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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708.0749 | Nodal free geometric phases: Concept and application to geometric
quantum computation | Nodal free geometric phases are the eigenvalues of the final member of a
parallel transporting family of unitary operators. These phases are gauge
invariant, always well-defined, and can be measured interferometrically. Nodal
free geometric phases can be used to construct various types of quantum phase
gates.
| quant-ph | nodal free geometric phases are the eigenvalues of the final member of a parallel transporting family of unitary operators these phases are gauge invariant always welldefined and can be measured interferometrically nodal free geometric phases can be used to construct various types of quantum phase gates | [['nodal', 'free', 'geometric', 'phases', 'are', 'the', 'eigenvalues', 'of', 'the', 'final', 'member', 'of', 'a', 'parallel', 'transporting', 'family', 'of', 'unitary', 'operators', 'these', 'phases', 'are', 'gauge', 'invariant', 'always', 'welldefined', 'and', 'can', 'be', 'measured', 'interferometrically', 'nodal', '... | [-0.22442440777693107, 0.32354290086937987, -0.11653995854051216, 0.05196694049822247, -0.042782832893704915, -0.19138982901147203, 0.009543713086041744, 0.37067306133331324, -0.30335552269673866, -0.2946202576200923, 0.06551121248175269, -0.2663688972065954, -0.0932892912229442, 0.16339160585978432, -0.058975359536302... |
708.075 | On the q-quantum gravity loop algebra | A class of deformations of the q-quantum gravity loop algebra is shown to be
incompatible with the combinatorics of Temperley-Lieb recoupling theory with
deformation parameter at a root of unity. This incompatibility appears to
extend to more general deformation parameters.
| gr-qc | a class of deformations of the qquantum gravity loop algebra is shown to be incompatible with the combinatorics of temperleylieb recoupling theory with deformation parameter at a root of unity this incompatibility appears to extend to more general deformation parameters | [['a', 'class', 'of', 'deformations', 'of', 'the', 'qquantum', 'gravity', 'loop', 'algebra', 'is', 'shown', 'to', 'be', 'incompatible', 'with', 'the', 'combinatorics', 'of', 'temperleylieb', 'recoupling', 'theory', 'with', 'deformation', 'parameter', 'at', 'a', 'root', 'of', 'unity', 'this', 'incompatibility', 'appears... | [-0.14420744319213555, 0.17186427842825652, -0.09430219492642208, 0.024046754697337747, -0.1454815963283181, -0.14744465032126755, -0.07700432286655996, 0.24730779794044794, -0.35849581761285665, -0.23714601518586279, 0.08049085942911915, -0.20347421830520035, -0.16230958020314573, 0.15243127006106078, -0.1758174105780... |
708.0751 | On the relativistic iron line and soft excess in the Seyfert 1 galaxy
Markarian 335 | We report on a 133 ks XMM-Newton observation of the Seyfert 1 galaxy
Markarian 335. The 0.4-12 keV spectrum contains an underlying power law
continuum, a soft excess below 2 keV, and a double-peaked iron emission feature
in the 6-7 keV range. We investigate the possibility that the double-peaked
emission might repres... | astro-ph | we report on a 133 ks xmmnewton observation of the seyfert 1 galaxy markarian 335 the 0412 kev spectrum contains an underlying power law continuum a soft excess below 2 kev and a doublepeaked iron emission feature in the 67 kev range we investigate the possibility that the doublepeaked emission might represent the char... | [['we', 'report', 'on', 'a', '133', 'ks', 'xmmnewton', 'observation', 'of', 'the', 'seyfert', '1', 'galaxy', 'markarian', '335', 'the', '0412', 'kev', 'spectrum', 'contains', 'an', 'underlying', 'power', 'law', 'continuum', 'a', 'soft', 'excess', 'below', '2', 'kev', 'and', 'a', 'doublepeaked', 'iron', 'emission', 'fea... | [-0.06504392953757888, 0.10070545691977148, -0.050061644750294856, 0.11219622891528432, -0.08708998168554358, -0.1421999034874544, 0.034540892193232337, 0.4888697128390541, -0.17003419300984918, -0.34538710431976094, 0.06485048169112839, -0.32741760127749797, 0.03650480062021194, 0.17436027571533783, 0.0064044608923329... |
708.0752 | Two-color photoassociation spectroscopy of ytterbium atoms and the
precise determinations of s-wave scattering lengths | By performing high-resolution two-color photoassociation spectroscopy, we
have successfully determined the binding energies of several of the last bound
states of the homonuclear dimers of six different isotopes of ytterbium. These
spectroscopic data are in excellent agreement with theoretical calculations
based on a... | physics.atom-ph | by performing highresolution twocolor photoassociation spectroscopy we have successfully determined the binding energies of several of the last bound states of the homonuclear dimers of six different isotopes of ytterbium these spectroscopic data are in excellent agreement with theoretical calculations based on a simpl... | [['by', 'performing', 'highresolution', 'twocolor', 'photoassociation', 'spectroscopy', 'we', 'have', 'successfully', 'determined', 'the', 'binding', 'energies', 'of', 'several', 'of', 'the', 'last', 'bound', 'states', 'of', 'the', 'homonuclear', 'dimers', 'of', 'six', 'different', 'isotopes', 'of', 'ytterbium', 'these... | [-0.09525871074699338, 0.22438109190838915, 0.0022117776707524343, 0.0007354334201885475, 0.1164459262508899, -0.20499579756638953, 0.055557738756760955, 0.4189935582985599, -0.16600186877795273, -0.2851165292548045, -0.07009579919903199, -0.3639632850914957, 0.01720087718687922, 0.19418571725679887, 0.1204907522935952... |
708.0753 | The Baryonic and Dark Matter Properties of High Redshift Gravitationally
Lensed Disk Galaxies | We present a detailed study of the structural properties of four
gravitationally lensed disk galaxies at z=1. Modelling the rotation curves on
sub-kpc scales we derive the values for the disk mass, the reference dark
matter density and core radius, and the angular momentum per unit mass. The
derived models suggest th... | astro-ph | we present a detailed study of the structural properties of four gravitationally lensed disk galaxies at z1 modelling the rotation curves on subkpc scales we derive the values for the disk mass the reference dark matter density and core radius and the angular momentum per unit mass the derived models suggest that the r... | [['we', 'present', 'a', 'detailed', 'study', 'of', 'the', 'structural', 'properties', 'of', 'four', 'gravitationally', 'lensed', 'disk', 'galaxies', 'at', 'z1', 'modelling', 'the', 'rotation', 'curves', 'on', 'subkpc', 'scales', 'we', 'derive', 'the', 'values', 'for', 'the', 'disk', 'mass', 'the', 'reference', 'dark', ... | [-0.1054162760762362, 0.1212055290598073, -0.09206398014794104, 0.11447133788715291, -0.07506334180167566, -0.03986927057576395, 0.002118571546210054, 0.40643990666527924, -0.16382181664691112, -0.36879398045130074, 0.024593914296929142, -0.26375041894546786, 0.02263920786693537, 0.17866180273796317, 0.0262702634406177... |
708.0754 | Magneto-elastic coupling in hexagonal YMnO_3 | We report an ultrasonic investigation of the elastic moduli on a single
crystal of hexagonal YMnO_3 as a function of temperature. Stiffening anomalies
in the antiferromagnetic N\'eel state below T_N = 72.4 K are observed on all
the four elastic moduli C_{ii}. The anomalies are the most important on C_{11}
and C_{66} ... | cond-mat.str-el | we report an ultrasonic investigation of the elastic moduli on a single crystal of hexagonal ymno_3 as a function of temperature stiffening anomalies in the antiferromagnetic neel state below t_n 724 k are observed on all the four elastic moduli c_ii the anomalies are the most important on c_11 and c_66 for inplane ela... | [['we', 'report', 'an', 'ultrasonic', 'investigation', 'of', 'the', 'elastic', 'moduli', 'on', 'a', 'single', 'crystal', 'of', 'hexagonal', 'ymno_3', 'as', 'a', 'function', 'of', 'temperature', 'stiffening', 'anomalies', 'in', 'the', 'antiferromagnetic', 'neel', 'state', 'below', 't_n', '724', 'k', 'are', 'observed', '... | [-0.2069130656664024, 0.2504736574191229, -0.01807828126749527, 0.02767250317031111, -0.09615910186160666, -0.09247586419658693, 0.04613457407117232, 0.3938452889714604, -0.2602976216183943, -0.2887747261416295, 0.061105023056600545, -0.3403929895614327, -0.12599478546535361, 0.15841007551536948, 0.0719554712300071, 0.... |
708.0755 | Notes on the Self-Reducibility of the Weil Representation and
Higher-Dimensional Quantum Chaos | In these notes we discuss the "self-reducibility property" of the Weil
representation. We explain how to use this property to obtain sharp estimates
of certain higher-dimensional exponential sums which originate from the theory
of quantum chaos. As a result, we obtain the Hecke quantum unique ergodicity
theorem for g... | math-ph math.MP math.RT | in these notes we discuss the selfreducibility property of the weil representation we explain how to use this property to obtain sharp estimates of certain higherdimensional exponential sums which originate from the theory of quantum chaos as a result we obtain the hecke quantum unique ergodicity theorem for generic li... | [['in', 'these', 'notes', 'we', 'discuss', 'the', 'selfreducibility', 'property', 'of', 'the', 'weil', 'representation', 'we', 'explain', 'how', 'to', 'use', 'this', 'property', 'to', 'obtain', 'sharp', 'estimates', 'of', 'certain', 'higherdimensional', 'exponential', 'sums', 'which', 'originate', 'from', 'the', 'theor... | [-0.12309295780194754, 0.09273101574402641, -0.17564629014920105, 0.13651872648730534, -0.0904772528912872, -0.13608413318341428, 0.03892287803094157, 0.2686084742403843, -0.35518951581960373, -0.19831921715628018, 0.10277808467455378, -0.2142838655293665, -0.20994707176631147, 0.20128287835554642, -0.1385631621391936,... |
708.0756 | Singular solutions of some nonlinear parabolic equations with spatially
inhomogeneous absorption | We study the limit behaviour of solutions of a class of solutions of
nonlinear parabolic equations with a degenerate strong absorption. We prove
that two types of phenomena can occur: the pointwise singularity or the
formation of razor blades (or persistent singularities).
| math.AP math.CA | we study the limit behaviour of solutions of a class of solutions of nonlinear parabolic equations with a degenerate strong absorption we prove that two types of phenomena can occur the pointwise singularity or the formation of razor blades or persistent singularities | [['we', 'study', 'the', 'limit', 'behaviour', 'of', 'solutions', 'of', 'a', 'class', 'of', 'solutions', 'of', 'nonlinear', 'parabolic', 'equations', 'with', 'a', 'degenerate', 'strong', 'absorption', 'we', 'prove', 'that', 'two', 'types', 'of', 'phenomena', 'can', 'occur', 'the', 'pointwise', 'singularity', 'or', 'the'... | [-0.2168206849046761, 0.051328567876702265, -0.10058407698358808, 0.09574122359377465, -0.09859465337580159, -0.15116870786905998, -0.009739277105490189, 0.27746879899253446, -0.2976115569472313, -0.20940794090607337, 0.1462276340185088, -0.32271398484174696, -0.15993161629220204, 0.1751210830462653, -0.029237253469459... |
708.0757 | Separable solutions of some quasilinear equations with source reaction | We study the existence of singular separable solutions to a class of
quasilinear equations with reaction term. In the 2-dim case, we use a dynamical
system approach to construct our solutions.
| math.AP math.DS | we study the existence of singular separable solutions to a class of quasilinear equations with reaction term in the 2dim case we use a dynamical system approach to construct our solutions | [['we', 'study', 'the', 'existence', 'of', 'singular', 'separable', 'solutions', 'to', 'a', 'class', 'of', 'quasilinear', 'equations', 'with', 'reaction', 'term', 'in', 'the', '2dim', 'case', 'we', 'use', 'a', 'dynamical', 'system', 'approach', 'to', 'construct', 'our', 'solutions']] | [-0.18012310197997478, -0.017432698994995124, -0.09799480514184031, 0.04124607652005169, -0.07469557466045502, -0.1164160669638565, -0.030130985222997203, 0.24058152488883464, -0.28746170178055763, -0.20058144014746498, 0.10056646799503435, -0.3201899320007332, -0.20556535199284554, 0.15279379258713416, -0.008545918142... |
708.0758 | A Subgroup of a Direct Product of Free Groups whose Dehn Function has a
Cubic Lower Bound | We establish a cubic lower bound on the Dehn function of a certain finitely
presented subgroup of a direct product of 3 free groups.
