id float64 706 1.8k | title stringlengths 1 343 | abstract stringlengths 6 6.09k | categories stringlengths 5 125 | processed_abstract stringlengths 2 5.96k | tokenized_abstract stringlengths 8 8.74k | centroid stringlengths 2.1k 2.17k |
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1,801.01469 | PHOENICS: A universal deep Bayesian optimizer | In this work we introduce PHOENICS, a probabilistic global optimization
algorithm combining ideas from Bayesian optimization with concepts from
Bayesian kernel density estimation. We propose an inexpensive acquisition
function balancing the explorative and exploitative behavior of the algorithm.
This acquisition func... | stat.ML physics.chem-ph | in this work we introduce phoenics a probabilistic global optimization algorithm combining ideas from bayesian optimization with concepts from bayesian kernel density estimation we propose an inexpensive acquisition function balancing the explorative and exploitative behavior of the algorithm this acquisition function ... | [['in', 'this', 'work', 'we', 'introduce', 'phoenics', 'a', 'probabilistic', 'global', 'optimization', 'algorithm', 'combining', 'ideas', 'from', 'bayesian', 'optimization', 'with', 'concepts', 'from', 'bayesian', 'kernel', 'density', 'estimation', 'we', 'propose', 'an', 'inexpensive', 'acquisition', 'function', 'balan... | [-0.06893374345341474, -0.007540839373257813, -0.10705113614090783, 0.09028697340403619, -0.10355271171755011, -0.15221001415179586, 0.07755566056401897, 0.43309698556110543, -0.2698809016121071, -0.28675776868824315, 0.06844508202685008, -0.20739478559918562, -0.23285181521359902, 0.19002009278936488, -0.0771108814251... |
1,801.0147 | A comparative study of aqueous DMSO mixtures by computer simulations and
integral equation theories | Several computer simulation studies of aqueous dimethylsulfoxyde with
different force field models, and conducted by different authors, point out to
an anomalous depressing of second and third neighbour correlations of the
water-water radial distribution functions. This seemingly universal feature can
be interpreted ... | physics.chem-ph | several computer simulation studies of aqueous dimethylsulfoxyde with different force field models and conducted by different authors point out to an anomalous depressing of second and third neighbour correlations of the waterwater radial distribution functions this seemingly universal feature can be interpreted as the... | [['several', 'computer', 'simulation', 'studies', 'of', 'aqueous', 'dimethylsulfoxyde', 'with', 'different', 'force', 'field', 'models', 'and', 'conducted', 'by', 'different', 'authors', 'point', 'out', 'to', 'an', 'anomalous', 'depressing', 'of', 'second', 'and', 'third', 'neighbour', 'correlations', 'of', 'the', 'wat... | [-0.06484789964603956, 0.09060369200629631, -0.10590306074539227, 0.1241075315481441, -0.06377510497617576, -0.11816610658277216, 0.006624799405933538, 0.4083419045113694, -0.2590180408320765, -0.32522783049646375, 0.03781989624605639, -0.2804460631850273, -0.15190136168476145, 0.15431941619643302, 0.001731471526923019... |
1,801.01471 | Potentiality, Actuality and Non-Separability in Quantum and Classical
Physics: Res Potentiae in the Macroscopic World | To help resolve stubborn aporias in quantum mechanics, Kastner, Kauffman and
Epperson have recently proposed a new interpretation of Heisenbergs ontological
duality of res extensa and res potentia. In related work, Khrennikov and Aerts
and their respective associates have explored the intermediate domain of
mesoscopi... | physics.hist-ph quant-ph | to help resolve stubborn aporias in quantum mechanics kastner kauffman and epperson have recently proposed a new interpretation of heisenbergs ontological duality of res extensa and res potentia in related work khrennikov and aerts and their respective associates have explored the intermediate domain of mesoscopic phen... | [['to', 'help', 'resolve', 'stubborn', 'aporias', 'in', 'quantum', 'mechanics', 'kastner', 'kauffman', 'and', 'epperson', 'have', 'recently', 'proposed', 'a', 'new', 'interpretation', 'of', 'heisenbergs', 'ontological', 'duality', 'of', 'res', 'extensa', 'and', 'res', 'potentia', 'in', 'related', 'work', 'khrennikov', ... | [-0.08554012068541339, 0.12507450385974386, -0.1217787864525468, 0.11047830639066748, -0.11750294472902822, -0.1564047777404388, 0.04246126542924545, 0.2867783967238397, -0.2688747978902076, -0.3132143822850851, 0.04508311012782192, -0.22546427193297766, -0.18081952190289322, 0.16128462007961786, -0.12857965427713516, ... |
1,801.01472 | Chiral-partner D mesons in a heat bath within QCD sum rules | Utilizing QCD sum rules, we extract the temperature dependences of the
spectral properties of the pseudo-scalar and scalar D mesons regarded as chiral
partners. Besides the masses also decay constants are analyzed as the D meson
yields in heavy-ion collisions may be sensitive to their altered decay
properties in an a... | nucl-th | utilizing qcd sum rules we extract the temperature dependences of the spectral properties of the pseudoscalar and scalar d mesons regarded as chiral partners besides the masses also decay constants are analyzed as the d meson yields in heavyion collisions may be sensitive to their altered decay properties in an ambient... | [['utilizing', 'qcd', 'sum', 'rules', 'we', 'extract', 'the', 'temperature', 'dependences', 'of', 'the', 'spectral', 'properties', 'of', 'the', 'pseudoscalar', 'and', 'scalar', 'd', 'mesons', 'regarded', 'as', 'chiral', 'partners', 'besides', 'the', 'masses', 'also', 'decay', 'constants', 'are', 'analyzed', 'as', 'the'... | [-0.09882953316785315, 0.30648101662895727, -0.06912766649376278, 0.08479609249381026, -0.08512082291812992, -0.16535283379360205, 0.057226530976168075, 0.32639213018590024, -0.2172432471609985, -0.20163901770533418, 0.000881795491879507, -0.32023460127666226, -0.010071814223336355, 0.085098344011284, 0.112712173398264... |
1,801.01473 | Portable multi-node LQCD Monte Carlo simulations using OpenACC | This paper describes a state-of-the-art parallel Lattice QCD Monte Carlo code
for staggered fermions, purposely designed to be portable across different
computer architectures, including GPUs and commodity CPUs. Portability is
achieved using the OpenACC parallel programming model, used to develop a code
that can be c... | hep-lat physics.comp-ph | this paper describes a stateoftheart parallel lattice qcd monte carlo code for staggered fermions purposely designed to be portable across different computer architectures including gpus and commodity cpus portability is achieved using the openacc parallel programming model used to develop a code that can be compiled f... | [['this', 'paper', 'describes', 'a', 'stateoftheart', 'parallel', 'lattice', 'qcd', 'monte', 'carlo', 'code', 'for', 'staggered', 'fermions', 'purposely', 'designed', 'to', 'be', 'portable', 'across', 'different', 'computer', 'architectures', 'including', 'gpus', 'and', 'commodity', 'cpus', 'portability', 'is', 'achiev... | [-0.11819143280188334, 0.02302613653420635, -0.06053233173545724, 0.044394502946114, -0.10355968829518293, -0.19339751777271671, 0.06877542989883188, 0.45618219522978454, -0.2725558796390781, -0.371428110766882, 0.0885043269235586, -0.2369898935601882, -0.09844834772144061, 0.24581969723701202, -0.06468084187808391, 0.... |
1,801.01474 | Galactic Effects on Habitability | The galactic environment has been suspected to influence planetary
habitability in many ways. Very metal-poor regions of the Galaxy, or those
largely devoid of atoms more massive than H and He, are thought to be unable to
form habitable planets. Moreover, if such planets do form, the young system is
subjected to clos... | astro-ph.EP astro-ph.GA astro-ph.SR | the galactic environment has been suspected to influence planetary habitability in many ways very metalpoor regions of the galaxy or those largely devoid of atoms more massive than h and he are thought to be unable to form habitable planets moreover if such planets do form the young system is subjected to close stellar... | [['the', 'galactic', 'environment', 'has', 'been', 'suspected', 'to', 'influence', 'planetary', 'habitability', 'in', 'many', 'ways', 'very', 'metalpoor', 'regions', 'of', 'the', 'galaxy', 'or', 'those', 'largely', 'devoid', 'of', 'atoms', 'more', 'massive', 'than', 'h', 'and', 'he', 'are', 'thought', 'to', 'be', 'unab... | [-0.09315384483913798, 0.19119500039990261, -0.04620116638800584, 0.13871399237561485, -0.15989432424743727, -0.06468174331485457, 0.06862085726499378, 0.38015780226676327, -0.16399755538241215, -0.3264333470772529, 0.05758532520289184, -0.2955917605003694, -0.09924385262992476, 0.2334808781875067, -0.10397213436464124... |
1,801.01475 | Generalization of Taylor's formula to particles of arbitrary inertia | One of the cornerstones of turbulent dispersion is the celebrated Taylor
formula. This formula expresses the rate of transport (i.e. the eddy
diffusivity) of a tracer as a time integral of the fluid velocity
auto-correlation function evaluated along the fluid trajectories. Here, we
review the hypotheses which permit ... | physics.flu-dyn | one of the cornerstones of turbulent dispersion is the celebrated taylor formula this formula expresses the rate of transport ie the eddy diffusivity of a tracer as a time integral of the fluid velocity autocorrelation function evaluated along the fluid trajectories here we review the hypotheses which permit to extend ... | [['one', 'of', 'the', 'cornerstones', 'of', 'turbulent', 'dispersion', 'is', 'the', 'celebrated', 'taylor', 'formula', 'this', 'formula', 'expresses', 'the', 'rate', 'of', 'transport', 'ie', 'the', 'eddy', 'diffusivity', 'of', 'a', 'tracer', 'as', 'a', 'time', 'integral', 'of', 'the', 'fluid', 'velocity', 'autocorrelat... | [-0.12334498864598573, 0.14556330191902817, -0.14863888756372035, 0.08408895525615662, -0.0465967190079391, -0.07912689421034884, -0.02539001022465527, 0.24449829913675786, -0.26912805999862033, -0.2875362787023187, 0.053872917302651334, -0.21619951099157333, -0.09612826665863394, 0.2090516807255335, -0.022691936591872... |
1,801.01476 | $N^\ast$ Form Factors based on a Covariant Quark Model | We discuss the results of the covariant spectator quark model for the several
$\gamma^\ast N \to N^\ast$ transitions, where $N$ is the nucleon and $N^\ast$ a
nucleon excitation. More specifically, we present predictions for the form
factors and transition amplitudes associated with the resonances
$N(1440)1/2^+$, $N(1... | hep-ph hep-ex hep-lat nucl-ex nucl-th | we discuss the results of the covariant spectator quark model for the several gammaast n to nast transitions where n is the nucleon and nast a nucleon excitation more specifically we present predictions for the form factors and transition amplitudes associated with the resonances n144012 n153512 n152032 delta162012 and... | [['we', 'discuss', 'the', 'results', 'of', 'the', 'covariant', 'spectator', 'quark', 'model', 'for', 'the', 'several', 'gammaast', 'n', 'to', 'nast', 'transitions', 'where', 'n', 'is', 'the', 'nucleon', 'and', 'nast', 'a', 'nucleon', 'excitation', 'more', 'specifically', 'we', 'present', 'predictions', 'for', 'the', 'f... | [-0.08825403251518894, 0.2219845227271246, -0.036854350346733226, 0.09223477546406861, -0.031191588925234007, -0.05995602014190336, 0.060775395705025985, 0.3435643089620711, -0.12961074002631395, -0.2631633933860349, -0.022308266439698878, -0.3428135332076919, -0.06125042057299817, 0.13343295599515367, 0.07254250763685... |
1,801.01477 | Double-Trace Deformations of Conformal Correlations | Large $N$ conformal field theories often admit unitary renormalization group
flows triggered by double-trace deformations. We compute the change in scalar
four-point functions under double-trace flow, to leading order in $1/N$. This
has a simple dual in AdS, where the flow is implemented by a change of boundary
condi... | hep-th | large n conformal field theories often admit unitary renormalization group flows triggered by doubletrace deformations we compute the change in scalar fourpoint functions under doubletrace flow to leading order in 1n this has a simple dual in ads where the flow is implemented by a change of boundary conditions and prov... | [['large', 'n', 'conformal', 'field', 'theories', 'often', 'admit', 'unitary', 'renormalization', 'group', 'flows', 'triggered', 'by', 'doubletrace', 'deformations', 'we', 'compute', 'the', 'change', 'in', 'scalar', 'fourpoint', 'functions', 'under', 'doubletrace', 'flow', 'to', 'leading', 'order', 'in', '1n', 'this', ... | [-0.19860857285969302, 0.21942855181600238, -0.07452615338522907, 0.03933834531472637, -0.0829715842633175, -0.11914437573078439, -0.06612886543548026, 0.31092294618282296, -0.18845146031272725, -0.19178838382791216, 0.11072882298068272, -0.27652508073375315, -0.19454844571957622, 0.1065436260894351, -0.033999720109848... |
1,801.01478 | Infrared photometry of the dwarf nova V2051 Ophiuchi: I - The mass donor
star and the distance | We report the analysis of time-series of infrared $JHK_s$ photometry of the
dwarf nova V2051 Oph in quiescence. We modelled the ellipsoidal variations
caused by the distorted mass-donor star to infer its $JHK_s$ fluxes. From its
infrared colors we estimate a spectral type of $M(8.0\pm 1.5)$ and an
equivalent blackbod... | astro-ph.SR | we report the analysis of timeseries of infrared jhk_s photometry of the dwarf nova v2051 oph in quiescence we modelled the ellipsoidal variations caused by the distorted massdonor star to infer its jhk_s fluxes from its infrared colors we estimate a spectral type of m80pm 15 and an equivalent blackbody temperature of ... | [['we', 'report', 'the', 'analysis', 'of', 'timeseries', 'of', 'infrared', 'jhk_s', 'photometry', 'of', 'the', 'dwarf', 'nova', 'v2051', 'oph', 'in', 'quiescence', 'we', 'modelled', 'the', 'ellipsoidal', 'variations', 'caused', 'by', 'the', 'distorted', 'massdonor', 'star', 'to', 'infer', 'its', 'jhk_s', 'fluxes', 'fro... | [-0.0495477372099197, 0.07479442312412882, -0.13334330478553763, 0.11326079297146795, -0.13296753294653846, -0.1046181448047584, 0.12412117995942633, 0.4437331072641192, -0.20085198180405078, -0.3131361963201521, 0.08650065950523303, -0.30678134970366955, -0.06397837706619477, 0.19436592178923698, -0.15466622064424748,... |
1,801.01479 | Black Holes as Quantum Gravity Condensates | We model spherically symmetric black holes within the group field theory
formalism for quantum gravity via generalised condensate states, involving sums
over arbitrarily refined graphs (dual to 3d triangulations). The construction
relies heavily on both the combinatorial tools of random tensor models and the
quantum ... | gr-qc hep-th | we model spherically symmetric black holes within the group field theory formalism for quantum gravity via generalised condensate states involving sums over arbitrarily refined graphs dual to 3d triangulations the construction relies heavily on both the combinatorial tools of random tensor models and the quantum geomet... | [['we', 'model', 'spherically', 'symmetric', 'black', 'holes', 'within', 'the', 'group', 'field', 'theory', 'formalism', 'for', 'quantum', 'gravity', 'via', 'generalised', 'condensate', 'states', 'involving', 'sums', 'over', 'arbitrarily', 'refined', 'graphs', 'dual', 'to', '3d', 'triangulations', 'the', 'construction'... | [-0.11665138906612287, 0.13277326488274743, -0.130153119878025, 0.0838545963184019, -0.07402928127857829, -0.1501850621795959, 0.033742917957362915, 0.26398655753864936, -0.24985851677642626, -0.28181703006284253, 0.08974485692681011, -0.270680620998257, -0.12812842050510825, 0.1751616675826495, -0.07329086130917087, 0... |
1,801.0148 | Matching factorization theorems with an inverse-error weighting | We propose a new fast method to match factorization theorems applicable in
different kinematical regions, such as the transverse-momentum-dependent and
the collinear factorization theorems in Quantum Chromodynamics. At variance
with well-known approaches relying on their simple addition and subsequent
subtraction of ... | hep-ph | we propose a new fast method to match factorization theorems applicable in different kinematical regions such as the transversemomentumdependent and the collinear factorization theorems in quantum chromodynamics at variance with wellknown approaches relying on their simple addition and subsequent subtraction of doublec... | [['we', 'propose', 'a', 'new', 'fast', 'method', 'to', 'match', 'factorization', 'theorems', 'applicable', 'in', 'different', 'kinematical', 'regions', 'such', 'as', 'the', 'transversemomentumdependent', 'and', 'the', 'collinear', 'factorization', 'theorems', 'in', 'quantum', 'chromodynamics', 'at', 'variance', 'with',... | [-0.021038072544880295, 0.07428864845678618, -0.1519616859890944, 0.13403902563335246, -0.09047447302013593, -0.10777729332105744, 0.03277273746789433, 0.38797722639389, -0.23653204190354285, -0.2667268742278049, 0.05005483165785501, -0.3014201336258008, -0.009092845370932164, 0.21111527225267226, -0.04385597755158828,... |
1,801.01481 | A Projected Estimate of the Reionization Optical Depth Using the CLASS
Experiment's Sample-Variance Limited E-Mode Measurement | We analyze simulated maps of the Cosmology Large Angular Scale Surveyor
(CLASS) experiment and recover a nearly cosmic-variance limited estimate of the
reionization optical depth $\tau$. We use a power spectrum-based likelihood to
simultaneously clean foregrounds and estimate cosmological parameters in
