id float64 706 1.8k | title stringlengths 1 343 | abstract stringlengths 6 6.09k | categories stringlengths 5 125 | processed_abstract stringlengths 2 5.96k | tokenized_abstract stringlengths 8 8.74k | centroid stringlengths 2.1k 2.17k |
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707.463 | Ground state properties of a homogeneous 2D system of Bosons with
dipolar interactions | The ground-state phase properties of a two-dimensional Bose system with
dipole-dipole interactions is studied by means of quantum Monte Carlo
techniques. Limitations of mean-field theory in a two-dimensional geometry are
discussed. A quantum phase transition from gas to solid is found. Crystal is
tested for existence... | cond-mat.other | the groundstate phase properties of a twodimensional bose system with dipoledipole interactions is studied by means of quantum monte carlo techniques limitations of meanfield theory in a twodimensional geometry are discussed a quantum phase transition from gas to solid is found crystal is tested for existence of a supe... | [['the', 'groundstate', 'phase', 'properties', 'of', 'a', 'twodimensional', 'bose', 'system', 'with', 'dipoledipole', 'interactions', 'is', 'studied', 'by', 'means', 'of', 'quantum', 'monte', 'carlo', 'techniques', 'limitations', 'of', 'meanfield', 'theory', 'in', 'a', 'twodimensional', 'geometry', 'are', 'discussed', ... | [-0.18233139152444175, 0.2507372015908836, -0.0866899050188875, 0.031152460457846285, 0.03600702553670457, -0.09885895360221571, 0.03931348706333046, 0.3334006993694508, -0.22229661133655526, -0.22272190972766343, 0.01884495030761637, -0.33474117604535114, -0.14077243424872768, 0.11324243404050456, 0.07035877533811838,... |
707.4631 | Measurements of the form-factors slopes of KL -> pi mu nu decay with the
KLOE Detector | We present a measurement of the K-$\pi$ form-factor parameters for the decay
\klpmn. We use 328 pb^{-1} of data collected in 2001 and 2002, corresponding
to
$\sim $ 1.8 million \semil events.
Measurements of semileptonic form factors provide information about the
dynamics of the strong interaction and are neces... | hep-ex | we present a measurement of the kpi formfactor parameters for the decay klpmn we use 328 pb1 of data collected in 2001 and 2002 corresponding to sim 18 million semil events measurements of semileptonic form factors provide information about the dynamics of the strong interaction and are necessary for evaluation of the ... | [['we', 'present', 'a', 'measurement', 'of', 'the', 'kpi', 'formfactor', 'parameters', 'for', 'the', 'decay', 'klpmn', 'we', 'use', '328', 'pb1', 'of', 'data', 'collected', 'in', '2001', 'and', '2002', 'corresponding', 'to', 'sim', '18', 'million', 'semil', 'events', 'measurements', 'of', 'semileptonic', 'form', 'facto... | [-0.08471539581859182, 0.14968306641193888, -0.061627921681158625, 0.07340590642172143, -0.08260214700299896, -0.0825504392075042, 0.07978050701487331, 0.2968894311537345, -0.20537312149117964, -0.29391253468954665, 0.02852243337776257, -0.3620185044665749, -0.04562422547600845, 0.16943921549763116, 0.06294459437664884... |
707.4632 | Inverse Scattering Theory for One-Dimensional Schroedinger Operators
with Steplike Periodic Potentials | We develop direct and inverse scattering theory for one-dimensional
Schroedinger operators with steplike potentials which are asymptotically close
to different finite-gap periodic potentials on different half-axes. We give a
complete characterization of the scattering data, which allow unique
solvability of the inver... | math.SP math-ph math.MP | we develop direct and inverse scattering theory for onedimensional schroedinger operators with steplike potentials which are asymptotically close to different finitegap periodic potentials on different halfaxes we give a complete characterization of the scattering data which allow unique solvability of the inverse scat... | [['we', 'develop', 'direct', 'and', 'inverse', 'scattering', 'theory', 'for', 'onedimensional', 'schroedinger', 'operators', 'with', 'steplike', 'potentials', 'which', 'are', 'asymptotically', 'close', 'to', 'different', 'finitegap', 'periodic', 'potentials', 'on', 'different', 'halfaxes', 'we', 'give', 'a', 'complete'... | [-0.11976988001216976, 0.1111102139506981, -0.059037369201486965, 0.07817569301235226, -0.11210316405983044, -0.1536426879026277, -0.037891488424546246, 0.3612860129302684, -0.29675711747610345, -0.21872641884212224, 0.10338596741444836, -0.3166370280086994, -0.1451855695121131, 0.16146836214575847, 0.03407866474381595... |
707.4633 | Generating trees for permutations avoiding generalized patterns | We construct generating trees with one, two, and three labels for some
classes of permutations avoiding generalized patterns of length 3 and 4. These
trees are built by adding at each level an entry to the right end of the
permutation, which allows us to incorporate the adjacency condition about some
entries in an oc... | math.CO | we construct generating trees with one two and three labels for some classes of permutations avoiding generalized patterns of length 3 and 4 these trees are built by adding at each level an entry to the right end of the permutation which allows us to incorporate the adjacency condition about some entries in an occurren... | [['we', 'construct', 'generating', 'trees', 'with', 'one', 'two', 'and', 'three', 'labels', 'for', 'some', 'classes', 'of', 'permutations', 'avoiding', 'generalized', 'patterns', 'of', 'length', '3', 'and', '4', 'these', 'trees', 'are', 'built', 'by', 'adding', 'at', 'each', 'level', 'an', 'entry', 'to', 'the', 'right'... | [-0.0932261118421627, 0.10966018169806077, -0.03983678757082497, 0.0985865956890423, -0.1068765886267212, -0.12132222923041086, 0.05925267115539967, 0.36586018495052774, -0.32203020644156594, -0.3350469510045956, 0.10787591873232937, -0.30571013468192026, -0.15935399395492034, 0.1918919357823678, -0.06676671304087216, ... |
707.4634 | A Study of the Radiative KL->pi nu e (g) Decay and Possible Osservation
of Direct Photon Emission with the KLOE Detector | We present the measurement of the ratio R =
\frac{\Gamma(\keg;\Estar>30\mev,\qstar>20^\circ)}{\Gamma(\kegf)} and a first
measurement of the direct emission contribution for the same process. We use
328 pb^{-1} of data collected at \kloe in 2001 and 2002, corresponding to about
3 million of \kegf events and about 9 th... | hep-ex | we present the measurement of the ratio r fracgammakegestar30mevqstar20circgammakegf and a first measurement of the direct emission contribution for the same process we use 328 pb1 of data collected at kloe in 2001 and 2002 corresponding to about 3 million of kegf events and about 9 thousand keg radiative events our re... | [['we', 'present', 'the', 'measurement', 'of', 'the', 'ratio', 'r', 'fracgammakegestar30mevqstar20circgammakegf', 'and', 'a', 'first', 'measurement', 'of', 'the', 'direct', 'emission', 'contribution', 'for', 'the', 'same', 'process', 'we', 'use', '328', 'pb1', 'of', 'data', 'collected', 'at', 'kloe', 'in', '2001', 'and... | [-0.08245989730708328, 0.07223636578076847, -0.028170316373956773, 0.01975041543239379, -0.02043843438492759, -0.04919548308723332, 0.10147977857987452, 0.3270390449256143, -0.18079085284090765, -0.41956703884352464, 0.08775282681830611, -0.38875859254039824, 0.04288051309584476, 0.18598679155933068, 0.0328500203048700... |
707.4635 | Ionized and neutral gas in the peculiar star/cluster complex in NGC 6946 | The characteristics of ionized and HI gas in the peculiar star/cluster
complex in NGC 6946, obtained with the 6-m telescope (BTA) SAO RAS, the Gemini
North telescope, and the Westerbork Synthesis Radio Telescope (WSRT), are
presented. The complex is unusual as hosting a super star cluster, the most
massive known in a... | astro-ph | the characteristics of ionized and hi gas in the peculiar starcluster complex in ngc 6946 obtained with the 6m telescope bta sao ras the gemini north telescope and the westerbork synthesis radio telescope wsrt are presented the complex is unusual as hosting a super star cluster the most massive known in an apparently n... | [['the', 'characteristics', 'of', 'ionized', 'and', 'hi', 'gas', 'in', 'the', 'peculiar', 'starcluster', 'complex', 'in', 'ngc', '6946', 'obtained', 'with', 'the', '6m', 'telescope', 'bta', 'sao', 'ras', 'the', 'gemini', 'north', 'telescope', 'and', 'the', 'westerbork', 'synthesis', 'radio', 'telescope', 'wsrt', 'are',... | [-0.1037832592250835, 0.07660445229109077, -0.060164287666868106, 0.06613395306334155, -0.10281889838355768, -0.05957199949251703, 0.009018354557558478, 0.41302720793574843, -0.18061358794853818, -0.29668933646271073, 0.08363132810533655, -0.29920460536066756, -0.056084628881092564, 0.16337976921201347, 0.0022159031150... |
707.4636 | Coherent spin rotations in open driven double quantum dots | We analyze the charge and spin dynamics in a DC biased double quantum dot
driven by crossed DC and AC magnetic fields. In this configuration, spatial
delocalization due to inter-dot tunnel competes with intra-dot spin rotations
induced by the time dependent magnetic field, giving rise to a complicated time
dependent ... | cond-mat.mes-hall | we analyze the charge and spin dynamics in a dc biased double quantum dot driven by crossed dc and ac magnetic fields in this configuration spatial delocalization due to interdot tunnel competes with intradot spin rotations induced by the time dependent magnetic field giving rise to a complicated time dependent behavio... | [['we', 'analyze', 'the', 'charge', 'and', 'spin', 'dynamics', 'in', 'a', 'dc', 'biased', 'double', 'quantum', 'dot', 'driven', 'by', 'crossed', 'dc', 'and', 'ac', 'magnetic', 'fields', 'in', 'this', 'configuration', 'spatial', 'delocalization', 'due', 'to', 'interdot', 'tunnel', 'competes', 'with', 'intradot', 'spin',... | [-0.20770500332457564, 0.27706783346491315, -0.010213299451636211, 0.049795330124055986, -0.0292160256004702, -0.1611211561843232, 0.028724804276510352, 0.4095562274257342, -0.3077576980996196, -0.27131927441505177, 0.01672987329963875, -0.23793928682683937, -0.050157136262534686, 0.21344544084477288, 0.029644162175671... |
707.4637 | Special Fuzzy Matrices for Social Scientists | This book introduces special classes of Fuzzy and Neutrosophic matrices.
These special classes of matrices are used in the construction of multi-expert
special fuzzy models using FCM, FRM and FRE and their Neutorosophic analogues
(simultaneous or otherwise, according to ones need). Using the six basic
models, we have... | math.GM | this book introduces special classes of fuzzy and neutrosophic matrices these special classes of matrices are used in the construction of multiexpert special fuzzy models using fcm frm and fre and their neutorosophic analogues simultaneous or otherwise according to ones need using the six basic models we have construct... | [['this', 'book', 'introduces', 'special', 'classes', 'of', 'fuzzy', 'and', 'neutrosophic', 'matrices', 'these', 'special', 'classes', 'of', 'matrices', 'are', 'used', 'in', 'the', 'construction', 'of', 'multiexpert', 'special', 'fuzzy', 'models', 'using', 'fcm', 'frm', 'and', 'fre', 'and', 'their', 'neutorosophic', 'a... | [-0.05741753788734378, 0.0683254913096071, -0.05695145828404317, 0.11069145724238631, -0.14234345978158608, -0.22326970970862658, 0.05199360330854624, 0.3831827932846002, -0.2700538347360858, -0.29520381538589535, 0.15013640596053415, -0.26820939885076595, -0.18124705094337595, 0.14616783985075654, -0.13190679836062422... |
707.4638 | Indication of multiscaling in the volatility return intervals of stock
markets | The distribution of the return intervals $\tau$ between volatilities above a
threshold $q$ for financial records has been approximated by a scaling
behavior. To explore how accurate is the scaling and therefore understand the
underlined non-linear mechanism, we investigate intraday datasets of 500 stocks
which consis... | q-fin.ST physics.soc-ph | the distribution of the return intervals tau between volatilities above a threshold q for financial records has been approximated by a scaling behavior to explore how accurate is the scaling and therefore understand the underlined nonlinear mechanism we investigate intraday datasets of 500 stocks which consist of the s... | [['the', 'distribution', 'of', 'the', 'return', 'intervals', 'tau', 'between', 'volatilities', 'above', 'a', 'threshold', 'q', 'for', 'financial', 'records', 'has', 'been', 'approximated', 'by', 'a', 'scaling', 'behavior', 'to', 'explore', 'how', 'accurate', 'is', 'the', 'scaling', 'and', 'therefore', 'understand', 'th... | [-0.07948848057644625, 0.11997415484005869, -0.1271124245146665, 0.15279970675852503, -0.029672707487788788, -0.09826536397468835, 0.06814642353802575, 0.3775658942452429, -0.2824467396878143, -0.31114593108372435, 0.09143068745335634, -0.3366717904951776, -0.09707868569089798, 0.19144073105992082, -0.01414127433250961... |
707.4639 | About Bianchi I with VSL | In this paper we study how to attack, through different techniques, a perfect
fluid Bianchi I model with variable G,c and Lambda, but taking into account the
effects of a $c$-variable into the curvature tensor. We study the model under
the assumption,div(T)=0. These tactics are: Lie groups method (LM), imposing a
par... | gr-qc | in this paper we study how to attack through different techniques a perfect fluid bianchi i model with variable gc and lambda but taking into account the effects of a cvariable into the curvature tensor we study the model under the assumptiondivt0 these tactics are lie groups method lm imposing a particular symmetry se... | [['in', 'this', 'paper', 'we', 'study', 'how', 'to', 'attack', 'through', 'different', 'techniques', 'a', 'perfect', 'fluid', 'bianchi', 'i', 'model', 'with', 'variable', 'gc', 'and', 'lambda', 'but', 'taking', 'into', 'account', 'the', 'effects', 'of', 'a', 'cvariable', 'into', 'the', 'curvature', 'tensor', 'we', 'stu... | [-0.14209675799804192, 0.11971974762855098, -0.13476753966194757, 0.07351314519148028, -0.11987998083741196, -0.14622983008487594, 0.03367247005643101, 0.35211105819868876, -0.2577849928699712, -0.2770605714963019, 0.11006781744984423, -0.24728029957840414, -0.12091468145407097, 0.15794695624099947, -0.0191145340643593... |
707.464 | Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties | We use a modified version of the halo-based group finder developed by Yang et
al. to select galaxy groups from the Sloan Digital Sky Survey (SDSS DR4). In
the first step, a combination of two methods is used to identify the centers of
potential groups and to estimate their characteristic luminosity. Using an
iterativ... | astro-ph | we use a modified version of the halobased group finder developed by yang et al to select galaxy groups from the sloan digital sky survey sdss dr4 in the first step a combination of two methods is used to identify the centers of potential groups and to estimate their characteristic luminosity using an iterative approac... | [['we', 'use', 'a', 'modified', 'version', 'of', 'the', 'halobased', 'group', 'finder', 'developed', 'by', 'yang', 'et', 'al', 'to', 'select', 'galaxy', 'groups', 'from', 'the', 'sloan', 'digital', 'sky', 'survey', 'sdss', 'dr4', 'in', 'the', 'first', 'step', 'a', 'combination', 'of', 'two', 'methods', 'is', 'used', 't... | [-0.05792774338647911, 0.005265283128474332, -0.12521099925581966, 0.06647661582692602, -0.14326382066769106, -0.02216645337889091, 0.07986679155944712, 0.4148530776897866, -0.1823970154491103, -0.38081574132816204, 0.07318029699625538, -0.26867526662141655, -0.04708464585400502, 0.21075721526323188, -0.058732590338613... |
707.4641 | Using rotation rates to probe age spreads in the Orion Nebula Cluster | The radii of young pre-main-sequence (PMS) stars in the Orion Nebula Cluster
(ONC) have been estimated using their rotation periods and projected equatorial
velocities. Stars at a given effective temperature have a spread in their
geometrically estimated projected radii that is larger than can be accounted
for with a... | astro-ph | the radii of young premainsequence pms stars in the orion nebula cluster onc have been estimated using their rotation periods and projected equatorial velocities stars at a given effective temperature have a spread in their geometrically estimated projected radii that is larger than can be accounted for with a coeval m... | [['the', 'radii', 'of', 'young', 'premainsequence', 'pms', 'stars', 'in', 'the', 'orion', 'nebula', 'cluster', 'onc', 'have', 'been', 'estimated', 'using', 'their', 'rotation', 'periods', 'and', 'projected', 'equatorial', 'velocities', 'stars', 'at', 'a', 'given', 'effective', 'temperature', 'have', 'a', 'spread', 'in'... | [-0.06339830218620651, 0.17789091963199116, -0.11552088057500458, 0.12084021608053629, -0.11150610929672719, -0.050885188188752005, 0.05607710906008485, 0.4658457859393174, -0.18093220362870596, -0.3741744681670566, 0.08782940724305373, -0.21940838131810447, 0.01905278512603107, 0.21323364929439692, -0.0861043706209895... |
707.4642 | Subnanosecond Ellipticity Detector for Laser Radiation (second version,
extended) | Two types of room temperature detectors of terahertz laser radiation have
been developed which allow in an all-electric manner to determine the plane of
polarization of linearly polarized radiation and the Stokes parameters of
elliptically polarized radiation, respectively. The operation of the detectors
is based on ... | cond-mat.mtrl-sci | two types of room temperature detectors of terahertz laser radiation have been developed which allow in an allelectric manner to determine the plane of polarization of linearly polarized radiation and the stokes parameters of elliptically polarized radiation respectively the operation of the detectors is based on photo... | [['two', 'types', 'of', 'room', 'temperature', 'detectors', 'of', 'terahertz', 'laser', 'radiation', 'have', 'been', 'developed', 'which', 'allow', 'in', 'an', 'allelectric', 'manner', 'to', 'determine', 'the', 'plane', 'of', 'polarization', 'of', 'linearly', 'polarized', 'radiation', 'and', 'the', 'stokes', 'parameter... | [-0.16281805749933578, 0.24916528599925714, -0.06688473119375933, -0.03779125154036783, -0.04635057662993571, -0.12691120748824783, -0.0187682661283026, 0.4688843386247754, -0.23378530823576607, -0.3190240980138218, 0.05467167609113906, -0.2831336708102179, -0.042709746349014734, 0.25475989579909336, 0.0446545465138593... |
707.4643 | Active Set and EM Algorithms for Log-Concave Densities Based on Complete
and Censored Data | We develop an active set algorithm for the maximum likelihood estimation of a
log-concave density based on complete data. Building on this fast algorithm, we
indidate an EM algorithm to treat arbitrarily censored or binned data.
| stat.ME stat.CO | we develop an active set algorithm for the maximum likelihood estimation of a logconcave density based on complete data building on this fast algorithm we indidate an em algorithm to treat arbitrarily censored or binned data | [['we', 'develop', 'an', 'active', 'set', 'algorithm', 'for', 'the', 'maximum', 'likelihood', 'estimation', 'of', 'a', 'logconcave', 'density', 'based', 'on', 'complete', 'data', 'building', 'on', 'this', 'fast', 'algorithm', 'we', 'indidate', 'an', 'em', 'algorithm', 'to', 'treat', 'arbitrarily', 'censored', 'or', 'bi... | [-0.06308780540046947, -0.005780260762964774, -0.1153321392734402, 0.1159145411436579, -0.10427290863756622, -0.15509442440899354, 0.11803288800375802, 0.44473178471837727, -0.21889901584280388, -0.32233899033495356, 0.14436912830652934, -0.25570534084524427, -0.12359489634233926, 0.19729098474739917, -0.10012417073927... |
707.4644 | Renormalization Group and Black Hole Production in Large Extra
Dimensions | It has been suggested that the existence of a non-Gaussian fixed point in
general relativity might cure the ultraviolet problems of this theory. Such a
fixed point is connected to an effective running of the gravitational coupling.
