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708.2649 | Quantization of neutron in Earth's gravity | Gravity is the weakest of all four known forces in the universe. Quantum
states of an elementary particle due to such a weak field is certainly very
shallow and would therefore be an experimental challenge to detect. Recently an
experimental attempt was made by V. V. Nesvizhevsky et al., Nature 415, 297
(2002), to me... | hep-th quant-ph | gravity is the weakest of all four known forces in the universe quantum states of an elementary particle due to such a weak field is certainly very shallow and would therefore be an experimental challenge to detect recently an experimental attempt was made by v v nesvizhevsky et al nature 415 297 2002 to measure the qu... | [['gravity', 'is', 'the', 'weakest', 'of', 'all', 'four', 'known', 'forces', 'in', 'the', 'universe', 'quantum', 'states', 'of', 'an', 'elementary', 'particle', 'due', 'to', 'such', 'a', 'weak', 'field', 'is', 'certainly', 'very', 'shallow', 'and', 'would', 'therefore', 'be', 'an', 'experimental', 'challenge', 'to', 'd... | [-0.09445263399998137, 0.19986715143006334, -0.060794768548003454, 0.08760985857013655, -0.05883382452006696, -0.09529805898551917, 0.049777679824317134, 0.3238756916792699, -0.22197083102060514, -0.36749640548102264, 0.0514305580268203, -0.280755796922402, -0.06734557089287861, 0.20358557113271997, -0.0347297009127474... |
708.265 | Optimal L^p-Riemannian Gagliardo-Nirenberg inequalities | Let (M,g) be a compact Riemannian manifold of dimension n \geq 2. In this
work we prove the validity of the optimal L^p-Riemannian Gagliardo-Nirenberg
inequality for 1 < p \leq 2. Our proof relies strongly on a new distance lemma
which. In particular, we extend L^p-Euclidean Gagliardo-Nirenberg inequalities
due to De... | math.DG math.AP | let mg be a compact riemannian manifold of dimension n geq 2 in this work we prove the validity of the optimal lpriemannian gagliardonirenberg inequality for 1 p leq 2 our proof relies strongly on a new distance lemma which in particular we extend lpeuclidean gagliardonirenberg inequalities due to del pino and dolbeaul... | [['let', 'mg', 'be', 'a', 'compact', 'riemannian', 'manifold', 'of', 'dimension', 'n', 'geq', '2', 'in', 'this', 'work', 'we', 'prove', 'the', 'validity', 'of', 'the', 'optimal', 'lpriemannian', 'gagliardonirenberg', 'inequality', 'for', '1', 'p', 'leq', '2', 'our', 'proof', 'relies', 'strongly', 'on', 'a', 'new', 'dis... | [-0.11172920527995654, 0.016605955638712453, -0.08682959336006353, 0.0968304188948335, -0.0802837363369162, -0.24816064846762007, 0.03410689905285835, 0.26293315679856366, -0.26183027608109816, -0.2906252931382868, 0.09747863059390276, -0.25114334541027467, -0.13128487784190163, 0.2211390741905498, -0.16575617978589668... |
708.2651 | Notes on the Jacobi equation | We discuss some properties of Jacobi fields that do not involve assumptions
on the curvature endomorphism. We compare indices of different spaces of Jacobi
fields and give some applications to Riemannian geometry.
| math.DG | we discuss some properties of jacobi fields that do not involve assumptions on the curvature endomorphism we compare indices of different spaces of jacobi fields and give some applications to riemannian geometry | [['we', 'discuss', 'some', 'properties', 'of', 'jacobi', 'fields', 'that', 'do', 'not', 'involve', 'assumptions', 'on', 'the', 'curvature', 'endomorphism', 'we', 'compare', 'indices', 'of', 'different', 'spaces', 'of', 'jacobi', 'fields', 'and', 'give', 'some', 'applications', 'to', 'riemannian', 'geometry']] | [-0.19649627816397697, 0.08154846483375877, -0.09735149738844484, 0.15921878002700396, -0.17945564194815233, -0.1080157546675764, -0.08255349670071155, 0.464994675014168, -0.2672551376745105, -0.22985398455057293, 0.15130984320421703, -0.23861399359884672, -0.20008097920799628, 0.24620063668589864, -0.15928688715212047... |
708.2652 | Decoherence in a superconducting flux qubit with a pi-junction | We consider the use of a pi-junction for flux qubits to realize degenerate
quantum levels without external magnetic field. On the basis of the
Caldeira-Leggett model, we derive an effective spin-Boson model, and study
decoherece of this type of qubits. We estimate the dephasing time by using
parameters from recent ex... | cond-mat.mes-hall cond-mat.supr-con | we consider the use of a pijunction for flux qubits to realize degenerate quantum levels without external magnetic field on the basis of the caldeiraleggett model we derive an effective spinboson model and study decoherece of this type of qubits we estimate the dephasing time by using parameters from recent experiments... | [['we', 'consider', 'the', 'use', 'of', 'a', 'pijunction', 'for', 'flux', 'qubits', 'to', 'realize', 'degenerate', 'quantum', 'levels', 'without', 'external', 'magnetic', 'field', 'on', 'the', 'basis', 'of', 'the', 'caldeiraleggett', 'model', 'we', 'derive', 'an', 'effective', 'spinboson', 'model', 'and', 'study', 'dec... | [-0.18002266957852486, 0.1673894114747118, 0.014293172145010653, 0.051028290227042965, -0.002680548315716756, -0.18550305933112632, 0.0957166475615137, 0.36753596813493483, -0.2111250526425932, -0.3157935175994361, 0.02929202886770253, -0.21907939093590184, -0.11352322792171853, 0.23922022779132365, -0.0092716014855918... |
708.2653 | Unusual Resonators: Plasmonics, Metamaterials, and Random Media | Superresolution, extraordinary transmission, total absorption, and
localization of electromagnetic waves are currently attracting growing
attention. These phenomena are related to different physical objects and are
usually studied within the context of different, sometimes rather
sophisticated, physical approaches. R... | physics.optics cond-mat.other physics.plasm-ph | superresolution extraordinary transmission total absorption and localization of electromagnetic waves are currently attracting growing attention these phenomena are related to different physical objects and are usually studied within the context of different sometimes rather sophisticated physical approaches remarkably... | [['superresolution', 'extraordinary', 'transmission', 'total', 'absorption', 'and', 'localization', 'of', 'electromagnetic', 'waves', 'are', 'currently', 'attracting', 'growing', 'attention', 'these', 'phenomena', 'are', 'related', 'to', 'different', 'physical', 'objects', 'and', 'are', 'usually', 'studied', 'within', ... | [-0.16180031439128878, 0.13093258395245608, -0.05505913406096656, 0.062036363429044665, -0.1288262607152413, -0.1493026581070996, 0.010405395372674382, 0.40005398862182306, -0.27434370752698983, -0.30650552310820284, 0.0532241316486134, -0.27504718763320224, -0.20988206147890667, 0.22241653880738685, -0.015632484153370... |
708.2654 | $^{77}$Se NMR evidence for the Jaccarino-Peter mechanism in the field
induced superconductor, $\lambda$(BETS)$_2$FeCl$_4$} | We have performed $^{77}$Se NMR on a single crystal sample of the field
induced superconductor $\lambda$-(BETS)$_{2}$FeCl$_{4}$. Our results obtained
in the paramagnetic state provide a microscopic insight on the exchange
interaction $J$ between the spins \textbf{s} of the BETS $\pi$ conduction
electrons and the Fe l... | cond-mat.str-el cond-mat.supr-con | we have performed 77se nmr on a single crystal sample of the field induced superconductor lambdabets_2fecl_4 our results obtained in the paramagnetic state provide a microscopic insight on the exchange interaction j between the spins textbfs of the bets pi conduction electrons and the fe localized d spins textbfs the a... | [['we', 'have', 'performed', '77se', 'nmr', 'on', 'a', 'single', 'crystal', 'sample', 'of', 'the', 'field', 'induced', 'superconductor', 'lambdabets_2fecl_4', 'our', 'results', 'obtained', 'in', 'the', 'paramagnetic', 'state', 'provide', 'a', 'microscopic', 'insight', 'on', 'the', 'exchange', 'interaction', 'j', 'betwe... | [-0.1433899471790768, 0.19722325384265238, -0.02199353275788125, -0.056415972669424795, -0.05164925968491061, -0.10419594424744245, 0.11572389401560433, 0.3473479505520054, -0.18971922178685038, -0.3292482770048082, -0.07440091559844807, -0.3430416539668777, -0.06253414363383727, 0.16172135910993918, 0.0306761173726341... |
708.2655 | CEDAR: tools for event generator tuning | I describe the work of the CEDAR collaboration in developing tools for tuning
and validating Monte Carlo event generator programs. The core CEDAR task is to
interface the Durham HepData database of experimental measurements to event
generator validation tools such as the UCL JetWeb system - this has
necessitated the ... | hep-ph | i describe the work of the cedar collaboration in developing tools for tuning and validating monte carlo event generator programs the core cedar task is to interface the durham hepdata database of experimental measurements to event generator validation tools such as the ucl jetweb system this has necessitated the migra... | [['i', 'describe', 'the', 'work', 'of', 'the', 'cedar', 'collaboration', 'in', 'developing', 'tools', 'for', 'tuning', 'and', 'validating', 'monte', 'carlo', 'event', 'generator', 'programs', 'the', 'core', 'cedar', 'task', 'is', 'to', 'interface', 'the', 'durham', 'hepdata', 'database', 'of', 'experimental', 'measurem... | [-0.08373962647241096, 0.024281139635359463, -0.07995651688669687, 0.06378141492807671, -0.09745036767714697, -0.15980976651139234, 0.00819561020673617, 0.34080775368796745, -0.24688594924771914, -0.3611052612895551, 0.13524141569075215, -0.2994635230335205, -0.07342041779471481, 0.2196899959878267, -0.0234631202446863... |
708.2656 | Hawking radiation from rotating brane black holes | We review recent work on the Hawking radiation of rotating brane black holes,
as may be produced at the LHC. We outline the methodology for calculating the
fluxes of particles, energy and angular momentum by spin-0, spin-1/2 and spin-1
quantum fields on the brane. We briefly review some of the key features of the
emi... | hep-th gr-qc hep-ph | we review recent work on the hawking radiation of rotating brane black holes as may be produced at the lhc we outline the methodology for calculating the fluxes of particles energy and angular momentum by spin0 spin12 and spin1 quantum fields on the brane we briefly review some of the key features of the emission in pa... | [['we', 'review', 'recent', 'work', 'on', 'the', 'hawking', 'radiation', 'of', 'rotating', 'brane', 'black', 'holes', 'as', 'may', 'be', 'produced', 'at', 'the', 'lhc', 'we', 'outline', 'the', 'methodology', 'for', 'calculating', 'the', 'fluxes', 'of', 'particles', 'energy', 'and', 'angular', 'momentum', 'by', 'spin0',... | [-0.11013865526563124, 0.20105284240360008, -0.041540204997822315, 0.1358987062400126, -0.05403323705389124, -0.1011726769325121, -0.0295525395498692, 0.31279260442470724, -0.1562276451251186, -0.3086576984015941, 0.06762695947722734, -0.3481502194443475, -0.030614631812331147, 0.21688997200639595, -0.00260404162311359... |
708.2657 | Mediated Homogenization | Homogenization protocols model the quantum mechanical evolution of a system
to a fixed state independently from its initial configuration by repeatedly
coupling it with a collection of identical ancillas. Here we analyze these
protocols within the formalism of "relaxing" channels providing an easy to
check sufficient... | quant-ph | homogenization protocols model the quantum mechanical evolution of a system to a fixed state independently from its initial configuration by repeatedly coupling it with a collection of identical ancillas here we analyze these protocols within the formalism of relaxing channels providing an easy to check sufficient cond... | [['homogenization', 'protocols', 'model', 'the', 'quantum', 'mechanical', 'evolution', 'of', 'a', 'system', 'to', 'a', 'fixed', 'state', 'independently', 'from', 'its', 'initial', 'configuration', 'by', 'repeatedly', 'coupling', 'it', 'with', 'a', 'collection', 'of', 'identical', 'ancillas', 'here', 'we', 'analyze', 't... | [-0.1599177034328813, 0.16353542141365798, -0.09203560317906996, 0.01246398484395088, 0.0005203054812939271, -0.21260807555594036, 0.09908619557466844, 0.3725817179671772, -0.26839838894084095, -0.2641976401290816, 0.08254664959487222, -0.2431494963719793, -0.09037146414832577, 0.12601911942879468, -0.02472749036615309... |
708.2658 | On positive opetopes, positive opetopic cardinals and positive opetopic
set | We introduce the notion of a positive opetope and positive opetopic cardinals
as certain finite combinatorial structures. The positive opetopic cardinals to
positive-to-one polygraphs are like simple graphs to free omega-categories over
omega-graphs, c.f. [MZ]. In particular, they allow us to give an explicit
combina... | math.GT | we introduce the notion of a positive opetope and positive opetopic cardinals as certain finite combinatorial structures the positive opetopic cardinals to positivetoone polygraphs are like simple graphs to free omegacategories over omegagraphs cf mz in particular they allow us to give an explicit combinatorial descrip... | [['we', 'introduce', 'the', 'notion', 'of', 'a', 'positive', 'opetope', 'and', 'positive', 'opetopic', 'cardinals', 'as', 'certain', 'finite', 'combinatorial', 'structures', 'the', 'positive', 'opetopic', 'cardinals', 'to', 'positivetoone', 'polygraphs', 'are', 'like', 'simple', 'graphs', 'to', 'free', 'omegacategories... | [-0.13528540566524802, 0.05486562365240388, -0.07657256793542426, 0.13486547073504576, -0.1783160813823391, -0.15012260543880984, -0.013887096977365824, 0.36320655948172015, -0.38389723118355806, -0.18560608426923864, 0.02915099400828088, -0.2564202407090003, -0.11335595898951094, 0.16646339219490378, -0.20591589513545... |
708.2659 | On ordered face structures and many-to-one computads | We introduce the notion of an ordered face structure. The ordered face
structures to many-to-one computads are like positive face structures to
positive-to-one computads. This allow us to give an explicit combinatorial
description of many-to-one computads in terms of ordered face structures.
| math.CT | we introduce the notion of an ordered face structure the ordered face structures to manytoone computads are like positive face structures to positivetoone computads this allow us to give an explicit combinatorial description of manytoone computads in terms of ordered face structures | [['we', 'introduce', 'the', 'notion', 'of', 'an', 'ordered', 'face', 'structure', 'the', 'ordered', 'face', 'structures', 'to', 'manytoone', 'computads', 'are', 'like', 'positive', 'face', 'structures', 'to', 'positivetoone', 'computads', 'this', 'allow', 'us', 'to', 'give', 'an', 'explicit', 'combinatorial', 'descript... | [-0.14393672679683991, 0.046358183786478116, -0.057300797663629055, 0.0922422501607798, -0.15692854805716447, -0.09882659930735826, -0.020830276034151513, 0.437909443463598, -0.3654428259802184, -0.22975015853132522, 0.04127284002745347, -0.2344467072814171, -0.21114089406494582, 0.08160969020710104, -0.163102929347327... |
708.266 | Tsallis distribution from minimally selected order statistics | We demonstrate that selection of the minimal value of ordered variables leads
in a natural way to its distribution being given by the Tsallis distribution,
the same as that resulting from Tsallis nonextensive statistics. The possible
application of this result to the multiparticle production processes is
indicated.
