id float64 706 1.8k | title stringlengths 1 343 | abstract stringlengths 6 6.09k | categories stringlengths 5 125 | processed_abstract stringlengths 2 5.96k | tokenized_abstract stringlengths 8 8.74k | centroid stringlengths 2.1k 2.17k |
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707.273 | Attractors with Vanishing Central Charge | We consider the Attractor Equations of particular $\mathcal{N}=2$, d=4
supergravity models whose vector multiplets' scalar manifold is endowed with
homogeneous symmetric cubic special K\"{a}hler geometry, namely of the
so-called $st^{2}$ and $stu$ models. In this framework, we derive explicit
expressions for the crit... | hep-th | we consider the attractor equations of particular mathcaln2 d4 supergravity models whose vector multiplets scalar manifold is endowed with homogeneous symmetric cubic special kahler geometry namely of the socalled st2 and stu models in this framework we derive explicit expressions for the critical moduli corresponding ... | [['we', 'consider', 'the', 'attractor', 'equations', 'of', 'particular', 'mathcaln2', 'd4', 'supergravity', 'models', 'whose', 'vector', 'multiplets', 'scalar', 'manifold', 'is', 'endowed', 'with', 'homogeneous', 'symmetric', 'cubic', 'special', 'kahler', 'geometry', 'namely', 'of', 'the', 'socalled', 'st2', 'and', 'st... | [-0.1896660607749012, 0.1154122390339069, -0.014469808853402205, 0.13020524496664487, -0.08141316010302604, -0.19816910617119637, -0.00896233060196064, 0.2671155539952968, -0.15068056897298823, -0.24586820938023765, 0.11366794563791323, -0.2887444052026888, -0.1980037780467575, 0.10031272882055602, -0.07742947301849415... |
707.2731 | Plasmon dispersion in metal nanoparticle chains from angle-resolved
scattering | We present angle and frequency resolved optical extinction measurements to
determine the dispersion relation of plasmon modes on Ag and Au nanoparticle
chains with pitches down to 75 nm. The large splitting between transverse and
longitudinal modes and the band curvature are inconsistent with reported
electrostatic n... | cond-mat.other | we present angle and frequency resolved optical extinction measurements to determine the dispersion relation of plasmon modes on ag and au nanoparticle chains with pitches down to 75 nm the large splitting between transverse and longitudinal modes and the band curvature are inconsistent with reported electrostatic near... | [['we', 'present', 'angle', 'and', 'frequency', 'resolved', 'optical', 'extinction', 'measurements', 'to', 'determine', 'the', 'dispersion', 'relation', 'of', 'plasmon', 'modes', 'on', 'ag', 'and', 'au', 'nanoparticle', 'chains', 'with', 'pitches', 'down', 'to', '75', 'nm', 'the', 'large', 'splitting', 'between', 'tran... | [-0.1446903906217231, 0.19171392640753374, -0.016633321879838535, 0.0575033305401637, -0.08089784857489772, -0.1696420047261232, 0.030351473855458805, 0.491903516824718, -0.2523087226777329, -0.30889138109931674, 0.046576612780021655, -0.27632877512558085, -0.08760968739636713, 0.23481871221090775, 0.04222818248200457,... |
707.2732 | An explicit formula for the characters of the symmetric group | We give an explicit expression of the normalized characters of the symmetric
group in terms of the contents of the partition labelling the representation.
| math.CO math.GR math.RT | we give an explicit expression of the normalized characters of the symmetric group in terms of the contents of the partition labelling the representation | [['we', 'give', 'an', 'explicit', 'expression', 'of', 'the', 'normalized', 'characters', 'of', 'the', 'symmetric', 'group', 'in', 'terms', 'of', 'the', 'contents', 'of', 'the', 'partition', 'labelling', 'the', 'representation']] | [-0.167935208339865, 0.01987707058772988, -0.1024469129818802, 0.017192833009175956, -0.04213983961381018, 0.03635318821761757, 0.028737332516660292, 0.31147511924306553, -0.2521470080440243, -0.2667049802063654, 0.05345404752976416, -0.2726491372450255, -0.1816138372911761, 0.09123059455305338, -0.06929158698767424, -... |
707.2733 | Origin of the Metallicity Dependence of Exoplanet Host Stars in the
Protoplanetary Disk Mass Distribution | The probability of a star hosting a planet that is detectable in radial
velocity surveys increases Ppl(Z) oc 10^2Z, where Z is metallicity. Core
accretion models reproduce this trend, since the protoplanetary disk of a high
metallicity star has a high density of solids and so forms cores which accrete
gas before the ... | astro-ph | the probability of a star hosting a planet that is detectable in radial velocity surveys increases pplz oc 102z where z is metallicity core accretion models reproduce this trend since the protoplanetary disk of a high metallicity star has a high density of solids and so forms cores which accrete gas before the primordi... | [['the', 'probability', 'of', 'a', 'star', 'hosting', 'a', 'planet', 'that', 'is', 'detectable', 'in', 'radial', 'velocity', 'surveys', 'increases', 'pplz', 'oc', '102z', 'where', 'z', 'is', 'metallicity', 'core', 'accretion', 'models', 'reproduce', 'this', 'trend', 'since', 'the', 'protoplanetary', 'disk', 'of', 'a', ... | [-0.09177131560281851, 0.15313233593312492, -0.06291860822488421, 0.09485961108304244, -0.09124907780871061, -0.07195060443232901, 0.03980085973286935, 0.36772529212092714, -0.15528490521579183, -0.32438739122423743, 0.06415779121743981, -0.2527865115486618, -0.06200738930560224, 0.170337768221972, -0.05062609781245036... |
707.2734 | Pulsating Casimir force | Based on the Lifshitz theory we show that the illumination of one (Si) plate
in the three-layer systems Au--ethanol--Si, Si--ethanol--Si and
$\alpha$-Al${}_2$O${}_3$--ethanol--Si with laser pulses can change the Casimir
attraction to Casimir repulsion and vice versa. The proposed effect opens novel
opportunities in n... | quant-ph | based on the lifshitz theory we show that the illumination of one si plate in the threelayer systems auethanolsi siethanolsi and alphaal_2o_3ethanolsi with laser pulses can change the casimir attraction to casimir repulsion and vice versa the proposed effect opens novel opportunities in nanotechnology to actuate the pe... | [['based', 'on', 'the', 'lifshitz', 'theory', 'we', 'show', 'that', 'the', 'illumination', 'of', 'one', 'si', 'plate', 'in', 'the', 'threelayer', 'systems', 'auethanolsi', 'siethanolsi', 'and', 'alphaal_2o_3ethanolsi', 'with', 'laser', 'pulses', 'can', 'change', 'the', 'casimir', 'attraction', 'to', 'casimir', 'repulsi... | [-0.16682289024370153, 0.2148913100862236, -0.10583768342969133, -0.03801105623202982, -0.06375936057362984, -0.1583424331064322, 0.05241679318714887, 0.3654681137665661, -0.2709263016316873, -0.27923463693639233, -0.0008360892173715993, -0.2913286885691445, -0.20207367241973362, 0.2186857822365058, -0.0840921241915159... |
707.2735 | The hard synchrotron X-ray spectrum of the TeV BL Lac 1ES 1426+428 | We have observed 1ES 1426+428 with INTEGRAL detecting it up to $\sim$150 keV.
The spectrum is hard, confirming that this source is an extreme BL Lac object,
with a synchrotron component peaking, in a $\nu F_\nu$ plot, at or above 100
keV, resembling the hard states of Mkn 501 and 1ES 2344+514. All these three
sources... | astro-ph | we have observed 1es 1426428 with integral detecting it up to sim150 kev the spectrum is hard confirming that this source is an extreme bl lac object with a synchrotron component peaking in a nu f_nu plot at or above 100 kev resembling the hard states of mkn 501 and 1es 2344514 all these three sources are tev emitters ... | [['we', 'have', 'observed', '1es', '1426428', 'with', 'integral', 'detecting', 'it', 'up', 'to', 'sim150', 'kev', 'the', 'spectrum', 'is', 'hard', 'confirming', 'that', 'this', 'source', 'is', 'an', 'extreme', 'bl', 'lac', 'object', 'with', 'a', 'synchrotron', 'component', 'peaking', 'in', 'a', 'nu', 'f_nu', 'plot', 'a... | [-0.029966215928637883, 0.16933001522497723, -0.04604657137069881, 0.19105866609796185, -0.07928426018196756, -0.13294186707343755, 0.0006781203749900063, 0.5018255373508465, -0.16264028936563954, -0.42160297500166466, 0.038108778137872674, -0.3424544160470094, 0.07135636594744657, 0.18794565362954224, -0.0160537497708... |
707.2736 | Non-Hermitian Quantum Systems and Time-Optimal Quantum Evolution | Recently, Bender et al. have considered the quantum brachistochrone problem
for the non-Hermitian $\cal PT$-symmetric quantum system and have shown that
the optimal time evolution required to transform a given initial state
$|\psi_i\rangle$ into a specific final state $|\psi_f\rangle$ can be made
arbitrarily small. A... | quant-ph | recently bender et al have considered the quantum brachistochrone problem for the nonhermitian cal ptsymmetric quantum system and have shown that the optimal time evolution required to transform a given initial state psi_irangle into a specific final state psi_frangle can be made arbitrarily small additionally it has b... | [['recently', 'bender', 'et', 'al', 'have', 'considered', 'the', 'quantum', 'brachistochrone', 'problem', 'for', 'the', 'nonhermitian', 'cal', 'ptsymmetric', 'quantum', 'system', 'and', 'have', 'shown', 'that', 'the', 'optimal', 'time', 'evolution', 'required', 'to', 'transform', 'a', 'given', 'initial', 'state', 'psi_... | [-0.12966132443165407, 0.12071350482292473, -0.06831180131528526, 0.01564375519170426, -0.048695951774716376, -0.1511319153616205, 0.006747129353461787, 0.3411450643185526, -0.25920879262499513, -0.2959589724056423, 0.09701427949243226, -0.23236749909818172, -0.2071473179291934, 0.196797639913857, -0.05354667511361186,... |
707.2737 | Black Holes in Cascading Theories: Confinement/Deconfinement Transition
and other Thermal Properties | We present numerical evidence for a transition between the Klebanov-Strassler
background and a solution describing a black hole in the class of cascading
solutions in the chirally restored phase. We also present a number of
properties of this solution, including the running of the coupling constant,
the viscosity to ... | hep-th gr-qc hep-ph | we present numerical evidence for a transition between the klebanovstrassler background and a solution describing a black hole in the class of cascading solutions in the chirally restored phase we also present a number of properties of this solution including the running of the coupling constant the viscosity to entrop... | [['we', 'present', 'numerical', 'evidence', 'for', 'a', 'transition', 'between', 'the', 'klebanovstrassler', 'background', 'and', 'a', 'solution', 'describing', 'a', 'black', 'hole', 'in', 'the', 'class', 'of', 'cascading', 'solutions', 'in', 'the', 'chirally', 'restored', 'phase', 'we', 'also', 'present', 'a', 'number... | [-0.18670808792775195, 0.1145397690275023, -0.09369257416936659, 0.020903837893368495, -0.02241699923310549, -0.06954809175353617, 0.08541001339824195, 0.29965730227770343, -0.1900434612086223, -0.2948797215977984, 0.08359216364859152, -0.3105190962913536, -0.11905497888613853, 0.11671974792355491, 0.004896919468357679... |
707.2738 | Confinement from gluodynamics in curved space-time | We determine the static potential for a heavy quark-antiquark pair from
gluodynamics in curved space-time. Our calculation is done within the framework
of the gauge-invariant, path-dependent, variables formalism. The potential
energy is the sum of a Yukawa and a linear potential, leading to the
confinement of static ... | hep-th | we determine the static potential for a heavy quarkantiquark pair from gluodynamics in curved spacetime our calculation is done within the framework of the gaugeinvariant pathdependent variables formalism the potential energy is the sum of a yukawa and a linear potential leading to the confinement of static charges | [['we', 'determine', 'the', 'static', 'potential', 'for', 'a', 'heavy', 'quarkantiquark', 'pair', 'from', 'gluodynamics', 'in', 'curved', 'spacetime', 'our', 'calculation', 'is', 'done', 'within', 'the', 'framework', 'of', 'the', 'gaugeinvariant', 'pathdependent', 'variables', 'formalism', 'the', 'potential', 'energy',... | [-0.13081020768731833, 0.14137028565164655, -0.11041694769907433, 0.10380640584723248, -0.05011810036861183, -0.09584616030527589, 0.04533912016389271, 0.32355079244977486, -0.18722726517201713, -0.23643053998239338, -0.03562756394239841, -0.2877280714067941, -0.09698061412200332, 0.06334322256346543, 0.040360939722935... |
707.2739 | On Cycles in the Transcription Network of Saccharomyces cerevisiae | We investigate the cycles in the transcription network of S. cerevisiae.
