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 |
|---|---|---|---|---|---|---|
709.1435 | Composition operators in the Lipschitz Space of the Polydiscs | In 1987, Shapiro shew that composition operator induced by symbol $\phi$ is
compact on the Lipschltz space if and only if the infinity norm of $\phi$ is
less than 1 by a spectral-theoretic argument, where $\phi$ is a holomorphic
self-map of the unit disk. In this paper, we shall generalize Shapiro's result
to the $n$... | math.FA math.CV | in 1987 shapiro shew that composition operator induced by symbol phi is compact on the lipschltz space if and only if the infinity norm of phi is less than 1 by a spectraltheoretic argument where phi is a holomorphic selfmap of the unit disk in this paper we shall generalize shapiros result to the ndimensional case | [['in', '1987', 'shapiro', 'shew', 'that', 'composition', 'operator', 'induced', 'by', 'symbol', 'phi', 'is', 'compact', 'on', 'the', 'lipschltz', 'space', 'if', 'and', 'only', 'if', 'the', 'infinity', 'norm', 'of', 'phi', 'is', 'less', 'than', '1', 'by', 'a', 'spectraltheoretic', 'argument', 'where', 'phi', 'is', 'a',... | [-0.15349795830182053, 0.1368320878552781, -0.08257112550940789, 0.031391676028513095, -0.09864408483051441, -0.11627205750820312, 0.01086796590084718, 0.3321281199089505, -0.27464081299575893, -0.18528094454245134, 0.09881150424903766, -0.27557371704077177, -0.1885316172784025, 0.19795251556418159, -0.1438230983574282... |
709.1436 | Extended Ces$\acute{a}$RO Operators on Zygmund Spaces in the Unit Ball | Let $g$ be a holomorphic function of the unit ball $B$ in the $n$-dimensional
space, and denote by $T_g$ and $I_g$ the induced extended Ces$\acute{a}$ro
operator and another integral operator. The boundedness and compactness of
$T_g$ and $I_g$ acting on the Zygmund spaces in the unit ball are discussed and
necessary ... | math.FA math.CV | let g be a holomorphic function of the unit ball b in the ndimensional space and denote by t_g and i_g the induced extended cesacutearo operator and another integral operator the boundedness and compactness of t_g and i_g acting on the zygmund spaces in the unit ball are discussed and necessary and sufficient condition... | [['let', 'g', 'be', 'a', 'holomorphic', 'function', 'of', 'the', 'unit', 'ball', 'b', 'in', 'the', 'ndimensional', 'space', 'and', 'denote', 'by', 't_g', 'and', 'i_g', 'the', 'induced', 'extended', 'cesacutearo', 'operator', 'and', 'another', 'integral', 'operator', 'the', 'boundedness', 'and', 'compactness', 'of', 't_... | [-0.14843155501474595, 0.15342730134404425, -0.01932491489750301, 0.04592659406901883, -0.09619912851585782, -0.05364766067439883, -0.014272222819272429, 0.35952774737158727, -0.3027294808677558, -0.17186702145584698, 0.20293648375784337, -0.2757139409217855, -0.14035669640348902, 0.17712965394884092, -0.13863233436734... |
709.1437 | A Geant4 based engineering tool for Fresnel lenses | Geant4 is a Monte Carlo radiation transport toolkit that is becoming a tool
of generalized application in areas such as high-energy physics, nuclear
physics, astroparticle physics, or medical physics. Geant4 provides an optical
physics process category, allowing the simulation of the production and
propagation of lig... | astro-ph | geant4 is a monte carlo radiation transport toolkit that is becoming a tool of generalized application in areas such as highenergy physics nuclear physics astroparticle physics or medical physics geant4 provides an optical physics process category allowing the simulation of the production and propagation of light its c... | [['geant4', 'is', 'a', 'monte', 'carlo', 'radiation', 'transport', 'toolkit', 'that', 'is', 'becoming', 'a', 'tool', 'of', 'generalized', 'application', 'in', 'areas', 'such', 'as', 'highenergy', 'physics', 'nuclear', 'physics', 'astroparticle', 'physics', 'or', 'medical', 'physics', 'geant4', 'provides', 'an', 'optica... | [-0.017757054118617895, 0.12200310749640847, -0.1070136988357185, 0.12159394560220538, -0.0748911077315186, -0.12705150479450822, -0.08084780235398323, 0.3793950890924068, -0.2703605180041508, -0.36130691822023786, 0.0964288267671091, -0.30636289324413274, -0.12007355520828686, 0.3496573804555699, 0.02915314801948819, ... |
709.1438 | Improved bounds in entropic uncertainty relations | Entropic uncertainty relations place nontrivial lower bounds to the sum of
Shannon information entropies for noncommuting observables. Here we obtain a
novel lower bound on the entropy sum for general pairs of observables in
finite-dimensional Hilbert space, which improves on the best bound known to
date [Maassen and... | quant-ph | entropic uncertainty relations place nontrivial lower bounds to the sum of shannon information entropies for noncommuting observables here we obtain a novel lower bound on the entropy sum for general pairs of observables in finitedimensional hilbert space which improves on the best bound known to date maassen and uffin... | [['entropic', 'uncertainty', 'relations', 'place', 'nontrivial', 'lower', 'bounds', 'to', 'the', 'sum', 'of', 'shannon', 'information', 'entropies', 'for', 'noncommuting', 'observables', 'here', 'we', 'obtain', 'a', 'novel', 'lower', 'bound', 'on', 'the', 'entropy', 'sum', 'for', 'general', 'pairs', 'of', 'observables'... | [-0.09072185593235883, 0.12181650585262105, -0.0794890227178777, 0.08812580211088061, -0.10032661445438862, -0.12742992884124674, 0.14265110437519893, 0.2234728413057469, -0.2283212108803647, -0.3366960457060486, -0.0028495359653052652, -0.28029630091484814, -0.1117927165358283, 0.2612710823748438, -0.15367149532262592... |
709.1439 | Plaquette Invariants and the Flavour Symmetric Description of Quark and
Neutrino Mixings | We present a complete set of new flavour-permutation-symmetric mixing
observables. We give expressions for these "plaquette invariants", both in
terms of the mixing matrix elements alone, and in terms of manifestly
Jarlskog-invariant functions of fermion mass matrices. While these quantities
are unconstrained in the ... | hep-ph | we present a complete set of new flavourpermutationsymmetric mixing observables we give expressions for these plaquette invariants both in terms of the mixing matrix elements alone and in terms of manifestly jarlskoginvariant functions of fermion mass matrices while these quantities are unconstrained in the standard mo... | [['we', 'present', 'a', 'complete', 'set', 'of', 'new', 'flavourpermutationsymmetric', 'mixing', 'observables', 'we', 'give', 'expressions', 'for', 'these', 'plaquette', 'invariants', 'both', 'in', 'terms', 'of', 'the', 'mixing', 'matrix', 'elements', 'alone', 'and', 'in', 'terms', 'of', 'manifestly', 'jarlskoginvarian... | [-0.12217777285322144, 0.19589948833202692, -0.035511548622502935, 0.1147749151631787, -0.034457894566527626, -0.10561421912935404, 0.06699171903761322, 0.3285722418075746, -0.20524936994256637, -0.2915959848376276, 0.05909258050021825, -0.2558909858795101, -0.11046054406743916, 0.1626442585723592, -0.00514286375596179... |
709.144 | Density Dependence of the Mass Function of Globular Star Clusters in the
Sombrero Galaxy and its Dynamical Implications | We have constructed the mass function of globular star clusters in the
Sombrero galaxy in bins of different internal half-mass density rho_h and
projected galactocentric distance R. This is based on the published
measurements of the magnitudes and effective radii of the clusters by Spitler
et al. (2006) in BVR images... | astro-ph | we have constructed the mass function of globular star clusters in the sombrero galaxy in bins of different internal halfmass density rho_h and projected galactocentric distance r this is based on the published measurements of the magnitudes and effective radii of the clusters by spitler et al 2006 in bvr images taken ... | [['we', 'have', 'constructed', 'the', 'mass', 'function', 'of', 'globular', 'star', 'clusters', 'in', 'the', 'sombrero', 'galaxy', 'in', 'bins', 'of', 'different', 'internal', 'halfmass', 'density', 'rho_h', 'and', 'projected', 'galactocentric', 'distance', 'r', 'this', 'is', 'based', 'on', 'the', 'published', 'measure... | [-0.06309773773099556, 0.12320157663060803, -0.10474805623547447, 0.05432207117100125, -0.034199933194618976, -0.03631439473653886, 0.03751542027143079, 0.4049584517220718, -0.1541289952272688, -0.3991505543105536, 0.015319581712619258, -0.27682167404730407, -0.05969336084003404, 0.1924649372361369, -0.0235509659736330... |
709.1441 | Information-theoretic analysis of MIMO channel sounding | The large majority of commercially available multiple-input multiple-output
(MIMO) radio channel measurement devices (sounders) is based on time-division
multiplexed switching (TDMS) of a single transmit/receive radio-frequency chain
into the elements of a transmit/receive antenna array. While being
cost-effective, s... | cs.IT math.IT | the large majority of commercially available multipleinput multipleoutput mimo radio channel measurement devices sounders is based on timedivision multiplexed switching tdms of a single transmitreceive radiofrequency chain into the elements of a transmitreceive antenna array while being costeffective such a solution ca... | [['the', 'large', 'majority', 'of', 'commercially', 'available', 'multipleinput', 'multipleoutput', 'mimo', 'radio', 'channel', 'measurement', 'devices', 'sounders', 'is', 'based', 'on', 'timedivision', 'multiplexed', 'switching', 'tdms', 'of', 'a', 'single', 'transmitreceive', 'radiofrequency', 'chain', 'into', 'the',... | [-0.22161902161824004, 0.10241165432814685, -0.011434876253126098, -0.01350150859782401, -0.033785434694238045, -0.1938593411930109, 0.09711785903047832, 0.39490474674524995, -0.21778927538658446, -0.27908762636507956, 0.1333957513917716, -0.25239884225865367, -0.15427107764967804, 0.19036411734608313, -0.1091176078189... |
709.1442 | Light-matter interaction in Mie nanolasers | By deriving a three dimensional vector set of Maxwell-Bloch equations, we
report on an ab-initio investigation of a spherical Mie nanolaser. Parallel
numerical simulations predict a rich physical scenario, ranging from a
nontrivial vectorial energy-matter interplay in the initial stage of evolution
to mode competitio... | physics.optics cond-mat.soft quant-ph | by deriving a three dimensional vector set of maxwellbloch equations we report on an abinitio investigation of a spherical mie nanolaser parallel numerical simulations predict a rich physical scenario ranging from a nontrivial vectorial energymatter interplay in the initial stage of evolution to mode competition and dy... | [['by', 'deriving', 'a', 'three', 'dimensional', 'vector', 'set', 'of', 'maxwellbloch', 'equations', 'we', 'report', 'on', 'an', 'abinitio', 'investigation', 'of', 'a', 'spherical', 'mie', 'nanolaser', 'parallel', 'numerical', 'simulations', 'predict', 'a', 'rich', 'physical', 'scenario', 'ranging', 'from', 'a', 'nontr... | [-0.1933456924056909, 0.1394734370513136, -0.1178370048520995, -0.0006915429973455726, -0.11592006500138612, -0.10347657083709282, 0.04584144458907549, 0.33178383176840964, -0.2458294603943092, -0.2911908398153352, 0.057774341709102645, -0.2409012771562719, -0.18632162350123047, 0.20024899726153397, 0.05996895392070387... |
709.1443 | Extended Ces$\acute{a}$RO Operators between Generalized Besov Spaces and
Bloch Type Spaces in the Unit Ball | Let $g$ be a holomorphic map of $B$, where $B$ is the unit ball of ${C}^n$.
Let $0<p<+\infty, -n-1<q<+\infty$, $q>-1$ and $\alpha>0$. This paper gives some
necessary and sufficient conditions for the Extended Ces$\acute{a}$ro Operators
induced by $g$ to be bounded or compact between generalized Besov space
$B(p,q)$ a... | math.FA math.CV | let g be a holomorphic map of b where b is the unit ball of cn let 0pinfty n1qinfty q1 and alpha0 this paper gives some necessary and sufficient conditions for the extended cesacutearo operators induced by g to be bounded or compact between generalized besov space bpq and alpha bloch space mathcal balpha | [['let', 'g', 'be', 'a', 'holomorphic', 'map', 'of', 'b', 'where', 'b', 'is', 'the', 'unit', 'ball', 'of', 'cn', 'let', '0pinfty', 'n1qinfty', 'q1', 'and', 'alpha0', 'this', 'paper', 'gives', 'some', 'necessary', 'and', 'sufficient', 'conditions', 'for', 'the', 'extended', 'cesacutearo', 'operators', 'induced', 'by', '... | [-0.1730878318910702, 0.17647610760580462, -0.010421084920660807, 0.0088878887024923, -0.10555098567587826, -0.1834420049115299, 0.01198974958074709, 0.33027212199969935, -0.3030139741559441, -0.16438641005124038, 0.10415921356672278, -0.221694584380692, -0.10501367192661676, 0.1622035993540731, -0.12058633699332579, -... |
709.1444 | Fermi-Bose transformation for the time-dependent Lieb-Liniger gas | Exact solutions of the Schrodinger equation describing a freely expanding
Lieb-Liniger (LL) gas of delta-interacting bosons in one spatial dimension are
constructed. The many-body wave function is obtained by transforming a fully
antisymmetric (fermionic) time-dependent wave function which obeys the
Schrodinger equat... | cond-mat.other | exact solutions of the schrodinger equation describing a freely expanding liebliniger ll gas of deltainteracting bosons in one spatial dimension are constructed the manybody wave function is obtained by transforming a fully antisymmetric fermionic timedependent wave function which obeys the schrodinger equation for a f... | [['exact', 'solutions', 'of', 'the', 'schrodinger', 'equation', 'describing', 'a', 'freely', 'expanding', 'liebliniger', 'll', 'gas', 'of', 'deltainteracting', 'bosons', 'in', 'one', 'spatial', 'dimension', 'are', 'constructed', 'the', 'manybody', 'wave', 'function', 'is', 'obtained', 'by', 'transforming', 'a', 'fully'... | [-0.1625077990665615, 0.18792711652870944, -0.06285292389038116, 0.059934252539455, -0.06284622694435182, -0.16902171217127523, -0.06124944432026971, 0.25863829157801704, -0.2408688634550616, -0.19279874535972502, 0.0178653732856124, -0.3136305122900365, -0.1057697036929095, 0.13740616731012045, 0.14178955377037847, 0.... |
709.1445 | The Formation of Fragments at Corotation in Isothermal Protoplanetary
Disks | Numerical hydrodynamics simulations have established that disks which are
evolved under the condition of local isothermality will fragment into small
dense clumps due to gravitational instabilities when the Toomre stability
parameter $Q$ is sufficiently low. Because fragmentation through disk
instability has been sug... | astro-ph | numerical hydrodynamics simulations have established that disks which are evolved under the condition of local isothermality will fragment into small dense clumps due to gravitational instabilities when the toomre stability parameter q is sufficiently low because fragmentation through disk instability has been suggeste... | [['numerical', 'hydrodynamics', 'simulations', 'have', 'established', 'that', 'disks', 'which', 'are', 'evolved', 'under', 'the', 'condition', 'of', 'local', 'isothermality', 'will', 'fragment', 'into', 'small', 'dense', 'clumps', 'due', 'to', 'gravitational', 'instabilities', 'when', 'the', 'toomre', 'stability', 'par... | [-0.10682632578320016, 0.13588556146486572, -0.13333651429845714, 0.108876438220874, -0.097597365002787, -0.07488905749393299, -0.015209431891265673, 0.34193951354616586, -0.22748539262273185, -0.28438453120636004, 0.10292498450657792, -0.22528621886729025, -0.12034154341866572, 0.14686688535627634, 0.00231021398897556... |
709.1446 | Algorithm for counting large directed loops | We derive a Belief-Propagation algorithm for counting large loops in a
directed network. We evaluate the distribution of the number of small loops in
a directed random network with given degree sequence. We apply the algorithm to
a few characteristic directed networks of various network sizes and loop
structures and ... | cond-mat.dis-nn | we derive a beliefpropagation algorithm for counting large loops in a directed network we evaluate the distribution of the number of small loops in a directed random network with given degree sequence we apply the algorithm to a few characteristic directed networks of various network sizes and loop structures and compa... | [['we', 'derive', 'a', 'beliefpropagation', 'algorithm', 'for', 'counting', 'large', 'loops', 'in', 'a', 'directed', 'network', 'we', 'evaluate', 'the', 'distribution', 'of', 'the', 'number', 'of', 'small', 'loops', 'in', 'a', 'directed', 'random', 'network', 'with', 'given', 'degree', 'sequence', 'we', 'apply', 'the',... | [-0.14981265335033336, 0.10730509694943997, -0.03489875687478945, 0.10810078227298399, -0.07061068167717292, -0.14135354436163244, 0.0681014192175527, 0.47112651250656995, -0.2532617519957538, -0.33374026660197254, 0.07862546800865909, -0.21636050889247108, -0.21010557675584293, 0.17248218132172252, -0.0426671951473958... |
709.1447 | Simple Finite Non-Abelian Flavor Groups | The recently measured unexpected neutrino mixing patterns have caused a
resurgence of interest in the study of finite flavor groups with two- and
three-dimensional irreducible representations. This paper details the
mathematics of the two finite simple groups with such representations, the
Icosahedral group A_5, a su... | hep-th hep-ph | the recently measured unexpected neutrino mixing patterns have caused a resurgence of interest in the study of finite flavor groups with two and threedimensional irreducible representations this paper details the mathematics of the two finite simple groups with such representations the icosahedral group a_5 a subgroup ... | [['the', 'recently', 'measured', 'unexpected', 'neutrino', 'mixing', 'patterns', 'have', 'caused', 'a', 'resurgence', 'of', 'interest', 'in', 'the', 'study', 'of', 'finite', 'flavor', 'groups', 'with', 'two', 'and', 'threedimensional', 'irreducible', 'representations', 'this', 'paper', 'details', 'the', 'mathematics', ... | [-0.1670329159953528, 0.2063484043917722, -0.11350798737947587, 0.041705259699719374, -0.09804813594867785, -0.07844917263503669, 0.027570250877437905, 0.3701257703618871, -0.2782392836417313, -0.25668015731153665, 0.12685130675176712, -0.25354815229635547, -0.15090262303473773, 0.1193776459398645, -0.05120699931177552... |
709.1448 | A few remarks concerning complex-analytic metric spaces | The special case of closed subsets of C^n is briefly discussed.