multipole spac... | astro-ph.CO | we analyze simulated maps of the cosmology large angular scale surveyor class experiment and recover a nearly cosmicvariance limited estimate of the reionization optical depth tau we use a power spectrumbased likelihood to simultaneously clean foregrounds and estimate cosmological parameters in multipole space using so... | [['we', 'analyze', 'simulated', 'maps', 'of', 'the', 'cosmology', 'large', 'angular', 'scale', 'surveyor', 'class', 'experiment', 'and', 'recover', 'a', 'nearly', 'cosmicvariance', 'limited', 'estimate', 'of', 'the', 'reionization', 'optical', 'depth', 'tau', 'we', 'use', 'a', 'power', 'spectrumbased', 'likelihood', 't... | [-0.10592471423830527, 0.11303340558273096, -0.04536807254965727, 0.12123491916960726, -0.07461634912760928, -0.08542254055500961, -0.0036731676150035734, 0.3275120531829695, -0.23876276930483678, -0.3281334255201121, 0.07715563729288988, -0.2775952434206071, -0.041130146236294726, 0.20247551162416735, 0.03288366242195... |
1,801.01482 | Finite semilattices with many congruences | For an integer $n\geq 2$, let NCSL$(n)$ denote the set of sizes of congruence
lattices of $n$-element semilattices. We find the four largest numbers
belonging to NCSL$(n)$, provided that $n$ is large enough to ensure that
$|$NCSL$(n)|\geq 4$. Furthermore, we describe the $n$-element semilattices
witnessing these numb... | math.RA math.CO | for an integer ngeq 2 let ncsln denote the set of sizes of congruence lattices of nelement semilattices we find the four largest numbers belonging to ncsln provided that n is large enough to ensure that ncslngeq 4 furthermore we describe the nelement semilattices witnessing these numbers | [['for', 'an', 'integer', 'ngeq', '2', 'let', 'ncsln', 'denote', 'the', 'set', 'of', 'sizes', 'of', 'congruence', 'lattices', 'of', 'nelement', 'semilattices', 'we', 'find', 'the', 'four', 'largest', 'numbers', 'belonging', 'to', 'ncsln', 'provided', 'that', 'n', 'is', 'large', 'enough', 'to', 'ensure', 'that', 'ncslng... | [-0.24609029100445862, 0.2198436087429317, 0.010494464119388298, 0.04227377189884216, -0.039828892670233144, -0.10672194447199052, 0.011716083835133097, 0.323904293843291, -0.2913274281785231, -0.28145353664347733, 0.08885843748099763, -0.3308621080253612, -0.07378083633110774, 0.18842808477347717, -0.03550619509240443... |
1,801.01483 | Numerical Solution of the Boundary Value Problems for Partial
Differential Equations. Crash course for holographer | These are the notes for a series of Numerical Study group meetings, held in
Lorentz institute in the fall of 2017. The aim of the notes is to provide a
non-specialist with the minimal knowledge in numerical methods used in BVP for
PDEs, necessary to solve the problems typically arising in applications of
holography t... | hep-th | these are the notes for a series of numerical study group meetings held in lorentz institute in the fall of 2017 the aim of the notes is to provide a nonspecialist with the minimal knowledge in numerical methods used in bvp for pdes necessary to solve the problems typically arising in applications of holography to cond... | [['these', 'are', 'the', 'notes', 'for', 'a', 'series', 'of', 'numerical', 'study', 'group', 'meetings', 'held', 'in', 'lorentz', 'institute', 'in', 'the', 'fall', 'of', '2017', 'the', 'aim', 'of', 'the', 'notes', 'is', 'to', 'provide', 'a', 'nonspecialist', 'with', 'the', 'minimal', 'knowledge', 'in', 'numerical', 'me... | [-0.08672469723889412, 0.04266315815038979, -0.08804884159552126, 0.07057667666833431, -0.1312145257573414, -0.11740372375713597, -0.010394924111535838, 0.29388748435705003, -0.22990599577716583, -0.3063507156109373, 0.16264800083670958, -0.27145123130296644, -0.1389008959723187, 0.2215972758171245, -0.1152295071655755... |
1,801.01484 | Scattering linear polarization of late-type active stars | Many active stars are covered in spots, much more so than the Sun, as
indicated by spectroscopic and photometric observations. It has been predicted
that star spots induce non-zero intrinsic linear polarization by breaking the
visible stellar disk symmetry. Although small, this effect might be useful for
star spot st... | astro-ph.SR | many active stars are covered in spots much more so than the sun as indicated by spectroscopic and photometric observations it has been predicted that star spots induce nonzero intrinsic linear polarization by breaking the visible stellar disk symmetry although small this effect might be useful for star spot studies an... | [['many', 'active', 'stars', 'are', 'covered', 'in', 'spots', 'much', 'more', 'so', 'than', 'the', 'sun', 'as', 'indicated', 'by', 'spectroscopic', 'and', 'photometric', 'observations', 'it', 'has', 'been', 'predicted', 'that', 'star', 'spots', 'induce', 'nonzero', 'intrinsic', 'linear', 'polarization', 'by', 'breaking... | [-0.08583598640645443, 0.1730039139815842, -0.06276616794857857, 0.09755271194550677, -0.12070930997597237, -0.11199741059406601, 0.08126368360442025, 0.4194778606501436, -0.17601418994015378, -0.36563006465726977, 0.08363677442269679, -0.2782671972100604, -0.05918765762873801, 0.21941240216193664, -0.04458701165513907... |
1,801.01485 | Variational analysis and variational rationality in behavioral sciences:
stationary traps | This paper concerns applications of variational analysis to some local
aspects of behavioral science modeling by developing an effective variational
rationality approach to these and related issues. Our main attention is paid to
local stationary traps, which reflect such local equilibrium and the like
positions in be... | math.OC | this paper concerns applications of variational analysis to some local aspects of behavioral science modeling by developing an effective variational rationality approach to these and related issues our main attention is paid to local stationary traps which reflect such local equilibrium and the like positions in behavi... | [['this', 'paper', 'concerns', 'applications', 'of', 'variational', 'analysis', 'to', 'some', 'local', 'aspects', 'of', 'behavioral', 'science', 'modeling', 'by', 'developing', 'an', 'effective', 'variational', 'rationality', 'approach', 'to', 'these', 'and', 'related', 'issues', 'our', 'main', 'attention', 'is', 'paid... | [-0.01722440937689195, 0.004371007662686882, -0.08444426382063991, 0.13917135713725454, -0.12888097932769194, -0.1574129911036127, 0.048186127728937815, 0.35523548035158053, -0.3104156963423722, -0.3186405163956806, 0.1294992681618573, -0.24058154341247345, -0.23070418124940867, 0.1805915840384033, -0.13105430990561015... |
1,801.01486 | Deep Cross Polarimetric Thermal-to-visible Face Recognition | In this paper, we present a deep coupled learning frame- work to address the
problem of matching polarimetric ther- mal face photos against a gallery of
visible faces. Polariza- tion state information of thermal faces provides the
miss- ing textural and geometrics details in the thermal face im- agery which
exist in ... | cs.CV | in this paper we present a deep coupled learning frame work to address the problem of matching polarimetric ther mal face photos against a gallery of visible faces polariza tion state information of thermal faces provides the miss ing textural and geometrics details in the thermal face im agery which exist in visible s... | [['in', 'this', 'paper', 'we', 'present', 'a', 'deep', 'coupled', 'learning', 'frame', 'work', 'to', 'address', 'the', 'problem', 'of', 'matching', 'polarimetric', 'ther', 'mal', 'face', 'photos', 'against', 'a', 'gallery', 'of', 'visible', 'faces', 'polariza', 'tion', 'state', 'information', 'of', 'thermal', 'faces', ... | [-0.04081960657392355, -0.03573476057705086, -0.07009493488482857, 0.035416464476763984, -0.10945012869094224, -0.1826428236628143, -0.013714006850632893, 0.42331437611514156, -0.29911201472175036, -0.2860993838756044, 0.09456204608397778, -0.30723913462613434, -0.1875043313484639, 0.13117621145348118, -0.1847464039940... |
1,801.01487 | First measurement of transverse-spin-dependent azimuthal asymmetries in
the Drell-Yan process | The COMPASS experiment at CERN, as part of its programme addresses the
exploration of the transverse spin structure of the nucleon by measuring spin
(in)dependent azimuthal asymmetries in semi-inclusive DIS and, recently, also
in Drell-Yan processes. Between 2002 and 2010 COMPASS performed a series of
SIDIS measureme... | hep-ex hep-ph | the compass experiment at cern as part of its programme addresses the exploration of the transverse spin structure of the nucleon by measuring spin independent azimuthal asymmetries in semiinclusive dis and recently also in drellyan processes between 2002 and 2010 compass performed a series of sidis measurements using ... | [['the', 'compass', 'experiment', 'at', 'cern', 'as', 'part', 'of', 'its', 'programme', 'addresses', 'the', 'exploration', 'of', 'the', 'transverse', 'spin', 'structure', 'of', 'the', 'nucleon', 'by', 'measuring', 'spin', 'independent', 'azimuthal', 'asymmetries', 'in', 'semiinclusive', 'dis', 'and', 'recently', 'also'... | [-0.061023215653744016, 0.24304618397121422, -0.18830367300064255, 0.09898420676667412, -0.04119840955372746, -0.05949598969237262, -0.004951107266122068, 0.4240087072238238, -0.19126680936559637, -0.22079380059934403, -0.06515220258028119, -0.33595823797468954, 0.055586998209015595, 0.1471860541827073, 0.1077447710724... |
1,801.01488 | Measurement of longitudinal-target-polarization dependent azimuthal
asymmetries in SIDIS at COMPASS experiment | Preliminary results obtained by the COMPASS experiment for
longitudinal-spin-dependent azimuthal asymmetries in single-hadron
muoproduction off protons are presented for the first time. The analysis was
carried out on the full data sample collected by COMPASS with longitudinally
polarized proton ($NH_3$) target in 20... | hep-ex hep-ph | preliminary results obtained by the compass experiment for longitudinalspindependent azimuthal asymmetries in singlehadron muoproduction off protons are presented for the first time the analysis was carried out on the full data sample collected by compass with longitudinally polarized proton nh_3 target in 2007 and 201... | [['preliminary', 'results', 'obtained', 'by', 'the', 'compass', 'experiment', 'for', 'longitudinalspindependent', 'azimuthal', 'asymmetries', 'in', 'singlehadron', 'muoproduction', 'off', 'protons', 'are', 'presented', 'for', 'the', 'first', 'time', 'the', 'analysis', 'was', 'carried', 'out', 'on', 'the', 'full', 'data... | [-0.037475390656879035, 0.1663175362402073, -0.13115223209067844, 0.11468535212021488, -0.029783218348426604, -0.07141503868337873, 0.008942740455047409, 0.41405823028910516, -0.18958946017187034, -0.3078078089921332, 0.008491128780826954, -0.3416362009011209, 0.05021382572560279, 0.18719732378428774, 0.100341107464007... |
1,801.01489 | All Models are Wrong, but Many are Useful: Learning a Variable's
Importance by Studying an Entire Class of Prediction Models Simultaneously | Variable importance (VI) tools describe how much covariates contribute to a
prediction model's accuracy. However, important variables for one
well-performing model (for example, a linear model
$f(\mathbf{x})=\mathbf{x}^{T}\beta$ with a fixed coefficient vector $\beta$)
may be unimportant for another model. In this pa... | stat.ME | variable importance vi tools describe how much covariates contribute to a prediction models accuracy however important variables for one wellperforming model for example a linear model fmathbfxmathbfxtbeta with a fixed coefficient vector beta may be unimportant for another model in this paper we propose model class rel... | [['variable', 'importance', 'vi', 'tools', 'describe', 'how', 'much', 'covariates', 'contribute', 'to', 'a', 'prediction', 'models', 'accuracy', 'however', 'important', 'variables', 'for', 'one', 'wellperforming', 'model', 'for', 'example', 'a', 'linear', 'model', 'fmathbfxmathbfxtbeta', 'with', 'a', 'fixed', 'coeffici... | [0.0011419886532214978, 0.05110480841101399, -0.06097411152921499, 0.140158947678294, -0.11238533406636662, -0.19976457527705602, 0.12468413868241465, 0.37880809007892535, -0.2487297278185863, -0.30984627955627664, 0.09343462328921767, -0.2530412865216257, -0.17194621684399272, 0.2126181956858586, -0.0912604853264475, ... |
1,801.0149 | The Magellanic Bridge cluster NGC 796: Deep optical AO imaging reveals
the stellar content and initial mass function of a massive open cluster | NGC 796 is a massive young cluster located 59 kpc from us in the diffuse
intergalactic medium of the 1/5-1/10 $Z_{\odot}$ Magellanic Bridge, allowing to
probe variations in star formation and stellar evolution processes as a
function of metallicity in a resolved fashion, providing a link between
resolved studies of n... | astro-ph.SR astro-ph.GA | ngc 796 is a massive young cluster located 59 kpc from us in the diffuse intergalactic medium of the 15110 z_odot magellanic bridge allowing to probe variations in star formation and stellar evolution processes as a function of metallicity in a resolved fashion providing a link between resolved studies of nearby solarm... | [['ngc', '796', 'is', 'a', 'massive', 'young', 'cluster', 'located', '59', 'kpc', 'from', 'us', 'in', 'the', 'diffuse', 'intergalactic', 'medium', 'of', 'the', '15110', 'z_odot', 'magellanic', 'bridge', 'allowing', 'to', 'probe', 'variations', 'in', 'star', 'formation', 'and', 'stellar', 'evolution', 'processes', 'as',... | [-0.0520668450571975, 0.09795513966230374, -0.1160811572754028, 0.10748009465623909, -0.08545496995520807, -0.033140225280021696, 0.08122857634816683, 0.4444551098786178, -0.15268262162771862, -0.38120813352543337, -0.022933806441642446, -0.24825188975955825, 0.008972892130259424, 0.17738728482299848, -0.03950187886766... |
1,801.01491 | The Action of Young Subgroups on the Partition Complex | We study the restrictions, the strict fixed points, and the strict quotients
of the partition complex $|\Pi_n|$, which is the $\Sigma_n$-space attached to
the poset of proper nontrivial partitions of the set $\{1,\ldots,n\}$.
We express the space of fixed points $|\Pi_n|^G$ in terms of subgroup posets
for general $... | math.AT math.CO | we study the restrictions the strict fixed points and the strict quotients of the partition complex pi_n which is the sigma_nspace attached to the poset of proper nontrivial partitions of the set 1ldotsn we express the space of fixed points pi_ng in terms of subgroup posets for general gsubset sigma_n and prove a formu... | [['we', 'study', 'the', 'restrictions', 'the', 'strict', 'fixed', 'points', 'and', 'the', 'strict', 'quotients', 'of', 'the', 'partition', 'complex', 'pi_n', 'which', 'is', 'the', 'sigma_nspace', 'attached', 'to', 'the', 'poset', 'of', 'proper', 'nontrivial', 'partitions', 'of', 'the', 'set', '1ldotsn', 'we', 'express'... | [-0.1935333911126108, 0.06564312572586102, -0.10634049152160126, 0.10797690088779592, -0.11946629523397738, -0.13363221628078667, 0.08146810540608967, 0.3144918956867095, -0.3375204750493671, -0.21960521876560837, 0.0531502812512198, -0.23103371541947126, -0.1247935338649543, 0.17203854197071175, -0.16465614478380466, ... |
1,801.01492 | Brightest group galaxies-II: the relative contribution of BGGs to the
total baryon content of groups at z<1.3 | We performed a detailed study of the evolution of the star formation rate
(SFR) and stellar mass of the brightest group galaxies (BGGs) and their
relative contribution to the total baryon budget within $R_{200}$
($f^{BGG}_{b,200}$). The sample comprises 407 BGGs selected from X-ray galaxy
groups ($M_{200}=10^{12.8}-1... | astro-ph.GA | we performed a detailed study of the evolution of the star formation rate sfr and stellar mass of the brightest group galaxies bggs and their relative contribution to the total baryon budget within r_200 fbgg_b200 the sample comprises 407 bggs selected from xray galaxy groups m_200101281014 m_odot out to zsim13 identif... | [['we', 'performed', 'a', 'detailed', 'study', 'of', 'the', 'evolution', 'of', 'the', 'star', 'formation', 'rate', 'sfr', 'and', 'stellar', 'mass', 'of', 'the', 'brightest', 'group', 'galaxies', 'bggs', 'and', 'their', 'relative', 'contribution', 'to', 'the', 'total', 'baryon', 'budget', 'within', 'r_200', 'fbgg_b200',... | [-0.022914704903895553, 0.14212814389697492, -0.04754934627756787, 0.11381788779302345, -0.04507179774534759, -0.001616544250282459, 0.07078685380030139, 0.48133597141713835, -0.10751584800487358, -0.40519751981486885, 0.0013219722758448268, -0.3262965563335456, 0.015956972995708283, 0.18129003454507459, -0.06711218101... |
1,801.01493 | NGC 4993, the shell galaxy host of GW170817: constraints on the recent
galactic merger | NGC 4993 is the shell galaxy host of the GRB170817A short gamma-ray burst and
the GW170817 gravitational-wave event produced during a binary-neutron-star
coalescence. The galaxy shows signs, including the stellar shells, that it has
recently accreted a smaller, late-type galaxy. The accreted galaxy might be the
origi... | astro-ph.GA astro-ph.HE | ngc 4993 is the shell galaxy host of the grb170817a short gammaray burst and the gw170817 gravitationalwave event produced during a binaryneutronstar coalescence the galaxy shows signs including the stellar shells that it has recently accreted a smaller latetype galaxy the accreted galaxy might be the original host of ... | [['ngc', '4993', 'is', 'the', 'shell', 'galaxy', 'host', 'of', 'the', 'grb170817a', 'short', 'gammaray', 'burst', 'and', 'the', 'gw170817', 'gravitationalwave', 'event', 'produced', 'during', 'a', 'binaryneutronstar', 'coalescence', 'the', 'galaxy', 'shows', 'signs', 'including', 'the', 'stellar', 'shells', 'that', 'it... | [-0.05230584769179263, 0.10516663009661653, -0.10910632047972452, 0.14060167786014335, -0.14691997440006102, 0.017485186700478838, 0.026028579953427035, 0.40844367564685885, -0.13409692037510135, -0.3474798402348433, 0.03134765920807577, -0.30680261738598347, 0.026651857937473343, 0.1824727851098844, 0.0058821048712738... |
1,801.01494 | Coincident SZ and $\gamma$-ray signals from cluster virial shocks | Virial shocks around galaxy clusters are expected to show a cutoff in the
thermal Sunyaev-Zel'dovich (SZ) signal, coincident with a leptonic ring.