Unlike a similar network of E. coli, it contains many cycles. We characterize
properties of these cycles and their place in the regulatory mechanism of the
cell. Almost all cycles in the transcription network of S. cerevisiae are
contained in a ... | q-bio.MN q-bio.GN | we investigate the cycles in the transcription network of s cerevisiae unlike a similar network of e coli it contains many cycles we characterize properties of these cycles and their place in the regulatory mechanism of the cell almost all cycles in the transcription network of s cerevisiae are contained in a single st... | [['we', 'investigate', 'the', 'cycles', 'in', 'the', 'transcription', 'network', 'of', 's', 'cerevisiae', 'unlike', 'a', 'similar', 'network', 'of', 'e', 'coli', 'it', 'contains', 'many', 'cycles', 'we', 'characterize', 'properties', 'of', 'these', 'cycles', 'and', 'their', 'place', 'in', 'the', 'regulatory', 'mechanis... | [-0.19853494190664978, 0.16056005889918254, 0.01924618556609236, 0.02977187436993552, 0.01942975292049097, -0.13259794188364712, 0.08355953851380711, 0.39505827026088025, -0.22049348437736196, -0.2782433902498979, 0.07974731438117345, -0.28141604791167446, -0.21179041868362591, 0.1650726902760361, -0.05089237524062898,... |
707.274 | Mass, radius, and composition of the outer crust of nonaccreting cold
neutron stars | The properties and composition of the outer crust of nonaccreting cold
neutron stars are studied by applying the model of Baym, Pethick, and
Sutherland, which was extended by including higher order corrections of the
atomic binding, screening, exchange and zero-point energy. The most recent
experimental nuclear data ... | astro-ph nucl-th | the properties and composition of the outer crust of nonaccreting cold neutron stars are studied by applying the model of baym pethick and sutherland which was extended by including higher order corrections of the atomic binding screening exchange and zeropoint energy the most recent experimental nuclear data from the ... | [['the', 'properties', 'and', 'composition', 'of', 'the', 'outer', 'crust', 'of', 'nonaccreting', 'cold', 'neutron', 'stars', 'are', 'studied', 'by', 'applying', 'the', 'model', 'of', 'baym', 'pethick', 'and', 'sutherland', 'which', 'was', 'extended', 'by', 'including', 'higher', 'order', 'corrections', 'of', 'the', 'a... | [-0.00754382039177353, 0.1922156749698131, -0.06964809864799937, 0.11380968968100522, -0.04805152953966804, -0.045491598975723205, 0.020034171881802055, 0.3275292565803165, -0.19921546782184715, -0.3508974711840932, 0.04657365180875944, -0.2825659409975228, 0.038035208419086815, 0.17850341035012643, 0.01967977919494328... |
707.2741 | Equidistribution of negative statistics and quotients of Coxeter groups
of type B and D | We generalize some identities and q-identities previously known for the
symmetric group to Coxeter groups of type B and D. The extended results include
theorems of Foata and Sch\"utzenberger, Gessel, and Roselle on various
distributions of inversion number, major index, and descent number. In order to
show our result... | math.CO | we generalize some identities and qidentities previously known for the symmetric group to coxeter groups of type b and d the extended results include theorems of foata and schutzenberger gessel and roselle on various distributions of inversion number major index and descent number in order to show our results we provid... | [['we', 'generalize', 'some', 'identities', 'and', 'qidentities', 'previously', 'known', 'for', 'the', 'symmetric', 'group', 'to', 'coxeter', 'groups', 'of', 'type', 'b', 'and', 'd', 'the', 'extended', 'results', 'include', 'theorems', 'of', 'foata', 'and', 'schutzenberger', 'gessel', 'and', 'roselle', 'on', 'various',... | [-0.1423054737405795, 0.07766741086644205, -0.05471470115254774, 0.05676225126918518, -0.08631252934874008, -0.1472320727383097, 0.06287950315428051, 0.32570424920766416, -0.27103578070686624, -0.31455568100015324, 0.11361142558885287, -0.25640970855161094, -0.15573747362941504, 0.21231298772335955, -0.1411568922922015... |
707.2742 | Description of double beta decay within continuum-QRPA | A method to calculate the nuclear double beta decay ($2\nu\beta\beta$- and
$0\nu\beta\beta$-) amplitudes within the continuum random phase approximation
(cQRPA) is formulated. Calculations of the $\beta\beta$ transition amplitudes
within the cQRPA are performed for ^{76}Ge, ^{100}Mo and ^{130}Te. A rather
simple nucl... | nucl-th | a method to calculate the nuclear double beta decay 2nubetabeta and 0nubetabeta amplitudes within the continuum random phase approximation cqrpa is formulated calculations of the betabeta transition amplitudes within the cqrpa are performed for 76ge 100mo and 130te a rather simple nuclear hamiltonian consisting of phen... | [['a', 'method', 'to', 'calculate', 'the', 'nuclear', 'double', 'beta', 'decay', '2nubetabeta', 'and', '0nubetabeta', 'amplitudes', 'within', 'the', 'continuum', 'random', 'phase', 'approximation', 'cqrpa', 'is', 'formulated', 'calculations', 'of', 'the', 'betabeta', 'transition', 'amplitudes', 'within', 'the', 'cqrpa'... | [-0.08097046003516378, 0.24539384396810984, -0.09732063811930732, 0.15580101851634842, 0.025180827304399734, -0.12874265026766807, 0.042085479126022805, 0.35804843921856633, -0.20856185469391017, -0.21959783875078348, -0.006629401328170608, -0.28578422215349714, -0.05772605344075067, 0.12258916763901903, 0.081064995526... |
707.2743 | Charge Order Superstructure with Integer Iron Valence in Fe2OBO3 | Solution-grown single crystals of Fe2OBO3 were characterized by specific
heat, Mossbauer spectroscopy, and x-ray diffraction. A peak in the specific
heat at 340 K indicates the onset of charge order. Evidence for a doubling of
the unit cell at low temperature is presented. Combining structural refinement
of diffracti... | cond-mat.str-el cond-mat.mtrl-sci | solutiongrown single crystals of fe2obo3 were characterized by specific heat mossbauer spectroscopy and xray diffraction a peak in the specific heat at 340 k indicates the onset of charge order evidence for a doubling of the unit cell at low temperature is presented combining structural refinement of diffraction data a... | [['solutiongrown', 'single', 'crystals', 'of', 'fe2obo3', 'were', 'characterized', 'by', 'specific', 'heat', 'mossbauer', 'spectroscopy', 'and', 'xray', 'diffraction', 'a', 'peak', 'in', 'the', 'specific', 'heat', 'at', '340', 'k', 'indicates', 'the', 'onset', 'of', 'charge', 'order', 'evidence', 'for', 'a', 'doubling'... | [-0.1321478254746559, 0.2162084993737111, 0.011761598795284193, 0.019734247547011217, -0.025401793661267432, -0.11631395462034054, 0.15266642564377034, 0.39996299416173337, -0.2377979210902785, -0.3028268635619518, 0.049233208331929214, -0.4043479338288307, -0.03210154674990579, 0.14615889184507216, 0.06826772965317549... |
707.2744 | Simulation of the Formation and Morphology of Ice Mantles on
Interstellar Grains | Although still poorly understood, the chemistry that occurs on the surfaces
of interstellar dust particles profoundly affects the growth of molecules in
the interstellar medium. An important set of surface reactions produces icy
mantles of many monolayers in cold and dense regions. The monolayers are
dominated by wat... | astro-ph | although still poorly understood the chemistry that occurs on the surfaces of interstellar dust particles profoundly affects the growth of molecules in the interstellar medium an important set of surface reactions produces icy mantles of many monolayers in cold and dense regions the monolayers are dominated by water ic... | [['although', 'still', 'poorly', 'understood', 'the', 'chemistry', 'that', 'occurs', 'on', 'the', 'surfaces', 'of', 'interstellar', 'dust', 'particles', 'profoundly', 'affects', 'the', 'growth', 'of', 'molecules', 'in', 'the', 'interstellar', 'medium', 'an', 'important', 'set', 'of', 'surface', 'reactions', 'produces',... | [-0.04069653933443433, 0.19512379785484868, -0.046962981624198506, 0.05681723338082856, 0.026848247890684303, -0.04148531852435347, -0.001755696330846994, 0.4266952226196039, -0.2504442337213467, -0.3020885050534568, 0.05313697850318454, -0.24832374027249873, -0.11616015293230245, 0.15086000690737025, -0.01234561910337... |
707.2745 | On the renormalization of the bosonized multi-flavor Schwinger model | The phase structure of the bosonized multi-flavor Schwinger model is
investigated by means of the differential renormalization group (RG) method. In
the limit of small fermion mass the linearized RG flow is sufficient to
determine the low-energy behavior of the N-flavor model, if it has been rotated
by a suitable rot... | hep-th | the phase structure of the bosonized multiflavor schwinger model is investigated by means of the differential renormalization group rg method in the limit of small fermion mass the linearized rg flow is sufficient to determine the lowenergy behavior of the nflavor model if it has been rotated by a suitable rotation in ... | [['the', 'phase', 'structure', 'of', 'the', 'bosonized', 'multiflavor', 'schwinger', 'model', 'is', 'investigated', 'by', 'means', 'of', 'the', 'differential', 'renormalization', 'group', 'rg', 'method', 'in', 'the', 'limit', 'of', 'small', 'fermion', 'mass', 'the', 'linearized', 'rg', 'flow', 'is', 'sufficient', 'to',... | [-0.18388025187776608, 0.21742292448170175, -0.0762721997751154, 0.06263003095384102, -0.041197698070736956, -0.16430176469335747, 0.014395779768420646, 0.32419568303325946, -0.22691272905727555, -0.2804180139768099, 0.09560647214212539, -0.2547888451848518, -0.11101995684853024, 0.10004830550525554, 0.0288171956030852... |
707.2746 | The primordial binary population II: Recovering the binary population
for intermediate mass stars in Sco OB2 | We characterize the binary population in the young and nearby OB association
Scorpius OB2 using available observations of visual, spectroscopic, and
astrometric binaries with intermediate-mass primaries. We take into account
observational biases by comparing the observations with simulated observations
of model assoc... | astro-ph | we characterize the binary population in the young and nearby ob association scorpius ob2 using available observations of visual spectroscopic and astrometric binaries with intermediatemass primaries we take into account observational biases by comparing the observations with simulated observations of model association... | [['we', 'characterize', 'the', 'binary', 'population', 'in', 'the', 'young', 'and', 'nearby', 'ob', 'association', 'scorpius', 'ob2', 'using', 'available', 'observations', 'of', 'visual', 'spectroscopic', 'and', 'astrometric', 'binaries', 'with', 'intermediatemass', 'primaries', 'we', 'take', 'into', 'account', 'observ... | [-0.12573802999419267, 0.12600648158631933, -0.06661604403879473, 0.10549524095444948, -0.10098280795834592, -0.08942294145852857, 0.12392032964669086, 0.38776257948420656, -0.162804305075052, -0.3460922620305028, 0.06289926380086995, -0.303778573879565, -0.026798970845929995, 0.18680380231985833, -0.0446595752133372, ... |
707.2747 | Magnetohydrodynamic properties of incompressible Meissner fluids | We consider a superconducting material that exists in the liquid state, more
precisely, in which the Meissner-Ochsenfeld effect persists in the liquid
state. First, we investigate how the shape of such a hypothetical Meissner
liquid will adapt to accomodate for an applied external field. In particular,
we analyse the... | cond-mat.supr-con | we consider a superconducting material that exists in the liquid state more precisely in which the meissnerochsenfeld effect persists in the liquid state first we investigate how the shape of such a hypothetical meissner liquid will adapt to accomodate for an applied external field in particular we analyse the case of ... | [['we', 'consider', 'a', 'superconducting', 'material', 'that', 'exists', 'in', 'the', 'liquid', 'state', 'more', 'precisely', 'in', 'which', 'the', 'meissnerochsenfeld', 'effect', 'persists', 'in', 'the', 'liquid', 'state', 'first', 'we', 'investigate', 'how', 'the', 'shape', 'of', 'such', 'a', 'hypothetical', 'meissn... | [-0.16520761586975174, 0.1840771903145651, -0.09726337455545685, 0.05991551642655395, -0.05793024736589619, -0.07936448252294212, 0.029120407552857483, 0.31510903462767603, -0.2301016064452207, -0.2466832512590502, 0.08481260238082282, -0.23472928021427444, -0.14022725677516842, 0.1917023169026444, -0.01280662126373499... |
707.2748 | Theory of gravitation theories: a no-progress report | Already in the 1970s there where attempts to present a set of ground rules,
sometimes referred to as a theory of gravitation theories, which theories of
gravity should satisfy in order to be considered viable in principle and,
therefore, interesting enough to deserve further investigation. From this
perspective, an a... | gr-qc astro-ph hep-th | already in the 1970s there where attempts to present a set of ground rules sometimes referred to as a theory of gravitation theories which theories of gravity should satisfy in order to be considered viable in principle and therefore interesting enough to deserve further investigation from this perspective an alternati... | [['already', 'in', 'the', '1970s', 'there', 'where', 'attempts', 'to', 'present', 'a', 'set', 'of', 'ground', 'rules', 'sometimes', 'referred', 'to', 'as', 'a', 'theory', 'of', 'gravitation', 'theories', 'which', 'theories', 'of', 'gravity', 'should', 'satisfy', 'in', 'order', 'to', 'be', 'considered', 'viable', 'in', ... | [-0.08120506135770005, 0.09247055547075886, -0.11787380242201301, 0.14232300453823968, -0.14888695802363516, -0.13334446124482288, 0.02984449257367564, 0.34564702324881985, -0.2488480047670318, -0.30912826491047196, 0.10184048461051315, -0.2425954247563058, -0.17657453885454852, 0.18018384188974268, -0.0978901502768977... |
707.2749 | Black holes: interfacing the classical and the quantum | The central idea advocated in this paper is that {forming the black hole
horizon is attended with transition from the classical regime of evolution to
the quantum one}. We justify the following criterion for discriminating between
the classical and the quantum: {spontaneous creations and annihilations of
particle-ant... | gr-qc | the central idea advocated in this paper is that forming the black hole horizon is attended with transition from the classical regime of evolution to the quantum one we justify the following criterion for discriminating between the classical and the quantum spontaneous creations and annihilations of particleantiparticl... | [['the', 'central', 'idea', 'advocated', 'in', 'this', 'paper', 'is', 'that', 'forming', 'the', 'black', 'hole', 'horizon', 'is', 'attended', 'with', 'transition', 'from', 'the', 'classical', 'regime', 'of', 'evolution', 'to', 'the', 'quantum', 'one', 'we', 'justify', 'the', 'following', 'criterion', 'for', 'discrimina... | [-0.11570050108307244, 0.12970873997614218, -0.12290229990848921, 0.10375072885358678, -0.06113182558286665, -0.11431365935604318, 0.012894316449882868, 0.32135395851008175, -0.2744716784218326, -0.2837582185756469, 0.05425312470617718, -0.2520217246348983, -0.14902632348104447, 0.1635510113399874, -0.05574870108883234... |
707.275 | Multiple Equilibria in a Single-Column Model of the Tropical Atmosphere | A single-column model run under the weak temperature gradient approximation,
a parameterization of large-scale dynamics appropriate for the tropical
atmosphere, is shown to have multiple stable equilibria. Under conditions
permitting persistent deep convection, the model has a statistically steady
state in which such... | physics.ao-ph | a singlecolumn model run under the weak temperature gradient approximation a parameterization of largescale dynamics appropriate for the tropical atmosphere is shown to have multiple stable equilibria under conditions permitting persistent deep convection the model has a statistically steady state in which such convect... | [['a', 'singlecolumn', 'model', 'run', 'under', 'the', 'weak', 'temperature', 'gradient', 'approximation', 'a', 'parameterization', 'of', 'largescale', 'dynamics', 'appropriate', 'for', 'the', 'tropical', 'atmosphere', 'is', 'shown', 'to', 'have', 'multiple', 'stable', 'equilibria', 'under', 'conditions', 'permitting',... | [-0.14043025299735531, 0.16497433834186215, -0.1288138345322188, 0.08194733627811622, -0.020501296662533766, -0.12162943454185392, 0.03219464199055972, 0.3546499735949671, -0.28706011921167374, -0.2893866618465194, 0.16270705267293928, -0.1549054255378638, -0.09858073580407482, 0.18244664493592128, -0.04426590449806741... |
707.2751 | Final stare interaction enhancement effect on the near threshold p\bar p
system in B^\pm\to p\bar p \p^\pm decay | We discuss the low-mass enhancement effect in the baryon-antibaryon invariant
mass in three-body baryonic B decays using final state interactions in the
framework of Regge theory. We show that the rescattering between baryonic pair
can reproduce the observed mass spectrum.
| hep-ph | we discuss the lowmass enhancement effect in the baryonantibaryon invariant mass in threebody baryonic b decays using final state interactions in the framework of regge theory we show that the rescattering between baryonic pair can reproduce the observed mass spectrum | [['we', 'discuss', 'the', 'lowmass', 'enhancement', 'effect', 'in', 'the', 'baryonantibaryon', 'invariant', 'mass', 'in', 'threebody', 'baryonic', 'b', 'decays', 'using', 'final', 'state', 'interactions', 'in', 'the', 'framework', 'of', 'regge', 'theory', 'we', 'show', 'that', 'the', 'rescattering', 'between', 'baryoni... | [-0.1116251271800138, 0.22546476325951517, -0.1432026035457966, 0.19479427682235836, -0.02043341366224922, -0.05166062577627599, -0.004470666161796544, 0.30755452984012666, -0.19653358813375235, -0.30690799045842143, -0.15145191796764265, -0.3071068813791499, -0.07906426071367605, 0.07396014304831625, 0.055388764245435... |
707.2752 | A Silver Anniversary Observation of the X-ray Emitting SN1978K in NGC
1313 | We describe the results of a 2003 Chandra ACIS-I observation of SN1978K. The
spectrum shows little flux below 0.6 keV, in contrast to the 2002 ACIS-S
observation that showed flux to 0.4 keV. Fitting the ACIS-I spectrum alone
leads to two solutions depending upon the value of the column density. A joint
fit using a du... | astro-ph | we describe the results of a 2003 chandra acisi observation of sn1978k the spectrum shows little flux below 06 kev in contrast to the 2002 aciss observation that showed flux to 04 kev fitting the acisi spectrum alone leads to two solutions depending upon the value of the column density a joint fit using a dual thermal ... | [['we', 'describe', 'the', 'results', 'of', 'a', '2003', 'chandra', 'acisi', 'observation', 'of', 'sn1978k', 'the', 'spectrum', 'shows', 'little', 'flux', 'below', '06', 'kev', 'in', 'contrast', 'to', 'the', '2002', 'aciss', 'observation', 'that', 'showed', 'flux', 'to', '04', 'kev', 'fitting', 'the', 'acisi', 'spectru... | [-0.03609100603909396, 0.10729790540319621, -0.09229389795458273, 0.05060936127967366, -0.05854097903322648, -0.0945232246975031, 0.1112050403306699, 0.3939349563134944, -0.19042134615216022, -0.39131579597425814, 0.07938010832020903, -0.31910372748970983, 0.016943721664959895, 0.19036951846963562, -0.06051415317034459... |
707.2753 | Extreme statistics for time series: Distribution of the maximum relative
to the initial value | The extreme statistics of time signals is studied when the maximum is
measured from the initial value. In the case of independent, identically
distributed (iid) variables, we classify the limiting distribution of the
maximum according to the properties of the parent distribution from which the
variables are drawn. Th... | cond-mat.stat-mech | the extreme statistics of time signals is studied when the maximum is measured from the initial value in the case of independent identically distributed iid variables we classify the limiting distribution of the maximum according to the properties of the parent distribution from which the variables are drawn then we tu... | [['the', 'extreme', 'statistics', 'of', 'time', 'signals', 'is', 'studied', 'when', 'the', 'maximum', 'is', 'measured', 'from', 'the', 'initial', 'value', 'in', 'the', 'case', 'of', 'independent', 'identically', 'distributed', 'iid', 'variables', 'we', 'classify', 'the', 'limiting', 'distribution', 'of', 'the', 'maximu... | [-0.10926818928885955, 0.17105463716188954, -0.10809648494474222, 0.07693556594587195, 0.003580719730587083, -0.10871341952118571, 0.024499049292764554, 0.3595795179946941, -0.28570590265963913, -0.27822174939912675, 0.08471014268065681, -0.28962476701149925, -0.08644848720028563, 0.17738518093382696, -0.02931924199898... |
707.2754 | On the internal space dependence of the static quark-antiquark potential
in ${\cal N}=4$ SYM plasma wind | We study the effect of the relative S^5-angle of a quark and an antiquark on
their static potential and the related screening length in a strongly coupled
moving ${\cal N}=4$ SYM plasma. The large velocity scaling law for the
screening length holds for any relative S^5-angle $\theta$. However, the
velocity independen... | hep-th | we study the effect of the relative s5angle of a quark and an antiquark on their static potential and the related screening length in a strongly coupled moving cal n4 sym plasma the large velocity scaling law for the screening length holds for any relative s5angle theta however the velocity independent prefactor z stro... | [['we', 'study', 'the', 'effect', 'of', 'the', 'relative', 's5angle', 'of', 'a', 'quark', 'and', 'an', 'antiquark', 'on', 'their', 'static', 'potential', 'and', 'the', 'related', 'screening', 'length', 'in', 'a', 'strongly', 'coupled', 'moving', 'cal', 'n4', 'sym', 'plasma', 'the', 'large', 'velocity', 'scaling', 'law'... | [-0.15596749464532844, 0.20498839261769863, -0.050348960938231074, 0.01646873111014519, -0.028942026123174546, -0.11778112514703362, 0.030772415059834236, 0.3653405737821703, -0.21061021480479358, -0.21943928738251145, 0.004086777575049595, -0.2848964583726577, -0.046377130410415524, 0.16459722214458902, 0.003229490986... |
707.2755 | Ricci Nilsoliton Black Holes | We follow a constructive approach and find higher-dimensional black holes
with Ricci nilsoliton horizons. The spacetimes are solutions to Einstein's
equation with a negative cosmological constant and generalises therefore,
anti-de Sitter black hole spacetimes. The approach combines a work by Lauret --
which relate so... | hep-th gr-qc math-ph math.MP | we follow a constructive approach and find higherdimensional black holes with ricci nilsoliton horizons the spacetimes are solutions to einsteins equation with a negative cosmological constant and generalises therefore antide sitter black hole spacetimes the approach combines a work by lauret which relate socalled ricc... | [['we', 'follow', 'a', 'constructive', 'approach', 'and', 'find', 'higherdimensional', 'black', 'holes', 'with', 'ricci', 'nilsoliton', 'horizons', 'the', 'spacetimes', 'are', 'solutions', 'to', 'einsteins', 'equation', 'with', 'a', 'negative', 'cosmological', 'constant', 'and', 'generalises', 'therefore', 'antide', 's... | [-0.1932251587257547, 0.0978801116414893, -0.07914316804164041, 0.1303467535516405, -0.14004948252606822, -0.2463563390754921, -0.11436238122504142, 0.32650244248620536, -0.07035732724688064, -0.23987529859325643, 0.1149353588491252, -0.35050091262654226, -0.15016881464901616, 0.15134472373608596, -0.10992919189571324,... |
707.2756 | First results on double beta decay modes of Cd, Te and Zn isotopes with
the COBRA experiment | Four 1cm^3 CdZnTe semiconductor detectors were operated in the Gran Sasso
National Laboratory to explore the feasibility of such devices for double beta
decay searches as proposed for the COBRA experiment. The research involved
background studies accompanied by measurements of energy resolution performed
at the surfa... | nucl-ex hep-ph nucl-th | four 1cm3 cdznte semiconductor detectors were operated in the gran sasso national laboratory to explore the feasibility of such devices for double beta decay searches as proposed for the cobra experiment the research involved background studies accompanied by measurements of energy resolution performed at the surface e... | [['four', '1cm3', 'cdznte', 'semiconductor', 'detectors', 'were', 'operated', 'in', 'the', 'gran', 'sasso', 'national', 'laboratory', 'to', 'explore', 'the', 'feasibility', 'of', 'such', 'devices', 'for', 'double', 'beta', 'decay', 'searches', 'as', 'proposed', 'for', 'the', 'cobra', 'experiment', 'the', 'research', 'i... | [-0.05799754775430569, 0.19024251219816507, -0.029096862695672934, 0.10079780010616078, 0.014687356361023644, -0.1434336730840561, 0.07060197675121291, 0.3436773848007707, -0.14693268763777964, -0.38362397786010716, 0.09404739903436754, -0.3575120045858271, 0.012517548856489799, 0.2540428336107117, 0.06912336949984926,... |
707.2757 | Singular Oscillatory Integrals on R^n | Let Pd,n denote the space of all real polynomials of degree at most d on R^n.