We calculate the effect of the running gravitational coupling on the black hole
produc... | hep-ph | it has been suggested that the existence of a nongaussian fixed point in general relativity might cure the ultraviolet problems of this theory such a fixed point is connected to an effective running of the gravitational coupling we calculate the effect of the running gravitational coupling on the black hole production ... | [['it', 'has', 'been', 'suggested', 'that', 'the', 'existence', 'of', 'a', 'nongaussian', 'fixed', 'point', 'in', 'general', 'relativity', 'might', 'cure', 'the', 'ultraviolet', 'problems', 'of', 'this', 'theory', 'such', 'a', 'fixed', 'point', 'is', 'connected', 'to', 'an', 'effective', 'running', 'of', 'the', 'gravit... | [-0.16943385616592052, 0.11818963414185357, -0.10149482850743047, 0.10273195443264509, -0.07005677682394951, -0.1297007826141129, -1.1706529421952822e-05, 0.28501745770385456, -0.19247479919912452, -0.28904299892611424, 0.07583093011388713, -0.3045814685776072, -0.1395663775945619, 0.15703541674982693, -0.0123698671222... |
707.4645 | OB Associations, Wolf-Rayet Stars, and the Origin of Galactic Cosmic
Rays | We have measured the isotopic abundances of neon and a number of other
species in the galactic cosmic rays (GCRs) using the Cosmic Ray Isotope
Spectrometer (CRIS) aboard the ACE spacecraft. Our data are compared to recent
results from two-component Wolf-Rayet (WR) models. The three largest deviations
of galactic cosm... | astro-ph | we have measured the isotopic abundances of neon and a number of other species in the galactic cosmic rays gcrs using the cosmic ray isotope spectrometer cris aboard the ace spacecraft our data are compared to recent results from twocomponent wolfrayet wr models the three largest deviations of galactic cosmic ray isoto... | [['we', 'have', 'measured', 'the', 'isotopic', 'abundances', 'of', 'neon', 'and', 'a', 'number', 'of', 'other', 'species', 'in', 'the', 'galactic', 'cosmic', 'rays', 'gcrs', 'using', 'the', 'cosmic', 'ray', 'isotope', 'spectrometer', 'cris', 'aboard', 'the', 'ace', 'spacecraft', 'our', 'data', 'are', 'compared', 'to', ... | [-0.06320126615409251, 0.1946087804101851, -0.05265395551964286, 0.10197770197188392, -0.04274152996506365, -0.040983552168611256, 0.07914741416572638, 0.42047725490161353, -0.1883934595477989, -0.3505935987014146, -0.016769059600552454, -0.3273608748047125, 0.014145345871691547, 0.21680049539676735, -0.014710937942644... |
707.4646 | On admissible rank one local systems | A rank one local system $\LL$ on a smooth complex algebraic variety $M$ is
1-admissible if the dimension of the first cohomology group $H^1(M,\LL)$ can be
computed from the cohomology algebra $H^*(M,\C)$ in degrees $\leq 2$. Under the
assumption that $M$ is 1-formal, we show that all local systems, except
finitely ma... | math.AG math.AT | a rank one local system ll on a smooth complex algebraic variety m is 1admissible if the dimension of the first cohomology group h1mll can be computed from the cohomology algebra hmc in degrees leq 2 under the assumption that m is 1formal we show that all local systems except finitely many on a nontranslated irreducibl... | [['a', 'rank', 'one', 'local', 'system', 'll', 'on', 'a', 'smooth', 'complex', 'algebraic', 'variety', 'm', 'is', '1admissible', 'if', 'the', 'dimension', 'of', 'the', 'first', 'cohomology', 'group', 'h1mll', 'can', 'be', 'computed', 'from', 'the', 'cohomology', 'algebra', 'hmc', 'in', 'degrees', 'leq', '2', 'under', '... | [-0.19782787106957567, 0.09355719827054033, -0.09542342790244322, 0.036096939244878674, -0.038453035451963824, -0.17490257790096914, -0.002619101628573295, 0.31699391487845274, -0.32352615805026497, -0.25980271899826685, 0.1307222109874447, -0.21536424815795333, -0.0775644192999264, 0.2268228450732938, -0.0779582457441... |
707.4647 | Comparing a model of cosmic ray production in the supernova remnant RX
J1713.7-3946 with observations | Explicitly time-dependent, nonlinear kinetic theory of cosmic ray (CR)
acceleration in supernova remnants (SNRs) has been employed to investigate the
properties of SNR RX J1713.7-3946. Observations of the nonthermal radio and
X-ray emission spectra as well as earlier H.E.S.S. measurements of the very
high energy $\ga... | astro-ph | explicitly timedependent nonlinear kinetic theory of cosmic ray cr acceleration in supernova remnants snrs has been employed to investigate the properties of snr rx j171373946 observations of the nonthermal radio and xray emission spectra as well as earlier hess measurements of the very high energy gammaray emission we... | [['explicitly', 'timedependent', 'nonlinear', 'kinetic', 'theory', 'of', 'cosmic', 'ray', 'cr', 'acceleration', 'in', 'supernova', 'remnants', 'snrs', 'has', 'been', 'employed', 'to', 'investigate', 'the', 'properties', 'of', 'snr', 'rx', 'j171373946', 'observations', 'of', 'the', 'nonthermal', 'radio', 'and', 'xray', ... | [-0.06100690322570947, 0.1277765169138134, -0.04439961282663386, 0.1511288189530288, -0.12186729728736365, -0.08294300989258442, -0.02645129147409038, 0.4422038031995974, -0.211654568572571, -0.3455613622156141, 0.020762004174519625, -0.2879618663057706, 0.010489032934649666, 0.22063821086339885, 0.051620358626347625, ... |
707.4648 | Quasiparticle bands in cuprates by quantum chemical methods: towards an
ab initio description of strong electron correlations | Realistic electronic-structure calculations for correlated Mott insulators
are notoriously hard. Here we present an ab initio multiconfiguration scheme
that adequately describes strong correlation effects involving Cu 3d and O 2p
electrons in layered cuprates. In particular, the O 2p states giving rise to
the Zhang-R... | cond-mat.str-el cond-mat.supr-con | realistic electronicstructure calculations for correlated mott insulators are notoriously hard here we present an ab initio multiconfiguration scheme that adequately describes strong correlation effects involving cu 3d and o 2p electrons in layered cuprates in particular the o 2p states giving rise to the zhangrice ban... | [['realistic', 'electronicstructure', 'calculations', 'for', 'correlated', 'mott', 'insulators', 'are', 'notoriously', 'hard', 'here', 'we', 'present', 'an', 'ab', 'initio', 'multiconfiguration', 'scheme', 'that', 'adequately', 'describes', 'strong', 'correlation', 'effects', 'involving', 'cu', '3d', 'and', 'o', '2p', ... | [-0.10133456990089533, 0.1435363852372445, -0.037975208965300614, 0.1251685250826995, -0.014675686688860878, -0.1599607868244805, 0.09065336277749989, 0.44500054771612796, -0.2572181917577317, -0.30567823571618646, -0.08275501663592877, -0.35929112349237713, -0.1686347007650641, 0.13767114791179275, 0.07010102827916853... |
707.4649 | Implications of Shock Wave Experiments with Precompressed Materials for
Giant Planet Interiors | This work uses density functional molecular dynamics simulations of fluid
helium at high pressure to examine how shock wave experiments with
precompressed samples can help characterizing the interior of giant planets. In
particular, we analyze how large of a precompression is needed to probe a
certain depth in a plan... | cond-mat.mtrl-sci | this work uses density functional molecular dynamics simulations of fluid helium at high pressure to examine how shock wave experiments with precompressed samples can help characterizing the interior of giant planets in particular we analyze how large of a precompression is needed to probe a certain depth in a planets ... | [['this', 'work', 'uses', 'density', 'functional', 'molecular', 'dynamics', 'simulations', 'of', 'fluid', 'helium', 'at', 'high', 'pressure', 'to', 'examine', 'how', 'shock', 'wave', 'experiments', 'with', 'precompressed', 'samples', 'can', 'help', 'characterizing', 'the', 'interior', 'of', 'giant', 'planets', 'in', 'p... | [-0.09958900634023266, 0.1995312467766687, -0.03508371983293611, 0.05222310990286179, -0.04155224056627888, -0.05243204255254032, 0.1054294756345021, 0.3612739142412559, -0.21948955815213805, -0.3950619403368387, 0.07337024392715345, -0.2751527880915465, -0.07879208131299283, 0.13945123459248301, -0.009333883633072942,... |
707.465 | Secondary resonances of co-orbital motions | The size distribution of the stability region around the Lagrangian point L4
is investigated in the elliptic restricted three-body problem as the function
of the mass parameter and the orbital eccentricity of the primaries. It is
shown that there are minimum zones in the size distribution of the stability
regions, an... | astro-ph | the size distribution of the stability region around the lagrangian point l4 is investigated in the elliptic restricted threebody problem as the function of the mass parameter and the orbital eccentricity of the primaries it is shown that there are minimum zones in the size distribution of the stability regions and the... | [['the', 'size', 'distribution', 'of', 'the', 'stability', 'region', 'around', 'the', 'lagrangian', 'point', 'l4', 'is', 'investigated', 'in', 'the', 'elliptic', 'restricted', 'threebody', 'problem', 'as', 'the', 'function', 'of', 'the', 'mass', 'parameter', 'and', 'the', 'orbital', 'eccentricity', 'of', 'the', 'primar... | [-0.17379212095188357, 0.17594828559275794, -0.08784942594784483, 0.0774631429717838, -0.04036730100704851, -0.03682461497849043, 0.03346404078777651, 0.31431412182472723, -0.2435372379722492, -0.3380131046477781, 0.11051191097572066, -0.2847026968564914, -0.07730371257223721, 0.17245080909093044, -0.05680993063243495,... |
707.4651 | Comments on the Reliability of Lawson and Hanson's Linear Distance
Programming Algorithm: Subroutine LDP | This brief paper: (1) Discusses strategies to generate random test cases that
can be used to extensively test any Linear Distance Program (LDP) software. (2)
Gives three numerical examples of input cases generated by this strategy that
cause problems in the Lawson and Hanson LDP module. (3) Proposes, as a standard
ma... | cs.MS | this brief paper 1 discusses strategies to generate random test cases that can be used to extensively test any linear distance program ldp software 2 gives three numerical examples of input cases generated by this strategy that cause problems in the lawson and hanson ldp module 3 proposes as a standard matter of accept... | [['this', 'brief', 'paper', '1', 'discusses', 'strategies', 'to', 'generate', 'random', 'test', 'cases', 'that', 'can', 'be', 'used', 'to', 'extensively', 'test', 'any', 'linear', 'distance', 'program', 'ldp', 'software', '2', 'gives', 'three', 'numerical', 'examples', 'of', 'input', 'cases', 'generated', 'by', 'this',... | [-0.07694318538150666, 0.07001673331145536, -0.08568097804673017, 0.12108344168465754, -0.09878147150051188, -0.22856956988742405, 0.04386559810425917, 0.3736502056687393, -0.26132497192275794, -0.3368142964487726, 0.12693635894260794, -0.22072010948746043, -0.13703060842076825, 0.214451652076307, -0.15284477851607584,... |
707.4652 | Laser tweezers for atomic solitons | We describe a controllable and precise laser tweezers for Bose-Einstein
condensates of ultracold atomic gases. In our configuration, a laser beam is
used to locally modify the sign of the scattering length in the vicinity of a
trapped BEC. The induced attractive interactions between atoms allow to extract
and transpo... | cond-mat.other | we describe a controllable and precise laser tweezers for boseeinstein condensates of ultracold atomic gases in our configuration a laser beam is used to locally modify the sign of the scattering length in the vicinity of a trapped bec the induced attractive interactions between atoms allow to extract and transport a c... | [['we', 'describe', 'a', 'controllable', 'and', 'precise', 'laser', 'tweezers', 'for', 'boseeinstein', 'condensates', 'of', 'ultracold', 'atomic', 'gases', 'in', 'our', 'configuration', 'a', 'laser', 'beam', 'is', 'used', 'to', 'locally', 'modify', 'the', 'sign', 'of', 'the', 'scattering', 'length', 'in', 'the', 'vicin... | [-0.14082233238590064, 0.20968083168627868, -0.06546021032518969, 0.013586985549291516, -0.0015071233560284265, -0.1460276809253013, 0.045119151791931204, 0.39647108006874004, -0.2769873388674405, -0.26521457819474975, -0.03419045324474171, -0.2786600945028309, -0.06281257422872075, 0.21990621799314997, 0.0456302405917... |
707.4653 | Correlation Effects in the Triangular Lattice Single-band System
Li_xNbO_2 | Superconductivity in hole-doped Li_xNbO_2 has been reported with T_c ~ 5 K in
the range 0.45 < x < 0.8. The electronic structure is based on a
two-dimensional triangular Nb lattice. The strong trigonal crystal field
results in a single Nb d(z^2) band isolated within a wide gap, leading to a
single-band triangular lat... | cond-mat.supr-con cond-mat.str-el | superconductivity in holedoped li_xnbo_2 has been reported with t_c 5 k in the range 045 x 08 the electronic structure is based on a twodimensional triangular nb lattice the strong trigonal crystal field results in a single nb dz2 band isolated within a wide gap leading to a singleband triangular lattice system the iso... | [['superconductivity', 'in', 'holedoped', 'li_xnbo_2', 'has', 'been', 'reported', 'with', 't_c', '5', 'k', 'in', 'the', 'range', '045', 'x', '08', 'the', 'electronic', 'structure', 'is', 'based', 'on', 'a', 'twodimensional', 'triangular', 'nb', 'lattice', 'the', 'strong', 'trigonal', 'crystal', 'field', 'results', 'in'... | [-0.1665482980418293, 0.17188148736792808, 0.015416761273038848, 0.06795486013973406, 0.00238953363698195, -0.202977784560062, 0.1476968823802, 0.43317452298395115, -0.251141625278465, -0.2805754100486143, -0.02598173138069208, -0.3776045115527642, -0.054872981200734264, 0.10325043792716529, 0.10959396719323088, -0.027... |
707.4654 | Multipole expansions for energy and momenta carried by gravitational
waves | We present expressions for the energy, linear momentum and angular momentum
carried away from an isolated system by gravitational radiation based on
spin-weighted spherical harmonics decomposition of the Weyl scalar $\Psi_4$. We
also show that the expressions derived are equivalent to the common expressions
obtained ... | gr-qc | we present expressions for the energy linear momentum and angular momentum carried away from an isolated system by gravitational radiation based on spinweighted spherical harmonics decomposition of the weyl scalar psi_4 we also show that the expressions derived are equivalent to the common expressions obtained when usi... | [['we', 'present', 'expressions', 'for', 'the', 'energy', 'linear', 'momentum', 'and', 'angular', 'momentum', 'carried', 'away', 'from', 'an', 'isolated', 'system', 'by', 'gravitational', 'radiation', 'based', 'on', 'spinweighted', 'spherical', 'harmonics', 'decomposition', 'of', 'the', 'weyl', 'scalar', 'psi_4', 'we',... | [-0.10745813319674478, 0.10066211373871808, -0.11687368167510542, 0.06981503817615493, -0.0912805782371344, -0.056449766006643094, -0.025979243695753843, 0.33123585748342943, -0.21051221168062723, -0.27091810150886886, 0.04943040961986229, -0.2755277198022948, -0.11245203279227448, 0.2625998492048194, 0.033255402947431... |
707.4655 | The intermediate-age globular cluster NGC 1783 in the Large Magellanic
Cloud | We present Hubble Space Telescope ACS deep photometry of the intermediate-age
