id float64 706 1.8k | title stringlengths 1 343 | abstract stringlengths 6 6.09k | categories stringlengths 5 125 | processed_abstract stringlengths 2 5.96k | tokenized_abstract stringlengths 8 8.74k | centroid stringlengths 2.1k 2.17k |
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706.3014 | Bayesian Calibrated Significance Levels Applied to the Spectral Tilt and
Hemispherical Asymmetry | Bayesian model selection provides a formal method of determining the level of
support for new parameters in a model. However, if there is not a specific
enough underlying physical motivation for the new parameters it can be hard to
assign them meaningful priors, an essential ingredient of Bayesian model
selection. He... | astro-ph gr-qc hep-ph hep-th | bayesian model selection provides a formal method of determining the level of support for new parameters in a model however if there is not a specific enough underlying physical motivation for the new parameters it can be hard to assign them meaningful priors an essential ingredient of bayesian model selection here we ... | [['bayesian', 'model', 'selection', 'provides', 'a', 'formal', 'method', 'of', 'determining', 'the', 'level', 'of', 'support', 'for', 'new', 'parameters', 'in', 'a', 'model', 'however', 'if', 'there', 'is', 'not', 'a', 'specific', 'enough', 'underlying', 'physical', 'motivation', 'for', 'the', 'new', 'parameters', 'it'... | [-0.053308173832854, 0.09162582817165954, -0.09101163001455874, 0.12980413110291755, -0.14607535344125194, -0.1769609468417581, 0.11010488475757567, 0.3724513725885613, -0.21057379310738972, -0.3307833547471091, 0.10420749499250881, -0.25535561540799045, -0.09365391548278487, 0.20293522786179727, -0.0607142905048518, 0... |
706.3015 | Oxide spintronics | Concomitant with the development of metal-based spintronics in the late
1980's and 1990's, important advances were made on the growth of high-quality
oxide thin films and heterostructures. While this was at first motivated by the
discovery of high-temperature superconductivity in perovskite Cu oxides, this
technologi... | cond-mat.mtrl-sci cond-mat.str-el | concomitant with the development of metalbased spintronics in the late 1980s and 1990s important advances were made on the growth of highquality oxide thin films and heterostructures while this was at first motivated by the discovery of hightemperature superconductivity in perovskite cu oxides this technological breakt... | [['concomitant', 'with', 'the', 'development', 'of', 'metalbased', 'spintronics', 'in', 'the', 'late', '1980s', 'and', '1990s', 'important', 'advances', 'were', 'made', 'on', 'the', 'growth', 'of', 'highquality', 'oxide', 'thin', 'films', 'and', 'heterostructures', 'while', 'this', 'was', 'at', 'first', 'motivated', 'b... | [-0.1262050886909462, 0.17170548729181526, 0.041041411477258136, -0.005620873907881234, -0.08416088194143577, -0.16017689388957831, 0.04648583135096855, 0.4229152194743396, -0.1988815821922267, -0.3210135863796818, 0.06008484755398431, -0.3426577834504061, -0.19178190278754534, 0.2812081116322896, -0.014332719837745417... |
706.3016 | AC conductivity of graphene: from tight-binding model to 2+1-dimensional
quantum electrodynamics | We consider the relationship between the tight-binding Hamiltonian of the
two-dimensional honeycomb lattice of carbon atoms with nearest neighbor hopping
only and the 2+1 dimensional Hamiltonian of quantum electrodynamics which
follows in the continuum limit. We pay particular attention to the symmetries
of the free ... | cond-mat.mes-hall cond-mat.str-el hep-ph | we consider the relationship between the tightbinding hamiltonian of the twodimensional honeycomb lattice of carbon atoms with nearest neighbor hopping only and the 21 dimensional hamiltonian of quantum electrodynamics which follows in the continuum limit we pay particular attention to the symmetries of the free dirac ... | [['we', 'consider', 'the', 'relationship', 'between', 'the', 'tightbinding', 'hamiltonian', 'of', 'the', 'twodimensional', 'honeycomb', 'lattice', 'of', 'carbon', 'atoms', 'with', 'nearest', 'neighbor', 'hopping', 'only', 'and', 'the', '21', 'dimensional', 'hamiltonian', 'of', 'quantum', 'electrodynamics', 'which', 'fo... | [-0.17068209981080146, 0.1977890178231367, 0.014798450372957935, 0.02698119052996238, -0.07310194893119236, -0.14901011295150965, 0.07896800209418871, 0.3900456780878206, -0.24735162458382548, -0.22924047862179578, 0.05856597522215452, -0.2966861515073106, -0.1427457948642162, 0.10477101400028914, 0.030559079112329832,... |
706.3017 | Relativistic Three-Fermion Wave Equations in Reformulated QED and
Relativistic Effects in Muonium Minus | The variational method, within the Hamiltonian formalism of reformulated QED
is used to determine relativistic wave equations for a system of three fermions
of arbitrary mass interacting electromagnetically. The interaction kernels of
the equations are, in essence, the invariant $\mathcal{M}$ matrices in lowest
order... | physics.atom-ph physics.chem-ph | the variational method within the hamiltonian formalism of reformulated qed is used to determine relativistic wave equations for a system of three fermions of arbitrary mass interacting electromagnetically the interaction kernels of the equations are in essence the invariant mathcalm matrices in lowest order the equati... | [['the', 'variational', 'method', 'within', 'the', 'hamiltonian', 'formalism', 'of', 'reformulated', 'qed', 'is', 'used', 'to', 'determine', 'relativistic', 'wave', 'equations', 'for', 'a', 'system', 'of', 'three', 'fermions', 'of', 'arbitrary', 'mass', 'interacting', 'electromagnetically', 'the', 'interaction', 'kerne... | [-0.11230317898569446, 0.1654355615404818, -0.03390873934361426, 0.13437555053992672, 0.00948300731697065, -0.12594857895472908, -0.03363899217790687, 0.30482120749851066, -0.20717485819705853, -0.31809023908092915, -0.0036550607354215838, -0.3058317150902368, -0.01869963658699656, 0.15234134402171726, 0.08155373453194... |
706.3018 | Tomographic Representation of Minisuperspace Quantum Cosmology and
Noether Symmetries | The probability representation, in which cosmological quantum states are
described by a standard positive probability distribution, is constructed for
minisuperspace models selected by Noether symmetries. In such a case, the
tomographic probability distribution provides the classical evolution for the
models and can ... | gr-qc hep-th | the probability representation in which cosmological quantum states are described by a standard positive probability distribution is constructed for minisuperspace models selected by noether symmetries in such a case the tomographic probability distribution provides the classical evolution for the models and can be con... | [['the', 'probability', 'representation', 'in', 'which', 'cosmological', 'quantum', 'states', 'are', 'described', 'by', 'a', 'standard', 'positive', 'probability', 'distribution', 'is', 'constructed', 'for', 'minisuperspace', 'models', 'selected', 'by', 'noether', 'symmetries', 'in', 'such', 'a', 'case', 'the', 'tomogr... | [-0.07215226635541001, 0.1185313381004699, -0.11894150142085878, 0.16809724335246146, -0.06763594143398821, -0.17264813423309833, -0.0133191462740149, 0.34509263937808066, -0.2491233639725267, -0.28187516492421494, 0.06257857267317452, -0.25345400575873733, -0.119758970831355, 0.1704073926331858, -0.05144029147029944, ... |
706.3019 | Neutrino Backgrounds to Dark Matter Searches | Neutrino coherent scattering cross sections can be as large as 10^{-39} cm^2,
while current dark matter experiments have sensitivities to WIMP coherent
scattering cross sections five orders of magnitude smaller; future experiments
plan to have sensitivities to cross sections as small as 10^{-48} cm^2. With
large targ... | astro-ph hep-ex nucl-ex | neutrino coherent scattering cross sections can be as large as 1039 cm2 while current dark matter experiments have sensitivities to wimp coherent scattering cross sections five orders of magnitude smaller future experiments plan to have sensitivities to cross sections as small as 1048 cm2 with large target masses and f... | [['neutrino', 'coherent', 'scattering', 'cross', 'sections', 'can', 'be', 'as', 'large', 'as', '1039', 'cm2', 'while', 'current', 'dark', 'matter', 'experiments', 'have', 'sensitivities', 'to', 'wimp', 'coherent', 'scattering', 'cross', 'sections', 'five', 'orders', 'of', 'magnitude', 'smaller', 'future', 'experiments'... | [-0.07691904799139593, 0.2609200908884001, 0.009503267724843075, 0.17840672264962146, -0.022243845004898805, -0.05955110059585422, -0.03439034308636716, 0.3712222348355378, -0.16629582015351238, -0.3902545514332208, -0.01239409052504925, -0.39621878543403, 0.09683837153716013, 0.22510677605168894, 0.10671989508167219, ... |
706.302 | Unconventional elasticity in smectic-A elastomers | We study two aspects of the elasticity of smectic-$A$ elastomers that make
these materials genuinely and qualitatively different from conventional
uniaxial rubbers. Under strain applied parallel to the layer normal, monodomain
smectic-$A$ elastomers exhibit a drastic change in Young's modulus above a
threshold strain... | cond-mat.soft | we study two aspects of the elasticity of smectica elastomers that make these materials genuinely and qualitatively different from conventional uniaxial rubbers under strain applied parallel to the layer normal monodomain smectica elastomers exhibit a drastic change in youngs modulus above a threshold strain value of a... | [['we', 'study', 'two', 'aspects', 'of', 'the', 'elasticity', 'of', 'smectica', 'elastomers', 'that', 'make', 'these', 'materials', 'genuinely', 'and', 'qualitatively', 'different', 'from', 'conventional', 'uniaxial', 'rubbers', 'under', 'strain', 'applied', 'parallel', 'to', 'the', 'layer', 'normal', 'monodomain', 'sm... | [-0.10885147969645348, 0.17015158100442473, -0.08036954081346037, -0.046859180758191836, -0.07524996386271296, -0.08810978526141024, 0.06119777765791881, 0.3978200952739464, -0.2532296448096054, -0.3269032989447774, 0.0253310354880862, -0.2606602752246686, -0.21622313757639522, 0.14596915573844668, -0.04630564546689517... |
706.3021 | Independence property and hyperbolic groups | We prove that existentially closed $CSA$-groups have the independence
property. This is done by showing that there exist words having the
independence property relatively to the class of torsion-free hyperbolic
groups.
| math.LO math.GR | we prove that existentially closed csagroups have the independence property this is done by showing that there exist words having the independence property relatively to the class of torsionfree hyperbolic groups | [['we', 'prove', 'that', 'existentially', 'closed', 'csagroups', 'have', 'the', 'independence', 'property', 'this', 'is', 'done', 'by', 'showing', 'that', 'there', 'exist', 'words', 'having', 'the', 'independence', 'property', 'relatively', 'to', 'the', 'class', 'of', 'torsionfree', 'hyperbolic', 'groups']] | [-0.203092029877007, 0.1640755985242625, -0.10545969412972529, 0.12768727894872428, -0.12007548635204633, -0.147217439673841, 0.013542577612679452, 0.43552399426698685, -0.32115611229091884, -0.2270184544691195, 0.0631098937941715, -0.23346945034960906, -0.1250838820046435, 0.18330073425119434, -0.12165472712367773, -0... |
706.3022 | Dynamical tunneling in macroscopic systems | We investigate macroscopic dynamical quantum tunneling (MDQT) in the driven
Duffing oscillator, charateristic for Josephson junction physics and
nanomechanics. Under resonant conditions between stable coexisting states of
such systems we calculate the tunneling rate. In macroscopic systems coupled to
a heat bath, MDQ... | cond-mat.supr-con | we investigate macroscopic dynamical quantum tunneling mdqt in the driven duffing oscillator charateristic for josephson junction physics and nanomechanics under resonant conditions between stable coexisting states of such systems we calculate the tunneling rate in macroscopic systems coupled to a heat bath mdqt can be... | [['we', 'investigate', 'macroscopic', 'dynamical', 'quantum', 'tunneling', 'mdqt', 'in', 'the', 'driven', 'duffing', 'oscillator', 'charateristic', 'for', 'josephson', 'junction', 'physics', 'and', 'nanomechanics', 'under', 'resonant', 'conditions', 'between', 'stable', 'coexisting', 'states', 'of', 'such', 'systems', ... | [-0.22159883435313232, 0.20455423165878203, -0.06296156411862945, 0.04431195233068238, 0.0251957956790822, -0.2364337091056681, 0.06843450065217402, 0.3557959399632599, -0.2743495256665533, -0.25301099252210907, 0.012679232989297542, -0.28231855162916936, -0.14805124863369823, 0.2599474281815761, -0.0021163711183997866... |
706.3023 | Impact of the Neutrino Magnetic Moment on the Neutrino Fluxes and the
Electron Fraction in core-collapse Supernovae | We explore the effect of the neutrino magnetic moment on neutrino scattering
with matter in a core-collapse Supernova. We study the impact both on the
neutrino fluxes and on the electron fraction. We find that sizeable
modifications require very large magnetic moments both for Dirac and Majorana
neutrinos.
| astro-ph | we explore the effect of the neutrino magnetic moment on neutrino scattering with matter in a corecollapse supernova we study the impact both on the neutrino fluxes and on the electron fraction we find that sizeable modifications require very large magnetic moments both for dirac and majorana neutrinos | [['we', 'explore', 'the', 'effect', 'of', 'the', 'neutrino', 'magnetic', 'moment', 'on', 'neutrino', 'scattering', 'with', 'matter', 'in', 'a', 'corecollapse', 'supernova', 'we', 'study', 'the', 'impact', 'both', 'on', 'the', 'neutrino', 'fluxes', 'and', 'on', 'the', 'electron', 'fraction', 'we', 'find', 'that', 'sizea... | [-0.12286655647524942, 0.263455199659802, 0.02761246038911243, 0.22763352538459003, -0.08987995353527367, -0.02410649596519458, 0.07292375881055098, 0.35992006794549525, -0.14523626359490058, -0.33981800836045295, -0.011667733063707905, -0.3306704583422591, -0.03809946697098591, 0.20364102732855827, 0.11195258794274802... |
706.3024 | On a generalization of Dehn's algorithm | Viewing Dehn's algorithm as a rewriting system, we generalise to allow an
alphabet containing letters which do not necessarily represent group elements.
This extends the class of groups for which the algorithm solves the word
problem to include nilpotent groups, many relatively hyperbolic groups
including geometrical... | math.GR math.GT | viewing dehns algorithm as a rewriting system we generalise to allow an alphabet containing letters which do not necessarily represent group elements this extends the class of groups for which the algorithm solves the word problem to include nilpotent groups many relatively hyperbolic groups including geometrically fin... | [['viewing', 'dehns', 'algorithm', 'as', 'a', 'rewriting', 'system', 'we', 'generalise', 'to', 'allow', 'an', 'alphabet', 'containing', 'letters', 'which', 'do', 'not', 'necessarily', 'represent', 'group', 'elements', 'this', 'extends', 'the', 'class', 'of', 'groups', 'for', 'which', 'the', 'algorithm', 'solves', 'the'... | [-0.1406717655101889, 0.10529213224117963, -0.1157293482585565, 0.061503870524220954, -0.15491283769523234, -0.15618303478940537, 0.005213167381129767, 0.4299311609007418, -0.344278220067683, -0.25339720756011574, 0.13370773910581576, -0.22899267299002724, -0.15515552469970365, 0.22795056858663693, -0.16900510638462085... |
706.3025 | Contact Interactions and Resonance-Like Physics at Present and Future
Colliders from Unparticles | High scale conformal physics can lead to unusual unparticle stuff at our low
energies. In this paper we discuss how the exchange of unparticles between
Standard Model fields can lead to new contact interaction physics as well as a
pseudoresonance-like structure, an unresonance, that might be observable at the
Tevatro... | hep-ph hep-ex hep-th | high scale conformal physics can lead to unusual unparticle stuff at our low energies in this paper we discuss how the exchange of unparticles between standard model fields can lead to new contact interaction physics as well as a pseudoresonancelike structure an unresonance that might be observable at the tevatron or l... | [['high', 'scale', 'conformal', 'physics', 'can', 'lead', 'to', 'unusual', 'unparticle', 'stuff', 'at', 'our', 'low', 'energies', 'in', 'this', 'paper', 'we', 'discuss', 'how', 'the', 'exchange', 'of', 'unparticles', 'between', 'standard', 'model', 'fields', 'can', 'lead', 'to', 'new', 'contact', 'interaction', 'physic... | [-0.05583571541146972, 0.18896729279572938, -0.12426743412820193, 0.17695133292671436, -0.13204211415424466, -0.18168853380633757, -0.025499470942379095, 0.3519782784084479, -0.31320675316218954, -0.35250453781097746, 0.05181378218306539, -0.2464380665586736, -0.0961892761510964, 0.17390501108139944, -0.004265899161020... |
706.3026 | Precise Determination of the I=2 pipi Scattering Length from
Mixed-Action Lattice QCD | The I=2 pipi scattering length is calculated in fully-dynamical lattice QCD
with domain-wall valence quarks on the asqtad-improved coarse MILC
configurations (with fourth-rooted staggered sea quarks) at four light-quark
masses. Two- and three-flavor mixed-action chiral perturbation theory at
next-to-leading order is ... | hep-lat hep-ph | the i2 pipi scattering length is calculated in fullydynamical lattice qcd with domainwall valence quarks on the asqtadimproved coarse milc configurations with fourthrooted staggered sea quarks at four lightquark masses two and threeflavor mixedaction chiral perturbation theory at nexttoleading order is used to perform ... | [['the', 'i2', 'pipi', 'scattering', 'length', 'is', 'calculated', 'in', 'fullydynamical', 'lattice', 'qcd', 'with', 'domainwall', 'valence', 'quarks', 'on', 'the', 'asqtadimproved', 'coarse', 'milc', 'configurations', 'with', 'fourthrooted', 'staggered', 'sea', 'quarks', 'at', 'four', 'lightquark', 'masses', 'two', 'a... | [-0.07526319891389838, 0.3629041919214786, -0.09889274023716217, 0.11924255959541145, 0.025397208661002958, -0.05791355000025984, 0.09389503101609054, 0.41463331775604817, -0.10474730938322087, -0.19560209737307782, -0.03677347465418279, -0.372886944130279, 0.05358971871327663, -0.020385279370795772, 0.1079050872906826... |
706.3027 | Final state radiation and a possibility to test a pion-photon
interaction model near two-pion threshold | Final state radiation in the process $e^+e^-\to\pi^+\pi^-$ is considered for
the cuts used in the analysis of KLOE data at large angles. By means of a Monte
Carlo event generator FEVA, effects of non-pointlike behaviour of pions are
estimated in the framework of Resonance Perturbation Theory. An additional
complicati... | hep-ph | final state radiation in the process eetopipi is considered for the cuts used in the analysis of kloe data at large angles by means of a monte carlo event generator feva effects of nonpointlike behaviour of pions are estimated in the framework of resonance perturbation theory an additional complication related with the... | [['final', 'state', 'radiation', 'in', 'the', 'process', 'eetopipi', 'is', 'considered', 'for', 'the', 'cuts', 'used', 'in', 'the', 'analysis', 'of', 'kloe', 'data', 'at', 'large', 'angles', 'by', 'means', 'of', 'a', 'monte', 'carlo', 'event', 'generator', 'feva', 'effects', 'of', 'nonpointlike', 'behaviour', 'of', 'pi... | [-0.07233111259120051, 0.1717968985129523, -0.15969061548821628, 0.1365128900565752, -0.03496476919390261, -0.08690404270568655, 0.017464284193960743, 0.3166929499556621, -0.22531725708653944, -0.29687070098718527, 0.027256857696920635, -0.33030122506121795, -0.024943627862052786, 0.15537663948618705, 0.074970576260238... |
706.3028 | On the discreteness and rationality of F-jumping coefficients | This paper studies the jumping coefficients of principal ideals of regular
local rings.
