Text Simplification Materials
Collection
A collection to store all models and datasets created while my undergrad thesis • 7 items • Updated
Datasets:
abstract stringlengths 36 9.99k | completion stringlengths 14 7.8k | label bool 2
classes | score float64 1.01 4.99 |
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additive models play an important role in semiparametric statistics .
this paper gives learning rates for regularized kernel based methods for additive models .
these learning rates compare favourably in particular in high dimensions to recent results on optimal learning rates for purely nonparametric regularized ... | This paper provides learning rates for regularized kernel-based methods of additive models, specifically focusing on semiparametric statistics in high dimensions. | false | 3.18 |
additive models play an important role in semiparametric statistics .
this paper gives learning rates for regularized kernel based methods for additive models .
these learning rates compare favourably in particular in high dimensions to recent results on optimal learning rates for purely nonparametric regularized ... | This article discusses learning rates for regularized kernel based methods in additive models, comparing these to recent results on optimal learning rates for purely nonparametric regularized kernel based quantile regression using the Gaussian radial basis function kernel. The researchers give a concrete example that s... | false | 3.26 |
we have studied the leptonic decay @xmath0 , via the decay channel @xmath1 , using a sample of tagged @xmath2 decays collected near the @xmath3 peak production energy in @xmath4 collisions with the cleo - c detector .
we obtain @xmath5 and determine the decay constant @xmath6 mev , where the first uncertainties are... | We analyzed leptonic decays using a specific decay channel, utilizing a tagged sample collected near the peak production energy in collisions with the CLEO-C detector. We determined the decay constant (mev) with both statistical and systematic uncertainties, after obtaining certain results. | false | 3.23 |
we have studied the leptonic decay @xmath0 , via the decay channel @xmath1 , using a sample of tagged @xmath2 decays collected near the @xmath3 peak production energy in @xmath4 collisions with the cleo - c detector .
we obtain @xmath5 and determine the decay constant @xmath6 mev , where the first uncertainties are... | We studied leptonic decay through a specific channel using tagged decays collected at peak production energy in collisions with the CLEO-C detector. We found results and determined the decay constant of MeV, where the first uncertainties are statistical and the second are systematic. | false | 3.33 |
we have studied the leptonic decay @xmath0 , via the decay channel @xmath1 , using a sample of tagged @xmath2 decays collected near the @xmath3 peak production energy in @xmath4 collisions with the cleo - c detector .
we obtain @xmath5 and determine the decay constant @xmath6 mev , where the first uncertainties are... | We studied the decay of a particle into leptons using data from tagged decays collected at a specific energy in collisions with the CLEO-c detector. We found a value of @xmath5 and determined the decay constant @xmath6 MeV, where the first uncertainties are statistical and the second are systematic. | false | 3.35 |
we have studied the leptonic decay @xmath0 , via the decay channel @xmath1 , using a sample of tagged @xmath2 decays collected near the @xmath3 peak production energy in @xmath4 collisions with the cleo - c detector .
we obtain @xmath5 and determine the decay constant @xmath6 mev , where the first uncertainties are... | We studied the leptonic decay using the @xmath1 channel with tagged @xmath2 decays collected near peak production energy in @xmath4 collisions, detected by CLEO-c. We measured @xmath5 and found the decay constant to be @xmath6 MeV, with statistical uncertainties first and systematic second. | false | 3.14 |
we have studied the leptonic decay @xmath0 , via the decay channel @xmath1 , using a sample of tagged @xmath2 decays collected near the @xmath3 peak production energy in @xmath4 collisions with the cleo - c detector .
we obtain @xmath5 and determine the decay constant @xmath6 mev , where the first uncertainties are... | We analyzed leptonic decays via channel decay, in collisions with tagged @xmath2 decays collected near @xmath3 peak production energy in @xmath4 collisions with cleo-c detector. We got a rate and determined the constant at 5 meV, with statistical and systematic uncertainties. | false | 3.07 |
we have studied the leptonic decay @xmath0 , via the decay channel @xmath1 , using a sample of tagged @xmath2 decays collected near the @xmath3 peak production energy in @xmath4 collisions with the cleo - c detector .
we obtain @xmath5 and determine the decay constant @xmath6 mev , where the first uncertainties are... | We analyzed lepton decay through channel, using tagged data from CLEO-c detector at peak energy in collisions. We find constants and their uncertainties. | false | 2.94 |
in 84 , 258 ( 2000 ) , mateos conjectured that current reversal in a classical deterministic ratchet is associated with bifurcations from chaotic to periodic regimes .
this is based on the comparison of the current and the bifurcation diagram as a function of a given parameter for a periodic asymmetric potential .
... | current reversals are associated with bifurcations from chaotic to periodic regimes | false | 1.95 |
in 84 , 258 ( 2000 ) , mateos conjectured that current reversal in a classical deterministic ratchet is associated with bifurcations from chaotic to periodic regimes .
this is based on the comparison of the current and the bifurcation diagram as a function of a given parameter for a periodic asymmetric potential .
... | Mateos proposed that changes in the direction of current in a ratchet system relate to shifts from chaotic to regular behavior. Barbi and Salerno studied this and found current changes can happen even without these shifts. Their studies focused on single particles, while ensemble behavior may differ. This paper examine... | true | 4.64 |
in 84 , 258 ( 2000 ) , mateos conjectured that current reversal in a classical deterministic ratchet is associated with bifurcations from chaotic to periodic regimes .
this is based on the comparison of the current and the bifurcation diagram as a function of a given parameter for a periodic asymmetric potential .