globular cluster NGC 1783 in the Large Magellanic Cloud. By using this
photometric dataset, we have determined the degree of ellipticity of the
cluster ($\epsilon$=0.14$\pm$0.03) and the radial density profile. This profile
is well reproduc... | astro-ph | we present hubble space telescope acs deep photometry of the intermediateage globular cluster ngc 1783 in the large magellanic cloud by using this photometric dataset we have determined the degree of ellipticity of the cluster epsilon014pm003 and the radial density profile this profile is well reproduced by a standard ... | [['we', 'present', 'hubble', 'space', 'telescope', 'acs', 'deep', 'photometry', 'of', 'the', 'intermediateage', 'globular', 'cluster', 'ngc', '1783', 'in', 'the', 'large', 'magellanic', 'cloud', 'by', 'using', 'this', 'photometric', 'dataset', 'we', 'have', 'determined', 'the', 'degree', 'of', 'ellipticity', 'of', 'the... | [-0.018514394570308127, 0.07569967934755745, -0.1380135242020486, 0.0992924983688826, -0.05748783616248257, -0.03076765477170895, 0.08292531584772121, 0.43341563494911617, -0.20172512120638447, -0.40289204694837877, 0.03182292352119093, -0.23329256770978118, -0.04441356213280826, 0.17292026966027205, -0.070879971966107... |
707.4656 | Communication under Strong Asynchronism | We consider asynchronous communication over point-to-point discrete
memoryless channels. The transmitter starts sending one block codeword at an
instant that is uniformly distributed within a certain time period, which
represents the level of asynchronism. The receiver, by means of a sequential
decoder, must isolate ... | cs.IT math.IT | we consider asynchronous communication over pointtopoint discrete memoryless channels the transmitter starts sending one block codeword at an instant that is uniformly distributed within a certain time period which represents the level of asynchronism the receiver by means of a sequential decoder must isolate the messa... | [['we', 'consider', 'asynchronous', 'communication', 'over', 'pointtopoint', 'discrete', 'memoryless', 'channels', 'the', 'transmitter', 'starts', 'sending', 'one', 'block', 'codeword', 'at', 'an', 'instant', 'that', 'is', 'uniformly', 'distributed', 'within', 'a', 'certain', 'time', 'period', 'which', 'represents', 't... | [-0.23014433532583656, 0.1347760588618769, -0.059157774741177095, 0.02203520069404739, -0.05145027428536106, -0.2542042520991438, 0.13019295300165823, 0.3459918899674096, -0.30266806605482693, -0.23656895606156206, 0.12871275394322781, -0.258124225901284, -0.11226568411161039, 0.14211718766585332, -0.08488446943720399,... |
707.4657 | The Informational Conception and Basic Physics | In our previous arXiv papers ("The Information and the Matter", v1, v5; more
systematically the informational conception is presented in the paper "The
Information as Absolute", 2010) it was rigorously shown that Matter in our
Universe - and Universe as a whole - are some informational systems
(structures), which exi... | physics.gen-ph | in our previous arxiv papers the information and the matter v1 v5 more systematically the informational conception is presented in the paper the information as absolute 2010 it was rigorously shown that matter in our universe and universe as a whole are some informational systems structures which exist as uninterrupted... | [['in', 'our', 'previous', 'arxiv', 'papers', 'the', 'information', 'and', 'the', 'matter', 'v1', 'v5', 'more', 'systematically', 'the', 'informational', 'conception', 'is', 'presented', 'in', 'the', 'paper', 'the', 'information', 'as', 'absolute', '2010', 'it', 'was', 'rigorously', 'shown', 'that', 'matter', 'in', 'ou... | [-0.10905523353424969, 0.1343969663818027, -0.14330148917969734, 0.11450277974565361, -0.09076333715703946, -0.12220047399810306, 0.021624447116794596, 0.3207301211814225, -0.26634786633402824, -0.33333741737130496, 0.06729079990966093, -0.2604687882991055, -0.16283847380676592, 0.1767600170925868, -0.0733554041718741,... |
707.4658 | Higgs Hadroproduction at Large Feynman x | We propose a novel mechanism for the production of the Higgs boson in
inclusive hadronic collisions, which utilizes the presence of heavy quarks in
the proton wave function. In these inclusive reactions the Higgs boson acquires
the momenta of both the heavy quark and antiquark and thus carries 80% or more
of the proj... | hep-ph | we propose a novel mechanism for the production of the higgs boson in inclusive hadronic collisions which utilizes the presence of heavy quarks in the proton wave function in these inclusive reactions the higgs boson acquires the momenta of both the heavy quark and antiquark and thus carries 80 or more of the projectil... | [['we', 'propose', 'a', 'novel', 'mechanism', 'for', 'the', 'production', 'of', 'the', 'higgs', 'boson', 'in', 'inclusive', 'hadronic', 'collisions', 'which', 'utilizes', 'the', 'presence', 'of', 'heavy', 'quarks', 'in', 'the', 'proton', 'wave', 'function', 'in', 'these', 'inclusive', 'reactions', 'the', 'higgs', 'boso... | [-0.018421456664937604, 0.2729803200568045, -0.10698280419113443, 0.13478883241015652, -0.012276641490376172, -0.1232614879763466, 0.03779180647860117, 0.32413398509516433, -0.22850655434269676, -0.24463436238686828, -0.06558011370943859, -0.352484603363144, 0.07016388157464783, 0.13970013094983777, 0.07169332046674647... |
707.4659 | Difference Equations in Massive Higher Order Calculations | The calculation of massive 2--loop operator matrix elements, required for the
higher order Wilson coefficients for heavy flavor production in deeply
inelastic scattering, leads to new types of multiple infinite sums over
harmonic sums and related functions, which depend on the Mellin parameter $N$.
We report on the s... | math-ph cs.MS hep-ph math.MP | the calculation of massive 2loop operator matrix elements required for the higher order wilson coefficients for heavy flavor production in deeply inelastic scattering leads to new types of multiple infinite sums over harmonic sums and related functions which depend on the mellin parameter n we report on the solution of... | [['the', 'calculation', 'of', 'massive', '2loop', 'operator', 'matrix', 'elements', 'required', 'for', 'the', 'higher', 'order', 'wilson', 'coefficients', 'for', 'heavy', 'flavor', 'production', 'in', 'deeply', 'inelastic', 'scattering', 'leads', 'to', 'new', 'types', 'of', 'multiple', 'infinite', 'sums', 'over', 'harm... | [-0.1357299656318944, 0.1678839380749398, -0.044310771047122895, 0.07932477114012554, -0.06379394558450532, -0.07426400948315859, 0.06311445826080643, 0.2969253915731633, -0.2471211530149929, -0.22474410835771808, 0.07110313670931473, -0.3459040614229346, -0.10736688114480958, 0.18497449281581102, 0.0811984237017376, 0... |
707.466 | Influence of Lorentz-violating terms on a two-level system | The influence of Lorentz- and CPT-violating terms of the extended Standard
Model on a semi-classical two-level system is analyzed. It is shown that the
Lorentz-violating background (when coupled with the fermion sector in a vector
way) is able to induce modifications on the Rabi oscillation pattern, promoting
sensiti... | hep-th | the influence of lorentz and cptviolating terms of the extended standard model on a semiclassical twolevel system is analyzed it is shown that the lorentzviolating background when coupled with the fermion sector in a vector way is able to induce modifications on the rabi oscillation pattern promoting sensitive modulati... | [['the', 'influence', 'of', 'lorentz', 'and', 'cptviolating', 'terms', 'of', 'the', 'extended', 'standard', 'model', 'on', 'a', 'semiclassical', 'twolevel', 'system', 'is', 'analyzed', 'it', 'is', 'shown', 'that', 'the', 'lorentzviolating', 'background', 'when', 'coupled', 'with', 'the', 'fermion', 'sector', 'in', 'a',... | [-0.14598046068766785, 0.19751052077350698, -0.03299451094423222, 0.11509983892289874, -0.07412793725315067, -0.11485150356928253, 0.014205176166346313, 0.30452318829444486, -0.2192225267505671, -0.28950521396075046, 0.07798000037944756, -0.2942429464151207, -0.13633751346228215, 0.2146162831196641, 0.01036845743417357... |
707.4661 | Theory of cosmic ray and $\gamma$-ray production in the supernova
remnant RX J0852.0-4622 (Vela Jr.) | Explicitly time-dependent, nonlinear kinetic theory of cosmic ray (CR)
acceleration in supernova remnants (SNRs) has been used to investigate the
properties of the very large SNR RX J0852.0-4622. The available observations do
not clearly distinguish between a ``nearby'' (at $\sim 200$ pc) and a
``distant'' (at $\sim ... | astro-ph | explicitly timedependent nonlinear kinetic theory of cosmic ray cr acceleration in supernova remnants snrs has been used to investigate the properties of the very large snr rx j085204622 the available observations do not clearly distinguish between a nearby at sim 200 pc and a distant at sim 1 kpc source scenario there... | [['explicitly', 'timedependent', 'nonlinear', 'kinetic', 'theory', 'of', 'cosmic', 'ray', 'cr', 'acceleration', 'in', 'supernova', 'remnants', 'snrs', 'has', 'been', 'used', 'to', 'investigate', 'the', 'properties', 'of', 'the', 'very', 'large', 'snr', 'rx', 'j085204622', 'the', 'available', 'observations', 'do', 'not'... | [-0.06732306636415229, 0.14028841356163677, -0.029888665812300905, 0.14219044277286333, -0.0761813953879096, -0.10581560984148451, 0.03648026647652447, 0.3991510964824625, -0.23131744991636502, -0.3608765563242278, 0.038540062520055554, -0.297032011499769, 0.04471275326883736, 0.20231548654209858, 0.05188369477334661, ... |
707.4662 | Preplanetary Nebulae: An HST Imaging Survey and a New Morphological
Classification System | Using the Hubble Space Telescope (HST), we have carried out a survey of
candidate preplanetary nebulae (PPNs). We report here our discoveries of
objects having well-resolved geometrical structures, and use the large sample
of PPNs now imaged with HST (including previously studied objects in this
class) to devise a co... | astro-ph | using the hubble space telescope hst we have carried out a survey of candidate preplanetary nebulae ppns we report here our discoveries of objects having wellresolved geometrical structures and use the large sample of ppns now imaged with hst including previously studied objects in this class to devise a comprehensive ... | [['using', 'the', 'hubble', 'space', 'telescope', 'hst', 'we', 'have', 'carried', 'out', 'a', 'survey', 'of', 'candidate', 'preplanetary', 'nebulae', 'ppns', 'we', 'report', 'here', 'our', 'discoveries', 'of', 'objects', 'having', 'wellresolved', 'geometrical', 'structures', 'and', 'use', 'the', 'large', 'sample', 'of'... | [-0.08893598206902555, 0.08893451448134979, -0.09273847619728517, 0.0681475102870276, -0.1316299969288853, -0.028063562711135352, 0.027924183119986474, 0.44666458574855433, -0.1613581221151565, -0.34325705941383994, 0.05526459888226652, -0.22534684442715452, -0.09774268357640332, 0.23148617168668092, -0.066182926642276... |
707.4663 | The Properties and Gaseous Environments of Powerful Classical Double
Radio Galaxies | The properties of a sample of 31 very powerful classical double radio
galaxies with redshifts between zero and 1.8 are studied. The source
velocities, beam powers, ambient gas densities, total lifetimes, and total
outflow energies are presented and discussed. The rate of growth of each side
of each source were obtain... | astro-ph | the properties of a sample of 31 very powerful classical double radio galaxies with redshifts between zero and 18 are studied the source velocities beam powers ambient gas densities total lifetimes and total outflow energies are presented and discussed the rate of growth of each side of each source were obtained using ... | [['the', 'properties', 'of', 'a', 'sample', 'of', '31', 'very', 'powerful', 'classical', 'double', 'radio', 'galaxies', 'with', 'redshifts', 'between', 'zero', 'and', '18', 'are', 'studied', 'the', 'source', 'velocities', 'beam', 'powers', 'ambient', 'gas', 'densities', 'total', 'lifetimes', 'and', 'total', 'outflow', ... | [-0.09876940127545807, 0.14379202137152902, -0.04748517611301887, 0.038896163854469826, -0.013865875106433898, -0.10658079079953042, 0.053565496964847824, 0.40982530373088144, -0.23294446849389186, -0.3348117836335779, 0.09355195480886669, -0.285191973431431, 0.060939816522182194, 0.2280378039408217, 0.0272425430528497... |
707.4664 | One-way quantum computation with four-dimensional photonic qudits | We consider the possibility of performing linear optical quantum computation
making use of extra photonic degrees of freedom. In particular we focus on the
case where we use photons as quadbits. The basic 2-quadbit cluster state is a
hyper-entangled state across polarization and two spatial mode degrees of
freedom. W... | quant-ph | we consider the possibility of performing linear optical quantum computation making use of extra photonic degrees of freedom in particular we focus on the case where we use photons as quadbits the basic 2quadbit cluster state is a hyperentangled state across polarization and two spatial mode degrees of freedom we exami... | [['we', 'consider', 'the', 'possibility', 'of', 'performing', 'linear', 'optical', 'quantum', 'computation', 'making', 'use', 'of', 'extra', 'photonic', 'degrees', 'of', 'freedom', 'in', 'particular', 'we', 'focus', 'on', 'the', 'case', 'where', 'we', 'use', 'photons', 'as', 'quadbits', 'the', 'basic', '2quadbit', 'clu... | [-0.15221633626827719, 0.20672193709509196, -0.037134617403451656, 0.008729170424221838, -0.041816236407219154, -0.1857598467943938, 0.09542921799977587, 0.3845946819496316, -0.27402474190298437, -0.28634438459836953, 0.05398928706779623, -0.2567363027609079, -0.08148096204810851, 0.16406133531819325, 0.007471741353731... |
707.4665 | Wormholes with a space- and time-dependent equation of state | The discovery that the Universe is undergoing an accelerated expansion has
suggested the existence of an evolving equation of state. This paper discusses
various wormhole solutions in a spherically symmetric spacetime with an
equation of state that is both space and time dependent. The solutions obtained
are exact an... | gr-qc | the discovery that the universe is undergoing an accelerated expansion has suggested the existence of an evolving equation of state this paper discusses various wormhole solutions in a spherically symmetric spacetime with an equation of state that is both space and time dependent the solutions obtained are exact and ge... | [['the', 'discovery', 'that', 'the', 'universe', 'is', 'undergoing', 'an', 'accelerated', 'expansion', 'has', 'suggested', 'the', 'existence', 'of', 'an', 'evolving', 'equation', 'of', 'state', 'this', 'paper', 'discusses', 'various', 'wormhole', 'solutions', 'in', 'a', 'spherically', 'symmetric', 'spacetime', 'with', ... | [-0.18487380074052992, 0.09937363888124218, -0.12925241458213935, 0.019827537059042034, -0.08449405474367283, -0.09082350220878498, -0.06911382762423196, 0.32608189765300793, -0.16551428970138907, -0.25100392295773755, 0.12548559952045837, -0.26866672028613797, -0.10084161909802233, 0.15038179689860445, -0.009667016171... |
707.4666 | From the Magnetization Profile to the Stray Field of Bistable Wires | We present new analytical calculations of the spatial dependence of the stray
field of a bistable magnetic wire from the magnetization profile of the wire.