Recently M. Blickle, M. Mustata and K. Smith showed that, when $R$ is of
essentially finite type over a field and $F$-finite, bounded intervals contain
finitely many jumping coefficients and that those are rational. In a later
p... | math.AC math.AG | this paper studies the jumping coefficients of principal ideals of regular local rings recently m blickle m mustata and k smith showed that when r is of essentially finite type over a field and ffinite bounded intervals contain finitely many jumping coefficients and that those are rational in a later paper they extende... | [['this', 'paper', 'studies', 'the', 'jumping', 'coefficients', 'of', 'principal', 'ideals', 'of', 'regular', 'local', 'rings', 'recently', 'm', 'blickle', 'm', 'mustata', 'and', 'k', 'smith', 'showed', 'that', 'when', 'r', 'is', 'of', 'essentially', 'finite', 'type', 'over', 'a', 'field', 'and', 'ffinite', 'bounded', ... | [-0.18129904767167165, 0.0515835536840621, -0.10238469515363095, 0.054519562859868656, -0.09190609068839325, -0.17081264741587596, -0.041322061258309166, 0.34005874959410914, -0.31917649616395505, -0.17019220276958716, 0.11187655286302685, -0.22900373765724893, -0.14385505312968466, 0.20903020993803142, -0.146548613891... |
706.3029 | Using integral transforms to estimate higher order derivatives | Integral transformations are used to estimate high order derivatives of
various special functions. Applications are given to numerical integration,
where estimates of high order derivatives of the integrand are needed to
achieve bounds on the error. The main idea is to find a suitable integral
representation of the f... | math.NA math.HO | integral transformations are used to estimate high order derivatives of various special functions applications are given to numerical integration where estimates of high order derivatives of the integrand are needed to achieve bounds on the error the main idea is to find a suitable integral representation of the functi... | [['integral', 'transformations', 'are', 'used', 'to', 'estimate', 'high', 'order', 'derivatives', 'of', 'various', 'special', 'functions', 'applications', 'are', 'given', 'to', 'numerical', 'integration', 'where', 'estimates', 'of', 'high', 'order', 'derivatives', 'of', 'the', 'integrand', 'are', 'needed', 'to', 'achie... | [-0.10570230337819367, 0.03051357397414518, -0.08256284333765507, 0.12701072014169767, -0.14722020841542294, -0.0473841615515112, -0.010146163211726216, 0.3791623076593334, -0.2863823674675642, -0.3419262756395972, 0.20321160866737817, -0.2611649081033344, -0.13050960391851593, 0.20757080188416172, -0.06672550020668881... |
706.303 | A Comparative Study of Optical and Ultraviolet Effective Temperatures
for DA White Dwarfs from the IUE Archive | We present a comparative study of effective temperatures determined from the
hydrogen Balmer lines and from the UV energy distribution for 140 DA white
dwarfs drawn from the IUE archive. Our results indicate that the optical and UV
temperatures of the majority of stars below T~40,000 K and within ~75 pc are in
fairly... | astro-ph | we present a comparative study of effective temperatures determined from the hydrogen balmer lines and from the uv energy distribution for 140 da white dwarfs drawn from the iue archive our results indicate that the optical and uv temperatures of the majority of stars below t40000 k and within 75 pc are in fairly good ... | [['we', 'present', 'a', 'comparative', 'study', 'of', 'effective', 'temperatures', 'determined', 'from', 'the', 'hydrogen', 'balmer', 'lines', 'and', 'from', 'the', 'uv', 'energy', 'distribution', 'for', '140', 'da', 'white', 'dwarfs', 'drawn', 'from', 'the', 'iue', 'archive', 'our', 'results', 'indicate', 'that', 'the... | [-0.03915889229263282, 0.11706350671665859, -0.052289746365406446, 0.10585754526772588, -0.04240604112338689, -0.08135011495970604, 0.12709258842514828, 0.4109229425071842, -0.19458278591240136, -0.36082712318230836, 0.04429152480378333, -0.33205372682876055, -0.06769093009384555, 0.21094379420133513, -0.03507410599591... |
706.3031 | Duality of antidiagonals and pipe dreams | Weighted enumeration of reduced pipe dreams (or rc-graphs) results in a
combinatorial expression for Schubert polynomials. The duality between the set
of reduced pipe dreams and certain antidiagonals has important geometric
implications [A. Knutson and E. Miller, Gr\"obner geometry of Schubert
polynomials, Ann. Math.... | math.CO | weighted enumeration of reduced pipe dreams or rcgraphs results in a combinatorial expression for schubert polynomials the duality between the set of reduced pipe dreams and certain antidiagonals has important geometric implications a knutson and e miller grobner geometry of schubert polynomials ann math 161 12451318 t... | [['weighted', 'enumeration', 'of', 'reduced', 'pipe', 'dreams', 'or', 'rcgraphs', 'results', 'in', 'a', 'combinatorial', 'expression', 'for', 'schubert', 'polynomials', 'the', 'duality', 'between', 'the', 'set', 'of', 'reduced', 'pipe', 'dreams', 'and', 'certain', 'antidiagonals', 'has', 'important', 'geometric', 'impl... | [-0.15086245452249913, -0.005256291190897555, -0.12174599996682159, 0.03631269397967691, -0.1658577612160068, -0.1409910573550549, 0.059798520170213455, 0.2292001446414935, -0.33820334262533214, -0.25430820543490545, 0.11391932620991659, -0.1698638379671856, -0.18664700480018692, 0.2047382640333748, -0.2258379632043407... |
706.3032 | The Solar Radius in the EUV during the Cycle XXIII | Aims. To determine the solar transition region and coronal radius at EUV
wavelengths and its time evolution during Solar Cycle XXIII.
Methods. We use daily 30.4 and 17.1 nm images obtained by the Extreme
Ultraviolet Imager (EIT) aboard the SoHO satellite and derive the solar radius
by fitting a circle to the limb b... | astro-ph | aims to determine the solar transition region and coronal radius at euv wavelengths and its time evolution during solar cycle xxiii methods we use daily 304 and 171 nm images obtained by the extreme ultraviolet imager eit aboard the soho satellite and derive the solar radius by fitting a circle to the limb brightness r... | [['aims', 'to', 'determine', 'the', 'solar', 'transition', 'region', 'and', 'coronal', 'radius', 'at', 'euv', 'wavelengths', 'and', 'its', 'time', 'evolution', 'during', 'solar', 'cycle', 'xxiii', 'methods', 'we', 'use', 'daily', '304', 'and', '171', 'nm', 'images', 'obtained', 'by', 'the', 'extreme', 'ultraviolet', 'i... | [-0.043048083076428156, 0.18492206723385607, 0.016417339040344814, 0.08301537305851525, -0.001494439500675071, -0.09598097526759375, 0.033074219716581865, 0.46167645321111195, -0.15243346614624897, -0.4072890205134172, 0.10141160763669177, -0.30581159437133465, -0.06765434112458024, 0.22907057470729342, -0.044971884356... |
706.3033 | Effect of antiferromagnetic spin correlations on lattice distortion and
charge ordering in Pr$_{0.5}$Ca$_{1.5}$MnO$_{4}$ | We use neutron scattering to study the lattice and magnetic structure of the
layered half-doped manganite Pr$_{0.5}$Ca$_{1.5}$MnO$_4$. On cooling from high
temperature, the system first becomes charge- and orbital- ordered (CO/OO) near
$T_{CO}=300$ K and then develops checkerboard-like antiferromagnetic (AF) order
be... | cond-mat.str-el | we use neutron scattering to study the lattice and magnetic structure of the layered halfdoped manganite pr_05ca_15mno_4 on cooling from high temperature the system first becomes charge and orbital ordered cooo near t_co300 k and then develops checkerboardlike antiferromagnetic af order below t_n130 k at temperatures a... | [['we', 'use', 'neutron', 'scattering', 'to', 'study', 'the', 'lattice', 'and', 'magnetic', 'structure', 'of', 'the', 'layered', 'halfdoped', 'manganite', 'pr_05ca_15mno_4', 'on', 'cooling', 'from', 'high', 'temperature', 'the', 'system', 'first', 'becomes', 'charge', 'and', 'orbital', 'ordered', 'cooo', 'near', 't_co3... | [-0.25792294565140833, 0.30858104567810457, 0.004536183079831151, 0.014451618361122468, -0.06561717836131506, -0.1066248101977216, 0.12206236412748694, 0.4074715769247097, -0.3149826761481224, -0.2315405338509556, 0.015025478144011954, -0.37825694913957636, -0.11918945457128917, 0.11347334530642804, 0.1536783922427133,... |
706.3034 | Enhancement of the dielectron continuum in sqrt{s_NN} = 200 GeV Au+Au
collisions | The PHENIX experiment has measured the dielectron continuum in sqrt{s_NN} =
200 GeV Au+Au collisions. In minimum bias collisions the dielectron yield in
the mass range between 150 and 750 MeV/c^2 is enhanced by a factor of 3.4 +/-
0.2(stat.) +/- 1.3(syst.) +/- 0.7(model) compared to the expectation from our
model of ... | nucl-ex | the phenix experiment has measured the dielectron continuum in sqrts_nn 200 gev auau collisions in minimum bias collisions the dielectron yield in the mass range between 150 and 750 mevc2 is enhanced by a factor of 34 02stat 13syst 07model compared to the expectation from our model of hadron decays the integrated yield... | [['the', 'phenix', 'experiment', 'has', 'measured', 'the', 'dielectron', 'continuum', 'in', 'sqrts_nn', '200', 'gev', 'auau', 'collisions', 'in', 'minimum', 'bias', 'collisions', 'the', 'dielectron', 'yield', 'in', 'the', 'mass', 'range', 'between', '150', 'and', '750', 'mevc2', 'is', 'enhanced', 'by', 'a', 'factor', '... | [-0.03206290720429804, 0.24860614035278558, -0.12950476410665682, 0.11437039635410266, 0.040335096046328546, -0.09687120052764103, -0.006082495257890384, 0.35746209914796057, -0.17430521982078928, -0.32454250307664984, -0.09347055047262637, -0.4227678288749996, 0.11937444164816823, 0.16399196461508317, 0.07995645737364... |
706.3035 | Massive Clumps in the NGC 6334 Star Forming Region | We report observations of dust continuum emission at 1.2 mm toward the star
forming region NGC 6334 made with the SEST SIMBA bolometer array. The
observations cover an area of $\sim 2$ square degrees with approximately
uniform noise. We detected 181 clumps spanning almost three orders of magnitude
in mass (3\Msun$-6\... | astro-ph | we report observations of dust continuum emission at 12 mm toward the star forming region ngc 6334 made with the sest simba bolometer array the observations cover an area of sim 2 square degrees with approximately uniform noise we detected 181 clumps spanning almost three orders of magnitude in mass 3msun6times103 msun... | [['we', 'report', 'observations', 'of', 'dust', 'continuum', 'emission', 'at', '12', 'mm', 'toward', 'the', 'star', 'forming', 'region', 'ngc', '6334', 'made', 'with', 'the', 'sest', 'simba', 'bolometer', 'array', 'the', 'observations', 'cover', 'an', 'area', 'of', 'sim', '2', 'square', 'degrees', 'with', 'approximatel... | [-0.08307161810646196, 0.13015888894716182, -0.06328627603342904, 0.07450152813143654, -0.03383325542843465, -0.05677256930715567, 0.03151857246097828, 0.4210418400665124, -0.14726486220578885, -0.3606977533781901, 0.05210279177233119, -0.28109945073753356, 1.3383447251740902e-05, 0.16678909742918294, -0.00604605723631... |
706.3036 | The Hubbard model: bosonic excitations and zero-frequency constants | A fully self-consistent calculation of the bosonic dynamics of the Hubbard
model is developed within the Composite Operator Method. From one side we
consider a basic set of fermionic composite operators (Hubbard fields) and
calculate the retarded propagators. On the other side we consider a basic set
of bosonic compo... | cond-mat.str-el cond-mat.supr-con | a fully selfconsistent calculation of the bosonic dynamics of the hubbard model is developed within the composite operator method from one side we consider a basic set of fermionic composite operators hubbard fields and calculate the retarded propagators on the other side we consider a basic set of bosonic composite op... | [['a', 'fully', 'selfconsistent', 'calculation', 'of', 'the', 'bosonic', 'dynamics', 'of', 'the', 'hubbard', 'model', 'is', 'developed', 'within', 'the', 'composite', 'operator', 'method', 'from', 'one', 'side', 'we', 'consider', 'a', 'basic', 'set', 'of', 'fermionic', 'composite', 'operators', 'hubbard', 'fields', 'an... | [-0.13561544285428703, 0.16407699071487802, -0.055992832383627344, 0.09001172453411233, -0.04997274337876232, -0.11500163686871054, 0.024686192209790847, 0.3110899938578913, -0.2532372867486849, -0.22764455209112472, 0.048738703677418886, -0.2840640133567107, -0.10514282205017508, 0.13716326381530683, 0.061007192508157... |
706.3037 | Implicit function density computation | If two random variables X and A are functionally related via f(X)=A for some
strictly monotone continuously differentiable function f:R->R, the distribution
of X may easily be computed from the distribution of A.
| math.GM | if two random variables x and a are functionally related via fxa for some strictly monotone continuously differentiable function frr the distribution of x may easily be computed from the distribution of a | [['if', 'two', 'random', 'variables', 'x', 'and', 'a', 'are', 'functionally', 'related', 'via', 'fxa', 'for', 'some', 'strictly', 'monotone', 'continuously', 'differentiable', 'function', 'frr', 'the', 'distribution', 'of', 'x', 'may', 'easily', 'be', 'computed', 'from', 'the', 'distribution', 'of', 'a']] | [-0.09193171340633523, 0.18317026117195687, -0.12387902141464027, 0.06737658268574512, -0.025181980225060022, -0.1781028312433398, 0.026691836389628323, 0.4021262637141979, -0.36900421435182745, -0.18361672222840064, 0.13996239675378258, -0.2685443161824492, -0.1438734701862841, 0.22997074035193885, -0.0509482486681504... |
706.3038 | Separability of a family of one parameter W and GHZ multiqubit states
using Abe-Rajagopal q-conditional entropy approach | We employ conditional Tsallis q entropies to study the separability of
symmetric one parameter W and GHZ multiqubit mixed states. The strongest
limitation on separability is realized in the limit q-->infinity, and is found
to be much superior to the condition obtained using the von Neumann conditional
entropy (q=1 ca... | quant-ph | we employ conditional tsallis q entropies to study the separability of symmetric one parameter w and ghz multiqubit mixed states the strongest limitation on separability is realized in the limit qinfinity and is found to be much superior to the condition obtained using the von neumann conditional entropy q1 case except... | [['we', 'employ', 'conditional', 'tsallis', 'q', 'entropies', 'to', 'study', 'the', 'separability', 'of', 'symmetric', 'one', 'parameter', 'w', 'and', 'ghz', 'multiqubit', 'mixed', 'states', 'the', 'strongest', 'limitation', 'on', 'separability', 'is', 'realized', 'in', 'the', 'limit', 'qinfinity', 'and', 'is', 'found'... | [-0.1084393362617483, 0.1423284971010085, -0.05193119326775724, 0.07561128583204534, -0.012364743213931268, -0.25813844110574813, 0.03623924652483411, 0.32738339806326316, -0.18625915401264445, -0.23440843741726977, 0.09889557784538136, -0.22348728548590238, -0.0337587610921254, 0.18606865229447941, -0.0838078711508446... |
706.3039 | The spectral density function of a toric variety | For a Kahler manifold (X, \omega) with a holomorphic line bundle L and metric
h such that the Chern form of L is \omega, the spectral measures are the
measures \mu_N = \sum |s_{N,i}|^2 \nu, where \{s_{N,i}\}_i is an
L^2-orthonormal basis for H^0(X, L^{\otimes N}), and \nu is Liouville measure.