... | Mateos and Barbi-Salerno both explored current reversals due to bifurcations, but Mateos' study suggested that these reversals occur regardless of whether there were any changes in the system's chaotic behavior. We investigated this further by examining how currents vary based on ensemble characteristics and conditions... | false | 3.06 |
the effect of a random phase diffuser on fluctuations of laser light ( scintillations ) is studied .
not only spatial but also temporal phase variations introduced by the phase diffuser are analyzed .
the explicit dependence of the scintillation index on finite - time phase variations is obtained for long propagat... | The study examines how a random phase diffuser affects laser light fluctuations (scintillations). Both spatial and temporal phase changes from the diffuser are analyzed. For long paths, it's found that larger phase fluctuations reduce the diffuser's ability to suppress scintillations. | true | 4.58 |
the effect of a random phase diffuser on fluctuations of laser light ( scintillations ) is studied .
not only spatial but also temporal phase variations introduced by the phase diffuser are analyzed .
the explicit dependence of the scintillation index on finite - time phase variations is obtained for long propagat... | The study examines how a random phase diffuser affects laser light fluctuations (scintillations). It analyzes both spatial and temporal changes in phase introduced by the diffuser. The research finds that for long distances, scintillation depends on time-limited phase changes. When phase fluctuations are large, this ti... | true | 4.58 |
the effect of a random phase diffuser on fluctuations of laser light ( scintillations ) is studied .
not only spatial but also temporal phase variations introduced by the phase diffuser are analyzed .
the explicit dependence of the scintillation index on finite - time phase variations is obtained for long propagat... | The study examines how a random phase diffuser affects laser light fluctuations (scintillations). It looks at both spatial and temporal phase changes caused by the diffuser. For long distances, it finds out how scintillation depends on short-term phase variations. It shows that large phase fluctuations reduce the diffu... | true | 4.53 |
the effect of a random phase diffuser on fluctuations of laser light ( scintillations ) is studied .
not only spatial but also temporal phase variations introduced by the phase diffuser are analyzed .
the explicit dependence of the scintillation index on finite - time phase variations is obtained for long propagat... | The study looks at how a random phase diffuser affects laser light fluctuations, known as scintillations. Both spatial and temporal phase changes caused by the diffuser are examined. The research finds how the scintillation index depends on short-term phase changes over long distances. It is shown that when phase fluct... | true | 4.65 |
the effect of a random phase diffuser on fluctuations of laser light ( scintillations ) is studied .
not only spatial but also temporal phase variations introduced by the phase diffuser are analyzed .
the explicit dependence of the scintillation index on finite - time phase variations is obtained for long propagat... | Researchers examine how random phase changes affect laser light fluctuations over long distances, considering both space and time effects. | false | 3.49 |
with a special intention of clarifying the underlying spin contents of the nucleon , we investigate the generalized form factors of the nucleon , which are defined as the @xmath0-th @xmath1-moments of the generalized parton distribution functions , within the framework of the chiral quark soliton model .
a particula... | The generalized form factors of the nucleon are defined as the x_th moment of the generalized parton distribution functions within the chiral quark soliton model, where we examine the pion mass dependence of final predictions and compare them with lattice qcd simulations. | false | 2.64 |
with a special intention of clarifying the underlying spin contents of the nucleon , we investigate the generalized form factors of the nucleon , which are defined as the @xmath0-th @xmath1-moments of the generalized parton distribution functions , within the framework of the chiral quark soliton model .
a particula... | To better understand the spin structure of protons, we studied their generalized form factors using a model called the chiral quark soliton model. These form factors are based on parton distribution functions. We focused on how the pion mass affects results and compared them to lattice QCD simulations in a high pion ma... | true | 4.53 |
with a special intention of clarifying the underlying spin contents of the nucleon , we investigate the generalized form factors of the nucleon , which are defined as the @xmath0-th @xmath1-moments of the generalized parton distribution functions , within the framework of the chiral quark soliton model .
a particula... | We study how generalized parton distribution functions affect nucleons, focusing on how changes in pion mass influence predictions. We find that these predictions can be very sensitive to such changes. | false | 3.4 |
we improve the currently known thresholds for basisness of the family of periodically dilated @xmath0-sine functions .
our findings rely on a beurling decomposition of the corresponding change of coordinates in terms of shift operators of infinite multiplicity .
we also determine refined bounds on the riesz consta... | We improve known thresholds for periodically dilated sine functions. Our findings use a Beurling decomposition involving shift operators. We also find better bounds for the Riesz constant. These results fill gaps in existing literature. | true | 4.59 |
we improve the currently known thresholds for basisness of the family of periodically dilated @xmath0-sine functions .
our findings rely on a beurling decomposition of the corresponding change of coordinates in terms of shift operators of infinite multiplicity .
we also determine refined bounds on the riesz consta... | our findings rely on a beurling decomposition of the corresponding change of coordinates in terms of shift operators of infinite multiplicity | false | 2.65 |
we improve the currently known thresholds for basisness of the family of periodically dilated @xmath0-sine functions .
our findings rely on a beurling decomposition of the corresponding change of coordinates in terms of shift operators of infinite multiplicity .
we also determine refined bounds on the riesz consta... | We have improved the known thresholds for the basisness of a family of periodically dilated sine functions. Our work uses a Beurling decomposition of the coordinate change involving infinite shift operators. We also found better bounds for the Riesz constant related to this family. These results fill gaps in previous r... | true | 4.78 |
we improve the currently known thresholds for basisness of the family of periodically dilated @xmath0-sine functions .
our findings rely on a beurling decomposition of the corresponding change of coordinates in terms of shift operators of infinite multiplicity .
we also determine refined bounds on the riesz consta... | We found better limits for identifying basic functions within a group of sine functions that are repeatedly expanded. This relies on breaking down the relevant coordinate change using operators that shift infinitely. We also found sharper limits for a constant related to this group of functions. These results resolve u... | true | 4.55 |
we improve the currently known thresholds for basisness of the family of periodically dilated @xmath0-sine functions .
our findings rely on a beurling decomposition of the corresponding change of coordinates in terms of shift operators of infinite multiplicity .
we also determine refined bounds on the riesz consta... | We improve the known limits for when a family of sine functions, which are periodically stretched, form a basis. Our work uses a Beurling decomposition that breaks down changes in coordinates using shift operators with infinite multiplicity. We also refine the bounds on the Riesz constant for this family. These results... | true | 4.69 |
we improve the currently known thresholds for basisness of the family of periodically dilated @xmath0-sine functions .
our findings rely on a beurling decomposition of the corresponding change of coordinates in terms of shift operators of infinite multiplicity .
