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language, and show how this natural color can be traced back from any deterministic parity automaton after two cheap and simple automaton transformations. The resulting *streamlined* automaton does not necessarily accept every word with its natural color, but it has a ‘co-run’, which is like a run, but can *once* move...
arxiv_0001219
equilibrium to be a valid assumption. Carbon ------ Our carbon model is similar to that of which in turn is based on observations of gas and ice in protoplanetary discs as well as ISM grain modelling. Throughout the entire disc, the carbon species are distributed as shown in table [tab:carbon]. The number abundances ...
arxiv_0001222
A thermodynamic framework for modelling membrane transporters ============================================================= Membrane transporters contribute to the regulation of the internal environment of cells by translocating substrates across cell membranes. Like all physical systems, the behaviour of membrane tran...
arxiv_0001225
the pulsars considered are obtained from gamma-ray light-curve modeling. Keeping in mind these results, we have taken the values which provide *χ*/*χ**f* ≤ 1 for the points of the plasma density profile. In fact, the values *χ*/*χ**f* > 1 may be quite realistic, since for the millisecond pulsars the assumption of a pu...
arxiv_0001233
Localising fast radio bursts and other transients using interferometric arrays ============================================================================== ### Received December, 2014; accepted February 2015 Introduction ============ In the past few years, a possible new population of sources emitting fast and bright...
arxiv_0001235
Boolean automata isolated cycles and tangential double-cycles dynamics ====================================================================== Abstract Our daily social and political life is more and more impacted by social networks. The functioning of our living bodies is deeply dependent on biological regulation netwo...
arxiv_0001236
the inverse of *U* is  − *U*, i.e., *U* ⊕ ( − *U*) = 0. 5. Associativity: (*W* ⊕ *V*) ⊕ *U* = *W* ⊕ (*V* ⊕ *U*). For most statements it is a matter of doing the algebra. For statement a), the function *g*(*V*)∣*V*∣ is a bijection of the interval [0, *C*) onto the nonnegative reals. ∣*U*∣, ∣*V*∣ < *C* ⇒ *g*(*U*)*U* + *...
arxiv_0001243
spatial distribution of intragroup light in both normal and compact groups, both on the observational and on the theoretical side. Theoretical studies give conflicting predictions on the fraction of the IGL component and of its variation with the group mass. Numerical simulations by predict a strong evolution of the ...
arxiv_0001246
Presupernova evolution of rotating solar metallicity stars in the mass range 13-120 $\rm M\_\odot~$and their explosive yields. ============================================================================================================================== We present the first set of a new generation of models of massive ...
arxiv_0001247
Insights Into the High-energy *γ*-ray Emission of Markarian 501 from Extensive Multifrequency Observations in the *Fermi* Era ============================================================================================================================= We report on the *γ*-ray activity of the blazar Mrk501 during the fi...
arxiv_0001250
On the Observable Shape of Black Hole Photon Rings ================================================== Motivated by the prospect of measuring a black hole photon ring, in previous work we explored the interferometric signature produced by a bright, narrow curve in the sky. Interferometric observations of such a curve me...
arxiv_0001253
, 26E10, 46F12, 52A20, 52B45. This research was supported by the ISRAEL SCIENCE FOUNDATION grant No. 1750/20.[↩](#fnref1) Quasianalyticity, uncertainty, and integral transforms on higher grassmannians ============================================================================== We investigate the support of a distr...
arxiv_0001256
Detailed Abundances for 28 Metal-poor Stars: Stellar Relics in the Milky Way ============================================================================ We present the results of an abundance analysis for a sample of stars with  − 4 < [Fe/H] <  − 2. The data were obtained with the HIRES spectrograph at Keck Observator...
arxiv_0001258
estimation of *θ*0, and are likely sensitive to the quality of this method; indeed, if the estimates of *f**i*\* are heavily biased due to poor first-stage estimation, it is unclear whether the corresponding moments will be sufficient for identification, let alone efficiency. By contrast, our method is guaranteed to b...
