\). No penalties were used in the loss function, due to our use of ‘mirrored’ \\(DSC\\) loss\\(^{71-73}\\). The final layer of the model was a sigmoid layer, providing three channel outputs for each voxel in the input volume, one output channel per tumor sub-compartment. While the generalized \\(DSC\\) score was calculated using a binarized version of the output (check sigmoid value against the threshold 0.5) for the final prediction, we used the floating point \\(DSC^{74}\\) during the training process.\n\n\\[\nDSC = \\frac{2 \\| RL \\odot PM \\|_1}{\\| RL \\|_1 + \\| PM \\|_1}\n\\]\n\nwhere RL serves as the reference label, \\(PM\\) is the predicted mask, \\(\\odot\\) is the Hadamard product\\(^{75}\\) (i.e., component wise multiplication), and \\(\\| x \\|_1\\) is the L1-norm\\(^{76}\\), i.e., sum of the absolute values of all components).\n\nThe Federation\n\nThe collaborative network of the present study spans 6 continents (Fig. 1), with data from 71 geographically distinct sites. The training process was initiated when each collaborator securely connected to a central aggregation server, which resided behind a firewall at the University of Pennsylvania. As soon as the secure connection was established, the public initial model was passed to the collaborating site. Using FL based on an aggregation server, collaborating sites then trained the same network architecture on their local data for one epoch, and shared model updates with the central aggregation server. The central aggregation server received model updates from all collaborators, combined them (by averaging model parameters) and sent the consensus model back to each collaborator to continue their local training. Each such iteration is called a “federated round”. After not observing any meaningful changes since round 42, we stopped the training after a total of 73 federated rounds. Additionally, we performed all operations on the aggregator on secure hardware (by leveraging trusted execution environments\\(^{77}\\)), in order to increase the trust by all parties in the confidentiality of the model\nupdates being computed and shared, as well as to increase the confidence in the integrity of the computations being performed\\(^{78}\\).\n\nThe federated training was initialized using a “public initial model” trained on 231 cases from 16 sites. This was done as opposed to a random initialization point to facilitate faster convergence of the model performance\\(^{79,80}\\). After the training process was complete, the “final consensus model” was obtained after model selection from all the global consensus models obtained for each federated round. Thus, the final consensus model was developed on 6,314 cases from 71 sites. To quantitatively evaluate the performance of the trained models, 20% of the total cases contributed by each participating site were excluded from the model training process and were used as “local validation data”. To further evaluate the generalizability of the models in unseen data, 6 sites were not involved in any of the training stages to represent an unseen “out-of-sample” data population of 590 cases. To facilitate further evaluation without burdening the collaborating sites, a subset (\\( n = 332 \\)) of these cases was aggregated to serve as a “centralized out-of-sample” dataset. Model performance was quantitatively evaluated here using the Dice Similarity Coefficient (\\( DSC \\)), which assesses the spatial agreement between the model’s prediction and the reference standard for each of the 3 tumor sub-compartments (ET, TC, WT).\n\nModel Run-time in Clinical Environments\n\nClinical environments typically have constrained computational resources, such as the availability of specialized hardware (e.g., DL acceleration cards) and increased memory, which affect the run-time performance of DL inference workloads. Thus, taking into consideration the potential deployment of the final consensus model in such low-resource settings, we decided to proceed with a single 3D-ResUNet, rather than an ensemble of multiple models. This decision ensured a reduced computational burden, when compared with running multiple models, which is typically done in academic research projects\\(^{54-57}\\).\n\nTo further facilitate use in low-resource environments, we plan to publicly release run-time optimized\\(^{81}\\) version of the final consensus model. For this model, graph level optimizations (i.e., operators fusion) were initially applied, followed by optimizations for low precision inference, i.e., converting the floating point single precision model to a fixed precision 8-bit integer model (a process known as “quantization”\\(^{82}\\)). In particular, we used accuracy-aware quantization\\(^{83}\\), where model layers were iteratively scaled to a lower precision format. These optimizations yielded several run-time performance benefits, such as lower inference latency (a platform-dependent \\(4.48\\times\\) average speedup and \\(2.29\\times\\) reduced memory requirement when compared with the original consensus model), and higher throughput (equal to the \\(4.48\\times\\) speedup improvement since the batch size used is equal to 1), while the trade-off was an insignificant (\\(P_{Average} < 7 \\times 10^{-5}\\)) drop in the average \\(DSC\\).\n\nCode availability\n\nMotivated by findability, accessibility, interoperability, and reusability (FAIR) criteria in scientific research\\(^{84}\\), all the code used to design the Federated Tumor Segmentation (FeTS) platform for this study is available at https://github.com/FETS-AI/Front-End. The functionality related to preprocessing (i.e., DICOM to NIfTI conversion, population-based harmonized pre-processing, co-registration) and manual refinements of annotation is derived from the open-source\nCancer Imaging Phenomics Toolkit (CaPTk, https://github.com/CBICA/CaPTk)85–87. The co-registration is performed using the Greedy framework88, available via CaPTk85–87, ITK-SNAP89, and the FeTS tool. The brain extraction90 is done using the BrainMaGe method91, and is available in https://github.com/CBICA/BrainMaGe and via the Generally Nuanced Deep Learning Framework (GaNDLF)92 at https://github.com/CBICA/GaNDLF. To generate automated annotations, DeepMedic’s93 integration with CaPTk was used, and we used the model weights and inference mechanism provided by the other algorithm developers (DeepScan94 and nnU-Net70 (https://github.com/MIC-DKFZ/nnunet)). DeepMedic’s original implementation is available in https://github.com/deepmedic/deepmedic, whereas the one we used in this study can be found at https://github.com/CBICA/deepmedic. The fusion of the labels was done using the Label Fusion tool95 available at https://github.com/FETS-AI/LabelFusion. The data loading pipeline and network architecture was developed using the GaNDLF framework92 by using PyTorch96. The data augmentation was done via GaNDLF by leveraging TorchIO97. The FL backend developed for this project has been open-sourced as a separate software library, to encourage further research on FL98 and is available at https://github.com/intel/openfl. The optimization of the consensus model inference workload was performed via OpenVINO99 (https://github.com/openvinotoolkit/openvino/tree/2021.4.1), which is an open-source toolkit enabling acceleration of neural network models through various optimization techniques. The optimizations were evaluated on an Intel Core® i7-1185G7E CPU @ 2.80GHz with \\(2 \\times 8\\) GB DDR4 3200MHz memory on Ubuntu 18.04.6 OS and Linux kernel version 5.9.0-050900-generic.\n\nResults\n\nAt the time of initialization of the federation, the public initial model was evaluated against the local validation data of all sites, resulting in an average (across all cases of all sites) \\(DSC\\) per sub-compartment, of: \\(DSC_{ET} = 0.63\\), \\(DSC_{TC} = 0.62\\), \\(DSC_{WT} = 0.75\\). To summarize the model performance with a single collective score, we then calculate the average \\(DSC\\) (across all 3 tumor sub-compartments per case, and then across all cases of all sites) as equal to 0.66.\n\nFollowing model training across all sites, the final consensus model garnered significant performance improvements against the collaborators’ local validation data of 27% (\\(p_{ET} < 1 \\times 10^{-36}\\)), 33% (\\(p_{TC} < 1 \\times 10^{-59}\\)), and 16% (\\(p_{WT} < 1 \\times 10^{-21}\\)), for ET, TC, and WT, respectively (Fig. 1.c).\n\nTo further evaluate the potential generalizability improvements of the final consensus model on unseen data, we compared it with the public initial model against the complete out-of-sample data, and noted significant performance improvements of 15% (\\(p_{ET} < 1 \\times 10^{-5}\\)), 27% (\\(p_{TC} < 1 \\times 10^{-16}\\)), and 16% (\\(p_{WT} < 1 \\times 10^{-7}\\)), for ET, TC, and WT, respectively (Fig. 1.d).\n\nNotably, the only difference between the public initial model and the final consensus model, was that the latter gained knowledge during training from increased datasets contributed by the complete set of collaborators. The conclusion of these findings reinforces the importance of using large and diverse data for generalizable models to ultimately drive patient care.\nDiscussion\n\nIn this study, we have described the largest real-world FL effort to-date utilizing data of 6,314 glioblastoma patients from 71 geographically unique sites spread across 6 continents, to develop an accurate and generalizable ML model for detecting glioblastoma sub-compartment boundaries. Notably, this extensive global footprint of the collaborating sites in this study, also yield the largest dataset ever reported in the literature assessing this rare disease. It is the use of FL that successfully enabled \\( i) \\) access to such an unprecedented dataset of the most common and fatal adult brain tumor, and \\( ii) \\) meaningful ML training to ensure generalizability of models across out-of-sample data. Since glioblastoma boundary detection is critical for treatment planning and the requisite first step for further quantitative analyses, the models generated during this study have the potential to make far-reaching clinical impact.\n\nThe large and diverse data that FL enabled, led to the final consensus model garnering significant performance improvements over the public initial model against both the collaborators’ local validation data and the complete out-of-sample data. The improved result is a clear indication of the benefit that can be afforded through access to more data. In comparison with the limited existing real-world FL studies\\(^{30,51}\\), our use case is larger in scale and substantially more complex, since it 1) addresses a multi-parametric multi-class problem, with reference standards that require expert collaborating clinicians to follow an involved manual annotation protocol, rather than simply recording a categorical entry from medical records, and 2) requires the data to be preprocessed in a harmonized manner to account for differences in MRI acquisition.\n\nWe have demonstrated the utility of an FL approach to develop an accurate and generalizable ML model for detecting glioblastoma sub-compartment boundaries, a finding which is of particular relevance for neurosurgical and radiotherapy planning in patients with this disease. This study is meant to be used as a blueprint for future FL studies that result in clinically deployable ML models. Building on this study, a continuous FL consortium would enable downstream quantitative analyses with implications for both routine practice and clinical trials, and most importantly, increase access to high-quality precision care worldwide. Furthermore, the lessons learned from this study with such a global footprint are invaluable and can be applied to a broad array of clinical scenarios with the potential for great impact to rare diseases and underrepresented populations.\n\nAcknowledgments\n\nResearch and main methodological developments reported in this publication were partly supported by the National Institutes of Health (NIH) under award numbers NIH/NCI:U01CA242871 (S.Bakas), NIH/NINDS:R01NS042645 (C.Davatzikos), NIH/NCI:U24CA189523 (C.Davatzikos), NIH/NCI:U24CA215109 (J.Saltz), NIH/NCI:U01CA248226 (P.Tiwari), NIH/NCI:P30CA51008 (Y.Gusev), NIH:R50CA211270 (M.Muzi), NIH/NCATS:UL1TR001433 (Y.Yuan), NIH/NIBIB:R21EB030209 (Y.Yuan), NIH/NCI:R37CA214955 (A.Rao), and NIH:R01CA233888 (A.L.Simpson). The authors would also like to acknowledge the following NIH funded awards for the multi-site clinical trial (NCT00884741, RTOG0825/ACRIN6686): U10CA21661, U10CA37422, U10CA180820, U10CA180794, U01CA176110, R01CA082500, CA079778, CA080098, CA180794, CA180820,\nCA180822, CA180868. Research reported in this publication was also partly supported by the National Science Foundation, under award numbers 2040532 (S.Baek), and 2040462 (B.Landman). Research reported in this publication was also supported by i) a research grant from Varian Medical Systems (Palo Alto, CA USA) (Y.Yuan), ii) the Ministry of Health of the Czech Republic (Grant Nr. NU21-08-00359) (M.Kerkovský and M.Kozubek), iii) Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) Project-ID 404521405, SFB 1389, Work Package C02, and Priority Programme 2177 “Radiomics: Next Generation of Biomedical Imaging” (KI 2410/1-1 — MA 6340/18-1) (P.Vollmuth), iv) DFG Project-ID B12, SFB 824 (B.Wiestler), v) the Helmholtz Association (funding number ZT-I-OO1 4) (K.Maier-Hein), vi) the Dutch Cancer Society (KWF project number EMCR 2015-7859) (S.R.van der Voort), vii) the Chilean National Agency for Research and Development (ANID-Basal FB0008 (AC3E) and FB210017 (CENIA)) (P.Guevara), viii) the Canada CIFAR AI Chairs Program (M.Vallières), ix) Leeds Hospital Charity (Ref: 9RO1/1403) (S.Currie), x) the Cancer Research UK funding for the Leeds Radiotherapy Research Centre of Excellence (RadNet) and the grant number C19942/A28832 (S.Currie), xi) Medical Research Council (MRC) Doctoral Training Programme in Precision Medicine (Award Reference No. 2096671) (J.Bernal), xii) The European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (Grant Agreement No. 757173) (B.Glocker), xiii) The UKRI London Medical Imaging & Artificial Intelligence Centre for Value Based Healthcare (K.Kamnitsas), xiv) Wellcome/Engineering and Physical Sciences Research Council (EPSRC) Center for Medical Engineering (WT 203148/Z/16/Z) (T.C.Booth), xv) American Cancer Society Research Scholar Grant RSG-16-005-01 (A.Rao), xvi) the Department of Defense (DOD) Peer Reviewed Cancer Research Program (PRCRP) W81XWH-18-1-0404, Dana Foundation David Mahoney Neuroimaging Program, the V Foundation Translational Research Award, Johnson & Johnson WiSTEM2D Award (P.Tiwari), xvii) RSNA Research & Education Foundation under grant number RR2011 (E.Calabrese), xviii) the National Research Fund of Luxembourg (FNR) (grant number: C20/BM/14646004/GLASS-LUX/Niclou) (S.P.Niclou), xix) EU Marie Curie FP7-PEOPLE-2012-ITN project TRANSACT (PITN-GA-2012-316679) and the Swiss National Science Foundation (project number 140958) (J.Slotboom), and xx) CNPq 303808/2018-7 and FAPESP 2014/12236-1 (A.Xavier Falcão). The content of this publication is solely the responsibility of the authors and does not represent the official views of the NIH, the NSF, the RSNA R&E Foundation, or any of the additional funding bodies.\n\nAuthor Contributions\n\nStudy Conception: S.Pati, U.Baid, B.Edwards, M.Sheller, G.A.Reina, J.Martin, S.Bakas.\nDevelopment of software used in the study: S.Pati, B.Edwards, M.Sheller, S.Wang, G.A.Reina, P.Foley, A.Gruzdev, D.Karkada.\nData Acquisition: M.Bilello, S.Mohan, E.Calabrese, J.Rudie, J.Saini, R.Y.Huang, K.Chang, T.So, P.Heng, T.F.Cloughesy, C.Raymond, T.Oughourlian, A.Hagiwara, C.Wang, M.To, M.Kerkovský, T.Kopřivová, M.Dostál, V.Vybíhál, J.A.Maldjian, M.C.Pinho, D.Reddy, J.Holcomb, B.Wiestler, M.Metz, R.Jain, M.Lee, P.Tiwari, R.Verma, Y.Gusev, K.Bhuvaneshwar, C.Bencheqroun, A.Belouali, A.Abayazeed, A.Abbassy, S.Gamal, M.Qayati, M.Mekhaimar, M.Reyes, R.R.Colen, M.Ak, P.Vollmuth, G.Brugnara, F.Sahm, M.Bendszus,\nW.Wick, A.Mahajan, C.Balaña Quintero, J.Capellades, J.Puig, Y.Choi, M.Muzi, H.F.Shaykh, A.Herrera-Trujillo, W.Escobar, A.Abello, P.LaMontagne, B.Landman, K.Ramadass, K.Xu, S.Chotai, L.B.Chambless, A.Mistry, R.C.Thompson, J.Bapuraj, N.Wang, S.R.van der Voort, F.Incekara, M.M.J.Wijnenga, R.Gahrmann, J.W.Schouten, H.J.Dubbink, A.J.P.E.Vincent, M.J.van den Bent, H.I.Sair, C.K.Jones, A.Venkataraman, J.Garrett, M.Larson, B.Menze, T.Weiss, M.Weller, A.Bink, B.Pouymayou, Y.Yuan, S.Sharma, T.Tseng, B.C.A.Teixeira, F.Sprenger, S.P.Niclou, O.Keunen, L.V.M.Dixon, M.Williams, R.G.H.Beets-Tan, H.Franco-Maldonado, F.Loayza, J.Slotboom, P.Radojewski, R.Meier, R.Wiest, J.Trenkler, J.Pichler, G.Necker, S.Meckel, E.Torche, F.Vera, E.López, Y.Kim, H.Ismael, B.Allen, J.M.Buatti, J.Park, P.Zampakis, V.Panagiotopoulos, P.Tsiganos, E.Challiasos, D.M.Kardamakis, P.Prasanna, K.M.Mani, D.Payne, T.Kurc, L.Poisson, M.Vallières, D.Fortin, M.Lepage, F.Morón, J.Mandel, C.Badve, A.E.Sloan, J.S.Barnholtz-Sloan, K.Waite, G.Shukla, S.Liem, G.S.Alexandre, J.Lombardo, J.D.Palmer, A.E.Flanders, A.P.Dicker, G.Ogbole, M.Soneye, D.Oyekunle, O.Odafe-Oyibotha, B.Osobu, M.Shu’aibu, F.Dako, A.Dorcas, D.Murcia, R.Haas, J.Thompson, D.R.Ormond, S.Currie, K.Fatania, R.Frood, J.Mitchell, J.Farinhas, A.L.Simpson, J.J.Peoples, R.Hu, D.Cutler, F.Y.Moraes, A.Tran, M.Hamghalam, M.A.Boss, J.Gimpel, B.Bialecki, A.Chelliah.\n\nData Processing: C.Sako, S.Ghodasara, E.Calabrese, J.Rudie, M.Jadhav, U.Pandey, R.Y.Huang, M.Jiang, C.Chen, C.Raymond, S.Bhardwaj, C.Chong, M.Agzarian, M.Kozubek, F.Lux, J.Michálek, P.Matula, C.Bangalore Yogananda, D.Reddy, B.C.Wagner, I.Ezhov, M.Lee, Y.W.Lui, R.Verma, R.Bareja, I.Yadav, J.Chen, N.Kumar, K.Bhuvaneshwar, A.Sayah, C.Bencheqroun, K.Kolodziej, M.Hill, M.Reyes, L.Pei, M.Ak, A.Kotrotsou, P.Vollmuth, G.Brugnara, C.J.Preetha, M.Zenk, J.Puig, M.Muzi, H.F.Shaykh, A.Abello, J.Bernal, J.Gómez, P.LaMontagne, K.Ramadass, S.Chotai, N.Wang, M.Smits, S.R.van der Voort, A.Alafandi, F.Incekara, M.M.J.Wijnenga, G.Kapsas, R.Gahrmann, A.J.P.E.Vincent, P.J.French, S.Klein, H.I.Sair, C.K.Jones, J.Garrett, H.Li, F.Kofler, Y.Yuan, S.Adabi, A.Xavier Falcão, S.B.Martins, D.Menotti, D.R.Lucio, O.Keunen, A.Hau, K.Kamnitsas, L.Dixon, S.Benson, E.Pelaez, H.Franco-Maldonado, F.Loayza, S.Quevedo, R.McKinley, J.Trenkler, A.Haunschildt, C.Mendoza, E.Ríos, J.Choi, S.Baek, J.Yun, P.Zampakis, V.Panagiotopoulos, P.Tsiganos, E.I.Zacharaki, C.Kalogeropoulou, P.Prasanna, S.Shreshtra, T.Kurc, B.Luo, N.Wen, M.Vallières, D.Fortin, F.Morón, C.Badve, V.Vadmal, G.Shukla, G.Ogbole, D.Oyekunle, F.Dako, D.Murcia, E.Fu, S.Currie, R.Frood, M.A.Vogelbaum, J.Mitchell, J.Farinhas, J.J.Peoples, M.Hamghalam, D.Kattil Veettil, K.Schmidt, B.Bialecki, S.Marella, T.C.Booth, A.Chelliah, M.Modat, C.Dragos, H.Shuaib.\n\nData Analysis & Interpretation: S.Pati, U.Baid, B.Edwards, M.Sheller, S.Bakas.\n\nSite PI/Senior member (of each collaborating group): C.Davatzikos, J.Villanueva-Meyer, M.Ingalhalikar, R.Y.Huang, Q.Dou, B.M.Ellingson, M.To, M.Kozubek, J.A.Maldjian, B.Wiestler, R.Jain, P.Tiwari, Y.Gusev, A.Abavazeed, R.R.Colen, P.Vollmuth, A.Mahajan, C.Balaña Quintero, S.Lee, M.Muzi, H.F.Shaykh, M.Trujillo, D.Marcus, B.Landman, A.Rao, M.Smits, H.I.Sair, R.Jeraj, B.Menze, Y.Yuan, A.Xavier Falcão, S.P.Niclou, B.Glocker, J.Teuwen, E.Pelaez, R.Wiest, S.Meckel, P.Guevara, S.Baek, H.Kim, D.M.Kardamakis, J.Saltz, L.Poisson, M.Vallières, F.Morón, A.E.Sloan, A.E.Flanders, G.Ogbole, D.R.Ormond, S.Currie, J.Farinhas, A.L.Simpson, C.Apgar, T.C.Booth.\n\nWriting the Original Manuscript: S.Pati, U.Baid, B.Edwards, M.Sheller, S.Bakas.\n\nReview, Edit, & Approval of the Final Manuscript: All authors.\nCompeting Interest Declaration\n\nThe Intel affiliated authors (B.Edwards, M.Sheller, S.Wang, G.A.Reina, P.Foley, A.Gruzdev, D.Karkada, P.Shah, J.Martin) would like to disclose the following (potential) competing interest as Intel employees. 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In: Proceedings of the IEEE/CVF International Conference on Computer Vision Workshops. 2019, pp. 783–787."} {"paper_id": "prb44", "title": "Transparent and Reproducible AI-based Medical Imaging Pipelines Using the Cloud", "text": "Transparent and Reproducible AI-based Medical Imaging Pipelines Using the Cloud\n\nDennis Bontempi\nMass General Brigham | Harvard Medical School\n\nLeonard Nuernberg\nMass General Brigham | Harvard Medical School\n\nDeepa Krishnaswamy\nBrigham and Women's Hospital\n\nAhmed Hosny\nMass General Brigham | Harvard Medical School\n\nKeyvan Farahani\nNIH NCI\n\nRon Kikinis\nBrigham and Women's Hospital\n\nAndrey Fedorov\nSurgical Planning Laboratory, Brigham and Women's Hospital and Harvard Medical School, Harvard University\n\nHugo JWl Aerts\nHAerts@bwh.harvard.edu\n\nMass General Brigham | Harvard Medical School https://orcid.org/0000-0002-2122-2003\n\nArticle\n\nKeywords:\n\nPosted Date: July 21st, 2023\n\nDOI: https://doi.org/10.21203/rs.3.rs-3142996/v1\n\nLicense: © This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: There is NO Competing Interest.\nVersion of Record: A version of this preprint was published at Nature Communications on August 13th, 2024. See the published version at https://doi.org/10.1038/s41467-024-51202-2.\nTransparent and Reproducible AI-based Medical Imaging Pipelines Using the Cloud\n\nAuthors | Dennis Bontempi^{1,2,3}, Leonard Nuernberg^{1,2,3}, Deepa Krishnaswamy^{5}, Ahmed Hosny^{1,3}, Keyvan Farahani^{5}, Ron Kikinis^{5}, Andrey Fedorov^{5}, Hugo JWL Aerts^{1,2,3,4}\n\nAffiliations | ^1 Artificial Intelligence in Medicine (AIM) Program, Mass General Brigham, Harvard Medical School, Boston, United States of America. ^2 Radiology and Nuclear Medicine, CARIM & GROW, Maastricht University, Maastricht, The Netherlands.^3 Department of Radiation Oncology, Brigham and Women’s Hospital, Dana-Farber Cancer Institute, Harvard Medical School, Boston, United States of America. ^4 Department of Radiology, Brigham and Women’s Hospital, Harvard Medical School, Boston, United States of America.^5 National Heart, Lung, and Blood Institute and National Cancer Institute, Bethesda, Maryland\n\nRunning title | Cloud Empowers Reproducible AI Medical Imaging\n\nCorresponding author | Hugo Aerts, Ph.D. Director, Artificial Intelligence in Medicine (AIM) Program, Mass General Brigham, Harvard University, Harvard Institutes of Medicine – HIM 343, 77 Avenue Louis Pasteur, Boston, MA 02115. P - 617.525.7156, F - 617.582.6037, Email: haerts@bwh.harvard.edu\nSummary | Artificial intelligence (AI) algorithms hold the potential to revolutionize medical imaging. However, a significant portion of the published literature lacks transparency and reproducibility, which hampers sustained progress toward clinical translation. Although several reporting guidelines have been proposed, identifying practical means to address this issue remains challenging. Here, we discuss the potential of cloud-based infrastructures for implementing and sharing transparent and reproducible AI-based medical imaging pipelines. Starting from a published cancer imaging study investigating an AI biomarker for the prognostication of non-small cell lung cancer patients, we demonstrate end-to-end reproducibility of the research from retrieving cloud-hosted data, through data pre-processing, deep learning inference, and post-processing, to the analysis and reporting of the final results. By leveraging cloud-based platforms, using data hosted by the Imaging Data Commons (IDC) combined with code and compute resources, we make every step of the analysis and the resulting data easy to access, reproduce, and share. Our approach demonstrates the potential of cloud resources for implementing, sharing, and using reproducible and transparent AI pipelines in medical imaging, which can accelerate the translation into clinical solutions.\n\nIntroduction | Recent advances in artificial intelligence (AI) are helping to address many challenges in different medical areas, such as radiology, radiation oncology, and pathology¹⁻⁴. Several factors contributed to these notable AI breakthroughs, including the progressive increase in computational processing power driven by the development of specialized hardware, the recent advances in deep learning (DL) algorithms, the availability of widely used open-source DL platforms, and the ever-growing amount of publicly available data to train and validate AI models on. Nonetheless, the lack of transparency and reproducibility of published research, as well as processing pipelines, remains one of the biggest challenges faced by the field⁵. Recent literature⁶,⁷ suggest that as little as one-quarter of the AI studies share all the resources to replicate the findings as reported. Although this so-called reproducibility crisis is\nnot exclusive to AI8, the sheer complexity and black-box nature of DL algorithms, the large amount of data required to develop and validate models with millions of parameters, and the poor documentation and sharing of AI research5 substantially worsen the problem.\n\nTransparency and reproducibility are of utmost importance, particularly in the medical field, where errors may result in unpredictable and potentially untoward consequences. While AI can improve the efficiency and effectiveness of patient care,9 poor implementations can introduce significant biases, exacerbate health disparities10, and even lead to misdiagnoses and suboptimal treatments11,12. Inadequate efforts in making AI research reproducible will make performance claims very difficult to verify13, ultimately leading to inflated accuracy rates14 and generalizability problems15,16, hindering the translation of these systems to the clinic17. Furthermore, such a lack of reproducibility often impedes comparing performance across different AI tools.\n\nSeveral reporting guidelines, checklists, and standards have been proposed in recent years to tackle these issues in the medical imaging field18–24. These protocols aim to instruct scientists on the best practices in documenting their research and help them identify aspects of the AI-based analyses that should be reported in publications to ensure reproducibility. Moreover, community-driven efforts led to the creation of other resources, such as a registry of AI models developed for biomedical applications25 that researchers can use to report minimal attributes of these systems. While these efforts present authors with the rules to follow during the experimental design process and manuscript preparation, they do not provide a practical way to share AI-based pipelines with the community. Even if part of the code is shared, building the pipeline to reproduce the results reported in a study is often “left as an exercise for the reader.” Furthermore, these pipelines often need domain-specific tools, specific software versions, or hardware capability to be reproduced - or even run - as intended without encountering errors, with this information being regularly withheld from the reader. Therefore, without the accurate implementation of all the steps, any community attempt to expand on a study or to identify critical issues with (and failing conditions for) a pipeline\nremains practically impossible. Overall, in contrast to other research fields being transformed by technologies - e.g., genomics, where the MIAME guidelines\\(^{26}\\) and efforts like the NCI Genomics Data Commons have been instrumental in improving reproducibility by establishing standardized reporting and facilitating data sharing\\(^{27,28}\\) - the lack of reproducibility in AI research for medical imaging is significantly more widespread\\(^{29}\\).\n\nCloud-based resources can facilitate a solution to these issues and improve the reproducibility and scalability of AI studies by revolutionizing the way researchers access and use data in their studies. The use of cloud platforms can facilitate access to large-scale cancer imaging data while delivering a more streamlined and consistent computing environment to conduct experiments. Furthermore, by providing public access to data, software, and hardware, cloud-based resources can enable researchers to inspect all the components needed to replicate AI studies (see **Figure 1**), ultimately contributing to the growth and advancement of the field.\n\nIn this study, we discuss a cloud-based infrastructure for implementing and sharing end-to-end reproducible and transparent AI pipelines in medical imaging. On the basis of a representative use case, we show end-to-end replication of a published AI study developing and validating an algorithm to enable outcome prediction in patients with non-small cell lung cancer (NSCLC)\\(^{30}\\). By leveraging the National Cancer Institute’s (CRDC) Imaging Data Commons (IDC)\\(^{31}\\) component for data and the Google Cloud Platform (GCP) component for code and computing, each step within the AI pipeline - from data fetching and pre-processing, deep learning inference, data post-processing, and the analysis of the final results - can be examined and reproduced. Our approach demonstrates the potential of cloud-based resources for implementing, sharing, and using reproducible and transparent AI pipelines, which can accelerate the translation of AI algorithms into the clinic.\n\n**Main text |** Here, we illustrate a general cloud-based workflow for medical imaging AI using the approach proposed in **Figure 2**. The Imaging Data Commons (IDC) can accelerate\nresearch by centralizing and providing easy access to a wide range of standardized medical imaging data. The cloud-based platform enables validation of medical imaging use cases using public datasets by allowing users to create cohorts of imaging study and image-derived data based on DICOM metadata. Furthermore, since IDC supports data versioning, the specific cohorts remain accessible at any point in time, ensuring long-term preservation and accessibility of imaging data for reproducibility and future research while helping to associate a set of processing results with a specific cohort version.\n\nCloud-based AI Pipelines can be implemented using computing infrastructures such as Google Colaboratory, among others. These cloud-based services provide users with a Jupyter Notebook environment for writing and running Python code alongside markdown annotation from a web browser - enabling researchers to easily share minimal working examples or full-fledged analyses, ensuring that others can replicate their findings accurately. Notebooks are especially suited to bolster transparency and reproducibility, as they allow for the integration of text, visualizations, and code in a single document, facilitating precise and comprehensive communication of the tools used, the inner workings of the data preparation and processing pipeline, and the research findings. Moreover, their procedural structure makes it easier for new users to comprehend and follow the pipeline workflow and eliminate the need for users to set up their own runtime environment. Finally, their integration with platforms like GitHub streamlines the development and collaboration process.\n\nCloud-based infrastructure also provides researchers with simplified access to analyses and methods, increasing the reliability and validity of research findings and boosting confidence in reported results. Tools like Google Colaboratory offer descriptive text and interactive visualizations alongside code, creating an ideal data exploration and analysis environment, especially for complex pipelines. The consistent computing environment and access to predetermined resources also ensure transparency in the reporting process concerning computational costs.\nTo demonstrate the proposed approach, we implemented a case study related to cancer imaging. We selected one of the field's first and most cited studies, presenting an innovative approach showing how convolutional neural networks (CNN) could be used to help improve lung cancer patient stratification\\(^{30}\\). In this investigation, the authors used both clinical and imaging data (standard-of-care computed tomography (CT) scans) from diverse cohorts of non-small cell lung cancer (NSCLC) imaging studies to assess the performance of deep learning for lung cancer prognostication, comparing the latter to conventional prognostic factors and other machine learning methodologies such as radiomics. This comparison was carried out using several metrics and survival analysis tools, such as the area under the receiver operating characteristic (ROC) curve (AUC) and Kaplan-Meier analysis, with the study concluding that deep learning techniques could provide valuable insights into lung cancer prognosis and potentially assist in personalized treatment decisions. The researchers trained a CNN for predicting outcomes by analyzing tumor lesions on CT images and shared the model with the original investigation, together with the AI-derived prognostic scores for the patients analyzed in the study. Although the authors shared an open-source implementation of the algorithm, the trained model weights, the code to run inference using the latter, and a written description of how to prepare data for inference, the data pre-processing component was not included, leaving the users with no alternative but to implement the missing pieces themselves – a step that, as thoroughly investigated, can substantially change the result of computational pipelines when ill-executed\\(^{5,32-34}\\). Besides its impact on the field, another reason we chose this study for our use case was the fact that the AI pipeline was validated using an independent cohort now hosted by the IDC, i.e., the NSCLC-Radiomics dataset\\(^{35}\\), allowing us to use the platform to reproduce the AI pipeline validation.\n\nWe re-implemented the AI workflow using Google Colaboratory, sharing additional resources researchers can use to replicate and build upon the study and highlighting how the cloud-based infrastructure addresses the previously mentioned issues related to transparency and reproducibility. We provide an overview of the re-implementation in **Figure 3**. We used\nthe IDC platform to define a data cohort matching the subset of the NSCLC-Radiomics dataset used in the original publication. By querying the accompanying metadata curated in IDC tables using SQL, we retrieved the necessary imaging data for the cohort in a transparent and reproducible manner. We make the query to generate the imaging data cohort (and its result) publicly available within the notebooks, together with a description of the procedure used to select the validation cohorts for our study. The resources we share also describe the details and provide an example of how to run the queries to generate the validation cohort. This makes it easier for others to replicate or extend the study by referring to the versioned IDC cohort.\n\nFollowing the textual description provided by the authors, we implemented a pre-processing pipeline for converting the imaging data retrieved from IDC to a format suited for the deep-learning pipeline, relying exclusively on well-adopted open-source tools regarded as robust by the imaging community\\(^{36,37}\\). These software tools are packaged and versioned and can thus be recovered and installed at any point in time. To promote forward compatibility, we also converted the original model weights in the open neural network exchange (ONNX)\\(^{38}\\). We make the code for the model conversion and additional details available as part of our project repository, together with a notebook that incorporates a comprehensive description of every step of the replication process to help users navigate the complexity of the pipeline. Finally, we share a notebook with the code used to generate the results we present in this publication\\(^{39}\\).\n\nIn order to replicate the tumor lesion analysis with the model by Hosny et Al., we used expert segmentations included in the NSCLC-Radiomics collection, also hosted by IDC. As these masks are a newer iteration of the set of labels used for the original publication, we anticipated differences in the results. As reported in **Figure 3b**, the AUC of the original pipeline, computed on the cohort of N=206 subjects, was AUC=0.7, while the replicated pipeline scored AUC=0.68. After testing with various statistical tools, we observed that the difference between the results produced by the pipeline originally published by Hosny et Al.\nand those generated by our pipeline are not statistically significant (two-sided Mann-Whitney U test p>0.05, N=206; DeLong test for correlated (paired) AUC curves p>0.05, N=206). Therefore, we can conclude that the discrepancy between the two predictive models is negligible. These results also prove the model's robustness to variation in the input segmentation mask, as the original work claims.\n\nFurthermore, we conducted a Kaplan-Meier analysis, as done in the original publication, to assess the stratification power of the AI pipeline. We found that both the original pipeline and the replicated pipeline can successfully stratify higher-risk patients from lower-risk patients (p<0.001 and p=0.023, for the original and the replicated pipeline, respectively; see Figure 3b) when the risk-score threshold shared with the original publication is used to compute the split. In the project repository, we share a notebook for the visualization, exploration, and interpretation of the results of this analysis. The users can use this notebook to replicate the quantitative findings resulting from the comparison of the two AI pipelines and to investigate all the details of our analyses39. Finally, the resources we provide can be easily extended to run the same analysis on any other collection hosted on the Imaging Data Commons, provided the dataset contains imaging data suited to the AI pipeline.\n\nDiscussion | In this paper, we showcased the potential of cloud-based infrastructures for implementing and sharing transparent and reproducible AI-based medical imaging pipelines. We demonstrated how cloud-based resources offer potential solutions to issues surrounding the reproducibility of AI studies by providing a consistent computing environment, simplifying data exploration and access, and enabling the storage and sharing of code and results. We highlighted how the IDC and the GCP offer easily accessible cloud-based data resources that facilitate the implementation and sharing of fully reproducible AI pipelines in medical imaging. This, paired with cloud-based resources like Google Colaboratory, makes sharing minimal working examples (MWE) of processing pipelines or full-fledged analyses feasible, enabling others to replicate findings correctly while promoting best practices and strategies for data\nharmonization. We demonstrated that the proposed cloud-based infrastructure supports the replication of published AI literature.\n\nWhile cloud-based infrastructure facilitates potential solutions to issues surrounding the reproducibility of AI studies, its adoption also comes with several challenges, the biggest of which is the learning curve for the user unaccustomed to the different interacting blocks and tools. Furthermore, as the value of cloud-based data resources increases with the amount of data hosted by such platforms, any friction in the growth of such resources might constitute a hurdle in the way of their adoption. In the case of platforms such as the IDC, this process may constitute a challenge for a number of users, as additional steps for anonymization and institutional approval may be required to dismiss security and privacy concerns regarding the sharing of protected health information data like medical imaging and the associated clinical data. Nevertheless, the cloud represents a significant advantage for researchers who may not have access to in-house data (or cannot generate data at the same scale as cloud-based data resources) and can help overcome system limitations often encountered in large-scale research studies.\n\nAs previously mentioned, one of the benefits of cloud computing is easy and ubiquitous access to a computational environment that requires no experience to be set up and maintained, which researchers can leverage without upfront investments in hardware or infrastructure. While this can be particularly advantageous for small research teams or individuals who may not have access to powerful computing resources, using cloud computing can lead to dependence on third-party providers, which can be a concern for researchers who may need to access resources and data in the long term. Cloud computing providers may change their pricing models or even discontinue services, which could disrupt the research workflow. Additionally, cloud computing may limit the control and flexibility of the user in some regards. For example, researchers may be limited in using obsolete code that requires specific hardware or software - although this problem is not limited to cloud resources but can easily extend to local computational clusters. Furthermore, cloud providers might update these\ncomponents without appropriately informing the users, resulting in the disruption, or even failure, of the previously developed pipelines. Cloud computing may not always be the most cost-efficient solution for all use cases, particularly for long-term or high-usage applications.\n\nFinally, while adopting cloud technologies can greatly benefit the medical AI research community, it requires researchers to learn new skills and adapt to a new computing environment. The learning curve can vary depending on a researcher's background and familiarity with cloud computing, and it typically involves gaining an understanding of cloud infrastructure and services and learning how to use cloud-based tools for data storage, processing, and analysis. However, many cloud providers and cloud resources (such as Google Colaboratory, GCP, the CRDC, and IDC) offer comprehensive documentation, training material, and access to a growing community of practitioners to provide guidance and support. With time and practice, the use of cloud technologies can become second nature for researchers, enabling them to take full advantage of the benefits of cloud computing in medical AI research.\n\nIn summary, cloud computing offers several advantages for reproducibility in AI research, including democratizing access to large standardized datasets and to free to use, easily accessible, consistent computational environments. There still are essential factors to consider when using cloud computing in AI research, often cost-related - but we believe embracing cloud technology could reduce its costs and ultimately yield the providers of cloud computing resources to develop more customized and cost-effective solutions for the medical image analysis research community. Finally, the long-term cost savings of cloud adoption span beyond direct infrastructure and computing expenses. By enabling greater collaboration and data sharing, cloud technology can accelerate medical AI research and the development of more accurate, effective, and personalized clinical tools. This underscores the compelling case for embracing cloud technology in medical AI research.\nDATA AND CODE AVAILABILITY\n\nAll of the pipeline components are versioned and can be run and accessed in the cloud.\n\nThe version of the NSCLC-Radiomics dataset used for the study can be explored and obtained from the Imaging Data Commons platform (https://portal.imaging.datacommons.cancer.gov).\n\nThe codebase and the relative documentation can be accessed at the project repository https://github.com/ImagingDataCommons/idc-radiomics-reproducibility/releases/tag/v1.0.0 and referred to through Zenodo (https://zenodo.org/record/8073712; https://doi.org/10.5281/zenodo.8073712).\n\nThe cloud implementation of the pipeline can be accessed and run through the notebooks found at https://github.com/ImagingDataCommons/idc-radiomics-reproducibility/tree/main/notebooks:\n• The minimal working example of the cloud pipeline can be run at https://colab.research.google.com/github/ImagingDataCommons/idc-radiomics-reproducibility/blob/main/notebooks/processing_example.ipynb\n• The complete model validation cloud pipeline can be run at https://colab.research.google.com/github/ImagingDataCommons/idc-radiomics-reproducibility/blob/main/notebooks/complete_inference.ipynb\n• The results analysis, generating all of the plots used in the manuscript figures, can be run at https://colab.research.google.com/github/ImagingDataCommons/idc-radiomics-reproducibility/blob/main/notebooks/results_comparison.ipynb\n\nCOMPETING INTERESTS\n\nThe authors declare no other competing interests in this work.\n\nAUTHOR CONTRIBUTIONS\n\nStudy conceptualization: D.B., H.A., A.F.\nCode implementation and result analyses: D.B.\nWriting of the manuscript: D.B., L.N., H.A., A.F., D.K.\nCritical revision of the manuscript: All authors\nStudy supervision: H.A., A.F.\nReferences\n\n1. 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F., Arganda-Carreras, I., Henriques, R. & Jacquemet, G. Avoiding a replication crisis in deep-learning-based bioimage analysis. Nat. Methods **18**, 1136–1144 (2021).\n\n22. Varoquaux, G. & Cheplygina, V. Machine learning for medical imaging: methodological failures and recommendations for the future. NPJ Digit Med **5**, 48 (2022).\n\n23. Gottesman, O. et al. Guidelines for reinforcement learning in healthcare. Nat. Med. **25**, 16–18 (2019).\n\n24. Mongan, J., Moy, L. & Kahn, C. E., Jr. Checklist for Artificial Intelligence in Medical Imaging (CLAIM): A Guide for Authors and Reviewers. Radiol Artif Intell **2**, e200029 (2020).\n\n25. Matschinske, J. et al. The AlMe registry for artificial intelligence in biomedical research. Nat. Methods (2021) doi:10.1038/s41592-021-01241-0.\n\n26. Brazma, A. et al. Minimum information about a microarray experiment (MIAME)-toward standards for microarray data. Nat. Genet. **29**, 365–371 (2001).\n\n27. Grossman, R. L. et al. Toward a Shared Vision for Cancer Genomic Data. N. Engl. J. Med. **375**, 1109–1112 (2016).\n\n28. Zhang, Z. et al. Uniform genomic data analysis in the NCI Genomic Data Commons. Nat. Commun. **12**, 1226 (2021).\n29. McDermott, M. B. A. et al. Reproducibility in machine learning for health research: Still a ways to go. Sci. Transl. Med. **13**, (2021).\n\n30. Hosny, A. et al. Deep learning for lung cancer prognostication: A retrospective multi-cohort radiomics study. *PLoS Med.* **15**, e1002711 (2018).\n\n31. Fedorov, A. et al. NCI Imaging Data Commons. *Cancer Res.* **81**, 4188–4193 (2021).\n\n32. Botvinik-Nezer, R. et al. Variability in the analysis of a single neuroimaging dataset by many teams. *Nature* **582**, 84–88 (2020).\n\n33. Moradmand, H., Aghamiri, S. M. R. & Ghaderi, R. Impact of image preprocessing methods on reproducibility of radiomic features in multimodal magnetic resonance imaging in glioblastoma. *J. Appl. Clin. Med. Phys.* **21**, 179–190 (2020).\n\n34. 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(2023). doi:10.5281/zenodo.8073712.\nFigure 1 | Potential of cloud-based resources for reproducible AI research. Cloud-based infrastructures offer solutions to challenges related to reproducibility by providing access to large standardized datasets, resources for data exploration, and standardized environments for code and hardware. Cloud-based resources can simplify data exploration by enabling researchers to explore data easily and overcome system limitations often encountered in local research studies. Cloud-based infrastructures can also facilitate storing and sharing code and results, promoting researchers to reproduce and verify results. Finally, cloud-based computational infrastructures offer a uniform environment, equipped with pre-built libraries and tools, for researchers to conduct their experiments more transparently and reproducibly.\nFigure 2 | Cloud-based workflow for medical imaging AI. Our proposed approach combines open-source components, commercially available tools, and infrastructure being established by the US National Cancer Institute (NCI) to implement reproducible image analysis workflows and simplify their external/independent evaluation. We propose using the NCI Imaging Data Commons (IDC) as the persistent location of public imaging data, ensuring that data is available for public use, harmonized, and can be accessed in a standardized fashion. To facilitate computational workflows, we propose using components from the Google Cloud Platform to provision preconfigured GPU-enabled resources for the execution of AI pipelines. To promote transparency and reproducibility, we propose the use of Google Colaboratory to evaluate the results of the AI pipeline; by providing a ready-to-use, cloud-based Jupyter Notebook environment, this eliminates the need for local software installation and configuration, allowing for easier verification and sharing of the results. The combination of these different tools ensures an easily accessible end-to-end pipeline that can be inspected and easily referenced in all of its components.\nFigure 3 | Cloud-based re-implementation of a published study. a) We demonstrate our proposed approach by re-implementing a cancer imaging analysis pipeline from Hosny et al. (PLOS Medicine, 2018) using cloud-based infrastructure. We obtained the data from the Imaging Data Commons and used Google Colab for computation, showcasing the benefits of our proposed cloud-based infrastructure for improving transparency and reproducibility. By leveraging the cloud, we are able to share every step of the pipeline with the community, from data fetching to the reporting of results, enabling researchers to easily verify, replicate and build upon the study. To provide a practical example of how the proposed approach can be useful for bolstering transparency and reproducibility, b) we compared our cloud-based pipeline with the original results shared by Hosny et Al. on a subset of the NSCLC-Radiomics dataset, which is made easily accessible thanks to the functionalities of the IDC platform. We found no statistically significant difference in the area under the curve (AUC), and we observed that the split based on Hosny et Al. AI risk score is still significant and able to stratify patients at higher risk. All the replication steps, including the code to generate this figure, are shared publicly at the project repository and can be accessed and run for free on the cloud."} {"paper_id": "prb45", "title": "Molecular simulations of enzymatic phosphorylation of disordered proteins and their condensates", "text": "Molecular simulations of enzymatic phosphorylation of disordered proteins and their condensates\n\nLukas Stelzl\nlstelzl@uni-mainz.de\n\nJohannes Gutenberg University Mainz https://orcid.org/0000-0002-5348-0277\nEmanuele Zippo\nJohannes Gutenberg University Mainz https://orcid.org/0009-0002-5623-3471\nDorothee Dormann\nMainz University https://orcid.org/0000-0002-9260-2775\nThomas Speck\nUniversity of Stuttgart\n\nArticle\n\nKeywords:\n\nPosted Date: September 25th, 2024\n\nDOI: https://doi.org/10.21203/rs.3.rs-5084780/v1\n\nLicense: © This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: There is NO Competing Interest.\n\nVersion of Record: A version of this preprint was published at Nature Communications on May 19th, 2025. See the published version at https://doi.org/10.1038/s41467-025-59676-4.\nMolecular simulations of enzymatic phosphorylation of disordered proteins and their condensates\n\nEmanuele Zippo1,2, Dorothee Dormann2,3, Thomas Speck4, Lukas S. Stelzl2,3,5\n\n1 Institute of Physics, Johannes Gutenberg University Mainz, Germany\n2 Institute of molecular Physiology (ImP), Johannes Gutenberg University Mainz, Germany\n3 Institute of Molecular Biology (IMB), Mainz, Germany\n4 Institute for Theoretical Physics IV, University of Stuttgart, Germany\n5 KOMET1, Institute of Physics, Johannes Gutenberg University Mainz, Germany\n\nAbstract\n\nUnderstanding the condensation and aggregation of intrinsically disordered proteins in a non-equilibrium environment is crucial for unraveling many biological processes. Active enzymes catalyse many processes by consuming chemical fuels such as ATP. Enzymes called kinases phosphorylate disordered regions of proteins and thus profoundly affect their properties and interactions. Protein phosphorylation is implicated in neurodegenerative diseases and may modulate pathogenesis. However, how protein sequence and molecular recognition of a disordered protein by kinases determine phosphorylation patterns is not understood. In principle, molecular dynamics simulations hold the promise to resolve how phosphorylation affects disordered proteins and their assemblies. In practice, chemically-detailed simulations of enzymatic reactions and the dynamics of enzymes are highly challenging, in particular it is difficult to verify whether implementations of driven simulations are thermodynamically consistent. We can now address this problem with residue-level coarse-grained molecular dynamics simulations, integrating Metropolis Monte Carlo steps to model chemical reactions. Importantly, we show how to verify by Markov-state modeling that the realisation of a non-equilibrium steady state satisfies local-detailed balance. We investigate TDP-43 phosphorylation by the kinase CK1δ in simulations, examining patterns of phosphorylation and assessing its preventive role in chain aggregation, which may be a cytoprotective mechanism in neurodegenerative diseases. We find that the degree of residue phosphorylation is determined by sequence preference and charges, rather than by the position in the chain. The phosphorylation frequency is also affected by the phosphorylation patterns, since the interactions between CK1δ and TDP-43 actively change after each reaction. For TDP-43, our simulations show condensates dissolution through phosphorylation with kinases binding to the condensates and phosphorylating TDP-43 in the condensates.\nIntroduction\n\nBiological systems operate far from equilibrium[1]. The functionalities of cells and of their organelles and compartments are possible only through a very precise self-organization, driven by a continuous injection of energy from the external environment [2]. In the cell, chemical energy is stored, e.g. in the form of ATP molecules among others[3]. This energy is then used to synthesize and degrade molecules through biological cycles. On time scales shorter than physiological changes, microscopic rates are approximately constant and the system enters a non-equilibrium steady states (NESS)[3]-[5].\n\nCellular compartmentalisation underpinning biological function is achieved not only by lipid membranes and organelles surrounded by such membranes, but also by phase separation of proteins, giving rise to biomolecular condensates[6]. Membrane-less compartments of phase-separated proteins can concentrate or exclude molecules and thus organize biochemical processes in time and space, which is analogous to the compartmentalisation provided by lipid membranes. These phase-separated condensates can often act as chemical reactions organizers[7]. However, these condensates of proteins can also age into solid aggregates, which are believed to contribute to neuronal dysfunction and neurodegeneration[8][9]. As condensates age and become less liquid-like, they frequently lose their biochemical functionalities[10]. Aggregates of intrinsically disordered proteins (IDPs) are often linked to neurodegenerative diseases. Some examples are Tau protein aggregates, associated with Alzheimer’s disease[11], α-synuclein aggregates, associated with Parkinson’s disease[12], or TAR DNA-binding protein 43 (TDP-43) aggregates, mostly found in patients with amyotrophic lateral sclerosis (ALS) [13], frontotemporal dementia [14], but also in many patients with Alzheimer’s disease [15].\n\nProteins within condensates can also undergo chemical reactions themselves [2], driving the system out of equilibrium by dissipating a biochemical fuel, such as ATP. The modification of those proteins by addition of chemical groups, such as phosphate groups, are referred to as post-translational modifications (PTMs). IDRs are not only essential in driving the condensation of proteins, but they are also prime targets of PTMs [16]. PTMs can drastically change the properties of individual proteins[17] and collectively of condensates [18], enhancing[11][19] or suppressing the condensation and aggregation of IDPs[20][21]. For instance, it has been shown that chemical reactions can stabilize the size of liquid droplets by suppressing Ostwald ripening [22][23].\n\nTo connect these advances in the understanding of active processes in condensates to the biological roles of proteins, it will be important to elucidate how ATP driven phosphorylation shapes the interactions of intrinsically disordered protein regions (IDRs) of neurodegeneration-linked proteins such as TDP-43. The disordered low-complexity domain (LCD) of TDP-43 is hyper-phosphorylated in disease, and in experiments such a hyper-phosphorylation has been found to suppress TDP-43 condensation and aggregation[24]. Enzymes can add PTMs to IDPs in dilute solution, but enzymatic addition of PTMs may also occur in protein condensates. Recently, it was shown that phase-separated condensates can speed up phosphorylation of Tau protein[25]. Phosphorylation of the TDP-43 C-terminal residues Ser 379, Ser 403, Ser 404, Ser 409, and Ser 410 in patient samples is associated with neurodegenerative disease[26]. TDP-43 is phosphorylated by Casein kinase 1δ (CK1δ). How the enzymatic phosphorylation of TDP-43 is modulated in dilute solution and how it is affected by protein condensates is not known. The disordered tail of CK1δ is auto-inhibitory[27][28], but how it inhibits TDP-43 phosphorylation is unclear on the molecular scale. IDRs of enzymes have multiple functions, such as auto-inhibition by binding to the active site. IDRs are involved in substrate binding, for instance IDRs can speed up reactions via fly casting effect, where the IDR\nFigure 1: Enzymatic phosphorylation cycle driven by the consumption of the chemical fuel ATP. In state **1** TDP-43 (grey) is unphosphorylated and is not bound to the kinase CK1δ (blue, active site in pink). In state **2** TDP-43 binds to CK1δ. In state **3** the reactive serine is phosphorylated by kinase, converting one ATP into one ADP. In state **4** phosphorylated TDP-43 dissociates from CK1δ. Phosphorylated and unphosphorylated TDP-43 are supplied through reservoirs and we consider exchanges between these reservoirs and our simulation box. Serines are colored in yellow, while phospho-serines in red.\n\nincreases the search volume for the binding of partner proteins[29].\n\nPhase behaviour of intrinsically disordered proteins (IDPs) and the biological functionalities of protein condensates have been studied in the past years using multi-scale molecular dynamics (MD) simulations. Such simulations capture the spontaneous condensation of hundreds or more proteins while maintaining enough chemical detail in the simulations to elucidate sequence-specific interactions of proteins[24][30]. Comparison to more highly-resolved coarse-grained methods [30]-[34] or atomistic molecular simulations [35][36] can then highlight important drivers of protein condensation[24].\n\nHowever most of these studies assume thermodynamic equilibrium, neglecting the dynamical changes in the properties of individual proteins and protein condensates, as well as the dissipation caused by chemical fluxes. Much progress has already been made in the simulations of mechanically-driven non-equilibrium steady state (NESS), where external mechanical forces give rise to driven dynamics [37]. An important step was the construction of Markov state models to better understand the effects of driving on the molecular scale[38]. Analogously, a biological chemically-driven NESS, such as molecular motors, can be simulated by maintaining a chemical potential difference, i.e. by fixing the ATP to ADP concentration ratio. [4][39] Chemical reactions could in principle also be modelled via quantum mechanical approaches[40], but these are computationally very demand-\ning, which can preclude their application to large-scales dynamics in complex biochemical systems. Recently, exciting progress has been made in integrating chemical reactions in molecular dynamics simulations via neural networks[41]. Even in the case of coarse-grained simulations, chemical reactions have been modelled through the use of reactive beads that can form bonds between molecules [42]. In many cases, one could model chemical reactions in complex system by combining MD with a suitably chosen Monte Carlo (MC) step [39] [43]. Arguably, the absence of a straightforward approach of validating the thermodynamic consistency of simulations of NESS has held back the widespread application of MD/MC approaches to biochemical reactions on the molecular scale.\n\nHere we demonstrate how to validate the thermodynamic consistency of simulations of enzymatic phosphorylation of proteins using TDP-43 LCD and its phosphorylation by CK1δ as an example. We do so by constructing a Markov state model (MSM), which is a generally applicable approach. Our coarse-grained simulations of enzymatic phosphorylation of TDP-43, show how the sequence specific interactions of CK1δ with TDP-43 LCD affects the phosphorylation frequency of serines residues in the TDP-43 LCD in dilute solution and in condensates. In particular the C-terminal domain is more phosphorylated than the N-terminus, in agreement with experiments. Indeed, multiple serines of TDP-43 LCD have been found phosphorylated in patient samples, in particular in the C-terminal region[44, 45], with Ser 409/Ser 410 phosphorylation being established as a hallmark of TDP-43 pathology in disease [26] and detected, together with Ser 403/Ser 404 and Ser 379, by phospho-specific antibodies[16]. The phosphorylation frequency is also affected by the phosphorylation patterns, since the interactions between CK1δ and TDP-43 actively change after each reaction, enhancing further phosphorylations[47]. Moreover we study the role of the CK1δ IDR (residues from 295 to 415) in phosphorylating TDP-43 both in condensate and dilute regime. CK1δ IDR strongly interacts with TDP-43 LCD, reducing its contacts with active site of the enzyme in dilute regime. In dense regime, the CK1δ tail anchors of the enzyme to the droplet surface.\n\nResults\n\nMarkov-state modeling demonstrates thermodynamic consistency of simulations of chemically-driven dynamics\n\nMolecular dynamics (MD) simulations together with a thermostat holding the temperature fixed can be employed to sample from the canonical equilibrium distribution. However, introducing phosphorylation reactions in MD simulations generally inject energy into the system, thus breaking detailed balance and displacing the system away from thermal equilibrium. We simulate the action of the kinase CK1δ (truncated at residue 294 for the purposes of this section) on the substrate protein TDP-43 by combining one-bead-per-residue implicit-solvent MD with MC phosphorylation steps and validate the thermodynamic consistency of our simulations by making use of Markov state models (MSMs). We assume that only the serines (Ser) of TDP-43 LCD can be phosphorylated into phospho-serines (pSer). The phosphorylation reaction is the following:\n\n\\[\n\\text{Ser} + \\text{ATP} \\rightleftharpoons \\text{pSer} + \\text{ADP}\n\\]\n\n(1)\n\nWhenever a Ser (or pSer) is in contact with the active site of the kinase, we try to swap it with a pSer (or the opposite) with acceptance probability given by\n\n\\[\nA(\\text{Ser}, \\text{pSer}) = \\min \\left(1, \\exp(-\\beta \\Delta U_P - \\beta \\Delta \\mu_P)\\right)\n\\]\n\n(2)\nFigure 2: Thermodynamic consistency of simulations with phosphorylation step using MSMs. (a) Example of trajectory of the distance between Ser 403 of TDP-43 LCD and the active site of CK1δ for the simulation at \\( \\Delta \\mu_P = -5 \\) kJ/mol. In red the two output states of the neural network (bound and unbound) with respective illustrative examples on the right. (b) Example of discretized 4-state MSM trajectory related to the trajectory in a, we highlight complete cycles in red. (c) Example of implied timescales from the 4-state MSM trajectory shown in b; they remain stable for \\( \\tau \\gtrsim 10^5 \\) MD steps (10 Markov chain steps). (d) Example of Chapman-Kolmogorov test from the 4-state MSM trajectory shown in b; prediction and model are in agreement. (e) We plot \\( \\Delta \\mu_{cycle} \\) vs \\( \\Delta \\mu_P \\); for all the six different phosphorylation sites, the chemical potential computed from Eq. [3] matches the applied chemical potential \\( \\Delta \\mu_P \\). Errorbars on \\( \\Delta \\mu_{cycle} \\) are obtained via bootstrapping of the total simulation trajectory collected.\n\nwhere \\( \\beta = 1/(k_B T) \\), \\( \\Delta U_P \\) is the difference between the potential energy of the configuration with pSer and the one of the configuration with Ser, and \\( \\Delta \\mu_P \\) is the chemical potential difference between the ATP and ADP molecules involved in the phosphorylation reaction (Eq. 1). ATP and ADP are modelled implicitly and are not explicitly simulated, with concentrations kept fixed and fully characterized through the choice of \\( \\Delta \\mu_P \\). Indeed biological reactions, such as the phosphorylation\nreaction, in living cells happen in open systems in which the concentrations of substrates, products and the chemical fuel are kept approximately constant over relevant timescales by e.g. metabolic processes. A non-zero value of \\( \\Delta \\mu_P \\) biases the chemical reaction, pushing the simulation away from thermodynamic equilibrium.\n\nThe first step is to validate the thermodynamic consistency of our simulations by showing that the energy gain in a phosphorylation cycle (referred to as \\( \\Delta \\mu_{cycle} \\) in the following) is equal to the chemical potential difference \\( \\Delta \\mu_P \\) in the phosphorylation step. In order to compute \\( \\Delta \\mu_{cycle} \\), we employ a discretization of the MD trajectory in a MSM. The simplest example of a phosphorylation cycle that we can build is a system with one enzyme and one substrate protein in which only one residue is reactive. In order to get complete phosphorylation cycles, we assume the exchange between TDP-43 and phosphorylated TDP-43 happens when substrate and enzyme are far away from each other without chemical driving and with equilibrium concentrations, through another MC step (Methods). This naturally happens in cells through the action of phosphatases that can catalyze a dephosphorylation reaction.\n\nTo gain insights into the effects of including phosphorylation through Eq. 2, we build an MSM from simulated MD trajectories. Firstly we distinguish between bound and unbound state using a neural network called VAMPnet [48]. VAMPnet is able to map molecular coordinates to Markov states through a score function called VAMP-2 score based on the Koopman’s theory. Finding the transformation of the input variables that maximizes the VAMP-2 score is equivalent to optimizing the Markovianity of the output states. In this way we can easily distinguish between the two slowest processes, binding and unbinding, without arbitrarily choosing an a priori criterion of contact. As input for the neural network, we use the 154 distances between each residue of TDP-43 LCD and the active site of CK1δ, while as output we ask for 2 states (ideally bound and unbound). We then filter spurious transitions using transition-based state assignment [49]. As an example, we show in Fig. 2a the trajectory of the distance between Ser 403 (the reactive residue) of TDP-43 LCD and the active site of CK1δ for the simulation at \\( \\Delta \\mu_P = -5 \\) kJ/mol (SI Movie 1). We can see that the two states predicted by the neural network comprise bound configurations (when the distance between Ser and CK1δ active site is smaller) and unbound configurations (when the distance is larger).\n\nBy distinguishing between Ser and pSer along the trajectory, we coarse-grain the system dynamics into the 4 states sketched in Fig. 1. Assuming that our system is a NESS, we can then compute the time-independent transition probabilities \\( T_{ij}(\\tau) \\) from state i to state j using the non-reversible Maximum Likelihood estimator [50], [51]. We report in Fig. 2b the resulting MSM discretized trajectory referred to the simulation in panel A. Complete cycles \\( 1 \\rightarrow 2 \\rightarrow 3 \\rightarrow 4 \\rightarrow 1 \\) are highlighted in red. Every step of the Markov chain corresponds to \\( 10^4 \\) MD steps, or 0.1 ns in simulation time. For all our simulations, we choose a lag time \\( \\tau = 10 \\) Markov chain steps (Methods). We show in Fig. 2c: the implied timescales for the example case of reactive Ser 403 and \\( \\Delta \\mu_P = -5 \\) kJ/mol. In the end, we estimate the goodness of the MSM by looking at the Chapman-Kolmogorov test (CK test) [52], [53]. In all the validation simulations, the CK tests suggest good agreement between model and prediction for a wide range of lag times, as shown in Fig. 2d for the example case of reactive Ser 403 and \\( \\Delta \\mu_{in} = -5 \\) kJ/mol (SI Table S1, Table S2, Fig. S1 for complete data, Methods).\n\nIf our system is a NESS, the local detailed balance condition must be satisfied [3], [5]:\n\n\\[\n\\Delta \\mu_{cycle} = -k_B T \\ln \\left( \\frac{T_{12}T_{23}T_{34}T_{41}}{T_{14}T_{43}T_{32}T_{21}} \\right)\n\\]\n\nwhere \\( \\Delta \\mu_{cycle} \\) is the energy injected into the system in one forward cycle \\( 1 \\rightarrow 2 \\rightarrow 3 \\rightarrow 4 \\rightarrow 1 \\). It\nis interesting to observe that the logarithm contains the ratio between the forward and backward transition probabilities. In many formulations, Eq. 3 is via rate coefficients rather than transition probabilities. For the short lag times considered here, we can estimate a rate matrix from the transition probability matrix and find virtually indistinguishable results for \\( \\Delta \\mu_{\\text{cycle}} \\) (SI Text). Since the transitions \\( 1 \\rightleftharpoons 2, 3 \\rightleftharpoons 4 \\) (the binding/unbinding of the enzyme with TDP-43 or phosphorylated TDP-43) and \\( 4 \\rightleftharpoons 1 \\) (the reservoir exchange step) satisfy detailed balance, while the phosphorylation reaction \\( 2 \\rightleftharpoons 3 \\) breaks detailed balance injecting into the system an amount of energy equal to \\( \\Delta \\mu_P \\), we expect \\( \\Delta \\mu_{\\text{cycle}} \\) to be equal to \\( \\Delta \\mu_P \\) (SI Text). We compute the estimated energy gain \\( \\Delta \\mu_{\\text{cycle}} \\) from the transition probabilities \\( T_{ij} \\) and plot them against the parameter \\( \\Delta \\mu_P \\) of the phosphorylation step for different reactive Ser and \\( \\Delta \\mu_P \\). Encouragingly, for all the six different phosphorylation sites, the chemical potential computed from Eq. 3 matches the applied chemical potential \\( \\Delta \\mu_P \\) (Fig. 2c).\n\nWe repeated the estimate of \\( \\Delta \\mu_{\\text{cycle}} \\) using a 3-states MSM, in which the unbound states 1 and 4 are merged into the new state 1. The results are in agreement with the 4-states MSM (SI Table S1, SI Fig. S1). Indeed, the transition between state 1 and 4 has a very high rate and can be associated with the smallest implied timescale, that is lower than the lag time for \\( \\tau = 10 \\) Markov chain steps or larger.\n\nWe also checked the reliability of VAMPnet by using considerably more input distances (4620 distances) and a different architecture for the case of reactive Ser 403 and \\( \\Delta \\mu_P = -5 \\) kJ/mol (Methods). The estimated \\( \\Delta \\mu_{\\text{cycle}} \\) with the new version of VAMPnet is \\( \\Delta \\mu_{\\text{cycle}} = 4.7 \\pm 0.6 \\) kJ/mol (implied timescales and CK test in SI Fig. S2).\n\nPhosphorylation preferences are determined by sequence-specific interactions\n\nHaving established a model of chemically-driven dynamics, we investigate how sequence context determines the phosphorylation of the disordered protein TDP-43 LCD by the enzyme CK1δ, so that we can begin to rationalize sequence-specificity of TDP-43 phosphorylation in experiments[24] and why C-terminal Ser residues such as Ser 410 are frequently found to be phosphorylated in experiments[24, 26, 44]. In our simulations, we follow directly the dynamics of TDP-43 LCD and CK1δ folded domain (truncated at residue 294) on the single molecule level (Fig. 3a). We run 100 simulations of TDP-43 LCD in presence of CK1δ and at physiological ATP/ADP ratio (\\( \\Delta \\mu_P = -48 \\) kJ/mol), which mimics in vitro kinase assays. In the simulations, unphosphorylated TDP-43 LCD will eventually encounter CK1δ and give rise to different phosphorylation patterns, as shown for an example simulation on Fig. 3b. In this simulation TDP-43 LCD is initially phosphorylated in the C-terminal region. The kinase dissociates after two phosphorylation events and then binds again to the substrate. Multiple Ser residues in the C-terminus of TDP-43 LCD are phosphorylated, including Ser 410, which gets phosphorylated after ten other residues. In our simulations, Ser residues towards the C-terminus of TDP-43 LCD (Ser 369 to Ser 410) are more readily phosphorylated than Ser residues in the N-terminal region of the LCD (Ser 266 to Ser 350), with the phosphorylation rate \\( r_P \\) on average roughly 3-4 times larger in the C-terminal segment than in the N-terminal segment (Fig. 3b). In mass spectrometry analysis of TDP-43 from ALS patient samples, the phosphorylated sites (the 12 residues Ser 373, Ser 375, Ser 379, Ser 387, Ser 389, Ser 393, Ser 395, Ser 403, Ser 404, Ser 407, Ser 409 and Ser 410 [24, 44] and also Ser 369 [45]) are mostly in the C-terminal region and, interestingly, they are among the ones with largest phosphorylation rate \\( r_P \\) in our simulations. In particular, Ser 409/Ser 410 phosphorylation has long\nFigure 3: Analyzing the sequence dependence in phosphorylation dynamics of TDP-43. (a) Example trajectory discretized in phosphorylation-states relative to Ser 410. np is the state with Ser 410 not phosphorylated and n other phosphorylated Ser, pS410 are all the states with phosphorylated Ser 410. (b) We compare the phosphorylation rates \\( r_p \\) for every Ser for the wild type TDP-43 (blue), the averaged-interaction sequence (orange) and the averaged-interaction with equally-spaced Ser (green). The C-terminal is more phosphorylated. The ticks on top show the position of the charged (red ‘+’ positive, blue ‘-’ negative) and aromatic (grey ‘a’) residues. (c) Same comparison for the rates of contact \\( r_c \\) between Ser residues of TDP-43 LCD and the active site of CK1δ in equilibrium simulations without phosphorylations. The positive charges in the N-terminal screen the interaction with the enzyme. Contact frequency are constant for the averaged-interaction sequence. (d) Correlation plot of contact frequency in equilibrium and phosphorylation rates for the wild type TDP-43. Ser 407 and Ser 410 have similar phosphorylation rate, but the probability of contact of Ser 410 is larger. (e) Probability \\( p(t(\\text{Ser}_i) < t(\\text{Ser}_j)) \\) of Ser_i being phosphorylated before Ser_j, data from 100 trajectories. C-terminal residues are much more likely to be phosphorylated before N-terminal residues. (f) Phosphorylation pattern representation for Ser 410. The thickness of the arrows represent the percentage of simulations in which Ser 410 was phosphorylated after n other Ser residues (e.g. 12% of simulations go from state 3p to pS410). We show in the inset some examples of 3p states.\n\nbeen established as a hallmark of TDP-43 pathology in disease [26]. This qualitative agreement with simulations tentatively suggests that sequence specific interactions of TDP-43 LCD with the CK1δ could explain why these residues are frequently found phosphorylated in experiments and in patient samples.\nThe differences in the phosphorylation rates can be largely accounted for by how readily Ser residues engage in contacts with the CK1δ active site (Fig. 3c), with the phosphorylation rates strongly correlated with a sample Pearson correlation coefficient of 0.84 (Fig. 3d). In order to compare the phosphorylation rates with the frequency of making contacts at equilibrium, we performed MD simulations of the same system without phosphorylation MC steps. To establish to what extent contacts predicts the relative phosphorylation rates, we consider a contact whenever all the three distances to residues Asp 149, Phe 150 and Gly 151 close to the active site are less than 1 nm, in the same way as for the MC phosphorylation step. By contrast, the acceptance probability for the phosphorylation MC step for Ser residues once they are in contact is > 0.97 for the entire sequence and the variations in the acceptance probability of the phosphorylation step are not correlated with the variation of the phosphorylation rates (SI Fig. S8). Ser residues in the C-terminal segment of the LCD, including Ser 369, Ser 393, Ser 395, Ser 403, and Ser 410, have the largest tendencies to form contacts, as tracked by \\( r_c \\), which is the rate at which a residue forms contacts with the CK1δ active site (Fig. 3c). At the same time these residues have within the statistical uncertainty the fastest phosphorylation rates of the TDP-43 LCD (Fig. 3b) . Ser residues in the N-terminal part of the LCD (Ser 266 to Ser 350) form fewer contacts than serines in the C-terminal segment (Ser 369 to Ser 410), with the exception of Ser 373 in the latter segment, which also forms few contacts with the active site of CK1δ. The N-terminus is enriched in charged amino acids (mostly positive) (Fig. 3a and c), which may hinder its binding to the CK1δ active site, since the active site features multiple charged residues and is overall positively charged (SI Fig. S7). On the other hand, the C-terminus has more aromatic residues, which increase the attraction through cation-pi and pi-pi interactions (Fig. 3b and c). This difference between the N- and C-terminal segments of the TDP-43 LCD is also apparent on the correlation plot in Fig. 3d, where the N-terminal residues have both low rates and low number of contacts, whereas the C-terminal residues have mostly high phosphorylation rates and many contacts with the active site.\n\nDynamics of TDP-43 serine phosphorylation is influenced by preceding phosphorylation events\n\nAlthough the correlation between the relative rates for CK1δ and TDP-43 contact formation and the phosphorylation rates is strong, there are deviations from the this simple relationship (Fig. 3d), which could hint at structural correlations and possible correlations between phosphorylation events. For instance, Ser 410 forms contacts more than two times more readily than Ser 407 but their phosphorylation rates are the same within the statistical uncertainty (Fig. 3b and Fig. 3c). To better understand the underlying correlations, we expanded our analysis of the phosphorylation kinetics. To estimate the phosphorylation rates \\( r_p \\), we assume that the phosphorylation process is a memory-less process, which follows single-exponential kinetics [55]. In this case, observing a single event is in principle sufficient to estimate the rates of a process. In addition to the number of events one observes, the time spent waiting before an event happens also contributes to the rate estimate. We checked the results by fitting the cumulative histograms of phosphorylation time for each Ser with a simple single-exponential process and an exponential process conditioned to another exponential process (e.g. the binding of TDP-43 to CK1δ) (Methods). Most of the times the conditioned exponential process fits perfectly. We found that the rate extrapolations from the two fits are in agreement with the Bayesian estimates (SI Fig. S9). It is interesting to notice that the fastest rate is different for every Ser (Ser 266 with a second rate coeffiecent of 13.5\\( \\mu s^{-1} \\) and Ser 393 of 56\\( \\mu s^{-1} \\)) suggesting that the phosphorylation of some serines could involve other\nprocesses than the binding to CK1δ, e.g. the previous phosphorylation of another Ser. For Ser 410, the two fit extrapolation and the single-exponential fit are in agreement, with differences in the phosphorylation rate of about 2% , while for Ser 403 the conditioned process fit leads to an 8% smaller rate compared to the single-exponential fit. For Ser 407, the conditioned process yields a 10% larger rate. These comparison suggests that the phosphorylation of Ser 403 and Ser 407 could actually follow a more complex process.\n\nWe determined the most likely order of phosphorylation to understand correlation between phosphorylation events and differences from what the contact statistics at equilibrium would predict better. In order to study more deeply the phosphorylation pattern of TDP-43, we count for each Ser couple (Ser_i, Ser_j) how many times Ser_i is phosphorylated before Ser_j by aggregating data from our 100 trajectories to compute the probability \\( p(t_P(\\text{Ser}_i) < t_P(\\text{Ser}_j)) \\), where \\( t_P(\\text{Ser}_i) \\) is the time of phosphorylation for Ser_i from the start of the simulation. We show \\( p(t_P(\\text{Ser}_i) < t_P(\\text{Ser}_j)) \\) as a heatmap in Fig. 3b. We see again that, on the single-molecule level, C-terminal residues are typically phosphorylated first. The lower right corner shows that on average C-terminal residues are much more likely to be phosphorylated before N-terminal residues and as a corollary, the upper left sub-matrix shows that C-terminal residues are rarely phosphorylated after N-terminal residues. Instead, looking at the lower left block, we see that Ser 266 and Ser 273 are usually the first phosphorylated in the N-terminal region, while the serines within residues 333 and 350 are the last ones. In the end, by focusing in the C-terminus on the upper right block, we see that the first phosphorylations occur on Ser 369, Ser 393, Ser 395, Ser 403 and Ser 410, followed by Ser between 377 and 389 and Ser 407. In Fig. 3c we aggregate the data from the different trajectories and illustrate the likelihood for Ser 410 of getting phosphorylated after n other Ser through the thickness of the arrows. In the figure, the state p$410 includes all the possible configurations in which Ser 410 is phosphorylated, while np are the configurations with n pSer different from Ser 410, as shown in the inset for four different examples of state 3p. Very often Ser 410 is among the first three residues to be phosphorylated. Only in a few trajectories, Ser 410 is phosphorylated after nine or eleven other Ser residues are already phosphorylated. Ser 395 shows similar behaviour to Ser 410 (SI Fig. S11). While Ser 403 and Ser 407 are also phosphorylated early on by this analysis, they are less frequently the first Ser residues to be phosphorylated compared to Ser 410 (SI Fig. S11), which is in line with the deviations from single-exponential behaviour (SI Fig. S9).\nA possible influence of prior phosphorylation can also be detected for Ser 373. Ser 373 forms few contacts but is readily phosphorylated. The phosphorylation rate of Ser 373 is just slightly lower than for Ser 375, which has twice as many contacts. Indeed Ser 369 engages in many more contacts and the rates are just slightly higher than for Ser 373 and Ser 375. Fig. 3e shows that the probability \\( p(t_P(\\text{Ser}_i) < t_P(\\text{Ser}_j)) \\) of Ser 369 to be phosphorylated before Ser 373 and Ser 375 is approximately 0.8 and 0.7. Fig. S11 (SI) demonstrates that Ser 373 and Ser 375 are phosphorylated when multiple Ser residues are already phosphorylated. Changes in the interaction of CK1δ with TDP-43 LCD as more residues are phosphorylated could explain why phosphorylation rates are not fully accounted for by the interaction propensities of the LCD with the active site of the enzyme. By analyzing long equilibrium MD simulations with VAMPnet[18], we find that the phosphorylation facilitates the binding of CK1δ to the substrate TDP-43 LCD, with the binding free energy going from 5.0 kJ/mol in the case of wild type TDP-43 LCD to 1.2 kJ/mol for a chain with pSer 395, pSer 403 and pSer 410 (SI Text). As a result, the first phosphorylation events speed up further phosphorylation events, in agreement to what suggested by experiments [17], and we find that, in the simulations of enzymatic phosphorylation of TDP-43, phosphorylated TDP-43 LCD stays attached to CK1δ (SI Fig. S3).\nPhosphorylation dynamics is determined by sequence context not relative position to N- and C-termini\n\nThe relative position of the Ser residues to the N- and C-termini does not affect the phosphorylation rates. It has been hypothesized that the tendency of C-terminal residues to get phosphorylated could be due to the greater accessibility of residues close to the N- and C-termini of a disordered protein chain [24]. In order to understand whether the phosphorylation pattern is affected by the position of the Ser residues along the TDP-43 LCD chain and not only by the neighboring residues, we repeated the same simulation but replacing all the residues of TDP-43 LCD different from Ser with an averaged interaction strength bead, 1) leaving the serines at their original positions and 2) spreading them equally spaced along the chain. From the contact frequency \\( r_c \\) in the lower panel in Fig. 3B, we can see that in equilibrium, before any phosphorylation occurs, the probability of contact is uniform along the chain, suggesting that the ends are not a priori more accessible and hence that sequence context and its effects on molecular recognition likely explain the prominence of C-terminal TDP-43 phosphorylation. By looking at the phosphorylation rates \\( r_P \\) (lower panel in Fig. 3B), we can see that the C-terminal domain is more phosphorylated in the case of simple averaged-interaction beads. We also computed the probability \\( p(t_P(\\text{Ser}_i) < t_P(\\text{Ser}_j)) \\) for the case of averaged-interaction chain (SI Fig. S10 left), which also demonstrated that the C-terminus is phosphorylated before the N-terminus. This suggests that the negative charges of the pSer also plays a role. These are denser in the C-terminus when TDP-43 gets hyper-phosphorylated. Indeed by distributing the Ser residues at equal distances, phosphorylation rates are constant within the statistical uncertainty. A similar behavior has already been found in experiments for the case of cyclin-dependent kinases phosphorylation of multisite targets[56]. Overall, the phosphorylation rates, as well as the contact frequency in equilibrium, are one order of magnitude smaller in the case of averaged interaction sequence compared to the wild type TDP-43, highlighting once more the importance of the sequence context.\n\nCK1δ binds to TDP-43 condensates and dissolves condensates by hyper-phosphorylation\n\nIn our simulations, CK1δ folded domain binds to TDP-43 LCD condensates and the LCD condensates dissolve when they are hyper-phosphorylated (Fig. 4A). In cells, TDP-43 often phase-separates into liquid-like droplets which has been linked to the formation of toxic aggregates. Recent experiments have shown that hyper-phosphorylation of TDP-43 LCD can prevent phase separation and aggregation by increasing the solubility of TDP-43 [24]. However it remains unclear whether kinases, such as CK1δ, actually bind to TDP-43 condensates, or only phosphorylate TDP-43 in dilute solution. Snapshots from an example simulation with five CK1δ enzymes are shown in Fig. 4A (SI Movie 3), with the first snapshot depicting the starting configuration with 200 TDP-43 chains phase-separated in a condensate and the enzymes (blue molecules) randomly placed in the box. After 1 \\( \\mu s \\) of simulation time the enzymes are all attached at the surface of the condensate and they are in the process of phosphorylating several serine residues (pSer in red). Hyper-phosphorylated TDP-43 chains start to disassociate from the condensate, which appears almost entirely dissolved after 5 \\( \\mu s \\) of simulation time in the last snapshot. We report in Fig. 4B the percentage of chains in the condensate (blue, left y-axis) and the percentage of phosphorylated Ser (red, right y-axis) over time from simulations with 1,3 and 5 enzymes, averaged over 4 independent replicas. The percentage of TDP-43 chains in condensate drops over time as the phosphorylation count increases.\nFigure 4: Analyzing the effect of hyper-phosphorylation of a TDP-43 LCD condensate and the interaction of CK1δ with the condensate. All the simulations involved in the plots are performed in a cubic box of 100 nm side length with 200 TDP-43 LCD chains. (a) Snapshots from simulation with 5 CK1δ in cubic box of 100 nm side length at times 0,1,3 and 5 \\( \\mu s \\) showing the dissolution of the TDP-43 condensate. The enzymes are colored in blue and the phospho-serine in red. (b) Percentage of TDP-43 chains in the condensate (blue, left y-axis) and percentage of phosphorylated Ser (red, right y-axis) in time for simulations with 1,3 and 5 CK1δ. The condensate starts to dissolve after about 24 % pSer. (c) Percentage of CK1δ attached to the condensate (blue, left y-axis) and percentage of phosphorylated Ser (red, right y-axis) in time for simulations with 1,3 and 5 CK1δ. The enzymes remain attached to the condensate after some phosphorylations. (d) Percentage of CK1δ attached to the condensate in time for equilibrium simulations without phosphorylation with 1,3 and 5 CK1δ. In absence of pSer, only about 35% of the enzymes stay attached to the condensate in average. (e) Comparison of phosphorylation rates \\( r_P \\) for every Ser of TDP-43 LCD divided by the number of CK1δ chains in dilute regime (grey) and in condensate in presence of 1,3 and 5 enzymes. In dense regime, phosphorylation of the ends of TDP-43 LCD is enhanced. The ticks on top show the position of the charged (red ‘+’ positive, blue ‘-’ negative) and aromatic (grey ‘a’) residues. (f) Contact rates \\( r_c \\) for every Ser of TDP-43 LCD divided by the number of CK1δ chains in dilute regime (grey) and in condensate in presence of 1,3 and 5 enzymes at equilibrium.\n\nWe computed the size of the condensate using a standard clustering analysis algorithm, thanks to which we were able to distinguish the chains in the larger condensate at every frame (Methods). In every simulation, the condensate starts to lose TDP-43 chains when about 24-25% of Ser are phosphorylated. As a result, the speed of phosphorylation decreases with time, as the TDP-43 chains start to migrate in the dilute regime, far from the action of the enzymes. This effect is\nparticularly evident in the case of 5 CK1δ after about 3.5 \\( \\mu s \\). It is interesting to notice that the speed of phosphorylation decreases slightly with time even before the beginning of the dissolution, with C-terminal Ser being the most affected (SI Fig. S5 upper panel). The slowing down of the phosphorylation rates of the most accessible Ser suggests a possible saturation effect. Moreover, we notice that, at least after about 5% of Ser are phosphorylated, most of the TDP-43 chains feature only 1 or 2 phosphates, with a small minority of chains being hyper-phosphorylated (SI Fig. S6 grey), supporting the idea of an early saturation of the most accessible phosphosites.\n\nTDP-43 phosphorylation facilitates CK1δ binding to the condensate, compared to unphosphorylated condensates at equilibrium. In Fig. 4, we show the percentage of enzymes attached to the condensate in time compared to the percentage of phosphorylated Ser, averaged again over 4 replicas. With increasing phosphorylations, CK1δ binds more stably to the condensate, suggesting that the negative charges of the pSer residues enhance the binding to the enzyme positively charged residues. In equilibrium simulations without phosphorylation only about 35 % of enzymes are attached to the droplet in average (Fig. 4).\n\nIn our simulations, the protein sequence context determines how much a given Ser residue is phosphorylated in the condensates. We compute the phosphorylation rates \\( r_P \\) for each Ser of TDP-43 LCD from the counts of phosphorylations and we compare them with the single-chain simulations results. For this computation, we use only the part of the simulations before the start of the condensate dissolution. We can see from Fig. 4 that the phosphorylation rates scale proportionally to the number of enzymes in the box. Moreover, the phosphorylation of the N- and C-terminal serines (namely Ser 266 and Ser 410) is enhanced, as well as for Ser 393, Ser 395 and Ser 403, compared to the single-chain case (see correlation plot in SI Fig. S13 left).\n\nThe probability of contact with the active site of CK1δ in the condensate for every Ser of TDP-43 LCD differs from the single-chain case roughly by a factor 6. The C-terminus is more accessible, in particular Ser 369, Ser 393, Ser 395, Ser 403 and Ser 410, as shown in Fig. 4, similar to what occurs in dilute regime. For the dense phase, the phosphorylation rates seem very well correlated to contact rates in equilibrium for the C-terminal serines (sample Pearson correlation 0.91), while the end of the N-terminus is more phosphorylated compared to what one would expect based on the contact statistics from equilibrium simulations (SI Fig. S14 left).\n\nThe role of CK1δ disordered domain in the phosphorylation of TDP-43 in dilute solution and condensates\n\nIn simulations with full-length CK1δ, we find that the disordered region of CK1δ (residues 295 to 415) slows down the phosphorylation of TDP-43 in accordance with experiments. In experiments truncated CK1δ is more active than the full-length enzyme[27]. First, we run simulations in dilute solution. In our simulations CK1δ is unphosphorylated and we do not allow possible autophosphorylations of the CK1δ IDR[28] (Fig. 5a, SI Movie 4). With the full-length enzyme, phosphorylation is more restricted to a few residues in the C-terminal region and N-terminal serines are almost never phosphorylated (Fig. 5b). This is due to a reduction of the contacts between TDP-43 residues and the active site of CK1δ, located in the folded domain of the enzyme. Indeed, in Fig. 5d we can see that also the rates of contact in equilibrium without pSer \\( r_c \\) are reduced by one order of magnitude. However, the Ser residues from residue 379 to 410 (10 of the 12 Ser residues found phosphorylated in patient samples) have at least three times the phosphorylation rate of the N-terminus also in the case of full-length CK1δ, while Ser 373 and Ser 375 are only slightly more phosphorylated than the N-terminal serines. The rate of active-site contact formation and the phosphorylation rates are\nFigure 5: Assessing the role of CK1δ disordered domain in phosphorylating TDP-43 LCD both in dilute and dense regime. (a) Example of simulation setup of full-length CK1δ (blue) and TDP-43 LCD (grey, Ser in yellow) in dilute regime. The inset shows TDP-43 interacting with CK1δ IDR (light blue, active site in red). (b) Example of simulation setup of full-length CK1δ and condensate of 200 TDP-43 chains. The inset shows CK1δ IDR (light blue) anchoring the folded domain (dark blue) to the surface of the condensate. (c–d) Phosphorylation rates \\( r_P \\) (c) and contact frequency in equilibrium \\( r_c \\) (d) for every Ser of TDP-43 LCD in presence of full-length CK1δ in dilute regime. The ticks on top show the position of the charged (red ‘+’ positive, blue ‘-’ negative) and aromatic (grey ‘a’) residues. Results from simulations without tail are reported in red on the right y-axis. (e–f) Phosphorylation rates \\( r_P \\) (e) and contact frequency in equilibrium \\( r_c \\) (f) for every Ser of TDP-43 LCD in presence of full-length CK1δ in condensate. Results from simulations without tail are reported in red on the right y-axis. (g–h) Contact rates for every residue of full-length CK1δ in dilute (g) and dense (h) regime at equilibrium. The disordered region (residues 295 to 415) has more contacts. Simulations with full-length CK1δ (red) have more contacts than without IDR (yellow), the insets show that contacts of the active site (Asp 149, Phe 150, Gly 151) are comparable.\nmore correlated in this case than for the folded domain alone (Fig. S12). However Ser 404, Ser 407 and Ser 409 have similar contacts in equilibrium compared to the N-terminal serines, but higher rate of phosphorylation. As neighboring Ser residues become phosphorylated, binding to the active site, and thus phosphorylation, is likely enhanced.\n\nThe disordered tail of CK1δ partially auto-inhibits the enzyme not by occluding the active site, but by sequestering the substrate. TDP-43 LCD interacts more strongly with the tail of CK1δ than with the folded domain of CK1δ (inset in Fig. 5a). Consequently, full-length CK1δ binds more strongly to TDP-43 LCD than the folded domain on its own. From equilibrium simulation of the enzyme and TDP-43 LCD as analysed by VAMPnet[48], the binding free energy energy goes from 5 kJ/mol to -4 kJ/mol. The tail sequesters the substrate in the dilute phase allowing less contacts with the active site, that is located on the opposite side of the enzyme surface, and thus resulting in fewer TDP-43 LCD phosphorylation events. We can see in of Fig. 5b that the disordered domain of CK1δ (residues from 295 to 415) has more contacts with TDP-43 LCD compared to the folded domain surface residues in equilibrium simulations without pSer. By looking instead to the residues in the folded domain (from 0 to 294), we notice that the full-length CK1δ (red) has in general more contacts than the CK1δ without tail (yellow), due to the stronger binding of TDP-43 LCD with the CK1δ IDR. However, the active site features a comparable amount of contacts in two cases, with residue 149 having even more contacts in the simulations without tail. By contrast, we find in our simulations that the IDR does not inhibit the CK1δ by occluding the active site. The disordered tail of CK1δ rarely forms close contacts with the active site and any close contacts are lost very rapidly (Fig. S15).\n\nWe run simulations with 200 chains of TDP-43 LCD in a cubic box of 100 nm side length, adding 1,2 and 3 chains of full-length CK1δ (Fig. 5b, SI Movie 5). In the dense regime there is high amount of chains, so both contacts and phosphorylation counts increase compared to the dilute case (Fig. 5e and f). Contacts and phosphorylation counts are also highly correlated in this case, since the abundance of chains allows the enzyme to neglect the less accessible phosphosites and phosphorylate the most accessible ones from every chain. This constitutes a disadvantage for Ser 389, Ser 404, Ser 407 and Ser 409 that are less phosphorylated compared to the dilute case. We note that the phosphorylation rates are directly proportional to the number of enzymes acting on the condensate, as well as the contact statistics (SI Fig. S14). By comparing the phosphorylation rates in condensate with the simulations without IDR, we notice that they are in general lower for the full-length case. The tail acts as a filter, allowing only the phosphorylation of Ser 369, Ser 393, Ser 395, Ser 403, Ser 410 and to a lesser extent Ser 377, Ser 379, Ser 387 and Ser 389, apart from some other very rare phosphorylation events. The effect of the tail on the relative phosphorylation rates is even more pronounced than what we observed in the simulations of CK1δ and single chains of TDP-43 LCD. When more than 5% of Ser residues in TDP-43 LCD are phosphorylated, most of the TDP-43 chains feature 1 or 2 phosphates. The distribution of the number of phosphorylated Ser residues per TDP-43 LCD chains is even narrower than in the simulations without the CK1δ disordered tail (SI Fig. S6 orange). As for the case without tail, the phosphorylation rate of the most accessible phosphosites decreases with time (SI Fig. S5). This saturation effect of the most reactive Ser residues is apparent even before the eventual dissolution of the condensate (SI Fig. S5 lower panel).\n\nThe disordered tail of CK1δ facilitates the binding of CK1δ to TDP-43 condensates. We observe that the tail recruits the condensate and keeps the folded region anchored to its surface, as illustrated in the inset of Fig. 5b. Also in this case the disordered domain of CK1δ has more contacts compared to the folded domain surface residues, as shown in Fig. 5h. Thanks to the disordered tail, the enzyme\nremains bound to the condensate surface even in absence of phosphorylations. As a consequence, the residues of the folded domain of CK1δ form more contacts with TDP-43 compared to the case without the tail (Fig. 5h, residues from 0 to 294). However, the number of contacts of TDP-43 with the active site are again comparable in the two cases, explaining why the rates of binding to the active site shown in Fig. 5 are not greater than the ones in Fig. 4f. As for the single-chain simulation, the inaccessibility of the active site seems to be due to its opposite location on the enzyme surface compared to the disordered tail. Despite the stable anchoring to the condensate, the enzyme active site faces outwards, making it less accessible to the TDP-43 serines. Even in this case the auto-inhibitory and self-regulatory effects of the enzyme tail do not seem to be due to an obstruction of the active site, since CK1δ IDR interacts strongly with the condensate (SI Fig. S16).\n\nDiscussion\n\nWe have demonstrated how Markov-state models enable us to straightforwardly validate molecular simulations of chemically-driven non-equilibrium steady states (NESS). Chemically-driven NESS are essential in cell biology[1]. Cells require the constant turnover of fuels and metabolites to grow and thrive. Chemically-driven NESS are likely also essential in the function of biomolecular condensates in the cells[2].\n\nWe envisage that our approach to establish the thermodynamic consistency of simulations and the combination of molecular dynamics and Monte Carlo can be readily applied to more complex systems and simulations of such systems in high resolution [41]. For more complex systems, extracting kinetically meaningful states becomes even more challenging. In this respect advances based on neural networks and Koopman theory are highly encouraging[48, 53, 57, 58].\n\nPTMs such as phosphorylation of proteins are a fundamental regulatory mechanism in cells and with molecular simulations we can start to investigate how protein sequence and structure determine substrate-enzyme interactions and PTM patterns. Our simulations demonstrate that the IDR of CK1δ could have important roles in TDP-43 phosphorylation, 1) by facilitating the binding to condensates and 2) by auto-inhibiting the enzyme, which our simulations capture in line with experiments [27, 28]. It is important to note that details of the conformations of proteins will be critical for the molecular recognition of potential phosphorylation sites by kinases and more detailed molecular simulations [59] will be required to fully understand the recognition mechanisms. A more detailed description of conformational flexibility will be particularly important to understand in detail how the disordered tail of CK1δ inhibits phosphorylation and whether sequestering of the disordered substrate rather than binding to the active site really underpins auto-inhibition by the CK1δ IDR. Overall our simulations point to a potential preference for the C-terminal residues of TDP-43 on account of its sequence. Aggregated TDP-43 in patient samples is frequently phosphorylated at, e.g., Ser 379, Ser 403/Ser 404 and Ser 409/Ser 410 [26, 46], which are among the most phosphorylated residues also in our simulations. Due to the high concentration of substrates in condensates, proteins are readily phosphorylated. The phosphorylation rates for Ser residues are larger for TDP-43 in condensates than in the dilute phase. Interestingly, phosphorylation patterns are overall similar in dilute solution and condensates. While there are differences in the phosphorylation propensities, sequence context still determines which sites can be phosphorylated. One can speculate that differences between phosphorylation in dilute and dense solution could be partly explained by the overall higher phosphorylation level in condensates, which means that some sites will effectively be more readily phosphorylated than in dilute solutions[25], while the kinase may retain sequence-dependent recognition of substrates in the condensates.\nMethods\n\nCoarse-grained MD simulations\n\nIn our work, we simulated TDP-43 LCD and the kinase CK1δ using a one-bead-per-residue coarse-grained model called hydrophobicity scale model [31] (HPS model) and a modified version of it, referred to as modified HPS model in the text (SI Text). In these models, the water solvent and the ions concentration are implicit in the pair potential definition. We used the original HPS for the thermodynamic consistency validation simulations, in which we preferred to give priority to the frequency of the binding and phosphorylation events at the expense of having a more realistic force field, in order to get better statistics. For the other simulations, we used the modified HPS model [80] in which cation-pi interactions are enhanced [60] and folded domains interaction are reduced by 30% [61, 62] (SI Text). Simulations were conducted using Langevin dynamics at a temperature of 300 K and friction coefficient of 0.001 ps^{-1} and in a cubic box with periodic boundary conditions of side length of 30 nm for the single TDP-43 chain simulations and 100 nm for the condensate simulations. The simulated TDP-43 LCD includes residues from 261 to 414 of the full-length TDP-43. The folded domain of CK1δ (residues from 1 to 294) follows a rigid body dynamics with rotational drag coefficient of 4 ps^{-1} for every axis, the structure is provided by https://alphafold.ebi.ac.uk/entry/P48730.\n\nFor the dilute regime, 100 simulations with phosphorylation reaction step and without reservoir exchange step were run, 2×10^{8} MD steps long (2 μs in simulation time) for the case with 1 wild type TDP-43 LCD and 1 CK1δ folded-domain, 4×10^{8} MD steps long (4 μs in simulation time) both for the case with 1 averaged-interaction polymer and 1 CK1δ folded-domain and for the case with 1 wild type TDP-43 LCD and 1 full-length CK1δ. To characterize the intrinsic affinity of the enzyme for TDP-43 LCD, we repeated the same simulations, but without phosphorylation reactions at thermodynamic equilibrium. We collected in total 450 μs of simulation time for the case of wild type TDP-43 LCD and CK1δ folded-domain and 900 μs for the averaged-interaction polymer and for full-length CK1δ. The averaged interaction polymer is built by substituting the TDP-43 LCD residues different from Ser with a bead having average TDP-43 LCD mass, size parameter σ and hydropathy parameter λ (SI Text) 1) leaving the serines at their original positions and 2) spreading them equally spaced along the chain.\n\nWe also simulated a condensate of 200 TDP-43 LCD chains. We ran 4 simulations 5×10^{8} MD steps long (5 μs in simulation time) with phosphorylation steps without reservoir exchange step (as for the single chain simulations) in presence of 1,3 or 5 CK1δ folded-domain chains and of 1,2 or 3 full-length CK1δ chains. We repeated the same simulations, but without phosphorylation reactions at thermodynamic equilibrium, collecting a total of 20 μs of simulation time for each case.\n\nAll the simulations involved in this paper were performed using the Python package HOOMD-blue version 3.8.1. The code used for the simulations is available at https://github.com/ezippo/hoomd3_phosphorylation. The Ashbaugh-Hatch pair potential for the non-bonded interactions is available at https://github.com/ezippo/ashbaugh_plugin as a HOOMD-blue plugin.\n\nPhosphorylation reaction through a Monte Carlo step\n\nIn addition to the standard MD simulation, we added a Monte Carlo step to mimic the phosphorylation reaction. Every 200 steps of MD simulation, we check if one of the TDP-43 phosphosites is in contact with the active site of CK1δ, the area of the enzyme that catalyzes the reaction, identified with the residues Asp149, Phe150 and Gly151. The contact criterion is the following: the three\ndistances between the TDP-43 phosphosite and the residues of the CK1δ active site must all be less than 1 nm; in case more than one phosphosite is in contact with the active site at the same time-step, only the closest one is taken into account. When a contact occurs, we try to switch the Ser in contact into pSer (or the opposite) with a Metropolis-like acceptance probability in Eq. [2]. The reverse reaction, that is the exchange of pSer with Ser, can also occur with probability \\( A(\\text{pSer}, \\text{Ser}) = \\min(1, \\exp(\\beta \\Delta U_P + \\beta \\Delta \\mu_P)) \\), but it is less likely to happen when there is a chemical potential difference favouring the protein phosphorylation. ATP, ADP are modelled implicitly and are not explicitly simulated, with concentrations kept fixed and fully characterized through the choice of \\( \\Delta \\mu_P \\).\n\nThe chemical potential difference in a reaction in units of \\( k_B T \\) is given by the logarithm of the product to substrate concentration ratio. Considering that the ATP concentration in cells is around 1 mM, the concentration of ADP is around 10 \\( \\mu \\)M and fixing a temperature \\( T = 300 \\) K for our simulations, we get a chemical potential difference for a phosphorylation reaction \\( \\Delta \\mu_P = \\mu_{ADP} - \\mu_{ATP} \\simeq -11.5 \\) kcal/mol \\( \\simeq -48 \\) kJ/mol (SI Text). Observe that the ATP concentration is two orders of magnitude larger than the ADP concentration, leading to a large negative \\( \\Delta \\mu_P \\) that favors the exchange of Ser into pSer and disfavors the opposite reaction. Moreover we can mimic the ATP to ADP concentration ratio by changing the chemical potential difference in our simulation at fixed temperature. We used \\( \\Delta \\mu_P = 0, -5, -10 \\) kJ/mol for the validation of the thermodynamic consistency simulations and \\( \\Delta \\mu_P = -48 \\) kJ/mol for all the other simulations in dilute regime and condensate.\n\nDephosphorylation step\n\nIn our validation simulations, we assume the exchange between TDP-43 and phosphorylated TDP-43 happens without chemical driving and with equilibrium concentrations, through another Metropolis-like step (reservoir exchange step). Every 200 MD steps, we check if the distances between the TDP-43 phosphosite and the 3 residues of the CK1δ active site is larger than 25 nm (half box side length). In that case, we randomly swap the pSer of the phosphorylated TDP-43 with a Ser (or the opposite) with a Metropolis-like acceptance probability:\n\n\\[\nA_D(\\text{pSer}, \\text{Ser}) = \\min(1, \\exp(-\\beta \\Delta U_D))\n\\]\n\nwhere \\( \\Delta U_D \\) is again the difference between the potential energy of the configuration with Ser and the one of the configuration with pSer. In this case there is no chemical driving force, the reaction obeys detailed balance and thus it does not inject any additional energy into the system. This exchange step mimics a larger reservoir of TDP-43 and phosphorylated TDP-43 and thus enables us to simulate multiple phosphorylation cycles on the level of a single enzyme and single substrate protein simulation.\n\nThermodynamic consistency validation simulations\n\nWe simulated the system with one CK1δ and one TDP-43 LCD with only one reactive residue. We repeated the simulation for 6 different reactive serines along the TDP-43 LCD, i.e. Ser292, Ser 317, Ser 369, Ser 387, Ser 403, Ser 409, and \\( \\Delta \\mu_P = 0, -5, -10 \\) kJ/mol. Simulations were conducted for 20 \\( \\mu \\)s in a cubic box of 50 nm side length with periodic boundaries using HPS model force field. In order to get better statistics, we took a 100\\( \\mu \\)s long trajectory for Ser 403 and \\( \\Delta \\mu_P = 0, -5 \\) kJ/mol. We used these longer trajectories for the estimates of \\( \\Delta \\mu_{cycle} \\) with different\nlag times and with the version of VAMPnet with more input distances. Errorbars on \\( \\Delta \\mu_{\\text{cycle}} \\) were obtained via bootstrapping of the total simulation trajectory collected.\n\nVAMPnet architecture and training\n\nFor the bound state recognition, we performed a nonlinear dimension reduction using a neural network with two identical lobes, following the VAMPnet architecture and the hyper-parameter optimization used by Mardt et al. [48]. Each lobe is composed by an input layer with 154 nodes, one for each residue of TDP-43 LCD, one hidden layer with 30 nodes that employs exponential linear units (ELU) and an output layer with 2 nodes, ideally bound and unbound state, and a final Softmax classifier to obtain probabilities of bound and unbound configurations as output. As input for the neural network, we used the 154 distances between each residue of TDP-43 LCD and the active site of CK1δ. We chose a learning rate of \\( 0.5 \\times 10^{-2} \\) and a batch size of \\( 4 \\times 10^4 \\). The neural network was trained for 100 epochs on 90\\( \\mu s \\) of equilibrium HPS model[31] simulation with one TDP-43 LCD and one CK1δ.\n\nThe neural network returns the probability of being in one of the 2 output states (ideally bound and unbound state) for each snapshot of the trajectory. We assigned each snapshot to the state with higher probability, filtering those with a probability between 30% and 70% using transition-based state assignment [49]. In other words, these configurations were assigned based on the state of the previous and following snapshots, in order to filter out spurious transitions.\n\nIn order to test the generality of our method, we repeated the bound state recognition with VAMPnet, but using more input nodes. In particular, we used the distances between all the residues of TDP-43 LCD and 30 equally spaced residues of CK1δ, resulting in an input layer of 4620 nodes. This time we used 2 hidden layers with 154 and 30 nodes each, and an output layer with 2 nodes. We reduced the learning rate to \\( 0.5 \\times 10^{-3} \\) and the batch size to \\( 10^4 \\).\n\nImplied timescales and Chapman-Kolmogorov test\n\nThe choice of the lag time was done by looking at the implied timescales. We can estimate the implied timescales of the Markov model from the eigenvalues of the transition matrix as:\n\n\\[\nt_i(\\tau) = -\\frac{\\tau}{\\ln|\\lambda_i(\\tau)|}\n\\]\n\nwith \\( \\lambda_i(\\tau) \\) the eigenvalues of \\( T_{ij}(\\tau) \\). We chose a lag time \\( \\tau \\) such that \\( t_i(\\hat{\\tau}) \\) is approximately constant for every \\( \\hat{\\tau} \\geq \\tau \\). We estimated \\( \\Delta \\mu_{\\text{cycle}} \\) for different lag times (1,10,20 Markov chain steps) for the case of reactive Ser 403 and \\( \\Delta \\mu_P = 0, -5 \\) kJ/mol. For \\( \\tau \\geq 10 \\) Markov chain steps, the estimated \\( \\Delta \\mu_{\\text{cycle}} \\) is in agreement with \\( \\Delta \\mu_P \\) (SI Table S2).\n\nWe estimated the goodness of the MSM by looking at the Chapman-Kolmogorov test (CK test) [52, 53]. In a Markovian process, the transition matrix satisfies the relation\n\n\\[\nT_{ij}(n\\tau) = [T_{ij}(\\tau)]^n\n\\]\n\nwith \\( n \\geq 1 \\). In other words, the transition matrix of the model estimated at lag time \\( n\\tau \\) must be equal to the transition matrix to the power \\( n \\) of the model estimated at lag time \\( \\tau \\). The CK test compares \\( T_{ij}(n\\tau) \\) (the estimated transition matrix) and \\( T_{ij}^n(\\tau) \\) (the predicted transition matrix) for every possible transition \\( i \\rightleftharpoons j \\) and different lag times \\( n\\tau \\).\nEstimate of phosphorylation rates and fit of phosphorylation processes\n\nIn all the single TDP-43 LCD chain simulations, we estimated the phosphorylation rates \\( r_P \\) assuming the phosphorylation process is without memory and thus follows single-exponential kinetics. In all the collected 100 simulations, we had at most one phosphorylation event for each Ser residue, happening at time \\( t_P^i < t_{tot} \\) for simulation \\( i \\), with \\( t_{tot} \\) the total time of the simulation. In this case, we can use the maximum likelihood estimator for the rate with uniform prior distribution [55]\n\n\\[\nr_P = \\frac{n + 1}{\\Theta}, \\quad \\text{var}(r_P) = \\frac{n + 1}{\\Theta^2}, \\text{ with } \\Theta = \\sum_{i=1}^{n} t_P^i + (100 - n)t_{tot}\n\\] (7)\n\nwhere \\( n \\) is the counts of simulations with one phosphorylation event for the Ser took in consideration. Instead, for the simulations in condensate, in which we have multiple TDP-43 chains and thus multiple phosphorylation events for each Ser residue, we computed \\( r_P \\) as the total count of phosphorylation events in the simulation divided by the total simulation time. In this case, the error on the estimate of the rate is computed as the standard error of the mean from the different replicas. In the same way we also computed all the contacts rates \\( r_c \\) and their error.\n\nHowever, since the phosphorylation of a Ser can happen only if TDP-43 is bound to the enzyme, it is more appropriate to take into account the conditional probability of the phosphorylation event given the binding of TDP-43 and CK1δ already occurred. Given \\( p_B(t)dt = r_B \\exp(-r_Bt)dt \\) the probability of binding between time \\( t \\) and \\( t + dt \\) and \\( p_P(t)dt = r_P \\exp(-r_Pt)dt \\) the probability of having a phosphorylation between time \\( t \\) and \\( t + dt \\), the conditional probability of having a phosphorylation between time \\( t \\) and \\( t + dt \\) given that TDP-43 is bound to CK1δ is\n\n\\[\nP(t|\\text{bound})dt = \\int_0^t p_B(t')dt'p_P(t-t')dt = \\frac{r_B r_P}{r_B - r_P} \\left( e^{-r_P t} - e^{-r_B t} \\right) dt\n\\] (8)\n\nIf we call \\( P_c(t < T) \\) the probability of having a phosphorylation event within time \\( T \\) in our simulations, we can write its complementary as:\n\n\\[\n1 - P_c(t < T) = 1 - \\int_0^T P(t)dt = \\frac{r_B r_P}{r_B - r_P} \\left( \\frac{e^{-r_P t}}{r_P} - \\frac{e^{-r_B t}}{r_B} \\right)\n\\] (9)\n\nInstead, if we assume that the binding process is much faster than the phosphorylation one (\\( r_B \\gg r_P \\)), than we can approximate \\( P(t|\\text{bound}) \\sim p_P(t) \\) and \\( 1 - P_c(t < T) \\sim \\exp(-r_P t) \\).\n\nFrom the 100 simulations used to estimate the phosphorylation rates, we computed the normalized inverse cumulative histogram of the phosphorylation events time \\( T \\), where each time bin gives the phosphorylation counts for that bin plus the counts of all the following bins, divided by the number of simulations. We fitted it with \\( 1 - P_c(t < T) \\) both for a single-exponential process and a conditioned single-exponential process.\n\nCondensate identification with clustering analysis\n\nIn order to identify the TDP-43 LCD condensate in the trajectory file, we used the DBSCAN (Density-Based Spatial Clustering of Applications with Noise) clustering analysis algorithm[63]. It is an efficient algorithm to identify clusters based on a euclidean distance cut-off \\( \\epsilon \\) and a minimum cluster size parameter \\( n_{min} \\). Particles with at least \\( n_{min} \\) neighbors within a distance \\( \\epsilon \\) are considered\ncore particles of the cluster. Instead, particles with less than \\( n_{\\min} \\) neighbors are considered non-core particles and they are assigned to a cluster only if at least one of their neighbors is a core particle.\n\nFor the estimate of the condensate size and of the percentage of CK1δ in contact with the condensate, we used the positions of every bead as input data and we chose the parameters \\( \\epsilon = 1 \\) nm and \\( n_{\\min} = 2 \\). With this choice, every isolated chain is considered as a cluster and two different chains belongs to the same cluster whenever at least one of their particles is in contact (within 1 nm). However, varying \\( \\epsilon \\) between 0.8 nm and 3 nm and \\( n_{\\min} \\) between 2 and 5 does not significantly change the results. We accounted for the periodic boundary conditions by centering the condensate in the box at every frame.\n\nAcknowledgments\n\nE.Z. was funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation), Project No. 233630050 – TRR 146. L.S.S. thank M³ODEL and ReALity (Resilience, Adaptation and Longevity) and Forschungsiniziative des Landes Rheinland-Pfalz for support. This project was funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) - SFB 1551 – Project No. 464588647 . Further, we gratefully acknowledge the computing time granted on the supercomputers Mogon II at Johannes Gutenberg University Mainz, which is a member of the AHRP (Alliance for High Performance Computing in Rhineland Palatinate) and the Gauss Alliance e.V. We thank Alex Holehouse for insightful discussions.\n\nAuthor contributions\n\nE.Z. ran the simulations, analysed data, interpreted results, wrote the manuscript. 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Ester, M., Kriegel, H.-P., Sander, J. & Xu, X. *A Density-Based Algorithm for Discovering Clusters in Large Spatial Databases with Noise* in Knowledge Discovery and Data Mining (1996).\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• SupplementaryInformation.pdf\n• Slmovie1.mp4\n• Slmovie2.mp4\n• Slmovie3.mp4\n• Slmovie4.mp4\n• Slmovie5.mp4"} {"paper_id": "prb46", "title": "polyBERT: A chemical language model to enable fully machine-driven ultrafast polymer informatics", "text": "polyBERT: A chemical language model to enable fully machine-driven ultrafast polymer informatics\n\nChristopher Kuenneth\nGeorgia Institute of Technology\nRampi Ramprasad (rampi.ramprasad@mse.gatech.edu)\nGeorgia Institute of Technology https://orcid.org/0000-0003-4630-1565\n\nArticle\n\nKeywords:\n\nPosted Date: December 13th, 2022\n\nDOI: https://doi.org/10.21203/rs.3.rs-2116998/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nAdditional Declarations: Yes there is potential Competing Interest. R.R. is the founder of the company Matmerize, Inc., that intends to provide polymer informatics services. A provisional patent on polyBERT has been filed by R.R. and C.K.\n\nVersion of Record: A version of this preprint was published at Nature Communications on July 11th, 2023. See the published version at https://doi.org/10.1038/s41467-023-39868-6.\npolyBERT: A chemical language model to enable fully machine-driven ultrafast polymer informatics\n\nChristopher Kuenneth and Rampi Ramprasad*\n\nSchool of Materials Science and Engineering, Georgia Institute of Technology, Atlanta, Georgia 30332, USA\n\nE-mail: rampi.ramprasad@mse.gatech.edu\n\nAbstract\n\nPolymers are a vital part of everyday life. Their chemical universe is so large that it presents unprecedented opportunities as well as significant challenges to identify suitable application-specific candidates. We present a complete end-to-end machine-driven polymer informatics pipeline that can search this space for suitable candidates at unprecedented speed and accuracy. This pipeline includes a polymer chemical fingerprinting capability called polyBERT (inspired by Natural Language Processing concepts), and a multitask learning approach that maps the polyBERT fingerprints to a host of properties. polyBERT is a chemical linguist that treats the chemical structure of polymers as a chemical language. The present approach outstrips the best presently available concepts for polymer property prediction based on handcrafted fingerprint schemes in speed by two orders of magnitude while preserving accuracy, thus making it a strong candidate for deployment in scalable architectures including cloud infrastructures.\nPolymers are an integral part of our everyday life and instrumental in the progress of technologies for future innovations.\\(^1\\) The sheer magnitude and diversity of the polymer chemical space provide opportunities for crafting polymers that accurately match application demands, yet also come with the challenge of efficiently and effectively browsing this gigantic space. The nascent field of polymer informatics\\(^{2-5}\\) allows access to the depth of the polymer universe and demonstrates the potency of machine learning (ML) models to overcome this challenge. ML frameworks have enabled substantial progress in the development of polymer property predictors\\(^{6-10}\\) and solving inverse problems in which polymers that meet specific property requirements are either identified from candidate sets,\\(^{11,12}\\) or are freshly designed using genetic\\(^{13,14}\\) or generative\\(^{15-17}\\) algorithms.\n\nAn essential step in polymer informatics pipelines is the conversion of polymer chemical structures to numerical representations that are often called fingerprints, features, or descriptors (see blue boxes in Figure 1a). Past and current handcrafted fingerprinting approaches\\(^{20-24}\\) utilize cheminformatics tools that numerically encode key chemical and structural features of polymers. Although such handcrafted fingerprints build on invaluable intuition and experience, they are tedious to develop, involve complex computations that often consume most of the time during model training and inference, and lack generalization to all polymer chemical classes (i.e., new features may have to be added to the catalog of features in an *ad hoc* manner). ML pipelines that use handcrafted fingerprints are thus prone to errors during the exploration of new polymer chemical classes. Also, handcrafted fingerprints present barriers for the development and deployment of fully machine-driven informatics pipelines, which are suited for scalability in cloud computing and high-throughput environments.\n\nThe present contribution overcomes the previously mentioned limitations by replacing handcrafted fingerprints with fully machine-crafted “Transformer” fingerprints (see right pipeline of Figure 1a). Transformers\\(^{25}\\) were recently developed in the field of Natural Language Processing (NLP) and have swiftly become the gold standard in ML language mod-\nFigure 1: Polymer informatics with polyBERT. **a** Prediction pipelines. The left pipeline shows the prediction using handcrafted fingerprints from cheminformatics tools, while the right pipeline (present work) portrays a fully end-to-end machine-driven predictor using polyBERT. Property symbols are defined in Table 1. ID1 and ID3 are copolymers, and ID2 is a homopolymer. **b** polyBERT is a polymer chemical language linguist. polyBERT canonicalizes, tokenizes, and masks polymer SMILES\\(^{18}\\) (PSMILES) strings strings before passing them to the DeBERTa model. A last dense layer with a softmax activation function finds the masked tokens. polyBERT fingerprints (dashed arrow) are the averages over the token dimension (sentence average) of the last Transformer encoder. **c** 100 million hypothetical PSMILES strings. First, 13 766 known (i.e., previously synthesized) polymers are decomposed to 4 424 fragments using the BRICS\\(^{19}\\) method. Second, re-assembling the BRICS fragments in many different ways generates 100 million hypothetical polymers by randomly and enumeratively combining the fragments.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
IDPolymer 1c1Polymer 2c2
1[*]CC[*]40[*]CC([*])C60
2[*]CCO[*]100-0
3[*]CC([*])C1CC130[*]CC([*])C1CC1C170
4............
\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
IDTgTmTdEεbσb...
123036168319046016...
222032660417026711...
332052062060011323...
4.....................
\neling. In this work, we envision simplified molecular-input line-entry system (SMILES)\\(^{18}\\) strings that have been used to represent polymers as the “chemical language” of polymers. We use millions of polymer SMILES (PSMILES) strings for training a language model called polyBERT to become an expert – a linguist – of the polymer chemical language. In combination with multitask deep neural networks,\\(^{6,7}\\) polyBERT enables a fully end-to-end machine-driven polymer informatics pipeline that uses and unleashes the true power of artificial intelligence methods. Multitask deep neural networks harness inherent correlations in multi-fidelity and multi-property data sets, scale effortlessly in cloud computing environments, and generalize to multiple prediction tasks.\n\nRecent studies\\(^{26-28}\\) demonstrated the benefits of using Transformers in the molecule chemical space. For example, Wang et al.\\(^{27}\\) have trained a BERT model\\(^{29}\\) (the most common general language model) with a data set of molecule SMILES strings. Using BERT’s latent space representations of molecules as fingerprints, the authors show that their approach outperforms other fingerprinting methods (including fingerprints of an unsupervised recurrent neural network and a graph-based neural network). Similarly, Schwaller et al.\\(^{30,31}\\) have developed a Transformer model to predict retrosynthesis pathways of molecules from reactants and reagents that outperforms known algorithms in the reaction prediction literature. No past study has applied Transformers to polymers.\n\nThis study has several critical and novel ingredients. First, we generate a data set of 100 million hypothetical polymers by enumeratively combining chemical fragments extracted from a list of more than 13 000 synthesized polymers. Next, we train polyBERT, a DeBERTa\\(^{32}\\)-based encoder-only Transformer, using this hypothetical polymer data set to become a polymer chemical linguist. During training, polyBERT learns to translate input PSMILES strings to numerical representations that we use as polymer fingerprints. Finally, we map the polyBERT fingerprints to about 3 dozen polymer properties using our multitask ML framework to yield fully machine-driven ultrafast polymer property predictors. For benchmarking, the performance (both accuracy and speed) of this new end-to-end prop-\nerty prediction pipeline is compared with the state-of-the-art handcrafted Polymer Genome\\(^8\\) (PG) fingerprint based pipeline pioneered previously. Using the ultrafast polyBRET polymer informatics pipeline, we are in a position to predict the properties of the 100 million hypothetical polymers intending to find property boundaries of the polymer universe. This work contributes to expediting the discovery, design, development, and deployment of polymers by harnessing the true power of language, data, and artificial intelligence models.\n\nResults\n\nData Sets Figure 1c sketches the two-step process for fabricating 100 million hypothetical PSMILES strings. We use the Breaking Retrosynthetically Interesting Chemical Substructures (BRICS)\\(^{19}\\) method (as implemented in RDKit\\(^{33}\\)) to decompose previously synthesized 13 766 polymers into 4 424 unique chemical fragments. Random and enumerative compositions of these fragments yield 100 million hypothetical PSMILES strings that we first canonicalize (see Methods section) and then use for training polyBERT. The hypothetical PSMILES strings are chemically valid polymers but, mostly, have never been synthesized before.\n\nOnce polyBERT has completed its unsupervised learning task using the 100 million hypothetical PSMILES strings, multitask supervised learning maps polyBERT polymer fingerprints to multiple properties to produce property predictors. We use the property data set in Table 1 for training the property predictors. The data set contains 28 061 (\\(\\approx 80\\%\\)) homopolymer and 7 456 (\\(\\approx 20\\%\\)) copolymer (total of 35 517) data points of 29 experimental and computational polymer properties that pertain to 11 145 different monomers and 1 338 distinct copolymer chemistries, respectively. Each of the 7 456 copolymer data points involves two distinct comonomers at various compositions. All data points in the data set have been used in past studies\\(^{6,7,11,34-41}\\) and were produced using computational methods or obtained from literature and other public sources. Supplementary Figures S3-S8 show\nTable 1: Training data set for the property predictors. The properties are sorted into categories, showed at the top of each block. The data set contains 29 properties (dielectric constants \\( k_f \\) are available at 9 different frequencies \\( f \\)). HP and CP stand for homopolymer and copolymer, respectively.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
PropertySymbolUnitSourceaData rangeData points
HPCPAll
Thermal
Glass transition temp.\\( T_g \\)KExp.[8e+01, 9e+02]5 1833 3128 495
Melting temp.\\( T_m \\)KExp.[2e+02, 9e+02]2 1321 5233 655
Degradation temp.\\( T_d \\)KExp.[3e+02, 1e+03]3 5841 0644 648
Thermodynamic & physical
Heat capacity\\( c_p \\)Jg\\(^{-1}\\)K\\(^{-1}\\)Exp.[8e-01, 2e+00]797979
Atomization energy\\( E_{at} \\)eV atom\\(^{-1}\\)DFT[-7e+00, -5e+00]390390390
Limiting oxygen index\\( O_i \\)%Exp.[1e+01, 7e+01]101101101
Crystall. tendency (DFT)\\( X_c \\)%DFT[1e-01, 1e+02]432432432
Crystall. tendency (exp.)\\( X_e \\)%Exp.[1e+00, 1e+02]111111111
Density\\( \\rho \\)g cm\\(^{-3}\\)Exp.[8e-01, 2e+00]910910910
Electronic
Band gap (chain)\\( E_{gc} \\)eVDFT[2e-02, 1e+01]4 2244 2244 224
Band gap (bulk)\\( E_{gb} \\)eVDFT[4e-01, 1e+01]597597597
Electron affinity\\( E_{ea} \\)eVDFT[4e-01, 5e+00]368368368
Ionization energy\\( E_i \\)eVDFT[4e+00, 1e+01]370370370
Electronic injection barrier\\( E_{ib} \\)eVDFT[2e+00, 7e+00]2 6102 6102 610
Cohesive energy density\\( \\delta \\)eVExp.[2e+01, 3e+02]294294294
Optical & dielectric
Refractive index (DFT)\\( n_c \\)DFT[1e+00, 3e+00]382382382
Refractive index (exp.)\\( n_e \\)Exp.[1e+00, 2e+00]516516516
Dielec. constant (DFT)\\( k_c \\)DFT[3e+00, 9e+00]382382382
Dielec. constant at freq. \\( f^b \\)\\( k_f \\)Exp.[2e+00, 1e+01]1 1871 1871 187
Mechanical
Young's modulus\\( E \\)MPaExp.[2e-02, 4e+03]592322914
Tensile strength at yield\\( \\sigma_y \\)MPaExp.[3e-05, 1e+02]21678294
Tensile strength at break\\( \\sigma_b \\)MPaExp.[5e-03, 2e+02]663318981
Elongation at break\\( \\epsilon_b \\)Exp.[3e-01, 1e+03]8682601 128
Permeability
O$_2$ gas permeability\\( \\mu_{O_2} \\)barrerExp.[5e-06, 1e+03]390210600
CO$_2$ gas permeability\\( \\mu_{CO_2} \\)barrerExp.[1e-06, 5e+03]286119405
N$_2$ gas permeability\\( \\mu_{N_2} \\)barrerExp.[3e-05, 5e+02]38499483
H$_2$ gas permeability\\( \\mu_{H_2} \\)barrerExp.[2e-02, 5e+03]24046286
He gas permeability\\( \\mu_{He} \\)barrerExp.[5e-02, 2e+03]23958297
CH$_4$ gas permeability\\( \\mu_{CH_4} \\)barrerExp.[4e-04, 2e+03]33147378
28 0617 45635 517
\n\na Experiments (Exp.); density functional theory (DFT)\nb \\( f \\in \\{1.78, 2, 3, 4, 5, 6, 7, 9, 15\\} \\) is the log$_{10}$(frequency in Hz); e.g., \\( k_3 \\) is the dielectric constant at a frequency of 1 kHz.\npolyBERT polyBERT iteratively ingests 100 million hypothetical PSMILES strings to learn the polymer chemical language, as sketched in Figure 1b. polyBERT is a DeBERTa\\(^{32}\\) model (as implemented in Huggingface’s Transformer Python library\\(^{42}\\)) with a supplementary three-stage preprocessing unit for PSMILES strings. First, polyBERT transforms a input PSMILES string into its canonical form (e.g., [*]CCOCCO[*] to [*]COC[*]) using the canonicalize_psmiles Python package developed in this work. Details can be found in the Methods section. Second, polyBERT tokenizes canonical PSMILES strings using the SentencePiece\\(^{43}\\) tokenizer. The tokens are frequent patterns in PSMILES strings and determined in a pretraining process of SentencePiece with the 100 million hypothetical PSMILES strings. Third, polyBERT masks 15% (default parameter for masked language models) of the tokens to create a self-supervised training task. In this training task, polyBERT is taught to predict the masked tokens using the non-masked surrounding tokens by adjusting the weights of the Transformer encoders (fill-in-the-blanks task). We use 80 million PSMILES strings for training and 20 million PSMILES strings for validation. The validation F1-score is > 99. This exceptionally good F1-score indicates that polyBERT finds the masked tokens in almost all cases. The total CO\\(_2\\) emissions for training polyBERT on our hardware are estimated to be 12.6 kgCO\\(_2\\)eq (see CO\\(_2\\) Emission section).\n\nThe training with 80 million PSMILES strings renders polyBERT an expert polymer chemical linguist who knows grammatical and syntactical rules of the polymer chemical language. polyBERT learns patterns and relations of tokens via the multi-head self-attention mechanism and fully connected feed-forward network of the Transformer encoders.\\(^{25}\\) The attention mechanism instructs polyBERT to devote more focus to a small but essential part of a PSMILES string. polyBERT’s learned latent spaces after each encoder block are numerical representations of the input PSMILES strings. The polyBERT fingerprint is the average over the token dimension (sentence average) of the last latent space (dotted\nline in Figure 1b). We use the Python package SentenceTransformers\\(^{44}\\) for extracting and computing polyBERT fingerprints.\n\n![Two-dimensional UMAP plots for polyBERT and Polymer Genome fingerprints](page_232_370_1167_388.png)\n\nFigure 2: Two-dimensional UMAP\\(^{45}\\) plots for polyBERT and Polymer Genome fingerprints and all homo- and copolymer chemistries in Table 1. The triangles (blue, orange, and green) in the first column indicate fingerprint positions in the UMAP spaces of three selected polymers. The colored dots in columns two, three, and four indicate property values of \\(T_g\\), \\(T_d\\), and \\(E_{gc}\\), which stand for the glass transition temperature, degradation temperature, and band gap (chain), respectively. Light gray dots show polymers with unknown property values. The PSMILES strings [*]CC([*])CC, [*]CC([*])CCC, and [*]CC([*])c1ccncc1 denote poly(but-1-ene), poly(pent-1-ene), and poly(4-vinylpyridine), respectively.\n\nFingerprints For acquiring analogies and juxtaposing chemical relevancy, we compare polyBERT fingerprints with the handcrafted Polymer Genome\\(^{8}\\) (PG) fingerprints that numerically encode polymers at three different length scales. A description of PG fingerprints can be found in the Methods section. The PG fingerprint vector for the data set in this work has 945 components and is sparsely populated (93.9 % zeros). The reason for this ultra sparsity is that many PG fingerprint components count chemical groups in polymers.\\(^{8}\\) A fingerprint component of zero indicates that a chemical group is not present. In contrast, polyBERT fingerprint vectors have 600 components and are fully dense (0 % zeros). Fully\ndense and lower-dimensional fingerprints are often advantageous for ML models whose computation time scales superlinear (\\( \\mathcal{O}(n^s), s > 1 \\)) with the data set size (\\( n \\)) such as Gaussian process or kernel ridge techniques. Moreover, in the case of neural networks, sparse and high-dimensional input vectors can cause unnecessary high memory load that reduces training and inference speed. We note that the dimensionality of polyBERT fingerprints is a parameter that can be chosen arbitrarily to yield the best training result. A summary of the key figures can be found in Supplementary Table S2.\n\nFigure 2 shows uniform manifold approximation and projection (UMAP)\\(^{45}\\) plots for all homo- and copolymer chemistries in Table 1. The colored triangles in the first column indicate the coordinates of three selected polymers for polyBERT and PG fingerprints. We observe for both fingerprint types that the orange and blue triangles are very close, while the green triangle is separate. We also note that polymers corresponding to the orange and blue triangles, namely poly(but-1-ene) and poly(pent-1-ene), have similar chemistry (different by only one carbon atom), but poly(4-vinylpyridine) represented by a green triangle, is different. This chemically intuitive positioning of fingerprints suggests the chemical relevancy of fingerprint distances. The cosine fingerprint distances reported in Supplementary Figure S1 allow for the same conclusion.\n\nThe second, third, and fourth columns of Figure 2 display the same UMAP plots as in the first column. Colored dots indicate the property values of \\( T_g \\), \\( T_d \\), and \\( E_{gc} \\), while light gray dots show polymer fingerprints with unknown property values. We observe localized clusters of similar color in each plot pertaining to polymers of similar properties. Although this finding is not surprising for the PG fingerprint because it relies on handcrafted chemical features that purposely position similar polymers next to each other, it is remarkable for polyBERT. With no chemical information and purely based on training on a massive amount of PSMILES strings, polyBERT has learned polymer fingerprints that match chemical intuition. This again shows that polyBERT fingerprints have chemical pertinence and their distances measure polymer similarity (e.g., using the cosine distance metric).\nFigure 3: Computation time of polymer fingerprints. The fingerprints are computed on one CPU core (Intel(R) Xeon(R) CPU E5-2667), except for polyBERT (GPU) fingerprints that are computed on one GPU (Quadro GP100). Computation times per PSMILES string, in the order of the legend, are 33.39, 0.76, and 163.59 ms/PSMILES (computed for \\(10^4\\) PSMILES), respectively.\n\nThe computation of polyBERT and PG fingerprints scales nearly linear with the number of PSMILES strings although their performance can be quite different, as shown in the log-log scaled Figure 3. The computation of polyBERT (GPU) is over two orders of magnitude (215 times) faster than computing PG fingerprints. polyBERT fingerprints may be computed on CPUs and GPUs. Because of the presently large efforts in industry to develop faster and better GPUs, we expect the computation of polyBERT fingerprint to become even faster in the future. Time is extremely important for high-throughput polymer informatics pipelines that identify polymers from large candidate sets.\\(^{11}\\) With an estimate of 0.30 ms/PSMILES for the multitask deep neural networks (see Property Prediction section), the total time using the polyBERT-based pipeline to predict 29 polymer properties sums to 1.06 ms/polymer/GPU.\n\nProperty Prediction For benchmarking the property prediction accuracy of polyBERT and PG fingerprints, we train multitask deep neural networks for each property category defined in Table 1. Multitask deep neural networks have demonstrated best-in-class results\nFigure 4: \\( R^2 \\) performance values for polyBERT (PB) and Polymer Genome (PG) fingerprints.\n**a** \\( R^2 \\) averages of the five cross-validation validation data sets along with standard deviations (\\(1\\sigma\\)). **b** \\( R^2 \\) values of the meta learner’s test data set. The category-averaged \\( R^2 \\) values are stated in the last rows of each block, while overall \\( R^2 \\) values are given in the very last block. The properties gas permeabilities (\\( \\mu_x \\)) and elongation at break (\\( \\epsilon_b \\)) are trained on log base 10 scale (\\( x \\mapsto \\log_{10}(x+1) \\)). The \\( R^2 \\) values are reported on this scale. **c** Minimum, mean, and maximum of polyBERT-based property predictions for 100 million hypothetical polymers. Symbols are defined in Table 1.\n\n![R^2 performance values for polyBERT (PB) and Polymer Genome (PG) fingerprints.](page_357_682_1167_693.png)\nfor polymer property predictions,\\(^{6,7,11}\\) while being fast, scalable, and readily amenable if more data points become available. Unlike single-task models, multitask models simultaneously predict numerous properties (tasks) and harness inherent but hidden correlations in data to improve their performance. Such correlation exists, for instance, between \\(T_g\\) and \\(T_m\\), but the exact correlation varies across specific polymer chemistries. Multitask models learn and improve from these varying correlations in data. The training protocol of the multitask deep neural networks follows state-of-the-art methods involving five-fold cross-validation and a consolidating meta learner that forecasts the final property values based upon the ensemble of cross-validation predictors. More details about multitask deep neural networks are provided in the Methods section. Their training process is outlined in Supplementary Figure S2.\n\nFigure 4a shows the color-encoded five-fold cross-validation coefficient of determination (\\(R^2\\)) averages across the five validation data sets for 29 polymer properties. Root-mean-square errors (RMSEs) can be found in Supplementary Table S1. Overall, PG performs best (\\(R^2 = 0.81\\)) but is very closely followed by polyBERT (\\(R^2 = 0.80\\)). This overall performance order of the fingerprint types is persistent with the category averages and properties, except for \\(X_c\\), \\(X_e\\), and \\(\\epsilon_b\\), where polyBERT slightly outperforms PG fingerprints. We note that polyBERT and PG fingerprints are both practical routes for polymer featurization because their \\(R^2\\) values lie close together and are generally high. polyBERT fingerprints have the accuracy of the handcrafted PG fingerprints but are over two orders of magnitude faster (see Figure 3).\n\nFigure 4b shows high \\(R^2\\) values for each meta learner (one for each category), suggesting an exceptional prediction performance across all properties. We train the meta learners on unseen 20% of the data set and validate using 80% of the data set (also used for cross-validation). The reported validation \\(R^2\\) values thus only partly measure the generalization performance with respect to the full data set. Meta learners can be conceived as taking decisive roles in selecting the best values from the predictions of the five cross-validation\nmodels. We use the meta learners for all property predictions in this work. Supplementary Figures S9-S14 show the meta learners’ parity plots.\n\nThe ultrafast and accurate polyBERT-based polymer informatics pipeline allows us to predict all 29 properties of the 100 million hypothetical polymers that were originally created to train polyBERT. Figure 4c shows the minimum, mean, and maximum for each property. Histograms are given in Supplementary Figures S17-S22. Given the vast size of our data set and consequent chemical space of the 100 million hypothetical polymers, the minimum and maximum values can be interpreted as potential boundaries of the total polymer property space. The data set with 100 million hypothetical polymers including the predictions of 29 properties is available for academic use. The total CO$_2$ emissions for predicting 29 properties of 100 million hypothetical polymers are estimated to be 5.5 kgCO$_2$eq (see CO$_2$ Emission section).\n\nOther Advantages of polyBERT: Beyond Speed and Accuracy\n\nThe feed-forward network (last layer in Figure 1b), which predicts masked tokens during the self-supervised training of polyBERT, enables the mapping of numerical latent spaces (i.e., fingerprints) to PSMILES strings. However, because we average over the token dimension of the last latent space to compute fingerprints, we cannot unambiguously map the current polyBERT fingerprints back to PSMILES strings. A modified future version of polyBERT that provides PSMILES strings encoding and fingerprint decoding could involve inserting a dimensionality-reducing layer after the last Transformer encoder. Fingerprint decoders are important elements of design informatics pipelines that invert the prediction pipeline to meet property specifications. We note that the current choice of computing polyBERT fingerprints as pooling averages stems from basic dimensionality reduction considerations that require no modification of the Transformer architecture.\n\nA second advantage of the polyBERT approach is interpretability. Analysing the chemical relevancy of polyBERT fingerprints (as discussed in the Fingerprints section) in greater\ndetail can reveal chemical functions and interactions of structural parts of the polymers. As shown for trained NLP Transformers,\\(^{46}\\) deciphering and visualizing the attention layers of the Transformer encoders can reveal such information. Saliency methods\\(^{47}\\) may explain the relationships between structural parts of the PSMILES strings (inputs) and polymer properties (outputs).\n\nDiscussion\n\nHere, we show a generalizable, ultrafast, and accurate polymer informatics pipeline that is seamlessly scalable on cloud hardware and suitable for high-throughput screening of huge polymer spaces. polyBERT, which is a Transformer-based NLP model modified for the polymer chemical language, is the critical element of our pipeline. After training on 100 million hypothetical polymers, the polyBERT-based informatics pipeline arrives at a representation of polymers and predicts polymer properties over two orders of magnitude faster but at the same accuracy as the best pipeline based on handcrafted PG fingerprints.\n\nThe accurate prediction of 29 properties for 100 million hypothetical polymers in a reasonable time demonstrates that polyBERT is an enabler to extensive explorations of the polymer universe at scale. polyBERT paves the pathway for the discovery of novel polymers 100 times faster (and potentially even faster with newer GPU generations) than state-of-the-art informatics approaches – but at the same accuracy as slower handcrafted fingerprinting methods – by leveraging Transformer-based ML models originallydro developed for NLP. polyBERT fingerprints are dense and chemically pertinent numerical representations of polymers that adequately measure polymer similarity. They can be used for any polymer informatics task that requires numerical representations of polymers such as property predictions (demonstrated here), polymer structure predictions, ML-based synthesis assistants, etc. polyBERT fingerprints have a huge potential to accelerate past polymer informatics pipelines by replacing the handcrafted fingerprints with polyBERT fingerprints. polyBERT may also be\nused to directly design polymers based on fingerprints (that can be related to properties) using polyBERT’s decoder that has been trained during the self-supervised learning. This, however, requires retraining and structural updates to polyBERT and is thus part of a future work.\n\nMethods\n\nPSMILES Canonicalization The string representations of homopolymer repeat units in this work are polymer SMILES (PSMILES) strings. PSMILES strings follow the SMILES\\(^{18}\\) syntax definition but use two stars to indicate the two endpoints of the polymer repeat unit (e.g., [*]CC[*] for polyethylene). The raw PSMILES syntax is non-unique; i.e., the same polymer may be represented using many PSMILES strings; canonicalization is a scheme to reduce the different PSMILES strings of the same polymer to a singel unique canonicalized PSMILES string. polyBERT requires canonicalized PSMILES strings because polyBERT fingerprints change with different writings of PSMILES strings. In contrast, PG fingerprints are invariant to the way of writing PSMILES strings and, thus, do not require canonicalization. Figure 5 shows three variances of PSMILES strings that leave the polymer unchanged. The translational variance of PSMILES strings allows to move the repeat unit window of polymers (cf., white and red box). The multiplicative variance permits to write polymers as multiples of the repeat unit (e.g., two-fold repeat unit of Nylon 6), while the permutational variance stems from the SMILES syntax definition\\(^{18}\\) and allows syntactical permutations of PSMILES strings that leave the polymer unchanged.\n\nFor this work, we developed the canonicalize_psmiles Python package that finds the canonical form of PSMILES strings in four steps; (i) it finds the shortest PSMILES string by searching and removing repetition patterns, (ii) it connects the polymer endpoints to create a periodic PSMILES string, (iii) it canonicalizes the periodic PSMILES string using RDKit\\(^{33}\\)’s canonicalization routines, (iv) it breaks the periodic PSMILES string to create\n![Translational, multiplicative, and permutational variances of PSMILES strings. The gray and red boxes represent the smallest repeat unit of poly(hexano-6-lactam) (Nylon 6). The red box can be translated to match the black box. The dashed boxes show the second smallest repeat unit (two-fold repeat unit) of Nylon 6.](page_184_120_1097_357.png)\n\nFigure 5: Translational, multiplicative, and permutational variances of PSMILES strings. The gray and red boxes represent the smallest repeat unit of poly(hexano-6-lactam) (Nylon 6). The red box can be translated to match the black box. The dashed boxes show the second smallest repeat unit (two-fold repeat unit) of Nylon 6.\n\nthe canonical PSMILES string. The canonicalize_psmiles package is available at https://github.com/Ramprasad-Group/canonicalize_psmiles.\n\nPolymer Fingerprinting Fingerprinting converts geometric and chemical information of polymers (based upon the PSMILES string) to machine-readable numerical representations in the form of vectors. These vectors are the polymer fingerprints and can be used for property predictions, similarity searches, or other tasks that require numerical representations of polymers.\n\nWe compare the polyBERT fingerprints, developed in this work, with the handcrafted Polymer Genome (PG) polymer fingerprints. PG fingerprints capture key features of polymers at three hierarchical length scales.\\(^{8,22}\\) At the atomic scale (1\\textsuperscript{st} level), PG fingerprints track the occurrence of a fixed set of atomic fragments (or motifs).\\(^{23}\\) The block scale (2\\textsuperscript{nd} level) uses the quantitative structure-property relationship (QSPR) fingerprints\\(^{20,36}\\) for capturing features on larger length-scales as implemented in the cheminformatics toolkit RDKit.\\(^{33}\\) The chain scale (3\\textsuperscript{rd} level) fingerprint components deal with “morphological descriptors” such as the ring distance or length of the largest side-chain.\\(^{36}\\) The PG fingerprints are developed within the Ramprasad research group and used, for example, at\nhttps://PolymerGenome.org. More details can be found in References 8,36.\n\nAs discussed recently,6,11 we sum the composition-weighted polymer fingerprints to compute copolymer fingerprints \\( \\mathcal{F} = \\sum_i^N \\mathbf{F}_i c_i \\), where \\( N \\) is the number of comonomers in the copolymer, \\( \\mathbf{F}_i \\) the \\( i \\)th comonomer fingerprint, and \\( c_i \\) the fraction of the \\( i \\)th comonomer. This approach renders copolymer fingerprints invariant to the order in which one may sort the comonomers and satisfies the two main demands of uniqueness and invariance to different (but equivalent) periodic unit specifications. Contrary to homopolymer fingerprints, copolymer fingerprints may not be interpretable (e.g., the composition-weighted sum of the fingerprint component “length of largest side-chain” of two homopolymers has no physical meaning).\n\nMultitask Neural Networks Multitask deep neural networks simultaneously learn multiple polymer properties to utilize inherent correlations of properties in data sets. The training protocol of the concatenation-conditioned multitask predictors follows state-of-the-art techniques involving five-fold cross-validation and a meta learner that forecasts the final property values based upon the ensemble of cross-validation predictors.6,7,11 Supplementary Figure S2 details this process. After shuffling, we split the data set into two parts and use 80\\% for the five cross-validation models and for validating the meta learners. 20\\% of the data set is used for training the meta learners. We perform data set stratification of all splits based on the polymer properties. All parameters of the neural networks, such as the number of layers, number of nodes, dropout rates, and activation functions, are optimized using the Hyperband method48 of the Python package KerasTuner.49 The multitask deep neural networks are implemented using the Python API of TensorFlow.50\n\nCO$_2$ Emission\n\nExperiments were conducted using a private infrastructure, which has an estimated carbon efficiency of 0.432 kgCO$_2$eq kWh$^{-1}$. A cumulative of 31 hours of computation was performed\non four Quadro-GP100-16GB (thermal design power of 235 W) for training polyBERT. Total emissions are estimated to be 12.6 kgCO_2eq. The total emissions for predicting 29 properties for 100 million hypothetical polymers are estimated to be 5.5 kgCO_2eq. Estimations were conducted using the Machine Learning Impact calculator presented in Reference 51.\n\nData and Code Availability\n\nThe polyBERT code and data set of 100 million hypothetical polymers with the predictions of 29 properties are available for academic use at https://github.com/Ramprasad-Group/polyBERT. The trained polyBERT model is available at https://huggingface.co/kuelumbus/polyBERT. The Python package for canonicalizing PSMILES strings is available at https://github.com/Ramprasad-Group/canonicalize_psmiles. polyBERT-based property predictions will be made accessible through the polymer informatics platform Polymer Genome at https://PolymerGenome.org.\n\nDeclaration of Interests\n\nR.R. is the founder of the company Matmerize, Inc., that intends to provide polymer informatics services. A provisional patent on polyBERT has been filed by R.R. and C.K.\n\nAcknowledgement\n\nC.K. thanks the Alexander von Humboldt Foundation for financial support. 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Click to download.\n\n• PolyBERTSI.pdf"} {"paper_id": "prb47", "title": "Artificial fingerprints engraved through block-copolymers as nanoscale physical unclonable functions for authentication and identification", "text": "# Abstract\n\nBesides causing financial losses and damage to the brand's reputation, counterfeiting can threaten the health system and global security. In this context, physical unclonable functions (PUFs) have been proposed to overcome limitations of current anti-counterfeiting technologies. Here, we report on artificial fingerprints that can be directly engraved on a wide range of substrates through self-assembled block-copolymer templating for secure authentication and identification. We show that engraved nanopatterns are unclonable unique objects that endow high encoding capacity density while satisfying main requirements of PUFs, including high aging and thermal stability. Besides showing that these nanopatterns can be encoded in binary code matrices with high entropy and high uniqueness, we propose a strategy for robust authentication and identification in real-world scenarios based on computer vision concepts. These results can shed new light on the realization of PUFs embracing the inherent stochasticity of self-assembled materials at the nanoscale.\n\nPhysical sciences/Nanoscience and technology/Nanoscale materials/Molecular self-assembly \nPhysical sciences/Nanoscience and technology/Nanoscale devices\n\n# Introduction\n\nCounterfeiting represents a growing problem for society that has not only enormous economic implications, from manufacturing of goods to specialized technologies, but represents a threat for the entire security and health systems.1 In the current era of Internet of Things (IoT), widely exploited anti-counterfeiting techniques based on tags such as graphical barcodes, watermarks and holograms realized through a deterministic process endow low complexity and high predictability, allowing easy forgery and cloning by counterfeiters.2 Also, widely exploited software-based authentication/identification systems endow intrinsic vulnerability due to electromagnetic interference and cyber-attacks.3 To overcome main limitations of current anti-counterfeiting technologies, hardware encryption systems based on physical unclonable functions (PUFs) have attracted a growing interest.4,5 These are physical one-way functions that enable the generation of a secret key based on the inherent physical characteristics of a physical system/device, where the uniqueness of the key relies on uncontrollable variabilities and high randomness of the physical system even when realized through the same fabrication process.6 In this framework, new perspectives for the realization of PUF can be enabled by exploiting the true essence of nanotechnology where the fabrication of materials and systems at the nanoscale is often hindered by unpredictable disturbances and fluctuations.7 This is because at this scale the influence of thermal and statistical fluctuations cannot be avoided, resulting in output material structures and properties that are not simply determined by known inputs. Leveraging the inherent stochasticity of nanotechnologies, a wide range of physical unclonable functions have been demonstrated by employing different taggants and detection methods. This includes random fractal structures,8 fluorescent, photoluminescent and chromic materials,9–12 spontaneously formed core-cell nanoparticles,13 3D printed and nanoimprinted materials,14,15 plasmonic nanomaterials,16–18 graphene-based devices,19 as well as metallic nanopatterns replicated from molecular self-assembly20,21. These techniques mainly imply the realization of unique nanopatterned devices as anti-counterfeiting tags that can be affixed to products requiring protection, but that can potentially be removed or detached through appropriate chemical/physical treatments.\n\nHere, we report on artificial nano fingerprints engraved in a wide range of materials as disorder based PUFs for secure authentication and identification. Besides proposing a strategy for user-independent extraction of nanopatterns without artifacts from micrographs, we show that by exploiting local features of nanopatterns it is possible to encode nano fingerprints in unique binary code matrices endowing high bit uniformity and entropy. Finally, we propose and test a computer vision-based strategy for robust authentication/identification through artificial fingerprints in real-world scenarios, opening new perspectives for the realization of PUF that utilizes the intrinsic unpredictability of self-assembling materials as a source of randomness.\n\n# Results\n\nSince ancient Babylon, fingerprints have been exploited as unique identifiers to secure commercial transactions, as testified by clay seals attached to their business documents. 22 In the era of Internet of Things, fingerprint matching is largely deemed to be a secure system for both authentication (i.e., matching a person’s biometric template) and identification (i.e., determining the identity of a person), as schematized in Fig. 1 a. Here, the validation and verification of a person’s identity are based on unique physical characteristics – biometrics – of their fingerprints. 23 The security of this process is guaranteed by the fact that, although two or more fingerprints may share the same global features, there are currently no known pairs of fingerprints with identical pattern of local features, also called minutiae points. 24 Besides the individuality of the fingerprint, the premises for fingerprint authentication/identification rely on the pattern persistence, meaning that the characteristics of fingerprints must be stable over time. 25 Similarly, artificial fingerprints can be exploited as PUFs for the authentication and/or identification of a product in the supply chain (the workflow of PUF generation, database initialization and authentication is schematized in Fig. 1 b). Inspired by fingerprint biometrics, we developed a process to directly transfer a nano fingerprint pattern into a wide range of target substrates, as schematized in Fig. 1 c. This process is based on i) molecular self-assembly of block copolymers (BCPs) on the target substrate, ii) selective removal of one of the BCP phase, and iii) pattern transferring to the target substrate. Molecular self-assembly relies on phase separation of chemically distinct and thermodynamically incompatible polymeric components of BCPs that occurs randomly under thermal fluctuations, resulting, under proper conditions, in lamellar fingerprint-like patterns (Supplementary Note 1). After achieving the self-assembled pattern, one of the two polymers comprising the BCP can be selectively removed, resulting in the formation of a disordered nanolithographic mask. Figure 1 d reports an example of self-assembled lamellar BCP showing fingerprint-like global features (fabrication details in Methods). Notably, these patterns are characterized by the presence of spatially distributed local features (defect points) closely resembling minutiae points of human fingerprints. In case of lamellar patterns, the defect taxonomy of both positive and negative phases includes terminal points, 3-way junctions and dots (Fig. 1 e). It is worth mentioning that typical features of lamellar structures such as typical dimensions, periodicity, correlation length, defect density and line-edge roughness can be tailored by appropriate choice of BCP molecular weights and processing conditions. 26, 27 The polymeric fingerprint-like pattern can be then transferred to the target substrate through selective reactive ion etching (RIE) or wet chemical etching, depending on the material of the target substrate. Examples of patterns successfully transferred to diamond, Si, quartz and Si2 target substrates are reported in Fig. 1 f-i (details of pattern transfer on different substrates in Methods). Additionally, patterns have been demonstrated to be transferable on metallic (Cu, Cr, Co, W, CoCrPt, Permalloy), 28–33 dielectric (Si3N4), 34 semiconductor (ITO, graphene) 28, 33 and flexible substrates 35, 36. The ability to conduct the self-assembly process of BCP on various materials opens the potential for directly engraving artificial fingerprints at the nanoscale onto a wide range of devices and products, including screens and microchips.\n\nAs for human fingerprints, a critical step for exploiting nanoscale fingerprints as PUFs is represented by the automatic extraction of the fingerprint pattern including minutiae (defects) from input images. This process is crucial and may heavily rely on the quality of the input fingerprint micrographs. Since ridge structures in poor-quality fingerprint images can be not well defined, the pattern can be not correctly detected, and spurious defects can be created while genuine defects can be ignored. To increase the robustness of pattern extraction with respect to the quality of input fingerprint images, we adapted a fingerprint enhancement algorithm able to adaptively improve the clarity of ridge and valley structures based on estimated local ridge orientation and frequency 37 (Fig. 2 a, details in Methods). This allows to obtain a binarized genuine fingerprint pattern that can be exploited to investigate BCP morphological parameters including defect localization (defect maps), line period, line width, line-edge roughness, line-width roughness, and correlation length (correlation maps) 38 through an automated analysis (Methods). An example of the process flow, from SEM image to fingerprint pattern enhancement and defect localization, is reported in Fig. 2 b. A comparison of a binarized pattern obtained by fingerprint enhancement algorithm and other common binarization thresholding techniques on the same micrograph is reported in Fig. 2 c (raw micrograph in Supplementary Figure S1). Here, the white phase of binarized images represents ridge lamellae structures, while the black phase represents valleys. Fingerprint pattern enhancement outperforms traditional thresholding techniques, allowing to obtain a binarized map with reduced noise and with a reduced number of artifacts (additional details in Supplementary Figure S2). Notably, whereas the effectiveness of traditional thresholding techniques relies on the image quality, contrast and brightness, fingerprint enhancement enables the automatized extraction of patterns even in case of poor quality and low contrast images (Supplementary Figure S3). Moreover, it eliminates the need for image-dependent adjustment of binarization parameters, thereby avoiding any potential bias from the user. As depicted in defect maps (Fig. 2 c), the reduced number of artifacts in images processed with fingerprint enhancement results in a limited number of spurious defects. Also, this approach enables the generation of correlation maps with a decreased noise level (Fig. 2 d). A statistical analysis, performed by considering SEM micrographs acquired on different areas of the same patterned sample, allows a quantitative evaluation on the effect of the binarization extraction of defects and correlation length of the structures. Figure 2 d reports the defect density obtained by analyzing images binarized with the different techniques. As evident, fingerprint enhancement results in a lower mean defect density, quantitatively showing the possibility of reducing the counting of spurious defects through this binarization technique. Furthermore, larger defect distributions obtained by conventional binarization techniques are due to overestimation of defects in images not properly binarized through these techniques (details in Supplementary Figure S4). More in detail, the radar chart in Fig. 2 e shows that conventional binarization techniques result in a higher overestimation of certain types of defects. Since defect density is inversely related to the dimensions of lamellae orientation domains, 38 fingerprint enhanced images result in a higher mean value of correlation length (Fig. 2 f). All these observations show that binarization through the fingerprint enhancement algorithm allows to retrieve a genuine fingerprint pattern that, besides reducing artifacts, is user independent and can automatically extract relevant information even from poor-quality images and images acquired with different contrast/brightness conditions. These are fundamental aspects for correct authentication and/or identification of PUFs based on BCP nanopatterned substrates in real-world scenarios.\n\nThese artificial fingerprints can be considered as PUF where the nanopattern represents the unique response r when the surface is scanned with a focused beam of electrons representing the input challenge c. In this context, the uniqueness of the PUF response r = f(c) is guaranteed by the intrinsic randomness of the self-assembly process of pattern formation, thereby relying on the internal and uncontrollable manufacturing variability of the system to establish the unique input/output relation f(∙). Note that the unique response of the PUF pattern can be probed also through other imaging techniques, such as atomic probe microscopy (AFM). A first approach to exploit nanopatterns as physical unclonable functions is to generate a cryptographic binary code response of the system based on local features of nanoscale morphologies, as similarly reported in previous works. 20, 39 In case of BCP templated patterns, the nano fingerprint feature can be converted to a binary code matrix by defining each pixel of the matrix as 1-bit or 0-bit depending on the presence or absence of minutiae in the corresponding spatial location, respectively, as reported in Fig. 3 a. In other words, the binary code map can be built based on the defect map (in this case defects of the positive phase were considered). This allows the realization of the corresponding binary code matrix reported in Fig. 3 b. Here, we show that the selection of the code matrix pixel size cannot be arbitrary but should be based on morphological characteristics of the pattern. Indeed, given a pattern area, the pixel size should be selected to maximize the randomness and uniqueness of encoded binary matrices. Figure 3 c reports the bit uniformity and fractional hamming distance (HD) (i.e., the percentage of bits that differs between two binary code matrices) between different binary code matrices as a function of the pixel size calculated by considering 200 different nanopattern micrographs (area of 2.38 × 2.38 µm2). As can be observed, the mean value of fractional HD of around 0.5 (meaning that code matrices are different and distinguishable) is achieved in correspondence of a pixel size of 238 nm when a bit uniformity of around 0.5 can be observed (i.e., when different binary code matrices have almost equal numbers of 0 and 1) (the relationship between fractional HD in between patterns and bit uniformity of patterns is reported in Fig. 3 d). This is because bit uniformity is beneficial to achieve the maximum randomness, 12 as testified by the maximum pattern entropy approaching the ideal value of 1 when bit uniformity is close to 0.5 (Fig. 3 e, fractional HD between different code matrices as a function of the entropy of patterns in Supplementary Figure S5). It is noteworthy that, a bit uniformity (and fractional HD) of 0.5 can be observed when the pixel size approximately coincides with the correlation length of BCP patterns (ξ = 207 ± 18 nm, details in Methods). It turns out that through appropriate selection of the pixel size of the binary code matrix (in this case 238 nm), it is possible to obtain binary code matrices with bit uniformity close to the ideal value of 0.5 (in this case 0.52 ± 0.06) (Fig. 3 f, Supplementary Figure S6), with unit entropy close to the ideal value of 1 (Supplementary Figure S7), and to achieve a distribution of fractional HD between different binary code matrices with mean value of 0.50 ± 0.06 (Fig. 3 g, fractional HD for each couple of binary code matrices in Fig. 3 h). These results confirm the high randomness of the binarized code matrix obtained from local nanopattern features. In this context, the encoding capacity of the system cp, defined as the number of possible responses exhibited by a random pattern where c is the number of responses for each pixel while p is the image area in pixels, is inherently related to the morphological properties of the nanopattern. The encoding capacity of the system can be therefore improved through two strategies: i) by increasing the image area (i.e., increasing the number of pixels without changing the pixel size) and/or ii) by reducing the pixel size of the binarized code matrices while maintaining bit uniformity and fractional inter-HD of ~ 0.5. Concerning the first strategy, Fig. 3 i reports the maximum encoding capacity of binary code matrices (c = 2) as a function of the image area (by considering the selected pixel size of 238 nm). Interestingly, an encoding capacity of the same order of magnitude of the world population can be achieved by considering an image with area below 2 µm2, while an encoding capacity larger than the number of atoms in the known universe is achievable by considering an image area larger than 12 µm2, showing the high density of encoding capacity of the system. Concerning the second strategy that aims to increase the encoding capacity of the system for unit area, it can be achieved by proper selection of molecular weight of involved polymers and processing conditions to increase the defect density while reducing the correlation length of the system 40 (examples in Supplementary Figure S8). The authentication protocols based on cryptographic codes obtained from fingerprint patterns PUFs can be further refined by considering not only the presence of defects in the pixel area but also defect density (Supplementary Figure S9) and/or defect types (Fig. 3 j, additional examples in Supplementary Figure S10).\n\nThe comparison of a binarized code matrix with a database code matrix, as required for authentication/identification, implies no misalignment of the image acquired by the end user with the corresponding image stored in the database. Even small translations, rotations and/or deformations of the end user image can cause incorrect authentication/identification due to a different conversion of the fingerprint pattern to the binary code matrix. Indeed, these transformations can cause bit flips in the related binary code matrix due to the different spatial localization of defects (Supplementary Figure S11). Here, we show that the robustness of the authentication/process in real-world scenarios can be enhanced by exploiting matching algorithms based on computer vision concepts, without the need of extracting a binary code matrix from the nanopattern. For this purpose, we synthesized 100 different PUF nanopatterns engraved on a SiO2 substrate, and we built a database consisting of micrograph images of the corresponding fingerprint patterns acquired by a first scan (details in Methods, Supplementary Figure S12). To obtain a set of images used for testing (test set), in a second scan we collected micrographs of the same PUF patterns. Authentication/identification were tested by comparing an image from the test set with a database image from the database, where the genuine nanopattern is obtained through the fingerprint enhancement algorithm discussed before. Noteworthy, the obtained binarized lamellar patterns inherently endow bit uniformity close to 0.5 (0.496 ± 0.008) and unit entropy close to 1 (values evaluated on the database set of images, details in Supplementary Figure S13). For a given pair of previously binarized images, which we will refer to as database and test image, respectively, we aim at determining whether they represent the same nanopattern. As expected in real-world scenarios, slight shifts, rotations, and different magnifications are present between the database and the test set image of the same nanopattern. Given a database/test pair of images, a set of matching key points between the two images are computed through a Scale-Invariant Feature Transform (SIFT) algorithm (other methods such as Speeded Up Robust Feature, SURF, algorithm and Oriented FAST and Rotated BRIEF, ORB, were tested and give similar results) and a FLANN (Fast Library for Approximate Nearest Neighbors)-based matcher. Then we select a few points providing the best matches (we tested between 10–15, not significantly affecting the results), and use those as a guide to build a homography transformation to map the test image on top of the database one. Examples of feature matching and overlapping of images by considering two images of the same nanopattern (example of successful matching) and on two images of different nanopatterns (example of non-successful matching) are reported in Fig. 4 a and b, respectively. If the two images are taken from the same nanopattern and thus only differ by slight deformations (e.g., rotation, shift, etc.), the homographic transformation automatically corrects for these effects, so that the resulting image should overlap with the database one, as can be evaluated by superimposing the test image on the top of the database image through the XOR operation (Fig. 4 a, Supplementary Figure S14). On the other hand, if the two images are from unrelated samples, the transformation obtained from the matching algorithm will be unable to return an image with a reasonable overlap with the database (Fig. 4 b, Supplementary Fig. 15). The quantification of the superposition is performed by considering the fractional HD calculated on the whole binary image obtained by superimposing the test image on top of the database image through XOR operation (details of the matching algorithm in Methods). Figure 4 c reports the fractional HD matrix obtained by comparing images from the test set with the database. As can be observed, HD values closer to 0 can be observed while comparing images of the same PUF (i.e., the test image has a small number of bit values that differs from the database one after the homographic transformation), while HD values of approximately 0.5 can be observed while comparing images of different PUFs. A clear separation of intra and fractional inter-HD distributions can be observed in Fig. 4 f, further showing the robustness of the authentication/identification protocol (mean values and std. dev. of inter and intra-HD distributions are 0.14 ± 0.01 and 0.500 ± 0.003, respectively). Here, a HD-based decision threshold of 0.45 can be identified (Supplementary Figure S16). It is worth noticing that the extraction of the binarized fingerprint pattern from the micrograph image through the fingerprint enhancement algorithm provides noise robustness to the authentication process, a crucial aspect for exploiting image based PUFs for real-world applications. In this context, clear separation of fractional intra and inter-HD distributions can be observed also by considering a test set of images acquired by different users operating with different equipment (details in Methods, Supplementary Figure S17 and Supplementary Figure S18), further corroborating the robustness of the authentication/identification protocol. An analysis of the stability shows that PUFs can be correctly authenticated/identified even after 6 months when the sample was left in normal ambient conditions (Fig. 4 d and g), revealing long-term reliable operation. Furthermore, the high thermal stability of PUFs was demonstrated by exposing samples to the harsh conditions of 200°C for 30 minutes, where the PUF also experienced a high heating rate of ~ 15°C s–1 and a high cooling rate of ~ 0.8°C s–1. Fractional intra and inter-HD distributions after thermal treatment still show clear separation (Fig. 4 e and h). Details on intra and fractional inter-HD mean values and standard deviations evaluated for each test are reported in Supplementary Table 1. In all these cases, successful authentication/identification of all PUF patterns without any false positive or false negative have been achieved by exploiting the decision threshold of 0.45 previously evaluated through the comparison of the test set of images with the database.\n\n# Discussion\n\nResults show that morphological characteristics of artificial fingerprints realized with a bottom-up approach through BCP self-assembly can be exploited for the realization of physical-disorder-based tags for authentication/identification. While global features of the nanopattern, such as correlation length and defect density, can be deterministically controlled by structural and processing parameters (e.g. molecular weights of the BCP, processing temperature and time), each nanopattern is a unique entity with peculiar local features thanks to the randomness arising from thermodynamic instabilities during the self-assembly process. In this framework, results show that the coexistence of deterministic and stochastic features in the same nanopattern can be further explored for increasing the encoding capacity density of the system, as revealed by the intrinsic relationship between the pixel size of the encoded binary code matrix, its bit uniformity and entropy, and the correlation length of the nanopattern. Besides the shown possibility of using additional morphological features such as defect types to further increase the encoding density, additional morphological parameters such as the line-edge roughness, line-width roughness and/or the 3D morphology obtainable through scanning probe microscopies can be explored (example in Supplementary Figure S19). Indeed, since it cannot be excluded a priori that a nanopattern can be cloned by using advanced and expensive lithographic tools with resolution < 10 nm (even if this is unlikely), line-edge roughness, line-width roughness, and the 3D morphology of systems are unlikely to be reproducible. In this context, it is worth noting that recent advancements in the synthesis of BCP with covariant properties allow for on-demand tuning of morphological characteristics (e.g., periodicity, line-edge roughness), long-range order and defectiveness.¹\n\nDifferently from previous works where nanoscale tags are affixed to the substrate of interest,²⁻²⁰⁴², the here proposed artificial fingerprint is directly engraved on the target substrate and, thus, cannot be removed (unless the substrate is mechanically scratched, but this will leave marks that can be considered as a trace of counterfeiting). As an important consequence, the PUF robustness and environmental stability relies on the physical/chemical/mechanical properties of the engraved substrate. This means that tailored choice of the substrate would enable the realization of PUF devices working even when exposed to harsh conditions (high/low temperatures, exposure to chemicals, mechanical agents, radiations, etc.) as required, for example, for space applications. In addition, these PUFs can be included in conventional tags such as QR codes in the context of a multiple-level security strategy. For anticounterfeiting applications, nanometer-scale artificial fingerprints can be exploited for secure authentication/identification by taking into advantage also that these tags are difficult to localize without an a-priori knowledge of their location. While on one hand the requirement of an electron microscope to challenge the PUF with a scanning focused electron beam can represent an obstacle (despite recent advances in low-cost and portable SEM equipment), on the other hand the requirement of a specialized equipment can further enhance the security of the authentication/identification process in a multiple-level security scenario. Furthermore, it is worth noticing that BCP-templating is compatible with CMOS technology,⁴³ allowing the integration of these PUF devices with conventional electronics. Note that the possibility of realizing fingerprints directly on chips to assess their legitimacy can be crucial to face back doors and hidden functionalities of fraudulent clone chips that, in the framework of global shortage of chips, can threaten global security.⁴⁴ All these characteristics enable artificial fingerprints based on BCP-templated substrates to comply with basic requirements for commercial applications, taking advantage of the intrinsic low-cost of BCP templating on a large scale that easily allows mass production.\n\n# Conclusions\n\nIn conclusion, we show that artificial fingerprints for counterfeiting applications can be engraved on a wide range of target substrates including - but not limited to - diamond, Si, SiO₂ and quartz to realize disorder-based PUFs readable through electron microscopy. By proposing a user-independent strategy for successfully extracting the nanopattern even from low-quality micrographs, we show that engraved nanopatterns can be encoded in binary code matrices endowing high bit uniformity and uniqueness. In this context, we show the importance of an appropriate encoding of nanopattern in the corresponding binary code matrix depending on morphological nanopattern features, including defects and correlation length. In addition, we propose a computer vision-based strategy that enables robust authentication/identification processes, as demonstrated by testing 100 PUF devices. These results shed new light on the realization of PUF that embraces the inherent stochasticity of nanoscale self-assembled materials as a randomness source.\n\n# Methods\n\n## Fabrication of self-assembled artificial fingerprint patterns by block copolymers\n\nThe surface of different materials (silicon, silicon oxide, quartz, diamond) were functionalized by RCP grafting process to promote the perpendicular orientation of lamellar BCP nanostructures. First, the substrates were cleaned in an ultrasonic bath in acetone followed by isopropyl alcohol, and functionalized by O₂ plasma treatment at 130 W for 20 min. Then, a solution of RCP (18 mg in 2 ml of toluene) was spincasted for 60 s at 3000 rpm onto the functionalized substrates. The grafting process was performed in a rapid thermal processing (RTP) machine Jipelec JetFirst200 at high temperature (Tₐ = 290°C) for an annealing time (tₐ) of 300 s, in a N₂ environment with a heating rate of 15°C s⁻¹. Automatic cooling to room temperature was set to 240 s. The non-grafted polymeric chains were then removed by sonication in toluene for 6 min, resulting in a final grafted RCP layer thickness of ∼7 nm, as measured by spectroscopic ellipsometry (alpha-SE ellipsometer from J.A. Wollam Co.). BCP solution (18 mg in 2 ml of toluene) was then spincasted over the RCP functionalized surface at 3000 rpm for 60 s resulting in a total BCP thickness of 35 nm. The self-assembly was promoted by RTP at 230°C for 600 s in a N₂ environment with a heating ramp of 15°C s⁻¹ and automatic cooling to room temperature for 240 s. Selective removal of the PMMA phase of self-assembled BCP was achieved by exposure of the samples to ultraviolet radiation (5 mW cm⁻², λ = 253.7 nm) for 180 s followed by isotropic O₂ plasma etching (40 W for 30 s).\n\nThe synthesis of α-hydroxy ω-Br polystyrene-stat-polymethyl methacrylate (PS-stat-PMMA) random copolymer (RCP) with M_w = 14.60 kg mol⁻¹, styrene fraction (f_PS) of 0.59 and polydispersity index (PDI) of 1.30, is described elsewhere. Lamellar-forming polystyrene-block-polymethyl methacrylate (PS-b-PMMA) BCP with M_w = 66 kg mol⁻¹, f_PS = 0.50 and PDI = 1.09, was purchased from Polymer Source Inc. and used without further purification. Toluene (99.8% anhydrous), acetone (99.5% anhydrous) and isopropyl alcohol (98% anhydrous) were purchased from Sigma Aldrich. Polymethyl methacrylate (PMMA) A4 positive electron-beam resist was purchased from MicroChem. Methyl isobutyl ketone (MIBK) developer was purchased from KemLab.\n\n## Engraving artificial nano fingerprints on target substrates and materials\n\nThe pattern transfer of the fingerprint pattern onto the substrate surface was performed by reactive ion etching (RIE) with different chemistries depending on the etched material. Silicon etching was achieved by SF₆/C₄F₈ RIE with ICP plasma of 750 W and RF table of 35 W. Silicon oxide and quartz etching was achieved by CHF₃/Ar RIE and power of 35 W. Diamond etching was achieved by O₂ RIE with ICP plasma of 2000 W and RF table of 200 W.\n\n## Morphological characterization of nanopatterns\n\nThe micrographs of artificial fingerprints were acquired by FEI Inspect-F field emission gun scanning electron microscope (FEG-SEM) using an Everhart-Thornley secondary electron detector (ETD). Additionally, a dual-beam SEM FEI Quanta 3D FEG was employed for authentication/identification of artificial fingerprints, enabling the collection of the SEM micrographs through alternative instrumentation.\n\n## Fingerprint enhancement algorithm for nanopattern binarization\n\nThe fingerprint enhancement algorithm exploited for pattern binarization was adapted from the algorithm described in ref. 37 by exploiting the fingerprint_enhancement python library. Parameters of the enhance_Fingerprint function were adapted on the basis of the pitch of the lamellar structures, obtained from the Fourier transform of the corresponding nanopattern image, and the resolution of the SEM image. The fingerprint enhancement binarization was compared to standard binarization techniques implemented through auto-local thresholding methods with default parameters of ADAblock. 38\n\n## Characterization of artificial nano fingerprints properties\n\nSpatial coordinates, types, and density of topological defects of binarized nanopatterns, as well as the analysis of correlation length, was performed through the automated defect analysis tool ADAblock described in ref. 38, modified to be integrated into an automated analysis process including the binarization through fingerprint enhancement algorithm. The analysis of Fig. 3 was performed over 200 nanopattern SEM images with an original area of 2.64 × 3.08 µm² acquired over different areas of the sample, while the correlation length of nanopatterns were evaluated by considering 11 images with an area of 4.14 x 3.56 µm² of the same nanopatterned sample (here, only images with a reduced magnification were used to have a higher grain size/image dimension ratio as required for the analysis of correlation length). The binary code matrices have been obtained from 200 SEM images of nanopattern micrographs by considering a central square area of the SEM image of 2.38 × 2.38 µm². The analysis of Fig. 2 was performed over about 30 images for each binarization technique, in fact, a couple of these images were discarded. The defect density reported in Fig. 2e is expressed as the median value of the density for the different defect types evaluated over about 30 images.\n\nThe bit uniformity (pᵢ) of the i-th binarized code matrix, defined as the distribution of 1s and 0s in the bit stream, have been calculated through the equation:\n\n$$\np_{i}=\\frac{1}{n}\\sum _{k=1}^{n}{R}_{i,k}\n$$\n\nwhere Rₖ is the binary bit response of the k-th pixel of the i-th binarized code matrix, while n is the number of pixels of the code matrix. A value of 1 means that all responses Rᵢ,ₖ of the i-th pattern are logic-1. The unit entropy of the i-th binarized code matrix have been evaluated through the Eq. 1:\n\n$$\nE_{i}= -\\left[p_{i}{\\text{log}}_{2}{p}_{i}+(1-{p}_{i}){\\text{log}}_{2}{p}_{i}(1-{p}_{i})\\right]\n$$\n\n## Fabrication of PUF devices based on artificial fingerprints at the nanoscale\n\nNanoscale PUF devices with dimensions of 3 µm x 3 µm were realized by creating a metallic frame surrounding the area of interest of the previously nanopatterned substrate, as shown in Supplementary Figure S12. For this purpose, the area of interest was defined by electron-beam lithography (EBL) in a dual-beam SEM FEI Quanta 3D FEG on PMMA A4 positive-tone resist on the patterned SiO₂ substrate. After the development with MIBK:IPA (3:1) developer solution, a double layer of Ti/Au (2 nm and 3 nm of thickness, respectively) was deposited by RF sputtering followed by a lift-off process under sonication.\n\n## Computer vision-based matching algorithm\n\nThe matching algorithm has been implemented by exploiting computer vision algorithms of OpenCV python library. As the first step, the image was cropped of 1.04 µm on each side of the SEM image to remove the Au frame of the PUF device that can interfere with the binarization process. The resulting image has an area of 1.47 x 2.06 µm² or 1.49 x 2.07 µm² on which to perform the following analysis. Then, the homographic transformation, required for overlapping the test image on top of the database image, was calculated through SIFT (SURF or ORB were tested to give similar results) and a FLANN-based matcher from OpenCV python library. Note that, after performing the homographic transformation, the transformed image (no longer binary) is binarized to 1 and 0 values through a thresholding technique, where the threshold was chosen halfway between the minimum and the maximum values. Then, quantification of the superposition was performed by calculating the fractional HD between considered images (calculation was performed over 987 x 708 or 996 x 717 pixels). Overlapped images in Fig. 4a and b have been obtained by superimposing test image after homographic transformation and the database image with XOR operation between the two. Note that XOR operation returns a 0-pixel value if the corresponding pixel of the test and database image are characterized by the same bit value, 1-pixel value otherwise. In these terms, an overlapped image with a high number of 0 values represents good overlapping between test and database images. Note that performing fractional HD is nothing but performing the XOR operation over two images, then summing all pixel values of the obtained overlapping image and normalizing over the number of pixels. Given the sharp nature of the binarized images, we typically obtain very clean cancellations when a good match is found, consistently leading to a clear separation of the fractional HD between good and bad matches.\n\n## Tests of PUF robustness\n\nThe thermal stability of PUF devices was tested by subjecting the samples to a heat treatment by the rapid thermal annealing at 200°C for 30 minutes. The annealing was performed in a RTP Jipelec JetFirst200 in N₂ environment and heating rate of 15°C s⁻¹ which puts the device into even harsher conditions when compared to conventional furnace heating. Then, an automatic cooling to room temperature was set to 240 s. 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Chop shop electronics. *IEEE Spectr* **50**, 41–45 (2013).\n\n# Supplementary Files\n\n- [SupplementaryMaterial.docx](https://assets-eu.researchsquare.com/files/rs-4170364/v1/32c5652f8bc6379746cfab96.docx)"} {"paper_id": "prb48", "title": "Lateral parabrachial FoxP2 neurons regulate respiratory responses to hypercapnia", "text": "# Abstract\n\nAlthough CGRP neurons in the external lateral parabrachial nucleus (PBel) neurons are critical for cortical arousal in response to hypercapnia, activating them has little effect on respiration. However, deletion of all Vglut2 expressing neurons in the PBel region suppresses both the respiratory and arousal response to high CO2. We identified a second population of non-CGRP neurons adjacent to the PBel group in the central lateral, lateral crescent and Kölliker-Fuse parabrachial subnuclei that are also activated by CO2 and project to the motor and premotor neurons that innvervate respiratory sites in the medulla and spinal cord. We hypothesize that these neurons may in part mediate the respiratory response to CO2 and that they may express the transcription factor, Fork head Box protein 2 (FoxP2), which has recently been found in this region. To test this, we examined the role of the PB FoxP2 neurons in respiration and arousal response to CO2, and found that they show cFos expression in response to CO2 exposure as well as increased intracellular calcium activity during spontaneous sleep-wake and exposure to CO2. We also found that optogenetically photo-activating PB FoxP2 neurons increases respiration and that photo-inhibition using archaerhodopsin T (ArchT) reduced the respiratory response to CO2 stimulation without preventing awakening. Our results indicate that PB FoxP2 neurons play an important role in the respiratory response to CO2 exposure during NREM sleep, and indicate that other pathways that also contribute to the response cannot compensate for the loss of the PB FoxP2 neurons. Our findings suggest that augmentation of the PB FoxP2 response to CO2 in patients with sleep apnea in combination with inhibition of the PBel CGRP neurons may avoid hypoventilation and minimize EEG arousals.\n\n[Biological sciences/Neuroscience/Neural circuits](/browse?subjectArea=Biological%20sciences%2FNeuroscience%2FNeural%20circuits) [Health sciences/Neurology/Neurological disorders](/browse?subjectArea=Health%20sciences%2FNeurology%2FNeurological%20disorders)\n\n# Introduction\n\nPatients with obstructive sleep apnea (OSA) have recurring arousals over the course of a night with loss of the upper airway muscle tone that results in obstruction of the airway, causing a reduction (hypopnea) or cessation (apnea) of ventilation, despite persisting respiratory efforts. The interruption of ventilation causes progressive hypercapnia and hypoxia, which in turn causes increased ventilatory effort. This increased ventilatory effort is measured by increased activity (as measured by EMG) of muscles related to ventilation, including both airway dilators such as the genioglossus (GG) and pump muscles such as the diaphragm, 1–6 and is associated ultimately with cortical arousal that further augments respiratory efforts that open up the airway and re-establish ventilation 5,7–9. However, these repeated awakenings cause sleep fragmentation, which is associated with deleterious cognitive, metabolic and cardiovascular consequences 5,7,8,10–15. The CO2 blood levels and ventilation increase rapidly during an apnea, but the fall in blood oxygenation typically lags behind the changes in CO2 blood levels and correlates poorly with the onset of the arousal 16–18. We have therefore developed a mouse model of the repeated periods of exposure to elevated CO2 and brief arousal that mimics the events in OSA 19–21. This model permits selective genetic targeting and manipulation of brain circuits that mediate the respiratory and EEG responses during the period of CO2 elevation associated with an apnea.\n\nOur earlier work supports the hypothesis that the brain circuits that respond to hypercapnia by elevating respiratory efforts may be distinct from those that cause cortical arousal 19,20,22. Specifically, we found that glutamatergic neurons (i.e., expressing Vglut2) in the lateral PB complex show cFos activation during elevated CO2, and that deletion of Vglut2 from these neurons in the lateral PB (LPB) caused both a delay in arousal and reduced ventilation to a CO2 stimulus 20. However, the two aspects of CO2 responses were not correlated across our deletions, which varied in their precise location, suggesting that the ventilatory and arousal responses were due to separate populations of glutamatergic neurons in the lateral PB region 20. We later found that a subset of these neurons in the external lateral parabrachial nucleus that express the peptide CGRP (PBelCGRP neurons) play a critical role in transmitting the arousal signal to cause EEG desynchronization in response to hypercapnia, with minimal effect on respiration 19. In addition, we observed a second population of non-CGRP neurons adjacent to the PBelCGRP group in the central lateral, lateral crescent and Kölliker-Fuse parabrachial subnuclei that are activated in response to CO2 exposure in mice 23–31. Recent studies showed that neurons in the lateral PB expressing the transcription factor Fork head Box protein 2 (FoxP2) 32–34 have a distribution that is complementary to the PBelCGRP neurons including the regions containing the non-CGRP neurons that express cFos after CO2 exposure and which project to premotor and motor neurons that innervate the diaphragm and genioglossus muscles 35. Therefore, we hypothesized that whereas the PBCGRP neurons wake up the forebrain during apneas, the adjacent PBFoxP2 neurons may trigger activation of ventilatory effort during apnea.\n\nTo test this hypothesis, we examined the role of the PBFoxP2 neurons in respiration and arousal response to CO2. We started by investigating their response (cFos expression) to CO2 exposure as well as in vivo recording of PBFoxp2 neuronal activity by using intracellular calcium imaging during spontaneous sleep-wake and during exposure to CO2. We also investigated their contribution to the respiratory changes by optogenetically photo-activating PBFoxP2 neurons at different frequencies during either normocapnia or hypercapnia and by optogenetically photo-inhibiting them using archaerhodopsin T (ArchT), while mice were exposed to a CO2 stimulus.\n\n# Results\n\n**Activation of the PB FoxP2 neurons by CO2**: \ncFos expression in the PB FoxP2 neurons: We subjected mice to either 2h of 10% CO2 (10%, CO2, 21% O2, 69% N2; n = 5) or normocapnic air (room air: 21% O2, 79% N2; n = 3) and then examined brain sections using immunohistochemistry for both FoxP2 and cFos, an immediate early gene, used as a functional marker for activity in neurons. Because both cFos and FoxP2 are transcription factors, they are localized to the nucleus of neurons (Fig. 1). Exposure to CO2 caused a large increase in number of FoxP2 neurons that also showed cFos expression in the KF (38.3 ± 5%) compared to room-air (8 ± 1%; F₁,₇ = 21.88, P = 0.003; Fig. a1-d1 and f). The doubly labeled KF neurons formed a cluster located medial to the ventral spinocerebellar tract along the ventrolateral surface of the rostral PB. Slightly more caudally in the lateral PB, large numbers of neurons that showed cFos activation in response to CO2 exposure were found in the PBel (non-FoxP2 neurons, in the region of the CGRP neurons) and in the central lateral PB, just dorsal to the CGRP cluster and wrapping around its lateral margin. 49 ± 5% of the total cFos immunoreactive neurons in the PBL were FoxP2 neurons (F₁,₇ = 11.95, P = 0.013; Fig. a2-d3 and f). After CO2 exposure, the majority of the cFos + neurons in both the PBcl (78 ± 2%) and in the KF (71 ± 4%) showed FoxP2 expression (PB- F₁,₇ = 31.85, P = 0.001; KF- F₁,₇ = 9.8, P = 0.02) compared to the 42 ± 8% in PBcl and 52 ± 4% in KF of the room-air group (Fig. 1e). Of the total population of FoxP2-expressing neurons in the PBcl (PB FoxP2 neurons) 30 ± 4% expressed cFos after CO2 exposure compared to 9 ± 3% in the control mice (room-air). Therefore, the PB FoxP2 and KF FoxP2 neurons constitute the bulk of the non-CGRP neurons in the region adjacent to the PBel CGRP neurons that were also responsive to CO2. Interestingly, we found a small number of KF FoxP2 neurons that express the gene for CGRP (Calca) (supplementary Fig. 1), by using florescence in situ hybridization for CGRP in FoxP2-L10 mice. The FoxP2 + CGRP neurons in the KF (mean diameter 18 ± 0.7 µm) tend to be significantly smaller (F₁, 18 = 72.4; P < 0.001) than the ones that are not FoxP2 + (26.3 ± 0.7 µm).\n\n**In vivo measurement of PB FoxP2 neuronal activity by fiber photometry**: \nTo capture and analyze the pattern of activation of the PB FoxP2 neurons by CO2 in vivo, we injected an adeno-associated viral vector (AAV) expressing Cre-dependent GCaMP6s into the lateral PB of Foxp2 tm1.1(cre)Rpa/J (FoxP2-Cre) transgenic mice (developed by Dr. Richard Palmiter at University of Washington, and donated to the Jackson Laboratory) [34, 36]. We double-labeled sections through the PB from FoxP2-Cre::L10 reporter mice (in which FoxP2 cell bodies are marked by GFP) with FoxP2 immunohistochemistry (which stained nuclei of FoxP2 expressing neurons magenta) to verify that Cre-recombinase was expressed eutopically in FoxP2 expressing neurons (supplementary Fig. 2a-d). All of the neurons transfected by an AAV that expressed Cre-dependent GCaMP6s (which also fluoresces green) also showed FoxP2 expression in their nuclei (red in Fig. 2b). The implanted glass fiber targeting the GCaMP expressing PB FoxP2 neurons allowed us to record intracellular calcium levels, a surrogate for neuronal activity (Fig. 2c). The population activity of the PB FoxP2 neurons was then correlated to the identified sleep-wake states, respiration and their changes in response to repetitive CO2 exposures.\n\nIn n = 5 mice, optical fibers were located in proximity to the GCaMP expressing PB FoxP2 neurons (Fig. 2b). A representative example of a fiber photometry recording across an exposure to CO2 is illustrated in Fig. 2d. In these mice, GCaMP fluorescence increased when the mouse transitioned from NREM sleep to either wake or REM sleep (supplementary Fig. 3a and b). The increased activity of PB FoxP2 neurons when emerging from NREM sleep may contribute to the sudden increase in respiratory effort when an animal exposed to CO2 awakens from NREM sleep.\n\nAll trials with 30 sec exposures to 10% CO2 also resulted in cortical arousal in the latter half of the trial. Therefore, to avoid the confounding effects of significantly higher GCaMP responses caused by transition to wakefulness, we chose to analyze only the first 15s of the trial segments, which in all cases preceded cortical arousal. Although the actual level of fluorescence during exposure to CO2 waxed and waned during individual exposures (see heatmaps in Fig. 2e), when the level of ΔF/F (change in GCaMP activity/ background fluorescence) was summated across trials (Fig. 2f) and over 15s prior to and during CO2 in all trials, there was a robust and statistically significant increase in fluorescence of FoxP2 neurons during exposure to CO2 (F₁, 1682 = 62.2; P < 0.001) (Fig. 2f, ΔF/F normalized to pre-CO2), with the fluorescence peak for each of the 59 trials during CO2 exposure increasing by 6.4 ± 0.9% (F₁, 116 = 45.95 P < 0.001) compared to pre-CO2. This increase in ΔF/F was also accompanied by an increase in respiratory efforts in response to CO2 as measured in 59 trials from 5 mice (Fig. 2g-i). During this period we found a significant increase in respiratory rate (RR, 40 ± 1% increase for the last 5 breaths of the 15 sec interval after onset of CO2 exposure compared to the last 5 breaths prior to onset of CO2; F₁, 1662 = 5.7, P < 0.001, Fig. 2h), and a smaller increase in tidal volume (V_T) that lagged behind the increase in RR (Fig. 2 h-i) but was statistically significant (28 ± 0.89% increase) for the last three breaths of the 15 sec interval (P = 0.025; P = 0.004 and P = 0.037) (Fig. 2i). The GCaMP fluorescence (ΔF/F) is also shown as heat-maps for all the trials for 15 s before and after CO2 exposure (Fig. 2e). Analysis of this data shows that the average latency of the increase in intracellular calcium (Ca_i) to its first peak was 9.6 ± 0.57 sec, and in only 13.5% of the trials was the latency less than 5 sec (Fig. 2f). This observation aligns with the rise in RR starting at about 5 sec (approximate time that it takes for CO2 levels to rise in the chamber and then reach the circulation). The RR increased progressively in all trials for at least the next 10 sec (Fig. 2h), and then increased abruptly at the time of cortical arousal, which occurred between 15 and 30 sec in all trials.\n\nWe then analyzed the neuronal calcium activity of 28 neurons for the periods where the mice (n = 3) were exposed to CO2 (Fig. 3b and c) in a plethysmograph that allowed us simultaneously to record their breathing as well as EEG and EMG. For this analysis, we wanted to prevent confounds introduced by cortical arousal (EEG desynchronization and increase in motor activity), so we reduced the CO2 concentration to 8% and only used trials that showed no cortical arousal during 30s of CO2 exposure and in the subsequent 15 sec when CO2 levels in the plethysmograph were still high (see Fig. 3d, also video-CO2 responsive neurons.mp4). In these experiments 8% CO2, caused a 65 ± 4.4% increase in RR (F₁, 530 = 4.95, P < 0.001, pre vs. post) to 249 ± 5 bpm 20-40sec after CO2, compared to 152 ± 2 bpm at pre-CO2 levels. Minute ventilation also increased significantly (MV, F₁, 530 = 5.8, P < 0.001) with a 87.5 ± 4.4% increase 20–40 sec after CO2 onset (22.3 ± 0.4 ml/min) compared to pre-CO2 levels of 12 ± 0.26 ml/min (Fig. 3d, f). V_T showed a smaller but still significant increase (F₁, 360 = 1.53; P = 0.043) by 28 ± 5% during 20-40sec after CO2 onset (0.094 ± 0.002ml) compared to 0.074 ± 0.0016ml at pre-CO2. An example of simultaneous neuronal activity profiles for 9 cells during one representative CO2 trial is shown in Fig. 3d. We analyzed the activity of all n = 28 cells, for 30s before and for 90s after the CO2 stimulus in 4–7 trials during which the animals remained in NREM sleep for this period of time, and plotted the normalized fluorescence (ΔF/F) as a heat map (Fig. 3e). A small number of cells (4/28, 14%) were more active prior to the CO2 exposure, and were less active during the exposure. We termed these CO2-Off cells. The remaining 24 CO2-On neurons all showed periodic increases in Ca_i after exposure to CO2, with 17/24 cells showing three distinct fluorescence peaks during and after CO2 exposure. 23/24 cells showed a first peak in activity with a mean latency of 11 ± 0.6 sec after onset of the CO2, 21/24 showed a second peak at a mean of 27 ± 1.6 sec, and then 17/24 at 41 ± 2.8 sec; 1/24 only peaked at 33s after CO2 onset (Fig. 3f). Of the 17 cells that showed all three peaks, 10 cells peaked first at 11 ± 0.21 sec after CO2 onset and then showed periodicity of 17–19 sec for appearance of the second and third peak. Smaller numbers of neurons (10–12) also showed peaks in activity at roughly 60 and 75 sec. None of these neurons displayed this pattern of periodic and synchronized activity during NREM sleep prior to CO2 exposure, although the periodic waves of activity were similar to those we observed in individual PB FoxP2 neurons in animals breathing room air during wake and REM sleep. These data suggest that PB FoxP2 neurons may have a tendency to be activated in periodic waves that are synchronous across the population during wake and REM, but that these waves of activity may be suppressed during NREM sleep. Exposure to CO2 may then remove this suppression, allowing resumption of periodic, synchrous waves of activity with a periodicity during CO2 exposure in NREM sleep of about 15 sec. Whether these synchronous waves of activity originate from a rhythmic pattern of input, or are generated by recurrent activity in a local network or even are a cell autonomous response is not clear.\n\n**Photo-activation of PB FoxP2 neurons and respiration**: \nTo test the effect of activation of PB FoxP2 cells on respiration, we injected the PB of FoxP2-cre mice (n = 10) bilaterally with cre-dependent AAV-Flex-ChR2-mCherry (Fig. 4a), and implanted them for EEG/EMG recording along with bilateral optical fibers to target illumination of the ChR2 expressing FoxP2 neurons in the PB (Fig. 4b). We recorded animals for sleep and breathing in normocapnic room air and during activation of ChR2 with a blue laser (473nm) using 10ms pulses at 5, 10 or 20Hz, for either 5s or 10s every 5 minutes. Trials in which mice were in NREM sleep for at least 30s before stimulation were analyzed for the effect of optostimulation on respiration. In 6 out of 10 implanted mice, the optical fibers accurately targeted the ChR2 expressing PB FoxP2 neurons as shown in Fig. 4b. These animals consistently showed respiratory responses during optostimulation but also had EEG arousal either late in the stimulation or shortly after offset (Fig. 4c, d) in 70% of the trials. In the four cases where fiber implants were placed either medial or lateral to the PB FoxP2 ChR2 expressing neurons, neither 10 nor 20Hz stimulation produced any effect on respiration or cortical arousals. To distinguish the increment in ventilation due to waking, we measured RR and V_T for 5 breaths pre-stimulation, 5 breaths just before the end of stimulation (or just before onset of arousal, whichever occurred first) and 5 breaths after the cortical arousal.\n\nWhile breathing normocapnic air, 10Hz stimulation progressively increased RR (18.5% with 5 sec and 42% with 10 sec stimulation, P = 0.013; F₂, 63 = 19.75, P < 0.001) and minute ventilation (MV) (17.9% with 5 sec and 26% with 10 sec stimulation, for 5 sec - P = 0.03; for 10 sec- P < 0.001; F₂, 63 = 10.43; P < 0.001) compared to the pre-stimulation period, but had little effect on tidal volume (F₂, 63 = 0.35; P = 0.71). Stimulation at 20 Hz increased RR by 35% at 5 sec vs. 69% at 10 sec (F₁, 106 = 122.9, P < 0.001) and MV by 25% at 5 sec and 40% at 10 sec (Fig. 4f). This pattern was consistent with the fiber photometry results, in which RR began to increase at the same time as calcium activity of PB FoxP2 neurons, but increases in V_T lagged by about 10 sec. However, no significant changes on respiration were observed with photo-stimulations at 5 Hz (Fig. 4f).\n\nTo explore the interaction between optogenetic stimulation and activation of PB FoxP2 neurons due to elevated CO2, we repeated the 20Hz, 10 sec stimulation in mice breathing 2% CO2 (Fig. 4e, representative example). First, we observed that the presence of 2% CO2 throughout the experiments dramatically decreased the latency of awakening to the laser stimulus to 2.22 ± 0.3 sec compared to 21.7 ± 1.7 sec in normocapnic air (F₄, 27 = 3.2; P = 0.031) (Fig. 4d). Despite the relatively brief period of laser stimulation before awakening in 2% CO2, we also found a large and almost immediate increase in RR (81%; F₂, 12 = 44.25; P < 0.001) and MV (38%; F₂, 12 = 8.08; P = 0.006), with no change in V_T (Fig. 4g), similar to that found with stimulation in normocapnic air (Fig. 4f). Interestingly, the EEG arousal occurred at around the same RR as with CO2 or optogenetic stimulation alone (i.e., approximately 240–250 bpm), raising the possibility that the arousal caused by stimulation of the PB FoxP2 neurons may be due to the sensory feedback from the increased ventilatory effort, rather than being a primary effect of the PB FoxP2 neurons.\n\nFurther, we used the mice from these experiments (n = 6) to map the projections of the ChR2-expressing PB FoxP2 neurons (Fig. 5a). We found extensive mCherry labeling of fibers and terminals in the pre-Bötzinger complex (PBZ) and caudal ventrolateral medulla (CVL), and more moderate numbers of labeled terminals in the nucleus of the solitary tract (NTS) and hypoglossal nucleus (XIIn) (Fig. 5 b and c). To confirm these projections we also injected a retrograde tracer CTb in the PBZ area (n = 3; Fig. 5d) and mapped the retrogradely labeled FoxP2 neurons in the PB and KF. Doubly labeled neurons were found in the KF (Fig. 5e1-e3), the central lateral PB subnucleus and in the lateral crescent zone along the lateral edge of the external lateral PB connecting the two major clusters (Fig. 5 f-g). Thus the PB FoxP2 population projects to medullary targets (Fig. 5) that are consistent with mediating CO2-evoked changes in ventilation. PB FoxP2 neurons also showed ascending projections to the median and lateral preoptic area and ventral to the zona incerta in the lateral hypothalamus, but do not project to the substantia innominata in the basal forebrain and the central nucleus of the amygdala, which are key targets of the PB CGRP neurons mediating CO2-induced EEG arousal.\n\n**Photo-inhibition of PB FoxP2 neurons during exposure to CO2**: \nTo test the necessity of PB FoxP2 neurons in producing the respiratory responses to CO2 during sleep, we photo-inhibited them during hypercapnia. FoxP2-cre mice were injected in the ventral part of the LPB with AAV-Flex-ArchT (n = 12) (Fig. 6a) and implanted with EEG/EMG electrodes and bilateral optical fibers targeting the PB FoxP2 neurons (Fig. 6c1-c5). We analyzed the respiratory responses to 10% CO2 given for 30s every 300s, with and without photo-inhibition of the PB FoxP2 neurons using a 593 nm laser light (Fig. 6b). The laser light was on for 60s, beginning 20s prior and extending to 10s after the CO2 stimulus (30s) (representative trials of CO2 exposure are shown in Fig. 6 d and e).\n\nPhotoinhibition of PB FoxP2 neurons significantly reduced the increase in V_T caused by CO2 (F₂, 27 = 9.67; P = 0.004) by 42% (p =-0.027) pre-arousal and by 34% (p = 0.015) after arousal. It also reduced the increase in MV caused by increased CO2 (F₂, 27 = 6.25; P = 0.017) by 37% post-arousal (P = 0.015), but the reduction pre-arousal was not statistically significant (p = 0.081) (Fig. 6g, h). Photoinhibition of PB FoxP2 neurons had little effect on the RR increases induced by CO2 (Fig. 6f) and no effect on latency to arousal.\n\n# Discussion\n\nOur previous work identified a population of CGRP neurons in the PBel that project to the forebrain and are required for arousal from sleep during CO2 exposure, but make little contribution to respiratory efforts. Here we report a second adjacent population of neurons that is marked by expression of the FoxP2 transcription factor and is required for normal respiratory response to CO2 during sleep, but not arousal. These PBFoxP2 neurons are located in clusters in the PBcl just dorsal to the CGRP group and in the KF subnucleus, and along a narrow bridge just lateral to the CGRP group (the lateral crescent) connecting the two major clusters. This population of PBFoxP2 neurons projects intensely to medullary respiratory areas as well as to hypothalamic targets (lateral hypothalamus, preoptic area) associated with regulation of wake-sleep. However, optogenetic stimulation of the PBFoxP2 neurons causes immediate increases in ventilation, but only delayed and inconsistent arousals, and while photoinhibition reduces the ventilatory increases caused by CO2 it does not affect arousal. Hence, we interpret the PBFoxP2 neurons as primarily mediating the ventilatory response to CO2.\n\nWe further found that optogenetically activating the PBFoxP2 neurons eventually also wakes the animal up, although often after the PBFoxP2 neurons are no longer being stimulated, and at levels of ventilatory effort that are similar to that at the time of arousal in an animal exposed to 10% CO2. We interpret these findings as an indication that CO2 exposure largely and independently activates populations of PBCGRP neurons that cause EEG arousal and PBFoxP2 neurons that cause increased ventilation. However if animals are forced to increase ventilation enough, they are awakened by the effort, and if they wake up during CO2 exposure, they further increase ventilation. This relationship underscores the synergy between the behavioral and respiratory motor responses to insure survival when an animal is either apneic or asphyxiated.\n\nWe used three different intersecting strategies to identify the role of the PBFoxP2 in the ventilatory response to CO2 during sleep. First, we showed that among the neurons in the PBcl and KF (i.e., outside the PBelCGRP group) that show cFos expression after CO2 exposure, nearly 75% express FoxP2. This PBFoxP2 population had no overlap with the PBelCGRP neurons (i.e., no PBelCGRP neurons expressed FoxP2), indicating that they are independent cell populations. Interestingly, we found a small number of KF neurons that are CGRP-immunoreactive (supplementary Fig. 1). These neurons are a bit smaller than those in the PBel, and as shown by Geerling and colleagues 34, they project to respiratory sites in the medulla, like the remainder of KF glutamatergic neurons (see also Yokota et al., 2015 35). We had missed this population in our previous reports because they appear to express CGRP at a lower level than the larger PBelCGRP neurons (Nardone, Saper and Lowell, in preparation) 37. We use Calca-ires-Cre-ER mice in our experiments for identifying and manipulating CGRP neurons, and apparently the level of Cre expression in these small KF CGRP neurons was not sufficient to cause recombination events. By contrast these neurons appear to have greater Cre expression in the Calca-Cre knockin mice used by Geerling et al., and so are more readily identified. Interestingly, our in situ hybridization results reported here (supplementary Fig. 1) indicate that at least some of the KFCGRP neurons also express FoxP2, underscoring that they are a separate population from the PBelCGRP neurons and demonstrating the value of FoxP2 as a marker for identifying the neurons that drive ventilatory responses to CO2. It should be pointed out, however, that FoxP2 is expressed more widely in more dorsally located neurons in the lateral PB, but only the FoxP2 neurons in the PBcl, KF and lateral crescent express cFos in response to CO2. We are currently searching for more selective markers for this neuronal population.\n\nThe second strategy we used to investigate the relationship of the PBFoxP2 neurons with the ventilatory response to CO2 was the employment of fiber photometry to study the intracellular calcium responses of PBFoxP2 neurons during wake-sleep and during CO2 exposure. The PBFoxP2 neurons were clearly wake and REM active. This finding is consistent with the general reduction of respiration during NREM sleep, and the fact that arousal from NREM sleep caused a rapid increase in both ventilation and in the calcium signals from the PBFoxP2 neurons. This population of neurons showed a brisk increase in calcium signal beginning a few seconds after onset of a 10% CO2 stimulus, but persisting for many seconds after the stimulus was removed. We then resolved the responses of individual PBFoxP2 neurons with GCaMP6s endoscopy during exposure to 8% CO2 (a concentration chosen because it generally did not wake up the animals during a 30 sec exposure). Surprisingly, the individual PBFoxP2 neurons showed multiple recurrent peaks of calcium activation, with the first peak at 11.0 ± 0.2 s after onset of the gas and then further peaks at roughly 17–19 sec intervals. The mechanism for these rhythmic pulses of activity in the PBFoxP2 neurons remains a mystery. These experiments admittedly involved only a small number of PBFoxP2 neurons and because of the limited depth of field of the GRIN lens we used, all of them were in a small cluster near the surface of the lens. However, if the larger population of PBFoxP2 neurons also responds rhythmically to CO2, our results would suggest that the much smoother population response as imaged by fiber photometry is probably a summation of the activity of different subsets of PBFoxP2 neurons that are activated at different times in different locations in the PBcl and KF during CO2 stimulation. Our anterograde and retrograde tracing experiments indicate that PBFoxp2 neurons may mediate these effects on respiration by their descending projections to the medullary targets involved in ventilatory rate and volume 35.\n\nThe third strategy we used to characterize the role of the PBFoxP2 neurons in the response to CO2 involved optogenetic excitation and inhibition. When the PBFoxP2 neurons were opto-stimulated at 10 or 20Hz while mice were breathing normocapnic air, they showed a statistically significant increase in RR and MV (but not VT) that was greater both with higher frequency or prolonged duration of stimulation. Interestingly, the animals only awakened either late in the stimulation episode or immediately afterward, suggesting that the EEG arousal was not a direct effect of the stimulation. In this regard, it was interesting that when animals were stimulated optogenetically while breathing 2% CO2, the latency of the arousal was shorter, but occurred at about the same RR as the opto-stimulation while breathing room air or in response to CO2 without optostimulation (i.e., awakening in all three conditions occurred at about 240–250 breaths/min, or when RR was about 50% greater than baseline). This observation suggests that the arousal may have been due to somatomotor feedback from the increased ventilatory effort. Alternatively, it is possible that either the PBFoxP2 neurons or brainstem cell groups downstream from them may have collaterals that activate PBelCGRP or some other arousal neurons. It would be useful to test whether simultaneous suppression of PBelCGRP neurons while activating PBFoxP2 neurons might permit increased ventilation without EEG arousal.\n\nOur results of PBFoxP2 photo-stimulation that enhanced the breathing frequency but had little effect on the VT are similar to those shown earlier 38–40 for photostimulation of the PreBotzinger (PBZ) region, where low power stimulation (20HZ at 2 mW) of inhibitory neurons (GABA-ergic and glycinergic) increased the RR but not the VT. Similarly, photo-activation of the adjacent catecholaminergic group in the rostral part of the ventrolateral medulla which projects to the respiratory rhythm-generating neurons located in the pre-Botzinger complex 41–45 also increased the RR in a dose dependent manner 43. These findings suggest that the PBFoxP2 neurons may target the pre-Botzinger complex to cause the increase in RR (Fig. 7).\n\nBy contrast, photo-inhibition of the PBFoxP2 neurons during a 30 sec exposure to CO2, did not prevent the rise in RR but did diminish the rise in VT and MV, not only during the CO2 exposure but even after the cortical arousal, when the largest increase in VT is generally observed. On the surface it may appear that the increase mainly in RR with photostimulation of the PBFoxP2 neurons and decrease mainly in the VT with photoinhibition of the same cells is inconsistent. However, the photostimulation was done while the animals were breathing room air, so the increase in RR cause by the PBFoxP2 neurons was not being masked by the contributions of other brainstem sites (such as the retro-trapezoid nucleus, para-facial complex, medullary raphe and the nucleus of solitary tract) that are also engaged by high CO2 levels 41, 43, 45–47. In addition, although the increase in VT was not statistically significant during these brief periods of stimulation, VT changes with hypercarbia lag considerably behind the increase in RR. On the other hand, during 10% CO2 stimulation, when these other CO2-responsive sites were already increasing RR to its maximum, 44, 48–50 the inhibition of PBFoxP2 neurons revealed although they are not needed to reach maximal RR, they are necessary to achieve the maximal increase in ventilatory volume. In other words, brief activation of the PBFoxP2 neurons is sufficient to drive RR (but not VT) when breathing room air, and necessary to drive increased VT during exposure to high CO2 levels 51–54. A schematic model describing the proposed neuronal circuit for hypercapnia induced increase in ventilation implicating the role of PBFoxP2 neurons is shown in Fig. 7.\n\nIn conclusion, our experiments reveal that PBFoxP2 neurons likely contribute both to the increases in RR and VT during exposure to CO2 in NREM sleep, but that they are not the only pathway driving these responses (Fig. 7). On the other hand, if ways could be found to augment the PBFoxP2 response to CO2, this may be sufficient to avoid hypoventilation and minimize EEG arousals in patients with obstructive sleep apnea. However, activating the PBFoxP2 neurons to increase RR by 50% or more above baseline may by itself contribute to EEG arousal. It is not known whether this arousal is due to the mechanical sensory feedback of increased ventilatory effort, or might represent collaterals from the PBFoxP2 neurons that indirectly activate PBelCGRP neurons or some other arousal pathways. However, for activation of PBFoxP2 neurons to be effective in treating patients with obstructive sleep apnea, it will be important to find ways to suppress the EEG arousal while augmenting the respiratory response to CO2.\n\n# Methods\n\nAnimals: We employed *Foxp2*tm1.1(cre)Rpa/J transgenic mice in which IRES-Myc tag-nuclear localization signal (NLS)-cre-GFP-frt-neomycin-frt were introduced just after the termination codon of the mouse Foxp2 gene via homologous recombination. The mutation was created via homologous recombination in (129S6/SvEvTac x C57BL/6) F1-derived G4 embryonic stem (ES) cells. The frt-flanked neomycin cassette was excised through crosses with animals that broadly expressing Flp recombinase. The GFP is believed to be nonfunctional. Resultant mice were backcrossed to C57BL/6J for 9 generations by the donating laboratory to the Jackson laboratory (Strain #:030541; RRID:IMSR_JAX:030541). All transgenic mice used here were heterozygous for the transgene and backcrossed to the C57BL6 strain and wildtype littermates were used as controls. We bred these mice in our animal facility and confirmed their genotype by using a Red Extract N-amp Tissue PCR kit (Sigma Aldrich; Catalog # XNAT-1000RXN) and Cre forward and reverse primers to detect the Cre recombinase gene. Their wildtype litter mates were used as controls, in each experiment.\n\nValidation of mice: To test if the Cre expression was eutopic with FoxP2 expression FoxP2-Cre mice from Jackson Labs, we also validated by crossing them to the L10 reporter mice. The cre-positive neurons were labeled with green fluorescent protein (GFP), and when the tissue was immuno-stained for FoxP2, we could observe nearly all green (GFP) neurons expressed labeling for Fox-P2 (red) in their nuclei (supplementary Fig.2a-d). This confirmed that we could reliably use these mice for expressing cre-dependent virus vectors in the FoxP2 neurons in the PB, and then use fiber-photometery or optogenetics to record their activity profiles or manipulate them (examples of cre dependent transfections- Fig.2b,4b and 6c). PBFoxp2 neurons did not overlap with the PBCGRP neurons in the lateral PB.\n\nAll mice used in these experiments were male because female mice of the same age are smaller, and including animals of various sizes would introduce noise into analysis of respiratory volumes (which scale with body size) across groups. Animals were maintained on a 12 h light/dark cycle with ad libitum access to water and food and were singly housed after surgery, with ambient temperature of 21-23oC and humidity levels between 40-60%. Male littermates were randomly assigned to the experimental groups. All animal procedures met National Institutes of Health standards, as described in the Guide for the Care and Use of Laboratory Animals, and all protocols were approved by the Beth Israel Deaconess Medical Center Institutional Animal Care and Use Committee.\n\nVectors: For fiber-photometry we used AAV-pSyn-GCaMP6s from Addgene_100843. For optogenetic experiments, we used the excitatory opsin (AAV-EF1a-DIO-hChR2(H134R)-mCherry- AAV-serotype8) and the optogenetic neural silencer AAV-CAG-FLEX-ArchT-GFP (AAV-serotype-8). These viral vectors was procured from the University of North Carolina (UNC) vector core and has been previously used for excitation as well as for silencing neurons and their terminals by us19,55. The viral vectors expressing excitatory and the inhibitory opsins were packaged at the UNC vector core.\n\nSurgery: Under surgical anesthesia, mice were instrumented for sleep with implantation of EEG and EMG electrodes in addition to implanting either the fiber photometry cannula (unilateral), or integrated grin lens with baseplate (unilateral) or bilateral optical fibers targeted to the PB area (AP: -5.1 to -5.3mm; DV- 2.6mm; ML: ±1.3mm). All implants were done after 5 weeks post injection of the injections of the viral vectors in the PB, to ensure optimal expression of the gene expression. After recovery from surgery, mice were recorded for sleep and respiration after acclimatizing them to the recording apparatus for at least once in a week before the actual recordings were performed. We recorded the arousal and respiratory responses to CO2 by placing them in the plethysmograph and recording them for both sleep and breathing by the procedure described previously19,21,55.\n\nExperiment 1a: C57BL/6J mice (n=8) were moved from the animal housing room and placed in the plethysmographs where they were exposed continuously to either hypercapnic (21% O2; 10% CO2; 69% N2) or room air (21% O2; 0% CO2; 79% N2) for two hours, after first habituating them to the chamber at room air for two hours. Air or hypercapnic exposures were performed between 10:00 and 12:00. At the end, mice were deeply anesthetized with chloral hydrate (500mg/kg, ip) and transcardially perfused with saline, followed by 10% formalin. Brains were removed, post-fixed overnight immersed in 20% sucrose and cut into four alternate series of 30 micron frozen sections. After immune-staining the tissue for cFos and FoxP2, using specific antibodies as per the methods described below, the cells that were double labeled for cFos and Foxp2 were counted in the PBcl (0.5mmX 0.6mm placed dorsal to the single labeled cFos in the PBel, as in Fig. 1a2-d3) and KF (0.5mm X 0.5 mm placed ventral to the ventral spino-cerebellar tract, as in Fig. 1a1-d1) sub-nuclei, after scanning the slides using a slide scanner (Olympus VS200 slide scanner) and acquiring the images in Olympus OlyVia 3.3 software using square grids. To avoid counting bias, the cell counts were performed by investigators blind to the treatment groups (NL and JDL). The original figures in Fig1a-d were taken by a confocal laser microscope (LasX Leica DMi8 confocal). We counted the sections that were separated by at least 120µm, and this also involved counting only the nuclei for both the FoxP2 and the Cfos, that reduced the chances of counting cells twice. Cell counts were also corrected for the cell size using the Abercrombie correction factor.\n\nExperiment 1b: Fiber-photometry implants: In vivo calcium monitoring during sleep-wake and with CO2 exposures was performed using fiber photometry. After 5 weeks of the viral injection of AAV-pSyn-GCaMP6s in the PB, laser light was passed into the brain via low-fluorescence fiber optic patch cord (0.48NA, Doric Lenses) connected to the implanted fiber optic cannula with a metal sleeve (Doric Lenses, MFC_400/430-0.48_5mm_MF-1.25). Using the patch cord, we simultaneously delivered light via LED drivers at 465 nm and 405 nm (Doric Lenses, CA), to measure the calcium-dependent and calcium-independent (UV, isobestic), excitation of the GCaMP. Excitation emission from the GCaMP protein passed back through the fiber optic patch cord and through the fluorescence Mini Cube (Doric Lenses) and detected by a photo-receiver (Doric Lenses). Signals detected by the photo-receiver were transmitted to Axon Digidata 1322A analog-to-digital converter and the signals were acquired using Axoscope software- v10 (Molecular Devices, Foster City, CA, USA), alongside the EEM/EMG and breathing signals. We used exported files to Spike2 and analyzed the respiratory signals using the spike respiratory scripts (Resp80t, Spike2, CED, UK) that were then correlated with the GCaMP activity.\n\nThe GCaMP6 raw data was normalized to the baseline fluorescence of each trial to obtain the ΔF/F (change in fluorescence intensity relative to the baseline fluorescence intensity) for different animals. The GCaMP ΔF/F values per second was calculated for 15 s before and during CO2 for each trial and statistically compared, along with RR and VT values for similar periods. The peak values of GCaMP ΔF/F, and the latency to peak during the entire 15s with CO2 exposure were also calculated. Two-way ANOVA was performed to compare the effects between pre and post CO2 exposures on the GCaMP ΔF/F and also for RR and VT.\n\nExperiment 1c: GRIN lens implants: Foxp2tm1.1(cre)Rpa/J mice (heterozygous FoxP2-Cre), after 3weeks of the virus injection (AAV-pSyn-GCaMP6s) in the PB were implanted with a microendoscopic ProView™ Integrated Lens 0.6mm x 7.3mm (Inscopix Catalogue #1050-004413) that allowed for visualizing the activity during the lens implant. The lens was targeted to be ~200-300 µm above the neurons using the following coordinates- -5.0mm posterior to bregma, -1.4mm lateral from midline and -2.8 to 3.0 mm ventral to the dura mater. The baseplate provide the interface for attaching the miniature microscope during the calcium-imaging experiments, but during other times a baseplate cover (Inscopix catalogue # 100-000241) was attached to prevent damage to the micro endoscopic lens. Out of approximately 8 mice injected with GCaMP6s virus, 4 had successful implants and were used for the study.\n\nCalcium imaging: We imaged the calcium activity at 5 frames per second, 200-ms exposure time at 20-30% LED power using the miniature microscope from Inscopix (nVista). These parameters caused minimal bleaching, and allowed long term recordings in mice. Mice were recorded for 5 min every hour for correlating the calcium activity to the 12h sleep-wake behavioral data. For correlating to the CO2 induced respiratory changes, mice were recorded in a plethysmograph, where they were subjected to repeated stimulus of 30s of 8% CO2 every 5 minutes, and the imaging was done for 4 trials (~20 min) every hour for 3h after 3-4h of habituation of mice to the recording chamber with every recording. This protocol caused minimum bleaching and allowed repetitive 2-3 recordings in an animal with a week of separation between subsequent recordings.\n\nExperiment 2: Optogenetic activation of the PBFoxP2 neurons: For selective activation of the PBFoxP2 neurons, we injected an adeno-associated viral vector expressing the excitatory opsin AAV-FLEX-ChR2-mCherry in the PB (AP: -5.1 to -5.3mm; DV- 2.6mm; ML: ±1.3mm) and implanted these mice (n=10) with bilateral optical fibers targeting the lateral PB. We also injected some wild type mice (n=3) with AAV- FLEX-mCherry as well, which served as control, we did not observe any expression of ChR2. We recorded these mice for sleep and respiration when they were exposed to the room air as per the method previously described. Mice were subjected to 5 or 10s of 467nm laser stimulus with pulse width of 10ms and with frequencies of either 5Hz or 10Hz or 20Hz, in a random order and with each treatment separated by at least 7-10 days.\n\nExperiment 3: Optogenetic inhibition of the PBFoxP2 neurons: A separate set of FoxP2 mice were injected in the PB with AAV-FLEX-ArchT-GFP (n=12), and to test whether PBFoxP2 neurons mediate CO2 induced changes in respiration, these mice were bilaterally implanted with optical fibers targeting the PB (AP: -5.1 to -5.3mm; DV- 2.6mm; ML: ±1.3mm) for the inhibition of the PBFoxP2 neurons. At 5 weeks post injection, these mice were recorded for sleep and breathing in plethysmography chamber, where the arousal and respiratory responses were assessed while they were subjected to repetitive CO2 stimulations as shown earlier19,20,55,56.\n\nHistology: At the conclusion of the experiments, the animals were perfused with 0.9% saline followed by 10% buffered formalin while under deep anesthesia. Brains were harvested for analysis of the effective location of the injection site. Brains were kept in 20% sucrose for 2 days and sections were cut at 30mm using a freezing microtome in four 1:4 series.\n\nImmunohistochemistry: C-Fos: Oncogene Sciences, cat # Ab5, rabbit polyclonal, raised against amino acids 4–17 of human c-Fos. This antibody stained a single band of 55 kDa on Western blots from rat brain (manufacturer’s technical information). Sections were processed for detection of c-Fos alone or c-Fos in combination with FoxP2. All incubations were performed on free-floating tissue sections at room temperature. Sections were first incubated overnight in c-Fos antibody. When c-Fos staining was to be combined with FoxP2, we used Rabbit anti-Fos antibody (diluted 1:10K in PBS with 0.2% Triton X-100). After rinsing, sections were incubated in Alexa488 (green fluorescence) conjugated donkey anti Rabbit-IgG (Invitrogen, A11055) at 1:500 in PBS containing 0.2% Triton-X and 2.5% normal donkey serum for three hours. After rinsing in PBS sections were next incubated overnight with rabbit anti-FoxP2 (diluted 1:5000 in PBS with 0.2% Triton X-100 and 2.5% normal donkey serum). After rinsing the next day sections were incubated in Cy3 (red fluorochrome) conjugated donkey anti-rabbit IgG (Jackson Immuno-Research Labs, code#111-165-003) or with streptavidin-pacific blue (1:200, ThermoFischer, cat-S11222) after reacting the tissue to the appropriate biotinylated secondary antibody.\n\nMice injected with either GCamP6s or ArchT or ChR2, were immunostained either for GFP (Rabbit anti-GFP, 1:10K, Molecular Probes Cat# A-11122, RRID:AB_221569) or with mcherry (rabbit anti DsRed. 1:2K, Clontech, Cat-632496 ) as per standard immunohistochemistry protocols described previously19,55. These were then double stained for FoxP2 using either anti-rabbit (Rabbit anti-Foxp2, 1:10K, Abcam Cat# ab16046, RRID:AB_2107107) or anti-sheep antibodies (Sheep anti FoxP2, 1:5K, R and D Systems Cat# AF5647, RRID:AB_2107133). We used rabbit polyclonal antibody raised against a Synthetic peptide conjugated to KLH derived from within residues 700 to the C-terminus of Human FOXP2 (AbCam) and for the sheep polyclonal antiserum raised against recombinant human FoxP2 isoform 1, Ala640-Glu715, Accession # O15409 (R&D Systems) and these have been previously used and validated by others57–59. Neither of these antibodies showed immunostaining when the primary antibodies were omitted, and when the tissue from control mice was used that were not injected with viral vector. Some of the brains (n=3) from WT mice were injected with CTb and were immunostained using Goat anti CTb (1:30K, Cat# 703, RRID: AB_10013220, List Biological Laboratories Inc., CA). Sections for double staining for GFP, mcherry, CTb or FoxP2 were incubated in fluorescent-labeled secondary antibodies (Alexa- 488 at 1:200 or Alexa- Cy3 at 1:200; Catalog #- A32790 and A10521, RRID- AB_2762833 and RRID- AB_2534030, Molecular probes, Thermo-Fischer Scientific) or with streptavidin-pacific blue (1:200, ThermoFischer, cat-S11222) for 2h and cover-slipped with fluorescence mounting medium (Dako, North America). When acquiring confocal images, sometimes pseudocolors were used to enhance clarity.\n\nFluorescent In situ hybridization (FISH using RNA Scope): We identified FoxP2 neurons by using Foxp2tm1.1(cre)Rpa/J mice crossed with R26-lox-STOPlox-L10-GFP reporter mice (FoxP2-L10, n=3), and labeled for Calca (the gene for CGRP) by using a set of FISH probes with RNAScope in brain sections from the KF and PBcl areas. The brain was sectioned at 30 µm and sections were mounted on glass slides in RNAs-free conditions, and RNA scope was performed using the multiplex fluorescent reagent Kit V2 (Cat# 323100, Advanced Cell Diagnostics, Hayward, CA). Brain sections on the slides were pretreated with hydrogen peroxide for 20 min at room temperature and then with target retrieval reagent for 5 minutes (at temperature above 99°C), followed by dehydration in 90% alcohol and then air-dried for 5 minutes. This is followed by a treatment with protease reagent (Protease III) for 30 minutes at 40°C. After rinsing in sterile water, sections were hybridized in CGRP/ Calca FISH probe (smFISH probe: Mm- Mm-Calca-tv2tv3-C1- Mus musculus, Calcitonin-related polypeptide alpha, transcript variant 2 mRNA; probe region: 63 – 995 Accession No. NM_001033954.3; Catalog# 420361; Advanced Cell Diagnostics, Hayward, CA) for 2 hours at 40°C, and this probe has been used previously to selectively label CGRP on the brain tissue60,61. Sections were then incubated in 3 amplification reagents (AMP) at 40°C (AMP1 for 30minutes, AMP2 for 30 minutes and AMP3 for 15 minutes) followed by Horse radish peroxidase –C1amplification at 40°C for 15 minutes. Sections were then incubated in tyramide signal amplification (TSA) reagents with Cy3 fluorophore (Cat# NEL744001KT, Perkin Elmer, 1:1000) for 30 min to amplify and visualize CGRP mRNA in red. In the final step, sections were subjected to HRP blocking for 15 min at 40°C. After each step, sections were washed with 1X wash buffer provided in the kit. Following the CGRP RNAscope in-situ hybridization, immuno-labeling of GFP was performed on the same sections, as in-situ procedure quench the green fluorescence. For this, the brain sections were incubated in rabbit anti-GFP (1:1500), (Cat#A6455; Lot#1220284; Molecular probes) for overnight at 4°C, washed in PBS (3X2 minutes) and then incubated in secondary antibody (Alexa Fluor- 488 Donkey anti Rabbit, Life Technologies, Cat# A-21206) for 2h at room temperature. Finally, the slides were dried and cover-slipped with Dako fluorescence mounting medium (Cat# S302380-2, Agilent, CA), and scanned for analysis.\n\nData acquisition: All recordings were done at five weeks after injection of the viral vectors. All sleep and respiration recordings were done in a plethysmography chamber (unrestrained whole-body plethysmograph, Buxco Research Systems) which allowed us to record the breathing of the mouse while continuously monitoring the gas in the chamber. Electroencephalogram (EEG) and electromyogram (EMG) were recorded using Pinnacle preamp cables connected to an analog adaptor (8242, Pinnacle Technology). Gas levels in the chamber were continuously monitored using CO2 and O2 monitors from CWE, Inc (Ardmore, PA, USA). EEG, EMG, respiration, and CO2 and O2 levels were fed into an Axon Digidata 1322A analog-to-digital converter and the signals were acquired using Axoscope software- v10 (Molecular Devices, Foster City, CA, USA), or by acquired by the 1401 (CED, Cambridge, UK) and Spike2 ver.7 (CED, Cambridge, UK). Mice were connected to cables for sleep recording as well as with the fiber-optic cables connected to the pre-implanted glass fiber in mice, for transmitting the laser light.\n\nMice were also placed in the plethysmography chamber beginning at 9:00 A.M. for 6 h during their lights-ON and behaviorally inactive period, on each test day for these recordings. Here, they underwent either the Laser-ON or Laser-OFF protocols, separated by a week and in random order.\n\nDuring the Laser-ON protocol, either 473nm or 593nm laser was ON for 5, 10 0r 60s followed by 5 mins off. With 473nm, the photo-stimulations were done at either 5, 10 or 20Hz with pulse width of 10ms, and these stimulations were done for either 5 or 10s on different days, with a period of 6-7days between each treatment. During photo-activation using the 473nm laser, only normocapnia air was used in the chamber. The inhibitory 593nm laser stimulations were continuous for 60s, and preceded each 30s of CO2 stimulus by 20s and lasted 10s after the hypercapnia stimulus. In the Laser-OFF condition, everything was the same, except that the laser light was not turned on. The gas input for the plethysmograph was switched either to normocapnic air (21% O2, 79% N2) or hypercapnic air (10% CO2, 21% O2, and 69% N2) for 30 sec with 5 minutes in between the two hypercapnic stimuli. For both the photo-activation and inhibition experiments, trials were analyzed for latency to arousal and respiratory changes only for those epochs where the mouse was in NREM sleep for at least 30 s before the stimulus onset.\n\nLaser light: Mice were allowed at least 2d to acclimate to fiberoptic cables (1.5 m long, 200 µm diameter; Doric Lenses, Quebec, QC, Canada) and connecting interfaces coated with opaque heat-shrink tubing before the experimental sessions. During Laser-ON experiments, light pulses were programmed using a waveform generator (Agilent Technologies, catalog #33220A, CA, USA) to drive either 10ms of 473nm (blue laser, Laser Glow, Toronto, ON, Canada) pulses at 5, 10 or 20Hz, or drive the orange-yellow light laser (593 nm; Laser Glow, Toronto, ON, Canada) to be continuously on for 60s beginning 20 s before the onset of the CO2 stimulus. We also used the splitter - TM105FS1B (Thorlabs, NJ) to split the laser stimulus for bilateral activation or inhibition. We adjusted the laser such that the light power exiting the bilateral fiber-optic cables was 8-10 mW, and this was checked before and after the experiment. The light power estimated at the PB is less than10 mW/mm2 (www.stanford.edu/group/dlab/cgi-bin/graph/chart.php), and a similar range has been used by most researchers and by us earlier19,55,62,63. Note that this is probably a high estimate because some light is probably lost at the interface between the fiber-optic cable and the implanted optic-fiber.\n\nData analysis: Latency and respiratory data analysis: EEG arousals in response to CO2 were identified by EEG transition from NREM to a waking state, which was usually accompanied by EMG activation, as described previously. The latency of all the EEG arousals after onset of stimulation were scored and were compared across the Laser-ON and Laser-OFF days. Respiratory data was analyzed by running the respiratory script in the Spike2 (CED, UK) software, which performs breath by breath analysis for many respiratory parameters such as RR, VT and MV. For both latency and respiratory data, the ranges for analysis were selected by individuals that were blind to the treatment groups, who based the selection off the following criteria: 1. Trials with at least 30 seconds of NREM sleep before CO2/ stimulation; 2. Select 5 breaths before CO2 or laser stimulation, during CO2/ stimulation before arousal and then at post- arousal for respiratory analysis; 3. Exclude trials with REM sleep.\n\nFiber photometry data: The voltage GCaMP and UV signals were Gaussian low-pass filtered at 4 Hz, and saved for offline analysis. Both signal channels (465 and 405 nm) were monitored continuously throughout recordings, with the 405 nm signal (UV) used as an isobestic control. Signals detected with 405 nm wavelength light are not calcium-dependent and are indicative of background fluorescence or motion artifacts. A change in fluorescence (ΔF/F) was calculated by normalizing F to baseline fluorescence. For generating heat maps, min-max normalization was performed that causes linear transformation and the data is scaled in the range (0,1).\n\nInscopix calcium-image processing: Calcium recording files were spatially filtered and motion corrected to correct the rigid brain movements using the Inscopix data processing (IDPS ver1.6). To extract the calcium activity traces from the individual cells, we used manually drawn small regions of interest. Raw traces were converted to ΔF/F (F-Fbaseline average/ Fbaseline average), where F was the fluorescent at any given point and Fbaseline average was the average baseline fluorescence. These baseline image calculations were performed by the IDPS to derive ΔF/F value for each cell.\n\nStatistical analysis: All statistical analyses were performed using SigmaPlot 12.3 (Systat Software, Inc.). For statistical comparisons, we first confirmed if the data meets with the assumptions of the ANOVA, then either one way or two-way ANOVA was performed to compare the effects between various treatment groups. If differences in the mean values among the treatment groups were greater than would be expected by chance; then all pairwise multiple comparisons were performed using the Holm-Sidak method. The F and P values are described in the results section with details of the statistical tests also given in the respective figure legends and represented in the figures. The ‘n’ is reported in the figures and results and represents the number of animals, and the error bars represent mean± SEM. 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Neurocytol. 31, 693–717 (2002).\n\n# Supplementary Files\n\n- [CO2responsiveneurons2.mp4](https://assets-eu.researchsquare.com/files/rs-2865756/v1/3e22f0cfcfb13dfd7cd49554.mp4) \n CO2 responsive neurons\n\n- [wakeactiveneurons.mp4](https://assets-eu.researchsquare.com/files/rs-2865756/v1/37601c5e5d2d692c6c4f6563.mp4) \n Wake-active neurons\n\n- [REMactiveneurons3.mp4](https://assets-eu.researchsquare.com/files/rs-2865756/v1/9e3314547234857b99501cb1.mp4) \n REM-active neurons\n\n- [Suppfig13.pdf](https://assets-eu.researchsquare.com/files/rs-2865756/v1/2e6ff02c6c32ea0862c8c851.pdf)"} {"paper_id": "prb49", "title": "Molecular and connectomic vulnerability shape cross-disorder cortical abnormalities", "text": "Molecular and connectomic vulnerability shape cross-disorder cortical abnormalities\n\nJustine Hansen\nMontreal Neurological Institute, McGill University https://orcid.org/0000-0003-3142-7480\n\nGolia Shafiei\nMcGill University https://orcid.org/0000-0002-2036-5571\n\nJacob Vogel\nUniversity of Pennsylvania https://orcid.org/0000-0001-6394-9940\n\nKelly Smart\nYale School of Medicine\n\nCarrie Bearden\nUniversity of California at Los Angeles https://orcid.org/0000-0002-8516-923X\n\nMartine Hoogman\nDepartment of Human Genetics, Radboud University Medical Center\n\nBarbara Franke\nRadboud University\n\nDaan van Rooij\nJan Buitelaar\nRadboud University Medical Center https://orcid.org/0000-0001-8288-7757\n\nCarrie McDonald\nUniversity of California, San Diego\n\nSanjay Sisodiya\nUniversity College London\n\nLianne Schmaal\nThe University of Melbourne https://orcid.org/0000-0001-9822-048X\n\nDick Veltman\nAmsterdam University Medical Center\n\nOdile van den Heuvel\nUniversity of Amsterdam\n\nDan Stein\nUniversity of Cape Town https://orcid.org/0000-0001-7218-7810\n\nTheo van Erp\nUniversity of California, Irvine https://orcid.org/0000-0002-2465-2797\n\nChristopher Ching\nUSC\nOle Andreassen\nOslo University Hospital and University of Oslo\n\nTomas Hajek\nDalhousie University\n\nNils Opel\nUniversity of Münster\n\nGemma Modinos\nKing's College London\n\nAndré Aleman\nUniversity Medical Center Groningen\n\nYsbrand van der Werf\nUniversity of Amsterdam\n\nNeda Jahanshad\nUniversity of California, Los Angeles\n\nSophia Thomopoulos\nPaul Thompson\nImaging Genetics Center, Mark and Mary Stevens Neuroimaging & Informatics Institute, Keck School of Medicine of the University of Southern California, Marina del Rey, California, USA\n\nRichard Carson\nYale University https://orcid.org/0000-0002-9338-7966\n\nAlain Dagher\nNeurology and Neurosurgery, McGill University https://orcid.org/0000-0002-0945-5779\n\nBratislav Misic (✉ bratislav.misic@mcgill.ca )\nMontreal Neurological Institute, McGill University https://orcid.org/0000-0003-0307-2862\n\nArticle\n\nKeywords:\n\nPosted Date: February 3rd, 2022\n\nDOI: https://doi.org/10.21203/rs.3.rs-1293721/v1\n\nLicense: © This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nVersion of Record: A version of this preprint was published at Nature Communications on August 10th, 2022. See the published version at https://doi.org/10.1038/s41467-022-32420-y.\nMolecular and connectomic vulnerability shape cross-disorder cortical abnormalities\n\nJustine Y. Hansen1, Golia Shafiei1, Jacob W. Vogel2, Kelly Smart3, Carrie E. Bearden4, Martine Hoogman5,6, Barbara Franke5,6, Daan van Rooij6, Jan Buitelaar6, Carrie R. McDonald7, Sanjay M. Sisodiya8, Lianne Schmaal9, Dick J. Veltman10, Odile A. van den Heuvel10, Dan J. Stein11, Theo G. M. van Erp12, Christopher R. K. Ching13, Ole A. Andreassen14, Tomas Hajek15, Nils Opel16, Gemma Modinos17, André Aleman18, Ysbrand van der Werf10, Neda Jahanshahi13, Sophia I. Thomopoulos13, Paul M. Thompson13, Richard E. Carson3, Alain Dagher1, Bratislav Misic1*\n\n1McConnell Brain Imaging Centre, Montréal Neurological Institute, McGill University, Montréal, Canada\n2Department of Psychiatry, Perelman School of Medicine, University of Pennsylvania, Philadelphia, PA, USA\n3Department of Radiology and Biomedical Imaging, Yale School of Medicine, New Haven, CT 06520, USA\n4Departments of Psychiatry and Biobehavioral Sciences and Psychology, Semel Institute for Neuroscience and Human Behavior, University of California, Los Angeles, CA, USA\n5Departments of Psychiatry and Human Genetics, Radboud University Medical Center, Nijmegen, the Netherlands\n6Donders Institute for Brain, Cognition and Behavior, Radboud University, Nijmegen, The Netherlands\n7Department of Psychiatry, University of California San Diego, La Jolla, CA, USA\n8Department of Clinical and Experimental Epilepsy, UCL Queen Square Institute of Neurology, London, UK\n9Centre for Youth Mental Health, The University of Melbourne, Melbourne, Australia\n10Amsterdam UMC, Vrije Universiteit Amsterdam, Amsterdam Neuroscience, Amsterdam, the Netherlands\n11SA MRC Unit on Risk & Resilience in Mental Disorders, Dept of Psychiatry & Neuroscience Institute, University of Cape Town, Cape Town, South Africa\n12Clinical Translational Neuroscience Laboratory, Department of Psychiatry and Human Behavior,\n& Center for the Neurobiology of Learning and Memory, University of California Irvine, 309 Qureshey Research Lab, Irvine, CA, USA\n13Keck School of Medicine,\nImaging Genetics Center, Mark and Mary Stevens Neuroimaging and Informatics Institute, University of Southern California, Los Angeles, CA, USA\n14NORMENT Centre,\nInstitute of Clinical Medicine, University of Oslo and Division of Mental Health and Addiction, Oslo University Hospital, Oslo, Norway\n15Department of Psychiatry, Dalhousie University, Halifax, NS, Canada\n16Institute of Translational Psychiatry,\nUniversity of Münster, Münster, Germany & Department of Psychiatry, Jena University Hospital/Friedrich-Schiller-University Jena, Jena, Germany\n17Department of Psychosis Studies & MRC Centre for Neurodevelopmental Disorders, King’s College London, London, UK\n18Department of Biomedical Sciences of Cells and Systems, University of Groningen, Groningen, the Netherlands\n\nNumerous brain disorders demonstrate structural brain abnormalities, which are thought to arise from molecular perturbations or connectome miswiring. The unique and shared contributions of these molecular and connectomic vulnerabilities to brain disorders remain unknown, and has yet to be studied in a single multi-disorder framework. Using MRI morphometry from the ENIGMA consortium, we construct maps of cortical abnormalities for thirteen neurodevelopmental, neurological, and psychiatric disorders from \\( N = 21\\,000 \\) patients and \\( N = 26\\,000 \\) controls, collected using a harmonized processing protocol. We systematically compare cortical maps to multiple micro-architectural measures, including gene expression, neurotransmitter density, metabolism, and myelination (molecular vulnerability), as well as global connectomic measures including number of connections, centrality, and connection diversity (connectomic vulnerability). We find that regional molecular vulnerability and macroscale brain network architecture interact to drive the spatial patterning of cortical abnormalities in multiple disorders. Local attributes, particularly neurotransmitter receptor profiles, constitute the best predictors of both disorder-specific cortical morphology and cross-disorder similarity. Finally, we find that cross-disorder abnormalities are consistently subtended by a small subset of network epicentres in bilateral sensory-motor, medial temporal lobe, precuneus, and superior parietal cortex. Collectively, our results highlight how local biological attributes and global connectivity jointly shape cross-disorder cortical abnormalities.\n\nINTRODUCTION\n\nThe brain is a network with intricate connection patterns among individual neurons, neuronal populations, and large-scale brain regions. The wiring of the network supports propagation of electrical signals, as well as molecules needed for growth and repair. This complex system is vulnerable to multiple neurological, psychiatric and neurodevelopmental disorders. Pathological perturbations—including altered cellular morphology, cell death, aberrant synaptic pruning and miswiring—disrupt inter-regional communication and manifest as overlapping groups of sensory, motor, cognitive and affective symptoms. How different disorders are shaped by local and global vulnerability is unknown.\n\nIndeed, several studies have demonstrated cross-disorder connectomic vulnerability, where regions and white matter pathways are targeted non-randomly. In particular, regions that are highly connected and potentially important for communication tend to be disproportionately affected by disease [26, 114]. A sim-\nFigure 1. Molecular and connectomic cortical profiles | (a)–(b) Brain surfaces show the z-scored molecular (a) and connectomic (b) predictors used in the multilinear regression models. Heatmaps on the right show Pearson’s correlation coefficients between pairs of features. See Methods for details on how each feature was derived. Molecular predictors: gene PC1 = first component of 11 560 genes’ expression; receptor PC1 = first component of 18 PET-derived receptor/transporter density; E:I ratio = excitatory:inhibitory receptor density ratio; glycolytic index = amount of aerobic glycolysis; glucose metabolism = [18F]-labelled fluorodeoxyglucose (FDG) PET image; synapse density = synaptic vesicle glycoprotein 2A (SV2A)-binding [11C]UCB-J PET tracer; myelination = T1w/T2w ratio. Connectivity predictors: strength = sum of weighted connections; betweenness = fraction of all shortest paths traversing region i; closeness = mean shortest path length between region i and all other regions; Euclidean distance = mean Euclidean distance between region i and all other regions; participation coefficient = diversity of connections from region i to the seven Yeo-Krienen resting-state networks [130]; clustering = fraction of triangles including region i; mean first passage time = average time for a random walker to travel from region i to any other region.\n\nilar phenomenon is observed for connections that support multiple communication pathways [28]. In neurodegenerative diseases such as Alzheimer’s and Parkinson’s diseases, emerging evidence suggests pathological misfolded proteins spread trans-synaptically, such that the connectivity of the brain shapes the course and expression of these diseases [56, 84, 90, 91, 101, 125, 128, 134]. Recent evidence also suggests that patterns of tissue volume loss in schizophrenia are circumscribed by structural and functional connection patterns [103, 124]. Collectively, these studies demonstrate that both neurodevelopmental and neurodegenerative brain diseases are influenced by network connectivity [40, 115].\n\nThe effects of disease can also be driven by local cellular and molecular vulnerability. Namely, local patterns of gene expression [4, 18, 75], neurotransmitter receptor profiles [53], cellular composition [100], and metabolism [15, 16, 122, 123] may predispose individual regions to stress and, ultimately, pathology. Importantly, local and global vulnerability are not necessarily mutually exclusive; some diseases may originate from local pathologies that spread selectively along the network to other vulnerable regions. How local attributes and global connectivity shape cross-disorder pathology remains an open question.\n\nHere we map local molecular attributes (“molecular vulnerability”) and global network connectivity (“connectomic vulnerability”) to case versus control cortical thickness abnormalities of thirteen different neurological, psychiatric, and neurodevelopmental diseases and disorders from the ENIGMA consortium [111]. We consistently find that disorder-specific cortical abnormality is shaped more by the local molecular fingerprints of brain regions than network embedding. Interestingly, for disorders that are better predicted by molecular attributes, we find that the spatial patterning of cortical abnormalities reflects the underlying network architecture, suggesting that the local molecular and global connectomic contributions to disorder effects may interact.\nFigure 2. Local and global contributions to disorder-specific cortical morphology | (a) A total of twenty-six multilinear models were fit between local molecular and global connectome predictors to cortical abnormality maps of thirteen different disorders (surface plots, left). Adjusted \\( R^2 \\) is shown in the bar plot (orange: molecular; blue: connectivity). (b) Dominance analysis was applied to assess the contribution of each input variable (done separately for molecular (orange) and connectivity (blue) predictors) to the fit of the model. Significance was assessed using the spin-test (two-tailed); asterisks represent \\( p_{spin} < 0.05 \\).\n\nNext, we study cross-disorder similarity and find that regions with similar molecular make-up tend to be similarly affected across disorders. Collectively, the present report highlights how local and global factors interact to shape cross-disorder cortical morphology.\n\nRESULTS\n\nWe collected thirteen spatial maps of cortical abnormalities from the ENIGMA consortium for the following diseases, disorders, and conditions: 22q11.2 deletion syndrome (22q) [109], attention-deficit/hyperactivity disorder (ADHD) [55], autism spectrum disorder (ASD) [119], idiopathic generalized epilepsy [127], right temporal lobe epilepsy [127], left temporal lobe epilepsy [127], depression [99], obsessive-compulsive disorder (OCD) [13], schizophrenia [117], bipolar disorder (BD) [51], obesity [82], schizotypy [62], and Parkinson’s disease (PD) [63]. For simplicity, we refer to diseases, disorders, and conditions as “disorders” throughout the text. While most disorders show decreases in cortical thickness, some (e.g. 22q, ASD, schizotypy) also show regional increases in cortical thickness. We therefore refer to the cortical measure as “cortical abnormality”. All cortical abnormality maps were collected from adult patients, following identical processing protocols, for a total of over 21 000 scanned patients against almost 26 000 controls. To assess the extent to which each abnormality pattern is informed by molecular attributes and network connectivity, we defined a molecular and connectivity fingerprint at each brain region. The molecu-\nFigure 3. Comparing molecular and connectomic contributions to disorder-specific cortical differences | The local molecular \\( R^2_{adj} \\) of each disorder is plotted against the global connectivity \\( R^2_{adj} \\). The grey line indicates the identity line and circle colour represents the difference between molecular and connectomic \\( R^2_{adj} \\), such that warm colours represent disorders that are better predicted by molecular predictors, and cool colours represent disorders that are better predicted by connectomic predictors.\n\nlar fingerprint of a region was defined using the gene expression gradient, neurotransmitter receptor gradient, excitatory-inhibitory receptor density ratio, glycolytic index, glucose metabolism, synapse density, and myelination (Fig. 1a). Likewise, we defined the connectivity fingerprint of a region by calculating the strength, betweenness centrality, closeness centrality, mean Euclidean distance, participation coefficient, clustering coefficient, and mean first passage time of a weighted structural connectivity matrix from 70 healthy adults (Fig. 1b; see Methods for details). Collectively, these graph measures aim to capture the connectedness, centrality, and connection diversity of regions in the network. All analyses were conducted using the 68-region Desikan Killiany parcellation [19, 29], as this is the native and only available representation of ENIGMA datasets.\n\nLocal and global contributions to disorder-specific cortical morphology\n\nTo assess the extent to which cortical abnormalities of all thirteen disorders are informed by molecular gradients versus measures of network connectivity, we fit a multilinear model between molecular or connectivity predictors and abnormality maps for each disorder separately, for a total of \\( 13 \\times 2 = 26 \\) model fits (Fig. 2a; for results when measures of network connectivity were computed on the binary structural connectome and the functional connectome, see Fig. S1; for results when molecular and connectomic predictors are combined, see Fig. S2). Next, we conducted a dominance analysis for each multilinear model [5, 17, 67, 102]. Dominance analysis distributes the \\( R^2_{adj} \\) across input variables as a measure of contribution (\"dominance\") that each input variable has on the cortical thinning pattern (Fig. 2b). Dominance was assessed against a spatial autocorrelation-preserving null model (\"spin test\", see Methods for details), and each model was cross-validated in a distance-dependent manner (Fig. S3; [46]).\n\nWe find that the fit between molecular predictors and cortical thinning is greater than that between connectivity predictors and cortical thinning for most disorders (Fig. 3). Notably, the variance in cortical thickness of schizophrenia (a possible precursor of schizophrenia that is poorly defined in the brain [66]) and idiopathic generalized epilepsy (a form of epilepsy that is thought to be informed by genetics instead of brain structural abnormalities [24, 35]) are poorly explained by both biological gradients and network measures of the brain. On the other hand, ADHD, ASD, OCD, PD, and depression are better predicted by biological predictors, whereas schizophrenia, 22q deletion syndrome, and bipolar disorder are better predicted by connectivity predictors (Fig. 3).\n\nFrom the dominance analysis, we find that certain predictors are consistently unimportant. Indeed, synapse density and myelination demonstrate less dominance than microscale gradients such as the gene expression gradient, neurotransmitter receptor gradient, and metabolic gradients. Connectivity predictors, particularly measures of centrality, demonstrate less dominance than more fundamental measures of connectivity such as number of connections (strength), distance, and connection diversity (participation coefficient). For completeness, we tested a third family of predictors related to temporal dynamics: magnetoencephalography (MEG)-derived power spectral densities for six canonical frequency bands (Fig. S4). However, no temporal predictors were significantly dominant toward any disorders so we excluded the temporal predictors from further analyses.\n\nInteractions between local and global vulnerability\n\nThe previous section separately addresses molecular and connectomic contributions to disease-specific cortical abnormalities. However, molecular attributes likely interact with network connectivity to shape disease pathology. These molecular mechanisms include gene expression, neurotransmitter expression, and metabolic pathways in the cell. In neurodegenerative diseases, this interaction may result in synaptic pruning and cortical atrophy whereas in neurodevelopmental disorders, the pathology may manifest as perturbations in network wiring during the embryonic stage [30]. We hypothesized that abnormalities in such molecular mechanisms at the regional level may spread trans-synaptically\nFigure 4. Interactions between molecular and connectomic vulnerability | (a) Left: schematic of structural connectivity informing disorder-related cortical changes. The correlation between SC-weighted mean neighbour abnormality and region abnormality represents the extent to which a disorder demonstrates network spreading disorder-specific cortical morphology. Right: this correlation coefficient was then correlated to both local molecular (left) and global connectivity (right) \\( R^2_{adj} \\). Yellow points refer to disorders where the correlation between region abnormality and SC-weighted mean neighbour abnormality is significant (\\( p_{spin} < 0.05 \\)) (b) Left: likewise, mean neighbour abnormality can be additionally weighted by functional connectivity between regions. Right: correlation between the extent to which a disorder demonstrates SC- and FC-informed network spreading cortical morphology and local molecular (left) and global connectivity (right) \\( R^2_{adj} \\). Yellow points refer to disorders where the correlation between region abnormality and SC- and FC-weighted mean neighbour abnormality is significant (\\( p_{spin} < 0.05 \\)) (c) Left: a region with high abnormality that is also connected to regions with high abnormality is considered a likely disorder epicentre. Middle: epicentre likelihood was calculated as the mean rank of region and neighbour abnormality. Right: mean epicentre likelihood was calculated for all seven disorders that show a significant correlation between regional and neighbour abnormality.\n\nbetween connected regions, resulting in connectome-informed changes in cortical morphology that reflect an interplay between local vulnerability and network structure. For instance, two regions may both participate in many connections (have high degree), but one may be connected to more regions with local vulnerability. Thus, despite the fact that their connectomic profiles are similar, one region may have greater disease exposure than the other [14, 134].\n\nTo test the hypothesis that a region’s cortical thickness is driven by “exposure” to abnormalities of connected regions, we measured the extent to which disorders demonstrate network spreading patterns of cortical morphology [23, 101, 103]. The extent to which\nFigure 5. Brain regions with similar molecular annotations are similarly affected across disorders | (a) Disorder similarity was computed as the pairwise correlation of regional cortical thickness across all thirteen disorders such that pairs of regions with high disorder similarity are similarly affected across disorders. (b) The upper triangle of the disorder similarity matrix is approximately normally distributed. (c) Disorder similarity is significantly correlated to molecular attribute similarity, after distance-regression (\\( r = 0.38, p < 0.001 \\)). (d) Disorder similarity is less correlated to global connectome attribute similarity after distance-regression (\\( r = 0.22, p < 0.001 \\)). (e) Disorder similarity is significantly correlated to neurotransmitter receptor similarity, after distance-regression (\\( r = 0.33, p < 0.001 \\)). (f) Left hemisphere disorder similarity is significantly correlated to gene coexpression, after distance-regression (\\( r = 0.36, p < 0.001 \\)). (g) Disorder similarity is significantly greater within intrinsic functional networks than between networks, against the spin test (\\( p = 0.005 \\); top). Disorder similarity is significantly greater between structurally connected regions than regions that are not connected, against a degree- and edge-length-preserving null model (\\( p = 0.003 \\) [11]). (h) Disorder similarity is significantly correlated to functional connectivity, after distance-regression (\\( r = 0.26, p < 0.001 \\)).\n\na disorder displays network-informed cortical changes is defined as the correlation between regional abnormality and mean abnormality of structurally connected neighbours (Fig. 4a). Importantly, significance was assessed using a spatial autocorrelation preserving null model to control for the effect of distance on cortical abnormality patterns. We also test the hypothesis that this network-spreading effect is functionally informed, whereby the cortical thickness of structurally connected neighbours is weighted by the functional connectivity between regions when calculating the mean (Fig. 4b; see Methods for details and Fig. S5 and S6 for scatter plots of regional abnormality versus mean neighbour abnormality across all thirteen disorders). We find that multiple disorders display a significant correlation between regional thickness and thickness of connected neighbours (\\( 0.23 < r < 0.80 \\)), suggesting that spatial patterning of disorders reflects the connection patterns between brain regions, above and beyond the effect of spatial autocorrelation (Fig. S5).\n\nDoes molecular or connectomic predictability of a disorder pattern (Fig. 2a) relate to network spreading? Interestingly, the extent to which a disorder can be predicted from molecular attributes (i.e. yellow \\( R^2 \\) in Fig. 2a) is positively correlated with the extent to which a disorder displays evidence of network spreading (\\( r = 0.61, p = 0.03 \\) when weighted by SC only as shown in Fig. 4a; \\( r = 0.75, p = 0.003 \\) when weighted by FC and SC as shown in Fig. 4b). Notably, we do not observe this relationship with the extent to which a disorder can be predicted from global connectivity (i.e. blue \\( R^2 \\) in Fig. 2a; \\( r = 0.24, p = 0.42 \\) when weighted by SC only, Fig. 4a; \\( r = 0.06, p = 0.84 \\) when weighted by FC and SC, Fig. 4b). In other words, for disorders with cortical morphologies that more strongly depend on molecular attributes, we also observe a greater effect of disorder exposure. Although we previously found that the cortical patterning of a disorder is less influenced by network embedding per se (e.g. centrality or connection diversity), here we show that it is instead more influenced by network-driven exposure to regions with local vulnerability. This finding is significant because it shows that connectome architecture interacts with local vulnerability.\n\nBrain regions with high abnormality and high neighbour abnormality are likely to act as an epicentre of the network spreading disorder pattern, since the region is both heavily affected and facilitates the spread of atypical morphology [14, 103, 133]. We calculated epicentre likelihood of each brain region as the mean rank of regional and neighbour abnormality, such that regions with high node and neighbour abnormality would be la-\nbeled as likely epicentres (Fig. 4c). The measure identifies “disorder hubs”—regions that are both vulnerable to disorder-specific changes but also embedded in a highly atypical network cluster. Epicentre likelihood was only calculated for brain maps with significant correlation between their node and neighbour abnormality (network spreading disorders). This list comprised of: 22q11.1 deletion syndrome, ADHD, ASD, right and left temporal epilepsy, bipolar disorder, and schizotypy (Fig. S7). We averaged epicentre likelihood of these seven disorders to produce a map of epicentre likelihood across disorders that demonstrate network spreading disorder-specific cortical morphology (Fig. 4c, right). We find that cross-disorder epicentre likelihood is highest in bilateral sensory-motor cortex, medial temporal lobe, precuneus, and superior parietal cortex.\n\nBrain regions with similar molecular annotations are similarly affected across disorders\n\nIn the previous sections, we mapped molecular annotations and network measures to each disorder separately. Here, we focused on disorder similarity. For every region we constructed a 13-element vector of abnormality values, where each element corresponds to cortical change in that region in one disorder. We then correlated regional vectors with each other to estimate how similarly two regions are affected across the thirteen disorders (Fig. 5a).\n\nWe first asked whether brain regions with similar molecular versus connectivity fingerprints show greater disorder similarity. Molecular similarity was likewise computed as the pairwise regional correlation of molecular predictors, and vice versa for connectivity. To account for spatial autocorrelation in molecular and connectomic attributes, we regressed the exponential trend with Euclidean distance out of molecular similarity, connectivity similarity, and disorder similarity (Fig. S8a, b, c). After distance-regression, we find that disorder similarity is significantly correlated with molecular similarity (\\( r = 0.38, p < 0.001 \\); Fig. 5c). On the other hand, the correlation between distance-regressed connectivity similarity and disorder similarity was smaller and less visually apparent, albeit significant (\\( r = 0.23, p < 0.001 \\); Fig. 5d).\n\nTwo of the molecular predictors included in the present report are summary measures of much more expansive molecular annotations: the gene expression gradient and the neurotransmitter receptor gradient. We therefore asked whether inter-regional similarity of these molecular attributes confers similar predisposition to disease. We computed gene coexpression and neurotransmitter receptor similarity matrices, regressed out the exponential trend with Euclidean distance as before (Fig. S8d, e, [39, 47]), and correlated these matrices with disorder similarity (Fig. 5e, f). We find a significant correlation between disorder similarity and neurotransmitter receptor similarity (\\( r = 0.33, p < 0.001 \\)) as well as gene coexpression (\\( r = 0.36, p < 0.001 \\)) [3, 47]. Altogether, our results indicate that regions with similar biological composition are similarly affected across disorders.\n\nWe finally ask whether disorder similarity might analogously be informed by structural and functional connectivity between regions. We compared the disorder similarity matrix to weighted structural and functional connectomes. First, we find that brain regions that are structurally connected are more likely to change similarly across disorders than regions that are not structurally connected, although this result is non-significant against a degree and edge-length preserving null model (Fig. 5g [11]; see Null models). Second, we find that brain regions that are within the same intrinsic functional network are more likely to change similarly than regions between functional networks, against the spin-test (Fig. 5g, \\( p_{spin} = 0.01 \\)). Finally, we find a positive significant correlation between disorder similarity and functional connectivity (\\( r = 0.26, p_{spin} = 0.002 \\); Fig. 5h). Consistent with the previous subsection, these results collectively suggest that areas that share molecular attributes and connections are similarly affected across disorders.\n\nDISCUSSION\n\nIn the present report, we comprehensively map local molecular attributes and global measures of connectivity to the cortical morphology of thirteen different neurological, psychiatric, and neurodevelopmental disorders. We consistently find that local attributes govern both disorder-specific abnormalities and cross-disorder similarity more than global connectivity and regional dynamics. In addition, we find that molecular mechanisms interact with the structural and functional architectures of the brain to guide cross-disorder abnormality patterns. Altogether, our results highlight how molecular and connectomic vulnerability shape cross-disorder cortical abnormalities.\n\nThis work builds on a growing literature on cross-disorder effects, and how shared vulnerability may potentially transcend traditional diagnostic boundaries [28, 61, 120, 129]. It is becoming increasingly clear that pathology is governed by layers of abnormal processes, at the molecular and cellular level, to neural dynamics, to large-scale brain networks. Aligning high-quality maps of disorder-specific cortical changes to a common reference frame of local and global attributes allows us to systematically relate the effect of disease to multiple scales of organization. By taking a cross-modal and cross-disorder approach we reveal that, despite different clinical presentation and label, there exists some commonality across diseases including predictors that are ubiquitously important as well as interplay between local vulnerability and network structure.\n\nInterestingly, we find that the principal gradient of\nreceptor distribution is particularly dominant towards disease-specific cortical morphology. This receptor gradient represents the maximal variance of density distributions from fourteen receptors and four transporters across nine different neurotransmitter systems, and therefore captures how brain regions may integrate exogenous signals differently [47, 104]. This gradient is a powerful predictor of ADHD, and is the only significantly dominant predictor of left temporal lobe epilepsy, depression, and Parkinson’s disease. Indeed, neurotransmitter dysfunction is thought to underlie multiple disorders, including dopamine release in PD and schizophrenia or serotonin reuptake in depression. Modern therapeutics are designed to selectively manipulate neurotransmitter function for the purpose of alleviating behavioural symptoms, as opposed to altering brain structure. Our findings confirm the fundamental contribution of neurotransmitters to a wide spectrum of diseases, but they also highlight an important link between the spatial patterning of neurotransmitter receptors and cortical disorder morphology itself [47].\n\nWe generally find that cortical abnormality is better predicted by local vulnerability compared to global connectomic vulnerability. One possible reason for the relatively poorer performance of connectivity predictors is that they are generic measures of a region’s embedding in a network (number of connections, centrality, connection diversion) but do not consider how this embedding exposes regions to pathology elsewhere in the network. Indeed, we find that disorders whose cortical morphology is better reflected by local vulnerability also bear a prominent signature of network architecture (e.g. ASD, ADHD, 22q, temporal lobe epilepsy, schizotypy, bipolar disorder). Namely, in these disorders, areas with greater change are disproportionately more likely to be structurally- and functionally-connected with each other. This suggests a network spreading phenomenon where focal pathology or perturbation propagates to connected regions, resulting in cortical abnormality that is correlated with the underlying connection patterns [40]. This interaction between local vulnerability and connectomic vulnerability has previously been reported in neurodegenerative syndromes where the trans-synaptic spreading of misfolded proteins appears to be guided and amplified by local gene expression [25, 50, 92].