However, until now, leptonic virial signals were reported only in Coma and in
stacked Fermi-LAT clusters, and an SZ virial shock signal was reported only in
A2319. We poin... | astro-ph.CO astro-ph.HE | virial shocks around galaxy clusters are expected to show a cutoff in the thermal sunyaevzeldovich sz signal coincident with a leptonic ring however until now leptonic virial signals were reported only in coma and in stacked fermilat clusters and an sz virial shock signal was reported only in a2319 we point out that a ... | [['virial', 'shocks', 'around', 'galaxy', 'clusters', 'are', 'expected', 'to', 'show', 'a', 'cutoff', 'in', 'the', 'thermal', 'sunyaevzeldovich', 'sz', 'signal', 'coincident', 'with', 'a', 'leptonic', 'ring', 'however', 'until', 'now', 'leptonic', 'virial', 'signals', 'were', 'reported', 'only', 'in', 'coma', 'and', 'i... | [-0.09540029876524399, 0.1273863336874187, -0.06409468548700319, 0.1262102196071769, -0.09691769102404654, -0.05123181288248636, 0.06589470921136753, 0.41533773856788453, -0.20517530996667246, -0.3347192662112205, 0.054460341395305235, -0.3505371813286255, 0.05870874974758587, 0.21227012933264683, 0.047257736987683555,... |
1,801.01495 | Electronic sound modes and plasmons in hydrodynamic two-dimensional
metals | Using an analytically tractable kinetic model of a two dimensional Fermi
liquid of electrons, we characterize the crossovers between zero sound, first
sound and plasmons. For experimentally realized Fermi liquids in a hydrodynamic
limit, both zero and first sound waves are essentially replaced by plasmons.
The plasmo... | cond-mat.str-el cond-mat.mes-hall | using an analytically tractable kinetic model of a two dimensional fermi liquid of electrons we characterize the crossovers between zero sound first sound and plasmons for experimentally realized fermi liquids in a hydrodynamic limit both zero and first sound waves are essentially replaced by plasmons the plasmon dispe... | [['using', 'an', 'analytically', 'tractable', 'kinetic', 'model', 'of', 'a', 'two', 'dimensional', 'fermi', 'liquid', 'of', 'electrons', 'we', 'characterize', 'the', 'crossovers', 'between', 'zero', 'sound', 'first', 'sound', 'and', 'plasmons', 'for', 'experimentally', 'realized', 'fermi', 'liquids', 'in', 'a', 'hydrod... | [-0.16327957844478078, 0.24280033087870834, -0.07782106436789035, 0.10088573680986883, -0.022679512843023986, -0.154509886080632, 0.043205468315863985, 0.3367844794993289, -0.23830427026841788, -0.19776524005574175, 0.002936357718135696, -0.3315356415390852, -0.11006916859187185, 0.24051340247679037, 0.0818893838440999... |
1,801.01496 | Vector Effective Field Theories from Soft Limits | We present a bottom-up construction of vector effective field theories using
the infrared structure of scattering amplitudes. Our results employ two
distinct probes of soft kinematics: multiple soft limits and single soft limits
after dimensional reduction, applicable in four and general dimensions,
respectively. Bot... | hep-th | we present a bottomup construction of vector effective field theories using the infrared structure of scattering amplitudes our results employ two distinct probes of soft kinematics multiple soft limits and single soft limits after dimensional reduction applicable in four and general dimensions respectively both approa... | [['we', 'present', 'a', 'bottomup', 'construction', 'of', 'vector', 'effective', 'field', 'theories', 'using', 'the', 'infrared', 'structure', 'of', 'scattering', 'amplitudes', 'our', 'results', 'employ', 'two', 'distinct', 'probes', 'of', 'soft', 'kinematics', 'multiple', 'soft', 'limits', 'and', 'single', 'soft', 'li... | [-0.1058291490909826, 0.2034687480418799, -0.09444973127167557, 0.09649505266276448, -0.07104278003470492, -0.15288605429196117, 0.04363873759860691, 0.32526219522906946, -0.22691422323552296, -0.26295128592155564, 0.04464342748535048, -0.23086185807112566, -0.17749076508484857, 0.14047089483368105, 0.02415645549784309... |
1,801.01497 | Massive optimal data compression and density estimation for scalable,
likelihood-free inference in cosmology | Many statistical models in cosmology can be simulated forwards but have
intractable likelihood functions. Likelihood-free inference methods allow us to
perform Bayesian inference from these models using only forward simulations,
free from any likelihood assumptions or approximations. Likelihood-free
inference generic... | astro-ph.CO | many statistical models in cosmology can be simulated forwards but have intractable likelihood functions likelihoodfree inference methods allow us to perform bayesian inference from these models using only forward simulations free from any likelihood assumptions or approximations likelihoodfree inference generically in... | [['many', 'statistical', 'models', 'in', 'cosmology', 'can', 'be', 'simulated', 'forwards', 'but', 'have', 'intractable', 'likelihood', 'functions', 'likelihoodfree', 'inference', 'methods', 'allow', 'us', 'to', 'perform', 'bayesian', 'inference', 'from', 'these', 'models', 'using', 'only', 'forward', 'simulations', 'f... | [-0.02797930398862809, -0.014933405202697031, -0.07589082124270499, 0.12069055414991453, -0.1421411902438849, -0.15559543280676008, 0.08074643350811675, 0.38858433796465397, -0.25780094174668194, -0.40624911442399025, 0.10841756315017119, -0.23065379870682956, -0.0987509395154193, 0.22634345252998173, -0.05620639590488... |
1,801.01498 | I. Analysis of candidates for interacting galaxy clusters | Merging galaxy clusters allows to study the different mass components, dark
and baryonic, separately. Also their occurrence enables to test the
$\Lambda$CDM scenario and they could put constrains in the self interacting
cross section of the dark matter particle. It is necessary to perform an
homogeneous analysis of t... | astro-ph.CO | merging galaxy clusters allows to study the different mass components dark and baryonic separately also their occurrence enables to test the lambdacdm scenario and they could put constrains in the self interacting cross section of the dark matter particle it is necessary to perform an homogeneous analysis of these syst... | [['merging', 'galaxy', 'clusters', 'allows', 'to', 'study', 'the', 'different', 'mass', 'components', 'dark', 'and', 'baryonic', 'separately', 'also', 'their', 'occurrence', 'enables', 'to', 'test', 'the', 'lambdacdm', 'scenario', 'and', 'they', 'could', 'put', 'constrains', 'in', 'the', 'self', 'interacting', 'cross',... | [-0.12775275820848941, 0.07122808459073032, -0.13089680288182207, 0.10349876623615877, -0.08736051641522569, -0.05611628394596295, 0.02373005909434475, 0.38169618945682676, -0.18774208942566506, -0.3444865897977033, 0.06808662371594036, -0.27956980928138364, -0.10506179152508002, 0.18791156274156734, 0.0161084673859536... |
1,801.01499 | A Model Connecting Galaxy Masses, Star Formation Rates, and Dust
Temperatures Across Cosmic Time | We investigate the evolution of dust content in galaxies from redshifts z=0
to z=9.5. Using empirically motivated prescriptions, we model galactic-scale
properties -- including halo mass, stellar mass, star formation rate, gas mass,
and metallicity -- to make predictions for the galactic evolution of dust mass
and du... | astro-ph.GA astro-ph.CO | we investigate the evolution of dust content in galaxies from redshifts z0 to z95 using empirically motivated prescriptions we model galacticscale properties including halo mass stellar mass star formation rate gas mass and metallicity to make predictions for the galactic evolution of dust mass and dust temperature in ... | [['we', 'investigate', 'the', 'evolution', 'of', 'dust', 'content', 'in', 'galaxies', 'from', 'redshifts', 'z0', 'to', 'z95', 'using', 'empirically', 'motivated', 'prescriptions', 'we', 'model', 'galacticscale', 'properties', 'including', 'halo', 'mass', 'stellar', 'mass', 'star', 'formation', 'rate', 'gas', 'mass', 'a... | [0.022047682947744854, 0.11708893524244046, -0.05665234175289814, 0.15191832146210332, -0.0986574762694848, -0.03261802855204456, 0.03129448476978817, 0.47315705538942265, -0.07122210416202553, -0.3565129068417427, 0.009123575101302076, -0.2925894047396305, 0.010657817349196054, 0.17690919202943453, -0.0018841679587076... |
1,801.015 | An ALMA study of the Orion Integral Filament: I. Evidence for narrow
fibers in a massive cloud | Abridged. Are all filaments bundles of fibers? To address this question, we
have investigated the gas organization within the paradigmatic Integral Shape
Filament (ISF). We combined two new ALMA Cycle 3 mosaics with previous IRAM 30m
observations to produce a high-dynamic range N$_2$H$^+$(1-0) emission map of
the ISF... | astro-ph.GA | abridged are all filaments bundles of fibers to address this question we have investigated the gas organization within the paradigmatic integral shape filament isf we combined two new alma cycle 3 mosaics with previous iram 30m observations to produce a highdynamic range n_2h10 emission map of the isf tracing its highd... | [['abridged', 'are', 'all', 'filaments', 'bundles', 'of', 'fibers', 'to', 'address', 'this', 'question', 'we', 'have', 'investigated', 'the', 'gas', 'organization', 'within', 'the', 'paradigmatic', 'integral', 'shape', 'filament', 'isf', 'we', 'combined', 'two', 'new', 'alma', 'cycle', '3', 'mosaics', 'with', 'previous... | [-0.14389588903216316, 0.09899711685588729, -0.05527752742884641, 0.052000796428967454, -0.04517466563678591, -0.06462429508613092, 0.03148460553559402, 0.4567196242063775, -0.22056255501972394, -0.30365525882241995, 0.05867129556854513, -0.23083506074506155, -0.0900716250712805, 0.1312628409029348, -0.0016511501291319... |
1,801.01501 | Dyakonov-Shur instability across the ballistic-to-hydrodynamic crossover | We numerically solve semiclassical kinetic equations and compute the growth
rate of the Dyakonov-Shur instability of a two-dimensional Fermi liquid in a
finite length cavity. When electron-electron scattering is fast, we observe the
well-understood hydrodynamic instability, and its disappearance due to viscous
dissip... | cond-mat.str-el cond-mat.mes-hall | we numerically solve semiclassical kinetic equations and compute the growth rate of the dyakonovshur instability of a twodimensional fermi liquid in a finite length cavity when electronelectron scattering is fast we observe the wellunderstood hydrodynamic instability and its disappearance due to viscous dissipation whe... | [['we', 'numerically', 'solve', 'semiclassical', 'kinetic', 'equations', 'and', 'compute', 'the', 'growth', 'rate', 'of', 'the', 'dyakonovshur', 'instability', 'of', 'a', 'twodimensional', 'fermi', 'liquid', 'in', 'a', 'finite', 'length', 'cavity', 'when', 'electronelectron', 'scattering', 'is', 'fast', 'we', 'observe'... | [-0.19759049975234544, 0.2019284206744231, -0.07253283462290402, 0.12589234995498308, -0.05724956544811352, -0.13864900868936952, -0.0003365118033580587, 0.30906580507912684, -0.29836656166319275, -0.18486429575148602, 0.0729358677709685, -0.27408554518437933, -0.1359071068491944, 0.21421923083056446, 0.023130208942514... |
1,801.01502 | The HST large programme on $\omega$ Centauri -- III. Absolute proper
motion | In this paper we report a new estimate of the absolute proper motion (PM) of
the globular cluster NGC 5139 ($\omega$ Cen) as part of the HST large program
GO-14118+14662. We analyzed a field 17 arcmin South-West of the center of
$\omega$ Cen and computed PMs with an epoch span of $\sim$15.1 years. We
employed 45 back... | astro-ph.GA astro-ph.SR | in this paper we report a new estimate of the absolute proper motion pm of the globular cluster ngc 5139 omega cen as part of the hst large program go1411814662 we analyzed a field 17 arcmin southwest of the center of omega cen and computed pms with an epoch span of sim151 years we employed 45 background galaxies to li... | [['in', 'this', 'paper', 'we', 'report', 'a', 'new', 'estimate', 'of', 'the', 'absolute', 'proper', 'motion', 'pm', 'of', 'the', 'globular', 'cluster', 'ngc', '5139', 'omega', 'cen', 'as', 'part', 'of', 'the', 'hst', 'large', 'program', 'go1411814662', 'we', 'analyzed', 'a', 'field', '17', 'arcmin', 'southwest', 'of', ... | [-0.10134147561814141, 0.07078559338944795, -0.07517610889575947, 0.027969816192903427, -0.07149919644611621, -0.0491856015737181, 0.08960910685335313, 0.4087105151343148, -0.18388955049937458, -0.3597721860075516, 0.046362788607733504, -0.3120143011895142, 0.03579575842303413, 0.23402886558855454, -0.09202033525556944... |
1,801.01503 | No Slip Gravity | A subclass of the Horndeski modified gravity theory we call No Slip Gravity
has particularly interesting properties: 1) a speed of gravitational wave
propagation equal to the speed of light, 2) equality between the effective
gravitational coupling strengths to matter and light, $G_{\rm matter}$ and
$G_{\rm light}$, h... | astro-ph.CO gr-qc | a subclass of the horndeski modified gravity theory we call no slip gravity has particularly interesting properties 1 a speed of gravitational wave propagation equal to the speed of light 2 equality between the effective gravitational coupling strengths to matter and light g_rm matter and g_rm light hence no slip betwe... | [['a', 'subclass', 'of', 'the', 'horndeski', 'modified', 'gravity', 'theory', 'we', 'call', 'no', 'slip', 'gravity', 'has', 'particularly', 'interesting', 'properties', '1', 'a', 'speed', 'of', 'gravitational', 'wave', 'propagation', 'equal', 'to', 'the', 'speed', 'of', 'light', '2', 'equality', 'between', 'the', 'effe... | [-0.1488768061687953, 0.12156329568497595, -0.11318186858611166, 0.13988816182042452, -0.14642489759265914, -0.1487342217547256, 0.00837326322794105, 0.31384660440042267, -0.23429352735429135, -0.3188461012950586, 0.030095400845509223, -0.27125941482986243, -0.1483503783292267, 0.20551288998577483, 0.022321580367725948... |
1,801.01504 | The HST large programme on $\omega$ Centauri - II. internal kinematics | In this second installment of the series, we look at the internal kinematics
of the multiple stellar populations of the globular cluster $\omega$ Centauri
in one of the parallel Hubble Space Telescope (HST) fields, located at about
3.5 half-light radii from the center of the cluster. Thanks to the over
15-year-long b... | astro-ph.GA astro-ph.SR | in this second installment of the series we look at the internal kinematics of the multiple stellar populations of the globular cluster omega centauri in one of the parallel hubble space telescope hst fields located at about 35 halflight radii from the center of the cluster thanks to the over 15yearlong baseline and th... | [['in', 'this', 'second', 'installment', 'of', 'the', 'series', 'we', 'look', 'at', 'the', 'internal', 'kinematics', 'of', 'the', 'multiple', 'stellar', 'populations', 'of', 'the', 'globular', 'cluster', 'omega', 'centauri', 'in', 'one', 'of', 'the', 'parallel', 'hubble', 'space', 'telescope', 'hst', 'fields', 'located... | [-0.08901837465033288, 0.14618816859729122, -0.06172267799725595, 0.07926238886245485, -0.08101663190810156, -0.015891927185203925, 0.06003463052079291, 0.39381516448494214, -0.18836957369566945, -0.36520101142776057, 0.037161340576753694, -0.3105421449122912, 0.001509661790090824, 0.22510916419009153, -0.0403153519395... |
1,801.01505 | Constraining sterile neutrino cosmologies with strong gravitational
lensing observations at redshift z~0.2 | We use the observed amount of subhaloes and line-of-sight dark matter haloes
in a sample of 11 gravitational lens systems from the Sloan Lens ACS Survey to
constrain the free-streaming properties of the dark matter particles. In
particular, we combine the detection of a small-mass dark matter halo by
Vegetti et al. 2... | astro-ph.CO | we use the observed amount of subhaloes and lineofsight dark matter haloes in a sample of 11 gravitational lens systems from the sloan lens acs survey to constrain the freestreaming properties of the dark matter particles in particular we combine the detection of a smallmass dark matter halo by vegetti et al 2010 with ... | [['we', 'use', 'the', 'observed', 'amount', 'of', 'subhaloes', 'and', 'lineofsight', 'dark', 'matter', 'haloes', 'in', 'a', 'sample', 'of', '11', 'gravitational', 'lens', 'systems', 'from', 'the', 'sloan', 'lens', 'acs', 'survey', 'to', 'constrain', 'the', 'freestreaming', 'properties', 'of', 'the', 'dark', 'matter', '... | [-0.05011914346947118, 0.17781184664844268, -0.03012698057448558, 0.15055006793201237, -0.10746655677420287, -0.0789557067671142, 0.03113369847415015, 0.3430840464425273, -0.13846607153495175, -0.44888614014364847, 0.010985133196170085, -0.32930751275437486, 0.037454048268305735, 0.20801358521047014, 0.0058630214688102... |
1,801.01506 | Time Delay Lens Modeling Challenge: I. Experimental Design | Strong gravitational lenses with measured time delay are a powerful tool to
measure cosmological parameters, especially the Hubble constant ($H_0$). Recent
studies show that by combining just three multiply-imaged AGN systems, one can
determine $H_0$ to 2.4% precision. Furthermore, the number of time-delay lens
syste... | astro-ph.CO astro-ph.GA | strong gravitational lenses with measured time delay are a powerful tool to measure cosmological parameters especially the hubble constant h_0 recent studies show that by combining just three multiplyimaged agn systems one can determine h_0 to 24 precision furthermore the number of timedelay lens systems is growing rap... | [['strong', 'gravitational', 'lenses', 'with', 'measured', 'time', 'delay', 'are', 'a', 'powerful', 'tool', 'to', 'measure', 'cosmological', 'parameters', 'especially', 'the', 'hubble', 'constant', 'h_0', 'recent', 'studies', 'show', 'that', 'by', 'combining', 'just', 'three', 'multiplyimaged', 'agn', 'systems', 'one',... | [-0.13354676768719687, 0.07015181345371538, -0.03569109574891627, 0.05441870787687958, -0.07744898222349333, -0.12763580611040473, 0.02826494288719853, 0.36927448130349844, -0.22784987174212032, -0.3919162517210356, 0.11986176802225149, -0.2975661533606557, -0.07648347152222022, 0.21928913799980218, -0.0433366120417505... |
1,801.01507 | Simulating radio emission from Low Mass Stars | Understanding the origins of stellar radio emission can provide invaluable
insight into the strength and geometry of stellar magnetic fields and the
resultant space weather environment experienced by exoplanets. Here, we present
the first model capable of predicting radio emission through the electron
cyclotron maser... | astro-ph.SR | understanding the origins of stellar radio emission can provide invaluable insight into the strength and geometry of stellar magnetic fields and the resultant space weather environment experienced by exoplanets here we present the first model capable of predicting radio emission through the electron cyclotron maser ins... | [['understanding', 'the', 'origins', 'of', 'stellar', 'radio', 'emission', 'can', 'provide', 'invaluable', 'insight', 'into', 'the', 'strength', 'and', 'geometry', 'of', 'stellar', 'magnetic', 'fields', 'and', 'the', 'resultant', 'space', 'weather', 'environment', 'experienced', 'by', 'exoplanets', 'here', 'we', 'prese... | [-0.05178720212078045, 0.1464710069078752, -0.034779678230029594, 0.11052112862087367, -0.13047874557672007, -0.06360228603460909, 0.04412839327995696, 0.4490087041062928, -0.164992966426825, -0.3644333872834806, 0.04301148920129775, -0.25468753545190875, -0.0662840901143814, 0.23392599771901126, 0.033716139217462616, ... |
1,801.01508 | Fast-growing SMBHs in Fast-growing Galaxies, at High Redshifts: the Role
of Major Mergers as Revealed by ALMA | We present a long-term, multi-wavelength project to understand the epoch of
fastest growth of the most massive black holes by using a sample of 40 luminous
quasars at z~4.8. These quasars have rather uniform properties, with typical
accretion rates and black hole masses of L/L_Edd~0.7 and M_BH~10^9 M_sol. The
sample ... | astro-ph.GA astro-ph.CO | we present a longterm multiwavelength project to understand the epoch of fastest growth of the most massive black holes by using a sample of 40 luminous quasars at z48 these quasars have rather uniform properties with typical accretion rates and black hole masses of ll_edd07 and m_bh109 m_sol the sample consists of fir... | [['we', 'present', 'a', 'longterm', 'multiwavelength', 'project', 'to', 'understand', 'the', 'epoch', 'of', 'fastest', 'growth', 'of', 'the', 'most', 'massive', 'black', 'holes', 'by', 'using', 'a', 'sample', 'of', '40', 'luminous', 'quasars', 'at', 'z48', 'these', 'quasars', 'have', 'rather', 'uniform', 'properties', ... | [-0.05063225422109442, 0.09218498631182812, -0.015010993527127694, 0.11329508846722332, -0.08430998530107076, -0.07218799273536172, 0.029832597086667346, 0.4673937290735578, -0.0851966682892899, -0.3403686055801545, 0.09385786751858485, -0.3273887840969453, -0.013953263967743865, 0.20794788681401116, 0.0225290264055695... |
1,801.01509 | Solar Flares and the Axion Quark Nugget Dark Matter Model | We advocate the idea that the nanoflares conjectured by Parker long ago to
resolve the corona heating problem, may also trigger the larger solar flares.