| math.AT | the special case of closed subsets of cn is briefly discussed | [['the', 'special', 'case', 'of', 'closed', 'subsets', 'of', 'cn', 'is', 'briefly', 'discussed']] | [-0.22436502745205705, 0.09233042970299721, 0.16130753606557846, 0.12652770706071434, -0.010819564488801088, -0.1295332945883274, 0.008328769525343721, 0.3853633837266402, -0.18824303488839755, -0.027245442298325626, 0.13269435411149805, -0.23076460893604567, -0.15441050359301947, 0.21967767314477402, -0.12670211595567... |
709.1449 | Supervised secure entanglement sharing for faithful quantum
teleportation via tripartite W states | We present a supervised secure entanglement sharing protocol via tripartite W
states for faithful quantum teleportation. By guaranteeing a secure
entanglement distribution in the charge of a third believed supervisor, quantum
information of an unknown state of a 2-level particle can be faithfully
teleported from the ... | quant-ph cs.CR | we present a supervised secure entanglement sharing protocol via tripartite w states for faithful quantum teleportation by guaranteeing a secure entanglement distribution in the charge of a third believed supervisor quantum information of an unknown state of a 2level particle can be faithfully teleported from the sende... | [['we', 'present', 'a', 'supervised', 'secure', 'entanglement', 'sharing', 'protocol', 'via', 'tripartite', 'w', 'states', 'for', 'faithful', 'quantum', 'teleportation', 'by', 'guaranteeing', 'a', 'secure', 'entanglement', 'distribution', 'in', 'the', 'charge', 'of', 'a', 'third', 'believed', 'supervisor', 'quantum', '... | [-0.19384755183699298, 0.1503622574105844, -0.10321131568435613, 0.04068229356067473, 0.05196375021845236, -0.3464319261906853, 0.12723148755964125, 0.34238035011583484, -0.2508141208155713, -0.24773583660187484, 0.05178759554883482, -0.28751309031436034, -0.06854503034605636, 0.1655715723838741, -0.116446113792827, 0.... |
709.145 | Computer simulation of the critical behavior of 3D disordered Ising
model | The critical behavior of the disordered ferromagnetic Ising model is studied
numerically by the Monte Carlo method in a wide range of variation of
concentration of nonmagnetic impurity atoms. The temperature dependences of
correlation length and magnetic susceptibility are determined for samples with
various spin con... | cond-mat.dis-nn cond-mat.stat-mech | the critical behavior of the disordered ferromagnetic ising model is studied numerically by the monte carlo method in a wide range of variation of concentration of nonmagnetic impurity atoms the temperature dependences of correlation length and magnetic susceptibility are determined for samples with various spin concen... | [['the', 'critical', 'behavior', 'of', 'the', 'disordered', 'ferromagnetic', 'ising', 'model', 'is', 'studied', 'numerically', 'by', 'the', 'monte', 'carlo', 'method', 'in', 'a', 'wide', 'range', 'of', 'variation', 'of', 'concentration', 'of', 'nonmagnetic', 'impurity', 'atoms', 'the', 'temperature', 'dependences', 'of... | [-0.13265540077370147, 0.2167718585114926, -0.0610065610328717, 0.056448029843332775, 0.029660145098816103, -0.14371795611414337, 0.05293812125281834, 0.33254657469780197, -0.23444664748663555, -0.2918100026783659, 0.06674944250166777, -0.3249985591452847, -0.11254646058312492, 0.23967010402398656, 0.09543198613087654,... |
709.1451 | Experimentally Constrained Molecular Relaxation: The case of
hydrogenated amorphous silicon | We have extended our experimentally constrained molecular relaxation
technique (P. Biswas {\it et al}, Phys. Rev. B {\bf 71} 54204 (2005)) to
hydrogenated amorphous silicon: a 540-atom model with 7.4 % hydrogen and a
611-atom model with 22 % hydrogen were constructed. Starting from a random
configuration, using physi... | cond-mat.mtrl-sci cond-mat.dis-nn | we have extended our experimentally constrained molecular relaxation technique p biswas it et al phys rev b bf 71 54204 2005 to hydrogenated amorphous silicon a 540atom model with 74 hydrogen and a 611atom model with 22 hydrogen were constructed starting from a random configuration using physically relevant constraints... | [['we', 'have', 'extended', 'our', 'experimentally', 'constrained', 'molecular', 'relaxation', 'technique', 'p', 'biswas', 'it', 'et', 'al', 'phys', 'rev', 'b', 'bf', '71', '54204', '2005', 'to', 'hydrogenated', 'amorphous', 'silicon', 'a', '540atom', 'model', 'with', '74', 'hydrogen', 'and', 'a', '611atom', 'model', '... | [-0.06077183055186592, 0.14910413954781246, -0.03482133146020732, -0.09005018578250414, 0.018696994964625235, -0.14317251580863077, 0.10478955190672287, 0.45209585993211265, -0.17612388881824248, -0.3408178567002902, -0.016512317132535523, -0.2888468188172746, -0.13787339844035906, 0.10545292834829643, 0.02251452974383... |
709.1452 | Pure Spinors on Lie groups | For any manifold M, the direct sum TM \oplus T*M carries a natural inner
product given by the pairing of vectors and covectors. Differential forms on M
may be viewed as spinors for the corresponding Clifford bundle, and in
particular there is a notion of \emph{pure spinor}.
In this paper, we study pure spinors and ... | math.DG math.SG | for any manifold m the direct sum tm oplus tm carries a natural inner product given by the pairing of vectors and covectors differential forms on m may be viewed as spinors for the corresponding clifford bundle and in particular there is a notion of emphpure spinor in this paper we study pure spinors and dirac structur... | [['for', 'any', 'manifold', 'm', 'the', 'direct', 'sum', 'tm', 'oplus', 'tm', 'carries', 'a', 'natural', 'inner', 'product', 'given', 'by', 'the', 'pairing', 'of', 'vectors', 'and', 'covectors', 'differential', 'forms', 'on', 'm', 'may', 'be', 'viewed', 'as', 'spinors', 'for', 'the', 'corresponding', 'clifford', 'bundl... | [-0.20819562861677443, 0.10316180711321643, -0.05559948643687928, 0.04154079616655328, -0.1335525699835824, -0.10704925698792968, -0.014224016828010652, 0.34969319886352757, -0.2534798033129756, -0.2327370419083993, 0.048702082495288096, -0.2483161356632072, -0.18911803885372264, 0.18012161752541023, -0.094383552698141... |
709.1453 | Remodeling the B-model | We propose a complete, new formalism to compute unambiguously B-model open
and closed amplitudes in local Calabi-Yau geometries, including the mirrors of
toric manifolds. The formalism is based on the recursive solution of matrix
models recently proposed by Eynard and Orantin. The resulting amplitudes are
non-perturb... | hep-th math.AG | we propose a complete new formalism to compute unambiguously bmodel open and closed amplitudes in local calabiyau geometries including the mirrors of toric manifolds the formalism is based on the recursive solution of matrix models recently proposed by eynard and orantin the resulting amplitudes are nonperturbative in ... | [['we', 'propose', 'a', 'complete', 'new', 'formalism', 'to', 'compute', 'unambiguously', 'bmodel', 'open', 'and', 'closed', 'amplitudes', 'in', 'local', 'calabiyau', 'geometries', 'including', 'the', 'mirrors', 'of', 'toric', 'manifolds', 'the', 'formalism', 'is', 'based', 'on', 'the', 'recursive', 'solution', 'of', '... | [-0.13564856676541068, 0.11317517575051951, -0.13497961198304773, 0.13463703017672463, -0.06960626386243525, -0.11502539608065014, 0.0243638320825994, 0.3394896572568273, -0.2339037514397962, -0.26000562340846195, 0.07800814158192541, -0.2152187232515656, -0.1818225759381566, 0.16687290345149852, -0.08763689154621539, ... |
709.1454 | Oligarchic planetesimal accretion and giant planet formation | Aims. In the context of the core instability model, we present calculations
of in situ giant planet formation. The oligarchic growth regime of solid
protoplanets is the model adopted for the growth of the core. Methods. The full
differential equations of giant planet formation were numerically solved with
an adaptati... | astro-ph | aims in the context of the core instability model we present calculations of in situ giant planet formation the oligarchic growth regime of solid protoplanets is the model adopted for the growth of the core methods the full differential equations of giant planet formation were numerically solved with an adaptation of a... | [['aims', 'in', 'the', 'context', 'of', 'the', 'core', 'instability', 'model', 'we', 'present', 'calculations', 'of', 'in', 'situ', 'giant', 'planet', 'formation', 'the', 'oligarchic', 'growth', 'regime', 'of', 'solid', 'protoplanets', 'is', 'the', 'model', 'adopted', 'for', 'the', 'growth', 'of', 'the', 'core', 'metho... | [-0.11481391298276636, 0.13406256823705232, -0.07631269075037, 0.04040439253685486, -0.03466349215697781, -0.011142143480205124, 0.006735690580179806, 0.31460175907966, -0.2159649375533777, -0.35409152541192657, 0.08028261382091005, -0.2283317143924434, -0.05385454168392872, 0.1729392613223733, -0.030787735400646256, 0... |
709.1455 | A Beale-Kato-Majda breakdown criterion for an Oldroyd-B fluid in the
creeping flow regime | We derive a criterion for the breakdown of solutions to the Oldroyd-B model
in $\R^3$ in the limit of zero Reynolds number (creeping flow). If the initial
stress field is in the Sobolev space $H^m$, $m> 5/2$, then either a unique
solution exists within this space indefinitely, or, at the time where the
solution break... | math.AP math-ph math.MP | we derive a criterion for the breakdown of solutions to the oldroydb model in r3 in the limit of zero reynolds number creeping flow if the initial stress field is in the sobolev space hm m 52 then either a unique solution exists within this space indefinitely or at the time where the solution breaks down the time integ... | [['we', 'derive', 'a', 'criterion', 'for', 'the', 'breakdown', 'of', 'solutions', 'to', 'the', 'oldroydb', 'model', 'in', 'r3', 'in', 'the', 'limit', 'of', 'zero', 'reynolds', 'number', 'creeping', 'flow', 'if', 'the', 'initial', 'stress', 'field', 'is', 'in', 'the', 'sobolev', 'space', 'hm', 'm', '52', 'then', 'either... | [-0.19500402639763814, 0.11876042804625982, -0.12348886097726576, 0.03730383298414595, -0.04697679141536355, -0.10366430338472128, 0.0046153803739477604, 0.21282572982942358, -0.3092794027261655, -0.23532699736602167, 0.15688233543803695, -0.23762240808676272, -0.07686574471402256, 0.12106003664324388, -0.0440035068566... |
709.1456 | Analysis of stochastic fluid queues driven by local time processes | We consider a stochastic fluid queue served by a constant rate server and
driven by a process which is the local time of a certain Markov process. Such a
stochastic system can be used as a model in a priority service system,
especially when the time scales involved are fast. The input (local time) in
our model is alw... | math.PR | we consider a stochastic fluid queue served by a constant rate server and driven by a process which is the local time of a certain markov process such a stochastic system can be used as a model in a priority service system especially when the time scales involved are fast the input local time in our model is always sin... | [['we', 'consider', 'a', 'stochastic', 'fluid', 'queue', 'served', 'by', 'a', 'constant', 'rate', 'server', 'and', 'driven', 'by', 'a', 'process', 'which', 'is', 'the', 'local', 'time', 'of', 'a', 'certain', 'markov', 'process', 'such', 'a', 'stochastic', 'system', 'can', 'be', 'used', 'as', 'a', 'model', 'in', 'a', 'p... | [-0.1246688632492089, 0.10871238775099769, -0.1273752873537667, 0.07878046723385386, -0.04211824926914591, -0.13883740655569868, 0.0871485215717588, 0.36446119611236183, -0.34912177213665213, -0.22395111366887718, 0.16541763421987662, -0.2230964824359751, -0.13485581952034298, 0.18274323072171572, -0.0967483047283057, ... |
709.1457 | What happens to geometric phase when spin-orbit interactions lift band
degeneracy? | Spin-orbit interaction lifts accidental band degeneracy. The geometric phase
gamma(C)=pi for circuits surrounding a line of such degeneracy cannot survive
completely unchanged. The change depends on how the spin is fixed during
adiabatic evolution. For spin fixed along the internal spin-orbit field,
gamma(C) decrease... | cond-mat.other | spinorbit interaction lifts accidental band degeneracy the geometric phase gammacpi for circuits surrounding a line of such degeneracy cannot survive completely unchanged the change depends on how the spin is fixed during adiabatic evolution for spin fixed along the internal spinorbit field gammac decreases to zero as ... | [['spinorbit', 'interaction', 'lifts', 'accidental', 'band', 'degeneracy', 'the', 'geometric', 'phase', 'gammacpi', 'for', 'circuits', 'surrounding', 'a', 'line', 'of', 'such', 'degeneracy', 'can', 'not', 'survive', 'completely', 'unchanged', 'the', 'change', 'depends', 'on', 'how', 'the', 'spin', 'is', 'fixed', 'durin... | [-0.27191260880125423, 0.2298807549423405, -0.0036984888969787528, 0.04461169658295278, -0.0820625015501199, -0.16321516751777382, 0.05696040538272688, 0.3843678207269737, -0.31771748026034663, -0.28110129658265837, 0.054318482388875315, -0.24467987386243684, -0.05634484067559242, 0.13398768185371798, 0.000256636585774... |
709.1458 | Hurwitz numbers, matrix models and enumerative geometry | We propose a new, conjectural recursion solution for Hurwitz numbers at all
genera. This conjecture is based on recent progress in solving type B
topological string theory on the mirrors of toric Calabi-Yau manifolds, which
we briefly review to provide some background for our conjecture. We show in
particular how thi... | math.AG hep-th | we propose a new conjectural recursion solution for hurwitz numbers at all genera this conjecture is based on recent progress in solving type b topological string theory on the mirrors of toric calabiyau manifolds which we briefly review to provide some background for our conjecture we show in particular how this bmode... | [['we', 'propose', 'a', 'new', 'conjectural', 'recursion', 'solution', 'for', 'hurwitz', 'numbers', 'at', 'all', 'genera', 'this', 'conjecture', 'is', 'based', 'on', 'recent', 'progress', 'in', 'solving', 'type', 'b', 'topological', 'string', 'theory', 'on', 'the', 'mirrors', 'of', 'toric', 'calabiyau', 'manifolds', 'w... | [-0.173735941711225, 0.07532583611380113, -0.12201671522404803, 0.1284000848444473, -0.1278157404035722, -0.17077059542858286, 0.040046046893602534, 0.27744208398814263, -0.2777430226805767, -0.263126455267009, 0.07283733606485551, -0.2406675714729844, -0.23858761871723752, 0.168740254919976, -0.18899397493683193, 0.03... |
709.1459 | The NICA/MPD Project at JINR (Dubna) | A new project of Nuclotron-based Ion Collider fAcility (NICA) and
Multi-Purpose Detector (MPD) is proposed at JINR (Dubna). Status of this
NICA/MPD project is outlined. Main system parameters and some construction
details are given.
| nucl-ex hep-ph nucl-th | a new project of nuclotronbased ion collider facility nica and multipurpose detector mpd is proposed at jinr dubna status of this nicampd project is outlined main system parameters and some construction details are given | [['a', 'new', 'project', 'of', 'nuclotronbased', 'ion', 'collider', 'facility', 'nica', 'and', 'multipurpose', 'detector', 'mpd', 'is', 'proposed', 'at', 'jinr', 'dubna', 'status', 'of', 'this', 'nicampd', 'project', 'is', 'outlined', 'main', 'system', 'parameters', 'and', 'some', 'construction', 'details', 'are', 'giv... | [-0.08168169078143205, 0.17504348326474428, -0.11546143003301147, 0.04555145690477837, -0.09368240963393713, -0.1945768831321723, -0.11070596525336013, 0.31574319587910876, -0.14444861298098283, -0.28021719953154817, 0.09380410318536793, -0.3179362196036998, 0.020933189699837172, 0.2332450541571769, -0.0356322263148339... |
709.146 | On deformations of metrics and their associated spinor structures | Smooth deformations of a Minkowski type metric in a four-dimensional
space-time manifold are considered. Deformations of the basic spin-tensorial
fields associated with this metric are calculated and their application to
calculating the energy-momentum tensor of a massive spin 1/2 particle is shown.
| math.DG math-ph math.MP | smooth deformations of a minkowski type metric in a fourdimensional spacetime manifold are considered deformations of the basic spintensorial fields associated with this metric are calculated and their application to calculating the energymomentum tensor of a massive spin 12 particle is shown | [['smooth', 'deformations', 'of', 'a', 'minkowski', 'type', 'metric', 'in', 'a', 'fourdimensional', 'spacetime', 'manifold', 'are', 'considered', 'deformations', 'of', 'the', 'basic', 'spintensorial', 'fields', 'associated', 'with', 'this', 'metric', 'are', 'calculated', 'and', 'their', 'application', 'to', 'calculatin... | [-0.1948750349443539, 0.1717247358368089, -0.04212581769873699, 0.10500032133201048, -0.09335966463688583, -0.10141827539718222, -0.13551587689601416, 0.34530873437012943, -0.19428762578449787, -0.20978093426674604, 0.09347909087747601, -0.2629866633741629, -0.19400144195450203, 0.11736702009026583, -0.0639961226178067... |
709.1461 | Average twin prime conjecture for elliptic curves | Let E be an elliptic curve over Q. In 1988, Koblitz conjectured a precise
asymptotic for the number of primes p up to x such that the order of the group
of points of E over the finite field F_p is prime. This is an analogue of the
Hardy and Littlewood twin prime conjecture in the case of elliptic curves.
