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 |
|---|---|---|---|---|---|---|
706.1314 | When Did Cosmic Acceleration Start ? | A precise determination, and comparison, of the epoch of the onset of cosmic
acceleration, at redshift z_acc, and of dark energy domination, at z_eq,
provides an interesting measure with which to parameterize dark energy models.
By combining several cosmological datasets we place constraints on the redshift
and age o... | astro-ph gr-qc hep-ph | a precise determination and comparison of the epoch of the onset of cosmic acceleration at redshift z_acc and of dark energy domination at z_eq provides an interesting measure with which to parameterize dark energy models by combining several cosmological datasets we place constraints on the redshift and age of cosmolo... | [['a', 'precise', 'determination', 'and', 'comparison', 'of', 'the', 'epoch', 'of', 'the', 'onset', 'of', 'cosmic', 'acceleration', 'at', 'redshift', 'z_acc', 'and', 'of', 'dark', 'energy', 'domination', 'at', 'z_eq', 'provides', 'an', 'interesting', 'measure', 'with', 'which', 'to', 'parameterize', 'dark', 'energy', '... | [-0.08764898034384136, 0.11816140904464356, -0.11804494870064611, 0.11815069805492054, -0.05668023995293135, -0.12349402892763134, 0.06722993510986933, 0.3364358917217363, -0.19841500668024475, -0.4347867976366119, 0.052470602859234945, -0.23603690986267545, 0.06460615901107138, 0.18369200155773963, 0.03048261851072311... |
706.1315 | The Dirac system on the Anti-de Sitter Universe | We investigate the global solutions of the Dirac equation on the
Anti-de-Sitter Universe. Since this space is not globally hyperbolic, the
Cauchy problem is not, {\it a priori}, well-posed. Nevertheless we can prove
that there exists unitary dynamics, but its uniqueness crucially depends on the
ratio beween the mass ... | math-ph math.AP math.MP | we investigate the global solutions of the dirac equation on the antidesitter universe since this space is not globally hyperbolic the cauchy problem is not it a priori wellposed nevertheless we can prove that there exists unitary dynamics but its uniqueness crucially depends on the ratio beween the mass m of the field... | [['we', 'investigate', 'the', 'global', 'solutions', 'of', 'the', 'dirac', 'equation', 'on', 'the', 'antidesitter', 'universe', 'since', 'this', 'space', 'is', 'not', 'globally', 'hyperbolic', 'the', 'cauchy', 'problem', 'is', 'not', 'it', 'a', 'priori', 'wellposed', 'nevertheless', 'we', 'can', 'prove', 'that', 'there... | [-0.2019515800796124, 0.14643365251905624, -0.1057653877595883, 0.11209135518283657, -0.06799156057818365, -0.13635020562270211, -0.00742387194334278, 0.3052842790881793, -0.24652071952420687, -0.22695651005894418, 0.1229944216093928, -0.26609417861918844, -0.13401380845803826, 0.16590909540675403, -0.02247153987945427... |
706.1316 | Coupling of Optical Lumped Nanocircuit Elements and Effects of
Substrates | We present here a model for the coupling among small nanoparticles excited by
an optical electric field in the framework of our optical lumped nanocircuit
theory [N. Engheta, A. Salandrino, and A. Alu Phys. Rev. Lett. 95, 095504
(2005)]. We derive how this coupling affects the corresponding nanocircuit
model by addin... | cond-mat.mtrl-sci | we present here a model for the coupling among small nanoparticles excited by an optical electric field in the framework of our optical lumped nanocircuit theory n engheta a salandrino and a alu phys rev lett 95 095504 2005 we derive how this coupling affects the corresponding nanocircuit model by adding controlled sou... | [['we', 'present', 'here', 'a', 'model', 'for', 'the', 'coupling', 'among', 'small', 'nanoparticles', 'excited', 'by', 'an', 'optical', 'electric', 'field', 'in', 'the', 'framework', 'of', 'our', 'optical', 'lumped', 'nanocircuit', 'theory', 'n', 'engheta', 'a', 'salandrino', 'and', 'a', 'alu', 'phys', 'rev', 'lett', '... | [-0.10665342995032136, 0.15606039330525942, -0.008314916302749355, -0.0744779676284192, -0.019877134568689923, -0.13712212907349958, 0.09079105229102424, 0.4083804573165253, -0.18420216894134814, -0.3254606704493718, 0.008551198750085729, -0.26511528025730513, -0.197810546688353, 0.20196361116541084, -0.039785346336429... |
706.1317 | A model for learning to segment temporal sequences, utilizing a mixture
of RNN experts together with adaptive variance | This paper proposes a novel learning method for a mixture of recurrent neural
network (RNN) experts model, which can acquire the ability to generate desired
sequences by dynamically switching between experts. Our method is based on
maximum likelihood estimation, using a gradient descent algorithm. This
approach is si... | nlin.AO | this paper proposes a novel learning method for a mixture of recurrent neural network rnn experts model which can acquire the ability to generate desired sequences by dynamically switching between experts our method is based on maximum likelihood estimation using a gradient descent algorithm this approach is similar to... | [['this', 'paper', 'proposes', 'a', 'novel', 'learning', 'method', 'for', 'a', 'mixture', 'of', 'recurrent', 'neural', 'network', 'rnn', 'experts', 'model', 'which', 'can', 'acquire', 'the', 'ability', 'to', 'generate', 'desired', 'sequences', 'by', 'dynamically', 'switching', 'between', 'experts', 'our', 'method', 'is... | [-0.018284802690839336, 0.009443171508610248, -0.11647182848574894, 0.04438220439028115, -0.11345679904784887, -0.1788291748162479, 0.05969597338849018, 0.4170016152724143, -0.2924999794231788, -0.33835250032322123, 0.05205493386564476, -0.19635820453986524, -0.23779327389033092, 0.21998049083406165, -0.122448197025204... |
706.1318 | Constructing a maximum utility slate of on-line advertisements | We present an algorithm for constructing an optimal slate of sponsored search
advertisements which respects the ordering that is the outcome of a generalized
second price auction, but which must also accommodate complicating factors such
as overall budget constraints. The algorithm is easily fast enough to use on
the... | cs.DM cs.DS | we present an algorithm for constructing an optimal slate of sponsored search advertisements which respects the ordering that is the outcome of a generalized second price auction but which must also accommodate complicating factors such as overall budget constraints the algorithm is easily fast enough to use on the fly... | [['we', 'present', 'an', 'algorithm', 'for', 'constructing', 'an', 'optimal', 'slate', 'of', 'sponsored', 'search', 'advertisements', 'which', 'respects', 'the', 'ordering', 'that', 'is', 'the', 'outcome', 'of', 'a', 'generalized', 'second', 'price', 'auction', 'but', 'which', 'must', 'also', 'accommodate', 'complicati... | [-0.07965052640159434, 0.05054909288165002, -0.09248114884981225, 0.10120176949403098, -0.15939386050036597, -0.13963463845392388, 0.11440303572829091, 0.40752446661973674, -0.30625990664045655, -0.3642979626273436, 0.153318430452923, -0.21592015158685465, -0.15840933672077354, 0.19856278123071178, -0.0871547237339039,... |
706.1319 | Dealing with delicate issues in waveforms calculations | We revisit the calculation of gravitational radiation through the use of Weyl
scalars. We point out several possible problems arising from gauge and tetrad
ambiguities and ways to address them. Our analysis indicates how, relatively
simple corrections can be introduced to remove these ambiguities.