The arguments are based on the model where emission of extreme ultra violet
(EUV) radiation and soft x-rays from the Sun are powered externally by incident
dark matt... | astro-ph.SR astro-ph.CO astro-ph.HE hep-ph physics.space-ph | we advocate the idea that the nanoflares conjectured by parker long ago to resolve the corona heating problem may also trigger the larger solar flares the arguments are based on the model where emission of extreme ultra violet euv radiation and soft xrays from the sun are powered externally by incident dark matter part... | [['we', 'advocate', 'the', 'idea', 'that', 'the', 'nanoflares', 'conjectured', 'by', 'parker', 'long', 'ago', 'to', 'resolve', 'the', 'corona', 'heating', 'problem', 'may', 'also', 'trigger', 'the', 'larger', 'solar', 'flares', 'the', 'arguments', 'are', 'based', 'on', 'the', 'model', 'where', 'emission', 'of', 'extrem... | [-0.11349419835521891, 0.28254296331764356, -0.04495488159424871, 0.1587122523511942, -0.09850463066533606, -0.07868098837024501, -0.0024015969619141184, 0.34500174167672537, -0.20455935916681242, -0.3994523320829056, 0.029578773696594132, -0.2520807919185265, -0.03857094489684074, 0.18911828257777552, -0.0049981530197... |
1,801.0151 | Diffusive Shock Re-Acceleration | We have performed 2D hybrid simulations of non-relativistic collisionless
shocks in the presence of pre-existing energetic particles ("seeds"); such a
study applies, for instance, to the re-acceleration of Galactic cosmic rays
(CRs) in supernova remnant (SNR) shocks and solar wind energetic particles in
heliospheric ... | astro-ph.HE astro-ph.SR physics.plasm-ph physics.space-ph | we have performed 2d hybrid simulations of nonrelativistic collisionless shocks in the presence of preexisting energetic particles seeds such a study applies for instance to the reacceleration of galactic cosmic rays crs in supernova remnant snr shocks and solar wind energetic particles in heliospheric shocks energetic... | [['we', 'have', 'performed', '2d', 'hybrid', 'simulations', 'of', 'nonrelativistic', 'collisionless', 'shocks', 'in', 'the', 'presence', 'of', 'preexisting', 'energetic', 'particles', 'seeds', 'such', 'a', 'study', 'applies', 'for', 'instance', 'to', 'the', 'reacceleration', 'of', 'galactic', 'cosmic', 'rays', 'crs', '... | [-0.13191836000775162, 0.25026440861782445, -0.010901199522345225, 0.15273982183513754, -0.09580683477780791, -0.0548873095079279, 0.004680604703890362, 0.37780683618937944, -0.27626703342169695, -0.30637593032149046, -0.026160123353445957, -0.25516578067084866, 6.918231599346393e-05, 0.20091931453657033, 0.05870642382... |
1,801.01511 | Radiation pressure in galactic disks: stability, turbulence, and winds
in the single-scattering limit | The radiation force on dust grains may be dynamically important in driving
turbulence and outflows in rapidly star-forming galaxies. Recent studies focus
on the highly optically-thick limit relevant to the densest ultra-luminous
galaxies and super star clusters, where reprocessed infrared photons provide
the dominant... | astro-ph.GA astro-ph.IM | the radiation force on dust grains may be dynamically important in driving turbulence and outflows in rapidly starforming galaxies recent studies focus on the highly opticallythick limit relevant to the densest ultraluminous galaxies and super star clusters where reprocessed infrared photons provide the dominant source... | [['the', 'radiation', 'force', 'on', 'dust', 'grains', 'may', 'be', 'dynamically', 'important', 'in', 'driving', 'turbulence', 'and', 'outflows', 'in', 'rapidly', 'starforming', 'galaxies', 'recent', 'studies', 'focus', 'on', 'the', 'highly', 'opticallythick', 'limit', 'relevant', 'to', 'the', 'densest', 'ultraluminous... | [-0.09083661702973768, 0.16093425925215707, -0.07254445787332953, 0.0863749349862337, -0.052583505355753006, -0.012637517486233265, 0.03605588846327737, 0.3978866922259331, -0.18410897418484093, -0.3043715551570058, 0.04735969295911491, -0.2570605172198266, -0.016035121537744997, 0.20410227146465332, -0.015340795515105... |
1,801.01512 | Hats: all or nothing | N players are randomly fitted with a colored hat (q different colors). All
players guess simultaneously the color of their own hat observing only the hat
colors of the other N-1 players. The team wins if all players guess right. No
communication of any sort is allowed, except for an initial strategy session
before th... | math.CO cs.DM cs.IT math.IT | n players are randomly fitted with a colored hat q different colors all players guess simultaneously the color of their own hat observing only the hat colors of the other n1 players the team wins if all players guess right no communication of any sort is allowed except for an initial strategy session before the game be... | [['n', 'players', 'are', 'randomly', 'fitted', 'with', 'a', 'colored', 'hat', 'q', 'different', 'colors', 'all', 'players', 'guess', 'simultaneously', 'the', 'color', 'of', 'their', 'own', 'hat', 'observing', 'only', 'the', 'hat', 'colors', 'of', 'the', 'other', 'n1', 'players', 'the', 'team', 'wins', 'if', 'all', 'pla... | [-0.09625665671227121, 0.13414145799284133, -0.11959333247960285, 0.057811277866874705, -0.05946742759009165, -0.24613043903618267, 0.14121386526446594, 0.44635568516454976, -0.20537138454391993, -0.33692367888174785, 0.04518162078378176, -0.323543687680162, -0.07262646911938891, 0.04149108994016914, -0.159834573150409... |
1,801.01513 | Non-Standard Neutrino Interactions : Obviating Oscillation Experiments | Searching for non-standard neutrino interactions, as a means for discovering
physics beyond the Standard Model, has one of the key goals of dedicated
neutrino experiments, current and future. We demonstrate here that much of the
parameter space accessible to such experiments is already ruled out by the RUN
II data of... | hep-ph hep-ex | searching for nonstandard neutrino interactions as a means for discovering physics beyond the standard model has one of the key goals of dedicated neutrino experiments current and future we demonstrate here that much of the parameter space accessible to such experiments is already ruled out by the run ii data of the la... | [['searching', 'for', 'nonstandard', 'neutrino', 'interactions', 'as', 'a', 'means', 'for', 'discovering', 'physics', 'beyond', 'the', 'standard', 'model', 'has', 'one', 'of', 'the', 'key', 'goals', 'of', 'dedicated', 'neutrino', 'experiments', 'current', 'and', 'future', 'we', 'demonstrate', 'here', 'that', 'much', 'o... | [-0.04803136039169788, 0.1733267958957835, -0.041792460805611754, 0.15491058226117665, -0.09951299448896732, -0.156121657886875, 0.05299325573391148, 0.2783894529233554, -0.25214480608701706, -0.32843279543366016, 0.12259638566424005, -0.3017329503615786, -0.052590164850698784, 0.273622129515778, 0.12482828703442854, 0... |
1,801.01514 | The GALAH survey: properties of the Galactic disk(s) in the solar
neighbourhood | Using data from the GALAH pilot survey, we determine properties of the
Galactic thin and thick disks near the solar neighbourhood. The data cover a
small range of Galactocentric radius ($7.9 \leq R_\mathrm{GC} \leq 9.5$ kpc),
but extend up to 4 kpc in height from the Galactic plane, and several kpc in
the direction o... | astro-ph.GA | using data from the galah pilot survey we determine properties of the galactic thin and thick disks near the solar neighbourhood the data cover a small range of galactocentric radius 79 leq r_mathrmgc leq 95 kpc but extend up to 4 kpc in height from the galactic plane and several kpc in the direction of galactic antiro... | [['using', 'data', 'from', 'the', 'galah', 'pilot', 'survey', 'we', 'determine', 'properties', 'of', 'the', 'galactic', 'thin', 'and', 'thick', 'disks', 'near', 'the', 'solar', 'neighbourhood', 'the', 'data', 'cover', 'a', 'small', 'range', 'of', 'galactocentric', 'radius', '79', 'leq', 'r_mathrmgc', 'leq', '95', 'kpc'... | [-0.0849314409177827, 0.1130047603222875, -0.043087314530716514, 0.028775286166583775, -0.040938881174802544, -0.06716452955816625, 0.03969504659393718, 0.4418979044294621, -0.22018202502709724, -0.3609158866535757, 0.0022294234308134382, -0.2841404263522891, 0.05394838068159029, 0.186528197954382, -0.08495787201916853... |
1,801.01515 | Hyperelastic antiplane ground cloaking | Hyperelastic materials possess the appealing property that they may be
employed as elastic wave manipulation devices and cloaks by imposing
pre-deformation. They provide an alternative to microstructured metamaterials
and can be used in a reconfigurable manner. Previous studies indicate that
exact elastodynamic invar... | physics.app-ph | hyperelastic materials possess the appealing property that they may be employed as elastic wave manipulation devices and cloaks by imposing predeformation they provide an alternative to microstructured metamaterials and can be used in a reconfigurable manner previous studies indicate that exact elastodynamic invariance... | [['hyperelastic', 'materials', 'possess', 'the', 'appealing', 'property', 'that', 'they', 'may', 'be', 'employed', 'as', 'elastic', 'wave', 'manipulation', 'devices', 'and', 'cloaks', 'by', 'imposing', 'predeformation', 'they', 'provide', 'an', 'alternative', 'to', 'microstructured', 'metamaterials', 'and', 'can', 'be'... | [-0.11357809629143131, 0.10849509257645372, -0.08084548018035488, 0.0003038790727250579, -0.14757097112320627, -0.14341626395565468, -0.06882594332258885, 0.44126556179664955, -0.25414470721252563, -0.25998383874280584, 0.12811589600621826, -0.251988079485888, -0.19010454184855474, 0.21420399792318354, -0.0219151279008... |
1,801.01516 | Integrated NFV/SDN Architectures: A Systematic Literature Review | Network Functions Virtualization (NFV) and Software-Defined Networking (SDN)
are new paradigms in the move towards open software and network hardware. While
NFV aims to virtualize network functions and deploy them into general purpose
hardware, SDN makes networks programmable by separating the control and data
planes... | cs.NI | network functions virtualization nfv and softwaredefined networking sdn are new paradigms in the move towards open software and network hardware while nfv aims to virtualize network functions and deploy them into general purpose hardware sdn makes networks programmable by separating the control and data planes nfv and ... | [['network', 'functions', 'virtualization', 'nfv', 'and', 'softwaredefined', 'networking', 'sdn', 'are', 'new', 'paradigms', 'in', 'the', 'move', 'towards', 'open', 'software', 'and', 'network', 'hardware', 'while', 'nfv', 'aims', 'to', 'virtualize', 'network', 'functions', 'and', 'deploy', 'them', 'into', 'general', '... | [-0.16986642508574157, -0.033954280356624, -0.016613637071733918, 0.01999916421641377, -0.1352804030286647, -0.21062363030724837, 0.03533138207521269, 0.47849838779679416, -0.2515938167404282, -0.31014059746861866, 0.09563892372550514, -0.2300668848637756, -0.18214197588901296, 0.22148865374069804, -0.11099932165819806... |
1,801.01517 | Probing the nature of AX J0043-737: Not an 87 ms pulsar in the SMC | AX J0043-737 is a source in the ASCA catalogue, the nature of which is
uncertain. It is most commonly classified as a Crab-like pulsar in the Small
Magellanic Cloud (SMC) following apparent detection of pulsations at ~ 87 ms
from a single ASCA observation. A follow-up ASCA observation was not able to
confirm this, an... | astro-ph.HE | ax j0043737 is a source in the asca catalogue the nature of which is uncertain it is most commonly classified as a crablike pulsar in the small magellanic cloud smc following apparent detection of pulsations at 87 ms from a single asca observation a followup asca observation was not able to confirm this and the xray de... | [['ax', 'j0043737', 'is', 'a', 'source', 'in', 'the', 'asca', 'catalogue', 'the', 'nature', 'of', 'which', 'is', 'uncertain', 'it', 'is', 'most', 'commonly', 'classified', 'as', 'a', 'crablike', 'pulsar', 'in', 'the', 'small', 'magellanic', 'cloud', 'smc', 'following', 'apparent', 'detection', 'of', 'pulsations', 'at',... | [-0.08324965166908581, 0.04950678729829423, -0.10243274492677301, 0.08223623675523693, -0.136366570365051, -0.09616415956854606, 0.08718428736252602, 0.44293346934808564, -0.2075486980275645, -0.3367727462542601, 0.12745003338652447, -0.35825680335983634, -0.025696436829793338, 0.22443764548132514, -0.05230894439871637... |
1,801.01518 | A stable wavelength-tunable triggered source of single photons and
cascaded photon pairs at the telecom C-band | The implementation of fiber-based long-range quantum communication requires
tunable sources of single photons at the telecom C-band. Stable and
easy-to-implement wavelength- tunability of individual sources is crucial to
(i) bring remote sources into resonance, to (ii) define a wavelength standard
and to (iii) ensure... | cond-mat.mes-hall | the implementation of fiberbased longrange quantum communication requires tunable sources of single photons at the telecom cband stable and easytoimplement wavelength tunability of individual sources is crucial to i bring remote sources into resonance to ii define a wavelength standard and to iii ensure scalability to ... | [['the', 'implementation', 'of', 'fiberbased', 'longrange', 'quantum', 'communication', 'requires', 'tunable', 'sources', 'of', 'single', 'photons', 'at', 'the', 'telecom', 'cband', 'stable', 'and', 'easytoimplement', 'wavelength', 'tunability', 'of', 'individual', 'sources', 'is', 'crucial', 'to', 'i', 'bring', 'remot... | [-0.09460940557132874, 0.22244572516796846, -0.005685749695237194, -0.0009584482822434179, -0.021856015737035446, -0.2849665775549199, 0.08715269597779428, 0.5017058551311493, -0.24395115329551378, -0.31764513515468157, 0.0110309091203713, -0.3031732169219426, -0.006101825900508889, 0.2551579998846033, -0.0013979490500... |
1,801.01519 | Characterizing topological order by the information convex | Motivated by previous efforts in detecting topological orders from the ground
state(s) wave function, we introduce a new quantum information tool, coined the
information convex, to capture the bulk and boundary topological excitations of
a 2D topological order. Defined as a set of reduced density matrices that
minimi... | cond-mat.str-el hep-th quant-ph | motivated by previous efforts in detecting topological orders from the ground states wave function we introduce a new quantum information tool coined the information convex to capture the bulk and boundary topological excitations of a 2d topological order defined as a set of reduced density matrices that minimizes the ... | [['motivated', 'by', 'previous', 'efforts', 'in', 'detecting', 'topological', 'orders', 'from', 'the', 'ground', 'states', 'wave', 'function', 'we', 'introduce', 'a', 'new', 'quantum', 'information', 'tool', 'coined', 'the', 'information', 'convex', 'to', 'capture', 'the', 'bulk', 'and', 'boundary', 'topological', 'exc... | [-0.16638429945737312, 0.20616745964292993, -0.08851763782470282, 0.08008927859018668, -0.07238979352701266, -0.13581275259602374, 0.06597085844802322, 0.3007992401056118, -0.28623026109821464, -0.2541620346612837, 0.06495362079516842, -0.3222983438497946, -0.16813517962700797, 0.12564386231666905, -0.03902126066544550... |
1,801.0152 | Effect of in-situ electric field assisted growth on anti-phase
boundaries in epitaxial Fe3O4 thin films on MgO | Anti-phase boundaries (APBs) normally form as a consequence of the initial
growth conditions in all spinel ferrite thin films. The presence of APBs in
epitaxial films of the inverse spinel Fe3O4 alters their electronic and
magnetic properties due to strong antiferromagnetic (AF) interactions across
these boundaries. ... | cond-mat.mtrl-sci | antiphase boundaries apbs normally form as a consequence of the initial growth conditions in all spinel ferrite thin films the presence of apbs in epitaxial films of the inverse spinel fe3o4 alters their electronic and magnetic properties due to strong antiferromagnetic af interactions across these boundaries the effec... | [['antiphase', 'boundaries', 'apbs', 'normally', 'form', 'as', 'a', 'consequence', 'of', 'the', 'initial', 'growth', 'conditions', 'in', 'all', 'spinel', 'ferrite', 'thin', 'films', 'the', 'presence', 'of', 'apbs', 'in', 'epitaxial', 'films', 'of', 'the', 'inverse', 'spinel', 'fe3o4', 'alters', 'their', 'electronic', '... | [-0.15509668056222592, 0.20349274707608495, -0.023897026312285862, -0.027864644998071356, -0.018957971731889182, -0.06431766548512145, 0.01584740469206171, 0.42134471332527096, -0.2890692491529752, -0.32840786502922176, 0.08980117142793392, -0.2561874642551686, -0.10524729306676558, 0.19699284394115488, 0.0536062637176... |
1,801.01521 | Correlation between clustering and degree in affiliation networks | We are interested in the probability that two randomly selected neighbors of
a random vertex of degree (at least) $k$ are adjacent. We evaluate this
probability for a power law random intersection graph, where each vertex is
prescribed a collection of attributes and two vertices are adjacent whenever
they share a com... | cs.SI math.CO math.PR physics.soc-ph | we are interested in the probability that two randomly selected neighbors of a random vertex of degree at least k are adjacent we evaluate this probability for a power law random intersection graph where each vertex is prescribed a collection of attributes and two vertices are adjacent whenever they share a common attr... | [['we', 'are', 'interested', 'in', 'the', 'probability', 'that', 'two', 'randomly', 'selected', 'neighbors', 'of', 'a', 'random', 'vertex', 'of', 'degree', 'at', 'least', 'k', 'are', 'adjacent', 'we', 'evaluate', 'this', 'probability', 'for', 'a', 'power', 'law', 'random', 'intersection', 'graph', 'where', 'each', 'ver... | [-0.1749227405829436, 0.17214416809197838, -0.04050792750153367, 0.02697051657267603, -0.07014163581112845, -0.20399498753249645, 0.09812596656442822, 0.3985825631686527, -0.26859284755166457, -0.24862106900621692, 0.027953721687916423, -0.39599617603032483, -0.14368260522251544, 0.06783882411052575, -0.071863917360568... |
1,801.01522 | Using abstract elastic membranes to learn about quantum measurements | We provide an accessible popular science version of a research article
published by Diederik Aerts and the author [Ann. Phys. 351 (2014) 975--1025,
arXiv:1404.2429], where an extended version of the quantum formalism was
proposed as a possible solution to the measurement problem.