We prove a new estimate for the logarithmic measure of the sublevel set of a
polynomial P in Pd,1. Using this estimate, we prove a sharp estimate for a
singular oscillatory integral on R^n.
| math.CA | let pdn denote the space of all real polynomials of degree at most d on rn we prove a new estimate for the logarithmic measure of the sublevel set of a polynomial p in pd1 using this estimate we prove a sharp estimate for a singular oscillatory integral on rn | [['let', 'pdn', 'denote', 'the', 'space', 'of', 'all', 'real', 'polynomials', 'of', 'degree', 'at', 'most', 'd', 'on', 'rn', 'we', 'prove', 'a', 'new', 'estimate', 'for', 'the', 'logarithmic', 'measure', 'of', 'the', 'sublevel', 'set', 'of', 'a', 'polynomial', 'p', 'in', 'pd1', 'using', 'this', 'estimate', 'we', 'prove... | [-0.17580134431365876, 0.036460449025034904, -0.07366481182165444, 0.031839968708809466, -0.04174702860414982, -0.10898144003003836, 0.01991986666165758, 0.2435675104893744, -0.3009449779544957, -0.16282719268463552, 0.09239585971226916, -0.30183479396626356, -0.12157232734258287, 0.23397331153973938, -0.07235797109664... |
707.2758 | Measurement of the Semileptonic Decays B --> D tau nubar and B --> D*
tau nubar | We present preliminary measurements of branching fractions for the
semileptonic decays B --> D tau nubar and B --> D* tau nubar, which are
potentially sensitive to non--Standard Model amplitudes. The data sample
comprises 232x10^6 Upsilon(4S) --> BBbar decays collected with the BaBar
detector at the PEP-II e+e- stora... | hep-ex | we present preliminary measurements of branching fractions for the semileptonic decays b d tau nubar and b d tau nubar which are potentially sensitive to nonstandard model amplitudes the data sample comprises 232x106 upsilon4s bbbar decays collected with the babar detector at the pepii ee storage ring we obtain bb d0 t... | [['we', 'present', 'preliminary', 'measurements', 'of', 'branching', 'fractions', 'for', 'the', 'semileptonic', 'decays', 'b', 'd', 'tau', 'nubar', 'and', 'b', 'd', 'tau', 'nubar', 'which', 'are', 'potentially', 'sensitive', 'to', 'nonstandard', 'model', 'amplitudes', 'the', 'data', 'sample', 'comprises', '232x106', 'u... | [-0.1041057739429582, 0.26469247974805477, 0.012447284342006858, 0.03691476602212323, 0.021768564894039156, -0.23377506307473309, 0.199994597820341, 0.250518934556136, -0.18543471262223066, -0.3138425387162015, -0.040879246666747374, -0.5274197127726069, 0.2027500359467546, 0.13711643289718636, 0.057495770940935255, 0.... |
707.2759 | Encapsulation, compensation, and substitution of catalyst particles
during continuous growth of carbon nanotubes | By sequential feeding of catalyst materials, it is revealed that the active
growth sites are at the bottom of the carbon nanotubes (CNTs), and that
catalyst particles are constantly encapsulated into nanotubes from the bottom.
This gives a better insight into the mechanism of CNT formation and on ways to
control the ... | cond-mat.mtrl-sci cond-mat.other | by sequential feeding of catalyst materials it is revealed that the active growth sites are at the bottom of the carbon nanotubes cnts and that catalyst particles are constantly encapsulated into nanotubes from the bottom this gives a better insight into the mechanism of cnt formation and on ways to control the growth ... | [['by', 'sequential', 'feeding', 'of', 'catalyst', 'materials', 'it', 'is', 'revealed', 'that', 'the', 'active', 'growth', 'sites', 'are', 'at', 'the', 'bottom', 'of', 'the', 'carbon', 'nanotubes', 'cnts', 'and', 'that', 'catalyst', 'particles', 'are', 'constantly', 'encapsulated', 'into', 'nanotubes', 'from', 'the', '... | [-0.062225340776855036, 0.18126097200660124, -0.020077201210716294, -0.04821094599682987, 0.007003607062090721, -0.14841233501543424, 0.07339000979083635, 0.44288598864694084, -0.2683607860401805, -0.31749131477304865, 0.07689899617911405, -0.28968079215320314, -0.1298548646764608, 0.1849110932283414, 0.026846294197076... |
707.276 | Spanning Trees with Many Leaves in Graphs without Diamonds and Blossoms | It is known that graphs on n vertices with minimum degree at least 3 have
spanning trees with at least n/4+2 leaves and that this can be improved to
(n+4)/3 for cubic graphs without the diamond K_4-e as a subgraph. We generalize
the second result by proving that every graph with minimum degree at least 3,
without dia... | math.CO | it is known that graphs on n vertices with minimum degree at least 3 have spanning trees with at least n42 leaves and that this can be improved to n43 for cubic graphs without the diamond k_4e as a subgraph we generalize the second result by proving that every graph with minimum degree at least 3 without diamonds and c... | [['it', 'is', 'known', 'that', 'graphs', 'on', 'n', 'vertices', 'with', 'minimum', 'degree', 'at', 'least', '3', 'have', 'spanning', 'trees', 'with', 'at', 'least', 'n42', 'leaves', 'and', 'that', 'this', 'can', 'be', 'improved', 'to', 'n43', 'for', 'cubic', 'graphs', 'without', 'the', 'diamond', 'k_4e', 'as', 'a', 'su... | [-0.12077009102811555, 0.14555743447719857, -0.04825609087149476, 0.018353546079788747, -0.10275901592877153, -0.15474162415529674, 0.10999018669460568, 0.37656363734480486, -0.24279379498187478, -0.3783789028843435, 0.11461773813194172, -0.29650398681161705, -0.12003159278619488, 0.1170435600826139, -0.058626210544961... |
707.2761 | Muon-fluorine entangled states in molecular magnets | The information accessible from a muon-spin relaxation experiment is often
limited since we lack knowledge of the precise muon stopping site. We
demonstrate here the possibility of localizing a spin polarized muon in a known
stopping state in a molecular material containing fluorine. The muon-spin
precession that res... | cond-mat.str-el | the information accessible from a muonspin relaxation experiment is often limited since we lack knowledge of the precise muon stopping site we demonstrate here the possibility of localizing a spin polarized muon in a known stopping state in a molecular material containing fluorine the muonspin precession that results f... | [['the', 'information', 'accessible', 'from', 'a', 'muonspin', 'relaxation', 'experiment', 'is', 'often', 'limited', 'since', 'we', 'lack', 'knowledge', 'of', 'the', 'precise', 'muon', 'stopping', 'site', 'we', 'demonstrate', 'here', 'the', 'possibility', 'of', 'localizing', 'a', 'spin', 'polarized', 'muon', 'in', 'a',... | [-0.07891519349861018, 0.1719852670373276, -0.04300664807174434, 0.09305210283367914, -0.10187667211210553, -0.08662475781772841, 0.09844430386177958, 0.3940701944396851, -0.3139332400664608, -0.2806861435479306, 0.08618220758990959, -0.3094074538651299, -0.025670114017904123, 0.18607940384622743, 0.013362572226237426,... |
707.2762 | Darboux Transformation of the Green Function for the Dirac Equation with
the Generalized Potential | We consider the Darboux transformation of the Green functions of the regular
boundary problem of the one-dimensional stationary Dirac equation. We obtained
the Green functions of the transformed Dirac equation with the initial regular
boundary conditions. We also construct the formula for the unabridged trace of
the ... | hep-th | we consider the darboux transformation of the green functions of the regular boundary problem of the onedimensional stationary dirac equation we obtained the green functions of the transformed dirac equation with the initial regular boundary conditions we also construct the formula for the unabridged trace of the diffe... | [['we', 'consider', 'the', 'darboux', 'transformation', 'of', 'the', 'green', 'functions', 'of', 'the', 'regular', 'boundary', 'problem', 'of', 'the', 'onedimensional', 'stationary', 'dirac', 'equation', 'we', 'obtained', 'the', 'green', 'functions', 'of', 'the', 'transformed', 'dirac', 'equation', 'with', 'the', 'init... | [-0.1562745295219369, 0.06970995044029334, -0.11117948213551235, 0.07779383536551025, -0.05518312099041765, -0.07982770582292598, 0.0212446815221683, 0.3139628856391697, -0.2865130176747238, -0.19659266641343032, 0.10050985915074637, -0.28052157182777354, -0.17375305466927016, 0.16410992018863108, 0.03290065668605186, ... |
707.2763 | Large Area Growth of Aligned CNT Arrays on Spheres: Towards the Large
Scale and Continuous Production | A novel strategy for the large scale and continuous production of aligned
carbon nanotube arrays using millimeter-diameter spheres as growth substrates
is reported. The present technique is more productive than the conventional
process on flat wafers because of the higher available growth surface and the
good fluidit... | cond-mat.mtrl-sci cond-mat.other | a novel strategy for the large scale and continuous production of aligned carbon nanotube arrays using millimeterdiameter spheres as growth substrates is reported the present technique is more productive than the conventional process on flat wafers because of the higher available growth surface and the good fluidity of... | [['a', 'novel', 'strategy', 'for', 'the', 'large', 'scale', 'and', 'continuous', 'production', 'of', 'aligned', 'carbon', 'nanotube', 'arrays', 'using', 'millimeterdiameter', 'spheres', 'as', 'growth', 'substrates', 'is', 'reported', 'the', 'present', 'technique', 'is', 'more', 'productive', 'than', 'the', 'conventiona... | [-0.07779885708587245, 0.1597590370103717, -0.00836781397062753, -0.016527762016916574, -0.032271425904972215, -0.17180431460895176, -0.006761259070065404, 0.4723504413318421, -0.2242030775706683, -0.2760653545065517, 0.12859278015925416, -0.25424907385105533, -0.090790258454425, 0.2529982103433992, 0.00544228261652668... |
707.2764 | Velocities from Cross-Correlation: A Guide for Self-Improvement | The measurement of Doppler velocity shifts in spectra is a ubiquitous theme
in astronomy, usually handled by computing the cross-correlation of the
signals, and finding the location of its maximum. This paper addresses the
problem of the determination of wavelength or velocity shifts among multiple
spectra of the sam... | astro-ph | the measurement of doppler velocity shifts in spectra is a ubiquitous theme in astronomy usually handled by computing the crosscorrelation of the signals and finding the location of its maximum this paper addresses the problem of the determination of wavelength or velocity shifts among multiple spectra of the same or v... | [['the', 'measurement', 'of', 'doppler', 'velocity', 'shifts', 'in', 'spectra', 'is', 'a', 'ubiquitous', 'theme', 'in', 'astronomy', 'usually', 'handled', 'by', 'computing', 'the', 'crosscorrelation', 'of', 'the', 'signals', 'and', 'finding', 'the', 'location', 'of', 'its', 'maximum', 'this', 'paper', 'addresses', 'the... | [-0.11527664202302204, 0.08970788144644375, -0.07617714354327243, 0.04109329725554409, -0.09241064295760895, -0.10836841545655931, 0.04867741727135389, 0.3599032564186736, -0.24748187274917177, -0.352638532535026, 0.08176996226018099, -0.27533904384625585, -0.06778486499893724, 0.2301886599155535, -0.050261063013519895... |
707.2765 | Magnetic domain fluctuations in an antiferromagnetic film observed with
coherent resonant soft x-ray scattering | We report the direct observation of slow fluctuations of helical
antiferromagnetic domains in an ultra-thin holmium film using coherent resonant
magnetic x-ray scattering. We observe a gradual increase of the fluctuations in
the speckle pattern with increasing temperature, while at the same time a
static contribution... | cond-mat.other cond-mat.dis-nn cond-mat.mes-hall cond-mat.str-el | we report the direct observation of slow fluctuations of helical antiferromagnetic domains in an ultrathin holmium film using coherent resonant magnetic xray scattering we observe a gradual increase of the fluctuations in the speckle pattern with increasing temperature while at the same time a static contribution to th... | [['we', 'report', 'the', 'direct', 'observation', 'of', 'slow', 'fluctuations', 'of', 'helical', 'antiferromagnetic', 'domains', 'in', 'an', 'ultrathin', 'holmium', 'film', 'using', 'coherent', 'resonant', 'magnetic', 'xray', 'scattering', 'we', 'observe', 'a', 'gradual', 'increase', 'of', 'the', 'fluctuations', 'in', ... | [-0.21220329069696806, 0.22578202366216027, -0.090840690796647, 0.02521321484271218, -0.008232146090663531, -0.0305151523090899, 0.06827276485752971, 0.38676206565955107, -0.3152573451618938, -0.29085736500428006, 0.034901153600281655, -0.2928340671693577, -0.0892022984513246, 0.16819499169257196, 0.034123799243174935,... |
707.2766 | A two-state model for helicase translocation and unwinding of nucleic
acids | Helicases are molecular motors that unwind double-stranded nucleic acids
(dsNA), such as DNA and RNA). Typically a helicase translocates along one of
the NA single strands while unwinding and uses adenosine triphosphate (ATP)
hydrolysis as an energy source. Here we model of a helicase motor that can
switch between tw... | physics.bio-ph | helicases are molecular motors that unwind doublestranded nucleic acids dsna such as dna and rna typically a helicase translocates along one of the na single strands while unwinding and uses adenosine triphosphate atp hydrolysis as an energy source here we model of a helicase motor that can switch between two states wh... | [['helicases', 'are', 'molecular', 'motors', 'that', 'unwind', 'doublestranded', 'nucleic', 'acids', 'dsna', 'such', 'as', 'dna', 'and', 'rna', 'typically', 'a', 'helicase', 'translocates', 'along', 'one', 'of', 'the', 'na', 'single', 'strands', 'while', 'unwinding', 'and', 'uses', 'adenosine', 'triphosphate', 'atp', '... | [-0.13541527288832836, 0.1344885595769821, -0.05056468798379813, 0.012043029025330075, -0.0021858736593276264, -0.1953464346671743, 0.09443145289218852, 0.38382178928170885, -0.24638098150491713, -0.27113367699984725, 0.02094843489650105, -0.2720824694221041, -0.1781589851064408, 0.19905112962504581, -0.042013366067050... |
707.2767 | Strange quark contributions to neutrino and antineutrino nucleus
scattering via neutral current in quasi-elastic region | Strange quark contributions to the neutral current reaction in the neutrino
scattering are investigated on the nucleon level and extended to the $^{12}$C
target nucleus through the neutrino-induced knocked-out nucleon process in the
quasi-elastic region within the framework of a relativistic single particle
model. Th... | nucl-th | strange quark contributions to the neutral current reaction in the neutrino scattering are investigated on the nucleon level and extended to the 12c target nucleus through the neutrinoinduced knockedout nucleon process in the quasielastic region within the framework of a relativistic single particle model the incident ... | [['strange', 'quark', 'contributions', 'to', 'the', 'neutral', 'current', 'reaction', 'in', 'the', 'neutrino', 'scattering', 'are', 'investigated', 'on', 'the', 'nucleon', 'level', 'and', 'extended', 'to', 'the', '12c', 'target', 'nucleus', 'through', 'the', 'neutrinoinduced', 'knockedout', 'nucleon', 'process', 'in', ... | [-0.03962621376793381, 0.2693631023303756, -0.05816022966164089, 0.17386002841294612, 0.003653965226417753, -0.07697579229716212, 0.0680162732906249, 0.3234562170241148, -0.19796241889707744, -0.266381558676761, -0.09961211442902324, -0.34894664406085446, 0.03159837547742251, 0.12602475588491577, 0.1362058130398509, 0.... |
707.2768 | Incompressible fluid inside an astrophysical black hole? | It is argued that under natural hypothesis the Fermions inside a black hole
formed after the collapse of a neutron star could form a non compressible fluid
(well before reaching the Planck scale) leading to some features of integer
Quantum Hall Effect. The relations with black hole entropy are analyzed.
