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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708.0049 | Near-Field Focusing Plates and Their Design | This paper describes the design of near-field focusing plates, which are
grating-like structures that can focus electromagnetic radiation to spots or
lines of arbitrarily small subwavelength dimension. A general procedure is
outlined for designing a near-field plate given a desired image, and its
implementation at mi... | physics.class-ph | this paper describes the design of nearfield focusing plates which are gratinglike structures that can focus electromagnetic radiation to spots or lines of arbitrarily small subwavelength dimension a general procedure is outlined for designing a nearfield plate given a desired image and its implementation at microwave ... | [['this', 'paper', 'describes', 'the', 'design', 'of', 'nearfield', 'focusing', 'plates', 'which', 'are', 'gratinglike', 'structures', 'that', 'can', 'focus', 'electromagnetic', 'radiation', 'to', 'spots', 'or', 'lines', 'of', 'arbitrarily', 'small', 'subwavelength', 'dimension', 'a', 'general', 'procedure', 'is', 'out... | [-0.15259297576121753, 0.11899670391867403, -0.034149307262850925, 0.031135061277018393, -0.11418893591617234, -0.1485791878309101, -0.009653093449014705, 0.4630182718858123, -0.2185639773029834, -0.2588093955651857, 0.06357897184207104, -0.27399607681436466, -0.17338160107901784, 0.2609399358247174, -0.054384792209748... |
708.005 | Evidence for charged B meson decays to a1(1260)+/- pi0 and a1(1260)0
pi+/- | We present measurements of the branching fractions for the decays B+/- -->
a1(1260)+/- pi0 and B+/- --> a1(1260)0 pi+/- from a data sample of 232 * 10^6
BB pairs produced in e+e- annihilation through the Y(4S) resonance. We measure
the branching fraction B(B+/- --> a1(1260)+/- pi0) * B(a1(1260)+/- --> pi- pi+
pi+/-) ... | hep-ex | we present measurements of the branching fractions for the decays b a11260 pi0 and b a112600 pi from a data sample of 232 106 bb pairs produced in ee annihilation through the y4s resonance we measure the branching fraction bb a11260 pi0 ba11260 pi pi pi 132 27 21 106 with a significance of 42 sigma and the branching fr... | [['we', 'present', 'measurements', 'of', 'the', 'branching', 'fractions', 'for', 'the', 'decays', 'b', 'a11260', 'pi0', 'and', 'b', 'a112600', 'pi', 'from', 'a', 'data', 'sample', 'of', '232', '106', 'bb', 'pairs', 'produced', 'in', 'ee', 'annihilation', 'through', 'the', 'y4s', 'resonance', 'we', 'measure', 'the', 'br... | [-0.1295869651106734, 0.20723558182225507, -0.05091693105504793, 0.03299469927271061, -0.0031102835529429073, -0.05954752245589214, 0.2568552853251972, 0.2202784596613663, -0.15196940397076747, -0.26775208277737395, -0.0668848825577537, -0.4703421443262521, 0.04876241072574083, 0.11920548822073375, 0.11587848500074709,... |
708.0051 | Evidence for a dynamic phase transition in [Co/Pt]_3 magnetic
multilayers | A dynamic phase transition (DPT) with respect to the period P of an applied
alternating magnetic field has been observed previously in numerical
simulations of magnetic systems. However, experimental evidence for this DPT
has thus far been limited to qualitative observations of hysteresis loop
collapse in studies of ... | cond-mat.stat-mech cond-mat.mtrl-sci | a dynamic phase transition dpt with respect to the period p of an applied alternating magnetic field has been observed previously in numerical simulations of magnetic systems however experimental evidence for this dpt has thus far been limited to qualitative observations of hysteresis loop collapse in studies of hyster... | [['a', 'dynamic', 'phase', 'transition', 'dpt', 'with', 'respect', 'to', 'the', 'period', 'p', 'of', 'an', 'applied', 'alternating', 'magnetic', 'field', 'has', 'been', 'observed', 'previously', 'in', 'numerical', 'simulations', 'of', 'magnetic', 'systems', 'however', 'experimental', 'evidence', 'for', 'this', 'dpt', '... | [-0.15793286166094903, 0.1400215997986195, -0.07134329045843726, 0.039364119762267905, -0.06175743282344271, -0.10395388543028149, 0.0692566459416903, 0.3728991477575373, -0.231045256761779, -0.30228548799273025, 0.05904674273375265, -0.2601514796820717, -0.1385455361532071, 0.2286044828709655, 0.009333902901187853, 0.... |
708.0052 | An Introduction to Relativistic Quantum Mechanics. I. From Relativity to
Dirac Equation | By using the general concepts of special relativity and the requirements of
quantum mechanics, Dirac equation is derived and studied. Only elementary
knowledge of spin and rotations in quantum mechanics and standard handlings of
linear algebra are employed for the development of the present work.
| physics.gen-ph quant-ph | by using the general concepts of special relativity and the requirements of quantum mechanics dirac equation is derived and studied only elementary knowledge of spin and rotations in quantum mechanics and standard handlings of linear algebra are employed for the development of the present work | [['by', 'using', 'the', 'general', 'concepts', 'of', 'special', 'relativity', 'and', 'the', 'requirements', 'of', 'quantum', 'mechanics', 'dirac', 'equation', 'is', 'derived', 'and', 'studied', 'only', 'elementary', 'knowledge', 'of', 'spin', 'and', 'rotations', 'in', 'quantum', 'mechanics', 'and', 'standard', 'handlin... | [-0.08238160572946071, 0.13916978446973693, -0.05059467140171263, 0.054744200167867046, -0.08187297536577616, -0.1630991603868703, -0.03025736369503041, 0.2715609842600922, -0.25224019964742994, -0.30538976316650707, 0.07918837449979037, -0.2127082066455235, -0.16885800699108383, 0.20500814548383156, -0.049745804547435... |
708.0053 | Periodic complementary sets of binary sequences | Let PCS_p^N denote a set of p binary sequences of length N such that the sum
of their periodic auto-correlation functions is a delta-function. In the 1990,
Boemer and Antweiler addressed the problem of constructing such sequences. They
presented a table covering the range p <= 12, N <= 50 and showing in which
cases i... | cs.IT math.CO math.IT | let pcs_pn denote a set of p binary sequences of length n such that the sum of their periodic autocorrelation functions is a deltafunction in the 1990 boemer and antweiler addressed the problem of constructing such sequences they presented a table covering the range p 12 n 50 and showing in which cases it was known at ... | [['let', 'pcs_pn', 'denote', 'a', 'set', 'of', 'p', 'binary', 'sequences', 'of', 'length', 'n', 'such', 'that', 'the', 'sum', 'of', 'their', 'periodic', 'autocorrelation', 'functions', 'is', 'a', 'deltafunction', 'in', 'the', '1990', 'boemer', 'and', 'antweiler', 'addressed', 'the', 'problem', 'of', 'constructing', 'su... | [-0.17646171594193827, 0.14355591706698762, -0.02026125373862063, 0.08151194127179527, -0.015713596968756367, -0.11844645957074439, 0.06991229997365736, 0.3322971339803189, -0.30314700174688675, -0.3430763529574809, 0.1213069520861609, -0.27491416458506135, -0.12227614940493367, 0.20638543981961752, -0.0567811884878513... |
708.0054 | Designing Conducting Polymers Using Bioinspired Ant Algorithms | Ant algorithms are inspired in real ants and the main idea is to create
virtual ants that travel into the space of possible solution depositing virtual
pheromone proportional to how good a specific solution is. This creates a
autocatalytic (positive feedback) process that can be used to generate
automatic solutions t... | cond-mat.mtrl-sci cond-mat.soft | ant algorithms are inspired in real ants and the main idea is to create virtual ants that travel into the space of possible solution depositing virtual pheromone proportional to how good a specific solution is this creates a autocatalytic positive feedback process that can be used to generate automatic solutions to ver... | [['ant', 'algorithms', 'are', 'inspired', 'in', 'real', 'ants', 'and', 'the', 'main', 'idea', 'is', 'to', 'create', 'virtual', 'ants', 'that', 'travel', 'into', 'the', 'space', 'of', 'possible', 'solution', 'depositing', 'virtual', 'pheromone', 'proportional', 'to', 'how', 'good', 'a', 'specific', 'solution', 'is', 'th... | [-0.08039790322072804, 0.12312692348496057, -0.10023766722103271, 0.06967820907760824, -0.14608640451721536, -0.18651712493253095, 0.03487849715505339, 0.4080612915204256, -0.30994139409449417, -0.32437319300758344, 0.07377166169681004, -0.24146492065726002, -0.22839963575825095, 0.20137113249317432, -0.105830639561948... |
708.0055 | Banach spaces with polynomial numerical index 1 | We characterize Banach spaces with polynomial numerical index 1 when they
have the Radon-Nikod\'ym property. The holomorphic numerical index is
introduced and the characterization of the Banach space with holomorphic
numerical index 1 is obtained when it has the Radon-Nikod\'ym property.