\n\nThe interaction between molecular vulnerability and network structure naturally raises the question of what are the network epicentres of cortical disorder maps. We find epicentres—regions with high abnormality that are also strongly connected with other regions with high abnormality—in the sensory-motor cortex, medial temporal lobe, precuneus, and superior parietal cortex. That the sensory-motor cortex is an epicentre is consistent with recent reports that multiple psychiatric and neurological disorders are accompanied by sensory deficits and reduced motor control [10, 57, 69]. Indeed, the sensory-motor cortex has been previously established as a functional hub in temporal lobe epilepsies and across multiple psychiatric disorders [61, 65]. Interestingly, both the bilateral precuneus and superior parietal cortex are members of the brain’s putative rich club—densely interconnected regions that are thought to support the integration and broadcasting of signals [113]. Rich club regions undergo changes in connectivity patterns in multiple diseases such as schizophrenia, Alzheimer’s, and Huntington’s [28, 115, 116]. We complement this work by showing that the precuneus and superior parietal cortex are both vulnerable to cortical abnormality and, by virtue of their network embedding, increase disease exposure to connected regions. Conversely, although the anterior cingulate cortex (ACC) is implicated across multiple psychiatric disorders [45, 103], we do not find that the ACC is an epicentre of cross-disorder cortical morphology. This suggests that although the ACC demonstrates considerable local vulnerability in a subset of brain disorders, it is not consistently involved across the seven disorders included in the epicentre analyses. Altogether, despite variable cortical morphology patterns across the thirteen disorders, when looked at through the lens of network connectivity, we see a more consistent and compact subset of potential epicentres, suggesting greater commonality among diseases than previously appreciated.\n\nThe present work should be considered along some important methodological considerations. First, although the ENIGMA consortium standardizes pre-processing pipelines and provides large \\( N \\) datasets, allowing for robust results and meaningful comparison between disorder-specific cortical abnormality maps, working with ENIGMA data also has caveats: (1) the measures of cortical abnormality are effect sizes between patients and controls and do not represent tissue volume loss/gain, (2) some of the patient populations included have co-morbidities and patients may be undergoing treatment, and (3) all analyses were conducted at the level of 68 cortical brain areas, limiting regional specificity and precluding analyses of the subcortex and cerebellum. Second, despite the fact that structural connectomes were reconstructed from high resolution diffusion spectrum imaging, diffusion tractography is still prone to false-positives and false-negatives [58, 68, 132]. Third, both local biological and global connectivity predictors are derived from state-of-the-art open-access datasets in healthy participants, but they do not capture individual variability or changes across the lifespan—both of which are key factors in neurological, psychiatric, and neurodevelopmental disorders. Additionally, the biological predictors are limited by imaging modality and, in the case of the gene and receptor gradients, by the subset of genes and receptors included in the data decomposition. Fourth, we assessed contribution of multiple predictors to disorder maps using simple but robust linear models that are not sensitive to non-linear contributions or higher-order interactions among the predictors. Fifth, the linear models used in the present analyses assume independence between observations, which is not the case\nin the brain; we therefore employ spatial-autocorrelation preserving null models to account for the spatial dependencies between regions throughout the report. Finally, although the present report spans a wide range of neurological, psychiatric, and neurodevelopmental disorders, results are only valid for this subset of disorders. Future work is needed to map local and global vulnerabilities to the many more brain diseases and disorders that exist.\n\nIn summary, we find that molecular and connectomic vulnerability jointly shape cross-disorder cortical abnormalities. Cross-disorder regional vulnerability is largely driven by molecular fingerprints, including neurotransmitter receptor densities and gene expression, while connection patterns among vulnerable regions further amplify this vulnerability. Our results highlight how an integrative, multi-modal approach can illuminate the contributions of local biology and connectome architecture to brain disease.\n\nMETHODS\n\nAll code and data used to perform the analyses can be found at https://github.com/netneurolab/hansen_crossdisorder_vulnerability. Molecular predictors can also be found in the neuromaps toolbox (https://netneurolab.github.io/neuromaps/ [71]).\n\nCortical disorder maps\n\nPatterns of cortical thickness were collected for the available thirteen neurological, neurodevelopmental, and psychiatric disorders from the ENIGMA consortium and the enigma toolbox (https://github.com/MICA-MNI/ENIGMA; [64]) including: 22q11.2 deletion syndrome (22q) [109], attention-deficit/hyperactivity disorder (ADHD) [55], autism spectrum disorder (ASD) [119], idiopathic generalized epilepsy [127], right temporal lobe epilepsy [127], left temporal lobe epilepsy [127], depression [99], obsessive-compulsive disorder (OCD) [13], schizophrenia [117], bipolar disorder (BD) [51], obesity [82], schizotypy [62], and Parkinson's disease (PD) [63]. The ENIGMA (Enhancing Neuroimaging Genetics through Meta-Analysis) Consortium is a data-sharing initiative that relies on standardized image acquisition and processing pipelines, such that disorder maps are comparable [111]. Altogether, over 21 000 patients were scanned across the thirteen disorders, against almost 26 000 controls. The values for each map are z-scored effect sizes (Cohen's d) of cortical thickness in patient populations versus healthy controls. Imaging and processing protocols can be found at http://enigma.ini.usc.edu/protocols/.\n\nStructural and functional data acquisition\n\nStructural and functional data were collected at the Department of Radiology, University Hospital Center and University of Lausanne, on \\( n = 70 \\) healthy young adults (16 females, \\( 25.3 \\pm 4.9 \\) years). Informed consent was obtained from all participants and the protocol was approved by the Ethics Committee of Clinical Research of the Faculty of Biology and Medicine, University of Lausanne. The scans were performed in a 3-T MRI scanner (Trio; Siemens Medical), using a 32-channel head coil. The protocol included (1) a magnetization-prepared rapid acquisition gradient echo (MPRAGE) sequence sensitive to white/grey matter contrast (1 mm in-plane resolution, 1.2 mm slice thickness), (2) a DSI sequence (128 diffusion-weighted volumes and a single b0 volume, maximum b-value 8000s/mm\\(^2\\), \\( 2.2 \\times 2.2 \\times 3.0 \\) mm voxel size), and (3) a gradient echo-planar imaging (EPI) sequence sensitive to blood-oxygen-level-dependent (BOLD) contrast (3.3 mm in-plane resolution and slice thickness with a 0.3 mm gap, TR 1920 ms, resulting in 280 images per participant). Participants were not subject to any overt task demands during the fMRI scan. The Lausanne dataset is available at https://zenodo.org/record/2872624#.XOJqE99fhM.\n\nStructural network reconstruction\n\nGrey matter was parcellated according to the 68-region Desikan-Killiany cortical atlas [29]. Structural connectivity was estimated for individual participants using deterministic streamline tractography. The procedure was implemented in the Connectome Mapping Toolkit [27], initiating 32 streamline propagations per diffusion direction for each which matter voxel. Collating each individual's structural connectome was done using a group-consensus approach that seeks to preserve the density and edge-length distributions of the individual connectomes [11].\n\nWe first collated the extant edges in the individual participant matrices and binned them according to length. The number of bins was determined heuristically, as the square root of the mean binary density across participants. The most frequently occurring edges were then selected for each bin. If the mean number of edges across participants in a particular bin is equal to \\( k \\), we selected the \\( k \\) edges of that length that occur most frequently across participants. To ensure that interhemispheric edges are not underrepresented, we carried out this procedure separately for inter- and intrahemispheric edges. The binary density for the final whole-brain structural connectome was 24.6%. For the weighted structural connectome, edges were weighted by the log-transform of the mean non-zero streamline density, scaled to values between 0 and 1.\nFunctional network reconstruction\n\nFunctional MRI data were preprocessed using procedures designed to facilitate subsequent network exploration [86]. fMRI volumes were corrected for physiological variables, including regression of white matter, cerebrospinal fluid, and motion (3 translations and 3 rotations, estimated by rigid body coregistration). BOLD time series were then subjected to a low-pass filter (temporal Gaussian filter with full width at half maximum equal to 1.92 s). The first four time points were excluded from subsequent analysis to allow the time series to stabilize. Motion “scrubbing” was performed as described by [86]. The data were parcelated according to the same 68-region Desikan-Killiany atlas used for the structural network. Individual functional connectivity matrices were defined as zero-lag Pearson correlation among the fMRI BOLD time series. A group-consensus functional connectivity matrix was estimated as the mean connectivity of pairwise connections across individuals. Note that one individual did not undergo an fMRI scan and therefore the functional connectome was composed of \\( n = 69 \\) participants.\n\nBiological predictors\n\nA total of seven local biological predictors were used in the multilinear model to represent the influence that local biological attributes have on disorder-specific cortical morphology.\n\nGene expression gradient. The first principal component of gene expression (“gene gradient”) was used to represent the variation in gene expression levels across the left cortex. Gene expression data was collected by the Allen Human Brain Atlas as described in Hawrylycz et al. [49] and processed by abagen, an open-source Python toolbox [70]. A total of 11 560 genes with differential stability greater than 0.1 were retained in the region by gene matrix [48]. The left gene gradient was mirrored in the right hemisphere. A detailed account of the specific processing choices made can be found in Hansen et al. [46].\n\nReceptor gradient. The first principal component of receptor density (“receptor gradient”) was used to represent the variation in receptor densities across the cortex. Receptor densities were estimated using PET tracer studies for a total of 18 receptors and transporters, across 9 neurotransmitter systems. These include dopamine (D₁ [59], D₂ [96, 105, 108, 131], DAT [33]), norepinephrine (NET [8, 22, 31, 95]), serotonin (5-HT₁A [98], 5-HT₁B [6, 41, 73, 76, 77, 85, 97, 98], 5-HT₂A [9], 5-HT₄ [9], 5-HT₆ [87, 88], 5-HTT [9]), acetylcholine (\\( \\alpha_4\\beta_2 \\) [6, 52], M₁ [78], VACHT [1, 7]), glutamate (mGluR₅ [32, 106]), GABA (GABAₐ [80]), histamine (H₃ [42]), cannabinoid (CB₁ [34, 79, 81, 93]), and opioid (MOR [60]). Volumetric PET images were registered to the MNI-ICBM 152 nonlinear 2009 (version c, asymmetric) template, averaged across participants within each study, then parcelated to 68 cortical regions. Parcellated PET maps were then z-scored before compiling all receptors/transporters into a region×receptor matrix of relative densities. Data were originally presented as an atlas in Hansen et al. [47].\n\nExcitatory-inhibitory ratio. The excitatory-inhibitory ratio was computed as the ratio of z-scored PET-derived excitatory to inhibitory neurotransmitter receptor densities in the cortex, using the same dataset that was used to compute the receptor gradient. Excitatory neurotransmitter receptors included are: 5-HT₂A, 5-HT₄, 5-HT₆, D₁, mGluR₅, \\( \\alpha_4\\beta_2 \\), and M₁. Inhibitory neurotransmitter receptors included are: 5-HT₁A, 5-HT₁B, CB₁, D₂, GABAₐ, H₃, and MOR.\n\nGlycolytic index. Aerobic glycolysis is the process of converting glucose to lactate in the presence of oxygen. It is traditionally calculated as the ratio of oxygen metabolism to glucose metabolism. Here, we use glycolytic index, a measure of aerobic glycolysis that mitigates certain limitations of using the traditional ratio [112]. Glycolytic index is defined as the residual after fitting glucose metabolism to oxygen metabolism in a linear regression model. Larger values indicate more aerobic glycolysis. Note that glycolytic index and the traditional ratio are highly correlated (see Vaishnavi et al. [112]). Data were collected, calculated, and made available by Vaishnavi et al. [112].\n\nGlucose metabolism. Glucose metabolism in the cortex was measured in 33 healthy adults by administering [¹⁸F]-labelled fluorodeoxyglucose (FDG) for a PET scan, as described in detail in Vaishnavi et al. [112].\n\nSynapse density. Synapse density in the cortex was measured in 76 healthy adults (45 males, 48.9 ± 18.4 years of age) by administering [¹¹C]UCB-J, a PET tracer that binds to the synaptic vesicle glycoprotein 2A (SV2A) [12, 20, 21, 36–38, 54, 74, 83, 89, 107, 126]. Data were collected on an HRRT PET camera for 90 minutes post injection. Non-displaceable binding potential (BPND) was modelled using SRTM2, with the centrum semiovale as reference and \\( k'_2 \\) fixed to 0.027 (population value).\n\nMyelination. Data from the Human Connectome Project (HCP, S1200 release) [43, 118] was used for measures of T1w/T2w ratios—a proxy for intracortical myelin—for 417 unrelated participants (age range 22–37 years, 193 males), as approved by the WU-Minn HCP Consortium. Images were acquired on a Siemens Skyra 3T scanner, and included a T1-weighted MPRAGE sequence at an isotropic resolution of 0.7mm, and a T2-weighted SPACE also at an isotropic resolution of 0.7mm. Details on imaging protocols and procedures are available at http://protocols.humanconnectome.org/HCP/3T/imaging-protocols.html. Image processing includes correcting for gradient distortion caused by non-linearities, correcting for bias field distortions, and registering the images to a standard reference space. T1w/T2w ratios for each participant was made available in the surface-based CIFTI file format and parcel-\nlated into 68 cortical regions according to the Lausanne anatomical atlas [19].\n\nConnectivity predictors\n\nA total of nine global connectome predictors were used in the multilinear model to represent the influence that global connectivity has on disorder-specific cortical morphology. In the main text, connectome measures were computed on the weighted structural connectome. Analyses were repeated using a binary structural connectome and an absolute functional connectome (Fig. S1). All connectivity measures were computed using the Python-equivalent of the Brain Connectivity Toolbox, bctpy.\n\nStrength. The strength of region \\( i \\) is the sum of the edges connected to region \\( i \\). For a binary structural connectome, the strength is equivalent to the degree, which is the number of links connected to region \\( i \\).\n\nBetweenness centrality. Betweenness centrality of region \\( i \\) is the fraction of all shortest paths between any two regions that traverse region \\( i \\).\n\nCloseness centrality. Closeness centrality is equivalent to the mean shortest path distance from region \\( i \\) to every other region in the network.\n\nEuclidean distance. Mean Euclidean distance of a region to all other regions in the network represents how spatially close one region is to all other regions.\n\nParticipation coefficient. Participation coefficient was computed using the putative intrinsic functional networks of the brain [130]. Participation coefficient represents the connection diversity of a region. A region with high participation coefficient is well connected to several different networks, whereas a region with low participation coefficient primarily makes local (within-network) connections.\n\nClustering coefficient. The clustering coefficient of region \\( i \\) is the fraction of all triangles that are around region \\( i \\). Equivalently, it is the fraction of all of region \\( i \\)'s neighbours that are also neighbours with each other. In the case of the weighted structural connectome, clustering coefficient is the average geometric mean of all triangles associated with the region.\n\nMean first passage time. The mean first passage time from region \\( i \\) to \\( j \\) is the expected amount of time it takes a random walker to reach region \\( j \\) from \\( i \\) for the first time. For each region, mean first passage time was averaged across regions, resulting in a mean mean first passage time representing the average amount of time it takes a random walker to travel from region \\( i \\) to any other region in the network for the first time.\n\nTemporal predictors\n\n6-minute resting-state eyes-open magenetoencephalography (MEG) time-series were acquired from the Human Connectome Project (HCP, S1200 release) for 33 unrelated subjects (age range 22—35, 17 males) [43, 118]. Complete MEG acquisition protocols can be found in the HCP S1200 Release Manual. For each subject, we computed the power of the run at the vertex level across six different frequency bands: delta (2–4 Hz), theta (5–7 Hz), alpha (8–12 Hz), beta (15–29 Hz), low gamma (30–59 Hz), and high gamma (60–90 Hz), using the open-source software, Brainstorm [110]. Each power band was then parcellated into 68 cortical regions [19].\n\nDominance analysis\n\nDominance analysis seeks to determine the relative contribution (“dominance”) of each input variable to the overall fit (adjusted \\( R^2 \\)) of the multiple linear regression model (https://github.com/dominance-analysis/dominance-analysis [5, 17]). This is done by fitting the same regression model on every combination of input variables (\\( 2^p - 1 \\) submodels for a model with \\( p \\) input variables). Total dominance is defined as the average of the relative increase in \\( R^2 \\) when adding a single input variable of interest to a submodel, across all \\( 2^p - 1 \\) submodels. The sum of the dominance of all input variables is equal to the total adjusted \\( R^2 \\) of the complete model, making total dominance an intuitive measure of contribution. Significant dominance was assessed using the spin test (see Null models), whereby dominance analysis was repeated between a spun disorder map and the original predictor matrix (1 000 repetitions).\n\nEach multilinear model was cross-validated using a distance-dependent method proposed by [46]. Briefly, for each of 1 000 iterations, the 75% of regions closest in Euclidean distance to a randomly chosen source node were selected as the training set, and the remaining 25% of regions as the test set. Predicted values in the test set were then correlated to true abnormality patterns, and the correlations are shown in Fig. S3.\n\nNetwork spreading\n\nNetwork spreading was computed as first introduced in Shafiei et al. [103] and later adopted in [23, 101]. Briefly, regional abnormality was defined as the normalized effect size used in all ENIGMA brain maps. For each region \\( i \\), its neighbours are those with which region \\( i \\) is connected via a structural connection, as defined by the structural connectivity matrix. Mean neighbour abnormality of region \\( i \\) (\\( D_i \\)) is the average abnormality of region \\( i \\)'s neighbours, where \\( d_j \\) represents the abnormality of neighbour \\( j \\). Notably, this method normalizes neighbour abnormality by the number of connections made by region \\( i \\) (\\( N_i \\)).\n\\[\nD_i = \\frac{1}{N_i} \\sum_{j \\neq i, j=1}^{N_i} d_j \\times SC_{ij}\n\\]\n\nWhen neighbour abnormality is weighted by functional connectivity, each neighbour’s abnormality are weighted by the functional connection to node \\(i\\) (\\(FC_{ij}\\)).\n\n\\[\nD_i = \\frac{1}{N_i} \\sum_{j \\neq i, j=1}^{N_i} d_j \\times SC_{ij} \\times FC_{ij}\n\\]\n\nEach brain region was assigned a rank in terms of their node abnormality and their mean neighbour abnormality. The average of node and neighbour abnormality ranks was defined as the epicentre likelihood of the node, where nodes with high abnormality and whose neighbours are also highly atypical are more likely to be an epicentre of the disorder.\n\nDisorder similarity\n\nFor every brain region, we constructed a 13-element vector of disorder abnormality, where each element represents a disorder’s cortical abnormality at the region. For every pair of brain regions, we correlated the abnormality vectors to quantify how similarly two brain regions are affected across disorders. This results in a region-by-region matrix of “disorder similarity” (Fig. 5a). We verified that no single disorder pattern was driving the disorder similarity matrix by recalculating the disorder similarity when a single disorder is excluded. We then correlated the leave-one-out disorder similarity matrix with the original disorder similarity matrix. The minimum correlation was \\(r = 0.95\\) (Fig. S9a). Finally, influence on the disorder similarity matrix by a disorder \\(i\\) was quantified as\n\n\\[\nI_i = 1 - \\text{Corr}(D, D_i)\n\\]\n\nwhere \\(D\\) is the original disorder similarity matrix and \\(D_i\\) is the disorder similarity matrix constructed when disorder \\(i\\) is excluded (Fig. S9b).\n\nNull models\n\nSpatial autocorrelation-preserving permutation tests were used to assess statistical significance of associations across brain regions, termed “spin tests” [2, 72]. We created a surface-based representation of the parcellation on the FreeSurfer fsaverage surface, via files from the Connectome Mapper toolkit (https://github.com/LTS5/cmp). We used the spherical projection of the fsaverage surface to define spatial coordinates for each parcel by selecting the coordinates of the vertex closest to the center of the mass of each parcel [121]. These parcel coordinates were then randomly rotated, and original parcels were reassigned the value of the closest rotated parcel (1 000 repetitions). Parcels for which the medial wall was closest were assigned the value of the next most proximal parcel instead. The procedure was performed at the parcel resolution rather than the vertex resolution to avoid upsampling the data, and to each hemisphere separately.\n\nA second null model was used to test whether disorder similarity is greater in connected regions than unconnected regions. This model generates a null structural connectome that preserves the density, edge length, and degree distributions of the empirical structural connectome [11, 44, 94]. Briefly, edges were binned according to Euclidean distance. Within each bin, pairs of edges were selected at random and swapped. This procedure was then repeated 10 000 times. To compute a p-value, the mean disorder similarity of unconnected edges was subtracted from the mean disorder similarity of connected edges, and this difference was compared to a null distribution of differences computed on the rewired networks.\n\nConflicts of Interest\n\nCRKC, NJ, PMT received partial research support from Biogen, Inc., for research unrelated to this manuscript. JB has been in the past 3 years a consultant to/member of advisory board of/and/or speaker for Takeda/Shire, Roche, Medice, Angelini, Janssen, and Servier. He is not an employee of any of these companies, and not a stock shareholder of any of these companies. He has no other financial or material support, including expert testimony, patents, royalties. BF has received educational speaking fees from Medice GmbH. D.J.S. has received research grants and/or consultancy honoraria from Lundbeck and Sun.\n\nAcknowledgments\n\nThis research was undertaken thanks in part to funding from the Canada First Research Excellence Fund, awarded to McGill University for the Healthy Brains for Healthy Lives initiative. BM acknowledges support from the Natural Sciences and Engineering Research Council of Canada (NSERC Discovery Grant RGPIN #017-04265), the Canada Research Chairs Program, the Brain Canada Future Leaders Fund and the Healthy Brains for Healthy Lives initiative. JYH acknowledges support from the Helmholtz International BigBrain Analytics & Learning Laboratory, the Natural Sciences and Engineering Research Council of Canada, and the Fonds de recherches de Québec.\n\nThe research studies produced by the ENIGMA Working Groups would not be possible without the contribu-\ntions of many researchers across the globe and the authors of this work thank all scientists who contribute to making this work possible. A full list of ENIGMA Consortium current and past members can be found here http://enigma.ini.usc.edu/ongoing/members/. The authors acknowledge the NIH Big Data to Knowledge (BD2K) award for foundational support and consortium development (U54 EB020403 to PMT) and support from NIMH R01MH116147 (PMT), NIMH R01MH116147 (JAT, TGMvE), NIMH R01 MH117601 (NJ, LS), NIMH R01MH085953 (CEB), NIMH R21MH116473 (CEB), NIMH 1U01MH119736 (CEB). For a complete list of ENIGMA-related grant support please see here: http://enigma.ini.usc.edu/about-2/funding. JB has been supported by the EU-AIMS (European Autism Interventions) and AIMS-2-TRIALS programmes which receive support from Innovative Medicines Initiative Joint Undertaking Grant No. 115300 and 777394, the resources of which are composed of financial contributions from the European Union’s FP7 and Horizon2020 Programmes, and from the European Federation of Pharmaceutical Industries and Associations (EFPIA) companies’ in-kind contributions, and AUTISM SPEAKS, Autistica and SFARI; and by the Horizon2020 supported programme CANDY Grant No. 847818). BF is supported by the European Community’s Horizon 2020 Programme (H2020/2014 – 2020) under grant agreements n° 667302 (CoCa), n° 728018 (Eat2BeNICE), and n° 847879 (PRIME). This work was supported by a personal Veni grant to MH from the Netherlands Organization for Scientific Research (NWO, grant number 91619115). CRM is supported by NIH R01 NS065838; R21 NS107739. DJS is supported by South African Medical Research Council. 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Neuroimage, 142:407–420.\n\n[133] Zeighami, Y., Ulla, M., Iturria-Medina, Y., Dadar, M., Zhang, Y., Larcher, K. M.-H., Fonov, V., Evans, A. C., Collins, D. L., and Dagher, A. (2015). Network structure of brain atrophy in de novo parkinson’s disease. elife, 4:e08440.\n\n[134] Zheng, Y.-Q., Zhang, Y., Yau, Y., Zeighami, Y., Larcher, K., Misic, B., and Dagher, A. (2019). Local vulnerability and global connectivity jointly shape neurodegenerative disease propagation. PLoS Biol, 17(11).\nFigure S1. Computing global network measures on different connectivity matrices | Global network measures were calculated on the binary structural connectivity matrix as well as the weighted functional connectivity matrix. (a) Adjusted \\( R^2 \\) between connectivity predictors and disorder maps (left-most surfaces) when connectivity measures were calculated on the binary structural connectome (dark blue), weighted structural connectome (medium blue; used in main text analyses), and weighted functional connectome (light blue). (b) Dominance analysis for the binary structural connectome (left) and weighted functional connectome (right). Asterisks represent \\( p_{\\text{spin}} < 0.05 \\).\nFigure S2. Combining molecular and connectomic predictors | Thirteen multivariate regression models were fit between the combined (molecular and connectomic) predictor set, to predict disorder-specific cortical thinning. Dominance analysis was applied to assess the predictors that contribute most to each mode. Asterisks represent \\( p_{\\text{spin}} < 0.05 \\).\n\nFigure S3. Distance-dependent cross-validation | Each model was cross-validated using a distance-dependent method. For 1 000 randomly chosen source regions, the model was fit on a training set, composed of the 75% of regions closes to the source region. Next, cortical abnormality values were predicted on the remaining 25% of regions and correlated to the empirical abnormality values. Circles represent the median and lines span the first to third quartiles.\nFigure S4. Mapping MEG-derived temporal predictors to disorder-specific cortical morphology | For each disorder, a multi-linear model was fit between six MEG-derived power distributions and the abnormality pattern. Dominance analysis extracted no significantly dominant predictors, and fits always underperformed compared to local biological predictors.\nFigure S5. Assessing network spreading disorder-specific cortical morphology using structural and functional connectivity | A disorder whose cortical morphology demonstrates network spreading was defined as one whose regional abnormality pattern is correlated to mean neighbour abnormality, weighted by structural connectivity and functional connectivity. Yellow scatter plots indicate significant (\\( p_{\\text{spin}} < 0.05 \\)) node-neighbour correlations.\n\n![Scatter plots showing node abnormality vs neighbour abnormality for various disorders, with yellow points indicating significant correlations](page_120_68_1347_495.png)\n\nFigure S6. Assessing network spreading disorder-specific cortical morphology using structural connectivity only | A disorder whose cortical morphology demonstrates network spreading was defined as one whose regional abnormality pattern is correlated to mean neighbour abnormality, weighted by structural connectivity only. Yellow scatter plots indicate significant (\\( p_{\\text{spin}} < 0.05 \\)) node-neighbour correlations.\n\n![Scatter plots showing node abnormality vs neighbour abnormality for various disorders, with yellow points indicating significant correlations](page_120_570_1347_495.png)\nFigure S7. Epicentre likelihood | Epicentre likelihoods of the seven disorders that demonstrate significant correlations between node abnormality and mean sc- and fc-weighted neighbour abnormality.\n\nFigure S8. Annotation similarity between brain regions decreases exponentially | Similarity matrices for (a) disorder-specific cortical morphology, (b) local molecular fingerprint similarity, (c) global connectome predictor similarity, (d) neurotransmitter receptor density, (e) gene coexpression, and (f) functional connectivity were plotted against Euclidean distance. Each panel shows a negative exponential relationship between regional annotation similarity and distance, indicating that regions that are further apart show less similar properties. Note that gene coexpression was computed only for the left hemisphere.\nFigure S9. Robustness of disorder similarity matrix | (a) Disorder similarity was correlated to a version of the disorder similarity matrix, constructed by excluding a single disorder, across all thirteen disorders. The minimum correlation, computed when 22q-deletion syndrome is excluded, is \\( r = 0.95 \\). (b) The influence that each disorder has on the disorder similarity matrix is calculated as the difference between 1 and the correlation coefficient calculated in (a)."} {"paper_id": "prb5", "title": "SE(3)-Equivariant Graph Neural Networks for Data-Efficient and Accurate Interatomic Potentials", "text": "SE(3)-Equivariant Graph Neural Networks for Data-Efficient and Accurate Interatomic Potentials\n\nSimon Batzner\nHarvard University\nTess Smidt\nLawrence Berkeley National Laboratory https://orcid.org/0000-0001-5581-5344\nLixin Sun\nMassachusetts Institute of Technology\nJonathan Mailoa\nBosch Research and Technology Center\nMordechai Kombluth\nRobert Bosch Research and Technology Center https://orcid.org/0000-0001-6705-8133\nNicola Molinari\nHarvard University\nBoris Kozinsky ( bkoz@seas.harvard.edu )\nHarvard University https://orcid.org/0000-0002-0638-539X\n\nArticle\n\nKeywords: Molecular Dynamics Simulations, Symmetry-aware Models, Equivariant Convolutions, Geometric Tensors\n\nPosted Date: March 1st, 2021\n\nDOI: https://doi.org/10.21203/rs.3.rs-244137/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nVersion of Record: A version of this preprint was published at Nature Communications on May 4th, 2022. See the published version at https://doi.org/10.1038/s41467-022-29939-5.\nSE(3)-Equivariant Graph Neural Networks for Data-Efficient and Accurate Interatomic Potentials\n\nSimon Batzner,1 Tess E. Smidt,2 Lixin Sun,1 Jonathan P. Mailoa,3 Mordechai Korubluth,3 Nicola Molinari,1 and Boris Kozinsky1,3\n\n1John A. Paulson School of Engineering and Applied Sciences, Harvard University, Cambridge, MA 02138, USA\n2Computational Research Division and Center for Advanced Mathematics for Energy Research Applications, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA\n3Robert Bosch Research and Technology Center, Cambridge, MA 02139, USA\n\nThis work presents Neural Equivariant Interatomic Potentials (NequIP), a SE(3)-equivariant neural network approach for learning interatomic potentials from ab-initio calculations for molecular dynamics simulations. While most contemporary symmetry-aware models use invariant convolutions and only act on scalars, NequIP employs SE(3)-equivariant convolutions for interactions of geometric tensors, resulting in a more information-rich and faithful representation of atomic environments. The method achieves state-of-the-art accuracy on a challenging set of diverse molecules and materials while exhibiting remarkable data efficiency. NequIP outperforms existing models with up to three orders of magnitude fewer training data, challenging the widely held belief that deep neural networks require massive training sets. The high data efficiency of the method allows for the construction of accurate potentials using high-order quantum chemical level of theory as reference and enables high-fidelity molecular dynamics simulations over long time scales.\n\nINTRODUCTION\n\nMolecular dynamics (MD) simulations are an indispensable tool for computational discovery in fields as diverse as energy storage, catalysis, and biological processes [1-3]. While the atomic forces required to integrate Newton’s equations of motion can in principle be obtained with high fidelity from quantum-mechanical calculations such as density functional theory (DFT), in practice the unfavorable computational scaling of first-principles methods limits simulations to short time scales and small numbers of atoms. This prohibits the study of many interesting physical phenomena beyond the time and length scales that are currently accessible, even on the largest supercomputers. Owing to their simple functional form, classical models for the atomic potential energy can typically be evaluated orders of magnitude faster than using first-principles methods, thereby enabling the study of large numbers of atoms over long time scales. However, due to their limited mathematical form, classical interatomic potentials, or force fields, are inherently limited in their predictive accuracy which has historically led to a fundamental trade-off between obtaining high computational efficiency while also predicting faithful dynamics of the system under study. The construction of flexible models of the interatomic potential energy based on Machine Learning (ML-IP), and in particular\nNeural Networks (NN-IP), has shown great promise in providing a way to move past this dilemma, promising to learn high-fidelity potentials from ab-initio reference calculations while retaining favorable computational efficiency [1][13]. One of the limiting factors of NN-IPs is that they typically require collection of large training sets of ab-initio calculations, often including thousands or even millions of reference structures [4][9][10][14][16]. This computationally expensive process of training data collection has severely limited the adoption of NN-IPs as it quickly becomes a bottleneck in the development of force-fields for new systems. Kernel-based approaches, such as e.g. Gaussian Processes (GP) [5][8] or Kernel Ridge Regression (KRR) [17], are a way to remedy this problem as they often generalize better from limited sample sizes. However, such methods generally tend to exhibit poor computational scaling with the number of reference configurations, in both training (cubic in training set size) and prediction (linear in training set size). This limits both the amount of training data they can be trained on as well as the length and size of simulations that can be simulated with them.\n\nIn this work, we present the Neural Equivariant Interatomic Potential (NequIP), a highly data-efficient deep learning approach for learning interatomic potentials from reference first-principles calculations. We show that the proposed method obtains high accuracy compared to existing ML-IP methods across a wide variety of systems, including small molecules, water in different phases, an amorphous solid, a reaction at a solid/gas interface, and a Lithium superionic conductor. Furthermore, we find that NequIP exhibits exceptional data efficiency, enabling the construction of accurate interatomic potentials from limited data sets of fewer than 1,000 or even as little as 100 reference ab-initio calculations, where other methods require orders of magnitude more. It is worth noting that on small molecular data sets, NequIP outperforms not only other neural networks, but is also competitive with kernel-based approaches, which typically obtain better predictive accuracy than NN-IPs on small data sets (although at significant additional cost scaling in training and prediction). We further demonstrate high data efficiency and accuracy with state-of-the-art results on a training set of molecular data obtained at the quantum chemical coupled-cluster level of theory. Finally, we validate the method through a series of simulations and demonstrate that we can reproduce with high fidelity structural and kinetic properties computed from NequIP simulations in comparison to ab-initio molecular dynamics simulations (AIMD). We directly verify that the performance gains are connected with the unique SE(3)-equivariant convolution architecture of the new NequIP model.\n\nRelated Work\n\nFirst applications of machine learning for the development of interatomic potentials were built on descriptor-based approaches combined with shallow neural networks or Gaussian Processes [4][5], designed to exhibit invariance with respect to translation, permutation of atoms of the same chemical species, and rotation. Recently, rotationally invariant graph neural networks (GNN-IPs) have emerged as a powerful architecture for deep learning of interatomic potentials\nthat eliminates the need for hand-crafted descriptors\\textsuperscript{148} and allows to instead learn representations on graphs\\textsuperscript{149} of atoms from invariant features of geometric data (e.g.\\textsuperscript{150} radial distances or angles) \\textcolor{red}{[9]} \\textcolor{green}{[11]} \\textcolor{blue}{[13]}. In GNN-IPs,\\textsuperscript{151} atomic structures are represented by collections of nodes and edges, where nodes in the graph correspond\\textsuperscript{153} to individual atoms and edges are typically defined\\textsuperscript{154} by simply connecting every atom to all other atoms\\textsuperscript{155} that are closer than some cutoff distance \\( r_c \\). Every node/atom \\( i \\) is associated with a feature \\( \\mathbf{h}_i \\in \\mathbb{R}^h \\),\\textsuperscript{157} consisting of scalar values, which is iteratively refined\\textsuperscript{158} via a series of convolutions over neighboring atoms \\( j \\)\\textsuperscript{159} based on both the distance to neighboring atoms \\( r_{ij} \\)\\textsuperscript{160} and their features \\( \\mathbf{h}_j \\). This iterative process allows\\textsuperscript{161} information to be propagated along the atomic graph\\textsuperscript{162} through a series of convolutional layers and can be\\textsuperscript{163} viewed as a message-passing scheme \\textcolor{orange}{[18]}. Operating\\textsuperscript{164} only on interatomic distances allows GNN-IPs to be\\textsuperscript{165} rotation- and translation-invariant, making both the\\textsuperscript{166} output as well as features internal to the network\\textsuperscript{167} invariant to rotations. In contrast, the method outlined\\textsuperscript{168} in this work uses relative position *vectors* rather than\\textsuperscript{169} simply distances (scalars), which makes internal features instead *equivariant* to rotation and allows for angular information to be used by rotationally equivariant filters. Similar to other methods, we can restrict convolutions to only a local subset of all other atoms that lie closer to the central atom than a chosen cutoff distance \\( r_c \\), see\\textsuperscript{170} Figure 1 left.\n\nA series of related methods have recently been\\textsuperscript{173} proposed: DimeNet \\textcolor{green}{[11]} expands on using pairwise\\textsuperscript{174} interactions in a single convolution to include angular,\\textsuperscript{175} three-body terms, but individual features are still\\textsuperscript{176} comprised of scalars (distances and three-body angles are invariant to rotation), as opposed to vectors used in this work. Another central difference to NequIP is that DimeNet explicitly enumerates angles between pairs of atoms and operates on a basis embedding of distances and angles, whereas NequIP operates on relative position *vectors* and a basis embedding of distances, and thus never explicitly computes three-body angles. Cormorant \\textcolor{green}{[19]} uses an equivariant neural network for property prediction on small molecules. This method is demonstrated on potential energies of small molecules but not on atomic forces or systems with periodic boundary conditions. Townshend et al. \\textcolor{green}{[20]} use the framework of Tensor-Field Networks \\textcolor{green}{[21]} to directly predict atomic force vectors. The predicted forces are not guaranteed by construction to conserve energy since they are not obtained as gradients of the total potential energy. This may lead to problems in simulations of molecular dynamics over long times. None of these three works \\textcolor{red}{[9]} \\textcolor{green}{[19]} \\textcolor{green}{[20]} demonstrates capability to perform molecular dynamics simulations.\n\nIn this work we present a deep learning energy-conserving interatomic potential for both molecules and materials built on SE(3)-equivariant convolutions over geometric tensors that yields state-of-the-art accuracy, outstanding data-efficiency, and can with high fidelity reproduce structural and kinetic properties from molecular dynamics simulations.\nFIG. 1: Left: a set of atoms is interpreted as an atomic graph with local neighborhoods. Middle: every atom carries a set of scalar and vector features with it. Right: atoms exchange information via filters, that are again scalars and vectors. The interactions of features and filters define five interactions.\n\nRESULTS\n\nEquivariance\n\nThe concept of equivariance arises naturally in machine learning of atomistic systems (see e.g. [22]): physical properties have well-defined transformation properties under translation and rotation of a set of atoms. As a simple example, if a molecule is rotated in space, the vectors of its atomic dipoles or forces also rotate accordingly, via equivariant transformation. Equivariant neural networks are able to more generally represent tensor properties and tensor operations of physical systems (e.g. vector addition, dot products, and cross products). Equivariant neural networks are guaranteed to preserve the known transformation properties of physical systems under a change of coordinates because they are explicitly constructed from equivariant operations. Formally, a function \\( f : X \\to Y \\) is equivariant with respect to a group \\( G \\) that acts on \\( X \\) and \\( Y \\) if:\n\n\\[\nD_Y[g]f(x) = f(D_X[g]x) \\quad \\forall g \\in G, \\forall x \\in X\n\\]\n\nwhere \\( D_X[g] \\) and \\( D_Y[g] \\) are the representations of the group element \\( g \\) in the vector spaces \\( X \\) and \\( Y \\), respectively. In this work, we focus on equivariance with respect to SE(3), i.e. the group of rotations and translations in 3D space.\n\nNeural Equivariant Interatomic Potentials\n\nGiven a set of atoms (a molecule or a material), we aim to find a mapping from atomic positions \\( \\vec{r}_i \\) and chemical species (identified by atomic numbers \\( Z_i \\)) to the total potential energy and the forces acting on the atoms:\n\n\\[\nf : \\{\\vec{r}_i, Z_i\\} \\to E_{pot}\n\\]\n\nForces are obtained as gradients of the predicted potential energy with respect to the atomic positions, which guarantees energy conservation:\n\n\\[\n\\vec{F}_i = -\\nabla_i E_{pot}\n\\]\n\nGradients can be obtained with relatively low computational overhead in modern auto-differentiation frameworks such as TensorFlow or PyTorch [23] [24]. Following previous work [4], we further define the total\npotential energy of the system as a sum of atomic potential energies:\n\n\\[\nE_{pot} = \\sum_{i \\in N_{atoms}} E_{i,atomic}\n\\] (4)\n\nThese atomic local energies \\( E_{i,atomic} \\) are the scalar node attributes predicted by the graph neural network. Even though the output of NequIP is the predicted potential energy \\( E_{pot} \\), which is invariant under translations and rotations, the network contains *internal features* that are tensors which are equivariant to rotation. This constitutes the core difference between NequIP and existing scalar-valued invariant GNN-IPs. The remainder of this section will discuss the design of the network in further detail.\n\nA series of methods has been introduced to realize rotationally equivariant neural networks [13, 21, 25, 26]. Here, we build on the layers introduced in Tensor-Field Networks (TFN) [21], which enable the construction of neural networks that exhibit equivariance to translation, permutation, and rotation. Every atom in NequIP is associated with a feature comprised of tensors of different order: scalars, vectors, and higher-order tensors. Formally, these features are geometric objects that comprise a direct sum of irreducible representations of the SO(3) symmetry group. Second, the convolutions that operate on these geometric objects are equivariant functions instead of invariant ones, i.e. if a feature at layer \\( k \\) is rotated, then the output of the convolution from layer \\( k \\to k+1 \\) rotates accordingly. In practice, the features are implemented as a dictionary \\( V^{(l)}_{acm} \\) with keys \\( l \\), where \\( l = 0, 1, 2, ... \\) is a non-negative integer and is called the “rotation order”, labeling the irreducible representations. The indices \\( a, c, m \\), correspond to the atoms, the channels (elements of the feature), and the representation index which takes values \\( m \\in [-l, l] \\), respectively.\n\nConvolution operations are naturally translation invariant, since their filters act on relative interatomic distance vectors. Moreover, they are permutation invariant since all convolution contributions are summed. Note that while atomic features are equivariant to permutation of atom indices, globally, the total potential energy of the system is invariant to permutation. To achieve rotation equivariance, the convolution filters are constrained to be products of learnable radial functions and spherical harmonics, which are equivariant under SO(3) [21]:\n\n\\[\nF(\\vec{r}_{ij}) = R(r_{ij}) Y_m^{(l)}(\\hat{r}_{ij})\n\\] (5)\n\nwhere if \\( \\vec{r}_{ij} \\) denotes the relative position from central atom \\( i \\) to neighboring atom \\( j \\), \\( \\hat{r}_{ij} \\) and \\( r_{ij} \\) are the associated unit vector and interatomic distance, respectively. It should be noted that all learnable weights in the filter lie in the rotationally invariant radial function \\( R(r_{ij}) \\). This radial function is implemented as a small neural network with one hidden layer and a shifted softplus activation function [9], operating on interatomic distances expressed in a basis of choice, \\( R(r_{ij}) : \\mathbb{R}^{N_b} \\to \\mathbb{R}^h \\), where \\( N_b \\) is the number of basis functions and \\( h \\) is the feature dimension:\n\n\\[\nR(r_{ij}) = W_2 \\ln(0.5 \\exp(W_1 B(r_{ij})) + 0.5)\n\\] (6)\nwhere \\( W_1 \\in \\mathbb{R}^{N_{hidden} \\times N_b} \\) and \\( W_2 \\in \\mathbb{R}^{h \\times N_{hidden}} \\) are weight matrices, \\( h \\) is the dimension of the feature and \\( N_{hidden} \\) is the dimension of the hidden layer in the feed-forward neural network (in our experiments, we use \\( N_{hidden} = N_b \\), resulting in comparatively small neural networks for the radial function). Radial Bessel functions and a polynomial envelope function \\( f_{env} \\) discussed in recent work [11] are used to expand the interatomic distances:\n\n\\[\nB(r_{ij}) = \\sqrt{\\frac{2}{r_c}} \\frac{\\sin(n \\pi r_{ij}/r_c)}{r_{ij}} f_{env}(r_{ij}, r_c)\n\\]\n\nwhere \\( r_c \\) is a local cutoff radius, restricting interactions to atoms closer than some cutoff distance and \\( f_{env} \\) is the polynomial defined in [11] with \\( p = 6 \\) operating on the interatomic distances normalized by the cutoff radius \\( \\frac{r_{ij}}{r_c} \\). The use of cutoffs/local atomic environments allows the computational cost of evaluation to scale linearly with the number of atoms. Similar to [11], we initialize the Bessel functions with \\( n = [1, 2, ..., N_b] \\) and subsequently optimize \\( n \\pi \\) via backpropagation rather than keeping it constant. For systems with periodic boundary conditions, we use the neighbor_list functionality as implemented in the ASE code [27] to identify appropriate atomic neighbors and then convolve over them.\n\nFinally, in the convolution, the input feature tensor and the filter have to again be combined in an equivariant manner, which is achieved via a geometric tensor product, yielding an output feature that again is rotationally equivariant. A tensor product of two geometric tensors is computed via Clebsch-Gordan coefficients, as outlined in [21]. Since NequIP deals with force vectors, the network design is simplified by only using scalar (\\( l=0 \\)) and vector (\\( l=1 \\)) representations. Thus, we can enumerate five distinct products or “interactions” between \\( l = 0 \\) and \\( l = 1 \\) filters and \\( l = 0 \\) and \\( l = 1 \\) features that correspond to simple operations between scalars and vectors:\n\n• \\( 0 \\otimes 0 \\to 0 \\) (product of two scalars)\n• \\( 0 \\otimes 1 \\to 1 \\) (scalar multiplication of a vector)\n• \\( 1 \\otimes 0 \\to 1 \\) (scalar multiplication of a vector)\n• \\( 1 \\otimes 1 \\to 0 \\) (dot product of two vectors)\n• \\( 1 \\otimes 1 \\to 1 \\) (cross product of two vectors)\n\nIt is trivial to include higher-order interactions, and previous works have increased the rotation order beyond \\( l = 1 \\) [20, 28]. However, it should be noted that every interaction comes with additional trainable radial functions and hence additional weights, which thus adds to the model capacity, increasing the number of model weights and the memory footprint of the model. Omitting all higher-order interactions that go beyond the \\( 0 \\otimes 0 \\to 0 \\) interaction will result in a conventional GNN-IP with invariant convolutions over scalar features, similar to e.g. SchNet [9]. Finally, as outlined in [21], a full convolutional layer \\( \\mathcal{L} \\) implementing an interaction with filter \\( f \\) acting on an input \\( i \\) producing output \\( o \\): \\( l_f \\otimes l_i \\to l_o \\) is given by:\n\\[\n\\mathcal{L}_{acm_o}^{(l_o)}(\\vec{r}_a, V_{acm_i}^{(l_i)}) = \\sum_{m_f, m_i} C_{(l_f, m_f)(l_i, m_i)}^{(l_o, m_o)} \\sum_{b \\in S} R_c^{(l_f, l_i)}(r_{ab}) Y_{m_f}^{(l_f)}(\\hat{r}_{ab}) V_{bcm_i}^{(l_i)}\n\\]\n\nwhere \\(a\\) and \\(b\\) index the central atom of the convolution and the neighboring atom \\(b \\in S\\), respectively, and \\(C\\) indicates the Clebsch-Gordan coefficients. As an example of this, we write out a full \\(1 \\otimes 1 \\rightarrow 1\\) operation (corresponding to a cross-product) in the Methods section. After every convolution, output tensors of a rotation order \\(l\\) stemming from different tensor products are concatenated on a per-atom basis. To update atomic features, the model also leverages self-interaction layers similar to SchNet [9], corresponding to dense layers that are applied in an atom-wise fashion with weights shared across atoms. While different weights are used for different rotation orders, the same set of weights is applied for all representation indices \\(m\\) of a given rotation order \\(l\\). Shifted softplus nonlinearities [9] are used as rotation-equivariant nonlinearities as introduced in [21], which are applied to the Euclidean norm of the input feature, the output of which is in turn combined with the input tensor, thus preserving overall equivariance.\n\nThe NequIP network architecture, shown in Figure 2, is built on an atomic embedding, followed by a series of interaction blocks, and finally an output block:\n\n• Embedding: following SchNet, the initial feature is generated using a trainable embedding, that operates on the atomic number \\(Z_i\\) (represented via a one-hot encoding) alone, implemented via a trainable self-interaction layer.\n\n• Interaction Block: interaction blocks encode interactions between neighboring atoms: the core of this block is the convolution function, outlined in equation 8. For every output rotation order \\(l_o\\), the features from different tensor product interactions are concatenated to give a new feature, which is in return refined with atom-wise self-interaction layers and equivariant non-linearities. We equip interactions blocks with a ResNet-style update [29] where the input feature \\(\\mathbf{x}\\) is updated atom-wise via the output of an interaction block \\(f(\\mathbf{x})\\) that gives the final feature \\(r(\\mathbf{x}) = f(\\mathbf{x}) + \\mathbf{x}\\) (features are added element-wise in the \\(m\\)-dimension). Note that this operation is equivariant since the addition of an equivariant feature \\(\\mathbf{x}\\) and an equivariant function \\(f(\\mathbf{x})\\) preserves equivariance. While later interaction blocks include all five interactions outlined above, the first interaction block operates on the \\(l = 0\\) embedding with a \\(0 \\otimes 0 \\rightarrow 0\\) and a \\(0 \\otimes 1 \\rightarrow 1\\) only.\n\n• Output Block: the \\(l = 0\\) feature of the final convolution is passed to an output block, which consists of another atom-wise self-interaction layer, an equivariant non-linearity, and a final atom-wise self-interaction layer.\n\nThe scalar atomic outputs of the final layer can be interpreted as atomic potential energies which are summed to give the total predicted potential energy of the system (Equation 1). Forces are subsequently obtained as the negative gradient of the predicted total potential energy, thereby ensuring both energy\nFIG. 2: The NequIP network architecture. Left: atomic numbers are embedded into \\( l = 0 \\) features, which are refined through a series of interaction blocks, creating \\( l = 0 \\) and \\( l = 1 \\) features. An output block generates atomic energies, which are pooled to give the total predicted energy. Middle: the interaction block consists of a series of convolutions, interwoven with self-interaction layers, equivariant nonlinearities and concatenation. Right: the convolution combines the radial function \\( R(r) \\) which operates only on interatomic distances with the spherical harmonics based on unit vector \\( \\hat{r} \\) via a tensor product.\n\nconservation as well as rotation-equivariant forces (see equation 3).\n\nExperiments\n\nWe validate the proposed method on a series of diverse and challenging data sets: first we demonstrate that we improve upon state-of-the-art accuracy on MD-17, a data set of small, organic molecules that is widely used for benchmarking ML-IPs [9, 11, 17, 30, 31]. Next, we show that NequIP can also accurately learn forces obtained on small molecules at the quantum chemical CCSD(T) level [31], opening the door to scalable and efficient molecular dynamics simulations with beyond-DFT accuracy. To broaden the applicability of the method beyond small isolated molecules, we explore a series of extended systems with periodic boundary conditions, consisting of both surfaces and bulk materials: water in different phases [15, 32], a chemical reaction at a solid/gas interface, an amorphous Lithium Phosphate [12], and a Li superionic conductor [13]. Details of the training procedure are provided in the Methods section.\n\nMD-17 small molecule dynamics\n\nWe first evaluate NequIP on MD-17 [17, 30, 31], a data set of eight small organic molecules in which reference values of energy and forces are generated by ab-initio MD simulations with DFT. For training we use N=1,000 structure configurations for each molecule, sampled uniformly from the full data set, the same number of configurations for validation, and evaluate\nthe test error on all remaining configurations in the data set. The mean absolute error in the force components is shown in Table I in units of [meV/\\AA]. We compare results using NequIP with those from published leading ML-IP models that were also trained on 1,000 structures: in particular SchNet [9], DimeNet [11] (both graph neural networks), sGDML [31], and FCHL19/GPR (kernel-based methods) [33]. We find that NequIP outperforms SchNet and sGDML on all molecules in the data set, DimeNet on 7 out of 8 molecules (on par on the remaining one), and performs on par with FCHL/19GPR. The consistent improvement in accuracy upon sGDML and the comparable performance to FCHL19/GPR are particularly surprising, as these are based on kernel methods, that typically tend to be more sample efficient. It should be noted, however, that the evaluation cost of kernel methods scales linearly with the number of training configurations. Note also that on some molecules, NequIP trained on 1,000 configurations even performs as well as SchNet trained on 50,000 structures [9]: on aspirin and naphthalene, for example, the NequIP network trained on 1,000 structures produces mean absolute errors in the forces of 15.1 meV/\\AA\\ and 4.2 meV/\\AA, respectively, compared to 14.3 meV/\\AA\\ and 4.8 meV/\\AA\\ of SchNet trained on 50x more molecules, hinting that NequIP exhibits exceptional data efficiency. On other molecules such as ethanol, however, SchNet trained with 50,000 molecules still clearly outperforms NequIP trained with 1,000 molecules (2.2 meV/\\AA\\ for SchNet for N=50,000 vs 9.0 meV/\\AA\\ for NequIP for N=1,000).\n\nForce training at quantum chemical accuracy\n\nAbility to achieve high accuracy on a comparatively small data set opens the door to training models on expensive high-order *ab-initio* quantum chemical methods. It has been shown that DFT can fail to capture important subtleties in the potential energy surface, potentially even identifying the wrong ground states [31]. This problem can be remedied through the use of more accurate reference calculations, such as coupled cluster methods CCSD(T), typically regarded as the gold standard of quantum chemistry. However, the high computational cost of CCSD(T) has thus far hindered the use of reference data structures at this level of theory, prohibited by the need for large data sets that are required by available NN-IPs. Leveraging the high data efficiency of NequIP, we evaluate it on a set of molecules computed at quantum chemical accuracy (aspirin at CCSD, all others at CCSD(T)) [31] and compare the results to those reported for sGDML [31]. The training/validation set consists of a total of 1,000 molecular structures which we split into 950 for training and 50 for validation (sampled uniformly), and we test the accuracy on all remaining structures (we use the train/test split provided with the data set, but further split the training set into training and validation sets). We find that NequIP achieves lower errors on four out of five molecules, performing on par with sGDML on the fifth molecule, as shown in Table II.\n\nLiquid Water and Ice Dynamics\n\nTo demonstrate the applicability of NequIP beyond small molecules, we evaluate the method on a series of\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
MoleculeNequIPSchNetsGDMLDimeNetFCHL19/GPR
Aspirin15.158.529.521.620.7
Benzene [17]8.113.4n/a8.1n/a
Benzene [31]2.3n/a2.6n/an/a
Ethanol9.016.914.310.05.9
Malonaldehyde14.628.617.816.610.6
Naphthalene4.225.24.89.36.5
Salicylic Acid10.336.912.116.29.6
Toluene4.424.76.19.48.8
Uracil7.524.310.413.14.6
\n\nTABLE I: MAE of force components on the MD-17 data set, trained on 1,000 configurations, forces in units of [meV/\\AA]. For the benzene molecule, two different data set exists from [17, 31] with different levels of accuracy in the DFT reference data.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
MoleculeNequIPsGDML
Aspirin14.733.0
Benzene0.81.7
Ethanol9.415.2
Malonaldehyde16.016.0
Toluene4.49.1
\n\nTABLE II: Force MAE for molecules at CCSD/CCSD(T) accuracy, reported in units of [meV/\\AA], with 1,000 reference configurations).\n\nextended systems with periodic boundary conditions. As a first example we use a joint data set consisting of liquid water and three ice structures [15][32], computed at the PBE0-TS level of theory. This data set contains [15]:\na) liquid water, P=1bar, T=300K, computed via path-integral AIMD, b) ice Ih, P=1bar, T=273K, computed via path-integral AIMD c) ice Ih, P=1bar, T=330K, computed via classical AIMD d) ice Ih, P=2.13 kbar, T=238K, computed via classical AIMD. The liquid water system consists of 64 H$_2$O molecules (192 atoms), while the ice structures consist of 96 H$_2$O molecules (288 atoms). A DeepMD NN-IP model was previously trained [15] for water and ice using a joint training set containing 133,500 reference calculations of these four systems. To assess data efficiency of the NequIP architecture, we similarly train a model jointly on all four parts of the data set, but using only 133 structures for training, i.e. 1000x fewer data. The 133 structures were sampled uniformly from the full data set available online, consisting of water and ice structures, made up of a total of 140,000 frames, coming from the same MD trajectories that were used in the earlier work [15]. We also use a validation set of 50 frames and report the test accuracy on all remaining structures in the data set. Table III shows the comparison of the predictive force accuracy of NequIP trained on the 133 structures vs DeepMD trained on 133,500 structures. We find that with 1000x fewer training data, NequIP significantly outperforms DeepMD on all four parts of the data set.\n\nHeterogeneous catalysis of formate dehydrogenation\n\nNext, we demonstrate application of NequIP to a catalytic surface reaction. In particular, we investigate the dynamics of formate undergoing dehydrogenation decomposition (HCOO$^* \\rightarrow$ H$^*$ + CO$_2$) on a Cu $<110>$ surface (see Figure 3). This system is highly heterogeneous, with both metallic and covalent types of bonding as well as charge transfer occurring between the metal and the molecule, making this a particularly challenging test system. Different states of the molecule\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
SystemNequIP, 133 data pointsDeepMD, 133,500 data points
Liquid Water35.940.4
Ice Ih (b)25.943.3
Ice Ih (c)16.626.8
Ice Ih (d)13.525.4
\n\nTABLE III: Root mean square error (RMSE) of force components on liquid water and the three ices in units of [meV/\\AA]. Note that the NequIP model was trained on \\(< 0.1\\%\\) of the training data of DeepMD.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
ElementMAE
C55.8
O86.7
H42.0
Cu54.5
Total structure55.6
\n\nTABLE IV: MAE of force components for Formate on Cu system, per-element basis. The training set consists of 2,500 structures, force units are [meV/\\AA]\n\nalso lead to dissimilar C-O bond lengths [34, 35].\nTraining structures consist of 48 Cu atoms and 4 atoms of the molecule (HCOO* or CO$_2$+H*). The MAE of the predicted forces using a NequIP model trained on 2,500 structures is shown in Table IV demonstrating that NequIP is able to accurately model the interatomic forces for this complex reactive system. A more detailed analysis of the resulting dynamics will be subject of a separate study.\n\nFIG. 3: Perspective view of atomic configurations of (a) bidentate HCOO (b) monodentate HCOO and (c) CO$_2$ and a hydrogen adatom on a Cu(110) surface. The blue, red, black, and white spheres represent Cu, O, C, and H atoms, respectively. The subset shown in each subplot is the corresponding top view along the \\(<110>\\) orientation.\n\n![Perspective view of atomic configurations of (a) bidentate HCOO (b) monodentate HCOO and (c) CO$_2$ and a hydrogen adatom on a Cu(110) surface.](page_104_1042_627_180.png)\n\nLithium Phosphate Amorphous Glass Formation\n\nFIG. 4: Quenched glass structure of Li$_4$P$_2$O$_7$. The insets show the P-O-O tetrahedral bond angle (bottom left) as well as the O-P-P bridging angle between corner-sharing phosphate tetrahedra (top right).\n\n![Quenched glass structure of Li$_4$P$_2$O$_7$. The insets show the P-O-O tetrahedral bond angle (bottom left) as well as the O-P-P bridging angle between corner-sharing phosphate tetrahedra (top right).](page_1042_370_370_370.png)\n\nTo examine the ability of the model to capture dynamical properties, we demonstrate that NequIP can describe structural dynamics in amorphous lithium phosphate with composition Li$_4$P$_2$O$_7$. This material is a member of the promising family of solid electrolytes for Li-metal batteries [12, 36, 37], with non-trivial Li-ion transport and phase transformation behaviors. The training data set consists of two 50ps-long AIMD simulations, one of the molten structure at T=3000 K, followed by another of a quenched glass structure at T=600 K. We train NequIP on a subset of 1,000 structures of the molten trajectory, each consisting of\n208 atoms, and sampled uniformly from the full data set of 25,000 AIMD frames. We use a validation set of 100 structures, and evaluate the model on all remaining structures. Table V shows the test set error in the force components on both the test set from the AIMD molten trajectory and the full AIMD quenched glass trajectory.\n\nTo then evaluate the physical fidelity of the trained model, we use it to run a MD simulation of length 50 ps at T=600 K in the NVT ensemble and compare the total radial distribution function (RDF) without element distinction as well as the angular distribution functions (ADF) of the P-O-O (P central atom) and O-P-P (O central atom) angles to the ab-initio trajectory at the same temperature. The P-O-O angle corresponds to the tetrahedral bond angle, while the O-P-P corresponds to a bridging angle between corner-sharing phosphate tetrahedra (Figure 4). Figure 5 shows that NequIP can accurately reproduce the RDF and the two ADFs, in comparison with AIMD, after training on only 1,000 structures. This demonstrates that the model generates the glass state and recovers its dynamics and structure almost perfectly, having seen only the high-temperature molten training data.\n\ndata set of 30,874 structures to study Li diffusion in Li3PO4). Here we demonstrate that not only does NequIP obtain small errors in the force components, but it also accurately predicts the diffusivity after training on a data set obtained from an AIMD simulation. Again, we find that very small training sets lead to highly accurate models, as shown in Table V for training set sizes of 10, 100, 1,000 and 2,500 structures. We run a series of MD simulations with the NequIP potential trained on 2,500 structures in the NVT ensemble at the same temperature as the AIMD simulation for a total simulation time of 50 ps and a time step of 0.25 fs, which we found advantageous for reliability and stability of long simulations. We measure the Li diffusivity in ten Nequip-driven MD simulations (computed via the slope of the mean square displacement), all of length 50 ps and started from different initial velocities, randomly sampled from a Maxwell-Boltzmann distribution. We find a mean diffusivity of \\(1.42 \\times 10^{-5}\\) cm\\(^2\\)/s, in excellent agreement with the diffusivity of \\(1.38 \\times 10^{-5}\\) cm\\(^2\\)/s computed from AIMD, thus achieving a relative error of as little as 3%. Figure 6 shows the mean square displacements of Li for an example run.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
SystemData Set SizeMAE
LiPS10157.1
LiPS10050.0
LiPS1,00025.1
LiPS2,50024.1
Li4P2O7, melt1,00063.2
Li4P2O7, quench1,00036.9
\n\nTABLE V: Force MAE for LiPS and Li4P2O7 for different data set sizes in units of [meV/A]. The model for Li4P2O7 was trained exclusively on structures from the melted trajectory; the reported test errors show the MAE on both the test set of the melted trajectory as well as the full quench trajectory.\n\nLithium Thiophosphate Superionic Transport\n\nTo show that NequIP can model kinetic transport properties from small training sets at high accuracy, we study Li-ion diffusivity in LiPS (Li6.75P3S11) a crystalline superionic Li conductor, consisting of a simulation cell of 83 atoms [13]. MD is widely used to study diffusion; however, training a ML-IP to the accuracy required to accurately predict kinetic properties has in the past required large training set sizes ([38] e.g. uses a\nFIG. 5: Left: Radial Distribution Function, middle: Angular Distribution Function, bridging oxygen, right: Angular Distribution Function, tetrahedral bond angle. All are defined as probability density functions.\n\nFIG. 6: Comparison of Lithium mean square displacement of AIMD and NequIP trajectories.\n\nData Efficiency\n\nIn the above experiments, NequIP exhibits exceptionally high data efficiency, i.e. it can be trained successfully to state-of-the-art accuracy from unexpectedly small training sets. It is interesting to consider the reasons for such high performance and verify that it is connected to the equivariant nature of the model. First, it is important to note that each training configuration contains multiple labels, thus increasing the total number of labels available beyond just the potential energy label associated with each structure. In particular, for a training set of \\( M \\) first-principles calculations with structures consisting of \\( N \\) atoms, the total number of labels available is \\( M(3N+1) \\) since every force component on every atom constitutes a label and so does the total energy of the reference calculation (we only train to atomic forces and not energies, thus using \\( 3MN \\) force components as labels).\n\nIn order to gain insight into the reasons behind increased accuracy and data efficiency, we perform a series of experiments with the goal of isolating the effect of using equivariant convolutions of geometric tensors compared to invariant convolutions over scalars. In particular, we run a set of experiments for a system with a fixed number of training configurations in which we explicitly turn on or off interactions of higher order than \\( l = 0 \\). This defines two settings: first, we train the network with both \\( l = 0 \\) and \\( l = 1 \\) features and all five interactions as previously outlined in this work. Second, when all interactions involving \\( l = 1 \\) are turned off, this turns the network into a conventional invariant GNN-IP, involving only invariant convolutions over scalar features in a SchNet-style fashion. As a test system we chose bulk water: in particular we use the data set introduced in [29], consisting of 1,593 bulk liquid water structures with 64 water molecules each. We train a series of networks with identical hyperparameters, but vary the training set sizes between 10 and 1,000 structures, sampled uniformly from the full data set, as well as a validation set consisting of 100 structures. We then evaluate the error on all\nremaining structures for a given training set size. As shown in Figure 7 we find that the equivariant setting (using \\( l = 0 \\) and \\( l = 1 \\)) significantly outperforms the invariant setting (using only \\( l = 0 \\)) for all data set sizes as measured by the MAE of force components. This suggests that it is indeed the use of tensor (in our specific case vector) features and equivariant convolutions that enables the high data efficiency of NequIP. We further note, that in [39], a Behler-Parrinello Neural Network (BPNN) was trained on 1303 structures, yielding a RMSE of \\( \\approx 120 \\) meV/\\(\\AA\\) in forces when evaluated on the remaining 290 structures. We find that NequIP models trained with as little as 50 and 100 data points obtain RMSEs of 122.9 meV/\\(\\AA\\) and 93.3 meV/\\(\\AA\\) on their respective test sets (note that Figure 7 shows the MAE). This provides further evidence that NequIP exhibits significantly improved data efficiency in comparison with existing methods.\n\n![Log-log plot of the predictive error in forces of NequIP with \\( l = 0 \\) vs. \\( l = 0/l = 1 \\) interactions as a function of data set size, measured via the force MAE.](page_682_1042_464_312.png)\n\nFIG. 7: Log-log plot of the predictive error in forces of NequIP with \\( l = 0 \\) vs. \\( l = 0/l = 1 \\) interactions as a function of data set size, measured via the force MAE.\n\nComputational Efficiency\n\nFinally, we report the computational efficiency of NequIP and compare it to that of the ab-initio methods on two examples shown in this work: for a molecular system, we choose the Toluene molecule, computed at the CCSD(T)-level of theory [31]; for a material with periodic boundary conditions, we choose the Formate on Cu system, in which reference data were obtained with DFT. For both systems, we report the time required for a single force call on a CPU node with 32 cores. The results are shown in Table VI. In both cases, NequIP gives a large speed-up over the ab-initio methods. In the case of the Toluene system, this means that 58.4 minutes of a NequIP simulation can obtain the simulation time equaling one century of a CCSD(T) simulation.\n\nDISCUSSION\n\nWe demonstrate that the Neural Equivariant Interatomic Potential (NequIP), a new type of graph neural network built on SE(3)-equivariant convolutions exhibits state-of-the-art accuracy and exceptional data efficiency on data sets of small molecules and periodic materials. Furthermore, we find that we can reproduce structural and kinetic properties from molecular dynamics simulations with very high fidelity in comparison to ab-initio simulations. The ability to both learn from small numbers of reference samples, while retaining high computational efficiency opens the door to performing simulations of large systems over long time-scales at quantum mechanical accuracy, using DFT or higher order methods such as coupled-cluster or quantum Monte Carlo data as reference. We expect the new method will enable researchers in computational chemistry, physics, biology, and materials science to conduct molecular dynamics simulations of complex reactions and phase transformations at increased accuracy and efficiency.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
SystemNumber of atomsNequIPAb-initioSpeed-up
Toluene1516 ms4 hours*900,000
Formate on Cu5258 ms1045.6 s18,028
\n\nTABLE VI: Time required for a single force call for NequIP in comparison to CCSD(T) for Toluene and DFT for Formate on Cu; * personal communication with Stefan Chmiela and Alexandre Tkatchenko.\n\nMETHODS\n\nReference Data Sets\n\nMD-17: MD-17 [17, 30, 31] is a data set of eight small organic molecules, obtained from MD simulations at T=500K and computed at the PBE+vdW-TS level of electronic structure theory, resulting in data set sizes between 133,770 and 993,237 structures. The data set was obtained from http://quantum-machine.org/gdml/#datasets\n\nMolecules@CCSD/CCSD(T): The data set of small molecules at CCSD and CCSD(T) accuracy [31] contains positions, energies, and forces for five different small molecules: Asprin (CCSD), Benzene, Malondaldehyde, Toluene, Ethanol (all CCSD(T)). Each data set consists of 1,500 structures with the exception of Ethanol, for which 2,000 structure are available. For more detailed information, we direct the reader to [31]. The data set was obtained from http://quantum-machine.org/gdml/#datasets\n\nLiquid Water and Ice: The data set of liquid waters and ice structures [15, 32] was generated from classical AIMD and path-integral AIMD simulations at different temperatures and pressures, computed with a PBE0-TS functional [15]. The data set, obtained from http://www.deepmd.org/database/deeppot-se-data/ contains a total of 140,000 structures, of which 100,000 are liquid water and 20,000 are Ice Ih b),10,000 are Ice Ih c), and another 10,000 are Ice Ih d).\n\nFormate decomposition on Cu: The decomposition process of formate on Cu involves configurations corresponding to the cleavage of the C-H bond, initial and intermediate states (monodentate, bidentate formate on Cu < 110 >) and final states (H ad-atom with a desorbed CO_2 in the gas phase). Nudged elastic band (NEB) method was first used to generate an initial reaction path of the C-H bond breaking. 12 short ab initio molecular dynamics, starting from different NEB images, were run to collect a total of 6855 DFT structures. The CP2K [40] code was employed for the AIMD simulations. Each trajectory was generated with a time step of 0.5 fs and 500 total steps. We train NequIP on 2,500 reference structures sampled uniformly from the full data set of 6,855 structures, use a validation set of 250 structures and evaluate the mean absolute error on all remaining structures. Due to the unbalanced nature of the data set (more atoms of Cu than in the molecule), we use a per-element weighed loss function in which atoms C, O_1, O_2, and H and the sum of all Cu atoms all receive equal weights.\n\nLi_4P_2O_7 glass: The Li_4P_2O_7 ab-initio data were generated using an ab-initio melt-quench MD simulation, starting with a stoichiometric crystal of 208 atoms (space\ngroup P21/c) in a periodic box of \\(10.4 \\times 14.0 \\times 16.0\\) Å. The dynamics used the Vienna Ab-Initio Simulation Package (VASP) [41][43], with a generalized gradient PBE functional [44], projector augmented wave (PAW) pseudopotentials [15], a NVT ensemble and a Nosé-Hoover thermostat, a time step of 2 fs, a plane-wave cutoff of 400 eV, and a Γ-point reciprocal-space mesh. The crystal was melted at 3000 K for 50 ps, then immediately quenched to 600 K and run for another 50 ps. The resulting structure was confirmed to be amorphous by plotting the radial distribution function of P-P distances. The training was performed only on the molten portion, and the MD simulations for a quenched simulation.\n\nLiPS: Lithium phosphorus sulfide (LiPS) based materials are known to exhibit high lithium ion conductivity, making them attractive as solid-state electrolytes for lithium-ion batteries. Other examples of known materials in this family of superionic conductors are LiGePS and LiCuPS-based compounds. The training data set is taken from a previous study on graph neural network force field [13], where the LiPS training data were generated using ab-initio MD of an LiPS structure with Li-vacancy (Li_{6.75}P_{3}S_{11}) consisting of 27 Li, 12 P, and 44 S atoms respectively. The structure was first equilibrated and then run at 520 K using the NVT ensemble for 50 ps with a 2.0 fs time step. The full data set contains 25,001 MD frames. We set aside 10,000 frames as a fixed test set. From the remaining frames, we choose training set sizes of 10, 100, 1,000, and 2,500 frames with a fixed validation set size of 100. In order to generate a diverse training set, we sample both the training and validation sets in a way such that 30% of both of them are comprised of the structures with the shortest interatomic distances out of all frames not in the test set and the remaining 70% of the training and validation set are uniformly sampled.\n\nLiquid Water, Cheng et al.: The training set used in the data efficiency experiments on water consists of 1,593 reference calculations of bulk liquid water at the revPBE0-D3 level of accuracy, with each structure containing 192 atoms, as given in [39]. Further information can be found in [39]. The data set was obtained from https://github.com/BingqingCheng/ab-initio-thermodynamics-of-water\n\nMolecular Dynamics Simulations. To run MD simulations, NequIP force outputs were integrated with the Atomic Simulation Environment (ASE) [27] in which we implement a custom version of the Nosé-Hoover thermostat. We use this in-house implementation for the both the Li_{4}P_{2}O_{7} as well as the LiPS MD simulations. The thermostat parameter was chosen to match the temperature fluctuations observed in the AIMD run. The RDF and ADFs for Li_{4}P_{2}O_{7} were computed with a maximum distance of 10 Å (RDF) and 2.5 Å (both ADFs).\n\nTraining. Networks are trained using a loss function based on atomic forces:\n\n\\[\n\\mathcal{L} = \\frac{1}{3N} \\sum_{i=1}^{N} \\sum_{\\alpha=1}^{3} \\| - \\frac{\\partial \\hat{E}}{\\partial r_{i,\\alpha}} - F_{i,\\alpha} \\|^{2}\n\\]\n\nwhere N is the number of atoms in the system and \\( \\hat{E} \\) is the predicted potential energy. Note that we do\nnot train on energies since atomic forces are the only quantities required to integrate Newton’s equations of motion. Since the predicted forces are computed as the gradient of a scalar potential, they are still conservative. If energies are of interest, however, one can add them to the loss function and determine the relative weighting via a trade-off parameter as done in previous works [9, 11]. In a similar fashion, it is trivial to add other quantities of interest to the loss function (e.g predicting atomic charges or multipole tensors can be of interest for modeling long-range interactions), where they may be scalar fields, vector fields, or higher-order tensor fields.\n\nHyperparameters. Training of models was performed on NVIDIA Tesla V100 GPUs. Throughout all experiments shown in this work, we use a feature dimension of \\( h = 64 \\), 6 interaction blocks, \\( N_b = 8 \\) Bessel basis functions and radial neural networks with one hidden layer, also of hidden dimension \\( N_{hidden} = 8 \\), giving light-weight radial functions with a comparatively small number of parameters. The final interaction block is followed by the output block, which first reduces the feature dimension to 16 through a self-interaction layer. An equivariant non-linearity is applied and finally through another self-interaction layer the feature dimension is reduced to a single scalar output value associated with each atom that is then summed over to give the total potential energy. Weights were initialized with the uniform Xavier initialization in the radial networks and orthogonal initialization in the self-interaction layers, biases were initialized with a constant value of 0. In all experiments, we use the Adam optimizer [16] with the TensorFlow 1.14 default settings of \\( \\beta_1 = 0.9, \\beta_2 = 0.999 \\), and \\( \\epsilon = 10^{-8} \\). We decrease the initial learning rate of 0.001 by a decay factor of 0.8 whenever the validation RMSE in the forces has not seen an improvement for a given number of epochs: for the small molecule tasks, we set this learning rate patience to 1,000, for all other tasks we use 100. We continuously save the model with the best validation RMSE and use the model with the overall best RMSE for evaluation on the test set and MD simulations. We stop the training if either a maximum number of 50,000 epochs (one epochs equals a full pass over the training set) has been reached, or the validation force RMSE has not improved for 2,500 epochs, or the maximum training time has been exceeded, whichever occurs first. All systems were trained for a maximum of 8 days (consisting of four runs of 48-hour time-limited compute jobs, which are restarted from the best saved model, i.e. potentially including repeats in the training) with the exception of the Li$_4$P$_2$O$_7$, which was trained for 12 days (six 48-hour compute jobs) and the LiPS systems, which were trained for 4 days (two 48-hour compute jobs). We use a batch size of 5 structures for all small molecule tasks, and a batch size of 1 structure for all other tasks. We found small batch sizes to be important for obtaining high predictive accuracy. We also found it important to choose the radial cutoff distance \\( r_c \\) appropriately. A list of the cutoff radii in units of [\\AA] that were used for the different systems is given in Table VII.\n\nExample of a tensor product interaction. To illustrate that the interactions outlined in this work reduce to a set of five simple operations, we write out the example of a full \\( 1 \\otimes 1 \\to 1 \\) interaction, i.e. a convolution that uses a \\( l = 1 \\) filter to operate on a \\( l = 1 \\) feature, yielding again a \\( l = 1 \\) output. This corresponds to\n\\( l_i = l_f = l_o = 1 \\), facilitating a cross-product interaction between two \\( l = 1 \\) tensors. In this case, the Clebsch-Gordan coefficients reduce to the Levi-Civita symbol [21]:\n\n\\[\nC^{(l_0=1,m_0)}_{(l_f=1,m_f),(l_i=1,m_i)} \\propto \\epsilon_{ofi} =\n\\begin{cases}\n1 & (o, f, i) \\in \\{(1,2,3), (2,3,1), (3,1,2)\\} \\\\\n-1 & (o, f, i) \\in \\{(1,3,2), (2,1,3), (3,2,1)\\} \\\\\n0 & \\text{else}\n\\end{cases}\n\\]\n\nEvaluating equation [8] as well as \\( \\epsilon_{ofi} \\) and using the relationship \\( Y^{(1)}(\\hat{r}) \\propto \\hat{r} \\), we recognize the output as the vector cross product, taken here between the relative positions and the input feature element \\( V_{bc}^{(l=1)} \\):\n\n\\[\n\\mathcal{L}_{ac}^{(l_o=1)}(\\vec{r}_a, V_{ac}^{(l_i=1)}) = \n\\begin{pmatrix}\n\\sum_{b \\in B} R_c(r_{ab}) \\hat{r}_2 V_{bc3}^{(l=1)} - \\sum_{b \\in B} R_c(r_{ab}) \\hat{r}_3 V_{bc2}^{(l=1)} \\\\\n\\sum_{b \\in B} R_c(r_{ab}) \\hat{r}_3 V_{bc1}^{(l=1)} - \\sum_{b \\in B} R_c(r_{ab}) \\hat{r}_1 V_{bc3}^{(l=1)} \\\\\n\\sum_{b \\in B} R_c(r_{ab}) \\hat{r}_1 V_{bc2}^{(l=1)} - \\sum_{b \\in B} R_c(r_{ab}) \\hat{r}_2 V_{bc1}^{(l=1)}\n\\end{pmatrix}\n\\]\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Data SetCutoff
MD-17 [17, 30, 31]4.0
Molecules, CCSD/CCSD(T) [31]4.0
Water+Ices, DeepMD [15, 32]6.0
Formate on Cu5.0
Li$_4$P$_2$O$_7$ [12]5.0
LiPS [13]5.0
Water, data efficiency tests [39]4.5
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URL https://doi.org/10.1103/physrevb.59.1758\n\n[46] Kingma, D. P. & Ba, J. Adam: A method for stochastic optimization. *arXiv preprint arXiv:1412.6980* (2014).\n\nACKNOWLEDGEMENTS\n\nWe thank Jonathan Vandermause, Cheol Woo Park, David Clark, Kostiantyn Lapchevskyi, Mario Geiger, Joshua Rackers, and Benjamin Kurt Miller for helpful discussions.\n\nWe thank Stefan Chmiela and Alexandre Tkatchenko for providing the timing data for the Toluene system.\n\nWork at Harvard was supported by Bosch Research and the Integrated Mesoscale Architectures for Sustainable Catalysis (IMASC), an Energy Frontier Research Center funded by the US Department of Energy (DOE), Office of Science, Office of Basic Energy Sciences under Award No. DE-SC0012573. N.M. acknowledges support from the Department of the Navy, Office of Naval Research.\n\nWork at Bosch Research was partially supported by ARPA-E Award No. DE-AR0000775 and used resources of the Oak Ridge Leadership Computing Facility at Oak Ridge National Laboratory, which is supported by the Office of Science of the Department of Energy under Contract DE-AC05-00OR22725.\n\nT.E.S. was supported by the Laboratory Directed Research and Development Program of Lawrence Berkeley National Laboratory and the Center for Advanced Mathematics for Energy Research Applications, both under U.S. Department of Energy Contract No. DE-AC02-05CH11231.\n\nThe authors acknowledge computing resources provided by the Harvard University FAS Division of Science Research Computing Group and by the Texas Advanced Computing Center (TACC) at The University of Texas at Austin under allocations DMR20009 and DMR20013.\n\nAUTHOR CONTRIBUTIONS\n\nS.B. initiated the project, conceived the NequIP model, implemented the software and conducted all software experiments under the guidance of B.K. T.E.S. contributed to the conception of the model, guidance of computational experiments, and the software implementation. L.S. created the data set for formate/Cu, guided work on training and MD simulations on this system, and contributed to development of the software implementation. J.P.M. guided the work on the LiPS conductor and implemented the thermostat for MD simulations together with S.B.. M.K. created the AIMD data set of Li$_4$P$_2$O$_7$, wrote software for the analysis of MD results and guided the benchmarking on this system. N.M. wrote software for the computation of the diffusion results and guided discussions on the interpretation of results. B.K. supervised the project from conception to design of experiments, implementation, theory, as well as analysis of data. All authors contributed to the manuscript and the discussion of results.\n\nCOMPETING INTERESTS\n\nThe authors declare no competing interests.\nFigures\n\nFigure 1\n\nLeft: a set of atoms is interpreted as an atomic graph with local neighborhoods. Middle: every atom carries a set of scalar and vector features with it. Right: atoms exchange information via filters, that are again scalars and vectors. The interactions of features and filters define five interactions.\n\nFigure 2\n\nThe NequIP network architecture. Left: atomic numbers are embedded into \\( l = 0 \\) features, which are refined through a series of interaction blocks, creating \\( l = 0 \\) and \\( l = 1 \\) features. An output block generates atomic energies, which are pooled to give the total predicted energy. Middle: the interaction block consists of a series of convolutions, interweaved with self-interaction layers, equivariant nonlinearities and concatenation. Right: the convolution combines the radial function \\( R(r) \\) which operates only on interatomic distances with the spherical harmonics based on unit vector \\( r^* \\) via a tensor product.\nFigure 3\n\nPerspective view of atomic configurations of (a) bidentate HCOO (b) monodentate HCOO and (c) CO2 and a hydrogen adatom on a Cu(110) surface. The blue, red, black, and white spheres represent Cu, O, C, and H atoms, respectively. The subset shown in each subplot is the corresponding top view along the <110> orientation.\n\n![Perspective view of atomic configurations of (a) bidentate HCOO (b) monodentate HCOO and (c) CO2 and a hydrogen adatom on a Cu(110) surface. The blue, red, black, and white spheres represent Cu, O, C, and H atoms, respectively. The subset shown in each subplot is the corresponding top view along the <110> orientation.](page_48_62_1472_393.png)\nFigure 4\n\nQuenched glass structure of Li4P2O7. The insets show the P-O-O tetrahedral bond angle (bottom left) as well as the O-P-P bridging angle between corner-sharing phosphate tetrahedra (top right).\nFigure 5\n\nLeft: Radial Distribution Function, middle: Angular Distribution Function, bridging oxygen, right: Angular Distribution Function, tetrahedral bond angle. All are defined as probability density functions.\n\n![Three plots showing radial distribution function, angular distribution function (bridging oxygen), and angular distribution function (tetrahedral bond angle)](page_42_68_1472_232.png)\n\nFigure 6\n\nComparison of Lithium mean square displacement of AIMD and NequIP trajectories.\n\n![Line plot comparing MSD vs Δτ for AIMD and NequIP, with log-log slope = 1 dashed line](page_120_393_1347_768.png)\n![Log-log plot showing MAE [meV/A] vs. Number of DFT training frames for LO Network, LO/L1 Network, and Best LO Network](page_184_120_1207_670.png)\n\nFigure 7\n\nLog-log plot of the predictive error in forces of NequIP with l = 0 vs. l = 0/l = 1 interactions as a function of data set size, measured via the force MAE.\n\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• codesubmission.zip"} {"paper_id": "prb50", "title": "A fully integrated, standalone stretchable device platform with in-sensor adaptive machine learning for rehabilitation", "text": "# Abstract\n\nPost-surgical treatments of the human throat and various diseases often require continuous monitoring of diverse vital and muscle activities. However, wireless, continuous monitoring and analysis of these activities directly from the (throat) skin still remain elusive. Here, we report the design and validation of a fully integrated standalone stretchable device platform that provides wireless measurements and cloud analysis of diverse vibrations and muscle electrical activities from the suprasternal throat. The modified composite hydrogel with low contact impedance and reduced adhesion provides high-quality long-term monitoring of local muscle electrical signals. The integrated triaxial broad-band accelerometer also measures large body movements and subtle physiological activities/vibrations. The combined data processed by a 2D-like sequential feature extractor with fully connected neurons facilitate the classification of various motion/speech features at a high accuracy of over 90%, which even adapts to the data with noise from motion artifacts or the data from new human subjects. The resulting standalone stretchable device with wireless monitoring and cloud processing capabilities paves the way to design and apply the next-generation wearable skin-interfaced systems for the remote monitoring and treatment evaluation of various diseases.\n\n- Physical sciences/Engineering\n- Physical sciences/Engineering/Electrical and electronic engineering\n- Stretchable device\n- Flexible electronics\n- Machine learning\n- Rehabilitation\n- Medical monitoring and treatment\n\n# Introduction\n\nWearable devices start to gain momentum in disease diagnostic confirmation, treatment evaluation, and healthy aging1–3. For those who suffer from genetic choking4,5 or neck cancer6–8, post-surgical treatment of the human throat often requires the clinician’s continuous monitoring and evaluation of swallowing ability9, vocal-fold motion10, oral intake of liquid11, and others12–14. Monitoring and diagnosis of these behaviors can also prevent secondary injuries that often occur in patients with dysphagia disorders during normal daily activities. Currently, the commercial devices to track laryngeal signatures are rigid, bulky, and tethered, including the lip-closing force gauge15, non-invasive belts16–18, thin-film pressure sensors19, and others20. The poor device/skin contact also results in attenuated signals that are also susceptible to motion artifacts. Therefore, soft on-throat devices are urgently needed to continuously monitor laryngeal activities for diagnosis and rehabilitation evaluation.\n\nDiverse laryngeal activities with serial muscle movements typically cause laryngeal muscle motions and local inertial vibrations21. Therefore, they are often used to evaluate the laryngeal health condition of patients. For instance, swallowing amplitude and rhythm reflect the intake ability of food and water22. However, features obtained by traditional wearable devices such as the single force sensor on the throat19 can only provide limited information about the patient’s health condition. Monitoring of both vibrations and muscle activities is mainly achieved by using separate inertial devices and force sensors on the skin. Efforts to address this challenge lead to the development of a wearable accelerometer for neck voice disorders23 and flexible surface electromyogram (sEMG) electrodes with a strain sensor for oropharyngeal swallowing disorders22,24. However, these flexible sensors suffer from low signal quality, motion artifacts, poor system integration20,25, and severe skin inflammation or allergy during long-term use26–28. It is important to integrate soft wearable electronics2,29,30 with data processing/transmission units31–33 to realize the full potential of the wide range of electro-mechanical signatures34,35. A recent development on a skin-mounted mechano-acoustic sensing system provides a prospective way to track the activity at the suprasternal notch36,37. However, high-quality sEMG signals without being affected by motion artifacts are yet to be integrated into the device platform and the data analysis based on the advanced machine learning algorithm on the cloud is still needed for remote monitoring and evaluation.\n\nMachine learning-based diagnosis is of great interest in the development of smart medicine, especially integrated with soft electronics (to classify the dysphagia severity)36,38,39. Early efforts include the use of the one-dimensional (1D) convolution neural network (CNN)-based deep learning for rehabilitation monitoring after orthopedic surgery40 and predicting knee joint postures41. Despite high recognition accuracy, these CNN models with individual-1D data sources only offer limited feature information during the learning processes for target predictions. These models without memory function and adaptive capabilities suffer from low prediction accuracies for data from new subjects, which is critical in practical applications.\n\nHerein, this work presents a fully integrated standalone stretchable device platform that can wirelessly measure and analyze diverse vibrations and muscle activities directly from the human skin. The modified composite hydrogel electrode interface is designed to maintain robust contact to the throat with low contact impedance for improved signal quality during motion and low adhesion for easy removal. Besides sEMG signals, the triaxial broad-bandwidth accelerometer integrated into the patch can also monitor large body movements (e.g., walking and jumping) and subtle physiological activities (e.g., heartbeats and respiration). With a 2D class sequence feature extractor based on the CNN algorithm, 13 general features from five healthy human subjects can be classified with a high accuracy of 98.2%. More importantly, the fully connected neurons of the 2D-like sequential feature-extracting model can allow the device system to adapt for use with noise from motion artifacts and on new subjects with a high prediction accuracy of 92%. A wireless user interface further enables remote monitoring and real-time evaluation of laryngeal activities on the cloud server, paving the way for the next-generation standalone stretchable device platform for laryngeal rehabilitation management and diagnosis and treatment evaluation of various diseases.\n\n# Results And Discussion\n\nDesign of the laryngeal patch \nThe standalone stretchable device platform consisting of hydrogel electrodes and functional electronic components with signal-processing units interconnected by the coplanar serpentine Cu network (Fig. 1a) can directly adhere to the human skin (Fig. 1b). The processed and wireless transmitted signals from the inertial triaxial accelerometer and hydrogel electrodes (Fig. 1c and Fig. S1) provide continuous and non-invasive monitoring of local vibrations and muscle activities from the larynx and other locations on the human body. Various activities can also be distinguished with an efficient convolutional neural network and the data processed on a cloud server further facilitate remote rehabilitation and disease diagnosis (Fig. 1d). The standalone stretchable device platform fabricated from low-cost processes (Figs. S2-5) exhibits robust performance upon various mechanical deformations (e.g., stretching, bending, and twisting) as verified by both finite element analysis (FEA) and experiments (Fig. 1e and movie S1-2).\n\nDesign and characterization of the composite hydrogel interface \nThe composite hydrogel mainly consists of monomer ([2-(Methacryloyloxy)ethyl]dimethyl-(3-sulfopropyl) ammonium hydroxide, DMAPS), crossed linker, photo-initiator, and ionic salt (see fabrication in Method). Without a need to strictly balance positive and negative charges during the copolymerization process, a wide range of monomer ratios, concentrations, and ionic strengths can be used to synthesize in this zwitterionic-type hydrogel42. To avoid oxidation of the copper-based electrode array and improve the contact quality to the skin for enhanced signal acquisition, a stretchable and highly conductive ionic hydrogel interface is designed by doping Ag nanowires (AgNWs) in the ionic composite with a polydimethylsiloxane (PDMS) skeleton (Fig. 2a). The design with the PDMS skeleton exhibits a reduced peak strain of 0.86 for a uniaxial stretching of 50%, compared to that of 3.13 in the one without (Fig. 2b). The stretchable PDMS with a higher modulus (~200kPa) and optimized number of vertical beams (Fig. S6) provides the modified hydrogel composite with improved load and strain bearing capabilities (14 kPa/200% for the tensile stress/strain) (Figs. 2c and S7). The AgNWs with optimized concentration (0.7 wt%, Figs. S8-9) in the hydrogel not only provide high conductivity, but also result in lower contact impedance than that of the commercial gel electrode (Fig. 2d and S10) for the high-quality acquisition of sEMG signals (Fig. 2e). The lower contact impedance results from the improved hydrogel/skin contact quality as observed on the skin replica (Fig. 2f). The increased contact impedance from drying can recover by applying pure water (Fig. S11). Meanwhile, it is interesting to note that the composite hydrogel presents a lower tensile strain (Fig. 2g) and ca. eight times smaller peeling force (Fig. 2h) compared with the commercial gel electrodes, which facilitates easy removal, especially from the skin of the infants or elderly. The composite hydrogel that can protect the skin from UV and IR radiation (Fig. S12) also exhibits high cell viability of (>80% of epithelial cells) and biocompatibility (Fig. 2i) for long-term monitoring. The modified hydrogel with excellent contact impedance and other properties suitable for integration with flexible circuits in the standalone device platform for health monitoring is superior compared to the previously reported hydrogels26, 43–59 (Table 1).\n\nElectrical and mechanical performance of the fully integrated patch \nThe fully integrated device is designed to provide high-quality wireless transmission. As shown in electromagnetic (EM) simulations, a miniaturized low-temperature co-fired ceramic (LTCC) antenna (Fig. S13) is integrated with the low-power Bluetooth module to investigate and demonstrate the transmission properties of the device. The LTCC antenna on the Cu serpentine network further encapsulated by a 500 µm-thick Ecoflex layer only shows a small frequency shift (<19 MHz) and maintains excellent impedance matching (with a return loss <10 dB) (Fig. 3a), leading to negligible impact on the near and far radiation fields (Figs. 3b-d). The biocompatible Ecoflex encapsulation also isolates the thermal radiation (Fig. 3e) even when the patch is powered by a lithium-ion battery (Fig. S14) due to low power consumption, which is suitable for long-term use on the skin. The tight coupling of the device to the skin provides high-quality sEMG signal even with motion artifacts such as from “talking”, as evidenced by the highest power spectral density and the lowest signal-to-noise ratio (SNR) compared to commercial devices (Figs. 3f-g and Fig. S15).\n\nThe device also exhibits high mechanical compliance and robustness, including a skin-like Young’s modulus of 89.5 kPa (Fig. S16) and a small force hysteresis of <6.4% for a tensile strain of 30% (Fig. 3h), leading to comfort integration on the skin upon various deformations (Fig. 3i). Even when the device is stretched to 30% that is the maximum strain on the skin60, the maximum principal strain (3%) in the Cu serpentine network (Fig. 3j) is still below the fracture strain of Cu (5%)61. The serpentine design of the Cu network also helps the device patch to maintain the mechanical property such as the stress-strain curve (Figs. S17-18) for high-quality monitoring during skin/body movements. The fully integrated device with superior mechanical and electrical properties for conformable monitoring (e.g., swallowing activities) during movements outperforms previous reports of laryngeal sensors15, 22, 23, 37, 62–69 (Table 2).\n\nMonitoring of various biophysical activities at the throat \nAs the throat provides rich information on vibrations and muscle activities for clinical diagnosis of various diseases and corresponding post-surgical training/evaluation14, the device is applied to this critical location for a proof-of-conception demonstration. The high-sensitivity accelerometer ADXL-345 with a sampling frequency of up to 800 Hz in the patch allows successful continuous monitoring of various activities, such as sitting, talking, swallowing, walking, and jumping (Fig. 4a and movie S3-4), with a wide frequency spectrum from 0 to 400 Hz (Fig. 4b). In the laryngeal events, the talking and swallowing signals follow the vibrational movements along the normal direction of the skin (z-axis), whereas walking and jumping signals stem from body motions along the throat skin from the neck to the head direction (y-axis). The time-frequency contour of the signals from the short-time Fourier transform (STFT) confirms the high-frequency (up to 200 Hz) responses with a lower amplitude (less than 0.4 g) of swallowing and talking (Figs. 4c-d). In contrast, walking and jumping are opposite with the slow-moving frequency and a large acceleration magnitude (Fig. S19). These features are highly consistent with the behavior of adults37. In addition, periodically weak vibrations of laryngeal bones from cardiac and lung dilatation processes provide routes to measure heart rate (HR) and respiration rate (RR) from recorded acceleration along the Z and Y axes, respectively. With digital filtering and peak-detection (Fig. 4e), the HR and RR of 19.2 and 50.4 times per minute can be decoupled from the original data (Fig. 4f). As the mounting position of the patch moves up the laryngeal skin, the measured cardiac behavior remains unchanged, but the respiration amplitude decreases (Fig. S20) due to significantly reduced movements (along the neck direction) farther away from the chest cavity. More importantly, the combination of the acceleration data with sEMG for muscular activities during talking (Fig. S21) can further decouple speaking for speech recognition and more precise diagnosis and evaluation of various diseases in the clinical practice.\n\nThe machine learning model for post-surgical rehabilitation \nAccording to the gold standard, the clinical evaluation for post-surgical laryngeal rehabilitation mainly focuses on four typical events (i.e., talking, swallowing, drinking water, and coughing) with long-term and extensive efforts70. To help automatically evaluate the post-surgical rehabilitative condition, a CNN-based 2D-like sequential feature extractor (2D-SFE) is explored to classify and infer pathological status based on the classification of physiological events (Fig. 5a). The collected 1D data (acceleration and sEMG) are first transferred to a 2D vector similar to an image matrix for processing by the CNN-based 2D-SFE that contains 62 filtering layers (Fig. S22) and 2 classifying layers (Fig. S23). In the training model with the above-labeled activities, the processing vectors are iterated from the convolutional layer to the pooling layer and then to the activation layer for achieving dimensionality reduction of the feature vectors. The extracted feature is further classified into special targets by evaluating the consistency of the softmax function in the full connection layer. In the proof-of-the-concept demonstration, five Chinese pinyin and five vowels are chosen as the acoustic states, together with swallowing, drinking water, and coughing behaviors as feature states from five volunteers (sampling rate of 333 Hz). The acceleration and sEMG data in 2D-like vector contours (Fig. 5b, SI Note1) also include noise from other motion actions (e.g., drinking water while coughing) to mimic real-world situations. Randomly dividing each 2D data of the laryngeal feature into 100 sequences with a fixed length of 1000 data points ensures data reliability (covering the entire test data of each feature). The triplet and cross-entropy are used as the objective function for feature extraction and classification, respectively (Fig. 5c). Finally, the classified feature ultimately corresponds to the tested states, forming the confusion matrix71.\n\nAfter training these features through 62 extracting layers and 2 classification layers, the accuracy of all states from training and testing data tends to peak at 60 epochs (Fig. 5d), which can also be verified by the normalized loss for the two objective functions during 100 iterations (Fig. 5e). Feature vectors (FVs) clustered by the t-distributed stochastic neighborhood embedding (T-SNE) algorithm during the training process help visualize the evolution of the principle component in the machine learning space (Fig. 5f). The machine learning model achieves an overall prediction accuracy of 98.2% for the 13 states/features studied in this work (Figs. 5g and S24), demonstrating the excellent performance of the CNN-based 2D-SFE for multidimensional vector prediction (e.g., multiple sequential targets over time)72.\n\nApplications for remote diagnosis and monitoring \nThe measured data wirelessly transmitted to the cloud server in real-time via the local cellular network also create opportunities for remote diagnosis and treatment evaluation over time (Figs. 6a and S25). In the proof-of-the-concept demonstration, the free Ali-cloud is chosen as the cloud hub and the user interface is custom-built according to the application development protocols. Validation of the CNN-based 2D-SFE with the laryngeal activities from another two subjects (SI Note1) shows the high accuracy of over 95% for the 13 features along with three performing states to simulate movement artifacts from choking, chewing, and nodding (Fig. 6b). To help evaluate the post-surgical state, a pathological rehabilitative degree is sorted into eight levels in the cloud-served interface based on three typical activities: swallowing, talking, and drinking water (Methods). The machine learning model with fully connected neurons can adapt to events from new human subjects, resulting in an overall classification accuracy of up to 92% (Fig. 6c). The challenge to separate the principal components of the three typical activities from talking (Fig. 6d) accounts for the relatively low prediction accuracy (Fig. S26), but the overall prediction accuracy still reaches 92%. Reducing the feature category from 13 to 4 (still from 13 different behaviors) leads to quick convergence of the adaptive system (Figs. 6e-f and S27) with a high accuracy of 89.7% (see Methods), demonstrating its power for use in new human subjects.\n\nThe decoupled measurements of HR, RR, and various behaviors over a long term are critical for precise diagnosis and treatment evaluation. Besides the good agreement in the HR between our patch and a commercial platform (BL-420) during sitting and breath-holding (Fig. 6g), the characteristic R, S, and T waveforms can also be clearly observed during long-term monitoring (Fig. 6h). Similarly, the RR tracking from our patch also highly correlates with that from the commercial device, an average RR of ca. 20.35 calculated from the peak-seeking algorithm (Fig. 6i). The relatively long-term monitoring required for perioperative or rehabilitation is further demonstrated by tracking various physiological events for 2.65 hours (Fig. 6j, top). Compared with the commercial counterpart, our device exhibits a larger amplitude in the time domain due to the high mechano-acoustic signal quality. The distinguished frequency spectrum width and power intensity can also help decouple these signals (Fig. 6j, bottom). The difference in the fundamental frequency (e.g., a higher value of over 100 Hz from talking and coughing compared with that of other events) allows the evaluation of various laryngeal conditions. Above all, the standalone stretchable device platform with wirelessly long-term monitored data processed by machine learning on the cloud provides a unique tool for diagnosis and rehabilitative evaluation.\n\n# Conclusion\n\nWe report a fully integrated standalone stretchable device platform for wireless monitoring and cloud-based processing of diverse vibrations and muscle activities directly from the skin. The design of the modified composite hydrogel interface provides a conform contact with the human skin, which achieves lower contact impedance for high signal quality during motions and reduced adhesion for easy removal. The integrated triaxial accelerometer with a broad bandwidth can also accurately monitor both large motions (e.g., walking and jumping) and subtle vibrations (e.g., heartbeats and respiration). The measured data from 13 general signatures/states during laryngeal activities processed by a 2D-like sequential feature extractor based on the CNN can be classified with a high accuracy of 98.2%. The fully connected neuron in the machine learning model further allows it to accurately classify the data from new human subjects with a 92% accuracy. In addition, the custom-built interface to process the data on the cloud opens up new opportunities for remote diagnosis and treatment evaluation for rehabilitation management and various disease applications.\n\n# Methods\n\nFabrication of the stretchable patch and hydrogel interface\n\nThe fabrication of the stretchable patch primarily comprises (i) the engraving and transfer of the conductive serpentine traces, (ii) the low-temperature reflow soldering of components, and (iii) the encapsulation with Ecoflex (Fig. S2). Firstly, the mixed PDMS precursor with a weight ratio of 10:1 for the base to curing agent (Dow Corning, Sylgard 184 A to B) was spin-coated on a clear glass plate at 600 rpm for 10 s, followed by curing at 70°C for 1.5 hrs to form the adhesive substrate. Next, a copper (Cu) foil with a thickness of 8 µm (Red copper, T1100), coated on polyimide (PI, 3 µm), was laminated on the PDMS film at a pressure of 100 kPa for 1h. With the designed CAD file, a 355 nm UV laser (Yuanlu corporation, Wuhan) was used to engrave the serpentine Cu structure with 100 kHz pulse frequency at a speed of 300 mm s⁻¹ for 4 times repeated cutting. Peeling off the residual left the conductive Cu network on the PDMS. The serpentine trace was then transferred to the uncured Ecoflex elastomer (Smooth-on, USA) mixed at a weight ratio of 1:1 (A: B) by a water-soluble tape (AQUASOL). Applying deionized water for 3 hrs dissolved the water-soluble tape. After placing laser-engraved rectangle PDMS isolators at the designed chip location, a thin layer of solder (AL656, Abond) was printed on the connecting pads through a laser-engraved PET mask. After placing all chips and components (smaller than 0.5 cm², Fig. S2 8), the entire patch was heated in a solder pot (ZB2520HL, HuaQi zhengbang) at 138°C for 30 mins. Next, the water-soluble tape was applied to the copper mesh electrode, and an insulting oil (PVB, Langyi Chemical, Zhongshan) was sprayed on the circuits (except the water-soluble tape). Finally, spin-coating silicone elastomer on the bare circuit at 500 rpm for 10 s and curing at 40°C for 1.5 hrs completed the fabrication.\n\nThe fabrication of the hydrogel electrode started with sequentially mixing the monomer (DMAPS), crossed linker (Methylene-Bis-Acrylamide, MBA), photo-initiator (α-Ketoglutaric acid, KGA), ionic salt (LiCl), and deionized water at a weight of 1833:2:1:400:3333. All materials were purchased from Aladdin. Next, the 2.83 mL AgNW solution (5 mg mL⁻¹ in isopropyl alcohol) was added to the obtained hydrogel precursor, followed by a continuous string for 2 hrs. The PDMS mesh was prepared by engraving a 100 µm-thick PDMS film with the UV laser at a pulse frequency of 50 kHz and speed of 300 mm/s for 20 times repeated cutting. After dissolving the water-soluble tape to expose the copper electrode, the PDMS mesh was placed and the hydrogel precursor solution was poured, followed by curing in the UV pot at 30 W for 120 min, to form hydrogel-interfaced electrodes.\n\nDesign of signal processing and transmission circuits\n\nAs illustrated in the detailed circuit schematic (Fig. S29), the signal processing unit included the low-power processor with 8-bit computing ability (Atmel, atmega328p), the inertial accelerometer (ANALOG, ADXL345), and the biological signal detection chip (NeuroSky, BMD101). The power management chip HT7133 (HOLTEK) was chosen due to its ability to convert the voltage from 3.7 to 3.3V. The Bluetooth module PW02 (Phangwei Link) had serial port transmission ability.\n\nFEA of mechanics and electromagnetics\n\nThe finite element analysis was carried out to study the mechanical behaviors of the hydrogel/patch under diverse deformations and the electromagnetic properties of the LTCC antenna. All material properties were assigned according to the material source in the FEA software. The Young's modulus of these materials, the modified hydrogel, copper, eco-flex, polymide, and skin replica, were set as 50 kPa, 80 GPa, 60 kPa, 800 MPa, 200 kPa, respectively.\n\nCharacterizations of mechanical/electrical and structural properties\n\nAll tensile tests were conducted by a mechanical testing machine (ZQ-990B, Zhi Qu). Material conductivity was measured with an LCR digital bridge meter (IM2536, HIOKI). A pair of electrodes with a size of 5.5 mm × 32 mm (or diameter of 18.36 mm for the commercial gel electrodes) separated by a distance of 40 mm on the forearm were used for the contact impedance test. The return loss of the LTCC antenna was measured by a vector network analyzer (SVA 1032X, SIGLENT). The electrophysiological signals were acquired by a multichannel tester (BL-420, TECHMAN, Chengdu). The morphologies of the materials were observed by the scanning electron microscope (HiVac, Apreo). The cell viability was tested by the MTT Assay microplate reader. The light transmittance was obtained by the solar film transmission meter (LS101, LinShang). HR and RR were obtained as the subject performed the instructed behaviors (e.g., holding the breath or sitting still).\n\nMachine learning algorithms for classification and prediction\n\nContinuous measurements from five participants were used as the training data and the measurements from another two volunteers (a male and a female) were used as testing data. First, all measured data were marked at different feature types and normalized to unify data dimensions. Randomly dividing each 2D data of the laryngeal feature into 100 sequences with a fixed length of 1000 data points (covering the entire test data of each feature such as swallowing, drinking, speaking, and coughing) ensured data reliability. Meanwhile, every label was coded via the one hot coding⁷¹. Next, the pretreated data were extracted through 8-weight blocks with 62 processing layers and fed into the classifier. The batch size in the learning model was set to 64 for extracting the feature. The iterative learning rate (LR) was calculated as\n\n$$${L}{R}=\\\\left(1+0.5\\\\mathbf{cos}\\\\left({x}+{\\\\pi }/{e}{p}{o}{c}{h}{s}\\\\right)\\\\right){*}(1-{i}{L}{R})$$\n\n, where x is the times at the corresponding training process, the epochs are iterative times during the training, and iLR is the initial LR (1e⁻⁴). The iterative attenuation rate (AR) was calculated from (with the initial value set as 0.9)\n\n$${{A}{R}}_{{t}}={{A}{R}}_{{t}-1}-{L}{R}{*}\\\\left(\\\\frac{{{m}}_{{t}}}{1-{{\\\\beta }}_{1}^{{t}}}\\\\right)/({\\\\epsilon }+\\\\sqrt{{{v}}_{{t}}/(1-{{\\\\beta }}_{2}^{{t}}})$$\n\n, where β₁ and β₂ are the first and second-order attenuation coefficients, respectively, mₜ is the biased first moment estimate, vₜ is the biased second raw moment estimate, and ε is the relative weight constant. Eq. (2) was based on the optimized machine learning algorithm (i.e., Adaptive moment estimation, Adam). The motion/movement artifacts (e.g., from drinking while coughing) were also accounted for in the testing data from the two new human subjects (see details in SI Note1).\n\nDevelopment of the APP and cloud-served interface\n\nThe app was programmed using java on the Android Studio platform. 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A wearable biosensing system with in-sensor adaptive machine learning for hand gesture recognition. *Nature Electronics* 4, 54–63 (2021).\n\n# tables\n\nTable 1 Comparison of different hydrogels (electrodes)\n\n| Reference | Conducti vity | Transmitt a nce | Biocomp a t ib ility | Stretchabi lity | Contact impedance (1 kHz) | Integrated with circuit |\n|-----------|---------------|-----------------|-------------------|-----------------|----------------------------|-------------------------|\n| 26 | - | Opaque | good | >100% | >10 kΩ | N |\n| 43 | 0.14 S m⁻¹ | 98.8% | good | 1529% | - | N |\n| 44 | 1 S m⁻¹ | 98% | good | 1000% | 10 kΩ | N |\n| 45 | 0.067 S m⁻¹ | - | good | 2636% | - | N |\n| 46 | 0.019 S m⁻¹ | Opaque | good | 450% | - | N |\n| 47 | 3.8 S m⁻¹ | Opaque | - | 3080% | 5~6.5 kΩ | N |\n| 48 | 0.91 S m⁻¹ | 85% | good | 105% | 14.5 kΩ | N |\n| 49 | 0.25 S m⁻¹ | 98.8% | good | 2900% | 31 kΩ | N |\n| 50 | 0.13 S m⁻¹ | 91% | good | 320% | - | N |\n| 51 | 1.2 S m⁻¹ | 80% | - | 850% | - | N |\n| 52 | 0.6 S m⁻¹ | - | good | 1530% | 6.3 kΩ | N |\n| 53 | 0.34 S m⁻¹ | 95% | - | 10000% | - | N |\n| 54 | 0.14 S m⁻¹ | - | - | 1400% | - | N |\n| 55 | 0.17 S m⁻¹ | 85% | good | 580% | - | N |\n| 56 | - | >80% | good | 150~200% | 10-20 kΩ | N |\n| 57 | 47.4 S cm⁻¹ | - | good | 20% | 40 kΩ | N |\n| 58 | - | <50% | None | None | 23.4~38.3 kΩ | N |\n| 59 | <0.5 S m⁻¹ | >80% | good | - | 10~20 kΩ | N |\n| This work | **1.7 S m⁻¹** | 50% | good | 200% | **4.7 kΩ** | **√** |\n\nN no, √ yes, Integrated with circuit: integration of the hydrogel with a flexible circuit in the integrated device for health monitoring.\n\nTable 2 Comparison of different laryngeal sensor patches\n\n| Sensor patch | Flexibility | Systemic integration | Wireless | Sensing mode | Monitoring | Trained by ML | Reference |\n|--------------|-------------|----------------------|----------|--------------|------------|---------------|-----------|\n| Flexible submental sensor | Semi-flexible | N | √ | Strain, EMG | Muscle activity, throat movements | N | 22 |\n| Wearable Accelerometer Sensor | Semi-flexible | N | N | Acceleration | Voices | N | 23 |\n| Mechano-acoustic device | Semi-flexible | √ | √ | Acceleration | Physiological processes, body motions | N | 37 |\n| Acoustic MEMS Sensor | / | N | N | Acoustic vibration | Chewing, Swallowing | √ | 58 |\n| Epidermal device | Full-soft | N | N | Acceleration, EMG | Electrophysiological signals | √ | 59 |\n| Dual-axis swallowing accelerometer | Semi-flexible | N | N | Acceleration | Swallowing | N | 60 |\n| Dual wearable sensor | Semi-flexible | √ | √ | Acceleration | Artifact-canceled physiological | N | 61 |\n| mechano-acoustic sensors | Semi-flexible | √ | √ | Acceleration | Swallowing, respirations | N | 62 |\n| Throat vibrator | Rigid | N | N | Microphone vibration | Dysphagia | √ | 63 |\n| Lip-closing force gauge | Rigid | N | N | Force, EMG | Lip-closing | N | 15 |\n| Neck belt | Semi-flexible | N | N | Displacements | Swallowing | N | 64 |\n| Acoustic detecting array | Semi-flexible | N | N | Acceleration, microphone | Swallowing sounds | N | 65 |\n| Proposed sensor patch | **Full-soft** | √ | √ | EMG, Acceleration | Swallowing, dysphagia | √ | This work |\n\nN no, √ yes, EMG Electromyogram, ML: Machine-learning\n\n# Supplementary Files\n\n- [Moviecaptions.docx](https://assets-eu.researchsquare.com/files/rs-2671531/v1/9cc9a4da580d78a0dc442ee4.docx)\n- [MovieS1.mp4](https://assets-eu.researchsquare.com/files/rs-2671531/v1/9636127294eac73dbd841bc0.mp4) \n Movie S1\n- [MovieS2.mp4](https://assets-eu.researchsquare.com/files/rs-2671531/v1/7499f4cafbc276e964b23e34.mp4) \n Movie S2\n- [MovieS3.mp4](https://assets-eu.researchsquare.com/files/rs-2671531/v1/cb23d8fb162a86b51a54431f.mp4) \n Movie S3\n- [MovieS4.mp4](https://assets-eu.researchsquare.com/files/rs-2671531/v1/4ef4f3ca767b7831e159e60b.mp4) \n Movie S4\n- [Supportinginformation.docx](https://assets-eu.researchsquare.com/files/rs-2671531/v1/a58325b319f50e9ef4aee879.docx) \n Supporting information"} {"paper_id": "prb51", "title": "", "text": "# Abstract\n\nLong-term robust intracortical microelectrode (IME) neural recording quality is negatively affected by the neuroinflammatory response following microelectrode insertion. This adversely impacts brain-machine interface (BMI) performance for patients with neurological disorders or amputations. Recent studies suggest that the leakage of blood-brain barrier (BBB) and microhemorrhage caused by the IME insertions lead to the increased neuroinflammation and reduced neural recording performance. Additionally, a sustained presence of activated platelets and coagulation factors is found near the insertion site. Thus, we hypothesized that the systemic administration of dexamethasone sodium phosphate-loaded platelet-inspired nanoparticle (SPPINDEX) can improve the neural recording performance of intracortical microelectrodes (IMEs) by promoting hemostasis, facilitating blood-brain barrier (BBB) healing, and achieving implant-targeted drug delivery. Leveraging the hemostatic and coagulation factor-binding properties of the platelet-inspired nanoparticle (PIN) drug delivery platform, SPPINDEX treatment can initially attenuate the invasion of neuroinflammatory triggers into the brain parenchyma caused by insertion-induced microhemorrhages or a compromised BBB. Furthermore, targeted delivery of the anti-inflammatory drug dexamethasone sodium phosphate (DEXSP) to the implant site via these nanoparticles can attenuate ongoing neuroinflammation, enhancing overall therapeutic efficacy. Weekly treatment with SPPINDEX for 8 weeks significantly improved the recording capabilities of IMEs compared to platelet-inspired nanoparticles alone (PIN), free dexamethasone sodium phosphate (Free DEXSP), and a diluent control trehalose buffer (TH), as assessed through extracellular single-unit recordings. Immunohistochemical analyses of neuron density, activated microglia/macrophage density, astrocyte density, and BBB permeability suggest that the improved neural recording performance may be attributed to reduced neuron degeneration, activated microglia and astrocytes at the implant interface caused by the decreased infiltration of blood-derived proteins that trigger neuroinflammation and the therapeutic effects from DEXSP. Overall, SPPINDEX treatment promotes an anti-inflammatory environment that improves neuronal density and enhances recording performance.\n\nPhysical sciences/Engineering/Biomedical engineering \nBiological sciences/Biological techniques/Electrophysiology/Extracellular recording \nIntracortical microelectrodes \nNeuroinflammation \nDexamethasone sodium phosphate \nLipid-based nanoparticles \nTargeted drug delivery \nBrain machine interfacing \nNeural engineering \nArtificial platelets\n\n# Highlights\n\n- We developed dexamethasone-loaded platelet-inspired nanoparticles (SPPINDEX).\n- We evaluated intracortical microelectrode (IME) recording performance for 8 weeks.\n- SPPINDEX treatment improved IME recording performance up to 8 weeks in rats.\n- SPPINDEX treatment increased the neuron density near the IME implant site.\n- Our treatment also reduced activated microglia, astrocyte and BBB permeability.\n\n# Introduction\n\nIntracortical microelectrodes (IMEs) are devices designed to record neuronal activity for neuroscience research and the treatment of neurological disorders [1–4]. Neural signals acquired by IMEs can be analyzed and decoded for brain-machine interface (BMI) applications, such as controlling external devices, prosthetics, and stimulators to restore motor function in patients with limb loss or spinal cord injuries [5–10]. However, the primary challenge for the clinical translation of BMI technology is the lack of long-term reliability and stability of IMEs [11–17]. The brain's neuroinflammatory response following IME insertion is widely recognized as a major cause of the decline in neural recording performance over time [4, 18, 19].\n\nUpon the insertion of IMEs into brain motor cortex, healthy neurons and the blood-brain barrier (BBB) are disrupted, leading to an initial reduction in neural recording cellular resources and the influx of blood-derived factors into the brain parenchyma [13, 15, 18, 20–27]. The disruption induces neuron death, and the infiltration of blood proteins triggers the first activation and recruitment of resident microglia, which produce proinflammatory cytokines and cytotoxic factors. This, in turn, leads to the recruitment of astrocytes and secondary neuron death [28–31]. The secondary neuron death further perpetuates neuroinflammation, resulting in the encapsulation of microglia and astrocytes around IME interface, which diminishes the neural recording performance of IMEs [32–36]. Additionally, activated platelets and coagulation factors such as von Willebrand Factor (vWF), collagen, fibrinogen have been observed to be exposed and/or infiltrated near IMEs interface, potentially contributing to neuroinflammation up to at least 8 weeks [37].\n\nOther groups in the field have attempted to reduce the sequelae of neuroinflammation using anti-inflammatory or anti-oxidative therapies after IME implantation. The approaches have ranged from systemic administration, local administration, and device modifications, including coatings, retrodialysis and others [16, 17, 28, 29, 38–44]. For example, Gaire et al have demonstrated that systemic administration of dexamethasone (DEX) acutely post IMEs insertion may not improve the recording functionality of IMEs, even though it attenuated neuroinflammation [38]. Furthermore, high-dose systemic administration of DEX is contraindicated due to potential adverse effects, including reduced bone mineral density, altered glucose levels, and impaired organ function [45]. Zhong et al have previously encapsulated dexamethasone into a nitrocellulose coating on the microelectrodes to achieve local release of drugs around the implantation site, which resulted in significant reduction of neuroinflammation and improvement in signal recording quality [39]. However, local delivery with DEX coated IMEs is not ideal and limited to single application of medicine after surgery since DEX coating will be entirely consumed in days. Moreover, direct modification of the IMEs could result in additional commercial and regulatory burden for integration with existing devices. Although extensive studies have focused on addressing IME insertion-induced neuroinflammation to improve recording stability, few proposed therapies specifically targeting the initial prevention of foreign substance invasion into the brain parenchyma or achieving repeatable and targeted delivery of anti-inflammatory agents to the IME implant site.\n\nPlatelet-inspired nanoparticles (PIN) have demonstrated the ability to attenuate the invasion of blood-derived proteins and achieve localized delivery near the IME implant site by colocalizing with activated platelets and enhancing hemostasis in response to IMEs insertion-induced microhemorrhage [46]. At a vascular injury site, PINs can bind to exposed collagen and vWF via their collagen- and vWF-binding peptides (CBP and VBP), and to activated platelet GPIIb-IIIa receptors via fibrinogen-mimetic peptides (FMP), thus actively accumulating at the injury site [47–49]. Therefore, we hypothesize that PIN can be used to targeted deliver anti-inflammatory drug dexamethasone sodium phosphate (DEXSP) to the IME implant site, thereby attenuating insertion-induced neuroinflammation. In combination with its function to promote hemostasis and reseal compromised BBB, reducing sources that trigger neuroinflammation, systemic administration of the multifunctional DEXSP-loaded PIN (SPPINDEX) therapy is expected to significantly reduce neuroinflammation and enhance the neural recording performance of IMEs.\n\nOur study aimed to evaluate the therapeutic efficacy of systemically administered SPPINDEX on the long-term IME electrophysiology recording quality. First, we investigated the feasibility of manufacturing SPPINDEX with high encapsulation efficiency to achieve an effective dosage of DEXSP under a limited particle dosage, using lipid thin-film rehydration with DEXSP-containing solution. An in vitro release study was conducted to characterize the drug release profile from PIN. We then assessed the IME recording performance of neuronal activity under weekly treatment over an 8-week period using extracellular single-unit recording. To further understand the therapeutic effect of SPPINDEX on neural recording performance, we quantified neuron density (NeuN) near the implantation site at the 8-week endpoint to verify neural health and viability. Additionally, activated microglia (CD68) and astrocytes (GFAP) were evaluated to assess neuroinflammation. The ability of SPPINDEX to reduce blood-derived protein invasion was characterized by immunoglobulin G (IgG) staining. Finally, to ensure that repeated weekly dosing of SPPINDEX over 8 weeks did not induce adverse effects on metabolic homeostasis, kidney and liver functions, or complications such as femur osteoporosis, we monitored rodent weight, glucose (GLU), alanine transaminase (ALT), creatinine (CREA) levels, and femur bone mineral density (BMD).\n\n# Materials and Methods\n\n## Intracortical Microelectrode Validation and Sterilization\n\nThe quality of 16-channel, single-shank intracortical microelectrode (A1x16-3mm-100-177-Z16, NeuroNexus, Ann Arbor, MI) was validated using electrochemical impedance spectroscopy (EIS) assays. A Gamry Interface 1010E Potentiostat was employed to perform EIS on each electrode site of the IME, using the electrode site as the working electrode, Ag | AgCl electrode as the reference and a platinum wire as the counter electrode. EIS measurements were conducted in 1× PBS electrolyte (pH 7.5) and all wire connections placed inside a Faraday cage. Impedances at each electrode site were tested across a frequency range of 1 HZ to 10⁶ Hz (12 points per decade) in a 50 mV rms AC voltage. The 1 kHz impedance was specifically measured to validate the quality of IME prior to in vivo single-unit electrophysiology recording. IMEs with normal 1 kHz impedance values (between 100 kΩ and 1 MΩ) across all 16 electrode sites were deemed suitable for IME implantation surgery. Validated IMEs and 2 mm × 123 µm × 15 µm non-functional Michigan-style single-shank silicon microelectrodes (Qualia Labs, Dallas, TX) were sterilized by Ethylene Oxide (EtO) prior to surgeries.\n\n## Intracortical Microelectrode Implantation Surgery\n\nAll studies described herein were reviewed and approved by the Institutional Animal Care and Use Committee (IACUC) at the Louis Stokes Cleveland Department of Veteran Affairs Medical Center, and were performed in accordance with the ARRIVE guidelines. 29 male rats with indwelling vascular catheters (Sprague Dawley, CD, Charles River Labs, Wilmington, MA) weighing 250–280 grams were included in this study. Surgeries to implant vascular catheters were performed by Charles River Labs. In this study, polyurethane catheters were inserted into the carotid artery and advanced the aortic arch for weekly dosing of treatments which was described in our previous study [46]. All rats were housed up to 1 week prior to further procedures.\n\nSurgical procedures for implanting functional intracortical microelectrodes (IMEs) in the rat cortex were adapted from previously published methods [22, 46, 50, 51]. All rats were initially anesthetized with 3.5% isoflurane and maintained at a surgical level of anesthesia with 1.5-3% isoflurane throughout the procedure. After ensuring anesthesia, eye ointment was applied to protect the corneas, and the nails were clipped to reduce the risk of premature removal of postoperative sutures. The surgical site was shaved, and the animals received subcutaneous injections of cefazolin (16 mg/kg) and meloxicam (1 mg/kg) to prevent infection and manage pain, respectively. Additionally, 0.2 mL of 0.25% Marcaine was administered locally to the incision site for localized pain relief. Following these preparations, the rat was secured in a stereotaxic frame using blunt ear bars and an incisor bar. Vital parameters, including SpO2, heart rate, and body temperature, were continuously monitored throughout the surgery. Regular toe pinches and observations of paw color were performed to confirm the maintenance of an adequate anesthetic plane. The incision area was sterilized with alternating applications of Betadine and isopropyl alcohol.\n\nUnder sterile conditions, a midline scalp incision (approximately one inch) was made to expose the skull for craniotomy procedures. Hydrogen peroxide was applied to the exposed skull to clean the area by removing blood and connective tissue, creating a dry surface. Butyl cyanoacrylate (VetBond, 3M, Saint Paul, MN) was used to control bleeding, maintain skull dryness, and enhance the adherence of the headcap. Craniotomies for stainless steel bone screws (Stoelting Co., Wood Dale, IL) for ground wires (-1.5 mm anterior/posterior, -1.5 mm lateral to bregma) and reference wires (-5.5 mm anterior/posterior, -1.5 mm lateral to the bregma) were performed using a dental drill with 1.35 mm diameter drill bit. Craniotomies for functional IMEs (+2 mm anterior/posterior, +3 mm lateral to the bregma) and non-functional IMEs (+2 mm anterior/posterior and −3 mm lateral to the bregma) were performed with 1.75 mm diameter drill bit (see schematic in Fig. 1 A). Once the dura mater was exposed from drilling, a dura pick was used to reflect the dura. Ground and reference wires on functional IMEs were wrapped and secured on screws before implantation of IMEs. Once the positions were secured, the functional IME was inserted to the motor cortex with 2 mm depth using the stereotaxic frame. Non-functional IMEs were manually implanted at approximately 2 mm depth for improving the sample size (N) for histology study. Excess bone debris and blood from drilling and insertion were then cleaned by applying saline, followed by the application of Kwik-cast to seal the empty space in the craniotomies with implants. Once the Kwik-cast cured, Teets Cold Cure dental cement was applied around all craniotomies to build a headcap for stabilizing all implants and fuse the base to the skull. After the dental cement was cured, 5−0 monofilament polypropylene sutures were used to suture the incision site. Cefazolin and meloxicam were subcutaneously administered to the animal as post-operative treatment for infection and pain in a previously reported frequency.\n\n## Dexamethasone Sodium Phosphate Loaded Nanoparticle Manufacture and Characterization\n\nDexamethasone sodium phosphate loaded platelet-inspired nanoparticles (SPPINDEX) were manufactured with the ‘thin-film rehydration and extrusion’ method adapted from previously established protocols [47, 49, 52, 53]. Briefly, DSPC, cholesterol, DSPE-mPEG(1k), DSPE-PEG(2k)-FMP, DSPE-PEG(2k)-VBP, DSPE-PEG(2k)-CBP and DSPE-Cy5 were homogeneously mixed in 1:1 chloroform:methanol organic solvent at 46.50, 45.00, 6.50, 0.50, 0.25, 0.25 and 1.00 mole percentages, respectively. After the thin lipid film was formed using rotary evaporator, the lipid thin-film was rehydrated with 5% w/v trehalose in 4.05 mg/mL HEPES solution (TH) containing 4 mg dexamethasone sodium phosphate. 10 freeze/thaw cycles were applied to the rehydrated lipid solution with liquid nitrogen and 75°C water bath to maximize drug encapsulation, followed by extrusion with 200 nm then 100 nm polycarbonate membranes using a pneumatic extruder (Evonik, Burnaby, Canada) to form small unilamellar vesicles. Nanoparticle characterizations, including hydrodynamic size distribution, zeta potential, and polydispersity index (PDI) of SPPINDEX, were conducted using dynamic light scattering (DLS) with a Data Litesizer (Anton Paar, Ashland, VA). Zeta potential measurements were performed using an Omega cuvette (Mat. No. 225288, Anton Paar, Ashland, VA) and analyzed under the Smoluchowski approximation with a Henry factor of 1.5. Measurements were conducted using water as the solvent, with the refractive index set to 1.33 and relative permittivity at 78.3. Endotoxin levels in SPPINDEX were evaluated using the Endosafe Limulus Amebocyte Lysate (LAL) kit (#3672151, Charles River Laboratories, Charleston, SC).\n\n## Dexamethasone Sodium Phosphate Loaded Nanoparticles Purification and Encapsulation Efficiency Characterization\n\nUnencapsulated dexamethasone sodium phosphate (DEXSP) was separated from SPPINDEX using a centrifugation method. Freshly manufactured SPPINDEX was transferred to a 10 kDa molecular weight cutoff (MWCO) Amicon filter (Millipore-Sigma, Burlington, MA, UFC801024) in a 15 mL Falcon tube, followed by an initial centrifugation at 3200 x g for 20 minutes. To wash the SPPINDEX trapped on the filters, 0.5 mL of TH solution was added, and a second centrifugation was performed to remove any remaining unencapsulated DEXSP. The mass of the separated unencapsulated DEXSP was quantified via reverse-phase high-performance liquid chromatography (RP-HPLC, Shimadzu). The analysis utilized a C18 reverse-phase column (Shimadzu, Columbia, MD, #220-91199-13) and a UV-vis detector (SPD40V, Shimadzu, Columbia, MD).\n\nFor RP-HPLC analysis, unknown encapsulated DEXSP samples and DEXSP standards were prepared using desoximetasone (DES) as an internal standard to account for variations in injection and HPLC system performance. The mobile phase consisted of an isocratic mixture of 32:68 v/v acetonitrile/10 mM phosphate buffer, with an injection volume of 30 µL and a flow rate of 1 mL/min. UV absorbance was measured at 240 nm, with retention times of 3.5 minutes for DEXSP and 22 minutes for DES. Standard calibration curves of the DEXSP-DES peak area ratios and DEXSP-DES concentration ratios were plotted using OriginLab software (OriginLab Corporation, Northampton, MA) to determine unknown DEXSP concentrations. Encapsulation efficiencies were calculated using Eq. (1).\n\nEncapsulation Efficiency (%) = [Total used drug (mg) − Unencapsulated drug (mg)] / Total used drug (mg) × 100% (1)\n\n## Dexamethasone Sodium Phosphate In Vitro Release\n\nDialysis membrane (DM) method was employed to characterize the in vitro release profile of DEXSP from SPPINDEX [54]. Briefly, 0.5 mL of purified SPPINDEX solution was transferred into a dialysis device (Slide-A-Lyzer™ MINI Dialysis Devices, Thermo Fisher Scientific, Waltham, MA) with a 10 kDa MWCO. The device was submerged in 14 mL of 1× PBS within a 15 mL Falcon tube and incubated at 37°C in a shaker set to 70 rpm. At specified time points, 1 mL aliquots were collected from the dialysis medium containing released DEXSP for quantification using RP-HPLC analysis. After each sampling, an equal volume of fresh 1× PBS was added to maintain the dialysis conditions.\n\n## Dexamethasone Sodium Phosphate Loaded Nanoparticles Administration\n\nTwenty-nine catheterized rats were assigned to receive weekly administrations of one of the following treatments: dexamethasone sodium phosphate-loaded platelet-inspired nanoparticles (SPPINDEX, n = 7, 2 mg/kg nanoparticle dosage and 0.3 mg/kg equivalent drug dosage), platelet-inspired nanoparticles (PIN, n = 7, 2 mg/kg nanoparticle dosage), free dexamethasone sodium phosphate (DEXSP, n = 8, 0.3 mg/kg drug dosage), or 5% w/v trehalose in 4.05 mg/mL HEPES solution (TH, n = 7) as diluent control. Administration timeline is shown in Fig. 1 B. The infusion method via indwelling vascular catheters was performed according to a previously established protocol [46]. Surgeries to implant vascular catheters were performed by Charles River Labs. Briefly, sterile syringes containing the treatments were connected to external tether tubing with PinPort injectors to access the carotid artery catheters. The treatments were infused towards the aortic arch at a rate of 0.1 mL/min using a syringe pump. Following the infusion, the catheters were maintained by flushing with 500 units/mL heparin to prevent clogging.\n\n## Electrophysiological Recordings\n\nNeural electrophysiology recordings were conducted twice per week for 8 weeks using functional intracortical microelectrodes (IMEs) implanted in rats adapted from previous reported methods [16, 17, 55–58]. The rats were initially anesthetized with 3.5% isoflurane and maintained under surgical anesthesia with 1.5-3% isoflurane during the cleaning of the exposed IME connectors to remove blood and tissue debris using isopropanol. Following this, the rats were transferred into a custom-made acrylic box within a Faraday cage while still under anesthesia. A 16-channel ZIF-Clip Headstage (Tucker-Davis Technologies Inc., Alachua, FL) was attached to both sides of the IME connectors, which were connected to the 32-channel Motorized Commutator System (#ACO32, Tucker-Davis Technologies Inc.). This setup allowed the rats to move freely and minimized motion artifacts. A 16-Channel Medusa Pre-Amp (RA16PA, Tucker-Davis Technologies Inc.) was connected to the commutator to amplify and digitize the analog signals, which were then transmitted to a Bioamp Processor (RZ5, Tucker-Davis Technologies Inc.) via fiber optic connectors for further signal processing. The processed signals were displayed and recorded using Synapse software (Tucker-Davis Technologies Inc.) on a computer. Neural recordings were conducted for 10 minutes after the rats awoke, at a sampling rate of 24.414 kHz with a built-in 300–3000 Hz bandpass filter to capture single-unit activity [59]. After the 10-minute recording session, the rats were disconnected from the headstage and returned to their housing cages.\n\n## Electrophysiological Analysis\n\nRecorded digital neural signals were analyzed using Plexon Offline Sorter (Plexon Inc., Dallas, TX) to identify single units [17, 51]. The data were first referenced to the common median across all 16 channels of the IMEs to eliminate potential artifacts arising from the rats' movement and common-mode signals. Spikes were detected using −4σ threshold from the mean of the peak heights. After spike detection, any spikes with amplitudes exceeding ±500 µV were considered abnormal neuronal signals and were excluded from the analysis. Additionally, spikes detected across more than 14 channels were classified as motion artifacts caused by the rats' grooming or movement and were removed. Following artifact removal, automatic sorting was performed using the K-Means Scan method to cluster the remaining spikes into individual single units. True positive signal units were manually verified following previously established protocols [58]. The active electrode yield in each treatment group for each week was calculated by dividing the total number of active channels (defined as those with at least one active unit) by the total number of channels (16 channels per IMEs device × number of animals for each treatment in the specific week, excluding channels that never have any active units). The proportion of active channels for each treatment group in each time phase (the first four weeks, W1-4, and the last four weeks, W5-8) was calculated similarly, but by summing the total active and total channels across all weeks in the respective time phase. On a weekly basis, the total number of channels (N) was as follows: 107 for SPPINDEX, 104 for PIN, 104 for TH, and 118 for Free DEXSP. For the entire phase, the total number of channels (N) was 428 for SPPINDEX, 416 for PIN, 416 for TH, and 472 for Free DEXSP.\n\nPeak-to-peak voltage (Vpp) was defined as the absolute voltage range from the positive to negative peak of a clustered and verified single unit. Noise was calculated as the root mean square (RMS) of the signal after spike exclusion. Signal-to-noise ratio (SNR) was determined by dividing the Vpp by the noise for each verified single unit. Spike rate was defined as the inverse of the median interspike interval for each verified single unit. Calculated recording parameters were obtained using custom-developed MATLAB software (Mathworks, Natick, MA). Units with a Vpp less than 40 µV were considered non-putative and excluded from further analysis [57]. The calculated recording parameters were grouped into two intervals: the first four weeks of the study (W1-4) and the last four weeks (W5-8). Outliers in the SNR for each unit, across all treatments and phases, were identified using the ROUT method with Q = 5%. Units with verified SNR outliers were excluded from further analysis. Vpp, noise, SNR, and spike rate values for each unit were averaged at the individual channel level for each IME within different treatment groups and time phases, resulting in a single averaged value of Vpp, noise, SNR, and spike rate for each active channel. The total number of units for each active channel was counted and divided by the number of weeks in the specific time phase to calculate the units per active channel. This yielded a single average number of units per active channel for each IME across different treatment groups and time phases, which was used for graph plotting and statistical analysis. For Vpp, noise, SNR, spike rate, and units per active channel data, the sample size (N) represents the total number of active channels for different treatment groups at different phases: 93 for W1-4 SPPINDEX, 51 for W1-4 SPPINDEX, 77 for W1-4 PIN, 43 for W5-8 PIN, 81 for W1-4 TH, 38 for W5-8 TH, 86 for W1-4 Free DEXSP, 30 for W5-8 Free DEXSP.\n\n## Animal Perfusion and Tissue Processing\n\nAt the 8-week endpoint, rats were administered an intraperitoneal overdose of ketamine (160 mg/kg) and xylazine (20 mg/kg). Cardiac perfusion and dissection procedures were adapted from a previously established method [60]. In brief, rats were perfused with 600–700 mL of 1× PBS at a flow rate of 50–70 mL/min. Once the liquid flowing from the right atrium was clear, an additional 300–400 mL of 10% neutral buffered formalin solution was perfused. The brains were then dissected and stored in 10% neutral buffered formalin at 4°C for 24 hours, followed by cryoprotection using a 30% w/v sucrose solution containing 0.01% sodium azide. A 10% stepwise increase in sucrose concentration was performed every 24 hours, with two exposures at 30%. The cryoprotected brains were subsequently embedded in Optimal Cutting Temperature (OCT) compound (Scigen Tissue-Plus™ O.C.T. Compound, Fisher Scientific, Hampton, NH, USA) and frozen on dry ice, then stored at -80°C. Brain sections were cut transversely at 20 µm thickness using a cryostat (CM1950, Leica, Deer Park, IL).\n\n## Immunohistochemistry, Imaging and Analysis\n\nImmunohistochemistry (IHC) staining was performed on brain slices to visualize and assess neuron loss, microglial activation, astrocyte activation, and blood-brain barrier (BBB) permeability (antibodies listed in Table S1). IHC procedures were adapted from previously reported methods [24, 37, 46, 61, 62]. Brain slices on slides were incubated for 15 minutes in a humidified chamber at room temperature, followed by washing with 1× PBS to remove the O.C.T. compound. The tissues were rehydrated and permeabilized with 1× PBS containing 0.1% Triton for 15 minutes. To prevent non-specific antibody binding, tissues were blocked in a 4% goat serum solution. Primary antibodies were applied and incubated overnight. On the following day, tissues were washed multiple times with 1× PBS containing 0.1% Triton to remove any remaining primary antibodies. Secondary antibodies were then applied for 2 hours. Afterward, a series of washing steps were performed to eliminate any residual secondary antibodies and Triton, followed by the application of DAPI Fluoromount-G mounting medium and coverslips. The slides were dried overnight and stored at 4°C for imaging.\n\nSlides with stained brain slices were imaged using Automatic Slide Scanner Axioscan Z7 (Zeiss Inc., Oberkochen, Germany) with the 20× objective. One slide from each type of staining was used to determine the optimal exposure time. The optimal exposure times were consistent over the entire study. The resulting images were subset around the implantation region and exported as 16-bit TIFF images (10,000 × 10,000 pixels by pixels) using ZEN 3.6 Blue Edition software for fluorescent intensity analysis. A custom Python program, based on SECOND [63], was employed to define implant holes and mask image artifacts. Concentric rings were generated by the program, starting from the outer edge of the implant hole and extending across the image in 50 µm intervals, to measure the average fluorescence intensities in each bin as a function of distance from the hole. Intensities in masked regions due to artifacts were excluded from the measurements. As reported in previous methods [46], average fluorescence intensities for each bin were normalized to the background intensity in the 600–650 µm bin. Since CD68-positive microglia and immunoglobulin G (IgG) are not expected in healthy brain parenchyma, their normalization factors were set to 0, whereas the factor for astrocytes (GFAP), which are normally present, was set to 1.\n\nTo count NeuN stained neurons around the implant hole, Cellpose algorithm was used to segment the neurons on NeuN stained slices [64]. As reported in a previous established workflow [65], a specialized cyto3-based model was further trained with at least one stained slide from each treatment group using default parameters. All NeuN images were segmented in batches using the trained model. A custom Python script calculated neuron density from the raw NeuN segmentation masks. Similar to the intensity analysis, neuron density (# of neuron per mm²) at each 50 µm bin was calculated by dividing neuron counts by the total area of each bin, starting from the implant site, and normalized to the density in the 600–650 µm bin.\n\nFor each IME implant hole, at least three different brain slice depths were analyzed for both the SECOND fluorescent intensity analysis and the Cellpose neuron density analysis. For each treatment group, brain tissues from a minimum of four animals were included in both analyses.\n\n## Blood Collection and Analysis\n\nAt weeks 0 (prior to treatment), 4, and 8 (following weekly treatments), rats were anesthetized with 3.5% isoflurane and maintained under a surgical plane of anesthesia (1.5-3% isoflurane). As described in a previously published method [46]. 300 µL of blood was then collected from the tail vein using a capillary blood collection tube (Multivette® 600 Lithium heparin LH, Sarstedt, Germany). After plasma was separated from whole blood by centrifugation, glucose (GLU), creatinine (CREA), and alanine transaminase (ALT) levels were measured in the plasma.\n\n## Statistics\n\nExcel (Microsoft Corporation, Redmon, WA), R Studio 2023.12.0 + 369 (RStudio, PBC, Boston, MA) and GraphPad Prism (Dotmatics, Boston, MA) were used for data analysis, rearrangement and statistical measurements. Custom R scripts were used to rearrange in vivo extracellular single-unit recording raw data, including the number of units and active channel yield across different animals, treatments, and weeks. A two-sided proportions z-test was performed using an R-based script to calculate significant statistical differences in active electrode yield between groups on a weekly basis, as well as the proportion of active electrode between and within groups at different study phases. Statistical differences in exported recording parameters (Vpp, noise, SNR, spike rate) were calculated using a mixed-effects model analysis with post hoc Tukey pair-wise comparisons in GraphPad. A one-way ANOVA with post hoc Tukey pair-wise test in GraphPad was used to compare normalized neuron density (NeuN) and normalized fluorescence intensity for astrocyte (GFAP), activated microglia/macrophage (CD68), and Immunoglobulin G (IgG) among treatment groups within each distance interval. The Kruskal-Wallis test with post hoc Dunn's pair-wise test in GraphPad was conducted to calculate statistical differences in blood parameters and weights measurements. Statistical significance was represented as * = p < 0.05, ** = p < 0.01, *** = p < 0.001 and **** = p < 0.0001 for all statistical analyses in this study. The standard error of the mean (SEM) was used to plot error bars for all box plots.\n\n# Results\n\n## Characterization of SPPINDEX and DEXSP Release Profile\n\nThe schematic of dexamethasone sodium phosphate-loaded platelet-inspired nanoparticles (SPPINDEX) is shown in Fig. 2 A. Due to its hydrophilicity, the DEXSP payload is assumed to be predominantly loaded in the aqueous core of the PIN. The encapsulation efficiency of DEXSP in PIN was 78.7 ± 5.5% based on averaged data from seven manufacturing batches. The overall surface charge of SPPINDEX was −13.9 ± 2.6 mV. The hydrodynamic diameter of SPPINDEX is 124.9 ± 16.5 nm, with 90% of the total particles are smaller than 151.4 ± 26.6 nm (Fig. 2 B).\n\nOver time, in an infinite sink model, approximately 65% of DEXSP was released within the first 24 hours (Fig. 2 D), with complete release occurring over 24 days into the 1× PBS dialysis solution. The initial burst release of DEXSP from SPPINDEX suggests the necessity of freshly preparing SPPINDEX prior to animal administration. In this study, fresh SPPINDEX was prepared on a weekly basis.\n\n## Therapeutic Efficacy of SPPINDEX on IMEs Recording Performance\n\nTo acquire and evaluate awake recordings, 16-channel, single-shank functional intracortical microelectrodes (IMEs) were implanted to animals’ brain primary motor cortex. Animals were separated to four cohorts based on the treatments: drug-loaded nanoparticles (SPPINDEX, n = 7), unloaded nanoparticles (PIN, n = 7), free drug (Free DEXSP, n = 8) and diluent control (TH, n = 7). The study timeline is shown in Fig. 1 B. Active electrode yield (AEY), calculated to assess recording performance, was determined by conducting biweekly recordings and analyses. It was defined as the percentage of active channels (channels with detected active units) relative to the total potential channels (excluding channels without any detected active units throughout the entire study). Functional IMEs in the SPPINDEX-treated animals demonstrated significantly better performance in terms of AEY compared to the Free DEXSP and TH groups over the 8-week period (see Fig. 3 B for trend and Fig. 3 C for significance levels). Compared to the PIN group, the AEY of the SPPINDEX group was significantly higher during most weeks, except for weeks 3, 4, and 6.\n\nActive electrode data were grouped to calculate the proportion of active electrodes, which was used to evaluate recording performance across two phases of the study (Fig. 3 D): the first four weeks (W1_4) and the last four weeks (W5_8). The SPPINDEX group showed a significantly higher proportion of active electrodes in both phases compared to all other groups (p < 0.001 to PIN, p < 0.0001 to TH, p < 0.0001 to Free DEXSP in W1_4; p < 0.0001 to all other groups in W5_8). The PIN group exhibited a significantly higher proportion of active electrodes in both phases compared to the TH and Free DEXSP groups (p < 0.05 to TH, p < 0.001 to Free DEXSP in W1_4; p < 0.001 to TH, p < 0.0001 to Free DEXSP in W5_8). No significant differences in the proportion of active electrodes were observed between the TH and Free DEXSP groups during the first week of the study. However, in the last four weeks, the proportion of active electrodes in the Free DEXSP group was significantly lower than in the TH group (p < 0.001). Within each treatment group, the proportion of active electrodes significantly decreased in the last four weeks of the study (p < 0.001 in SPPINDEX, p < 0.0001 in PIN, p < 0.0001 in TH, p < 0.0001 in Free DEXSP), indicating a decline in IME recording performance over time (Fig. 3 F – 3 I). Nevertheless, the SPPINDEX group exhibited a 17% decline in active electrode yield, which was less pronounced compared to the declines in the other groups: 25% for PIN, 37% for TH, and 54% for Free DEXSP.\n\nActive units per channel were calculated to assess the IMEs' ability to record single units (Fig. 3 E). During the first four weeks of the study, SPPINDEX treatment significantly improved active units per channel compared to all other groups (p < 0.0001 to PIN, p < 0.05 to TH, p < 0.0001 to Free DEXSP). In the last four weeks, SPPINDEX maintained significantly higher active units per channel compared to the TH and Free DEXSP groups (p < 0.05 to TH, p < 0.0001 to Free DEXSP), but not compared to the PIN group. Within each treatment group, no significant differences were observed between the different phases of the study for any treatment group.\n\nPeak-to-peak voltage (Vpp) was significantly higher in the SPPINDEX group compared to the PIN and Free DEXSP groups (p < 0.01 to PIN and Free DEXSP) during the first four weeks of the study, but there was no significant difference between the SPPINDEX and TH groups, suggesting that SPPINDEX treatment may not substantially influence signal intensity (Fig. 4 A). In the last four weeks of the study, no significant differences in Vpp were observed among the groups. Noise levels in the SPPINDEX group were significantly higher compared to the TH and Free DEXSP groups (p < 0.05 to TH, p < 0.001 to Free DEXSP) during the first four weeks, indicating a potential increase in noise associated with SPPINDEX treatment during the early weeks (Fig. 4 B). However, this effect did not persist in the later weeks of the study. Although the signal-to-noise ratio (SNR) was significantly lower in the SPPINDEX group compared to the TH group (p < 0.001 in W1_4, p < 0.0001 in W5_8) for both phases of the study, the mean SNR remained above 5 for all treatments, demonstrating high-quality recordings across all groups (Fig. 4 C). There were no significant differences in spike rate between the SPPINDEX group and the other groups (Fig. 4 D).\n\n## Therapeutic Effects of SPPINDEX on Neuron Health and Density\n\nThe acute death of resident neurons following IMEs insertion, along with secondary neuron death caused by the insertion-induced neuroinflammatory response, severely reduces healthy neuron density in the motor cortex, leading to a scarcity of neuronal activity recording resources. Neuronal populations were assessed using neuronal nuclei (NeuN) staining. To evaluate the therapeutic effects of SPPINDEX on neuronal health and viability around the insertion site, brain tissues from all groups were stained with NeuN at the 8-week endpoint. Weekly systemic administration of SPPINDEX over 8 weeks significantly attenuated the reduction in neuron density up to 150 µm from the implant site compared to the PIN, TH and Free DEXSP groups (Fig. 5 B). Specifically, the SPPINDEX group (59% neuron density normalized to neuron counts in 600–650 µm distant area of tissue) exhibited a 186% increase in neuron densities compared to the TH group (21% normalized neuron density) at the 0–50 µm bin from the implant site, indicating that SPPINDEX treatment significantly enhances the availability of healthy neurons for electrophysiology neural signal recording near the IME interface. This increase in neuron density likely contributes to the improved recording performance observed with SPPINDEX treatment.\n\n## Therapeutic Effects of SPPINDEX on Neuroinflammation and BBB Permeability\n\nIn addition to the acute neuron death caused by the IME insertion, microglia and macrophages are also activated and recruited to the implant site through both DAMPs (cell debris from neuron death) and PAMPs (influx of blood-derived proteins) signaling pathways [66–69]. Chronic activation and recruitment of microglia and macrophages induces self-perpetuating neuroinflammation and cell encapsulation on IMEs interface, leading to chronic failure of IME recording performance. At the 8-week endpoint, activated and recruited microglia intensity (CD68) was found significantly lower up to 50 µm from the implant site in animals treated with SPPINDEX in comparison to those treated with PIN, TH and Free DEXSP (Fig. 5 C). Animals treated with weekly SPPINDEX over 8 weeks had significantly lower expression of astrocyte (GFAP) up to 100 µm from the implant site in comparison to the TH and Free DEXSP groups (Fig. 5 D). Animals treated with weekly PIN over 8 weeks also showed significantly lower intensity of astrocyte up to 50 µm from the implant site in comparison to the TH and Free DEXSP groups. Free DEXSP groups showed the significantly highest activated microglia expression levels near the implant site.\n\nBBB permeability was evaluated by staining immunoglobulin G (IgG) to assess the potential resealing function of SPPINDEX and PIN groups. IgG is a classic biomarker for BBB leakage, as it is a blood serum protein and not commonly found in the brain parenchyma. In the SPPINDEX group, IgG intensity was significantly reduced up to 550 µm from the implant site in comparison to the TH group (Fig. 5 E, significant levels after 200 µm shown in Table S5). Similarly, animals treated with PIN also had significantly lower IgG intensity starting from 50 µm up to 600 µm from the implant site compared to the TH group (Table S5). The significantly reduced IgG levels in both the SPPINDEX and PIN groups suggest that the nanoparticles may facilitate blood-brain barrier (BBB) resealing and promote hemostasis at sites of IME insertion-induced microhemorrhage.\n\n## Side Effects of SPPINDEX on Metabolic Homeostasis and Organ Functions\n\nLong-term systematic dexamethasone treatment might induce multiple side effects including abnormally high glucose level, weight loss, and bone mineral density (BMD) loss in rodent model [45]. To ensure weekly dosage of SPPINDEX does not induce severe side effects on metabolism, liver and kidney functions in rats, we measured glucose levels, alanine transaminase (ALT) levels, and creatinine (CREA) levels at week 0, week 4 and week 8, weights weekly. No significant change on glucose levels and weights in the animals treated with SPPINDEX in comparison to those treated with control TH (Fig. 6 A, Fig. 6 C). Weights in the animals were significantly reduced in Free DEXSP group compared to the TH at week 4 and week 8, suggestion temporary effects on metabolism of animals from weekly repeated Free DEXSP treatment. ALT levels were also not significantly abnormal in the SPPINDEX group in comparison to the control TH group (Fig. 6 B). Most CREA levels were below detection limits, indicating minimal fluctuations of kidney functions among all groups (Table S6), and therefore the data was omitted from plotting in Fig. 6.\n\n# Discussion\n\nIntracortical microelectrodes are widely used in neuroscience research and BMI systems for restoring the loss of motor function in patients with limb loss and spinal cord injury [70–74]. However, electrophysiological recording quality significantly declines within weeks after implantation. This decline is primarily due to a self-perpetuating neuroinflammatory response triggered by IME insertion-induced tissue damage and the infiltration of blood-derived proteins and pathogens into the brain parenchyma through a compromised blood-brain barrier (BBB) [75–80].\n\nIME insertion-induced bleeding and tissue damage is unavoidable with current devices, prompting extensive research into novel therapies aimed at disrupting insertion-induced neuroinflammation in the brain parenchyma. This neuroinflammation is characterized by the infiltration of microglia and astrocytes at the implant site, accompanied by the release of proinflammatory cytokines such as TNF-alpha and IL-1 beta, as well as cytotoxic factors like reactive nitrogen species (RNS), reactive oxygen species (ROS), and nitric oxide (NO), causing secondary cellular and tissue damage (neuron death) surrounding the implant [78, 80].\n\nGaire et al. investigated the effects of acute systemic administration of DEX and found that it might not improve chronic recording quality due to off-target drug delivery. Additionally, long-term systemic dosing of DEX is contraindicated, as it can cause numerous side-effects and complications [38]. In contrast, Zhong et al. explored local delivery of DEX by coating microelectrodes with DEX-encapsulated nitrocellulose prior to insertion, aiming to avoid off-target effects and the safety risks associated with systemic administration [39]. Although this approach significantly reduced neuroinflammation and improved signal recording quality, it was limited by a single administration and depletion of the drug, making it inadequate for long-term treatment. Both systemic and local delivery of free DEX show promise for mitigating insertion-induced neuroinflammation, but each has its own limitations. There are limited studies focused on preventing the triggers of neuroinflammation, such as enhancing hemostasis to manage insertion-induced microhemorrhages and resealing the compromised blood-brain barrier (BBB) to reduce the infiltration of foreign substances into the brain parenchyma.\n\nThe physical damage to cells and tissues in the brain parenchyma caused by IME insertion is inevitable and partially induces a neuroinflammatory response through the DAMPs signaling pathway [66, 81]. Key triggers of neuroinflammation, such as the influx of blood-derived proteins and pathogens into the brain parenchyma through compromised blood vessels and the blood-brain barrier (BBB), can potentially be targeted and mitigated through the application of biomaterial-based hemostatic interventions. Biomaterials designed to enhance hemostasis in brain trauma and to repair brain tissue and blood vasculature show promise for reducing intracerebral hemorrhage, thereby preventing secondary injuries such as inflammation and cerebral edema [82]. Therefore, the principal hypothesis of the current study is that systemic administration of platelet-inspired nanoparticles (PIN) can promote hemostasis at the site of insertion-induced microhemorrhages and reseal the compromised BBB. This would reduce the infiltration of blood-derived proteins and pathogens into the brain parenchyma. Additionally, activated platelets and coagulation factors such as von Willebrand factor (vWF), collagen have been found to persist near the implant site and are associated with neuroinflammation for up to 8 weeks [37]. Localization and retention of PINs at the implant site could also enable targeted delivery of anti-inflammatory agents, such as dexamethasone sodium phosphate, further enhancing the attenuation of self-perpetuating neuroinflammation beyond their hemostatic function. This combination therapy, using anti-inflammatory drug-encapsulated hemostatic nanoparticles, has the potential to improve long-term neural recording performance.\n\nIn this study, we demonstrated that the decline in active electrode yield over time was significantly attenuated in animals treated with SPPINDEX compared to those receiving other treatments (PIN, TH, and Free DEXSP) throughout the 8-week study period. Specifically, the proportion of active electrodes was approximately 36% higher in the first half of the study and 82% higher in the second half with SPPINDEX treatment compared to TH treatment, indicating significantly improved neural recording performance in animals receiving weekly SPPINDEX administration. Significantly lower IgG levels around the implant sites were observed in the SPPINDEX group, suggesting that the improved recording performance may be due to reduced infiltration of blood-derived substances into the brain parenchyma. This reduction in blood-derived substance infiltration resulted in less activation and recruitment of microglia near the implant site in the SPPINDEX group compared to the TH and Free DEXSP groups, further supporting our hypothesis that the resealing and hemostatic properties of nanoparticles can mitigate the influx of blood-derived proteins, thereby reducing cells infiltration and neuroinflammation around the implant site.\n\nThe significant improvement in active electrode yield observed in the PIN-only group compared to the TH and Free DEXSP groups validates that the nanoparticle itself, even without drug loading, can enhance recording performance by resealing the compromised BBB and inhibiting the influx of blood-derived proteins, as seen in histological analysis. This reduced influx also attenuated astrocyte infiltration near the implant site compared to both the TH and Free DEXSP groups. The significant reduction in IgG levels in both the SPPINDEX and PIN groups, with no significant difference between these groups, provides further evidence that the PIN vehicle alone has the potential to reduce the influx of blood-derived substances by resealing the ruptured BBB.\n\nSurprisingly, the Free DEXSP group exhibited significantly worse recording performance compared to the negative control (TH group), consistent with findings from previous studies on the long-term therapeutic efficacy of systemic DEX administration for treating neuroinflammation and improving IME electrophysiology recording quality [38, 41]. Chen et al. reported that a single, non-targeted dose of dexamethasone promoted wound healing in septic mice with pathogenic inflammation but delayed wound healing in mice without pathogenic inflammation [83]. This observation may explain the exacerbated neuroinflammation observed in the Free DEXSP group in our study, as healthy rats without pathogenic inflammation were used. The poorer recording performance in the Free DEXSP group suggests the importance of targeted drug delivery. This study demonstrates that targeted delivery using PIN was successfully achieved.\n\nFor the SPPINDEX treatment, in addition to initially disrupting self-perpetuating neuroinflammation by reducing the invasion of foreign substances into the brain parenchyma, dexamethasone sodium phosphate (DEXSP) was potentially released into the brain parenchyma and absorbed by activated microglia near the implant site via the injury-targeted delivery platform (PIN). By binding to the glucocorticoid receptor (GC) on microglia, DEXSP can internalize into cytoplasm, where it binds to the cytokine-activated NF-κB complex (p50 and p65 subunits) and promotes expression of NF-kB inhibitor IκBα. This inhibits the activated NF-κB complex and reduces the expression of proinflammatory cytokines [84–86]. The attenuation of proinflammatory cytokines promotes an anti-inflammatory microenvironment near the implant site, potentially reducing the secondary neuronal damage and astrocytes recruitment, further disrupting the self-perpetuating neuroinflammation induced by IME insertion. This dual disruption of neuroinflammation fosters a less proinflammatory environment, leading to improved neuronal health, increased neuron density, reduced infiltration of activated microglia, and the most significant improvement in neural recording performance compared to all other treatments.\n\nIt is important to note that this study did not assess proinflammatory cytokine levels in brain tissue to investigate the mechanism of SPPINDEX’s therapeutical effects on promoting anti-inflammatory microenvironment near the implant site. This limitation was due to technical challenges in histologically staining extracellular cytokines on formalin-perfused tissues. To address this issue, future studies can focus on using spatial transcriptomics analysis on brain slices to evaluate the neuroinflammatory-specific DNA/RNA expression levels using NanoString for bulk tissue analysis at the microelectrode-tissue interface. Sydney et al. [87] demonstrated the successful evaluation of over 800 neuroinflammatory-specific DNA/RNA expression levels including IL-1B and TNF-alpha, two common proinflammatory cytokines produced by activated microglia.\n\nDexamethasone sodium phosphate is a synthetic glucocorticoid. High dose or long-term administration of DEXSP might develop several side effects such as hyperglycemia and weight loss due to its non-selective action in animals [45]. Additionally, we previously characterized the biodistribution of PINs in the livers and kidneys of rats, raising concerns about potential organ dysfunction with long-term PIN dosing. No significant differences in glucose levels were observed among groups at weeks 0, 4, and 8, indicating that hyperglycemia did not occur in the SPPINDEX group. For normalized animal weights with different treatment over 8 weeks, only the Free DEXSP group showed significantly lower weights compared to the TH group at week 4, suggesting that non-selective Free DEXSP administration may affect weight but not persist in later weeks. There were no significant differences in normalized weight between the SPPINDEX and TH groups, indicating that targeted delivery of DEXSP with PIN may reduce the long-term side effects of DEXSP on body weight compared to Free DEXSP treatment. Alanine transaminase (ALT) levels, a typical enzyme marker for liver function, did not show significant fluctuations among groups. Combined with low levels of creatinine (a kidney waste) among all group, weekly treatments of SPPINDEX, PIN and Free DEXSP didn’t induce dysfunctional liver and kidney. Overall, DEXSP encapsulated in PIN did not significantly impact metabolism, liver and kidney function in rats during the 8-week repeated dosing study, indicating the safety of this treatment approach.\n\nThe clinical translatability of intra-arterial administration is limited due to its unexpected risks, vascular and neural toxicity [88], particularly with repeated weekly dosing. The initial intention to use intra-arterial injection with pre-implanted catheters in this study was to avoid complications such as phlebitis from weekly tail vein injections, which could affect the quality of drug delivery. Future studies will focus on optimizing SPPINDEX dosing by reducing the treatment duration from 8 weeks of weekly administration to 4 weeks while evaluating whether the recording performance can be sustained up to 8 weeks and even 16 weeks, using a larger animal model such as rabbits via intravenous injection. This approach could potentially enhance the clinical translatability of systemic SPPINDEX treatment for reducing neuroinflammation and improving neural recording performance.\n\n# Conclusion\n\nDexamethasone sodium phosphate (DEXSP) is widely used to develop anti-inflammatory therapies aimed at mitigating IME insertion-induced neuroinflammation and enhancing electrophysiological recording performance through either systemic or local delivery, each with its own limitations. Our study demonstrates that treatment with DEXSP-loaded platelet-inspired nanoparticles significantly improves active electrode yield for up to 8 weeks. This enhanced neural recording performance is likely due to the initial prevention of blood-derived protein influx, facilitated by the resealing of the leaky blood-brain barrier (BBB) through the hemostatic function of platelet-inspired nanoparticles. Furthermore, the targeted delivery of DEXSP to the IME implant interface using injury-targeting platelet-inspired nanoparticles further attenuates IME insertion-induced neuroinflammation by disrupting the signaling pathways involved in the neuroinflammatory cascade. The combination of hemostasis-promoting platelet-inspired nanoparticles and targeted delivery of the anti-inflammatory drug DEXSP to the IME implant site significantly reduces neuroinflammation and improves the neural recording performance of IMEs. 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Brown, Complications After Unintentional Intra-arterial Injection of Drugs: Risks, Outcomes, and Management Strategies, 2005. www.mayoclinicproceedings.com783.\n\n# Supplementary Files\n\n- [SupportinginformationLongshunLi01232025.docx](https://assets-eu.researchsquare.com/files/rs-6018202/v1/98e6e93b70872a05b31cb8af.docx) \n Supplementary information\n\n- [GraphicalAbstract.docx](https://assets-eu.researchsquare.com/files/rs-6018202/v1/262f60ded677a0f356d05c0b.docx)"} {"paper_id": "prb52", "title": "Wireless Theranostic Smart Contact Lens for Monitoring and Control of Intraocular Pressure in Glaucoma", "text": "Wireless Theranostic Smart Contact Lens for Monitoring and Control of Intraocular Pressure in Glaucoma\n\nSei Kwang Hahn (skhanb@postech.ac.kr)\nPohang University of Science and Technology https://orcid.org/0000-0002-7718-6259\n\nTaeyeon Kim\nPohang University of Science and Technology\n\nJee Won Mok\nSeoul St. Mary’s Hospital/The Catholic University of Korea\n\nSang Hoon Hong\nPohang University of Science and Technology https://orcid.org/0000-0001-5109-3508\n\nSang Hoon Jeong\nPohang University of Science and Technology\n\nHyeon Sik Choi\nPHI BIOMED Co.\n\nSangbaie Shin\nPHI BIOMED Co.\n\nChoun-Ki Joo\nCK St. Mary’s Eye Center\n\nArticle\n\nKeywords:\n\nPosted Date: April 5th, 2022\n\nDOI: https://doi.org/10.21203/rs.3.rs-1465065/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: There is NO Competing Interest.\n\nVersion of Record: A version of this preprint was published at Nature Communications on November 10th, 2022. See the published version at https://doi.org/10.1038/s41467-022-34597-8.\nWireless Theranostic Smart Contact Lens for Monitoring and Control of Intraocular Pressure in Glaucoma\n\nTae Yeon Kim¹, Jee Won Mok³, Sang Hoon Hong¹, Sang Hoon Jeong¹, Hyeon Sik Choi², Sangbaie Shin², Choun-Ki Joo³ and Sei Kwang Hahn¹,²*\n\n¹ Department of Materials Science and Engineering, Pohang University of Science and Technology (POSTECH), 77 Cheongam-ro, Nam-gu, Pohang, Gyeongbuk 37673, Korea.\n\n² PHI BIOMED Co., #613, 12 Gangnam-daero 65-gil, Seocho-gu, Seoul 06612, Korea.\n\n³ CK St. Mary’s Eye Center, CK building, 559, Gangnam-daero, Seocho-gu, Seoul 06531, Korea.\n\n* CORRESPONDING AUTHOR FOOTNOTE\n\nTel.: +82 54 279 2159; Fax: +82 54 279 2399; E-mail address: skhanb@postech.ac.kr (S. K. Hahn)\nGlaucoma is one of the most menacing irreversible ocular diseases that can cause vision loss in some serious cases. Although Triggerfish has been commercialized for monitoring intraocular pressure (IOP) in glaucoma, there is no smart contact lens to monitor IOP and take appropriate drug treatment in response to the IOP levels. Here, we report a precisely integrated theranostic smart contact lens with a sensitive gold hollow nanowire (AuHNW) based IOP sensor, a flexible drug delivery system (DDS), wireless power and communication systems and an application specific integrated circuit (ASIC) chip for both monitoring and control of IOP in glaucoma. The AuHNW based IOP sensor shows high ocular strain sensitivity, chemical stability and biocompatibility. Furthermore, the flexible DDS can be used for on-demand delivery of timolol for IOP control. Taken together, the IOP levels can be successfully monitored and controlled by the theranostic smart contact lens in glaucoma induced rabbits. This theranostic smart contact lens would be harnessed as a futuristic personal healthcare platform for glaucoma and other ocular diseases.\n\nGlaucoma is a chronic eye disease requiring continuous medical care for patients’ life time. Intraocular pressure (IOP) is the major risk factor that indicates the glaucoma condition and the appropriate IOP control is currently the only available medical care for glaucoma patients [1,2]. The commercial tonometers such as a rebound tonometer and a goldmann applanation tonometer (GAT) have been used for the static IOP measurements in the clinic [3]. However, these measurements generally require clinical training for accurate IOP measurement, and the equipment is generally expensive and uncomfortable for patients in daily use. The conventional static IOP measurement can also cause the critical mismatch of IOP levels according to the measurement time\n[4,5]. Recently, the eye drop solutions are the important first medical treatment for the IOP control of glaucoma patients [6-8]. However, high dose and low bioavailability of eye drops can limit their therapeutic effects and inappropriate drug treatment without considering the IOP condition can cause serious side effects [9]. Furthermore, each patient can have the different therapeutic effect of drugs, which necessitate a different drug dose for each person [10]. Accordingly, it is important to monitor continuous IOP changes in real time and deliver drugs in response to the IOP profiles.\n\nSmart contact lens can provide a new paradigm in glaucoma as an excellent alternative to the conventional management methods with non-invasive, continuous IOP monitoring and on-demand drug deliver [11,12]. In particular, recent smart contact lenses based on strain gauges, resonant, microfluidic and optical systems have attracted great attention for continuous IOP monitoring including Triggerfish which achieved Food and Drug Administration (FDA) approval for the first time. Some of the smart IOP contact lenses have additional functions such as transparency and stretchability [13-15]. Furthermore, drug eluting smart contact lenses can increase bioavailability of drugs in many folds compared to eye drops by prohibiting the washout of drugs by eye blinking and tears [16]. Smart contact lenses with drug complexes [17,18] and micelles [19] have been widely investigated for the treatment of glaucoma. However, theses smart contact lenses still have some challenges for further applications such as low sensitivity, biocompatibility and stability for long-term IOP monitoring without drug delivery functions [13-19].\n\nHere, we report a highly integrated theranostic smart contact lens for both monitoring and control of IOP in glaucoma (Fig. 1a and b). The theranostic smart contact lens comprises of a gold hollow nanowire (AuHNW) based IOP sensor, a flexible drug delivery system (DDS), wireless circuits and a ultra-low power application-specific integrated circuit (ASIC) chip. For the IOP sensor, we synthesized AuHNW to achieve high sensitivity and stability with relatively high transparency for long-term IOP monitoring. Furthermore, the flexible DDS system with a\nbiocompatible protective layer was fabricated for high drug loading efficiency into a smart contact lens. All components were fabricated and highly integrated on-plane of parylene C substrate. The IOP sensor showed high sensitivity with high chemical stability and the flexible DDS could release timolol on-demand by the electrochemical dissolution of gold channels. We assessed the sensitivity of IOP sensor on the artificial eye and drug release efficiency in vitro. In vivo, we performed the demonstration of the theranostic smart contact lens for the successful monitoring and control of IOP in glaucoma animal models.\n\nSynthesis and characterization of AuHNWs\n\nHollow nanomaterials have many unique characteristics compared to bulk nanomaterials [20-24]. In particular, the gold based hollow nanomaterials have been widely used for biomedical applications such as drug delivery [25], photothermal therapy [26], and surface-enhanced Raman scattering (SERS) sensors [27] with their unique optical properties and increased surface area. Here, AuHNW was synthesized by etching Ag core of Ag@Au core-shell nanowire (Ag@AuNW) for high transmittance, sensitivity and chemical stability (Fig. 2a). The hollow structure of AuHNW (shell thickness of ca. 20-30 nm) was confirmed by high resolution transmission electron microscopy (HRTEM) (Fig. 2b). Fig. 2c shows the mapping for the distribution of Ag and Au to further confirm the hollow structure of AuHNW. The Ag core was selectively etched by diluted nitric acid, but the Au shell was not etched making the hollow structure. We compared the optical properties of AuHNW with those of Ag@AuNW. The absorbance peak was shift into near-infrared (NIR) region as synthesized from AgNW to AuHNW (Fig. 2d). Remarkably, the absorbance region of AuHNW was highly reduced in the visible region.\n\nThe optical microscopic (OM) images show the different optical properties in the visible region of Ag@AuNW and AuHNW (Fig. 2e). The nanowire solutions of AgNW, Ag@AuNW and\nAuHNW showed different colors with their different optical properties (Supplementary Fig. 1). The average transmittance of AuHNW was high compared to that of Ag@AuNW in the overall visible region (Fig. 2f), which might be ascribed to that the absorbance peak was shifted into NIR region and reduced in the visible region. The dark field OM images showed two different coated nanowires and each area fraction was analyzed by software program image J (Supplementary Fig. 2a). There were no critical differences in area fractions with two different coated nanowire films (Supplementary Fig. 2b). The transmittance spectra of Ag@AuNW and AuHNW were well matched with our absorbance spectra as we assumed (Supplementary Fig. 2c, d).\n\nWe also investigated the electromechanical properties of AuHNW. AuHNW showed higher sensitivity than Ag@AuNW with a reasonable stretchability of 30% (Fig. 2g). In the scanning electron microscopy (SEM) images, AuHNW maintained the network structure like Ag@AuNW in the film states (Supplementary Fig. 3a). To investigate the effect of Au shell thickness on the electromechanical properties, we synthesized three AuHNWs with different shell conditions by changing the amount of AgNW templates. The shell thickness was decreased with increasing amount of AgNW (Supplementary Fig. 3b). The sensitivity and stretchability of strain sensor were changed according to the different shell thickness (Supplementary Fig. 3c). We optimized the amount of AgNW (50 mg) to synthesize AuHNW for a reasonable stretchability above 30 % (Supplementary Fig. 3d).\n\nFor the characterization of thermoelectrical properties, AuHNW showed smaller resistance change than Ag@AuNW with increasing temperature (Fig. 2h). The temperature coefficient of resistance (TCR) of AuHNW was 0.08 %/°C which was significantly lower than that of Ag@AuNW (0.17). We also investigated the chemical stability of each nanowire in physiological conditions by immersing into hydrogen peroxide (H2O2) (30% in water). Although the absorbance peaks of AgNW and Ag@AuNW were decreased by Ag etching with H2O2 after 2 h, the AuHNW\nshowed no absorbance change (Supplementary Fig. 4a, b and c). The relative resistance change was not significantly changed even in the presence of H2O2 (30% in water) similar to the gold thin film (Fig. 2i). These results confirmed the feasibility of AuHNW for long-term sensitive monitoring of IOP.\n\nFabrication and Characterization of IOP sensor\n\nThe IOP smart contact lens sensor was fabricated in a circular design for monitoring the resistance change caused by the radial deformation of cornea with increasing IOP. The additional layer of poly(3,4-ethylenedioxythiophene):poly(styrenesulfonate) (PEDOT:PSS) incorporating D-sorbitol (D-PEDOT) was included to fill the empty place in micro-patterned AuHNW networks for making a conducting path across individual nanowires. This hybrid structure could preserve the electrical conductivity in the micro-patterned structure. The IOP sensor was patterned by the conventional lift-off process after sequential coating of AuHNW and D-PEDOT (Fig. 3a). The sheet resistance of AuHNW increased 10 times higher than that of Ag@AuNW because of core etching and that of the hybrid sensor slightly decreased because of the D-PEDOT additional layer (Supplementary Fig. 5a). After patterning the hybrid IOP sensor, thermoplastic polyurethane (TPU) was coated on the sensor for passivation, followed by transferring and embedding into smart contact lens. Although the transmittance of hybrid sensor slightly decreased, it still had high transparency (above 84% at 550 nm; Supplementary Fig. 5b). As shown in Fig. 3b, the fabricated IOP sensor embedded into the smart contact lens was also highly transparent. Finally, the hybrid IOP sensor was successfully integrated with gold electrodes for wireless monitoring of IOP (Fig. 3c).\n\nWe optimized the thickness of parylene C and AuHNW coating to improve the sensitivity of IOP sensor. The thick parylene C substrate showed high elastic modulus that could not match with that of the cornea. It was not easily deformed with the curvature change of cornea. Although the\nthin parylene C coating increased the sensitivity of IOP sensor, the thin parylene C could not support the DDS structure [28]. The IOP sensor with thin parylene C showed much higher sensitivity (300 nm and 32 % at 35 mmHg) than that of thick parylene C (1500 nm and less than 1 % at 35 mmHg) (Fig. 3d). AuHNW was spin coated by 5 times to form the electrical path and the IOP sensor was patterned in double line for the successful fabrication in the limited area of smart contact lens. The sensitivity increased 11 to 32 % at 35 mmHg by optimizing coating times and the sensor design. There was high correlation between IOP and relative resistance changes (Fig. 3e). We could also monitor real-time IOP as small as 3 mmHg (Supplementary Fig. 6a) and the repeated IOP fluctuation without any sensitivity change less than ~0.07% (Supplementary Fig. 6b). As shown in Supplementary Fig. 6c, there was no critical hysteresis when the IOP was recovered after increasing to 35 mmHg (less than ~0.14 %). Finally, IOP levels were measured repeatedly from 0 to 35 mmHg to confirm the reliability of sensor. There was no significant difference in the profile of relative resistance change according to IOP changes (Fig. 3f).\n\nFabrication and characterization of flexible DDS\n\nWe designed two different types of DDS for daily and weekly uses (Fig. 4a and b). The flexible DDS was fabricated on the parylene C substrate by depositing gold thin film (thickness of 100 nm) and integrating with the wireless circuits (thickness of 500 nm). The drug reservoirs were fabricated by photolithography of SU-8 with the thickness of 50 \\( \\mu \\)m and loaded with the IOP lowering drug powder of timolol. After that, the biodegradable polymer, poly(vinyl alcohol) (PVA), was coated on the loaded drugs as a protection layer. Finally, the additional parylene C layer (100 nm) was deposited on the DDS for drug sealing. The fabricated DDS was transferred on the supporting substrate and the back side of parylene C was selectively etched by reactive ion etching (RIE) to open the gold channel of DDS. The opened gold channel could be selectively dissolved in the\nphosphate buffered saline (PBS) by applying an electrical voltage of 1.85 V. As shown in Fig. 4c and d, the opened gold channel was fully dissolved by the electrochemical reaction between gold and Cl⁻ in the PBS or physiological fluid according to the following equations: Au + 4H₂O ↔ Au(H₂O)₄³⁺ + 3e⁻ and Au(H₂O)₄³⁺ + 4Cl⁻ ↔ AuCl₄⁻ + 4H₂O [29]. The electrochemical reaction between gold and Cl⁻ was analyzed by measuring the current-time (I-t) curve during the gold dissolution at the constant voltage of 1.85 V. As shown in Supplementary Fig. 7a, gold channels were fully dissolved within 160 s and the operation current was in the range from 5 to 9 μA. Furthermore, the gold channels could be dissolved in the artificial tear in the same manner with that in PBS (Supplementary Fig. 7b). The mechanical bending tests confirmed the flexibility of DDS to be embedded into a smart contact lens. As shown in the I-t curve, the dissolution time of bended DDS was within 140 s and the operation current was ca. 6 μA at the curvature of 6.25 mm (Fig. 4e). Because the curvature of contact lens is generally ca. 8 mm, we confirmed that this DDS was flexible enough to be embedded into the smart contact lens without any critical damages [30,31].\n\nIn order for therapeutic applications, it is important to load a sufficient amount of drug in the limited area of small reservoirs in a smart contact lens [16,29,32]. The drugs were loaded in the powder form to increase the amount of drug loading. The sufficient drugs could be loaded in six reservoirs with 42.78 μg for a daily type and 218.28 μg for a weekly type (Supplementary Fig. 7c). The amount of loaded drug in each type was corresponded to that in the one drop of commercial eye drop (50 μg). The parylene C as a sealing material penetrated into the powder during chemical vapor deposition and made difficult the drug dissolution. To alleviate this problem, biodegradable PVA polymer was introduced as a protection layer. As shown in Fig. 4f, while the timolol release was lower than 50 % without the PVA layer, the drug was fully dissolved out in the presence of PVA. Although the released timolol was less than 5 % without electrical triggering for 90 min,\nabout 85% of the loaded timolol was released out within 5 min and almost all the loaded timolol was fully released out within 30 min (Supplementary Fig. 7d). Three different reservoirs were sequentially activated one by one at 10, 25, and 40 min with 15 min intervals. As shown in Fig. 4g, there was no release of timolol until 10 min, but the release of timolol dramatically increased at each activation time of DDS.\n\nBiosafety of theranostic smart contact lens\n\nA variety of smart contact lenses have been widely investigated with diverse nanomaterials, but the biosafety issues of their nanomaterials have not been fully addressed [33-36]. Especially, silver-based nanomaterials for transparent or stretchable contact lens might damage cells or DNAs by releasing Ag^{+} ions [37]. We conducted live/dead fluorescent staining to assess the biosafety of nanomaterials in the IOP sensor. The cells were directly seeded on the parylene C substrate as a blank control, PEDOS:PSS film incorporated D-sorbitol (D-PEDOT) and AuHNW films for 3 days in an oven at 37 °C. As shown in Fig. 5a, live cells were stained in green and dead cells were in red on the fluorescent optical microscope images. Although almost cells were dead in the case of silver nanowire by the released Ag^{+} ion (less than 15 %), more than 92 % of cells survived in all kinds of materials in the IOP sensor (Fig. 5b). Furthermore, we investigated the temperature change of smart contact lens to assess the thermal biosafety. Finally, we confirmed no corneal damage by wearing smart contact lens (Fig. 5c). There was no inflammation in the cornea (Fig. 5d) and the thickness of cornea was not significantly changed by wearing smart contact lens (Fig. 5e). As shown in Fig. 5f and Supplementary Fig. 8, infrared thermal camera analyses showed no significant temperature increase in the smart contact lens on the rabbit eye during IOP data collection and DDS activation by wireless communication and electrical signaling. All these results revealed the\nbiosafety of our theranostic smart contact lens without critical damage in the glaucoma induced animal models.\n\nIn vivo IOP monitoring and control of theranostic smart contact lens\n\nThe IOP sensor, DDS and wireless circuits, and ASIC chip were integrated and embedded into a smart contact lens. Fig. 6a shows the fully integrated theranostic smart contact lens on the rabbit eye. For the IOP sensing, smart contact lens was designed with a diameter of 7.5 mm for perfect fitting on the rabbit eye (Supplementary Fig. 9). To assess the IOP control of theranostic smart contact lens, glaucoma was induced by injecting methylcellulose (MC) into anterior chamber or α-chymotrypsin (α–chy) into posterior chamber of rabbits. The glaucoma rabbits showed high IOP levels (over 25 mmHg) compared to normal rabbits. (Supplementary Fig. 10). After that, we assessed the theranostic smart contact lens for the IOP control by simultaneous IOP monitoring and on-demand drug delivery (Supplementary Fig. 11a). The rabbits were fixed in the cages and the theranostic smart contact lenses were worn on the rabbit eyes (Supplementary Fig. 11b and c). We previously reported the detailed principle of wireless communication systems [38]. The change of output codes was correlated with the IOP of each rabbit with a different eye size (Supplementary Fig. 12). The recorded output code was 0 mmHg before wearing smart contact lens and the output code was measured at more than two different IOP levels after wearing smart contact lens. The code change (%) by smart contact lens showed high correlation (R^2, more than 0.98) with the IOP (mmHg) by a tonometer. After calibration for this correlation, the measured IOP (mmHg) by the smart contact lens was compared with IOP (mmHg) by the tonometer. As shown in the Fig. 6b, there was a strong correlation between the measured IOP levels by the tonometer and the smart contact lens with a coefficient of determination (R^2) of 0.88, indicating a good intersession reproducibility. Furthermore, Bland-Altman analysis was performed to confirm the agreement of\nIOP measured by the smart contact lens and the tonometer (Supplementary Fig. 13). The limit of agreement (LoA) between the smart contact lens and the tonometer was in the range from -3.16 to 2.90 mmHg with 95 % confidence interval. We monitored the IOP profiles of oculus dextrus (OD) and oculus sinister (OS) eyes of a rabbit for 60 min at 15 min intervals with the smart contact lens and the tonometer (Fig. 6c). The IOP profiles showed the similar trend in each eye.\n\nFig. 6d shows the IOP change with and without the release of timolol from the smart contact lens. The released timolol could reduce ca. 22 % of IOP compared with non-treatment cases. Furthermore, there was no significant difference in the IOP change measured by a smart contact lens and a tonometer regardless of the timolol release. Finally, the IOP level was controlled with the theranostic smart contact lens by monitoring IOP and releasing timolol every other day for 5 days (Fig. 6e). On the first day, because the IOP level was in the high IOP range (above 22 mmHg), timolol was released out to reduce IOP and the IOP was reduced below normal range. On the third day, IOP was still above the normal range and the released timolol could reduce the IOP level near the normal range. On the final day, the IOP level was in the normal range and timolol was not released out from the smart contact lens. All these results confirmed the feasibility of our fully integrated theranostic smart contact lens for monitoring and control of the IOP with the feedback system of an IOP sensor and a DDS for further futuristic glaucoma treatment.\n\nIn vivo therapeutic effect by theranostic smart contact lens\n\nThe therapeutic effect of timolol released from the theranostic smart contact lens was analyzed and compared with that of eye drop (0.5 % Timoptic) in glaucoma induced rabbits. The right eyes of glaucoma rabbits were treated by eye drop every day or timolol released from the smart contact lens every other day for two weeks (Supplementary Fig. 14). The left eyes of glaucoma rabbits were treated with PBS as a negative control. As shown in Supplementary Fig. 15a and 16a, retina\nhistology revealed that the retina thickness was similar with that of normal in both treatment groups. However, the thickness of retina was thin in the case of non-treatment groups. Especially, there were significant differences in ganglion cell layers (GCL) with and without treatment. Furthermore, the inner nuclear layers (INL) of non-treatment groups were unstable and thinned compared to those of normal and treatment groups.\n\nWe also carried out immunohistochemical analyses to further confirm the therapeutic effect of timolol released from smart contact lens. Immunohistochemically stained images showed the significant differences between treatment and non-treatment groups of glaucoma rabbits. The retinal gliosis marker of glial fibrillary acidic protein (GFAP) related to retina damages increased in the case of non-treatment group, but the GFAP expression of treatment groups was similar to that of normal groups (Supplementary Fig. 15b and 16b). Furthermore, CD11b related to optic nerve injury was mainly expressed in glaucoma retina and non-treatment groups (Supplementary Fig. 15c and 16c). The brain-derived neurotrophic factor (BDNF) and the brain-specific hmeobox/POU domain protein 3A (Brn3a) which were related to the retinal ganglion cell marker were highly expressed in normal and treatment groups (Supplementary Fig. 15d, e and 16d, e).\n\nGlaucoma is a chronic eye disease with progressive neuropathy characterized by the death of retinal ganglion cells and the thinning of nerve fiber layers. Taken together, we could confirm the feasibility of our theranostic smart contact lens for prohibiting the progression of glaucoma [39].\n\nDISCUSSION\n\nSmart contact lenses have been developed using a variety of nanomaterials for diagnostic and therapeutic applications. Especially, smart IOP contact lenses were developed with various nanomaterials of graphene [11], AgNW [14] and silicon [12]. In this work, we used AuHNWs with\nsome unique optical and electromechanical properties, and biocompatibility. First, the absorbance region of AuHNW can be shifted into NIR region because of their surface plasmon resonance effect, which can result in high transparency in the visible region. Furthermore, AuHNW with a thin shell is flexible under the applied strain compared to bulk nanowires, which can result in high sensitivity and reasonable stretchability (Supplementary Fig. 17). Although some sensor materials should be passivated due to the biocompatibility and stability issues, AuHNW is highly biocompatible and stable under the physiological condition even without any passivation for further clinical development and applications.\n\nAlthough previous smart IOP contact lenses could continuously monitor IOP, there has been no report on the control of IOP in response to the IOP monitoring. We confirmed that our theranostic smart contact lens could reduce the IOP of glaucoma induced rabbits with different IOP levels (Supplementary Fig. 18). The progression of glaucoma was successfully prohibited with the well-preserved structure of retina. The sufficient amount of drugs could be loaded into the flexible DDS and released on-demand by electrical triggering for the control of IOP. Because glaucoma patients have different drug responses in certain physiological conditions, this feedback system for both monitoring and control of IOP can maximize the compliance of glaucoma patients with the minimized side effect. This futuristic smart contact lens for the personalized IOP control would open a new paradigm in the field of glaucoma.\n\nIn summary, we have here successfully developed a highly integrated smart theranostic contact lens containing a sensitive AuHNW based IOP sensor, a flexible DDS, an ASIC chip, and wireless power and communication systems for both monitoring and control of IOP in glaucoma. A flexible material of AuHNW was synthesized to fabricate a highly sensitive, stable and biosafe IOP sensor for long-term IOP monitoring. The IOP lowering drug of timolol was loaded into the flexible DDS with a biocompatible protection layer, which could be released from the reservoir by electrical\ntriggering for the control of IOP. The biosafety of smart theranostic contact lens was confirmed by live/dead assay of nanomaterials and analyses of corneal damage, corneal thickness change and thermal damage. Furthermore, in vivo experiments in glaucoma induced rabbits confirmed the feasibility of theranostic smart contact lens for both monitoring and control of IOP. Finally, the therapeutic effect of theranostic smart contact lens was successfully demonstrated by the analysis of the retinal structure and four different biomarkers of GFAP, CD11b, BDNF and Brn3a. This theranostic smart contact lens with a feedback system would open a new avenue to the personalized glaucoma treatment.\n\nMETHODS\n\nSynthesis and characterization of AuHNWs\nAuHNWs were synthesized by selective etching of Ag core in 30 % of dilute nitric acid (SAMCHUN). The nitric acid was slowly added into the Ag@AuNW solution at a volume ratio of 1:1. After 1 h, AuHNWs were washed with ethanol and DI water multiple times for further characterization. The structure of AuHNW was investigated by electron energy loss spectroscopy (EELS) equipped high resolution transmission electron microscopy (HRTEM, JEM-2200FS, JEOL). The networks and structures of AuHNW and Ag@AuNW were analyzed by scanning electron microscopy (SEM, MIRA3, TESCAN).\n\nOptical characterization\nFor the characterization of optical transmittance, AuHNW and Ag@AuNW were spin-coated on a parylene C substrate after plasma treatment. For the characterization of absorbance, the synthesized\nnanowires were dispersed into the ethanol. The optical transmittance and absorbance were measured with a UV-vis spectrometer (S-3100, Scinco Co.).\n\nElectrical characterization\n\nFor the characterization of electromechanical properties, nanowire samples were spin coated on polydimethylsiloxane (PDMS). The nanowire films were stretched by customized stretching machine and their resistance changes were measured with a source meter (Keithley 2450).\n\nFabrication of the hybrid IOP sensor\n\nParylene C as a substrate (300 nm) (LAVIDA 110, Femto Science) was deposited on the sacrificial layer. The AZ-nLoF was spin coated on the parylene C and patterned by photolithography for lift-off process. First, Ag@AuNW (1 mg/ml) dispersed in the mixed solution of ethanol and DI water at the volume ratio of 2:5 was spin coated 5 times and annealed at 110 \\(^\\circ\\)C for 2 min. After annealing, the nanowire coated substrate was dipped into nitric acid (30 % in DI water) to etch Ag core for 10 s. The AuHNW film was annealed at 110 \\(^\\circ\\)C for 2 min to fully remove the remaining nitric acid. Before D-PEDOT coating, the AuHNW film was treated with argon plasma (150 W, 2 min). For the D-PEDOT solution, D-sorbitol (20 mg/ml) was added into the PEDOT:PSS solution with stirring for 3 h. The solution of D-PEDOT was spin coated on the AuHNW film and annealed at 110 \\(^\\circ\\)C for 5 min. After that, the photoresist was removed with acetone and carefully washed with isopropyl alcohol (IPA) to prepare the hybrid IOP sensor. TPU (100 mg/ml) was finally spin-coated on the hybrid IOP sensor for passivation. The hybrid IOP sensor was transferred by dissolving PVA and placed into the contact lens mold. The silicone elastomer (MED-6015) was filled and cured at 100 \\(^\\circ\\)C for 1 h to make soft smart contact lens.\nCharacterization of the hybrid IOP sensor\n\nThe artificial eye model was fabricated with the PDMS mixing base and a curing agent at the weight ratio of 20:1 as we previously reported elsewhere [15]. The diameter of artificial eye model was 15 mm with a thickness of 500 μm. Two scalp vein sets were inserted into the artificial eye model to control the pressure of artificial eye model. One was connected to a customized pressure sensor and the other was connected to a syringe pump. After the smart contact lens was placed on the artificial model eye, the pressure of artificial model eye was controlled by injection or ejection of PBS. The resistance change of IOP sensor according to the pressure change was measured with a source meter at a constant voltage of 0.65 V.\n\nFabrication of the flexible DDS\n\nParylene C (300 nm) was deposited on the sacrificial layer. Gold was deposited and patterned on the parylene C with the thickness of 100 nm for the gold channel and 500 nm for the electrode. The SU-8 was spin-coated on the gold channel and electrode to fabricate drug reservoirs. The timolol powder was loaded into reservoirs and the PVA (100 mg/ml) solution as a protection layer was coated on the drugs and dried at room temperature. The additional parylene C layer (100 nm) was deposited to seal the DDS. The DDS was transferred by dissolving the sacrificial layer and the back side of DDS was patterned with a photoresist to selectively etch parylene C. The opened parylene C was selectively etched by RIE (O₂, 100 sccm, 150 W, 5 min) (Covance, Femto Science). The flexible DDS was embedded into a smart contact lens. During molding process, the gold channel and the cathode were open to allow gold dissolution by the electrochemical reaction of gold in the tear.\nCharacterization of the flexible DDS\n\nThe electrochemical reaction of gold was investigated in PBS (pH 7.4) and artificial tear with a constant voltage of 1.85 V *in vitro*. The voltage of 1.85 V was applied to anode and cathode of DDS for 5 min to release timolol from the reservoirs. The concentration of released timolol was quantified with a UV-vis spectrometer at the absorbance wavelength of 259 nm.\n\nFabrication of highly integrated theranostic smart contact lens\n\nFor the precise integration of wireless circuits, an IOP sensor and a DDS, and all other components were sequentially fabricated on the same substrate of parylene C. First, gold with a different thickness was deposited on the substrate and patterned by photolithography for DDS electrode (100 nm) and wireless circuits (500 nm) of an antenna and a chip pad, followed by flip-chip bonding of the ASIC chip. The IOP sensor was fabricated on the same substrate by lift-off process with sequentially coating of AuHNW and D-PEDOT. After that, the parylene C was selectively etched to separate the IOP sensor and wireless circuits by RIE. SU-8 was patterned as drug reservoirs and a protection layer of chip and antenna. The drug of timolol was loaded into the drug reservoirs and the protection layer of PVA was coated on the loaded drugs. TPU was spin coated on the fabricated theranostic system except drug reservoirs. Finally, parylene C (100 nm) was deposited for passivation and sealing the layer. The fabricated theranostic system was transferred by dissolving the sacrificial layer and embedded into the smart contact lens by simple molding.\n\nCell viability and biosafety analysis\n\nTo assess the cell viability and biosafety of nanomaterials, fibroblast cells (NIH 3T3) at a concentration of \\( 5.0 \\times 10^3 \\) cells/ml were directly seeded on the parylene C as a blank substrate, AuHNW, D-PEDOT and AgNW as a control. The concentration of each material was same with\nthat of IOP sensor. After cells on each film were incubated in the cell culture medium, Dulbecco’s modified Eagle medium (DMEM, Thermo Scientific) for 3 days, the cells were stained with calcein AM and ethidium homodimer-1 (EthD-1) in green and red, and observed with a fluorescent optical microscope. The cell viability was quantified by counting live (green) and dead (red) cells on the fluorescent OM images.\n\nIn vivo assessment of theranostic smart contact lens\nTo assess the IOP control capability of theranostic smart contact lens in vivo, the theranostic contact lenses were worn on the right (OD) and left (OS) rabbit’s eyes. For the IOP monitoring, the initial IOP level was measured with a commercialized tonometer and the IOP fluctuation was monitored by wearing smart contact lens. The output codes were collected for 30 min at the interval of 5 min. After 30 min, the smart contact lens was removed from the rabbit’s eye and the IOP was measured with a tonometer again. The output codes were converted into IOP (mmHg) based on our calibration standard curve for each rabbit.\n\nIn vivo therapeutic effects of smart contact lens and eye drop\nThe glaucoma induced rabbits and normal rabbits were divided into 3 groups to assess the therapeutic effects of smart contact lens and eye drop: Glaucoma induced by MC or α-chymotrypsin with eye drop (n = 3, group 1), glaucoma induced by MC or α-chymotrypsin with smart contact lens (n = 3, group 2), and the normal rabbits as a control (n = 3, group 3). After 7 days of glaucoma induction, the treatments were performed on right eyes of rabbits and non-treatments were performed on left eyes of rabbits. The eye drop was treated on the right eyes every day for 16 days except weekends (12 days treatment in total). The timolol (1 reservoir with 38 μg)\nwas delivered from the smart contact lens and treated on the right eyes every other day for 16 days except weekends (7 days treatment in total).\n\nAcknowledgments\n\nThis research was supported by the Basic Science Research Program (2020R1A2C3014070), the Korea Medical Device Development Fund grant (2020M3E5D8105732) and Bio & Medical Technology Development Program (2021M3E5E7021473) of the National Research Foundation (NRF) funded by the Ministry of Science and ICT, Korea.\nReferences\n\n1. Tsai, J. C. & Kanner, E. M. Current and emerging medical therapies for glaucoma. Expert opin. Emerg. Drugs. **10**, 109-118 (2005).\n\n2. Farkouh, A., Frigo, P. & Czejka, M. Systemic side effects of eye drops: a pharmacokinetic perspective. Clin. Ophthalmol. **10**, 2433 (2016).\n\n3. Zhao, J. L. et al. Comparative efficacy and safety of the fixed versus unfixed combination of latanoprost and timolol in Chinese patients with open-angle glaucoma or ocular hypertension. *BMC ophthalmol.* **11**, 1-8 (2011).\n\n4. Goldmann, H. A. N. S. & Schmidt, T. H. Über applanationstonometrie. *Ophthalmologica* **134**, 221-242 (1957).\n\n5. Salvetat, M. L. et al. Comparison of iCare tonometer and Goldmann applanation tonometry in normal corneas and in eyes with automated lamellar and penetrating keratoplasty. *Eye* **25**, 642-650 (2011).\n\n6. Xu, J. et al. Co-delivery of latanoprost and timolol from micelles-laden contact lenses for the treatment of glaucoma. *J. Control. Release* **305**, 18-28 (2019).\n\n7. Maulvi, F. A. et al. In vitro and in vivo evaluation of novel implantation technology in hydrogel contact lenses for controlled drug delivery. *J. Control. Release* **226**, 47-56 (2016).\n\n8. Kim, H. J., Zhang, K., Moore, L. & Ho, D. Diamond nanogel-embedded contact lenses mediate lysozyme-dependent therapeutic release. *ACS nano* **8**, 2998-3005 (2014).\n\n9. Trattler, W., Noecker, R. J. & Earl, M. L. A multicentre evaluation of the effect of patient education on acceptance of hyperaemia associated with bimatoprost therapy for glaucoma or ocular hypertension. *Adv. Ther.* **25**, 179-189 (2008).\n\n10. Shen, J. & Bejanian, M. Effect of preservative removal from fixed-combination bimatoprost/timolol on intraocular pressure lowering: a potential timolol dose–response phenomenon. *Clin. Ophthalmol.* **10**, 373 (2016).\n\n11. Liu, Z. et al. An Ultrasensitive Contact Lens Sensor Based On Self-Assembly Graphene For Continuous Intraocular Pressure Monitoring. *Adv. Funct. Mater.* **31**, 2010991 (2021).\n\n12. Kim, J. et al. A soft and transparent contact lens for the wireless quantitative monitoring of intraocular pressure. *Nat. Biomed. Eng.* **5**, 772-782 (2021).\n\n13. Xu, J. et al. 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Acta Biomater. 86, 350-362 (2019).\n\n19. Mun, J. et al. Drug-eluting contact lens containing cyclosporine-loaded cholesterol-hyaluronate micelles for dry eye syndrome. RSC Adv. 9, 16578-16585 (2019).\n\n20. Lee, J. et al. Targeted hyaluronate–hollow gold nanosphere conjugate for anti-obesity photothermal lipolysis. ACS Biomater. Sci. Eng. 3, 3646-3653 (2017).\n\n21. Qiao, Y. et al. Light-activatable synergistic therapy of drug-resistant bacteria-infected cutaneous chronic wounds and nonhealing keratitis by cupriferous hollow nanoshells. ACS nano 14, 3299-3315 (2020).\n\n22. Zheng, G. et al. Interconnected hollow carbon nanospheres for stable lithium metal anodes. Nat. Nanotechnol. 9, 618-623 (2014).\n\n23. Sun, J. et al. Bioinspired hollow semiconductor nanospheres as photosynthetic nanoparticles. Nat. Commun. 3, 1-7 (2012).\n\n24. Sun, L. et al. Double-shelled hollow rods assembled from nitrogen/sulfur-codoped carbon coated indium oxide nanoparticles as excellent photocatalysts. Nat. Commun. 10, 1-10 (2019).\n\n25. You, J., Zhang, G. & Li, C. Exceptionally high payload of doxorubicin in hollow gold nanospheres for near-infrared light-triggered drug release. ACS nano 4, 1033-1041 (2010).\n\n26. Ren, Y. et al. Sequential co-delivery of miR-21 inhibitor followed by burst release doxorubicin using NIR-responsive hollow gold nanoparticle to enhance anticancer efficacy. J. Control. Release 228, 74-86 (2016).\n\n27. Li, J. et al. A digital single-molecule nanopillar SERS platform for predicting and monitoring immune toxicities in immunotherapy. Nat. Commun. 12, 1-12 (2021).\n\n28. Kim, D.H. et al. Epidermal electronics. Science 333, 838-843 (2011).\n\n29. Han, S. et al. Upconversion nanoparticles coated organic photovoltaics for near infrared light controlled drug delivery systems. Nano Energy 81, 105650 (2021).\n\n30. González-Cavada, J. et al. Base curve influence on the fitting and comfort of the senofilcon A contact lens. J. Optom. 2, 90-93 (2009).\n\n31. Leonardi, M. et al. Wireless contact lens sensor for intraocular pressure monitoring: assessment on enucleated pig eyes. Acta Ophthalmol. 87, 433-437 (2009).\n32. Sung, S. H. et al. Flexible wireless powered drug delivery system for targeted administration on cerebral cortex. Nano Energy **51**, 102-112 (2018).\n\n33. Jang, J. et al. Smart contact lens and transparent heat patch for remote monitoring and therapy of chronic ocular surface inflammation using mobiles. *Sci. Adv.* **7**, eabf7194 (2021).\n\n34. Park, J. et al. Printing of wirelessly rechargeable solid-state supercapacitors for soft, smart contact lenses with continuous operations. *Sci. Adv.* **5**, eaay0764 (2019).\n\n35. Park, J. et al. Soft, smart contact lenses with integrations of wireless circuits, glucose sensors, and displays. *Sci. Adv.* **4**, eaap9841 (2018).\n\n36. Alam, F. et al. Prospects for Additive Manufacturing in Contact Lens Devices. *Adv. Eng. Mater.* **23**, 2000941 (2021).\n\n37. Choi, S. et al. Highly conductive, stretchable and biocompatible Ag–Au core–sheath nanowire composite for wearable and implantable bioelectronics. *Nat. Nanotechnol.* **13**, 1048-1056 (2018).\n\n38. Jeon, C. et al. A smart contact lens controller IC supporting dual-mode telemetry with wireless-powered backscattering LSK and EM-radiated RF transmission using a single-loop antenna. *IEEE J. Solid-State Circuits* **55**, 856-867 (2019).\n\n39. Mwanza, J. C. et al. Glaucoma diagnostic accuracy of ganglion cell-inner plexiform layer thickness: comparison with nerve fiber layer and optic nerve head. *Ophthalmology*, **119**, 1151-1158 (2012).\nFigure 1 | Schematic illustration of a theranostic smart contact lens for glaucoma treatment.\n\na, The structure of theranostic smart contact lens with a fully integrated AuHNW-based IOP senor, a DDS, and wireless circuits for wireless glaucoma treatments with a feedback system for IOP sensing and timolol release. b, Schematic representation of the previous continuous IOP monitoring and the IOP control by IOP monitoring and on-demand drug delivery for the treatment of glaucoma.\nFigure 2 | Characteristics of synthesized AuHNWs. a, Schematic illustration of Ag@AuNW and AuHNW. b, TEM images and c, EELS images of AuHNWs (scale bar, 1 μm and 100 nm). d, The normalized absorbance of AgNW, Ag@AuNW and AuHNW. e, OM images of Ag@AuNW and AuHNW films. f, The average transmittance change of each nanowire with increasing coating times. g, Electromechanical and h, thermoelectrical properties of Ag@AuNW and AuHNW. i, The relative resistance change of nanowires and gold thin film under H2O2 exposure.\nFigure 3 | Characteristics of IOP sensor. a, OM images of patterned IOP sensors. b, Photographic image of an IOP sensor embedded into a smart contact lens (scale bar, 3.5 mm). c, OM image of an integrated IOP sensor and wireless circuits (scale bar, 600 μm). The relative resistance change of IOP sensors with d, different substrate thicknesses and e, coating times and designs. f, The repeated measurement of relative resistance with increasing IOP by using the IOP sensor.\nFigure 4 | Characteristics of flexible DDS. Optical images of a, daily and b, weekly types of theranostic smart contact lenses (scale bar, 7 mm). c, Before and d, after selective electrochemical dissolution of the gold channel in PBS (scale bar, 400 μm). e, I-t curve of flexible DDS with different bending conditions. f, In vitro release of timolol from the flexible DDS. g, The cumulative release of timolol from three different reservoirs.\nFigure 5 | Biosafety assessment of nanomaterials and smart contact lens. a, Fluorescent microscopic images of NIH 3T3 cells after the live/dead assay. b, The relative cell viability of each sample (n = 3, ***P < 0.001) c, Fluorescein staining for corneal damage in rabbit eyes. d, OM images and e, the corneal thickness analysis of glaucoma induced rabbits’ corneas. f, Photo-images for wireless power transmission and communication, and the thermal characterization of theranostic smart contact lens on rabbit’s eye with a control board.\nFigure 6 | In vivo IOP control with a theranostic smart contact lens. a, Photo-image of a fully integrated theranostic smart contact on rabbit’s eye. b, Correlation of IOP measured with a smart contact lens and a tonometer (n = 80, R^2 = 0.88). c, IOP monitoring of right and left eyes with a smart contact lens and a tonometer. d, The IOP change by timolol released from the smart contact lens (n = 25, **P < 0.01). e, The IOP control of the theranostic smart contact lens by simultaneous IOP monitoring and timolol release.\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• NatureBMETheranosticSupplementary.pdf"} {"paper_id": "prb53", "title": "A Taxonomically-informed Mass Spectrometry Search Tool for Microbial Metabolomics Data", "text": "A Taxonomically-informed Mass Spectrometry Search Tool for Microbial Metabolomics Data\n\nPieter Dorrestein ( pdorrestein@health.ucsd.edu )\nUniversity of California San Diego https://orcid.org/0000-0002-3003-1030\n\nSimone Zuffa\nSkaggs School of Pharmacy and Pharmaceutical Sciences University of California San Diego 9500 Gilman Dr. San Diego CA 92093 https://orcid.org/0000-0001-7237-3402\n\nRobin Schmid\nSkaggs School of Pharmacy and Pharmaceutical Sciences University of California San Diego 9500 Gilman Dr. San Diego CA 92093\n\nAnelize Bauermeister\nSkaggs School of Pharmacy and Pharmaceutical Sciences University of California San Diego 9500 Gilman Dr. San Diego CA 92093\n\nPaulo Wender Portal Gomes\nSkaggs School of Pharmacy and Pharmaceutical Sciences https://orcid.org/0000-0001-5478-2448\n\nAndres Caraballo-Rodriguez\nSkaggs School of Pharmacy and Pharmaceutical Sciences University of California San Diego 9500 Gilman Dr. San Diego CA 92093\n\nYasin El Abiead\nSkaggs School of Pharmacy and Pharmaceutical Sciences University of California San Diego 9500 Gilman Dr. San Diego CA 92093\n\nAllegra Aron\nDepartment of Chemistry and Biochemistry University of Denver Denver CO 80210\n\nEmily Gentry\nVirginia Tech https://orcid.org/0000-0002-0016-8132\n\nJasmine Zemlin\nSkaggs School of Pharmacy and Pharmaceutical Sciences University of California San Diego 9500 Gilman Dr. San Diego CA 92093\n\nMichael Meehan\nSkaggs School of Pharmacy and Pharmaceutical Sciences University of California San Diego 9500 Gilman Dr. San Diego CA 92093\n\nNicole Avalon\nScripps Institution of Oceanography University of California San Diego 9500 Gilman Dr. La Jolla CA 92093\n\nRobert Cichewicz\nDepartment of Chemistry and Biochemistry College of Arts and Sciences University of Oklahoma 101 Stephenson Parkway Norman OK 73019\n\nEkaterina Buzun\nUniversity of California San Diego\n\nMarvic Carrillo-Terrazas\nUniversity of California, San Diego\n\nChia-Yun Hsu\nDepartment of Pathology School of Medicine University of California San Diego 9500 Gilman Dr. San Diego CA 92093\n\nRenee Oles\nDepartment of Pathology School of Medicine University of California San Diego 9500 Gilman Dr. San Diego CA 92093\n\nAdriana Vasquez Ayala\nUniversity of California San Diego\n\nJiaqi Zhao\nUniversity of California San Diego\n\nHiutung Chu\nUniversity of California, San Diego\n\nMirte Kuipers\nDepartment of Ecology, Behavior and Evolution School of Biological Sciences University of California San Diego 9500 Gilman Dr. San Diego CA 92093\n\nSara Jackrel\nDepartment of Ecology, Behavior and Evolution School of Biological Sciences University of California San Diego 9500 Gilman Dr. San Diego CA 92093\n\nFidele Tugizimana\nDepartment of Biochemistry Faculty of Science University of Johannesburg Auckland Park Johannesburg Gauteng 2006\n\nLerato Nephali\nDepartment of Biochemistry Faculty of Science University of Johannesburg Auckland Park Johannesburg Gauteng 2006\n\nIan Dubery\nUniversity of Johannesburg https://orcid.org/0000-0002-9079-4769\n\nNtakadzeni Madala\nDepartment of Biochemistry and Microbiology Faculty of Sciences, Agriculture and Engineering University of Venda Private Bag X5050, Thohoyandou Limpopo 950\n\nEduarda Moreira\nDepartment of BioMolecular Sciences School of Pharmaceutical Sciences of Ribeirão Preto University of São Paulo Avenida do Café Ribeirão Preto SP 14040-903\n\nLeticia Costa-Lotufo\nDepartment of Pharmacology Institute of Biomedical Sciences University of São Paulo Av. Lineu Prestes 1524 São Paulo SP 05508-000\n\nNorberto Lopes\nUniversity of Sao Paulo https://orcid.org/0000-0002-8159-3658\n\nPaula Rezende-Teixeira\nDepartment of Pharmacology Institute of Biomedical Sciences University of São Paulo Av. Lineu Prestes 1524 São Paulo SP 05508-000\n\nPaula Jimenez\nDepartment of Marine Science Institute of Marine Science Federal University of São Paulo Rua Carvalho de Mendonça, 144 Santos SP 11070-100\n\nBipin Rimal\nDepartment of Veterinary and Biomedical Sciences Pennsylvania State University 319 Life Sciences Building University Park PA 16802\n\nAndrew Patterson\nPennsylvania State University https://orcid.org/0000-0003-2073-0070\n\nMatthew Traxler\nUniversity of California, Berkeley https://orcid.org/0000-0001-8430-595X\n\nRita de Cassia Pessotti\nPlant and Microbial Biology College of Natural Resources University of California Berkeley 311 Koshland Hall Berkeley CA 94270 https://orcid.org/0000-0003-0805-8613\n\nDaniel Alvarado-Villalobos\nMetabolomics & Chemical Profiling Centro de Investigaciones en Productos Naturales (CIPRONA) Universidad de Costa Rica San Pedro de Montes de Oca San José 2061\n\nGiselle Tamayo-Castillo\nMetabolomics & Chemical Profiling Centro de Investigaciones en Productos Naturales (CIPRONA) Universidad de Costa Rica San Pedro de Montes de Oca San José 2061\n\nPriscila Chaverri\nMicrobial Biotechnology Centro de Investigaciones en Productos Naturales (CIPRONA) & Escuela de Biología Universidad de Costa Rica San Pedro de Montes de Oca San José 2061\n\nEfrain Escudero-Leyva\nMicrobial Biotechnology Centro de Investigaciones en Productos Naturales (CIPRONA) Universidad de Costa Rica San Pedro de Montes de Oca San José 2061\n\nLuis-Manuel Quiros-Guerrero\nSchool of Pharmaceutical Sciences University of Geneva Rue Michel-Servet 1 Genève GE 1206\n\nAlexandre Bory\nSchool of Pharmaceutical Sciences University of Geneva Rue Michel-Servet 1 Genève GE 1206\n\nJuliette Joubert\nSchool of Pharmaceutical Sciences University of Geneva Rue Michel-Servet 1 Genève GE 1206\n\nAdriano Rutz\nSchool of Pharmaceutical Sciences University of Geneva Rue Michel-Servet 1 Genève GE 1206\nJean-Luc Wolfender\nSchool of Pharmaceutical Sciences University of Geneva Rue Michel-Servet 1 Genève GE 1206\nPierre-Marie Allard\nDepartment of Biology University of Fribourg Chemin du Musée, 10 Fribourg FR 1700\nAndreas Sichert\nUniversity of Bremen, Center for Marine Environmental Sciences and Max Planck Institute for Marine Microbiology https://orcid.org/0000-0002-1386-5535\nSammy Pontrelli\nETH Zurich\nBenjamin Pullman\nDepartment of Computer Science and Engineering University of California San Diego 9500 Gilman Dr. San Diego CA 92093\nNuno Bandeira\nDepartment of Computer Science and Engineering University of California San Diego 9500 Gilman Dr. San Diego CA 92093\nWilliam Gerwick\nScripps Institution of Oceanography University of California San Diego 9500 Gilman Dr. San Diego CA 92093\nKatia Gindro\nPlant Protection Mycology group Agroscope Rte de Duillier, 50 Nyon VD 1260\nJosep Massana-Codina\nPlant Protection Mycology group Agroscope Rte de Duillier, 50 Nyon VD 1260\nBerenike Wagner\nDepartment of Microbiology and Organismic Interactions Interfaculty Institute of Microbiology and Infection Medicine University of Tuebingen Auf der Morgenstelle 28 Tuebingen 72076\nKarl Forchhammer\nUniversity of Tubingen https://orcid.org/0000-0003-3199-8101\nDaniel Petras\nCluster of Excellence “Controlling Microbes to Fight Infections” (CMFI) University of Tuebingen Auf der Morgenstelle 24 Tuebingen 72076\nNicole Aiosa\nSchool of Chemistry and Biochemistry Georgia Institute of Technology 950 Atlantic Drive Atlanta GA 30332\nNeha Garg\nSchool of Chemistry and Biochemistry Georgia Institute of Technology 950 Atlantic Drive Atlanta GA 30332\nManuel Liebeke\nMax Planck Institute for Marine Microbiology https://orcid.org/0000-0002-2339-1409\nPatric Bourceau\nDepartment of Symbiosis Metabolic Interactions Max Planck Institute for Marine Microbiology\nCelsiusstrasse 1 Bremen 28359\n\nKyo Bin Kang\nSookmyung Women's University https://orcid.org/0000-0003-3290-1017\n\nHenna Gadhavi\nMycobacterial Metabolism and Antibiotic Research Laboratory The Francis Crick Institute 1 Midland Road London NW1 1AT\n\nLuiz Pedro de Carvalho\nMycobacterial Metabolism and Antibiotic Research Laboratory The Francis Crick Institute 1 Midland Road London NW1 1AT\n\nMariana Silva dos Santos\nMetabolomics Science Technology Platform The Francis Crick Institute 1 Midland Road London NW1 1AT\n\nAlicia Pérez-Lorente\nDepartment of Microbiology Instituto de Hortofruticultura Subtropical y Mediterránea “La Mayora”, Universidad de Málaga-Consejo Superior de Investigacione\n\nCarlos Molina-Santiago\nInstituto de Hortofruticultura Subtropical y Mediterranea, Universidad de Malaga-Consejo Superior de Investigaciones Cientificas (IHSM-UMA-CSIC), Departamento de Microbiologia, Universidad de Malaga https://orcid.org/0000-0002-1131-8917\n\nDiego Romero\nUniversity of Malaga https://orcid.org/0000-0002-2052-6515\n\nRaimo Franke\nDepartment of Chemical Biology Helmholtz Centre for Infection Research Inhoffenstraße 7 Braunschweig 38124\n\nMark Broenstrup\nHelmholtz Centre for Infection Research https://orcid.org/0000-0002-8971-7045\n\nArturo Vera Ponce De Leon\nNorwegian University of Life Sciences (NMBU)\n\nPhillip Pope\nNorwegian University of Life Sciences https://orcid.org/0000-0002-2067-4059\n\nSabina La Rosa\nNorwegian University of Life Sciences (NMBU) https://orcid.org/0000-0003-3527-8101\n\nGiorgia La Barbera\nDepartment of Nutrition, Exercise and Sports University of Copenhagen Rolighedsvej 26 Frederiksberg 1958\n\nHenrik Roager\nUniversity of Copenhagen https://orcid.org/0000-0002-2504-8313\n\nMartin Laursen\nTechnical University of Denmark https://orcid.org/0000-0001-6017-7121\n\nFabian Hammerle\nDepartment of Pharmacognosy Institute of Pharmacy University of Innsbruck Innrain 80-82 Innsbruck 6020\n\nBianka Siewert\nDepartment of Pharmacognosy Institute of Pharmacy University of Innsbruck Innrain 80-82 Innsbruck 6020\n\nUrsula Peintner\nDepartment of Microbiology University of Innsbruck Technikerstr. 25 Innsbruck 6020\n\nCuauhtemoc Licona-Cassani\nEscuela de Ingeniería y Ciencias Centro de Biotecnología FEMSA Tecnologico de Monterrey Av. Eugenio Garza Sada 2501 Monterrey Nuevo Leon 64849\n\nLorena Rodriguez-Orduña\nEscuela de Ingeniería y Ciencias Centro de Biotecnología FEMSA Tecnologico de Monterrey Av. Eugenio Garza Sada 2501 Monterrey Nuevo Leon 64849\n\nEvelyn Rampler\nDepartment of Analytical Chemistry Faculty of Chemistry University of Vienna Waehringer Str. 38 Vienna 1090\n\nFelina Hildebrand\nDepartment of Analytical Chemistry Faculty of Chemistry University of Vienna Waehringer Str. 38 Vienna 1090 https://orcid.org/0000-0002-6946-6744\n\nGunda Koellensperger\nDepartment of Analytical Chemistry Faculty of Chemistry University of Vienna Waehringer Str. 38 Vienna 1090\n\nHarald Schoeny\nDepartment of Analytical Chemistry Faculty of Chemistry University of Vienna Waehringer Str. 38 Vienna 1090\n\nKatharina Hohenwallner\nDepartment of Analytical Chemistry Faculty of Chemistry University of Vienna Waehringer Str. 38 Vienna 1090\n\nLisa Panzenboeck\nDepartment of Analytical Chemistry Faculty of Chemistry University of Vienna Waehringer Str. 38 Vienna 1090\n\nRachel Gregor\nDepartment of Civil and Environmental Engineering School of Engineering Massachusetts Institute of Technology 77 Massachusetts Ave Cambridge MA 2142\n\nEllis O'Neill\nSchool of Chemistry University of Nottingham University Park Nottingham NG72RD\n\nEve Roxborough\nSchool of Chemistry University of Nottingham University Park Nottingham NG72RD\n\nJane Odoi\nFaculty of Engineering University of Nottingham University Park Nottingham NG72RD\n\nNicole Bale\nRoyal Netherlands Institute for Sea Research\n\nSu Ding\nNIOZ Royal Netherlands Institute for Sea Research\n\nJaap S. Sinninghe Damsté\nRoyal Netherlands Institute for Sea Research\n\nXueli Guan\nLee Kong Chian School of Medicine https://orcid.org/0000-0002-5189-8178\n\nJerry Cui\nDepartment of Microbiology College of Arts and Sciences The Ohio State University 484 W. 12th Ave Columbus OH 43210\n\nKou-San Ju\nDepartment of Microbiology College of Arts and Sciences The Ohio State University 484 W. 12th Ave Columbus OH 43210\n\nDenise Silva\nFaculty of Pharmaceutical Sciences, Food and Nutrition Federal University of Mato Grosso do Sul Av. Costa e Silva, s/n Campo Grande MS 79070-900\n\nFemanda Silva\nFaculty of Pharmaceutical Sciences, Food and Nutrition Federal University of Mato Grosso do Sul Av. Costa e Silva, s/n Campo Grande MS 79070-900\n\nGilvan da Silva\nEmbrapa Amazônia Ocidental AM-010 Roadway Manaus AM 69010-970\n\nHector Koolen\nEscola Superior de Ciências da Saúde Universidade do Estado do Amazonas 1777 Carvalho Leal Avenue Manaus AM 69065-001\n\nCarlismari Grundmann\nDepartment of Pharmaceutical Sciences School of Pharmaceutical Sciences of Ribeirão Preto University of São Paulo Avenida do Café Ribeirão Preto SP 14040-903\n\nJason Clement\nBaruch S. Blumberg Institute 3805 Old Easton Rd. Doylestown PA 18902\n\nHosein Mohimani\nCarnegie Mellon University https://orcid.org/0000-0003-3980-2505\n\nKirk Broders\nUSDA-ARS\n\nKerry McPhail\nDepartment of Pharmaceutical Sciences College of Pharmacy Oregon State University Weniger Hall, room 341 Corvallis OR 97331\nSidnee Ober-Singleton\nDepartment of Physics Study of Heavy-Element-Biomaterials University of Oregon 1255 E 13th Ave, Basement Eugene OR 97402\nChristopher Rath\n1480 64th St #300 Emeryville CA 94608\nDaniel McDonald\nDepartment of Pediatrics University of California San Diego 9500 Gilman Dr. San Diego CA 92093\nRob Knight\nDepartment of Pediatrics University of California San Diego 9500 Gilman Dr. San Diego CA 92093\nMingxun Wang\nDepartment of Computer Science and Engineering University of California Riverside 900 University Ave. Riverside CA 92521\n\nBrief Communication\n\nKeywords: metabolomics, microbiome, search tool, bacteria, fungi\n\nPosted Date: August 3rd, 2023\n\nDOI: https://doi.org/10.21203/rs.3.rs-3189768/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: Yes there is potential Competing Interest. PCD is an advisor to Cybele, consulted for MSD animal health in 2023, and he is a Co-founder and scientific advisor for Ometa Labs, Arome, and Enveda with prior approval by UC San Diego. MW is a Co-founder of Ometa labs. There are no known conflicts of interest in this work by the USDA, Agricultural Research Service, National Center for Agricultural Utilization Research, Mycotoxin Prevention and Applied Microbiology Research Unit. Mention of trade names or commercial products in this publication is solely for the purpose of providing specific information and does not imply recommendation or endorsement by the U.S. Department of Agriculture.\n\nVersion of Record: A version of this preprint was published at Nature Microbiology on February 5th, 2024. See the published version at https://doi.org/10.1038/s41564-023-01575-9.\nTitle - A Taxonomically-informed Mass Spectrometry Search Tool for Microbial Metabolomics Data\n\nKey words (5 words) - metabolomics, microbiome, search tool, bacteria, fungi\n\nAuthors list\nSimone Zuffa1,2*, Robin Schmid1,2*, Anelize Bauermeister1,2,3*, Paulo Wender P. Gomes1,2, Andres M. Caraballo-Rodriguez1,2, Yasin El Abied1,2, Allegra T. Aron4, Emily C. Gentry5, Jasmine Zemlin1,6, Michael J. Meehan1, Nicole E. Avalon7, Robert H. Cicchewicz2, Ekaterina Buzun8, Marvic Carrillo Terrazas9, Chia-Yun Hsu9, Renee Oles9, Adriana Vasquez Ayala9, Jiachi Zhao9, Huitung Chu5,10, Mirte C. M. Kuipers11, Sara L. Jackrel11, Fidele Tugizimana12,13, Lerato Pertunia Nephali12, Ian A. Dubery12, Ntakadzeni Edwin Madala14, Eduarda Antunes Moreira15, Letícia Veras Costa-Lotufo16, Norberto Peporine Lopes16, Paula Rezende-Teixeira9, Paula C. Jimenez16, Bipin Rimal17, Andrew D. Patterson18, Matthew F. Traxler19, Rita de Cassia Pessotti19, Daniel Alvarado-Villalobos20, Giselle Tamayo-Castillo20,21, Priscila Chaverri22,23, Efrain Escudero-Levy23, Luis-Manuel Quiros-Guerrero26,27, Alexandre Jean Bory26,27, Juliette Joubert26,27, Adriano Rutz26,27, Jean-Luc Wolfender26,27, Pierre-Marie Allard29,26,27, Andreas Sichert28, Sammy Pontrelli28, Benjamin S Pullman28, Nuno Bandeira28,31, William H. Gerwick31,1, Katia Gindro29, Josep Massana-Codina29, Berenice C. Wagner33, Karl Forchhammer33, Daniel Petras34, Nicole Aiosa35, Neha Garg35,36, Manuel Liebeke37, Patric Bourceau37, Kyu Bin Kang38, Henna Gadhavi39,40, Luiz Pedro Sorio de Carvalho39,41, Mariana Silva dos Santos42, Alicia Isabel Pérez-Lorente43, Carlos Molina-Santiago43, Diego Romero43, Raimo Franke44, Mark Brönstrup44,45, Arturo Vera Ponce de León46, Philip Byron Pope46, Sabina Leanti La Rosa46, Giorgia La Barbera46, Henrik M. Roager48, Martin Frederik Larsen49, Fabian Hammerle50, Bianka Siewert50, Ursula Peintner51, Cuauhtemoc Licona-Cassani52, Lorena Rodriguez-Orduña52, Evelyn Rample53, Felina Hildebrand53,54, Gunda Koellensperger53,55, Harald Schoeny59, Katharina Hohenwallner53,54, Lisa Panzenboeck53,54, Rachel Gregor56, Ellis Charles O'Neill57, Eve Tallulah Roxborough57, Jane Odo138, Nicole J. Bale59, Su Ding59, Jaap S. Sinninghe Damsté59, Xueli Li Guan60, Jerry J. Cul61, Kou-San Ju61,62,63,64, Denise Brentan Silva65, Fernanda Motta Ribeiro Silva65, Gilvan Ferreira da Silva65, Hector H. F. Koolen67, Carlismari Grundmann68, Jason A. Clement69, Hosein Mohimani70, Kirk Broders71, Kerry L. McPhail72, Sidnee E. Ober-Singleton73, Christopher M. Rath74, Daniel McDonald75, Rob Knight75,76, Mingxun Wang77, Pieter C. Dorrestein1,2,*\n\n* These authors equally contributed to this work\n^ Correspondence\n\nEmails and affiliations\n1Skaggs School of Pharmacy and Pharmaceutical Sciences, University of California San Diego, 9500 Gilman Dr., San Diego, CA, 92093, United States, 2Collaborative Mass Spectrometry Innovation Center, Skaggs School of Pharmacy and Pharmaceutical Sciences, University of California San Diego, 9500 Gilman Dr., San Diego, CA, 92093, United States, 3Department of Pharmacology, Institute of Biomedical Sciences, University of São Paulo, Av. Lineu Prestes 1524, São Paulo, SP, 05508-000, Brazil, 4Department of Chemistry and Biochemistry, University of Denver, Denver, CO, 80210, United States, 5Department of Chemistry, Virginia Tech, Blacksburg, VA, 24061, United States, 6Center for Microbiome Innovation, University of California San Diego, 9500 Gilman Dr., San Diego, CA, 92093, United States, 7Scripps Institution of Oceanography, University of California San Diego, 9500 Gilman Dr., La Jolla, CA, 92093, United States, 8Department of Chemistry and Biochemistry, College of Arts and Sciences, University of Oklahoma, 101 Stephenson Parkway, Norman, OK, 73019, United States, 9Department of Pathology, School of Medicine, University of California San Diego, 9500 Gilman Dr., San Diego, CA, 92093, United States, 10Center for Mucosal Immunology, Allergy, and Vaccines (cMAV), Chiba University-University of California San Diego, 9500 Gilman Dr., San Diego, CA, 92093, United States, 11Department of Ecology, Behavior and Evolution, School of Biological Sciences, University of California San Diego, 9500 Gilman Dr., San Diego, CA, 92093, United States, 12Department of Biochemistry, Faculty of Science, University of Johannesburg, Auckland Park, Johannesburg, Gauteng, 2006, South Africa, 13International Research and Development, Omnia Nutriology, Omnia Group (Pty) Ltd, 178 Montecasino Boulevard, Fourways, Johannesburg, Gauteng, 2191, South Africa, 14Department of Biochemistry and Microbiology, Faculty of Sciences, Agriculture and Engineering, University of Venda, Private Bag X5050, Thohoyandou, Limpopo, 950, South Africa, 15Department of BioMolecular Sciences, School of Pharmaceutical Sciences of Ribeirão Preto, University of São Paulo, Avenida do Café, Ribeirão Preto, SP, 14040-903, Brazil, 16Department of Marine Science, Institute of Marine Science, Federal University of São Paulo, Rua Carvalho de Mendonça, 144, Santos, SP, 11070-100, Brazil, 17Department of Veterinary and Biomedical Sciences, Pennsylvania State University, 319 Life Sciences Building, University Park, PA, 16802, United States, 18Department of Veterinary and Biomedical Sciences, Pennsylvania State University, 320 Life Sciences Building, University Park, PA, 16802, United States, 19Plant and Microbial Biology, College of Natural Resources, University of California Berkeley, 311 Koshland Hall, Berkeley, CA, 94270, United States, 20Metabolomics & Chemical Profiling, Centro de Investigaciones en Productos Naturales (CIPRONA), Universidad de Costa Rica, San Pedro de Montes de Oca, San José, 2061, Costa Rica, 21Escuela de Química, Universidad de Costa Rica, San Pedro de Montes de Oca, San José, 2061, Costa Rica, 22Microbial Biotechnology, Centro de Investigaciones en Productos Naturales (CIPRONA) & Escuela de Biología, Universidad de Costa Rica, San Pedro de Montes de Oca, San José, 2061, Costa Rica, 23Escuela de Biología, Universidad de Costa Rica, San Pedro de Montes de Oca, San José, 2061, Costa Rica, 24Department of Natural Sciences, Bowie State University, Bowie, Maryland, 20715, United States, 25Microbial Biotechnology, Centro de Investigaciones en Productos Naturales (CIPRONA), Universidad de Costa Rica, San Pedro de Montes de Oca, San José, 2061, Costa Rica, 26School of Pharmaceutical Sciences, University of Geneva, Rue Michel-Servet 1, Genève, GE, 1206, Switzerland, 27Institute of Pharmaceutical Sciences of Western Switzerland, University of Geneva, Rue Michel-Servet 1, Genève, GE, 1206, Switzerland, 28Institute of Molecular Systems Biology, ETH Zurich, Otto-Stern-Weg 3, Zürich, 8093, Switzerland, 29Department of Biology, University of Fribourg, Chemin du Musée, 10, Fribourg, FR, 1700,\nSwitzerland, 28Department of Computer Science and Engineering, University of California San Diego, 9500 Gilman Dr., San Diego, CA, 92093, United States, 31Scripps Institution of Oceanography, University of California San Diego, 9500 Gilman Dr., San Diego, CA, 92093, United States, 32Plant Protection, Mycology group, Agroscope, Rte de Duillier, 50, Nyon, VD, 1260, Switzerland, 33Department of Microbiology and Organismic Interactions, Interfaculty Institute of Microbiology and Infection Medicine, University of Tuebingen, Auf der Morgenstelle 28, Tuebingen, 72076, Germany, 34Cluster of Excellence “Controlling Microbes to Fight Infections” (CMFI), University of Tuebingen, Auf der Morgenstelle 24, Tuebingen, 72076, Germany, 35School of Chemistry and Biochemistry, Georgia Institute of Technology, 950 Atlantic Drive, Atlanta, GA, 30332, United States, 36Center for Microbial Dynamics and Infection, Georgia Institute of Technology, 311 Ferst Drive, Atlanta, GA, 30332, United States, 37Department of Symbiosis, Metabolic Interactions, Max Planck Institute for Marine Microbiology, Celsiusstrasse 1, Bremen, 28359, Germany, 38Research Institute of Pharmaceutical Sciences, College of Pharmacy, Sookmyung Women’s University, Cheongpa-ro 47 gil 100, Seoul, 04310, Korea, 39Mycobacterial Metabolism and Antibiotic Research Laboratory, The Francis Crick Institute, 1 Midland Road, London, NW1 1AT, UK, 40King’s College London, Strand, London, WC2R 2LS, UK, 41Chemistry Department, The Herbert Wertheim UF Scripps Institute for Biomedical Innovation & Technology, 110 Scripps Way, Jupiter, FL, 33458, United States, 42Metabolomics Science Technology Platform, The Francis Crick Institute, 1 Midland Road, London, NW1 1AT, UK, 43Department of Microbiology, Instituto de Hortofruticultura Subtropical y Mediterránea “La Mayora”, Universidad de Málaga-Consejo Superior de Investigaciones Científicas (IHSUM-UMA-CSIC), Bulevar Louis Pasteur (Campus Universitario de Teatinos), Málaga, Málaga, 29071, Spain, 44Department of Chemical Biology, Helmholtz Centre for Infection Research, Inhoffenstraße 7, Braunschweig, 38124, Germany, 45German Center for Infection Research (DZIF), Site Hannover-Braunschweig, Braunschweig, 38124, Germany, 46Faculty of Chemistry, Biotechnology and Food Science, Norwegian University of Life Sciences, Postboks 5003, Ås, 1433, Norway, 47Faculty of Biosciences, Norwegian University of Life Sciences, Postboks 5003, Ås, 1433, Norway, 48Department of Nutrition, Exercise and Sports, University of Copenhagen, Rolighedsvej 26, Frederiksberg, 1958, Denmark, 49National Food Institute, Technical University of Denmark, Kemitorvet B202, Lyngby, 2800, Denmark, 50Department of Pharmacognosy, Institute of Pharmacy, University of Innsbruck, Innrain 80-82, Innsbruck, 6020, Austria, 51Department of Microbiology, University of Innsbruck, Technikerstr. 25, Innsbruck, 6020, Austria, 52Escuela de Ingeniería y Ciencias, Centro de Biotecnología FEMSA, Tecnológico de Monterrey, Av. Eugenio Garza Sada 2501, Monterrey, Nuevo Leon, 64849, Mexico, 53Department of Analytical Chemistry, Faculty of Chemistry, University of Vienna, Waehringer Str. 38, Vienna, 1090, Austria, 54Vienna Doctoral School in Chemistry (DoSChem), Faculty of Chemistry, University of Vienna, Waehringer Str. 42, Vienna, 1090, Austria, 55Vienna Metabolomics Center (VIME), University of Vienna, Althanstr. 14, Vienna, 1090, Austria, 56Department of Civil and Environmental Engineering, School of Engineering, Massachusetts Institute of Technology, 77 Massachusetts Ave, Cambridge, MA, 02142, United States, 57School of Chemistry, University of Nottingham, University Park, Nottingham, NG72RD, UK, 58Faculty of Engineering, University of Nottingham, University Park, Nottingham, NG72RD, UK, 59Department of Marine Microbiology and Biogeochemistry, Netherlands Institute for Sea Research (NIOZ), Landsdiep 4, t Horntje (Texel), 1797 SZ, Netherlands, 60Lee Kong Chian School of Medicine, Nanyang Technological University, 59 Nanyang Drive, Singapore, Singapore, 639211, Singapore, 61Department of Microbiology, College of Arts and Sciences, The Ohio State University, 484 W. 12th Ave, Columbus, OH, 43210, United States, 62Division of Medicinal Chemistry and Pharmacognosy, College of Pharmacy, The Ohio State University, 484 W. 12th Ave, Columbus, OH, 43210, United States, 63Center for Applied Plant Sciences, The Ohio State University, 484 W. 12th Ave, Columbus, OH, 43210, United States, 64Infectious Diseases Institute, The Ohio State University, 484 W. 12th Ave, Columbus, OH, 43210, United States, 65Faculty of Pharmaceutical Sciences, Food and Nutrition, Federal University of Mato Grosso do Sul, Av. Costa e Silva, s/n, Campo Grande, MS, 79070-900, Brazil, 66Embrapa Amazônia Ocidental, AM-010 Roadway, Manaus, AM, 69010-970, Brazil, 67Escola Superior de Ciências da Saúde, Universidade do Estado do Amazonas, 1777 Carvalho Leal Avenue, Manaus, AM, 69065-001, Brazil, 68Department of Pharmaceutical Sciences, School of Pharmaceutical Sciences of Ribeirão Preto, University of São Paulo, Avenida do Café, Ribeirão Preto, SP, 14040-903, Brazil, 69Baruch S. Blumberg Institute, 3805 Old Easton Rd., Doylestown, PA, 18902, United States, 70Computational Biology Department, School of Computer Science, Carnegie Mellon University, 5000 Forbes Avenue, Pittsburgh, PA, 15213, United States, 71USDA, Agricultural Research Service, National Center for Agricultural Utilization Research, Mycotoxin Prevention and Applied Microbiology Research Unit, 1815 N. University, Peoria, IL, 61604, United States, 72Department of Pharmaceutical Sciences, College of Pharmacy, Oregon State University, Weniger Hall, room 341, Corvallis, OR, 97331, United States, 72Department of Physics, Study of Heavy-Element-Biomaterials, University of Oregon, 1255 E 13th Ave, Basement, Eugene, OR, 97402, United States, 741480 64th St #300, Emeryville, CA, 94608, United States, 75Department of Pediatrics, University of California San Diego, 9500 Gilman Dr., San Diego, CA, 92093, United States, 76Department of Bioengineering, University of California San Diego, 9500 Gilman Dr., San Diego, CA, 92093, United States, 77Department of Computer Science and Engineering, University of California Riverside, 900 University Ave., Riverside, CA, 92521, United States\nAbstract\n\nMicrobeMASST, a taxonomically-informed mass spectrometry (MS) search tool, tackles limited microbial metabolite annotation in untargeted metabolomics experiments. Leveraging a curated database of >60,000 microbial monocultures, users can search known and unknown MS/MS spectra and link them to their respective microbial producers via MS/MS fragmentation patterns. Identification of microbial-derived metabolites and relative producers, without a priori knowledge, will vastly enhance the understanding of microorganisms’ role in ecology and human health.\n\nMain\n\nMicroorganisms drive the global carbon cycle1 and can establish symbiotic relationships with host organisms, influencing their health, aging, and behavior2–6. Microbial populations interact with different ecosystems through the alteration of available metabolite pools and the production of specialized small molecules7,8. The vast genetic potential of these communities is exemplified by human-associated microorganisms, which encode approximately 100 times more genes than the human genome9,10. However, this metabolic potential remains unreflected in modern untargeted metabolomics experiments, where typically <1% of the annotated molecules can be classified as microbial. This problem particularly affects mass spectrometry (MS)-based untargeted metabolomics, a common technique to investigate molecules produced or modified by microorganisms11, which famously struggles with spectral annotation of complex biological samples. This is because the majority of spectral reference libraries are biased towards commercially available or otherwise accessible standards of primary metabolites, drugs, or industrial chemicals. Even when metabolites are annotated, extensive literature searches are required to understand whether these molecules have microbial origins and to identify the respective microbial producers. Public databases, such as KEGG12, MiMeDB13, NPAtlas14, and LOTUS15, can assist in this interpretation, but they are mostly limited to well-established, largely genome-inferred, metabolic models or to fully characterized and published molecular structures. Additionally, while targeted metabolomics efforts aimed at interrogating the gut microbiome mechanistically have been developed16, these focus only on relatively few commercially-available microbial molecules. Hence, the majority of the microbial chemical space remains unknown, despite the continuous expansion of MS reference libraries. To fill this gap, we have developed microbeMASST (https://masst.gnps2.org/microbemasst/), a search tool that leverages public MS repository data to identify the microbial origin of known and unknown metabolites and map them to their microbial producers.\n\nMicrobeMASST is a community-sourced tool that works within the GNPS17 ecosystem. Users can search tandem MS (MS/MS) spectra obtained from their experiments against MS/MS spectra previously detected in other extracts of bacterial, fungal, or archaeal monocultures. No other available resource or tool allows linking uncharacterized MS/MS spectra to characterized microorganisms. The microbeMASST reference database of monocultures has been generated through years of community contributions and metadata curation, and it contains microorganisms isolated from plants, soils, oceans, lakes, fish, terrestrial animals, and humans (Figure 1a). All available microorganisms are categorized according to the NCBI taxonomy18 at different taxonomic resolution (i.e. species, genus, family, etc.) or mapped to the closest taxonomically accurate level, if no NCBI ID was available at the time of database creation. As of June 2023, microbeMASST includes 60,781 liquid chromatography (LC)-MS/MS files, comprising >100 million MS/MS spectra, mapped to 541 strains, 1,336 species, 539 genera, 264 families, 109 orders, 41 classes, and 16 phyla from the three domains of life: Bacteria, Archaea, and Eukaryota (Figure 1b). Differently from MASST19, which uses a precomputed network of ~110 million MS/MS spectra to enable spectral searching, microbeMASST is based on the newly introduced Fast Search Tool (https://fasst.gnps2.org/fastsearch/)20. This tool, originally designed for proteomics, drastically improves search speed by several orders of magnitude by indexing all the\nMS/MS spectra present in GNPS/MassIVE and restricting the search space to the user input parameters. Because of this, search results are returned within seconds as opposed to 20 min per search or 24-48 hours for modification tolerant searches in the original implementation of MASST. Additionally, microbeMASST leverages the pre-curated file-associated metadata to aggregate results into taxonomic trees. This represents a major enhancement over MASST, where users have to manually inspect result tables and contextualize them, making interpretations tedious.\n\nIn microbeMASST, users can search MS/MS spectra using a Universal Spectrum Identifier (USI)21 or by inputting a precursor ion mass and its spectral fragmentation pattern (Supplementary Figure 1). Analogue search can also be enabled to discover molecules related to the MS/MS spectrum of interest across the taxonomic tree17,19,22. The microbeMASST web app displays query results in interactive taxonomic trees, which can be downloaded as HTML files. Nodes in the trees represent specific taxa and display rich information, such as taxon scientific name, NCBI taxonomic ID, number of deposited samples, number of found MS/MS matches, and proportion of found matches, which is also visualized through pie charts. Information for an MS/MS match in a particular taxon is propagated upstream through its lineage. The reactive interface of microbeMASST enables filtering of the tree to specific taxonomic levels or to a minimum number of matches observed per taxon. Additionally, three data tables are generated, linking the search job to other resources in the GNPS/MassIVE ecosystem. Each MS/MS query is searched against the public MS/MS reference library of GNPS (587,213 MS/MS spectra, June 2023). Annotations to such reference compounds are listed under the ‘Library matches’ tab (Supplementary Figure 2a). The ‘Datasets matches’ tab contains information on the matching scans, displaying scientific name, NCBI taxonomic ID and taxonomic rank, number of matching fragment ions, and modified cosine score together with a link to a mirror plot visualization (Supplementary Figure 2b). Finally, the ‘Taxa matches’ tab informs on how many matches were found per taxon and number of samples available for that taxon (Supplementary Figure 2c). Quality controls (QCs) and blank samples (n=2,902) present in the reference datasets of microbeMASST have been retained to provide information on possible contaminants and media components. Additionally, data from human cell line cultures (n=1,199) have been included to enable assessment of whether molecules can be produced by both human hosts and microorganisms.\nFigure 1. The microbeMASST search tool and reference database.\na) Community contributions of data and knowledge to GNPS17, ReDU23, and MassIVE from 2014 to 2022 were used to generate the microbeMASST reference database. Additionally, a public invitation to deposit data in June 2022 resulted in the further deposition of LC-MS/MS files from 25 different laboratories from 15 different countries across the globe, leading to the curation of a total of 60,781 LC-MS/MS files of microbial monoculture extracts. b) MicrobeMASST comprises 1,858 unique lineages, across three different domains of life, mapped to 541 unique strains, 1,336 species, 539 genera, 264 families, 109 orders, 41 classes, and 16 phyla. c) Examples of medically-relevant small molecules known to be produced by bacteria or fungi. Lovastatin, a cholesterol lowering drug originally isolated from Aspergillus genus24, salinosporamide A, a Phase III candidate to treat glioblastoma produced by Salinispora tropica25, and commendamide, a human G-protein–coupled receptor agonist26. d) MicrobeMASST search outputs of the three different molecules of interest confirm that they were exclusively found in monocultures of the only known producers. Pie charts display the proportion of MS/MS matches found in the deposited reference database. Blue indicates a match with a monoculture, while yellow represents a nonmatch. Searches were performed using MS/MS spectra deposited in the GNPS reference library: lovastatin (CCMSLIB00005435737), salinosporamide A (CCMSLIB00010013003), and commendamide (CCMSLIB00004679239).\n\nSearch results for lovastatin, salinosporamide A, and commendamide MS/MS spectra highlight how microbeMASST can correctly connect microbial molecules to their known producers (Figure 1c). In the case of lovastatin, a clinically-used cholesterol-lowering drug originally isolated from Aspergillus terreus24, spectral matches were unique to the genus Aspergillus (Figure 1d). The MS/MS spectrum for salinosporamide A, a Phase III candidate to treat glioblastoma27, only matched two strains of Salinispora tropica (Figure 1d), the only known producer25. Commendamide, first observed in cultures of Bacteroides vulgatus (recently reclassified as Phocaeicola vulgatus), is a G-protein–coupled receptor agonist26. Surprisingly it had many matches to several bacterial cultures, including in Flavobacteriaceae (Algibacter, Lutibacter, Maribacter, Polaribacter, Postechiella, and Winogradskyella) and Bacteroides cultures (Figure 1d). Additional examples include searches of mevastatin, arylomycin A4,\nyersiniabactin, promicroferrioxamine, and the microbial bile acid conjugates\\(^{28-30}\\) glutamate-cholic acid (Glu-CA) and glutamate-deoxycholic acid (Glu-DCA) (**Supplementary Figure 3**). Mevastatin, another cholesterol-lowering drug originally isolated from *Penicillium citrinum*\\(^{31}\\), was only found in samples classified as fungi. The antibiotic arylomycin A4 was observed in different *Streptomyces* species and it was originally isolated from *Streptomyces* sp. Tue 6075 in 2002\\(^{32}\\). Yersiniabactin, a siderophore originally isolated from *Yersinia pestis*\\(^{33}\\), whose monoculture is not yet present in the reference database of microbeMASST, was observed in *Escherichia coli* and *Klebsiella* species, consistent with previous observations\\(^{34,35}\\). Promicroferrioxamine, another siderophore, was observed to match *Micromonospora chokoriensis* and *Streptomyces* species. This molecule was originally isolated from an uncharacterized *Promicromonosporaceae* isolate\\(^{36}\\). The MS/MS spectrum of the gut microbiota-derived Glu-CA, an amidated tri-hydroxylated bile acid, was most frequently observed in cultures of *Bifidobacterium* species, while Glu-DCA was found only in one *Bifidobacterium* strain but also in two *Enterococcus* and *Clostridium* species. None of the aforementioned molecules were found in cultured human cell lines, highlighting the ability of microbeMASST to distinguish MS/MS spectra of molecules that can be exclusively produced by either bacteria or fungi. It is important to acknowledge that MS/MS data generally do not differentiate stereoisomers, but it can nevertheless provide crucial information on molecular families.\n\nMicrobeMASST can be also used to extract microbial information from mass spectrometry-based metabolomics studies without any *a priori* knowledge. To illustrate this, we reprocessed an untargeted metabolomics study comparing germ-free (GF) mice to those harboring microbial communities, also known as specific pathogen-free (SPF) mice\\(^{29}\\) (**Figure 2a**). We extracted 10,047 consensus MS/MS spectra uniquely present in SPF mice and queried them with microbeMASST. A total of 3,262 MS/MS spectra were found to have a microbial match. Of these, 837 were also found in human cell lines and for this reason were removed from further analysis. Among the remaining 2,425 MS/MS spectra, 1,673 were exclusively found in bacteria, 95 in fungi, and 657 in both (**Supplementary Figure 4**). These MS/MS spectra were then processed with SIRIUS\\(^{37}\\) and CANOPUS\\(^{38}\\) to tentatively annotate the metabolites and identify their chemical classes. A file containing all these spectra of interest can be explored and downloaded as .mgf format from GNPS (**see Methods**). To further validate the microbial origin of these MS/MS spectra, we assessed their overlap with data acquired from a different study comparing SPF mice treated with a cocktail of antibiotics to untreated controls\\(^{40}\\). Interestingly, 621 MS/MS spectra were also found in this second dataset and 512 were only present in animals not treated with antibiotics (**Figure 2b**). The distribution of these spectra and their classes across bacterial phyla was visualized using an UpSet plot\\(^{39}\\) (**Figure 2c**). Notably, the majority of the spectra classified as terpenoids were commonly observed across phyla while amino acids and peptides appeared to be more phylum specific. Of these 512 spectra, 23% had a level 2 or 3 annotation\\(^{41}\\), matching against the GNPS reference libraries (**Supplementary Table 1**). These included the recently described amidated microbial bile acids\\(^{19,28-30,42-47}\\), free bile acids originating from the hydrolysis of host derived taurine bile acid conjugates\\(^{48}\\), keto bile acids formed via microbial oxidation of alcohols\\(^{29}\\), N-acyl-lipids belonging to a similar class of metabolites as commendamide\\(^{26}\\) (a microbial N-acyl lipid), di- and tri-peptides seen in microbial digestion of proteins\\(^{49}\\), and soyasapogenol, a byproduct of the microbial digestion of complex saccharides from dietary soyasaponins\\(^{29}\\). Part of the remaining unannotated spectra can be identified as chemical modifications of the above annotated microbial metabolites through spectral similarity obtained from molecular networking (**Supplementary Figure 5**). Based on literature information, the list of annotated MS/MS spectra contained a small number of metabolites traditionally considered to be non-microbial in origin. One interpretation of this finding is that microorganisms are capable of producing metabolites previously described to only be made by mammalian hosts. Notable examples include serotonin\\(^{50}\\), γ-aminobutyric acid (GABA)\\(^{51}\\), and the glycocholic acid\\(^{42,52-54}\\), with microorganisms often being the primary producers of these metabolites in the gut. Additionally, an alternative hypothesis is that microorganisms can also selectively stimulate the production of host metabolites. Other limitations regarding annotations are discussed in **Methods**.\nTo assess if the observations from the mouse models translate to humans, we searched and found that 455 out of the 512 MS/MS spectra of interest matched to public human data (Figure 2d). Interestingly, these spectra were found in both healthy individuals and individuals affected by different health states, including type II diabetes, inflammatory bowel disease (IBD), Alzheimer’s diseases and other conditions. These spectra were most commonly found in stool samples (n=110,973 MS/MS matches) followed by blood, breast milk, and the oral cavity as well as other organs including the brain, skin, vagina, and biofluids, such as cerebrospinal fluid and urine (Figure 2e). These findings support the concept that a significant number of microbial metabolites reach and influence distant organs in the human body35.\n\nWe anticipate microbeMASST will be a key resource to enhance understanding of the role of microbial metabolites across a wide range of ecosystems, including oceans, plants, soils, insects, animals, and humans. This expanding resource will enable the scientific community to gain valuable taxonomic and functional insights into diverse microbial populations. The mass spectrometry community will play a key role in the evolution of this tool in the future through the continued deposition of data associated with novel microbial monocultures and the expansion of spectral reference libraries. Moreover, microbeMASST holds potential for various applications, ranging from aquaculture and agriculture to biotechnology and the study of microbial-mediated human health conditions. By harnessing the power of public data, we can unlock new opportunities for advancements in multiple fields and deepen our understanding of the intricate relationships between microorganisms and their ecosystems.\nFigure 2. MicrobeMASST can identify microbial MS/MS spectra within mouse and human datasets.\na) Workflow to extract microbial MS/MS spectra from biochemical profiles of 29 different tissues and biofluids of SPF mice that are not observed in GF mice29. The MS/MS spectra unique to SPF mice (10,047) were searched with microbeMASST. A total of 3,262 MS/MS spectra had a match; those MS/MS also matching human cell lines were removed, leaving a total of 2,425 putative microbial MS/MS spectra (see Methods to download .mgf file). b) The presence of the 2,425 MS/MS spectra was evaluated in an additional animal study looking at antibiotics usage40. A total of 512 MS/MS spectra, out of the 621 overlapping, was exclusively found in animals not receiving antibiotics. c) UpSet plot of the distribution of the detected MS/MS spectra (512) across bacterial phyla. Terpenoids were more commonly observed across phyla while amino acids and peptides appeared to be more phylum specific d) The 512 MS/MS spectra were searched in human datasets and 455 were found to have a match. These MS/MS spectra were present in both healthy individuals and individuals affected by different diseases. e) Most of the MS/MS spectra (n=411) matched fecal samples (n=110,973 matches), followed by blood, oral cavity, breast milk, urine, and several other organs. Abbreviations: CSF, cerebral spinal fluid; HIV, human immunodeficiency virus; PBI, primary bacterial infectious disease; SD, sleep disorder; AD, Alzheimer’s disease; IS, ischemic stroke; KD, Kawasaki disease; IBD, inflammatory bowel disease; T2D, type II diabetes.\nAcknowledgments\nThis work was carried out through the collaborative microbial metabolite center, which is supported by the National Institutes of Health (NIH) grant U24DK133658, the Alzheimer’s gut project U19AG063744 and BBSRC-NSF award 2152526. We thank Travis Adkins and Lisa McCormick from the USDA ARS Culture Collection for their assistance selecting and providing microbial strains used in this research. This project was supported in part by the U.S. Department of Agriculture, Agricultural Research Service. AMCR and HM were supported by the NIH grant 1DP2GM137413. Research reported in this publication was supported in part by the National Center for Complementary and Integrative Health of the NIH under award number F32AT011475 to NEA. KBK is supported by National Research Foundation of Korea (NRF) grants funded by the Korean Government (MSIT) (NRF-2020R1C1004046, 2022R1A5A2021216, and 2022M3HA2096191). BS is supported by the Austrian Science Fund (FWF) P31915 and KH is financed by the FWF research group program (grant FG3), DP is supported by the German Research Foundation (DFG) CMFI Cluster of Excellence (EXC 2124) and Collaborative Research Center CellMap (TRR 261). AB, EAM, COG, PCJ, LVCL, NPL are supported by The São Paulo Research Foundation - FAPESP #2018/24865-4, #2019/03008-9, #2020/06430-0, #2022/12654-4, #2015/17177-6, #2020/02207-5, #2021/10603-0) and CNPq. CLC received financial support from StrainBiotech and the FEMSA Biotechnology Centre from Tecnológico de Monterrey. LRO received a scholarship from the Mexican National Council of Science and Technology (CONACYT). PCT and WHG are supported by NIH R01 GM107530. NG is supported by the NSF CAREER Award #2047235. NS, SD and JSSD are supported by ERC Horizon 2020 (grant agreement No 694569) and by a Spinoza award to JSSD from NWO. BW is supported by CMFI Cluster of Excellence (EXC 2124). MS is supported by DZIF (Grant no TTU 09.722). AVPD, SLLR, and PP are supported by ERA-NET Corfund project BlueBio (grant agreement no. 311913), Research Council of Norway (300846). HMR, MFL and GLB are supported by Novo Nordisk Foundation (grant NNF19OC0056246, PRIMA—toward Personalized dietary Recommendations based on the Interaction between diet, Microbiome and Abiotic conditions in the gut). HMR is supported by the Independent Research Fund Denmark (MOTILITY; grant no. D171-00066B). ECON is supported by the Nottingham Research Fellowship. AIP1 is supported by FPU (PUV19/02099). MFT and RdCP were supported by R35GM12889. CMS is supported by Juan de la Cierva-Incorporación (UC2018-036923-I) and Proyectos dirigidos por jóvenes investigadores de la Universidad de Málaga (B1-2021_21). DR is supported by Plan Nacional de I+D+i del Ministerio de Ciencia e Innovación (PID2019-107724GB-I00), and Junta de Andalucía (P00_0479). XLG is supported by Nanyang Assistant Professorship. KSJ is supported by NIH R01 GM137135. AS is supported by EMBO fellowship ALTF 996-2021. SP is supported by ETH Zurich Career Seed Fellowship. RG is supported by the Simons Foundation Postdoctoral Fellowship in Marine Microbial Ecology. HC is supported by NIH R01AI167860 and CIFAR. MCT is supported by T32 DK007202 (NIDDK), the National Academies of Sciences, Engineering and Medicine through the Predoctoral Fellowship of the Ford Foundation, and the Howard Hughes Medical Institute (HHMI) Graduate Fellowships grant (GT15123). EEL is supported by VI-Universidad de Costa Rica, Grants numbers C1604 and C0469. PE is supported by VI-Universidad de Costa Rica, Grants numbers C1604 and C0469. U.S. National Science Foundation DBE-1638976. DAV and GTC are supported by VI-Universidad de Costa Rica, Grants numbers C1604 and C0469. KF is supported by CMFI Cluster of Excellence (EXC 2124). HHFK and GFS are supported by Fundação de Amparo à Pesquisa do Estado do Amazonas (FAPEAM). DBS is supported by Fundação de Apoio ao Desenvolvimento do Ensino, Ciência e Tecnologia do Estado de Mato Grosso do Sul - FUNDECT (process number: 71/032.390/2022, FUNDECT number: 311/2022). KLM is supported by NIH / 1R01GM132649. PMA is supported by a swissuniversities Open Research Data grant. MCMK and SLJ are supported by NIH R35GM142938. ADP is supported by NIH U01 DK119702 and S10 OD0021750. ATA was supported by the Betty and Gordon Moore Foundation. ML and PB are supported by the Max Planck Society. Omnia Group Ltd. is duly acknowledged for microbial cultures. BSP and NB were partially supported by NIH 1R01LM013115 and NSF ABI 1759980. RK is supported by NIH DP1AT010885. LPN is supported by Omnia Group Ltd. Shimadzu South Africa Ltd. is gratefully thanked for the analytical support. We thank James MacRae, head of The Metabolomics STP at the Francis Crick Institute for his guidance.\n\nDisclosures\nPCD is an advisor to Cybelle, consulted for MSD animal health in 2023, and he is a Co-founder and scientific advisor for Ometa Labs, Arome, and Enveda with prior approval by UC San Diego. MW is a Co-founder of Ometa labs. There are no known conflicts of interest in this work by the USDA, Agricultural Research Service, National Center for Agricultural Utilization Research, Mycotoxin Prevention and Applied Microbiology Research Unit. Mention of trade names or commercial products in this publication is solely for the purpose of providing specific information and does not imply recommendation or endorsement by the U.S. Department of Agriculture.\n\nAuthor contributions (names given as initials)\nSZ, RS, AB, MW, PCD - Conceptualized the method\nRS, SZ, MW - Developed microbeMASST\nPCD, SZ, AB, PWPG, AMCR, YEA, ATA, ECG, JZ, MJM, NEA, RHC, EB, MCT, CYH, RO, AVA, JZ, HC, MCMK, SJ, FT, LPN, NEM, IAD, EAM, LVCL, NPL, PRT, PCJ, BR, ADP, MFT, RCP, GTC, PC, EEL, DAV, LMQG, JLW, AS, SP, JJ, KG, JMC, PMA, BCW, KF, DP, NA, NG, ML, PB, KBK, AGG, HG, LPSC, MSS, AIP1, CMS, DR, RF, MB, AVPL, PBP, SLLR, GLB, MFL, HMR, AR, BS, FH, AJB, CLC, LRO, ER, FH, GK, HS, KH, LP, RG, ECON, ETR, JO, NJB, SD, XLG, JJC, KSJ, DBS, FMRS, GFS, HHFK, JAC, HM, KB, KLIM, SOS, CMR, and RK Contributed data and curated metadata\nSZ - Generated taxonomic tree and performed analyses\nRS - Developed the tree visualizer for enriched ontologies and output summaries\nBSP, NB - Developed the FAST Search Tool API\nMW - Developed the Fast Search Tool API\nSZ, RS, PCD - Tested microbeMASST\nSZ, RS, PCD - Wrote the manuscript\nAll authors reviewed the manuscript\nReferences\n\n1. 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Reproducible, interactive, scalable and extensible microbiome data science using QIIME 2. Nat. Biotechnol. **37**, 852–857 (2019).\nData and code availability\nData used to generate the reference database of microbeMASST are publicly available at GNPS/MassIVE (https://massive.ucsd.edu/). A list with all the accession numbers (MassIVE IDs) of the studies used to generate this tool is available in Supplementary Table 2. Interactive examples of the MS/MS queries illustrated in Figure 1d and Supplementary Figure 3 can be generated, visualized, and downloaded from the microbeMASST website (https://masst.gnps2.org/microbemasst/). Known molecules already present in the GNPS library (https://library.gnps2.org/) were used to facilitate interpretation and confirm that specific bacterial and fungal molecules were exclusively observed in the respective monocultures.\n\n- Lovastatin - CCMSLIB00005435737\n- Salinosporamide A - CCMSLIB00010013003\n- Commendamide - CCMSLIB00004679239\n- Mevastatin - CCMSLIB00005435644\n- Arylomycin A4 - CCMSLIB0000075066\n- Yersiniabactin - CCMSLIB00005435750\n- Promicroferioxamine - CCMSLIB00005716848\n- Glutamate-cholic acid (Glu-CA) - CCMSLIB00006582258\n- Glutamate-deoxycholic acid (Glu-DCA) - CCMSLIB00006582092\n\nData used to extract MS/MS spectra exclusively present in colonized (SPF) mice is publicly available in GNPS/MassIVE under the accession number MSV000079949. Data used to validate and assess antibiotics effect on microbial MS/MS spectra of interest is available under the accession number MSV000080918. List of datasets with data acquired from human biosamples that presented matches to the putative microbial MS/MS spectra of interest is available in Supplementary Table 3.\n\nThe microbeMASST code to query spectra, create interactive trees, and analyze results is available under open source license on GitHub (https://github.com/robinhschmid/microbe_masst). Code used to generate the microbeMASST web interface can be accessed on GitHub (https://github.com/mwang87/GNPS_MASST). Code used to perform the analysis and generate the figures present in the manuscript can be downloaded from GitHub (https://github.com/simonezuffa/Manuscript_microbeMASST)\n\nData collection and harmonization\nData deposited in GNPS/MassIVE was investigated manually and systematically, using ReDU23 (https://redu.ucsd.edu/), to extract all the publicly available MS/MS files (.mzML or .mzXML formats) acquired from monocultures of bacteria, fungi, archaea, and human cell lines. Only monocultures were included in this search tool to unequivocally associate the production of the detected metabolites to each specific taxon. A total of 60,781 files from 537 different GNPS/MassIVE datasets were selected to be used as a reference database of microbeMASST (Supplementary Table 2). These comprise files deposited in response to our call to the scientific community. Between May and July 2022, 25 different research groups deposited 65 distinct datasets in GNPS/MassIVE, comprising a total of 3,142 unique LC-MS/MS files. This represented a 5.45% increase in publicly available MS/MS data acquired from monocultures in just two months. To qualify as a contributor and be credited as one of the authors, researchers had to deposit high resolution LC-MS/MS data acquired either in positive or negative ionization modes from monocultures of either bacteria, fungi, or archaea. Harmonization of the acquired data and metadata represented a challenge. The NCBI taxonomic database is constantly expanding and evolving and ReDU latest updated (December 2021) does not accommodate the latest deposited taxa. For this reason, an additional metadata file (microbeMASST_metadata_massiveID) was generated specifically for the microbeMASST project and uploaded to the respective GNPS/MassIVE datasets deposited by the collaborators, if the ReDU workflow failed. All the collected information was finally\naggregate in one single .csv file (microbe_masst_table.csv) that can be found on GitHub, which contains: 1) Full MassIVE path of each sample, 2) Filename of each sample reported as its MassIVE ID/file name to avoid presence of duplicated names, 3) MassIVE ID, 4) Taxonomic name of the isolate as reported by the author submitting the associated metadata, 5) Alternative taxonomic name if the provided taxonomic name was incorrect or not present in NCBI, 6) Associated NCBI ID to the taxonomic name or the alternative taxonomic name, when present, 7) Definition if the taxonomic ID was automatically assigned or manually curated, and information if 8) ReDU metadata is available for that specific file and if the file correspond to a 9) Blank or 10) Quality control (QC) rather than an unique biological sample.\n\nUnique taxonomic names and NCBI IDs were extracted from the metadata associated with the selected samples. When metadata was not available and multiple species of bacteria or fungi were present in the same dataset, samples were generically classified as bacteria or fungi. Concordance between taxonomic names and NCBI IDs was checked by blasting taxonomic names against NCBI (https://www.ncbi.nlm.nih.gov/Taxonomy/TaxIdentifier/tax_identifier.cgi) to obtains respective NCBI IDs and updated taxonomic names. Results were manually investigated and missing IDs were recovered using the NCBI browser (https://www.ncbi.nlm.nih.gov/Taxonomy/Browser/wwwtax.cgi). If the taxonomic name was not found in NCBI, most likely because it was not deposited yet, the NCBI of the closest taxon was retrieved and used. For example, the strain Staphylococcus aureus CM05 was unavailable in NCBI and was curated to the species Staphylococcus aureus instead.\n\nTaxonomic tree generation\nThe microbeMASST taxonomic tree was generated using both R 4.2.2 (R Foundation for Statistical Computing) and Python 3.10 (Python Software Foundation). In R, the microbeMASST table was filtered and only unique NCBI IDs were retained (n = 1,834). The classification function from the ‘taxize’ package (v 0.9.100) was used to retrieve the full lineage of each NCBI ID56. Main taxonomic ranks (kingdom to strain) plus subgenus, subspecies, and varieties were kept in order to obtain taxonomic trees with a similar number of nodes per lineage. The list of NCBI IDs of all lineages was then imported in Python, where the ETE3 toolkit was used to generate a comprehensive taxonomic tree based on the provided NCBI IDs57. The generated Newick tree was then converted into JSON format and information such as taxonomic rank, number of samples available was added. Additionally, children nodes for blanks and QCs were created in order to be visualized in the same tree, if observed.\n\nMASST query\nMicrobeMASST web application was built using Dash and Flask open source libraries for Python (https://github.com/mwang87/GNPS_MASST/blob/master/dash_microbemasst.py). The web app can receive as inputs either a USI21 or an MS/MS spectrum (fragment ions and their intensities). Additionally, batch searches can be performed using a customisable python script that can read either a .tsv file containing a list of USIs or a single .mgf spectra file. Through the manuscript we showcase how we were able to search for more than 10,000 MS/MS spectra contained in a single .mgf file (approximately 2 hours run time). After receiving input information, microbeMASST leverages the Fast Search Tool (https://fasst.gnps2.org/fastsearch/) API and the sample-specific associated metadata to generate taxonomic trees. Fast searches are based on indexing all the MS/MS spectra present in GNPS/MassIVE according to the mass and intensity of their precursor ions and then restricting the search to only a set of relevant spectra that have a greater chance to achieve a high spectral similarity (modified cosine score) to the MS/MS of interest. Searches are customizable and default settings are the following: precursor and fragment ion mass tolerances = 0.05, minimum cosine score threshold = 0.7, minimum number of matching fragment ions = 3, and analog search = False. The JSON file of the microbeMASST taxonomic tree is then filtered according to the results and converted into a D3 JavaScript object that can be visualized as an HTML file.\nApplications\nWe envision microbeMASST having several applications. First, we showcase how researchers can investigate single MS/MS spectra, using the web interface, and obtain matching results if their known or unknown MS/MS spectrum was previously observed in any of the microbial monocultures present in the microbeMASST database. Nine small molecules of interest were investigated using MS/MS spectra already deposited in the GNPS reference library (see Data and code availability). Second, we show how microbeMASST can be leveraged to mine for known or unknown microbial metabolites in MS studies. To test this hypothesis, we reprocessed an LC-MS/MS dataset acquired from GF and SPF mice29. A comprehensive molecular network was generated (https://gnps.ucsd.edu/ProteoSAFE/status.jsp?task=893fd89b52dc4c07a29248540f97723). From the obtained job, the qiime2 artifact (qiime2_table.qza), the .mgf file (METABOLOMICS-SNETS-V2-893fd89b-download_clustered_spectra-main.mgf) containing all the captured MS/MS spectra, and the annotation table (METABOLOMICS-SNETS-V2-893fd89b-view_all_annotations_DB-main.tsv) were extracted. The .qza file first converted into a .bim file and then .tsv using QIIME258 to extract the feature table. This was then imported in R where only spectra present in tissues and biofluids of SPF animals were retained (n = 10,047). To add an extra layer of filtering, all MS/MS spectra that had an edge (cosine similarity > 0.7) and a delta parent ion mass +/- 0.02 Da with MS/MS spectra present in GF animals were removed (spectral pairs information is contained in networkedges_selfloop). All the MS/MS spectra were then run in batch using a custom python script of microbeMASST (processing time: ~2 hours, Apple M2 Max, 64GB RAM) to obtain microbial matches. Matching and filtered MS/MS spectra (n = 2,425) were aggregated into a single .mgf file that can be downloaded from GNPS (https://gnps.ucsd.edu/ProteoSAFE/status.jsp?task=aecd30b9fbd43bd8f57b88598a05553). Compound class of each MS/MS spectrum, with parent ion mass < 850 Da, was predicted with SIRIUS37 and CANOPUS38. The 2,425 MS/MS spectra were then searched against the MSV000080918 dataset containing animals treated or not with antibiotics40. Matching and filtered MS/MS spectra (n = 512) were aggregated into a single .mgf file that can be downloaded from GNPS (https://gnps.ucsd.edu/ProteoSAFE/status.jsp?task=c33855fc32c948049331e9730189d5c1). A list of the spectra with putative chemical class classification is available in Supplementary Table 1. Venn diagrams and UpSet plots were generated in R using ‘VennDiagram 1.7.3’, ‘UpSetR 1.4.0’, and ‘ComplexUpset 1.3.3’. Finally, the 512 MS/MS spectra were searched in batch against the GNPS public repository to observe if they were detected in human datasets (Supplementary Table 3)\n\nTechnical limitations\nAnalysis of the results should be considered with these limitations in mind. Molecule detection in microbeMASST is dependent on the availability of specific substrates in the reference monocultures. If the culture lacks the necessary substrates (or any other culture condition) to produce a certain molecule, this molecule will not be detected. Nevertheless, if related substrates are present then a different but related molecule may be produced instead, which can be detected using the analog search. To address this problem, it is crucial for the community to continue to gather data from as many diverse experimental conditions as possible to capture the full range of metabolites produced by different microorganisms. This will help in building the most comprehensive reference database that encompasses diverse microbial metabolic profiles. Isomers and stereoisomers, which are molecules with the same molecular formula but different structural arrangements, often exhibit similar MS/MS spectra. This means that their fragmentation patterns may not provide enough information to distinguish them. Differences in extraction conditions and instrument settings can lead to variations in the obtained MS/MS spectra. For example, the intensity of precursor ions used for fragmentation can impact the resulting spectra. If the precursor ion intensity is low, the fragmented spectrum may lack ions that are present in spectra obtained from high-intensity precursor ions. This may result in \"data leakage\", as the MS/MS spectrum may be missing ions, and leading to the two molecules not being recognized as the same molecule. To partially overcome this more permissive settings can be created. The majority of the data deposited in public repositories, GNPS included, and used in microbeMASST\nwere acquired using positive ionization mode, which limits the observation of molecules that cannot be ionized in positive mode. This means that certain metabolites may be underrepresented or not detected at all. The continuous curation of the microbeMASST reference database involves adding more diverse data in terms of ionization modes to improve the coverage of metabolites. Taxonomic tree was generated using associated NCBI IDs provided by the community. Specimen assignment prior to metabolomic analysis can not be checked by microbeMASST. The majority of the deposited data do not have associated genetic information and even if available, it was not used to build taxonomic tree. Thus, specimen mis-identification is possible. By addressing these challenges and continuously curating the reference database with more comprehensive and diverse data, microbeMASST coverage can be expanded to provide valuable insights into the role of microbiota and to facilitate our understanding of microbial metabolism in diverse ecosystems.\nSupplementary Figures\n\nSupplementary Figure 1. microbeMASST web app\nUsers can access the microbeMASST web app at https://masst.gnps2.org/microbemasst/. They can search for MS/MS spectrum against the microbeMASST reference database by either providing a USI in 'Spectrum USI' or by inputting fragment ions and their intensities and the precursor mass in 'Spectrum Peak' and 'Precursor m/z' respectively. Search parameters, such as parent ion and fragment ions tolerances, cosine threshold, and minimum matching peaks can be modified. Analog search can also be enabled. Finally, to submit a search query users have just to click either on 'Search microbeMASST by USI' or 'Search microbeMASST by Spectrum Peak' based on the information that they have provided. Search jobs can be easily shared by clicking on 'Copy Link'.\nSupplementary Figure 2. Complementary output of microbeMASST\na) The queried MS/MS spectrum is searched against the GNPS libraries and, if matches are found, possible annotations are returned. Information on cosine similarity and number of matching peaks is provided and users can explore the associated GNPS Library Spectrum page and inspect mirror plots.\nb) Information of matching scans in the sample from the different taxa is provided. In addition to cosine similarity score, matching fragments, and the possibility to inspect mirror plots, users can retrieve the MassIVE ascension number of the project together with contact information on who deposited the data.\nc) Number of matches for each taxonomic level are returned. Users can observe how many samples for that specific taxon are part of microbeMASST and see how broadly the molecule is distributed within it (fraction).\nSupplementary Figure 3. Examples of microbeMASST outputs\nAdditional examples of results obtained from searching from mevastatin, arylomycin A4, versiniabactin, promicroferrioxamine, glutamate-cholic acid, and glutamate deoxycholic acid. In all cases the molecules were found in the monocultures of known producers and not in human cell lines, confirming that microbeMASST can be used to search for microbial-derived molecules.\n\nSupplementary Figure 4. Distribution putative microbial metabolites across phyla\na) Of the 2,425 MS/MS spectra that had a match exclusively to microbial monocultures, 1,673 were found only in bacteria, 95 in fungi, and 657 in both. b) Chemical classes were then predicted using SIRIUS and CANOPUS and their distribution across the different phyla was visualized using an Upset plot.\nSupplementary Figure 5. Contextualization of the molecular network\nThe selected 512 MS/MS spectra were mapped back to the full molecular network generated from the data acquired from GF and SPF mice (MSV000079949). Only molecular families containing at least one of the MS/MS spectra of interest were retained and used to generate putative annotations of the unannotated spectra of interest. Each node represents a spectrum (ion), light blue indicates MS/MS of interest while green indicates spectra that were not retained in the performed downstream analysis. Within each node the m/z of the precursor ion is indicated, while on each edge the m/z difference between two connected nodes is reported. a) Ions with precursor mass 318.181 and directly connected to a spectrum annotated as the dipeptide Trp-Phe (m/z 352.144) can be tentatively annotated as Trp-Iso/Leu. b) Ions with precursor mass 423.362 connected to Soyasapogenol C, which can represent a soyasapogenol molecule with a loss of water (delta mass 18.01). Abbreviations: Trp, tryptophan; Phe, phenylalanine; Iso, isoleucine; Leu, leucine.\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• SupplementaryFigure1.ai\n• SupplementaryFigure2.ai\n• SupplementaryFigure3.ai\n• SupplementaryFigure4.ai\n• SupplementaryFigure5.ai\n• SupplementaryTable1.csv\n• SupplementaryTable2.csv\n• SupplementaryTable3.csv"} {"paper_id": "prb54", "title": "Detection of hidden antibiotic resistance through real-time genomics", "text": "Detection of hidden antibiotic resistance through real-time genomics\n\nLara Urban\nlara.h.urban@gmail.com\n\nHelmholtz Munich https://orcid.org/0000-0002-5445-9314\nEla Sauerborn\nHelmholtz Munich\nCarolina Corredor\nTechnical University of Munich\nTim Reska\nHelmholtz Munich\nAlbert Perlas\nHelmholtz Munich\nSamir Vargas da Fonseca Atum\nUniversidade de São Paulo\nNick Goldman\nEMBL-European Bioinformatics Institute https://orcid.org/0000-0001-8486-2211\nNina Wantia\nTechnical University of Munich\nClarissa Prazeres da Costa\nTechnical University of Munich\nEbenezer Foster-Nyarko\nLondon School of Hygiene & Tropical Medicine\n\nBrief Communication\n\nKeywords:\n\nPosted Date: December 5th, 2023\n\nDOI: https://doi.org/10.21203/rs.3.rs-3620416/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\nAdditional Declarations: There is NO Competing Interest.\n\nVersion of Record: A version of this preprint was published at Nature Communications on June 28th, 2024. See the published version at https://doi.org/10.1038/s41467-024-49851-4.\nDetection of hidden antibiotic resistance through real-time genomics\n\nEla Sauerborn1,2,3,4, Carolina Corredor4, Tim Reska1,2,3, Albert Perlas1,2, Samir Vargas da Fonseca Atum5,6, Nick Goldman7, Nina Wantia4, Clarissa Prazeres da Costa4,8,9, Ebenezer Foster-Nyarko10, Lara Urban1,2,3*\n\n1Helmholtz AI, Helmholtz Zentrum Muenchen, Neuherberg, Germany\n2Helmholtz Pioneer Campus, Helmholtz Zentrum Muenchen, Neuherberg, Germany\n3Technical University of Munich, School of Life Sciences, Freising, Germany\n4Institute of Medical Microbiology, Immunology and Hygiene, TUM School of Medicine and Health, Technical University of Munich, Germany\n5Departamento de Química Fundamental, Instituto de Química, Universidade de São Paulo, São Paulo, Brazil\n6Departamento de Bioquímica, Instituto de Química, Universidade de São Paulo, São Paulo, Brazil\n7European Molecular Biology Laboratory, European Bioinformatics Institute (EMBL-EBI), Wellcome Genome Campus, Cambridge, UK\n8Center for Global Health, TUM School of Medicine and Health, Technical University of Munich\n9German Center for Infection Research (DZIF), partner site Munich, Germany\n10Department of Infection Biology, London School of Hygiene & Tropical Medicine, Keppel Street, London, UK\n\n*Corresponding author: lara.h.urban@gmail.com\n\nAbstract\nReal-time genomics through nanopore sequencing holds the promise of fast antibiotic resistance prediction, but concerns remain about its accuracy. We here show that real-time genomics has the potential to improve clinical practice based on a multi-drug resistant Klebsiella pneumoniae bloodstream infection. In contrast to established diagnostics, real-time genomics can accurately identify complex antibiotic resistance patterns conferred through newly discovered low-abundance resistance genes, potentially significantly impacting clinical decision-making and patient outcome.\n\nMain\nThe World Health Organization has declared antibiotic resistance one of the ten most severe global health threats¹, with resistant infections leading to higher mortality and morbidity due to delayed or inappropriate therapy². The rapid and accurate identification of resistant bacterial pathogens could improve patient outcomes by facilitating the earlier administration of appropriate therapy. Real-time genomics through nanopore sequencing technology has the potential of speeding up pathogen and antibiotic resistance profiling in the clinical setting³ (Figure 1). The combination of real-time analysis and the technology’s portability for in situ data creation allows for cost-efficient adaptive application, where as much genomic data as necessary can be obtained to reach minimum certainty thresholds in timely, clinically relevant predictions⁴. Long nanopore sequencing reads can further be leveraged to\ncreate highly accurate, near-complete genome assemblies for strain-level identification and de novo detection of bacterial pathogens and their antibiotic resistance profiles\\(^5\\). This is especially relevant for complex infections where clinically established methods for taxonomic bacterial identification (*e.g.*, MALDI-TOF MS) and resistance profiling (*e.g.*, VITEK2; **Methods; Figure 1**) can lack resolution and where rapid targeted therapy can be particularly beneficial. However, concerns remain about the accuracy of real-time genomics for phenotypic antibiotic resistance prediction in comparison to established diagnostic approaches. We here showcase the potential power of *in situ* real-time genomics in the clinical setting through the example of a *Klebsiella pneumoniae* infection that harbors a newly discovered antibiotic resistance gene in low abundance.\n\n![Workflow overview of real-time genomic (top) and clinically established (bottom) diagnostic approaches for pathogen species identification and antibiotic resistance profiling.](page_374_682_1097_377.png)\n\nFigure 1. Workflow overview of real-time genomic (*top*) and clinically established (*bottom*) diagnostic approaches for pathogen species identification and antibiotic resistance profiling. After incubation and primary pathogen identification, pure bacterial isolates are recovered through sub-culturing, followed by pathogen and resistance profiling of the isolates. While the clinically established workflow can take up to 52 hours after subculturing, the real-time genomic workflow delivers first data after ~1.5 hours and can be employed in an adaptive manner to create the necessary amount of data.\n\nBriefly, an immunocompromised patient presented with fever at the University Hospital rechts der Isar in Germany, and was initially treated with the carbapenem Meropenem (**Figure 2**). Clinically established diagnostic approaches detected a carbapenem-resistant *K. pneumoniae* isolate in an endotracheal aspirate with KPC (*K. pneumoniae* carbapenemase) as the putative resistance-conferring mechanism (**Figure 2; Methods**). As such KPC-producing bacteria have become a significant resistance burden due to their ability to hydrolyze a variety of beta-lactam antibiotics including carbapenems\\(^6\\), Ceftazidime-Avibactam (CAZ-AVI) has been introduced as a new treatment option\\(^7\\). Accordingly, CAZ-AVI was administered to our patient and susceptibility was confirmed by additional phenotypic testing (**Figure 2; Methods**). After initial clinical improvement, the patient deteriorated under CAZ-AVI\ntherapy, and subsequent blood cultures grew a K. pneumoniae isolate which was now susceptible to carbapenems but resistant to CAZ-AVI. While new KPC-variants conferring resistance to CAZ-AVI are known to have emerged^{8–10}, no carbapenemase could be identified in our post-treatment isolate using clinically established approaches and Meropenem was additionally administered. However, the patient passed away shortly after (Figure 2).\n\n![Overview of the course and treatment of the infection case. The patient was firstly treated with Meropenem. Bacterial isolates of the first positive patient sample (endotracheal aspirate) were subjected to VITEK2 for general resistance testing and additional tests for CAZ-AVI resistance and KPC detection (R: resistant; S: susceptible; KPC+/-: absence or presence of KPC; Methods); the respective results led to a change in the antibiotic treatment to CAZ-AVI after three days. After clinical deterioration, the second positive patient sample (blood culture) showed reversed antibiotic resistance test results. While Meropenem was subsequently administered, the patient passed away shortly after. We used real-time genomics to sequence DNA from the pre- and post-CAZ-AVI treatment isolates using the portable nanopore sequencing device Mk1b. Both isolates were sequenced for 15 hours, and the first isolate was sequenced for another 20 hours to simulate the potential adaptive sequencing in the clinical setting.](page_347_629_1057_496.png)\n\nFigure 2. Overview of the course and treatment of the infection case. The patient was firstly treated with Meropenem. Bacterial isolates of the first positive patient sample (endotracheal aspirate) were subjected to VITEK2 for general resistance testing and additional tests for CAZ-AVI resistance and KPC detection (R: resistant; S: susceptible; KPC+/-: absence or presence of KPC; Methods); the respective results led to a change in the antibiotic treatment to CAZ-AVI after three days. After clinical deterioration, the second positive patient sample (blood culture) showed reversed antibiotic resistance test results. While Meropenem was subsequently administered, the patient passed away shortly after. We used real-time genomics to sequence DNA from the pre- and post-CAZ-AVI treatment isolates using the portable nanopore sequencing device Mk1b. Both isolates were sequenced for 15 hours, and the first isolate was sequenced for another 20 hours to simulate the potential adaptive sequencing in the clinical setting.\n\nWe simulated the retrospective clinical application of real-time genomics for antibiotic resistance prediction for this infection case as follows: We applied nanopore shotgun sequencing (Oxford Nanopore Technologies) to both K. pneumoniae isolates (pre- and post-CAZ-AVI treatment) by using the portable Mk1b sequencing device, rapid barcoding library preparation, and R9 nanopore\nchemistry (Figure 2; Methods). We processed the raw nanopore data using high-accuracy Guppy basecalling and flye, minimap2, and Racon for de novo genome assembly and polishing. We used EPI2ME WIMP for species classification, and EPI2ME Antimicrobial Resistance’s protein homolog model for antibiotic resistance predictions11 (Supplementary Figure 1; Methods). We additionally simulated the adaptive application of real-time genomics in the clinic, where the same patient sample can be sequenced as long as necessary to obtain more data and certainty on resistance predictions. We here sequenced the pre-treatment isolate for additional 20 hours (Figure 2; Methods).\n\nUsing this real-time genomic data, we correctly identified K. pneumoniae as the dominant pathogen in the pre- and post-treatment isolates. In the pre-treatment isolate, we detected the presence of accurate (> 90%) KPC-2 gene copies (n=40; Table 1), confirming the phenotypic Meropenem resistance (Figure 2)12. In the post-treatment isolate, we detected many copies of the KPC-14 gene (n=44; Table 1), which had previously been described as one of the few KPC subtypes that confer CAZ-AVI resistance and carbapenem susceptibility9. The genomics-based resistance prediction therefore accurately predicted the phenotypic antibiotic resistance, and it additionally identified KPC-14 as the putative resistance-conferring mechanism (Figure 1).\n\nOur real-time genomics approach importantly also detected one copy of the KPC-14 resistance gene in the pre-treatment isolate; while this one copy would have been too little evidence to predict phenotypic CAZ-AVI resistance, our simulation of the adaptive application of real-time genomics in the clinic showed us that less than 20 hours of additional sequencing would have resulted in the detection of four more highly accurate copies of KPC-14 (Table 1). The second KPC-14 gene copy would have already been detected after two hoursof additional sequencing and could have rapidly influenced antibiotic treatment through the early detection of CAZ-AVI resistance potential (Supplementary Figure 2; Methods).\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Sequencing runMeropenemCeftazidime-Avibactam