| math.GR math.GT | we establish a cubic lower bound on the dehn function of a certain finitely presented subgroup of a direct product of 3 free groups | [['we', 'establish', 'a', 'cubic', 'lower', 'bound', 'on', 'the', 'dehn', 'function', 'of', 'a', 'certain', 'finitely', 'presented', 'subgroup', 'of', 'a', 'direct', 'product', 'of', '3', 'free', 'groups']] | [-0.2527009256494542, 0.1333211585491275, -0.10231666742280747, 0.07483462725455563, -0.08255847861679892, -0.09765396835670496, 0.09748316432038943, 0.3296755589544773, -0.29935874153549474, -0.29503493026519817, 0.1346429191956607, -0.22643125181396803, -0.10264468883785109, 0.2889340332476422, -0.05205811921041459, ... |
708.0759 | Effective Action in a General Chiral Model: Next to Leading Order
Derivative Expansion in the Worldline Method | We present a formalism to determine the imaginary part of a general chiral
model in the derivative expansion. Our formalism is based on the worldline path
integral for the covariant current that can be given in an explicit chiral and
gauge covariant form. The effective action is then obtained by integrating the
covar... | hep-th hep-ph | we present a formalism to determine the imaginary part of a general chiral model in the derivative expansion our formalism is based on the worldline path integral for the covariant current that can be given in an explicit chiral and gauge covariant form the effective action is then obtained by integrating the covariant... | [['we', 'present', 'a', 'formalism', 'to', 'determine', 'the', 'imaginary', 'part', 'of', 'a', 'general', 'chiral', 'model', 'in', 'the', 'derivative', 'expansion', 'our', 'formalism', 'is', 'based', 'on', 'the', 'worldline', 'path', 'integral', 'for', 'the', 'covariant', 'current', 'that', 'can', 'be', 'given', 'in', ... | [-0.15123723201074843, 0.12213959850561291, -0.1468557428333798, 0.04055589144275981, -0.15943699885727997, -0.029146618999035683, -0.029237261882556948, 0.3397903900782941, -0.19562329231935033, -0.2214846659798996, 0.05508063846836025, -0.22375653328184605, -0.19035418963028214, 0.11287524744915634, 0.003817188253594... |
708.076 | De-coupling of Exchange and Persistence Times in Atomistic Models of
Glass Formers | With molecular dynamics simulations of a fluid mixture of classical particles
interacting with pair-wise additive Weeks-Chandler-Andersen potentials, we
consider the time series of particle displacements and thereby determine
distributions for local persistence times and local exchange times. These basic
characteriza... | cond-mat.stat-mech cond-mat.soft | with molecular dynamics simulations of a fluid mixture of classical particles interacting with pairwise additive weekschandlerandersen potentials we consider the time series of particle displacements and thereby determine distributions for local persistence times and local exchange times these basic characterizations o... | [['with', 'molecular', 'dynamics', 'simulations', 'of', 'a', 'fluid', 'mixture', 'of', 'classical', 'particles', 'interacting', 'with', 'pairwise', 'additive', 'weekschandlerandersen', 'potentials', 'we', 'consider', 'the', 'time', 'series', 'of', 'particle', 'displacements', 'and', 'thereby', 'determine', 'distributio... | [-0.11619191021324966, 0.21835130879756165, -0.0959927217304908, 0.05956337214573412, 0.04491762450984302, -0.14792341034154635, -0.03242492157261114, 0.385722782154492, -0.290085462936691, -0.28882717006411907, 0.060600160916864466, -0.256951913073961, -0.13175578960028753, 0.13308775513841947, 0.04243989741882762, 0.... |
708.0761 | Statistics of quantum transmission in one dimension with broad disorder | We study the statistics of quantum transmission through a one-dimensional
disordered system modelled by a sequence of independent scattering units. Each
unit is characterized by its length and by its action, which is proportional to
the logarithm of the transmission probability through this unit. Unit actions
and len... | cond-mat.stat-mech cond-mat.mes-hall | we study the statistics of quantum transmission through a onedimensional disordered system modelled by a sequence of independent scattering units each unit is characterized by its length and by its action which is proportional to the logarithm of the transmission probability through this unit unit actions and lengths a... | [['we', 'study', 'the', 'statistics', 'of', 'quantum', 'transmission', 'through', 'a', 'onedimensional', 'disordered', 'system', 'modelled', 'by', 'a', 'sequence', 'of', 'independent', 'scattering', 'units', 'each', 'unit', 'is', 'characterized', 'by', 'its', 'length', 'and', 'by', 'its', 'action', 'which', 'is', 'prop... | [-0.13662098218228894, 0.2384706479625183, -0.06599472787814563, 0.0014509734886974752, 0.0019241861786672865, -0.13786126953385935, 0.0499097720251654, 0.3663629286482439, -0.2828287932878503, -0.2943128388666722, 0.1140810683239149, -0.33081244885061795, -0.09879254721550292, 0.17297499036035183, -0.02049700721105622... |
708.0762 | Red Halos of Galaxies - Reservoirs of Baryonic Dark Matter? | Deep optical/near-IR surface photometry of galaxies outside the Local Group
have revealed faint and very red halos around objects as diverse as disk
galaxies and starbursting dwarf galaxies. The colours of these structures are
too extreme to be reconciled with stellar populations similar to those seen in
the stellar ... | astro-ph | deep opticalnearir surface photometry of galaxies outside the local group have revealed faint and very red halos around objects as diverse as disk galaxies and starbursting dwarf galaxies the colours of these structures are too extreme to be reconciled with stellar populations similar to those seen in the stellar halos... | [['deep', 'opticalnearir', 'surface', 'photometry', 'of', 'galaxies', 'outside', 'the', 'local', 'group', 'have', 'revealed', 'faint', 'and', 'very', 'red', 'halos', 'around', 'objects', 'as', 'diverse', 'as', 'disk', 'galaxies', 'and', 'starbursting', 'dwarf', 'galaxies', 'the', 'colours', 'of', 'these', 'structures',... | [-0.032823305173647094, 0.12598305576914776, -0.12871903163749118, 0.18526280403332135, -0.15941361863934977, -0.08386178039079316, 0.02581427519772808, 0.4577873118741568, -0.08525645581268987, -0.3916255213471866, 0.021764944419860408, -0.28355924968694357, -0.022545276629348653, 0.18735256200239367, -0.0775253170787... |
708.0763 | Diquark approach to calculating the mass and stability of multiquark
states | By using of vector diquark ideas in the chiral limit diquark correlations in
the relativistic region and imposing HF interactions between quarks in a vector
diquark we calculated the mass of two multiquark states (Theta pentaquark and H
dibaryon), also by using of tunneling method we simultaneously calculated their
d... | hep-ph | by using of vector diquark ideas in the chiral limit diquark correlations in the relativistic region and imposing hf interactions between quarks in a vector diquark we calculated the mass of two multiquark states theta pentaquark and h dibaryon also by using of tunneling method we simultaneously calculated their decay ... | [['by', 'using', 'of', 'vector', 'diquark', 'ideas', 'in', 'the', 'chiral', 'limit', 'diquark', 'correlations', 'in', 'the', 'relativistic', 'region', 'and', 'imposing', 'hf', 'interactions', 'between', 'quarks', 'in', 'a', 'vector', 'diquark', 'we', 'calculated', 'the', 'mass', 'of', 'two', 'multiquark', 'states', 'th... | [-0.10528692281713672, 0.2994606683724651, -0.0830260497556689, 0.18262875043586188, -0.0022727543597712238, -0.13778875716140165, 0.11731801777347631, 0.3865230386601944, -0.1564117965891081, -0.23915103402938329, -0.12057839185410343, -0.27003049441412386, -0.03011922706283775, 0.013938810091977026, 0.164787376577413... |
708.0764 | Experimental quantum state tomography of a solid state qubit | Full quantum state tomography is used to characterize the state of an
ensemble based qubit implemented through two hyperfine levels in Pr3+ ions,
doped into a Y2SiO5 crystal. We experimentally verify that single-qubit
rotation errors due to inhomogeneities of the ensemble can be suppressed using
the Roos-Moelmer dark... | quant-ph | full quantum state tomography is used to characterize the state of an ensemble based qubit implemented through two hyperfine levels in pr3 ions doped into a y2sio5 crystal we experimentally verify that singlequbit rotation errors due to inhomogeneities of the ensemble can be suppressed using the roosmoelmer dark state ... | [['full', 'quantum', 'state', 'tomography', 'is', 'used', 'to', 'characterize', 'the', 'state', 'of', 'an', 'ensemble', 'based', 'qubit', 'implemented', 'through', 'two', 'hyperfine', 'levels', 'in', 'pr3', 'ions', 'doped', 'into', 'a', 'y2sio5', 'crystal', 'we', 'experimentally', 'verify', 'that', 'singlequbit', 'rota... | [-0.09186575155814782, 0.2582039065290968, -0.014410216424285489, 0.06508955930578797, 0.04352917919921524, -0.17339979309917372, 0.09236947473083787, 0.4458139603628832, -0.21766732234288663, -0.2723325342816465, 0.03017909517237807, -0.2272492577047909, 0.00503038245746318, 0.1843360790544573, -0.017989600573063775, ... |
708.0765 | Anisotropic fluxes and nonlocal interactions in MHD turbulence | We investigate the locality or nonlocality of the energy transfer and of the
spectral interactions involved in the cascade for decaying magnetohydrodynamic
(MHD) flows in the presence of a uniform magnetic field $\bf B$ at various
intensities. The results are based on a detailed analysis of three-dimensional
numerica... | physics.flu-dyn physics.plasm-ph | we investigate the locality or nonlocality of the energy transfer and of the spectral interactions involved in the cascade for decaying magnetohydrodynamic mhd flows in the presence of a uniform magnetic field bf b at various intensities the results are based on a detailed analysis of threedimensional numerical flows a... | [['we', 'investigate', 'the', 'locality', 'or', 'nonlocality', 'of', 'the', 'energy', 'transfer', 'and', 'of', 'the', 'spectral', 'interactions', 'involved', 'in', 'the', 'cascade', 'for', 'decaying', 'magnetohydrodynamic', 'mhd', 'flows', 'in', 'the', 'presence', 'of', 'a', 'uniform', 'magnetic', 'field', 'bf', 'b', '... | [-0.1869035262321324, 0.2013451627595988, -0.007216805124657492, 0.09264262649496448, -0.02362918585419791, -0.07518442037204902, -0.02505238283187423, 0.3039555918705994, -0.28037223974551123, -0.30029775679949244, 0.04805008922416513, -0.2881053609456697, -0.04982782592125169, 0.18460763175546543, 0.08238048039878544... |
708.0766 | Invariant rigid geometric structures and smooth projective factors | We consider actions of non-compact simple Lie groups preserving an analytic
rigid geometric structure of algebraic type on a compact manifold. The
structure is not assumed to be unimodular, so an invariant measure may not
exist. Ergodic stationary measures always exist, and when such a measure has
full support, we sh... | math.DS math.DG | we consider actions of noncompact simple lie groups preserving an analytic rigid geometric structure of algebraic type on a compact manifold the structure is not assumed to be unimodular so an invariant measure may not exist ergodic stationary measures always exist and when such a measure has full support we show the f... | [['we', 'consider', 'actions', 'of', 'noncompact', 'simple', 'lie', 'groups', 'preserving', 'an', 'analytic', 'rigid', 'geometric', 'structure', 'of', 'algebraic', 'type', 'on', 'a', 'compact', 'manifold', 'the', 'structure', 'is', 'not', 'assumed', 'to', 'be', 'unimodular', 'so', 'an', 'invariant', 'measure', 'may', '... | [-0.18707745417461122, 0.06850019807667694, -0.10053292155241082, 0.0672600420917677, -0.1426061564990509, -0.14291612442069795, 0.0004472287651975598, 0.3694735936062262, -0.3081639155053196, -0.1838501003710965, 0.14044191048633042, -0.20853632570458658, -0.16315805081142096, 0.20744162670695182, -0.1573401992394696,... |
708.0767 | Collisionsless amplifying of longitudinal electron waves in two-stream
plasma | To better understanding the principal features of collisionless
damping/growing plasma waves we have implemented a demonstrative calculation
for the simplest cases of electron waves in two-stream plasmas with the
delta-function type electron velocity distribution function of each of the
streams with velocities v(1) a... | physics.plasm-ph | to better understanding the principal features of collisionless dampinggrowing plasma waves we have implemented a demonstrative calculation for the simplest cases of electron waves in twostream plasmas with the deltafunction type electron velocity distribution function of each of the streams with velocities v1 and v2 t... | [['to', 'better', 'understanding', 'the', 'principal', 'features', 'of', 'collisionless', 'dampinggrowing', 'plasma', 'waves', 'we', 'have', 'implemented', 'a', 'demonstrative', 'calculation', 'for', 'the', 'simplest', 'cases', 'of', 'electron', 'waves', 'in', 'twostream', 'plasmas', 'with', 'the', 'deltafunction', 'ty... | [-0.17347538731725062, 0.13492955699227616, -0.05036599276449959, 0.0809505550261419, -0.09591466934252225, -0.14976934355790497, -0.05839497370065236, 0.3246338199459104, -0.24757565487344124, -0.2085975977595987, 0.056982842845113214, -0.31550816416389266, -0.11143747962568505, 0.22485856879426197, 0.0432343144212147... |
708.0768 | Measurement of single electron emission in two-phase xenon | We present the first measurements of the electroluminescence response to the
emission of single electrons in a two-phase noble gas detector. Single
ionization electrons generated in liquid xenon are detected in a thin gas layer
during the 31-day background run of the ZEPLIN-II experiment, a two-phase xenon
detector f... | physics.ins-det | we present the first measurements of the electroluminescence response to the emission of single electrons in a twophase noble gas detector single ionization electrons generated in liquid xenon are detected in a thin gas layer during the 31day background run of the zeplinii experiment a twophase xenon detector for wimp ... | [['we', 'present', 'the', 'first', 'measurements', 'of', 'the', 'electroluminescence', 'response', 'to', 'the', 'emission', 'of', 'single', 'electrons', 'in', 'a', 'twophase', 'noble', 'gas', 'detector', 'single', 'ionization', 'electrons', 'generated', 'in', 'liquid', 'xenon', 'are', 'detected', 'in', 'a', 'thin', 'ga... | [-0.06817087491223026, 0.1707493939111888, -0.05729832252452396, 0.008592619813258215, 0.02616358568610729, -0.1179754924037898, 0.011768506275366922, 0.3842825014847067, -0.20702594688232495, -0.3565009701162366, 0.008685988613474622, -0.34565164549616695, -0.007597797172460353, 0.19220179015823272, 0.0476317018894303... |
708.0769 | Fragmentation functions for pions, kaons, protons and charged hadrons | We present new sets of pion, kaon, proton and inclusive charged hadron
fragmentation functions obtained in NLO combined analyses of single-inclusive
hadron production in electron-positron annihilation, proton-proton collisions,
and deep-inelastic lepton-proton scattering with either particles identified in
the final ... | hep-ph nucl-th | we present new sets of pion kaon proton and inclusive charged hadron fragmentation functions obtained in nlo combined analyses of singleinclusive hadron production in electronpositron annihilation protonproton collisions and deepinelastic leptonproton scattering with either particles identified in the final state at va... | [['we', 'present', 'new', 'sets', 'of', 'pion', 'kaon', 'proton', 'and', 'inclusive', 'charged', 'hadron', 'fragmentation', 'functions', 'obtained', 'in', 'nlo', 'combined', 'analyses', 'of', 'singleinclusive', 'hadron', 'production', 'in', 'electronpositron', 'annihilation', 'protonproton', 'collisions', 'and', 'deepi... | [0.017729614545325085, 0.2782445859563138, -0.16678022633173636, 0.18278631863317318, -0.0007592909437205111, -0.08227129928751051, -0.005800547984628273, 0.3175116748149906, -0.14018485760981483, -0.18167307223193346, -0.12273554473816017, -0.4045069180262674, 0.17252698796136037, 0.09436046220362186, 0.17608417408274... |
708.077 | Control of atomic entanglement by dynamic Stark effect | We study the entanglement properties of two three-level Rydberg atoms passing
through a single-mode cavity. The interaction of an atom with the cavity field
allows the atom to make a transition from the upper most (lower most) to the
lower most (upper most) level by emission (absoprtion) of two photons via the
middle... | quant-ph | we study the entanglement properties of two threelevel rydberg atoms passing through a singlemode cavity the interaction of an atom with the cavity field allows the atom to make a transition from the upper most lower most to the lower most upper most level by emission absoprtion of two photons via the middle level we e... | [['we', 'study', 'the', 'entanglement', 'properties', 'of', 'two', 'threelevel', 'rydberg', 'atoms', 'passing', 'through', 'a', 'singlemode', 'cavity', 'the', 'interaction', 'of', 'an', 'atom', 'with', 'the', 'cavity', 'field', 'allows', 'the', 'atom', 'to', 'make', 'a', 'transition', 'from', 'the', 'upper', 'most', 'l... | [-0.13387057208796493, 0.2140427729162886, -0.03966158772791512, 0.02174271564938847, 0.00219100090090937, -0.15992946096570693, 0.07024513294257234, 0.39299134011462067, -0.23669910188818796, -0.28018520637388117, 0.006016659506117347, -0.26364837681245923, -0.06692808440529703, 0.21396262857420315, 0.0177955522354452... |
708.0771 | Ejection of Supermassive Black Holes from Galaxy Cores | [Abridged] Recent numerical relativity simulations have shown that the
emission of gravitational waves during the merger of two supermassive black
holes (SMBHs) delivers a kick to the final hole, with a magnitude as large as
4000 km/s. We study the motion of SMBHs ejected from galaxy cores by such kicks
and the effec... | astro-ph | abridged recent numerical relativity simulations have shown that the emission of gravitational waves during the merger of two supermassive black holes smbhs delivers a kick to the final hole with a magnitude as large as 4000 kms we study the motion of smbhs ejected from galaxy cores by such kicks and the effects on the... | [['abridged', 'recent', 'numerical', 'relativity', 'simulations', 'have', 'shown', 'that', 'the', 'emission', 'of', 'gravitational', 'waves', 'during', 'the', 'merger', 'of', 'two', 'supermassive', 'black', 'holes', 'smbhs', 'delivers', 'a', 'kick', 'to', 'the', 'final', 'hole', 'with', 'a', 'magnitude', 'as', 'large',... | [-0.10852552017271709, 0.1731799276292947, -0.06664088567871435, 0.11073226344480844, -0.06669317370236123, -0.056244996050134326, 0.010588984683381692, 0.36121213171510314, -0.17246804501123905, -0.34300986204158085, 0.06860495417231038, -0.3038204921212416, -0.021279097918727764, 0.1952308176129853, 0.024569574047401... |
708.0772 | Design of a mode converter for efficient light-atom coupling in free
space | In this article, we describe how to develop a mode converter that transforms
a plane electromagnetic wave into an inward moving dipole wave. The latter one
is intended to bring a single atom or ion from its ground state to its excited
state by absorption of a single photon wave packet with near-100% efficiency.