arxiv_0001260
Classifying character degree graphs with seven vertices ======================================================= [1](#fn1) We study here the graphs with seven vertices in an effort to classify which of them appear as the prime character degree graphs of finite solvable groups. This classification is complete for the dis...
arxiv_0001262
the difference between the number of left-handed quarks (*N**L*) and right-handed (*N**R*) quarks by an integer, (NL - NR) = Nf Q, [eq:Delta] where *N**f* is the number of flavors. Therefore the electric current along the strong enough magnetic field should be sensitive to the topological fluctuations of the gluon ens...
arxiv_0001263
Hierarchical Online Convex Optimization ======================================= We consider online convex optimization (OCO) over a heterogeneous network with communication delay, where multiple workers together with a master execute a sequence of decisions to minimize the accumulation of time-varying global costs. The...
arxiv_0001264
\begin{aligned} t=&-\frac{1}{2} \sqrt{4 \varrho\_1^2-1}+\frac{1}{\sqrt{3}} \log \left(\frac{\sqrt{4 \varrho\_1^2-1}+\sqrt{3}}{\sqrt{4 \varrho\_1^2-1}-\sqrt{3}}\right), \label{5\_38} \\ \vartheta\_1=&-\arctan \sqrt{4 \varrho\_1^2-1}+\frac{1}{\sqrt{3}} \log \left(\frac{\sqrt{4 \varrho\_1^2-1}+\sqrt{3}}{\sqrt{4 \varrho\...
arxiv_0001266
1.\end{aligned}$$ Similar to the proof of Lemma [lem:scal-suf-metric-d], we can cover the nodes in $\mathcal{L}(\pi\_{3\tilde{\Delta}\_ib,\tilde{v}})$ by a lattice animal *ξ* on L*K* of size $f(\tilde{\Delta}\_i):=K\max\{c+1,b\}\cdot 3\tilde{\Delta}\_i+3b\tilde{\Delta}\_i+1$ containing $(0,\bm{0})$. Thus, $Wei\big(\...
arxiv_0001273
b}$, and in the regions that warping or breaking takes place, $Q \gtrsim 10$. Thus, self–gravity is not important in our calculations. In order to present a large number of simulations in this work, we choose to use 3 × 105 particles in most of our following simulations. We found this number to provide sufficient reso...
arxiv_0001276
Automorphism groupoids in noncommutative projective geometry ============================================================ ### 21st April 2022 We address a natural question in noncommutative geometry, namely the rigidity observed in many examples, whereby noncommutative spaces (or equivalently their coordinate algebras)...
arxiv_0001284
On an exponential attractor for a class of PDEs with degenerate diffusion and chemotaxis ======================================================================================== In this article we deal with a class of strongly coupled parabolic systems that encompasses two different effects: degenerate diffusion and ch...
arxiv_0001285
An effective likelihood-free approximate computing method with statistical inferential guarantees ================================================================================================= Approximate Bayesian computing is a powerful likelihood-free method that has grown increasingly popular since early applicat...
arxiv_0001288
Entropy production in collisions of gravitational shock waves and of heavy ions =============================================================================== ### May 2008 Introduction and summary ======================== Relativistic heavy ion collisions produce a lot of entropy. Consider for example gold ions collid...
arxiv_0001291
P Lett.  **103** (2016) no.10, 624] [arXiv:1602.04188 [gr-qc]]. N. Yunes, K. Yagi and F. Pretorius, “Theoretical Physics Implications of the Binary Black-Hole Mergers GW150914 and GW151226,” Phys. Rev. D **94**, no. 8, 084002 (2016) [arXiv:1603.08955 [gr-qc]]. B. P. Abbott *et al.* [LIGO Scientific and Virgo and Fermi-...
arxiv_0001292
.44568781957963477) – (-2.719999898820538,-0.4540328576286198); (-2.719999898820538,-0.4540328576286198) – (-2.7099998991914247,-0.46264275832726964); (-2.7099998991914247,-0.46264275832726964) – (-2.6999998995623113,-0.4714960014093833); (-2.6999998995623113,-0.4714960014093833) – (-2.689999899933198,-0.48057045837957...