we also determine refined bounds on the riesz consta... | We are improving known thresholds for periodic sine basisness functions, using Beurling decomposition to determine shift operators with infinite multiplicity. We're also determining refined bounds on Riesz constants associated to this family, sealing gaps in existing literature. | false | 3.36 |
synaptic memory is considered to be the main element responsible for learning and cognition in humans .
although traditionally non - volatile long - term plasticity changes have been implemented in nanoelectronic synapses for neuromorphic applications , recent studies in neuroscience have revealed that biological sy... | Synaptic memory is crucial for learning and thinking in humans. Traditionally, non-volatile long-term changes have been used in nanoelectronic synapses for neuromorphic applications. Recent neuroscience findings show that biological synapses undergo temporary strengthening followed by long-term enhancement when the sti... | true | 4.59 |
synaptic memory is considered to be the main element responsible for learning and cognition in humans .
although traditionally non - volatile long - term plasticity changes have been implemented in nanoelectronic synapses for neuromorphic applications , recent studies in neuroscience have revealed that biological sy... | the magnetization dynamics of a magnetic tunnel junction are similar to short - term plasticity and long - term potentiation observed in biological synapses | false | 2.58 |
synaptic memory is considered to be the main element responsible for learning and cognition in humans .
although traditionally non - volatile long - term plasticity changes have been implemented in nanoelectronic synapses for neuromorphic applications , recent studies in neuroscience have revealed that biological sy... | Synaptic memory is crucial for learning and thinking in humans. Traditionally, changes in nanoelectronic synapses were used to mimic long-term memory changes, but new research shows that biological synapses strengthen temporarily before stabilizing if the input stimulus is frequent enough. This process of strengthening... | true | 4.66 |
synaptic memory is considered to be the main element responsible for learning and cognition in humans .
although traditionally non - volatile long - term plasticity changes have been implemented in nanoelectronic synapses for neuromorphic applications , recent studies in neuroscience have revealed that biological sy... | Synaptic memory is key to learning and thinking. Recent neuroscience shows that biological synapses strengthen temporarily, then potentially long-term if stimulated often. This can inspire new computer architectures. This paper shows that a magnetic tunnel junction (MTJ) behaves like synapses, showing both short-term a... | true | 4.5 |
synaptic memory is considered to be the main element responsible for learning and cognition in humans .
although traditionally non - volatile long - term plasticity changes have been implemented in nanoelectronic synapses for neuromorphic applications , recent studies in neuroscience have revealed that biological sy... | The memory in our brain is made up of two elements; one for short term memory and another for long term. There are many neuroscience studies which have shown that when we expose the synapses to a certain frequency, there can be an increase or decrease in memory strength depending on how often we repeat the stimuli. Sim... | false | 3.01 |
this paper investigates , using prior shape models and the concept of ball scale ( b - scale ) , ways of automatically recognizing objects in 3d images without performing elaborate searches or optimization .
that is , the goal is to place the model in a single shot close to the right pose ( position , orientation , ... | This paper investigates using prior shape models and the concept of ball scale ( b - scale ) ways of automatically recognizing objects in 3D images without performing elaborate searches or optimization. | false | 3.32 |
this paper investigates , using prior shape models and the concept of ball scale ( b - scale ) , ways of automatically recognizing objects in 3d images without performing elaborate searches or optimization .
that is , the goal is to place the model in a single shot close to the right pose ( position , orientation , ... | This paper looks at ways to automatically recognize objects in 3D images using shape models and ball scale (b-scale) without needing complex searches or optimization. The goal is to quickly place a model close to the correct position, orientation, and scale in an image so that the model boundaries match the object boun... | true | 4.49 |
long time coverage and high radial velocity precision have allowed for the discovery of additional objects in known planetary systems .
many of the extrasolar planets detected have highly eccentric orbits , which raises the question of how likely those systems are to host additional planets .
we investigate six sy... | Scientists have found new objects in known planetary systems using long-term observations and precise radial velocity measurements. Many of the discovered extrasolar planets have highly eccentric orbits, which raises questions about the likelihood of other planets existing in these systems. The researchers studied six ... | true | 4.63 |
long time coverage and high radial velocity precision have allowed for the discovery of additional objects in known planetary systems .
many of the extrasolar planets detected have highly eccentric orbits , which raises the question of how likely those systems are to host additional planets .
we investigate six sy... | Long-term observations with precise radial velocity measurements have helped discover more planets in known systems. Many extrasolar planets have very eccentric orbits, making it uncertain if additional planets could exist there. We studied six systems with highly eccentric planets: HD 3651, HD 37605, HD 45350, HD 8060... | true | 4.52 |
long time coverage and high radial velocity precision have allowed for the discovery of additional objects in known planetary systems .
many of the extrasolar planets detected have highly eccentric orbits , which raises the question of how likely those systems are to host additional planets .
we investigate six sy... | highly eccentric orbits are highly likely to be associated with additional planets in these systems | false | 2.15 |
long time coverage and high radial velocity precision have allowed for the discovery of additional objects in known planetary systems .
many of the extrasolar planets detected have highly eccentric orbits , which raises the question of how likely those systems are to host additional planets .
we investigate six sy... | Long-term observations with precise measurements have led to finding more objects in known planetary systems. Many detected extrasolar planets have unusual, stretched-out orbits, making us wonder if these systems could have other planets too. We studied six such systems—HD 3651, HD 37605, HD 45350, HD 80606, HD 89744, ... | true | 4.62 |
long time coverage and high radial velocity precision have allowed for the discovery of additional objects in known planetary systems .
many of the extrasolar planets detected have highly eccentric orbits , which raises the question of how likely those systems are to host additional planets .
we investigate six sy... | Long-term observations with high precision in measuring radial velocity have made it possible to find more objects in known planetary systems. Many of the detected exoplanets have very elliptical orbits, which makes us wonder if these systems can have more planets. We studied six systems that each have a planet with a ... | true | 4.61 |
long time coverage and high radial velocity precision have allowed for the discovery of additional objects in known planetary systems .
many of the extrasolar planets detected have highly eccentric orbits , which raises the question of how likely those systems are to host additional planets .