| gr-qc | we revisit the calculation of gravitational radiation through the use of weyl scalars we point out several possible problems arising from gauge and tetrad ambiguities and ways to address them our analysis indicates how relatively simple corrections can be introduced to remove these ambiguities | [['we', 'revisit', 'the', 'calculation', 'of', 'gravitational', 'radiation', 'through', 'the', 'use', 'of', 'weyl', 'scalars', 'we', 'point', 'out', 'several', 'possible', 'problems', 'arising', 'from', 'gauge', 'and', 'tetrad', 'ambiguities', 'and', 'ways', 'to', 'address', 'them', 'our', 'analysis', 'indicates', 'how... | [-0.09597396160560576, 0.11082875022177839, -0.1023640452503142, 0.11581968434620649, -0.1764329848387702, -0.11303248291369528, 0.07903307104821909, 0.3594948551194234, -0.2894048248841004, -0.29423399752175267, 0.045194913358004254, -0.2806964546696029, -0.17501747218722646, 0.1560603161342442, -0.07720992108806968, ... |
706.132 | Accretion vs colliding wind models for the gamma-ray binary LS I +61
303: an assessment | LS I +61 303 is a puzzling Be/X-ray binary with variable gamma-ray emission
at up TeV energies. The nature of the compact object and the origin of the
high-energy emission are unclear. One family of models invokes particle
acceleration in shocks from the collision between the B-star wind and a
relativistic pulsar win... | astro-ph | ls i 61 303 is a puzzling bexray binary with variable gammaray emission at up tev energies the nature of the compact object and the origin of the highenergy emission are unclear one family of models invokes particle acceleration in shocks from the collision between the bstar wind and a relativistic pulsar wind while an... | [['ls', 'i', '61', '303', 'is', 'a', 'puzzling', 'bexray', 'binary', 'with', 'variable', 'gammaray', 'emission', 'at', 'up', 'tev', 'energies', 'the', 'nature', 'of', 'the', 'compact', 'object', 'and', 'the', 'origin', 'of', 'the', 'highenergy', 'emission', 'are', 'unclear', 'one', 'family', 'of', 'models', 'invokes', ... | [-0.0913058519271276, 0.09820704813821537, -0.08545866813644659, 0.12689852712402896, -0.0930592215899713, -0.13616821939324986, 0.016488550291162172, 0.3903234618977248, -0.21959701057845096, -0.32467163188078124, 0.0529688381541373, -0.28720768722337037, -0.04895451614833056, 0.23086153235154147, -0.00474962375709693... |
706.1321 | Detailed study of the GRB 030329 radio afterglow deep into the
non-relativistic phase | We explore the physics behind one of the brightest radio afterglows ever, GRB
030329, at late times when the jet is non-relativistic. We determine the
physical parameters of the blast wave and its surroundings, in particular the
index of the electron energy distribution, the energy of the blast wave, and
the density ... | astro-ph | we explore the physics behind one of the brightest radio afterglows ever grb 030329 at late times when the jet is nonrelativistic we determine the physical parameters of the blast wave and its surroundings in particular the index of the electron energy distribution the energy of the blast wave and the density structure... | [['we', 'explore', 'the', 'physics', 'behind', 'one', 'of', 'the', 'brightest', 'radio', 'afterglows', 'ever', 'grb', '030329', 'at', 'late', 'times', 'when', 'the', 'jet', 'is', 'nonrelativistic', 'we', 'determine', 'the', 'physical', 'parameters', 'of', 'the', 'blast', 'wave', 'and', 'its', 'surroundings', 'in', 'par... | [-0.07728674905433097, 0.14695570774660854, -0.06474423441630651, 0.0936118108770814, -0.11651788965923611, -0.06211636047303739, 0.027093875904813033, 0.4697406411046264, -0.1847089973898657, -0.312401057813301, 0.08557487622041754, -0.29805405062689566, -0.03976029857591761, 0.20318698905755192, 0.06613333714384562, ... |
706.1322 | Thermodynamics and the virial expansion for trapped fluids in arbitrary
external potentials | We present the full thermodynamics of a fluid confined by an arbitrary
external potential based on the virial expansion of the grand potential. The
fluid may be classical or quantum and it is assumed that interatomic
interactions are pairwise additive. We indicate how the appropriate
"generalized" volume and pressure... | cond-mat.stat-mech | we present the full thermodynamics of a fluid confined by an arbitrary external potential based on the virial expansion of the grand potential the fluid may be classical or quantum and it is assumed that interatomic interactions are pairwise additive we indicate how the appropriate generalized volume and pressure varia... | [['we', 'present', 'the', 'full', 'thermodynamics', 'of', 'a', 'fluid', 'confined', 'by', 'an', 'arbitrary', 'external', 'potential', 'based', 'on', 'the', 'virial', 'expansion', 'of', 'the', 'grand', 'potential', 'the', 'fluid', 'may', 'be', 'classical', 'or', 'quantum', 'and', 'it', 'is', 'assumed', 'that', 'interato... | [-0.12084122949470115, 0.1310470310424427, -0.12501190556369732, 0.05206548674432661, -0.02001375800889907, -0.08228350029907801, 0.08079266990534961, 0.32143248229097293, -0.2700270838279437, -0.25811957894393833, 0.0848741199262941, -0.2730721173637737, -0.12910214727944744, 0.15463755081372677, -0.019011792616658314... |
706.1323 | GRB 030329: 3 years of radio afterglow monitoring | Radio observations of gamma-ray burst (GRB) afterglows are essential for our
understanding of the physics of relativistic blast waves, as they enable us to
follow the evolution of GRB explosions much longer than the afterglows in any
other wave band. We have performed a three-year monitoring campaign of GRB