arxiv_0001296
intensively studied and is in many way the prototypical nova. With this close examination, GK Per was system in which four uncommon properties; nearly-periodic large-amplitude brightness oscillations during the transition stage, superluminal expanding light echoes, expanding gas shells, and dwarf nova eruptions, which...
arxiv_0001304
.85  ±  4.21 & 12.36  ±  5.12 & &... &... % Bulge & & 17.47  ±  6.79 & 22.33  ±  6.75 & 22.56  ±  8.31 & 34.28  ±  9.11 & &... &... ### Photometry As described in Section [sec:sample] and seen in the upper left panel of Fig. [galpics], NGC 2654 is a highly-inclined galaxy with a boxy/peanut-shaped bulge. We find th...
arxiv_0001306
Post-Newtonian corrections to Schrödinger equations in gravitational fields =========================================================================== In this paper we extend the WKB-like ‘non-relativistic’ expansion of the minimally coupled Klein–Gordon equationafter Kiefer and Singh, Lämmerzahl and Giulini and Groß...
arxiv_0001308
burg, S., Schwemmer, S., Shalchi, A., Skilton, J.L., Sol, H., Spangler, D., Stawarz, Ł., Steenkamp, R., Stegmann, C., Superina, G., Tam, P.H., Tavernet, J.-P., Terrier, R., Tibolla, O., van Eldik, C., Vasileiadis, G., Venter, C., Vialle, J.P., Vincent, P., Vivier, M., Völk, H.J., Volpe, F., Wagner, S.J., Ward, M., Zdzi...
arxiv_0001311
Radio Observations as an Extrasolar Planet Discovery and Characterization: Interior Structure and Habitability ============================================================================================================== Introduction ============ While the planet Jupiter has been known since antiquity, the serendipito...
arxiv_0001312
Sup: empiricalReUS] ---------------------------------------- It is also interesting to examine how the reproduction numbers have evolved in the US. This section presents estimates of R*e**t* for the US at the country and state levels. Figure [fig: USRe] presents the reported daily new cases (per 100, 000 people) and th...
arxiv_0001316
In this paper, we rigorously investigate the reduced density matrix (RDM) associated to the ideal Bose gas in harmonic traps. We present a method based on a sum-decomposition of the RDM allowing to treat not only the isotropic trap, but also general anisotropic traps. When focusing on the isotropic trap, the method is ...
arxiv_0001320
influence radius. This potentially leads us to underestimate the rate of orbital inspiral, since DF (and especially the stellar DF exerted by the bulge on the sMBH) can be of the same importance as the the loss cone scattering or viscous drag at separations where one mechanism transitions to another. If instead we too...
arxiv_0001325
grid cells intersect the pattern that we measure, i.e. the filamentary and wall networks. The number of intersecting grid cells gives the box count *N* at scale *l*. The method works by measuring the box counts at different scales and then investigating the dependence of *N* on *l*. In the case of a fractal there is a...
arxiv_0001330
Affective computing using speech and eye gaze: a review and bimodal system proposal for continuous affect prediction ==================================================================================================================== Speech has been a widely used modality in the field of affective computing. Recently h...
arxiv_0001334
, resulting in larger delays and energy consumption. If there is a constraint on the number of retransmissions, PSNR performance of multimedia transmission is affected by sensing errors. We have observed that improved sensing performance leads to better quality at reception. Less severe fading (i.e., larger *m*) is als...
arxiv_0001338
meal, thus (1) refers to the termination of an event. Contrast this with (2), where ‘finish’ instead combines with a noun phrase referring to a specific meal. The resulting sentence concerns the termination of an unspecified event involving ‘the meal’. Interestingly, the structure of (2), ]], does not include an event...
arxiv_0001339
Sparse Sequence-to-Sequence Models ================================== Sequence-to-sequence models are a powerful workhorse of NLP. Most variants employ a softmax transformation in both their attention mechanism and output layer, leading to dense alignments and strictly positive output probabilities. This density is was...