| quant-ph | in this article we describe how to develop a mode converter that transforms a plane electromagnetic wave into an inward moving dipole wave the latter one is intended to bring a single atom or ion from its ground state to its excited state by absorption of a single photon wave packet with near100 efficiency | [['in', 'this', 'article', 'we', 'describe', 'how', 'to', 'develop', 'a', 'mode', 'converter', 'that', 'transforms', 'a', 'plane', 'electromagnetic', 'wave', 'into', 'an', 'inward', 'moving', 'dipole', 'wave', 'the', 'latter', 'one', 'is', 'intended', 'to', 'bring', 'a', 'single', 'atom', 'or', 'ion', 'from', 'its', 'g... | [-0.13464628153101163, 0.17822199359916677, -0.07433758470385025, -0.002332198881992587, -0.09687845405467131, -0.12471593507669038, 0.0804810582038179, 0.38413223231004345, -0.26770841033646353, -0.22408021631202213, 0.02721365105955758, -0.30487484929876196, -0.04446738897564097, 0.13816817076790525, 0.05046595015597... |
708.0773 | S=-1,-2 baryon-baryon interactions in chiral effective field theory | We have constructed the leading order strangeness S=-1,-2 baryon-baryon
potential in a chiral effective field theory approach. The chiral potential
consists of one-pseudoscalar-meson exchanges and non-derivative four-baryon
contact terms. The potential, derived using SU(3) symmetry constraints,
contains six independe... | nucl-th | we have constructed the leading order strangeness s12 baryonbaryon potential in a chiral effective field theory approach the chiral potential consists of onepseudoscalarmeson exchanges and nonderivative fourbaryon contact terms the potential derived using su3 symmetry constraints contains six independent lowenergy coef... | [['we', 'have', 'constructed', 'the', 'leading', 'order', 'strangeness', 's12', 'baryonbaryon', 'potential', 'in', 'a', 'chiral', 'effective', 'field', 'theory', 'approach', 'the', 'chiral', 'potential', 'consists', 'of', 'onepseudoscalarmeson', 'exchanges', 'and', 'nonderivative', 'fourbaryon', 'contact', 'terms', 'th... | [-0.1836657215149678, 0.09963936179745801, -0.11028894635312485, 0.0863320311376204, -0.06071549864260085, -0.1573293940869696, -0.0042032784320216515, 0.3201645914690964, -0.14645582830505163, -0.27193705252879724, 0.0022611077716150744, -0.35476982469360036, -0.12451631902491278, 0.07789845677149115, 0.09265160184418... |
708.0774 | Ergodicity of the $\Delta_3$ statistic and purity of neutron resonance
data | The $\Delta_3(L)$ statistic characterizes the fluctuations of the number of
levels as a function of the length of the spectral interval. It is studied as a
possible tool to indicate the regular or chaotic nature of underlying dynamics,
detect missing levels and the mixing of sequences of levels of different
symmetry,... | nucl-th | the delta_3l statistic characterizes the fluctuations of the number of levels as a function of the length of the spectral interval it is studied as a possible tool to indicate the regular or chaotic nature of underlying dynamics detect missing levels and the mixing of sequences of levels of different symmetry particula... | [['the', 'delta_3l', 'statistic', 'characterizes', 'the', 'fluctuations', 'of', 'the', 'number', 'of', 'levels', 'as', 'a', 'function', 'of', 'the', 'length', 'of', 'the', 'spectral', 'interval', 'it', 'is', 'studied', 'as', 'a', 'possible', 'tool', 'to', 'indicate', 'the', 'regular', 'or', 'chaotic', 'nature', 'of', '... | [-0.13291032766677086, 0.11933576087871735, -0.10988008466639877, 0.1286473523328839, -0.002998286330726294, -0.08014685952360123, 0.057673415749135995, 0.32053486003944304, -0.23784216249411086, -0.3421766918020702, 0.06751615987097498, -0.2598916232355137, -0.08160264638615196, 0.19198536623755585, -0.010515227798471... |
708.0775 | Breit type equation for mesonic atoms | The finite size effects and relativistic corrections in pionic and kaonic
hydrogen are evaluated by generalizing the Breit equation for a spin-0 -
spin-1/2 amplitude with the inclusion of the hadron electromagnetic form
factors. The agreement of the relativistic corrections to the energies of the
mesonic atoms with o... | nucl-th hep-ph nucl-ex | the finite size effects and relativistic corrections in pionic and kaonic hydrogen are evaluated by generalizing the breit equation for a spin0 spin12 amplitude with the inclusion of the hadron electromagnetic form factors the agreement of the relativistic corrections to the energies of the mesonic atoms with other met... | [['the', 'finite', 'size', 'effects', 'and', 'relativistic', 'corrections', 'in', 'pionic', 'and', 'kaonic', 'hydrogen', 'are', 'evaluated', 'by', 'generalizing', 'the', 'breit', 'equation', 'for', 'a', 'spin0', 'spin12', 'amplitude', 'with', 'the', 'inclusion', 'of', 'the', 'hadron', 'electromagnetic', 'form', 'factor... | [-0.047515656605519985, 0.18017927000680603, -0.045299963481410084, 0.13877058094956474, -0.039806860908641516, -0.09683444813323061, 0.021411189439156687, 0.33720145493476505, -0.19352967747071959, -0.29525424545372736, -0.035626246690671576, -0.34929664379142855, 0.021397177623697073, 0.1618149850674602, 0.0774993417... |
708.0776 | Time scale competition leading to fragmentation and recombination
transitions in the coevolution of network and states | We study the co-evolution of network structure and node states in a model of
multiple state interacting agents. The system displays two transitions, network
recombination and fragmentation, governed by time scales that emerge from the
dynamics. The recombination transition separates a frozen configuration,
composed b... | physics.soc-ph physics.data-an | we study the coevolution of network structure and node states in a model of multiple state interacting agents the system displays two transitions network recombination and fragmentation governed by time scales that emerge from the dynamics the recombination transition separates a frozen configuration composed by discon... | [['we', 'study', 'the', 'coevolution', 'of', 'network', 'structure', 'and', 'node', 'states', 'in', 'a', 'model', 'of', 'multiple', 'state', 'interacting', 'agents', 'the', 'system', 'displays', 'two', 'transitions', 'network', 'recombination', 'and', 'fragmentation', 'governed', 'by', 'time', 'scales', 'that', 'emerge... | [-0.21277593656451302, 0.2420630045258337, -0.10045719790824614, 0.010564615365851307, 0.0244921114773745, -0.1500244518552404, 0.07068752165393392, 0.3548789460179025, -0.30198487246293676, -0.26366700883954763, 0.04954248055943444, -0.2867033621615656, -0.15868543449838737, 0.04227428492447114, 0.10437173217502052, -... |
708.0777 | Microstrip resonator for microwaves with controllable polarization | In this work the authors implemented a resonator based upon microstrip
cavities that permits the generation of microwaves with arbitrary polarization.
Design, simulation, and implementation of the resonators were performed using
standard printed circuit boards. The electric field distribution was mapped
using a scann... | cond-mat.other | in this work the authors implemented a resonator based upon microstrip cavities that permits the generation of microwaves with arbitrary polarization design simulation and implementation of the resonators were performed using standard printed circuit boards the electric field distribution was mapped using a scanning pr... | [['in', 'this', 'work', 'the', 'authors', 'implemented', 'a', 'resonator', 'based', 'upon', 'microstrip', 'cavities', 'that', 'permits', 'the', 'generation', 'of', 'microwaves', 'with', 'arbitrary', 'polarization', 'design', 'simulation', 'and', 'implementation', 'of', 'the', 'resonators', 'were', 'performed', 'using',... | [-0.1309192590010555, 0.06505459844323712, -0.06631937666215758, -0.0747256923713249, -0.05952960661733928, -0.18617338636566116, 0.029495172325751162, 0.42618504169302573, -0.17898820318362635, -0.3228784536645896, 0.06643406565274125, -0.258698460780948, -0.08166722183966119, 0.26382692569893773, 0.04237181998188675,... |
708.0778 | Singular integral operators on variable Lebesgue spaces with radial
oscillating weights | We prove a Fredholm criterion for operators in the Banach algebra of singular
integral operators with matrix piecewise continuous coefficients acting on a
variable Lebesgue space with a radial oscillating weight over a logarithmic
Carleson curve. The local spectra of these operators are massive and have a
shape of sp... | math.FA math.CA | we prove a fredholm criterion for operators in the banach algebra of singular integral operators with matrix piecewise continuous coefficients acting on a variable lebesgue space with a radial oscillating weight over a logarithmic carleson curve the local spectra of these operators are massive and have a shape of spira... | [['we', 'prove', 'a', 'fredholm', 'criterion', 'for', 'operators', 'in', 'the', 'banach', 'algebra', 'of', 'singular', 'integral', 'operators', 'with', 'matrix', 'piecewise', 'continuous', 'coefficients', 'acting', 'on', 'a', 'variable', 'lebesgue', 'space', 'with', 'a', 'radial', 'oscillating', 'weight', 'over', 'a', ... | [-0.12278152268492815, 0.09952686169252947, -0.0987363740013362, 0.0686187921750425, -0.07231520090047552, -0.12643130365382843, 0.050650388991631885, 0.3655451395069108, -0.300811477108962, -0.13738147250254346, 0.15260534494470882, -0.29683168851441205, -0.10987172197230687, 0.2127942136851036, -0.11452278550337962, ... |
708.0779 | Real-time gauge theory simulations from stochastic quantization with
optimized updating | We investigate simulations for gauge theories on a Minkowskian space-time
lattice. We employ stochastic quantization with optimized updating using
stochastic reweighting or gauge fixing, respectively. These procedures do not
affect the underlying theory but strongly improve the stability properties of
the stochastic ... | hep-lat hep-ph hep-th nucl-th | we investigate simulations for gauge theories on a minkowskian spacetime lattice we employ stochastic quantization with optimized updating using stochastic reweighting or gauge fixing respectively these procedures do not affect the underlying theory but strongly improve the stability properties of the stochastic dynami... | [['we', 'investigate', 'simulations', 'for', 'gauge', 'theories', 'on', 'a', 'minkowskian', 'spacetime', 'lattice', 'we', 'employ', 'stochastic', 'quantization', 'with', 'optimized', 'updating', 'using', 'stochastic', 'reweighting', 'or', 'gauge', 'fixing', 'respectively', 'these', 'procedures', 'do', 'not', 'affect', ... | [-0.11122175972504576, 0.1671187561005354, -0.10144985632373477, 0.1100385510977709, -0.0903082855116084, -0.14475208370647621, 0.04803409315601764, 0.45014976573018534, -0.23923137480006465, -0.24946507938065618, 0.12749291772796018, -0.20532763963740952, -0.18572476554117254, 0.12877728267933047, -0.03338666412241335... |
708.078 | A weight function theory of zero order basis function interpolants and
smoothers | I develop a weight func theory of zero order basis func interpolants and
smoothers.**Ch1 Basis funcs and data spaces are defined using wt funcs. Data
(native)spaces are used to formulate the variational problems which define our
interpolants /smoothers. Introduce the tensor prod extended B-splines.**Ch2
Prove the p't... | math.NA | i develop a weight func theory of zero order basis func interpolants and smoothersch1 basis funcs and data spaces are defined using wt funcs data nativespaces are used to formulate the variational problems which define our interpolants smoothers introduce the tensor prod extended bsplinesch2 prove the ptwise convergenc... | [['i', 'develop', 'a', 'weight', 'func', 'theory', 'of', 'zero', 'order', 'basis', 'func', 'interpolants', 'and', 'smoothersch1', 'basis', 'funcs', 'and', 'data', 'spaces', 'are', 'defined', 'using', 'wt', 'funcs', 'data', 'nativespaces', 'are', 'used', 'to', 'formulate', 'the', 'variational', 'problems', 'which', 'def... | [-0.04071671913059154, 0.045116227981853496, -0.08058504666820149, 0.11219409876127517, -0.05797080639486892, -0.07345736040909004, 0.00028106464009638543, 0.3563227279889514, -0.32727309615321215, -0.1939829141185302, 0.16665186162697532, -0.2698803040287441, -0.08797469228905823, 0.15550775931627359, -0.0855486961851... |
708.0781 | A new modified Galerkin method for the two-dimensional Navier-Stokes
equations | We present a new type of modified Galerkin method. It is a construction with
several (inductively defined) levels, that provides approximate solutions of
increasing accuracy with every new level. These solutions are constructed as
approximations of the so called induced trajectories (notion on which the
definition of... | math.NA math.AP | we present a new type of modified galerkin method it is a construction with several inductively defined levels that provides approximate solutions of increasing accuracy with every new level these solutions are constructed as approximations of the so called induced trajectories notion on which the definition of a class... | [['we', 'present', 'a', 'new', 'type', 'of', 'modified', 'galerkin', 'method', 'it', 'is', 'a', 'construction', 'with', 'several', 'inductively', 'defined', 'levels', 'that', 'provides', 'approximate', 'solutions', 'of', 'increasing', 'accuracy', 'with', 'every', 'new', 'level', 'these', 'solutions', 'are', 'constructe... | [-0.09122193202612892, 0.05486623659020379, -0.11326053438501225, 0.04905804850545431, -0.07548913359642029, -0.13797790787020137, 0.008790929591105808, 0.3466253120688692, -0.2621486575475761, -0.2790984536210696, 0.09977544398630954, -0.2315802431650578, -0.16165149965811343, 0.2164433454237287, -0.07526905540495164,... |
708.0782 | Universal regularization prescription for Lovelock AdS gravity | A definite form for the boundary term that produces the finiteness of both
the conserved quantities and Euclidean action for any Lovelock gravity with AdS
asymptotics is presented. This prescription merely tells even from odd bulk
dimensions, regardless the particular theory considered, what is valid even for
Einstei... | hep-th gr-qc | a definite form for the boundary term that produces the finiteness of both the conserved quantities and euclidean action for any lovelock gravity with ads asymptotics is presented this prescription merely tells even from odd bulk dimensions regardless the particular theory considered what is valid even for einsteinhilb... | [['a', 'definite', 'form', 'for', 'the', 'boundary', 'term', 'that', 'produces', 'the', 'finiteness', 'of', 'both', 'the', 'conserved', 'quantities', 'and', 'euclidean', 'action', 'for', 'any', 'lovelock', 'gravity', 'with', 'ads', 'asymptotics', 'is', 'presented', 'this', 'prescription', 'merely', 'tells', 'even', 'fr... | [-0.16593628095568352, 0.145124754426216, -0.08548064520231115, 0.15134903820928586, -0.10902631346505347, -0.18044029817617727, -0.032346626655081485, 0.2543921120488231, -0.2073618887452139, -0.23425685039446134, 0.11965752629498781, -0.2961944581987629, -0.15284552488991487, 0.11092004277772687, -0.09678280785527525... |
708.0783 | The HMW effect in Noncommutative Quantum Mechanics | The HMW effect in non-commutative quantum mechanics is studied. By solving
the Dirac equations on non-commutative (NC) space and non-commutative phase
space, we obtain topological HMW phase on NC space and NC phase space
respectively, where the additional terms related to the space-space and
momentum-momentum non-com... | hep-th | the hmw effect in noncommutative quantum mechanics is studied by solving the dirac equations on noncommutative nc space and noncommutative phase space we obtain topological hmw phase on nc space and nc phase space respectively where the additional terms related to the spacespace and momentummomentum noncommutativity ar... | [['the', 'hmw', 'effect', 'in', 'noncommutative', 'quantum', 'mechanics', 'is', 'studied', 'by', 'solving', 'the', 'dirac', 'equations', 'on', 'noncommutative', 'nc', 'space', 'and', 'noncommutative', 'phase', 'space', 'we', 'obtain', 'topological', 'hmw', 'phase', 'on', 'nc', 'space', 'and', 'nc', 'phase', 'space', 'r... | [-0.1679948058587556, 0.232250512501567, -0.03604578435877148, 0.1058649983261807, -0.06937283090296753, -0.11758539274486961, 0.005471204060642999, 0.29578257179153816, -0.252487126053596, -0.27372816763818264, 0.0516692698358235, -0.22828807522143638, -0.20501894549447663, 0.1516503051531558, -0.11517376650352867, 0.... |
708.0784 | Doppler-Free Spectroscopy of Weak Transitions: An Analytical Model
Applied to Formaldehyde | Experimental observation of Doppler-free signals for weak transitions can be
greatly facilitated by an estimate for their expected amplitudes. We derive an
analytical model which allows the Doppler-free amplitude to be estimated for
small Doppler-free signals. Application of this model to formaldehyde allows
the ampl... | physics.optics | experimental observation of dopplerfree signals for weak transitions can be greatly facilitated by an estimate for their expected amplitudes we derive an analytical model which allows the dopplerfree amplitude to be estimated for small dopplerfree signals application of this model to formaldehyde allows the amplitude o... | [['experimental', 'observation', 'of', 'dopplerfree', 'signals', 'for', 'weak', 'transitions', 'can', 'be', 'greatly', 'facilitated', 'by', 'an', 'estimate', 'for', 'their', 'expected', 'amplitudes', 'we', 'derive', 'an', 'analytical', 'model', 'which', 'allows', 'the', 'dopplerfree', 'amplitude', 'to', 'be', 'estimate... | [-0.09383965872934666, 0.15189323594024934, -0.07271592691540718, 0.05489618105388343, -0.04191102601330856, -0.13385547678275356, 0.11476335962752587, 0.404948169887387, -0.25773256374442755, -0.3286832990927686, 0.0779544756956527, -0.18127291017775987, -0.1132100974500645, 0.2540981019646379, 0.01815733364542368, 0.... |
708.0785 | SuperWASP-North Extra-solar Planet Candidates between 3hr < RA < 6hr | The Wide Angle Search for Planets (WASP) photometrically surveys a large
number of nearby stars to uncover candidate extrasolar planet systems by virtue
of small-amplitude lightcurve dips on a < 5-day timescale typical of the
``Hot-Jupiters.'' Observations with the SuperWASP-North instrument between
April and Septemb... | astro-ph | the wide angle search for planets wasp photometrically surveys a large number of nearby stars to uncover candidate extrasolar planet systems by virtue of smallamplitude lightcurve dips on a 5day timescale typical of the hotjupiters observations with the superwaspnorth instrument between april and september 2004 produce... | [['the', 'wide', 'angle', 'search', 'for', 'planets', 'wasp', 'photometrically', 'surveys', 'a', 'large', 'number', 'of', 'nearby', 'stars', 'to', 'uncover', 'candidate', 'extrasolar', 'planet', 'systems', 'by', 'virtue', 'of', 'smallamplitude', 'lightcurve', 'dips', 'on', 'a', '5day', 'timescale', 'typical', 'of', 'th... | [-0.07893420447286796, 0.08164935145032359, -0.07396627128279458, 0.0642835822084938, -0.09941929116515287, -0.10266128167859279, 0.12300515051295709, 0.39278576088448364, -0.1649999166414394, -0.4361748362813766, 0.1362866260260489, -0.3285166887556746, -0.05428117285070281, 0.23801309133705217, -0.0703249310715061, 0... |
708.0786 | Four-body quantum dynamics of two-center electronic transitions in
relativistic ion-atom collisions and target recoil momentum spectroscopy | We consider relativistic collisions of heavy hydrogen-like ions with hydrogen
and helium atoms in which the ion-atom interaction causes both colliding
particles to undergo transitions between their internal states. Using an
approach enabling one, for the first time, to give a detailed description of
this important ca... | physics.atom-ph | we consider relativistic collisions of heavy hydrogenlike ions with hydrogen and helium atoms in which the ionatom interaction causes both colliding particles to undergo transitions between their internal states using an approach enabling one for the first time to give a detailed description of this important case of t... | [['we', 'consider', 'relativistic', 'collisions', 'of', 'heavy', 'hydrogenlike', 'ions', 'with', 'hydrogen', 'and', 'helium', 'atoms', 'in', 'which', 'the', 'ionatom', 'interaction', 'causes', 'both', 'colliding', 'particles', 'to', 'undergo', 'transitions', 'between', 'their', 'internal', 'states', 'using', 'an', 'app... | [-0.08785502358370013, 0.22014669381657984, -0.08149382134339189, 0.11326401750083892, 0.01885154667666288, -0.10506220008208741, 0.011207667056365105, 0.3449991854528586, -0.2191979882413355, -0.2976985291343152, -0.05300467455858077, -0.3180836783722043, -0.000608406779242725, 0.1420651079927821, 0.08157938942918933,... |
708.0787 | Constraints on dark and visible mass in galaxies from strong
gravitational lensing | We give a non-exhaustive review of the use of strong gravitational lensing in
placing constraints on the quantity of dark and visible mass in galaxies. We
discuss development of the methodology and summarise some recent results.