030329 wi... | astro-ph | radio observations of gammaray burst grb afterglows are essential for our understanding of the physics of relativistic blast waves as they enable us to follow the evolution of grb explosions much longer than the afterglows in any other wave band we have performed a threeyear monitoring campaign of grb 030329 with the w... | [['radio', 'observations', 'of', 'gammaray', 'burst', 'grb', 'afterglows', 'are', 'essential', 'for', 'our', 'understanding', 'of', 'the', 'physics', 'of', 'relativistic', 'blast', 'waves', 'as', 'they', 'enable', 'us', 'to', 'follow', 'the', 'evolution', 'of', 'grb', 'explosions', 'much', 'longer', 'than', 'the', 'aft... | [-0.06980711375108015, 0.13443406393962007, -0.06735555693660289, 0.15249418477808468, -0.2104376890466944, -0.09408238856440844, 0.026478295056595887, 0.49789734450105116, -0.1260565240765373, -0.31793281363246784, 0.07555720358624518, -0.2816471006076987, -0.02523011432431179, 0.26056779355563425, 0.08632264442882207... |
706.1324 | GRB 030329: three years of radio afterglow monitoring | Radio observations of gamma-ray burst (GRB) afterglows are essential for our
understanding of the physics of relativistic blast waves, as they enable us to
follow the evolution of GRB explosions much longer than the afterglows in any
other wave band. We have performed a three-year monitoring campaign of GRB
030329 wi... | astro-ph | radio observations of gammaray burst grb afterglows are essential for our understanding of the physics of relativistic blast waves as they enable us to follow the evolution of grb explosions much longer than the afterglows in any other wave band we have performed a threeyear monitoring campaign of grb 030329 with the w... | [['radio', 'observations', 'of', 'gammaray', 'burst', 'grb', 'afterglows', 'are', 'essential', 'for', 'our', 'understanding', 'of', 'the', 'physics', 'of', 'relativistic', 'blast', 'waves', 'as', 'they', 'enable', 'us', 'to', 'follow', 'the', 'evolution', 'of', 'grb', 'explosions', 'much', 'longer', 'than', 'the', 'aft... | [-0.07326672201165232, 0.13710296679395853, -0.06644633380683507, 0.15127575167195023, -0.20904909253126758, -0.09655383358817218, 0.030050600449662325, 0.4986876045562783, -0.12682082671925526, -0.3210867624983293, 0.07650134150417154, -0.2767937420297186, -0.021860161500026277, 0.2596363197334212, 0.08319243812477406... |
706.1325 | Possible astronomical references in the planning of the Great Hopewell
Road | The possible existence of astronomical references in the planning of the
so-called Great Hopewell Road, a 90 Kilometres straight road composed of two
parallel earthen embankments which, according to recent surveys, likely
connected the Hopewell ceremonial centres of Newark and Chillicothe, Ohio, are
investigated. It ... | physics.hist-ph | the possible existence of astronomical references in the planning of the socalled great hopewell road a 90 kilometres straight road composed of two parallel earthen embankments which according to recent surveys likely connected the hopewell ceremonial centres of newark and chillicothe ohio are investigated it turns out... | [['the', 'possible', 'existence', 'of', 'astronomical', 'references', 'in', 'the', 'planning', 'of', 'the', 'socalled', 'great', 'hopewell', 'road', 'a', '90', 'kilometres', 'straight', 'road', 'composed', 'of', 'two', 'parallel', 'earthen', 'embankments', 'which', 'according', 'to', 'recent', 'surveys', 'likely', 'con... | [-0.15725822088780342, 0.10051286580379713, -0.073049169674806, 0.032640706310834884, -0.12182529234363661, -0.08966978786924443, 0.09172457392484724, 0.36465959301726386, -0.20394604618346632, -0.3105288463547923, 0.11261953106119793, -0.2619359239761252, -0.1178839396709552, 0.20971600042637922, -0.047112344461795574... |
706.1326 | The oscillation stability problem for the Urysohn sphere: A
combinatorial approach | We study the oscillation stability problem for the Urysohn sphere, an analog
of the distortion problem for $\ell_2$ in the context of the Urysohn space
$\Ur$. In particular, we show that this problem reduces to a purely
combinatorial problem involving a family of countable ultrahomogeneous metric
spaces with finitely... | math.MG math.CO | we study the oscillation stability problem for the urysohn sphere an analog of the distortion problem for ell_2 in the context of the urysohn space ur in particular we show that this problem reduces to a purely combinatorial problem involving a family of countable ultrahomogeneous metric spaces with finitely many dista... | [['we', 'study', 'the', 'oscillation', 'stability', 'problem', 'for', 'the', 'urysohn', 'sphere', 'an', 'analog', 'of', 'the', 'distortion', 'problem', 'for', 'ell_2', 'in', 'the', 'context', 'of', 'the', 'urysohn', 'space', 'ur', 'in', 'particular', 'we', 'show', 'that', 'this', 'problem', 'reduces', 'to', 'a', 'purel... | [-0.13937179489613638, 0.060771577925633584, -0.0663890438336952, 0.11373204996069784, -0.10012996897977941, -0.040325440685538685, 0.03521738057116083, 0.3519413612152943, -0.4058348304208587, -0.2054218072672466, 0.1350212039873369, -0.2956190697081825, -0.18009708445592254, 0.2223524629040256, -0.1660750932699325, 0... |
706.1327 | Hopf Algebras of Heap Ordered Trees and Permutations | It is known that there is a Hopf algebra structure on the vector space with
basis all heap-ordered trees. We give a new bialgebra structure on the space
with basis all permutations and show that there is a direct bialgebra
isomorphism between the Hopf algebra of heap-ordered trees and the bialgebra of
permutations.
