id float64 706 1.8k | title stringlengths 1 343 | abstract stringlengths 6 6.09k | categories stringlengths 5 125 | processed_abstract stringlengths 2 5.96k | tokenized_abstract stringlengths 8 8.74k | centroid stringlengths 2.1k 2.17k |
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706.2614 | Dust crystallinity in protoplanetary disks: the effect of
diffusion/viscosity ratio | The process of turbulent radial mixing in protoplanetary disks has strong
relevance to the analysis of the spatial distribution of crystalline dust
species in disks around young stars and to studies of the composition of
meteorites and comets in our own solar system.
A debate has gone on in the recent literature on... | astro-ph | the process of turbulent radial mixing in protoplanetary disks has strong relevance to the analysis of the spatial distribution of crystalline dust species in disks around young stars and to studies of the composition of meteorites and comets in our own solar system a debate has gone on in the recent literature on the ... | [['the', 'process', 'of', 'turbulent', 'radial', 'mixing', 'in', 'protoplanetary', 'disks', 'has', 'strong', 'relevance', 'to', 'the', 'analysis', 'of', 'the', 'spatial', 'distribution', 'of', 'crystalline', 'dust', 'species', 'in', 'disks', 'around', 'young', 'stars', 'and', 'to', 'studies', 'of', 'the', 'composition'... | [-0.08450945948688202, 0.15778088006780044, -0.08527665884733335, 0.04198048750809487, -0.06308087982947051, -0.07231304333376956, 0.028992329906470264, 0.39002324022487345, -0.20573537239064293, -0.3134910538568195, 0.07007221472645964, -0.23293521948697338, -0.08008282609755196, 0.18977875081178486, -0.05296758229219... |
706.2615 | Constraining scalar-tensor quintessence by cosmic clocks | Scalar-tensor quintessence models can be constrained by identifying suitable
cosmic clocks which allow to select confidence regions for cosmological
parameters. In particular, we constrain the characterizing parameters of
non-minimally coupled scalar-tensor cosmological models which admit exact
solutions of the Einst... | astro-ph gr-qc | scalartensor quintessence models can be constrained by identifying suitable cosmic clocks which allow to select confidence regions for cosmological parameters in particular we constrain the characterizing parameters of nonminimally coupled scalartensor cosmological models which admit exact solutions of the einstein fie... | [['scalartensor', 'quintessence', 'models', 'can', 'be', 'constrained', 'by', 'identifying', 'suitable', 'cosmic', 'clocks', 'which', 'allow', 'to', 'select', 'confidence', 'regions', 'for', 'cosmological', 'parameters', 'in', 'particular', 'we', 'constrain', 'the', 'characterizing', 'parameters', 'of', 'nonminimally',... | [-0.12313364848035248, 0.1406345541831361, -0.02761894537212506, 0.15717908217291005, -0.175135752198937, -0.19591275014442533, -0.03593772439898489, 0.3643897378128277, -0.18264443345674097, -0.34439231756411187, 0.03977746062605859, -0.22357956298359044, 0.02122051680894339, 0.17461329024948485, 0.005243060491621903,... |
706.2616 | The gravitational energy for stationary space-time | It is prove, that the gravity field energy formulas obtained for static
systems on the ground of local energy conservation law by test-particles fall,
is suitable for stationary systems.
| gr-qc | it is prove that the gravity field energy formulas obtained for static systems on the ground of local energy conservation law by testparticles fall is suitable for stationary systems | [['it', 'is', 'prove', 'that', 'the', 'gravity', 'field', 'energy', 'formulas', 'obtained', 'for', 'static', 'systems', 'on', 'the', 'ground', 'of', 'local', 'energy', 'conservation', 'law', 'by', 'testparticles', 'fall', 'is', 'suitable', 'for', 'stationary', 'systems']] | [-0.1961649139893466, 0.1225577976940007, -0.10441724907863757, 0.1472899481927141, 0.013779928393918893, -0.16148927647235065, -0.01312250504270196, 0.26715130885613375, -0.21077490180473904, -0.3105390390445446, 0.0850314131199286, -0.24167884822035657, -0.030792254231998634, 0.24152720398430166, -0.01492789533573347... |
706.2617 | On the relation between states and maps in infinite dimensions | Relations between states and maps, which are known for quantum systems in
finite-dimensional Hilbert spaces, are formulated rigorously in geometrical
terms with no use of coordinate (matrix) interpretation. In a tensor product
realization they are represented simply by a permutation of factors. This leads
to natural ... | math-ph math.MP | relations between states and maps which are known for quantum systems in finitedimensional hilbert spaces are formulated rigorously in geometrical terms with no use of coordinate matrix interpretation in a tensor product realization they are represented simply by a permutation of factors this leads to natural generaliz... | [['relations', 'between', 'states', 'and', 'maps', 'which', 'are', 'known', 'for', 'quantum', 'systems', 'in', 'finitedimensional', 'hilbert', 'spaces', 'are', 'formulated', 'rigorously', 'in', 'geometrical', 'terms', 'with', 'no', 'use', 'of', 'coordinate', 'matrix', 'interpretation', 'in', 'a', 'tensor', 'product', '... | [-0.08235979333474505, 0.13616321816126156, -0.06489333427080277, 0.11256338240757653, -0.07131373532337887, -0.10655606326238229, -0.029415964117705275, 0.3407039531668444, -0.3051556568172556, -0.17724834593501304, 0.1669383574789674, -0.24968150566706843, -0.17519235626152693, 0.2145688178048969, -0.1238152607054472... |
706.2618 | Mott-Hubbard Transition and Anderson Localization: Generalized Dynamical
Mean-Field Theory Approach | Density of states, dynamic (optical) conductivity and phase diagram of
strongly correlated and strongly disordered paramagnetic Anderson-Hubbard model
are analyzed within the generalized dynamical mean field theory (DMFT+\Sigma
approximation). Strong correlations are accounted by DMFT, while disorder is
taken into ac... | cond-mat.str-el cond-mat.dis-nn | density of states dynamic optical conductivity and phase diagram of strongly correlated and strongly disordered paramagnetic andersonhubbard model are analyzed within the generalized dynamical mean field theory dmftsigma approximation strong correlations are accounted by dmft while disorder is taken into account via th... | [['density', 'of', 'states', 'dynamic', 'optical', 'conductivity', 'and', 'phase', 'diagram', 'of', 'strongly', 'correlated', 'and', 'strongly', 'disordered', 'paramagnetic', 'andersonhubbard', 'model', 'are', 'analyzed', 'within', 'the', 'generalized', 'dynamical', 'mean', 'field', 'theory', 'dmftsigma', 'approximatio... | [-0.16794568544444372, 0.24782329009420526, -0.07663112692168261, 0.09247703205585098, 0.021184747319991194, -0.21858380296117239, 0.1079129441311275, 0.3811672317289461, -0.2302849346471173, -0.2534014813924634, -0.003745664013769683, -0.3287205383342903, -0.17740872466394048, 0.057917711445988396, 0.07519988781464558... |
706.2619 | Algorithms for Omega-Regular Games with Imperfect Information | We study observation-based strategies for two-player turn-based games on
graphs with omega-regular objectives. An observation-based strategy relies on
imperfect information about the history of a play, namely, on the past sequence
of observations. Such games occur in the synthesis of a controller that does
not see th... | cs.LO cs.GT | we study observationbased strategies for twoplayer turnbased games on graphs with omegaregular objectives an observationbased strategy relies on imperfect information about the history of a play namely on the past sequence of observations such games occur in the synthesis of a controller that does not see the private s... | [['we', 'study', 'observationbased', 'strategies', 'for', 'twoplayer', 'turnbased', 'games', 'on', 'graphs', 'with', 'omegaregular', 'objectives', 'an', 'observationbased', 'strategy', 'relies', 'on', 'imperfect', 'information', 'about', 'the', 'history', 'of', 'a', 'play', 'namely', 'on', 'the', 'past', 'sequence', 'o... | [-0.09949469106051967, 0.04175434244445771, -0.11910519677912816, 0.06020774647283057, -0.054641751144340056, -0.167070858034357, 0.11409790065566389, 0.4016939594048179, -0.2501481184735894, -0.30287376803624083, 0.12069216128762086, -0.2502519383405646, -0.13676402435521595, 0.17908349081666933, -0.1324644389225998, ... |
706.262 | Rhodium Mossbauer Supperadiance Induced by Liquid-Nitrogen Cooling | In the previous report, we have demonstrated cascade branching channels of
the multipolar E3 transition of rhodium Mossbauer gamma via the time- and
energy-resolved spectroscopy. Moreover, superradiance in the Borrmann channel
from inverted nuclei gives gamma entanglement. In this letter, we report
further four obser... | quant-ph physics.atom-ph | in the previous report we have demonstrated cascade branching channels of the multipolar e3 transition of rhodium mossbauer gamma via the time and energyresolved spectroscopy moreover superradiance in the borrmann channel from inverted nuclei gives gamma entanglement in this letter we report further four observations o... | [['in', 'the', 'previous', 'report', 'we', 'have', 'demonstrated', 'cascade', 'branching', 'channels', 'of', 'the', 'multipolar', 'e3', 'transition', 'of', 'rhodium', 'mossbauer', 'gamma', 'via', 'the', 'time', 'and', 'energyresolved', 'spectroscopy', 'moreover', 'superradiance', 'in', 'the', 'borrmann', 'channel', 'fr... | [-0.12556904677062689, 0.24359045186276107, -0.0428216700674966, 0.03293275429046174, 0.0055176108511851025, -0.17606509502634013, 0.11492897704521422, 0.4213411571016829, -0.2445815134662808, -0.2606679168611504, 0.013613179649773724, -0.3039088373382886, -0.04096295551004771, 0.1869481388773573, 0.08683937062660493, ... |
706.2621 | Some physical displays of the space anisotropy relevant to the
feasibility of its being detected at a laboratory | The impact of local space anisotropy on the transverse Doppler effect is
examined. Two types of laboratory experiments aimed at seeking and measuring
the local space anisotropy are proposed. In terms of the conventional special
relativity theory, which treats 3D space to be locally isotropic, the
experiments are of t... | gr-qc | the impact of local space anisotropy on the transverse doppler effect is examined two types of laboratory experiments aimed at seeking and measuring the local space anisotropy are proposed in terms of the conventional special relativity theory which treats 3d space to be locally isotropic the experiments are of the typ... | [['the', 'impact', 'of', 'local', 'space', 'anisotropy', 'on', 'the', 'transverse', 'doppler', 'effect', 'is', 'examined', 'two', 'types', 'of', 'laboratory', 'experiments', 'aimed', 'at', 'seeking', 'and', 'measuring', 'the', 'local', 'space', 'anisotropy', 'are', 'proposed', 'in', 'terms', 'of', 'the', 'conventional'... | [-0.14645876349238007, 0.19326810868572175, -0.026568790962535543, 0.03386460111678107, -0.06882896999943733, -0.10868019296442033, 0.014602474141901974, 0.3698520900696017, -0.25599689942006904, -0.2978521026154865, 0.07792821222887442, -0.3333695997092777, -0.0434859354653847, 0.2290871770303581, 0.03185225440790521,... |
706.2622 | Structure Through Colour: A Pixel Approach Towards Understanding
Galaxies | We present a study of pixel Colour Magnitude Diagrams (pCMDs) for a sample of
69 nearby galaxies chosen to span a wide range of Hubble types. Our goal is to
determine how useful a pixel approach is for studying galaxies according to
their stellar light distributions and content. The galaxy images were analysed
on a p... | astro-ph | we present a study of pixel colour magnitude diagrams pcmds for a sample of 69 nearby galaxies chosen to span a wide range of hubble types our goal is to determine how useful a pixel approach is for studying galaxies according to their stellar light distributions and content the galaxy images were analysed on a pixelby... | [['we', 'present', 'a', 'study', 'of', 'pixel', 'colour', 'magnitude', 'diagrams', 'pcmds', 'for', 'a', 'sample', 'of', '69', 'nearby', 'galaxies', 'chosen', 'to', 'span', 'a', 'wide', 'range', 'of', 'hubble', 'types', 'our', 'goal', 'is', 'to', 'determine', 'how', 'useful', 'a', 'pixel', 'approach', 'is', 'for', 'stud... | [-0.026597614607775304, 0.051500925944712596, -0.11895628008503645, 0.11885474892380667, -0.08001413766364408, -0.04430960096913029, 0.027638328598644332, 0.483995895940481, -0.14577433852814248, -0.3572280907284367, 0.023951112622946347, -0.26825434547129523, -0.06779222076419791, 0.17246510873494836, -0.0760445095429... |
706.2623 | Quantum Dyanmics of Loop Quantum Gravity | In the last 20 years, loop quantum gravity, a background independent approach
to unify general relativity and quantum mechanics, has been widely
investigated. The aim of loop quantum gravity is to construct a mathematically
rigorous, background independent, nonperturbative quantum theory for the
Lorentzian gravitatio... | gr-qc hep-th math-ph math.MP | in the last 20 years loop quantum gravity a background independent approach to unify general relativity and quantum mechanics has been widely investigated the aim of loop quantum gravity is to construct a mathematically rigorous background independent nonperturbative quantum theory for the lorentzian gravitational fiel... | [['in', 'the', 'last', '20', 'years', 'loop', 'quantum', 'gravity', 'a', 'background', 'independent', 'approach', 'to', 'unify', 'general', 'relativity', 'and', 'quantum', 'mechanics', 'has', 'been', 'widely', 'investigated', 'the', 'aim', 'of', 'loop', 'quantum', 'gravity', 'is', 'to', 'construct', 'a', 'mathematicall... | [-0.13561857938540992, 0.13152916760389433, -0.15452158262927992, 0.09789079767735759, -0.07248845338288627, -0.1408723613901718, -0.01608988175195902, 0.2603738879321378, -0.2293734382565326, -0.2652665027668951, 0.07842498248063347, -0.24296353990631597, -0.180094738532831, 0.19569752730328488, -0.05616983375616942, ... |
706.2624 | Demonstrating the negligible contribution of optical ACS/HST galaxies to
source-subtracted cosmic infrared background fluctuations in deep
IRAC/Spitzer images | We study the possible contribution of optical galaxies detected with the {\it
Hubble} ACS instrument to the near-IR cosmic infrared (CIB) fluctuations in
deep {\it Spitzer} images. The {\it Spitzer} data used in this analysis are
obtained in the course of the GOODS project from which we select four
independent $10^\p... | astro-ph | we study the possible contribution of optical galaxies detected with the it hubble acs instrument to the nearir cosmic infrared cib fluctuations in deep it spitzer images the it spitzer data used in this analysis are obtained in the course of the goods project from which we select four independent 10primetimes10prime r... | [['we', 'study', 'the', 'possible', 'contribution', 'of', 'optical', 'galaxies', 'detected', 'with', 'the', 'it', 'hubble', 'acs', 'instrument', 'to', 'the', 'nearir', 'cosmic', 'infrared', 'cib', 'fluctuations', 'in', 'deep', 'it', 'spitzer', 'images', 'the', 'it', 'spitzer', 'data', 'used', 'in', 'this', 'analysis', ... | [-0.04701020421391321, 0.11092164527720776, -0.10541493435442256, 0.1294381548820439, -0.06472077542444284, -0.03995107430085348, 0.001160975557636038, 0.42937227571982683, -0.23030772131104263, -0.3398653808861267, 0.06125626539113999, -0.36171954145626056, -0.08303173991692624, 0.17494218789596638, -0.008669903190095... |
706.2625 | Self-organized surface nanopatterning by ion beam sputtering | The production of nanopatterns on the surfaces of targets irradiated by ion
beams at low and intermediate energies has developed during the present decade
to a salient degree of control over the main pattern features. However, there
is still a wide experimental scatter in the type and relevance of various
dynamic int... | cond-mat.mtrl-sci | the production of nanopatterns on the surfaces of targets irradiated by ion beams at low and intermediate energies has developed during the present decade to a salient degree of control over the main pattern features however there is still a wide experimental scatter in the type and relevance of various dynamic interfa... | [['the', 'production', 'of', 'nanopatterns', 'on', 'the', 'surfaces', 'of', 'targets', 'irradiated', 'by', 'ion', 'beams', 'at', 'low', 'and', 'intermediate', 'energies', 'has', 'developed', 'during', 'the', 'present', 'decade', 'to', 'a', 'salient', 'degree', 'of', 'control', 'over', 'the', 'main', 'pattern', 'feature... | [-0.06716692552764074, 0.1367443855705003, -0.021328403435192756, 0.04086777887759652, -0.026738118765079918, -0.11480165842457067, 0.013512210348760928, 0.39953709398986587, -0.2525240937772561, -0.3489724633681802, 0.11551269261492197, -0.27921870760860124, -0.09634658279643583, 0.23882788897955468, -0.02981017326592... |
706.2626 | Geometrical approach to mutually unbiased bases | We propose a unifying phase-space approach to the construction of mutually
unbiased bases for a two-qubit system. It is based on an explicit
classification of the geometrical structures compatible with the notion of
unbiasedness. These consist of bundles of discrete curves intersecting only at
the origin and satisfyi... | quant-ph | we propose a unifying phasespace approach to the construction of mutually unbiased bases for a twoqubit system it is based on an explicit classification of the geometrical structures compatible with the notion of unbiasedness these consist of bundles of discrete curves intersecting only at the origin and satisfying cer... | [['we', 'propose', 'a', 'unifying', 'phasespace', 'approach', 'to', 'the', 'construction', 'of', 'mutually', 'unbiased', 'bases', 'for', 'a', 'twoqubit', 'system', 'it', 'is', 'based', 'on', 'an', 'explicit', 'classification', 'of', 'the', 'geometrical', 'structures', 'compatible', 'with', 'the', 'notion', 'of', 'unbia... | [-0.17840851378708106, 0.08139178859726046, -0.09871253187504961, 0.043660406487659835, -0.05490495951886734, -0.1166007352395631, 0.01810173815338994, 0.41171949237342115, -0.26039266163159325, -0.25519287578113703, 0.07909588101598353, -0.2359707108800016, -0.15621139272701365, 0.21556277595252893, -0.082711504671074... |
706.2627 | The Tidal Tails of NGC 5466 | The study of substructure in the stellar halo of the Milky Way has made a lot
of progress in recent years, especially with the advent of surveys like the
Sloan Digital Sky Survey. Here, we study the newly discovered tidal tails of
the Galactic globular cluster NGC 5466. By means of numerical simulations, we
reproduce... | astro-ph | the study of substructure in the stellar halo of the milky way has made a lot of progress in recent years especially with the advent of surveys like the sloan digital sky survey here we study the newly discovered tidal tails of the galactic globular cluster ngc 5466 by means of numerical simulations we reproduce the sh... | [['the', 'study', 'of', 'substructure', 'in', 'the', 'stellar', 'halo', 'of', 'the', 'milky', 'way', 'has', 'made', 'a', 'lot', 'of', 'progress', 'in', 'recent', 'years', 'especially', 'with', 'the', 'advent', 'of', 'surveys', 'like', 'the', 'sloan', 'digital', 'sky', 'survey', 'here', 'we', 'study', 'the', 'newly', 'd... | [-0.10077118604876274, 0.05718380381782236, -0.13674816362470849, 0.08815015780967085, -0.1097091552971475, 0.01605957125106256, 0.018906023210762173, 0.396022799948042, -0.2229946543661396, -0.3574512397682064, 0.08564511135814376, -0.25395709509029984, -0.03922425918635066, 0.21410614773539532, -0.05029610177538661, ... |
706.2628 | Phase Transition of Trapped Nuclear Exciton of Long-lived Rhodium
Mossbauer States | We report experimental observations of the long-lived rhodium Mossbauer
emissions by the time- and energy-resolved spectroscopy. The extraordinary
observations manifest the open-up of photonic band gap in analogy to the
superconducting gap of remarkable symmetry breakings at transition point. These
observations are o... | quant-ph gr-qc physics.atom-ph | we report experimental observations of the longlived rhodium mossbauer emissions by the time and energyresolved spectroscopy the extraordinary observations manifest the openup of photonic band gap in analogy to the superconducting gap of remarkable symmetry breakings at transition point these observations are of potent... | [['we', 'report', 'experimental', 'observations', 'of', 'the', 'longlived', 'rhodium', 'mossbauer', 'emissions', 'by', 'the', 'time', 'and', 'energyresolved', 'spectroscopy', 'the', 'extraordinary', 'observations', 'manifest', 'the', 'openup', 'of', 'photonic', 'band', 'gap', 'in', 'analogy', 'to', 'the', 'superconduct... | [-0.12957417085452705, 0.25193143002110713, -0.06571699173233453, 0.04360438768754654, -0.006347914667012507, -0.0882532061765208, 0.08112807222173218, 0.441320922575741, -0.2546295489453329, -0.3415882878705559, 0.01582504240655334, -0.3402038682939722, -0.05188840027936053, 0.14121374439123094, 0.10756344042543396, 0... |
706.2629 | Period-color and amplitude-color relations in classical Cepheid
variables V: The Small Magellanic Cloud Cepheid models | Period-colour (PC) and amplitude-colour (AC) relations at maximum, mean and
minimum light are constructed from a large grid of full amplitude hydrodynamic
models of Cepheids with a composition appropriate for the SMC (Small Magellanic
Cloud). We compare these theoretical relations with those from observations.