We study the asymptotic... | math.SP math-ph math.MP | for a kahler manifold x omega with a holomorphic line bundle l and metric h such that the chern form of l is omega the spectral measures are the measures mu_n sum s_ni2 nu where s_ni_i is an l2orthonormal basis for h0x lotimes n and nu is liouville measure we study the asymptotics in n of mu_n for x l a hamiltonian tor... | [['for', 'a', 'kahler', 'manifold', 'x', 'omega', 'with', 'a', 'holomorphic', 'line', 'bundle', 'l', 'and', 'metric', 'h', 'such', 'that', 'the', 'chern', 'form', 'of', 'l', 'is', 'omega', 'the', 'spectral', 'measures', 'are', 'the', 'measures', 'mu_n', 'sum', 's_ni2', 'nu', 'where', 's_ni_i', 'is', 'an', 'l2orthonorma... | [-0.22573257284919726, 0.0851704997662557, -0.09705220168042514, 0.039789267665875414, -0.06356022352548807, -0.13123760753915759, 0.048987258960593666, 0.3239939332890667, -0.25649220740956347, -0.17858070559930384, 0.06322299564027156, -0.31927949226630187, -0.11207183013596621, 0.16720584237795563, -0.07599033379644... |
706.304 | Experimental observation of strong photon localization in disordered
photonic crystal waveguides | We demonstrate experimentally that structural perturbations imposed on
highly-dispersive photonic crystal-based waveguides give rise to spectral
features that bear signatures of Anderson localization. Sharp resonances with
the effective Qs of over 30,000 are found in scattering spectra of disordered
waveguides. The r... | physics.optics physics.gen-ph | we demonstrate experimentally that structural perturbations imposed on highlydispersive photonic crystalbased waveguides give rise to spectral features that bear signatures of anderson localization sharp resonances with the effective qs of over 30000 are found in scattering spectra of disordered waveguides the resonanc... | [['we', 'demonstrate', 'experimentally', 'that', 'structural', 'perturbations', 'imposed', 'on', 'highlydispersive', 'photonic', 'crystalbased', 'waveguides', 'give', 'rise', 'to', 'spectral', 'features', 'that', 'bear', 'signatures', 'of', 'anderson', 'localization', 'sharp', 'resonances', 'with', 'the', 'effective', ... | [-0.16570842816018622, 0.18992209364660084, -0.07241682515418886, 0.06665142417035025, -0.012149500620105991, -0.17990127006424186, 0.004064960941753309, 0.47702472094122483, -0.22371766270826693, -0.28408606463800307, 0.025781123590169718, -0.3082795527196773, -0.12297411628685001, 0.17089984613804796, 0.0022139586255... |
706.3041 | Population synthesis of radio and gamma-ray millisecond pulsars from the
Galactic disk | We present results of a population synthesis of millisecond pulsars from the
Galactic disk. Excluding globular clusters, we model the spatial distribution
of millisecond pulsars by assuming their birth in the Galactic disk with a
random kick velocity and evolve them to the present within the Galactic
potential. We as... | astro-ph | we present results of a population synthesis of millisecond pulsars from the galactic disk excluding globular clusters we model the spatial distribution of millisecond pulsars by assuming their birth in the galactic disk with a random kick velocity and evolve them to the present within the galactic potential we assume ... | [['we', 'present', 'results', 'of', 'a', 'population', 'synthesis', 'of', 'millisecond', 'pulsars', 'from', 'the', 'galactic', 'disk', 'excluding', 'globular', 'clusters', 'we', 'model', 'the', 'spatial', 'distribution', 'of', 'millisecond', 'pulsars', 'by', 'assuming', 'their', 'birth', 'in', 'the', 'galactic', 'disk'... | [-0.08375644705895531, 0.13793277489726039, -0.05606228660939163, 0.14186972853081228, -0.13997794749478712, -0.08039560417436357, 0.06759598847680823, 0.45152374283459623, -0.1978343228386764, -0.31399756631397296, 0.031088906521051143, -0.2603968122995483, -0.050605730937891884, 0.2555331295037544, -0.005707225580025... |
706.3042 | Turbulent transport of material particles: An experimental study of
finite size effects | We use an acoustic Lagrangian tracking technique, particularly adapted to
measurements in open flows, and a versatile material particles generator (in
the form of soap bubbles with adjustable size and density) to characterize
Lagrangian statistics of finite sized, neutrally bouyant, particles transported
in an isotro... | physics.flu-dyn | we use an acoustic lagrangian tracking technique particularly adapted to measurements in open flows and a versatile material particles generator in the form of soap bubbles with adjustable size and density to characterize lagrangian statistics of finite sized neutrally bouyant particles transported in an isotropic turb... | [['we', 'use', 'an', 'acoustic', 'lagrangian', 'tracking', 'technique', 'particularly', 'adapted', 'to', 'measurements', 'in', 'open', 'flows', 'and', 'a', 'versatile', 'material', 'particles', 'generator', 'in', 'the', 'form', 'of', 'soap', 'bubbles', 'with', 'adjustable', 'size', 'and', 'density', 'to', 'characterize... | [-0.1277924325938026, 0.26501475062913316, -0.0994807251596025, 0.04726959013986209, -0.02640896258387892, -0.06293728395128652, -0.03880285047131428, 0.33209409434644005, -0.2830845017562665, -0.3116788572986566, 0.03621778754602438, -0.2582166353425395, -0.055109526429857524, 0.18738168666956, -0.04682034705691631, 0... |
706.3043 | Carbon and Strontium Abundances of Metal-Poor Stars | We present carbon and strontium abundances for 100 metal-poor stars measured
from R$\sim $7000 spectra obtained with the Echellette Spectrograph and Imager
at the Keck Observatory. Using spectral synthesis of the G-band region, we have
derived carbon abundances for stars ranging from [Fe/H]$=-1.3$ to
[Fe/H]$=-3.8$. T... | astro-ph | we present carbon and strontium abundances for 100 metalpoor stars measured from rsim 7000 spectra obtained with the echellette spectrograph and imager at the keck observatory using spectral synthesis of the gband region we have derived carbon abundances for stars ranging from feh13 to feh38 the formal errors are sim 0... | [['we', 'present', 'carbon', 'and', 'strontium', 'abundances', 'for', '100', 'metalpoor', 'stars', 'measured', 'from', 'rsim', '7000', 'spectra', 'obtained', 'with', 'the', 'echellette', 'spectrograph', 'and', 'imager', 'at', 'the', 'keck', 'observatory', 'using', 'spectral', 'synthesis', 'of', 'the', 'gband', 'region'... | [0.02208920153675646, 0.16046308602842435, -0.004078156661196816, 0.018485244318116004, -0.02778914007045919, -0.07033271204805137, 0.07376130450397685, 0.47500823231743333, -0.13863159093165361, -0.38906770050468875, -0.022319645629400704, -0.3584628786562329, 0.022758162923997675, 0.19756682916180934, -0.082017402438... |
706.3044 | On McQuillan's "tautological inequality" and the Weyl-Ahlfors theory of
associated curves | In 1941, L. Ahlfors gave another proof of a 1933 theorem of H. Cartan on
approximation to hyperplanes of holomorphic curves in P^n. Ahlfors' proof built
on earlier work of H. and J. Weyl (1938), and proved Cartan's theorem by
studying the associated curves of the holomorphic curve. This work has
subsequently been rew... | math.CV math.AG | in 1941 l ahlfors gave another proof of a 1933 theorem of h cartan on approximation to hyperplanes of holomorphic curves in pn ahlfors proof built on earlier work of h and j weyl 1938 and proved cartans theorem by studying the associated curves of the holomorphic curve this work has subsequently been reworked by hh wu ... | [['in', '1941', 'l', 'ahlfors', 'gave', 'another', 'proof', 'of', 'a', '1933', 'theorem', 'of', 'h', 'cartan', 'on', 'approximation', 'to', 'hyperplanes', 'of', 'holomorphic', 'curves', 'in', 'pn', 'ahlfors', 'proof', 'built', 'on', 'earlier', 'work', 'of', 'h', 'and', 'j', 'weyl', '1938', 'and', 'proved', 'cartans', '... | [-0.15479543562916, 2.518733775855711e-05, -0.15650186321429357, 0.055777351952457935, -0.11028847507757429, -0.17187475024303733, 0.052077037915540546, 0.23032150535075457, -0.2538934920722269, -0.25588093694274455, 0.08794602115901075, -0.23643032428746005, -0.18387992889464103, 0.22128944058790054, -0.18871619100619... |
706.3045 | The Future is Now: the Formation of Single Low Mass White Dwarfs in the
Solar Neighborhood | Low mass helium-core white dwarfs (M < 0.45 Msun) can be produced from
interacting binary systems, and traditionally all of them have been attributed
to this channel. However, a low mass white dwarf could also result from a
single star that experiences severe mass loss on the first ascent giant branch.
A large popula... | astro-ph | low mass heliumcore white dwarfs m 045 msun can be produced from interacting binary systems and traditionally all of them have been attributed to this channel however a low mass white dwarf could also result from a single star that experiences severe mass loss on the first ascent giant branch a large population of low ... | [['low', 'mass', 'heliumcore', 'white', 'dwarfs', 'm', '045', 'msun', 'can', 'be', 'produced', 'from', 'interacting', 'binary', 'systems', 'and', 'traditionally', 'all', 'of', 'them', 'have', 'been', 'attributed', 'to', 'this', 'channel', 'however', 'a', 'low', 'mass', 'white', 'dwarf', 'could', 'also', 'result', 'from... | [-0.0800377226489231, 0.17265234372472807, -0.07308551963058815, 0.1367692336053741, -0.12443763339416987, -0.0858948296072446, 0.10925089204410984, 0.3727596445152393, -0.1320439062681264, -0.3762656255666126, 0.052766553770184466, -0.2963869249863523, -0.06512181805860381, 0.21688877471343992, -0.1300229920132338, -0... |
706.3046 | Seismic study of the chemical composition of the solar convection zone | Recent downward revision of solar heavy-element abundances using
three-dimensional atmospheric model has introduced serious discrepancies
between standard solar models and helioseismic inferences about solar
structure. In this paper, we investigate the possibility of determining the
heavy-element abundances using hel... | astro-ph | recent downward revision of solar heavyelement abundances using threedimensional atmospheric model has introduced serious discrepancies between standard solar models and helioseismic inferences about solar structure in this paper we investigate the possibility of determining the heavyelement abundances using helioseism... | [['recent', 'downward', 'revision', 'of', 'solar', 'heavyelement', 'abundances', 'using', 'threedimensional', 'atmospheric', 'model', 'has', 'introduced', 'serious', 'discrepancies', 'between', 'standard', 'solar', 'models', 'and', 'helioseismic', 'inferences', 'about', 'solar', 'structure', 'in', 'this', 'paper', 'we'... | [-0.014389785061675039, 0.1675861636357943, 0.006109831280429552, 0.09687835102033039, -0.04753517744618214, -0.008353364183990793, 0.07641586686976636, 0.330811817469922, -0.25573914484544236, -0.41635134888823483, 0.04127060281938281, -0.2787580227479339, -0.10199774310511367, 0.16685391180005602, -0.0771382703445851... |
706.3047 | The Radio Properties of Type Ibc Supernovae | Over the past few years, long-duration gamma-ray bursts (GRBs), including the
subclass of X-ray flashes (XRFs), have been revealed to be a rare variety of
Type Ibc supernova (SN Ibc). While all these events result from the death of
massive stars, the electromagnetic luminosities of GRBs and XRFs exceed those
of ordin... | astro-ph | over the past few years longduration gammaray bursts grbs including the subclass of xray flashes xrfs have been revealed to be a rare variety of type ibc supernova sn ibc while all these events result from the death of massive stars the electromagnetic luminosities of grbs and xrfs exceed those of ordinary type ibc sne... | [['over', 'the', 'past', 'few', 'years', 'longduration', 'gammaray', 'bursts', 'grbs', 'including', 'the', 'subclass', 'of', 'xray', 'flashes', 'xrfs', 'have', 'been', 'revealed', 'to', 'be', 'a', 'rare', 'variety', 'of', 'type', 'ibc', 'supernova', 'sn', 'ibc', 'while', 'all', 'these', 'events', 'result', 'from', 'the... | [-0.0386539390553177, 0.13717292262255354, 0.017348661193285476, 0.22058473136407333, -0.16663882137226843, -0.14365896017989144, 0.07248970735324264, 0.4789447078594204, -0.14628249752797384, -0.31393623127951287, 0.04959892162349371, -0.35941296185641974, -0.0028265614880982675, 0.2753728028460914, -0.034300091985091... |
706.3048 | A Dark Core in Abell 520 | The rich cluster Abell 520 (z=0.201) exhibits truly extreme and puzzling
multi-wavelength characteristics. It may best be described as a "cosmic train
wreck." It is a major merger showing abundant evidence for ram pressure
stripping, with a clear offset in the gas distribution compared to the galaxies
(as in the bull... | astro-ph | the rich cluster abell 520 z0201 exhibits truly extreme and puzzling multiwavelength characteristics it may best be described as a cosmic train wreck it is a major merger showing abundant evidence for ram pressure stripping with a clear offset in the gas distribution compared to the galaxies as in the bullet cluster 1e... | [['the', 'rich', 'cluster', 'abell', '520', 'z0201', 'exhibits', 'truly', 'extreme', 'and', 'puzzling', 'multiwavelength', 'characteristics', 'it', 'may', 'best', 'be', 'described', 'as', 'a', 'cosmic', 'train', 'wreck', 'it', 'is', 'a', 'major', 'merger', 'showing', 'abundant', 'evidence', 'for', 'ram', 'pressure', 's... | [-0.0884897721479844, 0.1084170368939383, -0.11952845471856928, 0.15143888146756956, -0.10405671841923207, -0.06430936512406718, 0.03154780431872323, 0.416884580932597, -0.1789705055091646, -0.3550940460954157, 0.051798035274259746, -0.29769483189438545, -0.016711478584776163, 0.1955945365939033, -0.016828936554408983,... |
706.3049 | Beyond Twisted Tori | Exploiting the fact that Kaluza-Klein monopoles and the associated
generalized orbifold planes are sources for geometrical fluxes, omega, we show
that the standard constraint omega.omega=0, valid for superstring
compactifications on twisted tori, can be consistently relaxed. This leads to
novel possibilities for cons... | hep-th | exploiting the fact that kaluzaklein monopoles and the associated generalized orbifold planes are sources for geometrical fluxes omega we show that the standard constraint omegaomega0 valid for superstring compactifications on twisted tori can be consistently relaxed this leads to novel possibilities for constructing s... | [['exploiting', 'the', 'fact', 'that', 'kaluzaklein', 'monopoles', 'and', 'the', 'associated', 'generalized', 'orbifold', 'planes', 'are', 'sources', 'for', 'geometrical', 'fluxes', 'omega', 'we', 'show', 'that', 'the', 'standard', 'constraint', 'omegaomega0', 'valid', 'for', 'superstring', 'compactifications', 'on', '... | [-0.13817268689525883, 0.16457672281698746, -0.008608350215794204, 0.20699208257296545, -0.13048278712123246, -0.14570977178994904, 0.002138846145652525, 0.3353890055766353, -0.16478847516337772, -0.2574673852846994, 0.11032472850676239, -0.24478772845022478, -0.14949627394800064, 0.1594049041265283, -0.150386741070391... |
706.305 | Dark matter from "strong gravity" - consistent with CRESST, CoGeNT and
DAMA/LIBRA | Kelso, Hooper and Buckley [arXiv:1110.5338] found CRESST, CoGeNT and
DAMA/LIBRA results are consistent with 10 - 15 GeV dark matter particles.