| cond-mat.stat-mech hep-ph | we demonstrate that selection of the minimal value of ordered variables leads in a natural way to its distribution being given by the tsallis distribution the same as that resulting from tsallis nonextensive statistics the possible application of this result to the multiparticle production processes is indicated | [['we', 'demonstrate', 'that', 'selection', 'of', 'the', 'minimal', 'value', 'of', 'ordered', 'variables', 'leads', 'in', 'a', 'natural', 'way', 'to', 'its', 'distribution', 'being', 'given', 'by', 'the', 'tsallis', 'distribution', 'the', 'same', 'as', 'that', 'resulting', 'from', 'tsallis', 'nonextensive', 'statistics... | [-0.04801723483375254, 0.16567451657449944, -0.17524458083542102, 0.09222220070660114, -0.037881173748285216, -0.04580899610857856, 0.049064832533947486, 0.2824985463905366, -0.29998588625420913, -0.28729588138137724, 0.007605901401628681, -0.2848296862174856, -0.10147193755875243, 0.1660029942843508, -0.08893615724717... |
708.2661 | Improved photometry of SDSS crowded field images: Structure and dark
matter content in the dwarf spheroidal galaxy Leo I | We explore how well crowded field point-source photometry can be accomplished
with SDSS data: We present a photometric pipeline based on DoPhot, and tuned
for analyzing crowded-field images from the SDSS. Using Monte Carlo simulations
we show that the completeness of source extraction is above 80% to i < 21 (AB)
and ... | astro-ph | we explore how well crowded field pointsource photometry can be accomplished with sdss data we present a photometric pipeline based on dophot and tuned for analyzing crowdedfield images from the sdss using monte carlo simulations we show that the completeness of source extraction is above 80 to i 21 ab and a stellar su... | [['we', 'explore', 'how', 'well', 'crowded', 'field', 'pointsource', 'photometry', 'can', 'be', 'accomplished', 'with', 'sdss', 'data', 'we', 'present', 'a', 'photometric', 'pipeline', 'based', 'on', 'dophot', 'and', 'tuned', 'for', 'analyzing', 'crowdedfield', 'images', 'from', 'the', 'sdss', 'using', 'monte', 'carlo'... | [-0.037771936819265536, 0.039871140987140785, -0.11835252935830638, 0.10084932335952243, -0.10635541158178888, -0.08170210950893896, 0.06308482571550236, 0.39004527554317986, -0.17039605942178934, -0.34895407013333796, 0.04276007935262399, -0.28113980786606885, -0.044870004143311285, 0.2070037430370471, -0.061561976452... |
708.2662 | Direct generation of charge carriers in c-Si solar cells due to embedded
nanoparticles | It is known that silicon is an indirect band gap material, reducing its
efficiency in photovoltaic applications. Using surface plasmons in metallic
nanoparticles embedded in a solar cell has recently been proposed as a way to
increase the efficiency of thin film silicon solar cells. The dipole mode that
dominates the... | cond-mat.other | it is known that silicon is an indirect band gap material reducing its efficiency in photovoltaic applications using surface plasmons in metallic nanoparticles embedded in a solar cell has recently been proposed as a way to increase the efficiency of thin film silicon solar cells the dipole mode that dominates the plas... | [['it', 'is', 'known', 'that', 'silicon', 'is', 'an', 'indirect', 'band', 'gap', 'material', 'reducing', 'its', 'efficiency', 'in', 'photovoltaic', 'applications', 'using', 'surface', 'plasmons', 'in', 'metallic', 'nanoparticles', 'embedded', 'in', 'a', 'solar', 'cell', 'has', 'recently', 'been', 'proposed', 'as', 'a',... | [-0.11225561771695454, 0.1756184505164916, -0.006394355106599552, -0.014758758813373208, -0.047347831426994856, -0.061473142557307, 0.031729557181794925, 0.42138647234316956, -0.2313338518574757, -0.32543390240405023, 0.01759116559351804, -0.30600213666552123, -0.15144172555661387, 0.24260155683906615, -0.0706867998437... |
708.2663 | Hexagonal parquet tilings: k-isohedral monotiles with arbitrarily large
k | This paper addresses the question of whether a single tile with nearest
neighbor matching rules can force a tiling in which the tiles fall into a large
number of isohedral classes. A single tile is exhibited that can fill the
Euclidean plane only with a tiling that contains k distinct isohedral sets of
tiles, where k... | cond-mat.other math.GM math.MG | this paper addresses the question of whether a single tile with nearest neighbor matching rules can force a tiling in which the tiles fall into a large number of isohedral classes a single tile is exhibited that can fill the euclidean plane only with a tiling that contains k distinct isohedral sets of tiles where k can... | [['this', 'paper', 'addresses', 'the', 'question', 'of', 'whether', 'a', 'single', 'tile', 'with', 'nearest', 'neighbor', 'matching', 'rules', 'can', 'force', 'a', 'tiling', 'in', 'which', 'the', 'tiles', 'fall', 'into', 'a', 'large', 'number', 'of', 'isohedral', 'classes', 'a', 'single', 'tile', 'is', 'exhibited', 'th... | [-0.11914321539070379, 0.16060605127538613, -0.05716923050504256, 0.013666200137312907, -0.11729997741644616, -0.17960227675527543, 0.09688987520481036, 0.37887542192023116, -0.2690831921226182, -0.33479020823692, 0.10655937712131576, -0.27662359318263274, -0.12183891466030708, 0.11677913018827932, -0.09658495911561486... |
708.2664 | Sutherland Models for Complex Reflection Groups | There are known to be integrable Sutherland models associated to every real
root system -- or, which is almost equivalent, to every real reflection group.
Real reflection groups are special cases of complex reflection groups. In this
paper we associate certain integrable Sutherland models to the classical family
of c... | math-ph hep-th math.MP | there are known to be integrable sutherland models associated to every real root system or which is almost equivalent to every real reflection group real reflection groups are special cases of complex reflection groups in this paper we associate certain integrable sutherland models to the classical family of complex re... | [['there', 'are', 'known', 'to', 'be', 'integrable', 'sutherland', 'models', 'associated', 'to', 'every', 'real', 'root', 'system', 'or', 'which', 'is', 'almost', 'equivalent', 'to', 'every', 'real', 'reflection', 'group', 'real', 'reflection', 'groups', 'are', 'special', 'cases', 'of', 'complex', 'reflection', 'groups... | [-0.1793822423097826, 0.1224058286431406, -0.02381039090486693, 0.07935811135243497, -0.12622190175521797, -0.1638178762323464, -0.01698153566043214, 0.3965018979626997, -0.3098692059846081, -0.23793247514022997, 0.14278512063901871, -0.2761633765486326, -0.1738837766320573, 0.18749888351082739, -0.06978651629520002, -... |
708.2665 | The LHCb Upgrade | The LHCb detector has been designed to study CP violation and other rare
phenomena in B-meson decays up to a luminosity of $\sim 5.10^{32}\rm
cm^{-2}s^{-1}$. This paper will describe what is limiting LHCb to exploit the
much higher luminosities available at the LHC, and what are the baseline
modifications which will ... | hep-ex | the lhcb detector has been designed to study cp violation and other rare phenomena in bmeson decays up to a luminosity of sim 51032rm cm2s1 this paper will describe what is limiting lhcb to exploit the much higher luminosities available at the lhc and what are the baseline modifications which will remedy these limitati... | [['the', 'lhcb', 'detector', 'has', 'been', 'designed', 'to', 'study', 'cp', 'violation', 'and', 'other', 'rare', 'phenomena', 'in', 'bmeson', 'decays', 'up', 'to', 'a', 'luminosity', 'of', 'sim', '51032rm', 'cm2s1', 'this', 'paper', 'will', 'describe', 'what', 'is', 'limiting', 'lhcb', 'to', 'exploit', 'the', 'much', ... | [-0.03367884430465185, 0.19922950807958842, -0.056835964679097135, 0.1320069474193992, -0.09454865886622833, -0.13598244728830952, 0.023375461734313933, 0.3339944171615773, -0.18226763541913696, -0.3264931993765963, 0.061649943727792963, -0.36726573426793846, 0.026882576179276738, 0.15182883695233612, -0.02982760523445... |
708.2666 | Hyperbolic cusps with convex polyhedral boundary | We prove that a 3-dimensional hyperbolic cusp with convex polyhedral boundary
is uniquely determined by the metric induced on its boundary. Furthemore, any
hyperbolic metric on the torus with cone singularities of positive curvature
can be realized as the induced metric on the boundary of a convex polyhedral
cusp. Th... | math.DG | we prove that a 3dimensional hyperbolic cusp with convex polyhedral boundary is uniquely determined by the metric induced on its boundary furthemore any hyperbolic metric on the torus with cone singularities of positive curvature can be realized as the induced metric on the boundary of a convex polyhedral cusp the proo... | [['we', 'prove', 'that', 'a', '3dimensional', 'hyperbolic', 'cusp', 'with', 'convex', 'polyhedral', 'boundary', 'is', 'uniquely', 'determined', 'by', 'the', 'metric', 'induced', 'on', 'its', 'boundary', 'furthemore', 'any', 'hyperbolic', 'metric', 'on', 'the', 'torus', 'with', 'cone', 'singularities', 'of', 'positive',... | [-0.18767696254901955, 0.10104579400446755, -0.11131675142916989, 0.049962442851106285, -0.13210880719735973, -0.10914074886803989, -0.028617591671569305, 0.3348874607444054, -0.2730617463344433, -0.18234773210992228, 0.12413541605738068, -0.31219304223605965, -0.1715732818072448, 0.17833404312078216, -0.15435724559652... |
708.2667 | Migration of bosonic particles across a Mott insulator to superfluid
phase interface | We consider a boundary between a Mott insulator and a superfluid region of a
Bose-Hubbard model at unit filling. Initially both regions are decoupled and
cooled to their respective ground states. We show that, after switching on a
small tunneling rate between both regions, all particles of the Mott region
migrate to ... | cond-mat.str-el cond-mat.stat-mech quant-ph | we consider a boundary between a mott insulator and a superfluid region of a bosehubbard model at unit filling initially both regions are decoupled and cooled to their respective ground states we show that after switching on a small tunneling rate between both regions all particles of the mott region migrate to the sup... | [['we', 'consider', 'a', 'boundary', 'between', 'a', 'mott', 'insulator', 'and', 'a', 'superfluid', 'region', 'of', 'a', 'bosehubbard', 'model', 'at', 'unit', 'filling', 'initially', 'both', 'regions', 'are', 'decoupled', 'and', 'cooled', 'to', 'their', 'respective', 'ground', 'states', 'we', 'show', 'that', 'after', '... | [-0.1664712119475007, 0.1524617555178702, -0.06470317801460623, 0.042589508138597014, 0.011623280432075262, -0.14147152080759406, 0.12843331510946154, 0.3948546937480569, -0.21440853611007332, -0.25731030143797395, 0.05965582850854844, -0.31653786085825414, -0.11903095282614232, 0.17718451790633843, 0.05540242285421118... |
708.2668 | Zone and double zone diagrams in abstract spaces | A zone diagram is a relatively new concept which was first defined and
studied by T. Asano, J. Matousek and T. Tokuyama. It can be interpreted as a
state of equilibrium between several mutually hostile kingdoms. Formally, it is
a fixed point of a certain mapping. These authors considered the Euclidean
plane and prove... | math.MG cs.CG math.CO | a zone diagram is a relatively new concept which was first defined and studied by t asano j matousek and t tokuyama it can be interpreted as a state of equilibrium between several mutually hostile kingdoms formally it is a fixed point of a certain mapping these authors considered the euclidean plane and proved the exis... | [['a', 'zone', 'diagram', 'is', 'a', 'relatively', 'new', 'concept', 'which', 'was', 'first', 'defined', 'and', 'studied', 'by', 't', 'asano', 'j', 'matousek', 'and', 't', 'tokuyama', 'it', 'can', 'be', 'interpreted', 'as', 'a', 'state', 'of', 'equilibrium', 'between', 'several', 'mutually', 'hostile', 'kingdoms', 'for... | [-0.14870184891098628, 0.08766392609339223, -0.08886446282868424, 0.10715085893734208, -0.07411556197180143, -0.12012935461356275, 0.09234079306629757, 0.35106073070557847, -0.25470395903328374, -0.26989814564585685, 0.11640497975111488, -0.22639298415292175, -0.21131976064174407, 0.19526727528822038, -0.11198116487432... |
708.2669 | Schubert calculus on the grassmannian of hermitian lagrangian spaces | The grassmannian of hermitian lagrangian spaces in $\mathbb{C}^n\oplus
\mathbb{C}^n$ is a natural compactification of the space of hermitian $n\times
n$ matrices. We describe a Schubert-like, Whitney regular stratification on
this space which has a Morse theoretic origin. We prove that these strata
define closed suba... | math.GT math.AT math.DG | the grassmannian of hermitian lagrangian spaces in mathbbcnoplus mathbbcn is a natural compactification of the space of hermitian ntimes n matrices we describe a schubertlike whitney regular stratification on this space which has a morse theoretic origin we prove that these strata define closed subanalytic currents a l... | [['the', 'grassmannian', 'of', 'hermitian', 'lagrangian', 'spaces', 'in', 'mathbbcnoplus', 'mathbbcn', 'is', 'a', 'natural', 'compactification', 'of', 'the', 'space', 'of', 'hermitian', 'ntimes', 'n', 'matrices', 'we', 'describe', 'a', 'schubertlike', 'whitney', 'regular', 'stratification', 'on', 'this', 'space', 'whic... | [-0.2548239021303339, 0.082236197072133, -0.1168678267729572, 0.17326105298545574, -0.09331961268455619, -0.09973923603926475, -0.008664912333996553, 0.2896639393228624, -0.3189346335000462, -0.13497938609281038, 0.0758629361678484, -0.19455565399645516, -0.22473218921610774, 0.11619969384951724, -0.197990965589674, -0... |
708.267 | Environment-induced two-mode entanglement in quantum Brownian motion | The time evolution of quantum correlations of entangled two-mode continuous
variable states is examined in single-reservoir as well as two-reservoir
models, representing noisy correlated or uncorrelated non-Markovian quantum
channels. For this purpose the model of quantum Brownian motion is extended.