The th... | astro-ph | periodcolour pc and amplitudecolour ac relations at maximum mean and minimum light are constructed from a large grid of full amplitude hydrodynamic models of cepheids with a composition appropriate for the smc small magellanic cloud we compare these theoretical relations with those from observations the theoretical rel... | [['periodcolour', 'pc', 'and', 'amplitudecolour', 'ac', 'relations', 'at', 'maximum', 'mean', 'and', 'minimum', 'light', 'are', 'constructed', 'from', 'a', 'large', 'grid', 'of', 'full', 'amplitude', 'hydrodynamic', 'models', 'of', 'cepheids', 'with', 'a', 'composition', 'appropriate', 'for', 'the', 'smc', 'small', 'ma... | [-0.10869015947551719, 0.1254656327308606, -0.12634880631384965, 0.15244563319951618, -0.10490218701075442, -0.10702454987358277, 0.11789095306010386, 0.41876219154878314, -0.2595060117703104, -0.3536453191375989, 0.033381156709711285, -0.26929308144708736, -0.09766673606771063, 0.2299181409862466, -0.04837152110073493... |
706.263 | Parton shower Monte Carlos vs resummed calculations for interjet energy
flow observables | Parton showers in Monte Carlo event generators reflect to a certain accuracy
our understanding of QCD radiation at all orders. For observables sensitive to
interjet energy flow in well defined regions of phase space, it has been known
for some time that relevant all-order dynamics is substantially more
complicated th... | hep-ph | parton showers in monte carlo event generators reflect to a certain accuracy our understanding of qcd radiation at all orders for observables sensitive to interjet energy flow in well defined regions of phase space it has been known for some time that relevant allorder dynamics is substantially more complicated than th... | [['parton', 'showers', 'in', 'monte', 'carlo', 'event', 'generators', 'reflect', 'to', 'a', 'certain', 'accuracy', 'our', 'understanding', 'of', 'qcd', 'radiation', 'at', 'all', 'orders', 'for', 'observables', 'sensitive', 'to', 'interjet', 'energy', 'flow', 'in', 'well', 'defined', 'regions', 'of', 'phase', 'space', '... | [-0.06282829390814489, 0.17534893889038963, -0.1413618796505034, 0.20310243985174262, -0.04570433021581266, 0.004580980142539677, -0.0300427626734745, 0.4521955164382234, -0.18800793799649304, -0.3293705874627146, 0.008452528418274596, -0.2975180363767625, -0.029515695704806905, 0.1635524043328284, 0.018862978923910607... |
706.2631 | Minimal data rate stabilization of nonlinear systems over networks with
large delays | Control systems over networks with a finite data rate can be conveniently
modeled as hybrid (impulsive) systems. For the class of nonlinear systems in
feedfoward form, we design a hybrid controller which guarantees stability, in
spite of the measurement noise due to the quantization, and of an arbitrarily
large delay... | math.OC | control systems over networks with a finite data rate can be conveniently modeled as hybrid impulsive systems for the class of nonlinear systems in feedfoward form we design a hybrid controller which guarantees stability in spite of the measurement noise due to the quantization and of an arbitrarily large delay which a... | [['control', 'systems', 'over', 'networks', 'with', 'a', 'finite', 'data', 'rate', 'can', 'be', 'conveniently', 'modeled', 'as', 'hybrid', 'impulsive', 'systems', 'for', 'the', 'class', 'of', 'nonlinear', 'systems', 'in', 'feedfoward', 'form', 'we', 'design', 'a', 'hybrid', 'controller', 'which', 'guarantees', 'stabili... | [-0.20628096325812226, 0.10076125937715155, -0.05669021326164373, -0.0023201271586556316, -0.018123176043169407, -0.18308989057623887, 0.046460124958730954, 0.3490416322233556, -0.34263829104130783, -0.29912138553454154, 0.14675593897228753, -0.24866628124013165, -0.1480798252837591, 0.22272440515269962, -0.12573030670... |
706.2632 | A Dynamical Systems Approach to the Kadison-Singer Problem | In these notes we develop a link between the Kadison-Singer problem and
questions about certain dynamical systems. We conjecture that whether or not a
given state has a unique extension is related to certain dynamical properties
of the state. We prove that if any state corresponding to a minimal idempotent
point exte... | math.OA | in these notes we develop a link between the kadisonsinger problem and questions about certain dynamical systems we conjecture that whether or not a given state has a unique extension is related to certain dynamical properties of the state we prove that if any state corresponding to a minimal idempotent point extends u... | [['in', 'these', 'notes', 'we', 'develop', 'a', 'link', 'between', 'the', 'kadisonsinger', 'problem', 'and', 'questions', 'about', 'certain', 'dynamical', 'systems', 'we', 'conjecture', 'that', 'whether', 'or', 'not', 'a', 'given', 'state', 'has', 'a', 'unique', 'extension', 'is', 'related', 'to', 'certain', 'dynamical... | [-0.13621983987802308, 0.11410536417340515, -0.12099900655448437, 0.03533390660017525, -0.09591885781783151, -0.12084619417206116, 0.035933702195394934, 0.3090103366077329, -0.3773226581564913, -0.16152923565664112, 0.1663938984051602, -0.27741444803102977, -0.11398018681769553, 0.16298849186190237, -0.1240838039538835... |
706.2633 | Topological Gauge Theories on Local Spaces and Black Hole Entropy
Countings | We study cohomological gauge theories on total spaces of holomorphic line
bundles over complex manifolds and obtain their reduction to the base manifold
by U(1) equivariant localization of the path integral. We exemplify this
general mechanism by proving via exact path integral localization a reduction
for local curv... | hep-th math.AG | we study cohomological gauge theories on total spaces of holomorphic line bundles over complex manifolds and obtain their reduction to the base manifold by u1 equivariant localization of the path integral we exemplify this general mechanism by proving via exact path integral localization a reduction for local curves co... | [['we', 'study', 'cohomological', 'gauge', 'theories', 'on', 'total', 'spaces', 'of', 'holomorphic', 'line', 'bundles', 'over', 'complex', 'manifolds', 'and', 'obtain', 'their', 'reduction', 'to', 'the', 'base', 'manifold', 'by', 'u1', 'equivariant', 'localization', 'of', 'the', 'path', 'integral', 'we', 'exemplify', '... | [-0.18464656544261074, 0.10193870537413954, -0.08520290184880427, 0.14584608262470156, -0.06708135627406209, -0.11421369232662153, 0.008560206725776783, 0.2910999333355249, -0.22419710954030356, -0.25909461850594534, 0.06919111429893396, -0.2441821025537425, -0.18175356438497833, 0.17815783097032914, -0.091919162768151... |
706.2634 | Quivers and difference Painleve equations | We will describe natural `Lax pairs' for the difference Painleve equations
with affine Weyl symmetry groups of types E6, E7 and E8, showing that they do
indeed arise as symmetries of certain Fuchsian systems of differential
equations.
| math.AG nlin.SI | we will describe natural lax pairs for the difference painleve equations with affine weyl symmetry groups of types e6 e7 and e8 showing that they do indeed arise as symmetries of certain fuchsian systems of differential equations | [['we', 'will', 'describe', 'natural', 'lax', 'pairs', 'for', 'the', 'difference', 'painleve', 'equations', 'with', 'affine', 'weyl', 'symmetry', 'groups', 'of', 'types', 'e6', 'e7', 'and', 'e8', 'showing', 'that', 'they', 'do', 'indeed', 'arise', 'as', 'symmetries', 'of', 'certain', 'fuchsian', 'systems', 'of', 'diffe... | [-0.24180235925155716, 0.09668784500477282, -0.049534305527403545, 0.13475258139943755, -0.1935461469724573, -0.19323181647908044, -0.06276985826725895, 0.3321697903243271, -0.3036457485443837, -0.2501314542180783, 0.06414898121226076, -0.3110649219235858, -0.18592743653602697, 0.14962342495060954, -0.12447596920301786... |
706.2635 | Magnetic flux detection with an Andreev Quantum Dot | The charge of the subgap states in an Andreev quantum dot (AQD; this is a
quantum dot inserted into a superconducting loop) is very sensitive to the
magnetic flux threading the loop. We study the sensitivity of this device as a
function of its parameters for the limit of a large superconducting gap. In our
analysis, ... | cond-mat.mes-hall cond-mat.supr-con | the charge of the subgap states in an andreev quantum dot aqd this is a quantum dot inserted into a superconducting loop is very sensitive to the magnetic flux threading the loop we study the sensitivity of this device as a function of its parameters for the limit of a large superconducting gap in our analysis we accou... | [['the', 'charge', 'of', 'the', 'subgap', 'states', 'in', 'an', 'andreev', 'quantum', 'dot', 'aqd', 'this', 'is', 'a', 'quantum', 'dot', 'inserted', 'into', 'a', 'superconducting', 'loop', 'is', 'very', 'sensitive', 'to', 'the', 'magnetic', 'flux', 'threading', 'the', 'loop', 'we', 'study', 'the', 'sensitivity', 'of', ... | [-0.22938273633908796, 0.14824653845802876, -0.0423629534240049, 0.08111215585208756, 0.015695527689643652, -0.12006084862759853, 0.09023685680691108, 0.3307018786758544, -0.22086595849369664, -0.3042198372443756, 0.011967718351565033, -0.2588130518098373, -0.08519049029213836, 0.2080454787980002, 0.0044088360645909265... |
706.2636 | Optimal pointwise approximation of stochastic differential equations
driven by fractional Brownian motion | We study the approximation of stochastic differential equations driven by a
fractional Brownian motion with Hurst parameter $H>1/2$. For the mean-square
error at a single point we derive the optimal rate of convergence that can be
achieved by any approximation method using an equidistant discretization of the
driving... | math.PR math.NA | we study the approximation of stochastic differential equations driven by a fractional brownian motion with hurst parameter h12 for the meansquare error at a single point we derive the optimal rate of convergence that can be achieved by any approximation method using an equidistant discretization of the driving fractio... | [['we', 'study', 'the', 'approximation', 'of', 'stochastic', 'differential', 'equations', 'driven', 'by', 'a', 'fractional', 'brownian', 'motion', 'with', 'hurst', 'parameter', 'h12', 'for', 'the', 'meansquare', 'error', 'at', 'a', 'single', 'point', 'we', 'derive', 'the', 'optimal', 'rate', 'of', 'convergence', 'that'... | [-0.1511977291133787, 0.0731659537383599, -0.07403116027957626, 0.0178812105186461, -0.015957439433605898, -0.12459110031347899, 0.06400654519952478, 0.3753077103268532, -0.3176594900432974, -0.26263086311519146, 0.12729607499204576, -0.2612941189802119, -0.14177254689413876, 0.21431953345114987, -0.08493228076646725, ... |
706.2637 | One-step replica symmetry breaking solution for a highly asymmetric
two-sublattice fermionic Ising spin glass model in a transverse field | The one-step replica symmetry breaking (RSB) is used to study a
two-sublattice fermionic infinite-range Ising spin glass (SG) model in a
transverse field $\Gamma$. The problem is formulated in a Grassmann path
integral formalism within the static approximation. In this model, a parallel
magnetic field $H$ breaks the ... | cond-mat.str-el cond-mat.dis-nn | the onestep replica symmetry breaking rsb is used to study a twosublattice fermionic infiniterange ising spin glass sg model in a transverse field gamma the problem is formulated in a grassmann path integral formalism within the static approximation in this model a parallel magnetic field h breaks the symmetry of the s... | [['the', 'onestep', 'replica', 'symmetry', 'breaking', 'rsb', 'is', 'used', 'to', 'study', 'a', 'twosublattice', 'fermionic', 'infiniterange', 'ising', 'spin', 'glass', 'sg', 'model', 'in', 'a', 'transverse', 'field', 'gamma', 'the', 'problem', 'is', 'formulated', 'in', 'a', 'grassmann', 'path', 'integral', 'formalism'... | [-0.19341359156907748, 0.21386240720463626, -0.053184261684430446, 0.05645409794432102, -0.07088997312775343, -0.18733601950542392, 0.07572171275531596, 0.36432341870731944, -0.2667549327061982, -0.23250673921539053, 0.04377952442933243, -0.28094991792735674, -0.10269704529102708, 0.0595061990022106, 0.0501121861422445... |
706.2638 | Some applications of the Mellin transform to branching processes | We introduce a Mellin transform of functions which live on all of $\bR$ and
discuss its applications to the limiting theory of Bellman-Harris processes,
and specifically Luria-Delbr\"uck processes. More precisely, we calculate the
life-time distribution of particles in a Bellman-Harris process from their
first-genera... | math.PR | we introduce a mellin transform of functions which live on all of br and discuss its applications to the limiting theory of bellmanharris processes and specifically luriadelbruck processes more precisely we calculate the lifetime distribution of particles in a bellmanharris process from their firstgeneration offspring ... | [['we', 'introduce', 'a', 'mellin', 'transform', 'of', 'functions', 'which', 'live', 'on', 'all', 'of', 'br', 'and', 'discuss', 'its', 'applications', 'to', 'the', 'limiting', 'theory', 'of', 'bellmanharris', 'processes', 'and', 'specifically', 'luriadelbruck', 'processes', 'more', 'precisely', 'we', 'calculate', 'the'... | [-0.02816770498891576, 0.12097141595946236, -0.18804032839630003, 0.1595500185844635, -0.025715563492337754, -0.05043400223315744, 0.09588937794135316, 0.3582878088844674, -0.2998961813742766, -0.21035023180993048, 0.10863016561379882, -0.242193288292613, -0.17365528426675514, 0.1916157768675955, -0.054933228924010806,... |
706.2639 | Apparatus for excitation and detection of Rydberg atoms in quantum gases | We present and characterize a versatile experimental setup which allows for