we investigate six sy... | Advanced observations found more planets, especially those with unusual orbits. We studied six systems where an eccentric planet is detected and look for additional planets or determine stability using simulations. | false | 3.31 |
we study equilibrium configurations of swarming biological organisms subject to exogenous and pairwise endogenous forces . beginning with a discrete dynamical model
, we derive a variational description of the corresponding continuum population density .
equilibrium solutions are extrema of an energy functional , ... | we study equilibrium configurations of swarming biological organisms subject to exogenous and pairwise endogenous forces , | false | 2.39 |
we study equilibrium configurations of swarming biological organisms subject to exogenous and pairwise endogenous forces . beginning with a discrete dynamical model
, we derive a variational description of the corresponding continuum population density .
equilibrium solutions are extrema of an energy functional , ... | We study how groups of biological organisms form stable patterns due to outside forces and interactions among themselves. Starting with a model for individual organisms, we create a mathematical description for the overall population's density. Stable solutions are found by minimizing an energy function and solving a s... | true | 4.5 |
we study equilibrium configurations of swarming biological organisms subject to exogenous and pairwise endogenous forces . beginning with a discrete dynamical model
, we derive a variational description of the corresponding continuum population density .
equilibrium solutions are extrema of an energy functional , ... | We studied stable arrangements of swarming organisms influenced by external and internal forces. Starting with a step-by-step model, we created a continuous description of the population. These stable arrangements are found by minimizing an energy functional and solving an integral equation. We determined conditions fo... | true | 4.68 |
we study equilibrium configurations of swarming biological organisms subject to exogenous and pairwise endogenous forces . beginning with a discrete dynamical model
, we derive a variational description of the corresponding continuum population density .
equilibrium solutions are extrema of an energy functional , ... | A model for swarming biological organisms equilibrium configuration with exogenous forces and pairwise endogenous forces. Equilibrium solutions are the extrema of an energy functional, and are described by Fredholm integral equations. Local minima, global minima, and minimas with respect to infinitesimal displacements ... | false | 3.18 |
i discuss new results on absolute branching ratios of charm mesons into specific exclusive final states , cabibbo suppressed decay rates , inclusive decays to @xmath0 mesons , limits on @xmath1 mixing , cp violation and t violation .
preliminary results from cleo - c now dominate the world average absolute branching... | New results on absolute branching ratios of charm mesons into specific exclusive final states, Cabibbo suppressed decay rates, inclusive decays to xmath0 mesons, limits on xmath1 mixing, cp violation, and t-violation are consistent with the @xmath5 cleo measurements. Initial calculations have a world average of approxi... | false | 2.3 |
i discuss new results on absolute branching ratios of charm mesons into specific exclusive final states , cabibbo suppressed decay rates , inclusive decays to @xmath0 mesons , limits on @xmath1 mixing , cp violation and t violation .
preliminary results from cleo - c now dominate the world average absolute branching... | I discuss new findings on how often charm mesons decay into specific particles, including rare decays and total decay rates to @xmath0 mesons. I also explore limits on @xmath1 mixing, CP violation, and T violation. Recent results from CLEO-C provide the best average measurements for these decays. For key normalization ... | true | 4.67 |
i discuss new results on absolute branching ratios of charm mesons into specific exclusive final states , cabibbo suppressed decay rates , inclusive decays to @xmath0 mesons , limits on @xmath1 mixing , cp violation and t violation .
preliminary results from cleo - c now dominate the world average absolute branching... | I present new results on how often charm mesons decay into specific particles, including rare decays, and measurements related to mixing and CP violation. Recent data from CLEO-C is now the standard for many decay rates. For key decay modes, CLEO-C measures rates of @xmath4 for @xmath5. Using this rate, I calculate a b... | false | 3.42 |
cut - sky orthogonal mode analyses of the @xmath0-dmr 53 and 90 ghz sky maps are used to determine the normalization of a variety of open cosmogonical models based on the cold dark matter scenario . to constrain the allowed cosmological - parameter range for these open cosmogonies , the predictions of the dmr - normal... | The open cosmology model considered in this study utilizes sky maps from the xmath0-dmr, xmath9-dmr and xmath15-dmr models to determine the normalization of a variety of open cosmogonical models based on the cold dark matter scenario. The predictions of these normalized models are compared to various observational meas... | false | 1.8 |
cut - sky orthogonal mode analyses of the @xmath0-dmr 53 and 90 ghz sky maps are used to determine the normalization of a variety of open cosmogonical models based on the cold dark matter scenario . to constrain the allowed cosmological - parameter range for these open cosmogonies , the predictions of the dmr - normal... | In this paper, we analyze sky orthogonal mode analyses of the @xmath0-dmr 53 and 90 ghz sky maps to determine the normalization of a variety of open cosmological models based on the cold dark matter scenario. The predictions of the dmr - normalized models are compared with various observational measures of cosmography ... | false | 3.29 |
cut - sky orthogonal mode analyses of the @xmath0-dmr 53 and 90 ghz sky maps are used to determine the normalization of a variety of open cosmogonical models based on the cold dark matter scenario . to constrain the allowed cosmological - parameter range for these open cosmogonies , the predictions of the dmr - normal... | The DMR (Diffuse Microwave Radiation) data is used to analyze various open cosmogonical models based on the cold dark matter scenario. These analyses help determine the normalization of these models and constrain their allowed parameter ranges using observational measurements, including estimates like the age of the un... | false | 3.13 |
we present a two - channel model to describe the quantum state of two atoms with finite - range interaction near a feshbach resonance .
this model provides a simple picture to analytically derive the wave function and the binding energy of the molecular bound state .
the results agree excellently with the measurem... | We propose a two-channel model to describe the quantum state of two atoms with finite-range interactions near a Feshbach resonance. This model helps us analytically determine the wave function and binding energy of the molecular bound state. Our results match well with experiments and multi-channel calculations. For sm... | true | 4.62 |
we present a two - channel model to describe the quantum state of two atoms with finite - range interaction near a feshbach resonance .
this model provides a simple picture to analytically derive the wave function and the binding energy of the molecular bound state .
the results agree excellently with the measurem... | We use a two-channel model to explain the quantum state of two atoms with limited interaction near a Feshbach resonance. This model helps us analytically find the wave function and binding energy of the molecular bound state. Our results match well with measurements and multi-channel calculations. For small binding ene... | true | 4.65 |
we present a two - channel model to describe the quantum state of two atoms with finite - range interaction near a feshbach resonance .