| astro-ph | we give a nonexhaustive review of the use of strong gravitational lensing in placing constraints on the quantity of dark and visible mass in galaxies we discuss development of the methodology and summarise some recent results | [['we', 'give', 'a', 'nonexhaustive', 'review', 'of', 'the', 'use', 'of', 'strong', 'gravitational', 'lensing', 'in', 'placing', 'constraints', 'on', 'the', 'quantity', 'of', 'dark', 'and', 'visible', 'mass', 'in', 'galaxies', 'we', 'discuss', 'development', 'of', 'the', 'methodology', 'and', 'summarise', 'some', 'rece... | [-0.14369319529376096, 0.032614604130180344, -0.086202386714932, 0.08384960356892811, -0.12165262940753666, -0.018294533675846953, 0.012259686986605326, 0.353044705465436, -0.13433759682811797, -0.3232983248308301, 0.09427444387822309, -0.2500147903079374, -0.13294674523381722, 0.2407862922280199, -0.06708022923622695,... |
708.0788 | Unidirectional d-wave superconducting domains in the two-dimensional t-J
model | Motivated by the recently observed pattern of unidirectional domains in
high-T_c superconductors [Y. Kohsaka et al., Science 315, 1380 (2007)], we
investigate the emergence of spontaneous modulations in the d-wave
superconducting resonating valence bond phase using the t-J model at x=1/8
doping. Half-filled charge do... | cond-mat.str-el | motivated by the recently observed pattern of unidirectional domains in hight_c superconductors y kohsaka et al science 315 1380 2007 we investigate the emergence of spontaneous modulations in the dwave superconducting resonating valence bond phase using the tj model at x18 doping halffilled charge domains separated by... | [['motivated', 'by', 'the', 'recently', 'observed', 'pattern', 'of', 'unidirectional', 'domains', 'in', 'hight_c', 'superconductors', 'y', 'kohsaka', 'et', 'al', 'science', '315', '1380', '2007', 'we', 'investigate', 'the', 'emergence', 'of', 'spontaneous', 'modulations', 'in', 'the', 'dwave', 'superconducting', 'reson... | [-0.17607111957234642, 0.2662763514769419, -0.003838586557928162, 0.06391215069258276, -0.043445049858614006, -0.1636948950593554, 0.12072703371692721, 0.4145394741014267, -0.2416628948461342, -0.2938886087422361, -0.025079880359650513, -0.347583484215041, -0.09182742653259386, 0.10877836490302191, 0.06151665452246865,... |
708.0789 | Theory of point contact spectroscopy in electron-doped cuprates | In the hole-doped $d_{x^{2}-y^{2}}$-wave cuprate superconductor, due to the
midgap surface state (MSS), a zero bias conductance peak (ZBCP) is widely
observed in [110] interface point contact spectroscopy (PCS). However, ZBCP of
this geometry is rarely observed in the electron-doped cuprates, even though
their pairin... | cond-mat.supr-con cond-mat.str-el | in the holedoped d_x2y2wave cuprate superconductor due to the midgap surface state mss a zero bias conductance peak zbcp is widely observed in 110 interface point contact spectroscopy pcs however zbcp of this geometry is rarely observed in the electrondoped cuprates even though their pairing symmetry is still likely th... | [['in', 'the', 'holedoped', 'd_x2y2wave', 'cuprate', 'superconductor', 'due', 'to', 'the', 'midgap', 'surface', 'state', 'mss', 'a', 'zero', 'bias', 'conductance', 'peak', 'zbcp', 'is', 'widely', 'observed', 'in', '110', 'interface', 'point', 'contact', 'spectroscopy', 'pcs', 'however', 'zbcp', 'of', 'this', 'geometry'... | [-0.24502144915185464, 0.15660546372006623, -0.0585890527962163, 0.11904965841907565, -0.06712250072983933, -0.21872486278765124, 0.09116036494695905, 0.3715982779417888, -0.22761001707156106, -0.24660859837906784, -0.018624557965979126, -0.35248880104927144, -0.14450542811341216, 0.14654643070137147, -0.00640112452098... |
708.079 | Stellar Evolutionary Effects on the Abundances of PAH and SN-Condensed
Dust in Galaxies | Spectral and photometric observations of nearby galaxies show a correlation
between the strength of their mid-IR aromatic features, attributed to PAH
molecules, and their metal abundance, leading to a deficiency of these features
in low-metallicity galaxies. In this paper, we suggest that the observed
correlation rep... | astro-ph | spectral and photometric observations of nearby galaxies show a correlation between the strength of their midir aromatic features attributed to pah molecules and their metal abundance leading to a deficiency of these features in lowmetallicity galaxies in this paper we suggest that the observed correlation represents a... | [['spectral', 'and', 'photometric', 'observations', 'of', 'nearby', 'galaxies', 'show', 'a', 'correlation', 'between', 'the', 'strength', 'of', 'their', 'midir', 'aromatic', 'features', 'attributed', 'to', 'pah', 'molecules', 'and', 'their', 'metal', 'abundance', 'leading', 'to', 'a', 'deficiency', 'of', 'these', 'feat... | [0.010136505607869882, 0.11729937762804869, -0.05816396398412231, 0.10252300872040603, -0.038002652545928606, -0.013393239177210067, 0.06006089714946279, 0.4862190213229885, -0.15061339196425094, -0.33227593907951447, -0.041767835733902546, -0.29686084557392134, -0.0024990372697610164, 0.10387506874268064, -0.042077215... |
708.0791 | An unexpected outburst from A0535+262 | A0535+262 is a transient Be/X-ray binary system which was in a quiescent
phase from 1994-2005. In this paper we report on the timing and spectral
properties of the INTEGRAL detection of the source in October 2003. The source
is detected for ~6000 seconds in the 18-100 keV energy band at a luminosity of
~3.8 x 10^{35}... | astro-ph | a0535262 is a transient bexray binary system which was in a quiescent phase from 19942005 in this paper we report on the timing and spectral properties of the integral detection of the source in october 2003 the source is detected for 6000 seconds in the 18100 kev energy band at a luminosity of 38 x 1035 erg s1 this is... | [['a0535262', 'is', 'a', 'transient', 'bexray', 'binary', 'system', 'which', 'was', 'in', 'a', 'quiescent', 'phase', 'from', '19942005', 'in', 'this', 'paper', 'we', 'report', 'on', 'the', 'timing', 'and', 'spectral', 'properties', 'of', 'the', 'integral', 'detection', 'of', 'the', 'source', 'in', 'october', '2003', 't... | [-0.1288412024832058, 0.1277412825121002, -0.04269501418102442, 0.054326056459458635, -0.06247665370223907, -0.07415407990877766, 0.060812801713970056, 0.41492709869564304, -0.20087394675824838, -0.3518386809623846, 0.13830431662116585, -0.2912095740576638, -0.019593837439570938, 0.2337394446097655, -0.0659897548697389... |
708.0792 | The RHIC azimuth quadrupole: "perfect liquid" or gluonic radiation? | Large elliptic flow at RHIC seems to indicate that ideal hydrodynamics
provides a good description of Au-Au collisions, at least at the maximum RHIC
energy. The medium formed has been interpreted as a nearly perfect
(low-viscosity) liquid, and connections have been made to gravitation through
string theory. Recently,... | hep-ph | large elliptic flow at rhic seems to indicate that ideal hydrodynamics provides a good description of auau collisions at least at the maximum rhic energy the medium formed has been interpreted as a nearly perfect lowviscosity liquid and connections have been made to gravitation through string theory recently claimed ob... | [['large', 'elliptic', 'flow', 'at', 'rhic', 'seems', 'to', 'indicate', 'that', 'ideal', 'hydrodynamics', 'provides', 'a', 'good', 'description', 'of', 'auau', 'collisions', 'at', 'least', 'at', 'the', 'maximum', 'rhic', 'energy', 'the', 'medium', 'formed', 'has', 'been', 'interpreted', 'as', 'a', 'nearly', 'perfect', ... | [-0.11981363179377065, 0.17397267701856506, -0.20392731943955789, 0.12475354575390855, -0.06720089383709889, -0.10678676256121925, -0.12785032733451002, 0.3282727113423439, -0.22502688449234343, -0.29906827222842436, -0.01612653104463019, -0.3287103655676429, 0.0006122356012033728, 0.1543482763119615, -0.00934754465348... |
708.0793 | Gravitational Field of A Radiating Star in Higher Dimensions | We obtain fields of a relativistic radiating star of non-static mass in the
framework of higher dimensional spacetime. Assuming energy-momentum tensor in
Higher dimensions analogous to that considered by Vaidya in 4 dimensions we
obtain solution of a radiating spherically symmetric star. The solution
obtained here is... | astro-ph | we obtain fields of a relativistic radiating star of nonstatic mass in the framework of higher dimensional spacetime assuming energymomentum tensor in higher dimensions analogous to that considered by vaidya in 4 dimensions we obtain solution of a radiating spherically symmetric star the solution obtained here is new i... | [['we', 'obtain', 'fields', 'of', 'a', 'relativistic', 'radiating', 'star', 'of', 'nonstatic', 'mass', 'in', 'the', 'framework', 'of', 'higher', 'dimensional', 'spacetime', 'assuming', 'energymomentum', 'tensor', 'in', 'higher', 'dimensions', 'analogous', 'to', 'that', 'considered', 'by', 'vaidya', 'in', '4', 'dimensio... | [-0.12134488898196391, 0.1643164731462353, -0.06445713679256317, 0.029238445217613065, -0.051158958089737486, -0.11419012908092034, -0.037278740284299214, 0.3197269809565374, -0.1143459718275283, -0.27488240488206167, 0.07229057288350305, -0.2329858843835869, -0.10539480729494244, 0.1542226992106797, -0.046236899452716... |
708.0794 | Spin blockade and lifetime-enhanced transport in a few-electron Si/SiGe
double quantum dot | Spin blockade occurs when an electron is unable to access an energetically
favorable path through a quantum dot due to spin conservation, resulting in a
blockade of the current through the dot. Spin blockade is the basis of a number
of recent advances in spintronics, including the measurement and the
manipulation of ... | cond-mat.mes-hall | spin blockade occurs when an electron is unable to access an energetically favorable path through a quantum dot due to spin conservation resulting in a blockade of the current through the dot spin blockade is the basis of a number of recent advances in spintronics including the measurement and the manipulation of indiv... | [['spin', 'blockade', 'occurs', 'when', 'an', 'electron', 'is', 'unable', 'to', 'access', 'an', 'energetically', 'favorable', 'path', 'through', 'a', 'quantum', 'dot', 'due', 'to', 'spin', 'conservation', 'resulting', 'in', 'a', 'blockade', 'of', 'the', 'current', 'through', 'the', 'dot', 'spin', 'blockade', 'is', 'the... | [-0.16996034563549878, 0.22169399868396475, -0.0022766256143393762, 0.03419358981602058, -0.0008943892316892743, -0.19497478162006968, 0.050746829995392435, 0.4089745230808416, -0.27575741861672964, -0.275243971743347, 0.04316580945776556, -0.29102192658876236, -0.08798566658515483, 0.26695351607700374, -0.001668954973... |
708.0795 | A weight function theory of positive order basis function interpolants
and smoothers | In this document I develop a weight function theory of positive order basis
function interpolants and smoothers. **In Chapter 1 the basis functions and
data spaces are defined directly using weight functions. The data spaces are
used to formulate the variational problems which define the interpolants and
smoothers di... | math.NA | in this document i develop a weight function theory of positive order basis function interpolants and smoothers in chapter 1 the basis functions and data spaces are defined directly using weight functions the data spaces are used to formulate the variational problems which define the interpolants and smoothers discusse... | [['in', 'this', 'document', 'i', 'develop', 'a', 'weight', 'function', 'theory', 'of', 'positive', 'order', 'basis', 'function', 'interpolants', 'and', 'smoothers', 'in', 'chapter', '1', 'the', 'basis', 'functions', 'and', 'data', 'spaces', 'are', 'defined', 'directly', 'using', 'weight', 'functions', 'the', 'data', 's... | [-0.05876296013593674, 0.03503297904071492, -0.0732091377070052, 0.12670936603228908, -0.05940298038414754, -0.0869002742331819, 0.0028551202405321992, 0.36205026507053123, -0.32431083664343485, -0.25222461006380226, 0.16483010698307812, -0.2694662954895157, -0.15015495533771805, 0.1776341774009285, -0.0589426660058226... |
708.0796 | Summary of alphas determinations at ZEUS | The jet cross-section and structure-function measurements done with the ZEUS
detector to extract the strong coupling constant and to test its energy-scale
dependence are summarised. The values of alphas thus obtained and the HERA
average are also presented.