Koblitz's ... | math.NT | let e be an elliptic curve over q in 1988 koblitz conjectured a precise asymptotic for the number of primes p up to x such that the order of the group of points of e over the finite field f_p is prime this is an analogue of the hardy and littlewood twin prime conjecture in the case of elliptic curves koblitzs conjectur... | [['let', 'e', 'be', 'an', 'elliptic', 'curve', 'over', 'q', 'in', '1988', 'koblitz', 'conjectured', 'a', 'precise', 'asymptotic', 'for', 'the', 'number', 'of', 'primes', 'p', 'up', 'to', 'x', 'such', 'that', 'the', 'order', 'of', 'the', 'group', 'of', 'points', 'of', 'e', 'over', 'the', 'finite', 'field', 'f_p', 'is', ... | [-0.2111542217757391, 0.08264048738308939, -0.1798850796327157, 0.06322661556060548, -0.02587630508629524, -0.09344123679253719, 0.010071363616937204, 0.28119967589964684, -0.2967337198514977, -0.2722107663264741, 0.04920254798666777, -0.2641697131684455, -0.08479737308200287, 0.281267873764686, -0.16333388251697886, 0... |
709.1462 | Tau neutrino search with the MAGIC telescope | The MAGIC telescope located on the Roque de los Muchachos on the Canary
Island La Palma at a height of 2200 m a.s.l. is able to point to the sea. This
permits a search for air shower signatures induced by particles coming out of
the Earth. An analytical approximation results in tau neutrino effective areas
from ~10^3... | astro-ph | the magic telescope located on the roque de los muchachos on the canary island la palma at a height of 2200 m asl is able to point to the sea this permits a search for air shower signatures induced by particles coming out of the earth an analytical approximation results in tau neutrino effective areas from 103 m2 at 10... | [['the', 'magic', 'telescope', 'located', 'on', 'the', 'roque', 'de', 'los', 'muchachos', 'on', 'the', 'canary', 'island', 'la', 'palma', 'at', 'a', 'height', 'of', '2200', 'm', 'asl', 'is', 'able', 'to', 'point', 'to', 'the', 'sea', 'this', 'permits', 'a', 'search', 'for', 'air', 'shower', 'signatures', 'induced', 'by... | [-0.1065279064626007, 0.2347097935828709, -0.03291013164720101, 0.17516944983021118, -0.026932723466451317, -0.06921530487160235, 0.03220164176444848, 0.3434334399337454, -0.15838480411934874, -0.4023004730426988, 0.08411554613713781, -0.3433889214548665, -0.020251229390964028, 0.23613622376168247, 0.017174658827599165... |
709.1463 | Momentum and energy preserving integrators for nonholonomic dynamics | In this paper, we propose a geometric integrator for nonholonomic mechanical
systems. It can be applied to discrete Lagrangian systems specified through a
discrete Lagrangian defined on QxQ, where Q is the configuration manifold, and
a (generally nonintegrable) distribution in TQ. In the proposed method, a
discretiza... | math.NA math-ph math.DG math.MP | in this paper we propose a geometric integrator for nonholonomic mechanical systems it can be applied to discrete lagrangian systems specified through a discrete lagrangian defined on qxq where q is the configuration manifold and a generally nonintegrable distribution in tq in the proposed method a discretization of th... | [['in', 'this', 'paper', 'we', 'propose', 'a', 'geometric', 'integrator', 'for', 'nonholonomic', 'mechanical', 'systems', 'it', 'can', 'be', 'applied', 'to', 'discrete', 'lagrangian', 'systems', 'specified', 'through', 'a', 'discrete', 'lagrangian', 'defined', 'on', 'qxq', 'where', 'q', 'is', 'the', 'configuration', 'm... | [-0.16550736939278218, 0.0795856711856269, -0.12236334278393503, 0.057905963461829024, -0.09357663878846333, -0.13503803124377897, -0.04324966441698953, 0.3952649483850243, -0.28706677178553214, -0.29105238944565487, 0.10571158020394009, -0.180521816767137, -0.20611987768783482, 0.173424145275163, -0.11232993074632976,... |
709.1464 | Discrete Rotational Symmetry, Moment Isotropy, and High Order Lattice
Boltzmann Models | Conventional lattice Boltzmann models only satisfy moment isotropy up to
fourth order. In order to accurately describe improtant physical effects beyond
the isothermal Navier-Stokes fluid regime, higher order isotropy is required.
In this paper, we present some basic results on moment isotropy and its
relationship to... | physics.comp-ph physics.flu-dyn | conventional lattice boltzmann models only satisfy moment isotropy up to fourth order in order to accurately describe improtant physical effects beyond the isothermal navierstokes fluid regime higher order isotropy is required in this paper we present some basic results on moment isotropy and its relationship to the ro... | [['conventional', 'lattice', 'boltzmann', 'models', 'only', 'satisfy', 'moment', 'isotropy', 'up', 'to', 'fourth', 'order', 'in', 'order', 'to', 'accurately', 'describe', 'improtant', 'physical', 'effects', 'beyond', 'the', 'isothermal', 'navierstokes', 'fluid', 'regime', 'higher', 'order', 'isotropy', 'is', 'required'... | [-0.09474598664186291, 0.10512614359047164, -0.07871917593670455, 0.0870314574410283, -0.16233259912680936, -0.10723864765384712, 0.034094521228375065, 0.32981014916220225, -0.2790920865294096, -0.295220408336939, 0.07607954942677925, -0.2494454828304918, -0.06737316138035543, 0.12481630934603713, -0.004919216590555939... |
709.1465 | Fluctuations and Rheology in Active Bacterial Suspensions | We probe non-equilibrium properties of an active bacterial bath through
measurements of correlations of passive tracer particles and the response
function of a driven, optically trapped tracer. These measurements demonstrate
violation of the fluctuation-dissipation theorem and enable us to extract the
power spectrum ... | cond-mat.soft | we probe nonequilibrium properties of an active bacterial bath through measurements of correlations of passive tracer particles and the response function of a driven optically trapped tracer these measurements demonstrate violation of the fluctuationdissipation theorem and enable us to extract the power spectrum of the... | [['we', 'probe', 'nonequilibrium', 'properties', 'of', 'an', 'active', 'bacterial', 'bath', 'through', 'measurements', 'of', 'correlations', 'of', 'passive', 'tracer', 'particles', 'and', 'the', 'response', 'function', 'of', 'a', 'driven', 'optically', 'trapped', 'tracer', 'these', 'measurements', 'demonstrate', 'viola... | [-0.11061196072805154, 0.1926719359657506, -0.1328781500600184, 0.015449426561311076, 0.027030493922625916, -0.12916608012717548, 0.029504730982140084, 0.3216609605057519, -0.2857900963494955, -0.30372504612926066, 0.018508512246764346, -0.32470978379155263, -0.13144120607595844, 0.17480032539431337, 0.0020737536472586... |
709.1466 | A sharp bound for the Stein-Wainger oscillatory integral | Let Pd denote the space of all real polynomials of degree at most d. It is an
old result of Stein and Wainger that for every polynomial P in Pd:
|p.v.\int_R {e^{iP(t)} dt/t} | < C(d) for some constant C(d) depending only
on d. On the other hand, Carbery, Wainger and Wright claim that the true order
of magnitude of ... | math.CA | let pd denote the space of all real polynomials of degree at most d it is an old result of stein and wainger that for every polynomial p in pd pvint_r eipt dtt cd for some constant cd depending only on d on the other hand carbery wainger and wright claim that the true order of magnitude of the above principal value int... | [['let', 'pd', 'denote', 'the', 'space', 'of', 'all', 'real', 'polynomials', 'of', 'degree', 'at', 'most', 'd', 'it', 'is', 'an', 'old', 'result', 'of', 'stein', 'and', 'wainger', 'that', 'for', 'every', 'polynomial', 'p', 'in', 'pd', 'pvint_r', 'eipt', 'dtt', 'cd', 'for', 'some', 'constant', 'cd', 'depending', 'only',... | [-0.1438196494572741, 0.05457012764343423, -0.07616806514424217, 0.008809554981245823, -0.06161225827492993, -0.17231371883741198, 0.02239982853643596, 0.29410097858978107, -0.27782705896842186, -0.2536034302388811, 0.08563047074815533, -0.3034671291089206, -0.13138321788488505, 0.20442514865220907, -0.0773159741588375... |
709.1467 | Correlations of chiral condensates and quark number densities with
static quark sources | We investigate correlation functions of the Polyakov loop and static
meson/diquark systems with the chiral condensate and the quark number density
at finite temperature. In particular the latter observable can give insight in
the mechanism of screening and string breaking at finite temperature. We use
for our analysi... | hep-lat | we investigate correlation functions of the polyakov loop and static mesondiquark systems with the chiral condensate and the quark number density at finite temperature in particular the latter observable can give insight in the mechanism of screening and string breaking at finite temperature we use for our analysis gau... | [['we', 'investigate', 'correlation', 'functions', 'of', 'the', 'polyakov', 'loop', 'and', 'static', 'mesondiquark', 'systems', 'with', 'the', 'chiral', 'condensate', 'and', 'the', 'quark', 'number', 'density', 'at', 'finite', 'temperature', 'in', 'particular', 'the', 'latter', 'observable', 'can', 'give', 'insight', '... | [-0.11686022154000753, 0.29649367644879554, -0.09751752166570547, 0.079055537929868, -0.03242524713277817, -0.0847983409431489, 0.0796474980573882, 0.3821012124200078, -0.14663211763562525, -0.2734095193664817, 0.045151846134103835, -0.2570938778493334, -0.030780750400770236, 0.07854895372053279, 0.05525786590707653, 0... |
709.1468 | Spitzer Observations of Tidal Dwarf Galaxies | We present Spitzer observations of Tidal Dwarf Galaxies (TDGs) in three
interacting systems: NGC 5291, Arp105 and Stephan's Quintet. The spectra show
bright emission from polyaromatic hydrocarbons (PAHs), nebular lines and warm
molecular hydrogen, characteristic of recent episodes of star formation. The
PAH emission ... | astro-ph | we present spitzer observations of tidal dwarf galaxies tdgs in three interacting systems ngc 5291 arp105 and stephans quintet the spectra show bright emission from polyaromatic hydrocarbons pahs nebular lines and warm molecular hydrogen characteristic of recent episodes of star formation the pah emission that falls in... | [['we', 'present', 'spitzer', 'observations', 'of', 'tidal', 'dwarf', 'galaxies', 'tdgs', 'in', 'three', 'interacting', 'systems', 'ngc', '5291', 'arp105', 'and', 'stephans', 'quintet', 'the', 'spectra', 'show', 'bright', 'emission', 'from', 'polyaromatic', 'hydrocarbons', 'pahs', 'nebular', 'lines', 'and', 'warm', 'mo... | [-0.011071147384063807, 0.10712038552319428, -0.035229002218693496, 0.06880775732715846, 0.01543226484209299, -0.06094530308037065, 0.0239465408216347, 0.5184891572687775, -0.09491113579133525, -0.3087572687771171, -0.06564081100223121, -0.3165713710710406, -0.019263864768436178, 0.06277793514746008, -0.018100762821268... |
709.1469 | Intimate relations between electronic nematic, d-density wave and d-wave
superconducting states | This paper consists of two important theoretical observations on the
interplay between l = 2 condensates; d-density wave (ddw), electronic nematic
and d-wave superconducting states. (1) There is SO(4) invariance at a
transition between the nematic and d-wave superconducting states. The nematic
and d-wave pairing oper... | cond-mat.str-el cond-mat.supr-con | this paper consists of two important theoretical observations on the interplay between l 2 condensates ddensity wave ddw electronic nematic and dwave superconducting states 1 there is so4 invariance at a transition between the nematic and dwave superconducting states the nematic and dwave pairing operators can be rotat... | [['this', 'paper', 'consists', 'of', 'two', 'important', 'theoretical', 'observations', 'on', 'the', 'interplay', 'between', 'l', '2', 'condensates', 'ddensity', 'wave', 'ddw', 'electronic', 'nematic', 'and', 'dwave', 'superconducting', 'states', '1', 'there', 'is', 'so4', 'invariance', 'at', 'a', 'transition', 'betwee... | [-0.23123794878566903, 0.2806717117583113, -0.044770301392834104, 0.035281913590318126, -0.04021448819465669, -0.17636041053504284, 0.037463974065446694, 0.3170943854044059, -0.22302407713141292, -0.25583875461348465, -0.0038343570436284477, -0.36218563643550233, -0.11591423926209765, 0.0589958027603903, 0.084484664699... |
709.147 | On the Halo Occupation of Dark Baryons | We introduce a new technique that adopts the halo occupation framework for
understanding the origin of QSO absorption-line systems. Our initial study
focuses specifically on MgII absorbers. We construct a model of the gaseous
content in which the absorption equivalent width W_r is determined by the the
amount of cold... | astro-ph | we introduce a new technique that adopts the halo occupation framework for understanding the origin of qso absorptionline systems our initial study focuses specifically on mgii absorbers we construct a model of the gaseous content in which the absorption equivalent width w_r is determined by the the amount of cold gas ... | [['we', 'introduce', 'a', 'new', 'technique', 'that', 'adopts', 'the', 'halo', 'occupation', 'framework', 'for', 'understanding', 'the', 'origin', 'of', 'qso', 'absorptionline', 'systems', 'our', 'initial', 'study', 'focuses', 'specifically', 'on', 'mgii', 'absorbers', 'we', 'construct', 'a', 'model', 'of', 'the', 'gas... | [-0.09169203403261265, 0.11289196025310018, -0.029814131762607082, 0.08874989266933558, -0.02233840024752182, -0.057273623226548456, 0.03573892366201166, 0.4077468351010353, -0.17434492655053374, -0.36305141953503595, 0.016860931298710528, -0.2923157404143093, -0.002434760355490359, 0.14559784275432672, 0.0327548082700... |
709.1471 | Hypervelocity Stars III. The Space Density and Ejection History of Main
Sequence Stars from the Galactic Center | We report the discovery of 3 new unbound hypervelocity stars (HVSs), stars
traveling with such extreme velocities that dynamical ejection from a massive
black hole (MBH) is their only suggested origin. We also detect a population of
possibly bound HVSs. The significant asymmetry we observe in the velocity
distributio... | astro-ph | we report the discovery of 3 new unbound hypervelocity stars hvss stars traveling with such extreme velocities that dynamical ejection from a massive black hole mbh is their only suggested origin we also detect a population of possibly bound hvss the significant asymmetry we observe in the velocity distribution we find... | [['we', 'report', 'the', 'discovery', 'of', '3', 'new', 'unbound', 'hypervelocity', 'stars', 'hvss', 'stars', 'traveling', 'with', 'such', 'extreme', 'velocities', 'that', 'dynamical', 'ejection', 'from', 'a', 'massive', 'black', 'hole', 'mbh', 'is', 'their', 'only', 'suggested', 'origin', 'we', 'also', 'detect', 'a', ... | [-0.09070075211290411, 0.2104108661733335, -0.08403702552277537, 0.17012364095509724, -0.14594459800961582, -0.034742152297136876, 0.11052768738409213, 0.3826056687394157, -0.12918612704136953, -0.3878802463489895, 0.008888910101328898, -0.309725192229962, 0.008699914746102877, 0.18083394724696214, -0.07757790079510112... |
709.1472 | Constraints on Circumstellar Material Around the Type Ia Supernova
2007af | Patat et al. recently inferred the existence of circumstellar material around
a normal Type Ia supernova (SN) for the first time, finding time-variable Na I
D absorption lines in the spectrum of SN 2006X. We present high-resolution
spectroscopy of the bright SN Ia 2007af at three epochs and search for
variability in ... | astro-ph | patat et al recently inferred the existence of circumstellar material around a normal type ia supernova sn for the first time finding timevariable na i d absorption lines in the spectrum of sn 2006x we present highresolution spectroscopy of the bright sn ia 2007af at three epochs and search for variability in any of th... | [['patat', 'et', 'al', 'recently', 'inferred', 'the', 'existence', 'of', 'circumstellar', 'material', 'around', 'a', 'normal', 'type', 'ia', 'supernova', 'sn', 'for', 'the', 'first', 'time', 'finding', 'timevariable', 'na', 'i', 'd', 'absorption', 'lines', 'in', 'the', 'spectrum', 'of', 'sn', '2006x', 'we', 'present', ... | [-0.06454620234284032, 0.08271081097516171, 0.01318514845104295, 0.029259787076319915, -0.06905431283905167, -0.15083358311741676, 0.10017397054554603, 0.4446097777387954, -0.15798484243352318, -0.29046084694230234, 0.03091731719670592, -0.315556051146924, -0.009025037598758601, 0.13824776446837264, -0.0288029957994739... |
709.1473 | Converting Halpha luminosities into SFRs | Star-formation rates (SFRs) of galaxies are commonly calculated by converting
the measured Halpha luminosities (L_Halpha) into current SFRs. This conversion
is based on a constant initial mass function (IMF) independent of the total
SFR. As recently recognised the maximum stellar mass in a star cluster is
limited by ... | astro-ph | starformation rates sfrs of galaxies are commonly calculated by converting the measured halpha luminosities l_halpha into current sfrs this conversion is based on a constant initial mass function imf independent of the total sfr as recently recognised the maximum stellar mass in a star cluster is limited by the embedde... | [['starformation', 'rates', 'sfrs', 'of', 'galaxies', 'are', 'commonly', 'calculated', 'by', 'converting', 'the', 'measured', 'halpha', 'luminosities', 'l_halpha', 'into', 'current', 'sfrs', 'this', 'conversion', 'is', 'based', 'on', 'a', 'constant', 'initial', 'mass', 'function', 'imf', 'independent', 'of', 'the', 'to... | [-0.047874528713033354, 0.11037508485051871, -0.05764459320305063, 0.14233596783976954, -0.08378082913810302, -0.0023581035175578957, 0.035380478217714624, 0.42402952813609623, -0.13799321119163077, -0.355840592594451, 0.03531002894260192, -0.24599490767524082, 0.0013436654983984627, 0.21822975378845932, -0.05953682411... |