excitation and detection of Rydberg atoms in quantum gases. The novel concept
of the setup features two charged particle detectors and eight electrical field
plates inside the vacuum chamber, which allows the detection and manipulation
of Ryd... | quant-ph | we present and characterize a versatile experimental setup which allows for excitation and detection of rydberg atoms in quantum gases the novel concept of the setup features two charged particle detectors and eight electrical field plates inside the vacuum chamber which allows the detection and manipulation of rydberg... | [['we', 'present', 'and', 'characterize', 'a', 'versatile', 'experimental', 'setup', 'which', 'allows', 'for', 'excitation', 'and', 'detection', 'of', 'rydberg', 'atoms', 'in', 'quantum', 'gases', 'the', 'novel', 'concept', 'of', 'the', 'setup', 'features', 'two', 'charged', 'particle', 'detectors', 'and', 'eight', 'el... | [-0.11453024670481682, 0.24306339995403375, -0.032233418717182105, -0.017900187986725498, 0.07213258790739235, -0.1867462174301701, 0.025568182555781235, 0.36328027702513194, -0.1733583489876418, -0.29227518561695304, -0.009491059736215642, -0.25037782852609997, -0.03708199369055884, 0.18569012533629403, 0.051908860812... |
706.264 | Search for large-scale anisotropies with the Auger Observatory | We use more than two years of data from the Pierre Auger Observatory to
search for anisotropies on large scales in different energy windows. We account
for various systematics in the acceptance, in particular due to the array
growth and weather variations. We present the results of analyses and
consistency checks loo... | astro-ph | we use more than two years of data from the pierre auger observatory to search for anisotropies on large scales in different energy windows we account for various systematics in the acceptance in particular due to the array growth and weather variations we present the results of analyses and consistency checks looking ... | [['we', 'use', 'more', 'than', 'two', 'years', 'of', 'data', 'from', 'the', 'pierre', 'auger', 'observatory', 'to', 'search', 'for', 'anisotropies', 'on', 'large', 'scales', 'in', 'different', 'energy', 'windows', 'we', 'account', 'for', 'various', 'systematics', 'in', 'the', 'acceptance', 'in', 'particular', 'due', 't... | [-0.12229160256134088, 0.1446682523172866, -0.07991323956391877, 0.17800481632164317, -0.05918560948015915, 0.0028222317406390277, -0.009042011761468731, 0.40205739277492586, -0.22165051449297202, -0.3600457436922524, 0.10548014414315629, -0.3363992128935125, -0.0634813143664764, 0.24830057163166608, 0.0127663665916770... |
706.2641 | Performance Studies of Prototype II for the CASTOR forward Calorimeter
at the CMS Experiment | We present results of the performance of the second prototype of the CASTOR
quartz-tungsten sampling calorimeter, to be installed in the very forward
region of the CMS experiment at the LHC. The energy linearity and resolution,
as well as the spatial resolution of the prototype to electromagnetic and
hadronic showers... | physics.ins-det nucl-ex | we present results of the performance of the second prototype of the castor quartztungsten sampling calorimeter to be installed in the very forward region of the cms experiment at the lhc the energy linearity and resolution as well as the spatial resolution of the prototype to electromagnetic and hadronic showers are s... | [['we', 'present', 'results', 'of', 'the', 'performance', 'of', 'the', 'second', 'prototype', 'of', 'the', 'castor', 'quartztungsten', 'sampling', 'calorimeter', 'to', 'be', 'installed', 'in', 'the', 'very', 'forward', 'region', 'of', 'the', 'cms', 'experiment', 'at', 'the', 'lhc', 'the', 'energy', 'linearity', 'and', ... | [-0.019717414999443492, 0.20796127041299525, -0.07878192814768115, 0.06754285220600915, 0.022925853216497417, -0.1356661869526914, -0.04066504619942371, 0.4299289484487407, -0.13580609238549565, -0.3949026718233409, 0.028573624687687902, -0.36312463687042174, 0.07988320249185134, 0.2102784966484884, 0.01499563167519145... |
706.2642 | The twisted Mellin transform | The "twisted Mellin transform" is a slightly modified version of the usual
classical Mellin transform on $L^2(\mathbb R)$. In this short note we
investigate some of its basic properties. From the point of views of
combinatorics one of its most important interesting properties is that it
intertwines the differential o... | math.CO | the twisted mellin transform is a slightly modified version of the usual classical mellin transform on l2mathbb r in this short note we investigate some of its basic properties from the point of views of combinatorics one of its most important interesting properties is that it intertwines the differential operator dfdx... | [['the', 'twisted', 'mellin', 'transform', 'is', 'a', 'slightly', 'modified', 'version', 'of', 'the', 'usual', 'classical', 'mellin', 'transform', 'on', 'l2mathbb', 'r', 'in', 'this', 'short', 'note', 'we', 'investigate', 'some', 'of', 'its', 'basic', 'properties', 'from', 'the', 'point', 'of', 'views', 'of', 'combinat... | [-0.13517831792671453, 0.07174135449835482, -0.17106442453668397, 0.10365195533205919, -0.09861187884474502, -0.1160327770308975, -0.023261369362144787, 0.29986779137569314, -0.3409197075100725, -0.17127880079343039, 0.12065668397391324, -0.3065452691824997, -0.19846662257743233, 0.20152292715056855, -0.087702468081432... |
706.2643 | Measurement of the UHECR energy spectrum from hybrid data of the Pierre
Auger Observatory | More than two years of fluorescence detector data collected in coincidence
with at least one station of the surface detector array (``hybrid data'') are
used to measure the flux and energy spectrum of cosmic rays above about
10$^{18}$ eV. The hybrid measurement extends towards lower energies the
spectrum measured wit... | astro-ph | more than two years of fluorescence detector data collected in coincidence with at least one station of the surface detector array hybrid data are used to measure the flux and energy spectrum of cosmic rays above about 1018 ev the hybrid measurement extends towards lower energies the spectrum measured with the surface ... | [['more', 'than', 'two', 'years', 'of', 'fluorescence', 'detector', 'data', 'collected', 'in', 'coincidence', 'with', 'at', 'least', 'one', 'station', 'of', 'the', 'surface', 'detector', 'array', 'hybrid', 'data', 'are', 'used', 'to', 'measure', 'the', 'flux', 'and', 'energy', 'spectrum', 'of', 'cosmic', 'rays', 'above... | [-0.08994089056780927, 0.10685878128942088, -0.044350987271472964, 0.04444881631769528, -0.0038065331815213886, -0.08754784644571777, 0.010188549190529228, 0.36097124844943124, -0.1926474017763184, -0.424628794126059, 0.10046153427485723, -0.3853127479015552, 0.03255614854537008, 0.23750073207811134, -0.023230187440614... |
706.2644 | Some new equivalences of Anderson's paving conjectures | Anderson's paving conjectures are known to be equivalent to the
Kadison-Singer problem. We prove some new equivalences of Anderson's
conjectures that require the paving of smaller sets of matrices. We prove that
if the strictly upper triangular operatorss are pavable, then every 0 diagonal
operator is pavable. This r... | math.OA | andersons paving conjectures are known to be equivalent to the kadisonsinger problem we prove some new equivalences of andersons conjectures that require the paving of smaller sets of matrices we prove that if the strictly upper triangular operatorss are pavable then every 0 diagonal operator is pavable this result fol... | [['andersons', 'paving', 'conjectures', 'are', 'known', 'to', 'be', 'equivalent', 'to', 'the', 'kadisonsinger', 'problem', 'we', 'prove', 'some', 'new', 'equivalences', 'of', 'andersons', 'conjectures', 'that', 'require', 'the', 'paving', 'of', 'smaller', 'sets', 'of', 'matrices', 'we', 'prove', 'that', 'if', 'the', 's... | [-0.1417742141914603, 0.18194621955779822, -0.03619359122393163, 0.11160367338820115, -0.07825913829545147, -0.18417938418171712, -0.004139006566746454, 0.33658760072859495, -0.3238365015407142, -0.13857240649552918, 0.17041081286764606, -0.31264628239564207, -0.1951122711731219, 0.22546465925896833, -0.107625648367071... |
706.2645 | Compactness of the Complex Green Operator | Let $\Omega\subset\C^n$ be a bounded smooth pseudoconvex domain. We show that
compactness of the complex Green operator $G_{q}$ on $(0,q)$-forms on $b\Omega$
implies compactness of the $\bar{\partial}$-Neumann operator $N_{q}$ on
$\Omega$. We prove that if $1 \leq q \leq n-2$ and $b\Omega$ satisfies $(P_q)$
and $(P_{... | math.CV math.AP | let omegasubsetcn be a bounded smooth pseudoconvex domain we show that compactness of the complex green operator g_q on 0qforms on bomega implies compactness of the barpartialneumann operator n_q on omega we prove that if 1 leq q leq n2 and bomega satisfies p_q and p_nq1 then g_q is a compact operator and so is g_n1q o... | [['let', 'omegasubsetcn', 'be', 'a', 'bounded', 'smooth', 'pseudoconvex', 'domain', 'we', 'show', 'that', 'compactness', 'of', 'the', 'complex', 'green', 'operator', 'g_q', 'on', '0qforms', 'on', 'bomega', 'implies', 'compactness', 'of', 'the', 'barpartialneumann', 'operator', 'n_q', 'on', 'omega', 'we', 'prove', 'that... | [-0.159990119124164, 0.048279587189037035, -0.07250397312288571, 0.05986073147713406, -0.1153207808404529, -0.08302538250323518, 0.008500382154514747, 0.38728277437413844, -0.255875779681706, -0.17236667371720873, 0.16237410413928696, -0.27913881299485055, -0.10810644269388701, 0.24295317319151113, -0.12225092130912733... |
706.2646 | A quantitative version of the Besicovitch projection theorem via
multiscale analysis | By using a multiscale analysis, we establish quantitative versions of the
Besicovitch projection theorem (almost every projection of a purely
unrectifiable set in the plane of finite length has measure zero) and a
standard companion result, namely that any planar set with at least two
projections of measure zero is p... | math.CA math.MG | by using a multiscale analysis we establish quantitative versions of the besicovitch projection theorem almost every projection of a purely unrectifiable set in the plane of finite length has measure zero and a standard companion result namely that any planar set with at least two projections of measure zero is purely ... | [['by', 'using', 'a', 'multiscale', 'analysis', 'we', 'establish', 'quantitative', 'versions', 'of', 'the', 'besicovitch', 'projection', 'theorem', 'almost', 'every', 'projection', 'of', 'a', 'purely', 'unrectifiable', 'set', 'in', 'the', 'plane', 'of', 'finite', 'length', 'has', 'measure', 'zero', 'and', 'a', 'standar... | [-0.15058144052246852, 0.08400621477007267, -0.12709556676011968, 0.04714394373631758, -0.019679139731089017, -0.08452142147323141, 0.07469978426014642, 0.30238692308836557, -0.2677556797378249, -0.21594986752546452, 0.14405014964467663, -0.3035531350072812, -0.09156452972659623, 0.21967585093353864, -0.050252209199810... |
706.2647 | A note for Gromov's distance functions on the space of mm-spaces | This is just a note for \cite[Chapter$3{1/2}_+$]{gromov}. Maybe this note is
obvious for a reader who knows metric geometry. I wish that someone study
further in this direction.
| math.MG | this is just a note for citechapter312_gromov maybe this note is obvious for a reader who knows metric geometry i wish that someone study further in this direction | [['this', 'is', 'just', 'a', 'note', 'for', 'citechapter312_gromov', 'maybe', 'this', 'note', 'is', 'obvious', 'for', 'a', 'reader', 'who', 'knows', 'metric', 'geometry', 'i', 'wish', 'that', 'someone', 'study', 'further', 'in', 'this', 'direction']] | [-0.1189486196057664, 0.02758302038569969, -0.15465409543227265, 0.12668080984494062, -0.2261940246378934, -0.24177067261189222, 0.06673686903108049, 0.4352878817805537, -0.26502575049245797, -0.22457640017900202, 0.07015827568506615, -0.3062763538349558, -0.2376750542057885, 0.07544745339287652, -0.23691970337596205, ... |
706.2648 | Harder-Narasimhan categories | We propose a generalization of Quillen's exact category -- arithmetic exact
category and we discuss conditions on such categories under which one can
establish the notion of Harder-Narasimhan filtrations and Harder-Narsimhan
polygons. Furthermore, we show the functoriality of Harder-Narasimhan
filtrations (indexed by... | math.AG math.CT | we propose a generalization of quillens exact category arithmetic exact category and we discuss conditions on such categories under which one can establish the notion of hardernarasimhan filtrations and hardernarsimhan polygons furthermore we show the functoriality of hardernarasimhan filtrations indexed by mathbb r wh... | [['we', 'propose', 'a', 'generalization', 'of', 'quillens', 'exact', 'category', 'arithmetic', 'exact', 'category', 'and', 'we', 'discuss', 'conditions', 'on', 'such', 'categories', 'under', 'which', 'one', 'can', 'establish', 'the', 'notion', 'of', 'hardernarasimhan', 'filtrations', 'and', 'hardernarsimhan', 'polygons... | [-0.141659238608554, 0.019845526848387505, -0.13497881942229079, 0.15173665713518858, -0.09569367052504926, -0.16222920271268645, 0.010719231213442981, 0.3791776904836297, -0.41103350850088255, -0.21034737520052918, 0.0891941351832689, -0.13057526219303586, -0.1743994079131101, 0.17598449891167028, -0.2943043270830198,... |
706.2649 | Convergence of Harder-Narasimhan polygons | We establish in this article convergence results of normalized
Harder-Narasimhan polygons both in geometric and in arithmetic frameworks by
introducing the Harder-Narasimhan filtration indexed by $\mathbb R$ and the
associated Borel probability measure.