| quant-ph physics.pop-ph | we provide an accessible popular science version of a research article published by diederik aerts and the author ann phys 351 2014 9751025 arxiv14042429 where an extended version of the quantum formalism was proposed as a possible solution to the measurement problem | [['we', 'provide', 'an', 'accessible', 'popular', 'science', 'version', 'of', 'a', 'research', 'article', 'published', 'by', 'diederik', 'aerts', 'and', 'the', 'author', 'ann', 'phys', '351', '2014', '9751025', 'arxiv14042429', 'where', 'an', 'extended', 'version', 'of', 'the', 'quantum', 'formalism', 'was', 'proposed'... | [-0.022481672232970595, -0.007393241341196699, -0.08065414478187449, -0.005230709910392761, -0.10688328057294712, -0.11788274189457297, 0.03665254806983285, 0.262675580359064, -0.1732352282444481, -0.36823984268121424, 0.08299148551886901, -0.26536619383841753, -0.20026075476780533, 0.20975763518363238, -0.131833670497... |
1,801.01523 | Scalar-Vector-Tensor Gravity Theories | We construct the consistent ghost-free covariant scalar-vector-tensor gravity
theories with second order equations of motion with derivative interactions. We
impose locality, unitarity, Lorentz invariance and pseudo-Riemannian geometry
as the fundamental terms. In the tensor sector we require diffeomorphism
invarianc... | gr-qc astro-ph.CO hep-th | we construct the consistent ghostfree covariant scalarvectortensor gravity theories with second order equations of motion with derivative interactions we impose locality unitarity lorentz invariance and pseudoriemannian geometry as the fundamental terms in the tensor sector we require diffeomorphism invariance whereas ... | [['we', 'construct', 'the', 'consistent', 'ghostfree', 'covariant', 'scalarvectortensor', 'gravity', 'theories', 'with', 'second', 'order', 'equations', 'of', 'motion', 'with', 'derivative', 'interactions', 'we', 'impose', 'locality', 'unitarity', 'lorentz', 'invariance', 'and', 'pseudoriemannian', 'geometry', 'as', 't... | [-0.18994164898223873, 0.20260316222462477, -0.0697613497232433, 0.12157251858671599, -0.1538083228452534, -0.13335749273490463, -0.07855925284250564, 0.2843929090021128, -0.20012306499159643, -0.3169724998832051, 0.058377806301782464, -0.25680441154494277, -0.11646413449292399, 0.08944593786381537, -0.0041612017242162... |
1,801.01524 | Crystal growth and magnetic anisotropy in the spin-chain ruthenate
Na$_2$RuO$_4$ | We report single crystal growth, electrical resistivity $\rho$, anisotropic
magnetic susceptibiltiy $\chi$, and heat capacity $C_p$ measurements on the
one-dimensional spin-chain ruthenate Na$_2$RuO$_4$. We observe variable range
hopping (VRH) behaviour in $\rho(T)$. The magnetic susceptibility with magnetic
field pe... | cond-mat.str-el cond-mat.mtrl-sci | we report single crystal growth electrical resistivity rho anisotropic magnetic susceptibiltiy chi and heat capacity c_p measurements on the onedimensional spinchain ruthenate na_2ruo_4 we observe variable range hopping vrh behaviour in rhot the magnetic susceptibility with magnetic field perpendicular chi_perp and par... | [['we', 'report', 'single', 'crystal', 'growth', 'electrical', 'resistivity', 'rho', 'anisotropic', 'magnetic', 'susceptibiltiy', 'chi', 'and', 'heat', 'capacity', 'c_p', 'measurements', 'on', 'the', 'onedimensional', 'spinchain', 'ruthenate', 'na_2ruo_4', 'we', 'observe', 'variable', 'range', 'hopping', 'vrh', 'behavi... | [-0.21044929658685543, 0.24577976992900877, 0.01769936466882394, -0.044617493610480584, -0.07975354835111076, -0.1188073549819596, 0.08874397677015171, 0.39714725895219144, -0.24823738037797113, -0.3404909251657732, -0.0002991926122136825, -0.4030102394304118, -0.026342552763758444, 0.18334339599573607, 0.1189360201381... |
1,801.01525 | Bayesian Constraint Relaxation | Prior information often takes the form of parameter constraints. Bayesian
methods include such information through prior distributions having constrained
support. By using posterior sampling algorithms, one can quantify uncertainty
without relying on asymptotic approximations. However, sharply constrained
priors are ... | stat.ME | prior information often takes the form of parameter constraints bayesian methods include such information through prior distributions having constrained support by using posterior sampling algorithms one can quantify uncertainty without relying on asymptotic approximations however sharply constrained priors are a not n... | [['prior', 'information', 'often', 'takes', 'the', 'form', 'of', 'parameter', 'constraints', 'bayesian', 'methods', 'include', 'such', 'information', 'through', 'prior', 'distributions', 'having', 'constrained', 'support', 'by', 'using', 'posterior', 'sampling', 'algorithms', 'one', 'can', 'quantify', 'uncertainty', 'w... | [-0.04989442958715646, 0.045412799133319984, -0.09576463187661241, 0.10928607540862526, -0.11186246518593501, -0.13155001369578873, 0.10792199751731994, 0.42714244792073525, -0.29497140404384803, -0.32915820352294867, 0.12362971794859999, -0.21192723629338778, -0.11615166351308717, 0.18672033164595417, -0.0750397128558... |
1,801.01526 | An algebraic perspective on integer sparse recovery | Compressed sensing is a relatively new mathematical paradigm that shows a
small number of linear measurements are enough to efficiently reconstruct a
large dimensional signal under the assumption the signal is sparse.
Applications for this technology are ubiquitous, ranging from wireless
communications to medical ima... | math.NA math.NT | compressed sensing is a relatively new mathematical paradigm that shows a small number of linear measurements are enough to efficiently reconstruct a large dimensional signal under the assumption the signal is sparse applications for this technology are ubiquitous ranging from wireless communications to medical imaging... | [['compressed', 'sensing', 'is', 'a', 'relatively', 'new', 'mathematical', 'paradigm', 'that', 'shows', 'a', 'small', 'number', 'of', 'linear', 'measurements', 'are', 'enough', 'to', 'efficiently', 'reconstruct', 'a', 'large', 'dimensional', 'signal', 'under', 'the', 'assumption', 'the', 'signal', 'is', 'sparse', 'appl... | [-0.070559652799226, 0.08189677468900866, -0.09653323207109074, 0.08052875635492084, -0.11706419007277301, -0.1732278606239999, 0.015783643696813097, 0.39357223359048754, -0.33688526866586965, -0.30599103282152124, 0.1860857002463933, -0.23391629926645788, -0.2292495051512241, 0.21752091359952952, -0.13731253679832003,... |
1,801.01527 | Utilitarian Welfare and Representation Guarantees of Approval-Based
Multiwinner Rules | To choose a suitable multiwinner voting rule is a hard and ambiguous task.
Depending on the context, it varies widely what constitutes the choice of an
``optimal'' subset of alternatives. In this paper, we provide a quantitative
analysis of multiwinner voting rules using methods from the theory of
approximation algor... | cs.MA cs.AI | to choose a suitable multiwinner voting rule is a hard and ambiguous task depending on the context it varies widely what constitutes the choice of an optimal subset of alternatives in this paper we provide a quantitative analysis of multiwinner voting rules using methods from the theory of approximation algorithmswe es... | [['to', 'choose', 'a', 'suitable', 'multiwinner', 'voting', 'rule', 'is', 'a', 'hard', 'and', 'ambiguous', 'task', 'depending', 'on', 'the', 'context', 'it', 'varies', 'widely', 'what', 'constitutes', 'the', 'choice', 'of', 'an', 'optimal', 'subset', 'of', 'alternatives', 'in', 'this', 'paper', 'we', 'provide', 'a', 'q... | [-0.07500299453458265, -0.012580423761031221, -0.1315711097145253, 0.13981276370338663, -0.1596923349656103, -0.16714661811624676, 0.23026277992897476, 0.4038072391759512, -0.26876495729300603, -0.3085147807728653, 0.11091704359220356, -0.24073628274231287, -0.19747706969347514, 0.13900712431092893, -0.1000179181121720... |
1,801.01528 | A deep learning approach for detecting traffic accidents from social
media data | This paper employs deep learning in detecting the traffic accident from
social media data. First, we thoroughly investigate the 1-year over 3 million
tweet contents in two metropolitan areas: Northern Virginia and New York City.