Contributions from the outer shell and from the wire ends are neglected. The
results qualitatively agree with experimental data, taken from literature.
| cond-mat.mtrl-sci cond-mat.soft | we present new analytical calculations of the spatial dependence of the stray field of a bistable magnetic wire from the magnetization profile of the wire contributions from the outer shell and from the wire ends are neglected the results qualitatively agree with experimental data taken from literature | [['we', 'present', 'new', 'analytical', 'calculations', 'of', 'the', 'spatial', 'dependence', 'of', 'the', 'stray', 'field', 'of', 'a', 'bistable', 'magnetic', 'wire', 'from', 'the', 'magnetization', 'profile', 'of', 'the', 'wire', 'contributions', 'from', 'the', 'outer', 'shell', 'and', 'from', 'the', 'wire', 'ends', ... | [-0.12312652472842564, 0.10036547548395205, -0.09554628944618905, 0.012285804118406265, -0.04557466023462884, -0.10684801995793873, 0.03228267475447439, 0.3867923897948671, -0.21178981194153745, -0.3246654866936993, 0.010687515010779842, -0.3301457437746068, -0.05937527534254688, 0.21493213086270113, 0.0206035759418885... |
707.4667 | Macroscopic Distinguishability Between Quantum States Defining Different
Phases of Matter: Fidelity and the Uhlmann Geometric Phase | We study the fidelity approach to quantum phase transitions (QPTs) and apply
it to general thermal phase transitions (PTs). We analyze two particular cases:
the Stoner-Hubbard itinerant electron model of magnetism and the BCS theory of
superconductivity. In both cases we show that the sudden drop of the mixed
state f... | quant-ph cond-mat.str-el | we study the fidelity approach to quantum phase transitions qpts and apply it to general thermal phase transitions pts we analyze two particular cases the stonerhubbard itinerant electron model of magnetism and the bcs theory of superconductivity in both cases we show that the sudden drop of the mixed state fidelity ma... | [['we', 'study', 'the', 'fidelity', 'approach', 'to', 'quantum', 'phase', 'transitions', 'qpts', 'and', 'apply', 'it', 'to', 'general', 'thermal', 'phase', 'transitions', 'pts', 'we', 'analyze', 'two', 'particular', 'cases', 'the', 'stonerhubbard', 'itinerant', 'electron', 'model', 'of', 'magnetism', 'and', 'the', 'bcs... | [-0.18716998014673097, 0.17648195708478917, -0.04855714859718469, 0.04710714638523067, 0.015437336160573146, -0.13108642672540138, 0.11826856479677834, 0.31565156258297283, -0.2436898964124158, -0.22975898037868125, 0.06537515671063363, -0.3122933299545914, -0.18379327494632577, 0.13186758200002724, -0.0019072223645912... |
707.4668 | Atomic lattice excitons: from condensates to crystals | We discuss atomic lattice excitons (ALEs), bound particle-hole pairs formed
by fermionic atoms in two bands of an optical lattice. Such a system provides a
clean setup to study fundamental properties of excitons, ranging from
condensation to exciton crystals (which appear for a large effective mass ratio
between part... | cond-mat.other | we discuss atomic lattice excitons ales bound particlehole pairs formed by fermionic atoms in two bands of an optical lattice such a system provides a clean setup to study fundamental properties of excitons ranging from condensation to exciton crystals which appear for a large effective mass ratio between particles and... | [['we', 'discuss', 'atomic', 'lattice', 'excitons', 'ales', 'bound', 'particlehole', 'pairs', 'formed', 'by', 'fermionic', 'atoms', 'in', 'two', 'bands', 'of', 'an', 'optical', 'lattice', 'such', 'a', 'system', 'provides', 'a', 'clean', 'setup', 'to', 'study', 'fundamental', 'properties', 'of', 'excitons', 'ranging', '... | [-0.13770909635288836, 0.20703314479741444, -0.03208261832447821, 0.04852486696510919, 0.03747060841353806, -0.16933192929718643, 0.09628544772337926, 0.3957093687740302, -0.20695464289747179, -0.29538215177231714, 0.02846162623149882, -0.2708305527921766, -0.07968688133099165, 0.1760825449355731, 0.034223105525980874,... |
707.4669 | Giant magnon bound states from strongly coupled N=4 SYM | We calculate in a very simple way the spectrum of giant magnon bound states
at strong coupling in N=4 SYM, by utilizing the description of the field theory
vacuum in terms of a condensate of eigenvalues of commuting matrices. We
further show that these calculations can be understood in terms of the central
charge ext... | hep-th | we calculate in a very simple way the spectrum of giant magnon bound states at strong coupling in n4 sym by utilizing the description of the field theory vacuum in terms of a condensate of eigenvalues of commuting matrices we further show that these calculations can be understood in terms of the central charge extensio... | [['we', 'calculate', 'in', 'a', 'very', 'simple', 'way', 'the', 'spectrum', 'of', 'giant', 'magnon', 'bound', 'states', 'at', 'strong', 'coupling', 'in', 'n4', 'sym', 'by', 'utilizing', 'the', 'description', 'of', 'the', 'field', 'theory', 'vacuum', 'in', 'terms', 'of', 'a', 'condensate', 'of', 'eigenvalues', 'of', 'co... | [-0.1324013052461669, 0.17354886228451505, -0.0950463588302955, 0.06812111470731906, 0.01291071517392993, -0.062056269738823173, 0.03377356320503168, 0.32044585231691597, -0.15968433904170523, -0.27486466367263346, 0.035444703535176814, -0.25842074205633253, -0.1839744825474918, 0.11219159396074246, -0.0065591387427411... |
707.467 | Environmental dependence in the ellipsoidal collapse model | N-body simulations have demonstrated a correlation between the properties of
haloes and their environment. In this paper, we assess whether the ellipsoidal
collapse model can produce a similar dependence. First, we explore the
statistical correlation that originates from Gaussian initial conditions. We
derive analyti... | astro-ph | nbody simulations have demonstrated a correlation between the properties of haloes and their environment in this paper we assess whether the ellipsoidal collapse model can produce a similar dependence first we explore the statistical correlation that originates from gaussian initial conditions we derive analytic expres... | [['nbody', 'simulations', 'have', 'demonstrated', 'a', 'correlation', 'between', 'the', 'properties', 'of', 'haloes', 'and', 'their', 'environment', 'in', 'this', 'paper', 'we', 'assess', 'whether', 'the', 'ellipsoidal', 'collapse', 'model', 'can', 'produce', 'a', 'similar', 'dependence', 'first', 'we', 'explore', 'the... | [-0.11486232792564731, 0.1334297968056845, -0.11907465832090859, 0.12027168804447033, -0.049775220816989985, -0.035401731830604966, -0.008434321196518726, 0.3751980631298883, -0.18401260113017984, -0.35926410063744096, 0.04050399436916512, -0.2520305659093271, -0.12841239326070694, 0.15759088911896893, 0.00043343043977... |
707.4671 | Observational Evidence for Negative-Energy Dust in Late-Times Cosmology | We perform fits of unconventional dark energy models to the available data
from high-redshift supernovae, distant galaxies and baryon oscillations. The
models are based either on brane cosmologies or on Liouville strings in which a
relaxation dark energy is provided by a rolling dilaton field (Q-cosmology). An
intere... | astro-ph gr-qc hep-th | we perform fits of unconventional dark energy models to the available data from highredshift supernovae distant galaxies and baryon oscillations the models are based either on brane cosmologies or on liouville strings in which a relaxation dark energy is provided by a rolling dilaton field qcosmology an interesting fea... | [['we', 'perform', 'fits', 'of', 'unconventional', 'dark', 'energy', 'models', 'to', 'the', 'available', 'data', 'from', 'highredshift', 'supernovae', 'distant', 'galaxies', 'and', 'baryon', 'oscillations', 'the', 'models', 'are', 'based', 'either', 'on', 'brane', 'cosmologies', 'or', 'on', 'liouville', 'strings', 'in'... | [-0.07405535167675804, 0.13435260260051057, -0.12890148526702672, 0.14607287281811704, -0.12382339736148393, -0.14216635005500217, -0.019458316962004868, 0.31831623466274184, -0.2090925211006235, -0.33980109288611193, 0.05080654012851691, -0.2787888355984542, -0.0496476339312367, 0.19207628566854396, -0.003893026726319... |
707.4672 | Effects of non-uniform acceptance in anisotropic flow measurement | Applicability of anisotropic flow measurement techniques and their extension
for detectors with non-uniform azimuthal acceptance are discussed. Considering
anisotropic flow measurement with two and three (mixed harmonic) azimuthal
correlations we introduce a set of observables based on the x and y components
of the e... | nucl-th | applicability of anisotropic flow measurement techniques and their extension for detectors with nonuniform azimuthal acceptance are discussed considering anisotropic flow measurement with two and three mixed harmonic azimuthal correlations we introduce a set of observables based on the x and y components of the event f... | [['applicability', 'of', 'anisotropic', 'flow', 'measurement', 'techniques', 'and', 'their', 'extension', 'for', 'detectors', 'with', 'nonuniform', 'azimuthal', 'acceptance', 'are', 'discussed', 'considering', 'anisotropic', 'flow', 'measurement', 'with', 'two', 'and', 'three', 'mixed', 'harmonic', 'azimuthal', 'correl... | [-0.07880143774285292, 0.11908847161879142, -0.14162350007876132, 0.07392458964992936, -0.045688200637232515, -0.11677775454008951, -0.007787730424509694, 0.3701900770732512, -0.2337964204683279, -0.305915580301856, 0.09568927447932461, -0.2541776033351198, -0.06085096364064763, 0.2155089287960436, -0.00888604780969520... |
707.4673 | On the space of morphisms between \'etale groupoids | Given two \'etale groupoids $\Cal G$ and $\Cal G'$, we consider the set of
pointed morphisms from $\Cal G$ to $\Cal G'$. Under suitable hypothesis we
introduce on this set a structure of Banach manifold which can be considered as
the space of objects of an \'etale groupoid whose space of orbits is the space
of morphi... | math.GT | given two etale groupoids cal g and cal g we consider the set of pointed morphisms from cal g to cal g under suitable hypothesis we introduce on this set a structure of banach manifold which can be considered as the space of objects of an etale groupoid whose space of orbits is the space of morphisms from cal g to cal ... | [['given', 'two', 'etale', 'groupoids', 'cal', 'g', 'and', 'cal', 'g', 'we', 'consider', 'the', 'set', 'of', 'pointed', 'morphisms', 'from', 'cal', 'g', 'to', 'cal', 'g', 'under', 'suitable', 'hypothesis', 'we', 'introduce', 'on', 'this', 'set', 'a', 'structure', 'of', 'banach', 'manifold', 'which', 'can', 'be', 'consi... | [-0.20471957906903254, 0.11269765314188719, -0.05652080499936664, 0.020450040993709413, -0.1268942682811665, -0.06158068373296705, 0.008763094700592023, 0.4023820517200326, -0.33777548978844335, -0.25431712719774435, 0.05943511749824716, -0.22864789558604123, -0.0957656961584848, 0.14688593350232593, -0.209480599337627... |
707.4674 | Many-body exchange-correlation effects in graphene | We calculate, within the leading-order dynamical-screening approximation, the
electron self-energy and spectral function at zero temperature for extrinsic
(or gated/doped) graphene. We also calculate hot carrier inelastic scattering
due to electron-electron interactions in graphene. We obtain the inelastic
quasiparti... | cond-mat.mes-hall | we calculate within the leadingorder dynamicalscreening approximation the electron selfenergy and spectral function at zero temperature for extrinsic or gateddoped graphene we also calculate hot carrier inelastic scattering due to electronelectron interactions in graphene we obtain the inelastic quasiparticle lifetimes... | [['we', 'calculate', 'within', 'the', 'leadingorder', 'dynamicalscreening', 'approximation', 'the', 'electron', 'selfenergy', 'and', 'spectral', 'function', 'at', 'zero', 'temperature', 'for', 'extrinsic', 'or', 'gateddoped', 'graphene', 'we', 'also', 'calculate', 'hot', 'carrier', 'inelastic', 'scattering', 'due', 'to... | [-0.11050531952915822, 0.23346553597708836, -0.08427054829542827, 0.12232824582058717, -0.003861560677999959, -0.10943271449821837, 0.06078856654793901, 0.409426665317048, -0.2716545603950234, -0.24454721641343305, -0.11378631001399994, -0.390692102832391, -0.0981617399443434, 0.14647784628836877, 0.0859049950445564, 0... |
707.4675 | In silico design of metal-dielectric nanocomposites for solar energy
applications | Recently, a homogenization procedure has been proposed, based on the tight
lower bounds of the Bergman-Milton formulation, and successfully applied to
dilute ternary nanocomposites to predict optical data without using any fitting
parameters [Garcia et al. Phys. Rev. B, 75, 045439 (2007)]. The procedure has
been exte... | cond-mat.mtrl-sci | recently a homogenization procedure has been proposed based on the tight lower bounds of the bergmanmilton formulation and successfully applied to dilute ternary nanocomposites to predict optical data without using any fitting parameters garcia et al phys rev b 75 045439 2007 the procedure has been extended and applied... | [['recently', 'a', 'homogenization', 'procedure', 'has', 'been', 'proposed', 'based', 'on', 'the', 'tight', 'lower', 'bounds', 'of', 'the', 'bergmanmilton', 'formulation', 'and', 'successfully', 'applied', 'to', 'dilute', 'ternary', 'nanocomposites', 'to', 'predict', 'optical', 'data', 'without', 'using', 'any', 'fitti... | [-0.0429604117719767, 0.09310612355410638, -0.03708482117185162, -0.06452368966226156, -0.03051554163943769, -0.13997940590747426, 0.05730683609403463, 0.43766184378182516, -0.21471533697331324, -0.4028120419651613, 0.026609658131848037, -0.2788251615776163, -0.1446511576585989, 0.19297593459163587, -0.0489529378392035... |
707.4676 | Blazar Gamma-Rays, Shock Acceleration, and the Extragalactic Background
Light | The observed spectra of blazars, their intrinsic emission, and the underlying
populations of radiating particles are intimately related. The use of these
sources as probes of the extragalactic infrared background, a prospect
propelled by recent advances in TeV-band telescopes, soon to be augmented by
observations by ... | astro-ph hep-ph | the observed spectra of blazars their intrinsic emission and the underlying populations of radiating particles are intimately related the use of these sources as probes of the extragalactic infrared background a prospect propelled by recent advances in tevband telescopes soon to be augmented by observations by nasas up... | [['the', 'observed', 'spectra', 'of', 'blazars', 'their', 'intrinsic', 'emission', 'and', 'the', 'underlying', 'populations', 'of', 'radiating', 'particles', 'are', 'intimately', 'related', 'the', 'use', 'of', 'these', 'sources', 'as', 'probes', 'of', 'the', 'extragalactic', 'infrared', 'background', 'a', 'prospect', '... | [-0.026142010941197547, 0.21686303516617045, -0.08445949436110609, 0.16629349202712013, -0.11326829650822808, -0.07749677384751574, -0.03061860501903164, 0.4723100693252705, -0.15616546719170668, -0.3717885445050128, 0.0612212937181432, -0.34600392977111316, -0.04426308163879987, 0.2664903273068964, -0.0124153476550846... |
707.4677 | Extreme recoils: impact on the detection of gravitational waves from
massive black hole binaries | Recent numerical simulations of coalescences of highly spinning massive black
hole binaries (MBHBs) suggest that the remnant can suffer a recoil velocity of
the order of few thousands km/s. We study here, by means of dedicated
simulations of black holes build--up, how such extreme recoils could affect the
cosmologica... | astro-ph | recent numerical simulations of coalescences of highly spinning massive black hole binaries mbhbs suggest that the remnant can suffer a recoil velocity of the order of few thousands kms we study here by means of dedicated simulations of black holes buildup how such extreme recoils could affect the cosmological coalesce... | [['recent', 'numerical', 'simulations', 'of', 'coalescences', 'of', 'highly', 'spinning', 'massive', 'black', 'hole', 'binaries', 'mbhbs', 'suggest', 'that', 'the', 'remnant', 'can', 'suffer', 'a', 'recoil', 'velocity', 'of', 'the', 'order', 'of', 'few', 'thousands', 'kms', 'we', 'study', 'here', 'by', 'means', 'of', '... | [-0.1459981456661685, 0.21447058428531965, 0.022708745469414704, 0.13370421883033437, -0.06740366829609548, -0.07802280744890104, 0.0511735101759031, 0.32456674611044894, -0.13963955857765836, -0.36814491693685586, 0.11088703482701268, -0.33561227472901745, -0.054437264625134096, 0.24203530789189343, 0.0065172206434245... |
707.4678 | Dynamical clustering of counterions on flexible polyelectrolytes | Molecular dynamics simulations are used to study the local dynamics of
counterion-charged polymer association at charge densities above and below the
counterion condensation threshold. Surprisingly, the counterions form
weakly-interacting clusters which exhibit short range orientational order, and
which decay slowly ... | cond-mat.soft | molecular dynamics simulations are used to study the local dynamics of counterioncharged polymer association at charge densities above and below the counterion condensation threshold surprisingly the counterions form weaklyinteracting clusters which exhibit short range orientational order and which decay slowly due to ... | [['molecular', 'dynamics', 'simulations', 'are', 'used', 'to', 'study', 'the', 'local', 'dynamics', 'of', 'counterioncharged', 'polymer', 'association', 'at', 'charge', 'densities', 'above', 'and', 'below', 'the', 'counterion', 'condensation', 'threshold', 'surprisingly', 'the', 'counterions', 'form', 'weaklyinteractin... | [-0.08631377442493048, 0.21611060919285702, -0.050131360231618204, 0.09067250357334872, 0.0058276207966124075, -0.12093996326719601, 0.025611347523069077, 0.39207108868622637, -0.26226637676268455, -0.3194301306573023, 0.020002130507379322, -0.28580447496195516, -0.052663349033142605, 0.15318809621350235, 0.06957535068... |
707.4679 | On the Transfer of Adiabatic Fluctuations through a Nonsingular
Cosmological Bounce | We study the transfer of cosmological perturbations through a nonsingular
cosmological bounce in a special model in which the parameters of the bounce
and the equation of state of matter are chosen such as to allow for an exact
calculation of the evolution of the fluctuations. We find that the growing mode
of the met... | hep-th astro-ph gr-qc hep-ph | we study the transfer of cosmological perturbations through a nonsingular cosmological bounce in a special model in which the parameters of the bounce and the equation of state of matter are chosen such as to allow for an exact calculation of the evolution of the fluctuations we find that the growing mode of the metric... | [['we', 'study', 'the', 'transfer', 'of', 'cosmological', 'perturbations', 'through', 'a', 'nonsingular', 'cosmological', 'bounce', 'in', 'a', 'special', 'model', 'in', 'which', 'the', 'parameters', 'of', 'the', 'bounce', 'and', 'the', 'equation', 'of', 'state', 'of', 'matter', 'are', 'chosen', 'such', 'as', 'to', 'all... | [-0.15336029992199615, 0.1707184023317003, -0.15199653907260352, 0.053995948171653194, -0.022949872350474017, -0.08410676085302572, -0.022981837152614506, 0.2711828203413661, -0.25708880200298556, -0.24121849737856366, 0.13629049521234365, -0.290458732372184, -0.10016907503777141, 0.17126922203236422, 0.011750837813618... |
707.468 | Local three-nucleon interaction from chiral effective field theory | The three-nucleon (NNN) interaction derived within the chiral effective field
theory at the next-to-next-to-leading order (N2LO) is regulated with a function