| math.FA | we characterize banach spaces with polynomial numerical index 1 when they have the radonnikodym property the holomorphic numerical index is introduced and the characterization of the banach space with holomorphic numerical index 1 is obtained when it has the radonnikodym property | [['we', 'characterize', 'banach', 'spaces', 'with', 'polynomial', 'numerical', 'index', '1', 'when', 'they', 'have', 'the', 'radonnikodym', 'property', 'the', 'holomorphic', 'numerical', 'index', 'is', 'introduced', 'and', 'the', 'characterization', 'of', 'the', 'banach', 'space', 'with', 'holomorphic', 'numerical', 'i... | [-0.0935407584851108, 0.08770972158668972, -0.09456152873250043, 0.06958220483985071, -0.09447776676132912, -0.12068803258603666, -0.06445894590238245, 0.47731531111568937, -0.3593425668957757, -0.1594457072887297, 0.15585167532241562, -0.27352495325683823, -0.16431930152381338, 0.19177422881489847, -0.1387025787063488... |
708.0056 | Structural and transport properties of
GaAs/delta<Mn>/GaAs/InxGa1-xAs/GaAs quantum wells | We report results of investigations of structural and transport properties of
GaAs/Ga(1-x)In(x)As/GaAs quantum wells (QWs) having a 0.5-1.8 ML thick Mn
layer, separated from the QW by a 3 nm thick spacer. The structure has hole
mobility of about 2000 cm2/(V*s) being by several orders of magnitude higher
than in known... | cond-mat.mtrl-sci cond-mat.mes-hall | we report results of investigations of structural and transport properties of gaasga1xinxasgaas quantum wells qws having a 0518 ml thick mn layer separated from the qw by a 3 nm thick spacer the structure has hole mobility of about 2000 cm2vs being by several orders of magnitude higher than in known ferromagnetic twodi... | [['we', 'report', 'results', 'of', 'investigations', 'of', 'structural', 'and', 'transport', 'properties', 'of', 'gaasga1xinxasgaas', 'quantum', 'wells', 'qws', 'having', 'a', '0518', 'ml', 'thick', 'mn', 'layer', 'separated', 'from', 'the', 'qw', 'by', 'a', '3', 'nm', 'thick', 'spacer', 'the', 'structure', 'has', 'hol... | [-0.1276020356829276, 0.15283992804157046, -0.007669363870407661, -0.012331990770072722, 0.00019167540004957315, -0.12918228861070932, 0.0497156483894509, 0.4221639025585549, -0.25903115041261093, -0.3529433017149905, 0.03479061976582975, -0.3475480288216039, -0.09971926367011477, 0.19514310269245702, 0.036688354117079... |
708.0057 | Effects of Compton scattering on the Gamma Ray Spectra of Solar flares | Using fully relativistic GEANT4 simulation tool kit, the transport of
energetic electrons generated in solar flares was Monte-Carlo simulated, and
resultant bremsstrahlung gamma-ray spectra were calculated. The solar
atmosphere was approximated by 10 vertically-stacked zones. The simulation took
into account two impo... | astro-ph | using fully relativistic geant4 simulation tool kit the transport of energetic electrons generated in solar flares was montecarlo simulated and resultant bremsstrahlung gammaray spectra were calculated the solar atmosphere was approximated by 10 verticallystacked zones the simulation took into account two important phy... | [['using', 'fully', 'relativistic', 'geant4', 'simulation', 'tool', 'kit', 'the', 'transport', 'of', 'energetic', 'electrons', 'generated', 'in', 'solar', 'flares', 'was', 'montecarlo', 'simulated', 'and', 'resultant', 'bremsstrahlung', 'gammaray', 'spectra', 'were', 'calculated', 'the', 'solar', 'atmosphere', 'was', '... | [-0.023314634553815532, 0.23194878634133534, -0.0431337112095207, 0.17895337217586774, -0.06993602890771156, -0.082253849115677, -0.019132824728219974, 0.46162744186273436, -0.19975108558045154, -0.39060277121550424, -0.010780183023137109, -0.3064427214265778, -0.020291989804359107, 0.2731946794032233, 0.01242451218479... |
708.0058 | Direct Measurement of Periodic Electric Forces in Liquids | The electric forces acting on an atomic force microscope tip in solution have
been measured using a microelectrochemical cell formed by two periodically
biased electrodes. The forces were measured as a function of lift height and
bias amplitude and frequency, providing insight into electrostatic interactions
in liqui... | cond-mat.mtrl-sci | the electric forces acting on an atomic force microscope tip in solution have been measured using a microelectrochemical cell formed by two periodically biased electrodes the forces were measured as a function of lift height and bias amplitude and frequency providing insight into electrostatic interactions in liquids r... | [['the', 'electric', 'forces', 'acting', 'on', 'an', 'atomic', 'force', 'microscope', 'tip', 'in', 'solution', 'have', 'been', 'measured', 'using', 'a', 'microelectrochemical', 'cell', 'formed', 'by', 'two', 'periodically', 'biased', 'electrodes', 'the', 'forces', 'were', 'measured', 'as', 'a', 'function', 'of', 'lift'... | [-0.18091674472996463, 0.18583474906742878, -0.09123833665075982, -0.02800805548266057, -0.02793783704519913, -0.13165218600382408, 0.021301528519039513, 0.4102909617847012, -0.2753842322416203, -0.32535276023210374, -0.027176884774078605, -0.2419357776882187, -0.14216574597903478, 0.2371547136215433, 0.016413915141295... |
708.0059 | On the need to enhance physical insight via mathematical skills | It is becoming common to hear teaching advice about spending more time on the
"physics of the problem" so that students will get more physical insight and
develop a stronger intuition that can be very helpful when thinking about
physics problems. Based on this type of justification, mathematical skills such
as the ab... | physics.ed-ph | it is becoming common to hear teaching advice about spending more time on the physics of the problem so that students will get more physical insight and develop a stronger intuition that can be very helpful when thinking about physics problems based on this type of justification mathematical skills such as the ability ... | [['it', 'is', 'becoming', 'common', 'to', 'hear', 'teaching', 'advice', 'about', 'spending', 'more', 'time', 'on', 'the', 'physics', 'of', 'the', 'problem', 'so', 'that', 'students', 'will', 'get', 'more', 'physical', 'insight', 'and', 'develop', 'a', 'stronger', 'intuition', 'that', 'can', 'be', 'very', 'helpful', 'wh... | [-0.017336261108730357, 0.12877053820907516, -0.14255370519319435, 0.12829626701343919, -0.19626212395141246, -0.18590456573005168, 0.06663920092978515, 0.36385749954224367, -0.23079775991838103, -0.3864547386995436, 0.0628198814480623, -0.24599996162291018, -0.12623417150533908, 0.21762653185991732, -0.115340398293977... |
708.006 | The Nature of the Compact X-ray Source in Supernova Remnant RCW 103 | The discovery of the 6.67 hr periodicity in the X-ray source 1E 161348-5055
associated with the supernova remnant RCW 103 has raised interesting
suggestions about the nature of the X-ray source. Here we argue that in either