709.1474 | The Star Formation Law in a Multifractal ISM | The surface density of the star formation rate in different galaxies, as well
as in different parts of a single galaxy, scales nonlinearly with the surface
density of the total gas. This observationally established relation is known as
the Kennicutt-Schmidt star formation law. The slope of the star formation law
has ... | astro-ph | the surface density of the star formation rate in different galaxies as well as in different parts of a single galaxy scales nonlinearly with the surface density of the total gas this observationally established relation is known as the kennicuttschmidt star formation law the slope of the star formation law has been sh... | [['the', 'surface', 'density', 'of', 'the', 'star', 'formation', 'rate', 'in', 'different', 'galaxies', 'as', 'well', 'as', 'in', 'different', 'parts', 'of', 'a', 'single', 'galaxy', 'scales', 'nonlinearly', 'with', 'the', 'surface', 'density', 'of', 'the', 'total', 'gas', 'this', 'observationally', 'established', 'rel... | [-0.0928237477281721, 0.11926614759157937, -0.11972949077780957, 0.1070835886086282, -0.036050679664690014, -0.027032753586363378, 0.02183689330105144, 0.3603207566325857, -0.21534359652899426, -0.3315899729369079, 0.04988168099823657, -0.24081153772070563, -0.06960349199869255, 0.16304701211687067, -0.0047011238852478... |
709.1475 | Discovery of Very High Energy Gamma-Rays from the Distant Flat Spectrum
Radio Quasar 3C 279 with the MAGIC Telescope | The quasar 3C 279 is one of the best-studied flat spectrum radio quasars. It
is located at a comparatively large redshift of z=0.536: E>100 GeV observations
of such distant sources were until recently impossible both due to the expected
steep energy spectrum and the expected attenuation of the gamma-rays by the
extra... | astro-ph | the quasar 3c 279 is one of the beststudied flat spectrum radio quasars it is located at a comparatively large redshift of z0536 e100 gev observations of such distant sources were until recently impossible both due to the expected steep energy spectrum and the expected attenuation of the gammarays by the extragalactic ... | [['the', 'quasar', '3c', '279', 'is', 'one', 'of', 'the', 'beststudied', 'flat', 'spectrum', 'radio', 'quasars', 'it', 'is', 'located', 'at', 'a', 'comparatively', 'large', 'redshift', 'of', 'z0536', 'e100', 'gev', 'observations', 'of', 'such', 'distant', 'sources', 'were', 'until', 'recently', 'impossible', 'both', 'd... | [-0.07933182674848165, 0.14546634639555123, -0.0530605079450955, 0.10984189363080077, -0.10057598410639912, -0.09259835552074946, 0.0564001892998931, 0.44863070570863783, -0.107516369074195, -0.43090214147014194, 0.09253671020511926, -0.3235362168246259, -0.0198208371924314, 0.22051118803210557, -0.02111265690473374, -... |
709.1476 | Considerations for the habitable zone of super-Earth planets in Gliese
581 | We assess the possibility that planets Gliese 581 c and d are within the
habitable zone. In analogy with our solar system, we use an empirical
definition of the habitable zone. We include assumptions such as planetary
climates, and atmospheric circulation on gravitationally locked synchronous
rotation. Based on the d... | astro-ph | we assess the possibility that planets gliese 581 c and d are within the habitable zone in analogy with our solar system we use an empirical definition of the habitable zone we include assumptions such as planetary climates and atmospheric circulation on gravitationally locked synchronous rotation based on the differen... | [['we', 'assess', 'the', 'possibility', 'that', 'planets', 'gliese', '581', 'c', 'and', 'd', 'are', 'within', 'the', 'habitable', 'zone', 'in', 'analogy', 'with', 'our', 'solar', 'system', 'we', 'use', 'an', 'empirical', 'definition', 'of', 'the', 'habitable', 'zone', 'we', 'include', 'assumptions', 'such', 'as', 'plan... | [-0.15021665057274283, 0.2114230679975752, -0.061113253793083744, 0.05761034827828255, -0.11628125990611181, -0.05600711339931996, 0.13440750431666365, 0.3052325948584275, -0.15730245032759962, -0.3262563858517125, 0.11929954549862591, -0.22840154136828772, -0.14114024320647853, 0.20977405453726772, -0.1412718793888744... |
709.1477 | Random walks on quasisymmetric functions | Conditions are provided under which an endomorphism on quasisymmetric
functions gives rise to a left random walk on the descent algebra which is also
a lumping of a left random walk on permutations. Spectral results are also
obtained. Several well-studied random walks are now realized this way:
Stanley's QS-distribut... | math.CO math.PR | conditions are provided under which an endomorphism on quasisymmetric functions gives rise to a left random walk on the descent algebra which is also a lumping of a left random walk on permutations spectral results are also obtained several wellstudied random walks are now realized this way stanleys qsdistribution resu... | [['conditions', 'are', 'provided', 'under', 'which', 'an', 'endomorphism', 'on', 'quasisymmetric', 'functions', 'gives', 'rise', 'to', 'a', 'left', 'random', 'walk', 'on', 'the', 'descent', 'algebra', 'which', 'is', 'also', 'a', 'lumping', 'of', 'a', 'left', 'random', 'walk', 'on', 'permutations', 'spectral', 'results'... | [-0.10149034500876762, 0.11712789762845957, -0.11638491707532828, 0.04566639730634553, -0.058252728831199606, -0.14485649483133878, 0.02878965095291717, 0.34721936228492395, -0.31456432571827336, -0.19592562785115222, 0.11424164812819197, -0.2589403248616847, -0.1862944003098227, 0.2629239770888897, -0.1420642483160542... |
709.1478 | Efficient one- and two-qubit pulsed gates for an oscillator stabilized
Josephson qubit | We present theoretical schemes for performing high-fidelity one- and
two-qubit pulsed gates for a superconducting flux qubit. The "IBM qubit"
consists of three Josephson junctions, three loops, and a superconducting
transmission line. Assuming a fixed inductive qubit-qubit coupling, we show
that the effective qubit-q... | quant-ph cond-mat.supr-con | we present theoretical schemes for performing highfidelity one and twoqubit pulsed gates for a superconducting flux qubit the ibm qubit consists of three josephson junctions three loops and a superconducting transmission line assuming a fixed inductive qubitqubit coupling we show that the effective qubitqubit interacti... | [['we', 'present', 'theoretical', 'schemes', 'for', 'performing', 'highfidelity', 'one', 'and', 'twoqubit', 'pulsed', 'gates', 'for', 'a', 'superconducting', 'flux', 'qubit', 'the', 'ibm', 'qubit', 'consists', 'of', 'three', 'josephson', 'junctions', 'three', 'loops', 'and', 'a', 'superconducting', 'transmission', 'lin... | [-0.1969495841740247, 0.15751282557672205, 0.009768907807986525, 0.02367516098174212, 0.05716405343127382, -0.2337373794933014, 0.11072654774248161, 0.4506194372606628, -0.19469425142468774, -0.32079871377962477, 0.04243571910842815, -0.21549084785613506, -0.05930942683754598, 0.29402774162042666, -0.06911968459813472,... |
709.1479 | Weak lensing ellipticities in a strong lensing regime | It is now routine to measure the weak gravitational lensing shear signal from
the mean ellipticity of distant galaxies. However, conversion between
ellipticity and shear assumes local linearity of the lensing potential (ie that
the spatial derivatives of the shear are small), and this condition is not
satisfied in so... | astro-ph | it is now routine to measure the weak gravitational lensing shear signal from the mean ellipticity of distant galaxies however conversion between ellipticity and shear assumes local linearity of the lensing potential ie that the spatial derivatives of the shear are small and this condition is not satisfied in some of t... | [['it', 'is', 'now', 'routine', 'to', 'measure', 'the', 'weak', 'gravitational', 'lensing', 'shear', 'signal', 'from', 'the', 'mean', 'ellipticity', 'of', 'distant', 'galaxies', 'however', 'conversion', 'between', 'ellipticity', 'and', 'shear', 'assumes', 'local', 'linearity', 'of', 'the', 'lensing', 'potential', 'ie',... | [-0.10961198555347529, 0.07450333855592624, -0.10906443537915346, 0.1271506791640373, -0.09210962724035322, -0.06150405661408174, 0.013371423363362013, 0.34379127433807666, -0.2405770741609296, -0.32311665194140654, 0.09037521424761508, -0.25780492556139323, -0.08711539430990697, 0.20980349964446435, -0.022241345395124... |
709.148 | Connection between the Green functions of the supersymmetric pair of
Dirac Hamiltonians | The Sukumar theorem about the connection between the Green functions of the
supersymmetric pair of the Schr\"odinger Hamiltonians is generalized to the
case of the supersymmetric pair of the Dirac Hamiltonians.
| hep-th | the sukumar theorem about the connection between the green functions of the supersymmetric pair of the schrodinger hamiltonians is generalized to the case of the supersymmetric pair of the dirac hamiltonians | [['the', 'sukumar', 'theorem', 'about', 'the', 'connection', 'between', 'the', 'green', 'functions', 'of', 'the', 'supersymmetric', 'pair', 'of', 'the', 'schrodinger', 'hamiltonians', 'is', 'generalized', 'to', 'the', 'case', 'of', 'the', 'supersymmetric', 'pair', 'of', 'the', 'dirac', 'hamiltonians']] | [-0.15981037256818625, 0.10475321102046198, -0.04719202160354583, 0.13546979693590752, -0.0344184193414666, -0.1238470236740766, -0.007575032511545766, 0.2811912937510398, -0.20279239247282665, -0.24605803960754025, -0.017435149424859592, -0.34368094071866045, -0.15807096419795866, 0.16061949249236815, 0.04230326636423... |
709.1481 | Testing Spontaneous Parity Violation at the LHC | We construct a supersymmetric SU(2)_L X SU(2)_R X U(1)_B-L model in which a
discrete symmetry (C-parity) implements strict left-right symmetry in the
scalar (Higgs) sector. Although two electroweak bidoublets are introduced to
accommodate the observed fermion masses and mixings, a natural missing partner
mechanism in... | hep-ph | we construct a supersymmetric su2_l x su2_r x u1_bl model in which a discrete symmetry cparity implements strict leftright symmetry in the scalar higgs sector although two electroweak bidoublets are introduced to accommodate the observed fermion masses and mixings a natural missing partner mechanism insures that a sing... | [['we', 'construct', 'a', 'supersymmetric', 'su2_l', 'x', 'su2_r', 'x', 'u1_bl', 'model', 'in', 'which', 'a', 'discrete', 'symmetry', 'cparity', 'implements', 'strict', 'leftright', 'symmetry', 'in', 'the', 'scalar', 'higgs', 'sector', 'although', 'two', 'electroweak', 'bidoublets', 'are', 'introduced', 'to', 'accommod... | [-0.15200574714638126, 0.37645094252578665, 0.00020369781139359044, 0.2614411737788155, -0.1578766707922175, -0.2939175945455522, -0.04022380304679777, 0.3577207920947269, -0.20749217550155152, -0.26912162588972055, 0.011829884470377661, -0.2205427747816266, 0.04116102000973135, -0.009124380790136671, 0.046803871938812... |
709.1482 | Localized modes at a D-brane--O-plane intersection and heterotic Alice
strings | We study a system of $N_c$ $D3$-branes intersecting $D7$-branes and
$O7$-planes in 1+1-dimensions. We use anomaly cancellation and string dualities
to argue that there must be chiral fermion zero-modes on the $D3$-branes which
are localized near the $O7$-planes. Away from the orientifold limit we verify
this by using... | hep-th | we study a system of n_c d3branes intersecting d7branes and o7planes in 11dimensions we use anomaly cancellation and string dualities to argue that there must be chiral fermion zeromodes on the d3branes which are localized near the o7planes away from the orientifold limit we verify this by using index theory as well as... | [['we', 'study', 'a', 'system', 'of', 'n_c', 'd3branes', 'intersecting', 'd7branes', 'and', 'o7planes', 'in', '11dimensions', 'we', 'use', 'anomaly', 'cancellation', 'and', 'string', 'dualities', 'to', 'argue', 'that', 'there', 'must', 'be', 'chiral', 'fermion', 'zeromodes', 'on', 'the', 'd3branes', 'which', 'are', 'lo... | [-0.1572832172404569, 0.19049359699103194, -0.04773093489319141, 0.1504991433092181, -0.053529664597446375, -0.1820493547734574, 0.025703166037484414, 0.28773526620525536, -0.12182531203373824, -0.22260076508368595, 0.12578413681712666, -0.3484739796074089, -0.18216966833956172, 0.03864641747631059, -0.1507531826817753... |
709.1483 | Microcausality in Curved Space-Time | It is well known that in Lorentz invariant quantum field theories in flat
space the commutator of space-like separated local operators vanishes
(microcausality). We provide two different arguments showing that this is a
consequence of the causal structure of the classical theory, rather than of
Lorentz invariance. In... | hep-th gr-qc | it is well known that in lorentz invariant quantum field theories in flat space the commutator of spacelike separated local operators vanishes microcausality we provide two different arguments showing that this is a consequence of the causal structure of the classical theory rather than of lorentz invariance in particu... | [['it', 'is', 'well', 'known', 'that', 'in', 'lorentz', 'invariant', 'quantum', 'field', 'theories', 'in', 'flat', 'space', 'the', 'commutator', 'of', 'spacelike', 'separated', 'local', 'operators', 'vanishes', 'microcausality', 'we', 'provide', 'two', 'different', 'arguments', 'showing', 'that', 'this', 'is', 'a', 'co... | [-0.1941901782884934, 0.21665099952089042, -0.11329228768861571, 0.15026040330020235, -0.09734995333683612, -0.14621841622689782, -0.024699602935322407, 0.34507753836467514, -0.22492434992996413, -0.22033929796537471, 0.04966960521008776, -0.21986315630614583, -0.15158412191302104, 0.16123386072861248, -0.0517658126475... |
709.1484 | Ascertaining the Core Collapse Supernova Mechanism: An Emerging Picture? | Here we present the results from two sets of simulations, in two and three
spatial dimensions. In two dimensions, the simulations include multifrequency
flux-limited diffusion neutrino transport in the "ray-by-ray-plus"
approximation, two-dimensional self gravity in the Newtonian limit, and nuclear
burning through a ... | astro-ph | here we present the results from two sets of simulations in two and three spatial dimensions in two dimensions the simulations include multifrequency fluxlimited diffusion neutrino transport in the raybyrayplus approximation twodimensional self gravity in the newtonian limit and nuclear burning through a 14isotope alph... | [['here', 'we', 'present', 'the', 'results', 'from', 'two', 'sets', 'of', 'simulations', 'in', 'two', 'and', 'three', 'spatial', 'dimensions', 'in', 'two', 'dimensions', 'the', 'simulations', 'include', 'multifrequency', 'fluxlimited', 'diffusion', 'neutrino', 'transport', 'in', 'the', 'raybyrayplus', 'approximation', ... | [-0.10629130690646024, 0.16333087194527005, -0.03312042789328211, 0.08791004802069699, -0.0533993128646901, -0.0736693386157348, 0.024479176983267927, 0.3576054092987207, -0.2225926437542377, -0.29166359338457143, 0.1074870261172055, -0.25703412216298527, -0.0802566333532088, 0.19359728482737754, 0.03747771410527831, 0... |
709.1485 | Compact Stars as Dark Matter Probes | We discuss the consequences of the accretion of dark matter (DM) particles on
compact stars such as white dwarfs and neutron stars. We show that in large
regions of the DM parameter space, these objects are sensitive probes of the
presence of DM and can be used to set constraints both on the DM density and on
the phy... | astro-ph hep-ph | we discuss the consequences of the accretion of dark matter dm particles on compact stars such as white dwarfs and neutron stars we show that in large regions of the dm parameter space these objects are sensitive probes of the presence of dm and can be used to set constraints both on the dm density and on the physical ... | [['we', 'discuss', 'the', 'consequences', 'of', 'the', 'accretion', 'of', 'dark', 'matter', 'dm', 'particles', 'on', 'compact', 'stars', 'such', 'as', 'white', 'dwarfs', 'and', 'neutron', 'stars', 'we', 'show', 'that', 'in', 'large', 'regions', 'of', 'the', 'dm', 'parameter', 'space', 'these', 'objects', 'are', 'sensit... | [-0.10823122184309694, 0.20163776639789815, -0.09435047972060386, 0.16034209607021202, -0.12180103204907879, -0.003990724076709104, 0.029007333844515776, 0.32351361203288276, -0.1845825438254646, -0.3869363064508116, 0.04569874108687694, -0.28407591714390684, -0.01755317874134533, 0.22181207816752177, -0.00687108056560... |
709.1486 | Diquark Higgs at LHC | Existence of color sextet diquark Higgs fields with TeV masses will indicate
a fundamentally different direction for unification than conventional grand
unified theories. There is a class of partial unification models based on the
gauge group $SU(2)_L\times SU(2)_R\times SU(4)_c$ that implement the seesaw