Hennawi and Ostriker [arXiv:astro-ph/0108203] analyzed supermassive black hole
formation in the centers of galaxies, finding a best fit for dark matter
(self-interaction cross... | gr-qc astro-ph hep-th | kelso hooper and buckley arxiv11105338 found cresst cogent and damalibra results are consistent with 10 15 gev dark matter particles hennawi and ostriker arxivastroph0108203 analyzed supermassive black hole formation in the centers of galaxies finding a best fit for dark matter selfinteraction crosssectionmass ratio 00... | [['kelso', 'hooper', 'and', 'buckley', 'arxiv11105338', 'found', 'cresst', 'cogent', 'and', 'damalibra', 'results', 'are', 'consistent', 'with', '10', '15', 'gev', 'dark', 'matter', 'particles', 'hennawi', 'and', 'ostriker', 'arxivastroph0108203', 'analyzed', 'supermassive', 'black', 'hole', 'formation', 'in', 'the', '... | [-0.09100554506175029, 0.19097037166424202, -0.06745683579729536, 0.20713712657109284, -0.0699349877018577, -0.13517486969701564, -0.0051256586284114, 0.29220885801343965, -0.08440253922405343, -0.5398783744909824, -0.0530565420168643, -0.33123657717488897, 0.09781706652257782, 0.15641383851060453, 0.020855087452591993... |
706.3051 | Molecular Dipolar Crystals as High Fidelity Quantum Memory for Hybrid
Quantum Computing | We study collective excitations of rotational and spin states of an ensemble
of polar molecules, which are prepared in a dipolar crystalline phase, as a
candidate for a high fidelity quantum memory. While dipolar crystals are formed
in the high density limit of cold clouds of polar molecules under 1D and 2D
trapping ... | quant-ph cond-mat.other | we study collective excitations of rotational and spin states of an ensemble of polar molecules which are prepared in a dipolar crystalline phase as a candidate for a high fidelity quantum memory while dipolar crystals are formed in the high density limit of cold clouds of polar molecules under 1d and 2d trapping condi... | [['we', 'study', 'collective', 'excitations', 'of', 'rotational', 'and', 'spin', 'states', 'of', 'an', 'ensemble', 'of', 'polar', 'molecules', 'which', 'are', 'prepared', 'in', 'a', 'dipolar', 'crystalline', 'phase', 'as', 'a', 'candidate', 'for', 'a', 'high', 'fidelity', 'quantum', 'memory', 'while', 'dipolar', 'cryst... | [-0.20639832056127488, 0.2479728114210108, -0.008575526139466091, 0.028854522368249792, 0.03533864287659526, -0.1477727986127138, 0.06464615432312712, 0.38737402038648727, -0.22249361156796416, -0.2577941647808378, 0.02322292683723693, -0.2601844305545092, -0.060534385696131114, 0.17710687678307294, 0.03428235381220778... |
706.3052 | Two Classes of Hot Jupiters | We identify two classes of transiting planet, based on their equilibrium
temperatures and Safronov numbers. We examine various possible explanations for
the dichotomy. It may reflect the influence of planet or planetesimal
scattering in determining when planetary migration stops. Another possibility
is that some plan... | astro-ph | we identify two classes of transiting planet based on their equilibrium temperatures and safronov numbers we examine various possible explanations for the dichotomy it may reflect the influence of planet or planetesimal scattering in determining when planetary migration stops another possibility is that some planets lo... | [['we', 'identify', 'two', 'classes', 'of', 'transiting', 'planet', 'based', 'on', 'their', 'equilibrium', 'temperatures', 'and', 'safronov', 'numbers', 'we', 'examine', 'various', 'possible', 'explanations', 'for', 'the', 'dichotomy', 'it', 'may', 'reflect', 'the', 'influence', 'of', 'planet', 'or', 'planetesimal', 's... | [-0.10804741853064138, 0.23394777614010287, -0.09265814307794164, 0.15241851740531182, -0.12215808440659996, -0.1138478816498684, 0.10369340865578078, 0.3379943419860888, -0.20989796862925722, -0.3311791985142457, 0.06915479935882494, -0.2819943502545357, -0.11155137121736343, 0.15828528537862946, -0.09165821115993246,... |
706.3053 | A Survey of Intrinsic Absorption in Active Galaxies using the Far
Ultraviolet Spectroscopic Explorer | We present a survey of 72 Seyfert galaxies and quasars observed by the it Far
Ultraviolet Spectroscopic Explorer (FUSE). We have determined that 72 of 253
available active galactic nuclei (AGN) targets are viable targets for detection
of intrinsic absorption lines. We examined these spectra for signs of intrinsic
abs... | astro-ph | we present a survey of 72 seyfert galaxies and quasars observed by the it far ultraviolet spectroscopic explorer fuse we have determined that 72 of 253 available active galactic nuclei agn targets are viable targets for detection of intrinsic absorption lines we examined these spectra for signs of intrinsic absorption ... | [['we', 'present', 'a', 'survey', 'of', '72', 'seyfert', 'galaxies', 'and', 'quasars', 'observed', 'by', 'the', 'it', 'far', 'ultraviolet', 'spectroscopic', 'explorer', 'fuse', 'we', 'have', 'determined', 'that', '72', 'of', '253', 'available', 'active', 'galactic', 'nuclei', 'agn', 'targets', 'are', 'viable', 'targets... | [-0.0020591189595728704, 0.06263524601406349, -0.0031890108096754043, 0.0748625052801799, -0.08475495203364096, -0.1072496286360547, 0.06946119249133938, 0.4823335413707466, -0.08386091887099077, -0.3574070142650914, 0.019072466606569544, -0.35526815885337204, 0.006675091445752669, 0.1525302961037108, 0.011540639403037... |
706.3054 | The perfect lens on a finite bandwidth | The resolution associated with the so-called perfect lens of thickness $d$ is
$-2\pi d/\ln(|\chi+2|/2)$. Here the susceptibility $\chi$ is a Hermitian
function in $H^2$ of the upper half-plane, i.e., a $H^2$ function satisfying
$\chi(-\omega)=\bar{\chi(\omega)}$. An additional requirement is that the
imaginary part o... | physics.optics | the resolution associated with the socalled perfect lens of thickness d is 2pi dlnchi22 here the susceptibility chi is a hermitian function in h2 of the upper halfplane ie a h2 function satisfying chiomegabarchiomega an additional requirement is that the imaginary part of chi be nonnegative for nonnegative arguments gi... | [['the', 'resolution', 'associated', 'with', 'the', 'socalled', 'perfect', 'lens', 'of', 'thickness', 'd', 'is', '2pi', 'dlnchi22', 'here', 'the', 'susceptibility', 'chi', 'is', 'a', 'hermitian', 'function', 'in', 'h2', 'of', 'the', 'upper', 'halfplane', 'ie', 'a', 'h2', 'function', 'satisfying', 'chiomegabarchiomega',... | [-0.1702472850887312, 0.08173918897163175, -0.06578826021092633, 0.02694247384271067, -0.11154098722876774, -0.1278561437036842, 0.043173443256980845, 0.3524088295900987, -0.25549117732379173, -0.22438861239287589, 0.09184634905411965, -0.27721065581879684, -0.12452384018753138, 0.17873218275813593, -0.0383334682982725... |
706.3055 | A primer on the (2+1) Einstein universe | The Einstein universe is the conformal compactification of Minkowski space.
It also arises as the ideal boundary of anti-de Sitter space. The purpose of
this article is to develop the synthetic geometry of the Einstein universe in
terms of its homogeneous submanifolds and causal structure, with particular
emphasis on... | math.DG | the einstein universe is the conformal compactification of minkowski space it also arises as the ideal boundary of antide sitter space the purpose of this article is to develop the synthetic geometry of the einstein universe in terms of its homogeneous submanifolds and causal structure with particular emphasis on dimen... | [['the', 'einstein', 'universe', 'is', 'the', 'conformal', 'compactification', 'of', 'minkowski', 'space', 'it', 'also', 'arises', 'as', 'the', 'ideal', 'boundary', 'of', 'antide', 'sitter', 'space', 'the', 'purpose', 'of', 'this', 'article', 'is', 'to', 'develop', 'the', 'synthetic', 'geometry', 'of', 'the', 'einstein... | [-0.14659994965299003, 0.10317579129590623, -0.08347523713018745, 0.11122381851272357, -0.13290745938467163, -0.07766259718506087, -0.09729070602465541, 0.3142595432939068, -0.20068597583280456, -0.2235798485794916, 0.13321414333392656, -0.2257529048309211, -0.17644470981172017, 0.12836738929693256, -0.0843176124241924... |
706.3056 | Neutrino-driven explosions twenty years after SN1987A | The neutrino-heating mechanism remains a viable possibility for the cause of
the explosion in a wide mass range of supernova progenitors. This is
demonstrated by recent two-dimensional hydrodynamic simulations with detailed,
energy-dependent neutrino transport. Neutrino-driven explosions were not only
found for stars... | astro-ph | the neutrinoheating mechanism remains a viable possibility for the cause of the explosion in a wide mass range of supernova progenitors this is demonstrated by recent twodimensional hydrodynamic simulations with detailed energydependent neutrino transport neutrinodriven explosions were not only found for stars in the r... | [['the', 'neutrinoheating', 'mechanism', 'remains', 'a', 'viable', 'possibility', 'for', 'the', 'cause', 'of', 'the', 'explosion', 'in', 'a', 'wide', 'mass', 'range', 'of', 'supernova', 'progenitors', 'this', 'is', 'demonstrated', 'by', 'recent', 'twodimensional', 'hydrodynamic', 'simulations', 'with', 'detailed', 'ene... | [-0.11477082505717123, 0.22890761155612405, 0.01870124037775052, 0.1487578243746922, -0.1055041433268698, -0.0882111103444292, 0.026094756240348856, 0.33159022834208773, -0.18435192113833093, -0.3253510187766174, 0.08493693931263917, -0.2196305698252018, -0.05116404679450547, 0.23787506141347764, 0.006527214846245464, ... |
706.3057 | The characteristic polynomial on compact groups with Haar measure : some
equalities in law | This note presents some equalities in law for $Z_N:=\det(\Id-G)$, where $G$
is an element of a subgroup of the set of unitary matrices of size $N$, endowed
with its unique probability Haar measure. Indeed, under some general
conditions, $Z_N$ can be decomposed as a product of independent random
variables, whose laws ... | math.PR math-ph math.MP | this note presents some equalities in law for z_ndetidg where g is an element of a subgroup of the set of unitary matrices of size n endowed with its unique probability haar measure indeed under some general conditions z_n can be decomposed as a product of independent random variables whose laws are explicitly known ou... | [['this', 'note', 'presents', 'some', 'equalities', 'in', 'law', 'for', 'z_ndetidg', 'where', 'g', 'is', 'an', 'element', 'of', 'a', 'subgroup', 'of', 'the', 'set', 'of', 'unitary', 'matrices', 'of', 'size', 'n', 'endowed', 'with', 'its', 'unique', 'probability', 'haar', 'measure', 'indeed', 'under', 'some', 'general',... | [-0.13325713444852605, 0.12792884928895323, -0.09928024952071456, -0.016410253758603742, -0.0332823214977804, -0.10720366820306429, 0.045616173033848545, 0.3481778886964334, -0.2937130820146709, -0.2261901554977741, 0.14929503512970735, -0.2536773933800605, -0.13892664226817564, 0.1910416545886722, -0.13351410767063498... |
706.3058 | Size Effects in the Magnetoresistance of Graphite: Absence of
Magnetoresistance in Micrometer size Samples | We present a study of the magnetoresistance of highly oriented pyrolytic
graphite (HOPG) as a function of the sample size. Our results show
unequivocally that the magnetoresistance reduces with the sample size even for
samples of hundreds of micrometers size. This sample size effect is due the
large mean free path an... | cond-mat.mes-hall cond-mat.mtrl-sci | we present a study of the magnetoresistance of highly oriented pyrolytic graphite hopg as a function of the sample size our results show unequivocally that the magnetoresistance reduces with the sample size even for samples of hundreds of micrometers size this sample size effect is due the large mean free path and ferm... | [['we', 'present', 'a', 'study', 'of', 'the', 'magnetoresistance', 'of', 'highly', 'oriented', 'pyrolytic', 'graphite', 'hopg', 'as', 'a', 'function', 'of', 'the', 'sample', 'size', 'our', 'results', 'show', 'unequivocally', 'that', 'the', 'magnetoresistance', 'reduces', 'with', 'the', 'sample', 'size', 'even', 'for', ... | [-0.08393834595221515, 0.18071523456213376, -0.05688375337779814, 0.0018824144430896815, -0.046027559965081954, -0.10576959181230004, 0.07897877707328721, 0.4035961076836376, -0.23539404964129276, -0.3571431121295866, 0.03263623007303834, -0.2957713897066081, -0.08492182308406222, 0.2253701473659306, -0.053153766720902... |
706.3059 | Jet lag effect and leading hadron production | We propose a solution for the long standing puzzle of a too steeply falling
fragmentation function for a quark fragmenting into a pion, calculated by
Berger [1] in the Born approximation. Contrary to the simple anticipation that
gluon resummation worsens the problem, we find good agreement with data. Higher
quark Foc... | hep-ph nucl-th | we propose a solution for the long standing puzzle of a too steeply falling fragmentation function for a quark fragmenting into a pion calculated by berger 1 in the born approximation contrary to the simple anticipation that gluon resummation worsens the problem we find good agreement with data higher quark fock states... | [['we', 'propose', 'a', 'solution', 'for', 'the', 'long', 'standing', 'puzzle', 'of', 'a', 'too', 'steeply', 'falling', 'fragmentation', 'function', 'for', 'a', 'quark', 'fragmenting', 'into', 'a', 'pion', 'calculated', 'by', 'berger', '1', 'in', 'the', 'born', 'approximation', 'contrary', 'to', 'the', 'simple', 'antic... | [-0.06175466658813613, 0.208843511228943, -0.15827004504611805, 0.19079747706141678, -0.06972072527167343, -0.06491055573292431, 0.05464833569491193, 0.3616682653803201, -0.1919938452719223, -0.23018806205973738, 0.01122499622759365, -0.2603071268647909, -0.03445742114314011, 0.11194847068261532, -0.009027200218822275,... |
706.306 | N-Body Simulations on GPUs | Commercial graphics processors (GPUs) have high compute capacity at very low
cost, which makes them attractive for general purpose scientific computing. In
this paper we show how graphics processors can be used for N-body simulations
to obtain improvements in performance over current generation CPUs. We have
develope... | cs.CE cs.DC | commercial graphics processors gpus have high compute capacity at very low cost which makes them attractive for general purpose scientific computing in this paper we show how graphics processors can be used for nbody simulations to obtain improvements in performance over current generation cpus we have developed a high... | [['commercial', 'graphics', 'processors', 'gpus', 'have', 'high', 'compute', 'capacity', 'at', 'very', 'low', 'cost', 'which', 'makes', 'them', 'attractive', 'for', 'general', 'purpose', 'scientific', 'computing', 'in', 'this', 'paper', 'we', 'show', 'how', 'graphics', 'processors', 'can', 'be', 'used', 'for', 'nbody',... | [-0.13859555732135562, 0.030505232464003548, -0.050528975869413496, 0.010540142847794639, -0.03679899191137496, -0.1275143515518751, 0.027689093059075087, 0.44443688107546697, -0.22766252025222974, -0.4020482632216097, 0.08470714380599036, -0.2477330150436764, -0.10450706993275868, 0.31371185577990224, -0.0380786033385... |
706.3061 | Pump-probe polarized transient hole burning (PTHB) dynamics of hydrated
electron revisited | Femtosecond PTHB spectroscopy was expected to demonstrate the existence of
distinct s-p absorption subbands originating from the three nondegenerate
p-like excited states of hydrated electron in anisotropic solvation cavity. Yet
no conclusive experimental evidence either for this subband structure or the
reorientatio... | physics.chem-ph | femtosecond pthb spectroscopy was expected to demonstrate the existence of distinct sp absorption subbands originating from the three nondegenerate plike excited states of hydrated electron in anisotropic solvation cavity yet no conclusive experimental evidence either for this subband structure or the reorientation of ... | [['femtosecond', 'pthb', 'spectroscopy', 'was', 'expected', 'to', 'demonstrate', 'the', 'existence', 'of', 'distinct', 'sp', 'absorption', 'subbands', 'originating', 'from', 'the', 'three', 'nondegenerate', 'plike', 'excited', 'states', 'of', 'hydrated', 'electron', 'in', 'anisotropic', 'solvation', 'cavity', 'yet', 'n... | [-0.12143451415035951, 0.21998380361240089, -0.06440203997892202, 0.08485348235225286, -0.0376926072028264, -0.120516447876052, 0.01759408242741273, 0.4523025460963704, -0.27168898710731376, -0.2906488721287742, 0.05903350107957484, -0.28098226592098313, -0.048597209263573755, 0.15625748583403676, 0.04924059472978115, ... |
706.3062 | Carbon Detonation and Shock-Triggered Helium Burning in Neutron Star
Superbursts | The strong degeneracy of the 12C ignition layer on an accreting neutron star
results in a hydrodynamic thermonuclear runaway, in which the nuclear heating
time becomes shorter than the local dynamical time. We model the resulting
combustion wave during these superbursts as an upward propagating detonation.