| hep-ex | the jet crosssection and structurefunction measurements done with the zeus detector to extract the strong coupling constant and to test its energyscale dependence are summarised the values of alphas thus obtained and the hera average are also presented | [['the', 'jet', 'crosssection', 'and', 'structurefunction', 'measurements', 'done', 'with', 'the', 'zeus', 'detector', 'to', 'extract', 'the', 'strong', 'coupling', 'constant', 'and', 'to', 'test', 'its', 'energyscale', 'dependence', 'are', 'summarised', 'the', 'values', 'of', 'alphas', 'thus', 'obtained', 'and', 'the'... | [-0.053609373244015796, 0.1285384329722116, -0.08736209250300338, 0.0777578120683565, -0.07100653993333444, -0.12420954629717591, 0.0006205465301479164, 0.38702230091745915, -0.20820312339224314, -0.32733006589114666, 0.04215170244539255, -0.3368373377444713, 0.034214580590885724, 0.18531789658223524, 0.139092874198563... |
708.0797 | Near BPS Wilson Loop in beta-deformed Theories | We propose a definition of the Wilson loop operator in the N=1 beta-deformed
supersymmetric Yang-Mills theory. Although the operator is not BPS, it has a
finite expectation value at least up to order (g^2 N)^2. This does not happen
generally for a generic non-BPS Wilson loop whose expectation value is UV
divergent. F... | hep-th | we propose a definition of the wilson loop operator in the n1 betadeformed supersymmetric yangmills theory although the operator is not bps it has a finite expectation value at least up to order g2 n2 this does not happen generally for a generic nonbps wilson loop whose expectation value is uv divergent for this reason... | [['we', 'propose', 'a', 'definition', 'of', 'the', 'wilson', 'loop', 'operator', 'in', 'the', 'n1', 'betadeformed', 'supersymmetric', 'yangmills', 'theory', 'although', 'the', 'operator', 'is', 'not', 'bps', 'it', 'has', 'a', 'finite', 'expectation', 'value', 'at', 'least', 'up', 'to', 'order', 'g2', 'n2', 'this', 'doe... | [-0.14468064422080676, 0.17371383508032912, -0.07972653614922415, 0.10642098940504251, -0.0838874016805068, -0.15860647710211023, 0.005996686215288774, 0.329671073589051, -0.17015001466131757, -0.2257642356310788, 0.12296622526408967, -0.25792842764838486, -0.15066345965725625, 0.10770710688653731, -0.0906774513138759,... |
708.0798 | Cluster Complexes via Semi-Invariants | We define and study virtual representation spaces having both positive and
negative dimensions at the vertices of a quiver without oriented cycles. We
consider the natural semi-invariants on these spaces which we call virtual
semi-invariants and prove that they satisfy the three basic theorems: the First
Fundamental ... | math.RT math.RA | we define and study virtual representation spaces having both positive and negative dimensions at the vertices of a quiver without oriented cycles we consider the natural semiinvariants on these spaces which we call virtual semiinvariants and prove that they satisfy the three basic theorems the first fundamental theore... | [['we', 'define', 'and', 'study', 'virtual', 'representation', 'spaces', 'having', 'both', 'positive', 'and', 'negative', 'dimensions', 'at', 'the', 'vertices', 'of', 'a', 'quiver', 'without', 'oriented', 'cycles', 'we', 'consider', 'the', 'natural', 'semiinvariants', 'on', 'these', 'spaces', 'which', 'we', 'call', 'vi... | [-0.16978424067148962, 0.12489509284047477, -0.07522574727457151, 0.09621628153233239, -0.07836360042263944, -0.1277717676024929, 0.026875484846981174, 0.32565493028925124, -0.31223979109830885, -0.2315822302262826, 0.055636858824270226, -0.2317390115735267, -0.18799598903552325, 0.1197253296892327, -0.1418015349695616... |
708.0799 | Tests of mode coupling theory in a simple model for two-component
miscible polymer blends | We present molecular dynamics simulations on the structural relaxation of a
simple bead-spring model for polymer blends. The introduction of a different
monomer size induces a large time scale separation for the dynamics of the two
components. Simulation results for a large set of observables probing density
correlat... | cond-mat.soft | we present molecular dynamics simulations on the structural relaxation of a simple beadspring model for polymer blends the introduction of a different monomer size induces a large time scale separation for the dynamics of the two components simulation results for a large set of observables probing density correlations ... | [['we', 'present', 'molecular', 'dynamics', 'simulations', 'on', 'the', 'structural', 'relaxation', 'of', 'a', 'simple', 'beadspring', 'model', 'for', 'polymer', 'blends', 'the', 'introduction', 'of', 'a', 'different', 'monomer', 'size', 'induces', 'a', 'large', 'time', 'scale', 'separation', 'for', 'the', 'dynamics', ... | [-0.1841362485491861, 0.1684189357807965, -0.10783358761209554, 0.03494148614055287, -0.006650360935162352, -0.1304795327727803, 0.005301664286713687, 0.34361816960467045, -0.2950014627328323, -0.25442425393930046, 0.03786490705385003, -0.2311403520144923, -0.13691490269716708, 0.12615936188157448, 0.09114979879219606,... |
708.08 | Elliptic flow in the Gaussian model of eccentricity fluctuations | We discuss a specific model of elliptic flow fluctuations due to Gaussian
fluctuations in the initial spatial $x$ and $y$ eccentricity components
$\left\{\mean{(\sigma_y^2-\sigma_x^2)/(\sigma_x^2+\sigma_y^2)},
\mean{2\sigma_{xy}/(\sigma_x^2+\sigma_y^2)} \right\}$. We find that in this
model $\vfour$, elliptic flow de... | nucl-th | we discuss a specific model of elliptic flow fluctuations due to gaussian fluctuations in the initial spatial x and y eccentricity components leftmeansigma_y2sigma_x2sigma_x2sigma_y2 mean2sigma_xysigma_x2sigma_y2 right we find that in this model vfour elliptic flow determined from 4particle cumulants exactly equals the... | [['we', 'discuss', 'a', 'specific', 'model', 'of', 'elliptic', 'flow', 'fluctuations', 'due', 'to', 'gaussian', 'fluctuations', 'in', 'the', 'initial', 'spatial', 'x', 'and', 'y', 'eccentricity', 'components', 'leftmeansigma_y2sigma_x2sigma_x2sigma_y2', 'mean2sigma_xysigma_x2sigma_y2', 'right', 'we', 'find', 'that', 'i... | [-0.12865890275349212, 0.13553507667140213, -0.1535889019971979, 0.0566743902097994, 0.006520538948292674, -0.09086838918803654, -0.040925195794814906, 0.3324545994400978, -0.2721324817041381, -0.24908925572895563, 0.05835092107808008, -0.3219689780282198, -0.09352414935013988, 0.17928399130354414, -0.03337931605449445... |
708.0801 | Rapid directional alignment of velocity and magnetic field in
magnetohydrodynamic turbulence | We show that local directional alignment of the velocity and magnetic field
fluctuations occurs rapidly in magnetohydrodynamics for a variety of
parameters. This is observed both in direct numerical simulations and in solar
wind data. The phenomenon is due to an alignment between the magnetic field and
either pressur... | astro-ph | we show that local directional alignment of the velocity and magnetic field fluctuations occurs rapidly in magnetohydrodynamics for a variety of parameters this is observed both in direct numerical simulations and in solar wind data the phenomenon is due to an alignment between the magnetic field and either pressure gr... | [['we', 'show', 'that', 'local', 'directional', 'alignment', 'of', 'the', 'velocity', 'and', 'magnetic', 'field', 'fluctuations', 'occurs', 'rapidly', 'in', 'magnetohydrodynamics', 'for', 'a', 'variety', 'of', 'parameters', 'this', 'is', 'observed', 'both', 'in', 'direct', 'numerical', 'simulations', 'and', 'in', 'sola... | [-0.20123535803365475, 0.16306753034911964, -0.052302556017467985, 0.04407675798089276, -0.06471322322698328, -0.031229101001619568, -0.0596449095473254, 0.33402301835854653, -0.33001516887452453, -0.3024702693349275, 0.06460288129023557, -0.1873999331621182, -0.09869052880461716, 0.18128360652147782, -0.01224384464106... |
708.0802 | From Percolation to Logarithmic Conformal Field Theory | The smallest deformation of the minimal model M(2,3) that can accommodate
Cardy's derivation of the percolation crossing probability is presented. It is
shown that this leads to a consistent logarithmic conformal field theory at
c=0. A simple recipe for computing the associated fusion rules is given. The
differences ... | hep-th math-ph math.MP | the smallest deformation of the minimal model m23 that can accommodate cardys derivation of the percolation crossing probability is presented it is shown that this leads to a consistent logarithmic conformal field theory at c0 a simple recipe for computing the associated fusion rules is given the differences between th... | [['the', 'smallest', 'deformation', 'of', 'the', 'minimal', 'model', 'm23', 'that', 'can', 'accommodate', 'cardys', 'derivation', 'of', 'the', 'percolation', 'crossing', 'probability', 'is', 'presented', 'it', 'is', 'shown', 'that', 'this', 'leads', 'to', 'a', 'consistent', 'logarithmic', 'conformal', 'field', 'theory'... | [-0.1582361724599591, 0.1384037163096492, -0.09350518580426329, 0.11859021309986953, -0.08225695334084622, -0.18381916701358247, 0.0055855465656019405, 0.30288947812075934, -0.2266618495855432, -0.24840006194766853, 0.0329287805860596, -0.270691226212332, -0.20894108185326898, 0.1369859301273457, -0.07120625853732035, ... |
708.0803 | On the all-order epsilon-expansion of generalized hypergeometric
functions with integer values of parameters | We continue our study of the construction of analytical coefficients of the
epsilon-expansion of hypergeometric functions and their connection with Feynman
diagrams. In this paper, we apply the approach of obtaining iteratated
solutions to the differential equations associated with hypergeometric
functions to prove t... | hep-th hep-ph math-ph math.CA math.MP | we continue our study of the construction of analytical coefficients of the epsilonexpansion of hypergeometric functions and their connection with feynman diagrams in this paper we apply the approach of obtaining iteratated solutions to the differential equations associated with hypergeometric functions to prove the fo... | [['we', 'continue', 'our', 'study', 'of', 'the', 'construction', 'of', 'analytical', 'coefficients', 'of', 'the', 'epsilonexpansion', 'of', 'hypergeometric', 'functions', 'and', 'their', 'connection', 'with', 'feynman', 'diagrams', 'in', 'this', 'paper', 'we', 'apply', 'the', 'approach', 'of', 'obtaining', 'iteratated'... | [-0.16845392656850292, 0.016901015412928485, -0.12518595721941073, 0.03471824123938619, -0.08899797545234253, -0.08303440814060005, 0.015691582391110178, 0.28256410594702097, -0.25365805609540626, -0.24840037633695608, 0.05267931977517207, -0.262958867362813, -0.2251422677680359, 0.22927677660034254, -0.037687703762408... |
708.0804 | Some pseudo-Anosov maps on punctured Riemann surfaces represented by
multi-twists | This paper has been withdrawn by the author
| math.GT math.CV | this paper has been withdrawn by the author | [['this', 'paper', 'has', 'been', 'withdrawn', 'by', 'the', 'author']] | [-0.11762839742004871, -0.04127746832091361, -0.17016396392136812, -0.1582642109860899, -0.18072871817275882, -0.04020218155346811, -0.09601712167204823, 0.33764172717928886, -0.2455208501778543, -0.3865965995937586, 0.12438089866191149, -0.3554150704294443, -0.17133164615370333, -0.03124168887734413, -0.36054937075823... |
708.0805 | Cooperative Beamforming for Wireless Ad Hoc Networks | Via collaborative beamforming, nodes in a wireless network are able to
transmit a common message over long distances in an energy efficient fashion.
However, the process of making available the same message to all collaborating
nodes introduces delays. In this paper, a MAC-PHY cross-layer scheme is
proposed that enab... | cs.IT math.IT | via collaborative beamforming nodes in a wireless network are able to transmit a common message over long distances in an energy efficient fashion however the process of making available the same message to all collaborating nodes introduces delays in this paper a macphy crosslayer scheme is proposed that enables colla... | [['via', 'collaborative', 'beamforming', 'nodes', 'in', 'a', 'wireless', 'network', 'are', 'able', 'to', 'transmit', 'a', 'common', 'message', 'over', 'long', 'distances', 'in', 'an', 'energy', 'efficient', 'fashion', 'however', 'the', 'process', 'of', 'making', 'available', 'the', 'same', 'message', 'to', 'all', 'coll... | [-0.25656271583903484, 0.06517050946406906, -0.03197109864212255, -0.03827293425022017, -0.10463059904360945, -0.25623608434800693, 0.14392287652887542, 0.39120557962946517, -0.29658626430380614, -0.26503033011388827, 0.04982561689486945, -0.2725183691883935, -0.1456713504331345, 0.10856697023623287, -0.093201966044750... |
708.0806 | Decomposition theorems and kernel theorems for a class of functional
spaces | We prove new theorems about properties of generalized functions defined on
Gelfand-Shilov spaces $S^\beta$ with $0\le\beta<1$. For each open cone
$U\subset\mathbb R^d$ we define a space $S^\beta(U)$ which is related to
$S^\beta(\mathbb R^d)$ and consists of entire analytic functions rapidly
decreasing inside U and ha... | math.FA math-ph math.MP | we prove new theorems about properties of generalized functions defined on gelfandshilov spaces sbeta with 0lebeta1 for each open cone usubsetmathbb rd we define a space sbetau which is related to sbetamathbb rd and consists of entire analytic functions rapidly decreasing inside u and having order of growth le 11beta o... | [['we', 'prove', 'new', 'theorems', 'about', 'properties', 'of', 'generalized', 'functions', 'defined', 'on', 'gelfandshilov', 'spaces', 'sbeta', 'with', '0lebeta1', 'for', 'each', 'open', 'cone', 'usubsetmathbb', 'rd', 'we', 'define', 'a', 'space', 'sbetau', 'which', 'is', 'related', 'to', 'sbetamathbb', 'rd', 'and', ... | [-0.13378957347223128, 0.11492413943773486, -0.08183900161499255, 0.095132890444501, -0.043136177129371275, -0.08828313095158988, 0.027057957701574088, 0.3394640111556991, -0.31599116720315207, -0.141947146449098, 0.11394076737491204, -0.2634106249079332, -0.15893870166347965, 0.22324623716504952, -0.08263623723900296,... |
708.0807 | Dynamical magnetic susceptibility in the lamellar cobaltate
superconductor Na_xCoO_2$\cdot y$H_2O | We systematically analyze the influence of the superconducting gap symmetry
and the electronic structure on the dynamical spin susceptibility in
superconducting Na_xCoO_2$\cdot y$H_2O within a three different models: the
single a_{1g}-band model with nearest-neighbor hoppings, the realistic
three-band t_{2g}-model wi... | cond-mat.supr-con cond-mat.str-el | we systematically analyze the influence of the superconducting gap symmetry and the electronic structure on the dynamical spin susceptibility in superconducting na_xcoo_2cdot yh_2o within a three different models the single a_1gband model with nearestneighbor hoppings the realistic threeband t_2gmodel with and without ... | [['we', 'systematically', 'analyze', 'the', 'influence', 'of', 'the', 'superconducting', 'gap', 'symmetry', 'and', 'the', 'electronic', 'structure', 'on', 'the', 'dynamical', 'spin', 'susceptibility', 'in', 'superconducting', 'na_xcoo_2cdot', 'yh_2o', 'within', 'a', 'three', 'different', 'models', 'the', 'single', 'a_1... | [-0.18305244750635688, 0.2014724873754728, -0.028029343506897845, 0.05317341413077278, -0.050894450662391524, -0.1234444756943655, 0.09009193666445624, 0.37937672122470323, -0.21621457153066462, -0.2738504960971546, 0.003050358059616493, -0.34207472248956383, -0.08962914839919124, 0.1436349558990471, 0.0970104457574918... |
708.0808 | Statistical comparison of ensemble implementations of Grover's search
algorithm to classical sequential searches | We compare pseudopure state ensemble implementations, quantified by their
initial polarization and ensemble size, of Grover's search algorithm to
probabilistic classical sequential search algorithms in terms of their success
and failure probabilities. We propose a criterion for quantifying the resources
used by the e... | quant-ph | we compare pseudopure state ensemble implementations quantified by their initial polarization and ensemble size of grovers search algorithm to probabilistic classical sequential search algorithms in terms of their success and failure probabilities we propose a criterion for quantifying the resources used by the ensembl... | [['we', 'compare', 'pseudopure', 'state', 'ensemble', 'implementations', 'quantified', 'by', 'their', 'initial', 'polarization', 'and', 'ensemble', 'size', 'of', 'grovers', 'search', 'algorithm', 'to', 'probabilistic', 'classical', 'sequential', 'search', 'algorithms', 'in', 'terms', 'of', 'their', 'success', 'and', 'f... | [-0.07827366293316945, 0.10499515596959264, -0.08064520826101079, 0.08709115061744403, -0.004960104861625827, -0.1558428285538422, 0.12254602966578047, 0.3924079188390782, -0.23789324360038328, -0.3563235344477278, 0.09392879332793891, -0.22698021836970983, -0.12012759581054176, 0.20647885282593953, 0.01226088111253833... |
708.0809 | Compositional Bernoulli numbers | We define and study the combinatorial properties of compositional
Bernoulli numbers and polynomials within the framework of rational
combinatorics.