mechanism f... | hep-ph | existence of color sextet diquark higgs fields with tev masses will indicate a fundamentally different direction for unification than conventional grand unified theories there is a class of partial unification models based on the gauge group su2_ltimes su2_rtimes su4_c that implement the seesaw mechanism for neutrino m... | [['existence', 'of', 'color', 'sextet', 'diquark', 'higgs', 'fields', 'with', 'tev', 'masses', 'will', 'indicate', 'a', 'fundamentally', 'different', 'direction', 'for', 'unification', 'than', 'conventional', 'grand', 'unified', 'theories', 'there', 'is', 'a', 'class', 'of', 'partial', 'unification', 'models', 'based',... | [-0.1077091295572775, 0.27664914597045837, -0.058018073868593124, 0.2026825737882787, -0.12204763587329566, -0.1969527003875985, 0.025774190297687617, 0.40262031368361273, -0.19633628754311894, -0.3222747938194144, 0.05673290154251351, -0.22128756396384455, 0.0053336472657516485, 0.1307533637869839, 0.03462366892142207... |
709.1487 | Spectropolarimetry of the Type IIb Supernova 2001ig | We present spectropolarimetric observations of the Type IIb SN 2001ig in NGC
7424; conducted with the ESO VLT FORS1 on 2001 Dec 16, 2002 Jan 3 and 2002 Aug
16 or 13, 31 and 256 days post-explosion. These observations are at three
different stages of the SN evolution: (1) The hydrogen-rich photospheric phase,
(2) the ... | astro-ph | we present spectropolarimetric observations of the type iib sn 2001ig in ngc 7424 conducted with the eso vlt fors1 on 2001 dec 16 2002 jan 3 and 2002 aug 16 or 13 31 and 256 days postexplosion these observations are at three different stages of the sn evolution 1 the hydrogenrich photospheric phase 2 the type ii to typ... | [['we', 'present', 'spectropolarimetric', 'observations', 'of', 'the', 'type', 'iib', 'sn', '2001ig', 'in', 'ngc', '7424', 'conducted', 'with', 'the', 'eso', 'vlt', 'fors1', 'on', '2001', 'dec', '16', '2002', 'jan', '3', 'and', '2002', 'aug', '16', 'or', '13', '31', 'and', '256', 'days', 'postexplosion', 'these', 'obse... | [-0.07442916979959842, 0.1072521801019529, -0.03580576785436187, 0.04466908007791753, -0.07351959242876019, -0.11940087220906097, 0.027030911665045954, 0.4258807575543775, -0.21332237231636947, -0.3086326703108767, 0.09687399334986911, -0.2974522112214464, -0.06123239966610106, 0.16818624580742986, -0.02784584637265652... |
709.1488 | A novel concept for increasing the peak sensitivity of LIGO by detuning
the arm cavities | We introduce a concept that uses detuned arm cavities to increase the shot
noise limited sensitivity of LIGO without increasing the light power inside the
arm cavities. Numerical simulations show an increased sensitivity between 125
and 400 Hz, with a maximal improvement of about 80% around 225 Hz, while the
sensitiv... | gr-qc | we introduce a concept that uses detuned arm cavities to increase the shot noise limited sensitivity of ligo without increasing the light power inside the arm cavities numerical simulations show an increased sensitivity between 125 and 400 hz with a maximal improvement of about 80 around 225 hz while the sensitivity ab... | [['we', 'introduce', 'a', 'concept', 'that', 'uses', 'detuned', 'arm', 'cavities', 'to', 'increase', 'the', 'shot', 'noise', 'limited', 'sensitivity', 'of', 'ligo', 'without', 'increasing', 'the', 'light', 'power', 'inside', 'the', 'arm', 'cavities', 'numerical', 'simulations', 'show', 'an', 'increased', 'sensitivity',... | [-0.11791690092650242, 0.13258358321386018, -0.031389111888039715, 0.007856609310972719, -0.09673974621826066, -0.14892207499808416, 0.10878106039420415, 0.3892446933582855, -0.21305875052572587, -0.3485997823255065, 0.0851544799280908, -0.2900118474006796, -0.10512862997487761, 0.26377761779720177, -0.0789248213606277... |
709.1489 | Making black holes visible: accretion, radiation, and jets | With the fundamental stress mechanism of accretion disks
identified--correlated MHD turbulence driven by the magneto-rotational
instability--it has become possible to make numerical simulations of accretion
disk dynamics based on well-understood physics. A sampling of results from both
Newtonian 3-d shearing box and ... | astro-ph | with the fundamental stress mechanism of accretion disks identifiedcorrelated mhd turbulence driven by the magnetorotational instabilityit has become possible to make numerical simulations of accretion disk dynamics based on wellunderstood physics a sampling of results from both newtonian 3d shearing box and general re... | [['with', 'the', 'fundamental', 'stress', 'mechanism', 'of', 'accretion', 'disks', 'identifiedcorrelated', 'mhd', 'turbulence', 'driven', 'by', 'the', 'magnetorotational', 'instabilityit', 'has', 'become', 'possible', 'to', 'make', 'numerical', 'simulations', 'of', 'accretion', 'disk', 'dynamics', 'based', 'on', 'wellu... | [-0.13602380859816326, 0.1813739657170883, -0.06696102391633628, 0.11982263860576652, -0.09821998846898083, -0.10952549531935252, -0.04407088481862996, 0.34950605040188315, -0.23727057865157508, -0.31556149198264954, 0.05241366445502307, -0.2747040025319522, -0.042521654608116737, 0.2274926606860521, -0.007178414003293... |
709.149 | Ricci iterations on Kahler classes | In this paper we consider the dynamical system involved by the Ricci operator
on the space of K\"ahler metrics. A. Nadel has defined an iteration scheme
given by the Ricci operator for Fano manifold and asked whether it has some
nontrivial periodic points. First, we prove that no such periodic points can
exist. We de... | math.DG math.CV math.DS | in this paper we consider the dynamical system involved by the ricci operator on the space of kahler metrics a nadel has defined an iteration scheme given by the ricci operator for fano manifold and asked whether it has some nontrivial periodic points first we prove that no such periodic points can exist we define the ... | [['in', 'this', 'paper', 'we', 'consider', 'the', 'dynamical', 'system', 'involved', 'by', 'the', 'ricci', 'operator', 'on', 'the', 'space', 'of', 'kahler', 'metrics', 'a', 'nadel', 'has', 'defined', 'an', 'iteration', 'scheme', 'given', 'by', 'the', 'ricci', 'operator', 'for', 'fano', 'manifold', 'and', 'asked', 'whet... | [-0.19451503902673722, 0.016651833238089844, -0.1109918884622554, 0.09190517602449594, -0.07513700338701407, -0.1699165669172847, 0.012958925618052793, 0.38517156331799923, -0.2583954412334909, -0.16251889762546246, 0.12996769308131964, -0.2738116301130503, -0.22247267402126453, 0.16346534825182366, -0.1373806083012217... |
709.1491 | Moduli and multi-field inflation | Moduli with flat or run-away classical potentials are generic in theories
based on supersymmetry and extra dimensions. They mix between themselves and
with matter fields in kinetic terms and in the nonperturbative superpotentials.
As the result, interesting structure appears in the scalar potential which
helps to sta... | hep-th | moduli with flat or runaway classical potentials are generic in theories based on supersymmetry and extra dimensions they mix between themselves and with matter fields in kinetic terms and in the nonperturbative superpotentials as the result interesting structure appears in the scalar potential which helps to stabilise... | [['moduli', 'with', 'flat', 'or', 'runaway', 'classical', 'potentials', 'are', 'generic', 'in', 'theories', 'based', 'on', 'supersymmetry', 'and', 'extra', 'dimensions', 'they', 'mix', 'between', 'themselves', 'and', 'with', 'matter', 'fields', 'in', 'kinetic', 'terms', 'and', 'in', 'the', 'nonperturbative', 'superpote... | [-0.13301049123437683, 0.22291897805454353, -0.13232624564710774, 0.11509357923986735, -0.0936122802718554, -0.17917608267363208, -0.06184403452142659, 0.31032401972944723, -0.23826496715852877, -0.3217528278258181, 0.039655884009222556, -0.2291431902896291, -0.17300495856303583, 0.13390542702162983, -0.058175317632655... |
709.1492 | SGRs and AXPs proposed as ancestors of the Magnificent seven | The recently suggested correlation between the surface temperature and the
magnetic field in isolated neutron stars does not seem to work well for SGRs,
AXPs and X-ray dim isolated neutron stars (XDINs; specifically the Magnificent
Seven or M7). Instead by appealing to a Color-Flavor Locked Quark Star (CFLQS)
we find... | astro-ph | the recently suggested correlation between the surface temperature and the magnetic field in isolated neutron stars does not seem to work well for sgrs axps and xray dim isolated neutron stars xdins specifically the magnificent seven or m7 instead by appealing to a colorflavor locked quark star cflqs we find a more nat... | [['the', 'recently', 'suggested', 'correlation', 'between', 'the', 'surface', 'temperature', 'and', 'the', 'magnetic', 'field', 'in', 'isolated', 'neutron', 'stars', 'does', 'not', 'seem', 'to', 'work', 'well', 'for', 'sgrs', 'axps', 'and', 'xray', 'dim', 'isolated', 'neutron', 'stars', 'xdins', 'specifically', 'the', ... | [-0.10664268948951579, 0.22618758495653343, -0.07006944686383287, 0.17351620723863315, -0.18216840713502508, -0.050612203607109385, 0.09649374446544413, 0.40723291676595946, -0.1104798287318619, -0.3545114797687976, 0.029398346905135243, -0.32286160400955477, -0.10000416531584391, 0.23595498183472344, -0.06665041748538... |
709.1493 | Marginal and density atomic Wehrl entropies for the Jaynes-Cummings
model | In this paper, we develop the notion of the marginal and density atomic Wehrl
entropies for two-level atom interacting with the single mode field, i.e.
Jaynes-Cummings model. For this system we show that there are relationships
between these quantities and both of the information entropies and the von
Neumann entropy... | quant-ph | in this paper we develop the notion of the marginal and density atomic wehrl entropies for twolevel atom interacting with the single mode field ie jaynescummings model for this system we show that there are relationships between these quantities and both of the information entropies and the von neumann entropy | [['in', 'this', 'paper', 'we', 'develop', 'the', 'notion', 'of', 'the', 'marginal', 'and', 'density', 'atomic', 'wehrl', 'entropies', 'for', 'twolevel', 'atom', 'interacting', 'with', 'the', 'single', 'mode', 'field', 'ie', 'jaynescummings', 'model', 'for', 'this', 'system', 'we', 'show', 'that', 'there', 'are', 'relat... | [-0.1032485049776733, 0.17931473553180693, -0.05697709349915385, 0.03911328978370875, 0.07798671374097467, -0.18528946889564396, 0.041857837496791034, 0.341556493784301, -0.2728984531201422, -0.2522558622434735, 0.014642217608634383, -0.3487164221704006, -0.11100127527024597, 0.14019092253874987, -0.058044255988206714,... |
709.1494 | Spectral resolved Measurement of the Nitrogen Fluorescence Emissions in
Air induced by Electrons | For the calorimetric determination of the primary energy of extensive air
showers, measured by fluorescence telescopes, a precise knowledge of the
conversion factor (fluorescence yield) between the deposited energy in the
atmosphere and the number of emitted fluorescence photons is essential. The
fluorescence yield d... | astro-ph | for the calorimetric determination of the primary energy of extensive air showers measured by fluorescence telescopes a precise knowledge of the conversion factor fluorescence yield between the deposited energy in the atmosphere and the number of emitted fluorescence photons is essential the fluorescence yield depends ... | [['for', 'the', 'calorimetric', 'determination', 'of', 'the', 'primary', 'energy', 'of', 'extensive', 'air', 'showers', 'measured', 'by', 'fluorescence', 'telescopes', 'a', 'precise', 'knowledge', 'of', 'the', 'conversion', 'factor', 'fluorescence', 'yield', 'between', 'the', 'deposited', 'energy', 'in', 'the', 'atmosp... | [-7.555512049552148e-05, 0.18660416862889556, -0.037832543062433825, 0.011794404310338569, 0.06575259143666265, -0.060934467061522044, 0.04481394078965455, 0.4115107812148136, -0.2009742684463786, -0.40832543942302013, 0.048535945302887164, -0.33837258203550796, 0.028505801946529883, 0.227580275455121, 0.02402958893075... |
709.1495 | Thermodynamic restrictions on evolutionary optimization of transcription
factor proteins | Conformational fluctuations are believed to play an important role in the
process by which transcription factor proteins locate and bind their target
site on the genome of a bacterium. Using a simple model, we show that the
binding time can be minimized, under selective pressure, by adjusting the
spectrum of conforma... | cond-mat.soft q-bio.BM | conformational fluctuations are believed to play an important role in the process by which transcription factor proteins locate and bind their target site on the genome of a bacterium using a simple model we show that the binding time can be minimized under selective pressure by adjusting the spectrum of conformational... | [['conformational', 'fluctuations', 'are', 'believed', 'to', 'play', 'an', 'important', 'role', 'in', 'the', 'process', 'by', 'which', 'transcription', 'factor', 'proteins', 'locate', 'and', 'bind', 'their', 'target', 'site', 'on', 'the', 'genome', 'of', 'a', 'bacterium', 'using', 'a', 'simple', 'model', 'we', 'show', ... | [-0.11042989646517301, 0.18867749353060478, -0.045077715254495894, 0.05806740402587933, 0.015612845004132363, -0.12286245118799842, 0.08352706015967162, 0.42229936288389486, -0.26516756777593914, -0.294751095865746, 0.013182200323501848, -0.2298519296027654, -0.1471085056365855, 0.1615304436547006, -0.03795597686811424... |
709.1496 | Coalescence in low-viscosity liquids | The expected universal dynamics associated with the initial stage of droplet
coalescence are difficult to study visually due to the rapid motion of the
liquid and the awkward viewing geometry. Here we employ an electrical method to
study the coalescence of two inviscid droplets at early times. We measure the
growth d... | cond-mat.soft | the expected universal dynamics associated with the initial stage of droplet coalescence are difficult to study visually due to the rapid motion of the liquid and the awkward viewing geometry here we employ an electrical method to study the coalescence of two inviscid droplets at early times we measure the growth dynam... | [['the', 'expected', 'universal', 'dynamics', 'associated', 'with', 'the', 'initial', 'stage', 'of', 'droplet', 'coalescence', 'are', 'difficult', 'to', 'study', 'visually', 'due', 'to', 'the', 'rapid', 'motion', 'of', 'the', 'liquid', 'and', 'the', 'awkward', 'viewing', 'geometry', 'here', 'we', 'employ', 'an', 'elect... | [-0.11228032419140535, 0.1730778011328353, -0.1560818642610684, 0.033164188694420525, -0.028273157796568492, -0.13195650207026946, 0.010597144467861985, 0.34954743713288655, -0.24643701635597443, -0.28719212108196435, 0.1048816130906661, -0.2828298583838411, -0.1218790560325777, 0.1566929779814514, -0.02566346621923995... |
709.1497 | Selection of special orientations in relativistic collisions of deformed
heavy nuclei | We have studied U+U collisions at $\sqrt{s_{NN}}$ = 200 GeV using Monte Carlo
Glauber, UrQMD and AMPT models. We find that it is possible to separate central
tip-tip events as well as central body-body events on the basis of cuts on
multiplicity and magnitude of the reduced flow vector.
| hep-ph | we have studied uu collisions at sqrts_nn 200 gev using monte carlo glauber urqmd and ampt models we find that it is possible to separate central tiptip events as well as central bodybody events on the basis of cuts on multiplicity and magnitude of the reduced flow vector | [['we', 'have', 'studied', 'uu', 'collisions', 'at', 'sqrts_nn', '200', 'gev', 'using', 'monte', 'carlo', 'glauber', 'urqmd', 'and', 'ampt', 'models', 'we', 'find', 'that', 'it', 'is', 'possible', 'to', 'separate', 'central', 'tiptip', 'events', 'as', 'well', 'as', 'central', 'bodybody', 'events', 'on', 'the', 'basis',... | [-0.047971830082436405, 0.18491522539018965, -0.18055790939251892, 0.2111505146337246, 0.05233072986205419, -0.07202436813774209, -0.08280331462932129, 0.4208770792465657, -0.215255520810994, -0.32036552554927766, -0.023208341153804213, -0.3821730051810543, 0.11094398747081868, 0.17075583695744476, 0.057668535048530124... |
709.1498 | Some remarks on conic degeneration and bending of Poincar\'e-Einstein
metrics | Let $(M,g)$ be a compact K\"ahler-Einstein manifold with $c_1 > 0$. Denote by
$K\to M$ the canonical line-bundle, with total space $X$, and $X_0$ the
singular space obtained by blowing down $X$ along its zero section. We employ a
construction by Page and Pope and discuss an interesting multi-parameter family
of Poinc... | math.DG | let mg be a compact kahlereinstein manifold with c_1 0 denote by kto m the canonical linebundle with total space x and x_0 the singular space obtained by blowing down x along its zero section we employ a construction by page and pope and discuss an interesting multiparameter family of poincareeinstein metrics on x one ... | [['let', 'mg', 'be', 'a', 'compact', 'kahlereinstein', 'manifold', 'with', 'c_1', '0', 'denote', 'by', 'kto', 'm', 'the', 'canonical', 'linebundle', 'with', 'total', 'space', 'x', 'and', 'x_0', 'the', 'singular', 'space', 'obtained', 'by', 'blowing', 'down', 'x', 'along', 'its', 'zero', 'section', 'we', 'employ', 'a', ... | [-0.20624705356506942, 0.08617474331428336, -0.07367651321110316, -0.013557261927053333, -0.11820747337769717, -0.21704376647636917, 0.006626331018439183, 0.36541101853363217, -0.258505952412573, -0.1594507779183914, 0.09667618908376123, -0.34145876007775466, -0.10746983449207619, 0.1451438956564137, -0.115258181182434... |
709.1499 | Markoff Equation and Nilpotent Matrices | A triple (a,b,c) of positive integers is called a Markoff triple iff it
satisfies the diophantine equation a2 + b2 + c2 = abc .