PredictionEvidenceAccuracyCNPredictionEvidenceAccuracyCN
Pre-treatment 15hRKPC-293.7%40R?92.6%1
+20hR94.4%147R96.3%4
Post-treatment 15hS///R93.4%44
\n\nWe further analyzed our de novo assemblies using the Pathogenwatch12 platform which enables clustering of core-genome multilocus sequence types, and serves as a reference for complex K.\npneumoniae lineages (Methods). We found that the pre- and post-treatment isolates consisted of the same emerging high-risk sequence type ST147\\(^{15}\\). Functional annotation of the assembled plasmid genomes using BugSeq\\(^{16}\\) revealed that KPC-2 and KPC-14 were both located on IncN plasmids, which showed 99.7% identity according to sequence alignments (Supplementary Figure 3; Methods). These results suggest that the observed change in antibiotic resistance might have been caused by a complex infection of the same *K. pneumoniae* lineage with a low-abundance KPC-14-carrying IncN plasmid which became dominant due to its evolutionary selective advantage under CAZ-AVI exposure. Our genomic analyses further showed that we had actually discovered a new KPC resistance gene, KPC-159, that is very similar to the KPC-14 gene detected by our analysis (amino acid sequence similarity of 99.9%) and therefore conferred the same phenotypic antibiotic resistance (Methods).\n\nThe application of real-time genomics to this patient’s case indicates the profound potential of real-time genomics for rapidly and accurately profiling complex bacterial infections in the clinical setting. Our findings show that nanopore sequencing could have detected the phenotypically hidden CAZ-AVI resistance, which would have directly impacted antibiotic therapy, such as through the early administration of alternative antibiotics or combination therapy\\(^{17}\\). Further, the genomics-based identification of a KPC gene as the underlying CAZ-AVI resistance mechanism would have directly informed clinical infection prevention protocols to reduce the risk of between- and within-patient KPC transmission. The fast, adaptive, and *in situ* nature of antibiotic resistance profiling by nanopore sequencing would have therefore surpassed current clinical practice in accurately informing clinical management. Importantly, we could leverage our genomic data to trace the change in antibiotic resistance back to low copy-number plasmid variation in the patient’s original infection. The presence of multiple plasmids in an infection is a general public health hazard since it can accelerate the emergence of resistance when exposed to selection pressures\\(^{18,19}\\). This has previously been described as an underlying mechanism of the fast emergence of CAZ-AVI-resistance under CAZ-AVI exposure\\(^{19}\\). Given the expected high rate of antibiotic resistance emergence in the future, the demonstrated insufficiency of clinically established resistance detection approaches to accurately assess complex infections could pose a significant threat to efficient antibiotic treatment.\n\nWhile genomics-based predictions might not be able to replace phenotypic resistance assertions, we anticipate great potential of combining the advantages of phenotypic with real-time genomic technology for antibiotic resistance profiling in the clinical setting. We further envision that the low upfront investment requirements of nanopore sequencing could provide guidance on antibiotic\ntherapy globally, especially in low- and middle-income settings where expensive machinery for standard clinical diagnostics are likely to not be accessible in the foreseeable future.\n\nReferences\n1. EClinicalMedicine. Antimicrobial resistance: a top ten global public health threat. EClinicalMedicine **41**, 101221 (2021).\n2. Murray, C. J. L. *et al.* Global burden of bacterial antimicrobial resistance in 2019: a systematic analysis. *The Lancet* **399**, 629–655 (2022).\n3. Taxyt, A. M., Avershina, E., Frye, S. A., Naseer, U. & Ahmad, R. Rapid identification of pathogens, antibiotic resistance genes and plasmids in blood cultures by nanopore sequencing. *Sci Rep* **10**, 7622 (2020).\n4. Bloomfield, M. *et al.* Oxford nanopore next generation sequencing in a front-line clinical microbiology laboratory without on-site bioinformaticians. *Pathology* (2023)\n5. Foster-Nyarko, E. *et al.* Nanopore-only assemblies for genomic surveillance of the global priority drug-resistant pathogen, Klebsiella pneumoniae. *Microb Genom* **9**, (2023).\n6. Hammoudi Halat, D. & Ayoub Moubareck, C. The Current burden of Carbapenemases: Review of significant properties and dissemination among Gram-negative bacteria. *Antibiotics* **9**, 186 (2020).\n7. Lahiri, S. D. *et al.* Avibactam and Class C β-Lactamases: Mechanism of inhibition, conservation of the binding pocket, and implications for resistance. *Antimicrob Agents Chemother* **58**, 5704–5713 (2014).\n8. Wu, Y. *et al.* Identification of a KPC variant conferring resistance to Ceftazidime-Avibactam from ST11 Carbapenem-resistant Klebsiella pneumoniae strains. *Microbiol Spectr* **10**, (2022).\n9. Niu, S. *et al.* A Ceftazidime-Avibactam-resistant and Carbapenem-susceptible Klebsiella pneumoniae strain harboring bla *kpc-14* Isolated in New York City. *mSphere* **5**, (2020).\n10. Shi, Q. *et al.* Multiple Novel Ceftazidime-Avibactam-resistant variants of *bla kpc-2*-positive Klebsiella pneumoniae in two patients. *Microbiol Spectr* **10**, (2022).\n11. Alcock, B. P. *et al.* CARD 2023: expanded curation, support for machine learning, and resistome prediction at the Comprehensive Antibiotic Resistance Database. *Nucleic Acids Res* **51**, D690–D699 (2023).\n12. Mehta, S. C. *et al.* KPC-2 β-lactamase enables carbapenem antibiotic resistance through fast deacylation of the covalent intermediate. *Journal of Biological Chemistry* **296**, 100155 (2021).\n13. Argimón, S. *et al.* Rapid genomic characterization and global surveillance of Klebsiella using Pathogenwatch. *Clinical Infectious Diseases* **73**, S325–S335 (2021).\n14. Lam, M. M. C. *et al.* A genomic surveillance framework and genotyping tool for Klebsiella pneumoniae and its related species complex. *Nat Commun* **12**, 4188 (2021).\n15. Peirano, G., Chen, L., Kreiswirth, B. N. & Pitout, J. D. D. Emerging antimicrobial-resistant high-risk Klebsiella pneumoniae clones ST307 and ST147. *Antimicrob Agents Chemother* **64**, (2020).\n16. Chandrakumar, I. *et al.* BugSplit enables genome-resolved metagenomics through highly accurate taxonomic binning of metagenomic assemblies. *Commun Biol* **5**, 151 (2022).\n17. Lombardo, D., Ambretti, S., Lazzarotto, T. & Gaibani, P. In vitro activity of imipenem-relebactam against KPC-producing Klebsiella pneumoniae resistant to ceftazidime-avibactam and/or meropenem-vaborbactam. *Clinical Microbiology and Infection* **28**, 749–751 (2022).\n18. Diaz Caballero, J. *et al.* Mixed strain pathogen populations accelerate the evolution of antibiotic resistance in patients. *Nat Commun* **14**, 4083 (2023).\n19. Bianco, G., Boattini, M., Iannaccone, M., Cavallo, R. & Costa, C. Bloodstream infection by two subpopulations of *Klebsiella pneumoniae* ST1685 carrying KPC-33 or KPC-14 following ceftazidime/avibactam treatment: considerations regarding acquired heteroresistance and choice of carbapenemase detection assay. *Journal of Antimicrobial Chemotherapy* **75**, 3075–3076 (2020).\nMethods\n\nClinically established species identification and antibiotic susceptibility testing\n\nThe clinically established microbiological workflow consisted of plating out clinical samples on BD® Columbia Blood and MacConkey agar plates (Beck Dickinson GmbH, Heidelberg, Germany), which were then incubated for approximately 16-24 hours. For blood cultures or mixed cultures, as was the case in the endotracheal aspirate, a subculturing step was added, after which species identification was done from one colony forming unit (CFU) of pure bacterial cultures using Matrix-assisted laser desorption ionization time-of-flight mass spectrometry instructions (MALDI-TOF MS, Bruker Daltonics GmbH, Leipzig Germany) according to the manufacturer’s instructions. Antibiotic susceptibility testing was performed using VITEK2 (BioMérieux, Marcy l’Etoile, France). For this, up to three bacterial CFUs were transferred to a saline tube to generate a homogenous suspension with a density equivalent to 0.5 McFarland. Subsequently, Minimum Inhibitory Concentrations (MICs in mg/L) of the two isolates were measured and interpreted with the VITEK2 gram-negative (AST-GN69) card according EUCAST (European Committee on Antimicrobial Susceptibility Testing) guidelines20 (**Supplementary Table 1**). Of note, the AST-GN69 card does not detect the presence of carbapenemases or measure MICs for Ceftazidime-Avibactam (CAZ-AVI). Thus, for isolates with antibiotic susceptibility profiles indicative of carbapenem resistance, we identified carbapenemases with a multiplex immunochromatography assay consisting of lateral flow assays (O.K.N.V.I Resist-521). This test detects the presence of Oxa-48, NDM, VIM, IMP-carbapenemases and the most prevalent KPC subtypes (namely, the subtypes KPC-2, KPC-3, KPC-4) in a bacterial isolate21. In addition, the CAZ-AVI MIC was measured with the Liofilchem® MIC test strip (MTS™) (LIOFILCHEM s.r.l., Roseto degli Abruzzi, Italy). The test strip contains Ceftazidime concentrations ranging from 0,016-256 ug/ml with a fixed Avibactam concentration of 4ug/ml. Similar to the VITEK2 MIC measurements, up to three bacterial CFUs were transferred to a sterile saline tube to form a homogenised suspension with a density equivalent to 0.5 McFarland. This solution was then plated out on a BD® Muller Hinton Agar using sterile cotton-tipped swabs and incubated with a Ceftazidime-Avibactam Liofilchem® MTS™ for 16 hours. Again, MICs were interpreted following EUCAST guidelines (**Supplementary Table 1**). After completion of the phenotypic processing, the isolates were stored at -80°C.\nSupplementary Table 1. MIC measurements with VITEK2 and Liofilchem® MIC test strip for CAZ-AVI. The colouring scheme indicates the interpretation of MICs according to EUCAST guidelines (green: susceptible/intermediate; red: resistant).\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
AntibioticPre-treatment isolate MIC (mg/L)Post-treatment isolate MIC (mg/L)
Ampicillin>32>32
Ampicillin-Sulbactam>32>32
Piperacillin>128>128
Piperacillin-Tazobactam>128>128
Cefuroxime>64>64
Cefotaxime>64>64
Ceftriaxone>64>64
Ceftazidime>64>64
Imipenem>161
Meropenem>162
Ertapenem>8>8
Gentamicin>16>16
Ciprofloxacin>4>4
Ceftazidime-Avibactam2>256
\n\nNanopore sequencing workflow for species identification and resistance prediction\n\nThe stored isolates were thawed and grown overnight at 37°C on BD® Columbia blood agar plates. In the first round of sequencing, we isolated DNA from circa 10 CFUs of the pre-, and post-treatment samples using an automated magnetic-bead-based DNA purification approach with the Maxwell® RSC Blood DNA extraction protocol for gram-negative bacteria with the Promega Maxwell®RSC 48 Instrument (Promega Corporation, Madison, USA). DNA concentrations were measured with the Qubit™ (Thermo Fischer Scientific, Waltham, USA) dsDNA HS kit according to the manufacturer’s instructions. Nanopore libraries were generated using the SQK-RBK004 Rapid Barcoding Kit and sequenced on an Oxford Nanopore Technologies MinION MK1b device with R9.4.1 flow cells for 15 hours as previously described22, attaching one barcode per sample. The pore scan at the beginning of the sequencing run detected 781 pores with 378 remaining after the sequencing run was completed (MinKNOW version 22.10.5). For the second round of sequencing of the pre-treatment isolate, we increased the number of CFUs for DNA extraction to circa 50 and sequenced the extracted DNA for 20 hours on a new R.9.4.1 flow cell, maximising sequencing depth and coverage (Supplementary Table 2; Supplementary Figure 1). For this round of sequencing, 1651 pores were detected at the start and 1129 at the end of sequencing.\nSupplementary Table 2. Real-time genomic sequencing and assembly metrics before and after treatment with CAZ-AVI. Genomic material of each bacterial isolate was sequenced for 15 hours; the pre-treatment isolate was additionally sequenced for a further 20 hours to simulate adaptive sequencing in the clinical setting.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Genomic sequencing and assembly metricsPre-treatment samplePost-treatment sample
15h+20h15h
Median read quality (Phred)12.313.012.3
Median read length [kb]4.15.34.5
Total number of bases [Mb]4421,551194
Assembly coverage (median)6827130
Number of contigs (>50 kb)555
Contig N50 [Mb]5.25.25.3
\n\nFor both sequencing rounds, fast5 files were basecalled with Guppy v6.3.2 using the “High-accuracy” model (r9.4.1_450bps_hac)23, resulting in fastq files for each read. We then used Porechop version 0.2.3 (https://github.com/rrwick/Porechop) to trim the adapters and filtered out low-quality reads with a threshold quality score of 9 and short reads (<200b) with Nanofilt version 2.8.0 (https://github.com/wdecoster/nanofilt). Sequencing summaries were generated for each barcode using NanoStat v1.6.0 (https://github.com/wdecoster/nanostat24). We identified resistance-conferring genetic patterns with the EPI2ME Fastq Antimicrobial Resistance (v2023.04.26–1808834) workflow. This workflow includes quality control of the filtered and trimmed nanopore reads, taxa identification by the WIMP (What's in My Pot; v2023.06.13-1865548) workflow based on the NCBI RefSeq database and Centrifuge25 to then analyse classified nanopore reads for resistance genes using The Comprehensive Antibiotic Resistance Database (CARD, https://card.mcmaster.ca/home, accessed 14. May 202326). We then retained resistance gene matches identified via the protein homolog model, which is the most conservative model of the Fastq Antimicrobial Resistance workflow26. Additionally, we chose to only include respective KPC-2 and KPC-14 resistance genes with detection accuracies above 90% to minimise the chances of false positive resistance gene detection.\nSupplementary Figure 1. Bioinformatic workflow for species identification and antibiotic resistance prediction from nanopore sequencing data of pre- and post-treatment isolates (HAC: High-accuracy basecalling; ID: Identification; cgMLST: core genome Multi-Locus Sequence Typing).\n\nTo make inferences on KPC-14 copy number detection over time, we further matched the KPC-14 alignments provided by the Fastq Antimicrobial Resistance workflow to the timepoints of the corresponding reads in the filtered and trimmed fastq file (Supplementary Figure 2).\nSupplementary Figure 2. Timeline of KPC-14 copy number detection during simulation of adaptive sequencing in the clinical setting applied to the pre-treatment bacterial isolate. The run started with one KPC-14 copy number which was obtained in the first sequencing run of the pre-treatment isolate. The second KPC-14 copy was found after two hours, and all additional KPC-14 copies were detected within the first seven hours of sequencing.\n\nCore genome multi-locus sequence typing and chromosome/plasmid alignment analysis\n\nWe assembled the reads into contigs to prepare for core genome multi-locus sequence typing (cgMLST), which is a more stringent method for strain-level detection tailored to whole genome sequencing data compared to the seven locus MLST scheme\\(^{27,28}\\). In line with previous benchmarking studies for nanopore-only assemblies\\(^{22,29}\\), we assembled the bacterial genome using the nano-corr option from Flye v2.9.1 (https://github.com/fenderglass/Flye). To further increase the accuracy of our assemblies, we realigned the reads to the assembled contigs using Minimap2 v2.18\\(^{30}\\) followed by three polishing rounds with Racon 1.5 (https://github.com/isovic/racon, Supplementary Figure 1). Assembly sequencing depth was assessed with SAMTools depth v. 1.18 (https://github.com/samtools/samtools) after converting the polished contigs to sorted BAM files. We analyzed our *de novo* assemblies using the Pathogenwatch v2.3.1\\(^{28}\\) platform which integrates Kleborate\\(^{27}\\), facilitating *Klebsiella* species complex assignments, along with the identification of acquired virulence factors and recognized resistance markers, including both acquired genes and chromosomal mutations. Additionally, Pathogenwatch implements the Life Identification Number (LIN) code scheme, which enables sublineage and clonal groups assignment based on cgMLST profile comparisons\\(^{28}\\). Both isolates had a virulence score of 0/5 according to the Kleborate platform.\nFor more insight into the plasmid structures, we visualised the chromosomal and plasmid genome assemblies (Supplementary Figure 3) using Bandage v0.90 (https://github.com/rrwick/Bandage). Additionally, we uploaded the sequencing reads to BugSeq (https://bugseq.com/academic) for automated functional annotation of the plasmid genomes including resistance gene detection against a curated plasmid database31. Here, the IncN plasmid was identified as the carrier of the KPC-2 and KPC-14 genes respectively. To assess similarity between the IncN plasmids and the KPC-2 and KPC-14 genes on the plasmids, we aligned the respective IncN plasmids against each other, as well as the KPC gene sequences to the respective plasmids using the local alignment tool blastn provided by NCBI (https://www.ncbi.nlm.nih.gov; BLAST v2.14.1+).\n\n![Genome and plasmid de novo assemblies and respective contig lengths. The K. pneumoniae chromosome is highlighted in red and the IncN plasmid is highlighted by the blue square. Additional circular and non-circular accessory genomes are visualised in green, brown, and grey. A. Pre-treatment sample. B. Post-treatment sample.](page_355_678_1042_377.png)\n\nSupplementary Figure 3. Genome and plasmid de novo assemblies and respective contig lengths. The K. pneumoniae chromosome is highlighted in red and the IncN plasmid is highlighted by the blue square. Additional circular and non-circular accessory genomes are visualised in green, brown, and grey. A. Pre-treatment sample. B. Post-treatment sample.\n\nReference Center annotation of novel KPC variant\n\nUpon submission of the post-treatment bacterial isolate to the German National Reference Center for Gram-Negative Bacteria (https://memiserf.medmikro.ruhr-uni-bochum.de/nrz), the KPC resistance gene that our workflow defined as KPC-14 was identified as a previously unseen KPC and named KPC-159 (NCBI sequence ID: OQ450354.1). Using blastn, we confirmed that this KPC-159 gene shows 99.9% overlap in protein sequence (875/876 amino acids) with KPC-14,.\nData availability\nAll FAST5 nanopore sequencing data has been uploaded to NCBI (https://www.ncbi.nlm.nih.gov, SRA submission: SUB13974279).\n\nCode availability\nAll computational scripts for processing the FAST5 data are available here:\nhttps://github.com/Genomics4OneHealth/Klebsiella_pneumoniae_KPC_nanopore_sequencing\n\nReferences\n20. The European Committee on Antimicrobial Susceptibility Testing. Breakpoint tables for interpretation of MICs and zone diameters, version 13.1, 2023. [Internet]. [cited 2023 Oct 4]. Available from: https://www.eucast.org/clinical_breakpoints.\n21. Hong, J., Kang, D. & Kim, D. Performance Evaluation of the Newly Developed In Vitro Rapid Diagnostic Test for Detecting OXA-48-Like, KPC-, NDM-, VIM- and IMP-Type Carbapenemases: The RESIST-5 O.K.N.V.I. Multiplex Lateral Flow Assay. Antibiotics 10, 460 (2021).\n22. Wick, R. R., Judd, L. M., Gorrie, C. L. & Holt, K. E. Completing bacterial genome assemblies with multiplex MinION sequencing. Microb Genom 3, (2017).\n23. Oxford Nanopore Technologies, Guppy v6.3.2. [cited 2023 Oct 4]. Available from: https://github.com/nanoporetech/pyguppyclient.\n24. De Coster, W., D’Hert, S., Schultz, D. T., Cruts, M. & Van Broeckhoven, C. NanoPack: visualizing and processing long-read sequencing data. Bioinformatics 34, 2666–2669 (2018).\n25. Kim, D., Song, L., Breitwieser, F. P. & Salzberg, S. L. Centrifuge: rapid and sensitive classification of metagenomic sequences. Genome Res 26, 1721–1729 (2016).\n26. Alcock, B. P. et al. CARD 2023: expanded curation, support for machine learning, and resistome prediction at the Comprehensive Antibiotic Resistance Database. Nucleic Acids Res 51, D690–D699 (2023).\n27. Lam, M. M. C. et al. A genomic surveillance framework and genotyping tool for Klebsiella pneumoniae and its related species complex. Nat Commun 12, 4188 (2021).\n28. Argimón, S. et al. Rapid Genomic Characterization and Global Surveillance of Klebsiella Using Pathogenwatch. Clinical Infectious Diseases 73, S325–S335 (2021).\n29. Foster-Nyarko, E. et al. Nanopore-only assemblies for genomic surveillance of the global priority drug-resistant pathogen, Klebsiella pneumoniae. Microb Genom 9, (2023).\n30. Li, H. Minimap2: pairwise alignment for nucleotide sequences. Bioinformatics 34, 3094–3100 (2018).\n31. Chandrakumar, I. et al. BugSplit enables genome-resolved metagenomics through highly accurate taxonomic binning of metagenomic assemblies. Commun Biol 5, 151 (2022).\n\nAcknowledgements\nWe thank the laboratory technicians, especially Jacqueline Meindl, and physicians at the Institute of Medical Microbiology at the Technical University Munich for their support with phenotypic species identification, susceptibility testing, and sample storage and retrieval. We thank Sam Chorlton for helpful discussions on the BugSeq platform. We thank Niels Pfennigwerth from the German National Reference Center for Gram-Negative Bacteria for his work on identifying the novel KPC-159 subtype. We thank Dr. Youssef Hamway for his help with laboratory work and conceptualization of the study. This project was funded by a Helmholtz Principal Investigator Grant awarded to LU.\nContributions\nLU and ES conceptualised the project. ES, LU and EFN designed the experiments. ES, TR, and AP conducted the real-time sequencing experiments under LU’s supervision. ES, TR, and SV conducted the bioinformatic analysis including data curation, formal analysis, and visualisation, under LU’s and EFN’s supervision. NG consulted on genomic data analysis and interpretation. NW and CC supervised the clinical case and the phenotypic testing. CPC and NW provided samples and laboratory equipment. ES and LU wrote the manuscript with input from all co-authors.\n\nCompeting interests.\nWe declare no competing interests.\n\nAuthors information and affiliation\nHelmholtz AI, Helmholtz Zentrum Muenchen, Neuherberg, Germany\nHelmholtz Pioneer Campus, Helmholtz Zentrum Muenchen, Neuherberg, Germany\n Dr. Lara Urban, Ela Sauerborn, Tim Reska, Dr. Albert Perlas\n\nTechnical University of Munich, School of Life Sciences, Freising, Germany\n Dr. Lara Urban, Ela Sauerborn, Tim Reska\n\nInstitute of Medical Microbiology, Immunology and Hygiene, Technical University of Munich, Germany\n Ela Sauerborn, Carolina Corredor, Dr. Nina Wantia, Dr. Clarissa da Costa\n\nDepartamento de Química Fundamental, Instituto de Química, Universidade de São Paulo, São Paulo, Brazil\nDepartamento de Bioquímica, Instituto de Química, Universidade de São Paulo, São Paulo, Brazil\n Samir Vargas\n\nEuropean Molecular Biology Laboratory, European Bioinformatics Institute (EMBL-EBI), Wellcome Genome Campus, Cambridge, UK\n Dr. Nick Goldman\n\nCenter for Global Health, TUM School of Medicine and Health, Technical University of Munich\nGerman Center for Infection Research (DZIF), partner site Munich\n Dr. Clarissa Prazeres da Costa\n\nDepartment of Infection Biology, London School of Hygiene & Tropical Medicine, Keppel Street, London, UK\n Dr. Ebenezer Foster-Nyarko\n\nEthics declarations\nEthical approval was given by the ethics committee of the Technical University of Munich, Germany (2023-575-W-NP, 2022-611-S-KH). Informed patient consent was waived as samples were taken under routine diagnostics. The research conformed to the principles of the Helsinki Declaration."} {"paper_id": "prb55", "title": "Mass-spectrometry-based proteomics enables rapid and accurate diagnosis of Lyme neuroborreliosis in adults", "text": "# Abstract\n\nLyme neuroborreliosis (LNB), a severe nervous system infection caused by tick-borne spirochetes of the *Borrelia burgdorferi* sensu lato complex, represents one of the most frequent bacterial infections of the nervous system in Europe. Early diagnosis remains challenging due to limited sensitivity of current methods and requires invasive lumbar punctures, underscoring the need for improved, less invasive diagnostic tools.\n\nHere, we applied mass spectrometry-based proteomics to analyse 308 cerebrospinal fluid (CSF) samples and 207 plasma samples from patients with LNB, viral meningitis, controls and other manifestations of Lyme borreliosis. Diagnostic panels of regulated proteins were identified and evaluated through machine learning-assisted proteome analyses.\n\nIn CSF, the classifier distinguished LNB from viral meningitis and controls with AUCs of 0.92 and 0.90, respectively. In plasma, LNB was distinguished from controls with an AUC of 0.80.\n\nOur findings highlight the diagnostic potential of machine learning-assisted proteomics for LNB in CSF and plasma.\n\nHealth sciences/Health care/Diagnosis/Laboratory techniques and procedures \nHealth sciences/Diseases/Infectious diseases/Bacterial infection \nTick-Borne Diseases \nBorrelia \nLyme Borreliosis \nLyme Disease \nLyme Neuroborreliosis \nCentral Nervous System Infections \nMeningitis \nViral \nDelayed Diagnosis \nDiagnostic Techniques and Procedures \nProteomics \nMachine Learning\n\n# INTRODUCTION\n\nLyme neuroborreliosis (LNB) is a bacterial infection of the nervous system caused by spirochetes of the *Borrelia burgdorferi* sensu lato (*B. burgdorferi* s.l.) complex transmitted through bites from hard-shelled ticks of the *Ixodes* genus1. With an approximate incidence in endemic countries between 3.2 and 6.3 per 100 000 persons/year2–4, LNB is among the most frequent bacterial infections of the nervous system in Europe5,6. LNB can cause a wide range of clinical neurological conditions, but most frequently presents as a subacute painful meningo-radiculitis with radiating pain from the spine to neck, extremities, thorax or abdomen, lymphocytic meningitis and/or cranial neuropathies e.g., facial nerve palsy7. If relevant antibiotic therapy is administered at an early stage of disease, LNB has a favourable long-term prognosis8–10. However, delayed treatment is associated with an increased risk of residual symptoms and long-term sequelae9. In countries where LNB is endemic, the average time from onset of neurological symptoms to diagnosis is typically around 3 weeks and has remained unchanged for the last four decades6.\n\nThe cause of the diagnostic delay is multifactorial. Overlapping symptomatology with other more common diseases and the fact that only around 40% of patients with LNB report a tick bite and only 25% report a history of the classic skin rash erythema migrans makes it less likely that physicians and patients consider LNB as a differential diagnosis, especially in the absence of facial nerve palsy6,8.\n\nHowever, even when LNB is clinically suspected at an early stage, the diagnosis requires detection of *B. burgdorferi* s.l.- specific antibodies in the cerebrospinal fluid (CSF). Lumbar puncture is an uncomfortable and expensive procedure that may require hospitalization and general anesthesia for children. Direct pathogen identification of *B. burgdorferi* s.l. with polymerase chain reaction (PCR), cultivation or a combination has retained an exceedingly poor level of sensitivity both in blood and CSF despite several attempts to improve tools and techniques over the years11–14. Further, the serological response in LNB is not detectable early in the course of disease and antibodies may remain elevated for months to several years after full recovery of well-treated infections making it impossible to discriminate between past and current infection. Furthermore, the *B. burgdorferi* s.l.-specific IgG and IgM in blood, poorly predict nervous system involvement15.\n\nThus, in order to reduce the diagnostic delay in LNB, the need for novel diagnostic tools is evident. Especially improved blood-based diagnostic tests would be extremely valuable as they would both potentially help reduce the diagnostic delay and offer a less invasive diagnostic tool.\n\nUntargeted proteomic analysis enables accurate measurement of proteins in a sample and can be used to compare patterns of protein regulation in patients with and without disease to identify disease-specific protein response signatures16. When combined with machine-learning (ML) for data-evaluation and analysis, proteomic test results can be made available with turnaround times of just 2 hours making it highly attractive in real-life clinical settings.\n\nThe aim of this study was to explore the potential of ML-assisted MS-based proteomics as a novel diagnostic tool for LNB in CSF and plasma of adults.\n\n# RESULTS\n\n## Study population\n\nA total of 483 CSF and plasma samples from adult individuals were eligible for proteomics analysis: 155 samples from patients with LNB, 127 samples from patients with viral meningitis, 169 controls and 32 samples from patients with erythema migrans, acrodermatitis chronica atrophicans and post-treatment-Lyme-disease-syndrome (Table 1).\n\n**Table 1** Baseline characteristics of patients with Lyme neuroborreliosis, viral meningitis, controls, and other Lyme borreliosis manifestations.\n\n| Cohort | Diagnosis | n | Age Mean [IQR] | Females n (%) |\n|--------|-----------|----|----------------|----------------|\n| CSF Development | Lyme neuroborreliosis | 49 | 51[40-66] | 26 (53) |\n| N = 145 | Viral meningitis | 44 | 38[27-42] | 21 (47) |\n| | Control | 52 | 36[25-42] | 17 (32) |\n| CSF Validation | Lyme neuroborreliosis | 69 | 53[46-67] | 28 (40) |\n| N = 163 | Viral meningitis | 45 | 31[25-37] | 23 (51) |\n| | Control | 49 | 44[33-53] | 24 (48) |\n| Plasma Development | Lyme neuroborreliosis | 27 | 64[61-69] | 10 (37) |\n| N = 95 | Viral meningitis | 20 | 35[27-38] | 13 (65) |\n| | Control | 48 | 46[33-60] | 28 (58) |\n| Plasma Validation | Lyme neuroborreliosis | 10 | 59[56-63] | 4 (40) |\n| N = 80 | Viral meningitis | 18 | 38[24-43] | 10 (55) |\n| | Control | 20 | 36[28-42] | 6 (30) |\n| | Acrodermatitis chronica atrophicans | 6 | 66[59-74] | 6 (100) |\n| | Erythema migrans | 9 | 47[36-54] | 5 (55) |\n| | Post-treatment-Lyme-disease-syndrome | 17 | 58[48-64] | 10 (58) |\n\nAbbreviations: CSF = cerebrospinal fluid, IQR = Inner Quartile Range\n\n## CSF proteomics\n\n### CSF development cohort\n\nA total of 1,865 proteins were identified in CSF, with a median of 773 quantified pr. sample (Supplementary Figure 1). Fourteen samples were excluded due to low protein numbers. After filtering for missingness, a total of 654 proteins were included for further analysis.\n\nA total of 176 proteins were significantly different between LNB and viral meningitis, of these 10 had an absolute log2 fold change larger than 1 (Figure 1A, Supplementary Table1). A total of 464 proteins were significantly different between LNB and controls, of these 41 had an absolute log2 fold change larger than 1 (Figure 1B, Supplementary Table1).\n\nOf the significant proteins with high log2 fold changes in the two comparisons, 7 proteins overlapped (Figure 1C).\n\n### CSF validation cohort\n\nIn the validation cohort a total of 147 proteins were significantly different in LNB compared to viral meningitis and controls with high log2 fold changes, where 43/46 proteins from the development cohort overlapped (Figure 1B and Supplementary Figure 2,3).\n\n### Protein signatures of LNB in CSF\n\nProtein signatures were dominated by immunoglobulins (e.g., IGLV3-25, IGLV2-18, FCGBP, IGHM), proteins involved in innate immune responses (e.g. enolase 1, S100A9), neuroendocrine signalling (e.g. ECRG4, CHGA), cell-migration and cell-damage (e.g. PFN1, APCS, YWHAZ, H4C1, ACTA2) (Figure 1C). Immunoglobulins were generally upregulated, while proteins involved in innate immune responses and neuroendocrine signalling were relatively downregulated in LNB compared to viral meningitis and controls.\n\n## Diagnostic classifier for LNB based on machine learning and CSF proteomics\n\nThe protein profiles of the CSF development cohort were used to develop a ML model to evaluate the potential of MS-based proteomics coupled with ML as diagnostic support in LNB. Of the twelve ML models tested, the Logistic Regression (LR) model obtained the highest performance in the classification of viral meningitis vs. LNB, whereas the Support Vector Classifier (SVC) model produced the best result in the control vs. LNB classification (Supplementary Figure 4 and 5 respectively). The performance of the diagnostic classification model of viral meningitis vs. LNB on the test set had an area under the curve (AUC) of 0.91 (std. = 0.11) and a Matthews Correlation Coefficient (MCC) of 0.81 (std.=0.08) (Figure 2A). When applied on the validation cohort, the model obtained an AUC and MCC of 0.92 (std. = 0.02) and 0.7 (std.=0.06). According to their SHAP (SHapley Additive exPlanations) values, the most important proteins in the discrimination between viral meningitis and LNB are visualized in Figure 2B. The performance of the diagnostic classification model of control vs. LNB on the test set had an AUC of 0.93 (std. = 0.07) and a MCC of 0.76 (std.=0.14) (Figure 2C). When applied on the validation cohort, the model obtained an AUC and MCC of 0.9 (std. = 0.01) and 0.63 (std.=0.06). The most important proteins in the model according to their SHAP values (Figure 2D) were similarly related to innate and humoral immune responses, neuroendocrine signalling, and cell-damage.\n\n## Plasma proteomics\n\n### Plasma development cohort\n\nA total of 379 proteins were identified in plasma, with a median of 268 proteins quantified per sample (Supplementary Figure 6). One sample was excluded due to low protein number. After filtering for missingness, a total of 232 proteins were included for further analysis.\n\nA total of 61 proteins were significantly different between LNB and viral meningitis (Figure 3A, Supplementary Table2) and 63 for LNB versus controls (Figure 3B). The overlap between these two comparisons of significant proteins were 36 (Figure 3C, Supplementary Table2).\n\n### Plasma validation cohort\n\nIn the validation cohort a total of 25 proteins were significantly different in LNB compared to viral meningitis and controls. Ten overlapped with the significant proteins from the development cohort (Figure 3B and Supplementary Figure 7,8).\n\n### Protein signatures of LNB in plasma\n\nThe differences in protein profiles between the three patient groups are dominated by proteins involved in innate and humoral immune responses (Figure 3C). When comparing protein profiles of plasma samples from LNB and viral meningitis, patients with LNB generally seem to have a relative upregulation of proteins associated with innate immunity and complement activation (e.g., FCN3, SERPING1, SERPINA5), lipid metabolism (e.g., APOE, APOC1, APOM), and coagulation regulation (e.g., F13A1, PROC). In contrast, patients with viral meningitis have a plasma protein profile dominated by acute-phase and pro-inflammatory markers (e.g., CRP, S100A8, S100A9) and immunoglobulin production. In the comparison between LNB and controls, upregulated plasma-proteins in LNB are similarly involved in complement activation (e.g., C3, C5), coagulation and inflammation regulation (e.g., SERPINA3, SERPIND1), and immune system modulators (e.g., HP, ITIH4). In contrast to CSF, most immunoglobulins had a higher protein level in the plasma of control individuals compared to LNB patients.\n\n## Diagnostic classifier for LNB based on machine learning and plasma proteomics\n\nSimilar to the CSF analysis, plasma proteome data were subjected to ML algorithm- and hyperparameter selection in a 3-fold cross validation scheme. It was not deemed feasible to develop a model for the discrimination of viral meningitis and LNB due to the low number of viral meningitis cases, hence, the only model tested was the discrimination of controls and LNB. Of the twelve models tested, the SVC model obtained the best performance in the test set (Supplementary Figure 9) with an AUC of 0.96 (std.=0.03) and a MCC of 0.83 (std.=0.008) (Figure 4A). When applied on the validation cohort the model obtained an AUC of 0.80 (std.=0.02) and a MCC of 0.48 (std.=0.04) (Figure 4A). According to the SHAP feature importance values, the most predictive proteins for the diagnostic classification of controls vs. LNB (Figure 4B) were associated with innate immunity, humoral immune defence, coagulation and cellular metabolism. When the LNB classification model was applied to other diagnostic groups, it identified groups with active *Borrelia burgdorferi* s.l. infections; acrodermatitis chronica atrophicans and erythema migrans, as having significantly higher similarities to the LNB profile than groups with absence of active infection; Post-treatment-Lyme-disease-syndrome or unrelated aetiology; viral meningitis. Mann-Whitney U Test (acrodermatitis chronica atrophicans+erythema migrans vs Post-treatment-Lyme-disease-syndrome +Viral meningitis): U statistic = 5475.0, p-value = 2.65e-07. (Figure 4c).\n\n## Comparison of protein profiles in CSF and plasma\n\nWe found an overlap of 72 proteins that were significantly different between LNB and controls or viral meningitis in both CSF and plasma (Figure 5A, Supplementary Table 3). The majority of overlapping proteins (62/72) were relatively upregulated in CSF from patients with LNB compared to controls and viral meningitis, and 30 of these were inversely regulated in plasma. This group primarily included immunoglobulins (18/30) (Figure 5B).\n\n# DISCUSSION\n\nOur study shows that MS-based proteomics can accurately differentiate patients with LNB from patients with viral meningitis and non-LNB controls. Notably, we observed a high level of diagnostic accuracy in plasma, highlighting the potential of blood-based proteomics as a clinically valuable tool. Given the current need for novel diagnostic approaches to reduce delays and reliance on lumbar punctures, these findings could have significant implications for both initial diagnosis and monitoring of treatment response in LNB.\n\nTo our knowledge, this is the first study reporting the use of untargeted proteomics as a diagnostic tool in a large and well-defined cohort of adult LNB patients, investigating both CSF and plasma samples. Additionally, the inclusion of viral meningitis cases strengthens our findings by assessing the ability of proteomics to distinguish between two conditions with overlapping symptomatology and CSF findings. This approach enhances the translational potential of our results.\n\nPrevious studies investigating the diagnostic potential of proteomics in LNB have been limited in scope and methodology. A small US-based study assessing the diagnostic utility of proteomics in Lyme disease including a small sub-group with CNS involvement; Angel et al. (2013) found a panel of 13 proteins discriminated between cases and controls reaching an AUC of 0.817. However, the focus on other Lyme disease manifestations than LNB likely reflects the, somewhat debated, geographical difference in prevalence of neurological involvement with a *B. burgdorferi* s.l. strain-dependent lower incidence in North America compared to Europe18,19. More recent European studies have investigated the diagnostic use of protein panels in LNB, though with different methodologies and sample types: Fredriksson et al. (Sweden, 2024) analysed serum from 119 paediatric patients with LNB (n=61) and non-LNB (n=58) using a multiplex proximity extension assay that included a panel of 92 predefined inflammatory markers and found that a 5-protein-panel identified LNB with an AUC of 0.8820. Though the diagnostic groups and the use of blood-samples were comparable to our study, it is unclear to what extent results in children can be extrapolated to adults and the multiplex assay used is not comparable to the untargeted MS-based proteomics used in our study. Gęgotek et al. (Poland, 2024) performed LC-MS based proteomics on serum from patients with LNB (n=10) and controls (n=27) and found significant differences, but did not report measures of diagnostic accuracy21. Other investigations have primarily focused on characterizing patients with post-treatment-Lyme-disease-syndrome rather than acute LNB22,23. Despite differences in study design, a consistent pattern of immune activation has emerged across studies, emphasizing the role of innate immune responses, complement system and humoral immune defence in the human host response to *B. burgdorferi* s.l. infection.\n\nOur proteomic findings in CSF, indicate a distinct immune response characterized by elevated levels of immunoglobulin chains, complement-related proteins, and proteins involved in immune cell migration and cytoskeletal dynamics. These findings suggest a highly targeted immune response against *B. burgdorferi* s.l. antigens, involving adaptive immunity with significant antibody production and complement activation. This aligns with established knowledge of host immune response during infections with *B. burgdorferi* s.l.24. Interestingly, the antibody response exhibited opposite regulation in CSF and plasma, likely illustrating the significant compartmentalization of the humoral immune response to the CNS in LNB and reflects the fact that all patients with LNB in this study had a positive *B. burgdorferi* s.l.- specific intrathecal antibody index. Moreover, we observed overlapping regulation of key immune-related proteins in both plasma and CSF, suggesting a coordinated immune response across compartments. Plasma and CSF both showed changes in immunoglobulin chains, complement factors, and innate immune modulators in LNB compared to controls, indicating a systemic and localized immune activation. The CSF findings highlight immunoglobulin diversity and a direct antibody response, reflecting the local immune reaction in the CNS. Meanwhile, plasma proteomics revealed a strong systemic immune engagement, with upregulation of innate immune components such as ficolins and coagulation proteins, underscoring systemic inflammation. Notably, viral meningitis exhibited a different pattern, with both plasma and CSF showing elevated acute-phase reactants (e.g., CRP, S100A9) and immunoglobulins, consistent with a strong inflammatory and humoral response. Opposing regulation of certain proteins in CSF and plasma in LNB likely reflects a compartmentalized immune strategy, where the CNS immune response is tightly regulated, while plasma changes mirror systemic inflammation. Additionally, factors such as blood-brain barrier permeability, local versus systemic protein production, and clearance mechanisms may further influence these patterns.\n\nAdditionally, structural proteins involved in immune cell motility were upregulated in CSF, indicating active immune cell recruitment within the CNS, specifically in LNB. Viral meningitis patients present a pattern more focused on inflammatory markers and metabolic activity, consistent with an acute viral immune response.\n\nA small cluster of cytoskeleton and extracellular matrix proteins (VIM, ACTA2, PFN1, FN1 and ACTB) emerged among the top discriminatory markers, suggesting increased cell-turnover in LNB. While expected in LNB vs. controls, this is more surprising when compared to viral meningitis. Notably, *B. burgdorferi* s.l. spirochetes are hypothesized to extravasate early upon transmission and travel through the extracellular matrix to peripheral nerves eventually reaching the borders of the CNS and creating the inflammatory basis of radiculoneuritis18,25. Vimentin (VIM), a class III intermediate filament that regulates myelination in axons of peripheral nerves26, is particularly relevant given our limited understanding of CNS entry by *B. burgdorferi* s.l. spirochetes, the frequent cranial nerve involvement in LNB with painful radiculoneuritis9,27–29 and because proteins released from damaged nerves to the peripheral circulation could be potential biomarker candidates for early LNB, as previously shown with neurofilament light chain (NfL)30. Additionally, fibronectin (FN1) which is also found in this cluster, is considered essential for *B. burgdorferi* s.l. cell adhesion and migration through binding to *B. burgdorferi* s.l. surface proteins BBK3231 and RevA32.\n\nThe clinical implications of our findings are considerable. If validated in independent cohorts, CSF proteomics could aid in diagnosing LNB among adult patients with CNS infections with unknown aetiology. This may be particularly relevant for PCR-negative suspected viral meningitis cases, where CSF proteomics suggestive of LNB could prompt further testing or the direct initiation of relevant antibacterial treatment e.g. doxycycline. However, the most significant clinical implication would be the ability to diagnose LNB using a blood sample alone - a true gamechanger in LNB diagnostics. It would spare patients the discomfort and risk for complications of lumbar puncture and reduce healthcare-costs associated with referral to specialized healthcare facilities. A diagnostic blood test for LNB would likely reduce the diagnostic delay and thereby reduce the risk of residual symptoms. Even a modest improvement over current serology-based approaches, could lead to fewer invasive procedures and significantly ease treatment-effect monitoring. This would be particularly beneficial in children, who account for around 30% of all LNB patients, and often require general anaesthesia to have a lumbar puncture performed3334,35. Moreover, a blood-based test could address the unmet need for a less invasive method to monitor treatment response in patients with persistent symptoms after LNB treatment.\n\nWhile these findings demonstrate the diagnostic potential of proteomics in LNB, it is important to consider the strengths and limitations of our study. With 483 samples from patients with LNB, viral meningitis and non-LNB controls, our study represents the largest investigation to date. While we could not stratify patients in full accordance with the European Federation of Neurological Societies (EFNS) diagnostic criteria7 due to limited clinical data, our use of uniform case definition and the specificity of a first time positive *B. burgdorferi* sl. intrathecal antibody index minimizes the risk of false-positive LNB diagnoses36. Our selection of clinically relevant comparison groups, including viral meningitis and patients who were clinically suspected for LNB, enhances the real-world applicability of our findings by testing the robustness of proteomics in distinguishing LNB from other CNS infections. A key strength of our study is its focus on diagnostic feasibility, employing a proteomic workflow with a short turnaround time suitable for clinical implementation. However, the limited detection range inherent to this approach means that certain low-abundance but highly disease-specific proteins, such as CXCL13, may not be captured. Given that previous proteomic studies in LNB have also failed to detect CXCL13, this highlights a general challenge in proteomic biomarker discovery rather than a limitation of our study specifically37. As with all retrospective analyses, our study is constrained by sample availability and cohort composition. Differences in cohort sizes necessitated varying cross-validation strategies, and some observed differences in protein signatures may be influenced by factors such as disease stage, age, and sex38–42. However, our study population reflects real-world clinical variation, as patients were primarily recruited from referral hospitals. Furthermore, prioritizing clinically relevant diagnostic groups over strictly age- and sex-matched controls enhances the translational value of our findings.\n\nIn conclusion, our findings demonstrate that MS-based proteomics can accurately distinguish LNB from controls in both CSF and plasma. These results warrant further prospective validation, particularly with longitudinal sampling, to assess the diagnostic utility of plasma proteomics and its potential role in monitoring treatment response in LNB patients.\n\n# References\n\n1. Hansen K, Crone C, Kristoferitsch W. *Lyme Neuroborreliosis*. Vol 115. 1st ed. Elsevier B.V.; 2013. doi:10.1016/B978-0-444-52902-2.00032-1\n2. Dahl V, Wisell KT, Giske CG, Tegnell A, Wallensten A. Lyme neuroborreliosis epidemiology in Sweden 2010 to 2014: Clinical microbiology laboratories are a better data source than the hospital discharge diagnosis register. *Eurosurveillance*. 2019;24(20):1800453. doi:10.2807/1560-7917.ES.2019.24.20.1800453/CITE/PLAINTEXT\n3. Dessau RB, Espenhain L, Mølbak K, Krause TG, Voldstedlund M. Improving national surveillance of Lyme neuroborreliosis in Denmark through electronic reporting of specific antibody index testing from 2010 to 2012. *Eurosurveillance*. 2015;20(28):1-11. doi:10.2807/1560-7917.ES2015.20.28.21184\n4. Tetens MM, Haahr R, Dessau RB, et al. Changes in Lyme neuroborreliosis incidence in Denmark, 1996 to 2015. *Ticks Tick Borne Dis*. 2020;11(6). doi:10.1016/j.ttbdis.2020.101549\n5. Koelman DLH, Van Kassel MN, Bijlsma MW, Brouwer MC, Van De Beek D, Van Der Ende A. 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Bockenstedt LK, Wooten RM, Baumgarth N. Immune response to borrelia: Lessons from lyme disease spirochetes. *Curr Issues Mol Biol*. 2020;42:145-190. doi:10.21775/cimb.042.145\n25. Rupprecht TA, Koedel U, Fingerle V, Pfister HW. The pathogenesis of lyme neuroborreliosis: From infection to inflammation. *Mol Med*. 2008;14(3-4):205-212. doi:10.2119/2007-00091.Rupprecht\n26. Triolo D, Dina G, Taveggia C, et al. Vimentin regulates peripheral nerve myelination. *Development*. 2012;139(7):1359-1367. doi:10.1242/dev.072371\n27. Radzišauskienė D, Urbonienė J, Jasionis A, et al. Clinical and epidemiological features of Lyme neuroborreliosis in adults and factors associated with polyradiculitis, facial palsy and encephalitis or myelitis. *Sci Rep*. 2023;13(1):1-11. doi:10.1038/s41598-023-47312-4\n28. Solheim AM, Skarstein I, Quarsten H, et al. 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Borrelia burgdorferi RevA antigen binds host fibronectin. *Infect Immun*. 2009;77(7):2802-2812. doi:10.1128/IAI.00227-09\n33. Bruinsma RA, Zomer TP, Skogman BH, van Hensbroek MB, Hovius JW. Clinical manifestations of Lyme neuroborreliosis in children: a review. *Eur J Pediatr*. 2023;182(5):1965-1976. doi:10.1007/s00431-023-04811-w\n34. Garro A, Avery RA, Cohn KA, et al. Validation of the Rule of 7’s for Identifying Children at Low-risk for Lyme Meningitis. *Pediatr Infect Dis J*. 2021;40(4):306-309. doi:10.1097/INF.0000000000003003\n35. Skogman BH, Sjöwall J, Lindgren PE. The NeBoP score - a clinical prediction test for evaluation of children with Lyme Neuroborreliosis in Europe. *BMC Pediatr*. 2015;15(1):1-9. doi:10.1186/s12887-015-0537-y\n36. Blanc F, Jaulhac B, Fleury M, et al. Relevance of the antibody index to diagnose Lyme neuroborreliosis among seropositive patients. *Neurology*. 2007;69(10):953-958. doi:10.1212/01.wnl.0000269672.17807.e0\n37. Strle F, Henningsson AJ, Strle K. 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The PRIDE database resources in 2022: A hub for mass spectrometry-based proteomics evidences. *Nucleic Acids Res*. 2022;50(D1):D543-D552. doi:10.1093/nar/gkab1038\n\n# MATERIALS AND METHODS\n\n## Ethics\nSamples were obtained during diagnostic investigation and all patients had given their informed consent to the storage of biological material and its future use in research. The study was approved by Knowledge Center for Data Reviews (P-2019-707) and the local ethics committee (H-17024315). The biobanks were approved by the Danish Data Protection Agency (Rigshospitalet: j.nr.: 2012-41-0036).\n\n## Study design\nThis study was an observational retrospective cohort study.\n\n## Study population and setting\nWe identified a total of 483 CSF (n = 308) and plasma (n = 175) samples from adults (>18 years) with LNB, erythema migrans, acrodermatitis chronica atrophicans, post-treatment-Lyme-disease-syndrome, viral meningitis, and individuals who were investigated for suspected LNB, but had normal CSF (controls) from; i) The Danish National Biobank (samples collected from 2001-2011) and ii) the Biobank of the Department of Infectious Diseases at Copenhagen University Hospital, Rigshospitalet (samples collected from 2016-2022). After informed patient consent for storage and future use in research was provided, CSF samples were labelled and stored at -80°C and blood samples in EDTA tubes were spun and the supernatant was transferred to Eppendorf tubes, labelled, and stored at -80°C. Samples from the two sites of origin were kept separate in the subsequent analyses to preserve independent cohorts for model development and validation.\n\n## Cohorts\nSamples were divided in four cohorts for diagnostic model development and validation in CSF and plasma respectively. The CSF development cohort consisted of 145 CSF samples from patients diagnosed with LNB (n=49), viral meningitis (n=44) and controls (n=52). The CSF validation cohort included a total of 163 CSF samples from patients diagnosed with LNB (n=69), viral meningitis (n=45), and controls (n=49). The plasma development cohort included a total of 95 plasma samples from patients with LNB (n=27), viral meningitis (n=20) and controls (n=48) whereas the plasma validation cohort consisted of 80 plasma samples from patients with LNB (n=10), viral meningitis (n=18), controls (n=20) and an additional cohort of plasma samples from patients with manifestations of Lyme borreliosis without CNS involvement including post-treatment-Lyme-disease-syndrome (n=17), erythema migrans (n=9), and acrodermatitis chronica atrophicans (n=6).\n\n## Definitions of diagnostic groups\n**LNB:** Patients diagnosed with LNB based on a first-time positive *B. burgdorferi*-specific intrathecal antibody test and the International Classification of Diseases 10 revision (ICD-10) diagnosis code Borreliosis: A69.\n\n**Viral Meningitis:** Patients with a final clinical diagnosis of viral meningitis determined by an infectious disease specialist at a tertiary referral university hospital. The diagnosis was based on clinical presentation, CSF pleocytosis and exclusion of other diagnoses. In 76 cases a PCR-verified viral aetiology was determined (Herpes simplex virus 2 (n=32), Enterovirus (n=30), Varicella zoster (n=9), Influenza A virus (n=3), Epstein-Barr virus (n=1), Toscana virus (n=1)).\n\n**Controls:** Individuals who had a lumbar puncture performed because LNB was suspected, but where white-blood-cell (WBC) count in the CSF was within normal reference ranges (CSF-WBC: 0-5 x 10⁶/L) and the *B. burgdorferi* s.l. specific intrathecal antibody index was negative.\n\n**Post-treatment-Lyme-disease-syndrome:** Patients with persisting symptoms of Lyme borreliosis >6 months after diagnosis and treatment.\n\n**Erythema migrans:** Patients with a skin rash clinically diagnosed with *erythema migrans* at the Unit for Tick-Borne Infections, Copenhagen University Hospital, Rigshospitalet.\n\n**Acrodermatitis chronica atrophicans:** Patients clinically diagnosed with *acrodermatitis chronica atrophicans* skin rash and positive *B. burgdorferi* s.l. IgG in blood at the Unit for Tick Borne Infections, Copenhagen University Hospital, Rigshospitalet.\n\n## Proteomic analysis\nCSF and plasma samples were thawed and 100 µl were transferred to 96-well plates for analysis. The sample preparation was optimized based on the previously published methods described in . Briefly, 20 µl CSF was were first denatured with 30 µl PreOmics Lysis buffer, while 5 µl plasma was denatured with 45 µl PreOmics Lysis buffer . Both sample types were subsequently digested using LysC/trypsin enzyme mix. The resulting peptides were purified using two-gauge SDB-RPS StageTips, and the eluate analysed on Evosep One (Evosep Biosystem, Denmark) liquid chromatography system, coupled online to an Orbitrap Exploris 480 mass spectrometer. Data acquisition was performed in data-independent analysis (DIA), using 60 samples per day (SPD) gradient and 8 cm Pepsep column.\n\n## Data processing\nInitial data processing of the mass spectrometry raw files were performed with DIA-NN version 1.9 in a data independent search . The DIA-NN data underwent further processing using the Clinical Knowledge Graph (CKG), alphapeptstats and Jupyter Notebook . Initially, a stringent filter for missing data was applied: 1) samples with low protein count, defined by a value below 1.5IQR from the 25th quantile of the combined distribution, were excluded, and 2) proteins with a missingness of more than 40% across samples were excluded. Data was log2 transformed. The remaining missing values were imputed with a variational autoencoder using the PIMMS software . Assessment of sample quality was conducted as previously described . Batch correction was executed using combat to overcome potential plate-specific bias on subsequent analyses .\n\n## Data analysis\nProteins exhibiting significantly different levels between the cohorts were identified by unpaired t-tests. Multiple hypothesis correction was applied with the Benjamini-Hochberg method, with adjusted P-values < 0.05 deemed statistically significant. P-values and protein abundances were visualized in Volcano plots, with -log10(corrected p-value) and log2 of protein fold change between groups. Venn diagrams were used to visualize overlaps in significant proteins between statistical comparisons. Heatmaps in combination with Sankey plots of gene ontology terms were used to highlight protein changes of the significant proteins together with their biological processes . In the heatmaps, protein abundances were z-scored. Gene ontology terms were retrieved for each protein through UNIPROT. Gene ontology terms with frequency of less than 5% across proteins were not visualized.\n\n## Model development\nZ-scored data from the development cohorts were analysed using supervised machine learning to explore the potential for a diagnostic signature for LNB. Significant proteins identified by t-test analysis on the development cohorts were used as input features in the training data. Our data sets, comprising both samples from patients diagnosed with LNB and viral meningitis or control samples, was partitioned into a training set for model development and a test set for model validation using a 5-fold or 3-fold cross-validation (CV) approach for CSF and plasma respectively. The number of CV-folds was decided based on sample size with a minimum of 30 samples in each set. Both sets maintained an equal ratio of positive and negative cases (stratified k-fold cross-validation). The classification target used for analysis was the diagnosis of LNB and viral meningitis or LNB and control (yes/no). An appropriate ML model was determined by testing the performance of twelve different algorithms based on the area under the curve (AUC) and Matthews Correlation Coefficient (MCC) in the development test set cross-validations. For each algorithm, optimal hyperparameters and features were selected during cross-validation. Feature importance were highlighted for the top 10 most predictive features with SHAP (SHapley Additive exPlanations) values .\n\n## Model validation\nThe models trained on the development cohorts were subsequently applied to the validation cohorts and the performance was assessed by AUC and MCC. ROC curves and confusion matrices were used to visualize the performance of the classifiers.\n\n# Supplementary Files\n\n- [SupplementaryMaterial.docx](https://assets-eu.researchsquare.com/files/rs-6048306/v1/22f12199d7786c0b4860e11f.docx) \n Mass-spectrometry-based proteomics enables rapid and accurate diagnosis of Lyme neuroborreliosis in adults"} {"paper_id": "prb56", "title": "A synthetic receptor platform enables rapid and portable monitoring of liver dysfunction via engineered bacteria", "text": "# Abstract\n\nBacterial biosensors, or bactosensors, are promising field-deployable agents for medical and environmental diagnostics. However, the lack of scalable frameworks to systematically program ligand detection limits their applications. Here we present a synthetic receptor platform, termed EMeRALD (Engineered Modularized Receptors Activated via Ligand-induced Dimerization) which supports the modular assembly of sensing modules onto a high-performance, generic signaling scaffold controlling gene expression in *E. coli*. We applied EMeRALD to detect bile salts, a biomarker of liver dysfunction, by repurposing sensing modules from enteropathogenic *Vibrio* species. We improved the sensitivity and lowered the limit-of-detection of the sensing module by directed evolution. We then engineered a colorimetric bactosensor detecting pathological bile salt levels in serum from patients having undergone liver transplant, providing an output detectable by the naked-eye. The EMeRALD technology enables functional exploration of natural sensing modules and rapid engineering of synthetic receptors for diagnostics, environmental monitoring, and control of therapeutic microbes.\n\nSystems Biology \nBacteriology \nGeneral Biochemistry \nliver dysfunction \nEMeRALD (Engineered Modularized Receptors Activated via Ligand-induced Dimerization) \nbiosensors\n\n# Introduction\n\nEarly disease detection and monitoring of chronic pathologies help reduce mortality and improve patients' quality of life1, 2. In that context, *in vitro* diagnostics technologies play key roles at different stages of the healthcare chain3. However, many diagnostics technologies require heavy equipment, are expensive, and necessitate trained personnel, limiting testing to centralized facilities such as hospitals. Yet, as exemplified by glucose monitoring for diabetes, field-deployable diagnostic devices can tremendously improve patient healthcare, follow-up, and self-reliance4, 5. Robust, scalable, and cost-effective biosensing technologies for field-deployable diagnostics have thus been under intense research interest over the past decade6.\n\nBacteria must sense and respond to myriad chemical and physical signals to survive and reproduce, and are thus ideal candidates for engineering biosensors. Whole-cell biosensors (WCB) are genetically modified living cells that detect molecules of interest generally using a transcription factor regulated by the ligand of interest, and activating transcription of a reporter gene7. While explored since the dawn of genetic engineering8, recent advances in synthetic biology have improved whole-cell biosensor robustness, sensitivity, signal-to-noise ratio, and signal-processing capabilities, supporting their use in complex media like wastewater and clinical samples9, 10, 11. With these new capabilities, whole-cell biosensors have the potential to provide miniaturized, field-deployable, diagnostic devices capable of multiplexed detection and sophisticated computation10, 11. As a self-manufacturing and biodegradable platform, biology provides a cost-effective and environmentally friendly alternative to traditional diagnostic methods. The self-manufacturing nature of biology also offers a unique advantage for low-resource settings and remote, highly-constrained conditions, such as those found in space exploration12. Despite all these advantages, the scope of application for bacterial biosensors is limited by the difficulty to generate novel sensors detecting biomarkers of interest. Although significant progress has been recently made13, scalable platforms to rapidly generate new receptors are needed.\n\nLiver disease includes dozens of pathologies such as cirrhosis, hepatitis, liver cancer, hepatobiliary problems such as cholangitis, and drug-induced liver injury14–18. Liver disease is a global healthcare burden accounting for 2 million deaths per year, and impacts the quality of life of millions of people worldwide19. Liver is the second most common transplanted organ, but only 10% of needs are met. Currently, liver disease diagnostics and monitoring is performed by assessing a panel of biomarkers20. However, current methods for *in vitro* diagnostics are only available in hospitals and testing laboratories, limiting the frequency of monitoring for patients. In addition, most biomarkers appear at late disease stages (when significant cellular damage has already occurred) and lack specificity21. As liver diseases are chronic, evolutive pathologies, patients would benefit from portable monitoring devices that enable rapid and simple assessment of liver function with high sensitivity and specificity.\n\nAn alternative biomarker of liver dysfunction is the presence of bile salts in serum. Bile salts are key components of bile which are critical for digestion in which they help absorption of fat22. Interestingly, serum bile salts have emerged as a general biomarker of liver disease, and are the gold-standard diagnostic method for pregnancy cholangitis24, 25. In addition, several studies have pointed to bile salts as a general biomarker of interest for early cirrhosis, hepatitis, drug-induced liver injury. In addition, bile salts provide a highly specific and dynamic assessment of liver function. For example, serum bile salts are highly correlated with the obstruction state of the bile duct and rapidly decrease when biliary stenting is performed26. Furthermore, specific bile salt profiles may be associated with particular liver diseases27–29. Bile salts thus represent an ideal and specific biomarker for diagnosis and dynamic monitoring of liver disease. Yet, as for other biomarkers, current detection methods for bile salts based on enzymatic assays30 are only performed in a centralized fashion and cannot discriminate between different bile salts.\n\nTo address these challenges, we took advantage of the natural capacity of enteropathogenic bacteria to detect bile salts upon arrival into the gut to activate their virulence pathways31, 32. We rewired sensing modules for bile salt detection into our modular bacterial receptor platform termed EMeRALD (Engineered Modularized Receptors Activated via Ligand-induced Dimerization) operating in *Escherichia coli*33. As the synthetic receptor operates in a surrogate, non-pathogenic host, we performed directed evolution of the sensing module and improved its limit-of-detection (LOD) and sensitivity. Finally, we optimized a colorimetric version of the system to operate in clinical samples. The resulting bactosensor can detect pathological levels of bile salts in serum from patients having undergone liver transplant and provides a signal detectable with the naked eye. The bile salt bactosensor provided here could support field monitoring of liver function for a wide range of conditions. Our work highlights the flexibility and modularity of the EMeRALD receptor platform for rapid characterization and engineering of novel sensing capabilities in whole-cell biosensors.\n\n# Results\n\nEngineering of synthetic bile-salt receptors in *E. coli* using the EMeRALD platform.\n\nEnteropathogenic bacteria such as *Vibrio cholerae* or *Vibrio parahaemolyticus* cause acute intestinal infections mediated by toxin secretion34. These pathogens use bile salts as an intestinal location signal to activate their virulence pathways. Bile salt sensing is mainly under the control of inner membrane sensor/cofactor couples, TcpP-TcpH for *V. cholerae*31 and VtrA-VtrC for *V. parahaemolyticus*35. As using pathogens as biosensors would involve significant host-specific regulation correction35, 36 and biosafety containment issues, an alternative strategy is to rewire pathogen sensing modules of interest into a modular platform operating in a surrogate host (Fig. 1a).\n\nThe EMeRALD receptor platform, which we recently designed33 (Fig. 1b), is derived from membrane-bound one-component systems, which are bitopic proteins with a typical architecture of a cytoplasmic DNA Binding Domain (DBD), a juxtamembrane linker, a transmembrane region, and a periplasmic Ligand Binding Domain (LBD). Direct fusion between the LBD and the DBD provides a simple yet efficient solution to transduce incoming signals into a transcriptional output37, 38. The EMeRALD platform operates in *E. coli* and uses the DBD from the CadC pH and lysine sensor which is inactive in its monomeric state39. Ligand-induced dimerization of the LBD triggers dimerisation of the cytoplasmic DBD and transcriptional activation40. This straightforward mechanism offers the potential to modularize receptor sensing and signaling by domain swapping. We previously built a synthetic receptor responding to caffeine by using a nanobody for this ligand as LBD33.\n\nTo engineer a chimeric bile-salt receptor in *E. coli*, we fused the *V. cholerae* TcpP bile-salt sensing module and its transmembrane region (TM) to the DNA binding domain of CadC (Fig. 1c). As a reporter, we placed superfolder Green Fluorescent Protein (sfGFP)41 under the control of the CadC target promoter, pCadBA. We also expressed the cofactor protein TcpH, previously described to protect TcpP from proteolysis by the *V. cholerae* RseP protease once dimerized in response to bile salts42. We first confirmed using inducible gene expression systems that co-expression of the TcpH cofactor was necessary for TcpP function, using the primary bile salt taurocholic acid (TCA) as a ligand (Supplementary Fig. 1–3). These data suggest that the RseP homolog present in *E. coli* (UniProt:P0AEH1) can degrade TcpP when not bound by TcpH. We also found that the relative expression level of CadC-TcpP and TcpH were critical parameters affecting system performance (Supplementary Fig. 3).\n\nWe then placed both proteins under the control of constitutive promoters43. We used the strong constitutive promoter P5 for TcpH and three different constitutive promoters of increasing strengths, P9, P10, and P14, for CadC-TcpP (Fig. 2a) and tested their response to TCA42 (Fig. 2b, Supplementary Fig. 4–5). We found that the P9-CadC-TcpP variant had the lowest LOD, highest dynamic range, and highest signal strength. These data confirm that the stoichiometry between CadC-TcpP and TcpH is a key parameter influencing receptor performance.\n\nWe then assessed the versatility of the EMeRALD platform by connecting the VtrA/VtrC sensor system from *V. parahaemolyticus*32 (Fig. 2c). We built a dual-expression system consisting of P9-CadC-VtrA and P5-VtrC, and tested its response to its canonical ligand taurodeoxycholic acid (TDCA). We found that the VtrA/VtrC EMeRALD system was functional with a slightly higher LOD, similar dynamic range and signal strength than the TcpP/TcpH EMeRALD system (Fig. 2d, Supplementary Fig. 6). These results highlight the modularity and scalability of the EMeRALD platform, which supports the connection of different sensing modules to the receptor scaffold.\n\n## Synthetic bile salt receptors exhibit different specificity profiles.\n\nWe then assessed the specificity profile of the synthetic bile salt receptors. Bile salts are classified in two categories: primary bile salts (including taurocholic acid) are produced by the liver while secondary bile salts arise from modification of primary bile salts by gut microbiome metabolism. Primary bile salts are upregulated in serum and urine of patients with liver disease27–29. Previously identified virulence activating factors for *V. cholerae* include taurocholic acid, glycocholate, and cholic acid42. We measured the response of the bactosensor to a panel of twelve different bile salts, including both primary and secondary types (Fig. 2e, Supplementary Fig. 7–8). Interestingly, the CadC-TcpP system was highly specific for primary conjugated bile salts (especially TCA and GCDCA), while not responding to secondary bile salts. On the other hand, the CadC-VtrA system has a larger spectrum of bile salt specificity, mainly responding to secondary conjugated bile salts GDCA and TDCA. Due to the link between primary bile salts and liver diseases, we selected the TcpP/TcpH system to develop a bile salt bactosensor for medical diagnosis.\n\n## Directed evolution of TcpP sensing module for improved LOD and higher sensitivity.\n\nSensor sensitivity and LOD are key parameters for biosensors applications. We aimed to identify key residues determining the sensitivity of the TcpP sensing module, and targeted those to improve synthetic receptor sensitivity and LOD. To do so, we coupled comprehensive mutagenesis with functional screening and Next-Generation Sequencing (NGS), an approach which supports the identification of functional variants together with the sequence determinants within local structural motifs44–46. This strategy has also been used to engineer orthogonal two-component systems47.\n\nTransition from intramolecular to intermolecular disulfide bonds between TcpP monomers is a key determinant of TcpP response to bile salts and is mediated by two cysteine residues, Cys207 and Cys21842. By performing multiple sequence alignments of different TcpP bacterial homologs (Supplementary Fig. 9), we found a significant conservation of the amino-acids flanked by these two cysteines (Fig. 3a). Secondary structure prediction and *ab initio* 3D prediction using the Rosetta modelling suite (Fig. 3b and Supplementary Fig. 10) suggested that each cysteine was located in rigid beta-sheets separated by a flexible loop region between Asn211 and Gln214. This loop propensity to form a turn would allow the two beta sheets and the cysteines to come in close proximity and form an intramolecular disulfide bond. We hypothesized that the flexibility of the turn region between Cys207 and Cys218 was a key parameter controlling the transition rate between the two states, and that altering its amino-acid composition could change the system’s sensitivity to bile salts.\n\nWe thus built a comprehensive mutational library (NNK x 4, theoretical library complexity ≌ 1.05 x 106 variants, see methods for details) targeting the NYEK residues inside the turn, and cloned it into the plasmid constitutively expressing CadC-TcpP and producing GFP in response to bile salts (Fig. 3c). The resulting library was induced with TCA, and GFP-positive variants were isolated by fluorescence-activated cell sorting (FACS). We performed three rounds of enrichment (200 μM of TCA as ligand in 1st and 2nd rounds of selection, and 20 µM for the 3rd round) and observed an increasing fraction of the cell population responding to different ligand concentrations (20 to 80 µM) (Fig. 3d). We collected, cultured, and sequenced single variants and tested their response to TCA (Fig. 3e). We found that comprehensive mutagenesis of residues Asn210 to Gln213 could alter the limit of detection, the sensitivity, and the fold activation of our biosensor. The 3.3-fold difference in LOD between V18 and V22 (EC50 from 28.3 to 92.5 µM, Table 1) indicated the broad range of sensitivity engineering obtained by mutating the loop region of the TcpP sensing module. Further kinetic analysis revealed that the sequence variation of this loop region changes reaction speed and system interaction of bile salts with the synthetic receptor (Supplementary Fig. 11).\n\nTo better understand the sequence features influencing the response of TcpP to bile salts, we sequenced the whole pool of enriched variants by next-generation sequencing (NGS). Surprisingly, the sequence features of functional variants were different from those expected from natural TcpP homologs (Fig. 3f and Supplementary Fig. 12). First, and in contrast with *wt* TcpP homologs, we observed a strong depletion of long-chain, negatively charged amino-acids (Asp and Glu) along with long-chain polar amino-acids (Asn and Gln) at position 211. Lysine at position 211 also appeared to be depleted in functional variants (despite being commonly found at this position in other TcpP homologous proteins). Second, amino acids with bulky aromatic side chain such as Phe and Tyr were highly conserved in selected functional variants, but not among TcpP homologs (with the notable exception of Tyr211 in *V. cholerae* TcpP), strongly indicating the important role of aromatic residues at position 211 in the function of *V. cholerae* TcpP. We chose the best engineered variant, termed TcpP18, for further development of a clinical bactosensor.\n\n## Development of a colorimetric version of the bactosensor.\n\nColorimetric assay provides a simple and intuitive method for simple and direct estimation of test results by the naked eye. In addition, colorimetric assays support straightforward development of quantitative assays using smartphone-based platforms for POC or home-based diagnosis48. We used TcpP18 coupled with the reporter beta-galactosidase LacZ (termed TcpP18-LacZ) and its substrate chlorophenol red-β-D-galactopyranoside (CPRG) to provide a colorimetric output49 (Fig. 4a, see methods for details). Similarly to the biosensor equipped with a GFP output, the bile salt specificity profile of the TcpP18-LacZ system was slightly shifted from TCA to GCDCA (Fig. 4b, Supplementary Fig. 13). We thus evaluated the LOD and signal output threshold of TcpP18-LacZ in response to increasing concentrations of GCDCA. We also explored the influence of varying cell density and incubation time (Fig. 4c and Supplementary Fig. 14). Increasing cell density or incubation time both improved the dynamic and operating ranges of TcpP18-LacZ; however, background signal also increased. After optimization, the Tcp18-LacZ was able to detect clinically relevant bile salt concentrations, such as those corresponding to early cirrhosis (~ 5.2 µM GCDCA)50 or nonalcoholic fatty liver diseases with hepatocellular carcinoma (~ 56 µM GCDCA)51.\n\n## Bactosensor-mediated detection of elevated bile salts levels in serum from patients with liver transplant.\n\nWe then prototyped our bactosensor for the detection of bile salts in clinical conditions. To do so, we tested the sensor on samples from patients having undergone liver transplantation. After liver transplant, the main complications are bile ducts stenosis and acute cellular rejection. In order to detect these complications at an early stage, liver tests are performed regularly. Serum bile salt concentration has been shown to be a good indicator for the assessment of liver dysfunction after liver transplantation52. A field-deployable method for bile salt assessment would greatly improve the monitoring of these patients, ultimately allowing fine grained monitoring performed at-home by the patients themselves.\n\nWe tested our bactosensor in clinical 21 serum samples from liver transplantation patients (Fig. 5a and Supplementary Fig. 15). The patients were followed at the Montpellier hospital after their liver transplant, most of them having been performed in the last 2 years (see Supplementary Information). These patients had received a liver transplant for end-stage liver disease as a result of alcoholic related liver disease or non-alcoholic fatty liver disease, chronic cholangitis or liver cancer. A complete hepatic check-up was performed, and serum bile salts were also measured (Supplementary Tables 3–5 for clinical data). We found that patients who had a high potential of acute cellular rejection (ACR) after liver transplantation (serum bile acid > 37 µM)53 had significant and visible colorimetric signal changes (Supplementary Fig. 16) in bactosensor assays. Three patients in particular raised our attention: patients #5, 10 and 13. These three patients had elevated serum bile salts concentration. Two of them (5 and 10) presented abnormalities in their hepatic enzymatic values (ASAT, ALAT, GGT, Pal, and bilirubin). For these patients, the bile salt bactosensor produced the strongest colorimetric change easily detectable with the naked eye (Fig. 5b). We further compared the results of the bactosensor with a commercial bile salt enzymatic assay (Fig. 5c). The high correlation between enzymatic serum bile salt assay and our bactosensor measurements (r = 0.908, p < 0.0001) indicates the reliability of our assay. In addition, we compared the results from the bactosensor with other serum liver biomarkers (Supplementary Fig. 17), and found a high correlation to a common liver biomarker, total bilirubin. These results indicate that our bactosensor is able to provide a simple, reliable, and cost-effective method for monitoring patient condition after liver transplantation.\n\n# Discussion\n\nMicrobes detect and process myriad environmental signals, providing a vast sensing repertoire for engineering biosensors usable for several applications. However, the intricacy of signaling networks and our limited understanding of their biochemical properties restrain their direct use. Here we presented a general strategy to rewire sensing modules of interest into a well-characterized synthetic receptor platform, EMeRALD, enabling their fine tuning and repurposing for novel biomedical applications. In the future, these receptors could be coupled with genetic circuits performing multiplexing logic, memory and signal amplification to engineer even more sophisticated whole-cell biosensors54, 55.\n\nWe were able to connect two different bile salt sensing modules having different specificity profiles, the TcpP/H and VtrA/C systems, which respond mostly to primary and secondary bile salts, respectively. Importantly, our capacity to engineer synthetic bile salt signaling using only these protein domains demonstrates that these modules are the only essential components required for bile salt sensing in their natural host. By performing directed evolution of TcpP, we improved the sensitivity and decreased the LOD of the sensor. In addition, we discovered previously unknown amino-acid sequence features influencing TcpP function and potentially relevant for *V. cholerae* virulence. For instance, we found a stringent functional requirement for the presence of Tyr211 residue in the C-terminal loop of *V. cholerae* TcpP. The requirement for amino acids with a nonpolar aromatic side chain at Tyr211 indicates rigorous steric interactions located in the C-terminal loop region of *V. cholerae* TcpP. The exact role of Tyr211 is still unclear, but this residue may affect TcpP-TcpP dimer formation or TcpP-TcpH interaction. While the unique presence of Tyr at the 211 position in *V. cholerae* was visible on multiple sequence alignments, the link between this residue and TcpP function could not be inferred by this approach.\n\nThis discovery exemplifies how our synthetic receptor platform offers a powerful strategy to interrogate the sequence-function relationship of bacterial sensing modules in a massively-parallel fashion. Such studies in the natural pathogenic host would have been tedious because of complex pathway regulations and safety issues would have limited the final bactosensors to a few expert groups. In contrast, our platform provides a straightforward and scalable strategy to study pathogen signaling in surrogate hosts, usable by the larger scientific community. The EmeRALD system, coupled with the deep-mutational scanning, methods to navigate protein sequence space56–59, designer libraries, and Flow-Seq analysis46 can serve as a general platform for studying bacterial sensing modules, engineering their ligand specificity and their response properties. In particular, our system is ideal for understanding transmembrane one-component signaling, which mechanism and regulation are currently underexplored38. On the same line, EMeRALD receptors could be applied to the discovery of inhibitors of virulence pathways through screening of chemical or natural substances libraries.\n\nHere we show the application of EMeRALD to the field of medical diagnostics by detecting abnormal bile salt levels in patient samples. As bile salts dysregulation and gut dysbiosis are critical in the pathogenesis of liver diseases or gastrointestinal cancer60–65, there is an urgent need for POC assays for bile salt monitoring66. Our bactosensor results correlate well with hospital tests and produce a very strong signal detectable with the naked eye for the three most critical patients, demonstrating the potential of our technology for rapid POC estimation of liver dysfunction. In addition, our system uses very small sample volumes (5 µL) providing an efficient method for POC diagnostics. Yet, given the size of our patient cohort and its diversity, further clinical studies are needed to move our method towards the clinic. Interestingly, the bile salt sensing system could also be applied to control the activity of engineered probiotics upon arrival in the gut, as recently proposed in *Bacteroides thetaiotomicron*67.\n\nThe EMeRALD platform can accommodate natural or synthetic33 sensing modules, providing a versatile and scalable solution to develop new sensing modalities in bacteria. We anticipate that this platform will be repurposed for other applications in medical diagnostics, bacterial therapeutics, and environmental monitoring, supporting the transition of bacterial biosensors towards real-world applications.\n\n| # Variant | Sequence | EC50 (µM) | Response EC50 (RPU) | Max fold change |\n|---------|--------|--------|------------------|-------------|\n| V22 | YYVL | 92.531 | 56.19 | 69.06 |\n| TcpPwt | NYEQ | 89.405 | 56.5 | 164.74 |\n| V7 | WYVH | 86.029 | 53.37 | 51.31 |\n| V78 | FYES | 84.668 | 59.62 | 69.06 |\n| V11 | YYIV | 82.167 | 53.83 | 31.76 |\n| V14 | TFLA | 81.636 | 62.97 | 222.67 |\n| V3 | DFGV | 61.48 | 61.18 | 142.21 |\n| V19 | FFKA | 59.186 | 61.29 | 127.75 |\n| V16 | DFLT | 42.058 | 59.34 | 75.73 |\n| V18 | VFSD | 28.344 | 58.99 | 84.92 |\n\n# Methods\n\n**Plasmids and strains.** Genetic parts of constructs used in this study are provided in Supporting Information. All constructs were cloned into plasmid J64100_p15A with p15a origin of replication and chloramphenicol resistance gene by isothermal Gibson assembly. All experiments were performed using *E. coli* strain NEB10β (New England Biolabs). Plasmids and materials will be made available through Addgene. Sequences will be deposited into GENBANK.\n\n**Functional characterization of synthetic bile salt receptors.** Plasmids encoding different constructs were transformed into chemically competent *E. coli* NEB10β (New England Biolabs), plated on LB agar plates supplemented with 25 µg/mL chloramphenicol and incubated at 37ºC overnight. For each measurement, three fresh colonies were picked and inoculated into 5 mL of LB/chloramphenicol and grown at 37℃ with vigorous shaking for 16–18 hours. In the next day, the cultures were diluted 1:100 into 1 mL of LB/chloramphenicol medium with different concentration of bile salts in 96 deep-well plates (Greiner bio-one), incubated at 37℃ with vigorous shaking for a further 4 hours and analyzed by flow cytometry. All experiments were performed at least 3 times in triplicate on three different days. For bile salt specificity profiles for TcpPH-EMeRALD and VtrAC-EMeRALD systems, experiments were performed using each bile salt at a 80µM concentration. All chemicals used in this research were purchased from Sigma-Aldrich.\n\n**Calculation of Relative Promoter Units (RPUs).** Fluorescence intensity measurements among different experiments were converted into RPUs by normalizing them according to the fluorescence intensity of an *E. coli* strain NEB10β containing a reference construct and grown in parallel for each experiment. We used the constitutive promoter J23101 and RBS_B0032 as our in vivo reference standard and placed superfolder GFP as a reporter gene in plasmid pSB4K5. We quantified the geometric mean of fluorescence intensity (MFI) of the flow cytometry data and calculated RPUs according to the following equation:\n\nRPU = (MFIsample) / (MFIreference promoter)\n\n**Flow cytometry analysis.** Flow cytometry was performed using an Attune NxT cytometer coupled with high-throughput autosampler (Thermo Fisher Scientific) and Attune NxT™ Version 2.7 Software and BD LSR Fortessa (Becton Dickinson), with FACSDiVa software. 30,000 cells were collected for each data point. Flow cytometry data were analyzed using FlowJo (Treestar Inc., Ashland, USA). All raw data values are in Supplementary Information. FCS files have been deposited in Flow Repository (https://flowrepository.org/). IDs are available in supplementary file 2.\n\n**4 x NNK library construction.** Using P9-CadC-TcpP plasmid as template, the insert with 4 x NNK library was amplified by Phusion Flash High-Fidelity PCR Master Mix (Thermo Fisher Scientific) with the following primers: I5 - GGTCTCACAGCATCAATGTTCGGTGNNKNNK NNKNNKAAGACGTTGGAATGTACTAAGAACTAATAAAC, and I3 - GGTCTCAGGTCAATAA TACCGAAACTATTTTATTGTTC; the vector was amplified with the following primers: V5:GGTCTCAGACCACTTCCGAGTAGAATCG, and V3: GGTCTCAGCTGGTCGATAGCAAAGGTCAAC. The purified fragments were first digested with BsaI-HFv2 (New England Biolabs), and then ligated by T4 ligase at 4℃ overnight. 5 µg of ligation product was transformed into *E.coli* strain NEB10β with electroporation.\n\n**Cell sorting.** Cell sorting was performed using a S3 cell sorter (Bio-rad). 100,000 cells under different induction conditions (as shown in Fig. 3) were gated and collected in SOC medium at each round of sorting. The sorted cells were further inoculated in 10 mL of LB/chloramphenicol medium at 37°C with vigorous shaking for a further 16–18 hours. The cell cultures positively selected cells were then applied to the next round of selection. For the first two rounds, the loop variant library was induced with 200 µM of TCA. In the third round of evolution, cells were further induced at different concentrations of TCA to isolate more sensitive variants. For each round of screening, cells from an overnight culture were diluted 1:100 in LB with or without TCA and grown for 16 hours at 37℃ before being sorted.\n\n**Rosetta modeling.** Ab initio structural modeling. Structural models of the TcpP C-term segment (residues 182 to 211) were generated using the ROSETTA ab initio 3D prediction protocol68 with 1D sequence and 2D predicted secondary structure as input data.\n\n**Next Generation Sequencing.** Cells sorted from the third round of evolution were further induced with 320 µM of TCA to collect the fully activated TcpP variants. Plasmids extracted from sorted cells were further amplified and added UMI barcodes with first round primers (see supplementary materials for sequence details). After PCR clean up, the first round PCR products were further amplified by 2nd round PCR primers with NGS index. The PCR products were further purified with AMPure XP paramagnetic beads to remove the contaminants. Samples were sequenced on Illumina PE250 platform at Novogen (Hong Kong, China) with paired-end reads of 250 bases.\n\n**NGS data processing.** The datasets generated and analyzed during the current study are available in the NCBI SRA repository (BioProject ID: PRJNA714981 ; https://www.ncbi.nlm.nih.gov/bioproject/714981). The python scripts for NGS data processing are available upon request. Sequence counts were converted into amino acid sequences and listed in supplementary file 1. Sequence logos were prepared by R package Logolas69.\n\n**Colorimetric assay of bactosensors for bile salt detection.** Overnight cultures of TcpP-LacZ were diluted in 1/250 fold into 100 mL of LB with 25 µg/mL chloramphenicol, incubated at 37 ℃ for 4 hours to reach an OD600 of around 0.4. The cells were put on ice for 30 mins and then spun down at 4℃ and 2,200 g for 10 mins. The cell pellets were resuspended with LB medium (without antibiotics) at 1.1x of the final OD. 5 µL of different bile salts (prepared in LB medium) was added into 45 µL of resuspended cells in 96 well plates. The plate was incubated at 37℃ for 10–60 mins without shaking. After incubation, 50 µL of B-PER solution (Thermo Fisher) with 800 µM CPRG was added into the cell culture directly. The mixture was further incubated for 6 mins at room temperature and then 50 µL of 1M sodium carbonate was added to stop the reaction. The absorbance at 580 nm was measured with a plate reader (Biotek; Cytation3). For the clinical sample assay, serum samples were heat-inactivated by incubation in a 56℃ water bath for 30 mins. 5 µL of serum samples were added into 45 µL of resuspended cells in a 96 well plate and incubated at 37ºC without shaking for 2 hours before lysis.\n\n**Patient samples.** Serum samples were consecutively collected from hospitalized or ambulatory liver transplant patients at the Hepatology and Liver Transplantation Unit, Hôpital Saint-Eloi in Montpellier (France) in the month of July 2020. All patients underwent liver transplantation between November 2006 and April 2020. Clinical and biological data were also recorded for every patient included in the study from their medical files. Abnormal liver enzymes were defined by : alanine transaminase (ALT) > 41 U/L, aspartate transaminase (AST) > 40 U/L, alkaline phosphatase (ALP) > 130 U/L, gamma-glutamyl transferase (GGT) > 60 U/l or total bilirubin (TBil) > 21 µmol/L. 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A new sequence logo plot to highlight enrichment and depletion. *BMC Bioinformatics* **19**, 473 (2018).\n\n# Supplementary Files\n\n- [Supplementaryfile2RepositoryIDinFlowRespository.xlsx](https://assets-eu.researchsquare.com/files/rs-358332/v1/57331c5266f0b2a1fc015b86.xlsx) \n Flow repository IDs\n\n- [ChangEMeRALDSupplementary.pdf](https://assets-eu.researchsquare.com/files/rs-358332/v1/fd00fdcddf9e672adcdb1a78.pdf)\n\n- [DatabilesaltsExcel202103182.zip](https://assets-eu.researchsquare.com/files/rs-358332/v1/2ed881b813a5d075afd4dbe0.zip) \n Raw data\n\n- [ChangEMeRALDSupplementary.pdf](https://assets-eu.researchsquare.com/files/rs-358332/v1/e0a443dd00c4f62ceed8583b.pdf) \n Supplementary information\n\n- [Supplementaryfile1NGSdataofTcpPfunctionalvariants.xlsx](https://assets-eu.researchsquare.com/files/rs-358332/v1/94ad8da7e73845ccd60dc235.xlsx) \n NGS data\n\n- [BonnetEPCflat.pdf](https://assets-eu.researchsquare.com/files/rs-358332/v1/b56d5c18457ad2b1b8e516d6.pdf) \n Editorial Policy Checklist flat"} {"paper_id": "prb57", "title": "Formation of synthetic RNA protein granules using engineered phage-coat-protein -RNA complexes", "text": "# Abstract\n\nLiquid-solid transition, also known as gelation, is a specific form of phase separation in which the interacting molecules cross-link to form a highly interconnected compartment with solid – like dynamical properties. Here, we utilize RNA hairpin coat-protein binding sites to form synthetic RNA based gel-like granules via liquid-solid phase transition. we show both *in-vitro* and *in-vivo* that hairpin containing synthetic long non-coding RNA (slncRNA) molecules granulate into bright localized puncta. We further demonstrate that upon introduction of the coat-proteins, less-condensed gel-like granules form with the RNA creating an outer shell with the proteins mostly present inside the granule. Moreover, by tracking puncta fluorescence signals over time, we detected addition or shedding events of slncRNA-CP nucleoprotein complexes. Consequently, our granules constitute a genetically encoded storage compartment for protein and RNA with a programmable controlled release profile that is determined by the number of hairpins encoded into the RNA. Our findings have important implications for both the potential regulatory role that naturally occurring granules play and for the broader biotechnology and gene-expression sectors.\n\n# Introduction\n\nPhase separation, the process by which a homogeneous solution separates into multiple distinct phases, has been connected to a wide range of natural cellular processes in virtually all forms of life1–5. In cells, phase separation results in the formation of membrane-less compartments containing a high-concentration mix of biomolecules (e.g., proteins, RNA, etc.), which are surrounded by a low-concentration solution. Generally, phase separations are classified by the different material states which can lead to multiple types of transitions (e.g., liquid-solid, gas-liquid, etc.). The forms commonly reported in cellular biology are broadly liquid-liquid and liquid-solid (e.g., gelation), however determining the exact mechanisms for phase separation in a living cellular environment is often challenging5.\n\nLiquid-liquid phase transitions can be distinguished from liquid-solid by the dynamical properties of the resulting condensates. Liquid-based condensates show rapid internal rearrangement of molecules, fusions between different condensates upon contact, and dependency on the concentration of the molecules in the condensed phase6,7. On the other hand, liquid-solid based condensates show none of the above qualities and are mainly dependent on the number of ‘cross-linkers’, which are points of contact between the molecules, rather than on the concentration of the molecules themselves8–10.\n\nRecently, Jain & Vale11 reported on the formation of RNA granules both *in vivo* and *in vitro*, from highly repetitive RNA sequences associated with repeat expansion diseases. These RNA sequences, comprised of dozens of triplet-repeats of CAG or CUG nucleobases, form intramolecular hairpin structures12, which facilitate multivalent intermolecular interactions. The RNA granules presented features associated with liquid-solid phase transition systems: a lack of internal mobility, virtually no fusion events, and dependence on the number of repeats in the RNA sequence (i.e., cross linkers) rather than the concentration of the RNA. These characteristics helped establish the granules as physical solids.\n\nHairpin forming RNA sequences are widespread in the RNA world and are not strictly associated with disease phenotypes. Such sequences are commonly used in synthetic systems for biological research. Perhaps the most ubiquitous system is composed of RNA sequences that encode for multiple hairpin motifs that can bind the phage coat proteins (CPs) of PP7 or MS2. Using this system to label the 5’ or 3’ end of a transcript has become commonplace in the last two decades13–18, and enables visualization of RNA transcripts when the CPs are co-expressed. This approach, originally introduced by Singer and others13–15, was devised for the purpose of probing the dynamics of transcription and other RNA-related processes, irrespective of cell-type. When co-expressed, the coat-protein-bound RNA molecules yield bright puncta, which are similar in appearance to natural biomolecular condensates. Consequently, we hypothesized that co-suspension of synthetic RNA hairpin cassettes together with their binding CPs can lead to the formation of gel-like particles via liquid-solid phase separation *in vitro*. In addition, by utilizing the CP binding ability of the hairpins, we expect to be able to selectively incorporate proteins of our choosing into the solid-like granules, resulting in a selective platform for the stable concentration of proteins.\n\nIn this paper, we rely on our previous works19–21 to design and synthesize a variety of PP7 coat-protein (PCP) binding synthetic long non-coding RNA molecules (slncRNAs). Using fluorescent RNA nucleotides, we show that these slncRNAs form isolated puncta *in vitro* in a manner dependent on the number of hairpins encoded into the RNA. We further show that addition of fluorescent PCP to the suspension results in almost complete co-localization between protein and slncRNA. By tracking puncta fluorescence signals over time, we demonstrate that for all slncRNAs used, the various puncta emitted similar signals characterized by bursts of increasing or decreasing fluorescent intensity. We further show that signal intensities and temporal characteristics are dependent on the number of hairpins present in the RNA. Using these observations, we conclude that these “fluorescence-bursts” corresponded to addition or shedding of slncRNA-PCP nucleoprotein complexes. These events occur at rates that are consistent with the puncta being phase-separated solid-like granules. Consequently, we present these slncRNA-protein granules as a genetically encoded platform for the selective storage of proteins as well as a model system for exploration of liquid-solid phase separation.\n\n# Results\n\nHairpin containing RNA phase separates *in vitro* into gel-like granules\n\nTo test whether hairpin containing RNA can phase separate *in vitro* we designed six synthetic long non-coding RNA (slncRNA) binding-site cassettes using our binding site resource19–21. We divided our slncRNAs into two groups. For the first group (class I slncRNAs), we designed three cassettes consisting of three, four, or eight hairpins that encode for PCP binding sites (PCP-3x, PCP-4x, and PCP-8x, respectively). In this group, hairpins were spaced by a randomized sequence that did not encode for a particular structure. For the second group (class II slncRNAs), we encoded three cassettes that consisted of three, four, and fourteen PCP binding that were each spaced by hairpin structures that do not bind PCP (PCP-3x/MCP-3x, PCP-4x/MCP-4x, and PCP-14x/MCP-15x, respectively). The sequences encoding for the slncRNAs were cloned downstream to a pT7 promoter and transcribed *in vitro* to generate the corresponding RNA. To visualize the RNA, we incorporated fluorescent nucleotides in the transcription reaction such that an estimated 30% of uracil bases were tagged by Atto-488 fluorescent dye. Each slncRNA-type was separately mixed with granule forming buffer (see methods and Figure. 1a) at equal concentration (8.5 nM final concentration) and incubated for 1 hour at room temperature. 2 µl of the granule reaction were then deposited on a glass slide and imaged using an epi-fluorescent microscope.\n\nThe images show formation of a multitude of bright localized fluorescent condensates for all slncRNA types except for the PCP-3x case, where no such structures were detected (Figure 1b). In addition, the longer slncRNA molecules (e.g., PCP-8x and PCP-14x/MCP-15x) also exhibit larger structures, consistent with a gel like solid network, in addition to the smaller condensates or puncta. An examination of the median fluorescence obtained for each slncRNA type condensate (Figure 1c) reveals a dependence on the number of fluorescently labelled uracil nucleotides or the number of hairpins encoded into the slncRNA. However, the relationship between the median fluorescence values obtained for each species is not consistent with a linear dependence on hairpins, and instead suggests a more complex set of structures.\n\nTo further analyze the condensate structure, we fitted the measured condensate fluorescence intensity distributions to a modified Poisson distribution (see Figure 1d, Figure S1 and Supplementary methods). The panels reveal three characteristic distributions. For PCP-4x, an exponential distribution is recorded (i.e., λ=0). For PCP-3x/MCP-3x, PCP-4x/MCP-4x, and PCP-8x, a Poisson distribution of λ~1-2 seems to be the best fit. Finally, for the PCP-14x/MCP-15x, a Poisson distribution of λ~3-5 fit best. These results are consistent with the formation of condensates that are characterized by an increasing number of slncRNA molecules that are cross-linked to form a gel-like \"granule\", where the number of hairpins encoded into the slncRNA determines the average number of molecules or cross-links within the observed field of granules. Moreover, the interpretation suggested by the shape of the distribution is contrasted by the counter-intuitive observation of decreasing value of the of the fitting parameter *K*0 as a function of an increasing number of hairpins (Figure 1e). In this particular context, this observation is manifested by a significantly more gradual increase in mean or median granule fluorescence as compared to what would be naively expected by a simple rescale that takes into account the number of hairpins. Together, these observations suggest that slncRNA granules form via cross-linking interaction of multiple slncRNA molecules, and that an increasing number of hairpins and cross-links lead to a denser condensate. Denser granules, in turn, may result in fluorescence quenching of the labelled uracils22 leading only to a gradual and disproportionate increase in fluorescence observed.\n\nRNA-based granules co-localize with protein-binding partners\n\nTo test if the hairpins retain their ability to bind the PP7 phage coat protein while in the granule state, we added recombinant tandem dimer PP7 coat protein fused to mCherry (tdPCP-mCherry) to the granule formation reaction in excess amount (final concentration 25 nM) to account for the multiple binding sites present on one slncRNA molecule (Figure 2a). The tdPCP-mCherry version used lacks the necessary moiety to form the wildtype viral capsid23. The images (Figure 2b) show colocalization between the 488 nm channel (Atto-488) and the 585 nm channel (mCherry) for all slncRNA designs used in the experiment implying that PP7 coat proteins are able to bind the RNA hairpins in the condensate state. Hence, the slncRNA and their protein partners form synthetic RNA-protein (SRNP) granules. Unexpectedly, PP7-3x granules were witnessed in the presence of the protein, implying that tdPCP-mCherry adds a measure of multivalency to the system, and thus triggers condensation of RNA molecules that do not phase separate on their own. To check that this condensation was hairpin dependent, we tested whether a control RNA (of the same length and GC content as PCP-8x) containing no designed hairpin condensed either on its own or in the presence of tdPCP-mCherry forms granules. In both cases, no condensates were detected in either the 488 nm or 585 nm channels (data not shown). Finally, unlike for the slncRNA only case, SRNP granules (particularly for high number of hairpins) show an increased propensity to form large-scale extended structures, suggesting a more complex structure formation and condensation for the SRNP granules as compared with the slncRNA-only case.\n\nNext, we measured the median fluorescence intensity of the mCherry protein in different SRNP granules. The distributions of median values (Figure 2c) show a clear dependence on the number of binding sites available for protein binding. First, the PCP-3x/MCP-3x and PCP-4x granules appear to have a similar number of proteins in the granule and are both weaker than PCP-4x/MCP-4x granules, suggesting that PCP-4x slncRNAs inside the granules are not fully occupied by proteins. In addition, the PCP-14x/MCP-15x granules seems to be >2-fold brighter as compared with the PCP-8x granules, despite having <2-fold the number of hairpins. This stands in contrast to the observation that PCP-14x/MCP-15x granules appear to be ~3 times brighter than PCP-4x/MCP-4x granules, reflecting the difference in the number of binding sites available for binding. Finally, PCP-3x granules appear to be half as bright as PCP-14x/MCP-15x granules, providing more evidence that the former are not RNA-dependent entities. We also observe that when the spacing regions within the slncRNA encode for the MCP hairpins, the formed granules contain a larger protein cargo.\n\nTo confirm this observation, we also observed the SRNP granules in the 488 nm channel. Here a similar image emerges, whereby the median fluorescence values for each granule are percentage-wise more differentiated as compared with the slncRNA-only case, reflecting a more proportional increase in fluorescence (Figure. 2d). Together, the observations in both channels indicate that SRNP granules are less dense gel-like structures as compared with the slncRNA-only granules. To authenticate the granules as being solid-like RNA-protein structures, we imaged them using a SIM super resolution microscope with 120 nm resolution. Figure 2e shows a sample image of a PCP-14x/MCP-15x granule containing the tdPCP-mCherry protein. The image shows that slncRNA is found mainly in the periphery of the granule, with filaments protruding into its core, where a high amount of protein is amassed in a network like configuration. The RNA seems to encase the protein cargo in a reduced density structure.\n\nFinally, we explored the phase space of SRNP granule formation. To do so, we characterized formation of the PCP-14x/MCP-15x SRNP granules as a function of both slncRNA and protein concentration. For this we produced non-fluorescent RNA molecules (for higher concentrations) and mixed different titers of slncRNA and tdPCP-mCherry protein, each varied over two orders of magnitude. Puncta like structures were detected only for slncRNA and proteins concentrations of 100 ng/μl and above (Figure. 2f). The images display bright puncta that are embedded within a filamentous structure. Quantification of the maximal intensity of the puncta both at time T=0 (i.e., beginning of the reaction) and time T=1 [hr] (Figure. 2g) reveals a fluorescent intensity distribution which declines by two orders of magnitude (i.e., from ~105 to ~103) in a step-like function as the RNA concentration is reduced from 1000 to 10 ng/μl, providing further indication that RNA is essential for granule formation. Likewise, the intensity distribution of the puncta declines in a more gradual fashion as the protein concentration is reduced, but overall, a similar disappearance of puncta is observed.\n\nTemporal tracking of individual SRNP granules reveals that granules function as protein capacitors\n\nA hallmark of phase separation is the exchange of molecules between the dilute phase and the dense phase. This is also true for gels with non-permanent intermolecular interactions, wherein random breaks and rearrangement of the connections which form the inner network allow macromolecules (monomers and small polymers) to diffuse in and out of the gel phase8–11, albeit at a slow rate. These exchange events are predicted to occur independently of one another, at a rate which depends on multiple parameters: the probability of cross linking within the gel network (i.e., number of hairpins), the transient concentration of the molecules in the surrounding solution, and the average diffusion rate of the monomers. The movement of molecules (fluorescent CPs, slncRNA, and CP-bound slncRNA complexes) between the different phases should be reflected by changes in granule fluorescence intensity.\n\nTo test whether the synthetic granules display this characteristic, we tracked the fluorescence intensity of each granule in a given field-of-view for 60 minutes. We analyzed the brightness of each granule at every time point using a customized analysis algorithm (see Supplementary Methods). The resulting signals are either decreasing or increasing in overall intensity, and dispersed within them are sharp variations in brightness, that are also either increasing or decreasing. Next, we employed a statistical threshold which flagged these signal variation events, or “signal bursts”, whose amplitude was determined to not be part of the underlying signal distribution (p-value<1e-3) (See Supplementary Methods for definitions of bursts, algorithm details, and relevant numerical controls). The events were classified as either increasing bursts (green), decreasing bursts (red), or non-classified segments (blue), which are segments where molecular movement cannot be discerned from the noise (Figure. 3a). For each detected burst, we measure its amplitude (Δ intensity) and duration (Δ time), in addition to measuring the time between bursts and the order of their appearance. In Figure. 3b we plot the distributions of amplitudes for all three event types, obtained from ~156 signal traces, each gathered from a different granule composed of PCP-14x/MCP-15x and tdPCP-mCherry. We observe a bias towards negative burst or shedding events. Assuming an interpretation that fluorescent burst events correspond to insertion and shedding events of slncRNA-CP complexes into or out of the synthetic granules, the amplitude bias towards negative events is consistent with RNA degradation and lack of transcription within the *in vitro* suspension, leading to a net shedding of slncRNA molecules out of the granules over time.\n\nWe repeated the tracking process for granules produced from all previously-described slncRNA designs (including the PP7-3x which does not phase separate on its own). Comparison of the amplitude distributions per design (class I vs. II), (Figure. 3c) reveals a dependence on the number of hairpins available for protein binding, where more protein binding sites translate directly into larger amplitudes. Next, we also measured burst amplitude in the green-channel to confirm that bursts indeed correspond to the shedding of a slncRNA-protein complex from the granule. Figure. 3d shows a sample signal for the PCP-14x/MCP-15x granules showing concomitant occurrence of bursts in both the red and green channels, supporting our interpretation of this signal. Using the burst distributions, we then computed the ratio between the mean granule fluorescence and the mean burst amplitude, providing a measure for the number of slncRNA molecules within the granule. The results (Figure. 3e-f) show that with the exception of the PCP-4x based SRNP granules, the ratio in the green channel is 5, suggesting that a typical granule contains five slncRNAs. The ratio computed for the red channel is typically smaller, and for PCP-8x is ~2. This means that in every burst approximately half the protein content is released with the RNA. This further implies that PCP-8x may be permeable to proteins diffusing out of the granules due to reduced cross-linking as a result of a lack of hairpin spacing structures. For the PCP-3x/MCP-3x, PCP-4x/MCP-4x, and PCP-14x/MCP-15x the ratio in the red channel is approximately equal to that of the green channel, suggesting that these granules have a better protein storage capacity. Hence, the granules composed of class II slncRNA seem to form more robust and better insulated granules from the perspective of their protein storage capacity.\n\nTo provide further evidence for this interpretation, we measured the time duration between events for each granule type. For the granules, this rate (~5 minutes) is two orders of magnitude above the typical rate observed in liquid phase separated condensates24, but is in line with the measurements performed on RNA gels by Vale et. al.11, providing additional confirmation that the SRNP granules are gel-like particles. A closer examination of the duration boxplots (Figure. 3g) obtained for each granule-type reveals that more binding sites lead to longer durations on average, for both negative and positive bursts. Additionally, there appears to be a difference between the slncRNA designs themselves. While the granules composed of class I slncRNA granules present on average longer durations between positive bursts, compared to negative bursts, the opposite is true for the class II slncRNAs. Assuming a roughly uniform distribution of molecules outside of the granule (given enough time to equilibrate), this may mean that on average, a protein-bound slncRNA molecule has a higher probability of leaving a class I slncRNA granule than entering it, and vice versa for the class II slncRNA granules. This result confirms the interpretation of the burst ratio analysis, and together these results imply that class II granules are characterized by a highly-cross-linked slncRNA network which prevents the diffusion away of molecules (leading to a longer time between negative bursts), while the granule boundary still contains free cross-linking points that can latch on to incoming molecules more easily, increasing the chances of molecular entry (leading to a shorter time between positive bursts). Together, these SRNP granule characteristics are reminiscent of data and energy storage devices (e.g., capacitors), with the protein cargo replacing the electric charge in the biochemical analog.\n\nExpression of slncRNAs and protein in bacteria yields puncta-like condensates\n\nGiven the capacitor analogy, we hypothesized that *in vivo* the granules can be used as devices that store the granule-bound proteins. This is due to the steady state production of slncRNAs and proteins via the cellular transcriptional and translational machinery, that ensures a constant flux of proteins into the granules. To show this, we first proceeded to test whether the granule material characteristics that are measured *in vivo* match the *in vitro* measurements. To do so, we decided to utilize two previously reported slncRNA designs which were shown to yield bright localized puncta *in vivo* in earlier work19. The first slncRNA is of a class II design, PCP-4x/ QCP-5x, consisting of four native PCP binding sites and five native Qβ coat protein (QCP) hairpins used as spacers in an interlaced manner. The second slncRNA is the ubiquitous PCP-24x cassette25, which from the perspective of this work can be regarded as a class I design slncRNA.\n\nTo confirm the granules form conditions *in vivo*, we encoded the slncRNA component under the control of a T7 promoter, and the tdPP7-mCherry under the control of an inducible pRhlR promoter (Figure. 4a). We first wanted to test whether puncta develop *in vivo* and whether they are dependent on the existence of hairpins in the RNA. For this we co-transformed plasmids encoding either the negative control RNA or the PCP-4x/QCP-5x slncRNA, together with a plasmid encoding for the tdPCP-mCherry protein, into BL21-DE3 *E. coli* cells. Examination of cells expressing the slncRNA and protein following overnight induction of all components revealed the formation of bright puncta at the cell poles (Figure. 4b), which were absent in cells expressing the control RNA which lacks hairpins (Figure. 4c).\n\nNext, to test whether cellular concentration of slncRNA influences the formation of the granules, we quantified the fraction of puncta per cell for cells expressing the PCP-4x/QCP-5x from a multicopy expression vector, and cells expressing the same slncRNA from a bacterial artificial chromosome (BAC) expression vector which is maintained at a single copy level in cells. We found that cells containing the multicopy plasmid frequently present puncta in at least one of the poles, while cells containing the single copy generally show between zero and one punctum (Figure. 4d). Given that cells expressing the slncRNAs from single copy vectors still present puncta, we decided to continue using this expression vector in follow-up experiments to reduce variability stemming from copy number differences.\n\nWe compared cells expressing the PCP-4x/ QCP-5x or the PCP-24x (expressed from a BAC vector) in terms of the spot per cell fraction. Much like in the *in vitro* experiments, we found a dependence on the number of binding sites in accordance with the *in vitro* results and the cross linking model of gel phase formation6,26 (Figure. 4d). Finally, to test whether the polar localization of the granules is a consequence of nucleoid exclusion27, we grew the cells in starvation conditions for several hours, triggering a transition to stationary phase. In stationary phase the nucleoid is known to condense28–30, thus increasing the amount of cellular volume which is likely to be molecularly dilute. This, in turn, generates a larger accessible cellular volume for granule formation, which should lead to different presentation of the phase-separation phenomena as compared with exponentially growing cells. In Figure. 4e, we show images of bacteria displaying ‘bridging’ (the formation of a high intensity streak between the spots) of puncta (left), whereby granules seem to fill out the available dilute volume, and the emergence of a third puncta at the center of the cell (right). Both behaviors are substantially different than the puncta appearing under normal conditions. Such behavior was observed in >40% of the fluorescent cells and was not detected in non-stationary growth conditions. Thus, SRNP granules with characteristics that are consistent with the *in vitro* observations form *in vivo*, in a semi-dilute bacterial cytosolic environment and independent of cell-state.\n\nslncRNA expression increases cellular protein concentration\n\nTo investigate the dynamic properties of granules formed *in vivo*, we utilized the same analysis approach as was used in the *in vitro* experiments, with minor differences. Normalizing the fluorescence of the granule by that of the cell (see methods) for every time point results in a signal vs. time trace largely independent from the effects of photobleaching and cellular background noise, allowing us to search for and measure burst events, as was done previously. In Figure. 5a, we plot the distributions of amplitude (Δ intensity) of all three event types (positive, negative, and non-classified), obtained from 255 traces gathered from cells expressing the PCP-4x/QCP-5x slncRNA together with the tdPCP-mCherry protein. The symmetry in both shape and spread of the negative and positive distributions indicates that both are measurements of the same type of macromolecule, distinguished only by the direction in which it travels (into or out of the granule). Moreover, a similarly symmetric burst distribution is recorded for the PCP-24x slncRNA (Figure S1). This result contrasts with the *in vitro* amplitude distribution data (Figure 3b), which presented a skewness towards negative bursts. This implies that *in vivo*, the transcriptional and translational processes in the cell balance the loss of granule components due to degradation.\n\nNext, we measured the amplitudes of the bursts for both slncRNAs and found that positive and negative amplitudes are proportional to the number of binding sites within the encoded cassette (Figure 5b). In addition, a more quantitative analysis of these distributions (Figure S2) reveals that a single burst for the 24x cassette is ~2.5-3x more fluorescent as compared with the 4x cassette, indicating that the molecules transitioning in and out of the 24x granules are slncRNAs partially or fully bound rather than lone proteins. Moreover, estimations of the positive and negative amplitudes are practically equal per slncRNA, providing additional evidence that these are in fact representations of one physical process, with the difference being the directionality of the transitioning slncRNA-protein molecule. Finally, we measured the duration between burst events, revealing that slow shedding and absorption processes on the order of minutes are taking place for the *in vivo* granules as well (Figure 5c). Altogether, the non-existence of puncta in cells expressing the negative control RNA, the slow exit/entry rate of molecules, and the dependence on the number of binding sites, suggest that synthetic RNA protein granules are phase separated condensates *in vivo* and possess the same gel-like characteristics that were observed for the *in vitro* suspensions. Consequently, *in vivo* burst analysis is consistent with the capacitor model, where the amount of protein stored within the SRNP granule seems to be in steady state when there is a steady supply of protein and slncRNA.\n\nNext, to ascertain whether the granules facilitate increased protein titers *in vivo* in accordance with the capacitor model predictions, we measured for each bright granule the mean fluorescence intensity (Figure 5d), and the mean intensity of the cell which contains it (Figure 5e). We observed a dramatic increase in mean cellular fluorescence between cells which express only tdPCP-mCherry and cells which express it together with a slncRNA, suggesting that slncRNA molecules have some effect in the cytosol, regardless of the granules. To quantify this phenomenon more accurately, we measured the total fluorescence of the population using flow cytometry. For this, we grew cells expressing only the protein component (tdPCP-mCherry), and cells expressing both protein and a slncRNA (PCP-4x/QCP-5x or PCP-24x), with different combinations of induction: IPTG (induces the slncRNA) and C4HSL (induces the protein). The data (Figure 5f) shows that cells expressing a slncRNA, regardless of induction (due to T7 leakiness), show higher fluorescence than cells expressing the protein only. In addition, induction of slncRNA expression with IPTG results in an increase in fluorescence, indicating that slncRNA is a deciding factor in this behavior. Finally, cells expressing the PCP-24x slncRNA show higher fluorescence than cells expressing PCP-4x/QCP-5x, displaying a dependence of the cellular protein titer on number of binding sites available for protein binding.\n\n# Discussion\n\nIn this study, we show that synthetic gel-like RNA – protein granules can be designed and assembled using phage coat proteins and RNA molecules that encode multiple CP binding sites, both in suspension and *in vivo*. Using fluorescently labelled RNA, we show that granule formation is nucleated by RNA-RNA interactions that are proportional to the number of hairpins encoded into the RNA. In addition, the binding of the proteins seems to further enhance and assist the granule formation process. Using fluorescent single molecule signal analysis, we reveal entry and exit events of molecules into and out of the granules. By investigating their size and rate of occurrence, we show that these events correspond to entry and shedding of protein-bound slncRNA molecules, and that they are dependent on the number of hairpins available for protein binding. Transitioning of macro-molecules across a phase boundary is frequently observed in phase-separated condensates, particularly in liquid-liquid based system. In particular, the frequency of these transitions reflects the underlying order, internal interactions, and density of the condensed phase. While in liquid-liquid phase separation systems such transitions occur on the scale of seconds or less, here we observe shedding and insertion events on a much longer time scale of minutes or longer, that is more consistent with a solid or gel-like condensed phase. The slow release and strong internal interactions which keep the granules intact for long durations, combined with the selectivity of our system due to the RNA binding component, could be utilized as a programmable controlled release mechanism in suitable biological settings. Hence, our granules can be thought as protein and RNA storage modules akin to a capacitor, with a monophasic release profile that can be tuned based on the slncRNA design.\n\nWe further characterized two options for slncRNA design: a homogeneous design which is comprised of multiple CP hairpin binding site and non-structured spacing regions (class I), and a hybrid design which is comprised of hairpin binding sites and additional hairpins in the spacing regions (class II). We show that the design choice has implications for the granule’s protein-carrying capacity and dynamics. In particular, class II granules formed particles with increased cross-linking capability in the RNA-only granule, which in turn led to an increased ability to insulate the protein cargo in the SRNP granule phase. On the flip side, class I granules were characterized by decreased cross-linking in the RNA-only phase and increased permeability of the protein cargo in the SRNP-granule phase. In addition, class I granules displayed a faster shedding or dissolution rate, which in turn lead to a smaller protein cargo on average. This two-dimensional phase space of capacity vs. rigidity offers substantial flexibility and tunability when designing SRNP granules for a variety of applications.\n\nThe capacitor- or storage-like behavior displayed by the SRNP granules implies that *in vivo*, the granules together with the gene-expression machinery form a biochemical analog of an RC-circuit. In a conventional RC-circuit, energy is stored within the capacitor for release at a later time. Such circuits are often used to protect electrical devices against sudden surges or stoppages of power. Here, the protein and slncRNA flux into the cytosol correspond to the current, which results in the formation of fully \"charged\" SRNP granules. This genetically encoded slncRNA and protein storage facility, which is constantly maintained, effectively increases the protein and slncRNA content of the cell beyond the steady-state levels facilitated by standard transcription, translation, RNA degradation, and proteolysis. This storage capacity is precisely the function that is carried out by capacitors in RC-circuits, allowing electrical devices to function even after \"power\" is cut-off. In the case here, the granules can be used not only to increase levels of a protein of choice by nearly an order of magnitude (as shown in Fig. 5) without adversely affecting the cell, but may also provide a mechanism to increase the cell's ability to survive when a harsh or stressful environment is encountered. While the former may have important implications to the biotechnology sector, the latter may hint at an important function that natural granules (e.g., paraspeckles, p-bodies, etc.) may have evolved for *in vivo*. Further studies will be required to explore the biological relevance of RNP granules to the survivability of cells and organisms under various forms of stress.\n\n# Materials And Methods\n\n## Bacterial strains\n*E. coli* BL21-DE3 cells which encode the gene for T7 RNAP downstream from an inducible pLac/Ara promoter were used for all reported experiments. *E. coli* TOP10 (Invitrogen, Life Technologies, Cergy-Pontoise) was used for cloning procedures.\n\n## Addgene plasmids\npCR4-24XPP7SL was a gift from Robert Singer (Addgene plasmid # 31864; http://n2t.net/addgene:31864; RRID: Addgene_31864). \npBAC-lacZ was a gift from Keith Joung (Addgene plasmid # 13422; http://n2t.net/addgene:13422; RRID: Addgene_13422).\n\n## Construction of the slncRNA plasmids\nAll sequences encoding for the *in vitro* slncRNAs (i.e., PP7-3x, PP7-4x, PP7-3x/MS2-3x, PP7-4x/MS2-4x, PP7-8x and PP7-14x/MS2-15x) were ordered from Integrated DNA Technologies (IDT) (Coralville, Iowa) as gBlock gene fragments downstream to a T7 promoter and flanked by EcoRI restriction sites on both sides. gBlocks were cloned into a high-copy plasmid containing an Ampicillin resistance gene and verified using Sanger sequencing. \nThe 5Qβ/4PP7 slncRNA sequence was ordered from GenScript, Inc. (Piscataway, NJ), as part of a puc57 plasmid, flanked by EcoRI and HindIII restriction sites. pBAC-lacZ backbone plasmid was obtained from Addgene (plasmid #13422). Both insert and vector were digested using EcoRI and HindIII (New England Biolabs [NEB], Ipswich, MA) and ligated to form a circular plasmid. Sequence was verified by Sanger sequencing.\n\n## Design and construction of fusion-RBP plasmids\nFusion-RBP plasmids were constructed as previously reported 21. Briefly, RBP sequences lacking a stop codon were amplified via PCR off either Addgene or custom-ordered templates. Both RBPs presented (PCP and QCP) were cloned into the RBP plasmid between restriction sites KpnI and AgeI, immediately upstream of an mCherry gene lacking a start codon, under the so-called RhlR promoter containing the rhlAB las box 31 and induced by N-butyryl-L-homoserine lactone (C4-HSL) (Cayman Chemicals, Ann Arbor, Michigan). The backbone contained either an Ampicillin (Amp) or Kanamycin (Kan) resistance gene, depending on experiment.\n\n*In vitro* transcription of slncRNA \nA vector containing the slncRNA DNA sequence, flanked by two EcoRI restriction sites, was digested with EcoRI-HF (NEB, #R3101S) per the manufacturer’s instructions to form a linear fragment encoding the slncRNA sequence. The enzyme was then heat-inactivated by incubating the restriction reaction at 65⁰ C for 20 minutes. For fluorescently labelled RNA, 1 µg of the restriction product was used as template for in vitro transcription using HighYield T7 Atto488 RNA labeling kit (Jena Bioscience, Jena, Germany, RNT-101-488-S), according to the manufacturer’s instructions. Non-fluorescent RNA was transcribed using the HiScribe™ T7 High Yield RNA Synthesis Kit (NEB, #E2040S). Following *in vitro* transcription by either kit, the reaction was diluted to 90 µl and was supplemented with 10 µl DNAse I buffer and 2 µl DNAse I enzyme (NEB #M0303S) and incubated for 15 minutes at 37⁰ C to degrade the DNA template. RNA products were purified using Monarch RNA Cleanup Kit (NEB, #T2040S) and stored in -80⁰.\n\n## Protein expression and purification\n*E. coli* cells expressing tdPP7-mCherry fusion protein were grown overnight in 10 ml LB with appropriate antibiotics at 37⁰ C with 250 rpm shaking. Following overnight growth cultures were diluted 1/100 into two vials of 500 ml Terrific Broth (TB: 24 g yeast extract, 20 g tryptone, 4 ml glycerol in 1 L of water, autoclaved, and supplemented with 17 mM KH2PO4 and 72 mM K2HPO4), with appropriate antibiotics and induction (100 µl C4-HSL) and grown in 37⁰ C and 250 rpm shaking to OD600 > 10. Cells were harvested, resuspended in 30 ml resuspension buffer (50 mM Tris-HCl pH 7.0, 100 mM NaCl and 0.02% NaN3), disrupted by four passages through an EmulsiFlex-C3 homogenizer (Avestin Inc., Ottawa, Canada), and centrifuged (13,300 RPM for 30 min) to obtain a soluble extract. Fusion protein was purified using HisLink Protein purification resin (Promega) according to the manufacturer’s instructions. Buffer was changed to 1xPBS using multiple washes on Amicon columns (Biorad).\n\n*In vitro* granule microscopy \n*In vitro* experiments were performed in granule buffer (750 mM NaCl, 1 mM MgCl2, 10% PEG4000). Reactions were set up as follows: 8 µl granule buffer, 1 µl protein, 1 µl RNA and allowed to rest at room temperature for 1 hour. 1–2 µl from the reaction was then deposited on a glass slide and imaged in a Nikon Eclipse Ti-E epifluorescent microscope (Nikon, Japan). Excitation was performed at 488 nm (Atto 488) for experiments containing fluorescent RNA, and 585 nm (mCherry) wavelengths by a CooLED (Andover, UK) PE excitation system. Images were captured using the Andor iXon Ultra EMCCD camera with a 500 msec exposure time for 488 nm and 250 msec exposure time for 585 nm.\n\n*In vivo* microscopy \nBL21-DE3 cells expressing the two plasmid system (single copy plasmid containing the binding sites array, and a multicopy plasmid containing the fluorescent protein fused to an RNA binding protein) were grown overnight in 5 ml Luria Broth (LB), at 37⁰ with appropriate antibiotics (Cm, Amp), and in the presence of two inducers – 1.6 µl Isopropyl β-D-1-thiogalactopyranoside (IPTG) (final concentration 1 mM), and 2.5 µl C4-HSL (final concentration 60 µM) to induce expression of T7 RNA polymerase and the RBP-FP, respectively. Overnight culture was diluted 1:50 into 3 ml semi-poor medium consisting of 95% bioassay buffer (BA: for 1 L—0.5 g Tryptone [Bacto], 0.3 ml glycerol, 5.8 g NaCl, 50 ml 1 M MgSO4, 1 ml 10×PBS buffer pH 7.4, 950 ml DDW) and 5% LB with appropriate antibiotics and induced with 1 µl IPTG (final concentration 1 mM) and 1.5 µl C4-HSL (final concentration 60 µM). For stationary phase tests, cells were diluted into 3 ml Dulbecco's phosphate-buffered saline (PBS) (Biological Industries, Israel) with similar concentrations of inducers and antibiotics. Culture was shaken for 3 hours at 37⁰ before being applied to a gel slide [3 ml PBSx1, mixed with 0.045g SeaPlaque low melting Agarose (Lonza, Switzerland), heated for 20 seconds and allowed to cool for 25 minutes] 32. 1.5 µl cell culture was deposited on a gel slide and allowed to settle for an additional 30 minutes before imaging.\n\n## Live cell microscopy\nGel slide was kept at 37⁰ inside an Okolab microscope incubator (Okolab, Italy). 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Measuring Single-Cell Gene Expression Dynamics in Bacteria Using Fluorescence Time-Lapse Microscopy. *Nat Protoc* 2012, *7* (1), 80–88. https://doi.org/10.1038/nprot.2011.432.\n\n# Supplementary Files\n\n- [RNAgelssupplementaryinformation.docx](https://assets-eu.researchsquare.com/files/rs-1546005/v1/45c0356441627abfcb84a59f.docx) \n Supplementary Information"} {"paper_id": "prb58", "title": "Mucosal TLR2-activating protein-based vaccination induces potent pulmonary immunity and protection against SARS-CoV-2 in mice", "text": "# Abstract\n\nCurrent vaccines against SARS-CoV-2 substantially reduce mortality, but protection against infection is less effective. Enhancing immunity in the respiratory tract, via mucosal vaccination, may provide protection against infection and minimise viral spread. We tested a novel subunit vaccine in mice, consisting of SARS-CoV-2 Spike protein with a TLR2-stimulating adjuvant, delivered to mice parenterally or mucosally. Both routes of vaccination induced substantial neutralising antibody (nAb) titres, however, mucosal vaccination uniquely generated anti-Spike IgA, increased nAb in the serum and airways, and increased lung CD4+ T-cell responses. TLR2 is expressed by respiratory epithelia and immune cells. Using TLR2 deficient chimeric mice, we determined that TLR2 expression in either compartment facilitated early innate responses to mucosal vaccination. By contrast, TLR2 on hematopoietic cells was essential for optimal lung-localised, antigen-specific responses. In a K18-hACE2 mice, vaccination provided complete protection against disease and sterilising lung immunity against SARS-CoV-2. These data support mucosal vaccination as a strategy to improve protection in the respiratory tract against SARS-CoV-2 and other respiratory viruses.\n\n# Introduction\n\nThe emergence of SARS-CoV-2 in late 2019 and the subsequent global COVID-19 pandemic has led to substantial morbidity and mortality with currently over 260 million confirmed cases and 5.2 million deaths reported to the World Health Organisation. The development of vaccines against SARS-CoV-2 has reduced the morbidity and mortality associated with COVID-19 and limited the significant disruption to economies and freedom of movement arising from restrictive, but necessary, public health measures. Most current vaccines, either those approved for clinical use or in development, are delivered by intra-muscular injection and these predominantly induce systemic neutralising Immunoglobulin G (IgG) and T-cell responses, but poor mucosal responses¹. Serum IgG transudates into the lungs across the alveolar epithelium to reduce the risk of pulmonary viral infection, but does not prevent infection in the nasal passages and consequent virus shedding, unless neutralising serum IgG is at very high levels². Consequently, while the risk of infection and transmission is reduced by vaccination, breakthrough infections with ongoing spread can still occur³.\n\nOf concern is evidence for the waning of immunity post vaccination or infection⁴,⁵, combined with the impact of viral variants of concern (VOCs), including the very recent emergence of the Omicron variant⁶. Currently, resurgence of disease in highly vaccinated populations correlates with time since vaccination and also the emergence of the Delta variant⁷, for which there are suggestions that vaccine effectiveness and control of viral burden are reduced⁸. Additionally, issues surrounding vaccine equity, including affordability, transport of vaccines with complex storage requirements and ease of access, also remain to be fully addressed⁹. A large, partially protected population may create ideal evolutionary conditions to drive emergence of further VOCs with capacity for vaccine immune evasion characteristics or increased pathogenicity, including increased replicative capacity in the upper airway and consequent enhanced transmission. Thus, there remains a major need to continue investing in vaccine development for SARS-CoV-2.\n\nEnhancing mucosal immunity to provide a barrier against infection may increase protection, and importantly, minimise viral spread¹⁰. Mucosal vaccination has shown exciting potential in pre-clinical studies for multiple respiratory pathogens, generating immunity in the lower respiratory tract to prevent morbidity and mortality. Immunoglobulin A (IgA), which is actively transported across respiratory epithelium as a stabilized dimer¹¹, as well as resident memory B and T cells in the lungs, nasal passages and upper airways, is elicited by intranasal vaccination and can prevent infection and reduce viral shedding¹². In animal models, intranasal vaccination against SARS-CoV-2 can provide barrier protection against infection in both the lung and upper respiratory tract (URT), via the generation of secretory nAbs and memory T-cells in the mucosa¹³–¹⁹. Currently, primarily live-attenuated viruses or viral vector-vaccines have been used for mucosal vaccination, but these may have safety concerns and cannot be used for repeat booster immunization because of anti-vector immunity. Protein vaccines overcome these concerns and provide a cost-effective strategy that is suitable in a wide range of populations, include young, aged²⁰ and immunocompromised groups. However protein vaccines require the inclusion of appropriate immune stimulants to enhance their immunogenicity, and effective and safe mucosal adjuvants are urgently required¹⁰. In addition, direct activation of the respiratory epithelium may increase the delivery of soluble proteins to gain access to antigen presenting cells for immune activation²¹.\n\nToll-like-receptor 2 (TLR2) is an activating innate immune receptor expressed by both the respiratory epithelium and lung immune cells²²–²⁴, and is required for effective host defence against infection²⁵. We and others have recently shown that the TLR2 ligand, Pam₂Cys, is a highly effective mucosal adjuvant for peptide or protein-based vaccines²⁶–²⁸, 29,30. Pulmonary immunization with mycobacterial peptides or protein conjugated to Pam₂Cys stimulated protective immunity in the lung against *Mycobacterium tuberculosis* infection²⁶–²⁸. Thus, we examined the pattern of lung and systemic immune responses induced by a novel subunit vaccine, consisting of recombinant trimeric SARS-CoV-2 Spike protein admixed with the TLR2-stimulating adjuvant Pam₂Cys (Pam₂Cys Spike), delivered via the mucosal or systemic route. To establish the contribution of TLR2-expression by respiratory epithelia and lung immune cells to the mucosal vaccine response, we developed chimeric mice expressing TLR2 on haemopoietic cells or the epithelium and examined early innate responses and adaptive immunity after mucosal vaccination. Finally, the protective efficacy of the vaccine following mucosal and parenteral delivery was assessed in the K18-hACE2 murine model of SARS-CoV-2 infection³¹.\n\n# Results\n\n**Pam₂Cys Spike vaccination induces potent lung antibody and CD4⁺ T-cell responses**\n\nTo compare immune induction by parenteral versus mucosal Pam₂Cys Spike vaccination, C57BL/6 mice received three homologous immunizations two weeks apart, either by subcutaneous (s.c) injection or intranasal (i.n) instillation. Immunogenicity was assessed at one-week post-final vaccination by comparison to unvaccinated mice (Fig. 1a). Vaccination by either route induced potent titres of anti-Spike IgG in serum (10⁸) and broncho-alveolar lavage fluid (BALF) (10⁷), determined by ELISA, and this was significantly increased in mucosally immunized mice (Fig. 1b). Strikingly, anti-Spike IgA was only detected in the serum or BALF of i.n immunized mice, where it was present at very high titres. The neutralizing potential of these antibodies was assessed in a pseudovirus assay, using infection of HEK293-ACE2 cells with a SARS-CoV-2 Spike-expressing lentivirus (Fig. 1c), as well as against virulent SARS-CoV-2 infection of VeroE6 cells (Fig. 1d). nAb titre was defined as the dilution required to inhibit 50% of infection in either system (EC₅₀). Both s.c or i.n vaccination induced potent nAb titres in serum, however mucosally immunized mice had significantly greater nAb, and only the mucosal immunization route resulted in significantly elevated nAb in the airways.\n\nThe generation of local and systemic Spike-specific T-cell responses was assessed by ex vivo recall stimulation of lung and spleen leukocytes with Spike protein in the presence of Brefeldin A, intra-cytoplasmic cytokine staining and quantitation by flow cytometry (gating strategy in Fig. S1). Mucosally immunized mice had a substantial population of Spike-specific CD4⁺ T-cells locally in the lungs, predominantly secreting IL-17 (Fig. 2a), and a more diverse response systemically in the spleen, with IL-2, IL-17 and TNF-secreting populations significantly increased (Fig. 2b). No significantly increased populations of Spike-specific CD8⁺ T-cells secreting IFNγ, IL-2 or TNF were detected (Fig. 2c,d). Therefore, Pam₂Cys Spike vaccination was potently immunogenic, inducing powerful anti-SARS-CoV-2 nAb responses in serum, with i.n vaccination providing superior humoral and CD4⁺ T-cell responses in the lungs and airways.\n\n**TLR2 on both respiratory epithelia and lung immune cells contribute to early innate immune responses to mucosal vaccination**\n\nTLR2 is expressed by both the respiratory epithelia and lung immune cells¹²⁻¹⁴, and is required for effective host defence against infection¹⁵. We hypothesised that both compartments may contribute to mucosal vaccine responses, providing an explanation for the powerful immunity induced by i.n delivery of Pam₂Cys adjuvanted vaccines. To determine the role played by each compartment, irradiated wild type (WT; BALB/c) and TLR2 deficient (Tlr2⁻/⁻) mice¹⁴,¹⁵ were reconstituted with either WT or Tlr2⁻/⁻ (KO) bone marrow (BM), to create mice with TLR2 expression on neither compartment (KO/KO BM), immune cells only (KO/WT BM), non-immune cells only (WT/KO BM) or both compartments (WT/WT BM). Mice were rested for 12-weeks to allow hematopoietic reconstitution and replacement of radiation-resistant populations in the lungs and airways. To assess early innate responses to mucosal vaccination, mice were immunized i.n with Pam₂Cys Spike once, then immune populations of the lungs and airways examined by flow cytometry at 24-hours post vaccination (Fig. 3a).\n\nComputational analysis of lung leukocytes was first performed using the Spectre R package³², to perform unbiased clustering of all CD45⁺ cells. To verify bone marrow replacement, relative expression of TLR2 was examined by FIt-SNE, with expression above background detected only in mice receiving WT BM (Fig. 3b). Clusters with the highest degree of expression were identified, based on phenotypic markers, as alveolar macrophages (SiglecF⁺ CD11chi), neutrophils (Ly6G⁺ CD11bhi), and other myeloid subsets including DC (SiglecF⁻ CD11c⁺) and monocyte subsets (Ly6Chi CD11bhi, Ly6Cmid CD11bhi) (Fig. S2). Manual gating in FlowJo was then performed to identify these subsets, as well as other immune populations of interest (gating strategy in Fig. S3) and TLR2 expression on these cellular populations determined (Fig. S4). A comparison of the proportion of lung immune populations revealed that mice expressing TLR2 either on non-immune or immune compartments, had a similar lung immune profile post vaccination, which was dominated by neutrophil (Ly6G⁺ CD11bhi) influx (Fig. 3c). Quantitation of total lung leukocytes and neutrophil count also demonstrated a consistent elevation in mice expressing TLR2 on either compartment (Fig. 3d). Notably, however, innate cells that include classic antigen presenting cells, including dendritic cells (DC; SiglecF⁻ CD3⁻ B220⁻ CD11c⁺ MHCIIhi), alveolar macrophages (SiglecF⁺ CD11chi) and a monocyte subset (SiglecF⁻ CD3⁻ B220⁻ CD11c⁻ CD11bhi Ly6Cmid), were significantly elevated in mice that had TLR2 expression on non-immune cells, or both non-immune and immune cells (Fig. 3d). This was despite the expression of TLR2 on these cells only in mice that received WT BM (Fig. S4). Thus, activation of TLR2 on the respiratory epithelia plays a key role in recruiting these innate immune cells to the lungs early after mucosal vaccination.\n\nExamination of immune phenotypes in BALF samples revealed a similar pattern, whereby mice expressing TLR2 on either immune or non-immune cells had a similar profile of immune recruitment into the airways, dominated by neutrophils (Fig. S5a). Quantitation of total BALF leukocytes and neutrophils also demonstrated a consistent elevation in mice expressing TLR2 on either compartment (Fig. S5b). By contrast, other innate populations displayed a different pattern in BALF compared to lung tissue. Minimal changes were observed in alveolar macrophages and DCs, but elevation of a monocyte subset (SiglecF⁻ CD3⁻ B220⁻ CD11c⁻ CD11bhi Ly6Cmid) occurred in all groups expressing TLR2, and a significant elevation of inflammatory monocytes (SiglecF⁻ CD3⁻ B220⁻ CD11c⁻ CD11bhi Ly6Chi) was observed only in mice expressing TLR2 on immune cells (Fig. S5b). TLR2 expression on these cells was confirmed only in groups of mice receiving WT BM (Fig. S6). Thus, TLR2 on both respiratory epithelia and immune cells plays a role in early innate immune responses to Pam₂Cys Spike mucosal vaccination. Expression on either compartment is sufficient for neutrophil recruitment, but expression on non-immune cells leads to increased populations of antigen presenting cells, such as DC, in the lungs.\n\n**TLR2 on immune cells is required for optimal adaptive responses to mucosal Pam₂Cys Spike vaccination**\n\nTo determine the impact of TLR2 expression on non-immune versus immune cells on the generation of adaptive immune responses, a similar experimental protocol was performed, but mice received three i.n vaccinations with Pam₂Cys Spike, each 2 weeks apart (Fig. 4a). The immune profile in the lungs was examined 1 week post final booster vaccination. Computational clustering analysis of all lung leukocytes was again performed to examine the relative expression of TLR2 and verify bone marrow replacement (Fig. 4b). At this time point after booster vaccination, clusters with the highest degree of TLR2 expression were identified as alveolar (SiglecF⁺ CD11chi) and interstitial (SiglecF⁻ CD64⁺ CD11bhi) macrophages (Fig. S7). Manual gating in FlowJo was performed to quantitate these cells and confirm their TLR2 expression, and examine other immune cell populations of interest (Fig. S8). There was a significant increase in total lung leukocytes in groups expressing TLR2 on immune cells, and of interest, a substantial increase in both the proportion and number of T-cells, particularly CD4⁺ T-cells (Figs. 4c,d). A significant increase of B-cells (B220⁺ CD11c⁻) was apparent in Tlr2⁻/⁻ mice receiving WT BM, but not in WT mice receiving WT BM. In contrast, mice without TLR2 on immune cells against either a WT or Tlr2⁻/⁻ background, had a similar profile of lymphocyte populations.\n\nSpike antigen-specific humoral and T-cell responses were also examined. While all mice had detectable Spike-specific IgG responses in serum and BALF, expression of TLR2 on either immune or non-immune cells was required for the generation of substantial titres of IgG or IgA (Fig. 5a). There was a clear advantage in mice with expression of TLR2 on immune cells, with these groups generating significantly greater IgG and IgA titres, and importantly nAb in both serum and BALF (Fig. 5b). Consistent with this finding, while there was no change between groups in the proportion of total CD3⁺ CD4⁺ cells in the mediastinal lymph node (MLN), mice with TLR2 on immune cells had a significant increase in the proportion of Bcl6⁺ CD4⁺ T-cells, consistent with an increased T-follicular helper response (Fig. 5c, gating strategy in Fig. S9). In the lung tissue, Spike-specific cytokine secreting CD4⁺ T-cells again were significantly upregulated only in groups with TLR2 on immune cells, in particular IL-17A⁺ and TNF⁺ cells (Fig. 5d). Systemically in the spleen, Spike-specific cytokine-secreting CD4⁺ T-cells were detectable in all groups that expressed TLR2 on either non-immune or immune cells, but again, TLR2 expression on immune cells provided an advantage, and expression on both compartments provided the greatest response (Fig. 5e). Thus, TLR2 expression is required for the generation of consequential adaptive immune responses to the Spike protein following mucosal Pam₂Cys Spike vaccination, and expression of TLR2 on immune cells is required for optimal generation of adaptive immunity.\n\n**Pam₂Cys Spike vaccination induces sterilizing immunity against SARS-CoV-2 challenge in mice**\n\nTo determine if the potent immune responses induced by Pam₂Cys Spike vaccination were protective, an in vivo murine model of SARS-CoV-2 infection was utilized. C57BL/6 mice expressing human ACE2 (K18-hACE2) were immunized with Pam₂Cys adjuvant alone, or Pam₂Cys Spike either s.c or i.n, three times two weeks apart. Serum was collected at one week post final vaccination, and the induction of anti-Spike IgG and IgA responses were confirmed. As in wild type C57BL/6 mice (Fig. 1b), mucosal vaccination induced superior titres and uniquely generated IgA (Fig. 6a). The neutralizing potential of these antibodies to inhibit viral infection and cytopathic effect, was first tested in vitro in HEK293 cells overexpressing ACE2 and TMRPSS2 (HEK-ACE2-TMPRSS2), utilizing the ancestral (A.2.2) SARS-CoV-2 strain, and also Beta and Delta variants. Substantial nAb titres were generated against the ancestral strain, and while these titres were reduced against Beta and Delta strains, mucosal immunization induced significant and superior responses, with a mean nAb EC₅₀ greater than 10³ against both VOCs (Fig. 6b).\n\nAt three weeks post final booster vaccination, mice were challenged with SARS-CoV-2 i.n, and clinical data collected for 7 days. Mice receiving Pam₂Cys Spike vaccination, by either route, were completely protected from weight loss (Fig. 6c) and clinical indicators of disease (Fig. 6d). In contrast, mice immunized s.c with Pam₂Cys adjuvant only had no protection, however, 40% of mice receiving Pam₂Cys i.n notably did not lose weight or show clinical indicators of disease. A substantial influx of leukocytes in BALF was observed in Pam₂Cys s.c mice, including macrophages, neutrophils and lymphocytes, which were significantly reduced in the Pam₂Cys Spike s.c group. Interestingly, total leukocyte counts were reduced equivalently in both Pam₂Cys i.n and Pam₂Cys Spike i.n vaccinated mice, although neutrophils were significantly elevated in Pam₂Cys i.n mice (Fig. 6e). Consistent with the substantial antibody response generated by Pam₂Cys Spike, vaccination by either route induced sterilizing protection with no virus detected in the lung tissue at day 7 post infection (Fig. 6f). Intriguingly, 60% of mice receiving Pam₂Cys i.n also had no detectable virus in lung tissue. Consistent with these data, mice vaccinated with Pam₂Cys Spike by either route showed a marked reduction in inflammatory cell infiltration in the lung parenchyma observed by histological examination (Fig. 7). As previously observed, mice that received Pam₂Cys i.n had divergent responses, with 60% of mice displaying minimal inflammation which was comparable to those mice that were vaccinated with Pam₂Cys Spike by either route (Fig. 7). Thus, mucosal and systemic vaccination with Pam₂Cys Spike induced potent protective immunity in mice, with evidence of a non-specific beneficial effect of mucosal Pam₂Cys at this early time point after vaccination, a phenotype which has also been observed after i.n TLR2 activating lipopeptide in murine models of rhinovirus and influenza virus infection³³⁻³⁵.\n\n# Discussion\n\nThe ability to prevent infection and spread of SARS-CoV-2, or indeed other respiratory viruses of concern such as pathogenic coronaviruses and influenza, is critical to address with vaccine development. Vaccines that only partially protect against infection, coupled with large partially immunized populations, may provide a perfect evolutionary driver for VOCs that evade vaccine immune responses with increased ability to replicate in the respiratory mucosa. It may be difficult for parenterally administered vaccines to provide complete protection from infection owing to the systemic nature of the responses induced1. The generation of mucosal immunity, in the URT where viral replication first occurs, requires either local antigen exposure to generate mucosal immune responses, or very high plasma nAb titres that are unlikely to be maintained long term following parenteral vaccination12. Indeed, even recovered patients do not consistently show clear evidence of protective mucosal immune responses despite having plasma antibodies, indicating distinct tissue compartmentalization of immune responses to SARS-CoV-236. Mucosal vaccines, either in isolation or as boosters for parenteral vaccination, may provide a powerful strategy to generate local protective responses in the pulmonary environment, with the potential to reduce the risk of infection and transmission.\n\nHere, we demonstrate that vaccination with a novel protein-based subunit vaccine, Pam2Cys Spike administered either parenterally or mucosally, led to substantial serum anti-Spike IgG titres and high nAb against SARS-CoV-2 virus, including Beta and Delta variants (Fig. 1 and Fig. 6 a,b). In mice expressing human ACE2, this resulted in complete protection against viral infection in the lung tissue and from clinical indicators of disease (Fig. 6, 7). There is strong evidence for a correlation between high serum nAb titres and protection from COVID-1937, including against VOCs, supporting the benefits of booster vaccinations to maintain high serum nAb titres38. Studies in non-human primates demonstrate a correlation between increasing serum nAb titres and protection in the URT, so that lower nAb titres are sufficient to protect the lung alone, compared to higher nAb levels needed to protect both the URT and lungs39. Thus, while many of the currently deployed intramuscular vaccines can prevent SARS-CoV-2-induced pneumonia and severe COVID-19, there is greater variability in protection against URT infection and transmission. Importantly, Pam2Cys Spike mucosal vaccination generated high levels of anti-Spike IgA, as well as increased nAb in both the serum and airways (Fig. 1 and Fig. 6 a,b). Mucosal IgA reduces colonisation of the mucosa by other respiratory pathogens2, including when induced by i.n vaccination30,40. There is scope to explore the addition of defined Spike epitopes to the vaccine that may induce cross-reactive nAb against SARS-CoV-2 variants, or other pathogenic coronaviruses41. Mucosal vaccination also increased lung Spike-specific CD4+ T-cell responses (Fig. 2), that may contribute to the maintenance of protection. Inclusion of additional viral antigens, such as the nucleocapsid protein, to enhance T-cell immunity through broader epitope coverage42,43, may sustain long-term protective memory responses in the mucosa, including in individuals with antibody deficiency. This also has the potential to provide cross-protection against other coronaviruses.\n\nTLR2, the pattern recognition receptor activated by Pam2Cys in this vaccine, is widely distributed in the pulmonary environment, including expression by both respiratory epithelia and antigen presenting immune cells24,25. However, the relative contribution of these compartments to the mucosal vaccine response has not been defined. In our work, mice deficient in TLR2 on both the epithelia and hematopoietic compartments had minimal responses to mucosal Pam2Cys Spike vaccination, indicating that vaccine-induced immune activation was dependent on TLR2 stimulation. After TLR2 stimulation of the pulmonary epithelia, IL-6, TNF and IL-1 may be released to recruit neutrophils and activate APCs22–25. Interestingly, we demonstrate here that the induction of early neutrophil responses in the lungs and airways was facilitated to the same extent by TLR2 expression on either the epithelia or immune cells (Fig. 3 c). TLR2 expression on the epithelia provided an advantage for APC recruitment, including DC, alveolar macrophages and monocyte subsets (Fig. 3 d). Nevertheless, the expression of TLR2 in the hematopoietic compartment was required for the optimal generation of lung-localised, antigen-specific adaptive responses after booster vaccination (Figs. 4 and 5), in particular for the strong IL-17+CD4+ T-cell response, which is typical following mucosal delivery of protein-based vaccines44–46, particularly those activating TLR226,27.\n\nOf interest, SARS-CoV-2 challenge following parenteral and mucosal immunization revealed that the delivery of the adjuvant Pam2Cys by the i.n, but not the s.c route, resulted in a partial protective effect. This suggests that activation of TLR2 in the nasal and lung environment can induce antigen-independent innate immunity, even weeks after i.n delivery of Pam2Cys. This expands the observation that a Pam2Cys-based, TLR2 activating lipopeptide could activate the nasal epithelium and immune cells to protect against rhinovirus and influenza virus infection33–35. The method of delivery and volume of the vaccine may influence whether the immune activation occurs in the upper airways alone or the upper and lower respiratory tract. This is important for consideration of clinical translation, as i.n vaccination in humans typically delivers the vaccine primarily to the upper airways12. Prophylactic i.n delivery of a TLR2 agonist has recently been demonstrated to protect against URT viral shedding of SARS-CoV-2 in a ferret model47, and early clinical trials are underway to assess safety and tolerability in humans (ACTRN12621000607875p). This provides further support for Pam2Cys as a promising mucosal adjuvant for enhancing both local innate defences and induction of powerful adaptive immunity.\n\nCurrently, at least eight mucosal vaccines for COVID-19 have entered clinical trials, delivered either exclusively intra-nasally or by aerosol, or as a mucosal booster following parenteral prime48. Only one of these is a mucosal protein-based vaccine (utilising a receptor-binding domain recombinant protein, clinical trial RPCEC00000345), with the others being live-attenuated or viral vector-based formulations designed to express the Spike protein12. The induction of immunity to the viral vector itself will limit the use of the latter vaccines to boost immunity. As there will be an ongoing requirement for boosting the waning nAb levels to currently used COVID-19 vaccines, and subunit protein-based vaccines with safe and effective adjuvants, such as Pam2Cys Spike, will provide a safe alternative for delivery to the nasal mucosa in a needleless fashion.\n\nFuture studies will require an assessment of the durability of protective responses achievable with this vaccination approach, including in the URT such as the nasal mucosa and trachea, for which SARS-CoV-2 demonstrates a notable tropism49. In animal models of influenza, resident memory cells generated in the nasal passages show potential for preventing virus dissemination to the lung50. In addition, other animal models, such as hamsters or ferrets, could be used to determine the impact of vaccination on transmission to naïve animals31,51. As a large proportion of the world’s population has received, or will receive, an intramuscular vaccination for SARS-CoV-2, it will be important to test a “prime-pull” vaccination approach12,52. Memory T-cells induced by parenteral vaccination can be recruited to mucosal sites by subsequent mucosal boosting53, providing a strategy to optimise both systemic IgG and T-cell responses that protect the lower respiratory tract from severe disease, as well as appropriate mucosal immunity to prevent infection. Thus, the mucosal vaccination strategy described here has the potential to generate IgA-secreting memory B-cells and tissue resident T-cells in the respiratory tract, to provide protection from viral infection and reduce the risk of ongoing viral transmission with pandemic potential.\n\n# Methods\n\n## Vaccine production\nVaccine adjuvant was Pam2Cys-SK4-triethylene glycolate (Pam2Cys) as previously described27, 54. SARS-CoV-2 Spike HexaPro expression vector was a gift from Jason McLellan (Addgene plasmid # 154754; ; RRID:Addgene_154754)55. The HexaPro variant contains six beneficial proline substitutions providing ~10-fold higher expression than the parental construct and increased stability of the trimer in prefusion conformation. Hrv3C-His-Strep tags were included for purification purposes. Recombinant Spike protein was expressed in suspension-adapted Expi293F™ cells, harvested, and purified by immobilised metal affinity chromatography (IMAC) using Ni-NTA agarose as previously described56. The eluate following IMAC was dialysed to 2 mM Tris, pH 8.0, 200 mM NaCl, concentrated before being passed through a 0.22 µm filter, and subjected to gel filtration chromatography using HiLoad 16/600 Superdex 200 (Cytiva) in 2 mM Tris, pH 8.0, 200 mM NaCl. Doses per vaccination were as follows: 7.7 µg Pam2Cys-SK4-triethylene glycolate and 6 µg Spike, admixed in sterile cell culture grade phosphate buffered saline, endotoxin tested (PBS; Sigma D8537).\n\n## Mouse strains and immunization procedures\nAll animal experiments were conducted in full compliance with local and institutional guidelines, with approvals from the Sydney Local Health District Animal Welfare Committee (2020-003, 2020-019). These adhere to the Australian Code for the Care and Use of Animals for Scientific Purposes (2021) as set out by the National Health and Medical Research Council of Australia. Mice had access to standard rodent chow and water ad libitum. Female C57BL/6 (6-8 week-old) or BALB/c (various ages) mice were sourced from Animal BioResources (Mossvale, Australia) and housed at the Centenary Institute under specific-pathogen-free conditions. Female *Tlr2-/-* mice (BALB/c background) were bred at the Centenary Institute24, 25. Female K18-hACE2 mice57 were sourced from the Jackson Laboratory and bred at Australian BioResources and the Centenary Institute. For s.c injection, mice were anaesthetized with gaseous isoflurane (4%, O2 1 L/min) and injected at the base of tail with vaccine in a maximum of 200 µl volume. For i.n instillation, mice were either anaesthetized by intraperitoneal injection of ketamine/xylazine (50 mg/6.25 mg/kg) or gaseous isoflurane, then vaccine in 30-50 µL of PBS was applied to the nares such that mice inhaled the solution. For assessment of early innate responses mice were immunized once; for immunogenicity or protection studies mice were immunized three times 2 weeks apart and adaptive immune responses assessed 1 week after the last booster vaccination.\n\n## Generation of TLR2 chimeric mice\nWT BALB/c or *Tlr2-/-* female mice (between 6-17 weeks of age, similar aged WT and *Tlr2-/-* mice were compared in each experiment) were irradiated at a caesium source (800 RAD). Femurs were isolated aseptically from donor BALB/c or *Tlr2-/-* female mice into complete culture media, RPMI Glutamax (Gibco) with 10% FBS (Hyclone) and penicillin-streptomycin (100 U/ml; Gibco). Marrow cells were flushed from the femur with a 25G needle into complete media, 70 µm filtered and erythrocytes lysed with red blood cell lysing buffer Hybri-Max (Sigma). Cells were 70 µm filtered again before washing and suspending in PBS for i.v injection of 1.8 x106 cells (in 200 µl) per mouse. Mice were rested for 12 weeks to allow hematopoietic reconstitution. For the first 3 weeks post irradiation, mice received prophylactic antibiotics (Trivetrin; final concentration in drinking water 0.54 mg/ml trimethoprim and 2.7 mg/ml sulfadoxine) and extra dietary supplements (sunflower seeds, DietGel® Boost - Clear H2O) as supportive care.\n\n## Organ collection and processing\nMice were euthanized by CO2 asphyxiation, tissues collected aseptically and maintained at 4°C. Blood was collected by rupture of the inferior vena cava/portal vein and allowed to clot, before collection of sera after centrifugation (2000 xg, 15 min). BALF was obtained by tracheal intubation, inflation of the airways with 1 ml PBS and collection of the fluid. Cells were isolated by centrifugation, and BALF was immediately frozen to preserve for further analyses. Other tissues were collected into RPMI 1640 (Gibco) supplemented with 10% FCS (Sigma), 2-ME (0.05 mM), and penicillin–streptomycin (100 U/mL; Gibco). For lung tissue, circulating blood was removed by perfusion with PBS and heparin (20 U/mL; Sigma) injected into the right atrium of the heart. Lung lobes were diced and digested at 37°C for 45 min with collagenase type 4197 (50 U/mL; Sigma) and DNase I (13 µg/mL; Sigma), then filtered through a 70 µm sieve. Mediastinal lymph nodes and spleens were pressed through a 70 µm filter and the leukocytes pelleted by centrifugation. Erythrocytes were lysed with red blood cell lysing buffer Hybri-Max (Sigma), and leukocytes enumerated with Trypan Blue (0.04%) exclusion by hemocytometer.\n\n## Quantitation of anti-spike IgG and IgA\nSpike-specific IgG and IgA in serum and BALF were determined by indirect ELISA. High-binding ELISA plates (Corning Falcon) were coated overnight at 4°C with Spike protein (1 µg/ml) in carbonate/bicarbonate coating buffer (0.05 M, pH 9.6). Plates were washed with PBS (POCD) plus 0.05% (v/v) Tween 20 (Sigma), then blocked with 1% (w/v) BSA (Bovogen) in PBS (1 h at 37°C). Dilution series of sera (from 1:100) or BALF (from 1:40) were added (1 h at 37°C) to capture Spike-specific antibody, and then after washing, detected with either horseradish peroxidase-conjugated goat anti-mouse IgG (Invitrogen Novex, cat# A16090, used at 1:2000) or goat anti-mouse IgA (Invitrogen, cat# 626720, used at 1:2000). Washed plates were developed with tetramethylbenzidine substrate (Sigma), stopped with 2 M HCl, and then absorbance read at 450 nm with a 570 nm reference wavelength (Tecan Infinite M1000 PRO). The titre was estimated by the titration curve of each sample interpolated with the mean absorbance (+ 3SD) of the relevant negative samples from unvaccinated mice (1:100 sera, or 1:40 BALF).\n\n## Cell lines for infection assays\nHEK293T (ATCC CRL-3216) and VeroE6 (ATCC CRL-1586) cells were maintained in Dulbecco’s Modified Eagle Medium (DMEM; Invitrogen) or Minimal Essential Media (MEM; Invitrogen) supplemented with 10% FBS and 100 µg/mL Penicillin-Streptomycin (Gibco), and sub-cultured according to the supplier’s instructions. HEK293T cells stably expressing human ACE2 and/or TMPRSS2 were generated by transducing cells with lentiviral particles and clonal selection as previously described58. Cell lines were routinely checked for mycoplasma contamination (MycoAlert™ PLUS Mycoplasma Detection Kit; Lonza) and confirmed as negative.\n\n## Quantitation of nAb titres using a pseudovirus assay\nnAbs were quantitated against replication-deficient SARS-CoV-2 ancestral (Wuhan) Spike pseudotyped lentivirus particles as previously described59. Briefly, pseudovirus particles were generated by co-transfecting a Spike expression construct pCG1-SARS-2-S Δ1860,61 and GFP-luciferase vector with lentivirus packaging and helper plasmids into HEK293T cells, using Fugene HD (Promega)62. Pseudovirus particles were incubated with serially diluted serum or BALF samples at 37°C, 5% CO2 for 1 hr prior to spinoculation (800 xg, 35°C) of ACE2 over-expressing HEK293T cells. Seventy-two hr post-transduction, cells were fixed and stained with Hoechst 33342 (NucBlue™ Live ReadyProbes™ Reagent, Invitrogen) as per the manufacturers instructions, and imaged using the Opera Phenix high content screening system (Perkin Elmer). The percentage of GFP positive cells was enumerated (Harmony® high-content analysis software, Perkin Elmer) and neutralising endpoint titre determined as the dilution required for ≥50% inhibition of infection (EC50), estimated by sigmoidal curve and interpolation in GraphPad Prism software.\n\n## Quantitation of nAb titres against SARS-CoV-2\nHigh-content fluorescence microscopy was used to determine the neutralising capacity of serum and BALF from vaccinated mice to inhibit live SARS-CoV-2 ancestral virus (A.2.2) infection and the resulting cytopathic effect in permissive cells (VeroE6, final MOI=0.05), as previously described60. Alternatively, Beta (B1.351) and Delta (B.1617.2) variants were compared against ancestral virus (A.2.2) in HEK293 cells overexpressing ACE2 and TMPRSS258,60. The neutralisation endpoint titre of diluted serum or BALF samples was set to ≥50% neutralisation (EC50), estimated by sigmoidal curve and interpolation in GraphPad Prism software. All work utilising SARS-CoV-2 virus was performed in PC3/BSL3 facilities.\n\n## Flow cytometry and ex vivo antigen recall of leukocytes\nLung, BALF, spleen or mediastinal lymph node single cell suspensions were immunolabelled to facilitate phenotyping and data acquired by flow cytometry. Briefly, after washing in PBS, cells were incubated with live/dead fixable blue dead cell stain (Invitrogen) and Fc receptors blocked with anti-mouse CD16/CD32 (2.4G2; BD Biosciences). After washing in FACS wash (PBS with 2% FCS and 2 mM EDTA), surface markers were labelled. For lung and BAL immune profiling, antibodies were anti-mouse B220-BUV737 (RA3-6B2; BD), SiglecF-BV421 (E50-2440; BD), MHCII-V500 (M5/114.15.2; BD), Ly6G-BV650 (1A8; Biolegend), CD11b-BV785 (M1/70; Biolegend), CD45.2-FITC (104; BD), CD11c-PE (N418; Biolegend), CD3-PECF594 (145-2C11; BD), CD64-PECy7 (X54-5/7.1; Biolegend), TLR2-AF647 (6C2; BD), CD4-AF700 (RM4-5; Biolegend) or CD4-AF700 (GK1.5; eBioscience), and Ly6C-APCCy7 (HK1.4; Biolegend). For mediastinal lymph nodes, cells were first incubated with Fc receptor blocking anti-mouse CD16/CD32 (2.4G2; BD Biosciences) and anti-CXCR5-biotin (2G8; BD) at 37oC for 40 min, washed in PBS, then incubated with live/dead fixable blue dead cell stain (Invitrogen) and streptavidin-PE (BD) in PBS for 20 min at 4oC. Cells were then surface immunostained with anti-mouse PD1-BV785 (29F1A12; Biolegend), CD3-PECF594 (145-2C11; BD), CD44-PECy7 (IM7; BD), CD4-AF700 (RM4-5; Biolegend) or CD4-AF700 (GK1.5; eBioscience), and CD8-APCCy7 (53-6.7; BD). Transcription factor staining with anti-mouse Bcl6-AF647 (K112-91; BD) was performed using eBioscience FoxP3/Transcription Factor staining buffer set (Invitrogen), according to the manufacturer’s instructions.\n\nEnumeration of Spike-specific T-cell responses was performed by *ex vivo* antigen recall, intra-cytoplasmic staining and flow cytometry. Lung or spleen leukocytes were stimulated for 4 hr (37°C, 5% CO2) with Spike protein (5 µg/ml), or for controls media alone, or anti-mouse CD3 (1452C11; 5 µg/mL) and anti-mouse CD28 (37.51; 5 µg/mL; BD Pharmingen). Brefeldin A (10 µg/mL; Sigma) was added and further incubated such that cytokine accumulated intracellularly (12 h, 37°C, 5% CO2). Viability stain and Fc blocking was performed, then surface markers were immunolabelled with anti-mouse CD8-APCCy7 (53-6.7; BD Pharmingen), CD4-AF700 (RM4-5; Biolegend) or CD4-AF700 (GK1.5; eBioscience) and CD44-PECy7 (IM7; BD) and then cells were washed thoroughly. Cells were fixed with BD Cytofix/perm followed by thorough washing with BD Perm/Wash. Intracellular cytokines were labelled with anti-mouse IFNγ-FITC (XMG1.2; BD Pharmingen), IL-17A-PB (TC11-18H10.1; Biolegend), IL-4-PE (11B11; BD), TNF-PerCPCy5.5 (MP6-XT22; BD), and IL-2-APC (JES6-5H4; Biolegend) prepared in BD Perm/Wash buffer and then washed. Compensation controls were prepared in the same manner as experimental samples, viability stain was prepared from murine leukocytes, and UltraComp eBeads Compensation Beads (Invitrogen) were stained with the same antibody used in experimental panels. Samples were acquired using an LSRII 5L flow analyzer (BD Biosciences).\n\nComputational analysis of lung leukocytes was performed using the Spectre R package32, with instructions and source code provided at . Compensated sample data were initially prepared in FlowJo (BD) with quality control gating to exclude debris and dead cells, then the CD45+ population was exported as raw value CSV files. Arcsinh transformation was performed on the data in R using a co-factor of 1,000 to redistribute the data on a linear scale and compress low end values near zero. The dataset was then merged into a single data.table, with keywords denoting the sample, group and cell numbers. The FlowSOM algorithm63 was then run on the merged dataset to cluster the data into 30 clusters, where every cell is assigned to a specific cluster and metacluster. Subsequently, the data were downsampled and analysed by the dimensionality reduction algorithm FIt-SNE for cellular visualisation64. Alternatively, flow cytometry data were analysed with FlowJo (v10; BD), see Figs. S1, 3, 8 and 9 for gating strategies.\n\n## SARS-CoV-2 murine challenge model and organ collection\nMice were housed in a PC3/BSL3 facility in an IsoCage N biocontainment system (Tecniplast, Italy). Three weeks after final i.n vaccination, female K18-hACE2 mice were anaesthetised with gaseous isoflurane and infected i.n with 103 plaque forming units (PFU) of SARS-CoV-2 (VIC01/2020) in 30 µl final volume as previously described65. Clinical indicators of disease, including weight, were monitored for the following 7 days. Clinical signs were classified into four categories based on the following criteria: No clinical score - mice did not exhibit any clinical symptoms; Category 1 – weight loss, early lethargy and hunching; Category 2 – substantial weight loss, lethargy, hunching, ruffling and early laboured breathing; Category 3 – all signs in Category 2 are exacerbated, accompanied by immobility. Mice were euthanised with intraperitoneal overdose of pentobarbitone (Virbac, Australia). The multi-lobe lungs were tied off using surgical thread and BALF was collected from the single lung lobe via lavage with 1 mL HANKS solution (Sigma-Aldrich, USA) with a blunted 19-gauge needle inserted into an incision above the largest cartilage ring of the trachea. BALF was centrifuged (300 xg, 4oC, 7 min), and supernatants were collected and snap frozen. The remaining cell pellet was resuspended in 200 µL Red Blood Cell Lysis Buffer (ThermoFisher, USA) for 5 min, followed by addition of 700 µL HANKS solution and then centrifuged again. Following centrifugation, the supernatant was discarded and the cell pellet was resuspended in 160 µL HANKS solution and enumerated using a haemocytometer (Sigma-Aldrich, USA). Differential BALF counts were performed by depositing 70 µL of BALF leukocytes into a cytospin funnel and then centrifuging onto a glass slide (300 xg, 7 min). Slides were left to airdry overnight, after which they were stained using Quick Dip Stain Kit (Modified Giemsa Stain) protocol as per manufacturer’s instructions (POCD Scientific, Australia). Differential counts were determined based on cellular morphology and staining using light microscopy with a Primovert Zeiss Microscope under a 20X objective (Zeiss, Germany). Multi-lobe lungs were collected and snap frozen on dry ice. Lung homogenates were prepared fresh, with the third lobe of the multi-lobe lungs placed into a gentle MACS C-tube (Miltenyi Biotec, Australia) containing 2 mL HANKS solution. Lung tissue was homogenised using a gentleMACS tissue homogeniser, followed by centrifugation (300 xg, 7 min) to pellet cells, and collection of supernatants for plaque assays. The single lobe lungs were perfused with 0.9% NaCl solution via the heart, followed by inflation with 0.5 mL 10% neutral buffered formalin (Sigma-Aldrich, USA) through the tracheal incision, and placed into a tube containing 10% neutral buffered formalin. Lung lobes were fixed in formalin for at least 2 weeks after which, single lung lobes were transported to a PC2 facility for paraffin-embedding prior to being cut into 3 µm thick sections using a Leica microtome (Leica, Germany). Histology sections were stained using Quick Dip Stain Kit (Modified Giemsa Stain) protocol as per manufacturer’s instructions (POCD Scientific, Australia). Inflammatory cells in single lobe lungs were counted using a Zeiss Axio Imager.Z2 microscope with a 40X objective (Zeiss, Germany).\n\n## Plaque assays\nPlaque forming units (PFU) of SARS-CoV-2 viral titres were quantitated in VeroE6 cells65. Cells were deposited into a 24-well cell culture plate at 1.5x105 cells/well in a 0.5 mL volume and allowed to adhere overnight. The next day, virus-containing samples from lung homogenates were serially diluted in MEM cell culture medium and cell culture supernatants removed from the VeroE6 cells and 250 µL of virus-containing samples was added to the surface of the cell monolayers. Plates were placed in the cell culture incubator (37°C/5%CO2) and rocked gently every 15 min to facilitate viral adhesion. Following 1 hr incubation, 250 µL of 0.6% agar/MEM solution was overlaid gently onto the cell culture samples and placed into the incubator. At 3 days post-infection, an equal volume of 8% paraformaldehyde solution (4% final solution) was added to all wells and incubated at room temperature for 30 min. 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Here, we proposed health-oriented control strategies by integrating the unequal toxic potencies of the most polluting industrial PMs. Iron and steel industry (ISI)-emitted PM2.5 exhibit about one order of magnitude higher toxic potency than those of cement and power industries. Compared with the current mass-based control strategy (prioritizing implementation of ultralow emission standards in the power sector), the proposed health-oriented control strategy (priority control of the ISI sector) could generate 5.4 times higher reduction in population-weighted toxic potency-adjusted PM2.5 exposure among polluting industries in China. Furthermore, the marginal abatement cost per unit of toxic potency-adjusted mass of ISI-emitted PM2.5 is only a quarter of that of the other two sectors under ULE scenarios. We highlight a health-oriented air pollution control strategy is urgently required to achieve cost-effective reductions in particulate exposure risks.\n\nEarth and environmental sciences/Environmental sciences/Environmental impact \nPhysical sciences/Energy science and technology/Fossil fuels/Coal \nEarth and environmental sciences/Environmental social sciences/Socioeconomic scenarios\n\n# Introduction\n\nAir pollution attributable to particulate matter (PM) is one of the greatest environmental health risks worldwide1–5. Industrial sectors, constituting one of the major anthropogenic sources of ambient PM, contribute to approximately 0.9 million premature deaths and are a significant global health concern6, 7. Clean air actions have been adopted earlier in developed regions to address industrial sources of air pollution8, 9. Based on total PM mass emissions, these regulations initially focused on the most PM mass emission sectors, including power plants and coal-fired industrial facilities, and then spread to other industrial sectors since the early 1970s8, 10. Regulations have become increasingly strict to meet the ever-stringent air quality standards over the last four decades8, 11, 12. Referring to the total PM mass control strategies implemented in developed regions, similar emission control policies have been promulgated and prioritized among power plants and other industrial sectors in developing regions to combat the unprecedented air pollution over the last two decades12–14. PM emitted from industrial sectors have gradually decreased after decades of emission control policy implementation in major economies, including the USA, Europe, and even China. However, the current regulations aimed at reducing the PM emission quality cannot proportionately reduce the adverse health effects of industrial PM emissions.\n\nThe heterogeneity in source-specific PM, including the chemical composition and toxicological properties, and the toxicity effects of PM, such as the oxidative stress (OS) potency, have been verified as more health-relevant metrics than the PM mass15, 16. The components of source-specific PM, which comprise complex mixtures of chemicals3, 17, vary widely among industrial sectors18–20, owing to the notable discrepancies in raw materials, boiler facilities and/or production processes, as well as air pollution control technologies21–23. Different types of chemical components exhibit varying biological effects24. Transition metals and polycyclic aromatic hydrocarbons (PAHs) can induce the formation of reactive oxygen species (ROS), thus yielding negative health outcomes16, 17, 25, while many of the major PM components, including inorganic sulfate and nitrate, are commonly considered innocuous species17. Toxic components such as trace elements and PAHs and their roles in determining the toxic potency of source-specific PM have been scarcely identified and quantified26–28. Thus, the toxic potencies of PM emitted from different industrial sources, comprising specific components, could likely exhibit a notable discrepancy. However, the toxic potencies of PM emitted from industrial sectors have been scarcely investigated based on field study. The lack of information on source-specific chemicals and relevant chemical-specific toxicities limits the current understanding of the adverse impacts of exposure to industry-emitted PM, which also hinders the formulation of effective control strategies for human health protection.\n\nIn the present study, optimal health-relevant air pollution control strategies for industrial plants are proposed by integrating source-specific toxic potencies and reducing costs. The three most polluting industrial sectors, i.e., the iron and steel industry (ISI), cement industry, and power industry, were selected in this work. PM2.5 samples were collected from these three sectors in field across 21 provinces in mainland China (Supplementary Fig. 1 and Supplementary Tables 1−3), which exhibit the highest production and consumption levels of fossil fuel-fired power, steel, and cement worldwide23, 29. The obtained chemical composition and toxicological data (Supplementary Figs. 2−5 and Supplementary Table 4) were further integrated with the model-simulated PM mass concentration under the ultralow emission (ULE) scenarios, which was estimated by using the updated Air Benefit and Cost and Attainment Assessment System (ABaCAS) emission inventory combined with the Weather Research and Forecasting−Community Multiscale Air Quality (WRF-CMAQ) model30–32. The integrated results could provide insight into the adverse effects of exposure to industry-emitted PM and could facilitate the formulation of priority control strategies to achieve cost-effective reduction in toxic potency-adjusted PM exposure risks. Details of the experiments and analysis approach are provided in the Methods section.\n\n# Results And Discussion\n\nUnequal toxic potencies of industry-emitted PM₂.₅. Exposure to different industry-emitted PM₂.₅ samples exhibits substantial discrepancies in toxic potencies, including intracellular OS and cytotoxicity (CT) potency (Fig. 1 and Supplementary Fig. 2). EC₁.₅ (the concentration effectively leading to a 1.5-fold inhibition of intracellular ROS generation relative to that of the control) and IC₂₀ (the concentration effectively leading to a 20% inhibition relative to that of the control) values were determined to elucidate the endpoints of PM₂.₅-induced OS and CT potency, respectively. The toxic potency increased with decreasing EC₁.₅ and IC₂₀ values. ISI-emitted PM₂.₅ exhibited the highest OS potency (19.1 ± 10.9 µg/mL), which is nearly 5.0 and 5.4 times higher than that of power industry-emitted PM₂.₅ (94.9 ± 41.9 µg/mL) and cement industry-emitted PM₂.₅ (103.6 ± 46.3 µg/mL), respectively (Fig. 1a). Compared to the power and cement industries, the ISI involves a series of complex processes, mainly including sintering (and/or pelletizing), blast furnace (BF) based-ironmaking, basic oxygen furnace (BOF)-based or electric arc furnaces (EAF)-based steelmaking, and steel rolling 22. The EC₁.₅ values for the PM₂.₅ emitted from the three major polluting processes of BOF-based crude steel production, i.e., the sinter ore (21.3 ± 11.2 µg/mL), pig iron (20.7 ± 12.1 µg/mL), and crude steel (14.7 ± 7.8 µg/mL) generation, are shown in Supplementary Fig. 2b, while the EC₁.₅ values for other ISI processes (including pelletizing, EAF-based steelmaking, and steel rolling) are shown in Supplementary Fig. 3. The three processes contributed nearly 90% to the nationwide ISI PM₂.₅ emissions in China in 2019 29. The averaged OS potency of power industry-emitted PM₂.₅ resulted in very close EC₁.₅ values when the boilers were fed with different solid fuels, including coal (104 ± 44 µg/mL), solid waste (89.7 ± 48.1 µg/mL), and biomass (91.9 ± 35.7 µg/mL) (Supplementary Fig. 2c). Additionally, the EC₁.₅ values for the PM₂.₅ emitted from the major production processes of cement plants were close, at 113.4 ± 53.0 µg/mL for the kiln head and 98.7 ± 39.9 µg/mL for the kiln tail (Supplementary Fig. 2d).\n\nThe distribution of the IC₂₀ values further indicated similar substantial discrepancies among the three industrial sectors. The estimated CT potency of ISI-emitted PM₂.₅ (46.4 ± 28.2 µg/mL) was nearly 12.1 times that of power generation-emitted PM₂.₅ (561 ± 226 µg/mL) and 9.5 times that of cement production-emitted PM₂.₅ (442 ± 221 µg/mL) (Fig. 1b). The CT potency of ISI-emitted PM₂.₅ successively increased for the major production processes of sinter ore (60.0 ± 30.4 µg/mL), pig iron (43.4 ± 22.7 µg/mL), and crude steel (36.1 ± 26.4 µg/mL) (Supplementary Fig. 2f). The IC₂₀ values for the other ISI processes are shown in Supplementary Fig. 3. The CT potency of power industry-emitted PM₂.₅ slightly varied among the different fuel-fired units, including coal- (604 ± 254 µg/mL), biomass- (434 ± 212 µg/mL), and solid waste-fired units (539 ± 137 µg/mL) (Supplementary Fig. 2g). In terms of clinker production, the CT potency of kiln tail emitted-PM₂.₅ (396 ± 214 µg/mL) was also close to that of kiln head-emitted PM₂.₅ (487 ± 221 µg/mL) (Supplementary Fig. 2h).\n\nEstimation through laboratory and field studies of all the major processes under the same quality control conditions revealed that the PM₂.₅ emitted from the ISI is much more toxic than those of the power and cement industries, especially the PM₂.₅ emitted from BF-based ironmaking and BOF-based steelmaking processes. A substantial inequality in the toxicological properties of the PM₂.₅ samples obtained from the three industrial sectors is uncovered according to the estimated OS and CT potency. Source-specific PM₂.₅ comprises a complex mixture of inorganic and organic chemicals, some of which are potential contributors to PM₂.₅ related toxicity 16, 17. Hence, it is necessary to uncover and quantify the key chemical components that determine PM₂.₅ toxicological effects to better understand the causes of the abovementioned inequality in toxicological properties.\n\nSubstantial discrepancies among key toxic chemicals in PM₂.₅. The chemical composition, including carbonaceous species (i.e., organic matters and elemental carbon), water soluble inorganic ions, elements, widely varied among the PM₂.₅ originating from the three industrial sources (Supplementary Fig. 4 and Supplementary Table 4). Here, the targeted chemicals are focused on metals and PAHs, which are commonly regarded as key toxic components associated with the biological effects of PM₂.₅ 16, 17. Ten toxic metals (i.e., Fe, Zn, Mn, Pb, Cu, V, Cr, Ni, As, and Cd) were observed at substantially higher concentrations per unit mass of ISI-emitted PM₂.₅ (267 ± 104 mg/g), exceeding those per unit mass of power industry- (13.9 ± 3.7 mg/g) and the cement industry- (25.3 ± 5.7 mg/g) emitted PM₂.₅ by approximately 19 and 11 times, respectively (Fig. 2a). Fe dominated the mass concentrations, with relative concentrations ranging from 62.6 − 98.3%, 43.0 − 94.8%, and 80.4 − 94.1% in the selected metals within in PM₂.₅ emitted from the ISI, power, and cement industries, respectively (Fig. 2a). The observation results regarding the variation in toxic metals are consistent with those obtained in our previous study in regard to flue gases emitted from industrial plants 33. The concentration of metals per unit of PM₂.₅ emissions grouped by the prevailing processes in iron and steel production, the fuel type in power-generating units, and the prevailing processes in clinker and cement production are detailed in Supplementary Note 7 and Supplementary Fig. 5a.\n\nOther key toxic chemical in PM₂.₅, i.e., 16 US Environmental Protection Agency (EPA) priority PAHs (Supplementary Table 5), were also revealed to substantially differ among the three industrial sectors studied (Fig. 2b). The content of these 16 PAHs (612 ± 775 µg/g) in mass-normalized ISI-emitted PM₂.₅ was one order of magnitude higher than that in mass-normalized power sector-emitted PM₂.₅ (27.0 ± 39.2 µg/g) and cement sector-emitted PM₂.₅ (13.5 ± 14.8 µg/g). Compared to the PAHs emitted from the power and cement industries, higher carcinogenic species (with toxic equivalent factor (TEF) equal to or greater than 0.1) were more abundant in ISI-emitted PAHs, accounting for 31.2 − 37.8% of the total mass of the 16 PAHs. In contrast, two- and three-ring PAHs (species with a lower toxicity) were the dominant species among the PAHs emitted from power and cement industries, owing to the higher combustion efficiency of their practical boilers than that of the boilers at ISI plants. The corresponding toxic equivalent benzo[a]pyrene values (BaPₑq) of the 16 PAHs can directly reflect their potential toxic discrepancies (Supplementary Fig. 6). The BaPₑq value per unit mass of ISI-emitted PM₂.₅ (41.1 ± 58.7 µg/g) was two orders of magnitude higher than that per unit mass of power industry-emitted PM₂.₅ (0.20 ± 0.16 µg/g) and cement industry-emitted PM₂.₅ (0.54 ± 0.73 µg/g). Thus, the PAHs originating from the iron and steel production posed a much higher carcinogenic risk than those originating from the other two industrial sectors. The concentrations of the various PAHs per unit of PM₂.₅ emitted from individual iron- and steelmaking processes, power generation units driven by different fuel types, and individual clinker- and cement-making processes are detailed in the Supplementary Note 7 and Supplementary Fig. 5b.\n\nThe relative contributions of the targeted metals and PAHs to PM₂.₅-induced OS potency, quantified via the concentration addition reference model 34, are shown in Supplementary Fig. 7. The targeted metals contributed 84.6 ± 22.6%, 83.8 ± 9.8%, and 77.5 ± 8.4% to OS potency induced by the primary PM₂.₅ emitted from the ISI, power, and cement industries, respectively. While the identified PAHs accounted for minor fractions (2.7 − 3.6%) of the total PM₂.₅-induced OS potency among the three major sectors (Supplementary Fig. 7a). The results indicated that the PM₂.₅-induced OS potency could mainly be attributed to PM₂.₅-bound toxic metals. The higher concentration of toxic metals per unit mass of ISI-emitted PM₂.₅ led to a much higher ROS-inducing effect than that of the PM₂.₅ emitted from the power and cement industries. Thus, the unequal toxic potencies of industry-emitted PM₂.₅ could be attributed to the substantial discrepancies among toxic chemicals in PM₂.₅ emitted from the different industrial sectors (Supplementary Fig. 7b and c). Then the quantified toxic potencies of industries-emitted PM₂.₅ could be integrated with emission inventories to develop toxic potency-adjusted emission policies toward healthy air.\n\nThe iron and steel industry dominates PM₂.₅ toxic potency-adjusted emissions. The quantified toxic potencies were integrated into PM₂.₅ emission inventories as PM₂.₅-induced toxic potency-adjusted emissions of the three selected industrial sectors in China from 2005 − 2019, as shown in Fig. 3. As the largest contributor to PM₂.₅-induced toxic potency-adjusted emissions, the ISI is grouped by its major processes, including sintering, ironmaking, BOF-based steelmaking, and other processes. There existed substantial disproportionalities between the PM₂.₅ emissions and PM₂.₅-induced toxic potency-adjusted emissions of the three industrial sectors. ISI-emitted PM₂.₅ accounted for only 29.0 ± 7.6% of nationwide PM₂.₅ emissions among the three sectors in 2005, but accounted for approximately 70.7 ± 32.9% of PM₂.₅-induced OS potency-adjusted emissions (Fig. 3a). While power and cement industries-emitted PM₂.₅ accounted for 71.0 ± 16.4% of the total mass emissions, and only 29.3 ± 10.4% of the total PM₂.₅-induced OS potency-adjusted emissions. Owing to the drastic reduction in PM₂.₅ emitted from power industry under the enforcement of the toughest ULE standards since 2014 21, the relative fractional contribution of the ISI increased to 43.8 ± 12.0% of mass emissions and further contributed 81.8 ± 37.3% to the overall PM₂.₅-induced OS potency adjusted-emissions in 2019 (Fig. 3b).\n\nThe trends in total PM₂.₅-induced OS potency-adjusted emissions of the three industrial sectors between 2005 and 2019, as illustrated in Fig. 3c, substantially differed from the corresponding trends in PM₂.₅ emissions (Supplementary Fig. 8). The total PM₂.₅-induced OS potency-adjusted emissions fluctuated and eventually increased by approximately 12.2% between 2005 and 2012, although the total amount of nationwide PM₂.₅ emitted from the three sectors decreased by 20.0% during the same period. The increase in OS potency-adjusted emissions was mainly attributable to the ISI emission increase, particularly the emissions originating from BOF-based steelmaking and sintering processes. Since the per unit mass of ISI-emitted PM₂.₅ exhibit much higher OS toxic potencies, the slight increase (~ 10.4%) in ISI-emitted PM₂.₅ resulted in an increase of ~ 12.2% in the total PM₂.₅-induced OS potency-adjusted emissions. The reduced OS potency attributed to the reduction in PM₂.₅ emissions in the power (629 kt) and cement (1462 kt) sectors was offset by the slight increase (716 kt) in the ISI-emitted PM₂.₅. The PM₂.₅-induced OS potency-adjusted emissions of the three sectors decreased by ~ 65.1% between 2012 and 2019. The decreases in the toxic potencies were mainly driven by the corresponding reductions in the ISI sector, with a contribution of ~ 86.8% to OS potency-adjusted emissions. While the reductions in the power generation and cement production sectors jointly contributed only 13.2% to the overall reduction in PM₂.₅-induced OS potency-adjusted emissions, although these two sectors jointly accounted for ~ 47.2% of the reduction in total PM₂.₅ mass emissions.\n\nThe temporal changes in PM₂.₅-induced CT potency-adjusted emissions in the three industrial sectors exhibited a similar tendency to those in OS potency-adjusted emissions, as shown in Supplementary Fig. 9. Substantial reductions in the PM₂.₅ mass-based emissions of the power industry, which could be attributed to the implementation of the toughest-ever ULE standards based on the PM mass concentration, do not necessarily suggest an equivalent alleviation of PM₂.₅ health effects, as evidenced, for example, by the toxic potency (including OS and CT potency)-adjusted emissions in the present study. In contrast, the slight increases or decreases in ISI-emitted PM₂.₅ significantly dominated the variations in PM₂.₅ toxic potency-adjusted emissions among the three sectors. The disproportionate variation in nationwide PM₂.₅ toxic potency-adjusted emissions was mainly due to the unequal source-specific toxic potencies at equal PM₂.₅ mass concentrations. Furthermore, regional discrepancies in the industrial structure among the three sectors could lead to spatial variations in PM₂.₅ emissions and associated toxic potency-adjusted PM₂.₅ exposure risks across the nation.\n\nPriority control in the iron and steel industry can result in a cost-effective reduction in the population-weighted PM₂.₅ exposure risk. Two reduction routes were developed to quantify the reduction effects on mass-based industrial PM₂.₅ emissions and toxic potency-adjusted industrial PM₂.₅ emissions (including the estimation of OS and CT potency) if all facilities in power, cement, and iron and steel industries meet the ULE levels, respectively (Fig. 4a). The implementation of ULE standards in the power industry (1000 kt) could yield a nearly 1.5- and 1.6-fold higher reduction in nationwide mass-based PM₂.₅ emissions than that obtained via the implementation of ULE standards in the ISI (621 kt) and cement industry (653 kt), respectively. However, the implementation of ULE standards in the ISI could result in the largest reduction in PM₂.₅-induced toxic potency-adjusted emissions (including the estimation of OS and CT potency) among the three industrial sectors owing to the unequal OS and CT potency at an equal PM₂.₅ mass, respectively. Spatial distributions of the ambient PM₂.₅ concentration contributed by primary PM₂.₅ originating from the three sectors before and after ULE standards implementation in each sector are shown in Supplementary Fig. 10. The nationwide primary PM₂.₅ concentrations originating from the three industries if all existing units in the power, cement, and iron and steel industries, respectively, satisfied ULE standards in 2019 are shown in Supplementary Fig. 11. The nationwide annual mean population-weighted PM₂.₅ exposure could decrease by 37.6%, and 26.0%, and 36.4% if all facilities in power, cement, and ISI, respectively, met ULE standards in 2019 (Supplementary Table 6). The toxic potency-adjusted exposure risk (TPAE) metric was further developed to estimate a health-relevant risk index for exposure to industrial emitted PM₂.₅, including estimation of PM₂.₅-induced OS and CT potency-adjusted exposure risks (TPAEOS and TPAECT). The cited toxic equivalent values of PM₂.₅-induced OS and CT potencies are provided in Supplementary Table 7.\n\nFigure 4b − d show the spatial distributions of the corresponding reduction in the total TPAEOS value attributed to meeting ULE standards in the power, cement, and ISI in 2019, respectively. The decrease in the power and cement industries only accounted for a minor faction of the total reduction in the nationwide TPAEOS value if all their units achieved ULE standards in 2019 (Fig. 4b and 4c). The highest reductions in power industry- and cement industry-related TPAEOS could be occurred in north and central China, respectively, which were consistent with the density of power and cement plants population. While the significant reduction in the nationwide TPAEOS value could be obtained if all ISI facilities satisfied ULE standards in 2019 (Fig. 4d). Much higher reductions in ISI-associated TPAEOS could be observed on the northern and eastern China, especially in densely populated areas such as Hebei and Jiangsu. Since these populated areas concentrated with a large portion of iron- and steelmaking plants, and majority of these plants could attain ULE levels due to the priority implementation ULE standards and a range of advanced technologies 22. TPAEOS values attributed to each industry source with scenarios before and after ULE standards introduction are shown in Supplementary Fig. 12. The implementation of ULE standards in the power industry yielded the largest reduction in nationwide PM₂.₅ emissions (Fig. 4a) and PM₂.₅ concentration (Supplementary Figs. 10 and 11) among the three industrial sources. However, the implementation of ULE standards in the ISI sector could dominate the reduction in the nationwide TPAEOS value among the three sectors if the unequal OS potencies of source-specific PM₂.₅ were included (Supplementary Table 4).\n\nThe nationwide total population-weighted TPAEOS in the three sectors was dominated by the ISI (83%), owing to the higher OS potency per unit mass of ISI-emitted PM₂.₅. The implementation of ULE standards in the ISI sector could generate a 5.44 ± 3.95 and 8.16 ± 6.58 times higher reduction in the nationwide population-weighted TPAEOS than that obtained via the implementation of ULE standards in the power and cement industry sectors in 2019, respectively (Supplementary Table 8). The reduction in PM₂.₅-induced CT potency-adjusted emissions and the reduction effect on the nationwide TPAECT as well as population-weighted TPAECT exhibited similar tendencies to that of TPAEOS in mainland China (Fig. 4a and e − g, Supplementary Fig. 13 and Supplementary Table 8). The results indicate that implementation of ULE standards in the ISI sector can achieve the largest reduction effect in both nationwide TPAEOS and TPAECT in the three industrial sectors. Furthermore, the marginal reduction costs for PMs emitted from industries can be integrated into the analysis when installation and operating costs of dedusting systems to meet ULE standards are considered.\n\nFigure 5 shows the marginal reduction costs for per unit of mass of industry-emitted PM₂.₅ and per unit of toxic potency-adjusted mass of industry emitted-PM₂.₅ under the scenario with all facilities in each industrial sector meeting ULE standards across the nation in 2019. The marginal abatement cost per ton of the PM₂.₅ mass of the ISI sector was nearly 73% and 142% that per ton of the PM₂.₅ mass of the power and cement industries (Fig. 5a), respectively, while the abatement cost for per unit of OS potency-adjusted mass of ISI-emitted PM₂.₅ was only 14% and 25% that for per unit of OS potency-adjusted mass of power- and cement-emitted PM₂.₅ (Fig. 5b), respectively. The marginal cost for abating per unit of the CT potency-adjusted mass of ISI-emitted PM₂.₅ is only 12% and 15% that for per unit of CT potency-adjusted mass of power- and cement-emitted PM₂.₅ (Supplementary Fig. 14), respectively. The cost estimates indicated that reductions in the emission sources of higher toxic PM₂.₅ could greatly benefit the decrease in PM₂.₅-induced OS and CT potency-adjusted mass emissions instead of the reduction in the largest PM₂.₅ emission source. Thus, we suggest that priority control in the ISI could achieve a much more cost-effective reduction in the adverse impacts associated with exposure to PM₂.₅ originating from the three industrial sources.\n\n# Discussion And Policy Implication\n\nThe unequal toxic potencies of primary PM2.5 emitted from the different industrial sources, including the ISI, power, and cement industries, were elucidated via field measurements and laboratory analysis under the same quality control conditions. However, this health-relevant metric is still absent in current control policies based on pollutant mass concentrations worldwide3, 15. As the conventional top polluting industry ranked by the total PM mass emissions, the toughest control policies were primarily enforced at power plants. However, the reduction in the nationwide TPAE value attributed to the implementation of ULE control policies at power plants accounted for only 6.6 − 13.1% of total TPAE reduction among the three industrial sectors across mainland China, owing to the low toxic potency per unit mass of power industry-emitted PM2.5. In contrast, the decrease in the ISI after the implementation of ULE standards at all facilities dominated the nationwide reduction in the total TPAE value (76.2 − 86.7%) among the three sectors in 2019 across mainland China. Furthermore, the marginal abatement cost for the mitigation of per unit of toxic potency-adjusted mass of ISI-emitted PM2.5 is only 12 − 25% that for the mitigation of per unit of toxic potency-adjusted mass of power industry-emitted PM2.5 under the scenario whereby all ISI facilities in mainland China reach satisfied standards in 2019 (Fig.5). Therefore, the ISI should be prioritized among the three sectors, given its cost-effective role in reducing adverse impacts associated with exposure to industry emitted-PM2.5. We highlight that it is urgent to shift from the mass-based control strategy to the health-oriented control policies via integrating unequal toxicities of industrial particulate emissions.\n\nThe implementation of stricter control measures targeting ISI-emitted PM2.5 could be a big challenge in the real world because iron and steel production involves complex manufacturing processes and multiple emission sources22, including the major processes of sintering, ironmaking, and BOF-based steelmaking. Due to their highest PM2.5 emissions and highest PM2.5-induced toxic potency values, these major processes represent important targets for further adverse impacts reduction. Additionally, compared to the effects of conventional BOF-based steelmaking processes, EAF-based steelmaking processes could alleviate PM2.5-induced toxic potencies, as indicated by our limited EAF-emitted PM2.5 samples (Supplementary Fig. 3). The obtained toxicity results expand the previous recognition of EAFs as an advanced technology option for the mitigation of ISI-emitted air pollutants29. The shift from BOFs to EAFs is recommended over the next decades to achieve carbon neutrality and reduce ISI-emitted air pollutants, especially in developed regions. The uncertainties in the toxicity of EAF-emitted PM2.5 may hinder the evaluation of the effectiveness of current EAF technology in addressing the health effects of PM2.5 pollution. Hence, future efforts are warranted to quantify and clarify the toxic potency of EAF-emitted PM2.5. The obtained understanding may offer important insights to policymakers formulating targeted control policies to achieve air quality, climate, and health cobenefits in the ISI.\n\nSeveral limitations and uncertainties in field investigations and estimations exist in this study. Source-specific secondary and fugitive aerosols emission from manufacturing iron/steel and cement processes were not considered, which could result in underestimation of the adverse impacts associated with exposure to specific source-emitted aerosols. The observed toxic potencies based on in vitro cell tests are not strictly consistent with the actual PM2.5 exposure environment in the human body, and thus, toxic estimation methods limit the understanding of real-world human exposure scenarios. Additionally, the estimation of the contribution of a specific component to the overall toxic endpoints based on a chemical additional model may ignore the synergistic or inhibitory effects of different chemicals, and thus may generate additional uncertainties in quantitative contribution analysis of toxic components. Therefore, future efforts need to explore the industry source-emitted secondary and fugitive aerosols and their induced toxic potencies to comprehensively estimate the adverse impacts associated with exposure to industry-emitted PM2.5. In addition, more realistic toxicological exposure studies, including human organoid-based in vitro model, are required to elucidate the multiple health-relevant end points associated with exposure to industry-emitted PM2.5. In vivo and epidemiological studies are strongly encouraged to clarify and validate the relationship between exposure to industry-emitted PM2.5 and adverse health outcomes. On the other hand, the mixture effects of ambient PM2.5, particularly in industrial areas, should be determined to better characterize and to dissect the quantitative contribution of toxic components and finally elucidate contributions of hazardous sources to mixture effects. Multilevel evidence could shed light on reducing the uncertainty in the estimation of the health effects of industry PM2.5 pollution and the formulation of tailored industry source control policies for human health protection.\n\nDespite the above limitations, our analysis could offer a novel perspective to policymakers, thereby emphasizing that a focus shift from emission mass-oriented policies to health-oriented control policies could help facilitate the most cost-effective reduction in the health effects of industry PM2.5 pollution. The method can be applied to other sectors. The results may provide guidance for developing regions suffering from similarly severe air pollution driven by multiple industrial sources that are seeking economic approaches for the mitigating of the health effects of industry-related emissions, such as India and Brazil35. Since the industry structure, manufacturing processes, and energy consumption exhibit large discrepancies among different regions worldwide. Local measures to quantify and rank the toxicity of individual source-emitted PM2.5 are strongly recommended in the formulation of localized toxicity-based control policies to effectively mitigate source-specific PM2.5 effects on public health.\n\n# Methods\n\nField studies of eighty-two typical units of energy- and emission-intensive industrial sectors, including the iron and steel industry (ISI), power industry, and cement industry, were conducted in 21 provinces in China from 2017−2022 (Supplementary Fig. 1). These selected units covered the major iron/steel and cement production processes, as well as the major types of fuel-fired power generating units. Information on these typical units is detailed in Supplementary Notes 1−4 and Supplementary Tables 1−3. The air pollution control measures enforced in the various industrial sectors, including the ISI, power, and cement plants, are outlined in Supplementary Note 1 and Supplementary Tables 9−12. An isokinetic sampling system (C-5000, ESC, USA) was deployed to collect fine particulate matter (PM2.5) emission samples originating from stationary sources following US EPA Method 17 (Supplementary Note 5 and Supplementary Fig. 15). To prevent water vapor and fuel gas condensation, the deployed isokinetic sampling equipment was heated to and maintained at a temperature of 120 °C throughout the whole sampling process. PM2.5 samples were collected on both quartz fiber and Teflon filters for weighing and further analysis. The PM2.5 remaining on the filter holders was removed via rinsing twice with acetone and collected in clean glassware for further weighing. The sampling time for PM2.5 emitted from the three types of plants ranged from 30 to 120 min. The selected units were operated at a stable generating load at over 75% of their capacity during each test. Three successful measurements of the selected units were performed at each sampling site. The field sampling and quality control methods for the industrial emissions have been detailed in our previous studies20, 36.\n\nThe chemical composition of PM2.5 emitted from the three industrial sources, including organic carbon, elemental carbon, water soluble ions, PM2.5-bound 16 US EPA priority polycyclic aromatic hydrocarbons (PAHs) (i.e., Nap, Acy, Ace, Flu, Phe, Ant, Flt, Pyr, BaA, Chry, BbF, BkF, BaP, InP, DahA, and Bghip) and elements, was quantified with the use of standard methods20, 37, 38, as detailed in Supplementary Note 6. Gas chromatography coupled with mass spectrometry (Thermo Scientific ISQ 7000 GC−MS, USA) was employed to determine 16 EPA priority PAHs collected on quartz fiber filters. An inductively coupled plasma mass spectrometer (Thermo Scientific 7500a, USA) was used to examine elements collected on Teflon filters. Benzo(a)pyrene-equivalent carcinogenic potency (BaPeq) values were examined to estimate the carcinogenic risk of the 16 PAHs, which were estimated based on toxic equivalent factors (TEFs). The TEFs of 16 PAHs were retrieved from a previous study39. The full form, abbreviation, and the corresponding TEFs of the 16 PAHs are listed in Supplementary Table 5.\n\nHuman epithelial A549 cell lines were adopted to examine PM2.5-related biological effects, including PM2.5-induced oxidative stress (OS) potency and cytotoxicity (CT) potency. The PM2.5 filter samples were sonicated in methanol and ultra-purified water, and the obtained PM2.5 extracts were then dried under purified nitrogen. Description of the analysis process are provided in Supplementary Note 6. OS potency induced by the PM2.5 samples was examined with a 2’,7’-dichlorofluorescein diacetate protocol. The CT potency measurement was achieved via a 3-(4,5-dimethylthiazol-2-yl)-2,5-diphenyltetrazolium bromide assay. A microplate reader (Varioskan LUX, Thermo Scientific) was employed to investigate the fluorescence intensity and optical density, which were detected at wavelengths of 488/525 and 570 nm, respectively. The endpoints of PM2.5-induced OS potency and CT potency were reported as EC1.5 (the concentration effectively leading to a 1.5-fold inhibition of intracellular ROS generation relative to that of the control) and IC20 (the concentration effectively leading to a 20% inhibition relative to that of the control) values, respectively. The detailed procedures can be found in previous studies37, 40–42.\n\nThe Air Benefit and Cost and Attainment Assessment System (ABaCAS) emission inventory of air pollutants in China from 2005 to 2019 was developed based on an emission-factor method, and the emissions from power plants and key industrial processes, such as the ISI and cement industry, were quantified via a unit-based approach, as in our previous studies32, 43, 44. Regarding the ISI, all specific industrial processes, including sintering, pelletizing, blast furnace (BF)-based ironmaking, and basic oxygen furnace (BOF)- and electric arc furnace (EAF)-based steelmaking, were considered. Regarding the cement industry, cement grinding mills and cement clinkers, the latter of which include shaft kilns, rotary kilns, and new dry clinkers of different capacities, were considered. The activity data (energy consumption, product yield, etc.) from the energy statistical yearbooks and local or national surveys, such as the Second National Pollution Source Census, were collected45. For 2019, the detailed location, fuel type, energy consumption, product yields, and end-of-pipe control information of 5508 power plants, 742 BFs, 658 BOFs, 124 EAFs, and 1939 cement plants were collected for emission calculation and Weather Research and Forecasting−Community Multiscale Air Quality (WRF-CMAQ) simulation purposes, as in our previous study43.\n\nThree control scenarios (no ultralow emission standard for electricity generation (ELE_noULE) scenario, ULE standard for cement industry (CI_ULE) scenario, and ULE standard for iron and steel industry (ISI_ULE) scenario) were developed to evaluate the potential emission reduction due to the implementation of ULE standards or technology improvement based on the base emission inventory of 2019, detailed as follows: (1) ELE_noULE scenario. Under this scenario, we used the energy consumption and technology structure of power plants in 2019 and the end-of-pipe control measures and shares of PM of power plants in 2014. (2) CI_ULE scenario. Under this scenario, we considered the product yield and technology structure of the cement industry in 2019 and end-of-pipe control technology of the ULE standard for PM control in the cement industry. (3) ISI_ULE scenario. Under this scenario, we employed the product yield and technology structure of the ISI in 2019 and end-of-pipe control technology of the ULE standard for PM control in the ISI.\n\nAmbient PM2.5 concentrations were simulated with the WRF-CMAQ model. The simulation period covers the entirety of 2019. The WRF-CMAQ model with the updated ABaCAS emission inventory was adopted for baseline scenario simulation. The model simulation performance was evaluated via a comparison between the simulated parameter values and ground observations (Supplementary Note 8 and Supplementary Table 13). We operated the model with the above three emission control scenarios (including ELE_noULE, CI_ULE, and ISI_ULE) to estimate the reduction effect on toxic potency-adjusted exposure risk (TPAE) of the implementation of ULE standards and technology improvement. The differences between the baseline and ELE_noULE scenarios constitute the influence of the ULE standard for PM control implemented at power plants since 2015 in China. The differences between the baseline and CI_ULE and ISI_ULE scenarios represent the potential benefits of the implementation of ULE standards targeting the PM emissions from the cement industry and ISI, respectively.\n\nThree additional zero-emission scenarios for the energy and industrial sectors were designed based on the emission inventory of 2019, including no electricity (NoELE) scenario, no cement industry (NoCI) scenario, and no iron and steel industry (NoISI) scenario, to examine the the contributions of power, cement, and ISI sectors to the ambient PM2.5 concentration in the base year (Supplementary Table 14). Emission inventories excluding primary PM2.5 emissions from power, cement, and ISI sectors, as obtained with the baseline scenarios, were used to simulate the NoELE, NoCI, and NoISI scenarios, respectively. The differences in the simulated concentrations between the baseline scenario and the NoELE, NoCI, and NoISI scenarios were employed to estimate the ambient PM2.5 concentration attributable to the power, cement, and ISI sectors, respectively. The uncertainties of the emission inventory of each source were quantified with 10000 times Monte Carlo simulation based on the uncertainty range of the activity data, emission factors, and end-of-pipe control efficiencies (Supplementary Note 11), as detailed in our previous study44.\n\nThe population-weighted exposure (PWE) attributable to PM2.5 pollution originating from each industry sector can be calculated as follow:\n\n$$\\text{PWE = }\\frac{\\text{1}}{\\text{P}}\\sum _{\\text{i}}{\\text{P}}_{\\text{i}}\\text{·}{\\text{C}}_{\\text{i,s}}$$\n\nwhere P is the total population, Pi is the population in each geographic unit (i), and Ci,s is the ambient PM2.5 concentration attributable to each emission sector (s) in each geographic unit (i), respectively. PM2.5-induced toxic potencies were integrated to estimate the health-relevant risk index for exposure to industrial-emitted PM2.5, including estimation of the PM2.5-induced OS and CT potency-adjusted exposure risks (TPAEOS and TPAECT). TPAEOS and TPAECT were estimated as TPAEOS = Ci,s × OSi,s and TPAECT = Ci,s × CTi,s, respectively, where OSi,s and CTi,s are the toxic equivalent values of the PM2.5-induced OS and CT potency, respectively, originating from each industry sector (s) in each geographic unit (i). OSi,s and CTi,s (Supplementary Note 9 and Supplementary Table 7) were estimated on the basis of toxic units determined from the PM2.5-induced OS and CT potency values, as detailed in our previous study42. The population-weighted TPAEOS and TPAECT can be estimated as PWEi,s × OSi,s and PWEi,s × CTi,s, respectively (Supplementary Table 8). The uncertainties of population-weighted TPAE were quantified based on the uncertainties of PM2.5-induced toxic potency and PM2.5 emission inventory (Supplementary Note 11).\n\nThe unit cost (UCost) of the implementation of ULE standards for PM2.5 emission control in the ISI, power, and cement industries can be calculated as follows:\n\n$$UCos{t_{i,s}}=\\Delta TCos{t_{i,s}}/\\Delta Emi{s_{i,s}}$$\n\nwhere i and s denote a given end-of-pipe control measure and emission sector, respectively, DEmis is the abatement potential, and TCost is the total cost, which can be calculated with the same method as that in our previous study46–48, as follows:\n\n$$TCos{t_{i,s}}=C{C_{i,s}}+FO{M_{i,s}}+FUE{L_{i,s}}$$\n\nwhere CC is the annual average capital cost, FOM is the fixed operating and maintenance cost, and FUEL is the fuel cost per year. CC can be estimated as follows:\n\n$$C{C_{i,s}}=Cos{t_{i,s}} \\times \\frac{{\\alpha {{(1+\\alpha )}^t}}}{{{{(1+\\alpha )}^t} - 1}}$$\n\nwhere Costi,s is the initial investment cost, a is the discount rate, t is the lifetime of the considered end-of-pipe control measure. The discount rate and lifetime of the end-of-pipe control measures in these sectors were set to 10% and 20 years, respectively, based on a comprehensive analysis of pertinent literature and government reports48. The unit cost of the implementation of ULE standards for toxic potency-adjusted PM emission control (including estimation of OS and CT) in the ISI, power, and cement industries can be calculated as follows:\n\n$$\\text{UCos}{\\text{t}}_{\\text{OS}}\\text{=}\\Delta TCos{t}_{\\text{i,s}}\\text{/(}\\Delta Emi{s}_{\\text{i,s}}\\text{ } \\text{×}{\\text{ OS}}_{\\text{i,s}}\\text{)}$$\n\n$$\\text{UCos}{\\text{t}}_{\\text{CT}}\\text{=}\\Delta TCos{t}_{\\text{i,s}}\\text{/(}\\Delta Emi{s}_{\\text{i,s}}\\text{×}{\\text{ } \\text{CT}}_{\\text{i,s}}\\text{)}$$\n\nFurther descriptions of the methods and data for unit cost calculation are provided in Supplementary Note 10 and Supplementary Tables 15−18.\n\n# References\n\n1. Lelieveld, J., et al. (2015). The contribution of outdoor air pollution sources to premature mortality on a global scale. *Nature* 525, 367-71.\n2. Liu, C., et al. (2019). Ambient Particulate Air Pollution and Daily Mortality in 652 Cities. *N Engl J Med* 381, 705-715.\n3. 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Gaseous and Particulate Chlorine Emissions from Typical Iron and Steel Industry in China. *J. Geophys. Res-Atmos.* 125, e2020JD032729.\n37. Wu, D., et al. (2018). Primary Particulate Matter Emitted from Heavy Fuel and Diesel Oil Combustion in a Typical Container Ship: Characteristics and Toxicity. *Environ. Sci. Technol.* 52, 12943-12951.\n38. Ding, X., et al. (2021). Direct Observation of Sulfate Explosive Growth in Wet Plumes Emitted From Typical Coal-Fired Stationary Sources. *Geophys. Res. Lett.* 48, e2020GL092071.\n39. Nisbet, I. C. T.; Lagoy, P. K. (1992). Toxic equivalency factors (TEFs) for polycyclic aromatic hydrocarbons (PAHs). *Regul. Toxicol. Pharmacol.* 16, 290-230.\n40. Wu, D., et al. (2017). Chemical characterization and toxicity assessment of fine particulate matters emitted from the combustion of petrol and diesel fuels. *Sci. Total. Environ.* 605-606, 172-179.\n41. Roper, C., et al. (2019). PM2.5 Filter Extraction Methods: Implications for Chemical and Toxicological Analyses. *Environ. Sci. Technol.* 53, 434-442.\n42. Wu, D., et al. (2022). Toxic potency-adjusted control of air pollution for solid fuel combustion. *Nat. Energy* 7, 194-202.\n43. Zheng, H., et al. (2019). Development of a unit-based industrial emission inventory in the Beijing–Tianjin–Hebei region and resulting improvement in air quality modeling. *Atmospheric Chemistry and Physics* 19, 3447-3462.\n44. Li, S., et al. (2023). Emission trends of air pollutants and CO2 in China from 2005 to 2021. *Earth Syst. Sci. Data Discuss.* 2023, 1-22.\n45. Ministry of Ecology and Environment of the People's Republic of China, *Announcement on the release of the \"Second National Pollution Source Census\"*. Ministry of Ecology and Environment of the People's Republic of China: Beijing, 2020.\n46. Sun, J., et al. (2014). Cost estimate of multi-pollutant abatement from the power sector in the Yangtze River Delta region of China. *Energy Policy* 69, 478-488.\n47. Xing, J., et al. (2019). Least-cost control strategy optimization for air quality attainment of Beijing–Tianjin–Hebei region in China. *J. Environ. Manage.* 245, 95-104.\n48. Zhang, F., et al. (2020). Estimation of abatement potentials and costs of air pollution emissions in China. *J. Environ. Manage.* 260, 110069-110080.\n\n# Supplementary Files\n\n- [IndustryemissionSI20230228.pdf](https://assets-eu.researchsquare.com/files/rs-2645723/v1/491593d5edfce9325d6d2741.pdf) \n Supporting information for this study"} {"paper_id": "prb6", "title": "First in vivo images of the human brain revealed with the Iseult 11.7T MRI scanner", "text": "# Abstract\n\nThe understanding of the human brain is one of the main scientific challenges of the 21st century. In this context, in the early 2000s the French Atomic Energy Commission (CEA) launched a program to conceive and build the first human MRI scanner operating at 11.7T. More than a decade of developments followed to deliver the magnet while six more years were necessary to complete the commissioning and finally obtain approval from the regulatory agencies to acquire the first ever human brain images in vivo at such magnetic field. We deployed parallel transmission tools to mitigate the radiofrequency field inhomogeneity problem and tame the specific absorption rate. To assure the safety of human imaging at such high field strength, we performed physiological, vestibular, behavioral and genotoxicity measurements on the volunteers. The data shows no evidence of adverse effects. The unprecedented field strength combined with the acquisition techniques deployed yield T2 and T2*-weighted images reaching mesoscale resolutions within short acquisition times and with a high signal and contrast to noise ratio.\n\n- [Biological sciences/Biological techniques/Imaging/Magnetic resonance imaging](/browse?subjectArea=Biological%20sciences%2FBiological%20techniques%2FImaging%2FMagnetic%20resonance%20imaging)\n- [Biological sciences/Neuroscience/Diseases of the nervous system](/browse?subjectArea=Biological%20sciences%2FNeuroscience%2FDiseases%20of%20the%20nervous%20system)\n- [Biological sciences/Neuroscience/Cognitive neuroscience](/browse?subjectArea=Biological%20sciences%2FNeuroscience%2FCognitive%20neuroscience)\n- [Biological sciences/Neuroscience/Computational neuroscience](/browse?subjectArea=Biological%20sciences%2FNeuroscience%2FComputational%20neuroscience)\n- [Health sciences/Medical research/Translational research](/browse?subjectArea=Health%20sciences%2FMedical%20research%2FTranslational%20research)\n\n# Main\n\nUnderstanding the human brain, normal or diseased, is one the most significant scientific challenges of the 21st century, with academic, medical, societal and economic implications. In this context, neuroimaging, and especially Magnetic Resonance Imaging (MRI), has become an essential approach, as it allows maps of the brain anatomy, function, and structural connectivity to be obtained in patients and healthy volunteers *in situ* and non-invasively, as recognized by the Human Brain Project (now eBrain), the US Brain Initiatives and Brain Connects programs, and the China Brain Project [1]. Continuing efforts aim at boosting functional [2] and diffusion [3,4] MRI to explore the human brain *in vivo* at finer spatial resolutions [5]. By revealing at a mesoscopic scale the structural-functional links that compose the human brain (cytoarchitectonic of neuron clusters and their connections), one could bridge the gap toward both the extensive body of knowledge we already have at the microscopic scale on neurons and synapses, and the brain connectome at a macroscopic scale. This will allow us to confirm or refute our current hypotheses regarding its functioning and to generate new ones.\n\nBenefitting from a supralinear gain in sensitivity [6,7], this goal can be reached by boosting the magnetic field, B0, at which MRI systems operate. The Iseult project, originated in 2001, was based on this vision and aimed at building the first MRI magnet operating at 11.7T to investigate the human brain at an unprecedented scale. After nearly 20 years of research and development mainly led by the Department of Astrophysics, Particle Physics, Nuclear Physics and Associated Instrumentation (DAPNIA, since renamed IRFU) of CEA, the 132 tons 11.7T magnet (installation set-up shown in Figure 1) together with the scanner equipment delivered in 2021 its first images of the human brain *ex vivo* [8]. The drastic field homogeneity and temporal stability constraints for MRI were met respectively thanks to a careful design of the main superconducting coil (double pancakes) coupled with a passive iron shim, and an external power supply [9], reaching 0.9 ppm peak-to-peak over a 22 cm diameter sphere and 3 ppb/hour field drift at thermal equilibrium [8].\n\nWhen increasing B0, the radiofrequency (RF) field used to excite the nuclear spins becomes more and more inhomogeneous, a long-standing and major problem in MRI due to the shortening of the wavelength of the RF waves used (500 MHz at 11.7T for the hydrogen nucleus of water), leading to severe artifactual signal variations in the images visible already on the *ex-vivo* brain [8]. We tackled this problem by deploying parallel transmission hardware and software, first developed by the laboratory at 7T and further optimized for 11.7T (Methods). The specific absorption rate (SAR), also growing with Bo [10], was tamed with virtual observation points [11] and dedicated RF pulse design algorithms [12].\n\nApproval from the regulatory body and ethics committee to perform first tests *in vivo* on 20 healthy adult subjects was granted early 2023. Overall, for small flip angle excitations and large flip angle refocusing pulses, normalized root mean square errors (NRMSE) equal or lower than 13% thereby could be obtained over the whole brain, the latter value being the intrinsic inhomogeneity achieved at 3T with volume coils [13]. Inversion pulses remained difficult to achieve given the architecture of the coil, leaving very localized artefacts despite reaching 8% of NRMSE. Static B0 shimming was performed up to second order for each subject, using a brain mask and a quadratic programming approach yielding on average 82.7 Hz standard deviation over the brain (0.17 ppm). After B0 and RF field mapping for each subject, following the RF pulse designs T2 and T2*-weighted acquisitions were successfully performed by deploying the parallel transmission techniques (Fig. 2). The presented *in vivo* human brain images acquired at 11.7T thereby reveal good signal homogeneity consistent with the simulations, without severe RF field inhomogeneity artefacts. A 2D T2*-weighted acquisition was repeated with the same protocol (resolution, bandwidth, acquisition time, number of receive elements) at 3T and 7T on different volunteers. The comparison highlights the gain in signal:noise ratio (SNR) at 11.7T, which can be traded for higher spatial (or temporal) resolutions, enabling access to fine brain details. With the limited number of subjects authorized in this first protocol, and considering the problems induced by head motion, we could obtain good quality images with resolutions up to 0.19×0.19×1 mm3 resolution (36 nl voxel volume) in about 5 min. Images indicate sufficient SNR to boost further spatial resolution or decrease acquisition time in the future.\n\nWhether human beings could withstand 1.5-hour scans at 11.7T was also uncharted territory, while vestibular effects have been reported in mice [14], as well as mild genotoxic effects with repeated or chronic field exposures [15]. This first study, therefore, proceeded with care to gather reasonable evidence for the absence of harmful effects in more realistic conditions [16,17]. Physiologic (cardiac pulsation, arterial pressure), vestibular [18] and cognitive [19,20] measurements were implemented in the protocol to verify the innocuousness of the large magnetic field on humans. Those tests were performed on the 20 subjects scanned at 11.7T and on another cohort of 20 subjects with the magnetic field switched off, to disentangle any effect from a possible psychological bias (nocebo effect). The subjects of the 0T group were not informed of the absence of the magnetic field and received the same instructions as the volunteers scanned at 11.7T. Due to the absence of gradient coil vibrations at 0T, we mimicked the sound of MRI sequences with recordings played by a loudspeaker hidden at the back of the magnet. Genotoxicity was also assessed but only for the 11.7T group with blood samples drawn before and after the 90 min exposure to perform intra-subject comparisons. Across all the tests carried out in this protocol, the statistical analysis revealed no significant differences related to field exposure (Methods).\n\nThe next steps will focus on development and implementation of motion correction tools [21,22] together with highly accelerated sequences [23,24]. The deployment of more efficient RF coils [25], more receive channels count and more powerful gradients [5] is also underway to further increase performance, especially to perform high resolution fMRI and tractography. The safety and imaging data gathered in this first study confirm the applicability of MRI at 11.7T: humans can safely tolerate such intense magnetic fields while image mesoscale resolutions can be achieved on the brain in reasonable time, provided the RF field inhomogeneity problem is mitigated to return optimal SNR. It brings to the fingertips of the neuroscience community an extraordinary opportunity to discover the brain at an unprecedented scale, to explore the biological mechanisms underlying our mental life and to better identify the mechanisms at work in neurological (e.g. Alzheimer) or psychiatric diseases (depression, schizophrenia).\n\n# References\n\n1. N. Vogt. Human brain mapping. *Nat Methods* 2013: 1868-1871.\n2. Finn, E.S., Poldrack, R.A. & Shine, J.M. Functional neuroimaging as a catalyst for integrated neuroscience. *Nature* **623**, 263–273 (2023). https://doi.org/10.1038/s41586-023-06670-9.\n3. D. 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Grant, P-F. Van de Moortele, A. Monreal-Madrigal, G. Adriany, A. Vignaud, F. Mauconduit, C. Rabrait-Lerman, B. Poser, K. Ugurbil, N. Boulant. Magnetic field strength dependent SNR gain at the center of a spherical phantom and up to 11.7T. *Magn Reson Med* 2022 ; 88:2131–2138\n8. N. Boulant, L. Quettier, the Iseult Consortium. Commissioning of the Iseult CEA 11.7T whole-body MRI: current status, gradient-magnet interaction tests and first imaging experience. *Magn Reson Mater Phys.* 2023 ; 36 : 175-189 ; https://doi.org/10.1007/s10334-023-01063-5.\n9. D. Le Bihan and T. Schild. Human brain MRI at 500 MHz, scientific perspectives and technological challenges. *Supercond. Sci. Technol.* 2017 ; 30 033003\n10. Z. Cao, J. Park, Z-H Cho, C.M. Collins. Numerical evaluation of image homogeneity, signal-to-noise ratio, and specific absorption rate for human brain imaging at 1.5, 3, 7, 10.5, and 14T in an 8-channel transmit/receive array. Journal of Mag Reson Imag 2015;41:1432-1439.\n11. G. Eichfelder, M. Gebhardt, Local specic absorption rate control for parallel transmission by virtual observation points. Magn Reson Med 66 (2011) 1468-1476.\n12. A. Hoyos-Idrobo, P. Weiss, A. Massire, A. Amadon, N. Boulant. On variant strategies to solve the magnitude least squares optimization problem in parallel transmission and under strict SAR and power constraints. IEEE Transactions on Medical Imaging 33:739-748 (2014).\n13. N. Boulant, D. Le Bihan, A. Amadon. Strongly modulating pulses for counteracting RF inhomogeneity at high fields. Magn Reson Med 60 (2008) 701-708.\n14. I. Tkáč, MA Benneyworth, T Nichols‐Meade, et al. Long‐term behavioral effects observed in mice chronically exposed to static ultra‐high magnetic fields. Magnetic Resonance in Med 2021;86:1544–1559.\n15. C. Herate, P. Brochard, F. De Vathaire, M. Ricoul, B. Martins, L. Laurier, J-R Deverre, B. Thirion, L. Hertz-Pannier, L. Sabatier. The effects of repeated brain MRI on chromosomal damage. Eur Radiol Exp 6, 12 (2022).\n16. A. Grant, GJ Metzger, P-F Van de Moortele, et al. 10.5 T MRI static field effects on human cognitive, vestibular, and physiological function. Magnetic Resonance Imaging 2020;73:163–176.\n17. C. Le Ster, E. Selingue, R. Poirier, J-M. Edeline, S. Mériaux, N. Boulant. Behavioral and functional assessment of mice inner ear after chronic exposure to an ultrahigh B0 field of 11.7 T or 17.2 T. Magnetic Resonance in Med 2023;90:699–707\n18. I. Bargiotas, J. Audiffren, N. Vayatis, P.-P. Vidal, S. Buffat, A. P. Yelnik, and D. Ricard. On the importance of local dynamics in statokinesigram: A multivariate approach for postural control evaluation in elderly. PloS one, 13(2): e0192868, 2018.\n19. F. Jin, B. McCandliss, T. Sommer, A. Raz, and M.I. Posner. 2002. Testing the Efficiency and Independence of Attentional Networks. J Cogn Neurosci 14 (3): 340–47. https: //doi.org/10.1162/089892902317361886.\n20. F. Jin, X. Gu, K.G. Guise, X. Liu, J. Fossella, H. Wang, and M.I. Posner. 2009. Testing the Behavioral Interaction and Integration of Attentional Networks. Brain and Cognition 70 (2): 209–20. https://doi.org/10.1016/j.bandc.2009.02.002.\n21. M. Riedel, T. Ulrich, K. Pruessmann. Real-time correction of rigid motion and 1st-order shims using rapid 3D orbital navigators. *Proceedings of the annual meeting of the ISMRM*, 2023, Toronto, Canada, p 1017.\n22. M. Serger, R. Stirnberg, P. Ehses, T. Stoecker. Combining FID navigators with field probe monitoring for improved head motion tracking and prospective correction at 7T. *Proceedings of the annual meeting of the ISMRM*, 2023, Toronto, Canada, p 1834.\n23. R. Stirnberg, T. Stöcker. Segmented K-space blipped-controlled aliasing in parallel imaging for high spatiotemporal resolution EPI. *Magn Reson Med 2021* ;85 :1540-1551.\n24. C. Lazarus, P. Weiss, N. Chauffert, F. Mauconduit, L. El Gueddari, C. Destrieux, I. Zemmoura, A. Vignaud, P. Ciuciu. SPARKLING: variable-density k-space filling curves for accelerated T2*-weighted MRI. *Magn Reson Med* 2019; 81:3643-3661.\n25. S. Chu, V. Gras, F. Mauconduit, A. Massire, N. Boulant, S. Gunamony. Electromagnetic and RF pulse design simulation based optimization of an eight-channel loop array for 11.7T brain imaging. *Magn Reson Med* 2023; 90:770-783\n\n# Methods\n\n## Data acquisition and processing\n\nThe MR sessions were 90 min long and targeted anatomical T₁, T₂ and T₂* contrasts. A home-made parallel transmission RF coil (pTx) with dedicated virtual observation points for SAR monitoring was used [26]. The coefficient of variation (std/mean) of the B₁⁺ field in static RF shimming mode was 45% over the whole brain and on average over the subjects. Increased power losses at 500 MHz combined with the pairing strategy of the 16 transmit elements to be fed by 8 RF power amplifiers made inversion pulses particularly difficult to design, despite reaching 8% NRMSE on average over the subjects (5% min, 12% max). This underlined the necessity to have high power RF amplifiers (here 2 kW per channel) and the importance of low cable losses, transmit efficiency, a high transmit channels count and to optimize channels pairing. The small flip angle excitation (NRMSE»8% over the 3D brain) and high flip angle refocusing (~13%) pulses were designed with the kT-point [27] and GRAPE [28] approaches respectively, using an active-set algorithm [12] with simultaneous k-space optimization [29] and under explicit hardware (peak power, average power, maximum gradient slew rate) and SAR constraints. The GRAPE pulse was a universal RF pulse [28] and was designed offline on a database constituted of the 6 first subject field maps. The RF and DB₀ field maps were acquired for each subject for the pulse design and shimming using 2D interferometric turbo-FLASH [30] at 5 mm isotropic resolution and 3D multi-echo (TE = 1.6/3.5/6 ms) GRE acquisitions at 2.5 mm isotropic resolution respectively. Sequence parameters for the T₂-weighted variable flip angle turbo spin-echo acquisition were: resolution = 0.55 × 0.55 × 0.55 mm³, TR = 6 s, TA = 13 min, GRAPPA = 3 × 2, TE = 301 ms, matrix = 400 × 400 × 320, bandwidth = 250 Hz/pixel. All acquisitions were performed with up to second order shimming using quadratic programming and computed brain masks. Comparisons obtained with similar data acquired at 3T and 7T revealed less than linear B₀ field dispersions with field strength, indicating more than satisfying results in terms of effective B₀ homogeneity at 11.7T in the brain.\n\nSlice-selective “spoke” pTx pulses [31] were designed for the T₂*-weighted 2D GRE acquisitions. The sequence parameters were FA = 27°, TR = 600 ms, GRAPPA = 2, TE = 20 ms, resolution = 0.2 × 0.2 × 1 mm³, readout bandwidth = 40 Hz/pixel, TA = 4 min 20 s (2 spokes [32] for the axial acquisition) or TA = 8 min 30 s (TIAMO [33] for the sagittal acquisition). Another T₂*-weighted 2D GRE acquisition with resolution = 0.19 × 0.19 × 1 mm³ (2 spokes, TA = 5 min 16 s, same parameters as above otherwise) and a turbo spin-echo sequence of resolution = 0.3 × 0.3 × 1 mm³ (TIAMO, TR = 7 s, TE = 48 ms, bandwidth = 130 Hz/pixel, echo train length = 9, GRAPPA = 4, TA = 4 min 26 s, 7 slices) were implemented on the last volunteer. Careful analysis of the sequences aided with field monitoring [34] and sequence adjustments were performed prior to the in vivo experiments to minimize field perturbations during the acquisitions [35]. For the 0.2 × 0.2 × 1 mm³ high-resolution 2D GRE experiments, similar scans were performed at 3T and 7T on different subjects to visualize the gains brought by field strength (Fig. 2). Using a longer TE at 3T and 7T could increase the contrast to noise ratio but at the expense of SNR. The signal yet was robust with respect to flip angle variations given the slow increase of T₁ versus field strength, making the Ernst angle relatively constant. Acquisitions were performed with 1Tx (body coil)-32Rx, 8Tx-32Rx and 8Tx-32Rx head coils at 3T, 7T and 11.7T respectively.\n\n## Biological protocol and results\n\nThis study (IDRCB 2022-A02321-42) was approved by the French “Agence Nationale de Sûreté et du Médicament” (ANSM) regulatory body and a national ethics committee. Written informed consent was obtained from all volunteers. In addition to the usual counter-indications for MRI which constitute exclusion criteria (pacemakers, implants, metallic objects, tattoos, claustrophobia etc), one notable inclusion criterion was the age of the volunteers, comprised between 18 and 40 years to reduce inter subject variability in genotoxicity test results. Twenty volunteers (24.2±4.8 year old, 8 males) were scanned at 11.7T and performed the tests mentioned below. Another set of twenty volunteers (23.6±6.0 year old, 7 males) was exposed to a 0T, nocebo, field and underwent the same tests (except genotoxicity). For the latter group, the environment was the same 11.7T scanner but with the magnetic field ramped down. All volunteers received the same instructions. To minimize the number of field ramps for the magnet, the study first included the 0T group, followed by the 11.7T one.\n\nAnxiety of the participants was first evaluated with a questionnaire, whereby a score above 20 on the Hamilton scale constituted an exclusion criterion. The participants underwent cognitive (before, during and after the MRI exam) and vestibular (before and after) tests. The cognitive tests inside the MR scanner were performed with and without gradient noise to aim at isolating a potential impact of the loud acoustic noise on the results. Blood samples were drawn before and after the exams of the 11.7T group to conduct a genotoxicity analysis, subcontracted to an external and certified laboratory (GenEvolutioN, Porcheville, France), and see a potential effect due to exposure of the strong magnetic field [15]. Arterial pressure and cardiac pulsation were measured before, during and after the MRI exam.\n\n### Genotoxic tests\nGenotoxicity testing is based on the detection of chromosome damage in human cells. An alternative to measuring structural aberrations in mitotic cells is to measure micronuclei. These are produced from whole chromosomes or acentric fragments that are unable to attach to the spindle at mitosis and appear during the next interphase as small darkly staining bodies adjacent to the main daughter nucleus. Cytochalasin B (Cyto-B), if added to cultures, inhibits cytokinesis (cell division) but not karyokinesis (nuclear division) resulting in the formation of binucleate cells [36] including micronuclei. Having shown that the repetitive exposure to 3T in MRI [15] induces mainly terminal deletions, the micronuclei protocol was performed with cytochalasin B addition at 68h after lymphocyte growth stimulation and with gamma irradiation (IRCM irradiation platform, CEA, Fontenay-aux-roses, France) as positive controls.\n\n### Behavioral tests\nTo assess participants' executive functions, we employed the Attentional Network Task (ANT) [19,20], a paradigm designed to evaluate attentional focus capacity. In a sequence of trials, participants were instructed to promptly indicate the direction (left or right) of a target arrow presented on a computer screen. The target arrow was flanked by additional arrows that could either all align in the same direction as the target (congruent condition) or point towards the opposite direction (incongruent condition). Furthermore, in certain trials, advance cues provided information about the timing and/or location of the impending target.\n\nParticipants underwent this task on four occasions: prior to entering the scanner (Run \"1_out\"), within the scanner with no noise (Run \"2_in\"), inside the scanner with the added noise of an MR sequence (Run \"3_in_noise\"), and outside the scanner (Run \"4_out\"). Evaluations outside the scanner were conducted in a soundproofed room, with participants seated before a computer screen displaying the stimuli. Within the scanner, stimuli were visible through a mirror mounted on the head coil, with projections onto an LCD screen positioned at the rear of the scanner.\n\n### Balance tests\nThe participants' static balance was assessed before and approximately 25 minutes after the MR exposure (0T or 11.7T). A sensation questionnaire was filled after exiting the scanner in another room and before the vestibular test. The volunteers stood for 30s, first with their eyes open, then with eyes closed, on a force platform equipped with dedicated sensors and connected to a computer and software (AbilyCare, Paris, France) returning a stability score (ranging from 0 to 99) [18].\n\n### Results\nIn all tests performed throughout the protocol, no significant differences between the two groups exposed at 11.7T and 0T could be identified (extended data Fig. 3 and Table 1). No statistically significant differences in micronuclei count for genotoxicity for each subject before versus after exposure at 11.7T were found either. Follow up phone calls by the NeuroSpin medical team up to 1 week after exposure at 11.7T did not indicate any abnormality. Six/four out of twenty volunteers exposed to the 0T/11.7T field reported fatigue the same day or the day after. Four/one volunteers belonging to the 0T/11.7T group reported headaches. Notably different sensations experienced between the two groups involve transient dizziness when entering and exiting the magnet, as well as metallic taste in the mouth, which are known minor side effects occurring when moving in a magnetic field.\n\n## References\n\n26. M. Luong, G. Ferrand, E. Chazel, P-F Gapais, V. Gras, N. Boulant, A. Amadon. A Compact 16Tx-32Rx Geometrically Decoupled Phased Array for 11.7T MRI. Proceedings of the annual meeting of the ISMRM, 2023, Toronto, Canada, p 0707.\n\n27. M.A Cloos, N. Boulant, M. Luong, G. Ferrand, E. Giacomini, D. Le Bihan, A. Amadon. kT-points: short three-dimensional tailored RF pulses for flip angle homogenization over an extended volume. Magn Reson Med 2012 ; 67 : 72–80\n\n28. L. Van Damme, F. Mauconduit, T. Chambrion, N. Boulant, V. Gras. Universal nonselective excitation and refocusing pulses with improved robustness to off-resonance for Magnetic Resonance Imaging at 7 Tesla with parallel transmission. Magn Reson Med 2021 ;85 : 678-693.\n\n29. V. Gras, M. Luong, A. Amadon, N. Boulant. Joint design of kT-spokes trajectories and RF pulses under explicit SAR and power constraints in the large flip angle regime. Journal of Magnetic Resonance 261:181-189 (2015).\n\n30. DO Brunner, KP Pruessmann. B1þinterferometry for the calibration of RF transmitter arrays. Magn Reson Med 2009;61:1480–1488.\n\n31. K. Setsompop, LL Wald, V. Alagappan, BA Gagoski, E. Adalsteinsson. Magnitude least squares optimization for parallel radio frequency excitation design demonstrated at 7 Tesla with eight channels. Magn Reson Med 2008;59:908–915.\n\n32. F. Mauconduit, V. Gras, A. Vignaud, N. Boulant. MetaPulse2D: methodology to enable universal slice specic spokes pulses in parallel transmission. Proceedings of the annual meeting of the ISMRM, 2022, London, UK, p 0454.\n\n33. S. Orzada, S. Maderwald, B. A. Poser, A. K. Bitz, H. H. Quick, M. E. Ladd. RF excitation using time interleaved acquisition of modes (TIAMO) to address B1 inhomogeneity in high-field MRI. Magn Reson Med 2010 ;64 :327-333.\n\n34. S.J Vannesjo, M. Haeberlin, L. Kasper, M. Pavan, B.J Wilm, C. Barmet, K.P Pruessmann. Gradient system characterization by impulse response measurements with a dynamic field camera. Magn Reson Med 2013; 69:583–593\n\n35. N. Boulant, C. Le Ster, A. Amadon, G. Aubert, A. Beckett, J. Belorgey, C. Bonnelye, D. Bosch, D. O Brunner, G. Dilasser, O. Dubois, P. Ehses, D. Feinberg, S. Feizollah, V. Gras, S. Gross, Q. Guihard, H. Lannou, D. Le Bihan, F. Mauconduit, F. Molinié, F. Nunio, K. Pruessmann, L. Quettier, K. Scheffler, T. Stöcker, C. Tardif, K. Ugurbil, A. Vignaud, A. Vu, X. Wu. The possible influence of third-order shim coils on gradient–magnet interactions: an inter-field and inter-site study. Magn Reson Mater Phys. 2024 ; https://doi.org/10.1007/s10334-023-01138-3.\n\n36. M. Fenech, AA Morley. Measurement of micronuclei in lymphocytes. Mutat Res. 1985 Feb-Apr;147(1-2):29-36. doi: 10.1016/0165-1161(85)90015-9. PMID: 3974610.\n\n# Supplementary Files\n\n- [NatMetANTResults.tif](https://assets-eu.researchsquare.com/files/rs-3931535/v1/3656247642111aea60710a5a.tif) \n *Extended data Figure 3:* Results of the Attentional Network Task. Panel A (left). Mean decision times as a function of Run and Group. Both groups were slower inside the scanner than outside, which could be due to differences in the visibility of the stimuli (light conditions, distance from the screen). Panel B (right). Flanker cost (difference in decision-times between incongruent and congruent trials). Effects or interactions involving the Group factor were very small and not statistically significant (all p-values >0.1 in an analysis of variance), showing that field exposure has a negligible impact on attention (error bars indicate ±1 standard error).\n\n- [ExtendeddataTable1.docx](https://assets-eu.researchsquare.com/files/rs-3931535/v1/ebb24a23140a5c759dab159e.docx)"} {"paper_id": "prb60", "title": "Compound mortality impacts from extreme temperatures and pandemics", "text": "# Abstract\n\nClimate change and coronavirus-type pandemics are both major global health threats. Until now, no study has quantified the compound health consequences of the co-occurrence of these crises. We estimate the mortality attributable to short-term heat and cold events, which dominate the UK health burden from weather hazards, in England and Wales in the period 2020-2022, during which the COVID-19 pandemic peaked in terms of mortality. We show that temperature-related mortality exceeded COVID-19 mortality by 8% in South West England. Combined, extreme temperatures and COVID-19 led to 19 (in North West England) to 24 (in Wales) excess deaths per 100,000 population during heatwaves, and 80 (in Yorkshire and the Humber) to 127 (in East of England) excess deaths per 100,000 population during cold snaps. These numbers are at least ~2 times higher than the previous decade. Society must increase preparedness for compound health crises such as extreme weather coinciding with pandemics.\n\nEarth and environmental sciences/Natural hazards \nEarth and environmental sciences/Climate sciences/Climate change/Climate-change impacts\n\n# Introduction\n\nClimate change is deeply embedded in the long-term global health concern1, with much of its direct health burden coming from extreme weather events. However, it is a crisis that is nearly always considered in isolation from other crises, even though there can be compound socio-economic impacts when major crises occur in parallel. While the climate-conflict nexus is relatively well studied2, 3, other parallel crises such as climate change and obesity, climate change and artificial intelligence, and, as studied here, extreme weather and pandemics, are far less investigated.\n\nExtreme weather events are “shattering” observational records, disrupting infrastructure, and, in the worst cases, claiming lives4, 5. In the period that the most recent global pandemic – COVID-19 – was officially declared a public health emergency of international concern by the World Health Organization (between January 2020 and March 2023), the UK recorded 40.3°C unprecedented extreme heat6 and a record number of around 3,000 heatwave excess deaths7, western North America experienced one of the most extreme heatwaves ever recorded globally8 that led to hundreds of deaths9, Pakistan had floods that killed nearly 2,000 people and displaced 7 million more10, and the Horn of Africa experienced persistent droughts that led to over 3 million people requiring humanitarian assistance11. These life-threatening weather events, attributable in part to human-induced climate change12–14, prompted scientists to warn about compound societal risks arising from the intersection of climate hazards and pandemics like COVID-1915.\n\nOne way that the intersection of extreme weather events and pandemics can result in major societal risks is through overwhelming health systems. If health services are already operating at capacity because of one crisis, the additional health burden from another crisis can break the system entirely, endangering the lives of many people. From the emergence of COVID-19 in December 2019 to the writing of this paper in late 2023, almost 7,000,000 COVID-19 deaths have occurred worldwide16, with Peru and Bulgaria having the highest numbers of confirmed deaths per one million population17. In the UK, about 230,000 people, or 0.3% of the total population, have died from COVID-19 according to death certificates18. These numbers would likely have been much higher had there not been preventative measures put in place, such as social restrictions or vaccination19–21. The rapid development, severity, and adverse impacts of the pandemic on public health and the functioning of society meant that it dominated global news and everyday life for an extended period of time22.\n\nHowever, the exact respective and compound health impacts of extreme weather and COVID-19 remain unknown. Understanding these impacts from observations of recent events is extremely important to inform climate adaptation, long-term pandemic preparedness, and public health solutions that simultaneously address both15.\n\nHere, we use England and Wales as a well-observed and well-documented case study to illustrate the respective and combined mortality impacts of weather hazards and COVID-19, in the period between 30 January 2020 and 31 December 2022. The first COVID-19 death recorded on a death certificate in England and Wales was on 30 January 2020 (in South East England), so this date is chosen as the starting date for this study. We choose England and Wales because we already have location-specific epidemiological models linking temperature variability to daily mortality set up for regions within them23, and that daily COVID-19 mortality statistics for the same sub-national regions are publicly available from the UK Government dashboard18.\n\nWe consider excess mortality associated with non-optimal high and low temperatures because it dominates the short-term health impact of other weather hazards24, including floods, storms, and droughts in the UK25. Temperature-related mortality is also relatively straightforward to quantify through time series epidemiological modelling. Specifically, we focus on the hottest (heatwaves) and coldest (cold snaps) days during the study period, in order to understand the compound impacts when regional extreme temperatures coincide with the global pandemic.\n\n# Results\n\nFigure 1a shows that heat-related mortality (red lines, with red shading indicating its 95% confidence interval) in England and Wales primarily occurred between July and September during the study period of 30 January 2020 to 31 December 2022. A total of 8,481 excess deaths (95% confidence interval: 6,387–10,493) were attributable to high temperatures, with daily heat-related mortality peaking at 580 deaths (95% confidence interval: 484–670) on 19 July 2022, when England recorded 40.3°C unprecedented extreme heat. Figure 1b zooms in on the time evolution of mortality during this heatwave for greater legibility. Although the UK Met Office and UK Health Security Agency (UKHSA) had issued Level 2 (yellow) and Level 3 (amber) Heat Health Alerts for all regions except North East England since 11 July 2021 to warn the public about this heatwave, which they subsequently raised to the highest Level 4 (red) alert for all regions on 18 July 2021 to trigger a national emergency response26, peak heat-related mortality during this heatwave exceeded the maximum daily level from the previous ten years (i.e., 2010–2019; red error bar in Figure 1a), which was 376 deaths (95% confidence interval: 304–445).\n\nIn months other than July, August and September, cold-related mortality (blue lines, with blue shading indicating its 95% confidence interval) dominated over heat-related mortality. Over the study period, a total of 128,533 excess deaths (95% confidence interval: 107,430–153,642) were attributable to low temperatures, indicating a fifteen-fold larger cold than heat mortality burden. These results are consistent with the literature, which found that most days of the year are considered moderately cold in England and Wales in distributed lag non-linear models (DLNMs) for health modelling, resulting in a large number of cold-related deaths27. Daily cold-related mortality peaked at 531 excess deaths (95% confidence interval: 493–574) on 15 December 2022, but this falls within the range from the previous ten years (maximum: 691 deaths, 95% confidence interval: 643–743).\n\nThese temperature-related deaths are theoretically independent of COVID-19 deaths because they are calculated from DLNMs that describe the relationships between daily mean temperature and daily all-cause mortality, after COVID-19 mortality has been removed (see Methods). For comparison, Figure 1 also shows the time evolution of daily COVID-19 mortality according to death certificates (purple lines). Distinct surges in COVID-19 deaths were seen soon after the first emergence of COVID-19 in early 2020 and the domination of the Alpha variant in December 2020 (dotted vertical line in Figure 1a)28, with the highest daily mortality level being 1,382 deaths on 19 January 2021. The emergence of the Delta and Omicron variants were not followed by as large a surge in deaths, likely because COVID-19 vaccination had become more common by then (see Figure S1), with about half of the population above the age of 12 having had two doses of COVID-19 vaccines by 1 July 2021 (solid vertical line in Figure 1a), in all regions in England and Wales except London (see Table S1). Over the whole study period, 194,480 COVID-19 deaths were reported on death certificates in England and Wales.\n\nFigure 1a shows that from June to October 2020, March to August 2021, and from September 2021 to the end of 2022, temperature-related deaths (the sum of heat- and cold-related deaths) exceeded COVID-19 deaths. These exceedances were driven by heat-related mortality spikes when COVID-19 mortality was relatively low, e.g., during the July 2022 heatwave (Figure 1b), as well as cold-related mortality dominating in the colder months after COVID-19 vaccination was introduced. To further examine the respective mortality impacts of non-optimal temperatures and COVID-19, Figure 2 shows the ratios of cumulative deaths from these two causes for each region in England and Wales, across the whole study period (panel a), and during heatwaves and cold snaps therein (panels b and c).\n\nConsidering the whole study period of 30 January 2020 to 31 December 2022, cumulative temperature-related deaths exceeded cumulative COVID-19 deaths by 8% in South West England. While this exceedance did not occur in the other regions, temperature-related deaths amounted to 58% (East Midlands) to 75% (London) of COVID-19 deaths by the end of 2022. These results demonstrate that even during a global pandemic that dominated everyone’s lives, heat and cold were a comparable but arguably much more under-reported killer than COVID-19. Reducing temperature-related mortality would free up resources and capacity for the health services to respond to major pandemics when they occur.\n\nSince extreme weather events are where we would expect the health effects to be largest, focusing on them provides important information on their interplay with other parallel health crises, including their compound health effects. Figure 2b shows that during the ten heatwave episodes (spanning a total of 70 days; see Table S2) in the study period, identified through UKHSA’s Heat Mortality Monitoring Reports26,29,30, temperature-related deaths outnumbered COVID-19 deaths in 9 of the 10 regions (except in North West England). This exceedance is particularly apparent in the southern regions where heat stress is more pronounced31. The ratios of temperature-related deaths to COVID-19 deaths in the southern regions range from 1.7 in East of England and South East England to 2.7 in London. The ratios for the rest of the regions lie between 1.1 and 1.3, except for North West England which has a ratio of 0.8. These results highlight that even during the COVID-19 pandemic, heatwaves posed a serious threat to public health, which is often downplayed32 or misrepresented as something enjoyable by the media in the UK33.\n\nFigure 2c shows the corresponding results during eight cold snaps in the study period, which are defined here as days on which a Level 3 Cold Health Alert was issued by UKHSA for any region in England (also spanning 70 days; see Table S2). A Level 3 (amber) Cold Health Alert represents a situation in which impacts are likely to be felt across the health and social care sectors, and potentially the whole population34. During these cold snaps, temperature-related deaths were lower than COVID-19 deaths in all regions, with the ratios ranging from 0.4 in East of England to 0.8 in South West England. These results are likely to be driven by the large surges in COVID-19 mortality following the first emergence of the coronavirus and the domination of the Alpha variant, both of which occurred in winter (Figures 1a and S1). In this sense, our results should not be interpreted as low temperatures being less important than COVID-19 to health in winter, as we have already shown that cold-related mortality occurs throughout the year and dominated over COVID-19 in the second half of the study period (Figure 1a). Future outbreaks of COVID-19 or novel viruses could have a different seasonal pattern from the COVID-19 pandemic studied here. Therefore, they could have different health impacts relative to extreme cold in winter.\n\nThe co-occurrence of non-optimal temperatures and COVID-19 meant that all-cause mortality in England and Wales was, on average, higher in the study period than in the previous ten years (black line and bar in Figure 1a). During extreme events, the health system needed to deal with an unprecedented compound health impact from both extreme weather and COVID-19. Figure 3a shows the total number of deaths arising from high temperatures and COVID-19 during the 70 heatwave days in the study period. Regional compound (heat-related and COVID-19) mortality ranged from 19 deaths per 100,000 people (95% confidence interval: 16–22) in North West England, to 24 deaths per 100,000 people (95% confidence interval: 20–29) in Wales.\n\nThese compound mortality levels are put into context by comparing Figure 3a with Figure 3c, which shows the reference levels of heat-related mortality from 70 heatwave days, calculated from the average of all identified heatwaves in the ten years that preceded COVID-19 (i.e., 2010–2019; see Methods). Substantially fewer heat-related deaths occurred during 70 heatwave days in 2010–2019, with the regional number ranging from 5 deaths per 100,000 people (95% confidence interval: 3–8) in North West England, to 13 deaths per 100,000 people (95% confidence interval: 12–15) in London. In other words, demand on regional health services was 1.7 (London) to 3.8-fold (North West England) when extreme heat coincided with COVID-19 in the study period, compared to the previous decade.\n\nDuring the 70 cold snap days in the study period (30 January 2020 to 31 December 2022), regional compound (cold-related and COVID-19) mortality ranged from 80 per 100,000 people (95% confidence interval: 75–86) in Yorkshire and the Humber, to 127 deaths per 100,000 people (95% confidence interval: 123–132) in East of England (Figure 3b), highlighting the higher absolute demand on the health system during cold snaps that heatwaves in the study period. These compound mortality numbers are substantially higher than the reference numbers of cold-related deaths from the same number of cold snap days in 2010–2019 (Figure 3d), which ranged from 34 deaths per 100,000 people (95% confidence interval: 31–38) in London, to 48 deaths per 100,000 people (95% confidence interval: 34–50) in North East England. This means that depending on the region, demand on health services was 2.1 (South West England) to 3.5-fold (East of England) when extreme cold co-occurred with COVID-19, compared to extreme cold in the previous decade.\n\nBy adding temperature-related deaths (with COVID-19 deaths removed prior to calculation) and COVID-19 deaths together to estimate the compound mortality impact, we have assumed that they are independent of each other. Figure 4 shows the average number of temperature-related deaths per 100,000 population per day of individual heatwaves (panel a) and cold snaps (panel b) in all regions in 2016–2019 (non-COVID-19 years; grey markers) and 2020–2022 (COVID-19 years; coloured markers), versus the average temperatures of these events. While heat-related mortality generally increased with the average heatwave temperature for all events, and cold-related mortality generally decreased when cold snaps were milder, the extreme temperature events that co-occurred with COVID-19 have different distributions (grey dashed lines) from the events that occurred without COVID-19 co-occurrence (black solid lines). For heatwaves (Figure 4a), mean temperature and heat-related mortality shifted higher in the COVID-19 years, compared to events that were not affected by COVID-19. For cold snaps (Figure 4b), the variances in temperature and cold-related mortality were larger in events in the COVID-19 years than non-COVID-19 years. Two-sample Kolmogorov–Smirnov tests confirm that the COVID-19 event distributions are significantly different from the non-COVID-19 distributions at the 5% significance level. These results suggest that COVID-19 may have impacted temperature-related mortality during extreme weather events.\n\nOn the other hand, extreme heat may have exacerbated COVID-19 mortality in England and Wales too. This is evident on the hottest day ever recorded in the UK (19 July 2022), when the 91 more daily COVID-19 deaths occurred, compared to the average on days between 10 July and 25 July 2022 (Figure 1b). Modelling COVID-19 mortality is not within the scope of this study, but our results highlight the complex interplay between extreme temperatures and the COVID-19 pandemic, as well as its implications on population health and health services capacity.\n\n# Discussion\n\nThe 2023 UK National Risk Register states that extreme weather events and pandemics are two of the most serious risks facing the UK, alongside other risks such as terrorism, cyber attacks and conflicts35. In this study, we have demonstrated the respective mortality impacts of extreme temperatures and COVID-19, as well as the substantial compound mortality impact arising from the co-occurrence of these two crises, on all regions in England and Wales. UK summers are becoming hotter in a warming climate36, and extreme heat events are increasing in frequency, intensity, and duration. While UK winters are generally becoming milder36, extremely cold episodes driven by natural climate variability, such as the 2018 “Beast from the East”, will still have a large adverse health impact. Viewing extreme heat and cold as serious health threats on a par with the COVID-19 global pandemic and other major crises is an important first step to preventing further loss of lives to extreme weather.\n\nWith the latest long-term forecasts of COVID-19 for the UK predicting a steady 95% effective population immunity and a reduced death rate until at least May 202437, it is probable that cumulative temperature-related deaths would exceed COVID-19 deaths in more regions than South West England (Figure 2) in the next 2 to 5 years (not shown). While extreme temperatures cannot be vaccinated against, interventions such as increasing tree coverage in cities38, adding reflective or green roofs to buildings39, and installing external shutters to the housing stock40 have been shown to reduce the health risk of heat. Fitting mechanical ventilation with heat recovery systems in homes can simultaneously improve insulation and improve energy efficiency in the colder months, thereby reducing the health risk of cold, while maintaining ventilation41. It is vital to implement these interventions in urban planning and housing regulations, in order to improve population resilience to heat and cold in the UK.\n\nRecent analyses of NHS hospital beds show a persistent decline in the total number of beds, by 11% in England and 15% in Wales in the period 2010–202242,43. Even before the COVID-19 pandemic, average hospital bed occupancy consistently surpassed 85%, a level widely considered to be the upper limit for hospitals to operate safely and effectively44. Many hospitals trusts regularly exceeded an even higher capacity of 95% in winter42. These statistics highlight a significantly overwhelmed health system in England and Wales. The deadly consequences of an already overwhelmed NHS severely stretched to function through the compound crises of extreme weather and COVID-19, whose mortality impacts are additive to the first order, are clear in this paper. Decisive actions to improve NHS ability to substantially increase bed numbers and staff availability with little notice, since major crises tend to occur abruptly, are extremely important to build health resilience for future crises.\n\nAnticipating and preparing for the co-occurrence of extreme weather events and major disease outbreaks like COVID-19 would be lifesaving, not least because they share commonalities in who in the population are particularly vulnerable to them. For instance, extreme heat and cold adversely affect the health of older people (above the age of 65), young children (under the age of 5), people with pre-existing health conditions such as cardiovascular, respiratory and kidney conditions (kidney disease is a risk factor for heat-health), those who are socially isolated, those who are homeless, and those who live in deprived circumstances (a risk factor for cold-health), more than other population groups34,45,46. A number of these groups such as older people, people with various pre-existing conditions including severe asthma and chronic kidney disease, and those who are deprived are also at a higher risk of dying from COVID-19 in the UK47,48. Enhancing access to health and care services, support and guidance for these groups would simultaneously address their vulnerability to extreme weather and a future coronavirus-type outbreak, which is still a priority disease with pandemic potential according to the WHO, along with Zika, haemorrhagic fevers, influenza, and “disease X” (an unexpected new disease)49.\n\nBecause of the common risk factors for temperature-related and COVID-19 mortality, disentangling their effects on health and attributing mortality to a single cause is challenging. Here, we have suggested that COVID-19 may have confounded with temperature-related mortality in England and Wales during heatwaves or cold snaps in the period 2020–2022 (Figure 4), although the number of extreme temperature events sampled is limited by the short study period. This result is consistent with previous hypotheses that COVID-19 acted as a risk amplifier of heat-health impacts in the UK23 and other countries including Portugal50, potentially due to increased vulnerability, social restrictions, and people not seeking healthcare during the pandemic. On the contrary, another previous study found similar heatwave mortality in England in 2020 and the pre-pandemic period of 2016–2018, with no indication of more at-home heat-related deaths linked to COVID-19 social restrictions51.\n\nFuture work is recommended to understand the confounding effect(s) of COVID-19 on temperature-related health outcomes. For example, instead of using all available observed temperature and mortality data (1981–2022 data, but with reported COVID-19 mortality removed) to construct the DLNMs here (see Methods), future work can derive temperature-mortality associations using only data from the COVID-19 time period. We have not done this because two years of data (in the COVID-19 period of 2020–2022) are not enough to derive constrained temperature-mortality associations with low uncertainty on the regional level. This limitation will be reduced when more data become available going forward. Future work can also investigate the feasibility of controlling for time-varying COVID-19 effects in the models.\n\nOn the other hand, we have shown above-average COVID-19 mortality in July 2022 when temperatures were unprecedentedly high (Figure 1b). Detailed modelling of COVID-19 infections and mortality is out of the scope of this study, but future research on this topic is extremely important because the literature is inconclusive about the effect of temperature and humidity on the transmission of COVID-19, with some of these studies contradicting each other. For instance, previous studies found (i) low temperatures and/or low absolute humidity increased transmission52, but only in the absence of policy interventions such as lockdowns53; (ii) modest non-linear associations between these variables and COVID-19 transmission54; and (iii) no association between temperature and COVID-19 but weak negative associations with absolute and relative humidity55. Recent research found that most of the studies about weather effects on COVID-19 spread that were published in 2020 and 2021, did not include a time lag between weather exposure and reported COVID-19 cases, did not properly account for seasonality or other confounding factors of disease transmission, or did not go through rigorous peer review56. These aspects need to be thoroughly considered in future research, for the purpose of long-term planning and preparedness that are resilient to climate change.\n\n# Methods\n\n## Distributed Lag Nonlinear Models (DLNMs)\n\nFor each region in England and Wales, we derive the non-linear association between daily average temperature and daily mortality in the period 1981–2022. We calculate daily average temperature by averaging the daily maximum and minimum temperatures in the HadUK-Grid Climate Observations by Administrative Regions over the UK dataset57. We use daily all-cause death occurrences across all age and sex groups in the same time period. These data are provided by the Office for National Statistics (see Data availability). Since the 2020–2022 mortality data include COVID-19 deaths, which we want to separate from temperature-related deaths in this study, we remove deaths with COVID-19 on the death certificate from the all-cause mortality data. We then derive the non-linear association between the temperature and mortality time series using quasi-Poisson regression with DLNMs, adapting the methods from previous studies58.\n\nBriefly, we model the temperature-mortality association for each region using natural cubic splines with three internal knots at the 10th, 75th, and 90th percentiles of the 1981–2022 temperature distribution of that region. Since we are interested in both heat- and cold-related mortality, year-round temperatures are considered. It is known that the mortality effect of exposure to heat and cold can take up to a few days (heat) and a few weeks (cold) to be observed58, so we include a time lag association in each DLNM. We model this association with natural cubic splines with three internal knots that are equally spaced in the log-scale, following a standard set up in the literature27. We consider a maximum lag period of 21 days, which has been shown to be sufficient to capture cold health effects59.\n\nIn the main quasi-Poisson regression model, we also include an indicator of day of the week and a natural cubic spline of time with 8 degrees of freedom per year. This follows a standard set up in the literature59 and controls for residual variation and seasonality in the data. Through the methods described above, we find the overall temperature-mortality association across the 21-day lag period for each region in England and Wales. This overall association is centred on a ‘minimum mortality temperature’ (MMT) corresponding to the region. We constrain the MMT to the 2nd to 98th percentiles of the 1981–2022 daily average temperature distribution of the region. By definition, mortality risk at the MMT is the lowest among all observed temperatures of the same region. Increased mortality risk is expected above (considered as heat-related mortality) and below (cold-related mortality) the MMT.\n\nBased on the observed daily average temperature between 30 January 2020 and 31 December 2022 from HadUK-Grid, the derived mortality risk at each temperature, and the average number of all-cause deaths (excluding COVID-19 deaths) for each calendar day in a year based on the 1981–2022 period, best estimates of heat- and cold-related mortality for each day in the study period are calculated for each region. Their 95% empirical confidence intervals are estimated through Monte Carlo simulations of the spline model coefficients 100 times, assuming that the coefficients have a multivariate normal distribution.\n\n## Heatwaves and cold snaps before 2016\n\nThroughout this study, we focus on heatwaves and cold snaps when extreme temperatures have the largest mortality impacts. The dates of these events are extracted from the UKHSA Heatwave Mortality Reports and historical Level 3 Cold Health Alerts, as mentioned in the main text. However, these reports and the alerts record available to us only start in 2016, so we find the dates of heatwaves and cold snaps based on the same criteria for the period 2010–2015 for Figure 3. For heatwaves, we find days on which there was a UKHSA Level 3 Heat Health Alert, or days with a mean central England temperature greater than 20°C, plus one day before and after the time period identified through the first two criteria. The 2010–2015 heatwaves defined this way are published in the literature23. For cold snaps, we find periods during which any region in England and Wales had an average temperature below 2°C for two consecutive days or more. This follows the temperature criterion for a Level 3 Cold Health Alert in 201660.\n\n## Deaths per 100,000 population\n\nWe present number of deaths (temperature-related or COVID-19) per 100,000 population in the latter part of this manuscript to enable comparison of the results across the studied regions. These are calculated based on the mid-2021 UK population estimates provided by the Office for National Statistics (see Data availability). The regional population data are as follows - North East England: 2,646,772; North West England: 7,422,295; Yorkshire and the Humber: 5,481,431; East Midlands: 4,880,094; West Midlands: 5,954,240; East of England: 6,348,096; London: 8,796,628; South East England: 9,294,023; South West England: 5,712,840; and Wales: 3,105,410.\n\n# References\n\n1. Kanem N, Murray CJL, Horton R (2023) The Lancet Commission on 21st-Century Global Health Threats. The Lancet 401:10–11\n2. von Uexkull N, Buhaug H (2021) Security implications of climate change: A decade of scientific progress. *Journal of Peace Research* vol. 58 3–17 Preprint at https://doi.org/10.1177/0022343320984210\n3. Koubi V (2019) Climate Change and Conflict. Annu Rev Polit Sci 22:343–360\n4. Hopke JE (2020) Connecting Extreme Heat Events to Climate Change: Media Coverage of Heat Waves and Wildfires. Environ Commun 14:492–508\n5. Stoddart MCJ, Ramos H, Foster K (2023) Ylä-Anttila, T. Competing Crises? 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NHS hospital beds data analysis (2023)\n43. NHS Wales (2023) NHS beds by organisation and year, 2009-10 onwards. *Welsh Government* https://statswales.gov.wales/Catalogue/Health-and-Social-Care/NHS-Hospital-Activity/NHS-Beds/nhsbeds-by-organisation-site\n44. Pratt AC, Wood RM (2021) Addressing overestimation and insensitivity in the 85% target for average bed occupancy. Int J Qual Health Care 33:1–7\n45. Ballester J et al (2023) Heat-related mortality in Europe during the summer of 2022. Nat Med 29:1857–1866\n46. Ebi KL et al (2021) Hot weather and heat extremes: health risks. The Lancet 398:698–708\n47. Williamson EJ et al (2020) Factors associated with COVID-19-related death using OpenSAFELY. Nature 584:430–436\n48. Gansevoort RT, Hilbrands L (2020) B. CKD is a key risk factor for COVID-19 mortality. Nat Rev Nephrol 16:705–706\n49. Looi MK (2023) What could the next pandemic be? *Bmj* https://doi.org/10.1136/bmj.p909\n50. 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Department of Health Guidance 1–57\n\n# Supplementary Files\n\n- [Lotempcovidpapersupplv2.docx](https://assets-eu.researchsquare.com/files/rs-3866346/v1/c97a7ae4348477cfa8ab1680.docx)"} {"paper_id": "prb61", "title": "Population aging challenge future mitigation of deaths attributable to PM2.5 pollution in China", "text": "Population aging challenge future mitigation of deaths attributable to PM2.5 pollution in China\n\nFangjin Xu\nBeijing Normal University\nQingxu Huang ( qxhuang@bnu.edu.cn )\nBeijing Normal University https://orcid.org/0000-0003-4902-716X\nHuanbi Yue\nOcean University of China\nXingyun Feng\nBeijing Normal University\nHaoran Xu\nBeijing Normal University\nChunyang He\nBeijing Normal University https://orcid.org/0000-0002-8440-5536\nPeng Yin\nThe National Center for Chronic and Noncommunicable Disease Control and Prevention\nBrett Bryan\nDeakin University https://orcid.org/0000-0003-4834-5641\n\nArticle\n\nKeywords: PM2.5 pollution, population aging, CMIP6, shared socioeconomic pathways, representative concentration pathways, public health\n\nPosted Date: May 20th, 2022\n\nDOI: https://doi.org/10.21203/rs.3.rs-1618374/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\nPopulation aging challenge future mitigation of deaths attributable to PM_{2.5} pollution in China\n\nFangjin Xu^{1,2}, Qingxu Huang^{*,1,2}, Huanbi Yue^{3}, Xingyun Feng^{1,2}, Haoran Xu^{1,2}, Chunyang He^{1,4,5}, Peng Yin^{6}, Brett A. Bryan^{7}\n\n1 State Key Laboratory of Earth Surface Processes and Resource Ecology, Beijing Normal University, Beijing, 100875, China\n2 School of Natural Resources, Faculty of Geographical Science, Beijing Normal University, Beijing, 100875, China\n3 School of International Affairs and Public Administration, Ocean University of China, Qingdao, 266100, China\n4 Key Laboratory of Environmental Change and Natural Disasters, Ministry of Education, Beijing Normal University, Beijing 100875, China\n5 Academy of Disaster Reduction and Emergency Management, Ministry of Emergency Management and Ministry of Education, Beijing 100875, China\n6 National Center for Chronic and Non-communicable Disease Control and Prevention, Chinese Center for Disease Control and Prevention, Beijing 100050, China\n7 Centre for Integrative Ecology, Deakin University, Melbourne, VIC3125, Australia\n\n* Corresponding author at:\nState Key Laboratory of Earth Surface Processes and Resource Ecology, Beijing Normal University, 19 Xinjiekouwai Street, Beijing, 100875, China. E-mail: qxhuang@bnu.edu.cn.\nPopulation aging challenge future mitigation of death attributable to PM_{2.5} pollution in China\n\nAbstract: Estimating the health burden of air pollution in China against the background of population aging is of great significance for the well-being of elderly individuals and achieving the United Nations Sustainable Development Goals (SDGs). Since previous studies did not fully consider the differences on drivers of deaths attributable to PM_{2.5} pollution (DAPP) (i.e., socioeconomic factors, climate factors, and disease mortalities) among provinces in China, the impact of future population aging on DAPP cannot be comprehensively and objectively estimated. In this study, we estimated and verified the spatiotemporal changes of DAPP in China from 2005 to 2017 based on a risk assessment framework. Then, using the latest climate projections, we estimated the changes and drivers in DAPP under four scenarios in China from 2018 to 2035 based on decomposition analysis. The results show that from 2017 to 2035, DAPP in China will decrease between 31.9 (26.6-45.6) thousand and 178.8 (152.5-210.5) thousand across three scenarios (sustainable development (SSP1-2.6), business as usual (SSP2-4.5), and fossil fuel development (SSP5-8.5)). We found that population aging will be the leading driver contributing to the increase in DAPP and offset the positive gains achieved by improvement in air pollution and healthcare. In the future, reducing the exposure to air pollution and improving healthcare of the elderly is necessary to mitigate the global health burden of air pollution and this requires mutual cooperation and long-term efforts among countries worldwide.\n\nKey words: PM_{2.5} pollution, population aging, CMIP6, shared socioeconomic pathways; representative concentration pathways; public health\n\n1. Introduction\n\nRecently, air pollution caused by particulate matter with a diameter of 2.5 \\( \\mu \\)m or less (i.e., PM_{2.5}) has increased dramatically^{1}. Exposure to PM_{2.5} pollution has adverse effects on human health, such as premature death and pulmonary and cardiovascular disease^{2,3}. Consequently, the number of deaths attributable to PM_{2.5} pollution (DAPP) globally has also increased rapidly, from 1.14 million to nearly 3 million between 2005 and 2017^{4}, becoming the fifth-leading mortality risk factor^{5}. In parallel, the world’s population is aging which is further exacerbating the negative health effects of air pollution^{6-8}. From 2005 to 2017, the proportion of elderly population (i.e., those aged 65 and older) rose from 7.3% to 8.6% globally, making it the fastest growing age group^{9}. It is estimated that in 2016, 69% of global air pollution-related deaths were among the elderly^{10}. In the future, the proportion of elderly population is expected to rise to 19% by 2050^{11}.\n\nChina is experiencing particularly acute population aging, with the proportion of elderly growing from 7.0% to 12.6% from 2000-2019. It is expected that by 2030 and 2050, this proportion will increase to 17.1% and 26.3%, respectively^{11}, peaking at 437 million people by 2051^{12}. The United Nations Sustainable Development Goal (SDG) 3 states that “people of all ages need to live\nhealthy lives and that a substantial reduction in air pollution-related deaths needs to be achieved by 2030\\(^{13}\\). Understanding the health effects of air pollution in the context of population aging in China is of great significance for promoting the well-being of elderly people and the insights gained can help other countries deal with the health burden of air pollution in the context of population aging, promoting global progress towards the SDGs.\n\nCurrently, some studies have quantified DAPP in China and focused on the impact of population aging on DAPP\\(^{7,14}\\). In addition to the age structure of the population, DAPP is also affected by other socioeconomic development factors (e.g., medical conditions, and air pollution emissions) and climate change (e.g., transformation and diffusion of air pollution)\\(^{15,16}\\). Many studies have estimated the changes of DAPP in the future considering the change of socioeconomic development or climate change\\(^{17,18}\\). However, we still have a limited understanding of the future dynamics of DAPP for at least two reasons. First, from the perspective of scenario setting, most studies mainly focus on the changes in DAPP under the influence of a single factor, which does not consider the driving effect of socioeconomic development and climate change on DAPP simultaneously. For example, Maji et al\\(^{19}\\) only considered the changes in pollutant concentration in the context of the air pollution prevention and control policy and ignored the changes in socioeconomic factors such as population and medical conditions. Shen et al\\(^{20}\\) studied the impact of population migration on DAPP in China and did not consider the impact of climatic factors on DAPP. Although Rafaj et al\\(^{21}\\) considered the impact of the age structure on DAPP, their scenario setting was mainly based on the paths of climate change, ignoring changes in other socioeconomic factors such as medical conditions. Secondly, from the perspective of the data, most studies in China did not fully account for the differences in climatic factors and socioeconomic factors among provinces, which could affect the reliability of the estimations. For example, Yue et al\\(^{22}\\) predicted China's DAPP in 2030 in different air pollution prevention and control policy scenarios. This scenario setting does not take into account the differences in PM\\(_{2.5}\\) concentration changes in different provinces in the future. In addition, the health data used by Wu et al\\(^{23}\\) were national-scale data obtained from the Global Burden of Disease\\(^{24}\\) and did not include the differences in health levels across provinces. The population data used by Liu et al\\(^{17}\\) are also national-scale data, ignoring regional differences in population aging in China. In summary, we still do not have a reliable and effective estimate of DAPP that accounts for the driving factors of socioeconomic pathways and changes in climate across different provinces in China.\n\nThe sixth Coupled Model Intercomparison Project (CMIP6) considers socioeconomic development as well as climate change factors and can reflect the interaction between them, providing the possibility to effectively predict DAPP in the future. CMIP6 combines representative concentration pathways (RCPs) with shared socioeconomic pathways (SSPs). Specifically, RCPs are multi-model global scenarios of greenhouse gases that use the radiative forcing per unit area at the end of the century to represent the climate impact of future greenhouse gas concentrations, covering a variety of climate mitigation levels and providing the basis for the simulation of PM\\(_{2.5}\\) in different climate change scenarios. SSPs are socioeconomic development scenarios related to greenhouse gas emissions that take socioeconomic aspects such as economy, population, technology, lifestyle, policies, and institutions into account, making it possible to study the socioeconomic factors affecting DAPP. In addition, Yin et al\\(^{10}\\) estimated disease mortality associated with air\npollution across provinces in China from 1990 to 2017, providing an important database for estimating differences in DAPP at the provincial scale. Decomposition analysis\\(^{22}\\) can transform the nonlinear relationship between DAPP and its various drivers into a simple linear relationship, which takes into account the interaction between the various factors. Therefore, based on the CMIP6 dataset, provincial-level disease mortality data and decomposition analysis, this paper can study the driving effects of socioeconomic changes (especially population aging) and climate change on DAPP and their differences at the provincial scale in China.\n\nThe purpose of this study is to estimate the temporal and spatial patterns of DAPP and the impact of population aging in China under alternative future scenarios considering both socioeconomic development and climate change. We first estimated and verified the spatiotemporal pattern of DAPP in China from 2005 to 2017 based on the comparable risk assessment framework. Then, we estimated the changes in DAPP in China in different scenarios from 2018 to 2035 by combining the RCPs and SSPs. Based on the results, the influence of population aging as well as other driving factors (e.g., population growth, change in PM\\(_{2.5}\\) concentrations and disease mortalities) were evaluated via decomposition analysis. The differences across regions are discussed and policy recommendations are made for improving public health.\n\n2. Results\n\n2.1 Trends in driving factors\n\nFrom 2000 to 2017, China has experienced a steady increase in population by 9.8%, yet the projected population (2017-2035) varies under different scenarios (Figure 1). In the middle of the road scenario (SSP2-4.5) and the regional rivalry scenario (SSP3-7.0), the population grew from 2017, increasing by 3.0% and 5.9% in 2035, respectively. In the sustainability (SSP1-2.6) and fossil fuelled development (SSP5-8.5) scenarios, the population remained steady. The percentage of elderly people (65 years or older) continued to rise in all four scenarios, especially in SSP5-8.5 and SSP2-4.5, where it was projected to increase by 190% and 120% from 2017-2035, respectively. In SSP1-2.6 and SSP3-7.0, the percentage of elderly people increased 110% and 90%, respectively. The population-weighted PM\\(_{2.5}\\) concentration in China increased by 46.6% from 2000 to 2017, while 2010 was a turning point; we only observed an increase of 0.42 ug/m\\(^3\\) between 2010 and 2017 (Figure 1). The estimated trends of the population-weighted PM\\(_{2.5}\\) concentration revealed difference between the four scenarios (Figure 1). Specifically, only SSP3-7.0 saw an increase, with the population-weighted PM\\(_{2.5}\\) concentration in China reaching 43.33 ug/m\\(^3\\) by 2035. In the other three scenarios, the population-weighted PM\\(_{2.5}\\) concentration was projected to decrease (2017-2035), with SSP1-2.6 experiencing the greatest decrease of 50.0%, followed by SSP2-4.5 (39.1%) and SSP5-8.5 (30.7%).\n\nMost age-standardized death rates of diseases in different scenarios demonstrated a downward trend (Figure 1). With the joint effects of socioeconomic development and improvement in health care, most death rates of diseases saw a distinct decrease, especially in the sustainability scenario\n(SSP1-2.6) and the fossil fuel development scenario (SSP5-8.5). For instance, in the SSP1-2.6 scenario, the age-standardized death rates of COPD, LRIs and stroke (2017-2035) decreased by 42.7%, 17.6% and 53.8%, respectively.\n\n![Line graphs showing trends for total population, population-weighted PM_{2.5} concentrations, proportion of elderly people over 65 years old, COPD mortality, DM2 mortality, IHD mortality, LC mortality, LRI mortality, and stroke mortality from 2000 to 2035 under different scenarios.](page_184_370_1082_1012.png)\n\nFigure 1 2000-2035 Change Trend of Driving Factors\nNote: (d-i) Age-standardized disease mortality. COPD, DM2, IHD, LC and LRI refer to chronic obstructive pulmonary disease, type 2 diabetes, blood heart disease, lung cancer and lower respiratory tract infection, respectively. Shading indicates the 95% confidence interval.\n\n2.2 DAPP trends in China\n\nFrom 2017 to 2035, DAPP in China exhibited two contrasting trends for two stages in the four scenarios (Figure 2a). From 2017-2025, annual DAPP was projected to decline, with decreases of 132 (123-146, 95% CI) thousand (SSP1-2.6), 71 (64-81, 95% CI) thousand (SSP2-4.5), 26 (19-35, 95% CI) thousand (SSP3-7.0) and 118 (103-136, 95% CI) thousand (SSP5-8.5). Conversely, from 2025-2035, under SSP2-4.5, SSP3-7.0, and SSP5-8.5, DAPP in China was projected to grow by 37 (29-44 95% CI) thousand, 72 (62-81, 95% CI) thousand and 24 (19-33, 95% CI) thousand, respectively. DAPP in the SSP1-2.6 scenario will decline with a minor decrease of 44 (37-53, 95%\nCI) thousand.\n\nBetween 2017 and 2035, significant regional variation in DAPP occurred (Figure 2b). Taking the sustainability scenario (SSP1-2.6) as an example, the only increase (0.1%, 0%-0.13%) in DAPP was projected to occur in Northeast China, while in the six other regions DAPP declined. Central China showed the largest decrease (31%, 22.3% - 38.6%), while the eastern regions showed the smallest (8.8%, 3.2% - 10.7%, 95% CI). In addition, it is worth noting that between 2020 and 2035, except for the central and eastern regions where DAPP was projected to be higher than the national average value by 76.7% (64.2%-83.8%) and 29.1% (19.2%-37.8%).\n\nConsidering the changes in DAPP per capita in 2017-2035 (Figure 2c, 2d), Northeast China was again the only region expected to experience an increase (12.0%, 9.2-14.8%). In addition, DAPP per capita (2017-2035) in Northeast, Central and Northwest China was consistently above the national average value. By 2035, the DAPP per capita in Northeast China, Central China and Northwest China will reach 855, 679, and 634 people (per 10,000 people), respectively.\nFigure 2 Varying trends in DAPP from 2000 to 2035.\na.) Changes in the total amount of DAPP in China; b.) Changes in the total amount of DAPP among regions; c.) Changes in DAPP per capita in China; d.) Changes in DAPP per capita among regions. The value for each region in (b) and (d) is the average value of DAPP or DAPP per capita for the provinces within that region. National average represents the average of all provinces in the country.\n\nThere will be substantial spatial differences in the projected trends in DAPP in China (Figure 2). To illustrate, we describe the two most extreme scenarios—the sustainability scenario (SSP1-2.6) with the greatest decline in DAPP and the regional rivalry scenario (SSP3-7.0) with the greatest growth (See the full results in Table S1 and Figure S1). Across regions, Henan and Hebei were projected to have the largest decrease in DAPP. In the sustainability scenario (SSP1-2.6), the decrease in DAPP in each province the DAPP reduction in the two provinces is more than 4 times to the national average level in China, and under the regional rivalry scenario (SSP3-7.0) scenario is more than 14 times to the national average.\n\n2.3 Driving factors of DAPP\nOverall, population aging is the most significant factor affecting the increase in DAPP in 2017-2035 (Figure 3). Population aging is the only factor contributing to the growth of DAPP in the sustainable development (SSP1-2.6) scenario and fossil fuel development (SSP5-8.5) scenario, resulting in increases of 674 thousand and 703 thousand DAPP per annum, respectively. In the business as usual (SSP2-4.5) and regional competition (SSP3-7.0) scenarios, although population growth will also bring a small amount of DAPP growth, more than 98% of it is due to population aging. Specifically, in these two scenarios, population aging brings increases of 730 thousand (718-746, 95% CI) and 634 (608-656, 95% CI) thousand DAPP, respectively. Meanwhile, disease mortality is an important factor alleviating the growth in DAPP, and more than 70% of the reduction in DAPP is due to the reduction in disease mortality which decreased DAPP by 615 (602-636, 95% CI) thousand, 658(608-656, 95%CI) thousand, 693 (678-726, 95% CI) thousand, and 636 (611-657, 95% CI) thousand from 2017-2035 in the four scenarios, respectively.\n\nThe amount of DAPP growth caused by population aging was projected to offset the DAPP decline caused by the decrease in disease mortality in the future and lead to an increase in DAPP. Specifically, in the four scenarios, DAPP shows a decreasing trend from 2017 to 2025, which is mainly due to the decrease in disease mortality. In this period, taking the regional competition (SSP3-7.0) scenario as an example, the reduction in disease mortality resulted in a reduction in DAPP of 371(354-396, 95%CI) thousand, which effectively offset the increase in DAPP of 281(268-301, 95%CI) thousand due to population aging. From 2025 to 2035, the age structure will become the most important factor driving the growth in DAPP. The increase in the aging population has led to an increase of 353(328-376, 95% CI) thousand DAPP, an increase of 72 (57-96, 95% CI) thousand from a decade ago. The impact of disease mortality on DAPP was projected to level off. From 2025 to 2035, the reduction in disease mortality will bring a reduction of 266 (238-276, 95% CI) thousand DAPP, which is 49(29-56, 95% CI) thousand less than ten years ago. Therefore, the impact of age structure on DAPP will begin to exceed the impact of disease mortality on DAPP and become the main reason for the increase in DAPP from 2025-2035.\nFigure 3 Contributions of different factors to DAPP changes in China from 2017 to 2035\n\nThe contributions of different drivers to DAPP showed certain differences at the provincial scale (Figure 4). For regions with higher rates of aging, such as Heilongjiang and Jilin, age structure was the most important factor affecting the change in DAPP. In these regions, the increase in DAPP attributable to population aging exceeded 50% of the national average. Affected by the aging of the population, the total DAPP in these regions continued to rise under all four scenarios, and the total increase was 2 times the national average. Taking Heilongjiang Province with the highest level of aging population as an example, in the four scenarios, the total DAPP will increase by 10,000, 6,000, 10,000 and 3,000, respectively, which will be 1.2 times, 6.7 times, 5.8 times and 1.8 times higher than the average change in the national DAPP. In Tibet, Ningxia, and Guizhou, where the proportion of elderly population is lower, the growth in DAPP caused by population aging was projected to be less than half of the average change in the national DAPP. Although the reduction in DAPP caused by factors such as the improvement of medical conditions in these regions is also lower than the average of all provinces in the country, overall, the DAPP in these regions still shows a downward trend.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