| math.AG | we establish in this article convergence results of normalized hardernarasimhan polygons both in geometric and in arithmetic frameworks by introducing the hardernarasimhan filtration indexed by mathbb r and the associated borel probability measure | [['we', 'establish', 'in', 'this', 'article', 'convergence', 'results', 'of', 'normalized', 'hardernarasimhan', 'polygons', 'both', 'in', 'geometric', 'and', 'in', 'arithmetic', 'frameworks', 'by', 'introducing', 'the', 'hardernarasimhan', 'filtration', 'indexed', 'by', 'mathbb', 'r', 'and', 'the', 'associated', 'borel... | [-0.1566399305381558, 0.054520774562137594, -0.11874797732117727, 0.06636355126939827, -0.017389204776422543, -0.11992883462120187, 0.05697761097866477, 0.3759671914758104, -0.3828439735101931, -0.15653499907277751, 0.09835506046092081, -0.22821340213219324, -0.15724601145043518, 0.1477363153332562, -0.276141780259257,... |
706.265 | Comment on "Magnus force and acoustic Stewart-Tolman effect in type-II
superconductors, by Fil et al | Fil {\it et al.} has proposed an interesting experimental method to
investigate vortex dynamics. Some preliminary results have been obtained. In
this comment I discuss a few missing but strongly related theoretical models
and experiments on Hall anomaly and Magnus force. I conclude that those missing
literature can e... | cond-mat.supr-con cond-mat.stat-mech | fil it et al has proposed an interesting experimental method to investigate vortex dynamics some preliminary results have been obtained in this comment i discuss a few missing but strongly related theoretical models and experiments on hall anomaly and magnus force i conclude that those missing literature can enhance th... | [['fil', 'it', 'et', 'al', 'has', 'proposed', 'an', 'interesting', 'experimental', 'method', 'to', 'investigate', 'vortex', 'dynamics', 'some', 'preliminary', 'results', 'have', 'been', 'obtained', 'in', 'this', 'comment', 'i', 'discuss', 'a', 'few', 'missing', 'but', 'strongly', 'related', 'theoretical', 'models', 'an... | [-0.06910714588767446, 0.0805963984668453, -0.08173021988911944, 0.016825814152817562, -0.13526177595355618, -0.13806991300670735, 0.031090078708618435, 0.378886208132799, -0.20160912183884866, -0.35773641279717877, 0.05309381885732065, -0.2777111252366718, -0.25164396514587883, 0.22403070942234637, -0.1447001376481198... |
706.2651 | Transverse emittance dilution due to coupler kicks in linear
accelerators | One of the main concerns in the design of low emittance linear accelerators
(linacs) is the preservation of beam emittance. Here we discuss one possible
source of emittance dilution, the coupler kick, due to transverse
electromagnetic fields in the accelerating cavities of the linac caused by the
power coupler geomet... | physics.acc-ph physics.comp-ph | one of the main concerns in the design of low emittance linear accelerators linacs is the preservation of beam emittance here we discuss one possible source of emittance dilution the coupler kick due to transverse electromagnetic fields in the accelerating cavities of the linac caused by the power coupler geometry in a... | [['one', 'of', 'the', 'main', 'concerns', 'in', 'the', 'design', 'of', 'low', 'emittance', 'linear', 'accelerators', 'linacs', 'is', 'the', 'preservation', 'of', 'beam', 'emittance', 'here', 'we', 'discuss', 'one', 'possible', 'source', 'of', 'emittance', 'dilution', 'the', 'coupler', 'kick', 'due', 'to', 'transverse',... | [-0.17539110105554823, 0.16217242589547537, -0.043129127957494295, 0.010973070684309688, -0.06484620846343965, -0.19904464259192908, 0.004717616915976542, 0.4378737287001691, -0.2478244269006355, -0.2740449078137382, 0.1015204143556883, -0.2514279820292013, -0.046628105223402515, 0.25476367636516983, -0.062011903543363... |
706.2652 | The Spectrum of the Black Hole X-ray Nova V404 Cygni in Quiescence as
Measured by XMM-Newton | We present XMM observations of the black hole X-ray nova V404 Cygni in
quiescence. Its quiescent spectrum can be best fitted by a simple power-law
with slope 2. The spectra are consistent with that expected for the
advection-dominated accretion flow (ADAF). V404 Cyg was roughly equal in
luminosity compared to the pre... | astro-ph | we present xmm observations of the black hole xray nova v404 cygni in quiescence its quiescent spectrum can be best fitted by a simple powerlaw with slope 2 the spectra are consistent with that expected for the advectiondominated accretion flow adaf v404 cyg was roughly equal in luminosity compared to the previous obse... | [['we', 'present', 'xmm', 'observations', 'of', 'the', 'black', 'hole', 'xray', 'nova', 'v404', 'cygni', 'in', 'quiescence', 'its', 'quiescent', 'spectrum', 'can', 'be', 'best', 'fitted', 'by', 'a', 'simple', 'powerlaw', 'with', 'slope', '2', 'the', 'spectra', 'are', 'consistent', 'with', 'that', 'expected', 'for', 'th... | [-0.025798951144202338, 0.10168322706289712, -0.05303825438404303, 0.07176036706201916, -0.054626097137368, -0.12022465325464479, 0.08635477514624534, 0.4233600215329865, -0.13284284187496076, -0.3913639516065844, 0.10558543689587138, -0.36669844358426623, -0.00917457879309115, 0.2327858331674313, -0.021651734899515745... |
706.2653 | The UDF05 Follow-up of the HUDF: I. The Faint-End Slope of the
Lyman-Break Galaxy Population at z~5 | We present the UDF05 project, a HST Large Program of deep ACS (F606W, F775W,
F850LP) and NICMOS (F110W, F160W) imaging of three fields, two of which
coincide with the NICP1-4 NICMOS parallel observations of the Hubble Ultra Deep
Field (HUDF). In this first paper we use the ACS data for the NICP12 field, as
well as th... | astro-ph | we present the udf05 project a hst large program of deep acs f606w f775w f850lp and nicmos f110w f160w imaging of three fields two of which coincide with the nicp14 nicmos parallel observations of the hubble ultra deep field hudf in this first paper we use the acs data for the nicp12 field as well as the original hudf ... | [['we', 'present', 'the', 'udf05', 'project', 'a', 'hst', 'large', 'program', 'of', 'deep', 'acs', 'f606w', 'f775w', 'f850lp', 'and', 'nicmos', 'f110w', 'f160w', 'imaging', 'of', 'three', 'fields', 'two', 'of', 'which', 'coincide', 'with', 'the', 'nicp14', 'nicmos', 'parallel', 'observations', 'of', 'the', 'hubble', 'u... | [0.00028470386968751393, 0.04690419656117555, -0.09842646795512586, 0.10819952289419744, -0.10916868209915918, -0.05588343461285339, 0.0649034980769946, 0.46966487119684547, -0.12783030324352557, -0.3858385621084289, 0.03610726730544589, -0.2890780885157799, -0.0319542011043824, 0.1784132268814129, -0.01770898441427300... |
706.2654 | Reconstructing a model of quintessential inflation | We present an explicit cosmological model where inflation and dark energy
both could arise from the dynamics of the same scalar field. We present our
discussion in the framework where the inflaton field $\phi$ attains a nearly
constant velocity $m_P^{-1} |d\phi/dN|\equiv \alpha+\beta \exp(\beta N)$ (where
$N\equiv \l... | hep-th astro-ph gr-qc hep-ph | we present an explicit cosmological model where inflation and dark energy both could arise from the dynamics of the same scalar field we present our discussion in the framework where the inflaton field phi attains a nearly constant velocity m_p1 dphidnequiv alphabeta expbeta n where nequiv ln a is the efolding time dur... | [['we', 'present', 'an', 'explicit', 'cosmological', 'model', 'where', 'inflation', 'and', 'dark', 'energy', 'both', 'could', 'arise', 'from', 'the', 'dynamics', 'of', 'the', 'same', 'scalar', 'field', 'we', 'present', 'our', 'discussion', 'in', 'the', 'framework', 'where', 'the', 'inflaton', 'field', 'phi', 'attains',... | [-0.16369065200132843, 0.2227047846503386, -0.10928739644957101, 0.09857286973347554, -0.06900981774504315, -0.1609258384394478, -0.043899373888401996, 0.29829801374812, -0.2176643954404932, -0.3406108044926694, 0.0756730219882771, -0.22212820674989694, -0.05572430741208426, 0.1609892406337432, 0.021738369930658908, -0... |
706.2655 | Stability of string configurations dual to quarkonium states in AdS/CFT | We extend our earlier work, regarding the perturbative stability of string
configurations used for computing the interaction potential of heavy quarks
within the gauge/gravity correspondence, to cover a more general class of
gravity duals. We provide results, mostly based on analytic methods and
corroborated by numer... | hep-th | we extend our earlier work regarding the perturbative stability of string configurations used for computing the interaction potential of heavy quarks within the gaugegravity correspondence to cover a more general class of gravity duals we provide results mostly based on analytic methods and corroborated by numerical ca... | [['we', 'extend', 'our', 'earlier', 'work', 'regarding', 'the', 'perturbative', 'stability', 'of', 'string', 'configurations', 'used', 'for', 'computing', 'the', 'interaction', 'potential', 'of', 'heavy', 'quarks', 'within', 'the', 'gaugegravity', 'correspondence', 'to', 'cover', 'a', 'more', 'general', 'class', 'of', ... | [-0.14127506910651727, 0.13108190306348655, -0.07880558749138002, 0.08880390799454582, -0.04840727305388329, -0.12269072440229574, 0.04647230758496468, 0.3275685971153475, -0.16808988219120252, -0.2407051607209383, 0.08427194926590925, -0.25006724748902065, -0.12235092340658109, 0.20059755380668443, -0.0412525808008398... |
706.2656 | Dynamical Properties of z~2 Star Forming Galaxies and a Universal Star
Formation Relation | We present the first comparison of the dynamical properties of different
samples of z~1.4-3.4 star forming galaxies from spatially resolved imaging
spectroscopy from SINFONI/VLT integral field spectroscopy and IRAM CO
millimeter interferometry. Our samples include 16 rest-frame UV-selected, 16
rest-frame optically-se... | astro-ph | we present the first comparison of the dynamical properties of different samples of z1434 star forming galaxies from spatially resolved imaging spectroscopy from sinfonivlt integral field spectroscopy and iram co millimeter interferometry our samples include 16 restframe uvselected 16 restframe opticallyselected and 13... | [['we', 'present', 'the', 'first', 'comparison', 'of', 'the', 'dynamical', 'properties', 'of', 'different', 'samples', 'of', 'z1434', 'star', 'forming', 'galaxies', 'from', 'spatially', 'resolved', 'imaging', 'spectroscopy', 'from', 'sinfonivlt', 'integral', 'field', 'spectroscopy', 'and', 'iram', 'co', 'millimeter', '... | [-0.05491468160873323, 0.15949500092482638, -0.10149470924931978, 0.11864915080978314, -0.07744976023123377, -0.056263184978161004, 0.01207841011762087, 0.4715082087886653, -0.07376701066359168, -0.3642106053020273, 0.030574105627879145, -0.2977989220370849, 0.007497241040913477, 0.155229775059048, 0.02946689660173087,... |
706.2657 | Self-consistent slave rotor mean field theory for strongly correlated
systems | Building on work by Florens and Georges, we formulate and study a
self-consistent slave rotor mean field theory for strongly correlated systems.
This approach views the electron, in the strong correlation regime, as a
composite of a neutral spinon and a charged rotor field. We solve the coupled
spinon-rotor model sel... | cond-mat.str-el cond-mat.supr-con | building on work by florens and georges we formulate and study a selfconsistent slave rotor mean field theory for strongly correlated systems this approach views the electron in the strong correlation regime as a composite of a neutral spinon and a charged rotor field we solve the coupled spinonrotor model selfconsiste... | [['building', 'on', 'work', 'by', 'florens', 'and', 'georges', 'we', 'formulate', 'and', 'study', 'a', 'selfconsistent', 'slave', 'rotor', 'mean', 'field', 'theory', 'for', 'strongly', 'correlated', 'systems', 'this', 'approach', 'views', 'the', 'electron', 'in', 'the', 'strong', 'correlation', 'regime', 'as', 'a', 'co... | [-0.16235645952380123, 0.25192019377222835, -0.020633584342215693, 0.07390668105627238, -0.019580443070649548, -0.16332279842916048, 0.09330563859623874, 0.35892419315684865, -0.20177745818229462, -0.27772097165385884, -0.017663268098085945, -0.33745361758930675, -0.13068402456162773, 0.15556654349698132, 0.02730907769... |
706.2658 | Local and Non-local Shot Noise in Multiwalled Carbon Nanotubes | We have investigated shot noise in multiterminal, diffusive multiwalled
carbon nanotubes (MWNTs) at 4.2 K over the frequency f = 600 - 850 MHz.
Quantitative comparison of our data to semiclassical theory, based on
non-equilibrium distribution functions, indicates that a major part of the
noise is caused by a non-equi... | cond-mat.mes-hall | we have investigated shot noise in multiterminal diffusive multiwalled carbon nanotubes mwnts at 42 k over the frequency f 600 850 mhz quantitative comparison of our data to semiclassical theory based on nonequilibrium distribution functions indicates that a major part of the noise is caused by a nonequilibrium state i... | [['we', 'have', 'investigated', 'shot', 'noise', 'in', 'multiterminal', 'diffusive', 'multiwalled', 'carbon', 'nanotubes', 'mwnts', 'at', '42', 'k', 'over', 'the', 'frequency', 'f', '600', '850', 'mhz', 'quantitative', 'comparison', 'of', 'our', 'data', 'to', 'semiclassical', 'theory', 'based', 'on', 'nonequilibrium', ... | [-0.17908634736303644, 0.10628820126539612, -0.051109192769480755, -0.0023387247761038235, 0.03491499794490007, -0.1723773690467947, 0.1270358639766451, 0.3964999481497041, -0.23543325843042637, -0.2970847693013858, -0.00047683571773884167, -0.33340847599937257, -0.11554660965374346, 0.19297566547069744, -0.05569248170... |
706.2659 | Selection and identity rules for subductions of type A quantum
Iwahori-Hecke algebras | This paper is concerned with the subduction problem of type A quantum
Iwahori-Hecke algebras $\mathbb{C} \mathbf{H}(\mathfrak{S}_f,q^2)$ with a real
deformation parameter $q$, i.e. the problem of decomposing irreducible
representations of such algebras as direct sum of irreducible representations
of the subalgebras $... | math-ph hep-th math.MP | this paper is concerned with the subduction problem of type a quantum iwahorihecke algebras mathbbc mathbfhmathfraks_fq2 with a real deformation parameter q ie the problem of decomposing irreducible representations of such algebras as direct sum of irreducible representations of the subalgebras mathbbcmathbfhmathfraks_... | [['this', 'paper', 'is', 'concerned', 'with', 'the', 'subduction', 'problem', 'of', 'type', 'a', 'quantum', 'iwahorihecke', 'algebras', 'mathbbc', 'mathbfhmathfraks_fq2', 'with', 'a', 'real', 'deformation', 'parameter', 'q', 'ie', 'the', 'problem', 'of', 'decomposing', 'irreducible', 'representations', 'of', 'such', 'a... | [-0.14553399678414403, 0.09268017876826688, -0.04107379674185383, 0.02678575974660215, -0.1083816980303786, -0.11109511875912499, 0.0091764377676724, 0.3450353448042425, -0.3241637358954966, -0.18047709164793713, 0.13184125663740245, -0.22148968664728505, -0.12354016787509663, 0.18751380776481355, -0.05770492885494605,... |
706.266 | Stability of half-quantum vorticies in p_x+ip_y superconductors | We consider the stability conditions for half-quantum vortices in quasi two
dimensional $p_x+ip_y$ superconductor (such as ${\rm Sr_2 RuO_4}$ is believed
to be) through energetics calculations. Although the predicted exotic nature of
these excitations have recently attracted much attention but they have not been
obse... | cond-mat.supr-con cond-mat.str-el | we consider the stability conditions for halfquantum vortices in quasi two dimensional p_xip_y superconductor such as rm sr_2 ruo_4 is believed to be through energetics calculations although the predicted exotic nature of these excitations have recently attracted much attention but they have not been observed yet we pa... | [['we', 'consider', 'the', 'stability', 'conditions', 'for', 'halfquantum', 'vortices', 'in', 'quasi', 'two', 'dimensional', 'p_xip_y', 'superconductor', 'such', 'as', 'rm', 'sr_2', 'ruo_4', 'is', 'believed', 'to', 'be', 'through', 'energetics', 'calculations', 'although', 'the', 'predicted', 'exotic', 'nature', 'of', ... | [-0.17746200071182103, 0.23471134471018254, -0.058857050876443585, 0.07394070112379268, -0.07027748378148924, -0.15696838659855228, 0.009807005783853432, 0.3775987751036882, -0.2162867652469625, -0.2751567743656536, 0.04213065039754535, -0.2803162442147732, -0.09632717730477453, 0.15575438853198043, 0.01330678562986577... |
706.2661 | Einstein, incompleteness, and the epistemic view of quantum states | Does the quantum state represent reality or our knowledge of reality? In
making this distinction precise, we are led to a novel classification of hidden
variable models of quantum theory. Indeed, representatives of each class can be
found among existing constructions for two-dimensional Hilbert spaces. Our
approach a... | quant-ph | does the quantum state represent reality or our knowledge of reality in making this distinction precise we are led to a novel classification of hidden variable models of quantum theory indeed representatives of each class can be found among existing constructions for twodimensional hilbert spaces our approach also prov... | [['does', 'the', 'quantum', 'state', 'represent', 'reality', 'or', 'our', 'knowledge', 'of', 'reality', 'in', 'making', 'this', 'distinction', 'precise', 'we', 'are', 'led', 'to', 'a', 'novel', 'classification', 'of', 'hidden', 'variable', 'models', 'of', 'quantum', 'theory', 'indeed', 'representatives', 'of', 'each', ... | [-0.0789805056244534, 0.08363603766082343, -0.16247873010298053, 0.10840647567414095, -0.12379340458326143, -0.178880285804293, 0.07718752986357476, 0.30553242491537724, -0.23699445304317543, -0.2975737970363308, 0.06763814474778393, -0.2470443837528864, -0.17050942837562577, 0.19919400998380976, -0.13884237948370134, ... |
706.2662 | On the stabilization of ion sputtered surfaces | The classical theory of ion beam sputtering predicts the instability of a
flat surface to uniform ion irradiation at any incidence angle. We relax the
assumption of the classical theory that the average surface erosion rate is
determined by a Gaussian response function representing the effect of the
collision cascade... | cond-mat.mtrl-sci cond-mat.other | the classical theory of ion beam sputtering predicts the instability of a flat surface to uniform ion irradiation at any incidence angle we relax the assumption of the classical theory that the average surface erosion rate is determined by a gaussian response function representing the effect of the collision cascade an... | [['the', 'classical', 'theory', 'of', 'ion', 'beam', 'sputtering', 'predicts', 'the', 'instability', 'of', 'a', 'flat', 'surface', 'to', 'uniform', 'ion', 'irradiation', 'at', 'any', 'incidence', 'angle', 'we', 'relax', 'the', 'assumption', 'of', 'the', 'classical', 'theory', 'that', 'the', 'average', 'surface', 'erosi... | [-0.10997365580559684, 0.17074231531584474, -0.11660890984656241, 0.06233921695351695, -0.007292726143324739, -0.12653521599181866, 0.030966561269913304, 0.36567586263272966, -0.2703624354476856, -0.2885114530067144, 0.06301755042567017, -0.2581050358523572, -0.13518183380436286, 0.2131470769152121, -0.0116009918883026... |
706.2663 | Chandra ACIS Survey of M33 (ChASeM33): X-ray Imaging Spectroscopy of
M33SNR21, the Brightest X-ray Supernova Remnant in M33 | We present and interpret new X-ray data for M33SNR21, the brightest X-ray
supernova remnant (SNR) in M33. The SNR is in seen projection against (and
appears to be interacting with) the bright HII region NGC592. Data for this
source were obtained as part of the Chandra ACIS Survey of M33 (ChASeM33) Very
Large Project.... | astro-ph | we present and interpret new xray data for m33snr21 the brightest xray supernova remnant snr in m33 the snr is in seen projection against and appears to be interacting with the bright hii region ngc592 data for this source were obtained as part of the chandra acis survey of m33 chasem33 very large project the nearly on... | [['we', 'present', 'and', 'interpret', 'new', 'xray', 'data', 'for', 'm33snr21', 'the', 'brightest', 'xray', 'supernova', 'remnant', 'snr', 'in', 'm33', 'the', 'snr', 'is', 'in', 'seen', 'projection', 'against', 'and', 'appears', 'to', 'be', 'interacting', 'with', 'the', 'bright', 'hii', 'region', 'ngc592', 'data', 'fo... | [-0.04102529728712574, 0.11522659660446144, -0.0285660368739156, 0.10336466700353317, -0.04136868096088712, -0.08015611533854188, 0.04956961795404885, 0.4766973105866296, -0.12517197369993757, -0.39008392518393786, 0.06798742622229448, -0.3631262568123488, 0.12246806596651831, 0.1759782975001321, -0.022542769914263905,... |
706.2664 | On the connected component of compact composition operators on the Hardy
space | We show that there exist non-compact composition operators in the connected
component of the compact ones on the classical Hardy space $H^2$ on the unit
disc. This answers a question posed by Shapiro and Sundberg in 1990. We also
establish an improved version of a theorem of MacCluer, giving a lower bound
for the ess... | math.FA math.CV | we show that there exist noncompact composition operators in the connected component of the compact ones on the classical hardy space h2 on the unit disc this answers a question posed by shapiro and sundberg in 1990 we also establish an improved version of a theorem of maccluer giving a lower bound for the essential no... | [['we', 'show', 'that', 'there', 'exist', 'noncompact', 'composition', 'operators', 'in', 'the', 'connected', 'component', 'of', 'the', 'compact', 'ones', 'on', 'the', 'classical', 'hardy', 'space', 'h2', 'on', 'the', 'unit', 'disc', 'this', 'answers', 'a', 'question', 'posed', 'by', 'shapiro', 'and', 'sundberg', 'in',... | [-0.14510413848712475, 0.07663958150575886, -0.07064914500931738, 0.11070385959465057, -0.04320944781426953, -0.04887880440919271, 0.07313983283842666, 0.32079566525268854, -0.2376212622923187, -0.2525153524372019, 0.12763871701988333, -0.24532040085384174, -0.1371268154169091, 0.2421135764474733, -0.1353452638457706, ... |
706.2665 | Higgs Pair Production at the LHC in Models with Universal Extra
Dimensions | In this letter we study the process of gluon fusion into a pair of Higgs
bosons in a model with one universal extra dimension. We find that the
contributions from the extra top quark Kaluza-Klein excitations lead to a Higgs
pair production cross section at the LHC that can be significantly altered
compared to the Sta... | hep-ph | in this letter we study the process of gluon fusion into a pair of higgs bosons in a model with one universal extra dimension we find that the contributions from the extra top quark kaluzaklein excitations lead to a higgs pair production cross section at the lhc that can be significantly altered compared to the standar... | [['in', 'this', 'letter', 'we', 'study', 'the', 'process', 'of', 'gluon', 'fusion', 'into', 'a', 'pair', 'of', 'higgs', 'bosons', 'in', 'a', 'model', 'with', 'one', 'universal', 'extra', 'dimension', 'we', 'find', 'that', 'the', 'contributions', 'from', 'the', 'extra', 'top', 'quark', 'kaluzaklein', 'excitations', 'lea... | [-0.045868028746917845, 0.24125903678628113, -0.09418201751004045, 0.126276678573301, -0.043645082328182, -0.15654614131826047, 0.04580488938551683, 0.2823830489355784, -0.24279348728461908, -0.23774701730491452, -0.01781779757271019, -0.2877246853107443, -0.032946025121670504, 0.13901111010032205, 0.0336414055325664, ... |
706.2666 | On singular cubic surfaces | We study global log canonical thresholds of cubic surfaces with canonical
singularities, and we prove the existence of a Kahler-Einstein metric on two
singular cubic surfaces.