Various separabi... | quant-ph | the time evolution of quantum correlations of entangled twomode continuous variable states is examined in singlereservoir as well as tworeservoir models representing noisy correlated or uncorrelated nonmarkovian quantum channels for this purpose the model of quantum brownian motion is extended various separability crit... | [['the', 'time', 'evolution', 'of', 'quantum', 'correlations', 'of', 'entangled', 'twomode', 'continuous', 'variable', 'states', 'is', 'examined', 'in', 'singlereservoir', 'as', 'well', 'as', 'tworeservoir', 'models', 'representing', 'noisy', 'correlated', 'or', 'uncorrelated', 'nonmarkovian', 'quantum', 'channels', 'f... | [-0.15281208424444148, 0.23661238766314732, -0.10211600775657567, 0.07875857166499792, 0.03405204251921641, -0.2134494252536379, 0.03559248137404908, 0.3438971709170027, -0.2839791071294489, -0.23282578939984658, 0.08492573599183297, -0.26630357240778424, -0.07527444014342469, 0.1680561700043921, -0.007743363325835435,... |
708.2671 | On sequences of finitely generated discrete groups | We consider sequences of finitely generated discrete subgroups
Gamma_i=rho_i(Gamma) of a rank 1 Lie group G, where the representations rho_i
are not necessarily faithful. We show that, for algebraically convergent
sequences (Gamma_i), unless Gamma_i's are (eventually) elementary or contain
normal finite subgroups of ... | math.GR math.GT | we consider sequences of finitely generated discrete subgroups gamma_irho_igamma of a rank 1 lie group g where the representations rho_i are not necessarily faithful we show that for algebraically convergent sequences gamma_i unless gamma_is are eventually elementary or contain normal finite subgroups of arbitrarily hi... | [['we', 'consider', 'sequences', 'of', 'finitely', 'generated', 'discrete', 'subgroups', 'gamma_irho_igamma', 'of', 'a', 'rank', '1', 'lie', 'group', 'g', 'where', 'the', 'representations', 'rho_i', 'are', 'not', 'necessarily', 'faithful', 'we', 'show', 'that', 'for', 'algebraically', 'convergent', 'sequences', 'gamma_... | [-0.1965853138709394, 0.19536470639262105, -0.12305690089882422, 0.044503786731237435, -0.09747880405331609, -0.13561306689560665, 0.019840103097430218, 0.4162144479283108, -0.3504287840274139, -0.183818199211035, 0.12773403289586993, -0.25251161809149786, -0.10934596578639486, 0.19233035665208928, -0.1317883937882784,... |
708.2672 | Massive galaxies with very young AGN | Gigahertz Peaked Spectrum (GPS) radio galaxies are generally thought to be
the young counterparts of classical extended radio sources and live in massive
ellipticals. GPS sources are vital for studying the early evolution of
radio-loud AGN, the trigger of their nuclear activity, and the importance of
feedback in gala... | astro-ph | gigahertz peaked spectrum gps radio galaxies are generally thought to be the young counterparts of classical extended radio sources and live in massive ellipticals gps sources are vital for studying the early evolution of radioloud agn the trigger of their nuclear activity and the importance of feedback in galaxy evolu... | [['gigahertz', 'peaked', 'spectrum', 'gps', 'radio', 'galaxies', 'are', 'generally', 'thought', 'to', 'be', 'the', 'young', 'counterparts', 'of', 'classical', 'extended', 'radio', 'sources', 'and', 'live', 'in', 'massive', 'ellipticals', 'gps', 'sources', 'are', 'vital', 'for', 'studying', 'the', 'early', 'evolution', ... | [-0.0553707311293493, 0.09466235513786135, -0.06641526854348254, 0.159073922048763, -0.10159152410469936, -0.06438508532201387, 0.042383419183937655, 0.5093061669334157, -0.059536882548605743, -0.33323593919918143, 0.07777544722911481, -0.29496768781634636, -0.04621202990329786, 0.23294141339074362, -0.0083534203067881... |
708.2673 | Solitonic and Non-Solitonic Q-Stars | The properties of several types of Q-stars are studied and compared with
their flat space analogues, i.e. Q-balls. The analysis is based on calculating
the mass, global U(1) charge and binding energy for families of solutions
parametrized by the central value of the scalar field. The two most frequently
used Q-star m... | gr-qc hep-th | the properties of several types of qstars are studied and compared with their flat space analogues ie qballs the analysis is based on calculating the mass global u1 charge and binding energy for families of solutions parametrized by the central value of the scalar field the two most frequently used qstar models differi... | [['the', 'properties', 'of', 'several', 'types', 'of', 'qstars', 'are', 'studied', 'and', 'compared', 'with', 'their', 'flat', 'space', 'analogues', 'ie', 'qballs', 'the', 'analysis', 'is', 'based', 'on', 'calculating', 'the', 'mass', 'global', 'u1', 'charge', 'and', 'binding', 'energy', 'for', 'families', 'of', 'solut... | [-0.13012764697830095, 0.11557762874517499, -0.01730923113466157, 0.1357492723060219, -0.03160345905301411, -0.1332787154280255, -0.035152984588081394, 0.3613565825077334, -0.19741303971646793, -0.3141212709275513, 0.1185634996689008, -0.2819502295214471, -0.10831532596394693, 0.1939911790640752, -0.0017881817671818643... |
708.2674 | Governing Dynamics from cause and effect: -A novel formulation for
causality with applications in Quantum Gravity and Economic Theory | This paper defines an equation for causality. This equation is then combined
with the postulates of quantum mechanics and mass-energy equivalence to produce
a quantum mechanical telegrapher's equation and to reproduce the Schrodinger
and Klein-Gordon equations. The incompressible Navier-Stokes equations and
dynamic g... | physics.gen-ph | this paper defines an equation for causality this equation is then combined with the postulates of quantum mechanics and massenergy equivalence to produce a quantum mechanical telegraphers equation and to reproduce the schrodinger and kleingordon equations the incompressible navierstokes equations and dynamic general e... | [['this', 'paper', 'defines', 'an', 'equation', 'for', 'causality', 'this', 'equation', 'is', 'then', 'combined', 'with', 'the', 'postulates', 'of', 'quantum', 'mechanics', 'and', 'massenergy', 'equivalence', 'to', 'produce', 'a', 'quantum', 'mechanical', 'telegraphers', 'equation', 'and', 'to', 'reproduce', 'the', 'sc... | [-0.12926577811182963, 0.11900433165212347, -0.16038117198421892, 0.06937480008794177, -0.1430209950271961, -0.16588759743423093, -0.08435522926048236, 0.19522999694768703, -0.29733013526528285, -0.25948077764164296, 0.03691111976771195, -0.2921663296895217, -0.1476987096627446, 0.1444793572748261, -0.08536341281883847... |
708.2675 | An explanation why the Theta+ is seen in some experiments and not in
others | To understand the whole set of positive and null data on the Theta+(1530) -
production, we suggest the hypothesis that multiquark hadrons are mainly
generated from many-quark states, which emerge either as short-term hadron
fluctuations, or as hadron remnants in hard processes. This approach allows us
to describe bot... | hep-ph hep-ex nucl-ex nucl-th | to understand the whole set of positive and null data on the theta1530 production we suggest the hypothesis that multiquark hadrons are mainly generated from manyquark states which emerge either as shortterm hadron fluctuations or as hadron remnants in hard processes this approach allows us to describe both nonobservat... | [['to', 'understand', 'the', 'whole', 'set', 'of', 'positive', 'and', 'null', 'data', 'on', 'the', 'theta1530', 'production', 'we', 'suggest', 'the', 'hypothesis', 'that', 'multiquark', 'hadrons', 'are', 'mainly', 'generated', 'from', 'manyquark', 'states', 'which', 'emerge', 'either', 'as', 'shortterm', 'hadron', 'flu... | [-0.07445158565448773, 0.16834028878320867, -0.15280641539173567, 0.13456715724498639, -0.09922656593605494, -0.10605527244460507, 0.030269340608014256, 0.3491832416695662, -0.24082666638697314, -0.26335378898642003, 0.06343769793583749, -0.3019821187582028, -0.10287315064332743, 0.17741314894678947, 0.0273273373858477... |
708.2676 | Spectral analysis of high resolution near-infrared spectra of ultra cool
dwarfs | We present an analysis of high resolution spectra in the J band of five ultra
cool dwarfs from M6 to L0. A new ab initio water vapour line list and existing
line lists of FeH and CrH were used for spectra modelling. We find a good fit
for the Mn I 12899.76 A line. This feature is one of the few for which we have
a re... | astro-ph | we present an analysis of high resolution spectra in the j band of five ultra cool dwarfs from m6 to l0 a new ab initio water vapour line list and existing line lists of feh and crh were used for spectra modelling we find a good fit for the mn i 1289976 a line this feature is one of the few for which we have a reliable... | [['we', 'present', 'an', 'analysis', 'of', 'high', 'resolution', 'spectra', 'in', 'the', 'j', 'band', 'of', 'five', 'ultra', 'cool', 'dwarfs', 'from', 'm6', 'to', 'l0', 'a', 'new', 'ab', 'initio', 'water', 'vapour', 'line', 'list', 'and', 'existing', 'line', 'lists', 'of', 'feh', 'and', 'crh', 'were', 'used', 'for', 's... | [-0.06771734645762653, 0.03683538847975864, -0.035280146470500366, 0.04575593009056454, -0.0506947058873872, -0.1250919547483877, 0.06996477445311568, 0.4849639602557377, -0.17901763901959553, -0.3653067486843577, 0.04705501854574929, -0.31374734902271517, -0.05904263196237109, 0.17274694843562666, -0.00315726193840856... |
708.2677 | Structure of hard-hypersphere fluids in odd dimensions | The structural properties of single component fluids of hard hyperspheres in
odd space dimensionalities $d$ are studied with an analytical approximation
method that generalizes the Rational Function Approximation earlier introduced
in the study of hard-sphere fluids [S. B. Yuste and A. Santos, Phys. Rev. A
{\bf 43}, ... | cond-mat.stat-mech cond-mat.soft physics.chem-ph | the structural properties of single component fluids of hard hyperspheres in odd space dimensionalities d are studied with an analytical approximation method that generalizes the rational function approximation earlier introduced in the study of hardsphere fluids s b yuste and a santos phys rev a bf 43 5418 1991 the th... | [['the', 'structural', 'properties', 'of', 'single', 'component', 'fluids', 'of', 'hard', 'hyperspheres', 'in', 'odd', 'space', 'dimensionalities', 'd', 'are', 'studied', 'with', 'an', 'analytical', 'approximation', 'method', 'that', 'generalizes', 'the', 'rational', 'function', 'approximation', 'earlier', 'introduced'... | [-0.11765955185938555, 0.049031834262118185, -0.10332692531161368, 0.03246334743240508, -0.048847285603047706, -0.12274641205798477, 0.021639932180383206, 0.29528797217734304, -0.2319079658622146, -0.28184778139648886, 0.03030466632480966, -0.2650478865264701, -0.1445254516217504, 0.16035879293877559, 0.006944806194111... |
708.2678 | Eigen electric moments of magnetic-dipolar modes in quasi-2D ferrite
disk particles | A property associated with a vortex structure becomes evident from an
analysis of confinement phenomena of magnetic oscillations in a quasi-2D
ferrite disk with a dominating role of magnetic-dipolar
(non-exchange-interaction) spectra. The vortices are guaranteed by the chiral
edge states of magnetic-dipolar modes whi... | cond-mat.mtrl-sci cond-mat.mes-hall | a property associated with a vortex structure becomes evident from an analysis of confinement phenomena of magnetic oscillations in a quasi2d ferrite disk with a dominating role of magneticdipolar nonexchangeinteraction spectra the vortices are guaranteed by the chiral edge states of magneticdipolar modes which result ... | [['a', 'property', 'associated', 'with', 'a', 'vortex', 'structure', 'becomes', 'evident', 'from', 'an', 'analysis', 'of', 'confinement', 'phenomena', 'of', 'magnetic', 'oscillations', 'in', 'a', 'quasi2d', 'ferrite', 'disk', 'with', 'a', 'dominating', 'role', 'of', 'magneticdipolar', 'nonexchangeinteraction', 'spectra... | [-0.22903250448633822, 0.21145182252253944, -0.04073238579830178, 0.019571526257596835, -0.07969164960466478, -0.1071935684600731, 0.00031574469235516627, 0.37727602447706216, -0.23507684346838445, -0.29279944539184166, 0.04107142405285101, -0.2879425148118515, -0.08521316597732354, 0.1737268497331106, 0.04489804870610... |
708.2679 | Flow-deformed conformations of entangled polymers as persistent random
walks | Evolving structure and rheology across Kuhn scale interfaces in entangled
polymer fluids under flow play a prominent role in processing of manufactured
plastics, and have numerous other applications. Quantitative tracking of chain
conformation statistics on the Kuhn scale is essential for developing
computational mod... | cond-mat.soft cond-mat.mtrl-sci cond-mat.stat-mech | evolving structure and rheology across kuhn scale interfaces in entangled polymer fluids under flow play a prominent role in processing of manufactured plastics and have numerous other applications quantitative tracking of chain conformation statistics on the kuhn scale is essential for developing computational models ... | [['evolving', 'structure', 'and', 'rheology', 'across', 'kuhn', 'scale', 'interfaces', 'in', 'entangled', 'polymer', 'fluids', 'under', 'flow', 'play', 'a', 'prominent', 'role', 'in', 'processing', 'of', 'manufactured', 'plastics', 'and', 'have', 'numerous', 'other', 'applications', 'quantitative', 'tracking', 'of', 'c... | [-0.15119787640792648, 0.19428494680395797, -0.09418243395712049, 0.06288502894318855, -0.018141453316019587, -0.1805334896328359, 0.02012660649503112, 0.35873113537191853, -0.3201643143441867, -0.25086918805364117, 0.04173124344319044, -0.2363830785939209, -0.0913617708268075, 0.16236915372524696, 0.010454677692845402... |
708.268 | Paired composite fermion wavefunctions | We construct a family of BCS paired composite fermion wavefunctions that
generalize, but remain in the same topological phase as, the Moore-Read
Pfaffian state for the half-filled Landau level. It is shown that for a wide
range of experimentally relevant inter-electron interactions the groundstate
can be very accurat... | cond-mat.mes-hall | we construct a family of bcs paired composite fermion wavefunctions that generalize but remain in the same topological phase as the mooreread pfaffian state for the halffilled landau level it is shown that for a wide range of experimentally relevant interelectron interactions the groundstate can be very accurately repr... | [['we', 'construct', 'a', 'family', 'of', 'bcs', 'paired', 'composite', 'fermion', 'wavefunctions', 'that', 'generalize', 'but', 'remain', 'in', 'the', 'same', 'topological', 'phase', 'as', 'the', 'mooreread', 'pfaffian', 'state', 'for', 'the', 'halffilled', 'landau', 'level', 'it', 'is', 'shown', 'that', 'for', 'a', '... | [-0.1355218790368571, 0.24764848064828235, -0.06460897886539058, 0.17385070899931285, -0.025861527448376782, -0.15824574126432148, 0.04716277370999496, 0.33093883874467933, -0.23022143428142255, -0.28242877405136824, -0.009585826814425392, -0.22774053864682522, -0.1633982529433874, 0.14110886914512286, 0.04710454292720... |
708.2681 | Super-light electromagnetic wave with longitudinal and transversal modes | The transformation converting equations invariant under Lorentz into the
equations invariant under Galileo is obtained. On this basis: (1) the
super-light electromagnetic wave with longitudinal and transversal modes is
found out; (2) it is shown the wave velocity coincides with that of de
Broglie's wave; (3) the conn... | physics.gen-ph | the transformation converting equations invariant under lorentz into the equations invariant under galileo is obtained on this basis 1 the superlight electromagnetic wave with longitudinal and transversal modes is found out 2 it is shown the wave velocity coincides with that of de broglies wave 3 the connection between... | [['the', 'transformation', 'converting', 'equations', 'invariant', 'under', 'lorentz', 'into', 'the', 'equations', 'invariant', 'under', 'galileo', 'is', 'obtained', 'on', 'this', 'basis', '1', 'the', 'superlight', 'electromagnetic', 'wave', 'with', 'longitudinal', 'and', 'transversal', 'modes', 'is', 'found', 'out', '... | [-0.17216886450331487, 0.15706623601940795, -0.10844994004849993, 0.0862889875852238, -0.10045742869394225, -0.10930698222711409, -0.05172461734597631, 0.30494629465248607, -0.2195144933947456, -0.2729360813855988, 0.09107455494706818, -0.2690151748888263, -0.1621080475577384, 0.20828148028749222, -0.022537316939016002... |
708.2682 | Gemini GMOS/IFU spectroscopy of NGC 1569 - II: Mapping the roots of the
galactic outflow | We present a set of four Gemini-North GMOS/IFU observations of the central
disturbed regions of the dwarf irregular starburst galaxy NGC 1569, surrounding
the well-known super star clusters A and B. This continues on directly from a
companion paper, in which we describe the data reduction and analysis
techniques empl... | astro-ph | we present a set of four gemininorth gmosifu observations of the central disturbed regions of the dwarf irregular starburst galaxy ngc 1569 surrounding the wellknown super star clusters a and b this continues on directly from a companion paper in which we describe the data reduction and analysis techniques employed and... | [['we', 'present', 'a', 'set', 'of', 'four', 'gemininorth', 'gmosifu', 'observations', 'of', 'the', 'central', 'disturbed', 'regions', 'of', 'the', 'dwarf', 'irregular', 'starburst', 'galaxy', 'ngc', '1569', 'surrounding', 'the', 'wellknown', 'super', 'star', 'clusters', 'a', 'and', 'b', 'this', 'continues', 'on', 'dir... | [-0.09424479354885675, 0.07855217659129031, -0.07273609702569171, 0.050732070741347515, -0.05365726314384571, -0.0411479551430537, 0.05799003986335232, 0.4112982863573719, -0.2009818517676682, -0.2941524556087558, 0.07922794616432767, -0.2858853952711274, -0.041607157414336855, 0.18039143677732217, 0.010753893457384941... |
708.2683 | Automorphisms of the three-torus preserving a genus three Heegaard
splitting | The mapping class group of a Heegaard splitting is the group of connected
components in the set of automorphisms of the ambient manifold that map the
Heegaard surface onto itself. For the genus three Heegaard splitting of the
3-torus, we find an eight element generating set for this group. Six of these
generators ind... | math.GT | the mapping class group of a heegaard splitting is the group of connected components in the set of automorphisms of the ambient manifold that map the heegaard surface onto itself for the genus three heegaard splitting of the 3torus we find an eight element generating set for this group six of these generators induce ge... | [['the', 'mapping', 'class', 'group', 'of', 'a', 'heegaard', 'splitting', 'is', 'the', 'group', 'of', 'connected', 'components', 'in', 'the', 'set', 'of', 'automorphisms', 'of', 'the', 'ambient', 'manifold', 'that', 'map', 'the', 'heegaard', 'surface', 'onto', 'itself', 'for', 'the', 'genus', 'three', 'heegaard', 'spli... | [-0.25651554814917416, 0.10745103247766541, -0.06283668095145274, 0.03377084676931436, -0.07552343491162802, -0.09566193337652933, -0.013217548978187749, 0.36474112562231115, -0.34015164967324285, -0.29947521808129307, 0.09510039257175112, -0.28398164789620284, -0.11656367982819525, 0.20780588729256713, -0.071288175931... |
708.2684 | Gravitational lensing by Elliptical Galaxies, and the Schwarz Function | We discuss gravitational lensing by elliptical galaxies with some particular
mass distributions. Using simple techniques from the theory of quadrature
domains and the Schwarz function (cf. \cite{Sh}) we show that when the mass
density is constant on confocal ellipses, the total number of lensed images of
a point sour... | math-ph astro-ph math.CV math.MP | we discuss gravitational lensing by elliptical galaxies with some particular mass distributions using simple techniques from the theory of quadrature domains and the schwarz function cf citesh we show that when the mass density is constant on confocal ellipses the total number of lensed images of a point source cannot ... | [['we', 'discuss', 'gravitational', 'lensing', 'by', 'elliptical', 'galaxies', 'with', 'some', 'particular', 'mass', 'distributions', 'using', 'simple', 'techniques', 'from', 'the', 'theory', 'of', 'quadrature', 'domains', 'and', 'the', 'schwarz', 'function', 'cf', 'citesh', 'we', 'show', 'that', 'when', 'the', 'mass',... | [-0.11756172834805423, 0.05296740904250132, -0.08966253900159431, 0.09791096000085955, -0.057231216611320614, -0.10446165885616054, -0.016187767935065572, 0.3758968596136378, -0.22829488406498585, -0.2784731771636714, 0.10276402114334726, -0.3007453952925981, -0.14327210182904876, 0.2185730657550276, -0.095169400155384... |
708.2685 | A class of quantum doubles which are ribbon algebras | Andruskiewitsch and Schneider classify a large class of pointed Hopf algebras
with abelian coradical. The quantum double of each such Hopf algebra is
investigated. The quantum doubles of a family of Hopf algebras from the above
classification are ribbon Hopf algebras.
| math.RA math.QA | andruskiewitsch and schneider classify a large class of pointed hopf algebras with abelian coradical the quantum double of each such hopf algebra is investigated the quantum doubles of a family of hopf algebras from the above classification are ribbon hopf algebras | [['andruskiewitsch', 'and', 'schneider', 'classify', 'a', 'large', 'class', 'of', 'pointed', 'hopf', 'algebras', 'with', 'abelian', 'coradical', 'the', 'quantum', 'double', 'of', 'each', 'such', 'hopf', 'algebra', 'is', 'investigated', 'the', 'quantum', 'doubles', 'of', 'a', 'family', 'of', 'hopf', 'algebras', 'from', ... | [-0.2294999864406702, 0.0993141062648558, 0.01991859578141352, 0.09662013684070056, -0.17400616650446887, -0.23288396825423327, -0.052705808872038996, 0.30015061959260847, -0.42843119600197166, -0.16331467477650177, 0.1583050010305625, -0.20733484607644198, -0.1910993501816581, 0.24427885707558655, -0.1643224333004072,... |
708.2686 | The universal evolutionary computer based on super-recursive algorithms
of evolvability | This work exposes which mechanisms and procesess in the Nature of evolution
compute a function not computable by Turing machine. The computer with
intelligence that is not higher than one bacteria population could have, but
with efficency to solve the problems that are non-computable by Turing machine
is represented.... | cs.NE | this work exposes which mechanisms and procesess in the nature of evolution compute a function not computable by turing machine the computer with intelligence that is not higher than one bacteria population could have but with efficency to solve the problems that are noncomputable by turing machine is represented this ... | [['this', 'work', 'exposes', 'which', 'mechanisms', 'and', 'procesess', 'in', 'the', 'nature', 'of', 'evolution', 'compute', 'a', 'function', 'not', 'computable', 'by', 'turing', 'machine', 'the', 'computer', 'with', 'intelligence', 'that', 'is', 'not', 'higher', 'than', 'one', 'bacteria', 'population', 'could', 'have'... | [-0.06985839544722694, 0.13032130320789292, -0.13682005740702152, 0.08498932964357664, -0.13480272745073307, -0.19549980814190349, 0.014983077284341562, 0.3372673689154908, -0.30598620115051745, -0.30587523948634043, 0.09502095785683196, -0.20172573401941918, -0.23136889889428858, 0.2532954705093289, -0.109193378644704... |
708.2687 | Light Speed Invariance is a Remarkable Illusion | Though many experiments appear to have confirmed the light speed invariance
postulate of special relativity theory, this postulate is actually unverified.