| math.RA | it is known that there is a hopf algebra structure on the vector space with basis all heapordered trees we give a new bialgebra structure on the space with basis all permutations and show that there is a direct bialgebra isomorphism between the hopf algebra of heapordered trees and the bialgebra of permutations | [['it', 'is', 'known', 'that', 'there', 'is', 'a', 'hopf', 'algebra', 'structure', 'on', 'the', 'vector', 'space', 'with', 'basis', 'all', 'heapordered', 'trees', 'we', 'give', 'a', 'new', 'bialgebra', 'structure', 'on', 'the', 'space', 'with', 'basis', 'all', 'permutations', 'and', 'show', 'that', 'there', 'is', 'a', ... | [-0.21727465333873933, 0.10819869711643683, -0.033461224639190816, 0.07544316421482572, -0.23179323157682172, -0.08962482980997213, 0.04103146342314639, 0.40258235259438463, -0.40798192457208093, -0.19601208498736597, 0.11305917412007474, -0.19785708775919564, -0.22798823229617105, 0.16712687146972935, -0.0678049002088... |
706.1328 | N = 4 Superfiel Phase Space Coordinates and Hamiltonian Quantization | The N = 4 superfield phase space coordinates are given in the harmonic
superspace. The expressions of the N = 4 classical equations of motion are
determined in terms of the spinorial and harmonic supercharges. Furthermore,
the N = 4 supersymmetric actions are obtained by means of the fermionic and
harmonic functional... | hep-th | the n 4 superfield phase space coordinates are given in the harmonic superspace the expressions of the n 4 classical equations of motion are determined in terms of the spinorial and harmonic supercharges furthermore the n 4 supersymmetric actions are obtained by means of the fermionic and harmonic functionals on the ot... | [['the', 'n', '4', 'superfield', 'phase', 'space', 'coordinates', 'are', 'given', 'in', 'the', 'harmonic', 'superspace', 'the', 'expressions', 'of', 'the', 'n', '4', 'classical', 'equations', 'of', 'motion', 'are', 'determined', 'in', 'terms', 'of', 'the', 'spinorial', 'and', 'harmonic', 'supercharges', 'furthermore', ... | [-0.1793224040216629, 0.20936720741864961, 0.015640338369382497, 0.031773631169926375, -0.008985390337422872, -0.13258725380859313, -0.04986743694648911, 0.3198673195945911, -0.16189518141058776, -0.27947986328329605, 0.0789417341688815, -0.3112306218737593, -0.1731306163695617, 0.13429359060365897, -0.0230408858937712... |
706.1329 | Solidity of viscous liquids. V. Long-wavelength dominance of the
dynamics | This paper is the fifth in a series exploring the physical consequences of
the solidity of glass-forming liquids. Paper IV proposed a model where the
density field is described by a time-dependent Ginzburg-Landau equation of the
nonconserved type with rates in $k$ space of the form $\Gamma_0+Dk^2$. The
model assumes ... | cond-mat.soft | this paper is the fifth in a series exploring the physical consequences of the solidity of glassforming liquids paper iv proposed a model where the density field is described by a timedependent ginzburglandau equation of the nonconserved type with rates in k space of the form gamma_0dk2 the model assumes that dgggamma_... | [['this', 'paper', 'is', 'the', 'fifth', 'in', 'a', 'series', 'exploring', 'the', 'physical', 'consequences', 'of', 'the', 'solidity', 'of', 'glassforming', 'liquids', 'paper', 'iv', 'proposed', 'a', 'model', 'where', 'the', 'density', 'field', 'is', 'described', 'by', 'a', 'timedependent', 'ginzburglandau', 'equation'... | [-0.1345716065649564, 0.17132691676314507, -0.10738606119735374, 0.06106803818164634, -0.03789241892389125, -0.12946363258330773, -0.0021938381289752823, 0.31487934589385985, -0.26315567036055854, -0.2714638164473904, 0.08063841604097333, -0.25919214196813606, -0.15050041171101233, 0.15653391143261816, -7.8240593170954... |
706.133 | Note on: Considering the Case for Biodiversity Cycles: Reexamining the
Evidence for Periodicity in the Fossil Record, by Lieberman and Melott, arXiv
preprint 0704.2896 | Lieberman and Melott built their recent arXiv preprint 0704.2896 on my
published paper and (a preprint of) a subsequent comment by Liebermans
associate Cornette. But had this group waited for the Cornette comment to
actually appear in print together with the expected Reply, they would have
learned that his comment ex... | q-bio.PE astro-ph physics.geo-ph | lieberman and melott built their recent arxiv preprint 07042896 on my published paper and a preprint of a subsequent comment by liebermans associate cornette but had this group waited for the cornette comment to actually appear in print together with the expected reply they would have learned that his comment exposes c... | [['lieberman', 'and', 'melott', 'built', 'their', 'recent', 'arxiv', 'preprint', '07042896', 'on', 'my', 'published', 'paper', 'and', 'a', 'preprint', 'of', 'a', 'subsequent', 'comment', 'by', 'liebermans', 'associate', 'cornette', 'but', 'had', 'this', 'group', 'waited', 'for', 'the', 'cornette', 'comment', 'to', 'act... | [-0.07137909645680338, 0.0794217818444142, -0.14235368127313752, 0.04225600755695875, -0.17598997404954086, -0.1737996596429083, 0.10315505196987133, 0.3393224287136238, -0.1527879953177439, -0.3241734496382479, 0.11178065091242186, -0.29535673084772296, -0.1853214229715781, 0.14966296276284588, -0.23884296437932384, -... |
706.1331 | On a Smale Theorem and Nonhomogeneous Equilibria in Cooperative Systems | A standard result by Smale states that n dimensional strongly cooperative
dynamical systems can have arbitrary dynamics when restricted to unordered
invariant hyperspaces. In this paper this result is extended to the case when
all solutions of the strongly cooperative system are bounded and converge
towards one of on... | math.DS math.AP | a standard result by smale states that n dimensional strongly cooperative dynamical systems can have arbitrary dynamics when restricted to unordered invariant hyperspaces in this paper this result is extended to the case when all solutions of the strongly cooperative system are bounded and converge towards one of only ... | [['a', 'standard', 'result', 'by', 'smale', 'states', 'that', 'n', 'dimensional', 'strongly', 'cooperative', 'dynamical', 'systems', 'can', 'have', 'arbitrary', 'dynamics', 'when', 'restricted', 'to', 'unordered', 'invariant', 'hyperspaces', 'in', 'this', 'paper', 'this', 'result', 'is', 'extended', 'to', 'the', 'case'... | [-0.1785697404274662, 0.14511716188352175, -0.06273266784995155, 0.02130790981212996, 0.00961955831221798, -0.17665685174699106, -0.0067331921936962386, 0.3105460522221584, -0.3010268427395061, -0.22481300983139696, 0.11755756421389021, -0.27097605101252886, -0.1628208717938476, 0.14857005075935056, -0.043761144597007,... |
706.1332 | Constraints on Galaxy Structure and Evolution from the Light of Nearby
Systems | We review knowledge of galaxy structures obtained by their emitted light and
in the local universe where they can be studied in great detail. We discuss the
shapes of, and stellar motions within, galaxies, compositional clues derived
from their spectra, and what luminous matter implies about their dark matter