Insights comi... | gr-qc astro-ph cond-mat.mes-hall hep-th | it is argued that under natural hypothesis the fermions inside a black hole formed after the collapse of a neutron star could form a non compressible fluid well before reaching the planck scale leading to some features of integer quantum hall effect the relations with black hole entropy are analyzed insights coming fro... | [['it', 'is', 'argued', 'that', 'under', 'natural', 'hypothesis', 'the', 'fermions', 'inside', 'a', 'black', 'hole', 'formed', 'after', 'the', 'collapse', 'of', 'a', 'neutron', 'star', 'could', 'form', 'a', 'non', 'compressible', 'fluid', 'well', 'before', 'reaching', 'the', 'planck', 'scale', 'leading', 'to', 'some', ... | [-0.14132557942727467, 0.20969753681084163, -0.11943050396893128, 0.10621914010707657, -0.09522335385374817, -0.19361766399298277, -0.002927232438836385, 0.2636357034430092, -0.24057025214036307, -0.2830108746104402, 0.10155368814198876, -0.31599856685433125, -0.13020805637984548, 0.216718949423528, 0.00033331706108134... |
707.2769 | Dynamics of Dense Cores in the Perseus Molecular Cloud | We survey the kinematics of over one hundred and fifty candidate (and
potentially star-forming) dense cores in the Perseus molecular cloud with
pointed N2H+(1-0) and simultaneous C18O(2-1) observations. Our detection rate
of N2H+ is 62%, rising to 84% for JCMT SCUBA-selected targets. In agreement
with previous observ... | astro-ph | we survey the kinematics of over one hundred and fifty candidate and potentially starforming dense cores in the perseus molecular cloud with pointed n2h10 and simultaneous c18o21 observations our detection rate of n2h is 62 rising to 84 for jcmt scubaselected targets in agreement with previous observations we find that... | [['we', 'survey', 'the', 'kinematics', 'of', 'over', 'one', 'hundred', 'and', 'fifty', 'candidate', 'and', 'potentially', 'starforming', 'dense', 'cores', 'in', 'the', 'perseus', 'molecular', 'cloud', 'with', 'pointed', 'n2h10', 'and', 'simultaneous', 'c18o21', 'observations', 'our', 'detection', 'rate', 'of', 'n2h', '... | [-0.07682973296685114, 0.0918911905446796, -0.015950370924701678, 0.04761686983315058, -0.03726870920612008, -0.02975380938057659, 0.05222444266443609, 0.46392625303249496, -0.13657055074350333, -0.3295724854099652, 0.06614100713172197, -0.27206341135032597, -0.0258864082643011, 0.17002542359620662, -0.0059674083589201... |
707.277 | Neon Abundances from a Spitzer/IRS Survey of Wolf-Rayet Stars | We report on neon abundances derived from {\it Spitzer} high resolution
spectral data of eight Wolf-Rayet (WR) stars using the forbidden line of
[\ion{Ne}{3}] 15.56 microns. Our targets include four WN stars of subtypes
4--7, and four WC stars of subtypes 4--7. We derive ion fraction abundances
$\gamma$ of Ne^{2+} fo... | astro-ph | we report on neon abundances derived from it spitzer high resolution spectral data of eight wolfrayet wr stars using the forbidden line of ionne3 1556 microns our targets include four wn stars of subtypes 47 and four wc stars of subtypes 47 we derive ion fraction abundances gamma of ne2 for the winds of each star the i... | [['we', 'report', 'on', 'neon', 'abundances', 'derived', 'from', 'it', 'spitzer', 'high', 'resolution', 'spectral', 'data', 'of', 'eight', 'wolfrayet', 'wr', 'stars', 'using', 'the', 'forbidden', 'line', 'of', 'ionne3', '1556', 'microns', 'our', 'targets', 'include', 'four', 'wn', 'stars', 'of', 'subtypes', '47', 'and'... | [-0.01693818335317903, 0.1644646792534601, 0.029753407012860947, 0.036784922097231845, -0.007814981179156652, -0.0604262926865852, 0.11933461850060632, 0.4061100908934518, -0.09443868748214165, -0.35355386155209056, -0.028664255146092426, -0.35037427918157643, 0.08409609569719544, 0.17708473271664438, -0.06083699186867... |
707.2771 | The pressure confined wind of the massive and compact superstar cluster
M82-A1 | The observed parameters of the young superstar cluster M82-A1 and its
associated compact HII region are here shown to indicate a low heating
efficiency or immediate loss, through radiative cooling, of a large fraction of
the energy inserted by stellar winds and supernovae during the early evolution
of the cluster. Th... | astro-ph | the observed parameters of the young superstar cluster m82a1 and its associated compact hii region are here shown to indicate a low heating efficiency or immediate loss through radiative cooling of a large fraction of the energy inserted by stellar winds and supernovae during the early evolution of the cluster this imp... | [['the', 'observed', 'parameters', 'of', 'the', 'young', 'superstar', 'cluster', 'm82a1', 'and', 'its', 'associated', 'compact', 'hii', 'region', 'are', 'here', 'shown', 'to', 'indicate', 'a', 'low', 'heating', 'efficiency', 'or', 'immediate', 'loss', 'through', 'radiative', 'cooling', 'of', 'a', 'large', 'fraction', '... | [-0.07434527421124801, 0.12070939271780913, -0.06004610231586842, 0.06885116226953625, -0.08211773489001056, -0.032970689915581254, 0.05394482667249958, 0.38308621461312936, -0.23379706885785825, -0.32173088410248357, 0.0839352004733237, -0.22246683505801884, -0.029413903348638568, 0.20184223438858465, 0.00096418805759... |
707.2772 | Bures metric over thermal state manifolds and quantum criticality | We analyze the Bures metric over the manifold of thermal density matrices for
systems featuring a zero temperature quantum phase transition. We show that the
quantum critical region can be characterized in terms of the temperature
scaling behavior of the metric tensor itself. Furthermore, the analysis of the
metric t... | quant-ph | we analyze the bures metric over the manifold of thermal density matrices for systems featuring a zero temperature quantum phase transition we show that the quantum critical region can be characterized in terms of the temperature scaling behavior of the metric tensor itself furthermore the analysis of the metric tensor... | [['we', 'analyze', 'the', 'bures', 'metric', 'over', 'the', 'manifold', 'of', 'thermal', 'density', 'matrices', 'for', 'systems', 'featuring', 'a', 'zero', 'temperature', 'quantum', 'phase', 'transition', 'we', 'show', 'that', 'the', 'quantum', 'critical', 'region', 'can', 'be', 'characterized', 'in', 'terms', 'of', 't... | [-0.16107148603095037, 0.1737084279438836, -0.11422109184296507, 0.022986973572130268, -0.030189209254948716, -0.11647904042742754, 0.04859488059178387, 0.32508368033327556, -0.2550981215446403, -0.25354556448169446, 0.0994730630043992, -0.27906359492718413, -0.19806338203580756, 0.17884626278751775, -0.005309036874371... |
707.2773 | The dynamical hole in ultrafast photoassociation: analysis of the
compression effect | Photoassociation of a pair of cooled atoms by excitation with a short chirped
laser pulse creates a dynamical hole in the initial continuum wavefunction.
This hole is manifested by a void in the pair wavefunction and a momentum kick.
Photoassociation into loosely bound levels of the external well in Cs_2
0$_g^-$(6S +... | quant-ph | photoassociation of a pair of cooled atoms by excitation with a short chirped laser pulse creates a dynamical hole in the initial continuum wavefunction this hole is manifested by a void in the pair wavefunction and a momentum kick photoassociation into loosely bound levels of the external well in cs_2 0_g6s 6p_32 is c... | [['photoassociation', 'of', 'a', 'pair', 'of', 'cooled', 'atoms', 'by', 'excitation', 'with', 'a', 'short', 'chirped', 'laser', 'pulse', 'creates', 'a', 'dynamical', 'hole', 'in', 'the', 'initial', 'continuum', 'wavefunction', 'this', 'hole', 'is', 'manifested', 'by', 'a', 'void', 'in', 'the', 'pair', 'wavefunction', '... | [-0.1406314225253951, 0.20592731655078045, -0.07052960639317694, 0.07134132252368341, 0.01304405967207396, -0.09407099775946592, 0.07850745034757066, 0.37558096895189996, -0.24654133804992998, -0.299035685294261, 0.010480680334441295, -0.2485593881534591, -0.017719468501604857, 0.1554682798147814, 0.021717076476867478,... |
707.2774 | Mesoscopic model for the fluctuating hydrodynamics of binary and ternary
mixtures | A recently introduced particle-based model for fluid dynamics with continuous
velocities is generalized to model immiscible binary mixtures. Excluded volume
interactions between the two components are modeled by stochastic multiparticle
collisions which depend on the local velocities and densities. Momentum and
energ... | cond-mat.soft cond-mat.stat-mech | a recently introduced particlebased model for fluid dynamics with continuous velocities is generalized to model immiscible binary mixtures excluded volume interactions between the two components are modeled by stochastic multiparticle collisions which depend on the local velocities and densities momentum and energy are... | [['a', 'recently', 'introduced', 'particlebased', 'model', 'for', 'fluid', 'dynamics', 'with', 'continuous', 'velocities', 'is', 'generalized', 'to', 'model', 'immiscible', 'binary', 'mixtures', 'excluded', 'volume', 'interactions', 'between', 'the', 'two', 'components', 'are', 'modeled', 'by', 'stochastic', 'multipart... | [-0.12251685485748535, 0.17779504224241605, -0.10439141195835676, 0.03996247800728111, -0.020694600659181606, -0.127947943428388, -0.007802464836439886, 0.34318070069372236, -0.2330545804925732, -0.2879416790198196, 0.06228915442325097, -0.2912628008150398, -0.09622140589391591, 0.17769934014267438, 0.04465285412498288... |
707.2775 | Uniqueness theorem for 5-dimensional black holes with two axial Killing
fields | We show that two stationary, asymptotically flat vacuum black holes in 5
dimensions with two commuting axial symmetries are identical if and only if
their masses, angular momenta, and their ``rod structures'' coincide. We also
show that the horizon must be topologically either a 3-sphere, a ring, or a
Lens-space. Our... | gr-qc | we show that two stationary asymptotically flat vacuum black holes in 5 dimensions with two commuting axial symmetries are identical if and only if their masses angular momenta and their rod structures coincide we also show that the horizon must be topologically either a 3sphere a ring or a lensspace our argument is a ... | [['we', 'show', 'that', 'two', 'stationary', 'asymptotically', 'flat', 'vacuum', 'black', 'holes', 'in', '5', 'dimensions', 'with', 'two', 'commuting', 'axial', 'symmetries', 'are', 'identical', 'if', 'and', 'only', 'if', 'their', 'masses', 'angular', 'momenta', 'and', 'their', 'rod', 'structures', 'coincide', 'we', 'a... | [-0.18317099647639795, 0.14917878951704086, -0.09353785690050138, 0.0639548334793924, -0.07591304166762289, -0.1676920716120147, 0.0125551717491214, 0.37092012797244067, -0.18182072682890954, -0.26257002529509493, 0.12338306180331422, -0.2589356645557293, -0.13953767060762445, 0.15946115315675216, -0.08063644600211815,... |
707.2776 | A presentation for the mapping class group of a non-orientable surface
from the action on the complex of curves | We study the action of the mapping class group M(F) on the complex of curves
of a non-orientable surface F. We obtain, by using a result of K. S. Brown, a
presentation for M(F) defined in terms of the mapping class groups of the
complementary surfaces of collections of curves, provided that F is not
sporadic, i.e. th... | math.GT | we study the action of the mapping class group mf on the complex of curves of a nonorientable surface f we obtain by using a result of k s brown a presentation for mf defined in terms of the mapping class groups of the complementary surfaces of collections of curves provided that f is not sporadic ie the complex of cur... | [['we', 'study', 'the', 'action', 'of', 'the', 'mapping', 'class', 'group', 'mf', 'on', 'the', 'complex', 'of', 'curves', 'of', 'a', 'nonorientable', 'surface', 'f', 'we', 'obtain', 'by', 'using', 'a', 'result', 'of', 'k', 's', 'brown', 'a', 'presentation', 'for', 'mf', 'defined', 'in', 'terms', 'of', 'the', 'mapping',... | [-0.20786469169880872, 0.08444761399777583, -0.09247804214648994, 0.03820887556656, -0.08283353695806897, -0.102555607388049, 0.07479351167969497, 0.36544459800661344, -0.2551212341145233, -0.2605263422484751, 0.0887198442561598, -0.22682556974483126, -0.1831784177640522, 0.28327967628353723, -0.08440326572608571, -0.0... |
707.2777 | Suppression of hole-mediated ferromagnetism in GaMnP by hydrogen | We report the successful passivation of the Mn acceptors in GaMnP upon
exposure to a remote dc hydrogen plasma. The as-grown films are non-metallic
and ferromagnetic with a Curie temperature of T_C=55K. After hydrogenation the
sample resistivity increases by approximately three orders of magnitude at room
temperature... | cond-mat.mtrl-sci | we report the successful passivation of the mn acceptors in gamnp upon exposure to a remote dc hydrogen plasma the asgrown films are nonmetallic and ferromagnetic with a curie temperature of t_c55k after hydrogenation the sample resistivity increases by approximately three orders of magnitude at room temperature and si... | [['we', 'report', 'the', 'successful', 'passivation', 'of', 'the', 'mn', 'acceptors', 'in', 'gamnp', 'upon', 'exposure', 'to', 'a', 'remote', 'dc', 'hydrogen', 'plasma', 'the', 'asgrown', 'films', 'are', 'nonmetallic', 'and', 'ferromagnetic', 'with', 'a', 'curie', 'temperature', 'of', 't_c55k', 'after', 'hydrogenation'... | [-0.10894254031054694, 0.2211904362238962, 0.03494552506006086, -0.04852651095807589, 0.04600330840284918, -0.13005234786838876, 0.14191366254817694, 0.4428870475978828, -0.21065164553275442, -0.35196011221291973, 0.0164204724190081, -0.36914225514320764, -0.025409296278239173, 0.1635831177700311, 0.06860168201520163, ... |
707.2778 | Spitzer Transit and Secondary Eclipse Photometry of GJ 436b | We report the results of infrared (8 micron) transit and secondary eclipse
photometry of the hot Neptune exoplanet, GJ436b using Spitzer. The nearly
photon-limited precision of these data allow us to measure an improved radius
for the planet, and to detect the secondary eclipse. The transit (centered at
HJD = 2454280... | astro-ph | we report the results of infrared 8 micron transit and secondary eclipse photometry of the hot neptune exoplanet gj436b using spitzer the nearly photonlimited precision of these data allow us to measure an improved radius for the planet and to detect the secondary eclipse the transit centered at hjd 245428078149 000016... | [['we', 'report', 'the', 'results', 'of', 'infrared', '8', 'micron', 'transit', 'and', 'secondary', 'eclipse', 'photometry', 'of', 'the', 'hot', 'neptune', 'exoplanet', 'gj436b', 'using', 'spitzer', 'the', 'nearly', 'photonlimited', 'precision', 'of', 'these', 'data', 'allow', 'us', 'to', 'measure', 'an', 'improved', '... | [-0.1289239928153954, 0.14345906126128488, -0.10484076586875077, 0.06057162937168887, -0.0762115827433727, -0.06583140795689305, 0.08840062795206904, 0.3440679011163207, -0.1648222191819959, -0.378655980749778, 0.08662093588630954, -0.30521254397795666, -0.06721293299972099, 0.21200708968669404, -0.12191496747403349, 0... |
707.2779 | Independent Noise Approximation for Spin-Boson Decoherence | Quantum error correction is a solution to preserve the fidelity of quantum
information encoded in physical systems subject to noise. However, unfavorable
correlated errors could be induced even for non-interacting qubits through the
environment (bath), when they are "packed" together. The question is, to what
extent ... | quant-ph | quantum error correction is a solution to preserve the fidelity of quantum information encoded in physical systems subject to noise however unfavorable correlated errors could be induced even for noninteracting qubits through the environment bath when they are packed together the question is to what extent can we treat... | [['quantum', 'error', 'correction', 'is', 'a', 'solution', 'to', 'preserve', 'the', 'fidelity', 'of', 'quantum', 'information', 'encoded', 'in', 'physical', 'systems', 'subject', 'to', 'noise', 'however', 'unfavorable', 'correlated', 'errors', 'could', 'be', 'induced', 'even', 'for', 'noninteracting', 'qubits', 'throug... | [-0.13500752799997204, 0.18293070612605988, -0.058457242802863844, 0.11461125937823549, -0.01119093814243873, -0.22462701698225973, 0.04685071075596569, 0.3902144684015136, -0.282048395156795, -0.28004755486587163, 0.10377351886984941, -0.27758347416263923, -0.12727472538602325, 0.2304021103385215, -0.13075284075718005... |
707.278 | On the ergodic sum-rate performance of CDD in multi-user systems | The main focus of space-time coding design and analysis for MIMO systems has
been so far focused on single-user systems. For single-user systems, transmit
diversity schemes suffer a loss in spectral efficiency if the receiver is
equipped with more than one antenna, making them unsuitable for high rate
transmission. O... | cs.IT math.IT | the main focus of spacetime coding design and analysis for mimo systems has been so far focused on singleuser systems for singleuser systems transmit diversity schemes suffer a loss in spectral efficiency if the receiver is equipped with more than one antenna making them unsuitable for high rate transmission one such t... | [['the', 'main', 'focus', 'of', 'spacetime', 'coding', 'design', 'and', 'analysis', 'for', 'mimo', 'systems', 'has', 'been', 'so', 'far', 'focused', 'on', 'singleuser', 'systems', 'for', 'singleuser', 'systems', 'transmit', 'diversity', 'schemes', 'suffer', 'a', 'loss', 'in', 'spectral', 'efficiency', 'if', 'the', 'rec... | [-0.27090128267293917, 0.00968275985240445, -0.008375505384589945, 0.05376428101342274, -0.042302060451430194, -0.2859948551727479, 0.09581903694197536, 0.4071113894806131, -0.23907249794049945, -0.22115118917241527, 0.11134565753125392, -0.2365698109423757, -0.18406028324830254, 0.19241399125702638, -0.113802688690267... |
707.2781 | Set partition statistics and q-Fibonacci numbers | We consider the set partition statistics ls and rb introduced by Wachs and
White and investigate their distribution over set partitions avoiding certain
patterns. In particular, we consider those set partitions avoiding the pattern
13/2, $\Pi_n(13/2)$, and those avoiding both 13/2 and 123, $\Pi_n(13/2,123)$.