the proportion of the old (%)provincechanges of DAPP (per 10,000 people)population contributionPM2.5 concentration contributionstructure contributiondisease mortality contributionchanges of DAPP (per 10,000 people)population contributionPM2.5 concentration contributionstructure contributiondisease mortality contribution
21.98Anhui-1.27-0.24-0.892.26-2.4-0.67-0.18-0.372.47-2.59
27.01Beijing0.230.06-0.350.97-0.460.470.08-0.171.06-0.5
26.86Chongqing-0.62-0.22-0.51.74-1.63-0.41-0.02-0.31.84-1.75
22.36Fujian-0.240.04-0.350.94-0.870.020.07-0.131.03-0.95
21.92Gansu-0.490.02-0.281.54-1.54-0.360.06-0.111.51-1.32
18.33Guangdong0.650.09-1.072.57-2.850.280.08-0.342.82-3.07
19.08Guangxi-0.870.15-0.611.86-2.26-0.430.27-0.272.02-2.44
17.48Guzhou-0.80.13-0.530.94-1.35-0.450.22-0.261.04-1.45
20.31Hainan0.050.030.010.23-0.220.10.050.030.25-0.23
22.19Hebei-2.560.09-1.623.42-4.44-1.730.21-0.853.72-4.81
31.6Heilongjiang0.1-0.3-0.743.11-1.970.57-0.31-0.343.32-2.1
20.35Henan-3.230.04-2.044.48-5.71-2.060.22-0.994.89-6.2
25.94Hunan-1-0.19-1.363.91-3.37-0.29-0.11-0.754.21-3.65
24.22Inner Mongolia-1.82-0.28-1.634.45-4.39-1.03-0.14-0.934.79-4.74
28.83Mongolia0.03-0.040.19-1.19-1.090.02-0.07-1.511.16-1.68
27.96Jiangsu0.460.151.52-5.52-3.541.480.01-0.835.26-3.85
19.38Jiangxi-0.91-0.02-0.671.53-1.76-0.460.05-0.281.68-1.91
32.28Jilin0.17-0.21-0.581.98-1.030.59-0.16-0.292.16-1.12
32.33Liaoning-0.26-0.33-1.123.49-2.30.36-0.35-0.573.76-2.48
17.08Ningxia-0.150.03-0.060.11-0.22-0.10.04-0.030.12-0.24
18.65Qinghai-0.130.01-0.020.2-0.33-0.090.030.010.21-0.34
23.96Shaanxi-0.6-0.07-0.491.44-1.48-0.33-0.04-0.251.54-1.58
26.48Shandong-1.63-0.39-2.546.84-5.54-0.28-0.29-1.387.41-6.01
30.49Shanghai0.44-0.090.261.31-0.510.68-0.09-0.081.41-0.56
22.18Shanxi-0.62-0.03-0.51.16-1.26-0.310.01-0.231.77-1.35
25.1Sichuan-0.53-0.03-0.544.38-3.89-0.35-0.53-0.254.54-3.87
26.15Tianjin-0.23-0.22-0.371.08-0.720.02-0.23-0.181.17-0.78
13.77Tibet-0.09-0.010.010.04-0.13-0.06-0.010.050.04-0.14
17.55Xinjiang-0.630.16-0.221.18-1.75-0.440.25-0.111.24-1.82
18.03Yunnan-1.020.05-0.240.91-1.74-0.630.10.151.02-1.91
27.32Zhejiang10.46-0.762.58-1.281.880.55-0.292.82-1.39
23.42Average-0.58-0.04-0.732.18-1.98-0.10.01-0.332.36-2.14
\n\n(a) SSP1-2.6\n\n(b) SSP2-4.5\n\n(c) SSP3-7.0\n\n(d) SSP5-8.5\n\nChanges of DAPP: from lower to upper\n\nFigure 4 Contribution of each driver to DAPP in provinces in China from 2017-2035.\n\nIn addition, regarding types of diseases and considering all age groups affected by DAPP, the older individuals (65 years or older) are still the most vulnerable group to DAPP (Figure 5). By\n2035, in any scenario, the average proportion of older people dying from six diseases (i.e., chronic obstructive pulmonary disease, lung cancer, lower respiratory infection, ischemic heart disease, stroke and diabetes mellitus type 2) will account for more than 80% of the total DAPP. Specifically, the percentage of these individuals with chronic obstructive pulmonary disease and lower respiratory infection will be larger than 95% and 94%, respectively. Furthermore, the percentage of DAPP in older individuals for all six diseases will rise steadily from 2017 to 2035. Among them, the percentage attributable to lung cancer will increase the most, growing from 66% in 2017 to 81% in 2035 under SSP1-2.6, or showing an average increase of 23% in the four scenarios. For ischemic heart disease and diabetes mellitus type 2, the increase in the percentage will exceed 20%.\n\n![Line graphs showing the proportion of deaths among the elderly population by disease from 2000 to 2035 for COPD, DM2, IHD, LC, LRI, and stroke](page_184_670_1082_496.png)\n\nFigure 5 The proportion of deaths among the elderly population by disease from 2000 to 2035\nNote: COPD, DM2, IHD, LC, and LRI refer to chronic obstructive pulmonary disease, type 2 diabetes, ischemic heart disease, lung cancer, and lower respiratory tract infection, respectively. Shading indicates the 95% confidence interval.\n\n3. Discussion\n\n3.1 Population aging is the most important challenge in controlling DAPP\n\nPopulation aging is the leading challenge China faces in dealing with the problem of DAPP in the future. Our study found that population aging will be the primary factor driving an increase in DAPP from 2017-2035 (Figure 6). First, although the proportion of the elderly population is relatively small, the elderly will account for a large fraction of total DAPP. Between 2017 and 2035, while the proportion of elderly people will range from 10% to 35% in most regions, more than 70%(e.g., 95% in Northeast China) of the growth of DAPP will be caused by population aging.\nThese estimates are also in line with previous studies. For example, Bu et al\\(^{25}\\) found that the elderly have been affected disproportionately affected by DAPP from 1990-2017 on a global scale, and Wang et al\\(^{26}\\) attributed DAPP growth in China by 2020 and 2030 largely to population aging. Second, population aging will be the only driver of the increase in DAPP for most scenarios, except for the regional rivalry scenario (SSP3-7.5), in which population growth and air pollution will also contribute (approximately 2% only) to the increase in DAPP. In addition, although improvements in air quality and health care can decrease DAPP, DAPP was projected to grow in Northeast China which has the highest rate of population aging (Figure 9f).\n\n![Diagram showing the contribution of age structure to DAPP, with six circular diagrams labeled (a)-(f), each representing different factors such as the proportion of elderly individuals, age structure contribution, increase in DAPP contributed by other factors, total increase in DAPP, total reduction in DAPP, and total changes in DAPP.](page_340_682_1067_1012.png)\n\nFigure 6 Contribution of age structure to DAPP\nNotes: (a) Proportion of the elderly population in each region of China in 2017; (b) Change in DAPP due to population aging (per thousand people); (c) Increase in DAPP due to population growth and air pollution (per thousand people) from 2017 to 2035; (d) Total increase in DAPP due to population growth, population aging, and air pollution (per 1,000 people), 2017-2035; (e) Total reduction in DAPP due to improved air quality and decreased disease mortality (per 1,000 people), 2017-2035; (f) Net change in DAPP (per 1,000 people), 2017-2035\n\nIn addition, combined with the results of this study and previous studies, the DAPP-related challenges posed by population aging are mainly demonstrated in the following two aspects. First, the adverse impact of air pollution on people’s health will be enhanced with age. Since humans experience weakening physiological and metabolic processes when getting older8 and people are exposed to poisonous substances in ambient conditions that are absorbed by and then accumulate in the human body27, older people are the most vulnerable to air pollution. Our findings show that by 2035, the average proportion of elderly people dying of diabetes mellitus type 2 and ischemic heart disease will account for over 80% of the respective total deaths of all ages. In addition, among six diseases related to DAPP, the proportions of deaths of older people will consistently increase, and three types of diseases (e.g., lung cancer) will increase by over 20%. Third, with the fast-growing aging population in China, it is projected28 that by 2022, China will enter a stage where the aging population will account for more than 14% of the total population. By 2035, the proportion of those individuals who are 65 years old will account for 20% of the total population, further intensifying the situation. The aging speed in China has exceeded that in most developed countries29. As population aging continues, DAPP is likely to subsequently increase30.\n\nIn addition to directly causing the growth of DAPP, the aging of the population may also cause the increase of DAPP through the intermediating effect, by affecting the proportion of fossil energy consumption and the proportion of household medical and health expenditures. To this end, referring to existing studies, we used the KAYA model to verify the mediating effect of population aging on DAPP via energy consumptions and health expenditures (see Supplementary Texts 1 and Table S2 for details). The findings also confirm that population aging can negatively impact health by affecting fossil energy consumption and exacerbating air pollution. This is partly due to the fact that the elderly prefer indoor activities and/or heating in winter31,32, and partly the aging population may inhibit technological innovation33. In addition, the aging of the population will also increase the proportion of medical and health expenditure in the total household consumption by affecting the increase in DAPP. This means that the aging of the population will increase the pressure on household consumption, which is not conducive to the prevention and control of DAPP. This is also consistent with the results of existing studies7,34.\n\nHence, to alleviate the health burden caused by air pollution and decrease health risks, apart from improving air quality, China should pay special attention to older people who are directly exposed to air pollution. First, formulating plans for promoting public health awareness is suggested. This will encourage elderly individuals to conduct indoor activities during adverse weather conditions, thus reducing direct exposure to polluted air. For example, the U.S.A. and European\nUnion countries have implemented public health awareness plans\\(^8\\) to provide information on air pollution for elderly individuals, encouraging them to reduce their activities in highly contaminated conditions. Second, the government should improve health care by supporting additional investments in health care and adopting targeted measures to improve older people’s health care insurance and alleviate their economic burden. Other policies, such as providing people residing in polluted areas with medical compensation, incorporating medicines targeted at compulsory diseases into medical insurance and reducing the medical cost of treating air pollution-related diseases, are suggested as well. Studies\\(^{27}\\) have shown that assisting older people suffering from lung cancer and ischemic heart disease with economic support is effective in relieving the adverse health impacts of air pollution.\n\n3.2 International insight on DAPP Prevention and Control in different regions of China\n\nWith a rapidly aging society and room left to improve air quality and health care in Central, West and Northeast China, DAPP prevention and control in these regions is facing great challenges. Specifically, in Central and West China, in addition to the continuous increase in the proportion of the elderly population will hinder the prevention and control of DAPP, inferior medical treatment and environmental quality contribute a great deal. Zhang et al discussed the weak regulations on public health and environmental quality due to poor regional economic development\\(^{35}\\). Therefore, compared to the eastern regions, air pollution in poorer areas produced greater adverse effects on health. In Northeast China, population aging was the main driving factor in DAPP growth. In Heilongjiang and Jilin, the amount of DAPP caused by population aging equaled nearly twice the average amount among provinces. Confronted with high rates of population aging, even the improvement of health care and environmental quality could not reverse the DAPP trend, thus causing DAPP to grow consistently\\(^{10}\\). Although Central and Northeast China are faced with great challenges regarding DAPP prevention and control, Eastern, Southeast and Southwestern China have had some successes in this regard. The way of air pollution prevents and control and the equipped health care system in the area have set an imitable example for other regions. Kamal et al\\(^{19}\\) pointed out that the Air Pollution Prevention and Control Action Plan issued by the Chinese government makes it possible to contain PM\\(_{2.5}\\) pollution in certain cities, such as Shanghai and Guangzhou. Through the subsequent implementation of the plan, it is projected that by 2030, 280,000 premature deaths could be prevented. In terms of other socioeconomic aspects, Jiao et al\\(^{36}\\) found that in cities with better education and medical resources, such as Beijing and Shanghai, residents have better health awareness and public health insurance, thus offsetting the adverse effect caused by air pollution to some degree.\n\nThe future trends in DAPP in different regions of China are informative for other countries and regions (Table 1). First, air pollution poses the biggest threat to health in less economically developed regions such as Central and West China. In the assessment of air pollution and health\nfrom the WHO\\(^{37}\\) report, nearly 90% of air pollution-related deaths occurred in low-income and middle-income countries (e.g., South Asian and Western Pacific countries). Confined due to limitations in technology levels, most developing countries have substantial air pollution\\(^{38}\\). Therefore, these countries should draw lessons from developed countries in terms of adjusting their industrial structure and exploiting green energy to reduce air pollution, as well as improving health care levels.\n\nSecond, for countries and regions that have achieved preliminary economic development and improvement in air quality and health care (e.g., Northeast China), the threat of population aging was the main culprit for the increase in DAPP. Therefore, on the premise of establishing a complete system of health care, these countries and regions should pay special attention to providing medical help and perfecting basic pension plans for vulnerable people such as elderly individuals. For instance, Beard et al\\(^{31}\\) suggested that countries and regions should establish long-term nursing systems to fulfill the requirements of older people in all aspects of health care. In addition, governments should provide health services in regions adjacent to older people's residences, especially those live in polluted areas, guarantee their accessibility to vaccines and other medical products, and conduct targeted training for professional nursing personnel. Lloyd-Sherlock et al\\(^{32}\\) specifically focused on sub-Saharan African countries, identifying local governments that adopted measures to improve the health care of older people in the face of population aging.\n\nThird, for regions and countries with high-level economic development (a region such as East China), due to improvements in air quality and health care facilities, the decrease in DAPP brought by lowering the death rates of diseases and improving air quality can effectively offset the increase in DAPP led by population aging. For countries and regions such as the U.S.A.\\(^{39}\\) and the European Union\\(^{40,41}\\), continuously optimizing the health care system and further improving air quality are effective for controlling DAPP. In addition, conducting regional collaboration is encouraged to jointly address air pollution, develop a green economy and reduce health risks. For example, European countries have developed emissions reduction technology and encourage green business to reduce industrial pollution, thus reducing health risks\\(^{40}\\). In the case of China, Wu et al\\(^{42}\\) also pointed out that regions such as the Yangtze River Delta (Shanghai, Jiangsu and Zhejiang) should collaborate frequently to tackle air pollution, thus maximizing the benefits. Ji et al\\(^{43}\\) also pointed out that creating more green space can help prolong life and cope with China's aging society.\nTable 1. Health risks of air pollution in countries with varied incomes.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Income LevelsWorldChina
CountryPercentage of elderly individuals (65 years or more) (%)Death rate attributable to air pollution (per thousand)RegionsPercentage of elderly individuals (65 years or more) (%)Death rate attributable to air pollution (per thousand)
High incomeU.S., Japan, etc.22.574.5East, South22.258.8
Upper-middle incomeBrazil, Russia, etc.12.694.6North,28.474
Lower-middle and low incomeBangladesh, Pakistan, etc.4.8129Northeast,21.790.6
Central,
Northwest
\n\nGlobal population data and classifications by income levels were derived from publicly available World Bank information. Death rate data were accessed from Cohen et al\\(^5\\). The Chinese classifications by income levels are based on income rankings of China.\n\nIn summary, with the aging population increasing globally, the prevention and control of DAPP has become a common challenge faced by all countries worldwide. From 2000-2016, the proportion of people 60 years or older grew by 50%\\(^7\\). The growing proportion of older people is likely to add additional health costs brought by air pollution, making it more difficult to control DAPP and to achieve the Sustainable Development Goals (SDGs) over time. Therefore, it requires mutual cooperation and long-term continuous efforts among countries around the world to take actions to improve air quality, reduce the exposure of elderly individuals to air pollution, and improve health care for older people. On the one hand, immediate action is needed to improve air quality, adhere to a sustainable development path, and avoid the patterns of regional competition and burning of fossil fuels. This requires countries around the world to make efforts to reduce pollutant emissions from the source. At the same time, considering the fluidity of air pollution, cooperation in air pollution control will help all countries around the world jointly improve environmental quality, reducing the health risks from air pollution. On the other hand, attention needs to be paid to the health of the aging population. It is necessary to increase medical and health investment for the elderly population and to take more targeted measures to prevent elderly individuals from being exposed to air pollution and to take necessary measures to adjust the population structure to manage the aging of the population.\n\n4 Conclusions\n\nFrom 2017 to 2025, the trend in DAPP in China is estimated to decline by 19 -146 thousand (95% CI) in all four scenarios. From 2025-2035, the DAPP will begin to increase by 19-81 thousand (95% CI) in the three scenarios except the sustainable development scenario (SSP1-2.6), in which\nthe DAPP will decrease by 44 thousand (37-53, 95% CI). The changes in DAPP among the provinces of China will exhibit substantial differences. Taking the sustainable development (SSP1-2.6) scenario as an example, from 2017 to 2035, East China will be the region with the least reduction in DAPP, while Central China will be the region with the largest reduction in DAPP, 231(211-253, 95% CI) thousand, nearly 7 times more than East China.\n\nOverall, from 2017 to 2035, population aging will be the most important driver of DAPP growth. In the sustainable development (SSP1-2.6) and fossil fuel development (SSP5-8.5) scenarios, population aging is the only factor leading to DAPP growth in 2017-2035, resulting in increases of 718-746 (95% CI) thousand and 608-656 (95% CI) thousand DAPP, respectively. In the business as usual (SSP2-4.5) and regional competition (SSP3-7.0) scenarios, more than 98% (95% CI) of DAPP growth is due to population aging.\n\nIn the future, with the fast growth of global aging, the prevention and control of DAPP will require more effort from all countries to achieve the United Nations' Sustainable Development Goals. On the one hand, it is necessary to pay attention to the health problems caused by population aging, increase medical and health investment for the elderly population, separate heavy industry from where people (especially the elderly) live and take more targeted measures to avoid the exposure of the elderly population to air pollution. In addition, immediate action is needed to improve air quality, adhere to a sustainable development path, and avoid scenarios involving regional competition and the burning of fossil fuels. All these require mutual cooperation and the long-term efforts of all countries around the world.\nMaterials and methods\n\nStudy area\n\nThis paper focuses on the change in and driving factors of DAPP in China at the provincial scale. The GBD study showed that PM_{2.5} pollution caused 4.2 million deaths worldwide in 2015, of which China was the country with the largest number of deaths, reaching 1.11 million (IHME and HEI, 2017). In addition, China is the country with the largest elderly population in the world (United Nations, 2017). By the end of 2017, the population aged over 60 years in China was 240 million, accounting for 25% of the world's elderly population.\n\nThis study assessed 31 provinces, autonomous regions, and municipalities, with Hong Kong, Macau and Taiwan excluded due to data limitations. The 31 provinces were aggregated into North, Northeast, East, Central, South, Southwest, and Northwest regions (Appendix Figure S2). From 2000 to 2017, the population-weighted PM_{2.5} concentration and population aging in China showed an upward trend. The average population-weighted atmospheric PM_{2.5} concentration in China increased from 28.1 ug/cm^3 to 41.1 ug/cm^3, an increase of 46.3% (Global PM_{2.5} Assessment Dataset).\n\nData\n\nThe data used in this study includes pollutant concentration data, disease mortality data, historical socioeconomic data, air pollutant composition data, future socioeconomic data, and other geographic data (Table 2).\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
DataResource
Historical data (2000-2017)Concentration of PM_{2.5} on surface (spatial resolution 0.1°)
disease mortality data (provincial scale)
Socioeconomic data: population, GDP per capita, proportion of secondary industry, educational level, fertility rate (provincial scale)
Global PM_{2.5} Assessment Dataset44
Yin et al10
\"China Statistical Yearbook\"45
Components of PM_{2.5} data: sea salt, sulfate, organic aerosol, black carbon (spatial resolution 1°)CMIP6 dataset46
Future data (2017-2035)Socioeconomic Data: Population DataJiang et al47
Chen et al48
Geographic assistance dataProvincial administrative boundary data1:1 million data released by the National Bureau of Surveying, Mapping and Geographic Information
\nFuture PM_{2.5} composition data came from the CMIP6 dataset. Specifically, the data are based on the emissions, climate and meteorological specification under each scenario in the ScenarioMIP framework and are logically consistent with socioeconomic factors in the SSPs^{46}. We used the average of the simulation results of multiple models for each scenario^{49}.\n\nFuture socioeconomic data include data on China’s population age structure and population education level at the provincial scale^{48} and data on the total population at 0.5° grid cell resolution^{47}. Based on the latest provincial and prefecture-level city statistical yearbook data and population data in the RCP pathways, the dataset from Chen et al^{29} constructs the future population of China's provinces in five shared socioeconomic pathways from 2010 to 2100 for the first time and depicts the different developments of future economic and social systems. The data reflects the internally consistent relationships and logic of socio-economic development and climate change at the provincial scale. With 2010 as the base year, Jiang et al^{47} accumulated data on key elements such as fertility, mortality, and migration rates and estimated the annual population out to 2100 under each SSP.\n\n*Estimate and validate the spatiotemporal pattern of DAPP in China from 2005 to 2017*\n\nFirst, we used the comparable risk assessment framework^{24} to calculate DAPP^{50} as a function of the population attributable fraction (PAF), population, disease mortality and age structure^{37,51}:\n\n\\[\nDAPP = \\sum_{a,d}(PAF_{a,d} \\times POP \\times Rate_{a,d} \\times AgePa)\n\\] (1)\n\nwhere PAF_{a,d} refers to the attributable fraction of disease d in the population of age a, POP refers to the population, Rate_{a,d} refers to the mortality rate of disease d in the people of age a, and AgePa refers to the proportion of the population of age a in the total population. Among them, age a includes 15 stages: 25-30, 30-35, ..., 90-95, and >95 years old. Disease d includes 6 categories: chronic obstructive pulmonary disease, infectious lower respiratory tract infection, lung cancer, ischemic heart disease, stroke and type 2 diabetes^{37}. In addition, PAF_{a,d} is determined by the relative risk \\( RR_{a,d} \\) of death due to disease d in age group a^{37}. Specifically, it can be expressed as^{5},\n\n\\[\nPAF_{a,d} = \\frac{RR_{a,d}-1}{RR_{a,d}}\n\\] (2)\n\nwhen the PM_{2.5} exposure level is higher, the \\( RR_{a,d} \\) will be higher^{24,52}. The quantitative relationship between them can be obtained from the exposure-response function. The exposure-response function used in this study comes from the MR-BRT model recently announced in GBD2019^{24}, and the DAPP estimated based on the median value of the MR-BRT model as the primary result^{24}.\n\nWe used Pearson's correlation to verify the reliability of the results (Appendix Figure S3). Specifically, we compared the results obtained in Equation (1) with the estimates calculated by Yue et al^{22} based on the Integrated Exposure Response (IER) model, the estimates calculated by Geng et al^{14} based on the Global Exposure Mortality Model (GEMM), and the estimates calculated Yin et\nEstimate DAPP in China from 2017 to 2035\n\nWe calculated future the PM_{2.5} concentration in China based on empirical formulas and future pollutant concentration data. We used the GBD model to estimate future disease mortality in China and quantified DAPP based on a comparable risk assessment framework.\n\nSpecifically, referring to the study of Chowdhury et al^{53} and Van Donkelaar et al^{54}, we used the empirical formula to estimate PM_{2.5} concentration:\n\n\\[\n\\text{PM}_{2.5} = \\text{BC} + \\text{OA} + SO_4 + NH_4 + 0.25 \\times SS + 0.1 \\times dust\n\\] (3)\n\n\\[\nNH_4 = \\frac{(36 \\times SO_4)}{96}\n\\] (4)\n\nwhere BC represents black carbon, OA represents organic aerosol, and SS represents sea salt. Since the CMIP6 does not report the concentration of surface NH_4, we assumed that NH_4 exists only in the form of ammonium sulfate, and the concentration of NH_4 was estimated from the concentration of SO_4.\n\nSince the PM_{2.5} concentration obtained from the simulation is lower than the actual monitoring results, we calibrated the PM_{2.5} concentration calculated by the model and the observation results of the baseline period (2012-2017) as follows:\n\n\\[\nPM_{2.5,pentad=x}^{mod} = PM_{2.5,sat,pentad=bl} + PM_{2.5,sat,pentad=bl} \\times \\frac{PM_{2.5,model,pentad=x} - PM_{2.5,model,pentad=bl}}{PM_{2.5,model,pentad=bl}}\n\\] (5)\n\nwhere \\( PM_{2.5,sat,pentad=bl} \\) represents the PM_{2.5} concentration during the baseline period (2012-2017), \\( PM_{2.5,model,pentad=x} \\) represents the PM_{2.5} concentration obtained according to equation 5, and \\( PM_{2.5,model,pentad=bl} \\) represents the PM_{2.5} concentration during the baseline period obtained from equation 5,.\n\nIn addition, for future disease mortality, we used the GBD development prediction model to estimate it according to the study by Foreman et al^{55}. According to the model, the following relationship is satisfied between disease mortality and its drivers:\n\n\\[\nln(m) \\sim N(\\hat{y} + \\hat{\\epsilon}, \\sigma)\n\\] (6)\n\nwhere m represents the mortality rate of a specific disease, whose value is mainly determined by \\( \\hat{y} \\) (representing variables such as long-term trends, socioeconomic development, and risk factors) and \\( \\hat{\\epsilon} \\) (representing residuals that cannot be explained by the above factors).\n\n\\[\n\\hat{y} = \\beta_1 SDI_{<0.8} + \\beta_2 SDI_{\\geq0.8} + \\theta_a t + \\alpha_{la}\n\\] (7)\n\n\\[\n\\hat{\\epsilon} = ARIMA\\left( \\epsilon_{history} \\right)\n\\] (8)\n\nwhere \\( \\beta 0 \\) and \\( \\beta 1 \\) represent the global coefficients when the sociodemographic index (SDI) is less\nthan 0.8 and greater than 0.8, respectively. \\( \\theta_a \\) represents the long-term trend for a specific age group, and t represents time. \\( \\alpha_{1a} \\) refers to the intercept for a specific age in a specific region. \\( \\epsilon^* \\) can be calculated by the autoregressive integrated moving average function.\n\nFinally, based on the estimated results of PM\\(_{2.5}\\) concentration and disease mortality as well as the population and age structure data, we quantified the DAPP from 2018 to 2035 with the comparable risk assessment framework model of Formula (1). In addition, the upper and lower bounds of the confidence interval for DAPP in this study were determined by the upper and lower bounds of the exposure response function and the upper and lower bounds of confidence intervals for PM\\(_{2.5}\\) concentration and disease mortality. Among them, the upper and lower limits of the 95% confidence interval range of the exposure-response function are the 2.5% and 97.5% quantiles of each result in the 1000th curve fit of the meta-regression—the Bayesian, regularized, trimmed (MR-BRT) model\\(^{24}\\). The confidence interval of the PM\\(_{2.5}\\) concentration was determined by the difference of 11 models in the CMIP6 dataset\\(^{53}\\). This study assumed that the simulation results of each model conformed to the t-distribution\\(^{46}\\), and the 95% confidence interval of the PM\\(_{2.5}\\) concentration can be expressed as:\n\n\\[\nC_{CI} = Con_{mean} \\pm \\sqrt{Var(C)} * T_{95\\%}(n-1)\n\\]\n\nwhere \\( C_{CI} \\) represents the uncertainty interval of the PM\\(_{2.5}\\) concentration, \\( Con_{mean} \\) refers to the mean value of the PM\\(_{2.5}\\) concentration obtained by multiple models, and \\( Var(C) \\) refers to the variance in the PM\\(_{2.5}\\) concentration obtained from multiple models. \\( T_{95\\%(n-1)} \\) represents the t-statistic with n-1 degrees of freedom under the 95% confidence interval, where n is the number of correlated modes.\n\nDisease mortality is determined by \\( \\epsilon \\) in the linear model Formula (8)\\(^{55}\\), \\( \\epsilon \\) represents the residual between the estimated value and the actual value, obeying the mean of 0, and the variance of \\( Var(e_0) \\) is normally distributed. Therefore, the 95% confidence interval for ln(m) can be expressed as:\n\n\\[\n\\ln(m)_{CI} = \\hat{y} + \\hat{\\epsilon} \\pm \\sqrt{Var(\\epsilon - \\hat{\\epsilon})} * T_{95\\%}(n-2)\n\\]\n\nwhere \\( \\ln(m)_{CI} \\) represents the uncertainty interval for the natural logarithm of mortality from a specific type and age group of diseases, the sum of y* and \\( \\epsilon^* \\) represents the predicted value of \\( \\ln(m) \\), and \\( Var(\\epsilon - \\hat{\\epsilon}) \\) refers to the variance of the residual term in the regression model (Equation 3.10). \\( T_{95\\%(n-2)} \\) represents the t-statistic with n-2 degrees of freedom under the 95% confidence interval, where n is the sample size for constructing the regression model. \\( Var(\\epsilon - \\hat{\\epsilon}) \\) can be further obtained by the following formula.\n\n\\[\nVar(\\epsilon - \\hat{\\epsilon}) = \\frac{\\sum e_i^2}{n-2} \\times \\left[ \\frac{1}{n} \\times \\frac{(x_f-\\bar{x})^2}{(x_i-\\bar{x})^2} \\right]\n\\]\n\nwhere \\( \\sum e_i^2 \\) is the residual sum of squares of the regression model, \\( x_i \\) and \\( \\bar{x} \\) represent the mean of each independent variable and independent variable in the regression model, respectively, and \\( x_f \\) represents the input value of the independent variable when predicting the future based on the regression model.\n\nWe further compared the DAPP calculated in this paper of historical periods with previous\nstudies to verify the rationality of the quantitative method. We found that previous studies\\(^{10,14,22}\\) showed similar results to ours. Although some estimates based on the GEMM model were higher than our estimates\\(^{14}\\), the results showed a similar trend over time. This is because the RR estimated by GEMM model are higher compared to the RR values obtained by the IER function, especially in areas with high PM\\(_{2.5}\\) concentrations\\(^{7}\\). Also, we compared the results estimated under different future scenarios with the results estimated by GBDMAPS (Table S3). Different from the four scenarios in this study, the results in GBDMAPS was mainly based on different emission pathways under different energy utilization and air pollution control policies. Consistent with our findings, DAPP were lower under the sustainable development paths with policy interventions (such as the BAU2 and PC2 scenarios in GBDMAPS China and the SSP1-2.6 scenarios in this study). However, since we only considered outdoor air pollution when quantifying DAPP, ignoring indoor pollution and its interaction with outdoor air pollution, the amount of DAPP in this study is lower than the results of GBDMAPS China. In addition, the disease mortality data used in GBDMAPS was simulated based on the estimated value of GBD2013. It was assumed that the change trend of disease mortality is consistent with the change trend from 1990 to 2013, and the changes in socioeconomic levels such as medical conditions across different scenarios were not taken into account. Therefore, the disease mortality in GBDMAPS China were higher than the ones in our study. This is another reason for the higher estimated DAPP estimated by GBDMAPS than our estimates.\n\n*Analyze the drivers of DAPP by the decomposition method*\n\nIn addition to being affected by the age structure of the population, DAPP is also affected by the effects of population size, PM\\(_{2.5}\\) concentration and related disease mortality. Specifically, the total population and proportion of aged population, PM\\(_{2.5}\\) concentration, and disease mortality are all positively correlated with DAPP. Based on Cohen et al\\(^{5}\\) and Yue et al\\(^{22}\\), we quantified the influence of age structure and population size, PM\\(_{2.5}\\) concentration and related disease mortality on DAPP using the decomposition method. The advantage of decomposition method is to transform the nonlinear relationship between individual drivers and DAPP changes into a simple linear relationship\\(^{5}\\). Compared with simple sensitivity analysis, decomposition method takes into account the interaction of various factors, which makes the number of DAPP correspond to the contribution of driving factors. The net change of DAPP in a certain period of time can be expressed as the sum of the contributions of various driving factors to the change of DAPP, which is helpful for the quantitative analysis of the driving mechanism of DAPP. At the same time, the decomposition method converts the changes of different driving factors into contributions to the changes of DAPP, which supports the judgment of the relative importance of each factor.\n\nIn the decomposition analysis (Appendix Figure S4), we gradually introduced the\nchanges in age structure, population, PM_{2.5} concentration and disease mortality separately to calculate DAPP. The difference between the pre-introduction and post-introduction results is the contribution of age structure. In addition, considering that the order of introduction can affect the calculation results, this study calculated all 24 possible combinations of the order of the introduction and used the average of the contributions of the four drivers in each case as the final result. Based on the decomposition analysis, we calculated the driving factors of DAPP in China in 2017-2025, 2025-2030, and 2030-2035 and then analyzed the synergistic driving effect of age structure and other factors on DAPP.\n\nAcknowledgement\nWe thank Prof. Aaron J. Cohen (Health Effects Institute, Boston, USA) for his insightful comments on the manuscript. This work was supported by the National Key Research and Development Program of China (Grant No.2019YFA0607203), the National Natural Science Foundation of China (Grant No.41971270& 41621061) and National Foundation of China Scholarship Council (Grant No.201806040156).\n\nReferences\n1 Kumar, A., Yang, T. & Sharma, M. P. 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R. Ambient PM2.5 exposure and expected premature mortality to 2100 in India under climate change scenarios. Nature Communications 9, doi:10.1038/s41467-017-02755-y (2018).\n54 Van Donkelaar, A., Martin, R. V., Brauer, M. & Boys, B. L. J. E. H. P. Use of Satellite Observations for Long-Term Exposure Assessment of Global Concentrations of Fine Particulate Matter. 123 (2015).\n55 Foreman, K. J. et al. Forecasting life expectancy, years of life lost, and all-cause and cause-specific mortality for 250 causes of death: reference and alternative scenarios for 2016-40 for 195 countries and territories. Lancet 392, 2052-2090, doi:10.1016/s0140-6736(18)31694-5 (2018).\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• SupplemantraryMaterial.docx"} {"paper_id": "prb62", "title": "Demixing fluorescence time traces transmitted by multimode fibers", "text": "# Abstract\n\nFiber photometry is a significantly less invasive method compared to other deep brain imaging microendoscopy approaches due to the use of thin multimode fibers (MMF diameter < 500 µm). Nevertheless, the transmitted signals get scrambled upon propagation within the MMF, thus limiting the technique’s potential in resolving temporal readouts with cellular resolution. Here, we demonstrate how to separate the time trace signals of several fluorescent sources probed by a thin (≈ 200 µm) MMF with typical implantable length in a mouse brain. We disentangled several spatio-temporal fluorescence signals by using a general unconstrained non-negative matrix factorization (NMF) algorithm directly on the raw video data. Furthermore, we show that commercial and low-cost open-source miniscopes display enough sensitivity to image the same fluorescence patterns seen in our proof of principle experiment, suggesting that a whole new avenue for novel minimally invasive deep brain studies with multimode fibers in freely-behaving mice is possible.\n\nPhysical sciences/Optics and photonics/Optical techniques/Imaging and sensing \nPhysical sciences/Optics and photonics/Applied optics/Fibre optics and optical communications \nPhysical sciences/Optics and photonics/Optical techniques/Microscopy/Ca2+ imaging \nSpatio-temporal demixing \ntime traces \nscattering fingerprints \ntransient patterns \nshort multimode fiber \nneuronal microendoscopy \nnon-negative matrix factorization.\n\n# 1 Introduction\n\nFluorescence-based techniques are providing researchers with different ways to collect functional readouts from neuronal activity in the brain1–10. However, measuring neuronal activity at depths greater than 1 mm is still challenging mainly due to issues resulting from light scattering, especially in prominent paradigms such as freely behaving animals11–14. To address this problem, neuronal microendoscopy methods have emerged as complementary alternatives to linear and nonlinear fluorescence microscopy techniques for studying neuronal activity in deep brain regions using genetically encoded calcium indicators (GECI)13–16. Among these methods, conventional microendoscopic methods that use a single gradient index (GRIN) lens optics16–19, as well as fiber photometry recordings using multimode fiber (MMF)15,20–23, have been successfully used to obtain functional neuronal activity signals in deep brain regions in freely behaving mice15,22,24. Nonetheless, direct imaging techniques and fiber photometry approaches bring peculiar tradeoffs in terms of spatial and temporal discerning capabilities13,25,26. On one hand, albeit GRIN lens microendoscopy retrieves calcium transients with cellular resolution, it demands a somewhat invasive surgical procedure to implant the GRIN lens into the mouse brain. Commercial GRIN lenses are relatively thick (≥ 500 µm), and oftentimes it necessitates the removal of a significant amount of brain tissue to effectively conduct the experiment12,26. On the other hand, the use of thin multimode fibers (< 500 µm diameter) in photometric recordings, as well as in optogenetics experiments, has a significantly less invasive surgical procedure, which does not require any brain tissue removal, but only a careful penetration of the thin fiber through the mouse brain6,15,25. It is known that the implantation of multiple multimode fibers (up to a maximum of 48 fibers27) to optogenetically control and/or photometrically probe different regions in freely-behaving mouse brains is already a reality in neuroscience labs26–28. However, the light wavefront propagating inside multimode fiber gets spatio-temporally scrambled due to multimodal mixing (internal scattering)29–31. Generally, that is not a limitation for delivering light (optogenetics) to an ensemble of neurons in a given depth (unless one wants to probe specific neurons within the fiber field of view, FoV), but it poses a challenge for fiber photometry methods which limits the technique’s potential to resolve (demix) time traces from individual neurons. Consequently, fiber photometry time traces coming from a whole population of neurons transmitted through MMF are ensemble integrated during detection, and therefore, fast single-pixel detectors are frequently chosen to optimize the detection speed and sensitivity15,26. While the use of fast scientific Complementary Metal–Oxide–Semiconductor (sCMOS) cameras to simultaneously probe multiple fiber photometric signals has been demonstrated26,28, the mixing between all the spatial patterns transmitted by each MMF prevented the individual retrieval of each neuron time trace26.\n\nRecently, researchers have developed novel techniques that utilize the deterministic nature of the multimode fiber transmission matrix (TM) to perform bioimaging30–40. These approaches have enabled the acquisition of diffraction-limited images of fluorescently labeled brain structures and neuronal activity, even in deep brain regions (e.g., head-fixed mouse), using a multimode fiber microendoscope31. To achieve this, however, an extensive characterization of MMFs transmission properties is necessary, ideally taking into account TM changes whenever the MMF fiber is bending or changing its transmission properties during an experiment, as well discussed in previous research32,40,41. Consequently, while these techniques provide a minimally invasive method to obtain diffraction-limited resolution in deep brain regions, they are complex to implement and require a wavefront shaping device (e.g., spatial light modulator, SLM) to compensate for the fluorescence randomized wavefronts through a lengthy calibration procedure. Moreover, the calibration can be even more complex if the experiment is not performed in head-fixed mice, but in freely behaving mice, such as those in long-term social behavior studies31,32. Finally, the use of spatial light modulators and complex distal optical devices poses an extra challenge in future use in miniaturized wireless systems.\n\nIn this article, we propose a novel approach to perform minimally invasive fiber photometry experiments disentangling single-source time traces transmitted by short and thin multimode fibers (≈ 200 µm diameter and with < 10 mm length). Our method involves the demixing of fluorescence spatio-temporal signals by applying a single post-processing step on the recorded video data of 2D scattered fluorescence patterns transmitted by the fiber. By substituting the bucket detector with a camera (i.e., a pixelated detector such as CMOS sensor), we can profit from using the spatial information of the fluorescence patterns transmitted by the multimode fiber, enabling single-source temporal activity resolution. Analysis of the recorded video is performed employing a simple unconstrained Non-Negative Matrix Factorization (NMF) algorithm that separates each spatial scattering pattern component with its corresponding temporal trace (singular trace)42,43. With this approach, we show that it is possible to extract single-source time traces in fiber photometry without the need to perform any complicated calibration procedure.\n\nPrevious work from some of the authors showed that it is possible to spatio-temporally demix fluorescence scattering patterns (speckles) transmitted through a highly scattering media (e.g., mouse skull) by using a Non-Negative Matrix factorization (NMF) algorithm43,44. The NMF algorithm relies on the premise that the input data matrix only contains non-negative values, and it has been used to decompose datasets into their representative parts or components42,43,45–48. In addition, if a priori knowledge of the input dataset is known (e.g., sparsity, calcium transient profile, etc.), it is possible to improve the performance of NMF by adding some constraints49–52. Therefore, the video data of fluorescence speckles fluctuating over time are a highly appropriate input matrix for NMF, because the superposition of these intensity signals is naturally positive, linear, and sparse due to the incoherent nature of the fluorescence process (i.e., there is no destructive interference on the propagation process of incoherent light). Based on that, one could in principle apply the same algorithm to the video data from scattering patterns that are characteristic of the light transmitted through short multimode fibers of the same length as the ones implanted in fiber photometry26,53–55. It is well known that multimode fibers randomize the fluorescence wavefront propagating within it, acting as a scattering media over the fiber length due to multimodal mixing. Nevertheless, the multimode fibers (< 10 mm) typically implanted in living mice for chronic behavioral experiments are too short to generate a fully evolved speckle wavefront53,55. In fact, the light wavefront that emerges from such short fibers displays a very peculiar spatial distribution of light, which is structurally mixed, but not fully spatially randomized/sparse53,54. Hence, these scattering patterns cannot be considered yet a fully developed speckle (such as the ones in our previous work43), because they still display some continuous structures whose shape depends mostly on the multimode fiber core geometry56. Here, we call these short MMF patterns as scattering fingerprints.\n\nIn the present work, we designed a proof of principle experiment (Fig. 01) and we confirmed that a simple unconstrained NMF could also disentangle the short MMFs scattering fingerprints signals and retrieve their corresponding time traces. As a consequence, one may now temporally resolve and count the number of sources with singular time traces transmitted by a minimally invasive multimode fiber. Thus, the results of this paper consist of a proof of concept on how to obtain individual time trace resolution in fiber photometry methods. Besides, we validated our approach in a more realistic condition by selectively exciting a few structurally Gad-eGFP labeled neurons in a 50 µm fixed brain slice with literature-available time traces to mimic neuronal activity. Finally, we propose a novel method for probing neuronal microendoscopic signals by simply combining a miniscope and an implantable short multimode fiber, which we called MiniDART (for Miniaturized Deep Activity Recording with high Throughput). For that, we demonstrate that the inexpensive and commercially available open-source miniscope (Open Ephys Miniscope-v4.4) has already enough sensitivity and illumination power to detect the typical intricated patterns of short MMFs. This new way of measuring individual fluorescence time traces from an ensemble of fluctuating sources profits from the short length of multimode fibers that are naturally more rigid (bending resistant) and therefore very suitable to be used in long-term freely-moving mice neuroscience experiments.\n\n# 2 Results\n\n## 2.1 Proof of principle using phantom samples made of 10 µm diameter fluorescent beads\n\nTo demonstrate the validity of the method, we implemented an optical setup using a digital micromirror device (DMD), which was used to generate different excitation ground truth (GT) activity traces for each fluorescent source (10 µm fluorescent beads ≈ neuron soma size). Each source emits fluorescence that is collected and transmitted by the multimode fiber (see Fig. 01 and methods for details). Upon propagating through the MMF, the fluorescence wavefront undergoes scrambling, resulting in the emergence of fluorescence patterns upon exiting the fiber. The controlled excitation guarantees that each fluorescent source generates a fingerprint pattern whose intensity transiently fluctuates accordingly with the chosen GT time trace profile (see transient patterns in Fig. 01). Thereafter, we record a video of the transient patterns that emerge from a short multimode fiber and apply the NMF to the recorded data. In Fig. 02 we show the results retrieved by NMF and compared with the ground truth. The results consist of individual spatial fingerprint patterns (Fig. 02 e) and, most importantly, their corresponding single-activity time traces (Fig. 02 f) that without NMF would be mixed.\n\nAs can be seen in Fig. 02 a, the scattering patterns transmitted by the short MMF of 6 fluorescent bead sources (Fig. 02 c) have a significant overlap in space when all of the sources are simultaneously excited with the DMD (Fig. 02 a). On the other hand, whenever a fluorescent bead is excited individually, each detected spatial pattern has a very different spatial structure/morphology (see the GT scattering fingerprints in Fig. 02 d). After applying the unconstrained NMF on the recorded video data, the demixed spatio-temporal result by NMF had an overall good agreement with the GT. Not only the NMF retrieved well each singular temporal activity trace (Fig. 02 f-g), but also the individual spatial fingerprint patterns (Fig. 02 d-e). Since we know the GT activity, we sorted and assigned the source indexes in descending order of the correlation between their time trace obtained by the NMF and the GT. As we can see in Fig. 02 g, the GT-NMF temporal correlation coefficient values were high for all the first 5 beads, which were localized closer to the central region of the fiber (Fig. 02 c). More specifically, we obtained an average value of < δg,n > = δavg = 85.4% with a standard deviation of std = 3.6% (Fig. 02 g). However, the NMF algorithm could not reliably recover the time trace and fluorescence patterns corresponding to bead #6 due to low SNR, probably because it was localized too far from the center, i.e. at the edge of the field of view (fiber core border, see Fig. 02 c), as suggested by the low intensity of GT scattering pattern (Fig. 02 d, index 6). In the analysis process, the input rank of NMF determines the number of components the algorithm demixes the spatio-temporal signal. When we choose an NMF’s rank value higher than the real number of fluorescence sources, we obtain replicas of the scattering fingerprints and the background (see supp info), similar to what happened in a previous work48. Thus, counting the maximum number of unique patterns demixed by NMF could be a way to count the real number of sources probed by the fiber. A more technical analysis of it can be found in the supp info.\n\n## 2.2 Validation of the method while probing GFP-labelled neurons in a 50 µm thick fixed brain slice\n\nWe showed that our method works for a sample of fluorescent beads mimicking neuronal size and activity, however, a real GFP-labeled brain would display higher background and the labeled neurons would have a lower fluorescence signal43. Therefore, in a second set of experiments, we changed our fluorescent sample to a 50 µm fixed brain slice (structurally Gad-eGFP labeled neurons, see methods for more details), and carried out the same type of GT excitation on a few selected neurons in the fiber FoV (mimicking more realistically the neuronal activity in a living brain. After recording a video of the scattering transient patterns and applying the unconstrained NMF, we confirmed again (see Fig. 03) a good retrieval of the number of neurons, their scattering fingerprints (Fig. 03 d-e), and their individual activity traces (see Fig. 03 f-g and supp info). As in the previous experiment, the GT-NMF temporal trace correlation values obtained were high, with an average value of < δg,n > = δavg = 86.7%, and a standard deviation of std = 2.8%.\n\n## 2.3 Sensitivity of low-cost miniscopes in probing individual short MMF scattering fingerprints\n\nFinally, we investigated if an inexpensive miniscope (Open Ephys Miniscope-v.4.4) would have enough sensitivity to excite and image an individual fluorescence fingerprint pattern emitted from a single fluorescent source (Fig. 04 a). In other words, both the LED excitation from the miniscope and the fluorescence signal from the sample would be transmitted within the short MMF before imaging. This is an important question because the miniscope has simple, inexpensive, and compact components, such as the commercial-grade CMOS detector, rather than a high-end sCMOS camera as in our proof of principle tabletop experiment (see methods). To tackle this question, we combined a miniscope with a short MMF (the MiniDART) and tested the miniscope sensitivity with a very sparse bead sample: a single fluorescent bead that we can displace laterally in the fiber FoV (see methods and Fig. 04 b-c). When we set the miniscope for low LED power and with no camera gain (LED = 20% corresponds to a transmitted power through the short MMF of \\\\({P}_{MMF}\\\\) < 10 µW), it was already possible to detect short MMF scattering fingerprint patterns with very good contrast at the fastest framerate available in the miniscope control software (FPS = 30 Hz, see supp info). Interestingly, whenever raising the LED power, decreasing the framerate speed, or raising the camera gain value, the detected patterns by the miniscope got saturated, showing that the tested miniscope has already enough sensitivity to probe scattering fingerprints through short MMFs even from less bright fluorescent sources than the ones used here, especially when the fluorescent source is close to the center of the fiber core (see Fig. 04 a,d). At distances d < 20 µm from the core center, the CMOS got saturated while the miniscope GUI settings were: LED power = 20% (where LEDmax = 100%, corresponding to a transmitted power through the short MMF of \\\\({P}_{MMF}^{max}\\\\) = 125 µW), FPS = 10 Hz (where FPSmax = 30 Hz), and Gain = 1 (where Gainmax = 3.5).\n\nFundamentally, the MiniDART is not designed for imaging or localization (like in other works that used learning algorithm methods53,54). In many experiments, the relevant biological information does not depend on the shape or local position of the neurons, but mostly on the activity of each of them and their number. To extract this information, just demixing fluorescence time trace signals with NMF would be enough for relevant applications, since the number of neurons (NMF rank) could be obtained by counting the number of unique MMF fingerprints, and possibly confirmed by a post-mortem evaluation of the brain region right below the thin hole made by the MMF. In addition, recording the spatial fingerprints of each source would be useful for chronic experiments (to match the sources from one session to the next). However, as we can also see in Fig. 04, the morphology of short MMF fingerprints provides some interesting insights into the point source position at the fiber distal end - without the need for any computational learning method. As we move a single bead laterally in a radial manner (in the x,y-plane at the fiber’s distal end), a few easily interpretable geometrical properties of the fluorescence patterns systematically change in the fiber’s proximal end (Fig. 04 c-d). More specifically, when the bead is displaced from the center towards the fiber border (of a distance d) a bright ring (of diameter ρ) with some spiral ramifications is deterministically formed (see supp info for more details). Larger d distances yield wider rings (larger ρ, see Fig. 04 d). Thus, each fingerprint’s bright ring diameter is encoding radial information about the bead lateral localization at the distal end. The dependence of fingerprint shape features on the individual point source position is further discussed in the supplementary information.\n\n# 3 Discussion\n\nMultimode fibers are well known to be minimally invasive microendoscopic probes that could be promptly combined with optogenetics manipulation of neuronal activity for behavioral neuroscience studies in living mice15,27,28,55. It is well known from the literature that long multimode fibers (MMF length > 100 mm) could be used to transmit fluorescence activity signal and that would naturally generate a speckle wavefront due to internal multimodal mixing30,34,58,59. However, as well described in wavefront shaping experiments, speckle wavefronts are extremely sensitive to fiber bending, torsion movements, and temperature changes along the fiber, which demands a long and meticulous wavefront propagation characterization (e.g., calibration using spatial light modulators, SLM) to compensate for all the changes in spatial properties of the speckles32,41. In other words, there would be many experimental conditions to take into account to guarantee that the speckle patterns from each source would remain the same over time when using a long MMF as a photometric probe in freely-behaving mice experiments. That is using only a short and more stable multimode fiber for this type of application could be a very pragmatic solution.\n\nTo this end, we designed an experiment with known ground truth excitation to be able to evaluate if NMF could demix the individual spatio-temporal readouts characteristic of short MMFs. In this paper, we demonstrate that it is possible to demix such spatio-temporal signals. We used a simple and general unconstrained NMF algorithm on the video data recorded in our proof of principle experiment. It is the first time, to the best of our knowledge, that NMF is used to demix fluorescence fluctuating signals transmitted by a multimode fiber. In particular, the present work presents the proof of concept on how to obtain fluorescence activity readouts reaching single-source resolution in short multimode fibers. Since in our previous work, we already proved how to demix fluorescence speckles that are transmitted by highly scattering media (e.g., bone tissue43), the same principle is also readily applied for long MMF applications too. Therefore, this work opens a promising direction to improve fiber photometry fluorescence experiments by reaching single-source temporal activity resolution.\n\nTo benefit from the short MMF’s scattering fingerprint patterns and rigidity, one could directly image the proximal end of the short (implantable) MMF with a miniscope. That would be different from the typical scheme in fiber photometry, where there is an optical coupling between the transmitted light from the implantable MMF to another long MMF. In this sense, we tested and confirmed that even a low-cost miniscope would have enough LED power and CMOS speed/sensitivity to image the intricated scattering patterns transmitted by short MMFs emitted from just a single source. Both the multimode fiber and the miniscope (Open Ephys Miniscope-v4.4) are affordable and available in the market to carry out an experiment on living mice. Therefore, in this paper, we show a low-cost and simple way to expand the capacity of fiber photometry methods in resolving neuronal activity circuitry (that have already been used to investigate deep brain regions in chronic behavioral experiments in freely-behaving mice). In addition, as a minor result, we point out in Fig.04 that the short MMF scattering fingerprint morphology can have some interpretable geometry that has a relation with the source (≈ 10 µm size) localization at the distal end of the fiber. The relationship between the source localization and its fluorescence pattern shape is discussed in the supp info, but the key message for demixing is that the scattering fingerprint patterns seem to not be ambiguous depending on the source lateral position from the fiber axis.\n\nAlthough computational learning tools have already been applied on short MMF scattering fingerprints to retrieve back the ground truth structural image of deep brain regions from a fixed thick brain slice53,54, it is not yet proven that their approach could correctly assign the neuronal activity in living mice or any artificial condition. On the temporal resolution side, they tracked the movement of a fluorescently labeled worm in 2D with a framerate (2 Hz), which is relatively low for typical calcium transient imaging experiments performed in living mice. In the latter case, experiments are typically carried out with a framerate of at least 10 Hz (such as the one available in the miniscope DAQ software). Besides, any learning algorithm depends on the specific conditions of the training set (fiber properties, imaging optical components properties, etc.), which is less general and therefore less applicable to any other new neuroscience experiment.\n\nFinally, we emphasize that in our method we used a very simple and general unconstrained NMF directly on the raw data, which means that there is plenty of room for performance improvement, not only optically wise (tailoring new miniscopes for this specific application) but also on the computational analysis side. On the latter, one could add biophysical-inspired constraints on the NMF algorithm (spatio-temporal priors, such as in CNMF51,52) or simply add some extra data processing steps on the recorded data (e.g., matrix transformations, filtering, etc51). Indeed, it is already well known in the literature that CNMF is superior compared to NMF in demixing calcium trace signals in conventional GRIN lens imaging microendoscopy51,52. Regarding the miniscope potential improvements, when we spatially binned the video recorded by our high-end sCMOS camera (tabletop experiment) until we get a similar number of FoV pixels used in the miniscope, the retrieved results of NMF fingerprints and traces were visually indistinguishable (see supp info) compared to a non-binned analysis. This finding reinforces the idea that the current default design of the miniscope (LED power, camera speed/sensitivity, and FoV magnification) might be already enough to perform a living mouse experiment, although most pixels of the miniscope’s camera chip were not used in our case (less than 1/9 of the FoV pixels were used to image a single MMF proximal end tip). Nevertheless, another way to improve the technical performance would be to design new miniscopes specifically for the application of our method, such as having a smaller FoV, with faster and even more sensitive detection (e.g., having a bigger bit-depth).\n\n# 4 Conclusion\n\nIn this paper, we demonstrate how one could obtain single-source temporal activity resolution in fiber photometry experiments that use multimode fibers as a microendoscopic probe. Besides, we show that the currently available low-cost miniscope has enough sensitivity to image directly the implantable short MMF scattering fingerprints so that it could be advantageous for long-term microendoscopic studies in freely-behaving animals due to the rigidity of short fibers (< 10 mm). Therefore, we believe that this work can open a whole new avenue for novel and affordable minimally invasive deep brain microendoscopic studies to probe (potentially several) deep brain regions in freely-behaving animals, including experiments that could be conveniently coupled with optogenetics approaches like already been implemented in the neuroscience community.\n\n# 5 Methods\n\nProof of principle setup: \nThe proof of principle setup is visually illustrated and fully described in the supp info.\n\nFiber-ferrule preparation: \nThe multimode fiber was purchased from Thorlabs (FT200UMT, NA = 0.39, 200 ± 5 µm core diameter, 225 ± 5 µm cladding diameter). Around 10 cm of the fiber was initially cleaved with a ruby blade (Thorlabs, S90R), and the quality of the cleaved edge was inspected with a stereomicroscope (LEICA A60F, maximum magnification 30x). The fiber was glued within a 1.25 mm wide and 6 mm long stainless-steel ferrule (Thorlabs SFLC230-10, 230 ± 10µm bore diameter) using an ultraviolet curing glue (Norland optical adhesive 81) so that the cleaved end was chosen to be the distal end of the fiber (with 2mm of it sticking out of the ferrule). The excess of the fiber on the other end (proximal end) was cut close to the ferrule edge and then sequentially polished (KRELLTECH NOVA device) with 3 different silicon carbide polishing disks with gradually descending roughness (30 mm, 3 mm, 0.3 mm, PSA 4’’ polishing disks from KRELLTECH). The quality of the polished end (proximal end of the fiber) was verified with the LEICA A60F stereomicroscope. We used a customized titanium tweezer and baseplate to hold the ferrule and the miniscope respectively (YMETRY®).\n\nPreparation of the fluorescent bead sample: \nIn the proof of principle experiments, the samples consisted of randomly distributed fluorescent beads on borosilicate glass (22×40 mm cover glass, thickness Nb.1.5, purchased from VWR). An aliquot (100x diluted in milli-Q water) of the polystyrene (PS) particles aqueous suspension (PS - FluoGreen - Fi226–1mL, 10.23 ± 0.13 µm size, abs/em = 502/518 nm, purchase from microParticles GmbH, Germany) was used to randomly distribute the beads on the cover glass. The beads’ size was chosen to have similar size to typical neuron soma probed in calcium imaging experiments. Besides, the emission spectrum of the beads is close to the common GFP calcium indicators. For the single-bead sample, a more diluted aliquot (from 10⁶ to 10⁷ times dilution) was used to guarantee a very spatially sparse bead sample with density ≤ 1 bead/cm², so that there would be only a single bead throughout the Fiber FoV whenever translating the bead laterally in the miniDART experiment (easily inspected by the miniscope itself without the fiber).\n\nPreparation of the fixed brain slice sample: \nThe work includes data from one GAD65-EGFP transgenic mouse (heterozygote; male; aged 6 months) expressing EGFP in Gad65-positive interneurons in the brain and spinal cord. All procedures involving this animal complied with French and European legislations relative to the protection of animals used for experimental and other scientific purposes (2010/63/UE) and were approved by the “Charles Darwin” institutional ethics committee under the direction of the French National Committee of Ethical Reflection on Animal Experimentation under authorization number APAFIS 26667. The mouse was euthanized by cervical dislocation performed on the terminally anesthetized animal (5% isoflurane for 5 minutes in an induction chamber) and the brain was quickly removed from the skull and immediately transferred into a fixation solution (4% paraformaldehyde; pH 6.9 buffered; Sigma-Aldrich #1004965000). After 12 h at 5° the brain was transferred into phosphate-buffered saline (PBS) and cut into tangential slices of 50 to 100 µm thickness using a vibratome (Leica VT1000). Obtained slices were stored in multi-well plates with PBS and assessed with a fluorometric microscope before the experiment with the DMD.\n\nNMF Analysis in Python: \nThe raw video data [2D image, time] was reshaped to a 2D matrix [1D image, time] to fit the input format of NMF. We used the scikit-learn decomposition NMF package freely available online (Python)⁴⁴,⁶⁰. In the code pipeline, an optional pre-processing step was added, which included an option for pixel binning (see supp info). The NMF parameters chosen ignored the additional parametric terms that are introduced to account for the sparsity of the data. The parameters chosen were: init = ‘nndsvd’, random_state = 0, max_iter = 3000, solver = ‘cd’, l1_ratio = 1, beta_loss = 2, alpha_W = 0, alpha_H = 0. The parameter n_components (which is the chosen NMF rank) changes depending on the experiment and a more detailed discussion about how to choose this value can be found in the supp info. In particular, the rank used in Fig. 02 was rank Fig2 =9 (explained in the supp info), and the rank for Fig. 03 was rank Fig3 = 5. The results of Fig. 02 with different ranks are illustrated in the supp info.\n\nThe non-diagonal coefficients mean and standard deviation of the temporal correlation results: \nThe matrix of the non-diagonal elements ζ = ζᵢ≠ⱼ, where each element is the mean absolute error value between GT-NMF and GT-GT coefficients is detailed described in the supp info. The mean absolute error (MAE) value of a given element in ζᵢ≠ⱼ is given by: \n\n$${MAE}_{i,j}= \\left|{{\\nu }}_{i,j}-{{\\gamma }}_{i,j}\\right|$$ \n\nWhere, νᵢ,ⱼ is the (i,j) non-diagonal coefficient of GT-NMF temporal correlations, and is γᵢ,ⱼ the corresponding (i,j) non-diagonal coefficient of the GT-GT temporal correlations. The average value (ζₐᵥg) of all these non-diagonal elements and the standard deviation (σ) is given by: \n\n$${\\\\zeta }_{avg}=mean\\\\left({\\\\zeta }_{i \\\\ne j}\\\\right)=\\\\frac{1}{{2 (N}_{s}-1)}\\\\left(\\\\sum _{i\\\\ne j}^{{N}_{s}-1}\\\\left|{{\\\\nu }}_{i,j}-{{\\\\gamma }}_{i,j}\\\\right|\\\\right)$$ \n\n$${\\\\sigma }_{\\\\zeta }=std\\\\left({\\\\zeta }_{i \\\\ne j}\\\\right)$$ \n\nWhere Nₛ is the total number of sources. These two values (ζₐᵥg ± σₐᵥg), together with the diagonal values (δₐᵥg ± σₐᵥg), give us an estimation of whole experiment quality since (ζₐᵥg ± σₐᵥg) should ideally approach to zero.\n\n# References\n\n1. Akemann, W. et al. 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Two-photon quantum walk in a multimode fiber. *Sci Adv* **2**, (2016).\n\n60. sklearn.decomposition.NMF. https://scikit-learn/stable/modules/generated/sklearn.decomposition.nmf.html (2023).\n\n# Supplementary Files\n\n- [2023.05.30RimoliCVetalSupplInfoFinal.docx](https://assets-eu.researchsquare.com/files/rs-3010840/v1/5b1ad87d29dfab35025c1147.docx)"} {"paper_id": "prb63", "title": "Optical Neural Engine for Solving Scientific Partial Differential Equations", "text": "Optical Neural Engine for Solving Scientific Partial Differential Equations\n\nWeilu Gao\nweilu.gao@utah.edu\n\nThe University of Utah https://orcid.org/0000-0003-3139-034X\nYingheng Tang\nLawrence Berkeley National Laboratory\nRuiyang Chen\nThe University of Utah https://orcid.org/0000-0002-1538-1702\nMinhan Lou\nThe University of Utah\nJichao Fan\nThe University of Utah\nCunxi Yu\nUniversity of Maryland, College Park\nAndy Nonaka\nLawrence Berkeley National Laboratory\nZhi Yao\nLawrence Berkeley National Laboratory\n\nArticle\n\nKeywords:\n\nPosted Date: September 30th, 2024\n\nDOI: https://doi.org/10.21203/rs.3.rs-5061922/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: There is NO Competing Interest.\nVersion of Record: A version of this preprint was published at Nature Communications on May 17th, 2025. See the published version at https://doi.org/10.1038/s41467-025-59847-3.\nOptical Neural Engine for Solving Scientific Partial Differential Equations\n\nYingheng Tang$^{1*†}$, Ruiyang Chen$^{2†}$, Minhan Lou$^2$, Jichao Fan$^2$, Cunxi Yu$^3$, Andy Nonaka$^1$, Zhi (Jackie) Yao$^{1*}$, Weilu Gao$^{2*}$\n\n$^1$Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA.\n$^2$Department of Electrical and Computer Engineering, The University of Utah, Salt Lake City, UT 84112, USA.\n$^3$Department of Electrical and Computer Engineering, University of Maryland, College Park, MD 20742, USA.\n\n*Corresponding author(s). E-mail(s): ytang4@lbl.gov; jackie_zhiyao@lbl.gov; weilu.gao@utah.edu;\n†These authors contribute equally\n\nAbstract\nSolving partial differential equations (PDEs) is the cornerstone of scientific research and development. Data-driven machine learning (ML) approaches are emerging to accelerate time-consuming and computation-intensive numerical simulations of PDEs. Although optical systems offer high-throughput and energy-efficient ML hardware, there is no demonstration of utilizing them for solving PDEs. Here, we present an optical neural engine (ONE) architecture combining diffractive optical neural networks for Fourier space processing and optical crossbar structures for real space processing to solve time-dependent and time-independent PDEs in diverse disciplines, including Darcy flow equation, the magnetostatic Poisson’s equation in demagnetization, the Navier-Stokes equation in incompressible fluid, Maxwell’s equations in nanophotonic metasurfaces, and coupled PDEs in a multiphysics system. We numerically and experimentally demonstrate the capability of the ONE architecture, which not only leverages the advantages of high-performance dual-space processing for outperforming traditional PDE solvers and being comparable with state-of-the-art ML models but also can be implemented using optical computing hardware with unique features of low-energy and highly parallel constant-time processing irrespective of model scales and real-time reconfigurability for tackling multiple tasks with the same architecture. The demonstrated architecture offers a versatile and powerful platform for large-scale scientific and engineering computations.\nIntroduction\n\nPartial differential equations (PDEs) derived from physical laws have been a powerful and faithful computational tool to accelerate the exploration and validation of scientific hypotheses instead of performing expensive and time-consuming real-world experiments [1]. Hence, numerically solving PDEs is essential for scientific research and development in nearly every scientific domain. For example, the interaction of electromagnetic waves with materials and engineered structures in broad applications such as communication, imaging, sensing, and quantum technologies is governed by Maxwell’s equations [2]; automotive and flight aerodynamics for designing and manufacturing road vehicles and airplanes is determined by Navier-Stokes equation [3]; the Earth system including temperature, atmosphere, and ice sheets for understanding climate change and making policies is also described with a series of PDEs [4]. However, current numerical simulation methods to solve PDEs, such as finite difference/volume methods to solve Maxwell’s and the Navier-Stokes equations, are costly in computing time and resources.\n\nMachine learning (ML) offers a new perspective on solving PDEs through data-driven approaches to enable fast and accurate simulations of many multiphysics and multiscale processes [5–7]. However, the ML model deployment on electronic computing hardware requires substantial computing resources and consumes substantial energy. In the foreseeable future, the fundamental quantum mechanics limit will lead to a bottleneck of further reducing the energy consumption and simultaneously increasing the integration density of electronic circuits to catch up with the increasing scale of ML models in demand for solving complex problems [8, 9], thus urgently calling for new high-throughput and energy-efficient ML hardware accelerators. Recently, optical architectures, including photonic integrated circuits for matrix-vector multiplication (MVM) [10, 11], for neuro-inspired spiking neural networks [12, 13], and for photonic reservoir computing [14, 15], and free-space optical systems for MVM [16–18] and diffractive optical neural networks (DONNs) [19–22], are emerging as high-performance ML hardware accelerators by leveraging different particles – photons – to break down electronic bottleneck thanks to high parallelism and low static energy consumption of photons [23]. However, to date, there is no deployment of any optical computing systems for solving PDEs in any scientific domain.\n\nHere, we present a fully reconfigurable and scalable optical neural engine (ONE) architecture that combines DONN systems for processing data in Fourier space and optical crossbar (XBAR) structures for processing data in real space to solve two-dimensional (2D) spatiotemporal profiles in time-independent and time-dependent PDEs. The ONE architecture not only leverages the advantages of high-performance dual-space processing [24], but also can be implemented using optical computing hardware with unique features of low-energy and highly parallel constant-time processing irrespective of model scales, and real-time reconfigurability for tackling multiple tasks with the same architecture. We numerically and experimentally demonstrate the capability of the ONE architecture in solving a broad range of PDEs in diverse disciplines, including the Darcy flow equation in fluid dynamics, the magnetostatic Poisson’s equation in micromagnetics, the Navier-Stokes equation in aerodynamics, Maxwell’s equations in nanophotonics, and coupled electric current and heat transfer equations in\na multiphysics electrical heating problem. The ONE architecture not only outperforms traditional PDE solvers because of its data-driven nature, but also shows comparable and better performance with other ML models while with substantial hardware advantages because of its implementation in the optical domain. The demonstrated ONE architecture is versatile and can be tailored with different combinations of DONN and XBAR structures for solving various PDEs, offering a transformative universal solution for large-scale scientific and engineering computations.\n\nResults\n\nONE Architecture\n\nFigure 1a illustrates the ONE architecture, which takes the spatiotemporal data of an input physical quantity \\( \\mathbf{U} \\), described as a function \\( u(x, y, t) \\) in terms of positions \\( x \\) and \\( y \\) and time \\( t \\), to predict the spatiotemporal data of an output physical quantity \\( \\mathbf{G} \\) described using a function \\( g(x, y, t) \\). The input and output quantities \\( \\mathbf{U} \\) and \\( \\mathbf{G} \\) can be connected through either a single-physics PDE or coupled multiphysics PDEs. There are three branches inside the ONE architecture, including (i) Fourier space processing branch, (ii) real space processing branch, and (iii) physics parameter processing branch. The combination of both real and Fourier space processing has been proven fast, powerful, and efficient in solving PDEs [24], and the incorporation of additional physics parameter processing enables the fusion of multimodal data for complex tasks [25]. More importantly, most operations in these branches can be deployed on optical computing hardware in both real and Fourier space, enabling solving PDEs in high-throughput and energy-efficient manners. The details of each branch are described below.\n\nIn the first Fourier space processing branch, the core arithmetic operations are based on Fourier and inverse Fourier transformations to process input spatiotemporal data in the Fourier space. Their optical hardware implementations are mainly based on reconfigurable DONNs, which contain cascaded reconfigurable diffractive layers. Reconfigurable DONNs can be implemented in both integrated photonic chips [26, 27] and free space [19–21]; see Fig. 1b. There are two fundamental operations in DONNs – optical diffraction and spatial light modulation. For the optical diffraction operation, an optical field right after the \\( l \\)-th diffractive layer, \\( f_l \\), diffracts to the front of \\( (l+1) \\)-th layer, whose optical field, \\( f_{\\text{in},l+1} \\), is a convolution of \\( f_l \\) and the diffraction impulse function \\( h(x, y) \\). Specifically, the complex-valued field at point \\( (x, y) \\) on the input plane of \\( (l+1) \\)-th layer can be written as the convolution of all fields at the output plane of \\( l \\)-th layer as\n\n\\[\nf_{\\text{in},l+1}(x, y, z) = \\iint f_l(x', y', 0) h(x - x', y - y') dx' dy',\n\\]\n\nwhere \\( z \\) is the distance between two diffractive layers and \\( h(x, y) \\) is the impulse response function of free space. By the convolution theorem, this 2D convolution can be efficiently calculated in Fourier space based on Fourier and inverse Fourier transformations. Specifically, the 2D Fourier transformation \\( \\mathcal{F}_{xy} \\) of \\( f \\) and \\( h \\), \\( F \\) and \\( H \\), are\nFig. 1 ONE architecture and hardware implementations. (a) Illustration of processing branches and flows in the ONE architecture to predict output spatiotemporal output physical quantities from corresponding input and solve PDEs involving single or multiple physics. Illustrations of integrated and free-space implementations of reconfigurable (b) DONN and (c) XBAR structures.\n\nconnected through\n\n\\[\n\\mathcal{F}_{xy}(f_{in,t+1}(x,y,z)) = \\mathcal{F}_{xy}(f_t(x,y,0))\\mathcal{F}_{xy}(h(x,y)),\n\\]\n\\[\nF_{in,t+1}(\\alpha,\\beta,z) = F_t(\\alpha,\\beta,0)H(\\alpha,\\beta),\n\\]\n\nwhere \\( \\alpha, \\beta \\) are spatial domain indices. After diffraction, the 2D inverse Fourier transformation \\( \\mathcal{F}_{xy}^{-1} \\) of \\( F_{in,t+1}(\\alpha,\\beta,z) \\), \\( f_{in,t+1}(x,y,z) \\), is then spatially modulated. Each diffraction pixel at location \\( (x,y) \\) has a complex-valued electric field transmission coefficient \\( t(x,y,S)e^{\\phi(x,y,S)} \\), where \\( t(x,y,S) \\) (\\( \\phi(x,y,S) \\)) is the amplitude (phase) response as a function of external stimuli \\( S \\), such as voltages. The spatial light modulation operation is expressed as a pixel-wise multiplication\n\n\\[\nf_{t+1}(x,y,z) = \\mathcal{F}_{xy}^{-1}(F_{in,t+1}(\\alpha,\\beta,z))t(x,y,S)e^{\\phi(x,y,S)}\n\\]\n= f_{in,l+1}(x, y, z)t(x, y, S)e^{\\phi(x, y, S)},$\n\nwhere \\( f_{l+1}(x, y, z) \\) is the near-field output field right after the \\((l+1)\\)-th layer. More details can be found in Methods.\n\nBefore and between DONN kernels, there is a linear transformation operation based on fully connected layers to scale up the number of channels and a channel mixing operation based on matrix multiplications [24]. The core arithmetic operations are based on MVM. Their optical hardware implementations are mainly based on reconfigurable optical XBAR structures, which encode element values of vector \\( \\mathbf{v} \\) and matrix \\( \\mathbf{M} \\) into light intensity through electro-optic modulators, perform multiplications through cascaded modulators, and add signals at the output detector array. The signals are routed to follow mathematical calculations in MVM so that the reading from the detector array represents the output vector \\( \\mathbf{o} = \\mathbf{M} \\times \\mathbf{v} \\). Reconfigurable XBAR structures can also be implemented in both integrated photonic chips [10, 11] and free space [16–18]; see Fig. 1c. More details on the operation mechanism can be found in Methods and Supplementary Fig. 1.\n\nThe second real space processing branch contains fully connected layers, whose operations are also based on MVM and implemented with optical XBAR structures. The output from the Fourier space branch, \\( \\mathbf{F}(u) \\), and the output from the real space branch, \\( \\mathbf{R}(u) \\) are added and further processed with a nonlinear operation. Note that the nonlinear operation is the only operation performed in electronic hardware in the ONE architecture. Moreover, this combination of real space, Fourier space, and nonlinear processing is scaled up, repeated four times, and cascaded in series. The third branch is to perform a linear transformation on other relevant physics parameters \\( d(t) \\), which are time sequences instead of spatiotemporal data, based on fully connected layers. The obtained data \\( \\mathbf{T}(d) \\) is multiplied and merged onto two other branches to have the final output \\( g(x, y, t) \\). Hence, except nonlinear operations, all other operations can be done with DONN and optical XBAR systems. These two systems can be seamlessly assembled into a single integrated photonic chip or a single free-space optical system for all-optical operations without converting between optical and electronic hardware, fully leveraging the advantages of high throughput and high parallelism in optical computing systems. More details on the ONE architecture model are in Methods.\n\nDarcy flow and magnetostatic Poisson’s equations\n\nThe first PDE we solved with the ONE architecture is the Darcy flow equation in fluid dynamics physics. This PDE describes a fluid flow through a porous medium as shown in Fig. 2a. Specifically, the equation is\n\n\\[\n-\\nabla \\cdot (k(x, y) \\nabla u(x, y)) = f(x, y),\n\\]\n\nwhere \\( k(x, y) \\) is the permeability field of the medium, \\( u(x, y) \\) is the pressure field of the flow, and \\( f(x, y) \\) is the force function. The ONE architecture was trained to learn the mapping from the 2D function \\( k(x, y) \\) to function \\( u(x, y) \\). More details about the equation dataset generation and training are in Methods. Figure 2b displays the training loss curves for inputs with different resolutions. The training loss\nis generally low for all resolutions and slightly increases at the highest 421 resolution. Figure 2c shows the comparison of the training loss of our ONE architecture with other PDE solving models, including fully convolution networks (FCN) [28], principal component analysis-based neural network (PCANN) [29], reduced biased method (RBM) [30], graph neural operator (GNO) [31], low-rank kernel decomposition neural operator (LNO) [25], multipole graph neural operator (MGNO) [32], and Fourier neural operator (FNO) [24]. The performance of the ONE architecture is comparable with the state-of-the-art neural operators including GNO, LNO, MGNO, and FNO, and is better than FCN. Further, from the hardware perspective, the ONE architecture is constructed based on high-throughput optical computing hardware platforms so that all operations can be performed in parallel within a single clock cycle. In addition, the ONE architecture can be practically implemented on a large scale. For example, free-space reconfigurable DONNs [20, 21, 33] and optical MVM [17] are typically implemented using spatial light modulators (SLMs) with a scale > 1000 × 1000. Hence, the execution cost of solving PDEs with different scales and resolutions is invariant, meaning \\( \\mathcal{O}(1) \\), if the scale of the optical hardware in the ONE architecture is large enough. Figure 2d displays the input permeability field \\( k(x, y) \\), the expected ground truth of output pressure field \\( u(x, y) \\), the predicted output pressure field, the absolute error between the expected and predicted outputs, and the relative error between the expected and predicted outputs, at the lowest 85 and the highest 421 resolutions, respectively. This visualization further validates the ONE architecture in solving PDEs. More data on other resolutions are shown in Supplementary Fig. 2.\n\nThe second PDE we solved is the magnetostatic Poisson’s equation of demagnetization in micromagnetics physics. This PDE calculates the demagnetizing field \\( \\mathbf{H} \\) generated by the magnetization field \\( \\mathbf{M} \\) as shown in Fig. 2e. Specifically, the equation is obtained from Maxwell’s equation as\n\n\\[\n\\nabla \\cdot \\mathbf{H} = -\\nabla \\cdot \\mathbf{M}.\n\\]\n\nBy defining an effective magnetic charge density \\( \\rho = -\\nabla \\cdot \\mathbf{M} \\) and a magnetic scalar potential \\( \\Phi \\) assuming there is no free current, we can express the demagnetizing field \\( \\mathbf{H} = -\\nabla \\Phi \\) and rewrite the previous equation as a Poisson’s equation\n\n\\[\n\\nabla^2 \\Phi = -\\rho.\n\\]\n\nSimilar to solving the Darcy flow equation, the ONE architecture was trained to learn the mapping from components of \\( \\mathbf{M} \\) to \\( \\mathbf{H} \\) vector fields. More details about the equation dataset generation and training are in Methods. Figure 2f shows the validation loss curve and Fig. 2g shows the input one component of \\( \\mathbf{M} \\) field, the expected ground truth of output \\( H_x \\) component of \\( \\mathbf{H} \\) field, the predicted output \\( H_x \\) component, the absolute error between the expected and predicted outputs, and normalized error between the expected and predicted outputs with respect to the maximum field strength in the ground truth. Both confirm a good performance of the ONE architecture in solving the magnetostatic Poisson’s equation. More data on \\( H_y \\) and \\( H_z \\) components is shown in Supplementary Fig. 3.\nFig. 2 Solving Darcy flow and magnetostatic Poisson’s equations. (a) Illustration of the Darcy flow equation describing a fluid flow through a porous medium. The ONE architecture learns the mapping between the permeability and pressure fields. (b) Training loss curves for input data with different resolutions. (c) Comparison of the training loss of different models at various resolutions. (d) Input permeability field, the expected ground truth of output pressure field, the predicted output pressure field, the absolute error between the expected and predicted outputs, and the relative error between the expected and predicted outputs, at 85 and 421 resolutions. (e) Illustration of the magnetostatic Poisson’s equation calculating the demagnetizing field generated by the magnetization field. The ONE architecture learns the mapping between these two fields. (f) Validation loss curve for the ONE architecture solving the magnetostatic Poisson’s equation and (g) corresponding input magnetization field, the expected ground truth of output demagnetizing field, the predicted output demagnetizing field, the absolute and normalized errors between the expected and predicted outputs.\n\nNavier-Stokes and Maxwell’s equations\n\nIn addition to steady-state Darcy flow and magnetostatic Poisson’s equations without time evolution, we employed the ONE architecture to solve time-dependent PDEs, including the Navier-Stokes equation in fluid dynamics and Maxwell equations in electromagnetics and optics. In particular, the real-time reconfigurability of DONN and optical XBAR structures makes the ONE architecture suitable for such a purpose.\nSpecifically, we solved a 2D Navier-Stokes equation for a viscous, incompressible fluid in vorticity form on the unit torus as shown in Fig. 3a. This PDE calculates the time evolution of vorticity described as\n\n\\[\n\\partial_t w(x, y, t) + u(x, y, t) \\cdot \\nabla w(x, y, t) = v \\Delta w(x, y, t) + f(x, y),\n\\]\n\nwhere \\(u\\) is the velocity field, \\(w = \\nabla \\times u\\) is the vorticity, \\(v\\) is the viscosity coefficient, \\(f\\) is the forcing function. The ONE architecture was trained to learn the mapping from \\(w\\) in a time range from 0 to \\(t_0\\) to \\(w\\) in a time range from \\(t_0\\) to \\(t_1\\) (\\(t_1 > t_0\\)). More details about the equation dataset generation and training are in Methods. Further, we also solved Maxwell’s equations in a dielectric metasurface consisting of multiple cylindrical pillars in a unit cell of a periodic pattern as shown in Fig. 3b [34]. The general Maxwell’s equations can calculate the time evolution of an electric field through the following equations\n\n\\[\n\\nabla \\cdot \\mathbf{D} = \\rho,\n\\]\n\\[\n\\nabla \\cdot \\mathbf{B} = 0,\n\\]\n\\[\n\\nabla \\times \\mathbf{E} = -\\frac{\\partial \\mathbf{B}}{\\partial t},\n\\]\n\\[\n\\nabla \\times \\mathbf{H} = \\mathbf{J} + \\frac{\\partial \\mathbf{D}}{\\partial t},\n\\]\n\nwhere \\(\\mathbf{D}\\) is the electric displacement field, \\(\\rho\\) is the free charge density, \\(\\mathbf{B}\\) is the magnetic flux density, \\(\\mathbf{E}\\) is the electric field, \\(\\mathbf{H}\\) is the magnetic field, and \\(\\mathbf{J}\\) is the free current density. The ONE architecture was trained to learn the mapping from \\(\\mathbf{E}\\) in a time range from 0 to \\(t_0\\) to \\(\\mathbf{E}\\) in a time range from \\(t_0\\) to \\(t_1\\) (\\(t_1 > t_0\\)). More details about the dataset generation and training are in Methods. Figure 3c displays the validation loss curve for solving the Navier-Stokes equation with \\(t_0 = 10\\) and \\(t_1 = 20\\). Figure 3d displays the validation loss curves for solving Maxwell’s equations with \\(t_0 = 10\\) and \\(t_1 = 20, 30, 40\\), respectively. Moreover, Figure 3e and 3f show the expected ground truth of \\(w\\) field and the \\(E_x\\) component of the \\(\\mathbf{E}\\) field at \\(t_1\\), the corresponding predicted fields at \\(t_1\\), and the absolute and relative errors between ground truth and prediction for the Navier-Stokes equation and Maxwell’s equations, respectively. All confirm a good performance in solving time-dependent PDEs using the ONE architecture.\n\nMultiphysics PDEs\n\nMoreover, we employed the ONE architecture to solve coupled PDEs involving two physics. Specifically, we solved an electrical heating problem to obtain a temperature profile at an intermediate time step \\(t_n\\), \\(T(x, y, t_n)\\), in an electrical circuit when a time-dependent voltage signal was applied to the circuit pads, involving coupled electric current physics and heat transfer physics; see Fig. 4a. Specifically, for the electrical current physics, the corresponding PDE is\n\n\\[\nQ_e = d \\sigma \\nabla_t V(x, y, t),\n\\]\nFig. 3 Solving time-dependent Navier-Stokes and Maxwell’s equations. Illustrations of (a) Navier-Stokes equation for solving the time evolution of the vorticity field in a viscous, incompressible fluid in vorticity form on the unit torus and (b) Maxwell’s equations for solving the time evolution of the electric field in a dielectric metasurface. Validation loss curves for (c) solving the Navier-Stokes equation and (d) Maxwell’s equations using the ONE architecture. The expected ground truth field, the predicted field, and the absolute and relative errors between these two fields for (e) the Navier-Stokes equation and (f) Maxwell’s equations, respectively.\n\n\\[\nV(x_0, y_0, t) = \\mathrm{rect}(t),\n\\]\n\nwhere \\( Q_e \\) is the heat rate per unit area from an electromagnetic heating source, \\( d \\) is the thickness of the heating layer, \\( V(x, y, t) \\) is the voltage profile in the circuit that is subjected to a voltage boundary condition defined in the pads \\( V(x_0, y_0, t) \\), and \\( V(x_0, y_0, t) \\) is a pulse rectangular function \\( \\mathrm{rect}(t) \\) with pulse height and width. For the heat transfer physics, the corresponding PDE is\n\n\\[\n\\rho C_p \\frac{\\partial T}{\\partial t} + \\rho C_p \\mathbf{u} \\cdot \\nabla T - \\nabla \\cdot (k \\nabla T) = Q_e,\n\\]\n\nwhere \\( \\rho \\) is the mass density, \\( C_p \\) is the specific heat capacity, \\( T \\) is the absolute temperature, and \\( k \\) is the thermal conductivity. These two PDEs are connected through the quantity \\( Q_e \\). The ONE architecture was trained to learn the mapping from \\( V(x, y, t) \\)\nin a time range spanning all time steps in input pulses to \\( T(x, y, t_n) \\) at an intermediate pulse time step \\( t_n \\). In contrast to previous examples, the pulse information, including pulse height and width, was processed through the physics parameter processing branch in the ONE architecture (Fig. 1a) and multiplied with the output from cascaded real space processing and Fourier space processing branches to yield the final output. More details about the dataset generation and training are in Methods. Figure 4b displays the validation loss curve and Fig. 4c shows a few representative input 2D data \\( V(x, y, t) \\) at various time steps. Figure 4d shows the expected ground truth of \\( T(x, y, t_n) \\), the corresponding predicted temperature profile, and the absolute and relative errors between ground truth and prediction. All confirm a good performance in solving multiphysics PDEs using the ONE architecture.\n\n![Illustration of solving coupled PDEs in an electrical heating problem involving electric current physics and heat transfer physics. Validation loss curve. A few representative 2D voltage profiles in the circuit. The expected ground truth temperature profile, the predicted profile, and the absolute and relative errors between these two profiles.](page_370_682_1002_563.png)\n\nFig. 4 Solving multiphysics PDEs. (a) Illustration of solving coupled PDEs in an electrical heating problem involving electric current physics and heat transfer physics. (b) Validation loss curve. (c) A few representative 2D voltage profiles in the circuit. (d) The expected ground truth temperature profile, the predicted profile, and the absolute and relative errors between these two profiles.\n\nExperimental demonstration\n\nFinally, to demonstrate the experimental feasibility of the ONE architecture, we constructed a free-space reconfigurable DONN setup and evaluated the performance of\nsolving the Darcy flow equation under different hardware noise levels in optical XBAR structures. Figure 5a displays a photo and schematic of the reconfigurable DONN setup, which contains a laser source, a reconfigurable input encoder, two reconfigurable diffractive layers, and a camera. The reconfigurable encoder and diffractive layers were built upon SLMs, which can modulate the amplitude and phase of transmitted light when applying voltage. Multiple light polarization components, including polarizers and half-wave plates, were also employed to manipulate polarization states to achieve large phase modulation ranges. More details on the experimental setup are in Methods.\n\n(a)\n\n![Photo and schematic of a reconfigurable DONN experimental setup consisting of a reconfigurable input encoder, two reconfigurable diffractive layers, and a camera. Polarization components were used to configure SLMs in the phase modulation mode.](page_324_370_1096_282.png)\n\n(b) ![Output 2D data in one DONN kernel of the Fourier space processing branch in the ONE architecture obtained from model calculations and experimental measurements.](page_324_670_420_180.png)\n\n(c) ![Validation loss curves at different noise levels in optical XBAR structures.](page_744_670_246_180.png)\n\n(d) ![Loss at the final epoch as a function of noise level.](page_1010_670_180_180.png)\n\nFig. 5 Experimental demonstration. (a) Photo and schematic of a reconfigurable DONN experimental setup consisting of a reconfigurable input encoder, two reconfigurable diffractive layers, and a camera. Polarization components were used to configure SLMs in the phase modulation mode. (b) Output 2D data in one DONN kernel of the Fourier space processing branch in the ONE architecture obtained from model calculations and experimental measurements. (c) Validation loss curves at different noise levels in optical XBAR structures and (d) the loss at the final epoch as a function of noise level.\nAs shown in Supplementary Fig. 1, the experimentally measured amplitude and phase modulation responses of all three SLMs are not only discrete with respect to grey levels but also coupled and dependent. To leverage the gradient-based ML training algorithm, we utilized the Gumbel–softmax reparameterization technique to approximate a discrete distribution to a continuous distribution [21]. More details are described in Methods. Moreover, the values of input 2D data span both negative and positive values and were encoded as the grey level of the SLM in the reconfigurable input encoder (SLM0 in Fig. 5a). We performed the encoding through linear mapping from minimum and maximum values of input data to a grey-level range in the SLM. More details are described in Methods. In addition, we precisely aligned all SLMs with respect to each other within a range of a few pixels on the order of hundreds of \\( \\mu m \\); see Supplementary Fig. 5. Although the long optical path in the system makes the alignment sensitive to external variations, the system’s full reconfigurability can enable fast adaptive pixel-by-pixel re-alignment. Figure 5b shows output 2D data in one DONN kernel of the Fourier space processing branch in the ONE architecture (Fig. 1a) obtained from model calculations and experimental measurements, showing good agreement and experimentally validating the feasibility of the ONE architecture in solving PDEs. More data is shown in Supplementary Fig. 6. There are some speckles in the background of measured images, which probably originate from high-order diffraction interference, leading to numerical errors in the ONE architecture for performing regression tasks. This discrepancy between models and experiments can be mitigated through hardware-software co-design, such as incorporating loss functions based on experimental results for gradient calculations as demonstrated in prior works [20, 33, 35].\n\nWe also evaluated the performance of the ONE architecture under different noise levels of optical XBAR structures. Specifically, we added random Gaussian noise with zero mean and varying standard deviation (Std) to the values obtained from matrix multiplications to represent hardware noise, such as shot noise in photodetectors [36]. The corresponding MVM results and histograms of different noise standard deviation values are shown in Supplementary Fig. 7, and more details can be found in Methods. As shown in Fig. 5c and Fig. 5d, the validation loss increases with the increasing noise standard deviation value. The current hardware implementation of optical XBAR structures with advanced components and calibration algorithms [16–18], including the structure we demonstrated before [36], can achieve quite a small noise level similar or below the noise level corresponding to 0.5 Std. Hence, the noise influence in optical XBAR structures on the performance of the ONE architecture is not substantial.\n\nWe further estimated the potential throughput and power consumption of the ONE architecture implemented using optical computing hardware for inference. The throughput is mainly determined by the SLM refresh rate and camera frame rate. Current commercial SLMs and cameras can have rates > 1000 Hz, meaning that the inference time for one instance is < 1 ms. In contrast, it typically takes minutes to hours to numerically solve PDEs. Hence, the ONE architecture features \\( > 10^5 \\) (five orders of magnitude) acceleration compared to typical PDE solvers. This throughput is also comparable to the state-of-art ML model, such as FNO with a 5 ms inference time [24]. Moreover, the system throughput can be substantially improved with device\ninnovation. For example, an electro-optic SLM based on organic molecules can achieve > GHz switching speed [37], and an ultrafast camera can achieve a trillion frames per second [38]. With these devices, the ONE architecture can achieve an inference time < 1 ns. The power consumption is mainly determined by the leakage current of liquid crystal cells in SLMs. Because of the dielectric nature of liquid crystals and their high leakage resistance, the leakage current is typically < 1 \\( \\mu \\)A. Hence, assuming a 10 V driving voltage, the static power consumption of SLMs is \\( \\sim 10 \\mu \\)W, which is nearly \\( 10^7 \\) (seven orders of magnitude) smaller than typical GPU inference power \\( \\sim 100 \\) W.\n\nDiscussion\n\nWe have demonstrated the ONE architecture and validated its performance in solving a broad range of PDEs in diverse scientific domains. The ONE architecture is versatile and can be modified to reduce the interface and connection between DONN and optical XBAR structures and facilitate the hardware implementation of the whole system. Further, in a whole system, active learning and noise-aware training can be incorporated to mitigate the discrepancy between models and practical systems for accurate deployment. Moreover, in addition to solving PDEs, the ONE architecture can be tailored to accelerate ML models for other regression problems.\n\nMethods\n\nDONN diffraction model – The diffraction impulse function \\( h(x, y) \\) was described using the Fresnel equation as\n\n\\[\nh(x, y) = \\frac{e^{ikz}}{i \\lambda z} e^{\\frac{-ik}{2z}(x^2 + y^2)},\n\\]\n\nwhere \\( \\lambda \\) is the wavelength, \\( k = 2\\pi/\\lambda \\) is the free-space wavenumber, \\( (x, y) \\) are positions within a plane perpendicular to the wave propagation direction, \\( z \\) is the distance along the propagation direction, and \\( i \\) is the imaginary unit. The 2D Fourier transformation was directly performed on \\( h(x, y) \\) for model training and evaluation. To match the experimental setup as described below, \\( h(x, y) \\) was first discretized with respect to a defined rectangular mesh grid in the convolution calculation and then converted into the Fourier space through 2D Fourier transformation. More details can be found in our prior work [21].\n\nThe operation mechanism of optical XBAR structures - Supplementary Fig. 1a shows the detailed schematic of an integrated photonic XBAR structure. Specifically, the element values of a \\( n \\times 1 \\) input vector \\( \\mathbf{v} \\) are represented by the intensities of light at input waveguides, \\( \\{I_1, I_2, I_3, ..., I_n\\} \\), which can be implemented by modulating an equally distributed laser intensity through a \\( n \\times 1 \\) array of electro-optic modulators (red squares in Supplementary Fig. 1a) at input waveguides. The light on each row waveguide is then equally distributed to the column waveguides connected to that row waveguide and modulated through an electro-optic modulator on the coupled curved waveguide (yellow squares in Supplementary Fig. 1a). The element values of a \\( m \\times n \\)\nmatrix \\( \\mathbf{M} \\) are represented by the transmittance of modulators on curved waveguides, \\( \\{T_{ij}\\}, i \\in [1,m], j \\in [1,n] \\). At the end of each column waveguide, a photodetector collects all light intensity passing through the column waveguide. The obtained photocurrents or photovoltages of a \\( m \\times 1 \\) photodetector array represent the summation of multiplied input vector light intensity and matrix modulator transmittance, and the element values of output vector \\( \\mathbf{o} \\), \\( O_j = \\sum_{s=1}^n T_{js} I_s, j \\in [1,m] \\). Hence, this integrated photonic XBAR structure can implement MVM in the optical domain.\n\nSimilarly, Supplementary Fig. 1b shows the detailed schematic of a free-space optical XBAR structure. Specifically, the element values of a \\( n \\times 1 \\) input vector \\( \\mathbf{v} \\) are represented by the intensities of light, \\( \\{I_1, I_2, I_3, ..., I_n\\} \\), which is implemented through a \\( n \\times 1 \\) array of free-space vector SLM. The output light is broadcast to a \\( m \\times n \\) array of matrix SLM through lenses so that the light distribution from vector SLM is identical at each column of matrix SLM. The element values of a \\( m \\times n \\) matrix \\( \\mathbf{M} \\) are represented by the transmittance of matrix SLM, \\( \\{T_{ij}\\}, i \\in [1,m], j \\in [1,n] \\). Lenses are then used to focus the output light from each modulator on the same column of matrix SLM to a photodetector. The readings from a \\( m \\times 1 \\) photodetector array represent the element values of output vector \\( \\mathbf{o} \\), \\( O_j = \\sum_{s=1}^n T_{js} I_s, j \\in [1,m] \\). Hence, this free-space optical XBAR structure can also implement MVM in the optical domain.\n\n**ONE architecture model** – The ONE architecture model was constructed with two main modules – the DONN module processing data in the Fourier space and the optical XBAR module processing linear operations. The mathematical operations in DONN and optical XBAR structures have been described before and their accurate models have been implemented in our prior works, closely matching experimental results [21, 36]. Briefly, the DONN module was modeled by combining the Fresnel free-space diffraction with phase-only spatial light modulation in a range of \\( [0, 2\\pi] \\) in the model and coupled spatial light modulation as shown in Supplementary Fig. 4; the optical XBAR module was represented as matrix multiplication incorporating measurement noise. Both modules were implemented under the PyTorch 1.12 framework with graphics processing unit (GPU)-accelerated parallel computation and gradient backpropagation for training. The GPU used in this work was an Nvidia RTX 6000 card.\n\n**Darcy flow equation dataset and training** – A 2D Darcy flow equation on the unit box was employed as described in detail in Ref. [24]. The corresponding PDE is a second-order, linear, elliptic PDE as\n\n\\[\n-\\nabla \\cdot (k(x,y)\\nabla u(x,y)) = f(x,y), \\qquad x \\in (0,1), y \\in (0,1),\n\\]\n\\[\nu(x) = 0, \\qquad x \\in \\partial(0,1), y \\in \\partial(0,1)\n\\]\n\nwith a Dirichlet boundary condition. We used the Darcy flow dataset from the existing dataset in Ref. [24] with a boundary condition \\( u(x,y) = 0 \\) on domain edges. The coefficient \\( k(x,y) \\) was generated based on a specific distribution with the value 12 for positive inputs and 3 for negative inputs. The forcing term was fixed at \\( f(x,y) = 1 \\). The solution \\( u(x,y) \\) was computed using a second-order finite difference method on a \\( 421 \\times 421 \\) grid, and other resolutions were obtained with downsampling. We used a 10 : 1 ratio for the numbers of data in the training set and validation set, respectively.\nThe model was trained with a total of 600 epochs and a batch size of 40. The learning rate was 0.1 for the trainable parameters in DONNs and 0.001 for all other trainable parameters with the Adam optimizer.\n\nMagnetostatic Poisson’s equation dataset and training – The demagnetizing field \\( \\mathbf{H} \\) originates from the magnetization within the material itself, which can be calculated as the convolution of \\( \\mathbf{M} \\) with the demagnetization tensor \\( \\mathbf{N} \\) as\n\n\\[\n\\mathbf{H}(\\mathbf{r}) = \\int \\mathbf{N}(\\mathbf{r} - \\mathbf{r}') \\mathbf{M}(\\mathbf{r}') d\\mathbf{r}'.\n\\]\n\nThis convolution was computed through Fourier space representations of fields. Specifically, to create the dataset, we utilized the MagneX solver [39] to simulate the time evolution of magnetization in a thin magnetic film with dimensions of \\( 500 \\times 125 \\times 3.125 \\) nm. The modeling incorporated both demagnetization and exchange interactions. Initially, we relaxed the magnetic field into a stable S-state before subjecting the system to varying external magnetic fields in different scenarios. We uniformly sampled 8 bias \\( \\mathbf{H} \\) fields in the \\( x \\) and \\( y \\) directions, each with a magnitude of 19872 A/m. The system evolved for 1 ns, during which we collected paired data of \\( \\mathbf{M} \\) and \\( \\mathbf{H} \\) fields. Each field was represented by three channels corresponding to the field components in \\( x \\), \\( y \\), and \\( z \\) directions. The dataset was divided into training and testing sets with an 8 : 2 ratio. The training was conducted over 500 epochs with a batch size of 128. The learning rate was set to 1.0 for the trainable parameters in DONNs and 0.001 for all other trainable parameters with the Adam optimizer.\n\nNavier-Stokes equation dataset and training – A 2D Navier-Stokes equation for a viscous, incompressible fluid in vorticity form on the unit torus was used to generate spatiotemporal data for training the ONE architecture. The details are described in Ref. [24]. Specifically, the PDEs are\n\n\\[\n\\begin{align*}\n\\partial_t w(x, y, t) + u(x, y, t) \\cdot \\nabla w(x, y, t) &= v \\Delta w(x, y, t) + f(x, y), & x \\in (0, 1), y \\in (0, 1), t \\in (0, T] \\\\\n\\nabla \\cdot u(x, y, t) &= 0, & x \\in (0, 1), y \\in (0, 1), t \\in (0, T] \\\\\nw(x, y, 0) &= w_0(x, y), & x \\in (0, 1), y \\in (0, 1),\n\\end{align*}\n\\]\n\nwhere \\( w_0(x, y) \\) is the initial vorticity and boundary conditions were used. We utilized the existing dataset with the viscosity coefficient \\( v = 10^{-3} \\) from Ref. [24] for training and inference. The samples in the dataset were recorded with a time step of \\( 10^{-4} \\) s. We used 1000 data as the training set and 100 data as the validation set. We trained the ONE architecture model with the first 10 vorticity fields (\\( w(x, y, t) \\)) to predict the time evolution of the next 10 vorticity fields. The model was trained with a total of 600 epochs and a batch size of 40. The learning rate was 0.1 for the trainable parameters in DONNs and 0.001 for all other trainable parameters with the Adam optimizer.\n\nMaxwell’s equations dataset and training – We employed commercial Ansys Lumerical finite-difference-time-domain simulation software to generate an electric field dataset by solving Maxwell’s equations in dielectric metasurfaces. Specifically, the dielectric metasurface had a periodic pattern and we used four silicon cylindrical rods as the unit cell and periodic boundary condition. Data were generated by randomly\nselecting the radii of four cylindrical rods. The radius was chosen from 39.5\\( \\mu \\)m to 44.5 \\( \\mu \\)m with a step of 0.25 \\( \\mu \\)m. The simulation time was set as 300000 fs. We generated a total of 1200 data and used 1000 as the training set and the rest 200 as the validation set. The model was trained in an auto-regressive style for the \\( E_x \\) component processing. The \\( E_x \\) field data between 300000 fs to 160000 fs was backward fed into to the model to predict the next 40000 fs \\( E_x \\) field data. The model was trained with a total of 500 epochs and a batch size of 20. The learning rate was 0.1 for the trainable parameters in DONNs and 0.001 for all other trainable parameters with the Adam optimizer.\n\nMultiphysics dataset and training – We employed commercial COMSOL Multiphysics finite-element simulation software to generate a temperature profile dataset by solving coupled electric current and heat transfer PDEs in an electrical heating circuit. The circuit details can be found in Ref. [40]. Concisely, the circuit contained a serpentine-shaped Nichrome resistive layer with 10 \\( \\mu \\)m thick and 5 mm wide on top of a glass plate. A silver contact pad with a dimension 10 mm \\( \\times \\) 10 mm \\( \\times \\) 10 \\( \\mu \\)m was attached at each end. The deposited side of the glass plate was in contact with the surrounding air at 293.15 K and the back side was in contact with the heated fluid at 353 K. Two coupled physics modules, electrical current in layered shells and heat transfer in layered shells, were used in COMSOL simulations. The input voltage pulse height was set from 5 to 25 V with a step of 1 V and the pulse width was set from 20 to 60 s with a step of 1 s. The simulation time range was from 0 to 110 s. We generated a total number of 861 data and divided the data into training and testing set with the splitting ratio of 8 : 2. The ONE architecture took the electric current layer data as the input spatiotemporal data and the input voltage pulse information was fed into the physics parameter data processing branch to predict temperature field data at 55 s. The model was trained with a total of 100 epochs and a batch size of 40. The learning rate for the trainable parameters in DONNs was 0.1 and the learning rate for all other trainable parameters was 0.001 with the Adam optimizer.\n\nDONN experimental setup and alignment – The photo and schematic diagram of the DONN experimental setup are displayed in Fig. 5a. The laser diode with a center wavelength 532 nm (CPS532 from Thorlabs, Inc.) was used as a source. The distance between SLMs and between the last SLM and camera was set as 25.4 cm. The polarizers and half-wave plates before and after each SLM were configured so that each SLM operated with a strong modulation of the transmitted electric field phase (phase mode) together with a moderate modulation of light amplitude. The experimentally measured amplitude and phase modulation responses of three SLMs are shown in Supplementary Fig. 4. All transmissive SLMs are the LC 2012 model from HOLOEYE Photonics AG with a refresh rate of 60 Hz. The analog-to-digital converter has 8-bit precision for liquid crystal driving voltage, so that the grey level of SLMs is from 0 to 255. The pixel size of SLMs is 36 \\( \\mu \\)m \\( \\times \\) 36 \\( \\mu \\)m. The output data was captured on a CMOS camera with a frame rate of 34.8 frames per second (CS165MU1 from Thorlabs, Inc.).\n\nWe aligned the DONN setup by loading standard images on SLMs and comparing experimental results with simulation. Specifically, as shown in Supplementary Fig. 5a, standard Gaussian images, which were centered with a peak at 255 grey level and with a standard deviation of 6 pixels, were loaded in the input SLM and two diffractive\nSLMs. Supplementary Fig. 5b displays the simulation pattern for the perfectly aligned setup. During the alignment process, loaded images were moved up, down, left, and right pixel-by-pixel to match the captured images by the camera with the simulation pattern. Supplementary Fig. 5c displays the matched experimental diffraction pattern when the optical setup was aligned, while Supplementary Fig. 5d shows misaligned patterns when there was five-pixel misalignment in vertical and horizontal directions, respectively.\n\nDONN experimental training with reparameterization – The discrete look-up tables of device responses shown in Supplementary Fig. 4 break the gradient backpropagation in the ML training process in PyTorch. To solve this challenge, we utilized a differentiable reparameterization Gumbel-softmax technique, which was first introduced in Ref. [41] and demonstrated in our prior work [21]. Specifically, continuous noise from the Gumbel distribution was added to the discrete distribution. The argmax function was then used to find the optimized sample. The training problem after this Gumbel–argmax process is mathematically equivalent to the original training problem under one-hot representation [41]. Since the argmax function still breaks the gradient chain, it was replaced with the softmax function to enable differentiability. Hence, this Gumbel-softmax technique, which is also available in PyTorch, offers continuous and differentiable approximation to discrete distributions and the gradient can backpropagate to reduce the loss function.\n\nDONN experimental grey-level encoding – The global minimum and maximum values in input 2D data were calculated as \\( d_{\\min} \\) and \\( d_{\\max} \\). A grey level range from 130 to 255 in the input encoder SLM was selected for a relatively large amplitude modulation range to have enough contrast. Hence, any value \\( d \\) in the input 2D data was converted into a grey level through a linear mapping as\n\n\\[\nd = \\text{int}\\left( \\frac{255 - 130}{d_{\\max} - d_{\\min}} + 130 \\right),\n\\]\n\nwhere the int(\\(\\cdot\\)) operation rounded the expression to the nearest integer since the SLM grey level must be an integer.\n\nOptical XBAR noise – The MVM results from an optical XBAR structure were uniformly randomly generated in a range of \\(-15\\) to \\(15\\), which was the value range in the ONE architecture for solving the Darcy flow equation. The expected number \\( o \\) was then added with a randomly generated noise from a Gaussian distribution with a zero average and varying standard deviation. The noise-dressed number \\( \\tilde{o} \\) was used in ONE architecture calculations. Under different noise standard deviation levels, Supplementary Fig. 7a demonstrates \\( \\tilde{o} \\) with respect to \\( o \\) and Supplementary Fig. 7b displays histograms of \\( \\tilde{o} - o \\).\n\nData availability\n\nUpon publication, all data that support the plots within this paper and other findings of this study will be available on a public GitHub repository.\nCode availability\n\nUpon publication, all codes that support the plots within this paper and other findings of this study will be available on a public GitHub repository.\n\nAcknowledgements\n\nR.C., C.Y., and W.G. acknowledge support from the National Science Foundation through Grants No. 2235276, No. 2316627, and No. 2428520. M.L., J.F., and W.G. also acknowledge support from the University of Utah start-up fund. Y.T., Z.Y., and A.N. were supported by Laboratory Directed Research and Development (LDRD) funding from Berkeley Lab, provided by the Director, Office of Science, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231 and under NERSC GenAI award under No. DDR-ERCAP0030541.\n\nAuthor Contributions Statement\n\nY.T. and W.G. conceived the idea and W.G. supervised the project. Y.T. constructed models and performed machine learning calculations with the help of M.L., J.F., and C.Y and under the support of A.N., Z.Y, and W.G. R.C constructed an optical experimental setup, performed experiments, and performed numerical calculations under the supervision of W.G. 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However, the variability of the scattering MMF channel poses a challenge for achieving long-term accurate transmission over long distances, of which static optical propagation modeling with calibrated transmission matrix or data-driven learning will inevitably degenerate. In this paper, we present a self-supervised dynamic learning approach that achieves long-term, high-fidelity transmission of arbitrary optical fields through unstabilized MMFs. Multiple networks carrying both long- and short-term memory of the propagation model variations are adaptively updated and ensembled to achieve robust image recovery. We demonstrate >99.9% accuracy in the transmission of 1024 spatial degree-of-freedom over 1km-length MMFs lasting over 1000 seconds. The long-term high-fidelity capability enables compressive encoded transfer of high-resolution video with orders of throughput enhancement, offering insights for artificial intelligence promoted diffusive spatial transmission in practical applications.\n\nPhysical sciences/Optics and photonics/Optical techniques/Imaging and sensing \nPhysical sciences/Optics and photonics/Applied optics/Fibre optics and optical communications\n\n# Introduction\n\nPropagation of optical field for long distance is the essential requirement in remote imaging and optical communication applications. Optical fibers, especially the single-mode fiber, have been elaborately deployed in internet connection, however, they only allow for the transmission of a single Gaussian fundamental beam. Multimode-fiber (MMF), on the other hand, permits hundreds to several thousand spatial modes to pass through. This makes them a promising platform for direct image transmission and mode-division multiplexing transmission to boost the channel capacity [1-5], showing potential in applications such as compact endoscopy in bio-imaging [6-11], high-rate optical communication [12], and quantum key teleportation [13-15].\n\nHowever, the inevitable spatial mode dispersion in the MMFs induces a complex optical field mixing of the input image as it propagates through the fiber, resulting in intense scrambling of the output intensity distribution. Image restoration through diffuse media entails precise characterization of the physical system. Methods have been developed that measure the MMF’s forward process in the form of a complex transmission matrix (TM), and unscramble the output image via back-projection [3-4, 16-17]. However, the calibration of TM with huge number of elements is time-consuming and complicated in implementation. Artificial intelligent approaches have been proposed to model the forward process [2,19] or directly estimate the decoding process [20-24] for image inference from the scrambled output. Notwithstanding the notable progress in modeling scattering process, it is foreseen that the instability of the MMF propagation induced by system drifting and environmental disturbance will accumulate and severely deviate from the characterized model after long time, especially for long-distance transmission. As a consequence, most reported literatures have experimented on short MMFs (<10 m) [2-4,24] and were impeded from practical long-term high-fidelity image transmission. Therefore, developing a technique to support long-term accurate spatial information transmission over long-distance for remote video transfer remains a challenge.\n\nOne method to tackle the variation of scattering is to train a general network using large sets of data describing diverse conditions [22-25]. However, this requires a long-duration training data collection and will hinder its flexible application in practice. Moreover, the generalized model often achieves poorer performance at a certain timepoint than using a ‘specific’ network trained on data acquired within small time durations. Another inspiring approach is to use the mixture-of-expert framework, in which multiple expert networks each responsible for one sub-problem are fused together to achieve better generalization [25-28]. This architecture has been successfully applied for image denoising [29-31] and phase retrieval [32] to improve reconstruction accuracy and robustness to noise. However, the implementations have so far been confined to static contexts.\n\nIn this work, we develop a dynamic learning framework that can adaptively handle the time-varying optical propagation in long MMFs. The proposed network, termed multi-scale memory dynamic-learning network (MMDN), leverages the multi-expert framework to separately model the long- and short-term dynamics of the unstable MMF channel with multiple networks and combine the multi-scale memory by adaptive weighted ensemble. The network parameters are dynamically updated over time in a self-supervised manner, by learning from currently predicted pseudo-labels to synthesize the optimal inverse transmission model for subsequent image inference. MMDN achieves adaptive and accurate tracing of the variations on the optical propagation model in MMF, enabling parallel transmission of 1024 spatial degrees of freedom through 1km-length fibers with >99.9% accuracy for over 1000s-duration. The high-fidelity performance enables efficient transmission of high-resolution video with several orders throughput enhancement by using compressive encoding, showing the feasibility of long-term high-fidelity spatial transmission. The proposed dynamic memory framework opens up a new paradigm for demixing through unstabilized diffuse media.\n\n# Results\n\n## Multi-scale memory dynamic-learning network\n\nWe experimented on an amplitude-to-amplitude optical setup (see Fig. 1 (a) and Supplementary Fig. 1). The input pattern coupled into the MMF is transformed into a complex distorted field at the distal end due to spatial mode dispersion. We calibrated and analyzed the variations of diverse 100m and 1km-length MMF transmission channels and observed slowly changing system drifting (see Supplementary Fig. 2). Deep learning approaches have been reported to solve this nonlinear transformation problem to retrieve the input image from output speckle, however, one generalized neural network will fail to precisely model the gradually varying MMF channel over a long time. In this work, we proposed a dynamic learning framework that adaptively tracks the optical propagation characteristics to achieve long-term image transmission with high accuracy through long MMFs. Instead of training a fixed and generalized neural network, we designed a compact network that generalizes well on short-term transmission. The MMDN model will be dynamically updated by online training on the unlabeled streaming data using predicted input images as labels, hence working in a self-supervised architecture. According to the calibration results in Supplementary Fig. 2, the MMF transmission channels could sustain nearly unchanged within a 10-second duration, which ensures the feasibility of the self-supervised dynamic updating strategy.\n\nBesides slow-varying system drift, we also witnessed intense jitter effects that will cause severe MMF channel deviations (illustrated in Supplementary Fig. 3). This physical prior knowledge inspires us to develop an ensemble framework of subnetworks which carry multi-scale memory of the system variations for the MMDN block. As shown in Fig. 1 (c), the output speckle image is fed into three networks, where S1 and S2 indicate two transmission models with different short-term memories, and L3 indicates one model with long-term memory. A grading module was additionally designed for confidence evaluation of expert subnetworks, allowing adaptive memory fusing to produce an optimized prediction that has good adaptability to both slow drifting and abrupt jitter effect. For continuous data transmission, the multi-scale models are self-supervised updated at a short interval (i.e., 5 seconds). For S1 and S2 that aim to carry short-term information, we introduced the forgetting mechanism by alternatively wiping its memory of current model and rebuilding it with only the latest predicted data at specific intervals alternatively, as depicted in Fig. 1 (b); while the L3 will always keep the memory of previous transmission characterizations during the update process. The proposed MMDN is supposed to show better performance in long-term data recovery through scattering MMFs, attributed to the enriched perspectives provided by the adaptively updated multi-timescale models.\n\n## Long-term spatial transmission through unstabilized MMFs\n\nWe evaluated the performance of the proposed MMDN for long-term spatial transmission through diffuse media by experimenting on 100m- and 1km-length MMFs placed on the optical table without vibration isolation. To verify the ability to transmit arbitrary spatial information, we showed reconstruction of random binary patterns with spatial degree-of-freedom of 16×16 and 32×32, as opposed to the specified images such as the MNIST dataset. We additionally reshaped the common grid pixel assignment to accommodate the round-shape property of the MMF entry, and proved slightly enhanced performance (see Supplementary Fig. 5). The output speckle patterns were captured by a camera at 100 fps. At the preparation stage of data transmission, a sequence of known patterns is transmitted, and the MMDN is statically trained on the initial instances. Once finished, the MMDN is ready for dynamic update to support continuous image transmission.\n\nIn Fig. 2, we show the transmission results for over 1000 seconds on four different settings. The static neural network (StaticNN) trained on the first 500-second data and tested on the following 500-second is taken as the baseline method. The MMDN was dynamically updated at each 5-second interval. Comparing the reconstructed accuracy averaged on each 5-second batch, we observed an obvious degradation after 200s using StaticNN, especially for 1km fibers; while MMDN achieved ~ 100% accuracy throughout the 1000s period. Although the increase of fiber distance makes its scattering channel vary more intensely, the dynamic learning ability of proposed MMDN allows it to precisely model the dynamics and adapt to the current state of the physical process. We also illustrated representative recovered spatial profiles and the averaged spatial distribution of transmission accuracy. For 1km transmission, MMDN enables < 0.1% error rate across the spatial position and the average accuracy of 99.97%, which is two orders improved than using StaticNN. For 100m transmission cases, MMDN even reduce the averaged error rate to 2e-6 throughout the transmission period. As a result, we demonstrated that MMDN can permit long-term spatial information transmission with high fidelity.\n\n## Multi-scale memory ensemble improves instability robustness\n\nThe dynamic learning strategy for MMF dynamics modeling intuitively raises a critical demand for accurate inference on current batch, so as to provide reliable training sets for the subsequent update. However, two main factors exist that could hinder its naïve implementation from practical usage. First of all, the inevitable inference error for previous batch induces a bias to the model update, which will accumulate and largely deteriorate the network effectiveness after a long period. Besides, the abrupt disturbances happen frequently for unstabilized long MMFs, resulting in significant transmission characteristics distinguishment even between adjacent batches. MMDN incorporates the physical prior inspired multi-scale memory mixture architecture, providing a solution for precise and robust modeling of system dynamics.\n\nWe next investigated the benefits of long and short-term memory ensemble network design. We chose two highly variable MMF channels including a 100m-length gradient-indexed MMF of 200 μm diameter (GI-200) and a 1km-length step-indexed MMF of 200 μm diameter (SI-200) for spatial transmission of 16×16 and 32×32-pixel random binary patterns. We analyzed the contributions of different subnetworks in MMDN by evaluating their intermediate prediction accuracy. For GI-200 case, as shown in Fig. 3 (a), we presented the average accuracy over a 1000s duration using S1, S2, L3 and the confidence-based ensemble network, and observed that the multi-scale model improved the accuracy by around 10-fold compared to the short-term models and the long-term model. Comparing the time-varying transmission error rate shown in Fig. 3 (b), the long-term model shows degraded performance especially at the 40-55s period, while the short-term models provide ‘wiser’ predictions and contribute to producing a good ensemble model. Similar comparisons in averaged transmission accuracy and error rate at each timestep are also presented for the SI-200 case (see Fig. 3 (c)(d)). In this experiment, the long-term model works better than short-term models for most of the time, as the magnified time clip within 40-45s, and the multi-scale model outperforms all other single-scale models throughout the period. The above results verified that using a mixture of expert networks with different memory scales will enrich perspectives of the dynamic scattering channel by learning from the same data, and overcome diverse variations in MMFs to achieve spatial transmission with high accuracy over long periods.\n\n## Scalability and generalization of MMDN\n\nHaving validated long-term high-fidelity transmission of generalized patterns, we also noted that the MMDN is well applicable to transmit specific types of natural images. In Fig. 4 (a,b), we show a set of recovered hand-written digits and fashion symbols transmitted through a 1km-long fiber. The input images of 28×28 pixels are upsampled to be 32×32 and binarized by the greyscale threshold of 0.5. The initial MMDN model trained on 20,000 paired data is then dynamically updated to support continuous image transmission of over 1000s. To evaluate the quality of reconstructed images, we quantitively compared the SSIM and accuracy obtained using StaticNN and proposed MMDN. We observed nearly errorless transmission of both MNIST and fashion-MNIST datasets with MMDN during the whole period, and the SSIM is mostly above 0.99. Whereas, the static model will degrade in transmission accuracy and image similarity. This indicates the feasibility of image transmission in unstabilized scattering MMF using MMDN, laying the foundation for direct natural image transmission for remote imaging applications such as biological endoscopy.\n\nOne big concern of learning-based image reconstruction approach is whether the network is able to transfer to other unseen categories of images. To demonstrate the generalized performance of proposed network, we used the MMDN dynamically trained on Latin alphabet images for inference on the digit dataset (see Fig. 4 (c)) and measured the transmission accuracy (see Fig. 4 (d)). Examples of reconstructed input patterns right after the switch of image category as well as 10s and 150s after the switch are presented in Fig. 4 (e), respectively. We observed an average accuracy of 99.44% and good visual fidelity with a high SSIM of 0.978 even without fine-tuning the network (i.e., T = 0). The accuracy was further elevated up to 99.68% and the SSIM up to 0.989 after 2 batches (i.e., T = 10s) attributed to the dynamic update ability of MMDN, and the high accuracy could be well retained during the following 150s. This experiment demonstrates that the proposed MMDN has good generalization performance for image transmission.\n\n## Long-term high-throughput video transmission\n\nWe further propose a practical high-throughput video transmission protocol via unstabilized long MMFs, as shown in Fig. 5 (a). High-resolution video streams are compressively encoded into bit streams and spatially arranged to form a sequence of spatial-multiplexing-coded patterns. The spatial-multiplexed MMF setup can be used to support up to thousands of independent communication channels transmitting in parallel, and the proposed MMDN addresses the encoded spatial pattern recovery from recorded speckle images with nearly 100% accuracy to guarantee high-quality video decoding.\n\nWe experimented on the 1km transmission of a 6-minute full-color video of 480 × 480-pixel resolution and 20 fps. The video was encoded in the form of H.264 with a compression ratio of 1.39‰ and then converted into 32×32-pixel spatially multiplexed patterns. The proof-of-concept MMF setup with 150 fps acquisition rate guarantees adequate bandwidth for real-time transmission of encoded video. We evaluated the transmission accuracy of the spatial-multiplexed encoded signals in Fig. 5 (b) and the visual fidelity of decoded video frames using SSIM metric in Fig. 5 (c). When using the static network for image recovery, we observed that a slight signal accuracy deterioration of less than 2% starting at 100s would cause a significant drop in decoded video quality, leading to the SSIM of recovered video frames drastically dropping below 0.4. Noticeably, even when the transmission performance can be restored to good accuracy afterward, such as the 160-180s period as highlighted with the asterisk in Fig. 4 (b), the video decoding corruption still remains irreparable. By comparison, our proposed MMDN ensures high accuracy spatial transmission over long-term, hence can be incorporated into the highly-compressed encoded video transmission protocol to achieve high-quality image recovery with the SSIMs all above 0.995 within the 6-minute duration. Example recovered frames within 93-99s period are illustrated in Fig. 5 (d) to visualize the decoding corruption caused by the slight transmission error using static network. The results validated the superiority in decoding accuracy using MMDN for encoded video transmission, which offered over 700-fold efficiency enhancement compared to the plain coded video transmission scheme (see Supplementary Fig. 6).\n\n# Discussion\n\nSpatial reconstruction from diffusive MMF transmission is a challenging task, and has so far been limited to short-distance fibers and faced the tradeoff between high accuracy and long-time generalization. In the work, we described the MMDN, a multi-scale dynamic learning approach that can achieve >99.9% accuracy of long-time image transmission through unstabilized 1km MMF channels. The MMDN technique is developed based on the physically informed model of the diffusive MMF system that fully describes the long-term drifting and short-term abruption effects, therefore enabling good accommodation with the dynamics of the system characteristics. We compared MMDN with previous approaches in terms of time duration, reconstruction quality, and transmission distance, etc., and demonstrated a comprehensive improvement of our approach (see Supplementary Fig. 7). In particular, the high-fidelity long-term transmission performance of MMDN will allow for efficient video transmission in a highly compressed scheme. The superior decoding capability will also facilitate practical applications such as minimally invasive endoscopic imaging, spatial-multiplexed optical communication, and optical security taking diffusive channel as the decoding medium.\n\n# Methods\n\n## Experimental set-up\n\nThe optical setup for image transmission through the MMFs is described in Supplementary Fig. 1. The continuous-wave laser beam at wavelength 561nm is expanded by a pair of lenses ($f_{1}$ = 10 mm, $f_{2}$ = 100mm) and projected onto the SLM (V-7001) for binary amplitude modulation. The spatial modulated optical field is coupled by an objective lens (Nikon, 20X, 0.25NA) into the input facet of the MMF. At the output of the MMF, the speckle field at the distal end is magnified by another objective (Nikon, 20X, 0.25NA) and imaged by the CMOS (MER2-230-167U3M).\n\n## Stability analysis of MMF channel\n\nWe adopted three metrics to evaluate the transmission channel stability over a large variety of MMFs, as summarized in Supplementary Fig. 2. The first metric measures the SSIM of a sequence of output speckle patterns to the reference pattern captured at $T=0$ while transmission a fixed image. The SSIM calculation can be expressed as\n\n$$\\begin{array}{c}SSIM=\\frac{\\left(2*{\\mu }_{x}*{\\\\mu }_{y}+{C}_{1}\\\\right)*\\left(2*{\\\\sigma }_{xy}+{C}_{2}\\\\right)}{\\left({\\\\mu }_{x}^{2}+{\\\\mu }_{y}^{2}+{C}_{1}\\\\right)*\\left({\\\\sigma }_{x}^{2}+{\\\\sigma }_{y}^{2}+{C}_{2}\\\\right)}. \\#(1.)\\end{array}$$\n\nHere, $x$ and $y$ are the two images being compared, ${\\\\mu }_{x}$, ${\\\\mu }_{y}$ and ${\\\\sigma }_{x}^{2}$, ${\\\\sigma }_{y}^{2}$ are the mean values and variations of images $x$ and $y$, and ${\\\\sigma }_{xy}$ is the covariance between two images. The ${C}_{1}$ and ${C}_{2}$ are two constants used to prevent the denominator from becoming zero or the result becoming infinite.\n\nThe second metric measures the Helinger distance of the speckle energy distribution of two batches. The speckle energy distribution of each batch is obtained by summing up all speckle images in that batch, and one batch consists of 500 output speckle images captured within 5 seconds. For two discrete energy distributions $P=({p}_{1},{p}_{2}\\dots ,{p}_{n})$ and $Q=({q}_{1},{q}_{2}\\dots ,{q}_{n})$, $n$ is the total number of pixels in a single speckle image, the Hellinger distance can be calculated as\n\n$$\\begin{array}{c}{H}^{2}\\left(P,Q\\right)=\\frac{1}{2}\\sum _{i=0}^{n}{\\left(\\sqrt{{q}_{i}}-\\sqrt{{p}_{i}}\\right)}^{2}. \\#(2.)\\end{array}$$\n\nThe third metric computes the pixel-wise accuracy of recovered image at each time point, by using an approximate reconstruction algorithm termed real-value inverse transmission matrix (RVITM) [3]. The test image is transmitted right after the approximal transmission matrix is calibrated. The accuracy for each recovered image is the percentage of mis-distinguished pixels to the full number of pixels.\n\n## Data preparation\n\nOur research employed arbitrary random binary images, as well as natural scene images including the Fashion-MNIST dataset, Latin letters from the E-MNIST dataset, and handwritten digitals from the MNIST dataset. The input images tested in the experiments are of 16×16-pixel and 32×32-pixel resolution. According to the maximum number of spatial modes that is allowed to transmit through the MMF, it is theoretically possible to input images of larger pixel resolution. We used a binary SLM as the amplitude modulator to encode the spatial information, and the output speckles are captured by the monochromatic CMOS. To reduce computational complexity, we down-sampled the speckle images to 100×100-pixel and 150×150-pixel for reconstructing input patterns of 16×16-pixel and 32×32-pixel, respectively.\n\n## Neural network architecture\n\nWe designed an ensemble network consisting of three sub-networks with the same structure but updated differently over time. Each subnetwork is a convolutional neural network consisting of three convolutional layers and one fully-connected layer. Each convolution layer is followed by Dropout, Batch normalization, and ReLu activation. A sigmoid activation function is applied to the output layer. We employed cross-entropy as the loss function, and trained the networks with the AdaDelta optimizer at a learning rate of 0.1. The network training was executed on a workstation equipped with NVidia RTX3090 GPU.\n\n## Confidence-based ensemble algorithm\n\nEach subnetwork of the ensemble network calculates the average confidence level of one predicted instance as:\n\n$$\\begin{array}{c}c=\\frac{1}{N}\\sum _{i=1}^{N}\\left(\\left|{P}_{i} -0.5\\right|+0.5\\right) ,\\#(3.)\\end{array}$$\n\nwhere ${P}_{i}$ represents the predicted value of pixel $i$ from the subnetwork, which is binarized to be either 0 or 1, and $N$ is the spatial resolution of the input patterns. The confidence-based weight of each subnetwork is defined as:\n\n$$\\begin{array}{c}{w}_{k}=\\text{exp}\\left(\\frac{1-{c}_{k}}{\\left(1-{c}_{1}\\right)+\\left(1-{c}_{2}\\right)+\\left(1-{c}_{3}\\right)}\\right). \\#(4.)\\end{array}$$\n\nThe final ensemble prediction is the weighted summation of predictions from three subnetworks:\n\n$$\\begin{array}{c}P=\\frac{{w}_{1}*{p}_{1}+{w}_{2}*{p}_{2}+{w}_{3}*{p}_{3}}{{w}_{1}+{w}_{2}+{w}_{3}}. \\#(5.)\\end{array}$$\n\n# References\n\n1. Richardson, David J., John M. Fini, and Lynn E. Nelson. \"Space-division multiplexing in optical fibres.\" *Nature photonics* 7.5 (2013): 354–362.\n2. Caramazza, Piergiorgio, et al. \"Transmission of natural scene images through a multimode fibre.\" *Nature communications* 10.1 (2019): 2029.\n3. Zhao, Tianrui, et al. \"Seeing through multimode fibers with real-valued intensity transmission matrices.\" *Optics Express* 28.14 (2020): 20978–20991.\n4. Fan, Weiru, et al. “High-Fidelity Image Reconstruction through Multimode Fiber via Polarization‐Enhanced Parametric Speckle Imaging.” *Laser & Photonics Reviews* 15.5 (2021): 2000376.\n5. Li, Shuhui, et al. \"Compressively sampling the optical transmission matrix of a multimode fibre.\" *Light: science & applications* 10.1 (2021): 88.\n6. Bianchi, Silvio, and Roberto Di Leonardo. \"A multi-mode fiber probe for holographic micromanipulation and microscopy.\" *Lab on a Chip* 12.3 (2012): 635–639.\n7. Turtaev, Sergey, et al. \"High-fidelity multimode fibre-based endoscopy for deep brain in vivo imaging.\" *Light: Science & Applications* 7.1 (2018): 92.\n8. Choi, Youngwoon, et al. \"Scanner-free and wide-field endoscopic imaging by using a single multimode optical fiber.\" *Physical review letters* 109.20 (2012): 203901.\n9. Plöschner, Martin, Tomáš Tyc, and Tomáš Čižmár. \"Seeing through chaos in multimode fibres.\" *Nature Photonics* 9.8 (2015): 529–535.\n10. Turtaev, Sergey, et al. \"High-fidelity multimode fibre-based endoscopy for deep brain in vivo imaging.\" *Light: Science & Applications* 7.1 (2018): 92.\n11. Vasquez-Lopez, Sebastian A., et al. \"Subcellular spatial resolution achieved for deep-brain imaging in vivo using a minimally invasive multimode fiber.\" *Light: science & applications* 7.1 (2018): 110.\n12. Richardson, David J., John M. Fini, and Lynn E. Nelson. \"Space-division multiplexing in optical fibres.\" *Nature photonics* 7.5 (2013): 354–362.\n13. Li, Wei, et al. \"High-rate quantum key distribution exceeding 110 Mb s–1.\" *Nature Photonics* (2023): 1–6.\n14. Ding, Yunhong, et al. \"High-dimensional quantum key distribution based on multicore fiber using silicon photonic integrated circuits.\" *npj Quantum Information* 3.1 (2017): 25.\n15. Zhou, Yiyu, et al. \"High-fidelity spatial mode transmission through a 1-km-long multimode fiber via vectorial time reversal.\" *Nature communications* 12.1 (2021): 1866.\n16. Popoff, S. M., et al. \"Controlling light through optical disordered media: transmission matrix approach.\" *New Journal of Physics* 13.12 (2011): 123021.\n17. Čižmár, Tomáš, and Kishan Dholakia. \"Exploiting multimode waveguides for pure fibre-based imaging.\" *Nature communications* 3.1 (2012): 1027.\n18. Tahir, Waleed, Hao Wang, and Lei Tian. \"Adaptive 3D descattering with a dynamic synthesis network.\" *Light: Science & Applications* 11.1 (2022): 42.\n19. Rahmani, Babak, et al. \"Actor neural networks for the robust control of partially measured nonlinear systems showcased for image propagation through diffuse media.\" *Nature Machine Intelligence* 2.7 (2020): 403–410.\n20. Fan, Pengfei, et al. \"Learning enabled continuous transmission of spatially distributed information through multimode fibers.\" *Laser & Photonics Reviews* 15.4 (2021): 2000348.\n21. Borhani, Navid, et al. \"Learning to see through multimode fibers.\" *Optica* 5.8 (2018): 960–966.\n22. Resisi, Shachar, Sebastien M. Popoff, and Yaron Bromberg. \"Image transmission through a dynamically perturbed multimode fiber by deep learning.\" *Laser & Photonics Reviews* 15.10 (2021): 2000553.\n23. Li, Yunzhe, Yujia Xue, and Lei Tian. \"Deep speckle correlation: a deep learning approach toward scalable imaging through scattering media.\" *Optica* 5.10 (2018): 1181–1190.\n24. Rahmani, Babak, et al. \"Multimode optical fiber transmission with a deep learning network.\" *Light: science & applications* 7.1 (2018): 69.\n25. Tahir, Waleed, Hao Wang, and Lei Tian. \"Adaptive 3D descattering with a dynamic synthesis network.\" *Light: Science & Applications* 11.1 (2022): 42.\n26. Gupta, Harshit, et al. \"CNN-based projected gradient descent for consistent CT image reconstruction.\" *IEEE transactions on medical imaging* 37.6 (2018): 1440–1453.\n27. Li, Fengqiang, et al. “Compressive ghost imaging through scattering media with deep learning.” *Optics Express* 28.12 (2020): 17395–17408.\n28. Sun, Yu, Zhihao Xia, and Ulugbek S. Kamilov. \"Efficient and accurate inversion of multiple scattering with deep learning.\" *Optics express* 26.11 (2018): 14678–14688.\n29. Weigert, Martin, et al. \"Content-aware image restoration: pushing the limits of fluorescence microscopy.\" *Nature methods* 15.12 (2018): 1090–1097.\n30. Agostinelli, Forest, Michael R. Anderson, and Honglak Lee. \"Adaptive multi-column deep neural networks with application to robust image denoising.\" *Advances in neural information processing systems* 26 (2013).\n31. Choi, Joon Hee, Omar A. Elgendy, and Stanley H. Chan. \"Optimal combination of image denoisers.\" *IEEE Transactions on Image Processing* 28.8 (2019): 4016–4031.\n32. Deng, Mo, et al. \"Learning to synthesize: robust phase retrieval at low photon counts.\" *Light: Science & Applications* 9.1 (2020): 36.\n\n# Supplementary Files\n\n- [SupplementaryMovie1.mp4](https://assets-eu.researchsquare.com/files/rs-2858332/v1/de0a333c080170c46af982d1.mp4) \n Demo of continuous transmission of generalized patterns via unstabilized long MMFs\n\n- [SupplementaryMovie2.mp4](https://assets-eu.researchsquare.com/files/rs-2858332/v1/f6c3da5aa28aafcea10a41f6.mp4) \n Demo of continuous transmission of hand-written letters and fashion images via 1km-length MMF\n\n- [SupplementaryMovie3.mp4](https://assets-eu.researchsquare.com/files/rs-2858332/v1/fb2fc24fb5751de5408096da.mp4) \n Demo of high-throughput encoded video transmission via unstabilized 1km-length MMF\n\n- [MMDNSupplementary.docx](https://assets-eu.researchsquare.com/files/rs-2858332/v1/447f5fd71ced30673f18b34f.docx)"} {"paper_id": "prb65", "title": "Broadband Thermal Imaging using Meta-Optics", "text": "Broadband Thermal Imaging using Meta-Optics\n\nArka Majumdar\narka@uw.edu\n\nUniversity of Washington https://orcid.org/0000-0003-0917-590X\nLuocheng Huang\nUniversity of Washington\nZheyi Han\nUniversity of Washington\nAnna Wirth-Singh\nUniversity of Washington\nVishwanath Saragadam\nRice University https://orcid.org/0000-0001-8028-7520\nSaswata Mukherjee\nUniversity of Washington\nJohannes E Fröch\nUniversity of Washington\nJoshua Rollag\nAir Force Research Laboratory\nRicky Gibson\nAir Force Research Laboratory\nJoshua Hendrickson\nAir Force Research Laboratory https://orcid.org/0000-0002-5342-0346\nPhilip Hon\nNG Next, Northrop Grumman Corporation\nOrrin Kigner\nNorthrop Grumman Corporation https://orcid.org/0000-0002-0701-3002\nZachary Koppens\nNorthrop Grumman Corporation\nKarl Böhringer\nUniversity of Washington https://orcid.org/0000-0002-9428-2648\nAshok Veeraraghavan\nRice University https://orcid.org/0000-0001-5043-7460\nArticle\n\nKeywords: LWIR, inverse design, meta-optic, metasurface, broadband\n\nPosted Date: July 26th, 2023\n\nDOI: https://doi.org/10.21203/rs.3.rs-3186927/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nAdditional Declarations: There is NO Competing Interest.\n\nVersion of Record: A version of this preprint was published at Nature Communications on February 23rd, 2024. See the published version at https://doi.org/10.1038/s41467-024-45904-w.\nBroadband Thermal Imaging using Meta-Optics\n\nLuocheng Huang¹, Zheyi Han¹, Anna Wirth-Singh², Vishwanath Saragadam³, Saswata Mukherjee¹, Johannes E. Fröch¹,², Joshua Rollag⁴,⁵, Ricky Gibson⁵, Joshua R. Hendrickson⁵, Phillip W.C. Hon⁶, Orrin Kigner⁶, Zachary Coppens⁷, Karl F. Böhringer¹,⁸, Ashok Veeraraghavan³ and Arka Majumdar¹,²*\n\n¹Department of Electrical and Computer Engineering, University of Washington, Seattle, WA, USA.\n²Department of Physics, University of Washington, Seattle, WA, USA.\n³Department of Electrical Engineering, Rice University, Houston, TX, USA.\n⁴KBR, Inc., 3725 Pentagon Blvd., Suite 210 Beavercreek, OH, USA.\n⁵Sensors Directorate, Air Force Research Laboratory, 2241 Avionics Circle, Wright-Patterson AFB, OH, USA.\n⁶NG Next, Northrop Grumman Corporation, 1 Space Park Drive, Redondo Beach, CA, USA.\n⁷CFD Research Corporation, Huntsville, AL, USA.\n⁸Institute for Nano-Engineered Systems, University of Washington, Seattle, WA, USA.\n\n*Corresponding author(s). E-mail(s): arka@uw.edu;\n\nAbstract\nSubwavelength diffractive optics known as meta-optics have demonstrated the potential to significantly miniaturize imaging systems. However, despite impressive demonstrations, most meta-optical imaging systems suffer from strong chromatic aberrations, limiting their\nutilities. Here, we employ inverse-design to create broadband meta-optics operating in the long-wave infrared (LWIR) regime (8-12 \\( \\mu \\)m). Via a deep-learning assisted multi-scale differentiable framework that links meta-atoms to the phase, we maximize the wavelength-averaged volume under the modulation transfer function (MTF) of the meta-optics. Our design framework merges local phase-engineering via meta-atoms and global engineering of the scatterer within a single pipeline. We corroborate our design by fabricating and experimentally characterizing all-silicon LWIR meta-optics. Our engineered meta-optic is complemented by a simple computational backend that dramatically improves the quality of the captured image. We experimentally demonstrate a six-fold improvement of the wavelength-averaged Strehl ratio over the traditional hyperboloid metalens for broadband imaging.\n\nKeywords: LWIR, inverse design, meta-optic, metasurface, broadband\n\n1 Introduction\n\nLong-wavelength infrared (LWIR) imaging is a critical key technology for non-contact thermography, long-range imaging, and remote sensing, with applications spanning consumer electronics to defense [1]. High resolution imaging in LWIR typically requires bulky, and precisely engineered refractive surfaces, which ultimately add to the overall volume and weight of the imaging system, especially for high numerical aperture (NA) optics. To reduce the size and weight of LWIR imagers, diffractive optical elements such as multi-level diffractive lenses (MDL)[2] have been used as an alternative to traditional refractive optics. However, the use of MDLs has been limited by the complexity of the multi-layer fabrication and the large periodicity, resulting in higher order diffraction. Sub-wavelength diffractive optics, also known as meta-optics, have recently generated strong interest to spatially modulate the phase, amplitude, and polarization of the incident wavefront. These consist of scatterers, which are placed on a sub-wavelength periodic lattice to avoid any higher order diffraction, whereas the active layer thickness of the device corresponds to the height of the scatterers [3–15]. Due to the drastic thickness and weight reduction in meta-optics compared to refractive lenses, LWIR meta-optical imaging under ambient light conditions have been recently reported [16–18]. However, until this point, the captured image quality remained relatively poor compared to refractive lenses, primarily due to strong chromatic aberrations.\n\nSome drawbacks of meta-optics are inherited from their diffractive counterparts, the most significant one being their axial chromatic aberration. This happens because the phase wrapping condition for different wavelengths is met at different radii [13, 19]. The dispersion engineering approach can ameliorate this axial chromatic aberration to some degree, but ultimately faces fundamental limitations explicitly set by the achievable group delay and group\ndelay dispersion [20] for large aperture meta-optics. To overcome this fundamental limitation and enhance the image quality, chromatic aberrations in a large-aperture meta-optics can be mitigated via computational imaging using forward designed meta-optics that exhibit extended depth of focus (EDOF) properties, as demonstrated in the visible regime[21, 22].\n\nHowever, for forward designed meta-optics an optical designer has to strongly rely on experience and intuition about the functionality of the meta-optics. As such, this method does not provide a clear path to further improve the imaging quality. Unlike forward design, inverse design approaches define the performance of the optical element via a figure of merit (FoM), and computationally optimize their structure or arrangement to maximize the respective FoM. The inverse design methodology has been very successful in creating non-intuitive yet functional meta-optics [23–25], including EDOF lenses for broadband imaging in the visible. A further refinement and extension of this approach is end-to-end design, where the meta-optics and computational backend are co-optimized with a FoM defined by the final image quality[26]. While such an approach takes the entire system into account, the downside is that we often lack the insight into how and why the optic performs well. This can be detrimental when translating designs from the visible domain (with ample training data) to the thermal domain (with paucity of training data). As such, a new design paradigm is required for meta-optical imagers, which provides intuition on why such meta-optics can perform broadband imaging.\n\nIn this paper, we report a 1 cm (\\( \\sim 1000\\lambda \\)) aperture, f/1 (numerical aperture (NA): 0.45) broadband polarization-insensitive LWIR meta-optics, designed by a multi-scale optimization technique that maximizes the wavelength-averaged volume under the modulation transfer function (MTF) of the meta-optic. This method is “multi-scale” as distinct computational methods are used to calculate the electric fields at different length scales. The meta-optics are implemented in an all-silicon platform and we demonstrate that the captured images exhibit superior performance over traditional hyperboloid metalens. Unlike previous works, which relied either on local engineering of meta-atoms (dispersion engineering) or global engineering of the phase-mask, our optimization technique employs both meta-atom and phase-mask engineering. We show that such an extended approach clearly outperforms a phase-mask engineering only approach.\n\n2 Results\n\n2.1 Inverse Design Framework\n\nThe key to achieve meta-optical broadband LWIR imaging is a fully-differentiable inverse design framework that optimizes the binary structures (i.e., binary permittivity distribution) of the meta-atoms to achieve focusing of the desired wavelengths (**Fig. 1**(a)). However, designing a large-area (\\( \\sim 10^3\\lambda \\)) meta-optic is a computationally prohibitive problem, and full-wave simulation is not possible. Therefore, phase-mask optimization is generally used, but\nthe scatterer-to-phase mapping on a sub-wavelength scale is not differentiable and a look-up-table based approach does not work for such an optimization methodology. In the past, polynomial proxy functions have been employed to connect scatterers to the corresponding phase [26], but were limited to only a monotonic relation. However, for broadband operations meta-atoms with a large phase diversity with multiple phase wrappings are required but suffer from multiple resonances at various wavelengths.\n\nWe solve this problem by utilizing a deep neural network (DNN)-based surrogate model, that maps the geometrical parameters (\\( \\vec{p} \\)) of the meta-atom to its complex transmission coefficient \\( \\hat{\\mathbf{E}}(\\vec{p}, \\lambda) \\). The utilization of DNNs enable modeling highly complex functions, which are well suited for broadband meta-optics. To emphasize this point, we compare meta-atoms with different degrees of parameterization: the “simple” scatterers are defined by one design parameter (the width of the pillar), whereas the “complex” scatterers have three parameters, see Fig. 1(b). For each type of meta-atom, we sampled the parameters \\( \\vec{p} \\) uniformly for each feature dimension and simulated it using rigorous coupled wave analysis (RCWA) [27], across different wavelengths \\( \\lambda \\). The simulated meta-atom library is then taken as the training data set for the DNN that maps the parameterized features to the phase modulation. The RCWA simulations and the DNN fitting are pre-computed before the optimization loop, shown in Fig. 1(c). Although we are currently limited to parameterized meta-atoms, with the rapid progress of machine learning-enabled meta-optics design, we anticipate voxel-level meta-atom engineering will be possible in the near future. Also, our design currently relies on the local phase approximation, which is known to provide lower efficiency for meta-optics. However, recently a physics-inspired neural network has been used to design meta-optics without making such approximation and can be readily adapted for the scatterer-to-field mapping [28].\n\nWe define the FoM by computing the normalized MTFs first as \\( \\hat{M}(k_x, k_y; \\lambda, \\theta) \\), where \\( k_x, k_y \\) are defined as the spatial frequencies in the x and y direction, \\( \\lambda \\) is the optical wavelength, and \\( \\theta \\) signifies the incident angle (more details in Methods). The modified Strehl Ratio \\( \\mathbf{S} \\) can then be calculated using the following expression:\n\n\\[\n\\mathbf{S}(\\lambda, \\theta) = \\int_{-k_{y1}}^{k_{y1}} \\int_{-k_{x1}}^{k_{x1}} \\hat{M} (k_x, k_y; \\lambda, \\theta) \\, dk_x dk_y \\\\\n= \\sum_i \\sum_j \\hat{M} (k_x(i), k_y(j); \\lambda, \\theta) \\, \\Delta k_x \\Delta k_y\n\\]\n\nHere, \\( k_{x1} \\) and \\( k_{y1} \\) denote the cutoff spatial frequencies in the x and y direction. Using the modified Strehl Ratio, the FoM \\( \\mathbf{F} \\) is computed as:\n\n\\[\n\\mathbf{F} = \\log(\\prod_i \\prod_j S(\\lambda_i, \\theta_j))\n\\]\nFig. 1 Design methodology to create the broadband LWIR meta-optics. (a) Our objective is a LWIR meta-optic that focuses broadband light at the same focal plane. (b) Parameterization of the “complex” (red) and the “simple” (blue) scatterers. For the complex scatterers, three variable parameters control the binary profile, namely, \\( \\mathbf{p}_0, \\mathbf{p}_1, \\) and \\( \\mathbf{p}_2 \\). This method of parameterization ensures 4-fold symmetry of the geometry, thus ensuring polarization-insensitivity. The height \\( h \\) is kept constant at 10\\( \\mu \\)m. The meta-atoms sit on a Manhattan grid with a periodicity \\( \\Lambda \\) set to 4\\( \\mu \\)m. (c) Block diagram of the optimization routine. (d) The simulated Strehl ratio of the “simple”, “complex”, and hyperboloid meta-optic.\n\nThis FoM can be interpreted as the wavelength and incidence angle-averaged volume under the MTF surface, and we therefore term this optimization routine as “MTF engineering”. We emphasize that our FoM is maximized when all individual \\( S(\\lambda_i, \\theta_j) \\) are identical, thus constraining our meta-optics to have a uniform performance for the specified wavelengths without explicitly defining uniformity as an optimization criteria. Since the entirety of the forward computation of the FoM is implemented using differentiable operations, the gradient of the FoM with respect to the geometry parameters, i.e. \\( \\partial S / \\partial \\vec{p} \\), can be readily obtained using automatic differentiation through chain rule in the direction indicated by the red arrows in Fig. 1(b). A stochastic gradient descent algorithm then optimizes the structural parameters \\( \\vec{p} \\). The optimization routine halts when the value of FoM converges, yielding the final meta-optic design.\n\n2.2 Meta-optics Design\n\nUsing the “MTF engineering” framework, we designed the broadband LWIR meta-optics. We opted for an all-silicon platform, which is composed of silicon pillars on a silicon substrate, to simplify the fabrication process. We note that while silicon does absorb some of the LWIR light, we still expect about 80% light transmission.\nIn this study, we designed two different broadband meta-optics, each with a unique scatterer archetype shown in Fig. 1(b). Both archetypes were parameterized to ensure fourfold symmetry, which leads to polarization insensitivity. Additionally, we designed a hyperboloid metalens, based on a forward design approach [22], possessing similar height and periodicity, to serve as a baseline for comparison. All designed meta-optics have a nominal focal length of 1 cm and a numerical aperture of 0.45. In our simulations, the optimized broadband meta-optics displayed significantly larger wavelength-averaged Strehl Ratios—0.045 for the meta-optics with “complex” scatterers and 0.018 for those with “simple” scatterers, as compared to 0.0075 for the forward-designed hyperboloid metalens. The simulations were, however, limited to 8 optimized wavelengths spanning from 8 to 12 μm due to memory constraints. Fig. 1(d) depicts the simulated Strehl ratios of the optics described above in relation to the input wavelength. For these simulations, individual meta-atoms were simulated using RCWA, while DNN mapping was utilized solely for optimization. To mimic fabrication imperfections, we introduced normally distributed perturbation into each meta-atom’s design parameters. Remarkably, the complex meta-optic design yielded Strehl ratios at eight sampled wavelengths that are comparable to the Strehl ratio at a single operational wavelength of the hyperboloid metalens.\n\nAlthough the spectral regions between the sampled wavelengths exhibit relatively lower Strehl ratios compared to the peak values, these ratios for the non-sampled wavelengths still remain significantly larger than those of the hyperboloid lens at the same wavelengths. As such, when averaged over all the wavelengths of interest, we still obtain a six-fold improvement for the average Strehl ratio. Our experimental results demonstrate that, despite such polychromatic behavior, it is possible to capture images under broadband ambient thermal radiation. This highlights the practicality and adaptability of our broadband meta-optic designs in real-world scenarios.\n\n2.3 Fabrication\n\nWe fabricated the LWIR meta-optics in an all-silicon platform, with a set of devices shown in Fig. 2(a). We pattern the Si wafer with laser direct-write lithography and etch the patterns using deep reactive ion etching (details in Methods). We note that patterning can also be accomplished with a mask aligner – therefore our all-silicon platform can be adapted to large scale foundry processes. Scanning electron microscope images of the fabricated complex and simple meta-optics are depicted in Fig. 2(b) and 2(c), respectively.\n\n2.4 Imaging\n\nWe first characterized the PSF of the fabricated lenses (result in Supplementary materials), and observed less variation of the PSFs across the LWIR range as expected. To conclusively demonstrate that the MTF-engineered optics deliver superior imaging quality compared to the forward-designed metalens,\nFig. 2 Images of the fabricated meta-optics: (a) Camera image of a fabricated wafer with several meta-optics. SEM images of the meta-optics with (b) complex scatterers and (c) simple scatterers.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Hyperboloid MetalensMTF Engineered (simple scatterers)MTF Engineered (complex scatterers)
(a)(b)(c)
(d)(e)(f)
\n\nFig. 3 Broadband imaging results in the lab (after computation), comparing the hyperboloid metalens (a, d), MTF engineered meta-optic with simple scatterers (b, e), and MTF engineered meta-optic with complex scatterers (c, f). For each subfigure the imaging results are shown without a filter (top), with a \\(10 \\pm 0.25\\) μm bandpass filter (bottom left), and with a \\(12 \\pm 0.25\\) μm bandpass (bottom right). The scale bar is 0.56 mm. Imaging results using two different targets, namely are a modified USAF 1951 pattern (top) and a picture of a husky (bottom) are shown.\nwe evaluated their respective imaging performance under controlled conditions (see Methods for details). As illustrated in Fig. 3, the images captured using the MTF-engineered meta-optic with complex scatterers exhibit the highest level of clarity and detail. Stripe elements of an imaging target can be clearly distinguished and well separated, emphasizing the overall crispness of the images.\n\nTo highlight the broadband capability of the MTF-engineered meta-optics, we captured images using both 10 \\( \\mu \\)m and 12 \\( \\mu \\)m bandpass filters (each with a linewidth of 500nm). We ensured a consistent distance between the meta-optics and the imaging sensor, maintaining a nominal operating wavelength of 11 \\( \\mu \\)m. The resultant imaging outputs, which are presented without any denoising, are displayed at the bottom of each sub-figure in Fig. 3. Notably, the MTF-engineered meta-optic with complex scatterers outperforms both the simple scatterers and the forward-designed optics for both the line and husky targets. Additionally, the MTF-engineered meta-optic with simple scatterers demonstrates superior performance over the forward-designed hyperboloid metalens, as evidenced by a clearer image and higher peak signal-to-noise ratio (PSNR) for both patterns in both the 10 \\( \\mu \\)m and 12 \\( \\mu \\)m cases. A comprehensive list of PSNR values can be found in the supplementary information.\n\nTo further emphasize the capabilities of the MTF-engineered LWIR meta-optics, we performed imaging “in the wild” under both indoor and outdoor ambient daylight conditions, shown in Fig. 4. In each case, we captured a single image using a FLIR A65 sensor, and performed a numerical deconvolution (details in the Methods and supplementary information). The MTF-engineered meta-optic with complex scatterers and forward-designed meta-optics were tested against a refractive lens for the ambient imaging. First, we imaged a truck parked outdoors shown in Fig. 4(a). The vehicle details are clearly visible such as the front grill, as well as background details, such as the windows on the top right corner of the image, and the stairs on the left side of the image captured using MTF-engineered meta-optic. In contrast, the hyperboloid image suffers from strong glowing artifacts in the center and fails to recover sharp details. Fig. 4(b) shows images of a parked car. As with the previous example, the details are clearly visible, including the tires on the car, and the branches of the tree in the background with the MTF-engineered lens. Fig. 4(c) shows image of a person with hands stretched out. The difference between MTF-engineered lens and hyperboloid metalens is distinctly visible here. The sharp image features are clearly visible in the MTF-engineered lens, including variable heat patterns on the shirt. In contrast, the image formed by the hyperboloid lens is noisy with no clear features on the person.\n\n3 Discussion\n\nIn this work, we have devised an inverse design methodology for broadband imaging meta-optics, guided by readily translatable, intuitive, and universal objective function, given by the volume of a multi-chromatic MTF surface.\nFig. 4 LWIR imaging “in the wild”. Three scenes were imaged using the refractive LWIR lens (left), the hyperboloid metalens (middle), and the MTF engineered meta-optic with complex scatterers (right). Scenes (a) and (b) were captured outdoors on a sunny day while (c) was captured indoors.\n\nUtilizing this MTF-engineering approach, we achieve a sophisticated, yet easily fabricable, large-aperture, broadband LWIR meta-optic, suitable for “in the wild” imaging under ambient temperature conditions. We have experimentally verified this framework and demonstrated polarization-insensitive broadband LWIR meta-optics with a diameter of 1 cm and NA of 0.45. While previous works based on forward designed LWIR meta-optics have demonstrated imaging capabilities [22], they fell short in resolving fine features due to strong chromatic aberrations. In contrast, our MTF-engineered meta-optics show significantly improved performance over a broadband spectral range, as well as narrowband imaging capabilities for wavelengths outside the center wavelength.\n\nWe further elucidate, both in simulation and experiment, how a significant performance enhancement can be achieved for MTF-engineered meta-optics if we consider more structural degrees of freedom. Such complex parameterization of the meta-optics broadens the solution space during the optimization process, thereby increasing the likelihood of achieving an improved FoM. This provides a clear pathway for future designs to leverage a performance\nboost by employing a higher degree of parameterization for the meta-optic scatterer, combined with large-scale optimization of the meta-optic. We note that previous works primarily employed either meta-atom engineering or phase-mask optimization, often overlooking potential synergistic effects. We demonstrate unequivocally that by utilizing structural diversity along with global phase-mask engineering, a six-fold performance improvement can be achieved. However, a clear downside is that the sampling complexity increases exponentially with the number of structural parameters. Additionally, fabrication resolution requirements become more stringent with the increased complexity of the meta-atoms. Despite these challenges, they can potentially be overcome by using a more clever parameterization of the meta-atom, similar to what has been achieved in dispersion engineering approaches.\n\nOverall, the developed MTF-engineering framework provides a universal methodology for creating large-area broadband meta-optics. Our imaging and characterization results clearly demonstrate the advantages of employing the MTF-engineering methodology over the traditional forward design. We showcase that the MTF-engineered flat optics open a new avenue for miniaturizing LWIR imaging systems, with potential applications in unmanned aerial vehicles, thermal scopes, and perimeter security.\n\n4 Methods\n\n4.1 MTF Calculation\n\nEach meta-atom is assigned a position (x, y) on a Manhattan grid with a periodicity of \\( \\mathbf{\\Lambda} \\) and a height of \\( h \\), whose geometric parameters are \\( \\vec{p} \\). These geometric parameters are given random assigned initial values within the fabrication limited bounds. The spatial modulation of the meta-optic \\( \\hat{\\mathbf{E}}(x, y, \\lambda) \\) is calculated given the meta-atom position and the wavelengths of the incident fields. The spatial modulation is then multiplied by the incident field (planewave with incidence angle \\( \\theta \\)) and propagated to the sensor plane centered to the chief ray, using the shifted angular spectrum method [29]. The variable \\( I(x, y; \\lambda, \\theta) \\) represents the sampled intensities on the sensor plane given all permutations of the wavelengths and angles of incidence of the incident fields. This intensity is the point spread function (PSF) of the imaging system. The MTF (\\( M \\)) is computed from the PSF given by \\( \\mathbf{M}(k_x, k_y; \\lambda, \\theta) = |\\mathcal{F}(I(x, y; \\lambda, \\theta))| \\), where \\( \\mathcal{F} \\) is the Fourier transform. The diffraction limited MTFs are denoted as \\( D(k_x, k_y, \\lambda) \\). The normalized MTF is defined as \\( \\hat{M} = M(k_x, k_y, \\lambda)/D(k_x, k_y, \\lambda) \\).\n\n4.2 Optimization\n\nFor the design with the complex scatterer, we used 40 samples per feature dimension in \\( \\vec{p} \\) while keeping \\( h \\) constant at 10\\( \\mu \\)m. Combining with 101 samples of wavelengths \\( \\lambda \\), there are totally \\( 40^3 \\times 101 \\) RCWA simulations conducted for training of the DNN model. For the simple scatterer case, we sampled 1000\nvalues for the only structure variable \\( p_1 \\) and 101 wavelengths, also keeping \\( h \\) constant at 10\\( \\mu \\)m, resulting in \\( 1000 \\times 101 \\) training samples for the surrogate. For training the DNN surrogate model, the Adam optimizer is used with a learning rate of \\( 10^{-3} \\) for 1000 epochs. To span a diameter of 10 cm, a total of \\( 2500 \\times 2500 \\) meta-atoms are used with a periodicity of 10\\( \\mu \\)m. During optimization, a total of 13 samples of wavelengths are used uniformly spanning from 8\\( \\mu \\)m to 12\\( \\mu \\)m. We selected 0° and 10° to be the angles of incidence in our optimization.\n\nThe DNN surrogate model uses four layers of fully connected layers that have 256 units and hyperboloid tangent as the activation function for each layer. To ensure a differentiable mapping, the fitted surrogate model uses all differentiable operations.\n\nThe structure parameters \\( \\vec{p} \\) are assigned initial values within the fabrication limited bounds. There are two conditions for the optimization loop to halt: (1) \\( \\vec{p} \\) converges, i.e. \\( \\vec{p}_n - \\vec{p}_{n-1} < \\mathbf{T} \\), where \\( \\mathbf{T} \\) denotes a threshold, and \\( n \\) represents the iteration number; (2) the number iteration reaches a certain integer \\( N \\). When one halting conditions is met, the final meta-atom binary structure parameters are converted to GDSII files for fabrication.\n\n4.3 Characterization\n\nWe characterized the PSFs of the fabricated meta-optics using a confocal microscopy setup in the LWIR. In this configuration, a tunable, 8.23 - 10.93 \\( \\mu \\)m, quantum cascade laser (QCL) with 500 ns pulses and repetition rate of 100 kHz (Daylight Solutions 31090-CT) was incident on a Ge aspheric lens with focal length \\( f_1 = 20 \\) mm and NA of 0.63 (Edmund Optics #68-253). This lens focused the QCL onto a 30 \\( \\mu \\)m diameter pinhole (Thorlabs P30S) where approximately 30% of the incident power was transmitted. The QCL was then incident on the meta-optic, placed \\( 2f_{meta} + f_2 = 35 \\) mm from the pinhole. The beam was then collimated by a Ge aspheric lens with \\( f_2 = 15 \\) mm and NA of 0.83 (Edmund Optics #68-252) placed \\( f_{meta} + f_2 = 35 \\) mm after the meta-optic. The beam then traveled to a ZnSe plano-convex lens with \\( f_3 = 50.8 \\) mm which focused the beam onto the image plane. This ZnSe lens was created by Rocky Mountain Instrument Co. and had a custom coating covering the 3 – 12\\( \\mu \\)m range with a reflectivity \\( R_{avg} \\leq 5\\% \\). The image was captured on a strained layer superlattice (SLS) focal plane array (FPA) with a 15\\( \\mu \\)m pixel pitch and 640×512 pixels (FLIR A6751 SLS) cooled to 76 K. The camera acquisition time was 200 \\( \\mu s \\) to best fit the 14-bit dynamic range of the FPA and 100 frames were captured and averaged with background correction. The schematic of the setup and the component specifications are present in the supplement information. The measured PSFs are reported in the supplementary information.\n4.4 In-lab Imaging\n\nTo assess the improved imaging performance of the MTF-engineered meta-optics over the forward-designed metalens, we captured imaged under broadband illumination using black-body radiation from a hotplate with high-emissivity fiberglass tape heated to 150°C as the light source. Custom aluminum targets were made using laser cutting and finished with matte black paint to prevent reflections. These targets were placed in front of the hotplate, allowing patterned LWIR light to go through, creating contrast. A Boson 640 camera was placed on the imaging plane of the meta-optic in testing and sent the data to a PC for further post-processing, which included background subtracting, contrast stretching, and block-matching denoising. Through this predefined post-processing routine, we were able to improve the dynamic range and reduce microbolometer array artifacts.\n\n4.5 Solving the Deconvolution Inverse Problem\n\nFig. 4 shows images captured in the wild with our meta-optic. In each case, we deconvolved the measurements by solving an inverse problem using a data-free image prior. Each \\(640 \\times 512\\) image was modeled as output of an implicit neural representation (INR) [30, 31] \\(N_\\theta\\) with parameters \\(\\theta\\). INRs are continuous functions that map local coordinates (\\(x, y\\) for images) to a given output (image intensity). A unique property enabled by certain INRs, particularly ones equipped with a complex Gabor filter activation function, is the bias for images. This implies that the output tend to look more like images than noise. We leveraged this property to regularize the inverse problem. The specific inverse problem we solved is\n\n\\[\n\\min_{\\theta, K} \\sum_{n=1}^N \\sum_{m=1}^M \\|I_{obs}(m, n) - (K * N_\\theta)(m, n)\\|^2 + \\eta_{TV} TV(N_\\theta(m, n)),\n\\]\n\nwhere \\(I_{obs}\\) is the observed 2D image, \\(K\\) is the PSF of the optical system, \\(TV()\\) is the total variation loss function, and \\(\\eta_{TV}\\) is the weight for the total variation loss. We perform a semi-blind deconvolution where we initialize \\(K\\) to be the analytical PSF from our simulations, and then solve for the parameters of the network and the PSF together.\n\nLWIR sensors based on microbolometers suffer from fixed pattern noise, which causes horizontal and vertical striations. Inspired by recent work on removing fixed pattern noise in thermal images [32], we modeled it as a low-rank image. We then simultaneously solved for the fixed pattern noise, the PSF, and the parameters of the network, giving us\n\n\\[\n\\min_{\\theta, K, F} \\sum_{n=1}^N \\sum_{m=1}^M \\|I_{obs}(m, n) - F(m, n)(K * N_\\theta)(m, n)\\|^2 + \\eta_{TV} TV(N_\\theta(m, n)),\n\\]\ns.t. \\( \\operatorname{rank}(F) = r, \\)\nwhere \\( F \\) is the fixed pattern noise. We used the recently developed wavelet implicit neural representations (WIRE) [31] for the INR architecture as it resulted in highest qualitative accuracy. An overview of the reconstruction pipeline is shown in Fig. S5.\n\n4.6 Fabrication\n\nThe meta-optics are fabricated on a 500\\(\\mu\\)m thick double-side polished silicon wafer, lightly doped with boron, giving a sheet resistivity of 1-10 \\(\\Omega\\)-cm. Direct-write lithography (Heidelberg DWL 66+) defines the aperture locations in the photoresist covering the wafer surface. A 220 nm thick aluminum layer is deposited onto the patterned photoresist via electron beam evaporation (CHA Solution) and lifted off to construct the metal mask around the circular apertures, helping to reduce noise during the experiments. The wafer is coated with another photoresist and patterned with the meta-optic scatterers via direct-write lithography, aligned inside the defined apertures. The photoresist pattern of meta-optics is transferred to the bulk silicon to a depth of 10 \\(\\mu\\)m by deep reactive ion etching (SPTS DRIE), utilizing its capability to etch with high aspect ratios and vertical sidewalls. After etching, the photoresist residue is stripped, and the fabricated meta-optics are ready for characterization. This process is shown on Fig. S8 in the supplement.\n\nFunding\n\nFunding for this work was supported by the federal SBIR program. 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Express **18**(17), 18453–18463 (2010). https://doi.org/10.1364/OE.18.018453\n\n[30] Sitzmann, V., Martel, J., Bergman, A., Lindell, D., Wetzstein, G.: Implicit neural representations with periodic activation functions. Adv. Neural Info. Processing Systems (2020)\n\n[31] Saragadam, V., LeJeune, D., Tan, J., Balakrishnan, G., Veeraraghavan, A., Baraniuk, R.G.: WIRE: Wavelet Implicit Neural Representations. In: IEEE Comp. Vision and Pattern Recognition (CVPR) (2023)\n\n[32] Saragadam, V., Dave, A., Veeraraghavan, A., Baraniuk, R.G.: Thermal image processing via physics-inspired deep networks. In: IEEE Intl. Conf. Computer Vision (ICCV) (2021)\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• BroadbandThermalImagingusingMetaOpticsSI.pdf"} {"paper_id": "prb67", "title": "Type-printable photodetector arrays for multichannel meta-infrared imaging", "text": "Type-printable photodetector arrays for multichannel meta-infrared imaging\n\nJunxiong Guo\nguo.junxiong@cdu.edu.cn\n\nShuyi Gu\nChengdu University\n\nLin Lin\nUniversity of Electronic Science and Technology of China\n\nYu Liu\nTsinghua University\n\nJi Cai\nChengdu University\n\nHongyi Cai\nChengdu University\n\nYu Tian\nBeijing Normal University\n\nYuelin Zhang\nBeijing Normal University\n\nQinghua Zhang\nChinese Academy of Science\n\nZe Liu\nChengdu University\n\nYafei Zhang\nChengdu University\n\nXiaosheng Zhang\nUniversity of Electronic Science and Technology of China\n\nYuan Lin\nUniversity of Electronic Science and Technology of China https://orcid.org/0000-0002-9879-4341\n\nWen Huang\nUniversity of Electronic Science and Technology of China\n\nLin GU\nhttps://orcid.org/0000-0002-7504-031X\n\nJinxing Zhang\nArticle\n\nKeywords: multichannel infrared imaging, meta-imaging, ferroelectric superdomain, deep learning, edge detection\n\nPosted Date: March 18th, 2024\n\nDOI: https://doi.org/10.21203/rs.3.rs-3929576/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nAdditional Declarations: There is NO Competing Interest.\n\nVersion of Record: A version of this preprint was published at Nature Communications on June 18th, 2024. See the published version at https://doi.org/10.1038/s41467-024-49592-4.\nType-printable photodetector arrays for multichannel meta-infrared imaging\n\nJunxiong Guo1,2,#,* Shuyi Gu1,# Lin Lin2,# Yu Liu3,4*, Ji Cai1 Hongyi Cai1 Yu Tian5 Yuelin Zhang5 Qinghua Zhang6 Ze Liu1 Yafei Zhang1 Xiaosheng Zhang2 Yuan Lin2 Wen Huang2**, Lin Gu7 and Jinxing Zhang5,*\n\n1 School of Electronic Information and Electrical Engineering, Institute of Advanced Study, Chengdu University, Chengdu 610106, China\n2 School of Integrated Circuit Science and Engineering, National Exemplary School of Microelectronics, University of Electronic Science and Technology of China, Chengdu 610054, China\n3 School of Integrated Circuits, Tsinghua University, Beijing 100084, China\n4 The College of Integrated Circuit Science and Engineering, National and Local Joint Engineering Laboratory for RF Integration and Micro-Packing Technologies, Nanjing University of Posts and Telecommunications, Nanjing 210023, China\n5 Department of Physics, Beijing Normal University, Beijing 100875, China\n6 Institute of Physics, Chinese Academy of Science, Beijing National Laboratory of Condensed Matter Physics, Beijing 100190, China\n7 School of Materials Science and Engineering, Tsinghua University, Beijing 100084, China\n\n# These authors contributed equally: Junxiong Guo, Shuyi Gu, and Lin Lin\n\n* Corresponding authors\nE-mail addresses: guojunxiong@cdu.edu.cn (J.X. Guo), y-liu-17@tsinghua.org.cn (Y. Liu), uestchw@uestc.edu.cn (W. Huang), and jxzhang@bnu.edu.cn (J.X. Zhang)\nAbstract\n\nMultichannel meta-imaging, inspired by the parallel-processing capability of neuromorphic computing, offers significant advancements in resolution enhancement and edge discrimination in imaging systems, extending even into the mid- to far-infrared spectrum. Currently, high-performance multichannel infrared imaging systems typically consist of separate detector arrays and gratings or multi-camera integration, which require complex circuit design and heavy power consumption, hindering the implementation of advanced human-eye-like imagers. Here, we present a novel approach for printable graphene plasmonic photodetector arrays with zero-bias operation driven by a ferroelectric superdomain for multichannel meta-infrared imaging with enhanced edge discrimination. The fabricated photodetectors exhibited multiple spectral responses by directly rescaling the ferroelectric superdomain instead of reconstructing the gratings. We also demonstrated enhanced and faster shape classification (98.1%) and edge detection (98.2%) using our multichannel infrared images compared with single-channel detectors. Our proof-of-concept photodetector arrays simplify multichannel infrared imaging systems and hold great potential for applications in efficient edge detection in human-brain-type machine vision.\n\nKeywords: multichannel infrared imaging, meta-imaging, ferroelectric superdomain, deep learning, edge detection\nInfrared imaging systems can convert infrared radiation into human-eye-recognizable pseudoviews and are used in diverse applications, including security, surveillance, environmental monitoring, industrial inspections, and medical and health diagnoses\\(^{1-4}\\). Current advanced infrared imaging systems are typically based on focal plane array (FPA) infrared sensors and have shown great potential for target perception\\(^5\\). However, fundamental challenges remain in achieving ultra-high resolution beyond the optical diffraction limit and in bias operation with low power consumption for hardware implementation. The human visual system can excel at rapidly and accurately identifying objective features, such as color, depth, and edges, in complex environments through the parallel processing of input light signals (\\(\\textbf{Fig. 1a}\\)), and has allowed for the future manufacturing of artificial vision\\(^{6-9}\\). Inspired by this, recent efforts have been devoted to collecting multichannel information in terms of hardware, such as heat-assisted detection and ranging (HADAR) and meta-imagers, to enhance infrared image resolution and recognition efficiency\\(^{10, 11}\\). This inevitably faces common limitations in addition to separating grating or sensor components, which necessitates a complex circuit design.\n\nRegarding the smart perception of future infrared imaging development, graphene plasmonic photodetectors have become a promising candidate for large-scale integration into optoelectronic networks, as they directly detect infrared light with a tunable spectral response and make possible multipixel read-out circuits. Previous experiments demonstrated the excitation and tuning of plasmons in patterned graphene using traditional electrostatic gating techniques, resulting in infrared light detection with a tunable and selective response\\(^{12-15}\\). However, achieving high-quality patterned graphene remains a challenge because of the inevitable edge disorder and amorphization that occur during the patterning process using standard techniques such as chemical vapor deposition (CVD) growth, lithography, and ion/chemical etching\\(^{16-18}\\). Although alternative approaches have shown promise for modulating surface plasmons in continuous graphene through substrate patterning or metal gratings\\(^{19-21}\\), precise spatial modulation of the charge carrier density of graphene for tunable infrared light detection has remained challenging. Furthermore, current graphene plasmonic photodetectors employing top- or back-gate layers face common limitations in terms of complex fabrication of contact electrodes and high power consumption\\(^{16, 22, 23}\\).\n\nFerroelectric superdomains, characterized by nanoscale domains with alternating up/downward polarization arrays, have the advantage of spatially manipulating the graphene carrier density at nanoscale resolution to construct nonuniform conductivity patterns, thereby confining graphene\nplasmons for enhanced infrared detection with a tunable spectral response^{24-26}, suggesting its unique potential for nanophotonic applications. In this study, we designed a simple two-terminal zero-bias multichannel array (MCA) detector by artificially type-printing graphene carrier density using BiFeO$_3$ (BFO) superdomains with hundreds-nanoscale-wide stripes for a meta-infrared imaging application. Raman signal-based spatial monitoring of the carrier density indicates that non-uniform patterning of graphene conductivity can be achieved by reconfiguring the ferroelectric superdomain. When operating at zero-bias voltage and room temperature, our device array exhibited tunable transmission spectra and selective responsivity in the mid-infrared region. Importantly, we demonstrate the integration of MCA photodetectors for infrared imaging applications, showing enhanced recognition accuracy for both overall target shapes and edge detection, along with faster training and recognition speeds compared to single-channel array (SCA) detectors.\n\n**Conceptual design of multichannel meta-infrared-imaging**\n\nConventional infrared imaging using SCA sensors (**Fig. S1a, Supporting Information**), which uses a linear response to map the incident intensity, faces the fundamental challenge of achieving ultrahigh spatial resolution beyond the optical diffraction limit. Consequently, textureless images famously known as the “ghosting effect” are produced. Recent developments in multichannel imagers have demonstrated their ability to enhance imaging resolution. For example, the integration of different types of sensors (e.g., HADAR) allows an imaging system to mimic the parallel processing functions of the human eye. Recently, an alternative approach using multichannel meta-imagers with external angular gratings (**Fig. S1b**) was developed to accelerate the machine vision. However, both have complex spatial layouts; in particular, different devices require different bias voltages to drive, which significantly hinders the goal of achieving high energy efficiency.\n\nThe scheme of the multichannel meta-infrared imaging technique using ferroelectric superdomain-printed photodetectors is illustrated in **Fig. 1b**. Unlike the integration of diverse cameras, the pixel points of our meta-imaging were engineered to achieve a parallel multichannel using a single aperture implemented with type-printing detectors. To ensure that the photodetector can provide selective photocurrents along with a multispectral response, we optimized the plasmonic sensing layer by rescaling the geometric shape of the ferroelectric superdomain into a 6-channel-pixel at an imaging point to avoid externally separated grating layouts. This approach can recognize a curled thumb (**Fig. 1b** and **Fig. S1b**), whereas the conventional approach using SCA detectors cannot (**Fig. S1a**).\nFig. 1. Infrared imaging using type-printing multi-channel photodetector array.\n\n(a) Illustration of the human visual system. The optical pathways are depicted in the top and lateral views in the left and middle panels, demonstrating the components of the human visual system, including the eyes, connecting pathways to the visual cortex, and other regions of the brain. The schematic diagram of the retina in the right panel highlights its remarkable ability to process various types of input light information in parallel. (b) Schematic of the meta-infrared using type-printing photodetectors. The integrated sensing layer enables selective light detection with a multi-spectral response, which avoids externally separated grating filters.\n\nType-printing of photodetector\n\nAs early as the Qingli period of the Song Dynasty (1041-1048 AD), China's Bi Sheng (970-1051 AD) invented the clay type, marking the birth of the movable-type printing technique. Movable\nprinting is divided into the engraving, typesetting, and printing processes. Figure 2a illustrates the fabrication process and structure of the photodetector designed using the type-printing technique employed in this study (see Methods). Here, we used a conductive atomic force microscopy (AFM) probe (Bruker) with a platinum coating to create a ferroelectric superdomain, where the epitaxial ferroelectric BFO thin film was periodically switched to an adjacent up- and downward-striped domain array (step 1 corresponds to the engraving process of the type-printing technique). Additionally, the large-scale switching of ferroelectric superdomains was experimentally demonstrated in our previous study using a water-printing technique\\(^{27}\\). The crystal structure of the BFO thin film is depicted in Figs. 2b and c, obtained using annular bright-field (ABF) high-resolution scanning transmission electron microscopy (STEM). Under the microscope, the iron atoms (depicted as yellow spheres) shifted dramatically in the upward or downward domains, indicating a reversal in the direction of ferroelectric polarization. The phase difference between the adjacent domains was \\(180^\\circ\\), as characterized by piezoelectric force microscopy (PFM) (Fig. 2d). The period of polarized strips (\\(W\\), length of adjacent up- and down-ward domains) was controlled from 200 nm to 1 \\(\\mu\\)m within the same BFO film. The widths of the upward and downward domains were equal within each period, that is, the width of the ferroelectric domain stripes (\\(w\\)) ranged from 100 to 500 nm.\n\nNext, we transferred the CVD-grown single-layer graphene onto the BFO film (Step 2, corresponding to the printing process of the type-printing technique) using the wet transfer method\\(^{28}\\). Subsequently, we employed a noncontact Raman spectroscopy monitoring technique to evaluate the doping level of graphene induced by the electrostatic effect of remnant polarization in the ferroelectric domains. The spatially resolved Raman G-band frequency shifts were used as probes for detecting the graphene carrier density\\(^{29}\\). In Fig. 2e, Raman G-band frequency mapping revealed periodic stripes with lower and higher frequencies, corresponding to the upward and downward domains, respectively. Additionally, Raman shift analysis (Fig. S2) showed a high 2D-to-G peak intensity ratio (\\(I_{2D}/I_G = 2.15\\)) and a low D-band intensity, confirming the high-quality and single-layer characteristics of the transferred graphene. Furthermore, comparative analysis of the Raman G-band for graphene on various BFO substrates (Fig. S3a) demonstrated that the behavior of graphene on BFO with an upward domain is similar to that of a pristine BFO film, whereas the behavior differs significantly in the downward domain.\n\nTo facilitate photocurrent collection and reduce contact resistance, source/drain electrodes were deposited on the graphene sheet (step 3). Typically, if the source/drain electrodes are made of the\nsame metal, the device exhibits an overall zero photocurrent. In this study, we employed an asymmetric metal-doping scheme to disrupt the symmetric built-in electric field profile in the graphene channel, following a previous study on metal-graphene-metal operation at zero bias between the source and drain\\(^{30}\\). Specifically, we deposited 20-nm-thick layers of palladium (Pd) and titanium (Ti) onto a graphene sheet and covered it with an 80-nm-thick layer of gold (Au) on the contact electrodes. A magnified scanning electron microscopy (SEM) image of the active region of the as-fabricated device is presented in Fig. 2f, and the raw SEM image is shown in Fig. S4.\n\nFigure 2g shows the average Raman G-band frequency of graphene on BFO with a striped domain width of 500 nm. The peak position of the G-band (POG) in Raman shift for graphene on upward and downward domains were 1,586 and 1,597 cm\\(^{-1}\\) respectively. The periodic Raman frequency shifted from lower to higher frequencies, suggesting that graphene experienced a sharp transition from lower to higher carrier concentrations at the edges of the upward/downward domains\\(^{19}, ^{20}\\), confirming the feasibility of spatial printing of graphene carrier density without patterning of graphene sheets. Periodic patterns of graphene carrier-density modulation offer a novel approach for type-printing multiple parallel p–i junctions in a continuous graphene sheet without destroying the graphene sheet or applying complex gating electrodes (Fig. 2h). Owing to the reversible and nonvolatile characteristics and nanoscale size of the ferroelectric domain, this strategy of integrating continuous graphene with a ferroelectric superdomain provides a novel approach for printing graphene carrier density into desired patterns, enabling graphene plasmonic resonance and enhancing the photocurrent in the mid- to far-infrared ranges.\n\nTo better understand our goal to achieve selective light detection beyond broadband wavelength response in the designed device, we introduced a plasmonic resonance model (Fig. 2i) in a graphene/BFO superdomain hybrid structure with electromagnetic field simulation using finite element analysis. Figures 2j and k illustrate the simulated cross-sections of the electric field intensity in our device, and detailed numerical simulation procedures are presented in Supplementary sections S1-S3. In this scenario, we set the chemical potential (\\( \\mu_c = E_F \\)) of graphene doping by upward and downward domains with a width of 500 nm as +121 meV and –448 meV, respectively. Here, it follows the formula of \\( \\hbar \\Delta \\omega = \\alpha' |E_F| \\) (ref. 29) as shown in Supplementary section S1, where \\( \\hbar \\Delta \\omega \\) and \\( \\alpha' \\) are the POG shift of graphene and the integral constant, respectively. The energy of the transverse-magnetic (TM) mode is strongly confined at the graphene/ferroelectric interface with ultra-\nhigh enhanced electric field intensity. Although the energy flow enters the graphene structure on the upward ferroelectric domain, it is almost perfectly absorbed. This phenomenon might contribute to the electronic behavior near the upward and downward domains of doping graphene junctions. Importantly, for our designed plasmonic device, the resonance frequency (\\( \\omega_{spr} \\)) could be easily regulated by rescaling the ferroelectric superdomain width (\\( d \\)) which follows eqn. (1),\n\n\\[\n\\omega_{spr} = \\left( \\frac{e^2 E_F}{2 \\pi \\hbar^2 \\varepsilon_0 \\varepsilon_r} \\left( q_0 \\pm N \\frac{\\pi}{d} \\right) \\right)^{\\frac{1}{2}}\n\\]\n\nwhere \\( e \\), \\( \\hbar \\), \\( \\varepsilon_0 \\), \\( \\varepsilon_r \\), and \\( q_0 \\) represent the element charge, reduced Planck constant, vacuum dielectric constant, relative dielectric constant of BFO, free space wave vector of incident light, and \\( N = 1,\\ 2,\\ 3,\\ ... \\), respectively. A detailed derivation of the formula is provided in Supplementary section S4.\n\n![Fabrication and architecture of graphene/BFO superdomain-based plasmonic photodetector.](page_186_579_1077_1012.png)\n\nFig. 2. Fabrication and architecture of graphene/BFO superdomain-based plasmonic photodetector.\n(a) Schematic of the experimental setup for printing graphene/BFO superdomain-based plasmonic photodetector. The BFO film epitaxial growth on an STO substrate with a covering LSMO (La$_3$Sr$_{1-x}$MnO$_3$) electrode layer. Cross-sectional view of transmission electron microscopy images of the downward domain (b) and upward domain (c) in BFO thin film, with a scale bar of 5 nm. (d) PFM phase image of BFO superdomain, showing the periodical ribbons patterned adjacent to upward and downward domains. (e) G-band frequency mapping for graphene on BFO superdomain with a\nperiod of 1 \\( \\mu \\)m. (f) SEM image of the active area of the fabricated graphene/BFO device. The fake color focuses on the graphene on the BFO film. (g) Averaged Raman frequencies for graphene on upward and downward domains, with solid lines representing the Lorentz fitting results. (h) Schematic of the device focusing on the graphene/BFO interface, illustrating the p-doped and near-intrinsic graphene behaviors on downward and upward domains, respectively. (i) Schematic of the graphene plasmon resonator architecture for a plane wave normally infrared incidence. GSPP represents graphene surface plasmon polaritons. (j, k) Simulated electric field intensity for graphene plasmon resonator by a three-dimensional model (j) and corresponding two-dimensional model (k). The excited GSPP is highly confining in the borders of upward/downward domains at the graphene/BFO interface. SLG denotes single-layer graphene.\n\nRescaling ferroelectric superdomain for multi-spectral response\n\nTo validate the performance of this printable architecture, we fabricated a device array on the same BFO thin film by rescaling the ferroelectric domain width (corresponding to the type-printing process). Two types of device arrays were fabricated (Fig. S5) to facilitate the optical (sample size of 5 mm \\( \\times \\) 5 mm) and photoelectric (sample size of 10 mm \\( \\times \\) 10 mm) measurements. Each unit contained six BFO stripes with domain widths ranging from 100 to 500 nm. The optical and corresponding PFM phase images of the fabricated device array are shown in Fig. 3a. The AFM Raman images (Fig. 3b) and corresponding POG peaks (Fig. S3b) strongly support our idea of type-printing desired graphene carrier patterns by resetting the ferroelectric domain width.\n\nWe then focused on the spectral response of graphene to the BFO superdomains of different widths. To achieve this, we used an AFM probe to direct incident light precisely to specific microregions. The transmission measurements are schematically illustrated in the inset of Fig. 3c, where \\( T \\) and \\( T_0 \\) correspond to the transmission values of the BFO film epitaxially grown on the SrTiO\\(_3\\) (STO) substrate with and without graphene, respectively. The measured extinction spectra of the graphene/BFO hybrid structures are shown in Fig. 3c. Within the periodically printed graphene stripes on the BFO superdomains, we observed two notable features. First, a remarkably selective resonant peak appeared with domain widths ranging from 100 to 500 nm. Second, the resonant peaks shifted from low frequency (1084 cm\\(^{-1}\\)) to high frequency (1292 cm\\(^{-1}\\)) with a decreasing domain period. The coincidence between the blue-shift phenomenon and Equation (1) can be attributed to the matching of the wave vector of the incident wave in free space and the wave vector of the excited GSPP, thereby forming a resonant coupling effect.\n\nThe photocurrent of the device array was measured using an automated wavelength-tuning laser to generate incident signals that were added to the graphene sheet at a 90° angle (in the vertical\ndirection) with a zero-bias voltage. All the photocurrents were obtained by averaging the peak values from 12 points under illumination at different wavelengths. The highest photocurrent in each cell was achieved near the resonant wavelength (Fig. 3d). Additionally, we investigated the photoresponsivity using \\( R = I_{ph}/P_{in} \\), where \\( I_{ph} \\) and \\( P_{in} \\) represent the photocurrent and incident laser power, respectively. The plots in Fig. 3d demonstrate that our device array exhibits a significantly selective detection factor \\( \\beta \\), which is the ratio of the highest and lowest photoresponsivity values in each cell.\n\nWe then discussed the performances of typical infrared photodetectors based on emerging materials operating at room temperature, as shown in Fig. 3e. Compared to previously reported metal plasmon-enhanced graphene photodetectors, such as metal-graphene-metal structure\\(^{30}\\), the intrinsic plasmons in patterned graphene offer an incomparable advantage in the mid-infrared range. Its surface plasmons can be used to resonantly enhance the absorption for tunable photodetection controlled by the grating effect, providing appealing spectral selectivity with ultra-high tunability\\(^{15}\\). For the photodetector demonstrated herein, it achieved an enhanced photoresponsivity of approximately 30 mA W\\(^{-1}\\). While this photoresponsivity was not the highest recorded among current infrared photodetectors using emerging materials\\(^{31}\\), it was comparable to that of conventional graphene plasmonic devices for mid-infrared detection based on nanopatterned graphene photograting structures\\(^{31-34}\\). This can be attributed to the effective plasmon excitations and perfect crystallinity of the graphene sheet, with the latter effectively reducing light scattering compared to nanopatterned graphene. Another interesting phenomenon is that the device we designed can operate at zero bias voltage, with its detection range within the IR-C band (3 \\( \\mu \\)m to 1 mm, CIE 17-21-004, https://cie.co.at/eilvterm/17-21-004). This coincided with the biological thermal radiation, particularly the fact that over 50% of the energy emitted by the human body was concentrated in the range of 8 to 14 \\( \\mu \\)m, which our device could handle. Furthermore, the convenience of printing graphene carrier-density patterns by switching ferroelectric domains at the nanoscale without the need for complex nanofabrication, as seen in conventional graphene plasmonic devices, allows for a remarkably selective response over broadband wavelengths and features a simple multi-channel array integration for light detection in the infrared region. The characteristics exhibited by our device provide a promising route for advanced multi-channel infrared imaging that combines low power consumption with high recognition capability, as mentioned earlier.\nFig. 3. Characterization of type-printing detector array.\n(a) Integrating graphene photodetector array onto BFO film. The middle column is the optical image of the fabricated device array with a ferroelectric domain width ranging from 100 to 500 nm. The top and bottom columns are the PFM phase images of the corresponding BFO superdomains. (b) AFM-Raman mapping images for graphene carrier density printed by rescaling BFO superdomain. (c) Tunable transmission extinction spectra (1−\\( T/T_0 \\)) for graphene by rescaling BFO superdomain. (d) Photocurrent and normalized responsivity (\\( R_{max}/R_{min} \\)) as functions of incident wavelength depending on the width of the BFO superdomain. (e) Comparison of responsivity with typical types of infrared photodetectors using metal-semiconductor-metal structure working at room temperature. The data were collected from refs. 31-34.\n\nMultichannel infrared imaging for enhancing edge detection\n\nTo evaluate the imaging capability of the fabricated array of infrared photodetectors, we used the OPENZYNQ open-source project (https://github.com/openzynqhardware/openzynq.git) to simulate the process. A schematic of the simulation procedure is shown in Fig. S6. For data collection, we employed a commercial Melexis infrared camera with 192×144 pixels to capture the desired temperature. The simulations have already been demonstrated for both the SCA with a ferroelectric\ndomain width of 500 nm and MCA with ferroelectric domain widths ranging from 100 to 500 nm (Fig. 4a and Figs. S7-S9). We observed that MCA detectors excel at recognizing inner edge profiles such as curled fingers and overlapped leaves, whereas SCA detectors fall short in this regard. The images generated by the MCA showed a more pronounced temperature difference between the regions of the fingers and palms, indicating that the MCA can identify more complex edge features of the targets when processing images.\n\nAn off-chip learning task involving the classification of gesture images (0-5, as shown in Fig. 4a) was conducted to evaluate the learning capability of the MCA detectors in infrared imaging. The training accuracies for gesture recognition were 99.2% and 100% based on the SCA and MCA detectors, respectively, after 3,600 iterations (Fig. 4b). The MCA detectors exhibited a significantly faster training speed than the SCA detectors because of the intrinsic differences between the edge profiles. However, we analyzed the changes in classification accuracy over 100 epochs for gesture recognition, with each epoch consisting of 3,600 iterations. Figure 4c reveals two key findings. First, when dealing with a small sample size, the MCA performs better than the SCA in gesture recognition accuracy. For example, at 10 epochs, the recognition accuracies of the MCA-based- and SCA-based detectors were 96.7% and 63.7%, respectively. At 40 epochs, they reach 97.8% and 88.9%, respectively. Second, when faced with a large sample size, the difference in gesture recognition accuracies between the two methods became small. For example, at 100 epochs, the recognition accuracies of the MCA and SCA were 98.1% and 93.2%, respectively.\n\nThe second important application of MCA detectors is enhanced edge detection, which was demonstrated using an off-chip learning task involving the recognition of curled fingers. As shown in Fig. 4a, the curled finger edges extracted from the infrared images using the MCA method are much more distinct than the SCA, which failed to capture them. The same trend was observed in the images of the overlapped leaves (Fig. S7). The results of training in the presence and absence of curled fingers showed that the MCA and SCA methods had training accuracies of 76.3% and 99.8%, respectively (Fig. 4d). This difference was much larger than that of the gesture training, with the discrepancies decreasing from 0.8% to 23.5%. Similar to gesture training, the MCA detectors exhibited a significantly faster training speed than the SCA detectors for curled fingers. More importantly, during curled finger recognition, after 100 epochs, the recognition accuracy of the MCA approach reached a high level of 98.2%, whereas that of the SCA remained at approximately 69.7% (Fig. 4e). These results further demonstrate that the MCA method can significantly improve the accuracy of target\nrecognition in infrared imaging at the hardware level, particularly by enhancing the edge detection accuracy in complex environments.\n\n![Applications of type-printing detectors in gesture infrared imaging and recognition.](page_184_328_1079_410.png)\n\nFig. 4. Applications of type-printing detectors in gesture infrared imaging and recognition.\n(a) Infrared imaging for different gestures with single- and multi-channel array of type-printing photodetectors. (b, c) Evolution of classification accuracy over 100 epochs for gesture recognition, with each epoch consisting of 1,000 iterations. (d, e) Changes in the classification accuracy over 100 epochs for curled finger recognition, with each epoch including 1,000 iterations.\n\nConclusions\n\nWe developed a printable photodetector array by integrating monolayer graphene with a BFO thin film that features a nanoscale-wide stripe superdomain and demonstrated that this type of device array is designed for multichannel meta-infrared imaging applications and offers significant enhancement of edge detection. Graphene was monitored non-contactfully for dopants using Raman shifts, and doping patterns on ferroelectric superdomains were observed at the nanoscale. The printable photodetectors operated at a zero-bias voltage and exhibited a high photoresponsivity of approximately 30 mA W\\(^{-1}\\) at room temperature. This can be attributed to the resonant coupling of graphene plasmons with incident light. Moreover, the device arrays exhibited a selective response in the mid-infrared region through direct rescaling of the BFO superdomain width under ambient conditions. This work demonstrates the precise spatial control of graphene carrier density by reversing the ferroelectric domains at the nanoscale. The excellent compatibility of graphene sheets with different substrates offers several advantages over conventional devices that rely on complex\nnanofabrication techniques. Additionally, we proved that multichannel array detectors can enhance shape and edge detection in infrared imaging. These features allow for future integrated optoelectronic platforms with simple circuit designs and low power consumption.\n\nMethods\n\nBFO film epitaxial growth. BFO thin films were epitaxially grown on (001)-oriented STO substrates with LSMO as the bottom electrode using pulsed laser deposition. For the deposition of both LSMO and BFO films, a KrF excimer laser, with 248 nm wavelength, 5 Hz repetition rate, and ~1.5 J cm^{-2} energy density, was employed. The films were grown in an atmosphere of 0.2 mbar oxygen pressure at 700 °C. The thicknesses of the films were maintained at approximately 25 nm.\n\nDevice fabrication. For ferroelectric polarization switching, the upward and downward domains were switched by scanning the surface with a nanotip under a +12 V (−12 V) bias exceeding the coercive voltage (Fig. 1a, step 1). For the convenience of guiding the incident light to specific areas and fixing the active illuminating regions, the BFO film was patterned into an array with a fixed area, and the etched depth was controlled at approximately 10 nm in each unit using reactive ion etching (RIE) before polarization.\n\nSingle-layer graphene was transferred onto a BFO film using an improved wet method^{28} (Fig. 1a, step 2). Briefly, the polymethyl methacrylate (PMMA, Aladdin) solution (20 mg mL^{-1}) was spin-coated on CVD-grown monolayer graphene/copper foils (SixCarbon Technology Shenzhen) at 3,000 rpm for 30 s and dried at 120 °C for 90 s in air. Ammonium persulfate (0.1 M) was used to etch the copper substrate, and the PMMA/graphene film was washed several times with deionized water to remove the etchant residue. The prepolarized BFO film was then placed in water at a tilting angle underneath the PMMA/graphene film to support it. After drying in air, the PMMA was removed with an acetone bath at 50 °C and washed with ethanol. The monolayer graphene was etched to the same area as the marked BFO using oxygen plasmons. Subsequently, the Au/Ti and Au/Ni source and drain electrodes were deposited on the border of the graphene to fabricate the device (Fig. 1a, step 3). The thicknesses of the Au layer and Ti and Pd layers were 80 and 20 nm, respectively.\n\nMeasurements. PFM experiments were performed under ambient conditions at room temperature using an Infinity Asylum Research AFM instrument. The crystal structures of BFO were determined using TEM (JEOL 2100F) operated at 200 keV and equipped with a probe aberration\ncorrector (CEOS) and double spherical aberration (Cs) correctors. The spatial resolution of the microscope reached 90 pm at an incident semiangle of 20 mrad. Subsequently, a fast Fourier transform multislice approach was used for the STEM configuration. Raman-AFM mapping images and the corresponding spectral data in the same region were acquired using a fully integrated system based on the Smart SPM state-of-the-art scanning probe microscope and XploRA Raman microspectrometer (HORIBA). In all cases, 532 nm laser excitation and tip-enhanced Raman spectroscopic resolution were used. The transmission spectra were collected using a Spotlight 200i FT-IR Microscopy System (PerkinElmer Inc.) with a spot resolution better than 10 μm. The photocurrents were performed using a Keithley 4200A-SCS Parameter Analyzer (Tektronix), and the incident source was produced by a tunable laser (EKSPLA, 2.3–10 μm), at zero bias voltage between the contact electrodes. The laser intensities, including the Raman and electrical measurements, were set below 1 mW to avoid artifacts caused by laser-induced heating. All measurements were performed in ambient air at room temperature.\n\nNumerical simulations. The electrical properties of graphene were calculated using random phase approximation (RPA), and the dynamic optical response of graphene was derived from the Kubo formula (Supplementary Section S2) (ref. 35, 36). Electromagnetic field simulation was performed using the finite element method (Supplementary Section S3). Infrared imaging simulations were performed using an open-resource project, and the details are shown in Supplementary Section S5.\n\nAcknowledgments\nThe authors thank Ms. Xiaoxu Lai and Prof. Ronghui Guo from Sichuan University for their support with the Raman mapping and photocurrent measurements. We also thank Dr. Prof. Lei Bi from the University of Electronic Science and Technology of China for discussions on spectral response. This work was financially supported by the National Natural Science Foundation of China (Grant Nos. 62371095, 62201096, and 62074029), National Key Research and Development Program of China (Grant No. 2022YFB3206100), Key R&D Program of Sichuan Province (Grant Nos. 2022ZHCG0041, 2022JDTD0020, and 2022YFG0163), Natural Science Foundation of Sichuan Province (Grant Nos. 24NSFSC0409 and 2022NSFSC0652), and Aeronautical Science Foundation (Grant No. 20200024080001).\nAuthor contributions\nJ. G., Y. L., W. H., and J. Z. conceived and designed the experiments. Y.T., Y.Z., and J.Z. provided the epitaxially grown BFO films. Y.T. and Y.Z. wrote the ferroelectric superdomain using a type-printing technique and characterized the PFM images. J. G., Y. L., and L. L. fabricated the devices. Q. Z. and L. G. conducted high-resolution TEM characterization. L. L. conducted SEM characterization. J. G. and L. L. conducted the Raman characterization and optical transmission measurements. J. G. and L. L. conducted the photodetection experiments. J. G., Y. L., L. L., J. C., Z. L., and Y. Z. performed the theoretical models and calculations for the electromagnetic field simulations. J. G., S. G., Y. L., and H. C. designed and performed the infrared imaging and deep learning. J. G., Y. L., X. Z., Yuan. L., W. H., and J. Z. analyzed the data. J. G., Y. L., W. H., and J. Z. supervised the experiments. J. G. and Y. L. wrote the paper and Supporting Information. 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Click to download.\n\n• supplementaryinformationv2.pdf"} {"paper_id": "prb68", "title": "Convergent evolution in Afrotheria and non-afrotherians demonstrates high evolvability of the mammalian inner ear", "text": "Convergent evolution in Afrotheria and non-afrotherians demonstrates high evolvability of the mammalian inner ear\n\nNicole Grunstra\nnicolegrunstra@gmail.com\n\nUniversity of Vienna https://orcid.org/0000-0002-6708-2245\nFabian Hollinetz\nUniversity of Vienna\nGuillermo Bravo Morante\nUniversity of Vienna\nFrank Zachos\nNatural History Museum Vienna\nCathrin Pfaff\nUniversity of Vienna\nViola Winkler\nNatural History Museum Vienna\nPhilipp Mitteröcker\nUniversity of Vienna\nAnne Le Maitre\nUniversity of Vienna https://orcid.org/0000-0003-2690-7367\n\nArticle\n\nKeywords: Afrotheria, bony labyrinth, convergent evolution, evolvability, geometric morphometrics, mammals\n\nPosted Date: July 11th, 2023\n\nDOI: https://doi.org/10.21203/rs.3.rs-3125661/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: There is NO Competing Interest.\nVersion of Record: A version of this preprint was published at Nature Communications on September 16th, 2024. See the published version at https://doi.org/10.1038/s41467-024-52180-1.\nConvergent evolution in Afrotheria and non-afrotherians demonstrates high evolvability of the mammalian inner ear\n\nNicole D.S. Grunstra$^{1,2*}$, Fabian Hollinetz$^1$, Guillermo Bravo Morante$^1$, Frank E. Zachos$^{1,2,3}$, Cathrin Pfaff$^4$, Viola Winkler$^5$, Philipp Mitteroecker$^{18}$, Anne Le Maître$^{1,6\\text{§}}$\n\n$^1$Department of Evolutionary Biology, University of Vienna, Vienna, Austria\n\n$^2$Mammal Collection, Natural History Museum Vienna, Vienna, Austria\n\n$^3$Department of Genetics, University of the Free State, Bloemfontein, South Africa\n\n$^4$Department of Palaeontology, University of Vienna, Vienna, Austria\n\n$^5$Central Research Laboratories, Natural History Museum Vienna, Vienna, Austria\n\n$^6$Laboratoire Paléontologie Evolution Paléoécosystèmes Paléoprimatologie (PALEVOPRIM) – UMR 7262 CNRS INEE, Université de Poitiers, Poitiers, France\n\n§ Equal contributions\n\n* corresponding authors: N.D.S. Grunstra (nicole.grunstra@univie.ac.at) and A. Le Maître (anne.le.maitre@univie.ac.at)\nAbstract\n\nEvolutionary convergence in distantly related species is among the most convincing evidence of adaptive evolution. The mammalian ear, responsible for balance and hearing, is not only characterised by its spectacular evolutionary incorporation of several bones of the jaw, it also varies considerably in shape across modern mammals. Using a new multivariate approach, we show that in Afrotheria, a monophyletic clade with morphologically and ecologically highly disparate species, inner ear shape evolved similar adaptations as in non-aфrotherian mammals. We identified four trait combinations that underlie this convergence. The high evolvability of the mammalian ear is surprising: nowhere else in the skeleton are different functional units so close together; it includes the smallest bones of the skeleton, and is encapsulated within the densest bone. We suggest that this evolvability is a direct consequence of the increased genetic and developmental complexity of the mammalian ear compared to other vertebrates.\n\nKeywords: Afrotheria, bony labyrinth, convergent evolution, evolvability, geometric morphometrics, mammals\nIntroduction\n\nSome of the most spectacular macroevolutionary changes in the vertebrate ear - responsible for balance, posture, gaze stabilisation, and hearing - occurred in mammals. The transformation of jaw bones into the middle ear ossicles, which evolved at least three times independently in mammals, greatly increased the bandwidth of hearing (Luo 2011, Wang et al. 2019). The shape of the mammalian inner ear also deviates from that of other tetrapods, notably in the length of the cochlea and the evolutionary novelty of the organ of Corti with its electromotile outer hair cells (Manley 2012; Köppl & Manley 2018). The length and curvature of the cochlear canal is much more diverse in mammaliaforms compared to other groups (Gleich and Manley 2000; Ekdale 2013, 2016, Ruf et al. 2013; Luo et al. 2016). Extensive cochlear coiling even evolved multiple times independently in mammals (Ekdale 2013; Luo et al. 2016). Mammals are also the only group to have evolved an outer ear, composed of an auditory canal and pinna (Webster 1966). Not only is the mammalian ear system thus more heterogeneous and morphologically complex, it is also genetically and developmentally more complex than in other tetrapods (Fritzsch et al. 2015; Fuchs & Tucker 2015). We previously proposed that this increased heterogeneity and developmental complexity of the mammalian ear bestows it a higher evolvability, i.e., an enhanced capacity for adaptive evolution, and that this increase in evolvability likely contributed to the evolution of the spectacular disparity in mammalian body plans and ecological niches (Le Maître et al. 2020; see also below).\n\nSize and shape of the bony labyrinth (the bony wall surrounding the inner ear) differs considerably across mammalian lineages, which is assumed to reflect evolutionary adaptations to different locomotor behaviours, postures, and hearing capacities in mammals (e.g., Billet et al. 2013, Crumpton et al. 2015; Pfaff et al. 2015, Ekdale 2016, Grohé et al. 2016, Schwab et al. 2019, Benoit et al. 2020). For example, the semicircular canals, important for balance and posture control, are strongly reduced in size in cetaceans, which has been linked to their aquatic lifestyle (Spoor et al. 2002, Ekdale 2013). In fast and manoeuvrable terrestrial taxa, the semicircular canals are large relative to body mass and particularly thin (Spoor et al. 2007). The length and coiling of the cochlea of the inner ear (responsible for the detection and transmission of sound) is largest in mammals that rely heavily on hearing for prey or predator detection and environmental navigation, such as in bats and subterranean rodents (Lange et al. 2004; Ekdale 2013). An extended secondary bony lamina of the cochlea is associated with ultrasonic hearing in cetaceans (Mourlam & Orliac 2017, Costeur et al 2018, Park et al 2019). Apart from these strong functional signals, bony labyrinth morphology is also indicative of phylogenetic relatedness (e.g., Ekdale 2013, Benoit et al. 2015,\nGrohé et al 2016, Costeur et al 2018, Schwab et al 2019, del Rio et al 2021, Le Maître et al. 2023).\nThe bony labyrinth has therefore been intensively studied so as to reconstruct both environmental adaptations and the phylogenetic position of fossil mammals (e.g. Billet et al 2013, Benoît et al. 2015, Schmitt & Gheerbrant 2016, Mennecart et al 2017, Le Maître et al. 2023, Orliac et al 2023).\n\nBy comparison, the bony labyrinth of Afrotheria - one of the four main clades of placental mammals - has been understudied. Afrotherians show a high disparity to diversity ratio, i.e., they exhibit a striking degree of ecological and morphological disparity while comprising only few species. The crown group Afrotheria evolved on the African continent (including Madagascar), from which the clade derives its name, between ~90-70 Ma in the late Cretaceous (Bininda-Emonds et al. 2007; dos Reis et al. 2012; Meredith et al. 2013). Modern Afrotheria includes six higher taxa traditionally classified as “orders” that bear little resemblance to each other: Proboscidea (elephants), Hyracoidea (hyraxes), Sirenia (sea cows), Tubulidentata (the aardvark), Afrosoricida (golden moles, tenrecs, and otter shrews), and Macroscelidea (elephant shrews or “sengis”). They include fully aquatic (sea cows), semi-aquatic (otter shrew and some tenrecs), terrestrial (e.g., elephants, aardvark), arboreal (tree hyrax) and subterranean taxa (golden moles). Extant afrotherians also vary in body mass by more than five orders of magnitude (~40 g for an elephant shrew up to >4000 kg for an elephant). Many ecological and morphological similarities with non-afrotherian placentals exist, and until molecular phylogenetics resolved them as a separate clade, the different afrotherian subgroups were scattered throughout the placental mammalian phylogeny (Tabuce et al. 2008). Notably, the phylogenetic position of golden moles and tenrecs in Afrotheria long evaded detection due to their strong morphological similarity to “true” moles, hedgehogs and shrews (MacPhee & Novacek 1993; Asher et al. 2003; Springer 2022). The discordance between molecular and morphological similarities among Afrotheria and the many morphological homoplasies shared with other placental mammals attest to the high degree of evolutionary convergence in the external and internal morphology of Afrotheria.\n\nGiven the assumed high evolvability of the mammalian ear and the striking disparity of Afrotheria, here we study if the bony labyrinth evolved similar functional adaptations in afrotherian and non-afrotherian mammals. To this end, we compare bony labyrinth shape of 20 afrotherian taxa to that of 20 other, morphologically and ecologically analogous mammals using 3D geometric morphometrics and a multivariate phylogenetic comparative approach (Figs. 1 and 2). We show that afrotherians resemble their analogues more closely in labyrinth shape than they do each other or non-afrotherian non-analogues. Furthermore, afrotherians and their analogues share the same\nassociations of bony labyrinth shape to ecology and positional behaviour (posture and locomotion).\nOur results thus indicate that functional adaptation and convergence dominate over phylogenetic history in the pattern of similarity in inner ear shape at the level of major placental mammal clades, supporting the hypothesis that the mammalian ear has high evolvability.\n\n![Phylogeny and silhouettes depicting the sample of Afrotheria and their analogues.](page_184_370_1207_627.png)\n\nFig. 1: Phylogeny and silhouettes depicting the sample of Afrotheria and their analogues. (A) Phylogenetic relationships between Afrotheria (blue) and the other mammals in our sample (black), for which we follow the Atlantogenata hypothesis. (B) Taxa are depicted as their silhouettes, with each row showing the afrotherians (blue) and their ecological and/or morphological “analogue(s)” (black). See Table 1 for more details. Silhouettes from PhyloPic.org and by the authors.\nFig. 2: Landmark scheme used to quantify the shape of the bony labyrinth. The bony labyrinth, i.e., the osseous moulding of the inner ear, of a Javan mouse deer (Tragulus javanicus) from superior (left) and lateral (right) views. Linear accelerations of the head are detected in the vestibule (Ve), at the base of which the vestibular aqueduct (VA) is inserted, and head rotations are detected at the bulged base (ampulla) of each of the three semicircular ducts. The bony counterparts of these ducts are the lateral, anterior, and posterior semicircular canals (LSC, ASC, and PSC), with the latter two fused to form the common crus (CC). Sounds are detected in the cochlea (Co), due to the propagation of sound pressure waves from the vestibular window (VW) to the apex of the cochlea, then back to the cochlear window (CW) through which they dissipate. To quantify bony labyrinth shape we placed 13 anatomical landmarks (large numbered spheres) and 111 semilandmarks (smaller spheres), mostly on the centrelines of the semicircular canals and the cochlea, on every CT scan.\n\nResults\n\nEvolutionary convergence of overall labyrinth shape\n\nTo assess the overall convergence of bony labyrinth shape, we calculated the Procrustes distance (a measure of overall shape dissimilarity) between all pairs of afrotherians and non-afrotherians. The average Procrustes distance between afrotherians and their non-afrotherian analogues (Fig. 1, Table 1) was 0.238, whereas the average distance between afrotherians and (non-afrotherian) non-analogues was 0.281. In other words, the average shape distance for pairs of non-analogues was 18.0% higher than for pairs of analogues (\\( p < 0.001 \\)), reflecting convergent evolution in Afrotheria and other mammals. Even the average Procrustes distances among all pairs of Afrotheria (0.263),\ni.e., between afrotherians and other afrotherians, and among all pairs of non-afrotherians (0.292) exceeded the average distance between Afrotheria-analogue pairs, showing that functional adaptation dominates over phylogenetic history in the average magnitude of overall labyrinth similarity at this high taxonomic level.\n\nAdaptive signals in labyrinth shape\n\nTo identify the features that underlie this convergence in bony labyrinth shape, we performed a two-block partial least squares analysis (2B-PLS) between all 372 Procrustes shape coordinates and 12 contextual variables that capture multiple aspects of ecology and positional behaviour (Table 2).\n\nThe first four dimensions (or pairs of latent variables) together accounted for 93.8% of the summed squared covariances between the two blocks of variables (hierarchical permutation tests against a null hypothesis of no association yielded \\( p \\)-values of 0.001, 0.030, 0.043, and 0.103, respectively, for the four dimensions). Further dimensions accounted for only 2% or less. PLS 1 contrasted aquatic species from terrestrial species (Fig. 3). Aquatic and semi-aquatic species had smaller and rounder semicircular canals, particularly the posterior canal, which was shifted superiorly relative to the lateral canal, associated with a larger, rounder vestibular window, and a broad and flat cochlea with fewer turns. PLS 2 distinguished fossorial and pronograde species from species moving in 3D (i.e., moving in horizontal, vertical and lateral planes), and arboreal and scansorial taxa in particular. Fossorial species, especially fully subterranean ones, had a long common crus, nearly as high as the vertical (anterior and posterior) semicircular canals, an acute angle between anterior and lateral canals, a posteriorly projected lateral semicircular canal, as well as a narrow cochlea with many turns, compared to 3D-moving, arboreal, and scansorial species.\nFig. 3: Results for the partial least squares analysis of bony labyrinth shape and the contextual variables (PLS 1 and 2). First two dimensions of the two-block partial least squares (2B-PLS) analysis between the Procrustes shape coordinates of the bony labyrinth and the 12 contextual variables. Panels A and B show the loadings for the first PLS dimension, representing the shape pattern and the contextual pattern with highest covariance. The semicircular canals are in blue, the cochlea is in red, and the vestibular (oval) and cochlear (point) windows are in green. The orientation of the bony labyrinths is the same as in Fig. 2 (right panel). Panel C shows a scatterplot of the corresponding contextual and shape scores. The colour code corresponds to five habitat groups, but this grouping was not used for computing the PLS. Note that when a\nspecies’ common name appears several times, it corresponds to different species. Panels D-F show the loadings and scores for the second PLS dimension.\n\nPLS 3 contrasted agile species that pursue prey on the ground - and to some extent also agile aquatic species - with leaping or jumping arboreal species and subterraneous, fossorial species (Fig. 4). Along PLS 3, bony labyrinth shape mainly varied in the relative expansion of the semicircular canals (superior for the vertical canals and the common crus, and lateral for the lateral canal) and in the curvature and number of turns of the cochlea. PLS 4 was a contrast between slow, pronograde and to some extent large species (mainly driven by the elephant) versus leaping, jumping, and agile species moving in 3D. Along PLS 4, species varied in the anterior-posterior expansion of the anterior part of the bony labyrinth (i.e., the anterior and lateral semicircular canals, vestibular window and cochlea), relative to its posterior part.\n\nWe also conducted a phylogenetic 2B-PLS analysis (Figs. S3-4 in Supplementary Information), which showed that similar associations remain after accounting for phylogeny, though the ecomorphological associations are captured by the four PLS dimensions in slightly different ways.\n\nPhylogenetic signals in labyrinth shape\n\nDespite these patterns of convergent evolution, signals of phylogenetic history are also visible. Closely related species with relatively recent divergence dates, e.g., golden moles, elephant shrews, or hyraxes, have similar bony labyrinth morphologies and ecologies (Fig. 3F and 4F, Fig. S1-2). Such phylogenetic patterning at lower taxonomic levels (e.g., within an “order”) was supported by statistically significant phylogenetic signal in the four PLS shape scores; Blomberg's \\( K \\) was 0.52, 0.7, 0.48, and 0.43, respectively. But closely related species also tended to share a similar environment or lifestyle; the context scores showed \\( K \\)-values from 0.38-0.69. These results indicate that adaptive evolution in the inner ear of mammals reflects a combination of phylogenetic divergence (whereby closely related taxa share adaptations to a similar environment) and convergence (whereby distantly related species share adaptations to a similar environment).\nFig. 4: Results for the partial least squares analysis of bony labyrinth shape and the contextual variables (PLS 3 and 4). Dimensions 3 and 4 of the two-block partial least squares (2B-PLS) analysis between the Procrustes shape coordinates of the bony labyrinth and the 12 contextual variables. Panels A and B show the loadings for the third PLS dimension, and panel C the corresponding scores. The semicircular canals are in blue, the cochlea is in red, and the vestibular (oval) and cochlear (point) windows are in green. The orientation of the bony labyrinths are the same as in Fig. 2 (right panel). Panels D-F show the loadings and scores for the fourth PLS dimension.\nGiven the importance of habitat and locomotor behaviour to a species’ morphological adaptations, the four PLS dimensions described above estimate the “functional” aspects of labyrinth shape and - by and large - separate the functional part of shape space from those shape features that carry no or little functional signal. When computed only from these four PLS dimensions, the average shape distance for pairs of non-analogues was even 42.0% higher than for pairs of analogues (\\( p<0.001 \\)), reflecting strong convergent evolution of these shape features in ecologically, behaviourally, and morphologically similar mammals. By contrast, after removing these four dimensions from the data, the average Procrustes distances of non-analogue pairs and analogue pairs were of similar magnitude (0.197 versus 0.190; \\( p=0.13 \\)). This indicates that the pattern of convergence is successfully captured by the four PLS dimensions.\n\nDiscussion\n\nConvergent adaptation in distantly related species to shared environmental or functional regimes is among the most convincing evidence of adaptive evolution. Here we have introduced a multivariate exploratory approach to study evolutionary convergence and showed that in Afrotheria, a monophyletic clade with morphologically and ecologically highly disparate species, bony labyrinth shape evolved similar adaptations as in non-afrotherian mammals. We were able to identify four dimensions of shape space, i.e., four combinations of bony labyrinth traits, that underlie this evolutionary convergence.\n\nAll strictly aquatic marine mammals (the manatee, dugong, and dolphin) had very small semicircular canals, leading to a low sensitivity to head rotations, a feature which has been proposed to be an adaptation for moving in all directions under water while having limited flexibility of the neck (Yamada and Yoshizaki 1959; Spoor et al. 2002, but see Muller, 1999). All aquatic and semi-aquatic mammals had a cochlea with a limited number of turns, and hence a short cochlear canal, which is linked to a reduced sensitivity to low-frequency sounds in terrestrial mammals (West 1985; Manoussaki et al. 2008). Most of them also had a broad basal cochlear turn that is not tightly coiled with the next one, a feature associated with high-frequency hearing in aquatic mammals (Fleischer 1976; Ekdale & Racicot 2015; Moore et al. 2021). Arboreal mammals, especially the scansorial taxa, were characterised by a short common crus, and hence reduced mechanical coupling between the two vertical semicircular\ncanals (Muller & Verhagen, 2002). They also tended to have small semicircular canals, which leads to low sensitivity and might avoid flow disturbance in the ducts in case of vigorous rotations, and thus help to prevent overreactions to head movements while balancing on, e.g., tree branches (Muller, 1999; Pfaff et al 2015). Leaping and jumping arboreal taxa had a long cochlear canal with a graded curvature, indicating good low-frequency hearing and sound localisation abilities (West 1985; Heffner & Heffner 1992; Manoussaki et al. 2008). On the contrary, all subterranean taxa have evolved a long common crus allowing for a strong coupling of the vertical semicircular canals, and hence an efficient detection of vertical head movements (Muller & Verhagen, 2002), which likely is important to detect the direction of gravity (vertical acceleration) in environments with few other cues for orientation. Most subterranean taxa had very large semicircular canals, yielding increased sensitivity to head rotations in all directions (McVean, 1999; Muller, 1999; Pfaff et al 2015). Additionally, subterranean taxa were characterised by a very long cochlea with many turns, leading to a high sensitivity to low-frequency sounds, which attenuate less rapidly in underground environments (Lange et al. 2004; Ekdale 2013; Crumpton et al. 2015; Mason et al. 2016). Finally, agile species that pursue moving prey evolved very large semicircular canals, conferring increased sensitivity to head rotations in all directions, which is necessary for fast movements and good reflexes with respect to posture, balance and eye movements (Muller, 1999; Spoor et al. 2007).\n\nBecause the signal of overall convergence (as measured by average Procrustes distances) diminished after removing the aforementioned four dimensions from the data, adaptive evolution in labyrinth shape seems to be largely captured by these four shape patterns. These patterns were estimated as linear combinations with maximal covariance with the contextual variables, but this does not necessarily imply that our contextual variables represent the actual (or all) functional parameters that were under selection. For example, we did not have the actual auditory parameters that describe a species’ hearing ability (e.g., hearing range, sensitivity threshold at low and high frequencies). Nonetheless, as proxies our contextual variables sufficiently captured the adaptive signal.\n\nWhile convergent evolution in traits such as body size, body proportions, and life history traits is well documented and easy to understand, it is less obvious how the vertebrate ear realises such a stunning evolvability. Nowhere else in the vertebrate skeleton are different functional units so close together, comprising the smallest bones of the skeleton that are jointly encapsulated in the surrounding temporal bone. Moreover, growth of the inner ear is already completed around birth\n(e.g. Hoyte, 1961; Berlioz et al. 2021; Costeur et al. 2017; Richard et al. 2017), which may further limit the ability to evolve. In Le Maître et al. (2020), we suggested that this evolvability is a consequence of the genetic and developmental complexity of the mammalian ear. The evolutionary integration of several bones of the vertebrate jaw into the mammalian middle ear has – in addition to any direct enhancement and decoupling of mastication and hearing – considerably increased the genetic, regulatory, and developmental complexity of the mammalian ear. For example, the mammalian middle ear derives from both the first and second pharyngeal arches, whereas in other tetrapods only the second pharyngeal arch contributes to the ear bones (Sienknecht, 2013; Anthwal & Thompson, 2016). This increase in the number of genetic and developmental factors, in turn, likely has increased the genetic variation of ear morphology that natural selection can act on (Houle 1992; Hansen et al. 2011). Because of overlapping pleiotropic effects, it may also have increased the ability of different functional ear components to evolve independently (Wagner & Altenberg, 1996; Altenberg 2005; Mitteroecker, 2009; Pavlicev & Wagner, 2012). In other words, it has increased the evolutionary degrees of freedom for an independent adaptation of the different functional units of the ear - the number of genetic and developmental “knobs” for natural selection to turn.\n\nThis increased evolvability of the ear and its sensory functions may have contributed to the adaptive diversification of mammals into an astonishing range of niches, reflected by the high disparity to diversity ratios of mammals in general and of Afrotheria in particular. Furthermore, both mammals and its afrotherian subclade have hearing abilities that far exceed those of other tetrapod clades, being capable of perceiving infrasonic to ultrasonic sounds (Dooling et al. 2000; Mason 2013). Similarly, mammals also run the gamut of positional behaviours, which is mirrored almost entirely by Afrotherians alone (with the exception of flying and gliding). Although the current study did not comprise a comparison with non-mammals, our findings nonetheless offer support for this evolvability hypothesis.\n\nMaterials and Methods\n\nComparative sample\n\nThe sample consists of 20 Afrotheria and 20 non-afrotherian mammals considered to be their “analogues”. Analogues were identified based on their overall body morphology (e.g., the greater hedgehog tenrec, Setifer setosus, and the true hedgehog, Erinaceus europaeus), specific morphological traits such as relative hindlimb length (as in the case of the larger-bodied elephant\nshrews, e.g., Rhynchocyon cirnei, the mouse deer, Tragulus javanicus, and rabbit, Oryctolagus cuniculus), or locomotion and habitat (e.g., the subterraneous golden moles and true moles, or sea cows and cetaceans). The analogues mostly comprise non-afrotherian placentals. We also included a marsupial and a monotreme as phylogenetic outgroups, each of which also serve as an analogue. Most afrotherians have more than one analogue and some species share the same analogue (e.g., the European mole is an analogue for the two species of golden mole as well as for the rice tenrec). All taxa used in the study are presented in Figure 1 and Table 1. Elephants do not have any appropriate living analogues, but because they are very distinct extant afrotherians, we nonetheless included them in our study. The sample was carefully composed based on the phylogenetic, morphological, and ecological disparity within Afrotheria, their appropriate analogues, and the ability of our team to acquire high-resolution micro-CT scans of the desired taxa.\n\nTable 1 Afrotherian and non-afrotherian mammals used in this study, including the basis for analogy.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Afrotheria (common name)Non-afrotherian analogues (common name)Basis for analogy
Hemicentetes semispinosus (streaked tenrec), Setifer setosus (greater hedgehog tenrec), Tenrec ecaudatus (tailless tenrec)Erinaceus europaeus (European hedgehog)Overall appearance, body shape and size, foraging behaviour, terrestrial locomotion with climbing ability.