depending on the magnitude of the momentum transfer. The regulated NNN
interaction is then local in the coordinate space, which is advantages for some
many-body... | nucl-th | the threenucleon nnn interaction derived within the chiral effective field theory at the nexttonexttoleading order n2lo is regulated with a function depending on the magnitude of the momentum transfer the regulated nnn interaction is then local in the coordinate space which is advantages for some manybody techniques ma... | [['the', 'threenucleon', 'nnn', 'interaction', 'derived', 'within', 'the', 'chiral', 'effective', 'field', 'theory', 'at', 'the', 'nexttonexttoleading', 'order', 'n2lo', 'is', 'regulated', 'with', 'a', 'function', 'depending', 'on', 'the', 'magnitude', 'of', 'the', 'momentum', 'transfer', 'the', 'regulated', 'nnn', 'in... | [-0.11691790392311911, 0.16832268905228026, -0.05292918005049872, 0.08769986671424344, 0.002019868120206175, -0.06993542472475472, -0.011449522731170335, 0.39032824712311043, -0.22143203877832418, -0.20321436352268965, -0.08204011211349962, -0.35093157022133653, -0.12348114074219341, 0.012326468500872085, 0.16733842228... |
707.4681 | A more direct representation for complex relativity | An alternative to the representation of complex relativity by self-dual
complex 2-forms on the spacetime manifold is presented by assuming that that
the bundle of real 2-forms is given an almost-complex structure. From this, one
can define a complex orthogonal structure on the bundle of 2-forms, which
results in a mo... | gr-qc | an alternative to the representation of complex relativity by selfdual complex 2forms on the spacetime manifold is presented by assuming that that the bundle of real 2forms is given an almostcomplex structure from this one can define a complex orthogonal structure on the bundle of 2forms which results in a more direct ... | [['an', 'alternative', 'to', 'the', 'representation', 'of', 'complex', 'relativity', 'by', 'selfdual', 'complex', '2forms', 'on', 'the', 'spacetime', 'manifold', 'is', 'presented', 'by', 'assuming', 'that', 'that', 'the', 'bundle', 'of', 'real', '2forms', 'is', 'given', 'an', 'almostcomplex', 'structure', 'from', 'this... | [-0.20646714111293865, 0.07737470618053148, -0.0653446895513134, 0.04334526939783245, -0.13076342420927325, -0.0955277394358313, -0.09474682262869644, 0.369118586632988, -0.2453047331178286, -0.214820910359687, 0.07973257067315585, -0.19256218512099785, -0.2814733567036933, 0.17341382322512322, -0.10119817372732108, -0... |
708.0001 | The effects of Chern-Simons gravity on bodies orbiting the Earth | One of the possible low-energy consequences of string theory is the addition
of a Chern-Simons term to the standard Einstein-Hilbert action of general
relativity. It can be argued that the quintessence field should couple to this
Chern-Simons term, and if so, it drives in the linearized theory a
parity-violating inte... | astro-ph gr-qc hep-ph hep-th | one of the possible lowenergy consequences of string theory is the addition of a chernsimons term to the standard einsteinhilbert action of general relativity it can be argued that the quintessence field should couple to this chernsimons term and if so it drives in the linearized theory a parityviolating interaction be... | [['one', 'of', 'the', 'possible', 'lowenergy', 'consequences', 'of', 'string', 'theory', 'is', 'the', 'addition', 'of', 'a', 'chernsimons', 'term', 'to', 'the', 'standard', 'einsteinhilbert', 'action', 'of', 'general', 'relativity', 'it', 'can', 'be', 'argued', 'that', 'the', 'quintessence', 'field', 'should', 'couple'... | [-0.18180079241925529, 0.15534605527425122, -0.08732224428416069, 0.07853248387330276, -0.12990365569190732, -0.10541206913406094, -0.07243191764453137, 0.2482151657158252, -0.22098251062059968, -0.2994051232917941, 0.018195804214538557, -0.26280326185073577, -0.18634419039228994, 0.1484682616127398, -0.089232529120134... |
708.0002 | 1E 1547.0-5408: a radio-emitting magnetar with a rotation period of 2
seconds | The variable X-ray source 1E 1547.0-5408 was identified by Gelfand & Gaensler
(2007) as a likely magnetar in G327.24-0.13, an apparent supernova remnant. No
X-ray pulsations have been detected from it. Using the Parkes radio telescope,
we discovered pulsations with period P = 2.069 s. Using the Australia Telescope
Co... | astro-ph | the variable xray source 1e 154705408 was identified by gelfand gaensler 2007 as a likely magnetar in g32724013 an apparent supernova remnant no xray pulsations have been detected from it using the parkes radio telescope we discovered pulsations with period p 2069 s using the australia telescope compact array we locali... | [['the', 'variable', 'xray', 'source', '1e', '154705408', 'was', 'identified', 'by', 'gelfand', 'gaensler', '2007', 'as', 'a', 'likely', 'magnetar', 'in', 'g32724013', 'an', 'apparent', 'supernova', 'remnant', 'no', 'xray', 'pulsations', 'have', 'been', 'detected', 'from', 'it', 'using', 'the', 'parkes', 'radio', 'tele... | [-0.12857180991085004, 0.1624470908303111, -0.05132267843776693, 0.10215425175847485, -0.137541436607501, -0.12350154381969737, 0.0881274473172164, 0.4711372423356537, -0.15021454623611472, -0.3556319298037259, 0.1198087782840486, -0.30634860922582446, -0.015646138405254868, 0.2590662337089371, -0.03482053592300939, -0... |
708.0003 | One-dimensional quantum wires: A pedestrian approach to bosonization | In these lecture notes we will consider systems in which the motion of
electrons is confined to one dimension (1D). In these so-called quantum wires
electron-electron interaction effects play an important role because the
restricted dimensions enhance the scattering between the electrons and
completely destroy the qu... | cond-mat.str-el | in these lecture notes we will consider systems in which the motion of electrons is confined to one dimension 1d in these socalled quantum wires electronelectron interaction effects play an important role because the restricted dimensions enhance the scattering between the electrons and completely destroy the quasipart... | [['in', 'these', 'lecture', 'notes', 'we', 'will', 'consider', 'systems', 'in', 'which', 'the', 'motion', 'of', 'electrons', 'is', 'confined', 'to', 'one', 'dimension', '1d', 'in', 'these', 'socalled', 'quantum', 'wires', 'electronelectron', 'interaction', 'effects', 'play', 'an', 'important', 'role', 'because', 'the',... | [-0.11027150317000187, 0.21409431079593225, -0.08633712333465489, 0.10068568696279188, -0.062226800502239894, -0.16756783228139488, 0.0015047290754428475, 0.31827740741855637, -0.20653164866784282, -0.26649845965510727, 0.02602679948607574, -0.26399438862441754, -0.17633456318658225, 0.15243208441617234, -0.03355726840... |
708.0004 | The DEEP2 Galaxy Redshift Survey: Color and Luminosity Dependence of
Galaxy Clustering at z~1 | We present measurements of the color and luminosity dependence of galaxy
clustering at z~1 in the DEEP2 Galaxy Redshift Survey. Using volume-limited
subsamples in bins of both color and luminosity, we find that: 1) The
clustering dependence is much stronger with color than with luminosity and is
as strong with color ... | astro-ph | we present measurements of the color and luminosity dependence of galaxy clustering at z1 in the deep2 galaxy redshift survey using volumelimited subsamples in bins of both color and luminosity we find that 1 the clustering dependence is much stronger with color than with luminosity and is as strong with color at z1 as... | [['we', 'present', 'measurements', 'of', 'the', 'color', 'and', 'luminosity', 'dependence', 'of', 'galaxy', 'clustering', 'at', 'z1', 'in', 'the', 'deep2', 'galaxy', 'redshift', 'survey', 'using', 'volumelimited', 'subsamples', 'in', 'bins', 'of', 'both', 'color', 'and', 'luminosity', 'we', 'find', 'that', '1', 'the', ... | [-0.022309235313588745, 0.09443963596728876, -0.11595970617960377, 0.14594743021402065, -0.0977751588326408, -0.0456342867014715, -0.002558396550239026, 0.501972319918328, -0.09993089965049551, -0.33551402330800173, -0.00015178634257135448, -0.31912567762988636, -0.031507526011964423, 0.1738513823612472, -0.01612357814... |
708.0005 | Colored Unparticles | We examine a scenario where the new physics at the LHC includes an
approximate conformal field theory, where some of the degrees of freedom (aka
"unparticles") carry a color charge. We present a simple argument showing that
the production cross section for scalar unparticles mediated by a gauge
interaction is given b... | hep-ph | we examine a scenario where the new physics at the lhc includes an approximate conformal field theory where some of the degrees of freedom aka unparticles carry a color charge we present a simple argument showing that the production cross section for scalar unparticles mediated by a gauge interaction is given by 2d tim... | [['we', 'examine', 'a', 'scenario', 'where', 'the', 'new', 'physics', 'at', 'the', 'lhc', 'includes', 'an', 'approximate', 'conformal', 'field', 'theory', 'where', 'some', 'of', 'the', 'degrees', 'of', 'freedom', 'aka', 'unparticles', 'carry', 'a', 'color', 'charge', 'we', 'present', 'a', 'simple', 'argument', 'showing... | [-0.15244510269753556, 0.22259000392938455, -0.08451660316774344, 0.11873285188609403, -0.0892315288916468, -0.1655143615492481, 0.02804356511617872, 0.2751710174129681, -0.20692997772563645, -0.2478737065548751, -0.02314435690146019, -0.27918306337867643, -0.16038856833697634, 0.10167710743274817, 0.042129446583938725... |
708.0006 | Lyman-alpha Emitters During the Early Stages of Reionization | We investigate the potential of exploiting Lya Emitters (LAEs) to constrain
the volume-weighted mean neutral hydrogen fraction of the IGM, x_H, at high
redshifts (specifically z~9). We use "semi-numerical'' simulations to
efficiently generate density, velocity, and halo fields at z=9 in a 250 Mpc
box, resolving halos... | astro-ph | we investigate the potential of exploiting lya emitters laes to constrain the volumeweighted mean neutral hydrogen fraction of the igm x_h at high redshifts specifically z9 we use seminumerical simulations to efficiently generate density velocity and halo fields at z9 in a 250 mpc box resolving halos with masses m22e8 ... | [['we', 'investigate', 'the', 'potential', 'of', 'exploiting', 'lya', 'emitters', 'laes', 'to', 'constrain', 'the', 'volumeweighted', 'mean', 'neutral', 'hydrogen', 'fraction', 'of', 'the', 'igm', 'x_h', 'at', 'high', 'redshifts', 'specifically', 'z9', 'we', 'use', 'seminumerical', 'simulations', 'to', 'efficiently', '... | [-0.03742694097810247, 0.12425669037477849, -0.04240397005142637, 0.13374642405028414, -0.07930814615606624, -0.06645311736266205, 0.03242130586442606, 0.425634280586405, -0.10714446444694924, -0.3893266914209445, 0.0018836347364045041, -0.2889907137610395, -0.021737333184202356, 0.1819675452889447, 0.02076292421726749... |
708.0007 | The Sightline to Q2343-BX415: Clues to Galaxy Formation in a Quasar
Environment | (Abridged) We have discovered a strong DLA coincident in redshift with the
faint QSO Q2343-BX415 (R = 20.2, z_em = 2.57393). Follow-up observations at
intermediate spectral resolution reveal that the metal lines associated with
this 'proximate' DLA consist of two sets of absorption components. One set is
moving towar... | astro-ph | abridged we have discovered a strong dla coincident in redshift with the faint qso q2343bx415 r 202 z_em 257393 followup observations at intermediate spectral resolution reveal that the metal lines associated with this proximate dla consist of two sets of absorption components one set is moving towards the quasar with ... | [['abridged', 'we', 'have', 'discovered', 'a', 'strong', 'dla', 'coincident', 'in', 'redshift', 'with', 'the', 'faint', 'qso', 'q2343bx415', 'r', '202', 'z_em', '257393', 'followup', 'observations', 'at', 'intermediate', 'spectral', 'resolution', 'reveal', 'that', 'the', 'metal', 'lines', 'associated', 'with', 'this', ... | [-0.06684456905129606, 0.10542748002417009, -0.01642410707956349, 0.023056610860900644, -0.05744065008845858, -0.12595502229823702, 0.039122844908971194, 0.4491993887984956, -0.16457489489932248, -0.3076179568412375, 0.029638639070044243, -0.33647763417243504, 0.011410844907390348, 0.14587591607502845, -0.0030083309196... |
708.0008 | Ovrview: The Shape of Hadrons | In this article we address the physical basis of the deviation of hadron
shapes from spherical symmetry (non-spherical amplitudes) with focus on the
nucleon and $\Delta$. An overview of both the experimental methods and results
and the current theoretical understanding of the issue is presented. At the
present time t... | hep-ph hep-ex nucl-ex nucl-th | in this article we address the physical basis of the deviation of hadron shapes from spherical symmetry nonspherical amplitudes with focus on the nucleon and delta an overview of both the experimental methods and results and the current theoretical understanding of the issue is presented at the present time the most qu... | [['in', 'this', 'article', 'we', 'address', 'the', 'physical', 'basis', 'of', 'the', 'deviation', 'of', 'hadron', 'shapes', 'from', 'spherical', 'symmetry', 'nonspherical', 'amplitudes', 'with', 'focus', 'on', 'the', 'nucleon', 'and', 'delta', 'an', 'overview', 'of', 'both', 'the', 'experimental', 'methods', 'and', 're... | [-0.08536184705922951, 0.2016656768871621, -0.08075700964710081, 0.09840774489681947, -0.04947349891910274, -0.06549273872065663, 0.011664307374843755, 0.38210921090022465, -0.1897414586637031, -0.2949539665732127, -0.005511430221250151, -0.30416552823193665, -0.09018875330243961, 0.14675071477050902, 0.066811621128892... |
708.0009 | Functional relations from the Yang-Baxter algebra: Eigenvalues of the
XXZ model with non-diagonal twisted and open boundary conditions | In this work we consider a functional method in the theory of exactly
solvable models based on the Yang-Baxter algebra. Using this method we derive
the eigenvalues of the XXZ model with non-diagonal twisted and open boundary
conditions for general values of the anisotropy and boundary parameters.
| nlin.SI | in this work we consider a functional method in the theory of exactly solvable models based on the yangbaxter algebra using this method we derive the eigenvalues of the xxz model with nondiagonal twisted and open boundary conditions for general values of the anisotropy and boundary parameters | [['in', 'this', 'work', 'we', 'consider', 'a', 'functional', 'method', 'in', 'the', 'theory', 'of', 'exactly', 'solvable', 'models', 'based', 'on', 'the', 'yangbaxter', 'algebra', 'using', 'this', 'method', 'we', 'derive', 'the', 'eigenvalues', 'of', 'the', 'xxz', 'model', 'with', 'nondiagonal', 'twisted', 'and', 'open... | [-0.11996058429135605, 0.07381975543784335, -0.05513359511152227, 0.027758763840501296, -0.06354191823505816, -0.1625829133641054, -0.009518247565868845, 0.3439937549385619, -0.2657608603711854, -0.25628529298812786, 0.11883780114015842, -0.21801778761313317, -0.17641937027269222, 0.17802979509801942, -0.01099538850657... |
708.001 | Velocity Dispersion Profiles of Seven Dwarf Spheroidal Galaxies | We present stellar velocity dispersion profiles for seven Milky Way dwarf
spheroidal (dSph) satellite galaxies. We have measured 8394 line-of-sight
velocities (+/- 2.5 km/s) for 6804 stars from high-resolution spectra obtained
at the Magellan and MMT telescopes. We combine these new data with previously
published vel... | astro-ph | we present stellar velocity dispersion profiles for seven milky way dwarf spheroidal dsph satellite galaxies we have measured 8394 lineofsight velocities 25 kms for 6804 stars from highresolution spectra obtained at the magellan and mmt telescopes we combine these new data with previously published velocities to obtain... | [['we', 'present', 'stellar', 'velocity', 'dispersion', 'profiles', 'for', 'seven', 'milky', 'way', 'dwarf', 'spheroidal', 'dsph', 'satellite', 'galaxies', 'we', 'have', 'measured', '8394', 'lineofsight', 'velocities', '25', 'kms', 'for', '6804', 'stars', 'from', 'highresolution', 'spectra', 'obtained', 'at', 'the', 'm... | [-0.05656446562147138, 0.07774704101626785, -0.11017761102770098, 0.09890658254675472, -0.111753448124569, -0.05499550135125621, 0.037275389389087185, 0.42060667508019084, -0.1163013246632778, -0.44639445177148074, -0.01943098239149922, -0.34457402512765467, 0.06332793675261573, 0.23422372621970658, -0.0096213750226664... |
708.0011 | An Extremely Massive Dry Galaxy Merger in a Moderate Redshift Cluster | We have identified perhaps the largest major galaxy merger ever seen. While
analysing Spitzer IRAC images of CL0958+4702, an X-ray selected cluster at
z=0.39, we discovered an unusual plume of stars extending $\gtrsim$110 kpc
outward from the bright central galaxy (BCG). Three galaxies 1-1.5 mag fainter
than the BCG ... | astro-ph | we have identified perhaps the largest major galaxy merger ever seen while analysing spitzer irac images of cl09584702 an xray selected cluster at z039 we discovered an unusual plume of stars extending gtrsim110 kpc outward from the bright central galaxy bcg three galaxies 115 mag fainter than the bcg lie within 17 kpc... | [['we', 'have', 'identified', 'perhaps', 'the', 'largest', 'major', 'galaxy', 'merger', 'ever', 'seen', 'while', 'analysing', 'spitzer', 'irac', 'images', 'of', 'cl09584702', 'an', 'xray', 'selected', 'cluster', 'at', 'z039', 'we', 'discovered', 'an', 'unusual', 'plume', 'of', 'stars', 'extending', 'gtrsim110', 'kpc', ... | [-0.052459511377899344, 0.11445020669022776, -0.08939363593313547, 0.10234658004449111, -0.09499882514759991, -0.01906986280137899, 0.02613274488054025, 0.48431719264413026, -0.1175192108506407, -0.3317243826641822, 0.046475536670247446, -0.35574803058550963, 0.011127430002622027, 0.20478620711289283, -0.04786808078606... |
708.0012 | The quantum vs classical aspects of one dimensional electron-phonon
systems revisited by the renormalization group method | An extension of the renormalization group method that includes the effect of
retardation for the interactions of a fermion gas is used to re-examine the
quantum and classical properties of Peierls- like states in one dimension. For
models of spinless and spin-1/2 fermions interacting with either intra or
intermolecul... | cond-mat.str-el cond-mat.stat-mech | an extension of the renormalization group method that includes the effect of retardation for the interactions of a fermion gas is used to reexamine the quantum and classical properties of peierls like states in one dimension for models of spinless and spin12 fermions interacting with either intra or intermolecular phon... | [['an', 'extension', 'of', 'the', 'renormalization', 'group', 'method', 'that', 'includes', 'the', 'effect', 'of', 'retardation', 'for', 'the', 'interactions', 'of', 'a', 'fermion', 'gas', 'is', 'used', 'to', 'reexamine', 'the', 'quantum', 'and', 'classical', 'properties', 'of', 'peierls', 'like', 'states', 'in', 'one'... | [-0.16689355393949276, 0.25256393221226364, -0.05640704247246807, 0.09577756320747237, -0.035196246771762765, -0.17670531808088222, 0.051154312705621124, 0.3347430343925953, -0.25869318151225645, -0.20494086912833154, -0.03041863003280014, -0.3380086958532532, -0.08662778379706045, 0.13336548568991324, 0.09458712783021... |
708.0013 | Beltrami States for Compressible Barotropic Flows | Beltrami states for compressible barotropic flows are deduced by minimizing
the total kinetic energy while keeping the total helicity constant. A
Hamiltonian basis for these Beltrami states is also sketched.