We show ... | math.CO | we consider the set partition statistics ls and rb introduced by wachs and white and investigate their distribution over set partitions avoiding certain patterns in particular we consider those set partitions avoiding the pattern 132 pi_n132 and those avoiding both 132 and 123 pi_n132123 we show that the distribution o... | [['we', 'consider', 'the', 'set', 'partition', 'statistics', 'ls', 'and', 'rb', 'introduced', 'by', 'wachs', 'and', 'white', 'and', 'investigate', 'their', 'distribution', 'over', 'set', 'partitions', 'avoiding', 'certain', 'patterns', 'in', 'particular', 'we', 'consider', 'those', 'set', 'partitions', 'avoiding', 'the... | [-0.1836761523986102, 0.1632727472577244, -0.046772030546812206, 0.13108322713524104, -0.07421759663238411, -0.10425365143233821, 0.08184805371399437, 0.2991707010815541, -0.3062198955565691, -0.33659905393918355, 0.06385794226856281, -0.3018517015767949, -0.17240317965902033, 0.1996451826677436, -0.11201032897945316, ... |
707.2782 | Mass-Selection and the Evolution of the Morphology-Density Relation from
z=0.8 to z=0 | We examined the morphology-density relations for galaxy samples selected by
luminosity and by mass in each of five massive X-ray clusters from z=0.023 to
0.83 for 674 spectroscopically-confirmed members. Rest-frame optical colors and
visual morphologies were obtained primarily from Hubble Space Telescope images.
Morp... | astro-ph | we examined the morphologydensity relations for galaxy samples selected by luminosity and by mass in each of five massive xray clusters from z0023 to 083 for 674 spectroscopicallyconfirmed members restframe optical colors and visual morphologies were obtained primarily from hubble space telescope images morphologydensi... | [['we', 'examined', 'the', 'morphologydensity', 'relations', 'for', 'galaxy', 'samples', 'selected', 'by', 'luminosity', 'and', 'by', 'mass', 'in', 'each', 'of', 'five', 'massive', 'xray', 'clusters', 'from', 'z0023', 'to', '083', 'for', '674', 'spectroscopicallyconfirmed', 'members', 'restframe', 'optical', 'colors', ... | [-0.019376142417058873, 0.1110435917007635, -0.04876960032925126, 0.1205145319240728, -0.057886612112270086, -0.0028429516132746357, 0.08528804669708734, 0.4439153436833294, -0.025132077028388267, -0.418533400727938, -0.015189929738426144, -0.35704370591338375, 0.03436715234511212, 0.19502181717416534, -0.0276994572413... |
707.2783 | On the Origin of Cosmic Magnetic Fields | We review the literature concerning how the cosmic magnetic fields pervading
nearly all galaxies actually got started. some observational evidence involves
the chemical abundance of the light elements Be and B, while another one is
based on strong magnetic fields seen in high red shift galaxies. Seed fields,
whose st... | astro-ph | we review the literature concerning how the cosmic magnetic fields pervading nearly all galaxies actually got started some observational evidence involves the chemical abundance of the light elements be and b while another one is based on strong magnetic fields seen in high red shift galaxies seed fields whose strength... | [['we', 'review', 'the', 'literature', 'concerning', 'how', 'the', 'cosmic', 'magnetic', 'fields', 'pervading', 'nearly', 'all', 'galaxies', 'actually', 'got', 'started', 'some', 'observational', 'evidence', 'involves', 'the', 'chemical', 'abundance', 'of', 'the', 'light', 'elements', 'be', 'and', 'b', 'while', 'anothe... | [-0.1252043699557697, 0.19233009983834468, -0.04124511178509381, 0.09408407042486176, -0.11882814067786585, -0.03678427241424, 0.020601388172699922, 0.3824476998446411, -0.24477836504382522, -0.3359055441167009, 0.05113887208158543, -0.23591452348046005, -0.08908002415869544, 0.1942298596312819, -0.02753791167082167, -... |
707.2784 | A Note on the Pfaffian Integration Theorem | Two alternative, fairly compact proofs are presented of the Pfaffian
integration theorem that is surfaced in the recent studies of spectral
properties of Ginibre's Orthogonal Ensemble. The first proof is based on a
concept of the Fredholm Pfaffian; the second proof is purely linear-algebraic.
| math-ph cond-mat.dis-nn hep-th math.MP math.PR nlin.SI | two alternative fairly compact proofs are presented of the pfaffian integration theorem that is surfaced in the recent studies of spectral properties of ginibres orthogonal ensemble the first proof is based on a concept of the fredholm pfaffian the second proof is purely linearalgebraic | [['two', 'alternative', 'fairly', 'compact', 'proofs', 'are', 'presented', 'of', 'the', 'pfaffian', 'integration', 'theorem', 'that', 'is', 'surfaced', 'in', 'the', 'recent', 'studies', 'of', 'spectral', 'properties', 'of', 'ginibres', 'orthogonal', 'ensemble', 'the', 'first', 'proof', 'is', 'based', 'on', 'a', 'concep... | [-0.1658696548798947, 0.02166950749233365, -0.1884976253760132, 0.08154194516034542, -0.1407788676125082, -0.0956266947958449, -0.016160323697311633, 0.31704663432372565, -0.17924398827281865, -0.2183487436480143, 0.1395306239957625, -0.20155169048600577, -0.18379574827849865, 0.24439522700214927, -0.07820197789591145,... |
707.2785 | Multifloquet to single electronic channel transition in the transport
properties of a resistive 1D driven disordered ring | We investigate the dc response of a 1D disordered ring coupled to a reservoir
and driven by a magnetic flux with a linear dependence on time. We identify two
regimes: (i) A localized or large length L regime, characterized by a dc
conductance, g_{dc}, whose probability distribution P(g_{dc}) is identical to
the one e... | cond-mat.mes-hall | we investigate the dc response of a 1d disordered ring coupled to a reservoir and driven by a magnetic flux with a linear dependence on time we identify two regimes i a localized or large length l regime characterized by a dc conductance g_dc whose probability distribution pg_dc is identical to the one exhibited by a 1... | [['we', 'investigate', 'the', 'dc', 'response', 'of', 'a', '1d', 'disordered', 'ring', 'coupled', 'to', 'a', 'reservoir', 'and', 'driven', 'by', 'a', 'magnetic', 'flux', 'with', 'a', 'linear', 'dependence', 'on', 'time', 'we', 'identify', 'two', 'regimes', 'i', 'a', 'localized', 'or', 'large', 'length', 'l', 'regime', ... | [-0.24232906360179185, 0.1958306985362433, -0.02270846636593342, -0.008047758961096406, 0.01221760021150112, -0.22177725060284137, 0.06150709518883377, 0.33513435468822717, -0.30392142206430434, -0.25033095468580724, 0.04377100684307516, -0.27490310110151767, -0.08492189811356365, 0.17030868597887455, 0.036754415690898... |
707.2786 | Twisting gauged non-linear sigma-models | We consider gauged sigma-models from a Riemann surface into a Kaehler and
hamiltonian G-manifold X. The supersymmetric N=2 theory can always be twisted
to produce a gauged A-model. This model localizes to the moduli space of
solutions of the vortex equations and computes the Hamiltonian Gromov-Witten
invariants. When... | hep-th math.DG | we consider gauged sigmamodels from a riemann surface into a kaehler and hamiltonian gmanifold x the supersymmetric n2 theory can always be twisted to produce a gauged amodel this model localizes to the moduli space of solutions of the vortex equations and computes the hamiltonian gromovwitten invariants when the targe... | [['we', 'consider', 'gauged', 'sigmamodels', 'from', 'a', 'riemann', 'surface', 'into', 'a', 'kaehler', 'and', 'hamiltonian', 'gmanifold', 'x', 'the', 'supersymmetric', 'n2', 'theory', 'can', 'always', 'be', 'twisted', 'to', 'produce', 'a', 'gauged', 'amodel', 'this', 'model', 'localizes', 'to', 'the', 'moduli', 'space... | [-0.19137388560920954, 0.1184283763053827, -0.09467865764163434, 0.1194545043152175, -0.11647730972617865, -0.23491340467589908, -0.0656783045764314, 0.27755223102867604, -0.2787200095131993, -0.2096241870895028, 0.05108066479151603, -0.2713108441210352, -0.21095699380675798, 0.09637179304263555, -0.1703858948065317, 0... |
707.2787 | The Evolution of the Field and Cluster Morphology-Density Relation for
Mass-Selected Samples of Galaxies | The Sloan Digital Sky Survey (SDSS) and photometric/spectroscopic surveys in
the GOODS-South field (the Chandra Deep Field-South, CDFS) are used to
construct volume-limited, stellar mass-selected samples of galaxies at
redshifts 0<z<1. The CDFS sample at 0.6<z<1.0 contains 207 galaxies complete
down to M=4x10^10 Msol... | astro-ph | the sloan digital sky survey sdss and photometricspectroscopic surveys in the goodssouth field the chandra deep fieldsouth cdfs are used to construct volumelimited stellar massselected samples of galaxies at redshifts 0z1 the cdfs sample at 06z10 contains 207 galaxies complete down to m4x1010 msol for a diet salpeter i... | [['the', 'sloan', 'digital', 'sky', 'survey', 'sdss', 'and', 'photometricspectroscopic', 'surveys', 'in', 'the', 'goodssouth', 'field', 'the', 'chandra', 'deep', 'fieldsouth', 'cdfs', 'are', 'used', 'to', 'construct', 'volumelimited', 'stellar', 'massselected', 'samples', 'of', 'galaxies', 'at', 'redshifts', '0z1', 'th... | [-0.0131167136317278, 0.07606134372078331, -0.09074525888327782, 0.10255483661662802, -0.09193049025403835, -0.02393013534961435, 0.05562044719349578, 0.4734665848223901, -0.057204927189078755, -0.3707880861602905, 0.031177804780730265, -0.3438177773108085, 0.010113306331251392, 0.19570397347972796, -0.0465910190700295... |
707.2788 | Evolutionary Fitting Methods for the Extraction of Mass Spectra in
Lattice Field Theory | We present an application of evolutionary algorithms to the curve-fitting
problems commonly encountered when trying to extract particle masses from
correlators in Lattice QCD. Harnessing the flexibility of evolutionary methods
in global optimization allows us to dynamically adapt the number of states to
be fitted alo... | hep-lat physics.comp-ph | we present an application of evolutionary algorithms to the curvefitting problems commonly encountered when trying to extract particle masses from correlators in lattice qcd harnessing the flexibility of evolutionary methods in global optimization allows us to dynamically adapt the number of states to be fitted along w... | [['we', 'present', 'an', 'application', 'of', 'evolutionary', 'algorithms', 'to', 'the', 'curvefitting', 'problems', 'commonly', 'encountered', 'when', 'trying', 'to', 'extract', 'particle', 'masses', 'from', 'correlators', 'in', 'lattice', 'qcd', 'harnessing', 'the', 'flexibility', 'of', 'evolutionary', 'methods', 'in... | [-0.005798508253480707, 0.0858799672371658, -0.1332509441833411, 0.09701023128665319, -0.09408390818695937, -0.10951441233046352, 0.05469377922625946, 0.39098505675792694, -0.29701938210720463, -0.37722976497773614, 0.0443846263157736, -0.25295628625587724, -0.08870977167971432, 0.1711172425670416, -0.04577924864632743... |
707.2789 | Nonthermal steady states after an interaction quench in the
Falicov-Kimball model | We present the exact solution of the Falicov-Kimball model after a sudden
change of its interaction parameter using non-equilibrium dynamical mean-field
theory. For different interaction quenches between the homogeneous metallic and
insulating phases the system relaxes to a non-thermal steady state on time
scales on ... | cond-mat.str-el cond-mat.stat-mech | we present the exact solution of the falicovkimball model after a sudden change of its interaction parameter using nonequilibrium dynamical meanfield theory for different interaction quenches between the homogeneous metallic and insulating phases the system relaxes to a nonthermal steady state on time scales on the ord... | [['we', 'present', 'the', 'exact', 'solution', 'of', 'the', 'falicovkimball', 'model', 'after', 'a', 'sudden', 'change', 'of', 'its', 'interaction', 'parameter', 'using', 'nonequilibrium', 'dynamical', 'meanfield', 'theory', 'for', 'different', 'interaction', 'quenches', 'between', 'the', 'homogeneous', 'metallic', 'an... | [-0.1444269119094208, 0.19180719041255276, -0.1353284895639209, 0.06602863387807327, 0.029100290666717817, -0.12234541804064065, 0.07488607845460886, 0.32306127002024476, -0.2659913732122411, -0.2734824385713128, 0.07873415546491742, -0.2455977590645061, -0.10101047823315158, 0.12610896238851743, 0.06117894400787704, 0... |
707.279 | The Evolving Faint-End of the Luminosity Function | We investigate the evolution of the faint-end slope of the luminosity
function, $\alpha$, using semi-analytical modeling of galaxy formation. In
agreement with observations, we find that the slope can be fitted well by
$\alpha (z) =a+b z$, with a=-1.13 and b=-0.1. The main driver for the evolution
in $\alpha$ is the ... | astro-ph | we investigate the evolution of the faintend slope of the luminosity function alpha using semianalytical modeling of galaxy formation in agreement with observations we find that the slope can be fitted well by alpha z ab z with a113 and b01 the main driver for the evolution in alpha is the evolution in the underlying d... | [['we', 'investigate', 'the', 'evolution', 'of', 'the', 'faintend', 'slope', 'of', 'the', 'luminosity', 'function', 'alpha', 'using', 'semianalytical', 'modeling', 'of', 'galaxy', 'formation', 'in', 'agreement', 'with', 'observations', 'we', 'find', 'that', 'the', 'slope', 'can', 'be', 'fitted', 'well', 'by', 'alpha', ... | [-0.07274744793339151, 0.13402176162244045, -0.1019767415127717, 0.12167535498106033, -0.05751307205606156, -0.05630425682516191, -0.005719787320764414, 0.41938823988211565, -0.15332239530659442, -0.3604816451404296, -0.02201213417795551, -0.2719809954969919, -0.04217993839772354, 0.16597672632608387, 0.007517881884143... |
707.2791 | Shadow vacuum alignment and dark energy | In a recent model of dark energy (with several phenomenological
consequences), the universe is assumed to be trapped in a false vacuum with an
energy density of the order of (10^{-3} eV)^4, mimicking the presently
successful $\Lambda CDM$ scenario. This involves a new gauge group SU(2)_Z,
{\em the shadow sector}, whi... | hep-ph astro-ph | in a recent model of dark energy with several phenomenological consequences the universe is assumed to be trapped in a false vacuum with an energy density of the order of 103 ev4 mimicking the presently successful lambda cdm scenario this involves a new gauge group su2_z em the shadow sector which becomes strong at a s... | [['in', 'a', 'recent', 'model', 'of', 'dark', 'energy', 'with', 'several', 'phenomenological', 'consequences', 'the', 'universe', 'is', 'assumed', 'to', 'be', 'trapped', 'in', 'a', 'false', 'vacuum', 'with', 'an', 'energy', 'density', 'of', 'the', 'order', 'of', '103', 'ev4', 'mimicking', 'the', 'presently', 'successfu... | [-0.18482294775227584, 0.22190503867102784, -0.0641163043144, 0.10015998443974773, -0.06510800544297458, -0.1281184144878885, 0.02392036589245857, 0.2750105253965935, -0.22894346622591158, -0.2932095421739377, 0.06736693277823023, -0.23948400403747744, -0.07233096099538137, 0.08337163904727232, -0.0005054297287687204, ... |
707.2792 | Distributed Compression and Multiparty Squashed Entanglement | We study a protocol in which many parties use quantum communication to
transfer a shared state to a receiver without communicating with each other.