This paper resolves this issue by first showing the manner in which an illusion
of light speed invariance occurs in two-way light speed measurement in the
framewor... | physics.gen-ph | though many experiments appear to have confirmed the light speed invariance postulate of special relativity theory this postulate is actually unverified this paper resolves this issue by first showing the manner in which an illusion of light speed invariance occurs in twoway light speed measurement in the framework of ... | [['though', 'many', 'experiments', 'appear', 'to', 'have', 'confirmed', 'the', 'light', 'speed', 'invariance', 'postulate', 'of', 'special', 'relativity', 'theory', 'this', 'postulate', 'is', 'actually', 'unverified', 'this', 'paper', 'resolves', 'this', 'issue', 'by', 'first', 'showing', 'the', 'manner', 'in', 'which'... | [-0.156877160001936, 0.15037385013843155, -0.15878508781654174, 0.06139883954283716, -0.07252532598930736, -0.11920689296540479, 0.08110544629405837, 0.3464093171872285, -0.29480289496741324, -0.31148456939127905, 0.047285446002375504, -0.19307356520804989, -0.1431453031227859, 0.18805973451086427, -0.13199883129794238... |
708.2688 | Hydrodynamic crystals: collective dynamics of regular arrays of
spherical particles in a parallel-wall channel | Simulations of over $10^3$ hydrodynamically coupled solid spheres are
performed to investigate collective motion of linear trains and regular square
arrays of particles suspended in a fluid bounded by two parallel walls. Our
novel accelerated Stokesian-dynamics algorithm relies on simplifications
associated with the ... | cond-mat.soft | simulations of over 103 hydrodynamically coupled solid spheres are performed to investigate collective motion of linear trains and regular square arrays of particles suspended in a fluid bounded by two parallel walls our novel accelerated stokesiandynamics algorithm relies on simplifications associated with the helesha... | [['simulations', 'of', 'over', '103', 'hydrodynamically', 'coupled', 'solid', 'spheres', 'are', 'performed', 'to', 'investigate', 'collective', 'motion', 'of', 'linear', 'trains', 'and', 'regular', 'square', 'arrays', 'of', 'particles', 'suspended', 'in', 'a', 'fluid', 'bounded', 'by', 'two', 'parallel', 'walls', 'our'... | [-0.19765534468087148, 0.2728986292215133, -0.042164934063215316, -0.034061344248461134, -0.014003608306800877, -0.08004535511595967, -0.02076421814315297, 0.3840610314229572, -0.2817597786930424, -0.2317648092859689, 0.05553659869438428, -0.2893035708248247, -0.13388553197369163, 0.1264560319279194, 0.0349766675290870... |
708.2689 | Nilsson diagrams for light neutron-rich nuclei with weakly-bound
neutrons | Using Woods-Saxon potentials and the eigenphase formalism for one-particle
resonances, one-particle bound and resonant levels for neutrons as a function
of quadrupole deformation are presented, which are supposed to be useful for
the interpretation of spectroscopic properties of some light neutron-rich
nuclei with we... | nucl-th | using woodssaxon potentials and the eigenphase formalism for oneparticle resonances oneparticle bound and resonant levels for neutrons as a function of quadrupole deformation are presented which are supposed to be useful for the interpretation of spectroscopic properties of some light neutronrich nuclei with weaklyboun... | [['using', 'woodssaxon', 'potentials', 'and', 'the', 'eigenphase', 'formalism', 'for', 'oneparticle', 'resonances', 'oneparticle', 'bound', 'and', 'resonant', 'levels', 'for', 'neutrons', 'as', 'a', 'function', 'of', 'quadrupole', 'deformation', 'are', 'presented', 'which', 'are', 'supposed', 'to', 'be', 'useful', 'for... | [-0.06558329695638951, 0.17800791302538463, -0.08237667960724727, 0.1437783722165631, -0.007590555992554611, -0.11595155241977896, 0.0451141277010041, 0.36953636262775724, -0.2063101726878454, -0.3001686207258182, -0.054112613015040806, -0.3359480932564803, -0.09391458333850326, 0.16057369384494885, 0.00891670245557538... |
708.269 | Effects of Schwarzschild Black Hole Horizon on Isothermal Plasma Wave
Dispersion | The 3+1 GRMHD equations for Schwarzschild spacetime in Rindler coordinates
with isothermal state of plasma are formulated. We consider the cases of
non-rotating and rotating backgrounds with non-magnetized and magnetized
plasmas. For these cases, the perturbed form of these equations are linearized
and Fourier analyz... | gr-qc astro-ph | the 31 grmhd equations for schwarzschild spacetime in rindler coordinates with isothermal state of plasma are formulated we consider the cases of nonrotating and rotating backgrounds with nonmagnetized and magnetized plasmas for these cases the perturbed form of these equations are linearized and fourier analyzed by in... | [['the', '31', 'grmhd', 'equations', 'for', 'schwarzschild', 'spacetime', 'in', 'rindler', 'coordinates', 'with', 'isothermal', 'state', 'of', 'plasma', 'are', 'formulated', 'we', 'consider', 'the', 'cases', 'of', 'nonrotating', 'and', 'rotating', 'backgrounds', 'with', 'nonmagnetized', 'and', 'magnetized', 'plasmas', ... | [-0.16768263488328494, 0.125693865035479, -0.0587399887278348, 0.06308651396070472, -0.10318601600614921, -0.10315983681558813, -0.016300962912065193, 0.31827603497267143, -0.19462767814186477, -0.31253374828341995, 0.0958717532416384, -0.30347825770717374, -0.11095309077100184, 0.21855501579882214, 0.00363806376831149... |
708.2691 | The Heterotic Road to the MSSM with R parity | In a previous paper, referred to as a "Mini-Landscape" search, we explored a
"fertile patch" of the heterotic landscape based on a Z6-II orbifold with
SO(10) and E6 local GUT structures. In the present paper we extend this
analysis. We find many models with the minimal supersymmetric standard model
spectra and an exa... | hep-th hep-ph | in a previous paper referred to as a minilandscape search we explored a fertile patch of the heterotic landscape based on a z6ii orbifold with so10 and e6 local gut structures in the present paper we extend this analysis we find many models with the minimal supersymmetric standard model spectra and an exact r parity in... | [['in', 'a', 'previous', 'paper', 'referred', 'to', 'as', 'a', 'minilandscape', 'search', 'we', 'explored', 'a', 'fertile', 'patch', 'of', 'the', 'heterotic', 'landscape', 'based', 'on', 'a', 'z6ii', 'orbifold', 'with', 'so10', 'and', 'e6', 'local', 'gut', 'structures', 'in', 'the', 'present', 'paper', 'we', 'extend', ... | [-0.10764789587525694, 0.18333670306908392, -0.011112944970210625, 0.1831107238522377, -0.07592489113742414, -0.19467561188435487, 0.034563951546239646, 0.34129526089631423, -0.1568800944098553, -0.30779421038459986, 0.0662535546020814, -0.25804109360243, -0.09680664390614328, 0.1200955332412074, -0.01988397626740526, ... |
708.2692 | Search for effects beyond Standard Model in photon scatterings and in
nonminimal gauge theories on linear colliders of new generation | The main possibilities of investigation of leptons and bosons production in
interaction of polarized photons are considered. The usage of $\gamma\gamma\to
f\bar{f}[+\gamma]$ reactions for the luminosity measurement on linear photon
collider is analyzed. The achievable precision of the luminosity measuring is
consider... | hep-ph | the main possibilities of investigation of leptons and bosons production in interaction of polarized photons are considered the usage of gammagammato fbarfgamma reactions for the luminosity measurement on linear photon collider is analyzed the achievable precision of the luminosity measuring is considered and calculate... | [['the', 'main', 'possibilities', 'of', 'investigation', 'of', 'leptons', 'and', 'bosons', 'production', 'in', 'interaction', 'of', 'polarized', 'photons', 'are', 'considered', 'the', 'usage', 'of', 'gammagammato', 'fbarfgamma', 'reactions', 'for', 'the', 'luminosity', 'measurement', 'on', 'linear', 'photon', 'collider... | [-0.104423136706464, 0.22731345729747165, -0.020534588656543444, 0.14901888923195655, -0.009426392393652349, -0.15042983655196926, -0.01364035380538553, 0.3435512350872159, -0.19855265921602647, -0.2812135575824262, -0.016615755942378505, -0.37883573678943017, 0.03425616964232177, 0.16053983157811066, 0.113492745552988... |
708.2693 | On the stability of precessing superfluid neutron stars | We discuss a new superfluid instability occuring in the interior of mature
neutron stars with implications for freely precessing neutron stars. This
short-wavelength instability is similar to the instability which is responsible
for the formation of turbulence in superfluid Helium. Its existence raises
serious questi... | astro-ph | we discuss a new superfluid instability occuring in the interior of mature neutron stars with implications for freely precessing neutron stars this shortwavelength instability is similar to the instability which is responsible for the formation of turbulence in superfluid helium its existence raises serious questions a... | [['we', 'discuss', 'a', 'new', 'superfluid', 'instability', 'occuring', 'in', 'the', 'interior', 'of', 'mature', 'neutron', 'stars', 'with', 'implications', 'for', 'freely', 'precessing', 'neutron', 'stars', 'this', 'shortwavelength', 'instability', 'is', 'similar', 'to', 'the', 'instability', 'which', 'is', 'responsib... | [-0.11828802889656453, 0.2187832765621207, -0.08143492289892738, 0.14397469650222255, -0.19866505835855763, -0.02695494575337285, 0.050793776436457556, 0.2537777529704192, -0.21009790371467787, -0.2705678583625408, 0.07006365829886543, -0.2582828634167238, -0.004711358645369136, 0.24168821640076146, -0.0576160421284536... |
708.2694 | Self-sensitive torsional microresonators based on a charge-density wave
system | Recently, there have been dramatic advances in the miniaturization of
electromechanical devices. Most of the micro- and nanoelectromechanical systems
(MEMS-NEMS) operate in the resonant modes1. The micron-, and, the more, the
submicron-sizes devices, are driven usually by electrostatic forces, as
piezoelectric and el... | cond-mat.str-el cond-mat.mtrl-sci | recently there have been dramatic advances in the miniaturization of electromechanical devices most of the micro and nanoelectromechanical systems memsnems operate in the resonant modes1 the micron and the more the submicronsizes devices are driven usually by electrostatic forces as piezoelectric and electromagnetic en... | [['recently', 'there', 'have', 'been', 'dramatic', 'advances', 'in', 'the', 'miniaturization', 'of', 'electromechanical', 'devices', 'most', 'of', 'the', 'micro', 'and', 'nanoelectromechanical', 'systems', 'memsnems', 'operate', 'in', 'the', 'resonant', 'modes1', 'the', 'micron', 'and', 'the', 'more', 'the', 'submicron... | [-0.2012072982314911, 0.17240314161612208, -0.009531402026847508, -0.034931432376761926, -0.08969237343948064, -0.12444090625667126, 0.01121398104255758, 0.39755835881285767, -0.26007261406686516, -0.27714843594059707, 0.06501480253303091, -0.30307314297913207, -0.15765422822880573, 0.2579628658989345, -0.0259778348212... |
708.2695 | The Inner Jet of the Radio Galaxy M87 | We report new 2 cm VLBA images of the inner radio jet of M87 showing a limb
brightened structure and unambiguous evidence for a faint 3 mas long
counter-feature which also appears limb brightened. Multi-epoch observations of
seven separate jet features show typical speeds of less than a few percent of
the speed of li... | astro-ph | we report new 2 cm vlba images of the inner radio jet of m87 showing a limb brightened structure and unambiguous evidence for a faint 3 mas long counterfeature which also appears limb brightened multiepoch observations of seven separate jet features show typical speeds of less than a few percent of the speed of light d... | [['we', 'report', 'new', '2', 'cm', 'vlba', 'images', 'of', 'the', 'inner', 'radio', 'jet', 'of', 'm87', 'showing', 'a', 'limb', 'brightened', 'structure', 'and', 'unambiguous', 'evidence', 'for', 'a', 'faint', '3', 'mas', 'long', 'counterfeature', 'which', 'also', 'appears', 'limb', 'brightened', 'multiepoch', 'observ... | [-0.11762987431227734, 0.11671354147979314, -0.08711112336297135, 0.10363543255085564, -0.1473562267496233, -0.11141970639775513, -0.030444667407661486, 0.4669650636708281, -0.23457774871687412, -0.337386043160964, 0.08034494554454899, -0.22801011053335135, -0.01915392793928552, 0.2127870347174359, 0.001709857282294019... |
708.2696 | Do flares in Sagittarius A* reflect the last stage of tidal capture? | In recent years the case for the presence of 3-4 10^6 M_sun black hole in our
Galactic Center has gained strength from results of stellar dynamics
observations and from the detection of several rapid X-ray and IR flares
observed in the Sagittarius A* from 2000 to 2004. Here we explore the idea that
such flares are pr... | astro-ph | in recent years the case for the presence of 34 106 m_sun black hole in our galactic center has gained strength from results of stellar dynamics observations and from the detection of several rapid xray and ir flares observed in the sagittarius a from 2000 to 2004 here we explore the idea that such flares are produced ... | [['in', 'recent', 'years', 'the', 'case', 'for', 'the', 'presence', 'of', '34', '106', 'm_sun', 'black', 'hole', 'in', 'our', 'galactic', 'center', 'has', 'gained', 'strength', 'from', 'results', 'of', 'stellar', 'dynamics', 'observations', 'and', 'from', 'the', 'detection', 'of', 'several', 'rapid', 'xray', 'and', 'ir... | [-0.060842227563261984, 0.10926642040586254, -0.03921748276799917, 0.08196168571710587, -0.051994976277152695, -0.021975392991056046, 0.03702026151741544, 0.3487866618484259, -0.16994058116649588, -0.35461682161316277, 0.0925277427661543, -0.36725306225319704, -0.11336393998625378, 0.2398995215538889, -0.11010857295865... |
708.2697 | Epsilon Expansion for Multicritical Fixed Points and Exact
Renormalisation Group Equations | The Polchinski version of the exact renormalisation group equations is
applied to multicritical fixed points, which are present for dimensions between
two and four, for scalar theories using both the local potential approximation
and its extension, the derivative expansion. The results are compared with the
epsilon e... | hep-th cond-mat.other | the polchinski version of the exact renormalisation group equations is applied to multicritical fixed points which are present for dimensions between two and four for scalar theories using both the local potential approximation and its extension the derivative expansion the results are compared with the epsilon expansi... | [['the', 'polchinski', 'version', 'of', 'the', 'exact', 'renormalisation', 'group', 'equations', 'is', 'applied', 'to', 'multicritical', 'fixed', 'points', 'which', 'are', 'present', 'for', 'dimensions', 'between', 'two', 'and', 'four', 'for', 'scalar', 'theories', 'using', 'both', 'the', 'local', 'potential', 'approxi... | [-0.12653913798393482, 0.05863254818330964, -0.12392422649789742, 0.06702808088786993, -0.058210254835738044, -0.12308741810456293, 0.011368117866299625, 0.27810770097633813, -0.22927048356043842, -0.2555016531263414, 0.12562913282513735, -0.31682873533675504, -0.1391247647914028, 0.17123021053021434, 0.039020798961286... |
708.2698 | Fisher information of orthogonal polynomials I | Following the lead of J. Dehesa and his collaborators, we compute the Fisher
information of the Meixner-Pollaczek, Meixner, Krawtchouk and Charlier
polynomials.
| math.CA | following the lead of j dehesa and his collaborators we compute the fisher information of the meixnerpollaczek meixner krawtchouk and charlier polynomials | [['following', 'the', 'lead', 'of', 'j', 'dehesa', 'and', 'his', 'collaborators', 'we', 'compute', 'the', 'fisher', 'information', 'of', 'the', 'meixnerpollaczek', 'meixner', 'krawtchouk', 'and', 'charlier', 'polynomials']] | [-0.12786615178698585, 0.04156009378355174, -0.14200427808931895, 0.08469823994562917, -0.0831604218997416, -0.17180701380684263, 0.04093273141465727, 0.2541820540514198, -0.26234468622576623, -0.1965442585448424, 0.08865819851468716, -0.3253768274471873, -0.23913340447914033, 0.12272194613303457, -0.15936759477924733,... |
708.2699 | The mean-square of Dirichlet L-functions | We verify the conjecture of [CFKRS] for the mean square near the critical
point of Dirichlet L-functions for a composite modulus q. We also prove a kind
of reciprocity formula when the second moment for a prime modulus is twisted by
a character evaluated at a different prime.