this model provides a simple picture to analytically derive the wave function and the binding energy of the molecular bound state .
the results agree excellently with the measurem... | We propose a two-channel model to explain the quantum state of two atoms interacting over a limited range near a Feshbach resonance. This model allows us to simply derive the wave function and binding energy of the molecular bound state. The results match well with experimental measurements and calculations using multi... | true | 4.6 |
large numbers of supernovae ( sne ) have been discovered in recent years , and many more will be found in the near future . once discovered , further study of a sn and its possible use as an astronomical tool ( e.g. , as a distance estimator ) require knowledge of the sn type .
current classification methods rely al... | Recently, many supernovae (SNe) have been discovered and more will be found soon. To use an SN as a tool for astronomical studies, such as determining distance, you need to know its type. Currently, classifying SNe relies mainly on analyzing their spectra, but this may not be feasible when SNe are faint, numerous, or f... | true | 4.59 |
large numbers of supernovae ( sne ) have been discovered in recent years , and many more will be found in the near future . once discovered , further study of a sn and its possible use as an astronomical tool ( e.g. , as a distance estimator ) require knowledge of the sn type .
current classification methods rely al... | Lots of supernovae (SNe) have been found recently, with even more expected soon. To study them further and use them as tools, like measuring distances, we need to know their types. Currently, classification mainly uses spectra analysis, but this isn't always feasible, especially when SNe are faint or numerous. We propo... | true | 4.57 |
large numbers of supernovae ( sne ) have been discovered in recent years , and many more will be found in the near future . once discovered , further study of a sn and its possible use as an astronomical tool ( e.g. , as a distance estimator ) require knowledge of the sn type .
current classification methods rely al... | We present a classification method for supernovae based on the comparison of their observed colors with synthetic ones, calculated from a large database of multi-epoch optical spectra of nearby events. | false | 3.41 |
large numbers of supernovae ( sne ) have been discovered in recent years , and many more will be found in the near future . once discovered , further study of a sn and its possible use as an astronomical tool ( e.g. , as a distance estimator ) require knowledge of the sn type .
current classification methods rely al... | In recent years, many supernovae (SNe) have been discovered, with more expected soon. To use these as tools for studying space, like measuring distances, we need to know their types. Traditionally, this is done by analyzing their spectra, but that's not always possible when SNe are faint or numerous. We propose a new m... | true | 4.55 |
large numbers of supernovae ( sne ) have been discovered in recent years , and many more will be found in the near future . once discovered , further study of a sn and its possible use as an astronomical tool ( e.g. , as a distance estimator ) require knowledge of the sn type .
current classification methods rely al... | Many supernovae (SNe) have been found recently, with more expected. To study them and use them as tools, we need to know their type. Currently, this is done by analyzing their spectra. However, spectroscopy isn't always possible or practical. We present a new method using colors of SNe compared to synthetic ones from n... | true | 4.74 |
large numbers of supernovae ( sne ) have been discovered in recent years , and many more will be found in the near future . once discovered , further study of a sn and its possible use as an astronomical tool ( e.g. , as a distance estimator ) require knowledge of the sn type .
current classification methods rely al... | Many supernovae (SNe) are being discovered, and more will be found soon. To study SNe and use them to measure distances, scientists need to know their type. Currently, SNe are classified by analyzing their spectra, but this isn't always possible, especially for faint or numerous SNe, or those found in old data.
We pr... | true | 4.59 |
large numbers of supernovae ( sne ) have been discovered in recent years , and many more will be found in the near future . once discovered , further study of a sn and its possible use as an astronomical tool ( e.g. , as a distance estimator ) require knowledge of the sn type .
current classification methods rely al... | Many supernovae have been found recently, and more will be discovered soon. To study them and use them as tools for measuring distances in space, we need to know their type. Currently, scientists classify supernovae mainly by analyzing their spectra. However, this method isn't always possible or practical when the supe... | true | 4.55 |
large numbers of supernovae ( sne ) have been discovered in recent years , and many more will be found in the near future . once discovered , further study of a sn and its possible use as an astronomical tool ( e.g. , as a distance estimator ) require knowledge of the sn type .
current classification methods rely al... | Many supernovae (SNe) have been discovered and more are likely to be found soon. To study them effectively, we need to classify SNe types based on their observed colors rather than just using spectra. We developed a method comparing SN colors with synthetic ones derived from nearby events' multi-epoch optical spectra. ... | true | 4.54 |
the general expression of the stern - gerlach force is deduced for a relativistic charged spin-@xmath0 particle which travels inside a time varying magnetic field .
this result was obtained either by means of two lorentz boosts or starting from dirac s equation .
then , the utilization of this interaction for atta... | the general expression of the stern - gerlach force for a relativistic charged spin-@xmath0 particle which travels inside a time varying magnetic field | false | 2.98 |
the general expression of the stern - gerlach force is deduced for a relativistic charged spin-@xmath0 particle which travels inside a time varying magnetic field .
this result was obtained either by means of two lorentz boosts or starting from dirac s equation .
then , the utilization of this interaction for atta... | The Stern-Gerlach force for a charged, spinning particle moving in a changing magnetic field can be found using two Lorentz boosts or from Dirac's equation. This interaction is then used to separate spin states in a new example with a radio-frequency setup. | true | 4.67 |
the general expression of the stern - gerlach force is deduced for a relativistic charged spin-@xmath0 particle which travels inside a time varying magnetic field .
this result was obtained either by means of two lorentz boosts or starting from dirac s equation .
then , the utilization of this interaction for atta... | The force on a charged spinning particle moving in a changing magnetic field is calculated using relativity. This calculation was done using either Lorentz boosts or Dirac's equation. This interaction can be used to separate spin states, as demonstrated with a new radio frequency setup. | true | 4.5 |
the general expression of the stern - gerlach force is deduced for a relativistic charged spin-@xmath0 particle which travels inside a time varying magnetic field .
this result was obtained either by means of two lorentz boosts or starting from dirac s equation .