Limnogale mergulus (web-footed tenrec)Ornithorhynchus anatinus (duck-billed platypus), Sorex araneus (Eurasian shrew)Morphology (S. araneus), semi-aquatic lifestyle and habitat (O. anatinus)
Orizoryctes tetradactylus (four-toed rice tenrec)Talpa europaea (European mole)Overall appearance, fossorial locomotion,
Potamogale velox (otter shrew)Lutra lutra (Eurasian otter), Ornithorhynchus anatinus (duck-billed platypus)Semi-aquatic lifestyle, overall appearance (L. lutra), foraging behaviour
Amblysomus hottentotus (Hottentot golden mole), Chrysochloris asiatica (Cape golden mole)Cryptomys hottentotus (common mole-rat), Talpa europaea (European mole)Overall morphology, body size, fossorial locomotion, and subterranean habitat
Elephantulus rufescens (East African long-eared elephant shrew),Microtus arvalis (common vole), Mus musculus (house mouse), Rattus rattus (black rat),Overall body shape and size (except R. rattus), fast, terrestrial locomotion
\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Elephantulus rupestris (Western rock elephant shrew), Macroscelestes proboscideus (round-eared elephant shrew)Sorex araneus (Eurasian shrew)(although no living “microcursorial” mammals other than elephant shrews exist)
Petrodromus tetradactylus (four-toed sengi), Rhynchocyon cirnei (checkered sengi)Oryctolagus cuniculus (European rabbit), Rattus rattus (black rat), Tragulus javanicus (Javan mouse deer)Fast, terrestrial locomotion, relative hindlimb size (O. cuniculus, T. javanicus)
Orycteropus afer (aardvark)Manis tricuspis (tree pangolin), Tolypeutes matacus (southern three-banded armadillo)Fossorial/burrowing locomotion, foraging behaviour
Heterohyrax brucei (bush hyrax), Procavia capensis (rock hyrax)Marmota marmota (alpine marmot), Ochotona rufescens (Afghan pika)Rocky/open/mountainous habitat, terrestrial and climbing locomotion
Dendrohyrax arboreus (tree hyrax)Didelphis sp. (opossum) Tamandua mexicana (northern tamandua)Arboreality, climbing locomotion
Dugong dugon (dugong), Trichechus sp. (manatee)Odobenus rosmarus (walrus), Phoca vitulina (harbour seal), Sotalia fluviatilis (tucuxi/gray dolphin)Aquatic lifestyle, overall body size and shape (O. rosmarus), foraging behaviour (O. rosmarus)
Elephas maximus (Asian elephant)n/an/a
\n\nAll afrotherian “orders” are represented. Higher taxonomic groups of the analogues are as follows: Xenarthra (Tamandua mexicana, Tolypeutes matacus), Carnivora (Lutra lutra, Phoca vitulina, Odobenus rosmarus), Pholidota (Manis tricuspis), Cetartiodactyla (Tragulus javanicus, Sotalia fluviatilis), Eulipotyphla (Erinaceaeus europaeus, Sorex araneus, Talpa europaea), Rodentia (Mus musculus, Rattus rattus, Microtus arvalis, Marmota marmota, Cryptomys hottentotus), Lagomorpha (Oryctolagus cuniculus, Ochotona rufescens), Marsupialia (Didelphis sp.), and Monotremata (Ornithorhynchus anatinus).\n\nContextual data\n\nRelevant data on positional behaviour (locomotion and posture) and certain aspects of ecology were collected from the literature for each species. Data that directly measure auditory capacity could unfortunately not be included because common parameters of hearing ability (e.g., minimum/maximum perceived frequency, or frequency of greatest hearing sensitivity) were\nunknown for many species in the sample. However, habitat type (e.g., aquatic, subterranean, or ground-dwelling) carries information about the medium through which species detect sound and may thus indirectly also reflect basic aspects of hearing. Multiple aspects of ecology and positional behaviour were captured by 11 ordinal variables, presented in Table 2. Locomotion and postures of mammals vary extensively and they have been studied in varying levels of detail for the species in our sample. For the purpose of this study, positional behaviour was measured on an ordinal scale. Species’ mean body mass correlates with both ecology and locomotor behaviour across mammals, and so it was included as an additional contextual variable, measured on an interval scale.\n\nTable 2 The 12 contextual variables of body size, ecology, and positional behaviour used in this study.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
TypeVariables \\( p \\)Measurement levelsNotes
Body size\\( p = 1 \\) (body mass)Continuous (in g)
Food acquisition\\( p = 1 \\) (pursuit of moving prey)1 = never or rarely,
2 = mixed diet / sometimes,
3 = often or always
See text for further explanation.
Habitat type\\( p = 3 \\)
- aquatic;
- ground-dwelling;
- arboreal
1 = never or rarely,
2 = sometimes,
3 = often or always.
For aquatic only:
1 = never or rarely,
2 = moves freely on land and in water,
3 = mainly aquatic, only rests on land,
4 = strictly aquatic.
Subterranean habitats are captured by a fossorial mode of locomotion (see below).
Mode of locomotion\\( p = 4 \\)
- scansorial/climbing;
- cursorial/running;
- leaping/jumping/hopping;
- fossorial/burrowing
1 = typical/frequent,
2 = occasional,
3 = atypical/rare.
Dimensionality of movement\\( p = 1 \\) (moves three-dimensionally)1 = never or rarely,
2 = sometimes,
3 = often or always.
Refers to whether animals move in 3D at any given point in time.
Agility\\( p = 1 \\) (agility)1 = extra slow,
2 = slow,
Capturing both speed and manoeuvrability.
\n\n \n \n \n \n \n \n \n \n \n \n \n \n
3 = medium slow,
4 = medium,
5 = medium fast,
6 = fast
Adapted from Spoor et al. 2007.
Posture\\( p = 1 \\)
(orthogrady vs. pronogrady)
1 = fully orthograde,
2 = mostly orthograde,
sometimes pronograde,
3 = mixed,
4 = mostly pronograde,
sometimes orthograde,
5 = fully pronograde
Orthograde = trunk is upright;
pronograde = trunk is horizontal.
No taxa in this study are fully orthograde.
\n\nWith the exception of body mass, all variables were scored on an ordinal scale.\n\nBody mass was collected from PanTHERIA (Jones et al. 2009), and the other data were collected from mammalogical reference works (Wilson & Mittermeier 2009, 2011; Mittermeier & Wilson, 2014, 2015, 2018; Wilson et al. 2016, 2017), supplemented by other written sources (Spoor et al. 2007; Lovegrove & Mowoe 2014) or, where necessary, videographic documentation of species’ positional behaviour. We define agility as a combination of speed and manoeuvrability (adapted from Spoor et al. 2007). We defined agility as a combination of speed and manoeuvrability (adapted from Spoor et al. 2007).\n\nPhylogeny\n\nThe phylogenetic position of Afrotheria within Placentalia is not fully resolved, but molecular phylogenetic data supports Afrotheria as a monophyletic lineage separate from the more speciose clade Boreoeutheria (comprising Laurasiatheria and Euarchontoglires) (e.g., Stanhope et al. 1998; Bininda-Emonds et al. 2007; dos Reis et al. 2012; Meredith et al. 2013; see also refs in Tabuce et al. 2008). Most likely, Afrotheria is either sister to Boreoeutheria and Xenarthra combined (“Exafroplacentalia”), or it forms a clade together with Xenarthra (“Atlantogenata”) which is sister to Boreoeutheria (reviewed in Zachos 2020). We followed the Atlantogenata hypothesis herein and employed the phylogeny in Fig. 1, downloaded from www.VertLife.org (Upham et al. 2019).\n\nData acquisition\n\nWe landmarked a single bony labyrinth per species. As we are dealing with a sample of disparate taxa, most of which are separated by long evolutionary time spans, interspecific variation likely far exceeds within-species variation. Contextual data were also only available on a species level. Bony labyrinth morphology is only slightly sexually dimorphic (Braga et al., 2019; Boucherie et al., 2021), likely rendering dimorphism negligible compared to the disparity across species (Gonzales et al.,\n2019). Similarly, asymmetry between left and right ears is likely minute relative to the variation between species (Della Santina et al., 2005; Lebrun et al., 2021). Hence, we did not consider within-species variation, sexual dimorphism, and bilateral asymmetry; instead we aimed to maximise taxonomic, phylogenetic, and ecological breadth of the sample.\n\nWe downloaded the microCT scans of 13 crania from MorphoSource (www.MorphoSource.org, Duke University), which have resolutions ranging from 7.88 to 82.67 μm (isometric voxel size), except for the aardvark (93*93*200 μm) and the opossum (59.6*59.6*132.0). We also scanned crania of 24 species curated at the Natural History Museum of Vienna, Austria, with resolutions ranging from 7.13 to 106.67 μm, as well as three specimens from the Palaeontology Institute of the University of Vienna, Austria, with resolutions ranging from 9.62 to 24.95 μm. For each specimen, we virtually extracted the surface of one bony labyrinth using the software Amira (Thermo Fisher Scientific) version 2020.2.\n\nTo quantify the morphology of the bony labyrinth (Fig. 2, Table 3), we placed 13 anatomical landmarks (LM) and 111 semilandmarks (SL) on every microCT scan. Apart from (semi)landmarks placed on the surface to quantify the centre of the cochlear window (LM 11) and the outline of the vestibular window (LM 12-13 and six semilandmarks), we positioned all landmarks on the centrelines of the semicircular canals, the common crus and the cochlea, computed using the AutoSkeleton module in Amira. Following Gunz et al. (2012), our anatomical landmarks included nine landmarks (LM 1-9) on the three semicircular canals: the proximal and distal extremities of each ampulla (LM 1, 2, 5, 6, 8, 9), the junction of the anterior and posterior semicircular canals at the common crus (LM 3), and the insertion of the common crus (LM 4) and the lateral canal (LM 7) on the vestibule. A final anatomical landmark (LM 10) was placed at the apex of the cochlea. The morphology of each canal was described by a curve comprising 20 semilandmarks, including two semilandmarks on the ampulla. We also placed five semilandmarks on the common crus, and 40 semilandmarks on the cochlea. In many species, the posterior segment of the lateral semicircular canal is partially fused with the ampulla of the posterior canal before entering the vestibule, thus forming a secondary common crus. In this case, we landmarked the lateral semicircular canal up to the vestibule as if it were separate from the ampulla, because the corresponding membranous ducts are not fused internally (Berlioz et al., 2021).\nTable 3 Definition of the 13 anatomical landmarks and the 111 semilandmarks on the bony labyrinth.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
#TypeDefinition
Anatomical landmarks
1ASC ampulla to vestibule (midline)
2ASC ampulla to slender part of ASC (midline)
3CC to ASC & PSC (midline)
4CC to vestibule (midline)
5Slender part of PSC to ampulla (midline)
6PSC ampulla to vestibule (midline)
7Slender part of LSC to vestibule (midline)
8Slender part of LSC to ampulla (midline)
9LSC ampulla to vestibule (midline)
10Helicotrema
11Centre of the round window
12Posterior extremity of the axis of maximum elongation of the oval window
13Anterior extremity of the axis of maximum elongation of the oval window
Semilandmarks
1-20SL (20)Midline curve of the ASC: LM 1 → 2 → 3 (2 SL: ampulla, 18 SL: slender part)
21-40SL (20)Midline curve of the PSC: LM 6 → 5 → 3 (2 SL: ampulla, 18 SL: slender part)
41-45SL (5)Midline curve of the CCR: LM 3 → 4
46-65SL (20)Midline curve of the LSC: LM 9 → 8 → 7 (2 SL: ampulla, 18 SL: slender part)
66-105SL (40)Midline curve of the cochlea: apical side of the RW → LM 10
106-111SL (6)Outline of the oval window: LM 13 → 12 (inferior), then 12 → 13 (superior)
\n\nLandmarks 1-10 and all semilandmarks are defined as in Gunz et al. (2012), except for the different numbers of semilandmarks along each curve. For the semilandmarks, we indicate the order in which they are placed between anatomical landmarks. LM, anatomical landmark, SL, semilandmark. See Fig. 2 for visualisation.\nData analysis\n\nIn order to standardise for overall location, scale, and orientation of the landmark configurations, we performed a Generalised Procrustes Analysis (GPA) with mirroring allowed because the sample comprised both left and right ears (Rohlf & Slice, 1990; Mitteroecker & Gunz, 2009). We chose the minimum bending energy as a criterion to slide semilandmarks (Gunz et al., 2005; Gunz and Mitteroecker, 2013). Due to the huge variation in cochlear morphology, the magnitude of sliding per iteration was reduced by a factor of 0.1 and the number of iterations was increased accordingly.\n\nIn the case of adaptive convergence, a given afrotherian species is expected to share more similarities in labyrinth morphology with analogues than non-analogues. In order to test this, we computed pairwise Procrustes distances between taxa and compared average distances for pairs of analogues and for pairs of non-analogues. Because elephants do not have a living analogue, we excluded this species in the computations. We also computed the average Procrustes distance for pairs of afrotherians, to compare the signal of convergent evolution with that of phylogenetic history. Significance tests of the H0 of equal average distances were based on permutation tests that permuted the affiliation of species across Afrotheria-analogue pairs.\n\nTo explore the morphological diversity of the bony labyrinth across species, we performed a principal component analysis (PCA) of the Procrustes shape coordinates (results are shown in the Supplementary Information). We also performed a two-block partial least squares (2B-PLS) analysis to investigate the association between bony labyrinth shape and the 12 contextual variables (Rohlf & Corti, 2000; Bookstein et al., 2003; Mitteroecker & Bookstein, 2007). The contextual variables were mean-centred and scaled to unit variance. Additionally, we conducted a phylogenetic 2B-PLS, based on phylogenetic generalised least squares (PGLS; Adams & Felice, 2014) and the phylogeny in Fig. 1, in order to assess whether the associations between bony labyrinth shape and the contextual variables were mediated through the species’ phylogenetic relationships (Figs. S3-4). PCA, 2B-PLS, and shape visualisations were performed using the software Wolfram Mathematica 12. Scatter plots were generated using the packages ggplot2 3.4.2 (Wickham, 2016) and ggrepel 0.9.3 (Slowikowski, 2023) of the software R version 4.2.2 (R Development Core team, 2022).\n\nFinally, to evaluate to what extent the associations between bony labyrinth shape, ecology and positional behaviour are phylogenetically patterned, we quantified the phylogenetic signal of the\nPLS dimensions by means of Blomberg’s \\( K \\) (Blomberg et al. 2003). Phylogenetic signal, or the tendency for closely related species to resemble each other in ecology and/or morphology, is expected to be high when close relatives are more similar to each other than they are to distant relatives. Conversely, phylogenetic signal is low when trait values vary randomly across the phylogenetic tree or when distant relatives tend to resemble each other more than closely related species, as in evolutionary convergence (e.g. Blomberg et al. 2003; Revell et al. 2008). To compute Blomberg's \\( K \\) for the shape and context scores along the PLS dimensions we used the function ‘phylosig’ from the package phytools (Revell 2012) and the phylogenetic tree, with branch lengths scaled to time, in Fig. 1.\n\nData availability\n\nAll data are available in an online data repository (https://osf.io/9mtwh/?view_only=88a550a637f84615b5666d69278309d4).\n\nAcknowledgements\n\nP.M., N.D.S.G., C.P. and A.L.M. disclose support for the research of this work from the Austrian Science Fund [FWF grant number P33736]. The California Academy of Sciences, Museum of Vertebrate Zoology at Berkeley, as well as Museum of Comparative Zoology, Harvard University, and Peabody Museum, Yale University provided access to some CT-scans, the collection of which was funded by oVert TCN. Robert Asher provided access to data originally appearing in Asher et al. 2017 (http://dx.doi.org/10.1080/02724634.2017.1317638). 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Click to download.\n\n• GrunstraetalSupplementaryInfo.docx"} {"paper_id": "prb69", "title": "", "text": "Environment-induced heritable variations are common\n\nYuan-Ye Zhang\nzhangyuanye@xmu.edu.cn\n\nXiamen University https://orcid.org/0000-0002-8636-2242\nXiaohe Lin\nXiamen University\nJunjie Yin\nXiamen University\nYifan Wang\nXiamen University\nJing Yao\nXiamen University\nQingshun Q. Li\nGraduate College of Biomedical Sciences, Western University of Health Sciences, Pomona, CA91766, USA\nVit Latzel\nAcademy of Sciences of the Czech Republic\nOliver Bossdorf\nUniversity of Tübingen https://orcid.org/0000-0001-7504-6511\n\nArticle\n\nKeywords:\n\nPosted Date: October 20th, 2023\n\nDOI: https://doi.org/10.21203/rs.3.rs-3416426/v1\n\nLicense: © This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: There is NO Competing Interest.\nVersion of Record: A version of this preprint was published at Nature Communications on May 30th, 2024. See the published version at https://doi.org/10.1038/s41467-024-49024-3.\nEnvironment-induced heritable variations are common\n\nXiaohe Lin1†, Junjie Yin1†, Yifan Wang1†, Jing Yao1, Qingshun Q. Li1,2, Vit Latzel3, Oliver Bossdorf4, Yuan-Ye Zhang1*\n\n1Key Laboratory of the Ministry of Education for Coastal and Wetland Ecosystems, College of the Environment and Ecology, Xiamen University, Xiamen, Fujian, China\n2Biomedical Sciences, College of Dental Medicine, Western University of Health Sciences, Pomona, California, USA\n3Institute of Botany of the CAS, Zamek 1, 252 43 Pruhonice, Czech Republic\n4Institute of Ecology & Evolution, University of Tübingen, Auf der Morgenstelle 5, 72076 Tübingen, Germany\n† These authors contributed equally to this work.\n* Correspondence: zhangyuanye@xmu.edu.cn (Y.-Y.Z.)\nAbstract\nParental or ancestral environments can induce heritable phenotypic changes, but whether such environment-induced heritable changes are a common phenomenon remains unexplored. Here, we subjected 14 genotypes of Arabidopsis thaliana to 10 different environmental treatments and observed phenotypic and genome-wide gene expression changes over successive generations. We found that all environmental treatments caused heritable phenotypic and gene expression changes, with a substantial proportion stably transmitted over all observed generations. Intriguingly, the susceptibility of a genotype to environmental inductions could be predicted based on the transposon abundance in the genome. Our study thus challenges the classic view that the environment only participates in the selection of heritable variation and suggests that the environment can broadly contribute to the generation of heritable variation.\nIntroduction\n\nHeritable variation is the foundation of biodiversity and adaptation to the changing climate\\(^{1,2}\\), ultimately generated through mutations and moulded by forces of environmental selection—a tenet well established in textbooks\\(^3\\). Several pioneering studies suggested that heritable variation is also directly introduced by parental or ancestral environments\\(^{4-7}\\), causing stably transmitted phenotypic and gene expression changes that potentially enhance offspring resistance to environmental stress\\(^{4,7,8}\\). However, whether such environment-induced heritable changes are a common phenomenon remains unexplored, and it is also unknown whether the phenomenon is an occasional exception or a fundamental principle. Therefore, exploring the prevalence of environment-induced heritable changes will challenge the textbook knowledge of the origin of heritable variation and provide critical insights for predicting the adaptive response to global environmental changes.\n\nThe phenomenon in which the parental or ancestral environment induces offspring phenotypic changes is conventionally referred to as the parental or transgenerational effect\\(^4\\), and the major challenge in understanding the prevalence of this phenomenon could be the scale of the experiments\\(^9\\). Expanding the scale of these experiments to include different genetic backgrounds has revealed that such environment-induced changes are genotype specific\\(^{10,11}\\) and predictable based on the climate of the genotype’s origin\\(^{12,13}\\), while this predictability decreases when sacrificing the number of genotypes to include various environmental treatments\\(^9\\). Nevertheless, these studies span only one or two offspring generations, and it is unclear whether environment-induced changes are heritably stable. A large-scale experiment encompassing multiple genotypes, environments, and generations is necessary to reveal the prevalence and predictability of environment-induced heritable changes.\n\nTo address the prevalence and predictability of environment-induced heritable changes, we subjected 14 natural accessions (genotypes) of *Arabidopsis thaliana* to 10 ancestral environmental treatments and assessed environment-induced phenotypic changes over four offspring generations (Test I, Fig. 1, Extended Data Fig. 1a, Supplementary Table 1). To explore the reproducibility of environment-induced\nchanges, we planted all four offspring generations together under uniform conditions to eliminate any heterogeneity between generations in the growth conditions (Test II, Fig. 1). Besides performing phenotypic observations, we analysed the genome-wide gene expression of samples from Test II to investigate whether heritable phenotypic changes were predicted by heritable gene expression changes and whether the induced expression changes were nonrandom with respect to environments.\n\nResults\n\nPrevalence of environment-induced heritable phenotypic changes\n\nIn the ancestral generation, we subjected A. thaliana genotypes to the control environment and 10 treatment environments: jasmonic acid addition (JA), control for JA, nutrient addition, nutrient depletion, leaf removal, drought, low and high concentrations of cadmium, and low and high concentrations of salinity. The statistics showed that the genotype, environmental treatment and their interaction significantly affected all phenotypes measured (except for the interaction effect on flowering time, Supplementary Table 2). Among the specific treatments, nutrient addition significantly increased aboveground biomass, and jasmonic acid addition slightly enhanced fruit production, representing benign environments (Extended Data Fig. 2a). Other treatments significantly decreased fruit production and thus represented stressful environments (Extended Data Fig. 2a). High concentrations of cadmium and salinity generated more stressful conditions than the corresponding low-concentration treatments, resulting in either smaller plants with fewer fruits or shorter plants with fewer fruits (Extended Data Fig. 2a). Therefore, our experiment provided a gradient of benign and stressful environments to assess their effects on offspring phenotypes.\n\nIn the offspring generations, we found little evidence of significant main effects of the ancestral environments on phenotypes but significant genotype-by-ancestral_environment interactions (G × A.E) on all phenotypes measured except for fruit number (Extended Data Fig. 2b, Supplementary Table 2). More importantly, the G × A.E interactions remained significant in the four successive offspring generations. These results demonstrated that the effects of the ancestral environments on offspring phenotypes (i.e., transgenerational effects) depended on the genotypes and persisted for\nfour offspring generations. To understand the stable transmission of such genotype-specific changes caused by ancestral environments, we estimated the effect sizes of changes for different genotypes and environments and plotted them in the order of generations (Fig. 2a). The plot showed considerable variation in the magnitude and direction of the phenotypic changes. In some notable cases, such as the response of genotype Abd-0 to high cadmium and the response of TRE-1 to high salinity, we found that the environment-induced phenotypic changes were stably transmitted over four generations of offspring (Fig. 2a). Therefore, our study demonstrates that environment-induced phenotypic changes are genotype-specific and can be stably transmitted (i.e., are heritable) for at least four offspring generations.\n\nWhile several cases of environment-induced heritable changes have been identified, a fundamental question remains: how prevalent are these changes across different environments? To answer this question, we transformed the quantitative estimates of effect sizes into qualitative assessments, defining an environment-induced change as occurring when the effect size significantly deviated from zero. The occurrence data revealed environment-induced phenotypic changes in each genotype and environment (Fig. 2b). Importantly, a substantial proportion (36.8% 10.4%, and 7.5%) of these changes occurred in two, three, and four offspring generations, suggesting that these environment-induced changes were heritable. Furthermore, we observed heritable changes (changes occurring in at least two generations) in all environments and persistent changes (changes occurring in three generations and remaining significant in the fourth generation) in seven environments (Fig. 2b). Consequently, these findings demonstrate that environment-induced heritable changes commonly occur across various environments.\n\nPredictability and reproducibility of environment-induced phenotypic changes\n\nThe qualitative data revealed that the genotype, ancestral treatment, offspring generation, and phenotype significantly affected the occurrence of environment-induced phenotypic changes (Fig. 3a). The frequency of occurrence of fruit number was lowest among phenotypes and was marginally significantly lower than those of flowering time and plant height. This frequency also varied across different offspring\ngenerations, but no consistent decline was observed over successive generations. In general, the magnitude of the ancestral treatment effect did not predict the frequency of occurrence. For instance, the leaf removal treatment, affecting only fruit number, appeared to be much less stressful than the low-salinity treatment (affecting four phenotypes), but the occurrence frequencies associated with these two treatments were similar (Extended Data Fig. 2a, Fig. 3a). Only within the same treatment type was a higher intensity of treatment associated with an increase in the occurrence frequency of induced phenotypic changes (high vs. low concentrations of cadmium/salinity, Fig. 3a).\n\nAmong the factors affecting the occurrence of environment-induced changes, genotype emerged as the primary explanatory variable. This factor accounted for the largest proportion of the variance in occurrence frequency (Fig. 3a), and removing the three genotypes with the highest frequencies (TRE-1, Abd-0, Sap-0) rendered the effect of ancestral environments on occurrence insignificant (Extended Data Fig. 3a). To explore which factor predicted the susceptibility of a genotype to environmental induction, we regressed the occurrence frequency of genotypes against different explanatory variables (climate of origin, methylation levels, and transposon abundance) and found that the abundance of transposons in the Gypsy (r = -0.840) and MuDR (r = 0.815) superfamilies explained a significant proportion of the variation (Fig. 3b, Extended Data Fig. 3b). Therefore, these findings suggest that genotype may be a primary predictor of the occurrence of environment-induced changes, and this property of a genotype can be predicted by the number of transposons in its genome.\n\nAlthough the occurrence of environment-induced changes is predictable to some extent, predicting the effect sizes of these changes proved challenging. Consistent with a previous study9, the responses of the ancestors showed little, if any, predictability related to the effect sizes of offspring (Fig. 3c). Nevertheless, it was encouraging to find that the effect sizes of offspring could exceed the range of ancestral responses, as observed for flowering time (Fig. 3c). For this trait, the fixed G × A.E effect also explained a greater proportion of the total variation than G × E (Extended Data Fig. 3c). Compared to ancestor-offspring correlations, the coefficients estimated between offspring generations were significantly greater and consistently significantly deviated\nfrom zero, except for fruit number, for which the coefficient reached 0.682 (median = 0.474) (Fig. 3d, Extended Data Fig. 4a-b). The coefficient increased to 0.857 (median = 0.614) when including only significant effect sizes in the analysis and declined substantially and insignificantly deviated from zero for most cases when excluding significant effect sizes from the analysis (Extended Data Fig. 4c). A similar pattern of correlation coefficients was also observed when comparing effect sizes between Test I and Test II (Fig. 3e, Extended Data Fig. 4a, please also see below for Test II). Intriguingly, when we scaled down the experiment to include only one genotype (but multiple treatments) or one treatment (but multiple genotypes), we found that the chances of obtaining significantly correlated effect size correlations between generations declined substantially (Extended Data Fig. 4d). Therefore, our study demonstrates that the effect sizes of environment-induced phenotypic changes are reproducible between offspring generations and tests, and conducting large-scale experiments to obtain abundant significant effect sizes is crucial for achieving this reproducibility.\n\nDespite the findings regarding the predictability and reproducibility of environment-induced changes, some unresolved questions remained: why did some significant phenotypic changes disappear in one generation but reappear in the next (Fig. 2b), and why did the occurrence frequency of induced changes vary between offspring generations (Fig. 3a)? A potential explanation is that the growth conditions differed between offspring generations, as evidenced by significant phenotypic variation between generations in the control group (Extended Data Fig. 2c, Supplementary Table 3). Such variation may also contribute to the inconsistent effect sizes observed between generations (significant G × A.E × F, Supplementary Table 4). To eliminate the influence of variable growth conditions, we conducted a second test of ancestral treatment effects (Test II), where we selected a subset of 10 genotypes and five treatments and grew F1 to F4 plants together under the same conditions (Fig. 1). Consistent with the results of Test I, Test II revealed that the effect of ancestral environments depended on the genotypes (Extended Data Fig. 5a, Supplementary Table 5); that environment-induced heritable changes were common across environments\n(Extended Data Fig. 6); that the occurrence frequency of these changes varied significantly between genotypes (Extended Data Fig. 7a); and that the variation among genotypes could be predicted by the abundance of several transposon superfamilies, including HAT (\\( r = 0.893, P = 0.041 \\)), Mariner (\\( r = 0.873, P = 0.053 \\)), and MuDR (\\( r = 0.846, P = 0.071 \\)) (Extended Data Fig. 7b-c).\n\nSurprisingly, the repeatability of the effect sizes between generations in Test II did not increase compared to that in Test I (Fig. 3d, Extended Data Fig. 7d). We still found significant phenotypic variations between generations in the control group (Extended Data Fig. 5b, Supplementary Table 6), and the genotype-specific ancestral treatment effects varied significantly between generations for flowering time and aboveground biomass (significant G \\( \\times \\) A.E \\( \\times \\) F, Supplementary Table 7). As all plants in Test II were grown under the same conditions, the observed generation effects could only be introduced by different growth conditions of previous generations in Test I. Taken together, these results suggest that both the current conditions and conditions of previous generations can affect the measurements of environment-induced changes, and conducting large-scale experiments under well-controlled conditions is the key to achieving high reproducibility and an in-depth understanding of environment-induced changes.\n\nEnvironment-induced heritable gene expression changes\n\nIn Test II, we conducted transcriptomic analysis of offspring generations (F1-F4) to investigate genome-wide gene expression changes induced by ancestral environments (Fig. 1). The patterns of genome-wide gene expression were primarily determined by genotypes (Extended Data Fig. 8a), with noticeable treatment-specific differentiation observed only in the high-cadmium treatment of Abd-0 and drought treatment of TRE-1 (Extended Data Fig. 8b). The number of differentially expressed genes (DEGs) induced by the ancestral treatment ranged from 146 to 3694 (Fig. 4a), which varied significantly between genotypes but not between environmental treatments or generations (Fig. 4b). Importantly, a significant proportion (15.5%, 3.43%, and 1.54%) of these genes exhibited differential expression in two, three, and four offspring generations (Fig. 4c), indicating that the gene expression changes were\nheritable. We considered those genes that were differentially expressed for at least two generations to be heritable DEGs, and the number of heritable DEGs ranged from 69 to 2668. Importantly, we identified heritable DEGs in each genotype and environment; heritable DEGs that remained differentially expressed over four offspring generations were also found in each environment (Fig. 4c). The number of heritable DEGs for each genotype and treatment was significantly related to the occurrence frequency of induced phenotypic changes (Extended Data Fig. 9a) and was also significantly explained by the number of transposons in several superfamilies (Fig. 4d, Extended Data Fig. 9b). Therefore, these results demonstrate that environment-induced heritable gene expression changes were common across different environments, and the number of genes showing heritable expression changes can be predicted by the abundance of transposons in the genomes.\n\nAn important unanswered question is whether the induced gene expression changes are directional or unidirectional. If these changes are directional, we expect the DEGs induced by different environments to have distinct functions. To test this hypothesis, we conducted GO and KEGG functional enrichment analyses of heritable DEGs and found that 80.2% (73 out of 91) of enriched GO terms and 58% (27 out of 46) of enriched KEGG pathways were shared between treatments (Fig. 5a-b, Extended Data Fig. 9c-d). The overlapping functions appeared to be primarily associated with the stress response (Fig. 5a) and metabolic pathways (Extended Data Fig. 9c). These results indicated that, contrary to our expectations, heritable DEGs induced by different environmental treatments were functionally similar, which may be associated with these treatments (drought and low and high concentrations of cadmium) generating similar stresses (i.e., inducing hypoxia in the root system).\n\nIntriguingly, in addition to being shared between different environmental treatments, a substantial proportion of terms/pathways were also shared between genotypes (Fig. 5b, Extended Data Fig. 9d). The shared terms/pathways likely originated from heritable DEGs that were shared between treatments and/or genotypes (Fig. 5b-c, Extended Data Fig. 9d-e). As the heritable expression changes in these genes were repeatedly induced in two or more treatments or genotypes, these genes could be\nconsidered susceptible to environmental induction. We hypothesize that the susceptibility of these genes is explained by certain genomic features, such as the abundance of transposons in their promoter and gene body regions. To test this hypothesis, we identified all heritable DEGs shared between genotypes or treatments (Extended Data Fig. 10a) and found that the abundance of members of several superfamilies, including Gypsy, HAT, Mariner, and Helitron, upstream and body of these susceptible genes was significantly higher than that of background genes (Extended Data Fig. 10b). Therefore, these results suggest that environment-induced changes may be nonrandom in the sense of genomic features.\n\nTo investigate whether the heritable phenotypic changes were associated with heritable gene expression changes, we focused on the phenotype of flowering time, which has a comparatively well-characterized molecular basis\\(^{14-16}\\). Among the 79 genes underlying flowering time changes identified in the literature, 16 were differentially expressed in at least one genotype or treatment, and seven were heritable DEGs (Extended Data Fig. 10c). The heritable gene expression changes of six genes co-occurred with heritable flowering time changes, including the early flowering of Abd-0 in response to high cadmium and drought-induced late flowering in TRE-1 in response to drought (Fig. 5d, Extended Data Fig. 6). In Abd-0, ancestral treatment with high cadmium caused downregulation of *FLC* and *MAF4* and upregulation of *FT* and *SOC1*, promoting early flowering (Fig. 5d). In TRE-1, ancestral drought treatment caused the upregulation of *MAF3* and *MAF4* and downregulation of *FT* and *SOC1*, which was associated with delayed flowering time (Fig. 5d). *FLC* is the primary determinant of the vernalization requirement and negatively regulates the expression of *FT* \\(^{17,18}\\). *MAFs* are paralogues of *FLC*, which act redundantly with *FLC* as floral repressors\\(^{17,19}\\). Therefore, these results suggest that heritable expression changes in key genes underlie environmentally induced heritable phenotypic changes.\n\n**Discussion**\n\nHere, we conducted a large-scale multigenerational experiment, and the main finding of our study was that environment-induced heritable changes were caused by each ancestral environmental treatment. These results extend the understanding of the\nphenomenon of environment-induced heritable changes beyond occasional findings under specific environmental conditions\\(^{4,5,13}\\) and suggest that this phenomenon could be a fundamental principle of genetics. Our work challenges the textbook understanding that environments are only involved in the selection of heritable variation\\(^{3}\\) and suggests that environments are broadly involved in the generation of heritable variation.\n\nThe scale of our experiment allowed us to explore the stochasticity of environment-induced heritable changes and reveal genotypes with a higher abundance of transposons that are more susceptible to environmental inductions. Furthermore, our study revealed that genes with more transposons are also prone to environmental induction. These results indicate that transposons play a central role in mediating environment-induced changes, which could occur through epigenetic modifications of transposons (i.e., DNA methylation\\(^{20,21}\\) and RNA interference\\(^{22}\\)) that simultaneously regulate the expression of downstream genes or through *de novo* transposon insertions that alter gene expression patterns\\(^{23,24}\\). The rates of *de novo* transposon insertions have been found to increase under both biotic and abiotic stresses\\(^{25}\\), and these rates varied by orders of magnitude between genotypes\\(^{26}\\). A comprehensive analysis that connects environment-induced variations with the mechanisms controlling transposon activity is an essential next step to revolutionize our fundamental understanding of the origins of genetic variation.\n\nThe finding that environment-induced heritable changes are common across environments also indicates that, besides standing genetic variation within populations\\(^{27,28}\\), *de novo* heritable variations caused by environmental changes can serve as another primary source for rapid adaptation. These *de novo* heritable variations may arise from the mechanisms discussed earlier, including epigenetic changes (DNA methylation\\(^{29}\\), histone modifications\\(^{30}\\), and small interfering RNAs\\(^{6}\\)) or *de novo* insertion of transposons\\(^{23,24}\\). Therefore, investigating environment-induced heritable changes not only expands our knowledge in the context of basic research but also contributes to assessing the evolutionary potential and consequences of populations under global environmental changes.\nFig. 1 | Design of the experiment. The experiment subjected 14 genotypes of Arabidopsis thaliana to one control and ten environmental treatments and lasted seven generations. Plants were grown for two generations before launching the “ancestral generation” to eliminate variation due to seed collection or storage. The ten ancestral environmental treatments included jasmonic acid addition (JA), control for JA, nutrient addition, nutrient depletion, leaf removal, drought, low cadmium, high cadmium, low salinity and high salinity. The control and each treatment group consisted of 12 and six replicates, resulting in a total of 1008 lines. To test the ancestral environmental effect on offspring, we established Test I to grow all these lines in the control environment over four successive generations (F1 to F4). To explore the reproducibility and assess the gene expression changes, we established Test II, where we selected ten genotypes and six environments and planted all four offspring generations together in the control environment.\nFig. 2 | Prevalence of environment-induced heritable phenotypic changes. a, The effect sizes of environment-induced phenotypic changes measured in Test I. b, The occurrence of significant and marginally significant environment-induced changes and this occurrence summed over phenotypes. Environment-induced heritable changes (significant changes in at least two generations) marked with dash lines are found in each environment.\nFig. 3 | Predictability and reproducibility of environment-induced phenotypic changes. a, The occurrence frequency of significant environment-induced changes varied between genotypes, ancestral environmental treatments, offspring generations and phenotypes. b, The occurrence frequency of different genotypes could not be predicted from the climate at origin or methylation, but from the abundance of transposons in certain superfamilies. c, The effect sizes of induced changes show limited correlations with ancestor response. d, The effect sizes are quantitatively reproducible between offspring generations. e, The effect sizes are quantitatively reproducible between Test I and Test II. Solid circles represent significant effect sizes in either the generation or test, and transparent circles represent nonsignificant effect sizes in both generations and tests. FT: Flowering time; PH: Plant height; AB: Aboveground biomass; RD: Rosette diameter; FN: Fruit number.\nFig. 4 | Environment-induced heritable gene expression changes are found in each ancestral environmental treatment, and the predictability of environment-induced gene expression changes. **a**, The number of differentially expressed genes (DEGs) for each genotype, ancestral environment treatment and offspring generation. **b**, The number of DEGs varied significantly between different genotypes, but not between treatments and generations. The error bars indicate the standard error. **c**, The number of heritable DEGs (genes significantly differentially expressed in two, three or four offspring generations) for each genotype and treatment. **d**, The number of heritable DEGs for different genotypes could be predicted from the abundance of transposons in several superfamilies.\nFig. 5 | Heritable gene expression changes induced by various environments were functionally similar and explained the induced phenotype changes. a, Gene ontology (GO) enrichment results of heritable differentially expressed genes (DEGs) show that induced gene expression changes are functionally similar between environmental treatments and genotypes. b, Venn plot shows the numbers of shared terms between environmental treatments and genotypes. c, Venn plot shows the number of heritable DEGs within the shared terms. d, The heritable DEGs explained the environment-induced heritable changes in flowering time.\nMethods\n\nPlant materials and the experimental design\n\nArabidopsis thaliana is a model plant species for molecular biology research and is increasingly used to address questions in ecology and evolution31. It is a self-pollinating annual weed that originates from North Africa32 and is broadly distributed across Europe, Asia, and North America. Seeds collected from different geographic sites, known as natural accessions or ecotypes, are preserved at the Arabidopsis Biological Resource Centre (ABRC). As this species is predominantly selfing, different accessions are also taken as different genotypes11,13. Here, we adopted 14 A. thaliana genotypes ordered from the ABRC, including Abd-0 (from Aberdeen, UK), Ang-0 (Namur, Belgium), Col-0 (Columbia, US), Dja-1 (Chui, Kyrgyzstan), En-1 (Frankfurt, Germany), Fei-0 (Aveiro, Portugal), Kar-1 (Suusamyr, Kyrgyzstan), Ler-0 (Munich, Germany), Olympia-2 (Olympia, Greece), Sap-0 (Hokkaido, Japan), Tol-0 (Ohio, USA), TRE-1 (Marne, France), Tri-0 (Sevilla, Spain) and Ws-2 (Belarus, Belarus) (Extended Data Fig. 1a, Supplementary Table 1). Four seeds per genotype were planted in a common environment for two generations to eliminate the variation due to seed collection or storage. In the second generation, seeds of the four resulting plants were pooled for each genotype to establish the ancestral generation.\n\nTo investigate whether environmental changes caused heritable changes in offspring (i.e., transgenerational effects), we subjected the ancestral generation to different environmental treatments and assessed the offspring phenotypic changes over four generations in a common environment. The ancestral environments included the control and ten treatments: jasmonic acid addition (JA), control for JA, nutrient addition, nutrient depletion, leaf removal, drought, low cadmium, high cadmium, low salinity and high salinity (Fig. 1). Each treatment included six replicate plants per genotype, and the control included 12 plants per genotype, resulting in 1008 plants grown or lines established in the ancestral generation. Following the single-seed descendant approach, the offspring of all lines were grown generation-by-generation in the control environment for four generations (F1-F4) (Test I), and altogether, 4032 plants were grown for Test I.\nThe growth room contained four shelves, each with four layers (Extended Data Fig. 1b). In each layer, we organized the plants into six rows and 14 columns, and this organization allowed one replicate per treatment/genotype to be planted in two layers. For one replicate of the ancestral generation, treatments were randomly assigned to rows in two layers, and genotypes were distributed randomly among columns in a row (Extended Data Fig. 1c). For the offspring of this replicate, we assigned them to two random layers and distributed the plants randomly among different positions (Extended Data Fig. 1c). All randomization was conducted using the “RAND” function in Excel.\n\nTo eliminate the potential influence of growth conditions that varied between generations, we planted all four offspring generations together in the control environment (Test II). Due to limited space in the growth room, Test II included a subset of ten genotypes (Abd-0, Col-0, Ang-0, Dja-1, Fei-0, Ler-0, Sapporo-0, Tol-0, TRE-1 and Tri-0) and six different environments (the control, drought, low cadmium, high cadmium, low salinity and high salinity) and a total of 1440 plants. We adopted a completely random design, assigning the 1440 plants randomly into positions among the 16 layers, with six rows and 15 columns each (Extended Data Fig. 1c). Due to the insufficient storage of seeds, especially for the F1 generation, Test II eventually involved 1252 plants. The randomization was conducted using the “RAND” function in Excel.\n\nGrowth conditions, phenotype measurements, and sample collection\n\nThe experiment was conducted by four graduate students who assisted each other (Extended Data Fig. 1d). Prior to sowing, we placed 10-15 seeds in a 2 mL centrifuge tube, added 1 mL of sterilized distilled water, and kept the tubes in a 4 °C freezer in the dark for 7 days. The soaked seeds were then evenly distributed into pots (5.5 × 5.5 × 6.0 cm) filled with a mixture of 1:1 sterilized soil and vermiculite. The plants were subjected to a photoperiod of 16 hours light (7:00 am to 11:00 pm) and 8 hours dark (11:00 pm to 7:00 am), with temperatures ranging between 22 and 24 °C. On the tenth day, one A. thaliana seedling was randomly selected and retained. Lines that failed to germinate were transplanted by seedling of a randomly selected replicate from the same genotype and treatment. For the control environment, we watered the plants from the\nbottom every four days and substituted water with half Hoagland solution every 16 days. For the jasmonic acid treatment, we sprayed the plants with 100 \\( \\mu \\)mol/L jasmonic acid solution (dissolved in 0.5% ethanol) every four days and sprayed 0.5% ethanol solution to plants in the JA control treatment. For the nutrient addition treatment, we watered plants with half Hoagland solution every four days and never gave Hoagland solution to plants in the nutrient depletion treatment. For the leaf removal treatment, we removed half of the total number of leaves 30 days after germination. For the drought treatment, plants were watered every eight days. We dissolved CaCl\\(_2\\) in water or half Hoagland solution to form 500 \\( \\mu \\)mol/L and 1500 \\( \\mu \\)mol/L CdCl\\(_2\\) solutions and watered the plants with these solutions in low- and high-cadmium treatments. For the low- and high-salinity treatments, we watered the plants with 50 mmol/L NaCl solutions. These treatments started 25 days after sowing and lasted for 32 days. Seeds for the next generation were collected 50-60 days after sowing. In the ancestral generation, 26 out of 1008 (2.58%) lines died before seed production, and their offspring generation was replaced with seeds of a randomly selected replicate from the same genotype and treatment.\n\nWe collected phenotypic data from the ancestral and offspring generations in Test I and Test II. Flowering time was checked daily and recorded as the days from sowing to the opening of the first flower. Fruit number was the number of siliques for a plant, used as a proxy for plant fitness. Rosette diameter was measured as the length of the most extended rosette cross centre. Plant height was the height of a plant when pulled straight. Aboveground biomass was the weight of the aboveground parts after drying in an oven at 80 \\( ^\\circ \\)C for 48 h.\n\n**Statistical analysis of phenotypic data**\n\nTo assess the effects of the environmental treatment and genotype on the ancestral generation, we applied a linear mixed-effect model to each phenotype (flowering time, plant height, aboveground biomass, rosette leaf diameter and fruit number). The model included genotype (G), environment (E), and their interaction (G \\( \\times \\) E) as fixed effects and the layer (A.Layer) and row (A.Row) as random effects, which was coded as \\( Y_{Anc} \\sim G + E + G:E + (1 \\mid A.\\text{Layer}) + (1 \\mid A.\\text{Row}) \\) (1). Note that the row number was unique\nand differed between layers.\n\nTo assess the effects of ancestral treatment and genotype on offspring generations, we applied a linear mixed-effect model to each phenotype measured in Tests I and II. The model included offspring layer (O. Layer), genotype (G), ancestral environment (A.E), and their interaction (G × A.E) as fixed effects and ancestor layer (A. Layer) and row (A. Row) as random effects and was coded as \\( Y_{\\text{Off}} \\sim O.\\text{Layer} + G + A.E + G:A.E + (1 | A.\\text{Layer}) + (1 | A.\\text{Row}) \\) (2). We also integrated all four offspring generations in a model. The model included offspring layer (O. Layer), genotype (G), ancestral environment (A.E), and offspring generation (F) and their two and three interactions as fixed effects and line (Line), ancestral layer (A.Layer) and row (A.Row) as random effects and was coded as \\( Y_{\\text{Off}} \\sim O.\\text{Layer} + G + A.E + F + G:A.E + G:F + A.E: F + G:A.E:F + (1 | \\text{Line}) + (1 | A.\\text{Layer}) + (1 | A.\\text{Row}) \\) (3). In Test I, generation was nested in the offspring layer, removing the effect of which also removed that of generation, and Model (3) ~.- F was applied to Test I. In addition, we applied a generalized linear mixed-effect model to the subsets of data, including only the offspring of the control environment. This model included the genotype (G) and offspring generation (F) and their interaction as fixed effects and was coded as \\( Y \\sim G + F + G:F+ (1 | A.\\text{Layer}) + (1 | A.\\text{Row}) \\) (4).\n\nThese models were formulated with function *lmer* in the R ver.3.6.2 package “lme4”\\( ^{33} \\). Statistics of fixed effects were estimated with the *Anova* function in the “car” package\\( ^{34} \\), and those of random effects were estimated with the *ranova* function in the “lmerTest” package\\( ^{35} \\). The effect sizes of ancestral responses to environmental treatments for different genotypes were extracted from model (1), and those of induced changes in offspring generations for different genotypes were extracted from model (2) with the *summary* function following Groot et al\\( ^{13} \\). For the JA treatment, the effect sizes were estimated by applying the models to a subset of data consisting of JA and JA control, and for other treatments, the effect sizes were estimated by applying the models to the respective treatment and the control. The significance of effect sizes was obtained with the *summary* function in the “lmerTest” package. According to these significances, we converted the effect sizes to qualitative occurrence data, where significant effect\nsizes were assigned a value of one, and nonsignificant effect sizes were assigned a value of zero.\n\nTo estimate the variance explained by different variables in mixed-effects models (1) and (2), we converted these models into full random effect models and applied the function VarCorr (package “lme4”) to the models. Model (1) was converted to \\( Y_{Anc} \\sim 1 + (1 | G) + (1 | E) + (1 | G \\times E) + (1 | A.Layer) + (1 | A.Row) \\), and Model (2) was converted to \\( Y_{Off} \\sim 1 + O.Layer + (1 | G) + (1 | A.E) + (1 | G \\times A.E) + (1 | A.Layer) + (1 | A.Row) \\). The estimated variance was visualized with the function geom_scatterpie in the R package “scatterpie” (available at https://github.com/GuangchuangYu/scatterpie).\n\nPredictability and reproducibility analysis\n\nTo estimate whether the genotype, treatment, generation, and phenotype significantly affected the occurrence of transgenerational effects, we applied generalized linear mixed-effect models to the qualitative occurrence data of Test I and Test II. The model included the genotype, treatment, generation and trait as fixed effects and an additional factor group as a random effect. As effect sizes of different traits were estimated from the same group of six replicate plants per genotype/treatment/generation, we defined the six replicates as one group, which was assigned a group ID. The model was formulated with function glmer in the R ver.3.6.2 package “lme4” and was coded as \\( Y \\sim G + A.E + F + Trait + (1 | group.id) \\) (5). Statistics of fixed effects were estimated with the Anova function in the “car” package. Furthermore, we used the glht function in the “multcomp” package\\(^{36}\\) to further investigate the differences in occurrence frequency among different ancestral treatments, generations, and phenotypes.\n\nTo explore which factors could predict the genotypic variation in the occurrence of transgenerational effects, we related the occurrence probability of genotypes to climates at the origin sites, the DNA methylation level, and the number of transposons in the genomes. We extracted climate data (Bio1-Bio19) from WorldClim (https://worldclim.org), including monthly climate data between 1901 and 2000. The data were extracted with the coordinates of genotypes from a 30-second spatial resolution (~1 km2) by the R package “raster” (Supplementary Table 1). The raw\nmethylation data of 14 genotypes were obtained from published sources37. Quality control was performed using Trimmomatic v0.3638 with the following parameters: ILLUMINA_CLIP: TruSeq3-PE.fa:2:30:10\" LEADING:20 TRAILING:20 SLIDINGWINDOW:4:20 MINLEN:50. We aligned the reads against the TAIR10 reference with bwa-meth39 with the default parameters. The aligned reads with mapping quality higher than 30 were obtained with SAMtools v 1.740 with the -q 30 option, and duplicates were marked and removed by Picard v2.18.10 (http://broadinstitute.github.io/picard) and SAMtools (-F 1024). The methylation level of each cytosine for different contexts (CG, CHG, and CHH) was extracted with MethylDackel (https://github.com/dpryan79/MethylDackel). We excluded cytosines with a read depth lower than 5, and the average methylation level per cytosine was estimated for each context (Supplementary Table 1). Furthermore, we extracted the number of transposable elements from published sources25. The original file contained copy number estimation based on read coverage for the 317 TE families analysed across 211 A. thaliana accessions. We summarized the total number of TEs according to superfamilies and then used log-transformed counts for further analysis. These data were available for seven genotypes, including Abd-0, Ang-0, Col-0, Dja-1, Sap-0, Tol-0, and Ws-2 (Supplementary Table 1). The transposon data of Col-0 were not included in the subsequent analysis because Col-0 is the reference genome and shows biased (much more detailed) annotation of transposons compared to other genotypes. We applied arcsine square root transformation to the occurrence frequency and log transformation to the number of transposons in different superfamilies, regressed the transformed occurrence frequency per genotype against the climate data, average methylation levels and transformed transposon number, and extracted the correlation coefficient and \\( P \\) value from the regression.\n\nTo investigate whether the effect size of environment-induced changes can be quantitatively predicted from the ancestor’s responses, we calculated the pairwise Pearson correlation coefficients between the ancestor’s responses and the effect sizes of different offspring generations. To assess the reproducibility of effect sizes between offspring generations and tests, we also computed pairwise Pearson correlation\ncoefficients between offspring generations for each test and between the tests. These correlation coefficients were estimated for subsets of data, including significant effects in either generation only or excluding these significant effects. In addition, for Test I, we used subsets of data, including the effect sizes of only one genotype or only one treatment, to calculate correlation coefficients between generations. Visualization was conducted using the ggplot function in the R package “ggplot2”.\n\nGenome-wide gene expression analyses\n\nTo assess patterns of gene expression changes caused by ancestral treatments, we collected fresh leaf samples from plants in Test II and conducted transcriptomic analysis. This analysis included four genotypes (Abd-0, Ang-0, Tol-0, TRE-1), four environments (the control, drought, low cadmium, and high cadmium), four generations (F1-F4), each with three replicates, and a total of 144 samples. These genotypes and environments were carefully selected to include genotypes and treatments representing a high/low occurrence probability of transgenerational effects. For instance, Abd-0 and TRE-1 represent genotypes sensitive to environmental induction, whereas Ang-0 and Tol-0 represent genotypes resistant to environmental induction. We sampled two to three rosette leaves per plant, immediately froze the samples in liquid nitrogen, and stored them at −80 °C before RNA extraction. We extracted total RNA with TRIzol reagent (Invitrogen)41. The samples of total RNA were subjected to quality assessment with an Agilent 2100 Bioanalyzer. The transcriptome sequencing library was prepared with the NEBNext® UltraTM RNA Library Prep Kit for Illumina® (NEB, USA). The library was sequenced with the Illumina NovaSeq platform to produce 150 bp paired-end reads. Quantity assessment, library preparation and sequencing were conducted by Novogene (Beijing, China). Sequencing yielded 19.5 to 29.4 million pairs of reads (average: 22.6) per sample (Supplementary Table 8).\n\nTo improve the quality of reads, we trimmed and filtered the reads with Trimmomatic v0.36 with the following parameters: “ILLUMINA_CLIP: TruSeq3-PE.fa:2:30:10” LEADING:20 TRAILING:20 SLIDINGWINDOW:4:20 MINLEN:50. Reads with improved quality were aligned to the TAIR10 reference genome using STAR v 2.7.942 with the default parameters and a TAIR10 gff-converted gtf-format file\n(parameter ‘-sjdbGTFfile’) (Supplementary Table 8). The conversion was conducted with gffread v.0.12.743. We extracted the gene expression matrix using featureCounts v1.22.2 44, with the ‘-p’ option to count the meta-features of genes using the TAIR10 gtf file. Genes were included in subsequent analysis if the sum CPM (counts per million) over all samples for the treatment and control per genotype was greater than one. The retained gene and the expression were subjected to cluster analysis of different samples with the plotPCA function in the DESeq2 v1.36.0 package45, and cluster analysis results were visualized using the R package “ggplot2”. We subjected the retained genes and their expression to differential expression analysis with the R package DESeq2 v1.36.0 (these genes were also used for random sampling, please see below). For each genotype, the difference in gene expression was estimated by comparing the expression of a particular gene between the ancestral treatment and the control. The expression matrix was normalized by function vst in package “DESeq2”. The difference in gene expression was estimated with function DESeq, and the differentially expressed genes (DEGs) were filtered by | log2FoldChange | >1.5 and adjusted \\( P < 0.05 \\). A gene was considered to be a heritable DEG if it was significantly differentially expressed for at least two generations. To explore the factors that explained the number of heritable DEGs, we regressed the log-transformed number per genotype and treatment against the arcsine-transformed occurrence frequency per genotype and treatment as well as the log-transformed number of transposons per genotype and extracted the correlation coefficient and \\( P \\) value from the regression.\n\nTo investigate the function of DEGs, we focused on genes that were differentially expressed in at least two offspring generations (heritable DEGs) and conducted KEGG and Gene Ontology (GO) enrichment analysis. The enrichment analysis was conducted with functions enrichKEGG and enrichGO in the “clusterProfiler v4.4.4” package46. Enrichment analysis was conducted separately for four genotypes and three environments, which resulted in 12 sets of enrichment results (Supplementary Table 9). For the KEGG results, we took the union of significantly enriched pathways of the 12 sets, clustered the pathways according to the maps (https://www.genome.jp/kegg/pathway.html) and visualized the results. For the GO\nresults, we removed duplicated terms for each set with function simplify in the package (Supplementary Tables 10). Then, we filtered out terms with less than five genes enriched and selected the top 15 terms with the smallest \\( P \\) values for each set, took their union, and visualized the results. KEGG and GO visualization was conducted with the R package “pheatmap v1.0.12” (https://github.com/raivokolde/pheatmap). To facilitate visualization, we characterized the terms into functions of response to stimulus, biosynthetic and metabolic processes, cellular process, signalling, biological regulation, rhythmic process, and developmental process. Then, we extracted the mapped heritable DEGs in pathways and terms and summarized their overlapping patterns between genotypes and environments.\n\nWe found 2669 heritable DEGs shared between genotypes or environments, which are considered genes sensitive to environmental induction. We hypothesized that their sensitivity was related to the enrichment of transposons in their regulatory and gene body regions. To test this hypothesis, we randomly sampled 2669 genes from the genes subjected to the differential expression analysis and estimated the sum of the number of transposons per superfamily overlapping the 2 kb upstream and gene body regions. Through random sampling 10000 times, we obtained the null distribution of transposon abundance upstream of genes for different superfamilies. Then, we compared the observed transposon abundance upstream of the 2669 heritable DEGs against this distribution. The \\( P \\) value was estimated as the proportion of randomly sampled values greater than the observed value, and significant \\( P \\) values indicate significant enrichment of transposons upstream of heritable DEGs compared with the null expectation. We adopted the transposon annotation of TAIR10 and performed the analysis using a customized script coded with R package “GenomicRanges” v.1.42.0\\(^{47}\\) (available at https://github.com/Xiaohe-Lin/Heritable_variation/). Notably, our study adopted Col-0 as the reference, and genotype-specific genome assembly is necessary for a comprehensive understanding of this nonrandom phenomenon.\n\nTo investigate whether the heritable phenotypic changes were caused by heritable gene expression changes, we focused on flowering time and identified 79 flowering time-related genes from the literature\\(^{14-16}\\) (Supplementary Table 11). We visualized the\nexpression patterns of a subset of genes that were DEGs for at least one generation using the R package “pheatmap”.\n\nData availability\n The phenotypic data of the ancestral generation, Test I and Test II are available on GitHub (https://github.com/Xiaohe-Lin/Heritable_variation). Raw RNA-seq data are available from the NCBI SRA database with accession ID PRJNA997595.\n\nCode availability\n Codes for data processing are available on GitHub (https://github.com/Xiaohe-Lin/Heritable_variation).\nReferences\n\n1 Hoffmann, A. A. & Sgrò, C. M. 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Y. clusterProfiler: an R package for comparing biological themes among gene clusters. Omics **16**, 284-287 (2012).\n\nLawrence, M. et al. Software for computing and annotating genomic ranges. PLoS Comput. Biol. **9**, e1003118 (2013).\nAcknowledgements: We thank Wenjing Hong, Gang Wang, and Rong Wang for their constructive suggestions. We thank Ming Zhou, Xianwen Ma, Jiayi Ding, and Xinwei Wang for their help in the growth room and Xiuxiu Wang and Haidong Qu for their technical assistance.\n\nAuthor contributions: Y-Y.Z., O.B. and V.L. conceived the idea of this project; Y-Y.Z. and JJ.Y. designed the experiments; Y-Y.Z. supervised and Q.Q.L. co-supervised the project; JJ.Y., Y.W., J. Y, and X. L carried out the experiments; JJ.Y., Y.W., and X. L analysed the data; X. L wrote the first draft of this manuscript, and all authors contributed to the revision of the manuscript.\n\nFunding: This study was supported by the National Natural Science Foundation of China (32371558, 32071485) and the Fundamental Research Funds for the Central Universities of China (20720210075).\n\nCompeting interests: The authors declare no competing interests.\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• supportingdata.xlsx\n• Extendeddatafigures.pdf"} {"paper_id": "prb7", "title": "Measurement of the 2S1/2,F=0 ↔ 2P1/2,F=1 transition in Muonium", "text": "Measurement of the 2S1/2,F=0 ↔ 2P1/2,F=1 transition in Muonium\n\nGianluca Janka\nETH Zurich https://orcid.org/0000-0002-9147-6885\n\nBen Ohayon\nETH Zurich\n\nIrene Cortinovis\nETH Zurich\n\nZak Burkley\nETH Zurich\n\nLucas de Sousa Borges\nETH Zurich\n\nEmilio Depero\nETH Zurich\n\nArtem Golovizin\nP.N. Lebedev Physical Institute https://orcid.org/0000-0002-2747-1297\n\nXiaojie Ni\nPaul Scherrer Institute\n\nZaher Salman\nPaul Scherrer Institute https://orcid.org/0000-0002-3431-8135\n\nAndreas Suter\nPaul Scherrer Institut https://orcid.org/0000-0002-9214-6474\n\nThomas Prokscha\nPaul Scherrer Institute https://orcid.org/0000-0002-7643-4695\n\nPaolo Crivelli (paolo.crivelli@cem.ch)\nInstitute for Particle Physics, ETH Zurich https://orcid.org/0000-0001-5430-9394\n\nArticle\n\nKeywords:\n\nPosted Date: June 22nd, 2022\n\nDOI: https://doi.org/10.21203/rs.3.rs-1718825/v1\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nAdditional Declarations: There is NO Competing Interest.\n\nVersion of Record: A version of this preprint was published at Nature Communications on November 25th, 2022. See the published version at https://doi.org/10.1038/s41467-022-34672-0.\nMeasurement of the \\(2S_{1/2}, F=0 \\rightarrow 2P_{1/2}, F=1\\) transition in Muonium\n\nG. Janka,\\textsuperscript{1} B. Ohayon,\\textsuperscript{1} I. Cortinovis,\\textsuperscript{1} Z. Burkley,\\textsuperscript{1} L. de Sousa Borges,\\textsuperscript{1} E. Depero,\\textsuperscript{1} A. Golovizin,\\textsuperscript{2} X. Ni,\\textsuperscript{3} Z. Salman,\\textsuperscript{3} A. Suter,\\textsuperscript{3} T. Prokscha,\\textsuperscript{3} and P. Crivelli\\textsuperscript{1,*}\n(Mu-MASS collaboration)\n\n\\textsuperscript{1}Institute for Particle Physics and Astrophysics, ETH Zürich, CH-8093 Zürich, Switzerland\n\\textsuperscript{2}P.N. Lebedev Physical Institute, 53 Leninsky prospect., Moscow 119991, Russia\n\\textsuperscript{3}Laboratory for Muon Spin Spectroscopy, Paul Scherrer Institute, CH-5232 Villigen PSI, Switzerland\n(Dated: June 2, 2022)\n\nMuons are puzzling physicists since their discovery when they were first thought to be the meson predicted by Yukawa to mediate the strong force. The recent results at Fermilab on the muon g-2 anomaly puts the muonic sector once more under the spotlight and calls for new measurements with this fascinating particle. Here we present the results of the first measurement of the \\(2S_{1/2}, F=0 \\rightarrow 2P_{1/2}, F=1\\) transition in Muonium, the hydrogen-like bound state of a positive muon and an electron. The measured value of 580.6(68) MHz is in agreement with the theoretical calculations. From this measurement a value of the Lamb shift of 1045.5(68) MHz is extracted, compatible with previous experiments. We also determine for the first time the \\(2S\\) hyperfine splitting in Muonium to be 559.6(72) MHz. The measured transition being isolated from the other hyperfine levels holds the promise to provide an improved determination of the Muonium Lamb shift at a level where bound state QED recoil corrections not accessible in hydrogen could be tested. Such a measurement will also be sensitive to new physics in the muonic sector, e.g. to new bosons which might provide an explanation of the g-2 muon anomaly or Lorentz and CPT violation. We also present the first observation of Muonium in the \\(n = 3\\) excited state opening up the possibility of new precise microwave measurements as realized in hydrogen.\n\nI. INTRODUCTION\n\nThe discovery of muons has an intriguing history. As in the case of the positron, they were first detected in cosmic radiation by Anderson and Neddermayer in 1936 [1]. Interestingly, the first hints of muons were actually already seen in 1933 by Kunze [2] in his Wilson chamber, but he was not confident enough about his results to claim the discovery of a new particle.\n\nThe muon was first thought to be the pion predicted by Yukawa (1935) [3], the heavy quantum (meson) responsible of mediating the nuclear (strong) force in analogy to the light quantum (photon) for the electromagnetic interaction. The pion based on the range of the nuclear force should have had a mass of 100 to 200 times the mass of the electron and should be both positively and negatively charged. The muon (207 times the electron mass) seemed to have just the expected value. However, in 1946 an experiment of Conversi et al. [4] showed that their interaction with nuclei was too weak to be attributed to pions. They observed that the negative mesotron would decay instead of being absorbed by carbon after having formed a pionic atom as predicted by Tomonaga-Araki [5]. This was the first indication of the formation of muonic atoms as it was realized a few years later. Moreover, the lifetime of the muon was of the order of \\(10^{-6}\\) s which is \\(10^{12}\\) times longer than expected by strong interaction processes. Finally in 1947, Powell et al. [6] detected the pion using photographic emulsions at high altitudes and verified that it decays into a muon and a neutral particle that was identified to be a neutrino. The possibility that this could be a photon was eliminated by the non-observation of pair production as expected in this case. This led Isidor Rabi to come up with his famous quote: “Who ordered that?”.\n\nThe fascinating history of the muon continues to this day. The recent results at Fermilab [7] confirming that the measured muon anomalous magnetic moment (g-2 muon) deviates from the standard model prediction by 4.2 standard deviations calls for further scrutiny. Muonium (M), the bound state of the positive muon (\\(\\mu^+\\)) and an electron is an ideal system to study the muon properties and hunt for possible new effects. Due to its lack of sub-structure it is free from finite size effects and is therefore an excellent candidate to probe bound-state QED [8] and search for new physics beyond the Standard Model [9–11].\n\nPrecise measurements of the ground-state hyperfine structure (HFS) [12] and the \\(1S - 2S\\) transition [13] in Muonium were performed, with improvements proposed by MuSEUM (HFS, [14]) and Mu-MASS (\\(1S - 2S\\), [15]) ongoing. All the measurements so far of the M Lamb shift (LS) are limited by statistics [16–18]. Only recently, the formation of an intense metastable M(2S) beam was demonstrated by the Mu-MASS collaboration at the low-energy muon beamline (LEM) at PSI [19], opening up the possibility for a new generation of precision measurements of the M LS.\n\nA first measurement at the LEM beamline resulted in a M LS value of 1047.2(25) MHz [20], representing an order of magnitude improvement upon the previous measurements. With the muCool beamline [21] and (if approved)\nthe high intensity muon beam (HiMB) upgrade at PSI [22], the \\( \\mu^+ \\) beam quality and flux will further improve, making it feasible to reach statistical uncertainties of the order of a few tens of kHz within a few days of beamtime. This would allow to probe QED corrections enhanced in the Muonium system such as the Barker-Glover effect (160\\(\\mathrm{kHz}\\)) or the nucleus self-energy (40\\(\\mathrm{kHz}\\)), which are still not in reach for hydrogen [23].\n\nThe prospect of not being limited by statistics calls for a systematically more robust method to extract the LS. Following the example of the most precise measurements of the hydrogen Lamb shift [24–26], extracting the LS from the isolated hyperfine transition \\(2S_{1/2}, F=0 \\rightarrow 2P_{1/2}, F=1\\) is preferred over the other two allowed transitions (see Fig. 1). Due to the reduced influence of other nearby transitions, the systematic uncertainties related to line-pulling would become negligible.\n\nWe report here the first measurement of the isolated hyperfine transition, from which we extract the M LS. Combining this result with our previous measurement [20], we determine the 2S hyperfine splitting in Muonium for the first time. Additionally, we present the first observation of Muonium in the \\(n = 3\\) excited state.\n\nII. EXPERIMENTAL METHOD\n\nThe LEM beamline at PSI provides low (1-30 keV) energy muons with a rate of up to 20 kHz using a solid neon moderator [27]. In our experiment, we set the energy of the \\( \\mu^+ \\) to 7.5 keV in order to maximize the number of M(2S) available for the measurement [19]. The beam transport is optimized with several lenses along the beamline, eventually focusing the muons onto a carbon foil at the entrance of the setup shown in Fig. 2.\n\nIn contrast to the LS measurements with protons, the flux of muons is around ten orders of magnitude smaller, which makes it essential to have an efficient background suppression without sacrificing efficiency. Therefore, the incoming muons are tagged on an event by event basis to be able to discriminate their times-of-flight (TOFs). When impinging onto the 10 nm thin carbon foil, a \\( \\mu^+ \\) releases secondary electrons. These electrons are detected by a microchannel plate (Tag MCP) to give the start signal of the TOF measurement. Upon leaving the foil, the tagged \\( \\mu^+ \\) has a probability of picking up an electron and form M, primarily in the ground state. From measurements with hydrogen [28, 29], 5% to 10% is expected to be formed in \\( n = 2 \\) and 2% in \\( n = 3 \\). This expectation was confirmed with a measurement of 11(4)% [19] for M in the metastable state. The M(2S) lifetime is limited by the decay time of the muon itself (\\( \\tau_{M(2S)} = 2.2 \\) \\(\\mu\\)s). M(3S) is unstable (\\( \\tau_{M(3S)} = 158 \\) ns) and will relax back to the ground state via the intermediate 2P state (\\( \\tau_{M(2P)} = 1.6 \\) ns).\n\nThe formed beam passes first through a transmission line (TL) which depopulates unwanted hyperfine states (HFS TL). As established by the most precise H LS measurements, this reduces the background and at the same time narrows and simplifies the overall line-shape to be fitted. By setting the HFS TL at a frequency of 1140 MHz and with an average power of roughly 29 W, according to our simulation, we depopulate the \\( F=1, m_F = \\pm 1 \\) states by 88% and the \\( F=1, m_F = 0 \\) state by 16%. The transition of interest \\( 2S_{1/2}, F=0 \\rightarrow 2P_{1/2}, F=1 \\) at 583 MHz remains almost unaffected, where its initial state \\( F=0, m_F = 0 \\) is only depopulated by 4%. With a second TL (Scanner TL) we scan the line-shape of this transition. Seven frequency points are measured in the range of 200 MHz to 800 MHz with an average power of 22.3 W. An additional data point is taken with the Scanner TL turned off. The output powers of both TLs are continuously monitored with power meters to ensure the stability of the measurement.\n\nDue to the short lifetime of the 2P states, the atoms excited by the microwave relax to the ground state before reaching the detection setup. The remaining excited states are quenched by applying an electrical field of the order of 250 V cm\\(^{-1}\\) between the two grids mounted in front of the coated Ly\\(\\alpha\\)-MCPs (see Fig.2) and relax back to the ground state with the emission of UV photons (2P Ly\\(\\alpha\\): 121.5 nm, 3P Ly\\(\\beta\\): 102.5 nm). These photons interact with the coating and release single electrons, which are in turn detected by the Ly\\(\\alpha\\)-MCPs. The beam then continues onto the Stop-MCP, giving the stop time for the TOF measurement. An event is recorded only if a coincidence signal between the Tag- and Stop-MCP is seen above threshold (double coincidence). The time window for a valid event is set to 10 \\(\\mu\\)s and multiple hits in the detectors are recorded. The signature for the detection of M 2S atoms is defined as the double coincidence and additionally the Ly\\(\\alpha\\)-MCP signal in the time region of interest (triple coincidence, see also Fig. 2).\n\nIn Fig. 3, the measured TOFs between Tag- and Stop-MCP (x-axis) are correlated with the TOFs between Tag- and Ly\\(\\alpha\\)-MCP (y-axis). The energy distribution of the M atoms after the carbon foil is well-known from previous measurements at the LEM beamline and reproduced by simulation [30]. The most-probable energy of the \\( \\mu^+ \\) after the foil is 5.7(2) keV. The expected TOF of an M atom from the Tag- to the Stop-MCP ranges from 90 ns to 135 ns, with a most-probable TOF of\n\n![The hyperfine transitions of the M 2S_{1/2} - 2P_{1/2} levels, including the 2S and 2P hyperfine splittings.](page_101_1342_1047_312.png)\n\nFIG. 1. The hyperfine transitions of the M 2S_{1/2} – 2P_{1/2} levels, including the 2S and 2P hyperfine splittings.\nFIG. 2. Schematic view of the experimental setup. The signal signature consists of a coincidence signal between Tag, Lyα and Stop-MCP. The coloured line-shapes above the TLs correspond to the observable transitions (1326 MHz (green), 1140 MHz (orange), 583 MHz (blue) and the combined \\(3S_{1/2} - 3P_{1/2}\\) (yellow) contribution). The time scale is given for the most-probable Muonium atom with an energy of 5.7 keV.\n\n117 ns. Applying this time cut, we extract the detected amount of M and \\( \\mu^+ \\), which serves as normalization factor \\( S_{Norm} = N_M + N_{\\mu^+} \\), accounting for variations in the beam intensity. The TOF between the tagging and the emission of a Lyα photon is calculated to be in the range of 30 ns to 75 ns. Applying both of these cuts, we identify our signal region, portrayed in Fig. 3. The amount of signal events are extracted for each frequency point (\\( S_{Lyα}(f) \\)). The normalized signals per frequency point are then calculated as \\( S(f) = S_{Lyα}(f)/S_{Norm} \\).\n\nIn region A of Fig. 3, events with longer TOFs than expected are summarized. Those events might be caused by either convoy electrons created at the foil [31] or by ionization products of a \\( \\mu^+ \\) interacting with the residual gas. The region A is leaking into the signal region, contributing to the measured background. The region B contains the events where the TOFs between the Lyα- and Stop-MCP are almost zero. These MCPs are close to each other, which leads to the risk of one detector picking up a noise signal when the other one is firing or vice versa. This noise signal can have a large amplitude with an intense after-ringing, which is mistaken as an additional signal that contributes to the events in region C.\n\nThe average power inside the TLs is frequency-dependent. To be able to fit a line-shape, all frequency points are corrected to the same “global” power of 22.5 W, obtaining the corrected signal \\( S_c \\). The applied correction is given by:\n\n\\[\nS_c(f) = (S(f) - S_{BKG}) \\cdot C(f) + S_{BKG},\n\\]\n\nwhere \\( S_{BKG} \\) is the background level. The correction factors \\( C(f) \\) are extracted by simulating the scaling ratio between the excitation probabilities at the effectively measured power and the global power for each frequency.\n\nFIG. 3. Correlation plot of the TOF between the Tag- and Stop-MCP and the TOF between the Tag- and Lyα-MCP. The signal region of Lyα events is circled. The regions labelled A,B,C are explained in the main text.\n\nBecause of the linear polarization of the field in the TLs, we can approximate our system to two levels and use the relevant optical Bloch equations [32] in the simulation. Single atom trajectories through both TLs reaching the Stop-MCP are simulated. While being in one of the TLs, the optical Bloch equations are numerically solved by an adaptive stepsize Runge-Kutta algorithm\n[33]. To reproduce the field inside the TLs, for each TL a field map is generated in SIMION, following the procedure of Lundeen and Pipkin [25]. The numbers of excited and ground state atoms detected in the Stop-MCP are counted and from that the average excitation probability calculated. As input parameter to the simulation we assign to each atom an initial state with its specific resonance frequency, and the power for both TLs operating at random phases of the fields. The momentum and initial position of the specific particle from the LEM is simulated with the musrSIM package [34] beforehand, from which the simulation randomly draws an atom.\n\nThe individual line-shape \\( P^{(i)} \\), where \\( i \\) stands for the assigned resonance frequency in MHz, is constructed by simulating the excitation probability for each initial state with large statistics over a frequency range between 200 MHz to 2000 MHz in steps of 1 MHz. Combining all relevant transitions, a global line-shape \\( P_n \\) for a \\( n \\) state is obtained:\n\n\\[\nP_{n=2} = 0.5 \\cdot P^{(1140)} + 0.25 \\cdot P^{(583)} + 0.25 \\cdot P^{(1326)}\n\\]\n\\[\nP_{n=3} = 0.5 \\cdot P^{(339)} + 0.25 \\cdot P^{(174)} + 0.25 \\cdot P^{(394)},\n\\]\n\nwhere the constant factors are coming from spin statistics.\n\nThe fitting function is constructed with the simulated line-shapes:\n\n\\[\nS_c = S_{BKG} + \\sum_n \\left[ B_n \\cdot P_n (f - f_{offset}) \\right],\n\\]\n\nwhere \\( B_n \\) is scaling the line-shape \\( P_n \\) for a specific \\( n \\) state and \\( f_{offset} \\) is introduced to allow for a global frequency offset compared to the theoretical resonance frequency used in the simulation.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
3SSBKGB2SB3Sfoffset\\( \\chi^2 \\)
x7.8(8)22.0(18)--24.8(74)6.7
✓3.4(11)25.0(19)5.0(9)2.3(68)2.0
\n\nFIG. 4. Muonium scan at 22.5 W in the range of 200 to 800 MHz. The fitted black line is with, the gray line without the 3S contribution. The colored areas represent the underlying contributions from \\( 2S-2P_{1/2} \\) transitions, namely 583 MHz (blue), 1140 MHz (orange), 1326 MHz (green), and the combined \\( 3S-3P_{1/2} \\) (yellow). The data point with TL OFF is not displayed in the figure, but is included in the fit; it lies at \\( 20.4(4) \\times 10^{-4} \\).\n\nshift is approximately halved and the one coming from the uncertainty in the MW field intensity is doubled.\n\nFrom this measurement we extract the \\( 2S_{1/2}, F=0 \\rightarrow 2P_{1/2}, F=1 \\) resonance frequency to be 580.6(68) MHz and determine the M LS to be 1045.5(68) MHz. Our result agrees well with the theoretical value and is limited by the statistical uncertainty. A summary of all available measured values of the M LS is shown in Fig. 5. Using our previous results of the \\( 2S_{1/2}, F=1 \\rightarrow 2P_{1/2}, F=1 \\) resonance frequency [20], we extract for the first time the 2S hyperfine splitting in Muonium to be 559.6(72) MHz.\n\nThe detected \\( B_{3S}/B_{2S} \\) ratio is 0.20(4). In the 60 ns from the foil to the entrance of the detection setup for an average M atom, 32% of the 3S states relax back to the ground state. Therefore, the effectively detected amount of 3S/2S created at the foil is 0.29(7). This agrees with the estimations done by C. Fry [36] of 0.36 and is slightly lower than the estimate of 0.44(4) from a combination of hydrogen population measurements [28, 29]. An additional uncertainty in the estimated 3S/2S ratio could arise from the assumption that the detection efficiency of Lyα and Lyβ is similar. In fact, the efficiency depends on a number of factors, which make an accurate determination of its wavelength-dependency challenging (see Ref. [37, 38]).\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Central ValueUncertainty
Fitting580.26.8
MW-Beam alignment< 0.16
MW field intensity< 0.07
M velocity distribution< 0.01
AC Stark \\(2P_{3/2}\\)+0.39< 0.02
2nd-order Doppler+0.03< 0.01
Earth’s Field< 0.05
Quantum Interference< 0.04
\\(2S, F=0-2P_{1/2}, F=1\\)580.66.8
Lamb Shift1045.56.8
Theoretical value LS [23]1047.4980.001
2S HFS559.67.2
Theoretical value HFS (*)557.9< 0.1
\n\n* The value was estimated by taking the most precise 1S HFS measurement in muonium [12] and dividing it by a factor of \\(2^3\\). The uncertainty was estimated by calculating the QED \\(D_{21}\\) difference [35].\n\nTABLE I. Central values and uncertainty contributions in MHz.\n\n![Summary of all measurements of the n = 2 Lamb shift in Muonium (black) [16–18, 20] and the latest theoretical value (orange) [23].](page_186_1012_627_377.png)\n\nFIG. 5. Summary of all measurements of the \\(n = 2\\) Lamb shift in Muonium (black) [16–18, 20] and the latest theoretical value (orange) [23].\n\nIV. CONCLUSIONS\n\nTo conclude, we measured for the first time the \\(2S_{1/2}, F=0 \\rightarrow 2P_{1/2}, F=1\\) transition in Muonium. This is the same hyperfine transition as the one used for the most precise determination of the hydrogen Lamb shift [26]. Since this transition is even more isolated from the other hyperfine transitions in Muonium compared to hydrogen, this is the best candidate for future precision M LS measurements. By combining the data set with the scan of the 1140 MHz resonance and leaving the 2S HFS splitting as a free parameter, we extract the 2S hyperfine splitting in Muonium also for the first time. Furthermore, we detected M(3S) for the first time. This observation opens up the possibility for new microwave spectroscopy experiments with M such as the \\(n = 3\\) LS or the two-photon transition \\(3S - 3D_{5/2}\\). Both these transitions were measured in H to a high precision [39, 40].\n\nIn our measurement, the comparably large population of 3S states distorts the line-shape and introduces line-pulling, which might seem to defeat the purpose of choosing the isolated \\(n = 2\\) transition. However, the \\(n = 3\\) population can be electrically quenched with a weak electrical field, leaving a large fraction of the \\(n = 2\\) population unharmed as shown by measurements from Bezginov et al. [41]. Extending the beamline to depopulate the 3S due to its lifetime is another option, but the strong beam straggling at the foil and resulting diffuse beam would reduce the 2S flux significantly. This problem could be overcome by exchanging the carbon foil with only a few layers of graphene (around 1 nm thickness) [42] or moving to a gaseous target. Additionally, with a new apparatus such as muCool to compress and cool the beam, or the HiMB project to increase the \\(\\mu^+\\) flux at PSI, the measurements would not be statistically limited anymore. 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Trattner, Optical Engineering 53, 1 (2014)."} {"paper_id": "prb70", "title": "Ontogeny shapes individual specialization", "text": "# Abstract\n\nIndividual dietary specialization, where individuals occupy a subset of a population’s wider dietary niche, is of key importance for species’ resilience against environmental change. However, the ontogeny of individual specialization, as well as associated underlying social learning, genetic, and environmental drivers remain poorly understood. Using a multigenerational dataset of female European brown bears (*Ursus arctos*) followed since birth, we discerned the relative contributions of social learning, genetic predisposition, environmental forcings, and maternal effects to individual dietary specialization. Individual specialization varied from omnivorous to carnivorous diets spanning half a trophic position. The main determinants of this dietary specialization were maternal learning during rearing (13%), environmental similarity (12%), maternal effects (11%), and permanent individual effects (8%), whereas the contribution of genetic heritability was negligible. Importantly, the offspring’s trophic position closely resembled the trophic position of their mothers during the first 3–4 years after separation from the mother, but this relationship ceased with increasing time since separation. Our study reveals that social learning and maternal effects are as important for individual dietary specialization as environmental forcings. We propose a tighter integration of social effects into future studies of range expansion and habitat selection under global change that, to date, are mostly explained by environmental drivers.\n\n**Biological sciences/Ecology/Behavioural ecology** \n**Biological sciences/Ecology/Stable isotope analysis** \n**Biological sciences/Developmental biology/Differentiation** \n**Earth and environmental sciences/Ecology/Evolutionary ecology** \n**Dietary specialization** \n**heritability** \n**maternal effects** \n**maternal learning** \n**trophic position** \n**trophic niche** \n**omnivore** \n**stable isotopes** \n**nitrogen-15** \n**Ursus arctos**\n\n# INTRODUCTION\n\nAmong individuals of the same species, niche variation is common and may occur when availability of food resources or habitat structure change across the species’ range. Ecological generalists, species with a wide niche, also seem to exhibit more individual specialization and are hence particularly well adapted to persist under shifts in resource availability or composition enabling them to occupy larger distributional ranges than ecological specialists. Individual variation is key for making species resilient towards changing resource availabilities in a rapidly changing world and may ultimately determine local persistence or extinction of species.\n\nInter- and intraspecific competition, predation and ecological opportunity, alter resource availability and have been identified as the main ecological drivers explaining variation in the degree of individual specialization among populations. Yet, how individual variation emerges and is maintained within populations has been rarely quantified in the wild. In principle, four potential sources of variation exist: social and individual learning, genetic inheritance, the environment, and maternal effects. Individual differences in resource preference or competence to secure a resource may therefore be determined during early ontogeny through social (e.g., maternal) learning via imitation leading to similarities between the offspring’s and their mother’s dietary phenotype. Effects of maternal learning can be lifelong or are subsequently modified through individual experiential learning. Resource preferences have also been suggested to be genetically determined through genes inherited from both mother and father, where closely related individuals have more similar diets than distantly related individuals. In addition, maternal effects account for lifelong similarities in dietary phenotype among offspring of the same mother. Such similarities can arise from social interactions, maternal genotype, or maternal environment. Statistically, maternal effects are quantified as the similarity of repeated samples from siblings of the same mother but not as the similarity of behavioral expression between mother and offspring (i.e., “maternal learning”). In range resident species, where individuals occupy a subset of a population’s range, the environment, in terms of habitat composition or availability of particular food resources, may differ among home ranges and lead to individual specialization. Accounting for the environmental heterogeneity when studying the drivers of individual specialization is therefore essential in range resident species.\n\nAttributing variation in diet to the individual level, to isolate its sources and to identify developmental drivers of diet preferences requires multigenerational datasets of repeated measures of the diet of individuals throughout their life. We used a 30-year longitudinal dataset of 72 female Scandinavian brown bears (*Ursus arctos*) of known mothers with repeated annual isotopic estimates of trophic position to assess whether individual dietary specialization occurs. Using information about their mother’s diet, a genetic pedigree, and individual movement data we then attributed individual variation in diet to its sources: maternal learning, genetic heritability, environment, and maternal effects.\n\nBrown bears are ecological generalists with a species range spanning the northern hemisphere from tundra to deserts, paralleled by extensive variation in diet: from populations tracking food resource pulses, such as spawning fish, scavenging on ungulate carcasses or preying on ungulates neonates, or feeding extensively on invertebrates, to populations using primarily fruiting plant based diets. Given this extreme dietary plasticity, it is not surprising that great dietary variation has been found within populations, however, the determinants and ontogeny of this variation at the individual level remain largely unknown. In ecology, differences in diet are often primarily attributed to differences in resource availability and abundance. Even within populations inhabiting a continuous biome, home range scale variation in habitat composition can lead to variation in resource availability. The most parsimonious source of variation in diet are, therefore, differences in the environment. Brown bears maintain non-territorial home ranges but live a solitary lifestyle except for the period of offspring rearing involving up to three years of maternal care, after which female offspring often settle close to their mother’s home range. In their first years of life, bear cubs accompany their mother and it is therefore reasonable to assume that brown bear offspring learn behaviors such as habitat, den site, or diet selection from their mothers and hence show similar behavior to them. If mothers differ in their dietary selection, these differences may hence be maintained in the population through learning by imitation of the mother (hereafter \"maternal learning”), even after offspring gain independence, however, such similarities may wane over time. On the other hand, genetic heritability or maternal effects can have lifelong effects on offspring phenotype. Body size has been shown to be genetically heritable in our study population suggesting greater similarity among closely related individuals also in other linked traits, such as trophic position. Alternatively, maternal effects (i.e., maternal genotype or maternal environment) alone can shape the phenotype of offspring. For example, milk quantity or quality can vary among females either due to genetic differences or differences in the environments, leading to greater similarity among all offspring from the same mother (e.g. being smaller or larger in body size), which in turn could cause similarities in trophic position among siblings. To assess individual specialization along a continuum from a more plant-based to a more meat- or insect-based diet, we analyzed annual trophic positions from stable- nitrogen isotopes (δ¹⁵N) in bear hair keratin. Stable isotopes reflect cumulative diet intake and are deposited into the hair during growth with, a delay of approximately one month (i.e. a growing hair in June reflects the diet intake in May). Bear hair is regularly renewed through molting in June, regrows over the summer and fall and stops growing during winter hibernation (Fig. 1A, ). Guard hair samples collected in spring and early summer (April - June) therefore reflect an individual’s diet during the previous active season prior to hibernation. Using repeated samples of known mother-daughter pairs, we fit a spatially explicit Bayesian hierarchical model (i.e. ´animal model´) to disentangle the relative contributions of maternal learning, genetic relatedness, the environment, and maternal effects as determinants of individual specialization. Specifically, the model accounted for genetic relatedness with a pedigree and for environmental similarity of bear home ranges with pairwise habitat similarity encompassing the proportion of mature habitat such as old and mid-successional forests, disturbed habitat such as clearcuts and regenerating young forest, and habitat diversity (measured as Simpson’s diversity index) in a bear’s home range. The model also accounted for maternal effects by incorporating the mother’s ID as a random effect (i.e. if daughters from the same mother behaved in a similar fashion throughout life), and for maternal learning as the fixed effect of a mother’s trophic positions on her daughter’s trophic position. To this end, we determined maternal trophic positions from a population-wide model accounting for sexual dimorphism, age, and individual consistency in diet (). Because bears may alter diet selection over time through individual learning, we allowed the effect of maternal learning to shift with time since the offspring gained independence. Last, we also accounted for permanent individual effects that could not be attributed to any of the aforementioned sources, by including a random effect for bear ID. We focused on the effect of maternal trophic position on female offspring trophic position, because male offspring were only monitored for a short period after family breakup. In the supplementary material we provide an additional analysis of the relationship between maternal and both female and male offspring trophic position in the first 4 years after family breakup and of the relationship between paternal trophic position and offspring trophic position. We also provide an alternative analysis accounting for spatial correlation via a spatial distance instead of a habitat similarity matrix, as well as a reduced model excluding the effect of environmental similarity to test whether spatial and genetic effects were confounded in philopatric female bears. Last, we validated our effect of maternal learning by refitting the model to a reduced dataset with observed maternal trophic positions during rearing, instead of modeled-averaged maternal trophic positions.\n\n# RESULTS\n\nWe analyzed annual trophic positions in 213 hair samples collected from 71 female brown bears born to 33 unique mothers (1–7 daughters per mother; median 2 daughters). Repeated sampling (median 3 years; range 1–11 years) revealed that female trophic position was unaffected by age (explained variance = 1% [0–4%]) and that individuals showed long-term individual specialization, accounting for 48% [31–61%] (median [89% equal tails credible interval]) of the total variance in trophic position (Fig. 2, Basic model). Individual specialization spanned half a trophic position ranging from 2.7 to 3.1 for individual females (Fig. 1B), which is equivalent to the difference between an omnivore feeding on a mix of plants and animal prey and a carnivore feeding predominantly on animal prey.\n\nIndividual specialization was primarily driven by initial maternal learning, the environment, and maternal effects. Maternal trophic position dynamic over the time since separation accounted for 13% [5% − 23%] of variation in trophic position, while environmental similarity accounted for 9% [0.1–5%] of the total phenotypic variation in trophic position. Additionally, maternal effects accounted for 11% [0.5% − 30%] of variation in trophic position, indicating that siblings (full and half) of the same mother were more similar in trophic position throughout life as compared to non-siblings. A remaining 8% [0.3–26%] of variance in trophic position was attributed to permanent individual effects (Fig. 2). Genetically more closely related individuals did not share a more similar trophic position (3% [< 0.1% – 17%] of variance explained) providing no evidence that dietary specialization could be heritable in this population (Fig. 2).\n\nAfter separating from their mother, female offspring initially maintained a similar trophic position as their mother (Pearson’s r = 0.66 in the first two years after separation), which gradually became more dissimilar over time (Pearson’s r = 0.31 in year 3–4 after separation, Fig. 3). In the first years, offspring of more carnivorous mothers also had a high trophic position while offspring of less carnivorous mothers had a lower trophic position. About five years after the separation of the mother, this correlation ceased to exist. Bears inhabiting home ranges with a similar composition of mature and disturbed forest, as well as a similar habitat diversity in the home range, also had more similar trophic positions. The distance between pairwise home range centroids ranged from 0.7 to 172 km with a median pairwise distance of 48 km and individuals living in closer proximity had a more similar trophic position than individuals living farther apart (Supplementary material S6). Spatial distance and maternal effects seemed to be confounded in this female philopatric species: After excluding spatial distance, maternal learning and maternal effects but not heritability explained more variance in trophic position, corroborating that spatial proximity is confounded with philopatric females forming clusters of mothers and daughter in space, so called matrilines (Supplementary material S7). In a separate analysis (Supplementary material S8) we could also show that the relationship between maternal and offspring trophic position in the first years after family breakup was not sex-specific. Both male (n = 31, Pearson correlation coefficient = 0.4) and female (n = 69, Pearson correlation coefficient = 0.45) offspring’s trophic positions resembled their mother’s trophic position in the first 4 years of independence, corroborating our findings that initial maternal learning determines foraging behavior in the early years after family breakup. Conversely, paternal trophic position had no effect on offspring trophic position in the first 4 years of independence (Pearson correlation coefficient = 0.13, Supplementary material S9). While the modelled maternal trophic position correlated strongly with the observed trophic position in any given year (Supplementary material S3), maternal learning explained even more of the phenotypic variance in daughter trophic position (22% [8% − 27%] instead of 13%, Supplementary material S10) when fitting the observed maternal trophic position during rearing, instead of the modelled posterior average maternal trophic position to a reduced dataset (62 hair samples collected from 38 daughters). Our estimates of maternal learning are therefore likely conservative and may underestimate the true effect of maternal learning on dietary specialization.\n\n# DISCUSSION\n\nOur multigenerational dataset reveals unique insights into the ontogeny of individual dietary specialization along a continuum from a more herbivorous to a more carnivorous diet in a long-lived omnivore. Specifically, the foraging strategy of sons and daughters was intimately tied to the foraging strategy of their mother, a relationship that lasted up to four years after independence. We interpret this relationship as evidence that maternal learning plays an important role in shaping an individual’s dietary specialization. Five years into independence, the similarity between the mothers’ and their daughters’ trophic position slowly faded, likely due to individual learning and experience. In addition, siblings of the same mother also shared lifelong similarities in their trophic position, potentially mediated through maternal genetic or environmental effects on body size25. In general, previous ecological studies have mainly concentrated on resource availability as the main driver of resource selection34 and individual specialization4, however our results show that, within populations, the environment is only one of several components shaping individual dietary variation. We conclude that early-life imitation of maternal dietary preferences and maternal effects (i.e., maternal genotype and environment), which together explained about 24% of the variation in trophic position, play a pivotal role in spreading and maintaining feeding strategies within populations, even in species with otherwise solitary lifestyles. In addition, variation solely linked to individual variation (in our study 8 %) demonstrates potential for behavioral innovation and the potential to adapt to changing conditions.\n\nOur findings are particularly relevant for species in which dietary specialization impacts individual fitness7, 35, 36. For example, protein-rich diets may promote greater offspring survival or mass gain37. Maternal and social learning in general therefore present an important, yet understudied pathway by which alternative behavioral strategies can establish and spread more rapidly within populations than by genetic evolution alone38. Species more adept in social learning of dietary strategies may therefore show greater behavioral variability at the population level, which could give them an advantage when adapting to changing environments due to landscape modification or urbanization, climatic variations or global change in general. Moreover, there is evidence that the strength of social learning in shaping individual phenotypes is not only species-specific, but can also vary among populations or individuals of the same species39.\n\nOur research also points to several aspects of maternal learning that warrant future research. First, there is little information on whether maternal care and maternal learning tend to be more prevalent in species or populations with greater dietary specialization. There is some evidence that within populations, dietary generalists (i.e. those with a wider dietary niche) seem to provide more intense parental care40, than their conspecific dietary specialists (i.e. ones with a narrower dietary niche), but the links to parental learning of foraging preferences remains unclear. Second, while generalist species with a wide ecological niche have been frequently shown to be more successful under changing environmental conditions, such as urban environments or fragmented landscapes, than specialist species41, 42, 43, it is currently unknown whether this success could be partially mediated by social or maternal learning. Last, social learning could alternatively limit behavioral innovation and adaptation due to adherence to social traditions44. We therefore suggest that alternative hypotheses should be evaluated that consider how social learning impacts individual specialization and in turn the adaptability of species under global change.\n\nOur findings that dietary specialization can be socially learned and transmitted are particularly relevant for species where specialization is related to human-wildlife conflict45. For example, the removal of single individuals which are known to cause conflict is an effective strategy to halt the spread of problematic behavior, increase societal acceptance by effectively mitigating the conflict, while minimizing the impact for species conservation goals45. Foraging behavior that causes conflict has also been shown to change in ursids across life time, remarking the crucial role of individuality and plasticity in behavior46. Maternal learning of behavior47, including dietary specialization and foraging on anthropogenic food resources is commonly observed in ursids48, 49, 50, 51. However, none of these studies tracked offspring diet over their lifetimes or were able to simultaneously account for the mother’s diet, genetics, the environment, and other maternal effects, that could explain similar patterns of dietary specialization. While some of the aforementioned studies suggest either the environment or maternal learning as primary drivers of individual specialization, we suggest using caution in assigning causality in dietary specialization, when potentially confounding alternative sources cannot be accounted for. Specifically, in female-biased philopatric species, spatial proximity does not only encode for spatial variation in resource abundance but is also conflated with relatedness and, in particular, with maternal effects. In brown bears, some daughters settle close to their mother’s home range23 creating spatial clusters of closely related females, so called matrilinear assemblages52. Due to spatial dependence of these assemblages, it can therefore be difficult to disentangle maternal learning from other maternal effects (i.e., maternal genotype or maternal environment) or the ambient environment. Our study population spanned over 170 km with spatial proximity explaining 59% of the total phenotypic variation in trophic position of female bears: individuals further apart tended to have more different diets. However, when replacing spatial proximity with environmental similarity among home ranges, the explanatory power was attributed to maternal learning and maternal effects along with the environment. Our results therefore demonstrate that individual dietary specialization is not caused by a single driver in isolation but the product of many factors, namely maternal learning, maternal effects, and the environment.\n\nOur finding that maternal learning has a similar impact on resource selection as the environment provides important insights for a range of studies on habitat selection, dispersal, and range expansion. For example, a popular theory known as “natal habitat preference induction” suggests that dispersing animals select areas for settlement that resemble their natal habitat, even at fine habitat scales21. Our results challenge the notion that habitat similarity alone drives natal settlement strategies and rather suggest that maternally induced diet preferences, and hence the selection for food resources themselves, could play an important role in producing similar patterns of settlement selection like induced natal habitat preferences. Recent studies of migration and short stopover behavior in whooping cranes (Grus americana) have also observed that social learning rather than environmental conditions53 or genetic inheritance54 led to the emergence and establishment of alternative migratory behavior. Similar to what our study shows with respect to dietary specialization, social learning of migration strategies primarily determined behavior in early life whereas individual-experiential learning shaped behavior later in life55.\n\n# Conclusion\n\nDrivers of dietary specialization are well documented among populations of the same species, however, systematic studies delineating the sources of individual specialization within populations are lacking, likely because suitable datasets including multigenerational, genetic, environmental, and life-history information are rare. We show here that in addition to the environment, maternal learning and (other) maternal effects can be important sources of dietary specialization.\n\n# METHODS\n\n**Bear sample collection** \nWe collected brown bear hair samples in south-central Sweden (~ N61°, E15°) as part of a long-term, individual-based monitoring project (Scandinavian Brown Bear Research Project; www.bearproject.info). Hair samples were collected from known individuals and their offspring during bear captures in spring (April - June) 1993–2016 after bears emerged from hibernation. Bears were immobilized from a helicopter (Arnemo & Fahlman, 2011). A vestigial premolar tooth was collected from all bears not captured as a yearling to estimate age based on the cementum annuli in the root56. Bears were weighed in a stretcher suspended beneath a spring scale. Tissue samples (stored in 95% alcohol) were taken for DNA extraction to assign parentage and construct a genetic pedigree52. Guard hairs and follicles were plucked with pliers from a standardized spot between the shoulder blades and archived at the Swedish National Veterinary Institute. All animal captures and handling were performed in accordance with relevant guidelines and regulations and were approved by the Swedish authorities and ethical committee (Uppsala Djurförsöksetiska Nämnd: C40/3, C212/9, C47/9, C210/10, C7/12, C268/12, C18/ 15. Statens Veterinärmediciniska Anstalt, Jordbruksverket, Naturvårdsverket: Dnr 35–846/03, Dnr 412-7093-08 NV, Dnr 412-7327-09 Nv, Dnr 31-11102/12, NV-01758-14). We used data of adult bears (solitary or with offspring) and of offspring after separation from their mother. Bear cubs are born in January or February during winter hibernation and are typically first captured together with their mother as yearlings at the age of ~ 15 months. Cubs in this population separate from their mother during the mating season in May or June after 1.5 or 2.5 years57. Only hair samples of solitary, independent offspring taken in spring and early summer at least 10 months after separation from the mother were included in this study. A hair sample taken in spring reflects the summer-fall diet of the bear in the previous active season (Fig. 1 A).\n\n**Food sample collection** \nWe collected samples of the natural foods most important for brown bear in the study area, including 21 samples of moose hair (Alces alces), the most common meat source in the brown bears’ diet in our study area58, in the spring-autumn field season of 2014 (Fig S1). Samples were placed in a paper envelope and dried at ambient temperature.\n\n**Stable isotope analyses** \nHair samples were rinsed with a 2:1 mixture of chloroform:methanol or washed with pure methanol to remove surface oils59. Dried samples were ground with a ball grinder (Retsch model MM-301, Haan, Germany). We weighed 1 mg of ground hair into pre-combusted tin capsules and combusted at 1030°C in a Carlo Erba NA1500 elemental analyser. N2 and CO2 were separated chromatographically and introduced to an Elementar Isoprime isotope ratio mass spectrometer (Langenselbold, Germany). Two reference materials were used to normalize the results to VPDB and AIR: BWB III keratin (δ13C =- 20.18‰, δ15N = 14.31‰, respectively) and PRC gel (δ13C =-13.64‰, δ15N = 5.07‰, respectively). Measurement precisions as determined from both reference and sample duplicate analyses were ± 0.1‰ for both δ13C and δ15N.\n\n**Bear trophic position** \nWe calculated the trophic position of each bear hair sample relative to the average δ15N value of moose (mean ± sd = 1.8 ± 1.26‰, n = 21, Fig S1). Trophic position is calculated as the discrepancy of δ15N in a secondary consumer and its food source divided by the enrichment of δ15N per trophic level, plus lambda, the trophic position of the food source (e.g. 1 for primary producers, 2 for primary consumers, 3 for secondary consumer, 4 for tertiary consumers)60. We used an average trophic enrichment factor of 3.4‰60 and added a lambda of 2 given that the moose baseline trophic position as a strict herbivore. \nBear trophic position = (δ15NUrsus arctos – average(δ15NAlces alces)) / 3.4 + 2 \nUnder an omnivorous diet including the consumption of herbivores (in particular moose but also ants such as Formica spp., Camponotus herculeanus with average δ15N indistinguishable from moose), bear trophic position values were expected to fall between 2 and 3. Values approaching 4 indicate a trophic enrichment through consumption of other omnivorous or carnivorous animals.\n\n**Genetic pedigree and parentage assignment** \nA genetic pedigree based on 16 microsatellite loci was available for the population including 1614 individual genotypes61. Genotyping followed the protocols of Waits, Taberlet62, Taberlet, Camarra63, and Andreassen, Schregel64. All female offspring in this study were genotyped and included in the population’s genetic pedigree. All females included in this study had a known mother that was also captured and followed. We used Cervus 3.065 for assignment of fathers and COLONY66 for creating putative unknown mother or father genotypes and sibship reconstruction (see61 for details).\n\n**Maternal trophic position** \nBased on repeated hair samples of 115 female (nfemale = 335) and 98 male (nmale = 219) bears, we fitted a basic linear mixed effects model for female and male bears respectively, to estimate sex-specific among individual variation in trophic position (Supplementary analysis 3). We modelled trophic position as a function of a quadratic relationship with age and we controlled for individual random intercepts. Female trophic position did not vary with age but was highly repeatable over multiple years. For all daughters, we extracted their mother’s (and father’s) trophic position as the median of the posterior distribution of their respective random intercept. The modelled posterior trophic position and the observed trophic position in a given sampling year were highly positively correlated (Pearson correlation coefficient r = 0.78, t = 22.63, df = 336, p < 0.001).\n\n**Environmental similarity** \nResources may not be distributed evenly in space. For moose, population density and hunting quotas (which determine availability of slaughter remains) vary across the study area. For ants, the availability of old forests and clearcuts determine their abundance67. Further, brown bear daughters are often philopatric with limited dispersal and settle close to their mother’s home range23. Genetic, spatial, and maternal learning effects may therefore be confounded with related bears occupying adjacent ranges with similar environments and resource availability. Elsewhere, accounting for environmental similarity through spatial autocorrelation in animal models has revealed that a major portion of variance may be attributed to environmental similarity rather than genetic heritability31, 32, 68, but see also69. Here, we accounted for environmental similarity by extracting habitat composition in each bear’s lifetime home range. For individuals with sufficient locations (> 1000 GPS locations or VHF locations on at least 25 days) we constructed home ranges using a 95% kernel density estimator. We used a Corine landcover map (25 m resolution) which we updated annually with polygons of newly emerged clearcuts (data obtained from the Swedish Forest Agency). We extracted home range composition in the year when diet was assessed. When individuals were monitored for multiple years, we extracted the home range composition for the median year. We calculated the proportion of mid-aged and old forest and proportion of disturbed forest (clearcuts and regenerating young forest) within the 95% utilization distribution. Additionally, we calculated habitat diversity using the Simpson diversity index from the R package landscapemetrics70. Following Thomson et al.31 we calculated the Euclidean distance between scaled and centered habitat composition and habitat diversity in multivariate space, assuming equal importance of each component. Pairwise distances were scaled between 0 and 1, where increasing values indicated more similar habitat composition. In the supplementary material we provide an alternative analysis accounting for spatial autocorrelation in dietary specialization with a pairwise spatial distance matrix (S matrix; Supplementary analysis 5, Fig S5).\n\n**Statistical analysis** \nWe applied a two-step modelling approach. First, we fitted a basic linear mixed effects model to estimate individual specialization as among individual variation in annual trophic position. We accounted for a nonlinear effect of age (second order polynomial) and for repeated measures of the same individual with individual random intercepts. We extracted the variance in fitted values (variance explained by fixed effects), among-individual, and residual variance and estimated the proportional contribution of fixed and random effects on the total phenotypic variance through variance standardization (i.e. repeatability71, marginal and conditional R2-values72). Second, we used a spatially explicit Bayesian hierarchical model (i.e. ‘animal model’)31, 33 to partition among-individual variance in trophic position into environmental similarity (σ2env), additive genetic (σ2a), permanent among-individual (σ2ind), maternal (σ2mat), and residual within-individual effects (σ2r). Similar to the basic model, we accounted for a nonlinear effect of age on trophic position (fitted as time since separation of mother and daughter scaled by the standard deviation, true age and time since separation were perfectly correlated: Pearson correlation coefficient > 0.99). We tested for maternal effects on offspring trophic position by incorporating the mother’s trophic position as a covariate into the model. To account for a potential decrease of the maternal effect over time, we let maternal trophic position interact with the time since separation of mother and daughter (both scaled by their standard deviation and centered). We partitioned the variance explained by the two components of the fixed effect, the effect of maternal learning over time (i.e. maternal trophic position and the interaction between maternal trophic position and time since separation) and age (i.e. the main effect of time since separation), respectively, by calculating the independent contribution of each component to the total variance explained by the fixed effects, following the approach by Stoffel, Nakagawa73 adapted to a Bayesian framework (see code under74). \nAll models were fit using the R package “brms”75 based on the Bayesian software Stan76, 77. We ran four chains to evaluate convergence which were run for 6,000 iterations, with a warmup of 3,000 iterations and a thinning interval of 10. All estimated model coefficients and credible intervals were therefore based on 1200 posterior samples and had satisfactory convergence diagnostics with \\\\(\\widehat{R}\\\\) < 1.01, and effective sample sizes > 40078. 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(2020).\n\n# Supplementary Files\n\n- [2023AGHMaternalLearningSupplement.docx](https://assets-eu.researchsquare.com/files/rs-2926801/v1/ea661eec5e586625a8f9ce96.docx)\n\n- [rs.pdf](https://assets-eu.researchsquare.com/files/rs-2926801/v1/d2aaf65e5476b984811c53c8.pdf) \n Reporting Summary"} {"paper_id": "prb71", "title": "Robotized indoor phenotyping allows genomic prediction of adaptive traits in the field", "text": "Robotized indoor phenotyping allows genomic prediction of adaptive traits in the field\n\nFrancois Tardieu (francois.tardieu@inrae.fr)\nFrench National Institute for Agricultural Research https://orcid.org/0000-0002-7287-0094\nJugurta Bouidghaghen\nFrench National Institute for Agricultural Research\nLaurence Moreau\nINRAE\nKatia Beauchene\nArvalis\nRomain Chapuis\nINRAE - National Research Institute for Agriculture, Food and Environment\nNathalie Mangel\nArvalis\nLLorenç Cabrera Bosquet\nINRAE\nClaude Welcker\nFrench National Institute for Agricultural Research https://orcid.org/0000-0002-8275-1259\nMatthieu Bogard\nArvalis Institut du Végétal https://orcid.org/0000-0003-1349-8330\n\nArticle\n\nKeywords:\n\nPosted Date: May 8th, 2023\n\nDOI: https://doi.org/10.21203/rs.3.rs-2879665/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nAdditional Declarations: There is NO Competing Interest.\nVersion of Record: A version of this preprint was published at Nature Communications on October 19th, 2023. See the published version at https://doi.org/10.1038/s41467-023-42298-z.\nRobotized indoor phenotyping allows genomic prediction of adaptive traits in the field\n\nJugurta Bouidghaghen1,2, Laurence Moreau3, Katia Beauchêne2, Romain Chapuis4, Nathalie Mangel2, Llorenç Cabrera-Bosquet1, Claude Welcker1, Matthieu Bogard2, François Tardieu1*\n\n1 LEPSE, Univ Montpellier, INRAE, Montpellier, France\n2 ARVALIS, Chemin de la côte vieille, Baziège, France\n3 GQE-Le Moulon, INRAE, Université Paris-Sud, CNRS, AgroParisTech, Université Paris-Saclay, Gif-sur-Yvette, France\n4 DIASCOPE, Université de Montpellier, INRAE, Montpellier, France\n\n* Corresponding author, email: francois.tardieu@inrae.fr\nAbstract\n\nBreeding for resilience to climate change requires considering adaptive traits such as plant architecture, stomatal conductance and growth, beyond the current selection for yield. Robotized indoor phenotyping allows measuring such traits at high throughput for speed breeding, but is often considered as non-relevant for field conditions. We show that maize adaptive traits can be inferred in different fields, based on genotypic values obtained indoor and on environmental conditions in each considered field. The modelling of environmental effects allowed translation from indoor to fields, but also from one field to another field. Furthermore, genotypic values of considered traits matched between indoor and field conditions. Genomic prediction resulted in adequate ranking of genotypes for the tested traits, although with lesser precision for elite varieties presenting reduced phenotypic variability. Hence, it distinguished genotypes with high or low values for adaptive traits, conferring either spender or conservative strategies for the diversity of future climates.\nIntroduction\n\nBreeding for the improvement of crop resilience is increasingly necessary for the sustainability of cropping systems and for food security in the context of climate change and growing population\\(^{1,2}\\). Most current breeding schemes are based on yield measurement of thousands of genotypes grown under diverse environmental scenarios, assisted by genomic selection that allows yield prediction for many thousands of untested genotypes based on their genomic information\\(^{3,4}\\). In this approach, the measurement of other traits is most often limited to crop cycle duration, which defines the growing areas in which resulting genotypes can be grown, and to traits that may jeopardize the commercialization of selected candidates, such as resistance to diseases or quality performance (e.g. oil content or protein content in rape seed and wheat, respectively)\\(^{5}\\). However, in the context of climate change, other traits that affect light interception, plant development, transpiration and growth are important for predicting, via statistical or crop models, the suitability of tested genotypes to future environmental conditions\\(^{6-8}\\). Furthermore, a recent analysis of maize genetic progress suggests that physiological traits involved in plant response to heat and drought, such as leaf growth rate or stomatal conductance, have not been improved over the last 60 years of maize selection\\(^{9}\\). Yield was improved via other traits such as the fine-tuning of phenology and the constitutive increase of grain number, but physiological adaptive traits are still a potential reservoir of interesting alleles for climate change\\(^{9}\\).\n\nThe progress of high-throughput phenotyping now allows one to measure physiological traits for hundreds of genotypes. Robotized indoor phenotyping platforms allow estimation, with typical time definitions of some minutes to one day, of traits that underlie the genetic variability of leaf area and their responses to environmental conditions, e.g. leaf expansion rate, leaf width, phyllochron and leaf number\\(^{10-13}\\). They also allow estimation of traits controlling transpiration, e.g. stomatal conductance\\(^{14}\\) and those controlling plant architecture, e.g. the vertical distribution of leaf area and the azimuthal distribution of leaves along the stem, with good heritability\\(^{15}\\). Then, light interception, transpiration and radiation use efficiency can be simulated in virtual field canopies, which reproduce 3D plants characterized in the indoor platform\\(^{15-17}\\). Field phenotyping also allows measuring leaf area at several dates, for hundreds of genotypes in different fields characterized by measured\nenvironmental conditions\\(^{18-20}\\). It also enables estimation of intercepted light in the same fields and, via model inversion, of leaf area and plant architecture\\(^{21-23}\\).\n\nHowever, the use in breeding of these physiological and growth-related traits faces the difficulty of their high sensitivity to environmental conditions, resulting in large genotype x environment interactions\\(^{24-27}\\). This difficulty is not limited to the extrapolation of trait values from indoor to field conditions: most of these traits also largely vary between fields depending on environmental conditions, making difficult the prediction of traits in one field from those measured in another field\\(^{24,28,29}\\). The relationship between these traits and yield is also highly depending on environmental scenarios\\(^{30,31}\\). These difficulties caused a lack of adoption of physiological adaptive traits in breeding programs\\(^{9,32}\\).\n\nThe recent development of speed breeding in controlled conditions may offer new opportunities for selection strategies involving plant traits. Speed breeding reduces the duration of each generation, thereby allowing up to eight generations of selection per year\\(^{33,34}\\). Yield and agronomic traits like disease resistance are predicted based on genomic information at each generation, while a full phenotyping of the most promising genotypes is carried out in the field after some generations\\(^{35}\\). However, this approach also potentially includes, in the breeding decisions, other traits measured indoor. For instance, in wheat, Watson *et al.* (2019)\\(^{36}\\) performed speed breeding involving the length of flag leaves and ear length, in addition to yield.\n\nWe evaluate here the extent to which physiological adaptive traits translate from indoor conditions to the field, and can be estimated *via* genomic prediction models. Three panels of maize hybrids were used: a ‘diversity panel’ with 246 hybrids\\(^{31}\\), a ‘genetic progress panel’ with a historical series of 56 commercial hybrids\\(^{9}\\) and a ‘recent hybrids panel’ with 86 commercial hybrids marketed from 2008 to 2020 (most measurements on 20 contrasting hybrids, Supplementary Tables 2, 3). We first show that genotypic values of traits measured indoor closely correlate with those in the field, either directly or via modelling (Table 1). We then show that, although absolute trait values differ if measured indoor or in the field, they still follow common trends in response to environmental conditions, and can be inferred by using an ecophysiological model. Finally, we examine to what extent measurements in indoor platforms can serve to train statistical prediction models that calculate genotypic values of traits based on genomic information only (Table 1).\nResults\n\nTraits measured indoor had genotypic values that correlated with those in the field, but to different extents depending on categories of traits\n\nA genetic approach based on indoor trait measurements requires that the latter are genetically correlated to measurements of the same traits in the field. However, such comparison is not always possible, because robotized indoor phenotyping can measure traits that would be impossible, or very tedious, to measure in the field, such as stomatal conductance or the 3D leaf distribution on the plant stem. Conversely, some traits measured indoor are largely irrelevant to the field, in particular those performed on whole canopies. Hence, comparisons of the genetic variability of trait values obtained indoor and in the field face different levels of difficulty depending on traits. We focused our study on traits that are heritable and have a direct impact on biomass accumulation (Table 1). They present contrasting ‘phenotypic distances’\\(^{37}\\) between indoor and field measurements, thereby causing different degrees of difficulty for comparisons of indoor vs field values.\n\nTable 1. Summary of the results for each studied trait\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Method indooraMethod fieldbCorrelation indoor vs fieldcCorrelation field vs fielddGenomic prediction cross-validationeGenomic prediction externalf
Leaf appearancee rate (LAR)Time courseTime course0.570.490.570.53
Architecture (rhPAD / ALA)3D imagingUAV imaging0.78 / 0.58 / 0.600.50.650.39
Vegetative phase durationNot relevantRecorded-0.69 / 0.470.840.71
Stomatal conductanceModel inversionNot measurable at HTP--0.55-
Leaf Expansion Rate (LER)Time courseNot measurable at HTP--0.770.33
Leaf area index (LAI)ModellingUAV imaging0.63---
\n\na,b Method for trait measurement indoor and field, respectively. HTP, high-throughput phenotyping. c Correlation between genotypic values indoor and in the field, several figures are stated for different fields when relevant. d Correlation between genotypic values from one field to another field. e Correlation between G-BLUP predicted values and measured values in a cross-validation scheme including diversity and genetic progress panels. f External validation: Correlation between G-BLUP predicted values (with training on diversity and genetic progress panels) and measured values in recent hybrids panel. The duration of the vegetative phase, a trait commonly measured in breeding schemes, is shown for comparison with other traits. For detail, see Supplementary Tables 4 and 5\n\nLeaf appearance rate (LAR) represents the simplest case, as it can be measured both indoor and in the field with the same protocol. It was highly heritable in the diversity panel\\(^{31}\\) and\ntended to decrease across years of breeding elite maize hybrids9. Here, LAR was measured in the ‘recent hybrid panel’ in experiments either indoor or in two fields (Fig. 1, Table 1, Supplementary Tables 3, 4). Correlations between genotypic values indoor and in the field (Fig. 1a) were slightly better than those between one field and another one (Fig. 1b, r=0.57 and 0.49, respectively). Importantly, the ranking of hybrids and their distribution in highest and lowest quartiles were essentially conserved between indoor and field conditions, a necessary condition for breeding (Supplementary Table 4). Furthermore, these correlations and rankings were similar to those between fields for the duration of the vegetative phase, a trait that is already commonly measured in breeding programmes (Fig. 2ab).\n\n![Four scatter plots comparing observed and predicted leaf appearance rate (LAR) values between indoor and field, and using genomic information.](page_384_668_682_482.png)\n\nFig. 1. Leaf appearance rate (LAR) had similar correlations between genotypic values measured indoor and a field (a), as from one field to another field (b), and could be predicted based on genomic information (c,d). c: Comparison of observed mean genotypic values and mean (G-BLUP) predicted values in a 5-fold cross-validation scheme with 10 iterations, in the ‘diversity’ and ‘genetic progress’ panels. d: Comparison of observed mean genotypic values and predicted values in an independent dataset with elite recent hybrids, with observed values originating from data of a-b (BLUEs) and G-BLUP model calibration made using dataset of c. In a, b and d, light blue circles, mid-early hybrids (G2), dark blue squares, intermediate hybrids (G3), red triangles, mid-late hybrids (G4). In c, purple empty circles, diversity panel, red and yellow empty circles, genetic progress panel, hybrids released before 1980 and 2000, respectively; green empty circles, hybrids released after 2000. In a, r=0.57, p = 0.0066, \\( CV_{RMSE} = 7.7\\% \\). In b, r=0.49, p = 0.011, \\( CV_{RMSE} = 5.3\\% \\). In c, r=0.57, p = 2.20E-16, \\( CV_{RMSE} = 5.2\\% \\). In d, r=0.53, p = 0.00013, \\( CV_{RMSE} = 2.8\\% \\). For rho (spearman correlation of ranks) and other statistics, see Supplementary tables 4, 5.\nFig. 2. The duration of the vegetative phase, a trait measured in most breeding schemes, was not better related between different fields than other traits compared indoor and in the field in Fig. 1-4.\na and b: Comparison of observed values in 3 field experiments. c: Comparison of observed mean genotypic values and mean (G-BLUP) predicted values in a 5-fold cross-validation scheme with 10 iterations. d: Comparison of observed mean genotypic values and predicted values, in an independent dataset with elite recent hybrids. Observed values originate from data of a-b (BLUEs) and G-BLUP model calibration made using dataset of c. In a, b and d, light blue circles, mid-early hybrids (G2), dark blue squares, intermediate hybrids (G3), red triangles, mid-late hybrids (G4). In c, purple empty circles, diversity panel, red and yellow empty circles, genetic progress panel, hybrids released before 1980 and 2000, respectively; green empty circles, hybrids released after 2000. In a, r=0.69, p = 9.41E-09, \\( CV_{RMSE} \\) = 4.4%. In b, r=0.47, p = 0.000304, \\( CV_{RMSE} \\) = 7%. In c, r=0.84, p = 2.20E-16, \\( CV_{RMSE} \\) = 2.7%. In d, r=0.71, p = 3.19E-10, \\( CV_{RMSE} \\) = 2.5%. For rho and other statistics, see Supplementary tables 4, 5.\n\nPlant architecture is a more difficult case because its measurement relies on different principles in indoor vs field experiments (Fig. 3, Table 1, Supplementary Tables 3, 4). The architectural trait considered indoor (\\( rh_{PAD} \\)) was derived from 3D reconstructions of individual plants, via the difference in altitude between the top of the plant and the point where half of leaf area is reached, normalized by plant height\\(^{15}\\). This trait, which is closely related to light interception by a canopy\\(^{15}\\) and had heritabilities of 0.7 to 0.9 in different panels over several experiments\\(^{9,15}\\). It cannot be measured in the field, where 3D reconstruction of individual plants cannot be performed. Conversely, drone imaging in the field results in the calculation of a related trait, the Average Leaf inclination Angle (ALA), derived from the inversion of the\nradiative transfer model ‘PROSAIL’\\(^{38,39}\\), which takes into account the deviation of light interception efficiency of a given canopy in relation to a standard canopy having the same leaf area. The genotypic values of ALA measured in the field were well correlated to those of \\(rh_{PAD}\\) measured in a phenotyping platform in an experiment with 56 maize hybrids of the ‘genetic progress’ panel (Fig. 3a, Field 5, Supplementary Tables 3, 4). The same applied to 20 hybrids of the ‘recent hybrids’ panel in two field experiments, with good relationships between \\(rh_{PAD}\\) and ALA (Fig. 3bc), high heritability of both variables (Supplementary Fig. 2) and good conservation of lowest and highest quartiles (Supplementary Table 4). Notably, ALA values and heritability were very sensitive to crop phenological stage whereas those of \\(rh_{PAD}\\) were more stable (Supplementary Fig. 2). Hence, architectural data collected indoor are, in this case, as appropriate for characterizing each genotype in models of light interception, whereas ALA measured in the field would be more complex to use in this context.\n\n![Scatter plots comparing observed and predicted values for plant architecture traits](page_172_624_1097_1012.png)\n\nFig. 3. The genotypic values of two traits related to plant architecture had a high correlation, \\(rh_{PAD}\\) indoor and ALA obtained via drone imaging in the field (a,b,c); comparison between mean observed values and predicted values for plant architecture traits (d,e). a - c, coupled values of \\(rh_{PAD}\\) obtained\nvia indoor 3D imaging and values in fields 5, 4 and 2, with the “genetic progress” in a and the ‘recent hybrids’ panel in b and c. d. , Comparison of observed mean genotypic values and mean (G-BLUP) predicted values in a 5-fold cross-validation scheme with 10 iterations for \\( rh_{PAD} \\). e. Comparison of mean genotypic values of ALA in the independent dataset “recent hybrids” (observed BLUEs), with \\( rh_{PAD} \\) predicted values (BLUPs). \\( rh_{PAD} \\), relative altitude, from the top of the plant, where 50% of leaf area is reached\\(^{15}\\). ALA: average leaf angle estimated at flowering time from UAV images, via inversion of the model PROSAIL\\(^{38,71}\\). In a, b and d, light blue circles, mid-early hybrids (G2), dark blue squares, intermediate hybrids (G3), red triangles, mid-late hybrids (G4). In c, purple empty circles, diversity panel, red and yellow empty circles, genetic progress panel, hybrids released before 1980 and 2000, respectively ; green empty circles, hybrids released after 2000. In a, r=0.78, p=2.39e-12. In b, r=0.58, p = 0.012. In c, r=0.60, p = 0.009. In d, r=0.65, p = 2.20E-16, \\( CV_{RMSE} = 9.4\\%\\). In e, rho=0.34, p = 0.031 (r=0.28, p=0.08). For rho and other statistics, see Supplementary tables 4, 5.\n\nIn the same way the leaf expansion rate of individual plants (LER) can only be measured indoor (Table 1), with good heritability\\(^{40}\\). Corresponding measurements in the field are leaf area or leaf dimensions at given dates, so direct comparisons were not possible. However, we show below that the final width and length of maize 8\\(^{th}\\) leaf matched between indoor and field conditions for the diversity panel. Hence, final leaf dimensions potentially allow indirect calculation of LER in the field\\(^{41}\\).\n\nLeaf area index (LAI), a key feature for light interception and transpiration, is defined for a fraction of field canopy (typically 1m\\(^2\\)). Although heritable within a given field, it largely differs between fields in relation to environmental conditions and plant density\\(^{42}\\). It can be measured indoor, but a direct comparison makes no sense because the density and spatial arrangement of plants in indoor experiments make the considered canopy irrelevant to the field\\(^{24,43}\\). For such a case, we compared LAI measured in the field at flowering time to LAI simulated from upstream traits in indoor experiments (Table 1, Fig. 4). We compared (i) measured values in the field, obtained via UAV imaging and the inversion of the PROSAIL radiative transfer model\\(^{38,39}\\) with (ii) the LAI simulated by a crop model\\(^{11}\\) for which model inputs were the genotypic values of four traits measured in indoor platform (LAR, maximum leaf growth rate, response of leaf growth rate to VPD and final leaf number), plus plant density and the environmental conditions recorded every hour in the considered field. The correspondence between measured and estimated LAI, tested on the ‘genetic progress’ panel suggested that this approach is promising (r=0.63, Fig. 4, Supplementary Table 4). Notably, the PROSAIL model inversion allowing LAI estimation in the field resulted in values lower than 5 because light interception is nearly complete at these values of LAI\\(^{44}\\).\nFig 4. Genotypic values of leaf area index (LAI) measured in the field is correlated to LAI derived via a model from genotypic values of traits measured indoor and from environmental data in the considered field. Field values were obtained at flowering time from UAV images via inversion of the model PROSAIL\\(^{38,39}\\). Values on the x axis were obtained via the crop model of Lacube et al. (2020)\\(^{14}\\), fed with measured values of (i) environmental conditions in the same field, (ii) genotypic values measured in the platform for leaf appearance rate, maximum leaf growth rate, response of leaf growth rate to vapour pressure deficit (VPD) and final leaf number per plant. Each point represents a couple of observed genotypic values for one different hybrid of genetic progress panel. Dotted line, linear regression. \\( r=0.63,\\ p = 2.16E-06,\\ CV_{RMSE} = 22.9\\% \\). For rho and other statistics, see Supplementary table 4.\n\n![Scatter plot showing correlation between field and model-derived LAI values](page_153_120_370_370.png)\n\n- Finally, stomatal conductance represents the difficult cases in which traits cannot be directly measured at high throughput, either in the field or in indoor platforms. Its measurement for one leaf requires between 3 and 15 minutes, depending on the considered device, making high-throughput measurements impossible. However, it can be indirectly estimated at plant level in platform experiments by inversion of the Penman-Monteith equation, based on measurements of individual plant transpiration, leaf area, light and VPD\\(^{14}\\). Resulting estimations of whole-plant stomatal conductance were well related to leaf stomatal conductance measured via gas exchange, between well-watered and water deficit treatments (Fig. 5a, Supplementary Table 1), but also between genotypes in the well-watered treatment (\\( r^2 = 0.54 \\)). Because values measured in water deficit did not differ significantly in tested hybrids, the ranking of genotypic responses of stomatal conductance to water deficit can be estimated as the difference between well-watered and dry conditions for each tested hybrid.\n\nOverall, the ranking of genotypes for leaf appearance rate, plant architecture and LAI were consistent between field and indoor conditions, thereby opening the way for a prediction of values in the field based on platform information (Table 1, Supplementary Table 4). This could not be tested for stomatal conductance, for which field measurements cannot be performed and indirect measurements via canopy temperature are not precise enough in non-extreme conditions.\nFig. 5. Integrated stomatal conductance can be measured at plant level in an indoor phenotyping platform (a), and can be predicted from genomic information (cross-validation) (b). a, Comparison between values obtained at leaf level via gas exchange, and at plant level via inversion of the Penman-Monteith equation14, in well-watered and drought treatments. b, Comparison of observed mean genotypic values and mean (G-BLUP) predicted values in a 5-fold cross-validation scheme with 10 iterations for plant max stomatal conductance. In a, each symbol corresponds to coupled values of the results for gas exchange and inversion of the Penman-Monteith equation; blue, well-watered; red, water deficit. In b, each symbol corresponds to coupled values observed vs predicted. Purple empty circles, genetic progress panel, hybrids released before 1980 and 2000, respectively ; green empty circles, hybrids released after 2000. In a, black line, linear regression. In b, black line is the first bisector. In a, r=0.92, \\( CV_{RMSE} = 13\\% \\). In b, r=0.55, p = 2.20E-16, \\( CV_{RMSE} = 8.4\\% \\). For rho and other statistics, see Supplementary table 5.\n\nThe differences in absolute values of traits measured in indoor platforms or in fields are accounted for by relationships with environmental conditions\n\nBeyond the correlations between genotypic values of traits measured indoor and in the field, it is the absolute values of traits, measured in each experiment, that eventually drive the adaptation of studied genotypes to drought and high temperatures. For example, a correct estimation of genotype ranking for LAI has a very small impact on light interception if all genotypes have a LAI higher than 4, whereas the same genotype ranking in a range of LAI from 2 to 4 has a large impact44. Meta analyses showed that phenotypic values differ between controlled conditions and field24. However, they also largely vary from one field to another one11,24. Hence, we tested if the difficulty for translating values between two experiments may not be specific to field – platform comparisons, but would apply to comparisons between any environment and another one, depending on environmental conditions in each experiment.\nFig. 6. Leaf width (a) and length (b) respond to common environmental conditions in fields and indoor platforms. a: Relationship between leaf width (\\( W_{max,8} \\)) and the cumulated light intercepted by plants during leaf widening. b: Relationship between leaf length (\\( L_8 \\)) and leaf to air vapour pressure deficit (VPD\\(_{10}\\): mean of maximum daily values) during leaf elongation. Each point is a coupled value of maize hybrid (B73 x UH007) leaf dimension in one experiment and of the corresponding environmental condition. Leaf width and length values of four leaf ranks (8 to 11) were corrected for leaf rank so equivalent values for leaf 8 are presented\\(^{41}\\). Dot shapes represent leaf rank correspondence (from 8 to 11, circles, squares, diamonds and triangles, respectively). Blue dots: field data, red dots: platform data. Black lines, linear regressions. In a, \\( r=0.75,\\ p < 0.001 \\). In b, \\( r=0.62,\\ p < 0.001 \\).\n\nThis hypothesis was first tested by examining the mean absolute values of maize leaf length and width between field and indoor platforms for the diversity panel in Lacube et al. (2017)\\(^{41}\\). A superficial analysis would suggest that the mean dimensions of leaf 8 largely differed between indoor and field conditions, with a mean leaf length of 115 vs 76 cm, respectively, and a mean leaf width of 6.8 cm vs 7.5 cm, respectively (note the inversion of ranking between the two traits). However, leaf dimensions also largely varied among field experiments, from 6.8 to 10 cm for leaf width and from 68 to 102 cm for leaf length (Fig. 6ab). We showed earlier that leaf width depends on the amount of light intercepted during the growth of the considered leaf\\(^{41}\\). Accordingly, leaf width in the field was linearly related to the cumulated intercepted light (\\( r=0.75 \\)), and the same relationship accounted for the difference between experiments in fields and platform (Fig. 6a). In the same way, the large variability of leaf length, in field and controlled conditions, was accounted for by the vapour pressure deficit (VPD) during leaf growth (Fig. 6b, \\( r=0.62 \\)), consistent with studies showing a linear effect of VPD on leaf elongation rate\\(^{40}\\). Hence, leaf width and length did not differ intrinsically between indoor and field conditions: differences were accounted for by the same environmental conditions than those that accounted for differences between one field and another one, and could be calculated via a crop model\\(^{11}\\).\nA similar case occurred with temperature-dependent traits, such as the duration of the vegetative phase (Fields 1, 2 and 3, Supplementary Table 3) or the leaf appearance rate (Fields 1, 3 and PhenoArch, Supplementary Table 3). When expressed in calendar time, these trait values differed greatly between environments (Supplementary Fig. 1ab), whereas they were consistent if the effect of temperature was taken into account via a model of thermal time\\(^{45,46}\\). Expressed in this way, measured values were similar between field experiments for the duration of the vegetative phase and for LAR (Fig. 2ab, Fig. 1b, respectively) or between a field experiment and an indoor platform experiment (Fig. 1a), although some differences still existed between experiments (\\(CV_{RMSE} = 4.4\\%\\) and 7% in Fig. 2ab, \\(CV_{RMSE} = 5.3\\%\\) and 7.7% in Fig. 1ab). Among possibilities for explaining such differences in duration of the vegetative phase and LAR, the frequency of field visits was three days on average, but slightly differed between experiments.\n\nOverall, values translation from indoor platforms to field, and from one field to another field, could be carried out for a range of traits by taking into account appropriate environmental variables.\n\n**Measurements in indoor platforms can be used for genomic prediction of traits**\n\nHigh-throughput phenotyping allows characterization of some hundreds of genotypes (at most) whereas many thousands of genotypes are required for breeding\\(^{3,4}\\). In the same way, it would not be feasible to phenotype the offspring at each generation of speed breeding because of the resulting cost and workload\\(^{34,36}\\). Hence, the use of physiological traits in breeding requires one’s ability to predict them based on genomic information, as it is the case for yield\\(^{47,48}\\). We have tested this possibility for the traits presented in the former paragraphs. Briefly, we trained a G-BLUP model based on the 246 hybrids of the ‘diversity panel’ and the 56 hybrids of the ‘genetic progress’ panel (Supplementary Table 1). This training was performed with the genotypic means (BLUEs over the experiments carried out in Millet et al. (2019)\\(^{31}\\) and Welcker et al. (2022)\\(^{9}\\)) of the duration of the vegetative phase, the leaf appearance rate, maximum leaf expansion rate (calculated with two methods based on different assumptions, see Methods), the architectural trait \\(rh_{PAD}\\) and stomatal conductance. Predictions were performed using the genomic information at 440 000 polymorphic SNPs. Prediction accuracies and RMSEs were assessed either with a 5-fold cross-validation scheme (random sampling of hybrids using a stratification strategy for respecting the proportions of\ngenetic groups, Supplementary Fig. 4), or with an external validation set made of genotypic trait means estimated in the ‘recent hybrids panel’ (BLUEs over experiments, Supplementary Table 2).\n\n![Comparison of observed mean genotypic values and mean (G-BLUP) predicted values in a 5-fold cross-validation scheme with 10 iterations for plant max leaf expansion rate (LER). b, Comparison of observed mean genotypic values and predicted values for recent hybrids, with G-BLUP model calibration made using dataset of a. LER (Leaf Expansion Rate) was extracted from time courses of leaf area in the platform14 and determined as the slope of the linear regression between leaf area and thermal time during the period from 24 to 45 d20°C. In a, purple empty circles, diversity panel, red and yellow empty circles, genetic progress panel, hybrids released before 1980 and 2000, respectively; green empty circles, hybrids released after 2000. In b, light blue circles, mid-early hybrids (G2), dark blue squares, intermediate hybrids (G3), red triangles, mid-late hybrids (G4). In a, r=0.77, p = 2.20E-16, CV_{RMSE} = 8.7%. In b, r=0.33, p = 0.157, CV_{RMSE} = 13.6%. For rho and other statistics, see Supplementary table 5.](page_184_370_484_484.png)\n\nFig. 7. Maximum leaf expansion rate (LER) can be predicted from genomic information in cross validations in panels with large phenotypic variability but predictions are not accurate for the recent hybrids panel. a, Comparison of observed mean genotypic values and mean (G-BLUP) predicted values in a 5-fold cross-validation scheme with 10 iterations for plant max leaf expansion rate (LER). b, Comparison of observed mean genotypic values and predicted values for recent hybrids, with G-BLUP model calibration made using dataset of a. LER (Leaf Expansion Rate) was extracted from time courses of leaf area in the platform14 and determined as the slope of the linear regression between leaf area and thermal time during the period from 24 to 45 d20°C. In a, purple empty circles, diversity panel, red and yellow empty circles, genetic progress panel, hybrids released before 1980 and 2000, respectively; green empty circles, hybrids released after 2000. In b, light blue circles, mid-early hybrids (G2), dark blue squares, intermediate hybrids (G3), red triangles, mid-late hybrids (G4). In a, r=0.77, p = 2.20E-16, CV_{RMSE} = 8.7%. In b, r=0.33, p = 0.157, CV_{RMSE} = 13.6%. For rho and other statistics, see Supplementary table 5.\n\nCross-validation provided good predictive abilities for studied traits (Table 1). This was the case for leaf appearance rate (r = 0.57, CV_{RMSE} = 5.2% in Fig. 1c), leaf expansion rate (r = 0.77, CV_{RMSE} = 8.7% in Fig. 7a), rh_{PAD} (r = 0.65, CV_{RMSE} = 9.4% in Fig. 3d) and stomatal conductance (r = 0.55, CV_{RMSE} = 8.4% in Fig. 5b) (Supplementary Table 5). These values are similar but slightly lower than those for the duration of the vegetative phase in our study (r = 0.84, CV_{RMSE} = 2.7% in Fig. 2c), and for yield or flowering time traits in other studies48–51. Notably, genomic prediction performed similarly for the genotypes originating from the two panels, in spite of the difference of structure and origins of these panels (Supplementary Fig. 3ab) and the fact that measurements were performed in different experiments. The range of predicted values was expectedly smaller, for all tested traits, than that of observed values. This bias is linked to the fact that the narrow-sense heritability estimated using genomic additive and dominance relationships of studied traits was lower than 1 (0.84, 0.75, 0.73, 0.80 and 0.44 for the duration of the vegetative phase, LAR, leaf expansion rate, rh_{PAD} and stomatal conductance,\nrespectively), so the prediction based on genomic information cover a smaller range of values than original data.\n\nThe ‘recent hybrid panel’ (used for external validation) covered smaller ranges of trait phenotypic values than those in the ‘diversity’ and ‘genetic progress’ panels considered jointly. As a consequence, the comparison of observed vs predicted values led to lower prediction accuracies than in the case of cross validation (Table 1). This applied to traits measured indoor (LAR, Fig. 1d, LER, Fig. 7b and rh_{PAD}, Fig. 3e) as well as for the duration of the vegetative phase measured in the field (Fig. 2d) (Supplementary Table 5), so this problem was not specific of indoor genomic prediction.\n\nDiscussion\n\nThree conditions can be considered as requirements for traits measured indoor to be used in trait-based selection in a context of climate change. Firstly, traits measured indoor should be genetically correlated to those in fields (regardless of absolute values either indoor or in each field), so indoor breeding is relevant to field conditions. Secondly, the absolute value of indoor traits should translate to that in fields with diverse climate scenarios, either directly or via models. Finally, indoor traits need to be predicted with sufficient accuracy from the genomic information of non-phenotyped genotypes.\n\nThe traits presented here satisfied the first condition. Close correlations were observed between the genotypic values of traits measured indoor and in multi-site field experiments. This was the case when the considered trait was measured with similar protocols indoor or in the field, for instance leaf appearance rate or the duration of the vegetative phase. It was also the case when the trait was measured with different methods as in the case of plant architecture. Finally, the integrated trait LAI, which is highly dependent on the plant density and environmental conditions in the considered canopy, required a method involving crop modelling. The correlations observed in these three cases between indoor platform and fields are therefore higher (r= 0.57 to 0.78, Table 1) than those reported by Poorter et al. (2016)\\(^{24}\\) for a set of growth-related traits meta-analysis (median r = 0.51). Two reasons may explain this disparity. (i) Traits considered in Poorter’s meta-analysis, namely yield, leaf nitrogen concentration and specific leaf area are more integrated than those studied here (except LAI) and, therefore more prone to high genotype x environment interactions and changes in the\nranking of genotypes. (ii) The traits studied here had moderate to high heritabilities over experiments, thereby showing a low residual variance resulting from experimental errors. Furthermore, measuring yield or yield components in phenotyping platforms is probably not relevant because these traits result from cumulative processes over a long period, during which conditions indoor are very different from those in the field. For such case, the use of modelled phenotypic values is probably preferable, as we show here for the case of leaf area index.\n\nThe second condition, namely that trait values can translate from indoor conditions to a diversity of fields, was fulfilled for the traits reported here provided that the differences in environmental conditions were taken into account.\n- Modelling temperature effects allowed consistency between field and platform experiments for leaf appearance rate and the duration of the vegetative phase in this study. This result can be generalized to traits related to the progression of plant development of many species. In particular, germination rate, leaf appearance rate, the reciprocal of the duration of growth of individual leaves and reproductive organs are common to a large range of environments provided that they are expressed in thermal time\\(^{52}\\). Crop models, based on this result, successfully predict plant phenology in wide ranges of environments\\(^{30,8}\\).\n– The amount of intercepted light was also needed for other traits to be consistent between experiments. This was the case here for maize leaf width measured indoor and in several fields. Beyond this particular trait, Monteith (1994)\\(^{44}\\) showed that biomass accumulation is proportional to the cumulated light intercepted by plants. In particular, we showed that, in a series of experiments with maize, the time course of plant biomass largely differed between experiments but was consistent if expressed as a function of intercepted light\\(^{16}\\). Again, crop models based on intercepted light can predict plant biomass accumulation with reasonable accuracy\\(^{30,53}\\).\n- Plant water status was, in addition, necessary to account for differences in traits related to organ expansive growth (expressed in terms of volume or length). Its effect can be predicted from the cell scale\\(^{54}\\) to the organ scale\\(^{55–57}\\). Here, this was the case for leaf length in well-irrigated maize fields, as a function of air VPD. Leaf elongation rate is closely related to a combination of soil water potential and VPD in maize, Festuca or barley\\(^{55,58}\\), so our result can probably be extended to other species. Stomatal conductance can also be predicted from a\ncombination of soil water status, evaporative demand and incident light via functional models involving chemical and hydraulic signals\\(^{59}\\). Crop models that take into account light, soil water content and evaporative demand can predict stomatal conductance and net photosynthesis by simulating physiological processes\\(^{60,61}\\), so photosynthesis in controlled conditions can be extended to a range of field conditions\\(^{61}\\).\n\nOverall, we confirmed that raw phenotypic traits cannot translate directly from indoor platforms to fields, as reviewed in Poorter et al. (2016)\\(^{44}\\). However, taking into account specific environmental conditions allowed this translation for the range of traits presented here, which depend on one or two environmental conditions. Again, more integrated traits such as leaf area index, grain number or grain yield measured in a platform cannot be directly extended to field via simple relationships as presented in former paragraphs. These traits can be predicted in a range of field conditions based on genotype-specific parameters and environmental conditions measured in the considered fields. This was the case here for leaf area index, based on a dynamic model\\(^{11}\\), but was also the case for grain number and grain yield in a multi-site field experiments, based on a mixed model involving genetic parameters and environmental conditions\\(^{31}\\).\n\nThe third condition was that traits can be predicted from genomic information. Here, cross-validation based on a large genetic range showed good results (compared to Guo et al. (2020)\\(^{51}\\), Yuan et al. (2019)\\(^{50}\\) or Toda et al. (2020)\\(^{48}\\)), with r ranging from 0.55 to 0.84 for the studied traits (Table 1, Supplementary Table 5). External validation on the panel of recent hybrid varieties provided less accurate results, but correlations between predicted and observed values still ranged from 0.33 to 0.71 and mostly with significant p-values (from 3.2\\times10^{-10} to 0.031) and acceptable CV of errors (from 2.5% to 15.8%) (Supplementary Table 5). By using this panel for external validation, we chose the most challenging case, in which one attempts to use genomic prediction, trained with a panel with wide genetic variability, and tested with elite genotypes that have a reduced phenotypic variability for studied traits. Hence, our results could not be considered as fully satisfactory if the purpose was to rank elite genotypes (Supplementary table 5). Conversely, the cross-validation in a wider genetic range suggests that genomic prediction may be used for identifying genotypes with high or low genotypic values for studied traits in breeding populations with higher genetic and phenotypic variabilities, thereby allowing the design of ideotypes with contrasting strategies in relation to\nwater and heat stress, namely 'conservative' ideotypes with low stomatal conductance, leaf growth, leaf appearance rate, for stress-prone areas, vs 'spender' ideotypes with highest values for each of these traits.\nMethods\n\nGenetic material. Three panels of maize hybrids were used in this study (Supplementary Table 1). First, a diversity panel included 246 hybrids resulting from the cross of a common flint parent (UH007) with 246 dent lines that maximized the diversity in the dent group while keeping a restricted flowering window\\(^{31,62}\\). This panel involved four genetic groups, namely lodent (39 hybrids), Lancaster (45 hybrids), Stiff-Stalk (55 hybrids) and diverse-dent hybrids (107) consisting in an admixture of the former three groups\\(^{62}\\). Second, a ‘genetic progress’ panel included 56 highly successful commercial hybrids released on the European market from 1950 to 2015\\(^9\\). This panel showed a limited range of maturity classes, from mid-early (FAO 280) to mid-late (FAO 480), covering the largest growing area in Europe. Finally, a ‘recent hybrids’ panel included 86 commercial hybrids released from 2008 to 2020, belonging to mid-early to mid-late maturity classes (Supplementary Table 2). Yield data in 30 sites x 2 years per hybrid were available at the beginning of this study (ARVALIS, www.varmais.fr)\n\nPlatform experiments. Platform experiments were performed in PhenoArch, an indoor robotized and image-based phenotyping platform that allows precise measurement of plant architecture, plant phenology and growth, transpiration, stomatal conductance and water use efficiency (https://www6.montpellier.inrae.fr/lepse/Plateformes-de-phenotypage-M3P/Montpellier-Plant-Phenotyping-Platforms-M3P/PhenoArch,\\(^{16}\\)) hosted at Montpellier Plant Phenotyping Platforms (M3P). The diversity panel was evaluated in four experiments (in spring 2012, 2013 and 2016, and winter 2013) described in Prado et al. (2018)\\(^{14}\\). Three or two plants per hybrid were grown depending on the experiment (Supplementary Table 1). The ‘genetic progress’ panel was evaluated in four experiments, with most data used here originating from an experiment with seven replicates per hybrid\\(^9\\). A subset of 20 hybrids of the ‘recent hybrids’ panel was evaluated in one experiment during winter 2021, with three replicates per hybrid. All experiments followed an alpha-lattice design, with two levels of soil water content imposed, namely retention capacity (well-watered, soil water potential of −0.05 MPa) and water deficit (soil water potential from −0.3 to −0.6 MPa depending on the experiment). Soil water content in pots was maintained at target values by compensating transpired water three times per day via individual measurements of each plant\\(^{16}\\). Soil water potential was estimated from soil water content based on a water release curve\\(^{14}\\). Air temperature and humidity were measured at six positions in the platform every 15 min. Daily\nincident photosynthetic photon flux density (PPFD) over each plant within the platform was estimated by combining a 2D map of light transmission, and the outside PPFD measured every 15 min with a sensor placed on the greenhouse roof\\(^{16}\\). The greenhouse temperature was maintained at 25 ± 4 °C during the day and 17 ± 2 °C during the night. Supplemental light was provided either during daytime when external solar radiation was below 300 W m\\(^{-2}\\) or to extend the photoperiod by using 400 W HPS Plantastar lamps.\n\nIn each experiment, the number of visible leaves of every plant was manually scored weekly during the vegetative phase. Leaf appearance rate (LAR, reciprocal of the phyllochron) was calculated as the slope of the linear relationship between the number of visible leaves and thermal time, during the period from plant emergence to 12-leaf stage. Red-Green-Blue (2056 × 2454) images taken from 13 views (12 side views from 30° rotational difference and one top view) were captured daily for each plant during the night. Plant pixels from each image were segmented from those of the background and used for estimating the whole plant leaf area and fresh biomass\\(^{63}\\). The time courses of leaf area and plant fresh biomass were then fitted individually by using P-spline growth curve models\\(^{64}\\). The architectural trait \\( \\mathrm{rh}_{PAD} \\) was calculated daily from 3D reconstructions of each plant, based on RGB images at PhenoArch platform\\(^{15}\\). \\( \\mathrm{rh}_{PAD} \\) index represented the point in the distribution of leaf area along the stem (from the top of the plant, relative to total plant height) where half of the cumulative leaf area is reached. Whole-plant stomatal conductance was calculated over 4 time-periods per day for 20 days for each hybrid plant in PhenoArch platform, via inversion of the Penman–Monteith equation based on transpiration, plant growth, net radiation and VPD collected in the experiment\\(^{14}\\). Its value under saturating light was estimated for each hybrid by combining coupled values of stomatal conductance and incident light observed in all experiments. The maximum leaf expansion rate (LER) was extracted from time courses of leaf area in the platform and corresponded to the maximum first-order derivative of P-spline fitted growth curves from 24 to 45 days at 20°C after emergence\\(^{64}\\). Because this method provided somewhat unstable results, we also calculated maximum LER as the slope of the linear regression between leaf area and thermal time during the whole period from 24 to 45 days at 20°C.\n\nGenotypic values (BLUEs) for each trait were calculated by correcting raw traits values for spatial effects, by fitting a mixed model (R package SpATS,\\(^{65}\\)), with a fixed term for genotype and random effects for rows and columns as well as a smooth surface defined on row and\ncolumn coordinates. Broad-sense heritabilities were calculated daily with the same R package, using the same model but with the genotype effect included as a random term. Regarding longitudinal traits, genotypic values at individual time points, t, were obtained from their smoothed time series using a generalized additive model fitted to the spatially adjusted daily measurements, \\( \\tilde{y}_{i,k}(t) \\), for each plant k of genotype i (model 1):\n\n\\[\n\\tilde{y}_{i,k}(t) = \\alpha_i + f_i(t) + \\epsilon_{i,k}(t), \\quad \\epsilon_{i,k}(t) \\sim N(0, \\sigma^2)\n\\] (1)\n\nwhere \\( \\alpha_i \\) is a genotype-specific intercept, \\( f_i(t) \\) is a genotype-specific thin plate regression spline function on time, and \\( \\epsilon_{i,k}(t) \\) is a random error term (R package statgenHTP,\\(^{64,66}\\)). Narrow-sense heritability was estimated for each trait with a model considering genomic-based additive and dominance relationship matrices\\(^{67}\\), using the R package “Heritability”\\(^{68}\\).\n\nField experiments. The diversity panel was grown in 25 experiments (defined as combinations of site × year × water regime), either rainfed or irrigated, in ten sites in 2012 or 2013\\(^{31}\\). Sites were distributed on a west–east transect across Europe, at latitudes from 44° to 49° N. The ‘genetic progress’ panel was grown in 26 field experiments either rainfed or irrigated, in 16 European sites from 2010 to 2017 spread along the same climatic transect as for experiments with the diversity panel\\(^{9}\\). The ‘recent hybrids’ panel was grown in four field experiments under irrigated conditions in the same range of latitudes, in 2021 or 2022 in France (Supplementary Table 3). Experiments followed an alpha-lattice design or randomised complete block design (RCBD) and were split by varieties maturity classes (Supplementary Table 3), each with three replicates of four-rows plots, 6 m long. The targeted plant density was 9 plants m\\(^{-2}\\). In all experiments, anthesis and silking dates were scored by visiting experiments every third day. The number of appeared leaves was scored every week on ten plants per hybrid during the vegetative phase, and leaf appearance rate was calculated as in indoor experiments (Supplementary Table 3).\n\nThe duration of the vegetative phase was defined as the period from plant emergence to anthesis, expressed in thermal time (equivalent days at 20 °C,\\(^{45}\\)). Leaf appearance rate was estimated as in platform experiments.\n\nUAV flights were performed three times in one experiment of the ‘genetic progress’ panel during the period from plant emergence to flowering, and seven times in two experiments for the ‘recent hybrids’ panel during the same period (Supplementary Table 3). Quadcopter\ndrone (DJI Phantom 4) were equipped with a DJI multispectral camera with 5.7 mm focal length lens, acquiring 1600x1300 pixel images. They flew at a controlled altitude of 20 m and a constant speed of 2.2 m s\\(^{-1}\\) for about 20 min per flight, with images captured at a one-second interval. Flights were performed during clear and cloudless days between 8:00 and 10:00 solar time. An automatic image-processing pipeline was applied by Hiphen, Avignon, France (http://www.hiphen-plant.com), following methods presented in Blancon et al. (2019)\\(^{20}\\). Environmental variables were recorded every hour in all experiments, including light, air temperature, relative humidity (RH), rainfall and wind speed. Soil water potential was measured every day with tensiometers at 30, 60, and 90 cm depths with three or two replicates, located in plots sown with a common reference hybrid.\n\nThe architectural trait ALA (Average Leaf inclination Angle to the soil level) and Leaf Area Index (LAI) were calculated by inversion of the PROSAIL model\\(^{38,69}\\), based on multispectral images of field UAV flights. The PROSAIL model couples the PROSPECT leaf optical properties model with the SAIL canopy bidirectional reflectance model. It links the spectral variation of canopy reflectance, which is mainly related to leaf biochemical contents, with its directional variation, which is primarily related to canopy architecture and soil/vegetation contrast\\(^{70}\\). This link allows simultaneous estimation of canopy biophysical/structural variables from remote sensing, including ALA and LAI traits\\(^{39,71}\\).\n\nLeaf area index was also calculated by using a crop model (APSIM model as modified in Lacube et al. (2020)\\(^{11}\\)) parameterized with the genotypic values (BLUEs) of four traits measured in PhenoArch platform (LAR, maximum leaf growth rate, response of leaf growth rate to VPD and final leaf number), plus the environmental and growing conditions recorded in the considered field.\n\nSpatial corrections, calculations of genotypic values and heritabilities of traits were performed with the same methods as in indoor experiments.\n\nCorrelation analysis between experiments. Pearson (r) and Spearman (rho) correlation coefficients were calculated to evaluate to which extent the genotypic values of traits match between experiments, either in one field and another one, or in one field and the indoor platform. Both types of correlations was performed on the hybrids that were common to considered experiments (common hybrids number ranged from 18 to 56, Supplementary\nTables 2, 4). Significance of correlation coefficients was evaluated based on the null hypothesis that there is no correlation between the variables (r or rho = 0). Root mean squared error of estimations (RMSE) and bias showing the discrepancy between experiments genotypic values were also calculated. We present them as a coefficient of variation of the error (\\( \\mathrm{CV}_{\\mathrm{RMSE}} \\)) or bias (\\( \\mathrm{CV}_{\\mathrm{Bias}} \\)), which is the RMSE or bias expressed as a percentage of the mean value. Finally, to appreciate the consistency between experiments of the highest and lowest genotypic values, we evaluated the frequency of similar assignment to the highest or the lowest quartile between experiments for each trait. This consisted in estimating how many hybrids of the highest quartile of one experiment were also present in the highest quartile of the other experiment (Supplementary Table 4). The same was performed for the lowest quartile.\n\nGenotypic data and Diversity analyses. All panels were genotyped using the 600K Affymetrix® Axiom® array\\(^{72}\\). Genotypes of the hybrids were either inferred from genotypes of the parental lines (diversity panel) or resulted from the direct genotyping of the hybrids (genetic progress and recent hybrids panels). After quality control, 440 000 polymorphic SNPs were retained for diversity analyses and genomic prediction (excluding SNPs with minor allele frequency lower than 0.05 and/or missing values for more than 20% of hybrids). Missing values were otherwise imputed using BEAGLE v3\\(^{73}\\).\n\nGenotypic data generated were organized as M matrices with N rows and L columns, N and L being the panel size and number of markers, respectively. Genotype of hybrid n at locus (SNP marker) j was coded as 0 (the homozygote for B73 line allele), 1 (the heterozygote) or 2 (the other homozygote). “snpReady” R package\\(^{74}\\) was used to estimate observed heterozygosity as \\( H_0 = 1/L \\sum_{j=1}^L (nH_j/N) \\) and Nei’s index of genetic diversity as \\( \\mathrm{Nei\\_GD} = 1/ L \\sum_{j=1}^L (1 - p_j^2 - (1 - p_j)^2) \\), with N the number of hybrids, nH\\(_j\\) is the number of heterozygous hybrids at the j\\(^{\\text{th}}\\) biallelic locus, L is the total number of loci, and p\\(_j\\) is the frequency of the reference (B73 line allele) at locus j. Principal Coordinate Analysis (PCoA) was also performed on SNP markers data (Supplementary Fig. 3).\n\nGenomic prediction model. Genomic predictions of each trait was performed with a genomic best linear unbiased prediction model (GBLUP-AD), including random additive and dominance effects (model 2) :\n\n\\[\ny = \\mu 1_n + Z_a a + Z_d d + \\varepsilon\n\\]\n\n(2)\nwhere y is the vector of trait genotypic means (BLUEs over experiments) of n hybrids, \\( \\mu \\) is the overall mean (intercept), a is the vector of additive genetic effects, and is assumed to follow a normal distribution \\( \\sim N(0, G_A \\sigma_a^2) \\) with \\( G_A \\) as the genomic-based additive relationship matrix described below and \\( \\sigma_a^2 \\) as the additive genetic variance; d is the vector of random dominance effects which follows a normal distribution \\( \\sim N(0, G_D \\sigma_d^2) \\) with \\( G_D \\) as the genomic-based dominance relationship matrix described below and \\( \\sigma_d^2 \\) as the dominance genetic variance; \\( \\varepsilon \\sim N(0, I \\sigma_\\varepsilon^2) \\) is the vector of random residual effects, where I denotes the identity matrix and \\( \\sigma_\\varepsilon^2 \\) is the residual variance. \\( Z_a \\) and \\( Z_d \\) are the incidence matrices for a and d, respectively.\n\nThe genomic-based relationship matrices were built as defined in Vitezica et al. (2017)\\(^{67}\\) and González-Diéguez et al. (2021)\\(^{75}\\). The genomic-based additive relationship matrix (\\( G_A \\)), called realized relationship matrix was estimated as \\( G_A = \\frac{H_a H_a'}{tr(H_a H_a')/N} \\) where \\( H_a \\) is a rescaled genotype matrix \\( H_a = M - P \\), where M is the genotype matrix coded as 0, 1, and 2 for genotypes BB, Bb and bb respectively and with dimensions number of hybrids (N) by number of loci (L); P is the matrix of locus scores 2p,, with p_j being the reference allele frequency of the j\\textsuperscript{th} SNP biallelic locus (having alleles B/b); tr is the trace. The genomic-based dominance relationship matrix (\\( G_D \\)) was estimated as \\( G_D = \\frac{H_d H_d'}{tr(H_d H_d')/N} \\) where \\( H_d \\) is the matrix containing elements h_d for each individual and locus equal to:\n\n\\[\nh_d = \\begin{cases}\n-2p_{BB}p_{bb} [p_{BB} + p_{bb} - (p_{BB} - p_{bb})^2]^{-1} \\\\\n4p_{BB}p_{bb} [p_{BB} + p_{bb} - (p_{BB} - p_{bb})^2]^{-1} & \\text{for genotypes } \\begin{cases} BB \\\\ Bb \\\\ bb \\end{cases}\n\\\\\n-2p_{Bb}p_{BB} [p_{BB} + p_{bb} - (p_{BB} - p_{bb})^2]^{-1}\n\\end{cases}\n\\]\n\nwhere \\( p_{BB}, p_{Bb} \\) and \\( p_{bb} \\) are the genotypic frequencies for the genotypes BB, Bb and bb respectively at the locus.\n\nFor moderate heritability physiological traits (LER and gs max), in addition to random additive and dominance effects estimated from genomic-based relationship matrices, the genotypes of markers associated to quantitative trait loci (QTLs), previously identified in a genome-wide association study (GWAS) of the diversity panel\\(^{14}\\), were added as fixed effects in prediction models (3):\n\n\\[\ny = \\mu 1_n + X \\beta + Z_a a + Z_d d + \\varepsilon\n\\]\n\nwhere X is an n × l marker genotype matrix for n hybrids and l markers associated to trait QTLs and \\( \\beta \\) is the markers fixed effects vector.\nOther genomic prediction models (RR-BLUP, BayesB, BayesC and BayesR) were also tested but showed no significantly better results than those presented in this paper.\n\nAll prediction models were fitted using the Bayesian Generalized Linear Regression (BGLR) R package\\(^{76}\\), based on 60 000 iterations, after discarding 10 000 cycles for burn-in period and using a thinning rate of 5.\n\nTraining and validation schemes of genomic predictions. Genomic predictions were first evaluated by a 5-fold cross-validation scheme repeated ten times, applied to diversity and genetic progress panels datasets. Each training set was sampled randomly but proportionally to ‘diversity panel’ genetic groups and across years of release of ‘genetic progress’ hybrids (Supplementary Fig. 4). This sampling method was chosen to maintain a good coverage of the total genetic space covered by the training set\\(^{77}\\). The ‘recent hybrids’ panel dataset was then considered as an external validation of the prediction models. 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A powerful tool for genome analysis in maize: development and evaluation of the high density 600 k SNP genotyping array. BMC Genomics 15, 823 (2014).\n\n73. Browning, B. L., Zhou, Y. & Browning, S. R. A One-Penny Imputed Genome from Next-Generation Reference Panels. The American Journal of Human Genetics 103, 338–348 (2018).\n\n74. Granato, I. S. C. et al. snpReady: a tool to assist breeders in genomic analysis. Mol Breeding 38, 102 (2018).\n\n75. González-Diéguez, D. et al. Genomic prediction of hybrid crops allows disentangling dominance and epistasis. Genetics 218, iyab026 (2021).\n\n76. Pérez, P. & de los Campos, G. Genome-Wide Regression and Prediction with the BGLR Statistical Package. Genetics 198, 483–495 (2014).\n\n77. Bustos-Korts, D. et al. Combining Crop Growth Modeling and Statistical Genetic Modeling to Evaluate Phenotyping Strategies. Front. Plant Sci. 10, 1491 (2019).\nAcknowledgements\n\nAuthors are grateful to M. Lis, R. Le Roy and M. Combes for their technical assistance in the PhenoArch experiment, as well as to key persons from the 2021 and 2022 field experiments at ARVALIS, namely: Y. Pousset, P. Raccurt, S. Bourrely, F. Binet, D. Lasserre, L. Pligot, C. Huet, M. Heredia, L. Diez, C. Drillaud and B. Baron. We are also grateful to I. Granato, N. Abu-Samra Spencer, E. Millet, S. Prado and C. Fournier for their help with data analysis or advice for R packages. This work was supported by ARVALIS, INRAE and ANRT’s CIFRE fundings.\n\nAuthor contributions\n\nJB, LM, CW, MB and FT and MB designed research. JB performed experiments, supervised by KB, NM, CW and MB. LI CB and RC performed experiments. JB, LM, CW and MB performed genomic analyses, JB, CW and FT performed phenotypic and modelling analyses. FT, JB, CW, LM and MB wrote the paper.\n\nCompeting interests\n\nThe authors declare no competing interests.\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• Supplementaryinformatonbouidghaghen.pdf"} {"paper_id": "prb72", "title": "DeBreak: Deciphering the exact breakpoints of structural variations using long sequencing reads", "text": "DeBreak: Deciphering the exact breakpoints of structural variations using long sequencing reads\n\nYu Chen\nUniversity of Alabama at Birmingham https://orcid.org/0000-0002-2037-7337\nAmy Wang\nUniversity of Alabama at Birmingham https://orcid.org/0000-0003-0478-2313\nCourtney Barkley\nUniversity of Alabama at Birmingham\nXinyang Zhao\nUniversity of Alabama at Birmingham\nMin Gao\nUniversity of Alabama at Birmingham\nMicky Edmonds\nUniversity of Alabama at Birmingham\nZechen Chong (zchong@uab.edu)\nUniversity of Alabama at Birmingham https://orcid.org/0000-0001-5750-1808\n\nMethods Article\n\nKeywords:\n\nPosted Date: January 21st, 2022\n\nDOI: https://doi.org/10.21203/rs.3.rs-1261915/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\nDeBreak: Deciphering the exact breakpoints of structural variations using long sequencing reads\n\nYu Chen1,2, Amy Y. Wang2,3, Courtney A. Barkley1, Xinyang Zhao4, Min Gao2,5, Mick D. Edmonds1, and Zechen Chong1,2,*\n\n1Department of Genetics, Heersink School of Medicine, University of Alabama at Birmingham, Birmingham, AL 35294, USA. 2Informatics Institute, Heersink School of Medicine, University of Alabama at Birmingham, Birmingham, AL 35294, USA. 3Department of Medicine, Division of General Internal Medicine, Heersink School of Medicine, University of Alabama at Birmingham, Birmingham, AL 35294, USA. 4Department of Biochemistry and Molecular Genetics, Heersink School of Medicine, University of Alabama at Birmingham, Birmingham, AL 35294. 5Department of Medicine, Division of Cardiovascular Disease, Heersink School of Medicine, University of Alabama at Birmingham, AL 35233 Birmingham, USA.\n\n* Correspondence: zchong@uabmc.edu\n\nAbstract\n\nLong-read sequencing has demonstrated great potential for characterizing all types of structural variations (SVs). However, existing algorithms have insufficient sensitivity and precision. To address these limitations, we present DeBreak, a novel method for comprehensive and accurate SV discovery. Based on alignment results, DeBreak employs a density-based approach for clustering SV candidates together with a local de novo assembly approach for reconstructing long insertions. A partial order alignment algorithm ensures precise SV breakpoints with single base-pair resolution, and a k-means clustering method can report multi-allelic SV events. DeBreak outperforms existing tools on both simulated and real long-read sequencing data from both PacBio and Nanopore platforms. An important application of DeBreak is analyzing cancer genomes for potentially tumor-driving SVs. DeBreak also demonstrates excellent performance in supplementing whole-genome assembly methods.\n\nIntroduction\n\nIn humans, structural variations (SVs), or genomic rearrangements, including deletions, insertions, inversions, duplications, translocations, and complex forms of multiple events,\ncompose the majority of genomic variations. At nucleotide level, SVs contribute more diversity than other types of variants\\( ^{1-3} \\) and play a pathogenic role in a wide range of genomic disorders\\( ^{4-8} \\). In non-human organisms, SVs are also associated with various phenotypes\\( ^{9-11} \\). Therefore, comprehensive characterization of all forms of SVs is critical for fully understanding their contribution to genetic diversity, species divergence, and other phenotypic traits.\n\nThe currently available real-time long-read sequencing platforms, Pacific BioSciences (PacBio) and Oxford Nanopore, generate very long reads (\\( >20 \\) kbp on average) and have demonstrated superior performance over short reads on SV discovery. For example, many rare genetic diseases have been solved using long-read sequencing technologies\\( ^{12-15} \\). Long-read sequencing can potentially delineate the full landscape of SVs in individual genomes. By sequencing and analyzing a haploid human genome (CHM1) using single-molecule, real-time (SMRT) DNA sequencing, Chaisson et al.\\(^{16}\\) resolved the complete sequence of 26,079 euchromatic structural variations, which is a 6-fold increase when compared with a previous study\\( ^2 \\) using short read sequencing, and most of these SVs had not been reported previously. Recent work by the Human Genome Structural Variation Consortium (HGSVC) resulted in a 7-fold increase in SV number using multiple platforms in which the PacBio results contributed the most\\( ^3 \\).\n\nAlthough great strides have been made, existing computational tools for SV detection using long reads remain few in number and can be further enhanced and optimized. These methods usually can only characterize a subset of SVs, and sensitivity and precision are not ideal. For example, PBHoney\\( ^{17} \\) uses BLASR\\( ^{18} \\) to map the PacBio subreads to collect soft-clipped reads and remap clipped tails (\\( >200 \\)bp) to compose a “piece alignment”. However, PBHoney can only infer simple deletions, tandem duplications, inversions, and translocations and does not perform well for insertions and other types of SVs. Another alignment-based method, Sniffles\\( ^{19} \\) uses both within-read alignments and split-read alignments from NGMLR aligner. Sniffles can analyze both PacBio and Nanopore sequencing data and report some\ncomplex forms of SVs besides simple SVs. For both PBHoney and Sniffles, the breakpoints inferred from clusters of alignments usually are not precise, preventing experimental validation and mechanism analysis\\(^{20-23}\\) that rely on SV junction sequences. Moreover, both tools are deficient in detecting the full spectrum of SVs. For instance, long insertions close to or longer than nearby read lengths are often missed. These issues remain a concern with a recently published alignment-based method, CuteSV\\(^{24}\\).\n\nBesides alignment-based methods, methods using local *de novo* assembly of mapped reads are also applied to SV discovery\\(^{3,16,25}\\). These local assembly-based methods utilize reads from haploid genomes or phased reads from diploid genomes and perform *de novo* assembly in a window. The consensus sequences generated can usually identify precise breakpoints. However, they only report deletions, insertions, and subsets of inversions. During phasing, only about two-thirds of reads in each sample can be haplotype-partitioned. These partitions require different tools applied to the data from other platforms, preventing more generic and broader applications of SV analysis.\n\nWhole genome *de novo* assembly can be considered the ultimate solution for SV characterization. Although researchers have made progress on this front\\(^{26-29}\\), whole genome *de novo* assembly with long noisy reads is inherently challenging. It requires high-coverage sequencing data, and difficulties remain in dealing with long repetitive sequences, tandem repeats, as well as heterozygosity. Moreover, whole genome *de novo* assembly usually requires high-memory computing nodes and long running time, and it is difficult to evaluate accuracy.\n\nHere, we present DeBreak, a novel algorithm for comprehensive and accurate SV discovery from long reads. DeBreak detects SV events using two different strategies, depending on whether SVs can be spanned within reads (**Fig. 1**, Methods). For SVs contained within reads, DeBreak scans all read alignments for raw SV signals for each category of SV, and then clusters these signals using a unique density-based clustering algorithm with flexible clustering window sizes. This approach allows accurate SV candidate identification for SVs with varying\nlengths and local sequence contents. In the next step, the SV breakpoint refinement with partial order alignment (POA)\\(^{30}\\) algorithm can accurately infer SV breakpoints with single base-pair resolution. With its automatic sequencing-depth estimation and parameter optimization, DeBreak filters SV candidates and reports a high-confidence SV callset with genotyping information. For SVs that are too large to be spanned within reads, DeBreak first identifies candidate SV breakpoints and then performs local *de novo* assembly to reconstruct SV containing sequences. DeBreak completes the analysis by integrating all identified SV events together to form a final, confident SV callset.\n\nResults\n\nBenchmark on simulated dataset\n\nTo benchmark the performance of SV discovery, we first compared DeBreak with three SV callers, Sniffles, pbsv, and cuteSV, using *in silico* datasets. A total of 22,200 SVs were simulated and embedded into the human reference genome (GRCh38), serving as the ground truth. The sizes of simulated SVs follow similar distributions observed in real human samples, with Alu and LINE peaks\\(^{31}\\) (**Fig S1**). Long reads were simulated based on a modified genome with pbsim\\(^{32}\\) and aligned to the human reference genome. To mimic PacBio reads generated from different library preparation protocols, three sets of data with different insert sizes were simulated (**Fig S1b**). We applied these SV callers to identify SVs and compared the SV callsets to the ground truth to assess SV discovery accuracy for each SV caller. In all five types of simulated SVs, DeBreak consistently achieved the highest F1 scores among the four tested SV callers (**Table 1**, **Fig S2a**). All evaluated SV callers have a critical parameter—“minimum number of supporting reads”—which determines the sensitivity of SV detection for these tools. We manually set the parameter of “minimum number of supporting reads” to a series of values for each caller and assessed the sensitivity of SV discovery at different thresholds.\nAlthough the recall of all SV callers dropped as the number of supporting reads increased, DeBreak consistently demonstrated the highest sensitivity at each threshold (Fig S2b).\nWe then investigated the accuracy of detection of SV breakpoints. By refining SV breakpoints with the partial order alignment algorithm, DeBreak reconstructed the consensus sequences flanking the SVs, which showed much higher base accuracy than the raw reads (Fig. S3a).\nFrom the accurate consensus sequences, DeBreak can infer more precise SV breakpoints than merely from the raw reads (Fig S3b). DeBreak identified 59.81% of SVs with exact breakpoint positions and 81.33% of SVs with ±1bp shift around the SV breakpoint. These results demonstrated that DeBreak can detect all five types of SVs in the simulated datasets with high accuracy.\n\nBenchmark on real human genome\nWe next benchmarked the SV discovery accuracy on a real human genome, HG002, from the Genome in a Bottle (GIAB) Consortium33. We aligned PacBio CLR, HiFi, and Nanopore reads of HG002 to the human reference genome and applied four SV callers, DeBreak, Sniffles, pbsv, and cuteSV, on the three datasets. The GIAB community genome provided an SV callset of 4,237 deletions and 5,440 insertions from multiple platforms in defined “high-confidence” regions34. Thus, we first benchmarked the SV discovery accuracy in these high-confidence regions. In all three datasets, DeBreak achieved the highest SV discovery accuracy among the four tested SV callers, especially for insertions (Table 2). The higher SV discovery accuracy of DeBreak resulted from its advanced clustering algorithm, in which clustering window size is adjustable for SVs of different types, sizes, and local sequence content. Instead of setting a clustering window of fixed size, DeBreak computes the density of raw SV signals and determines the boundaries of the clustering window based on the density pattern. The clustering window is larger for longer SV events and smaller for shorter SV events, which improves effectiveness by merging raw SV signals into SV candidate while excluding noisy signals nearby\n(Fig S4). For SVs located in repetitive regions, the clustering window is automatically adjusted to tolerate shifts of raw SV signals caused by repeated segments (Fig S5).\n\nPrevious work\\(^{35}\\) has highlighted the functional importance of multi-allelic copy number variations (CNVs) in gene dosage and gene expression. DeBreak can accurately identify multi-allelic SVs (mSVs). After density-based clustering, raw SV signals of candidate mSVs are further clustered through a \\(k\\)-means clustering algorithm to characterize two non-reference alleles (Fig S6). We applied this method to identify putative mSVs in HG002. In total, we identified 802 multi-allelic SVs in a single genome.\n\nWe also benchmarked genotyping accuracy of the four tested SV callers with the high-confidence SV callset. On the three datasets, DeBreak and cuteSV performed better than pbsv and Sniffles (Table S1). DeBreak achieved the highest genotyping accuracy in PacBio CLR and Nanopore datasets, while cuteSV achieved slightly higher genotyping accuracy in the PacBio HiFi dataset.\n\nWe then assessed the SV discovery accuracy for SVs of different sizes. DeBreak achieved stable and high accuracy for small and large SVs, especially in detecting insertions (Fig 2a). Notably, for ultra-large insertions longer than the sequencing reads (>10kbp), DeBreak achieved higher accuracy, recall, and precision than the other three SV callers (Fig S7), benefiting from its large-insertion detection module with local de novo assembly. In the PacBio HiFi and Nanopore datasets, DeBreak also achieved relatively high accuracy for SVs of different sizes (Fig S8). We next evaluated the accuracy of SV breakpoint positions reported by DeBreak. The high sequencing error rate of long reads often causes imprecise inference of SV breakpoints. We compared SV callsets from the four tested SV callers to high-confidence benchmark SV callset to assess for shifts in breakpoint positions. With the breakpoint refinement module, DeBreak identified 59.90% of SVs that were consistent with exact SV breakpoints reported in GIAB, higher than pbsv (49.17%), Sniffles (4.99%), and cuteSV (5.18%)\nusing the PacBio CLR dataset (Fig 2b). For PacBio HiFi and Nanopore datasets, DeBreak also achieved the highest SV breakpoint accuracy among the four evaluated SV callers (Fig S9).\n To assess the effect of sequencing depth on SV discovery accuracy, we downsampled the PacBio CLR, HiFi, and Nanopore datasets by a series of depths by randomly sampling the reads. At each depth, DeBreak and pbsv were applied with the default parameters. In contrast, a set of parameters were tested for Sniffles and cuteSV, and the SV calls with the highest F1 scores were selected for comparison. Overall, SV discovery was more accurate for datasets having higher sequencing depth (Fig 2c). Starting from 20x, DeBreak already achieved accuracy of over 90% for PacBio CLR, HiFi, and Nanopore datasets. For datasets with depth \\( \\geq 20x \\), DeBreak consistently identified SVs with the highest accuracy among the four tested SV callers. Note that DeBreak and pbsv automatically adapted to lower depths using default settings, while Sniffles and cuteSV both required extra effort in manually tuning parameters to optimize performance (Fig S10). Taken together, these results highlight that DeBreak can accurately identify different types of SVs with precise breakpoints in real human genomes.\n\nComparison to assembly-based SV discovery\nCurrently, de novo assembly is used to comprehensively characterize genome-wide SVs\\(^{26-29}\\). To compare alignment-based with assembly-based SV discovery approaches, we applied DeBreak, pbsv and cuteSV on six samples from the Human Genome Structural Variation Consortium (HGSVC). Three of these six samples were sequenced with the PacBio CLR platform, and the other three were sequenced with the PacBio HiFi platform. For these samples, highly accurate assembly-based SV callsets were generated by performing haplotype-resolved de novo assembly with phased sequencing reads and subsequent SV discovery from whole-genome assembly with the PAV pipeline\\(^{26}\\). Overall, the assembly-based SV approach discovered a slightly higher number of SV events (22,897 – 27,187) compared with alignment-based methods. By treating these SVs as the “ground truth”, we evaluated the SV discovery\naccuracy of three alignment-based SV callers. DeBreak identified SV with an average F1 score of 80.09% in the six samples, which was higher than pbsv (72.68%) and cuteSV (77.38%) (Table S2). In each sample, DeBreak achieved both higher recall and precision than pbsv and cuteSV (Fig 3a), suggesting higher consistency with the assembly-based SV discovery than the other two alignment-based SV callers. As assembly-based SV calls usually have accurate SV breakpoints inferred from assembled contigs, we also compared the SV breakpoint accuracy of three SV callers. With the breakpoint-refinement module, DeBreak identified 32,813 SVs with exact SV breakpoints on the three PacBio CLR datasets, while pbsv reported 27,345 and cuteSV reported 1,927 precise SV breakpoints, respectively (Fig 3b). For the three PacBio HiFi datasets, DeBreak also achieved better breakpoint accuracy than pbsv and cuteSV, as 41,691, 34,691, and 11,218 SVs were identified with exact SV breakpoints by DeBreak, pbsv, and cuteSV, respectively.\n\nApproximately 82% of DeBreak SV calls overlapped with the assembly-based SV callset. There are several thousand unique SVs were reported either by DeBreak or by the assembly approach. To characterize these SVs, we performed a four-way comparison of SV callsets from DeBreak, pbsv, cuteSV, and PAV on the sample HG00096. For the SVs identified by PAV but not by DeBreak, 27.1% of deletions and 30.5% of insertions were reported by either pbsv or cuteSV (Fig 3c, Fig S11). In contrast, 71.9% of deletions and 71.5% of insertions reported by DeBreak but not PAV were also reported by either pbsv or cuteSV, suggesting that alignment-based SV callers identified SV calls more consistently. We further characterized the 3,385 SVs only reported by PAV and 1,292 SVs only reported by DeBreak in all six samples. Note that DeBreak reported the fewest number of unique SVs. By examining the SV locations on the genome, we found that there was strong enrichment in telomere regions for PAV-unique SVs (43.5% located near telomeres, 5.8% located near centromeres, and 46.4% located in repetitive regions) (Fig 3d, Fig S12). While DeBreak-unique SVs were enriched in the telomere and centromere regions (31.2% located near telomeres, 27.7% located near centromeres, and\n38.7% located in repetitive regions). Although DeBreak controls read depth and minimum number of supporting reads, alignment-based SV discovery may have inaccurate read alignment in these regions. However, it is also challenging to assemble reads with abnormal coverage and ascertain phasing status of individual reads without bias. Additional efforts are needed to validate these SVs.\n\nSV discovery in cancer genomes\n\nSVs play important roles in cancer development and progression^{36-38}. Unlike germline SVs, cancer genomes may contain more large-scale deletions, duplications, inversions, translocations, and other complex SVs^{39-41}. DeBreak includes a “tumor” mode to identify “abnormal” SVs and SVs with clustered breakpoints in cancer genomes. To assess SV discovery in cancer genomes, we applied the four SV callers to identify SVs in a breast cancer cell line, SKBR3. Under the “tumor” mode, DeBreak identified 8,249 deletions, 9,226 insertions, 3,129 duplications, 190 inversions, and 137 translocations. We compared the SV callsets from the four SV callers. As expected, a large proportion of the SVs were identified by all four SV callers (**Fig S13**). Among the four SV callers, DeBreak reported relatively fewer singleton SV calls, especially in insertion/duplication detection, suggesting high precision of DeBreak SV callsets. We also compared the SV callset of DeBreak to previously reported SV lists from long-read and short-read data^{42} (**Fig S14**). DeBreak reported 1,333 deletions, 3,073 insertion/duplications, 51 inversions, and 91 translocations that were not previously discovered. To validate potential cancer-related SVs reported only by DeBreak, we designed primers flanking breakpoints for 15 randomly selected SVs (6 deletions, 4 duplications, 3 inversions, and 2 translocations) that spanned more than 10kbp (**Fig S15**). Polymerase chain reaction (PCR) experiments validated 12 out of 15 DeBreak-novel SVs, with a validation rate of 80% (**Supp file 2**).\nWe further analyzed SVs in the SKBR3 breast cancer cell line by annotating breakpoints and identified 41 putative gene fusions. By cross-validating these gene fusion events with Iso-Seq data (Methods), we found 11 gene fusions that can be validated at the transcripts level (Supp file 3). 6 out of 11 gene fusions have been previously reported using transcriptomic data\\(^{42-45}\\). Therefore, SV discovery using DNA-seq data with DeBreak identified 5 novel gene fusions: WDR82-PBRM1, PDE4D-DEPDC1B, CPNE1-PHF20, CSE1L-KCNB1, and CSNK2A1-NCOA3. The fusion of WDR82 and PBRM1 was caused by a hemizygous deletion of 392kbp on chromosome 3, with the fusion junction located in the intronic region of both genes (**Fig S16**). A deletion of 259kbp on chromosome 20 caused the fusion of CSE1L and KCNB1, where the seventh exon of CSE1L was fused with the intron of KCNB1 (**Fig S17**). The gene fusion junction locations observed in the Iso-Seq reads were highly consistent with SV breakpoint positions inferred by DeBreak, suggesting that DeBreak can accurately predict SV breakpoint positions in cancer genomes. These results indicate that DeBreak can be applied to cancer genomes and identify previously unknown SVs.\n\n**Runtime and memory usage**\n\nDeBreak and other SV callers were tested on Intel Xeon E5-2680 v3 CPUs with 12 cores and 2.5GHz of frequency. It took 12.4 hours for DeBreak to identify SVs from a human genome (SKBR3 cell line) using the 67x PacBio CLR dataset with peak memory of 63 GB (**Table S3**). Due to the local assembly module and partial order alignments, DeBreak consumed more runtime and memory than Sniffles (3.0h, 13GB) and cuteSV (1.5h, 3GB). However, DeBreak was much faster and consumed less memory than pbsv (45.1h, 72GB).\nDiscussion\n\nIn this work we present DeBreak, a method for efficient and accurate structural variation detection from long-read sequencing data. Based on simulation data, real human genome data, and cancer cell line data, DeBreak has demonstrated excellent performance when compared with several state-of-the-art long-read SV callers. The improved performance is due to several innovative design features: 1) the density-based clustering method can accurately identify candidate SV events with a variety of sizes; 2) the partial order alignments can produce a consensus sequence for accurate breakpoint inference, which is helpful for experimental validation and mechanism inference^{20-23}; 3) local de novo assembly facilitates discovery of long insertion events, which usually cannot be inferred within individual reads; 4) \\( k \\)-means approach can accurately identify multi-allelic SVs, which are functionally important; and 5) multiple functions can be applied to both healthy and unhealthy genomes.\n\nAlthough the benchmark was based on human genomes, DeBreak can be applied to other diploid or haploid non-human long-read resequencing data. The overall workflow may be applied to polyploid genomes as well. Based on our knowledge and experience, SV discovery in polyploid genomes is challenging for any currently available tools. More sophisticated benchmarking work is needed.\n\nWe observed that SV callers reporting more accurate breakpoint positions (DeBreak and pbsv) required more computational resource than SV callers with less accurate breakpoints (Sniffles and cuteSV). During SV discovery for DeBreak, breakpoint refinement and ultra-large insertion detection were the two most time-consuming steps, accounting for approximately 45% and 32% of total runtime, respectively. When we disabled these two features, DeBreak accomplished SV detection within 2.8 hours for the same sample, similar to the runtime of Sniffles and cuteSV. The extra runtime and memory usage helped improve the quality and accuracy of the DeBreak SV callset. No matter what situation, DeBreak and other alignment-based methods consume much less computational resources. Although comprehensive\nevaluation and validation between alignment-based and assembly-based approaches are needed, alignment-based methods will continue to serve important roles for SV analysis.\n\nMethods\n\n1. DeBreak workflow\n\n1.1 Overall workflow of DeBreak\n\nDeBreak detects SVs from read-to-reference alignments generated by any long-read aligner, such as minimap2, pbmm2, and ngmlr. The workflow of DeBreak includes 1) raw SV signal detection, 2) large insertion identification, 3) SV signal clustering, 4) SV breakpoint refinement, and 5) SV filtering and genotyping. The output of DeBreak is a standard VCF file containing confident SV calls.\n\n1.2 Raw SV signal detection and clustering\n\nRaw SV signals are detected from read-to-contig alignment. DeBreak scans all read alignments for intra-alignment and inter-alignment SV signals. Smaller indels can be contained within a single alignment. For larger indels, inversions, duplications, and translocations, DeBreak utilizes split-read information and classifies SV type based on orientation and clipping location of two segments from the same read. Once a raw SV signal meets criteria, DeBreak records features of the signal and the read supporting it, including SV type, SV coordinate, SV size, read name, and read mapping quality. As it scans through read alignments, DeBreak also estimates sequencing depth of the input dataset and automatically adjusts parameters used in the following clustering and filtering processes.\n\nRaw SV signals are then clustered into SV candidates with a density-based clustering algorithm. All signals from the same chromosome are sorted based on coordinates. The density of SV raw signals is computed for each position on the chromosome (supp fig). DeBreak scans the chromosome for peaks above a predefined threshold. The boundary of the SV region is\ndefined on both side of the summit when density drops to 10% of the summit or lower than the predefined threshold. All raw signals located within one SV region are then merged into one SV candidate.\n\nFor each SV candidate, DeBreak determines whether it is a multi-allele SV based on the first quartile (Q1) and third quartile (Q3) of SV size from all raw signals. If Q3 is smaller than twice of Q1, all raw signals are merged into a single-allele SV, excluding outliers of extremely large or small size. If Q3 is larger than twice Q1, DeBreak separates raw SV signals for each allele with \\( k \\)-means clustering (\\( k = 2 \\) for diploid genomes) and merges signals from each cluster separately as a multi-allele SV candidate. The detection and clustering of SV signals are processed separately for each chromosome, allowing DeBreak to perform multi-thread SV detection, drastically reducing runtime.\n\n1.3 SV breakpoint refinement\n\nAfter SV signal clustering, DeBreak assigns each SV candidate a breakpoint coordinate by computing the mean value of raw signals. Raw signals can be highly imprecise due to the high error rate of long-read sequencing and the presence of low-complexity regions in the genome. DeBreak implants the POA algorithm from wtdbg2\\(^{46}\\) to refine breakpoint locations. For each SV candidate, DeBreak collects all reads containing this SV candidate and performs POA to generate accurate consensus sequences. DeBreak then aligns these consensus sequences to the reference genome with minimap2 and detects SVs from consensus sequence alignments. The breakpoint location detected from consensus sequence is used to refine the breakpoint coordinates of SV candidates. If POA fails to generate consensus sequences for an SV candidate, or the consensus sequence cannot be properly aligned back to the genome, DeBreak will keep the mean value of the raw signals as breakpoint coordinates.\n1.4 Depth-based filtering and genotyping\n\nDuring raw SV signal detection, DeBreak records the total length of aligned reads on each chromosome and computes the average sequencing depth. The minimum threshold of supporting reads (\\( N_{supp} \\)) is determined based on the average sequencing depth: \\( N_{supp} = \\frac{Depth}{10} + 2 \\). SV candidates supported by at least \\( N_{supp} \\) reads are kept for further consideration, and the rest are discarded to remove background noise. SVs of low mapping quality are also filtered to remove false positives caused by inaccurate read alignment. For multi-allele SVs, DeBreak filters each allele independently. If only one allele passes, a single-allele SV will be reported instead. SVs are genotyped based on the ratio of SV supporting reads to the local sequencing depth at each SV location.\n\n1.5 Large insertion detection via local assembly\n\nDeBreak utilizes a local de novo assembly approach to detect ultra-large insertions that are too long to be spanned within a single read. While scanning read alignments for raw SV signals, DeBreak also records positions of clipped end of read alignments. After scanning through a chromosome, DeBreak identifies candidate insertion breakpoint regions with enriched clipped alignment. It collects all the reads clipped at each candidate breakpoint region and performs local de novo assembly with these reads to reconstruct the inserted sequence. DeBreak aligns assembled contigs to the reference genome with minimap2 and detects insertions from these contigs. Detected insertions are filtered out if 1) multiple contigs are assembled during local de novo assembly, 2) a detected insertion is located in another chromosome or too far away from the candidate insertion breakpoint, or 3) the detected insertion is smaller than 1kbp.\n1.6 Duplication identification\n\nDeBreak includes an optional duplication-rescuing module that distinguishes tandem duplications from insertion calls, as smaller tandem duplications are often treated as insertions by aligners. The inserted sequence of tandem duplication shows high similarity with the duplicated region, while insertions usually consistent of novel sequence or sequences from distinct regions of the genome. For each insertion call, DeBreak collects reads supporting the SV event and extracts inserted sequence from each read. It utilizes minimap2 to re-align these inserted sequences back to the local region (1kbp flanking the insertion breakpoint) on the reference genome. If more than 50% of inserted sequences can be aligned back to the local region, DeBreak corrects the SV type to tandem duplication for this insertion call.\n\n2. Benchmark in simulated dataset\n\n2.1 Simulated dataset generation\n\nThree simulated datasets with ground-truth SVs were generated for benchmarking. For each dataset, a total of 22,200 SVs (10,000 deletions, 10,000 insertions, 1,000 duplications, 1,000 inversions and 200 translocations) were randomly simulated on Chr1 to Chr22 and ChrX. The sizes of simulated SVs followed the geometric distribution as observed in real human genomes, including peaks at ~350bp and ~6000bp. These simulated SVs were assigned as heterozygotes and homozygotes with a ratio of 2:1, and heterozygous SVs were randomly assigned to two haplotypes. The human reference genome GRCh38 (autosomes and the X chromosome) were modified according to the type and size of simulated SVs to generate haplotype 1 and haplotype 2. Long reads were simulated from the modified genome using pbsim with options “--data-type CLR --model_qc model_qc_clr --depth 25 --accuracy-mean 0.85”. The depth was set to 25X for each haplotype, generating a simulated dataset of 50X when merging all reads from both haplotypes. The average read length was set to 10kbp, 15kbp, and 20kbp for three simulated datasets.\n2.2 SV discovery in simulated datasets\n\nThe simulated reads were aligned to the reference genome with minimap2, ngmlr, and pbmm2 under default settings. DeBreak was applied to minimap2 alignment results with default settings. pbsv was run on pbmm2 alignment results with default settings, and Sniffles was run on the ngmlr alignment results with options “--genotype -s 4/5/6/7/8/9/10”. A serious of -s (minimum number of reads supporting an SV) was tested for Sniffles, and the threshold with best accuracy was selected for comparison with other SV callers. cuteSV was run on minimap2 alignment results with options “--genotype”. All SVs with length \\( \\geq 45 \\)bp were selected for benchmark.\n\n The SV callsets of DeBreak, Sniffles, pbsv, and cuteSV were compared to the ground-truth SV set to assess the recall, precision, and F1 score. An SV call (DEL, INS, DUP, and INV) is considered as true positive (TP) if all three conditions are met:\n\n 1) Type_G = Type_C\n 2) ABS(Cor_G – Cor_C ) <= 1kbp\n 3) 0.5 * Size_G <= Size_C <= 2 * Size_G\n\nWhere the Type_G, Type_C, Cor_G, Cor_C, Size_G, and Size_C are the SV type, start coordinates and size of the ground truth SV call and the candidate SV call. For translocations (TRAs), the coordinates of both breakpoints on two chromosomes should be within 1kbp flanking the ground-truth breakpoints to be determined as TP.\n\n3. Benchmark in HG002 dataset\n\n3.1 SV discovery accuracy benchmark\n\nRaw sequencing reads (PacBio CLR, HiFi, and Nanopore data) were downloaded and aligned to GRCh37 with minimap2\\(^{47}\\), ngmlr, and pbmm2 with default settings. DeBreak and cuteSV were applied to minimap2 alignment with default settings. pbsv was applied to pbmm2 alignment with default settings. Sniffles was applied to ngmlr alignment with option “--genotype -\ns 9/9/12” for PacBio CLR, HiFi, and Nanopore dataset, respectively. A series of minimal supporting read (-s option) were tested for Sniffles, and the callset with best performance was used for evaluation. SV callsets of four SV callers were benchmarked within the high-confidence regions (HG002_SVs_Tier1_v0.6.bed) by comparing to the benchmark SV callset using the same criterial as in simulation benchmark. Shift of SV breakpoint was also evaluated with the high-confidence SV benchmark callset. The SV coordinates in DeBreak and cuteSV callsets are 1-based, so all the breakpoint positions were transformed to 0-based to keep consistent with the benchmark callset. Genotyping accuracy of four SV callers was evaluated based on the genotype information in the benchmark callset.\n\n3.2 Down-sampling\n\nTo evaluate SV callers at varying sequencing depths, we downsampled the PacBio CLR dataset of HG002 to a series of depth from 10X to 70X. Sequencing reads were randomly selected to generate datasets with desired depth. The depth of each down-sampled dataset was validated by the total number of bases in reads divided by human genome size (3.1Gbp). Four SV callers were first applied to downsampled datasets with default settings. In addition, to achieve the best performance of Sniffles and cuteSV, a series of min_supp (-s option) was provided to Sniffles and cuteSV at each depth, and the SV callset with the highest accuracy was selected for comparison.\n\n4. Comparison with assembly-based SV callset\n\nRaw PacBio CLR or HiFi reads of sample HG00096, HG01505, HG01596, HG02818, HG03486, and NA12878 were downloaded and aligned to GRCh38 with minimap2 and pbmm2 under default settings. DeBreak, pbsv and cuteSV were applied to the alignment files to identify SVs with default settings. The merged assembly-based SV callset was downloaded from HGSVC2 data portal, and SVs of each sample were extracted with custom script. The comparison of SV\ncalls was performed for autosomes and the X chromosome. SVs located within 5Mbp of both ends of the chromosomes were classified as ‘near telomere’. SVs located within 5Mbp of centromere were classified as ‘near centromere’. Remaining SVs were annotated according to the repeat annotation from Table Browser. SV Distribution on the genome was plotted with karyoploteR48.\n\n5. SV validation in SKBR3 cell line\n\n5.1 PCR validation of novel SVs\n\nPCR validation was performed for SVs identified by DeBreak that were not reported previously by Sniffles and short-read SV callers42. Fifteen putative cancer-related SVs were randomly selected from SVs spanning more than 10kbp on the genome. Insertions were not validated due to length limitations of PCR. PCR primers were designed for each type of SV with Primer3 (v0.4.0)49, and the specificity was verified with UCSC in-silico PCR (Fig S15). An SV event was validated if the PCR and following gel electrophoresis confirmed PCR product of the predicted size.\n\n5.2 Gene fusion annotation and validation with Iso-Seq data\n\nPacBio CLR sequencing data of SKBR3 was aligned to GRCh38 for SV discovery with DeBreak. Breakpoints of deletions, duplications, inversions, and translocations were annotated based on the Ensembl GRCh38 annotation (v104). An SV was considered to cause gene fusion when its two breakpoints were located within two different genes. Iso-Seq reads were downloaded from NCBI and aligned to GRCh38. For each gene fusion event, the total number of Iso-Seq reads aligned to both genes were counted. Gene fusion events supported by at least 3 Iso-Seq reads were considered as validated.\nData availability\n\nPacBio CLR, HiFi, and Nanopore HG002 sequences were downloaded from GIAB at https://github.com/genome-in-a-bottle/giab_data_indexes, where PacBio 70x (CLR), PacBio CCS 15kb_20kb chemistry2 (HiFi), and Oxford Nanopore ultralong were used for SV discovery.\n\nThe Tier1 benchmark SV callset and high-confidence HG002 region were obtained from https://ftp-trace.ncbi.nlm.nih.gov/ReferenceSamples/giab/data/AshkenazimTrio/analysis/NIST_SVs_Integration_v0.6/. Sequencing reads and assembly-based SV callsets of HG00096, HG01505, HG01596, HG02818, HG03486, and NA12878 were downloaded from the HGSVC2 data portal at https://www.internationalgenome.org/data-portal/data-collection/hgsvc2. The PacBio CLR and IsoSeq data of SKBR3 cell line were downloaded from NCBI SRA under BioProject PRJNA476239.\n\nCode availability\n\nDeBreak is publicly available at https://github.com/Maggi-Chen/DeBreak under the MIT License.\n\nWe used v1.0.2 version for SV discovery and benchmark presented in the manuscript.\n\nAcknowledgements\n\nThis work was supported by grant from National Institute of General Medical Sciences (1R35GM138212); the BioData Catalyst Fellowship from National Heart, Lung, and Blood Institute (a subaward from 1OT3HL147154) to Z.C.; and the Center for Clinical and Translational Science grant from the National Center for Advancing Translational Sciences (UL1TR003096) to A.Y.W.\nAuthor contributions\n\nZ.C. conceived and managed the project. Y.C. implemented the algorithm, collected all datasets, and performed primary data analysis. Z.C. and M.G. were involved in data analysis and testing of the algorithm, and Z.C., A.Y.M, and M.G. were involved in interpretation of the results. Y.C., Z.C., and A.Y.W. wrote the manuscript. X.Z., C.A.B, and M.D.E. performed experimental validation. All authors have read and approved the final manuscript.\nReferences\n\n1. Redon, R. et al. Global variation in copy number in the human genome. Nature **444**, 444-454 (2006).\n2. Sudmant, P.H. et al. An integrated map of structural variation in 2,504 human genomes. Nature **526**, 75-81 (2015).\n3. Chaisson, M.J.P. et al. Multi-platform discovery of haplotype-resolved structural variation in human genomes. Nat Commun **10**, 1784 (2019).\n4. Stankiewicz, P. & Lupski, J.R. Structural variation in the human genome and its role in disease. Annu Rev Med **61**, 437-455 (2010).\n5. Weischenfeldt, J., Symmons, O., Spitz, F. & Korbel, J.O. 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Edgren, H. et al. Identification of fusion genes in breast cancer by paired-end RNA-sequencing. Genome Biol **12**, R6 (2011).\n45. Chen, K. et al. BreakTrans: uncovering the genomic architecture of gene fusions. Genome Biol **14**, R87 (2013).\n46. Ruan, J. & Li, H. Fast and accurate long-read assembly with wtdbg2. Nat Methods **17**, 155-158 (2020).\n47. Li, H. Minimap2: pairwise alignment for nucleotide sequences. Bioinformatics **34**, 3094-3100 (2018).\n48. Gel, B. & Serra, E. karyoploteR: an R/Bioconductor package to plot customizable genomes displaying arbitrary data. Bioinformatics **33**, 3088-3090 (2017).\n49. Untergasser, A. et al. Primer3--new capabilities and interfaces. Nucleic Acids Res **40**, e115 (2012).\nFigure 1 Workflow of DeBreak. The major steps of DeBreak SV discovery include SV signal detection, signal clustering, breakpoint refinement, and filtering and genotyping. Detailed descriptions of each step can be found in Methods.\nTable 1 SV discovery accuracy on simulated datasets\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
TypeDeBreakSnifflespbsvcuteSV
RecPreF1RecPreF1RecPreF1RecPreF1
DEL99.5999.5099.5495.5099.8397.6297.2199.5898.3896.9499.8298.36
INS98.5199.6599.0892.3599.5295.8095.3896.2295.8094.5894.7194.64
DUP98.2797.0497.6590.8098.6394.5544.5397.1160.9744.1399.0361.05
INV99.1099.4099.2594.5797.2295.8882.6799.9290.4796.5350.0065.88
TRA99.1799.6799.4197.6795.6096.6297.6725.0439.8699.0050.3066.70
Total99.0299.4599.2393.8599.4796.5893.3695.3494.3493.5092.3992.94
\n\nThe unit for recall, precision, and F1 score is %. The highest recall, precision, and F1 score among four tested SV callers are marked in bold.\nRec = Recall. Pre = Precision. F1 = F1 score.\nTable 2 SV discovery accuracy on HG002\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
DeBreakSnifflespbsvcuteSV
RecPreF1RecPreF1RecPreF1RecPreF1
Deletion
CLR97.7396.4897.1095.1496.6995.9195.2896.2195.7497.3194.1895.72
HiFi98.1695.1196.6197.4591.6794.4796.7494.8895.8097.7193.3395.47
Nano98.4095.0796.7196.2994.6295.4597.4081.0888.5098.1889.2793.51
Insertion
CLR97.1593.3695.2288.3889.5888.9893.2283.4388.0595.4081.6788.00
HiFi97.2692.8495.0090.9087.7989.3297.4180.4288.1096.6489.8893.14
Nano97.4693.9195.6590.5790.0190.2995.0785.6090.0996.9989.2792.97
\n\nThe unit for recall, precision, and F1 score is %. The highest recall, precision, and F1 score among four tested SV callers are marked in bold.\nRec = Recall. Pre = Precision. F1 = F1 score.\nFigure 2 SV discovery in HG002. a SV discovery accuracy for insertions (positive SV size) and deletions (negative SV size) at different size ranges. Bars indicates the number of SVs in each size range, and lines show the SV discovery accuracy for each SV caller. b SV breakpoint accuracy for four tested SV callers. SVs with breakpoint shifting >100bp were included in the ±100bp bins. c SV discovery accuracy in downsampled PacBio CLR (left), HiFi (middle), and Nanopore (right) datasets for HG002.\nFigure 3 Alignment-based and assembly-based SV discovery. a SV discovery recall and precision of alignment-based SV callers when compared with the assembly-based SV callset. b SV breakpoint accuracy of DeBreak, pbsv, and cuteSV in PacBio CLR (top) and HiFi (bottom) datasets. c Venn diagram showing the overlap among the four SV callsets. The number of SV events in each category is labeled within each section. d Distribution of PAV-unique and DeBreak-unique SV calls on chromosomes 1-5. Red boxes indicate positions of centromeres.\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• SupplementaryFigure.pdf\n• SupplementaryFile2.xlsx\n• SupplementaryFile3.xlsx"} {"paper_id": "prb73", "title": "Sequence variants affect the genome-wide rate of germline microsatellite mutations", "text": "Sequence variants affect the genome-wide rate of germline microsatellite mutations\n\nSnaedis Kristmundsdottir\ndeCODE genetics/Amgen Inc.\n\nHákon Jónsson\ndeCODE genetics/Amgen, Inc., Reykjavik, Iceland https://orcid.org/0000-0001-6197-494X\n\nMarteinn Hardarson\ndeCODE genetics/Amgen Inc. https://orcid.org/0000-0003-1130-8601\n\nGunnar Pálsson\ndeCODE genetics / Amgen Inc. https://orcid.org/0000-0002-8231-3961\n\nDoruk Beyter\ndeCODE genetics / Amgen Inc.\n\nHannes Eggertsson\ndeCODE Genetics (Iceland) https://orcid.org/0000-0002-1674-9978\n\nArnaldur Gylfason\ndeCODE Genetics\n\nGarðar Sveinbjornsson\ndeCODE Genetics/Amgen Inc.\n\nGuillaume Holley\ndeCODE genetics/Amgen, Inc.\n\nOlafur Stefansson\ndeCODE genetics/Amgen, Inc.\n\nSigurgeir Olafsson\ndeCODE genetics https://orcid.org/0000-0003-1711-2757\n\nGudny Amadottir\ndeCODE genetics/Amgen Inc. https://orcid.org/0000-0001-6571-423X\n\nPall Olason\ndeCODE Genetics (Iceland)\n\nOgmundur Eiriksson\nhttps://orcid.org/0000-0003-0139-5107\n\nGisli Masson\ndeCODE genetics / Amgen Inc.\n\nUnnur Thorsteinsdottir\ndeCODE genetics / Amgen Inc.\n\nThorunn Rafnar\ndeCODE genetics https://orcid.org/0000-0003-0491-7046\n\nPatrick Sulem\ndeCODE Genetics (Iceland) https://orcid.org/0000-0001-7123-6123\n\nAgnar Helgason\ndeCODE Genetics\n\nDaniel Gudbjartsson\ndeCODE Genetics (Iceland) https://orcid.org/0000-0002-5222-9857\n\nBjarni Halldorsson (✉ Bjami.Halldorsson@decode.is)\ndeCODE genetics/Amgen Inc. https://orcid.org/0000-0003-0756-0767\n\nKari Stefansson\ndeCODE genetics https://orcid.org/0000-0003-1676-864X\n\nArticle\n\nKeywords:\n\nPosted Date: June 29th, 2022\n\nDOI: https://doi.org/10.21203/rs.3.rs-1716464/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\nSequence variants affect the genome-wide rate of germline microsatellite mutations\n\nAuthors: Snaedis Kristmundsdottir1,2, Hakon Jonsson1, Marteinn T. Hardarson1,2, Gunnar Palsson1, Doruk Beyter1, Hannes P. Eggertsson1, Arnaldur Gylfason1, Gardar Sveinbjornsson1, Guillaume Holley1, Olafur A. Stefansson1, Sigurgeir Olafsson1, Gudny. A. Arnadottir1,4, Pall I. Olason1, Ogmundur Eiriksson1, Gisli Masson1, Unnur Thorsteinsdottir1,4, Thorunn Rafnar1, Patrick Sulem1, Agnar Helgason1,5, Daniel F. Gudbjartsson1,3, Bjarni V. Halldorsson1,2*, Kari Stefansson1*\n\nAffiliations:\n\n1 deCODE genetics / Amgen Inc., Sturlugata 8, Reykjavik, Iceland\n\n2 School of Technology, Reykjavik University, Reykjavik, Iceland\n\n3 School of Engineering and Natural Sciences, University of Iceland, Reykjavik, Iceland\n\n4 Faculty of Medicine, School of Health Sciences, University of Iceland, Reykjavik, Iceland\n\n5 Department of Anthropology, University of Iceland, Reykjavik, Iceland\nAbstract\n\nMicrosatellites are polymorphic tracts of short tandem repeats (STRs) with one to six base-pair (bp) motifs and are some of the most polymorphic markers in the genome. Using 6,084 Icelandic parent-offspring trios we estimate 63.7 (95% CI: 61.9-65.4) microsatellite de novo mutations (mDNMs) per offspring per generation. Paternal mDNMs occur at longer repeats, while maternal mDNMs affect more bp. mDNMs increase by 0.97 (95% CI: 0.90–1.04) and 0.31 (95% CI: 0.25-0.37) per year of father’s and mother’s age at conception, respectively. We found two independent coding variants associated with an increased number of mDNMs transmitted to offspring; A missense variant (allele frequency (AF) = 1.9%) in MSH2, a mismatch repair gene, increases transmitted mDNMs from both parents (effect: 13.1 paternal and 7.8 maternal mDNMs). A synonymous variant (AF = 20.3%) in NEIL2, a DNA damage repair gene, increases paternally transmitted mDNMs (effect: 4.4 mDNMs). Thus, the microsatellite mutation rate in humans is in part under genetic control.\n\nIntroduction\n\nMutations enable life to evolve and adapt. Accurate estimates of the rate of mutations and the processes behind them are therefore imperative for understanding evolution, making inferences about population history\\( ^{1-6} \\) and understanding the genetics of disease and other phenotypes\\( ^{7-11} \\).\n\nAround 3% of the human genome are short tandem repeats (STRs)\\(^{12}\\), some of which are polymorphic, i.e. microsatellites, and mutate several orders of magnitude faster than non-repetitive sequences\\(^{13}\\). The forces that shape age related mDNM accumulation in the two sexes and the effects of parental genotypes on accumulation is largely unknown.\n\nGenetic factors responsible for genome integrity can be expected to play a role in DNM accumulation. Sequence variants that increase single nucleotide polymorphism (sDNM) and mDNM rates are known in somatic tissues in humans \\(^{14}\\) and sequence variants that increase the sDNM rate are known in animal and yeast models\\( ^{15,16} \\). Apart from a handful of clinical cases\\( ^{17,18} \\),\nno human germline mutators are known that affect the de novo mutation rate of microsatellites or other types of variants.\n\nMost mDNMs are believed to occur as a result of failure in the processes responsible for sequence fidelity during DNA replication. These processes verify the correct pairing of bp and replace incorrectly paired or damaged DNA bases\\(^{19,20}\\). Loss of function mutations affecting genes responsible for sequence fidelity are known to cause somatic microsatellite instability, which in turn can result in increased risk of colorectal, gastric, endometrial and other types of cancer\\(^{21}\\).\n\nRecombination, DNA damage repair and nonhomologous end joining (NHEJ) have also been implicated as determinants of mDNMs\\(^{22,23}\\) and since the two germlines have different exposure to these processes it is logical to assume that the mDNM accumulation is different between the sexes. Spermatogonia undergo mitosis continuously, increasing the risk of replication errors while the recombination rate is higher in females\\(^{24}\\) and oocytes wait in dictyate arrest from the mother’s birth to reproduction, exposed to DNA damage to be repaired by NHEJ or homologous recombination\\(^{25}\\). The rate of mDNMs in humans has been shown to vary by a number of microsatellite properties \\(^{26-28}\\), parent of origin, and paternal\\(^{29}\\) age, but researchers have to date been unable to detect a relationship with maternal age.\n\nPrevious studies of mDNMs have largely been confined to small sets of well-characterized microsatellites or focused on specific diseases \\(^{1,29}\\). Here, we identified and genotyped microsatellites in two large sequencing cohorts with the aim of estimating polymorphism and mDNM rate and identifying environmental and genetic determinants of mDNMs.\n\nResults\n\nSTR identification and genotyping\n\nWe used popSTR\\(^{30}\\) to call genotypes at 5,401,401 autosomal short tandem repeats (STRs) in two large WGS datasets, 53,026 Icelanders and 150,119 participants in the UKB, sequenced to\nan average coverage of 39.2x (min: 19.7, max: 608.3) and 32.5x (min: 23.6, max: 128.1), respectively.\n\nThe STRs were identified by Tandem repeats finder\\(^{31,32}\\). Each STR has a repeat motif along with start and end positions in the reference and we refer to the sequence between these positions as the reference repeat tract (RRT) and its length as RRT length. For motif lengths between one and three bp, we compared the behavior of motif equivalence classes where all members in a class are either a circular shift or a reverse complement of each other. For example, the members of the AAT motif equivalence class are: AAT, ATA, TAA, ATT, TAT and TTA (Table S1).\n\nWe found 1,394,292 (25.8%) and 2,393,292 (44.3%) of the STRs to be polymorphic in the Icelandic and UK datasets, respectively and will refer to these polymorphic STRs as microsatellites. We describe microsatellite diversity through polymorphism rate (the fraction of STRs that are polymorphic) and expected heterozygosity\\(^{32,33}\\) (Fig. S1, Fig. S2, Table S18, Table S19, Table S20, Table S21). In both the Icelandic and UKB datasets, polymorphism rate and expected heterozygosity were correlated with the number of bp in the motif (motif length), RRT length, fraction of G/C bases in the STR’s motif (motif GC content), and repeat purity\\(^{32}\\) (Supplementary note 1). Our microsatellite genotyping is limited by read length (151 bp for most samples), resulting in a decrease in accuracy when detecting and determining genotypes of alleles with long RRTs. While the RRT length limit for inclusion in our study is 140bp, the average expected heterozygosity in our datasets decreases at RRT lengths exceeding 80 bp (Fig. S1, Fig. S2), so we conclude that this is the length where the effect of the RRT length on the genotyping accuracy becomes pronounced.\n\nmDNM rate\n\nWe detected 76,987 mDNMs in 6,084 Icelandic trios (mean: 12.7 mDNMs per trio) in 634,406 high quality microsatellites, where the genotypes of the offspring were inconsistent with those of the parents\\(^{32}\\). The trios yielded on average 256,066 microsatellites (40.4%) where all three genotypes passed quality filters and we were able to test for mDNMs.\nWe estimated the false positive rate of our method between 2.0-5.6% using three approaches; PacBio CCS sequence data, mDNM sharing between monozygotic twins and haplotype sharing across three-generation families (Supplementary note 2).\n\nWe estimated the average mDNM rate across all motif lengths as \\(4.95 \\cdot 10^{-5}\\) mutations per microsatellite per generation (MMG), consistent with previous results (Supplementary note 5). We observed an order of magnitude difference in mDNM rates between motif lengths, ranging from \\(1.04 \\cdot 10^5\\) MMG for hexanucleotide repeats to \\(1.07 \\cdot 10^4\\) MMG for dinucleotide repeats (Table 1, Fig. 2)\\(^{32}\\). Using motif length specific mutation rates and the average number of markers available for each trio to extrapolate to the full set of 1,394,292 microsatellites gives an expected number of 63.7 mDNMs (95% CI: 61.9-65.4) per offspring per generation\\(^{32}\\). This extrapolated number is comparable with the de novo mutational load of SNPs and indels detected through short read sequencing\\(^{34,35}\\).\n\nWe find that mDNMs are depleted within functionally annotated and early replicating regions\\(^{32}\\). We also find that exon intersecting microsatellites contain more interruptions than intergenic ones (Supplementary note 4). Since longer uninterrupted repeats associate with higher mDNM rates\\(^{27}\\), this suggests that variants interrupting the repeat structure are positively selected in exons as a way to reduce the occurrence of high impact mDNMs.\n\nWe further replicate known mutation rate behaviors such as expansion biases at shorter RRTs and contraction biases at longer RRTs (Supplementary note 3).\n\nParent of origin effects\n\nTo determine the differences between the sexes in mDNM formation, we assigned a parent of origin to 46,171 (60.0%) of the mDNMs using a combination of three methods; read pair tracing, allele sharing and haplotype sharing in three-generation families\\(^{32}\\). The concordance was above 93% between all three methods (Table S11, Table S12, Table S13). We found mDNMs from fathers (N=35,501, 76.9%) to be 3.3 (95% CI: 3.2-3.4, chi squared test \\(P < 1 \\cdot 10^{-320}\\)) times more common than from mothers (N=10,670, 23.1%) (Table S29).\n\nMaternal and paternal mDNMs occurred with different probabilities at different RRT lengths, motif lengths, and motif equivalence classes. First, a larger fraction of maternal mDNMs\noccurred at homopolymers, tri-, penta-, and hexanucleotide microsatellites, whereas a larger fraction of paternal mDNMs occurred at di- and tetranucleotide microsatellites (Table S25, Fig. 3, Supplementary note 7). Second, the average number of bp affected by each mDNM was greater from mothers (3.4 bp, 95% CI: 3.3-3.4) than fathers (3.1 bp, 95% CI: 3.1-3.1) (Mann-Whitney U test \\( P = 5.0 \\cdot 10^{-8} \\), Table 3), consistent with previous results\\(^{29}\\). Stratifying by motif length revealed that maternal mDNMs affected more bp than paternal mDNMs on average at homopolymer, di- and tetranucleotide microsatellites (Table S7). Paternal mDNMs occurred at microsatellites with greater RRT lengths. Stratifying by motif length, we observed significant RRT length differences between the sexes at di-, tetra-, penta- and hexanucleotide microsatellites (Table S8).\n\nIt seems likely that the sex differences in the accumulation of mDNMs transmitted to offspring are due to differences in the exposure to mutagens of the germlines leading to oocytes and spermatogonia. For di- and trinucleotide microsatellites, the relative frequency of maternal and paternal mDNMs differed between the motif classes (Table S9). An enrichment of CCG motifs in maternal mDNMs may be the result of the vulnerability of GC rich sequences to alkylation\\(^{36}\\) or oxidative damage\\(^{37}\\) and the long time oocytes spend in dictyate arrest before meiosis. Building on this, we considered all non-trinucleotide mDNMs in microsatellites whose motif contained only G or C and found a 2.3 (95% CI: 1.7-3.7) fold enrichment of maternal mDNMs indicating that purely GC repeats are more prone to mutate in maternal than paternal germlines. Because of a known trend towards paternal expansion at an ATTCT repeat associated with spinocerebellar ataxia 10 (\\( SCA10 \\))\\(^{38,39}\\), we examined motifs from this class specifically to determine if the bias observed at \\( SCA10 \\) could be observed genome-wide (Table S9). The maternal contribution at pentanucleotide mDNMs was 25.9% overall, but for the ATTCT motif equivalence class, the ratio was only 18.9% (chi squared test \\( P = 0.037 \\)). On average, we see an addition of 0.3 bp in paternal mDNMs at microsatellites with ATTCT motifs, compared to a loss of 3.2 bp in maternal mDNMs (Mann-Whitney U test \\( P = 5.0 \\cdot 10^{-4} \\)). This suggests that the paternal expansion bias observed at the \\( SCA10 \\) microsatellite also affects other ATTCT microsatellites in the genome.\n\nParental age influences number of mDNMs\nThe number of mDNMs transmitted to the offspring was affected by both paternal (\\( P = 5.4 \\cdot 10^{-176} \\)) and maternal (\\( P = 7.2 \\cdot 10^{-24} \\)) age at conception\\(^{32}\\). The increase was 0.97 mDNMs per year in fathers (95% CI: 0.90-1.04) and 0.31 mDNMs per year in mothers (95% CI: 0.25-0.37), resulting in an expected number of 51.2 (35.7 paternal and 15.5 maternal) mDNMs and 77.0 (55.1 paternal and 21.8 maternal) mDNMs extrapolated genome-wide in offspring with 20- and 40-year-old parents, respectively. An increase of mDNMs with paternal age is consistent with previous studies\\(^{29}\\), but, to our knowledge, this is the first demonstration that mDNMs are also affected by maternal age.\n\nmDNMs at mono-, di-, tri- and tetranucleotide microsatellites increased significantly with paternal age and mDNMs at di-, tetra- and hexanucleotide repeats increase with maternal age (Table 2). An age effect is likely for all motif lengths in both sexes but we lack power to detect it in less frequent motif lengths.\n\nWhen we consider the fraction of mDNMs of each motif length that each individual carries we see a clear difference in the mutagens acting on the two sexes (Supplementary note 8). The fraction of dinucleotide paternal mDNMs decreased with paternal age, while the fraction of tetranucleotide mDNMs increased with paternal age (Fig. 3). The fraction of hexanucleotide maternal mDNMs increased with maternal age (Fig. 3). The heterogeneity between the sexes in motif length fractions that change with age indicates that, for each sex, the processes behind age related mDNM accumulation are more likely to mutate microsatellites at different motif lengths.\n\n**Parental genotypes associate with number of mDNMs in offspring**\n\nTo determine whether there are variants in the genome that affect the number of mDNMs transmitted by parents to their offspring, we performed a genome-wide association study (GWAS) using the number of mDNMs originating from each parent as a phenotype, adjusting for age, sex, sequencing method and sample type\\(^{32}\\).\n\nThree correlated SNPs rs4987188, rs112587140 and rs113983130 (Table S5) were associated with an increase in mDNMs for all motif lengths. We selected \\(^{40}\\) rs4987188[A], a missense\nvariant (p.Gly322Asp, AF=1.9%) in the *MSH2* gene, a mismatch repair gene\\(^{41,42}\\), as the lead marker for the association (Fig. 4, Table S6).\n\nEach copy of rs4987188[A] is associated (\\(P = 3.6 \\cdot 10^{-10}\\)) with a 0.37 s.d. (95% CI: 0.26-0.48) increase in the number of transmitted mDNMs, corresponding to 13.1 and 7.8 mDNMs genome-wide per paternal and maternal copy, respectively. No significant difference in effect was found in the increase between the two parental sexes (\\(P = 0.14\\)). However, we see a nominal association (\\(P = 0.019\\)) between paternal age and mutation count in offspring of male carriers, suggesting an increase in the effect of rs4987188[A] with paternal age.\n\nThe protein encoded by *MSH2* forms two heterodimeric mismatch repair complexes. One predominantly required for repairing mismatched bp and the other mainly responsible for repairing insertion/deletion loops between one and twelve bp\\(^{43,44}\\). Multiple variants in *MSH2* have been reported to cause Lynch syndrome (also known as hereditary non-polyposis colorectal cancer, HNPCC), which results in increased risk of endometrial, colorectal and other cancers\\(^{45}\\). We tested rs4987188[A] for association with an increased risk of endometrial and colorectal cancer in both the Icelandic and combined meta-analysis data sets available at deCODE genetics, but found no such association. Functional studies of the yeast homologue of rs4987188 indicate that it results in a modest decrease in mismatch repair efficiency\\(^{46,47}\\).\n\nHomopolymer mDNMs have a higher false positive rate than other mDNM categories. To assess the robustness of our results, we reran the GWAS on mDNM counts per parent without mDNMs occurring at homopolymers. The *MSH2* association was retained with a similar effect of 0.39 s.d. (\\(P = 1.3 \\cdot 10^{-10}\\)). Furthermore, we find a novel association between mDNM counts without homopolymers and two correlated (\\(r^2\\)=0.988) SNPs, rs8191642 (\\(P =5.6 \\cdot 10^{-10}\\)) a synonymous variant (Pro188), and rs8191649 (1.4 \\(\\cdot\\) 10\\(^{-9}\\)), an intronic variant, both in *NEIL2*, a glycolase involved in both transcription and replication associated base excision repair of DNA damaged by oxidation or by mutagenic agents\\(^{48}\\). We selected \\(^{40}\\) rs8191642[G] (AF = 20.3%), as the lead marker for the association.\nTesting rs8191642[G] for mothers and fathers separately revealed heterogeneity in effect between the sexes (\\(P = 1.2 \\cdot 10^{-3}\\)). Each copy of rs8191642[G] is associated with (\\(P = 7.2 \\cdot 10^{-12}\\))\na 0.21 s.d. (95% CI: 0.15-0.27) increase in the number of paternally transmitted mDNMs with motif lengths greater than one bp, corresponding to 4.4 mDNMs genome-wide per copy, but associated with a modest increase in the number of maternally transmitted mDNMs (\\( P = 0.015 \\), effect=0.072 s.d.).\n\nTo assess the effect of these microsatellite mutator alleles on other types of genetic variation, we compared sDNMs transmitted from carrier and non-carrier mothers and fathers. The results of these comparisons suggest that the effects of rs4987188[A] and rs8191642[G] are confined to microsatellite and they do not otherwise affect the fidelity of the mismatch or base-excision repair pathways (Supplementary note 9).\n\n**Discussion**\n\nWe generated two large microsatellite genotype sets. The microsatellite genotypes for the UKB samples are publicly available and have been tested for association with various phenotypes\\(^{49}\\).\n\nIn the Icelandic set, we identified 76,987 mDNMs and found an association between the number of mDNMs transmitted to offspring and the age of both mothers and fathers at conception and parental genotypes. We observed a previously unreported increase in the number of maternal mDNMs transmitted to offspring with maternal age, consistent with the increase of both SNP/indel DNMs\\(^{34}\\) and recombination with maternal age\\(^{24,50}\\). mDNMs are often associated with replication adducts\\(^{26,27,51–54}\\), however the maternal effect gives novel insight into the formation of mDNMs, as oocytes are in dictyate arrest compared to the actively dividing spermatogonia in aging fathers. The maternal age effect indicates that, mDNMs can also occur outside of DNA synthesis during S-phase replication, presumably since DNA polymerases operate during most types of DNA repair on long tracts and in homologous recombination pathways\\(^{26}\\).\n\nThe observation of different frequencies of mDNM motif classes transmitted by older mothers and fathers allows us to shed light on the mutational processes acting in the germlines. Since spermatogonia undergo a greater number of mitotic cell divisions than oocytes, we propose that the paternal enrichment of AC motif class mDNMs is due to out-of-register realignments\nduring replication \\(^{53}\\), whereas the maternal enrichment of mDNMs at pure GC repeats is likely to be a result of damage accumulated during the dictyate arrest of oocytes.\n\nSequence variants detected in humans that decrease sequence stability have for the most part been very deleterious and under strong negative selection\\(^{55}\\). Interestingly, the microsatellite mutators at *MSH2* and *NEIL2* identified here are both present in high frequencies and have large effects, thereby indicating that a genome-wide increase in the mDNM rate is not sufficiently deleterious to result in strong selection against these variants. The similar effect of the missense variant in *MSH2* across the sexes, indicates that gametes from both sexes are subject to the same sequence fidelity maintenance process. *NEIL2* has been reported to function in both transcription and replication coupled repair\\(^{48}\\) and thus, it is likely that the association between the synonymous variant in *NEIL2* and the number of paternally transmitted mDNMs is due to the more frequent replication of spermatogonia.\n\nWe have identified the first germline variants, segregating at high frequencies, that directly affect the mDNM rate in humans. 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Distribution and abundance of microsatellites in the yeast genome can be explained by a balance between slippage events and point mutations. Mol. Biol. Evol. **17**, (2000).\n\n86. Khristich, A. N. & Mirkin, S. M. On the wrong DNA track: Molecular mechanisms of repeat-mediated genome instability. Journal of Biological Chemistry **295**, (2020).\n\n87. Alexandrov, L. B. et al. The repertoire of mutational signatures in human cancer. Nature **578**, (2020).\nMethods\n\nIdentification of tandem repeats\n\nTo generate a set of STR locations we ran version 4.09 of Tandem repeats finder31 on the GRCh3856 human reference genome with the following parameters:\n./trf409.linux64 genome.fa 2 7 7 80 10 22 100 –d –h –ngs > trf_out_100\n\nPurity computation\n\nWe define the ratio between the observed repeat units in a STR and the number of expected repeat units in a perfectly pure STR as the repeat purity.\n\n\\[\npurity = \\frac{observed\\ repeats}{E[repeats\\ |\\ 100\\% \\ pure]}\n\\]\n\nExpected heterozygosity computation\n\nWe compute expected heterozygosity using the following formula33\n\n\\[\ngene\\ diversity = \\left[ \\frac{n}{(n-1)} \\right] \\left( 1 - \\sum_{i=1}^{k} p_i^2 \\right)\n\\]\n\nwhere \\( n \\) is the total number of sequences, \\( k \\) is the number of alleles at the marker and \\( p_i \\) is the frequency of each allele.\n\nGenotype and marker filtering\n\nFor a trio comparison we require all members of the trio to have a phred scaled genotype quality value higher than 60. We removed microsatellites which imputed to a 0% frequency and ones that failed our best practices filters. These filters consider coverage, genotype quality, number of samples genotyped and fraction of reads not supporting the reported genotype and are described in49.\n\nWe further removed microsatellites outside the Tier 1 regions defined by GIAB57 and microsatellites lying within CNV regions annotated by CNVnator58.\n\nAfter using long range phased SNP genotypes to phase and impute our microsatellite genotypes into the Icelandic population59, microsatellites with alleles showing a strong deviation from the Hardy Weinberg equilibrium (\\( P < 1 \\cdot 10^{-6} \\)) or a frequency weighted imputation information lower than 0.9 were removed60. We also required the frequency weighted phasing information to be greater than 0.6 and the r^2 for leave one out cross validation of phased genotypes to be greater than 0.5.\n\nWe looked for offspring with homozygous mDNMs less than 1Mbp apart, implying a haploid state, and checked them for large CNVs covering the region, causing autozygosity and spurious\nmDNM calls. Last, we crossed all mDNMs with deletions and duplications imputed into the offspring\\(^{61}\\) and removed the ones intersecting.\n\n**De novo detection**\n\nFor marker-trio combinations where all conditions described above are met, we define a mDNM as a trio genotype combination satisfying neither of the following logical statements:\n\n (1) \\( proband_{A1} \\in M \\) and \\( proband_{A2} \\in F \\)\n (2) \\( proband_{A1} \\in F \\) and \\( proband_{A2} \\in M \\)\n\nwhere \\( proband_{A1} \\) and \\( proband_{A2} \\) refer to the two alleles carried by the offspring and \\( M \\) and \\( F \\) define the allele pairs carried by the mother and father, respectively.\n\n**Microsatellite attribute regression on mDNM rate**\n\nWe performed a Poisson regression using the number of available markers per trio as an offset on the full data set and stratified by motif length to examine if the effects of other attributes on the mDNM rate remained consistent across motif lengths.\n\nThe direction and statistical significance for both RRT length and repeat purity remain consistent for all motif lengths but the effect of GC content in repeat motif is positive for homopolymer repeats (Table S2).\n\n**Obtaining confidence intervals for mDNM rate estimates**\n\nWe used the boot package for R\\(^{62,63}\\) to obtain confidence intervals for both our genome wide mDNM rate estimate and the motif length specific estimates. 100 replicates were used in all cases and 95% confidence intervals extracted using the resulting quantiles.\n\n**Extrapolation from mDNM rate to expected number of mDNMs**\n\nThe per motif mDNM rate was determined from our set of high-quality microsatellite calls. We estimated the expected number of per motif mDNMs among all microsatellites by multiplying the mDNM rate and the number of microsatellites per motif length. The total expected mDNMs is the sum over all motif lengths\n\n\\[\nE[mDNMs] = \\sum_{i=1}^{6} r_i \\cdot n_i\n\\]\n\nwhere \\( r_i \\) is the mDNM rate at motif length \\( i \\) and \\( n_i \\) is the genome-wide number of microsatellites with motif length \\( i \\).\n\n**mDNM overrepresentation analysis**\n\nWe counted mDNMs within and outside of regions with various annotations and computed overrepresentation (OR) for each annotation type using the following equation\nOR = \\frac{mDNMs_a/bp_a}{mDNMs_{out}/bp_{out}}\n\nWhere \\( mDNMs_a \\) enumerates the number of mDNMs within the annotated regions, \\( bp_a \\) represents the total size of the annotated region in bp, \\( mDNMs_{out} \\) enumerates the number of mDNMs outside of the annotated region and \\( bp_{out} \\) represents the number of bp outside the annotated region.\n\nMicrosatellite mDNM phasing\n\nWe determined the parent of origin of mDNMs, using three distinct methods; read pair tracing, allele sharing and haplotype sharing in three-generation families.\n\nFirst, we used long range phased\\(^{59}\\) SNP and indel genotypes available at deCODE genetics\\(^{59}\\) to phase reads reporting mDNMs when possible. Read phases enabled us to assign a parent of origin to mDNMs according to the phase of the reads reporting the event since a read phased to one parent and reporting a mDNM indicates that the mDNM was transmitted from that parent. Not all mDNMs had supporting reads containing phased markers and for these, assigning a parent of origin was not possible (Fig. S5).\n\nSecond, for trios where the de novo allele was seen in neither parent and the other offspring allele was only seen in one parent we phased the mDNM to the other parent (Fig. S6).\n\nLast, we used haplotype sharing in three generation families such that if the mDNM was transmitted from offspring to their children, we phased the de novo to the parent sharing a haplotype with its grandchild, and to the parent not sharing a haplotype if de novo was not transmitted (Fig. S7).\n\nParental age effect regression\n\nWe applied a Poisson regression model described in\\(^{34}\\) on our data with the number of available markers in each trio as a covariate to determine the effect of parental age at conception on the number of mDNMs transmitted to the offspring.\n\nTo determine whether the coefficients were robust to the phasing method, we repeated the analysis\\(^{34}\\) and split the phased markers by phasing method and performed the regression on each subset. Both maternal and paternal age remained significant in all subsets (Table S28).\n\nWe compute the total predicted number of de novo mutations in a offspring with an \\( X \\) year old father and a \\( Y \\) year old mother from the coefficients from our regression model:\n\n\\[\n(I_F + \\beta_F \\cdot X + I_M + \\beta_M \\cdot Y)/(\\mu_{markers}^{1,394,292})\n\\]\n\nWhere \\( I_F \\) is the paternal intercept, \\( \\beta_F \\) is the paternal age effect, \\( I_M \\) is the maternal intercept, \\( \\beta_M \\) is the maternal age effect, \\( \\mu_{markers} \\) is the mean value of available markers across our trios and 1,394,292 is the total number of microsatellites we detect.\n\nConstruction of mDNM phenotypes\nWe used maternal and paternal counts at each offspring to construct phenotypes for the parents quantifying the number of mDNMs passed on to the offspring. In addition to correcting for the parental gender (mother/father), we corrected for parental age at birth of offspring, sequencing method, sample type and number of microsatellites available for de novo detection in the trio. For parents with more than one offspring in our trio set, we used the average of all their offspring. After regressing out the coefficients, we used rank inverse normalization to normalize the phenotype.\nFig. 1 | Overview of the analysis. We use WGS data from Iceland and UKB and genealogy data from Iceland. From the WGS data we generate microsatellite genotypes. Using trios in the genealogy and the genotypes we detect and phase mDNMs and count the number of mDNMs per trio. We associate the individual mDNM counts with genotypes of the parents in the trios. We compute population wide expected heterozygosity based on the genotypes and observe how it is affected by sequence context. From the phased mDNMs we also estimate age and sex effects on the mDNM rate and to create parental phenotypes based on number of mDNMs found in offspring from the phased mDNMs.\nFig. 2|mDNM rate a) Histogram showing the number of mDNMs per microsatellite. Only microsatellites with at least one mDNM are shown and the counts are on a log-scale. b) Histogram showing the number of trios available to check for mDNMs per microsatellite with at least one mDNM. c) mDNM rates of motif equivalence classes for motif lengths between one and three bp with error bars representing 95% confidence intervals. d) mDNM rate as function of RRT length stratified on motif length. The RRT length affects mDNM rates in a similar way for all motif lengths. e) mDNM rate as function of GC content in motif. f) mDNM rate as a function of repeat purity stratified on motif length. The mDNM rate increases with purity for all motif lengths.\nFig. 3 | Sex differences and age effects a) Relative frequencies of paternal and maternal mDNMs at different motif lengths. b) Relative frequencies of paternal and maternal mDNMs at different motif lengths without homopolymer mDNMs. c) Fraction of di- and tetranucleotide paternal mDNMs as a function of paternal age. The tetranucleotide fraction increases while the dinucleotide fraction decreases. d) The fraction of hexanucleotide maternal mDNMs increases with maternal age. e) Paternal and maternal age effect regression lines within our mDNM set. The age effect reported is interpolated to a genome-wide value using the fraction between average number of available microsatellites and total number of microsatellites. Fractions in c) and d) are computed after excluding homopolymers.\nFig. 4 | Genome-wide association a) Manhattan plot showing a missense variant in the MSH2 gene associating with an increased number of mDNMs transmitted to offspring. b) Region plot for the missense variant in MSH2. Two correlated markers also reach genome-wide significance. c) Manhattan plot showing a synonymous variant in the NEIL2 gene which associates with an increased number of mDNMs with motif lengths greater than one bp transmitted to offspring. The plot also shows the p-value for the MSH2 missense variant considering mDNMs with motif lengths greater than one bp. d) Region plot for a synonymous variant in the NEIL2 gene. No other markers at the locus reach genome wide significance.\nChromosomes on Manhattan plots are marked with alternating colors and the threshold for genome wide significance was set as \\(1 \\cdot 10^{-9}\\).\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif (bp)mDNM rate (95% CI)#microsatellites#DNMs
12.15 \\cdot 10^{-5} (2.11 \\cdot 10^{-5}-2.19 \\cdot 10^{-5})399,087 (62.9%)17,194 (22.3%)
21.07 \\cdot 10^{-4} (1.06 \\cdot 10^{-4}-1.09 \\cdot 10^{-4})93,653(14.8%)33,025 (42.9%)
34.92 \\cdot 10^{-5} (4.70 \\cdot 10^{-5}-5.21 \\cdot 10^{-4})29,869 (4.7%)5,469 (7.1%)
48.57 \\cdot 10^{-5} (8.28 \\cdot 10^{-4}-8.86 \\cdot 10^{-4})66,541 (10.5%)18,795 (24.4%)
52.58 \\cdot 10^{-5} (2.37 \\cdot 10^{-5}-2.86 \\cdot 10^{-5})29,992 (4.7%)2,132 (2.8%)
61.04 \\cdot 10^{-5} (9.07 \\cdot 10^{-6}-1.23 \\cdot 10^{-5})15,264 (2.4%)372 (0.5%)
Total4.95 \\cdot 10^{-5} (4.88 \\cdot 10^{-5}-5.02 \\cdot 10^{-5})634,40676,987
\n\nTable 1: mDNM rate, number of microsatellites in high quality set and number of mDNMs, all by motif lengths. Dinucleotide repeats have the highest mDNM rate and represent almost 43% of our mDNMs.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Data setPaternal age effect (95% CI)Maternal age effect (95% CI)#paternal/#maternal
All markers0.178(0.165-0.190)0.058(0.047-0.069)35,501/10,670
Motif length 10.013(0.006-0.020)0.007(-0.001-0.014)5,141/2,948
Motif length 20.078(0.069-0.087)0.029(0.022-0.037)17,388/4,084
Motif length 30.011(0.008-0.014)0.002(-0.001-0.004)2,663/883
Motif length 40.056(0.050-0.062)0.013(0.008-0.017)9,184/2,354
Motif length 50.004(-0.003-0.011)-0.002(-0.007-0.003)977/341
Motif length 6-0.008(-0.021-0.005)0.016(0.003-0.029)148/60
\n\nTable 2: Maternal and paternal age effect for all motif lengths and conditioning on motif length. mDNMs at mono-, di-, tri- and tetranucleotide repeats increase with paternal age while mDNMs at di- and tetra- and hexanucleotide repeats increase with maternal age. Bold represents significant association (\\( P < 0.05 \\)).\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
MotifMutation size (In motifs)
<-2 (p/m)-2 (p/m)-1 (p/m)1 (p/m)2 (p/m)>2 (p/m)
1312(168/144)140(69/71)2,782(1,671/1,111)3,962(2,777/1,185)214(121/93)679(335/344)
2610(399/211)2,482(2,101/381)7,124(6,192/932)8,933(6,936/1,997)1,849(1,490/359)474(270/204)
390(52/38)160(117/43)1,516(1,053/463)1,524(1,251/273)228(171/57)28(19/9)
4134(90/44)237(170/67)5,229(3,972/1,257)5,798(4,861/937)107(73/34)33(18/15)
514(11/3)44(30/14)583(392/191)651(533/118)13(7/6)13(4/9)
60(0/0)4(3/1)79(50/29)117(90/27)6(3/3)2(2/0)
Total1,160(720/440)3,067(2,490/577)17,313(13,330/3,983)20,985(16,448/4,573)2,417(1,865/552)1,229(648/576)
\n\nTable 3: Counts of mutation sizes of phased mDNMs per motif length and for all motif lengths combined. Maternal and paternal counts are given in brackets. Maternal mDNMs are larger on average than paternal ones and we see the ratio of maternal mDNMs increases with their size.\nSupplementary information\n\nSupplementary note 1: STR properties correlate with polymorphism rate and expected heterozygosity\n\nA number of STR properties correlate with the polymorphism rate and expected heterozygosity33. Both the motif length and how many times the motif is repeated in its RRT (repeat number) affect the polymorphism rate and the expected heterozygosity. Almost all homopolymers are polymorphic and both the fraction of polymorphic STRs and expected heterozygosity decrease with motif length (linear regression \\( P < 1 \\cdot 10^{-320} \\) for both datasets, Fig. S1, Fig. S2). For all motif lengths, an increase in repeat number results in both a higher polymorphism rate and expected heterozygosity (linear regression \\( P < 1 \\cdot 10^{-320} \\) for both datasets, Fig. S1, Fig. S2).\n\nThe fraction of G/C bases in an STR’s motif (motif GC content) is negatively correlated with polymorphism rate (Table S21) while negative correlation with expected heterozygosity is only observed for motif lengths above two bp (Table S20). Homopolymers from the C motif class have higher expected heterozygosity than A class homopolymers (Table S20) but account for only 0.8% of all homopolymers (Table S15). CpG microsatellites (CG motif class) also have on average higher expected heterozygosity than the other dinucleotide motif classes but account for only 0.4% of all dinucleotide repeats (Table S15, Table S20). Thus, although C class homopolymers and CG class dinucleotide microsatellites have higher expected heterozygosity values than other classes with equal motif lengths, their overall effect on microsatellite diversity is small since they are so rare.\n\nEnrichment of A motif class homopolymers in the human genome is thought to be a result of the microsatellite-like structure often found at 3′ ends of reverse transcribed RNA sequences, i.e. poly-A tails64,65 and the high expected heterozygosity rate at CG class microsatellites is consistent with CpG sites acting as mutational hot spots66. Negative correlation of GC content to polymorphism rates and expected heterozygosity can likely be explained by the three hydrogen bonds between paired G/C bp, compared to two between A/T bp, making the slippage-causing disassociation from the template strand during replication less likely.\nWe define repeat purity as the ratio between the number of times the STR’s repeat motif is observed in its RRT and the maximum number of repeat motifs if the sequence contained no interruptions (where the highest possible repeat purity is 1). Stratified on RRT length, all correlations between repeat purity and both expected heterozygosity and polymorphism rate were positive (Table S18, Table S19, Fig. S3, Fig. S4). This is consistent with\\(^{67-70}\\), reporting a positive correlation between repeat purity and mDNM rate. Interruptions of the repeat sequence decrease the number of locations where replication slippage can occur and thus the mDNM rate\\(^{27}\\).\n\n**Supplementary note 2: False positive estimation**\n\nTo estimate the false positive rate of our method we used two methods; PacBio CCS sequence data, available for four of our trios, and mDNM sharing in nine Icelandic monozygotic twin pairs in our set. We used haplotype resolved assemblies of the PacBio data and while we were unable to verify homopolymer mDNMs as the PacBio sequencing error rate was too high\\(^{71}\\) we were able to verify the existence of 27 mDNMs with motif length >1. Out of these, 26 were true positives and one was a false positive at a dinucleotide repeat, giving an expected false positive rate of 3.7% for motif lengths greater than 1. (Table S4).\n\nFor mDNMs observed in offspring with a monozygotic twin also present in our set, we checked whether the mDNM genotypes were concordant between both twins. We compared mDNM calls where the genotype was present in the monozygotic twin of the offspring. We treated genotype calls of the other twin present if the genotype quality was higher than or equal to 30, which is half of the value we require for trio mDNM detection. Out of the 230 comparable MZ-twin mDNMs, 217 were found in both twins and 13 were discordant (Table S30) which gives a false positive rate estimate of 5.6%. We note that this is likely to be an overestimate, as some of the differences between the twin pairs could be due to result of post zygotic mutations, representing true differences between twins\\(^{72}\\).\n\nUsing haplotype sharing across 540 three-generation families (795 trios), we counted how many times an mDNM was transmitted from an offspring to its child and estimated the transmission rate. The expected value of the transmission rate is 0.50 and deviations from it\nquantify false positive mDNM detection rates. For example, if the observed mutations were somatic and thus false positive as mDNMs, we would not observe transmission from the offspring to its child. We observe a transmission rate of 0.49 (N = 11,228, 95% CI: 0.48-0.50) which gives an estimated false positive rate of 2%, although transmission rates vary between motif lengths and thus the error rate estimates as well (Table S14). Notably, the transmission rate for homopolymers is only 0.4 while the other motif lengths have transmission rates much closer or equal to 0.5.\n\nSupplementary note 3: Replication of mutation rate trends\n\nAs the RRT length increased from ten to 100 bp the mDNM rate also increased for all motif lengths (Fig. 2), consistent with findings from previous studies\\(^{26,73–75}\\) and, intuitively, the opportunities for errors during replication increase with a microsatellite’s RRT length.\n\nMicrosatellites with longer RRTs have been shown to be more likely to contract and shorter ones to expand\\(^{26,76–81}\\). We replicate this. For all RRT length thresholds, a higher fraction of mDNMs had a gain of repeat motifs below the threshold than above it, i.e., the microsatellite group with shorter overall RRTs were more likely to expand than the group with longer RRTs (Table S26).\n\nThe mDNM rate for homopolymers was positively correlated with the motif G/C content, while di-, tri-, tetra- and pentanucleotide repeats had a negative correlation with the mDNM rate and for hexanucleotide repeats we lacked power to detect a correlation with the mDNM rate (Fig. 2, Table S2).\n\nRepeat purity correlated positively with the mDNM rate for all motif lengths (effect = 0.12, \\( P < 1 \\cdot 10^{-320} \\), Fig. 2, Table S2), consistent with previously published results\\(^{75}\\). The correlation remained positive in most cases after conditioning on RRT lengths (Table S3).\n\nmDNM rates varied by repeat motif class, AAT motif mDNMs were by far the most common ones among trinucleotides. The rare C homopolymers mutated more frequently than the A homopolymers and AC motif microsatellites had the highest mutation rate of the dinucleotide\nmicrosatellites before correcting for RRT length and CG motif microsatellites after correction (Supplement, Fig. 2, Table S1).\n\nSupplementary note 4: mDNMs in functionally annotated and early replicating regions\n\nPrevious studies have reported increased efficiency of mismatch repair (MMR) in early-replicating regions of the human genome\\(^{82}\\). Our results are in line with this since we see 1.28 (95% CI: 1.25-1.31) fold depletion of mDNMs in early replicating regions of the genome\\(^{83}\\).\n\nExonic mDNMs are rarer than their intergenic and intronic counterparts. In 2,568,858 transmissions of microsatellites intersecting exons by one or more bp, we observed 33 mDNMs.\n\nWe estimated the exonic mDNM rate as \\(1.3 \\cdot 10^{-5}\\) MMG, which is 3.9 (95% CI: 2.8-5.6) times lower than the genome-wide estimate. mDNMs are further 1.7 (95% CI: 1.3-2.1), 1.4 (95% CI: 1.3-1.5) and 4.2 (95% CI: 1.2-34.4)-fold depleted in 5′UTR and 3′UTR and splice regions, respectively. The 33 exonic mDNMs occurred at 21 unique microsatellites, of which 19 had motif lengths that were multiples of three and since amino acids are coded with three bp codons, mutations at microsatellites with multiple of three motif lengths are unlikely to cause a frameshift but rather an in-frame alteration of a gene. Sixteen of the exonic mDNMs were trinucleotide microsatellites, three were hexanucleotide microsatellites and the remaining two were homopolymers.\n\nTri- and hexanucleotide repeats were enriched in coding exons (chi squared test \\(P < 1 \\cdot 10^{-320}\\)) compared with the rest of genome. Microsatellites with motif lengths that are multiples of three accounted for 93.3% of exon intersecting microsatellites and 70.9% of all exon intersecting non polymorphic STRs (Table S16). In contrast, 12.3% of all microsatellites had motifs that are multiples of three (Table S16) and 44.5% of non-polymorphic STRs.\n\nThe average purity of microsatellites was 0.94, while among microsatellites in exons the purity was notably lower (0.87, Mann-Whitney \\(P = 1 \\cdot 10^{-153}\\)). Purity was positively correlated with the mDNM rate, so decreased purity in exons may decrease occurrences of possibly pathogenic mDNMs. This indicates that there is a possible positive selection for point mutations that\nreduce the purity of exonic microsatellites or a possible negative selection for point mutations that increase in their purity. The purity difference is largest for trinucleotide repeats, the most common motif length for exon intersecting microsatellites (Table S17). Non-polymorphic coding STRs do not have decreased purity compared to their intergenic counterparts, so point mutations are less likely to be the mechanism preventing mutations at these exonic STRs (Table S17).\n\nSupplementary note 5: mDNM rate estimate comparison\n\nOur mDNM rate estimate is nominally lower than a previous estimate\\(^{29}\\) of \\(5.6 \\cdot 10^{-5}\\) and lower than the two estimates of \\(10.0 \\cdot 10^{-4}\\) and \\(2.7 \\cdot 10^{-4}\\) for tetra- and dinucleotide repeats, respectively\\(^1\\). This apparent discrepancy could be a result of a more conservative filtering in our study, a younger set of parents, a generally healthier cohort and a different range of motif lengths considered. However, the most likely reason for the apparent discrepancy is the sample size difference between the studies. Our set contains 53,026 individuals while the set analyzed by Mitra et al.\\(^{29}\\) contained 6,548 individuals. Thus, our minimum detection frequency is \\(1/(2 \\cdot 53,026) = 9.0 \\cdot 10^{-6}\\) compared to the minimum detection frequency\\(^{29}\\) of \\(1/(2 \\cdot 6,548) = 7.6 \\cdot 10^{-5}\\) enforced by the smaller sample size. We recomputed our mutation rate estimate conditioning on microsatellite frequency (Table S27) and confirmed that at a detection frequency cutoff of \\(7.6 \\cdot 10^{-5}\\) our estimate becomes \\(5.6 \\cdot 10^{-5}\\) and matches the one presented by Mitra et al.\\(^{29}\\). Similarly, at a minimum frequency of 10% our estimate is comparable to the one from Sun et al.\\(^1\\) Based on this we conclude that a mDNM rate estimate depends on the size of the sample set studied.\n\nSupplementary note 6: mDNM rate comparison between motif equivalence classes\n\nThe mDNM rate is higher for C class homopolymers than for A class ones (Mann-Whitney U test \\(P < 1 \\cdot 10^{-230}\\), Fig. 2), but C homopolymers are much rarer and represent only 0.8% of all homopolymers in our set (Table S15). The AC motif class has the highest mDNM rate of the dinucleotide microsatellites (Table S22, Fig. 2). However, the average RRT length of the AC\nmotif class is longest among dinucleotide classes. Including RRT length as a covariate the CG motif class has a higher mDNM rate than all other dinucleotide classes (Table S23), in line with the fact that CpG sites have been shown to act as mutational hot spots66.\n\nThe AAT motif class had a higher mDNM rate than eight of the other nine trinucleotide repeat motif classes. Only the rarest class (ACG) did not show a significantly different mDNM rate (Table S24). The AAT motif class accounts for 38.4% of all trinucleotide microsatellites and 79.0% of trinucleotide mDNMs and has an mDNM rate 1.5 times higher than the second highest class (Table S23). A higher mDNM rate for AAT class motifs has been previously reported for other organisms84,85 but not, to our knowledge for, humans.\n\nAn in vitro study of how repeat motifs affect the frequency of polymerase slippage during replication reported that motifs less likely to stall replication were more likely to mutate during replication. Of the dinucleotide repeat classes, microsatellites from the AC class had the lowest replication stall affinity53. The higher mDNM rate of microsatellites in the AAT motif class could be a result of its low replication stall affinity53. The two hydrogen bonds between A/T base-pairs compared to the three between G/C base-pairs also makes A/T pairs more likely to disassociate from each other, enabling the formation of secondary structures and possible mDNMs. Finally, repeats with a high A/T-content also have a sequence composition similar to elements involved in DNA unwinding at replication origins86 during mitosis. These repeats could therefore function as aberrant replication origins and cause a higher mDNM rate during replication in S phase86.\n\nSupplementary note 7: Motif length enrichment excluding homopolymers\n\nA higher fraction of maternal mDNMs occur at tri-, penta- and hexanucleotide microsatellites while dinucleotide microsatellites represent a larger fraction of paternal mDNMs (Table S25, Fig. 3).\nThe average number of bp involved without homopolymers is larger in maternal mDNMs than in paternal mDNMs (3.9 vs 3.4 bp, Mann-Whitney U test \\( P = 2.6 \\cdot 10^{-23} \\)). Stratifying on motif length reveals that maternal mDNMs affect more bp on average at di- and tetranucleotide microsatellites (Table S7).\nConsidering mDNMs with motif lengths above one, the number of repeats in the reference is higher for paternal mDNMs (16.8 vs 15.7 repeats, Mann-Whitney U test \\( P = 2.8 \\cdot 10^{-51} \\)).\n\nSupplementary note 8: Motif length fraction change with age including homopolymers\n\nTetranucleotide mDNMs increase their fraction with paternal age (Linear regression \\( P = 1.5 \\cdot 10^{-6} \\)) and the fraction of di- and hexanucleotide mDNMs increases with maternal age.\n\nFor both maternal and paternal mDNMs the fraction of mDNMs at homopolymers decreases with age.\n\nSupplementary note 9: Effects on microsatellite mutator alleles on sDNMs\n\nSomatic and germline mutations in mismatch-repair genes are known to cause microsatellite instability and hypermutator phenotypes in tumors of the colon and endometrium. Sequencing of large cohorts of tumors has revealed several mutational signatures associated with mismatch repair deficiency\\(^{87}\\).\n\nThese signatures show a strong correlation with somatic microsatellite instability. Mutations in components of the base-excision repair pathway, most notably *NTHL1* and *MUTYH*, also cause distinct mutational signatures in tumors with these mutations (COSMIC signatures SBS30 and SBS36\\(^{87}\\), respectively). Given the effects of rs4987188[A] and rs8191642[G] on the rate of mDNMs, we were interested in knowing if they also affect the mutational spectra of single-base-substitution DNMs, for example by altering the MMR/BER pathways in the testis.\n\nUsing only phased DNMs, we compared the 96-class trinucleotide spectra of DNMs transmitted from carrier and non-carrier mothers and fathers. All spectra were highly similar (pairwise cosine similarities >0.95) and showed no hint of MMR deficient related mutational signatures (Fig. S8). This suggests that the effects of rs4987188[A] and rs8191642[G] are confined to microsatellite sites and they do not otherwise affect the fidelity of the mismatch or base-excision repair pathways.\nFig. S1 Average expected heterozygosity in UKB as a function of repeat number stratified on motif length. The drop in all motif lengths is most likely due our inability to reliably detect long alleles from short reads, causing underestimation of expected heterozygosity values at microsatellite with long reference alleles.\nFig. S2 Average expected heterozygosity in Icelandic data set as a function of repeat number stratified on motif length.\n\n![Average expected heterozygosity in Icelandic data set as a function of repeat number stratified on motif length.](page_184_186_1207_1092.png)\nFig. S3 Average repeat purity as a function of repeat number stratified on motif length for the Icelandic data set. Red marks polymorphic STRs (microsatellites) and blue non-polymorphic STRs.\nFig. S4 Average repeat purity as a function of repeat number stratified on motif length for the UKB data set. Red marks polymorphic STRs (microsatellites) and blue non-polymorphic STRs.\nFig. S5 Read pair phasing. We use read pairs which contain a long range phased marker and report an mDNM. Reads with long range phased markers covering the de novo site but supporting the other allele can also further give information on the parent of origin. An example of a maternal mDNM where three read pairs report a long range phased maternal marker and a de novo allele, one pair is not informative and one contains a long range phased paternal marker and not the de novo allele.\n\n![Diagram showing read pairs with de novo events and phased markers](page_184_232_1017_496.png)\n\nLegend:\nDe novo event\nLong range phased maternal marker\nLong range phased paternal marker\nFig. S6 Allele based phasing: If the de novo allele is present in neither parent and the other allele is present only in one parent we phase the de novo event to the other parent. Here we phase the de novo event to the father since a maternal allele is seen in the offspring but neither of the paternal ones.\n\n![Diagram showing allele-based phasing: M1/M2 (red), F1/F2 (blue), and M1/X (green) with arrows indicating the phasing process](page_184_153_495_377.png)\nFig. S7 Haplotype sharing in three generation families: If the de novo is transmitted from the offspring to its child we phase the de novo to the parent sharing a haplotype with the offspring, and to the parent not sharing a haplotype if de novo is not transmitted.\n\n![Diagram showing haplotype sharing in three generation families](page_184_120_654_496.png)\nFig. S8: sDNM mutation signatures for offspring of paternal and maternal carriers and non-carriers of both rs4987188 and rs8191642. The signatures are not different in any of the four comparisons so we assume that the variants do not affect the generation of sDNMs.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Class representativeOther members
AT
CG
ACCA, GT, TG
AGGA, CT, TC
ATTA
CGGC
AACACA, CAA, GTT, TGT, TTG
AAGAGA, GAA, CTT, TCT, TTC
AATATA, TAA, ATT, TAT, TTA
ACCCAC, CCA, GGT, GTG, TGG
ACGCGA, GAC, CGT, TCG, GTC
ACTCTA, TAC, AGT, TAG, GTA
AGCGCA, CAG, GCT, TGC, CTG
AGGGAG, GGA, CCT, CTC, TCC
ATCTCA, CAT, GAT, TGA, ATG
CCGCGC, GCC, CGG, GCG, GGC
\n\nTable S1 Motif equivalence classes and their members.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
MotifRepeat tract lengthPurityGC contentMotif length
All0.10 (<1 · 10^{-320})0.12(<1 · 10^{-320})9.47 · 10^{-5}(0.58)-0.15 (<1 · 10^{-320})
1bp0.16(<1 · 10^{-320})0.28(<1 · 10^{-320})0.02(<1 · 10^{-320})X
2 bp0.10(<1 · 10^{-320})0.17(<1 · 10^{-320})-0.01(8.6 · 10^{-87})X
3 bp0.12 (<1 · 10^{-320})0.14 (<1 · 10^{-320})-0.03(3.0 · 10^{-235})X
4 bp0.10(<1 · 10^{-320})0.10 (<1 · 10^{-320})-0.003(2.2 · 10^{-10})X
5 bp0.1 (<1 · 10^{-320})0.05(4.4 · 10^{-121})-0.003(2.4 · 10^{-2})X
6 bp0.09(<1 · 10^{-320})0.02(8.9 · 10^{-18})7.5 · 10^{-4} (0.76)X
\n\nTable S2 Poisson multiple regression coefficients and p-values for the effect on the mDNM rate by RRT length, repeat purity, GC content and motif length for all markers and stratified on motif length. Repeat tract length and repeat purity remain significant and consistent in their effect directionality across the full data set and all motif length subsets. GC-content is positively correlated to the mDNM rate for homopolymers but for di-, tri-, tetra-, and pentanucleotide repeats the motif GC-content has an inverse correlation to the mDNM rate.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Bp1 bp motif2 bp motif3 bp motif4 bp motif5 bp motif6 bp motif
11-200.13(3.2 · 10^{-93})0.04(1.2 · 10^{-9})0.05(5.7 · 10^{-4})-0.005(0.36)-0.006(0.25)-0.01(0.17)
21-300.21(< 1.0 · 10^{-320})0.16(< 1.0 · 10^{-320})0.13(3.4 · 10^{-38})0.05(2.0 · 10^{-35})-0.002(0.56)0.002(0.65)
31-400.20(2.0 · 10^{-36})0.17(< 1.0 · 10^{-320})0.18(7.3 · 10^{-136})0.11(2.2 · 10^{-211})0.06(1.1 · 10^{-28})0.01(0.01)
41-500.06(0.23)0.16(< 1.0 · 10^{-320})0.12(1.4 · 10^{-35})0.09(1.3 · 10^{-293})0.08(4.4 · 10^{-46})0.03(1.0 · 10^{5})
51-60-0.50(3.7 · 10^{-4})0.15(3.0 · 10^{-252})0.11(5.1 · 10^{-40})0.07(5.8 · 10^{-216})0.06(3.5 · 10^{-24})0.06(1.1 · 10^{14})
61-70-1.13(5.9 · 10^{-5})0.12(1.6 · 10^{-36})0.12(1.8 · 10^{-12})0.06(3.9 · 10^{-115})0.06(1.4 · 10^{-18})0.06(2.2 · 10^{9})
71-800.65(0.48)0.14(9.3 · 10^{-10})0.03(0.34)0.04(4.4 · 10^{-42})0.03(6.1 · 10^{6})0.02(0.15)
81-90X0.05(0.58)0.47(0.31)0.04(7.6 · 10^{-12})0.05(5.0 · 10^{5})0.06(0.06)
>90XX5.43(1.00)0.03(4.3 · 10^{-5})0.008(0.42)0.04(0.34)
\n\nTable S3 Poisson regression coefficients and p-values for effect of repeat purity on mDNM rate split into ten bp RRT length bins stratified on motif length. Data for regression was not available for homopolymers above 80 bp and dinucleotide microsatellites above 90 bp.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
ChromPosMotifRef. (No repeats)Offspring gtFather gtMother gtVerified
chr1180254522CTAT1515/1511/1615/15yes
chr12100919737TATC1515/1815/1715/17yes
chr2199703012GTTT89/98/108/9yes
chr4115864579TG1111/1311/1211/11no
chr786946160CA1614/1816/1815/18yes
chr1143435069AGAT1617/1715/1815/17yes
chr1354157465TA2016/1918/2116/22yes
chr1482746964AATA88/108/98/9yes
chr1754067449TTTTA77/87/77/7yes
chr183742950CTTC1111/1411/1211/13yes
chr1863468251AAC810/128/1010/10yes
chr110498281AAAAC88/79/97/9yes
chr4140179641TGTTT87/98/55/7yes
chr644850746ATCT1316/1615/1510/16yes
chr1669147179AAT1514/1615/1515/14yes
chr1180853627AC2119/2519/2619/20yes
chr2034877898AGAT1215/1613/1616/16yes
chr385784531TATC1313/1210/1411/12yes
chr4169443052TATC1312/1514/1413/12yes
chr638464486TTTTC66/56/76/7yes
chr729184144AGAT1414/1511/1614/13yes
chr8110980554ATCT1012/1211/1112/13yes
chr1122272303CA2222/1923/2622/25yes
chr1229413662AC1516/2014/1614/19yes
chr1380326450TG99/88/88/8yes
chr1172791800AT77/147/77/13yes
chr819119757TA99/139/129/12yes
\n\nTable S4 mDNMs verified by haplotype resolved assemblies generated from pacBio HiFi sequencing data. We were unable to verify homopolymer mDNMs due to high error rates.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Marker 1Marker 2Conditional \\( P \\) 1-2Conditional \\( P \\) 2-1R2
chr2:47416318chr2:474940688.9 · 10-25.1 · 10-20.74
chr2:47416318chr2:47491330:03.6 · 10-22.3 · 10-20.60
chr2:47416318chr2:47491330:13.6 · 10-22.3 · 10-20.60
chr2:47494068chr2:47491330:00.170.180.80
chr2:47494068chr2:47491330:10.170.180.80
chr2:47491330:0chr2:47491330:11.001.001.00
\n\nTable S5 Conditional association p-values for markers significantly associating with increased mDNM rate (*MSH2* missense marker in bold). All markers are correlated but a residual signal remains after conditioning the intergenic signal at chr2:47491330 for the missense marker\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
PopulationAllele frequency of rs4987188
Iceland1.9%
UKB1.5%
Fingen3.0%
Africa0.2%
Asia0.0%
\n\nTable S6 Allele frequency of rs4987188 in different populations, it is most frequent in the Finnish population and not found in Asians.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif (bp)PaternalMotifs affectedMaternalMotifs affectedMann-Whitney P
15,141(14.5%)1.672,962(27.6%)2.131.9 \\cdot 10^{-23}
217,388(49.0%)1.384,119(38.4%)1.716.0 \\cdot 10^{-13}
32,663(7.5%)1.22887(8.2%)1.335.5 \\cdot 10^{-2}
49,184(25.9%)1.062,365(22.0%)1.129.6 \\cdot 10^{-5}
5977(2.8%)1.08343(3.2%)1.210.38
6148(0.4%)0.9562(0.6%)0.770.26
\n\nTable S7 Motif length composition of paternal and maternal mDNMs, mean number of motifs added/removed for each motif length in each parent and Mann-Whitney U test p-values for different step sizes between parents. Bold represents significant difference in step size between parents (p<0.05).\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif length (bp)Mean RRT length(bp) (pat/mat)\\( P \\)
117.0/16.90.12
239.2/37.21.9 \\cdot 10^{-24}
340.8/40.40.72
452.2/50.15.6 \\cdot 10^{-3}
554.7/51.11.6 \\cdot 10^{-3}
649.8/42.62.2 \\cdot 10^{-2}
\n\nTable S8 Mean RRT lengths for paternal and maternal mDNMs. The paternal mDNMs have longer RRT at di-, tetra-, penta- and hexanucleotide microsatellites. Bold represents significant difference in RRT length between paternal and maternal mDNMs (p<0.05).\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n
Members of ATTCT motif equivalence class
ATTCT
TTCTA
TCTAT
CTATT
TATTC
AGAAT
GAATA
AATAG
ATAGA
TAGAA
\n\nTable S9 Members of the ATTCT motif equivalence class considered for paternal expansion bias.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif equivalence class% of paternal% of maternalOdds ratio maternal/paternal (\\( P \\))
AAC10.7%7.6%0.68[0.52;0.90] (7.6 · 10^{-3})
AAG2.1%2.7%1.28[0.77;2.05] (0.36)
AAT80.9%84.2%1.26[1.03;1.55] (0.02)
ACC0.3%0.0%No maternal mDNMs.