arxiv_0001348
Linearized supergravity with a dynamical preferred frame ======================================================== CERN-TH-2016-219 INR-TH-2016-038 Introduction and summary ======================== The possibility to modify the laws of gravity has been the subject of an intensive theoretical research during recent dec...
arxiv_0001349
–0.02) that we can reasonably reproduce the full set of observations. To summarise, after implementing detailed chemical evolution in the semi-analytic model of S08, we can now reproduce the mass–metallicity and mass–[*α*/Fe] relations for local early-type galaxies, provided we use a slightly flatter Chabrier IMF and a...
arxiv_0001352
Inelastic neutron scattering study and Hubbard model description of the antiferromagnetic tetrahedral molecule Ni4Mo12 ====================================================================================================================== ### Received: date / Revised version: date Introduction ============ In the recent...
arxiv_0001355
. 1 and UVOT Obs. 10 (filter M2), and OM Obs. 10 and UVOT Obs. 12 (filter W1). Using the OM SEDs of Obs. 1 and Obs. 10, we calculated the expected OM flux at the effective wavelengths of the UVOT M2 and W1 filters. Then by taking the ratio of the OM and UVOT fluxes, normalisation factors for the M2 and W1 filters of OM...
arxiv_0001358
A Finite Volume method for the simulation of elastoviscoplastic flows and its application to the lid-driven cavity case ======================================================================================================================= We propose a Finite Volume Method for the simulation of elastoviscoplastic flows...
arxiv_0001361
The Dispirited Case of Gauged *U*(1)*B* − *L* Dark Matter ========================================================= Introduction ============ The nature of the dark matter in the Universe and the origin of the tiny neutrino masses are two unsolved fundamental questions in particle physics. Small neutrino masses are nat...
arxiv_0001366
Mixed motives and Quotient stacks: Abelian varieties ==================================================== Introduction ============ In this paper, we investigate the structure of the motivic Galois group of mixed motives tensor-generated by an abelian variety. In our papers, and, we developed tannakian constructions f...
arxiv_0001367
Constructing a fully homomorphic encryption schemewith the Yoneda Lemma ======================================================================= This paper redefines the foundations of asymmetric cryptography’s homomorphic cryptosystems through the application of the Yoneda Lemma. It explicitly illustrates that widely a...
arxiv_0001369
 ( Cambridge University Press,  1998)   and   , @noop Phys. Rev. B **80**,  104432 ( 2009)  ,  ,  ,  ,  and   , @noop Phys. Rev. B  **43**,  14414 ( 1991)  ,  ,  ,  and  , @noop Phys. Rev. B **54**,  1610 ( 1996)  ,  ,  ,  ,  and   , @noop *Electronic Structure of Disordered Alloys, Surfaces and Interfaces...
arxiv_0001371
check, L., Janka, H.-T., Foglizzo, T., & Kifonidis, K. 2008, A&A, 477, 931, Scheck, L., Kifonidis, K., Janka, H.-T., & Müller, E. 2006, A&A, 457, 963, Sedov, L. I. 1959, Similarity and Dimensional Methods in Mechanics Sinnott, B., Welch, D. L., Rest, A., Sutherland, P. G., & Bergmann, M. 2013, ApJ, 767, 45, Spyromilio,...
arxiv_0001381
,0.000000)(25.294693,0.000000)(25.502596,0.000000)(25.710499,0.000000)(25.918401,0.000802)(26.126304,0.000000)(26.334207,0.000000)(26.542109,0.000000)(26.750012,0.000000)(26.957915,0.000000)(27.165817,0.000000)(27.373720,0.000000)(27.581623,0.000000)(27.789526,0.000000)(27.997428,0.000000)(28.205331,0.000000)(28.413234...
arxiv_0001383
Bounds on Rayleigh-Bénard convection with general thermal boundary conditions. Part 1. Fixed Biot number boundaries =================================================================================================================== We investigate the influence of the thermal properties of the boundaries in turbulent Ra...