Recasting the Markoff tree, whose vertices are Markoff triples, in the
framework of intergral upper triangular 3x3 matrices, it will be shown that the
largest member of such a triple deter... | math.NT | a triple abc of positive integers is called a markoff triple iff it satisfies the diophantine equation a2 b2 c2 abc recasting the markoff tree whose vertices are markoff triples in the framework of intergral upper triangular 3x3 matrices it will be shown that the largest member of such a triple determines the other two... | [['a', 'triple', 'abc', 'of', 'positive', 'integers', 'is', 'called', 'a', 'markoff', 'triple', 'iff', 'it', 'satisfies', 'the', 'diophantine', 'equation', 'a2', 'b2', 'c2', 'abc', 'recasting', 'the', 'markoff', 'tree', 'whose', 'vertices', 'are', 'markoff', 'triples', 'in', 'the', 'framework', 'of', 'intergral', 'uppe... | [-0.23483659233726725, 0.10559121101601597, -0.03773133466978941, 0.059543107389746344, -0.08712920078131206, -0.19710291678305059, 0.01591067566187121, 0.306193065497449, -0.32499670229085226, -0.2464915223981199, 0.1036824658016592, -0.32387955248465433, -0.1444150116157663, 0.14395297234467067, -0.017594241016708752... |
709.15 | The Graver Complexity of Integer Programming | In this article we establish an exponential lower bound on the Graver
complexity of integer programs. This provides new type of evidence supporting
the presumable intractability of integer programming. Specifically, we show
that the Graver complexity of the incidence matrix of the complete bipartite
graph $K_{3,m}$ s... | math.CO cs.CC cs.DM math.AC | in this article we establish an exponential lower bound on the graver complexity of integer programs this provides new type of evidence supporting the presumable intractability of integer programming specifically we show that the graver complexity of the incidence matrix of the complete bipartite graph k_3m satisfies g... | [['in', 'this', 'article', 'we', 'establish', 'an', 'exponential', 'lower', 'bound', 'on', 'the', 'graver', 'complexity', 'of', 'integer', 'programs', 'this', 'provides', 'new', 'type', 'of', 'evidence', 'supporting', 'the', 'presumable', 'intractability', 'of', 'integer', 'programming', 'specifically', 'we', 'show', '... | [-0.19185817079143783, 0.05382141714953297, -0.06943896539308422, 0.07355686106865167, -0.10750663735191612, -0.1363531863682118, 0.08877173752761354, 0.2892530451428291, -0.26561485464666407, -0.2893306985862699, 0.11075050652931061, -0.24394097003866644, -0.2002551857126402, 0.1535839071570366, -0.09797211135646292, ... |
709.1501 | The Luminous and Carbon-Rich Supernova 2006gz: A Double Degenerate
Merger? | Spectra and light curves of SN 2006gz show the strongest signature of
unburned carbon and one of the slowest fading light curves ever seen in a type
Ia event (Delta m_15 = 0.69 +/- 0.04). The early-time Si II velocity is low,
implying it was slowed by an envelope of unburned material. Our best estimate
of the luminos... | astro-ph | spectra and light curves of sn 2006gz show the strongest signature of unburned carbon and one of the slowest fading light curves ever seen in a type ia event delta m_15 069 004 the earlytime si ii velocity is low implying it was slowed by an envelope of unburned material our best estimate of the luminosity implies m_v ... | [['spectra', 'and', 'light', 'curves', 'of', 'sn', '2006gz', 'show', 'the', 'strongest', 'signature', 'of', 'unburned', 'carbon', 'and', 'one', 'of', 'the', 'slowest', 'fading', 'light', 'curves', 'ever', 'seen', 'in', 'a', 'type', 'ia', 'event', 'delta', 'm_15', '069', '004', 'the', 'earlytime', 'si', 'ii', 'velocity'... | [-0.09558187812714405, 0.12998374128340112, -0.04461509327790359, 0.11571593626498858, -0.08525298406631208, -0.15924325411026252, 0.0791741458063082, 0.390363423517201, -0.1671205635307493, -0.3001184389903778, 0.052987670552882754, -0.3145193724052572, -0.011024561640380586, 0.23062211015011844, -0.08208822587891142,... |
709.1502 | Ignition of superconducting vortices by acoustic standing waves | Nucleation of vortices in a superconductor below the first critical field can
be assisted by transverse sound in the GHz frequency range. Vortices will enter
and exist the superconductor at the frequency of the sound. We compute the
threshold parameters of the sound and show that this effect is within
experimental re... | cond-mat.supr-con | nucleation of vortices in a superconductor below the first critical field can be assisted by transverse sound in the ghz frequency range vortices will enter and exist the superconductor at the frequency of the sound we compute the threshold parameters of the sound and show that this effect is within experimental reach | [['nucleation', 'of', 'vortices', 'in', 'a', 'superconductor', 'below', 'the', 'first', 'critical', 'field', 'can', 'be', 'assisted', 'by', 'transverse', 'sound', 'in', 'the', 'ghz', 'frequency', 'range', 'vortices', 'will', 'enter', 'and', 'exist', 'the', 'superconductor', 'at', 'the', 'frequency', 'of', 'the', 'sound... | [-0.18113593021945024, 0.2778420904830385, -0.06262356946423936, 0.009480988069509085, -0.07824170247477014, -0.0708249491514065, 0.09902947274251626, 0.34319359193054527, -0.22632368141785264, -0.27115945199217933, 0.07125631147153819, -0.24958822483984897, -0.04742390476167202, 0.22809675009921193, 0.0381790517533842... |
709.1503 | A Scintillator Purification System for the Borexino Solar Neutrino
Detector | Purification of the 278 tons of liquid scintillator and 889 tons of buffer
shielding for the Borexino solar neutrino detector was performed with a system
that combined distillation, water extraction, gas stripping and filtration. The
purification of the scintillator achieved unprecedented low backgrounds for the
larg... | physics.ins-det | purification of the 278 tons of liquid scintillator and 889 tons of buffer shielding for the borexino solar neutrino detector was performed with a system that combined distillation water extraction gas stripping and filtration the purification of the scintillator achieved unprecedented low backgrounds for the large sca... | [['purification', 'of', 'the', '278', 'tons', 'of', 'liquid', 'scintillator', 'and', '889', 'tons', 'of', 'buffer', 'shielding', 'for', 'the', 'borexino', 'solar', 'neutrino', 'detector', 'was', 'performed', 'with', 'a', 'system', 'that', 'combined', 'distillation', 'water', 'extraction', 'gas', 'stripping', 'and', 'fi... | [-0.06913109729755793, 0.20025503338853778, -0.050626367924882, -0.030551760097487682, 0.06559596408930558, -0.15471785093694435, 0.053429648882133494, 0.30069967320090846, -0.17759517697911514, -0.38838781032245606, 0.13763309754798875, -0.34759386133794723, -0.017516502730646415, 0.16549233803648108, -0.1019413979527... |
709.1504 | Maximum Entropy, Time Series and Statistical Inference | A brief discussion is given of the traditional version of the Maximum Entropy
Method, including a review of some of the criticism that has been made in
regard to its use in statistical inference. Motivated by these questions, a
modified version of the method is proposed and applied to a simple problem,
demonstrating ... | physics.data-an | a brief discussion is given of the traditional version of the maximum entropy method including a review of some of the criticism that has been made in regard to its use in statistical inference motivated by these questions a modified version of the method is proposed and applied to a simple problem demonstrating its us... | [['a', 'brief', 'discussion', 'is', 'given', 'of', 'the', 'traditional', 'version', 'of', 'the', 'maximum', 'entropy', 'method', 'including', 'a', 'review', 'of', 'some', 'of', 'the', 'criticism', 'that', 'has', 'been', 'made', 'in', 'regard', 'to', 'its', 'use', 'in', 'statistical', 'inference', 'motivated', 'by', 'th... | [-0.04207101840068374, -0.02193358274209395, -0.12050773250756033, 0.06682842587153509, -0.10164078236802628, -0.10611573201522492, 0.05311829663747758, 0.3420881673759013, -0.24751692500553632, -0.3031211283155962, 0.15217604904982932, -0.24347981454379725, -0.16524924994691423, 0.2292153714714866, -0.1467044776174844... |
709.1505 | The Higgs Decay Width in Multi-Scalar Doublet Models | We show that there are regions of parameter space in multi-scalar doublet
models where, in the first few hundred inverse femtobarns of data, the new
charged and neutral scalars are not directly observable at the LHC and yet the
Higgs decay rate to b bbar is changed significantly from its standard model
value. For a l... | hep-ph | we show that there are regions of parameter space in multiscalar doublet models where in the first few hundred inverse femtobarns of data the new charged and neutral scalars are not directly observable at the lhc and yet the higgs decay rate to b bbar is changed significantly from its standard model value for a light h... | [['we', 'show', 'that', 'there', 'are', 'regions', 'of', 'parameter', 'space', 'in', 'multiscalar', 'doublet', 'models', 'where', 'in', 'the', 'first', 'few', 'hundred', 'inverse', 'femtobarns', 'of', 'data', 'the', 'new', 'charged', 'and', 'neutral', 'scalars', 'are', 'not', 'directly', 'observable', 'at', 'the', 'lhc... | [-0.040484700952851754, 0.24388365874145024, -0.016602723410319604, 0.14691859732791893, -0.06681646325508367, -0.16343112074502347, 0.019922650003008278, 0.326540037437515, -0.2590050243237195, -0.3217453227607076, 0.04988836189996853, -0.2974738435496292, 0.029337757172252604, 0.1829719424964358, 0.05294689106124782,... |
709.1506 | On the asymptotic of likelihood ratios for self-normalized large
deviations | Motivated by multiple statistical hypothesis testing, we obtain the limit of
likelihood ratio of large deviations for self-normalized random variables,
specifically, the ratio of $P(\sqrt{n}(\bar X +d/n) \ge x_n V)$ to
$P(\sqrt{n}\bar X \ge x_n V)$, as $n\toi$, where $\bar X$ and $V$ are the
sample mean and standard ... | math.ST math.PR stat.TH | motivated by multiple statistical hypothesis testing we obtain the limit of likelihood ratio of large deviations for selfnormalized random variables specifically the ratio of psqrtnbar x dn ge x_n v to psqrtnbar x ge x_n v as ntoi where bar x and v are the sample mean and standard deviation of iid x_1 x_n respectively ... | [['motivated', 'by', 'multiple', 'statistical', 'hypothesis', 'testing', 'we', 'obtain', 'the', 'limit', 'of', 'likelihood', 'ratio', 'of', 'large', 'deviations', 'for', 'selfnormalized', 'random', 'variables', 'specifically', 'the', 'ratio', 'of', 'psqrtnbar', 'x', 'dn', 'ge', 'x_n', 'v', 'to', 'psqrtnbar', 'x', 'ge',... | [-0.15098235909486327, 0.10780101633683695, -0.0466980135136443, 0.017951853749364977, 0.020055883215755466, -0.1681368434877415, 0.08457803095849913, 0.34556133871542183, -0.31604435178829826, -0.25674561099187143, 0.07538769415218186, -0.31951354827534983, -0.05717357153137313, 0.15102020514243078, -0.052752671331712... |
709.1507 | Surgery description of colored knots | The pair (K,r) consisting of a knot K and a surjective map r from the knot
group onto a dihedral group is said to be a p-colored knot. D. Moskovich
conjectured that for any odd prime p there are exactly p equivalence classes of
p-colored knots up to surgery along unknots in the kernel of the coloring. We
show that th... | math.GT | the pair kr consisting of a knot k and a surjective map r from the knot group onto a dihedral group is said to be a pcolored knot d moskovich conjectured that for any odd prime p there are exactly p equivalence classes of pcolored knots up to surgery along unknots in the kernel of the coloring we show that there are at... | [['the', 'pair', 'kr', 'consisting', 'of', 'a', 'knot', 'k', 'and', 'a', 'surjective', 'map', 'r', 'from', 'the', 'knot', 'group', 'onto', 'a', 'dihedral', 'group', 'is', 'said', 'to', 'be', 'a', 'pcolored', 'knot', 'd', 'moskovich', 'conjectured', 'that', 'for', 'any', 'odd', 'prime', 'p', 'there', 'are', 'exactly', '... | [-0.23732576567893196, 0.1384265000730231, -0.12512138892546487, 0.06472688821399478, -0.06475643991718104, -0.19261350410628567, 0.034960320686541826, 0.33707390167708895, -0.29447806736670884, -0.3326586429563582, 0.040777487470471795, -0.2542994459913035, -0.13803349512371169, 0.18444103356984676, -0.122114002058033... |
709.1508 | The Bizarre Spectral Variability of Central Stars of Planetary Nebulae | A radial velocity (RV) survey to detect central stars in binary systems was
carried out between 2002 and 2004. De Marco et al. (2004) reported that 10 out
of 11 monitored stars exhibited strong RV variability, but periods were not
detected. Since other mechanisms, such as wind variability, can cause apparent
RV varia... | astro-ph | a radial velocity rv survey to detect central stars in binary systems was carried out between 2002 and 2004 de marco et al 2004 reported that 10 out of 11 monitored stars exhibited strong rv variability but periods were not detected since other mechanisms such as wind variability can cause apparent rv variations we mon... | [['a', 'radial', 'velocity', 'rv', 'survey', 'to', 'detect', 'central', 'stars', 'in', 'binary', 'systems', 'was', 'carried', 'out', 'between', '2002', 'and', '2004', 'de', 'marco', 'et', 'al', '2004', 'reported', 'that', '10', 'out', 'of', '11', 'monitored', 'stars', 'exhibited', 'strong', 'rv', 'variability', 'but', ... | [-0.09687853159959472, 0.11511253975170516, -0.0690353309236229, 0.15072479772581054, -0.16082880824997828, -0.13881366881562066, 0.0748945958598656, 0.4432274814074238, -0.18887674080427672, -0.36939131349196164, 0.1106408756282745, -0.28572807703794634, -0.07915524840435553, 0.22601795056518265, -0.14071195161482117,... |
709.1509 | On well-posedness of the linear Cauchy problem with the distributional
right-hand side and discontinuous coefficients | We prove the well-posedness of the Cauchy problem for the linear differential
system of the form $x^{\prime}-A(t)x=f$, where $f$ is a distribution and $A$
possesses at most first-kind discontinuities together with all its derivatives
defined almost everywhere. The left-hand side of this system contains the
product of... | math.FA math.CA | we prove the wellposedness of the cauchy problem for the linear differential system of the form xprimeatxf where f is a distribution and a possesses at most firstkind discontinuities together with all its derivatives defined almost everywhere the lefthand side of this system contains the product of a distribution and i... | [['we', 'prove', 'the', 'wellposedness', 'of', 'the', 'cauchy', 'problem', 'for', 'the', 'linear', 'differential', 'system', 'of', 'the', 'form', 'xprimeatxf', 'where', 'f', 'is', 'a', 'distribution', 'and', 'a', 'possesses', 'at', 'most', 'firstkind', 'discontinuities', 'together', 'with', 'all', 'its', 'derivatives',... | [-0.1636827082040101, 0.05671916174129617, -0.09529530705652968, 0.011513735963045245, -0.03720645436228518, -0.11614517952879741, -0.032997300080618526, 0.3222958013741639, -0.3242780437342904, -0.20077019698074916, 0.1293820247124629, -0.3144163102654861, -0.13556419482223525, 0.15467440743461577, -0.0451518887565573... |
709.151 | The Most Dark Matter Dominated Galaxies: Predicted Gamma-ray Signals
from the Faintest Milky Way Dwarfs | We use kinematic data from three new, nearby, extremely low-luminosity Milky
Way dwarf galaxies (Ursa Major II, Willman 1, and Coma Berenices) to constrain
the properties of their dark matter halos, and from these make predictions for
the gamma-ray flux from annihilation of dark matter particles in these halos.