ACG0.0%0.0%No mDNMs
ACT1.6%0.8%0.49[0.20;1.04] (7.2 · 10^{-2})
AGC0.6%1.4%2.14[0.99;4.50] (5.1 · 10^{-2})
AGG0.2%0.2%1.56[0.19;8.48] (0.64)
ATC3.4%2.1%0.63[0.37;1.02] (7.2 · 10^{-2})
CCG0.3%1.0%3.39[1.28;9.20] (2.0 · 10^{-2})
Motif equivalence class% of paternal% of maternalEnrichment
AC88.7%79.8%0.50[0.46;0.55] (2.9 · 10^{-48})
AG4.6%7.4%1.65[1.43;1.88] (4.5 · 10^{-12})
AT6.6%12.7%2.05[1.84;2.29] (3.6 · 10^{-35})
CG0.04%0.1%3.04[0.88;9.76] (6.2 · 10^{-2})
\n\nTable S10 Motif equivalence class odds ratios for di- and trinucleotide microsatellites. Maternal mDNMs are more common at AAT, CCG, AG and AT motif class microsatellites while paternal mDNMs are more common at AAC and AC motif class microsatellites. Bold represents significant enrichment (p<0.05).\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif lengthCoefficient (P) for lower step size than homopolymers
PaternalMaternal
2-0.3(5.3 \\cdot 10^{-50})-0.5(2.0 \\cdot 10^{-22})
3-0.4(3.2 \\cdot 10^{-31})-0.6(6.6 \\cdot 10^{-15})
4-0.5(7.6 \\cdot 10^{-104})-0.8(8.9 \\cdot 10^{-41})
5-0.5(5.4 \\cdot 10^{-23})-0.6(7.5 \\cdot 10^{-7})
6-0.6(7.8 \\cdot 10^{-7})-0.9(8.9 \\cdot 10^{-4})
\n\nTable S11 Linear regression coefficients and p-values for the effect of increasing motif length on step size in paternal and maternal mDNMs. All motif lengths have lower step sizes than homopolymers.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Read pair tracingTotal
PaternalMaternal
3 generationPaternal2,199702,269(75.5%)
Maternal118619737(24.5%)
Total2,317(77.1%)689(22.9%)
\n\nTable S12 Comparison of phasing results for mDNMs phased using both three generation and read pair phasing. The concordance between the methods is 93.7% and the ratio between maternal and paternal mDNMs is similar in both sets.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Allele based
PaternalMaternalTotal
3 generationPaternal2,390392,429(78.2%)
Maternal103576679(21.8%)
Total2,493(80.2%)615(19.8%)
\n\nTable S13 Comparison of phasing results for mDNMs phased using both three generation and allele based phasing. The concordance between the methods is 95.4% and the ratio between maternal and paternal mDNMs is similar in both sets.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Allele basedRead pair tracingTotal
PaternalMaternalTotal
Paternal8,86598,874(79.6%)
Maternal212,2582,279(20.4%)
Total8,886 (79.7%)2,267(20.3%)
\n\nTable S14 Comparison of phasing results for mDNMs phased using both read pair and allele based phasing. The concordance between the methods is 99.7%.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif length (bp)Transmission rateError estimate
10.40 (861/2,156)20%
20.50 (2,558/5,083)0%
30.51 (433/857)2%
40.53 (1,458/2,764)6%
50.55 (169/310)10%
60.47 (27/58)6%
Total0.49 (5,506/11,228)2%
\n\nTable S15 Transmission rate by motif length and combined for all mDNMs phased using haplotype sharing in three-generation families.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif classMaternalPaternalFull marker setTRF output
A97.5%97.7%99.2%99.2%
C2.5%2.3%0.8%0.8%
AC67.6%84.3%49.1%54.4%
AG8.9%5.6%19.9%23.4%
AT23.2%10.0%30.5%21.7%
CG0.4%0.1%0.4%0.4%
AAC13.0%13.3%27.1%20.8%
AAG3.8%2.0%15.0%10.0%
AAT75.3%77.6%34.9%32.9%
ACC0.8%0.4%4.0%7.4%
ACG0.0%0.0%0.1%0.1%
ACT1.2%0.9%0.9%1.9%
AGC2.1%1.2%3.0%7.8%
AGG0.8%0.6%7.5%11.3%
ATC2.4%3.9%4.3%6.1%
CCG0.6%0.2%3.1%1.6%
\n\nTable S16 Fraction of each motif equivalence class within homopolymers, di- and trinucleotide repeats split on maternal and paternal mDNMs, fraction of each motif equivalence class in full marker set and in the Tandem Repeats Finder (TRF) output.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif length (bp)All microsatellitesMicrosatellites in coding exonsNon polymorphic STRs in coding exons
150.0%1.8%0.003%
216.7%0.5%0.6%
35.8%76.2%17.5%
413.2%3.0%6.4%
57.1%1.5%22.1%
66.5%17.1%53.4%
\n\nTable S17 Motif length composition for all microsatellites and exon intersecting microsatellites.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif lengthAll microsatellitesCoding microsatellitesNon-polymorphic STRsCoding non-polymorphic STRs
10.980.97 (0.25)0.970.95 (0.05)
20.950.96 (0.14)0.930.97 (5.9 · 10^{-12})
30.930.89 (9.0 · 10^{-66})0.940.93 (1.3 · 10^{-8})
40.890.88 (0.87)0.930.96 (5.7 · 10^{-43})
50.840.89 (3.0 · 10^{-4})0.960.97 (2.3 · 10^{-26})
60.810.80 (0.12)0.940.94 (3.8 · 10^{-4})
Overall0.940.87 (1 · 10^{-153})0.950.95 (9.6 · 10^{-14})
\n\nTable S18 Average purity values per motif length for all microsatellites, coding microsatellites, all non-polymorphic STRs and coding non-polymorphic STRs. Mann-Whitney U-test p-values for significant difference in purity values between exonic and non-exonic microsatellites in each motif length in brackets.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
RRT lengthPurity effect (Ice/UKBB)\\( P \\) (Ice/UKBB)
11-200.39/0.23< \\( 1.0 \\cdot 10^{-320} \\)/< \\( 1.0 \\cdot 10^{-320} \\)
21-300.71/0.67< \\( 1.0 \\cdot 10^{-320} \\)/< \\( 1.0 \\cdot 10^{-320} \\)
31-400.87/0.85< \\( 1.0 \\cdot 10^{-320} \\)/< \\( 1.0 \\cdot 10^{-320} \\)
41-501.17/1.15< \\( 1.0 \\cdot 10^{-320} \\)/< \\( 1.0 \\cdot 10^{-320} \\)
51-601.17/1.18< \\( 1.0 \\cdot 10^{-320} \\)/< \\( 1.0 \\cdot 10^{-320} \\)
61-701.10/1.13< \\( 1.0 \\cdot 10^{-320} \\)/< \\( 1.0 \\cdot 10^{-320} \\)
71-801.05/1.08< \\( 1.0 \\cdot 10^{-320} \\)/< \\( 1.0 \\cdot 10^{-320} \\)
81-900.96/1.073.9 \\cdot 10^{-141}/6.8 \\cdot 10^{183}
>900.76/0.835.4 \\cdot 10^{56}/6.1 \\cdot 10^{57}
\n\nTable S19 Linear regression coefficients and p-values for the effect of repeat purity on expected heterozygosity within ten base pair bins of RRT length for both the Icelandic and UKB datasets.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
RRT lengthPurity effect (Ice/UKBB)P (Ice/UKBB)
11-207.86/5.31< 1.0 \\cdot 10^{-320}/< 1.0 \\cdot 10^{-320}
21-307.84/6.09< 1.0 \\cdot 10^{-320}/< 1.0 \\cdot 10^{-320}
31-406.11/5.47< 1.0 \\cdot 10^{-320}/< 1.0 \\cdot 10^{-320}
41-505.94/4.96< 1.0 \\cdot 10^{-320}/< 1.0 \\cdot 10^{-320}
51-604.78/3.668< 1.0 \\cdot 10^{-320}/2.4 \\cdot 10^{-83}
61-704.42/2.722.8 \\cdot 10^{-164}/6.0 \\cdot 10^{-17}
71-804.22/1.952.0 \\cdot 10^{-61}/7.1 \\cdot 10^{-6}
81-904.03/-0.096.2 \\cdot 10^{-26}/0.9
>902.72/0.611.0 \\cdot 10^{-16}/0.1
\n\nTable S20 Logistic regression coefficients and p-values for the effect of repeat purity on polymorphism rate within ten base pair bins of RRT length for both the Icelandic and UKB datasets.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif lengthEffect (Ice/UKBB)\\( P \\) (Ice/UKBB)
10.15/0.174.5 \\cdot 10^{-312}/< 1.0 \\cdot 10^{-320}
20.14/0.10< 1.0 \\cdot 10^{-320}/< 1.0 \\cdot 10^{-320}
3-0.12/-0.05< 1.0 \\cdot 10^{-320}/< 1.0 \\cdot 10^{-320}
4-0.07/-0.041.1 \\cdot 10^{-155}/< 1.0 \\cdot 10^{-320}
5-0.06/-0.038.0 \\cdot 10^{-141}/< 1.0 \\cdot 10^{-320}
6-0.02/-0.013.9 \\cdot 10^{-18}/1.52 \\cdot 10^{-95}
\n\nTable S21 Linear regression coefficients and p-values for the effect of GC motif content on expected heterozygosity within motif lengths for both the Icelandic and UKB datasets.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif lengthEffect (Ice/UKBB)\\( P \\) (Ice/UKBB)
1-0.20/-1.334.9 \\cdot 10^{-3}/4.6 \\cdot 10^{41}
2-0.29/-0.211.3 \\cdot 10^{-7}/1.6 \\cdot 10^{-15}
3-0.79/-1.12< 1.0 \\cdot 10^{-320}/< 1.0 \\cdot 10^{-320}
4-1.47/-1.97< 1.0 \\cdot 10^{-320}/< 1.0 \\cdot 10^{-320}
5-2.02/-1.67< 1.0 \\cdot 10^{-320}/< 1.0 \\cdot 10^{-320}
6-1.55/-1.34< 1.0 \\cdot 10^{-320}/< 1.0 \\cdot 10^{-320}
\n\nTable S22 Logistic regression coefficients and p-values for the effect of GC motif content on polymorphism rate within motif lengths for both the Icelandic and UKB datasets.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif equivalence classRegression \\( \\alpha \\) and (P) for comparison with AC-class mDNM rate
AG-1.20 (<1 · \\( 10^{-320} \\))
AT-1.08 (<1 · \\( 10^{-320} \\))
CG-0.43 (7.7 · \\( 10^{-3} \\))
\n\nTable S23 Regression coefficients and p-values from a Poisson regression comparing the mDNM rate of the other motif equivalence classes to the AC class using available trios per marker as exposure but without correcting for RRT length. All motif classes have significantly lower mDNM rates.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif equivalence classRegression α and (P) for comparison with CG-class mDNM rate
AC-0.81 (5.7 · 10^{-7})
AG-1.48 (1.7 · 10^{-19})
AT-1.18 (5.8 · 10^{-13})
\n\nTable S24 Regression coefficients and p-values from a Poisson regression comparing the mDNM rate of the other motif equivalence classes to the CG class after correcting for RRT length and using available trios per marker as exposure. All motif classes have significantly lower mDNM rates.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif equivalence classRegression α (P) for comparison with AAT mDNM rate
AAC-1.35 (2.7 · 10^{-217})
AAG-1.67 (5.3 · 10^{-75})
ACC-2.99 (5.6 · 10^{-29})
ACG-0.06 (0.92)
ACT-2.49 (3.3 · 10^{-88})
AGC-1.8 (8.6 · 10^{-41})
AGG-3.09(4.9 · 10^{-37})
ATC-1.78 (1.2 · 10^{-120})
CCG-1.14(1.7 · 10^{-11})
\n\nTable S25 Regression coefficients and p-values from a Poisson regression comparing the mDNM rate of the other motif equivalence classes to the AAT class, correcting for RRT length and using available trios per marker as exposure. All motif classes expect for the rarest one (ACG) have significantly lower mDNM rates.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif length (bp)Odds ratio maternal/paternal (95% CI)Fisher exact test \\( P \\)
12.25 (2.14-2.37)2.0 \\cdot 10^{-188}
20.65 (0.62-0.68)6.3 \\cdot 10^{-84}
31.11 (1.03-1.20)1.0 \\cdot 10^{-2}
40.81 (0.77-0.85)4.2 \\cdot 10^{-16}
51.17 (1.03-1.32)1.7 \\cdot 10^{-2}
61.39 (1.03-1.86)3.0 \\cdot 10^{-2}
Motif length (without 1bp)Odds ratio maternal/paternal (95% CI) (no 1 bp)Fisher exact test \\( P \\) (no 1 bp)
20.84 (0.80-0.88)1.0 \\cdot 10^{-11}
31.34 (1.24-1.45)3.3 \\cdot 10^{-12}
41.01 (0.95-1.06)0.78
51.39 (1.22-1.57)6.3 \\cdot 10^{-7}
61.64 (1.21-2.20)1.9 \\cdot 10^{-3}
\n\nTable S26 Per motif length enrichment of mDNMs between maternally and paternally phased mDNMs. Top half shows enrichment including homopolymers and bottom half without them. Tri-, penta- and hexanucleotide repeats are enriched in maternal mDNMs while dinucleotide microsatellites are paternally enriched.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Length threshold (bp)percentage adding bp belowpercentage adding bp above
2059.4%52.1%
3059.6%50.7%
4056.9%49.5%
5054.2%49.9%
6053.5%51.2%
7053.5%50.2%
8053.4%46.2%
9053.4%50.0%
10053.4%42.9%
\n\nTable S27 Fraction of mDNMs adding bp above and below different repeat tract length thresholds. The fraction of mDNMs adding bp is higher below the threshold in all cases.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Detection frequencyDNM rate estimate
9.0 \\cdot 10^{-6}5.0 \\cdot 10^{-5}
7.6 \\cdot 10^{-5}5.6 \\cdot 10^{-5}
1.0 \\cdot 10^{-2}8.1 \\cdot 10^{-5}
5.0 \\cdot 10^{-2}9.3 \\cdot 10^{-5}
0.11.0 \\cdot 10^{-4}
\n\nTable S28 Microsatellite mDNM rate estimates for different detection frequencies, the number of markers included in the analysis depends on the detection frequency defined by the sample size.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Phasing methodPaternal effect\\( P \\)Maternal effect\\( P \\)
Allele based0.17 [0.15;0.18]1.2 \\cdot 10^{-102}0.07 [0.05;0.08]5.1 \\cdot 10^{-16}
Read back0.16 [0.15;0.18]3.6 \\cdot 10^{-101}0.07 [0.06;0.09]7.1 \\cdot 10^{-21}
3 generation0.18 [0.15;0.21]9.8 \\cdot 10^{-34}0.05 [0.03;0.07]1.7 \\cdot 10^{-6}
\n\nTable S29 Poisson regression coefficients and p-values for subsets of phased markers by each method applied. The effects for allele based phasing and read back phasing match but the three generation phasing subset gives a stronger paternal effect and a weaker maternal one.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif length (bp)MaternalPaternalMaternal percentage
12,9625,14136.6%
24,11917,38819.2%
38872,66325.0%
42,3659,18420.5%
534397726.0%
66214829.5%
Total10,73835,50123.2%
\n\nTable S30 Parental ratios of mDNMs stratified on motif length and on the full set.\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Motif length (bp)SharedNot sharedError rate
147611.3%
210865.3%
31615.9%
44400%
5200%
6000%
\n\nTable S31 Sharing of mDNMs between monozygotic twins stratified on motif length.\nAuthor Contributions\nPaper was written by SK, supervised by BVH, with input from HJ, OAS, GAA, UT, TR, DFG and KS. SK, HPE, AG, PIO, GM and BVH developed analysis tools, with input from HJ, OE and DFG. GP performed mDNM enrichment analysis. AG and DB generated SV genotypes. GS performed gene burden test. GH assembled and haplotype tagged PacBio HiFi data. Association analysis was performed by SK, TR and BVH. Age effect regression model was implemented by HJ. SNP mutation signatures were created by SO. SNP genotyping was performed by HPE and PIO. Microsatellite genotyping was performed by SK. Figures were drawn by MTH and SK. Study was supervised by BVH and KS. All authors agreed to the final version of the manuscript."} {"paper_id": "prb74", "title": "SurVIndel2: improving CNVs calling from next-generation sequencing using novel hidden information", "text": "SurVIndel2: improving CNVs calling from next-generation sequencing using novel hidden information\n\nWing-Kin Sung\nkwksung@cuhk.edu.hk\n\nChinese University of Hong Kong https://orcid.org/0000-0001-7806-7086\nRamesh Rajaby\nHong Kong Genome Institute https://orcid.org/0000-0001-9980-1913\n\nArticle\n\nKeywords:\n\nPosted Date: November 29th, 2023\n\nDOI: https://doi.org/10.21203/rs.3.rs-3525542/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nAdditional Declarations: There is NO Competing Interest.\n\nVersion of Record: A version of this preprint was published at Nature Communications on December 2nd, 2024. See the published version at https://doi.org/10.1038/s41467-024-53087-7.\nSurVIndel2: improving CNVs calling from next-generation sequencing using novel hidden information\n\nRamesh Rajaby1,2 and Wing-Kin Sung1,2,3,4,5,*\n\n1Hong Kong Genome Institute, Hong Kong Science Park, Shatin, Hong Kong, China\n2A*STAR Genome Institute of Singapore, 60 Biopolis Street, Singapore 138672, Singapore\n3Department of Chemical Pathology, The Chinese University of Hong Kong, Hong Kong, China\n4Laboratory of Computational Genomics, Li Ka Shing Institute of Health Sciences, The Chinese University of Hong Kong, Hong Kong, China\n5School of Computing, National University of Singapore, 13 Computing Drive, Singapore 117417, Singapore\n*Corresponding author: Wing-Kin Sung, kwksung@cuhk.edu.hk\n\nAbstract\n\nDeletions and tandem duplications (commonly called CNVs) represent the majority of structural variations. They can be identified using short reads, but because they frequently occur in repetitive regions, existing methods fail to detect most of them. This is because CNVs in repetitive regions often do not produce the evidence needed by existing short reads-based callers (split reads, discordant pairs or read depth change). Here, we introduce a new CNV short reads-based caller named SurVIndel2. SurVIndel2 builds on statistical techniques we previously developed, but also employs a novel type of evidence, hidden split reads, that can uncover many CNVs missed by existing algorithms. We use public benchmarks to show that SurVIndel2 outperforms other popular callers, both on human and non-human datasets. Then, we demonstrate the practical utility of the method by generating a catalogue of CNVs for the 1000g project that contains hundreds of thousands of CNVs missing from the most recent public catalogue. We also show that SurVIndel2 is able to complement small indels predicted by Google DeepVariant, and the two software used in tandem produce a remarkably complete catalogue of variants in an individual. Finally, we characterise how the limitations of current sequencing technologies contribute significantly to the missing CNVs.\n1 Introduction\n\nStructural Variations (SVs) are mutations in a genome that involve 50 nucleotides or more. Although they are less frequent than point mutations, SVs account for more heritable differences in populations due to their large scale and play a major role in many genetic diseases [3]. Deletions and tandem duplications are two important classes of SVs. Deletions occur when a contiguous sequence of bases is lost, while tandem duplications occur when a source sequence of DNA is duplicated in-place; they are called unbalanced SVs because they alter the copy number of the genome. A recent study of the SVs in 14,891 human genomes [6] identified deletions as the most frequent SV and tandem duplications as the third most common, after insertions. However, the SVs were detected using short reads, and existing SV callers miss most duplications, as demonstrated in the following sections. When detecting SVs using high-quality long reads, tandem duplications are as common as deletions (Section 2.3). Aside from being an important source of polymorphism, deletions and tandem duplications are implicated in many genetic diseases, such as Smith-Magenis syndrome, Potocki-Lupski syndrome and Williams-Beuren syndrome [11]. Deletions and tandem duplications are often described as *copy number variants* (CNV). In this manuscript, we will refer to them as such.\n\nNowadays, CNVs can be accurately detected using long read sequencing technologies, like PacBio HiFi reads and ONT nanopore reads. However, these technologies are still expensive and this limits their use in large-scale population studies. A less costly solution is to use short-reads sequencing technologies such as Illumina, which is often used for sequencing large populations [6][13]. Short read datasets are rapidly increasing in number, with studies on tens of thousands of genomes already published. As the Hong Kong Genome Project, Singapore SG100K, the European '1+ Million Genomes' Initiative, and the All of Us Research Project (among others) continue to generate large amounts of sequencing data, short-read whole genome sequencing will remain at the forefront of genomics for the foreseeable future.\n\nHowever, detecting deletions and especially tandem duplications from short reads is very challenging. Despite a large number of callers published in the last decade, the sensitivity of even the best methods is still low. Manta, a widely used SV caller employed in many large-scale population studies [6][3], as well as the best performing tool according to recent benchmarking efforts [22][4], detects around 40% of the existing deletions and less than 10% of the existing tandem duplications when tested on a recent benchmark dataset (see Section 2.3).\n\nIn a previous study [18], we found that most of the CNVs missed by existing callers were located in tandem repetitive regions. This is because CNVs in tandem repetitive regions often do not generate split reads; this result was confirmed in this study (Section 2.1). Furthermore, shorter CNVs generate few or no discordant pairs, and read depth methods are known to only work for large CNVs [27]. Thus, naively counting the number of discordant pairs and split reads will miss many CNVs in repetitive regions. Finally, we showed that the problem can be mitigated by considering the insert sizes of all the read pairs containing the putative CNVs, and performing statistical tests to determine whether they deviate from expectation. Using this technique we developed SurVIndel [18], a CNV caller that improved the detection rate in repetitive regions over existing methods.\nHowever, SurVIndel suffered from two problems. First, it generated many false positives. This is a serious issue when generating catalogues of CNVs for large populations. Second, because split reads are often unavailable in repetitive regions, many of the CNVs detected had imprecise boundaries. Subsequent steps in population studies, such as clustering of the CNVs across samples, regenotyping and downstream analysis, all rely and greatly benefit from precise breakpoints.\n\nTo address these issues, we have developed a new caller called SurVIndel2, which significantly reduces the number of false positives while improving the sensitivity of the original SurVIndel. Additionally, SurVIndel2 generates precise breakpoints for most of the called CNVs. This new caller utilizes split reads, discordant pairs, and a novel type of evidence called hidden split reads to detect candidate CNVs. Hidden split reads allow us to identify the existence and the precise breakpoints of CNVs in repetitive regions, which leads to a more accurate and comprehensive set of candidate CNVs. SurVIndel2 then applies the statistical approach of SurVIndel, along with depth-based filters, to generate a set of confident CNVs.\n\nThis paper is organised as follows. In Section 2.1 we introduce the notion of hidden split reads, and we explain why they can improve CNV detection. Section 2.2 gives an overview of the algorithm of SurVIndel2. Sections 2.3 and 2.4 use publicly available datasets, both human and non-human, to compare the performance of SurVIndel2 to the best methods in the literature, according to a recent benchmark [4]. Then, in Section 2.5 we use SurVIndel2 to generate a dataset of deletions and duplications in the 1000 Genomes Project. We show that our dataset is significantly more complete than that produced by a state of the art pipeline: it contains more than twice as many deletions and five times as many duplications, with high validation rates according to long reads. In Section 2.6 we illustrate that SurVIndel2 is also able to effectively call CNVs that are smaller than 50 bp, and it can be used to enhance callsets generated by state-of-the-art small variants callers such as DeepVariant [23]. Finally, in Section 2.7 we investigate why many CNVs are hard to detect, and we reach the surprising conclusion that it is not only due to the repetitive nature of the genome, but mostly due to the sequencing platforms employed being unable to correctly sequence many regions of the genome.\n\nSurVIndel2 is fully open source and available at https://github.com/kensung-lab/SurVIndel2 It is easy to run and only requires a BAM or a CRAM file and a reference genome, and it outputs a fully standard VCF file.\n\n2 Results\n\n2.1 Hidden split reads\n\nLet \\( D \\) be a deleted region in a sample and let \\( L \\) and \\( R \\) be its left and right-flanking regions, respectively. \\( L \\) and \\( R \\) will be adjacent in the sample genome, but not in the reference genome. The concatenation of \\( L \\) and \\( R \\) (we refer to it as \\( LR \\)) is called the junction sequence of the deletion. When the junction sequence is a novel sequence, i.e., it is not present in the reference genome, the reads sequenced from it will be “split”, meaning that a portion of the read will align to \\( L \\) and the rest will align to \\( R \\). Split reads are commonly used to detect deletions. Fig.1 shows an example of\nFigure 1: (a) The red segment (\\( D \\)) of the reference is deleted in the sample, causing the green (\\( L \\)) and the blue (\\( R \\)) regions to be adjacent. Reads sequenced partly from the \\( L \\) and partly from \\( R \\) may not fully align to the reference, causing the read to be clipped. (b) Similarly, tandem duplications may also create clipped reads. (c) When the prefixes (circled) of \\( D \\) and \\( R \\) are homologous, many reads sequenced across the breakpoint of the deletion will fully align to the reference, instead of being clipped. If the length of the prefixes is longer than the read length, no clipped reads will be produced. (d) Similarly, when the suffixes of \\( D \\) and \\( L \\) are homologous, little or no clipped reads will be produced. (e) Deletions of full copies in tandem repeats are a prime example of (c), which is why they often do not cause clipped reads. However, in practice, different copies of a tandem repeat are often not identical, and we may get hidden split reads. In this example, a sequence (white) is repeated twice in the reference, but only once in the sample. The two copies of the sequence are identical except for one position (first copy has a T, the second has an A). The single copy in the sample has an A, therefore we want to report that the first copy was deleted. Reads spanning both the green left-flanking region and the A character can be aligned to the reference in two ways: fully with one mismatch, or explicitly clipped. Aligners will normally choose the former. While this is usually a reasonable choice, in this case it will hide the existence of the deletion. We call such reads hidden split reads.\n\n![Diagram showing deletion and duplication scenarios in sequencing reads](page_324_678_1096_355.png)\na deletion creating a split read. Similarly, tandem duplications may also produce split reads (Fig. 1b).\n\nSome deletions will not produce split reads. One reason for this is that the junction sequence is not novel. For example, if a sufficiently long prefix of \\( D \\) is homologous to a prefix of \\( R \\), the deletion will not create split reads (Fig. 1f). Similarly, when a suffix of \\( D \\) is homologous to a suffix of \\( L \\), no split reads will support the deletion (Fig. 1d). Tandem repeats are common examples of this.\n\nWe have a tandem repeat when a sequence (\\( repeat\\ unit \\)) appears consecutively multiple times. Deletions and duplications of entire repeat units often do not create split reads [18]: because \\( L, R \\) and \\( D \\) are identical, the junction sequence \\( LR \\) will be identical to \\( LD \\) and to \\( DR \\), so any read sequenced from \\( LR \\) will fully align to either \\( LD \\) or \\( DR \\) (Supplementary Fig. S2h).\n\nHowever, in practice, the copies in a tandem repeat may present some differences between each other. Suppose \\( D \\) and \\( R \\) are similar but not identical, and let \\( r \\) be a read sequenced from \\( LR \\). The algorithm that aligns \\( r \\) to the reference genome has two choices:\n\n1. split \\( r \\) between \\( L \\) and \\( R \\), obtaining two (partial) perfect alignments; or\n2. align \\( r \\) fully to either \\( LD \\) or \\( DR \\), accepting mismatches or gaps in the alignment.\n\nWhich option the aligner chooses depends on many factors, including the mapping algorithm used, its parameters and how similar \\( L, D \\) and \\( R \\) are. The more different they are, the more likely option 1 will be chosen. When option 2 is chosen, we say that \\( R \\) is a hidden split read (see Fig. 1e for an example). Similarly, tandem duplications may also produce hidden split reads (Supplementary Fig. S3b).\n\nNext, we provide a formal definition of hidden split read. Given a genomic fragment \\( s \\), let \\( score(s) \\) be the score of the alignment of \\( s \\) to the reference genome. Given a read \\( r[1..n] \\), we say that \\( r \\) is a hidden split read if there exists \\( i \\in [1..n-1] \\) such that \\( score(r) < score(r[1..i]) + score(r[i+1..n]) \\); in other words, if \\( r \\) is allowed to split into two without penalty and the two parts can align independently, the score of the alignment will increase. \\( score(r[1..i]) + score(r[i+1..n]) - score(r) \\) is the HSR-score of \\( r \\). See Supplementary Fig. S5f for an example of HSR-score calculation.\n\nIn order to confirm that CNVs mostly delete or insert full repeat units and the importance of hidden split reads in detecting such CNVs, we use two publicly available human genomes: HG002 and HG00512. A detailed explanation of the data used and the experiments mentioned below is provided in the Supplementary Methods.\n\nAround 64% of the deletions and 93% of the tandem duplications in HG002 (Fig. 2a) are located in tandem repetitive regions. Fig. 2b demonstrates that indeed most CNVs delete or insert an integer number of repeat units. For this reason, the number of CNVs in tandem repeats supported by split reads is low. Only 25.2% of the deletions and 29.0% of the duplications in tandem repeats were supported by split reads, compared to 90.2% and 83.3%, respectively, for deletions and duplications not in tandem repeats (Fig. 2c, Fig. 2d). However, hidden split reads can help us uncover a significant number of CNVs not supported by split reads. Using both split reads and hidden split reads, the number of deletions in tandem repeats that we are potentially able to discover is more than double (25.2% using split reads, 58.9% using both split reads and hidden\nsplit reads, \\(2.3 \\times\\)). We obtain similar figures for duplications (29.0% using split reads, 63.7% using both split reads and hidden split reads, \\(2.2 \\times\\)). Supplementary Fig. S6 shows that the statistics are virtually identical for HG00512.\n\nAlthough hidden split reads have the potential to identify a substantial portion of repetitive CNVs that are typically missed by traditional split-read methods, their use presents significant challenges. Fig. 2 shows the binned HSR-score distribution for hidden split reads that support CNVs in HG002. Most hidden split reads have low HSR-score. Fig. 2 shows that most CNVs detected by realigning hidden split reads are actually noise. Interestingly, reads with high HSR-score do not produce significantly less false positives, in relative terms. Distinguishing hidden split reads that support existing CNVs is not trivial, and novel and sophisticated techniques need to be developed. In the remainder of this paper, we propose an algorithm that uses hidden split reads to detect deletions and duplications in a sample genome, and significantly outperforms the current state of the art.\n\n2.2 Overview of the method\n\nSurVIndel2 requires (1) a reference genome (in FASTA format) and (2) a BAM or CRAM alignment file containing paired reads sequenced from a single sample aligned to the reference genome. It outputs a VCF file containing a list of predicted deletions and tandem duplications. Fig. 3 shows a high-level overview of the full algorithm. Detailed explanations and examples for individual steps are provided in Supplementary Methods.\n\nAs a first step, SurVIndel2 iterates through the alignment file and gathers the evidence that will be later used to determine the candidate CNVs: split reads, hidden split reads and discordant pairs. Split reads and hidden split reads were described in Section 2.1. SurVIndel2 considers potential hidden split reads to be all the reads that are not clipped and present at least three differences with the reference genome (defined as number of mismatches plus number of indels). Discordant read pairs are pairs of reads that map inconsistently to the library preparation parameters. A deletion may produce pairs where the two reads map very far apart (Fig. S15). Let \\( \\mu \\) and \\( \\sigma \\) be the mean and the standard deviation of the distribution of insert sizes for the library: we define as discordant any pair that has insert size greater than \\( \\mu + 3\\sigma \\) (we will refer to this quantity as \\( maxIS \\) throughout the paper). On the other hand, a duplication may produce pairs that have the wrong relative orientation, i.e., the forward-facing read is mapped downstream of the reverse-complemented read (Fig. S15b). We define such pairs as discordant.\n\nGiven the split reads, hidden split reads and discordant pairs, candidate CNVs are generated by two different modules: the split module uses split reads and hidden split reads, while the discordant module uses discordant pairs. Then, we calculate a set of features for each putative CNV, such as the number of supporting split and hidden split reads, their mapping quality, the number of discordant and concordant pairs, alignment score of the junction sequence when realigned to the reference, depth of the CNV and flanking regions, and others (Fig 3). Additionally, we use the distribution of the insert sizes of the read pairs around the CNV to calculate a confidence interval for its size, as well as a p-value estimating the probability that the CNV is a false positive. Such features were first\nFigure 2: The impact of CNVs deleting or duplicating full repeat units and the importance of hidden split reads in detecting such CNVs, studied on HG002. (a) We consider a CNV to be contained in a tandem repeat if at least 90% of the CNV is covered by the repetitive region. Nearly two thirds of the deletions and more than 93% of the tandem duplications in this dataset are contained in a tandem repeat. (b) For every CNV that overlaps with a tandem repeat, we calculated the number of repeat units that are deleted or inserted, by dividing the length of the CNV by the length of the repeat unit. Bars representing an integer number of copies (i.e., the length of the CNV is a multiple of the length of the repeat unit) are coloured red. Most CNVs add or delete an integer number of repeat units. (c,d) Number of deletions (c) and tandem duplications (d) inside and outside of tandem repeats that are supported by split reads (SR), by hidden split reads (HSR), and by neither. Hidden split reads have the potential to recover a significant number of deletions and duplications missed by regular split reads. (e) HSR-scores of the hidden split reads supporting the existing CNVs in HG002. Most reads have low (<20) HSR-score. (f) We found all hidden split reads in 10,000 randomly sampled repetitive regions, and for each we tried to predict a CNV by finding the optimal split alignment. Most CNVs (>91%) detected this way were false positive. This shows that using hidden split reads to detect CNVs is challenging, and effective filters must be employed to distinguish real from false CNVs.\nFigure 3: Overview of the SurVIndel2 method. It primarily identifies candidate CNVs by using split reads and hidden split reads. Candidate CNVs that do not generate clipped reads are identified using discordant pairs. Finally, the candidate CNVs are tested by a series of filters, mainly (i) statistically testing the distribution of the read pairs surrounding the CNV and (ii) testing changes in read depth in the CNV region as well as its flanking regions.\n\nintroduced by SurVIndel [15]. Finally, all of the features are used in the filtering step (Fig. 3f), which aims at removing most false positives, while retaining the correct CNVs. In order to do so, it uses a pre-trained random forest. If a pre-trained forest is not available, a set of fixed hard filters are used. Below, we explain how the split and the discordant modules find candidate CNVs.\n\nThe split module first generates consensus sequences by clustering left-clipped reads and hidden split reads into left-clipped consensus sequences and right-clipped reads and hidden split reads into right-clipped sequences (Fig. 3a, 3b). The consensus sequences are partitioned into left and right-clipped. Consensus sequences in each group potentially represents either the left or the right breakpoint of a CNV: furthermore, using the mates of the clustered reads, we can calculate a putative range for the location of the second breakpoint (Fig. S1): we call this range opposite breakpoint range. We pair the consensuses so that each pair contains a left-clipped and a right-clipped consensus, and the consensuses are within each other’s opposite breakpoint range (Fig. 3c). For each pair we generate a junction sequence by overlapping the left-clipped and right-clipped consensuses. The junction sequence is expected to be the DNA sequence at the precise junction where two different genomic regions have been joined together as a result of the variant (the left and right-flanking regions for deletions, the two copies of the duplicated region for tandem duplications, examples in Fig. 1a and Fig. 1b). For consensuses that are not paired, we attempt generate the junction sequence by extending them using an overlap-layout-consensus approach (Fig. 3d). Finally we realign the junction sequence to the reference genome to obtain the precise breakpoints of the CNV (Fig.3e).\nThe discordant module is considerably simpler, and it clusters discordant pairs in order to detect CNVs (Fig.3). One drawback is that, unlike split reads, discordant pairs often provide an approximate position for the breakpoints, rather than a precise one. When the same CNV is predicted by both the split module and the discordant module, the coordinates from the split module are retained, since they are deemed precise.\n\n2.3 HGSVC2 benchmark\n\nAs mentioned in Section 2.1, the Human Genome Structural Variation Consortium (HGSVC) has published a catalogue (called HGSVC2) of insertions and deletions in 35 human genomes (34 from the 1000 genomes project, plus HG002), identified from long-read PacBio whole-genome sequencing and Strand-seq data [7]. Furthermore, the New York Genome Center (NYGC) has recently performed high-coverage, PCR-free sequencing for the 2,504 original samples in the 1000g genome project, along with 698 additional samples. We downloaded the CRAM files published by NYGC for the 34 samples in the HGSVC2 benchmark (30x coverage, except for one sample which had 60x coverage). We also obtained a 50x short-read dataset for HG002 by downloading runs from SRR1766442 to SRR1766486, and mapping them to hg38 using BWA-MEM. We use these datasets to benchmark the performance of SurVIndel2, and three highly cited methods that performed well in a recent benchmarking analysis [4]: Delly [19], Lumpy [12] (which we ran using the Smoove package, as recommended by the authors) and Manta [5]. These SV callers were used in some of the major studies on SVs in human populations [6][1][3]. We also included the original SurVIndel [18] in the comparison. Note that the callers may report some of the duplications as insertions. For this reason, the sensitivity for each caller was evaluated using both the duplications and the insertions. Precision was only computed on the duplications.\n\nThe machine learning model of SurVIndel2 was trained using the 34 samples in HGSVC2 sampled by the NYGC. For this reason, when testing them, we use a leave-one-out strategy. More precisely, for each sample S in HGSVC2 we train a separate model by excluding S from the training set, and we use it to filter the raw calls by SurVIndel2 detected from S.\n\nSurVIndel2 outperforms the other methods in both deletions and duplications, often by a large margin (Fig. 4 and Fig. 5.). For deletions, Manta is the only method that almost matches SurVIndel2 precision (average precision is 0.84 for Manta, 0.87 for SurVIndel2), but at the expense of greatly reduced sensitivity (average sensitivity is 0.41 for Manta, 0.60 for SurVIndel2, 46% increase). SurVIndel is the second most sensitive method (0.5 average sensitivity and average precision 0.57), but it is considerably less precise than both Manta and SurVIndel2.\n\nTandem duplications are far more difficult to predict than deletions using short reads. SurVIndel2 is the most sensitive and precise method (average sensitivity 0.35 and average precision 0.8). The next best method in term of sensitivity is SurVIndel (average sensitivity 0.3 and average precision 0.3). The next best method in term of precision is Manta (average sensitivity 0.1 and average precision 0.53)\n\nThe datasets used for training the model are very homogeneous: they were all sequenced by one sequencing center (NYGC), with the same platform (Illumina NovaSeq 6000), with the same sequencing depth (30x, except for one which was 60x), which can lead to overfitting. However, the HG002 sample confirms that this is not the case for our model. HG002\nFigure 4: Sensitivity and precision for deletions (a) and tandem duplications (b) on the in the HGSVC2 catalogue. Each sample is a dot, its x coordinate is the sensitivity while its y coordinate is the precision. SurVIndel2 has higher sensitivity and precision than the other methods. (c) Sensitivity of the methods in predicting deletions in HG002, stratified by supporting evidence. Split reads (SR)-supported deletions are relatively easy for all methods, although SurVIndel2 has a clear advantage. However, SurVIndel2 is the only method that can detect most deletions with strong HSR support. (d) For tandem duplications, existing methods perform poorly even for SR-supported events. SurVIndel2 can detect nearly twice as many duplications as existing methods that are supported by split and hidden split reads.\nwas sequenced by a different entity (GIAB Consortium) using a different platform (Illumina HiSeq 2500) and its depth is different (50×). SurVIndel2 performs just as well on it; sensitivity and precision were 0.64 and 0.84 for deletions, 0.37 and 0.76 for duplications.\n\nIn Section [2.1] we have partitioned the CNVs in HG002 depending on whether they were supported by split reads, hidden split reads, or unsupported. In order to maintain a high precision, our algorithm only considers HSRs that have at least three differences with the reference genome (an indel or a mismatch relative to the reference is counted as one difference, see Supplementary Methods). Let us call such HSRs as strong HSRs. Therefore, we expect that SurVIndel2 will be able to detect HSR-supported CNVs that have good support from strong HSRs, but not the rest. To study this, we partition HSR-supported CNVs into two categories: CNVs with strong HSR support (supported by at least 5 strong HSRs) and with weak HSR support (supported by less than 5 strong HSRs). 53% and 67% of the HSR-supported deletions and duplications, respectively, have strong HSR support.\n\nAll tested methods tend to perform well in detecting deletions that are supported by split reads (Fig. [4]). SurVIndel2 detects nearly all true positive deletions in this category (0.97 sensitivity). As expected, SurVIndel2 has a large advantage over the other methods in finding deletions supported by strong HSRs (0.74 sensitivity for SurVIndel2, 0.39 for SurVIndel). Predictably, detection power drops for deletions with weak or no support, although SurVIndel2 and the original SurVIndel are still the most sensitive methods.\n\nSurprisingly, SurVIndel2 has a large advantage not only for tandem duplications supported by strong HSRs, but also for those supported by split reads (Fig. [4]). Methods other than SurVIndel and SurVIndel2 are essentially unable to call duplications not supported by split reads, which explains their poor sensitivity.\n\nWe observed from Fig. [2] and Fig. [2] that CNVs outside of repetitive regions are more likely to be supported by split reads, while the CNVs within repetitive regions are mostly supported by hidden split reads or they are unsupported. The proportion of split reads support, hidden split reads support and no support in repetitive regions is similar between deletions and duplications; however, because a much larger proportion of duplications is within repetitive regions (Fig. [2]: 64% of deletions and 93% of duplications are in tandem duplication regions), it follows that a larger portion of duplications is not supported by split reads compared to deletions. This might explain, together with our observations from Section [2.7] why tandem duplications are so difficult to call compared to deletions.\n\n2.4 Performance on different organisms\n\nThe filtering model we provide was trained on the CNVs called from the 34 human samples. We call this the default model. For this reason, we are interested in (i) how SurVIndel2 performs on different organisms using the default model and (ii) what are the implications on the sensitivity and precision of the method if a more targeted training set is used (i.e., the model is retrained using data from the target organism). To address these questions, we conducted an analysis by running the callers on seven Arabidopsis thaliana samples that were sequenced as part of the 1001 Genomes Project. These samples were mapped to the TAIR10 reference\nFigure 5: (a) Sensitivity and precision for deletions (left) and tandem duplications (right) in the Arabidopsis Thaliana benchmark. Unsurprisingly, the A. Thaliana-trained SurVIndel2 performs the best; however, the human-trained SurVIndel2 still performs better than the existing methods. (b) F1-score for deletions (left) and duplications (right) for five non-human libraries: two bos taurus (Cattle LIB1 and Cattle LIB2), one mus musculus (Mouse) and two oryza sativa (Rice Minghui 63 and Rice Zhenshan 97). Benchmark catalogues were obtained by running Sniffles2 on PacBio HiFi reads. SurVIndel2 performs better for every organism. The advantage is particularly evident for tandem duplications. SurVIndel failed to run for the two Cattle libraries.\n\ngenome. We generated a benchmark dataset by using Sniffles2 [24] on PacBio HiFi reads for the same samples. For SurVIndel2, we used two classification models: one trained on the 34 human samples with long reads in the 1000 Genome Project (Section 2.3), and one trained on the seven A. Thaliana using a leave-one-out cross-validation (i.e., when classifying sample S, sample S is excluded from the training set).\n\nSurVIndel2 outperforms all of the existing methods (Fig. 5). Two key points that must be noted are a) when trained on A. Thaliana data, SurVIndel2 shows noticeably improved performance in calling A. Thaliana CNVs compared to when trained on human data and b) SurVIndel2 trained on human data still outperforms existing methods. This means that if a reliable catalogue of CNVs (i.e., obtained from long reads) is available for the target organism, it is possible to increase the performance of SurVIndel2; however, if such catalogue is not available, the default model works well.\n\nWe also selected samples of other species (bos taurus [8], mus musculus [16] and oryza sativa [30, 25]) for which both Illumina paired reads and PacBio HiFi reads were available. All of the selected organisms are\nFigure 6: (a,b) Count of deletions and duplications in different superpopulations. Africans have more deletions and duplications compared to non-Africans: the median count was 7,509 deletions and 5,129 duplications for Africans vs 6,294 deletions and 4,478 duplications for non-Africans. (c) The size distribution for deletions and duplications detected in 1000g, adjusted by their frequency in the population. For deletions, the expected peaks associated with ALU (~310bp) and LINE (~6000bp) deletions are visible. (d) PCA is able to clearly separate the superpopulations.\n\nimportant either as food sources or as model organisms. Once again, SurVIndel2 has the best performance for every sample, both for deletions and duplications (Fig. 5b). We expect that the performance would be even better if the model was trained for the specific organism, as in the case of A. Thaliana.\n\n2.5 A catalogue of deletions and tandem duplications for the 3,202 genomes in the 1000 genomes project\n\nWe used SurVIndel2 to generate a catalogue of deletions and tandem duplications for 3,202 samples from the 1000g genomes project sequenced by the NYGC. SurVIndel2 was run on each individual sample, and the calls were left-aligned and clustered across samples (Supplementary Methods). The final catalogue contained 247,822 deletions and 232,227 tandem duplications. 205,258 deletions (82.8%) and 189,413 duplications (81.6%) were rare (detected in 1% of the population or less), and 90,137 deletions (36.4%) and 74,369 duplications (32.0%) were singletons (detected in only one individual). Africans had more deletions (Fig. 6b) and duplications\nFigure 7: Comparison between the 1000g-SV and SurVIndel2 datasets. (a,b) Sensitivity and the precision for the 34 samples in HGSCVC2 for deletions (a) and tandem duplications (b). The dataset produced by SurVIndel2 is both more sensitive and more precise than the 1000g-SV dataset. (c) Overlap between deletions in 1000g-SV and SurVIndel2 datasets. Between parentheses, the validation rates of calls in samples with long reads. Not only SurVIndel2 covers nearly all of the deletions in 1000g-SV, but it predicts 130,657 deletions that are not present in the latter. The validation rate for SurVIndel2-unique events is far higher than the validation rate of 1000g-SV unique events. (d) Similarly, SurVIndel2 predicts a large portion of the tandem duplications in 1000g-SV, and the ones that are not predicted have very low validation rate. SurVIndel2 also predicts 197,008 duplications that are not present in 1000g-SV, with high validation rate.\n\n(Fig. 6b) compared to non-Africans: the median count was 7,509 deletions and 5,129 duplications for Africans vs 6,294 deletions and 4,478 duplications for non-Africans. The number of events was similar in the remaining superpopulations. Fig. 6 shows the size distribution for the deletions and duplications predicted. The peaks associated with ALU (~310 bp) and LINE (~6 kbp) deletions are clearly visible. PCA is able to separate the superpopulations (Fig. 8f). This is also true when performing the PCA using deletions and tandem duplications separately (Fig. S16). Furthermore, PCA was able to segregate the superpopulations into subpopulation (Fig. S17).\n\nThe NYGC also generated a catalogue of SVs (including deletions and tandem duplications) [3] by integrating multiple callers, including Manta. We refer to this catalogue as 1000g-SV. Fig. 7 shows a comparison between 1000g-SV and our catalogue. Similarly to Section 2.3 we measured sensitivity and precision for 1000g-SV and for SurVIndel2 on the 34 samples in HGSCVC2. SurVIndel2 had consistently higher sensitivity and precision. For deletions (Fig. 7a), SurVIndel2 was on average nearly twice as sensitive (average sensitivity was 0.345 for 1000g-SV and 0.60\nfor SurVIndel2), while being more precise (average precision was 0.78 for 1000g-SV and 0.87 for SurVIndel2). For tandem duplications (Fig. 7b), SurVIndel2 was more than 4× more sensitive (average sensitivity was 0.084 for 1000g-SV and 0.35 for SurVIndel2) and significantly more precise (0.55 for 1000g-SV, 0.80 for SurVIndel2). When comparing the full catalogues (Fig. 7f; 7h), SurVIndel2 captures the vast majority of the deletions in 1000g-SV, and deletions in 1000g-SV but not predicted by SurVIndel2 have low validation rate according to HGSVc2 (0.14). Furthermore, SurVIndel2 predicts 130,657 deletions not present in 1000g-SV, with high validation rate (0.87). The difference in detected tandem duplications is even more striking. Duplications predicted by 1000g-SV but not by SurVIndel2 have again very low validation rate (0.19). The two datasets share 35,219 duplications, and SurVIndel2 predicts an additional 197,008 duplications, with high validation rate (0.85). Overall, it appears that SurVIndel2 is able to predict a more accurate and significantly more complete catalogue of both deletions and tandem duplications.\n\n2.6 SurVIndel2 enhances small indels callers\n\nAlthough SurVIndel2 was developed and tuned to detect SVs (\\( \\geq 50 \\) bp), its approach is theoretically able to recover some of the smaller indels, as long as they produce a sufficient number of split or hidden split reads. Therefore, we investigated whether SurVIndel2 is able to complement and complete the calls provided by DeepVariant, since it has been found the best-performing tool for small indels [20][11]. We focused on indels of size between 30 and 50 bp, since smaller indels are unlikely to generate enough evidence for SurVIndel2 to use.\n\nIn order to measure the sensitivity of the methods, we use the benchmark catalogue for small indels provided by HGSVC2. However, we noticed that this benchmark underestimates the precision of the methods. Upon manual inspection using PacBio HiFi reads and IGV [21], most of the calls by DeepVariant or SurVIndel2 that were missing from the benchmark were clearly supported by the long reads. For this reason, in order to more accurately measure precision, we created a more complete benchmark for both HG00512 and HG002 by concatenating three callsets: i) HGSVC2; ii) Sniffles2 calls on PacBio HiFi reads and iii) DeepVariant calls on PacBio HiFi reads.\n\nFig. 8 and Supplementary Fig. S18 illustrate the improved sensitivity achieved by using both DeepVariant and SurVIndel2 for the detection of deletions. On average, the sensitivity for DeepVariant alone was 0.6, whereas this increased to 0.71 when SurVIndel2 was added. This increase was not at the expense of precision, which stayed the same (0.97).\n\nThe improvement in sensitivity was even more pronounced for small insertions (Fig. 8): by adding SurVIndel2 the average sensitivity increased from 0.38 to 0.52. There was an apparent decrease in precision, from 0.99 with DeepVariant alone to 0.93 when combined with SurVIndel2 for HG00512, and from 0.97 to 0.92 for HG002. However, upon manual inspection of PacBio HiFi reads using IGV, we noticed that a significant portion of the insertions marked as false positives had clear support from the alignment of the reads. In particular, we randomly selected 30 examples of insertions marked as false positives in HG00512, and for 15 of them (50%) the HiFi long reads supported the presence of an insertion (IGV views available for all 30 in Data Availability). Similarly for HG002, 17 out of 30 (57%) of the apparent false positive had clear support from\nFigure 8: SurVIndel2 recovers small indels (30 to 50 bp) missed by DeepVariant. a) By using both DeepVariant and SurVIndel2, we are able to recover more true positive small deletions compared to using DeepVariant alone (average sensitivity was 0.6 for DeepVariant, 0.71 for DeepVariant plus SurVIndel2). The precision was not changed (0.97 for both). b) The increase in sensitivity was even greater for small insertions. The average sensitivity for DeepVariant was 0.38, which increased to 0.52 when introducing SurVIndel2. Precision apparently decreased from 0.99 to 0.93; however, when manually examining 30 random calls marked as true positives, 15 of them showed clear support from PacBio HiFi reads. Therefore, the projected precision of DeepVariant plus SurVIndel2 is 0.975. Supplementary Fig. S18 and S19 show the sensitivity for all 35 samples in HGSV2C.\n\nthe HiFi long reads (IGV views available for all 30 in Data Availability). Consequently, the projected precision for the DeepVariant and SurVIndel2 combination is recalibrated to be approximately 0.975 for HG00512 and 0.966 for HG002, which suggests that the decrease in precision was far more modest than it initially appeared.\n\nOverall, our findings indicate that the integration of SurVIndel2 with DeepVariant can provide a remarkably sensitive and precise catalogue of variants for an individual, from very small to very large, far more complete than what was possible without SurVIndel2.\n\n2.7 Reasons for unsupported CNVs\n\nMany existing CNVs have no support. In particular, in Fig. 2j and Fig. 2l we showed that 41% of deletions and 36% of duplications in tandem repetitive regions in HG002 have no sufficient support from split and hidden split reads. We will refer to them as *unsupported CNVs*. This section aims to find the reasons behind the lack of supporting reads for unsupported\nCNVs.\n\nAs mentioned in Section[2.1], we expect that the major cause of unsupported CNV is that the sequences flanking the junction sequence created by the CNV (deletion or duplication) is not a novel sequence. Every read sequenced from such junction sequence will perfectly align to the reference genome, hence it will not support the existence of a CNV. This scenario is illustrated in Fig. [I] and Fig. [II].\n\nTo formalise this notion, we present a probability measure for each CNV, which we call the expected support (ES) score. The ES score for a CNV represents the likelihood that a read which contains a breakpoint of the CNV will provide evidence for the presence of the CNV when it is aligned to the reference sequence (i.e., it will be a split or a hidden split read). When ES is 0, we do not expect any read to support the CNV, while a ES of 1 means that we expect every read containing a breakpoint to support the CNV. The calculation of the ES value is described in Supplementary Methods. We expect that most unsupported CNVs will be due to a very low ES score.\n\nA large portion of the unsupported deletions in HG002 does indeed have low ES score (Fig. [9], left), while supported deletions tend to have much higher ES values (Fig. [9], right). However, more than 40% of the unsupported deletions have high ES (\\( \\geq 0.5 \\)), which suggests that a low ES is not the only reason for lack of support. We found that many deletions are unsupported because the reads sequenced from the breakpoint region are very low in quality. Supplementary Fig. [S7] and [S8] show examples of such deletions.\n\nTo demonstrate how common this issue is, we built high-quality alternative alleles for a subset of CNVs in HG002 (Supplementary Methods). Then, we used BWA MEM to map the paired reads of HG002 (Illumina HiSeq 2500) to the alternative alleles, and, for each CNV, we counted the reads correctly sequenced (i.e., without mismatches or indel) that contain a breakpoint. Given that the dataset has a coverage of about 50x, we expect the number of reads covering the breakpoint of the deletion to be around 25 for a heterozygous deletion and 50 for a homozygous one. Fig. [D] shows that unsupported deletions with high ES tend to have fewer reads covering the breakpoint than expected: 91% of them have < 10 reads, and 64% have < 5. Conversely, supported deletions tend to have more reads containing the breakpoints (average 18.4 for supported high ES deletions, 3.7 for unsupported high ES deletions). Therefore, two ingredients determine the level of support for a deletion: the ES score, and the number of reads that contain the breakpoint.\n\nSurprisingly, unlike unsupported deletions, we observed that most unsupported tandem duplications (77%) have high ES score (Fig. [10]). Only 16% have low ES score. In fact, excluding the very low ES values (0-0.1), the distribution of ES score is similar between unsupported (left) and supported (right) duplications. The issue of poorly sequenced breakpoint regions is even more prevalent in duplications than it is in deletions: 96% have < 10 reads, and 85% have < 5. As for deletions, supported duplications tend to have a much higher number of reads containing a breakpoint (average 16.6 for supported high ES duplications, 1.6 for unsupported high ES duplications).\n\nRepeating these experiments on the HG00512 sample sequenced by the NYGC using a different platform (Illumina NovaSeq 6000) yields the same conclusions (Supplementary Fig. [S9] and [S10]. These experiments demonstrate that there is a serious issue in sequencing a large number\nof the regions containing CNVs, and variant calling is unlikely to further improve significantly unless such issues are mitigated.\n\nTo reinforce our hypothesis, we create a synthetic dataset for HG002, which we refer to as HG002-SIM, that closely resembles actual sequencing data but does not have the issue of poorly sequenced regions. We achieve this by using the ART read simulator [10] to simulate an Illumina HiSeq 2500 50x dataset from a high-quality HG002 T2T assembly [29, 20]. The results match out expectations: nearly all unsupported deletions and duplications have low ES (Supplementary Fig. S11, S12), and their number is greatly reduced. For this reason the sensitivity of SurVIndel2 is noticeably higher on the synthetic dataset, especially for duplications (Supplementary Fig. S13 and S14).\n\nIn conclusion, our findings reveal that lack of evidence for the existing CNVs is only partially due to the regions containing the CNVs being very repetitive: another major reason is that the sequencing of many such regions is extremely noisy. This seems to be especially true for regions prone to tandem duplications. We have shown through a realistic synthetic dataset that without this issue, the number of CNVs detectable using short reads would be much higher.\n\n3 Discussion\n\nExisting CNV callers rely on read depth, split reads and discordant pairs when detecting CNVs from short reads. In this paper, we described how CNVs in repetitive regions often do not generate such evidence. For this reason, we introduced a new type of evidence, called hidden split reads. By using it, we are potentially able to discover more than double the number of deletions and duplications compared to only using split reads. From this observation, we developed SurVIndel2, a CNV caller that uses split reads and discordant pairs as well as hidden split reads to produce a comprehensive set of candidate CNVs. SurVIndel2 borrows the idea of statistical testing from its predecessor, SurVIndel, and uses it in a machine-learning filtering algorithm to produce a comprehensive and accurate catalogue of CNVs.\n\nWe used publicly available benchmarks to show that SurVIndel2 outperforms the state of the art in CNV calling. On the HGSVC2 benchmark, a comprehensive catalogue of the CNVs in 35 human samples, SurVIndel2 was the most sensitive and precise caller for both deletions and duplications, often by a large margin. The improvements were particularly large for duplications, since all of the existing methods had either very low sensitivity or very low precision.\n\nOur machine learning filtering was trained on human data, so we were interested in two key questions: how does it performs on non-human data, and is it possible to improve the performance by training for the target organism. We investigated this using a variety of different organisms, and we learned that (i) the human model works well for every tested organism and (ii) the performance increase even further when the model is trained for the specific organism.\n\nTo demonstrate how SurVIndel2 is useful in practice, we used it to generate a catalogue of deletions and tandem duplications for the 1000 Genome Project, and compared it to a recently published catalogue generated using state-of-the-art pipelines. Our catalogue revealed hundreds of thousands of events that were not present in the existing one, and the\nFigure 9: Factors that contribute to absence of support for deletions in HG002. a) As expected, a large portion of unsupported deletions have low expected support (ES) score (left). ES score is the probability that a read containing the breakpoint of the deletion will support its existence, i.e., it will be either a split or a hidden split read. On the other hand, most deletions with support have very high ES score (right). However, a low ES score is not the only factor that contributes to lack of support: more than 40% of the unsupported deletions have ES score \\( \\geq 0.5 \\). b) Another factor is a lack of correctly sequenced reads containing the breakpoint of the deletions. For each deletion with a high quality alternative allele (Supplementary Methods), we mapped the short reads of HG002 to the alternative allele and counted the reads correctly sequenced (i.e., without mismatches or indels) and containing the deletion breakpoint. We further stratified the deletions into low ES (\\( < 0.3 \\)), medium ES (\\( \\geq 0.3 \\) and \\( < 0.5 \\)) and high ES (\\( \\geq 0.5 \\)). High ES unsupported deletions (left) tend to have very few or no reads correctly sequenced that contain the breakpoint, while deletions with a higher number of reads containing the breakpoint have low ES. Supported deletions (right), on the other hand, have both ingredients necessary for support: reads containing the breakpoint, and high ES.\nFigure 10: Factors that contribute to absence of support for duplications in HG002. a) Surprisingly, only 16% of the unsupported duplications (left) have low ES (< 0.3). Most unsupported duplications (77%) have high ES (\\( \\geq 0.5 \\)). Supported duplications also have high ES, as expected (right). b) The effect of poorly sequenced regions is even more dramatic on tandem duplications than it is on deletions. Despite the high ES, most unsupported sequences have very few or no reads containing a breakpoint.\nlong read-based validation rates for those events were high. We expect that SurVIndel2 will be beneficial to the community, and will help uncover a large number of CNVs that would be missed by using existing tools, while maintaining the number of false positives to a minimum.\n\nWe also examined the ability of SurVIndel2 to complement small variant callers, in particular DeepVariant. Our findings indicate that incorporating SurVIndel2 with DeepVariant significantly improved the sensitivity for both deletions and small insertions detection. Notably, this increase in sensitivity did not compromise precision. Using DeepVariant with SurVIndel2 provides a view of the full spectrum of variants in an individual, from small to large, that is more precise and complete than what was previously possible.\n\nFinally, we investigated why a large portion of CNVs lacked support from both split and hidden split reads. We found that the reads in the breakpoint regions of many CNVs were extremely noisy, and for many CNVs not a single correctly sequenced reads contained a breakpoint. This was especially serious for tandem duplications, and we have also shown by simulation that if this issue was not present, the number of true positive duplications predicted would greatly increase. Although it is known that some genomic regions are difficult to sequence, this was the first study, to our knowledge, that systematically investigated the magnitude of the problem and its impact on CNV calling.\n\n4 Data availability\n\nThe CNVs catalogue produced by SurVIndel2 for the 1000g project is available at: http://ramesh-research.s3.ap-east-1.amazonaws.com/public/1000g-CNv.vcf.gz\n\nThe IGV screenshot for manual validation of 60 reported false positive small CNVs (30 in HG002 and 30 in HG00512) is available at: http://ramesh-research.s3.ap-east-1.amazonaws.com/public/validation-screenshots.zip\n\nReferences\n\n[1] Haley J Abel, David E Larson, Allison A Regier, Colby Chiang, Indraniel Das, Krishna L Kanchi, Ryan M Layer, Benjamin M Neale, William J Salerno, Catherine Reeves, Steven Buyske, NHGRI Centers for Common Disease Genomics, Tara C Matise, Donna M Muzny, Michael C Zody, Eric S Lander, Susan K Dutcher, Nathan O Stitziel, and Ira M Hall. 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A quantitative genomics map of rice provides genetic insights and guides breeding. Nat Genet, 53(2):243–253, Feb 2021.\n[31] Joachim Weischenfeldt, Orsolya Symmons, François Spitz, and Jan O Korbel. Phenotypic impact of genomic structural variation: insights from and for human disease. Nat Rev Genet, 14(2):125–38, Feb 2013.\nSupplementary Methods\n\nDetermining number of repeat units deleted\n\nThe Human Genome SV Consortium (HGSVC) has created a comprehensive catalogue [7] (named HGSVC2) of the SVs in 35 samples: 34 samples from the 1000g project (including HG00512), plus HG002 (alternatively called NA24385). Using these two catalogues, we investigate whether most CNVs in the human genome delete or duplicate whole repeat units. We determined the number of tandem repeat units deleted by the examined deletions as follows. We downloaded TRF [2] annotations for hg38 from the UCSC Genome Browser. For each deletion, we found the tandem repeat that contains the deletion; when we found multiple such repeats, we selected the one with the shortest repeat unit. The number of deleted copies was simply obtained by dividing the length of the deletion by the length of the repeat unit.\n\nBuilding accurate alternative alleles\n\nBy building an accurate alternative allele for each CNV and aligning the reads to it, we can precisely identify reads that are supposed to support it. We downloaded PacBio HiFi reads for both HG00512 (SRR13606079 to SRR13606084) and HG002 (SRR10382244 to SRR10382249), and aligned the reads to hg38 using minimap2 [11].\n\nFirst, we selected a subset of CNVs so that no two CNVs were within 4000 bp of each other. Then, for a given CNV \\( C \\), let \\( s \\) be the start of \\( C \\) minus 2000 bp, and \\( e \\) be the end of \\( C \\) plus 2000 bp. For each HiFi read overlapping \\( C \\), we extract the portion overlapping the region from \\( s \\) to \\( e \\). In case of heterozygosity, we want to identify the subset of reads supporting \\( C \\). In order to accomplish this, for each subread, we compute two numbers \\( d \\) and \\( i \\): the sum of the lengths of all deletions and insertions, respectively (\\( \\geq 10 \\) bp in order to exclude most sequencing errors). Then, we cluster the reads according to \\( d \\) and \\( i \\) using DBSCAN [9]. Each cluster represents an allele. In order to find the cluster that represents the allele with \\( C \\), we find the cluster that minimises the following formula\n\n\\[\n\\sum_{r \\in S} \\min_{x \\in indels(r)} (size(x) - size(C))^2\n\\]\n\nwhere \\( S \\) is a cluster of reads and \\( indels(r) \\) is the set of indels in a read \\( r \\). Intuitively, we want to find the cluster with the minimum sum of squared errors, where the error in a read is the difference between the length of the expected CNV and the observed one. Finally, we use the selected reads to assemble the alternative allele using SPOA [28].\n\nNext, we aim at selecting a subset of alleles that are extremely likely to be correct. We apply a series of filters to our set of assembled alleles:\n\n• **No reads**: no reads span the whole region from \\( s \\) to \\( e \\), therefore no alternative allele could be built;\n• **No SV**: when aligning the built alternative allele to the reference, no SV \\( \\geq 50 \\) bp could be identified;\n• **Multiple SVs**: when aligning the built alternative allele to the reference, multiple SVs \\( \\geq 50 \\) bp could be identified;\n• **Incompatible SV**: when aligning the built alternative allele to the reference, an SV could be identified, but the length was very different from the expected CNV (size difference >100 bp);\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
HG002 DELHG002 DUPHG00512 DELHG00512 DUP
No reads126106224179
No SV467232417214
Multiple SVs111217119202
Incompatible SV288576262551
No good LR support845734729833
Other45584144
High quality6150479661484585
\n\nTable 1: Each putative alternative allele undergoes a strict filtering process, in order to remove potentially incorrect sequences.\n\n• **No long-read support**: when realigning the HiFi reads to the alternative allele using minimap2, we expect to find at least 3 reads that (i) cover the whole alternative allele and (ii) they have no large indels (>10bp) and a low error rate (<0.1%). Furthermore, we use these reads to call phased variants using PEPPER-Margin-DeepVariant [23]. If the allele is correctly built, we expect one of the haplotypes to present no variant. If both haplotypes have variants, we filter the allele;\n• **Other**: alternative allele was excluded for other reasons;\n• **High quality**: the final set of alternative alleles retained for further analysis.\n\nSupplementary Table\\ref{tab:filtering} shows the number of assembled alleles removed in each step.\n\n**Detecting split reads and hidden split reads supporting CNVs and expected support score**\n\nThe Genome in a Bottle (GIAB) Consortium released a short-read sequencing dataset for HG002 using the Illumina HiSeq 2500 platform, and the New York Genome Center (NYGC) released a dataset for HG00512 sequenced with the Illumina NovaSeq 6000 platform. Using these datasets, we show that many CNVs in repetitive regions are not supported by split reads, but they are supported by hidden split reads.\n\nFor each CNV for which we obtained a high quality assembly, we identify the split reads and hidden split reads supporting it as follows. We align the alternative allele to the reference genome to calculate the precise coordinates of the breakpoints of the CNV, both on the alternative allele and on the reference genome. Then, we map the short reads on the alternative allele using BWA MEM [13], and we extract all reads overlapping a breakpoint. These reads should, in theory, support the existence of the CNV when mapped to the reference genome. Let us call \\( S \\) the set of such reads.\n\nWe extract the reference sequence \\( R_{ref} \\) between the start and the end of the CNV, plus 2000 bp of flanking sequences in each direction. Then, we create a second sequence \\( R_{cnv} \\) by introducing the CNV in \\( R_{ref} \\) (i.e., deleting the deleted part or inserting the inserted sequence). Finally, we map the reads in \\( S \\) to both \\( R_{ref} \\) and \\( R_{cnv} \\): The reads that are clipped when aligned to \\( R_{ref} \\) but not when aligned to \\( R_{cnv} \\) are split reads supporting the CNV, and reads that are not clipped and have a better alignment\nscore when aligned to \\( R_{cnv} \\) than when aligned to \\( R_{ref} \\) are hidden split reads supporting the CNV.\n\nIn order to calculate the expected score (ES) for a CNV, we fix a read length \\( l \\), and sample from the alternative allele all of the possible reads of length \\( l \\) containing the breakpoint(s). In other words, let \\( b_1 \\) and \\( b_2 \\) be the breakpoints of the CNV on the alternative allele \\( A \\) and let \\( R = \\{A[i..i+l] \\mid i < b_1 < i+l \\text{ or } i < b_2 < i+l\\} \\) be the set of all possible reads sequenced from the alternative allele that contain a breakpoint. Let \\( R' \\) be the subset of reads in \\( R \\) that aligns better to \\( R_{cnv} \\) than to \\( R_{ref} \\): then, \\( ES = \\frac{|R'|}{|R|} \\).\n\nRealigning individual hidden split reads to detect potential CNVs\n\nIn order to show that hidden split reads must be used carefully, we randomly select 10,000 repetitive regions in hg38. For each tandem repeat region, we select all reads that do not align perfectly to the reference. For each read, we split it into two at every possible location, and locally align the two half reads independently to the repetitive region. We select the split that has the highest score (calculated as the alignment score of the left half of the read plus the alignment score of the right half of the read). Let \\( s_l, e_l \\) be the start and end coordinates of the optimal alignment of the left half of the read, and \\( s_r, e_r \\) be the start and end coordinates of the optimal alignment of the right half of the read. If \\( s_r > e_l \\), we detect a deletion from \\( e_l \\) to \\( s_r \\); vice versa, if \\( s_r < e_l \\), we detect a duplication from \\( s_r \\) to \\( e_l \\). Finally, we retain all CNVs \\( \\geq 50 \\)bp.\n\nClustering split reads\n\nWe aim at clustering clipped reads and hidden split reads and, for each cluster of size at least three, generating a consensus sequence. Each consensus sequence represents a potential breakpoint of a CNV, and it is marked as right-clipped or left-clipped.\n\nIn the current algorithm, clipped reads and hidden split reads are not clustered together; in other words, a cluster cannot contain both clipped reads and hidden split reads. Left-clipped (resp. right-clipped) reads that are clipped at the same position (with a tolerance of 3 bp) are clustered together.\n\nFor hidden split reads, we heuristically determine whether a read is left or right-clipped as follows. We divide it into two halves, and count the number of differences with the reference (defined as number of mismatches plus the number of indels) for the left and the right half. If the left half has a higher number of differences than the right half, we mark the read as left-clipped; otherwise, we mark it as right-clipped. Left-clipped (resp. right-clipped) hidden split reads are clustered so that the overlap within any pair of reads within a cluster is at least half the read length.\n\nThe consensus generation proceeds identically whether the reads in the cluster are clipped or hidden split reads. For each cluster of size at least three, a consensus sequence is generated by casting a majority vote base by base [18]. Then, every read in the cluster is realigned against the consensus sequence: if the alignment contains any indel or the fraction of mismatches is greater than \\( \\epsilon \\) (\\( \\epsilon \\) is a user-defined value that represents the maximum expected fraction of sequencing errors in a read, 0.04 by default), the read is removed from the cluster. If less than three reads are\nFigure S1: (a) An example of a right-clipped reads \\( R \\) and its mate \\( M \\). \\( R \\) determines the left breakpoint of the deletion, and remapping the clipped sequence can determine the right breakpoint. By the definition of read pair, the right half of \\( R \\) and \\( M \\) must be within \\( max_{IS} \\) bp of each other; therefore, we define as the acceptable range for the right breakpoint of the deletion to be \\([e - max_{IS}..e]\\), where \\( e \\) is the endpoint of \\( M \\). (b) For duplications the situation is similar, except that the \\( R \\) determines the right breakpoint, and remapping the clipped sequence determines the left breakpoint. The acceptable range for the left breakpoint is therefore \\([e - max_{IS}..e]\\), where \\( e \\) is the endpoint of \\( M \\).\n\nretained, the whole cluster is discarded. Otherwise, a new, final consensus sequence is generated from the retained reads. Left-clipped (right-clipped) reads will produce a left-clipped (right-clipped) consensus.\n\nFinding a putative range for breakpoints\n\nAs mentioned in Section 2.2, the consensus sequence of a cluster of split reads represents a potential breakpoint of a CNV. Since a CNV has two breakpoints on the reference, we are interested in defining a range where to search for the second breakpoint. Fig. S1 shows how to calculate the range from a single right-clipped read. In order to calculate the range for a right-clipped cluster, we simply calculate the intersection of the ranges of the individual reads. The calculation of the range for left-clipped clusters is simply symmetrical.\n\nGenerating the junction sequence\n\nGiven a right-clipped consensus sequence \\( R[1..r] \\) and a left-clipped consensus sequence \\( L[1..l] \\), we generate a junction sequence as follows. Let \\( n \\) be the largest integer such that the hamming distance between \\( R[r-n+1:r] \\) and \\( L[1:n] \\) is at most \\( n\\cdot\\epsilon \\) (see Supp. Sec. [1] for a definition of \\( \\epsilon \\)). If \\( n \\geq 15 \\), the junction sequence is formed by concatenating \\( R \\) and \\( L[n+1:l] \\); otherwise, no sequence is generated.\n\nExtending a consensus sequence\n\nConsensus sequences obtained by split and hidden split reads tend to be short, often not much longer than the length of a read. For this reason, when realigning them to repetitive regions we may obtain incorrect or ambiguous locations. By extending the consensus sequences using assembly we aim at improving the confidence of the realignment. This happens in two steps: first, a set of target reads are identified; second, the target reads are used to extend using an overlap-layout-consensus approach.\nFigure S2: Detection of the target reads for the extension of a consensus sequence. (a) First, we identify the target region that contains the reads we will use to extend the consensus. In this case, since we are extending a left-clipped consensus to the left, the target region (in red) is the opposite breakpoint range of the consensus. (b) Next, we collect the reads within the target region (reads in black). Furthermore, an additional read is collected from an entirely different genomic location (described as chrB in the figure). This is because the location of its mate (in blue) suggests that the read might belong to the target region.\n\nIn order to detect the target reads, we first identify a target region where the desired reads are likely to be mapped. The target region is calculated as follows:\n• If we are extending a right-clipped consensus to the left, the target sequence is the \\( maxIS \\) bp region left-flanking the consensus;\n• If we are extending a left-clipped consensus to the right, the target sequence is the \\( maxIS \\) bp region right-flanking the consensus;\n• If we are extending a right-clipped consensus to the right or a left-clipped consensus to the left, the target region is the opposite breakpoint range (see Section 2.2).\n\nThen, all reads mapped within the target region are target reads. Furthermore, we search for pairs such that a read \\( R_1 \\) is aligned to the forward (resp. reverse) strand within \\( maxIS \\) bp upstream (resp. downstream) of the target region and their mate \\( R_2 \\) is aligned to a different genomic location: \\( R_2 \\) is added to the target reads (Supplementary Fig. S2).\n\nNext, we use the target reads to extend the consensus. A directed graph is built where each node is a read, and an edge connects two reads \\( R_1 \\to R_2 \\) if a suffix of \\( R_1 \\) and a prefix of \\( R_2 \\) of at least read length/2 bp are identical. The consensus sequence is treated as a read. If the connected component containing the consensus sequence contains a cycle, we remove every edge that touches a node in the cycle. Then, we find the longest path either starting from or ending at the consensus sequence, depending on whether we are extending the consensus to the left or to the right.\n\nClustering discordant pairs\n\nGiven a set of discordant read pairs, we want to partition them into clusters so that all read pairs in a cluster support the same CNV. For this purpose, we use the algorithm used by SurVIIndel [15]. Here we provide a brief, high-level description.\n\nEach cluster is composed of two segments, a forward and a reverse segment. We define a merging operation between two segments as follows: given two segments \\( S_1 = (s_1, e_1) \\) and \\( S_2 = (s_2, e_2) \\), we create a new segment \\( S_m = (min(s_1, s_2), max(e_1, e_2)) \\). We then define a merging operation between two clusters by merging the two forward segments and the two reverse segments. We also define the distance between the\ntwo segments \\( S_1 \\) and \\( S_2 \\) is defined as \\( max(e_1, e_2) - min(s_1, s_2) \\), and the distance between two clusters as the maximum distance between (a) the distance between the two forward segments and (b) the distance between the two reverse segments.\n\nThe algorithm proceeds as follows. Initially, each individual read pair forms a cluster, and its forward (resp. reverse) strand read is the forward (resp. reverse) segment of the cluster. Then, we keep merging the pair of clusters with the shortest distance, as long as the distance is less than \\( maxIS \\). Intuitively, if a segment is longer than \\( maxIS \\), it means that its cluster includes two reads that are more than \\( maxIS \\) bp apart. Therefore, it is unlikely that such reads support the breakpoint of the same CNV.\n\nInsertion size-based features\n\nAs mentioned in Section 2.2, CNVs will distort the insert size of read pairs. In particular, a read pair with a fragment size \\( L \\) crossing a deletion of size \\( d \\) will be mapped to the reference with an insert size of \\( L + d \\); when \\( d \\) is large, the read pair will be clearly discordant. However, when \\( d \\) is small, determining that the pair supports the presence of a deletion is not as easy. Note that we define a read pair as discordant when the insert size is greater than \\( maxIS = \\mu + 3\\sigma \\). Consider a read pair that contains a deletion, and assume its fragment size is \\( \\mu \\) bp. If the deletion is less than \\( 3\\sigma \\) bp, the read pair will not be detected as discordant.\n\nMore precisely, define \\( minIS = \\mu - 3\\sigma \\) to be the minimum acceptable insert size for a read pair. Remember that \\( maxIS \\) was defined similarly as the maximum acceptable insert size for a read pair. Then, when the deletion is of size greater than \\( maxIS - minIS = 6\\sigma \\), we expect that all pairs containing the deletion can be identified as discordant, and we use a positive-to-negative ratio. Let \\( P \\) and \\( N \\) be the set of discordant and concordant (i.e., not discordant) pairs that contain the midpoint of the tested deletion. We compute the positive-to-negative ratio as \\( |P|/(|P| + |N|) \\), and we reject the deletion if it is too low (lower than 0.25 by default).\n\nHowever, this approach cannot be used for smaller deletions. This problem was tackled in SurVIndel [18] by analysing the distribution of all pairs that potentially contain the deletion. Although it may be impossible to determine whether a single pair supports the deletion or not, we expect the read pairs to have a larger insert size, on average, than a set of pairs that do not contain a deletion. Therefore, statistical tests are employed to determine whether a set of reads may contain a deletion.\n\nHere, we calculate two features using two different tests. Both tests have two ingredients: a distribution \\( C \\) of read pairs that do not contain a deletion, and a distribution \\( D \\) of pairs that contain the candidate deletion that is being tested. \\( C \\) is generated by choosing 1 million random locations in the genome and sampling the pairs that contain any of those locations. \\( D \\) is the set of read pairs that contain the midpoint of the deletion. The first test determines a confidence interval for the size of the deletion, by computing a 99% confidence interval for the difference of means between \\( D \\) and \\( C \\), and tests whether the size of the predicted deletion falls within this range. The second tests employs a Kolmogorov-Smirnoff test to calculate a p-value estimating whether \\( C \\) and \\( D \\) are significantly different. The lower the p-value, the more likely \\( C \\) and \\( D \\) are different.\n\nFor the first test, the feature we obtain is 0 if the size of the deletion falls within the confidence interval, otherwise it is a positive number indicating how far outside the confidence interval the deletion falls. The\nsecond feature is the p-value of the KS-test.\n\nThe statistical tests are not currently applied to tandem duplications, because the distribution of reads pairs is far more complicated and challenging to use.\n\nComparing deletions and tandem duplications\n\nWhen comparing two indels, we use a set of three parameters: the max distance, the min overlap and the maximum length difference. Two deletions or two tandem duplications are considered to match if:\n\n1. The distance in bp between the two start coordinates and between the two end coordinates are less than or equal to max distance;\n2. The fraction of the shortest indel that overlaps with the largest indel is at least min overlap;\n3. The difference between the lengths of the two events is less than or equal to maximum length difference.\n\nWe use two sets of parameters, a precise (stricter) set and an imprecise (more permissive) set. When one or both the indels are marked as imprecise by the callers, we use the imprecise set, otherwise we use the precise set. For the precise set, we used (in order, max distance, min overlap, maximum length difference) 100 bp, 0.8, 100 bp. For the imprecise set, we used 500 bp, 0.5, 500 bp.\n\nThe same deletion or a tandem duplication in a tandem repetitive region may be represented using different coordinates. As an example, consider three genomic sequence A, B and C that appear as ABBBC in the reference and as ABBC in the sample (on B was deleted). Any of the copies of B in the reference may be marked as deleted and it would represent the same deletion. For this reason, we employ a repeat-aware comparison method. When two deletions or two tandem duplications fall within the same tandem repeat, we only check whether the lengths of the two events is less than or equal to maximum length difference.\n\nAs mentioned before, tandem duplications in the benchmark catalogues we used are represented as insertions, i.e., as an insertion site and an inserted sequence. In order to compare an insertion with a tandem duplication, we use a slightly modified method. The insertion site must be within max distance bp of either the start or the end of the duplication. Furthermore, we check whether the inserted sequence of the insertion and the duplicated sequence of the duplication match. Let \\( I[1..i] \\) be the inserted sequence and \\( D[1..d] \\) be the duplicated sequence in the reference. First, we find the number of times \\( D \\) was duplicated as \\( n = \\lceil \\frac{d}{i} \\rceil \\), and create \\( D' \\) by concatenating \\( D \\) \\( n \\) times. Then, we compute the local alignment between \\( I \\) and \\( D' \\) using a scoring scheme of +1, -4, -6, -1 (match, mismatch, gap opening, gap extension). If we alignment covers at least 80% of \\( I \\), we accept that the insertion and the duplication match.\n\nThe comparisons performed for Fig. 7 were all performed using the imprecise parameters, to account for the possible shifting of the breakpoints due to clustering.\n\nThe code of the comparison algorithm is available at https://github.com/Mesh89/SurVClusterer.\n\nClustering deletions and tandem duplications\n\nIn order to cluster a set of indels, we use the algorithm described in [15]. First, the set of indels is represented as a compatibility graph, where ev-\nery indel is represented as a vertex and the two indels are compatible, i.e., they potentially represent the same variant. We say that two indels are compatible if they match according to the comparison algorithm described in Supplementary Methods (we do not perform the repeat-aware comparison for efficiency reasons). After that, we heuristically compute the minimum clique cover (computing the optimal solution is not computationally feasible), and every clique is a cluster of indels. More details about the heuristic used can be found in [15]. The code of the clustering algorithm was published at https://github.com/Mesh89/SurVClusterer.\n\nOther organisms genomic data\n\nWe downloaded Illumina paired-end and PacBio HiFi reads for seven Arabidopsis Thaliana: Alo-0 (ERR10084935 and SRR1946106), Cas-0 (ERR10084942 and SRR1946392), Cat-0 (ERR10084948 and SRR1946393), Cvi-0 (ERR10084078 and SRR1945758), Evs-0 (ERR10084952 and SRR1946405), Hom-4 (ERR10084958 and SRR1946144) and Hum-2 (ERR10084063 and SRR1946147). All of the samples were aligned to TAIR10, using BWA MEM for short reads and minimap2 for long reads.\n\nFor the Bos Taurus samples, we downloaded PacBio HiFi reads (ERR10378054 to ERR10378058) and two short read libraries, which we treated as independent (ERR10310239 and ERR10310240). We aligned the reads to the ARS-UCD1.3. For the Mus Musculus sample, we downloaded PacBio HiFi reads (SRR23686163) and short reads (SRR23690179), and aligned them to the GRChm39 reference genome. For Oryza sativa, we downloaded PacBio HiFi reads (SRR10238608 for MH63, SRR13280199 for ZS97) and short reads (SRR13124689 for MH63, SRR13124696 for ZS97), and aligned them to the IRGSP-1.0 reference genome.\n\nBenchmark datasets for each sample were obtained by running Sniffles2 on the long read datasets.\nFigure S3: A region \\( D_s \\) covering the reference from position \\( a \\) to position \\( b \\), is deleted. \\( A \\) and \\( B \\) are the left- and right-flanking regions of \\( D_s \\), respectively. In the sample genome, \\( A \\) and \\( B \\) are adjacent. Therefore, a read \\( R \\) of \\( r \\)-bp may be sequenced so that its \\( r_1 \\)-bp long prefix is sequenced from \\( A \\) and its \\( r_2 \\)-bp long suffix is sequenced from \\( B \\) (clearly, \\( r_1 + r_2 = r \\)). When \\( R \\) is aligned to the reference, it will not completely align to any location. Rather, its first \\( r_1 \\)-bp will align to the \\( r_1 \\)-bp long suffix of \\( A \\), and its last \\( r_2 \\)-bp will align to the \\( r_2 \\)-bp long prefix of \\( B \\).\n\n![Diagram showing deletion and split reads](page_186_154_1077_120.png)\n\nFigure S4: (a) Assume there is a tandem repeat with \\( n > 1 \\) repeat units in the reference, its repeat units are all identical, and its length is greater than the read length. If the same tandem repeat in the sample has \\( m > n \\) repeat units, no split read will support the duplication. (b) Similarly to deletions, when copies of a tandem repeat are not identical, a duplication may generate hidden split reads.\n\n![Diagram showing hidden split reads and explicit clips](page_186_495_1077_120.png)\n\nSupplementary Figures\n![A diagram showing two alignments: one with two mismatches (contiguous alignment score: 90) and one without mismatches (two-part alignment score: 100)](page_420_670_583_120.png)\n\nFigure S5: A read is aligned to the reference with two mismatches. Suppose we assign +1 to a match and -4 to a mismatch; its alignment score will be 90 (98 matches and 2 mismatches = 98 - 8 = 90). If we allow the read to split into two, and its two parts to align independently without penalty, we can align both parts without mismatches. Therefore, the score is 100 (100 matches). The HSR-score of this read is 100 - 90 = 10.\nFigure S6: The impact of deletions deleting full repeat units and the importance of hidden split reads in detecting such deletions, studied on HG00512. (a) We consider a deletion to be contained in a tandem repeat if at least 90% of the deletion is covered by a repetitive region. Nearly two thirds of the deletions in this dataset are contained in a tandem repeat. (b) For every deletion that overlaps with a tandem repeat, we calculated the number of repeat units that it deletes by dividing the length of the deletion by the length of the repeat unit. Bars representing an integer number of copies (i.e., the length of the deletion is multiple of the length of the repeat unit) are coloured red. Most deletions delete an integer number of repeat units. (c,d) Percentages of deletions outside (c) and contained (d) in tandem repeats that are supported by split reads, by hidden split reads, and by neither. Hidden split reads have the potential to recover a significant number of deletions missed by regular split reads. (e) HSR-scores of the hidden split reads supporting the existing CNVs in HG00512. Most reads have low (<20) HSR-score. (f) We found all hidden split reads in 10,000 randomly sampled repetitive regions, and for each we tried to predict a CNV by finding the optimal split alignment. Most CNVs (>91%) detected this way were false positive. This shows that using hidden split reads to detect CNVs is challenging, and effective filters must be employed to distinguish real from false CNVs.\nFigure S7: An example of unsupported deletion in the HGSVC2 catalogue for HG002, called chr10-729000-DEL-76. The deletion is clearly supported by the HiFi reads aligned to hg38, but the HiSeq 2500 reads in the region appear to be very noisy. When aligned to the alternative allele, we observe that only one good quality read (BWA-MEM AS≥ 140, read length 150) contains the breakpoint. For this reason, despite having a high ES score (0.72), we cannot find reads supporting the deletion: for this reason, SurVIndel2 does not call it. However, in the simulated reads, plenty of correctly aligned reads contain the breakpoint. Unsurprisingly, SurVIndel2 can detect the deletion in the simulated dataset.\nFigure S8: An example of unsupported deletion in the HGSVC2 catalogue for HG00512, called chr1-2262046-DEL-70. The deletion is clearly supported by the HiFi reads aligned to hg38, but the Illumina reads in the region appear to be very noisy. When aligned to the alternative allele, we observe that there are no good quality reads (BWA-MEM AS≥ 140, read length 150) that contain the breakpoint. For this reason, despite having a high ES score (0.633), we cannot find any reads supporting the deletion. Many HiFi reads perfectly align the the alternative allele, which confirms that the alternative allele is correct.\n\n![Example of unsupported deletion in the HGSVC2 catalogue](page_320_613_1047_496.png)\nFigure S9: Factors that contribute to the absence of support for deletions in HG00512. The results confirm our findings on HG002. a) As for HG002, a large portion of unsupported deletions have low ES. However, 44% of the unsupported deletions have high EQ (\\( \\geq 0.5 \\)), which suggest that there is another reason the lack of support. b) Another factor is an absence of correctly sequenced reads containing the breakpoint of the deletions.\nFigure S10: Factors that contribute to the absence of support for duplications in HG00512. The results confirm our findings on HG0002. a) As for HG0002, most unsupported deletions (75%) have high EQ (\\( \\geq 0.5 \\)), which suggest that there is another reason the lack of support. b) The absence of correctly sequenced reads containing the breakpoints of the duplication is even more prevalent than in deletions.\nFigure S11: Factors that contribute to the absence of support for deletions, in a realistic synthetic dataset for HG002. a) As expected, the vast majority of unsupported deletions have low ES, while supported deletions have high ES. Unlike the real dataset (Fig. 9), nearly no unsupported deletions have high ES. b) The real dataset exhibited a large number of deletions that have high ES but no correctly sequenced reads containing their breakpoints. This phenomenon is absent from the synthetic dataset.\nFigure S12: Factors that contribute to the absence of support for duplications, in a realistic synthetic dataset for HG002. a) As expected, the vast majority of unsupported duplications have low ES, while supported duplications have high ES. This is in stark contrast to the real dataset, where the majority of unsupported duplications had high ES (Fig. 10). b) The real dataset exhibited a large number of duplications that have high ES but no correctly sequenced reads containing their breakpoints. This phenomenon is absent from the synthetic dataset.\nFigure S13: Support for deletions in the synthetic versus the real dataset. a) The simulated dataset has less unsupported deletions. b) The sensitivity of some methods is increased. This is particularly true for Manta (increase from 0.43 to 0.5) and SurVIndel2 (increase from 0.64 to 0.69). c) However, when stratified by evidence available, the sensitivity of the methods for each category are very similar between the real (Fig. 4i) and the synthetic datasets. This, combined with Supplementary Fig. S11 shows that the increase in sensitivity is due to less unsupported deletions.\nFigure S14: Support for tandem duplications in the synthetic versus the real dataset. a) The simulated dataset has far less unsupported duplications. b) The sensitivity of all the methods is considerably increased. Particularly notable is the performance of SurVIndel2 improves from 0.37 to 0.58. c) Once again, when stratified by evidence available, the sensitivity of the methods for each category are very similar between the real (Fig. 4f) and the synthetic datasets. This, combined with Supplementary Fig. S12 shows that the methods are severely limited because the regions containing the tandem duplications are not sequenced correctly.\n\nFigure S15: (a) Consider a read pair s.t. one read was sequenced upstream and one downstream of the deletion breakpoint, sequenced from a fragment of size \\( L \\). After mapping the pair to the reference, its insert size will be \\( L + d \\), where \\( d \\) is the size of the deletion. If the deletion is large enough, the insert size will also be abnormally large, when compared to the insert size distribution of the library. (b) When a duplication is large, reads sequenced from different copies of the duplicated sequence may show the wrong relative orientation when aligned to the reference.\nFigure S16: PCA based on deletions (a) and tandem duplications (b). Both event types are able to clearly separate the superpopulations.\n\n![PCA plots showing deletions and duplications for different populations](page_324_728_1097_355.png)\nFigure S17: PCA based on both deletions and duplications was able to segregate each superpopulation into subpopulations. (a) For Africans (AFR), two subpopulations are clearly separated from the others: Mende in Sierra Leone (MSL) and Gambian in Western Division (GWD). Americans (AMR) subpopulations are segregated on PC1, while PC2 is dominated by heterogeneity among Puerto Ricans (PUR). (c) East Asians (EAS) form three major clusters: (1) Vietnamese and Dai Chinese, (2) Han Chinese from Beijing with Southern Han Chinese and (3) Japanese. Some degree of separation between Han Chinese from Beijing and Southern Han Chinese is also observed. Similarly (d), Europeans (EUR) are also clustered into three clusters: (1) Finnish, (2) British and Utah residents with Northern and Western European ancestry and (3) Italians from Tuscany and Spanish. (e) South Asians (SAS) structure is much less obvious than other superpopulations. Furthermore, there appears to be high heterogeneity among Punjabi from Lahore (P JL). These results agree what we previously observed from insertions [17]\nFigure S18: Sensitivity of DeepVariant and DeepVariant plus SurVIndel2 on the 35 HGSVC2 samples, for deletions between 30 and 50 bp.\n\nFigure S19: Sensitivity of DeepVariant and DeepVariant plus SurVIndel2 on the 35 HGSVC2 samples, for insertions between 30 and 50 bp."} {"paper_id": "prb75", "title": "A de-risking experimental framework defines the physiological interactome of TCR-based therapeutics in human tissues", "text": "A de-risking experimental framework defines the physiological interactome of TCR-based therapeutics in human tissues\n\nEstelle Marrer-Berger\nRoche Pharma\nAnnalisa Nicastri\nUniversity of Oxford\nAngelique Augustin\nRoche Pharma Research and Early Development, Pharmaceutical Sciences – Biomarkers, Bioinformatics and Omics & Pathology, Roche Innovation Center Basel, F. Hoffmann-La Roche Ltd\nVesna Pulko\nRoche Pharma\nHanqing Liao\nUniversity of Oxford\nLydia Duemer\nRoche Pharma\nTina Wienzierl\nRoche Pharma\nLauriane Cabon\nRoche\nEmmanuelle Lezan\nUniversity of Basel\nChristian Klein\nRoche Innovation Center Zurich, Schlieren, Switzerland\nPablo Umaña\nRoche Innovation Center Zurich\nIsaac Woodhouse\nUniversity of Oxford https://orcid.org/0000-0002-8221-7697\nAlexander Bujotzek\nRoche (Germany) https://orcid.org/0000-0001-5052-0221\nNicola Ternette (nicola.ternette@ndm.ox.ac.uk)\nUniversity of Oxford https://orcid.org/0000-0002-9283-0743\nKeywords:\n\nPosted Date: July 20th, 2022\n\nDOI: https://doi.org/10.21203/rs.3.rs-1828302/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\nA de-risking experimental framework defines the physiological interactome of TCR-based therapeutics in human tissues\n\nShort title: The in situ interactome of TCR-based therapeutics\n\nEstelle Marrer-Berger1#, Annalisa Nicastri2*, Angelique Augustin1*, Vesna Pulko3*, Hanqing Liao2, Lydia Jasmin Duerner3, Tina Wienzierl3, Lauriane Cabon1, Emmanuelle Lezan1, Christian Klein3, Pablo Umana3, Isaac Woodhouse2, Alexander Bujotzek4, Nicola Ternette2,5#\n\n1 Roche Pharma Research & Early Development, Roche Innovation Center Basel, 4070 Basel, Switzerland\n2 The Jenner Institute, Old Road Campus Research Building, Oxford, OX37DQ, UK\n3 Roche Innovation Center Zürich, 8952 Schlieren, Switzerland\n4 Roche Pharma Research & Early Development, Roche Innovation Center Munich, Penzberg, Germany\n5 Centre for Immuno-Oncology, Old Road Campus Research Building, Oxford, OX37DQ, UK\n\n*equal contribution\n\n#Correspondence to: estelle.marrer-berger@roche.com; nicola.ternette@ndm.ox.ac.uk\nABSTRACT\n\nSelective binding of TCR-based therapies that target a single tumour-specific peptide epitope presented by human leukocyte antigens (HLA) is the absolute prerequisite for their therapeutic suitability and patient safety. To date, selectivity assessment has been limited to peptide library screening and predictive computational modeling. We developed the first experimental platform to de novo identify interactomes of TCR-like molecules directly in human tissues using mass spectrometry. As proof of concept, we confirm the target epitope of a novel MAGE-A4-specific TCR-like antibody. We further determine 16 cross-reactive sequences for ESK1, a TCR-like bispecific antibody recognizing WT-1 with known off-target activity, in healthy liver tissue. We observe strong, off-target-induced T cell activation for 8/16 sequences, demonstrating the high specificity of the approach. Off-target sequences define a previously missed amino acid compensation motif that structurally mimics the target peptide groove coordination and allows for peptide interaction with the engager molecule. We establish the importance of the identified off-target activity by demonstrating 3D liver spheroid killing in the presence of ESK1 and healthy donor PBMC. Finally, we utilize our approach to de-risk our novel MAGE-A4 targeting TCR-like bispecific antibody prior to entering now ongoing clinical trials. We conclude that our strategy offers an accurate, scalable route for de-risking TCR-based therapeutics prior to first-in-human clinical application.\nABSTRACT\n\nSelective binding of TCR-based cancer therapeutics that target a single epitope presented by HLA is the absolute prerequisite for therapeutic suitability and patient safety. To date, selectivity assessment has been limited to library screening and predictive modeling. We developed the first experimental platform to de novo identify interactomes of TCR-like molecules in human tissues. As proof of concept, we confirm the target epitope of a novel MAGE-A4-specific TCR-like antibody. We further determine cross-reactive sequences for ESK1, a TCR-like bispecific antibody with known off-target activity, in healthy liver tissue with high specificity, and establish causality by demonstrating 3D liver spheroid killing. We define a non-predictable compensation motif that structurally mimics the target peptide. Finally, we utilize our approach to de-risk our novel MAGE-A4 targeting TCR-like bispecific antibody prior to entering now ongoing clinical trials. We conclude that our strategy offers an accurate, scalable route for de-risking TCR-based therapeutics prior to first-in-human clinical application.\n\nSTATEMENT OF SIGNIFICANCE\n\nWe present an experimental strategy to define physiological interactomes of TCR-like therapeutics which is suitable for on- and causal off-target discovery in human tissues. We propose the integration of our framework with existing strategies for de-risking TCR-like molecules prior to first-in-human clinical trials.\nINTRODUCTION\n\nT lymphocytes play a critical role in cancer immunity. Their ability to elicit antigen-mediated cytotoxicity has become a key therapeutic strategy to engage the immune system to fight cancer. Peptides presented by human leukocyte antigen (HLA) are the natural target of T cells, and represent the largest pool of cell surface-presented cancer-specific targets. Therapeutically targeting specific peptide epitopes in complex with HLA complexes (HLAp) is thought to provide greater tumor selectivity over healthy tissues than targeting whole protein surface-expressed targets(1, 2).\n\nBispecific antibodies that bind to a HLAp surface antigen on cancer cells and an activating T cell antigen such as CD3ε can, through the forced interaction, trigger the lysis of cancer cells. While a vast majority of the CD3 bispecific antibodies developed in cancer target surface oncoproteins, the recent FDA approval of Tebentafusp, the first bispecific gp100 peptide-HLA-directed CD3 T cell engager provides the first clinical Proof of Concept of this approach for solid tumor therapy(3, 4).\n\nAn inherent downside of TCR-based therapies is their potential to cross-react with HLA molecules presenting related peptides besides the desired one, which can result in severe off-target effects and organ toxicities(1, 5, 6). Reported clinical fatalities related to off-epitope targeting with adoptive T cell therapies underpin the paramount importance of defining the unique specificity of these therapeutic molecules for their target before entering clinical trials. For TCR-like molecules, the strict human specificity of the HLA-I molecules, together with the limited overlap in protein processing and resulting peptide repertoires between humans and other species, invalidates the conventional toxicity testing in animals.\n\nIn the absence of a human relevant cross-reactive toxicology species, the non-clinical safety evaluation of TCR-like molecules is generally supported by new alternative methods. At an early stage of development, in silico strategies integrating peptide binding prediction and TCR contact profile elucidation through structural computational modeling are leveraged to predict potential off-targets(7). In silico strategies interrogating TCR repertoires rely on interactome data obtained from large peptide or HLA peptide complex libraries that enable\nthe estimation of the TCR specificity(8-14). Further advances were made by bioinformatic approaches relying entirely on prediction of TCR interactomes based on TCR sequence features and their interacting peptide target(15-19). However, it has been recognized that these approaches are still limited as the specificity of prediction is low, and hundreds of sequence candidates need to enter validation assays with generally low confirmed off-target hit rate. Furthermore, TCR specificity is expanded by a dramatic HLAp structural adaptability, demonstrated by unanticipated rearrangements in the peptide and presenting HLA protein(20). These limitations and gaps highlight the need for novel, physiologically relevant technologies for off-target sequence identification(21).\n\nAlthough human primary cells and organ models provide a unique opportunity to evaluate if the TCR-like engagers also trigger any relevant T cell effector function such as T-cell dependent lysis, it remains therefore challenging to identify the causality of the cross-reactivity in primary healthy human tissues. In addition, most of the human model systems available still bear physiological and cellular gaps, rising the need to assess off-target binding in situ rather than in vitro.\n\nThus, to further increase the confidence in the selectivity of clinical TCR-like therapeutic candidates, we here adapt a mass-spectrometry technology-based approach to enable the systematic and robust identification of physiologically relevant off-target peptide-MHC complexes bound by TCR-like molecules in situ(22). We utilize this technology to support the development of a novel TCR-like antibody targeting HLA-A*02:01 in complex with peptide GVYDGREHTV originating from MAGE-A4. Using this approach, we were further able to define causal off-targets of ESK1, a well characterized TCR-like T cell bispecific antibody, which is known to unselectively target peptide RMFPNAPYL derived from the intracellular oncoprotein WT1 (WT1_{126-134}) presented on HLA-A*02:01(23-25), with high specificity. We demonstrate how a mimic motif allows off-target interaction with ESK1 and T cell activation which had been missed in previous prediction-validation approaches. Our data demonstrate the high binding selectivity of the MAGE-A4 antibody and support its further clinical development.\nTogether, we show that our platform represents a game changing strategy to assess cross-reactivities of TCR-based molecules, and that this approach will assist the development of highly specific and safe immunotherapies.\n\nRESULTS\n\nA novel, functional HLA-A2-specific MAGE-A4 epitope targeting TCR-like T-cell bispecific\n\nWe generated antibodies specific for the MAGE-A4 peptide (GVYDGREHTV, MAGE-A4_{230-239}) HLA-A*02:01 complex using phage display technology (further details are given in the Methods section). The 57D03 antibody was selected due to its selectivity profile and characterization in cell assay, and reformatted into a trivalent 2+1 IgG TCB antibody with bivalent recognition of the MAGE-A4–pMHC complex and monovalent binding to the CD3ε chain of the TCR. This was facilitated by fusion of a second fragment antigen-binding region (Fab) to the N-terminus of the variable-light (VL) domain of the anti-CD3 Fab, resulting in a heterodimeric 2+1 antibody (CrossMAbVH-VL)(26). Introduction of P329G and L234A-L235A (PG LALA) mutations renders it inactive for immune effector functions(26-29). For the work presented here, a CD3 binder based on the humanized antibody V9 derived from UCHT1, was used, yielding HLA-A2 MAGE-A4 targeting TCR-like TCB (henceforward named MAGE-A4 TCB, Figure 1A). Association and dissociation constants for HLA-A*02- GVYDGREHTV and CD3ε are summarized in Supplementary Figure S1.\n\nOur aim was then to confirm functionality of the MAGE-A4 TCB in HLA-A*02:01-positive malignant melanoma cell line A375 which expresses MAGE-A4. We decided to optimize our assay using A375 cells and xenograft material to demonstrate killing both in tumour cells and tissue material. We first confirmed and quantified presentation of the MAGE-A4 target peptide sequence by HLA-A*02:01 on A375 cells using a standard, targeted immunopeptidomics approach, and determined the target peptide abundance to a minimum of 30-50 copies per cell in cells and xenografts (Figure 1B). The experiment was controlled by a parallel investigation using A375 xenografts in which the target antigen MAGE-A4 had been removed by CRISPR-KO (A375-KO). We finally\nconfirmed that the measured interaction of the MAGE-A4 antibody with the target peptide induces killing of the A375 cells when co-cultured with human PBMCs. We determined concentration dependent, highly effective lysis of A375 cells, validating the functionality of the TCB (Figure 1C).\n\nDe novo identification of on-target binding of the MAGE-A4 TCB to its target peptide GVYDGREHTV using a novel experimental framework\n\nTo demonstrate the on-target binding of the MAGE-A4 antibody to the target HLAp, we developed a reverse immunopeptidomics strategy that uses the HLAp targeting antibody as a bait to enrich interacting HLAp from A375 xenografts (Figure 1C). For this purpose, we immobilized the IgG on Protein A beads by cross-linking, and exposed the molecule to the solubilized proteome, including membrane bound HLAp, of the A375 xenografts. We subsequently eluted the interacting HLAp bound to the MAGE-A4 IgG, and purified the HLA-associated peptides through a 5 kDa molecular weight filter before liquid chromatography tandem mass spectrometry (LC-MS\\(^2\\)) analysis for sequence determination (Figure 1D). The experiment was controlled by an isotype control antibody targeting an irrelevant HLAp, and A375-KO xenograft tissue as before. The target peptide of the MAGE-A4 TCB, GVYDGREHTV, was identified in all three replicate analyses in A375 xenografts with high confidence, and was not identified in the A375-KO nor when an isotype control was used as a bait, as expected (Figure 1E,F). It is noteworthy that in addition to the target peptide, a shorter version of the target peptide (YDGREHTV) was detected with lower intensity (Supplementary Figure S2).\n\nFurthermore, out of all detected peptides predicted to bind to HLA-A*02:01, GVYDGREHTV was the only sequence identified as enriched in two independent biological repeat experiments, indicating a highly selective binding capacity of the MAGE-A4 IgG. These results show that we were able to enrich and identify HLA-peptide complexes using TCBs in IgG format, and that we can de novo identify the target peptide sequence by LC-MS\\(^2\\) using this approach.\nDirect comparison of interactomes of MAGE-A4 to ESK-1, a known TCR-like antibody with off-target activity, identifies ESK1 cross-reactive peptides in healthy liver tissue\n\nWe then aimed to expand our assay from xenograft tissue to healthy human tissues for evaluation of off-target reactivity. Next to our novel clinical candidate, we decided to include a second TCR-like antibody, ESK1, as a control. ESK1 was developed to recognize HLA-A*02:01 presented peptide derived from the intracellular oncoprotein WT-1 (RMFPNAPYL, WT1_{126-134})(23-25). The antibody has never entered clinical development due to off-target binding and lysis of diverse human primary cells. Candidate off-target sequences have been proposed recently(24, 25), however, the presentation of causal off-target peptide sequences in primary human tissues has not been confirmed to date.\n\nWe chose to perform a “head to head” immune-enrichment from primary liver tissue resections using both, MAGE-A4 and ESK1 IgGs. Since both target antigens MAGE-A4 WT-1 are not expressed in A375 cells (data not shown), the ESK1 enrichment could serve as isotype control for the MAGE-A4 IgG, and vice versa. The comparison of significantly enriched interactomes for both antibodies uncovered 16 HLA-A*02:01 peptides for Esk1, and 1 peptide for the MAGE-A4 TCB (Figure 2A, Table 1). The sequence motif of peptides significantly enriched by ESK1 shows a preference for a R/K/A in the first position, while A2 anchor residues are maintained (Figure 2B). This observation is in alignment of the previous observation that ESK1 interacts mainly with the N-terminal domain of the HLA-A*02:01-bound peptide(25).\n\nWe then proceeded to compare our identified HLAp sequences with off-target sequences published by Gejman et al. 2020(24). In this study, a genetic minigene platform (PresentER) was used to experimentally test predicted peptide sequences for interaction with ESK1. Authors identified 100 peptide sequences to be interacting with ESK1, of which 27 entered validation assays. We observed similarities in the obtained weighted sequence motif of the 27 shortlisted peptide sequences from these experiments, and the weighted motif determined in our study (Figure 2C). Both motifs accurately reflect the first for amino acids of the ESK1 target peptide sequence RMFPNAPYL (R-M-F-P are present in the obtained motif at positions 1-4, Figure 2C), which is not present in\nhealthy liver tissue. Nine out of the 27 Gejman et al. 2020 reported peptides are known to be expressed in liver (Supplementary Table S1), however, none of the sequences were confirmed in our assays as physiological ligands presented by HLA in healthy (non-cancerous) human liver tissue (Figure 2D).\n\nHalf of the identified ESK1-cross reactive peptides are potent to elicit T cell activation\n\nThe 16 peptides enriched by the ESK1 IgG were evaluated for their potential recognition by ESK1 TCB using Jurkat NFAT activation assay. T2 cells were first pulsed with the peptides and then co-incubated with JNFAT effector cells in the presence of different concentrations of ESK1 TCB. The target peptide RMFPNAPYL (WT1_{126-134}) was used as a positive control, while VLDFAPPGA, a WT1-derived non-relevant peptide (WT1_{37-45}) was used as negative control. Eight peptides resulted in a positive signal in two independent experiments. While the known targeted RMFPNAPYL peptide elicited the expected signal, SHC1_{469-477}, RMB4B_{59-67}, USP9Y_{1674-1682}, ARHGEF26_{863-871} CRYL1_{130-138}, CYP2C8_{59-67}, gave a higher signal than the RMFPNAPYL target peptide sequence in the JNFAT reporter assay, while ILF2_{127-135}, SF3B4_{78-86} gave positive signal that was weaker than the target peptide in direct comparison (Figure 3A). Furthermore, the signal of the 6 peptides that showed higher T cell activation in the presence of ESK1 TCB remained consistently higher than those of the RMFPNAPYL target peptide even at 100-fold diluted peptide concentrations (Figure 3B). Interestingly, the ESK1-reactive peptides all exhibited a high fold-enrichment in the interactome assay (\\( \\geq 4.5\\)-fold enrichment) with one exception, SHC1_{469-477}, which was 2.4-fold enriched but conversely resulted in the highest activation response. We did not observe a significant correlation between the measured fold enrichment and the degree of T cell activation (Supplementary figure S3). All peptides were also evaluated for their potential recognition by MAGE-A4 TCB using the same assay, including peptide EIF3F_{348-357}, which had been detected as enriched in by the MAGE-A4 TCB in the interactome assay. The target peptide (MAGA4_{230-239}) was used as a positive control, while WT1_{37-45} and WT1_{126-134} were used as negative controls. No signal was observed with MAGA4 TCB other than with its target peptide sequence (Figure 3C).\nESK1 off-target activity leads to killing of 2D liver spheroids\n\nTo confirm that the observed cross-reactivities of ESK1 in situ are relevant for killing of primary hepatocytes, and to validate the high specificity observed for the MAGE-A4 antibody, we employed an in vitro T cell dependent lysis assay performed with a 3D HLA-A*02:01 human liver spheroid cell model. The in vitro killing assays were performed by exposing co-cultures of liver spheroids and primary allogenic PBMCs to the relevant TCBs. The assays were controlled by testing co-cultures upon incubation in medium only, and assaying the negative control DP47 TCB (a non-tumor targeted TCB) side by side with MAGE-A4 TCB and ESK1 TCB. The absence of expression of both target proteins, MAGE-A4 and WT1, in the liver spheroids allowed the exclusion of a target-mediated effect by MAGE-A4- and ESK1 TCBs, respectively (data not shown). Cytotoxicity was assessed by live imaging using measurement of Granzyme B secretion, and by monitoring the levels of aspartate aminotransferase. As expected by the in situ cross-reactivity data, ESK1 TCB triggered significant dose-dependent target cell lysis accompanied by T cell activation/proliferation and cytokine release (data not shown) in liver spheroid tissue (Figure 3D). In alignment with our observation that the MAGE-A4 TCB has high selectivity for its target peptide sequence, no significant effects were observed in this model, suggesting the absence of off-target cross-reactivity (Figure 3D).\n\nESK1 off-target sequences are defined by a compensation binding motif, which structurally mimics the ESK1 target peptide motif, allowing interaction with ESK1 despite complete amino acid sequence divergence\n\nTo explore how ESK1 might be able to bind to the off-target peptides when being presented on HLA-A*02:01, we generated a molecular model of all of the Jurkat-NFAT confirmed eight peptides in complex with HLA-A*02:01 and in the presence of the Fab of ESK1, based on the X-ray crystal structure (PDB-ID: 4WUU) of the ESK1 Fab binding to HLA-A*02:01-WT1_{126-134} (RMFPNAPYL). These analyses show that all cross-reactive peptides can be accommodated in the structure without significant steric clashes (Figure 4A). In the structural alignment, the four N-terminal peptide positions are showing a high degree of similarity with regards to backbone conformation\nand sidechain orientation, while the central part of the peptide (positions 5-7) is structurally divergent. The amino acid on position 8 as well as the anchor residue on position 9 are again tightly aligned.\n\nThe crystal structure of ESK1 binding to the HLA-A*02:01-WT_{126-134} complex documents that ESK1 is binding in the proximity of the N-terminal half of the RMFPNAPYL peptide (Table 2), and that direct chemical interactions between ESK1 and the RMFPNAPYL peptide are only occurring with the arginine residue on position 1 (Figure 4B). Further interactions between position 4 of the peptide and CDR-L3 residue D93 of ESK1 are conceivable due to their short distance of only 3.4 Å.\n\nThe most active peptide SHC1_{469-477} (RVPPPPQSV) is identical to WT1_{126-134} (RMFPNAPYL) on the critical positions 1 and 4. This provides a clear structure-based rationale for the recognition by ESK1 via the RXXP motif and the observed binding mode (Figure 2C). However, and in marked contrast to SHC1_{469-477}, three out of the eight peptides did not share a single amino acid at any given position with the WT1_{126-134} target peptide (RMB4B_{59-67} (KLHGVNINV), CYP2C8_{59-67} (KVYGPVFTV), SF3B4_{78-86} (KLYGKPIRV), Table 2). The most reactive peptide amongst these, RBM4B_{59-67} (KLHGVNINV), was able to adapt a very similar conformation in the peptide binding groove (Figure 4C, D). Residue G4 of the RMB4B_{59-67} (KLHGVNINV) peptide is able to substitute for P at position 4 of the WT1_{126-134} (RMFPNAPYL) peptide and promotes a turn in the backbone. Similarity is also found on position 1 (with R and K both carrying a positive charge) and position 3 (with F and H both being of similar size and having an aromatic ring). In addition, the same holds true for the pairs of hydrophobic amino acids found on the classical anchor positions 2 and 9. The same amino acid motif, KXXG and an aromatic amino acid (H, Y) on position 3 [KXX_{H/Y}G], is also found for the two other cross-reactive peptides CYP2C8_{59-67} (KVYGPVFTV) and SF3B4_{78-86} (KLYGKPIRV) and consequently a very similar binding mode to RBM4B_{59-67} can be expected.\n\nInterestingly, the cross-reactive peptides ARHGEF26_{863-871} (RLLGLETNV) and USP9Y_{1674-1682} (RLWGEPVNL) seem to contain a hybrid of the RXXP and KXXG motifs observed here [RXX_{L/W}G]. Once more, G is confirmed as a favorable substitution for P on position 4, although the set of cross-reactive peptides also contains one instance of A on\nposition 4 (huCRYL1_{130-138}, KLFAGLVHV). This specificity profile of position 4 is in line with earlier binding studies of ESK1 involving mutated versions of the WT1_{126-134} peptide(24).\n\nFinally, the peptides shown to be non-activating in the JNFAT assay (Table 1) also share structural features that set them apart from the activating peptides: In all but one of the cases, this is a charged residue (3 x E, 1 x D, 1 x K) or a polar, uncharged residue (2 x S, 1 x N) at position 4. As an exemption to this rule, the non-activating peptide HNRNPA1_{15-23} (KLFIGGLSF) has an I on position 4, which is hydrophobic (same as the A which is tolerated on this position) but seems to cause steric hindrance and non-favorable chemical interactions with CDR-L3 of ESK1. Notably, the presence of these non-tolerated amino acids on position 4 seems to overrule the presence of a favorable residue on position 1 (3 x K, 1 x R).\n\nThe MAGE-A4 TCB is a highly specific molecule\n\nFinally, in order to extend the functionality of our approach for de-risking of the novel MAGE-A4 TCB, we applied our interactome assay to two further healthy tissues from lung and colonic tissue. We used an isotype control targeting HLA-DQ, a low expressed HLA class II surface molecule. No peptides were significantly enriched by the MAGE-A4 IgG in these experiments (Figure 5A). As expected, we did not identify the target peptide, nor any other peptide from the source protein MAGE-A4, in any of the two healthy tissues interrogated here.\n\nTo confirm that these results result in an absence of activating activity in these tissues in the presence of the MAGE-A4 TCB and primary human PBMC, we again performed *in vitro* killing assays. As before, we controlled the in vitro assays by testing MAGE-A4 TCB and ESK1 TCB side by side with a negative control DP47 TCB (a non-tumor targeted TCB). MAGE-A4 and WT1 were not expressed in either lung or colonic 2D models. Cytotoxicity was assessed by live imaging using a Caspase 3/7 fluorescent probe. No significant off-target effects were detected for the MAGE-A4 antibody, mirroring the lack of specific peptide enrichment in either tissue observed with the\nMAGE-A4 antibody (Figure 5B). In contrast, ESK1 again showed off-target activity in both lung and colonic 2D models (Figure 5B).\n\nWe conclude that MAGE-A4 TCB is a highly specific, novel therapeutic engager molecule, with no observed off-target activity in liver, lung and colon tissues.\n\nDISCUSSION\n\nAn urgent priority for the development of HLA-peptide specific immunotherapies is the establishment of strategies for off-target screening to de-risk these therapies in the absence of suitable *in vivo* strategies prior to entering human clinical trials. Animal models have limited validity due to species specific MHC binding specificities and an altered antigen processing machinery(30). The definition of off-target peptide sequences by integration of library data, prediction and structural modelling has advanced our understanding of TCR interactomes, but has not been sufficient to define physiologically relevant risk antigens in the past(21).\n\nWe present here a novel approach that is able to test the TCR-like molecule against the whole naturally processed and presented peptidome repertoire of a given primary human tissue, for which thousands of HLA-associated peptides can be identified by immunopeptidomics approaches. We use a TCR-like antibody enrichment strategy and an LC-MS readout to evaluate the interactome of a novel TCR-like TCB targeting MAGE-A4\\(_{230-239}\\) in the HLA-A*02:01 context. We confirmed the functionality of the approach in a proof of concept experiment, in which we demonstrated the significant enrichment of the target peptide using the TCR-like antibody as a bait in A375 xenograft tissue. In addition to the target peptide we also identified a shorter 9mer version of the target peptide at low intensity, which could result from MAGE-A4 antibody binding and co-enrichment but is likely a result from in-source fragmentation during MS acquisition(31).\n\nWe further investigate interactomes of the MAGE-A4 antibody and ESK1, a TCR-like TCB targeting WT1\\(_{126-134}\\) which has not entered clinical development due to off-target binding and lysis of diverse human primary cells.\n\nEpitope binding of ESK1 relies almost exclusively on peptide residue Arg1(24, 25). Candidate off-target sequences\nhave been proposed recently(24), however, the physiological presentation of off-target peptide sequences in primary human tissues has not been confirmed to date. Strikingly, using our methodology, we identify here 16 novel ESK1 interacting HLA-presented peptide sequences in primary healthy liver tissue. Neither of these peptide candidates had been previously identified as an off-target candidate for ESK1, despite the fact that amino acid motifs for off-target sequences identified between our study and Gejman et al. 2020 show a remarkable similarity (Figure 2B), and that predicted sequence requirements for ESK1 recognition by Ataie et al. 2016 were in alignment with our observations. The most apparent difference between our study and Gejman et al. 2020 was a strong requirement for a proline residue at position 4 of the peptide enabling interaction with ESK1, that could not be observed in our data. Instead, we determined a stronger requirement for an aromatic or hydrophobic amino acid in position three, despite a lack of evidence for this residue to be important for ESK1 Fab engagement.\n\nWe further observed the ability to induce T-cell activation for eight out of the 16 (50%) identified peptide sequences in the presence of the TCR-like TCB in a Jurkat NFAT activation assay. Six of the active peptides induced higher T cell activation than the target peptide. These six peptides belong to the most significantly enriched peptides in the interactome assay, with high enrichment ratios. In depth analysis of the structure of the highest reactive peptide, SHC1_{469-477} (RVPPPPPQSV), did not immediately conclude why the peptide is significantly more active than the RMF target sequence. Possibly, the quadruple P motif leads to a more favorable backbone conformation for recognition by ESK1 as P4 in the modeled complex is situated “higher” than P4 in the RMFPNAPYL complex, and thereby more available for interactions with the CDR-L3 loop of ESK1 (Figure 4C).\n\nThree peptides, RMB4B_{59-67} (KLHGVNINV), CYP2C8_{59-67} (KVGYPVFTV), SF3B4_{78-86} (KLYGKPIRV) did not have any sequence identity with the target peptide sequence, and had a KXXG motif rather than the previously observed RXXP recognition motif for ESK1. Birnbaum et al. showed in 2014 that unrelated peptide sequences can emerge from sequence clustering and structural analysis, and conclude that TCR interactomes share many common features with regards to docking geometry and interaction chemistry(9). The authors describe “hot spots” on a\npeptide, while tolerating extensive diversity at other positions. Dash et al. later confirm these observations by identification of shared core sequence similarities for a clustered group of receptors, but also observe a diverse set of outlier sequences(32). It is therefore generally accepted that TCR cross-reactivity is shaped by structural adaptability of the HLAp rather than by sequence alone(20).\n\nNeither of the remaining ESK1-enriched peptide sequences that were unable to elicit a JNFAT signal had either of the two detected sequence motifs RXXP, KXXG/A, and RXXG, suggesting that these motifs are in fact predictive for T cell activation via the ESK1 TCB. These results emphasize that the incorporation of the structural interphase of the MHC-peptide complex and TCR is essential to enhance predictive algorithms, and highlight that reliance on sequence homology prediction is limited to capture only a part of the potential interactome of a given TCR-like molecule.\n\nWe finally confirm that the observed cross-reactivities lead to killing in 3D healthy human liver cells in co-culture with ESK1 and PBMC, confirming the validity of our assay and causality of the detected cross-reactive HLAp sequences. We further demonstrate that the high specificity observed for the MAGE-A4 antibody is accurate, as no significant killing in lung, colonic and liver cells is observed in our killing assays.\n\nIn conclusion, the presented experimental platform harbors the ability to discover sequence-related and -unrelated on- and off-target sequences, and is uniquely placed for systematic interrogation of TCR-based molecule interactomes in the future. The presented strategy can replace costly high-throughput platforms and provide an effective way for de-risking of clinical candidates prior to entry into human trials. Other approaches have successfully identified requirements and binding rules, including off-target sequences, for TCR and TCR-like molecules, however, neither study has yet demonstrated the confirmed off-target antigens to be presented in healthy tissue and therefore physiologically relevant. In contrast, our methodology further demonstrates suitability to evaluate interactomes TCR-based therapeutics directly in human tissues of physiological or pathological relevance. This possibility fundamentally expands and circumvents the limitations of existing strategies and prioritizes relevant off-targets for ex vivo validation.\nDespite achieving high sensitivity and the detection and identification of the target peptide with an estimated abundance of 10th of copies, a limitation of the method remains the high requirements of test antibody (hundreds of micrograms) and human tissues (tens of milligrams). With a fast-expanding market of increasingly sensitive mass spectrometers and a miniaturization of the workflow, such “interactomics” assays could however be established as high-throughput platforms, and tissues screened systematically for off-target activity.\n\nWe conclude that in silico predictions and biostructural modeling are to date not sufficient for de-risking of TCR-based therapeutics. To overcome these limitations and to de-risk the development of novel drug candidates, we propose that a functional interactome characterization can, if complemented with ex vivo testing in human primary cells and tissues, enable successful assessment and optimization of TCR-based molecules, and ultimately minimize risks for patients.\nMETHODS\n\nPrimary tissues and cell lines\n\nHuman liver samples were obtained from Cytes Biotechnologies (Spain) and human lung and colon samples were obtained from HTCR (Germany) with all ethical approval and patient consent in place.\n\nHybridoma cell lines for pan-HLA antibody production were grown in serum-free medium (17.5 ml of hybridoma mix [20g peptone (Sigma), 25g D-glucose (Sigma), 100ml L-glutamine solution (200mM, 100x Gibco/Invitrogen), 100ml Penicillin streptomycin (100x Gibco/Invitrogen), 100ml Non-essential amino acids (100x, Gibco/Invitrogen), 150ul 2-mercaptoethanol (1% in dH2O, Sigma)] in 500 ml Hybridoma SFM (Gibco/Invitrogen). Hybridoma cells were seeded at 8 Mio cells and maintained in bioreactor flasks CL350 (Thermo Scientific) according to the manufacturer’s instruction.\n\nThe T2 cell line (DSMZ# ACC598) is a hybrid of B-lymphoblastoid cell line 721.174 and 8-azaguanine and ouabain-resistant variant of T-lymphoblastoid cell line human ovarian epithelial –serous cancer cell line. Cells are TAP deficient and express only small amounts of HLA-A2 and no B5 antigen on their surface. The cells were cultured in RPMI containing 10 % FCS and split every three to four days (to 0.6 mio/mL) before reaching confluence.\n\nJurkat NFAT cell line is T lymphocyte cell line (developed by Signosis) with transfected NFAT luciferase construct. The cells were cultured in RPMI containing 10 % FCS and 0.2 µg/ml Hygromycin B. Cells were split every three to four days (to 0.5 mio/ml) before reaching confluence.\n\nMAGE-A4 TCB generation: Generation of antigen and selection of specific antibodies by phage display\n\nThe DNA sequences of both the HLA-A*02:01 extracellular domain (position 25-299, Uniprot Q53Z42) and the beta-2-microglobulin (position 21-119, Uniprot P61769) were synthesized and inserted in frame into a prokaryotic recipient vector. A 2-fold G4S linker was inserted between the protein fragment and an N-terminal Avi-tag and His-Tag allowed specific biotinylation during co-expression with BirA biotin ligase.\nRecombinant soluble MHC alpha chain (HLA-A*02:01) and beta2-microglobulin were isolated from E.coli as inclusion bodies. Additionally, the HLA chain was in vivo biotinylated in E.coli by co-expression of the enzyme biotin ligase BirA. The solubilized proteins were refolded together with the peptide using a renaturation process and subsequent purification using standard chromatographic procedures. Peptides used were derived from the huMAGE-A4 protein (GVYDGREHTV, residues 230-239), and as a tool for pre-clearing a peptide derived from the human WT1 protein (VLDFAPPGA, residues 37-45). Anti-HLA-A2/MAGE-A4_{230-239} specific Fabs were selected by phage display from synthetic Fab libraries either consisting of VL and VH pairings derived from different V-domain families. More precisely, clone 57D03 was selected from antibody library DutaLibTM-4H. The library is built by diversification of the same human antibody scaffold, Dutalys Dummy34.1. This scaffold comprises human VH3 consensus and human VK1 consensus framework region sequences, and CDR sequences that are similar to human VH3-23 and human VK1-O2 germline sequences.\n\nSelection rounds (bio panning) were performed in solution according to the following pattern: (i) pre-clearing of ~ 1012 phagemid particles per library pool on neutravidin coated 96 well plates coated with 500nM of an unrelated biotinylated HLA-A2/ WT1_{37-45} complex, (ii) incubation of the non-HLA-A2/ WT1_{37-45}-binding phagemid particles with 100nM biotinylated HLA-A2/MAGE-A4_{230-239} complex for 0.5 h in a total volume of 800µl, (iii) capture of biotinylated HLA-A2/MAGE-A4_{230-239} and specifically binding phage by adding 80µl of streptavidin-coated magnetic particles for 20 min on a shaker, (iv) washing of respective magnetic particles 5-10x with 1ml PBS/Tween20 and 5-10x with 1ml PBS using a magnetic particle separator, (v) elution of phage particles by addition of 1 ml 100mM TEA (triethylamine) for 5-10 min and neutralization by addition of an 1/2 volume of 1M Tris/HCl pH 7.4, (vi) re-infection of log-phase E. coli TG1 cells with the eluted phage particles, incubation on a shaker at 37°C for 0.5 h, infection with helper phage VCSM13, incubation on a shaker at 30°C over night and subsequent PEG/NaCl precipitation of phagemid particles to be used in the next selection round. Selections were carried out over 3 to 4 rounds using decreasing antigen concentrations of 100 nM, 50 nM, 50 nM and 10 nm, respectively.\nMAGE-A4 TCB generation: ELISA for characterization Fabs obtained by phage display\n\nIn case of the DutaLibTM-4H, after selection round 3 and 4, part of the reinfected bacteria were used to prepare a dense TG1 E.coli culture was prepared and incubated 7-16 h at 30°C. Following preparation of the polyclonal plasmid mini-prep, all of the Fab clones in the mini-prep, jointly representing the selection round output, are re-formatted in batch for soluble Fab fragment (sFab) expression, to enable screening ELISAs. The first step in this re-formatting process was to excise the Gene3 stump CDS contained in the selected Fab constructs in a restriction digest. The restriction digest was performed either using BamHI, in order to obtain soluble Fabs tagged with a T7 sequence. The resulting linear fragment was gel-purified, circularized in a standard ligation reaction and transformed into competent TG1 E.coli cells. Transformants were plated onto 2xYT agar or supplemented with 100 µg/ml Carbenicillin and 2% w/v glucose.\n\nIndividual clones were bacterially expressed as 1ml cultures in 96-well format and supernatants were subjected to a screening by ELISA. Specific binders were defined as signals higher than 5 × background for HLA-A2/MAGE_{230-239} and signals lower than 3 x background for HLA-A2/ WT1_{37-45}. More precisely, Thermo Fisher neutravidin 96 well strip plates were coated with 10nM of biotinylated HLA-A2/MAGE-A4_{230-239} complex or 50nM of biotinylated HLA-A2/ WT1_{37-45} complex at 37°C for 30min followed by blocking of the plate with 2% MPBS (200 µl/well) for 1-2h at room temperature. The plate was washed 3 times with PBS, then Fab containing bacterial supernatants were added and the plate was incubated at room temperature for 1h. After another 3 washing steps with PBS, anti-FLAG-HRP secondary antibody (1:4000) or anti-T7-HRP secondary antibody (1:10000) was added and the plate was incubated for 1h at room temperature. The plate was washed 3 times with PBS and developed by adding 100ul/well BM Blue POD (Roche). The enzymatic reaction was stopped by adding 50ul/well 1M H2SO4. The OD was read at 450 nm (reference at 900 nm) for a final read-out of OD450-900. Clones specifically binding to HLA-A2/MAGE-A4_{230-239} complex but not to biotinylated HLA-A2/ WT1_{37-45} complex were sequenced and forwarded to IgG conversion for further characterization in cell activation assays.\nMAGE-A4 TCB generation: Cloning of variable antibody domains into expression vectors\n\nAll Fabs demonstrating specific binding to HLA-A2/MAGE-A4_{230-239} complex by ELISA were converted into an IgG1/kappa antibody with PG LALA mutation on Fc. Therefore, the PCR-amplified DNA fragments of heavy and light chain v-domains were inserted in frame into either the human IgG1 constant heavy chain or the human constant kappa light chain containing respective recipient mammalian expression vector. The antibody expression was driven by an MPSV promoter and transcription was terminated by a synthetic polyA signal sequence located downstream of the CDS. In addition to the expression cassette, each vector contained an EBV oriP sequence for autonomous replication in EBV-EBNA expressing cell lines.\n\nMAGE-A4 TCB generation: Surface plasmon resonance for affinity characterization of IgG and TCB to HLA-A2/MAGE-A4_{230-239} complex\n\nSpecific binders identified by cell activation assays were characterized for their binding properties by surface plasmon resonance-screening (SPR) of hu IgG PGLALA using BioRad’s ProteOn XPR36 biosensor.\n\nSPR experiments were performed on a Biacore T200 with HBS-EP+ as running buffer (0.01 M HEPES pH 7.4, 0.15 M NaCl, 0.005% Surfactant P20 (BR-1006-69, GE Healthcare)). Anti-human Fc specific antibodies (GE Healthcare BR-1008-39) were directly immobilized by amine coupling on a CM5 chip (GE Healthcare). The IgGs or T cell bispecific constructs were captured for 60 s at 2.5 nM. A three-fold dilution serie of the refolded HLA-A2/MAGE-A4_{230-239} complex was passed over the ligand at 30 ml/min for 240 sec to record the association phase. The dissociation phase was monitored for 240 s and triggered by switching from the sample solution to HBS-EP+. The chip surface was regenerated after every cycle using two injections of 3M MgCl2 for 30 sec. Bulk refractive index differences were corrected for by subtracting the response obtained on the reference flow cell 1. The affinity constants were derived from the kinetic rate constants by fitting to a 1:1 Langmuir binding using the Biaeval software (GE Healthcare). The measure was performed in triplicate with independent dilution series.\nTargeted MS assay for validation of GVYDGREHTV HLA-presentation in A375 cells\n\nCell pellets were lysed in a hypotonic buffer (Hepes 50mM pH7) containing 1% non-ionic detergent (NP40) and protease inhibitors. Xenografts tissues have been homogenized in the same buffer using a Potter-Elvehjem tissue grinder. Lysates have been cleared by centrifugation. After immunoprecipitation of HLA-A2 molecules with biotinylated mouse anti-HLA-A2 (clone BB7.2; Biolegend) antibody, protein-peptides complexes were purified on streptavidin cartridges using the AssayMAP Bravo automated platform (Agilent). HLA-associated peptides were eluted and purified with reverse phase cartridges using the AssayMAP Bravo automated platform (Agilent). Eluted peptides were lyophilized using an Eppendorf Concentrator. Lyophilized peptides were resuspended in 2% acetonitrile and 5% formic acid solution, containing an isotopically labeled GVYDGREHTV [U-13C5,15N-Val] reference peptide. Peptide composition was analyzed by liquid chromatography (nano capillary system, Dionex Corporation, Sunnyvale, CA, USA) on a C18 reversed-phase nano-high-performance liquid chromatography column connected to a mass spectrometer (Q-Exactive HF-X, Thermo, CA, USA) via electrospray ionization (LC–ESI–MS/MS). Total AUC per peptide is the sum of areas under the curve for three [GVYDGREHTV] mass spectrometric transitions from the doubly charged precursor ion (m/z: 569.7796): Y [y8] ion (m/z=976.4483); D [y7] (m/z=813.3850); G [y6] (m/z=698.3580). Complex quantification has been calculated as the average ratio of endogenous [GVYDGREHTV] peptide area under the curve (AUC) by comparison to spiked-in isotopically labeled [GVYDGREHTV] peptide AUC. The estimated copy number of endogenous [GVYDGREHTV] per cell is calculated by comparison to a spiked-in isotopically labeled [GVYDGREHTV] peptide, assuming 100% recovery for both standard and endogenous peptides at the end of the workflow.\n\nInteractome Assay: HLA-ligand purification\n\nAll TCR-like TCB antibodies were purified from transiently transfected HEK293-EBNA or CHO cells via protein A affinity chromatography and size exclusion chromatography(33-35). HLA-class II antibody was purified from\nhybridoma supernatants (clone SPVL3) using Protein A/G Sepharose beads (GE healthcare). Cross-linking of purified antibodies was performed as follows: 500 µg of antibody per 0.25 ml Protein A/G-bead mixture was incubated for 1 h at 4°C and then washed with 5 ml borate buffer (0.05 M boric acid, 0.05 M KCl, 4 mM NaOH, pH 8.0), and cross-linked with 5 ml of 40 mM dimethyl pimelimidate in borate buffer. After 30 min, crosslinking was terminated by addition of 5 ml ice-cold 0.2 M Tris pH 8.0 and the beads were washed three times with 5 ml 50 ml Tris pH 8.0. 100 mg of xenograft material or healthy tissue were lysed in a Precellys Evolution tissue homogenizer (Bertin Instruments) in 1 ml lysis buffer (0.5% (v/v) IGEPAL 630, 50 mM Tris pH 8.0, 150 mM NaCl and 1 tablet cOmplete Protease Inhibitor Cocktail EDTA-free (Roche) per 10 ml buffer) at 4°C. Lysate clarification was achieved by centrifugation at 3,000 x g for 10 mins followed by a 20,000 × g spin step for 60 min at 4°C. Lysates were pre-cleared with 1.5 ml of Protein A/G-bead mixture, and then incubated with antibody beads for at least 5 h at 4°C with gentle rotation. The antibody-resin was then washed sequentially with 5 ml of 50 mM Tris pH 8.0 containing 150 mM NaCl, 450 mM NaCl and lastly, no salt. Peptides were eluted from the captured HLA-complexes by addition of 1.5 ml of 10% acetic acid and dried by vacuum centrifugation. Peptides were further purified by solid phase extraction (Oasis columns, Waters) following the manufacturer's instructions. Further purification from larger protein material was achieved through filtering through a MWCO filter (Ultrafree-MC-PLHCC (5K) Filter, Millipore). Purified peptides were then dried and resuspended in 20 µl of loading buffer (1%ACN, 0.1% TFA in water) for LC-MS analysis.\n\nInteractome Assay: Liquid chromatography - mass spectrometric (LC-MS) acquisition and analysis\n\nAll experiments were performed in triplicates. Peptides were analysed by an Ultimate 3000 HPLC system coupled to a high field Q-Exactive (HFX) Orbitrap mass spectrometer (Thermo Scientific). Peptides were initially trapped in loading solvent, before RP separation with a 60 min linear acetonitrile in water gradient of 2-25% across a 75 µm × 50 cm PepMap RSLC C18 EasySpray column (Thermo Scientific) at a flow rate of 250 nl/min. Gradient solvents contained additional 1%(v/v) DMSO and 0.1%(v/v) formic acid. An EasySpray source was used to ionize\npeptides at 2000 V, and peptide ions were introduced to the MS at an on transfer tube temperature of 305°C.\n\nIons were analysed by data-dependent acquisition. Initially a full-MS1 scan (120,000 resolution, 60 ms accumulation time, AGC 3X10^6) was followed by 20 data-dependent MS2 scans (60,000 resolution, 120 ms accumulation time, AGC 5X10^5), with an isolation width of 1.6 m/z and normalized HCD energy of 25%. Dynamic exclusion was set for 30 s.\n\nRaw data files were analysed in Progenesis (Nonlinear Dynamics, Waters), and spectral identification was performed with PEAKS X software (Bioinformatic Solutions) using a protein sequence fasta file containing 20,397 reviewed human Uniprot entries downloaded on 04.03.2020. No enzyme specificity was set, peptide mass error tolerances were set at 5 ppm for precursors and 0.03 Da for MS2 fragments. Additionally, post translational modifications were identified utilizing the Peaks PTM inbuilt de novo-led search for 303 common modifications. A score cutoff of -10lgP=20 was chosen to result in an acceptable false discovery rate (FDR) below 5.5%.\n\nSignificant changes between samples and in peptide abundance were calculated using the inbuild PCA and Anova evaluation in Progenesis. NetMHCpan 4.1 (services.healthtech.dtu.dk) was used to predict HLA peptide sequences to the regarding alleles present in the A375 cell line. Sequence logos were generated by Seq2logo2.0 and GibbsCluster2.0 (services.healthtech.dtu.dk).\n\nJurkat NFAT activation assay\n\nTCB antibody dilutions were prepared in RPMI assay medium. A dilution row of 7 dilutions (1:10) was prepared by transferring and mixing 10 μL (starting with 110 μL/well in row A) to the subsequent wells containing 100 uL/well of RPMI media. T2 cells were washed with PBS and their viability was determined by Trypan Blue stain using EVE cell counter (>90%). T2 cells were pulsed with peptides (cells were incubated in 1 ml media at a density of 1 mio/ml in IMDM 10 % FCS in the presence of 1x10-4M – 1x10-9M POTP or control RMF peptide for 2 hrs at 37°C and washed with IMDM 10% FCS). Cells were resuspended in 2.5 ml IMDM 10% FCS to obtain a cell density of 400 000 cells per ml and 50 μl of this cell suspension were plated per well of a 96-well U- bottom well plate.\nThis corresponds to 20 000 target cells per well. Jurkat NFAT effector cells were counted (their viability was >90% (determined by Trypan Blue stain using EVE cell counter (NanoTek)) and adjusted to 2.0 Mio/ml in RPMI 10% FCS. 50 µl of the cell suspension (100 000 cells) were transferred to the wells of the assay plates, containing TCB and target cells to final E:T ratio of 5:1.\n\n100µl of the antibody dilutions or medium were added per well, followed by 100 000 Jurkat NFAT effector cells and 20 000 target cells. The final E:T was 5:1 and the final volume per well was 200 ul. Assay plates were covered with lids, and incubated for 6 hrs for endpoint measurements, at 37°C in a humidified CO2. Roughly 1h before the readout, the appropriate amount of frozen aliquots of prepared ONE-Glo solution was thawed at room temperature. The assay plates were taken out of the incubator and 100 µl were removed from each well. ONE-Glo solution was added in equivalent volumes (1:1 v/v of substrate solution and total assay medium per well; here either 100 µl ONE-Glo per well). The wells were mixed thoroughly by pipetting up and down and the mixture was transferred into white plates, which were then incubated for 10 min at room temperature in the dark, while shaking to allow lysis of target cells. Luminescence was measured using Perkin Elmer (for 96 well plates).\n\nT-cell-dependent lysis assay\n\nCo-cultures of HLA-A*02:01 human primary cells/organoids/OoC and allogenic peripheral blood mononuclear cells (PBMC) from healthy donors (purchased at Lonza and StemCell Technologies) were exposed to increasing concentrations of MAGE-A4 TCB and in vitro cytotoxicity evaluated with the most appropriate readout in all systems at 72h. The in vitro assays were controlled by testing co-cultures upon incubation in medium only. The negative control DP47 (a non-tumor targeted, CD3 TCB) and the positive control ESK1 TCB (a non-selective HLA-A*02:01/WT1 molecule targeting multiple peptide-HLA-A*02:01 complexes, also referred to as “ESK1”) were assayed side by side with MAGE-A4 TCB.\n\nFor the lung, a 3D lung-on-chip constituted of alveolar type 1 and type 2 epithelial cells isolated from fresh lung tissue and seeded on a porous breathing membrane to mimic the alveolar barrier was used as described in Stucki et al 2018. After verification of the HLA-A02 haplotype, allogenic PBMCs prior stained with a proliferation dye\n(CellTrace #C34564, Life technologies) were added to the chip and apoptosis measured by live incubation with a Caspase 3/7 fluorescent probe (CellEvent #C34564, Thermofisher) later imaged by microscopy (EVOS M700) and analyzed with the Image J software.\n\nFor the liver, liver spheroids were generated with same-donor primary human hepatocytes and liver non-parenchymal cells as previously described (Bell, 2016) and pre-characterized for HLA-A02 haplotype (provided by Kaly-cell, Cytes Biotechnologies or Lonza). The spheroids were treated with antibodies in co-culture with allogenic PBMC. Hepatotoxicity was assessed by monitoring Aspartate Transaminase (AST) activity using commercially available test kits (Bayer EC 1.1.1.27) on an ADVIA 1650 autoanalyzer (Bayer HealthCare AG) according to the manufacturer’s instructions.\n\nFor the intestine, duodenum- and colon-derived organoids were expanded from primary patient intestinal samples as previously described (Sato et al, 2011) and grown in “differentiation” conditions using commercially available media (#06010, #100-0212, #100-0191, Stemcell Technologies). Once reached maturation, organoids were passaged and resuspended in 50% Matrigel (#356231, Corning) with allogenic PBMC. The day after, treatments were added together with a Caspase 3/7 fluorescent probe (CellEvent #C34564, Thermofisher). Co-cultures were imaged using the Operetta High-Content Imaging System (PerkinElmer) and organoid apoptosis later quantified by measuring the total fluorescence signal of the Caspase-3/7 Green Detection Reagent per well (ImageJ software).\nREFERENCES\n\n1. E. Dolgin, First soluble TCR therapy opens 'new universe' of cancer targets. Nat Biotechnol, (2022).\n2. N. Liddy et al., Monoclonal TCR-redirected tumor cell killing. Nat Med 18, 980-987 (2012).\n3. M. R. Middleton et al., Tebentafusp, A TCR/Anti-CD3 Bispecific Fusion Protein Targeting gp100, Potently Activated Antitumor Immune Responses in Patients with Metastatic Melanoma. Clin Cancer Res 26, 5869-5878 (2020).\n4. P. Nathan et al., Overall Survival Benefit with Tebentafusp in Metastatic Uveal Melanoma. N Engl J Med 385, 1196-1206 (2021).\n5. G. P. Linette et al., Cardiovascular toxicity and titin cross-reactivity of affinity-enhanced T cells in myeloma and melanoma. Blood 122, 863-871 (2013).\n6. A. D. Martin et al., Re-examination of MAGE-A3 as a T-cell Therapeutic Target. J Immunother 44, 95-105 (2021).\n7. C. Jost et al., CAR-J cells for antibody discovery and lead optimization of TCR-like immunoglobulins. MAbs 12, 1840709 (2020).\n8. F. Crawford et al., Use of baculovirus MHC/peptide display libraries to characterize T-cell receptor ligands. Immunol Rev 210, 156-170 (2006).\n9. M. E. Birnbaum et al., Deconstructing the peptide-MHC specificity of T cell recognition. Cell 157, 1073-1087 (2014).\n10. A. K. Bentzen et al., Large-scale detection of antigen-specific T cells using peptide-MHC-I multimers labeled with DNA barcodes. Nat Biotechnol 34, 1037-1045 (2016).\n11. M. H. Gee et al., Antigen Identification for Orphan T Cell Receptors Expressed on Tumor-Infiltrating Lymphocytes. Cell 172, 549-563 e516 (2018).\n12. S. Q. Zhang et al., High-throughput determination of the antigen specificities of T cell receptors in single cells. Nat Biotechnol, (2018).\n13. A. R. Karapetyan et al., TCR Fingerprinting and Off-Target Peptide Identification. Front Immunol 10, 2501 (2019).\n14. C. J. Holland et al., Specificity of bispecific T cell receptors and antibodies targeting peptide-HLA. J Clin Invest 130, 2673-2688 (2020).\n15. I. Springer, H. Besser, N. Tickotsky-Moskovitz, S. Dvorkin, Y. Louzoun, Prediction of Specific TCR-Peptide Binding From Large Dictionaries of TCR-Peptide Pairs. Front Immunol 11, 1803 (2020).\n16. W. D. Chronister et al., TCRMatch: Predicting T-Cell Receptor Specificity Based on Sequence Similarity to Previously Characterized Receptors. Front Immunol 12, 640725 (2021).\n17. A. M. Luu, J. R. Leistico, T. Miller, S. Kim, J. S. Song, Predicting TCR-Epitope Binding Specificity Using Deep Metric Learning and Multimodal Learning. Genes (Basel) 12, (2021).\n18. A. Montemurro et al., NetTCR-2.0 enables accurate prediction of TCR-peptide binding by using paired TCRAalpha and beta sequence data. Commun Biol 4, 1060 (2021).\n19. E. Jokinen, J. Huhtanen, S. Mustjoki, M. Heinonen, H. Lahdesmaki, Predicting recognition between T cell receptors and epitopes with TCRGP. PLoS Comput Biol 17, e1008814 (2021).\n20. T. P. Riley et al., T cell receptor cross-reactivity expanded by dramatic peptide-MHC adaptability. Nat Chem Biol 14, 934-942 (2018).\n21. H. F. Jones, Z. Molvi, M. G. Klatt, T. Dao, D. A. Scheinberg, Empirical and Rational Design of T Cell Receptor-Based Immunotherapies. Front Immunol 11, 585385 (2020).\n22. A. W. Purcell, S. H. Ramarathinam, N. Ternette, Mass spectrometry-based identification of MHC-bound peptides for immunopeptidomics. Nat Protoc 14, 1687-1707 (2019).\n23. T. Dao et al., Therapeutic bispecific T-cell engager antibody targeting the intracellular oncoprotein WT1. Nat Biotechnol 33, 1079-1086 (2015).\n24. R. S. Gejman et al., Identification of the Targets of T-cell Receptor Therapeutic Agents and Cells by Use of a High-Throughput Genetic Platform. Cancer Immunol Res 8, 672-684 (2020).\n25. N. Ataie et al., Structure of a TCR-Mimic Antibody with Target Predicts Pharmacogenetics. J Mol Biol 428, 194-205 (2016).\n26. C. Klein et al., Engineering therapeutic bispecific antibodies using CrossMab technology. Methods 154, 21-31 (2019).\n27. T. Schlothauer et al., Novel human IgG1 and IgG4 Fc-engineered antibodies with completely abolished immune effector functions. Protein Eng Des Sel 29, 457-466 (2016).\n28. S. Chtarbova et al., Murine Nr4a1 and Herpud1 are up-regulated by Wnt-1, but the homologous human genes are independent from beta-catenin activation. Biochem J 367, 723-728 (2002).\n29. S. Herter et al., GA101 P329GLALA, a variant of obinutuzumab with abolished ADCC, ADCP and CDC function but retained cell death induction, is as efficient as rituximab in B-cell depletion and antitumor activity. Haematologica 103, e78-e81 (2018).\n30. M. F. Kotturi et al., Of mice and humans: how good are HLA transgenic mice as a model of human immune responses? Immunome Res 5, 3 (2009).\n31. J. Fritsche et al., Pitfalls in HLA ligandomics - How to catch a li(e)gand. Mol Cell Proteomics, 100110 (2021).\n32. P. Dash et al., Quantifiable predictive features define epitope-specific T cell receptor repertoires. Nature 547, 89-93 (2017).\n33. M. Bacac et al., CD20-TCB with Obinutuzumab Pretreatment as Next-Generation Treatment of Hematologic Malignancies. Clin Cancer Res 24, 4785-4797 (2018).\n34. M. Bacac et al., A Novel Carcinoembryonic Antigen T-Cell Bispecific Antibody (CEA TCB) for the Treatment of Solid Tumors. Clin Cancer Res 22, 3286-3297 (2016).\n35. A. Seckinger et al., Target Expression, Generation, Preclinical Activity, and Pharmacokinetics of the BCMA-T Cell Bispecific Antibody EM801 for Multiple Myeloma Treatment. Cancer Cell 31, 396-410 (2017).\n\nACKNOWLEDGEMENT\n\nWe thank Prof. Christian Brander and Dr. Christoph T. Berger for critical review of the manuscript. The Hybridoma clone SPVL3 was a gift from Prof. Anthony Purcell.\n\nCOMPETING INTERESTS\n\nNT is or has been a paid consultant Roche Pharma, Grey Wolf Therapeutics, T-Cypher Bio, Infinitopes, and Enara Bio.\n\nDATA AVAILABILITY\n\nAll data will be made available to academic researchers upon reasonable request.\nTABLES\n\nTable 1: TCB-enriched peptides identified in primary liver tissue. +: Positive signal in JNFAT assay, ++: Positive signal in JNFAT assay higher than ESK1-target peptide, -: negative in JNFAT assay. Red highlighted: Positive signal in presence of ESK1-TCR in JNFAT assay.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
NameSequenceA*02:01 AccessionProtein NameIntensity Ratio (ESK1/MAGE)-log(p)Esk1 JNFAT signal
ILF2127-135KILPTLEAV0.051 Q12905Interleukin enhancer-binding factor 264.04.59+
RBM4B59-67KLHGVNINV0.03 Q9BQ04RNA-binding protein 4B84.42.94++
RLS117-125KIYEGQVEV0.004 P4677760S ribosomal protein L54.62.67-
SEPT2121-129YIDEQFERY1.77 Q15019Septin-24.32.19-
SET150-158KVLSKEFHL0.324 Q01105Protein SET48.53.76-
SF3B478-86KLYGKPIRV0.004 Q15427Splicing factor 3B subunit 4238.91.93+
SHC1469-477RVPPPPPQSV0.183 P29353SHC-transforming protein 15.32.7++
ARHGFEF26863-871RLLLGLETNV0.059 Q96DR7Rho guanine nucleotide exchange factor 26181.01.8++
CRYL1130-138KLFAGLVHV0.004 Q9Y2S2Lambda-crystallin homolog256.03.36++
MSMO1164-172RIKYIHKV0.03 Q15800Methylsterol monooxygenase 113.02.94-
CYP2C859-67KVYGPVFTV0.011 P10632Cytochrome P450 2C822.63.6++
USP9Y1674-1682RLWGEVPVNL0.014 O00507Prob. ubiquitin carboxyl-terminal hydrolase FAF-Y27.93.95++
PLG92-100VLFEEKVYL0.008 P00747Plasminogen4.92.67-
MAF116-124ALISNSHQL0.038 Q75444Transcription factor Maf3.03-
ALDOA216-224ALSDDHIYL0.011 P04075Fructose-bisphosphate aldolase A3.52-
HNRNPA115-23KLFIGGLSF1.625 P09651Heterogeneous nuclear ribonucleoprotein A15.33.57-
EIF3F348-357IALNEKLVNL0.613 O00303Eukaryotic translation initiation factor 3 subunit F0.41.99-
\nTable 2: Change of the solvent-accessible surface area (ΔSASA) of the RMF peptide in the absence of the ESK1 Fab (calculated from the X-ray crystal structure with PDB ID 4WUU) and comparison to the confirmed cross-reactive peptides, ordered by their signal in the JNFAT activation assay. Bold font, red: Amino acid identical to respective residue in RMF peptide. Grey background: HLA anchor residues.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Position123456789
WT126_134 (RMF)RMFPNAPYL
ΔSASA without ESK169.10.00.035.715.10.00.00.00.0
Interacts with ESK1✓xx(✓)xxxxx
SHC1469-477RVPPPPQSV
ARHGEF26863-871RLLGLETNV
RBM4B59-67KLHGVNINV
USP9Y1674-1682RLWGEPVNL
CYP2C859-67KVYGPVFTV
CRYL1130-138KLFAGLVHV
SF3B478-86KLYGKPIRV
\nFIGURE LEGENDS\n\nFigure 1: An experimental framework de novo identifies on-target binding of the novel, functional MAGE-A4-specific TCB recognizing the peptide GYVDGREHTV presented by HLA-A*02:01. (A) Schematic of the MAGE-A4 TCB and its mode of action. (B) Average ratio of endogenous GYVDGREHTV peptide area under the curve (AUC) by comparison to spiked-in isotopically labeled GYVDGREHTV peptide AUC (n=4), measured in elution fractions from HLA-A2 immunoprecipitation in A375 tumor cells lines and MAGE-A4 KO (A375-KO) and equivalent lines in a xenograft model (XA375 and XA375-KO). Error bars represent standard error of the mean (SEM). The estimated copy number of endogenous GYVDGREHTV per cell (shown on top of each bar graph) is calculated by comparison to a spiked-in isotopically labeled GYVDGREHTV peptide, assuming 100% recovery for both standard and endogenous peptides at the end of the workflow. (C) A375 wild type cells and A375-KO cells were incubated with human PBMCs at an E:T ratio of 10:1. Depicted are dose-response curves of tumor cell lysis after 24 hours of incubation with different concentrations of MAGE-A4 TCB as determined by quantification of LDH release in the supernatant (triplicates with SD). (D) Schematic workflow using TCR-like antibodies to enrich interacting HLA-peptide complexes. Tissues were lysed, and solubilized HLA-peptide complexes were immunoprecipitated using the MAGE-A4 tool antibody as a bait. Peptides were enriched in acidic conditions through a 5 kDa molecular weight cut-off filter, and analysed by LC-MS² (E) Peptide intensity as measured in three biological replicate analyses demonstrates significant enrichment (p=1.5·10E-3) of the target peptide GYVDGREHTV in XA375, and not in MAGE-KO equivalent tissues (F) LC-MS spectrum leading to identification of the target peptide GYVDGREHTV in XA375 after enrichment using the MAGE-A4 IgG. The spectral identifier, the measured mass of the precursor peptide ion (m/z), charge state (z), and retention time (RT), at which the peptide ion was selected for fragmentation, are stated within the spectral panel. C-terminal fragment ions are indicated as “y”, N-terminal fragments are designated “b”, pre: unfragmented precursor peptide, +: singly charged ion, ++: doubly charged ion.\nFigure 2: Off-target interaction of ESK1 with common HLAp sequences in primary liver tissue. (A) Volcano plots showing significant enrichment of peptides for ESK1 and MAGE-A4 in liver tissue (all peptide, left panel; peptides predicted to bind to HLA-A*02:01 (B) Sequence motif of the ESK1-enriched peptides that are predicted to bind to HLA-A*02:01. Shown is the frequency (probability) of each amino acid in each position across the peptide sequence from N- to C-terminus (left to right, positions 1-9). (C) Sequence motifs from Gejman et al. (left panel) and our study (right panel). (D) Venn diagram depicting the lack of overlap of peptide sequences shortlisted by Gejman et al. and our study as Esk1 binders.\n\nFigure 3: Off-target binding activates effector cells and conveys killing of liver spheroids in the presence of ESK1. (A) T2 cells were first pulsed with the 16 ESK1-enriched peptides and then co-incubated with JNFAT effector cells in the presence of different concentrations of ESK1 TCB. The target peptide (WT1_{126-134}) was used as positive control, while WT1_{37-45}, a non-relevant peptide was used as negative control. Effector cells activation was evaluated after 6 hrs by measuring luminescence signal using ONEGlo. (B) Equivalent to (A) using MAGE-A4 TCB, and MAGE-A4 target peptide huMAGA4_{230-239} as a control. (C) Titration curves for JNFAT assay with indicated peptides and ESK1 TCB concentrations. (D) Liver spheroids were cocultured with peripheral blood mononuclear cells at a ratio of 5 effector to 1 target cell and target cell killing evaluated by granzyme B secretion and aspartate aminotransferase expression. Values were normalized to the non-targeted control TCB. Each graph represents two independent experiments with two independent human donors in quadruplicates.\n\nFigure 4: Structural mimicry is a feature of ESK1 off-target activity. (A) Overlay of RMF (purple, from X-ray structure with PDB ID 4WUU) with models of the confirmed cross-reactive peptides in the presence of the Fab of ESK1. The HLA-A*02:01 peptide binding groove is indicated in grey. The numbers indicate the approximate position of the amino acid side chain at the respective peptide position. (B) RMF peptide within the HLA-A*02:01 binding groove and interactions with the ESK1 Fab (PDB ID 4WUU). (C) Non-bonded interactions between the\nFab of ESK1 and RMF (grey) in the HLA-A*02:01-WT1RMF pMHC (X-ray crystal structure with PDB ID 4WUU).\nModels of the cross-reactive peptides huSHC1469-477 (cyan) and huRBM4B59-67 (orange) are shown for comparison. (D) Overlay of RMF peptide (purple, from X-ray structure with PDB ID 4WUU) with modeled huRBM4B59-67 peptide (cyan) in the peptide binding groove of HLA-A*02:01.\n\nFigure 5: MAGEA4 TCB is a highly specific clinical therapeutic candidate. (B) Lung alveolus-on-chip and intestinal differentiated organoids were cocultured with peripheral blood mononuclear cells at a ratio of 5 effector to 1 target cell and target cell killing evaluated by caspase 3/7 probe imaging. Values were normalized to the non-targeted control TCB. A dashed line was added to the Y axis to indicate the control TCB threshold. Each graph represents two independent experiments with two independent human donors in triplicates.\nFIGURES\n\nFIGURE1\n\nA\n\n![Diagram showing cancer cell with MAGE-A4 and HLA antigens, and T-cell interaction](page_232_256_768_256.png)\n\nB\n\n![Bar graph comparing AUC ratio sample/standard peptide for different cell lines](page_232_512_384_256.png)\n\nC\n\n![Line graph showing % tumor cell lysis over concentration (nM) for A375 and A375 MAGE-A4 ko](page_616_512_384_256.png)\n\nD\n\n![Diagram showing tissue sample, TCR-like antibody-directed HLA-I complex purification, acid elution and filtration, LC-MS/MS acquisition and sequence annotation](page_232_768_768_256.png)\n\nE\n\n![Bar graph comparing signal intensity for GVYDGREHTV peptide in different samples](page_232_1024_384_256.png)\n\nF\n\n![Mass spectrum and sequence annotation for GVYDGREHTV peptide](page_616_1024_384_256.png)\nFIGURE2\n\nA\n\nLiver (tissue)\nLiver (HLA-A*02:01)\n\nB\n\nprobability\nWebLogo 3.7.4\n\nC\nGejman et al. 2020 (27 sequences)\nOUR STUDY (16 sequences)\n\nD\nGejman et al. 2020\nOur Study\nFIGURE3\n\nA\n\nB\n\nC\n\nD\nFIGURE4\n\nA\nB\nRMFPNAPYL\n\nC\nRVPPPOSV (cyan)\nKLHGVNINV (orange)\nRMFPNAPYL (grey)\n\nD\nKLHGVNINV (cyan)\nRMFPNAPYL (purple)\nFIGURE 5\n\nA\n\nLung (tissue)\nLung (HLA-A*02:01)\nIntestine (tissue)\nIntestine (HLA-A*02:01)\n\nB\n\nLung (alveolus on chip)\nIntestine (differentiated organoids)\nApoptosis (caspase 3/7)\nApoptosis (caspase 9/7)\nMAGEA4 TCB\nESK1 TCB\n\n![Scatter plots showing gene expression and apoptosis data for lung and intestine tissues, and alveolus on chip and differentiated organoids](page_186_180_1207_495.png)\nSUPPLEMENTARY MATERIAL\n\nSUPPLEMENTARY FIGURE 1\n\n\n \n \n \n \n \n \n \n \n
pMHC affinityCD3 Affinity
\n \\( K_D = 40 \\)nM (25°C)
\n \\( k_a = 1.1 +/- 0.0 E+06 \\) 1/Ms (25°C)
\n \\( k_d = 4.3E-02 +/- 0.1 E-02 \\) 1/s (25°C)\n
\n \\( K_D = 3.7 +/- 0.8 \\) nM (25°C)
\n \\( 11.3 +/- 0.1 \\) nM (37°C)
\n \\( k_a = 1.4 +/- 0.0 E+05 \\) 1/Ms (25°C)
\n \\( k_d = 1.6 +/- 0.0 E-03 \\) 1/s (25°C)\n
\n\n\\( K_D \\), equilibrium dissociation constant; \\( k_a \\), association rate constant; \\( k_d \\), dissociation rate constant.\n\nSupplementary Figure 1: Association and dissociation constants for HLA-A*02- GVYDGREHTV and CD3 epsilon\nSUPPLEMENTARY FIGURE 2\n\n![Bar graph showing peptide signal intensity for YDGREHTV in different groups: MAGE-A4 (XA375), MAGE-A4 (XA375-KO), CTRL (XA375), CTRL (XA375-KO). The MAGE-A4 (XA375) group shows significantly higher signal intensity compared to others, indicated by ****.](page_186_222_627_393.png)\n\nSupplementary Figure 2: Significant enrichment (Anova p<0.0001) of a fragment of the target peptide GVYDGREHTV, the 8mer sequence YDGREHTV, in A375 Xenografts using the MAGE A4 antibody as a bait.\nSUPPLEMENTARY FIGURE 3\n\n![Scatter plot showing correlation between ESK1 HLAp enrichment ratio and maximal RLU in Jurkat reporter assay](page_246_370_579_482.png)\n\nSupplementary Figure 3: No correlation could be observed between the detected ESK1 HLAp enrichment ratio and the measured maximal RLU in a Jurkat reporter assay using peptide-pulsed T2 cells in the presence of ESK1.\nSupplementary Table S1: Gejman et al. Identified ESK1-binding sequences and their expression profiles in liver tissue\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Peptide SequenceESK1 bindingNatureProtein originExpression in the liver
RMFPNAPYLyescontrolsp|P19544|WT1_HUMANNot detected
RMFWNAPYLyescontrolsp|P19544|WT1_HUMAN, 1 aa substitutionna
RMFGNAPYLyescontrolsp|P19544|WT1_HUMAN, 1 aa substitutionna
QLQNPSYDKnocontrolno match
RAFPNAPYVnopredictedsp|P19544|WT1_HUMAN, 2 aa substitutionna
RLLPDFFGVyespredictedsp|Q96S15|WDR24_HUMANHepatocytes: medium, Cholangiocytes: low
RLFPLASLVyespredictedsp|Q9NY72|SCN3B_HUMANNot detected
RVLPNLVAVyespredictedsp|Q8IY22|CMIP_HUMANHepatocytes: low, Cholangiocytes: low
RMFPNAFLYyespredictedsp|P19544|WT1_HUMAN, 1 aa substitutionNot detected
RVMPCLAEVyespredictedsp|Q6ZMD2|SPNS3_HUMANNot detected
RLFPLAWTVyespredictedsp|P20827|EFNA1_HUMANNot detected
RLLPLPLGVyespredictedsp|Q8NDA2|HMCN2_HUMANNot detected
RLLPLLNSVyespredictedsp|Q8IU68|TMC8_HUMAN; sp|Q5STAT6|CODA1_HUMAN;Hepatocytes: medium
RLLPLLRTVyespredictedsp|P52798|EFNA4_HUMANHepatocytes: Low
RLWPSLAVSyespredictedno match
RVMPSSFFLyespredictedsp|O75663|TIPRL_HUMANHepatocytes: low
RMFFNAPYLyespredictedsp|P19544|WT1_HUMAN, 1 aa substitutionna
RLWPQGRGVyespredictedsp|Q9UQQ1-6|NALDL_HUMANNot detected
RVLPAAFLVyespredictedtr|AOA075B7D9.1|TAF15_HUMANHepatocytes: high; Cholangiocytes: medium
RILPLFQGVyespredictedsp|Q9UN76|S6A14_HUMANNot detected
RIIPYLIHVyespredictedsp|P56645|PER3_HUMANHepatocytes: high; Cholangiocytes: medium
RLLPALASVyespredictedsp|Q03154|ACY1_HUMANHepatocytes: high; Cholangiocytes: low
KLMGAISFFIyespredictedsp|Q8NF4M|ADCY4_HUMANHepatocytes: low; Cholangiocytes: low
MNLNVIAIVnopredictedsp|Q8IZF0|NALCN_HUMANNot detected
RVIMPCNWVVyespredictedsp|Q9H2S6|TNMD_HUMANNot detected
RLLGGMALLLyespredictedsp|Q9NX94-2|WBP1L_HUMANNot detected
RLMAMVDVLVyespredictedsp|Q8NFP9|NBEA_HUMANNot detected
KTDPTVLLFVnopredictedsp|Q9H3R1|NDST4_HUMANNot detected
RMFSGVGVYLyespredictedsp|Q969Y0|NXPE3_HUMANNot detected
ALLTAALWYInopredictedsp|P17813|EGLN_HUMANNot detected
YIHFTPNFLLnopredictedsp|Q9UQC9|CLCA2_HUMAN; sp|Q9Y6N3|CLCA3_HUMANNot detected
"} {"paper_id": "prb76", "title": "", "text": "Transgenic T cell therapy targeting the glioblastoma stem cell antigen PTPRZ1 with a vaccine-induced, patient-derived T cell receptor\n\nLukas Bunse\nl.bunse@dkfz.de\n\nGerman Cancer Research Center https://orcid.org/0000-0002-4490-7574\n\nYu-Chan Chih\nGerman Cancer Research Center\n\nAmelie Christina Dietsch\nGerman Cancer Research Center\n\nPhilipp Koopmann\nGerman Cancer Research Center\n\nXiujuan Ma\nGerman Cancer Research Center\n\nDennis Alexander Agardy\nGerman Cancer Research Center\n\nBinghao Zhao\nGerman Cancer Research Center\n\nAlice De Roia\nGerman Cancer Research Center\n\nAlexandros Kourtessakis\nGerman Cancer Research Center\n\nMichael Kilian\nAnn Romney Center for Neurologic Diseases, Brigham and Women's Hospital, Harvard Medical School\n\nChristopher Krämer\nGerman Cancer Research Center\n\nAbigail K. Suwala\nInstitute for Pathology, Department of Neuropathology, Heidelberg University\n\nMiriam Stenzinger\nInstitute for Clinical Transfusion Medicine and Cell Therapy\n\nHalvard Bonig\nGoethe University\n\nAgnieszka Blum\nArdigen, ul. Podole 76\nVictor Pieńkowski\nArdigen, ul. Podole 76\nKuralay Aman\nGerman Cancer Research Center\nJonas P Becker\nGerman Cancer Research Center\nHenrike Feldmann\nDepartment of Neurology, Medical Faculty Mannheim, Mannheim Center for Translation Neuroscience (MCTN)\nTheresa Bunse\nGerman Cancer Research Center\nRichard Harbottle\nGerman Cancer Research Center\nAngelika B. Riemer\nGerman Cancer Research Center\nHai-Kun LIU\nGerman Cancer Research Center https://orcid.org/0000-0003-3338-4066\nNima Etminan\nDept. of Neurosurgery, University Hospital Mannheim\nFelix Sahm\nDepartment of Neuropathology, Heidelberg University Hospital, and CCU Neuropathology, German Consortium for Translational Cancer Research (DKTK), German Cancer Research Center (DKFZ), Heidelberg https://orcid.org/0000-0001-5441-1962\nMiriam Ratliff\nUniversity Hospital Mannheim https://orcid.org/0000-0002-9464-6544\nWolfgang Wick\nUniversity of Heidelberg https://orcid.org/0000-0002-6171-634X\nMichael Platten\nGerman Cancer Research Center https://orcid.org/0000-0002-4746-887X\nEdward Wilhelm Green\nGerman Cancer Research Center\n\nArticle\n\nKeywords:\n\nPosted Date: August 9th, 2024\n\nDOI: https://doi.org/10.21203/rs.3.rs-4782908/v1\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License.\nRead Full License\n\nAdditional Declarations: Yes there is potential Competing Interest. The identified reactive TCR was patented by Y-C.C., M.K., C.K., E.W.G., W.W., M.P. and L.B., “T cell receptor derived binding polypeptides” (WO 2023/213904). E.W.G. and M.P. are founders of TCellTech.\n\nVersion of Record: A version of this preprint was published at Nature Communications on February 1st, 2025. See the published version at https://doi.org/10.1038/s41467-025-56547-w.\nTransgenic T cell therapy targeting the glioblastoma stem cell antigen PTPRZ1 with a vaccine-induced, patient-derived T cell receptor\n\nAuthors: Yu-Chan Chih1,2,3,4, Amelie C. Dietsch1,2, Philipp Koopmann1,2, Xiujian Ma2,5*, Dennis A. Agardy1,2,3,4, Binghao Zhao1,2, Alice De Roia1,2,3,4,6, Alexandros Kourtseakis2,7,8, Michael Kilian1,2,4,9, Christopher Krämer1,2,4, Abigail K. Suwala2,10,11, Miriam Stenzinger1,2,13, Halvard Bonig14,15, Agnieszka Blum16, Victor Murcia Pienkowski16, Kuralay Aman1,2, Jonas P. Becker2,17,18, Henrike Feldmann3,4, Theresa Bunse1,2, Richard Harbottle2,6, Angelika B. Riemer2,17,18, Hai-Kun Liu2,5, Nima Etminan19, Felix Sahm2,10,11, Miriam Ratliff19, Wolfgang Wick2,7,8, Michael Platten1,2,4,20,21,22, Edward W. Green1,2, Lukas Bunse1,2,4,22\n\nAffiliations:\n1Clinical Cooperation Unit (CCU) Neuroimmunology and Brain Tumor Immunology, German Cancer Research Center (DKFZ), Heidelberg, Germany\n2German Cancer Consortium (DKTK), DKFZ, core center Heidelberg, Germany\n3Faculty of Biosciences, Heidelberg University, Heidelberg, Germany\n4Department of Neurology, Medical Faculty Mannheim, Mannheim Center for Translation Neuroscience (MCTN), Heidelberg University, Mannheim, Germany\n5Division of Molecular Neurogenetics, DKFZ, DKFZ-ZMBH alliance, Heidelberg, Germany\n6DNA Vector Laboratory, DKFZ, Heidelberg, Germany\n7Neurology Clinic, Heidelberg University Hospital, Heidelberg, Germany\n8CCU Neurooncology, DKFZ, Heidelberg, Germany\n9Ann Romney Center for Neurologic Diseases, Brigham and Women's Hospital, Harvard Medical School, Boston, MA, USA\n10Institute for Pathology, Department of Neuropathology, Heidelberg University, Heidelberg, Germany\n11CCU Neuropathology, DKFZ, Heidelberg, Germany\n12Institute for Clinical Transfusion Medicine and Cell Therapy, Heidelberg, Germany\n13Institute for Immunology, Heidelberg University Hospital, Heidelberg, Germany\n14Faculty of Medicine, Goethe University, Frankfurt a.M., Germany\n15Institute for Transfusion Medicine and Immunohematology, German Red Cross Blood Service Baden-Württemberg-Hessen, Frankfurt a.M., Germany\n16Ardigen, ul. Podole 76, Kraków, Poland\n17Division of Immunotherapy and Immunoprevention, DKFZ, Heidelberg, Germany\n18Molecular Vaccine Design, German Center for Infection Research (DZIF), partner site Heidelberg, Germany\n19Department of Neurosurgery, University Hospital Mannheim, Mannheim, Germany\n20Immune Monitoring Unit, National Center for Tumor Diseases (NCT), NCT Heidelberg, a partnership between DKFZ and Heidelberg University Hospital, Heidelberg, Germany\n21Helmholtz Institute for Translational Oncology Mainz (HI-TRON Mainz) – A Helmholtz Institute of the DKFZ, Mainz, Germany\n22DKFZ Hector Cancer Institute at the University Medical Center Mannheim, Mannheim, Germany\n\nABSTRACT\n\nResponse to CAR-T cell therapy in glioblastoma (GB) patients is limited, particularly because of the paucity of cell surface immunotherapeutic targets or low antigen sensitivity. Moreover, tonic CAR signaling leads to T cell dysfunction eventually resulting in non-durable responses. T cell receptor-engineered T (TCR-T) cell therapy circumvents the latter limitation by allowing safe and ubiquitous targeting of the GB-derived peptideome. Protein tyrosine phosphatase receptor type Z1 (PTPRZ1), a GB antigen associated with GB cell stemness, was previously targeted in multipeptide vaccination trials. Here, we identify a therapeutic HLA-A*02-restricted PTPRZ1-reactive TCR retrieved from a vaccinated GB patient. Single-cell sequencing of primary brain tumor samples showed *PTPRZ1* overexpression exclusively in malignant cells and most pronounced in GB stem cells and astrocyte (AC)- or oligodendrocyte-progenitor (OPC)-like cells. The validated vaccine-induced TCR recognized the endogenously processed antigen without cross-reactivity to *in silico* predicted low-risk off-targets. PTPRZ1-specific TCR-engineered human primary T cells (PTPRZ1-TCR-T) killed target cells antigen-specifically. Intravenous adoptive cell transfer against experimental brain tumors alone was not efficacious, but the addition of intracerebroventricular administration of PTPRZ1-TCR-T\nresulted in potent tumor rejection. PTPRZ1-TCR-T maintained stem cell memory phenotype *in vitro* and *in vivo*. PTPRZ1-TCR-T lysed all examined HLA-A*02+ primary GB cell lines with a preference for slow-cycling GB stem cells (GSCs) and AC-like cells. To further develop PTPRZ1-TCR-T as off-the-shelf therapy for HLA-A*02 GB patients, a phase I first-in-human clinical trial INVENT4GB is in preparation.\n\n**Main text:**\n\n**INTRODUCTION**\n\nEngineered T cell therapy has constituted a great success in combating hematopoietic cancers in the last decade with more than half of the patients demonstrating clinical responses leading to long-term survival in many studies\\(^{1-3}\\). On the other hand, its efficacy in treating solid tumors is still limited\\(^4\\). This is largely due to poor T cell infiltration, intratumoral T cell dysfunction and limited T cell persistence. These challenges are particularly pronounced in glioblastoma (GB), where the tumor is compartmentalized by the blood-brain barrier (BBB) excluding even unleashed peripheral tumor-reactive T cells, making GB one of the least responsive tumors to immunotherapies\\(^{5-8}\\).\n\nGB carries relatively few mutations\\(^9\\). Given the paucity of tumor-specific cell surface antigens, only a limited number of candidate targets can be exploited. Several chimeric antigen receptor (CAR)-T cell therapy clinical trials have been launched to target GB-associated surface antigens, e.g., IL13Ra2, HER2 and GD2, with fewer focusing on the GB-specific but subclonal antigen, EGFRvIII\\(^{10,11}\\). Primarily driven by sophisticated synthetic improvements of cellular approaches, some patients showed response to CAR-T cell therapy\\(^{12}\\). In addition, combinatorial treatments are under exploitation\\(^{13,14}\\). Unlike CARs, T cell receptors (TCRs) enable targeting both intracellular and extracellular antigens that are processed and loaded onto the major histocompatibility complex (MHC)\\(^{15}\\). This nature of antigen recognition by TCRs conceivably broadens the range of targetable antigens. Moreover, in comparison to CARs, TCRs display superior antigen sensitivity, reduced tonic signaling, and engage differential proinflammatory intracellular pathways\\(^{16,17}\\). Encouraging results have been demonstrated in Phase I and II clinical trials using TCR-engineered T cells (TCR-T) to treat solid tumors\\(^{18}\\). Despite current progress in advancing cell therapy, TCR-T cell therapy has not yet been investigated in GB patients. Previously, we have isolated and validated vaccine-induced glioma-reactive TCRs targeting the tumor-associated antigen, NLGN4X\\(^{19}\\), and neoantigens, IDH1R132H, H3K27M and CICR215W/Q\\(^{20-22}\\). In a multinational European GB immunotherapy clinical trial, Glioma Actively Personalized Vaccine Consortium 101 (GAPVAC-101), newly diagnosed GB patients were immunized with a warehouse of unmuted GB-associated peptides (APVAC1), and a warehouse of individual-specific mutated peptides (APVAC2)\\(^{23}\\). 92% of APVAC1-vaccinated patients developed MHC class I (MHC-I)-dependent immunogenicity. PTPRZ1\\(^{1814-1822}\\), an HLA-A*02-restricted epitope derived from the GB-associated antigen protein tyrosine phosphatase receptor type Z1, PTPRZ1, was administered to four patients within APVAC1 and elicited 100% immunogenicity\\(^{23,24}\\). Multimer-sorted PTPRZ1\\(^{1814-1822}\\)T cells demonstrated cytotoxicity against HLA-A*02+ GB cell lines with PTPRZ1 expression.\n\nPTPRZ1 is involved in central nervous system development\\(^{25,26}\\). Binding to its ligands, PTN and MK, leads to oligomerization and inactivation of the phosphatase receptor, resulting in sustained phosphorylation of its substrates, such as β-catenin and ALK\\(^{27,28}\\). Its absence leads to early onset of oligodendrocyte differentiation and disruption of the perineuronal net\\(^{25,29}\\).\nWhile its expression is very limited across adult tissues, it is essential for gliomagenesis. In gliomas, PTPRZ1 takes part in cancer cell proliferation, migration, and invasiveness30-32. In addition, it contributes to angiogenesis and tumor radioresistance33,34. Notably, depletion of PTPRZ1 results in significant impairment of glioma cell sphere formation *in vitro* and delays tumor growth *in vivo*, indicating a strong associated of PTPRZ1 with glioma cell stemness35,36. Recent studies have employed PTPRZ1 along with other markers to define GB stem cells (GSCs) in single-cell transcriptomic and flow cytometric analyses37,38. Here, we performed a comprehensive multimodal assessment of PTPRZ1 in GB, demonstrated that it is a highly attractive immunotherapeutic target, and developed an off-the-shelf TCR-T therapy, in principle, applicable for all HLA-A*02+ glioma patients.\n\nRESULTS\n\nPTPRZ1 is exclusively overexpressed and presented in glioma cells, and associated with distinct cellular states and stemness in GB\n\nTo evaluate the extent of PTPRZ1 association with gliomas, we first examined its expression at transcript and protein levels in human GB tissues. In TCGA bulk RNA sequencing (RNA-seq) data, *PTPRZ1* was significantly upregulated in GB compared to adjacent normal (Fig. 1A). In addition, *PTPRZ1* was overexpressed in low-grade glioma (LGG) (Fig. S1A), and its expression correlated positively with ABSOLUTE tumor purity (Fig. S1B,C)39. In order to detail *PTPRZ1* at cellular resolution, we interrogated publicly available GB and isocitrate dehydrogenase (IDH)-mutant glioma single-cell RNA-seq (scRNA-seq) datasets40,41, and found *PTPRZ1* to be highly expressed in malignant cells but not in immune cells such as T cells and macrophages, nor in normal glial cells, oligodendrocytes and microglia (Fig. 1B and Fig. S1D-H). In a paired glioma and stromal cell scRNA-seq dataset (n(GB)=16, n(IDH-mut glioma)=3, and n(pediatric high-grade glioma)=1), we independently validated malignant cell-type specificity of *PTPRZ1* expression (Fig. 1C,D and Fig. S1I,J). Interindividual levels of *PTPRZ1* overexpression varied across patients but were found in all gliomas (Fig. S1K,L). To evaluate protein abundance, we analyzed n=20 matched primary and recurrent GB samples and found patient-individual PTPRZ1 levels without temporal alterations between primary and recurrent tumors (Fig. 1E,F). In concordance with transcriptomic data using GFAP to depict tumor purity, abundance of PTPRZ1+ cells correlated positively with GFAP+ cells (Fig. 1G). To address whether PTPRZ1 upregulation leads to PTPRZ1-derived epitope presentation, we performed untargeted human leukocyte antigen (HLA) ligandomics. PTPRZ1-derived ligands were found across examined primary GB cell lines, and PTPRZ11814-1822, in particular, was among the overlapping PTPRZ1-derived ligands (Fig. 1H and Fig. S1I).\n\nDistinct cellular states were demonstrated in GB (Fig. S2A)41, and *PTPRZ1* expression was found to be enriched in astrocyte-like (AC-like) and oligodendrocyte-progenitor-like (OPC-like) GB cells and positively correlated with their module scores (Fig. S2B,C). Similarly, in our own cohort, we found higher *PTPRZ1* expression levels in AC-like and OPC-like GB cells (Fig. 1I-K). Comparable to previous results41, the distribution of cell states differed across patients (Fig. S2D). To assess correlation with GB stemness, a GSC score of each cell was derived from a previously defined gene set38. Indeed, *PTPRZ1* was positively correlated with GSC score in both cohorts (Fig. 1L and Fig. S2E). Additionally, we grouped TCGA-GB tumors according to dominant GB cell states (Fig. S2F), and concluded again that *PTPRZ1* was positively correlated with an AC-like state and GSC (Fig. S2G,H). Collectively, we found that *PTPRZ1* expression correlates positively with AC-like and OPC-like GB states and GB stemness, and that its robust expression results in a high MHC ligand load in GB.\nA vaccine-induced T cell receptor binds intracellularly processed PTPRZ1^{1814-1822} without evidence of off-target reactivity\n\nTo discover therapeutic PTPRZ1-reactive TCRs, peripheral blood mononuclear cells (PBMCs) were retrieved from a female HLA-A*02+ GAPVAC-101 patient, pt.16, who had undergone 11 APVAC1 vaccinations at the time of sample collection with a favorable clinical course, showing immune responses to the examined PTPRZ1 peptides (Fig. 2A)^{23}. Reactive T cells were sorted following in vitro restimulation with PTPRZ1^{1347-1355} or PTPRZ1^{1814-1822} peptide and then subjected to scTCR-seq. The TCR repertoire of the sorted T cells following in vitro restimulation with PTPRZ1^{1347-1355} peptide was polyclonal while the one following in vitro restimulation with PTPRZ1^{1814-1822} peptide was oligo-clonal, with the top CDR3 taking up 75.09% and the second top 19.76% of the repertoire (Fig. 2A). Interestingly, the top CDR3 was constituted of one β chain paired with different α chains. Subsequently, the dominant TCRs for both peptides were cloned into a non-viral, non-integrating episomal scaffold matrix attachment region (S/MAR) DNA vector^{42}. Constant regions of TCR α and β chains were murinized to avoid mispairing with endogenous human TCRs^{43}. For subsequent TCR validation, TCRs were electroporated into Jurkat cells carrying NFAT, AP-1, and NF-κB reporters or electroporated along with a plasmid encoding a reporter into Jurkat cells (Fig. 2B, Fig. S3A). TCR-Jurkat cells were then cocultured with peptide-loaded presenter cells for 24 hours. Out of the top two TCRs for PTPRZ1^{1814-1822}, sharing the same β chain but paired with different α chains, one demonstrated strong reactivity against peptide-loaded target cells (Fig. 2C). None of the tested dominant TCRs for PTPRZ1^{1347-1355} were reactive to peptide-loaded target cells (Fig. S3B,C). Thus, the identified reactive TCR for PTPRZ1^{1814-1822} was subsequently further examined.\n\nExogenous peptides do not necessarily induce immunogenicity against naturally processed and presented antigens^{44}. Therefore, we next assessed whether the peptide vaccine-induced TCR was indeed reactive to the endogenously processed and presented antigen PTPRZ1^{1814-1822}. Since the complete open reading frame (ORF) of *PTPRZ1* is large (~7kbp), we generated a well-characterized HLA-A*02+ GB cell line (U87) stably expressing a tandem minigene (TMG) encoding several antigens derived from the GAPVAC-101 and IMA950 trials, including the PTPRZ1 antigens of interest (Fig. S4A,B and Table. S1)^{23,45}. Upon coculture with U87 TMG cells, TCR-Jurkat cells also showed strong reporter activity (Fig. 2D), indicating that the identified TCR is able to recognize the intracellularly processed and presented antigen PTPRZ1^{1814-1822}. Next, we aimed to evaluate the safety profile of the PTPRZ1^{1814-1822} TCR. *PTPRZ1* is, if at all, barely expressed across adult tissues^{24}, and the TCR was isolated from a vaccinated patient without notable adverse events^{23}; hence, we hypothesized that the TCR had undergone thymic selection, making both off-target and on-target off-tumor toxicities unlikely. Nevertheless, to experimentally assess potential off-targets, we applied ARDitox, an *in silico* artificial intelligence (AI)-based prediction tool for off-target TCR binding^{46}. A panel of potential off-targets for the PTPRZ1^{1814-1822} TCR was generated with various off-target-specific safety and presentation scores (Fig. 2E, Table S2). No high-risk (safety score < 3) potential off-targets were predicted while 12 low-risk (safety score > 3) off-targets with relevant presentation probabilities on HLA-A*02 were predicted. In a subsequent Jurkat reporter assay, we did not find reactivity against any of these 12 potential off-targets (Fig. 2F). Together, these data reveal a patient-derived vaccine-induced PTPRZ1^{1814-1822}-reactive TCR that binds to both exogenous and intracellularly processed and presented antigen on MHC-I and does not react against AI-predicted low-risk off-targets.\nPTPRZ1^{1814-1822} TCR engineered primary human T cells exert effector functions and maintain T_{SCM} phenotype in vitro\n\nWe next endeavored to explore whether the PTPRZ1^{1814-1822} TCR elicits effector functions in primary human T cells. We employed a GMP-compatible retroviral system commonly used for CAR-T cell manufacturing to transduce the constant region-murinized PTPRZ1-TCR. Assessed by flow cytometric analysis of murine constant TCR β chain surface abundance and representative for multiple experiments, transduction efficiency was >85% for PTPRZ1-TCR and negative control Influenza (Flu)-TCR, targeting the HLA-A*02-restricted epitope GILGFVFTL (Fig. S5A). Without further enrichment, the TCR surface expression was maintained without a decrease in frequency 20 days post transduction in vitro (Fig. 3A). Of note, our culture conditions using IL-7 and IL-15 for stimulation and maintenance instead of conventional IL-2 stimulation favored the expansion of CD8^{+} T cells (Fig. 3B)^{47}. Subsequent longitudinal subtyping of CD8^{+} TCR-T cell into stem cell memory (T_{SCM}, CD45RA^{+} CD62L^{+}), central memory (T_{CM}, CD45RA^{+} CD62L^{+}), effector memory (T_{EM}, CD45RA^{+} CD62L^{-}), and CD45RA^{+} effector memory (T_{EMRA}, CD45RA^{+} CD62L^{-}) revealed a long-lasting and predominant adaptation to a T_{SCM} phenotype over the course of three weeks in vitro regardless of TCR expression (Fig. 3C). In contrast to previous studies, we did not enrich for naïve T cells yet still were able to generate T_{SCM}-abundant engineered T cell products^{47}. The generated TCR-T cells were then cocultured with various target cells. Only upon contact with cognate peptide-loaded target cells or U87 TMG, CD8^{+} TCR-T cells were activated (Fig. 3D). Importantly, the primary HLA-A*02^{+} GB cell line P3, endogenously expressing PTPRZ1^{23}, also activated CD8^{+} PTPRZ1^{1814-1822} TCR-T cells (Fig. 3D). Moreover, the frequencies of effector cytokine- and cytolytic protein- expressing CD8^{+} TCR-T cells were increased in an antigen-specific fashion (Fig. 3E and Fig. S5B-D). PTPRZ1^{1814-1822} TCR-T cells (PTPRZ1-TCR-T) demonstrated antigen-specific dose-dependent cytotoxicity with an optimal E:T ratio of 2:1 (Fig. 3F,G).\n\nA recent study suggests that cytotoxic CD4^{+} CAR-T cells facilitate long-term tumor control^{48}. Our TCR-T cell manufacturing process transduced both CD4^{+} and CD8^{+} T cells, and we observed that CD4^{+} TCR-T cells, even without the co-receptor CD8, were activated in an antigen-dependent manner (Fig. S6A-C). Moreover, additional irradiation of tumor cells in vitro resulted in increased lysis of target cells likely due to enhanced activation of PTPRZ1-TCR-CD4^{+}-T but not PTPRZ1-TCR-CD8^{+}-T (Fig. 3D,E, Fig. S5E-H and Fig. S6C-F). Although cytolytic proteins were elevated in PTPRZ1-TCR-CD4^{+}-T, it remained unclear if PTPRZ1-TCR-CD4^{+}-T encountered target cells directly to execute cytotoxicity or to support neighboring cytotoxic PTPRZ1-TCR-CD8^{+}-T. Thus, we further unraveled the role of CD4^{+} T cells engineered with the CD8-restricted PTPRZ1^{1814-1822} TCR on tumor cell lysis in vitro through enriching CD4^{+} and CD8^{+} T cells via magnetic-activated cell sorting (MACS) post transduction (Fig. 3H). As expected, serial dilution of PTPRZ1-TCR-CD4^{+}-T in comparison to that of PTPRZ1-TCR-CD8^{+}-T revealed that CD4^{+} T cells play a minor role in target cell killing (Fig. 3I,J). However, we found a moderate increase in cytotoxicity when both CD4^{+} and CD8^{+} T cells carried the PTPRZ1^{1814-1822} TCR compared to the combination of PTPRZ1^{1814-1822}-reactive CD8^{+} T cells with non-target-specific CD4^{+} T cells (Fig. 3K). Thus, our data suggest a differential but synergistic role for CD4^{+} and CD8^{+} T cells following antigen-specific activation via PTPRZ1^{1814-1822} TCR.\n\nPTPRZ1-TCR-T is efficacious in experimental flank and brain tumors\n\nTo investigate the therapeutic potential of the PTPRZ1^{1814-1822} TCR in vivo, we first inoculated U87 TMG cells subcutaneously (s.c.) in the flank of immunodeficient mice, followed by two\ndoses of intravenous (i.v.) TCR-T cell administration (Fig. 4A). Following adoptive cell transfer (ACT) with PTPRZ1-TCR-T, flank tumors regressed over time while control mice without treatment or treated with an irrelevant TCR-T product showed sustained tumor growth and met termination criteria by day 40 post tumor inoculation (Fig. 4B and Fig.S7A-D). Of note, after initial tumor regression, some PTPRZ1-TCR-T-treated animals experienced tumor recurrence starting from day 42 onwards, yet by the predefined experimental endpoint, 33% (3 out of 9) of PTPRZ1-TCR-T cell-treated animals remained tumor-free, resulting in prolonged survival (Fig. S7C,D).\n\nSubsequently, we advanced to investigate PTPRZ1-TCR-T in experimental brain tumors. A recent study has demonstrated that repeated systemic i.v. CAR-T delivery does not result in GB control in a phase I trial, not even in a combinatorial treatment with immune checkpoint blockade14. At least in part, this might be attributed to the BBB resulting in the exclusion of T cells infiltrating via the blood stream into the CNS5,6. Indeed, when we delivered PTPRZ1-TCR-T into mice bearing intracranial U87 TMG tumors i.v. (Fig. S8A), no therapeutic effect was observed (Fig. S8B). Hence, we adapted our ACT regime to two doses of intracerebroventricular (i.cv.) ACT following one dose of i.v. ACT (Fig. 4C). Notably, by combined i.v. and i.cv. PTPRZ1-TCR-T, mice showed preclinical response (Fig. 4D,E). 5 out of 7 (71.4%) of PTPRZ1-TCR-T-treated tumor-bearing mice responded radiographically to ACT while tumors of control-treated mice continued to grow (Fig. 4E). Only PTPRZ1-TCR-T-treated mice (4 out of 7; 57.1%) survived till the experimental endpoint (Fig. 4F and Fig. S9A-C). One out of the survivors remained tumor-free macroscopically while the others experienced tumor recurrence at experimental endpoint (Fig. S9C). To assess persistence of the TCR-T cell in vivo, we monitored T cell engraftment in the blood. Three weeks post first ACT, TCR-T cells were detected in all mice receiving ACT (Fig. 4G). Adoptive transfer of different CD8+ T cell subsets is known to affect T cell engraftment and T cell effector functions. Paradoxically, ACT with more stem-like or central memory T cells outperforms other CD8+ subsets as they retain self-renewal capacity but nonetheless, have less cytotoxic and cytokine-releasing capacity49-51. Hence, we characterized engrafted T cells by flow cytometry. Up to three weeks following first ACT, we found the T_{SCM} phenotype to remain dominant in vivo with negligible inter-individual differences (Fig. 4H,I). No difference in population frequencies was observed when comparing therapeutic PTPRZ1-TCR-T- with control TCR-T-treated mice (Fig. 4I), suggesting that the engraftment and CD8+ T cell subset maintenance were independent of cognate antigen encounter in vivo.\n\nTo decipher if in recurrent tumors, either dormant GB cells regain proliferative capacity when reactive TCR-T cells are no longer present within the GB microenvironment52,53, or MHC and/or antigen loss occurs54,55, we analyzed post-mortem tumors reaching preclinical termination criteria or experimental endpoint. We found that transferred human T cells in the tumor could only be detected in mice treated with PTPRZ1-TCR-T (Fig. 4J,K), even after 76 days following the last ACT (Fig. S9D). In addition, MHC1 expression was maintained in recurrent tumors (Fig. 4J). We thereby examined antigen expression with RNAscope™ and found that TMG transcripts were greatly diminished in the recurrent tumors (Fig. 4L,M). These data demonstrate the on-target activity of PTPRZ1-TCR-T and highlights the ACT route-dependent efficacy in experimental GB. Intriguingly, the reactive TCR-T cell product persists in experimental brain tumors, and the relapse is driven by downregulation and/or loss of the tandem antigens in this model.\n\nPTPRZ1-TCR-T shows cytotoxicity against patient-derived HLA-A*02+ GB spheroid cell lines and preferentially targets slow-cycling cells\nTo assess PTPRZ1-TCR-T efficacy on primary GB, we established patient-derived primary GB cell lines following previously described protocols of tumor cell isolation via FACS or MACS (Fig. S11)56. The established primary GB cell lines were maintained in serum-free medium and cultured in spheroids to maintain stemness. Benchmarking cytotoxicity, we cocultured PTPRZ1-TCR-T with primary HLA-A*02+ GB cell lines, D170_44 and P3, and found comparable cytotoxicities (Fig. 5A). Again, both CD8+ and CD4+ PTPRZ1-TCR-T cells were activated by the primary GB cell line D170_44 (Fig. S10A,B).\n\nSlow-cycling GB cells are considered stem-like as they have the potential for tumor initiation, therapy resistance, and generation of large number of progenies37,57,58. As PTPRZ1 was defined as a GSC marker and found to be highly associated with GSC scores, we hypothesized that PTPRZ1-TCR-T preferentially targeted stem-like slow-cycling cells (SCC). To identify SCC, primary GB cell lines were labeled with fluorescent dye, and the top 10% dye-retaining cells after expansion were considered SCC while the rest were defined as fast-cycling cells (FCC). Upon coculture with PTPRZ11814-1822 TCR-T cells, dye-retaining SCC and dye-losing FCC were enumerated by flow cytometry to assess differential cytotoxicity (Fig. 5B). Indeed, in the first five hours, PTPRZ11814-1822 TCR-T cells preferentially killed SCC while after 24 hours, both SCC and FCC were lysed (Fig. 5C and Fig. S10C), suggesting a preferential anti-tumor activity on stem-like SCC by PTPRZ1-TCR-T.\n\nFurthermore, to demonstrate HLA-A*02-dependency and assess the breadth of anti-tumor activity by PTPRZ11814-1822 TCR, we established five additional primary GB cell lines, of which MA120, MA140, and D170_108 were HLA-A*02+, and MA108 and MA118 were HLA-A*02- (Fig. 5D). Upon coculture, PTPRZ1-TCR-T exclusively killed HLA-A*02+ lines (Fig. 5E). Primary HLA-A*02+ GB cell lines led to activation of CD8+ PTPRZ1-TCR-T at various degrees and additionally activated CD4+ PTPRZ1-TCR-T in a moderate fashion. Conversely, HLA-A*02- GB cell lines did not elicit any activation nor were lysed (Fig. 5E-H and Fig. S10D). Together, these data demonstrate that PTPRZ11814-1822 TCR can broadly and specifically target HLA-A*02+ GB primary cell lines (5 out of 5) with a preference for stem-like SCC.\n\nPTPRZ1-TCR-T impacts GB cell states and targets GB stemness in individual patient tumor organoids (IPTOs)\n\nAs previously shown, *PTPRZ1* is higher expressed in AC-like and OPC-like cells and associated with GB stemness (Fig. 1L,M). Therefore, we evaluated whether PTPRZ1-enriched subsets of malignant cells were targeted preferentially by PTPRZ1-TCR-T. Individual patient tumor organoids (IPTOs) maintain tumor multicellular characteristics and are thereby suitable to study PTPRZ1-TCR-T-mediated alterations in a realistic multicellular-orchestrated microenvironment (Fig. 6A). IPTOs from three HLA-A*02+ patients were treated with TCR-T cells and interrogated by scRNA-seq. GB cells and immune cells were identified based on the absence of EGFP and presence of B2M, respectively (Fig. 6B, Fig. S11A,B), as host feeder organoid cells are engineered to be EGFP-expressing and B2M-deficient. The GB cell cluster expressed high levels of *PTPRZ1* (Fig. 6B). Upon PTPRZ1-TCR-T treatment, malignant cell frequency was decreased (Fig. 6C), and average *PTPRZ1* expression in malignant cells was lowered (Fig. 6D). To understand the underlying mechanism of lowered *PTPRZ1* expression, we aimed to decipher cell state distribution in post-treatment IPTOs. Assessing cell states, we again observed that *PTPRZ1* was associated with AC-like tumor cells (Fig. 6E), but upon PTPRZ1-TCR-T cell treatment, AC-like score and AC-like tumor cell frequency were reduced\nsignificantly (Fig. 6F,G). Corroborating our previous findings, a positive correlation of GSC score and *PTPRZ1* was identified (Fig. 6H), and PTPRZ1-TCR-T coculture led to a drop of GSC cell frequency (Fig. 6I). Collectively, the results confirm that *PTPRZ1* is highly expressed in malignant brain tumor cells, most abundantly in GSCs, and that AC-like cells and GSCs are primarily targeted by PTPRZ1*1814-1822* TCR-T cells.\n\nDISCUSSION\n\nIn this study, we profiled the expression of PTPRZ1, a GB-associated antigen and GSC marker, across bulk and scRNA-seq datasets in publicly available and own cohorts, and took advantage of a previous multinational European GB vaccination trial, enabling us to retrieve an HLA-A*02-restricted PTPRZ1-reactive TCR in a reverse translation research paradigm. The TCR was comprehensively examined *in vitro* and *in vivo* for its anti-tumor activity against experimental flank and brain tumors, primary GB cell lines, and IPTOs. Besides the validated TCR reactivity, we identified and excluded low-risk off-targets. In addition to the robust *in vivo* efficacy of PTPRZ1-TCR-T, we found universal targeting of HLA-A*02* primary GB cell lines and malignant cells in IPTOs with a preference for stem-like SCC and AC-like tumor cells.\n\nPTPRZ1 is essential during neurodevelopment but not in adults\\(^{25,26}\\); however, its expression re-emerges and is required for gliomagenesis and tumor progression. Whereas the mechanistic relevance of PTPRZ1 in GB remains elusive, its functions and contributions to disease malignancy are well-demonstrated, ranging from cancer cell proliferation and stemness to angiogenesis and therapy resistance\\(^{30-34}\\). Here, we explored treatment with the identified PTPRZ1*1814-1822* TCR, yet therapies for non-HLA-A*02* patients and combinatorial therapies should be investigated further, particularly when taking all the variety of PTPRZ1-derived MHCI-ligands into consideration (Fig. 1H). Apart from PTPRZ1 upregulation in GB, we also found robust overexpression of PTPRZ1 in IDH-mutant gliomas. Further investigations are required to examine whether PTPRZ1-TCR-T can be applied to oligodendrogliomas and astrocytomas or other cancer entities that display elevated *PTPRZ1* expression\\(^{59}\\). Moreover, our results further support PTPRZ1 as a GSC marker, not only from the bioinformatic analyses but also from *in vitro* assays showing preferential killing of stem-like SCCs. Therefore, from a neuro-oncological perspective, targeting a cell population that drives disease initiation, progression, and treatment resistance, supports future clinical investigations of PTPRZ1-TCR-T.\n\nA major advantage of TCR-T therapy is its capability to target all proteins, including intracellular neoantigens, as long as they are processed and presented on MHC. As studied by others, PTPRZ1, a transmembrane receptor, can be, in principle, targeted by CAR-T cells\\(^{60}\\). However, protein glycosylation is often altered in cancers, including brain tumors\\(^{61,62}\\). Such aberrant post-translational modification may impact CAR-T cell therapy efficacy\\(^{63}\\), and increasing evidence is emerging suggesting TCR but not tonic CAR signaling cascades to be associated with favorable intratumoral T cell fate\\(^{16,17}\\). Conversely, limitations of TCR-T are HLA-type dependency and the prerequisite of MHC expression. Despite HLA restriction which is inherently associated with the need of therapy individualization, our TCR covers a common HLA and targets the intracellular domain of PTPRZ1 presented on MHCI. As MHC antigen processing and presentation machinery is rarely altered in GB\\(^{55}\\), TCR-T cell therapy presents a highly promising approach. Of note, in our glioma model overexpressing but not depending on TMG *in vivo*, we found loss of the cognate antigen (Fig .4L). It remains speculative, if this is a unique feature of our model as *PTPRZ1* expression remained stable during disease\nprogression in patients (Fig. 1F). Nevertheless, more GB-reactive TCRs should be developed to expand the HLA coverage and to allow multivalent cell therapy, preventing escape through antigen loss.\n\nIn our study, the presence of CD4+ T cells within PTPRZ1-TCR-T was required for optimal cytotoxicity in vitro. In line with this, the relevance of the CD4+::CD8+::APC immune triad for solid tumor eradication has been highlighted recently64. In PTPRZ1-TCR-T, CD4+ T cells also produced effector proteins and cytokines, suggesting a dual action of moderate direct cytotoxicity and paracrine reprogramming of CD8+ T cells. Whether CD4+ T cells engineered with CD8-restricted TCR can hijack tumor cells to form triad to restore and improve CD8+ T cell functions will require further experimental investigations. Notably, CD4+ CAR-T cell persistence was associated with long-term survival in leukemia patients, but on the other hand, CD4+ CAR-T cells are implicated in cytokine release syndrome. Here, fine tuning of CD4+::CD8+ T cell ratio without impacting anti-tumor immunity is required48,65.\n\nEncouraged by the preclinical results, we are initiating a phase I clinical trial, Intraventricular T cell receptor transgenic T cell therapy to treat glioblastoma (INVENT4GB)66, to assess the feasibility and safety of CD4+/CD8+ PTPRZ1-TCR-T cell therapy in patients with recurrent GB. It will mark the first-in-human TCR-T cell therapy against GB and highlight the here proposed “bedside to bench to bedside” approach.\n\nMATERIALS AND METHODS\n\nCell lines\nU87 was cultured in DMEM supplemented with 10% fetal bovine serum (FBS) and 1% Penicillin/Streptomycin (P/S). U87 TMG cell line was generated by transfection with pMXs-IRES-PuroR plasmid encoding TMG as illustrated in Fig. S2C. Transfection was performed with Fugene HD transfection reagent (#E2312, Promega) following the manufacturer instructions. Briefly, U87 cells were seeded at a density of 3 x 10^5 cells per well in a 6-well plate and rested for 24h. On the next day, the medium was replenished, and the cells were transfected with 2 μg of the DNA plasmid and rested for another 48h. Cells stably expressing TMG were then selected with 2 μg/ml Puromycin. T2 cells were kindly provided by Dr. Angelika Riemer, Division of Immunotherapy and Prevention, DKFZ, and cultured in RPMI-1640 supplemented with 20% FBS and 2% L-Glutamine.\nHEK293 cells were cultured in IMDM supplemented with 10% FBS.\nJurkat TCR deficient cells were purchased from ATCC, and Jurkat 76-Triple parameter reporter (J76-TPR) was kindly provided by Prof. Peter Steinberger, Division for Immune Receptors and T Cell Activation, Institute of Immunology, Medical University of Vienna67. Jurkat cells were cultured in RPMI-1640 supplemented with 10% FBS and 1% P/S.\nPrimary brain tumor samples were collected at the University hospital of Mannheim. All patients have provided written signed informed consent in accordance to the WMA Declaration of Helsinki principles. Ethical approval for the isolation of brain tumor tissue and analyses was obtained from the Mannheim Medical Faculty Ethics Committee (2017-589N-MA, 608-22, 574-23). The harvested tumors were processed with tumor dissociation kit (#130-095-929, Miltenyi Biotec) and further enriched for tumor cells with tumor cell isolation kit (#130-108-339, Miltenyi Biotec) following the manufacture instructions. The isolated tumor cells and previously established primary GB cell lines were cultured in DMEM-F12 supplemented with B27 (#17504044, Thermo Fisher), 5 μg/ml Insulin (#I9278, Sigma-Aldrich), 5 μg/ml Heparin (#H4784, Sigma-Aldrich), 20 ng/ml epidermal growth factor (EGF, #AF-100-15, Peprotech) and 20 ng/ml fibroblast growth factor (FGF, #100-18b, Peprotech)56.\nAll cell lines were incubated at 37°C and 5% CO₂ with saturated humidity.\n\nMice\nNOD-Prkdcscid-Il2rgTm1/Rj (NXG) mice were purchased from Janvier labs. NOD.Cg-Prkdcscid H2-K1lmtBpe H2-Ab1lem1Mvw H2-D1lmtBpe Il2rgtm1Wjl/SzJ (NSG MHC KO) mice were bred at the DKFZ animal facility. Mice were housed under Specific and Opportunistic Pathogen Free (SOPF) conditions and under 12h day/night cycle with water and chow ad libitum. All animal procedures were conducted in compliance with the institutional laboratory animal research guidelines and were approved by the governmental institutions (Regional Administrative Authority Karlsruhe, Germany, file number: G-263/18 and G-130/23).\n\nIPTO generation and culture\nInduced pluripotent stem cells (iPSCs; AICS-0036-006, Institute for Cell Science) expressing enhanced green fluorescent protein (EGFP) were utilized to generate cerebral organoids. Organoid generation adhered to a published method⁶⁸, beginning with the seeding of dissociated iPSCs in 96-well round bottom ultra-low attachment plates with previously described hESC medium⁶⁸, supplemented with 4 ng/ml basic fibroblast growth factor (bFGF; #PeproTech, 100-18B), and 50 μM ROCK inhibitor (#72304, Stemcell Technologies). Formed embryoid bodies were subsequently transferred to 24-well ultra-low attachment plates and 6-well ultra-low attachment plates in previously described Neural Induction Medium⁶⁸, followed by a transition to improved differentiation medium -A and improved differentiation medium +A⁶⁹, with agitation introduced from day 18. Resected tumor tissues were processed and dissected into small explants, which were subsequently inserted into incised cerebral organoids and embedded in Matrigel. Generated IPTOs were then cultured in improved differentiation medium +A on an orbital shaker in an incubator (75 rpm, 37°C). After 10 days of incubation, the IPTOs were ready for TCR-T testing.\n\nElectroporation of Jurkat cells\nNeon transfection system (Thermo Fisher) was employed to deliver TCR and reporters. For transfection of Jurkat cells without reporters, 2 x 10⁶ Jurkat cells were resuspend in 100 μl R buffer with 5 μg of TCR and 5 μg of reporter plasmids. For transfection of J76-TPR, 2 x 10⁶ cells were resuspend in 100 μl R buffer with 5 μg of TCR plasmid. Electroporation was then performed at 1325 V, 3 pulses, 10 ms.\n\nTransduction of primary human T cells\nRetroviral transduction was performed as previously described⁷⁰. Briefly, TCR were inserted into SFG-IRES-GFP retroviral vector (kind provision from Dr. Martin Pule, Addgene #22493; RRID:Addgene_22493) with In-Fusion Cloning (#638947, Takara). 3 x 10⁶ HEK293 cells were seeded a day before transfection in 10ml IMDM supplemented with 10% FBS in 60.1 cm² dish. On the day of transfection, 3.75 μg TCR-SFG along with 3.75 μg PeqPam and 2.5 μg RD114 packaging plasmids were resuspended in 470 ml IMDM and 30 μl Fugene HD transfection reagent. PeqPam and RD114 packaging plasmids were kindly gifted by Dr. Tim Sauer. After 10-minute incubation, cells were transfected with the DNA-Fugene HD mix and incubated for 48h. The viral supernatant was then collected and strained through 0.45 μm strainers. Human T cells were obtained from healthy donors via density gradient separation followed by MACS with Pan T cell isolation kit (#130-096-535, Miltenyi) in accordance with manufacturer instructions. Isolated T cells were activated in CTL medium (45% RPMI-1640, 45% Click’s medium, 10% FBS, 10 ng/ml IL-7 [#200-7, Peprotech] and 5 ng/ml IL-15 [#200-15, Peprotech]) with T Cell TransAct (#130-111-160, Miltenyi) for 48h at a concentration of 1 x 10⁶ cells/ml. The strained viral supernatant was plated 0.5 ml per well in a non-tissue culture\ntreated 24-well plate (#351147, Falcon) precoated o/n with 0.5 ml of 7 μg/ml RetroNectin (#T100B, Takara) and centrifuged at 2000g for 90 minutes at 4°C. Later, the supernatant was removed and activated T cells were seeded at a concentration of 0.5x10^6 cell/ml in 1 ml CTL medium per well and centrifuged at 500g for 5 minutes. After 4 days of incubation, TCR-T cells were ready for expression analysis or coculture assays. TCR-T cells were maintained in culture with CTL medium over the course of described time, and the medium was refreshed every 3-4 days.\n\nSubcutaneous tumor inoculation\nU87 TMG cell line was prepared at a concentration of 4 x 10^6 cells/ml in PBS-Matrigel mixture at a ratio of 1:1. Immunodeficient mice were shaved at the flank site before injecting subcutaneously 200 μl of prepared tumor cells (8 x 10^5 cells) with 27G needle slowly and steadily into it. Tumor-bearing mice were then monitored routinely for tumor-related symptoms and measured for tumor growth with a caliper. Upon termination criteria or the experimental endpoint, mice were sacrificed with anesthesia and organs of interest were harvested for downstream analyses.