then , the utilization of this interaction for atta... | This result was obtained using either two Lorentz boosts or Dirac's equation to analyze a relativistic charged spin-1 particle's behavior in a magnetic field that is changing over time. The interaction, which involves this force, is then considered for attaining spin states separation by reconsidering the utilization i... | false | 3.07 |
the general expression of the stern - gerlach force is deduced for a relativistic charged spin-@xmath0 particle which travels inside a time varying magnetic field .
this result was obtained either by means of two lorentz boosts or starting from dirac s equation .
then , the utilization of this interaction for atta... | A special way to understand how particles move through changing magnetic fields has been found. This helps us see differences in particle spins more easily. | false | 3.06 |
we calculate cross sections for low energy elastic exciton - exciton scattering within the effective mass approximation .
unlike previous theoretical approaches , we give a complete , non - perturbative treatment of the four - particle scattering problem .
diffusion monte carlo is used to calculate the essentially... | We calculate cross sections for low energy elastic exciton - exciton scattering within the effective mass approximation using diffusion Monte Carlo techniques. Unlike previous theoretical approaches, we provide a complete non-perturbative treatment of the four particle scattering problem by introducing diffusion monte ... | false | 3.14 |
we calculate cross sections for low energy elastic exciton - exciton scattering within the effective mass approximation .
unlike previous theoretical approaches , we give a complete , non - perturbative treatment of the four - particle scattering problem .
diffusion monte carlo is used to calculate the essentially... | We use a new method to calculate how excitons interact at low energy, focusing on full scattering without simplifications. We use a special computer simulation technique to get exact results for the energies and shapes of these interactions. For matching pairs (singlet and triplet excitons) we find distinct interaction... | false | 3.15 |
we present a novel method for calculating the primordial non - gaussianity produced by super - horizon evolution during inflation .
our method evolves the distribution of coarse - grained inflationary field values using a transport equation .
we present simple evolution equations for the moments of this distributi... | We present a novel method for calculating primordial non-gaussianity produced by super - horizon evolution during inflation. | false | 3.25 |
we present a novel method for calculating the primordial non - gaussianity produced by super - horizon evolution during inflation .
our method evolves the distribution of coarse - grained inflationary field values using a transport equation .
we present simple evolution equations for the moments of this distributi... | We introduce a new way to calculate primordial non-gaussianity caused by super-horizon evolution during inflation. This method uses a transport equation to track the distribution of coarse-grained field values in inflation. We provide simple equations for moments like variance and skewness. Our approach has advantages ... | true | 4.64 |
we present a novel method for calculating the primordial non - gaussianity produced by super - horizon evolution during inflation .
our method evolves the distribution of coarse - grained inflationary field values using a transport equation .
we present simple evolution equations for the moments of this distributi... | We developed a new method to calculate how much the early universe deviated from being perfectly uniform during a period of rapid expansion called inflation. Our method tracks the changes in the distribution of field values using a mathematical equation. We derived simple equations to calculate properties of this distr... | true | 4.61 |
we present a novel method for calculating the primordial non - gaussianity produced by super - horizon evolution during inflation .
our method evolves the distribution of coarse - grained inflationary field values using a transport equation .
we present simple evolution equations for the moments of this distributi... | We introduce a new method to calculate primordial non-Gaussianity created during inflation by super-horizon evolution. Our approach uses a transport equation to track how the distribution of inflationary field values changes over time. We provide simple equations to describe key features like variance and skewness. Thi... | true | 4.57 |
we present a novel method for calculating the primordial non - gaussianity produced by super - horizon evolution during inflation .
our method evolves the distribution of coarse - grained inflationary field values using a transport equation .
we present simple evolution equations for the moments of this distributi... | We've developed an innovative method to measure primordial non-Gaussianity during inflation, using fine-grained field values. We calculated moments like variance and skewness based on these values' movement patterns, which helps us understand the early universe better. | false | 2.63 |
for @xmath0 and @xmath1 , we consider certain admissible sequences of @xmath2 lattice paths in a colored @xmath3 square .
we show that the number of such admissible sequences of lattice paths is given by the sum of squares of the number of standard young tableaux of partitions of @xmath4 with height @xmath5 , which ... | the number of admissible sequences of lattice paths in a colored square whose sum is 10 | false | 2.34 |
for @xmath0 and @xmath1 , we consider certain admissible sequences of @xmath2 lattice paths in a colored @xmath3 square .
we show that the number of such admissible sequences of lattice paths is given by the sum of squares of the number of standard young tableaux of partitions of @xmath4 with height @xmath5 , which ... | For two variables xmath0 and xmath1, we look at certain sequences of lattice paths in a colored square. We find that the number of these sequences is equal to the sum of squares of the number of standard Young tableaux for partitions of xmath4 with height xmath5. This also equals the number of xmath6-avoiding permutati... | true | 4.69 |
various new physics models predict a light cp - odd higgs boson ( labeled as @xmath0 ) and open up new decay modes for @xmath1-boson , such as @xmath2 , @xmath3 and @xmath4 , which could be explored at the gigaz option of the ilc . in this work
we investigate these rare decays in several new physics models , namely ... | The predicted branching ratios for @xmath5 , @xmath6 , @xmath8 , @xmath9 are significantly larger than those from the other models, indicating that these rare decays at the gigaz might be accessible. | false | 1.92 |
various new physics models predict a light cp - odd higgs boson ( labeled as @xmath0 ) and open up new decay modes for @xmath1-boson , such as @xmath2 , @xmath3 and @xmath4 , which could be explored at the gigaz option of the ilc . in this work
we investigate these rare decays in several new physics models , namely ... | New physics models suggest a light CP-odd Higgs boson, which could lead to new decay modes for the Z-boson. These decays can be studied at the GigaZ option of the ILC. We examined these rare decays in several models: Type-II Two-Higgs Doublet Model, Lepton-Specific Two-Higgs DoubleT Model, Nearly Minimal Supersymmetric... | true | 4.57 |
various new physics models predict a light cp - odd higgs boson ( labeled as @xmath0 ) and open up new decay modes for @xmath1-boson , such as @xmath2 , @xmath3 and @xmath4 , which could be explored at the gigaz option of the ilc . in this work
we investigate these rare decays in several new physics models , namely ... | New physics models suggest a light CP-odd Higgs boson and new decay paths for the Z-boson, like Z→invisible particles and other rare decays. This study looks at these decays in four models: Type-II 2HDM, Lepton-Specific 2HDM, NMSSM, and nMSSM. Current data allows branching ratios as high as 1e-7 for Z→invisible + W- an... | true | 4.48 |
various new physics models predict a light cp - odd higgs boson ( labeled as @xmath0 ) and open up new decay modes for @xmath1-boson , such as @xmath2 , @xmath3 and @xmath4 , which could be explored at the gigaz option of the ilc . in this work
we investigate these rare decays in several new physics models , namely ... | Various new physics theories predict the existence of a light CP-odd Higgs boson, which offers new ways for another Higgs particle to decay, such as into particles like photons, Z bosons, and others. These decays could be studied in detail at the ILC's Gigaz facility.