accreting neutron star or magnetar model, a supernova fallback disk may be a
critical ingredie... | astro-ph | the discovery of the 667 hr periodicity in the xray source 1e 1613485055 associated with the supernova remnant rcw 103 has raised interesting suggestions about the nature of the xray source here we argue that in either accreting neutron star or magnetar model a supernova fallback disk may be a critical ingredient in th... | [['the', 'discovery', 'of', 'the', '667', 'hr', 'periodicity', 'in', 'the', 'xray', 'source', '1e', '1613485055', 'associated', 'with', 'the', 'supernova', 'remnant', 'rcw', '103', 'has', 'raised', 'interesting', 'suggestions', 'about', 'the', 'nature', 'of', 'the', 'xray', 'source', 'here', 'we', 'argue', 'that', 'in'... | [-0.10535493524806512, 0.11342714606159991, -0.07486641194139208, 0.13412979096094685, -0.18998826081240242, -0.10686489651081982, 0.12381410703144885, 0.4119178914761805, -0.21654618646089846, -0.3279486563834515, 0.14061136693171747, -0.2707005654881289, -0.05010314639094848, 0.2560835508987881, -0.0787604089550019, ... |
708.0061 | Cross Validation for Comparing Multiple Density Estimation Procedures | We demonstrate the consistency of cross validation for comparing multiple
density estimators using simple inequalities on the likelihood ratio. In
nonparametric problems, the splitting of data does not require the domination
of test data over the training/estimation data, contrary to Shao (1993). The
result is comple... | math.ST stat.TH | we demonstrate the consistency of cross validation for comparing multiple density estimators using simple inequalities on the likelihood ratio in nonparametric problems the splitting of data does not require the domination of test data over the trainingestimation data contrary to shao 1993 the result is complementary t... | [['we', 'demonstrate', 'the', 'consistency', 'of', 'cross', 'validation', 'for', 'comparing', 'multiple', 'density', 'estimators', 'using', 'simple', 'inequalities', 'on', 'the', 'likelihood', 'ratio', 'in', 'nonparametric', 'problems', 'the', 'splitting', 'of', 'data', 'does', 'not', 'require', 'the', 'domination', 'o... | [-0.04939998765388187, -0.030465223967044982, -0.1100506759687977, 0.07645139340003777, -0.10561538540389177, -0.08442452312710713, 0.072003585220543, 0.31556048412930293, -0.16330254811767209, -0.3775429458023523, 0.11595760964357979, -0.2833369059997769, -0.0884227484271352, 0.22043790374794658, -0.127012073730101, 0... |
708.0062 | On Information Theory, Spectral Geometry and Quantum Gravity | We show that there exists a deep link between the two disciplines of
information theory and spectral geometry. This allows us to obtain new results
on a well known quantum gravity motivated natural ultraviolet cutoff which
describes an upper bound on the spatial density of information. Concretely, we
show that, toget... | gr-qc | we show that there exists a deep link between the two disciplines of information theory and spectral geometry this allows us to obtain new results on a well known quantum gravity motivated natural ultraviolet cutoff which describes an upper bound on the spatial density of information concretely we show that together wi... | [['we', 'show', 'that', 'there', 'exists', 'a', 'deep', 'link', 'between', 'the', 'two', 'disciplines', 'of', 'information', 'theory', 'and', 'spectral', 'geometry', 'this', 'allows', 'us', 'to', 'obtain', 'new', 'results', 'on', 'a', 'well', 'known', 'quantum', 'gravity', 'motivated', 'natural', 'ultraviolet', 'cutoff... | [-0.10971048638044346, 0.12657216840995705, -0.16204928899664553, 0.09760316546821106, -0.10164954606193288, -0.07805211698356014, 0.04460027269388159, 0.38229111226535933, -0.23538749495781558, -0.3118824185002395, 0.049324336715833715, -0.24677961314943875, -0.1967751977624752, 0.19307776589587491, -0.125928080220135... |
708.0063 | Information flow between composite stock index and individual stocks | We investigate the strength and the direction of information transfer in the
U.S. stock market between the composite stock price index of stock market and
prices of individual stocks using the transfer entropy. Through the
directionality of the information transfer, we find that individual stocks are
influenced by th... | q-fin.ST physics.soc-ph | we investigate the strength and the direction of information transfer in the us stock market between the composite stock price index of stock market and prices of individual stocks using the transfer entropy through the directionality of the information transfer we find that individual stocks are influenced by the inde... | [['we', 'investigate', 'the', 'strength', 'and', 'the', 'direction', 'of', 'information', 'transfer', 'in', 'the', 'us', 'stock', 'market', 'between', 'the', 'composite', 'stock', 'price', 'index', 'of', 'stock', 'market', 'and', 'prices', 'of', 'individual', 'stocks', 'using', 'the', 'transfer', 'entropy', 'through', ... | [-0.07401009063447281, 0.09998494307598416, -0.13477871679472472, 0.13676071567636616, -0.04363187247852109, -0.09069492172379538, 0.1667227695854205, 0.4663796855031319, -0.3349079912844694, -0.29729622753583035, 0.12228232028867768, -0.35154060949132127, -0.13853509073971576, 0.15929689525433308, -0.05755159592712825... |
708.0064 | The Effect of Variability on the Estimation of Quasar Black Hole Masses | We investigate the time-dependent variations of ultraviolet (UV) black hole
mass estimates of quasars in the Sloan Digital Sky Survey (SDSS). From SDSS
spectra of 615 high-redshift (1.69 < z < 4.75) quasars with spectra from two
epochs, we estimate black hole masses, using a single-epoch technique which
employs an ad... | astro-ph | we investigate the timedependent variations of ultraviolet uv black hole mass estimates of quasars in the sloan digital sky survey sdss from sdss spectra of 615 highredshift 169 z 475 quasars with spectra from two epochs we estimate black hole masses using a singleepoch technique which employs an additional automated n... | [['we', 'investigate', 'the', 'timedependent', 'variations', 'of', 'ultraviolet', 'uv', 'black', 'hole', 'mass', 'estimates', 'of', 'quasars', 'in', 'the', 'sloan', 'digital', 'sky', 'survey', 'sdss', 'from', 'sdss', 'spectra', 'of', '615', 'highredshift', '169', 'z', '475', 'quasars', 'with', 'spectra', 'from', 'two',... | [-0.026788012252785685, 0.052034517334269885, -0.020106966469928707, 0.13535160136675944, -0.07427905934203542, -0.06494224383077177, 0.08331619299754627, 0.44331577232923736, -0.11625601295800356, -0.39431400656741994, 0.07053351102349756, -0.35414055971365965, -0.01578052176144288, 0.2276113883688983, -0.070107313223... |
708.0065 | Localization of Matters on Pure Geometrical Thick Branes | In the literatures, several types of thick smooth brane configurations in a
pure geometric Weyl integrable 5-dimensional space time have been presented.