We solve t... | astro-ph | the strong degeneracy of the 12c ignition layer on an accreting neutron star results in a hydrodynamic thermonuclear runaway in which the nuclear heating time becomes shorter than the local dynamical time we model the resulting combustion wave during these superbursts as an upward propagating detonation we solve the re... | [['the', 'strong', 'degeneracy', 'of', 'the', '12c', 'ignition', 'layer', 'on', 'an', 'accreting', 'neutron', 'star', 'results', 'in', 'a', 'hydrodynamic', 'thermonuclear', 'runaway', 'in', 'which', 'the', 'nuclear', 'heating', 'time', 'becomes', 'shorter', 'than', 'the', 'local', 'dynamical', 'time', 'we', 'model', 't... | [-0.07128905519393497, 0.23510607996072866, -0.029393371215676246, 0.0763085820985123, -0.07177301923792552, -0.09859612983789953, 0.06514640743362493, 0.3715389345427333, -0.24256779277368032, -0.2767160237236912, 0.05855499683419676, -0.31758132012127416, -0.026575450351911372, 0.18862716545218378, 0.0144967144066146... |
706.3063 | Self-similar shear-thickening behavior in CTAB/NaSal surfactant
solutions | The effect of salt concentration Cs on the critical shear rate required for
the onset of shear thickening and apparent relaxation time of the
shear-thickened phase, has been investigated systematically for dilute
CTAB/NaSal solutions. Experimental data suggest a self-similar behavior of the
critical shear rate and re... | physics.flu-dyn | the effect of salt concentration cs on the critical shear rate required for the onset of shear thickening and apparent relaxation time of the shearthickened phase has been investigated systematically for dilute ctabnasal solutions experimental data suggest a selfsimilar behavior of the critical shear rate and relaxatio... | [['the', 'effect', 'of', 'salt', 'concentration', 'cs', 'on', 'the', 'critical', 'shear', 'rate', 'required', 'for', 'the', 'onset', 'of', 'shear', 'thickening', 'and', 'apparent', 'relaxation', 'time', 'of', 'the', 'shearthickened', 'phase', 'has', 'been', 'investigated', 'systematically', 'for', 'dilute', 'ctabnasal'... | [-0.15527889711504234, 0.18736433217970813, -0.10749806830642263, -0.013502182900319222, -0.008918554547967182, -0.11143213920553939, 0.040600126282596544, 0.31351548283688585, -0.2790432983526477, -0.24007817525017783, 0.0786544227190057, -0.2316513300153289, -0.1347856130397068, 0.15472177529483344, 0.020202334474931... |
706.3064 | Growing Matter | We investigate quintessence cosmologies with a matter component consisting of
particles with an increasing mass. While negligible in early cosmology, the
appearance of a growing matter component has stopped the evolution of the
cosmon field at a redshift around six. In turn, this has triggered the
accelerated expansi... | astro-ph hep-ph hep-th | we investigate quintessence cosmologies with a matter component consisting of particles with an increasing mass while negligible in early cosmology the appearance of a growing matter component has stopped the evolution of the cosmon field at a redshift around six in turn this has triggered the accelerated expansion of ... | [['we', 'investigate', 'quintessence', 'cosmologies', 'with', 'a', 'matter', 'component', 'consisting', 'of', 'particles', 'with', 'an', 'increasing', 'mass', 'while', 'negligible', 'in', 'early', 'cosmology', 'the', 'appearance', 'of', 'a', 'growing', 'matter', 'component', 'has', 'stopped', 'the', 'evolution', 'of', ... | [-0.1406299504149076, 0.2363696814979224, -0.11531111450875715, 0.060149317636009454, -0.05320252458770554, -0.06773588326215357, -0.050812072132701995, 0.3122851959809165, -0.2056375260815605, -0.34888592735688845, 0.044335032943273324, -0.2909576219065091, 0.012910897541162255, 0.10249738557288399, 0.0492933904510233... |
706.3065 | Double Chargino Production in $e^{-}e^{-}$ scattering | We point out the production of the charginos and neutralinos in
electron-electron process in several supersymmetric models, in order to show
that the International Linear Collider can discover double charged charginos if
these particles really exist in nature.
| hep-ph hep-ex | we point out the production of the charginos and neutralinos in electronelectron process in several supersymmetric models in order to show that the international linear collider can discover double charged charginos if these particles really exist in nature | [['we', 'point', 'out', 'the', 'production', 'of', 'the', 'charginos', 'and', 'neutralinos', 'in', 'electronelectron', 'process', 'in', 'several', 'supersymmetric', 'models', 'in', 'order', 'to', 'show', 'that', 'the', 'international', 'linear', 'collider', 'can', 'discover', 'double', 'charged', 'charginos', 'if', 'th... | [-0.10336857787823599, 0.2579389493177204, -0.06022233369539639, 0.19660980203733694, -0.026132596092984864, -0.18359624824829793, 0.018307834667594808, 0.3536050653967418, -0.28501061195703714, -0.258665288847528, 0.011882475093252173, -0.3625777369659198, -0.0574400220066309, 0.14909791872885667, 0.06081708035382785,... |
706.3066 | Dielectric microscopy with submillimeter resolution | In analogy with optical near-field scanning methods, we use tapered
dielectric waveguides as probes for a millimeter wave vector network analyzer.
By scanning thin samples between two such probes we are able to map the
spatially varying dielectric properties of materials with sub-wavelength
resolution; using a 150 GH... | cond-mat.soft cond-mat.mtrl-sci | in analogy with optical nearfield scanning methods we use tapered dielectric waveguides as probes for a millimeter wave vector network analyzer by scanning thin samples between two such probes we are able to map the spatially varying dielectric properties of materials with subwavelength resolution using a 150 ghz probe... | [['in', 'analogy', 'with', 'optical', 'nearfield', 'scanning', 'methods', 'we', 'use', 'tapered', 'dielectric', 'waveguides', 'as', 'probes', 'for', 'a', 'millimeter', 'wave', 'vector', 'network', 'analyzer', 'by', 'scanning', 'thin', 'samples', 'between', 'two', 'such', 'probes', 'we', 'are', 'able', 'to', 'map', 'the... | [-0.08173155385955441, 0.12310665528994144, -0.0545425013690142, -0.046284548178735396, -0.043340733218029504, -0.16437090249027966, 0.004141348150059036, 0.5505835700598432, -0.2517080525526913, -0.2996884886993141, 0.06210602037097532, -0.3068321810626402, -0.15559583863743195, 0.226933104974195, 0.02430871131875348,... |
706.3067 | Fitting analysis provides further evidence for eradication of hiv/aids
infection under combined liposome drug delivery treatment | It is now evident that the commonly accepted strategy for treatment of
HIV/AIDS by highly active antiretroviral therapy (HAART) will not lead to
eradication of HIV in a reasonable time. This is straightforward from the
typical exponential viral load decay upon treatment revealing initial
considerable but incomplete r... | q-bio.TO | it is now evident that the commonly accepted strategy for treatment of hivaids by highly active antiretroviral therapy haart will not lead to eradication of hiv in a reasonable time this is straightforward from the typical exponential viral load decay upon treatment revealing initial considerable but incomplete reducti... | [['it', 'is', 'now', 'evident', 'that', 'the', 'commonly', 'accepted', 'strategy', 'for', 'treatment', 'of', 'hivaids', 'by', 'highly', 'active', 'antiretroviral', 'therapy', 'haart', 'will', 'not', 'lead', 'to', 'eradication', 'of', 'hiv', 'in', 'a', 'reasonable', 'time', 'this', 'is', 'straightforward', 'from', 'the'... | [-0.05360992606541123, 0.15065170498094474, -0.08498977662788497, 0.12615474419329653, -0.07246599299362813, -0.2272458569936906, 0.13059318268370598, 0.3817145183230891, -0.17782684436274898, -0.2410994368426577, 0.0991757465373593, -0.2231588012943364, -0.192640383238669, 0.1815515925468068, -0.13721037145722845, 0.0... |
706.3068 | A 12um ISOCAM Survey of the ESO-Sculptor Field: Data Reduction and
Analysis | We present a detailed reduction of a mid-infrared 12um (LW10 filter) ISOCAM
open time observation performed on the ESO-Sculptor Survey field (Arnouts et
al. 1997). A complete catalogue of 142 sources (120 galaxies and 22 stars),
detected with high significance (equivalent to 5sigma), is presented above an
integrated ... | astro-ph | we present a detailed reduction of a midinfrared 12um lw10 filter isocam open time observation performed on the esosculptor survey field arnouts et al 1997 a complete catalogue of 142 sources 120 galaxies and 22 stars detected with high significance equivalent to 5sigma is presented above an integrated flux density of ... | [['we', 'present', 'a', 'detailed', 'reduction', 'of', 'a', 'midinfrared', '12um', 'lw10', 'filter', 'isocam', 'open', 'time', 'observation', 'performed', 'on', 'the', 'esosculptor', 'survey', 'field', 'arnouts', 'et', 'al', '1997', 'a', 'complete', 'catalogue', 'of', '142', 'sources', '120', 'galaxies', 'and', '22', '... | [-0.01589779957677379, 0.024384890185055238, -0.10325872782533142, 0.1076173051457965, -0.1038499973347467, -0.026515505925724, 0.1085084294378193, 0.457659599111613, -0.09026430590699117, -0.3983950520047184, 0.052755707397238547, -0.3069265125912021, -0.04149546433578838, 0.19194998899333632, -0.08717775757452756, 0.... |
706.3069 | Network synchronization: Spectral versus statistical properties | We consider synchronization of weighted networks, possibly with asymmetrical
connections. We show that the synchronizability of the networks cannot be
directly inferred from their statistical properties. Small local changes in the
network structure can sensitively affect the eigenvalues relevant for
synchronization, ... | cond-mat.dis-nn nlin.AO | we consider synchronization of weighted networks possibly with asymmetrical connections we show that the synchronizability of the networks cannot be directly inferred from their statistical properties small local changes in the network structure can sensitively affect the eigenvalues relevant for synchronization while ... | [['we', 'consider', 'synchronization', 'of', 'weighted', 'networks', 'possibly', 'with', 'asymmetrical', 'connections', 'we', 'show', 'that', 'the', 'synchronizability', 'of', 'the', 'networks', 'can', 'not', 'be', 'directly', 'inferred', 'from', 'their', 'statistical', 'properties', 'small', 'local', 'changes', 'in', ... | [-0.17045422523176368, 0.08120165175840824, -0.0637571163522669, 0.10437778521423476, -0.03209663933449531, -0.1285054169217997, 0.020394332509464288, 0.4151886993005306, -0.3624082136946388, -0.3244966338801233, 0.05313640709559704, -0.23687822276820678, -0.22043916128009935, 0.11311705857279557, -0.0637115776963249, ... |
706.307 | Potential for the slow-roll inflation, mass scale hierarchy and Dark
Energy from the Type IIA supergravity | The magnetic fluxbrane solution with a strongly warped throat is studied in
the Type IIA supergravity theory with co-dimension one local source which
surves as $Z_{2}$-symmetric UV boundary of the throat. Overall volume of extra
space is stabilized since introduction of the local source breaks the no-scale
structure ... | hep-th | the magnetic fluxbrane solution with a strongly warped throat is studied in the type iia supergravity theory with codimension one local source which surves as z_2symmetric uv boundary of the throat overall volume of extra space is stabilized since introduction of the local source breaks the noscale structure of the the... | [['the', 'magnetic', 'fluxbrane', 'solution', 'with', 'a', 'strongly', 'warped', 'throat', 'is', 'studied', 'in', 'the', 'type', 'iia', 'supergravity', 'theory', 'with', 'codimension', 'one', 'local', 'source', 'which', 'surves', 'as', 'z_2symmetric', 'uv', 'boundary', 'of', 'the', 'throat', 'overall', 'volume', 'of', ... | [-0.17140512589386778, 0.1351200854284635, -0.07226918028086166, 0.11795110285593025, -0.09666661243795584, -0.19832303383484526, 0.003066088108620418, 0.27417702718524833, -0.22269658399126735, -0.2980921102870751, 0.1010067703651878, -0.25376753864077733, -0.0864854797177862, 0.13080387905299276, -0.05795530843662200... |
706.3071 | Extreme values for Benedicks-Carleson quadratic maps | We consider the quadratic family of maps given by $f_{a}(x)=1-a x^2$ with
$x\in [-1,1]$, where $a$ is a Benedicks-Carleson parameter. For each of these
chaotic dynamical systems we study the extreme value distribution of the
stationary stochastic processes $X_0,X_1,...$, given by $X_{n}=f_a^n$, for
every integer $n\g... | math.DS math.PR math.ST stat.TH | we consider the quadratic family of maps given by f_ax1a x2 with xin 11 where a is a benedickscarleson parameter for each of these chaotic dynamical systems we study the extreme value distribution of the stationary stochastic processes x_0x_1 given by x_nf_an for every integer ngeq0 where each random variable x_n is di... | [['we', 'consider', 'the', 'quadratic', 'family', 'of', 'maps', 'given', 'by', 'f_ax1a', 'x2', 'with', 'xin', '11', 'where', 'a', 'is', 'a', 'benedickscarleson', 'parameter', 'for', 'each', 'of', 'these', 'chaotic', 'dynamical', 'systems', 'we', 'study', 'the', 'extreme', 'value', 'distribution', 'of', 'the', 'stationa... | [-0.12681925935892885, 0.1499014166376015, -0.108968809075064, 0.031986894281452884, -0.02516733266310681, -0.15747384637820647, 0.041813222000401024, 0.34107863767192176, -0.3049779778363508, -0.1996469443638322, 0.11650998744667175, -0.25844124042647443, -0.13323283559266785, 0.16763120804221257, -0.09440071431390189... |
706.3072 | Efficient vibrational state coupling in an optical tilted-washboard
potential via multiple spatial translations and application to pulse echo | We measure the application of simple and compound pulses consisting of
time-dependent spatial translations to coupling vibrational states of ultracold
85Rb atoms in a far-detuned 1D optical lattice. The lattice wells are so
shallow as to support only two bound states, and we prepare the atoms in the
ground state. The... | quant-ph | we measure the application of simple and compound pulses consisting of timedependent spatial translations to coupling vibrational states of ultracold 85rb atoms in a fardetuned 1d optical lattice the lattice wells are so shallow as to support only two bound states and we prepare the atoms in the ground state the lattic... | [['we', 'measure', 'the', 'application', 'of', 'simple', 'and', 'compound', 'pulses', 'consisting', 'of', 'timedependent', 'spatial', 'translations', 'to', 'coupling', 'vibrational', 'states', 'of', 'ultracold', '85rb', 'atoms', 'in', 'a', 'fardetuned', '1d', 'optical', 'lattice', 'the', 'lattice', 'wells', 'are', 'so'... | [-0.09507391767233218, 0.20041744948911758, -0.07194410527864026, 0.054984809831256115, -0.0016827215468850334, -0.15239329280723868, 0.04977159438700027, 0.5012318802703368, -0.2289571034503339, -0.244296180240825, 0.05370556320410659, -0.2766891751836171, -0.0953298393110952, 0.22863361054017145, 0.007282859981361671... |
706.3073 | Tau-function of discrete isomonodromy transformations and probability | We introduce the tau-function of a rational d-connection and its isomonodromy
transformations. We show that in a continuous limit our tau-function agrees
with the Jimbo-Miwa-Ueno tau-function, compute the tau-function for the
isomonodromy transformations leading to difference Painleve V and difference
Painleve VI equ... | math.AG math-ph math.MP math.PR | we introduce the taufunction of a rational dconnection and its isomonodromy transformations we show that in a continuous limit our taufunction agrees with the jimbomiwaueno taufunction compute the taufunction for the isomonodromy transformations leading to difference painleve v and difference painleve vi equations and ... | [['we', 'introduce', 'the', 'taufunction', 'of', 'a', 'rational', 'dconnection', 'and', 'its', 'isomonodromy', 'transformations', 'we', 'show', 'that', 'in', 'a', 'continuous', 'limit', 'our', 'taufunction', 'agrees', 'with', 'the', 'jimbomiwaueno', 'taufunction', 'compute', 'the', 'taufunction', 'for', 'the', 'isomono... | [-0.1416972719564818, -0.015691584586697307, -0.06871278332276405, 0.11486586090177298, -0.0996677120472642, -0.1430480160035085, 0.004810210560326991, 0.2844481666072987, -0.3594562457739443, -0.18586837542175816, 0.061705156838507864, -0.27239669459885446, -0.23140276774116184, 0.18033083072067171, -0.111359180862326... |
706.3074 | A review of wildland fire spread modelling, 1990-present, 1: Physical
and quasi-physical models | In recent years, advances in computational power and spatial data analysis
(GIS, remote sensing, etc) have led to an increase in attempts to model the
spread and behaviour of wildland fires across the landscape. This series of
review papers endeavours to critically and comprehensively review all types of
surface fire... | physics.geo-ph physics.ao-ph physics.flu-dyn | in recent years advances in computational power and spatial data analysis gis remote sensing etc have led to an increase in attempts to model the spread and behaviour of wildland fires across the landscape this series of review papers endeavours to critically and comprehensively review all types of surface fire spread ... | [['in', 'recent', 'years', 'advances', 'in', 'computational', 'power', 'and', 'spatial', 'data', 'analysis', 'gis', 'remote', 'sensing', 'etc', 'have', 'led', 'to', 'an', 'increase', 'in', 'attempts', 'to', 'model', 'the', 'spread', 'and', 'behaviour', 'of', 'wildland', 'fires', 'across', 'the', 'landscape', 'this', 's... | [-0.021618336032617896, 0.0653659432862168, -0.058713966287717585, 0.05398473911730933, -0.05774849097079207, -0.10784621527906688, 0.018622494266075533, 0.3640184106320263, -0.2370831789749284, -0.34735226138464864, 0.16289864224757278, -0.30841495669371777, -0.202618106151931, 0.2167405653519616, -0.10869241092399123... |
706.3075 | Stochastic Lorentz forces on a point charge moving near the conducting
plate | The influence of quantized electromagnetic fields on a nonrelativistic
charged particle moving near a conducting plate is studied. We give a
field-theoretic derivation of the nonlinear, non-Markovian Langevin equation of
the particle by the method of Feynman-Vernon influence functional. This
stochastic approach incor... | hep-th quant-ph | the influence of quantized electromagnetic fields on a nonrelativistic charged particle moving near a conducting plate is studied we give a fieldtheoretic derivation of the nonlinear nonmarkovian langevin equation of the particle by the method of feynmanvernon influence functional this stochastic approach incorporates ... | [['the', 'influence', 'of', 'quantized', 'electromagnetic', 'fields', 'on', 'a', 'nonrelativistic', 'charged', 'particle', 'moving', 'near', 'a', 'conducting', 'plate', 'is', 'studied', 'we', 'give', 'a', 'fieldtheoretic', 'derivation', 'of', 'the', 'nonlinear', 'nonmarkovian', 'langevin', 'equation', 'of', 'the', 'par... | [-0.1594672242317618, 0.19607755553752834, -0.0949837879238813, 0.05673123261990458, -0.047862416101414215, -0.08579280929632853, -0.015169518990127879, 0.32511346659732865, -0.27298553138369336, -0.25860496454238324, 0.08329565125692834, -0.25917069613225335, -0.09227972957588902, 0.18180604304758896, 0.00986020181668... |
706.3076 | On the Performance of Joint Fingerprint Embedding and Decryption Scheme | Till now, few work has been done to analyze the performances of joint
fingerprint embedding and decryption schemes. In this paper, the security of
the joint fingerprint embedding and decryption scheme proposed by Kundur et al.
is analyzed and improved. The analyses include the security against
unauthorized customer, ... | cs.MM cs.CR | till now few work has been done to analyze the performances of joint fingerprint embedding and decryption schemes in this paper the security of the joint fingerprint embedding and decryption scheme proposed by kundur et al is analyzed and improved the analyses include the security against unauthorized customer the secu... | [['till', 'now', 'few', 'work', 'has', 'been', 'done', 'to', 'analyze', 'the', 'performances', 'of', 'joint', 'fingerprint', 'embedding', 'and', 'decryption', 'schemes', 'in', 'this', 'paper', 'the', 'security', 'of', 'the', 'joint', 'fingerprint', 'embedding', 'and', 'decryption', 'scheme', 'proposed', 'by', 'kundur',... | [-0.12985753862934266, -0.08046433513475305, -0.09953246123364402, 0.06686041126980584, -0.0710530247953203, -0.25328685668366097, 0.11235446431264454, 0.38313505056969543, -0.27434714671862487, -0.32983478034536046, 0.13649835594804716, -0.27909122969679256, -0.1506120874977636, 0.2037346984208044, -0.1723221315855712... |
706.3077 | Exact solution of the Faddeev-Volkov model | The Faddeev-Volkov model is an Ising-type lattice model with positive
Boltzmann weights where the spin variables take continuous values on the real
line. It serves as a lattice analog of the sinh-Gordon and Liouville models and
intimately connected with the modular double of the quantum group U_q(sl_2).