In this study, we looked at these rare decays with... | true | 4.48 |
various new physics models predict a light cp - odd higgs boson ( labeled as @xmath0 ) and open up new decay modes for @xmath1-boson , such as @xmath2 , @xmath3 and @xmath4 , which could be explored at the gigaz option of the ilc . in this work
we investigate these rare decays in several new physics models , namely ... | Some new physics models predict light CP-odd Higgs bosons (labeled as @xmath0), opening up new decay modes for @xmath1-boson, such as @xmath2, @xmath3, and @xmath4. These decays may be explored at the GigaZ option of the ILC. In this work, the authors investigate these rare decays in several models including Type II 2H... | true | 4.64 |
a positive , non - saturating and dominantly linear magnetoresistance is demonstrated to occur in the surface state of a topological insulator having a wavevector - linear energy dispersion together with a finite positive zeeman energy splitting .
this linear magnetoresistance shows up within quite wide magnetic - f... | a positive, non-saturating, and dominantly linear magnetoresistance is demonstrated in the surface state of a topological insulator with a wavevector - linear energy dispersion and a finite positive zeeman energy splitting | false | 3.02 |
a positive , non - saturating and dominantly linear magnetoresistance is demonstrated to occur in the surface state of a topological insulator having a wavevector - linear energy dispersion together with a finite positive zeeman energy splitting .
this linear magnetoresistance shows up within quite wide magnetic - f... | A special type of magnetoresistance happens on the surface of certain materials called topological insulators. It is very strong and appears in a wide range of magnetic fields. | false | 3.31 |
dwarf galaxies in the local group provide a unique astrophysical laboratory . despite their proximity some of these systems still lack a reliable distance determination as well as studies of their stellar content and star formation history .
we present first results of our survey of variable stars in a sample of six... | Dwarf galaxies in the Local Group provide a unique astrophysical lab. Despite their proximity, some lack reliable distance measurements, as well as studies on their stellar content and star formation history. We present first results from our survey of variable stars in six dwarf irregular galaxies in the Local Group. ... | true | 4.78 |
dwarf galaxies in the local group provide a unique astrophysical laboratory . despite their proximity some of these systems still lack a reliable distance determination as well as studies of their stellar content and star formation history .
we present first results of our survey of variable stars in a sample of six... | dwarf galaxies in the local group provide a unique astrophysical laboratory despite their proximity some of these systems still lack a reliable distance determination as well as studies of their stellar content and star formation history. | false | 2.65 |
dwarf galaxies in the local group provide a unique astrophysical laboratory . despite their proximity some of these systems still lack a reliable distance determination as well as studies of their stellar content and star formation history .
we present first results of our survey of variable stars in a sample of six... | Dwarf galaxies in our local group are unique for studying astrophysics, but some lack accurate distance measurements and studies on their stars and star formation history. We studied variable stars in six dwarf irregular galaxies and used Leo A as an example to describe how we observed and processed data. We found two ... | true | 4.56 |
dwarf galaxies in the local group provide a unique astrophysical laboratory . despite their proximity some of these systems still lack a reliable distance determination as well as studies of their stellar content and star formation history .
we present first results of our survey of variable stars in a sample of six... | Nearby dwarf galaxies are useful for studying astronomy. Some of these galaxies lack good distance measurements and studies of their stars and star formation.
We studied variable stars in six nearby dwarf galaxies. Using the Leo A galaxy as an example, we describe how we observed and processed the data.
We discuss t... | true | 4.58 |
dwarf galaxies in the local group provide a unique astrophysical laboratory . despite their proximity some of these systems still lack a reliable distance determination as well as studies of their stellar content and star formation history .
we present first results of our survey of variable stars in a sample of six... | Dwarf galaxies in our cosmic neighborhood serve as unique labs for studying astrophysics. However, some of these nearby systems still don't have accurate distance measurements or detailed studies of their stars and star formation history. We report initial findings from a survey of variable stars in six small, irregula... | true | 4.79 |
dwarf galaxies in the local group provide a unique astrophysical laboratory . despite their proximity some of these systems still lack a reliable distance determination as well as studies of their stellar content and star formation history .
we present first results of our survey of variable stars in a sample of six... | The text talks about variable stars in dwarf irregular galaxies. It gives two examples of variable stars from Leo A Dwarf galaxy and discusses their placement within a previously derived p-L relation. The results of surveys are presented, but it's unclear if the survey was reliable or not. | false | 2.97 |
dwarf galaxies in the local group provide a unique astrophysical laboratory . despite their proximity some of these systems still lack a reliable distance determination as well as studies of their stellar content and star formation history .
we present first results of our survey of variable stars in a sample of six... | A survey of variable stars is conducted in nearby dwarf irregular galaxies to learn more about their star formation and history. | false | 2.62 |
the generation of hydrodynamic radiation in interactions of pulsed proton and laser beams with matter is explored .
the beams were directed into a water target and the resulting acoustic signals were recorded with pressure sensitive sensors .
measurements were performed with varying pulse energies , sensor positio... | Scientists studied how powerful proton and laser beams create sound waves in matter by shooting them into water and measuring the sound. They changed many factors like energy, sensor position, beam size, and temperature. The results match simulations from a thermo-acoustic model with a 10% uncertainty. This shows that ... | true | 4.55 |
the generation of hydrodynamic radiation in interactions of pulsed proton and laser beams with matter is explored .