The Weyl geometry is a non-Riemannian modification of 5-dimensional
Kaluza--Klein (KK) theory. All these thick brane solutions preserve
4-dimensional Poincar\'e inva... | hep-th | in the literatures several types of thick smooth brane configurations in a pure geometric weyl integrable 5dimensional space time have been presented the weyl geometry is a nonriemannian modification of 5dimensional kaluzaklein kk theory all these thick brane solutions preserve 4dimensional poincare invariance and some... | [['in', 'the', 'literatures', 'several', 'types', 'of', 'thick', 'smooth', 'brane', 'configurations', 'in', 'a', 'pure', 'geometric', 'weyl', 'integrable', '5dimensional', 'space', 'time', 'have', 'been', 'presented', 'the', 'weyl', 'geometry', 'is', 'a', 'nonriemannian', 'modification', 'of', '5dimensional', 'kaluzakl... | [-0.1785521119693543, 0.2064882237383259, -0.056019499005231864, 0.0804666845528857, -0.09847788001973441, -0.19955243040554793, -0.038683515065723165, 0.32619207714470155, -0.1863170985162338, -0.22474527954158777, 0.07502854319867046, -0.27273125425703265, -0.10997637576563035, 0.11665543107151546, -0.001655155643422... |
708.0066 | Symmetries of spatial graphs and Simon invariants | An ordered and oriented 2-component link L in the 3-sphere is said to be
achiral if it is ambient isotopic to its mirror image ignoring the orientation
and ordering of the components. Kirk-Livingston showed that if L is achiral
then the linking number of L is not congruent to 2 modulo 4. In this paper we
study orient... | math.GT | an ordered and oriented 2component link l in the 3sphere is said to be achiral if it is ambient isotopic to its mirror image ignoring the orientation and ordering of the components kirklivingston showed that if l is achiral then the linking number of l is not congruent to 2 modulo 4 in this paper we study orientationpr... | [['an', 'ordered', 'and', 'oriented', '2component', 'link', 'l', 'in', 'the', '3sphere', 'is', 'said', 'to', 'be', 'achiral', 'if', 'it', 'is', 'ambient', 'isotopic', 'to', 'its', 'mirror', 'image', 'ignoring', 'the', 'orientation', 'and', 'ordering', 'of', 'the', 'components', 'kirklivingston', 'showed', 'that', 'if',... | [-0.20894721299033575, 0.14553430851097948, -0.027539458295161075, 0.047947993209218664, -0.11066536338896388, -0.1529015363805523, 0.011117762285096552, 0.4283050350995377, -0.266861360379015, -0.3330420087928874, 0.08162131755626902, -0.2761947555900222, -0.15063329687285604, 0.06982806792854322, -0.09673974115984758... |
708.0067 | Pirogov-Sinai Theory With New Contours for Symmetric Models | The contour argument was introduced by Peierls for two dimensional Ising
model. Peierls benefited from the particular symmetries of the Ising model. For
non-symmetric models the argument was developed by Pirogov and Sinai. It is
very general and rather difficult. Intuitively clear that the Peierls argument
does work ... | math-ph math.MP | the contour argument was introduced by peierls for two dimensional ising model peierls benefited from the particular symmetries of the ising model for nonsymmetric models the argument was developed by pirogov and sinai it is very general and rather difficult intuitively clear that the peierls argument does work for any... | [['the', 'contour', 'argument', 'was', 'introduced', 'by', 'peierls', 'for', 'two', 'dimensional', 'ising', 'model', 'peierls', 'benefited', 'from', 'the', 'particular', 'symmetries', 'of', 'the', 'ising', 'model', 'for', 'nonsymmetric', 'models', 'the', 'argument', 'was', 'developed', 'by', 'pirogov', 'and', 'sinai', ... | [-0.0512995513335971, 0.10535574267110363, -0.12241468460891734, 0.116545103834307, -0.14948030324144798, -0.23381706335243177, 0.048329526488669214, 0.3489603691649708, -0.21870776330390734, -0.2407316472762349, 0.044515827584969386, -0.2009735915832359, -0.2197222761471163, 0.1878460159768689, -0.0883543971333314, 0.... |
708.0068 | Faithful qubit transmission against collective noise without ancillary
qubits | We present a faithful qubit transmission scheme with linear optics against
collective noise, not resorting to ancillary qubits. Its set-up is composed of
three unbalanced polarization interferometers, based on a polarizing beam
splitter, a beam splitter and a half-wave plate, which makes this scheme more
feasible tha... | quant-ph | we present a faithful qubit transmission scheme with linear optics against collective noise not resorting to ancillary qubits its setup is composed of three unbalanced polarization interferometers based on a polarizing beam splitter a beam splitter and a halfwave plate which makes this scheme more feasible than others ... | [['we', 'present', 'a', 'faithful', 'qubit', 'transmission', 'scheme', 'with', 'linear', 'optics', 'against', 'collective', 'noise', 'not', 'resorting', 'to', 'ancillary', 'qubits', 'its', 'setup', 'is', 'composed', 'of', 'three', 'unbalanced', 'polarization', 'interferometers', 'based', 'on', 'a', 'polarizing', 'beam'... | [-0.1835584953143964, 0.14686900033093309, -0.08205395887763996, -0.009762842928604135, -0.024140847113229474, -0.27408433483720246, 0.07753158387956473, 0.4342021449064871, -0.21153067117381208, -0.2773988259833236, 0.08492408377197483, -0.2421433310955763, -0.09869860312989298, 0.24912510220101983, -0.102869355726003... |
708.0069 | Twisted Gauge and Gravity Theories on the Groenewold-Moyal Plane | Recent work [hep-th/0504183,hep-th/0508002] indicates an approach to the
formulation of diffeomorphism invariant quantum field theories (qft's) on the
Groenewold-Moyal (GM) plane. In this approach to the qft's, statistics gets
twisted and the S-matrix in the non-gauge qft's becomes independent of the
noncommutativity... | hep-th gr-qc hep-ph math-ph math.MP math.QA | recent work hepth0504183hepth0508002 indicates an approach to the formulation of diffeomorphism invariant quantum field theories qfts on the groenewoldmoyal gm plane in this approach to the qfts statistics gets twisted and the smatrix in the nongauge qfts becomes independent of the noncommutativity parameter thetamunu ... | [['recent', 'work', 'hepth0504183hepth0508002', 'indicates', 'an', 'approach', 'to', 'the', 'formulation', 'of', 'diffeomorphism', 'invariant', 'quantum', 'field', 'theories', 'qfts', 'on', 'the', 'groenewoldmoyal', 'gm', 'plane', 'in', 'this', 'approach', 'to', 'the', 'qfts', 'statistics', 'gets', 'twisted', 'and', 't... | [-0.14025256498632488, 0.17566417285957062, -0.12917518686230306, 0.08918917328393196, -0.1317329051181657, -0.13518213780756988, -0.0340693510043734, 0.3357855149995687, -0.23366199533678422, -0.27653277312232627, 0.09011097653448683, -0.21783662317699976, -0.17362560285255313, 0.14794667165439862, -0.0997903188511442... |