| math.NT | we verify the conjecture of cfkrs for the mean square near the critical point of dirichlet lfunctions for a composite modulus q we also prove a kind of reciprocity formula when the second moment for a prime modulus is twisted by a character evaluated at a different prime | [['we', 'verify', 'the', 'conjecture', 'of', 'cfkrs', 'for', 'the', 'mean', 'square', 'near', 'the', 'critical', 'point', 'of', 'dirichlet', 'lfunctions', 'for', 'a', 'composite', 'modulus', 'q', 'we', 'also', 'prove', 'a', 'kind', 'of', 'reciprocity', 'formula', 'when', 'the', 'second', 'moment', 'for', 'a', 'prime', ... | [-0.2116759546655924, 0.0750182126747801, -0.14443230114758332, 0.0942851823204732, -0.05598444154763475, -0.13103850176954207, 0.059642677399716244, 0.2711228644871648, -0.3009408707631395, -0.21452269197300453, 0.0900727924197278, -0.2315963645752995, -0.13740388605188816, 0.23527492822564028, -0.031124479870529884, ... |
708.27 | On the Enormous Effect of Electric Field on the Crystalline Lattice of
the Conductors with Charge-Density Waves | We discuss deformation of quasi 1-dimensional conductors with charge-density
wave (CDW) under the electric field deforming the CDW. In case of ``strong''
CDW-lattice interaction the effect can be treated in terms of the converse
piezoelectric effect with enormous piezomodulus, $\sim L_c/\lambda$ times
larger than tha... | cond-mat.str-el | we discuss deformation of quasi 1dimensional conductors with chargedensity wave cdw under the electric field deforming the cdw in case of strong cdwlattice interaction the effect can be treated in terms of the converse piezoelectric effect with enormous piezomodulus sim l_clambda times larger than that in ionic crystal... | [['we', 'discuss', 'deformation', 'of', 'quasi', '1dimensional', 'conductors', 'with', 'chargedensity', 'wave', 'cdw', 'under', 'the', 'electric', 'field', 'deforming', 'the', 'cdw', 'in', 'case', 'of', 'strong', 'cdwlattice', 'interaction', 'the', 'effect', 'can', 'be', 'treated', 'in', 'terms', 'of', 'the', 'converse... | [-0.22659314337037154, 0.27659947159787956, -0.00011740655216546554, 0.01838428574890988, -0.04617374021349088, -0.11092181039209706, 0.020359235398365923, 0.3862329467357892, -0.2794211020447173, -0.2107247663178604, -0.010207993453939638, -0.3144489200873617, -0.12815311099270815, 0.1291126994183287, 0.05067967664826... |
708.2701 | Theory and Phenomenology of Exotic Isosinglet Quarks and Squarks | Extensions of the MSSM often predict the existence of new fermions and their
scalar superpartners which are vectorlike with respect to the standard model
gauge group but may be chiral under additional gauge factors. In this paper we
explore the production and decay of an important example, i.e., a heavy
isosinglet ch... | hep-ph hep-ex | extensions of the mssm often predict the existence of new fermions and their scalar superpartners which are vectorlike with respect to the standard model gauge group but may be chiral under additional gauge factors in this paper we explore the production and decay of an important example ie a heavy isosinglet charge 13... | [['extensions', 'of', 'the', 'mssm', 'often', 'predict', 'the', 'existence', 'of', 'new', 'fermions', 'and', 'their', 'scalar', 'superpartners', 'which', 'are', 'vectorlike', 'with', 'respect', 'to', 'the', 'standard', 'model', 'gauge', 'group', 'but', 'may', 'be', 'chiral', 'under', 'additional', 'gauge', 'factors', '... | [-0.10501846642000601, 0.2893812426353063, -0.045917368246282037, 0.1668860469517506, -0.08305249493470059, -0.18368379721520817, 0.03540444011590846, 0.31115878149594595, -0.20664148631089546, -0.2905052919516667, 0.055547180676590056, -0.29218801986822424, -0.022217923835999867, 0.09188274083166145, 0.044156880532217... |
708.2702 | The Mass Assembly of Fossil Groups of Galaxies in the Millennium
Simulation | The evolution of present-day fossil galaxy groups is studied in the
Millennium Simulation. Using the corresponding Millennium gas simulation and
semi-analytic galaxy catalogues, we select fossil groups at redshift zero
according to the conventional observational criteria, and trace the haloes
corresponding to these g... | astro-ph | the evolution of presentday fossil galaxy groups is studied in the millennium simulation using the corresponding millennium gas simulation and semianalytic galaxy catalogues we select fossil groups at redshift zero according to the conventional observational criteria and trace the haloes corresponding to these groups b... | [['the', 'evolution', 'of', 'presentday', 'fossil', 'galaxy', 'groups', 'is', 'studied', 'in', 'the', 'millennium', 'simulation', 'using', 'the', 'corresponding', 'millennium', 'gas', 'simulation', 'and', 'semianalytic', 'galaxy', 'catalogues', 'we', 'select', 'fossil', 'groups', 'at', 'redshift', 'zero', 'according', ... | [-0.06662345208963023, 0.12294078989163082, -0.10743134705186949, 0.1371873600276116, -0.060524571970705696, -0.012784251696404701, 0.019452793584739576, 0.3899393394548711, -0.17571550233116567, -0.3752123189509892, 0.06946412583970836, -0.29030711757772365, -0.0032470729151140147, 0.19782546556000014, 0.0106317797965... |
708.2703 | The Nature of Nearby Counterparts to Intermediate-Redshift Luminous
Compact Blue Galaxies. III. Interferometric Observations of Neutral Atomic
and Molecular Gas | We present the results of a VLA and OVRO-MMA follow-up to our single-dish
surveys of the neutral atomic and molecular gas in a sample of nearby Luminous
Compact Blue Galaxies (LCBGs). These luminous, blue, high surface brightness,
starbursting galaxies were selected using criteria similar to that used to
define LCBGs... | astro-ph | we present the results of a vla and ovromma followup to our singledish surveys of the neutral atomic and molecular gas in a sample of nearby luminous compact blue galaxies lcbgs these luminous blue high surface brightness starbursting galaxies were selected using criteria similar to that used to define lcbgs at higher ... | [['we', 'present', 'the', 'results', 'of', 'a', 'vla', 'and', 'ovromma', 'followup', 'to', 'our', 'singledish', 'surveys', 'of', 'the', 'neutral', 'atomic', 'and', 'molecular', 'gas', 'in', 'a', 'sample', 'of', 'nearby', 'luminous', 'compact', 'blue', 'galaxies', 'lcbgs', 'these', 'luminous', 'blue', 'high', 'surface',... | [-0.05336051519244923, 0.09969057686871467, -0.0693286743976943, 0.08314896928834924, -0.06066660221210487, -0.06476689333585259, 0.049269034139470286, 0.48227942946681873, -0.08370419263692318, -0.347984279278103, 0.06985320807384367, -0.3072975284064845, -0.04507298559442886, 0.19086222962256777, -0.02056045735419587... |
708.2704 | Edge States and Interferometers in the Pfaffian and anti-Pfaffian States | We compute the tunneling current in a double point contact geometry of a
Quantum Hall system at filling fraction $\nu=5/2$, as function of voltage and
temeprature, in the weak tunneling regime. We quantitatively compare two
possible candidates for the state at $\nu=5/2$: the Moore-Read Pfaffian state,
and its particl... | cond-mat.mes-hall cond-mat.str-el | we compute the tunneling current in a double point contact geometry of a quantum hall system at filling fraction nu52 as function of voltage and temeprature in the weak tunneling regime we quantitatively compare two possible candidates for the state at nu52 the mooreread pfaffian state and its particlehole conjugate th... | [['we', 'compute', 'the', 'tunneling', 'current', 'in', 'a', 'double', 'point', 'contact', 'geometry', 'of', 'a', 'quantum', 'hall', 'system', 'at', 'filling', 'fraction', 'nu52', 'as', 'function', 'of', 'voltage', 'and', 'temeprature', 'in', 'the', 'weak', 'tunneling', 'regime', 'we', 'quantitatively', 'compare', 'two... | [-0.1797128325575434, 0.16081876198083514, -0.11452751399742232, 0.09855112497821267, -0.00915896668340321, -0.19276316970425808, 0.11565542632403474, 0.3450863508760561, -0.23860431092296852, -0.30246093845063887, -0.012901834331533331, -0.29914324737533377, -0.15587659656173652, 0.1885135215419678, 0.0323819055647393... |
708.2705 | Characterizing algebraic stacks | We extend the notion of algebraic stack to an arbitrary subcanonical site C.
If the topology on C is local on the target and satisfies descent for
morphisms, we show that algebraic stacks are precisely those which are weakly
equivalent to representable presheaves of groupoids whose domain map is a
cover. This leads n... | math.AT math.CT | we extend the notion of algebraic stack to an arbitrary subcanonical site c if the topology on c is local on the target and satisfies descent for morphisms we show that algebraic stacks are precisely those which are weakly equivalent to representable presheaves of groupoids whose domain map is a cover this leads natura... | [['we', 'extend', 'the', 'notion', 'of', 'algebraic', 'stack', 'to', 'an', 'arbitrary', 'subcanonical', 'site', 'c', 'if', 'the', 'topology', 'on', 'c', 'is', 'local', 'on', 'the', 'target', 'and', 'satisfies', 'descent', 'for', 'morphisms', 'we', 'show', 'that', 'algebraic', 'stacks', 'are', 'precisely', 'those', 'whi... | [-0.15336646208805696, 0.07323567173630831, -0.07809440380494509, 0.1289427902632659, -0.12243573149400098, -0.14412096140773167, 0.01441390562602984, 0.4059482173894399, -0.4054837729781866, -0.20714221959268408, 0.07867874702704804, -0.24157071399302887, -0.11980800601387663, 0.19319323615304063, -0.17514244399166534... |
708.2706 | Observation of the First Excited State in 23O | The first excited state in neutron-rich 23O was observed in a (2p1n)
knock-out reaction from 26Ne on a beryllium target at a beam energy of 86
MeV/A. The state is unbound with respect to neutron emission and was
reconstructed from the invariant mass from the 22O fragment and the neutron. It
is unbound by 45(2) keV co... | nucl-ex | the first excited state in neutronrich 23o was observed in a 2p1n knockout reaction from 26ne on a beryllium target at a beam energy of 86 meva the state is unbound with respect to neutron emission and was reconstructed from the invariant mass from the 22o fragment and the neutron it is unbound by 452 kev corresponding... | [['the', 'first', 'excited', 'state', 'in', 'neutronrich', '23o', 'was', 'observed', 'in', 'a', '2p1n', 'knockout', 'reaction', 'from', '26ne', 'on', 'a', 'beryllium', 'target', 'at', 'a', 'beam', 'energy', 'of', '86', 'meva', 'the', 'state', 'is', 'unbound', 'with', 'respect', 'to', 'neutron', 'emission', 'and', 'was'... | [-0.026619237253212108, 0.20923745262062649, -0.09267454698989319, 0.11098221103842977, 0.0037943489995719256, -0.06441649757123188, 0.08765987871700655, 0.3259389771796439, -0.2079369445209918, -0.3571022338336384, -0.05602275940296038, -0.3397209772070789, 0.0661653240069585, 0.13960923138074577, 0.07881515892222524,... |
708.2707 | Learning and innovative elements of strategy adoption rules expand
cooperative network topologies | Cooperation plays a key role in the evolution of complex systems. However,
the level of cooperation extensively varies with the topology of agent networks
in the widely used models of repeated games. Here we show that cooperation
remains rather stable by applying the reinforcement learning strategy adoption
rule, Q-l... | q-bio.MN cond-mat.dis-nn nlin.AO physics.bio-ph | cooperation plays a key role in the evolution of complex systems however the level of cooperation extensively varies with the topology of agent networks in the widely used models of repeated games here we show that cooperation remains rather stable by applying the reinforcement learning strategy adoption rule qlearning... | [['cooperation', 'plays', 'a', 'key', 'role', 'in', 'the', 'evolution', 'of', 'complex', 'systems', 'however', 'the', 'level', 'of', 'cooperation', 'extensively', 'varies', 'with', 'the', 'topology', 'of', 'agent', 'networks', 'in', 'the', 'widely', 'used', 'models', 'of', 'repeated', 'games', 'here', 'we', 'show', 'th... | [-0.14479970259661662, 0.0764376853522969, -0.07854756792847883, 0.07542968586704789, -0.05106987675557281, -0.1557301165907081, 0.11319849711847815, 0.4319974756177096, -0.27996814374084816, -0.2870467822391161, 0.07392549020410043, -0.18204987377306836, -0.263690775434641, 0.13064058820398294, -0.0884033500585446, -0... |
708.2708 | Population of neutron unbound states via two-proton knockout reactions | The two-proton knockout reaction 9Be(26Ne,O2p) was used to explore excited
unbound states of 23O and 24O. In 23O a state at an excitation energy of
2.79(13) MeV was observed. There was no conclusive evidence for the population
of excited states in 24O.
| nucl-ex | the twoproton knockout reaction 9be26neo2p was used to explore excited unbound states of 23o and 24o in 23o a state at an excitation energy of 27913 mev was observed there was no conclusive evidence for the population of excited states in 24o | [['the', 'twoproton', 'knockout', 'reaction', '9be26neo2p', 'was', 'used', 'to', 'explore', 'excited', 'unbound', 'states', 'of', '23o', 'and', '24o', 'in', '23o', 'a', 'state', 'at', 'an', 'excitation', 'energy', 'of', '27913', 'mev', 'was', 'observed', 'there', 'was', 'no', 'conclusive', 'evidence', 'for', 'the', 'po... | [-0.04295006664469838, 0.2577310210243013, -0.08957901111061801, 0.21261247051879764, 0.08419680876177153, -0.08989131093258038, 0.11176181291230022, 0.3893701083958149, -0.09939920427277685, -0.30306623167125507, -0.12951318065752276, -0.3588707521557808, 0.07895578476600348, 0.09747130959294736, 0.1311157365096733, 0... |
708.2709 | Bicomponents and the robustness of networks to failure | A common definition of a robust connection between two nodes in a network
such as a communication network is that there should be at least two
independent paths connecting them, so that the failure of no single node in the
network causes them to become disconnected. This definition leads us naturally
to consider bico... | cond-mat.stat-mech cond-mat.dis-nn | a common definition of a robust connection between two nodes in a network such as a communication network is that there should be at least two independent paths connecting them so that the failure of no single node in the network causes them to become disconnected this definition leads us naturally to consider bicompon... | [['a', 'common', 'definition', 'of', 'a', 'robust', 'connection', 'between', 'two', 'nodes', 'in', 'a', 'network', 'such', 'as', 'a', 'communication', 'network', 'is', 'that', 'there', 'should', 'be', 'at', 'least', 'two', 'independent', 'paths', 'connecting', 'them', 'so', 'that', 'the', 'failure', 'of', 'no', 'single... | [-0.15563298819718815, 0.07238785158915562, -0.07191347816600076, 0.052431294173099253, -0.06550553749790804, -0.17771628741562986, 0.05958107792321243, 0.40815994897881563, -0.2475896211987371, -0.28637531682034023, 0.10711254984016705, -0.2840847971092444, -0.23321687845721803, 0.1666759352434989, -0.0608302335876942... |
708.271 | The quantization of a toric manifold is given by the integer lattice
points in the moment polytope | We describe a very nice argument, which we learned from Sue Tolman, that the
dimension of the quantization space of a toric manifold, using a Kaehler
polarization, is given by the number of integer lattice points in the moment
polytope.