This protocol is a multiparty version of the fully quantum Slepian-Wolf
protocol for two senders and arises through the repeated application of the
two-sender protocol. W... | quant-ph cs.IT math.IT | we study a protocol in which many parties use quantum communication to transfer a shared state to a receiver without communicating with each other this protocol is a multiparty version of the fully quantum slepianwolf protocol for two senders and arises through the repeated application of the twosender protocol we desc... | [['we', 'study', 'a', 'protocol', 'in', 'which', 'many', 'parties', 'use', 'quantum', 'communication', 'to', 'transfer', 'a', 'shared', 'state', 'to', 'a', 'receiver', 'without', 'communicating', 'with', 'each', 'other', 'this', 'protocol', 'is', 'a', 'multiparty', 'version', 'of', 'the', 'fully', 'quantum', 'slepianwo... | [-0.22760893152250597, 0.08147938786548861, -0.06227472472707169, 0.03491022682078836, 0.030336313378555996, -0.2403125097370592, 0.13693425003970205, 0.3445664504216167, -0.2919359128562766, -0.2584238420158886, 0.0956844333692029, -0.2371123404152234, -0.08932877554284539, 0.22552192484012298, -0.10480613039710493, 0... |
707.2793 | Detection of circumstellar material in a normal Type Ia Supernova | Type Ia supernovae are thought to be thermonuclear explosions of accreting
white dwarfs that reach a critical mass limit. Despite their importance as
cosmological distance indicators, the nature of their progenitors has remained
controversial. Here we report the detection of circumstellar material in a
normal Type Ia... | astro-ph | type ia supernovae are thought to be thermonuclear explosions of accreting white dwarfs that reach a critical mass limit despite their importance as cosmological distance indicators the nature of their progenitors has remained controversial here we report the detection of circumstellar material in a normal type ia supe... | [['type', 'ia', 'supernovae', 'are', 'thought', 'to', 'be', 'thermonuclear', 'explosions', 'of', 'accreting', 'white', 'dwarfs', 'that', 'reach', 'a', 'critical', 'mass', 'limit', 'despite', 'their', 'importance', 'as', 'cosmological', 'distance', 'indicators', 'the', 'nature', 'of', 'their', 'progenitors', 'has', 'rem... | [-0.09711613143794239, 0.14276022461242974, -0.08440279555972666, 0.07842872362583876, -0.1780954860773636, -0.07555315655190498, 0.10431897986680269, 0.370984699241817, -0.1814892605924979, -0.266423334274441, 0.08052001277217641, -0.28416664239019157, -0.036594612547196446, 0.1846951160673052, -0.08217370956444939, -... |
707.2794 | Nonadiabatic charged spherical gravitational collapse | We present a complete set of the equations and matching conditions required
for the description of physically meaningful charged, dissipative, spherically
symmetric gravitational collapse with shear. Dissipation is described with both
free-streaming and diffusion approximations. The effects of viscosity are also
take... | gr-qc astro-ph | we present a complete set of the equations and matching conditions required for the description of physically meaningful charged dissipative spherically symmetric gravitational collapse with shear dissipation is described with both freestreaming and diffusion approximations the effects of viscosity are also taken into ... | [['we', 'present', 'a', 'complete', 'set', 'of', 'the', 'equations', 'and', 'matching', 'conditions', 'required', 'for', 'the', 'description', 'of', 'physically', 'meaningful', 'charged', 'dissipative', 'spherically', 'symmetric', 'gravitational', 'collapse', 'with', 'shear', 'dissipation', 'is', 'described', 'with', '... | [-0.16604239614241742, 0.15985489336341835, -0.08317897686113913, 0.05782023806081059, -0.045525822796069246, -0.04990834909815179, -0.04282143823313189, 0.2582088053104994, -0.2557625303659048, -0.2957532899690441, 0.038438102698621704, -0.2656362725867201, -0.08979084454746782, 0.1372631549484272, 0.01975925569759978... |
707.2795 | Neutron-skin thickness of finite nuclei in relativistic mean-field
models with chiral limits | We study several structure properties of finite nuclei using relativistic
mean-field Lagrangians constructed according to the Brown-Rho scaling due to
the chiral symmetry restoration at high densities. The models are consistent
with current experimental constraints for the equations of state of symmetric
matter at bo... | nucl-th | we study several structure properties of finite nuclei using relativistic meanfield lagrangians constructed according to the brownrho scaling due to the chiral symmetry restoration at high densities the models are consistent with current experimental constraints for the equations of state of symmetric matter at both no... | [['we', 'study', 'several', 'structure', 'properties', 'of', 'finite', 'nuclei', 'using', 'relativistic', 'meanfield', 'lagrangians', 'constructed', 'according', 'to', 'the', 'brownrho', 'scaling', 'due', 'to', 'the', 'chiral', 'symmetry', 'restoration', 'at', 'high', 'densities', 'the', 'models', 'are', 'consistent', ... | [-0.05494781275004502, 0.2142660992532751, -0.11191190399202335, 0.09642709294770824, -0.029006170639156423, -0.10851418501255612, 0.022676446339129096, 0.34411275968716964, -0.20972310180646658, -0.3120913973832707, 0.015512322841711805, -0.30328840683520275, -0.024791562935697717, 0.09312313951952994, 0.0369590230857... |
707.2796 | Random perturbations of stochastic chains with unbounded variable length
memory | We consider binary infinite order stochastic chains perturbed by a random
noise. This means that at each time step, the value assumed by the chain can be
randomly and independently flipped with a small fixed probability. We show that
the transition probabilities of the perturbed chain are uniformly close to the
corre... | math.PR | we consider binary infinite order stochastic chains perturbed by a random noise this means that at each time step the value assumed by the chain can be randomly and independently flipped with a small fixed probability we show that the transition probabilities of the perturbed chain are uniformly close to the correspond... | [['we', 'consider', 'binary', 'infinite', 'order', 'stochastic', 'chains', 'perturbed', 'by', 'a', 'random', 'noise', 'this', 'means', 'that', 'at', 'each', 'time', 'step', 'the', 'value', 'assumed', 'by', 'the', 'chain', 'can', 'be', 'randomly', 'and', 'independently', 'flipped', 'with', 'a', 'small', 'fixed', 'probab... | [-0.118527330259981, 0.1910474771755703, -0.025446862634271383, 0.06979968477417493, -0.028130787449134956, -0.1561028220380346, 0.0803710642980323, 0.3768070543096179, -0.323728165757798, -0.24116500260397083, 0.15555989246349783, -0.256172587243574, -0.1280354412693885, 0.11902179153015216, -0.04100061816473802, 0.05... |
707.2797 | Outer boundary conditions for Einstein's field equations in harmonic
coordinates | We analyze Einstein's vacuum field equations in generalized harmonic
coordinates on a compact spatial domain with boundaries. We specify a class of
boundary conditions which is constraint-preserving and sufficiently general to
include recent proposals for reducing the amount of spurious reflections of
gravitational r... | gr-qc | we analyze einsteins vacuum field equations in generalized harmonic coordinates on a compact spatial domain with boundaries we specify a class of boundary conditions which is constraintpreserving and sufficiently general to include recent proposals for reducing the amount of spurious reflections of gravitational radiat... | [['we', 'analyze', 'einsteins', 'vacuum', 'field', 'equations', 'in', 'generalized', 'harmonic', 'coordinates', 'on', 'a', 'compact', 'spatial', 'domain', 'with', 'boundaries', 'we', 'specify', 'a', 'class', 'of', 'boundary', 'conditions', 'which', 'is', 'constraintpreserving', 'and', 'sufficiently', 'general', 'to', '... | [-0.12826357467565686, 0.05439221716677331, -0.06799930815871519, 0.05008668334668096, -0.10336135625869083, -0.09995832937196471, 0.0012339665845502168, 0.3053111273747606, -0.23216908144501922, -0.28550376190254706, 0.16024944142853387, -0.2312724589764212, -0.15865266030558792, 0.1753600898254006, -0.105459020616343... |
707.2798 | Study of B0 -> pi0 pi0, B -> pi pi0, and B -> K pi0 Decays, and Isospin
Analysis of B -> pipi Decays | We present updated measurements of the branching fractions and CP asymmetries
for B0 -> pi0 pi0, B+ -> pi+ pi0, and B+ -> K+ pi0. Based on a sample of 383 x
10^6 Upsilon(4S) -> B Bbar decays collected by the BABAR detector at the PEP-II
asymmetric-energy B factory at SLAC, we measure B(B0 -> pi0 pi0) =(1.47 +/-
0.25 ... | hep-ex | we present updated measurements of the branching fractions and cp asymmetries for b0 pi0 pi0 b pi pi0 and b k pi0 based on a sample of 383 x 106 upsilon4s b bbar decays collected by the babar detector at the pepii asymmetricenergy b factory at slac we measure bb0 pi0 pi0 147 025 012 x 106 bb pi pi0 502 046 029 x 106 an... | [['we', 'present', 'updated', 'measurements', 'of', 'the', 'branching', 'fractions', 'and', 'cp', 'asymmetries', 'for', 'b0', 'pi0', 'pi0', 'b', 'pi', 'pi0', 'and', 'b', 'k', 'pi0', 'based', 'on', 'a', 'sample', 'of', '383', 'x', '106', 'upsilon4s', 'b', 'bbar', 'decays', 'collected', 'by', 'the', 'babar', 'detector', ... | [-0.15373895581317717, 0.2833186857506772, -0.06301871530937954, 0.027881242391418353, -0.01963450757038092, -0.16217292259908586, 0.27698086582616005, 0.25517648043302454, -0.110143292677876, -0.2275835982758865, -0.15445904694845744, -0.5935536942697156, 0.19016588917959518, 0.10680867112067606, 0.1382289181839322, 0... |
707.2799 | High resolution X-ray scattering studies of structural phase transitions
in underdoped La$_{2-x}$Ba$_x$CuO$_4$ | We have studied structural phase transitions in high quality underdoped
La$_{2-x}$Ba$_x$CuO$_4$ single crystals using high resolution x-ray scattering
techniques. Critical properties associated with the continuous High Temperature
Tetragonal (HTT, $I4/mmm$) to Middle Temperature Orthorhombic (MTO, $Cmca$)
phase trans... | cond-mat.supr-con | we have studied structural phase transitions in high quality underdoped la_2xba_xcuo_4 single crystals using high resolution xray scattering techniques critical properties associated with the continuous high temperature tetragonal htt i4mmm to middle temperature orthorhombic mto cmca phase transition were investigated ... | [['we', 'have', 'studied', 'structural', 'phase', 'transitions', 'in', 'high', 'quality', 'underdoped', 'la_2xba_xcuo_4', 'single', 'crystals', 'using', 'high', 'resolution', 'xray', 'scattering', 'techniques', 'critical', 'properties', 'associated', 'with', 'the', 'continuous', 'high', 'temperature', 'tetragonal', 'ht... | [-0.15408341457391633, 0.2833122495047813, -0.02960758714927543, -0.042767911418980245, -0.03787286882060489, -0.13964879270597344, 0.13352550057535673, 0.4593647475829165, -0.22814110053221548, -0.25577473292108993, 0.056004293765712934, -0.3339095431923245, -0.12076374503964211, 0.14319758765130103, 0.026641270378604... |
707.28 | Dielectric spectroscopy in benzophenone: The beta relaxation and its
relation to the mode-coupling Cole-Cole peak | We report a thorough characterization of the glassy dynamics of benzophenone
by broadband dielectric spectroscopy. We detect a well pronounced beta
relaxation peak developing into an excess wing with increasing temperature. A
previous analysis of results from Optical-Kerr-effect measurements on this
material within t... | cond-mat.dis-nn cond-mat.soft | we report a thorough characterization of the glassy dynamics of benzophenone by broadband dielectric spectroscopy we detect a well pronounced beta relaxation peak developing into an excess wing with increasing temperature a previous analysis of results from opticalkerreffect measurements on this material within the mod... | [['we', 'report', 'a', 'thorough', 'characterization', 'of', 'the', 'glassy', 'dynamics', 'of', 'benzophenone', 'by', 'broadband', 'dielectric', 'spectroscopy', 'we', 'detect', 'a', 'well', 'pronounced', 'beta', 'relaxation', 'peak', 'developing', 'into', 'an', 'excess', 'wing', 'with', 'increasing', 'temperature', 'a'... | [-0.06517204944771947, 0.1309991556314344, -0.1262038129195571, 0.030859393540304154, -0.08623319184407592, -0.13219742172863336, 0.066523533212021, 0.41078192692250015, -0.27317404258530587, -0.296449294812046, 0.06333919203723781, -0.29202921958640216, -0.1980447492096573, 0.16494676487520338, -0.026643027582904325, ... |
707.2801 | Testing Chameleon Theories with Light Propagating through a Magnetic
Field | It was recently argued that the observed PVLAS anomaly can be explained by
chameleon field theories in which large deviations from Newton's law can be
avoided. Here we present the predictions for the dichroism and the
birefringence induced in the vacuum by a magnetic field in these models. We
show that chameleon part... | hep-ph astro-ph gr-qc hep-th | it was recently argued that the observed pvlas anomaly can be explained by chameleon field theories in which large deviations from newtons law can be avoided here we present the predictions for the dichroism and the birefringence induced in the vacuum by a magnetic field in these models we show that chameleon particles... | [['it', 'was', 'recently', 'argued', 'that', 'the', 'observed', 'pvlas', 'anomaly', 'can', 'be', 'explained', 'by', 'chameleon', 'field', 'theories', 'in', 'which', 'large', 'deviations', 'from', 'newtons', 'law', 'can', 'be', 'avoided', 'here', 'we', 'present', 'the', 'predictions', 'for', 'the', 'dichroism', 'and', '... | [-0.09319068225291134, 0.28815115680812264, -0.10407821680895392, 0.1275887459222841, -0.0873503004920415, -0.1398337929911742, -0.041439315761884, 0.3679994192313064, -0.2163993251742795, -0.36646978646008804, 0.002947176923044026, -0.2541765462056818, -0.1630541100960479, 0.2018969140692868, 0.001082026370568201, 0.0... |
707.2802 | Determination of the mass of the neutron star in SMC X-1, LMC X-4 and
Cen X-3 with VLT/UVES | We present the results of a spectroscopic monitoring campaign of the OB-star
companions to the eclipsing X-ray pulsars SMC X-1, LMC X-4 and Cen X-3.