arxiv_0001385
in the decoupling limit we have S &=& - $ \Gamma^{\omega}\mn \, S^{\mu \nu} $ &=&- $ \p^\omega \p\_\mu \p\_\nu \pi S^{\mu \nu} $ + … &=& - $\p^\omega \p\_\mu \pi S^{\mu \nu} $+(4-4)+…where in the last step we made use of the fact that the failure of conservation of *S**μ**ν* is a term only relevant at a higher s...
arxiv_0001387
it is conformal, albeit there are at least two other connected motivations. One is that this theory forms one side of the most known example of AdS/CFT correspondence, as it lives on the 4*d* Minkowski boundary of its gravitational *dual*, the type IIB superstring theory on *A**d**S*5 × *S*5. The second reason is that...
arxiv_0001390
possible; we will find that, in fact, all of them are redundant, leaving us with just L2 and L4 Horndeski terms. To do the field redefinitions we follow the strategy outlined in the bottom-up case: start by using metric redefinitions to remove curvature-only terms like *R*2, then use metric redefinitions again to elim...
arxiv_0001391
ergence  that is a *two-sided projective divergence*: *D**γ*[*λ**p* : *λ*ʹ*q*] = *D*[*p* : *q*] = *D*[*p̃* : *q̃*] for any *λ*, *λ*ʹ > 0 and converge to the KLD when *γ* → 0. However, the *γ*-divergence between a mixture model and an unnormalized PEF does not yield a closed-form formula. Moreover, the *γ*-divergence be...
arxiv_0001394
the compliance score has been discussed in the literature since at least and, we have not seen it used before for the specific purpose of predicting who the compliers are, nor have we seen any discussion of the error of this task. In contrast, most work seems to focus on the related but separate problem of estimating...
arxiv_0001397
3d we have 34 = 81. As a basis in ${\mathcal T}$, we can take tensor products of basis elements in *V*, *e**i*1 ⊗ *e**i*2 ⊗ ⋯ ⊗ *e**i**p* . Accordingly, an arbitrary contravariant tensor of rank *p* can be expressed as *T* = *T**i*1*i*2⋯*i**p* *e**i*1 ⊗ *e**i*2 ⊗ ⋯ ⊗ *e**i**p* . Under a transformation ([basis...
arxiv_0001407
Family-specific scaling laws in bacterial genomes. ================================================== Among several quantitative invariants found in evolutionary genomics, one of the most striking is the scaling of the overall abundance of proteins, or protein domains, sharing a specific functional annotation across ge...
arxiv_0001411
Observer-based Adaptive Optimal Output Containment Control problem of Linear Heterogeneous Multi-agent Systems with Relative Output Measurements ================================================================================================================================================ Introduction ============ Dist...
arxiv_0001412
Tauberian conditions, Muckenhoupt weights, and differentiation properties of weighted bases =========================================================================================== [1](#fn1) [2](#fn2) [3](#fn3) Let B be a homothecy invariant collection of convex sets in R*n*. Given a measure *μ*, the associated weig...
arxiv_0001418
1-loop Perturbative Corrections to the Matter and Galaxy Bispectrum with non-Gaussian Initial Conditions ======================================================================================================== We derive the expressions for the 1-loop corrections in cosmological, Eulerian, perturbation theory to the *ma...
arxiv_0001419
Expressibility-induced Concentration of Quantum Neural Tangent Kernels ======================================================================= Quantum tangent kernel methods provide an efficient approach to analyzing the performance of quantum machine learning models in the infinite-width limit, which is of crucial im...
arxiv_0001420
Deformation theory of deformed Hermitian Yang–Mills connections and deformed Donaldson–Thomas connections ========================================================================================================= [1](#fn1) A deformed Donaldson–Thomas (dDT) connection is a Hermitian connection of a Hermitian line bundle ...
arxiv_0001427
(1992) who determined a lag of about 80 days after 15 years of monitoring with a total of about 65 photometric measurements in the U and K bands and interpreted it as the response from a dusty torus. Glass (2004) reported a longer lag ( ∼ 190 days) but pointed out that the sampling of the new data were not good. He al...