content... | astro-ph | we review knowledge of galaxy structures obtained by their emitted light and in the local universe where they can be studied in great detail we discuss the shapes of and stellar motions within galaxies compositional clues derived from their spectra and what luminous matter implies about their dark matter content implic... | [['we', 'review', 'knowledge', 'of', 'galaxy', 'structures', 'obtained', 'by', 'their', 'emitted', 'light', 'and', 'in', 'the', 'local', 'universe', 'where', 'they', 'can', 'be', 'studied', 'in', 'great', 'detail', 'we', 'discuss', 'the', 'shapes', 'of', 'and', 'stellar', 'motions', 'within', 'galaxies', 'compositional... | [-0.055494239614879495, 0.11380625561215595, -0.11587849529612748, 0.1747417034267364, -0.11719301412431676, 0.006562210634717199, -0.01886830531007259, 0.4409941788762808, -0.20513297434224456, -0.38387184681706743, 0.03904487339390411, -0.23541599812871608, -0.0918121989205724, 0.1634875420441247, -0.0207089289725132... |
706.1333 | An explicit construction of the Quillen homotopical category of dg Lie
algebras | Let $\g_1$ and $\g_2$ be two dg Lie algebras, then it is well-known that the
$L_\infty$ morphisms from $\g_1$ to $\g_2$ are in 1-1 correspondence to the
solutions of the Maurer-Cartan equation in some dg Lie algebra
$\Bbbk(\g_1,\g_2)$. Then the gauge action by exponents of the zero degree
component $\Bbbk(\g_1,\g_2)^... | math.KT math.QA | let g_1 and g_2 be two dg lie algebras then it is wellknown that the l_infty morphisms from g_1 to g_2 are in 11 correspondence to the solutions of the maurercartan equation in some dg lie algebra bbbkg_1g_2 then the gauge action by exponents of the zero degree component bbbkg_1g_20 on mcsubsetbbbkg_1g_21 gives an expl... | [['let', 'g_1', 'and', 'g_2', 'be', 'two', 'dg', 'lie', 'algebras', 'then', 'it', 'is', 'wellknown', 'that', 'the', 'l_infty', 'morphisms', 'from', 'g_1', 'to', 'g_2', 'are', 'in', '11', 'correspondence', 'to', 'the', 'solutions', 'of', 'the', 'maurercartan', 'equation', 'in', 'some', 'dg', 'lie', 'algebra', 'bbbkg_1g_... | [-0.18093719683459092, 0.053791216651884965, -0.09120618157602589, 0.0965457110384736, -0.14289140736619974, -0.1539045396806865, -0.07469510102949652, 0.413689871142811, -0.42287654759811943, -0.20028365361343684, 0.08910194297345227, -0.23062402203614857, -0.12800432803141404, 0.1409419885804427, -0.2033752826203046,... |
706.1334 | Transients from initial conditions based on Lagrangian perturbation
theory in N-body simulations | We explore the initial conditions for cosmological N-body simulations
suitable for calculating the skewness and kurtosis of the density field. In
general, the initial conditions based on the perturbation theory (PT) provide
incorrect second-order and higher-order growth. These errors implied by the use
of the perturb... | astro-ph | we explore the initial conditions for cosmological nbody simulations suitable for calculating the skewness and kurtosis of the density field in general the initial conditions based on the perturbation theory pt provide incorrect secondorder and higherorder growth these errors implied by the use of the perturbation theo... | [['we', 'explore', 'the', 'initial', 'conditions', 'for', 'cosmological', 'nbody', 'simulations', 'suitable', 'for', 'calculating', 'the', 'skewness', 'and', 'kurtosis', 'of', 'the', 'density', 'field', 'in', 'general', 'the', 'initial', 'conditions', 'based', 'on', 'the', 'perturbation', 'theory', 'pt', 'provide', 'in... | [-0.10705759212995351, 0.11966542834206746, -0.12443817829912047, 0.12088684921330783, -0.01806463900524495, -0.07035613787789526, -0.012885532332741227, 0.3542448149801407, -0.19660968351795266, -0.2942563130342391, 0.14733993700114237, -0.2620667586144939, -0.10219661858354812, 0.21636383336304238, 0.0230088281707466... |
706.1335 | Geometric mesoscopic correlations in quasi-one dimension | We study analytically and numerically field/intensity correlations in wave
transport through volume-disordered waveguide. The obtained channel and spacial
correlations deviate from those found in framework of
Dorokhov-Mello-Pereyra-Kumar (DMPK) formalism, that we relate to
inapplicability of equivalent channel approx... | cond-mat.mes-hall cond-mat.dis-nn | we study analytically and numerically fieldintensity correlations in wave transport through volumedisordered waveguide the obtained channel and spacial correlations deviate from those found in framework of dorokhovmellopereyrakumar dmpk formalism that we relate to inapplicability of equivalent channel approximation in ... | [['we', 'study', 'analytically', 'and', 'numerically', 'fieldintensity', 'correlations', 'in', 'wave', 'transport', 'through', 'volumedisordered', 'waveguide', 'the', 'obtained', 'channel', 'and', 'spacial', 'correlations', 'deviate', 'from', 'those', 'found', 'in', 'framework', 'of', 'dorokhovmellopereyrakumar', 'dmpk... | [-0.1226732041731122, 0.10673076143346927, -0.10654981408179516, 0.0827337926996517, -0.019109881372146663, -0.152852341404096, 0.0008101875716376872, 0.406844744920021, -0.23984982731441656, -0.259442780960706, 0.050483144215485526, -0.284190659946762, -0.17522180344732036, 0.18803790321662311, 0.016978957282290572, 0... |
706.1336 | Can aerosols be trapped in open flows? | The fate of aerosols in open flows is relevant in a variety of physical
contexts. Previous results are consistent with the assumption that such
finite-size particles always escape in open chaotic advection. Here we show
that a different behavior is possible. We analyze the dynamics of aerosols both
in the absence and... | nlin.CD astro-ph physics.flu-dyn | the fate of aerosols in open flows is relevant in a variety of physical contexts previous results are consistent with the assumption that such finitesize particles always escape in open chaotic advection here we show that a different behavior is possible we analyze the dynamics of aerosols both in the absence and prese... | [['the', 'fate', 'of', 'aerosols', 'in', 'open', 'flows', 'is', 'relevant', 'in', 'a', 'variety', 'of', 'physical', 'contexts', 'previous', 'results', 'are', 'consistent', 'with', 'the', 'assumption', 'that', 'such', 'finitesize', 'particles', 'always', 'escape', 'in', 'open', 'chaotic', 'advection', 'here', 'we', 'sho... | [-0.1666411429294385, 0.22847797764380548, -0.06313183638690548, 0.0979134601720778, 0.008482816836542704, -0.09658032336949625, -0.026979464309459383, 0.3218611769378185, -0.24599974029697477, -0.27665317133915696, 0.09429212247487158, -0.2794574227438054, -0.14958635627673092, 0.20218666868115012, -0.0397462772036140... |
706.1337 | A note on Poisson homogeneous spaces | We identify the cotangent bundle Lie algebroid of a Poisson homogeneous space
G/H of a Poisson Lie group G as a quotient of a transformation Lie algebroid
over G. As applications, we describe the modular vector fields of G/H, and we
identify the Poisson cohomology of G/H with coefficients in powers of its
canonical l... | math.DG math.SG | we identify the cotangent bundle lie algebroid of a poisson homogeneous space gh of a poisson lie group g as a quotient of a transformation lie algebroid over g as applications we describe the modular vector fields of gh and we identify the poisson cohomology of gh with coefficients in powers of its canonical line bund... | [['we', 'identify', 'the', 'cotangent', 'bundle', 'lie', 'algebroid', 'of', 'a', 'poisson', 'homogeneous', 'space', 'gh', 'of', 'a', 'poisson', 'lie', 'group', 'g', 'as', 'a', 'quotient', 'of', 'a', 'transformation', 'lie', 'algebroid', 'over', 'g', 'as', 'applications', 'we', 'describe', 'the', 'modular', 'vector', 'f... | [-0.23392459465056595, 0.01648093922995031, -0.07489591158168801, 0.06332379530610169, -0.22600956126984398, -0.08820246804852859, -0.02215964876715157, 0.427553831015603, -0.37783963476323473, -0.18775090262672658, 0.07207034170524991, -0.17205814104842937, -0.19543570770203308, 0.18282555064218023, -0.166615447558273... |