\n\nIntracranial tumor inoculation\nU87 TMG cell line was resuspended at a concentration of 75 x 10^6 cells/ml in PBS and 2 μl of which, namely 1.5 x 10^5 cells, was stereotactically implanted into the right hemisphere of immunodeficient mice with the following coordinates: 2 mm right lateral of the bregma and 1 mm anterior to the coronal suture at the depth of 3 mm below the dural surface. A 10-μl Hamilton micro-syringe driven by a fine-step stereotactic device (Stoelting) was employed for injection. The surgery was conducted under anesthesia (Ketamin, 100 mg/kg i.p. and Xylazin, 10 mg/kg i.p.) and analgesia (Carprofen, 5 mg/kg s.c.). Mice continued to receive analgesia for 3 days post surgery and was checked daily for tumor-related symptoms. Upon termination criteria or the experimental endpoint, mice were sacrificed with anesthesia and organs of interest were harvested for downstream analyses.\n\nIntravenous adoptive cell transfer\nTCR-T cells generated as described above were resuspended at a concentration of 25 x 10^6 cells/ml in PBS. Mice were shortly warmed with red-light lamp before intravenously receiving ACT of 5 x 10^6 cells in 200 μl PBS with 27G needle. On the day of and the day after ACT, mice were given 5 x 10^4 units of IL-2 i.p. in 100 μl PBS.\n\nIntracerebroventricular adoptive cell transfer\n5 x 10^6 TCR-T cells were resuspended in 4 μl PBS and stereotactically injected into the cerebral ventricle of the mice with the following coordinates: 0.5 mm left lateral to the bregma at the depth of 1.8 mm below the dural surface. A 10-μl Hamilton micro-syringe driven by a dine step stereotactic device (Stoelting) was employed for injection. The surgery was conducted under anesthesia (Ketamin, 100 mg/kg i.p. and Xylazin, 10 mg/kg i.p.) and analgesia (Carprofen, 5 mg/kg s.c.). Mice continued to receive analgesia for 3 days post surgery.\n\nAdoptive cell transfer on IPTO\nUpon the establishment of IPTOs, 150 x 10^3 TCR-T cells were injected in 3 μl with a 10-μl Hamilton micro-syringe. After 3-day incubation, feeder cells were first macroscopically removed with a scalpel, and the remained tumor chunk was processed with tumor dissociation kit (#130-095-929, Miltenyi Biotec).\n\nMagnetic resonance imaging\nMRI was conducted by the small animal imaging core facility at DKFZ with a Bruker BioSpec 3Tesla (Ettlingen, Germany) with Para Vision software 360 V1.1. Mice were anesthetized with 3.5% sevoflurane in air, and the imaging was performed with a T2 TurboRARE sequence: TE = 48 ms, TR = 3350 ms, FOV 20x20 mm, slice thickness 1 mm, averages = 3, Scan Time = 3m21s, echo spacing 12 ms, rare factor 8, slices 20, image size 192 x 192. Tumor volume was assessed by manual segmentation using Bruker Para Vision software 6.0.1.\n\nUntargeted ligandomics\nImmunoprecipitation of HLA class I:peptide complexes was performed as previously described with additional steps for the forced oxidation of methionine using H2O2 and reduction and alkylation of cysteine using tris(2-carboxyethyl)phosphine and iodoacetamide71. Lyophilized peptides were dissolved in 12 μl of 5% ACN in 0.1% TFA and spiked with 0.5μl of 100 fmol/μl Peptide Retention Time Calibration Mixture and 10 fmol/μl JPTRT 11, a subset of peptides from the Retention Time Standardization Kit (JPT), and transferred to QuanRecovery Vials with MaxPeak HPS (Waters, Milford, MA, USA). All samples were analyzed using an UltiMate 3000 RSLCnano system coupled to an Orbitrap Exploris 480 equipped with a FAIMS Pro Interface (Thermo Fisher). For chromatographic separation, peptides were first loaded onto a trapping cartridge (Acclaim PepMap 100 C18 μ-Precolumn, 5μm, 300 μm i.d. x 5 mm, 100 Å; Thermo Fisher) and then eluted and separated using a nanoEase M/Z Peptide BEH C18 130A 1.7μm, 75μm x 200mm (Waters). Total analysis time was 120 min, and separation was performed using a flow rate of 0.3 μl/min with a gradient starting from 1% solvent B (100% ACN, 0.1% TFA) and 99% solvent A (0.1% FA in H2O) for 0.5 min. Concentration of solvent B was increased to 2.5% in 12.5 min, to 28.6% in 87 min and then to 38.7% in 1.4 min. Subsequently, concentration of solvent B was increased to 80% in 2.6 min and kept at 80% solvent B for 5 min for washing. Finally, the column was re-equilibrated at 1% solvent B for 11 min. The LC system was coupled on-line to the mass spectrometer using a Nanospray-Flex ion source (Thermo Fisher), a SimpleLink Uno liquid junction (FossillOnTech) and a CoAnn ESI Emitter (Fused Silica 20 μm ID, 365 μm OD with orifice ID 10 μm; CoAnn Technologies). The mass spectrometer was operated in positive mode and a spray voltage of 2400 V was applied for ionization with an ion transfer tube temperature of 275 °C. For ion mobility separation, the FAIMS module was operated with standard resolution and a total carrier gas flow of 4.0 l/min. Each sample was injected twice using either a compensation voltage of -50 V or -65 V for maximal orthogonality and thus increased immunopeptidome coverage. Full Scan MS spectra were acquired for a range of 300 – 1650 m/z with a resolution of 120,000 (RF Lens 50%, AGC Target 300%). MS/MS spectra were acquired in data-independent mode using 44 previously determined dynamic mass windows optimized for HLA class I peptides with an overlap of 0.5 m/z. HCD collision energy was set to 28% and MS/MS spectra were recorded with a resolution of 30,000 (normalized AGC target 3000%). MS raw data was analyzed using Spectronaut software (version 17.6, Biognosys)72, and searched against the UniProtKB/Swiss-Prot database (retrieved: 21.10.2021, 20387 entries). Search parameters were set to non-specific digestion and a peptide length of 7 -15 amino acids. Carbamidomethylation of cysteine and oxidation of methionine were included as variable modifications. Results were reported with 1% FDR at the peptide level. Peptides identified by Spectronaut were further analyzed using NetMHCpan 4.173. Predicted non-binders were excluded from the analysis.\n\nRNAscope™\nTarget RNA transcripts on slides were detected with RNAscope 2.5 HD Duplex Kit (#322435, Advanced Cell Diagnostics) following manufacture instructions. Briefly, slides with sectioned frozen murine brains were removed from -80°C and immediately fixated with pre-chilled 10% neutral buffered formalin at 4°C. To dehydrate the slides, they were then serially immersed in\n50%, 70% and 100% EtOH at RT. After another immersion in fresh 100% EtOH, slides were either immediately used or stored in 100% EtOH at -20°C for up to a week. To stain the slides, they were first air-dried and pre-treated with RNAscope Hydrogen Peroxide. After a quick wash with PBS, they were then pre-treated with RNAscope Protease IV. Slides were subsequently quickly rinsed with PBS. For target detection, custom probes were manufactured, and the probe mix was applied on slides and incubated in HybEZ Oven for 2h at 40°C. Next, the slides were washed with 1X Wash Buffer and kept in 5X SSC at RT o/n. On the next day, slides were washed with 1X Wash Buffer and underwent a series of amplification steps with Amp 1-6 following the manual. First probe was then detected with FastRed. After more washes with 1X Wash Buffer, slides underwent another series of amplification steps with Amp 7-10 following the instructions. Second probe was then detected with FastGreen. After more washes with 1X Wash Buffer, slides were counterstained with 50% Hematoxylin staining solution. Next, slides were immediately rinsed with tap water, followed by drying in HybEZ Oven at 60°C. Once the slides cooled down, they were briefly dipped in fresh Xylene and mounted with VectaMount Mounting Medium (#H-5000, Vector Labs).\n\nARDitox off-target prediction\nOff-targets were predicted as described previously46. Briefly, 9-mer peptides of human proteome that share at least 5 amino acids with the target epitope were shortlisted. Next, epitopes derived from frequent single nucleotide polymorphisms with a frequency more than 1% were included. High-affinity presented epitopes predicted with ARDisplay were selected74. Safety score compared the physico-chemical properties of probable TCR-facing amino acids.\n\nTCGA and publicly available dataset analysis\nTCGA data were downloaded through the package TCGAbiolinks (2.28.4)75. Sc GB and glioma datasets were downloaded according to the instructions40,41. The data were handled with Seurat (5.0.3)76. Cell state scores were directly used if specified in the dataset; otherwise, they were calculated based on the defined gene sets with AddModuleScore function41. GSC scores were calculated with the published gene set38.\n\nSingle-cell RNA-seq and analysis\nIsolated primary tumor cells and non-tumor cells from brain tumor samples and IPTO cells were resuspended in 0.04% BSA in PBS; Up to 20 x 10^3 cells were loaded for 5’ single cell sequencing (#1000263, 10x Genomics), and the libraries were prepared according to the manufacturer protocol. Single-cell data were aligned with cellranger (7.0.0) and handled with Seurat (5.0.3). Cells expressing few transcripts or genes were excluded before normalization. Doublets were identified and excluded with scDblFinder (1.14.0)77. Harmony (1.0.3) was subsequently used to integrate datasets78. Canonical markers were employed to identify and annotate the cell type. Module gene sets were derived from previous studies and their scores were calculated using AddModuleScore function in Seurat. Plots were made with ggplot2 (3.5.0) and SCpubr (2.0.2)79,80.\n\nStatistical analysis and Figures\nData are presented as individual values or as mean ± SEM unless stated otherwise. Applied statistical tests are indicated in Figure legends. GraphPad Prism 9.0 was used for statistical tests and plots. Some Figures were created with BioRender.com.\n\nREFERENCES\n1 Hirayama, A. V. et al. High rate of durable complete remission in follicular lymphoma after CD19 CAR-T cell immunotherapy. Blood 134, 636-640, doi:10.1182/blood.2019000905 (2019).\n2 Schuster, S. J. et al. 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Nat Biotechnol 42, 293-304, doi:10.1038/s41587-023-01767-y (2024).\n77 Germain, P. L., Lun, A., Garcia Meixide, C., Macnair, W. & Robinson, M. D. Doublet identification in single-cell sequencing data using scDbIfinder. F1000Res 10, 979, doi:10.12688/f1000research.73600.2 (2021).\n78 Korsunsky, I. et al. Fast, sensitive and accurate integration of single-cell data with Harmony. Nat Methods 16, 1289-1296, doi:10.1038/s41592-019-0619-0 (2019).\n79 Wickham, H. ggplot2: Elegant Graphics for Data Analysis. (Springer-Verlag New York, 2016).\n80 Blanco-Carmona, E. Generating publication ready visualizations for Single Cell transcriptomics using SCpubr. bioRxiv, 2022.2002.2028.482303, doi:10.1101/2022.02.28.482303 (2022).\n\nAuthor contributions\nY.C.C. conceptualized the study, designed and performed experiments, analyzed and interpreted data, and wrote the manuscript. A.C.D., D.A.A., A.D.R., A.K., M.K. and C.K. performed in vitro and in vivo experiments and edited the manuscript. X.M. and H-K.L. established and processed organoids and edited the manuscript. P.K. and B.Z. analyzed patient and organoid scRNA-seq data and edited the manuscript. A.K.S. and F.S. collected GB histology samples and edited the manuscript. M.S., H.B., T.B., R.H. and W.W. interpreted data and edited the manuscript. A.B. and V.M.P. predicted off-targets. K.A., J.P.B. and A.B.R. performed the ligandomics analysis and edited the manuscript. H.F. and N.E. collected patient\ntumor samples and edited the manuscript. M.R. established primary GB cell lines and edited the manuscript. M.P. supervised the study, interpreted the data, provided funding and edited the manuscript. E.W.G. provided cloning methodology, retrieved the TCR and edited the manuscript. L.B. conceptualized and supervised the study, interpreted the data, and wrote the manuscript.\n\nAcknowledgements and funding\nWe acknowledge the support of the DKFZ Light Microscopy Facility, Genomics and Proteomics Core Facility, Center for Preclinical Research, Flow Cytometry Core Facility and single-cell Open Lab. We also would like to highlight and acknowledge the technical support from Viktoria Sachs, Chris Pagel, Kristine Jähne and Rebecca Köhler. This study was supported by grants from the Swiss Cancer Foundation (Swiss Bridge Award), the Else Kröner Fresenius Foundation (2019_EKMS.49), the University Heidelberg Foundation (Hella Bühler Award), the DFG (German Research Foundation), project 404521405 (SFB1389 UNITE Glioblastoma B03), the DKFZ Hector institute (T-SIRE), the Hertie Foundation, and the University of Heidelberg, ExploreTech! Grant to L.B.; the DKTK Joint Funding AMI2GO, the Rolf Schwiete Foundation (2021-009) to M.P. and L.B.; the HI-TRON strategy project PACESSETTING and the DKTK Joint Funding Program INNOVATION INVENT4GB to W.W., M.P., and L.B. The DFG, project 404521405 (SFB1389 UNITE Glioblastoma B01) to T.B. and M.P. Y-C.C. received an international fellowship from the Helmholtz International Graduate School at DKFZ and was supported by RTG 2099 and UNITE SFB1389. A.C.D. was supported by Mildred-Scheel scholarship. P.K. and D.A.A. were funded by RTG 2099 and UNITE SFB1389.\n\nCompeting interests\nThe identified reactive TCR was patented by Y-C.C., M.K., C.K., E.W.G., W.W., M.P. and L.B., “T cell receptor derived binding polypeptides” (WO 2023/213904). E.W.G. and M.P. are founders of TCellTech.\nFIGURES\n\nFig. 1. PTPRZ1 is upregulated in GB, particularly in GSCs and AC-like GB.\n(A) *PTPRZ1* expression in primary tumor compared to adjacent normal tissues in TCGA-GB dataset with t-test. (B) *PTPRZ1* expression in single cells of GB from previously published dataset\\(^{41}\\). Cell type annotation is in Fig. S1D. (C) UMAP of scRNA-sequenced glioma and GB samples from Fig. S1I with cell type annotation. (D) Gene expression of *PTPRZ1* for (C). More cell type-defining genes are shown in Fig. S1J. (E) & (F) Protein expression of PTPRZ1 and GFAP from 20 primary and 20 recurrent GB matched samples. Each dot is the average of all tumor pieces of a patient. (G) Correlation of PTPRZ1\\(^+\\) and GFAP\\(^+\\) cell frequencies. Each dot represents a tumor piece. (H) Untargeted ligandomics of primary GB cell lines with overlapping of PTPRZ1 ligands across primary GB cell line. The highlighted overlapped peptide is PTPRZ1\\(^{1814-1822}\\). (I) & (J) Cellular states of cancer cells in (C) and *PTPRZ1* expression. (K) & (L) *PTPRZ1* expression across distinct cellular states and its correlation with GSC score. (K) was analyzed with one-way ANOVA multiple comparison corrected with Holm-Šidák method. (L) was analyzed with Spearman correlation.\nFig. 2. A PTPRZ1-reactive TCR was identified from a vaccinated GB patient.\n(A) Schematic workflow depicting the sorting and sequencing of PTPRZ1-reactive T cells with CDR3 frequency plots showing dominant TCRs. The later identified reactive TCR is highlighted. (B) Validation of dominant TCR clonotypes from (A) using Jurkat cells transfected with a TCR and a reporter plasmid (top) or Jurkat reporter cells transfected with a TCR plasmid (bottom). (C) Luminescence reporter signal of TCR-Jurkat cells upon overnight coculture with peptide-loaded target cells. (D) Luminescence reporter signal following overnight coculture with peptide-loaded or antigen-expressing target cells. (E) in silico AI-predicted off-targets of the identified PTPRZ1-reactive TCR with presentation probability indicated in blue circles and safety score indicated in red squares. Presentation probability predicts whether the peptide is presented on MHC, and lower safety score denotes a higher likelihood of cross-reactivity. (F) Fluorescence reporter signal of TCR-Jurkat cells upon overnight coculture with various peptide-loaded target cells.\nFig. 3. PTPRZ1^{1814-1822} TCR-T product was persistent, T_{SCM}-abundant and efficient in target cell killing.\n(A) TCR expression on primary human T cells over 3-week period. (B) Percentage of CD4^{+} and CD8^{+} T cells in TCR-T cell products over 3 weeks. (C) CD8^{+} T cell subsets on the day of PBMC isolation and after transduction with longitudinal monitoring on the right. (D) Percentage of surface activation marker-positive, CD137^{+}, cells in CD8^{+} TCR-T cells upon 24h coculture with target cells. (E) Percentage of effector protein-positive, Granzyme B^{+}, cells in CD8^{+} TCR-T cells upon 24h coculture with target cells. (F) Detection of LDH released into the medium after 24h coculture of TCR-T cells and target cells. (G) Titration of E:T ratio with TCR-T cells and target cells, measured with LDH release. 1 unit is 75 x 10^{3} cells. Specific OD is OD_{PTPRZ1}-OD_{Flu}. (H) Schematic of isolating CD4^{+} and CD8^{+} TCR-T cells with MACS and subjecting them to various cocultures. (I) Cytotoxicity upon serial diluting CD4^{+} T cells. (J) Cytotoxicity upon serial diluting CD8^{+} T cells. (I) and (J) were measured with LDH release, and 1 unit equals to 75 x 10^{3} cells in. (K) Cytotoxicity of coculture using reactive CD8^{+} T cells with the target cell and either reactive or non-reactive CD4^{+} T cells, measured with cell counting through flow cytometry. (D)-(F) were analyzed with two-way ANOVA multiple comparison corrected with Holm-Šidák method. (K) was analyzed with paired t-test.\nFig. 4. Intravenous and intracerebroventricular delivery of PTPRZ1-TCR-T is efficacious in experimental flank and brain tumors\n\n(A) Workflow of i.v. ACT on s.c. tumor model. (B) Longitudinal s.c. tumor growth monitoring. (C) Workflow of i.v. and i.cv. ACT on i.c. tumor model. (D) i.c. tumor imaging with preclinical MRI. (E) Longitudinal monitoring of i.c. tumor size with MRI and assessment of radiographic response upon ACT treatment. (F) T cell engraftment validation with cheek blood after ACT, measured with cell counting through flow cytometry. (G) Contour plot of CD8+ TCR-T cell subsets of transferred T cells in the host. (H) Percentages of different CD8+ T cell subsets of transferred T cells. (I) Overall survival of i.c. tumor-bearing mice treated with i.v. and i.cv. ACT. (J) Immunofluorescent staining of grafted i.c. tumor cells, MHC I+, and transferred T cells, CD3+ MHC I+. (K) Transferred T cell numbers in tumoral and non-tumoral tissues in (J) upon ACT treatment. (L) RNAscope™ identifying TMG expression in i.c. tumors. (M) H score analysis of TMG expression in (L). (B) and (E) were analyzed with nonlinear regression. (I) was analyzed with Log-rank test. (F) and (K) were analyzed with one-way and two-way ANOVA multiple comparison, respectively, corrected with Holm-Šidák method. (M) was analyzed with nonparametric t-test.\nFig. 5. PTPRZ1^{1814-1822} TCR-T cells broadly lyse HLA-A*02+ GB primary cells, particularly stem-like SCCs.\n(A) Cytotoxicity measured with LDH release of primary cell line upon coculture with TCR-T cells. (B) Experimental design to assess preferential killing of TCR-T cells on dye-retaining SCCs or dye-losing FCCs. (C) Assessment of specific lysis of SCCs and FCCs upon short-term, 5h, or long-term, 24h, coculture with TCR-T cells, measured with cell counting by flow cytometry. (D) HLA-A2 typing of established GB primary cell lines. (E) Assessment of specific lysis by PTPRZ1^{1814-1822} TCR-T cells normalized to Flu TCR-T cell-treated HLA-A*02+ or HLA-A*02- tumors. (F) & (G) Activation of CD8+ TCR-T cells after 24h coculture with various GB primary cell lines that are HLA-A*02+ or HLA-A*02-. (H) Activation of CD4+ TCR-T cells after 24h coculture with GB primary cell lines. All analyses were performed with two-way ANOVA multiple comparison corrected with Holm-Šidák method.\nFig. 6. IPTOs reveal predominant targeting of AC-like cells and GSCs by PTPRZ1^{1814-1822} TCR-T cells.\n(A) IPTO generation from 3 HLA-A*02+ GB samples and treatment with TCR-T cells. (B) UMAP of malignant cells and T cells derived from Fig. S11A with their marker expression on the right. More canonical markers are visualized in Fig. S11B. (C) Frequency of cell content in IPTOs upon TCR-T cell treatment. (D) *PTPRZ1* expression after TCR-T cell treatment. (E) Cellular states of generated IPTOs with *PTPRZ1* expression. (F) & (G) AC-like module score and frequency of distinct cellular states after ACT. (H) & (I) Correlation of *PTPRZ1* expression and GSC module score in malignant cells in IPTOs and frequency of GSC upon TCR-T cell treatment. Cells score over 0.15 GSC module score are defined as GSCs. (D) & (F) were analyzed with one-way ANOVA multiple comparison corrected with Holm-Šídák method. (C), (G) & (I) were analyzed with Fisher’s exact test. (H) were analyzed with spearman correlation.\nFigures\n\nFigure 1\n\nPTPRZ1 is upregulated in GB, particularly in GSCs and AC-like GB. (A) PTPRZ1 expression in primary tumor compared to adjacent normal tissues in TCGA-GB dataset with t-test. (B) PTPRZ1 expression in single cells of GB from previously published dataset41. Cell type annotation is in Fig. S1D. (C) UMAP of scRNA-sequenced glioma and GB samples from Fig. S1I with cell type annotation. (D) Gene expression of PTPRZ1 for (C). More cell type-defining genes are shown in Fig. S1J. (E) & (F) Protein expression of PTPRZ1 and GFAP from 20 primary and 20 recurrent GB matched samples. Each dot is the average of all tumor pieces of a patient. (G) Correlation of PTPRZ1+ and GFAP+ cell frequencies. Each dot represents a tumor piece. (H) Untargeted ligandomics of primary GB cell lines with overlapping of PTPRZ1 ligands across primary GB cell line.\nThe highlighted overlapped peptide is PTPRZ11814-1822. (I) & (J) Cellular states of cancer cells in (C) and PTPRZ1 expression. (K) & (L) PTPRZ1 expression across distinct cellular states and its correlation with GSC score. (K) was analyzed with one-way ANOVA multiple comparison corrected with Holm–Šídák method. (L) was analyzed with Spearman correlation.\n\nFigure 2\n\nA PTPRZ1-reactive TCR was identified from a vaccinated GB patient. (A) Schematic workflow depicting the sorting and sequencing of PTPRZ1-reactive T cells with CDR3 frequency plots showing dominant TCRs. The later identified reactive TCR is highlighted. (B) Validation of dominant TCR clonotypes from (A) using Jurkat cells transfected with a TCR and a reporter plasmid (top) or Jurkat reporter cells transfected with a TCR plasmid (bottom). (C) Luminescence reporter signal of TCR-Jurkat cells upon overnight coculture with peptide-loaded target cells. (D) Luminescence reporter signal following overnight coculture with peptide-loaded or antigen-expressing target cells. (E) in silico AI-predicted off-targets of the identified PTPRZ1-reactive TCR with presentation probability indicated in blue circles and safety score indicated in red squares. Presentation probability predicts whether the peptide is presented on MHC, and lower safety score denotes a higher likelihood of cross-reactivity. (F) Fluorescence reporter signal of TCR-Jurkat cells upon overnight coculture with various peptide-loaded target cells.\nFigure 3\n\nPTPRZ11814-1822 TCR-T product was persistent, TSCM-abundant and efficient in target cell killing. (A) TCR expression on primary human T cells over 3-week period. (B) Percentage of CD4+ and CD8+ T cells in TCR-T cell products over 3 weeks. (C) CD8+ T cell subsets on the day of PBMC isolation and after transduction with longitudinal monitoring on the right. (D) Percentage of surface activation marker-positive, CD137+, cells in CD8+ TCR-T cells upon 24h coculture with target cells. (E) Percentage of effector protein-positive, Granzyme B+, cells in CD8+ TCR-T cells upon 24h coculture with target cells. (F) Detection of LDH released into the medium after 24h coculture of TCR-T cells and target cells. (G) Titration of E:T ratio with TCR-T cells and target cells, measured with LDH release. 1 unit is 75 x 103 cells. Specific OD is ODPTPRZ1-ODFlu. (H) Schematic of isolating CD4+ and CD8+ TCR-T cells with MACS and subjecting them to various cocultures. (I) Cytotoxicity upon serial diluting CD4+ T cells. (J) Cytotoxicity upon serial diluting CD8+ T cells. (I) and (J) were measured with LDH release, and 1 unit equals to 75 x 103 cells in.\n(K) Cytotoxicity of coculture using reactive CD8+ T cells with the target cell and either reactive or non-reactive CD4+ T cells, measured with cell counting through flow cytometry. (D)-(F) were analyzed with two-way ANOVA multiple comparison corrected with Holm-Šídák method. (K) was analyzed with paired t-test.\n\nFigure 4\n\nIntravenous and intracerebroventricular delivery of PTPRZ1-TCR-T is efficacious in experimental flank and brain tumors (A) Workflow of i.v. ACT on s.c. tumor model. (B) Longitudinal s.c. tumor growth monitoring. (C) Workflow of i.v. and i.cv. ACT on i.c. tumor model. (D) i.c. tumor imaging with preclinical MRI. (E) Longitudinal monitoring of i.c. tumor size with MRI and assessment of radiographic response upon ACT treatment. (F) T cell engraftment validation with cheek blood after ACT, measured with cell counting through flow cytometry. (G) Contour plot of CD8+ TCR-T cell subsets of transferred T cells in the host. (H) Percentages of different CD8+ T cell subsets of transferred T cells. (I) Overall survival of i.c. tumor-\nbearing mice treated with i.v. and i.cv. ACT. (J) Immunofluorescent staining of grafted i.c. tumor cells, MHC I+, and transferred T cells, CD3+ MHC I+. (K) Transferred T cell numbers in tumoral and non-tumoral tissues in (J) upon ACT treatment. (L) RNAscope™ identifying TMG expression in i.c. tumors. (M) H score analysis of TMG expression in (L). (B) and (E) were analyzed with nonlinear regression. (I) was analyzed with Log-rank test. (F) and (K) were analyzed with one-way and two-way ANOVA multiple comparison, respectively, corrected with Holm–Šidák method. (M) was analyzed with nonparametric t-test.\n\nFigure 5\n\nPTPRZ11814-1822 TCR-T cells broadly lyse HLA-A*02+ GB primary cells, particularly stem-like SCCs. (A) Cytotoxicity measured with LDH release of primary cell line upon coculture with TCR-T cells. (B) Experimental design to assess preferential killing of TCR-T cells on dye-retaining SCCs or dye-losing FCCs. (C) Assessment of specific lysis of SCCs and FCCs upon short-term, 5h, or long-term, 24h, coculture with TCR-T cells, measured with cell counting by flow cytometry. (D) HLA-A2 typing of established GB primary cell lines. (E) Assessment of specific lysis by\nPTPRZ11814-1822 TCR-T cells normalized to Flu TCR-T cell-treated HLA-A*02+ or HLA-A*02- tumors. (F) & (G) Activation of CD8+ TCR-T cells after 24h coculture with various GB primary cell lines that are HLA-A*02+ or HLA-A*02-. (H) Activation of CD4+ TCR-T cells after 24h coculture with GB primary cell lines. All analyses were performed with two-way ANOVA multiple comparison corrected with Holm–Sidak method.\n\n![Diagram showing iPSC-derived cerebral organoid, tumor organoid, and cell types](page_120_120_670_350.png)\n\n![UMAP plot of malignant cells and immune cells](page_800_120_670_350.png)\n\n![Bar graph comparing cell content % between Immune cell and Malignant cell](page_120_500_670_350.png)\n\n![Boxplot comparing PTPRZ1 expression between Tumor, Flu, and PTPRZ11814-1822 treatments](page_800_500_670_350.png)\n\n![Scatter plot showing cell state meta-module score distribution](page_120_900_670_350.png)\n\n![Scatter plot showing AC-like module score correlation with GSC module score](page_800_900_670_350.png)\n\n![Bar graph comparing GSC (%) between Tumor, Flu, and PTPRZ11814-1822 treatments](page_120_1300_670_350.png)\n\nFigure 6\n\nIPTOs reveal predominant targeting of AC-like cells and GSCs by PTPRZ11814-1822 TCR-T cells. (A) IPTO generation from 3 HLA-A*02+ GB samples and treatment with TCR-T cells. (B) UMAP of malignant cells and T cells derived from Fig. S11A with their marker expression on the right. More canonical markers are visualized in Fig. S11B. (C) Frequency of cell content in IPTOs upon TCR-T cell treatment. (D) PTPRZ1 expression after TCR-T cell treatment. (E) Cellular states of generated IPTOs with PTPRZ1 expression. (F) & (G) AC-like module score and frequency of distinct cellular states after ACT. (H) & (I) Correlation of PTPRZ1 expression and GSC module score in malignant cells in IPTOs and frequency of GSC upon TCR-T cell treatment. Cells score over 0.15 GSC module score are defined as GSCs. (D) & (F) were analyzed with one-way\nANOVA multiple comparison corrected with Holm-Šidák method. (C), (G) & (I) were analyzed with Fisher’s exact test. (H) were analyzed with spearman correlation.\n\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• SFigure1.pdf\n• SFigure2.pdf\n• SFigure3.pdf\n• SFigure4.pdf\n• SFigure5.pdf\n• SFigure6.pdf\n• SFigure7.pdf\n• SFigure8.pdf\n• SFigure9.pdf\n• SFigure10.pdf\n• SFigure11.pdf\n• TransgenicTcelltherapytargetingtheglioblastomastemcellantigenPTPRZ1withavaccineinducedpatientderivedTcellreceptorSupplementary.pdf"} {"paper_id": "prb77", "title": "Divergently Access N-center 5,6,7-Perifused Cycle", "text": "# Abstract\n\nNitrogen-containing heterocycles are the key components in many pharmaceuticals and functional materials. In this study, we reported a transition metal-catalyzed high-order reaction sequence for synthesizing a structurally unique N-center 5,6,7-perifused cycle (NCPC). The key characteristics included the formation of a seven-membered ring by the 8π electrocyclization of various alkenes and aromatic heterocycles as π-components, in which metal carbene species generated that further induced the cleavage of the α-C-H or -C-C bond. Specifically, the latter could react with various nucleophilic reagents containing -O, -S, -N, and -C. The stereo-controlled late-stage modification of some complicated pharmaceuticals indicated the versatility of this protocol.\n\n[Physical sciences/Chemistry/Organic chemistry/Synthetic chemistry methodology](/browse?subjectArea=Physical%20sciences%2FChemistry%2FOrganic%20chemistry%2FSynthetic%20chemistry%20methodology) [Physical sciences/Chemistry/Organic chemistry/Reaction mechanisms](/browse?subjectArea=Physical%20sciences%2FChemistry%2FOrganic%20chemistry%2FReaction%20mechanisms) [Physical sciences/Chemistry/Medicinal chemistry/Drug discovery and development](/browse?subjectArea=Physical%20sciences%2FChemistry%2FMedicinal%20chemistry%2FDrug%20discovery%20and%20development)\n\n# Introduction\n\nNatural products are often used as the lead compounds1–5 in designing or searching for pharmaceuticals. For example, 5,6,7-perifused carboncycle compounds, tricyclic compounds that share the same center atom, form the core skeleton in many bioactive natural products (Fig. 1 a)6–9. These scaffolds might be used as the lead structures for guiding the synthesis of analogs, thus, promoting drug development. In contrast, N-center perifused cycles (NCPC) might further reveal interesting perspectives for fundamental studies and technological applications because the nitrogen atom has higher electronegativity and smaller van der Waals radius than the carbon atom, which can increase molecular polarity, and water solubility10,11, thus improving molecular selectivity12 and availability (Fig. 1 b). However, when the nitrogen atom is located in the central position of the tricyclic system, the valence state and non-bonding ion pairs can increase the difficulty of synthesis. Specifically, when the medium ring is involved, the difficulty in synthesis might be further increased due to its high torsional strain, unfavorable entropic and enthalpic factors13–18, and other reasons. Previous routes for synthesizing NCPC start from α-formyl-pyrrole19–22 or -pyridine23 as raw materials involved a cumbersome multi-step strategy, and the related methods were also extremely rare (Fig. 1 c). In some contexts, the lack of a simple catalytic protocol to access skeletons might also hinder their applications in synthetic chemistry. Therefore, an efficient synthetic method needs to be developed to further extract or elucidate their application in organic synthesis.\n\nTransition metal-catalyzed cascade cyclization24–26 represents an efficient strategy for assembling various polycyclic systems. As shown in Fig. 1 d, we speculated that the metal-catalyzed 5-endo-annulization of pyridine-alkyne might form zwitterionic vinyl metal species27–40 that might resonate to become a reactive conjugated 8π electronic system and a metal carbene41–43. Electrocyclization reactions44–49 can be driven by heating and are not affected by external conditions. However, the reactivity of metal carbene is closely related to the reaction system. Thus, electrocyclization might be conducted for constructing seven-membered ring structures, promoting the formation of NCPC metal carbene intermediates that provide a great opportunity for applying reactive metal carbene species as a common intermediate for the divergent synthesis of substituted NCPC with high efficiency and flexibility. The metal carbene is a highly versatile intermediate, and NCPC metal carbene provide synthetic chemists access to various structural motifs. The present method might be a suitable alternative for synthesizing NCPC derivatives and could be a way to produce the related N-center substituted series of natural products, which cannot be prepared using other means.\n\nThe protocol included the following points. 1) The final seven-membered ring was constructed by 8π electrocyclization, which was interesting due to its value in addressing the differences in the formation of a medium ring in complicated polycyclic systems. 2) The process included multi-chemical events, which helped in constructing NCPC structural units directly and rapidly through a high-order reaction sequence. 3) The “non-classical” tricyclic metal carbene species were used as a common intermediate while synthesizing the NCPC. 4) The structurally unique NCPC might be used as a platform model for discovering some synthetically useful compounds. 5) This study might provide useful information for designing novel perifused ring analogs with potent activity. Here we reported the results of metal-catalyzed cascade cyclization for the divergent synthesis of NCPC.\n\n# RESULTS AND DISCUSSION\n\nWe used the propargylic derivative of 6-vinylpyridine **1a** as our model substrate for cleaving α-C-H triggered by metal carbene (Table 1). Initially, we screened various metals based on the known alkynophilicity of gold, 50, 51 silver, 52, 53 and copper compounds. 54–56 When the solution of **1a** (0.05 mmol) in toluene was reacted using chloro(triphenylphosphine) gold (AuPPh3Cl) as the catalyst at 90 °C, the expected NCPC product **2a** was formed with a 31% yield (Table 1, entry 1), and its structure was confirmed by X-ray single crystal diffraction analysis. Because gold and silver salts combine to release highly active gold species, improving the catalytic ability of the gold catalyst and then combining AuPPh3Cl and AgOTf showed high reactivity and significantly improved the yield to 60% (Table 1, entry 2). Switching Au(I) to various silver salts, such as AgSbF6, AgOTf, and Ag3PO4, yielded only trace amounts of the product (Table 1, entries 3−5). In contrast, various copper salts yielded the expected products in high yields in all cases (Table 1, entries 6−9). Among them, CuTc was used to produce the cyclization product with the highest yield (96%) (Table 1, entry 9). Subsequently, decreasing the reaction temperature from 90 °C to 60 °C decreased the yield (Table 1, entry 9). Finally, applying commonly used solvents, such as 1,2-DCE, THF and DMF, did not have a better effect (Table 1, entries 10−12).\n\nAfter establishing the optimized reaction conditions, we investigated the scope of NCPCs under Cu-catalysis (Table 2). The eneyne moieties possessing different aryl (**2a**−**2f**), heteroaryl (**2g** and **2h**), alkenyl (**2i**), and alkyl (**2j** and **2k**) substituents at the end of the alkene underwent smooth conversion to yield the corresponding NCPCs with excellent yields. Adding a substituent at the internal position of the eneyne moieties (**2l**−**2n**) also produced the desired products in high yields. The generality of this transformation was further extended by placing various substituents, including aryl (**2o**−**2s**), heteroaryl (**2t**), alkenyl (**2u**), and alkyl (**2v** and **2w**) substituents, on the alkenyl segment at the C6 position of pyridine, where these substrates could be converted into the expected products in high yields. Halogen-containing aryl-substituents (**2e**, **2m** and **2s**) were also competent in the cascade cyclization process, providing an additional functional handle for further modification.\n\nWe further investigated the generality of this transformation by using the annular eneynes that were efficiently converted into the corresponding tetracyclic products (**2x** and **2y**) with excellent yields. When the annular eneyne was replaced by thiophene, the transformation was successful irrespective of whether the α-position or β-position of thiophene was used. Through this process, tetracycle products were formed with a fused aromatic ring (**2z** and **2aa**). The O- or N-containing aromatic compounds, such as benzofuran and indole, also underwent the cascade cyclization sequence, thus providing access to novel fused pentacyclic scaffolds (**2ab** and **2ac**). To confirm the structure of the products, a single crystal X-ray structure of product **2z** was obtained, and the structure of other products was deduced from their NMR spectra.\n\nA part of this study involved research on the α-C-C bond cleavage triggered by metal carbene, in which the highly versatile carbocation intermediate was formed and subsequently reacted with various nucleophilic reagents, leading to the formation of various nucleophilic substituted NCPC products. The three-membered cycle showed high structural strain, 57, 58 which provided a dynamic momentum and a thermodynamic driving force for α-C-C cleavage. Using this, the substrate bearing a cyclopropyl between pyridine and alkyne (**3a**) was synthesized, and the corresponding reaction was conducted to determine whether the ring-opening nucleophilic substitution reaction would occur through the α-C-C cleavage at the α-position of metal carbene. To our delight, we found that the cascade sequence also formed the expecting product (**4a**) with an 11% yield using CuTc as the catalyst and NaOAc as the nucleophilic reagent. In principle, the success of this divergent synthesis process depended on subtle differences in the reactivity between the starting material and the metal catalyst because both metal carbene of different reactivity triggered different transformations. We focused mainly on screening the metal catalyst to further improve the yield. After extensive screening, we found that the silver salts highly stimulated the α-C-C cleavage. Finally, using silver phosphate as the catalyst and TEBA as an additive in the presence of NaOAc, product **4a** was formed with an 80% yield (Detailed conditions screening, please see SI, Table S1).\n\nNext, we investigated the scope of the cascade sequence (Table 3). First, when the phenyl at the end of the eneyne was replaced with thienyl, the ring-opening reaction proceeded slowly to generate the thienyl-substituted product (**4b**) with an 89% yield. Besides aromatic rings, the alkenyl (**4c**) or alkyl (**4d** and **4e**) substitutions at the same position were also suitable substrates, affording the corresponding products in high yields. Similarly, the C2 and C3 positions of thiophene could be changed to obtain the desired tetracyclic products (**4f** and **4g**) with yields of 69% and 78%, respectively. The conversion of thiophene into indole was tolerated and led to the formation of the pentacyclic product (**4h**) with a 71% yield. When the cyclopropyl with a 4-Me-phenyl (**4i**) or 4-F-phenyl (**4j**), was exposed to the standard reaction condition to determine the effect of the substituents, the results indicated that the latter led to a lower yield probably because the para-F-substitution was not favorable for the stability of the carbocation intermediate. Additionally, using sodium formate as a nucleophilic reagent also generated the desired product (**4k**) with a satisfactory yield. Although the nucleophilicity of phenoxyl was relatively weak, it led to the corresponding oxo-substitution of NCPC (**4l**) with a 52% yield.\n\nSubsequently, the reaction was conducted to test whether the transformation could be performed using different types of nucleophilic reagents. The results indicated that 2-thiol-benzothiazole as a nucleophilic reagent could produce the corresponding product (**4m**) with a 63% yield. The nitrogen-containing nucleophiles, such as aniline, sodium azide, 1,2,3-triazole, and tetrazole, were also investigated, and the results indicated that all nucleophilic reagents reacted effectively under standard conditions, resulting in the formation of the desired products (**4n**−**4q**) with satisfactory yields. Regarding the nucleophilicity of the carbon atom, we used the sodium salt of malononitrile and indole as nucleophilic reagents. Both substrates participated in this intermolecular ring-opening substitution reaction, forming the desired products (**4r** and **4s**) with satisfactory yields.\n\nThe late-stage modification of pharmaceuticals 59, 60 is of significant importance for the discovering new drugs or improving bioactivity (Fig. 2). To further demonstrate the potential of this strategy, we examined the application of the ring-opening nucleophilic substitution in the late-stage modification of biologically active small molecules. The different marketed pharmaceuticals, including structurally complicated Gemfibrozil, Idometacin, Estrone, Riluzole, and Candesartan cilexetil, accessing divergent products (**4t**−**4x**) with satisfactory yields. These modifications can also provide key advantages from the perspective of medicinal chemistry. The catalytic system showed high compatibility with several nucleophilic reagents and rapidly established molecular complexity and diversity.\n\nTo demonstrate the practicability of our methodology, the gram-scale reactions of **1c** and **3a** were conducted, and the products **2c** and **4a** were formed with yield of 81% and 71% (Fig. 3 a), respectively. Additionally, the hydrolysis of product **4a** occurred in the presence of potassium carbonate to deliver **4a-1** with a 96% yield. Next, oxidative dehydrogenation proceeded sluggishly; DDQ (1,2-dihloro-4,5-dicyanobenzoquinone) was used as an oxidant, which allowed the conversion of **4a** into **4a-2** rather than cycloazine (Fig. 3 b). This selective oxidation might be attributed to the stability of the tertiary radical at the α-position of phenyl and the oxygen atom.\n\nTo understand this mechanism and elucidate some specific processes of the reaction, several control experiments were conducted. First, the deuterated starting material **1a'** was exposed to the standard conditions. The NMR spectra showed that the reaction generated product **2a** rather than the deuterated product **2a'** (Fig. 4 a), indicating that the intramolecular 1, 2-hydride shift triggered by metal carbene was not involved in the process. To identify the H source, the nondeuterated substrate **1a** was reacted with a mixture of toluene with D2O (toluene/D2O = 1/0.2), and the reaction produced the deuterated product **2a''**; the C4 and C2' positions were deuterated at a 90% and 100% deuterated ratio, respectively (Fig. 4 b). These results suggested that the reaction underwent protonation twice in the presence of the proton donor that came from H2O in the solvent.\n\nBased on the above mechanistic investigations and the results of our experiments, we proposed a plausible catalytic cycle (Fig. 4 c). First, the 5-endo-cyclizations of substrates **1** and **3** proceeded under metal catalysis to form the intermediates **I** and **I′**, which formed the common metal carbene intermediates (**II**) and (**II′**), respectively, via 8π electrocyclization. The results of our control experiment showed that intermediate **II** triggered deprotonation through the cleavage of C-H to produce vinyl metal intermediate **III**, which allowed protonation in the presence of H2O to produce intermediate **IV** along with the release of the metal catalyst. Intermediate **II′** underwent ring-opening via a C-C bond cleavage, which involved nucleophilic substitution along with the generation of vinyl metal intermediate **III′**. A similar protonation process formed intermediate **IV′**. These two polyene intermediates **IV** and **IV′** underwent further isomerization to form final products **2** and **4**, respectively. The whole reaction underwent intermolecular protonation twice rather than intramolecular H-migration.\n\n# CONCLUSION\n\nWe showed the unique synthetic potential of cascade cyclization for constructing structurally diverse N-center polycycle skeletons. The key feature of this transformation was that the 8π electrocyclization could be used to construct the medium ring along with the generation of NCPC metal carbene, which served as versatile building blocks for α-C-H or -C-C cleavage. This procedure is an effective way to rapidly access structurally divergent nitrogen-containing polycyclic products. The 8π electrocyclization might also be used to develop new strategies for rapidly constructing a library of fused polycycles. These structurally attractive NCPC skeletons might be interesting since they can help further enhance the utility of this powerful synthetic strategy.\n\n# Methods\n\n## General procedure for α-C-H bond cleavage\n\nThe freshly prepared 1 (0.05 mmol, 1.0 equiv.), CuTc (10.0 mol%), and toluene (1.0 mL) were added to a 5.0 mL round bottom flask at room temperature, the reaction mixture was stirred at 90°C for 0.5 h and then cooled to room temperature. After completion, the reaction mixture was filtered, and the organic solution was concentrated under vacuo, residue was purified by column chromatography on alkaline alumina to afford the desired product.\n\n## General procedure for α-C-C bond cleavage\n\nAg₃PO₄ (20.0 mol%), TEBA (0.2 mmol, 2.0 equiv.) and nucleophilic reagent (0.3 mmol, 3.0 equiv.) were added to a solution of freshly prepared 3 (0.1 mmol, 1.0 equiv.) in CHCl₃ (2.0 mL) for a Schlenk tube at room temperature, the reaction mixture was stirred at 100°C for 24.0 h and then cooled to room temperature. After completion, the reaction mixture was filtered, and the organic solution was concentrated under vacuo, residue was purified by column chromatography on silica gel to afford the desired product.\n\n# References\n\n1. Newman, D. J. & Giddings, L.-A. Natural products as leads to antitumor drugs. *Phytochem. Rev*. **13**, 123–137 (2014).\n\n2. Shen, B. 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Chem* **5**, 522–545 (2021).\n\n# Tables\n\nTables 1 to 3 are available in the Supplementary Files section.\n\n# Supplementary Files\n\n- [supportinginformation.pdf](https://assets-eu.researchsquare.com/files/rs-2873173/v1/944dcb81546534af8aabf71f.pdf) - supporting information\n- [3a.cif](https://assets-eu.researchsquare.com/files/rs-2873173/v1/24787c54eae04caa2adabce3.cif) - 3a\n- [3a.pdf](https://assets-eu.researchsquare.com/files/rs-2873173/v1/497463ec2f6230b55cdcbbba.pdf) - 3a\n- [2a.pdf](https://assets-eu.researchsquare.com/files/rs-2873173/v1/5bface4394f5c1cb3d431b66.pdf) - 2a\n- [2a.cif](https://assets-eu.researchsquare.com/files/rs-2873173/v1/8a06b78cc9805b2c1b95efc0.cif) - 2a\n- [2z.cif](https://assets-eu.researchsquare.com/files/rs-2873173/v1/399563bbd5f12f217a8bec60.cif) - 2z\n- [2z.pdf](https://assets-eu.researchsquare.com/files/rs-2873173/v1/83a30870b5a465712df732e1.pdf) - 2z\n- [4m.cif](https://assets-eu.researchsquare.com/files/rs-2873173/v1/94042526f4934335c3eb1d14.cif) - 4m\n- [4m.pdf](https://assets-eu.researchsquare.com/files/rs-2873173/v1/deb9ffffce842b3aa44bbd4d.pdf) - 4m\n- [Tables.docx](https://assets-eu.researchsquare.com/files/rs-2873173/v1/189d1f7e73df5b93e388a88e.docx)"} {"paper_id": "prb78", "title": "Electrochemical C-C Bond Cleavage of Cyclopropanes towards the Synthesis of 1,3-Difunctionalized Molecules", "text": "# Abstract\n\nElectrochemistry had a lot of inherent advantages in organic synthesis and many redox reactions have been achieved under electrochemical condition. However, the electrochemical C-C bond cleavage and functionalization reactions are less studied. Here we developed electrochemical C-C bond cleavage and 1,3-difuntionalization of arylcyclopropanes under catalyst-free and external-oxidant-free conditions. 1,3-difluorination, 1,3-oxyfluorination and 1,3-dioxygenation of arylcyclopropanes were achieved with a highly chemo- and regioselectivity by the strategic choice of nucleophiles. This protocol has good functional groups tolerance and can be scaled up. Mechanistic studies demonstrate that arylcyclopropane radical cation yielded from the anode oxidation and the following generated benzyl carbonium are the key intermediates in this transformation. This development provides a new scenario for constructing 1,3-difunctionalized molecules.\n\n- Electrochemistry\n- electrochemical C-C bond cleavage\n- 1\n- 3-difunctionalized molecules\n\n# Introduction\n\nC-C bonds are the basic skeleton of organic compounds and widely existed in nature, it’s deconstructive functionalization are meaningful. [1-2] Cyclopropanes are important building blocks, ring strain release driven C-C bond cleavage and ring-opening of cyclopropanes have been widely applied in total synthesis and pharmacy. [3-4] Donor–acceptor cyclopropanes (DACs) which are activated by vicinal electron-donating and electron-withdrawing groups, are predisposed to ring-opening under Lewis acid catalysis due to the inherent electronic bias. [5-7] Although more common in nature, non-activated cyclopropanes are harder to ring-opening due to insufficient electronic bias. One ring-opening method relies on oxidative addition by transition metals. However, specific directing groups are normally needed for selective ring-opening functionalization and this kind of reaction is limited to ring-opening rearrangement and cycloaddition reactions. [8] Another ring-opening method relies on electrophilic activation with Lewis acidic species. However, most of this kind of transformation is limited to electrophilic addition reactions. [9-17] Ring-opening functionalization of arylcyclopropanes initiated through the single electron oxidation to yield the corresponding radical cations was discovered in the 1970s. [18-19] In recent years, this strategy is further applied in 1,3-aminofunctionalization, 1,3-oxoamination and 1,3-oxochlorination of arylcycropropanes in the presence of oxidants or light. However, in most cases large scalability aplication was not studied, and arylcycropropanes with electron-withdrawing groups could not be well compatible due to high oxidative potential of electron-withdrawing groups substituted arylcycropropanes (Figure 1a). [20-24]\n\nOrganic electrochemistry is reviving due to the ease of scalability, the avoidance of stoichiometric oxidizers or reducing agents, and flexible reaction tunability. [25] Various redox reactions have been achieved by the comsumption of traceless electrons under constant potential or current conditions. [26-38] As a main part of preparative electrosynthesis, anode processes such as C-H functionalization, oxidative coupling, decarboxylation and olefin functionalization had been developed. [39-48] However, electrochemical oxidative C−C bond cleavage and functionalization are rarely developed due to the inertness and weak electronic bias of C−C bonds, which are always encumbered by other bonds. [8-49-50] Herein we developed the electrochemical C−C bond cleavage and 1,3-difunctionalization of arylcyclopropanes under constant current electrolysis based on the following mechanistic proposal (Figure 1b): Firstly, arylcyclopropane is oxidized to the radical cation by anode, which result in the weakness of the Cα-Cβ bond, as the BDE of Cα-Cβ bond decreases more than 30 kcal/mol from the neutral cyclopropane to the corresponding radical cation. [51] Then the radical cation undergoes three-electron SN2 reaction to give the benzyl radical. [52] Different from thermochemical and photochemical conditions, benzyl radical can further lose one electron at anode and be converted to benzyl carbonium under electrochemical conditions. [43] The following nucleophilic attack to the benzyl carbonium can yield the 1,3-difunctionalization product. 1,3-difluorination, 1,3-oxyfluorination and 1,3-dioxygenation of arylcyclopropanes could be accessible with a highly chemo- and regioselectivity by the strategic choice of nucleophiles, and fluorinated products could be prepared by employing Et3N∙3HF as nucleophilic fluorine source. [53-58] A wide variety of arylcyclopropanes with electron-donating and electron-withdrawing groups could be converted to the 1,3-difunctionalized molecules.\n\n# Results\n\n## Investigation of reaction conditions.\nWe began our investigation by exploring the selective synthesis of 1,3-difluorination, 1,3-oxyfluorination and 1,3-dioxygenation products from phenylcyclopropane. After extensive screening of various conditions (for more details, see SI), 1,3-difluorination product **2** was obtained in 77% yield using Et₃N∙3HF as fluorine source by conducting the electrolysis under constant current of 16 mA in an undivided cell equipped with platinum plate as both anode and cathode (Table 1, Entry 1). 1,3-oxyfluorination product **3** was obtained in 47% yield with the concomitant formation of other three 1,3-difuntionalization products under the existence of both Et₃N∙3HF and MeOH (Table 1, Entry 2). The yield of 1,3-oxyfluorination product **3** increased slightly when decreasing the reaction temperature to 0°C (Table 1, Entry 3). An obviously improved yield was observed by using carbon cloth as anode materials (Table 1, Entry 4). The influence of the concentration of phencyclopropane to the reaction could be neglected (Table 1, Entry 5). 1,3-oxyfluorination product **3** was finally observed in 76% yield by adjusting the ratio of Et₃N∙3HF/MeOH (Table 1, Entry 6). The good selectivity of the 1,3-oxyfluorination product **3** was speculated to be controlled by kinetics. At the first step, the reaction rate between MeOH and arylcyclopropane radical cation is larger than reaction rate between Et₃N∙3HF and arylcyclopropane radical cation, which possibly due to lower nucleophilicity of Et₃N∙3HF than MeOH.[57] So arylcropropane radical cation mainly reacts with MeOH instead of Et₃N∙3HF. According to the rate constant equation proposed by Mayr et al, the reaction rate of benzyl carbonium with MeOH or Et₃N∙3HF are both very fast and determined by diffusion rate,[59-60] so fluorination is the major process in the second step because of the excess amount of fluorine source compared with methanol in the reaction system. Further condition screening demonstrated that 1,3-dioxygenation products could be obtained in 95% yield under the electrolysis in MeOH with Bu₄NBF₄ as supporting electrolyte (Table 1, Entry 7).\n\n[IMAGE_RESULTS_1]\n\n## Substrate scope.\nTo investigate the substrate scope of the 1,3-difluorination reaction, we tested diverse range of arylcyclopropanes under the optimized condition (Figure 2). Phenylcyclopropane gave 75% NMR yield (**2**). Methanesulfonyl group no matter at *para* or *meta* position was well amenable to this protocol to give the desired products in good yields (**6** and **7**). Halogen groups such as F, Cl, Br and I were also compatible with this transformation (**8–12**), these groups could supply potential reactive sites for further transformation through coupling reactions. *Ortho* substituted arylcyclopropane was also suitable reaction partner, furnishing the desired 1,3-difluorination product with 58% yield (**13**). Arylcyclopropanes with electron-withdrawing groups (such as ester, amide, acetyl, cyano, nitro and aldehyde groups) were also amenable, furnishing the desired products in 42–56% yields by prolonging the reaction time (**14**–**20**), although these substrates have higher oxidative potential. Trifluoromethyl and oxytrifluoromethyl substituted arylcyclopropanes gave the corresponding products in 49% and 53% yields, respectively (**21–22**). TMS group was retained in this transformation with 52% yield (**23**). Alkyl group such as tert-butyl group underwent the reaction in lower yield of 40% (**24**). 3-Methyl-4-ester substituted arylcyclopropane provided the desired product with 54% yield (**25**). Moreover, heterocyclic arylcyclopropane such as thienyl cyclopropane was also suitable for this reaction (**26**). Then, the feasibility of 1,1-disubstituted cyclopropanes and 1,2-disubstituted cyclopropanes were also tested. 1,1-disubstituted cyclopropanes were good reaction partners to this reaction, giving the 1,3-difluorination products with tertiary-carbon-fluorine bonds formation in good yields (**27–29**). Trans 1,2-diphenylcyclopropane provided 1,3-difluorination products with 61% yield and 1.3:1 diastereoselectivity (**30**). 1,2-diphenylcyclopropane radical cation had been determined to be open geometries.[51] Tri-substituted cyclopropane was also tolerated in this transformation (**31**). Moreover, arylcyclopropanes containing complex nature product scaffolds were also compatible in this transformation. L-menthol scaffold substrate provided the desired product in 86% yield (**32**). 5α-cholestan-3β-ol scaffold substrate provided the coresponding product in 65% yield with 10% starting material recoverd (**33**). Protected sugar group was also tolerated, and 82% yield was obtained (**34**). Androsterone scaffold substrate gave the desired product in 33% yield with 36% starting material recoverd (**35**). The compatibility of these complex substrates further confirm the practicality of this transformation.\n\nThe scope of the 1,3-oxyfluorination reaction was also explored, as shown in Figure 3. *Para*-bromine substituted phenylcyclopropane was compatible to give the target product in moderate yield (**36**). Both electro-donating group and electro-withdrawing groups could be tolerated in this transformation (**37**–**39**). Subsequently, the scope of the alcohols was examined. Alcohols such as EtOH, *n*-BuOH and long-chain primary alcohols (*n*-C₆H₁₃OH and *n*-C₈H₁₇OH) were transformed into desired products with good efficiency (**40**–**43**). 2-Chloro-1-ethanol afforded the desired product in 40% yield (**44**). Secondary alcohols (*i*-PrOH and cyclohexanol) were suitable substrates (**45**–**46**). Sterically hindered tertiary alcohol was also tolerant (**47**). Besides alcohols, ethers could also participate in this reaction as oxygen nucleophiles (Figure 3). 1,3-Oxyfluorination could proceed smoothly when using ether as both reactant and solvent (**48**–**50**). Cyclic ether such as tetrahydrofuran gave interesting product **48** in 43% yields with etheric ring-opening, accompanying with 14% 1,3-difluorination product. 1,2-Dimethoxyethane gave 1,3-oxyfluorination product **49** in 44% yield. The reaction system was separated into two phases and not conductive when using tetrahydropyran as both reactant and solvent. To solve the problem of solubility and conductivity, DCE was added to enhance the solubility and 1,3-oxyfluorination product **50** was obtained in 36% yield. Notably, C-O etheric bond was broken in these transformations. It is proposed that oxonium is the key intermediate for cleavage of C-O etheric bond (for more details, see SI).[61–62]\n\nFinally, the scope of the 1,3-dioxygenation reaction was investigated (Figure 4). Arylcyclopropanes with electron-donating groups (-OMe, -OPh) gave 74% and 93% yields, respectively (**51**–**52**). *Para* tert-butyl substituted arylcyclopropane underwent the reaction in 85% yield (**53**). Both TMS and halogen groups could be tolerated (**54**–**55**). The electronically deficient arylcyclopropane could also give 1,3-dioxygenation products with high yields (**56–57**).\n\nThe scalability of the method was demonstrated by using carbon cloth as anode and nickel foam as cathode instead of expensive platinum electrode with equivalent amount of Et₃N∙3HF (Figure 5). The yields increased for most of the tested substrates when operated at gram scale. The yields increased from 75% to 90% for *para*-methanesulfonyl substituted phenylcyclopropane (**6**). The yields increased to 65% and 63% for ester (**14**) and oxytrifluoromethyl (**22**) substituted arylcyclopropanes. Only for 4-bromocyclopropylbenzene (**10**), the yields decreased slightly from 67% to 63%.\n\n# Discussion\n\nTo gain more insight into the aforementioned transformation, mechanistic studies were conducted. Redox potential of the cyclopropanes was tested by cyclic voltammetry experiments (Figure 6a). The alkyl substituted cyclopropane **1c** has high oxidation potential and no oxidation peak can be observed under 3V. In contrast, arylcyclopropanes even with strong electron withdrawing group (-NO₂) have relatively lower oxidative potential (Eonset = 1.68 V for **1** and Eonset = 1.99 V for **1a**). These results illustrate that aryl group is important for the oxidation of the cyclopropane substrates. The charge distribution of phenylcyclopropane radical cation has been studied by DFT calculation (Figure 6b). The results show that distal C atom in cyclopropane motif possess partial positive charge and are the potential nucleophilic attack sites. Considering the reaction between benzyl radical and dioxygen was very fast (rate constant 2.8×10⁹ L∙mol⁻¹∙s⁻¹),[63] the reaction was run in the presence of dioxygen instead of nitrogen in order to trap the possible benzyl radical intermediate. The detection of the oxygenation products highly proposed the formation of the benzyl radical during the reaction (Figure 6c). In addition, the existence of benzyl radical was also evidenced by the trapping experiment using BrCCl₃.[64-65] Furthermore, the electrolysis of phenylcyclopropane and Et₃N∙3HF in CH₃CN resulted in isolation of amidation product, which suggest the involvement of benzyl carbonium intermediate during the reaction (Figure 6d).[66-67]\n\nIn conclusion, we have developed a electrochemical C-C bond cleavage of arylcyclopropanes, enabling 1,3-difunctionalization of arylcyclopropanes to yield 1,3-difluorination, 1,3-oxyfluorination and 1,3-dioxygenation products. Neither additional oxidant and catalyst were needed in this transformation. Productive gram-scale 1,3-difluorination reaction was running by using stoichiometric amount of commercial available Et₃N∙3HF as fluorine source. Mechanistic studies show that arylcyclopropane radical cation and benzyl carbonium play paramount role in this reaction. 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S. Intermolecular Ritter-Type C–H Amination of Unactivated sp3 Carbons. *J. Am. Chem. Soc.* **134**, 2547–2550 (2012).\n\n# Supplementary Files\n\n- [SI.pdf](https://assets-eu.researchsquare.com/files/rs-126490/v1/99409edaf43b7fe51d64747e.pdf) \n Supporting Information"} {"paper_id": "prb79", "title": "Next Generation Thiazolyl Ketone Inhibitors of Cytosolic Phospholipase A2 α: from Synthesis to Chemotherapeutic Mechanism of Action", "text": "Next Generation Thiazolyl Ketone Inhibitors of Cytosolic Phospholipase A2 α: from Synthesis to Chemotherapeutic Mechanism of Action\n\nBerit Johansen\nberit.johansen@ntnu.no\n\nNorwegian University of Science and Technology\n\nFelicity Ashcroft\nNorwegian University of Science and Technology\n\nAsimina Bourmpoula\nNational and Kapodistrian University of Athens\n\nNur Mahammad\nNorwegian University of Science and Technology\n\nEfrosini Barbayianni\nNational and Kapodistrian University of Athens\n\nAstrid Feuerherm\nNorwegian University of Science and Technology\n\nKonstantinos Alevizopoulos\nVentac Partners\n\nEdward Dennis\nUniversity of California at San Diego https://orcid.org/0000-0003-3738-3140\n\nGeorge Kokotos\nNational and Kapodistrian University of Athens https://orcid.org/0000-0003-3753-7082\n\nArticle\n\nKeywords:\n\nPosted Date: November 28th, 2023\n\nDOI: https://doi.org/10.21203/rs.3.rs-3485987/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\nAdditional Declarations: Yes there is potential Competing Interest. AJF and BJ, EAD and GK are shareholders, while FJA and NM were employees of Coegin Pharma at the time of results generation.\n\nVersion of Record: A version of this preprint was published at Nature Communications on January 2nd, 2025. See the published version at https://doi.org/10.1038/s41467-024-55536-9.\nNext Generation Thiazolyl Ketone Inhibitors of Cytosolic Phospholipase A2 α: from Synthesis to Chemotherapeutic Mechanism of Action\n\nFelicity J. Ashcroft1, Asimina Bourmpoula2,3, Nur Mahammad1, Efrosini Barbayianni2, Astrid J. Feuerherm1, Konstantinos Alevizopoulos4, Edward A. Dennis5, George Kokotos2,3*, Berit Johansen1,6*.\n\nAffiliations\n\n1. Department of Biology, Norwegian University of Science and Technology, Realfagbygget, 7491 Trondheim, Norway\n\n2. Department of Chemistry, National and Kapodistrian University of Athens, Panepistimiopolis, Athens 15771, Greece\n\n3. Center of Excellence for Drug Design and Discovery, National and Kapodistrian University of Athens, Panepistimiopolis, Athens 15771, Greece\n\n4. Ventac Partners, Ch. du Vallon 4, 1400, Yverdon-les-Bains, Switzerland\n\n5. Department of Chemistry and Biochemistry and Department of Pharmacology, School of Medicine, University of California at San Diego, La Jolla, California, USA\n\n6. email: berit.johansen@ntnu.no\n\n* Corresponding authors\n\nAbstract\n\nEicosanoids regulate the pathologies of inflammation and carcinogenesis and limiting their production by inhibiting group IVA cytosolic phospholipase A2 (cPLA2α) is a potential approach to cancer treatment. Here we report the synthesis of a new generation of thiazolyl ketone inhibitors of cPLA2α starting from compound GK470 (AVX235), and the discovery of a more potent and selective lead, GK420 (AVX420), with significant chemotherapeutic properties. A cancer cell line screen revealed the selective growth inhibitory effects of AVX420 in acute leukemias, uncovering a novel function of cPLA2α to promote cancer cell survival during oxidative stress by epigenetic control of tumour suppressor gene transcription. Moreover, we showed that in sensitive cells, AVX420 increased intracellular reactive oxygen species (ROS) and instigated a transcriptional response resulting in cell death. Our study suggests AVX420 has the potential to treat acute leukemias, and other cancers with specific adaptations to a high ROS burden.\nIntroduction\n\nThe polyunsaturated fatty acid arachidonic acid (AA) and its metabolites, eicosanoids, i.e. prostaglandins, thromboxanes, leukotrienes, etc., have attracted considerable interest in relation to inflammatory processes and diseases, including cancer, cardiovascular and autoimmune diseases, and metabolic disorders.\\(^{1-3}\\) AA is generated by the action of phospholipase A\\(_2\\) (PLA\\(_2\\)), which catalyzes its hydrolytic cleavage from membrane glycerophospholipids.\\(^{4}\\) PLA\\(_2\\) enzymes constitute a superfamily of enzymes, divided into many groups and subgroups. Among them, cytosolic Group IVA PLA\\(_2\\) (cPLA\\(_2\\alpha\\)) plays a critical role in the release of AA and is the most well-studied PLA\\(_2\\) in inflammation.\\(^{4,5}\\)\n\nThe involvement of PLA\\(_2\\)s in various inflammatory conditions renders them attractive targets for the development of new medicinal agents. Accordingly, a variety of synthetic PLA\\(_2\\) inhibitors, targeting the most relevant human PLA\\(_2\\)s, have been reported in the scientific and patent literature.\\(^{4,6}\\) Considerable attention has been focused on the pharmaceutical inhibition of cPLA\\(_2\\alpha\\) and some of the most important inhibitors studied in clinical and pre-clinical trials are shown in Figure 1. Ecopladiab and giripladiab (\\(\\mathbf{1}\\), **Fig. 1**) are indole-based cPLA\\(_2\\alpha\\) inhibitors, presenting in vivo efficacy, whose clinical trials for osteoarthritis were terminated, when gastroenterological side effects were observed in a phase II study.\\(^{7,8}\\) An inhibitor of related structure, ZPL-5,212,372 (\\(\\mathbf{2}\\), **Fig. 1**), demonstrated excellent efficacy in animal models of airway and skin inflammation and entered trials for topical application\\(^9\\). Another potent indole-based cPLA\\(_2\\alpha\\) inhibitor, ASB14780 (\\(\\mathbf{3}\\), Fig. 1), was found to exhibit beneficial effects for the treatment of nonalcoholic fatty liver diseases.\\(^{10,11}\\) AK106-001616 (\\(\\mathbf{4}\\), **Fig. 1**) demonstrated strong in vitro inhibition of cPLA\\(_2\\alpha\\) and considerable in vivo efficacy for inflammation, neuropathic pain, and pulmonary fibrosis.\\(^{12}\\) The potent inhibitor pyrrophenone\\(^{13}\\) (\\(\\mathbf{5}\\), **Fig. 1**) has been used in various in vitro and in vivo studies, while RSC-3388 (\\(\\mathbf{6}\\), **Fig. 1**) has been shown to sensitize aggressive breast cancer to doxorubicin through suppressing ERK and mTOR kinases,\\(^{14}\\) and to halt Streptococcus pneumonia-induced polymorphonuclear cells transepithelial migration in vitro, highlighting the importance of cPLA\\(_2\\alpha\\) in eliciting pulmonary inflammation during pneumococcal infection.\\(^{15}\\) Our groups have developed a series of 2-oxoamides as inhibitors of cPLA\\(_2\\alpha\\) and studied their in vitro and in vivo activities.\\(^{16}\\) AX048 (\\(\\mathbf{7}\\), **Fig. 1**) exhibited an antihyperalgesic effect in rats, blocking PGE\\(_2\\) release evoked by substance P.\\(^{17}\\) Among a series of 1-heteroarylpropan-2-ones, compound \\(\\mathbf{8}\\) (**Fig. 1**) was found to be a highly potent inhibitor of cPLA\\(_2\\alpha\\).\\(^{18}\\) We have also developed a series of thiazolyl ketones and demonstrated that GK470 (AVX235, \\(\\mathbf{9}\\), **Fig. 1**) has in vivo anti-inflammatory effects both in a preventative and a curative arthritis model induced by collagen comparable to the reference drugs methotrexate and Enbrel, respectively.\\(^{19}\\)\n\nIn addition to driving inflammatory processes, eicosanoids have established roles in promoting cancer and prostaglandin E\\(_2\\) (PGE\\(_2\\)) is the best studied example of this.\\(^{20}\\) As such, cPLA\\(_2\\alpha\\) is now generating interest as a chemotherapeutic target,\\(^{21}\\) particularly in breast cancer, where PLA2G4A overexpression was initially associated with Her-2 positive basal-like subtype and predicted poor\nresponse to endocrine therapy.\\(^{22}\\) Subsequent studies showed that enhanced choline metabolism in basal-like xenograft models was associated with higher cPLA\\(_2\\)α activity\\(^{23}\\) and inhibition of cPLA\\(_2\\)α with AVX235 inhibited tumor growth as effectively as a dual PI-3K mTOR inhibitor.\\(^{24}\\) In line with this, a separate study showed that ASB14780 reduced AA levels and inhibited the growth of triple-negative breast cancer xenografts, dependent on the oncogenic activity of PI3KCA and restricted dietary AA.\\(^{25}\\) The effects of cPLA\\(_2\\)α inhibition in this study were predicted to be mediated via suppression of PGE\\(_2\\) release. In other cancers where cPLA\\(_2\\)α has prognostic significance e.g., lung cancer, acute myeloid leukemia and glioblastoma, synthetic cPLA\\(_2\\)α inhibitors have been shown to suppress cancer cell or tumor growth\\(^{20,26-30}\\) and in preclinical models of ovarian and cervical cancers were effective sensitization agents for radiation or chemotherapy.\\(^{31-33}\\) There is therefore a strong drive to develop more potent, selective, and safe cPLA\\(_2\\)α inhibitors for systemic use as targeted anti-cancer drugs and a parallel need to understand the oncogenic events that support cPLA\\(_2\\)α dependency in cancer for effective targeting of their use. To this end, we utilized GK470 (AVX235), which had previously been shown to be effective and safe in preclinical disease models, as a starting point for a new series of thiazolyl ketone inhibitors and were successful in improving upon its potency and selectivity. By exploring the mechanism of action of the new lead compound, we uncovered a highly sensitive potential susceptibility of acute leukemias to cPLA\\(_2\\)α inhibition, based on a novel role of the enzyme in oxidative stress signaling.\nFigure 1. Selected inhibitors of cPLA2α studied in clinical or pre-clinical trials.\n\nResults\n\nDesign and synthesis of the inhibitors\n\nThe inhibitors in the present work were designed starting from the structure of the lead thiazolyl ketone GK470 (AVX235), which possesses a ClogP value of 5.96 (calculated using ChemOffice Ultra 11.00). To develop new analogs obeying the Lipinski rule,\\(^{34}\\) the lipophilicity could be reduced by replacing the medium carbon chain of the benzene ring by a chain introducing either a heteroatom such as oxygen or sulfur or a phenyl group (**Scheme 1A**). Furthermore, introducing a\nmethyl group at the carbon atom between the activated carbonyl and the oxygen atom could potentially improve the metabolic stability.\n\nPhenols **10a-e** and thiol **10f** were appropriately alkylated to afford esters **11a-j**, which further reduced to alcohols **12a-j** by DIBALH (**Scheme 1B**). Oxidation of **12a-j** to aldehydes with NaOCl in the presence of TEMPO and subsequent treatment with TBDMSCN and KCN led to cyanohydrins **13a-j**. Thiazolines **14a-j** were synthesized by reaction of the cyano group of **13a-j** with either methyl or ethyl cysteinate, while aromatization to **15a-j** was achieved by oxidation with BrCCl\\(_3\\) in the presence of DBU. Finally, the target thiazolyl ketones **17a-j** were synthesized after deprotection of **15a-j** with HCl/MeOH, followed by oxidation of **16a-j** with Dess-Martin periodinane.\nA. Design of new thiazolyl ketones\n\nReduction of lipophilicity by replacing the medium chain\n\nGK470 (AVX235)\n\nPotential increase of plasma stability by introducing a methyl group\n\nB. Synthesis of inhibitors\n\n![Synthetic scheme showing the synthesis of inhibitors from GK470 (AVX235)](page_186_320_1207_1092.png)\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
10-17XYR1R2R3
aCH2On-C7H15HC2H517a: GK401
bOOn-C7H15HCH317b: GK420
cOOC6H5HCH317c: GK403
dOOp-F-C6H4HCH317d: GK440
eSOn-C6H13HCH317e: GK427
fOSn-C6H13HCH317f: GK419
gCH2On-C7H15CH3CH317g: GK402
hOOn-C7H15CH3CH317i: GK428
iOOC6H5CH3CH317j: GK449
jSOn-C6H13CH3CH3
\n\nScheme 1. Reagents and conditions: (a) BrCH2COOEt, Et3N, CHCl3; (b) CH3(CH2)5Br, K2CO3, acetone; (c) BrCH2COOEt, or BrCH(CH3)COOEt K2CO3, acetone; (d) DIBALH, Et2O; (e) i. NaOCl, TEMPO, NaBr, NaHCO3, EtOAc/PhCH3/H2O 3:3:0.5, -5 °C; ii. TBDMSCN, 18-crown-6, KCN, CH2Cl2; (f) HCl.H-L-Cys-O-Me or HCl.H-L-Cys-OEt, CH3COO-NH4+, MeOH; (g) DBU, BrCCl3, CH2Cl2; (h) 4N HCl/MeOH or 4N HCl/Et2O; (i) Dess-Martin periodinane, CH2Cl2.\nAn alternative route for the construction of the thiazolyl ring was also explored, in case of lack of commercially available TBDMSCN. Alcohols **12b,g-i** were oxidized to the corresponding aldehydes by Dess-Martin periodinane and cyanohydrins **18a-d** were synthesized by treatment with NaHSO\\(_3\\), followed by KCN (**Scheme 2**). Cyclization to thiazolines by reaction with methyl cysteinate and subsequent aromatization by treatment with DBU/BrCCl\\(_3\\) afforded compounds **17b,g-i**.\n\n![Reaction scheme showing the synthesis of compounds 12b,g-i, 18a-d, and 17b,g-i](page_495_367_1017_246.png)\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
18XR1R2
aOn-C7H15H
bCH2n-C7H15CH3
cOn-C7H15CH3
dOC6H5CH3
\n\nScheme 2. (a) i. Dess-Martin periodinane, CH\\(_2\\)Cl\\(_2\\), ii. NaHSO\\(_3\\) 4N, CH\\(_2\\)Cl\\(_2\\), iii. KCN 4N, H\\(_2\\)O/THF 1:1; (b) i. HCl.H-L-Cys-OMe, CH\\(_3\\)COO-NH\\(_4^+\\), MeOH, ii. DBU, BrCCl\\(_3\\), CH\\(_2\\)Cl\\(_2\\).\n\nIn vitro inhibition of cPLA\\(_{2\\alpha}\\), GVIA iPLA\\(_2\\) and GV sPLA\\(_2\\).\n\nAll synthesized thiazolyl ketones were tested for their in vitro inhibitory activity on recombinant human cPLA\\(_{2\\alpha}\\) and selectivity over human calcium-independent GVIA iPLA\\(_2\\) and secreted GV sPLA\\(_2\\) using our previously described group-specific radioactivity-based mixed micelle assays.\\(^{16}\\) The inhibition results are presented either as percent inhibition or as \\(X_l(50)\\) values in Table 1. First, the percent of inhibition for each PLA\\(_2\\) enzyme at 0.091 mol fraction of each inhibitor was determined and then, the \\(X_l(50)\\) values were measured for compounds that displayed greater than 90% inhibition of cPLA\\(_{2\\alpha}\\). The \\(X_l(50)\\) is defined as the mole fraction of the inhibitor in the total substrate interface required to inhibit the enzyme activity by 50%. For comparison purposes, data for the inhibitor GK470 are included in **Table 1**.\n\nAt first, ethyl ester GK401 showed weaker inhibition in comparison to GK470 (Table 1), indicating that the small methyl ester group is preferable as a substituent on the thiazolyl ring. The introduction of an oxygen atom in replacement of the carbon attached to the phenyl group led to inhibitor GK420, which clearly exhibits more potent inhibitory activity against cPLA\\(_{2\\alpha}\\) (\\(X_l(50)\\) 0.0016). However, shortening the carbon chain by one atom (GK419) led to considerable reduction of the inhibitory potency. Thus, an heptyloxy group seems to have the optimum length on the\nphenyl group, offering potent inhibition and at the same time being acceptable according to the Lipinski rules with ClogP 5.02. Replacing the oxygen atom of GK419 by sulfur (compound GK427) led to increased inhibition of cPLA2α (\\( X_{i}(50) \\) 0.0010), which is comparable to GK420. Increased inhibition of cPLA2α in comparison to GK470, was also observed for GK403 (\\( X_{i}(50) \\) 0.0014), carrying a phenoxy group instead of the heptyloxy one. Furthermore, the introduction of a fluorine group at the para position of the phenoxy group (GK440) led to potent inhibition of cPLA2α (\\( X_{i}(50) \\) 0.0010). All the new analogs mentioned above can be considered selective inhibitors of cPLA2α, because all present minimal inhibition of GVIA iPLA2 and GV sPLA2 at high concentrations (0.091 mole fraction), as shown in Table 1.\n\nTable 1. In vitro inhibitory activities and human plasma stability of GK470 analogs.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
In vitro assaysHuman plasma stability
cPLA2α
% Inhib
\\( X_{i}(50) \\)
GVIA iPLA2
% Inhib
GV sPLA2
% Inhib
(4 h)(20+ h)
GK470>90
0.011 ± 0.005
864160.610.55*
GK40188404669.316.25*
GK42099
0.0016 ± 0.0002
04663.318.05
GK419500298252.7
GK42798
0.0010 ± 0.0001
7.54461.38.05
GK40395
0.0014 ± 0.0001
343221.5ND*
GK440100
0.0010 ± 0.0001
03121.30.9 *
GK40279615079.747.3*
GK43997
0.0029 ± 0.0004
675359.912.8*
GK42894
0.0038 ± 0.0001
543635.91.65
GK44997
0.0017 ± 0.0005
67536318.35*
\n\nThe % inhibition of the compounds are reported at 0.091 mole fraction for each inhibitor (% Inhib). Their stability in human plasma is reported as the % of the compound that is remaining after 4 hours incubation (4 h) or after 20 h, 24h 39 min*, or 25 h, (20+ h) incubation.\n\nNext, we evaluated the new thiazolyl ketones carrying an α-methyl group to the activated carbonyl group. In all cases, this small substituent resulted in reduction of the inhibitory potency on cPLA2α. Introduction of the methyl on GK470 (compound GK402) resulted in considerable loss of inhibitory activity. However, α-methyl substituted analogs GK439, GK428 and GK449 retained inhibitory potency (\\( X_{i}(50) \\) 0.0029, 0.0038 and 0.0017, respectively), reduced in comparison to the corresponding analogs without methyl. Again, α-methyl substituted analogs can be considered selective inhibitors of cPLA2α, because all present minimal inhibition of GVIA iPLA2 and GV sPLA2 at high concentrations (0.091 mole fraction) (Table 1).\n\nThe stability of the new analogs in human plasma was studied over approximately 24 hours by LC-MS/MS and the results at 4 hours and the final timepoint (20 -25 hours) are included in Table 1. Inhibitors GK420, GK427 and GK449, which are 7 to 11 times more potent than GK470, present similar recoveries. On the contrary, GK403 and GK440, although potent inhibitors, were considerably less stable in human plasma.\nGK420 is a potent inhibitor of cPLA2α in cellular assays.\n\nTo test the inhibitory activity of the compounds in cells, we measured their effect on the release of AA from synoviocytes stimulated with IL1β (Table 2). GK420 was the most potent compound, inhibiting 99 % of AA release at 1 μM with an IC50 of 160 nM. Combined with favorable selectivity and stability it was thus chosen for further evaluation. We looked specifically at how it modulated eicosanoid levels in response to stimulation both in whole blood and in isolated peripheral blood mononuclear cells (PBMCs) and checked for off-target effects on AA metabolism in whole blood by also measuring the effect of GK420 on eicosanoid release in the presence of exogenous free AA.\n\nTable 2. Inhibition of arachidonic acid release.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Arachidonic acid release
% Inhibition (1 μM)IC50 (μM)
GK47069 ± 110.68 ± 0.18
GK40152 ± 60.98 ± 0.39
GK40223 ± 7NA
GK40359 ± 100.74 ± 0.28
GK41983 ± 90.24 ± 0.06
GK42099 ± 130.16 ± 0.07
GK42771 ± 150.52 ± 0.20
GK42813 ± 9NA
GK43980 ± 110.41 ± 0.16
GK44090 ± 130.25 ± 0.11
GK44965 ± 80.64 ± 0.12
\n\nSW982 synoviocytes were stimulated with IL-1β for 4 hours. The % inhibition is reported at 1 μM and IC50 values were calculated based on testing of the compounds in the range of 1 - 5 μM. NA indicates that the IC50 could not be calculated in the dose range used.\n\nIn whole blood, bacterial lipopolysaccharide (LPS) stimulated the release of PGE2, TXB2, and 15-HETE. GK420 suppressed their production but had no effect when excess free AA was included (Fig. 3a) indicating AA metabolism was not affected by GK420. In contrast, the non-selective COX inhibitor indomethacin suppressed the production of PGE2 and TXB2 in the absence and presence of exogenous free AA. The levels of LTB4, 12-HETE, 5-HETE and 11,12-EET were not affected by LPS stimulation, but increased when exogenous AA was included, irrespective of the presence of AVX420 (Fig. S1a).\n\nIn PBMCs, the calcium ionophore A23187 stimulated the release of TXB2, PGE2, 6-keto PGF1α, LTB4 and 12-HETE. LTB4 showed the greatest induction versus unstimulated control in this cell type with an 18-fold increase versus between a 4-to-6-fold increase for the other eicosanoids. GK420 dose-dependently inhibited LTB4, PGE2 and TXB2 with IC50 values of\n317 nM, 1.1 μM, and 2.2 μM respectively, indicating inhibitory potency might be related to level of stimulation (Fig. 3b). A tendency to suppress both 6-keto PGF1α and 12-HETE was also observed although IC_{50} values could not be calculated (Fig. S1b). In summary, GK420 was found to be a specific inhibitor of cPLA_{2α}, which prevents the stimulated release of AA and production of both COX and LOX-derived metabolites of AA in primary human cells with no discernable inhibition of COX or LOX enzymes. Together, this data was considered sufficient to move GK420 forward to a cell line-based assessment of its anti-cancer potential, and GK420 will hereafter be referred to as AVX420.\n\n![Ex vivo suppression of eicosanoid production by GK420. Panels a and b show boxplots of PGE2, TxB2, 15-HETE, and LTB4 levels in plasma and supernatants, respectively, under various conditions.](page_256_682_1092_1012.png)\n\nFigure 3. Ex vivo suppression of eicosanoid production by GK420. a. Eicosanoid levels in the plasma of whole blood pretreated with vehicle or inhibitors (GK420 (3, 10 or 30 μM), ATK (10 μM), indomethacin (1 μM)) before stimulation with LPS (1 μg/ml, 24 h). In LPS+AA, 5 μM AA was included for the final 30 min. b. Eicosanoid levels in the supernatants of isolated human PBMCs pretreated with vehicle (DMSO), GK420, naproxen, celecoxib, or NDGA for 90 min before addition of A23187 (30 μM, 15 min). Data are\nthe mean and standard deviation, with min and max (whiskers) of the eicosanoid levels in pmol/ml from four blood donors Repeated measures one way ANOVA was performed, followed by Dunnets multiple comparison test between inhibitors and appropriate stimulated control, * indicates p<0.1, ** p<0.05 and *** p<0.01.\n\ncPLA2α inhibitors target cancers where survival depends on PRC2- dependent transcriptional repression.\n\nTargeting specific molecular vulnerabilities in cancer is considered a key approach to reducing the adverse effects of chemotherapy. However, the events that govern the susceptibility to suppression of the cPLA2α-AA signaling pathway in cancer remain largely unexplored. We therefore took the approach of screening the antiproliferative activity of AVX420 in a panel of 66 cancer cell lines (hereafter referred to as the cancer cell line screen or CCLS) to allow us to investigate molecular and genetic vulnerabilities to the drug. AVX235 and AVX002, a cPLA2α inhibitor of a different chemical class,\\(^{35}\\) were screened alongside AVX420, such that factors that were found to be in common between compounds could be more reliably considered to be specific to cPLA2α inhibition. All three compounds were broadly effective in the screen, with average IC\\(_{50}\\) values <20 \\(μ\\)M). AVX420 however showed stronger cell line selectivity than either AVX235 or AVX002 (**Fig. S2**), which manifested in more robust associations with genetic factors in later analyses and may reflect its higher potency.\n\nComparing the activity of novel compounds against a reference library of known chemotherapeutics has been used historically to predict their mechanism of action.\\(^{36}\\) We thus compared the activity profiles of the cPLA2α inhibitors to 121 drugs of known function. In a network tree where linkages with Pearson’s correlation of >0.5 are shown, the cPLA2α inhibitors are linked to one another, and AVX002 and AVX235 had no additional linkages. This supports the unique targeted action of these inhibitors. AVX420 had two additional linkages, to cytarabine and melphalan (**Fig. 4a**). Unsupervised hierarchical clustering of the drug correlations revealed an interesting similarity between the action of cPLA2α inhibitors and multiple histone methyltransferase inhibitors (**Fig. S3**), specifically drugs targeting EZH2, the catalytically active component of the polycomb group repressive complex 2 (PRC2). The finding suggests that cPLA2α may play a novel role in epigenetic silencing of transcription in cancer. A full list of the drugs and their targets, and a table listing the compounds that, based on the hierarchical clustering, showed the most similarity cPLA2α inhibitors can be found in supplemental information (**Table S1** and **Table S2** respectively).\nFigure 4. Oncogenic pathways associated with sensitivity to cPLA2α inhibition a. Network tree showing linkages between related compounds (Pearson correlation coefficient >0.5). Colors indicate to which hierarchical clusters the inhibitors belong (as shown in Fig. S3). cPLA2α inhibitors are indicated in red. b-d. Gene set enrichment analysis based on a ranking of Pearson’s correlation with compound activities performed against the Oncogenic signatures collection (C6) in MSigDB. Significantly enriched gene sets (FDR of < 5%) are shown.\nMutations to oncogenes and tumor suppressor genes are major driver of tumour phenotype and can predict the response to classes of chemotherapeutic drugs.\\(^{37}\\) We tested whether mutations to 114 validated cancer driver genes represented by at least 3 cell lines in the CCLS were associated with a significant shift in the IC\\(_{50}\\) of the inhibitors. We found that sensitivity to both AVX420 and AVX235 was associated with mutation to the mixed lineage leukemia gene (MLL) and additional sex combs-like 2 (ASXL2), while there were no genes whose mutational status was associated with sensitivity to AVX002. MLL and ASXL2 are both involved in the control of transcription by modulating histone 3 (H3) methylation. MLL, which had the most significant association in each case, codes for a histone lysine [K]-methyl transferases (KMT2A) that activates transcription by trimethylating H3K4 and antagonizes transcriptional repression by PRC2.\\(^{38}\\) Loss of function mutations, such as occur in approximately 4% of all cancers,\\(^{39}\\) would likely contribute to target gene repression by PRC2. A full list of genes where mutations were associated with sensitivity to AVX420 can be found in Table S3.\n\nGenome-wide gene expression data made available via the cancer cell line encyclopedia\\(^{40}\\) was then used to associate drug sensitivity with basal transcript levels. The expression of 18900 genes was available for 56 of the 66 cell lines screened and we correlated this with the activity of each inhibitor. Negative correlations signify association with drug sensitivity and positive correlations with drug resistance. The correlations were first ranked, and relevant signaling pathways associated with inhibitor susceptibility were identified by gene set enrichment analysis (GSEA)\\(^{41}\\) against the oncogenic signatures collection in the molecular signature database (MSigDB) (Fig. 4b-d). In line with the previous results, a strong association between sensitivity to all three cPLA\\(_2\\)α inhibitors and high basal activity of PRC2 was indicated by the enrichment of gene sets upregulated by knockdown of components of PRC2, including EZH2. The activity of the mTORC1 pathway, indicated by enrichment of gene sets upregulated by treatment with the mTORC1 inhibitor rapamycin was also associated with sensitivity to all three inhibitors. The latter result is perhaps unsurprising given the evidence for an interaction between cPLA\\(_2\\)α activity and mTOR signaling, particularly in breast cancers.\\(^{25,42,43}\\) We additionally found that sonic hedgehog (SHH) and janus associated kinase 2 (JAK2) activation was associated with sensitivity to both AVX420 and AVX235. Of note, the JAK2 inhibitor ruxolitinib clustered along with the cPLA\\(_2\\)α and EZH2 inhibitors in the compound activity profiling (Table S2) further suggesting involvement of this pathway in drug sensitivity.\n\nIndividual cancer-related genes, whose basal expression was associated with sensitivity to cPLA\\(_2\\)α inhibition, were identified from a list of 361 genes with known links to cancer. When correlations with an FDR of 5% were considered significant, only associations with AVX420 were identified (Table S4). Several common associations were found by relaxing the FDR to 20% (Table S5) and, in line with the previous results, this list included genes that encode histone methyltransferases including EZH2, as well as MEN1, MLL4, and MGA, and other\ntranscriptional repressors (IZKF1, SPEN, and CHD). An exception was E2F3, which is a transcriptional activator.\n\nWhile drug sensitivity can correlate to both high and low expression of the target,\\(^{44}\\) we found no correlation between PLA2G4A expression and sensitivity to the cPLA\\(_2\\)α inhibitors either in the cell panel as a whole or after grouping the cell lines based on their tissue of origin (**Fig. S4**). To date, PLA2G4A transcript levels have only been associated with the response to chemical inhibition in acute myeloid leukemia cells,\\(^{28}\\) whereas Koundouros et al.\\(^{25}\\) showed that it was the stability and activity of cPLA\\(_2\\)α protein that predicted response to inhibition. The expression of four genes encoding alternative phospholipase or phospholipase-related proteins did however show a significant negative correlation with AVX420 sensitivity. These were PLCL1, PLCL2, GPLD1, and LPL. None have type II phospholipase activity but are reported to be involved in regulating the use of fatty acids as an energy supply.\\(^{45-48}\\)\n\n**Protection against oxidative stress defines resistance to cPLA\\(_2\\)α inhibition.**\n\nIndividual genes whose basal expression was associated with insensitivity to cPLA\\(_2\\)α inhibition were identified from a list of 405 genes with prior association to drug resistance. Again, when positive correlations with an FDR of 5% were considered significant, we only found associations with AVX420, and the genes identified were NFE2L2, CCND1, TSPO and SOCS3. Using an FDR of 20%, common associations were found with the expression of NFE2L2, CAV1, SLC38A7, BCAR3, and GNA12. The strongest positive correlations were to NFE2L2, which is the gene encoding Nrf2, a transcription factor that coordinates cellular protection against oxidative stress in both normal and transformed cells.\\(^{49}\\) The low number of associations to known drug resistance mechanisms led us to take a second approach that did not use filtering based on prior knowledge. Instead, the activity data from the 121 pre-profiled chemotherapy drugs was used to filter out non-specific associations, and the identified genes are listed in **Table S6**. Consistent with the first approach there was enrichment of NFE2L2 target genes, but the second approach additionally revealed associations with olefinic, unsaturated fatty acid, and eicosanoid metabolic processes (**Fig. 5a**). Of note, the gene list included three members of the aldo-ketone reductase (AKR) family of enzymes (AKR1C3 AKR1B10, AKR1C2). These targets of the Nrf2 pathway are involved in the detoxification of lipid peroxidation products to protect cells from oxidative stress.\\(^{50}\\) These findings indicated that Nrf2 signaling may protect against the effect of cPLA\\(_2\\)α inhibition and thus implicated oxidative stress in the chemotherapeutic mechanism of action.\na.\n\nDrug resistance\n\nNFE2L2\nOLEFINIC_COMPOUND_METABOLIC_PROCESS\nUNSATURATED_FATTY_ACID_METABOLIC_PROCESS\nMEK_UP_V1_UP\nEICOSANOID_METABOLIC_PROCESS\nAPOPTOTIC_PROCESS\nLIPID_METABOLIC_PROCESS\nPROSTANOID_METABOLIC_PROCESS\nSMALL_MOLECULE_METABOLIC_PROCESS\nHORMONE_METABOLIC_PROCESS\n\nOverlapping gene count\nFDR q-value\n4×10^{-5} 2×10^{-3} 2×10^{-3}\n\nb. (i) CCRF-CEM\n(ii) Jurkat E6.1\nRLU (% of Control)\nAVX420 (μM)\n\nc. (i) MV-4-11\n(ii) HL-60\nFluorescence (% of control)\nlog10 AVX420 (μM)\n\nd. T-cells\nPercentage of cells\nLive cells\nDead cells\nAVX420 (μM)\nStau 0.5 μM\n****\n\ne. (i) CCRF-CEM\n(ii) Jurkat E6.1\nPercentage of Cells\nROS Negative Cells\nROS Positive Cells\nControl\nAVX420 (μM)\nH_{2}O_{2} 1 mM\nRSL-3 1 μM\nDox 1 μM\n\nf. (i) CCRF-CEM\n(ii) Jurkat E6.1\nPercentage of Cells\nControl\nAVX420 0.5 μM\nAVX420 1 μM\nGSH 0.0625 μM\nNAC 0.0625 μM\nML-210 0.0625 μM\nGSH 2.5 mM\nNAC 2.5 mM\n#\nFigure 5. AVX420 causes oxidative stress-dependent cell death in acute leukemia cells. a. The top 10 gene sets from the transcription factor target (C3), gene ontology (C5), and oncogenic signatures (C6) collections in the MSigDB, which overlapped with the genes that were associated with resistance to cPLA2α inhibition b. Cell viability assessed by CTG assays in (i) CCRF-CEM and (ii) Jurkat E6.1 cells c. Cell viability assessed by resazurin assays in (i) MV-4-11 and (ii) HL-60 cells d. Viability of healthy T-cells measured by propidium iodide exclusion. e. Proportion of intracellular ROS positive cells measured by ROS-red staining and flow cytometry. e. Cell viability measured by CTG assay in cells preincubated with glutathione (GSH) or N-acetyl cysteine (NAC) for 30 mins before addition of AVX420 for 24 hours. Data are the mean ± standard error for 3 independent experiments. ****p<0.001 versus vehicle-treated control. # p<0.0001 versus the AVX420 -treated control.\n\nBased on this, we investigated the role of reactive oxygen species (ROS) in the response to AVX420 in cell lines that were highly sensitive to the drug. We reported previously that the cell lines in the CCLS that were derived from hematopoietic cancers were more susceptible to cPLA2α inhibition than those derived from solid tumours.51 Of these, the cell lines from acute leukemias (CCRF-CEM, Jurkat E6.1 and MOLT-4) stood out as being the most sensitive to AVX420 (Fig. S5). We confirmed the strong dose-dependent effect of AVX420 on the viability of Jurkat E6.1 and CCRF-CEM cell lines, which are derived from T-cell acute lymphoblastic leukemias (T-ALL) (Fig. 5b) and further demonstrated that cell lines derived from acute leukemias of a myeloid lineage (MV-4-11 and HL-60) are also susceptible (Fig. 5c). This was in sharp contrast to healthy immune cells (CD3+ T-cells and PBMCs) where AVX420 had no effect up to a maximum dose tested of 32 \\( \\mu \\)M (Fig. 5d and Fig. S6). We measured the levels of intracellular reactive oxygen species (iROS) by flow cytometric analysis of ROS-red staining in Jurkat E6.1 and CCRF-CEM cells. AVX420 treatment induced a dose-dependent increase in iROS in both cell lines (Fig. 5e). The response occurred within 30 min, peaked at 8-12 hours, and preceded the loss of cell viability (Fig. S7). Importantly, pretreatment with ROS scavengers (glutathione and N-acetyl cystine) rendered the cells completely resistant to cell death induced by AVX420 (Fig. 5f).\n\nAVX420 initiates an ATF4-dependent but ISR-independent transcriptional program to initiate cell death.\n\nGiven our findings that the sensitivity to AVX420 was dependent on increased intracellular ROS, we hypothesized that activation of the integrated stress response (ISR) by oxidative damage to DNA and proteins may be the cause of cell death. The ISR converges on deactivation of the eukaryotic translation initiation factor 2 alpha (eIF2α) to globally suppress translation, with the exception of selected genes (e.g., the transcription factor ATF4) which activate robust transcriptional changes to restore homeostasis and promote survival or, when oxidative damage is sustained, to initiate programmed cell death.52 To investigate this, we used a combination of RNA-SEQ and Ribosomal RNA-SEQ (Ribo-SEQ) to measure the global transcriptional and translational response to AVX420 in CCRF-CEM cells. No significant changes in gene expression were seen after 1 hour, 16 genes were upregulated after 6 hours (Table 3) and there were 82 differentially expressed genes (DEGs) after 16 hours (Fig.6A, Table S7). Translational\neffects were determined by calculating the proportion of total transcript associated with the ribosome (ribosomal occupancy (RO)). We did not identify any transcripts with differential RO, indicating that AVX420 did not affect translation. As a positive control we treated cells for 1 hour with the dual mTOR inhibitor Torin-1, which reduced the RO of 20 mRNAs. As expected, GO term enrichment analysis showed these predominantly represented genes coding for ribosomal proteins and translation factors (Table S8 and S9).\n\nTable 3. Differentially expressed genes after 6 hours of AVX420 treatment.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Gene namelog2FCAdjusted p-value
CHAC12.258.12E-38
L3MBTL2-AS12.138.90E-05
SESN21.593.07E-28
SLC7A111.579.03E-06
ADM21.491.65E-10
ENSG000002604981.446.37E-03
LINC-PINT1.342.15E-11
VLDLR1.273.68E-10
SLC6A91.252.93E-06
GPT21.243.60E-05
ULBP11.25.06E-04
DDIT31.151.13E-18
LY91.051.81E-03
ATF31.052.20E-08
YAP11.049.19E-04
VLDLR-AS11.025.37E-05
\n\np-value cut off of 0.01 after multiple testing adjustments and a log2 fold change >1 or <-1\n\nClose inspection of the genes upregulated after 6 hours treatment with AVX420 revealed that many are established targets of ATF4 (E.g., CHAC1, ADM2, SESN2, SLC7A11, DDIT3, ULBP1, ATF3) and GO term and KEGG pathway enrichment analysis performed on the 82 DEGs at 16 hours predicted a response to endoplasmic reticulum (ER) stress (Table S10). While these findings supported the hypothesis that AVX420 initiated cell death via the ATF4 dependent ISR pathway, the absence of translational repression, or selective upregulation of ATF4 translation in response to AVX420, would strongly argue against this, and an alternative mechanism for activation of ATF4 target genes is more likely.\n\nGiven our findings showing a correlation between PRC2 activity and sensitivity to cPLA_{2α} inhibition, we instead propose that cPLA_{2α} could be important for maintaining H3K27 trimethylation- dependent transcriptional suppression of certain ATF4 target genes for example ATF3, which was upregulated by AVX420 and is indeed known to be repressed by PRC2.\\(^{53,54}\\)\nATF3 has additional function of stabilizing ATF4 protein.\\(^{55}\\) Loss of H3K27 trimethylation has also been shown to be important for the transcription of another of the genes upregulated by AVX420, DDIT3 (CHOP)\\(^{56}\\). In line with this hypothesis, we found a significant overlap between the genes upregulated by AVX420 at 16 hours and genes upregulated by the knockdown of BMI1, which is an important component of PRC1 and related to the activity of PRC2 (**Fig. 6b**). ATF3 and DDIT3 (CHOP) are strong candidates for mediating ATF4-dependent induction of cell death. An alternative mechanism for upregulation of DDIT3 (CHOP) could involve L3MBTL2-AS1, an RNA that was upregulated at 6 hours, which has been shown to downregulate the expression of L3MBTL2, a transcriptional repressor of DDIT3 (CHOP).\\(^{57}\\) Consistent with the predicted role of mTOR signaling in the response to cPLA\\(_2\\)α inhibition, AVX420 upregulated genes computationally overlapped with those upregulated by treatment with the mTOR inhibitor rapamycin. We also found significant overlaps with Nrf2-dependent genes (**Fig. 6b**), and predicted targets of the transcription factors MafG, Nrf1 and Hes2 (**Fig. 6c**). Both MafG and Nrf1 are known to cooperate with Nrf2 to regulate the expression of antioxidant response genes,\\(^{58}\\) \\(^{59}\\) while Hes2 is a little studied member of the Hes family of transcription repressors downstream of Notch.\\(^{60}\\) Given the importance of Notch signaling in T-ALL, interactions between cPLA\\(_2\\)α and Hes2 warrant further investigation.\n\nWe conclude that the transcriptional response to cPLA\\(_2\\)α inhibition is compatible with the induction of oxidative stress and loss of mTOR/PRC2-dependent transcriptional repression, which could together activate an ATF4 dependent stress response program leading to cell death (**Fig. 6d**). While the mechanism behind the increase in iROS in response to cPLA\\(_2\\)α inhibition is not directly evident from this data, we showed that the iROS increased rapidly, and in the absence of any transcriptional or translational alterations. This favors metabolic consequences and/or post translational effects and will require a deeper investigation into the role of cPLA\\(_2\\)α in cancer cell fatty acid metabolism to be fully understood.\nFigure 6. AVX420 activates a transcriptional response to oxidative stress. a. DEGs at 16 hours after treatment with 0.5 μM AVX420. b. Top 10 transcription factor target (C3) gene sets in MSigDB that overlapped with genes overexpressed following treatment with 0.5 μM AVX420 c. Top ten oncogenic gene sets in MSigDB that overlapped with genes overexpressed following treatment with 0.5 μM AVX420. d. Model for the role cPLA2α in inhibitor-sensitive cancers. Cancers which rely on mitochondrial fatty acid oxidation (FAO) for energy derived from oxidative phosphorylation (OXPHOS) have a high oxidative burden. We propose cPLA2α-derived arachidonic acid is integral to cancer cell survival in this case, both as a fuel source, and for maintaining epigenetic suppression of programmed cell death mediators via activation of mTOR/EZH2. Inhibition of cPLA2α will thus lead to mitochondrial stress and allow activation of programmed cell death in response to oxidative stress.\n\nDiscussion\n\nAs a therapeutic target, cPLA2α is well studied in the context of inflammation, and small molecule inhibitors have shown promise for treating diverse chronic inflammatory conditions.61 Now cPLA2α is emerging as a cancer target, but mechanistic studies relating the cPLA2α -AA cascade to oncogenesis are limited and methods for predicting the response to cPLA2α inhibition\nare not available. Here we describe a new series of cPLA2α inhibitors, which were designed starting from the previous lead inhibitor GK470 (AVX235), a molecule that has shown efficacy in preclinical murine models of both inflammatory disease and cancer.19,24 GK420 (AVX420), was selected as the lead compound based on high potency and selectivity in vitro and ex vivo. We found that AVX420 targeted cancer cells by a dual mechanism of action that involved the induction of cellular ROS and reactivation of stress response genes, to trigger cell death. This, along with potential therapeutic uses of AVX420, is discussed below.\n\nCellular transformation relies on metabolic reprogramming that results from both genetic and epigenetic changes. Fatty acids are recognized as a highly relevant source of energy for cancer cells, particularly under nutrient deprivation, and mitochondrial fatty acid oxidation (FAO) is increased in stem cells and cancer-initiating cells.62,63 As an energy source, FAO produces high levels of mitochondrial ROS, which can trigger programmed cell death. Adaptive mechanisms for survival are therefore employed to either increase the antioxidant capacity of the cell or prevent oxidative stress-dependent cell death. We found that AVX420 was a potent inducer of ROS-dependent cell death and hypothesize that it targets a hitherto unexplored function of cPLA2α in the epigenetic adaptation to ROS. Epigenetic changes that act on transcription are a universal feature of cancers and altered histone methylation can lead to aberrant gene silencing or activation by affecting chromatin accessibility.64 We found strong correlations between activity of the histone methyltransferase PRC2 and sensitivity to cPLA2α inhibition, and cPLA2α inhibitors showed similar anti-cancer activity to inhibitors of the catalytic component of PRC2, EZH2, suggesting overlapping mechanisms of action. Overexpression of EZH2 is a common feature of many solid tumors, where it appears to be important for maintaining cancer stem cell populations and regulating lipid metabolism.65 It suppresses target gene transcription by trimethylation of H3K2766 and antagonism is provided by the trithorax group proteins MLL and MLL2, which trimethylate H3K4 to facilitate target gene transcription.38 Mutations to MLL and MLL2 were also associated with sensitivity to AVX420. We thus propose that cPLA2α activity regulates transcriptional repression by EZH2 to protect cancer cells that are reliant on fatty acids as an energy source. A direct regulation of epigenetic modifiers by cPLA2α signaling has to our knowledge not been described to date. However, there is evidence that EZH2 is controlled by mTOR in breast cancer and glioblastomas67 and can reciprocally promote mTOR activity.68 mTOR is the central kinase component of two important signaling hubs (mTORC1 and mTORC2) that maintain metabolic homeostasis and regulation of cPLA2α by mTOR and vice versa have been described before.25,43 We found that mTOR activation was also associated with sensitivity to cPLA2α inhibition and AVX420 induced rapamycin-like transcriptional responses. mTOR thus presents as the logical connection between cPLA2α and epigenetic suppression by PRC2.\n\nInducing ROS-dependent cell death has become a key approach in cancer biology.69 An example is the unprecedented success of the combined use of hypomethylating agents e.g., 5-azacytidine\nand decitabine in combination with the Bcl-2 inhibitor venetoclax for treating acute myeloid leukemia (AML). These agents were shown to induce mitochondrial ROS-dependent cell death and were reported to synergize based on the ability of venetoclax to suppress the Nrf2-dependent antioxidant response.\\(^{70}\\) Based on this, venetoclax may also suppress the observed Nrf2 dependent antioxidant response to AVX420, providing synergistic effects, or conversely, by lowering the threshold for cell death, AVX420 could synergize with other ROS inducing agents. Finally, altered fatty acid metabolism appears as an increasingly important mechanism of chemotherapy resistance,\\(^{71}\\) including following treatment with venetoclax and hypomethylating agents.\\(^{72}\\) AVX420 may be beneficial in instances such as this where resistance involves increased use of fatty acids as an energy source, especially if epigenetic suppression of cell death is also indicated.\n\nWhile our study demonstrates the potential of cPLA\\(_{2\\alpha}\\) inhibitors for use in chemotherapy, including the possibility of targeting the vulnerabilities of cancer stem cells and drug resistance in acute leukemias, it also highlights the strong need to address our limited understanding of the involvement of cPLA\\(_{2\\alpha}\\) in cellular fatty acid metabolism in cancer. This knowledge will be key to fully harnessing the chemotherapeutic potential of cPLA\\(_{2\\alpha}\\) inhibitors, and new potent and selective cPLA\\(_{2\\alpha}\\) inhibitors such as AVX420 will also serve us well in this important quest.\nMethods\n\nGeneral Procedures for Synthesis of Inhibitors\n\nGeneral method for the synthesis of compounds 11a-j. To a stirred solution of phenols 10a-e or 10k (1.00 mmol) in acetone (10 mL), K2CO3 (3.00 mmol, 415 mg) and ethyl bromoacetate or ethyl 2-bromopropionate or hexyl bromide (1.10 mmol) were added, and the reaction mixture was refluxed for 5 h. Then, the mixture was filtrated over Celite, and the organic solvent was evaporated under reduced pressure. The residue was purified by column chromatography [EtOAc-petroleum ether (bp 40-60 °C), 1:9].\n\nGeneral method for the synthesis of alcohols 12a-j. To a stirred solution of esters 11a-j, (1.00 mmol) in dry Et2O (10 mL), DIBALH (2.5 mL, 2.50 mmol, 1.0 M in hexane) was added at 0 °C under Ar atmosphere, and the reaction mixture was stirred for 2 h at room temperature. Water was then added (5 mL), the reaction mixture was stirred for 30 more minutes and filtrated over Celite. The organic solvent was evaporated under reduced pressure and the residue was purified by column chromatography [EtOAc-petroleum ether (bp 40-60 °C), 3:7].\n\nGeneral method for the synthesis of nitriles 13a-j. To a solution of alcohols 12a-j, (1.00 mmol) in a mixture of toluene (3 mL) and EtOAc (3 mL), a solution of NaBr (1.10 mmol, 110 g) in water (0.5 mL) was added followed by 2,2,6,6-tetramethylpiperidine-1-yloxy free radical (TEMPO) (0.01 mmol, 2.2 mg). To the resulting biphasic system, which was cooled at 0 °C, an aqueous solution of 0.35 M NaOCl (1.10 mmol, 3.1 mL) containing NaHCO3 (3.00 mmol, 250 mg) was added dropwise under vigorous stirring, at 0 °C over a period of 1 h. After the reaction mixture had been stirred for a further 15 min at 0 °C, EtOAc (10 mL) and H2O (10 mL) were added. The aqueous layer was separated and washed with EtOAc (2 × 10 mL). The combined organic layers were washed consecutively with 5% aqueous citric acid (10 mL) containing KI (40 mg), 10% aqueous Na2S2O3 (10 mL), and brine and dried over Na2SO4. The solvents were evaporated under reduced pressure and the residue was used without any further purification.\n\nTo a mixture of TBDMSCN (1.00 mmol, 141 mg), potassium cyanide (0.20 mmol, 13 mg) and 18-crown-6 (0.40 mmol, 106 mg), a solution of the aldehyde (1.00 mmol) in CH2Cl2 derived from alcohol, according to the NaBr/TEMPO protocol mentioned above, was added dropwise at room temperature under nitrogen over 30 min. After addition was complete, the reaction mixture was stirred overnight at room temperature. The organic solvent was evaporated under reduced pressure and the residue was purified by column chromatography [EtOAc-petroleum ether (bp 40-60 °C), 0.5:9.5].\n\nGeneral method for the synthesis of thiazolines 14a-j. To a stirred solution of the nitriles 13a-j (1.00 mmol) and CH3COONH4+ (3.60 mmol, 277 mg) in MeOH (4 mL), HCl.H-L-Cys-OMe (3.00 mmol, 515 mg) was added, and the reaction mixture was stirred overnight at room temperature. The organic solvent was evaporated under reduced pressure and the residue was purified by column chromatography [EtOAc-petroleum ether (bp 40-60 °C), 1:9].\n\nGeneral method for the synthesis of thiazoles 15a-j. To a solution of thiazolines 14a-j (1.00 mmol) in CH2Cl2 (20 mL), BrCCl3 (6.00 mmol, 0.59 mL) and DBU (6.00 mmol, 0.90 mL) were\nadded at 0 °C. The reaction was stirred for 2 h at 0 °C and overnight at room temperature. The organic solvent was evaporated under reduced pressure and the residue was purified by column chromatography [EtOAc-petroleum ether (bp 40-60 °C), 1:9].\n\n**General method for the synthesis of 16a-j.** Compounds **15a-j** (1.00 mmol) were treated with a solution of 2N HCl in MeOH (10 mL). After TLC indicated complete disappearance of the starting material, the organic solvent was evaporated under reduced pressure and the residue was recrystallized from ether/petroleum ether (bp 40-60 °C).\n\n**General method for the synthesis of thiazolyl ketones 17a-j.** To a solution of compounds **16a-j** (1.00 mmol) in dry CH$_2$Cl$_2$ (10 mL), Dess-Martin periodinane was added (1.50 mmol, 637 mg) and the reaction mixture was stirred for 1 h at room temperature. The organic solvent was evaporated under reduce pressure and Et$_2$O (30 mL) was added. The organic phase was washed with saturated aqueous NaHCO$_3$ (20 mL) containing Na$_2$S$_2$O$_3$ (9.50 mmol, 1.50 g), H$_2$O (20 mL), dried over Na$_2$SO$_4$, and the organic solvent was evaporated under reduced pressure. The residue was purified by column chromatography using petroleum ether (bp 40-60 °C)/EtOAc 7:3 as eluent.\n\n**General method for the synthesis of nitriles 18a-d.** To a solution of alcohols **12b, g-i** (1.00 mmol) in dry CH$_2$Cl$_2$ (10 mL), Dess-Martin periodinane was added (1.50 mmol, 637 mg) and the reaction mixture was stirred for 2 h at room temperature. The organic solvent was evaporated under reduce pressure and Et$_2$O (30 mL) was added. The organic phase was washed with saturated aqueous NaHCO$_3$ (20 mL) containing Na$_2$S$_2$O$_3$ (9.50 mmol, 1.50 g), H$_2$O (20 mL), dried over Na$_2$SO$_4$, and the organic solvent was evaporated under reduced pressure. The residue was purified by column chromatography [petroleum ether (bp 40-60 °C)/EtOAc 8:2], affording the corresponding aldehyde.\n\nTo a stirred solution of aldehyde (1.00 mmol) in CH$_2$Cl$_2$ (3.5 mL), an aqueous solution of NaHSO$_3$ 4N (3.00 mmol, 312 mg) in water (0.75 mL) was added at room temperature. After stirring for 30 min, the organic solvent was concentrated under reduced pressure, water (4.6 mL) was added, and the reaction mixture was cooled to 0 °C. Then, an aqueous solution of KCN 4N (3.00 mmol, 195 mg) in water (0.75 mL) was added dropwise, and the reaction mixture was left stirring for 16 h. After the completion of the reaction, CH$_2$Cl$_2$ (5 mL) was added and the organic layer was washed with brine (10 mL), dried over Na$_2$SO$_4$ and concentrated under reduced pressure. Purification by column chromatography [petroleum ether (bp 40-60 °C)/EtOAc 6:4], affording the desired product.\n\nMaterials, along with details of the synthesis, HPLC chromatograms of inhibitors 17a-d and 17g-i, and $^1$H and $^{13}$C NMR traces are available in the supplementary information.\n\n**In Vitro PLA$_2$ Activity Assay.**\nA previously described radioactivity-based group-specific mixed micelle assay was carried out for the determination of activities of human recombinant cPLA$_2\\alpha$, GVIA iPLA$_2$ and GV sPLA$_2$. 16,19 In brief, to achieve optimum activity for each enzyme, the substrate was prepared using slightly different conditions: (i) cPLA$_2\\alpha$ mixed micelle substrate consisted of 400 μM Triton X-100, 95.3 μM 1-palmitoyl-2-arachidonylphosphatidylcholine (PAPC), 1.7 μM arachidonyl-1-$^{14}$C\nPAPC, and 3 μM PIP_2 in a buffer containing 100 mM 4-(2-hydroxyethyl)-1-piperazineethanesulfonic acid (HEPES) of pH 7.5, 90 μM CaCl_2, 2 mM dithiothreitol (DTT), and 0.1 mg/mL bovine serum albumin (BSA); (ii) GVIA iPLA_2 mixed micelle substrate consisted 400 μM Triton X-100, 98.3 μM PAPC, and 1.7 μM arachidonyl-1-^{14}C PAPC in a buffer containing 100 mM HEPES of pH 7.5, 2 mM ATP, and 4 mM DTT; and (iii) GV sPLA_2 mixed micelles substrate consisted 400 μM Triton X-100, 98.3 μM PAPC, and 1.7 μM arachidonyl-1-^{14}C PAPC in a buffer containing 50 mM Tris-HCl of pH 8.0, and 5 mM CaCl_2. Inhibitors were initially screened at 0.091 mol fraction (5 μL of 5 mM inhibitor in DMSO) in substrate (495 μL). X_{i}(50) values were determined for compounds exhibiting greater than 90% inhibition.\n\nPlasma stability assays\nThe metabolic stability of the compounds was determined through in vitro stability assays in human plasma. Compounds (20 mM) were prepared in DMSO and diluted to 5 μg/ml in 50% methanol for infusion into the MS/MS system and spiking of calibration standards and control samples. For the MS detection, positive ionization in ESI mode was used. Good sensitivity, retention and peak shaped was achieved using a gradient with 5 mM ammonium carbamate in water and ammonium carbamate in 90% acetonitrile on a reversed phase column (ACE3AQ). Calibration standards were spiked in a calibration range of 0.5-100 ng/ml. Control samples were spiked at LLOQ, low, medium, and high concentration levels. The spiked plasma samples were prepared by protein precipitation using acetonitrile containing appropriate internal standard (IS). A LLOQ of 0.5 ng/ml was reached for all compounds in human plasma and linearity was good. Samples were prepared for analysis by taking 50 μL of plasma sample and adding 100 μL of IS working solution in acetonitrile followed by vortexing at 2500 rpm for 2 min. Samples were centrifuged at 5300 rpm for 3 min and the supernatant transferred to the autosampler. Recovery was determined by comparing the prepared matrix samples (protein precipitation) with a direct sample (analytes spikes in 67% acetonitrile = injection solution) such that the recovery of the sample preparation and the matrix effects were determined together.\n\nCellular arachidonic acid (AA) release assay\nThe human synovial sarcoma cell line SW982 (ATCC, London, UK) was used to measure AA release. The cells were maintained as previously described.^{73} Experiments were performed at 3 days post-confluency following overnight serum deprivation in serum-free DMEM to ensure differentiation and synchronization of the cells.\nAA release was analyzed as previously described.^{74} Briefly, postconfluent, serum-starved cells were labeled overnight with ^{3}H-AA (0.4 μCi/mL) in serum-free DMEM. The cells were washed twice with PBS containing fBSA (2 mg/mL) to remove unincorporated radioactivity. Inhibitors, or DMSO vehicle control were added for 1 hour prior to IL-1β stimulation (10 ng/mL, 4 h). Supernatants were collected and centrifuged at 13 000 rpm for 5 min. The release of ^{3}H-AA from the cells was assessed by liquid scintillation counting (LS 6500 Multi-Purpose Scintillation Counter, Beckman Coulter, Inc., USA). The cells were dissolved in 1 N NaOH to determine\nincorporated \\( ^3\\mathrm{H}\\)-AA. The results are given as inhibition of released \\( ^3\\mathrm{H}\\)-AA and \\( ^{14}\\mathrm{C}\\)-OA in the supernatants relative to total \\( ^3\\mathrm{H}\\)-AA incorporated into the cells.\n\nAnalysis of eicosanoid release in whole blood\nBlood was collected from voluntary, anonymous male donors. Aliquots of 0.4 mL of heparinized whole blood were mixed with 1.6 mL of serum-free RPMI cultivation medium with- or without Indomethacin (# I7378, Sigma-Aldrich), GK420 or ATK (Cayman #62120), prior to the addition of lipopolysaccharides (LPS) (1 \\( \\mu \\)g/mL) to activate the cPLA\\(_{2\\alpha}\\) enzyme (LPS was from E. coli 026:B6 \\( \\gamma \\)-irradiated, #L2654, Sigma-Aldrich). Exogenous arachidonic acid (5-10 \\( \\mu \\)M) (#3555, Sigma-Aldrich) was added after 23.5 hours, for the final 30 mins of the 24-hour stimulation. Following treatment (24 hours, 37 \\( ^\\circ \\)C, 5% CO\\(_2\\)), the diluted blood was centrifuged (2000 rpm for 10 min at 4 \\( ^\\circ \\)C) to isolate the plasma from the cell fraction. Plasma samples were stored at -80 \\( ^\\circ \\)C until analysis. Samples were analyzed at the Lipid Maps Consortium, UCSD according to the standard methods. 200 \\( \\mu \\)l of sample was subjected to solid phase extraction of the eicosanoids using the StrataX solid phase extraction columns from Phenomenex and analyzed by UHPLC-MS/MS using full standards mix.\n\nAnalysis of eicosanoid release from peripheral blood mononuclear cells\nPBMCs were isolated from buffy coats using Lymphoprep as described by the manufacturer (STEMCELL Technologies, Vancouver, Canada). Red blood cells were lysed and removed using RBC lysis buffer (Roche, Basel, Switzerland) and the remaining cells were resuspended in 10 ml of RPMI-1640 supplemented with 5% FBS. The TC20 automated cell counter (BIO-RAD, Hercules, California, USA) was used to count the number of cells and check the viability by staining with trypan blue (0.4%) (NanoEnTek, Waltham, MA, USA). For experiments, 5 x 10\\(^5\\) cells were seeded in 0.5 mL in 24 well plates with RPMI medium supplemented with 5% FBS, 0.3 mg/mL glutamine, and 0.1 mg/mL gentamicin. Cells were preincubated with inhibitors for 2 h before incubating with 30 \\( \\mu \\)M Ca\\(^{2+}\\) ionophore A23187 for 15 minutes to activate cPLA\\(_{2\\alpha}\\). After incubation, the supernatant was obtained by centrifugation at 2000 rpm for 10 min at 4 degree and stored at -80 until assayed for PGE2, LTB4, TxB2, 6-Keto PGF1\\( \\alpha \\) and 12S-HETE using enzyme-linked immunosorbent assays (ELISAs) (Cayman #514435, Cayman #10009292, Cayman #501020, Cayman #15210, and Enzo Lifesciences #ADI-900-050). The enzymatic conversion of the substrate was read at OD420 nm after supernatants were hybridized overnight. A 4-parameter logistic fit model was used to process the data.\n\nCancer Cell line Screening\nScreening of compound activities in 66 cancer cell lines was carried out at the Netherlands Translation Research Center. Briefly, proliferation assays were performed 72 hours after compound addition using ATPlite 1step reagent (Perkin Elmer). IC\\(_{50}\\)s calculated by non-linear regression analysis were used as a measure of compound activity for investigating associations with genetic factors. A complete description of the laboratory and data analysis methods are\navailable in the supplementary information (Supplemental Methods: Cancer Cell Line Screening).\n\nCell culture experiments\n\nReagents and chemicals\nCell culture media RPMI 1640 (#R0883), Gentamycin (#G1397), Dimethyl sulfoxide (DMSO) (#2650), A23187, naproxen, celecoxib, and lipopolysaccharide (LPS) were purchased from Sigma-Aldrich (St. Louis, MO, USA). Fetal Bovine Serum (FBS) (#10270106) was purchased from Thermo Fisher Scientific (Waltham, Massachusetts, USA). L-glutamine (#17-605E) was purchased from Lonza Pharma & Biotech (Hochbergerstrasse, Basel, Switzerland). Nordihydroguaiaretic acid (NDGA) and Arachidonyl Trifluoromethyl Ketone (#62120-10) were obtained from Cayman chemicals (Ann Arbor, MI, USA). AVX002 \\(^{35}\\) and AVX235 \\(^{19}\\) were synthesized by Synthetica AS, Oslo. AVX002, AVX235 and AVX420 were stored at -80 °C in DMSO.\n\nCell culture and plating\nCCRF-CEM and Jurkat E6.1 cell lines were purchased from American Type Culture Collection (ATCC) (Manassas, VA, USA) while HL-60 and MV-4-11 cells were a kind gift from Prof. Bjørn Tore Gjertsen (University of Bergen, Norway). MV-4-11 were cultured in Iscove's Modified Dulbecco's Medium (Sigma, I3390). CCRF-CEM, Jurkat E6.1 and HL-60 cells were cultured in RPMI 1640 Medium RPMI-1640 medium (Sigma, R5886). Medias were supplemented with 10% FBS (heat-inactivated), 2 mM L-glutamine, 0.1 mg/ml gentamycin, and 10 % FBS (complete media) and kept in a humidified incubator at 37°C with 5% CO2. Cell lines were tested to ensure the absence of mycoplasma. Cell viability was measured by trypan blue staining, and for experiments, the cells were seeded at a density of 200,000 live cells/ml in 24-well flat-bottom plates. Experiment using CCRF-CEM and Jurkat E6.1 cells were carried out in complete media while experiments using MV-4-11 and HL-60 cells were carried out in media supplemented with 4% heat-inactivated FBS.\n\nCell Viability Assays\nThe cell titer glo (CTG) and resazurin cell viability assay were performed as described previously.\\(^{51}\\) Data was acquired using the Cytation 5 cell imaging multimode reader (Biotek Instruments, Winooski, VT, USA). Propidium iodide exclusion was used to assess cell death. Following incubation with AVX420, the cells were washed once with PBS and stained with 1.4 µg/ml propidium iodide (PI) for 5 minutes before quantification of PI negative and positive cells using a CytoFLEX flow cytometer (California, United States).\nROS detection\nThe cells were stained with cellular ROS Assay Kit (Cat. No. ab186029; Abcam, Cambridge, United Kingdom) following the manufacturer's instruction and ROS positive cells were quantified by flow cytometry using either the NovoCyte flow cytometer from ACEA Biosciences, Agilent Technologies (Santa Clara, USA), or the CytoFLEX flow cytometer from Beckman Coulter (California, United States). The data were analyzed using Novoexpress Software v1.5.0 from Agilent Technologies (Santa Clara, USA).\n\nRNA sequencing and ribosome-associated RNA-sequencing\nCCRF-CEM cells seeded at 200K viable cells/ml were treated with AVX420 (0.5 μM) or DMSO (0.1 %) and harvested after 1 hour, 6 hours, or 16 hours. Torin-1 (100 nM) treatment was harvested after 1 hour. The flasks were placed on ice and the cell suspensions were transferred to 50 ml conical tubes for centrifugation (1500 rpm, 4°C, 5 min). Cell pellets were washed once in 10 ml of chilled Dulbecco’s (D) PBS and resuspended in 5 ml of chilled DPBS for UV crosslinking using 254-nm UV light with an energy setting of 400 mJoules/cm^2 (UVP CL-1000 Ultraviolet Crosslinker). The cells were collected and centrifuged at 550 g for 5 minutes at 4°C. The supernatant was discarded, and the cells were suspended in 1 ml of DPBS before centrifugation at 1000 g for 5 min at 4°C. Resulting cell pellets were snap frozen in liquid nitrogen and stored at -80 °C.\nRNA-Seq and ribosome-associated RNA(Ribo)-Seq was performed by Eclipsebio (eclipsebio.com). In short, the cytosolic fraction of crosslinked cell pellets was isolated and RNA quality and quantity was assessed before 250 ng of the isolated RNA was used to build 3’ RNA-Seq libraries. 10 μg RNA was used for immunoprecipitation (IP) for Ribo-SEQ analysis. Non-crosslinked RNA was removed from the IP through multiple wash steps and the remaining RNA was released via proteinase digestion. RNA from both sources was fragmented and libraries were generated from the poly(A) tails. Libraries were sequenced on a NextSeq 2000. After sequencing, samples were processed with Eclipsebio’s proprietary analysis pipeline (v1). Unique molecular identifiers (UMIs) were pruned from read sequences using umitools (v1.1.1). Next 3' adapters were trimmed from reads using cutadapt (v3.2). Reads were then mapped to a custom, curated database of repetitive elements and rRNA sequences. All non-repeat mapped reads were mapped to the genome hg38 using STAR (v2.7.7a) and PCR duplicates were removed using umi_tools (v1.1.1). Gene coverage was calculated using Eclipsebio’s proprietary feature counting algorithm and ribosome occupancy was calculated by dividing coverage in the ribosome-associated (IP) library by the RNA-Seq library. Differentially expressed and occupied genes were identified using DESeq2. Significant differential expression was defined using a cutoff on p.value < 0.01 (after multiple testing adjustment, \"padj\" metric) and requiring the fold change in gene coverage to be greater than 1 or less than -1 (log_2 scale). Significance of the ribosomal occupancy (RO) difference was determined by extending DESeq2 models to include RO fold change as an interaction between the experimental condition and the library type. Genes\nwith a RO log2 (fold change) > 1 or <-1 and an adjusted p-value < 0.01 were considered significant. Only genes annotated as protein-coding or lncRNA are included. Volcano plots were produced using plotly.js (v2.12.2). GO and KEGG analyses were performed with clusterProfiler's enrichGO and enrichKEGG functions available through the Bioconductor package clusterProfiler. For each term, the adjusted p-value for the enrichment analysis and the average fold change of all genes included are calculated and shown in the relevant tables.\n\nAcknowledgments\n\nThis study was funded by a research sponsorship agreement between Coegin Pharma (former Avexxin) and Norwegian University of Science and Technology, supported by grant NFR235344 from the Norwegian Research Council (NFR). We would like to thank Randi Røsbak and Sandra Kristiansen for technical support and Dr Magne Børseth and Dr Samah Elsaadi for helpful discussions and advice. We would also like to thank Eclipsebio (https://eclipsebio.com/) for their support in the processing and analysis of eRibo Count experiments. 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Functional Coupling between Secretory and Cytosolic Phospholipase A2 Modulates Tumor Necrosis Factor-\\( \\alpha \\)- and Interleukin-1\\( \\beta \\)-induced NF-\\( \\kappa \\)B Activation*. Journal of Biological Chemistry **276**, 30527-30536 (2001). https://doi.org:https://doi.org/10.1074/jbc.M008481200\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• JohansenAVX420Supplemental.docx"} {"paper_id": "prb8", "title": "Observation of an exotic narrow doubly charmed tetraquark", "text": "Observation of an exotic narrow doubly charmed tetraquark\n\nLHCb collaboration†\n\nAbstract\n\nConventional hadronic matter consists of baryons and mesons made of three quarks and quark-antiquark pairs, respectively. The observation of a new type of hadronic state, a doubly charmed tetraquark containing two charm quarks, an anti-u and an anti-d quark, is reported using data collected by the LHCb experiment at the Large Hadron Collider. This exotic state with a mass of about \\(3875\\ \\mathrm{MeV}/c^2\\) manifests itself as a narrow peak in the mass spectrum of \\(D^0 D^0 \\pi^+\\) mesons just below the \\(D^{**} D^0\\) mass threshold. The near-threshold mass together with a strikingly narrow width reveals the resonance nature of the state.\n\n†Authors are listed at the end of this Letter.\nQuantum chromodynamics (QCD), the theory of the strong force, describes interactions of coloured quarks and gluons and the formation of hadronic matter, the so-called mesons and baryons. While QCD makes precise predictions at high energies, the theory has difficulties describing the interactions of quarks in hadrons from first principles due to the highly non-perturbative regime at the corresponding energy scale. Hence, the field of hadron spectroscopy is driven by experimental discoveries that sometimes are unexpected, which could lead to changes in the research landscape. Along with conventional mesons and baryons, made of a quark-antiquark pair (\\( q_1 \\overline{q}_2 \\)) and three quarks (\\( q_1 q_2 q_3 \\)), respectively, particles with an alternative quark content, known as exotic states, have been actively discussed since the birth of the constituent quark model [1,6]. The discussion has been revived by recent observations of numerous tetraquark \\( q_1 q_2 \\overline{q}_3 \\overline{q}_4 \\) and pentaquark \\( q_1 q_2 q_3 q_4 \\overline{q}_5 \\) candidates [7,33]. Due to the closeness of their masses to known particle-pair thresholds [34,35], many of these states are likely to be hadronic molecules [36,39] where colour-singlet hadrons are bound by residual nuclear forces similar to the electromagnetic van der Waals forces attracting electrically neutral atoms and molecules. An ordinary example of a hadronic molecule is the deuteron formed by a proton and a neutron. On the other hand, an interpretation of exotic states as compact multiquark structures is also possible [40].\n\nAll exotic hadrons observed so far decay via the strong interaction and their decay widths vary from a few to a few hundred MeV. A discovery of a long-lived exotic state, stable with respect to the strong interaction, would be intriguing. A hadron with two heavy quarks Q and two light antiquarks \\( \\overline{q} \\), *i.e.* \\( Q_1 Q_2 \\overline{q}_1 \\overline{q}_2 \\), is a prime candidate to form such a state [41–46]. In the limit of a large heavy-quark mass the two heavy quarks \\( Q_1 Q_2 \\) form a point-like heavy colour-antitriplet object, that behaves similarly to an antiquark, and the corresponding state should be bound. It is expected that the b quark is heavy enough to sustain the existence of a stable bb\\(\\overline{u}\\)\\(\\overline{d}\\) state with its binding energy of about 200 MeV with respect to the sum of masses of the pseudoscalar and vector beauty mesons that defines the minimal mass for the strong decay to be allowed. In the case of the bc\\(\\overline{u}\\)\\(\\overline{d}\\) and cc\\(\\overline{u}\\)\\(\\overline{d}\\) systems, there is currently no consensus as to whether such states exist and are narrow enough to be detected experimentally. The similarity of the cc\\(\\overline{u}\\)\\(\\overline{d}\\) tetraquark state and the \\( \\Xi_{cc}^{++} \\) baryon containing two c quarks and a u quark, leads to a relationship between the properties of the two states. In particular, the measured mass of the \\( \\Xi_{cc}^{++} \\) baryon with quark content ccu [47,49] implies that the mass of the cc\\(\\overline{u}\\)\\(\\overline{d}\\) tetraquark is close to the sum of masses of D\\( ^0 \\) and D\\( ^{**} \\) mesons with quark content of c\\(\\overline{u}\\) and c\\(\\overline{d}\\), respectively, as suggested in Ref. [50]. Theoretical predictions for the mass of the cc\\(\\overline{u}\\)\\(\\overline{d}\\) ground state with spin-parity quantum numbers J\\( ^P \\)=1\\( ^+ \\) and isospin I=0, denoted hereafter as T\\( _{cc}^+ \\), relative to the D\\( ^{**} \\)D\\( ^0 \\) mass threshold\n\n\\[\n\\delta m \\equiv m_{T_{cc}^+} - (m_{D^{**}} + m_{D^0}) ,\n\\]\n\nlie in the range \\(-300 < \\delta m < 300\\) MeV/\\(c^2\\) [50,81], where \\( m_{D^{**}} \\) and \\( m_{D^0} \\) denote the known masses of the D\\( ^{**} \\) and D\\( ^0 \\) mesons [35]. Lattice QCD calculations also do not provide a definite conclusion on the existence of the T\\( _{cc}^+ \\) state and the binding energy [70,82,84]. The observation of the \\( \\Xi_{cc}^{++} \\) baryon [47,48] and of a new exotic resonance decaying to a pair of J/\\( \\psi \\) mesons [26] by the LHCb experiment, motivates the search of the T\\( _{cc}^+ \\) state.\n\nIn this Letter, the observation of a narrow state in the D\\( ^0 \\)D\\( ^0 \\)\\( \\pi^+ \\) mass spectrum\\( ^1 \\) near the D\\( ^{**} \\)D\\( ^0 \\) mass threshold compatible with being a T\\( _{cc}^+ \\) tetraquark state is reported.\n\n\\( ^1 \\)Throughout this Letter, charge conjugate decays are implied.\nThe study is based on proton-proton (pp) collision data collected with the LHCb detector at the Large Hadron Collider (LHC) at CERN at centre-of-mass energies of 7, 8 and 13 TeV, corresponding to integrated luminosity of 9 fb\\(^{-1}\\). The LHCb detector [85,86] is a single-arm forward spectrometer covering the pseudorapidity range \\(2 < \\eta < 5\\), designed for the study of particles containing b or c quarks and is further described in Methods.\n\nThe D\\(^0\\)D\\(^0\\pi^+\\) final state is reconstructed by selecting events with two D\\(^0\\) mesons and a positively charged pion all produced at the same pp interaction point. Both D\\(^0\\) mesons are reconstructed in the D\\(^0 \\to K^- \\pi^+\\) decay channel. The selection criteria are similar to those used in Ref. [87]. To subtract background not originating from two D\\(^0\\) candidates an extended unbinned maximum-likelihood fit to the two-dimensional distribution of the masses of the two D\\(^0\\) candidates is performed. The corresponding procedure, together with the selection criteria, is described in detail in Methods. To improve the \\(m\\) mass resolution and to make the determination insensitive to the precision of the D\\(^0\\) meson mass, the mass of the D\\(^0\\)D\\(^0\\pi^+\\) combinations is calculated with the mass of each D\\(^0\\) meson constrained to the known value [35]. The resulting D\\(^0\\)D\\(^0\\pi^+\\) mass distribution for selected D\\(^0\\)D\\(^0\\pi^+\\) combinations is shown in Fig. 1. A narrow peak near the D\\(^{*+}\\)D\\(^0\\) mass threshold is clearly visible.\n\nAn extended unbinned maximum-likelihood fit to the D\\(^0\\)D\\(^0\\pi^+\\) mass distribution is performed using a model consisting of signal and background components. The signal component is described by the convolution of the detector resolution with a resonant shape, which is modelled by a relativistic P-wave two-body Breit–Wigner function modified by a Blatt–Weisskopf form factor [88,89] with a meson-radius parameter of 3.5 GeV\\(^{-1}\\). The use of a P–wave resonance is motivated by the expected J\\(^P = 1^+\\) quantum numbers for the T\\(_{cc}^+\\) state. A two-body decay structure T\\(_{cc}^+ \\to\\) AB is assumed with \\(m_A = 2m_{D^0}\\) and \\(m_B = m_{\\pi^+}\\), where \\(m_{\\pi^+}\\) stands for the known mass of the \\(\\pi^+\\) meson. Several alternative prescriptions are used for evaluation of systematic uncertainties. Despite its simplicity, the model serves well to quantify the existence of the T\\(_{cc}^+\\) state and to measure its properties, such as the position and the width of the resonance. A follow-up study [90] investigates the underlying nature of the T\\(_{cc}^+\\) state, expanding on the modelling of the signal shape and determining its physical properties. The detector resolution is modelled by the sum of two Gaussian functions with a common mean, where the additional parameters are taken from simulation (see Methods) with corrections applied [29,91,92]. The root mean square of the resolution function is around 400 keV/\\(c^2\\). A study of the D\\(^0\\pi^+\\) mass distribution for D\\(^0\\)D\\(^0\\pi^+\\) combinations in the region above the D\\(^{*+}\\)D\\(^0\\) mass threshold and below 3.9 GeV/\\(c^2\\) shows that approximately 90% of all random D\\(^0\\)D\\(^0\\pi^+\\) combinations contain a genuine D\\(^{*+}\\) meson. Based on this observation, the background component is parametrised by the product of a two-body phase space function [93] and a positive second-order polynomial. The resulting function is convolved with the detector resolution.\n\nThe fit results are shown in Fig. 1, and the parameters of interest, namely the signal yield, \\(N\\), the mass parameter of the Breit–Wigner function relative to the D\\(^{*+}\\)D\\(^0\\) mass threshold, \\(\\delta m_{BW} \\equiv m_{BW} - (m_{D^{*+}} + m_{D^0})\\), and the width parameter, \\(\\Gamma_{BW}\\), are listed in Table 1. The statistical significance of the observed T\\(_{cc}^+ \\to\\) D\\(^0\\)D\\(^0\\pi^+\\) signal is estimated using Wilks’ theorem [94] to be 22 standard deviations. The fit suggests that the mass parameter of the Breit–Wigner shape is slightly below the D\\(^{*+}\\)D\\(^0\\) mass threshold. The statistical significance of the hypothesis \\(\\delta m_{BW} < 0\\) is estimated to be 4.3 standard deviations.\n\nTo validate the presence of the signal component, several additional cross-checks are performed. The data are categorised according to data-taking periods (including the polar-\nFigure 1: **The \\( \\mathrm{D}^0\\mathrm{D}^0\\pi^+ \\) mass distribution.** The \\( \\mathrm{D}^0\\mathrm{D}^0\\pi^+ \\) mass distribution where the contribution of the non-\\( \\mathrm{D}^0 \\) background has been statistically subtracted. The result of the fit described in the text is overlaid.\n\nTable 1: Signal yield, \\( N \\), Breit–Wigner mass relative to \\( \\mathrm{D}^{*+}\\mathrm{D}^0 \\) mass threshold, \\( \\delta m_{\\mathrm{BW}} \\), and width, \\( \\Gamma_{\\mathrm{BW}} \\), obtained from the fit to the \\( \\mathrm{D}^0\\mathrm{D}^0\\pi^+ \\) mass spectrum. The uncertainties are statistical only.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
ParameterValue
\\( N \\)117 ± 16
\\( \\delta m_{\\mathrm{BW}} \\)−273 ± 61 keV/\\( c^2 \\)
\\( \\Gamma_{\\mathrm{BW}} \\)410 ± 165 keV
\n\nity of the LHCb dipole magnet) and the charge of the \\( \\mathrm{T}_{cc}^+ \\) candidates. In addition, instead of the statistical subtraction of non-\\( \\mathrm{D}^0 \\) background, the mass of each \\( \\mathrm{D}^0 \\to \\mathrm{K}^- \\pi^+ \\) candidate is required to be within a narrow region around the known mass of the \\( \\mathrm{D}^0 \\) meson [35]. The results are found to be consistent among all samples and analysis techniques. Furthermore, dedicated studies are performed to ensure that the observed signal is not caused by kaon or pion misidentification, doubly Cabibbo-suppressed \\( \\mathrm{D}^0 \\to \\mathrm{K}^+ \\pi^- \\) decays and \\( \\mathrm{D}^0 \\overline{\\mathrm{D}}^0 \\) oscillations, decays of charm hadrons originating from beauty hadrons, or artefacts\nTable 2: Systematic uncertainties for the \\( \\delta m_{\\mathrm{BW}} \\) and \\( \\Gamma_{\\mathrm{BW}} \\) parameters. The total uncertainty is calculated as the sum in quadrature of all components except for those related to \\( J^P \\) quantum numbers assignment, which are handled separately.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Source\\( \\sigma_{\\delta m_{\\mathrm{BW}}} \\) [keV/\\( c^2 \\)]\\( \\sigma_{\\Gamma_{\\mathrm{BW}}} \\) [keV]
Fit model
Resolution model27
Resolution correction factor130
Background model330
Model parameters< 1< 1
Momentum scale3--
Energy loss corrections1--
D*+ – D0 mass difference2--
Total543
J^P quantum numbers+11
-14
+18
-38
\n\ndue to the track reconstruction creating duplicate tracks.\n\nSystematic uncertainties for the \\( \\delta m_{\\mathrm{BW}} \\) and \\( \\Gamma_{\\mathrm{BW}} \\) parameters are summarised in Table~\\ref{tab:sysunc} and described below. The largest systematic uncertainty is related to the fit model and is studied using pseudoexperiments with alternative parametrisations of the D0D0\\( \\pi^+ \\) mass shape. Several variations in the fit model are considered: changes in the signal model due to the imperfect knowledge of the detector resolution, an uncertainty in the correction factor for the resolution taken from control channels, parametrisation of the background component and the additional model parameters of the Breit–Wigner function. The model uncertainty related to the assumption of \\( J^P = 1^+ \\) quantum numbers of the state is estimated and listed separately. The results are affected by the overall detector momentum scale, which is known to a relative precision of \\( \\delta \\alpha = 3 \\times 10^{-4} \\)~[95]. The corresponding uncertainty is estimated using simulated samples where the momentum-scale is modified by factors of \\( (1 \\pm \\delta \\alpha) \\). In the reconstruction, the momenta of charged tracks are corrected for energy loss in the detector material, the amount of which is known with a relative uncertainty of 10%~[96]. The resulting uncertainty is assessed by varying the energy loss correction by \\( \\pm 10\\% \\). As the mass of the D0D0\\( \\pi^+ \\) combinations is calculated with the mass of each D0 meson constrained to the known value of the D0 mass, the \\( \\delta m_{\\mathrm{BW}} \\) parameter is insensitive to the precision of the D0 mass. However, the small uncertainty of 2 keV/\\( c^2 \\) for the D*+ – D0 mass difference~[35,97,98] directly affects the \\( \\delta m_{\\mathrm{BW}} \\) value. The corresponding systematic uncertainty is added.\n\nIn summary, using the full dataset corresponding to an integrated luminosity of 9 fb\\(^{-1}\\), collected by the LHCb experiment at centre-of-mass energies of 7, 8 and 13 TeV, a narrow peak is observed in the mass spectrum of D0D0\\( \\pi^+ \\) candidates produced promptly in pp collisions. The statistical significance of the peak is overwhelming. Using the Breit–Wigner parametrisation, the location of the peak relative to the D*+D0 mass threshold, \\( \\delta m_{\\mathrm{BW}} \\),\nand the width, \\( \\Gamma_{\\mathrm{BW}} \\), are determined to be\n\n\\[\n\\delta m_{\\mathrm{BW}} = -273 \\pm 61 \\pm 5^{+11}_{-14} \\text{ keV}/c^2,\n\\]\n\\[\n\\Gamma_{\\mathrm{BW}} = 410 \\pm 165 \\pm 43^{+18}_{-38} \\text{ keV},\n\\]\n\nwhere the first uncertainty is statistical, the second systematic and the third is related to the J\\(^P\\) quantum numbers assignment. The measured \\( \\delta m_{\\mathrm{BW}} \\) value corresponds to a mass of approximately 3875 MeV. This is the narrowest exotic state observed to date [34, 35]. The minimal quark content for this newly observed state is ccu\\(\\overline{d}\\). Two heavy quarks of the same flavour make it manifestly exotic, *i.e.* beyond the conventional pattern of hadron formation found in mesons and baryons. Moreover, a combination of the near-threshold mass, narrow decay width and its appearance in prompt hadroproduction show its genuine resonance nature. This is the first such exotic resonance ever observed. The measured mass and width are consistent with the expected values for a T\\(_{cc}^+\\) isoscalar tetraquark ground state with quantum numbers J\\(^P = 1^+\\). The precision of the mass measurement with respect to the corresponding threshold is superior to those of all other exotic states, which will give better understanding of the nature of exotic states. A dedicated study of the reaction amplitudes for the T\\(_{cc}^+ \\to D^0D^0\\pi^+\\) and T\\(_{cc}^+ \\to D^0D^+\\pi^0(\\gamma)\\) decays that uses the isospin symmetry for the T\\(_{cc}^+ \\to D^*D\\) transition [90] yields insights on the fundamental resonance properties, like the pole position, the scattering length and the effective range. The observation of this ccu\\(\\overline{d}\\) tetraquark candidate close to the D\\(^{*+}\\)D\\(^0\\) threshold further supports the existence of a bbu\\(\\overline{d}\\) tetraquark that is stable with respect to the strong and electromagnetic interactions.\n\nAcknowledgements\n\nThis Letter is dedicated to the memory of our dear colleague Simon Eidelman, whose friendship, deep physics insights and contributions to improving the quality of our papers were greatly appreciated and will be missed. We express our gratitude to our colleagues in the CERN accelerator departments for the excellent performance of the LHC. We thank the technical and administrative staff at the LHCb institutes. We acknowledge support from CERN and from the national agencies: CAPES, CNPq, FAPERJ and FINEP (Brazil); MOST and NSFC (China); CNRS/IN2P3 (France); BMBF, DFG and MPG (Germany); INFN (Italy); NWO (Netherlands); MNiSW and NCN (Poland); MEN/IFA (Romania); MSHE (Russia); MICINN (Spain); SNSF and SER (Switzerland); NASU (Ukraine); STFC (United Kingdom); DOE NP and NSF (USA). We acknowledge the computing resources that are provided by CERN, IN2P3 (France), KIT and DESY (Germany), INFN (Italy), SURF (Netherlands), PIC (Spain), GridPP (United Kingdom), RRCKI and Yandex LLC (Russia), CSCS (Switzerland), IFIN-HH (Romania), CBPF (Brazil), PL-GRID (Poland) and NERSC (USA). We are indebted to the communities behind the multiple open-source software packages on which we depend. Individual groups or members have received support from ARC and ARDC (Australia); AvH Foundation (Germany); EPLANET, Marie Skłodowska-Curie Actions and ERC (European Union); A*MIDEX, ANR, IPhU and Labex P2IO, and Région Auvergne-Rhône-Alpes (France); Key Research Program of Frontier Sciences of CAS, CAS PIFI, CAS CCEPP, Fundamental Research Funds for the Central Universities, and Sci. & Tech. Program of Guangzhou (China); RFBR, RSF and Yandex LLC (Russia); GVA, XuntaGal and GENCAT (Spain); the Leverhulme Trust, the Royal Society and UKRI (United Kingdom).\nMethods\n\nExperimental setup\nThe LHCb detector [85][86] is a single-arm forward spectrometer covering the pseudo-rapidity range \\(2 < \\eta < 5\\), designed for the study of particles containing b or c quarks. The detector includes a high-precision tracking system consisting of a silicon-strip vertex detector surrounding the pp interaction region, a large-area silicon-strip detector located upstream of a dipole magnet with a bending power of about 4 Tm, and three stations of silicon-strip detectors and straw drift tubes placed downstream of the magnet. The tracking system provides a measurement of the momentum, \\(p\\), of charged particles with a relative uncertainty that varies from 0.5% at low momentum to 1.0% at 200 GeV/\\(c\\). The minimum distance of a track to a primary pp collision vertex (PV), the impact parameter (IP), is measured with a resolution of \\((15 + 29/p_T)\\) \\( \\mu m \\), where \\(p_T\\) is the component of the momentum transverse to the beam, in GeV/\\(c\\). Different types of charged hadrons are distinguished using information from two ring-imaging Cherenkov detectors [99]. Photons, electrons and hadrons are identified by a calorimeter system consisting of scintillating-pad and preshower detectors, an electromagnetic and a hadronic calorimeter. Muons are identified by a system composed of alternating layers of iron and multiwire proportional chambers. The online event selection is performed by a trigger, which consists of a hardware stage, based on information from the calorimeter and muon systems, followed by a software stage, which applies a full event reconstruction. The trigger selection algorithms are primarily based on identifying key characteristics of beauty and charm hadrons and their decay products, such as high \\(p_T\\) final state particles, and a decay vertex that is significantly displaced from any of the pp interaction vertices in the event.\n\nSimulated samples\nSimulation is required to model the effects of the detector acceptance, resolution and the imposed selection requirements. In the simulation, pp collisions are generated using PYTHIA [100] with a specific LHCb configuration [101]. Decays of unstable particles are described by EVTGEN [102], in which final-state radiation is generated using PHOTOS [103]. The interaction of the generated particles with the detector, and its response, are implemented using the GEANT4 toolkit [104] as described in Ref. [105].\n\nSelection\nThe selection of \\(D^0 \\rightarrow K^- \\pi^+\\) candidates and \\(D^0 D^0 \\pi^+\\) combinations is similar to those used in Refs. [87][106][108]. Kaon and pion candidates are selected from well-reconstructed tracks within the acceptance of the spectrometer. Particle identification is provided using information from the ring-imaging Cherenkov detectors. Kaons and pions that have transverse momenta larger than 250 MeV/\\(c\\) and are inconsistent with being produced in a pp interaction vertex are combined together to form \\(D^0\\) candidates. The resulting \\(D^0\\) candidates are required to have good vertex quality, mass within \\(\\pm 65\\) MeV/\\(c^2\\) of the known \\(D^0\\) mass [35], transverse momentum larger than 1 GeV/\\(c\\), decay time larger than 100 \\( \\mu m/c \\) and a momentum direction that is consistent with the vector from the primary to the secondary vertex. Selected pairs of \\(D^0\\) candidates consistent with originating\nfrom a common primary vertex are then combined with pion candidates of the same charge as the pions from the \\( D^0 \\rightarrow K^- \\pi^+ \\) decay candidates to form \\( D^0 D^0 \\pi^+ \\) candidates. At least one of the two \\( D^0 \\pi^+ \\) combinations is required to have good vertex quality and mass not exceeding the known \\( D^0 \\) mass by more than \\( 155\\,\\mathrm{MeV}/c^2 \\). For each \\( D^0 D^0 \\pi^+ \\) candidate a kinematic fit [109] is performed. This fit requires both \\( D^0 \\) candidates and a pion to originate from the same primary vertex. A requirement on the quality of this fit is applied to further suppress combinatorial background and reduce the background from \\( D^0 \\) candidates produced in two independent pp interactions or in decays of beauty hadrons [87]. To suppress background from kaon and pion candidates reconstructed from one common track, all track pairs of the same charge are required to have opening angle inconsistent with being zero and mass of the combination to be inconsistent with the sum of masses of the two constituents.\n\nNon-D\\( ^0 \\) background subtraction\n\nThe two-dimensional distribution of the mass of one \\( D^0 \\) candidate versus the mass of the other \\( D^0 \\) candidate from selected \\( D^0 D^0 \\pi^+ \\) combinations is used to subtract the background from fake \\( D^0 \\) candidates. The procedure employs the sPlot technique [110], where an extended unbinned maximum-likelihood fit to the two-dimensional distribution is performed. The signal is described using a modified Novosibirsk function [111] and the background is modelled by a product of an exponential function and a positive polynomial function [87]. Each candidate is assigned a positive weight for being signal-like or a negative weight for being background-like, with the masses of the two \\( D^0 \\) candidates as the discriminating variables. All candidates are then retained and the weights are used in the further analysis for statistical subtraction of non-D\\( ^0 \\) background.\n\nSystematic uncertainties\n\nSeveral sources of systematic uncertainty on the mass \\( \\delta m_{BW} \\) and width \\( \\Gamma_{BW} \\) of the \\( T_{cc}^+ \\) state have been evaluated. The largest systematic uncertainty is related to the fit model and is studied using a set of alternative parametrisations and pseudoexperiments. For each alternative model, an ensemble of pseudoexperiments is produced; each is generated using the model under consideration with parameters obtained from a fit to the data. A subsequent fit with the default model to each pseudoexperiment is performed and the mean values of the parameters of interest over the ensemble are evaluated. The absolute value of the difference between the ensemble mean and the value of the parameter obtained from the fit to the data sample is used to characterise the difference between the alternative model and the default model. The maximal value of such a difference over the considered set of alternative models is taken as the corresponding systematic uncertainty for the mass \\( \\delta m_{BW} \\) and width \\( \\Gamma_{BW} \\) of the \\( T_{cc}^+ \\) state. The following sources of systematic uncertainties related to the fit model are considered:\n\n• Imperfect knowledge of detector resolution model: to estimate the associated systematic uncertainty alternative resolution functions are studied, namely a symmetric variant of an Apollonios function [112]; a modified Gaussian function with symmetric power-law tails on both sides of the distribution [113,114]; a generalised symmetric Student’s t-distribution [115,116]; a symmetric Johnson’s Su distribution [117,118]; and a modified Novosibirsk function [111].\n• Difference in detector resolution due to imperfect modelling: a correction factor of 1.05 for the resolution is applied for the default fit to account for such a difference. This factor was studied for several other decays measured with the LHCb detector and found to lie between 1.0 and 1.1 [29,91,92,119,121]. For decays with relatively low-momentum tracks, this factor is close to 1.05. The factor is also cross-checked using large samples of \\( \\mathrm{D}^{*+} \\to \\mathrm{D}^0 \\pi^+ \\) decays, where a value of 1.06 is obtained. To assess the systematic uncertainty related to this factor, detector resolution models with correction factors of 1.0 and 1.1 are studied as alternative models.\n\n• Parametrisation of the background component: to assess the associated systematic uncertainty, the order of the positive polynomial function used for the baseline fit is varied. In addition, to estimate the possible effect of a small contribution from \\( \\mathrm{D}^0 \\mathrm{D}^0 \\pi^+ \\) combinations without an intermediate \\( \\mathrm{D}^{*+} \\) meson, a three-body background component is added to the fit. This component is described by a product of the three-body phase space function [122,123] and a positive linear or second-order polynomial function.\n\n• Model parameters of the Breit–Wigner function: alternative parametrisations include different choices for the decay structure, \\( m_A = m_{\\mathrm{D}^0} \\) and \\( m_B = m_{\\mathrm{D}^0} + m_{\\pi^+} \\); the meson radius, 1.5 GeV\\(^{-1}\\) and 5 GeV\\(^{-1}\\), and the orbital angular momentum between A and B particles, corresponding to S- and D-waves. The effect of the different decay structure and choice of meson radius is smaller than 1 keV/\\(c^2\\) and 1 keV for the \\( \\delta m_{\\mathrm{BW}} \\) and \\( \\Gamma_{\\mathrm{BW}} \\) parameters, respectively. The parameters of interest are more sensitive to the choice of orbital angular momentum, in which the S-wave function gives larger \\( \\delta m_{\\mathrm{BW}} \\) and smaller \\( \\Gamma_{\\mathrm{BW}} \\), and the D-wave function corresponds to smaller \\( \\delta m_{\\mathrm{BW}} \\) and larger \\( \\Gamma_{\\mathrm{BW}} \\). As the S-wave and D-wave imply that the quantum numbers of the T\\(^{cc}\\) state differ from J\\(^\\mathrm{P} = 1^+\\), the corresponding systematic uncertainty is considered separately and is not included it in the total systematic uncertainty.\n\nThe calibration of the momentum scale of the tracking system is based upon large calibration samples of \\( \\mathrm{B}^+ \\to \\mathrm{J}/\\psi \\mathrm{K}^+ \\) and \\( \\mathrm{J}/\\psi \\to \\mu^+ \\mu^- \\) decays [124]. The accuracy of the procedure has been checked using other fully reconstructed B decays together with two-body \\( \\Upsilon(\\mathrm{nS}) \\) and \\( \\mathrm{K}_S^0 \\) decays and the largest deviation of the bias in the momentum scale of \\( \\delta \\alpha = 3 \\times 10^{-4} \\) is taken as the uncertainty [95]. This is then propagated to uncertainties for the parameters of interest using simulated samples, where momentum scale corrections of \\( (1 \\pm \\delta \\alpha) \\) are applied. Half of the difference between the peak locations obtained with \\( 1 + \\delta \\alpha \\) and \\( 1 - \\delta \\alpha \\) corrections applied to the same simulated sample is taken as an estimate of the systematic uncertainty due to the momentum scale.\n\nIn the reconstruction the momenta of the charged tracks are corrected for the energy loss in the detector material. The energy loss corrections are calculated using the Bethe–Bloch formula [125,126]. The amount of material traversed in the tracking system by a charged particle is known to 10% accuracy [96]. To assess the corresponding uncertainty, the magnitude of the calculated corrections is varied by ±10%. Half of the difference between the peak locations obtained with +10% and −10% corrections applied to the same simulated sample is taken as an estimate of the systematic uncertainty due to the energy loss corrections.\n\nThe mass of the \\( \\mathrm{D}^0 \\mathrm{D}^0 \\pi^+ \\) combinations is calculated with both \\( \\mathrm{D}^0 \\) candidate masses constrained to the known \\( \\mathrm{D}^0 \\) meson mass [35]. This procedure removes the uncertainty on\nthe \\( \\delta m_{BW} \\) parameter related to imprecise knowledge of the D\\( ^0 \\) mass. 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Alvarez Cartelle55, S. Amato2,\nJ.L. Amey54, Y. Amhis11, L. An48, L. Anderlini22, A. Andreianov38, M. Andreotti21,\nF. Archilli17, A. Artamonov44, M. Artuso68, K. Arzynamot42, E. Aslanides10, M. Atzeni50,\nB. Audurier12, S. Bachmann17, M. Bachmayer49, J.J. Back56, P. Baladron Rodriguez46,\nV. Balagural2, W. Baldini21, J. Baptista Leite1, M. Barbetti22,g, R.J. Barlow62, S. Barsuk11,\nW. Barter61, M. Bartolini24,h, F. Baryshnikov83, J.M. Basels14, S. Bashir34, G. Bassi29,\nB. Batsukh68, A. Battig15, A. Bay49, A. Beck56, M. Becker15, F. Bedeschi29, I. Bediaga1,\nA. Beiter68, V. Belavin42, S. Belin27, V. Bellec50, K. Belous44, I. Belov40, I. Belyaev41,\nG. Bencivenni23, E. Ben-Haim13, A. Berezhnoy40, R. Bernet50, D. Berninghoff17,\nH.C. Bernstein68, C. Bertella48, A. Bertolin28, C. Betancourt50, F. Betti48, Ia. Bezshyiko50,\nS. Bhasin54, J. Bhom35, L. Bian73, M.S. Bicker15, S. Bifani53, P. Billoir13, M. Birch61,\nF.C.R. Bishop55, A. Bitadze62, A. Bizzeti22,k, M. Björn63, M.P. Blago48, T. Blake56, F. Blanc49,\nS. Blusk68, D. Bobulska59, J.A. Boelhauve15, O. Boente Garcia46, T. Boettcher65,\nA. Boldyrev82, A. Bondar43, N. Bondar38,48, S. Borghi62, M. Borisyak42, M. Borsato17,\nJ.T. Borsuk35, S.A. Bouchiba49, T.J.V. Bowcock60, A. Boyer48, C. Bozzi21, M.J. Bradley61,\nS. Braun66, A. Brea Rodriguez46, J. Brodzicka35, A. Brossa Gonzalo56, D. Brundu27,\nA. Buonaura50, L. Buonincontri28, A.T. Burke62, C. Burr48, A. Bursche72, A. Butkevich39,\nJ.S. Butter32, J. Buytaert48, W. Byczynski48, S. Cadeddu27, H. Cai73, R. Calabrese21,f,\nL. Calefice15,13, L. Calero Diaz23, S. Cali23, R. Calladine53, M. Calvi26,j, M. Calvo Gomez85,\nP. Camargo Magalhaes54, P. Campana23, A.F. Campoverde Quezada6, S. Capelli26,j,\nL. Capriotti20,d, A. Carbone20,d, G. Carboni31, R. Cardinale24,h, A. Cardinelli27, I. Carli4,\nP. Carniti26,j, L. Carus14, K. Carvalho Akiba32, A. Casais Vidal46, G. Casse60, M. Cattaneo48,\nG. Cavallero48, S. Celani49, J. Cerasoli10, D. Cervenkov63, A.J. Chadwick60, M.G. Chapman54,\nM. Charles13, Ph. Charpentier48, G. Chatzikonstantinidis53, C.A. Chavez Barajas60,\nM. Chefdeville8, C. Chen3, S. Chen4, A. Chernov35, V. Chobanova46, S. Cholak49,\nM. Chrzaszcz35, A. Chubykin38, V. Chulikov38, P. Ciambrone23, M.F. Cicala56, X. Cid Vidal46,\nG. Ciezarek48, P.E.L. Clarke58, M. Clemencic48, H.V. Cliff55, J. Cloisier48, J.L. Cobbedick62,\nV. Coco48, J.A.B. Coelho11, J. Cogan10, E. Cogneras9, L. Cojoariu37, P. Collins48,\nT. Colombo48, L. Congedo19,c, A. Contu27, N. Cooke53, G. Coombs39, I. Corredoira 46,\nG. Corti48, C.M. Costa Sobral56, B. Couturier48, D.C. Craik64, J. Crkovská67, M. Cruz Torres1,\nR. Currie58, C.L. Da Silva67, S. Dadabaev83, L. Dai71, E. Dall’Occo15 , J. Dalseno46,\nC. D’Ambrosio48, A. Danilina41, P. d’Argent48, J.E. Davies62, A. Davis62,\nO. De Aguilar Francisco62, K. De Bruyn79, S. De Capua62, M. De Cian49, J.M. De Miranda1,\nL. De Paula2, M. De Serio19,c, D. De Simone50, P. De Simone23, F. De Vellis15, J.A. de Vries80,\nC.T. Dean67, F. Deberardis19,c, D. Decamp8, V. Dediu10, L. Del Buono13, B. Delaney55,\nH.-P. Dembinski15, A. Dendek34, V. Denysenko50, D. Derkach82, O. Deschamps9, F. Desse11,\nF. Dettori27,e, B. Dey77, A. Di Cicco23, P. Di Nezza23, S. Didenko83, L. Dieste Maronas46,\nH. Dijkstra48, V. Dobishuk52, C. Dong3, A.M. Donohoe18, F. Dordei27, A.C. dos Reis1,\nL. Douglas59, A. Dovbnya51, A.G. Downes8, M.W. Dudek25, L. Dufour48, V. Duk78,\nP. Durante48, J.M. Durham67, D. Dutta62, A. Dziurda35, A. Dzyuba38, S. Easo57, U. Egede69,\nV. Egorychev41, S. Eidelman43,u,l, S. Eisenhardt58, S. Ek-In49, L. Elkhund59,86, S. Ely68,\nA. Ene37, E. Epple67, S. Escher14, J. Eschle50, S. Esen13, T. Evans48, A. Falabella20, J. Fan3,\nY. Fan6, B. Fang73, S. Farry60, D. Fazzini26,j, M. Féo48, A. Fernandez Prieto46, A.D. Fernezz66,\nF. Ferrari20,d, L. Ferreira Lopes49, F. Ferreira Rodrigues2, S. Ferreres Sole32, M. Ferrillo50,\nM. Ferro-Luzzi18, S. Filippov39, R.A. Fini19, M. Fiorini21,f, M. Firlej34, K.M. Fischer63,\nD.S. Fitzgerald87, C. Fitzpatrick62, T. Fiutowski34, A. Fkiaras48, F. Fleuret12, M. Fontana13, F. Fontanelli24,h, R. Forty48, D. Foulds-Holt55, V. Franco Lima60, M. Franco Sevilla66, M. Frank48, E. Franzoso21, G. Frau17, C. Frei48, D.A. Friday59, J. Fu6, Q. Fuehring15, E. Gabriel32, G. Galati19,e, A. Gallas Torreira46, D. Galli20,d, S. Gambetta58,48, Y. Gan3, M. Gandelman2, P. Gandini25, Y. Gao5, M. Garau27, L.M. Garcia Martin56, P. Garcia Moreno45, J. García Pardinas26,j, B. García Plana46, F.A. Garcia Rosales12, L. Garrido45, C. Gaspar48, R.E. Geertsema32, D. Gerick17, L.L. Gerken15, E. Gersabeck62, M. Gersabeck62, T. Gershon56, D. Gerstel10, L. Giambastiani28, V. Gibson55, H.K. Gienma36, A.L. Gilman63, M. Giovannetti23,p, A. Gioventù46, P. Gironella Gironell45, L. Giubega37, C. Giugliano21,f,48, K. Gizdov58, E.L. Gkougkousis48, V.V. Gligorov13, C. Göbel70, E. Golobardes85, D. Golubkov41, A. Golutvin61,83, A. Gomes1,a, S. Gomez Fernandez45, F. Goncalves Abrantes63, M. Goncerz35, G. Gong3, P. Gorbounov41, I.V. Gorelov40, C. Gottu26, E. Govorkova48, J.P. Grabowski17, T. Grammatico13, L.A. Granado Cardoso48, E. Grauges45, E. Graverini49, G. Graziani22, A. Grecu37, L.M. Greeven32, N.A. Grieser4, L. Grillo62, S. Gromov83, B.R. Gruber Cazon33, C. Gu3, M. Guarise21, M. Guittiere11, P. A. Günther17, E. Gushchin39, A. Guth14, Y. Guz44, T. Gys48, T. Hadavizadeh69, G. Haefeli49, C. Haen48, J. Haimberger48, T. Halewood-leagas60, P.M. Hamilton66, J.P. Hamacher60, Q. Han7, X. Han17, T.H. Hancock63, E.B. Hansen62, S. Hansmann-Menzemer17, N. Harnew63, T. Harrison60, C. Hasse48, M. Hatch48, J. He6,b, M. Hecker61, K. Heijhoff32, K. Heinicke15, A.M. Hennequin48, K. Hennessy60, L. Henry48, J. Heuel14, A. Hicheur2, D. Hill49, M. Hilton62, S.E. Hollitt15, R. Hou7, Y. Hou8, J. Hu17, J. Hu72, W. Hu7, X. Hu3, W. Huang73, W. Hulsbergen32, R.J. Hunter56, M. Hushchyn82, D. Hutchcroft60, D. Hynds32, P. Ibis15, M. Idzik34, D. Ilin38, P. Ilten65, A. Inglessi38, A. Ishteev80, K. Ivshin38, R. Jacobsson48, H. Jage14, S. Jakobsen48, E. Jans32, B.K. Jashal47, A. Jawahery66, V. Jevtic15, F. Jiang3, M. John63, D. Johnson48, C.R. Jones55, T.P. Jones56, B. Jost48, N. Jurik48, S.H. Kalavan Kadavath34, S. Kandybei51, Y. Kang3, M. Karacson48, M. Karpov82, F. Keizer48, D.M. Keller68, M. Kenzie56, T. Ketel33, B. Khanji15, A. Kharisova84, S. Kholodenko44, T. Kirn14, V.S. Kirsebom49, O. Kitoumi64, S. Klaver32, N. Kleijne29, K. Klimaszewski36, M.R. Kmiec36, S. Kollijev52, A. Kondybayeva83, A. Konoplyannikov41, P. Kopciewicz34, R. Kopecná17, P. Koppenburg32, M. Korolev40, I. Kostiuk32,52, O. Kot52, S. Kotriakhova21,38, P. Kravchenko38, L. Kravchuk39, R.D. Krawczyk48, M. Kreps56, F. Kress61, S. Kretzschmar14, P. Krokovny43,u, W. Krupa34, W. Krzemien36, M. Kucharczyk35, V. Kudryavtsev43,u, H.S. Kuindersma32,33, G.J. Kunde67, T. Kvaratskheliya41, D. Lacarrère48, G. Lafferty62, A. Lau27, A. Lampis27, T. Lanfranchi50, J.J. Lane62, R. Lane54, G. Lanfranchi23, C. Langenbruch14, J. Langer15, O. 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Petrov81, S. Petrucci58, M. Petruzzo25, T.T.H. Pham68, L. Pica29,m, M. Piccini78, B. Pietrzyk8, G. Pietrzyk49, M. Pili63, D. Pinci30, F. Pisani48, M. Pizzichemi26,48,j, Resmi P.K10, V. Placinta37, J. Plews53, M. Plo Casasus46, F. Polci13, M. Poli Lener23, M. Poliakova68, A. Polevukov10, N. Polukhina83,t, I. Polyakov68, E. Polycarpo2, S. Ponce48, D. Popov6,48, S. Popov42, S. Poslavskii44, K. Prasanth35, L. Promberger48, C. Prouve46, V. Pugatch52, V. Puill11, H. Pullen63, G. Punzi29,n, H. Qi3, W. Qian6, J. Qin6, N. Qin3, R. Quagliani49, B. Quintana8, N.V. Raab18, R.I. Rabadan Trejo6, B. Rachwal34, J.H. Rademacker54, M. Rama29, M. Ramos Pernas56, M.S. Rangel2, F. Ratnikov42,82, G. Raven33, M. Reboud8, F. Redi49, F. Reiss52, C. Remon Alepuz47, Z. Ren3, V. Renaudin63, R. Ribatti29, S. Ricciardi57, K. Rinnert60, P. Robbe11, G. Robertson58, A.B. Rodrigues49, E. Rodrigues60, J.A. Rodriguez Lopez74, E.R.R. Rodriguez Rodriguez46, A. Rollings63, P. Roloff48, V. Romanovsky44, M. Romero Lamas46, A. Romero Vidal46, J.D. Roth87, M. Rotondo23, M.S. Rudolph68, T. Ruf48, R.A. Ruiz Fernandez46, J. Ruiz Vidal47, A. Ryzhikov82, J. Ryzka34, J.J. Saborido Silva46, N. Sagidova38, N. Sahoo56, B. Saitta27,e, M. Salomoni48, C. Sanchez Gras32, R. Santacesaria30, C. Santamarina Rios46, M. Santimaria23, E. Santovetti31,p, D. Saranin83, G. Sarpis14, M. Sarpis75, A. Sarti30, C. Satriano30,o, A. Satta31, M. Saur15, D. Savrina41,40, H. Sazak9, L.G. Scantlebury Smead63, A. Scarabotto13, S. Schael14, S. Scherl60, M. Schiller59, H. Schindler48, M. Schnelling16, B. Schmidt48, S. Schmitt14, O. Schneider49, A. Schopper48, M. Schubiger32, S. Schulze49, M.H. Schune11, R. Schwemmer48, B. Sciascia23,48, S. Sellam46, A. Semennikov41, M. Senghi Soares33, A. Sergi24,h, N. Serra50, L. Sestini28, A. Seuthe15, Y. Shang8, D.M. Shangase87, M. Shapkin44, I. Shechenyov83, L. Shchutska49, T. Shears60, L. Shekhtman43,u, Z. Shen5, V. Shevchenko81, E.B. Shields26,j, Y. Shimizu11, E. Shmanin83, J.D. Shupperd68, B.G. Siddi21, R. Silva Coutinho50, G. Simi28, S. Simone19,c, N. Skidmore62, T. Skwarnicki68, M.W. Slater53, I. Slazyk21,f, J.C. Smallwood63, J.G. Smeaton55, A. Smetkina41, E. Smith50, M. Smith61, A. Snoch32, M. Soares20, L. Soares Lavra9, M.D. Sokoloff65, F.J.P. Soler59, A. Solovev38, I. Solovyev38, F.L. Souza De Almeida2, B. Souza De Paula2, B. Spaan15, E. Spadaro Norella25, P. Spradlin59, F. Stagni48, M. Stahl65, S. Stahl48, S. Stanislaus63, O. Steinkamp50,83, O. Stenyakin44, H. Stevens15, S. Stone68, M. Straticiuc37, D. Strekalina83, F. Suljik63, J. Sun27, L. Sun73, Y. Sun66, P. Svihra62, P.N. Swallow53, K. Swientek34, A. Szabelski36, T. Szumlak34, M. Szymanski48, S. Taneja62, A.R. Tanner54, M.D. Tat63, A. Terentev83, F. Teubert48, E. Thomas48, D.J.D. Thompson53, K.A. Thomson60, V. Tisserand9, S. T'Jampens8, M. Tobin4, L. Tomassetti21,f, X. Tong5, D. Torres Machado1, D.Y. Tou13, E. Trifonova83, C. Tripli49,\nG. Tuci6, A. Tully49, N. Tuning32,48, A. Ukleja36, D.J. Unverzagt17, E. Ursov83, A. Usachov32, A. Ustyuzhanin42,82, U. Uwer17, A. Vagner84, V. Vagnoni20, A. Valassi48, G. Valenti20, N. Valls Canudas85, M. van Beuzekom32, M. Van Dijk49, E. van Herwijnen83, C.B. Van Hulse18, M. van Veghel79, R. Vazquez Gomez45, P. Vazquez Regueiro46, C. Vázquez Sierra48, S. Vecchi21, J.J. Velthuis54, M. Veltri22,r, A. Venkateswaran68, M. Veronesi32, M. Vesterinen56, D. Vieira65, M. Vieites Diaz49, H. Viennmann76, X. Vilasis-Cardona85, E. Vilella Figueras60, A. Villa20, P. Vincent13, F.C. Volle11, D. Vom Bruch10, A. Vorobyev38, V. Vorobyev43,u, N. Voropaev38, K. Vos80, R. Waldi17, J. Walsh29, C. Wang17, J. Wang5, J. Wang4, J. Wang3, J. Wang73, M. Wang3, R. Wang54, Y. Wang7, Z. Wang50, Z. Wang3, Z. Wang6, J.A. Ward56, N.K. Watson53, S.G. Weber13, D. Websdale61, C. Weisser64, B.D.C. Westhenry54, D.J. White62, M. Whitehead54, A.R. Wiederhold56, D. Wiedner15, G. Wilkinson63, M. Wilkinson68, I. Williams55, M. Williams64, M.R.J. Williams58, F.F. Wilson57, W. Wislicki36, M. Wittek35, L. Witola17, G. Wormser11, S.A. Wotton55, H. Wu68, K. Wylie48, Z. Xiang6, D. Xiao7, Y. Xie7, A. Xu5, J. Xu6, L. Xu3, M. Xu7, Q. Xu6, Z. Xu5, Z. Xu6, D. Yang3, S. Yang6, Y. Yang6, Z. Yang5, Z. Yang66, Y. Yao68, L.E. Yeomans50, H. Yin7, J. Yu71, X. Yuan68, O. Yushchenko44, E. Zaffaroni49, M. Zavertyaev16,t, M. Zdybal35, O. Zenaiev48, M. Zeng3, D. Zhang7, L. Zhang3, S. Zhang71, S. Zhang5, Y. Zhang5, Y. Zhang63, A. Zharkova83, A. Zhelezov17, Y. Zheng6, T. Zhou5, X. Zhou6, Y. Zhou6, V. Zhovkovska11, X. Zhu3, X. Zhu7, Z. Zhu6, V. Zhukov14,40, J.B. Zonneveld58, Q. Zou4, S. Zucchelli20,d, D. Zuliani28, G. Zunică62.\n\n1 Centro Brasileiro de Pesquisas Físicas (CBPF), Rio de Janeiro, Brazil\n2 Universidade Federal do Rio de Janeiro (UFRJ), Rio de Janeiro, Brazil\n3 Center for High Energy Physics, Tsinghua University, Beijing, China\n4 Institute Of High Energy Physics (IHEP), Beijing, China\n5 School of Physics State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing, China\n6 University of Chinese Academy of Sciences, Beijing, China\n7 Institute of Particle Physics, Central China Normal University, Wuhan, Hubei, China\n8 Univ. Savoie Mont Blanc, CNRS, IN2P3-LAPP, Annecy, France\n9 Université Clermont Auvergne, CNRS/IN2P3, LPC, Clermont-Ferrand, France\n10 Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France\n11 Université Paris-Saclay, CNRS/IN2P3, IJCLab, Orsay, France\n12 Laboratoire Leprince-Ringuet, CNRS/IN2P3, Ecole Polytechnique, Institut Polytechnique de Paris, Palaiseau, France\n13 LPNHE, Sorbonne Université, Paris Diderot Sorbonne Paris Cité, CNRS/IN2P3, Paris, France\n14 I. Physikalisches Institut, RWTH Aachen University, Aachen, Germany\n15 Fakultät Physik, Technische Universität Dortmund, Dortmund, Germany\n16 Max-Planck-Institut für Kernphysik (MPIK), Heidelberg, Germany\n17 Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany\n18 School of Physics, University College Dublin, Dublin, Ireland\n19 INFN Sezione di Bari, Bari, Italy\n20 INFN Sezione di Bologna, Bologna, Italy\n21 INFN Sezione di Ferrara, Ferrara, Italy\n22 INFN Sezione di Firenze, Firenze, Italy\n23 INFN Laboratori Nazionali di Frascati, Frascati, Italy\n24 INFN Sezione di Genova, Genova, Italy\n25 INFN Sezione di Milano, Milano, Italy\n26 INFN Sezione di Milano-Bicocca, Milano, Italy\n27 INFN Sezione di Cagliari, Monserrato, Italy\n28 Università degli Studi di Padova, Università e INFN, Padova, Padova, Italy\n29 INFN Sezione di Pisa, Pisa, Italy\n30 INFN Sezione di Roma La Sapienza, Roma, Italy\n31 INFN Sezione di Roma Tor Vergata, Roma, Italy\n32 Nikhef National Institute for Subatomic Physics, Amsterdam, Netherlands\n33 Nikhef National Institute for Subatomic Physics and VU University Amsterdam, Amsterdam, Netherlands\n34 AGH - University of Science and Technology, Faculty of Physics and Applied Computer Science, Kraków, Poland\n35 Henryk Niewodniczanski Institute of Nuclear Physics Polish Academy of Sciences, Kraków, Poland\n36 National Center for Nuclear Research (NCBJ), Warsaw, Poland\n37 Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest-Magurele, Romania\n38 Petersburg Nuclear Physics Institute NRC Kurchatov Institute (PNPI NRC KI), Gatchina, Russia\n39 Institute for Nuclear Research of the Russian Academy of Sciences (INR RAS), Moscow, Russia\n40 Institute of Nuclear Physics, Moscow State University (SINP MSU), Moscow, Russia\n41 Institute of Theoretical and Experimental Physics NRC Kurchatov Institute (ITEP NRC KI), Moscow, Russia\n42 Yandex School of Data Analysis, Moscow, Russia\n43 Budker Institute of Nuclear Physics (SB RAS), Novosibirsk, Russia\n44 Institute for High Energy Physics NRC Kurchatov Institute (IHEP NRC KI), Protvino, Russia, Protvino, Russia\n45 ICCUB, Universitat de Barcelona, Barcelona, Spain\n46 Instituto Galego de Física de Altas Enerxías (IGFAE), Universidade de Santiago de Compostela, Santiago de Compostela, Spain\n47 Instituto de Física Corpuscular, Centro Mixto Universidad de Valencia - CSIC, Valencia, Spain\n48 European Organization for Nuclear Research (CERN), Geneva, Switzerland\n49 Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland\n50 Physik-Institut, Universität Zürich, Zürich, Switzerland\n51 NSC Kharkiv Institute of Physics and Technology (NSC KIPT), Kharkiv, Ukraine\n52 Institute for Nuclear Research of the National Academy of Sciences (KINR), Kyiv, Ukraine\n53 University of Birmingham, Birmingham, United Kingdom\n54 H.H. Wills Physics Laboratory, University of Bristol, Bristol, United Kingdom\n55 Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom\n56 Department of Physics, University of Warwick, Coventry, United Kingdom\n57 STFC Rutherford Appleton Laboratory, Didcot, United Kingdom\n58 School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom\n59 School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom\n60 Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom\n61 Imperial College London, London, United Kingdom\n62 Department of Physics and Astronomy, University of Manchester, Manchester, United Kingdom\n63 Department of Physics, University of Oxford, Oxford, United Kingdom\n64 Massachusetts Institute of Technology, Cambridge, MA, United States\n65 University of Cincinnati, Cincinnati, OH, United States\n66 University of Maryland, College Park, MD, United States\n67 Los Alamos National Laboratory (LANL), Los Alamos, United States\n68 Syracuse University, Syracuse, NY, United States\n69 School of Physics and Astronomy, Monash University, Melbourne, Australia, associated to 56\n70 Pontifícia Universidade Católica do Rio de Janeiro (PUC-Rio), Rio de Janeiro, Brazil, associated to 2\n71 Physics and Micro Electronic College, Hunan University, Changsha City, China, associated to 7\n72 Guangdong Provincial Key Laboratory of Nuclear Science, Guangdong-Hong Kong Joint Laboratory of Quantum Matter, Institute of Quantum Matter, South China Normal University, Guangzhou, China, associated to 3\n73 School of Physics and Technology, Wuhan University, Wuhan, China, associated to 3\n74 Departamento de Física , Universidad Nacional de Colombia, Bogota, Colombia, associated to 13\n75 Universität Bonn - Helmholtz-Institut für Strahlen und Kernphysik, Bonn, Germany, associated to 17\n76 Institut für Physik, Universität Rostock, Rostock, Germany, associated to 17\n77 Eotvos Lorand University, Budapest, Hungary, associated to 48\n78 INFN Sezione di Perugia, Perugia, Italy, associated to 21\n79 Van Swinderen Institute, University of Groningen, Groningen, Netherlands, associated to 32\n80 Universiteit Maastricht, Maastricht, Netherlands, associated to 32\n81 National Research Centre Kurchatov Institute, Moscow, Russia, associated to 41\n82 National Research University Higher School of Economics, Moscow, Russia, associated to 42\n83 National University of Science and Technology “MISIS”, Moscow, Russia, associated to 41\n84 National Research Tomsk Polytechnic University, Tomsk, Russia, associated to 41\n85 DS4DS, La Salle, Universitat Ramon Llull, Barcelona, Spain, associated to 45\n86 Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden, associated to 59\n87 University of Michigan, Ann Arbor, United States, associated to 68\n\na Universidade Federal do Triângulo Mineiro (UFTM), Uberaba-MG, Brazil\nb Hangzhou Institute for Advanced Study, UCAS, Hangzhou, China\nc Università di Bari, Bari, Italy\nd Università di Bologna, Bologna, Italy\ne Università di Cagliari, Cagliari, Italy\nf Università di Ferrara, Ferrara, Italy\ng Università di Firenze, Firenze, Italy\nh Università di Genova, Genova, Italy\ni Università degli Studi di Milano, Milano, Italy\nj Università di Milano Bicocca, Milano, Italy\nk Università di Modena e Reggio Emilia, Modena, Italy\nl Università di Padova, Padova, Italy\nm Scuola Normale Superiore, Pisa, Italy\nn Università di Pisa, Pisa, Italy\no Università della Basilicata, Potenza, Italy\np Università di Roma Tor Vergata, Roma, Italy\nq Università di Siena, Siena, Italy\nr Università di Urbino, Urbino, Italy\ns MSU - Iligan Institute of Technology (MSU-IIT), Iligan, Philippines\nt P.N. Lebedev Physical Institute, Russian Academy of Science (LPI RAS), Moscow, Russia\nu Novosibirsk State University, Novosibirsk, Russia\n\n† Deceased"} {"paper_id": "prb80", "title": "Sparse Estimation of Correlations among Microbiomes (SECOM)", "text": "Sparse Estimation of Correlations among Microbiomes (SECOM)\n\nHuang Lin\nEunice Kennedy Shriver National Institute of Child Health and Human Development (NICHD), National Institutes of Health\n\nMerete Eggesbo\nNorwegian Institute of Public Health\n\nShyamal Peddada (Shyamal.peddada@nih.gov)\nEunice Kennedy Shriver National Institute of Child Health and Human Development (NICHD), National Institutes of Health https://orcid.org/0000-0003-1276-7252\n\nArticle\n\nKeywords:\n\nPosted Date: April 1st, 2022\n\nDOI: https://doi.org/10.21203/rs.3.rs-1497744/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nVersion of Record: A version of this preprint was published at Nature Communications on August 23rd, 2022. See the published version at https://doi.org/10.1038/s41467-022-32243-x.\nSparse Estimation of Correlations among Microbiomes (SECOM)\n\nHuang Lin1, Merete Eggesbø2, and Shyamal Das Peddada1,*\n\n1Biostatistics and Bioinformatics Branch, NICHD, NIH, Bethesda, MD, USA\n2Norwegian Institute of Public Health, Oslo, Norway\n*shyamal.peddada@nih.gov\n\nABSTRACT\n\nIt is well-known that human gut microbiota form a complex ecosystem where microbes correlate with each other. Due to complex underlying interactions, some microbes may correlate nonlinearly. Yet, there are no measures in the literature that quantify these nonlinear relationships. We introduce a novel concept of correlation that allows for linear and nonlinear relationships among microbes. It is well-known that infant gut evolves as the child grows. Using the proposed methodology, for the first time in the literature we characterize temporal changes in correlations among bacterial families during a baby’s first year after birth. For example, we discover for the first time that Lachnospiraceae and Ruminococcaceae, which play important roles in degrading complex polysaccharides into short-chain fatty acids, interact with several families during a baby’s first year of birth. Similarly, Bifidobacteriaceae, Bacteroidiceae, Lachnospiraceae, and Clostridiaceae, are all negatively correlated with Enterobacteriaceae, a family that contains pathogens such as Salmonella, Shigella and Escherichia coli. Statistical properties of the proposed methodology are evaluated analytically and by using synthetic data.\n\nIntroduction\n\nIn any given ecosystem, members maintain complex interactions among themselves for the growth and stability of the whole community. This is also true for microbial ecosystems. Some bacteria display mutualism where they help or benefit from each other, commensalism where one benefits while the others are not affected, parasitism or mutual exclusion where one may benefit at the expense of another1. One needs to understand perturbations or changes in the interactions among microbiota within and between ecosystem(s) because they can potentially impact various health outcomes, such as obesity2, inflammatory bowel diseases3, HIV4, and so on. To make such assessments, there is an urgent need for statistical and computational methods to characterize interactions among microbiota.\n\nAlthough there exists considerable literature on methods for performing differential abundance analysis and analysis of diversity5,6, methods for describing interactions among microbiota are not as well developed. As the first step to characterize interactions, one typically is interested in describing the correlation coefficient between a pair of microbes.\n\n16S ribosomal RNA (rRNA) and other high-throughput sequencing techniques enable profiling of microbial communities, revealing the abundances and phylogeny of microbial populations across diverse ecosystems. The observed counts of taxa are constrained by an arbitrary sequencing depth (library size), which is due to a fixed upper bound on the number of reads per sequencing instrument. Thus, the observed counts are an unknown fraction of the underlying true abundance of taxa in a unit volume of the ecosystem6,7. Consequently, they are relative abundances and hence are compositional data7–13. It is well-recognized in the literature that due to compositionality of the observed microbiome data, standard methods such as Pearson, or Spearman correlation coefficients for these data are theoretically invalid which results in misinterpretations of the data9,14–17. The effects of compositionality on these methods are pronounced when the number of taxa is limited, such as microbiome data at the phylum level, and when the microbial diversity is small14. Additionally, sequencing efficiencies are not necessarily the same for each taxon, which leads to a taxon-specific bias when some taxa are preferentially measured over others during the sequencing experimental workflow18. A concrete example of this bias can be seen by the differential sequencing efficiencies between gram-negative and gram-positive bacteria. Gram-positive bacteria have strong cell walls, which makes them harder to extract than gram-negative bacteria in the data preparation step. Thus, gram-positive bacteria may be underrepresented in the observed abundances. We illustrate the problems of using standard concepts of correlation coefficients with the help of a toy example shown in Fig. 1. A total of 100 taxa were generated from a Negative-Binomial distribution. For simplicity of visualization, scatter plots corresponding to 5 taxa are shown in the figure. The data were generated so that the underlying true abundances for taxa T1 and T3 are perfectly linearly correlated, whereas taxa T2 and T4 are parabolic in their relationship, and the remaining pairs are uncorrelated (Fig. 1a). These correlations were completely distorted in the observed counts (Fig. 1b) due to differential sampling fractions6,7 (across samples) and sequencing efficiencies (across taxa). Without\nproperly addressing these two sources of biases, the standard concepts of correlation coefficients between a pair of taxa, such as the Pearson and the Spearman correlation coefficients, are erroneously positive (Fig. 1c) with very significant p-values. The distribution of p-values is far from the diagonal line corresponding to uniform distribution (Supplementary Fig. 1a). This phenomenon is purely driven by the artifacts of variations in sampling fractions and sequencing efficiencies.\n\nA second challenge is that the next-generation sequencing (NGS) technologies yield massive high-dimensional data, where the number of microbiota \\( d \\) often far exceeds the sample size \\( n \\). Since \\( d \\) often exceeds \\( n \\), statistically the correlation matrix of the microbiota is singular (positive semi-definite matrix)\\(^{19}\\), unless a condition of sparsity is imposed. In simple terms, sparsity means that many pairwise correlations are zero. Thus, compositionality aside, due to the high dimensionality, it is well-known that the sample Pearson and Spearman correlation matrices provide biased estimates of the correlation matrix\\(^{20}\\). A host of approaches have been proposed to estimate the covariance matrices in high dimensions\\(^{21-29}\\). However, since the observed high dimensional microbiome data contain a large number of zeros and are compositional, problem of estimating the correlation matrices in the present setting further complicates. It is well-known that microbiome abundance table could contain as many as 90% zero entries\\(^{6,30}\\), therefore it is reasonable to assume that most taxa are not correlated or at best weakly correlated with each other. Thus, the sparsity assumption noted above is reasonable in the present context.\n\nThirdly, since microbiota have complex inter-dependencies between each other, not all inter-relationships are expected to be linear. Consider, for example, the relationship between *Ruminococcaceae* and *Staphylococcaceae* depicted in Supplementary Fig. 2, which is based on data obtained from the Norwegian Microbiome study (NoMIC)\\(^{31,32}\\). While, linear fit seems reasonable, the relationship appears to be very nonlinear. In more complex settings, nonlinear correlations among taxa within an ecosystem or across systems (e.g., gut and oral environments) are ubiquitous\\(^{33}\\). Such nonlinear interactions among microbiota are known to influence microbial composition and host health\\(^{34,35}\\). However, standard concepts of correlation such as the Pearson or Spearman correlation coefficients are designed for quantifying linear relationships and not suitable for quantifying nonlinear relationships. Recent methods such as Sparse Correlations for Compositional data (SparCC)\\(^{14}\\), proportionality\\(^{15}\\), and Sparse Inverse Covariance Estimation for Ecological Association Inference (SPIEC-EASI)\\(^{16}\\) were developed for computing compositional correlations. However, they too are designed for quantifying linear relationships and may not be suitable for nonlinear relationships. For instance, in the example shown in Fig. 1, the relationship between T2 and T4 is parabolic, and the correlation coefficient provided by SparCC is zero (Fig. 1d), suggesting no linear relationship. Researchers often misconstrue that two taxa are independent if correlation coefficients such as the above are zero. It is also important to note that although SparCC is designed for quantifying linear relationships in compositional data, it may falsely declare linear relationship when two taxa are truly uncorrelated in the ecosystem. For example, taxa T3 and T4 are uncorrelated in the ecosystem (Fig. 1), and yet, SparCC resulted in a significant non-zero correlation coefficient (Fig. 1d).\n\nTo quantify nonlinear correlations between a pair of variables, the concept of distance correlation was introduced in the literature for the Euclidean space data\\(^{36}\\). The difference between distance correlation and Pearson/Spearman correlations is illustrated in Supplementary Fig. 3. All three measures (Pearson, Spearman, and distance correlations) detected the relationship between \\( x \\) and \\( y \\) with a correlation coefficient of 1 when the two random variables are linearly correlated. However, when \\( x \\) and \\( y \\) are nonlinearly related, e.g., \\( y = (x - 5)^2 \\), the Pearson and Spearman correlations were both 0, whereas the distance correlation was \\( \\sim 0.5 \\). It is important to note that a value of zero distance correlation implies statistical independence between two variables whereas a zero Pearson or Spearman or SparCC correlation coefficients only implies lack of linear relationship.\n\nLastly, correlation coefficient methods for compositional data such as SparCC, proportionality\\(^{15}\\), and SPIEC-EASI\\(^{16}\\) are scale invariant for computing correlations between taxa within a single ecosystem. Note that a function \\( f \\) is scale invariant if \\( f(ax) = f(x) \\) for every \\( x \\in \\mathbb{S}^d \\) and for every \\( a > 0 \\), where \\( \\mathbb{S}^d = \\{ \\vec{x} = [x_1, \\ldots, x_d] | x_i > 0, i = 1, \\ldots, d; \\sum_{i=1}^d x_i = \\kappa \\} \\) is a simplex\\(^{37}\\). However, these methods are not scale invariant when computing correlations between taxa across two or more ecosystems.\n\nMotivated by the above limitations of the existing methods, in this article we introduce a new methodology called Sparse Estimation of Correlations among Microbiomes (SECOM) which provides two measures of correlations between a pair of taxa, one for linear relationships and the other for nonlinear relationships using the concept of distance correlations. As can be seen in Fig. 1e, SECOM is useful for quantifying linear as well as nonlinear relationships. In the Methods section of the paper we provide guidance on how to use these measures when describing dependencies between a pair of taxa. The proposed methodology is statistically rigorous and accounts for compositionality and differential sequencing efficiencies by explicitly estimating library-specific sampling fraction\\(^{6,7}\\) and taxon-specific sequencing efficiency\\(^{38,39}\\). The resulting observed counts, corrected for two sources of biases will be called \"bias corrected\" counts which can be used for drawing inferences on the abundance of taxa in a unit volume of an ecosystem\\(^{6,7}\\). Furthermore, as can be seen from the p-value distribution provided in Supplementary Fig. 1b, unlike the existing methods, SECOM does not suffer from inflated false correlations between taxa.\n\nThe performance of SECOM is evaluated using a variety of simulations studies. The results are described in the Results section of this paper. The statistical details are provided in the Methods section of the paper. In addition to results based on synthetic data, we also illustrate SECOM using the infant gut microbiome data from the Norwegian Microbiome study (NoMIC). All theoretical proofs are provided in the Supplementary Notes.\nResults\n\nPerformance of SECOM using simulated data\nUsing simulated data, in this section we compare the performance of SECOM with some existing methods, namely, proportionality\\(^{15}\\), SparCC\\(^{14}\\), SPIEC-EASI\\(^{16}\\), and standard Pearson correlation coefficient. All details regarding the simulation study design are provided in the Supplementary Notes.\n\nWe begin by comparing CPU run times of various methods for computing correlation matrices using a simulated data set consisting of 200 taxa and 100 samples. All comparisons are made using RStudio with 1 CPU, x86\\_64-w64-mingw32/x64 (64-bit) and Windows 10 x64 (build 18363). Results are summarized in Supplementary Table 1. On average, SPIEC-EASI using either network inference method (MB or GL) took nearly hundred times more CPU time than other approaches, while SECOM was competitive with other compositional methods, such as SparCC and Proportionality.\n\nNext we compare the performance of SECOM with other methods for estimating the correlation matrix. We use the following average relative norm loss as the criterion for evaluating the performance of a method:\n\n\\[\n\\mathbb{E} \\left\\{ \\frac{\\| \\hat{R} - R^0 \\|_*}{\\| R^0 \\|_*} \\right\\}.\n\\]\n\nWe use the two commonly used matrix norms \\( \\| \\|_* \\), namely, Frobenius norm (\\( \\|A\\|_F = (\\sum_{ij} a_{ij}^2)^{1/2} \\)) and spectral norm (\\( \\|A\\|_\\infty = \\lambda_{\\max}(A) \\), which is the largest singular value of \\( A \\)). Additionally, we also evaluated the performance of the various methods in their ability to discover true non-zero correlations, defined as the true positive rate (TPR), and falsely declaring non-zero correlations when the correlations are truly zero, defined as false positive rate (FPR). Thus, estimated TPR and FPR are as defined below:\n\n\\[\n\\text{TPR} = \\frac{\\#\\{(l,m): \\hat{\\rho}_{lm} \\neq 0, \\rho^0_{lm} \\neq 0\\}}{\\#\\{(l,m): \\rho^0_{lm} \\neq 0\\}},\n\\]\n\\[\n\\text{FPR} = \\frac{\\#\\{(l,m): \\hat{\\rho}_{lm} \\neq 0, \\rho^0_{lm} = 0\\}}{\\#\\{(l,m): \\rho^0_{lm} = 0\\}},\n\\]\n\nwhere \\( R^0 = [\\rho^0_{lm}]_{l,m=1,\\ldots,d}, \\hat{R} = [\\hat{\\rho}_{lm}]_{l,m=1,\\ldots,d} \\).\n\nSimulation studies are based based on three different scenarios of ecosystems, namely, (1) an ecosystem where some taxa are linearly correlated and the rest uncorrelated, (2) an ecosystem where some taxa are nonlinearly correlated and the rest are uncorrelated, and (3) two ecosystems where some taxa are linearly correlated between ecosystems and the rest (either within each ecosystem or between ecosystems) are uncorrelated. Sparse correlation matrix obtained from SECOM is either by a data-driven thresholding approach (denote it as \"SECOM (Thresholding)\") or by p-value filtering (denote it as \"SECOM (Filtering)\").\n\nLinear correlations. Fig. 2 summarizes the results using different approaches to estimate the correlation matrix under different sample size/taxon number/dispersion combinations (\\( n/d/\\alpha \\)). As expected, under both norms, all compositional methods had uniformly smaller average relative norm loss than the standard Pearson correlation coefficient (Fig. 2a). For example, with 100 samples, 200 taxa, and the dispersion parameter equals to 0.5, the standard Pearson correlation coefficient had approximately 9 times higher average loss under both norms in comparison to SECOM (Frobenius: 9 vs. 1; Spectral: 45 vs. 5). The SparCC method had the second largest average loss especially when there is greater variability in the underlying true abundances (overdispersion parameter \\( \\alpha = 2 \\), Fig. 2a). Both versions of SECOM, namely, Thresholding and Filtering, together with proportionality and both SPIEC-EASI methods outperformed other methods in terms of average loss (Fig. 2a). In addition to the estimation accuracy, SECOM (Thresholding and Filtering) and SPIEC-EASI (MB and GL) also performed well in recovering the sparsity pattern (Fig. 2b). They not only outperformed other methods substantially in controlling FPR, but they competed well in terms of TPR. However, as mentioned above, SPIEC-EASI is substantially more computationally intensive than SECOM. Under this simulation setting, SPIEC-EASI required a CPU time of 76.15 hours in comparison to 1.2 CPU hours for SECOM. Both SparCC and standard Pearson correlation coefficients achieved high TPR in this simulation study but were subject to very high FPR as compared to SECOM and SPIEC-EASI. Note that the FPR of standard Pearson correlation can be as large as 80%, which could make most discoveries meaningless and even misleading. Although proportionality performed well in terms of FPR, it has very small TPR when there are larger variations in taxa abundance. For example, when the underlying true dispersion parameter increased to 2, the TPR of proportionality method dramatically reduced to almost 0. It is also worth noting that for a fixed dispersion parameter, as the sample size \\( n \\) and the number of taxa \\( d \\) increased, there is an increase in TPR together with a decrease in FPR for both SECOM methods. This is consistent with the concentration results described in Theorem 0.1.\nNonlinear correlations. We also performed a simulation study comparing the performance of various methods in identifying nonlinear relationships. The settings were similar to the simulation study conducted for linear correlations described above, except that each taxon was set to be quadratically correlated with its adjacent taxon among the first 50 taxa. Since, with the exception of SECOM, none of the existing methods are designed to measure nonlinear relationships, we only compared these methods in their ability to recover sparsity. We implemented SECOM with p-value filtering strategy (i.e., SECOM (Filtering)) but did not implement the data-driven thresholding strategy (i.e., SECOM (Thresholding)) because it involves a step of data splitting to divide data into training and test sets, which requires much larger sample size when it comes to the detection nonlinear relationships. The sparsity strategies for SparCC and proportionality, and the tuning parameters for SPIEC-EASI used in this simulation set-up are same as those used for linear case mentioned earlier. As expected, none of the competing methods identify nonlinear relationship (Fig. 3). They all have TPRs approximately 0. Although standard Pearson correlation coefficient achieves a TPR at around 50%, but its FPR was sometimes even higher, leading to misleading discoveries when detecting complex microbial inter-relationships. With the adoption of distance correlation concept, SECOM successfully achieved almost perfect TPR (100%), and also had significantly smaller FPR than existing methods.\n\nMultiple ecosystems. In addition to quantifying correlations between taxa in a single homogeneous ecosystem, we also compared SECOM with existing methods in quantifying microbial correlations across two ecosystems. Specifically, a simulation study was conducted by generating count tables from two ecosystems with different sampling fractions and sequencing efficiencies in each simulation run. The first 50 taxa in the first ecosystem were linearly correlated with the corresponding taxa in the second ecosystem. Rest of the taxa are uncorrelated within or between ecosystems. Details of the study design are provided in the Supplementary Notes. For all the methods, we used the same methodology as described in the other simulation studies mentioned above. As seen in Fig. 4, SECOM methods outperformed all competitors in terms of both estimation accuracy (the smallest average relative Frobenius/Spectral norm loss) and sparsity recovery (the smallest FPR and the highest TPR). In general, SECOM (Thresholding) had the most precise correlation estimate, the smallest FPR, and comparable TPR as SECOM (Filtering). Both SECOM methods achieve almost perfect TPR (~ 100%) while SECOM (Filtering) performed slightly better. On the contrary, standard Pearson correlation coefficients together with existing compositional techniques either suffered from loss of TPR, or inflated FPR, making them unsuitable for detecting microbial inter-relationships across ecosystems.\n\nAs a summary of simulation studies, SECOM performed consistently well regardless of whether correlations are linear or nonlinear. The thresholding version of SECOM is entirely data-driven and is theoretically proved to be a consistent estimator of the true correlation matrix in the Frobenius norm (Theorem 0.3 in the Methods section). However, since the thresholding method requires splitting data into training and test sets, it generally needs a larger sample size especially when it comes to the detection of nonlinear relationships. On the other hand, the filtering version of SECOM screens the estimates of correlation coefficients based on their p-values. Correlation coefficients with statistically non-significant p-values are discarded to achieve sparsity. The filtering method requires smaller sample size than thresholding method as there is no data splitting step. However, the determination of significance level is heuristic since controlling the type I error is not the primary purpose of SECOM. For example, setting the significance level \\( \\alpha = 0.05 \\) does not mean the overall type I error rate (or family-wise error rate (FWER), or false discovery rate (FDR) if the multiple comparison correction is implemented) is controlled at 5%, especially for the detection of nonlinear relationships. It should simply be viewed as a filtering mechanism to achieve sparsity. For simplicity of exposition, we only implemented SECOM (Filtering) in the following Illustration section.\n\nIllustration: Norwegian infant gut microbiome data\nWe illustrate SECOM using the data obtained from the Norwegian Microbiome study (NoMIC)\\(^{31,32}\\). The prospective NoMIC study was established to study the development of infant gut microbiota and its relation to health outcomes. Mothers were recruited from the maternity ward at a county hospital in south-eastern Norway from 2002 to 2005. Stool samples were obtained at days 30, 120 and 365 after birth. Samples were retrieved from the mothers and kept frozen at -20°C until DNA was extracted by an automated procedure and amplified by PCR reactions using 16S rRNA specific primers. The V4 region of the 16S rRNA gene was then sequenced using Illumina HiSeq. Details on the study population have been reported previously\\(^{31,32}\\). Written informed consent was obtained from the mothers prior to enrolment. The study was approved by the Norwegian Data Inspectorate, and the Norwegian Regional Committee for Medical and Health Research Ethics. In this illustration we restricted to children who were vaginally delivered with no perinatal antibiotics exposure and all exclusively breastfed during the first four months of life. We chose to study the correlations at 30, 120, and 365 days as they represent different feeding patterns, which resulted in 46, 44, and 34 sequenced samples, respectively. As an infant grows from infancy to toddler stage, their environment changes dramatically due to changes in diet (from breastfeeding to solid foods), external contacts, environment, and activities. These changes necessarily impact their gut microbiota and likely contributes to normal growth and development of a baby\\(^{40,41}\\). We focused on analyzing data at the family level. The prevalence for each family is provided in Supplementary Table 2.\n\nBar graphs of temporal changes in the bias corrected counts and relative abundances of top ten prominent families are\nprovided in Fig. 5. Similar plots at the phylum level are provided in the Supplementary Fig. 4. Since all babies are breastfed during the first 30 days after birth and are in constant maternal contact, consistent with literature, we found greater relative abundance of the phylum Actinobacteria, specifically the family Bifidobacteriaceae (55%), along with families of Firmicutes, such as Clostridiaceae (10%), Lachnospiraceae (1%), Ruminococcaceae (9%), and opportunistic Staphylococcaceae (1%). Since these babies were born vaginally, we also see some Bacteroidaceae (6%) during the first 30 days. We also found pro-inflammatory bacterial families Enterobacteriaceae (9%) and Pasteurellaceae (2%), in the phylum Proteobacteria in the 30-day old babies. As the baby’s environment and activities begin to change, in particular transitioning from breastfeeding to other foods, we begin to notice changes in the microbial compositions in our cohort of babies. As one would expect the relative abundance of Bifidobacteriaceae, which is largely due to breastfeeding, temporally decreases by the end of the first year (55%, 35%, 5% at Day 30, 120, 365, respectively). We also notice changes in the relative abundance of Clostridiaceae (10%, 30%, 3% at Day 30, 120, 365, respectively). The relative abundance of Enterobacteriaceae was generally constant throughout the first year (9%, 9%, 6% at Day 30, 120, 365, respectively). As babies begin to crawl, touch various objects and are in contact with other people or environment, one would expect several new families to colonize the gut by Day 365. For example, we see the arrival of Moraxellaceae (1%) in the gut at Day 365 and numerous other families which are grouped as “Others” (68%).\n\nTo the best of our knowledge, this is the first paper to characterize correlations among different families of bacteria during the first year of development of a baby. The correlations (linear and nonlinear) among the top 10 prevalent families are summarized in Fig. 6. To deal with sparsity, we filtered all correlations that were below 0.1 and p-value exceeding 0.1 by setting them to zero. If the estimated linear as well as distance correlations are non-zero, then it suggests a potential linear or nonlinear association between the two microbes. If the estimated linear correlation is zero but the distance correlation is different from zero then it suggests a nonlinear relationship between the pair of taxa. However, due to power, sometimes a linear correlation is significantly different from zero even though the nonlinear correlation is not significantly different from zero.\n\nDuring the first 30 days of birth, important families of bacteria that promote baby’s health begin to colonize the gut with little or no interactions among themselves. However, we see significant negative linear correlations between Enterobacteriaceae and Bifidobacteriaceae (linear correlation -0.44, distance correlation 0.44) and between Enterobacteriaceae and Bacteroidaceae (linear correlation -0.61, distance correlation 0.61). As noted above, Day 120 is a critical transition age when the gut microbial diversity increases as new taxa arrive in the gut. Consequently, we hypothesize that inter-relationships among the gut microbiota changes from how they were at Day 30. We discovered strong negative linear relationships between the pathogenic family Enterobacteriaceae several important commensal families such as Lachnospiraceae (linear correlation -0.89, distance correlation 0.92), Clostridiaceae (linear correlation -0.75, distance correlation 0.73) and Ruminococcaceae (linear correlation 0, distance correlation 0.51). We also saw negative correlation between Bifidobacteriaceae and Clostridiaceae (linear correlation -0.49, distance correlation 0). By Day 365, an infant’s physical activity, diet and environment would substantially change and hence many new families start colonizing the gut and developing complex interactions among them. Again, we see Lachnospiraceae increase interactions with other microbes with age. At Day 365, as the (bias corrected) abundance of phylum Actinobacteria decreases (Supplementary Fig. 4) in particular as the abundance of Bifidobacteriaceae decreases, Lachnospiraceae begins to increase (Fig. 5a) and the two families are linearly negatively correlated with a correlation coefficient of -0.45 (distance correlation 0.5). Lachnospiraceae is also negatively correlated with Enterobacteriaceae with a linear correlation of -0.37 (distance correlation 0.42), and with opportunistic family Staphylococcaceae, with a linear correlation of -0.74 (distance correlation 0.78). Lachnospiraceae is also nonlinearly correlated with another important gut microbiota Ruminococcaceae, with a distance correlation of 0.42. Similar to Lachnospiraceae, the Ruminococcaceae family is also found to be negatively correlated with the pathogen Enterobacteriaceae with a linear correlation of -0.42 (distance correlation 0.45) and also negative correlated with opportunistic family Staphylococcaceae with a linear correlation coefficient of -0.56 (distance correlation coefficient of 0.62). Not surprisingly, Ruminococcaceae family is positively linearly correlated with Bacteroidaceae with a correlation of 0.34 (distance correlation 0.37). We see nonlinear relationship between Ruminococcaceae and Bifidobacteriaceae with a distance correlation 0.36. We also find a nonlinear relationship between Bifidobacteriaceae and opportunistic family Staphylococcaceae with a distance correlation 0.56. A nonlinear relationship was seen between Bacteroidaceae and Pasteurellaceae with a distance correlation of 0.56. A positive correlation between Enterobacteriaceae and Clostridiaceae of 0.36 was seen (distance correlation 0.39). Thus, in most cases we notice that the distance and linear correlation seem to track each other. However, there are instances where the relationships appear to be nonlinear with a zero linear correlations.\n\nIn summary, we find that starting Day 120, Lachnospiraceae and Ruminococcaceae to be interactive with several families during the first year of a baby’s growth and development. These two families play an important role in degrading complex polysaccharides to short-chain fatty acids such as acetic, butyric, and propionic acid, which have numerous biochemical functions[42]. Thus, it is not surprising that during the development of a baby, these families interact with many other families of bacteria to achieve a balance in the gut ecology, especially as the baby begins to ingest more complex foods beyond breast milk. Not surprisingly, during the early days of gut colonization (Day 30 and Day 120), important families that promote infants’\nhealth, such as Bifidobacteriaceae, Bacteroidiceae, Lachnospiraceae, and Clostridiaceae, are all negatively correlated with Enterobacteriaceae, a family of bacteria that contains many familiar pathogens, such as Salmonella, Shigella and Escherichia coli.\n\nIt is important to note that microbial ecology is very complex and dynamic and hence it is not reasonable to expect very high correlation coefficients. This is because, a family of bacteria consists of numerous genera and many species within a genus. Thus, relationships between a pair of families could be affected by complex inter-relationships between species or even strains of bacteria. The description provided in this paper should be viewed as proof of concept of the methodology. Should a researcher be interested in drilling down the correlations at a lower level of the phylogenetic tree, then larger sample sizes would be necessary.\n\nDiscussion\n\nHumans have co-evolved with microorganisms since the beginning of time. A symbiosis exists whereby functions performed by the human microbiome did not need to be established by the human host. However, modern lifestyle has severely depleted the commensal microbiomes in the human host, whereby many functions humans rely on, have been lost. This conveys a risk of lower well-being and disease. However, it also offers an opportunity for prevention and treatment of diseases if we were to replenish the gut microbiome back to an optimal state. This prospect offers great promise, yet has to be based on knowledge of what constitutes an optimal gut microbial ecosystem, of which we yet possess limited knowledge. Moreover, replenishing the ecosystem is not straightforward as introducing new microbes will affect microbes already present, thus we need to learn more about how microbes and microbial groups are correlated. Additionally, correlations are likely different in an ecosystem of ancestral microbes in contrast to an ecosystem disrupted by medical interventions. Thus, we chose to study correlations in a selected subset of infants who had not been subjected to medical interventions such as cesarean delivery and perinatal antibiotics, know to profoundly disrupt the microbiome for a prolonged period and with long term effects on health.\n\nUnderstanding interactions among microbes is a challenging scientific problem. It is further complicated by the statistical challenges due to the compositional structure in the data. Traditional methods to describe correlations, such as Pearson and Spearman correlation coefficients are not valid. Further, as demonstrated in this paper, relationships between a pair of microbes is not always linear as there exist complex interactions among them. Unfortunately, Pearson and Spearman correlation coefficients are measures of linear associations and may not be suitable to describe nonlinear relationships. This paper introduces a measure of linear as well as nonlinear relationship between a pair of microbes. The resulting methodology is called Sparse Estimation of Correlations for Microbiomes (SECOM). The new methodology overcomes the various challenges experienced with microbiome data.\n\nApplication of SECOM to an infant gut microbiome data set obtained from the NoMIC study, lets us discover interesting temporal patterns in correlations between a pair of taxa. Correlations among various microbes evolves with the development of a baby. During the early days of life (30 days from birth), new microbes are continuously colonizing the gut. Four months after birth is a critical window in an infant’s growth and development when many babies begin are weaned from breast milk to solid foods. In response, the gut at this age undergoes microbial changes and accordingly the correlations among microbiota evolve with age. By the time an infant is about one year old, the infant gut matures with the inclusion of many new microbial families. Accordingly, the gut undergoes further transformation and many new relationships among bacteria are formed. For the first time in the literature, we discover linear and nonlinear relationships among various families. By investigating the group of babies who were vaginally born, breastfed for the first four months of life and not exposed to antibiotics during this time, we develop a baseline understanding of naturally occurring correlations among various families. In the future, we would be interested in understanding how these relationships are modified when there has been clinical interventions such as C-section and the use of antibiotics, which are becoming popular in the modern societies around the world. Subsequently, we will also be interested in investigating the effects of these associations on various health outcomes among infants. A limitation of the present study is that due to the small sample size, we may have missed some significant correlations.\n\nMethods\n\nDescription of some existing methods\n\nProportionality The \\( \\phi \\) statistic was proposed to describe the strength of proportionality between two variables, which is closely related but not identical to correlation coefficient. Instead, it is a \"goodness-of-fit to proportionality\" statistic to assess the extent to which a pair of random variables are proportional\\(^{15}\\). \\( \\phi = 0 \\) indicates two random variables are exactly proportional (e.g. \\( y = ax \\)); on the other hand, \\( \\phi \\neq 0 \\) as long as two random variables are not exactly proportional, even if they are perfectly linearly correlated (e.g. \\( y = ax + b \\)). Additionally, unlike the standard concept of correlation coefficients, it is hard to interpret \\( \\phi \\) values as it lacks a scale. For instance, \\( \\phi = 0.1 \\) does not imply how strong two random variables are related to each other without considering all \\( \\phi \\) statistics. If all \\( \\phi \\) statistics range from 0 to 1, \\( \\phi = 0.1 \\) could indicate a strong proportionality; while if\nall \\( \\phi \\) statistics range from 0 to 0.1, \\( \\phi = 0.1 \\) could otherwise represent a weak proportionality. Also, \\( \\phi \\) statistics is not symmetric (\\( \\phi(x, y) \\neq \\phi(y, x) \\)), making it inappropriate to serve as a dissimilarity measure for downstream analyses such as ordination or clustering analysis. Lastly, there is no clear criterion to produce a sparse matrix based on \\( \\phi \\) statistics.\n\nSparse Correlations for Composition Data (SparCC)\\(^{14}\\) It is designed to estimate the correlation coefficients for log-transformed abundances while addressing bias due to compositionality in the data. It assumes that (1) the number of taxa is large, and (2) the underlying true correlation matrix is sparse. However, similar to proportionality method, it is not a statistically rigorous approach to obtain a sparse correlation matrix for SparCC. An arbitrary cutoff of \\( r = 0.3 \\) was suggested in\\(^{14}\\) to declare if a pair of taxa are correlated or not.\n\nSparse Inverse Covariance Estimation for Ecological Association Inference (SPIEC-EASI\\(^{16}\\)) It is a measure of association that exploits the concept of conditional independence and graphical models. Two taxa are conditionally independent if given the abundances of all other taxa, neither taxon provides additional information about the abundance of the other. Otherwise, these taxa are not conditionally independent and there is a linear relationship between them as the method is essentially estimating the inverse covariance matrix (precision matrix). While conceptually it is a useful measure, as one would expect, SPIEC-EASI is computationally very intensive compared to the above existing methods.\n\nSECOM model set-up\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
TermDefinition
iSample, \\( i = 1, \\ldots, n \\).
jTaxon, \\( j = 1, \\ldots, d \\).
\\( A_{ij} \\)The absolute abundance in the ecosystem for taxon \\( j \\) in sample \\( i \\).
\\( O_{ij} \\)The observed abundance for taxon \\( j \\) in sample \\( i \\).
\\( S_i \\)Sample-specific sampling fraction.
\\( C_j \\)Taxon-specific sampling efficiency.
\\( E_{ij} \\)Random error for taxon \\( j \\) in sample \\( i \\).
\\( a_{ij} \\)\\( \\log A_{ij} \\).
\\( o_{ij} \\)\\( \\log O_{ij} \\).
\\( s_i \\)Sample-specific sampling fraction in log scale.
\\( c_j \\)Taxon-specific sequencing efficiency in log scale.
\\( e_{ij} \\)Random error for taxon \\( j \\) in sample \\( i \\) in log scale.