arxiv_0001428
3 Å region, containing V I and Fe I lines, whose shapes, depths, and relative strengths are highly sensitive to effective temperature (Padgett et al. 1996). We find that the K5 template is a much better match to the RX J1633.9-2442 spectrum than the K7 template is and hence adopt this new and slightly revised spectral ...
arxiv_0001434
Modulation theory and resonant regimes for dispersive shock waves in nematic liquid crystals ============================================================================================ A full analysis of all regimes for optical dispersive shock wave (DSW) propagation in nematic liquid crystals is undertaken. These dis...
arxiv_0001440
**Solving Coupled Nonlinear Forward-backward Stochastic Differential Equations: An Optimization Perspective with Backward Measurability Loss[4](#fn4)** ======================================================================================================================================================= This paper aims ...
arxiv_0001443
above parameters in Eqs.([pulloff],[iondrag],[lebedev]) we end up with *F*po ∼ 102*F*idsc ∼ 103*F*idabs ∼ 103*F*E ∼ 106*F*g . It is apparent that the pull-off force is orders of magnitude larger than the plasma forces and gravity. Therefore, previous investigations of dust remobilization that neglected adhesion a...
arxiv_0001454
State and Control Path-Dependent Stochastic Zero-Sum Differential Games: Viscosity Solutions of Path-Dependent Hamilton-Jacobi-Isaacs Equations =============================================================================================================================================== Jun Moon\* (Communicated by the ...
arxiv_0001461
.8 & 5 & 1.9 ⋅ 10− 7 & 4.0 & 5.6 ⋅ 10− 6 & 3.9********** [H] [tab:advexamplegrid3] c||c||c|c||c|c order&**& **ℓ2 error & **conv. rate &**ℓ∞ error & **conv. rate 2 &0 & 2.6 ⋅ 10− 1 & — & 8.5 ⋅ 10− 1 & — &1 & 2.0 ⋅ 10− 1 & 0.4 & 7.0 ⋅ 10− 1 & 0.3 &2 & 1.3 ⋅ 10− 1 & 0.7 & 4.9 ⋅ 10− 1 & 0.5 &3 & 5.3 ⋅ 10− 2 & 1.3...
arxiv_0001472
the inclusions $\iota\_{\mathbb{H}}: {\mathbb{H}}\hookrightarrow {\mathbb{V}}$ and $\iota\_{\mathbb{G}}: {\mathbb{G}}\hookrightarrow {\mathbb{V}}$, and define the morphism R : H × G → V by ${\mathcal{R}}\coloneqq \iota\_{\mathbb{H}}+ \iota\_{\mathbb{G}}$. Thus we have that: $$\left( {\mathcal{R}}({\mathcal{H}}\mid ...
arxiv_0001475
Algorithmic Risk Assessments Can Alter Human Decision-Making Processes in High-Stakes Government Contexts ========================================================================================================= Governments are increasingly turning to algorithmic risk assessments when making important decisions, such a...
arxiv_0001482
* = 0), for a given value of density, as we move from *f**s* = 0 to *f**s* = 0.5, the energy of *D*− meson is observed to decrease by 10 (71) MeV from the value of 1842 (1708) MeV at *f**s*=0, at a density of *ρ*0 (4*ρ*0). The decrease in the energy of *D̄* mesons as a function of the strangeness fraction of the medium...
arxiv_0001485
1.0] (\x-0.3,0.7) rectangle (\x+0.3,1.3); \filldraw[fill=myblue!80, draw=myblue, line width=1.0] (-0.6,-0.1) rectangle (-0.8,1.1); \filldraw[fill=myblue!80, draw=myblue, line width=1.0] (0.6,-0.1) rectangle (0.8,1.1); \node[black] at (0,1.0) {$V\_{{\mathsf{k}}^{{\mathrm{w}}}}$}; \node[black] at (0,0) {$C$}; \node[myblu...
arxiv_0001487
ological Perturbations,” Phys. Rev. D **22**, 1882 (1980). V. F. Mukhanov, H. A. Feldman and R. H. Brandenberger, “Theory of cosmological perturbations. Part 1. Classical perturbations. Part 2. Quantum theory of perturbations. Part 3. Extensions,” Phys. Rept.  **215**, 203 (1992). R. H. Brandenberger, “Lectures on the ...