| math.SG | we describe a very nice argument which we learned from sue tolman that the dimension of the quantization space of a toric manifold using a kaehler polarization is given by the number of integer lattice points in the moment polytope | [['we', 'describe', 'a', 'very', 'nice', 'argument', 'which', 'we', 'learned', 'from', 'sue', 'tolman', 'that', 'the', 'dimension', 'of', 'the', 'quantization', 'space', 'of', 'a', 'toric', 'manifold', 'using', 'a', 'kaehler', 'polarization', 'is', 'given', 'by', 'the', 'number', 'of', 'integer', 'lattice', 'points', '... | [-0.16587432916276157, 0.0723946840967983, -0.13487825812771917, 0.08345688473491464, -0.11040988474851474, -0.1475705005810596, 0.04565889794175746, 0.3211761438753456, -0.27099448163062334, -0.2126851593144238, 0.08383637502265628, -0.240091841830872, -0.1891754156909883, 0.11870485665276646, -0.1439808240858838, 0.0... |
708.2711 | Low angular momentum accretion in the collapsar: how long can a long GRB
be? | The collapsar model is the most promising scenario to explain the huge
release of energy associated with long duration gamma-ray-bursts (GRBs). Within
this scenario GRBs are believed to be powered by accretion through a
rotationally support torus or by fast rotation of a compact object. In both
cases then, rotation o... | astro-ph | the collapsar model is the most promising scenario to explain the huge release of energy associated with long duration gammaraybursts grbs within this scenario grbs are believed to be powered by accretion through a rotationally support torus or by fast rotation of a compact object in both cases then rotation of the pro... | [['the', 'collapsar', 'model', 'is', 'the', 'most', 'promising', 'scenario', 'to', 'explain', 'the', 'huge', 'release', 'of', 'energy', 'associated', 'with', 'long', 'duration', 'gammaraybursts', 'grbs', 'within', 'this', 'scenario', 'grbs', 'are', 'believed', 'to', 'be', 'powered', 'by', 'accretion', 'through', 'a', '... | [-0.11091360219288618, 0.14226096818705022, -0.06706254738577021, 0.12446719284610784, -0.14349273400536428, -0.08146098667833333, 0.04724713697845194, 0.4135898213435818, -0.2072592567021881, -0.32551835567865056, 0.12098327509399193, -0.21837931778245548, -0.04819400276173837, 0.23701695547109314, -0.0842025161415222... |
708.2712 | Maximum Likelihood method for ultrahigh energy cosmic ray cross
correlations with astrophysical sources | We extend the Maximum Likelihood method used by HiRes to study cross
correlations between a catalog of candidate astrophysical sources and Ultrahigh
Energy Cosmic Rays (UHECRs), to allow for differing source luminosities. Our
approach permits individual sources to be ranked according to their likelihood
of having emi... | astro-ph | we extend the maximum likelihood method used by hires to study cross correlations between a catalog of candidate astrophysical sources and ultrahigh energy cosmic rays uhecrs to allow for differing source luminosities our approach permits individual sources to be ranked according to their likelihood of having emitted t... | [['we', 'extend', 'the', 'maximum', 'likelihood', 'method', 'used', 'by', 'hires', 'to', 'study', 'cross', 'correlations', 'between', 'a', 'catalog', 'of', 'candidate', 'astrophysical', 'sources', 'and', 'ultrahigh', 'energy', 'cosmic', 'rays', 'uhecrs', 'to', 'allow', 'for', 'differing', 'source', 'luminosities', 'our... | [-0.034013436042072104, 0.13797918457976788, -0.06395155855122654, 0.18777035050202515, -0.07140623167927923, -0.08614690084781113, 0.08547303655677228, 0.45915897640174835, -0.20020882030109335, -0.4420567720207846, -0.026932404125002266, -0.3564253799448689, -0.0350343255090645, 0.21701174900578013, 0.019583731814790... |
708.2713 | Comment on "Radiative effect on natural convection flows in porous
media, A.A. Mohammadein, M. A. Mansour, Sahar M. Abd El Gaied and Rama Subba
Reddy Gorla [Transport in Porous Media 32:263-283, 1998]" | In the above paper the authors treat the natural convection boundary layer
flow in a Darcy-Brinkman-Forchheimer porous medium. In the energy equation the
radiation effect has been taken into account. A two-parameter perturbation
method is used for the solution of the equations. The first order results are
presented i... | physics.flu-dyn | in the above paper the authors treat the natural convection boundary layer flow in a darcybrinkmanforchheimer porous medium in the energy equation the radiation effect has been taken into account a twoparameter perturbation method is used for the solution of the equations the first order results are presented in tables... | [['in', 'the', 'above', 'paper', 'the', 'authors', 'treat', 'the', 'natural', 'convection', 'boundary', 'layer', 'flow', 'in', 'a', 'darcybrinkmanforchheimer', 'porous', 'medium', 'in', 'the', 'energy', 'equation', 'the', 'radiation', 'effect', 'has', 'been', 'taken', 'into', 'account', 'a', 'twoparameter', 'perturbati... | [-0.11819846965866446, 0.09502187375685688, -0.09376895489086481, 0.059655192472167655, -0.06383401099028009, -0.0705704431783295, -0.021839290841440248, 0.3413635766923879, -0.26185558199402736, -0.27773708109320566, 0.11267401892550741, -0.31302536538604536, -0.13442034790800375, 0.19182666371378934, -0.0523105987601... |
708.2714 | Large scale magnetic field of the Milky Way from WMAP3 data | We report on initial results from a project to constrain the large-scale and
turbulent magnetic fields of the Milky Way galaxy, which eventually will
incorporate all of the relevant observational data. In this paper we fit
popular large scale magnetic field models to WMAP3 polarization maps. We find
that the polariza... | astro-ph | we report on initial results from a project to constrain the largescale and turbulent magnetic fields of the milky way galaxy which eventually will incorporate all of the relevant observational data in this paper we fit popular large scale magnetic field models to wmap3 polarization maps we find that the polarization d... | [['we', 'report', 'on', 'initial', 'results', 'from', 'a', 'project', 'to', 'constrain', 'the', 'largescale', 'and', 'turbulent', 'magnetic', 'fields', 'of', 'the', 'milky', 'way', 'galaxy', 'which', 'eventually', 'will', 'incorporate', 'all', 'of', 'the', 'relevant', 'observational', 'data', 'in', 'this', 'paper', 'we... | [-0.108793627223196, 0.12358569175397095, -0.09027507608070186, 0.12714913564636127, -0.16232370553342135, -0.07298730013548936, 0.004130786952660664, 0.38179743256615967, -0.29294037836309716, -0.38847986941691487, 0.06392288684330293, -0.23662145248749047, -0.08755864957898954, 0.19588902707358724, 0.0020761165375772... |
708.2715 | Dissociative recombination of H3+ in the ground and excited vibrational
states | The article presents calculated dissociative recombination (DR) rate
coefficients for H+3 . The previous theoretical work on H+3 was performed using
the adiabatic hyperspherical approximation to calculate the target ion
vibrational states and it considered just a limited number of ionic rotational
states. In this stu... | physics.atom-ph | the article presents calculated dissociative recombination dr rate coefficients for h3 the previous theoretical work on h3 was performed using the adiabatic hyperspherical approximation to calculate the target ion vibrational states and it considered just a limited number of ionic rotational states in this study we use... | [['the', 'article', 'presents', 'calculated', 'dissociative', 'recombination', 'dr', 'rate', 'coefficients', 'for', 'h3', 'the', 'previous', 'theoretical', 'work', 'on', 'h3', 'was', 'performed', 'using', 'the', 'adiabatic', 'hyperspherical', 'approximation', 'to', 'calculate', 'the', 'target', 'ion', 'vibrational', 's... | [-0.0782835407859374, 0.14898408595727458, -0.01518868951861579, 0.07771156032668045, 0.02870394888689007, -0.10941661756647669, 0.0651370832980003, 0.37447786069712286, -0.18380057518746448, -0.28224761931005843, 0.025858356607268037, -0.2843135719112358, -0.023233929168872583, 0.2097232503793347, 0.04558997995202771,... |
708.2716 | The performance of an idealized large-area array of moderate-sized IACTs | We present simulations of a large array of imaging atmospheric Cherenkov
telescopes (IACTs), for which the size of the array footprint is much larger
than the size of the Cherenkov lightpool. To evaluate limitations of the
imaging atmospheric Cherenkov technique, the array is simulated under the
assumption of ideal o... | astro-ph | we present simulations of a large array of imaging atmospheric cherenkov telescopes iacts for which the size of the array footprint is much larger than the size of the cherenkov lightpool to evaluate limitations of the imaging atmospheric cherenkov technique the array is simulated under the assumption of ideal optics h... | [['we', 'present', 'simulations', 'of', 'a', 'large', 'array', 'of', 'imaging', 'atmospheric', 'cherenkov', 'telescopes', 'iacts', 'for', 'which', 'the', 'size', 'of', 'the', 'array', 'footprint', 'is', 'much', 'larger', 'than', 'the', 'size', 'of', 'the', 'cherenkov', 'lightpool', 'to', 'evaluate', 'limitations', 'of'... | [-0.13149072877244977, 0.15943608955788707, -0.022678494839588316, 0.06353142230423182, -0.08778152582273493, -0.0652160063173955, -0.014086966563727918, 0.42348573629449054, -0.1873917455436677, -0.3912858530061274, 0.14839263045516743, -0.2821611630980198, -0.07012888339605576, 0.27525742319450386, 0.0105068253209375... |
708.2717 | Aggregation Languages for Moving Object and Places of Interest Data | We address aggregate queries over GIS data and moving object data, where
non-spatial data are stored in a data warehouse. We propose a formal data model
and query language to express complex aggregate queries. Next, we study the
compression of trajectory data, produced by moving objects, using the notions
of stops an... | cs.DB | we address aggregate queries over gis data and moving object data where nonspatial data are stored in a data warehouse we propose a formal data model and query language to express complex aggregate queries next we study the compression of trajectory data produced by moving objects using the notions of stops and moves w... | [['we', 'address', 'aggregate', 'queries', 'over', 'gis', 'data', 'and', 'moving', 'object', 'data', 'where', 'nonspatial', 'data', 'are', 'stored', 'in', 'a', 'data', 'warehouse', 'we', 'propose', 'a', 'formal', 'data', 'model', 'and', 'query', 'language', 'to', 'express', 'complex', 'aggregate', 'queries', 'next', 'w... | [-0.12347207494111409, 0.07683875308766101, -0.08990236690554482, 0.11807074352915291, -0.1279056544836539, -0.13525715348525688, 0.10810282821218536, 0.42737106746062636, -0.34434230199370247, -0.33774023298890543, 0.09727295904303901, -0.3256569550498031, -0.05354217877790619, 0.13718695316884594, -0.1230389567253251... |
708.2718 | CPD-20 1123 (Albus 1) is a bright He-B Subdwarf | Based on photometric and astrometric data it has been proposed that Albus 1
(also known as CPD-20 1123) might be a hot white dwarf similar to G191-B2B or,
alternatively, a hot subdwarf. We obtained a series of optical spectra showing
that CPD-20 1123 is a bright He-B subdwarf. We analyzed the HI Balmer and HeI
line s... | astro-ph | based on photometric and astrometric data it has been proposed that albus 1 also known as cpd20 1123 might be a hot white dwarf similar to g191b2b or alternatively a hot subdwarf we obtained a series of optical spectra showing that cpd20 1123 is a bright heb subdwarf we analyzed the hi balmer and hei line spectra and m... | [['based', 'on', 'photometric', 'and', 'astrometric', 'data', 'it', 'has', 'been', 'proposed', 'that', 'albus', '1', 'also', 'known', 'as', 'cpd20', '1123', 'might', 'be', 'a', 'hot', 'white', 'dwarf', 'similar', 'to', 'g191b2b', 'or', 'alternatively', 'a', 'hot', 'subdwarf', 'we', 'obtained', 'a', 'series', 'of', 'opt... | [-0.053434392204508185, 0.1133935494387212, -0.1114913630153751, 0.0815708725337269, -0.14902850568372136, -0.126585010123866, 0.11177096733202536, 0.43945716771607596, -0.14093643675247827, -0.31234702066285536, 0.08501631484978134, -0.3334269991610199, -0.046963200848646615, 0.20954242363829204, -0.11980957478711692,... |
708.2719 | The Stellar Populations of Praesepe and Coma Berenices | We present the results of a stellar membership survey of the nearby open
clusters Praesepe and Coma Berenices. We have combined archival survey data
from the SDSS, 2MASS, USNOB1.0, and UCAC-2.0 surveys to compile proper motions
and photometry for ~5 million sources over 300 deg^2. Of these sources, 1010
stars in Prae... | astro-ph | we present the results of a stellar membership survey of the nearby open clusters praesepe and coma berenices we have combined archival survey data from the sdss 2mass usnob10 and ucac20 surveys to compile proper motions and photometry for 5 million sources over 300 deg2 of these sources 1010 stars in praesepe and 98 s... | [['we', 'present', 'the', 'results', 'of', 'a', 'stellar', 'membership', 'survey', 'of', 'the', 'nearby', 'open', 'clusters', 'praesepe', 'and', 'coma', 'berenices', 'we', 'have', 'combined', 'archival', 'survey', 'data', 'from', 'the', 'sdss', '2mass', 'usnob10', 'and', 'ucac20', 'surveys', 'to', 'compile', 'proper', ... | [-0.07784658370362667, 0.11499140775751669, -0.08935616678529412, 0.12069728376719263, -0.1024409248782394, -0.020894684527401428, 0.10334110865098706, 0.4293764914176607, -0.10954021875608475, -0.427519051289518, 0.026095649280292958, -0.29363868740394483, -0.0022453548381729557, 0.19554538225264165, -0.09908342715930... |
708.272 | Simulating binary neutron stars: dynamics and gravitational waves | We model two mergers of orbiting binary neutron stars, the first forming a
black hole and the second a differentially rotating neutron star. We extract
gravitational waveforms in the wave zone. Comparisons to a post-Newtonian
analysis allow us to compute the orbital kinematics, including trajectories and
orbital ecce... | gr-qc astro-ph | we model two mergers of orbiting binary neutron stars the first forming a black hole and the second a differentially rotating neutron star we extract gravitational waveforms in the wave zone comparisons to a postnewtonian analysis allow us to compute the orbital kinematics including trajectories and orbital eccentricit... | [['we', 'model', 'two', 'mergers', 'of', 'orbiting', 'binary', 'neutron', 'stars', 'the', 'first', 'forming', 'a', 'black', 'hole', 'and', 'the', 'second', 'a', 'differentially', 'rotating', 'neutron', 'star', 'we', 'extract', 'gravitational', 'waveforms', 'in', 'the', 'wave', 'zone', 'comparisons', 'to', 'a', 'postnew... | [-0.146830693356848, 0.07971213423879817, -0.11921003266858558, 0.10143266732338815, -0.11878644270279134, -0.09586736674342926, 0.014582443480806735, 0.3285967973138516, -0.20078707475913687, -0.30697443288130066, 0.051598787099161804, -0.2839359424814271, -0.07627134727857386, 0.19023525009009365, -0.0051068258103138... |
708.2721 | Directed random growth models on the plane | This is a brief survey of laws of large numbers, fluctuation results and
large deviation principles for asymmetric interacting particle systems that
represent moving interfaces on the plane. We discuss the exclusion process, the
Hammersley process and the related last-passage growth models.