We sh... | astro-ph | we use kinematic data from three new nearby extremely lowluminosity milky way dwarf galaxies ursa major ii willman 1 and coma berenices to constrain the properties of their dark matter halos and from these make predictions for the gammaray flux from annihilation of dark matter particles in these halos we show that thes... | [['we', 'use', 'kinematic', 'data', 'from', 'three', 'new', 'nearby', 'extremely', 'lowluminosity', 'milky', 'way', 'dwarf', 'galaxies', 'ursa', 'major', 'ii', 'willman', '1', 'and', 'coma', 'berenices', 'to', 'constrain', 'the', 'properties', 'of', 'their', 'dark', 'matter', 'halos', 'and', 'from', 'these', 'make', 'p... | [-0.06393962887012969, 0.16306690032315718, -0.07954490177715863, 0.16161877134597147, -0.10888642121058006, -0.010022703113711694, -0.005625180697503996, 0.39418446534470497, -0.14835294631578924, -0.46202559944532523, -0.014000113263526666, -0.3240977516155932, 0.019104807693571722, 0.20632297933999716, -0.0044541923... |
709.1511 | Competition between attractive and repulsive interactions in
two-component Bose-Einstein condensates trapped in an optical lattice | We consider effects of inter-species attraction on two-component gap solitons
(GSs) in the binary BEC with intra-species repulsion, trapped in the
one-dimensional optical lattice (OL). Systematic simulations of the coupled
Gross-Pitaevskii equations (GPEs) corroborate an assumption that, because the
effective mass of... | cond-mat.other | we consider effects of interspecies attraction on twocomponent gap solitons gss in the binary bec with intraspecies repulsion trapped in the onedimensional optical lattice ol systematic simulations of the coupled grosspitaevskii equations gpes corroborate an assumption that because the effective mass of gss is negative... | [['we', 'consider', 'effects', 'of', 'interspecies', 'attraction', 'on', 'twocomponent', 'gap', 'solitons', 'gss', 'in', 'the', 'binary', 'bec', 'with', 'intraspecies', 'repulsion', 'trapped', 'in', 'the', 'onedimensional', 'optical', 'lattice', 'ol', 'systematic', 'simulations', 'of', 'the', 'coupled', 'grosspitaevski... | [-0.2417873415045527, 0.2352678272299547, -0.027348269565135166, 0.09055569217754203, 0.008859660843289782, -0.2045842325693906, 0.021018308229158296, 0.3825330515500418, -0.24105007816344665, -0.17759798917118028, 0.0005358913933674177, -0.3149698792826818, -0.07816620288568354, 0.11348323632562317, 0.0906701349566330... |
709.1512 | The effect of the motion of the Sun on the light-time in interplanetary
relativistic experiments | In 2002 a measurement of the effect of solar gravity upon the phase of
coherent microwave beams passing near the Sun has been carried out with the
Cassini mission, allowing a very accurate measurement of the PPN parameter
$\gamma$. The data have been analyzed with NASA's Orbit Determination Program
(ODP) in the Baryc... | gr-qc physics.gen-ph | in 2002 a measurement of the effect of solar gravity upon the phase of coherent microwave beams passing near the sun has been carried out with the cassini mission allowing a very accurate measurement of the ppn parameter gamma the data have been analyzed with nasas orbit determination program odp in the barycentric cel... | [['in', '2002', 'a', 'measurement', 'of', 'the', 'effect', 'of', 'solar', 'gravity', 'upon', 'the', 'phase', 'of', 'coherent', 'microwave', 'beams', 'passing', 'near', 'the', 'sun', 'has', 'been', 'carried', 'out', 'with', 'the', 'cassini', 'mission', 'allowing', 'a', 'very', 'accurate', 'measurement', 'of', 'the', 'pp... | [-0.12190430743362883, 0.11862841027885161, -0.10151784209281624, 0.047670769347038504, -0.04613958241353775, -0.05271898843026881, 0.07369880402733668, 0.324947017816634, -0.22540691951289774, -0.36997271801890996, 0.09961359359580894, -0.2721095444763015, -0.09934291836548725, 0.21204363266367401, -0.0700013382263995... |
709.1513 | CMB Polarization Systematics Due to Beam Asymmetry: Impact on
Inflationary Science | CMB polarization provides a unique window into cosmological inflation; the
amplitude of the B-mode polarization from last scattering is uniquely sensitive
to the energetics of inflation. However, numerous systematic effects arising
from optical imperfections can contaminate the observed B-mode power spectrum.
In part... | astro-ph | cmb polarization provides a unique window into cosmological inflation the amplitude of the bmode polarization from last scattering is uniquely sensitive to the energetics of inflation however numerous systematic effects arising from optical imperfections can contaminate the observed bmode power spectrum in particular s... | [['cmb', 'polarization', 'provides', 'a', 'unique', 'window', 'into', 'cosmological', 'inflation', 'the', 'amplitude', 'of', 'the', 'bmode', 'polarization', 'from', 'last', 'scattering', 'is', 'uniquely', 'sensitive', 'to', 'the', 'energetics', 'of', 'inflation', 'however', 'numerous', 'systematic', 'effects', 'arising... | [-0.12195108082669322, 0.13004642002633773, -0.12782252493780105, 0.09959184428444132, -0.10685265695210547, -0.0642982571182074, -0.03045286295819096, 0.33991004872368646, -0.2852144916076213, -0.29104545270092785, 0.07302635258565715, -0.2822222085669637, -0.13818098154879407, 0.21924271043244517, 0.01553550868120510... |
709.1514 | On differentiability of the Parisi formula | It was proved by Michel Talagrand in [10] that the Parisi formula for the
free energy in the Sherrington-Kirkpatrick model is differentiable with respect
to inverse temperature parameter. We present a simpler proof of this result by
using approximate solutions in the Parisi formula and give one example of
application... | math.PR math-ph math.MP | it was proved by michel talagrand in 10 that the parisi formula for the free energy in the sherringtonkirkpatrick model is differentiable with respect to inverse temperature parameter we present a simpler proof of this result by using approximate solutions in the parisi formula and give one example of application of th... | [['it', 'was', 'proved', 'by', 'michel', 'talagrand', 'in', '10', 'that', 'the', 'parisi', 'formula', 'for', 'the', 'free', 'energy', 'in', 'the', 'sherringtonkirkpatrick', 'model', 'is', 'differentiable', 'with', 'respect', 'to', 'inverse', 'temperature', 'parameter', 'we', 'present', 'a', 'simpler', 'proof', 'of', 't... | [-0.0783998087739967, 0.07812281847211787, -0.11132796258298737, 0.11620845937762748, -0.05548345004067277, -0.10275568119532456, 0.05477171838212984, 0.2919808296825398, -0.21888934038438354, -0.3035953732068072, 0.1136128181806822, -0.24827920329566536, -0.1069059677485546, 0.16976215046562368, -0.055764586513484544,... |
709.1515 | Azumaya-type noncommutative spaces and morphisms therefrom: Polchinski's
D-branes in string theory from Grothendieck's viewpoint | We explain how Polchinski's work on D-branes re-read from a noncommutative
version of Grothendieck's equivalence of local geometries and function rings
gives rise to an intrinsic prototype definition of D-branes (of B-type) as an
Azumaya-type noncommutative space. Several originally open-string induced
properties of ... | math.AG hep-th math.SG | we explain how polchinskis work on dbranes reread from a noncommutative version of grothendiecks equivalence of local geometries and function rings gives rise to an intrinsic prototype definition of dbranes of btype as an azumayatype noncommutative space several originally openstring induced properties of dbranes can b... | [['we', 'explain', 'how', 'polchinskis', 'work', 'on', 'dbranes', 'reread', 'from', 'a', 'noncommutative', 'version', 'of', 'grothendiecks', 'equivalence', 'of', 'local', 'geometries', 'and', 'function', 'rings', 'gives', 'rise', 'to', 'an', 'intrinsic', 'prototype', 'definition', 'of', 'dbranes', 'of', 'btype', 'as', ... | [-0.14171046234192686, 0.09586214779268723, -0.14975072823775312, 0.1298388191110765, -0.09620448784568371, -0.09716357694914898, -0.005712992022148309, 0.31629071857493657, -0.26253537576513525, -0.2611035398947887, 0.05613995352700257, -0.18807308534040856, -0.16632019566037717, 0.17407801574788606, -0.19740080186285... |
709.1516 | On Universal Prediction and Bayesian Confirmation | The Bayesian framework is a well-studied and successful framework for
inductive reasoning, which includes hypothesis testing and confirmation,
parameter estimation, sequence prediction, classification, and regression. But
standard statistical guidelines for choosing the model class and prior are not
always available ... | math.ST cs.IT cs.LG math.IT stat.ML stat.TH | the bayesian framework is a wellstudied and successful framework for inductive reasoning which includes hypothesis testing and confirmation parameter estimation sequence prediction classification and regression but standard statistical guidelines for choosing the model class and prior are not always available or fail i... | [['the', 'bayesian', 'framework', 'is', 'a', 'wellstudied', 'and', 'successful', 'framework', 'for', 'inductive', 'reasoning', 'which', 'includes', 'hypothesis', 'testing', 'and', 'confirmation', 'parameter', 'estimation', 'sequence', 'prediction', 'classification', 'and', 'regression', 'but', 'standard', 'statistical'... | [-0.043709219335343934, 0.016691174043646444, -0.0909831824877377, 0.13861548189581502, -0.1251671845287395, -0.20105265164359784, 0.07051890346823105, 0.41587772263705525, -0.2741270739263402, -0.3343421871864444, 0.10215399753724341, -0.18960784724266785, -0.16563724448496941, 0.17894700097127092, -0.1213119183917620... |
709.1517 | Possible theoretical limits on holographic quintessence from weak
gravity conjecture | The holographic dark energy model is one of the important ways for dealing
with the dark energy problems in the quantum gravity framework. In this model,
the dimensionless parameter $c$ plays an essential role in determining the
evolution of the holographic dark energy. In particular, the holographic dark
energy with... | astro-ph | the holographic dark energy model is one of the important ways for dealing with the dark energy problems in the quantum gravity framework in this model the dimensionless parameter c plays an essential role in determining the evolution of the holographic dark energy in particular the holographic dark energy with cgeq 1 ... | [['the', 'holographic', 'dark', 'energy', 'model', 'is', 'one', 'of', 'the', 'important', 'ways', 'for', 'dealing', 'with', 'the', 'dark', 'energy', 'problems', 'in', 'the', 'quantum', 'gravity', 'framework', 'in', 'this', 'model', 'the', 'dimensionless', 'parameter', 'c', 'plays', 'an', 'essential', 'role', 'in', 'det... | [-0.13231326654177467, 0.1486940989154658, -0.11644792989528643, 0.12938561099111487, -0.10165831863606742, -0.18526603223397098, -0.03632621821379203, 0.2492986120574108, -0.21319578739241996, -0.366652175433797, 0.029952730667358693, -0.23219569302762116, -0.037176550861550584, 0.1732157183695721, -0.0124979543012626... |
709.1518 | Scaling Properties of Fidelity in Spin-one Anisotropic Model | By means of the density matrix renormalization group technique, the scaling
relation of the fidelity susceptibility proposed recently is verified for the
spin-one XXZ spin chain with an on-site anisotropic term. Moreover, from the
results of both the fidelity susceptibility and the entanglement entropy, the
critical ... | quant-ph cond-mat.stat-mech | by means of the density matrix renormalization group technique the scaling relation of the fidelity susceptibility proposed recently is verified for the spinone xxz spin chain with an onsite anisotropic term moreover from the results of both the fidelity susceptibility and the entanglement entropy the critical points a... | [['by', 'means', 'of', 'the', 'density', 'matrix', 'renormalization', 'group', 'technique', 'the', 'scaling', 'relation', 'of', 'the', 'fidelity', 'susceptibility', 'proposed', 'recently', 'is', 'verified', 'for', 'the', 'spinone', 'xxz', 'spin', 'chain', 'with', 'an', 'onsite', 'anisotropic', 'term', 'moreover', 'from... | [-0.15412163653106997, 0.15150795410817308, -0.08064402241466774, 0.015822166878367877, -0.002185644887180792, -0.11876964134474595, 0.0930812161286465, 0.33443642649411537, -0.20283452010092637, -0.2519580230530765, 0.10582851565494719, -0.3302126904535625, -0.14636884329633582, 0.23632209725264047, 0.0564794062636792... |
709.1519 | Transport properties and magnetic field induced localization in the
misfit cobaltite
[Bi$_2$Ba$_{1.3}$K$_{0.6}$Co$_{0.1}$]$^{RS}$[CoO$_2$]$_{1.97}$ single crystal | Resistivity under magnetic field, thermopower and Hall coefficient are
systematically studied for
[Bi$_2$Ba$_{1.3}$K$_{0.6}$Co$_{0.1}$]$^{RS}$[CoO$_2$]$_{1.97}$ single crystal.
In-plane resistivity ($\rho_{ab}$(T)) shows metallic behavior down to 2 K with
a $T^2$ dependence below 30 K; while out-of-plane resistivity ... | cond-mat.str-el cond-mat.mtrl-sci | resistivity under magnetic field thermopower and hall coefficient are systematically studied for bi_2ba_13k_06co_01rscoo_2_197 single crystal inplane resistivity rho_abt shows metallic behavior down to 2 k with a t2 dependence below 30 k while outofplane resistivity rho_ct shows metallic behavior at high temperature an... | [['resistivity', 'under', 'magnetic', 'field', 'thermopower', 'and', 'hall', 'coefficient', 'are', 'systematically', 'studied', 'for', 'bi_2ba_13k_06co_01rscoo_2_197', 'single', 'crystal', 'inplane', 'resistivity', 'rho_abt', 'shows', 'metallic', 'behavior', 'down', 'to', '2', 'k', 'with', 'a', 't2', 'dependence', 'bel... | [-0.20242477880509677, 0.2499409302682528, -0.0568060581308772, -0.03291419407963436, -0.06544963620550368, -0.22232289510814227, 0.06218297218570029, 0.3807866176379458, -0.27105056643837466, -0.3033888654888801, -0.008239948153407927, -0.3737181997242964, -0.1233840786636684, 0.21339153810645858, 0.08235200001629737,... |
709.152 | Fermions in gravity and gauge backgrounds on a brane world | We solve the fermionic zero modes in gravity and gauge backgrounds on a brane
involving a warped geometry, and study the localization of spin 1/2 fermionic
field on the brane world. The result is that there exist massless spin 1/2
fermions which can be localized on the bulk with the exponentially decreasing
warp fact... | hep-th | we solve the fermionic zero modes in gravity and gauge backgrounds on a brane involving a warped geometry and study the localization of spin 12 fermionic field on the brane world the result is that there exist massless spin 12 fermions which can be localized on the bulk with the exponentially decreasing warp factor if ... | [['we', 'solve', 'the', 'fermionic', 'zero', 'modes', 'in', 'gravity', 'and', 'gauge', 'backgrounds', 'on', 'a', 'brane', 'involving', 'a', 'warped', 'geometry', 'and', 'study', 'the', 'localization', 'of', 'spin', '12', 'fermionic', 'field', 'on', 'the', 'brane', 'world', 'the', 'result', 'is', 'that', 'there', 'exist... | [-0.18679170689493832, 0.25632397955956143, -0.004894513960203363, 0.10273482144273455, -0.07082776551962727, -0.19984455274081686, -0.052179036325671606, 0.3296515339623309, -0.11281712727698807, -0.24384472705423832, 0.11700119258118018, -0.29049787594380583, -0.12836712936081718, 0.12883414952860525, -0.017108316766... |
709.1521 | Ricci Flow with hyperbolic warped product metrics | In this short note, we show that the negative curvature is preserved in the
deformation of hyperbolic warped product metrics under Ricci flow. It is also
showed that the flow converges to a flat metric as time going to infinity.