| math.CO | we define and study the combinatorial properties of compositional bernoulli numbers and polynomials within the framework of rational combinatorics | [['we', 'define', 'and', 'study', 'the', 'combinatorial', 'properties', 'of', 'compositional', 'bernoulli', 'numbers', 'and', 'polynomials', 'within', 'the', 'framework', 'of', 'rational', 'combinatorics']] | [-0.15543034794054142, 0.08772381096097984, -0.1318407129300268, 0.08811324969620297, -0.10370926823663085, -0.05174425450202666, 0.10937528400436829, 0.25548835260499464, -0.44657577770320994, -0.2753007847227548, 0.026723357995874004, -0.16579615491393365, -0.25995051664741414, 0.15560047289258555, -0.133364347116041... |
708.081 | All-optical formation of a Bose-Einstein condensate for applications in
scanning electron microscopy | We report on the production of a F=1 spinor condensate of 87Rb atoms in a
single beam optical dipole trap formed by a focused CO2 laser. The condensate
is produced 13mm below the tip of a scanning electron microscope employing
standard all-optical techniques. The condensate fraction contains up to 100,000
atoms and w... | cond-mat.stat-mech | we report on the production of a f1 spinor condensate of 87rb atoms in a single beam optical dipole trap formed by a focused co2 laser the condensate is produced 13mm below the tip of a scanning electron microscope employing standard alloptical techniques the condensate fraction contains up to 100000 atoms and we achie... | [['we', 'report', 'on', 'the', 'production', 'of', 'a', 'f1', 'spinor', 'condensate', 'of', '87rb', 'atoms', 'in', 'a', 'single', 'beam', 'optical', 'dipole', 'trap', 'formed', 'by', 'a', 'focused', 'co2', 'laser', 'the', 'condensate', 'is', 'produced', '13mm', 'below', 'the', 'tip', 'of', 'a', 'scanning', 'electron', ... | [-0.13806742731649735, 0.25195790450451283, -0.009770920057399352, -0.01951317343150922, 0.05521586250330581, -0.14374741049269674, 0.12402376688283975, 0.4366422056174669, -0.1290418554066879, -0.2833870597733337, -0.025311476530003377, -0.3212241725843461, 0.05428793806521619, 0.2145424566124795, 0.0322911456135697, ... |
708.0811 | Star product algebras of test functions | We prove that the Gelfand-Shilov spaces $S^\beta_\alpha$ are topological
algebras under the Moyal star product if and only if $\alpha\ge\beta$. These
spaces of test functions can be used in quantum field theory on noncommutative
spacetime. The star product depends on the noncommutativity parameter
continuously in the... | math-ph hep-th math.MP math.QA | we prove that the gelfandshilov spaces sbeta_alpha are topological algebras under the moyal star product if and only if alphagebeta these spaces of test functions can be used in quantum field theory on noncommutative spacetime the star product depends on the noncommutativity parameter continuously in their topology we ... | [['we', 'prove', 'that', 'the', 'gelfandshilov', 'spaces', 'sbeta_alpha', 'are', 'topological', 'algebras', 'under', 'the', 'moyal', 'star', 'product', 'if', 'and', 'only', 'if', 'alphagebeta', 'these', 'spaces', 'of', 'test', 'functions', 'can', 'be', 'used', 'in', 'quantum', 'field', 'theory', 'on', 'noncommutative',... | [-0.10994662032317137, 0.19748782835085876, -0.13418313542933902, 0.09381003171438351, -0.0732151277770754, -0.09665409605077002, -0.026641449590897537, 0.3828345418733079, -0.3073733330529649, -0.14706739550456405, 0.13418103016192617, -0.23285368649521843, -0.17644912787363864, 0.20155657941359095, -0.124120724649401... |
708.0812 | Quark-Gluon Plasmas and Thermalization | In these lectures, I will attempt a pedagogical and qualitative introduction
to the theory of equilibrium and thermalization of quark-gluon plasmas. I
assume only that the reader is familiar with quantum field theory at zero
temperature and with QCD as the theory of the strong interactions. I focus on
the limit of sm... | hep-ph nucl-th | in these lectures i will attempt a pedagogical and qualitative introduction to the theory of equilibrium and thermalization of quarkgluon plasmas i assume only that the reader is familiar with quantum field theory at zero temperature and with qcd as the theory of the strong interactions i focus on the limit of small al... | [['in', 'these', 'lectures', 'i', 'will', 'attempt', 'a', 'pedagogical', 'and', 'qualitative', 'introduction', 'to', 'the', 'theory', 'of', 'equilibrium', 'and', 'thermalization', 'of', 'quarkgluon', 'plasmas', 'i', 'assume', 'only', 'that', 'the', 'reader', 'is', 'familiar', 'with', 'quantum', 'field', 'theory', 'at',... | [-0.09925704733865667, 0.25455506161837155, -0.1258621976170292, 0.10760588225341843, -0.045938222459697906, -0.15054006438861176, -0.011047100755674836, 0.29629027083256215, -0.2164701272466386, -0.26001337125478674, 0.03326666933329155, -0.28566187134286924, -0.06228798904362344, 0.10555913864613273, 0.01684786688289... |
708.0813 | Experimental test of nonlocal realistic theories without the rotational
symmetry assumption | We analyze the class of nonlocal realistic theories that was originally
considered by Leggett [Found. Phys. 33, 1469 (2003)] and tested by us in a
recent experiment [Nature (London) 446, 871 (2007)]. We derive an
incompatibility theorem that works for finite numbers of polarizer settings and
that does not require the... | quant-ph | we analyze the class of nonlocal realistic theories that was originally considered by leggett found phys 33 1469 2003 and tested by us in a recent experiment nature london 446 871 2007 we derive an incompatibility theorem that works for finite numbers of polarizer settings and that does not require the previously assum... | [['we', 'analyze', 'the', 'class', 'of', 'nonlocal', 'realistic', 'theories', 'that', 'was', 'originally', 'considered', 'by', 'leggett', 'found', 'phys', '33', '1469', '2003', 'and', 'tested', 'by', 'us', 'in', 'a', 'recent', 'experiment', 'nature', 'london', '446', '871', '2007', 'we', 'derive', 'an', 'incompatibilit... | [-0.09480976185170553, 0.1488491536873225, -0.05800474755546098, 0.11137422430454202, -0.05970569202295875, -0.20243189600045963, 0.06686253836678882, 0.29751852235846943, -0.13517883838334632, -0.3694757840205585, -0.0035685943502191736, -0.24991606304081537, -0.09381093428299953, 0.2298946408980516, -0.06228013860402... |
708.0814 | The Young Cluster Population of M82 Region B | We present observations obtained with the Advanced Camera for Surveys on
board the Hubble Space Telescope of the "fossil" starburst region B in the
nearby starburst galaxy M82. By comparing UBVI photometry with models, we
derive ages and extinctions for 35 U-band selected star clusters. We find that
the peak epoch of... | astro-ph | we present observations obtained with the advanced camera for surveys on board the hubble space telescope of the fossil starburst region b in the nearby starburst galaxy m82 by comparing ubvi photometry with models we derive ages and extinctions for 35 uband selected star clusters we find that the peak epoch of cluster... | [['we', 'present', 'observations', 'obtained', 'with', 'the', 'advanced', 'camera', 'for', 'surveys', 'on', 'board', 'the', 'hubble', 'space', 'telescope', 'of', 'the', 'fossil', 'starburst', 'region', 'b', 'in', 'the', 'nearby', 'starburst', 'galaxy', 'm82', 'by', 'comparing', 'ubvi', 'photometry', 'with', 'models', '... | [-0.032964879825997814, 0.09524305935152778, -0.09593161457829927, 0.12436038938202185, -0.09524847966888865, -0.014495778523010792, 0.05381914417496359, 0.46216347220645854, -0.13650047009295546, -0.3658104571761817, 0.06258022712513298, -0.26760310987727, -0.01810397685935291, 0.18702928525996368, -0.0394409234160571... |
708.0815 | Scaling Relations from Sunyaev-Zel'dovich Effect and Chandra X-ray
measurements of high-redshift galaxy clusters | We present Sunyaev-Zel'dovich Effect (SZE) scaling relations for 38 massive
galaxy clusters at redshifts 0.14<z0.89, observed with both the Cchandra X-ray
Observatory and the centimeter-wave SZE imaging system at the BIMA and OVRO
interferometric arrays. An isothermal beta-model with central 100 kpc excluded
from the... | astro-ph | we present sunyaevzeldovich effect sze scaling relations for 38 massive galaxy clusters at redshifts 014z089 observed with both the cchandra xray observatory and the centimeterwave sze imaging system at the bima and ovro interferometric arrays an isothermal betamodel with central 100 kpc excluded from the xray data is ... | [['we', 'present', 'sunyaevzeldovich', 'effect', 'sze', 'scaling', 'relations', 'for', '38', 'massive', 'galaxy', 'clusters', 'at', 'redshifts', '014z089', 'observed', 'with', 'both', 'the', 'cchandra', 'xray', 'observatory', 'and', 'the', 'centimeterwave', 'sze', 'imaging', 'system', 'at', 'the', 'bima', 'and', 'ovro'... | [-0.01215833569463763, 0.04890829316695266, -0.10179000706411898, 0.10929931573825137, -0.08070475040754724, -0.049140207655727866, 0.05069707127197856, 0.4380659312490494, -0.17298606791864, -0.3780371831910264, 0.07209122903915423, -0.360324266991548, -0.029415946655095584, 0.23839059205004764, 0.05943297306225905, 0... |
708.0816 | Parton energy loss in an expanding quark-gluon plasma: Radiative vs
collisional | We perform a comparison of the radiative and collisional parton energy losses
in an expanding quark-gluon plasma. The radiative energy loss is calculated
within the light-cone path integral approach. The collisional energy loss is
calculated using the Bjorken method with an accurate treatment of the binary
collision ... | hep-ph | we perform a comparison of the radiative and collisional parton energy losses in an expanding quarkgluon plasma the radiative energy loss is calculated within the lightcone path integral approach the collisional energy loss is calculated using the bjorken method with an accurate treatment of the binary collision kinema... | [['we', 'perform', 'a', 'comparison', 'of', 'the', 'radiative', 'and', 'collisional', 'parton', 'energy', 'losses', 'in', 'an', 'expanding', 'quarkgluon', 'plasma', 'the', 'radiative', 'energy', 'loss', 'is', 'calculated', 'within', 'the', 'lightcone', 'path', 'integral', 'approach', 'the', 'collisional', 'energy', 'lo... | [-0.019445126162721746, 0.16766615115248182, -0.10643278059339331, 0.15366957809710977, -0.003299058492605885, -0.026258203886970078, 0.004763385035618338, 0.4250751581563744, -0.20358162074379862, -0.2716609718258022, -0.039761539791480345, -0.29749797875442174, 0.04718713065789592, 0.18507042228774997, 0.047339539371... |
708.0817 | Values at s=-1 of L-functions for multi-quadratic extensions of number
fields, and the fitting ideal of the tame kernel | Fix a Galois extension E/F of totally real number fields such that the Galois
group G has exponent 2. Let S be a finite set of primes of F containing the
infinite primes and all those which ramify in E, let S_E denote the primes of E
lying above those in S, and let O_E^S denote the ring of S_E-integers of E. We
then ... | math.NT math.KT | fix a galois extension ef of totally real number fields such that the galois group g has exponent 2 let s be a finite set of primes of f containing the infinite primes and all those which ramify in e let s_e denote the primes of e lying above those in s and let o_es denote the ring of s_eintegers of e we then compare t... | [['fix', 'a', 'galois', 'extension', 'ef', 'of', 'totally', 'real', 'number', 'fields', 'such', 'that', 'the', 'galois', 'group', 'g', 'has', 'exponent', '2', 'let', 's', 'be', 'a', 'finite', 'set', 'of', 'primes', 'of', 'f', 'containing', 'the', 'infinite', 'primes', 'and', 'all', 'those', 'which', 'ramify', 'in', 'e'... | [-0.20909357466167067, 0.1060976855848666, -0.07108398361653998, 0.01854102952383095, -0.054977296292568874, -0.14216051186241846, -0.016799740283182117, 0.25862452442326195, -0.30280690032012036, -0.24760415291175156, 0.045207720619013035, -0.280104109073319, -0.059136994765140116, 0.21045306606627093, -0.033422378522... |
708.0818 | Dressing the Giant Gluon | We demonstrate the applicability of the dressing method to the problem of
constructing new classical solutions for Euclidean worldsheets in anti-de
Sitter space. The motivation stems from recent work of Alday and Maldacena, who
studied gluon scattering amplitudes at strong coupling using a generalization
of a particu... | hep-th | we demonstrate the applicability of the dressing method to the problem of constructing new classical solutions for euclidean worldsheets in antide sitter space the motivation stems from recent work of alday and maldacena who studied gluon scattering amplitudes at strong coupling using a generalization of a particular w... | [['we', 'demonstrate', 'the', 'applicability', 'of', 'the', 'dressing', 'method', 'to', 'the', 'problem', 'of', 'constructing', 'new', 'classical', 'solutions', 'for', 'euclidean', 'worldsheets', 'in', 'antide', 'sitter', 'space', 'the', 'motivation', 'stems', 'from', 'recent', 'work', 'of', 'alday', 'and', 'maldacena'... | [-0.1354951438261196, 0.13341769530889716, -0.10895696872992829, 0.10382549452600023, -0.1118498821327887, -0.10611920378696506, 0.027180007071059088, 0.3332856907924213, -0.17625163948753536, -0.20167248123463724, 0.07046200535467614, -0.2923735917112467, -0.17326086650759276, 0.15419955658127027, -0.06225134913883366... |
708.0819 | Shot Noise in SU(N) Quantum Dot Kondo Effects | We study shot noise in the current of quantum dots whose low-energy behaviour
corresponds to an SU(N) Kondo model, focusing on the case N=4 relevant to
carbon nanotube dots. For general N, two-particle Fermi liquid interactions
have two distinct effects: they can enhance the noise via back-scattering
processes with a... | cond-mat.mes-hall | we study shot noise in the current of quantum dots whose lowenergy behaviour corresponds to an sun kondo model focusing on the case n4 relevant to carbon nanotube dots for general n twoparticle fermi liquid interactions have two distinct effects they can enhance the noise via backscattering processes with an ndependent... | [['we', 'study', 'shot', 'noise', 'in', 'the', 'current', 'of', 'quantum', 'dots', 'whose', 'lowenergy', 'behaviour', 'corresponds', 'to', 'an', 'sun', 'kondo', 'model', 'focusing', 'on', 'the', 'case', 'n4', 'relevant', 'to', 'carbon', 'nanotube', 'dots', 'for', 'general', 'n', 'twoparticle', 'fermi', 'liquid', 'inter... | [-0.12310219931659168, 0.20463759251082514, -0.04252089353157435, 0.09439339355499808, 0.018153647750454104, -0.17853173868143526, 0.018247514621496364, 0.35828218399800116, -0.23295997094322482, -0.28921516290258453, 0.007083000880969769, -0.35017407682481344, -0.1658684753271265, 0.13757067739346024, -0.0442207641241... |
708.082 | Multiple Sources toward the High-mass Young Star S140 IRS1 | S140 IRS1 is a remarkable source where the radio source at the center of the
main bipolar molecular outflow in the region is elongated perpendicular to the
axis of the outflow, an orientation opposite to that expected if the radio
source is a thermal jet exciting the outflow. We present results of 1.3 cm
continuum an... | astro-ph | s140 irs1 is a remarkable source where the radio source at the center of the main bipolar molecular outflow in the region is elongated perpendicular to the axis of the outflow an orientation opposite to that expected if the radio source is a thermal jet exciting the outflow we present results of 13 cm continuum and h2o... | [['s140', 'irs1', 'is', 'a', 'remarkable', 'source', 'where', 'the', 'radio', 'source', 'at', 'the', 'center', 'of', 'the', 'main', 'bipolar', 'molecular', 'outflow', 'in', 'the', 'region', 'is', 'elongated', 'perpendicular', 'to', 'the', 'axis', 'of', 'the', 'outflow', 'an', 'orientation', 'opposite', 'to', 'that', 'e... | [-0.11552010806867989, 0.07450819351879323, -0.009027141375785194, 0.003881550884078734, -0.06931117490933436, -0.12117873051930673, -0.014975703390678618, 0.49936423231734006, -0.20055494934729323, -0.2765731300749793, 0.10277690564611609, -0.2677705344675881, -0.008944286851257813, 0.12659412333968936, 0.032138679244... |
708.0821 | A massive cluster of Red Supergiants at the base of the Scutum-Crux arm | We report on the unprecedented Red Supergiant (RSG) population of a massive
young cluster, located at the base of the Scutum-Crux Galactic arm. We identify
candidate cluster RSGs based on {\it 2MASS} photometry and medium resolution
spectroscopy. With follow-up high-resolution spectroscopy, we use CO-bandhead
equival... | astro-ph | we report on the unprecedented red supergiant rsg population of a massive young cluster located at the base of the scutumcrux galactic arm we identify candidate cluster rsgs based on it 2mass photometry and medium resolution spectroscopy with followup highresolution spectroscopy we use cobandhead equivalent width and h... | [['we', 'report', 'on', 'the', 'unprecedented', 'red', 'supergiant', 'rsg', 'population', 'of', 'a', 'massive', 'young', 'cluster', 'located', 'at', 'the', 'base', 'of', 'the', 'scutumcrux', 'galactic', 'arm', 'we', 'identify', 'candidate', 'cluster', 'rsgs', 'based', 'on', 'it', '2mass', 'photometry', 'and', 'medium',... | [-0.05081708214578059, 0.05805676694943247, -0.08940137895070312, 0.05269202967133324, -0.12824551799562287, -0.034099503422344704, 0.10607515523694291, 0.4310055870054052, -0.1796528431320243, -0.3673692807475195, 0.0645196847855457, -0.2976749735137669, -0.025395912362369277, 0.17203913145136532, -0.02969349813687313... |
708.0822 | Thermal Emission from Transiting Very-Hot Jupiters: Prospects for
Ground-based Detection at Optical Wavelengths | Very hot Jupiters (VHJs) are defined as Jupiter-mass extrasolar planets with
orbital periods shorter than three days. For low albedos the effective
temperatures of irradiated VHJs can reach 2500-3000 K. Thermal emission from
VHJs is therefore potentially strong at optical wavelengths. We explore the
prospects of dete... | astro-ph | very hot jupiters vhjs are defined as jupitermass extrasolar planets with orbital periods shorter than three days for low albedos the effective temperatures of irradiated vhjs can reach 25003000 k thermal emission from vhjs is therefore potentially strong at optical wavelengths we explore the prospects of detecting opt... | [['very', 'hot', 'jupiters', 'vhjs', 'are', 'defined', 'as', 'jupitermass', 'extrasolar', 'planets', 'with', 'orbital', 'periods', 'shorter', 'than', 'three', 'days', 'for', 'low', 'albedos', 'the', 'effective', 'temperatures', 'of', 'irradiated', 'vhjs', 'can', 'reach', '25003000', 'k', 'thermal', 'emission', 'from', ... | [-0.1120783217450177, 0.21519876822130754, -0.050251190183432, 0.053355129331854795, -0.12010719028573173, -0.13617453929036855, 0.06381832742287467, 0.43029256977606567, -0.17065633356881638, -0.38095737357313436, 0.11498003711749334, -0.3166867089625157, -0.05418503204903876, 0.23836325648784015, -0.04555338708451018... |
708.0823 | Toward metastable string vacua from magnetized branes | The scalar potential of recombination fields of magnetized branes in Type IIB
orientifold compactifications is analyzed in the absence of any closed string
fluxes. Considering its perturbative F and D-term contributions in a quadratic
approximation, we present the conditions for which its minima are
supersymmetric. W... | hep-th | the scalar potential of recombination fields of magnetized branes in type iib orientifold compactifications is analyzed in the absence of any closed string fluxes considering its perturbative f and dterm contributions in a quadratic approximation we present the conditions for which its minima are supersymmetric we show... | [['the', 'scalar', 'potential', 'of', 'recombination', 'fields', 'of', 'magnetized', 'branes', 'in', 'type', 'iib', 'orientifold', 'compactifications', 'is', 'analyzed', 'in', 'the', 'absence', 'of', 'any', 'closed', 'string', 'fluxes', 'considering', 'its', 'perturbative', 'f', 'and', 'dterm', 'contributions', 'in', '... | [-0.18960244111941968, 0.2403802744758139, -0.04716074800277068, 0.16257795370853464, -0.07800662150040415, -0.18129619111739148, -0.0051535682606638645, 0.3562557720183547, -0.19856683221749133, -0.23162565968346363, 0.11461860599419334, -0.2314388839728838, -0.11922799928259908, 0.08885791120454183, -0.05444438116978... |
708.0824 | Existence of quasi-arcs | We show that doubling, linearly connected metric spaces are quasi-arc
connected. This gives a new and short proof of a theorem of Tukia.