706.1338 | Supersymmetric Hamiltonian Approach to Edge Excitations in $\nu = 5/2$
Fractional Quantum Hall Effect | A supersymmetric Hamiltonian is constructed for the edge excitations of the
Moore-Read (Pfaffian) like state, which is a realization of the N=2
supersymmetric CS model. Fermionic generators and their conjugates are
introduced to deal with the fermion pairing, whose condensation form a BCS like
state. After Bogoliubov... | hep-th cond-mat.mes-hall | a supersymmetric hamiltonian is constructed for the edge excitations of the mooreread pfaffian like state which is a realization of the n2 supersymmetric cs model fermionic generators and their conjugates are introduced to deal with the fermion pairing whose condensation form a bcs like state after bogoliubov transform... | [['a', 'supersymmetric', 'hamiltonian', 'is', 'constructed', 'for', 'the', 'edge', 'excitations', 'of', 'the', 'mooreread', 'pfaffian', 'like', 'state', 'which', 'is', 'a', 'realization', 'of', 'the', 'n2', 'supersymmetric', 'cs', 'model', 'fermionic', 'generators', 'and', 'their', 'conjugates', 'are', 'introduced', 't... | [-0.11344086237243443, 0.22675093465451418, -0.09428649430628866, 0.10812781666131091, -0.04461829559087554, -0.19376335663504765, 0.014021451922807111, 0.28818915606409845, -0.18379797089645372, -0.2726804301367208, 0.03264120626928551, -0.30920809070604655, -0.12811596305774792, 0.09790107604931109, 0.006740605177973... |
706.1339 | Verification theorem and construction of $\epsilon$-optimal controls for
control of abstract evolution equations | We study several aspects of the dynamic programming approach to optimal
control of abstract evolution equations, including a class of semilinear
partial differential equations. We introduce and prove a verification theorem
which provides a sufficient condition for optimality. Moreover we prove sub-
and superoptimalit... | math.OC | we study several aspects of the dynamic programming approach to optimal control of abstract evolution equations including a class of semilinear partial differential equations we introduce and prove a verification theorem which provides a sufficient condition for optimality moreover we prove sub and superoptimality prin... | [['we', 'study', 'several', 'aspects', 'of', 'the', 'dynamic', 'programming', 'approach', 'to', 'optimal', 'control', 'of', 'abstract', 'evolution', 'equations', 'including', 'a', 'class', 'of', 'semilinear', 'partial', 'differential', 'equations', 'we', 'introduce', 'and', 'prove', 'a', 'verification', 'theorem', 'whi... | [-0.18117319546373828, -0.030450427095794503, -0.11924368365933853, 0.10638873082020187, -0.15467495281648422, -0.15740113842600426, 0.04558365249041734, 0.27179811063355636, -0.3300024586330567, -0.3020516783331654, 0.1769196612835263, -0.17548728007490613, -0.19676508238938237, 0.20393062733845518, -0.087825521876636... |
706.134 | Cluster abundances and S-Z power spectra: effects of non-Gaussianity and
early dark energy | In the standard Lambda CDM cosmological model with a Gaussian primordial
density fluctuation field, the relatively low value of the mass variance
parameter (sigma_8=0.74{+0.05}{-0.06}, obtained from the WMAP 3-year data)
results in a reduced likelihood that the measured level of CMB anisotropy on
the scales of cluste... | astro-ph | in the standard lambda cdm cosmological model with a gaussian primordial density fluctuation field the relatively low value of the mass variance parameter sigma_8074005006 obtained from the wmap 3year data results in a reduced likelihood that the measured level of cmb anisotropy on the scales of clusters is due to the ... | [['in', 'the', 'standard', 'lambda', 'cdm', 'cosmological', 'model', 'with', 'a', 'gaussian', 'primordial', 'density', 'fluctuation', 'field', 'the', 'relatively', 'low', 'value', 'of', 'the', 'mass', 'variance', 'parameter', 'sigma_8074005006', 'obtained', 'from', 'the', 'wmap', '3year', 'data', 'results', 'in', 'a', ... | [-0.09604855603977756, 0.09971456913178298, -0.1235026642973037, 0.11739451396967278, -0.05680548469389572, -0.04083587205822363, 0.026938473141705326, 0.31823936940621844, -0.19904658583771884, -0.3573990672059451, 0.029099225707252586, -0.2768045060172583, -0.02527164461958052, 0.1817842873601161, 0.04275063100218210... |
706.1341 | A Study in Depth of f0(1370) | Claims have been made that f0(1370) does not exist. The five primary sets of
data requiring its existence are refitted. Major dispersive effects due to the
opening of the 4pi threshold are included for the first time; the sigma -> 4pi
amplitude plays a strong role. Crystal Barrel data on pbar-p -> 3pizero at rest
req... | hep-ex | claims have been made that f01370 does not exist the five primary sets of data requiring its existence are refitted major dispersive effects due to the opening of the 4pi threshold are included for the first time the sigma 4pi amplitude plays a strong role crystal barrel data on pbarp 3pizero at rest require f01370 sig... | [['claims', 'have', 'been', 'made', 'that', 'f01370', 'does', 'not', 'exist', 'the', 'five', 'primary', 'sets', 'of', 'data', 'requiring', 'its', 'existence', 'are', 'refitted', 'major', 'dispersive', 'effects', 'due', 'to', 'the', 'opening', 'of', 'the', '4pi', 'threshold', 'are', 'included', 'for', 'the', 'first', 't... | [-0.12891002837969953, 0.16542420324055884, -0.041910015972566675, 0.10804336805608467, -0.05774351139502712, -0.12586774827709057, 0.05171635142399062, 0.33970050489658427, -0.1739323998710419, -0.295365835944105, 0.06125576023933017, -0.35936316919523753, 0.004582241811821687, 0.17392803107163515, 0.05871624586937799... |
706.1342 | Low-temperature electron dephasing time in AuPd revisited | Ever since the first discoveries of the quantum-interference transport in
mesoscopic systems, the electron dephasing times, $\tau_\phi$, in the
concentrated AuPd alloys have been extensively measured. The samples were made
from different sources with different compositions, prepared by different
deposition methods, a... | cond-mat.mes-hall cond-mat.dis-nn | ever since the first discoveries of the quantuminterference transport in mesoscopic systems the electron dephasing times tau_phi in the concentrated aupd alloys have been extensively measured the samples were made from different sources with different compositions prepared by different deposition methods and various ge... | [['ever', 'since', 'the', 'first', 'discoveries', 'of', 'the', 'quantuminterference', 'transport', 'in', 'mesoscopic', 'systems', 'the', 'electron', 'dephasing', 'times', 'tau_phi', 'in', 'the', 'concentrated', 'aupd', 'alloys', 'have', 'been', 'extensively', 'measured', 'the', 'samples', 'were', 'made', 'from', 'diffe... | [-0.11221767778915819, 0.21949388787616045, -0.06095125029969495, 0.0376623510645004, 0.01302882738491462, -0.18675636455081984, 0.02245876572560519, 0.38144483740907165, -0.24000444435878307, -0.310036566411145, 0.0540897875551309, -0.334632760938257, -0.07056904862329247, 0.21402402693493058, 0.016634543662075885, 0.... |