| math.AG math.DG | we study global log canonical thresholds of cubic surfaces with canonical singularities and we prove the existence of a kahlereinstein metric on two singular cubic surfaces | [['we', 'study', 'global', 'log', 'canonical', 'thresholds', 'of', 'cubic', 'surfaces', 'with', 'canonical', 'singularities', 'and', 'we', 'prove', 'the', 'existence', 'of', 'a', 'kahlereinstein', 'metric', 'on', 'two', 'singular', 'cubic', 'surfaces']] | [-0.2707478411209125, -0.012852159678004682, -0.10925170535651538, 0.13675666428529298, -0.08023911248892546, -0.1602116116644958, 0.007470024212335165, 0.3521317997947335, -0.19936302630230784, -0.1766823374737914, 0.06144670479429456, -0.34008125523821664, -0.2519216656398315, 0.147014723231013, -0.10448527060305843,... |
706.2667 | Longitudinal double spin asymmetry in jet production at STAR | We present recent measurements of the longitudinal double-spin asymmetry A_LL
for the inclusive production of jets at midrapidity in polarized proton-proton
collisions at sqrt(s)=200GeV. The data amount to an integrated luminosity of
3pb-1 and were collected with the STAR detector at the Relativistic Heavy Ion
Collid... | hep-ex | we present recent measurements of the longitudinal doublespin asymmetry a_ll for the inclusive production of jets at midrapidity in polarized protonproton collisions at sqrts200gev the data amount to an integrated luminosity of 3pb1 and were collected with the star detector at the relativistic heavy ion collider during... | [['we', 'present', 'recent', 'measurements', 'of', 'the', 'longitudinal', 'doublespin', 'asymmetry', 'a_ll', 'for', 'the', 'inclusive', 'production', 'of', 'jets', 'at', 'midrapidity', 'in', 'polarized', 'protonproton', 'collisions', 'at', 'sqrts200gev', 'the', 'data', 'amount', 'to', 'an', 'integrated', 'luminosity', ... | [-0.04544586212858746, 0.21238697543308124, -0.11685713379164085, 0.06952223154443382, -0.027307767042363384, -0.065527654083615, -0.04829975306479768, 0.3942526942401221, -0.15844773073125668, -0.3343573409424286, -0.02600768084444971, -0.4202222701237358, 0.1796713696388208, 0.17423500547025617, 0.08014962753525587, ... |
706.2668 | A jelly model for a ball of an extremely hot plasma | A simple model is applied to study a high temperature rather dense plasma
ball. It is assumed that the ions and delocalized electrons are distributed
uniformly throughout the ball, and extra/missing charge is found in a thin
layer on the surface of a ball. It is shown in the framework of this model that
regarded plas... | physics.plasm-ph physics.ao-ph | a simple model is applied to study a high temperature rather dense plasma ball it is assumed that the ions and delocalized electrons are distributed uniformly throughout the ball and extramissing charge is found in a thin layer on the surface of a ball it is shown in the framework of this model that regarded plasma bal... | [['a', 'simple', 'model', 'is', 'applied', 'to', 'study', 'a', 'high', 'temperature', 'rather', 'dense', 'plasma', 'ball', 'it', 'is', 'assumed', 'that', 'the', 'ions', 'and', 'delocalized', 'electrons', 'are', 'distributed', 'uniformly', 'throughout', 'the', 'ball', 'and', 'extramissing', 'charge', 'is', 'found', 'in'... | [-0.09478147669662056, 0.21697409139299878, -0.11140698434937062, 0.07166037839072358, 0.008892533169793231, -0.14327278063746587, 0.02060769306381746, 0.3947119428491106, -0.2636747322406392, -0.22724332432357633, 0.06168530721511996, -0.25955174116379753, -0.0793579326353359, 0.15803392584392878, -0.06012292992209597... |
706.2669 | A search for possible anisotropies of cosmic rays with 0.1<E<10 EeV in
the region of the Galactic Centre | We present updated results for anisotropy searches in the direction of the
Galactic Center (GC) at energies in the ranges: 0.1<E<1 EeV and 1<E<10 EeV. We
use data from the Pierre Auger Observatory up to March, 2007. Present analyzes
are therefore based on a substantially larger data set than our previous
published re... | astro-ph | we present updated results for anisotropy searches in the direction of the galactic center gc at energies in the ranges 01e1 eev and 1e10 eev we use data from the pierre auger observatory up to march 2007 present analyzes are therefore based on a substantially larger data set than our previous published results a limit... | [['we', 'present', 'updated', 'results', 'for', 'anisotropy', 'searches', 'in', 'the', 'direction', 'of', 'the', 'galactic', 'center', 'gc', 'at', 'energies', 'in', 'the', 'ranges', '01e1', 'eev', 'and', '1e10', 'eev', 'we', 'use', 'data', 'from', 'the', 'pierre', 'auger', 'observatory', 'up', 'to', 'march', '2007', 'p... | [-0.0246434947301168, 0.1709376218961552, -0.0289286968880333, 0.1305508046178147, -0.08686162467347458, -0.00980133776902221, 0.07657276969985105, 0.39259062688797713, -0.15060998353292235, -0.42513794943224636, 0.045298278963309714, -0.38121237557497806, 0.02870845147408545, 0.26474960402119907, 0.03186098314472474, ... |
706.267 | Correlation Functions of Asymmetric Real Matrices | We give a closed form for the correlation functions of ensembles of
asymmetric real matrices in terms of the Pfaffian of an antisymmetric matrix
formed from a $2 \times 2$ matrix kernel associated to the ensemble. We also
derive closed forms for the matrix kernel and correlation functions for
Ginibre's real ensemble.... | math-ph math.MP | we give a closed form for the correlation functions of ensembles of asymmetric real matrices in terms of the pfaffian of an antisymmetric matrix formed from a 2 times 2 matrix kernel associated to the ensemble we also derive closed forms for the matrix kernel and correlation functions for ginibres real ensemble | [['we', 'give', 'a', 'closed', 'form', 'for', 'the', 'correlation', 'functions', 'of', 'ensembles', 'of', 'asymmetric', 'real', 'matrices', 'in', 'terms', 'of', 'the', 'pfaffian', 'of', 'an', 'antisymmetric', 'matrix', 'formed', 'from', 'a', '2', 'times', '2', 'matrix', 'kernel', 'associated', 'to', 'the', 'ensemble', ... | [-0.12246302196469444, 0.1074619487651664, -0.04785172406655665, 0.11897208745806263, 0.04491244170528192, -0.07568119226310116, -0.010583869727829901, 0.38091671008330125, -0.23063612438720435, -0.1910081424195176, 0.09109882599127908, -0.2824731239547523, -0.24061716195697394, 0.15318180796636555, 0.07912740756112796... |
706.2671 | Monte Carlo Simulations of an Extended Feynman-Kikuchi Model | We present Quantum Monte Carlo simulations of a generalization of the
Feynman-Kikuchi model which includes the possibility of vacancies and
interactions between the particles undergoing exchange. By measuring the
winding number (superfluid density) and density structure factor, we determine
the phase diagram, and sho... | cond-mat.stat-mech | we present quantum monte carlo simulations of a generalization of the feynmankikuchi model which includes the possibility of vacancies and interactions between the particles undergoing exchange by measuring the winding number superfluid density and density structure factor we determine the phase diagram and show that i... | [['we', 'present', 'quantum', 'monte', 'carlo', 'simulations', 'of', 'a', 'generalization', 'of', 'the', 'feynmankikuchi', 'model', 'which', 'includes', 'the', 'possibility', 'of', 'vacancies', 'and', 'interactions', 'between', 'the', 'particles', 'undergoing', 'exchange', 'by', 'measuring', 'the', 'winding', 'number',... | [-0.17047363811138053, 0.255040948641383, -0.09086347444314959, 0.043833544908988255, 0.03617109806725272, -0.08519323811762863, 0.0953413341453092, 0.3455721180610083, -0.23768321536826315, -0.36344603242145646, -0.017041535651380266, -0.3165587682828859, -0.1526929229773857, 0.0924163324094412, 0.10981550804097895, -... |
706.2672 | Using Three-Body Recombination to Extract Electron Temperatures of
Ultracold Plasmas | Three-body recombination, an important collisional process in plasmas,
increases dramatically at low electron temperatures, with an accepted scaling
of T_e^-9/2. We measure three-body recombination in an ultracold neutral xenon
plasma by detecting recombination-created Rydberg atoms using a
microwave-ionization techn... | physics.atom-ph physics.plasm-ph | threebody recombination an important collisional process in plasmas increases dramatically at low electron temperatures with an accepted scaling of t_e92 we measure threebody recombination in an ultracold neutral xenon plasma by detecting recombinationcreated rydberg atoms using a microwaveionization technique with the... | [['threebody', 'recombination', 'an', 'important', 'collisional', 'process', 'in', 'plasmas', 'increases', 'dramatically', 'at', 'low', 'electron', 'temperatures', 'with', 'an', 'accepted', 'scaling', 'of', 't_e92', 'we', 'measure', 'threebody', 'recombination', 'in', 'an', 'ultracold', 'neutral', 'xenon', 'plasma', 'b... | [-0.03404987255001769, 0.3037665193672771, -0.03282626387937104, 0.04947688892179405, 0.10246623978840516, -0.16189463039421859, 0.041407549834591065, 0.3739178072003757, -0.2012680869878215, -0.3006605929749854, -0.03461034362040022, -0.29464980727472506, 0.06262218361063039, 0.21081048979916994, 0.038088157652493786,... |
706.2673 | Le th\'eor\`eme de Riemann-Roch et ses applications | The Riemann-Roch theorem is of utmost importance in the algebraic geometric
theory of compact Riemann surfaces. It tells us how many linearly independent
meromorphic functions there are having certain restrictions on their poles. The
aim of this article is to present a simple direct proof of this theorem and
explore ... | math.CV math.AG | the riemannroch theorem is of utmost importance in the algebraic geometric theory of compact riemann surfaces it tells us how many linearly independent meromorphic functions there are having certain restrictions on their poles the aim of this article is to present a simple direct proof of this theorem and explore some ... | [['the', 'riemannroch', 'theorem', 'is', 'of', 'utmost', 'importance', 'in', 'the', 'algebraic', 'geometric', 'theory', 'of', 'compact', 'riemann', 'surfaces', 'it', 'tells', 'us', 'how', 'many', 'linearly', 'independent', 'meromorphic', 'functions', 'there', 'are', 'having', 'certain', 'restrictions', 'on', 'their', '... | [-0.18729748573855726, 0.04382937504076883, -0.18650389072340126, 0.14819619407901516, -0.17433578539760664, -0.09425756227612109, 0.04756496901255004, 0.29903026590389864, -0.2744967475436725, -0.23261690653207434, 0.12019412402869066, -0.2149370998059484, -0.2190167624140521, 0.28903522335186405, -0.1465231469868646,... |
706.2674 | The Lorenz number in CeCoIn$_5$ inferred from the thermal and charge
Hall currents | The thermal Hall conductivity $\kappa_{xy}$ and Hall conductivity
$\sigma_{xy}$ in CeCoIn$_5$ are used to determine the Lorenz number ${\cal
L}_H$ at low temperature $T$. This enables the separation of the observed
thermal conductivity into its electronic and non-electronic parts. We uncover
evidence for a charge-neu... | cond-mat.str-el cond-mat.supr-con | the thermal hall conductivity kappa_xy and hall conductivity sigma_xy in cecoin_5 are used to determine the lorenz number cal l_h at low temperature t this enables the separation of the observed thermal conductivity into its electronic and nonelectronic parts we uncover evidence for a chargeneutral fielddependent therm... | [['the', 'thermal', 'hall', 'conductivity', 'kappa_xy', 'and', 'hall', 'conductivity', 'sigma_xy', 'in', 'cecoin_5', 'are', 'used', 'to', 'determine', 'the', 'lorenz', 'number', 'cal', 'l_h', 'at', 'low', 'temperature', 't', 'this', 'enables', 'the', 'separation', 'of', 'the', 'observed', 'thermal', 'conductivity', 'in... | [-0.1812977394879316, 0.26693146686775804, -0.0763976170841341, -0.009929945745336061, -0.03523134149968474, -0.13118139082904567, 0.06679166608132572, 0.3272063047578088, -0.2781492756642025, -0.27756458226440833, -0.04222325958320965, -0.35815922031649433, -0.0959156382772507, 0.1856304557354312, 0.03156252799913137,... |
706.2675 | Optical vortices with starlight: Implications for ground-based stellar
coronagraphy | Using an l = 1 blazed fork-hologram at the focal plane of the Asiago 122 cm
telescope, we obtained optical vortices from the stellar system Rasalgethi
(alpha Herculis) and from the single star Arcturus (alpha Bootis). We have
analyzed the structure of the optical vortices obtained from non-monochromatic
starlight und... | physics.optics astro-ph physics.ins-det | using an l 1 blazed forkhologram at the focal plane of the asiago 122 cm telescope we obtained optical vortices from the stellar system rasalgethi alpha herculis and from the single star arcturus alpha bootis we have analyzed the structure of the optical vortices obtained from nonmonochromatic starlight under very poor... | [['using', 'an', 'l', '1', 'blazed', 'forkhologram', 'at', 'the', 'focal', 'plane', 'of', 'the', 'asiago', '122', 'cm', 'telescope', 'we', 'obtained', 'optical', 'vortices', 'from', 'the', 'stellar', 'system', 'rasalgethi', 'alpha', 'herculis', 'and', 'from', 'the', 'single', 'star', 'arcturus', 'alpha', 'bootis', 'we'... | [-0.10670380762038643, 0.0956282533632689, -0.11099391597792205, 0.026318029842942077, -0.07742390445919763, -0.14237852548317545, 0.04326146482472883, 0.4540427336058415, -0.20300782805733272, -0.33496244970079075, 0.10152785885849666, -0.28926676010493846, -0.09633295949521091, 0.23346288465579754, -0.066271851438453... |
706.2676 | D-term chaotic inflation in supergravity | Even though the chaotic inflation is one of the most popular inflation models
for its simple dynamics and compelling resolutions to the initial condition
problems, its realization in supergravity has been considered a challenging
task. We discuss how the chaotic inflation dominated by the D-term can be
induced in sup... | hep-ph astro-ph hep-th | even though the chaotic inflation is one of the most popular inflation models for its simple dynamics and compelling resolutions to the initial condition problems its realization in supergravity has been considered a challenging task we discuss how the chaotic inflation dominated by the dterm can be induced in supergra... | [['even', 'though', 'the', 'chaotic', 'inflation', 'is', 'one', 'of', 'the', 'most', 'popular', 'inflation', 'models', 'for', 'its', 'simple', 'dynamics', 'and', 'compelling', 'resolutions', 'to', 'the', 'initial', 'condition', 'problems', 'its', 'realization', 'in', 'supergravity', 'has', 'been', 'considered', 'a', 'c... | [-0.14187285628923701, 0.15960646538980425, -0.11407136878678723, 0.14620776445833997, -0.1087195531775554, -0.22453297266647929, -0.073402154067206, 0.3162717934298728, -0.2172617447758389, -0.26097568609411753, 0.1648555541510827, -0.1875052098036995, -0.2019896807060355, 0.1957147204028886, -0.13990339274621671, 0.0... |
706.2677 | Unparticles: Scales and High Energy Probes | Unparticles from hidden conformal sectors provide qualitatively new
possibilities for physics beyond the standard model. In the theoretical
framework of minimal models, we clarify the relation between energy scales
entering various phenomenological analyses. We show that these relations always
counteract the effectiv... | hep-ph hep-ex | unparticles from hidden conformal sectors provide qualitatively new possibilities for physics beyond the standard model in the theoretical framework of minimal models we clarify the relation between energy scales entering various phenomenological analyses we show that these relations always counteract the effective fie... | [['unparticles', 'from', 'hidden', 'conformal', 'sectors', 'provide', 'qualitatively', 'new', 'possibilities', 'for', 'physics', 'beyond', 'the', 'standard', 'model', 'in', 'the', 'theoretical', 'framework', 'of', 'minimal', 'models', 'we', 'clarify', 'the', 'relation', 'between', 'energy', 'scales', 'entering', 'vario... | [-0.1185764156450419, 0.2070994979770082, -0.06880602139479867, 0.1705381859972225, -0.11469986877116428, -0.17413027360051023, 0.03995595892183331, 0.3062209575020564, -0.24077278432886806, -0.3297770665428503, 0.05183895968650354, -0.296877443226342, -0.14166956545588205, 0.17590855457819998, 0.037745605904336385, 0.... |
706.2678 | CP-violation and unitarity triangle test of the Standard Model | Phenomenological issues of the CP violation in the quark sector of the
Standard Model are discussed. We consider quark mixing in the SM, standard and
Wolfenstein parametrization of the $CKM$ mixing matrix and unitarity triangle.