708.007 | Bohmian Mechanics at Space-Time Singularities. I. Timelike Singularities | We develop an extension of Bohmian mechanics to a curved background
space-time containing a singularity. The present paper focuses on timelike
singularities. We use the naked timelike singularity of the super-critical
Reissner-Nordstrom geometry as an example. While one could impose boundary
conditions at the singula... | quant-ph | we develop an extension of bohmian mechanics to a curved background spacetime containing a singularity the present paper focuses on timelike singularities we use the naked timelike singularity of the supercritical reissnernordstrom geometry as an example while one could impose boundary conditions at the singularity tha... | [['we', 'develop', 'an', 'extension', 'of', 'bohmian', 'mechanics', 'to', 'a', 'curved', 'background', 'spacetime', 'containing', 'a', 'singularity', 'the', 'present', 'paper', 'focuses', 'on', 'timelike', 'singularities', 'we', 'use', 'the', 'naked', 'timelike', 'singularity', 'of', 'the', 'supercritical', 'reissnerno... | [-0.10344186820125637, 0.13245412983615296, -0.16705019378287533, 0.11803775334928915, -0.0822738649727838, -0.1711134474166761, -0.025660180700379988, 0.28854637223572194, -0.27098611871210426, -0.2125510965770745, 0.07626293612718275, -0.2953635779296427, -0.1338191318509916, 0.1427347635777391, -0.067333500587975, 0... |
708.0071 | Coulomb effects on the formation of proton halo nuclei | The exotic structures in the 2s_{1/2} states of five pairs of mirror nuclei
^{17}O-^{17}F, ^{26}Na-^{26}P, ^{27}Mg-^{27}P, ^{28}Al-^{28}P and
^{29}Si-^{29}P are investigated with the relativistic mean-field (RMF) theory
and the single-particle model (SPM) to explore the role of the Coulomb effects
on the proton halo ... | nucl-th | the exotic structures in the 2s_12 states of five pairs of mirror nuclei 17o17f 26na26p 27mg27p 28al28p and 29si29p are investigated with the relativistic meanfield rmf theory and the singleparticle model spm to explore the role of the coulomb effects on the proton halo formation the present rmf calculations show that ... | [['the', 'exotic', 'structures', 'in', 'the', '2s_12', 'states', 'of', 'five', 'pairs', 'of', 'mirror', 'nuclei', '17o17f', '26na26p', '27mg27p', '28al28p', 'and', '29si29p', 'are', 'investigated', 'with', 'the', 'relativistic', 'meanfield', 'rmf', 'theory', 'and', 'the', 'singleparticle', 'model', 'spm', 'to', 'explor... | [-0.08458150273228138, 0.2222557014550571, -0.09309221065538649, 0.1566879570145289, -0.003971823994854078, -0.1011839372980164, 0.026994143246723765, 0.34851192618434385, -0.20134043540934674, -0.3297355433137589, -0.0249010187978303, -0.33803958436566417, -0.05268169205986185, 0.1324685199052501, 0.04434413844108637,... |
708.0072 | Vortex states in superconductors with strong Pauli-paramagnetic effect | Using the quasiclassical theory, we analyze the vortex structure of
strong-paramagnetic superconductors.There, induced paramagnetic moments are
accumulated exclusively around the vortex core. We quantitatively evaluate the
significant paramagnetic effect in the H-dependence of various quantities, such
as low temperat... | cond-mat.supr-con | using the quasiclassical theory we analyze the vortex structure of strongparamagnetic superconductorsthere induced paramagnetic moments are accumulated exclusively around the vortex core we quantitatively evaluate the significant paramagnetic effect in the hdependence of various quantities such as low temperature speci... | [['using', 'the', 'quasiclassical', 'theory', 'we', 'analyze', 'the', 'vortex', 'structure', 'of', 'strongparamagnetic', 'superconductorsthere', 'induced', 'paramagnetic', 'moments', 'are', 'accumulated', 'exclusively', 'around', 'the', 'vortex', 'core', 'we', 'quantitatively', 'evaluate', 'the', 'significant', 'parama... | [-0.1635222897575413, 0.2198866251100962, 0.00311480974778533, 0.07084564234104913, -0.07146776954932893, -0.03907302609720343, 0.08972607545925908, 0.3478935893776046, -0.25276593894169136, -0.28671768675180703, 0.0036878377243222014, -0.3469137451989022, -0.07825502605064193, 0.14405714329080405, 0.0645743955266536, ... |
708.0073 | Suzaku wide-band observations of SN 1006 | We report on the wide band spectra of SN 1006 as observed by Suzaku. Thermal
and nonthermal emission are successfully resolved thanks to the excellent
spectral response of Suzaku's X-ray CCD XIS. The nonthermal emission cannot be
reproduced by a simple power-law model but needs a roll-off at 5.7$\times
10^{16}$ Hz = ... | astro-ph | we report on the wide band spectra of sn 1006 as observed by suzaku thermal and nonthermal emission are successfully resolved thanks to the excellent spectral response of suzakus xray ccd xis the nonthermal emission cannot be reproduced by a simple powerlaw model but needs a rolloff at 57times 1016 hz 023 kev the rollo... | [['we', 'report', 'on', 'the', 'wide', 'band', 'spectra', 'of', 'sn', '1006', 'as', 'observed', 'by', 'suzaku', 'thermal', 'and', 'nonthermal', 'emission', 'are', 'successfully', 'resolved', 'thanks', 'to', 'the', 'excellent', 'spectral', 'response', 'of', 'suzakus', 'xray', 'ccd', 'xis', 'the', 'nonthermal', 'emission... | [0.0001821206762256582, 0.1174049263642159, -0.05019692280277442, 0.0964455801347438, -0.07468098099343479, -0.1391353142039662, 0.056779954645238565, 0.4850931148452873, -0.15484644124791905, -0.3888412057160494, 0.08050639010453073, -0.33266418343514537, 0.04362061044222183, 0.24031062851976498, -0.016772768350339, -... |
708.0074 | Rational solutions of the Noumi and Yamada system of type $A_4^{(1)}$ | In this paper, we completely classify the raional solutions of the Noumi and
Yamada system of type A_4^{(1)}, which is a generalization of the forth
Painlev\'e equation. The rational solutions are classified to three types by
the B\"acklund transformation group.