\n\nTable 1. Definitions of key notations\n\nThe absolute abundances \\( A_{ij} \\) in the ecosystem are non-negative. Let \\( \\mathcal{T} \\) be the set of all possible configurations of presence or absence of a taxon, then\n\n\\[\n\\mathcal{T} = \\left\\{ (1, 1, \\ldots, 1), \\right. \\\\\n\\left. (0, 1, \\ldots, 1), \\ldots, (1, 1, \\ldots, 0) \\right. \\\\\n\\vdots \\\\\n\\left. (0, 0, \\ldots, 1), \\ldots, (1, 0, \\ldots, 0) \\right\\}\n\\]\n\nwhere 0 and 1 correspond to the cases where a taxon is missing (zero) or present in a sample, respectively. We represent each event in \\( \\mathcal{T} \\) by \\( T \\) and it is indexed by \\( t = 1, \\ldots, 2^d - 1 \\). For example, \\( T_1 \\) corresponds to the case where all taxa are present in a sample, and \\( T_{2^{d-1}} \\) is the case where only the first taxon is present, and all remaining taxa are zeros.\n\nWe further assume that for each sample, the pattern of taxon presence is generated by independent r.v. \\( M_{ij}, 1 \\leq i \\leq n, 1 \\leq j \\leq d \\) such that\n\n\\[\nP(M_{i} = T_t) = \\delta_t^j, 0 \\leq \\delta_t^j \\leq 1,\n\\]\n\nwhere \\( M_i = (M_{i1}, \\ldots, M_{id})^T \\).\n\nWe propose that the observed abundance is generated by the following multiplicative model:\n\n\\[\nO_{ij} = S_i C_j A_{ij} E_{ij}.\n\\]\nFor \\( A_{ij} \\) with \\( M_{ij} = 1 \\), i.e., for the non-zero absolute abundance, perform the log transformation, the above multiplicative model can be transformed into an additive model,\n\n\\[\no_{ij} = s_i + c_j + a_{ij} + e_{ij}.\n\\]\n\nAssume that conditional on \\( M_i = 1 \\), the absolute abundance has finite second moment:\n\n\\[\nE(a_{ij}) = \\alpha_j, Var(a_{ij}) = \\sigma^0_{jj}.\n\\]\n\nAdditionally, we assume that:\n\n\\( s_i \\) is a sample-specific constant,\n\\( c_j \\) is a taxon-specific constant,\n\\( e_{ij} \\sim i.i.d.\\ F_e \\) with \\( E(e_{ij}) = 0, Var(e_{ij}) = \\sigma^2_e \\),\n\\( a_{ij} \\perp \\perp e_{ij} \\).\n\nWe define two concepts of correlation coefficients in this section. One quantifies the strength of linear relationship between a pair of taxa by modifying Pearson and Spearman correlation coefficients for sparse high-dimensional compositional data. The second quantifies the strength of nonlinear relationship between a pair of taxa by modifying distance correlation coefficient. We provide both measures.\n\nRemark 1. Since distance correlation coefficient is a measure of nonlinear relationship between a pair of taxa, it does not have a sign and is always non-negative. On the other hand, the measure of linear correlation coefficient described below can take positive or negative values depending upon whether they are positively or negatively linearly correlated.\n\nRemark 2. A distance correlation coefficient of zero between two taxa implies that the taxa are independent. It is well-known that if Pearson or Spearman correlation coefficients between two taxa is zero then it only suggests a lack of linear relationship but not independence.\n\nRemark 3. Our proposed SECOM methodology outputs both linear as well as distance correlation coefficients between pairs of taxa. If the relationship between a pair is nonlinear then we expect the distance correlation between the two taxa to be nonzero whereas the linear correlation could be zero. On the other hand if the relationship is linear then the linear correlation coefficient is expected to be nonzero and sign of the coefficient is positive or negative depending upon whether the two taxa are positively or negatively associated. When the linear correlation coefficient is nonzero then we expect the distance correlation coefficient also to be nonzero. This is because linear correlation coefficient is a special case of nonlinear correlation coefficient. In such cases, we recommend the user to use the value provided by the linear correlation coefficient. However, there may be situations where the estimated linear correlation is nonzero but the distance correlation is zero. This can happen due sample size and power issues and the sparsity constraints. In such cases again we recommend the researcher to use linear correlation coefficient value.\n\nEstimation of linear correlation coefficients\nIn this section we develop methodology for estimating linear correlation coefficient between the abundances of pairs of taxa \\( l \\) and \\( m, 1 \\leq l,m \\leq d \\), while noting that for each subject \\( i \\), the abundances \\( a_{il} \\) and \\( a_{im} \\) are not observable. The only observable values are the observed counts, e.g. OTUs, \\( o_{il} \\) and \\( o_{im} \\). According to our hypothesized model, the actual abundance \\( a_{ij} \\) of the \\( j^{th} \\) taxon in a unit volume of the specimen from the \\( i^{th} \\) subject, in expectation, is a function of observed counts \\( o_{ij} \\), and unknown nuisance parameters \\( s_i \\) and \\( c_j \\). Therefore, to obtain an approximate unbiased estimator of \\( a_{ij} \\) using the observable \\( o_{ij} \\), we need to estimate and nuisance parameters \\( s_i \\) and \\( c_j \\) and eliminate the bias introduced by them. Once that is done, we can define a Pearson or Spearman correlations using the modified observed counts \\( o_{ij} \\) to derived bias-corrected estimates of the true correlation coefficient between the abundance of a pair of taxa. In the following we now describe the methodology to eliminate the nuisance parameters \\( s_i \\) and \\( c_j \\).\n\nDenote the covariance matrix of \\( a_{ij} \\) as \\( \\Sigma^0 = [\\sigma^0_{lm}]_{l,m=1,\\ldots,d} \\), and the Pearson correlation coefficient matrix as \\( R^0 = [\\rho^0_{lm}]_{l,m=1,\\ldots,d} \\). We make the following sparsity assumption regarding the covariance matrix.\n\nAssumption 0.1 (Approximately sparse covariance matrices).\n\n\\[\n\\mathcal{U}(K) = \\{ \\Sigma : \\sigma_{jj} < K, \\frac{1}{d^2} \\sum_{l \\neq m} \\sigma_{lm} = o(1) \\}.\n\\]\nTwo examples of matrices which satisfy this condition are (1) a d-diagonal matrix, and (2) the AR(1) covariance matrix.\n\nFrom (2), (3), (4), and (5), by centering the data suitably, we eliminate the effect of taxon-specific sampling efficiency \\( c_j \\) as follows:\n\n\\[\no_{ij} - \\bar{o}_j = (s_i - \\bar{s}_.) + (a_{ij} - \\bar{a}_j) + (e_{ij} - \\bar{e}_j) = \\textcircled{1} + \\textcircled{2} + \\textcircled{3},\n\\]\n\nwhere, for the \\( j^{th} \\) taxon and \\( i = 1, 2, ..., n \\), \\( \\bar{s}_. = \\frac{1}{n} \\sum_{i=1}^n s_i \\), \\( \\bar{a}_j = \\frac{1}{n} \\sum_{i=1}^n a_{ij} \\), \\( \\bar{e}_j = \\frac{1}{n} \\sum_{i=1}^n e_{ij} \\). Note that:\n\n(1) We call \\( \\textcircled{1} \\) the \"sampling fraction difference\", which is a sample-specific bias term,\n\n(2) For \\( \\textcircled{2} \\): \\( E(a_{ij} - \\bar{a}_j) = 0, Var(a_{ij} - \\bar{a}_j) = (1 - \\frac{1}{n}) \\sigma_{jj}^0 \\),\n\n(3) For \\( \\textcircled{3} \\): \\( E(e_{ij} - \\bar{e}_j) = 0, Var(e_{ij} - \\bar{e}_j) = (1 - \\frac{1}{n}) \\sigma_e^2 \\).\n\nDefine the set of non-zero taxa in sample \\( i \\) by \\( d(i) = \\{ j : M_{ij} = 1, 1 \\leq j \\leq d \\} \\). Then by on Assumption 0.1, we have\n\n\\[\n\\frac{1}{|d(i)|} \\sum_{j \\in d(i)} \\left\\{ (o_{ij} - \\bar{o}_j) - \\textcircled{1} \\right\\} = \\frac{1}{|d(i)|} \\sum_{j \\in d(i)} \\textcircled{2} + \\frac{1}{|d(i)|} \\sum_{j \\in d(i)} \\textcircled{3} \\longrightarrow_p 0 \\text{ as } |d(i)| \\to \\infty.\n\\] (6)\n\nTherefore, a quick and simple estimator of the sampling fraction difference is the arithmetic mean of the difference between observed abundances, i.e. \\( \\textcircled{1} = \\bar{s}_i - \\bar{s}_. = \\frac{1}{|d(i)|} \\sum_{j \\in d(i)} (o_{ij} - \\bar{o}_j) \\). Taking into account the variance of residuals \\( o_{ij} - \\bar{o}_j \\), a weighted average is proposed as follows:\n\n\\[\n\\textcircled{1} = \\bar{s}_i - \\bar{s}_. = \\sum_{j \\in d(i)} w_j (o_{ij} - \\bar{o}_j),\n\\] (7)\n\nwhere \\( w_j = \\frac{1}{Var(o_{ij} - \\bar{o}_j)} / \\sum_{l \\in d(i)} \\frac{1}{Var(o_{lj} - \\bar{o}_l)} \\).\n\nDenote the centered absolute abundance by \\( x_{ij} = a_{ij} - \\bar{a}_j, 1 \\leq i \\leq n, 1 \\leq j \\leq d \\). Then\n\n\\[\nCov(x_{il}, x_{im}) = (1 - \\frac{1}{n}) \\sigma_{lm}^0, \\quad Var(x_{ij}) = (1 - \\frac{1}{n}) \\sigma_{jj}^0, \\quad Corr(x_{il}, x_{im}) = \\rho_{lm}^0.\n\\]\n\nSimilarly, define the centered absolute abundance with noise by\n\n\\[\ny_{ij} := (a_{ij} - \\bar{a}_j) + (e_{ij} - \\bar{e}_j) = x_{ij} + (e_{ij} - \\bar{e}_j) = (o_{ij} - \\bar{o}_j) - (s_i - \\bar{s}_.),\n\\]\n\nand denote \\( Cov(y_{il}, y_{im}) := \\sigma_{lm}, Corr(y_{il}, y_{im}) := \\rho_{lm}, \\Sigma = [\\sigma_{lm}]_{l,m=1,...,d}, R = [\\rho_{lm}]_{l,m=1,...,d} \\). Then the off diagonal and diagonal elements of \\( \\Sigma \\) are, respectively,\n\n\\[\n\\sigma_{lm} = (1 - \\frac{1}{n}) \\sigma_{lm}^0, \\quad \\sigma_{ll} = (1 - \\frac{1}{n})(\\sigma_{ll}^0 + \\sigma_e^2).\n\\]\n\nWe make the following assumption that noise to signal ratio is very small.\n\nAssumption 0.2 (Small noise-to-signal ratio).\n\n\\[\n\\sigma_e^2 \\ll \\sigma_{ll}^0.\n\\]\n\nThen we have:\n\n\\[\n\\rho_{lm} = \\frac{\\sigma_{lm}}{\\sqrt{\\sigma_{ll} \\sigma_{mm}}} = \\frac{\\sigma_{lm}^0}{\\sqrt{(\\sigma_{ll}^0 + \\sigma_e^2)(\\sigma_{mm}^0 + \\sigma_e^2)}} \\approx \\frac{\\sigma_{lm}^0}{\\sqrt{\\sigma_{ll}^0 \\sigma_{mm}^0}} = \\rho_{lm}^0,\n\\]\n\nwhich means the Pearson correlation coefficient among \\( y'_{ij}'s \\) provides a good approximation to the Pearson correlation coefficient among \\( x'_{ij}'s \\) as well as among \\( a'_{ij}'s \\). Since \\( y_{ij} = (o_{ij} - \\bar{o}_j) - (s_i - \\bar{s}_.) \\). From (7), we estimate \\( y_{ij} \\) by \\( \\hat{y}_{ij} = (o_{ij} - \\bar{o}_j) - \\bar{s}_i - \\bar{s}_. \\). Thus, from (6),\n\n\\[\n\\hat{y}_{ij} \\longrightarrow_p (o_{ij} - \\bar{o}_j) - (s_i - \\bar{s}_.) = y_{ij}, \\text{ as } |d(i)| \\to \\infty.\n\\] (8)\nIn the sequel, for all \\(1 \\leq l,m \\leq d\\), denote \\(n(l) = \\{i : M_{il} = 1, 1 \\leq i \\leq n\\}\\) and \\(n(l,m) = \\{i : M_{il} = M_{im} = 1, 1 \\leq i \\leq n\\}\\), where \\(n(l)\\) is the number of samples where \\(l^{th}\\) taxon is observed, and \\(n(l,m)\\) represents the number of samples where both \\(l^{th}\\) and \\(m^{th}\\) are observed. For each \\(1 \\leq l,m \\leq d\\), let\n\n\\[\n\\hat{\\mu}_l = \\frac{1}{|n(l)|} \\sum_{i \\in n(l)} \\hat{y}_{il},\n\\]\n\\[\n\\hat{\\sigma}_{lm} = \\frac{1}{|n(l,m)|} \\sum_{i \\in n(l,m)} (\\hat{y}_{il} - \\hat{\\mu}_l)(\\hat{y}_{im} - \\hat{\\mu}_m),\n\\]\n\\[\n\\Sigma_n = [\\hat{\\sigma}_{lm}]_{l,m=1,\\ldots,d},\n\\]\n\\[\nR_n = [\\hat{\\rho}_{lm}]_{l,m=1,\\ldots,d} = \\left[ \\frac{\\hat{\\sigma}_{lm}}{\\sqrt{\\hat{\\sigma}_{ll} \\hat{\\sigma}_{mm}}} \\right]_{l,m=1,\\ldots,d}.\n\\]\n\nTo prove the consistency of the proposed covariance estimator, we make the following mild Assumption 0.3 that each taxon (Assumption 0.3(i)) or each pair of taxa (Assumption 0.3(ii)) is present with a nonzero probability (\\(\\delta_{min}\\)).\n\n**Assumption 0.3 (Minimal probability). Define**\n\n\\[\nC_l(l) = \\{t : \\text{taxon } l \\text{ is present in } T_t \\text{ in } M_t, 1 \\leq t \\leq 2^d - 1\\},\n\\]\n\\[\nC_l(l,m) = \\{t : \\text{taxa } l \\text{ and } m \\text{ are present in } T_t \\text{ in } M_t, 1 \\leq t \\leq 2^d - 1\\}.\n\\]\n\n*There exists a constant \\(\\delta_{min} > 0\\) such that for any \\(1 \\leq l,m \\leq d\\),\n\n\\[(i) \\frac{1}{n} \\sum_{l=1}^n \\sum_{t \\in C_l(l)} \\delta_l^t = \\delta_l > \\delta_{min}, \\quad (ii) \\frac{1}{n} \\sum_{l=1}^n \\sum_{t \\in C_l(l,m)} \\delta_l^t = \\delta_{l,m} > \\delta_{min}.\\]*\n\n**Theorem 0.1.** *Suppose \\(\\Sigma^0\\) satisfies Assumption 0.1 and Assumption 0.3 is valid, then*\n\n\\[\n\\left\\| R_n - R \\right\\|_\\infty = O_p\\left( \\sqrt{\\frac{\\log d}{n}} \\right).\n\\]\n\nThus, the empirical correlation matrix \\(R_n\\) based on \\(\\hat{y}_{ij}'s\\) consistently estimates the correlation matrix \\(R\\) of \\(y_{ij}\\) in the *Sup* norm. Under the Assumption 0.2, \\(R\\) is a reasonable approximation to the true correlation matrix \\(R^0\\). The details of the proof are provided in the Supplementary Notes.\n\nInstead of Pearson correlation coefficient, if the Spearman correlation coefficient is of interest, then we convert \\(x_{ij}, y_{ij}, \\hat{y}_{ij}\\) into ranks \\(r_{ij}^0, r_{ij}, \\hat{r}_{ij}\\). Clearly, for \\(r_{ij}^0, r_{ij}, \\hat{r}_{ij} \\in \\{1,2,\\ldots,n\\}\\),\n\n\\[\n\\hat{r}_{ij} \\longrightarrow_p r_{ij}, \\text{ as } |d(i)| \\to \\infty,\n\\]\n\\[\nr_{ij} \\approx r_{ij}^0 \\text{ as long as Assumption 0.2 holds.}\n\\]\n\nWith a slight abuse of notations, denote \\(Corr(r_{il}, r_{im}) = s_{lm}\\), \\(Corr(\\hat{r}_{il}, \\hat{r}_{im}) = \\hat{s}_{lm}\\), \\(S = [s_{lm}]_{l,m=1,\\ldots,d}\\), \\(S_n = [\\hat{s}_{lm}]_{l,m=1,\\ldots,d}\\). Then we have the following result.\n\n**Theorem 0.2.** *Suppose \\(\\Sigma^0\\) satisfies Assumption 0.1 and Assumption 0.3 is true, then:*\n\n\\[\n\\left\\| S_n - S \\right\\|_\\infty = O_p\\left( \\sqrt{\\frac{\\log d}{n}} \\right).\n\\]\n\nThe proof of this result relies on the observation that standardized rank \\(\\zeta_{il} = \\frac{\\hat{r}_{il} - E(\\hat{r}_{il})}{\\sqrt{Var(\\hat{r}_{il})}}\\) is naturally bounded, which allows the applicability of the Hoeffding’s inequality. The details of the proof are deferred to the Supplementary Notes.\n\nWhen computing correlations of high-throughput sequencing data, it is reasonable to assume that only a small fraction of features (genes/proteins/taxa etc.) are correlated with each other, i.e. the correlation matrix is sparse. Inspired by the Sparse Estimation of the Correlation matrix (SEC) approach\\(^{43}\\), we estimate the sparse correlation matrix by solving\n\n\\[\n\\hat{R} = \\arg\\min_R \\frac{1}{2} \\|R - R_n\\|_F^2 + \\lambda \\|R\\|_1, \\text{ s.t. } R \\succeq \\varepsilon I, R_{jj} = 1, j = 1,\\ldots,d.\n\\]\n\nwhere\n(1) \\( \\| \\cdot \\| \\) is the Frobenius norm,\n\n(2) \\( R \\succeq \\varepsilon I \\) means that \\( R - \\varepsilon I \\) is semipositive definite,\n\n(3) \\( \\lambda \\) is the regularization parameter for the \\( l_1 \\) norm.\n\nDenote the non-diagonal support of \\( R \\) as \\( A_0 = \\{l, m : l \\neq m, \\rho_{lm} \\neq 0\\} \\) and its cardinality as \\( q \\). The convergence of \\( \\hat{R} \\) to \\( R \\) in Frobenius norm is established in the following theorem.\n\n**Theorem 0.3.** *Suppose \\( \\Sigma^0 \\) satisfies Assumption 0.1 and Assumption 0.3 is valid, and \\( \\lambda = M \\sqrt{\\frac{\\log d}{n}} \\) for some constant \\( M \\), we have the estimator defined in (11) such that*\n\n\\[\n\\| \\hat{R} - R \\|_F^2 = O_p(q \\frac{\\log d}{n})\n\\]\n\nA sketch of the proof is provided in the Supplementary Notes.\n\nFrom the computational point of view, the penalized likelihood problem stated in (11) can be replaced with the soft thresholding operator\n\n\\[\n\\hat{R} = \\text{sign}(R_n)((|R_n| - \\lambda)_+,\n\\]\n\nwhere the tuning parameter \\( \\lambda \\) is selected by cross-validation \\( \\lambda = \\min_\\lambda \\| \\hat{R} - R_n \\|_F \\).\\footnote{23}\n\nSince the solution \\( \\hat{R} \\) may not be symmetric in general, the final estimate of \\( \\hat{R} \\) is obtained by forcing \\( \\hat{\\rho}_{ll} = 1 \\) and choosing \\( \\hat{\\rho}_{lm} = \\hat{\\rho}_{lm} I(\\hat{\\rho}_{lm} \\leq \\hat{\\rho}_{ml}) + \\hat{\\rho}_{ml} I(\\hat{\\rho}_{lm} > \\hat{\\rho}_{ml}) \\). We denote the \\( \\hat{R} \\) obtained from the thresholding procedure as \"SECOM (Thresholding)\".\n\nThe sparse matrix \\( \\hat{R} \\) can also be obtained by thresholding on the basis of on p-values. Let \\( p_{lm} \\) be the corresponding p-value for \\( \\hat{\\rho}_{lm} \\), then \\( \\hat{R} \\) can be defined as\n\n\\[\n\\hat{R} = [\\hat{\\rho}_{lm} I(p_{lm} < \\alpha)]_{l,m=1,\\ldots,d},\n\\]\n\nwhere \\( \\alpha \\) is a pre-specified significance level, e.g. \\( \\alpha = 0.005 \\). We denote the \\( \\hat{R} \\) obtained based on p-values as \"SECOM (Filtering)\".\n\n**Estimation of nonlinear correlation coefficient**\nIn addition to linear correlation, we are also interested in describing nonlinear correlations among taxa within an ecosystem (e.g., gut or oral environments) or across ecosystems. Therefore, the concept of distance correlation\\textsuperscript{36} was adopted to quantify general dependence between a pair of taxa.\n\n**Definition 0.1** (Distance correlation coefficient). Let \\( X \\) and \\( Y \\) denote two random variables. Then the distance covariance and correlation coefficient between \\( X \\) and \\( Y \\) are defined as following\n\n(1) \\( dCov^2(X,Y) = \\frac{1}{\\pi^2} \\iint \\frac{\\| f_{X,Y}(t,s) - f_X(t)f_Y(s) \\|^2}{t^2 s^2} dt ds \\),\n\n(2) \\( dVar^2(X) = \\frac{1}{\\pi^2} \\iint \\frac{\\| f_{X,X}(t,s) - f_X(t)f_X(s) \\|^2}{t^2 s^2} dt ds \\),\n\n(3) \\( dCor(X,Y) = \\frac{dCov(X,Y)}{\\sqrt{dVar(X)dVar(Y)}} \\).\n\nwhere \\( \\| \\cdot \\| \\) denotes Euclidean norm, and\n\n(1) \\( 0 \\leq dCor(X,Y) \\leq 1 \\),\n(2) \\( dCor(X,Y) = 0 \\) if and only if \\( X \\) and \\( Y \\) are independent,\n(3) \\( dCor(X,Y) = 1 \\) implies that dimensions of the linear subspaces spanned by \\( X \\) and \\( Y \\) samples respectively are almost surely equal.\n\nEstimator of the distance correlation coefficient based on random samples \\( X = (X_1, X_2, \\ldots, X_n)' \\) and \\( Y = (Y_1, Y_2, \\ldots, Y_n)' \\) is derived as follows. Define pairwise distances as \\( d_{ij} = |x_i - x_j|, e_{ij} = |y_i - y_j| \\), and doubly centered distances as \\( D_{ij} = d_{ij} - d_i - d_j + d \\), \\( E_{ij} = e_{ij} - \\bar{e}_i - \\bar{e}_j + \\bar{e} \\), \\( i \\neq j \\), the empirical estimates of distance covariance and correlation can be obtained by\n\n(1) \\( dCov_n^2(X,Y) = \\frac{1}{n^2} \\sum_{i=1}^n \\sum_{j=1}^n D_{ij} E_{ij}, \\)\n(2) \\( dVar_n^2(X,Y) = \\frac{1}{n^2} \\sum_{i=1}^n \\sum_{j=1}^n D_{ij}^2. \\)\n\nNote that the rank-transformed data also preserve the general dependence in the original data. We illustrate this using both linear and quadratic examples as shown in Supplementary Fig. 5a and b, respectively. In Supplementary Fig. 5a, \\( y = 2x + e, x \\sim U[-2,2], e \\sim N(0,1) \\); whereas in Supplementary Fig. 5b, \\( y = x^2 + e, x \\sim U[-2,2], e \\sim N(0,1) \\). It is easy to see from the figure that even though the shape of \\((X,Y)\\) is not perfectly recovered using ranks (denoted as \\((r(X), r(Y))\\)), distance correlations computed using the original data and the rank-transformed data (denoted as \\(dCor(X,Y)\\) and \\(dCor(r(X), r(Y))\\), respectively) are close enough to each other with a minimal numerical difference, which means the distance correlation computed from the rank-transformed data provides a reasonably good approximation for the distance correlation computed from the original data. Therefore, researchers can use either original abundances or the rank-transformed abundances to calculate distance correlations.\n\nSimilar to the procedure shown in the estimation of linear correlation coefficients, define\n\n\\[\n\\begin{align*}\nd_{lm} &:= dCor(y_{il}, y_{jm}) \\quad \\text{(or } dCor(r_{il}, r_{jm})) \\\\\n\\hat{d}_{lm} &:= dCor(\\hat{y}_{il}, \\hat{y}_{jm}) \\quad \\text{(or } dCor(\\hat{r}_{il}, \\hat{r}_{jm})) \\\\\nD &= [d_{lm}]_{l,m=1,\\ldots,d}, \\\\\nD_n &= [\\hat{d}_{lm}]_{l,m=1,\\ldots,d},\n\\end{align*}\n\\]\n\nthe sparse distance correlation matrix estimation can be obtained by thresholding or p-values:\n\n\\[\n\\begin{align*}\n\\hat{D} &= sign(D_n)(|D_n| - \\lambda)_+ \\text{, or} \\\\\n\\hat{D} &= [\\hat{d}_{lm} I(p_{lm} < \\alpha)]_{l,m=1,\\ldots,d}.\n\\end{align*}\n\\]\n\nData availability\nSimulation data can be found under https://github.com/FrederickHuangLin/SECOM-Code-Archive. 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Sparse estimation of high-dimensional correlation matrices. Comput. Stat. & Data Analysis **93**, 390–403 (2016).\n\nAcknowledgements\nWe are grateful to all HUMIS cohort participants. The research of SDP and HL was funded in part by the Intramural Research Program of the Eunice Kennedy Shriver National Institute of Child Health and Human Development (NICHD), National Institutes of Health, Bethesda, MD. The research of ME was funded in part by the Research Council of Norway, NEVRINOR [grant agreement no. 226402].\n\nAuthor contributions\nTheory and Methodology were conceived and developed by HL and SDP. Illustration section was developed by HL, ME and SDP. Interpretation of the results from the analysis of NoMIC study were performed by ME and SDP. All numerical works were carried out by HL and ME. All three authors contributed towards writing the paper.\n\nCompeting interests\nAuthors declare no conflicts of interest.\nFigure 1. A toy example showing the difference between correlation methods. a A total of 100 taxa were generated, where the true abundances in the ecosystem were generated using a Negative-Binomial distribution. Taxa T1 and T3 are perfectly linearly correlated, and taxa T2 and T4 are quadratically correlated. The remaining taxa are uncorrelated. Only the first 5 taxa (T1 to T5) are provided for the simplicity of exposition. The lower triangular part of the matrix shows the pairwise scatter plots, the upper triangular part of the matrix shows the corresponding pairwise Pearson correlation coefficients, and the diagonal of the matrix shows the density plots for each taxon. b Observed abundances were generated by incorporating sample-specific sampling fractions and taxon-specific sequencing efficiencies to the true abundances. The lower triangular part of the matrix shows the pairwise scatter plots, the upper triangular part of the matrix shows the corresponding pairwise Pearson correlation coefficients, and the diagonal of the matrix shows the density plots for each taxon. c, d, e Pairwise correlation coefficients returned from the standard Pearson correlation coefficients, SparCC, and SECOM based on the observed abundances, respectively. The correlation coefficient ranges from -1 to 1, color coded by blue to red, correspondingly.\nFigure 2. Comparisons of estimation accuracy and sparsity recovery for linear relationships within an ecosystem. The average relative norm loss (Frobenius and Spectral) and sparsity recovery (FPR/TPR) of various correlation methods are shown in a and b, respectively. Synthetic data were generated from Negative-Binomial (NB) distributions. The X-axis denotes the simulation settings, which are a combination of sample size \\( n \\), number of taxa \\( d \\), and the dispersion parameter \\( \\alpha \\) of the corresponding NB distribution. The number of iterations for each simulation setting = 100. Data are represented by the mean of all iterations and error bars represent standard errors. Color and the name of the corresponding correlation methods are shown at the bottom within the graph. The results demonstrate that SECOM (Thresholding and Filtering) and SPIEC-EASI (MB and GL) outperformed all existing methods not only in terms of estimation accuracy, but also in terms of uniformly small FPR, and comparable TPR.\nFigure 3. Comparisons of sparsity recovery for nonlinear relationships within an ecosystem. Synthetic data were generated from Negative-Binomial (NB) distributions. The X-axis denotes the simulation settings, which are a combination of sample size \\( n \\), number of taxa \\( d \\), and the dispersion parameter \\( \\alpha \\) of the corresponding NB distribution. The number of iteration for each simulation setting = 100. Data are represented by the mean of all iterations and error bars represent standard errors. Color and the name of the corresponding correlation methods are shown at the bottom within the graph. Results showed that only SECOM controlled the FPR while maintaining high TPR. Other than SECOM, none of existing methods identify nonlinear relationships.\n\n![Bar chart comparing sparsity recovery metrics for different correlation methods across various simulation settings](page_246_573_1097_482.png)\nFigure 4. Comparisons of estimation accuracy and sparsity recovery for linear relationships between two ecosystems. The relative norm loss (Frobenius and Spectral) and sparsity recovery (FPR/TPR) of various correlation methods are shown in a and b, respectively. Synthetic data were generated from Negative-Binomial (NB) distributions. The X-axis denotes the simulation settings, which are the combinations of sample size \\( n \\), number of taxa \\( d \\), and the dispersion parameter \\( \\alpha \\) of the corresponding NB distribution. Data from different ecosystems have different sampling fractions and sequencing efficiencies in each simulation run. The number of iterations for each simulation setting = 100. Data are represented by the mean of all iterations and error bars represent standard errors. Color and the name of the corresponding correlation methods are shown at the bottom within the graph. Results demonstrated that SECOM methods, namely, SECOM(Thresholding) and SECOM(Filtering) were the only methods successfully quantified microbial correlations between ecosystems.\nFigure 5. Temporal patterns of bias corrected abundance (a) and relative abundances (b) for Norwegian infant gut microbiome data among families. The x-axis represents days (30, 120, and 365 days) and y-axis denotes either the bias corrected abundances or relative abundances. The top 10 most abundant taxa up to 365 days were selected for the visualization purpose. Families with prevalence across samples < 10% were not shown separately and grouped into \"Others\". Different taxa were coded by different colors as shown on the legends.\nFigure 6. Temporal patterns of correlations for Norwegian infant gut microbiome data among families. The correlation metrics (Linear and Distance) are represented by rows and days (30, 120, and 365 days) are represented by columns, respectively. The top 10 most abundant families up to 365 days were initially selected for the visualization purpose. Families with prevalence across samples < 10% were discarded and left blank in the heatmap. The linear correlation coefficient ranges from -1 to 1, color coded by blue to red, respectively.\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• SECOMSupplementaryInformation.pdf\n• suppfig1.pdf\n• suppfig2.pdf\n• suppfig3.pdf\n• suppfig4.pdf\n• suppfig5.pdf"} {"paper_id": "prb81", "title": "AC amplification gain in organic electrochemical transistors for impedance-based single cell sensors", "text": "# Abstract\n\nResearch on water-gated and organic electrochemical transistor (OECT) architectures is motivated by the prospect of a highly biocompatible interface capable of amplifying bioelectronic signals at the site of detection. Despite many demonstrations in these directions, a quantitative model for OECTs as impedance biosensors is still lacking. We overcome this issue by introducing a model experiment where we simulate the detection of a single cell by the impedance sensing of a dielectric microparticle. The highly reproducible experiment allows us to study the impact of transistor geometry and operation conditions on device sentivity. With the data we rationalize a mathematical model that provides clear guidelines for the optimization of OECTs as single cell sensors, and we verify the quantitative predictions in an in-vitro experiment. In the optimized geometry, the OECT-based impedance sensor allows to record single cell adhesion and detachment transients, showing a maximum gain of (20.2±0.9) dB with respect to a single electrode based impedance sensor.\n\n# Introduction\n\nIn recent years water gated and electrochemical transistor architectures have found broad attention in biosensor research.¹,² The interest is motivated by the possibility to combine electrochemical transduction mechanisms known from metallic electrodes with the intrinsic amplification properties of a transistor structure.³ The amplification is highly wanted to improve signal to noise ratio in challenging sensor applications aiming for instance at biochemical detection in complex mixtures⁴ or single cell bioelectronic monitoring.⁵ Significant progress on this concept has been made by the introduction of organic or carbon-based semiconducting materials with high stability in water such as carbon nanotubes,⁶,⁷ graphene,⁸,⁹ or organic semiconductors.¹⁰ When patterned into a semiconducting channel connected to a source and drain electrode, these materials enable transistor-like structures to replace single metallic working electrodes. Since the semiconducting channel is in direct contact with the aqueous electrolyte, a strong capacitive coupling results between the channel’s electronic carrier concentration and the electrochemical potential in the solution.¹¹ Events that alter the electrochemical potential and impact on the ionic distribution at the channel-electrolyte interface thus gate the sensor’s semiconducting channel conductivity. Even small perturbations in the ionic distribution can cause a large variation in the number of electronic carriers flowing through the channel from source to drain electrode, hence leading to an amplification effect.¹² This qualitative argument is demonstrated by improved sensitivity in several applications realized with water gated transistor structures.¹³ However, to achieve optimized sensor devices, a quantitative understanding of such signal gain is needed. The goal of this work is to derive a quantitative model that relates transistor amplification gain to semiconductor material properties and water gated transistor architecture.\n\nA widely explored class of water gated transistors are organic electrochemical transistors (OECTs).¹⁴ OECTs exploit organic mixed ionic and electronically conductors such as poly(3,4-ethylenedioxythiophene):polystyrene sulfonate (PEDOT:PSS).² The high chemical stability, the facile, solvent-based processing and the high biocompatibility, make PEDOT:PSS a material of choice for healthcare applications.¹⁵ In PEDOT:PSS, electronic transport is achieved by mobile hole charges present in the oxidized semiconducting polymer PEDOT. The positive charge of the holes is counterbalanced by fixed, negative ionic charges of the polyanion PSS.¹⁶ Oxidized organic semiconductor and ionic polyanion form a nanophase separated network that generates close electrostatic interaction between the two phases combined with efficient electronic as well as ionic charge transport.¹⁵,¹⁷ Consequently, high electronic carrier mobility (µ > 10 cm² V⁻¹ s⁻¹)¹⁸ is combined with a strong volumetric capacitive coupling between the ionic phase and the electronic phase (c > 30 F/cm³).¹⁹ In OECTs this properties combination gives rise to large values of transconductance gm = ∂Ich/∂Vg that express how small changes in the electrostatic potential ∂Vg of the electrolyte gate the electronic channel current Ich.²⁰ Relying on the large transconductance combined with the biocompatible material properties, many research works propose OECTs as amplifying transistor to be integrated in electrochemical and bioelectronic sensors for healthcare applications.²¹ Established examples regard potentiometric sensors used to quantify the concentration of ionic or redox active analytes²² and to record electrophysiological signals.²³ In this case, the electrical circuit involving the OECT must operate ultimately as a voltage amplifier, that produces an amplified output voltage ready for digitization. Gain is then expressed as the ratio between the original potentiometric signal and the output voltage. Depending on the circuit design, DC amplification gains reaching 30 V/V have been demonstrated in OECT based potentiometric sensors.²⁴,³\n\nA second, emerging class of biosensors that takes advantage of OECT amplification regards impedance based sensors for monitoring cellular adhesion and cell layer barrier properties as quantified by the transepithelial electrical resistance (TEER).²⁵,⁴ Monitoring such cellular properties is of importance in studies of wound healing, cancer development, toxicity assays or recognition processes in the immune system.²⁵ Impedance based biosensors quantify the ionic current that passes through a cellular layer when an AC voltage is applied.²⁶ Changes in cellular adhesion or intercellular barrier properties change the measured current signal thus providing a simple means for real-time monitoring.²⁷ By replacing the metallic working electrode of a traditional impedance sensor with a water gated OECT, amplification of the current signal is achieved thus increasing sensitivity and reducing possible noise pickup.²⁸ Current amplification becomes particularly important in high impedance applications as encountered when the sensor size is scaled down to micrometric scales matching cellular dimensions. Such downscaling opens the opportunity to translate impedance based cellular monitoring to the single cell level.²⁹ This ultimate sensor resolution is highly desired in biomedical research as the importance of single cell phenotyping is increasingly recognized for the study of cell development and physiology, as well as for research on cellular pathologies such as cancer.³⁰ An important step in this direction was recently achieved by Hempel et al. by demonstrating single cell sensitivity in an OECT enabled impedance sensor. The authors found that significant differences in the sensors transfer function are caused by cells adhering to the transistor surface. Such changes in transfer function are usually quantified as the transistor bandwidth (or response time) and equivalent circuit models were developed to explain the observed frequency response and its relation to impedances at the cell/PEDOT:PSS interface.⁵\n\nDespite the promising results, a quantitative study on the transistor amplification gain in the frequency spectrum relevant for cellular impedance sensing is still lacking. Different studies demonstrate that the high OECT transconductance is limited to the low frequency regime and strongly depends on transistor geometry and materials properties.²⁰ Consequently, there is a need for a quantitative model that relates impedance sensor gain to OECT transconductance and other device properties in order to enable a rational optimization of OECT based impedance sensors. A clear understanding of gain is also desired to define when OECT amplification has significant advantages over one-terminal, low-impedance microelectrode-based sensors offering simpler fabrication and electrical operation. To overcome the issue, we introduce in this work a model experiment that allows a quantitative analysis of amplification gain in OECT based impedance sensors. As cellular in-vitro experiments are inherently difficult to control we substitute the cell by a dielectric microparticle of similar dimensions. We control the position of the microparticle on top of the microscale impedance sensors with an AFM and achieve highly reproducible measurements that enable to compare the current output of OECT based sensors with equivalent microelectrode sensors. To rationalize the findings, we develop an analytical model that describes the gain as a function of the applied frequency, the device geometry and PEDOT:PSS materials properties. Relying on this model, we design an optimized device and demonstrate its efficiency by measuring the transients of single cell adhesion and detachment in in-vitro experiments. Noteworthy, we observe a significant AC gain reaching values of (20.2±0.9) dB for the transistor structure, thereby demonstrating the advantages arising from the OECT amplification in single-cell impedance sensing experiments.\n\n# Results\n\nImpedance sensing of a dielectric microparticle: The first objective of our work is to introduce a novel experiment to quantify the sensitivity of electrochemical impedance sensors operated in OECT or microelectrode configuration. To this end we realized the experimental setup shown in Figure 1a and 1b. The setup contains a dielectric microparticle (with diameter of 50 µm) attached to the bottom part of an AFM cantilever to have micrometric control of its position in the 3 spatial directions (Figure 1c). Once the microparticle is finely aligned with the x-y coordinates on the center of the sensor surface, we use the z-stage of the microscope to control the particle-sample distance d. Contact of the microparticle with the sensor surface is determined by the onset of a repulsive force acting on the AFM cantilever. The electric circuit to operate the OECT impedance sensor contains a Ag/AgCl wire that is used as the gate electrode, controlling the electrical potential of the aqueous electrolyte solution (0.1 M PBS). A DC voltage VD,DC is applied between the source (S) and drain (D) electrodes of the OECT to drive the electronic current ID,DC in the PEDOT:PSS channel. The measured transfer and output characteristics of a typical OECT (Figure 1d), demonstrate that the gate voltage effectively modulates the channel current. For impedance sensing we superimpose a small sinusoidal oscillation signal VG,AC (with amplitude 10 mV and angular frequency ω) on the gate bias VG,DC. This leads to an AC current in the PEDOT:PSS layer, which is measured by a lock-in amplifier connected to the source contact (IS,AC).\n\nIn the microelectrode configuration (Figure 1b) the circuit is simplified, as source and drain electrodes are in short circuit and are jointly connected to the lock-in amplifier. Therefore, no OECT channel current is present, and all the electric current measured during impedance sensing is the gate current IG,AC, flowing from the electrolyte into the PEDOT:PSS layer. All other components are identical to the OECT configuration to permit a direct comparison.\n\nIn Figure 1e we show the results of a typical microparticle distance - AC current experiment conducted at 1.17 kHz excitation frequency. The amplitudes of the AC currents in OECT and microelectrode configuration are plotted as a function of time. During the experiment, the microparticle is approached and retracted from the device channel for three consecutive times. For both configurations, the current amplitude follows the motion of the microparticle in a highly reproducible manner over consecutive cycles, highlighting the stability of the characterization method. In Figure 1f, the same data is plotted as a function of the distance between microparticle and sensor surface. Both types of devices produce a reversible, linear response in which the approach leads to a reduction in AC amplitude. Qualitatively, this response is expected, as the microsphere represents a barrier for the ionic current in the electrolyte: when it is close to the sensor surface, the half space through which ions can approach the active layer is reduced, thus increasing the effective impedance of the electrolyte Zel. Consequently, upon approach, the interfacial impedance measured with the sensor increases and the AC current amplitude drops. We note that in first order approximation a similar response is expected when a biological cell adheres to the sensor surface.\n\nThe results are crucial for our goal as they permit the quantitative assessment of the sensitivity of the impedance sensor. For the case of a high sensitivity, small changes in the impedance Zel cause large variation in AC current amplitude. Therefore, we define the sensitivity as s = ∂IAC/∂Zel. In our experiment, ∂Zel is directly related to the microparticle displacement ∂Zel = p*∂d. The proportionality constant p is independent on the sensor configuration (OECT vs microelectrode) and we obtain its numerical value by fitting the microelectrode impedance spectra (see Supp. Inf S2). Accordingly, the sensitivity is given by the slope of the approach curves shown in Figure 1e. We obtain numerical values for this particular case (WxL = 100x100 µm) of sOECT = (0.059±0.002) nA/Ω and sµE = (0.023±0.006) nA/Ω. The values show a greater sensitivity in the OECT device with respect to the microelectrode, due to the contribution of OECT channel current to the AC response.\n\nQuantitative model for PEDOT:PSS-based impedance sensors: We developed an analytical model to express the impedance sensitivity s as a function of the sensor operation conditions, material properties and geometry. Objective is a quantitative understanding of the factors that increase sensitivity in OECT configuration with respect to PEDOT:PSS microelectrodes. Many studies decouple charge transport in OECTs in an electronic and an ionic circuit. A schematic of this representation is reported in Figure 2a, where the components of the electronic and the ionic circuit are indicated in blue and orange, respectively. Electronic charge carriers (holes) are driven by the drain voltage VD,DC and carry the channel current in an OECT, while ionic charge carriers are driven by the gate voltage VG = VG,DC + VG,AC and modulate the concentration of holes and, consequently, the electronic conductivity of the transistor channel. The limited conductivity of the electrolyte as well as the presence of dielectric objects close to the sensor surface generate an impedance Zel which causes a potential drop in the electrolyte, and the voltage at the electrolyte/channel interface VG* can be considered as the effective gate voltage that acts on the channel and determines the drain current. For the impedance sensing we are interested in the AC response of the transistor and we express the AC current flowing in the OECT channel as Ich,AC = gm,AC*VG*,AC. Following Bernards model, gm,AC can be expressed as gm,AC^lin = -W/L µp cv t VD,DC and gm,AC^sat = -W/L µp cv (VG,DC - Vt) in linear or saturation conditions. In these expressions, W, L and t indicate the width, length and thickness of the sensor channel, µp the holes mobility, cv the volumetric capacitance of PEDOT:PSS and Vt the OECT threshold voltage.\n\nTo derive the overall AC current, it is important to note that in AC transport conditions the source (and drain) current signals are composed of two contributions:\n$$\n{I}_{S,AC }= {I}_{ch,AC } + {f}_{OECT}\\\\bullet {I}_{G,AC } \\quad (1)\n$$\nThe first (Ich,AC) originates from the channel current, whereas the second (IG,AC) is due to the gate current and regards the capacitive current that has increasing importance at higher frequencies. Its value is given by IG,AC = VG,AC / ZG in which ZG = Zel + Zch is the overall impedance of the sensor given by the series combination of the electrolyte impedance Zel and the impedance related to the PEDOT:PSS channel capacitance Zch = 1/(iω Cch). The channel capacitance can further be related to the geometry and the volumetric capacitance of the PEDOT:PSS layer: Cch = cv*W*L*t. Possible contributions due to parasitic capacitances are neglected for simplicity. The factor fOECT in eqn. 1 determines how the gate current is distributed between the source and the drain terminal and is typically assumed to be equal to 0.5. Several studies demonstrate that the fOECT factor is slightly dependent on VD,DC, and VG,DC as well as on channel geometry. For this reason, fOECT was not assumed as constant in this experiment, but its value was set for each sensor in order to best fit the experimental data with the model.\n\nThe figure of merit of the OECT as impedance sensor (the sensitivity sOECT) indicates its capability to transduce a variation of Zel in a current output. This can be calculated from the model by differentiating eq. (1):\n$$\n{s}_{OECT }= \\\\left|\\\\frac{\\\\partial ({I}_{ch,AC}+{f}_{OECT}{I}_{G,AC})}{\\\\partial {Z}_{el}}\\\\right|=|{s}_{ch}+{f}_{OECT}\\\\bullet {s}_{\\\\mu E}| \\quad (2)\n$$\nAfter inserting the expressions for the two AC current contributions and differentiation we obtain for the channel sensitivity:\n$$\n{s}_{ch}=\\\\frac{{g}_{m,AC}}{{Z}_{G}}\\\\left(1-\\\\frac{{Z}_{el}}{{Z}_{G}}\\\\right){V}_{G,AC}\n$$\nand the sensitivity of the microelectrode is:\n$$\n{s}_{\\\\mu E}= \\\\frac{{V}_{G,AC}}{{Z}_{G}^{2}} \\quad (4)\n$$\nThe suitability of this simple approach to model the AC response of an OECT is demonstrated in Figure 2b and c. Figure 2b compares the frequency response of an OECT and of a microelectrode with the model predictions. The PEDOT:PSS channel width and length are W = 100 µm and L = 100 µm, respectively. The channel capacitance and the electrolyte impedance Zel were extracted for each device geometry by fitting the microelectrode impedance spectrum. The average volumetric capacitance of PEDOT:PSS resulted to be cv = (30.0 ± 1.3) F/cm³, obtaining a result consistent with literature findings. The OECT device shows a significantly higher current in the low frequency domain. Here the electronic channel current Ich prevails, and the transistor demonstrates clear amplifying properties. Then, above a cutoff frequency fc = 645 Hz, the transistor response is limited by the slow ionic transport between the channel and the electrolyte. At the same time the microelectrode’s response increases with frequency until a current limitation is reached due to the electrolyte impedance. As a consequence, in the high frequency limit both impedance sensor configurations yield the same current response. Importantly, the cutoff frequency that determines the OECT amplification is determined by the channel geometry as demonstrated in Figure 2c. The plot of the current amplitude versus frequency for OECTs with different channel sizes clearly shows that with increasing channel area and length a strong reduction in fc is observed.\n\nFinally, we systematically study the OECTs sensitivity towards electrolyte impedance changes with the microsphere experiment introduced above. Figure 2d shows the measured values for sOECT obtained for three different channel geometries at different AC frequencies. Eq. 2 is in excellent agreement with the frequency dependence of the measured data. In the low-frequency range the sensitivity shows a linear increase with frequency until it reaches a sensitivity maximum sOECT^max. Beyond the maximum, a smaller decrease in sensitivity is observed until it settles to a constant value for high frequencies. It is important to highlight that the position of sOECT^max corresponds to the device cutoff frequency fc (see Supp. Inf. S3 for the full mathematical treatment), and hence is a geometry-dependent parameter.\n\nIn Figure 2e we compare the sensitivity of a microelectrode and an OECT with the same dimensions (WxL = 200x50 µm). The transistor amplification, which is significant at low frequencies, has a relevant impact on the sensitivity. However, at high frequencies the response of both devices is limited by the electrolyte resistance and no significant differences are present. Such an observation is reflected by a frequency dependent OECT gain, which can be directly calculated with our model from eq. 2 and 4:\n$$\n{gain }_{OECT}= 20\\\\bullet {{log}}_{10}\\\\left(\\\\frac{{s}_{OECT}}{{s}_{microel}}\\\\right) \\quad (5)\n$$\nThe OECT gain is highest in the low-frequency regime, but is still significant in the 0.1-10 kHz range, where the impedance of the cell layers is typically measured. This justifies the use of a transistor structure for high precision bioelectronic impedance sensing experiments. Figure 2f demonstrates that the OECT gain is a geometry-dependent parameter. The smallest device (WxL = 50x50 µm) shows the highest gain, while a rectangular channel geometry is preferable for OECTs with the same area, since the gain is proportional to W/L ratio.\n\nSingle cell impedance sensor experiment: We demonstrated the value of the mathematical model here proposed for the optimization of a PEDOT:PSS-based single cell impedance sensor by monitoring single cell adhesion and detachment in an in-vitro experiment, simultaneously measuring the impedance changes with both an OECT and a microelectrode. According to the model prediction and the AFM experiment, we patterned the device channels with a 200x50 µm rectangular geometry, which provides the best performances in terms of sensitivity. The T98G cell line cultured in Minimum Essential Medium was diluted to have a final density of 1 x 10³ cells/cm³ and poured on the surface of the impedance sensors (see the Methods section for full details). After seeding, the cells reached the underlying substrate by gravity. We microfabricated a linear array of 10 PEDOT:PSS channels (see Supp. Inf. S4) to largely increase the probability of a single cell settling onto a sensor. An optical image of the final experimental configuration is reported in Figure 3a, showing a single T98G cell positioned at the center of the PEDOT:PSS channel. The encapsulation of the metallic electrodes with negative photoresist insulates the device from all the remaining cells which are not lying in the PEDOT:PSS active layer. We acquired the current spectra of both the OECT and the microelectrode at consecutive time intervals to make a real-time detection of the cell adhesion process. To stress the full consistency of the measurements acquired with the OECT and the microelectrode, we plot in Figure 3b the current amplitudes measured at 625 Hz as a function of time. The sensing frequency was selected in correspondence to the OECT cutoff (measured at time t=0), where the model indicates the maximum sensitivity. The signals acquired at the beginning of the experiment are stable around a maximum value. Afterwards, at time t=20 min the current start to decrease, indicating the beginning of the cell adhesion process. This produces a rapidly varying response until t=60 min, when the decrease becomes slower, and the current stabilizes around a minimum value. At t=200 min, we used a cell dissociation agent (trypsin) to completely remove the cell from the sample surface, and devices recovered their original current amplitude.\n\nWe report in Figure 3c the full current spectra acquired before and after the treatment with trypsin (t=180 min and t=240 min, respectively). The cell adhesion produced a large shift of the OECT low-pass cutoff towards smaller frequency. In parallel, the current spectrum of a control device placed in the same reservoir, but with no cell seeded on the PEDOT:PSS layer, remained unaltered (see Supp. Inf. S5). After trypsinization, the initial cutoff frequency is fully recovered. These combined observations clearly demonstrate that the cutoff shift is only caused by the single cell adhesion on the PEDOT:PSS layer. The same considerations can be extended to the PEDOT:PSS microelectrode. Here, the cell adhesion process is revealed by a decrease in the gate current amplitude, which reaches its minimum at t=180 min, coherently with the OECT measurements. After the cell detachment (t=240 min), the current increases to its original values.\n\nTo provide a direct comparison between the sensing performances, we averaged the current amplitudes acquired when the cell is detached (t<30 min and t=240 min) and attached (1205\n\nImportantly, our quantitative approach to compare bioelectronic impedance sensors is not limited to PEDOT:PSS based OECTs but can easily be extended to different water gated transistor architectures. The crucial parameter that describes the different material properties in our model is the channel transconductance. Large transconductances have been demonstrated for different channel materials and device architectures. They result from high capacitive couplings, as observed in organic mixed ionic and electronic conductors (e. g. PEDOT:PSS) or high carrier mobilities as found for example in graphene or carbon nanotubes.86 Current research in the material properties of such water stable semiconductors warrants further improvements in mobility or volumetric capacitance and will also augment the sensitivity of bioelectronic impedance sensors.26 Our quantitative approach can serve as a guideline for the development of impedance sensors with maximized sensitivity and establishes a metric to compare future devices.\n\n# Methods\n\n**Device fabrication**: Glass substrates (50×25 mm2) were cleaned by sonication in water and soap (10%)/acetone/isopropanol/distilled water baths. After a dehydration step (10 minutes at 110° C), the Microposit S1818 positive photoresist was spin coated (4000 rpm for 60 s) and annealed at 110°C for 1 minute. Metallic contacts were patterned through direct laser lithography by using the ML3 Microwriter (from Durham Magneto Optics). The photoresist was developed with Microposit MF-319 developer. Then, 10 nm of chromium and 25 nm of gold were deposited by thermal evaporation. Samples were immersed in acetone for 4 hours for photoresist lift-off. Metallic contacts were encapsulated with the mr-DWL 5 negative photoresist (from Micro Resist Technology). The resin was spin coated at 3000 rpm for 30 s and annealed at 100°C for 2 minutes. After laser exposure, samples were baked at 100°C for 2 minutes and relaxed for 1 hour at room temperature. Development was performed with mr-Dev 600 developer (Micro Resist Technology), and the resist was finally baked at 120°C for 30 minutes. A double layer of S1818 was deposited and treated for 6 minutes in chlorobenzene for the photolithography of the PEDOT:PSS channel.37 After the development, substrates were treated with air plasma (15 W for 2 min) and the PEDOT:PSS solution (94% PEDOT:PSS (Heraeus, Clevios PH1000), 5% of ethylene glycol (EG) (Sigma Aldrich), 1% of 3-glycidoxypropyltrimethoxysilane (GOPS), and 0.25% of 4-dodecylbenzenesulfonicacid (DBSA)) was spin coated at 3000 rpm for 10 s. The resulting film thickness was (100 ±10) nm. The samples were subsequently annealed at 120°C for 1 h, and S1818 was finally lifted-off after 4 hours in acetone.\n\n**Electrical measurements**: DC characteristics of the OECTs were carried out with the Keysight 2912A source-measure unit (SMU), using a Ag/AgCl wire as gate electrode. The acquired data were analyzed to set the working point of the transistor during impedance sensing, i.e. the DC gate and drain voltages at which the transconductance *g**m,DC* assumes its maximum value (Supp. Inf. S1). AC measurements were performed with the MFLI lock-in amplifier (from Zurich Instruments). A constant DC offset voltage and a sinusoidal oscillation (amplitude 10 mV) with desired frequency were applied to the gate terminal. The resulting AC current flowing in the PEDOT:PSS channel was demodulated to acquire the current amplitude of the impedance sensors. In the OECT configuration, a constant DC voltage was applied between the source and the drain electrodes to bias the device at its working point. The microelectrode configuration was obtained by shorting the drain and the source terminals.\n\n**Microparticle sensing experiment**\n\nTo fabricate the AFM probe supporting the dielectric microparticle, we dispersed a powder of pyrophosphate microspheres (Polymat) on a glass slide. A PPP-NCHR cantilever of the Park NX10 AFM (force constant 34.55 N/m) was approached onto a drop of glue, and then put in contact with the upper part of a microsphere (with diameter of about 50 µm) until complete adhesion.\n\nAFM measurements were performed in liquid, using 0.1 *m* PBS as electrolyte and an Ag/AgCl wire as gate electrode. To measure the current-distance spectroscopies, we placed the microparticle in the center of the PEDOT:PSS channel of the impedance sensor and we performed an AFM force-distance spectroscopy. The probe was lifted to the vertical coordinate *z*0, distant 5µm from the contact position, then gradually approached to the sample surface (scan speed 0.3 µm/s), and finally retracted again to *z*0. During this process, we applied a constant modulation frequency to the gate terminal, and we measured the current amplitude flowing in the PEDOT:PSS layer, obtaining a current-distance spectroscopy curve. The experiment was repeated at 5 different frequencies (117, 330, 1170, 3330, and 11700 Hz) both in the OECT and in the microelectrode configurations.\n\n**Single cell detection experiment**: The human malignant glioma cell line, T98G (CRL-1690™), derived from a glioblastoma multiform tumor, was selected for the single cell detection experiment. This is characterized by indefinite lifespan and adherence properties previously reported also on PEDOT:PSS layers.38 It was purchased from ATCC (Manassas, VA, USA) and cultured in Minimum Essential Medium (MEM) (Gibco™ 51200046, ThermoFisher scientific), supplemented with 10% fetal bovine serum, 1% L-glutamine, 10% sodium pyruvate and antibiotics (1% penicillin and 1% streptomycin) at 37°C in 5% CO2 incubator. All chemicals were from Merck. The experimental day, the sub-confluent (70-80%) cells population was detached by 0.25% trypsin in 0.02% EDTA (both from Merck) solution, re-suspended in fresh supplemented MEM and counted by the hemocytometric chamber. An aliquot, calculated to have a final density of 1 x 103 cells/cm3 was diluted in 600 µL of supplemented MEM and poured on the surface of the impedance sensors, previously sterilized by 20 min of UV exposure. A polydimethylsiloxane (PDMS) well was attached onto the sample substrate to host both the solution containing the cells and the Ag/AgCl gate electrode. After seeding, the cells reached the underlying substrate by gravity. For the experiment, we microfabricated a linear array of 10 PEDOT:PSS channels with dimensions WxL=200x50 µm (an optical image is reported in Supp. Inf. S4). In this way, the probability of a single cell falling onto a device channel after seeding was largely increased. Once this configuration was achieved, the sample was connected for the electrical measurements. The current spectra of the impedance sensor were acquired both in the OECT and the microelectrode configurations every 10 minutes after cell seeding. During each acquisition, the modulation frequency applied at the gate terminal was swept between 10 and 105 Hz. At time *t* = 200 min, trypsin was used to completely remove the cells from the sample surface. 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Interfaces **9**, 6679–6689 (2017).\n\n# Supplementary Files\n\n- [SuppInf.docx](https://assets-eu.researchsquare.com/files/rs-1307502/v1/826dbf0657f8746e7cf8fee3.docx) \n Supplementary Information"} {"paper_id": "prb82", "title": "A sub-wavelength Si LED integrated in a CMOS platform", "text": "# Abstract\n\nResearch on water-gated and organic electrochemical transistor (OECT) architectures is motivated by the prospect of a highly biocompatible interface capable of amplifying bioelectronic signals at the site of detection. Despite many demonstrations in these directions, a quantitative model for OECTs as impedance biosensors is still lacking. We overcome this issue by introducing a model experiment where we simulate the detection of a single cell by the impedance sensing of a dielectric microparticle. The highly reproducible experiment allows us to study the impact of transistor geometry and operation conditions on device sentivity. With the data we rationalize a mathematical model that provides clear guidelines for the optimization of OECTs as single cell sensors, and we verify the quantitative predictions in an in-vitro experiment. In the optimized geometry, the OECT-based impedance sensor allows to record single cell adhesion and detachment transients, showing a maximum gain of (20.2±0.9) dB with respect to a single electrode based impedance sensor.\n\n# Introduction\n\nIn recent years water gated and electrochemical transistor architectures have found broad attention in biosensor research.¹,² The interest is motivated by the possibility to combine electrochemical transduction mechanisms known from metallic electrodes with the intrinsic amplification properties of a transistor structure.³ The amplification is highly wanted to improve signal to noise ratio in challenging sensor applications aiming for instance at biochemical detection in complex mixtures⁴ or single cell bioelectronic monitoring.⁵ Significant progress on this concept has been made by the introduction of organic or carbon-based semiconducting materials with high stability in water such as carbon nanotubes,⁶,⁷ graphene,⁸,⁹ or organic semiconductors.¹⁰ When patterned into a semiconducting channel connected to a source and drain electrode, these materials enable transistor-like structures to replace single metallic working electrodes. Since the semiconducting channel is in direct contact with the aqueous electrolyte, a strong capacitive coupling results between the channel’s electronic carrier concentration and the electrochemical potential in the solution.¹¹ Events that alter the electrochemical potential and impact on the ionic distribution at the channel-electrolyte interface thus gate the sensor’s semiconducting channel conductivity. Even small perturbations in the ionic distribution can cause a large variation in the number of electronic carriers flowing through the channel from source to drain electrode, hence leading to an amplification effect.¹² This qualitative argument is demonstrated by improved sensitivity in several applications realized with water gated transistor structures.¹³ However, to achieve optimized sensor devices, a quantitative understanding of such signal gain is needed. The goal of this work is to derive a quantitative model that relates transistor amplification gain to semiconductor material properties and water gated transistor architecture.\n\nA widely explored class of water gated transistors are organic electrochemical transistors (OECTs).¹⁴ OECTs exploit organic mixed ionic and electronically conductors such as poly(3,4-ethylenedioxythiophene):polystyrene sulfonate (PEDOT:PSS).² The high chemical stability, the facile, solvent-based processing and the high biocompatibility, make PEDOT:PSS a material of choice for healthcare applications.¹⁵ In PEDOT:PSS, electronic transport is achieved by mobile hole charges present in the oxidized semiconducting polymer PEDOT. The positive charge of the holes is counterbalanced by fixed, negative ionic charges of the polyanion PSS.¹⁶ Oxidized organic semiconductor and ionic polyanion form a nanophase separated network that generates close electrostatic interaction between the two phases combined with efficient electronic as well as ionic charge transport.¹⁵,¹⁷ Consequently, high electronic carrier mobility (µ > 10 cm² V⁻¹ s⁻¹)¹⁸ is combined with a strong volumetric capacitive coupling between the ionic phase and the electronic phase (c > 30 F/cm³).¹⁹ In OECTs this properties combination gives rise to large values of transconductance gm = ∂Ich/∂Vg that express how small changes in the electrostatic potential ∂Vg of the electrolyte gate the electronic channel current Ich.²⁰ Relying on the large transconductance combined with the biocompatible material properties, many research works propose OECTs as amplifying transistor to be integrated in electrochemical and bioelectronic sensors for healthcare applications.²¹ Established examples regard potentiometric sensors used to quantify the concentration of ionic or redox active analytes²² and to record electrophysiological signals.²³ In this case, the electrical circuit involving the OECT must operate ultimately as a voltage amplifier, that produces an amplified output voltage ready for digitization. Gain is then expressed as the ratio between the original potentiometric signal and the output voltage. Depending on the circuit design, DC amplification gains reaching 30 V/V have been demonstrated in OECT based potentiometric sensors.²⁴,³\n\nA second, emerging class of biosensors that takes advantage of OECT amplification regards impedance based sensors for monitoring cellular adhesion and cell layer barrier properties as quantified by the transepithelial electrical resistance (TEER).²⁵,⁴ Monitoring such cellular properties is of importance in studies of wound healing, cancer development, toxicity assays or recognition processes in the immune system.²⁵ Impedance based biosensors quantify the ionic current that passes through a cellular layer when an AC voltage is applied.²⁶ Changes in cellular adhesion or intercellular barrier properties change the measured current signal thus providing a simple means for real-time monitoring.²⁷ By replacing the metallic working electrode of a traditional impedance sensor with a water gated OECT, amplification of the current signal is achieved thus increasing sensitivity and reducing possible noise pickup.²⁸ Current amplification becomes particularly important in high impedance applications as encountered when the sensor size is scaled down to micrometric scales matching cellular dimensions. Such downscaling opens the opportunity to translate impedance based cellular monitoring to the single cell level.²⁹ This ultimate sensor resolution is highly desired in biomedical research as the importance of single cell phenotyping is increasingly recognized for the study of cell development and physiology, as well as for research on cellular pathologies such as cancer.³⁰ An important step in this direction was recently achieved by Hempel et al. by demonstrating single cell sensitivity in an OECT enabled impedance sensor. The authors found that significant differences in the sensors transfer function are caused by cells adhering to the transistor surface. Such changes in transfer function are usually quantified as the transistor bandwidth (or response time) and equivalent circuit models were developed to explain the observed frequency response and its relation to impedances at the cell/PEDOT:PSS interface.⁵\n\nDespite the promising results, a quantitative study on the transistor amplification gain in the frequency spectrum relevant for cellular impedance sensing is still lacking. Different studies demonstrate that the high OECT transconductance is limited to the low frequency regime and strongly depends on transistor geometry and materials properties.²⁰ Consequently, there is a need for a quantitative model that relates impedance sensor gain to OECT transconductance and other device properties in order to enable a rational optimization of OECT based impedance sensors. A clear understanding of gain is also desired to define when OECT amplification has significant advantages over one-terminal, low-impedance microelectrode-based sensors offering simpler fabrication and electrical operation. To overcome the issue, we introduce in this work a model experiment that allows a quantitative analysis of amplification gain in OECT based impedance sensors. As cellular in-vitro experiments are inherently difficult to control we substitute the cell by a dielectric microparticle of similar dimensions. We control the position of the microparticle on top of the microscale impedance sensors with an AFM and achieve highly reproducible measurements that enable to compare the current output of OECT based sensors with equivalent microelectrode sensors. To rationalize the findings, we develop an analytical model that describes the gain as a function of the applied frequency, the device geometry and PEDOT:PSS materials properties. Relying on this model, we design an optimized device and demonstrate its efficiency by measuring the transients of single cell adhesion and detachment in in-vitro experiments. Noteworthy, we observe a significant AC gain reaching values of (20.2±0.9) dB for the transistor structure, thereby demonstrating the advantages arising from the OECT amplification in single-cell impedance sensing experiments.\n\n# Results\n\nImpedance sensing of a dielectric microparticle: The first objective of our work is to introduce a novel experiment to quantify the sensitivity of electrochemical impedance sensors operated in OECT or microelectrode configuration. To this end we realized the experimental setup shown in Figure 1a and 1b. The setup contains a dielectric microparticle (with diameter of 50 µm) attached to the bottom part of an AFM cantilever to have micrometric control of its position in the 3 spatial directions (Figure 1c). Once the microparticle is finely aligned with the x-y coordinates on the center of the sensor surface, we use the z-stage of the microscope to control the particle-sample distance d. Contact of the microparticle with the sensor surface is determined by the onset of a repulsive force acting on the AFM cantilever. The electric circuit to operate the OECT impedance sensor contains a Ag/AgCl wire that is used as the gate electrode, controlling the electrical potential of the aqueous electrolyte solution (0.1 M PBS). A DC voltage VD,DC is applied between the source (S) and drain (D) electrodes of the OECT to drive the electronic current ID,DC in the PEDOT:PSS channel. The measured transfer and output characteristics of a typical OECT (Figure 1d), demonstrate that the gate voltage effectively modulates the channel current. For impedance sensing we superimpose a small sinusoidal oscillation signal VG,AC (with amplitude 10 mV and angular frequency ω) on the gate bias VG,DC. This leads to an AC current in the PEDOT:PSS layer, which is measured by a lock-in amplifier connected to the source contact (IS,AC).\n\nIn the microelectrode configuration (Figure 1b) the circuit is simplified, as source and drain electrodes are in short circuit and are jointly connected to the lock-in amplifier. Therefore, no OECT channel current is present, and all the electric current measured during impedance sensing is the gate current IG,AC, flowing from the electrolyte into the PEDOT:PSS layer. All other components are identical to the OECT configuration to permit a direct comparison.\n\nIn Figure 1e we show the results of a typical microparticle distance - AC current experiment conducted at 1.17 kHz excitation frequency. The amplitudes of the AC currents in OECT and microelectrode configuration are plotted as a function of time. During the experiment, the microparticle is approached and retracted from the device channel for three consecutive times. For both configurations, the current amplitude follows the motion of the microparticle in a highly reproducible manner over consecutive cycles, highlighting the stability of the characterization method. In Figure 1f, the same data is plotted as a function of the distance between microparticle and sensor surface. Both types of devices produce a reversible, linear response in which the approach leads to a reduction in AC amplitude. Qualitatively, this response is expected, as the microsphere represents a barrier for the ionic current in the electrolyte: when it is close to the sensor surface, the half space through which ions can approach the active layer is reduced, thus increasing the effective impedance of the electrolyte Zel. Consequently, upon approach, the interfacial impedance measured with the sensor increases and the AC current amplitude drops. We note that in first order approximation a similar response is expected when a biological cell adheres to the sensor surface.\n\nThe results are crucial for our goal as they permit the quantitative assessment of the sensitivity of the impedance sensor. For the case of a high sensitivity, small changes in the impedance Zel cause large variation in AC current amplitude. Therefore, we define the sensitivity as s = ∂IAC/∂Zel. In our experiment, ∂Zel is directly related to the microparticle displacement ∂Zel = p*∂d. The proportionality constant p is independent on the sensor configuration (OECT vs microelectrode) and we obtain its numerical value by fitting the microelectrode impedance spectra (see Supp. Inf S2). Accordingly, the sensitivity is given by the slope of the approach curves shown in Figure 1e. We obtain numerical values for this particular case (WxL = 100x100 µm) of sOECT = (0.059±0.002) nA/Ω and sµE = (0.023±0.006) nA/Ω. The values show a greater sensitivity in the OECT device with respect to the microelectrode, due to the contribution of OECT channel current to the AC response.\n\nQuantitative model for PEDOT:PSS-based impedance sensors: We developed an analytical model to express the impedance sensitivity s as a function of the sensor operation conditions, material properties and geometry. Objective is a quantitative understanding of the factors that increase sensitivity in OECT configuration with respect to PEDOT:PSS microelectrodes. Many studies decouple charge transport in OECTs in an electronic and an ionic circuit. A schematic of this representation is reported in Figure 2a, where the components of the electronic and the ionic circuit are indicated in blue and orange, respectively. Electronic charge carriers (holes) are driven by the drain voltage VD,DC and carry the channel current in an OECT, while ionic charge carriers are driven by the gate voltage VG = VG,DC + VG,AC and modulate the concentration of holes and, consequently, the electronic conductivity of the transistor channel. The limited conductivity of the electrolyte as well as the presence of dielectric objects close to the sensor surface generate an impedance Zel which causes a potential drop in the electrolyte, and the voltage at the electrolyte/channel interface VG* can be considered as the effective gate voltage that acts on the channel and determines the drain current. For the impedance sensing we are interested in the AC response of the transistor and we express the AC current flowing in the OECT channel as Ich,AC = gm,AC*VG*,AC. Following Bernards model, gm,AC can be expressed as gm,AC^lin = -W/L µp cv t VD,DC and gm,AC^sat = -W/L µp cv (VG,DC - Vt) in linear or saturation conditions. In these expressions, W, L and t indicate the width, length and thickness of the sensor channel, µp the holes mobility, cv the volumetric capacitance of PEDOT:PSS and Vt the OECT threshold voltage.\n\nTo derive the overall AC current, it is important to note that in AC transport conditions the source (and drain) current signals are composed of two contributions:\n$$\n{I}_{S,AC }= {I}_{ch,AC } + {f}_{OECT}\\\\bullet {I}_{G,AC } \\quad (1)\n$$\nThe first (Ich,AC) originates from the channel current, whereas the second (IG,AC) is due to the gate current and regards the capacitive current that has increasing importance at higher frequencies. Its value is given by IG,AC = VG,AC / ZG in which ZG = Zel + Zch is the overall impedance of the sensor given by the series combination of the electrolyte impedance Zel and the impedance related to the PEDOT:PSS channel capacitance Zch = 1/(iω Cch). The channel capacitance can further be related to the geometry and the volumetric capacitance of the PEDOT:PSS layer: Cch = cv*W*L*t. Possible contributions due to parasitic capacitances are neglected for simplicity. The factor fOECT in eqn. 1 determines how the gate current is distributed between the source and the drain terminal and is typically assumed to be equal to 0.5. Several studies demonstrate that the fOECT factor is slightly dependent on VD,DC, and VG,DC as well as on channel geometry. For this reason, fOECT was not assumed as constant in this experiment, but its value was set for each sensor in order to best fit the experimental data with the model.\n\nThe figure of merit of the OECT as impedance sensor (the sensitivity sOECT) indicates its capability to transduce a variation of Zel in a current output. This can be calculated from the model by differentiating eq. (1):\n$$\n{s}_{OECT }= \\\\left|\\\\frac{\\\\partial ({I}_{ch,AC}+{f}_{OECT}{I}_{G,AC})}{\\\\partial {Z}_{el}}\\\\right|=|{s}_{ch}+{f}_{OECT}\\\\bullet {s}_{\\\\mu E}| \\quad (2)\n$$\nAfter inserting the expressions for the two AC current contributions and differentiation we obtain for the channel sensitivity:\n$$\n{s}_{ch}=\\\\frac{{g}_{m,AC}}{{Z}_{G}}\\\\left(1-\\\\frac{{Z}_{el}}{{Z}_{G}}\\\\right){V}_{G,AC}\n$$\nand the sensitivity of the microelectrode is:\n$$\n{s}_{\\\\mu E}= \\\\frac{{V}_{G,AC}}{{Z}_{G}^{2}} \\quad (4)\n$$\nThe suitability of this simple approach to model the AC response of an OECT is demonstrated in Figure 2b and c. Figure 2b compares the frequency response of an OECT and of a microelectrode with the model predictions. The PEDOT:PSS channel width and length are W = 100 µm and L = 100 µm, respectively. The channel capacitance and the electrolyte impedance Zel were extracted for each device geometry by fitting the microelectrode impedance spectrum. The average volumetric capacitance of PEDOT:PSS resulted to be cv = (30.0 ± 1.3) F/cm³, obtaining a result consistent with literature findings. The OECT device shows a significantly higher current in the low frequency domain. Here the electronic channel current Ich prevails, and the transistor demonstrates clear amplifying properties. Then, above a cutoff frequency fc = 645 Hz, the transistor response is limited by the slow ionic transport between the channel and the electrolyte. At the same time the microelectrode’s response increases with frequency until a current limitation is reached due to the electrolyte impedance. As a consequence, in the high frequency limit both impedance sensor configurations yield the same current response. Importantly, the cutoff frequency that determines the OECT amplification is determined by the channel geometry as demonstrated in Figure 2c. The plot of the current amplitude versus frequency for OECTs with different channel sizes clearly shows that with increasing channel area and length a strong reduction in fc is observed.\n\nFinally, we systematically study the OECTs sensitivity towards electrolyte impedance changes with the microsphere experiment introduced above. Figure 2d shows the measured values for sOECT obtained for three different channel geometries at different AC frequencies. Eq. 2 is in excellent agreement with the frequency dependence of the measured data. In the low-frequency range the sensitivity shows a linear increase with frequency until it reaches a sensitivity maximum sOECT^max. Beyond the maximum, a smaller decrease in sensitivity is observed until it settles to a constant value for high frequencies. It is important to highlight that the position of sOECT^max corresponds to the device cutoff frequency fc (see Supp. Inf. S3 for the full mathematical treatment), and hence is a geometry-dependent parameter.\n\nIn Figure 2e we compare the sensitivity of a microelectrode and an OECT with the same dimensions (WxL = 200x50 µm). The transistor amplification, which is significant at low frequencies, has a relevant impact on the sensitivity. However, at high frequencies the response of both devices is limited by the electrolyte resistance and no significant differences are present. Such an observation is reflected by a frequency dependent OECT gain, which can be directly calculated with our model from eq. 2 and 4:\n$$\n{gain }_{OECT}= 20\\\\bullet {{log}}_{10}\\\\left(\\\\frac{{s}_{OECT}}{{s}_{microel}}\\\\right) \\quad (5)\n$$\nThe OECT gain is highest in the low-frequency regime, but is still significant in the 0.1-10 kHz range, where the impedance of the cell layers is typically measured. This justifies the use of a transistor structure for high precision bioelectronic impedance sensing experiments. Figure 2f demonstrates that the OECT gain is a geometry-dependent parameter. The smallest device (WxL = 50x50 µm) shows the highest gain, while a rectangular channel geometry is preferable for OECTs with the same area, since the gain is proportional to W/L ratio.\n\nSingle cell impedance sensor experiment: We demonstrated the value of the mathematical model here proposed for the optimization of a PEDOT:PSS-based single cell impedance sensor by monitoring single cell adhesion and detachment in an in-vitro experiment, simultaneously measuring the impedance changes with both an OECT and a microelectrode. According to the model prediction and the AFM experiment, we patterned the device channels with a 200x50 µm rectangular geometry, which provides the best performances in terms of sensitivity. The T98G cell line cultured in Minimum Essential Medium was diluted to have a final density of 1 x 10³ cells/cm³ and poured on the surface of the impedance sensors (see the Methods section for full details). After seeding, the cells reached the underlying substrate by gravity. We microfabricated a linear array of 10 PEDOT:PSS channels (see Supp. Inf. S4) to largely increase the probability of a single cell settling onto a sensor. An optical image of the final experimental configuration is reported in Figure 3a, showing a single T98G cell positioned at the center of the PEDOT:PSS channel. The encapsulation of the metallic electrodes with negative photoresist insulates the device from all the remaining cells which are not lying in the PEDOT:PSS active layer. We acquired the current spectra of both the OECT and the microelectrode at consecutive time intervals to make a real-time detection of the cell adhesion process. To stress the full consistency of the measurements acquired with the OECT and the microelectrode, we plot in Figure 3b the current amplitudes measured at 625 Hz as a function of time. The sensing frequency was selected in correspondence to the OECT cutoff (measured at time t=0), where the model indicates the maximum sensitivity. The signals acquired at the beginning of the experiment are stable around a maximum value. Afterwards, at time t=20 min the current start to decrease, indicating the beginning of the cell adhesion process. This produces a rapidly varying response until t=60 min, when the decrease becomes slower, and the current stabilizes around a minimum value. At t=200 min, we used a cell dissociation agent (trypsin) to completely remove the cell from the sample surface, and devices recovered their original current amplitude.\n\nWe report in Figure 3c the full current spectra acquired before and after the treatment with trypsin (t=180 min and t=240 min, respectively). The cell adhesion produced a large shift of the OECT low-pass cutoff towards smaller frequency. In parallel, the current spectrum of a control device placed in the same reservoir, but with no cell seeded on the PEDOT:PSS layer, remained unaltered (see Supp. Inf. S5). After trypsinization, the initial cutoff frequency is fully recovered. These combined observations clearly demonstrate that the cutoff shift is only caused by the single cell adhesion on the PEDOT:PSS layer. The same considerations can be extended to the PEDOT:PSS microelectrode. Here, the cell adhesion process is revealed by a decrease in the gate current amplitude, which reaches its minimum at t=180 min, coherently with the OECT measurements. After the cell detachment (t=240 min), the current increases to its original values.\n\nTo provide a direct comparison between the sensing performances, we averaged the current amplitudes acquired when the cell is detached (t<30 min and t=240 min) and attached (1205\n\nImportantly, our quantitative approach to compare bioelectronic impedance sensors is not limited to PEDOT:PSS based OECTs but can easily be extended to different water gated transistor architectures. The crucial parameter that describes the different material properties in our model is the channel transconductance. Large transconductances have been demonstrated for different channel materials and device architectures. They result from high capacitive couplings, as observed in organic mixed ionic and electronic conductors (e. g. PEDOT:PSS) or high carrier mobilities as found for example in graphene or carbon nanotubes.86 Current research in the material properties of such water stable semiconductors warrants further improvements in mobility or volumetric capacitance and will also augment the sensitivity of bioelectronic impedance sensors.26 Our quantitative approach can serve as a guideline for the development of impedance sensors with maximized sensitivity and establishes a metric to compare future devices.\n\n# Methods\n\n**Device fabrication**: Glass substrates (50×25 mm2) were cleaned by sonication in water and soap (10%)/acetone/isopropanol/distilled water baths. After a dehydration step (10 minutes at 110° C), the Microposit S1818 positive photoresist was spin coated (4000 rpm for 60 s) and annealed at 110°C for 1 minute. Metallic contacts were patterned through direct laser lithography by using the ML3 Microwriter (from Durham Magneto Optics). The photoresist was developed with Microposit MF-319 developer. Then, 10 nm of chromium and 25 nm of gold were deposited by thermal evaporation. Samples were immersed in acetone for 4 hours for photoresist lift-off. Metallic contacts were encapsulated with the mr-DWL 5 negative photoresist (from Micro Resist Technology). The resin was spin coated at 3000 rpm for 30 s and annealed at 100°C for 2 minutes. After laser exposure, samples were baked at 100°C for 2 minutes and relaxed for 1 hour at room temperature. Development was performed with mr-Dev 600 developer (Micro Resist Technology), and the resist was finally baked at 120°C for 30 minutes. A double layer of S1818 was deposited and treated for 6 minutes in chlorobenzene for the photolithography of the PEDOT:PSS channel.37 After the development, substrates were treated with air plasma (15 W for 2 min) and the PEDOT:PSS solution (94% PEDOT:PSS (Heraeus, Clevios PH1000), 5% of ethylene glycol (EG) (Sigma Aldrich), 1% of 3-glycidoxypropyltrimethoxysilane (GOPS), and 0.25% of 4-dodecylbenzenesulfonicacid (DBSA)) was spin coated at 3000 rpm for 10 s. The resulting film thickness was (100 ±10) nm. The samples were subsequently annealed at 120°C for 1 h, and S1818 was finally lifted-off after 4 hours in acetone.\n\n**Electrical measurements**: DC characteristics of the OECTs were carried out with the Keysight 2912A source-measure unit (SMU), using a Ag/AgCl wire as gate electrode. The acquired data were analyzed to set the working point of the transistor during impedance sensing, i.e. the DC gate and drain voltages at which the transconductance *g**m,DC* assumes its maximum value (Supp. Inf. S1). AC measurements were performed with the MFLI lock-in amplifier (from Zurich Instruments). A constant DC offset voltage and a sinusoidal oscillation (amplitude 10 mV) with desired frequency were applied to the gate terminal. The resulting AC current flowing in the PEDOT:PSS channel was demodulated to acquire the current amplitude of the impedance sensors. In the OECT configuration, a constant DC voltage was applied between the source and the drain electrodes to bias the device at its working point. The microelectrode configuration was obtained by shorting the drain and the source terminals.\n\n**Microparticle sensing experiment**\n\nTo fabricate the AFM probe supporting the dielectric microparticle, we dispersed a powder of pyrophosphate microspheres (Polymat) on a glass slide. A PPP-NCHR cantilever of the Park NX10 AFM (force constant 34.55 N/m) was approached onto a drop of glue, and then put in contact with the upper part of a microsphere (with diameter of about 50 µm) until complete adhesion.\n\nAFM measurements were performed in liquid, using 0.1 *m* PBS as electrolyte and an Ag/AgCl wire as gate electrode. To measure the current-distance spectroscopies, we placed the microparticle in the center of the PEDOT:PSS channel of the impedance sensor and we performed an AFM force-distance spectroscopy. The probe was lifted to the vertical coordinate *z*0, distant 5µm from the contact position, then gradually approached to the sample surface (scan speed 0.3 µm/s), and finally retracted again to *z*0. During this process, we applied a constant modulation frequency to the gate terminal, and we measured the current amplitude flowing in the PEDOT:PSS layer, obtaining a current-distance spectroscopy curve. The experiment was repeated at 5 different frequencies (117, 330, 1170, 3330, and 11700 Hz) both in the OECT and in the microelectrode configurations.\n\n**Single cell detection experiment**: The human malignant glioma cell line, T98G (CRL-1690™), derived from a glioblastoma multiform tumor, was selected for the single cell detection experiment. This is characterized by indefinite lifespan and adherence properties previously reported also on PEDOT:PSS layers.38 It was purchased from ATCC (Manassas, VA, USA) and cultured in Minimum Essential Medium (MEM) (Gibco™ 51200046, ThermoFisher scientific), supplemented with 10% fetal bovine serum, 1% L-glutamine, 10% sodium pyruvate and antibiotics (1% penicillin and 1% streptomycin) at 37°C in 5% CO2 incubator. All chemicals were from Merck. The experimental day, the sub-confluent (70-80%) cells population was detached by 0.25% trypsin in 0.02% EDTA (both from Merck) solution, re-suspended in fresh supplemented MEM and counted by the hemocytometric chamber. An aliquot, calculated to have a final density of 1 x 103 cells/cm3 was diluted in 600 µL of supplemented MEM and poured on the surface of the impedance sensors, previously sterilized by 20 min of UV exposure. A polydimethylsiloxane (PDMS) well was attached onto the sample substrate to host both the solution containing the cells and the Ag/AgCl gate electrode. After seeding, the cells reached the underlying substrate by gravity. For the experiment, we microfabricated a linear array of 10 PEDOT:PSS channels with dimensions WxL=200x50 µm (an optical image is reported in Supp. Inf. S4). In this way, the probability of a single cell falling onto a device channel after seeding was largely increased. Once this configuration was achieved, the sample was connected for the electrical measurements. The current spectra of the impedance sensor were acquired both in the OECT and the microelectrode configurations every 10 minutes after cell seeding. During each acquisition, the modulation frequency applied at the gate terminal was swept between 10 and 105 Hz. At time *t* = 200 min, trypsin was used to completely remove the cells from the sample surface. 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Interfaces **9**, 6679–6689 (2017).\n\n# Supplementary Files\n\n- [SuppInf.docx](https://assets-eu.researchsquare.com/files/rs-1307502/v1/826dbf0657f8746e7cf8fee3.docx) \n Supplementary Information"} {"paper_id": "prb83", "title": "Self-powered, ultraflexible photonic skin for continuous bio-signal detection via air-operation-stable polymer light-emitting diodes", "text": "# Abstract\n\nFlexible organic optical devices have been used extensively in next-generation wearable electronics owing to advantages such as light-weight, thinness, and flexibility. Making such organic optical devices ultrathin enables long-term monitoring of health conditions owing to the increased conformability of ultrathin devices to human skin. Long-term biological signal monitoring also requires the integration of organic optical devices with an energy harvesting power sources which does not require recharging; to make devices self-powered. However, system-level integration of such thin organic optical sensors with power sources is challenging. An important obstacle to this type of integration is the insufficient operational stability of ultrathin organic light-emitting diodes under ambient air conditions. Here we develop an ultrathin self-powered organic optical system for photoplethysmogram (PPG) monitoring. This system consists of three types of ultrathin electronic devices: polymer light-emitting diodes (PLEDs), organic solar cells, and organic photodetectors. By adopting an inverted structure and a polyethylenimine ethoxylated layer doped with 8-hydroxyquinolinato-lithium as the electron-transport layer, PLEDs exhibit improved operational stability under ambient air conditions without external encapsulation. Ultraflexible PLEDs with no passivation retain 70% of the initial luminance lifetime of 11.3 h under ambient air. Integrated optical sensors exhibit a high linearity with the light intensity exponent of 0.98 by PLED light source. Such self-powered, ultraflexible PPG sensors can perform long-term stable monitoring of blood pulse signals on human hands.\n\nElectronic Materials and Devices \nElectrical Engineering \nphotonic skin \ncontinuous bio-signal detection \nlight-emitting diodes\n\n# Introduction\n\nOrganic semiconducting devices have been used extensively in next-generation wearable electronics because of their light-weight, thinness, and flexibility [1–3]. Flexible displays consisting of organic light-emitting diodes (LEDs) have been installed in smartwatches and wristband-type applications, contributing to a reduction in power consumption [4]. In addition, an all-organic optoelectronic sensor has been developed for pulse oximetry, by integrating organic LEDs and organic photodetectors [5]. Imparting flexibility to such organic optical sensors enables long-term monitoring of health conditions with reduced discomfort when these sensors are attached directly on human skin.\n\nRecent advances in the field of flexible optical integrated devices have made these devices favourable for optical sensor applications, such as photoplethysmogram (PPG) [6]–[10], pulse oximetry [10]–[12]. High-resolution imaging devices have been used in advanced applications, such as vein authentication [13, 14], fingerprint imaging [13, 15], and X-ray imaging [16, 17]. Self-powered systems such as thermoelectric conversion devices [18] and organic solar cells [19] have been developed by integrating organic optical sensors and flexible energy-harvesting devices. Another approach involves combining organic LEDs with battery modules to develop a patch system for photobiomodulation that can be used for wound healing [20].\n\nIn addition to integrated devices, devices with improved conformability to biological tissues are necessary for stable long-term monitoring of biological signals. Conformability can be achieved by combining two approaches: using soft materials having Young’s moduli similar to biological tissues, and reducing total device thickness [21]. Thanks to smaller Young’s moduli of organic materials compared to inorganic materials, and the compatibility of organic devices to low-temperature and solution processes, the total thickness can be reduced to 1–2 µm without sacrificing the device performance leading to the reduction of discomfort on the skin [22]–[25]. An ultrathin organic optical sensor has been developed with several microns thick [26]–[29].\n\nHowever, system-level integration of such thin organic optical sensors with power sources remains challenging. An significant obstacle to this type of integration is the insufficient operational stability of ultrathin organic LEDs under ambient air conditions [26]–[28], which hinders the long-term monitoring of biological signals.\n\nHere we propose an ultrathin self-powered organic optical system for plethysmogram monitoring. This system consists of three ultrathin electronic devices: polymer light-emitting diodes (PLEDs), organic solar cells, and organic photodetectors. By adopting an inverted structure and a polyethylenimine ethoxylated (PEIE) layer doped with 8-quinolinolato lithium (Liq) [30] as the electron transport layer (ETL), organic light-emitting diodes exhibit improved operation stability under ambient air conditions. Because of the intrinsic air operational stability of inverted PLED with PEIE:Liq electron injection layers, the fabricated ultraflexible PLED with no passivation retains 70% of its initial luminance lifetime of 11.3 h under ambient air, which is more than three times the luminance lifetime of conventional ultraflexible PLEDs. Integrated optical sensor exhibits a high linearity with the light intensity exponent of 0.98 by PLED light source. Such self-powered, ultraflexible PPG sensor shows a blood pulse monitoring during 7 s and can detect blood pulse rate of 77 beats per minute (bpm) on human hands.\n\n# Air-operation-stable Pleds\n\nFigure 1a and Supplementary Fig. 1 shows a schematic and photographs of ultraflexible, self-powered, PPG sensor operated on a human hand. The PPG sensors consisted of two types of ultraflexible devices: an ultraflexible PLED and ultraflexible organic photodiodes (OPD) (Supplementary Fig. 2). The ultraflexible PPG sensors and organic photovoltaic (OPV) modules were connected with flexible gold wiring, which was a 100-nm-thick gold electrode fabricated on a 12.5-µm-thick polyimide film (Fig. 1b). A top-view image of an OPV module and a PPG sensor are shown in Fig. 1c, and 1d, respectively. Figure 1e shows a schematic of the electrical circuit of a self-powered PPG device. The PLEDs were powered by ultraflexible OPV modules, and PPG data obtained from the OPD was transferred to the oscilloscope. The PLEDs were fabricated on a 1.5-µm-thick flexible substrate made with a 1-µm-thick parylene substrate and a 500-nm-thick planarisation layer of SU-8. The PLED comprised stacked layers of ITO/Zinc oxide (ZnO) /PEIE:Liq/Super Yellow (SY)/MoX/Al (Fig. 2a).\n\nA polymer of SY was used as the emission layer, providing highly efficient light emission [31]. To achieve air-stable operation of the PLED, an inverted structure was introduced with an electron injection layer of Liq-doped PEIE. While the inverted structure allows the use of an air-stable cathode in PLEDs and improves the air stability of PLEDs [32], doping PEIE with Liq can significantly improve the operational stability of PLEDs. To optimize the doping concentration of PEIE with Liq, the effect of the Liq wt% on the inverted PLED was examined (Supplementary Fig. 3). The J–L–V characteristics of the PLED show comparable electrical and optical outputs (> 10⁴ cd m⁻² at 10 V of applied voltage) for each doping concentration (Supplementary Fig. 3a and 3b). As shown in Supplementary Fig. 3c, 30 wt% of Liq was observed to be an optimal ratio in terms of current efficiency. For the air-operation stability, 10 wt% and 30 wt% of Liq show longer lifetime to be half of initial luminance (Supplementary Fig. 3d). Supplementary Fig. 3e summarises the variations in the efficiency and lifetime of the PLED with varying doping concentrations of Liq in the PEIE layer. From these results, we concluded that 30 wt% is the optimal Liq doping concentration to achieve an air-operation-stable inverted PLED. Therefore, the PEIE layer doped with 30 wt% Liq was used as the ETL for successive experiments. While the WF of PEIE:Liq shifts to the shallower level until the concentration of Liq up to 50 wt%, WF shifts back to the deeper level after the concentration of Liq over 50%. This WF shifts correspond to the electron injection of the PLED, which is improved by WF shifts to the shallower level. As a result of WF shift, 30 wt% showed the best result of efficiency [30]. The device stabilities under constant 8-V operation in ambient air were compared between various reported structures and ETLs (Supplementary Fig. 4). As a conventional structure, ITO/Poly(3,4-ethylenedioxythiophene)-poly(styrenesulfonate) (PEDOT:PSS) /SY/NaF/Al was used. As inverted structures with different ETLs, ITO/ZnO/SY/MoX/Al, ITO/ZnO/Poly-ethylenimine (PEI) /SY/MoX/Al, and ITO/ZnO/PEIE:Liq/SY/MoX/Al were compared. While the inverted structure with PEI layers initially showed an efficient luminance of 5 cd A⁻¹, its air stability became lower than that of the structure without PEI layers. The conventional structure showed a relatively stable luminance for up to 200 min, after which its luminance decreased abruptly. The PEIE:Liq layer showed the best air-stability among all the examined PLED structures. A comparison of the current efficiencies of various inverted-structure PLEDs is shown in Supplementary Fig. 5. We chose F8BT as a conventional emission layer polymer and PEI as a conventional ETL polymer. When the current efficiency of the inverted-structure PLED with F8BT and PEI reached 3.4 cd A⁻¹, the current efficiencies of the inverted-structure PLED with SY and PEI and that with SY and PEIE reached 6.9 cd A⁻¹ and 11.7 cd A⁻¹, respectively. The operational lifetime and turn-on voltage of the inverted PLED with PEIE:Liq and SY were compared to those in previous studies (Fig. 2b) [28, 33–45]. The inverted PLED has an excellent half luminance lifetime of 41.5 h with 8-V operation in ambient air without encapsulation, while maintaining a low turn-on voltage (4.7 V). Turn-on voltage is determined as the voltage at which the luminance reaches to more than 1000 cd m⁻². Also, their angular distribution follows with Lambert's cosine law, which means our PLED has almost ideal diffusely reflecting surface (Supplementary Fig. 6).\n\nAfter the characteristics of the inverted PLED on the glass substrate were examined, the inverted PLED on the ultraflexible substrate was fabricated. When the PLED was fabricated on an ultraflexible substrate, it showed a turn-on voltage of 4.7 V, which is equal to that of the PLED on the glass substrate (4.7 V) (Fig. 2c). Figure 2d shows the ultraflexible inverted PLED during 6-V operation in air. As shown in Fig. 2e, the ultraflexible PLED exhibits a current efficiency of 14 cd A⁻¹ at a current density of 24 mA cm⁻²; this efficiency is comparable to or even higher than that of the PLED on the glass substrate. The EQE of PLED on ultraflexible substrate also shows comparable value to that on glass substrate (Supplementary Fig. 7). The mechanical durability of ultraflexible PLED was evaluated with the cyclic bending test. In the cyclic bending test, the ultraflexible PLED was bent cyclically to the bending radius of 5 mm. The results of the bending test is shown in Supplementary Fig. 8. Even after the device was bent cyclically with 50 times, the J-V curves did not show any degradation (Supplementary Fig. 8). Also, the luminance of PLED still remains 982 cd/m² which is comparable value as that of the initial value (918 cd/m²) after the 50 cyclic bending (Supplementary Fig. 8b). Finally, to evaluate the operational stability under ambient air, the operational lifetimes of the PLEDs on both substrates under ambient air were evaluated under a constant current of 8 mA cm⁻² (Fig. 2f). The inverted PLED on the glass substrate showed lifetime for 70% of initial luminance as 14.7 h. In the inverted PLED encapsulated with a 1-µm-thick parylene layer, the air-operation stability of the PLED improved to 33.4 h. When the PLED was fabricated on the ultraflexible substrate, the lifetime for 70% of its initial luminance decreased to 11.3 h. This is because of the low gas barrier property of ultraflexible substrates compared with that of glass [46]. Although the lifetime of the ultraflexible PLED was lower than that of the PLED fabricated on glass, it was still more than three times to the lifetime of a conventional ultraflexible PLED, which is 4 h [28]. To assess the reason of non-diode behaviour of our ultraflexible PLED (Fig. 2c), surface morphology of the PLED interface layer was studied by using atomic force microscope (AFM) (Supplementary Fig. 9). In the AFM images, the morphological difference clearly observed between bare ITO surface and ZnO interface layer (Supplementary Fig. 9a and b), which shows surface roughness increase in ZnO layer. However, addition of Liq into ZnO layer does not affect morphology dramatically (Supplementary Fig. 9b and c). These results proof us that the ZnO layer is a main contribution for increasing roughness, which would result in the non-diode behavior of our ultraflexible inverted PLED.\n\n# Ultraflexible Organic Photodetectors\n\nFor an ultraflexible OPD, a blended film of PTzNTz-BOBO and PC71BM is used as the active layer. A stack of ITO/ZnO/PTzNTz-BOBO:PC71BM/MoOx/Ag was chosen as the OPD structure in this study (Fig. 3a). To use OPD as an application of PPG sensors, linearity factors determined by using the input light intensity (*L*), short circuit current (*J*SC), logarithmic *L*, and open-circuit voltage (*V*OC) are required [13]. Thus, the linearity of the OPD was examined for several light sources, such as simulated sunlight and light emitted from PLEDs. The dependence of the light intensity on *J*SC and *V*OC for the OPD, with simulated sunlight, is shown in Fig. 3a. The red dashed line and blue dashed line in Fig. 3b represent linearly fitted lines for *L* and *J*SC and for *L* and log(*V*OC), respectively. The *J*SC of OPD and the *L* of simulated sunlight were fitted with the equation , in which A is a constant value determined using the power-conversion efficiency (PCE) of the OPD. α is the light intensity exponent, which indicates the linearity and accuracy of the OPD’s response to the input light intensity. The α calculated from the experimental result was 0.95 for sunlight. The obtained value of α for sunlight was excellent because the value was quite close to the theoretical limit (1) of linearity of the OPD. Additionally, the external quantum efficiency (EQE) of the OPD at wavelengths of 300–900 nm was measured (Fig. 3c). The electroluminescence (EL) spectra of the ultraflexible inverted PLED are also shown in Fig. 3c. The EQE results represent broad light conversion of the OPD from 300 nm to 800 nm. The EL spectra of PLED had a peak wavelength of 590 nm and the width ranging from 500 nm to 800 nm. These results prove that the EQE spectra of the OPD and the EL spectra of the PLED are considerably overlapped over a range of wavelengths; thus, the fabricated OPD is capable of efficiently absorbing the light emitted from the ultraflexible PLED. The EL wavelength of our PLED has favourable properties to PPG because of their penetration depth. Since our body tissues have a greater absorption in yellow/green wavelength [47], the penetration depth of yellow/green light is shorter compared to that of infrared. Thus, the yellow/green light will suppress the artifact of the reflection and scattering from deeper tissue and leads advantageous light properties for reflection-mode PPG [48–51]. To ensure efficient and accurate PLED light detection, the linearity of the OPD with the input PLED light was examined, as shown in Fig. 3d and Fig. 3e. *L* and *J*SC were fitted well with the same equation as used in the sunlight experiment. The α with PLED light was calculated as 0.98 which proves that our OPD can accurately measure the light intensity of the PLED. The frequency response of the OPD was examined (Supplementary Fig. 10a). The rising time and falling time were calculated as 1 ms, respectively, which is fast enough to measure blood pulse with the frequency around 1 Hz (Supplementary Fig. 10b, c). The mechanical durability of ultraflexible OPD was evaluated with the cyclic bending test. Even after the device was bent cyclically with 150 times, the *J-V* curves did not show any degradation as a difference in the current density of light state and dark state (Supplementary Fig. 11a). The *J*SC difference between light state and dark state maintains the value of 2.15 mA/cm2, which remains 98% of the initial value before bending (Supplementary Fig. 11b). Also, our ultraflexible OPD shows excellent storage stability up to 100000 min under ambient air (Supplementary Fig. 12). The excellent air stability proofs a favourable characteristics of our ultraflexible OPD for self-powered devices. The OPD and PLED were used for the PPG sensor in further experiments.\n\n# Self-powered Ultraflexible Ppg Sensors\n\nA sufficient output power from the OPV is required to drive the PLED and make the PPG sensor self-powered. In order to increase the output power and voltage of OPV single cells, OPV modules containing several OPV single cells were designed and optimized. To optimize the OPV module design, the output current and voltage of the OPV module for varying numbers of series connections were calculated from the single-cell characteristics. The output current and voltage were calculated as \n$$I_{OUT}=0.8\\times \\frac{I_{SC}}{n}$$ \n, \n$$V_{OUT}=0.8\\times V_{OC}\\times n$$ \n, in which $I_{SC}$ is the short-circuit current of the single cell; $V_{OC}$ is the open-circuit voltage of the single cell; and $n$ is the number of series-connected single cells that constitute the module. $J_{SC}$ and $V_{OC}$ are multiplied by 0.8 to compromise typical value of fill-factor as 0.64 of OPV modules. Making the output current and voltage of the OPV modules equal to that of the PLED is crucial for efficient operation of self-powered PPG sensors. The results of the calculation indicated that OPV modules with 10 series-connected single cells have the highest overlap with the $I–V$ characteristics of the PLED (Supplementary Fig. 13). Based on this observation, OPV modules with series numbers of 6, 8, and 10 were fabricated (Supplementary Fig. 14a–c). In the OPV modules, $I_{OUT}$ decreased and $V_{OUT}$ increased proportionally as the increase in the number of series connections. As the maximum output powers of all the OPV modules became similar, the voltage required to obtain the maximum power point increased proportionally with an increase in the number of series connections (Supplementary Fig. 14d). The constant output power characteristics were examined by keeping the total area of the module, which is the area of individual cells multiplied by series number, constant (1.2 cm²) for every OPV module in this experiment. The operational point of the PLED powered by the OPV module was examined by overlaying the reversed $I–V$ curves of PLED with the $I–V$ curves of the OPV module (Supplementary Fig. 14e). From the results, the number of series connections required for the optimal OPV module design was calculated to be 10. This finding was similar to the result obtained from the previous calculation using single-cell properties; hence, we concluded that having 10 series connections is optimal for PLED operation. Hence, OPV modules with 10 series connections were fabricated on an ultraflexible substrate (Supplementary Fig. 15a and 15b). These ultraflexible OPV modules exhibited a PCE of 5.8%, which is comparable to the PCE of the module on the glass substrate (6.5%) (Supplementary Table 1). The operational stability of our OPV modules under air is also important. The ultraflexible OPV cells with same material showed 90% of initial PCE even after 3 h continuous 1-sun illumination with maximum power point (MPP) tracking test under ambient air, which indicates our OPV module should also has comparably stable characteristics under MPP tracking [52].\n\nSubsequently, PLED operation with a 10 series connected OPV module was experimentally examined. Simulated sunlight with a neutral density filter and with various optical densities was used as a variable-intensity input light source. A photograph depicting PLED operation with the OPV, and a schematic of the electrical circuit with the PLED and OPV are shown in Supplementary Fig. 16a and 16b, respectively. The light-intensity dependences of the OPV modules were measured and overlaid with the PLED $I-V$ curve (Supplementary Fig. 16c). From the results of Supplementary Fig. 16c, circuit current of PLED and OPV were expected to increase with the increase in the input light intensity. Supplementary Fig. 16d shows the experimentally measured dependence of the circuit current and PLED luminance on the light intensity. As expected, circuit current and luminance proportionally increased with the increase in the light intensity. The PLED was observed to emit bright light with an input light intensity of about 5000 µW/cm², which is 0.05 times the intensity of sunlight (Supplementary Fig. 16e). The PCE of OPV under indoor light shows 28.1% with 1000 lux of fluorescent lamp illumination [53]. This value is equivalent as power output of 78.2 µW/cm² whereas power output under 5000 µW/cm² simulated sunlight is 290 µW/cm². With these results, our self-powered PPG system should work under 1000 lux of indoor light with OPV modules of 4.5 cm² device area.\n\nFinally, the operation of the self-powered PPG sensor was demonstrated. The operation mechanism of a PPG sensor is shown in Fig. 4a. When light is emitted from the PLED and penetrates the finger, a part of the light is reflected at the blood vessels, while the remaining part is absorbed into the blood. The volume of blood vessels changes with every blood pulse, and the intensity of the reflected light is consistent with the volume pulsation of the blood vessel. The intensity of the reflected light can be detected by an OPD placed on the finger, and the blood pulse rate can be calculated from the OPD signals [5]. First, a self-powered PPG sensor consisting of an OPD, PLED, and OPV module on a glass substrate was fabricated and examined. The PLED was powered by an OPV module with 10 series connections, and the OPV module was illuminated with simulated sunlight of one-sun intensity. The PLED switched on when the OPV module was exposed to the sunlight, and it switched off when the OPV module was stored in the dark. Supplementary Fig. 17 shows the OPD signals when the PLED light was switched on and off by intermittently exposing the OPV module to the simulated sunlight. When the PLED light switched off, the OPD showed an almost constant voltage, as indicated by the black line in Supplementary Fig. 17. However, the OPD showed a clear periodic peak at 1.2 Hz, which is the frequency of the blood pulse, when the PLED was turned on. As shown in Fig. 4b, our PPG sensor performs very stable signal detection, even when the measurement duration is 20 s. The raw data of PPG signal without signal filtering also shows a large artifact in the low frequency (Supplementary Fig. 18). Also, there should be certain artifact from the body and finger movement. Therefore, there will be a certain challenge in the external circuit to process signal during the measurement and to monitor the signal continuously for the long-term measurement.\n\nAfter the self-powered PPG detection was confirmed to be operational on the glass substrate, self-powered PPG sensors on an ultraflexible substrate were fabricated. For this fabrication, previously reported lamination methods with 6 µm-thick adhesive tape¹ were used to combine the ultraflexible OPV module, OPD, and PLED (Supplementary Fig. 19). A photograph of the ultraflexible, self-powered PPG sensor is shown in Fig. 4c. Finally, the PPG signals from the self-powered ultraflexible PPG sensor were measured (Fig. 4d). Based on the results, blood pulse frequency was calculated to be 77 bpm. Although the periodic signal of the OPD was visible in the result, a large noise in the detected signal was also observed. Some of the reasons for the high noise in the ultraflexible PPG sensor were the large leak current of the ultraflexible OPD and the weak light intensity of the ultraflexible PLED due to the limited power supply from the ultraflexible OPV module.\n\nThe reason of poor signal quality with ultraflexible PPG sensors might be the dark current increase of ultraflexible OPDs. While the previous research used the conventional structure OPD [28], this work used the inverted structure OPD with ZnO, which is air stable, but would have a higher rigidity and roughness [54], which would leads high dark current of OPD and poor signal quality of PPG. The active voltage regulator (AVR) circuit would be critical for stable power output in self-powered devices [55]. Since the AVR has an input voltage range from 7–15 V, the AVR have a feasibility to be combined with our 10 series-connected OPV module (8.2 V output) and regulate the voltage to 6.5 V for stable power output. Another critical requirement for self-powered device is the auxiliary battery, especially for their stable operation in dark situation. In Supplementary Fig. 20, the circuit with auxiliary rechargeable battery are explained. While the OPV module differs their current and voltage by the light intensity, the battery has stable current and voltage output and thus, the stable output light of PLED will be achieved. 180 µm-thick battery [56] and 40 µm-thick supercapacitor [57] would be used to achieve self-powered PPG sensors with auxiliary battery. Lastly, signal sampling is a critical problem for state-of-the-art flexible, self-powered electronics. In both an ultraflexible self-powered organic electrochemical transistor [58] and a flexible self-powered PPG sensor [56], the sampling systems were rigid ICs and separately connected as external circuits. Though our OPV module is capable to operate signal monitoring ICs because their power comsumtion is is ~ 0.2µW (TWILITE, Mono Wireless), certain effort is necessary to make these ICs ultraflexible and integrate to the self-powered systems.\n\n# Conclusion\n\nIn this study, a self-powered, ultraflexible PPG sensor employing air-operation-stable, ultraflexible PLEDs was fabricated. To the best of our knowledge, this is the first study that demonstrates the use of self-powered optoelectrical sensors in ultraflexible organic devices. This self-power technology used in this study will pave the wave of ultraflexible wearable optoelectronic devices which take an important role for future ubiquitous healthcare society.\n\n# Methods\n\n## Materials\nThe PTzNTz-BOBO samples were synthesised according to a previously reported procedure [59]. PC₇₁BM was purchased from Solenne BV Corporation. PEIE, Liq, Zinc acetate dihydrate, 2-methoxyethanol, and 2-aminoethanol were purchased from Wako Chemical. The yellow light-emitting polymer, SY, was purchased from Sigma-Aldrich. The glass substrate with a patterned ITO electrode was purchased from EHC Ltd.. The sheet resistance of ITO was <10 Ω/sq.\n\n## Ultraflexible Film Substrate Fabrication\nThe ultra-thin film substrates were composed of double-layered parylene (diX-SR, Daisan Kasei Co., Ltd.) and epoxy (SU-8 3005, MicroChem). First, a 1-μm-thick parylene layer was deposited via chemical vapour deposition (CVD) on a glass substrate whose surface was coated with a fluorinated polymer (Novec 1700, 3M). A 500-nm-thick epoxy layer was then spin-coated (5000 rpm for 60 s) on a 1-µm-thick parylene layer as the planarisation layer. The film was then annealed at 95 °C for 3 min after ultraviolet exposure. were annealed under a nitrogen atmosphere at 180 °C for 30 min. All ultra-thin devices were electrically connected with thin Au wiring on a 12.5-μm-thick polyimide substrate using anisotropic conductive film (3M, ECATT 9703) tapes as contact parts.\n\n## Inverted PLED Fabrication\nA 100-nm-thick ITO layer was subsequently formed as the transparent electrode by DC sputtering. The ITO electrodes were patterned via photolithography using a ZPN (Nihon Zeon) negative resist and an ITO-07N (Kanto Chemical) ITO etcher. A 20-nm-thick ZnO layer was used as the electron-transport layer. The substrates were spin-coated with a ZnO precursor (5000 rpm for 30 s) solution prepared by dissolving zinc acetate dehydrate (0.5 g) and ethanolamine (0.16 mL) in 5 mL 2-methoxyethanol [60]. The substrates were then baked in air at 180 °C for 30 min. To form PEIE:Liq layer, the mixture of 1.5 wt% solution of PEIE and Liq with 2-methoxyethanol was deposited on a substrate via spin-coating (4000 rpm 60 s). After annealing the substrate at 100 °C for 1 min, the device was rinsed with ethanol and annealed at 100 °C for 1 min again. The SY layer was deposited via spin-coating using a toluene solution of 6 mg/ml. Subsequently, the MoOₓ (10 nm) and Al (80 nm) layers were deposited via vacuum evaporation. Finally, a 1-μm-thick parylene layer was deposited via CVD to form a passivation layer.\n\n## OPV and OPD Fabrication\nA ZnO layer was deposited using the same methods as that used for the PLED. PTzNTZ-BOBO and PC₇₁BM were mixed as a 1:1.5 of weight ratio. Then, chlorobenzene was added to a mixture with 5 g L⁻¹ PTzNTZ-BOBO concentration. The solution was stirred at 100 °C for 1 h, and 1 vol% of 1,8-Diiodooctane was added based on the amount of chlorobenzene after the temperature of the solution decreased back to 20-30 °C in under N₂ atmosphere. The solution was spin-coated on the device in a glove box at 600 rpm for 20 s. The active layer thickness is 200 nm. MoOₓ (7.5 nm) and Ag (100 nm) were sequentially deposited via thermal evaporation, under a pressure of less than 1 × 10⁻³ Pa, as a top interlayer and an anode, respectively. Finally, a 1-μm-thick parylene layer was deposited via CVD to form a passivation layer.\n\n## Device characterisation\nThe OPV modules with a total cell area of 1.2 cm² and OPD with an active area of 0.04 cm² were characterised under one-sun illumination using a solar simulator (AM 1.5 global spectrum with 1000 W m⁻² intensity calibrated using a silicon reference diode, Bunkokeiki). The J–V characteristics were recorded using a Keithley 2400 source metre for every 10 mV in an ambient laboratory atmosphere, without humidity or temperature control (with an approximate temperature of 20 °C and humidity of 30% relative humidity (RH)). Accordingly, external gold wirings were used for the electrical contacts of the OPVs on the ultrathin substrates. The 100-nm-thick gold wirings were deposited under a vacuum through a shadow mask onto 12.5-μm-thick polyimide films. One side of the wirings were connected to the electrodes on the freestanding foils using an electrically conductive adhesive transfer tape (3M™, ECATT 9703). The other sides were connected to the source metre using alligator clips. Light power of the PLED was calibrated with optical power meter (1936-R, Newport).\n\nTo evaluate the PLED characteristics, a light distribution measurement system (C9920-11, Hamamatsu Photonics) and an external quantum efficiency measurement system (C9920-12, Hamamatsu Photonics) were used. For the air-stability tests, the devices were operated under ambient air (~20 °C, 30% RH). The measurements were also performed in an ambient atmosphere.\n\nTo perform the PLED operation experiment with the OPV as a power source, a solar simulator and an optical filter were used to modulate the light intensity for simulated sunlight input. A schematic of the experimental setup is shown in Supplementary Fig. 21. Anode of PLED and OPV module are electrically connected. 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Vohra, V. et al. “Efficient inverted polymer solar cells employing favourable molecular orientation.” *Nat. Photonics* **9**, 403–408 (2015).\n\n# Supplementary Files\n\n- [SIJinnno.docx](https://assets-eu.researchsquare.com/files/rs-117283/v1/6a32ce7968f49b86fa4409fd.docx)"} {"paper_id": "prb84", "title": "Skin-inspired, sensory robots for electronic implants", "text": "# Abstract\n\nLiving organisms with motor and sensor units integrated seamlessly demonstrate effective adaptation to dynamically changing environments. Drawing inspiration from cohesive integration of skeletal muscles and sensory skins in these organisms, we present a design strategy of soft robots, primarily consisting of an electronic skin (e-skin) and an artificial muscle, that naturally couples multifunctional sensing and on-demand actuation in a biocompatible platform. We introduce an *in situ* solution-based method to create an e-skin layer with diverse sensing materials (e.g., silver nanowires, reduced graphene oxide, MXene, and conductive polymers) incorporated within a polymer matrix (e.g., polyimide), imitating complex skin receptors to perceive various stimuli. Biomimicry designs (e.g., starfish and chiral seedpods) of the robots enable various motions (e.g., bending, expanding, and twisting) on demand and realize good fixation and stress-free contact with tissues. Furthermore, integration of a battery-free wireless module into these robots enables operation and communication without tethering, thus enhancing the safety and biocompatibility as minimally invasive implants. Demonstrations range from a robotic cuff encircling a blood vessel for detecting blood pressure, to a robotic gripper holding onto a bladder for tracking bladder volume, an ingestible robot residing inside stomach for pH sensing and on-site drug delivery, and a robotic patch wrapping onto a beating heart for quantifying cardiac contractility, temperature and applying cardiac pacing, highlighting the application versatilities and potentials of the nature-inspired soft robots. Our designs establish a universal strategy with a broad range of sensing and responsive materials, to form integrated soft robots for medical technology and beyond.\n\n- Physical sciences/Materials science/Soft materials/Gels and hydrogels\n- Physical sciences/Engineering/Electrical and electronic engineering\n- Physical sciences/Engineering/Mechanical engineering\n- Physical sciences/Engineering/Biomedical engineering\n- Physical sciences/Materials science/Materials for devices/Sensors and biosensors\n\n# Introduction\n\nThe dynamically changing environments drive living organisms to evolve toward inseparable integration of motor and sensor functions [1–3]. Especially, coherent integration between skeletal muscles and sensory skins enables their rational and well-organized cooperation orchestrated by neural systems to execute perceptive actions with intelligence. A diverse variety of receptors (mechano, thermal, pain, and others) embedded in the soft skin gathers and encodes tactile data, which not only guides muscular motions to the optimum but also interprets the environment for enhanced awareness and cognition [4–6]. Such motor-sensor integration established in the biological systems inspires development of intelligent robotic systems mimicking skin softness to safely explore and interact with dynamic, unstructured, and often uncertain environments, particularly when robots interface with biological tissues and organs to enable precision therapeutics [7–10]. However, existing robots often lack a seamless integration among actuators, sensors, and controllers, that naturally preserve physical softness and biocompatibility [11,12].\n\nCreating such nature-inspired somatosensory soft robots as implants holds promising potential to innovate medical technology, especially in surgery, diagnosis, drug delivery, prostheses, artificial organs, and tissue-mimicking active simulators for rehabilitation [13–17]. Conceptually distinct types of soft robotic implants take the form of shape-morphing and functionalization, are capable of compliance matching biological tissues, retrieving their functional signature, and offering therapeutic treatments [10,13,14,18–21]. For example, an integrated bladder system consisting of interdigitated capacitive sensors capable of continuous bladder volume detection, and a shape memory alloy-based actuator with strong emptying force for urine voiding, allows for real-time bladder control [18]. A soft gripper based on a shape memory polymer with integration of silver nanowires and a crack-based strain sensor enables conformable contact with a carotid of swine model and measuring its blood pressure [19]. Taking inspiration from the ventricular teeth of hookworm, thera-grippers made of a metal-polymer hybrid actuator and a drug-eluting patch can latch onto the mucosal tissue inside gastrointestinal GI lumen and extend drug release [20]. The combination of sensing and actuation not only enhances diagnostic and/or therapeutic precision for implants via dynamically modulating the structural interface to targeted tissues, but also enables possibility to become artificial organs that offer both needed structural transformation and physiological functions (e.g. electrical signaling, and hormone secretion) [17,20,22]. Despite the promising progress in soft robotic implants, grand challenges remain in designing materials and manufacturing technologies, to leverage multi-faceted requirements of device performance, including compliant mechanics to match tissue softness, biocompatibility of constituent materials to ensure implantation safety, structural adaptability to prolong device longevity, and biomimicry to enhance device functionality [11,12,18,23].\n\nHere we present concepts and device designs to achieve untethered, soft robots that follow a biomimicry integration of actuators, sensors, and stimulators, to enable structural adaption and dynamic reconfiguration that minimize tissue damage during implant deployment, release stress at biotic-abiotic interface, increase biocompatibility, and enhance device multi-modal performance with spatiotemporal precision (Fig. 1 and Fig. S1). Demonstrated examples of utilizing such nature-inspired robots include: i) a robotic gripper that wraps around a bladder to enable coordinated, closed-loop operation of bladder-volume evaluation and electrical stimulation to treat overactive bladder, ii) a robotic cuff that can enclose around a blood vessel for measure blood flow and pressure, iii) an ingestible robot that can expand when arriving in a stomach for prolonged monitoring and drug delivery, and iv) a robotic patch that can actively grasp and release a beating heart for epicardial sensing and pacing, which collectively highlight potential impacts of the nature-inspired robotic designs that naturally integrate actuation, sensing and stimulation within a coherent entity as next-generation electronic implant with physical intelligence.\n\nThe soft robots primarily consist of two integrated, functional layers that emulate relations between sensory skin and underlying muscles. Specifically, one layer represents an electronic skin (e-skin), that is made of functional nanocomposites predominantly based on an in situ solution-based fabrication approach. The other layer represents an artificial muscle, that is based on poly(N-isopropylacrylamide) (PNIPAM) hydrogel, which can reversibly contract and relax upon activation trigger. Significantly, hydrogels, known for their exceptional softness, low activation temperature and nonfibrotic biocompatibility, are generally preferred over other stimuli-responsive materials in implantable applications [24–27]. The bilayer design composed of the e-skin and artificial muscle represents a heterogeneous configuration with a variety of responsiveness upon exposure to environmental stimuli, which orchestrates its robotic motion. Our in situ solution-based method successfully embeds multiple sensing materials (e.g., silver nanowires ~ AgNWs, reduced graphene oxide ~ RGO, MXene and poly(3,4-ethylenedioxythiophene) polystyrene sulfonate ~ PEDOT:PSS) into a polymer matrix (e.g., polyimide ~ PI, and polydimethylsiloxane ~ PDMS), enabling the e-skin a versatile platform that highly mimics the skin with complex receptors, and accurately detects the external signals. These functionalities encompass touch, pressure, temperature, and chemical sensing, surpassing the integrative complexity and heterogeneity achievable with 3D printing or other conventional approaches [28–30]. Moreover, inspired by nature (e.g., starfish and chiral seedpods), we can vary designs of the soft robots, enabling various motions (e.g., bending, expanding, and twisting), and corresponding 3D deformed configurations. In addition, the soft robots allow both on-demand transformation and local-region actuation via embedded control circuits, which further increases structural versatility and capability. Moreover, the soft robots can move, sense, and communicate in a wireless closed-loop fashion via integration of control module and data analytics, enabling minimally invasive operations with safe and stable access to enclosed small spaces inside human body.\n\n# Results\n\nThe integrated architecture between the skin and skeletal muscles enables safe and closed-loop interactions with surrounding environment, bringing a feeling of touch and acting of motion seamlessly together in space and time [31–33]. A feature of particular interest in skin is the mechanoreceptors localized at the interface between the epidermis and dermis of skin, which are responsible for detecting a variety of mechanical stimuli, including the fast-adapting (FA) receptors that respond to dynamic forces and slow-adapting (SA) receptors that respond to static pressures (Fig. 2 A) [34–36]. By mimicking the hierarchical architectures of skin and muscle with associated biological functions, our soft robots integrate multi-electronic modules and thermally actuatable hydrogels, realizing both receptor-like sensing functions to detect various stimuli, and on-demand muscle-like contraction to generate physically adaptive motion, from a single integrated platform, endowing soft robots with intelligence in navigating through real-world environments autonomously (Fig. 2 B). Figure 2 C shows a fabricated multi-modal sensory soft robot with geometry emulating a starfish. The robot consists of three primary layers: a flexible nanocomposite layer as a multi-modal electronic-skin (e-skin) embedded with distinct sensors (strain, pressure, pH, and temperature) and stimulators (thermal and electrical), a thermally responsive hydrogel layer as an artificial muscle generating actuation force, and a thin bio-adhesive layer as a cushioning medium to form interfacial binding between the e-skin and artificial muscle.\n\nOur approach for fabricating the flexible nanocomposite layer can be generally applicable to a wide variety of soft materials and nanomaterials heterogeneously composited within a single matrix material, which enables the potential to form highly integrated systems with a broad range of sensors and stimulators. Specifically, here we demonstrate (1) a thermal sensor made of a nanocomposite of reduced graphene oxide (RGO) and polyimide (PI), (2) a strain sensor made of a nanocomposite of silver nanowires (AgNWs) and polydimethylsiloxane (PDMS), (3) sensing and stimulation electrodes made of a nanocomposite of poly(3,4-ethylenedioxythiophene): polystyrene sulfonate (PEDOT:PSS) and PI, and (4) a thermal heater made of a nanocomposite of AgNWs and PI. The flexibility and versatility of this strategy allow the as-fabricated functional units to be easily integrated into each arm of the starfish robot in a monolithic fashion, as illustrated in Fig. 2 D, realizing a sensory skin for the robot to enable environmental awareness. Figure 2 E and Fig. S2B display an example of an ultrathin multi-modal e-skin equipped with six nanocomposite sensors (The detailed fabrication process appears in Fig. S2A.). The e-skin is further encapsulated with a parylene layer (thickness ~ 2 µm) to enhance its durability during prolonged applications (Fig. S3A, and Supplementary Note S1) [37,38]. This is subsequently attached onto a piece of predesigned thermally responsive PNIPAM hydrogel that serves as an artificial muscle for the soft robot (Fig. S3B). The PNIPAM hydrogel can undergo a notable volumetric change about 90% as the temperature change from 23°C to 40°C, and thus provide excellent actuation in biological environment (Fig. S4A - C) [39,40]. The as-fabricated soft robot can form a highly conformal interface with diverse biological surfaces, indicating its inherent mechanical softness and high biocompatibility (Fig. 2 F, Fig. 2 G, and Fig. S2C-E). At an elevated temperature (40°C), the robot consisting of the stimuli-responsive artificial muscle (PNIPAM layer) and non-stimuli-responsive e-skin (multi-modal layer) tends to bend toward the muscle side on the basis of asymmetrical responsive properties (Fig. 2 H, Fig. S2F and Fig. S4D - F) [41,42].\n\nFigure 2 I, Fig. S2F, and Supplementary Movie S1 provide an example of a robotic starfish reversibly closing and opening its rays under a temperature shift between 23°C and 40°C. Furthermore, such multi-layer integration allows a diverse collection of robotic designs that undergo various types of actuation. Fig. S5 & 6 and Supplementary Movie S2 highlight soft sensory robots featuring starfish-like structures with an arbitrary number of rays (e.g., four and six) and a fishbone-like structure with four pins. In addition, tuning the design layout of the multi-layer structure can yield complex deformation and structural reconfiguration beyond simple bending motion. Here, inspired by the self-twisting of chiral seedpods, we constructed a geometry with parallel strips in the e-skin layer (Additional details appear in Fig. S7A and Fig. S8A.). Upon thermal stimulation, concentrated internal stresses at the bonding areas are built simultaneously, leading to local saddle-like curvature and twisting motion of the integrated robotic systems (Fig. 2 J, Fig. S7B, Fig. S8B, and Supplementary Movie S3). We also develop a soft robotic pill based on an anchored hydrogel/nanocomposite tri-layer structure, where a hydrogel-muscle layer is surrounded by two separate e-skin layers that bond to the muscle layer at the edges (Fig. S9A and Fig. S10A show the detailed structure design.). Upon thermal actuation, the pill can self-expand into a 3D ring shape, since the contraction of the muscle layer drives the e-skin layers to buckle out of the plane, as shown in Fig. 2 K, Fig. S9B, Fig. S10B, and Supplementary Movie S4. Furthermore, compared with a make-and-transfer method, our in situ solution-based fabrication approach for full integration of sensors into the e-skin layer, in which the sensing material and passive polymer-based skin are structured monolithically, endows the as-fabricated e-skin as a versatile platform that can be constructed using a broad range of functional nanomaterials hybridized with a polymeric matrix to form a multi-modal sensing system, emulating the skin with complex somatosensory system, where various mechanoreceptors and thermoreceptors distributed in the epidermal and dermal layers enable the spatiotemporal recognition of the magnitude and location of touch and temperature stimuli [43,44]. Fig. S11 provides a representative example of in situ integration of AgNW/PDMS-based strain sensor, in which the strain sensor has a good response to the stretching. Figure 2 L shows the proposed solution-based approach enables a freestanding PI film to integrate multi-functional modalities including an RGO/PI-based temperature sensor and an AgNW/PI-based heater (Fig. S12A), endowing soft robots with both thermal sensing and stimulation. Moreover, Fig. 2 M displays a more complicated integration paradigm with multi-layer stacking, where different electronic components (e.g., PEDOT:PSS/PI-based conductive electrodes and RGO/PI temperature sensors) can be distributed in different layers of the e-skin to achieve functional versatility simultaneously and with high proximity (Fig. S12B). The X-ray photoelectron spectroscopy (XPS) characterization on the e-skin layers reveals the chemistry of the composite assembled at nanoscale with the active nanomaterials and a polymer matrix. The detailed chemical composition analysis of the nanocomposite appears in Figs. S13 - S15 and Supplementary Note S2 [45–49]. These functionalities would be of great value for soft robots that seek to achieve multifunctionality and local sensing capabilities approaching skin.\n\nProgrammable stimuli-responsive soft robotic systems capable of working in enclosed or confined spaces and adapting functions under changing situations hold great promise as next-generation medical robots [50,51]. The realization of versatile morphing modes through local-actuation control is crucial for enhancing on-demand actuation. Here, we develop soft robots with cognitive capabilities via unifying programmable actuation and in situ sensing. Figure 3 A shows a sensory robotic arm primarily consisting of a PNIPAM-hydrogel-based muscle layer and a multi-modal e-skin layer that is designed with an AgNW/PI nanocomposite actuation heater and an RGO/PI nanocomposite thermal sensor. Fig. S16A shows layer-by-layer stacking as a simple and effective approach for fabricating the e-skin. Fig. S16B and Fig. 3 B demonstrate the multifunctional nanocomposite film is highly flexible and can be tightly bonded onto the hydrogel layer via n-butyl cyanoacrylate adhesive. When the liquid PI is cast onto the nanomaterial film (e.g., AgNWs and RGO), the liquid PI penetrates into the interconnected pores of the three-dimensional (3D) network, owing to the low viscosity and low surface energy of the liquid PI [52]. The scanning electron microscope (SEM) images (Fig. 3 C&D, Fig. S17A - C, and Fig. S23A - C) present that the curing process fully buries all the nanomaterials inside the PI matrix without generating observable voids. This prevents separation of the nanomaterials from the polymeric matrix, thus minimizing untended side effects to the neighboring tissues. The Fourier-transform infrared spectroscopy (FTIR) and X-ray powder diffraction (XRD) results (Fig. S17D & E, Fig. S23D & E, and Supplementary Note S3) also confirm the chemical structure of AgNW/PI and RGO/PI nanocomposites suggesting a successful fabrication of high-quality nanocomposite of functional materials and polymer matrix [53–56]. Figure 3 E demonstrates that the resultant AgNW/PI nanocomposite conductor is highly conductive, twistable, and bendable, and thus used as a highly flexible heater for electrothermal actuation. Thermal images in Fig. 3 E and Fig. S18A show the infrared thermograph of a Joule-heated e-skin in the resting state and under both bending and twisting conditions. The electrical heater distributed inside the e-skin exhibits a stable and uniform temperature distribution without degradation of the temperature level at the deformed points, ensuring effective thermal transport from the heater to the hydrogel-based muscle layer. Figure 3 F and Fig. S18B & C depict the transient electrothermal response of the flexible heater applied by various powers in an ex vivo environment. The saturation temperature of AgNW/PI nanocomposite heater increases with the supplied power as more Joule heat is generated, and the lower critical solution temperature (LCST) of PNIPAM hydrogel at 34°C can be obtained at low input power (< ~1W) (Fig. S19A). As shown in Fig. S18C, the flexible electrical heater exhibits steady heating and cooling cycles, indicating high repeatability and remarkable heating stability using AgNW/PI nanocomposite. Figure 3 G and Fig. S19B show varying the amount of electric power applied to the heater effectively modulates the resultant bending angle θ (as defined in Fig. S18D) of the robotic arm, thus realizing precise, on-demand access to intermediate morphologies along the bending pathway. We also investigate the bending behavior of the soft robotic finger in a tissue culture incubator (37°C) mimicking in vivo condition (Fig. S20). As expected, a lower electrical power is found to be sufficient for achieving a bending performance similar to that obtained in an in vitro condition (ambient condition). We further evaluated the mechanical force generated by the soft robotic finger under various input powers. Fig. S19C shows that the static force exhibits a noticeable increase with rising temperature. At a temperature of 40°C, the force reaches a maximum of 32 mN. Additionally, it is observed that the generated force remains consistent throughout 40 cycles of alternating power on and off (0.35 W), indicating the robust reversibility of the soft robot (Fig. S19D). When compared to similar hydrogel-based soft actuators, our design consistently achieves a relatively high output force, as shown in Table S1 [57–64]. Furthermore, Fig. S21 demonstrates local activation of a series of motions via integrating multiple AgNW/PI-nanocomposite heaters into a single e-skin platform and precisely commanding them to generate local heating, further highlighting the advantage of our in situ solution-based fabrication approach, with high design versatility, simplicity, integrability, and low cost. To exemplify this versatility, we have also successfully fabricated MXene-based sensors, as illustrated in Fig. 3 J, Fig. 3 K and Fig. S22. MXene-based materials possess inherent biocompatibility, rendering them ideally suited for incorporation into implantable biomedical devices without eliciting adverse reactions or compromising the surrounding biological environment [65,66]. The ability to precisely identify the real-time information of temperature during the muscle motion using an RGO/PI-nanocomposite temperature sensor forms a closed feedback loop for the robotic control. The in situ solution processing ensures RGO network is uniformly distributed in PI matrix to provide precise pattern registration with good electrical conductivity (~ 400 S/m) and stable performance in aspects of electrical linearity, sensitivity, and repeatability. Figure 3 H illustrates the resistive change in a relatively linear relation with temperature for the RGO/PI thermal sensor. The temperature coefficient of the resistance (TCR) of the RGO/PI thermal sensor is > 0.5%/°C, featuring its high thermal sensitivity. On the other hand, the RGO/PI-based thermal sensor exhibits a stable performance after 1000 bending cycles, and even after immersing in PBS solution. Figure 3 I and Fig. S23F show performance of the thermal sensor in response to cycles of temperature rise and drop, indicating good sensing stability. In addition, the in situ solution process allows fabrication of thin films of AgNW/PI nanocomposite as thermal sensors. Fig. S24A shows the AgNW/PI thermal sensor exhibits a linear relationship between the resistance and temperature with sensitivity ~ 0.4%/°C over the range of 23–80°C. Notably, the sensor showcases minimal performance degradation even when subjected to bending and immersion in PBS. Moreover, to evaluate the biostability of the sensor, it is immersed in a PBS solution at 37°C simulating an in vivo condition. Fig. S24B indicates the performance of the AgNW-based nanocomposite sensor with outstanding bio-stability over a week. Fig. S24C demonstrates good sensing stability of the AgNW/PI-nanocomposite thermal sensor under cyclic temperature test between 25 and 40°C. In addition, Fig. S23G and Fig. S24D show consistent measurements of both RGO/PI and AgNW/PI nanocomposite sensing performance in comparison with a commercial thermal resistor (ERT-J0ET102H), indicating excellent sensing accuracy.\n\nWell-controlled shape morphability with high spatiotemporal resolution is essential for soft robots to execute complicated tasks safely in biological environments [67,68]. Here, the integration of e-skin and artificial muscle allows the nature-inspired soft robots to realize motions of local regions independently, which collectively can lead to a wide range of shape morphability. Figure 3 L demonstrates the locally controlled morphability with a soft robotic finger, of which the e-skin includes a series of AgNW/PI-based heaters for localized thermal activation, and RGO/PI-based thermal sensors for temperature monitoring (Fig. S25A). As shown in Fig. 3 L and Fig. S25B, the robotic finger undergoes a stepwise self-coiling motion via a sequential stimulus and perceives its local temperature simultaneously by the embedded thermal sensors (Fig. 3 M). More complex actuation modes or configurations are accessible owing to the combined ease of processing and ability to introduce multifunctional units. Figure 3 N presents a three-arm soft robotic gripper where each arm contains various types of sensors, including an optical sensor, a thermal sensor, and a strain sensor, respectively, and an electrical heater (Fig. S26A), to enable independent control of motion for each arm, thus allowing on-demand gripping and interaction with targeted objects (Supplementary Movie S5). Moreover, the soft robotic systems can be structurally tailored to support a range of motions. For example, Fig. S26B & C highlights a soft starfish-like robot with four sensory arms, and a soft robotic cuff with optoelectronic sensors, respectively. The electrothermal stimulus along with distributed sensing capabilities enables programmed actuation not only on demand but also regulated simultaneously by the sensing feedback (e.g., Supplementary Movie S6).\n\nWireless operation of actuation as well as therapeutic and/or diagnostic functions is essential for implantable robots to minimize tissue damage and implant infection [67,69–71]. However, existing schemes for wireless operation of robots mostly require sophisticated circuitry for energy harvesting and storage, which may introduce non-negligible heat (~ 80°C), unfavored space occupation, system complexity, limited lifetimes, and high cost [72,73]. To overcome the preceding challenges of actuation/sensing integration in soft implantable robots, we report a nature-inspired soft robot as a representative example to demonstrate remote, battery-free operation and communication in both sensing and actuation.\n\nFigure 4 A-C show schematic illustrations of the system design consisting of sensor and actuator components. Our strategy for wireless sensing relies on a passive inductor-capacitor (LC) resonance circuit formed by a planar inductor coil and a parallel plate based on capacitor polyacrylamide (PAAm) hydrogel, as illustrated in Fig. 4 B. A change in a biomechanical event (e.g., vessel filling, cardiac contraction/relaxion, and bladder filling/voiding) can lead to a corresponding change in capacitance of the hydrogel-based capacitor, which can be quantified by recording shift in resonance frequency (fs) of the LC circuit according to the equation fs=1/2π√LC, where L and C are the inductance and capacitance of the resonance circuit, respectively [74,75]. The inductor coil couples to an alternating electromagnetic field through a readout probe, enabling quantitative measurement of the input return loss (S11) using a vector network analyzer (VNA) (Fig. 4 D and Supplementary Note S4). The proposed PAAm-based sensor with relatively low modulus, intrinsic stretchability, and biocompatibility, can detect the pressure through variation of capacitance between the two electrodes. Figure 4 F shows a linear correlation between the measured ΔC/C0 and applied pressure. The slope of the linear fitting curve reports gauge factor (GF) of the sensor reaching ~ 3%/kPa in the clinically relevant range of pressure (0–4 kPa). Figure 4 G& H shows the resonant frequency decreases from 340 MHz to 260 MHz in response to the applied pressure decreasing from 0 to 3.5 kPa, and the pressure sensitivity of the sensor is ~ 26.7 kHz/kPa.\n\nMoreover, wireless electromagnetic power transmission is an attractive solution to overcome limitations imposed by implantable systems with discrete batteries, especially for devices operating in enclosed places such as the human body [75–77]. Here, we demonstrate the nature-inspired, sensory robot allows for electrically controlled locomotion in this wireless, battery-free manner (Fig. 4 A). Figure 4 C shows layout of the wireless actuation design including a PNIPAM actuation hydrogel, a flexible electrical heater, and a radio-frequency (RF) power harvester based on a Cu coil. The RF harvester that is made of a triple-layer structure (Fig. S27A & B), can be integrated with medical implants (Fig. S27C and Fig. S41D - I). Magnetic coupling between the transmitting and receiving coil generates electric currents to the heater that thermally stimulates the artificial muscle (Fig. 4 E & Fig. S27D). As shown in Fig. 4 J and Fig. S28B & C, the robotic finger can undergo a bending motion upon receipt of electromagnetic energy from a power-transfer module. Figure 4 I shows an infrared image of the robotic finger highlighting concentrated heat on the electrical heater and minimum heat on the receiving inductor, which collectively ensures a stable power supply and minimum heat damage to surrounding bio-environments in potential usage as implants. Figure 4 K shows the output power as a function of frequency. The wireless power transfer system achieves the highest harvested power ~ 1.05 W at a frequency of 15 MHz. Figure 4 L indicates the harvested power can be tuned via varying the input power at the optimal frequency 15 MHz, and the power efficiency reaches around 80%, which is sufficient to trigger the heater for raising local temperature to drive motions of the soft robot (Fig. 4 M).\n\nThe soft robotic system features spatiotemporal locomotion wirelessly controlled by RF signal modulation. To demonstrate the working principle of this method, we fabricate a soft robotic gripper with three arms as an illustrative example. This strategy employs a three-lead LC receiver coil designed based on the frequency-response characteristics of magnetic resonance coupling (Fig. S29A & B), allowing for the formation of two different configurations with distinct inductive values. These configurations are paired with corresponding capacitors to form LC circuits with different resonant frequencies (Fig. S29C). By coupling with different transmission coils operating at distinct transmission frequencies, the coils can selectively deliver power to specific heaters, thereby enabling the activation of individual robotic arms (Fig. S29D - F). Furthermore, we conduct a further investigation into the influence of shape deformation, including bending, twisting, and distorting, on the transfer performance of the RF harvester (Fig. 4 N). Fig. S27E demonstrates that the zeros of the reactance of the receiving circuit remain constant throughout the entire process, indicating minimal disruption to the coil’s resonance frequency [78,79]. Additionally, Fig. 4 K and Fig. 4 O exhibit a reduction in transmission efficiency resulting from decreased mutual inductance between the transmission and the receiving coils due to shape deformation. For all the deformations shown here, the resonance frequency of the coil remains within an acceptable range for power harvesting, and the power transmitted remains above the minimum level required for the robotic actuation. Supplementary Note S5 and Figs. S30-S32 further demonstrate the effect of various design and operational parameters on the power transfer system [80–82]. This yields systematic metrics for designing a well-tuned WPT system, capable of fulfilling the specifications of the targeted application, concurrently decreasing power expenditure, and evading possible risks to living organisms [83,84]. Such wireless robotic systems may serve as a promising solution to safe, real-time monitoring of internal pressure needed for various medical procedures. Notably, Fig. S27C shows the circuits for wireless sensing and actuation can be integrated together onto a single e-skin, realizing device miniaturization and efficiency. On the basis of integrated high performance, the confluence of wireless technology and biosensors offers the possibility to detect and manage medical conditions remotely, beyond clinical settings.\n\nSoft sensory robots have significant potential for medical-device applications that warrant safe, synergistic interaction with humans [85,86]. The robotic implants developed here can enable minimally invasive implantation. Here, the devices can be stored in a thin catheter and transported safely through small incisions without phase transition until reaching the LCST, in contrast to open surgery where large incisions are required [87,88]. Fig. S33 provides a schematic illustration of a minimally invasive catheter with a retractable nitinol wire that guides the starfish-structure robot (Fig. S33A, Fig. S34A, Fig. S34C - F & Supplementary Movie S7) and hand-structure robot (Fig. S33B, Fig. S34B, Fig. S34G - J & Supplementary Movie S7) to the heart and blood vessel, respectively. As shown in Fig. S33A, the delivery involves the following steps: (i) the starfish robot is soft, flexible, resilient and robust, making it easy to be enclosed inside a catheter; (ii) the robot undergoes unfolding motion as it is pushed out of the catheter at the targeted site; (iii) the robot conformally attaches to the epicardial surface due to the inherent softness and adhesiveness of the hydrogel, which accommodates curvilinear surfaces; (iv) the hydrogel layer can be activated by body temperature or joule heating (depending on the LCST of PNIPAAM hydrogel), allowing the starfish-structure robot to form a stress-free interface with the beating heart. Moreover, the device can be further miniaturized to fit within the size constraints of various types of catheters. Fig. S33B demonstrates an example of a hand-shape robot approaching the blood vessel via a catheter insertion (Fig. S33Bi - ii). Upon stimulation, the robot tightly holds the blood vessel and forms a conformal, stress-free interface (Fig. S33Biii - iv). Figs. S35 - S39, and Supplementary Movie S8 demonstrate that the skin-inspired soft robots can be designed with a diverse array of configurations, to enable minimally invasive deployment extensive interfacial engagement, and structural reconfiguration to transform between these two stages. Furthermore, in line with pioneering research [89–96], our soft robots feature a profound versatility in geometrical and dimensional design, ensuring a refined adaptability to the specific preferences and requirements of individual cases (Fig. S40 & S41, Table S2, and Supplementary Note S7). Here, incorporation of acrylamide (AAm) into the PNIPAM hydrogel to form poly(NIPAM-co-acrylamide) (P(NIPAM-AAM)) effectively increases its LCST [64,97–99]. This ensures that the as-prepared robot maintains an unactuated configuration during its passage through the body, while being actuated upon a digitally controlled thermal trigger, thereby providing surgeons with a sufficient time window to perform needed procedures (Supplementary Note S6 and Figs. S42 - S44). Notably, the temperature-dependent hydrogel adhesion could further minimize device migration and delamination due to potential reswelling at a slightly decreased temperature (Fig. S45 & S46, and Supplementary Note S8). This suggests that our proposed design can be customized and developed to facilitate various types of minimally invasive implantation. In vivo tests with artificial organ models demonstrate the versatilities and capabilities of our soft robots for enhanced sensing, stimulation, and drug delivery.\n\nUrinary bladder dysfunction is one of the emerging issues in an aging society, which not only leads to loss of voluntary control over the bladder muscles, but also cuts off sensorial feedback to central nervous system [100]. In most cases of bladder dysfunction, the patients are not able to sense the fullness of bladder with urination, making it a challenge to time the action for voiding treatment (e.g., electrical stimulation) [101]. Therefore, realizing the voiding treatment in a timely manner requires a monitoring system that measures the bladder status continuously. Here, we develop a soft robotic gripper for both real-time assessment of bladder volume and voiding treatment in a wireless closed-loop control fashion. The as-prepared robotic system, illustrated in Figs. 5 A-5 C & Fig. S47A, consists of a flexible hydrogel-based actuator, a 3D buckled strain sensor, an electrical stimulator, and a control module. The actuator includes a passive layer made of a patterned Au/PI bilayer as an electrical heater, and an active layer of PNIPAM hydrogel. Upon an electrical trigger delivered via an inductive coil, the robotic gripper can bend and wrap around the bladder conformally and gently (Fig. 5 A) to ensure precise measurement of bladder volume and minimized stress at the interface. The strain sensor integrated into the robot is capable of detecting bladder volume continuously. Here, the strain sensor includes an elastic PAAm hydrogel film and a serpentine Au/PI resistor to form a buckled 3D structure for enhanced sensitivity. The fabrication steps for the buckled sensor appear in Materials and Methods. We use a balloon model to mimic the natural bladder behavior of filling and emptying to validate performance of the integrated soft robotic gripper. Fig. S47B shows the sensor conformally attaches onto the balloon surface with the biocompatible adhesiveness of PAAm hydrogel [102]. The softness of PAAm hydrogel in the robot achieves minimal strain disruption to the bladder during the device operation. Injecting and extracting water into the balloon with a syringe pump realize the behavior of bladder filling and emptying (Fig. 5 D). The change of sensor resistance exhibits a strong linear correlation with bladder volume during its expansion and shrinkage (Fig. 5 E, and Fig. S47C & D), thus serving as an indicator in bladder-volume control. Figure 5 F demonstrates the system repeatability in real-time monitoring during multiple cycles of bladder filling and emptying.\n\nThe readout of the bladder volume is achieved through a voltage divider circuit (VDC) consisting of a reference resistor connected in series with the as-fabricated strain sensor. This configuration has minimal impact on the wireless power transmission between coils (Fig. S48). To achieve a closed-loop control of electrical stimulation in the treatment of a dysfunction bladder system, we further program the Bluetooth-Low-Energy (BLE) System-on-Chip (SoC) (BLE SoC) to enable a pulse-width modulation (PWM) instance. The instance, together with on-board power amplification and filtering circuits, facilitates the application of programmable electrical stimulation in response to an increased strain in the bladder. This enables on-demand electrotherapy and closed-loop control of the robotic implant, as illustrated in Fig. 5 B and Fig. 5 C. A demonstration of the control scheme can be found in Fig. S49 and Fig. 5 G. When the balloon reaches a certain volume threshold, the control system triggers a command for electrical stimulation.\n\nThe on-demand motion provided by the soft robot facilitates device implantation and ensures benign and stable contact with targeted tissue or organs [10,103,104]. Here we develop a soft robotic cuff that can enclose around a blood vessel upon thermal stimulation (Fig. 5 H), to enable real-time measurement of blood pressure. As shown in Fig. S50A, the soft robotic cuff consists of a muscle layer based on a PNIPAM and an e-skin layer embedded with a strain sensor based on a serpentine Au ribbon. Notably, the e-skin layer uses a pattern of parallel strips in the PI film, that forms a 45° angle with the longitudinal direction of the device, which, by coupling with the muscle layers, facilitates formation of a helix structure. An in vitro model of artery that uses a rubbery tube with a pulsatile flow of water to create a simulated pulsation pattern validates performance of the soft robotic cuff (Fig. S50B & C and Fig. 5 I). The helix formation of the robotic cuff provides a gentle and stable coupling with the artificial artery, of which the measured signal (resistive change) exhibits a linear relation with the inner fluid pressure (Fig. 5 J). Figure 5 K demonstrates the capability in continuous measurement that captures patterns of simulated pulsation, further confirming its utility in measuring blood pressure.\n\nFurthermore, such nature-inspired designs of soft sensory robots can also configure into an ingestible platform. Here, we show that a soft ingestible robot is capable of prolonged residence in the stomach for pH monitoring and drug delivery. Fig. S51A depicts the proposed structure of the ingestible robot based on a slab-shaped muscle layer sandwiched by two e-skin layers consisting of a drug delivery module and a pH sensing module (Fig. 5 L, more details appear in the Materials and Methods.). The miniaturized size of the robot facilitates swallowing and transport through the esophagus to stomach (Fig. 5 L). Once in the stomach, the robot self-expands that prevents passage through the pylorus for an extended duration in the gastric environment (Fig. 5 M and Fig. S51B). The soft pH sensors based on PEDOT:PSS/poly(vinyl alcohol) (PVA) embedded onto the e-skin of the robot provide continuous measurements of gastric pH (Fig. S51C and Fig. 5 N). The pH sensor exhibits a linear relationship between the resistive change and pH of the fluidic environment within the range of acidic (pH ~ 3) to basic (pH ~ 8) (Fig. S51E). To realize prolonged drug release, the integrated drug patches use poly(lactic-co-glycolic acid) (PLGA) as a matrix to load drugs and the robotic motion as a trigger mechanism that exposes the drug-loaded patches to stomach fluid for initiating drug release. As a demonstration, we use a biocompatible dye, rhodamine-B (RB), as a model drug (5 mg of RB per 0.5g PLGA). Figure 5 O and Fig. S51H show the UV-vis absorption spectra and the corresponding dosages, respectively, of the RB-loaded drug patch, immersed in PBS solution (at pH ~ 5) for 1 h under various temperatures ranging from 25°C to 45°C (Fig. S51F & G show the calibration curve based on the measured UV-vis absorption spectra.). Such ingestible soft robot highlights a synergistic combination between sensing function and robotic motion to realize on-demand, prolonged control of drug delivery.\n\nCardiac implants that can monitor and regulate heart rhythms are critical for patients with severe cardiac diseases [105,106]. Despite the broad implementation of cardiac implants or pacemakers in clinical settings, however, existing devices are usually rigid, undeformable, and lack structural reconfigurability to adapt to dynamic motions of beating heart, which precludes optimum performance chronically and safely [107]. Here, we report a soft robotic thera-gripper that can gently envelop a heart to perform spatiotemporal monitoring of electrophysiological activity, temperature, and strain, and provide therapeutic capabilities (e.g., electrical pacing). The soft robotic thera-gripper contains four multi-functional arms, emulating a starfish, to ensure effective latching onto the epicardial surface of which the soft mechanics ensures negligible disruption to cardiac dynamics. Fig. S52A presents an exploded view of the robotic thera-gripper, which contains actuators based on PINPAM actuation hydrogel, two temperature sensors made of thermal resistors, two pacing electrodes made of Au, and four strain sensors made of serpentine Au/PI resistors (The fabrication approach appears in Materials and Methods, and Fig. S52B.). Figure 6 C shows the thera-gripper at its resting state features minimally invasive insertion with a medical catheter, and forms a bowl shape at the actuation state, via a slightly raised temperature, to gently hold a beating heart for a safe, stable interface (Fig. 6 C). Figure 6 D shows the corresponding FEA result of an actuated soft robotic thera-gripper. Moreover, we examined the biocompatibility of the soft robots in vitro and in vivo. Here, mouse 3T3-J-2 cells exposed to complete soft robotic devices with constituent materials including pure PNIPAM hydrogel and functional nanocomposites (e.g., AgNWs, RGO, PEDOT:PSS & MXene), remain robust healthy and maintain stable viability (Fig. 6 A, Fig. 6 B, Fig. S53 & Fig. S54) [108,109]. Additionally, histological analysis reveals that the soft robots implanted inside chest chamber of mice induce no observable inflammation or other adverse effects to surrounding tissues, indicating good biocompatibility for long-term operation (Fig. S55 & Fig. S56). The incorporated temperature sensors provide feedback information on device temperature that govern the structural transformation, upon contact with cardiac tissues (Fig. 6 F). The pacing electrodes integrated into our thera-gripper can generate electrical impulses to regulate cardiac pacing (Fig. 6 G and Fig. S52C & D). Fig. S57 shows measured ECG traces, highlighting effective transmission of electrical impulses (voltage ranges from 500 mV to 2 V with 1 ms width at 2.65 Hz) onto cardiac tissues. The e-skin layer consists of microelectrodes for capturing electrical activity of heart, which serves as essential guidance in operating electrical stimulation/pacing (Fig. S58). Figs. S59 - S61 showcase simultaneous sensing and stimulation from a robotic thera-gripper on a beating heart with an in vivo mouse model, demonstrating its capability in closed-loop operation of cardiac pacing.\n\nCardiovascular disease is one of the leading causes of death worldwide affecting more than 17.9 million people per year [110]. Real-time and continuous monitoring of myocardial functions (e.g., contractility) is desired for patients with high risks of cardiac arrest, which not only ensures proactive treatment prior to occurrence of adverse events, but also provides comprehensive evaluations of therapeutic effects during postoperative care [111–113]. A soft thera-gripper, integrated with strain sensors distributed on its arms, can provide continuous, spatially resolved quantification of myocardial strains, holding great potential in precision treatment for cardiac diseases. Here, a chronic model of myocardial infarction (MI) with permanent ligation of the left coronary artery (LCA) of a mouse enables assessment of the sensing capability of a thera-gripper post to its robotic motions to establish optimized sensing interfaces (details appear in Materials and Methods.). Figure 6 H& I show the infarcted area that turns into pale myocardium. Echocardiographic strain imaging provides continuous quantification of regional myocardial function. Fig. S62B & C show the short-axis views in echocardiographic imaging (B-mode) from a normal and post-MI left ventricle (LV) of heart, respectively. The M-mode images, as shown in Fig. 6 J& K, display the fraction shortening (FS) decreases from 75–15% upon occurrence of MI, indicating the heart exhibiting moderate dysfunction accompanied by regional contractility loss (Supplementary Note S9 and Fig. S62D & E) [114,115]. Although echocardiography is an invaluable tool allowing for reliable diagnostic information necessary for the clinical decision, it often lacks convenient accessibility and usually takes more than 30 minutes to capture the movement and function of the heart muscle and heart valves [116]. Figure 6 L and Fig. S63C show that the multi-strain sensors (labeled as S1, S2, S3, and S4) of the implanted thera-gripper distributed across four chambers of the heart, respectively, highlighting the key advantage of our thera-gripper with real-time strain sensing over traditional imaging tools in recording local contractions continuously and simultaneously. Fig. S63A shows the response of a representative strain sensor, revealing mechanical rhythms of the cardiac cycles, consistent with ECG recordings. Ligation of coronary artery leads to myocardial infarction that causes ST-segment elevation, as shown in Fig. S63B. Figure 6 M& N show the contractility patterns of the right and left atria (RA and LA), and the right and left ventricles (RV and LV) under normal and MI conditions, respectively, measured by an implanted thera-gripper where the output features of the sensors are determined by their experienced strain that significantly correlates to their positions on epicardial surface. The S4 (LV) displays the largest amplitude due to a maximum experienced strain, indicating the intrinsic highest myocardium strength in the LV chamber. Figure 6 I reveals the area of infarction two weeks after the MI surgery. The results in Fig. 6 N demonstrate that the LV outflow obstruction changes patterns of ventricular contraction. The sensors S2 (RV) and S4 (LV) experience a reduced strain change due to the consequent loss of contractile myocardium, which, correspondingly, reduces force of myocardial contractility and decreases heart rate. Collectively, such nature-inspired design establishes a foundation for implantable robots to harness on-demand motion for structural adaptation inside body and sensory functions for real-time optimization of therapeutic outcomes.\n\n# Discussion\n\nIn this study, we report concepts and device designs to achieve untethered soft robots that highly emulate biological systems and seamlessly integrate actuators, sensors, and stimulators to enable structural adaption and reconfigurable interfaces that minimize tissue damage *in vivo*, enhance mechanical match at biotic-abiotic interface, increase biocompatibility, and improve multimodal functionality with spatiotemporal precision. Our soft robots primarily consist of an e-skin layer made of multi-modal nanocomposites that mimic receptors in biological skin to perceive various external stimuli, and an artificial-muscle layer made of thermally responsive PNIPAM hydrogel to generate adaptive motion. We employ an *in situ* solution-based approach to fabricate the flexible multi-modal e-skin. This facile method represents a versatile platform, for a broad range of functional materials (e.g., AgNWs, RGO, and PEDOT:PSS) to be incorporated into a polymeric matrix (e.g., PDMS and PI) to form various types of sensors (e.g., temperature, pressure, and strain) with high spatiotemporal resolution. Such biomimicry design of soft robots offers versatility in mechanical motions including bending, twisting, and expanding as well as diversity in structural deformation, including configurations resembling starfish, fishbone, chiral seedpod, and others. On-demand actuation triggered by electrothermal stimulation from electrical heaters embedded in the e-skin allows precise, independent control of regional parts of the soft body. Furthermore, integration with wireless modules enables the robots to be controlled and communicated without tethering, even when implanted inside body. To demonstrate the broad utility, we develop soft robots that are tailored for specific application scenarios. Specifically, we fabricate a soft robotic gripper that can wrap around a bladder to enable coordinated, closed-loop operation of bladder-volume evaluation and electrical stimulation to treat an overactive bladder, a robotic cuff that can twist around a blood vessel for measuring blood pressure, and an ingestible robot that can reside in a stomach for prolonged pH sensing and drug delivery. *In vivo* studies with a mouse model demonstrate capabilities of a soft robotic thera-gripper in gently enveloping a beating heart, spatiotemporal assessment of electrophysiological activity, quantification of cardiac contractility, and supplying electrical stimulation for pace regulation. These demonstrations showcase the potential applications of such soft robots as next-generation biomedical implants with structural intelligence and multi-functionalities. Future advancements could further enhance the synergistic interaction between soft implantable robots and biological tissues, to achieve long-term biocompatibility and stability in dynamic physiological environments for improving treatment of chronic diseases.\n\n# Materials and methods\n\nMaterials: N-isopropylacrylamide (NIPAM, 98%) was purchased from TCI. Poly (vinyl alcohol) (PVA, 99+% hydrolyzed), poly(D,L-lactide-co-glycolide) (Mw 50,000–75,0000), acrylamide (AAm, 99%), N, N′-Methylenebisacrylamide (BIS, 99%), N,N,N′,N′-Tetramethyl-ethylenediamine (TMEDA, 99%), and ammonium persulfate (APS, > 98%) were purchased from Sigma-Aldrich. Rhodamine B and silver nitrate (AgNO₃ 99.9% ) was purchased from Themo Scientific. Ethylene glycol (EG, > 99%) was purchased from BDH Chemicals. Polyvinylpyrrolidone (Mw ≈55000, PVP) and poly(3,4-ethylenedioxythiophene)-poly(styrenesulfonate) (PEDOT:PSS, 3.0–4.0%) were purchased from Sigma-Aldrich. Copper chloride (CuCl₂) was purchased from Ward’s Science. The graphite powder was purchased from Spectrum Chemical Manufacturing Corp. The sodium nitrate (NaNO₃, > 99%), hydrogen peroxide (H₂O₂, 30% w/w), the potassium permanganate (KMnO₄, > 99%), hydrochloric acid (HCl, 36.5–38%) and sulfuric acid (H₂SO₄, 95%-98%) were purchased from BDH chemicals. Ethylenediamine (EDA, 99%) was purchased from Alfa Aesar.\n\nMaterials characterization: The SEM images were taken by the field emission scanning electron microscope (Hitachi S-4700 with EDS). The XPS spectra were obtained by Kratos Axis Supra x-ray photoelectron spectrometer, allowing to determine the elemental composition of the top ~ 10 nm of the sample surface. The XRD patterns of functional nanocomposites were obtained using the Rigaku SmartLab theta-theta diffractometer. The FTIR spectra were recorded using Hyperion 1000 with Tensor 27 spectrometer. The thermal images were taken with an infrared (IR) camera (FLIR ETS320). The performance of the drug-release patch was characterized with a Ultraviolet-visible (UV-vis) spectrometer (VWR UV-1600PC).\n\n## Multi-modal sensory soft robots with nature-inspired designs\n\nThe fabrication of thermo-responsive hydrogel: Poly(N-isopropylacrylamide) (PNIPAM) was synthesized based on precipitation polymerization. In a typical example, 500 µL NIPAM as monomer (25 wt%), 50 µL BIS as crosslinker (0.5 wt%), 140 µL APS (1 wt%)/200 µL TEMED (2 wt%) as initiator were mixed to form the precursor solution. After 30 mins, the precursors can polymerize, in situ, to form the thermos-responsive PNIPAM hydrogel.\n\nThe fabrication of AgNWs: AgNWs were synthesized based on a modified polyol method. 100 mL of EG containing NaCl (~ 0.05 mM), PVP (~ 189 mM), AgNO₃ (~ 0.0014 mM), and CuCl₂ (~ 0.017 mM) were added to a round-bottom flask and heated at 185°C for 1h in an oil bath. Then, 30 mL AgNO₃ EG solution (~ 0.12 M) was added dropwise with vigorous stirring. After the reaction was completed, the flask was cooled to room temperature. The AgNW suspension in the EG was diluted with 30 mL water and sedimented for 14h. The supernatant was decanted, the water was added to reach 160 mL in total volume of the solution. The suspension was sedimented for 14h and decanted. Then, 50 mL water was added to this mixture, and 100 mL acetone was slowly added with gentle mixing. After centrifugation, the as-formed AgNW pellets was fully resuspended in a 20 mL PVP aqueous solution (~ 0.5 wt%). The cleaning process was repeated 4 times. Finally, the AgNW pellets were stored in water for later use.\n\nThe fabrication of reduced graphene oxide: The graphene oxide (GO) was synthesized based on a modified Hummers method. In general, 5 g of graphite powder and 2.5 g of NaNO₃ were added into 120 mL sulfuric acid in an ice bath under stirring for 2h. Subsequently, 15 g of KMnO₄ was slowly added into the solution under a temperature < 20°C. After 1 h, the reaction temperature was raised to 35°C for overnight reaction. 150 mL H₂O was added to the mixture for 12 h reaction under 98°C. Then, 500 mL of H₂O and 20 mL of H₂O₂ were added to the mixed solution. Finally, the solution was washed with HCl (1M) and H₂O until the pH was natural. The EDA was used as the reducing agent to reduce the graphene oxide.\n\nThe fabrication of a soft robot inspired by a starfish: The fabrication process of the multi-modal functional electronic-skin (e-skin) is shown in Fig. S2A. A polyimide (PI) substrate (thickness ~ 10 µm) was patterned on a pre-cleaned and plasma-pretreated glass silde using laser-cutter (six rectangular, each is 15mm x 6mm). The AgNWs solution (50 wt%), the RGO suspension (5 wt%), and PEDOT:PSS solution were dropcast onto the patterned glass slide and heated at 50°C for drying. After the solution was dried, the structured functional materials were fabricated with laser cutting (SFX-50GS). Then, a thin layer of liquid PI was spin-coated onto the patterned thin film of functional nanomaterials and cured at 150°C for 1h. Finally, the resultant film was cutted out with a laser beam and peeled off from the glass slide. The as-formed multi-modal e-skin was encapsulated with a layer of parylene (thickness ~ 2 µm) and bonded onto PNIPAM hydrogels via the adhesive glue (3M Vetbond 1469c) (Fig. 2 C) to generate the multi-modal sensory soft robot with a nature-inspired starfish design.\n\nThe fabrication of a soft robot inspired by chiral seedpods: The gold nanomembrane (Au, thickness ~ 200 nm) and adhesive chromium layer (Cr, thickness ~ 10 nm) were deposited by the magnetron sputtering on the PI film (thickness ~ 10 µm). The patterns for Au electronics and PI substrate shown in Fig. S8A were formed using the laser cutting machine. Then the e-skin made of patterned Au/PI film and encapsulated by a parylene layer (thickness ~ 2 µm), is attached to the PNIPAM hydrogel (15mm x 6mm) using the bioadhesive layer.\n\nThe fabrication of a soft robotic pill: Firstly, the PEDOT:PSS solution was dropcast onto a pre-treated glass slide spacer, dried under 50°C and patterned using a laser-cutter. Secondly, the PEDOT:PSS/PI nanocomposite thin film was formed by spin-coating liquid PI onto the patterned PEDOT:PSS, and fully curing at 150°C for 1h. Next, the e-skin layer received a protective coating of parylene, ~ 2 µm in thickness. Finally, two pieces of PEDOT:PSS/PI nanocomposite film were adhered to a piece of PNIPAM hydrogel at the edges (Fig. S10A).\n\n## Static finite element analysis for various soft robots\n\n3D finite element analyses (FEA) in commercial software ABAQUS were utilized to predict the shape transformation process of soft robots with different patterns and dimensions. The elastic modulus (E) and poison’s ratio (υ)) used in the simulations were EPNIPAM = 90 KPa, υPNIPAM = 0.30 for PNIPAM hydrogel, and EPI = 2.5 GPa, υPI = 0.34 for PI.\n\n## Wireless sensing and actuation of soft sensory robot\n\nThe fabrication of polyacrylamide (PAAm) hydrogel pressure sensor: In polyacrylamide (PAAm) hydrogel synthesis, 500 µL AAm as monomer (25 wt%), 50 µL BIS as crosslinker (0.5 wt%), 140 µL APS (1 wt%)/200 µL TEMED (2 wt%) as initiator were mixed to form the precursor solution. After 10 mins, the precursor can polymerize, in situ, to form the PAAm hydrogel. Then a parallel-plate capacitor-based pressure sensor was formed through sandwiching PAAm hydrogel between two electrodes made of Au/PI bilayer (Fig. 4 B).\n\nThe fabrication of the soft sensory robot: Laser cutting of the Au/PI bilayer formed the electrical heater that was connected to a Cu receiver coil (Fig. 4 C). This assembly was then covered with a thin layer of parylene (thickness ~ 2 µm). Following this, the PNIPAM muscle was bonded to the electrical heater to form the bilayer structure. Finally, the actuation component was integrated with the PAAm-based pressure sensor (Fig. 4 A). Here, the circuits for sensing and actuating can be integrated together onto a single piece of Au/PI bilayer film (Fig. S27C).\n\nThe characterization of wireless power transmitting and pressure sensing: The detailed power transfer performance and pressure sensing data acquisition are explained in Supplementary Note S3.\n\nWireless control of locomotion: We implement a three-lead LC receiving network based on the frequency response characteristics of magnetic resonance coupling (Fig. S29A). In this system, two leads are connected to the full length of the coil, while a third electrode is connected to the middle of the coil loops, resulting in the formation of a smaller inductor with the common electrode (Fig. S29B). The two coil loops with different inductive values are paired with different capacitors (Full length ~ 200 pF; Half length ~ 47 pF) to form LC circuits with different resonant frequencies yet similar small quality factors (Fig. S29C). Each soft robotic arm is connected to an individual pair of leads to harvest RF power transmitted at different frequencies.\n\n## LCST tunability of PNIPAM-based hydrogel\n\nThe synthesis of poly(NIPAM-co-acrylamide) (P(NIPAM-AAm)) hydrogel: The synthesis of the PNIPAM-co-PAAm was conducted through a free radical polymerization method. In a typical procedure, a mixture of 450 µL NIPAM monomer (25 wt%) and 50 µL AAm monomer (at concentrations of 5 wt%, 10 wt%, 15 wt%, 20 wt% and 25 wt%) was prepared. Additionally, 50 µL of BIS crosslinker (0.5 wt%), 140 µL of APS initiator (1 wt%) and 200 µL of TEMED (2 wt%) were added to form the precursor solution. After 30 mins, the precursors can polymerize to form the thermos-responsive P(NIPAM-AAm) hydrogel.\n\nMeasurement of bending angle of soft robots based on PNIPAM-co-PAAm hydrogel: The bending angles were measured as a function of time under different electrical powers in both a simulated in vivo environment (37°C, PBS solution) and an in vitro condition (room temperature, PBS solution). The measurements were performed for three different levels of AAm incorporation: 0 wt%, 5 wt%, and 10 wt%.\n\n## A soft robotic gripper for bladder control\n\nThe fabrication of a robotic gripper: The process began with the fabrication of e-skin layer via laser cutting Au/PI bilayer film and applying a parylene coating. The e-skin layer includes electrical heaters, electrical stimulators, and serpentine Au resistors (Fig. S47A). Then, the PNIPAM hydrogel was adhered onto the electrical heater, and the Au/PI resistor was anchored onto one piece of PAAm hydrogel at the edges to form a strain sensor with a buckled structure (Fig. S47B).\n\nMeasurement of biomimetic bladder volume: A balloon model was used to mimic the natural bladder to evaluate the actuation and sensing performance of the soft gripper. After thermal stimulation, the soft gripper can wrap around the balloon and the strain sensor can attach onto the balloon surface via the PAAm hydrogel. A syringe pump was used to inject and extract water into the balloon to imitate the filling and emptying behavior of natural bladder. The PowerLab (Model 16/35, AD Instruments) allowed the recording of output signals.\n\nWireless sensing of resistive strain sensor and close-looped control of bladder electrical therapy robot: A power harvesting and signal conditioning circuit was fabricated and soldered using the method of soft PCB fabrications (Supplementary Note S4). We developed an alternative approach for powering and signal conditioning. This strategy enables the accurate readout of the resistive strain sensor without significantly affecting the wireless power transmission between coils. Specifically, we fabricate a full-bridge rectifier with surface-mount diodes, enabling the conversion of the alternative current (AC) obtained via the receiver coil into direct current (DC). Subsequently, the rectified DC is fed into a 3.3V low-dropout (LDO) regulator. The output from this regulator serves as the power source for both a Bluetooth-Low-Energy (BLE) System-on-Chip (SoC) and a voltage divider circuit. The voltage divider circuit consists of a reference resistor connected in series with the as-fabricated resistive strain sensor. The voltage divider circuit consists of a reference resistor connected in series with the as-fabricated resistive strain sensor. The voltage across the resistive strain sensor through the voltage divider circuit was sampled by a 14-bit on-chip Successive Approximation Analog to Digital Converter (SAADC). A custom BLE service transmits the sampling value to host terminals acting as BLE clients and parsers to allow wireless readout of strain values. For achieving a closed-loop control of electrical stimulation in the treatment of dysfunctional bladder system, we further programmed the BLE SoC by enabling a pulse-width modulation (PWM) instance. The instance, combined with on-board power amplification and filtering system, enables the programmed electrical stimulation corresponding to detected bladder strain variations.\n\n## A robotic cuff for vascular system\n\nThe fabrication of a robotic cuff: Firstly, we used laser cutter to fabricate the e-skin layer with a pattern of parallel strips that exhibit a 45° angle with the longitudinal direction of the device. The e-skin layer contains a serpentine Au ribbon as a strain sensor (Fig. S50A). Subsequently, this layer was coated with a parylene film ~ 2 µm in thickness. Finally, the PNIPAM hydrogel-muscle layer was bonded to the e-skin layer.\n\nMeasurement of biomimetic blood pressure: A rubbery tube was used to mimic the artery system to evaluate the performance of the soft robotic cuff. The soft robotic cuff can twist around the artificial artery upon thermal stimulation. A pulsatile flow of water was created to simulate the pulsation pattern of the artery system. The measured signals of the strain sensor were recorded with the PowerLab.\n\n## An ingestible robot for digestive system\n\nThe fabrication of a drug-releasing patch: In brief, 5 mg poly(lactic-co-glycolic acid) (~ PLGA) was dissolved in 5.1g acetone containing 5 mg Rhodamine B (~ RhB). Then the mixture was poured into a poly(dimethylsiloxane) (~ PDMS) spacer, and acetone was removed from the mixture under vacuum condition. Finally, the as-formed film of PLGA/RhB was cut into small pieces of drug-release patch with a diameter ~ 2 mm.\n\nThe fabrication of PEDOT:PSS/PVA hydrogel sensor: For hybrid hydrogel fabrication, first a 10 wt% PVA solution was made by dissolving PVA powder in water. Then 5 wt% PEDOT:PSS aqueous dispersion was added into the PVA solution followed by slow mixing for 24 h. The prepared PEDOT:PSS/PVA solution was poured into glass spacer, followed by freezing at -20°C for 8 h and thawing at 25°C for 3 h for three times.\n\nThe fabrication of a soft ingestible robot: The process began with the formation of e-skin layer. The circuits for sensing were fabricated on Au/PI bilayer film with a laser cutter, while the remaining parts received a parylene coating. The PEDOT:PSS/PVA hydrogel pH sensors were adhered onto the side of Au/PI film with conductive electrodes, while the drug-release patches were integrated onto the other side. Then, two pieces of e-skin layer were adhered to a piece of PNIPAM hydrogel at the edges, as shown in Fig. S51A.\n\nQuantification of RhB release from the drug patch: The drug-release patches of PLGA/RhB mixture were immersed into phosphate-buffered saline (~ PBS) solutions (pH ~ 5) for 1 h under different temperatures ranging from 25 to 45°C. The UV-vis absorbance spectrometer was used to analyze the amount of the RhB released from the drug-patch.\n\nMeasurement of pH sensitivity: The PEDOT:PSS hybrid hydrogels were submerged into PBS solutions with different pH values ranging from 3 to 8. In 5 mins, hydrogels were removed from PBS solutions and their resistance was measured with PowerLab. The effect of pH on the electrical properties of the PEDOT:PSS/PVA hydrogel is attributed to the ionic interaction between PEDOT and PSS polymer chains. Under acidic conditions, PEDOT chains are uniformly distributed along the PSS polymer chains, ensuring the formation of continuous electrical connections between PEDOT segments. While pH shifts from acidic to more alkaline, the homogenous distribution of PEDOT along the PSS polymer chains is interrupted by negatively charged hydroxy groups, and buried inside the insulating PSS phase, as illustrated in Fig. S51D.\n\n## Cell morphology analysis, cell viability test and histological analysis\n\nCell morphology analysis: Swiss 3T3-J-2 cells are seeded in a 96-well plate with 10,000 cells per well and cultured for 48h at 37°C. Here, the cells are exposed to pure PNIPAM hydrogel, AgNWs/PI nanocomposite, RGO/PI nanocomposite, PEDOT:PSS/PI nanocomposite, MXene/PI nanocomposite, and the integrated soft robot. Notably, each of these functional units was encapsulated with a parylene film (thickness ~ 2 µm). For examining the effect of thermal stimulation on cell viability, the 3T3-J-2 cells with a soft robot are subjected to an environment at 39°C for a duration of 48h. To detect Vimentin antigen, chromogenic Immunohistochemistry (IHC) is performed on paraffin-embedded cells that were sectioned at 5 microns. This IHC is carried out using the Leica Bond Rx Autostainer system. Slides are dewaxed in Bond Dewax solution (AR9222) and hydrated in Bond Wash solution (AR9590). Heat-induced antigen retrieval is performed at 100ºC in Bond-Epitope Retrieval solution 1 pH-6.0 (AR9961). After pretreatment, slides are incubated with Vimentin Antibody (5741, Cell Signaling Technologies) at 1:1000 for 30m followed with Novolink Polymer (RE7260-CE) secondary. Antibody detection with 3,3′-diaminobenzidine (DAB) is performed using the Bond Intense R detection system (DS9263). Stained slides are dehydrated and coverslipped with Cytoseal 60 (8310-4, Thermo Fisher Scientific). A positive control tissue is included for this run. High-resolution acquisition of IF slides is performed with the Aperio Versa 200 scanner (Leica Biosystems Inc.) at an apparent magnification of 20X. Immunofluorescence reaction (IF) is performed on paraffin-embedded cells that are sectioned at 5 microns. This assay is carried out on the Bond Rx fully automated slide staining system (Leica Biosystems) using the Bond Research Detection kit (DS9455). Slides are dewaxed in Bond Dewax solution (AR9222) and hydrated in Bond Wash solution (AR9590). Heat induced antigen retrieval is performed at 100ºC in Bond-Epitope Retrieval solution 1 pH-6.0 (AR9961) for 30 minutes. After pretreatment, slides are incubated with Vimentin Antibody (5741, Cell Signaling Technologies) at 1:1000 for 30m. Ready-to use secondary antibody, Leica’s Novolink Polymer (RE7260-CE) is used followed by TSA Cy5 (SAT705A001EA, Akoya Biosciences) to visualize the target of interest. Nuclei were stained with Hoechst 33258 (Invitrogen). The stained slides are mounted with ProLong Gold antifade reagent (P36930, Life Technologies). Positive controls are included for each assay. High resolution acquisition of IF slides is performed with the Aperio Versa 200 scanner (Leica Biosystems Inc.) at an apparent magnification of 20X.\n\nCell viability test: Swiss 3T3-J-2 cells are seeded in a 96-well plate with 10,000 cells per well and cultured for 48h. Here, the cells are exposed to pure PNIPAM hydrogel, and the integrated soft robot. For examining the effect of thermal stimulation on cell viability, the 3T3-J-2 cells with a soft robot are subjected to an environment at 39°C for a duration of 48h. We use the Aperio Cytoplasmic version 2 algorithm on image regions that were annotated to exclude artifacts. The algorithm input parameters included Clear Area Intensity, Optical Density values (RGB) for both counterstain and biomarker detection, intensity threshold values, and minimum/maximum size and smoothing values for cell segmentation. Several of these parameters were adjusted to apply to the specific marker (Vimentin) and cells.\n\nHistological analysis: Explanted organs were bisected and stored in 10% buffered formalin inside 50 mL conical tubes. Following this, these tissue samples were subsequently prepared for histological evaluation with H&E staining and were imaged using Leica Biosystems.\n\n## A soft robotic thera-gripper for epicardial sensing and pacing\n\nThe fabrication of a robotic thera-gripper: The e-skin layer of the soft robotic gripper is formed using the laser cutting machine, consisting of four strain sensors made of serpentine Au/PI resistors, two Au pacing electrodes, and two temperature sensors made of thermal resistors, as shown in Fig. S52A & B. Following the application of a parylene film, four pieces of PNIPAM hydrogel were bonded onto the e-skin layer to form the actuators. The soft robotic gripper can gently hold a mouse heart during its beating movement.\n\nIn vivo animal experiment: Procedures used in the study were reviewed and approved by the Institutional Animal Care and Use Committee and Research Animal Resources at the North Carolina University Chapel Hill (IACUC ID:21–241.0). Female mice (weight 20 to 30 g; age, 10 weeks) were purchased from the Jackson Laboratory. The detailed surgery process is described in Supplementary Note S9. The electrocardiography (ECG) and heart function were monitored simultaneously using commercial equipment (PowerLab). The myocardial infarction surgery was conducted by permanently occluding the left coronary artery (LCA). 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Proc. 60 (1985) 321–343. https://doi.org/10.1016/s0025-6196(12)60540-0.\n\n# Supplementary Files\n\n- [SupportingInformation11252023.pdf](https://assets-eu.researchsquare.com/files/rs-3665801/v1/aa9da08c9f18f5c51e8787e1.pdf) \n Supplementary information\n\n- [SupplementarymovieS1.mp4](https://assets-eu.researchsquare.com/files/rs-3665801/v1/e2f21b4465958ecf3dd59943.mp4) \n Supplementary movie S1: Soft robot with a nature-inspired starfish design\n\n- [SupplementarymovieS2.mp4](https://assets-eu.researchsquare.com/files/rs-3665801/v1/0547282cb7f7f48cc3e0325e.mp4) \n Supplementary movie S2: Shape transformation of soft robots with various configurations\n\n- [SupplementarymovieS3.mp4](https://assets-eu.researchsquare.com/files/rs-3665801/v1/29cfe1f3a66b70358151f604.mp4) \n Supplementary movie S3: Soft robot with a helical structure biomimicking a chiral seedpod\n\n- [SupplementarymovieS4.mp4](https://assets-eu.researchsquare.com/files/rs-3665801/v1/747bbf200558eb7573eded87.mp4) \n Supplementary movie S4: The shape transformation of a soft robotic pill\n\n- [SupplementarymovieS5.mp4](https://assets-eu.researchsquare.com/files/rs-3665801/v1/9812d2bc0a3df3420439f20c.mp4) \n Supplementary movie S5: A three-arm soft robotic gripper via sequentially programming input power\n\n- [SupplementarymovieS6.mp4](https://assets-eu.researchsquare.com/files/rs-3665801/v1/d2dd7881b40af8a5bb14e23f.mp4) \n Supplementary movie S6: A four-arm soft robotic gripper via simultaneously programming input power\n\n- [SupplementaryMovieS7.mp4](https://assets-eu.researchsquare.com/files/rs-3665801/v1/1f7dd513e0cf9a2e15c665c7.mp4) \n Supplementary movie S7: The storing and release process of bioelectronic robots in a medical catheter\n\n- [SupplementaryMovieS8.mp4](https://assets-eu.researchsquare.com/files/rs-3665801/v1/bc48728efdc85281761ccb0b.mp4) \n Supplementary movie S8: The safe transportation of soft robotic devices through the inner lumens of swine tissue/organ"} {"paper_id": "prb85", "title": "Dynamics of the compartmentalized Streptomyces chromosome during metabolic differentiation", "text": "Dynamics of the compartmentalized Streptomyces chromosome during metabolic differentiation\n\nVirginia Lioy\nInstitute for Integrative Biology of the Cell https://orcid.org/0000-0002-5366-0462\n\nJean-Noël Lorenzi\nUniversité Paris-Saclay CEA CNRS Institute for Integrative Biology of the Cell (I2BC) https://orcid.org/0000-0002-4520-1266\n\nSoumaya Najah\nUniversité Paris-Saclay CEA CNRS Institute for Integrative Biology of the Cell (I2BC)\n\nThibault Poinsignon\nUniversité Paris-Saclay CEA CNRS Institute for Integrative Biology of the Cell (I2BC)\n\nLeh Hervé\nUniversité Paris-Saclay CEA CNRS Institute for Integrative Biology of the Cell (I2BC)\n\nCorinne Saulnier\nUniversité Paris-Saclay CEA CNRS Institute for Integrative Biology of the Cell (I2BC)\n\nBertrand Aigle\nhttps://orcid.org/0000-0001-5266-5926\n\nSylvie Lautru\nUniversité Paris-Saclay CEA CNRS Institute for Integrative Biology of the Cell (I2BC)\n\nAnnabelle Thibessard\nUniversité de Lorraine INRAE DynAMic https://orcid.org/0000-0001-9604-9113\n\nOlivier Lespinet\nUniversité Paris-Saclay CEA CNRS Institute for Integrative Biology of the Cell (I2BC)\n\nPierre Leblond\nUniversité de Lorraine INRAE DynAMic\n\nYan Jaszczyszyn\nInstitute for Integrative Biology of the Cell (I2BC), UMR 9198CNRS, CEA, Paris-Sud University F-91198, Gif-sur-Yvette\n\nKevin Gorrichon\nUniversité Paris-Saclay CEA CNRS Institute for Integrative Biology of the Cell (I2BC)\n\nNelle Varoquaux\nTIMC-IMAG CNRS - Université Grenoble Alpes Grenoble France\n\nIvan Junier\nTIMC-IMAG CNRS - Université Grenoble Alpes Grenoble France\n\nFrédéric Boccard\nUniversité Paris-Saclay CEA CNRS Institute for Integrative Biology of the Cell (I2BC)\n\nJean-Luc Pernodet\nUniversité Paris-Saclay CEA CNRS Institute for Integrative Biology of the Cell (I2BC)\n\nStéphanie Bury-Moné (stephanie.bury-mone@i2bc.paris-saclay.fr)\nUniversité Paris-Saclay, CEA, CNRS, Institute for Integrative Biology of the Cell (I2BC)\n\nArticle\n\nKeywords: Chromosome conformation, Transcriptomics, Genome dynamics, Genomic islands, Compartmentalization, Specialized metabolism biosynthetic gene clusters, Antibiotic production, Streptomyces\n\nPosted Date: January 25th, 2021\n\nDOI: https://doi.org/10.21203/rs.3.rs-145840/v1\n\nLicense: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License\n\nVersion of Record: A version of this preprint was published at Nature Communications on September 1st, 2021. See the published version at https://doi.org/10.1038/s41467-021-25462-1.\nDynamics of the compartmentalized Streptomyces chromosome during metabolic differentiation\n\nVirginia Lioy1,*, Jean-Noël Lorenzi1, Soumaya Najah1, Thibault Poinsignon1, Hervé Leh1, Corinne Saulnier1, Bertrand Aigle2, Sylvie Lautru1, Annabelle Thibessard2, Olivier Lespinet1, Pierre Leblond2, Yan Jaszczyszyn1, Kevin Gorrichon1, Nelle Varoquaux3, Ivan Junier3, Frédéric Boccard1, Jean-Luc Pernodet1, Stéphanie Bury-Moné1,*\n\n1Université Paris-Saclay, CEA, CNRS, Institute for Integrative Biology of the Cell (I2BC), 91198, Gif-sur-Yvette, France.\n2Université de Lorraine, INRAE, DynAMic, F-54000 Nancy, France\n3TIMC-IMAG, CNRS - Université Grenoble Alpes, Grenoble, France\n*Address correspondence to: stephanie.bury-mone@i2bc.paris-saclay.fr, virginia.lioy@i2bc.paris-saclay.fr\n\nRunning Title: Dynamics of a compartmentalized genome\n\nKeywords: Chromosome conformation; Transcriptomics; Genome dynamics; Genomic islands; Compartmentalization; Specialized metabolism biosynthetic gene clusters; Antibiotic production; Streptomyces\nAbstract\n\nStreptomyces are among the most prolific bacterial producers of specialized metabolites, including antibiotics. The linear chromosome is partitioned into a central region harboring core genes and two extremities enriched in specialized metabolite biosynthetic gene clusters (SMBGCs). The molecular mechanisms governing structure and function of these compartmentalized genomes remain mostly unknown. Here we show that in exponential phase, chromosome structure correlates with genetic compartmentalization: conserved, large and highly transcribed genes form boundaries that segment the central part of the chromosome into domains, whereas the terminal ends are transcriptionally, largely quiescent compartments with different structural features. Onset of metabolic differentiation is accompanied by remodeling of chromosome architecture from an ‘open’ to a rather ‘closed’ conformation, in which the SMBGCs are expressed forming new boundaries. Altogether, our results reveal that S. ambofaciens’ linear chromosome is partitioned into structurally distinct entities, indicating a link between chromosome folding, gene expression and genome evolution.\n\nIntroductory paragraph\n\nBacteria of the genus Streptomyces are amongst the most prolific producers of specialized metabolites with applications in medicine, agriculture and the food industry1. The biosynthesis of these specialized metabolites (e.g. antibiotics and pigments) generally occurs after ‘metabolic differentiation’, a physiological transition from primary to specialized metabolism2,3. This transition coincides with morphological differentiation4 (e.g. formation of the secondary multinucleated mycelium, sporulation) that occurs late in the growth phase. These metabolic and\nmorphological changes are controlled by highly interconnected regulatory mechanisms that have been studied mostly at the transcriptional, translational and post-translational levels4-7. However, a clear link between global chromosome organization and metabolic differentiation has yet to be established.\n\nStreptomyces possess an unusual linear chromosome. Moreover, its extremities, or ‘terminal arms’, contain terminal inverted repeats (TIRs) capped by telomere-like sequences. In addition, the chromosome is large (6-15 Mb) with an extreme GC content (circa 72%). Finally, the Streptomyces chromosome presents a remarkable genetic compartmentalization, with a distinguishable central region and the terminal arms. The central region primarily contains core genes, common to all Streptomyces species, these being often essential8-13. The terminal arms are mainly composed of conditionally adaptive genes, in particular, enriched in specialized metabolite biosynthetic gene clusters (SMBGCs)14. In addition, they are prone to large DNA rearrangements and frequent recombination12,15,16,17. Importantly, many SMGBCs appear silent or poorly expressed under laboratory conditions, giving rise to the concept of ‘cryptic’ SMBGCs. The basis of the regulation of these clusters in relation to the overall genome dynamics remains to be explored.\n\nThe development of chromosome conformation capture (3C) methods coupled to deep sequencing provided novel concepts in bacterial chromosome biology18,19. Notably pioneer studies revealed that bacterial chromosomes present a high degree of 3D-organization in macrodomains and/or ‘chromosome interacting domains’ (CIDs), mediated by multiple structural factors, including transcription and replication20-27. Here, we explore the dynamics of the Streptomyces chromosome during metabolic differentiation. By combining multi-omic approaches, we show that the dynamics of gene expression correlate with the folding of the linear chromosome\nof Streptomyces ambofaciens ATCC 23877 into transcriptionally active and silent compartments. Moreover, metabolic differentiation is accompanied by a huge remodeling of chromosome architecture from an ‘open’ to a rather ‘closed’ conformation, SMBGCs forming new boundaries. Altogether, our results highlight a link between chromosome folding, gene expression and genome evolution.\n\nResults\n\nCompartmentalization of the Streptomyces ambofaciens genome highlighted by comparative genomics and functional annotation\n\nThe genetic compartmentalization of the S. ambofaciens ATCC 23877 genome was previously reported12. However, here we took advantage of the numerous Streptomyces available sequences to update the cartography of the genome. We also used gene persistence28 as a new indicator to describe the organization of Streptomyces genome. Gene persistence reflects the tendency for genes to be conserved in a large number of genomes. As shown in other bacteria, gene persistence is associated with gene essentiality and similar expression levels28-30. Here, we calculated a gene persistence index by determining the frequency of a given gene in a panel of 125 complete Streptomyces genomes (Supplementary Table 1)31. The highest level of persistence associated with the best reciprocal matches between genes of all these genomes defines the core-genome31. In addition, we mapped the genes encoding the ‘actinobacterial signature’ previously identified32 as those coding sequences (CDSs) that are nearly universal among actinobacteria. In contrast, we searched the S. ambofaciens ATCC 23877 genome for variable regions, potentially acquired by horizontal gene transfer. For this purpose, we identified unique genes as well as genomic islands (GIs,\nSupplementary Table 2, Supplementary Fig. 1). These are defined as DNA sequences that are inserted in regions of synteny (i.e. same orthologous gene order in closely related genomes, see Methods). Thus genes from the core, the actinobacterial signature and/or presenting a high level of persistence are enriched in the central region, whereas GIs and unique CDSs are enriched in chromosome extremities. The results clearly highlight the compartmentalization of the S. ambofaciens genome (Fig.1, Supplementary Table 3). Synteny gradually disappears in terminal arms (Fig.1), as previously reported\\(^{12}\\). This makes it difficult to have an operational delineation of the limits of these arms. However, since the first and last ribosomal operons approximately mark the limits of a central region beyond which the synteny level falls (Fig.1), these operons were used as limits for definition of the left and right extremities in this study.\n\nFunctional annotation also highlighted a bias of gene distribution along the chromosome (Fig.1, Supplementary Table 3). As a proxy for major metabolic processes, we used the functional RNA genes (encoding rRNA, tRNA, tmRNA, RNase-P RNA, SRP-RNA) and genes encoding functions related to translation and/or RNA stability. We also mapped the genes encoding nucleoid-associated proteins (NAPs) and chromatin structural factors, further shorten 'NAPSFs', that play a central role in the dynamic organization of the bacterial chromosome and are enriched in the central region (Fig.1, Supplementary Table 3). Finally, we used the antiSMASH secondary metabolite genome mining pipeline (version 5.1.0)\\(^{33}\\) to identify putative SMBGCs (Supplementary Table 4). These genes are preferentially located in the terminals arms and almost half of them are present within GIs (Fig.1, Supplementary Table 3). Accordingly, GIs are 3.5-fold enriched in SMBGC genes (\\(p\\) value < \\(2.2 \\times 10^{-6}\\), Fisher's exact test for count data). These results illustrate that the\nhigh variability of Streptomyces extremities relates in particular to functions involved in metabolic differentiation.\n\nTogether, these analyses confirm the strong genetic compartmentalization of the S. ambofaciens chromosome. In this context, we then explored the extent to which this genetic organization correlates with gene expression and chromosome architecture.\n\nTranscription of the S. ambofaciens genome is strongly compartmentalized\n\nTo focus specifically on transcriptome dynamics during metabolic differentiation, while limiting cellular physiological heterogeneity in the colony, we took advantage of the fact that S. ambofaciens, like many Streptomyces\\(^2\\), does not sporulate in liquid medium. We chose MP5 and YEME liquid media (Table 1) in which S. ambofaciens grows in a rather dispersed manner that makes the cells also more accessible to further 3C-treatments. Moreover, for S. ambofaciens, MP5 medium was previously reported to be suited for the production of the antibiotics spiramycin\\(^{34}\\) and congocidine\\(^{35}\\) by S. ambofaciens while there is only limited antibiotic production in YEME medium (**Extended Data Fig.1.A&B**). The results showed that the transcriptomes were rather similar in exponential phase in both media, while commitment to specialized metabolism (C4, C5 and C7 conditions) was accompanied by major transcriptional changes that form a distinct cluster (**Fig.2.A&B**, **Extended Data Fig.1.C&D**). Notably, at the earliest time points in the growth period in both media, the terminal regions were rather poorly expressed, whereas transcription gradually increased toward terminal ends over the growth period (**Fig.2.B**), as previously reported in S. coelicolor\\(^{10,36}\\). We observed that the S. ambofaciens genome has a transcriptional landscape with approximately 90 % of the\ngenes significantly expressed ('CAT_1' level or more) and/or regulated (DESeq2 statistical analysis) in at least one condition (Extended Data Fig.2.A&B, Supplementary Table 5).\n\nAs shown by scanning the genome with respect to gene expression levels, we found a marked bias in the localization of poorly versus highly expressed genes along the genome as well as a positive correlation between gene persistence and expression (Fig. 2C, Extended Data Fig.2.C & D). The 332 chromosomal genes expressed at very high level in all conditions are mainly enriched in the central region of the genome (Supplementary Table 3, Fig.3D), whereas most (> 60 %) of the SMBGCs, GIs and mobile genetic elements (pSAM1, pSAM2 and a prophage) are silent or poorly expressed in at least one condition. Up to 19 and 23 % of SMBGC and GI genes, respectively, were found in this category in all tested conditions (Extended Data Fig.2.B). However, compared to other poorly conserved genes, SMBGCs have a higher proportion of highly induced genes, from 'CAT_0' to the highest ('CAT_3' or 'CAT_4') categories (Extended data Fig.2.C).\n\nInterestingly, as previously described in S. coelicolor36, we observed significant antisense-transcription throughout the genome. Considering the absolute number of transcripts, this antisense-transcription was positively correlated to the level of sense-transcription (Extended Data Fig.2.E), suggesting that spurious antisense-transcription can arise from highly transcribed regions. To investigate the relative importance of this antisense-transcription, we defined the 'antisense index' as the level of antisense-transcription over the total (sense plus antisense) transcription. Interestingly, in exponential phase, the antisense index was particularly high for GIs, mobile genetic elements and SMBGCs and very low in conserved regions enriched in the central region (except for pSAM2) (Extended Data Fig.2.F). During metabolic\ndifferentiation the antisense indices of GIs, pSAM1, prophage and especially SMBGCs tended to decrease (Extended Data Fig.2.F). This observation suggests that antisense-transcription could be a consequence of or directly involved in the regulation of gene expression concerning metabolic differentiation.\n\nTogether, these results indicate that the genetic compartmentalization of the Streptomyces genome clearly correlates with a compartmentalization of transcription, both sense and antisense.\n\nCompartmentalized architecture of the Streptomyces ambofaciens chromosome in exponential phase\n\nWe next asked the question, is a compartmentalized transcriptome correlated with a specific chromosome folding. We first performed 3C-seq on cells harvested in the exponential growth phase (Fig.3, Fig.4.A). The contact map displayed a main diagonal reflecting the frequency of contacts, which extends up to 1 Mb (Extended Fig.3.A). This diagonal contains loci acting as boundaries delimiting segments (visualized as squares, Fig.3.A, Fig.4.A) reminiscent of CIDs in other bacteria\\(^{20-22}\\).\n\nTo define these domains precisely in S. ambofaciens, we computed the ‘frontier index’, a domain boundary indicator built from a multiscale analysis of the contact map\\(^{37}\\). Briefly, two indices are computed, reflecting the intensity of the loss of contact frequencies when going downwards or upwards, respectively, to each genome position (Extended Fig.3.B). In this context, a boundary is defined by a significant change in both the downstream (green peaks, Fig.3.B) and upstream (orange peaks, Fig.3.B) directions (see method section for details). In exponential phase in YEME medium (non-optimal for antibiotic production, condition C6), we found 10 boundaries that defined the central region, delimited by the first and last rDNA operons, 9\ndomains ranging in size from 240 kbp to 700 kbp (**Fig.3.B**). These central domains resembled regular CIDs\\(^{20,23}\\) both in size and in the presumably nature of its formation (see below). The central boundaries are also conserved in exponential phase in MP5 medium, which is optimized for antibiotic production (**Fig.4.A**). Only four additional boundaries are observed in this medium (**Fig.4.A**). All rDNA operons coincide with the sharpest boundaries (**Fig.3.B, Fig.4.A**). The genes surrounding these operons, as well as those of other boundaries, are enriched in consecutive genes expressed at very high level (**Fig.4.B, Supplementary Table 5**), as previously reported in other bacterial models\\(^{20,23}\\). Interestingly, in exponential phase, we report a clear correlation between the level of gene conservation and the formation of boundaries (**Fig.4.C**). Moreover, the transcription of the genes present within boundaries tends to be oriented in the direction of continuous replication (odds ratio 1.8, \\( p \\) value 1.4.\\(10^{-8} \\), Fisher’s exact test for count data), with a very low antisense index (**Extended Data Fig.3.C**).\n\nGenome extremities form two large terminal compartments of 1.46 and 2.46 Mbp, respectively, with different structural features (**Fig.3**, **Fig.4.A** and **Extended Data Fig.3B**). Interestingly, within the terminal arms, the low transcriptional activity in exponential phase in YEME medium correlates well with the absence of boundaries. Of note, the boundaries present in each terminal domain in MP5 medium (one of which is composed of an active prophage) do not contain highly expressed genes and do not divide the terminal compartment into two parts (**Fig.4.A**). To compare the dynamics of contacts within regions, we thus calculated a dispersion index, reflecting the variability of the 3C-seq signal in each region (**Fig.4.D, Extended Data Fig.3.E**). Despite that the plots for the probability of contacts as a function of genomic distance are similar for both the terminal and central regions (**Extended Data Fig.3.D**), the\nterminal ends present a higher dispersion index than the central compartment in both media for contacts longer than 100 kbp (Fig.4.D, Extended Data Fig.3.E). This indicates that contacts between loci in the terminal regions are more variable than in the central compartment.\n\nThus, at the conformational level, the chromosome of exponentially growing cells of S. ambofaciens is partitioned into three compartments: a central compartment, actively transcribed and structured in multiple domains formed by the high-level expression of persistent genes and two large terminal compartments rich in GIs and SMBCGs and rather transcriptionally silent in which large-scale contacts are highly variable. Since in exponential phase, the boundaries are very similar in YEME and MP5 media and correspond mostly to persistent CDSs (Fig.4.C) or rDNA, their orthologous sequences may also structure the spatial organization of the chromosome in other Streptomyces species at a similar growth phase.\n\nChromosome remodeling during metabolic differentiation\n\nAs shown above, during metabolic differentiation we observed that the level of transcription gradually increased within the terminal ends (Fig.2). To determine whether transcription dynamics influence the 3D-organization of the chromosome, we performed 3C-seq on Streptomyces cells during metabolic differentiation in MP5 medium (48 h, condition C4) (Fig.4.E). The frontier index revealed changes in the boundaries along the primary diagonal; the boundaries identified in exponential phase were not detected anymore after 48 h in the growth medium (Fig.4.E). By contrast, the appearance of a very sharp boundary within the right terminal region that divides this arm into two domains of 1,350 kbp and 1,000 kbp, correlates very well with the increased level of transcription of the congocidine biosynthetic gene\ncluster (BGC, Fig.4.B & E). In a replicate experiment, we observed that the expression of another SMBGC, encoding the biosynthesis of a siderophore, could generate the formation of an additional boundary (Supplementary Fig.3.C). This illustrates some variability in the expression of SMBGCs during metabolic differentiation. Together, these results highlight the correlation between SMBGC expression and the formation of boundaries after 48 h. Accordingly, the level of conservation of genes present within the boundaries switches from highly persistent in exponential phase to poorly conserved during metabolic differentiation (Fig.4.C). In addition, a second boundary detected within the right compartment is located in the stambomycin BGC that is not or is poorly expressed in this condition. Interestingly, accompanying the formation of boundaries and the increase of transcription in the terminal compartments, the variability in the long-range contacts within the terminal compartments is comparable to that of the central compartment (Fig 4.D).\n\nThe contact map also revealed the appearance of a secondary diagonal after 48 h of growth, indicating an increase in the frequency of contacts between regions along the entire arms of the chromosome. This suggests that late in the cell cycle and in the absence of a central compartment segmented into multiple domains, the two chromosome arms are closer to each other (Fig.4.E & F). Remarkably, the second diagonal is slightly tilted when it moves away from the origin, representing an asymmetry in the contacts between loci within the terminal compartments.\n\nIn summary, our results indicate that the central and transcriptionally active compartments in exponential phase present no boundaries after 48 h of growth, whereas the terminal domains are locally remodeled concomitantly with the expression of SMBGCs and with a decrease in the variability of the long-range contacts. In addition, inter-arm contacts become more frequent. These results\nindicate that metabolic differentiation is accompanied by major remodeling of the 3D-architecture of the chromosome, both at the local and global levels (Fig.4.F).\n\nDiscussion\n\nIn this study, we demonstrated that in Streptomyces, compartmentalization of gene organization, transcription and architecture are correlated. We explore the transcriptional landscape of S. ambofaciens ATCC 23877 during metabolic differentiation: its large genome is highly dynamic, most of the genes (\\( \\approx 90\\% \\)) being significantly expressed in at least one condition. This situation is very similar to Bacillus subtilis, another Gram-positive bacteria from soil\\(^{38}\\). Interestingly, the SMBGCs (e.g. antibiotic clusters) are generally considered as 'cryptic' under most growth conditions\\(^{10,39}\\). We observed that they are poorly expressed in exponential phase. However their expression is characterized by up regulation after 48 h in the growth medium, compared to the rest of the chromosome including other genes putatively acquired by horizontal gene transfer (e.g. Gls). This result highlights that SMBGCs in S. ambofaciens have evolved regulatory mechanisms, such as the induction of cluster-situated transcriptional factor genes (Supplementary Fig.2) that efficiently and specifically regulate gene expression during metabolic differentiation, as reported in other Streptomyces species\\(^{4-7}\\).\n\nMoreover, we show that changes in gene expression dynamics are correlated with metabolic differentiation. Indeed, the terminal regions become transcriptionally active after 48 h of growth (see also references\\(^{10,36}\\)) (Fig.2). Interestingly, the ratio, antisense- over sense-transcription is high within the terminal compartments but decreases over the growth period, especially in the SMBGCs (Extended Data Fig.2.F). This suggests that this antisense-transcription may reflect regulatory\nprocesses that remain to be explored. This is particularly interesting since some NAPs suppress antisense-transcription in S. venezuelae^{40}.\n\nIn addition, 3C-seq analysis revealed that in exponential phase the central compartment forms a multiple domain structure, delineated by boundaries, whereas the terminal regions form two large compartments in which contacts are more variable at larger distances. As previously shown for bacteria with circular genomes^{20-23,26}, long and highly expressed genes (LHEGs encoding rRNA, ribosomal proteins, or respiratory chain components) are found at the boundaries in the *Streptomyces* chromosome (**Supplementary Table 5**, **Fig.4**). The positions of these boundaries are both conserved (under certain circumstances) and dynamic, since they change over the growth phase (**22**, this work). Notably, most of the boundaries observed at early growth times were correlated with the presence of persistent genes (**Fig.4C**). Within the central compartment, domains are a direct consequence of boundary formation. Additionally, no trivial role in gene expression or in chromosome conformation have been assigned to chromosome interacting domains (CIDs) in bacteria^{41}. Here we propose that boundaries are likely to act as transcriptional hubs for clustered and persistent genes^{42}, associated with very high levels of transcription in exponential phase. Moreover, in exponential phase, the first and last rDNA operons form the sharpest boundaries, recapitulating the borders that were arbitrarily used to define the central region beyond which genome synteny falls (**Figure 1**). We thus propose that they also constitute an evolutionary barrier that limits the occurrence of single recombination events within the central region. Interestingly, some boundaries in *Streptomyces* do not display high levels of gene expression (**Supplementary Table 5**). These are generally located within the terminal arms,\nsuggesting the existence of other mechanisms, yet to be discovered that impose chromosome constraints.\n\nFurthermore, we show for the first time that the central and terminal compartments present different organizational features, an observation independently demonstrated for the S. venezuelae chromosome (see accompanying paper, Szafran et al.). We favor the idea that the different organization of the terminal compartments could be a consequence of multiple factors: i) the lack of constraints imposed by active and sense-transcription; ii) the high level of anti-sense transcription; iii) the enrichment of horizontally acquired NAPs and other transcriptional regulators that, by increasing the dynamics of DNA intramolecular interactions, ensure appropriate SMBGC repression in exponential phase.\n\nInterestingly, it was shown in S. venezuelae that during sporulation the HupS NAP is involved in promoting optimal contacts along the whole chromosome, but seems to be particularly important for the organization of the terminal regions (see accompanying paper, Szafran et al.).\n\nDuring metabolic differentiation, the changes in transcriptional dynamics are accompanied by a huge remodeling of chromosome folding, switching from an ‘open’ to a ‘closed’ conformation, in which highly expressed SMBGC genes form new boundaries (Fig.4.E & F). This may illustrate a relocation of transcriptional hubs from clustered and persistent genes (in exponential phase) to SMBGCs at the onset of metabolic differentiation. Remarkably, the central region is no longer structured into multiple domains. The lack of boundaries in the central compartment after 48 h growth is correlated with a slight decrease in transcripts from genes that were present in boundaries in exponential phase. Indeed most of these genes remain expressed at high level (‘CAT-3’ or ‘CAT_4’) but below a threshold classically\nassociated with boundaries (a string of genes with above 20 000 normalized reads per kb, Supplementary Table 5). Moreover, we cannot exclude the possibility that some of these transcripts are stable RNAs produced in exponential rather than stationary phase^{43}. This loss of boundaries in the central compartment is reminiscent of the phenomena observed in eukaryotes during G1-to-mitosis transition^{44} and could reflect a more general phenomenon of genome compaction during the cell cycle.\n\nAt larger scales, there is an increase in the frequency of inter-arm DNA contacts. The most likely candidate to be involved in this reorganization is the Smc-ScpAB condensin complex, which is recruited to the origin region by ParB bound to parS^{45,46}. From the parS sites, Smc-ScpAB promotes inter-arm contacts by translocating to the terminal region of the chromosome, likely by loop extrusion^{20,21,24,27,47-52}. Streptomyces spp. encode both a ParABS system^{53-55} and a Smc-ScpAB complex^{56}. Interestingly, during sporulation Streptomyces chromosomes need to be compacted and segregated to ensure correct spore formation^{57 56}. Indeed, HiC studies during sporogenic development in S. venezuelae showed that inter-arm contacts are dependent on Smc-ScpAB (Szafran et al., see accompanying paper).\n\nThe global remodeling of the Streptomyces chromosome going from an 'open' to a 'closed' conformation seems to occur similarly during metabolic (this work) and sporogenic development (Szafran et al., see accompanying paper). Such a global rearrangement has not been previously described in wild-type bacteria. Interestingly, we observed a slight tilt in the secondary diagonal in contact analysis when it approaches to the terminal compartments (**Fig.4.E**, **Supplementary Fig.3.C**). This is consistent with a slow-down of Smc-ScpAB activity when interacting with the transcription machinery^{50,58}, in agreement with the fact that transcription in the\nterminal compartment is higher than in the central compartment during metabolic differentiation (Fig.4.E, Supplementary Fig.3.C).\n\nCollectively, these results indicate a link between evolutionary processes, including genome-compartmentalization and the molecular mechanisms (e.g. transcription, 3D-folding) that shape the structure and function of genes and genomes in Streptomyces. We therefore hypothesize that the efficiency of the regulatory processes controlling conditional expression of SMBGCs may be an emerging property of spatial compartmentalization. We believe that this study will open new insights into setting the rules governing chromosome spatial organization, expression and stability, and the optimal design of Streptomyces genomes for SMBCG expression.\n\nMethods\n\nStreptomyces strains and growth conditions\n\nS. ambofaciens ATCC 23877 was grown on solid soy flour-mannitol (SFM) medium59 at 28°C unless otherwise indicated. The strain was grown in the following media: MP5 medium (7 g/l yeast extract, 20.9 g/l MOPS, 5 g/l NaCl, 1 g/l NaNO₃, 36 ml/l glycerol – pH 7.5) 34, or YEME medium 10.3 % sucrose (3 g/l yeast extract, 5 g/l bactotryptone, 3 g/l malt extract, 10 g/l glucose, 103 g/l sucrose; pH 7.0-7.2 ; adapted from59). Twenty million spores of S. ambofaciens ATCC 23877 were inoculated in 100 ml of media before growth at 30°C in a shaking agitator (220 rpm, INFORS HT multitron standard).\n\nBioassays\nFor bioassays from liquid cultures, 50 μl of filtered supernatants were spotted on to agar medium using cylinder (diameter 0.5 cm) and allowed to dry until complete penetration into a plate containing 50 ml of DIFCO antibiotic medium 5 (DIFCO 227710). Thereafter 7 ml of SNA medium (2 g/l agar, 8 g/l nutrient broth MP Biomedicals Cat#1007917) containing Micrococcus luteus (final OD_{600nm} 0.04) were overlaid on the plate and incubated at 37°C. The growth inhibition area was measured 24 h later.\n\nGenomic island (GI) identification\n\nWe designed the Synteruptor program (http://bim.i2bc.paris-saclay.fr/synteruptor/)⁶⁰ to compare the sequences of chromosomes of species close enough to have synteny blocks, and to identify the genomic islands existing in each respective chromosome. We define synteny breaks as genomic regions between two consecutive synteny blocks when comparing two genomes, with the two blocks having the same direction. The genome of S. ambofaciens ATCC 23877 was compared to the chromosome of 7 closely related strains: S. ambofaciens DSM40697, S. coelicolor A3(2), S. lividans 1326, S. lividans TK24, S. mutabilis, Streptomyces sp. FXJ7.023, Streptomyces spp. M1013. To define a region harbouring GIs, we used a threshold of 15 CDS as the minimal number of CDSs within the synteny break, in at least one of the strains used for the pairwise comparison. Of note, a GI can therefore correspond to 15 CDS in one strain but less CDS in the other one. However, when the corresponding position within the S. ambofaciens genome contained less than 2 CDS or only tRNAs, compared to at least 15 CDSs in the chromosome of the compared species, it was considered as an insertion point (but not a GI) within S. ambofaciens. When the GIs were identified during several pairwise comparisons of S. ambofaciens ATCC 23877 and/or\noverlapping, they were fused and considered thereafter as a single GI. The complete list of GIs identified in the S. ambofaciens genome is presented in Supplementary Fig. 1 and Supplementary Table 2.\n\nSMBGCs identification\n\nWe used antiSMASH5.1.033 to identify putative SMBGCs. Thirty SMBGCs have thus been identified in the S. ambofaciens genome, the one encoding kinamycin biosynthesis being duplicated owing to its location within the TIRs. The definition of cluster boundaries has been manually refined on the basis of literature data for characterized SMBGCs (Supplementary Table 4). Of note, SMBGC genes are \\( \\approx 1.5 \\) times larger than the average, and only 13 of them (from 4 SMBGCs, namely ‘CL4_Indole’, ‘CL10_Furan’, ‘CL11_NRPS’, ‘CL20_Hopenoid’) belong to the core genome.\n\nNAPSFs, identification\n\nIn this study, we considered NAPs and chromosome structural factors sensu lato by including orthologues of classical NAPs and structural factors (HU, sIHf, Lsr2, Lrp/AsnC, SMC, Dps, CbpA, DnaA or IciA family proteins)61 and/or proteins associated with S. coelicolor chromatin62. This list is available in Supplementary Table 5.\n\nDefinition of indexes for genome conservation analyses\n\nWe selected 125 Streptomyces genomes from the NCBI database representative of the Streptomyces genus by keeping only complete genomes of distinct species. When genomes share an average nucleotide identity (ANlB) value greater than or equal to 96 %, they are considered as members of the same species31\n(Supplementary Table 1). We made one exception by keeping two strains of S. ambofaciens (ATCC 23877 and DSM 40697). Orthologous genes were identified by BLASTp best hits\\(^{63}\\) with at least 40 % of identity, 70 % coverage and an E-value lower than \\(1e^{-10}\\)\\(^{31}\\). The gene persistence index was calculated as \\(N_{orth}/N\\), where \\(N_{orth}\\) is the number of genomes carrying a given orthologue and \\(N\\) the number of genomes searched\\(^{28}\\). Pairwise comparisons are achieved using a sliding window and comparing a reference strain (species A) to another (species B). Here is considered a window containing 8 genes noted from 1 to 8 in the reference species. To calculate the GOC index (Gene Order Conservation), which is the number of contiguous syntenic orthologs between the two chromosomes over the number of orthologs between the two chromosomes, calculated in a sliding window, the pair of contiguous genes present in the window in the reference species are searched and counted as contiguous pairs of orthologues in the whole genome of species B related to the number of orthologs is defined by the window.\n\nTranscriptome analysis\n\nFor RNA-seq analysis performed in liquid cultures, \\( \\approx 2.10^7 \\) spores of S. ambofaciens ATCC 23877 were inoculated in 100 ml of liquid medium. Thereafter, 25 ml (for samples harvested after 24 h growth) or 10 ml of cultures (for other time points) were added to an equal volume of cold ethanol.\n\nCells were then harvested by centrifugation for 15 min at 4,000 \\(g\\) at 4\\(^\\circ\\)C, and stored at -20\\(^\\circ\\)C. Pellets were washed with 1 ml of DEPC water, centrifuged for 5 min at 16,000 \\(g\\) at 4\\(^\\circ\\)C and homogenized with glass beads (\\(\\leq 106\\) \\(\\mu\\)m; G4649, SIGMA) in 350 \\(\\mu\\)l of lysis buffer (RNeasy Plus Mini Kit, QIAGEN) supplemented with 10 \\(\\mu\\)l/ml \\(\\beta\\)-mercaptoethanol. Samples were processed 3 times for 45 sec each in FastPrep-24™ 5G instrument (MP Biomedicals) at setting 6 with 1 min cooling between the stages.\nAfter centrifugation for 10 min at 16,000 g at 4°C, total RNAs were isolated from the supernatants using an RNeasy Plus Mini Kit (QIAGEN) and gDNA Eliminator columns, following the manufacturer’s recommendations. To remove genomic DNA, RNA samples were incubated for 30 min at 37°C with 20 U of RNase-free DNase I (Roche) in a final reaction volume of 30 μl. RNAs were then cleaned up using the RNeasy Mini Kit (QIAGEN), following the manufacturer’s recommendations. The absence of DNA in the preparations was checked by PCR on an aliquot. RNA samples were quantified using Qubit™ RNA HS Assay kit (ThermoFischer Scientific), following manufacturer’s recommendations.\n\nTotal RNA quality was assessed in an Agilent Bioanalyzer 2100, using RNA 6000 pico kit (Agilent Technologies). 500 ng of total RNA were treated with DNAse (Baseline Zero DNAse, Epicentre) prior to ribosomal RNA depletion using the RiboZero bacteria magnetic Kit from Illumina according to the manufacturer’s recommendations. After the Ribo-Zero step, the samples were checked in the Agilent Bioanalyzer for complete rRNA depletion. Directional RNA-seq libraries were constructed using the Illumina ScriptSeq kit V2 (discontinued) for samples corresponding to C5 conditions and Illumina Stranded library preparation kit for all other samples, according to the manufacturer’s recommendations.\n\nLibraries were pooled in equimolar proportions and sequenced (Paired-end 2x43 bp) with an Illumina NextSeq500 instrument, using a NextSeq 500 High Output 75 cycles kit. Demultiplexing was done (bcl2fastq2 V2.2.18.12) and adapters (adapter_3p_R1: AGATCGGAAGAGCACACGTCTGAACT; adapter_3p_R2: AGATCGGAAGAGCGTCGTGTAGGGA) were trimmed with Cutadapt1.15, only reads longer than 10 bp were kept.\nSTAR software \\(^{64}\\) was used for mapping RNA-seq to the reference genome (genome-build-accession NCBI_Assembly: GCF_001267885.1) containing only one terminal inverted repeat (TIR). This avoids any biases with multiple mapping within the duplicated extremities of the genome (since the two TIR sequences are indistinguishable). We used the featureCounts program\\(^{65}\\) to quantify reads (in sense- and antisense- orientation) generated from RNA-sequencing technology in terms of “Gene” feature characteristics of S. ambofaciens ATCC 23877 most recent annotation (GCF_001267885.1_ASM126788v1_genomic.gff – released on the 06/15/2020).\n\nBioinformatic analysis of RNA-seq count data\n\nSARTools (Statistical Analysis of RNA-Seq data Tools) DESeq2-based R pipeline\\(^{66}\\) was used for systematic quality controls and the detection of differentially expressed genes. PCA and sample clustering used homoscedastic data transformed with Variance Stabilizing Transformation (VST). For the differential analysis, the Benjamini and Hochberg's method was used with a threshold of statistical significance adjusted to 0.05. The reference condition was C1 (medium “MP5_24h”). All parameters of SARTools that have default values were kept unchanged. Genes with null read counts in the 37 samples were not taken into account for the analysis with DESeq2. Genes corresponding to the second TIR (not used for the mapping) or the rRNAs (RiboZero treatment) were excluded from further analysis.\n\nSupplementary Table 5 presents the normalized counts per gene in each growth condition. To ensure that antisense-transcription did not affect the normalization of sense-transcription data, the latter were normalized as follows: the percentage of transcription in antisense orientation of each gene was determined with the raw data, then the normalized antisense-transcription was evaluated by applying this\npercentage to the normalized sense-transcript counts. To determine the category of gene expression the normalized counts obtained by the SARTools DESeq2-based pipeline were again normalized with respect to gene size (number of DESeq2 normalized reads/gene size x 1000 bp), and thereafter expressed in RPK (reads per kb). This allowed us to compare directly the relative levels of gene expression of individual genes. Data were analyzed with R software\\(^{67}\\) and the Integrative Genomics Viewer (IGV) tool was used to simultaneously visualize RNAseq data and genomic annotations\\(^{68}\\).\n\n**Multidimensional analyses of the data**\n\nWe used the FactoShiny R package\\(^{69}\\) to perform clustering, principal component analyses and correspondence analyses. This overlay factor map presented in **Extended Data Fig.2.C** results from the correspondence analysis performed using a contingency table indicating the number of genes in each category of expression level depending on the genome features of interest. Max', 'Mean' and 'Min' refer to the maximal, mean and minimal expression levels in all studied condition, from the lowest category ('0') to the highest ('4'). These categories were defined by considering the distribution parameters of the normalized number of reads (**Extended Fig.2.A.**). These gene expression categories as well as the number of genes switched ON ('Switch', meaning that the expression level switches from CAT_0 in at least one condition to CAT_3 or more in another condition), or presenting a very low ('AS < 0.05') or high ('AS > 0.5') level of antisense index were used to build the map, and projected on the plan. Here are some basic explanations of how to interpret the results of correspondence analysis. On **Extended Data Fig.2.C**, the squares correspond to the raw labels (genome features). The triangles\ncorrespond to the column labels (e.g. category of level of mean, maximal, minimal sense-transcription, antisense index < 0.05, antisense index > 0.5).\n\nChromosome conformation capture (3C)\n\nSpores of S. ambofaciens ATCC 23877 (\\( \\approx 4.10^7 \\)) were inoculated in 200 ml of MP5 or YEME liquid medium. In these media, bacterial growth was monitored by opacimetry. At the indicated time point, cells were harvested from 100 ml samples of culture, adjusted to an OD\\(_{600\\ nm}\\) of about 0.15 (with the appropriate fresh medium) and fixed by adding formaldehyde solution (3 % final concentration). Cells were then incubated under moderate agitation for 30 min at RT and 30 min more at 4°C.\n\nGlycine (250 mM final concentration) was added, and the bacteria incubated 30 min at 4°C with moderate agitation. Cells were then harvested by centrifugation for 10 min at 4,000 \\( g \\) at 4°C. The cells were gently suspended in 50 ml of PBS 1X and then again harvested by centrifugation for 10 min at 4,000 \\( g \\) at 4°C. This washing step was repeated once before suspending the cells in 1 ml of PBS before final harvesting by 10 min at 4,000 \\( g \\) at 4°C. The dry pellets were stored at -80°C until use.\n\nFrozen pellets of exponentially grown cells were thawed, suspended in 600 \\( \\mu \\)l Tris 10 mM EDTA 0.5 mM (TE) (pH 8) with 4 \\( \\mu \\)l of lysozyme (35 U/\\( \\mu \\)l; Tebu Bio) and incubated at RT for 20 min. For the samples collected after 48 h, the pellets were thawed, suspended in TE (pH 8) with 4 \\( \\mu \\)l of lysozyme (35 U/\\( \\mu \\)l; Tebu Bio) for 45 min and then homogenized with a Bioruptor sonication device (3 cycles of 30 seconds, with a pause of 30 second pause for each). Then, for both 24 h and 48 h samples, SDS was added to the mix (final concentration 0.5%) of cells and incubated for 10 minutes at RT. 500 \\( \\mu \\)l of lysed cells were transferred to a tube containing 4.5 ml of digestion mix (1X NEB 3 buffer, 1% triton X-100) and 100 \\( \\mu \\)l of the lysed cells were transferred to a tube containing 0.9 ml of digestion mix. 800 units of Sall were added\nto the 5 ml digestion mix. Both tubes were then incubated for 2 h at 37°C and 250 units of Sall were added to the 5 ml tube and further incubated, 2 h at 37°C. To stop the digestion reaction, 4 ml of the digestion mix were immediately centrifuged for 20 min at 20,000 \\( g \\), and pellets suspended in 4 ml of sterile water. The digested DNA (4 ml in total) was split into 4 aliquots and diluted in 8 ml ligation buffer (1X ligation buffer NEB 3 (without ATP), 1 mM ATP, 0.1 mg/ml BSA, 125 Units of T4 DNA ligase 5 U/\\(\\mu\\)l). Ligation was performed at 16°C for 4 h, followed by incubation overnight at 65°C with 100 \\(\\mu\\)l of proteinase K (20 mg/ml) and 100\\(\\mu\\)l EDTA 500 mM. DNA was then precipitated with an equal volume of 3 M Na-Acetate (pH 5.2) and two volumes of iso-propanol. After one hour at -80°C, DNA was pelleted and suspended in 500 \\(\\mu\\)l 1X TE buffer. The remaining 1ml digestion mix with or without Sall were directly incubated with 100 \\(\\mu\\)l of proteinase K (20 mg/ml) overnight at 65°C. Finally, all the tubes were transferred into 2 ml centrifuge tubes (8 tubes), extracted once with 400 \\(\\mu\\)l phenol-chloroform pH 8.0, precipitated, washed with 1 ml cold ethanol 70% and diluted in 30 \\(\\mu\\)l 1X TE buffer in the presence of RNase A (1 \\(\\mu\\)g/ml). Tubes containing the ligated DNA (3C libraries) were pooled. The efficiency of the 3C preparation was assayed by running aliquots of the 3C-librairies, the digested DNA or the non-digested DNA on 1% agarose gel. Finally the 3C libraries were quantified on the gel using QuantityOne software (BioRad).\n\nProcessing of libraries for Illumina sequencing\n\nApproximately 5 \\(\\mu\\)g of a 3C library was suspended in water (final volume 130 \\(\\mu\\)L) and sheared using a Covaris S220 instrument (Duty cycle 5, Intensity 5, cycles/burst 200, time 60 sec for 4 cycles). The DNA was purified using a Qiaquick® PCR purification kit, DNA ends were prepared for adapter ligation following standard protocols\\(^{70}\\). Custom-made adapters\\(^{21}\\) were ligated overnight at 4°C. Ligase was\ninactivated by incubating the tubes at 65°C for 20 min. To purify DNA fragments ranging in size from 400 to 900 pb, a PippinPrep apparatus (SAGE Science) was used. For each library, one PCR reaction of 12 cycles was performed using 2 to 3 \\( \\mu l \\) of 3C library, 0.2 \\( \\mu M \\) Illumina primers PE1.0 and PE2.0 and 1 unit of Taq Phusion [Finnzymes]. The PCR product was purified on Qiagen MinElute columns and dimers of primers were removed from the 3C library by using AMPure XP beads following the manufacturer’s protocol (Beckman Coulter). Finally, libraries were subjected to 75 bp paired-end sequencing in an Illumina sequencer (NextSeq500).\n\nProcessing of sequencing data\n\nPCR duplicates from each 3C library sequence dataset were discarded using the 6 Ns of custom-made adapters\\(^{21}\\). Reads were aligned independently using Bowtie 2 in very sensitive mode\\(^{71}\\). Only reads with mapping quality > 30 were kept to establish contact maps.\n\nGeneration of contact maps\n\nContact maps were built as described previously\\(^{72}\\). Briefly, each read was assigned to a restriction fragment. Non-informative events such as self-circularized restriction fragments, or uncut co-linear restriction fragments were discarded\\(^{73}\\). The chromosome of S. ambofaciens devoid of the TIRs was divided into 10 kbp bins and the frequencies of contacts between genomic loci for each bin were assigned. Contact frequencies were visualized as heatmaps. Raw contact maps were normalized with the sequential component normalization procedure (SCN\\(^{73}\\)). To facilitate visualization, contact matrices are visualized as log matrices. First we applied to the SCN matrices the log10 and then a Gaussian filter (H=1) to smooth the image. The contact score for a pair of bins that due to mapping was identified as an\noutlier (z-score>contact score) was replaced with the median value of the contact matrix.\n\nFrontier Index determination\n\nTo analyze the domain organization of S. ambofaciens, we used the frontier index (FI) method that quantifies the involvement of each bin in the frontier of any domain, i.e. at any scale – see technical details in37. Briefly, this method consists, first, in computing derivatives of the contact maps. To this end, we used normalized contact maps where the average contact frequency, \\( P(s) \\), was substracted to reduce noise coming from the natural overall decrease of contact frequencies as the genomic distance (\\( s \\)) between loci increase. Here, we also added pseudocounts (equal to \\( m/20 \\) where \\( m \\) is the maximal value of the contact frequencies) such that all values of the contact maps are strictly positive and we considered the logarithm of the resulting maps in order to mitigate the strongest variations close to the diagonal. We then considered separately the derivatives of these maps along the vertical and horizontal axes, whose large positive values (in the upper part of the maps) are respectively associated with upstream and downstream frontiers of domains, respectively. After setting negative values to zero (to reduce noise even more), for each bin the corresponding upstream and downstream FIs were defined as the sum over all other bins at a distance below 600 kb of the resulting signals. We then computed the profile of upstream and downstream FIs. We considered peaks that are located above the median of the peak values plus two times the standard deviation (estimated by the 1.48 times the median absolute deviation to mitigate the impact of outliers). These statistics were computed separately for the left terminal arm, the central region and the right terminal arm as these compartments have distinct\nstatistical 3C-seq features. Altogether, this led us to a list of significant upstream (orange) and downstream (green) peaks, respectively.\n\nA boundary was then allocated to any bin (as well as to pairs of consecutive bins to cope with uncertainty of peak positions) for which both the upstream and downstream peaks were significant. To analyze the genetic environment associated with a boundary, we considered the environment around the boundary identified by the frontier index (± 2 bins). Note that due to intrinsically noisy nature of 3C-seq data, we detected bins with only an upstream or a downstream significant peak (Supplementary Fig.3.D). These bins with an ‘orphan’ peak were not associated with a boundary, and hence, were removed from the analysis.\n\nThe dispersion index\n\nThe dispersion index of a signal reflects the range of variations relative to the mean value of the signal. Here, we compute it for the frequency of contacts. More precisely, it is defined as: \\( I(s) = \\text{var}(s)/P(s) \\), where \\( P(s) \\) and \\( \\text{var}(s) \\) are, respectively, the mean value and variance of the frequency of contacts between bins separated by the genomic distance. These quantities are then computed separately in each compartment of the genome. The larger the dispersion index is, the more variable are the contact frequencies within a compartment.\n\nStatistical procedure\n\nData were analyzed with R software\\(^{67}\\). For the RNA-seq analyses, three independent experiments (performed on different days) were carried out for each studied condition, except for C3, C9 and C10 that were performed in duplicate and C5 in quadruple. The statistical significance of RNA-seq analysis was assessed using the SARTools DESeq2-based pipeline\\(^{66}\\). For the 3C-seq analyses, two independent experiments (performed on different days) were carried out for each condition. To\nquantify gene regionalization, we defined the left and right terminal arms using as limits the first (genome position: 1,469,670-1,474,823 bp) and last (genome position: 5,802,471-5,807,629 bp) rDNA operons, respectively. The statistical significance was assessed by means of Fisher’s exact test for count data, which is appropriated to the analysis of contingency tables.\n\nData availability\n\nThe datasets generated during this study have been deposited in the NCBI Gene Expression Omnibus (GEO, https://www.ncbi.nlm.nih.gov/geo/) under the accession number GSE162865.\n\nList of abbreviations\n\n3C: Chromosome Conformation Capture\n“Actino. Sign.”: Actinobacterial Signature\nBGC: Biosynthetic Gene Cluster\nCDS: coding sequence\nCID: Chromosome Interacting Domain\nGI: Genomic island\nIGV: Integrative Genomics Viewer\nLHEG: long and highly expressed genes\nNAP: Nucleoid Associated Protein\nNAPSFs: Nucleoid Associated Proteins and structural factors\nPCA: Principal Component Analysis\nrDNA: ribosomal RNA encoding DNA\nRPK: Read per kb\nSARTools: Statistical Analysis of RNA-Seq data Tools\nSMBGC: Specialized Metabolite Biosynthetic Gene Cluster\nTIR: Terminal inverted repeat\n\nVST: Variance Stabilizing Transformation\n\nAcknowledgments\n\nWe acknowledge the High-throughput sequencing facility of I2BC for its sequencing and bioinformatics expertise. We thank Barry Holland and Christophe Possoz for careful reading of the manuscript and the members of F. B. and S. L. for fruitful discussions and advice.\nFigure legend\n\nFigure 1: The genetic compartmentalization of S. ambofaciens linear chromosome\n\nThe terminal inverted repeats (TIRs, 200 kb) and the origin of replication (oriC) are indicated in black. The distribution of gene presenting features of interest are represented in blue or red when enriched in the central region or within the extremities (defined by the first and last rDNA operons), respectively (see Supplementary Table 3 for a statistical analysis of the data). The dot and asterisk indicate the position of pSAM2 and of a complete prophage, respectively. The position of the SMBGC encoding the biosynthesis of all known antibacterial compounds of S. ambofaciens ATCC 23877 is also indicated. The level of synteny along the chromosome of S. ambofaciens ATCC 23877 is represented as a heat map of GOC (Gene Order Conservation) scores using a sliding window (8 CDSs with 1 CDS steps). Each line corresponds to the GOC profile of the reference against another species. The species are organized from the phylogenetically closest to the furthest compared to S. ambofaciens. The vertical black dotted line represents the location of the dnaA gene delineating the two replichores. “NA” (in yellow) indicates the absence of orthologs in the corresponding window. S. ambofaciens ATCC 23877 also harbors a circular pSAM1 plasmid (≈ 89 kbp).\n\nAbbreviations: ‘Actino. Sign. CDSs’ (coding sequences of the actinobacterial signature); BGC (biosynthetic gene cluster); ‘C.’ (congocidine BGC); ‘Chr.’ (whole chromosome); GIs (genes belonging to genomic islands); ‘K.’ (kinamycin BGC); ‘Persist>0.95 CDSs’ (coding sequences of S. ambofaciens ATCC 23877 presenting a gene persistence superior to 95 % in 124 other Streptomyces genomes); ‘Transl. CDSs’ (genes encoding functions involved in translation process and/or RNA stability);\nNAPSFs (nucleoid associated proteins and structural factors); SMBGCs (specialized metabolite BGCs); ‘Sp.’ (spiramycin BGC); ‘St.’ (stambomycin BGC); ‘rRNA’ (ribosomal RNA).\n\nFigure 2: Transcriptome dynamics depending on genome features and metabolic differentiation\n\nA. Transcriptome changes over growth. Heatmaps of the normalized number of reads per gene, ranked by their expression level at 24 h.\n\nB. Transcription along the chromosome over growth. The normalized counts (DESeq2 analysis) were mapped on S. ambofaciens chromosome. The two clusters to which the different conditions belong were obtained by hierarchical classification (Extended Data Fig.1C). Whereas the cluster 1 corresponds to exponential phases (no ATB production), the cluster 2 gathers conditions associated to the activation of SMBGC encoding at least two known antibacterial activities (Supplementary Fig.2). ‘C1’ to ‘C7’ refer to the name of the studied conditions: C1 to C5, cells grown in MP5 during 24 h, 30 h, 36 h, 48 h and 72 h, respectively; C6 and C7: cells grown in YEME during 24h and 48h, respectively (see Table 1, for details).\n\nC. Boxplot presenting the mean level of gene expression depending on features of interest. The distribution of the number of counts (normalized by DESeq and on gene size) as the mean of all studied conditions is presented depending on the genome features of interest (see the legend of Figure 1 for abbreviations). For clarity, outliers were excluded from this graphical representation (but were taken into account for the numerical exploitation of the data). The significant differences by Wilcoxon rank sum test with continuity\ncorrection compared to the chromosome ('Chr.') are indicated by asterisks (**, \\( p < 0.01 \\), ***, \\( p < 0.001 \\)). Other abbreviation: 'Func. RNA (-rRNA)' (Functional RNA excluding rRNA)\n\nFigure 3: Spatial organization of S. ambofaciens chromosome and transcriptome in absence of metabolic differentiation\n\n3C-seq and RNA-seq were performed on S. ambofaciens grown in exponential phase in YEME medium (24 h, C6 condition). The normalized contact map was obtained from asynchronous populations. The x and y axes represent the genomic coordinates of the reference genome. To simplify the analyses, TIRs were removed from the reference genome. In panel A, the colour scale reflects the frequency of the contacts between genome loci, from white (rare contacts) to dark purple (frequent contacts). In panel B, the frontier index analysis is able to detect, for a given genome 10 kb bin, the change in the contact bias with their neighbouring bins. Thus, a boundary is defined as any bin in which there is a change in the right bias of contacts towards the left bias (\\( \\pm 2 \\) bin, green and orange peaks, respectively). Red and black circles indicate the position of rDNAs and highly expressed genes (HEGs), respectively. In panel C, the normalized counts (DESeq2 analysis) measured in cells grown in the same condition were mapped on S. ambofaciens chromosome and binned in 10 kb. The panel D highlights genomic and transcriptional features of interest. The right and left compartment were defined owing the outer boundaries of the central compartment, which correspond to the first and last rDNA operon position. The 'synteny-break' right arm corresponds to the beginning of the spiramycin BGC. The replicate of this experiment is presented in the Supplementary Fig. 3.A.\nFigure 4: Chromosome remodeling during metabolic differentiation\n\nA. 3C-seq and RNA-seq performed after 24 h in MP5 growth medium (C1 condition). Same legend than Figure 3. The replicate of this experiment is presented in the Supplementary Fig. 3.B.\n\nB. Level of gene expression depending on gene location within boundaries or domains. The box-plot presents the sense-transcription (normalized number of read per Kb) depending on gene location in exponential phase either in MP5 (C1) or in YEME (C6), or after 48 h of growth in MP5 medium (C4). Boundaries in common between MP5 24 h and YEME 24 h conditions ('Common C1 & C6') were also analyzed separately. The significant differences by Wilcoxon rank sum test with continuity correction (boundaries versus domains) are indicated by asterisks (**, \\( p < 0.01 \\); ***, \\( p < 0.001 \\)).\n\nC. Level of gene persistence depending on gene location within boundaries or domains. The box-plot presents the persistence index depending on gene location in exponential phase (C1: MP5; C6: YEME) or after 48 h of growth in MP5 medium (C4). Boundaries in common between MP5 24 h and YEME 24 h conditions ('Common C1 & C6') were also analyzed separately. The significant differences by Wilcoxon rank sum test with continuity correction (boundaries versus domains) are indicated by asterisks (***, \\( p < 0.001 \\)).\n\nD. Dispersion index of the left, central and right compartments plotted as a function of genomic distance. The index of dispersion (\\( Var(s)/P(s) \\)) reflects the range of variations relative to the mean value as a function of the genome distance for the contact maps obtained for cells grown 24 h and 48 h in MP5 medium. Long-range DNA contacts within the terminal compartments (> 100 kbp) are more variable than within the central compartment.\nE. 3C-seq and RNA-seq performed after 48 h in MP5 growth medium (C4 condition). Same legend than Figure 3. The arrow indicates the position of the congocidine biosynthetic gene cluster (BGC). The replicate of this experiment is presented in the Supplementary Fig.3.C.\n\nF. Schematic representation of genome dynamics during metabolic differentiation. The Streptomyces linear chromosome is represented as dark gray (central compartment) and dark red sticks (left and right compartments). The origin of replication is indicated as a light yellow circle (oriC). In exponential phase, the chromosome of Streptomyces is organized into one transcriptionally active (light green) central compartment and two rather silent compartments (pink grey). The transcriptionally active compartment is enriched in core genes and is segmented in multiple domains, flanked by long and highly expressed conserved genes. The low frequency of contacts between the two arms is represented as an open conformation of the chromosome. After 48 h of growth, the transcription of the congocidine cluster is accompanied by a global remodeling of the chromosome. The increase in the frequency of contacts between the two chromosomal regions around the origin is represented as a closed conformation. Interestingly, a slight tilt on the secondary diagonal towards the ends of the chromosome shows an asymmetry between contacts within the terminal ends that was not schematized in the figure. In addition, since TIRs cannot be distinguished at the sequence level, they were neither considered in this analysis nor represented in this figure. However they may be located close to each other\\(^{74}\\), although this remains controversial\\(^{75}\\).\nExtended Data Figure 1: The metabolic differentiation of Streptomyces ambofaciens analyzed at the transcriptional level\n\nA. Growth curves of Streptomyces ambofaciens in MP5 and YEME liquid media. In these media, S. ambofaciens grows under a rather dispersed way, so that growth can be monitored by optical density (OD_{600nm}). We although refer to “pseudo-opacymetry” because of the presence of some clumps of bacteria. Values are means ± standard errors (error bars) from 3 independent experiments.\n\nB. Bioassays performed in conditions used in this study. Bioassays performed against Micrococcus luteus with the supernatants of S. ambofaciens ATCC 23877 grown in MP5 or YEME liquid media and harvested at different time points. Non-inoculated media were used as negative controls (“T-“). ‘C1’ to ‘C7’ refer to the name of the studied conditions (Table 1). The width of the plates is 12 cm. The presence of a halo indicates the presence of one or more antibacterial activities. The expression of the SMBGCs encoding known ATB is presented in Supplementary Fig.2.\n\nC. Multidimensional analyses of the studied conditions. Left panel - Axes 1 and 2 of the principal component analysis (PCA) of the whole data set (21 samples), with percentages of variance associated with each axis. The numbers indicate the condition (as indicated in Table 1) with a distinct letter (a, b, c, d) for each replica. Right panel- Ascending hierarchical classification (Euclidean distance, Ward criterion) and its inertia gain. The conditions form 2 clusters (1 and 2) and 5 subclusters which are boxed. The cluster 1 corresponds to the earliest growth time points (24 h, 30 h and 36 h) in which no ATB production was detected by bioassay. The cluster 2 corresponds to\nconditions associated to metabolic differentiation and the latest growth time points. Its sub-clusters separate owing the growth time and medium: 48 h in MP5 (subcluster 2.1), 72 h in MP5 (subcluster 2.2), 48 h in YEME (subcluster 2.3).\n\nD. MA-plot of the data for the comparison of transcriptomes over growth and over media. The MA-plot represents the log ratio of differential expression as a function of the mean intensity for each pairwise comparison. The differentially expressed features are highlighted in red, and the number of up- and down-regulated genes indicated on each graph. Triangles correspond to features having a too low/high \\( \\log_2(\\text{fold change}) \\) to be displayed on the plot.\n\nExtended Data Figure 2: The dynamic of Streptomyces ambofaciens transcriptome\n\nA. Distribution of the normalized read counts per gene and definition of gene expression level categories. The boxplot represents the distributions of the read counts per gene (normalized by DESeq and on gene size, RPK) individually for each tested condition and as the mean expression of each gene in all tested conditions. For clarity outliers were excluded from this graphical representation (but were taken into account for the numerical exploitation of the data). The genes were classified owing their expression level by considering the distribution parameters as indicated. These parameters were calculated both for each condition individually, and for the mean expression in all tested condition.\n\nB. Pattern of gene expression depending on genome features of interest. The genes were classified owing their mean (upper panel) or their\nminimal of maximal (lower panel) expression level in all studied conditions, as described in panel A. The table presents the statistical analysis of the data (Fisher’s exact test for count data).\n\nC. Multidimensional analysis (overlay factor map) of genomic and transcriptomic data. The squares and triangles correspond to genomic and transcriptomic features of interest, respectively (see abbreviations below). The closer the squares or triangles are to the origin of the graph, the closer they are likely to be to the mean data. Proximity between triangles or between squares indicates similarity. A small angle (*e.g.* less than 30°) connecting a triangle and a square to the origin indicate that they are probably associated. If they are located at the opposite, they are probably negatively associated. The proximity between the variables ‘SMBGCs’ and ‘Switch’ is due to the fact that a high proportion (19.3 %) of the SMBGC genes switched on at the transcriptional level in at least one studied condition (compared to 4.4 % at the level of the whole genome, odds ratios 5.2, *p*-value < \\(2.2 \\times 10^{-16}\\); 7.6 % of genes within GIs, odds ratios 2.9, *p*-value \\(2.2 \\times 10^{-9}\\), Fisher’s exact test for count data).\n\nGenomic feature abbreviations: ‘Actino. Sign. CDSs’ (coding sequences of the actinobacterial signature); ‘Chr.’ (whole chromosome); ‘Func. RNA (-rRNA)’ (Functional RNA excluded rRNA); GIs (genes belonging to genomic islands); ‘Persist\\(_{0.95}\\) CDSs’ (coding sequences of *S. ambofaciens* ATCC 23877 presenting a gene persistence superior to 95 % in 124 other *Streptomyces* genomes); ‘Transl. CDSs’ (genes encoding functions involved in translation process and/or RNA stability); NAPSFs (nucleoid associated proteins and structural factors); SMBGCs (specialized metabolite BGCs).\nExpression feature abbreviations: ‘AS < 0.05’ and ‘AS > 0.5’ correspond to very low (below 0.05) or very high (above 0.5) antisense-transcription indices. ‘Max’, ‘Mean’ and ‘Min’ refer to the maximal, mean and minimal expression levels in all studied condition, from the lowest category (‘0’) to the highest (‘4’). ‘Switch’ correspond to the expression level switch from CAT_0 in at least one condition to CAT_3 or more in another condition.\n\nD. Correlation between gene persistence and the transcription in sense orientation. The correlation between gene persistence and the mean number of counts (normalized by DESeq2 and on gene size, RPK) in sense- orientation for each gene (over all studied conditions) was analyzed by a Spearman’s rank correlation test (not sensitive to the log2 conversion of the data).\n\nE. Correlation between sense- and antisense-transcriptions. The correlation between the mean number of counts (normalized by DESeq2 and on gene size, RPK) in sense- and antisense- orientation for each gene (over all studied conditions) was analyzed by a Spearman’s rank correlation test (not sensitive to the log2 conversion of the data).\n\nF. Boxplot presenting the antisense index over growth in MP5 medium depending on feature of interest. The distribution of the antisense index defined as the number of counts in antisense over total counts (in sense- and antisense- orientation) is presented depending on the genome features of interest (see panel C for abbreviations). For clarity outliers were excluded from this graphical representation (but were taken into account for the numerical exploitation of the data). The significant differences by Wilcoxon rank sum test with continuity correction are indicated by asterisks (*, \\( p < 0.05 \\);\n**, \\( p < 0.01 \\); ***, \\( p < 0.001 \\)), in grey when comparing results after 24 h *versus* 48 h of growth for a given genome feature of interest, in violet and green when comparing a genome feature of interest to the whole set of chromosomal genes after 24 h *versus* 48 h of growth, respectively.\n\n**Extended Data Figure 3: Data exploration linking the chromosome architecture, transcription and gene persistence**\n\nA. **Contact probability, \\( P(s) \\), plotted as a function of genomic distance in exponential phase in YEME medium (C6 condition)**. The plot represent the intra-chromosomal contact probability, \\( P(s) \\), for pairs of loci separated by a genomic distance (in base pairs) on the chromosome, showing that the probability of contact extends up to approximately 1 Mb. The results of two replicates (#1 and #2) are presented.\n\nB. **Derivative of the contact matrix for exponentially growing WT cells**. The map shows for each genome locus the tendency of contact frequencies to go downwards or upwards. Boundaries are visualized as the black vertices of the squares along the diagonal. Regions with no upstream/downstream bias show no squares (*e.g.* terminal regions).\n\nC. **Boxplot presenting the antisense index over growth depending of genes depending on their architectural location**. The distribution of the antisense index defined as the number of counts in antisense over total counts (in sense- and antisense- orientation) is presented depending on the location of the genes (within boundaries or domains). For clarity, outliers were excluded from this graphical representation (but were taken into account for the numerical exploitation of the data). The significant differences by Wilcoxon rank sum test\nwith continuity correction (boundaries *versus* domains) are indicated by asterisks (***, \\( p < 0.001 \\)).\n\nD. **Contact probability, \\( P(s) \\), of the left, central and right compartments plotted as a function of genomic distance.** The plot represents the intra-chromosomal contact probability, \\( P(s) \\), for pairs of loci separated by a genomic distance (in base pairs) on the three compartments.\n\nE. **Dispersion index, \\( Var(s)/P(s) \\), of the left, central and right compartments plotted as a function of genomic distance in YEME after 24 h of growth (C6 condition).** The index of dispersion (\\( Var(s)/P(s) \\)) reflects the range of variations relative to the mean value as a function of the genome distance for the contact maps obtained for cells grown 24 h in YEME medium. Long-range DNA contacts within the terminal compartments (> 100 kbp) are more variable than within the central compartment.\n\n**Supplementary Figure 1: Size distribution of S. ambofaciens ATCC 23877 GIs**\nUsing a minimal threshold of 15 CDS within the synteny break in at least one of the compared genome, 50 GIs (composed of 2 to 158 CDSs) and 22 insertion points (\\( \\leq 1 \\) CDS within the synteny break) were identified in S. ambofaciens ATCC 23877 genome.\n\n**Supplementary Figure 2: Transcriptomes over growth of the four biosynthetic gene clusters encoding all known antibacterial activities of Streptomyces ambofaciens ATCC 23877**\nThe genes expressed at the highest level is boxed in red for the congocidine, spiramycin and kinamycin BGCs. They correspond to *cgc1* (SAM23877_RS39345,\nencoding a transcriptional regulator), *srmB* (SAM23877_RS26680, encoding the ABC-F type ribosomal protection protein SrmB) and *alpZ* (SAM23877_RS00890, encoding a transcriptional regulator) genes, respectively. The gene encoding SrmS (SAM23877_RS26595), the transcriptional regulator of the spiramycin BGC, is boxed in black. The dots are joined by a line for clarity (but the lines do neither report a real observation nor a model).\n\n**Supplementary Figure 3: 3C-contact-maps for *S. ambofaciens* grown in the studied conditions**\n\nA. Replicate of cells after 24 h in YEME growth medium, C6 condition\nB. Replicate of after 24 h in MP5 growth medium, C1 condition\nC. Replicate of after 48 h in MP5 growth medium, C4 condition. The violet and pink arrows indicate the location of boundaries formed at desferrioxamin and congocidine BGCs, respectively.\nD. Results of the frontier index analysis including peaks that do not form boundaries. This panel presents the frontier index analysis of the 3C-maps presented in Fig.3 and Fig.4, showing single peaks that where not considered as indicative of a boundary. At each locus, two indices are computed, reflecting the intensity of the loss of contact frequencies when going downwards (green peaks) or upwards (orange peaks), respectively, to the locus. A boundary is defined as any bin in which there is a change in the right bias of contacts towards the left bias (± 2 bin, green and orange peaks, respectively). The detection of bins with only an upstream or a downstream significant peak reflects the intrinsically noisy nature of 3C-seq data.\nSupplementary table 1: Collection of 125 Streptomyces genomes used in this study\n\nName: Species name\nGenome Assembly ID: Unique identifier used in the NCBI Genome Assembly database\nChromosome length (bp): Chromosome length expressed in bp\nPlasmid length (bp): Cumulative length of plasmids [Number of plasmids] expressed in bp\nCDSs nb: Number of CDSs in chromosome [CDSs in plasmids]\nTIR length (bp): Size of one copy of a TIR expressed in bp.\n\nSupplementary table 2: List of the GIs identified in S. ambofaciens ATCC 23877 genome\n\nSupplementary table 3: Gene distribution in the central region versus the extremities (defined by the first and last rDNA operons) of Streptomyces ambofaciens ATCC 23877 chromosome depending on features of interest\n\nSupplementary table 4: List of the SMBGCs identified in S. ambofaciens ATCC 23877 genome\nSupplementary table 5: Overall results from the comparative genomics, RNA-seq and 3C-seq analyses\n\nID: Gene identifier (NCBI annotation).\nSUPPORT: genetic support, either chromosome (CHR) or pSAM1 plasmid.\nTIR: ‘TIR’ if the gene is located within a TIR, ‘NA’ otherwise.\nSTART: start position of the gene on the genetic support.\nEND: end position of the gene on the genetic support.\nSTRAND: orientation of the gene on the genetic support.\nREPLICATION_ORIENTATION: orientation of the gene regarding the origin of replication, either on the “leading” or the “lagging” strand.\nGENE_SIZE: size of the gene (in bp).\nProtein_ID: Protein identifier (NCBI annotation).\nGO_ID: Gene product identifier (Uniprot or RNA Central, suitable for GO analysis).\nGene_Name: Gene name (from NCBI and manual annotation from SMBGCs encoding known antibiotics).\nUNIPROT_Gene_Name: Uniprot gene name, old locus tag.\nProduct (NCBI annotation): Product annotation from NCBI.\nProduct (Uniprot annotation): Product annotation from Uniprot.\nACTINO_SIGN: ‘ACTINO_SIGN’ if the gene encodes a protein of the actinobacterial signature, ‘NA’ otherwise.\nCORE: ‘CORE’ if the gene belongs to the core CDSs identified by comparing 125 Streptomyces genomes (see Methods section for details, as well as Supplementary Table 1).\nPERSIST95: ‘PERSIST95’ if the gene persistence is superior to 95 %, ‘NOT_PERSIST95’ otherwise.\nGI: annotation as to whether or not the gene belongs to a GI (see details about GI names on Supplementary Table 2).\n\nStrain-specific_CDSs: ‘UNIQ’ if the gene is only present in S. ambofaciens ATCC23877 (in a panel of 125 Streptomyces genomes described in Supplementary Table 1), ‘NOT_UNIQ’ otherwise.\n\nFunc_RNA: annotation as to whether or not the gene encodes a functional RNA (tRNA, tmRNA, SRP RNA, RNase P RNA) excluding rRNA.\n\nTransl._CDS: ‘translation’ if the CDS encodes a function related to translation and/or RNA stability, ‘NA’ otherwise\n\nNAPSF: ‘NAPSF’ if the gene encodes a nucleoid-associated protein or a chromosome structural protein and/or a protein experimentally found associated to Streptomyces chromatin (see Methods for details), ‘NA’ otherwise.\n\nSMBGC: annotation as to whether or not the gene belongs to a SMBGC (see details about SMBGC names on Supplementary Table 4).\n\npSAM2: ‘pSAM2’ if the gene belongs to pSAM2 integrative plasmid, ‘NA’ otherwise.\n\nPROPHAGE: ‘PROPHAGE’ if the gene belongs to the prophage integrated in S. ambofaciens ATCC23877 genome, ‘NA’ otherwise\n\nPERSIST_INDEX: Persistence index (\\( N_{orth}/N \\), where \\( N_{orth} \\) is the number of genomes carrying a given orthologue and \\( N \\) the number of genomes searched, 124 in our case). This persistence index was calculated only for CDSs (functional RNAs were not considered).\n\n‘SENSE’ columns: Number of normalized counts (DESeq2 normalization and normalized on gene size) per kb for each gene in the sense orientation, as the mean of the number of counts in all tested conditions (‘SENSE_Mean’) or of the replicates in each condition considered individually (‘SENSE_C1’ to ‘SENSE_C7’)\n‘ANTISENSE INDEX’ columns: Number of reads in the antisense orientation over the total (sense plus antisense) number of reads for each gene in all tested conditions ('ANTISENSE_INDEX_Mean') or in each condition considered individually ('ANTISENSE_INDEX_C1' to 'ANTISENSE_INDEX_C7')\n\n‘DIFF’ columns: annotation as to whether or not the gene is statistically differentially expressed compared to C1 condition, with an adjusted \\( p \\) value \\( < 0.05 \\) ('DIFF0.05'), 0.01 ('DIFF0.01') or 0.001 ('DIFF0.001').\n\n‘CAT’ columns: Gene expression level category in all tested conditions ('CAT_Mean'), in each condition considered individually ('CAT_C1' to 'CAT_C7'), maximal category in all tested conditions ('CAT_MAX') and minimal category in all tested conditions ('CAT_MIN').\n\nSWITCH: annotation as to whether or not the gene expression level switches from CAT_0 to a maximal CAT_3 ('SWITCH0->3') or CAT_4 ('SWITCH0->4') category, when considering all studied conditions.\n\n‘BORDER’ columns: annotation as to whether or not the gene belongs to a boundary observed on the map contact obtained in C1 ('C1_BORDER'), C4 ('C4_BORDER') and/or C6 condition ('C4_BORDER'). 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Genomics of Actinobacteria: tracing the evolutionary history of an ancient phylum. *Microbiol Mol Biol Rev* **71**, 495-548, doi:10.1128/MMBR.00005-07 (2007).\nFigures\n\n![Comparative genomic and functional annotation of Streptomyces ambofaciens ATCC 23877 chromosome](page_184_156_1207_627.png)\n\nFigure 1\n\nThe genetic compartmentalization of S. ambofaciens linear chromosome The terminal inverted repeats (TIRs, 200 kb) and the origin of replication (oriC) are indicated in black. The distribution of gene presenting features of interest are represented in blue or red when enriched in the central region or within the extremities (defined by the first and last rDNA operons), respectively (see Supplementary Table 3 for a statistical analysis of the data). The dot and asterisk indicate the position of pSAM2 and of a complete prophage, respectively. The position of the SMBGC encoding the biosynthesis of all known antibacterial compounds of S. ambofaciens ATCC 23877 is also indicated. The level of synteny along the chromosome of S. ambofaciens ATCC 23877 is represented as a heat map of GOC (Gene Order Conservation) scores using a sliding window (8 CDSs with 1 CDS steps). Each line corresponds to the GOC profile of the reference against another species. The species are organized from the phylogenetically closest to the furthest compared to S. ambofaciens. The vertical black dotted line represents the location of the dnaA gene delineating the two replichores. “NA” (in yellow) indicates the absence of orthologs in the corresponding window. S. ambofaciens ATCC 23877 also harbors a circular pSAM1 plasmid (= 89 kbp). Abbreviations: ‘Actino. Sign. CDSs’ (coding sequences of the actinobacterial signature); BGC (biosynthetic gene cluster); ‘C.’ (congocidine BGC); ‘Chr.’ (whole chromosome); GIs (genes belonging to genomic islands); ‘K.’ (kinamycin BGC); ‘Persist.->0.95 CDSs’ (coding sequences of S. ambofaciens ATCC 23877 presenting a gene persistence superior to 95 % in 124 other Streptomyces genomes); ‘Transl. CDSs’ (genes encoding functions involved in translation process and/or RNA stability); NAPSFs (nucleoid\nassociated proteins and structural factors); SMBGCs (specialized metabolite BGCs); ‘Sp.’ (spiramycin BGC); ‘St.’ (stambomycin BGC); ‘rRNA’ (ribosomal RNA).\n\n![Heatmap and transcriptional profiles of genes over growth phases](page_120_186_1347_579.png)\n\nFigure 2\n\nTranscriptome dynamics depending on genome features and metabolic differentiation A. Transcriptome changes over growth. Heatmaps of the normalized number of reads per gene, ranked by their expression level at 24 h. B. Transcription along the chromosome over growth. The normalized counts (DESeq2 analysis) were mapped on S. ambofaciens chromosome. The two clusters to which the different conditions belong were obtained by hierarchical classification (Extended Data Fig.1C). Whereas the cluster 1 corresponds to exponential phases (no ATB production), the cluster 2 gathers conditions associated to the activation of SMBGC encoding at least two known antibacterial activities (Supplementary Fig.2). ‘C1’ to ‘C7’ refer to the name of the studied conditions: C1 to C5, cells grown in\nMP5 during 24 h, 30 h, 36 h, 48 h and 72 h, respectively; C6 and C7: cells grown in YEME during 24h and 48h, respectively (see Table 1, for details). C. Boxplot presenting the mean level of gene expression depending on features of interest. The distribution of the number of counts (normalized by DESeq and on gene size) as the mean of all studied conditions is presented depending on the genome features of interest (see the legend of Figure 1 for abbreviations). For clarity, outliers were excluded from this graphical representation (but were taken into account for the numerical exploitation of the data). The significant differences by Wilcoxon rank sum test with continuity correction compared to the chromosome ('Chr.') are indicated by asterisks (**, p< 0.01, ***, p< 0.001). Other abbreviation: 'Func. RNA (-rRNA)' (Functional RNA excluding rRNA)\nFigure 3\n\nSpatial organization of S. ambofaciens chromosome and transcriptome in absence of metabolic differentiation 3C-seq and RNA-seq were performed on S. ambofaciens grown in exponential phase in YEME medium (24 h, C6 condition). The normalized contact map was obtained from asynchronous populations. The x and y axes represent the genomic coordinates of the reference genome. To simplify the analyses, TIRs were removed from the reference genome. In panel A, the colour scale reflects the\nfrequency of the contacts between genome loci, from white (rare contacts) to dark purple (frequent contacts). In panel B, the frontier index analysis is able to detect, for a given genome 10 kb bin, the change in the contact bias with their neighbouring bins. Thus, a boundary is defined as any bin in which there is a change in the right bias of contacts towards the left bias (± 2 bin, green and orange peaks, respectively). Red and black circles indicate the position of rDNAs and highly expressed genes (HEGs), respectively. In panel C, the normalized counts (DESeq2 analysis) measured in cells grown in the same condition were mapped on S. ambofaciens chromosome and binned in 10 kb. The panel D highlights genomic and transcriptional features of interest. The right and left compartment were defined owing the outer boundaries of the central compartment, which correspond to the first and last rDNA operon position. The ‘synteny-break’ right arm corresponds to the beginning of the spiramycin BGC. The replicate of this experiment is presented in the Supplementary Fig. 3.A.\nFigure 4\n\nChromosome remodeling during metabolic differentiation A. 3C-seq and RNA-seq performed after 24 h in MP5 growth medium (C1 condition). Same legend than Figure 3. The replicate of this experiment is presented in the Supplementary Fig. 3.B. B. Level of gene expression depending on gene location within boundaries or domains. The box-plot presents the sense-transcription (normalized number of read per Kb) depending on gene location in exponential phase either in MP5 (C1) or in YEME (C6), or after 48 h of\ngrowth in MP5 medium (C4). Boundaries in common between MP5 24 h and YEME 24 h conditions ('Common C1 & C6') were also analyzed separately. The significant differences by Wilcoxon rank sum test with continuity correction (boundaries versus domains) are indicated by asterisks (**, p < 0.01; ***, p < 0.001). C. Level of gene persistence depending on gene location within boundaries or domains. The box-plot presents the persistence index depending on gene location in exponential phase (C1: MP5; C6: YEME) or after 48 h of growth in MP5 medium (C4). Boundaries in common between MP5 24 h and YEME 24 h conditions ('Common C1 & C6') were also analyzed separately. The significant differences by Wilcoxon rank sum test with continuity correction (boundaries versus domains) are indicated by asterisks (***, p < 0.001). D. Dispersion index of the left, central and right compartments plotted as a function of genomic distance. The index of dispersion (Var(s)/P(s)) reflects the range of variations relative to the mean value as a function of the genome distance for the contact maps obtained for cells grown 24 h and 48 h in MP5 medium. Long-range DNA contacts within the terminal compartments (> 100 kbp) are more variable than within the central compartment. E. 3C-seq and RNA-seq performed after 48 h in MP5 growth medium (C4 condition). Same legend than Figure 3. The arrow indicates the position of the congocidine biosynthetic gene cluster (BGC). The replicate of this experiment is presented in the Supplementary Fig.3.C. F. Schematic representation of genome dynamics during metabolic differentiation. The Streptomyces linear chromosome is represented as dark gray (central compartment) and dark red sticks (left and right compartments). The origin of replication is indicated as a light yellow circle (oriC). In exponential phase, the chromosome of Streptomyces is organized into one transcriptionally active (light green) central compartment and two rather silent compartments (pink grey). The transcriptionally active compartment is enriched in core genes and is segmented in multiple domains, flanked by long and highly expressed conserved genes. The low frequency of contacts between the two arms is represented as an open conformation of the chromosome. After 48 h of growth, the transcription of the congocidine cluster is accompanied by a global remodeling of the chromosome. The increase in the frequency of contacts between the two chromosomal regions around the origin is represented as a closed conformation. Interestingly, a slight tilt on the secondary diagonal towards the ends of the chromosome shows an asymmetry between contacts within the terminal ends that was not schematized in the figure. In addition, since TIRs cannot be distinguished at the sequence level, they were neither considered in this analysis nor represented in this figure. However they may be located close to each other74, although this remains controversial75.\n\nSupplementary Files\n\nThis is a list of supplementary files associated with this preprint. Click to download.\n\n• SupplementaryFigure1bioRxiv.pdf\n• Supplementaryfigure2bioRxiv.pdf\n• SupplementaryFigure3bioRxiv.pdf\n• SupplementaryfilesLegendNEW.pdf\n• 0Table1bioRxiv.pdf\n• Supplementarytable1.pdf\n• Supplementarytable2.xlsx\n• Supplementarytable3NEW.pdf\n• Supplementarytable4.xlsx\n• SupplementaryTable5bioRxivNEW.xlsx\n• 5ExtendedDataFigure1bioRxiv.pdf\n• 6ExtendedDataFigure2bioRxivNEW.pdf\n• 7ExtendedDataFigure3bioRxiv.pdf"} {"paper_id": "prb9", "title": "Observation of charge-parity symmetry breaking in baryon decays", "text": "Observation of charge-parity symmetry breaking in baryon decays\n\nLHCb collaboration†\n\nAbstract\n\nThe Standard Model of particle physics, the theory of particles and interactions at the smallest scale, predicts that matter and antimatter interact differently due to violation of the combined symmetry of charge conjugation (\\( C \\)) and parity (\\( P \\)). Charge conjugation transforms particles into their antimatter particles, while the parity transformation inverts spatial coordinates. This prediction applies to both mesons, which consist of a quark and an antiquark, and baryons, which are composed of three quarks. However, despite having been discovered in various meson decays, \\( CP \\) violation has yet to be observed in baryons, the type of matter that makes up the observable Universe. This article reports a study of the decay of the beauty baryon \\( \\Lambda_b^0 \\) to the \\( p K^- \\pi^+ \\pi^- \\) final state and its \\( CP \\)-conjugated process, using data collected by the LHCb (Large Hadron Collider beauty) experiment at CERN. The results reveal significant asymmetries between the decay rates of the \\( \\Lambda_b^0 \\) baryon and its \\( CP \\)-conjugated antibaryon, marking the first observation of \\( CP \\) violation in baryon decays, thus demonstrating the different behaviour of baryons and antibaryons. In the Standard Model, \\( CP \\) violation arises from the Cabibbo–Kobayashi–Maskawa mechanism, while new forces or particles beyond the Standard Model could provide additional contributions. This discovery opens a new path to search for physics beyond the Standard Model.\n\nSubmitted to Nature\nIn 1928, Dirac proposed a theory of electron motion that predicted the existence of the positron, the antimatter counterpart to the electron [1]. Since then, all antimatter partners of known elementary particles, as well as those of composite particles made of quarks (referred to as hadrons), have been discovered in accelerator-based experiments or cosmic rays [2, 3]. Astronomical observations suggest that other stars and planets in the Universe are composed of the same type of matter that constitutes the solar system, namely protons and neutrons forming nuclei that are orbited by electrons, while the amount of antimatter particles is negligible [4].\n\nAccording to cosmological models, matter and antimatter were created in equal amounts at the Big Bang [4]. Then matter and antimatter mostly annihilated in pairs as the Universe cooled down, with a tiny fraction of matter remaining. The persistence of matter requires the violation of both \\( C \\) and \\( CP \\) symmetries in conjunction with other conditions, as proposed by Sakharov in 1967 [5]. Experimentally, it was established in 1957–1958 that the weak force breaks both \\( P \\) and \\( C \\) symmetries [6, 7]. The violation of the combined \\( CP \\) symmetry was first observed in strange-meson decays in 1964 [8]. This phenomenon was later also observed in beauty-meson decays in 2001 [9, 10] and in charm-meson decays in 2019 [11]. Here, strange, charm, and beauty refer to the flavours of constituent quarks.\n\nQuark dynamics are described by the Standard Model of particle physics, where \\( CP \\) violation arises from the Cabibbo–Kobayashi–Maskawa (CKM) mechanism [12]. The CKM mechanism employs a complex \\( 3 \\times 3 \\) matrix to describe how quarks of different generations mix under the weak interaction, which is mediated by the exchange of \\( W^\\pm \\) bosons. The structure of this mixing is ultimately linked to the Higgs mechanism, which gives mass to the quarks. The matrix contains a nonzero phase parameter, providing the only known source of \\( CP \\) symmetry breaking. In general, the CKM mechanism is very successful in describing experimental data for \\( CP \\) asymmetries and decay rates [13]. However, the amount of matter-antimatter asymmetry explained by the CKM mechanism is vastly smaller than what astronomical observations suggest, presenting a significant challenge to the Standard Model and hinting at the presence of additional sources of \\( CP \\) violation [14]. Ongoing exploration of \\( CP \\) violation may open new avenues for the discovery of physics beyond the Standard Model.\n\nThe lack of observed \\( CP \\) violation in baryons, the predominant form of matter in the visible Universe, remains a puzzle. Similar levels of \\( CP \\) violation in meson and baryon decays are expected due to identical quark-level transitions. Yet, \\( CP \\) violation has so far only been detected in mesons. This discrepancy is especially pronounced in beauty-baryon decays, where large \\( CP \\) asymmetries are anticipated, as seen in beauty mesons. For instance, the beauty-meson decay \\( B_s^0 \\to K^- \\pi^+ \\) shows a \\( (23.6 \\pm 1.7)\\% \\) \\( CP \\) asymmetry [15, 16], while the corresponding baryon decays \\( \\Lambda_b^0 \\to p h^- \\), where \\( h \\) denotes a \\( K \\) or \\( \\pi \\) meson, exhibit no such asymmetry with 0.7% precision [17]. Similarly, three-body beauty-meson decays such as \\( B^+ \\to \\pi^+ \\pi^- \\pi^+ \\) display \\( CP \\) asymmetries of up to 75% [18], while no significant \\( CP \\) violation has been observed in beauty-baryon decays [19, 20]. The \\( \\Lambda_b^0 \\to \\Lambda K^+ K^- \\) decay exhibits a hint of \\( CP \\) asymmetries below 20% with a significance of 3.1 standard deviations, requiring further confirmation [21]. No \\( CP \\) violation has been observed in strange and charm baryon decays, nor in unflavoured baryon decays.\n\nIn this work, \\( CP \\) violation in baryon decays is observed for the first time, specifically in the decay of the \\( \\Lambda_b^0 \\) baryon to a proton, a kaon, and a pair of oppositely charged pions, represented as \\( \\Lambda_b^0 \\to p K^- \\pi^+ \\pi^- \\). In the following, \\( CP \\)-conjugated particles or decays are\nFigure 1: Illustration of the \\( \\Lambda_b^0 \\) production in a \\( pp \\) collision and decay into the \\( p K^- \\pi^+ \\pi^- \\) final state. The two inset diagrams on the left illustrate the fundamental tree-type and loop-type quark-level processes that mediate the \\( \\Lambda_b^0 \\to p K^- \\pi^+ \\pi^- \\) decay, where the quarks eventually form the \\( p \\), \\( K^- \\), \\( \\pi^+ \\) and \\( \\pi^- \\) hadrons detected by the LHCb experiment.\n\nincluded if not otherwise specified. The constituents of the \\( \\Lambda_b^0 \\) baryon are similar to those of the proton (made of \\( uud \\) quarks), with one of the \\( u \\) quarks replaced by a \\( b \\) quark. The amount of \\( CP \\) violation in \\( \\Lambda_b^0 \\) decays is quantified by the asymmetry, \\( \\mathcal{A}_{CP} \\), defined as the relative difference between the rates, \\( \\Gamma \\), of the \\( \\Lambda_b^0 \\) decay and the \\( CP \\)-conjugated \\( \\overline{\\Lambda}_b^0 \\) decay,\n\n\\[\n\\mathcal{A}_{CP} \\equiv \\frac{\\Gamma(\\Lambda_b^0 \\to p K^- \\pi^+ \\pi^-) - \\Gamma(\\overline{\\Lambda}_b^0 \\to \\overline{p} K^+ \\pi^- \\pi^+)}{\\Gamma(\\Lambda_b^0 \\to p K^- \\pi^+ \\pi^-) + \\Gamma(\\overline{\\Lambda}_b^0 \\to \\overline{p} K^+ \\pi^- \\pi^+)} .\n\\]\n\nAccording to the Standard Model, this asymmetry arises from the interference between the “tree” and “loop” quark-level amplitudes [22] of the \\( \\Lambda_b^0 \\) baryon decay, mediated by the weak interaction, as illustrated by the Feynman diagrams in Fig. 1. These two complex amplitudes [23] are associated with phases (referred to as weak phases) derived from the products of CKM matrix elements \\( V_{ub} V_{us}^* \\) and \\( V_{tb} V_{ts}^* \\). The difference in weak phases between the two amplitudes plays a crucial role in \\( CP \\) violation. Additionally, strong interactions between quarks can introduce a possible strong-phase difference between the two amplitudes. The weak phases change sign from \\( \\Lambda_b^0 \\) to \\( \\overline{\\Lambda}_b^0 \\) decays, whereas the strong phases are the same. For sizeable \\( CP \\) violation to occur, the two amplitudes must have similar magnitudes and substantial differences in both weak and strong phases. However, while the weak phases are defined by the CKM mechanism, the strong phases and magnitudes of the amplitudes are process-dependent and are challenging to calculate due to low-energy strong-interaction effects [24]. Studies on multibody \\( B \\)-meson decays suggest that interactions among final-state particles in the decay can significantly enhance the strong phase [25–27]. The \\( \\Lambda_b^0 \\to p K^- \\pi^+ \\pi^- \\) decay can proceed through a rich spectrum of hadrons, such as excited nucleons decaying to the \\( p \\pi^+ \\pi^- \\) final state, which may create the necessary conditions for the manifestation of significant \\( CP \\) asymmetries [28]. Moreover, the size of the \\( CP \\) asymmetry may vary across the phase space [29], defined in terms of two-body and three-body masses of the final states, allowing enlarged effects to be\nFigure 2: Mass distributions together with the fit projections. Displayed are the mass distributions for the signal channel: (a) \\( \\Lambda_b^0 \\to p K^- \\pi^+ \\pi^- \\) and (b) \\( \\overline{\\Lambda}_b^0 \\to \\overline{p} K^+ \\pi^- \\pi^+ \\). The different components utilised in the fit are described in detail in the Methods section and listed in the legend. The area under a curve represents the yield of the corresponding component.\n\nobserved by selecting regions with appropriate contributions from hadronic resonances.\n\nThe \\( CP \\) asymmetry in the \\( \\Lambda_b^0 \\) decay, as defined in Eq. (1), is inferred through the yield asymmetry between the numbers (\\( N \\)) of observed \\( \\Lambda_b^0 \\to p K^- \\pi^+ \\pi^- \\) and \\( \\overline{\\Lambda}_b^0 \\to \\overline{p} K^+ \\pi^- \\pi^+ \\) decays, defined as\n\n\\[\n\\mathcal{A}_N \\equiv \\frac{N(\\Lambda_b^0 \\to p K^- \\pi^+ \\pi^-) - N(\\overline{\\Lambda}_b^0 \\to \\overline{p} K^+ \\pi^- \\pi^+)}{N(\\Lambda_b^0 \\to p K^- \\pi^+ \\pi^-) + N(\\overline{\\Lambda}_b^0 \\to \\overline{p} K^+ \\pi^- \\pi^+)}.\n\\]\n\nAs depicted in Fig. 1, the \\( \\Lambda_b^0 \\) and \\( \\overline{\\Lambda}_b^0 \\) baryons in this study are produced in high-energy proton-proton (\\( pp \\)) collisions provided by the Large Hadron Collider at CERN from 2011 to 2018. The total integrated luminosity of the data is about 9\\( \\text{fb}^{-1} \\). Beauty baryons from \\( pp \\) collisions then decay into final-state particles, which are detected by the LHCb detector. The LHCb experiment was designed to study \\( CP \\) violation in particles containing \\( b \\) or \\( c \\) quarks. Detailed descriptions of the LHCb detector and its performance can be found in Refs. [30, 31].\n\nAn event selection is performed to reduce background, primarily arising from random combinations of final-state particles. Due to its relatively long lifetime, the \\( \\Lambda_b^0 \\) baryon travels a measurable distance before decaying, resulting in a decay vertex displaced from the \\( pp \\) collision point. The final-state particles of the signal decay have relatively high transverse momentum, *i.e.* the component of the momentum transverse to the beam direction, reflecting the large \\( \\Lambda_b^0 \\) mass. These characteristics are exploited to suppress background due to random combinations of \\( p, K^-, \\pi^+ \\) and \\( \\pi^- \\) particles through a machine-learning technique implemented with a boosted decision tree classifier [32, 33]. Background involving misidentified particles, such as the \\( \\Lambda_b^0 \\to p \\pi^- \\pi^+ \\pi^- \\) decay where a \\( \\pi^- \\) candidate is reconstructed as a \\( K^- \\), is mitigated using particle identification (PID) information.\n\nThe mass distributions of \\( \\Lambda_b^0 \\) and \\( \\overline{\\Lambda}_b^0 \\) candidates, \\( m(p K^- \\pi^+ \\pi^-) \\) and \\( m(\\overline{p} K^+ \\pi^- \\pi^+) \\), are displayed in Fig. 2, showing prominent peaks corresponding to the \\( \\Lambda_b^0 \\) and \\( \\overline{\\Lambda}_b^0 \\) signal\ndecays, along with remaining background components including the \\( \\Xi_b^0 \\rightarrow p K^- \\pi^+ \\pi^- \\) decay, random combinations of final-state particles, partially reconstructed \\( \\Lambda_b^0 \\) decays and those involving misidentified particles. Extended unbinned maximum-likelihood fits to the mass spectra are performed to extract the signal yields. In these fits, all identified contributions are modelled using empirical functions or distributions based on simulations, with the distribution for each component assumed to be identical for baryon and antibaryon decays. The yields are determined to be \\( N(\\Lambda_b^0 \\rightarrow p K^- \\pi^+ \\pi^-) = (4.184 \\pm 0.025) \\times 10^4 \\) and \\( N(\\overline{\\Lambda}_b^0 \\rightarrow \\overline{p} K^+ \\pi^- \\pi^+) = (3.885 \\pm 0.023) \\times 10^4 \\), giving a yield asymmetry of \\( \\mathcal{A}_N = (3.71 \\pm 0.39)\\% \\).\n\nThe measured yield asymmetry \\( \\mathcal{A}_N \\) differs from the \\( CP \\) asymmetry \\( \\mathcal{A}_{CP} \\) due to several biasing effects. First, due to the nonzero net baryon quantum number in \\( pp \\) collisions, the production cross-section of the \\( \\Lambda_b^0 \\) baryon is slightly higher than that of the \\( \\overline{\\Lambda}_b^0 \\) baryon [34], resulting in a production asymmetry. Second, since particles and antiparticles have different behaviours when they interact with the detector material, which is made of matter rather than antimatter, a small detection asymmetry arises. These effects, collectively referred to as nuisance asymmetries, are measured to be around 1%, depending on the momenta of the beauty baryon or the final-state particles, and must be subtracted from \\( \\mathcal{A}_N \\).\n\nThe decay \\( \\Lambda_b^0 \\rightarrow \\Lambda_c^+ \\pi^- \\) with \\( \\Lambda_c^+ \\rightarrow p K^- \\pi^+ \\) is used as the control channel to subtract the nuisance asymmetries. It proceeds through a single dominant quark-level process, therefore \\( CP \\) violation is not expected. Consequently, the yield asymmetry in the control channel is primarily due to the nuisance asymmetries, measured as \\( \\mathcal{A}_N = (1.25 \\pm 0.23)\\% \\). Mass distributions for the control channel are shown in Extended Data Fig. 1. The difference between nuisance asymmetries in the signal channel and the control channel is measured to be 0.01%, demonstrating an effective cancellation between the two decays. Details on the measurement of nuisance asymmetries are given in the Methods section.\n\nThe \\( CP \\) asymmetry of the signal decay is obtained from its yield asymmetry by subtracting the control-channel yield asymmetry and the difference in nuisance asymmetries, leading to the measurement\n\n\\[\n\\mathcal{A}_{CP} = (2.45 \\pm 0.46 \\pm 0.10)\\% .\n\\]\n\nThe first uncertainty arises from the sample sizes of both the signal and control channels, while the second is due to nuisance asymmetries and the choice of \\( \\Lambda_b^0 \\) and \\( \\overline{\\Lambda}_b^0 \\) mass-fit model. This \\( CP \\) asymmetry differs from zero by 5.2 standard deviations, marking the observation of \\( CP \\) violation. The robustness of the measurement is confirmed across different data collection periods, LHCb magnetic-field configurations affecting the trajectory of charged particles, varied event-selection scenarios, and different momentum intervals for beauty baryons, among other factors. The results are consistent across the different subsamples and align with previous measurements that used a fraction of the data and employed different event selections [35].\n\nThe \\( \\Lambda_b^0 \\rightarrow p K^- \\pi^+ \\pi^- \\) decay occurs primarily via hadronic resonances that decay into two or three final-state particles. Identified resonances include excited baryons in the \\( p K^- \\), \\( p \\pi^+ \\), \\( p \\pi^- \\), or \\( p \\pi^+ \\pi^- \\) mass spectra, denoted as \\( R(pK^-) \\), \\( R(p\\pi^+) \\), \\( R(p\\pi^-) \\), and \\( R(p\\pi^+ \\pi^-) \\), respectively. Additionally, excited strange mesons, \\( R(K^- \\pi^+ \\pi^-) \\), \\( R(K^- \\pi^+) \\), and light unflavoured mesons, \\( R(\\pi^+ \\pi^-) \\), are also observed. The production mechanisms for these resonances are complicated, and the associated strong phases and relative strengths of tree and loop amplitudes are expected to vary among resonances. This variability leads\nTable 1: Measurements of \\( CP \\) asymmetries in four phase-space regions. The regions are selected using two-body or three-body masses.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
Decay topologyMass region (\\( \\mathrm{GeV}/c^2 \\))\\( \\mathcal{A}_{CP} \\)
\\( \\Lambda_b^0 \\to R(pK^-)R(\\pi^+\\pi^-) \\)\\( m_{pK^-} < 2.2 \\)
\\( m_{\\pi^+\\pi^-} < 1.1 \\)
(5.3 ± 1.3 ± 0.2)%
\\( m_{\\pi^+\\pi^-} < 1.7 \\)
\\( \\Lambda_b^0 \\to R(p\\pi^-)R(K^-\\pi^+) \\)0.8 < \\( m_{\\pi^+K^-} \\) < 1.0
or \\( 1.1 < m_{\\pi^+K^-} < 1.6 \\)
(2.7 ± 0.8 ± 0.1)%
\\( \\Lambda_b^0 \\to R(p\\pi^+\\pi^-)K^- \\)\\( m_{p\\pi^+\\pi^-} < 2.7 \\)(5.4 ± 0.9 ± 0.1)%
\\( \\Lambda_b^0 \\to R(K^-\\pi^+\\pi^-)p \\)\\( m_{K^-\\pi^+\\pi^-} < 2.0 \\)(2.0 ± 1.2 ± 0.3)%
\n\nto differences in the \\( CP \\) asymmetry across the final-state phase space of the beauty-baryon decay. The global \\( CP \\) asymmetry reported above represents a measurement that is averaged over the entire phase space. To investigate the resonance contributions to the global \\( CP \\) violation, the analysis is performed across regions of the \\( \\Lambda_b^0 \\) decay phase space, chosen upon their resonance compositions. Among the different possible resonance topologies, four are found to make significant contributions to the \\( \\Lambda_b^0 \\) decay and have been selected for further measurements. Data corresponding to these decays are chosen according to relevant two-body or three-body masses. The local \\( CP \\) asymmetries between \\( \\Lambda_b^0 \\) and \\( \\bar{\\Lambda}_b^0 \\) decays in these regions are obtained in a way similar to the global \\( \\mathcal{A}_{CP} \\) measurement.\n\nA summary of the local phase-space decay topologies, selections and \\( CP \\) asymmetries is provided in Table 1. The \\( CP \\) asymmetry is found to be most significant for the \\( \\Lambda_b^0 \\to R(p\\pi^+\\pi^-)K^- \\) decay, with \\( \\mathcal{A}_{CP} = (5.4 \\pm 0.9 \\pm 0.1)\\% \\), differing from zero by 6.0 standard deviations. The mass distributions for the \\( p\\pi^+\\pi^- \\) system and the corresponding \\( \\Lambda_b^0 \\) and \\( \\bar{\\Lambda}_b^0 \\) baryons are shown in Fig. 3 for \\( \\Lambda_b^0 \\to R(p\\pi^+\\pi^-)K^- \\) decays. Mass distributions for other two-body or three-body systems, along with their corresponding \\( \\Lambda_b^0 \\) and \\( \\bar{\\Lambda}_b^0 \\) baryons, are shown in Extended Data Figs. 2 and 3. The second most significant \\( CP \\) asymmetry is observed for the \\( \\Lambda_b^0 \\to R(pK^-)R(\\pi^+\\pi^-) \\) decay, with \\( \\mathcal{A}_{CP} = (5.3 \\pm 1.3 \\pm 0.2)\\% \\). The \\( CP \\) asymmetries for the other two decay topologies are not significant.\n\nThe \\( CP \\) asymmetry depends on decay topologies, suggesting the relative magnitudes and/or strong phases of the tree and loop amplitudes vary across the phase space. In general, the complicated hadronic effects pose significant challenges for predicting \\( CP \\) asymmetries within the Standard Model. Various approaches have been proposed, such as employing a model-independent investigation of angular distributions [36] or utilising scattering data to extract the hadronic amplitude [28]. Applying this method using \\( \\pi^+n \\to p\\pi^+\\pi^- \\) scattering data [37], an estimate of the \\( CP \\) asymmetry in \\( \\Lambda_b^0 \\to R(p\\pi^+\\pi^-)K^- \\) decays aligns with the measurement in this work.\n\nEach decay topology receives multiple resonant or nonresonant contributions that often overlap and interfere with each other. The intrinsic \\( CP \\) asymmetry may vary in magnitude and could even change sign between different contributions. As a result, the \\( CP \\)\nFigure 3: Mass distributions in the \\( R(p\\pi^+\\pi^-) \\) resonance phase space. (a) Distribution of the \\( p\\pi^+\\pi^- \\) mass including both \\( \\Lambda_b^0 \\) and \\( \\overline{\\Lambda}_b^0 \\) candidates. The low-mass structure corresponds to excited nucleon resonances decaying to the \\( p\\pi^+\\pi^- \\) final state, while the broad structure at higher masses arises from other decay processes of the \\( \\Lambda_b^0 \\) baryon. Mass distributions of candidates within the region delimited by the red box in (a) are shown for (b) \\( \\Lambda_b^0 \\to pK^-\\pi^+\\pi^- \\) and (c) \\( \\overline{\\Lambda}_b^0 \\to \\overline{p}K^+\\pi^-\\pi^+ \\) decays, together with the fit projections and individual components.\n\nasymmetries reported here represent values averaged over phase space. An investigation of the amplitude structure of this decay is left for future studies.\n\nIn summary, this article presents the first observation of \\( CP \\) violation in baryon decays, based on extensive samples of \\( \\Lambda_b^0 \\to pK^-\\pi^+\\pi^- \\) and \\( \\overline{\\Lambda}_b^0 \\to \\overline{p}K^+\\pi^-\\pi^+ \\) decays collected with the LHCb detector. The measured \\( CP \\) asymmetry, \\( \\mathcal{A}_{CP} = (2.45 \\pm 0.46 \\pm 0.10)\\% \\), with a significance of 5.2 standard deviations, reveals a difference in behaviour between baryonic matter and antimatter. An investigation of various phase-space regions has been conducted to better understand the source of the observed \\( CP \\) violation. In particular, the \\( CP \\) asymmetry is found to be most pronounced in the region dominated by the resonant decays \\( \\Lambda_b^0 \\to R(p\\pi^+\\pi^-)K^- \\), measured to be \\( \\mathcal{A}_{CP} = (5.4 \\pm 0.9 \\pm 0.1)\\% \\), which differs from zero by 6.0 standard deviations. This discovery strongly suggests that specific intermediate resonances play a key role in generating \\( CP \\) violation in \\( \\Lambda_b^0 \\) decays. Furthermore, the generally small \\( CP \\) asymmetries in beauty-baryon decays imply that the dynamics in baryon decays are more complicated than in meson decays. For instance, the \\( CP \\) asymmetries for various angular-momentum amplitudes of the same resonance may cancel [38]. This discovery of baryon decay asymmetry paves the way for further theoretical and experimental investigations into the nature of \\( CP \\) violation in baryon decays, potentially offering new constraints on scenarios beyond the Standard Model.\nMethods\n\nDerivation of the \\( CP \\) asymmetry The \\( CP \\) asymmetry arises from an interference between the tree and loop processes. The total amplitude of the \\( \\Lambda_b^0 \\) decay is the sum of the tree and loop amplitudes,\n\n\\[\nA(\\Lambda_b^0) = |A_T| e^{+i\\phi_T} e^{i\\delta_T} + |A_L| e^{+i\\phi_L} e^{i\\delta_L},\n\\]\n\nwhere \\( \\phi_T \\) (\\( \\delta_T \\)) and \\( \\phi_L \\) (\\( \\delta_L \\)) are the weak (strong) phases of the tree and loop processes, respectively, with \\( |A_T| \\) and \\( |A_L| \\) being their magnitudes. Similarly, the total amplitude for the \\( \\overline{\\Lambda}_b^0 \\) decay is given by\n\n\\[\nA(\\overline{\\Lambda}_b^0) = |A_T| e^{-i\\phi_T} e^{i\\delta_T} + |A_L| e^{-i\\phi_L} e^{i\\delta_L}.\n\\]\n\nSubstituting into Eq. 1, where the decay rate \\( \\Gamma \\) is proportional to the squared amplitude, the \\( CP \\) asymmetry is obtained as\n\n\\[\n\\mathcal{A}_{CP} = \\frac{|A(\\Lambda_b^0)|^2 - |A(\\overline{\\Lambda}_b^0)|^2}{|A(\\Lambda_b^0)|^2 + |A(\\overline{\\Lambda}_b^0)|^2} = \\frac{2 \\sin \\Delta \\delta \\sin \\Delta \\phi}{|A_T/A_L| + |A_L/A_T| + 2 \\cos \\Delta \\delta \\cos \\Delta \\phi}.\n\\]\n\nA sizable \\( \\mathcal{A}_{CP} \\) requires \\( A_T \\) and \\( A_L \\) to have comparable magnitudes, along with significant differences in both the weak (\\( \\Delta \\phi \\)) and strong (\\( \\Delta \\delta \\)) phases.\n\nLHCb detector The Large Hadron Collider (LHC) at the European Organisation for Nuclear Research (CERN) near Geneva is the world’s largest particle accelerator. Constructed within a 27 km underground circular tunnel, the LHC accelerates two counter-rotating proton beams to speeds near that of light, colliding them at designated interaction points to produce high-energy particles. The LHCb detector [30,31] is located at one of these interaction points to capture and analyse particles produced in the \\( pp \\) collisions. Optimised to record decays of hadrons containing \\( b \\) quarks, the LHCb detector is a forward spectrometer enabling a broad physics programme including high-precision measurements of \\( CP \\) violation and searches for rare decay processes. It consists of a tracking system to reconstruct the trajectories of charged particles and measure their momenta with a relative uncertainty that varies from 0.5% at low momentum to 1.0% at 200 GeV/\\( c \\). The tracking system also measures the particle impact parameter relative to the \\( pp \\) interaction point with a resolution of \\( (15 \\pm 29/p_T) \\) \\( \\mu \\)m, where \\( p_T \\) is the transverse momentum of the particle in GeV/\\( c \\). These capabilities enable precise vertex reconstruction and kinematic analysis, essential for distinguishing signal events from the background. Alongside the tracking system, the LHCb detector includes two ring-imaging Cherenkov detectors, a calorimeter system, and a muon-detection system to provide PID information for final-state particles. Collectively, these components enable the LHCb experiment to rigorously test the Standard Model and search for new physics through precise measurements.\n\nData and simulation samples The measurement is performed using data collected by the LHCb experiment in \\( pp \\) collisions at centre-of-mass energies of 7 TeV (2011) and 8 TeV (2012), referred to hereafter as the Run 1 period, and 13 TeV (2015–2018), referred to as the Run 2 period. Simulated \\( \\Lambda_b^0 \\) decays are used to perform event selections and study the mass distributions. In the simulation, \\( pp \\) collisions are generated using PYTHIA [39]\nwith a specific LHCb configuration [40]. Decays of unstable particles are described by EvtGen [41], in which final-state radiation is generated using PHOTOS [42]. The interaction of the generated particles with the detector, and its response, are implemented using the GEANT4 toolkit [43] as described in Ref. [44].\n\nEvent selection The online event selection for \\( b \\)-hadron decays is performed by a trigger system designed to retain beauty and charm hadrons of interest while rejecting light-hadron background [45]. The system consists of two parts: a hardware-based first-level trigger, which selects hadrons, photons, and electrons with high-energy deposits in the calorimeter, as well as muons with high \\( p_T \\); and a software-based high-level trigger, which reconstructs and selects decays of interest. The software trigger requires a two-, three- or four-track secondary vertex with a significant displacement from any \\( pp \\) collision point, known as primary vertex. At least one charged particle must have a large \\( p_T \\) and be inconsistent with originating from a primary vertex. A multivariate algorithm [46, 47] is used for the identification of secondary vertices consistent with the decay of a \\( b \\) hadron.\n\nIn the analysis, the \\( \\Lambda_b^0 \\) baryon is reconstructed by combining four tracks identified as proton, kaon and pions. Additional selection criteria are applied to suppress background while retaining most of the signal decays. The same selection requirements are applied to the \\( \\Lambda_b^0 \\to p K^- \\pi^+ \\pi^- \\) and \\( \\bar{\\Lambda}_b^0 \\to \\overline{p} K^+ \\pi^- \\pi^+ \\) decays. To reduce background from tracks originating at a primary vertex, a large impact parameter with respect to any primary vertex is required for each final-state track. The four tracks must form a common vertex with a significant displacement from any primary vertex. Furthermore, the \\( \\Lambda_b^0 \\) momentum, calculated from the final-state particles, is required to point back to the associated primary vertex.\n\nA few categories of background are further suppressed to obtain a high-purity \\( \\Lambda_b^0 \\) sample. Fake \\( \\Lambda_b^0 \\) candidates, formed by random combinations of tracks, identified as \\( p, K^-, \\pi^+, \\) or \\( \\pi^- \\), are suppressed using a boosted-decision-tree multivariate classifier [46]. The classifier is trained with a simulated sample for the signal and data from the high-mass sideband for the background, and utilises information related to the large \\( \\Lambda_b^0 \\) mass and long lifetime, as well as the decay topology. The large \\( \\Lambda_b^0 \\) mass results in relatively high \\( p_T \\) for final-state particles compared to those originating directly from \\( pp \\) collisions. The long \\( \\Lambda_b^0 \\) lifetime causes a displacement of the decay vertex from the primary vertex, leading to final-state particles with relatively large impact parameters. A second type of background arises from the decays proceeding through intermediate charmed resonances. The final states of these charmed decays are similar to signal decays in that they form well-reconstructed displaced vertices and are difficult to completely remove through PID, kinematic, or topological selections. Nevertheless, charmed resonances manifest as distinct peaks in the mass spectra of their decay products. For example, the \\( \\Lambda_b^0 \\to p D^0 \\pi^- \\) decay with \\( D^0 \\to K^- \\pi^+ \\) has the same final state as the signal decay, but with the \\( K^- \\pi^+ \\) mass peaking around the known \\( D^0 \\) mass [29]. By analysing these spectra, charmed resonances are identified, and candidates near the charm mass peaks are excluded, effectively suppressing the charmed background. Background arising from the misidentification of final-state particle species, such as a kaon misidentified as a proton or pion, is mitigated using a set of neural-network-based PID variables [48]. In addition, some misidentified particles originate from intermediate charmed resonances. By reconstructing the mass spectra with the appropriate particle masses, prominent resonance peaks are identified and excluded, effectively reducing this background contribution.\nThe otherwise excluded \\( \\Lambda_b^0 \\to \\Lambda_c^+ (\\to p K^- \\pi^+) \\pi^- \\) decay, which shares the same final state as the signal channel, instead comprises the control channel. The \\( CP \\) asymmetry in the \\( \\Lambda_b^0 \\to \\Lambda_c^+ \\pi^- \\) decay is expected to be negligible in the Standard Model, as it is dominated by the tree-level \\( b \\to c \\bar{u} d \\) transition, making it suitable for calibrating and cancelling nuisance asymmetries. All \\( \\Lambda_b^0 \\to \\Lambda_c^+ (\\to p K^- \\pi^+) \\pi^- \\) candidates are selected using the same criteria as imposed for the signal candidates, with the \\( p K^- \\pi^+ \\) mass confined to a region centred around the known \\( \\Lambda_c^+ \\) mass [29].\n\nAsymmetry measurement The asymmetry measurement is conducted separately for Run 1 and Run 2 samples, from signal yield extraction to the evaluation of nuisance asymmetries and systematic uncertainties. The signal yields from the two samples are then combined, while the results of the nuisance asymmetries and systematic uncertainties are statistically averaged. This averaging uses weights inversely proportional to the squared statistical uncertainties, which are determined from the respective mass fits. The yield asymmetries of the signal decay are measured to be \\( \\mathcal{A}_N = (5.12 \\pm 0.96)\\% \\) for Run 1 and \\( \\mathcal{A}_N = (3.42 \\pm 0.43)\\% \\) for Run 2, while those for the control mode are \\( \\mathcal{A}_N = (1.08 \\pm 0.55)\\% \\) for Run 1 and \\( \\mathcal{A}_N = (1.32 \\pm 0.25)\\% \\) for Run 2.\n\nThe signal yields for the \\( \\Lambda_b^0 \\to p K^- \\pi^+ \\pi^- \\) and \\( \\overline{\\Lambda}_b^0 \\to \\overline{p} K^+ \\pi^- \\pi^+ \\) decays are determined from a simultaneous extended unbinned maximum-likelihood fit to their mass spectra. The signal shape is modelled as a combination of a Gaussian and two Crystal Ball functions [49], all sharing the same peak position. The parameters of the signal function are determined from simulated events and are fixed in the fit to data, except for the Gaussian width, the average width of the Crystal Ball functions, and the peak position, which accounts for imperfections in the simulation. Various background sources are modelled separately in the fit. The background from partially reconstructed events, specifically the \\( \\Lambda_b^0 \\to p K^- \\pi^+ \\pi^- \\pi^0 \\) decay, where the \\( \\pi^0 \\) meson is not reconstructed, is described by an ARGUS function [50]. The background from the \\( \\Lambda_b^0 \\to p K^- \\eta' (\\to \\pi^+ \\pi^- \\gamma) \\) decay, where the photon is not reconstructed, is modelled with a distribution obtained using fast-simulated decays [51].\n\nThe decays \\( \\Lambda_b^0 \\to p \\pi^- \\pi^+ \\pi^- \\), \\( \\Lambda_b^0 \\to p K^- K^+ \\pi^- \\), and \\( \\Xi_b^0 \\to p K^- \\pi^+ K^- \\) may be incorrectly reconstructed as the \\( \\Lambda_b^0 \\to p K^- \\pi^+ \\pi^- \\) decay, with one final-state particle misidentified. Their mass distributions are modelled using simulation. The \\( \\Xi_b^0 \\to p K^- \\pi^+ \\pi^- \\) decay is described by the same model used for the \\( \\Lambda_b^0 \\) signal, but with the peak position shifted by the difference of the known \\( \\Xi_b^0 \\) and \\( \\Lambda_b^0 \\) baryon masses, and the width scaled by their mass ratio [52]. The combinatorial background, due to random combinations of final-state \\( p \\), \\( K^- \\), \\( \\pi^+ \\) and \\( \\pi^- \\) hadrons, is modelled as a linear function.\n\nFor the control channel, the \\( \\Lambda_b^0 \\) mass distribution is modelled using the same function as for the signal channel, with parameters determined independently from simulated \\( \\Lambda_b^0 \\to \\Lambda_c^+ (\\to p K^- \\pi^+) \\pi^- \\) decays. The background consists of a combinatorial component modelled by a linear function, a partially reconstructed background from the \\( \\Lambda_b^0 \\to \\Lambda_c^+ \\pi^- \\pi^0 \\) decay modelled as an ARGUS function, and a misidentified background from the \\( \\Lambda_b^0 \\to \\Lambda_c^+ K^- \\) decay, which is modelled based on a sample of simulated decays.\n\nIn the simultaneous fit, the same probability density function for each component is used for both baryon and antibaryon decays, with the yields allowed to differ between the two samples. The yield asymmetries obtained from the mass fits are affected by nuisance effects arising from asymmetries in the \\( b \\)-baryon production cross-section, as well as from the detection, reconstruction, and selection of final-state particles. Most of these\neffects cancel in the difference between the yield asymmetries of the signal and the control channels. Nevertheless, the difference in the \\( \\Lambda_b^0 \\) or final-state kinematics between the signal and control channels leads to an incomplete cancellation of nuisance asymmetries. To address this, the nuisance asymmetry difference is subtracted from the yield asymmetry difference after all such experimental asymmetries are accounted for.\n\nThe origins and corrections for experimental asymmetries are outlined below. The initial \\( pp \\) collision is a two-baryon system, which produces slightly more \\( \\Lambda_b^0 \\) baryons than \\( \\overline{\\Lambda}_b^0 \\) baryons, resulting in an asymmetry that depends on their rapidity \\( y \\) and their \\( p_T \\) [34]. The background-subtracted distributions of \\( y \\) and \\( p_T \\) for both the signal and control channels are first obtained using the sPlot technique [53]. Subsequently, the control-channel distributions are weighted to match those of the signal channel. As a result, the difference in production asymmetry between the signal channel and the kinematics-weighted control channel vanishes.\n\nPositively and negatively charged particles exhibit different behaviour when interacting with matter, resulting in different detection efficiencies, whose magnitude depends on the momentum of the particle. The final-state particles in this analysis include protons, kaons and pions. The proton detection asymmetry as a function of momentum is measured in Ref. [54]. The kaon detection asymmetry is studied using kaons from the \\( D^+ \\to K^- \\pi^+ \\pi^- \\) decay [55], while the pion detection asymmetry is investigated through \\( D^{**} \\to \\pi^+ D^0 (\\to K^- \\pi^+ \\pi^- \\pi^+) \\) and \\( D^0 \\to K_S^0 \\pi^+ \\pi^- \\) decays [56, 57]. Subsequently, the detection asymmetry for each final-state particle as a function of kinematics is averaged over the kinematic distribution in both the signal and control channels. Finally, the overall detection asymmetry is obtained by summing the detection asymmetry contributions from each final-state particle. The difference in detection asymmetry between the signal and control channels is presented in Extended Data Table 1, with the uncertainties estimated using pseudoexperiments. The same approach is applied to estimate the uncertainties from the PID asymmetry and trigger asymmetry discussed below.\n\nThe PID requirements applied to the final-state particles can introduce asymmetries between positively and negatively charged particles. Particle identification efficiencies and asymmetries for final-state particles of \\( \\Lambda_b^0 \\) and \\( \\overline{\\Lambda}_b^0 \\) decays are evaluated in bins of momentum, \\( p \\), and pseudorapidity, \\( \\eta \\), using calibration data [58, 59]. Then the PID asymmetry for each final-state particle is averaged over the distribution in the \\( p-\\eta \\) plane for the signal and control channels. The difference in PID asymmetry between the signal and control channels is presented in Extended Data Table 1.\n\nDetermination of the hardware-trigger efficiency asymmetry between oppositely charged hadrons uses the same methodology as for the PID asymmetry. The trigger efficiencies are studied separately for two categories of events: trigger on signal, where the trigger decision is based on the final state of the \\( \\Lambda_b^0 \\) decay, and trigger independent of signal, where the trigger decision depends on other particles rather than those from the signal decay. The trigger-on-signal efficiency and its asymmetry for a final-state particle, as a function of its energy deposit in the calorimeter, are determined using the \\( \\Lambda_b^0 \\to \\Lambda_c^+ (\\to p K^- \\pi^+) \\pi^- \\) sample for protons and a \\( D^0 \\to K^- \\pi^+ \\) sample for kaons and pions. Conversely, the trigger-independent-of-signal efficiency and its asymmetry, as a function of the \\( \\Lambda_b^0 \\) transverse momentum, are estimated utilising a control sample of \\( \\Lambda_b^0 \\) decays [60]. The total trigger efficiency asymmetry is calculated as a weighted average of the asymmetries of the two categories of events, with the difference between the signal and control channels presented in Extended Data Table 1.\nThe total nuisance asymmetry difference is the sum of the detection asymmetry, PID asymmetry, and trigger asymmetry differences between the signal and control channels. The corresponding uncertainties are calculated as the quadrature sum of the individual contributions. Results are also shown in Extended Data Table 1. The combined nuisance asymmetry difference for Run 1 and Run 2 is determined to be (0.01 ± 0.07)%.\n\nSystematic uncertainties In addition to the systematic uncertainties arising from the nuisance asymmetries, an additional uncertainty is associated with the \\( \\Lambda_b^0 \\) mass fit. This uncertainty is estimated by using alternative fit models, with the largest variation in the yield asymmetry among these models assigned as the systematic uncertainty. As alternative signal models, the fixed parameters of the signal shapes are modified up and down by one standard deviation, the \\( \\Lambda_b^0 \\) signal model is replaced with the sum of a Gaussian and a Hypatia function [61], and the difference between the \\( \\Xi_b^0 \\) and \\( \\Lambda_b^0 \\) masses, which is fixed during the fit, is varied by one standard deviation [29]. The combinatorial background distribution is changed from a linear function to an exponential function. The mass distribution of the \\( \\Lambda_b^0 \\to p\\pi^-\\pi^+\\pi^- \\) decay, reconstructed as the \\( \\Lambda_b^0 \\to pK^-\\pi^+\\pi^- \\) decay, is modelled in the baseline fit using a simulated sample generated with the mixture of a uniform distribution in phase space and intermediate resonances. As an alternative, the mass distribution is modelled using simulated decays with only a uniform distribution in the phase space. Finally, the partially reconstructed background from the \\( \\Lambda_b^0 \\to pK^-\\eta'(\\to \\pi^+\\pi^-\\gamma) \\) decay is modelled using a simulated sample with additional kinematic requirements applied. To evaluate the impact of the imperfect modelling of the partially reconstructed background from the \\( \\Lambda_b^0 \\to pK^-\\pi^+\\pi^- \\) decay, the \\( \\Lambda_b^0 \\) mass fit range is changed from \\( 5.40 < m(pK^-\\pi^+\\pi^-) < 6.10\\,\\mathrm{GeV}/c^2 \\) to \\( 5.45 < m(pK^-\\pi^+\\pi^-) < 6.10\\,\\mathrm{GeV}/c^2 \\), where this background is reduced by around a factor of two. The results are presented in Extended Data Table 2.\n\nThe total systematic uncertainty is taken as the quadratic sum of the systematic uncertainties arising from nuisance asymmetries and the mass fit, as presented in Extended Data Table 2. The combined systematic uncertainty for Run 1 and Run 2 is 0.10%.\n\nLocalised \\( CP \\) violation in the phase space Local \\( CP \\) asymmetries are studied in four regions of phase space, selected based on the \\( \\Lambda_b^0 \\to pK^-\\pi^+\\pi^- \\) decay topology. In total, seven resonance topologies are possible, with several hadronic resonances potentially contributing to each topology. Three of these topologies, namely \\( \\Lambda_b^0 \\to R(p\\pi^+)K^-\\pi^- \\), \\( \\Lambda_b^0 \\to R(pK^-\\pi^-)\\pi^+ \\) and \\( \\Lambda_b^0 \\to R(pK^-\\pi^+)\\pi^- \\), are strongly suppressed due to either the absence of relevant hadronic resonances or the flavour symmetry of the Standard Model [62], and are not selected for localised \\( CP \\) measurements. Two-body and three-body mass distributions and the selected regions are shown in Extended Data Figs. 2 and 3, respectively. The four phase-space regions correspond to:\n\n• Two-body decays where the \\( pK^- \\) and \\( \\pi^+\\pi^- \\) two-body systems result from separate intermediate resonance decays, \\( R(pK^-) \\) and \\( R(\\pi^+\\pi^-) \\). The \\( pK^- \\) mass is required to be less than 2.2 GeV/\\( c^2 \\), dominated by excited \\( \\Lambda \\) resonances, and the \\( \\pi^+\\pi^- \\) mass is required to be less than 1.1 GeV/\\( c^2 \\), containing light unflavoured \\( f_0(500) \\), \\( \\rho(770) \\) and \\( f_0(980) \\) resonances and a nonresonant \\( \\pi^+\\pi^- \\) component.\n\n• Two-body decays where the \\( p\\pi^- \\) and \\( \\pi^+K^- \\) two-body systems result from separate intermediate resonance decays, \\( R(p\\pi^-) \\) and \\( R(K^-\\pi^+) \\). It is required that\n\\( m(p\\pi^-) < 1.7 \\) GeV/\\( c^2 \\), delimiting a region dominated by excited nucleon (\\( N \\)) resonances, and \\( 0.8 < m(\\pi^+K^-) < 1.0 \\) GeV/\\( c^2 \\) or \\( 1.1 < m(\\pi^+K^-) < 1.6 \\) GeV/\\( c^2 \\), containing mostly \\( K^{*0} \\) resonances.\n\n• Three-body decay of excited \\( N^+ \\) resonances into the \\( p\\pi^+\\pi^- \\) final state, \\( R(p\\pi^-\\pi^+) \\). The requirement on the three-body mass is \\( m(p\\pi^+\\pi^-) < 2.7 \\) GeV/\\( c^2 \\).\n\n• Three-body decay of excited \\( K^- \\) resonances into the \\( K^-\\pi^+\\pi^- \\) final state, \\( R(K^-\\pi^+\\pi^-) \\). The mass region \\( m(K^-\\pi^+\\pi^-) < 2.0 \\) GeV/\\( c^2 \\) includes \\( K_1(1270)^- \\), \\( K_1(1400)^- \\) and \\( K^*(1410)^- \\) resonances.\n\nFor each phase-space region, the \\( CP \\) asymmetry is measured with the same method as for the global \\( \\mathcal{A}_{CP} \\) result.\n\nInterpretation For the \\( \\Lambda_b^0 \\to R(p\\pi^+\\pi^-)K^- \\) decay, the \\( u \\) quark produced from the \\( b \\to u\\bar{u}s \\) process combines with the \\( ud \\) quarks within the \\( \\Lambda_b^0 \\) baryon to form the \\( R \\) resonances, while the remaining \\( \\bar{u}s \\) quarks form the \\( K^- \\) meson. A similar process occurs in the \\( \\Lambda_b^0 \\to R(K^-\\pi^+\\pi^-)p \\) decay, where the \\( uud \\) quarks form the proton and the \\( \\bar{u}s \\) quarks contribute to the formation of the \\( R \\) resonances. The measured \\( CP \\) asymmetry is different for the two decays, suggesting different relative magnitudes of the tree and loop diagrams and/or strong phases. The \\( \\Lambda_b^0 \\to R(p\\pi^-)R(K^-\\pi^+) \\) decay involves a \\( b \\to d\\bar{d}s \\) transition, where the \\( d \\) quark forms the \\( R(p\\pi^-) \\) baryon together with \\( ud \\) quarks from the initial \\( \\Lambda_b^0 \\) baryon and the remaining \\( \\bar{d}s \\) quarks forms the \\( R(K^-\\pi^+) \\) meson. In this case, the tree amplitude does not contribute, and thus \\( CP \\) symmetry is expected to hold. Conversely, the \\( \\Lambda_b^0 \\to R(pK^-)R(\\pi^+\\pi^-) \\) decay represents a hybrid process involving both the \\( \\Lambda_b^0 \\to R(pK^-)f_0(980)(\\to \\pi^+\\pi^-) \\) process as well as nonresonant \\( \\pi^+\\pi^- \\) contributions. The former is predominantly driven by the \\( b \\to s\\bar{s}s \\) loop diagram, where an \\( s \\) quark and the \\( ud \\) quarks from the initial \\( \\Lambda_b^0 \\) baryon hadronise into the \\( R(pK^-) \\) baryon, and the rest forms the \\( f_0(980) \\) hadron. The latter may arise from both tree and loop diagrams of the \\( b \\to u\\bar{u}s \\) decay, where the \\( u\\bar{u} \\) quarks form the nonresonant \\( \\pi^+\\pi^- \\) system, allowing \\( CP \\) violation to emerge.\n\nSignificance and look-elsewhere effect For the global \\( \\mathcal{A}_{CP} \\), the baseline method to evaluate the significance is the \\( z \\)-score which is the \\( \\mathcal{A}_{CP} \\) absolute value divided by its total uncertainty. For the local \\( \\mathcal{A}_{CP} \\), the preliminary significance is obtained by dividing \\( \\mathcal{A}_{CP} \\) by its total uncertainty. Subsequently, the look-elsewhere effect [63] is accounted for to correct for the increased probability of observing a significant result due to multiple measurements. The look-elsewhere effect is determined through pseudoexperiments, which also consider correlations among \\( \\mathcal{A}_{CP} \\) measurements in different phase-space regions.\nExtended Data Figure 1: Mass distributions of the control channel together with the fit projections. Displayed are the mass distributions for the control channel: (a) \\( A_b^0 \\rightarrow A_c^+ \\pi^- \\), (b) \\( \\overline{A}_b^0 \\rightarrow \\overline{A}_c^- \\pi^+ \\).\n\nExtended Data Table 1: Nuisance asymmetry differences between signal and control channels for Runs 1 and 2.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
ContributionRun 1Run 2
Detection asymmetry difference(0.055 ± 0.128)%(0.081 ± 0.050)%
PID asymmetry difference(0.026 ± 0.141)%(−0.028 ± 0.002)%
Trigger asymmetry difference(−0.039 ± 0.029)%(−0.050 ± 0.008)%
Total nuisance asymmetry difference(0.042 ± 0.193)%(0.003 ± 0.051)%
\n\nExtended Data Table 2: Systematic uncertainties of the global \\( \\mathcal{A}_{CP} \\) measurement for Runs 1 and 2.\n\n\n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n \n
ContributionRun 1Run 2
Nuisance asymmetry difference0.193%0.051%
Mass fit0.044%0.067%
Total systematic uncertainty0.198%0.084%
\nExtended Data Figure 2: Distributions of two-body and three-body masses of final-state particles. The mass distributions of (a) \\( pK^- \\) and (b) \\( \\pi^+\\pi^- \\), corresponding to the \\( \\Lambda_b^0 \\to R(pK^-)R(\\pi^+\\pi^-) \\) phase-space region; (c) \\( p\\pi^- \\) and (d) \\( K^-\\pi^+ \\), corresponding to the \\( \\Lambda_b^0 \\to R(p\\pi^-)R(K^-\\pi^+) \\) phase-space region; (e) \\( p\\pi^+\\pi^- \\), representing the \\( \\Lambda_b^0 \\to R(p\\pi^+\\pi^-)K^- \\) phase-space region; and (f) \\( K^-\\pi^+\\pi^- \\), representing the \\( \\Lambda_b^0 \\to R(K^-\\pi^+\\pi^-)p \\) phase-space region. The \\( \\Lambda_b^0 \\) and \\( \\bar{\\Lambda}_b^0 \\) samples are combined for the plots.\nExtended Data Figure 3: Mass distributions in regions of phase space with the fit projections also shown. Mass distributions of \\( \\Lambda_b^0 \\to p K^- \\pi^+ \\pi^- \\) and \\( \\bar{\\Lambda}_b^0 \\to \\bar{p} K^+ \\pi^- \\pi^+ \\) for (a, b) \\( \\Lambda_b^0 \\to R(pK^-)R(\\pi^+\\pi^-) \\), (c, d) \\( \\Lambda_b^0 \\to R(p\\pi^-)R(\\pi^+K^-) \\), and (e, f) \\( \\Lambda_b^0 \\to R(K^- \\pi^+ \\pi^-)p \\) decays.\nAcknowledgements\n\nWe express our gratitude to our colleagues in the CERN accelerator departments for the excellent performance of the LHC. We thank the technical and administrative staff at the LHCb institutes. We acknowledge support from CERN and from the national agencies: ARC (Australia); CAPES, CNPq, FAPERJ and FINEP (Brazil); MOST and NSFC (China); CNRS/IN2P3 (France); BMBF, DFG and MPG (Germany); INFN (Italy); NWO (Netherlands); MNiSW and NCN (Poland); MCIID/IFA (Romania); MICIU and AEI (Spain); SNSF and SER (Switzerland); NASU (Ukraine); STFC (United Kingdom); DOE NP and NSF (USA). We acknowledge the computing resources that are provided by ARDC (Australia), CBPF (Brazil), CERN, IHEP and LZU (China), IN2P3 (France), KIT and DESY (Germany), INFN (Italy), SURF (Netherlands), Polish WLCG (Poland), IFIN-HH (Romania), PIC (Spain), CSCS (Switzerland), and GridPP (United Kingdom). We are indebted to the communities behind the multiple open-source software packages on which we depend. Individual groups or members have received support from Key Research Program of Frontier Sciences of CAS, CAS PIFI, CAS CCEPP, Fundamental Research Funds for the Central Universities, and Sci. & Tech. Program of Guangzhou (China); Minciencias (Colombia); EPLANET, Marie Sklodowska-Curie Actions, ERC and NextGenerationEU (European Union); A*MIDEX, ANR, IPhU and Labex P2IO, and Région Auvergne-Rhône-Alpes (France); Alexander-von-Humboldt Foundation (Germany); ICSC (Italy); Severo Ochoa and María de Maeztu Units of Excellence, GVA, XuntaGal, GENCAT, InTalent-Inditex and Prog. 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Molina Cardenas85, T. Mombacher49, M. Monk57,1, S. Monteil11, A. Morcillo Gomez47, G. Morello28, M.J. Morello35,r, M.P. Morgenthaler22, J. Moron40, W. Morren38, A.B. Morris49, A.G. Morris13, R. Mountain69, H. Mu4,b, Z. M. Mu6, E. Muhammad57, F. Muheim59, M. Mulder79, K. Müller51, F. Muñoz-Rojas9, R. Murta62, V. Mytrochenko52, P. Naik61, T. Nakada50, R. Nandakumar58, T. Nanut49, I. Nasteva3, M. Needham59, E. Nekrasova44, N. Neri30,n, S. Neubert18, N. Neufeld49, P. Neustroev44, J. Nicolini49, D. Nicotra80, E.M. Niel49, N. Nikitin44, Q. Niu73, P. Nogaroli3, P. Nogga18, C. Normand55, J. Novoa Fernandez47, G. Nowak66, C. Nunez85, H. N. Nur60, A. Oblakowska-Mucha40, V. Obraztsov44, T. Oeser17, S. Okamura26,k, A. Okhotnikov44, O. Okhrimenko53, R. Oldeman32,j, F. Oliva59, M. Olocco19, C.J.G. Onderwater80, R.H. O'Neil49, D. Osthues19, J.M. Otalora Goicochea3, P. Owen51, A. Oyanguren48, O. Ozcelik59, F. Paciolla35,v,\nA. Padde42, K.O. Padeken18, B. Pagare57, T. Pajero49, A. Palano24, M. Palutan28, X. Pan4,6, G. Panshin56, L. Paolucci57, A. Papapanestis58,49, M. Pappagallo34,g, L.L. Pappalardo26, C. Pappenheimer66, C. Parkes63, D. Parmar76, B. Passalacqua26,k, G. Passaleva27, D. Passaro35,r,49, A. Pastore24, M. Patel62, J. Patoc64, C. Patrignani25,i, A. Paul69, C.J. Pawley80, A. Pellegrino38, J. Peng5,7, M. Pepe Altarelli28, S. Perazzini25, D. Pereima44, H. Pereira Da Costa68, A. Pereiro Castro47, P. Perret11, A. Perrevoort79, A. Perro49,13, M.J. Peters66, K. Petridis55, A. Petrolini29,m, J. P. Pflaum66, H. Pham69, L. Pica36, M. Piccini34, L. Piccolo32, B. Pietrzyk10, G. Pietrzyk14, R. N. Pilato61, D. Pinci36, F. Pisani49, M. Pizziichemi31,o,49, V. Placinta43, M. Plo Casasus47, T. Poeschl49, F. Polci16, M. Poli Lener28, A. Poluektov15, N. Polukhina44, I. Polyakov63, E. Polycarpo3, S. Ponce49, D. Popov7,49, S. Poslavskii44, K. Prasanth59, C. Prouve82, D. Provenzano32,j, V. Pugatch53, G. Punzi35,s, S. Qasim51, Q. Q. Qian6, W. Qian7, N. Qin4,b, S. Qu4,b, R. Quagliani49, R.I. Rabadan Trejo57, J.H. Rademacker55, M. Rama35, M. Ramírez García85, V. Ramos De Oliveira70, M. Ramos Pernas57, M.S. Rangel3, F. Ratnikov44, G. Raven39, M. Rebollo De Miguel48, F. Redi30,h, J. Reich55, F. Reiss20, Z. Ren7, P.K. Resmi64, M. Ribalda Galvez45, R. Ribatti50, G. Ricart15,12, D. Riccardi35,r, S. Ricciardi58, K. Richardson55, M. Richardson-Sliper59, K. Rinnert61, P. Robbe14,49, G. Robertson60, E. Rodrigues61, A. Rodriguez Alvarez45, E. Rodriguez Fernandez47, J.A. Rodriguez Lopez75, E. Rodriguez Rodriguez49, J. Roensch19, A. Rogachev44, A. Rogovsky58, D.L. Rolff19, P. Roloff19, V. Romanovskiy66, A. Romero Vidal47, G. Romolini26, F. Ronchetti50, T. Rong6, M. Rotondo28, S. R. Roy22, M.S. Rudolph69, M. Ruiz Diaz22, R.A. Ruiz Fernandez47, J. Ruiz Vidal80, J. Rycka40, J. J. Saavedra-Arias9, J.J. Saborido Silva47, R. Sadek15, N. Sagidova44, D. Sahoo77, N. Sahoo54, B. Saitta32,j, M. Salomoni31,49,o, I. Sanderswood48, R. Santacesaria36, C. Santamarina Rios47, M. Santimaria28, L. Santoro2, E. Santovetti37, A. Saputti26,49, D. Sarain44, A. Sarntatskiy79, G. Sarpis59, M. Sarpis78, C. Satriano36,t, A. Satta37, D. Savrina44, H. Sazak17, F. Sborzaczak49,28, A. Scarabotto19, S. Schaef17, S. Scherl61, M. Schiller60, H. Schindler49, M. Schmelling21, B. Schmidt49, S. Schmitt17, H. Schmitz18, O. Schneider50, A. Schopper62, N. Schulte19, S. Schulte50, M.H. Schune14, G. Schwering17, B. Sciascia28, A. Sciuciatti49, I. Segal76, S. Sellam47, A. Semennikov44, T. Senger51, M. Senghi Soares39, A. Sergi29,m, N. Serra51, L. Sestini27, A. Seuthe19, D.Y. Shang6, D.M. Shangase85, M. Shapkin44, R. S. Sharma69, I. Shchemberov44, L. Shchutska50, T. Shears61, L. Shekhtman44, Z. Shen38, D. S. Sheng5,7, D. V. Shevchenko44, B. Shi7, Q. Shi7, Y. Shimizu14, E. Shmanin25, R. Shorkin44, J.D. Shupperd69, R. Silva Coutinho69, G. Simi33,p, S. Simone24,g, M. Singha77, N. Skidmore57, T. Skwarnicki69, M.W. Slater54, E. Smith65, K. Smith68, M. Smith62, A. Snoch38, L. Soares Lavra59, M.D. Sokoloff66, F.J.P. Soler60, A. Solomin55, A. Solovev44, I. Solovyev44, N. Sommerfeld18, R. Song1, Y. Song50, Y. Song4,b, Y. S. Song6, F.L. Souza De Almeida69, B. Souza De Paula3, E. Spadaro Norella29,m, E. Spedicato25, J.G. Speer19, E. Spiridenkov44, P. Spradlin60, V. Sriskaran49, F. Stagni49, M. Stahl76, S. Stahl49, S. Stanislaus64, M. Stefaniak86, E.N. Stein49, O. Steinkamp51, O. Stenyakin44, H. Stevens19, D. Strekalina44, Y. Su7, F. Suljik64, J. Sun32, L. Sun74, D. Sundfeld26, W. Sutcliffe51, K. Swientek40, F. Swystun56, A. Szabelski42, T. Szumlak40, Y. Tan4,b, Y. Tang74, M.D. Tat22, A. Terentev44, F. Terzuoli35,v,49, F. Teubert49, E. Thomas49, D.J.D. Thompson54, H. Tilquin62,\nV. Tisserand11, S. T'Jampens10, M. Tobin5,49, L. Tomassetti26,k, G. Tonani30,n, X. Tong6, D. Tork30, D. Torres Machado2, L. Toscano19, D.Y. Tou4,b, C. Tripli46, G. Tuci22, N. Tuning38, L.H. Uecker22, A. Ukleja40, D.J. Unverzagt22, A. Upadhyay77, B. Urbach59, A. Usachov39, A. Ustyuzhanin44, U. Uwer22, V. Vagnoni25, V. Valcarce Cadenas47, G. Valenti25, N. Valls Canudas49, J. van Eldik49, H. Van Hecke68, E. van Herwijnen62, C.B. Van Hulse47,y, R. Van Laak50, M. van Veghel38, G. Vasquez51, R. Vazquez Gomez45, P. Vazquez Regueiro47, C. Vázquez Sierra82, S. Vecchi26, J.J. Velthuis59, M. Veltri27,w, A. Venkateswaran50, M. Verdoglia32, M. Vesterinen57, D. Vico Benet64, P. Vidrier Villalba45, M. Vieites Diaz47, X. Vilasis-Cardona46, E. Vilella Figueras61, A. Villa25, P. Vincent16, B. Vivacqua3, F.C. Volle54, D. vom Bruch13, N. Voropaev44, K. Vos80, C. Vrashas59, J. Wagner19, J. Walsh35, E.J. Walton1,57, G. Wan6, A. Wang12, C. Wang22, G. Wang8, H. Wang73, J. Wang6, J. Wang5, J. Wang4,b, J. Wang74, M. Wang49, N. W. Wang7, R. Wang35, X. Wang8, X. Wang72, X. W. Wang62, Y. Wang6, Y. W. Wang73, Z. Wang14, Z. Wang4,b, Z. Wang30, J.A. Ward57,1, M. Waterlaat49, N.K. Watson54, D. Websdale62, Y. Wei6, J. Wendel82, B.D.C. Westhenry55, C. White56, M. Whitehead60, E. Whiter54, A.R. Wiederhold63, D. Wiedner19, G. Wilkinson64, M.K. Wilkinson66, M. Williams65, M. J. Williams49, M.R.J. Williams59, R. Williams56, Z. Williams55, F.F. Wilson58, M. Winn12, W. Wislicki42, M. Witek41, L. Witola19, G. Wormser14, S.A. Wotton56, H. Wu69, J. Wu8, X. Wu74, Y. Wu56, Z. Wu7, K. Wylie49, S. Xian72, Z. Xiang5, Y. Xie8, T. X. Xing30, A. Xu35, L. Xu4,b, L. Xu4,b, M. Xu87, Z. Xu19, Z. Xu7, Z. Xu7, K. Yang62, S. Yang7, X. Yang6, Y. Yang29,m, Z. Yang6, V. Yeroshenko14, H. Yeung63, H. Yin8, X. Yin7, C. Y. Yu6, J. Yu71, X. Yuan5, Y. Yuan5,7, E. Zaffaroni50, M. Zavertyaev21, M. Zdybal11, F. Zenesimi25, C. Zeng5,7, M. Zeng4,b, C. Zhang6, D. Zhang8, J. Zhang7, L. Zhang4,b, S. Zhang71, S. Zhang64, Y. Zhang6, Y. Z. Zhang4,b, Z. Zhang4,b, Y. Zhao22, A. Zhelezov22, S. Z. Zheng6, X. Z. Zheng4,b, Y. Zheng7, T. Zhou6, X. Zhou8, Y. Zhou7, V. Zhokhovska57, L. Z. Zhu7, X. Zhu4,b, X. Zhu8, V. Zhukov17, J. Zhuo48, Q. Zou5,7, D. Zuliani33,p, G. Zunica50.\n\n1School of Physics and Astronomy, Monash University, Melbourne, Australia\n2Centro Brasileiro de Pesquisas Físicas (CBPF), Rio de Janeiro, Brazil\n3Universidade Federal do Rio de Janeiro (UFRJ), Rio de Janeiro, Brazil\n4Department of Engineering Physics, Tsinghua University, Beijing, China\n5Institute Of High Energy Physics (IHEP), Beijing, China\n6School of Physics State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing, China\n7University of Chinese Academy of Sciences, Beijing, China\n8Institute of Particle Physics, Central China Normal University, Wuhan, Hubei, China\n9Consejo Nacional de Rectores (CONARE), San Jose, Costa Rica\n10Université Savoie Mont Blanc, CNRS, IN2P3-LAPP, Annecy, France\n11Université Clermont Auvergne, CNRS/IN2P3, LPC, Clermont-Ferrand, France\n12Université Paris-Saclay, Centre d’Etudes de Saclay (CEA), IRFU, Saclay, France, Gif-Sur-Yvette, France\n13Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France\n14Université Paris-Saclay, CNRS/IN2P3, IJCLab, Orsay, France\n15Laboratoire Leprince-Ringuet, CNRS/IN2P3, Ecole Polytechnique, Institut Polytechnique de Paris, Palaiseau, France\n16LPNHE, Sorbonne Université, Paris Diderot Sorbonne Paris Cité, CNRS/IN2P3, Paris, France\n17I. Physikalisches Institut, RWTH Aachen University, Aachen, Germany\n18Universität Bonn - Helmholtz-Institut für Strahlen und Kernphysik, Bonn, Germany\n19 Fakultät Physik, Technische Universität Dortmund, Dortmund, Germany\n20 Physikalisches Institut, Albert-Ludwigs-Universität Freiburg, Freiburg, Germany\n21 Max-Planck-Institut für Kernphysik (MPIK), Heidelberg, Germany\n22 Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany\n23 School of Physics, University College Dublin, Dublin, Ireland\n24 INFN Sezione di Bari, Bari, Italy\n25 INFN Sezione di Bologna, Bologna, Italy\n26 INFN Sezione di Ferrara, Ferrara, Italy\n27 INFN Sezione di Firenze, Firenze, Italy\n28 INFN Laboratori Nazionali di Frascati, Frascati, Italy\n29 INFN Sezione di Genova, Genova, Italy\n30 INFN Sezione di Milano, Milano, Italy\n31 INFN Sezione di Milano-Bicocca, Milano, Italy\n32 INFN Sezione di Cagliari, Monserrato, Italy\n33 INFN Sezione di Padova, Padova, Italy\n34 INFN Sezione di Perugia, Perugia, Italy\n35 INFN Sezione di Pisa, Pisa, Italy\n36 INFN Sezione di Roma La Sapienza, Roma, Italy\n37 INFN Sezione di Roma Tor Vergata, Roma, Italy\n38 Nikhef National Institute for Subatomic Physics, Amsterdam, Netherlands\n39 Nikhef National Institute for Subatomic Physics and VU University Amsterdam, Amsterdam, Netherlands\n40 AGH - University of Krakow, Faculty of Physics and Applied Computer Science, Kraków, Poland\n41 Henryk Niewodniczanski Institute of Nuclear Physics Polish Academy of Sciences, Kraków, Poland\n42 National Center for Nuclear Research (NCBJ), Warsaw, Poland\n43 Horia Hulubei National Institute of Physics and Nuclear Engineering, Bucharest-Magurele, Romania\n44 Authors affiliated with an institute formerly covered by a cooperation agreement with CERN.\n45 ICCUB, Universitat de Barcelona, Barcelona, Spain\n46 La Salle, Universitat Ramon Llull, Barcelona, Spain\n47 Instituto Galego de Física de Altas Enerxías (IGFAE), Universidade de Santiago de Compostela, Santiago de Compostela, Spain\n48 Instituto de Física Corpuscular, Centro Mixto Universidad de Valencia - CSIC, Valencia, Spain\n49 European Organization for Nuclear Research (CERN), Geneva, Switzerland\n50 Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland\n51 Physik-Institut, Universität Zürich, Zürich, Switzerland\n52 NSC Kharkiv Institute of Physics and Technology (NSC KIPT), Kharkiv, Ukraine\n53 Institute for Nuclear Research of the National Academy of Sciences (KINR), Kyiv, Ukraine\n54 School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom\n55 H.H. Wills Physics Laboratory, University of Bristol, Bristol, United Kingdom\n56 Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom\n57 Department of Physics, University of Warwick, Coventry, United Kingdom\n58 STFC Rutherford Appleton Laboratory, Didcot, United Kingdom\n59 School of Physics and Astronomy, University of Edinburgh, Edinburgh, United Kingdom\n60 School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom\n61 Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom\n62 Imperial College London, London, United Kingdom\n63 Department of Physics and Astronomy, University of Manchester, Manchester, United Kingdom\n64 Department of Physics, University of Oxford, Oxford, United Kingdom\n65 Massachusetts Institute of Technology, Cambridge, MA, United States\n66 University of Cincinnati, Cincinnati, OH, United States\n67 University of Maryland, College Park, MD, United States\n68 Los Alamos National Laboratory (LANL), Los Alamos, NM, United States\n69 Syracuse University, Syracuse, NY, United States\n70 Pontifícia Universidade Católica do Rio de Janeiro (PUC-Rio), Rio de Janeiro, Brazil, associated to \\( ^{3} \\)\n71 School of Physics and Electronics, Hunan University, Changsha City, China, associated to \\( ^{8} \\)\n72 Guangdong Provincial Key Laboratory of Nuclear Science, Guangdong-Hong Kong Joint Laboratory of\nQuantum Matter, Institute of Quantum Matter, South China Normal University, Guangzhou, China, associated to 4\n73 Lanzhou University, Lanzhou, China, associated to 5\n74 School of Physics and Technology, Wuhan University, Wuhan, China, associated to 4\n75 Departamento de Fisica , Universidad Nacional de Colombia, Bogota, Colombia, associated to 16\n76 Ruhr Universitaet Bochum, Fakultae t. Physik und Astronomie, Bochum, Germany, associated to 19\n77 Eotvos Lorand University, Budapest, Hungary, associated to 49\n78 Faculty of Physics, Vilnius University, Vilnius, Lithuania, associated to 20\n79 Van Swinderen Institute, University of Groningen, Groningen, Netherlands, associated to 38\n80 Universiteit Maastricht, Maastricht, Netherlands, associated to 38\n81 Tadeusz Kosciuszko Cracow University of Technology, Cracow, Poland, associated to 41\n82 Universidade da Coruña, A Coruña, Spain, associated to 46\n83 Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden, associated to 60\n84 Taras Shevchenko University of Kyiv, Faculty of Physics, Kyiv, Ukraine, associated to 14\n85 University of Michigan, Ann Arbor, MI, United States, associated to 60\n86 Ohio State University, Columbus, United States, associated to 68\n\na Centro Federal de Educaçao Tecnológica Celso Suckow da Fonsca, Rio De Janeiro, Brazil\nb Center for High Energy Physics, Tsinghua University, Beijing, China\nc Hangzhou Institute for Advanced Study, UCAS, Hangzhou, China\nd LIP6, Sorbonne Université, Paris, France\ne Lamarr Institute for Machine Learning and Artificial Intelligence, Dortmund, Germany\nf Universidad Nacional Autónoma de Honduras, Tegucigalpa, Honduras\ng Università di Bari, Bari, Italy\nh Università di Bergamo, Bergamo, Italy\ni Università di Bologna, Bologna, Italy\nj Università di Cagliari, Cagliari, Italy\nk Università di Ferrara, Ferrara, Italy\nl Università di Firenze, Firenze, Italy\nm Università di Genova, Genova, Italy\nn Università degli Studi di Milano, Milano, Italy\no Università degli Studi di Milano-Bicocca, Milano, Italy\np Università di Padova, Padova, Italy\nq Università di Perugia, Perugia, Italy\nr Scuola Normale Superiore, Pisa, Italy\ns Università di Pisa, Pisa, Italy\nt Università della Basilicata, Potenza, Italy\nu Università di Roma Tor Vergata, Roma, Italy\nv Università di Siena, Siena, Italy\nw Università di Urbino, Urbino, Italy\nx Universidad de Ingeniería y Tecnología (UTEC), Lima, Peru\ny Universidad de Alcalá, Alcalá de Henares , Spain\nz Facultad de Ciencias Físicas, Madrid, Spain\n\n† Deceased"}