The free ener... | cond-mat.stat-mech hep-th math-ph math.MP | the faddeevvolkov model is an isingtype lattice model with positive boltzmann weights where the spin variables take continuous values on the real line it serves as a lattice analog of the sinhgordon and liouville models and intimately connected with the modular double of the quantum group u_qsl_2 the free energy of the... | [['the', 'faddeevvolkov', 'model', 'is', 'an', 'isingtype', 'lattice', 'model', 'with', 'positive', 'boltzmann', 'weights', 'where', 'the', 'spin', 'variables', 'take', 'continuous', 'values', 'on', 'the', 'real', 'line', 'it', 'serves', 'as', 'a', 'lattice', 'analog', 'of', 'the', 'sinhgordon', 'and', 'liouville', 'mo... | [-0.12958563380308596, 0.13611569441070293, -0.09591667198429943, 0.06313171620850506, -0.04183216248559035, -0.17623425608354748, 0.014152622484948998, 0.2726024934341766, -0.29144287023547233, -0.18398316556989563, 0.07173103786543851, -0.27600707900573446, -0.13396472465612141, 0.157806551152402, -0.0174539768657482... |
706.3078 | Index Theorem in Finite Noncommutative Geometry | Index theorem is formulated in noncommutative geometry with finite degrees of
freedom by using Ginsparg-Wilson relation. It is extended to the case where the
gauge symmetry is spontaneously broken. Dynamical analysis about topological
aspects in gauge theory is also shown.
| hep-th hep-lat | index theorem is formulated in noncommutative geometry with finite degrees of freedom by using ginspargwilson relation it is extended to the case where the gauge symmetry is spontaneously broken dynamical analysis about topological aspects in gauge theory is also shown | [['index', 'theorem', 'is', 'formulated', 'in', 'noncommutative', 'geometry', 'with', 'finite', 'degrees', 'of', 'freedom', 'by', 'using', 'ginspargwilson', 'relation', 'it', 'is', 'extended', 'to', 'the', 'case', 'where', 'the', 'gauge', 'symmetry', 'is', 'spontaneously', 'broken', 'dynamical', 'analysis', 'about', 't... | [-0.14632046384213027, 0.23857049318030477, -0.1534415737609379, 0.10002858318621292, -0.10452595589449629, -0.16149950692488346, -0.029527822401723823, 0.3151820011902601, -0.24920792640186845, -0.29678923287428916, 0.08538685573148541, -0.23085214868187903, -0.21215048301964998, 0.046612193784676494, -0.0890493872109... |
706.3079 | Revisiting the QCD corrections to the R-parity violating processes
$p\bar{p}/pp \to e\mu+X$ | We present the theoretical predictions up to QCD NLO for the cross section of
high-mass electron-muon pair production at the Tevatron and the LHC,
considering only the dominant contributions from the third-generation
sneutrino. The dependence of the renormalization and factorization scales on
the total cross section,... | hep-ph | we present the theoretical predictions up to qcd nlo for the cross section of highmass electronmuon pair production at the tevatron and the lhc considering only the dominant contributions from the thirdgeneration sneutrino the dependence of the renormalization and factorization scales on the total cross section and the... | [['we', 'present', 'the', 'theoretical', 'predictions', 'up', 'to', 'qcd', 'nlo', 'for', 'the', 'cross', 'section', 'of', 'highmass', 'electronmuon', 'pair', 'production', 'at', 'the', 'tevatron', 'and', 'the', 'lhc', 'considering', 'only', 'the', 'dominant', 'contributions', 'from', 'the', 'thirdgeneration', 'sneutrin... | [-0.07796619741764682, 0.15699446015589108, -0.11963439560812814, 0.1520021844930439, -0.018529670979742976, -0.010291080072585662, 0.011080816468827172, 0.32791238758628344, -0.19014501692303878, -0.26918738447553053, -0.024768438382042488, -0.3682340895757079, 0.06349844169347886, 0.10098041714677079, 0.1108245022531... |
706.308 | Does a black hole rotate in Chern-Simons modified gravity? | Rotating black hole solutions in the (3+1)-dimensional Chern-Simons modified
gravity theory are discussed by taking account of perturbation around the
Schwarzschild solution. The zenith-angle dependence of a metric function
related to the frame-dragging effect is determined from a constraint equation
independently of... | gr-qc | rotating black hole solutions in the 31dimensional chernsimons modified gravity theory are discussed by taking account of perturbation around the schwarzschild solution the zenithangle dependence of a metric function related to the framedragging effect is determined from a constraint equation independently of a choice ... | [['rotating', 'black', 'hole', 'solutions', 'in', 'the', '31dimensional', 'chernsimons', 'modified', 'gravity', 'theory', 'are', 'discussed', 'by', 'taking', 'account', 'of', 'perturbation', 'around', 'the', 'schwarzschild', 'solution', 'the', 'zenithangle', 'dependence', 'of', 'a', 'metric', 'function', 'related', 'to... | [-0.15177609521289548, 0.10524194292716742, -0.0988729501490496, 0.08835773644894952, -0.10232583183189115, -0.14752947948207812, -0.0050200973609684126, 0.2861726592583138, -0.21625270385531678, -0.28378901454723543, 0.0960771321810575, -0.2979258638363154, -0.05191606587715565, 0.1699709758838816, -0.0468186783171924... |
706.3081 | Strong Uniqueness of the Ricci Flow | In this paper, we derive some local a priori estimates for Ricci flow. This
gives rise to some strong uniqueness theorems. As a corollary, let $g(t)$ be a
smooth complete solution to the Ricci flow on $\mathbb{R}^{3}$, with the
canonical Euclidean metric $E$ as initial data, then $g(t)$ is trivial, i.e.
$g(t)\equiv E... | math.DG math.AP | in this paper we derive some local a priori estimates for ricci flow this gives rise to some strong uniqueness theorems as a corollary let gt be a smooth complete solution to the ricci flow on mathbbr3 with the canonical euclidean metric e as initial data then gt is trivial ie gtequiv e | [['in', 'this', 'paper', 'we', 'derive', 'some', 'local', 'a', 'priori', 'estimates', 'for', 'ricci', 'flow', 'this', 'gives', 'rise', 'to', 'some', 'strong', 'uniqueness', 'theorems', 'as', 'a', 'corollary', 'let', 'gt', 'be', 'a', 'smooth', 'complete', 'solution', 'to', 'the', 'ricci', 'flow', 'on', 'mathbbr3', 'with... | [-0.16252103635969645, 0.03502112443899163, -0.15644714368793827, 0.06406606061052746, -0.14582721523654002, -0.18032065235400715, -0.02891429995249312, 0.3106743110916935, -0.27429995882378605, -0.1953660713043064, 0.11651090915592459, -0.27241402223276406, -0.10140694314255737, 0.16492121659953576, -0.139629440361974... |
706.3082 | Configurations of Extremal Even Unimodular Lattices | We extend the results of Ozeki on the configurations of extremal even
unimodular lattices. Specifically, we show that if L is such a lattice of rank
56, 72, or 96, then L is generated by its minimal-norm vectors.
| math.NT | we extend the results of ozeki on the configurations of extremal even unimodular lattices specifically we show that if l is such a lattice of rank 56 72 or 96 then l is generated by its minimalnorm vectors | [['we', 'extend', 'the', 'results', 'of', 'ozeki', 'on', 'the', 'configurations', 'of', 'extremal', 'even', 'unimodular', 'lattices', 'specifically', 'we', 'show', 'that', 'if', 'l', 'is', 'such', 'a', 'lattice', 'of', 'rank', '56', '72', 'or', '96', 'then', 'l', 'is', 'generated', 'by', 'its', 'minimalnorm', 'vectors'... | [-0.15387569054176933, 0.18649374400755683, 0.0023430227853455826, 0.027801261111897856, -0.03349722871605895, -0.13284491699979348, 0.07228933679136007, 0.37882816972897243, -0.23427283085000358, -0.2302750933572258, 0.15895477155419557, -0.3071671470411514, -0.18539779722126887, 0.14921374226258577, -0.04139899169585... |
706.3083 | Perturbative spectrum of a Yukawa-Higgs model with Ginsparg-Wilson
fermions | A Yukawa-Higgs model with Ginsparg-Wilson (GW) fermions, proposed recently by
Bhattacharya, Martin and Poppitz as a possible lattice formulation of chiral
gauge theories, is studied. A simple argument shows that the gauge boson always
acquires mass by the St\"uckelberg (or, in a broad sense, Higgs) mechanism,
regardl... | hep-lat hep-th | a yukawahiggs model with ginspargwilson gw fermions proposed recently by bhattacharya martin and poppitz as a possible lattice formulation of chiral gauge theories is studied a simple argument shows that the gauge boson always acquires mass by the stuckelberg or in a broad sense higgs mechanism regardless of strength o... | [['a', 'yukawahiggs', 'model', 'with', 'ginspargwilson', 'gw', 'fermions', 'proposed', 'recently', 'by', 'bhattacharya', 'martin', 'and', 'poppitz', 'as', 'a', 'possible', 'lattice', 'formulation', 'of', 'chiral', 'gauge', 'theories', 'is', 'studied', 'a', 'simple', 'argument', 'shows', 'that', 'the', 'gauge', 'boson',... | [-0.1916513608037671, 0.31262908562357666, -0.049508053919188444, 0.09026909283438957, -0.1205315244725988, -0.2225298905815882, 0.03435183645968762, 0.31245749038231524, -0.148333334971125, -0.2699626826127119, -0.026352685559364153, -0.23640823588246787, -0.1556199438180303, 0.024659002532805258, 0.02885140913621157,... |
706.3084 | VLA H53alpha observations of the central region of the Super Star
Cluster Galaxy NGC 5253 | We present observations in the H53alpha line and radio continuum at 43 GHz
carried out with the VLA in the D array (2'' angular resolution) toward the
starburst galaxy NGC 5253. VLA archival data have been reprocessed to produce a
uniform set of 2, 1.3 and 0.7 cm high angular (0.''2 X 0.''1) radio continuum
images. T... | astro-ph | we present observations in the h53alpha line and radio continuum at 43 ghz carried out with the vla in the d array 2 angular resolution toward the starburst galaxy ngc 5253 vla archival data have been reprocessed to produce a uniform set of 2 13 and 07 cm high angular 02 x 01 radio continuum images the rrl h53alpha a p... | [['we', 'present', 'observations', 'in', 'the', 'h53alpha', 'line', 'and', 'radio', 'continuum', 'at', '43', 'ghz', 'carried', 'out', 'with', 'the', 'vla', 'in', 'the', 'd', 'array', '2', 'angular', 'resolution', 'toward', 'the', 'starburst', 'galaxy', 'ngc', '5253', 'vla', 'archival', 'data', 'have', 'been', 'reproces... | [-0.08764848253188327, 0.10648771846122558, -0.006522912481820888, 0.03401120537918442, -0.0035500633794899013, -0.05566833175213436, 0.04845386421815916, 0.4469996760493483, -0.09440040339673446, -0.3504094406499379, 0.07211799366500186, -0.28112089686857705, 0.09463113043933515, 0.14309332189507337, -0.00307362381218... |
706.3085 | The optical spectrum of R Coronae Borealis close to 2003 decline | Two sets of high-resolution spectra of R CrB obtained during the 2003 light
decline are described. The first set was obtained on the descending branch of
the light curve when V ~12.0 and the second one in the recovery phase with V
~7.5. The usual sharp and broad emissions are described and the lines radial
velocities... | astro-ph | two sets of highresolution spectra of r crb obtained during the 2003 light decline are described the first set was obtained on the descending branch of the light curve when v 120 and the second one in the recovery phase with v 75 the usual sharp and broad emissions are described and the lines radial velocities measured... | [['two', 'sets', 'of', 'highresolution', 'spectra', 'of', 'r', 'crb', 'obtained', 'during', 'the', '2003', 'light', 'decline', 'are', 'described', 'the', 'first', 'set', 'was', 'obtained', 'on', 'the', 'descending', 'branch', 'of', 'the', 'light', 'curve', 'when', 'v', '120', 'and', 'the', 'second', 'one', 'in', 'the',... | [-0.1137513270988956, 0.09415817432318788, -0.012933772166094211, -0.0005619782708567854, -0.004679872717482047, -0.1547369537744497, 0.04752541762541666, 0.46223563094249115, -0.2309820941387171, -0.32463566582676057, 0.08229337751465006, -0.3354564523759568, -0.014782543537842335, 0.18995782969384584, -0.029291033916... |
706.3086 | Estimates of Gromov's box distance | In 1999, M. Gromov introduced the box distance function $\sikaku$ on the
space of all mm-spaces. In this paper, by using the method of T. H. Colding
(cf. \cite[Lemma 5.10]{Colding}), we estimate
$\sikaku(\mathbb{S}^n,\mathbb{S}^m)$ and $\sikaku (\mathbb{C}P^n,
\mathbb{C}P^m)$, where $\mathbb{S}^n$ is the $n$-dimens... | math.MG | in 1999 m gromov introduced the box distance function sikaku on the space of all mmspaces in this paper by using the method of t h colding cf citelemma 510colding we estimate sikakumathbbsnmathbbsm and sikaku mathbbcpn mathbbcpm where mathbbsn is the ndimensional unit sphere in mathbbrn1 and mathbbcpn is the ndimension... | [['in', '1999', 'm', 'gromov', 'introduced', 'the', 'box', 'distance', 'function', 'sikaku', 'on', 'the', 'space', 'of', 'all', 'mmspaces', 'in', 'this', 'paper', 'by', 'using', 'the', 'method', 'of', 't', 'h', 'colding', 'cf', 'citelemma', '510colding', 'we', 'estimate', 'sikakumathbbsnmathbbsm', 'and', 'sikaku', 'mat... | [-0.1311161938383309, 0.0642356546096528, -0.04067077379413815, 0.0496690757044721, -0.09762902250567582, -0.10814508457863053, 0.019246306033469305, 0.35507350319693254, -0.2057427137028859, -0.2214434894863083, 0.10867513935244101, -0.2790594581720354, -0.17219614134262165, 0.1503278269340436, -0.18699320667791505, -... |
706.3087 | Stark units and main conjectures for totally real fields | Main theorem of [Buyukboduk, arXiv:0706.0377v1] suggests that it should be
possible to lift the Kolyvagin systems of Stark units constructed in
[Buyukboduk, arXiv:math/0703426v1] to a Kolyvagin system over the cyclotomic
Iwasawa algebra. This is what we prove in this paper. This construction gives
the first example t... | math.NT | main theorem of buyukboduk arxiv07060377v1 suggests that it should be possible to lift the kolyvagin systems of stark units constructed in buyukboduk arxivmath0703426v1 to a kolyvagin system over the cyclotomic iwasawa algebra this is what we prove in this paper this construction gives the first example towards a more ... | [['main', 'theorem', 'of', 'buyukboduk', 'arxiv07060377v1', 'suggests', 'that', 'it', 'should', 'be', 'possible', 'to', 'lift', 'the', 'kolyvagin', 'systems', 'of', 'stark', 'units', 'constructed', 'in', 'buyukboduk', 'arxivmath0703426v1', 'to', 'a', 'kolyvagin', 'system', 'over', 'the', 'cyclotomic', 'iwasawa', 'algeb... | [-0.16919333554286478, 0.03060320777738776, -0.16886280809432783, 0.08194728160441596, -0.1139071968681147, -0.12605785727019198, 0.004995080447707582, 0.2675052226585304, -0.3145372846388611, -0.25619215322337274, 0.07583609224269006, -0.20121417490058932, -0.19212798600823716, 0.23700638669783827, -0.1833955334766963... |
706.3088 | Quantum and thermal fluctuations in a two-dimensional correlated band
ferromagnet -- Goldstone-mode preserving investigation with self-energy and
vertex corrections | Ferromagnetism in the t-t' Hubbard model is investigated on a square lattice.