High-resolution optical spectra obtained with UVES on the ESO Very Large
Telescope are used to determine the radial-velocity orbit of the OB
(super)giants with high prec... | astro-ph | we present the results of a spectroscopic monitoring campaign of the obstar companions to the eclipsing xray pulsars smc x1 lmc x4 and cen x3 highresolution optical spectra obtained with uves on the eso very large telescope are used to determine the radialvelocity orbit of the ob supergiants with high precision the exc... | [['we', 'present', 'the', 'results', 'of', 'a', 'spectroscopic', 'monitoring', 'campaign', 'of', 'the', 'obstar', 'companions', 'to', 'the', 'eclipsing', 'xray', 'pulsars', 'smc', 'x1', 'lmc', 'x4', 'and', 'cen', 'x3', 'highresolution', 'optical', 'spectra', 'obtained', 'with', 'uves', 'on', 'the', 'eso', 'very', 'larg... | [-0.09990673212916157, 0.06401365942262861, -0.08317458002177175, 0.10360460757532375, -0.12375258973567681, -0.08059014395384817, 0.1365421563655235, 0.42045522483193826, -0.17118870047419626, -0.352900893562456, 0.07380212273069599, -0.3194886505029071, -0.00685133670238591, 0.2547640437982997, -0.060744375080479564,... |
707.2803 | Deformed strings in the Heisenberg model | We investigate solutions to the Bethe equations for the isotropic S = 1/2
Heisenberg chain involving complex, string-like rapidity configurations of
arbitrary length. Going beyond the traditional string hypothesis of undeformed
strings, we describe a general procedure to construct eigenstates including
strings with g... | cond-mat.str-el cond-mat.stat-mech hep-th | we investigate solutions to the bethe equations for the isotropic s 12 heisenberg chain involving complex stringlike rapidity configurations of arbitrary length going beyond the traditional string hypothesis of undeformed strings we describe a general procedure to construct eigenstates including strings with generic de... | [['we', 'investigate', 'solutions', 'to', 'the', 'bethe', 'equations', 'for', 'the', 'isotropic', 's', '12', 'heisenberg', 'chain', 'involving', 'complex', 'stringlike', 'rapidity', 'configurations', 'of', 'arbitrary', 'length', 'going', 'beyond', 'the', 'traditional', 'string', 'hypothesis', 'of', 'undeformed', 'strin... | [-0.1759655264444476, 0.13523222667403345, -0.03576679654192006, 0.1690613390650427, -0.06355034509608738, -0.16043244525357042, 0.010895671542235759, 0.3365853786750069, -0.24247352542290682, -0.20805771869802198, 0.07952469813929827, -0.30470811646583296, -0.1286790319447687, 0.15350428476474834, 0.025558571057762346... |
707.2804 | Generalized kinetic equations for charge carriers in graphene | A system of generalized kinetic equations for the distribution functions of
two-dimensional Dirac fermions scattered by impurities is derived in the Born
approximation with respect to short-range impurity potential. It is proven that
the conductivity following from classical Boltzmann equation picture, where
electron... | cond-mat.mes-hall cond-mat.stat-mech | a system of generalized kinetic equations for the distribution functions of twodimensional dirac fermions scattered by impurities is derived in the born approximation with respect to shortrange impurity potential it is proven that the conductivity following from classical boltzmann equation picture where electrons or h... | [['a', 'system', 'of', 'generalized', 'kinetic', 'equations', 'for', 'the', 'distribution', 'functions', 'of', 'twodimensional', 'dirac', 'fermions', 'scattered', 'by', 'impurities', 'is', 'derived', 'in', 'the', 'born', 'approximation', 'with', 'respect', 'to', 'shortrange', 'impurity', 'potential', 'it', 'is', 'prove... | [-0.11319002032348323, 0.17139267179927545, -0.05993490901491562, 0.07988637949152072, -0.013017420362202672, -0.14466572068460765, 0.05065967149550839, 0.30724046276583244, -0.27595554258879446, -0.2528589724999887, -0.03058419424886687, -0.34951819413674806, -0.08971510017760645, 0.16252642665741915, 0.02415829198007... |
707.2805 | Piezomagnetic Quantum Dots | We study the influence of deformations on magnetic ordering in quantum dots
doped with magnetic impurities. The reduction of symmetry and the associated
deformation from circular to elliptical quantum confinement lead to the
formation of piezomagnetic quantum dots. The strength of elliptical deformation
can be contro... | cond-mat.mes-hall cond-mat.mtrl-sci | we study the influence of deformations on magnetic ordering in quantum dots doped with magnetic impurities the reduction of symmetry and the associated deformation from circular to elliptical quantum confinement lead to the formation of piezomagnetic quantum dots the strength of elliptical deformation can be controlled... | [['we', 'study', 'the', 'influence', 'of', 'deformations', 'on', 'magnetic', 'ordering', 'in', 'quantum', 'dots', 'doped', 'with', 'magnetic', 'impurities', 'the', 'reduction', 'of', 'symmetry', 'and', 'the', 'associated', 'deformation', 'from', 'circular', 'to', 'elliptical', 'quantum', 'confinement', 'lead', 'to', 't... | [-0.180332547693979, 0.22501107175291205, -0.02877428637293633, -0.01683543380931951, -0.025961526031702913, -0.11651586450170726, 0.01115692176487452, 0.4052491795349245, -0.2689544781848478, -0.3331466658273712, 0.013086864285772512, -0.26240982487797737, -0.13436676822796775, 0.19521557806486575, -0.0087490052780291... |
707.2806 | Aromatic Features in AGN: Star-Forming Infrared Luminosity Function of
AGN Host Galaxies | We describe observations of aromatic features at 7.7 and 11.3 um in AGN of
three types including PG, 2MASS and 3CR objects. The feature has been
demonstrated to originate predominantly from star formation. Based on the
aromatic-derived star forming luminosity, we find that the far-IR emission of
AGN can be dominated ... | astro-ph | we describe observations of aromatic features at 77 and 113 um in agn of three types including pg 2mass and 3cr objects the feature has been demonstrated to originate predominantly from star formation based on the aromaticderived star forming luminosity we find that the farir emission of agn can be dominated by either ... | [['we', 'describe', 'observations', 'of', 'aromatic', 'features', 'at', '77', 'and', '113', 'um', 'in', 'agn', 'of', 'three', 'types', 'including', 'pg', '2mass', 'and', '3cr', 'objects', 'the', 'feature', 'has', 'been', 'demonstrated', 'to', 'originate', 'predominantly', 'from', 'star', 'formation', 'based', 'on', 'th... | [0.02421651473253549, 0.10530172532889992, -0.06561351323647327, 0.13388624524630263, -0.08866867299596044, -0.034807265549285434, 0.0032099783052935414, 0.49630556762904715, -0.10260446195024997, -0.34945078789084955, 0.029155141096500876, -0.3401886626257022, 0.011651114503987819, 0.1655754054020355, 0.00885827329597... |
707.2807 | Experimental Realization of Polarization Qutrits from Non-Maximally
Entangled States | Based on a recent proposal [Phys. Rev. A 71, 062337 (2005)], we have
experimentally realized two photon polarization qutrits by using non-maximally
entangled states and linear optical transformations. By this technique high
fidelity mutually unbiased qutrits are generated at a high brilliance level.
| quant-ph | based on a recent proposal phys rev a 71 062337 2005 we have experimentally realized two photon polarization qutrits by using nonmaximally entangled states and linear optical transformations by this technique high fidelity mutually unbiased qutrits are generated at a high brilliance level | [['based', 'on', 'a', 'recent', 'proposal', 'phys', 'rev', 'a', '71', '062337', '2005', 'we', 'have', 'experimentally', 'realized', 'two', 'photon', 'polarization', 'qutrits', 'by', 'using', 'nonmaximally', 'entangled', 'states', 'and', 'linear', 'optical', 'transformations', 'by', 'this', 'technique', 'high', 'fidelit... | [-0.1012125535912457, 0.24504989312429512, 0.002554287989845588, -0.0779001192283994, 0.04807937593709323, -0.22939961088732594, 0.11289870763929295, 0.4569661129332547, -0.07925889889399211, -0.30754827424174264, 0.005410842142910475, -0.2945343231161435, -0.0778834164541747, 0.2548062102425666, -0.06820233354699753, ... |
707.2808 | Synchrotron flaring behaviour of CygnusX-3 during the February-March
1994 and September 2001 outbursts | Aims: In this paper we study whether the shock-in-jet model, widely used to
explain the outbursting behaviour of quasars, can be used to explain the radio
flaring behaviour of the microquasar Cygnus X-3.
Method: We have used a method developed to model the synchrotron outbursts of
quasar jets, which decomposes mult... | astro-ph | aims in this paper we study whether the shockinjet model widely used to explain the outbursting behaviour of quasars can be used to explain the radio flaring behaviour of the microquasar cygnus x3 method we have used a method developed to model the synchrotron outbursts of quasar jets which decomposes multifrequency li... | [['aims', 'in', 'this', 'paper', 'we', 'study', 'whether', 'the', 'shockinjet', 'model', 'widely', 'used', 'to', 'explain', 'the', 'outbursting', 'behaviour', 'of', 'quasars', 'can', 'be', 'used', 'to', 'explain', 'the', 'radio', 'flaring', 'behaviour', 'of', 'the', 'microquasar', 'cygnus', 'x3', 'method', 'we', 'have'... | [-0.04456655058256899, 0.11145307154995258, -0.12201171257385166, 0.12669913988902068, -0.10247582633692388, -0.10832694809117885, 0.0212977931548615, 0.44937364620409, -0.19966617605222442, -0.34252910239021694, 0.08200211673605073, -0.2504382212385187, -0.10063487197333407, 0.22203054206302197, -0.035624750305585144,... |
707.2809 | Multipartite positive-partial-transpose inequalities exponentially
stronger than local reality inequalities | We show that positivity of {\it every} partial transpose of $N$-partite
quantum states implies new inequalities on Bell correlations which are stronger
than standard Bell inequalities by a factor of $2^{(N-1)/2}$. A violation of
the inequality implies the system is in a bipartite distillable entangled
state. It turns... | quant-ph | we show that positivity of it every partial transpose of npartite quantum states implies new inequalities on bell correlations which are stronger than standard bell inequalities by a factor of 2n12 a violation of the inequality implies the system is in a bipartite distillable entangled state it turns out that a family ... | [['we', 'show', 'that', 'positivity', 'of', 'it', 'every', 'partial', 'transpose', 'of', 'npartite', 'quantum', 'states', 'implies', 'new', 'inequalities', 'on', 'bell', 'correlations', 'which', 'are', 'stronger', 'than', 'standard', 'bell', 'inequalities', 'by', 'a', 'factor', 'of', '2n12', 'a', 'violation', 'of', 'th... | [-0.17454160394606322, 0.17246571289732643, -0.0506183681499264, 0.010340166947172878, 0.024313286929199956, -0.2685977617112843, 0.09923481370628595, 0.22193088276592426, -0.13469348926227126, -0.28515505997387514, 0.00022432977199707537, -0.306931503404136, -0.12679401182965055, 0.18801984544014175, -0.08967742246052... |
707.281 | Determinant Bounds and the Matsubara UV Problem of Many-Fermion Systems | It is known that perturbation theory converges in fermionic field theory at
weak coupling if the interaction and the covariance are summable and if certain
determinants arising in the expansion can be bounded efficiently, e.g. if the
covariance admits a Gram representation with a finite Gram constant. The
covariances... | math-ph cond-mat.str-el math.MP | it is known that perturbation theory converges in fermionic field theory at weak coupling if the interaction and the covariance are summable and if certain determinants arising in the expansion can be bounded efficiently eg if the covariance admits a gram representation with a finite gram constant the covariances of th... | [['it', 'is', 'known', 'that', 'perturbation', 'theory', 'converges', 'in', 'fermionic', 'field', 'theory', 'at', 'weak', 'coupling', 'if', 'the', 'interaction', 'and', 'the', 'covariance', 'are', 'summable', 'and', 'if', 'certain', 'determinants', 'arising', 'in', 'the', 'expansion', 'can', 'be', 'bounded', 'efficient... | [-0.11944552869742434, 0.15086056413289545, -0.09987228226577266, 0.09048811095168016, -0.09062498998759415, -0.1203576124059908, 0.003941304426585218, 0.3574121796383793, -0.27351055888853637, -0.2417089987059899, 0.11219651968128924, -0.24013127480053487, -0.1283199521483569, 0.1653943546122087, -0.018139101067395063... |
707.2811 | Operational Quantification of Continuous Variable Correlations | We quantify correlations (quantum and/or classical) between two continuous
variable modes in terms of how many correlated bits can be extracted by
measuring the sign of two local quadratures. On Gaussian states, such `bit
quadrature correlations' majorize entanglement, reducing to an entanglement
monotone for pure st... | quant-ph | we quantify correlations quantum andor classical between two continuous variable modes in terms of how many correlated bits can be extracted by measuring the sign of two local quadratures on gaussian states such bit quadrature correlations majorize entanglement reducing to an entanglement monotone for pure states for n... | [['we', 'quantify', 'correlations', 'quantum', 'andor', 'classical', 'between', 'two', 'continuous', 'variable', 'modes', 'in', 'terms', 'of', 'how', 'many', 'correlated', 'bits', 'can', 'be', 'extracted', 'by', 'measuring', 'the', 'sign', 'of', 'two', 'local', 'quadratures', 'on', 'gaussian', 'states', 'such', 'bit', ... | [-0.11692893125545105, 0.22245988246908416, -0.10366094824558961, 0.10331866180325576, 0.044515994643373843, -0.18703732132450293, 0.054328278557252176, 0.3507885050387421, -0.2773835947541515, -0.24979888645231452, 0.04015664281985731, -0.29206318573154716, -0.09665250204879483, 0.18519466410502108, -0.031278515695978... |
707.2812 | The top squark-mediated annihilation scenario and direct detection of
dark matter in compressed supersymmetry | Top squark-mediated annihilation of bino-like neutralinos to top-antitop
pairs can play the dominant role in obtaining a thermal relic dark matter
abundance in agreement with observations. In a previous paper, it was argued
that this can occur naturally in models of compressed supersymmetry, which
feature a running g... | hep-ph | top squarkmediated annihilation of binolike neutralinos to topantitop pairs can play the dominant role in obtaining a thermal relic dark matter abundance in agreement with observations in a previous paper it was argued that this can occur naturally in models of compressed supersymmetry which feature a running gluino ma... | [['top', 'squarkmediated', 'annihilation', 'of', 'binolike', 'neutralinos', 'to', 'topantitop', 'pairs', 'can', 'play', 'the', 'dominant', 'role', 'in', 'obtaining', 'a', 'thermal', 'relic', 'dark', 'matter', 'abundance', 'in', 'agreement', 'with', 'observations', 'in', 'a', 'previous', 'paper', 'it', 'was', 'argued', ... | [-0.10341071038572174, 0.20683555836759268, -0.08959689473868498, 0.14580894907187264, -0.0929061621624691, -0.13651301446858974, -0.0034103643199834494, 0.338664980209057, -0.2062149806203501, -0.3761307089852409, 0.03410741794692923, -0.22300221321488461, -0.04636640202314142, 0.1796233234607855, 0.026337828549120815... |
707.2813 | Large time asymptotics of growth models on space-like paths I: PushASEP | We consider a new interacting particle system on the one-dimensional lattice
that interpolates between TASEP and Toom's model: A particle cannot jump to the
right if the neighboring site is occupied, and when jumping to the left it
simply pushes all the neighbors that block its way.
We prove that for flat and step ... | math-ph cond-mat.stat-mech math.MP math.PR | we consider a new interacting particle system on the onedimensional lattice that interpolates between tasep and tooms model a particle cannot jump to the right if the neighboring site is occupied and when jumping to the left it simply pushes all the neighbors that block its way we prove that for flat and step initial c... | [['we', 'consider', 'a', 'new', 'interacting', 'particle', 'system', 'on', 'the', 'onedimensional', 'lattice', 'that', 'interpolates', 'between', 'tasep', 'and', 'tooms', 'model', 'a', 'particle', 'can', 'not', 'jump', 'to', 'the', 'right', 'if', 'the', 'neighboring', 'site', 'is', 'occupied', 'and', 'when', 'jumping',... | [-0.1275998755783132, 0.20398664998921376, -0.06953853291902438, 0.060746809838393936, -0.01563860196394177, -0.17641483219702123, 0.041195986783403214, 0.35685657203034726, -0.30823803511764675, -0.21320434097648208, 0.08585113413559581, -0.2973739576087451, -0.08844448351391672, 0.14481389869085864, -0.00065731523034... |
707.2814 | Coverage Probability of Random Intervals | In this paper, we develop a general theory on the coverage probability of
random intervals defined in terms of discrete random variables with continuous
parameter spaces. The theory shows that the minimum coverage probabilities of
random intervals with respect to corresponding parameters are achieved at
discrete fini... | math.ST math.PR stat.ME stat.TH | in this paper we develop a general theory on the coverage probability of random intervals defined in terms of discrete random variables with continuous parameter spaces the theory shows that the minimum coverage probabilities of random intervals with respect to corresponding parameters are achieved at discrete finite s... | [['in', 'this', 'paper', 'we', 'develop', 'a', 'general', 'theory', 'on', 'the', 'coverage', 'probability', 'of', 'random', 'intervals', 'defined', 'in', 'terms', 'of', 'discrete', 'random', 'variables', 'with', 'continuous', 'parameter', 'spaces', 'the', 'theory', 'shows', 'that', 'the', 'minimum', 'coverage', 'probab... | [-0.06299009892771408, 0.16360058076103393, -0.07011937914821918, 0.11137455937309688, -0.07165300492012855, -0.16465359773615948, 0.120930991279616, 0.40799556042547197, -0.2804583592321908, -0.23959300748480594, 0.08985680276366632, -0.24497952024535377, -0.11136789726886419, 0.1696828182159674, -0.13015887031958687,... |
707.2815 | Very high energy observations of the BL Lac objects 3C 66A and OJ 287 | Using the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE), we
have observed the BL Lac objects 3C 66A and OJ 287. These are members of the
class of low-frequency-peaked BL Lac objects (LBLs) and are two of the three
LBLs predicted by Costamante and Ghisellini to be potential sources of very
high energy (... | astro-ph | using the solar tower atmospheric cherenkov effect experiment stacee we have observed the bl lac objects 3c 66a and oj 287 these are members of the class of lowfrequencypeaked bl lac objects lbls and are two of the three lbls predicted by costamante and ghisellini to be potential sources of very high energy 100 gev gam... | [['using', 'the', 'solar', 'tower', 'atmospheric', 'cherenkov', 'effect', 'experiment', 'stacee', 'we', 'have', 'observed', 'the', 'bl', 'lac', 'objects', '3c', '66a', 'and', 'oj', '287', 'these', 'are', 'members', 'of', 'the', 'class', 'of', 'lowfrequencypeaked', 'bl', 'lac', 'objects', 'lbls', 'and', 'are', 'two', 'o... | [-0.042526613276628454, 0.1904764004777525, -0.005631216605001226, 0.16348417076294247, -0.10450861452083135, -0.13388188892236813, 0.05614056384014287, 0.4590357186931089, -0.08390152184212388, -0.4916728305758844, 0.06584771513810446, -0.31564222658374186, 0.0454320642507057, 0.23058650571981382, -0.03880882241104826... |
707.2816 | Regularity of solutions to higher-order integrals of the calculus of