| math.MG math.CA | we show that doubling linearly connected metric spaces are quasiarc connected this gives a new and short proof of a theorem of tukia | [['we', 'show', 'that', 'doubling', 'linearly', 'connected', 'metric', 'spaces', 'are', 'quasiarc', 'connected', 'this', 'gives', 'a', 'new', 'and', 'short', 'proof', 'of', 'a', 'theorem', 'of', 'tukia']] | [-0.2557337541619073, 0.18518268814026986, -0.14147258744291638, 0.1001286412457652, -0.1386006739112022, -0.14488587208578121, 0.04763552576870374, 0.35169184191719344, -0.258782336893289, -0.16204306169453522, 0.10269855430511676, -0.2366785450798014, -0.18912486294689385, 0.26965527074492496, -0.1916586312100939, -0... |
708.0825 | The Sloan Digital Sky Survey Quasar Lens Search. III. Constraints on
Dark Energy from the Third Data Release Quasar Lens Catalog | We present cosmological results from the statistics of lensed quasars in the
Sloan Digital Sky Survey (SDSS) Quasar Lens Search. By taking proper account of
the selection function, we compute the expected number of quasars lensed by
early-type galaxies and their image separation distribution assuming a flat
universe,... | astro-ph | we present cosmological results from the statistics of lensed quasars in the sloan digital sky survey sdss quasar lens search by taking proper account of the selection function we compute the expected number of quasars lensed by earlytype galaxies and their image separation distribution assuming a flat universe which i... | [['we', 'present', 'cosmological', 'results', 'from', 'the', 'statistics', 'of', 'lensed', 'quasars', 'in', 'the', 'sloan', 'digital', 'sky', 'survey', 'sdss', 'quasar', 'lens', 'search', 'by', 'taking', 'proper', 'account', 'of', 'the', 'selection', 'function', 'we', 'compute', 'the', 'expected', 'number', 'of', 'quas... | [-0.06524665949917915, 0.03623161563882604, -0.06941995798519605, 0.09002933793251738, -0.16782807155201832, -0.09589886511417313, 0.052022141170002416, 0.37391888562382924, -0.12837574945135405, -0.36791379933694973, 0.04198851504608885, -0.31508837847246063, -0.0023563740542158484, 0.2233796494035687, 0.0038989763625... |
708.0826 | Stellar populations across the NGC4244 truncated galactic disk | We use HST/ACS to study the resolved stellar populations of the nearby,
nearly edge-on galaxy NGC4244 across its outer disk surface density break. The
stellar photometry allows us to study the distribution of different stellar
populations and reach very low equivalent surface brightnesses. We find that
the break occu... | astro-ph | we use hstacs to study the resolved stellar populations of the nearby nearly edgeon galaxy ngc4244 across its outer disk surface density break the stellar photometry allows us to study the distribution of different stellar populations and reach very low equivalent surface brightnesses we find that the break occurs at t... | [['we', 'use', 'hstacs', 'to', 'study', 'the', 'resolved', 'stellar', 'populations', 'of', 'the', 'nearby', 'nearly', 'edgeon', 'galaxy', 'ngc4244', 'across', 'its', 'outer', 'disk', 'surface', 'density', 'break', 'the', 'stellar', 'photometry', 'allows', 'us', 'to', 'study', 'the', 'distribution', 'of', 'different', '... | [-0.06973359840277209, 0.16155618524941268, -0.08702788084252354, 0.1235727429995998, -0.0596750701889487, -0.047570205310145025, 0.04171438408129867, 0.39663499224857957, -0.21429568857374584, -0.3929215051158441, 0.04916995796363564, -0.2560839554878875, -0.010115051121615311, 0.15802845307859803, -0.0352883424390764... |
708.0827 | Simulating Quantum Correlations with Finite Communication | Assume Alice and Bob share some bipartite $d$-dimensional quantum state. A
well-known result in quantum mechanics says that by performing two-outcome
measurements, Alice and Bob can produce correlations that cannot be obtained
locally, i.e., with shared randomness alone. We show that by using only two
bits of communi... | quant-ph | assume alice and bob share some bipartite ddimensional quantum state a wellknown result in quantum mechanics says that by performing twooutcome measurements alice and bob can produce correlations that cannot be obtained locally ie with shared randomness alone we show that by using only two bits of communication alice a... | [['assume', 'alice', 'and', 'bob', 'share', 'some', 'bipartite', 'ddimensional', 'quantum', 'state', 'a', 'wellknown', 'result', 'in', 'quantum', 'mechanics', 'says', 'that', 'by', 'performing', 'twooutcome', 'measurements', 'alice', 'and', 'bob', 'can', 'produce', 'correlations', 'that', 'can', 'not', 'be', 'obtained'... | [-0.1446531767136242, 0.15511286439429414, -0.1398332706966096, 0.04033227924010855, 0.001412215301453477, -0.30276512895885965, 0.04547106961968659, 0.33736874581323845, -0.2750711190505045, -0.2985976439080026, 0.06158522824701475, -0.32024322741545075, -0.0840590528678149, 0.2008097345000225, -0.08751661246002762, 0... |
708.0828 | The Sloan Digital Sky Survey Quasar Lens Search. II. Statistical Lens
Sample from the Third Data Release | We report the first results of our systematic search for strongly lensed
quasars using the spectroscopically confirmed quasars in the Sloan Digital Sky
Survey (SDSS). Among 46,420 quasars from the SDSS Data Release 3 (~4188 deg^2),
we select a subsample of 22,683 quasars that are located at redshifts between
0.6 and ... | astro-ph | we report the first results of our systematic search for strongly lensed quasars using the spectroscopically confirmed quasars in the sloan digital sky survey sdss among 46420 quasars from the sdss data release 3 4188 deg2 we select a subsample of 22683 quasars that are located at redshifts between 06 and 22 and are br... | [['we', 'report', 'the', 'first', 'results', 'of', 'our', 'systematic', 'search', 'for', 'strongly', 'lensed', 'quasars', 'using', 'the', 'spectroscopically', 'confirmed', 'quasars', 'in', 'the', 'sloan', 'digital', 'sky', 'survey', 'sdss', 'among', '46420', 'quasars', 'from', 'the', 'sdss', 'data', 'release', '3', '41... | [-0.02582439785958502, 0.031385279391380416, -0.010457757465000259, 0.08864803848574823, -0.14299095281550672, -0.07119518866523185, 0.05186765445084129, 0.46183642320459783, -0.0495877200451435, -0.41822662503932023, 0.04683327456798363, -0.43511500467634734, 0.012928908935347415, 0.2247434208864169, 0.014949702720194... |
708.0829 | Discovery of 442-Hz Pulsations from an X-ray Source in the Globular
Cluster NGC 6440 | We report on the serendipitous discovery of a 442-Hz pulsar during a Rossi
X-ray Timing Explorer (RXTE) observation of the globular cluster NGC 6440. The
oscillation is detected following a burst-like event which was decaying at the
beginning of the observation. The time scale of the decay suggests we may have
seen t... | astro-ph | we report on the serendipitous discovery of a 442hz pulsar during a rossi xray timing explorer rxte observation of the globular cluster ngc 6440 the oscillation is detected following a burstlike event which was decaying at the beginning of the observation the time scale of the decay suggests we may have seen the tailen... | [['we', 'report', 'on', 'the', 'serendipitous', 'discovery', 'of', 'a', '442hz', 'pulsar', 'during', 'a', 'rossi', 'xray', 'timing', 'explorer', 'rxte', 'observation', 'of', 'the', 'globular', 'cluster', 'ngc', '6440', 'the', 'oscillation', 'is', 'detected', 'following', 'a', 'burstlike', 'event', 'which', 'was', 'deca... | [-0.09615044938096695, 0.20454660793353405, -0.07815011545625541, 0.1493503433806829, -0.176065419940462, -0.08381325525614496, 0.07880753437940606, 0.4253185333724579, -0.18585518576764307, -0.33389313825638045, 0.11120992082141463, -0.33425091073126806, -0.08078202267136911, 0.29127811075265525, -0.05142693630173037,... |
708.083 | Constraining Dark Energy Anisotropic Stress | We investigate the possibility of using cosmological observations to probe
and constrain an imperfect dark energy fluid. We consider a general
parameterization of the dark energy component accounting for an equation of
state, speed of sound and viscosity. We use present and future data from the
cosmic microwave backg... | astro-ph | we investigate the possibility of using cosmological observations to probe and constrain an imperfect dark energy fluid we consider a general parameterization of the dark energy component accounting for an equation of state speed of sound and viscosity we use present and future data from the cosmic microwave background... | [['we', 'investigate', 'the', 'possibility', 'of', 'using', 'cosmological', 'observations', 'to', 'probe', 'and', 'constrain', 'an', 'imperfect', 'dark', 'energy', 'fluid', 'we', 'consider', 'a', 'general', 'parameterization', 'of', 'the', 'dark', 'energy', 'component', 'accounting', 'for', 'an', 'equation', 'of', 'sta... | [-0.10457586322130787, 0.12714690186505714, -0.1086593038273497, 0.1260361912285884, -0.16886898287181817, -0.09819088170302534, 0.012759188196395297, 0.3282155832149894, -0.2716705779280715, -0.3366317611433113, 0.09184100026991596, -0.2590126576503059, -0.03842561876612111, 0.2050286683323164, 0.0023180742706687386, ... |
708.0831 | Photon wave functions, wave-packet quantization of light, and coherence
theory | The monochromatic Dirac and polychromatic Titulaer-Glauber quantized field
theories (QFTs) of electromagnetism are derived from a photon-energy wave
function in much the same way that one derives QFT for electrons, that is, by
quantization of a single-particle wave function. The photon wave function and
its equation ... | quant-ph | the monochromatic dirac and polychromatic titulaerglauber quantized field theories qfts of electromagnetism are derived from a photonenergy wave function in much the same way that one derives qft for electrons that is by quantization of a singleparticle wave function the photon wave function and its equation of motion ... | [['the', 'monochromatic', 'dirac', 'and', 'polychromatic', 'titulaerglauber', 'quantized', 'field', 'theories', 'qfts', 'of', 'electromagnetism', 'are', 'derived', 'from', 'a', 'photonenergy', 'wave', 'function', 'in', 'much', 'the', 'same', 'way', 'that', 'one', 'derives', 'qft', 'for', 'electrons', 'that', 'is', 'by'... | [-0.12418243767419443, 0.18268104864055112, -0.12312320714135687, 0.08968752828133553, -0.07476175590631018, -0.13225927295607662, -0.004366198234345178, 0.37643115441811265, -0.2577189082506723, -0.23756492711594188, 0.0100534443872352, -0.2782872808756789, -0.1572358070076136, 0.17906008320175074, 0.01749758513143219... |
708.0832 | Two Jovian-Mass Planets in Earthlike Orbits | We report the discovery of two new planets: a 1.94 M_Jup planet in a 1.8-year
orbit of HD 5319, and a 2.51 M_Jup planet in a 1.1-year orbit of HD 75898. The
measured eccentricities are 0.12 for HD 5319 b and 0.10 for HD 75898 b, and
Markov Chain Monte Carlo simulations based on derived orbital parameters
indicate tha... | astro-ph | we report the discovery of two new planets a 194 m_jup planet in a 18year orbit of hd 5319 and a 251 m_jup planet in a 11year orbit of hd 75898 the measured eccentricities are 012 for hd 5319 b and 010 for hd 75898 b and markov chain monte carlo simulations based on derived orbital parameters indicate that the radial v... | [['we', 'report', 'the', 'discovery', 'of', 'two', 'new', 'planets', 'a', '194', 'm_jup', 'planet', 'in', 'a', '18year', 'orbit', 'of', 'hd', '5319', 'and', 'a', '251', 'm_jup', 'planet', 'in', 'a', '11year', 'orbit', 'of', 'hd', '75898', 'the', 'measured', 'eccentricities', 'are', '012', 'for', 'hd', '5319', 'b', 'and... | [-0.16920884615657003, 0.16758323049342091, -0.06014443375170231, 0.030270793881605973, -0.10158281253693117, -0.09222306892360475, 0.09345056621188468, 0.3632529917765747, -0.11295626345937225, -0.33468196419152346, 0.054056660874365746, -0.2771206562153318, -0.02963585796215656, 0.22795034503691236, -0.11433852770450... |
708.0833 | The Host Galaxy of GRB 060505: Host ISM Properties | We investigate the ISM environment of GRB 060505. Using optical emission-line
diagnostic ratios, we compare the ISM properties of the GRB 060505 host region
with the hosts of unambiguous long- and short-duration GRBs. We show that the
metallicity, ionization state, and star formation rate of the GRB 060505
environmen... | astro-ph | we investigate the ism environment of grb 060505 using optical emissionline diagnostic ratios we compare the ism properties of the grb 060505 host region with the hosts of unambiguous long and shortduration grbs we show that the metallicity ionization state and star formation rate of the grb 060505 environment are more... | [['we', 'investigate', 'the', 'ism', 'environment', 'of', 'grb', '060505', 'using', 'optical', 'emissionline', 'diagnostic', 'ratios', 'we', 'compare', 'the', 'ism', 'properties', 'of', 'the', 'grb', '060505', 'host', 'region', 'with', 'the', 'hosts', 'of', 'unambiguous', 'long', 'and', 'shortduration', 'grbs', 'we', '... | [-0.05222850696527925, 0.0968487113835695, 0.005890850261177706, 0.2074437083737196, -0.12694169720229895, -0.08652120069398181, 0.08714087712376015, 0.5760132695021837, -0.058692047971746195, -0.2877771837717813, -0.037270673754139116, -0.32136496669086423, 0.04600426918098136, 0.2403356499382821, 0.003332014850836814... |
708.0834 | TrES-4: A Transiting Hot Jupiter of Very Low Density | We report the discovery of TrES-4, a hot Jupiter that transits the star GSC
02620-00648 every 3.55 days. From high-resolution spectroscopy of the star we
estimate a stellar effective temperature of Teff = 6100 +/- 150 K, and from
high-precision z and B photometry of the transit we constrain the ratio of the
semi-majo... | astro-ph | we report the discovery of tres4 a hot jupiter that transits the star gsc 0262000648 every 355 days from highresolution spectroscopy of the star we estimate a stellar effective temperature of teff 6100 150 k and from highprecision z and b photometry of the transit we constrain the ratio of the semimajor axis and the st... | [['we', 'report', 'the', 'discovery', 'of', 'tres4', 'a', 'hot', 'jupiter', 'that', 'transits', 'the', 'star', 'gsc', '0262000648', 'every', '355', 'days', 'from', 'highresolution', 'spectroscopy', 'of', 'the', 'star', 'we', 'estimate', 'a', 'stellar', 'effective', 'temperature', 'of', 'teff', '6100', '150', 'k', 'and'... | [-0.08667514716224069, 0.11404370884731034, -0.11261106988580767, 0.019909381303491434, -0.12505083740573025, -0.08728812364583362, 0.12124049415654359, 0.35840917910583575, -0.1487146209049692, -0.3800261349635041, 0.08801137081542011, -0.31187887789116275, -0.04268426826717193, 0.19512208459773728, -0.097469865379215... |
708.0835 | Rest-Frame Ultraviolet to Near Infrared Observations of an Interacting
Lyman Break Galaxy at z = 4.42 | We present the rest-frame ultraviolet through near infrared spectral energy
distribution for an interacting Lyman break galaxy at a redshift z=4.42, the
highest redshift merging system known with clearly resolved tidal features. The
two objects in this system - HDF-G4 and its previously unidentified companion -
are b... | astro-ph | we present the restframe ultraviolet through near infrared spectral energy distribution for an interacting lyman break galaxy at a redshift z442 the highest redshift merging system known with clearly resolved tidal features the two objects in this system hdfg4 and its previously unidentified companion are both b_435 ba... | [['we', 'present', 'the', 'restframe', 'ultraviolet', 'through', 'near', 'infrared', 'spectral', 'energy', 'distribution', 'for', 'an', 'interacting', 'lyman', 'break', 'galaxy', 'at', 'a', 'redshift', 'z442', 'the', 'highest', 'redshift', 'merging', 'system', 'known', 'with', 'clearly', 'resolved', 'tidal', 'features'... | [-0.06015902187967309, 0.11489107135370562, -0.08254325428437552, 0.11386126611855697, -0.04089471364680391, -0.08223094032889992, 0.0006129208155880137, 0.43797368569486944, -0.12603558722977146, -0.39349142627338685, 0.048838859907566354, -0.29887238389553406, 0.00311416077300818, 0.16671046968060407, -0.003654296485... |
708.0836 | Can experiments distinguish between Radiative Electroweak Symmetry
breaking and Conventional breaking? | We present a comparative study of radiative electroweak symmetry breaking and
conventional standard model breaking, and pose the question whether experiments
can distinguish one breaking mode from the other. The importance of the problem
lies in the fact that the two breaking modes have very different physical
interp... | hep-ph | we present a comparative study of radiative electroweak symmetry breaking and conventional standard model breaking and pose the question whether experiments can distinguish one breaking mode from the other the importance of the problem lies in the fact that the two breaking modes have very different physical interpreta... | [['we', 'present', 'a', 'comparative', 'study', 'of', 'radiative', 'electroweak', 'symmetry', 'breaking', 'and', 'conventional', 'standard', 'model', 'breaking', 'and', 'pose', 'the', 'question', 'whether', 'experiments', 'can', 'distinguish', 'one', 'breaking', 'mode', 'from', 'the', 'other', 'the', 'importance', 'of'... | [-0.14683830177747323, 0.1858844275845856, -0.05256204227687883, 0.11847119824102026, -0.10983695447841874, -0.13094111993817276, 0.041535453821272876, 0.31915900086770294, -0.2966808134109759, -0.3131362194286995, 0.11560710988839569, -0.2488503791697201, -0.11681445938397626, 0.0823168524533327, 0.04932451730624574, ... |
708.0837 | Atomic Collapse and Quasi-Rydberg States in Graphene | Charge impurities in graphene can host an infinite family of Rydberg-like
resonance states of massless Dirac particles. These states, appearing for
supercritical charge, are described by Bohr-Sommerfeld quantization of
collapsing classical trajectories that descend on point charge, in analogy to
Rydberg states relati... | cond-mat.mes-hall | charge impurities in graphene can host an infinite family of rydberglike resonance states of massless dirac particles these states appearing for supercritical charge are described by bohrsommerfeld quantization of collapsing classical trajectories that descend on point charge in analogy to rydberg states relation with ... | [['charge', 'impurities', 'in', 'graphene', 'can', 'host', 'an', 'infinite', 'family', 'of', 'rydberglike', 'resonance', 'states', 'of', 'massless', 'dirac', 'particles', 'these', 'states', 'appearing', 'for', 'supercritical', 'charge', 'are', 'described', 'by', 'bohrsommerfeld', 'quantization', 'of', 'collapsing', 'cl... | [-0.1876248787973345, 0.24518167795691417, -0.03527277886637093, 0.06439702802328105, -0.002032551261567578, -0.15454576194728004, 0.07162717667998765, 0.3128486527634074, -0.24161004132024713, -0.2674815562774533, -0.07579366556613601, -0.34309391670658723, -0.13337672892573876, 0.11651917437533128, -0.003492245589834... |
708.0838 | A separable non-remainder of H | We prove that there is a compact separable continuum that (consistently) is
not a remainder of the real line.