| math.PR | this is a brief survey of laws of large numbers fluctuation results and large deviation principles for asymmetric interacting particle systems that represent moving interfaces on the plane we discuss the exclusion process the hammersley process and the related lastpassage growth models | [['this', 'is', 'a', 'brief', 'survey', 'of', 'laws', 'of', 'large', 'numbers', 'fluctuation', 'results', 'and', 'large', 'deviation', 'principles', 'for', 'asymmetric', 'interacting', 'particle', 'systems', 'that', 'represent', 'moving', 'interfaces', 'on', 'the', 'plane', 'we', 'discuss', 'the', 'exclusion', 'process... | [-0.1489231221466547, 0.16670709122194066, -0.10466993498128085, 0.12626986592840694, -0.05722477808151217, -0.10711868052991728, 0.06324495144751079, 0.28666350799834445, -0.28198095894463004, -0.26668421799937886, 0.12325815661876861, -0.32328947391804486, -0.13663895396027892, 0.20138768689052777, -0.014655317423776... |
708.2722 | Kappa-symmetric SL(2,R) covariant D-brane actions | A superspace formulation of IIB supergravity which includes the field
strengths of the duals of the usual physical one, three and five-form field
strengths as well as the eleven-form field strength is given. The
superembedding formalism is used to construct kappa-symmetric SL(2,R) covariant
D-brane actions in an arbi... | hep-th | a superspace formulation of iib supergravity which includes the field strengths of the duals of the usual physical one three and fiveform field strengths as well as the elevenform field strength is given the superembedding formalism is used to construct kappasymmetric sl2r covariant dbrane actions in an arbitrary super... | [['a', 'superspace', 'formulation', 'of', 'iib', 'supergravity', 'which', 'includes', 'the', 'field', 'strengths', 'of', 'the', 'duals', 'of', 'the', 'usual', 'physical', 'one', 'three', 'and', 'fiveform', 'field', 'strengths', 'as', 'well', 'as', 'the', 'elevenform', 'field', 'strength', 'is', 'given', 'the', 'superem... | [-0.13746752624152875, 0.12947475464749672, -0.0052918367353933194, 0.1015092550197198, -0.14204780833453548, -0.14970790194727632, -0.10085249981101678, 0.3072452535187559, -0.1208593837004535, -0.25469254442889777, 0.054301539324319026, -0.18016359894251338, -0.1704582575689621, 0.1024263289433961, -0.093335840052792... |
708.2723 | Characterizing Temporal Distinguishability of an N-Photon State by
Generalized Photon Bunching Effect with Multi-Photon Interference | The complementary principle of quantum mechanics relates qualitatively the
visibility of quantum interference with path indistinguishability. Here we
propose a scheme of constructive quantum interference involving superposition
between an $N$-photon state and a single-photon state to characterize
quantitatively the d... | quant-ph | the complementary principle of quantum mechanics relates qualitatively the visibility of quantum interference with path indistinguishability here we propose a scheme of constructive quantum interference involving superposition between an nphoton state and a singlephoton state to characterize quantitatively the degree o... | [['the', 'complementary', 'principle', 'of', 'quantum', 'mechanics', 'relates', 'qualitatively', 'the', 'visibility', 'of', 'quantum', 'interference', 'with', 'path', 'indistinguishability', 'here', 'we', 'propose', 'a', 'scheme', 'of', 'constructive', 'quantum', 'interference', 'involving', 'superposition', 'between',... | [-0.14802981164436513, 0.1873362764584753, -0.16986021391280434, 0.06936834673123325, -0.02125793125699548, -0.21270135620280223, 0.08489037753315642, 0.35812149243429303, -0.28843853561728094, -0.2536322434350629, -0.05308876861133339, -0.22157711936982677, -0.1543960830415873, 0.19100790793377467, -0.0813479399965966... |
708.2724 | Physical approaches to DNA sequencing and detection | With the continued improvement of sequencing technologies, the prospect of
genome-based medicine is now at the forefront of scientific research. To
realize this potential, however, we need a revolutionary sequencing method for
the cost-effective and rapid interrogation of individual genomes. This
capability is likely... | physics.bio-ph cond-mat.soft q-bio.BM | with the continued improvement of sequencing technologies the prospect of genomebased medicine is now at the forefront of scientific research to realize this potential however we need a revolutionary sequencing method for the costeffective and rapid interrogation of individual genomes this capability is likely to be pr... | [['with', 'the', 'continued', 'improvement', 'of', 'sequencing', 'technologies', 'the', 'prospect', 'of', 'genomebased', 'medicine', 'is', 'now', 'at', 'the', 'forefront', 'of', 'scientific', 'research', 'to', 'realize', 'this', 'potential', 'however', 'we', 'need', 'a', 'revolutionary', 'sequencing', 'method', 'for', ... | [-0.06561067342623382, 0.12638056641934733, -0.04317215455597953, 0.03154151225830183, -0.057942588303826356, -0.15394900786861973, 0.0715834091294949, 0.40112145794065374, -0.30240170851741965, -0.29905299111698314, 0.09124881373718381, -0.2622916837844777, -0.1562056728454895, 0.23030402129791727, -0.0683715951408406... |
708.2725 | Hochschild cohomology and Atiyah classes | In this paper we prove that on a smooth algebraic variety the HKR-morphism
twisted by the square root of the Todd genus gives an isomorphism between the
sheaf of poly-vector fields and the sheaf of poly-differential operators, both
considered as derived Gerstenhaber algebras. In particular we obtain an
isomorphism be... | math.KT math.QA | in this paper we prove that on a smooth algebraic variety the hkrmorphism twisted by the square root of the todd genus gives an isomorphism between the sheaf of polyvector fields and the sheaf of polydifferential operators both considered as derived gerstenhaber algebras in particular we obtain an isomorphism between h... | [['in', 'this', 'paper', 'we', 'prove', 'that', 'on', 'a', 'smooth', 'algebraic', 'variety', 'the', 'hkrmorphism', 'twisted', 'by', 'the', 'square', 'root', 'of', 'the', 'todd', 'genus', 'gives', 'an', 'isomorphism', 'between', 'the', 'sheaf', 'of', 'polyvector', 'fields', 'and', 'the', 'sheaf', 'of', 'polydifferential... | [-0.1947510469911563, 0.029611170592887696, -0.0791959004495673, 0.09874770097786142, -0.1510468502267625, -0.09286807421879957, -0.0653664875972769, 0.3288053511356821, -0.36187056720028726, -0.26723828375795666, 0.07299514823802272, -0.1667456447374912, -0.1865890461889723, 0.21725800919479557, -0.1837124622198848, -... |
708.2726 | Large Scale B-Field in Stationary Accretion Disks | We reconsider the problem of the formation of a large-scale magnetic field in
the accretion disks around black holes. In contrast with previous work we take
into account the nonuniform vertical structure of the disk. The high electrical
conductivity of the outer layers of the disk prevents the outward diffusion of
th... | astro-ph | we reconsider the problem of the formation of a largescale magnetic field in the accretion disks around black holes in contrast with previous work we take into account the nonuniform vertical structure of the disk the high electrical conductivity of the outer layers of the disk prevents the outward diffusion of the mag... | [['we', 'reconsider', 'the', 'problem', 'of', 'the', 'formation', 'of', 'a', 'largescale', 'magnetic', 'field', 'in', 'the', 'accretion', 'disks', 'around', 'black', 'holes', 'in', 'contrast', 'with', 'previous', 'work', 'we', 'take', 'into', 'account', 'the', 'nonuniform', 'vertical', 'structure', 'of', 'the', 'disk',... | [-0.1811178847724064, 0.09237207679755309, -0.024454997048120607, 0.03374779075777231, -0.0658160343330789, 0.007050065293472695, 0.0073133129868414495, 0.33478114507221557, -0.2596158338166386, -0.30340117649719506, 0.06316971319407079, -0.22333609929547174, -0.03662935371038976, 0.1600929515847525, -0.020740575846526... |
708.2727 | Limits and C*-algebras of low rank or dimension | We explore various limit constructions for C*-algebras, such as composition
series and inverse limits, in relation to the notions of real rank, stable
rank, and extremal richness. We also consider extensions and pullbacks. We
identify some conditions under which the constructions preserve low rank for
the C*-algebras... | math.OA | we explore various limit constructions for calgebras such as composition series and inverse limits in relation to the notions of real rank stable rank and extremal richness we also consider extensions and pullbacks we identify some conditions under which the constructions preserve low rank for the calgebras or their mu... | [['we', 'explore', 'various', 'limit', 'constructions', 'for', 'calgebras', 'such', 'as', 'composition', 'series', 'and', 'inverse', 'limits', 'in', 'relation', 'to', 'the', 'notions', 'of', 'real', 'rank', 'stable', 'rank', 'and', 'extremal', 'richness', 'we', 'also', 'consider', 'extensions', 'and', 'pullbacks', 'we'... | [-0.08401579156086064, 0.11534701031147658, -0.0643831505170227, 0.13016510277014712, -0.06915475976774874, -0.16722806193190964, -0.014386933803916032, 0.3683189709495375, -0.335607194415955, -0.18851906833225401, 0.19361035928950118, -0.25879354218183004, -0.1644064959972098, 0.1882750984531004, -0.12151619138709013,... |
708.2728 | Gravitational wave radiometry: Mapping a stochastic gravitational wave
background | The problem of the detection and mapping of a stochastic gravitational wave
background (SGWB), either of cosmological or astrophysical origin, bears a
strong semblance to the analysis of CMB anisotropy and polarization. The basic
statistic we use is the cross-correlation between the data from a pair of
detectors. In ... | gr-qc astro-ph | the problem of the detection and mapping of a stochastic gravitational wave background sgwb either of cosmological or astrophysical origin bears a strong semblance to the analysis of cmb anisotropy and polarization the basic statistic we use is the crosscorrelation between the data from a pair of detectors in order to ... | [['the', 'problem', 'of', 'the', 'detection', 'and', 'mapping', 'of', 'a', 'stochastic', 'gravitational', 'wave', 'background', 'sgwb', 'either', 'of', 'cosmological', 'or', 'astrophysical', 'origin', 'bears', 'a', 'strong', 'semblance', 'to', 'the', 'analysis', 'of', 'cmb', 'anisotropy', 'and', 'polarization', 'the', ... | [-0.1071528337868173, 0.05085118163943327, -0.09237187899316775, 0.10362009348786613, -0.07755979999889477, -0.059079290213596536, 0.005025409160313442, 0.38033020918752625, -0.24623135771069218, -0.2991969663905998, 0.08439827013023364, -0.3343434597739472, -0.11911149210141639, 0.23615622956593102, 0.0266683106795368... |
708.2729 | The Mid-Infrared Spectrum of the Short Orbital Period Polar EF Eridani
from the Spitzer Space Telescope | We present the first mid-infrared (5.5-14.5 micron) spectrum of a highly
magnetic cataclysmic variable, EF Eridani, obtained with the Infrared
Spectrograph on the Spitzer Space Telescope. The spectrum displays a relatively
flat, featureless continuum. A spectral energy distribution model consisting of
a 9500 K white ... | astro-ph | we present the first midinfrared 55145 micron spectrum of a highly magnetic cataclysmic variable ef eridani obtained with the infrared spectrograph on the spitzer space telescope the spectrum displays a relatively flat featureless continuum a spectral energy distribution model consisting of a 9500 k white dwarf l5 seco... | [['we', 'present', 'the', 'first', 'midinfrared', '55145', 'micron', 'spectrum', 'of', 'a', 'highly', 'magnetic', 'cataclysmic', 'variable', 'ef', 'eridani', 'obtained', 'with', 'the', 'infrared', 'spectrograph', 'on', 'the', 'spitzer', 'space', 'telescope', 'the', 'spectrum', 'displays', 'a', 'relatively', 'flat', 'fe... | [-0.08054094532203368, 0.11907844696040282, -0.09145567707053166, 0.08500471187204205, -0.0917633960591903, -0.12614917334319806, 0.04181052138986107, 0.4592885599088143, -0.15251209065044188, -0.3156678806331269, 0.02438071135410984, -0.30158704871257, -0.0011769644676378982, 0.16324574201580083, -0.0578360533059715, ... |
708.273 | Magnetic Field Estimation at and beyond 1/N Scaling via an Effective
Nonlinearity | We provide evidence, based on direct simulation of the quantum Fisher
information, that 1/N scaling of the sensitivity with the number of atoms N in
an atomic magnetometer can be surpassed by double-passing a far-detuned laser
through the atomic system during Larmor precession. Furthermore, we predict
that for N>>1, ... | quant-ph | we provide evidence based on direct simulation of the quantum fisher information that 1n scaling of the sensitivity with the number of atoms n in an atomic magnetometer can be surpassed by doublepassing a fardetuned laser through the atomic system during larmor precession furthermore we predict that for n1 the proposed... | [['we', 'provide', 'evidence', 'based', 'on', 'direct', 'simulation', 'of', 'the', 'quantum', 'fisher', 'information', 'that', '1n', 'scaling', 'of', 'the', 'sensitivity', 'with', 'the', 'number', 'of', 'atoms', 'n', 'in', 'an', 'atomic', 'magnetometer', 'can', 'be', 'surpassed', 'by', 'doublepassing', 'a', 'fardetuned... | [-0.13422348450474214, 0.21073570505519235, -0.04918345467497905, -0.030604775882128513, 0.024598680239057903, -0.13674975959160787, 0.09739143780616084, 0.3825962779457878, -0.21219022482436037, -0.3258931510376208, 0.02828888633732938, -0.27560442320607376, -0.07227441347839142, 0.2285025960229563, 0.0126566088786630... |
708.2731 | CKM matrix fits including constraints on New Physics | I review the status of global fits to the CKM matrix within the framework of
the Standard Model and also allowing for New Physics contributions in B-Bbar
mixing. The driving force is coming from the large data sets collected by the
B-factory experiments BABAR and Belle. Additional important inputs to the B_s
sector a... | hep-ph | i review the status of global fits to the ckm matrix within the framework of the standard model and also allowing for new physics contributions in bbbar mixing the driving force is coming from the large data sets collected by the bfactory experiments babar and belle additional important inputs to the b_s sector are pro... | [['i', 'review', 'the', 'status', 'of', 'global', 'fits', 'to', 'the', 'ckm', 'matrix', 'within', 'the', 'framework', 'of', 'the', 'standard', 'model', 'and', 'also', 'allowing', 'for', 'new', 'physics', 'contributions', 'in', 'bbbar', 'mixing', 'the', 'driving', 'force', 'is', 'coming', 'from', 'the', 'large', 'data',... | [-0.011529224657121745, 0.18594251984152302, -0.08484446887868917, 0.10614884622534201, -0.09889977247636209, -0.13421221209111914, 0.07252776293062616, 0.2416941224030037, -0.2273008019031807, -0.2748001049508223, 0.02105680771236276, -0.3992064377271581, -0.036667882454121246, 0.18439160760267284, 0.05251742656149998... |
708.2732 | Secrecy Capacity Region of Binary and Gaussian Multiple Access Channels | A generalized multiple access channel (GMAC) with one confidential message
set is studied, where two users (users 1 and 2) attempt to transmit common
information to a destination, and user 1 also has confidential information
intended for the destination. Moreover, user 1 wishes to keep its confidential
information as... | cs.IT math.IT | a generalized multiple access channel gmac with one confidential message set is studied where two users users 1 and 2 attempt to transmit common information to a destination and user 1 also has confidential information intended for the destination moreover user 1 wishes to keep its confidential information as secret as... | [['a', 'generalized', 'multiple', 'access', 'channel', 'gmac', 'with', 'one', 'confidential', 'message', 'set', 'is', 'studied', 'where', 'two', 'users', 'users', '1', 'and', '2', 'attempt', 'to', 'transmit', 'common', 'information', 'to', 'a', 'destination', 'and', 'user', '1', 'also', 'has', 'confidential', 'informat... | [-0.2242139764960007, -0.007597995025225648, 0.012272077188412151, 0.08190369956647184, -0.10926167583000837, -0.3731958524019706, 0.1691504399347497, 0.386570556660985, -0.31661276762733365, -0.20795833753735418, 0.12997306399692846, -0.35541593721413084, -0.06695507769011846, 0.08657557456431413, -0.10713456504826092... |
708.2733 | Secure Communications over Fading Channels | The fading wire-tap channel is investigated, where the source-to-destination
channel and the source-to-wire-tapper channel are corrupted by multiplicative
fading gain coefficients in addition to additive Gaussian noise terms. The
channel state information is assumed to be known at both the transmitter and
the receive... | cs.IT math.IT | the fading wiretap channel is investigated where the sourcetodestination channel and the sourcetowiretapper channel are corrupted by multiplicative fading gain coefficients in addition to additive gaussian noise terms the channel state information is assumed to be known at both the transmitter and the receiver the para... | [['the', 'fading', 'wiretap', 'channel', 'is', 'investigated', 'where', 'the', 'sourcetodestination', 'channel', 'and', 'the', 'sourcetowiretapper', 'channel', 'are', 'corrupted', 'by', 'multiplicative', 'fading', 'gain', 'coefficients', 'in', 'addition', 'to', 'additive', 'gaussian', 'noise', 'terms', 'the', 'channel'... | [-0.29311064549353943, 0.035217045202015844, -0.027421759116705975, 0.0013277813647443256, -0.06540051745172559, -0.359844447747499, 0.1366139556390836, 0.3714390047551954, -0.34082743605332716, -0.19191283492387093, 0.13287462511964673, -0.21947409290851666, -0.07599311843005736, 0.07875208346615349, -0.14658026453577... |
708.2734 | Universal properties of a trapped two-component Fermi gas at unitarity | We treat the trapped two-component Fermi system, in which unlike fermions
interact through a two-body short-range potential having no bound state but an
infinite scattering length. By accurately solving the Schroedinger equation for
up to N=6 fermions, we show that no many-body bound states exist other than
those bou... | cond-mat.other | we treat the trapped twocomponent fermi system in which unlike fermions interact through a twobody shortrange potential having no bound state but an infinite scattering length by accurately solving the schroedinger equation for up to n6 fermions we show that no manybody bound states exist other than those bound by the ... | [['we', 'treat', 'the', 'trapped', 'twocomponent', 'fermi', 'system', 'in', 'which', 'unlike', 'fermions', 'interact', 'through', 'a', 'twobody', 'shortrange', 'potential', 'having', 'no', 'bound', 'state', 'but', 'an', 'infinite', 'scattering', 'length', 'by', 'accurately', 'solving', 'the', 'schroedinger', 'equation'... | [-0.14082988856630138, 0.1879129510247214, -0.0961525230189768, 0.09835606644682969, -0.011638898915985477, -0.19776994464744893, 0.05517040983617097, 0.3513510047989053, -0.1931326079800307, -0.2948822527253461, -0.002524671468461611, -0.34000071834459483, -0.1121299489549248, 0.20366385484793742, 0.08297638964913263,... |
708.2735 | Long range forces and limits on unparticle interactions | Couplings between standard model particles and unparticles from a nontrivial
scale invariant sector can lead to long range forces. If the forces couple to