variations | We obtain new regularity conditions for problems of calculus of variations
with higher-order derivatives. As a corollary, we get non-occurrence of the
Lavrentiev phenomenon. Our main regularity result asserts that autonomous
integral functionals with a Lagrangian having coercive partial derivatives with
respect to th... | math.OC | we obtain new regularity conditions for problems of calculus of variations with higherorder derivatives as a corollary we get nonoccurrence of the lavrentiev phenomenon our main regularity result asserts that autonomous integral functionals with a lagrangian having coercive partial derivatives with respect to the highe... | [['we', 'obtain', 'new', 'regularity', 'conditions', 'for', 'problems', 'of', 'calculus', 'of', 'variations', 'with', 'higherorder', 'derivatives', 'as', 'a', 'corollary', 'we', 'get', 'nonoccurrence', 'of', 'the', 'lavrentiev', 'phenomenon', 'our', 'main', 'regularity', 'result', 'asserts', 'that', 'autonomous', 'inte... | [-0.14772252476651151, 0.010620535017465646, -0.10875310544978897, 0.08419288027117837, -0.17235963074226845, -0.08142302116765729, -0.044404818377686, 0.31866175273679337, -0.3081681323501299, -0.27157223786618384, 0.12938385191461388, -0.27243861447105994, -0.16120920049132043, 0.15321502381197685, -0.150053856753796... |
707.2817 | The kinetic energy operator in the subspaces of wavelet analysis | At any resolution level of wavelet expansions the physical observable of the
kinetic energy is represented by an infinite matrix which is ``canonically''
chosen as the projection of the operator $-\Delta/2$ onto the subspace of the
given resolution. It is shown, that this canonical choice is not optimal, as
the regul... | physics.chem-ph physics.comp-ph | at any resolution level of wavelet expansions the physical observable of the kinetic energy is represented by an infinite matrix which is canonically chosen as the projection of the operator delta2 onto the subspace of the given resolution it is shown that this canonical choice is not optimal as the regular grid of the... | [['at', 'any', 'resolution', 'level', 'of', 'wavelet', 'expansions', 'the', 'physical', 'observable', 'of', 'the', 'kinetic', 'energy', 'is', 'represented', 'by', 'an', 'infinite', 'matrix', 'which', 'is', 'canonically', 'chosen', 'as', 'the', 'projection', 'of', 'the', 'operator', 'delta2', 'onto', 'the', 'subspace', ... | [-0.11771300143411148, 0.1312118014201232, -0.09786129568854582, 0.07666125044763236, -0.07940768532837365, -0.08936347806554855, 0.0012211612578395088, 0.35674087482424366, -0.2760380939025407, -0.2691645869979055, 0.09802286733799176, -0.23655409532728672, -0.1461669709780161, 0.17254424017170963, -0.0433695248215588... |
707.2818 | Dispersion of Observed Position Angles of Submillimeter Polarization in
Molecular Clouds | One can estimate the characteristic magnetic field strength in GMCs by
comparing submillimeter polarimetric observations of these sources with
simulated polarization maps developed using a range of different values for the
assumed field strength. The point of comparison is the degree of order in the
distribution of p... | astro-ph | one can estimate the characteristic magnetic field strength in gmcs by comparing submillimeter polarimetric observations of these sources with simulated polarization maps developed using a range of different values for the assumed field strength the point of comparison is the degree of order in the distribution of pola... | [['one', 'can', 'estimate', 'the', 'characteristic', 'magnetic', 'field', 'strength', 'in', 'gmcs', 'by', 'comparing', 'submillimeter', 'polarimetric', 'observations', 'of', 'these', 'sources', 'with', 'simulated', 'polarization', 'maps', 'developed', 'using', 'a', 'range', 'of', 'different', 'values', 'for', 'the', 'a... | [-0.1102590284861412, 0.10129393971183623, -0.056214896847104914, 0.04612598187640852, -0.030175117522336637, -0.05411871912287949, 0.006308342406048758, 0.3851196186593439, -0.19918089425795463, -0.3654876729205274, 0.06396235343174939, -0.26715625095169376, -0.08810299972574745, 0.2061602336743587, 0.0180979430310050... |
707.2819 | Propagation equations for deformable test bodies with microstructure in
extended theories of gravity | We derive the equations of motion in metric-affine gravity by making use of
the conservation laws obtained from Noether's theorem. The results are given in
the form of propagation equations for the multipole decomposition of the matter
sources in metric-affine gravity, i.e., the canonical energy-momentum current
and ... | gr-qc astro-ph | we derive the equations of motion in metricaffine gravity by making use of the conservation laws obtained from noethers theorem the results are given in the form of propagation equations for the multipole decomposition of the matter sources in metricaffine gravity ie the canonical energymomentum current and the hypermo... | [['we', 'derive', 'the', 'equations', 'of', 'motion', 'in', 'metricaffine', 'gravity', 'by', 'making', 'use', 'of', 'the', 'conservation', 'laws', 'obtained', 'from', 'noethers', 'theorem', 'the', 'results', 'are', 'given', 'in', 'the', 'form', 'of', 'propagation', 'equations', 'for', 'the', 'multipole', 'decomposition... | [-0.16958633985572086, 0.14898123895263027, -0.11307027729548466, 0.06285429721813839, -0.13002973683415706, -0.09314964469640878, -0.06442605185242381, 0.2507768738036085, -0.22855264140785359, -0.3288397895658662, 0.02419247549949629, -0.23642615774412087, -0.12718955134961066, 0.14106835907912416, -0.022676943915534... |
707.282 | Rare decays of heavy flavor at the Tevatron | In this report I review recent results in the field of rare decays at the
Tevatron CDF II and D0 experiments. The presentation is focused on rare decays
of charm and bottom mesons with two muons in the final state. This includes
improvements over the previously available limits on the following branching
ratios: $B(D... | hep-ex | in this report i review recent results in the field of rare decays at the tevatron cdf ii and d0 experiments the presentation is focused on rare decays of charm and bottom mesons with two muons in the final state this includes improvements over the previously available limits on the following branching ratios bd to pi ... | [['in', 'this', 'report', 'i', 'review', 'recent', 'results', 'in', 'the', 'field', 'of', 'rare', 'decays', 'at', 'the', 'tevatron', 'cdf', 'ii', 'and', 'd0', 'experiments', 'the', 'presentation', 'is', 'focused', 'on', 'rare', 'decays', 'of', 'charm', 'and', 'bottom', 'mesons', 'with', 'two', 'muons', 'in', 'the', 'fi... | [-0.10734013683144204, 0.19925325353489184, -0.013942155538113427, 0.034098932220560346, 0.01322483373202866, -0.11780609913411544, 0.16305165159140828, 0.28460085188313355, -0.1543257283716858, -0.27695551787992173, -0.003663741594026361, -0.3702074900376711, 0.040369467568590486, 0.14154121348728166, 0.04461872732440... |
707.2821 | On the combined gravity gradient modeling for applied geophysics | Gravity gradiometry research and development has intensified in recent years
to the extent that technologies providing a resolution of about 1 Eotvos per 1
sec average shall likely soon be available for multiple critical applications
such as natural resources exploration, oil reservoir monitoring and defence
establis... | physics.geo-ph physics.ins-det | gravity gradiometry research and development has intensified in recent years to the extent that technologies providing a resolution of about 1 eotvos per 1 sec average shall likely soon be available for multiple critical applications such as natural resources exploration oil reservoir monitoring and defence establishme... | [['gravity', 'gradiometry', 'research', 'and', 'development', 'has', 'intensified', 'in', 'recent', 'years', 'to', 'the', 'extent', 'that', 'technologies', 'providing', 'a', 'resolution', 'of', 'about', '1', 'eotvos', 'per', '1', 'sec', 'average', 'shall', 'likely', 'soon', 'be', 'available', 'for', 'multiple', 'critic... | [-0.08736141495308772, 0.1138044561839838, -0.09208634977255935, 0.07273327728119287, -0.09087820528404099, -0.12164352688452472, -0.009671957139263226, 0.35854356165003515, -0.2637548948557157, -0.3651457841818531, 0.17684765727819363, -0.265039324288027, -0.1290123675312118, 0.22173335418051135, -0.11420425021197593,... |
707.2822 | Centralizers in the Hecke algebras of complex reflection groups | How far can the elementary description of centralizers of parabolic
subalgebras of Hecke algebras of finite real reflection groups be generalized
to the complex reflection group case? In this paper we begin to answer this
question by establishing results in two directions. First, under conditions
closely analogous to... | math.RT | how far can the elementary description of centralizers of parabolic subalgebras of hecke algebras of finite real reflection groups be generalized to the complex reflection group case in this paper we begin to answer this question by establishing results in two directions first under conditions closely analogous to thos... | [['how', 'far', 'can', 'the', 'elementary', 'description', 'of', 'centralizers', 'of', 'parabolic', 'subalgebras', 'of', 'hecke', 'algebras', 'of', 'finite', 'real', 'reflection', 'groups', 'be', 'generalized', 'to', 'the', 'complex', 'reflection', 'group', 'case', 'in', 'this', 'paper', 'we', 'begin', 'to', 'answer', ... | [-0.14791740758566937, 0.06846905566516086, -0.052608051838474036, 0.06874004320012156, -0.14664936606918197, -0.10696845551007497, -0.0004919700649455745, 0.36187491962797386, -0.33387933932453284, -0.2276207732919381, 0.11592955087092635, -0.24672398001038984, -0.17802508233450423, 0.2294667793660244, -0.120346411951... |
707.2823 | Management of localized energy in discrete nonlinear transmission lines | The manipulation of locked intrinsic localized modes/discrete breathers is
studied experimentally in nonlinear electric transmission line arrays.
Introducing a static lattice impurity in the form of a capacitor, resistor or
inductor has been used both to seed or destroy and attract or repel these
localized excitation... | nlin.PS | the manipulation of locked intrinsic localized modesdiscrete breathers is studied experimentally in nonlinear electric transmission line arrays introducing a static lattice impurity in the form of a capacitor resistor or inductor has been used both to seed or destroy and attract or repel these localized excitations in ... | [['the', 'manipulation', 'of', 'locked', 'intrinsic', 'localized', 'modesdiscrete', 'breathers', 'is', 'studied', 'experimentally', 'in', 'nonlinear', 'electric', 'transmission', 'line', 'arrays', 'introducing', 'a', 'static', 'lattice', 'impurity', 'in', 'the', 'form', 'of', 'a', 'capacitor', 'resistor', 'or', 'induct... | [-0.204937798301266, 0.24638846043327992, -0.036294440395960754, 0.0347392900264822, -0.08952145833014087, -0.20539909408491275, 0.03846372106027874, 0.4526527141644196, -0.26301868253609756, -0.2336126554080031, 0.08168054313017901, -0.3111503932159394, -0.0963290765310045, 0.15127805067776617, 0.03413198916347359, 0.... |
707.2824 | Quasi--local angular momentum of non--symmetric isolated and dynamical
horizons from the conformal decomposition of the metric | A new definition of quasi--local angular momentum of non--axisymmetric
marginally outer trapped surfaces is proposed. It is based on conformal
decomposition of the two--dimensional metric and the action of the group of
conformal symmetries. The definition is completely general and agrees with the
standard one in axi-... | gr-qc | a new definition of quasilocal angular momentum of nonaxisymmetric marginally outer trapped surfaces is proposed it is based on conformal decomposition of the twodimensional metric and the action of the group of conformal symmetries the definition is completely general and agrees with the standard one in axisymmetric s... | [['a', 'new', 'definition', 'of', 'quasilocal', 'angular', 'momentum', 'of', 'nonaxisymmetric', 'marginally', 'outer', 'trapped', 'surfaces', 'is', 'proposed', 'it', 'is', 'based', 'on', 'conformal', 'decomposition', 'of', 'the', 'twodimensional', 'metric', 'and', 'the', 'action', 'of', 'the', 'group', 'of', 'conformal... | [-0.15918779101533195, 0.13081260275309128, -0.12714797768179173, 0.023888232300426655, -0.1175208977656439, -0.11017084722213137, -0.08906277556282778, 0.30240865944263834, -0.1998445268254727, -0.23156071508613726, 0.0604212917072194, -0.2460651903723677, -0.11647260788595304, 0.1873544916161336, -0.09812210347202684... |
707.2825 | Dark Energy in Global Brane Universe | We discuss the exact solutions of brane universes and the results indicate
the Friedmann equations on the branes are modified with a new density term.
Then, we assume the new term as the density of dark energy. Using Wetterich's
parametrization equation of state (EOS) of dark energy, we obtain the new term
varies wit... | gr-qc | we discuss the exact solutions of brane universes and the results indicate the friedmann equations on the branes are modified with a new density term then we assume the new term as the density of dark energy using wetterichs parametrization equation of state eos of dark energy we obtain the new term varies with the red... | [['we', 'discuss', 'the', 'exact', 'solutions', 'of', 'brane', 'universes', 'and', 'the', 'results', 'indicate', 'the', 'friedmann', 'equations', 'on', 'the', 'branes', 'are', 'modified', 'with', 'a', 'new', 'density', 'term', 'then', 'we', 'assume', 'the', 'new', 'term', 'as', 'the', 'density', 'of', 'dark', 'energy',... | [-0.1810795466911483, 0.15930284351086269, -0.126574658032797, 0.10573984609082245, -0.11324766082326312, -0.10531183181620844, -0.012574983301100793, 0.2848615272986618, -0.21399245357939176, -0.31269221206183556, 0.023240705469756255, -0.25950376932545527, -0.013008020933136924, 0.12642993103083852, 0.033514556097011... |
707.2826 | Testing the External Shock Model of Gamma-Ray Bursts using the Late-Time
Simultaneous Optical and X-ray Afterglows | We study the ``normal'' decay phase of the X-ray afterglows of gamma-ray
bursts (GRBs), which follows the shallow decay phase, using the events
simultaneously observed in the R-band. The classical external shock model -- in
which neither the delayed energy injection nor time-dependency of shock
micro-physics is consi... | astro-ph | we study the normal decay phase of the xray afterglows of gammaray bursts grbs which follows the shallow decay phase using the events simultaneously observed in the rband the classical external shock model in which neither the delayed energy injection nor timedependency of shock microphysics is considered shows that th... | [['we', 'study', 'the', 'normal', 'decay', 'phase', 'of', 'the', 'xray', 'afterglows', 'of', 'gammaray', 'bursts', 'grbs', 'which', 'follows', 'the', 'shallow', 'decay', 'phase', 'using', 'the', 'events', 'simultaneously', 'observed', 'in', 'the', 'rband', 'the', 'classical', 'external', 'shock', 'model', 'in', 'which'... | [-0.07459936502944821, 0.18168355504480693, -0.06654180085214857, 0.16204098143274537, -0.04775912669988779, -0.11383618800900877, 0.09170963726937771, 0.3807831630683862, -0.20833714943952286, -0.3189373503080927, 0.053507598406241204, -0.3384076730849651, -0.029471575708773273, 0.20809107565885196, 0.0317521385382860... |
707.2827 | Debris Disks in NGC 2547 | We have surveyed the 30 Myr-old cluster NGC 2547 for planetary debris disks
using Spitzer. At 4.5-8 um we are sensitive to the photospheric level down to
mid-M stars (0.2 Msol) and at 24 um to early-G stars (1.2 Msol). We find only
two to four stars with excesses at 8 um out of ~400-500 cluster members,
resulting in ... | astro-ph | we have surveyed the 30 myrold cluster ngc 2547 for planetary debris disks using spitzer at 458 um we are sensitive to the photospheric level down to midm stars 02 msol and at 24 um to earlyg stars 12 msol we find only two to four stars with excesses at 8 um out of 400500 cluster members resulting in an excess fraction... | [['we', 'have', 'surveyed', 'the', '30', 'myrold', 'cluster', 'ngc', '2547', 'for', 'planetary', 'debris', 'disks', 'using', 'spitzer', 'at', '458', 'um', 'we', 'are', 'sensitive', 'to', 'the', 'photospheric', 'level', 'down', 'to', 'midm', 'stars', '02', 'msol', 'and', 'at', '24', 'um', 'to', 'earlyg', 'stars', '12', ... | [-0.019990686535446413, 0.14971590050822903, -0.007907492409282624, 0.06964426582076673, -0.029479653524119676, -0.06985076547890767, 0.07816433242207739, 0.4280424043920237, -0.14090913539175087, -0.424561697653658, 0.04815510608503096, -0.3682296127753006, 0.06780750121676468, 0.17566140444790848, -0.0304227816472046... |
707.2828 | Rapid Transport of Glassy Supersolid Helium in Wavy-Rough Nanpores | We show that the presumed wavy roughness distributed along the wall of
different nanopores (radius : a around 3.5 nm for Vycor or a silica glass;
around 245 nm for porous gold) will induce larger volume flow rates of solid
helium (of which there is a minimum) which might explain reported experimental
differences of t... | physics.gen-ph | we show that the presumed wavy roughness distributed along the wall of different nanopores radius a around 35 nm for vycor or a silica glass around 245 nm for porous gold will induce larger volume flow rates of solid helium of which there is a minimum which might explain reported experimental differences of the superso... | [['we', 'show', 'that', 'the', 'presumed', 'wavy', 'roughness', 'distributed', 'along', 'the', 'wall', 'of', 'different', 'nanopores', 'radius', 'a', 'around', '35', 'nm', 'for', 'vycor', 'or', 'a', 'silica', 'glass', 'around', '245', 'nm', 'for', 'porous', 'gold', 'will', 'induce', 'larger', 'volume', 'flow', 'rates',... | [-0.09095516256293502, 0.27469224493824324, -0.07672538417312554, -0.016994032888452255, 0.02570500998300011, -0.13509599087065308, 0.060742769169352825, 0.4373268522124864, -0.2251765773457996, -0.2778494249461061, 0.0745193622296013, -0.31833522560043354, -0.04489922059810389, 0.16035488537923134, -0.0473791654932044... |
707.2829 | Correspondence Between DGP Brane Cosmology and 5D Ricci-flat Cosmology | We discuss the correspondence between the DGP brane cosmology and 5D
Ricci-flat cosmology by letting their metrics equal each other. By this
correspondence, a specific geometrical property of the arbitrary integral
constant I in DGP metric is given and it is related to the curvature of 5D
bulk. At the same time, the ... | gr-qc | we discuss the correspondence between the dgp brane cosmology and 5d ricciflat cosmology by letting their metrics equal each other by this correspondence a specific geometrical property of the arbitrary integral constant i in dgp metric is given and it is related to the curvature of 5d bulk at the same time the relatio... | [['we', 'discuss', 'the', 'correspondence', 'between', 'the', 'dgp', 'brane', 'cosmology', 'and', '5d', 'ricciflat', 'cosmology', 'by', 'letting', 'their', 'metrics', 'equal', 'each', 'other', 'by', 'this', 'correspondence', 'a', 'specific', 'geometrical', 'property', 'of', 'the', 'arbitrary', 'integral', 'constant', '... | [-0.1409211721814548, 0.1117945341199326, -0.058340089738420725, 0.11019060105253528, -0.1378592575310904, -0.19907750433776528, -0.024293791670869622, 0.31124921833785874, -0.2140145514988237, -0.25741101366778213, 0.04415489574441583, -0.2944213996201547, -0.13147525443087538, 0.09648783361384024, -0.0742351331670458... |
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