| math.CA | in this paper we completely classify the raional solutions of the noumi and yamada system of type a_41 which is a generalization of the forth painleve equation the rational solutions are classified to three types by the backlund transformation group | [['in', 'this', 'paper', 'we', 'completely', 'classify', 'the', 'raional', 'solutions', 'of', 'the', 'noumi', 'and', 'yamada', 'system', 'of', 'type', 'a_41', 'which', 'is', 'a', 'generalization', 'of', 'the', 'forth', 'painleve', 'equation', 'the', 'rational', 'solutions', 'are', 'classified', 'to', 'three', 'types', ... | [-0.1879069817562898, -0.017962373052843105, -0.07709679504235585, 0.027912069279222917, -0.11629624784183808, -0.17750064874641025, 0.024504580388729196, 0.24857161566615105, -0.3252744154097178, -0.23605290236763465, 0.1206421595132456, -0.329564476146912, -0.21100937298093086, 0.1451268014139854, -0.0879098309012941... |
708.0075 | A multi-objective optimization procedure to develop
modified-embedded-atom-method potentials: an application to magnesium | We have developed a multi-objective optimization (MOO) procedure to construct
modified-embedded-atom-method (MEAM) potentials with minimal manual fitting.
This procedure has been applied successfully to develop a new MEAM potential
for magnesium. The MOO procedure is designed to optimally reproduce multiple
target va... | cond-mat.mtrl-sci | we have developed a multiobjective optimization moo procedure to construct modifiedembeddedatommethod meam potentials with minimal manual fitting this procedure has been applied successfully to develop a new meam potential for magnesium the moo procedure is designed to optimally reproduce multiple target values that co... | [['we', 'have', 'developed', 'a', 'multiobjective', 'optimization', 'moo', 'procedure', 'to', 'construct', 'modifiedembeddedatommethod', 'meam', 'potentials', 'with', 'minimal', 'manual', 'fitting', 'this', 'procedure', 'has', 'been', 'applied', 'successfully', 'to', 'develop', 'a', 'new', 'meam', 'potential', 'for', '... | [-0.013318070297365979, 0.029375272950837538, -0.09933785132561175, 0.05988033448940971, -0.030134438477929622, -0.15388127728291448, 0.06142518733210477, 0.45678040642838275, -0.2036266477283327, -0.3656222048910364, -0.015994907705120683, -0.2890423552857505, -0.14593016762557368, 0.20343847157773637, 0.0172997542642... |
708.0076 | Optical and radio survey of Southern Compact Groups of galaxies. I.
Pilot study of six groups | Multi-wavelength observations of Hickson's Compact Groups (HCGs) have shown
that many of these groups are physical bound structures and are in different
stage of evolution, from spiral-dominated systems to almost merged objects.
Very few studies have analysed the Southern Compact Groups (SCGs) sample, which
is though... | astro-ph | multiwavelength observations of hicksons compact groups hcgs have shown that many of these groups are physical bound structures and are in different stage of evolution from spiraldominated systems to almost merged objects very few studies have analysed the southern compact groups scgs sample which is though to be young... | [['multiwavelength', 'observations', 'of', 'hicksons', 'compact', 'groups', 'hcgs', 'have', 'shown', 'that', 'many', 'of', 'these', 'groups', 'are', 'physical', 'bound', 'structures', 'and', 'are', 'in', 'different', 'stage', 'of', 'evolution', 'from', 'spiraldominated', 'systems', 'to', 'almost', 'merged', 'objects', ... | [-0.0868970709718549, 0.08576122118710117, -0.12453913414038909, 0.05567440310140881, -0.09692805322508018, -0.041509981882065915, 0.03445778792807593, 0.4924618168137012, -0.1414044286387089, -0.36439009653165555, 0.12407791058574684, -0.262933336938612, -0.10429689903648044, 0.25142133637116504, -0.05531325603787524,... |
708.0077 | Multi-Photon Interference and Temporal Distinguishability of Photons | A number of recent interference experiments involving multiple photons are
reviewed. These experiments include generalized photon bunching effects,
generalized Hong-Ou-Mandel interference effects and multi-photon interferometry
for demonstrations of multi-photon de Broglie wavelength. The multi-photon
states used in ... | quant-ph | a number of recent interference experiments involving multiple photons are reviewed these experiments include generalized photon bunching effects generalized hongoumandel interference effects and multiphoton interferometry for demonstrations of multiphoton de broglie wavelength the multiphoton states used in these expe... | [['a', 'number', 'of', 'recent', 'interference', 'experiments', 'involving', 'multiple', 'photons', 'are', 'reviewed', 'these', 'experiments', 'include', 'generalized', 'photon', 'bunching', 'effects', 'generalized', 'hongoumandel', 'interference', 'effects', 'and', 'multiphoton', 'interferometry', 'for', 'demonstratio... | [-0.16468623452782025, 0.2380663751506453, -0.0886238360005181, 0.09536820180653556, -0.011471445800933412, -0.1187874162039621, 0.04850058870984438, 0.3876107551642065, -0.24390845483062956, -0.3164271386832423, -0.057495008857837475, -0.2968044932023054, -0.14654847755422437, 0.1979333726817939, -0.02996924015451071,... |
708.0078 | Soft gamma-ray galactic ridge emission as unveiled by SPI aboard
INTEGRAL | The origin of the soft gamma-ray (200 keV - 1 MeV) galactic ridge emission is
one of the long-standing mysteries in the field of high-energy astrophysics.
Population studies at lower energies have shown that emission from accreting
compact objects gradually recedes in this domain, leaving place to another
source of g... | astro-ph | the origin of the soft gammaray 200 kev 1 mev galactic ridge emission is one of the longstanding mysteries in the field of highenergy astrophysics population studies at lower energies have shown that emission from accreting compact objects gradually recedes in this domain leaving place to another source of gammaray emi... | [['the', 'origin', 'of', 'the', 'soft', 'gammaray', '200', 'kev', '1', 'mev', 'galactic', 'ridge', 'emission', 'is', 'one', 'of', 'the', 'longstanding', 'mysteries', 'in', 'the', 'field', 'of', 'highenergy', 'astrophysics', 'population', 'studies', 'at', 'lower', 'energies', 'have', 'shown', 'that', 'emission', 'from',... | [-0.026480471930097275, 0.1422240869650596, -0.0907110230938328, 0.1375604253181995, -0.12277115446120179, -0.06816376689232714, 0.031096394085485875, 0.45678819850857916, -0.2425435144031399, -0.3436027456545967, 0.056615135170808385, -0.3099439563297422, -0.015811823078313435, 0.21183505471281963, 0.02685757249797127... |
708.0079 | Semiparametrically efficient rank-based inference for shape II. Optimal
R-estimation of shape | A class of R-estimators based on the concepts of multivariate signed ranks
and the optimal rank-based tests developed in Hallin and Paindaveine [Ann.