| math.GN math.LO | we prove that there is a compact separable continuum that consistently is not a remainder of the real line | [['we', 'prove', 'that', 'there', 'is', 'a', 'compact', 'separable', 'continuum', 'that', 'consistently', 'is', 'not', 'a', 'remainder', 'of', 'the', 'real', 'line']] | [-0.13394056613508024, 0.07862610943419368, -0.14999824644703613, 0.11987167514713579, -0.08935759941998281, -0.11111656787168038, 0.02291550879415713, 0.4916957389367254, -0.18146179175298466, -0.07766421109830078, 0.1454249914294403, -0.23149817133028255, -0.17722115440196112, 0.21910468665392777, -0.0589276928650705... |
708.0839 | Quantum graphs where back-scattering is prohibited | We describe a new class of scattering matrices for quantum graphs in which
back-scattering is prohibited. We discuss some properties of quantum graphs
with these scattering matrices and explain the advantages and interest in their
study. We also provide two methods to build the vertex scattering matrices
needed for t... | math-ph math.MP | we describe a new class of scattering matrices for quantum graphs in which backscattering is prohibited we discuss some properties of quantum graphs with these scattering matrices and explain the advantages and interest in their study we also provide two methods to build the vertex scattering matrices needed for their ... | [['we', 'describe', 'a', 'new', 'class', 'of', 'scattering', 'matrices', 'for', 'quantum', 'graphs', 'in', 'which', 'backscattering', 'is', 'prohibited', 'we', 'discuss', 'some', 'properties', 'of', 'quantum', 'graphs', 'with', 'these', 'scattering', 'matrices', 'and', 'explain', 'the', 'advantages', 'and', 'interest',... | [-0.10016803823265374, 0.1459644392461461, -0.036972403772832715, 0.1120798253915364, -0.07187108067320842, -0.11948007254806511, 0.027705139398355696, 0.4244852009886766, -0.27772305956950377, -0.245827542572264, 0.10401962140538529, -0.2911432286651403, -0.216897148419829, 0.1858962711092888, -0.04929583970749495, 0.... |
708.084 | Multiple complex networks emerging from individual interactions | Systems composed of distinct complex networks are present in many real-world
environments, from society to ecological systems. In the present paper, we
propose a network model obtained as a consequence of interactions between two
species (e.g. predator and prey). Fields are produced and sensed by the
individuals, def... | physics.bio-ph physics.comp-ph | systems composed of distinct complex networks are present in many realworld environments from society to ecological systems in the present paper we propose a network model obtained as a consequence of interactions between two species eg predator and prey fields are produced and sensed by the individuals defining spatio... | [['systems', 'composed', 'of', 'distinct', 'complex', 'networks', 'are', 'present', 'in', 'many', 'realworld', 'environments', 'from', 'society', 'to', 'ecological', 'systems', 'in', 'the', 'present', 'paper', 'we', 'propose', 'a', 'network', 'model', 'obtained', 'as', 'a', 'consequence', 'of', 'interactions', 'between... | [-0.1667926769269995, 0.1553037847527309, -0.025601134724513426, 0.05635358238711007, 0.008613451629157656, -0.15418816768630808, 0.05881757334135867, 0.35945757301080794, -0.2787119716543842, -0.30165467110694083, 0.053152978909941064, -0.29294655586361257, -0.19859242969113722, 0.10100379810673456, -0.044213327321731... |
708.0841 | Triangularization of a Jordan Algebra of Schatten Operators | We show that a Jordan algebra of compact quasinilpotent operators which
contains a nonzero trace class operator has a common invariant subspace. As a
consequence of this result, we obtain that a Jordan algebra of quasinilpotent
Schatten operators is simultaneously triangularizable.
| math.OA | we show that a jordan algebra of compact quasinilpotent operators which contains a nonzero trace class operator has a common invariant subspace as a consequence of this result we obtain that a jordan algebra of quasinilpotent schatten operators is simultaneously triangularizable | [['we', 'show', 'that', 'a', 'jordan', 'algebra', 'of', 'compact', 'quasinilpotent', 'operators', 'which', 'contains', 'a', 'nonzero', 'trace', 'class', 'operator', 'has', 'a', 'common', 'invariant', 'subspace', 'as', 'a', 'consequence', 'of', 'this', 'result', 'we', 'obtain', 'that', 'a', 'jordan', 'algebra', 'of', 'q... | [-0.19681823249088554, 0.08886259444847294, -0.07527297389943426, 0.05511153221312093, -0.1263488347687554, -0.16221986899561272, -0.04095628625917726, 0.3280526884808773, -0.3290719210011203, -0.10156829955010879, 0.1332071369411651, -0.26383694851907286, -0.18335213101037393, 0.13963844686201432, -0.14637878457674894... |
708.0842 | The Crepant Resolution Conjecture for 3-dimensional flags modulo an
involution | After fixing a non-degenerate bilinear form on a vector space V we define an
involution of the manifold of flags F in V by taking a flag to its orthogonal
complement. When V is of dimension 3 we check that the Crepant Resolution
Conjecture of J. Bryan and T. Graber holds: the genus zero (orbifold)
Gromov-Witten poten... | math.AG | after fixing a nondegenerate bilinear form on a vector space v we define an involution of the manifold of flags f in v by taking a flag to its orthogonal complement when v is of dimension 3 we check that the crepant resolution conjecture of j bryan and t graber holds the genus zero orbifold gromovwitten potential funct... | [['after', 'fixing', 'a', 'nondegenerate', 'bilinear', 'form', 'on', 'a', 'vector', 'space', 'v', 'we', 'define', 'an', 'involution', 'of', 'the', 'manifold', 'of', 'flags', 'f', 'in', 'v', 'by', 'taking', 'a', 'flag', 'to', 'its', 'orthogonal', 'complement', 'when', 'v', 'is', 'of', 'dimension', '3', 'we', 'check', 't... | [-0.24904554789405195, 0.027985000319242847, -0.088987123040903, 0.03472947759831685, -0.07224039397683114, -0.22628728274421225, 0.03776084980739641, 0.32621713639086775, -0.3103749140526258, -0.18096319171074296, 0.05137187963344097, -0.23306294546496392, -0.11389755538754887, 0.13960384147151583, -0.1401734397701558... |
708.0843 | Landau levels and oscillator strength in a biased bilayer of graphene | We obtain analytical expressions for the eigenstates and the Landau level
spectrum of biased graphene bilayers in a magnetic field. The calculations are
performed in the context of a four-band continuum model and generalize previous
approximate results. Solutions are presented for the spectrum as a function of
interl... | cond-mat.mes-hall | we obtain analytical expressions for the eigenstates and the landau level spectrum of biased graphene bilayers in a magnetic field the calculations are performed in the context of a fourband continuum model and generalize previous approximate results solutions are presented for the spectrum as a function of interlayer ... | [['we', 'obtain', 'analytical', 'expressions', 'for', 'the', 'eigenstates', 'and', 'the', 'landau', 'level', 'spectrum', 'of', 'biased', 'graphene', 'bilayers', 'in', 'a', 'magnetic', 'field', 'the', 'calculations', 'are', 'performed', 'in', 'the', 'context', 'of', 'a', 'fourband', 'continuum', 'model', 'and', 'general... | [-0.14915722940007553, 0.12202742810069478, -0.04960906056815064, 0.10372919332710843, -0.029329604140537625, -0.10119388931357831, 0.07915040277693347, 0.3983527276591927, -0.19840375534897925, -0.3380311208722346, -0.007208266688109029, -0.2656479130782114, -0.11410422091755797, 0.1722867208414291, 0.0707925982298512... |
708.0844 | Emergence of Small-Scale Magnetic Loops in the Quiet Sun Internetwork | We study the emergence of magnetic flux at very small spatial scales (less
than 2 arcsec) in the quiet Sun internetwork. To this aim, a time series of
spectropolarimetric maps was taken at disk center using the instrument SP/SOT
on board Hinode. The LTE inversion of the full Stokes vector measured in the Fe
I 6301 an... | astro-ph | we study the emergence of magnetic flux at very small spatial scales less than 2 arcsec in the quiet sun internetwork to this aim a time series of spectropolarimetric maps was taken at disk center using the instrument spsot on board hinode the lte inversion of the full stokes vector measured in the fe i 6301 and 6302 a... | [['we', 'study', 'the', 'emergence', 'of', 'magnetic', 'flux', 'at', 'very', 'small', 'spatial', 'scales', 'less', 'than', '2', 'arcsec', 'in', 'the', 'quiet', 'sun', 'internetwork', 'to', 'this', 'aim', 'a', 'time', 'series', 'of', 'spectropolarimetric', 'maps', 'was', 'taken', 'at', 'disk', 'center', 'using', 'the', ... | [-0.15179513034987638, 0.1540919826644014, -0.017116334321999875, 0.0729164170412305, -0.05233680727933325, -0.0408152890975462, 0.031243100908320786, 0.41997818723876973, -0.2272694452366889, -0.347167192860993, 0.07467658822285707, -0.23253243546526786, -0.03681766983024331, 0.15406639654356152, -0.00988238828001579,... |
708.0845 | The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- V. Submillimetre
properties of near-infrared--selected galaxies in the Subaru/XMM--Newton deep
field | We have studied the submillimetre (submm) properties of the following classes
of near-infrared (NIR)-selected massive galaxies at high redshifts:
BzK-selected star-forming galaxies (BzKs); distant red galaxies (DRGs); and
extremely red objects (EROs). We used the SCUBA HAlf Degree Extragalactic
Survey (SHADES), the l... | astro-ph | we have studied the submillimetre submm properties of the following classes of nearinfrared nirselected massive galaxies at high redshifts bzkselected starforming galaxies bzks distant red galaxies drgs and extremely red objects eros we used the scuba half degree extragalactic survey shades the largest uniform submm su... | [['we', 'have', 'studied', 'the', 'submillimetre', 'submm', 'properties', 'of', 'the', 'following', 'classes', 'of', 'nearinfrared', 'nirselected', 'massive', 'galaxies', 'at', 'high', 'redshifts', 'bzkselected', 'starforming', 'galaxies', 'bzks', 'distant', 'red', 'galaxies', 'drgs', 'and', 'extremely', 'red', 'object... | [-0.03128874301018166, 0.07704950287564442, -0.07718715354218997, 0.15753444655030205, -0.10372353192116304, -0.07357168465217127, 0.06369298116183317, 0.4933855339313728, -0.021917655624608155, -0.3554938615250476, 0.057462772944207936, -0.3365046502308526, -0.030440728336039006, 0.16434674383444406, -0.03872835840779... |
708.0846 | Cooperative game theory and the Gaussian interference channel | In this paper we discuss the use of cooperative game theory for analyzing
interference channels. We extend our previous work, to games with N players as
well as frequency selective channels and joint TDM/FDM strategies.
We show that the Nash bargaining solution can be computed using convex
optimization techniques. ... | cs.IT cs.GT math.IT | in this paper we discuss the use of cooperative game theory for analyzing interference channels we extend our previous work to games with n players as well as frequency selective channels and joint tdmfdm strategies we show that the nash bargaining solution can be computed using convex optimization techniques we also s... | [['in', 'this', 'paper', 'we', 'discuss', 'the', 'use', 'of', 'cooperative', 'game', 'theory', 'for', 'analyzing', 'interference', 'channels', 'we', 'extend', 'our', 'previous', 'work', 'to', 'games', 'with', 'n', 'players', 'as', 'well', 'as', 'frequency', 'selective', 'channels', 'and', 'joint', 'tdmfdm', 'strategies... | [-0.15032408534066885, 0.0268703501176008, -0.07923529478388705, 0.041753818929594545, -0.03822313080724728, -0.23177330452017486, 0.14020213779960095, 0.4508396309434569, -0.2772265937445419, -0.26479293580632657, 0.08528099273826228, -0.2497434551499152, -0.18840550339414872, 0.13023634738887527, -0.08039710894393336... |
708.0847 | Direct Observational Test Rules Out Small MgII Absorbers | Recent observations suggest the incidence of strong intervening MgII
absorption systems along the line-of-sight to gamma ray burst (GRB) afterglows
is significantly higher than expected from analogous quasar sightlines. One
possible explanation is a geometric effect, arising because MgII absorbers only
partially cove... | astro-ph | recent observations suggest the incidence of strong intervening mgii absorption systems along the lineofsight to gamma ray burst grb afterglows is significantly higher than expected from analogous quasar sightlines one possible explanation is a geometric effect arising because mgii absorbers only partially cover the qu... | [['recent', 'observations', 'suggest', 'the', 'incidence', 'of', 'strong', 'intervening', 'mgii', 'absorption', 'systems', 'along', 'the', 'lineofsight', 'to', 'gamma', 'ray', 'burst', 'grb', 'afterglows', 'is', 'significantly', 'higher', 'than', 'expected', 'from', 'analogous', 'quasar', 'sightlines', 'one', 'possible... | [-0.07913043682190884, 0.09081654717418843, 0.004439921896314112, 0.1550785345948165, -0.11231942153990088, -0.15682101861585113, 0.04367289337948555, 0.5021554394511552, -0.14344680140777377, -0.29465331259842326, 0.021937381670662632, -0.34250485188350444, -0.029302466887889837, 0.16687241165966885, -0.01736481515396... |
708.0848 | Validation of spallation neutron production and propagation within
Geant4 | Using simulations to understand backgrounds from muon-induced neutrons is
important in designing next-generation low-background underground experiments.
Validation of relevant physics within the Geant4 simulation package has been
completed by comparing to data from two recent experiments. Verification
focused on the ... | nucl-ex | using simulations to understand backgrounds from muoninduced neutrons is important in designing nextgeneration lowbackground underground experiments validation of relevant physics within the geant4 simulation package has been completed by comparing to data from two recent experiments verification focused on the product... | [['using', 'simulations', 'to', 'understand', 'backgrounds', 'from', 'muoninduced', 'neutrons', 'is', 'important', 'in', 'designing', 'nextgeneration', 'lowbackground', 'underground', 'experiments', 'validation', 'of', 'relevant', 'physics', 'within', 'the', 'geant4', 'simulation', 'package', 'has', 'been', 'completed'... | [0.007185243107789361, 0.12179181035881971, -0.06387250560938436, 0.1455273790343199, -0.018908069688169396, -0.10716918361482813, -0.006885654556647162, 0.393912598490715, -0.15591948900563532, -0.4173082610975732, 0.08484177853439606, -0.38699739335981365, -0.020576392053900397, 0.31541919349418845, 0.060925049375167... |
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