| math.DG math.AP | in this short note we show that the negative curvature is preserved in the deformation of hyperbolic warped product metrics under ricci flow it is also showed that the flow converges to a flat metric as time going to infinity | [['in', 'this', 'short', 'note', 'we', 'show', 'that', 'the', 'negative', 'curvature', 'is', 'preserved', 'in', 'the', 'deformation', 'of', 'hyperbolic', 'warped', 'product', 'metrics', 'under', 'ricci', 'flow', 'it', 'is', 'also', 'showed', 'that', 'the', 'flow', 'converges', 'to', 'a', 'flat', 'metric', 'as', 'time',... | [-0.17900282605551182, 0.13042805892764592, -0.14260133721400053, 0.07330218620190862, -0.0674855801742524, -0.14417642970802264, -0.1014309442602098, 0.41812900961376726, -0.29953300980851055, -0.14479302022082266, 0.1363500404113438, -0.27878970466554165, -0.2032621859572828, 0.1398350407835096, -0.1573815786279738, ... |
709.1522 | The BV Master Equation for the Wilson Action in general Yang-Mills Gauge
Theory | The Wilson effective action for general Yang-Mills gauge theory is shown to
satisfy the usual form of Batalin-Vilkovisky (BV) master equation, despite that
a momentum cutoff apparently breaks the gauge invariance. In the case of
Abelian gauge theory, in particular, it actually deduces the Ward-Takahashi
identity for ... | hep-th | the wilson effective action for general yangmills gauge theory is shown to satisfy the usual form of batalinvilkovisky bv master equation despite that a momentum cutoff apparently breaks the gauge invariance in the case of abelian gauge theory in particular it actually deduces the wardtakahashi identity for wilson acti... | [['the', 'wilson', 'effective', 'action', 'for', 'general', 'yangmills', 'gauge', 'theory', 'is', 'shown', 'to', 'satisfy', 'the', 'usual', 'form', 'of', 'batalinvilkovisky', 'bv', 'master', 'equation', 'despite', 'that', 'a', 'momentum', 'cutoff', 'apparently', 'breaks', 'the', 'gauge', 'invariance', 'in', 'the', 'cas... | [-0.141864408235191, 0.19013878574165013, -0.153334606725436, 0.15356810929370113, -0.13583232319125763, -0.16188549365884122, -0.004198040155013307, 0.3263996228432426, -0.19077054103120014, -0.2460045826334793, 0.016689360898453742, -0.20600344892591238, -0.18639239425269458, 0.06857893739092666, -0.10938450910795766... |
709.1523 | String Theory and Quantum Chromodynamics | I review recent progress on the connection between string theory and quantum
chromodynamics in the context of the gauge/gravity duality. Emphasis is placed
on conciseness and conceptual aspects rather than on technical details. Topics
covered include the large-Nc limit of gauge theories, the gravitational
description... | hep-th | i review recent progress on the connection between string theory and quantum chromodynamics in the context of the gaugegravity duality emphasis is placed on conciseness and conceptual aspects rather than on technical details topics covered include the largenc limit of gauge theories the gravitational description of gau... | [['i', 'review', 'recent', 'progress', 'on', 'the', 'connection', 'between', 'string', 'theory', 'and', 'quantum', 'chromodynamics', 'in', 'the', 'context', 'of', 'the', 'gaugegravity', 'duality', 'emphasis', 'is', 'placed', 'on', 'conciseness', 'and', 'conceptual', 'aspects', 'rather', 'than', 'on', 'technical', 'deta... | [-0.11750380109879188, 0.18176073226745107, -0.10896551888436079, 0.11430371813185047, -0.08840143517591059, -0.12503853666774895, 0.05693269313945036, 0.29836703391213504, -0.1372018952138855, -0.26704525887700065, 0.05586162624656156, -0.30197662667238284, -0.15570630665336335, 0.11036661510089678, -0.044950411663324... |
709.1524 | Sfermion Mass Relations in Orbifold Family Unification | We derive relations among sfermion masses based on orbifold family
unification models. Sfermion mass relations are specific to each model and can
be useful for a selection of realistic model.
| hep-ph | we derive relations among sfermion masses based on orbifold family unification models sfermion mass relations are specific to each model and can be useful for a selection of realistic model | [['we', 'derive', 'relations', 'among', 'sfermion', 'masses', 'based', 'on', 'orbifold', 'family', 'unification', 'models', 'sfermion', 'mass', 'relations', 'are', 'specific', 'to', 'each', 'model', 'and', 'can', 'be', 'useful', 'for', 'a', 'selection', 'of', 'realistic', 'model']] | [-0.10002552109460036, 0.1458084440169235, -0.02731913160532713, 0.24727240776022275, -0.15459661688655615, -0.24104274615334967, 0.06125367737064759, 0.39753991067409516, -0.17291701646366467, -0.37727940604090693, 0.08123233166212837, -0.21019834851225216, -0.07995823261638482, 0.2222258424308772, -0.0034502998304863... |
709.1525 | Tensor representations of classical locally finite Lie algebras | We study the structure of tensor representations of the classical
infinite-dimensional locally finite Lie algebras $gl_\infty$, $sl_\infty$,
$sp_\infty$ and $so_\infty$. In contrast with the finite-dimensional case,
these tensor representations are not semisimple. We explicitly describe their
Jordan-Holder constituen... | math.RT | we study the structure of tensor representations of the classical infinitedimensional locally finite lie algebras gl_infty sl_infty sp_infty and so_infty in contrast with the finitedimensional case these tensor representations are not semisimple we explicitly describe their jordanholder constituents socle filtrations a... | [['we', 'study', 'the', 'structure', 'of', 'tensor', 'representations', 'of', 'the', 'classical', 'infinitedimensional', 'locally', 'finite', 'lie', 'algebras', 'gl_infty', 'sl_infty', 'sp_infty', 'and', 'so_infty', 'in', 'contrast', 'with', 'the', 'finitedimensional', 'case', 'these', 'tensor', 'representations', 'are... | [-0.15898405857892198, 0.1223247079390355, -0.06632898714583875, 0.05363199406896125, -0.2015057297169485, -0.09991468461653726, -0.12260707323862748, 0.4313597399741411, -0.3944499913222072, -0.08983656560832803, 0.1104880567978729, -0.20542561643841592, -0.1684355230708289, 0.0708142501429062, -0.12383924280716614, -... |
709.1526 | Jarlskog Invariant of the Neutrino Mapping Matrix | The Jarlskog Invariant $J_{\nu-map}$ of the neutrino mapping matrix is
calculated based on a phenomenological model which relates the smallness of
light lepton masses $m_e$ and $m_1$ (of $\nu_1$) with the smallness of $T$
violation. For small $T$ violating phase $\chi_l$ in the lepton sector,
$J_{\nu-map}$ is proport... | hep-ph | the jarlskog invariant j_numap of the neutrino mapping matrix is calculated based on a phenomenological model which relates the smallness of light lepton masses m_e and m_1 of nu_1 with the smallness of t violation for small t violating phase chi_l in the lepton sector j_numap is proportional to chi_l but m_e and m_1 a... | [['the', 'jarlskog', 'invariant', 'j_numap', 'of', 'the', 'neutrino', 'mapping', 'matrix', 'is', 'calculated', 'based', 'on', 'a', 'phenomenological', 'model', 'which', 'relates', 'the', 'smallness', 'of', 'light', 'lepton', 'masses', 'm_e', 'and', 'm_1', 'of', 'nu_1', 'with', 'the', 'smallness', 'of', 't', 'violation'... | [-0.15855005055911736, 0.3117669911201422, 0.027268074826376203, 0.119400093184797, -0.05848539373578711, -0.18395405528523648, 0.0723528001803465, 0.25150032507048714, -0.18068430164001054, -0.32755595181758207, 0.03044761129907177, -0.31272286026635104, -0.012495084717455838, 0.12583969565457664, -0.01599547198404454... |
709.1527 | Origin of Chromatic Features in Multiple Quasars -Variability, Dust, or
Microlensing - | Aims:In some of the lensed quasars, color differences between multiple images
are observed at optical/near-infrared wavelengths. There are three possible
origins of the color differences: intrinsic variabilities of quasars,
differential dust extinction, and quasar microlensing. We examine how these
three possible sce... | astro-ph | aimsin some of the lensed quasars color differences between multiple images are observed at opticalnearinfrared wavelengths there are three possible origins of the color differences intrinsic variabilities of quasars differential dust extinction and quasar microlensing we examine how these three possible scenarios can ... | [['aimsin', 'some', 'of', 'the', 'lensed', 'quasars', 'color', 'differences', 'between', 'multiple', 'images', 'are', 'observed', 'at', 'opticalnearinfrared', 'wavelengths', 'there', 'are', 'three', 'possible', 'origins', 'of', 'the', 'color', 'differences', 'intrinsic', 'variabilities', 'of', 'quasars', 'differential'... | [-0.04509891235347952, 0.09042843623078259, -0.08329910839470854, 0.2037036612020779, -0.07745004722918053, -0.1250074725240575, -0.017047327339000364, 0.5096830764070365, -0.1679970453128051, -0.35673747819923396, 0.02625627561540771, -0.3111324503629411, -0.08150481753201214, 0.18110667701073485, -0.07042447754768964... |
709.1528 | Multiwavelength Observations of the Powerful Gamma-ray Quasar PKS
1510-089: Clues on the Jet Composition | We present the results from a multiwavelength campaign of the powerful
Gamma-ray quasar PKS 1510-089. This campaign commenced with a deep Suzaku
observation lasting three days for a total exposure time of 120 ks, and
continued with Swift monitoring over 18 days. Besides Swift observations, the
campaign included groun... | astro-ph | we present the results from a multiwavelength campaign of the powerful gammaray quasar pks 1510089 this campaign commenced with a deep suzaku observation lasting three days for a total exposure time of 120 ks and continued with swift monitoring over 18 days besides swift observations the campaign included groundbased o... | [['we', 'present', 'the', 'results', 'from', 'a', 'multiwavelength', 'campaign', 'of', 'the', 'powerful', 'gammaray', 'quasar', 'pks', '1510089', 'this', 'campaign', 'commenced', 'with', 'a', 'deep', 'suzaku', 'observation', 'lasting', 'three', 'days', 'for', 'a', 'total', 'exposure', 'time', 'of', '120', 'ks', 'and', ... | [-0.05445567671949051, 0.1532737084399854, -0.06609947952243049, 0.09038494073014972, -0.07834900188615566, -0.1180286564191015, 0.05086085848311444, 0.4433345646677671, -0.20026294206712075, -0.39587129454027287, 0.08167143979293821, -0.32045814070732015, -0.0122250212105305, 0.20363470348477197, -0.008498403250751232... |
709.1529 | The Existence of Pure Free Resolutions | Let d1,...,dn be a strictly increasing sequence of integers. Boij and
S\"oderberg [arXiv:math/0611081] have conjectured the existence of a graded
module M of finite length over any polynomial ring K[x_1,..., x_n], whose
minimal free resolution is pure of type (d1,...,dn), in the sense that its i-th
syzygies are gener... | math.AC math.RT | let d1dn be a strictly increasing sequence of integers boij and soderberg arxivmath0611081 have conjectured the existence of a graded module m of finite length over any polynomial ring kx_1 x_n whose minimal free resolution is pure of type d1dn in the sense that its ith syzygies are generated in degree di in this paper... | [['let', 'd1dn', 'be', 'a', 'strictly', 'increasing', 'sequence', 'of', 'integers', 'boij', 'and', 'soderberg', 'arxivmath0611081', 'have', 'conjectured', 'the', 'existence', 'of', 'a', 'graded', 'module', 'm', 'of', 'finite', 'length', 'over', 'any', 'polynomial', 'ring', 'kx_1', 'x_n', 'whose', 'minimal', 'free', 're... | [-0.18766222131569266, 0.0863010297838819, -0.0808959156479033, 0.04802466796613053, -0.0746370142391115, -0.1725499065625563, -0.08182539458063905, 0.3557075437754719, -0.37393119653458134, -0.19153017509450906, 0.1104916976468654, -0.2086991847108788, -0.1301375796626273, 0.18845934712270832, -0.17546610706159027, -0... |
709.153 | Application of spectral methods for high-frequency financial data to
quantifying states of market participants | Empirical analysis of the foreign exchange market is conducted based on
methods to quantify similarities among multi-dimensional time series with
spectral distances introduced in [A.-H. Sato, Physica A, 382 (2007) 258--270].
As a result it is found that the similarities among currency pairs fluctuate
with the rotatio... | q-fin.ST physics.data-an physics.soc-ph | empirical analysis of the foreign exchange market is conducted based on methods to quantify similarities among multidimensional time series with spectral distances introduced in ah sato physica a 382 2007 258270 as a result it is found that the similarities among currency pairs fluctuate with the rotation of the earth ... | [['empirical', 'analysis', 'of', 'the', 'foreign', 'exchange', 'market', 'is', 'conducted', 'based', 'on', 'methods', 'to', 'quantify', 'similarities', 'among', 'multidimensional', 'time', 'series', 'with', 'spectral', 'distances', 'introduced', 'in', 'ah', 'sato', 'physica', 'a', '382', '2007', '258270', 'as', 'a', 'r... | [-0.08390610076469154, 0.06681873079460975, -0.12334329638486871, 0.12341595546055872, -0.05977529298621588, -0.12143211881451021, 0.0695827272362434, 0.43997661614647277, -0.26751191555164183, -0.2915548318423904, 0.06262213785935623, -0.3567787431538678, -0.16522963341647903, 0.21386798701893825, -0.079052077104839, ... |
709.1531 | Scaling analysis of FLIC fermion actions | The Fat Link Irrelevant Clover (FLIC) fermion action is a variant of the
$O(a)$-improved Wilson action where the irrelevant operators are constructed
using smeared links. While the use of such smearing allows for the use of
highly improved definitions of the field strength tensor $F_{\mu\nu},$ we show
that the standa... | hep-lat | the fat link irrelevant clover flic fermion action is a variant of the oaimproved wilson action where the irrelevant operators are constructed using smeared links while the use of such smearing allows for the use of highly improved definitions of the field strength tensor f_munu we show that the standard 1loop clover t... | [['the', 'fat', 'link', 'irrelevant', 'clover', 'flic', 'fermion', 'action', 'is', 'a', 'variant', 'of', 'the', 'oaimproved', 'wilson', 'action', 'where', 'the', 'irrelevant', 'operators', 'are', 'constructed', 'using', 'smeared', 'links', 'while', 'the', 'use', 'of', 'such', 'smearing', 'allows', 'for', 'the', 'use', ... | [-0.1465883462679112, 0.2189866403631609, -0.07310139495429807, 0.0776740792220801, -0.0783190453376878, -0.14969929975013238, 0.039262870160712934, 0.37834785878658295, -0.17547726708239522, -0.2610213325155535, 0.07266836830591462, -0.2791995639116945, -0.13950845070354556, 0.11306344517024941, -0.038400093987370015,... |
709.1532 | Asymptotic Spectroscopy of Rotating Black Holes | We calculate analytically the transmission and reflection amplitudes for
waves incident on a rotating black hole in d=4, analytically continued to
asymptotically large, nearly imaginary frequency. These amplitudes determine
the asymptotic resonant frequencies of the black hole, including quasinormal
modes, total-tran... | hep-th astro-ph gr-qc | we calculate analytically the transmission and reflection amplitudes for waves incident on a rotating black hole in d4 analytically continued to asymptotically large nearly imaginary frequency these amplitudes determine the asymptotic resonant frequencies of the black hole including quasinormal modes totaltransmission ... | [['we', 'calculate', 'analytically', 'the', 'transmission', 'and', 'reflection', 'amplitudes', 'for', 'waves', 'incident', 'on', 'a', 'rotating', 'black', 'hole', 'in', 'd4', 'analytically', 'continued', 'to', 'asymptotically', 'large', 'nearly', 'imaginary', 'frequency', 'these', 'amplitudes', 'determine', 'the', 'asy... | [-0.22277640390629863, 0.16110095454211, -0.0902422229193297, 0.08033930037659136, -0.08320490201916911, -0.14769915342970075, 0.08697774737169418, 0.30263037049193303, -0.16505272232233456, -0.2134164315739683, 0.03754107081491098, -0.3392320044188048, -0.12152097692402701, 0.19279118331477924, 0.04583074348777825, 0.... |
709.1533 | Bright continuous-variable entanglement from the quantum optical dimer | We show theoretically that two evanescently coupled $\chi^{(2)}$ second
harmonic generators inside a Fabry-Perot cavity provide a tunable source of
quadrature squeezed light, Einstein-Podolsky-Rosen correlations and quantum
entanglement. Unlike systems using coupled downconverters, second harmonic
generation has no o... | quant-ph | we show theoretically that two evanescently coupled chi2 second harmonic generators inside a fabryperot cavity provide a tunable source of quadrature squeezed light einsteinpodolskyrosen correlations and quantum entanglement unlike systems using coupled downconverters second harmonic generation has no oscillation thres... | [['we', 'show', 'theoretically', 'that', 'two', 'evanescently', 'coupled', 'chi2', 'second', 'harmonic', 'generators', 'inside', 'a', 'fabryperot', 'cavity', 'provide', 'a', 'tunable', 'source', 'of', 'quadrature', 'squeezed', 'light', 'einsteinpodolskyrosen', 'correlations', 'and', 'quantum', 'entanglement', 'unlike',... | [-0.1789207995271958, 0.29234900095743005, -0.07023381372488549, 0.02729186130581302, -0.004146909665154374, -0.23057301803087088, 0.00015075128201557243, 0.42451359736530675, -0.23963100198939766, -0.2471372834811716, 0.03041944012005368, -0.2780856665517406, -0.09116994069747465, 0.24945916105871616, 0.03780555674482... |
709.1534 | Rigidity and percolation of center vortices | Effective action of center vortices in SU(2) lattice gauge theory is
investigated by studying the correlation between the action density on their
worldsheets and their geometric properties. It turns out that center vortices
are rigid, however, their dynamics is more complicated than that of rigid
random surfaces, sin... | hep-lat | effective action of center vortices in su2 lattice gauge theory is investigated by studying the correlation between the action density on their worldsheets and their geometric properties it turns out that center vortices are rigid however their dynamics is more complicated than that of rigid random surfaces since some ... | [['effective', 'action', 'of', 'center', 'vortices', 'in', 'su2', 'lattice', 'gauge', 'theory', 'is', 'investigated', 'by', 'studying', 'the', 'correlation', 'between', 'the', 'action', 'density', 'on', 'their', 'worldsheets', 'and', 'their', 'geometric', 'properties', 'it', 'turns', 'out', 'that', 'center', 'vortices'... | [-0.18225814024772263, 0.2157185399904847, -0.13179998269770293, 0.09116246487974422, -0.061026140209287406, -0.1275228394777514, 0.020293079513066914, 0.40071047807578, -0.2303756543667987, -0.24488601725315676, 0.07867506462789606, -0.252769524618634, -0.17616356031503527, 0.15134497431572527, -0.013632028202118817, ... |
Subsets and Splits
No community queries yet
The top public SQL queries from the community will appear here once available.