Statist. 34 (2006)] is proposed for the estimation of the shape matrix of an
elliptical distribution. These R-estimators are root-n consistent under any
radial density ... | math.ST stat.TH | a class of restimators based on the concepts of multivariate signed ranks and the optimal rankbased tests developed in hallin and paindaveine ann statist 34 2006 is proposed for the estimation of the shape matrix of an elliptical distribution these restimators are rootn consistent under any radial density g without any... | [['a', 'class', 'of', 'restimators', 'based', 'on', 'the', 'concepts', 'of', 'multivariate', 'signed', 'ranks', 'and', 'the', 'optimal', 'rankbased', 'tests', 'developed', 'in', 'hallin', 'and', 'paindaveine', 'ann', 'statist', '34', '2006', 'is', 'proposed', 'for', 'the', 'estimation', 'of', 'the', 'shape', 'matrix', ... | [-0.047244405828869754, 0.032445725939109445, -0.12219346254967509, 0.11261006118423354, -0.06760672937257607, -0.12636760514425605, 0.034659628084275605, 0.4022805955211975, -0.1663533465922994, -0.28290793498500105, 0.14385364212763593, -0.23701812937169484, -0.1474257697914972, 0.19435657212038918, -0.12813131424206... |
708.008 | Farey Statistics in Time n^{2/3} and Counting Primitive Lattice Points
in Polygons | We present algorithms for computing ranks and order statistics in the Farey
sequence, taking time O (n^{2/3}). This improves on the recent algorithms of
Pawlewicz [European Symp. Alg. 2007], running in time O (n^{3/4}). We also
initiate the study of a more general algorithmic problem: counting primitive
lattice point... | math.NT | we present algorithms for computing ranks and order statistics in the farey sequence taking time o n23 this improves on the recent algorithms of pawlewicz european symp alg 2007 running in time o n34 we also initiate the study of a more general algorithmic problem counting primitive lattice points in planar shapes | [['we', 'present', 'algorithms', 'for', 'computing', 'ranks', 'and', 'order', 'statistics', 'in', 'the', 'farey', 'sequence', 'taking', 'time', 'o', 'n23', 'this', 'improves', 'on', 'the', 'recent', 'algorithms', 'of', 'pawlewicz', 'european', 'symp', 'alg', '2007', 'running', 'in', 'time', 'o', 'n34', 'we', 'also', 'i... | [-0.15319332471984787, 0.044687594232313776, -0.03747961414503116, 0.04561141570436531, -0.004830194089342566, -0.05712519581520967, 0.0900742841916451, 0.3955148683459151, -0.2131909858070168, -0.31519295172948464, 0.07879035607865993, -0.24671734014854713, -0.14951950709755515, 0.16469856132479274, -0.122363197142440... |
708.0081 | d-alpha Correlation functions and collective motion in Xe+Au collisions
at E/A=50 MeV | The interplay of the effects of geometry and collective motion on d-$\alpha$
correlation functions is investigated for central Xe+Au collisions at E/A=50
MeV. The data cannot be explained without collective motion, which could be
partly along the beam axis. A semi-quantitative description of the data can be
obtained ... | nucl-ex | the interplay of the effects of geometry and collective motion on dalpha correlation functions is investigated for central xeau collisions at ea50 mev the data cannot be explained without collective motion which could be partly along the beam axis a semiquantitative description of the data can be obtained using a monte... | [['the', 'interplay', 'of', 'the', 'effects', 'of', 'geometry', 'and', 'collective', 'motion', 'on', 'dalpha', 'correlation', 'functions', 'is', 'investigated', 'for', 'central', 'xeau', 'collisions', 'at', 'ea50', 'mev', 'the', 'data', 'can', 'not', 'be', 'explained', 'without', 'collective', 'motion', 'which', 'could... | [-0.10463486283855594, 0.16554207101707225, -0.1319035339402035, 0.08021779547941507, -0.053894973996806504, -0.08128531018282166, 0.009288382458338596, 0.3869888963096816, -0.2862051170795103, -0.301082503941396, 0.05175900475992619, -0.2980868276006178, -0.05711307834185984, 0.18995474124803086, 0.010818921960890293,... |
708.0082 | Measurement of the near-threshold $e^+e^- \to D \bar D$ cross section
using initial-state radiation | We report measurements of the exclusive cross section for $e^+e^- \to D \bar
D $, where $D=D^0$ or $D^+$, in the center-of-mass energy range from the $D
\bar D $ threshold to $5\mathrm{GeV}/c^2$ with initial-state radiation. The
analysis is based on a data sample collected with the Belle detector with an
integrated l... | hep-ex | we report measurements of the exclusive cross section for ee to d bar d where dd0 or d in the centerofmass energy range from the d bar d threshold to 5mathrmgevc2 with initialstate radiation the analysis is based on a data sample collected with the belle detector with an integrated luminosity of 673 mathrmfb1 | [['we', 'report', 'measurements', 'of', 'the', 'exclusive', 'cross', 'section', 'for', 'ee', 'to', 'd', 'bar', 'd', 'where', 'dd0', 'or', 'd', 'in', 'the', 'centerofmass', 'energy', 'range', 'from', 'the', 'd', 'bar', 'd', 'threshold', 'to', '5mathrmgevc2', 'with', 'initialstate', 'radiation', 'the', 'analysis', 'is', ... | [-0.07120393843934783, 0.1056866529246656, -0.11089441223280891, -0.022972236850896395, -0.015027758600036526, -0.12106688885580537, 0.03452260699123144, 0.3387365296904771, -0.15278988349128445, -0.3269524826264044, -0.017063786400886218, -0.4440951099056961, 0.09775332007820736, 0.14733064851178876, 0.105360428521515... |
708.0083 | 2004 IMS Medallion Lecture: Local Rademacher complexities and oracle
inequalities in risk minimization | Let $\mathcal{F}$ be a class of measurable functions $f:S\mapsto [0,1]$
defined on a probability space $(S,\mathcal{A},P)$. Given a sample
(X_1,...,X_n) of i.i.d. random variables taking values in S with common
distribution P, let P_n denote the empirical measure based on (X_1,...,X_n). We
study an empirical risk min... | math.ST stat.TH | let mathcalf be a class of measurable functions fsmapsto 01 defined on a probability space smathcalap given a sample x_1x_n of iid random variables taking values in s with common distribution p let p_n denote the empirical measure based on x_1x_n we study an empirical risk minimization problem p_nfto min fin mathcalf g... | [['let', 'mathcalf', 'be', 'a', 'class', 'of', 'measurable', 'functions', 'fsmapsto', '01', 'defined', 'on', 'a', 'probability', 'space', 'smathcalap', 'given', 'a', 'sample', 'x_1x_n', 'of', 'iid', 'random', 'variables', 'taking', 'values', 'in', 's', 'with', 'common', 'distribution', 'p', 'let', 'p_n', 'denote', 'the... | [-0.09154868728731025, 0.06584431965373201, -0.07246238505159387, 0.11325693289619802, -0.05708114657433864, -0.14060367925388628, 0.10570569053933715, 0.3507022373008215, -0.2771645562710944, -0.2738100252428789, 0.11795958330922618, -0.29621360477504155, -0.1231625278562073, 0.2312646473199746, -0.13942877071237328, ... |