706.1343 | Interacting like charges in Landau levels: Planar geometry, symmetries,
and effective quasiparticles | We consider a system of two interacting particles with like but unequal
charges in a magnetic field in the planar geometry. We construct a complete
basis of states compatible with both the axial symmetry and magnetic
translations. The basis is obtained using a canonical transformation that
generates effective quasipa... | cond-mat.mes-hall | we consider a system of two interacting particles with like but unequal charges in a magnetic field in the planar geometry we construct a complete basis of states compatible with both the axial symmetry and magnetic translations the basis is obtained using a canonical transformation that generates effective quasipartic... | [['we', 'consider', 'a', 'system', 'of', 'two', 'interacting', 'particles', 'with', 'like', 'but', 'unequal', 'charges', 'in', 'a', 'magnetic', 'field', 'in', 'the', 'planar', 'geometry', 'we', 'construct', 'a', 'complete', 'basis', 'of', 'states', 'compatible', 'with', 'both', 'the', 'axial', 'symmetry', 'and', 'magne... | [-0.17599427152083874, 0.1699019609443327, -0.05568979789634318, 0.07840520132443693, -0.05010225824403143, -0.12304293726672336, 0.02335427279150722, 0.36969374138677474, -0.21852347969381822, -0.27475785434541133, 0.028244530748677357, -0.2587512659478361, -0.1511794573461434, 0.12249342760642862, 0.0369962978778732,... |
706.1344 | A Class of Partially Solvable Two-Dimensional Quantum Models with
Periodic Potentials | The supersymmetrical approach is used to analyse a class of two-dimensional
quantum systems with periodic potentials. In particular, the method of
SUSY-separation of variables allowed us to find a part of the energy spectra
and the corresponding wave functions (partial solvability) for several models.
These models ar... | hep-th cond-mat.mes-hall math-ph math.MP quant-ph | the supersymmetrical approach is used to analyse a class of twodimensional quantum systems with periodic potentials in particular the method of susyseparation of variables allowed us to find a part of the energy spectra and the corresponding wave functions partial solvability for several models these models are not ame... | [['the', 'supersymmetrical', 'approach', 'is', 'used', 'to', 'analyse', 'a', 'class', 'of', 'twodimensional', 'quantum', 'systems', 'with', 'periodic', 'potentials', 'in', 'particular', 'the', 'method', 'of', 'susyseparation', 'of', 'variables', 'allowed', 'us', 'to', 'find', 'a', 'part', 'of', 'the', 'energy', 'spectr... | [-0.13488255563677978, 0.08472458893590121, -0.06882719471974744, 0.0591988708816327, -0.06801425958426831, -0.14356339301752008, -0.028183607414931706, 0.3349216586262312, -0.2915219978996269, -0.25972513080594817, 0.10808600482794092, -0.28738071163103956, -0.1373996635210579, 0.2111104403966633, 0.000485032202129292... |
706.1345 | Spectroscopy and multiband photometry of the afterglow of intermediate
duration gamma-ray burst 040924 and its host galaxy | We present optical photometry and spectroscopy of the afterglow and host
galaxy of gamma-ray burst 040924. This GRB had a rather short duration of T90
~2.4s, and a well sampled optical afterglow light curve. We aim to use this
dataset to find further evidence that this burst is consistent with a massive
star core-col... | astro-ph | we present optical photometry and spectroscopy of the afterglow and host galaxy of gammaray burst 040924 this grb had a rather short duration of t90 24s and a well sampled optical afterglow light curve we aim to use this dataset to find further evidence that this burst is consistent with a massive star corecollapse pro... | [['we', 'present', 'optical', 'photometry', 'and', 'spectroscopy', 'of', 'the', 'afterglow', 'and', 'host', 'galaxy', 'of', 'gammaray', 'burst', '040924', 'this', 'grb', 'had', 'a', 'rather', 'short', 'duration', 'of', 't90', '24s', 'and', 'a', 'well', 'sampled', 'optical', 'afterglow', 'light', 'curve', 'we', 'aim', '... | [-0.029039196902019112, 0.05156798877987386, -0.08761417178952313, 0.1373893323166177, -0.13234857466329444, -0.10732437748699747, 0.06638570524098232, 0.510448341356947, -0.1624191192919983, -0.3141093985038869, 0.0484563824522527, -0.33568488629336685, -0.007759797827717155, 0.19141718777035305, -0.007583711773870473... |
706.1346 | Southern wide very low-mass stars and brown dwarfs in resolved binary
and multiple systems | The results of the Koenigstuhl survey in the Southern Hemisphere are
presented. I have searched for common-proper motion companions to 173 field
very low-mass stars and brown dwarfs with spectral types > M5.0V and magnitudes
J <= 14.5 mag. I have measured for the first time the common-proper motion of
two new wide sy... | astro-ph | the results of the koenigstuhl survey in the southern hemisphere are presented i have searched for commonproper motion companions to 173 field very lowmass stars and brown dwarfs with spectral types m50v and magnitudes j 145 mag i have measured for the first time the commonproper motion of two new wide systems containi... | [['the', 'results', 'of', 'the', 'koenigstuhl', 'survey', 'in', 'the', 'southern', 'hemisphere', 'are', 'presented', 'i', 'have', 'searched', 'for', 'commonproper', 'motion', 'companions', 'to', '173', 'field', 'very', 'lowmass', 'stars', 'and', 'brown', 'dwarfs', 'with', 'spectral', 'types', 'm50v', 'and', 'magnitudes... | [-0.12493654417722852, 0.13624166350780775, -0.026538359673245797, 0.04949777038426056, -0.07533165850069468, -0.11389631870249876, 0.042324907267230406, 0.40066495469824376, -0.15099105896734738, -0.3907804889250783, 0.05626383624879549, -0.28149743921630366, -0.019395476230714893, 0.19923941607740295, -0.026466082006... |
706.1347 | The Two-State Vector Formalism | The two-state vector formalism (TSVF), the time-symmetric description of the
standard quantum mechanics originated by Aharonov, Bergmann and Lebowitz is
reviewed. The TSVF describes a quantum system at a particular time by two
quantum states: the usual one, evolving forward in time, defined by the results
of a comple... | quant-ph | the twostate vector formalism tsvf the timesymmetric description of the standard quantum mechanics originated by aharonov bergmann and lebowitz is reviewed the tsvf describes a quantum system at a particular time by two quantum states the usual one evolving forward in time defined by the results of a complete measureme... | [['the', 'twostate', 'vector', 'formalism', 'tsvf', 'the', 'timesymmetric', 'description', 'of', 'the', 'standard', 'quantum', 'mechanics', 'originated', 'by', 'aharonov', 'bergmann', 'and', 'lebowitz', 'is', 'reviewed', 'the', 'tsvf', 'describes', 'a', 'quantum', 'system', 'at', 'a', 'particular', 'time', 'by', 'two',... | [-0.13012417171150445, 0.21603723692397275, -0.12738236819083493, 0.045905707511119546, 0.02580189565817515, -0.1503308530834814, 0.04306890801837047, 0.2521462833881378, -0.23131328789517283, -0.26383082032824556, 0.042486306463057795, -0.2405848994354407, -0.08598034419119358, 0.18209326927860578, -0.0176310753573973... |
706.1348 | Weak Value and Weak Measurements | The weak value of a variable O is a description of an effective interaction
with that variable in the limit of weak coupling. It is particularly important
for a pre- and post-selected quantum system.