| physics.flu-dyn | beltrami states for compressible barotropic flows are deduced by minimizing the total kinetic energy while keeping the total helicity constant a hamiltonian basis for these beltrami states is also sketched | [['beltrami', 'states', 'for', 'compressible', 'barotropic', 'flows', 'are', 'deduced', 'by', 'minimizing', 'the', 'total', 'kinetic', 'energy', 'while', 'keeping', 'the', 'total', 'helicity', 'constant', 'a', 'hamiltonian', 'basis', 'for', 'these', 'beltrami', 'states', 'is', 'also', 'sketched']] | [-0.21408353025714558, 0.2746707226615399, -0.003677645993108551, 0.12183790761434163, -0.06416148844485482, -0.1028069423045963, -0.06625002504636844, 0.22960758196810882, -0.2894263649980227, -0.3386864231278499, 0.03079195637255907, -0.2722639667491118, 0.025204891338944435, 0.16437395876273514, 0.021286524242411058... |
708.0014 | Cover slip external cavity diode laser | The design of a 671 nm diode laser with a mode-hop-free tuning range of 40
GHz is described. This long tuning range is achieved by simultaneously ramping
the external cavity length with the laser injection current. The external
cavity consists of a microscope cover slip mounted on piezoelectric actuators.
In such a c... | physics.optics physics.atom-ph | the design of a 671 nm diode laser with a modehopfree tuning range of 40 ghz is described this long tuning range is achieved by simultaneously ramping the external cavity length with the laser injection current the external cavity consists of a microscope cover slip mounted on piezoelectric actuators in such a configur... | [['the', 'design', 'of', 'a', '671', 'nm', 'diode', 'laser', 'with', 'a', 'modehopfree', 'tuning', 'range', 'of', '40', 'ghz', 'is', 'described', 'this', 'long', 'tuning', 'range', 'is', 'achieved', 'by', 'simultaneously', 'ramping', 'the', 'external', 'cavity', 'length', 'with', 'the', 'laser', 'injection', 'current',... | [-0.14604994776132313, 0.1906698646743873, 0.016269592025681682, -0.10469763038740695, -0.046135144227224846, -0.2344001757112615, 0.06812694113721827, 0.5034352228045463, -0.23255558220629136, -0.3539663868267899, 0.05418616737259309, -0.22201212049745347, 0.009954200838894948, 0.29200336359765217, -0.0492879225953441... |
708.0015 | Is there a link between the neutron-star spin and the frequency of the
kilohertz quasi-periodic oscillations? | There is a general consensus that the frequencies of the kilohertz
Quasi-Periodic Oscillations (kHz QPOs) in neutron-star low-mass X-ray binaries
are directly linked to the spin of the neutron star. The root of this idea is
the apparent clustering of the ratio of the frequency difference of the kHz
QPOs and the neutr... | astro-ph | there is a general consensus that the frequencies of the kilohertz quasiperiodic oscillations khz qpos in neutronstar lowmass xray binaries are directly linked to the spin of the neutron star the root of this idea is the apparent clustering of the ratio of the frequency difference of the khz qpos and the neutronstar sp... | [['there', 'is', 'a', 'general', 'consensus', 'that', 'the', 'frequencies', 'of', 'the', 'kilohertz', 'quasiperiodic', 'oscillations', 'khz', 'qpos', 'in', 'neutronstar', 'lowmass', 'xray', 'binaries', 'are', 'directly', 'linked', 'to', 'the', 'spin', 'of', 'the', 'neutron', 'star', 'the', 'root', 'of', 'this', 'idea',... | [-0.14772252668244917, 0.21650739414159392, -0.009757695654712495, 0.09075555867958264, -0.10473503862110684, -0.09278017357297119, 0.0838480987662419, 0.38020721186318845, -0.21116636696531146, -0.3111786898111039, 0.1321485629123941, -0.29077529478207476, -0.04135797695508685, 0.2742536518050999, -0.00268061976253864... |
708.0016 | Nearing the Horizon of a Heterotic String | It is argued that recent developments point to the existence of an AdS_3 x
S^2 x T^5 holographic dual for the 2D CFT living on the worldsheet of N
coincident heterotic strings in a T^5 compactification, which can in turn be
described by an exact worldsheet CFT. A supergravity analysis is shown to imply
that the globa... | hep-th | it is argued that recent developments point to the existence of an ads_3 x s2 x t5 holographic dual for the 2d cft living on the worldsheet of n coincident heterotic strings in a t5 compactification which can in turn be described by an exact worldsheet cft a supergravity analysis is shown to imply that the global super... | [['it', 'is', 'argued', 'that', 'recent', 'developments', 'point', 'to', 'the', 'existence', 'of', 'an', 'ads_3', 'x', 's2', 'x', 't5', 'holographic', 'dual', 'for', 'the', '2d', 'cft', 'living', 'on', 'the', 'worldsheet', 'of', 'n', 'coincident', 'heterotic', 'strings', 'in', 'a', 't5', 'compactification', 'which', 'c... | [-0.12948465580871749, 0.1259839758319187, -0.06793335539236244, 0.07314273445761853, -0.09707768824231881, -0.20388275591696622, -0.06425854941249214, 0.31850583808776994, -0.15560250988190052, -0.22224033527296558, 0.12302409947889867, -0.3235722937976681, -0.1723647521012613, 0.13018188155907137, -0.1235661996223072... |
708.0017 | Greybody Factors for d-Dimensional Black Holes | Gravitational greybody factors are analytically computed for static,
spherically symmetric black holes in d-dimensions, including black holes with
charge and in the presence of a cosmological constant (where a proper
definition of greybody factors for both asymptotically dS and AdS spacetimes is
provided). This calcu... | hep-th astro-ph gr-qc hep-ph | gravitational greybody factors are analytically computed for static spherically symmetric black holes in ddimensions including black holes with charge and in the presence of a cosmological constant where a proper definition of greybody factors for both asymptotically ds and ads spacetimes is provided this calculation i... | [['gravitational', 'greybody', 'factors', 'are', 'analytically', 'computed', 'for', 'static', 'spherically', 'symmetric', 'black', 'holes', 'in', 'ddimensions', 'including', 'black', 'holes', 'with', 'charge', 'and', 'in', 'the', 'presence', 'of', 'a', 'cosmological', 'constant', 'where', 'a', 'proper', 'definition', '... | [-0.14484835973013008, 0.13643233849270403, -0.035036645035131944, 0.0969744194839008, -0.06817222407137259, -0.173187600047471, 0.00954535379545487, 0.3147863571358554, -0.14104869805219736, -0.25799247770155903, 0.12339238259240191, -0.31298676936421543, -0.10674582770494426, 0.18445275508012524, 0.015480840913424651... |
708.0018 | q-Terms, singularities and the extended Bloch group | Our paper originated from a generalization of the Volume Conjecture to
multisums of $q$-hypergeometric terms. This generalization was sketched by
Kontsevich in a problem list in Aarhus University in 2006; \cite{Ko}. We
introduce the notion of a $q$-hypergeometric term (in short, $q$-term). The
latter is a product of ... | math.AG math.NT | our paper originated from a generalization of the volume conjecture to multisums of qhypergeometric terms this generalization was sketched by kontsevich in a problem list in aarhus university in 2006 citeko we introduce the notion of a qhypergeometric term in short qterm the latter is a product of ratios of qfactorials... | [['our', 'paper', 'originated', 'from', 'a', 'generalization', 'of', 'the', 'volume', 'conjecture', 'to', 'multisums', 'of', 'qhypergeometric', 'terms', 'this', 'generalization', 'was', 'sketched', 'by', 'kontsevich', 'in', 'a', 'problem', 'list', 'in', 'aarhus', 'university', 'in', '2006', 'citeko', 'we', 'introduce',... | [-0.1614603779903662, 0.07274366983114497, -0.09601460801633566, 0.054632787865978714, -0.059434441423141644, -0.052812253669100376, 0.028005660069175063, 0.2828189773742404, -0.29864714840292245, -0.24666472403822762, 0.10807353490412137, -0.244828137136861, -0.19494161911823443, 0.20007261782762056, -0.13296874202052... |
708.0019 | Semigroups of valuations on local rings | In this paper the question of which semigroups are realizable as the
semigroup of values attained on a Noetherian local ring which is dominated by a
valuation is considered. We give some striking examples, indicating that there
may be no constraints on the semigroup beyond those known classically.
| math.AG math.AC | in this paper the question of which semigroups are realizable as the semigroup of values attained on a noetherian local ring which is dominated by a valuation is considered we give some striking examples indicating that there may be no constraints on the semigroup beyond those known classically | [['in', 'this', 'paper', 'the', 'question', 'of', 'which', 'semigroups', 'are', 'realizable', 'as', 'the', 'semigroup', 'of', 'values', 'attained', 'on', 'a', 'noetherian', 'local', 'ring', 'which', 'is', 'dominated', 'by', 'a', 'valuation', 'is', 'considered', 'we', 'give', 'some', 'striking', 'examples', 'indicating'... | [-0.1422493018132324, 0.09320391439056645, -0.05895453093883892, 0.12490108012813532, -0.0661685654389051, -0.1609791203130347, -0.0020301881959312595, 0.3492512969921033, -0.33510162386422354, -0.20057531694571176, 0.1658280037008808, -0.26207666902337223, -0.11783503030892462, 0.2938606753014028, -0.11339672732477386... |
708.002 | Spin solitons in magnetized pair plasmas | A set of fluid equations, taking into account the spin properties of the
electrons and positrons in a magnetoplasma, are derived. The
magnetohydrodynamic limit of the pair plasma is investigated. It is shown that
the microscopic spin properties of the electrons and positrons can lead to
interesting macroscopic and co... | physics.plasm-ph astro-ph | a set of fluid equations taking into account the spin properties of the electrons and positrons in a magnetoplasma are derived the magnetohydrodynamic limit of the pair plasma is investigated it is shown that the microscopic spin properties of the electrons and positrons can lead to interesting macroscopic and collecti... | [['a', 'set', 'of', 'fluid', 'equations', 'taking', 'into', 'account', 'the', 'spin', 'properties', 'of', 'the', 'electrons', 'and', 'positrons', 'in', 'a', 'magnetoplasma', 'are', 'derived', 'the', 'magnetohydrodynamic', 'limit', 'of', 'the', 'pair', 'plasma', 'is', 'investigated', 'it', 'is', 'shown', 'that', 'the', ... | [-0.15079058075697152, 0.2719855430388436, -0.0697255618132577, 0.12811929232205754, -0.07058137793803938, -0.09583160667080838, -0.08556152921916899, 0.31064982336973496, -0.2500230132574492, -0.23910152777513066, -0.0034622580405453793, -0.27912408883434414, -0.08173774486628942, 0.2536161598371397, 0.052184572019199... |
708.0021 | Protein-DNA interactions: reaching and recognizing the targets | This paper has been withdrawn because of the requirement from the journal
where the modified version of the paper is to be published.