Our results show that paired tokens can capture the association rules inherent
in the acc... | cs.SI stat.OT | this paper employs deep learning in detecting the traffic accident from social media data first we thoroughly investigate the 1year over 3 million tweet contents in two metropolitan areas northern virginia and new york city our results show that paired tokens can capture the association rules inherent in the accidentre... | [['this', 'paper', 'employs', 'deep', 'learning', 'in', 'detecting', 'the', 'traffic', 'accident', 'from', 'social', 'media', 'data', 'first', 'we', 'thoroughly', 'investigate', 'the', '1year', 'over', '3', 'million', 'tweet', 'contents', 'in', 'two', 'metropolitan', 'areas', 'northern', 'virginia', 'and', 'new', 'york... | [-0.06629866934719841, 0.04005942137128143, -0.05243518283417405, 0.10320197220141783, -0.11524302419275045, -0.14642890803326397, 0.13291954789039961, 0.40521719421281716, -0.24420808545681974, -0.37040641941563335, 0.10971607737978216, -0.37640802726842637, -0.1394541058591892, 0.16976384616261997, -0.107275692718969... |
1,801.01529 | A novel calibration framework for survival analysis when a binary
covariate is measured at sparse time points | The goals in clinical and cohort studies often include evaluation of the
association of a time-dependent binary treatment or exposure with a survival
outcome. Recently, several impactful studies targeted the association between
aspirin-taking and survival following colorectal cancer diagnosis. Due to
surgery, aspirin... | stat.AP stat.ME stat.OT | the goals in clinical and cohort studies often include evaluation of the association of a timedependent binary treatment or exposure with a survival outcome recently several impactful studies targeted the association between aspirintaking and survival following colorectal cancer diagnosis due to surgery aspirintaking v... | [['the', 'goals', 'in', 'clinical', 'and', 'cohort', 'studies', 'often', 'include', 'evaluation', 'of', 'the', 'association', 'of', 'a', 'timedependent', 'binary', 'treatment', 'or', 'exposure', 'with', 'a', 'survival', 'outcome', 'recently', 'several', 'impactful', 'studies', 'targeted', 'the', 'association', 'between... | [-0.04800808254597001, 0.04857647386214566, -0.10150136652509657, 0.10263724725900149, -0.08306257408996297, -0.1551521897893698, 0.11312009537913761, 0.38862111263554844, -0.20109288837078382, -0.2915993143709745, 0.12586793094813664, -0.25464937582067004, -0.12901019293909524, 0.19263023964034762, -0.1226846894876842... |
1,801.0153 | The Mutating Contact Process: Model Introduction and Qualitative
Analysis of Phase Transitions in its Survival | We introduce and study the mutating contact process, a variant of the
multitype contact process, where one type mutates at a constant rate to the
other type. We prove that on $\mathbb{Z}$ a single mutant cannot survive while
on $\mathbb{T}_{d}$ there are distinct weak survival and extinction of a single
mutant phases... | math.PR | we introduce and study the mutating contact process a variant of the multitype contact process where one type mutates at a constant rate to the other type we prove that on mathbbz a single mutant cannot survive while on mathbbt_d there are distinct weak survival and extinction of a single mutant phases yet the limiting... | [['we', 'introduce', 'and', 'study', 'the', 'mutating', 'contact', 'process', 'a', 'variant', 'of', 'the', 'multitype', 'contact', 'process', 'where', 'one', 'type', 'mutates', 'at', 'a', 'constant', 'rate', 'to', 'the', 'other', 'type', 'we', 'prove', 'that', 'on', 'mathbbz', 'a', 'single', 'mutant', 'can', 'not', 'su... | [-0.13550855476124626, 0.12870094960089773, -0.06006932971326427, 0.042044252889910344, -0.0180990333448992, -0.20517023727815184, 0.12223383583801074, 0.3652118362175922, -0.2580857987308668, -0.20735645013822554, 0.08627577867850454, -0.25726214374622536, -0.13193107462332895, 0.16520624788891938, -0.0536815749558930... |
1,801.01531 | Slugbot: An Application of a Novel and Scalable Open Domain Socialbot
Framework | In this paper we introduce a novel, open domain socialbot for the Amazon
Alexa Prize competition, aimed at carrying on friendly conversations with users
on a variety of topics. We present our modular system, highlighting our
different data sources and how we use the human mind as a model for data
management. Addition... | cs.CL cs.HC | in this paper we introduce a novel open domain socialbot for the amazon alexa prize competition aimed at carrying on friendly conversations with users on a variety of topics we present our modular system highlighting our different data sources and how we use the human mind as a model for data management additionally we... | [['in', 'this', 'paper', 'we', 'introduce', 'a', 'novel', 'open', 'domain', 'socialbot', 'for', 'the', 'amazon', 'alexa', 'prize', 'competition', 'aimed', 'at', 'carrying', 'on', 'friendly', 'conversations', 'with', 'users', 'on', 'a', 'variety', 'of', 'topics', 'we', 'present', 'our', 'modular', 'system', 'highlightin... | [-0.08667898144423296, -0.00409440099909781, -0.06922773989000623, 0.07075717362853798, -0.15137086029218544, -0.12469032883018372, 0.10402551150452512, 0.41264078034354107, -0.24511514277297206, -0.3123635903050724, 0.10260234015939725, -0.3187878193940768, -0.20614738652979472, 0.22073382033392722, -0.117288575476517... |
1,801.01532 | SN2013fs and SN2013fr: Exploring the circumstellar-material diversity in
Type II supernovae | We present photometry and spectroscopy of SN2013fs and SN2013fr in the first
100 days post-explosion. Both objects showed transient, relatively narrow
H$\alpha$ emission lines characteristic of SNeIIn, but later resembled normal
SNeII-P or SNeII-L, indicative of fleeting interaction with circumstellar
material (CSM).... | astro-ph.HE astro-ph.SR | we present photometry and spectroscopy of sn2013fs and sn2013fr in the first 100 days postexplosion both objects showed transient relatively narrow halpha emission lines characteristic of sneiin but later resembled normal sneiip or sneiil indicative of fleeting interaction with circumstellar material csm sn2013fs was d... | [['we', 'present', 'photometry', 'and', 'spectroscopy', 'of', 'sn2013fs', 'and', 'sn2013fr', 'in', 'the', 'first', '100', 'days', 'postexplosion', 'both', 'objects', 'showed', 'transient', 'relatively', 'narrow', 'halpha', 'emission', 'lines', 'characteristic', 'of', 'sneiin', 'but', 'later', 'resembled', 'normal', 'sn... | [-0.04354523776618894, 0.11226738219665158, -0.09455543338093733, 0.10508875000279744, -0.08717497603664565, -0.16559583996530883, 0.04634112573965171, 0.47296158310978914, -0.16333614201447386, -0.2869936089367108, 0.08872065603743892, -0.2538133751081173, -0.04253999580910733, 0.13803315187102524, -0.0373391026782608... |
1,801.01533 | Computational Analysis for the Rational Design of Anti-Amyloid Beta
(ABeta) Antibodies | Alzheimer's Disease (AD) is a neurodegenerative disorder that lacks effective
treatment options. Anti-amyloid beta (ABeta) antibodies are the leading drug
candidates to treat AD, but the results of clinical trials have been
disappointing. Introducing rational mutations into anti-ABeta antibodies to
increase their eff... | q-bio.BM | alzheimers disease ad is a neurodegenerative disorder that lacks effective treatment options antiamyloid beta abeta antibodies are the leading drug candidates to treat ad but the results of clinical trials have been disappointing introducing rational mutations into antiabeta antibodies to increase their effectiveness i... | [['alzheimers', 'disease', 'ad', 'is', 'a', 'neurodegenerative', 'disorder', 'that', 'lacks', 'effective', 'treatment', 'options', 'antiamyloid', 'beta', 'abeta', 'antibodies', 'are', 'the', 'leading', 'drug', 'candidates', 'to', 'treat', 'ad', 'but', 'the', 'results', 'of', 'clinical', 'trials', 'have', 'been', 'disap... | [-0.07477699644082496, 0.08825782889344413, -0.06722557348980297, 0.0997769929844165, -0.05943577883224333, -0.18093716678239646, 0.1070620910865405, 0.406915718070682, -0.20456947737163114, -0.2574859693240855, 0.0032380211065643496, -0.2756527264677589, -0.2079760350685026, 0.16866451795363138, -0.059250165521687805,... |
1,801.01534 | Do we need to modify Maxwell's equations? | Maxwell's equations are modified to incorporate a scalar field to account for
the London's superconductivity. Assuming the electromagnetic field is described
by the Klein-Gordon equation, London's equations of superconductivity are then
derived, which are invariant under a new set of transformations. The invariance
o... | physics.gen-ph | maxwells equations are modified to incorporate a scalar field to account for the londons superconductivity assuming the electromagnetic field is described by the kleingordon equation londons equations of superconductivity are then derived which are invariant under a new set of transformations the invariance of the modi... | [['maxwells', 'equations', 'are', 'modified', 'to', 'incorporate', 'a', 'scalar', 'field', 'to', 'account', 'for', 'the', 'londons', 'superconductivity', 'assuming', 'the', 'electromagnetic', 'field', 'is', 'described', 'by', 'the', 'kleingordon', 'equation', 'londons', 'equations', 'of', 'superconductivity', 'are', 't... | [-0.2007940083886813, 0.17908404639117348, -0.08676849526253719, 0.07436804966413353, -0.15801326480232974, -0.11627659554258712, -0.07163556697733194, 0.3132512703791116, -0.27062399287536304, -0.2916287201461247, 0.03895066880611974, -0.224052327169666, -0.13434330227522595, 0.16348030095359364, 0.004968228917207243,... |
1,801.01535 | Improvement to the Prediction of Fuel Cost Distributions Using ARIMA
Model | Availability of a validated, realistic fuel cost model is a prerequisite to
the development and validation of new optimization methods and control tools.
This paper uses an autoregressive integrated moving average (ARIMA) model with
historical fuel cost data in development of a three-step-ahead fuel cost
distribution... | stat.AP eess.SP | availability of a validated realistic fuel cost model is a prerequisite to the development and validation of new optimization methods and control tools this paper uses an autoregressive integrated moving average arima model with historical fuel cost data in development of a threestepahead fuel cost distribution predict... | [['availability', 'of', 'a', 'validated', 'realistic', 'fuel', 'cost', 'model', 'is', 'a', 'prerequisite', 'to', 'the', 'development', 'and', 'validation', 'of', 'new', 'optimization', 'methods', 'and', 'control', 'tools', 'this', 'paper', 'uses', 'an', 'autoregressive', 'integrated', 'moving', 'average', 'arima', 'mod... | [-0.03392878546089689, 0.02425243093241804, -0.09093122058702711, 0.11370973393257539, -0.05507176504893736, -0.121041448780342, 0.06197616690586621, 0.39745659730234345, -0.2478935187487127, -0.33314122277852537, 0.13635497077423558, -0.3076345591278343, -0.08783729636872356, 0.20617837339828532, -0.1181696314507952, ... |
1,801.01536 | Separated Kaon Electroproduction Cross Section and the Kaon Form Factor
from 6 GeV JLab Data | The $^{1}H$($e,e^\prime K^+$)$\Lambda$ reaction was studied as a function of
the Mandelstam variable $-t$ using data from the E01-004 (FPI-2) and E93-018
experiments that were carried out in Hall C at the 6 GeV Jefferson Lab. The
cross section was fully separated into longitudinal and transverse components,
and two i... | nucl-ex | the 1heeprime klambda reaction was studied as a function of the mandelstam variable t using data from the e01004 fpi2 and e93018 experiments that were carried out in hall c at the 6 gev jefferson lab the cross section was fully separated into longitudinal and transverse components and two interference terms at fourmome... | [['the', '1heeprime', 'klambda', 'reaction', 'was', 'studied', 'as', 'a', 'function', 'of', 'the', 'mandelstam', 'variable', 't', 'using', 'data', 'from', 'the', 'e01004', 'fpi2', 'and', 'e93018', 'experiments', 'that', 'were', 'carried', 'out', 'in', 'hall', 'c', 'at', 'the', '6', 'gev', 'jefferson', 'lab', 'the', 'cr... | [-0.03713213023862669, 0.1979410631981279, -0.11321745312656276, 0.09893628207234932, -0.03326957558015627, -0.09832376987008112, 0.05384848432083215, 0.3606575860455632, -0.1837965536649738, -0.2987393788035427, -0.034593412141049544, -0.3511313799263111, 0.01693209302212511, 0.20328526522432055, 0.0936407111252525, 0... |
1,801.01537 | Tauberian class estimates for vector-valued distributions | We study Tauberian properties of regularizing transforms of vector-valued
tempered distributions, that is, transforms of the form
$M^{\mathbf{f}}_{\varphi}(x,y)=(\mathbf{f}\ast\varphi_{y})(x)$, where the
kernel $\varphi$ is a test function and
$\varphi_{y}(\cdot)=y^{-n}\varphi(\cdot/y)$. We investigate conditions whi... | math.FA | we study tauberian properties of regularizing transforms of vectorvalued tempered distributions that is transforms of the form mmathbff_varphixymathbffastvarphi_yx where the kernel varphi is a test function and varphi_ycdotynvarphicdoty we investigate conditions which ensure that a distribution that a priori takes valu... | [['we', 'study', 'tauberian', 'properties', 'of', 'regularizing', 'transforms', 'of', 'vectorvalued', 'tempered', 'distributions', 'that', 'is', 'transforms', 'of', 'the', 'form', 'mmathbff_varphixymathbffastvarphi_yx', 'where', 'the', 'kernel', 'varphi', 'is', 'a', 'test', 'function', 'and', 'varphi_ycdotynvarphicdoty... | [-0.051715834981923066, 0.06902751048059705, -0.13627979329500634, 0.14548738572585324, -0.12416087045522335, -0.06558701421062534, 0.013136205075660165, 0.3908210463033846, -0.2695032322170356, -0.20101607708224598, 0.09746649104188411, -0.22579537386011977, -0.1465496953863364, 0.23401140253274486, -0.139901854939615... |
1,801.01538 | Understanding Hormonal Crosstalk in Arabidopsis Root Development via
Emulation and History Matching | A major challenge in plant developmental biology is to understand how plant
growth is coordinated by interacting hormones and genes. To meet this
challenge, it is important to not only use experimental data, but also
formulate a mathematical model. For the mathematical model to best describe the
true biological syste... | stat.AP | a major challenge in plant developmental biology is to understand how plant growth is coordinated by interacting hormones and genes to meet this challenge it is important to not only use experimental data but also formulate a mathematical model for the mathematical model to best describe the true biological system it i... | [['a', 'major', 'challenge', 'in', 'plant', 'developmental', 'biology', 'is', 'to', 'understand', 'how', 'plant', 'growth', 'is', 'coordinated', 'by', 'interacting', 'hormones', 'and', 'genes', 'to', 'meet', 'this', 'challenge', 'it', 'is', 'important', 'to', 'not', 'only', 'use', 'experimental', 'data', 'but', 'also',... | [-0.0749357431116559, 0.08976242527230338, -0.034907478658319675, 0.0660476853886791, -0.06644602565578574, -0.10695873654121985, 0.08661198449090521, 0.34666285147094755, -0.2721702877016177, -0.3465029702824767, 0.10296137229984771, -0.24193804312804804, -0.18145096295250995, 0.19802712625710892, -0.07506323597185964... |
1,801.01539 | DeepIso: A Deep Learning Model for Peptide Feature Detection | Liquid chromatography with tandem mass spectrometry (LC-MS/MS) based
proteomics is a well-established research field with major applications such as
identification of disease biomarkers, drug discovery, drug design and
development. In proteomics, protein identification and quantification is a
fundamental task, which ... | q-bio.QM cs.NE physics.med-ph | liquid chromatography with tandem mass spectrometry lcmsms based proteomics is a wellestablished research field with major applications such as identification of disease biomarkers drug discovery drug design and development in proteomics protein identification and quantification is a fundamental task which is done by f... | [['liquid', 'chromatography', 'with', 'tandem', 'mass', 'spectrometry', 'lcmsms', 'based', 'proteomics', 'is', 'a', 'wellestablished', 'research', 'field', 'with', 'major', 'applications', 'such', 'as', 'identification', 'of', 'disease', 'biomarkers', 'drug', 'discovery', 'drug', 'design', 'and', 'development', 'in', '... | [-0.006658944360663698, 0.05303624677725837, -0.04263569468432188, 0.009547097326599453, -0.09088972584689609, -0.1777230789394755, 0.02680623353501831, 0.40749829865403864, -0.2425918068537405, -0.32618400866672265, 0.09204553891935288, -0.29037023426376674, -0.19230911073406642, 0.21830605222075655, -0.08457920227297... |
1,801.0154 | Jacob's Ladder: Prime numbers in 2d | Prime numbers are one of the most intriguing figures in mathematics. Despite
centuries of research, many questions remain still unsolved. In recent years,
computer simulations are playing a fundamental role in the study of an immense
variety of problems. In this work, we present a simple representation of prime
numbe... | math.HO | prime numbers are one of the most intriguing figures in mathematics despite centuries of research many questions remain still unsolved in recent years computer simulations are playing a fundamental role in the study of an immense variety of problems in this work we present a simple representation of prime numbers in tw... | [['prime', 'numbers', 'are', 'one', 'of', 'the', 'most', 'intriguing', 'figures', 'in', 'mathematics', 'despite', 'centuries', 'of', 'research', 'many', 'questions', 'remain', 'still', 'unsolved', 'in', 'recent', 'years', 'computer', 'simulations', 'are', 'playing', 'a', 'fundamental', 'role', 'in', 'the', 'study', 'of... | [-0.1943560854853907, 0.13834835228170655, -0.09176057267934085, 0.08441989898293589, -0.05834488199402889, -0.09647326852194965, 0.031573287979699674, 0.33825605812172094, -0.2722357973260417, -0.3548043203478058, 0.07063758941289658, -0.2644084294405184, -0.16888231202494353, 0.2453010411777844, -0.09411379852332175,... |
1,801.01541 | The structure factor of primes | Although the prime numbers are deterministic, they can be viewed, by some
measures, as pseudo-random numbers. In this article, we numerically study the
pair statistics of the primes using statistical-mechanical methods, especially
the structure factor $S(k)$ in an interval $M \leq p \leq M + L$ with $M$
large, and $L... | cond-mat.stat-mech | although the prime numbers are deterministic they can be viewed by some measures as pseudorandom numbers in this article we numerically study the pair statistics of the primes using statisticalmechanical methods especially the structure factor sk in an interval m leq p leq m l with m large and lm smaller than unity we ... | [['although', 'the', 'prime', 'numbers', 'are', 'deterministic', 'they', 'can', 'be', 'viewed', 'by', 'some', 'measures', 'as', 'pseudorandom', 'numbers', 'in', 'this', 'article', 'we', 'numerically', 'study', 'the', 'pair', 'statistics', 'of', 'the', 'primes', 'using', 'statisticalmechanical', 'methods', 'especially',... | [-0.16714455035841372, 0.17378151776298006, -0.08797012390513084, 0.12011896907895647, -0.013446552993682307, -0.1025160250008597, 0.03067573931411154, 0.3572241581507964, -0.2510650992493876, -0.29749076730923024, 0.02989173728364804, -0.30283433652042363, -0.14205423803040815, 0.21310498854870388, -0.0151710526398689... |