Correlation effects in the form of self-energy and vertex corrections are
systematically incorporated within a spin-rotationally-symmetric scheme which
explicitly preserves the Goldstone mode and is therefore in accord with the
Mermin-Wagne... | cond-mat.str-el | ferromagnetism in the tt hubbard model is investigated on a square lattice correlation effects in the form of selfenergy and vertex corrections are systematically incorporated within a spinrotationallysymmetric scheme which explicitly preserves the goldstone mode and is therefore in accord with the merminwagner theorem... | [['ferromagnetism', 'in', 'the', 'tt', 'hubbard', 'model', 'is', 'investigated', 'on', 'a', 'square', 'lattice', 'correlation', 'effects', 'in', 'the', 'form', 'of', 'selfenergy', 'and', 'vertex', 'corrections', 'are', 'systematically', 'incorporated', 'within', 'a', 'spinrotationallysymmetric', 'scheme', 'which', 'exp... | [-0.16417281527680694, 0.1948499010955812, -0.058849310254581, 0.0799874964404417, -0.010171237988740298, -0.10180607844612624, 0.040364184464682235, 0.3434685563805736, -0.256733961323379, -0.25523110892676515, 0.0207262845849904, -0.33095089441016773, -0.12434386422691947, 0.1514885076278809, 0.04675591944722585, 0.0... |
706.3089 | Can Chandra resolve the remaining cosmic X-ray background? | The deepest extragalactic X-ray observation, the 2 Ms Chandra Deep Field
North (CDF-N), resolves ~80% of the total extragalactic cosmic X-ray background
(CXB) in the 1-2 keV band. Recent work has shown that 70% of the remaining CXB
flux is associated with sources detected by the Hubble Space Telescope (HST).
This pap... | astro-ph | the deepest extragalactic xray observation the 2 ms chandra deep field north cdfn resolves 80 of the total extragalactic cosmic xray background cxb in the 12 kev band recent work has shown that 70 of the remaining cxb flux is associated with sources detected by the hubble space telescope hst this paper uses the existin... | [['the', 'deepest', 'extragalactic', 'xray', 'observation', 'the', '2', 'ms', 'chandra', 'deep', 'field', 'north', 'cdfn', 'resolves', '80', 'of', 'the', 'total', 'extragalactic', 'cosmic', 'xray', 'background', 'cxb', 'in', 'the', '12', 'kev', 'band', 'recent', 'work', 'has', 'shown', 'that', '70', 'of', 'the', 'remai... | [-0.028443250199611497, 0.11303468411288047, -0.03773218995221883, 0.1654232251265448, -0.10195582003759851, -0.06825881642250975, 0.07551455644222961, 0.45501422083143855, -0.12123012569375059, -0.43373192492333695, 0.07252696360709639, -0.37618198722970386, 0.0354154125579502, 0.21080001946519444, -0.0354636817985822... |
706.309 | Flexible-to-semiflexible chain crossover on the pressure-area isotherm
of lipid bilayer | We found theoretically that competition between ~Kq^4 and ~Qq^2 terms in the
Fourier transformed conformational energy of a single lipid chain, in
combination with inter-chain entropic repulsion in the hydrophobic part of the
lipid (bi)layer, may cause a crossover on the bilayer pressure-area isotherm
P(A)~(A-A_0)^{-... | q-bio.QM q-bio.BM | we found theoretically that competition between kq4 and qq2 terms in the fourier transformed conformational energy of a single lipid chain in combination with interchain entropic repulsion in the hydrophobic part of the lipid bilayer may cause a crossover on the bilayer pressurearea isotherm paaa_0n the crossover manif... | [['we', 'found', 'theoretically', 'that', 'competition', 'between', 'kq4', 'and', 'qq2', 'terms', 'in', 'the', 'fourier', 'transformed', 'conformational', 'energy', 'of', 'a', 'single', 'lipid', 'chain', 'in', 'combination', 'with', 'interchain', 'entropic', 'repulsion', 'in', 'the', 'hydrophobic', 'part', 'of', 'the',... | [-0.18625525899232956, 0.2076120781377445, -0.06784010156296692, 0.0027608859407551147, 0.0017412862286969922, -0.18138783870362282, 0.07552864340140052, 0.3440730961806634, -0.31781732812645586, -0.23923122139002373, -0.03514690206118318, -0.32348370132054766, -0.13535479867063901, 0.10314742636599036, 0.0443670279772... |
706.3091 | On the well-posedness of the Cauchy problem for the generalized
Korteweg-de Vries-Burgers equation | Considered is the generalized Korteweg-de Vries-Burgers equation $$
u_{t}+u_{xxx}+uu_{x}+|D_{x}|^{2\alpha}u=0,\quad t\in \mathbb{R}^{+}, x\in
\mathbb{R}, $$ with $0\leq \alpha\le 1$. We prove a sharp results on the
associated Cauchy problem in the Sobolev space $ {H}^s(\mathbb{R})$. For
$s>-\min\{\frac {3+2\alpha}4, ... | math.AP | considered is the generalized kortewegde vriesburgers equation u_tu_xxxuu_xd_x2alphau0quad tin mathbbr xin mathbbr with 0leq alphale 1 we prove a sharp results on the associated cauchy problem in the sobolev space hsmathbbr for sminfrac 32alpha4 1 we give the wellposedness of solutions of the cauchy problem while for f... | [['considered', 'is', 'the', 'generalized', 'kortewegde', 'vriesburgers', 'equation', 'u_tu_xxxuu_xd_x2alphau0quad', 'tin', 'mathbbr', 'xin', 'mathbbr', 'with', '0leq', 'alphale', '1', 'we', 'prove', 'a', 'sharp', 'results', 'on', 'the', 'associated', 'cauchy', 'problem', 'in', 'the', 'sobolev', 'space', 'hsmathbbr', '... | [-0.15773647791205872, 0.027899554266628844, 0.03247917581487585, 0.11431306085540671, -0.02818784243599684, -0.17048548623333099, -0.10009191737130836, 0.310701421186052, -0.3252420904873698, -0.11221964429650041, 0.2021532736403902, -0.4089655738875822, -0.11521540463177694, 0.17373142583744117, -0.08390749789153536,... |
706.3092 | On $(2k)$-Minimal Submanifolds | Recall that a submanifold of a Riemannian manifold is said to be minimal if
its mean curvature is zero. It is classical that minimal submanifolds are the
critical points of the volume function. In this paper, we examine the critical
points of the total $(2k)$-th Gauss-Bonnet curvature function, called
$(2k)$-minimal ... | math.DG | recall that a submanifold of a riemannian manifold is said to be minimal if its mean curvature is zero it is classical that minimal submanifolds are the critical points of the volume function in this paper we examine the critical points of the total 2kth gaussbonnet curvature function called 2kminimal submanifolds we p... | [['recall', 'that', 'a', 'submanifold', 'of', 'a', 'riemannian', 'manifold', 'is', 'said', 'to', 'be', 'minimal', 'if', 'its', 'mean', 'curvature', 'is', 'zero', 'it', 'is', 'classical', 'that', 'minimal', 'submanifolds', 'are', 'the', 'critical', 'points', 'of', 'the', 'volume', 'function', 'in', 'this', 'paper', 'we'... | [-0.22511328123958715, 0.13741883012769093, -0.08760663650436215, 0.13242647168787577, -0.08392222082040396, -0.11322090956550765, -0.03967099111802113, 0.3211083053863686, -0.27212193735078516, -0.19923133851892977, 0.11595970658159041, -0.3080650385895587, -0.22302342913147197, 0.14345850351726613, -0.192536646915397... |
706.3093 | Addendum: "On the nature of the phase transition in the itinerant
helimagnet MnSi", arXiv:cond-mat/0702460v1 [cond-mat.str-el] | New high resolution data for heat capacity, heat capacity under applied
magnetic fields and resistivity of high quality single crystal of MnSi are
reported. Striking mirror symmetry between temperature derivative of
resistivity and thermal expansion coefficient of MnSi is displayed. Close
similarity between variation... | cond-mat.str-el | new high resolution data for heat capacity heat capacity under applied magnetic fields and resistivity of high quality single crystal of mnsi are reported striking mirror symmetry between temperature derivative of resistivity and thermal expansion coefficient of mnsi is displayed close similarity between variation of t... | [['new', 'high', 'resolution', 'data', 'for', 'heat', 'capacity', 'heat', 'capacity', 'under', 'applied', 'magnetic', 'fields', 'and', 'resistivity', 'of', 'high', 'quality', 'single', 'crystal', 'of', 'mnsi', 'are', 'reported', 'striking', 'mirror', 'symmetry', 'between', 'temperature', 'derivative', 'of', 'resistivit... | [-0.1942185036449057, 0.20636457874916675, -0.010792514931115254, -0.040096852075160914, -0.11535139010492258, -0.12307293522285252, 0.09810990216664789, 0.39124350931222845, -0.28287342822224626, -0.30364759625276416, 0.06280502907522931, -0.3244872893683794, -0.08214408089974667, 0.22568211291076207, 0.01231963814395... |
706.3094 | Direct-current control of radiation-induced differential
magnetoresistance oscillations in two-dimensional electron systems | Magnetoresistance oscillations in two-dimensional electron systems driven
simultaneously by a strong direct current and a microwave irradiation, are
analyzed within a unified microscopic scheme treating both excitations on an
equal footing. The microwave-induced resistance oscillations are described by a
parameter $\... | cond-mat.mes-hall | magnetoresistance oscillations in twodimensional electron systems driven simultaneously by a strong direct current and a microwave irradiation are analyzed within a unified microscopic scheme treating both excitations on an equal footing the microwaveinduced resistance oscillations are described by a parameter epsilon_... | [['magnetoresistance', 'oscillations', 'in', 'twodimensional', 'electron', 'systems', 'driven', 'simultaneously', 'by', 'a', 'strong', 'direct', 'current', 'and', 'a', 'microwave', 'irradiation', 'are', 'analyzed', 'within', 'a', 'unified', 'microscopic', 'scheme', 'treating', 'both', 'excitations', 'on', 'an', 'equal'... | [-0.18299059814878502, 0.1899413922700321, 0.01894074245629942, -0.04658101050196873, -0.052646523085879346, -0.121721565928858, 0.08177534623445906, 0.27520087301073703, -0.17958118530976422, -0.32478465045820554, -0.014741333118210747, -0.3071902321295484, -0.13072758576120524, 0.2391448707557192, -0.066801222089185,... |
706.3095 | Channeling Effect and Improvement of the Efficiency of Charged Particle
Registration with Crystal Scintillators | The importance is emphasized of taking into account the channeling along the
low index crystallographic axes and planes of a part of low-energy (1-10 keV)
recoil ions in measurements of their parameters with crystal scintillators of
the type of NaI(Tl) etc. Because the nucleus stopping power in channels is low
as com... | physics.ins-det hep-ph | the importance is emphasized of taking into account the channeling along the low index crystallographic axes and planes of a part of lowenergy 110 kev recoil ions in measurements of their parameters with crystal scintillators of the type of naitl etc because the nucleus stopping power in channels is low as compared wit... | [['the', 'importance', 'is', 'emphasized', 'of', 'taking', 'into', 'account', 'the', 'channeling', 'along', 'the', 'low', 'index', 'crystallographic', 'axes', 'and', 'planes', 'of', 'a', 'part', 'of', 'lowenergy', '110', 'kev', 'recoil', 'ions', 'in', 'measurements', 'of', 'their', 'parameters', 'with', 'crystal', 'sci... | [-0.06893718586950347, 0.24025702239144497, -0.05059762085993709, 0.03759995210228141, -0.015170851968726966, -0.11207388069339876, 0.026029404772575513, 0.37451293305385597, -0.20888981173629873, -0.3512410388441843, 0.05048732464621385, -0.33347897265691223, 0.04787637711080268, 0.20002212925532528, -0.01148166715811... |
706.3096 | The frequency separations of stellar p-modes | Aims. The purpose of this work is to investigate a new frequency separation
of stellar p-modes and its characteristics. Methods. Frequency separations are
deduced from the asymptotic formula of stellar p-modes. Then, using the
theoretical adiabatic frequencies of stellar model, we compute the frequency
separations. R... | gr-qc | aims the purpose of this work is to investigate a new frequency separation of stellar pmodes and its characteristics methods frequency separations are deduced from the asymptotic formula of stellar pmodes then using the theoretical adiabatic frequencies of stellar model we compute the frequency separations results a ne... | [['aims', 'the', 'purpose', 'of', 'this', 'work', 'is', 'to', 'investigate', 'a', 'new', 'frequency', 'separation', 'of', 'stellar', 'pmodes', 'and', 'its', 'characteristics', 'methods', 'frequency', 'separations', 'are', 'deduced', 'from', 'the', 'asymptotic', 'formula', 'of', 'stellar', 'pmodes', 'then', 'using', 'th... | [-0.09190751422300107, 0.12909183289027876, -0.09875287075561506, 0.10718536707572639, -0.07396287528315076, -0.06302838846696196, 0.04070743310472204, 0.3102918919175863, -0.23339757570582959, -0.3144732054047011, 0.06065532682308306, -0.2527087896372433, -0.03839377628777314, 0.2067545676379706, -0.051381487771868704... |
706.3097 | The nature of the fluorescent iron line in V 1486 Ori | The fluorescent 6.4 keV iron line provides information on cool material in
the vicinity of hard X-ray sources as well as on the characteristics of the
X-ray sources themselves. First discovered in the X-ray spectra of the flaring
Sun, X-ray binaries and active galactic nuclei (AGN), the fluorescent line was
also obse... | astro-ph | the fluorescent 64 kev iron line provides information on cool material in the vicinity of hard xray sources as well as on the characteristics of the xray sources themselves first discovered in the xray spectra of the flaring sun xray binaries and active galactic nuclei agn the fluorescent line was also observed in a nu... | [['the', 'fluorescent', '64', 'kev', 'iron', 'line', 'provides', 'information', 'on', 'cool', 'material', 'in', 'the', 'vicinity', 'of', 'hard', 'xray', 'sources', 'as', 'well', 'as', 'on', 'the', 'characteristics', 'of', 'the', 'xray', 'sources', 'themselves', 'first', 'discovered', 'in', 'the', 'xray', 'spectra', 'of... | [-0.01729706591685717, 0.11966869081961462, -0.0024932330736413266, 0.13077848558685964, -0.06739658031067297, -0.12427701172507422, 0.07712528110524293, 0.4981177761130913, -0.14163235814962183, -0.3920889058444266, 0.03869574889540672, -0.35562875594221366, 0.013505905498121954, 0.19959202175959945, 0.009016384915962... |
706.3098 | Bayesian analysis of joint strong gravitational lensing and dynamic
galactic mass in SLACS: evidence of line-of-sight contamination | We readdress the calculation of the mass of early-type galaxies using strong
gravitational lensing and stellar dynamics. Our sample comprises 27 galaxies in
the Sloan Lens ACS (SLACS) Survey. Comparing the mass estimates from these two
independent methods in a Bayesian framework, we find evidence of significant
line-... | astro-ph | we readdress the calculation of the mass of earlytype galaxies using strong gravitational lensing and stellar dynamics our sample comprises 27 galaxies in the sloan lens acs slacs survey comparing the mass estimates from these two independent methods in a bayesian framework we find evidence of significant lineofsight m... | [['we', 'readdress', 'the', 'calculation', 'of', 'the', 'mass', 'of', 'earlytype', 'galaxies', 'using', 'strong', 'gravitational', 'lensing', 'and', 'stellar', 'dynamics', 'our', 'sample', 'comprises', '27', 'galaxies', 'in', 'the', 'sloan', 'lens', 'acs', 'slacs', 'survey', 'comparing', 'the', 'mass', 'estimates', 'fr... | [-0.07474833940052324, 0.02895416314293268, -0.1247467632336473, 0.11615307587112679, -0.08435950494992236, -0.047212190788963604, 0.02182345414292757, 0.3565992736154132, -0.14159021514847323, -0.38646260272297595, -0.0003609611609674714, -0.28458568023310765, -0.07941203267934421, 0.18857060112059115, -0.011896843601... |
706.3099 | An Improved Process for Fabricating High-Mobility Organic Molecular
Crystal Field-Effect Transistors | In this paper we present an improved process for producing elastomer
transistor stamps and high-mobility organic field-effect transistors (FETs)
based on semiconducting acene molecular crystals. In particular, we have
removed the need to use a silanized Si wafer for curing the stamps and to
handle a fragile micron-th... | cond-mat.soft cond-mat.mtrl-sci | in this paper we present an improved process for producing elastomer transistor stamps and highmobility organic fieldeffect transistors fets based on semiconducting acene molecular crystals in particular we have removed the need to use a silanized si wafer for curing the stamps and to handle a fragile micronthickness p... | [['in', 'this', 'paper', 'we', 'present', 'an', 'improved', 'process', 'for', 'producing', 'elastomer', 'transistor', 'stamps', 'and', 'highmobility', 'organic', 'fieldeffect', 'transistors', 'fets', 'based', 'on', 'semiconducting', 'acene', 'molecular', 'crystals', 'in', 'particular', 'we', 'have', 'removed', 'the', '... | [-0.12789059728460356, 0.13920242474598096, -0.01067449010862801, -0.09653456116204145, 0.019590519788507066, -0.22107932299803026, 0.09922335233031696, 0.46384581676149955, -0.19652364859510152, -0.3133619673947086, 0.04002620765298116, -0.3230073663909904, -0.11553721122642155, 0.20004471686103795, -0.093132419817027... |
706.31 | Cooling a Micromechanical Beam by Coupling it to a Transmission Line | We study a method to cool down the vibration mode of a micro-mechanical beam
using a capacitively-coupled superconducting transmission line. The Coulomb
force between the transmission line and the beam is determined by the driving
microwave on the transmission line and the displacement of the beam. When the
frequency... | cond-mat.mes-hall cond-mat.supr-con | we study a method to cool down the vibration mode of a micromechanical beam using a capacitivelycoupled superconducting transmission line the coulomb force between the transmission line and the beam is determined by the driving microwave on the transmission line and the displacement of the beam when the frequency of th... | [['we', 'study', 'a', 'method', 'to', 'cool', 'down', 'the', 'vibration', 'mode', 'of', 'a', 'micromechanical', 'beam', 'using', 'a', 'capacitivelycoupled', 'superconducting', 'transmission', 'line', 'the', 'coulomb', 'force', 'between', 'the', 'transmission', 'line', 'and', 'the', 'beam', 'is', 'determined', 'by', 'th... | [-0.17788140742573888, 0.19134916939772664, -0.06195445267483592, -0.06072205597767606, -0.03882763296132907, -0.16817309729754926, 0.0773364992509596, 0.4293362297490239, -0.24751694966107607, -0.2561129310168326, 0.04994841172243469, -0.24133986849337816, -0.019754700288176538, 0.26383690680377186, 0.0272354828647803... |
706.3101 | The Penna Model of Biological Aging | This review deals with computer simulation of biological ageing, particularly
with the Penna model of 1995.