| cond-mat.soft cond-mat.stat-mech | this paper has been withdrawn because of the requirement from the journal where the modified version of the paper is to be published | [['this', 'paper', 'has', 'been', 'withdrawn', 'because', 'of', 'the', 'requirement', 'from', 'the', 'journal', 'where', 'the', 'modified', 'version', 'of', 'the', 'paper', 'is', 'to', 'be', 'published']] | [-0.020126074876474297, -0.00424065404450116, -0.12288143680147502, -0.07726040466324142, -0.14474386298705055, -0.06077107123058775, -0.025060818196557786, 0.24522391212699207, -0.28806388529989385, -0.3779940365449242, 0.13617825402837733, -0.2721879079978427, -0.1458855639819218, 0.1430038990371901, -0.2339453081721... |
708.0022 | Embedding the Pentagon | The Pentagon Model is an explicit supersymmetric extension of the Standard
Model, which involves a new strongly-interacting SU(5) gauge theory at
TeV-scale energies. We show that the Pentagon can be embedded into an SU(5) x
SU(5) x SU(5) gauge group at the GUT scale. The doublet-triplet splitting
problem, and proton ... | hep-th hep-ph | the pentagon model is an explicit supersymmetric extension of the standard model which involves a new stronglyinteracting su5 gauge theory at tevscale energies we show that the pentagon can be embedded into an su5 x su5 x su5 gauge group at the gut scale the doublettriplet splitting problem and proton decay compatible ... | [['the', 'pentagon', 'model', 'is', 'an', 'explicit', 'supersymmetric', 'extension', 'of', 'the', 'standard', 'model', 'which', 'involves', 'a', 'new', 'stronglyinteracting', 'su5', 'gauge', 'theory', 'at', 'tevscale', 'energies', 'we', 'show', 'that', 'the', 'pentagon', 'can', 'be', 'embedded', 'into', 'an', 'su5', 'x... | [-0.08080940808952047, 0.24452323979171853, -0.05650479393079877, 0.17385132421532973, -0.09273781739991427, -0.16562774814317271, -0.01871129309340889, 0.3602419924759066, -0.23389742453822615, -0.30568521124185977, 0.035386341377929544, -0.21182531059345172, -0.04837777338845214, 0.10147565317618631, -0.0140603296626... |
708.0023 | Renormalized spin wave excitations in the antiferromagnetic
Heisenberg-Kondo model for heavy fermions | Recent inelastic neutron scattering experiments in CeIn3 and CePd2Si2 single
crystals, measured spin wave excitations at low temperatures. These two heavy
fermion compounds exhibit antiferromagnetic long-range order, but a strong
competition between the Ruderman-Kittel-Kasuya-Yosida(RKKY) interaction and
Kondo effect... | cond-mat.str-el | recent inelastic neutron scattering experiments in cein3 and cepd2si2 single crystals measured spin wave excitations at low temperatures these two heavy fermion compounds exhibit antiferromagnetic longrange order but a strong competition between the rudermankittelkasuyayosidarkky interaction and kondo effect is evidenc... | [['recent', 'inelastic', 'neutron', 'scattering', 'experiments', 'in', 'cein3', 'and', 'cepd2si2', 'single', 'crystals', 'measured', 'spin', 'wave', 'excitations', 'at', 'low', 'temperatures', 'these', 'two', 'heavy', 'fermion', 'compounds', 'exhibit', 'antiferromagnetic', 'longrange', 'order', 'but', 'a', 'strong', 'c... | [-0.16567342973505267, 0.27944535656282915, -0.018356634420939745, 0.0946098561386745, -0.0266314549670101, -0.16426575877823127, 0.07631960609235251, 0.36979222187700755, -0.23767142159124025, -0.2707371210727172, -0.034688865140271495, -0.4010970949553526, -0.09087010173974798, 0.1399328742821056, 0.1451307077581684,... |
708.0024 | The Mirage of w=-1 | We demonstrate that cosmic microwave background observations consistent with
a cosmological constant universe predict in a well-defined sense that lower
redshift measures will nearly automatically deliver w=-1 for the dark energy
equation of state value unless they are sensitive to w(z). Thus low redshift
data pointi... | astro-ph | we demonstrate that cosmic microwave background observations consistent with a cosmological constant universe predict in a welldefined sense that lower redshift measures will nearly automatically deliver w1 for the dark energy equation of state value unless they are sensitive to wz thus low redshift data pointing to w1... | [['we', 'demonstrate', 'that', 'cosmic', 'microwave', 'background', 'observations', 'consistent', 'with', 'a', 'cosmological', 'constant', 'universe', 'predict', 'in', 'a', 'welldefined', 'sense', 'that', 'lower', 'redshift', 'measures', 'will', 'nearly', 'automatically', 'deliver', 'w1', 'for', 'the', 'dark', 'energy'... | [-0.11372452089265099, 0.14232697002003042, -0.10173223115591787, 0.11776135299596789, -0.16863274064802336, -0.17697591592345063, 0.0430654785247505, 0.3603306829885352, -0.2284692453264486, -0.33566562403140104, 0.06483424296804272, -0.2524176231974105, -0.02908822492967675, 0.1897844968282977, -0.031005427681320294,... |
708.0025 | Goal-oriented Atomistic-Continuum Adaptivity for the Quasicontinuum
Approximation | We give a goal-oriented a posteriori error estimator for the
atomistic-continuum modeling error in the quasicontinuum method, and we use
this estimator to design an adaptive algorithm to compute a quantity of
interest to a given tolerance by using a nearly minimal number of atomistic
degrees of freedom. We present co... | math.NA math-ph math.MP | we give a goaloriented a posteriori error estimator for the atomisticcontinuum modeling error in the quasicontinuum method and we use this estimator to design an adaptive algorithm to compute a quantity of interest to a given tolerance by using a nearly minimal number of atomistic degrees of freedom we present computat... | [['we', 'give', 'a', 'goaloriented', 'a', 'posteriori', 'error', 'estimator', 'for', 'the', 'atomisticcontinuum', 'modeling', 'error', 'in', 'the', 'quasicontinuum', 'method', 'and', 'we', 'use', 'this', 'estimator', 'to', 'design', 'an', 'adaptive', 'algorithm', 'to', 'compute', 'a', 'quantity', 'of', 'interest', 'to'... | [-0.11533375816341017, -0.0005180500429304002, -0.08500077425908874, 0.016174604399720023, -0.03000243919783495, -0.12004975630232775, 0.10055950277117671, 0.3881712420318853, -0.24502337375052377, -0.31970874157170176, 0.09431462964325041, -0.19896488193370088, -0.21289795240990714, 0.20003555606539086, -0.10871123235... |
708.0026 | CP Asymmetry in Charged Higgs Decays to Chargino-Neutralino | We analyze the charge-parity (CP) asymmetry in the charged Higgs boson decays
to chargino-neutralino pairs, H^- -> chargino_i + neutralino_j. We show first
that these modes have a large branching ratio for m_H^- > 600 GeV. We use
Cutkosky rules to obtain the analytical formulas needed for the evaluation of
the asymme... | hep-ph | we analyze the chargeparity cp asymmetry in the charged higgs boson decays to charginoneutralino pairs h chargino_i neutralino_j we show first that these modes have a large branching ratio for m_h 600 gev we use cutkosky rules to obtain the analytical formulas needed for the evaluation of the asymmetry under considerat... | [['we', 'analyze', 'the', 'chargeparity', 'cp', 'asymmetry', 'in', 'the', 'charged', 'higgs', 'boson', 'decays', 'to', 'charginoneutralino', 'pairs', 'h', 'chargino_i', 'neutralino_j', 'we', 'show', 'first', 'that', 'these', 'modes', 'have', 'a', 'large', 'branching', 'ratio', 'for', 'm_h', '600', 'gev', 'we', 'use', '... | [-0.12099496842800783, 0.2102763084623103, -0.02120256982385539, 0.1565782960334148, -0.06736119302132955, -0.14645861274419494, 0.0974536133876357, 0.29691961176980003, -0.23124698537330216, -0.3078110510411744, 0.03329063655110076, -0.28504332132937493, -0.0021973687403190594, 0.1254751544087552, 0.0771093696468877, ... |
708.0027 | The ACS Survey of Galactic Globular Clusters: M54 and Young Populations
in the Sagittarius Dwarf Spheroidal Galaxy | We present new Hubble Space Telescope photometry of the massive globular
cluster M54 (NGC 6715) and the superposed core of the tidally disrupted
Sagittarius (Sgr) dSph galaxy as part of the ACS Survey of Galactic Globular
Clusters. Our deep (F606W~26.5), high-precision photometry yields an
unprecedentedly detailed co... | astro-ph | we present new hubble space telescope photometry of the massive globular cluster m54 ngc 6715 and the superposed core of the tidally disrupted sagittarius sgr dsph galaxy as part of the acs survey of galactic globular clusters our deep f606w265 highprecision photometry yields an unprecedentedly detailed colormagnitude ... | [['we', 'present', 'new', 'hubble', 'space', 'telescope', 'photometry', 'of', 'the', 'massive', 'globular', 'cluster', 'm54', 'ngc', '6715', 'and', 'the', 'superposed', 'core', 'of', 'the', 'tidally', 'disrupted', 'sagittarius', 'sgr', 'dsph', 'galaxy', 'as', 'part', 'of', 'the', 'acs', 'survey', 'of', 'galactic', 'glo... | [-0.05174636827963455, 0.0826754710723545, -0.1258152942748863, 0.11857207210166482, -0.1338594948564615, -0.044182961783627725, 0.09763135713816794, 0.429557480780244, -0.14245379503508057, -0.3890115158750092, 0.0014276888341755495, -0.2768364531866909, -0.028273320214433986, 0.20886560460964504, -0.1018186942981249,... |
708.0028 | High-pressure x-ray diffraction study of SrMoO4 and pressure-induced
structural changes | SrMoO4 was studied under compression up to 25 GPa by angle-dispersive x-ray
diffraction. A phase transition was observed from the scheelite-structured
ambient phase to a monoclinic fergusonite phase at 12.2(9) GPa with cell
parameters a = 5.265(9) A, b = 11.191(9) A, c = 5.195 (5) A, and beta = 90.9, Z
= 4 at 13.1 GP... | cond-mat.mtrl-sci | srmoo4 was studied under compression up to 25 gpa by angledispersive xray diffraction a phase transition was observed from the scheelitestructured ambient phase to a monoclinic fergusonite phase at 1229 gpa with cell parameters a 52659 a b 111919 a c 5195 5 a and beta 909 z 4 at 131 gpa there is no significant volume c... | [['srmoo4', 'was', 'studied', 'under', 'compression', 'up', 'to', '25', 'gpa', 'by', 'angledispersive', 'xray', 'diffraction', 'a', 'phase', 'transition', 'was', 'observed', 'from', 'the', 'scheelitestructured', 'ambient', 'phase', 'to', 'a', 'monoclinic', 'fergusonite', 'phase', 'at', '1229', 'gpa', 'with', 'cell', 'p... | [-0.1443503940138006, 0.2099357352940583, -0.05858786541545775, -0.0002853290007901064, -0.017920014514170725, -0.10124042405649746, 0.12900105649619678, 0.4130572784074976, -0.232778697420323, -0.2741388671751494, 0.07984375805191216, -0.3043988594111124, -0.13141279286480698, 0.1166486850142639, 0.0438702385801182, 0... |
708.0029 | Collective modes of CP(3) Skyrmion crystals in quantum Hall ferromagnets | The two-dimensional electron gas in a bilayer quantum Hall system can sustain
an interlayer coherence at filling factor nu=1 even in the absence of tunneling
between the layers. This system has low-energy charged excitations which may
carry textures in real spin or pseudospin. Away from filling factor nu =1 a
finite ... | cond-mat.mes-hall | the twodimensional electron gas in a bilayer quantum hall system can sustain an interlayer coherence at filling factor nu1 even in the absence of tunneling between the layers this system has lowenergy charged excitations which may carry textures in real spin or pseudospin away from filling factor nu 1 a finite density ... | [['the', 'twodimensional', 'electron', 'gas', 'in', 'a', 'bilayer', 'quantum', 'hall', 'system', 'can', 'sustain', 'an', 'interlayer', 'coherence', 'at', 'filling', 'factor', 'nu1', 'even', 'in', 'the', 'absence', 'of', 'tunneling', 'between', 'the', 'layers', 'this', 'system', 'has', 'lowenergy', 'charged', 'excitatio... | [-0.21565676164653327, 0.264831486941481, -0.05980833359120161, -0.0033384616565296558, -0.044919409647338676, -0.15849347813859765, 0.06978780589039618, 0.35644066117995193, -0.2383282018934162, -0.24892024872364638, 0.006930524585366157, -0.2952011815605708, -0.07221245401109656, 0.11025356011965347, 0.07017275925012... |
708.003 | A Galaxy Photometric Redshift Catalog for the Sloan Digital Sky Survey
Data Release 6 | We present and describe a catalog of galaxy photometric redshifts (photo-z's)
for the Sloan Digital Sky Survey (SDSS) Data Release 6 (DR6). We use the
Artificial Neural Network (ANN) technique to calculate photo-z's and the
Nearest Neighbor Error (NNE) method to estimate photo-z errors for ~ 77 million
objects classi... | astro-ph | we present and describe a catalog of galaxy photometric redshifts photozs for the sloan digital sky survey sdss data release 6 dr6 we use the artificial neural network ann technique to calculate photozs and the nearest neighbor error nne method to estimate photoz errors for 77 million objects classified as galaxies in ... | [['we', 'present', 'and', 'describe', 'a', 'catalog', 'of', 'galaxy', 'photometric', 'redshifts', 'photozs', 'for', 'the', 'sloan', 'digital', 'sky', 'survey', 'sdss', 'data', 'release', '6', 'dr6', 'we', 'use', 'the', 'artificial', 'neural', 'network', 'ann', 'technique', 'to', 'calculate', 'photozs', 'and', 'the', 'n... | [0.0038063184759260095, -0.06857319301619691, -0.03381883153941714, 0.12764134706698194, -0.11856965901479669, -0.09882116430595408, 0.1194628859533636, 0.4768020624938985, -0.08524449957521076, -0.3836446529947711, 0.07137883831508947, -0.394574789123025, -0.02647904449450124, 0.2578535387547428, -0.04902573061060079,... |
708.0031 | Lensing Corrections to Features in the Angular Two-Point Correlation
Function and Power Spectrum | It is well known that magnification bias, the modulation of galaxy or quasar
source counts by gravitational lensing, can change the observed angular
correlation function. We investigate magnification-induced changes to the shape
of the observed correlation function w(\theta) and the angular power spectrum
C_{\ell}, p... | astro-ph | it is well known that magnification bias the modulation of galaxy or quasar source counts by gravitational lensing can change the observed angular correlation function we investigate magnificationinduced changes to the shape of the observed correlation function wtheta and the angular power spectrum c_ell paying special... | [['it', 'is', 'well', 'known', 'that', 'magnification', 'bias', 'the', 'modulation', 'of', 'galaxy', 'or', 'quasar', 'source', 'counts', 'by', 'gravitational', 'lensing', 'can', 'change', 'the', 'observed', 'angular', 'correlation', 'function', 'we', 'investigate', 'magnificationinduced', 'changes', 'to', 'the', 'shape... | [-0.08392631006511164, 0.1382246261178045, -0.06941048380000928, 0.14538700312429817, -0.09267585594391968, -0.10749194897553255, 0.019080713088708234, 0.3752165851771616, -0.23355639886509438, -0.37854935330446365, 0.047148241566927825, -0.32759980935795024, -0.018804147257049323, 0.18737815917361972, 0.01943940159928... |
708.0032 | Towards conformal invariance of 2D lattice models | Many 2D lattice models of physical phenomena are conjectured to have
conformally invariant scaling limits: percolation, Ising model, self-avoiding
polymers, ... This has led to numerous exact (but non-rigorous) predictions of
their scaling exponents and dimensions. We will discuss how to prove the
conformal invarianc... | math-ph math.CV math.MP math.PR | many 2d lattice models of physical phenomena are conjectured to have conformally invariant scaling limits percolation ising model selfavoiding polymers this has led to numerous exact but nonrigorous predictions of their scaling exponents and dimensions we will discuss how to prove the conformal invariance conjectures e... | [['many', '2d', 'lattice', 'models', 'of', 'physical', 'phenomena', 'are', 'conjectured', 'to', 'have', 'conformally', 'invariant', 'scaling', 'limits', 'percolation', 'ising', 'model', 'selfavoiding', 'polymers', 'this', 'has', 'led', 'to', 'numerous', 'exact', 'but', 'nonrigorous', 'predictions', 'of', 'their', 'scal... | [-0.12481027572671426, 0.19453253439974552, -0.14244249298730316, 0.12114372793539409, -0.10042053012305177, -0.2515598024223365, -0.019071403306488897, 0.38737579383293863, -0.22456902563206704, -0.2394642970506467, 0.08084609376622692, -0.2859661127166713, -0.20786390869019955, 0.14933192232788048, -0.035111734734884... |
708.0033 | Survey Requirements for Accurate and Precise Photometric Redshifts for
Type Ia Supernovae | In this paper we advance the simple analytic photometric redshift estimator
for Type Ia supernovae (SNe Ia) proposed by Wang (2007), and use it to study
simulated SN Ia data. We find that better than 0.5% accuracy in z_phot (with
RMS[(z_phot-z_spec)/(1+z_spec)]<0.005) is possible for SNe Ia with well sampled
lightcur... | astro-ph | in this paper we advance the simple analytic photometric redshift estimator for type ia supernovae sne ia proposed by wang 2007 and use it to study simulated sn ia data we find that better than 05 accuracy in z_phot with rmsz_photz_spec1z_spec0005 is possible for sne ia with well sampled lightcurves in three observed p... | [['in', 'this', 'paper', 'we', 'advance', 'the', 'simple', 'analytic', 'photometric', 'redshift', 'estimator', 'for', 'type', 'ia', 'supernovae', 'sne', 'ia', 'proposed', 'by', 'wang', '2007', 'and', 'use', 'it', 'to', 'study', 'simulated', 'sn', 'ia', 'data', 'we', 'find', 'that', 'better', 'than', '05', 'accuracy', '... | [-0.016645248631521323, 0.025783864846294975, -0.02613900878098736, 0.10688709033535287, -0.08166112897653179, -0.10099455487718921, 0.09907227888326793, 0.46384752364714205, -0.11769585258810332, -0.3598152828420064, 0.04634680258854649, -0.3456240569305661, -0.024130958855370588, 0.23935857800519622, -0.1168187607179... |
708.0034 | Analytic Formulation, Exact Solutions, and Generalizations of the
Elephant and the Alzheimer Random Walks | An analytic formulation of memory-possessing random walks introduced recently
[Cressoni et al., Phys. Rev. Lett. 98, 070603 (2007) and Sch\"utz and Trimper,
Phys. Rev. E 70, 045101 (2004)] for Alzheimer behavior and related phenomena is
provided along with exact solutions on the basis of Fokker-Planck equations.
The ... | cond-mat.stat-mech | an analytic formulation of memorypossessing random walks introduced recently cressoni et al phys rev lett 98 070603 2007 and schutz and trimper phys rev e 70 045101 2004 for alzheimer behavior and related phenomena is provided along with exact solutions on the basis of fokkerplanck equations the solution of a delaydiff... | [['an', 'analytic', 'formulation', 'of', 'memorypossessing', 'random', 'walks', 'introduced', 'recently', 'cressoni', 'et', 'al', 'phys', 'rev', 'lett', '98', '070603', '2007', 'and', 'schutz', 'and', 'trimper', 'phys', 'rev', 'e', '70', '045101', '2004', 'for', 'alzheimer', 'behavior', 'and', 'related', 'phenomena', '... | [-0.06599610926804883, 0.04994614137121527, -0.061871309458028254, -0.051115846054106046, -0.11221665627800109, -0.10074065693245246, 0.030449859775239375, 0.29761910695219185, -0.12752245224603428, -0.32207375905680946, -0.002674190418385878, -0.298706821052403, -0.23471711878096913, 0.27232984660147896, -0.1076010468... |
708.0035 | Polarization probes of vorticity in heavy ion collisions | We discuss the information that can be deduced from a measurement of particle
(hyperon or vector meson) polarization in ultrarelativistic nuclear collisions.