1,801.01542 | Congruences of Power Sums | The following congruence for power sums, $S_n(p)$, is well known and has many
applications: $1^n+2^n +\dots +p^n \equiv\begin{cases} -1 \text{ mod } p, &
\text{ if } \ p-1 \ | \ n; 0 \text{ mod } p, & \text{ if } \ p-1 \ \not| \ n,
\end{cases}$ where $n\in{\mathbb N}$ and $p$ is prime. We extend this
congruence, in p... | math.NT | the following congruence for power sums s_np is well known and has many applications 1n2n dots pn equivbegincases 1 text mod p text if p1 n 0 text mod p text if p1 not n endcases where ninmathbb n and p is prime we extend this congruence in particular to the case when p is any power of a prime we also show that the seq... | [['the', 'following', 'congruence', 'for', 'power', 'sums', 's_np', 'is', 'well', 'known', 'and', 'has', 'many', 'applications', '1n2n', 'dots', 'pn', 'equivbegincases', '1', 'text', 'mod', 'p', 'text', 'if', 'p1', 'n', '0', 'text', 'mod', 'p', 'text', 'if', 'p1', 'not', 'n', 'endcases', 'where', 'ninmathbb', 'n', 'and... | [-0.23867289094230185, 0.10751568930005873, -0.03106876457104, 0.024676224263687315, -0.03704232694097347, -0.2575271140856596, -0.030086308359410372, 0.337354862887122, -0.35578446378084744, -0.21146773409050007, 0.03366802970715496, -0.37098140598504575, -0.11025999460744297, 0.15890321164246793, -0.09015473372653707... |
1,801.01543 | Time Dependent Geometry in Massive Gravity | In this paper, we will analyze a time dependent geometry in a massive theory
of gravity. This will be done by analyzing Vaidya space-time in such a massive
theory of gravity. As gravitational collapse is a time dependent system, we
will analyze it using the Vaidya space-time in massive gravity. The Vainshtein
and dRG... | physics.gen-ph | in this paper we will analyze a time dependent geometry in a massive theory of gravity this will be done by analyzing vaidya spacetime in such a massive theory of gravity as gravitational collapse is a time dependent system we will analyze it using the vaidya spacetime in massive gravity the vainshtein and drgt mechani... | [['in', 'this', 'paper', 'we', 'will', 'analyze', 'a', 'time', 'dependent', 'geometry', 'in', 'a', 'massive', 'theory', 'of', 'gravity', 'this', 'will', 'be', 'done', 'by', 'analyzing', 'vaidya', 'spacetime', 'in', 'such', 'a', 'massive', 'theory', 'of', 'gravity', 'as', 'gravitational', 'collapse', 'is', 'a', 'time', ... | [-0.192325676003979, 0.14194725073704664, -0.1452290335035121, 0.16489684958836404, -0.06683952646668662, -0.1091066304678944, -0.028849550475239415, 0.2884540904313326, -0.20154102046720007, -0.26847733213375746, 0.10935840315333652, -0.24379374303601004, -0.20507226883095098, 0.13680812189863487, -0.05791115920398045... |
1,801.01544 | Boundary value problem with measures for fractional elliptic equations
involving source nonlinearities | We are concerned with positive solutions of equation (E) $(-\Delta)^s u=f(u)$
in a domain $\Omega \subset \mathbb{R}^N$ ($N>2s$), where $s \in
(\frac{1}{2},1)$ and $f\in C^{\alpha}_{loc}(\mathbb{R})$ for some $\alpha
\in(0,1)$. We establish a universal a priori estimate for positive solutions of
(E), as well as for t... | math.AP | we are concerned with positive solutions of equation e deltas ufu in a domain omega subset mathbbrn n2s where s in frac121 and fin calpha_locmathbbr for some alpha in01 we establish a universal a priori estimate for positive solutions of e as well as for their gradients then for c2 bounded domain omega we prove the exi... | [['we', 'are', 'concerned', 'with', 'positive', 'solutions', 'of', 'equation', 'e', 'deltas', 'ufu', 'in', 'a', 'domain', 'omega', 'subset', 'mathbbrn', 'n2s', 'where', 's', 'in', 'frac121', 'and', 'fin', 'calpha_locmathbbr', 'for', 'some', 'alpha', 'in01', 'we', 'establish', 'a', 'universal', 'a', 'priori', 'estimate'... | [-0.1815507075823615, 0.11378503724235607, -0.030076552226716662, 0.04571069752800341, -0.06641478701301799, -0.21469888355057298, 0.045256213219322126, 0.3248061931640641, -0.2655834290398959, -0.16638597761183702, 0.11207137173798758, -0.37407157358147797, -0.09582208245856962, 0.1638118265363805, -0.0194015075064098... |
1,801.01545 | Radiation Forces and the Abraham-Minkowski Problem | Recent years have witnessed a number of beautiful experiments in radiation
optics. Our purpose with this mini-review is to highlight some developments of
radiation pressure physics in general, and thereafter to focus on the
importance of the mentioned experiments in regard to the classic
Abraham-Minkowski problem. Th... | physics.class-ph quant-ph | recent years have witnessed a number of beautiful experiments in radiation optics our purpose with this minireview is to highlight some developments of radiation pressure physics in general and thereafter to focus on the importance of the mentioned experiments in regard to the classic abrahamminkowski problem that mean... | [['recent', 'years', 'have', 'witnessed', 'a', 'number', 'of', 'beautiful', 'experiments', 'in', 'radiation', 'optics', 'our', 'purpose', 'with', 'this', 'minireview', 'is', 'to', 'highlight', 'some', 'developments', 'of', 'radiation', 'pressure', 'physics', 'in', 'general', 'and', 'thereafter', 'to', 'focus', 'on', 't... | [-0.09006083764561293, 0.1409167267631778, -0.10904751296308775, 0.07232283389846285, -0.11214507671946794, -0.09176053655617054, -0.0021393885379945186, 0.3694451136572152, -0.2377711232378359, -0.31730067547465934, 0.0634404012246883, -0.29219040916944594, -0.15149104320348153, 0.21333572806156786, -0.072171210365360... |
1,801.01546 | Characterization of distributions of $Q$-independent random variables on
locally compact Abelian groups | Let $X$ be a second countable locally compact Abelian group. We prove some
group analogues of the Skitovich--Darmois, Heyde and Kac--Bernstein
characterisation theorems for $Q$-independent random variables taking values in
the group $X$. The proofs of these theorems are reduced to solving some
functional equations on... | math.PR | let x be a second countable locally compact abelian group we prove some group analogues of the skitovichdarmois heyde and kacbernstein characterisation theorems for qindependent random variables taking values in the group x the proofs of these theorems are reduced to solving some functional equations on the character g... | [['let', 'x', 'be', 'a', 'second', 'countable', 'locally', 'compact', 'abelian', 'group', 'we', 'prove', 'some', 'group', 'analogues', 'of', 'the', 'skitovichdarmois', 'heyde', 'and', 'kacbernstein', 'characterisation', 'theorems', 'for', 'qindependent', 'random', 'variables', 'taking', 'values', 'in', 'the', 'group', ... | [-0.2010213228383621, 0.10636038782719809, -0.16552872425661638, 0.05379361417278862, -0.10593182998351179, -0.09736610362485337, 0.08782834423562655, 0.33665424251767734, -0.3076531443422517, -0.18433134503161105, 0.1607788041247449, -0.2768877579185825, -0.050213568727485836, 0.23387175733156396, -0.1132135286103361,... |
1,801.01547 | Photoevaporating PDR models with the Hydra PDR Code | Recent Herschel and ALMA observations of Photodissociation Regions (PDRs)
have revealed the presence of a high thermal pressure (P ~ 10^7-10^8 K cm-3)
thin compressed layer at the PDR surface where warm molecular tracer emission
(e.g. CH+, SH+, high-J CO, H2,...) originate. These high pressures (unbalanced
by the sur... | astro-ph.GA | recent herschel and alma observations of photodissociation regions pdrs have revealed the presence of a high thermal pressure p 107108 k cm3 thin compressed layer at the pdr surface where warm molecular tracer emission eg ch sh highj co h2 originate these high pressures unbalanced by the surrounding environment and a c... | [['recent', 'herschel', 'and', 'alma', 'observations', 'of', 'photodissociation', 'regions', 'pdrs', 'have', 'revealed', 'the', 'presence', 'of', 'a', 'high', 'thermal', 'pressure', 'p', '107108', 'k', 'cm3', 'thin', 'compressed', 'layer', 'at', 'the', 'pdr', 'surface', 'where', 'warm', 'molecular', 'tracer', 'emission... | [-0.09191255426150746, 0.14032783358037704, -0.042277230931445954, 0.0659418329547625, -0.007775951513089239, -0.08189840616192669, 0.007994129998609423, 0.4489694350035861, -0.2207617028299719, -0.3292491542436182, 0.006074079612269997, -0.2323393061980605, -0.04116549025848508, 0.09392771430499852, 0.0402167342173634... |
1,801.01548 | Frequency Independent Framework for Synthesis of Programmable
Non-reciprocal Networks | Passive and linear nonreciprocal networks at microwave frequencies hold great
promises in enabling new front-end architectures for wireless communication
systems. Their nonreciprocity has been achieved by disrupting the time-reversal
symmetry using various forms of biasing schemes, but only over a limited
frequency r... | eess.SP | passive and linear nonreciprocal networks at microwave frequencies hold great promises in enabling new frontend architectures for wireless communication systems their nonreciprocity has been achieved by disrupting the timereversal symmetry using various forms of biasing schemes but only over a limited frequency range h... | [['passive', 'and', 'linear', 'nonreciprocal', 'networks', 'at', 'microwave', 'frequencies', 'hold', 'great', 'promises', 'in', 'enabling', 'new', 'frontend', 'architectures', 'for', 'wireless', 'communication', 'systems', 'their', 'nonreciprocity', 'has', 'been', 'achieved', 'by', 'disrupting', 'the', 'timereversal', ... | [-0.22634820621201046, 0.09206336882501831, 0.013214495274231589, -0.05329199669138937, -0.11439564298979081, -0.23646927839011062, 0.053171355816662956, 0.47818691607752295, -0.22797249096760647, -0.35159580999811135, 0.049585964224173974, -0.19466990945699938, -0.15618218536147002, 0.28504556325337976, -0.03399109310... |
1,801.01549 | Moving unstable particles and special relativity | In Poincare-Wigner-Dirac theory of relativistic interactions, boosts are
dynamical. This means that - just like time translations - boost
transformations have non-trivial effect on internal variables of interacting
systems. This is different from space translations and rotations, whose actions
are always universal, t... | physics.gen-ph | in poincarewignerdirac theory of relativistic interactions boosts are dynamical this means that just like time translations boost transformations have nontrivial effect on internal variables of interacting systems this is different from space translations and rotations whose actions are always universal trivial and int... | [['in', 'poincarewignerdirac', 'theory', 'of', 'relativistic', 'interactions', 'boosts', 'are', 'dynamical', 'this', 'means', 'that', 'just', 'like', 'time', 'translations', 'boost', 'transformations', 'have', 'nontrivial', 'effect', 'on', 'internal', 'variables', 'of', 'interacting', 'systems', 'this', 'is', 'differen... | [-0.13758866613016024, 0.2496105726828338, -0.13926305871717232, 0.08406841192301863, -0.06958416633067592, -0.14229798448767753, -0.0004922141244645, 0.3859868573966206, -0.29660792645788, -0.2974522608383659, 0.0646118500159793, -0.2523259616366798, -0.10324586619452764, 0.16148154955402377, -0.08809539929072382, 0.0... |
1,801.0155 | An All-Sky Search for Bursts of Very High Energy Gamma Rays with HAWC | A new ground-based wide-field extensive air shower array known as the
High-Altitude Water Cherenkov (HAWC) Observatory promises a new window to
monitoring the $\sim$100 GeV gamma-ray sky with the potential for detecting a
high energy spectral cutoff in gamma-ray bursts (GRBs). It represents a roughly
15 times sensiti... | astro-ph.HE | a new groundbased widefield extensive air shower array known as the highaltitude water cherenkov hawc observatory promises a new window to monitoring the sim100 gev gammaray sky with the potential for detecting a high energy spectral cutoff in gammaray bursts grbs it represents a roughly 15 times sensitivity gain over ... | [['a', 'new', 'groundbased', 'widefield', 'extensive', 'air', 'shower', 'array', 'known', 'as', 'the', 'highaltitude', 'water', 'cherenkov', 'hawc', 'observatory', 'promises', 'a', 'new', 'window', 'to', 'monitoring', 'the', 'sim100', 'gev', 'gammaray', 'sky', 'with', 'the', 'potential', 'for', 'detecting', 'a', 'high'... | [-0.05663466961615576, 0.1638464345127338, -0.014477082368177482, 0.12733392634321578, -0.11832245104611876, -0.09156489775110131, 0.05033045216009785, 0.46351981897575734, -0.14794055364357356, -0.42264837979888303, 0.0700654078149595, -0.3585619578806636, 0.05328173926100135, 0.2646376927251904, 0.020034307074279358,... |
1,801.01551 | Neutrino Astronomy 2017 | This overview of neutrino astronomy emphasizes observation of astrophysical
neutrinos by IceCube and interesting limits on Galactic neutrinos from IceCube
and ANTARES.
| astro-ph.HE | this overview of neutrino astronomy emphasizes observation of astrophysical neutrinos by icecube and interesting limits on galactic neutrinos from icecube and antares | [['this', 'overview', 'of', 'neutrino', 'astronomy', 'emphasizes', 'observation', 'of', 'astrophysical', 'neutrinos', 'by', 'icecube', 'and', 'interesting', 'limits', 'on', 'galactic', 'neutrinos', 'from', 'icecube', 'and', 'antares']] | [-0.0359363009179519, 0.30674798075448384, 0.052797375416213814, 0.3288997440249659, -0.21346777423538946, -0.005317139989611777, 0.06967036476866766, 0.29193754883652384, -0.09246217383241112, -0.4372693252834407, 0.012698520652272484, -0.3922890702431852, -0.026368811387907375, 0.309571774168448, 0.0852821649221534, ... |
1,801.01552 | Asymptotic bounds for spherical codes | The set of all error-correcting codes C over a fixed finite alphabet F of
cardinality q determines the set of code points in the unit square with
coordinates (R(C), delta (C)):= (relative transmission rate, relative minimal
distance). The central problem of the theory of such codes consists in
maximizing simultaneous... | cs.IT math.IT | the set of all errorcorrecting codes c over a fixed finite alphabet f of cardinality q determines the set of code points in the unit square with coordinates rc delta c relative transmission rate relative minimal distance the central problem of the theory of such codes consists in maximizing simultaneously the transmiss... | [['the', 'set', 'of', 'all', 'errorcorrecting', 'codes', 'c', 'over', 'a', 'fixed', 'finite', 'alphabet', 'f', 'of', 'cardinality', 'q', 'determines', 'the', 'set', 'of', 'code', 'points', 'in', 'the', 'unit', 'square', 'with', 'coordinates', 'rc', 'delta', 'c', 'relative', 'transmission', 'rate', 'relative', 'minimal'... | [-0.16550840350954482, 0.04060347024351359, -0.03093010924756527, 0.03810634326888249, 0.00308986767505606, -0.1754596124465267, 0.0916287619736977, 0.3154710678275054, -0.3362034810769061, -0.294790546791628, 0.057586811844957994, -0.27560625611804423, -0.07921297738949458, 0.200178187036654, -0.10543504931692345, 0.0... |
1,801.01553 | Split-gate device for indirect excitons | We present a concept and experimental proof of principle for split-gate
devices for indirect excitons (IXs). The split-gate forms a narrow channel, a
point contact, for IX current. Control of IX flow through the split-gate with
both gate voltage and excitation power is demonstrated.
| cond-mat.mes-hall | we present a concept and experimental proof of principle for splitgate devices for indirect excitons ixs the splitgate forms a narrow channel a point contact for ix current control of ix flow through the splitgate with both gate voltage and excitation power is demonstrated | [['we', 'present', 'a', 'concept', 'and', 'experimental', 'proof', 'of', 'principle', 'for', 'splitgate', 'devices', 'for', 'indirect', 'excitons', 'ixs', 'the', 'splitgate', 'forms', 'a', 'narrow', 'channel', 'a', 'point', 'contact', 'for', 'ix', 'current', 'control', 'of', 'ix', 'flow', 'through', 'the', 'splitgate',... | [-0.20833594096951524, 0.0501245193881914, -0.04957225698639046, -0.011420096807837994, -0.05046951331579211, -0.27134222525637597, 0.11036157520720735, 0.4333547843112187, -0.2660233234901997, -0.25673970444635913, 0.04486795829143375, -0.26650640327187086, -0.08725133961574598, 0.2922351020176641, 0.04176707703366198... |
1,801.01554 | An Implementation of Back-Propagation Learning on GF11, a Large SIMD
Parallel Computer | Current connectionist simulations require huge computational resources. We
describe a neural network simulator for the IBM GF11, an experimental SIMD
machine with 566 processors and a peak arithmetic performance of 11 Gigaflops.
We present our parallel implementation of the backpropagation learning
algorithm, techniq... | cs.LG cs.DC cs.NE | current connectionist simulations require huge computational resources we describe a neural network simulator for the ibm gf11 an experimental simd machine with 566 processors and a peak arithmetic performance of 11 gigaflops we present our parallel implementation of the backpropagation learning algorithm techniques fo... | [['current', 'connectionist', 'simulations', 'require', 'huge', 'computational', 'resources', 'we', 'describe', 'a', 'neural', 'network', 'simulator', 'for', 'the', 'ibm', 'gf11', 'an', 'experimental', 'simd', 'machine', 'with', '566', 'processors', 'and', 'a', 'peak', 'arithmetic', 'performance', 'of', '11', 'gigaflop... | [-0.0973247789478229, 0.006538506415432443, -0.03976982299375211, 0.03320806208424843, -0.06628124615490123, -0.1866899549348892, 0.06982279275674243, 0.41353201111322724, -0.25235649848021435, -0.3909380336038091, 0.08283726589011771, -0.3068315791457865, -0.12829727603943197, 0.2775395614814691, -0.04765933171774332,... |
1,801.01555 | Reeb Posets and Tree Approximations | A well known result in the analysis of finite metric spaces due to Gromov
says that given any $(X,d_X)$ there exists a \emph{tree metric} $t_X$ on $X$
such that $\|d_X-t_X\|_\infty$ is bounded above by twice $\mathrm{hyp}(X)\cdot
\log(2\,|X|)$. Here $\mathrm{hyp}(X)$ is the \emph{hyperbolicity} of $X$, a
quantity tha... | math.MG | a well known result in the analysis of finite metric spaces due to gromov says that given any xd_x there exists a emphtree metric t_x on x such that d_xt_x_infty is bounded above by twice mathrmhypxcdot log2x here mathrmhypx is the emphhyperbolicity of x a quantity that measures the emphtreeness of 4tuples of points in... | [['a', 'well', 'known', 'result', 'in', 'the', 'analysis', 'of', 'finite', 'metric', 'spaces', 'due', 'to', 'gromov', 'says', 'that', 'given', 'any', 'xd_x', 'there', 'exists', 'a', 'emphtree', 'metric', 't_x', 'on', 'x', 'such', 'that', 'd_xt_x_infty', 'is', 'bounded', 'above', 'by', 'twice', 'mathrmhypxcdot', 'log2x'... | [-0.11832935026518389, 0.1481051584030839, -0.09802266985182492, 0.11949170297259186, -0.1170933917524734, -0.11344719271216056, 0.07164459598277682, 0.33996404578981265, -0.33315949914032134, -0.25732696546322625, 0.11228220371511463, -0.2685744195663627, -0.15972025466718429, 0.17581749016841972, -0.16231927562478013... |
1,801.01556 | A bound on the inducibility of cycles | In 1975, Pippenger and Golumbic conjectured that every n-vertex graph has at
most $n^k/(k^k - k)$ induced cycles of length k for k at least 5. We prove that
every n-vertex graph has at most $2 n^k/k^k$ induced cycles of length k.