We discuss the phenomenology of the CP violation in $K^{0}_{L}$ and $B_{d}^{0}
(\bar B_{d... | hep-ph | phenomenological issues of the cp violation in the quark sector of the standard model are discussed we consider quark mixing in the sm standard and wolfenstein parametrization of the ckm mixing matrix and unitarity triangle we discuss the phenomenology of the cp violation in k0_l and b_d0 bar b_d0decays the standard un... | [['phenomenological', 'issues', 'of', 'the', 'cp', 'violation', 'in', 'the', 'quark', 'sector', 'of', 'the', 'standard', 'model', 'are', 'discussed', 'we', 'consider', 'quark', 'mixing', 'in', 'the', 'sm', 'standard', 'and', 'wolfenstein', 'parametrization', 'of', 'the', 'ckm', 'mixing', 'matrix', 'and', 'unitarity', '... | [-0.1331875007497249, 0.19133620197465132, -0.03807290760124778, 0.15488819283264393, -0.056134058510536676, -0.1646964886062011, 0.0897632670578557, 0.22967253309664326, -0.26013672243097574, -0.21729888116101642, 0.04554959341812019, -0.3170422757719899, -0.049940095559417544, 0.07435714598018471, 0.02375239634292793... |
706.2679 | Bounds on the concentration function in terms of Diophantine
approximation | We demonstrate a simple analytic argument that may be used to bound the Levy
concentration function of a sum of independent random variables. The main
application is a version of a recent inequality due to Rudelson and Vershynin,
and its multidimensional generalisation.
| math.PR | we demonstrate a simple analytic argument that may be used to bound the levy concentration function of a sum of independent random variables the main application is a version of a recent inequality due to rudelson and vershynin and its multidimensional generalisation | [['we', 'demonstrate', 'a', 'simple', 'analytic', 'argument', 'that', 'may', 'be', 'used', 'to', 'bound', 'the', 'levy', 'concentration', 'function', 'of', 'a', 'sum', 'of', 'independent', 'random', 'variables', 'the', 'main', 'application', 'is', 'a', 'version', 'of', 'a', 'recent', 'inequality', 'due', 'to', 'rudelso... | [-0.08037558127017248, 0.0671525108627975, -0.16076945628793465, 0.07875269383380544, -0.10831936094022933, -0.10487803123847005, 0.10833825893877518, 0.29020383798827726, -0.26607245823279735, -0.25343289634301547, 0.14401740262595317, -0.23379999523361525, -0.20283727755858785, 0.2190667133600939, -0.1634942552385231... |
706.268 | BPS Explained I: Temperature Relaxation in a Plasma | This is the first of two lectures on a new powerful technique employed by
Brown, Preston, and Singleton (BPS) to calculate transport quantities in a
plasma. This exposition will be self-contained and intended for those who are
not specialists in quantum field theory, where the technique of dimensional
continuation ex... | physics.plasm-ph hep-ph hep-th | this is the first of two lectures on a new powerful technique employed by brown preston and singleton bps to calculate transport quantities in a plasma this exposition will be selfcontained and intended for those who are not specialists in quantum field theory where the technique of dimensional continuation exploited b... | [['this', 'is', 'the', 'first', 'of', 'two', 'lectures', 'on', 'a', 'new', 'powerful', 'technique', 'employed', 'by', 'brown', 'preston', 'and', 'singleton', 'bps', 'to', 'calculate', 'transport', 'quantities', 'in', 'a', 'plasma', 'this', 'exposition', 'will', 'be', 'selfcontained', 'and', 'intended', 'for', 'those', ... | [-0.0797595134049862, 0.15679919160909886, -0.11676732585694509, 0.09721073196009558, -0.048644869115562914, -0.12985230921436725, 0.02541127524853963, 0.318470326228644, -0.20334431820733445, -0.292552460391585, 0.06310651189207955, -0.2740486139859437, -0.12350212509606771, 0.1955518236851821, -0.025291242218354177, ... |
706.2681 | Enhancing Mixing and Diffusion with Plastic Flow | We use numerical simulations to examine two-dimensional particle mixtures
that strongly phase separate in equilibrium. When the system is externally
driven in the presence of quenched disorder, plastic flow occurs in the form of
meandering and strongly mixing channels. In some cases this can produce a fast
and comple... | cond-mat.stat-mech cond-mat.soft | we use numerical simulations to examine twodimensional particle mixtures that strongly phase separate in equilibrium when the system is externally driven in the presence of quenched disorder plastic flow occurs in the form of meandering and strongly mixing channels in some cases this can produce a fast and complete mix... | [['we', 'use', 'numerical', 'simulations', 'to', 'examine', 'twodimensional', 'particle', 'mixtures', 'that', 'strongly', 'phase', 'separate', 'in', 'equilibrium', 'when', 'the', 'system', 'is', 'externally', 'driven', 'in', 'the', 'presence', 'of', 'quenched', 'disorder', 'plastic', 'flow', 'occurs', 'in', 'the', 'for... | [-0.1597442755497299, 0.28322651741507077, -0.047034393432875014, 0.04187346152084078, 0.03764181705408318, -0.10412829285920706, 0.03261087776356658, 0.38098168217165523, -0.28228089055804495, -0.2660854556164596, 0.09330917409550789, -0.25180343187652354, -0.14366048052473818, 0.12972539736142077, 0.01719736195775832... |
706.2682 | A unified description of diffractive deep inelastic scattering with
saturation | We propose a new description of inclusive diffraction in deep inelastic
scattering (DIS). The diffractive structure functions are expressed in the
dipole picture and contain heavy-quark contributions. The dipole scattering
amplitude, a saturation model fitted on inclusive DIS data, features a
saturation scale Q_s(x) ... | hep-ph | we propose a new description of inclusive diffraction in deep inelastic scattering dis the diffractive structure functions are expressed in the dipole picture and contain heavyquark contributions the dipole scattering amplitude a saturation model fitted on inclusive dis data features a saturation scale q_sx larger than... | [['we', 'propose', 'a', 'new', 'description', 'of', 'inclusive', 'diffraction', 'in', 'deep', 'inelastic', 'scattering', 'dis', 'the', 'diffractive', 'structure', 'functions', 'are', 'expressed', 'in', 'the', 'dipole', 'picture', 'and', 'contain', 'heavyquark', 'contributions', 'the', 'dipole', 'scattering', 'amplitude... | [-0.05174093947355305, 0.15487159594332658, -0.14876470273180353, 0.17409611216706214, -0.0383580179123949, -0.04893878873022053, 0.0013375860608873828, 0.3612132916847865, -0.23229576251719908, -0.24602038379738567, 0.0006795385839938316, -0.34109846742883804, -0.047696774645197774, 0.15785456092537492, 0.070877942026... |
706.2683 | Calibration of the Relationship between Precipitable Water Vapor and 225
GHz Atmospheric Opacity via Optical Echelle Spectroscopy at Las Campanas
Observatory | We report precipitable water vapor (PWV) measurements made at Las Campanas
Observatory using optical spectra of H2O lines obtained with the Magellan
echelle spectrograph, and calculated using a robust technique that is accurate
to 5-10%. Calibration of the relationship between our PWV measurements and
opacity values ... | astro-ph | we report precipitable water vapor pwv measurements made at las campanas observatory using optical spectra of h2o lines obtained with the magellan echelle spectrograph and calculated using a robust technique that is accurate to 510 calibration of the relationship between our pwv measurements and opacity values at 225 g... | [['we', 'report', 'precipitable', 'water', 'vapor', 'pwv', 'measurements', 'made', 'at', 'las', 'campanas', 'observatory', 'using', 'optical', 'spectra', 'of', 'h2o', 'lines', 'obtained', 'with', 'the', 'magellan', 'echelle', 'spectrograph', 'and', 'calculated', 'using', 'a', 'robust', 'technique', 'that', 'is', 'accur... | [-0.07293186281943538, 0.13459960227853365, -0.0864512666382573, -0.0008721073452651387, -0.04534390282104582, -0.10319553956982087, 0.11139273330406992, 0.4462538850564284, -0.11506880690858727, -0.4033713453294088, 0.16420119924904694, -0.3591951144520532, -0.08671396974982186, 0.23371667328826856, -0.012131523658436... |
706.2684 | Unzipping Vortices in Type-II Superconductors | The unzipping of vortex lines using magnetic-force microscopy from extended
defects is studied theoretically. We study both the unzipping isolated vortex
from common defects, such as columnar pins and twin-planes, and the unzipping
of a vortex from a plane in the presence of other vortices. We show, using
analytic an... | cond-mat.stat-mech cond-mat.soft cond-mat.supr-con | the unzipping of vortex lines using magneticforce microscopy from extended defects is studied theoretically we study both the unzipping isolated vortex from common defects such as columnar pins and twinplanes and the unzipping of a vortex from a plane in the presence of other vortices we show using analytic and numeric... | [['the', 'unzipping', 'of', 'vortex', 'lines', 'using', 'magneticforce', 'microscopy', 'from', 'extended', 'defects', 'is', 'studied', 'theoretically', 'we', 'study', 'both', 'the', 'unzipping', 'isolated', 'vortex', 'from', 'common', 'defects', 'such', 'as', 'columnar', 'pins', 'and', 'twinplanes', 'and', 'the', 'unzi... | [-0.1300046863123296, 0.13458260144236395, -0.0722586905467324, 0.028831742543843575, -0.015543228707328025, -0.0734425734068888, 0.06504139104759411, 0.3686836880321304, -0.2540381469298154, -0.2406461463801356, 0.07659878982263359, -0.27898281616055304, -0.1420751770492643, 0.20986287300022216, 0.021581193768522806, ... |
706.2685 | Structure of potentials with $N$ Higgs doublets | Extensions of the Standard Model with $N$ Higgs doublets are simple
extensions presenting a rich mathematical structure. An underlying Minkowski
structure emerges from the study of both variable space and parameter space.
The former can be completely parametrized in terms of two future lightlike
Minkowski vectors wit... | hep-ph hep-th math-ph math.MP | extensions of the standard model with n higgs doublets are simple extensions presenting a rich mathematical structure an underlying minkowski structure emerges from the study of both variable space and parameter space the former can be completely parametrized in terms of two future lightlike minkowski vectors with spat... | [['extensions', 'of', 'the', 'standard', 'model', 'with', 'n', 'higgs', 'doublets', 'are', 'simple', 'extensions', 'presenting', 'a', 'rich', 'mathematical', 'structure', 'an', 'underlying', 'minkowski', 'structure', 'emerges', 'from', 'the', 'study', 'of', 'both', 'variable', 'space', 'and', 'parameter', 'space', 'the... | [-0.13874543179498197, 0.19757466750077304, -0.032343574647361845, 0.12199724152518544, -0.09191296279403524, -0.185517195308281, 0.0005255783919262915, 0.31260837694236004, -0.2504479196728565, -0.2501246079023426, 0.04702265558052414, -0.24418075456588456, -0.09633019255124964, 0.10183724233782133, -0.016588996058719... |
706.2686 | Singular Loci of Hibi toric varieties | We first construct explicit bases for the cotangent spaces at singular points
on Hibi toric varieties, i.e., toric varieties associated to distributive
lattices. We then determine the singular loci of these toric varieties.