We describe the sensitivity of polarization to initial conditions, hydrodynamic
evolution and mean free path, and find that the polarization observable is
sensi... | nucl-th hep-ph nucl-ex | we discuss the information that can be deduced from a measurement of particle hyperon or vector meson polarization in ultrarelativistic nuclear collisions we describe the sensitivity of polarization to initial conditions hydrodynamic evolution and mean free path and find that the polarization observable is sensitive to... | [['we', 'discuss', 'the', 'information', 'that', 'can', 'be', 'deduced', 'from', 'a', 'measurement', 'of', 'particle', 'hyperon', 'or', 'vector', 'meson', 'polarization', 'in', 'ultrarelativistic', 'nuclear', 'collisions', 'we', 'describe', 'the', 'sensitivity', 'of', 'polarization', 'to', 'initial', 'conditions', 'hyd... | [-0.10909754541145437, 0.1968806775664364, -0.12301688470662546, 0.08191418838188318, -0.04716568101555042, -0.03843550348860195, -0.006613404226040335, 0.38616166692060816, -0.2845404836864743, -0.29128683449900045, 0.047720407321841254, -0.27160022797761485, -0.039507736836510175, 0.1637822903817323, 0.03686440820872... |
708.0036 | Unparticle Physics with Jets | Using methods of effective field theory, we show that after resummation of
Sudakov logarithms the spectral densities of interacting quark and gluon fields
in ordinary quantum field theories such as QCD are virtually indistinguishable
from those of "unparticles" of a hypothetical conformal sector coupled to the
Standa... | hep-ph | using methods of effective field theory we show that after resummation of sudakov logarithms the spectral densities of interacting quark and gluon fields in ordinary quantum field theories such as qcd are virtually indistinguishable from those of unparticles of a hypothetical conformal sector coupled to the standard mo... | [['using', 'methods', 'of', 'effective', 'field', 'theory', 'we', 'show', 'that', 'after', 'resummation', 'of', 'sudakov', 'logarithms', 'the', 'spectral', 'densities', 'of', 'interacting', 'quark', 'and', 'gluon', 'fields', 'in', 'ordinary', 'quantum', 'field', 'theories', 'such', 'as', 'qcd', 'are', 'virtually', 'ind... | [-0.06400452006608248, 0.2769586125639034, -0.13000013143857359, 0.1633042948629918, -0.06842675661609973, -0.1569656684086658, -0.026160772745497524, 0.2956928372196853, -0.21718163535930216, -0.30146464542485774, 0.019371349730063228, -0.2861426010727882, -0.12167736889095977, 0.13742826122324914, 0.01939013621304184... |
708.0037 | From the Einstein-Cartan to the Ashtekar-Barbero canonical constraints,
passing through the Nieh-Yan functional | The Ashtekar-Barbero constraints for General Relativity with fermions are
derived from the Einstein-Cartan canonical theory rescaling the state
functional of the gravity-spinor coupled system by the exponential of the
Nieh-Yan functional. A one parameter quantization ambiguity naturally appears
and can be associated ... | gr-qc | the ashtekarbarbero constraints for general relativity with fermions are derived from the einsteincartan canonical theory rescaling the state functional of the gravityspinor coupled system by the exponential of the niehyan functional a one parameter quantization ambiguity naturally appears and can be associated with th... | [['the', 'ashtekarbarbero', 'constraints', 'for', 'general', 'relativity', 'with', 'fermions', 'are', 'derived', 'from', 'the', 'einsteincartan', 'canonical', 'theory', 'rescaling', 'the', 'state', 'functional', 'of', 'the', 'gravityspinor', 'coupled', 'system', 'by', 'the', 'exponential', 'of', 'the', 'niehyan', 'func... | [-0.17420020959236557, 0.168354555633333, -0.13331965431571008, 0.08891568614376916, -0.12457644835942322, -0.17331946833162673, -0.001490965436419679, 0.20420688079773552, -0.29158858586516645, -0.3399256230228477, 0.04971181047666404, -0.2485678832564089, -0.15710138218063446, 0.10571734824528296, -0.0640257858360807... |
708.0038 | Tracking the Orbital and Super-orbital Periods of SMC X-1 | The High Mass X-ray Binary (HMXB) SMC X-1 demonstrates an orbital variation
of 3.89 days and a super-orbital variation with an average length of 55 days.
As we show here, however, the length of the super-orbital cycle varies by
almost a factor of two, even across adjacent cycles. To study both the orbital
and super-o... | astro-ph | the high mass xray binary hmxb smc x1 demonstrates an orbital variation of 389 days and a superorbital variation with an average length of 55 days as we show here however the length of the superorbital cycle varies by almost a factor of two even across adjacent cycles to study both the orbital and superorbital variatio... | [['the', 'high', 'mass', 'xray', 'binary', 'hmxb', 'smc', 'x1', 'demonstrates', 'an', 'orbital', 'variation', 'of', '389', 'days', 'and', 'a', 'superorbital', 'variation', 'with', 'an', 'average', 'length', 'of', '55', 'days', 'as', 'we', 'show', 'here', 'however', 'the', 'length', 'of', 'the', 'superorbital', 'cycle',... | [-0.17641187463252042, 0.11808036264682993, -0.1214457372063771, 0.0868233917077834, -0.07604404017921876, -0.11165985166518526, 0.11804056057283147, 0.4680101603151045, -0.23537172929129818, -0.35238668924366884, 0.1122282160568813, -0.2842976396400693, -0.12360032700933515, 0.22464038380506363, -0.0874508838948201, 0... |
708.0039 | Conformal invariance in random cluster models. I. Holomorphic fermions
in the Ising model | We construct discrete holomorphic observables in the Ising model at
criticality and show that they have conformally covariant scaling limits (as
mesh of the lattice tends to zero). In the sequel those observables are used to
construct conformally invariant scaling limits of interfaces. Though Ising
model is often cit... | math-ph math.MP math.PR | we construct discrete holomorphic observables in the ising model at criticality and show that they have conformally covariant scaling limits as mesh of the lattice tends to zero in the sequel those observables are used to construct conformally invariant scaling limits of interfaces though ising model is often cited as ... | [['we', 'construct', 'discrete', 'holomorphic', 'observables', 'in', 'the', 'ising', 'model', 'at', 'criticality', 'and', 'show', 'that', 'they', 'have', 'conformally', 'covariant', 'scaling', 'limits', 'as', 'mesh', 'of', 'the', 'lattice', 'tends', 'to', 'zero', 'in', 'the', 'sequel', 'those', 'observables', 'are', 'u... | [-0.11529493731433067, 0.1406664297497575, -0.10844496271127592, 0.13221513190934353, -0.08420866589480336, -0.19952258944808357, -0.05125905994319128, 0.353498301482287, -0.22678440474513648, -0.24613129728190278, 0.10280227645104616, -0.28186451192216383, -0.15789916063321457, 0.13451972358819583, -0.0368868394255422... |
708.004 | An exact chiral spin liquid with non-Abelian anyons | We establish the existence of a chiral spin liquid (CSL) as the exact ground
state of the Kitaev model on a decorated honeycomb lattice, which is obtained
by replacing each site in the familiar honeycomb lattice with a triangle. The
CSL state spontaneously breaks time reversal symmetry but preserves other
symmetries.... | cond-mat.str-el cond-mat.mes-hall | we establish the existence of a chiral spin liquid csl as the exact ground state of the kitaev model on a decorated honeycomb lattice which is obtained by replacing each site in the familiar honeycomb lattice with a triangle the csl state spontaneously breaks time reversal symmetry but preserves other symmetries there ... | [['we', 'establish', 'the', 'existence', 'of', 'a', 'chiral', 'spin', 'liquid', 'csl', 'as', 'the', 'exact', 'ground', 'state', 'of', 'the', 'kitaev', 'model', 'on', 'a', 'decorated', 'honeycomb', 'lattice', 'which', 'is', 'obtained', 'by', 'replacing', 'each', 'site', 'in', 'the', 'familiar', 'honeycomb', 'lattice', '... | [-0.2399488604084278, 0.32257867781803584, -0.03365359216546401, 0.05480013276265266, -0.07134485321167187, -0.23794865570007226, 0.07181081189833677, 0.34695687930648905, -0.23874553185529435, -0.22749634829755777, 0.0694019003586175, -0.30628789254488087, -0.09368945146576525, 0.05452367318018029, 0.06970998012007047... |
708.0041 | Microscopic Wrinkles on Supported Surfactant Monolayers | We discuss mechanical buckling instabilities of a rigid film under
compression interacting repulsively with a substrate through a thin fluid
layer. The buckling occurs at a characteristic wavelength that increases as the
1/4th power of the bending stiffness, like a gravitational instability studied
previously by Miln... | cond-mat.soft | we discuss mechanical buckling instabilities of a rigid film under compression interacting repulsively with a substrate through a thin fluid layer the buckling occurs at a characteristic wavelength that increases as the 14th power of the bending stiffness like a gravitational instability studied previously by milner et... | [['we', 'discuss', 'mechanical', 'buckling', 'instabilities', 'of', 'a', 'rigid', 'film', 'under', 'compression', 'interacting', 'repulsively', 'with', 'a', 'substrate', 'through', 'a', 'thin', 'fluid', 'layer', 'the', 'buckling', 'occurs', 'at', 'a', 'characteristic', 'wavelength', 'that', 'increases', 'as', 'the', '1... | [-0.17801256077031472, 0.1801751391087439, -0.04176258756261733, -0.009325911941391134, -0.02752194840401884, -0.1692998135787627, -0.0024882154742492334, 0.3219358553252523, -0.28745445223998217, -0.26567146579720197, -0.004234016548642623, -0.2901814275140327, -0.2102462529456095, 0.17094668184983589, 0.0160852970503... |
708.0042 | A solid angle theory for real polytopes | We extend many theorems from the context of solid angle sums over rational
polytopes to the context of solid angle sums over real polytopes. Moreover, we
consider any real dilation parameter, as opposed to the traditional integer
dilation parameters. One of the main results is an extension of Macdonald's
solid angle ... | math.CO math.AC | we extend many theorems from the context of solid angle sums over rational polytopes to the context of solid angle sums over real polytopes moreover we consider any real dilation parameter as opposed to the traditional integer dilation parameters one of the main results is an extension of macdonalds solid angle quasipo... | [['we', 'extend', 'many', 'theorems', 'from', 'the', 'context', 'of', 'solid', 'angle', 'sums', 'over', 'rational', 'polytopes', 'to', 'the', 'context', 'of', 'solid', 'angle', 'sums', 'over', 'real', 'polytopes', 'moreover', 'we', 'consider', 'any', 'real', 'dilation', 'parameter', 'as', 'opposed', 'to', 'the', 'tradi... | [-0.12199937773571498, 0.07192146932167183, -0.0726290701524071, 0.04072253605303611, -0.1170951904648024, -0.10352363585211012, 0.026991561379121697, 0.32757408094956825, -0.36778944730758667, -0.19433582545784506, 0.13633021487570976, -0.2751025826656732, -0.1843916808889396, 0.2611618000420107, -0.14735129240400874,... |
708.0043 | Quantifying structural damage from self-irradiation in a plutonium
superconductor | The 18.5 K superconductor PuCoGa5 has many unusual properties, including
those due to damage induced by self-irradiation. The superconducting transition
temperature decreases sharply with time, suggesting a radiation-induced Frenkel
defect concentration much larger than predicted by current radiation damage
theories.... | cond-mat.str-el cond-mat.dis-nn cond-mat.mtrl-sci | the 185 k superconductor pucoga5 has many unusual properties including those due to damage induced by selfirradiation the superconducting transition temperature decreases sharply with time suggesting a radiationinduced frenkel defect concentration much larger than predicted by current radiation damage theories extended... | [['the', '185', 'k', 'superconductor', 'pucoga5', 'has', 'many', 'unusual', 'properties', 'including', 'those', 'due', 'to', 'damage', 'induced', 'by', 'selfirradiation', 'the', 'superconducting', 'transition', 'temperature', 'decreases', 'sharply', 'with', 'time', 'suggesting', 'a', 'radiationinduced', 'frenkel', 'def... | [-0.07432432586236536, 0.22254369456518805, -0.018936653131108105, 0.05698481947389654, -0.04144013959881479, -0.12803785894807856, 0.055878277887606714, 0.42566503384933535, -0.23737740417761086, -0.3250619007225058, 0.014985716921293827, -0.37559922584291316, -0.12317171099027042, 0.1733020582541296, 0.00404542296649... |
708.0044 | Exploring the Local Milky Way: M Dwarfs as Tracers of Galactic
Populations | We have assembled a spectroscopic sample of low-mass dwarfs observed as part
of the Sloan Digital Sky Survey along one Galactic sightline, designed to
investigate the observable properties of the thin and thick disks. This sample
of ~7400 K and M stars also has measured ugriz photometry, proper motions, and
radial ve... | astro-ph | we have assembled a spectroscopic sample of lowmass dwarfs observed as part of the sloan digital sky survey along one galactic sightline designed to investigate the observable properties of the thin and thick disks this sample of 7400 k and m stars also has measured ugriz photometry proper motions and radial velocities... | [['we', 'have', 'assembled', 'a', 'spectroscopic', 'sample', 'of', 'lowmass', 'dwarfs', 'observed', 'as', 'part', 'of', 'the', 'sloan', 'digital', 'sky', 'survey', 'along', 'one', 'galactic', 'sightline', 'designed', 'to', 'investigate', 'the', 'observable', 'properties', 'of', 'the', 'thin', 'and', 'thick', 'disks', '... | [-0.05330853671960843, 0.0921851238158221, -0.07847570864638935, 0.05342047247395385, -0.13211220683685193, -0.010922658947917323, 0.049813807169751576, 0.5054014538259556, -0.23349391917387644, -0.34337040455866374, 0.031257221083311984, -0.3065085485189532, 0.025261436185489098, 0.19409772095192845, -0.01900935245018... |
708.0045 | Persistence of Induced Wormholes in Brane Worlds | Higher-dimensional black holes have long been considered within the context
of brane worlds. Recently, it was shown that the brane-world ethos also permits
the consideration of higher-dimensional wormholes. When such a wormhole,
preexisting in the bulk, impinges upon our universe, taken to be a
positive-tension 3-bra... | gr-qc | higherdimensional black holes have long been considered within the context of brane worlds recently it was shown that the braneworld ethos also permits the consideration of higherdimensional wormholes when such a wormhole preexisting in the bulk impinges upon our universe taken to be a positivetension 3brane it induces... | [['higherdimensional', 'black', 'holes', 'have', 'long', 'been', 'considered', 'within', 'the', 'context', 'of', 'brane', 'worlds', 'recently', 'it', 'was', 'shown', 'that', 'the', 'braneworld', 'ethos', 'also', 'permits', 'the', 'consideration', 'of', 'higherdimensional', 'wormholes', 'when', 'such', 'a', 'wormhole', ... | [-0.15539229764879026, 0.173010665676729, -0.14760109189966764, 0.1486912554035101, -0.13405864309105608, -0.15422105560838073, -0.05026698201912007, 0.29404980387814617, -0.19657147566753405, -0.29881915568063655, 0.0657679077539662, -0.24440107402991054, -0.09107519034296274, 0.1316453360547139, -0.035635404821692244... |
708.0046 | Sparse and stable Markowitz portfolios | We consider the problem of portfolio selection within the classical Markowitz
mean-variance framework, reformulated as a constrained least-squares regression
problem. We propose to add to the objective function a penalty proportional to
the sum of the absolute values of the portfolio weights. This penalty
regularizes... | q-fin.PM math.FA stat.AP | we consider the problem of portfolio selection within the classical markowitz meanvariance framework reformulated as a constrained leastsquares regression problem we propose to add to the objective function a penalty proportional to the sum of the absolute values of the portfolio weights this penalty regularizes stabil... | [['we', 'consider', 'the', 'problem', 'of', 'portfolio', 'selection', 'within', 'the', 'classical', 'markowitz', 'meanvariance', 'framework', 'reformulated', 'as', 'a', 'constrained', 'leastsquares', 'regression', 'problem', 'we', 'propose', 'to', 'add', 'to', 'the', 'objective', 'function', 'a', 'penalty', 'proportion... | [-0.040341302557625684, -0.028872406049429075, -0.06564791316665924, 0.12110887613549046, -0.11689655414606998, -0.1590939385856947, 0.11749343528915061, 0.4182663649401587, -0.28934162219081994, -0.3472712499703672, 0.13383592132300112, -0.24946863394902524, -0.11962376782616628, 0.17226509470323884, -0.17169133408511... |
708.0047 | High energy scattering in Quantum Chromodynamics | In this series of three lectures, we discuss several aspects of high energy
scattering among hadrons in Quantum Chromodynamics. The first lecture is
devoted to a description of the parton model, Bjorken scaling and the scaling
violations due to the evolution of parton distributions with the transverse
resolution scal... | hep-ph nucl-th | in this series of three lectures we discuss several aspects of high energy scattering among hadrons in quantum chromodynamics the first lecture is devoted to a description of the parton model bjorken scaling and the scaling violations due to the evolution of parton distributions with the transverse resolution scale the... | [['in', 'this', 'series', 'of', 'three', 'lectures', 'we', 'discuss', 'several', 'aspects', 'of', 'high', 'energy', 'scattering', 'among', 'hadrons', 'in', 'quantum', 'chromodynamics', 'the', 'first', 'lecture', 'is', 'devoted', 'to', 'a', 'description', 'of', 'the', 'parton', 'model', 'bjorken', 'scaling', 'and', 'the... | [-0.06955321668439345, 0.2270198647997209, -0.1968200575793162, 0.12565827380499936, -0.01431679610894727, -0.010650476351396978, -0.05349449220479333, 0.31629401717301725, -0.17265259960549884, -0.2510493690913011, 0.004348506652084845, -0.29952678372917163, 0.015550670979012336, 0.07759304822580557, -0.00013903597885... |
708.0048 | A renormalization approach to irrational rotations | We introduce a renormalization procedure which allows us to study in a
unified and concise way different properties of the irrational rotations on the
unit circle $\beta \mapsto \set{\alpha+\beta}$, $\alpha \in \R\setminus \Q$. In
particular we obtain sharp results for the diffusion of the walk on $\Z$
generated by t... | math.DS math.NT | we introduce a renormalization procedure which allows us to study in a unified and concise way different properties of the irrational rotations on the unit circle beta mapsto setalphabeta alpha in rsetminus q in particular we obtain sharp results for the diffusion of the walk on z generated by the location of points of... | [['we', 'introduce', 'a', 'renormalization', 'procedure', 'which', 'allows', 'us', 'to', 'study', 'in', 'a', 'unified', 'and', 'concise', 'way', 'different', 'properties', 'of', 'the', 'irrational', 'rotations', 'on', 'the', 'unit', 'circle', 'beta', 'mapsto', 'setalphabeta', 'alpha', 'in', 'rsetminus', 'q', 'in', 'par... | [-0.12567968546310823, 0.0914763596821066, -0.07496529883921962, 0.02435535105098396, -0.027574166221773787, -0.11276305813903678, 0.12906467739958316, 0.4095045308238023, -0.2658435245082803, -0.2198297701335882, 0.06697359742526578, -0.2663393792258145, -0.15795492313240897, 0.22897684446548763, -0.046992466737171765... |
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