| math.CO | in 1975 pippenger and golumbic conjectured that every nvertex graph has at most nkkk k induced cycles of length k for k at least 5 we prove that every nvertex graph has at most 2 nkkk induced cycles of length k | [['in', '1975', 'pippenger', 'and', 'golumbic', 'conjectured', 'that', 'every', 'nvertex', 'graph', 'has', 'at', 'most', 'nkkk', 'k', 'induced', 'cycles', 'of', 'length', 'k', 'for', 'k', 'at', 'least', '5', 'we', 'prove', 'that', 'every', 'nvertex', 'graph', 'has', 'at', 'most', '2', 'nkkk', 'induced', 'cycles', 'of',... | [-0.2687404568856343, 0.21946145644268164, -0.05776787992232503, -0.06143265560221595, 0.009496351298040304, -0.18805512633079138, 0.026799671351909637, 0.3912965720280623, -0.24009392059479767, -0.34497419921442485, 0.04843612707470758, -0.4099581170445069, -0.13462801125999063, 0.1460700857285888, -0.0180955985799813... |
1,801.01557 | Plan in 2D, execute in 3D: An augmented reality solution for cup
placement in total hip arthroplasty | Reproducibly achieving proper implant alignment is a critical step in total
hip arthroplasty (THA) procedures that has been shown to substantially affect
patient outcome. In current practice, correct alignment of the acetabular cup
is verified in C-arm X-ray images that are acquired in an anterior-posterior
(AP) view... | cs.CV | reproducibly achieving proper implant alignment is a critical step in total hip arthroplasty tha procedures that has been shown to substantially affect patient outcome in current practice correct alignment of the acetabular cup is verified in carm xray images that are acquired in an anteriorposterior ap view favorable ... | [['reproducibly', 'achieving', 'proper', 'implant', 'alignment', 'is', 'a', 'critical', 'step', 'in', 'total', 'hip', 'arthroplasty', 'tha', 'procedures', 'that', 'has', 'been', 'shown', 'to', 'substantially', 'affect', 'patient', 'outcome', 'in', 'current', 'practice', 'correct', 'alignment', 'of', 'the', 'acetabular'... | [-0.07854689114015934, 0.03441501362518149, -0.07096488158086962, -0.008402748720824171, -0.09272102115842838, -0.13952954019085786, 0.06876377376560729, 0.4354901517078321, -0.1800453866369777, -0.358364914726142, 0.10789440817145236, -0.26348808577344957, -0.1474794936005745, 0.19604700608381434, -0.18168707556374694... |
1,801.01558 | TopP-S: Persistent homology based multi-task deep neural networks for
simultaneous predictions of partition coefficient and aqueous solubility | Aqueous solubility and partition coefficient are important physical
properties of small molecules. Accurate theoretical prediction of aqueous
solubility and partition coefficient plays an important role in drug design and
discovery. The prediction accuracy depends crucially on molecular descriptors
which are typicall... | q-bio.QM | aqueous solubility and partition coefficient are important physical properties of small molecules accurate theoretical prediction of aqueous solubility and partition coefficient plays an important role in drug design and discovery the prediction accuracy depends crucially on molecular descriptors which are typically de... | [['aqueous', 'solubility', 'and', 'partition', 'coefficient', 'are', 'important', 'physical', 'properties', 'of', 'small', 'molecules', 'accurate', 'theoretical', 'prediction', 'of', 'aqueous', 'solubility', 'and', 'partition', 'coefficient', 'plays', 'an', 'important', 'role', 'in', 'drug', 'design', 'and', 'discovery... | [-0.07149260032631506, 0.05492596453649663, -0.07972025521309734, 0.044143125886175846, -0.09191051121405532, -0.14079498471403742, 0.03000307985026682, 0.3951447098392301, -0.27379672952352785, -0.3074164122461024, 0.06351478902475735, -0.24228603828006087, -0.19556528272336984, 0.1841097359784541, -0.0688198448954133... |
1,801.01559 | Fingerprints of Berry phases in the bulk exciton spectrum of a
topological insulator | We examine excitons formed in the bulk of a topological insulator as the
system is tuned via a parameter between topological and trivial insulating
phases, arguing that nontrivial topology has fingerprints in the spectrum of
these excitons. The closely related hydrogen atom problem is well known to have
a degeneracy ... | cond-mat.mes-hall | we examine excitons formed in the bulk of a topological insulator as the system is tuned via a parameter between topological and trivial insulating phases arguing that nontrivial topology has fingerprints in the spectrum of these excitons the closely related hydrogen atom problem is well known to have a degeneracy due ... | [['we', 'examine', 'excitons', 'formed', 'in', 'the', 'bulk', 'of', 'a', 'topological', 'insulator', 'as', 'the', 'system', 'is', 'tuned', 'via', 'a', 'parameter', 'between', 'topological', 'and', 'trivial', 'insulating', 'phases', 'arguing', 'that', 'nontrivial', 'topology', 'has', 'fingerprints', 'in', 'the', 'spectr... | [-0.15395542035553733, 0.1757355291139463, -0.10475261039010265, 0.07127000303248522, -0.05087122565199589, -0.15320033234511984, 0.0708131237373013, 0.3440103875151996, -0.28507519497311323, -0.2952801214017231, 0.05179656325550429, -0.2740109947847267, -0.1926399219588473, 0.14398205714773965, -0.01861004880790053, 0... |
1,801.0156 | On-the-fly Augmented Reality for Orthopaedic Surgery Using a Multi-Modal
Fiducial | Fluoroscopic X-ray guidance is a cornerstone for percutaneous orthopaedic
surgical procedures. However, two-dimensional observations of the
three-dimensional anatomy suffer from the effects of projective simplification.
Consequently, many X-ray images from various orientations need to be acquired
for the surgeon to a... | cs.CV | fluoroscopic xray guidance is a cornerstone for percutaneous orthopaedic surgical procedures however twodimensional observations of the threedimensional anatomy suffer from the effects of projective simplification consequently many xray images from various orientations need to be acquired for the surgeon to accurately ... | [['fluoroscopic', 'xray', 'guidance', 'is', 'a', 'cornerstone', 'for', 'percutaneous', 'orthopaedic', 'surgical', 'procedures', 'however', 'twodimensional', 'observations', 'of', 'the', 'threedimensional', 'anatomy', 'suffer', 'from', 'the', 'effects', 'of', 'projective', 'simplification', 'consequently', 'many', 'xray... | [-0.03473540480740774, 0.02626825074355727, -0.08230669657982251, 0.04084582477052127, -0.10893215621508198, -0.13300258001109577, 0.04370402890727613, 0.4239229245808735, -0.22142805028359197, -0.3488404606535183, 0.11953005214305638, -0.25154650458509886, -0.20222302558456692, 0.25698983421222577, -0.1310222609781746... |
1,801.01561 | Multiplicity freeness of unitary representations in sections of
holomorphic Hilbert bundles | We prove several results asserting that the action of a Banach-Lie group on
Hilbert spaces of holomorphic sections of a holomorphic Hilbert space bundle
over a complex Banach manifold is multiplicity free. These results require the
existence of compatible antiholomorphic bundle maps and certain multiplicity
freeness ... | math.RT math.OA | we prove several results asserting that the action of a banachlie group on hilbert spaces of holomorphic sections of a holomorphic hilbert space bundle over a complex banach manifold is multiplicity free these results require the existence of compatible antiholomorphic bundle maps and certain multiplicity freeness assu... | [['we', 'prove', 'several', 'results', 'asserting', 'that', 'the', 'action', 'of', 'a', 'banachlie', 'group', 'on', 'hilbert', 'spaces', 'of', 'holomorphic', 'sections', 'of', 'a', 'holomorphic', 'hilbert', 'space', 'bundle', 'over', 'a', 'complex', 'banach', 'manifold', 'is', 'multiplicity', 'free', 'these', 'results'... | [-0.18021594549084954, 0.07174017959273818, -0.10617432682219585, 0.09103728311858353, -0.11651007530339268, -0.10015518664288411, -0.013846980775236536, 0.4029042271346093, -0.27407910107259015, -0.19619451699043633, 0.12025621277280152, -0.23292690371120467, -0.15324861898915756, 0.24312967541542144, -0.1850279529126... |
1,801.01562 | The Distortion of the Reeb Quotient Map on Riemannian Manifolds | Given a metric space $X$ and a function $f: X \to \mathbb{R}$, the Reeb
construction gives metric a space $X_f$ together with a quotient map $X \to
X_f$. Under suitable conditions $X_f$ becomes a metric graph and can therefore
be used as a graph approximation to $X$. The Gromov-Hausdorff distance from
$X_f$ to $X$ is... | math.MG math.DG | given a metric space x and a function f x to mathbbr the reeb construction gives metric a space x_f together with a quotient map x to x_f under suitable conditions x_f becomes a metric graph and can therefore be used as a graph approximation to x the gromovhausdorff distance from x_f to x is bounded by the half of the ... | [['given', 'a', 'metric', 'space', 'x', 'and', 'a', 'function', 'f', 'x', 'to', 'mathbbr', 'the', 'reeb', 'construction', 'gives', 'metric', 'a', 'space', 'x_f', 'together', 'with', 'a', 'quotient', 'map', 'x', 'to', 'x_f', 'under', 'suitable', 'conditions', 'x_f', 'becomes', 'a', 'metric', 'graph', 'and', 'can', 'ther... | [-0.1782612031748315, 0.07210664097877599, -0.13202280391539847, 0.06745934366354202, -0.0881040423126312, -0.08315742358627941, 0.04544614060261451, 0.3901217831063922, -0.32652296017495397, -0.20509731556688035, 0.06099345479669253, -0.26522128253455174, -0.14248621632822422, 0.1658043723060366, -0.14326131494105362,... |
1,801.01563 | DENSER: Deep Evolutionary Network Structured Representation | Deep Evolutionary Network Structured Representation (DENSER) is a novel
approach to automatically design Artificial Neural Networks (ANNs) using
Evolutionary Computation. The algorithm not only searches for the best network
topology (e.g., number of layers, type of layers), but also tunes
hyper-parameters, such as, l... | cs.NE | deep evolutionary network structured representation denser is a novel approach to automatically design artificial neural networks anns using evolutionary computation the algorithm not only searches for the best network topology eg number of layers type of layers but also tunes hyperparameters such as learning parameter... | [['deep', 'evolutionary', 'network', 'structured', 'representation', 'denser', 'is', 'a', 'novel', 'approach', 'to', 'automatically', 'design', 'artificial', 'neural', 'networks', 'anns', 'using', 'evolutionary', 'computation', 'the', 'algorithm', 'not', 'only', 'searches', 'for', 'the', 'best', 'network', 'topology', ... | [-0.05846507364262931, 0.03245050693000481, -0.003540191702802289, 0.04769129326512562, -0.10051805770490319, -0.15316914126494938, 0.04291693083607552, 0.45003909962449934, -0.2552484809321926, -0.3706862844348429, 0.07388598716847519, -0.24296787996934924, -0.1949113209030908, 0.20882848260721112, -0.052943056117851,... |
1,801.01564 | Expansion of Iterated Stratonovich Stochastic Integrals of Multiplicity
3 Based on Generalized Multiple Fourier Series Converging in the Mean:
General Case of Series Summation | The article is devoted to the development of the method of expansion and
mean-square approximation of iterated Ito stochastic integrals based on
generalized multiple Fourier series converging in the mean. We adapt this
method for iterated Stratonovich stochastic integrals of multiplicity 3 from
the Taylor-Stratonovic... | math.PR | the article is devoted to the development of the method of expansion and meansquare approximation of iterated ito stochastic integrals based on generalized multiple fourier series converging in the mean we adapt this method for iterated stratonovich stochastic integrals of multiplicity 3 from the taylorstratonovich exp... | [['the', 'article', 'is', 'devoted', 'to', 'the', 'development', 'of', 'the', 'method', 'of', 'expansion', 'and', 'meansquare', 'approximation', 'of', 'iterated', 'ito', 'stochastic', 'integrals', 'based', 'on', 'generalized', 'multiple', 'fourier', 'series', 'converging', 'in', 'the', 'mean', 'we', 'adapt', 'this', 'm... | [-0.12878051454779402, -0.012855928463475972, -0.12663130345553608, 0.03870991171851497, -0.062414913622919344, -0.014610221273273808, -0.010865022841808868, 0.3069246381778142, -0.3001854001656817, -0.22779067209118914, 0.1242571564186525, -0.2577504156526692, -0.1931225609933508, 0.2424452350974677, -0.08713995873655... |
1,801.01565 | A Study on the Use of Eye Tracking to Adapt Gameplay and Procedural
Content Generation in First-Person Shooter Games | This paper studies the use of eye tracking in a First-Person Shooter (FPS)
game as a~mechanism to: (1) control the attention of the player's avatar
according to the attention deployed by the player, and (2) guide the gameplay
and game's procedural content generation, accordingly. This results in a more
natural use of... | cs.HC | this paper studies the use of eye tracking in a firstperson shooter fps game as amechanism to 1 control the attention of the players avatar according to the attention deployed by the player and 2 guide the gameplay and games procedural content generation accordingly this results in a more natural use of eye tracking in... | [['this', 'paper', 'studies', 'the', 'use', 'of', 'eye', 'tracking', 'in', 'a', 'firstperson', 'shooter', 'fps', 'game', 'as', 'amechanism', 'to', '1', 'control', 'the', 'attention', 'of', 'the', 'players', 'avatar', 'according', 'to', 'the', 'attention', 'deployed', 'by', 'the', 'player', 'and', '2', 'guide', 'the', '... | [-0.041163208747662584, 0.024329057404077956, -0.1372689062163828, 0.03997536582738001, -0.10974643380592572, -0.21887918004331872, 0.03841024585870992, 0.4375735314968585, -0.198398182340012, -0.3696599105498725, 0.10864024891652327, -0.29326087666641165, -0.18522656666960544, 0.17212573348036025, -0.1966409260504222,... |
1,801.01566 | Adaptive Finite Element Solution of the Porous Medium Equation in
Pressure Formulation | A lack of regularity in the solution of the porous medium equation poses a
serious challenge in its theoretical and numerical studies. A common strategy
in theoretical studies is to utilize the pressure formulation of the equation
where a new variable called the mathematical pressure is introduced. It is
known that t... | math.NA | a lack of regularity in the solution of the porous medium equation poses a serious challenge in its theoretical and numerical studies a common strategy in theoretical studies is to utilize the pressure formulation of the equation where a new variable called the mathematical pressure is introduced it is known that the n... | [['a', 'lack', 'of', 'regularity', 'in', 'the', 'solution', 'of', 'the', 'porous', 'medium', 'equation', 'poses', 'a', 'serious', 'challenge', 'in', 'its', 'theoretical', 'and', 'numerical', 'studies', 'a', 'common', 'strategy', 'in', 'theoretical', 'studies', 'is', 'to', 'utilize', 'the', 'pressure', 'formulation', 'o... | [-0.08420057382873089, 0.0629940802459732, -0.11703142900042986, 0.030490112726047548, -0.08073874539514489, -0.11965974097607607, 0.009462070165193869, 0.3627926570790048, -0.30622156680260826, -0.26611324903058753, 0.14143612801916317, -0.25564666696577715, -0.1321917573354254, 0.18180309227171285, -0.095297979022437... |
1,801.01567 | Spatial Variations in the Dust-to-Gas Ratio of Enceladus' Plume | On day 138 of 2010, the plume of dust and gas emerging from Enceladus' South
Polar Terrain passed between the Sun and the Cassini spacecraft. This solar
occultation enabled Cassini's Ultraviolet Imaging Spectrograph (UVIS) and the
Visual and Infrared Mapping Spectrometer (VIMS) to obtain simultaneous
measurements of ... | astro-ph.EP | on day 138 of 2010 the plume of dust and gas emerging from enceladus south polar terrain passed between the sun and the cassini spacecraft this solar occultation enabled cassinis ultraviolet imaging spectrograph uvis and the visual and infrared mapping spectrometer vims to obtain simultaneous measurements of the plumes... | [['on', 'day', '138', 'of', '2010', 'the', 'plume', 'of', 'dust', 'and', 'gas', 'emerging', 'from', 'enceladus', 'south', 'polar', 'terrain', 'passed', 'between', 'the', 'sun', 'and', 'the', 'cassini', 'spacecraft', 'this', 'solar', 'occultation', 'enabled', 'cassinis', 'ultraviolet', 'imaging', 'spectrograph', 'uvis',... | [-0.07023623142657535, 0.16824996366943065, -0.07000765488683967, 0.01422966159159495, -0.04485594519258787, -0.04117265700894807, 0.002451697160999867, 0.39130951024458877, -0.1901285495179417, -0.38339181233286146, 0.1022160175444913, -0.3083180957606861, -0.09300563067109102, 0.20207922357478222, -0.1045343142978492... |
1,801.01568 | Computational Higher Type Theory IV: Inductive Types | This is the fourth in a series of papers extending Martin-L\"of's meaning
explanation of dependent type theory to higher-dimensional types. In this
installment, we show how to define cubical type systems supporting a general
schema of indexed cubical inductive types whose constructors may take dimension
parameters an... | cs.LO | this is the fourth in a series of papers extending martinlofs meaning explanation of dependent type theory to higherdimensional types in this installment we show how to define cubical type systems supporting a general schema of indexed cubical inductive types whose constructors may take dimension parameters and have a ... | [['this', 'is', 'the', 'fourth', 'in', 'a', 'series', 'of', 'papers', 'extending', 'martinlofs', 'meaning', 'explanation', 'of', 'dependent', 'type', 'theory', 'to', 'higherdimensional', 'types', 'in', 'this', 'installment', 'we', 'show', 'how', 'to', 'define', 'cubical', 'type', 'systems', 'supporting', 'a', 'general'... | [-0.11620484789969718, 0.055663145645755835, -0.04416695130114421, 0.09479443566368256, -0.12528770200045006, -0.14632255407674918, 0.030227077686903636, 0.304300001779821, -0.268373545043443, -0.2882781906845616, 0.08324159392107437, -0.20301019440535684, -0.14893772816832074, 0.18609458358572206, -0.14526853641273635... |
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