arxiv_0001489
paths have antecedent conditions for their activation. A small terminal developmental network -------------------------------------- Some normal developmental networks are terminal where all developmental paths result in terminal cells that no longer divide as seen in. [style=mystyle] (m) [matrix of math nodes, row se...
arxiv_0001498
Social reputations facilitate cooperation: those who help others gain a good reputation, making them more likely to receive help themselves. But when people hold private views of one another, this cycle of indirect reciprocity breaks down, as disagreements lead to the perception of unjustified behavior that ultimately ...
arxiv_0001500
mass and spin range accessible to the ringdown search when signals have *ε* = 1%, several sets of ringdown waveforms were injected with a uniform distribution in *M* and *â*: 50 ≤ *M*/M⊙ ≤ 900 and 0.0 ≤ *â* ≤ 0.99. Additionally, we also injected a set of full coalescence waveforms with isotropically-distributed sky ...
arxiv_0001504
= neg 2.4 sent(*S*,object) = neg  →  sent(*S*,badFor) = pos 3.1 sent(*S*,goodFor) = pos  →  sent(*S*,agent) = pos 3.2 sent(*S*,goodFor) = neg  →  sent(*S*,agent) = neg 3.3 sent(*S*,badFor) = pos  →  sent(*S*,agent) = pos 3.4 sent(*S*,badFor) = neg  →  sent(*S*,agent) = neg 4.1 sent(*S*,agent) = pos  ...
arxiv_0001510
to the intrinsic coordinates *y**a* = (*t*, *ɛ*) defines a set of basis vectors *e**a**α* on the submanifold, given by *e**t**α* = (*ω*, *ɛ*, 0) and *e**ɛ**α* = (∂*ɛ**ϕ*, *t*, 1). Because we are provided with sufficient boundary data for an ODE, rather than for a PDE, we must place some constraints on the function *F*...
arxiv_0001512
Representation Learning: A Review and New Perspectives ====================================================== The success of machine learning algorithms generally depends on data representation, and we hypothesize that this is because different representations can entangle and hide more or less the different explanator...
arxiv_0001516
splitting for our AGN 1. Thus, AGN with cos*θ* < 0.4 will not show double peaks. The range of polar angles for AGN 2 to show double peaks is then 45 to 66 degrees, giving ⟨cos*θ*⟩ = 0.55 and *w*1/*w*2 = 1.54. (2) In a rotating disk model with circular velocity *V*rot, the observed velocity splitting is *V* = *V*0sin*θ...
arxiv_0001520
**Matrix Completion Methods for Causal Panel Data Models [6](#fn6)** ==================================================================== In this paper we study methods for estimating causal effects in settings with panel data, where some units are exposed to a treatment during some periods and the goal is estimating c...
arxiv_0001522
lower than the values obtained in the hydrodynamic simulations. We thus restrict the dredge-up depth in our models to layers just above the He-free core of the CO WD (ranging from  ∼ 5.4% in the A-TP to  ∼ 15% in the E-AGB CO WD model, Table [hydromod]). ccccccccccccc 1 & 0.53 & 0.37 & E-AGB & 15.0 & 0.4505 & 0.0295 &...
arxiv_0001524
Marginal Interventional Effects[1](#fn1) ======================================== @path“C:/Users/Xiang Zhou/Dropbox/HeteroM/MIEZhou/” Conventional causal estimands, such as the average treatment effect (ATE), reflect how the mean outcome in a population or subpopulation would change if *all* units received treatment ve...
arxiv_0001527
Frequency shifts in the EPR spectrum of 39K due to spin-exchange collisions with polarized 3He and precise 3He polarimetry ========================================================================================================================== The Zeeman splittings and EPR frequencies of alkali-metal atoms are shifte...