| math.AG | we first construct explicit bases for the cotangent spaces at singular points on hibi toric varieties ie toric varieties associated to distributive lattices we then determine the singular loci of these toric varieties | [['we', 'first', 'construct', 'explicit', 'bases', 'for', 'the', 'cotangent', 'spaces', 'at', 'singular', 'points', 'on', 'hibi', 'toric', 'varieties', 'ie', 'toric', 'varieties', 'associated', 'to', 'distributive', 'lattices', 'we', 'then', 'determine', 'the', 'singular', 'loci', 'of', 'these', 'toric', 'varieties']] | [-0.20717103982513602, -0.06029397257688371, -0.029482691562875654, 0.17276398984320235, -0.11203087942505424, -0.19253797219558197, -0.008729287112752596, 0.3339767816730521, -0.3899419851826899, 0.0020557314891255264, 0.11904016691683368, -0.2465137350090751, -0.1391449241588513, 0.16297720383965608, -0.2558444329135... |
706.2687 | The Luminosity Function of the Milky Way Satellites | We quantify the detectability of stellar Milky Way satellites in the Sloan
Digital Sky Survey (SDSS) Data Release 5. We show that the effective search
volumes for the recently discovered SDSS--satellites depend strongly on their
luminosity, with their maximum distance, $D_{max}$, substantially smaller than
the Milky ... | astro-ph | we quantify the detectability of stellar milky way satellites in the sloan digital sky survey sdss data release 5 we show that the effective search volumes for the recently discovered sdsssatellites depend strongly on their luminosity with their maximum distance d_max substantially smaller than the milky way halos viri... | [['we', 'quantify', 'the', 'detectability', 'of', 'stellar', 'milky', 'way', 'satellites', 'in', 'the', 'sloan', 'digital', 'sky', 'survey', 'sdss', 'data', 'release', '5', 'we', 'show', 'that', 'the', 'effective', 'search', 'volumes', 'for', 'the', 'recently', 'discovered', 'sdsssatellites', 'depend', 'strongly', 'on'... | [-0.04830287837761543, 0.08892801538431308, -0.06939052983597364, 0.14328348101948254, -0.11571366285733391, 0.0018200466071166808, 0.04282331203631613, 0.4106662105990663, -0.1618050571359206, -0.42337596066118705, 0.030588244023549902, -0.3353168866029764, 0.009387659317802726, 0.24501843440659632, -0.011018135608072... |
706.2688 | Proximity effects induced by a gold layer on La0.67Sr0.33MnO3 thin films | We report about La0.67Sr0.33MnO3 single crystal manganite thin films in
interaction with a gold capping layer. With respect to uncoated manganite
layers of the same thickness, Au-capped 4 nm-thick manganite films reveal a
dramatic reduction (about 185 K) of the Curie temperature TC and a lower
saturation low-temperat... | cond-mat.mtrl-sci | we report about la067sr033mno3 single crystal manganite thin films in interaction with a gold capping layer with respect to uncoated manganite layers of the same thickness aucapped 4 nmthick manganite films reveal a dramatic reduction about 185 k of the curie temperature tc and a lower saturation lowtemperature magneti... | [['we', 'report', 'about', 'la067sr033mno3', 'single', 'crystal', 'manganite', 'thin', 'films', 'in', 'interaction', 'with', 'a', 'gold', 'capping', 'layer', 'with', 'respect', 'to', 'uncoated', 'manganite', 'layers', 'of', 'the', 'same', 'thickness', 'aucapped', '4', 'nmthick', 'manganite', 'films', 'reveal', 'a', 'dr... | [-0.15517765712540815, 0.22513141168918296, 0.016978727007175193, -0.09326301619602258, -0.03125151128453367, -0.18442948730114628, 0.15543498911840073, 0.4532363190808717, -0.2540291840320124, -0.3670733844950412, -0.019494051334229025, -0.3814308067455011, -0.05727106606286457, 0.16083026570541895, 0.0162868731983882... |
706.2689 | Long-range forces between two excited mercury atoms and associative
ionization | The long-range quadrupole-quadrupole ($\sim R^{-5}$) and leading dispersion
($\sim R^{-6}$) interactions between all pairs of excited Hg($6s6p$) $^3P_0$,
$^3P_1$, $^3P_2$, and $^1P_1$ atoms are determined. The quadrupole moments are
calculated using the {\it ab initio} relativistic configuration-interaction
method co... | physics.atom-ph | the longrange quadrupolequadrupole sim r5 and leading dispersion sim r6 interactions between all pairs of excited hg6s6p 3p_0 3p_1 3p_2 and 1p_1 atoms are determined the quadrupole moments are calculated using the it ab initio relativistic configurationinteraction method coupled with manybody perturbation theory the va... | [['the', 'longrange', 'quadrupolequadrupole', 'sim', 'r5', 'and', 'leading', 'dispersion', 'sim', 'r6', 'interactions', 'between', 'all', 'pairs', 'of', 'excited', 'hg6s6p', '3p_0', '3p_1', '3p_2', 'and', '1p_1', 'atoms', 'are', 'determined', 'the', 'quadrupole', 'moments', 'are', 'calculated', 'using', 'the', 'it', 'a... | [-0.1262557408466053, 0.19235708909885338, -0.029599838406603227, 0.10566724108413614, 0.03787879021266442, -0.1558568213960123, -0.05025749970247904, 0.3861294109374285, -0.18817382780508252, -0.2758483628726058, -0.0941873166123977, -0.3864869899075609, -0.06163699663113476, 0.16364074694482902, 0.1538009540659882, 0... |
706.269 | Hydromagnetic Instability in plane Couette Flow | We study the stability of a compressible magnetic plane Couette flow and show
that compressibility profoundly alters the stability properties if the magnetic
field has a component perpendicular to the direction of flow. The necessary
condition of a newly found instability can be satisfied in a wide variety of
flows i... | astro-ph | we study the stability of a compressible magnetic plane couette flow and show that compressibility profoundly alters the stability properties if the magnetic field has a component perpendicular to the direction of flow the necessary condition of a newly found instability can be satisfied in a wide variety of flows in l... | [['we', 'study', 'the', 'stability', 'of', 'a', 'compressible', 'magnetic', 'plane', 'couette', 'flow', 'and', 'show', 'that', 'compressibility', 'profoundly', 'alters', 'the', 'stability', 'properties', 'if', 'the', 'magnetic', 'field', 'has', 'a', 'component', 'perpendicular', 'to', 'the', 'direction', 'of', 'flow', ... | [-0.255335831316188, 0.21784078362344933, -0.10640379403379154, 0.048294158931557, -0.08094356536854651, -0.07473768008640036, -0.047946565713077274, 0.30180719147161156, -0.33485533288595354, -0.27931436464529147, 0.11828567487298808, -0.16426927426999266, -0.08027127598920329, 0.243245715031993, 0.018167899233627726,... |
706.2691 | Logarithmic growth law in the two-dimensional Ising spin glass state
resulting from the electron doping in single-layered manganites | The ac-susceptibility of the electron doped single-layered manganite
La$_{1.1}$Sr$_{0.9}$MnO$_4$ is analyzed in detail. A quasi two-dimensional
(2$D$) antiferromagnetic (AFM) order with Ising anisotropy is stabilized below
$T_N$ $\sim$ 80K. We show that below $T_N$, a rare 2$D$ spin-glass (SG)
correlation develops wi... | cond-mat.mtrl-sci cond-mat.str-el | the acsusceptibility of the electron doped singlelayered manganite la_11sr_09mno_4 is analyzed in detail a quasi twodimensional 2d antiferromagnetic afm order with ising anisotropy is stabilized below t_n sim 80k we show that below t_n a rare 2d spinglass sg correlation develops with the same ising anisotropy as the af... | [['the', 'acsusceptibility', 'of', 'the', 'electron', 'doped', 'singlelayered', 'manganite', 'la_11sr_09mno_4', 'is', 'analyzed', 'in', 'detail', 'a', 'quasi', 'twodimensional', '2d', 'antiferromagnetic', 'afm', 'order', 'with', 'ising', 'anisotropy', 'is', 'stabilized', 'below', 't_n', 'sim', '80k', 'we', 'show', 'tha... | [-0.1409823676839358, 0.19136028515420161, -0.06281869965041, 0.0537943497783448, -0.03463441806944144, -0.1470552983298672, 0.046855356573580524, 0.3378665831582056, -0.24234999030313426, -0.2696281208967169, 0.07778215854054768, -0.3398803475270556, -0.134385610214491, 0.1704667670860407, 0.06457730569650955, 0.05712... |
706.2692 | Detection of broad 21-cm absorption at z = 0.656 in the complex
sight-line towards 3C336 | We report the detection of 21-cm absorption at z = 0.656 towards 1622+238
(3C336). The line is very broad with a Full-Width Half Maximum (FWHM) of 235
km/s, giving a velocity integrated optical depth of 2.2 km/s. The centroid of
the line is offset from that of the known damped Lyman-alpha absorption (DLA)
system by 5... | astro-ph | we report the detection of 21cm absorption at z 0656 towards 1622238 3c336 the line is very broad with a fullwidth half maximum fwhm of 235 kms giving a velocity integrated optical depth of 22 kms the centroid of the line is offset from that of the known damped lymanalpha absorption dla system by 50 kms and if the lyma... | [['we', 'report', 'the', 'detection', 'of', '21cm', 'absorption', 'at', 'z', '0656', 'towards', '1622238', '3c336', 'the', 'line', 'is', 'very', 'broad', 'with', 'a', 'fullwidth', 'half', 'maximum', 'fwhm', 'of', '235', 'kms', 'giving', 'a', 'velocity', 'integrated', 'optical', 'depth', 'of', '22', 'kms', 'the', 'centr... | [-0.08986630154149879, 0.09780992085562788, -0.014724448683542491, -0.006864938990342138, -0.07055592455350569, -0.14226855982747608, 0.025146439049501708, 0.4475393505481473, -0.1748757095800128, -0.2969046054802237, 0.07304083562564839, -0.3052700094769906, 0.01145430722606987, 0.18873288110238465, 0.0471614641617926... |
706.2693 | Reaction cross sections for proton scattering from stable and unstable
nuclei based on a microscopic approach | Microscopic optical model potential results for reaction cross sections of
proton elastic scattering are presented. The applications cover the 10-1000 MeV
energy range and consider both stable and unstable nuclei. The study is based
on in-medium g-matrix full-folding optical model approach with the appropriate
relati... | nucl-th | microscopic optical model potential results for reaction cross sections of proton elastic scattering are presented the applications cover the 101000 mev energy range and consider both stable and unstable nuclei the study is based on inmedium gmatrix fullfolding optical model approach with the appropriate relativistic k... | [['microscopic', 'optical', 'model', 'potential', 'results', 'for', 'reaction', 'cross', 'sections', 'of', 'proton', 'elastic', 'scattering', 'are', 'presented', 'the', 'applications', 'cover', 'the', '101000', 'mev', 'energy', 'range', 'and', 'consider', 'both', 'stable', 'and', 'unstable', 'nuclei', 'the', 'study', '... | [-0.07890978422546818, 0.17838445618143603, -0.05770914993845045, 0.15337081475014305, 0.01381501463700863, -0.12716572677974655, 0.0007823785102576207, 0.3905841568544222, -0.16650119500388955, -0.3013493942369701, -0.03583836463683397, -0.3473895583806002, -0.008119037274010242, 0.19743038547984593, 0.095077914162094... |
706.2694 | Mirror dark matter | A mirror sector of particles and forces provides a simple explanation of the
inferred dark matter of the Universe. The status of this theory is reviewed -
with emphasis on how the theory explains the impressive DAMA/NaI annual
modulation signal, whilst also being consistent with the null results of the
other direct d... | hep-ph astro-ph | a mirror sector of particles and forces provides a simple explanation of the inferred dark matter of the universe the status of this theory is reviewed with emphasis on how the theory explains the impressive damanai annual modulation signal whilst also being consistent with the null results of the other direct detectio... | [['a', 'mirror', 'sector', 'of', 'particles', 'and', 'forces', 'provides', 'a', 'simple', 'explanation', 'of', 'the', 'inferred', 'dark', 'matter', 'of', 'the', 'universe', 'the', 'status', 'of', 'this', 'theory', 'is', 'reviewed', 'with', 'emphasis', 'on', 'how', 'the', 'theory', 'explains', 'the', 'impressive', 'dama... | [-0.1386995435393644, 0.1515189960932816, -0.1360555082331148, 0.10237490856703722, -0.11205009592451015, -0.10668008080420066, 0.01265202648498399, 0.2986002487112891, -0.16743143619354464, -0.34277014413251067, 0.08461241048040255, -0.2861570749291272, -0.1330695074789648, 0.19902868182310518, -0.028306117180277996, ... |
706.2695 | Functional medium-dependence of the nonrelativistic optical model
potential | By examining the structure in momentum and coordinate space of a two-body
interaction spherically symmetric in its local coordinate, we demonstrate that
it can be disentangled into two distinctive contributions. One of them is a
medium-independent and momentum-conserving term, whereas the other is
functionally --and ... | nucl-th | by examining the structure in momentum and coordinate space of a twobody interaction spherically symmetric in its local coordinate we demonstrate that it can be disentangled into two distinctive contributions one of them is a mediumindependent and momentumconserving term whereas the other is functionally and exclusivel... | [['by', 'examining', 'the', 'structure', 'in', 'momentum', 'and', 'coordinate', 'space', 'of', 'a', 'twobody', 'interaction', 'spherically', 'symmetric', 'in', 'its', 'local', 'coordinate', 'we', 'demonstrate', 'that', 'it', 'can', 'be', 'disentangled', 'into', 'two', 'distinctive', 'contributions', 'one', 'of', 'them'... | [-0.11956028269570587, 0.12660418067420584, -0.09273294170104367, 0.05455262937716075, -0.0685182664493498, -0.07385987673353936, 0.0026267952285706996, 0.34295953170263344, -0.29353438361680934, -0.2738857198760213, 0.06927755703135127, -0.25898300043772904, -0.13215178452166063, 0.16304545936041645, -0.01176768238157... |
706.2696 | Three-dimensional simulations of molecular cloud fragmentation regulated
by magnetic fields and ambipolar diffusion | We employ the first fully three-dimensional simulation to study the role of
magnetic fields and ion-neutral friction in regulating gravitationally-driven
fragmentation of molecular clouds. The cores in an initially subcritical cloud
develop gradually over an ambipolar diffusion time while the cores in an
initially su... | astro-ph | we employ the first fully threedimensional simulation to study the role of magnetic fields and ionneutral friction in regulating gravitationallydriven fragmentation of molecular clouds the cores in an initially subcritical cloud develop gradually over an ambipolar diffusion time while the cores in an initially supercri... | [['we', 'employ', 'the', 'first', 'fully', 'threedimensional', 'simulation', 'to', 'study', 'the', 'role', 'of', 'magnetic', 'fields', 'and', 'ionneutral', 'friction', 'in', 'regulating', 'gravitationallydriven', 'fragmentation', 'of', 'molecular', 'clouds', 'the', 'cores', 'in', 'an', 'initially', 'subcritical', 'clou... | [-0.1646190916260206, 0.16558406289499236, -0.05238273018695624, 0.010591310729325133, 0.022916899075028942, -0.0389325661612609, 0.01551437636338909, 0.3719166892934853, -0.25884377084095295, -0.2789809930361283, 0.05151286401989227, -0.22116984021653172, -0.048716936649059434, 0.13865165446776714, 0.04487019499028462... |
706.2697 | Fluctuations of the chiral condensate and quasi-particle spectra near
phase transition | We investigate the quark spectrum near but above the critical temperature of
the chiral transition, taking into account the precursory soft modes. It is
found that there appear novel excitation spectra of quasi-quarks and
quasi-antiquarks with a three-peak structure. By a detailed analysis on the
formation of the thr... | hep-ph nucl-th | we investigate the quark spectrum near but above the critical temperature of the chiral transition taking into account the precursory soft modes it is found that there appear novel excitation spectra of quasiquarks and quasiantiquarks with a threepeak structure by a detailed analysis on the formation of the threepeak s... | [['we', 'investigate', 'the', 'quark', 'spectrum', 'near', 'but', 'above', 'the', 'critical', 'temperature', 'of', 'the', 'chiral', 'transition', 'taking', 'into', 'account', 'the', 'precursory', 'soft', 'modes', 'it', 'is', 'found', 'that', 'there', 'appear', 'novel', 'excitation', 'spectra', 'of', 'quasiquarks', 'and... | [-0.10124202248727099, 0.2509710043635934, -0.10997944976677936, 0.08209691318345494, -0.025999206775689825, -0.10373850915507943, 0.08089516546540693, 0.3523066647569923, -0.20802289313253233, -0.26661250521154967, 0.01047951109506482, -0.28588310232860786, -0.06641099808335889, 0.11708448741438926, 0.0861962784227787... |
706.2698 | Pygmy dipole resonance in exotic nuclei | The evolution of the PDR strength with the neutron excess is investigated in
Sn isotopic and N=82 isotonic chains with regard to its possible connection
with the neutron skin thickness. For this purpose a recently proposed method
incorporating both HFB and multi-phonon QPM theory is applied. Analysis of the
correspon... | nucl-th | the evolution of the pdr strength with the neutron excess is investigated in sn isotopic and n82 isotonic chains with regard to its possible connection with the neutron skin thickness for this purpose a recently proposed method incorporating both hfb and multiphonon qpm theory is applied analysis of the corresponding n... | [['the', 'evolution', 'of', 'the', 'pdr', 'strength', 'with', 'the', 'neutron', 'excess', 'is', 'investigated', 'in', 'sn', 'isotopic', 'and', 'n82', 'isotonic', 'chains', 'with', 'regard', 'to', 'its', 'possible', 'connection', 'with', 'the', 'neutron', 'skin', 'thickness', 'for', 'this', 'purpose', 'a', 'recently', '... | [-0.025883047287512957, 0.12560330670736408, -0.043168993562395716, 0.10198330354539613, -0.03835391484457871, -0.0932029134880928, 0.03323931054107781, 0.3976535762756549, -0.1652542730343753, -0.2730800740717878, -0.021000482473153108, -0.31013533029833745, -0.05450294999323448, 0.12559513572266262, 0.052374270150502... |
706.2699 | Instanton representation of Plebanski gravity. Application to Bianchi
Type A metrics | Using the instanton representation method we construct a general solution for
GR in the spatially homogeneous case restricted to diagonal variables. This
paper provides a testing ground and physical intuition for many of the salient
features of general relativity which it is suggested should be preserved in the
full ... | gr-qc | using the instanton representation method we construct a general solution for gr in the spatially homogeneous case restricted to diagonal variables this paper provides a testing ground and physical intuition for many of the salient features of general relativity which it is suggested should be preserved in the full the... | [['using', 'the', 'instanton', 'representation', 'method', 'we', 'construct', 'a', 'general', 'solution', 'for', 'gr', 'in', 'the', 'spatially', 'homogeneous', 'case', 'restricted', 'to', 'diagonal', 'variables', 'this', 'paper', 'provides', 'a', 'testing', 'ground', 'and', 'physical', 'intuition', 'for', 'many', 'of',... | [-0.08827767855487764, 0.05534880636259913, -0.13226361822336913, 0.1078989990055561, -0.09393706161528825, -0.15701678225770593, -0.000889838794246316, 0.3243824046384543, -0.25671260226517917, -0.24145370110869407, 0.08135556570719928, -0.2010719208791852, -0.1950602212920785, 0.15226188242435457, -0.0673584088869392... |