| quant-ph | the weak value of a variable o is a description of an effective interaction with that variable in the limit of weak coupling it is particularly important for a pre and postselected quantum system | [['the', 'weak', 'value', 'of', 'a', 'variable', 'o', 'is', 'a', 'description', 'of', 'an', 'effective', 'interaction', 'with', 'that', 'variable', 'in', 'the', 'limit', 'of', 'weak', 'coupling', 'it', 'is', 'particularly', 'important', 'for', 'a', 'pre', 'and', 'postselected', 'quantum', 'system']] | [-0.17351990417741678, 0.1489316644596436, -0.08739263446563307, 0.06356728885678903, -0.007899383466471644, -0.18094543341602035, 0.07427323414423667, 0.3308717522989301, -0.22518576031057713, -0.2754276844618075, 0.07710766813868437, -0.2206464069758487, -0.09175409672453123, 0.20045206871102839, 0.002119112444822402... |
706.1349 | Improved quark mass density- dependent model with quark-sigma meson and
quark-omega meson couplings | An improved quark mass density- dependent model with the non-linear scalar
sigma field and the $\omega$-meson field is presented. We show that the present
model can describe saturation properties, the equation of state, the
compressibility and the effective nuclear mass of nuclear matter under mean
field approximatio... | nucl-th | an improved quark mass density dependent model with the nonlinear scalar sigma field and the omegameson field is presented we show that the present model can describe saturation properties the equation of state the compressibility and the effective nuclear mass of nuclear matter under mean field approximation successfu... | [['an', 'improved', 'quark', 'mass', 'density', 'dependent', 'model', 'with', 'the', 'nonlinear', 'scalar', 'sigma', 'field', 'and', 'the', 'omegameson', 'field', 'is', 'presented', 'we', 'show', 'that', 'the', 'present', 'model', 'can', 'describe', 'saturation', 'properties', 'the', 'equation', 'of', 'state', 'the', '... | [-0.08949738389766607, 0.1722926608018184, -0.1216065138502077, 0.09349240882505404, -0.021291071182635964, -0.09149740813452689, -0.024347918726442777, 0.3324669703047295, -0.21661528228919524, -0.319574434157522, 0.026962283548334093, -0.22415815678532006, -0.09025954633767976, 0.09438129421323538, 0.0663173584282764... |
706.135 | The Anisotropic Distribution of Satellite Galaxies | We identify satellites of isolated galaxies in SDSS and examine their angular
distribution. Using mock catalogues generated from cosmological N-body
simulations, we demonstrate that the selection criteria used to select isolated
galaxies and their satellites must be very strict in order to correctly
identify systems ... | astro-ph | we identify satellites of isolated galaxies in sdss and examine their angular distribution using mock catalogues generated from cosmological nbody simulations we demonstrate that the selection criteria used to select isolated galaxies and their satellites must be very strict in order to correctly identify systems in wh... | [['we', 'identify', 'satellites', 'of', 'isolated', 'galaxies', 'in', 'sdss', 'and', 'examine', 'their', 'angular', 'distribution', 'using', 'mock', 'catalogues', 'generated', 'from', 'cosmological', 'nbody', 'simulations', 'we', 'demonstrate', 'that', 'the', 'selection', 'criteria', 'used', 'to', 'select', 'isolated',... | [-0.0940727335671207, 0.08780358080344086, -0.1190742028664365, 0.12774875324981616, -0.10951250900683597, -0.012380935820273022, -0.004343118815951412, 0.4283469962339834, -0.17625449741414437, -0.3654684985182091, 0.06214363870476041, -0.2750485715759772, -0.051810841553945663, 0.18338115069464073, -0.016460350707845... |
706.1351 | Scattering of charge carriers by point defects in bilayer graphene | Theory of scattering of massive chiral fermions in bilayer graphene by radial
symmetric potential is developed. It is shown that in the case when the
electron wavelength is much larger than the radius of the potential the
scattering cross-section is proportional to the electron wavelength. This leads
to the mobility ... | cond-mat.mes-hall cond-mat.mtrl-sci | theory of scattering of massive chiral fermions in bilayer graphene by radial symmetric potential is developed it is shown that in the case when the electron wavelength is much larger than the radius of the potential the scattering crosssection is proportional to the electron wavelength this leads to the mobility indep... | [['theory', 'of', 'scattering', 'of', 'massive', 'chiral', 'fermions', 'in', 'bilayer', 'graphene', 'by', 'radial', 'symmetric', 'potential', 'is', 'developed', 'it', 'is', 'shown', 'that', 'in', 'the', 'case', 'when', 'the', 'electron', 'wavelength', 'is', 'much', 'larger', 'than', 'the', 'radius', 'of', 'the', 'poten... | [-0.11189681316206518, 0.20766412906157664, 0.004060372614707702, 0.01763231722632041, 0.028880215384281024, -0.148716765957383, -0.020618725842676867, 0.358816639185907, -0.1867433495533008, -0.24586163844483402, -0.010266160861087533, -0.33874487640479434, -0.119865174305279, 0.18083889037370682, 0.005714095167767925... |
End of preview. Expand in Data Studio
README.md exists but content is empty.
- Downloads last month
- 37