arxiv_0001540
On Riemann zeroes, Lognormal Multiplicative Chaos, and Selberg Integral ======================================================================= Rescaled Mellin-type transforms of the exponential functional of the Bourgade-Kuan-Rodgers statistic of Riemann zeroes are conjecturally related to the distribution of the tota...
arxiv_0001548
] for a precise one. Given a subset *A* ⊂ *X* in a metric space *X*, we shall denote *A*+ *R* the *R*-neighbourhood of *A*, i.e. the set of points at distance at most *R* from *A*. [defIntro:coarseSep] Let *X* be a graph with bounded degree and let S be a family of subsets of *X*. We say that S *coarsely separates *X**...
arxiv_0001550
**Weyl’s search for a difference between ‘physical’ and ‘mathematical’ automorphisms** ====================================================================================== ### July 11, 2016 During his whole scientific life Hermann Weyl was fascinated by the interrelation of physical and mathematical theories. From th...
arxiv_0001553
The “non-regularizability” of gapless free fermion Hamiltonian protected by on-site symmetries ============================================================================================== The non-regularizability of free fermion field theories, which is the root of various quantum anomalies, plays a central role in p...
arxiv_0001562
Theory and Experiment for Wireless-Powered Sensor Networks: How to Keep Sensors Alive ===================================================================================== In this paper, we investigate a multi-node multi-antenna wireless-powered sensor networks (WPSN) comprised of one power beacon and multiple sensor n...
arxiv_0001563
DCrossing] We will start by defining the cube of resolutions for a negative crossing. Since there are *X* basepoints at *A*0 and *A*−, the intersection point *x* becomes special, as it induces a filtration on the complex. Let *X* denote the component of the knot Floer complex with generators containing the *x* intersec...
arxiv_0001573
Kohnert tableaux and a lifting ofquasi-Schur functions ====================================================== We introduce the quasi-key basis of the polynomial ring which contains the quasi-Schur polynomials of Haglund, Luoto, Mason and van Willigenburg. We prove that stable limits of quasi-key polynomials are quasi-S...
arxiv_0001584
Exclusion statistics for quantum Hall states in Tao-Thouless limit ================================================================== We consider spin-polarized abelian quantum Hall states in the Tao-Thouless limit, *ie* on a thin torus. For any filling factor *ν* = *p*/*q* a well-defined sector of low-energy states is...
arxiv_0001586
Z(3) metastable states in Polyakov Quark Meson model ==================================================== We study the existence of Z(3) metastable states in the presence of the dynamical quarks within the ambit of Polyakov quark meson (PQM) model. Within the parameters of the model, it is seen that for temperatures T*...
arxiv_0001593
calculated using analytical formulae and was plotted only to show what we aim to reproduce. The obtained final rotation curve exceeds the observed data by tens of km s− 1 in the inner  ∼ 3 kpc. This is due to the bar formation in this region, which affects the potential of the galaxy. In the outer parts, the simulated...
arxiv_0001596
Symmetric Bernoulli distributions and minimal dependence copulas ================================================================ The key result of this paper is to find all the joint distributions of random vectors whose sums *S* = *X*1 + … + *X**d* are minimal in convex order in the class of symmetric Bernoulli distr...
arxiv_0001597
Indecomposability parameters in chiral Logarithmic Conformal Field Theory ========================================================================= Work of the last few years has shown that the key algebraic features of Logarithmic Conformal Field Theories (LCFTs) are already present in some finite lattice systems (suc...
arxiv_0001600
next well-known lemma characterizes quasi-polynomials. appears in and. The following are equivalent: (a) *a*(*n*) is a quasi-polynomial of period *π* (b) the generating series $$G\_a(z)=\frac{P(z)}{Q(z)}$$ is a rational function where $P(z), Q(z) \in \BC[z]$, every zero $\a$ of *Q*(*z*) satisfies $\a^\pi=1$ (p...
arxiv_0001601
Linear polarization structures in LOFAR observations of the interstellar medium in the 3C196 field ================================================================================================== ### Received xxx / Accepted xxx We have used the high band antennas (HBA) of LOFAR to image this region and Rotation Measu...
arxiv_0001606