the beams were directed into a water target and the resulting acoustic signals were recorded with pressure sensitive sensors .
measurements were performed with varying pulse energies , sensor positio... | The study investigates how pulsed proton and laser beams interact with matter, specifically generating hydrodynamic radiation. The beams were aimed at water targets, and the resulting acoustic signals were recorded using pressure sensors. Various factors like pulse energy, sensor placement, beam size, and temperature w... | true | 4.5 |
the generation of hydrodynamic radiation in interactions of pulsed proton and laser beams with matter is explored .
the beams were directed into a water target and the resulting acoustic signals were recorded with pressure sensitive sensors .
measurements were performed with varying pulse energies , sensor positio... | The generation of hydrodynamic radiation in interactions of pulsed proton and laser beams with matter is explored. | false | 3.03 |
the generation of hydrodynamic radiation in interactions of pulsed proton and laser beams with matter is explored .
the beams were directed into a water target and the resulting acoustic signals were recorded with pressure sensitive sensors .
measurements were performed with varying pulse energies , sensor positio... | The study explores how hydrodynamic radiation is created when pulsed proton and laser beams interact with matter. These beams were aimed at a water target, and the resulting sound waves were recorded using pressure sensors. Experiments varied pulse energy, sensor positions, beam sizes, and temperatures. The data matche... | true | 4.49 |
the generation of hydrodynamic radiation in interactions of pulsed proton and laser beams with matter is explored .
the beams were directed into a water target and the resulting acoustic signals were recorded with pressure sensitive sensors .
measurements were performed with varying pulse energies , sensor positio... | Researchers studied how pulsed proton and laser beams interact with water, generating sound waves. They measured acoustic signals from different pulse energies, sensor positions, beam sizes, and temperatures. The data matched simulations based on a thermo-acoustic model within a 10% uncertainty range. The main way thes... | true | 4.78 |
the generation of hydrodynamic radiation in interactions of pulsed proton and laser beams with matter is explored .
the beams were directed into a water target and the resulting acoustic signals were recorded with pressure sensitive sensors .
measurements were performed with varying pulse energies , sensor positio... | The study looks at how pulsed proton and laser beams interacting with matter create hydrodynamic radiation. The beams were aimed at a water target, and pressure sensors recorded the sound signals produced. Experiments varied pulse energy, sensor positions, beam size, and temperature. The data matches simulations using ... | true | 4.73 |
the generation of hydrodynamic radiation in interactions of pulsed proton and laser beams with matter is explored .
the beams were directed into a water target and the resulting acoustic signals were recorded with pressure sensitive sensors .
measurements were performed with varying pulse energies , sensor positio... | This study explores how sound is created when pulsed proton and laser beams interact with water. The beams were aimed into water, and the resulting sound signals were measured using sensors. Measurements were taken with different beam strengths, sensor locations, beam sizes, and water temperatures. The experimental dat... | true | 4.54 |
the wide field camera 3 ( wfc3 ) on the _ hubble space telescope _ ( _ hst _ ) enabled the search for the first galaxies observed at @xmath0 ( @xmath1 myr after the big bang ) . to continue quantifying the number density of the most luminous galaxies ( @xmath2 ) at the earliest epoch observable with _ hst
_ , we sea... | The WFC3 camera on the Hubble Space Telescope helped find the first galaxies seen about 400 million years after the Big Bang. To keep counting the most luminous galaxies in the earliest observable period, scientists searched through data from the BORG[z8] survey. They found six possible galaxies (f125w-dropouts) that f... | false | 3.43 |
the wide field camera 3 ( wfc3 ) on the _ hubble space telescope _ ( _ hst _ ) enabled the search for the first galaxies observed at @xmath0 ( @xmath1 myr after the big bang ) . to continue quantifying the number density of the most luminous galaxies ( @xmath2 ) at the earliest epoch observable with _ hst
_ , we sea... | The wfc3 camera on the hst (hst) enabled the search for the first galaxies observed at xmath0 (xmath1 myr after the big bang). To continue quantifying the number density of the most luminous galaxies f125w (f125w - dropouts) in archival data from the brightest reionizing galaxy survey borg[z8] originally designed for d... | false | 2.7 |
_ this paper presents invariants under gamma correction and similarity transformations .
the invariants are local features based on differentials which are implemented using derivatives of the gaussian .
the use of the proposed invariant representation is shown to yield improved correlation results in a template m... | this paper presents invariants under gamma correction and similarity transformations. | false | 2.99 |
we investigate the emergence of magnetic flux in the quiet sun at very small spatial scales , focusing on the magnetic connection between the photosphere and chromosphere .
the observational data consist of spectropolarimetric measurements and filtergrams taken with the hinode satellite and the dutch open telescope ... | The magnetic flux in the quiet sun at very small spatial scales, focusing on the magnetic connection between the photosphere and chromosphere, is observed as a significant fraction of new flux that appears in @xmath0-shaped loops. | false | 2.28 |
we apply the statefinder diagnostic to the torsion cosmology , in which an accounting for the accelerated universe is considered in term of a riemann - cartan geometry : dynamic scalar torsion .
we find that there are some typical characteristic of the evolution of statefinder parameters for the torsion cosmology th... | the statefinder diagnostic divides the torsion parameter @xmath0 into differential ranges | false | 2.16 |
we apply the statefinder diagnostic to the torsion cosmology , in which an accounting for the accelerated universe is considered in term of a riemann - cartan geometry : dynamic scalar torsion .
we find that there are some typical characteristic of the evolution of statefinder parameters for the torsion cosmology th... | We used a statefinder diagnostic to study torsion cosmology, which explains the accelerating universe using a special geometry with dynamic scalar torsion. We found that the evolution of statefinder parameters in torsion cosmology differs from other cosmological models. The statefinder diagnostic also relates to critic... | true | 4.6 |
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This repository contains the synthetic KTO dataset created in the our thesis Training Language Models on Synthetic Data for Scientific Text Simplification. It contains 61391 preferences together with the original abstract that was simplified, the scores we assigned for the simplification and if the simplification is desireable or not.
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