quantities such as baryon or lepton (electron) number, stringent limits result
from tests of the gravitational inverse square law. These limits are much
stronger t... | hep-ph | couplings between standard model particles and unparticles from a nontrivial scale invariant sector can lead to long range forces if the forces couple to quantities such as baryon or lepton electron number stringent limits result from tests of the gravitational inverse square law these limits are much stronger than fro... | [['couplings', 'between', 'standard', 'model', 'particles', 'and', 'unparticles', 'from', 'a', 'nontrivial', 'scale', 'invariant', 'sector', 'can', 'lead', 'to', 'long', 'range', 'forces', 'if', 'the', 'forces', 'couple', 'to', 'quantities', 'such', 'as', 'baryon', 'or', 'lepton', 'electron', 'number', 'stringent', 'li... | [-0.0665467775909713, 0.289592315149666, -0.054655337533741084, 0.1830995719603918, -0.13803804455393995, -0.16562414291332028, 0.010677444998657814, 0.2522471244274466, -0.2673307686733703, -0.38486353699462833, 0.03832391440799391, -0.33465886172079656, -0.026678396220732894, 0.2365251837074067, 0.08960608935363039, ... |
708.2736 | Eulerian conjugate stress and strain | New results are presented for the stress conjugate to arbitrary Eulerian
strain measures. The conjugate stress depends on two arbitrary quantities: the
strain measure f(V) and the corotational rate defined by the spin \Omega. It is
shown that for every choice of f there is a unique spin, called the f-spin,
which make... | cond-mat.mtrl-sci | new results are presented for the stress conjugate to arbitrary eulerian strain measures the conjugate stress depends on two arbitrary quantities the strain measure fv and the corotational rate defined by the spin omega it is shown that for every choice of f there is a unique spin called the fspin which makes the conju... | [['new', 'results', 'are', 'presented', 'for', 'the', 'stress', 'conjugate', 'to', 'arbitrary', 'eulerian', 'strain', 'measures', 'the', 'conjugate', 'stress', 'depends', 'on', 'two', 'arbitrary', 'quantities', 'the', 'strain', 'measure', 'fv', 'and', 'the', 'corotational', 'rate', 'defined', 'by', 'the', 'spin', 'omeg... | [-0.15561594822432476, 0.14089103158147745, -0.07011459393750046, 0.03178705384739298, -0.07770265805080903, -0.09362636745930457, -0.03494571781912549, 0.33028472916892737, -0.32526443278309236, -0.22315735785552293, 0.06619023079627909, -0.271166089968371, -0.16458305832160222, 0.1802305470380455, -0.0432178014504515... |
708.2737 | Extragalaxtic Stellar Astronomy | Despite their paucity, massive hot stars are real cosmic engines of
fundamental importance in shaping our Universe, from its very early stages up
to its current appearance. Understanding the physics of massive stars is then a
key issue for many relevant astrophysical phenomena. Probing the massive
stellar population ... | astro-ph | despite their paucity massive hot stars are real cosmic engines of fundamental importance in shaping our universe from its very early stages up to its current appearance understanding the physics of massive stars is then a key issue for many relevant astrophysical phenomena probing the massive stellar population of nea... | [['despite', 'their', 'paucity', 'massive', 'hot', 'stars', 'are', 'real', 'cosmic', 'engines', 'of', 'fundamental', 'importance', 'in', 'shaping', 'our', 'universe', 'from', 'its', 'very', 'early', 'stages', 'up', 'to', 'its', 'current', 'appearance', 'understanding', 'the', 'physics', 'of', 'massive', 'stars', 'is', ... | [-0.050629897433152236, 0.10430099866685591, -0.08905591564875083, 0.11621057122725428, -0.15720432713195415, -0.017832149298296178, 0.040890235917426514, 0.3744210232481627, -0.1758013429186706, -0.3754524258298001, 0.05423626082483679, -0.2778438542343013, -0.08379602343172467, 0.2510214606702448, -0.0426673076290171... |
708.2738 | The Physical Process First Law for Bifurcate Killing Horizons | The physical process version of the first law for black holes states that the
passage of energy and angular momentum through the horizon results in a change
in area $\frac{\kappa}{8 \pi} \Delta A = \Delta E - \Omega \Delta J$, so long
as this passage is quasi-stationary. A similar physical process first law can
be de... | gr-qc hep-th | the physical process version of the first law for black holes states that the passage of energy and angular momentum through the horizon results in a change in area frackappa8 pi delta a delta e omega delta j so long as this passage is quasistationary a similar physical process first law can be derived for any bifurcat... | [['the', 'physical', 'process', 'version', 'of', 'the', 'first', 'law', 'for', 'black', 'holes', 'states', 'that', 'the', 'passage', 'of', 'energy', 'and', 'angular', 'momentum', 'through', 'the', 'horizon', 'results', 'in', 'a', 'change', 'in', 'area', 'frackappa8', 'pi', 'delta', 'a', 'delta', 'e', 'omega', 'delta', ... | [-0.14503199628088623, 0.1478921251378051, -0.09410832639783621, 0.08839384888540736, -0.06773190713254734, -0.1801328224968165, 0.03162908937782049, 0.3137154038622975, -0.22634101071977056, -0.27625286486931144, 0.1152157643440296, -0.2836594485770911, -0.10336158997262829, 0.18467737923027017, -0.06721954408800229, ... |
708.2739 | Stabilization of an overloaded queueing network using measurement-based
admission control | Admission control can be employed to avoid congestion in queueing networks
subject to overload. In distributed networks the admission decisions are often
based on imperfect measurements on the network state. This paper studies how
the lack of complete state information affects the system performance by
considering a ... | math.PR | admission control can be employed to avoid congestion in queueing networks subject to overload in distributed networks the admission decisions are often based on imperfect measurements on the network state this paper studies how the lack of complete state information affects the system performance by considering a simp... | [['admission', 'control', 'can', 'be', 'employed', 'to', 'avoid', 'congestion', 'in', 'queueing', 'networks', 'subject', 'to', 'overload', 'in', 'distributed', 'networks', 'the', 'admission', 'decisions', 'are', 'often', 'based', 'on', 'imperfect', 'measurements', 'on', 'the', 'network', 'state', 'this', 'paper', 'stud... | [-0.20761787510241153, 0.034831801792243856, -0.05923809724642182, 0.043991566842796835, -0.08484428463951237, -0.18884572329894675, 0.14065173016286564, 0.4129602795878014, -0.28504918997067136, -0.2981814143864752, 0.14508445617476745, -0.225280082585024, -0.17868287495621663, 0.1622891448311169, -0.19184181514209706... |
708.274 | Galactic Edge Clouds I: Molecular Line Observations and Chemical
Modelling of Edge Cloud 2 | Edge Cloud 2 (EC2) is a molecular cloud, about 35 pc in size, with one of the
largest galactocentric distances known to exist in the Milky Way. We present
observations of a peak CO emission region in the cloud and use these to
determine its physical characteristics. We calculate a gas temperature of 20 K
and a densit... | astro-ph | edge cloud 2 ec2 is a molecular cloud about 35 pc in size with one of the largest galactocentric distances known to exist in the milky way we present observations of a peak co emission region in the cloud and use these to determine its physical characteristics we calculate a gas temperature of 20 k and a density of nh2... | [['edge', 'cloud', '2', 'ec2', 'is', 'a', 'molecular', 'cloud', 'about', '35', 'pc', 'in', 'size', 'with', 'one', 'of', 'the', 'largest', 'galactocentric', 'distances', 'known', 'to', 'exist', 'in', 'the', 'milky', 'way', 'we', 'present', 'observations', 'of', 'a', 'peak', 'co', 'emission', 'region', 'in', 'the', 'clou... | [-0.07204425720603115, 0.1028527471386159, -0.044283267468952225, 0.08206889901550547, -0.011676257992300638, -0.043802127706207235, 0.07081465808618899, 0.40819244522790205, -0.184784649618073, -0.3725394931651892, 0.03625507368373552, -0.27144221579580896, -0.011042651671156865, 0.16714391015493632, -0.03823087826153... |
708.2741 | Schwarzschild-Couder two-mirror telescope for ground-based gamma-ray
astronomy | Schwarzschild-type aplanatic telescopes with two aspheric mirrors, configured
to correct spherical and coma aberrations, are considered for application in
gamma-ray astronomy utilizing the ground-based atmospheric Cherenkov technique.
We use analytical descriptions for the figures of primary and secondary mirrors
and... | astro-ph | schwarzschildtype aplanatic telescopes with two aspheric mirrors configured to correct spherical and coma aberrations are considered for application in gammaray astronomy utilizing the groundbased atmospheric cherenkov technique we use analytical descriptions for the figures of primary and secondary mirrors and by mean... | [['schwarzschildtype', 'aplanatic', 'telescopes', 'with', 'two', 'aspheric', 'mirrors', 'configured', 'to', 'correct', 'spherical', 'and', 'coma', 'aberrations', 'are', 'considered', 'for', 'application', 'in', 'gammaray', 'astronomy', 'utilizing', 'the', 'groundbased', 'atmospheric', 'cherenkov', 'technique', 'we', 'u... | [-0.07627561219246126, 0.1085801811888814, -0.04984551455639303, 0.06693547657877207, -0.11749458234384656, -0.17931373180262744, -0.056929652653634547, 0.46702457624673843, -0.17776430820673705, -0.40287697795033456, 0.1361595235010609, -0.30713886916637423, -0.13153579878248275, 0.2921209602337331, -0.105177047987002... |
708.2742 | The Gamma-ray Albedo of the Moon | We use the GEANT4 Monte Carlo framework to calculate the gamma-ray albedo of
the Moon due to interactions of cosmic ray (CR) nuclei with moon rock. Our
calculation of the albedo spectrum agrees with the EGRET data. We show that the
spectrum of gamma rays from the Moon is very steep with an effective cutoff
around 3-4... | astro-ph | we use the geant4 monte carlo framework to calculate the gammaray albedo of the moon due to interactions of cosmic ray cr nuclei with moon rock our calculation of the albedo spectrum agrees with the egret data we show that the spectrum of gamma rays from the moon is very steep with an effective cutoff around 34 gev 600... | [['we', 'use', 'the', 'geant4', 'monte', 'carlo', 'framework', 'to', 'calculate', 'the', 'gammaray', 'albedo', 'of', 'the', 'moon', 'due', 'to', 'interactions', 'of', 'cosmic', 'ray', 'cr', 'nuclei', 'with', 'moon', 'rock', 'our', 'calculation', 'of', 'the', 'albedo', 'spectrum', 'agrees', 'with', 'the', 'egret', 'data... | [-0.0392749851689095, 0.19892320531659796, -0.07893262771173246, 0.1671796732001124, -0.10277008968704329, -0.06600636560632428, 0.03592630335117212, 0.4015386670550986, -0.2290150621939484, -0.41237417583328645, 0.014099901511652715, -0.344541030931748, -0.0032271847510626454, 0.291855901660899, -0.0411860996643333, 0... |
708.2743 | The clock ambiguity and the emergence of physical laws | The process of identifying a time variable in time reparameterization
invariant theories results in great ambiguities about the actual laws of
physics described by a given theory. A theory set up to describe one set of
physical laws can equally well be interpreted as describing any other laws of
physics by making a d... | hep-th gr-qc | the process of identifying a time variable in time reparameterization invariant theories results in great ambiguities about the actual laws of physics described by a given theory a theory set up to describe one set of physical laws can equally well be interpreted as describing any other laws of physics by making a diff... | [['the', 'process', 'of', 'identifying', 'a', 'time', 'variable', 'in', 'time', 'reparameterization', 'invariant', 'theories', 'results', 'in', 'great', 'ambiguities', 'about', 'the', 'actual', 'laws', 'of', 'physics', 'described', 'by', 'a', 'given', 'theory', 'a', 'theory', 'set', 'up', 'to', 'describe', 'one', 'set'... | [-0.11068443530855794, 0.16214037469762843, -0.13555597816806575, 0.1027515215119741, -0.07613701295941115, -0.1517285185527975, 0.05541564421898358, 0.32964639489849407, -0.2960603638939117, -0.32592450642371423, 0.09311889235002571, -0.19314774903405, -0.18531088329709164, 0.17016949187156205, -0.0770922656358139, 0.... |
708.2744 | Nonlocal Lagrangians for Accelerated Systems | Acceleration-induced nonlocality and the corresponding Lorentz-invariant
nonlocal field equations of accelerated systems in Minkowski spacetime are
discussed. Under physically reasonable conditions, the nonlocal equation of
motion of the field can be derived from a variational principle of stationary
action involving... | hep-th gr-qc | accelerationinduced nonlocality and the corresponding lorentzinvariant nonlocal field equations of accelerated systems in minkowski spacetime are discussed under physically reasonable conditions the nonlocal equation of motion of the field can be derived from a variational principle of stationary action involving a non... | [['accelerationinduced', 'nonlocality', 'and', 'the', 'corresponding', 'lorentzinvariant', 'nonlocal', 'field', 'equations', 'of', 'accelerated', 'systems', 'in', 'minkowski', 'spacetime', 'are', 'discussed', 'under', 'physically', 'reasonable', 'conditions', 'the', 'nonlocal', 'equation', 'of', 'motion', 'of', 'the', ... | [-0.16530239297888982, 0.1586318065170557, -0.10480017247251593, 0.0825905478022133, -0.07689459109977366, -0.11822959002202903, -0.07591658638408169, 0.29833265998138064, -0.2691835682863035, -0.25987066295093453, 0.042175702593969897, -0.20351183569679657, -0.14537869854710805, 0.18644687541736624, -0.019282818604738... |
708.2745 | Measuring Type Ia Supernova Distances and Redshifts From Their
Multi-band Light Curves | The distance and redshift of a type Ia supernova can be determined
simultaneously through its multi-band light curves. This fact may be used for
imaging surveys that discover and obtain photometry for large numbers of
supernovae; so many that it would be difficult to obtain a spectroscopic
redshift for each. Using av... | astro-ph | the distance and redshift of a type ia supernova can be determined simultaneously through its multiband light curves this fact may be used for imaging surveys that discover and obtain photometry for large numbers of supernovae so many that it would be difficult to obtain a spectroscopic redshift for each using availabl... | [['the', 'distance', 'and', 'redshift', 'of', 'a', 'type', 'ia', 'supernova', 'can', 'be', 'determined', 'simultaneously', 'through', 'its', 'multiband', 'light', 'curves', 'this', 'fact', 'may', 'be', 'used', 'for', 'imaging', 'surveys', 'that', 'discover', 'and', 'obtain', 'photometry', 'for', 'large', 'numbers', 'of... | [-0.027092245284102416, 0.11935061176086248, -0.11644860162895414, 0.1235477743058225, -0.15443359560117886, -0.1467798032437361, 0.06780022918371864, 0.45690935806581573, -0.19778297998271482, -0.3269006560196079, 0.09351061672718335, -0.2910144566232839, -0.01157457336548075, 0.2605007221604327, -0.07006328866911096,... |
708.2746 | Neutron and X-ray Scattering Studies of the Lightly-Doped Spin-Peierls
System Cu(1-x)Cd(x)GeO3 | Single crystals of the lightly-doped spin-Peierls system Cu(1-x)Cd(x)GeO3
have been studied using bulk susceptibility, x-ray diffraction, and inelastic
neutron scattering techniques. We investigate the triplet gap in the magnetic
excitation spectrum of this quasi-one dimensional quantum antiferromagnet, and
its relat... | cond-mat.str-el | single crystals of the lightlydoped spinpeierls system cu1xcdxgeo3 have been studied using bulk susceptibility xray diffraction and inelastic neutron scattering techniques we investigate the triplet gap in the magnetic excitation spectrum of this quasione dimensional quantum antiferromagnet and its relation to the spin... | [['single', 'crystals', 'of', 'the', 'lightlydoped', 'spinpeierls', 'system', 'cu1xcdxgeo3', 'have', 'been', 'studied', 'using', 'bulk', 'susceptibility', 'xray', 'diffraction', 'and', 'inelastic', 'neutron', 'scattering', 'techniques', 'we', 'investigate', 'the', 'triplet', 'gap', 'in', 'the', 'magnetic', 'excitation'... | [-0.16097210543663348, 0.20247203250670112, -0.06572604103576998, 0.07360648549957807, -0.05023161841686382, -0.09078856574934582, 0.09373554942295562, 0.411997483046942, -0.28715216230904295, -0.2603350951617887, -0.019079692901361214, -0.3847131107089131, -0.09289986305859287, 0.12846266983759178, 0.14441345994858895... |
708.2747 | Aspects of Integrability in N =4 SYM | Various recently developed connections between supersymmetric Yang-Mills
theories in four dimensions and two dimensional integrable systems serve as
crucial ingredients in improving our understanding of the AdS/CFT
correspondence. In this review, we highlight some connections between
superconformal four dimensional Y... | hep-th | various recently developed connections between supersymmetric yangmills theories in four dimensions and two dimensional integrable systems serve as crucial ingredients in improving our understanding of the adscft correspondence in this review we highlight some connections between superconformal four dimensional yangmil... | [['various', 'recently', 'developed', 'connections', 'between', 'supersymmetric', 'yangmills', 'theories', 'in', 'four', 'dimensions', 'and', 'two', 'dimensional', 'integrable', 'systems', 'serve', 'as', 'crucial', 'ingredients', 'in', 'improving', 'our', 'understanding', 'of', 'the', 'adscft', 'correspondence', 'in', ... | [-0.12164691496765663, 0.17098760346592473, -0.05809784962740891, 0.112485065166995, -0.04846819498020561, -0.18310126524121195, -0.03863430703880594, 0.2934644519813171, -0.1541284573491381, -0.2417117700366178, 0.10192973595288653, -0.2832124801861326, -0.23879168489008767, 0.14928913579768494, -0.04095340237224929, ... |
708.2748 | Optical and dc transport properties of a strongly correlated charge
density wave system: exact solution in the ordered phase of the spinless
Falicov-Kimball model with dynamical mean-field theory | We derive the dynamical mean-field theory equations for transport in an
ordered charge-density-wave phase on a bipartite lattice. The formalism is
applied to the spinless Falicov-Kimball model on a hypercubic lattice at half
filling. We determine the many-body density of states, the dc charge and heat
conductivities,... | cond-mat.str-el | we derive the dynamical meanfield theory equations for transport in an ordered chargedensitywave phase on a bipartite lattice the formalism is applied to the spinless falicovkimball model on a hypercubic lattice at half filling we determine the manybody density of states the dc charge and heat conductivities and the op... | [['we', 'derive', 'the', 'dynamical', 'meanfield', 'theory', 'equations', 'for', 'transport', 'in', 'an', 'ordered', 'chargedensitywave', 'phase', 'on', 'a', 'bipartite', 'lattice', 'the', 'formalism', 'is', 'applied', 'to', 'the', 'spinless', 'falicovkimball', 'model', 'on', 'a', 'hypercubic', 'lattice', 'at', 'half',... | [-0.17208968225349963, 0.24627751566288225, -0.06171778666475802, 0.03789054976823536, -0.016652380239975173, -0.08431221795490274, 0.1293292099444443, 0.35199454316170886, -0.2679917859732086, -0.20986906776670367, 0.06449088826593652, -0.33866449461493175, -0.1275867630411085, 0.09037872888984566, 0.06989516115208971... |
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