706.27 | Universal flattening of Frobenius | For a variety $X$ of positive characteristic and a non-negative integer $e$,
we define its $e$-th F-blowup to be the universal flattening of the
$e$-iterated Frobenius of $X$. Thus we have the sequence (a set labeled by
non-negative integers) of blowups of $X$. Under some condition, the sequence
stabilizes and leads ... | math.AG math.AC | for a variety x of positive characteristic and a nonnegative integer e we define its eth fblowup to be the universal flattening of the eiterated frobenius of x thus we have the sequence a set labeled by nonnegative integers of blowups of x under some condition the sequence stabilizes and leads to a nice for instance mi... | [['for', 'a', 'variety', 'x', 'of', 'positive', 'characteristic', 'and', 'a', 'nonnegative', 'integer', 'e', 'we', 'define', 'its', 'eth', 'fblowup', 'to', 'be', 'the', 'universal', 'flattening', 'of', 'the', 'eiterated', 'frobenius', 'of', 'x', 'thus', 'we', 'have', 'the', 'sequence', 'a', 'set', 'labeled', 'by', 'non... | [-0.19746054301672764, 0.051210112707770386, -0.1187700170321741, 0.06763225829606687, -0.06905289944531261, -0.1956905283479263, 0.021846077359362465, 0.3442552776777766, -0.3547169534705471, -0.21639857586959135, 0.07412494600925973, -0.22502847637414283, -0.10388213435552367, 0.1608546682856167, -0.1414888302485148,... |
706.2701 | Differential rotation of stretched and twisted thick magnetic flux tube
dynamos in Riemannian spaces | The topological mapping between a torus of big radius and a sphere is applied
to the Riemannian geometry of a stretched and twisted very thick magnetic flux
tube, to obtain spherical dynamos solving the magnetohydrodynamics (MHD)
self-induction equation for the magnetic flux tubes undergoing differential
(non-uniform... | astro-ph | the topological mapping between a torus of big radius and a sphere is applied to the riemannian geometry of a stretched and twisted very thick magnetic flux tube to obtain spherical dynamos solving the magnetohydrodynamics mhd selfinduction equation for the magnetic flux tubes undergoing differential nonuniform rotatio... | [['the', 'topological', 'mapping', 'between', 'a', 'torus', 'of', 'big', 'radius', 'and', 'a', 'sphere', 'is', 'applied', 'to', 'the', 'riemannian', 'geometry', 'of', 'a', 'stretched', 'and', 'twisted', 'very', 'thick', 'magnetic', 'flux', 'tube', 'to', 'obtain', 'spherical', 'dynamos', 'solving', 'the', 'magnetohydrod... | [-0.16946565045071102, 0.14460826501536192, -0.05590386867058506, 0.09349808278571518, -0.11329244561181658, -0.06906779875557979, -0.03084499132137543, 0.33997231248033594, -0.2422352795670331, -0.2818497121334076, 0.10845273955984266, -0.18373196910406517, -0.08402226939914303, 0.24180150713000026, -0.071530116474787... |
706.2702 | Nonlinear gravitons from the initial value constraints of GR in Ashtekar
variables | In this paper we provide a possible realization of Penrose's idea of
nonlinear gravitons by constructing a solution to the initial value constraints
in Ashtekar variables. The solution inputs are a spatial SU(2) connection and
two free functions of position, and can be constructed as a formal operatorial
expansion in... | gr-qc | in this paper we provide a possible realization of penroses idea of nonlinear gravitons by constructing a solution to the initial value constraints in ashtekar variables the solution inputs are a spatial su2 connection and two free functions of position and can be constructed as a formal operatorial expansion in powers... | [['in', 'this', 'paper', 'we', 'provide', 'a', 'possible', 'realization', 'of', 'penroses', 'idea', 'of', 'nonlinear', 'gravitons', 'by', 'constructing', 'a', 'solution', 'to', 'the', 'initial', 'value', 'constraints', 'in', 'ashtekar', 'variables', 'the', 'solution', 'inputs', 'are', 'a', 'spatial', 'su2', 'connection... | [-0.15429494519740705, 0.07445351523915078, -0.09573326204767132, 0.04640434748101298, -0.15287999343127012, -0.12111069755515129, 0.01415710216927592, 0.3363003018425732, -0.2381809760430237, -0.24801141397300652, 0.13481131536891774, -0.22081497488770543, -0.16833064684689772, 0.12426254859693893, -0.0221662997699728... |
706.2703 | Exact Solitonic Solutions of the Gross-Pitaevskii Equation with a Linear
Potential | We derive classes of exact solitonic solutions of the time-dependent
Gross-Pitaevskii equation with repulsive and attractive interatomic
interactions. The solutions correspond to a string of bright solitons with
phase difference between adjacent solitons equal to $\pi$. While the relative
phase, width, and distance b... | cond-mat.other | we derive classes of exact solitonic solutions of the timedependent grosspitaevskii equation with repulsive and attractive interatomic interactions the solutions correspond to a string of bright solitons with phase difference between adjacent solitons equal to pi while the relative phase width and distance between adja... | [['we', 'derive', 'classes', 'of', 'exact', 'solitonic', 'solutions', 'of', 'the', 'timedependent', 'grosspitaevskii', 'equation', 'with', 'repulsive', 'and', 'attractive', 'interatomic', 'interactions', 'the', 'solutions', 'correspond', 'to', 'a', 'string', 'of', 'bright', 'solitons', 'with', 'phase', 'difference', 'b... | [-0.18444985621986357, 0.1502109408202405, -0.0850798460895611, 0.07404085473988105, -0.05777100656131232, -0.15866869969318645, 0.042887157886414916, 0.3405512349327674, -0.27204945066478103, -0.293067182137354, 0.009385417901432595, -0.3139548245471323, -0.053602456694116465, 0.09610314352588879, 0.06909271340968239,... |
706.2704 | Kernel Regression For Determining Photometric Redshifts From Sloan
Broadband Photometry | We present a new approach, kernel regression, to determine photometric
redshifts for 399,929 galaxies in the Fifth Data Release of the Sloan Digital
Sky Survey (SDSS). In our case, kernel regression is a weighted average of
spectral redshifts of the neighbors for a query point, where higher weights are
associated wit... | astro-ph | we present a new approach kernel regression to determine photometric redshifts for 399929 galaxies in the fifth data release of the sloan digital sky survey sdss in our case kernel regression is a weighted average of spectral redshifts of the neighbors for a query point where higher weights are associated with points t... | [['we', 'present', 'a', 'new', 'approach', 'kernel', 'regression', 'to', 'determine', 'photometric', 'redshifts', 'for', '399929', 'galaxies', 'in', 'the', 'fifth', 'data', 'release', 'of', 'the', 'sloan', 'digital', 'sky', 'survey', 'sdss', 'in', 'our', 'case', 'kernel', 'regression', 'is', 'a', 'weighted', 'average',... | [-0.045691794311514475, 0.01374485794253446, -0.05737963400944766, 0.10987617204208053, -0.12274231687125221, -0.13374757253237674, 0.11098371475708445, 0.42679701708225737, -0.22987770840424943, -0.29841958408910985, 0.14141996991285752, -0.34864641803417457, -0.07381753240888184, 0.21812968704585187, -0.0998423036181... |
706.2705 | Exact Solitonic Solutions of the One-Dimensional Gross-Pitaevskii
Equation with a Time-Dependent Harmonic Potential and Interatomic Interaction | We derive exact solitonic solutions of the one-dimensional time-dependent
Gross-Pitaevskii equation with time-dependent strengths of the harmonic
external potential and the interatomic interaction. The time-dependence of the
external potential and interatomic interaction are given in terms of a general
function of ti... | cond-mat.other | we derive exact solitonic solutions of the onedimensional timedependent grosspitaevskii equation with timedependent strengths of the harmonic external potential and the interatomic interaction the timedependence of the external potential and interatomic interaction are given in terms of a general function of time for a... | [['we', 'derive', 'exact', 'solitonic', 'solutions', 'of', 'the', 'onedimensional', 'timedependent', 'grosspitaevskii', 'equation', 'with', 'timedependent', 'strengths', 'of', 'the', 'harmonic', 'external', 'potential', 'and', 'the', 'interatomic', 'interaction', 'the', 'timedependence', 'of', 'the', 'external', 'poten... | [-0.18479747701399396, 0.12296500909594603, -0.05110249764719369, 0.04440938854719152, -0.030183844683267694, -0.11689431628322985, 0.003793821384263511, 0.35642923178649183, -0.2788155738536342, -0.27124847997311907, 0.042186635443802446, -0.2527674347355888, -0.11128281573257824, 0.19237519607021666, 0.07826040228621... |
706.2706 | Holonomic rank of A-hypergeometric differential-difference equations | We introduce A-hypergeometric differential-difference equation and prove that
its holonomic rank is equal to the normalized volume of A with giving a set of
convergent series solutions.
| math.CA | we introduce ahypergeometric differentialdifference equation and prove that its holonomic rank is equal to the normalized volume of a with giving a set of convergent series solutions | [['we', 'introduce', 'ahypergeometric', 'differentialdifference', 'equation', 'and', 'prove', 'that', 'its', 'holonomic', 'rank', 'is', 'equal', 'to', 'the', 'normalized', 'volume', 'of', 'a', 'with', 'giving', 'a', 'set', 'of', 'convergent', 'series', 'solutions']] | [-0.21811720632292605, 0.032288803787970985, -0.10456969547602865, 0.011480570757865079, -0.0771930191355447, -0.13013218862384004, 0.0053373481075848555, 0.26338455577691394, -0.31420531896529375, -0.17655350830130004, 0.12210261018049938, -0.2959037688043382, -0.17718999194740145, 0.1742669715097657, -0.1182717524675... |
706.2707 | The p-modular Descent Algebra of the Symmetric Group | The descent algebra of the symmetric group, over a field of non-zero
characteristic p, is studied. A homomorphism into the algebra of generalised
p-modular characters of the symmetric group is defined. This is then used to
determine the radical, and its nilpotency index. It also allows the irreducible
representations... | math.CO | the descent algebra of the symmetric group over a field of nonzero characteristic p is studied a homomorphism into the algebra of generalised pmodular characters of the symmetric group is defined this is then used to determine the radical and its nilpotency index it also allows the irreducible representations of the de... | [['the', 'descent', 'algebra', 'of', 'the', 'symmetric', 'group', 'over', 'a', 'field', 'of', 'nonzero', 'characteristic', 'p', 'is', 'studied', 'a', 'homomorphism', 'into', 'the', 'algebra', 'of', 'generalised', 'pmodular', 'characters', 'of', 'the', 'symmetric', 'group', 'is', 'defined', 'this', 'is', 'then', 'used',... | [-0.16312453751119652, 0.07836693642223379, -0.1520204043481499, 0.03613426876004918, -0.11639084547225918, -0.13759041538495304, -0.07362550846301019, 0.3424727702513337, -0.42312184821016025, -0.18970809286526805, 0.11523645752043064, -0.18443456545381715, -0.10763854379599382, 0.1429566331706675, -0.0905440685705148... |
706.2708 | Overview of event-by-event analysis of high energy nuclear collisions | The event-by-event analysis of high energy nuclear collisions aims at
revealing the richness of the underlying event structures and provide unique
measures of dynamical fluctuations associated with QGP phase transition. The
major challenge in these studies is to separate the dynamical fluctuations from
the many other... | nucl-ex | the eventbyevent analysis of high energy nuclear collisions aims at revealing the richness of the underlying event structures and provide unique measures of dynamical fluctuations associated with qgp phase transition the major challenge in these studies is to separate the dynamical fluctuations from the many other sour... | [['the', 'eventbyevent', 'analysis', 'of', 'high', 'energy', 'nuclear', 'collisions', 'aims', 'at', 'revealing', 'the', 'richness', 'of', 'the', 'underlying', 'event', 'structures', 'and', 'provide', 'unique', 'measures', 'of', 'dynamical', 'fluctuations', 'associated', 'with', 'qgp', 'phase', 'transition', 'the', 'maj... | [-0.14432736225339962, 0.1854879262348361, -0.1289340938286235, 0.11791074706814941, -0.00455038552172482, -0.034955179126915974, -0.05575133044557232, 0.34940211761190937, -0.22360315454985807, -0.32233744073245263, 0.05765657363237416, -0.3478049446345755, -0.02894159345197733, 0.14512990182238691, 0.0145201974772606... |
706.2709 | Rumsfeld Hadrons | Donald Rumsfeld, in attempting to excuse the inexcusable, once (in)famously
said that ``there are things that we know we know; there are things that we
know we don't know; and then there are things that we don't know that we don't
know". Recent discoveries about hadrons with heavy flavours fall into those
categories.... | hep-ph | donald rumsfeld in attempting to excuse the inexcusable once infamously said that there are things that we know we know there are things that we know we dont know and then there are things that we dont know that we dont know recent discoveries about hadrons with heavy flavours fall into those categories it is of course... | [['donald', 'rumsfeld', 'in', 'attempting', 'to', 'excuse', 'the', 'inexcusable', 'once', 'infamously', 'said', 'that', 'there', 'are', 'things', 'that', 'we', 'know', 'we', 'know', 'there', 'are', 'things', 'that', 'we', 'know', 'we', 'dont', 'know', 'and', 'then', 'there', 'are', 'things', 'that', 'we', 'dont', 'know... | [-0.0863200603902491, 0.14153774351989096, -0.09924673137406038, 0.16811844540722165, -0.18690699393030358, -0.17624446842819452, 0.02022552621122953, 0.39356907547728437, -0.2478763208853559, -0.28578999195549937, 0.11053993239388424, -0.38649732730275876, -0.18634432967047435, 0.16296233750275663, -0.1513367666787392... |
706.271 | Compulsory Deep Mixing of 3He and CNO Isotopes in the Envelopes of
low-mass Red Giants | Three-dimensional stellar modeling has enabled us to identify a deep-mixing
mechanism that must operate in all low mass giants. This mixing process is not
optional, and is driven by a molecular weight inversion created by the
3He(3He,2p)4He reaction. In this paper we characterize the behavior of this
mixing, and stud... | astro-ph | threedimensional stellar modeling has enabled us to identify a deepmixing mechanism that must operate in all low mass giants this mixing process is not optional and is driven by a molecular weight inversion created by the 3he3he2p4he reaction in this paper we characterize the behavior of this mixing and study its impac... | [['threedimensional', 'stellar', 'modeling', 'has', 'enabled', 'us', 'to', 'identify', 'a', 'deepmixing', 'mechanism', 'that', 'must', 'operate', 'in', 'all', 'low', 'mass', 'giants', 'this', 'mixing', 'process', 'is', 'not', 'optional', 'and', 'is', 'driven', 'by', 'a', 'molecular', 'weight', 'inversion', 'created', '... | [-0.05683529890329172, 0.20951459609040474, -0.00816118353691694, 0.08465156362581183, -0.03263686534469831, -0.07644939877284891, 0.12706015898982895, 0.35612887120937226, -0.20978103511793128, -0.35587659587631115, 0.03966779992613142, -0.2626540158812146, -0.02386267595703445, 0.1450630600937763, -0.0520697860704934... |
706.2711 | On the Descent Algebra of Type $D$ | Here we give a combinatorial interpretation of Solomon's rule for
multiplication in the descent algebra of Weyl groups of type $D$, $\Sigma D_n$.
From here we show that $\Sigma D_n$ is a homomorphic image of the descent
algebra of the hyperoctahedral group, $\Sigma B_{n-2}$.
| math.CO | here we give a combinatorial interpretation of solomons rule for multiplication in the descent algebra of weyl groups of type d sigma d_n from here we show that sigma d_n is a homomorphic image of the descent algebra of the hyperoctahedral group sigma b_n2 | [['here', 'we', 'give', 'a', 'combinatorial', 'interpretation', 'of', 'solomons', 'rule', 'for', 'multiplication', 'in', 'the', 'descent', 'algebra', 'of', 'weyl', 'groups', 'of', 'type', 'd', 'sigma', 'd_n', 'from', 'here', 'we', 'show', 'that', 'sigma', 'd_n', 'is', 'a', 'homomorphic', 'image', 'of', 'the', 'descent'... | [-0.17631027432666582, 0.04480556305497885, -0.13161518348550255, 0.04602515724201856, -0.11606466770172119, -0.18413975341668862, 0.04992855040208352, 0.3756907487457449, -0.37888528288088064, -0.18359574802558531, 0.103409664808582, -0.21319332756386508, -0.19746060273610055, 0.1541333245113492, -0.14965747337026353,... |
706.2712 | Morphological Dependence of MIR Properties of SDSS Galaxies in the
Spitzer SWIRE Survey | We explore the correlation between morphological types and mid-infrared (MIR)
properties of an optically flux-limited sample of 154 galaxies from the Forth
Data Release (DR4) of Sloan Digital Sky Survey (SDSS), cross-correlated with
Spitzer SWIRE (Spitzer Wide-Area InfraRed Extragalactic Survey) fields of
ELAIS-N1, E... | astro-ph | we explore the correlation between morphological types and midinfrared mir properties of an optically fluxlimited sample of 154 galaxies from the forth data release dr4 of sloan digital sky survey sdss crosscorrelated with spitzer swire spitzer widearea infrared extragalactic survey fields of elaisn1 elaisn2 and lockma... | [['we', 'explore', 'the', 'correlation', 'between', 'morphological', 'types', 'and', 'midinfrared', 'mir', 'properties', 'of', 'an', 'optically', 'fluxlimited', 'sample', 'of', '154', 'galaxies', 'from', 'the', 'forth', 'data', 'release', 'dr4', 'of', 'sloan', 'digital', 'sky', 'survey', 'sdss', 'crosscorrelated', 'wit... | [0.008595617538698466, 0.009587782029874299, -0.10447526555903355, 0.12400328599323984, -0.12570368228469825, 0.004486691827228891, 0.05175551291904412, 0.5222455023322254, -0.11275370349591997, -0.34370828879348536, 0.045439033026923425, -0.35199572045322775, -0.05105931264863882, 0.2122468791198376, -0.04711276450169... |
706.2713 | Contraction groups in complete Kac-Moody groups | Let $G$ be an abstract Kac-Moody group over a finite field and $\bar{G}$ be
the closure of the image of $G$ in the automorphism group of its positive
building. We show that if the Dynkin diagram associated to $G$ is irreducible
and neither of spherical nor of affine type, then the contraction groups of
elements in $\... | math.GR | let g be an abstract kacmoody group over a finite field and barg be the closure of the image of g in the automorphism group of its positive building we show that if the dynkin diagram associated to g is irreducible and neither of spherical nor of affine type then the contraction groups of elements in barg which are not... | [['let', 'g', 'be', 'an', 'abstract', 'kacmoody', 'group', 'over', 'a', 'finite', 'field', 'and', 'barg', 'be', 'the', 'closure', 'of', 'the', 'image', 'of', 'g', 'in', 'the', 'automorphism', 'group', 'of', 'its', 'positive', 'building', 'we', 'show', 'that', 'if', 'the', 'dynkin', 'diagram', 'associated', 'to', 'g', '... | [-0.2083842961190196, 0.1840332149569166, -0.10943032220586554, -0.023132289945776877, -0.13269398917818997, -0.13539275404839934, -0.010534633065924628, 0.4339913296235072, -0.32430697315941, -0.20214149453858662, 0.13928498193022928, -0.236941462479435, -0.14129293881139005, 0.1860840003211777, -0.13627847215816888, ... |
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