context_before stringlengths 0 199 | equation stringlengths 5 80 | context_after stringlengths 0 249 | spoken_English stringlengths 0 119 |
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$ \lambda_ { max } $ | , and | Lambda sub max. | |
99 | $ \pm $ | 0.15 & 1.00 | Plus or minus. |
and | $ \Gamma $ | on spheres , deforming the boundary action of | Gamma. |
settle and the similarity between features can be uniformly measured by | $ \phi ( \cdot , \cdot ) $ | . BN and ReLU are the batch normalization and ReLU activation layers . | phi of dot comma dot. |
and | $ c $ | becomes slightly larger . Therefore , the inter-layer coupling is more pronounced in the bulk. | c |
To understand | $ \sigma $ | intuitively , we first note that 1-minus each token 's unigram probability : | Sigma. |
and | $ j \in [ n ] $ | . Without loss of generality , we assume | j belongs to the set of integers from 1 to n. |
% for % some constant | $ c > 0 $ | depending only on | c greater than zero |
there exists | $ K \in \N $ | such that | K belongs to the set of natural numbers. |
The dominant instability at given | $ \mu $ | and | mu. |
_2 | $ ) $ | closing parenthesis | |
we see that the appearance of the peak at | $ k = 1 $ | precedes that of the flattening of the structure factor near the origin , and that there exists a range of temperatures for which the peak exists but the structure factor | k equals one. |
-norm of | $ x $ | , see | x |
where | $ \gamma_ { ry } =0 $ | indicates full discount and | gamma sub r y equals zero. |
surface states present AM because L | $ _1 $ | does not merge with L | One. |
as | $ x ' $ | . Based on how we have defined the partitions in | the derivative of x. |
if | $ V $ | satisfies the following conditions : | V |
For a given scenario | $ s\in \mathcal { S } $ | , the inequalities | s belongs to the set S. |
and | $ j $ | is determined by the shortest path between them . The efficiency is then defined as the inverse of the shortest path length : | j |
The top left panel shows the effect of changing | $ \Omega_m $ | . For low | Omega m. |
& | $ R_ { 8 } $ | & | R sub 8. |
since each of two cycles of | $ G $ | is in | G |
06 & 374 | $ \pm $ | 31 & -0.58 | Plus or minus. |
write | $ f = [ \phi ] _ { \wh M } $ | and | f equals the phi sub Q M. |
we design a process with a global autoregressive effect of order | $ p = 1 $ | . Also , the stage-1 neighbourhood is considered together with two exogenous regressors and corresponding time lags | p equals one. |
$ 1 $ | } & | one | |
fix a generator | $ h_i $ | of the cyclic subgroup | h sub i. |
plots the | $ u-r $ | color versus the stellar mass for NGC 7392 and for the latest sample of TDE candidates from the ZTF survey | u minus r. |
- | $ y $ | cross-section area , which leads to | y |
in | $ G $ | . | G |
$ F_2 $ | = | F sub 2. | |
em | $ f_\theta $ | transforms each element of the partition to | f sub theta |
belongs to | $ \bb_\eta $ | . | b sub eta |
we say that the odd girth of | $ G $ | is the length of the smallest odd cycle . If there are no odd cycles , we say that the odd girth is infinite . | G |
Let | $ R $ | be a monomial subring . Fix | R |
denote the total length of the hospitals ' preference lists in | $ J $ | . We claim that | J |
-constructible sheaves on | $ X $ | is denoted by | X |
fermions coupling to | $ H_1 $ | and | H sub 1. |
& | $ \frac32 \mathbf { k } \cdot \mathbf { k } ^\prime $ | & | Fraction 32 k dot k prime. |
The result shows a remarkably small dependence on the renormalization-scale parameter | $ X $ | ( see Fig.~ | X |
or | $ \pm $ | ~20 | Plus or minus. |
Observe that | $ e \in { \prod } _ { k \in l } { { 2 } ^ { \Pset ( k ) } } $ | and that for all | e belongs to the Cartesian product over k in l of 2 raised to the power of the P set of k. |
of | $ ( r_ { t } ) _ { t\in [ 0 , T ] } $ | is independent of | r sub t, sub t in the interval from 0 to T. |
& 2 & 2 & N & | $ ( 0,0 ) $ | & | zero comma zero. |
on | $ \hat { X } $ | , and | X hat. |
probability of | $ \fn $ | to obtain the | eff en |
For | $ N=1 $ | we have a | N equals one. |
to | $ \hat { P } ( i ) $ | , for | P hat of i |
~Peng | $ ^ { 71,58 } $ | , K.~Peters | to the power of seventy-one, fifty-eight. |
The MV model result is applied at the initial scale | $ Q_0 $ | =3 GeV . The gluon | Q zero. |
strong decays and branching ratios of | $ b\overline { b } $ | meson upto higher states with | b bar b |