| q-bio.PE | this review deals with computer simulation of biological ageing particularly with the penna model of 1995 | [['this', 'review', 'deals', 'with', 'computer', 'simulation', 'of', 'biological', 'ageing', 'particularly', 'with', 'the', 'penna', 'model', 'of', '1995']] | [-0.04245478264056146, 0.09057073609437793, -0.057849348057061434, -0.024884052378183696, -0.01035920181311667, -0.16872597392648458, -0.08310717041604221, 0.3323680148459971, -0.23445848043775186, -0.34713450260460377, 0.08558815106516704, -0.22403338123694994, -0.2586313639767468, 0.20415873067395296, -0.152611058205... |
706.3102 | Complete Hamiltonian description of wave-like features in classical and
quantum physics | The analysis of the Helmholtz equation is shown to lead to an exact
Hamiltonian system of equations describing in terms of ray trajectories a very
wide family of wave-like phenomena (including diffraction and interference)
going much beyond the limits of the ordinary geometrical optics approximation,
which is contain... | quant-ph | the analysis of the helmholtz equation is shown to lead to an exact hamiltonian system of equations describing in terms of ray trajectories a very wide family of wavelike phenomena including diffraction and interference going much beyond the limits of the ordinary geometrical optics approximation which is contained as ... | [['the', 'analysis', 'of', 'the', 'helmholtz', 'equation', 'is', 'shown', 'to', 'lead', 'to', 'an', 'exact', 'hamiltonian', 'system', 'of', 'equations', 'describing', 'in', 'terms', 'of', 'ray', 'trajectories', 'a', 'very', 'wide', 'family', 'of', 'wavelike', 'phenomena', 'including', 'diffraction', 'and', 'interferenc... | [-0.1190923657582101, 0.08826672815750657, -0.13914074355169484, 0.0743955015640139, -0.07845107971275549, -0.13032156478451645, 0.009629726468625924, 0.24855879225322733, -0.28213892083453096, -0.28585500298877775, 0.06416297679281105, -0.28915007538162174, -0.12635892422910294, 0.23130804223170423, -0.036565513503940... |
706.3103 | Production of high energy particles in laser and Coulomb fields and
e^+e^- antenna | A strong laser field and the Coulomb field of a nucleus can produce
e^{+}e^{-} pairs. It is shown for the first time that there is a large
probability that electrons and positrons created in this process collide after
one or several oscillations of the laser field. These collisions can take place
at high energy resul... | physics.atom-ph | a strong laser field and the coulomb field of a nucleus can produce ee pairs it is shown for the first time that there is a large probability that electrons and positrons created in this process collide after one or several oscillations of the laser field these collisions can take place at high energy resulting in seve... | [['a', 'strong', 'laser', 'field', 'and', 'the', 'coulomb', 'field', 'of', 'a', 'nucleus', 'can', 'produce', 'ee', 'pairs', 'it', 'is', 'shown', 'for', 'the', 'first', 'time', 'that', 'there', 'is', 'a', 'large', 'probability', 'that', 'electrons', 'and', 'positrons', 'created', 'in', 'this', 'process', 'collide', 'aft... | [-0.11170231341113618, 0.2687076660551766, -0.08958176234303865, 0.13052930717513359, 0.026156481499819792, -0.11243271089498272, 0.020554183159283427, 0.37135547026991844, -0.25202624921058847, -0.27265902376163376, -0.08895665986279329, -0.3421330993433073, 0.047629251800001014, 0.20729882005320557, 0.100091675281986... |
706.3104 | Group Testing with Random Pools: optimal two-stage algorithms | We study Probabilistic Group Testing of a set of N items each of which is
defective with probability p. We focus on the double limit of small defect
probability, p<<1, and large number of variables, N>>1, taking either p->0
after $N\to\infty$ or $p=1/N^{\beta}$ with $\beta\in(0,1/2)$. In both settings
the optimal num... | cs.DS cond-mat.dis-nn cond-mat.stat-mech cs.IT math.IT | we study probabilistic group testing of a set of n items each of which is defective with probability p we focus on the double limit of small defect probability p1 and large number of variables n1 taking either p0 after ntoinfty or p1nbeta with betain012 in both settings the optimal number of tests which are required to... | [['we', 'study', 'probabilistic', 'group', 'testing', 'of', 'a', 'set', 'of', 'n', 'items', 'each', 'of', 'which', 'is', 'defective', 'with', 'probability', 'p', 'we', 'focus', 'on', 'the', 'double', 'limit', 'of', 'small', 'defect', 'probability', 'p1', 'and', 'large', 'number', 'of', 'variables', 'n1', 'taking', 'eit... | [-0.12685843162813826, 0.10936561319977045, -0.059387226400020365, 0.01615391384180197, -0.03411075025249054, -0.16420495834831586, 0.12490661590469672, 0.3412149468820323, -0.23835349311668644, -0.3048447244143223, 0.12015561789808357, -0.2410439977696275, -0.10430674436502159, 0.1572049270151183, -0.06153110237244297... |
706.3105 | Hadronic Final States | In this summary we give a concise overview of the experimental and
theoretical results, which were presented during the QCD and Hadronic Final
State Working Group sessions at the DIS 2007 workshop.
| hep-ph | in this summary we give a concise overview of the experimental and theoretical results which were presented during the qcd and hadronic final state working group sessions at the dis 2007 workshop | [['in', 'this', 'summary', 'we', 'give', 'a', 'concise', 'overview', 'of', 'the', 'experimental', 'and', 'theoretical', 'results', 'which', 'were', 'presented', 'during', 'the', 'qcd', 'and', 'hadronic', 'final', 'state', 'working', 'group', 'sessions', 'at', 'the', 'dis', '2007', 'workshop']] | [-0.04241682462452445, 0.15226168440131005, -0.16918220250227023, 0.034243409096234245, -0.10866406816057861, -0.04225838957063388, 0.06722859994624741, 0.3598147928714752, -0.11427996726706624, -0.32760400674305856, 0.10239805510718725, -0.2726839988536085, -0.056559434189694, 0.13842904998455197, -0.0295382036420051,... |
706.3106 | Tuning the domain wall orientation in thin magnetic strips by induced
anisotropy | We report on a method to tune the orientation of in-plane magnetic domains
and domain walls in thin ferromagnetic strips by manipulating the magnetic
anisotropy. Uniaxial in-plane anisotropy is induced in a controlled way by
oblique evaporation of magnetic thin strips. A direct correlation between the
magnetization d... | cond-mat.other | we report on a method to tune the orientation of inplane magnetic domains and domain walls in thin ferromagnetic strips by manipulating the magnetic anisotropy uniaxial inplane anisotropy is induced in a controlled way by oblique evaporation of magnetic thin strips a direct correlation between the magnetization directi... | [['we', 'report', 'on', 'a', 'method', 'to', 'tune', 'the', 'orientation', 'of', 'inplane', 'magnetic', 'domains', 'and', 'domain', 'walls', 'in', 'thin', 'ferromagnetic', 'strips', 'by', 'manipulating', 'the', 'magnetic', 'anisotropy', 'uniaxial', 'inplane', 'anisotropy', 'is', 'induced', 'in', 'a', 'controlled', 'way... | [-0.22960723121650517, 0.20109545927727596, -0.006884605186060071, -0.041532628636341544, -0.1749387020431459, -0.07028970023384318, 0.011705474872142076, 0.5434233246743679, -0.3115291116060689, -0.31123402759432794, 0.05561519454466179, -0.19177539507858454, -0.04122222654521465, 0.23561335977399722, 0.06606112852226... |
706.3107 | Spinorial Characterization of Surfaces into 3-dimensional homogeneous
Manifolds | We give a spinorial characterization of isometrically immersed surfaces into
3-dimensional homogeneous manifolds with 4-dimensional isometry group in terms
of the existence of a particular spinor, called generalized Killing spinor.
This generalizes results by T. Friedrich for $\R^3$ and B. Morel for $\Ss^3$
and $\HH^... | math.DG | we give a spinorial characterization of isometrically immersed surfaces into 3dimensional homogeneous manifolds with 4dimensional isometry group in terms of the existence of a particular spinor called generalized killing spinor this generalizes results by t friedrich for r3 and b morel for ss3 and hh3 the main argument... | [['we', 'give', 'a', 'spinorial', 'characterization', 'of', 'isometrically', 'immersed', 'surfaces', 'into', '3dimensional', 'homogeneous', 'manifolds', 'with', '4dimensional', 'isometry', 'group', 'in', 'terms', 'of', 'the', 'existence', 'of', 'a', 'particular', 'spinor', 'called', 'generalized', 'killing', 'spinor', ... | [-0.17150702840322024, 0.12026281051289339, -0.07003669985025734, 0.00675772132908369, -0.1437786878751857, -0.08919058754653125, -0.07791354416494632, 0.2863447852553679, -0.19245616497181647, -0.20618842383725688, 0.07868372948686048, -0.22000111731422411, -0.15493608628061006, 0.13919322306362839, -0.070735748155744... |
706.3108 | Mapped Chebyshev pseudospectral method to study multiple scale phenomena | In the framework of mapped pseudospectral methods, we introduce a new
polynomial-type mapping function in order to describe accurately the dynamics
of systems developing almost singular structures. Using error criteria related
to the spectral interpolation error, the new polynomial-type mapping is
compared against pr... | physics.comp-ph physics.optics | in the framework of mapped pseudospectral methods we introduce a new polynomialtype mapping function in order to describe accurately the dynamics of systems developing almost singular structures using error criteria related to the spectral interpolation error the new polynomialtype mapping is compared against previousl... | [['in', 'the', 'framework', 'of', 'mapped', 'pseudospectral', 'methods', 'we', 'introduce', 'a', 'new', 'polynomialtype', 'mapping', 'function', 'in', 'order', 'to', 'describe', 'accurately', 'the', 'dynamics', 'of', 'systems', 'developing', 'almost', 'singular', 'structures', 'using', 'error', 'criteria', 'related', '... | [-0.11002603044718011, 0.044274738707992416, -0.05714129027718109, 0.0826811088010484, -0.019271699434592705, -0.0940851542582997, -0.024490829860245086, 0.37035554792147035, -0.28492473271359836, -0.2741142416003445, 0.09292424680311079, -0.27280632035483504, -0.16312712133469537, 0.2457882958687534, 0.015002826625127... |
706.3109 | Itinerant ferromagnetism in the multiorbital Hubbard model: a dynamical
mean-field study | In order to resolve the long-standing issue of how the itinerant
ferromagnetism is affected by the lattice structure and Hund's coupling, we
have compared various three-dimensional lattice structures in the single- and
multiorbital Hubbard models with the dynamical mean-field theory with an
improved quantum Monte Car... | cond-mat.str-el | in order to resolve the longstanding issue of how the itinerant ferromagnetism is affected by the lattice structure and hunds coupling we have compared various threedimensional lattice structures in the single and multiorbital hubbard models with the dynamical meanfield theory with an improved quantum monte carlo algor... | [['in', 'order', 'to', 'resolve', 'the', 'longstanding', 'issue', 'of', 'how', 'the', 'itinerant', 'ferromagnetism', 'is', 'affected', 'by', 'the', 'lattice', 'structure', 'and', 'hunds', 'coupling', 'we', 'have', 'compared', 'various', 'threedimensional', 'lattice', 'structures', 'in', 'the', 'single', 'and', 'multior... | [-0.13486150425008459, 0.17401711317298063, -0.053636848602605904, 0.11221504509853927, -0.04886584807511257, -0.13815537462233687, 0.08924411662307609, 0.36675234712336374, -0.29011967604898886, -0.264386083384085, 0.00735516636936075, -0.32205919351266776, -0.16164942432356919, 0.08406039166021283, 0.0680438843613956... |
706.311 | Interstellar Dust in the Solar System | The Ulysses spacecraft has been orbiting the Sun on a highly inclined ellipse
almost perpendicular to the ecliptic plane (inclination 79 deg, perihelion
distance 1.3 AU, aphelion distance 5.4 AU) since it encountered Jupiter in
1992. The in-situ dust detector on board continuously measured interstellar
dust grains wi... | astro-ph | the ulysses spacecraft has been orbiting the sun on a highly inclined ellipse almost perpendicular to the ecliptic plane inclination 79 deg perihelion distance 13 au aphelion distance 54 au since it encountered jupiter in 1992 the insitu dust detector on board continuously measured interstellar dust grains with masses ... | [['the', 'ulysses', 'spacecraft', 'has', 'been', 'orbiting', 'the', 'sun', 'on', 'a', 'highly', 'inclined', 'ellipse', 'almost', 'perpendicular', 'to', 'the', 'ecliptic', 'plane', 'inclination', '79', 'deg', 'perihelion', 'distance', '13', 'au', 'aphelion', 'distance', '54', 'au', 'since', 'it', 'encountered', 'jupiter... | [-0.10802920081079248, 0.21433271660417733, -0.03931604118359381, 0.013303703112695884, -0.04568474091744671, -0.024405102364080784, -0.0064243330432671225, 0.4071951891205067, -0.23512797721627135, -0.403849106118152, 0.02383830601603323, -0.29884476155792883, -0.01102294120290834, 0.1699285652344029, -0.0401730759032... |
706.3111 | Wave-front engineering by Huygens-Fresnel principle for nonlinear
optical interactions in domain engineered structures | The wave-front engineering for nonlinear optical interactions was discussed.
Using Huygens-Fresnel principle we developed a general theory and technique for
domain engineering with conventional quasi-phase-matching structures being the
special cases. By Fourier analysis we put forward the concept of local
quasi-phase... | physics.optics | the wavefront engineering for nonlinear optical interactions was discussed using huygensfresnel principle we developed a general theory and technique for domain engineering with conventional quasiphasematching structures being the special cases by fourier analysis we put forward the concept of local quasiphase matching... | [['the', 'wavefront', 'engineering', 'for', 'nonlinear', 'optical', 'interactions', 'was', 'discussed', 'using', 'huygensfresnel', 'principle', 'we', 'developed', 'a', 'general', 'theory', 'and', 'technique', 'for', 'domain', 'engineering', 'with', 'conventional', 'quasiphasematching', 'structures', 'being', 'the', 'sp... | [-0.10532746253563252, 0.0808147188408525, -0.08285033036121729, 0.027806508855629262, -0.12903343744832893, -0.1461129697433127, -0.0003410043598329327, 0.45555908847921367, -0.2532342397487433, -0.26324381050653756, 0.10989829451789083, -0.22182583825959792, -0.19904330868579062, 0.28506625299181404, 0.00518217019672... |
706.3112 | Almost-Commutative Geometries Beyond the Standard Model III: Vector
Doublets | We will present a new extension of the standard model of particle physics in
its almostcommutative formulation. This extension has as its basis the algebra
of the standard model with four summands [11], and enlarges only the particle
content by an arbitrary number of generations of left-right symmetric doublets
which... | hep-th | we will present a new extension of the standard model of particle physics in its almostcommutative formulation this extension has as its basis the algebra of the standard model with four summands 11 and enlarges only the particle content by an arbitrary number of generations of leftright symmetric doublets which couple... | [['we', 'will', 'present', 'a', 'new', 'extension', 'of', 'the', 'standard', 'model', 'of', 'particle', 'physics', 'in', 'its', 'almostcommutative', 'formulation', 'this', 'extension', 'has', 'as', 'its', 'basis', 'the', 'algebra', 'of', 'the', 'standard', 'model', 'with', 'four', 'summands', '11', 'and', 'enlarges', '... | [-0.061822717516826324, 0.1625384186505611, -0.06364402481659244, 0.07832213352398518, -0.05630667163775517, -0.13451783092191014, -0.021947320848434735, 0.3167596807022794, -0.2285788442599229, -0.3890426382511997, 0.0696426931032105, -0.2311072676585844, -0.05644320167798119, 0.12154008402453306, -0.01852493215119466... |
706.3113 | Bursty stellar populations and obscured AGN in galaxy bulges | [Abridged] We investigate trends between the recent star formation history
and black hole growth in galaxy bulges in the Sloan Digital Sky Survey (SDSS).
The galaxies lie at 0.01<z<0.07 where the fibre aperture covers only the
central 0.6-4.0kpc diameter of the galaxy. We find strong trends between black
hole growth,... | astro-ph | abridged we investigate trends between the recent star formation history and black hole growth in galaxy bulges in the sloan digital sky survey sdss the galaxies lie at 001z007 where the fibre aperture covers only the central 0640kpc diameter of the galaxy we find strong trends between black hole growth as measured by ... | [['abridged', 'we', 'investigate', 'trends', 'between', 'the', 'recent', 'star', 'formation', 'history', 'and', 'black', 'hole', 'growth', 'in', 'galaxy', 'bulges', 'in', 'the', 'sloan', 'digital', 'sky', 'survey', 'sdss', 'the', 'galaxies', 'lie', 'at', '001z007', 'where', 'the', 'fibre', 'aperture', 'covers', 'only',... | [-0.06577518583824336, 0.055062179102417855, -0.052579284655652814, 0.11020834938671183, -0.08324604017403105, -0.06670640069983322, 0.02579636493766006, 0.4225517634045461, -0.15098268398212206, -0.3295272279546821, 0.09088951725952311, -0.2598434435595068, -0.052344876331485934, 0.21616021279975217, -0.02867757772689... |
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