the catalogue contains all of the brightest galaxies giving 90\ % of the total | $ B $ | -band and | B |
increases a bit to | $ 0.55\pi $ | . Now , when | 0.55 times pi. |
and | $ g_i $ | denotes an | g sub i. |
small than | $ \min\ { \epsilon_D,1\ } /10 $ | , where | Minimum of epsilon sub D, 1 divided by 10. |
Let | $ Z_0=\cL_y^ { max } ( \F^h ) \subset X $ | be the fiber at the central point | Z sub zero equals c times L sub y to the power of max times F to the power of h, subset X. |
by less than | $ 20\ % $ | . This is a trivial consequence of the fact that for large values of | Twenty percent. |
$ ^\textrm { \scriptsize 62b } $ | , | 62b | |
This type of modified theories are usually known as | $ f ( R ) $ | theories , and there exists a vast literature on these theories , for which a review on them is beyond our scope . Nevertheless , a construction of such theories | f of R |
These traveling waves are `` running '' in the positive or negative | $ x $ | -direction depending on the sign of | x |
V | $ } , which is obtained from $ | D | where there exists a variable from. |
and | $ \Omega_ { \Lambda } $ | is the dark energy density parameter , i.e . , the parameters of the standard | Omega sub Lambda. |
that | $ e_i $ | is an edge of | e sub i. |
for | $ n = 1 , 2 , \dots $ | , then | n equals one, two, ellipsis. |
color temperature | $ T_ { \rm C } $ | through the Wouthuysen†“ Field coupling | T sub C. |
has a definite value or magnitude at some initial time | $ 0 $ | . Then the subject system must be in a specific configuration with probability | zero |
on | $ \Sigma $ | is a finite collection | Sigma. |
It must be noted that the CPR might change if | $ P $ | is too high due to non-equilibrium effects~ | P |
& | $ \checkmark $ | & | Checkmark. |
is | $ \Pi_1 $ | -conservative over | Pi sub 1. |
updates | $ G $ | whenever the rule in ( 1 ) is satisfied by the temporal pattern of events , i.e . , | G |
top anion layer with the same concentration | $ x $ | as in the underlying | x |
-covered by the set | $ \calB_1 $ | , i.e . , | B sub 1. |
& | $ 0 $ | & | zero |
The following lemma shows we can solve for | $ F $ | in the above equation , with high probability . | F |
of | $ q $ | nodes are leaders , and the remaining | q |
be the tangent vector at | $ x_0 $ | to the unit speed geodesic | x sub zero. |
and | $ p^ { n+1 } $ | as follows : | p to the power of n plus 1. |
since it is impossible for more than | $ s $ | candidates to have more than this number of votes ) . | s |
If | $ \vecF_0 $ | is an | vector F sub zero. |
$ F $ | is a finite extension of | F | |
$ \zeta_l $ | is the 1d FI parameter associated with | zeta sub l. | |
and | $ b $ | are both dimensionless constants . In particular , | b |
we can observe this by measuring the | $ L^ { \infty } $ | and | L to the power of infinity. |
where each % | $ \beta_i $ | is an SCS of | Beta sub i. |
Thus it suffices to show that if | $ C $ | is any connected component of | C |
be the vertex of | $ C_j $ | which is adjacent to both | C sub j. |
& | $ 0 $ | & | zero |
The goal of the agent is then to find an optimal policy | $ \pi^ * $ | satisfying | pi star. |
Let the trial data | $ Y $ | with the fill distance | Y |
$ \bm { \beta } ^ * $ | denoting | beta star. | |
where | $ e_ { ij } $ | are the | e sub i j. |
-invariant | $ 1 $ | -form ( or even a contact form ) , but this is clearly in error . Lutz also discusses the classification up to equivariant diffeomorphism . | one |
:326 | $ - $ | 31 . % | minus |
-class estimators that takes | $ ( \tilde { y } , \tilde { X } , \tilde { Z } ) $ | is proportional to | Open parenthesis, tilde y, comma, tilde X, comma, tilde Z, close parenthesis. |
The degrees of | $ G $ | are then | G |
the evaluation of significance of LSP peaks | $ - $ | commonly called False Alarm Probabilities | minus |
We have assumed each orbital is in the Fermi liquid state with a bandwidth governed by | $ \rho_r $ | . Therefore , doing the integral and replacing | rho sub r. |
We crawl over | $ 20 $ | k timelines and collect over | Twenty. |
Of another interesting point is that we found the range of critical polarization values for the appearance of vortices in the momentum spectra for different cycles with | $ \Delta\phi=0 $ | and | Delta phi equals zero. |
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