708.0084 | Equivariant Birch-Swinnerton-Dyer conjecture for the base change of
elliptic curves: An example | Let E be an elliptic curved defined over $\Q$ and let $K/\Q$ be a finite
Galois extension with Galois group G. The equivariant Birch-Swinnerton-Dyer
conjecture for $h^1(E\times_{\Q} K)(1)$ viewed as a motive over $\Q$ with
coefficients in $\Q[G]$ relates the twisted L-values associated with E with the
arithmetic inva... | math.NT | let e be an elliptic curved defined over q and let kq be a finite galois extension with galois group g the equivariant birchswinnertondyer conjecture for h1etimes_q k1 viewed as a motive over q with coefficients in qg relates the twisted lvalues associated with e with the arithmetic invariants of the same in this paper... | [['let', 'e', 'be', 'an', 'elliptic', 'curved', 'defined', 'over', 'q', 'and', 'let', 'kq', 'be', 'a', 'finite', 'galois', 'extension', 'with', 'galois', 'group', 'g', 'the', 'equivariant', 'birchswinnertondyer', 'conjecture', 'for', 'h1etimes_q', 'k1', 'viewed', 'as', 'a', 'motive', 'over', 'q', 'with', 'coefficients'... | [-0.2155285425972016, 0.046662978168959465, -0.17258857760489696, -0.010933822191353621, -0.06528968172192219, -0.1584659733510177, -0.053453981331715895, 0.2843923036097771, -0.32884727637948735, -0.27116190854992184, 0.02911415454166542, -0.23539977488828645, -0.10204742487985641, 0.27008284766980933, -0.177336480310... |
708.0085 | X-Rays From Massive OB Stars: Thermal Emission From Radiative Shocks | Chandra gratings spectra of a sample of 15 massive OB stars were analyzed
under the basic assumption that the X-ray emission is produced in an ensemble
of shocks formed in the winds driven by these objects. Shocks develop either as
a result of radiation-driven instabilities or due to confinement of the wind by
relati... | astro-ph | chandra gratings spectra of a sample of 15 massive ob stars were analyzed under the basic assumption that the xray emission is produced in an ensemble of shocks formed in the winds driven by these objects shocks develop either as a result of radiationdriven instabilities or due to confinement of the wind by relatively ... | [['chandra', 'gratings', 'spectra', 'of', 'a', 'sample', 'of', '15', 'massive', 'ob', 'stars', 'were', 'analyzed', 'under', 'the', 'basic', 'assumption', 'that', 'the', 'xray', 'emission', 'is', 'produced', 'in', 'an', 'ensemble', 'of', 'shocks', 'formed', 'in', 'the', 'winds', 'driven', 'by', 'these', 'objects', 'shoc... | [-0.0788430251120198, 0.16510850236002872, -0.062458054232193486, 0.11766364134219258, -0.05285288591729912, -0.06012232897576885, 0.0513472289639029, 0.4373032471391364, -0.2011378034862263, -0.3165696257400048, 0.06387171691945084, -0.2945228413620634, 0.0012782451622710329, 0.2059573740393759, 0.0036680594970097888,... |
708.0086 | Neutron star cooling after deep crustal heating in the X-ray transient
KS 1731-260 | We simulate the cooling of the neutron star in the X-ray transient KS
1731-260 after the source returned to quiescence in 2001 from a long (>~ 12.5
yr) outburst state. We show that the cooling can be explained assuming that the
crust underwent deep heating during the outburst stage. In our best theoretical
scenario t... | astro-ph | we simulate the cooling of the neutron star in the xray transient ks 1731260 after the source returned to quiescence in 2001 from a long 125 yr outburst state we show that the cooling can be explained assuming that the crust underwent deep heating during the outburst stage in our best theoretical scenario the neutron s... | [['we', 'simulate', 'the', 'cooling', 'of', 'the', 'neutron', 'star', 'in', 'the', 'xray', 'transient', 'ks', '1731260', 'after', 'the', 'source', 'returned', 'to', 'quiescence', 'in', '2001', 'from', 'a', 'long', '125', 'yr', 'outburst', 'state', 'we', 'show', 'that', 'the', 'cooling', 'can', 'be', 'explained', 'assum... | [-0.04112561099530979, 0.20062837592358218, -0.13807363791562532, 0.05957459510255862, -0.09290438061365965, -0.03685151752427049, 0.0924031645402141, 0.41565098270945167, -0.2511719859622676, -0.2831890834843333, 0.11754632080589346, -0.2704434508200863, 0.0071332287712386625, 0.2172764784003469, -0.044384695517284606... |
708.0087 | Quantum toboggans with two branch points | Wave functions describing quantum toboggans with two branch points (QT2) are
defined along complex contours of coordinates which spiral around these branch
points. The classification of QT2 is found in terms of certain ``winding
descriptors" $\varrho$. A mapping $x^{(\varrho)}(s) \to y^{(0)}(s)$ is then
presented whi... | quant-ph | wave functions describing quantum toboggans with two branch points qt2 are defined along complex contours of coordinates which spiral around these branch points the classification of qt2 is found in terms of certain winding descriptors varrho a mapping xvarrhos to y0s is then presented which rectifies the contours for ... | [['wave', 'functions', 'describing', 'quantum', 'toboggans', 'with', 'two', 'branch', 'points', 'qt2', 'are', 'defined', 'along', 'complex', 'contours', 'of', 'coordinates', 'which', 'spiral', 'around', 'these', 'branch', 'points', 'the', 'classification', 'of', 'qt2', 'is', 'found', 'in', 'terms', 'of', 'certain', 'wi... | [-0.20089211239694402, 0.07329426820461567, -0.06351456764297417, 0.030370965550761096, -0.048900647626186795, -0.096223398971443, 0.025060212754536994, 0.3155811141388348, -0.23097060689514576, -0.21973757143132389, 0.07870085075130472, -0.2929007513448596, -0.18695865899252778, 0.19171359189427817, -0.045146140878876... |
708.0088 | Magneto-gyrotropic photogalvanic effects due to inter-subband absorption
in quantum wells | We report on the observation of the magneto-photogalvanic effect (MPGE) due
to inter-subband transitions in (001)-oriented GaAs quantum wells. This effect
is related to the gyrotropic properties of the structures. It is shown that
inter-subband absorption of linearly polarized radiation may lead to
spin-related as we... | cond-mat.mtrl-sci | we report on the observation of the magnetophotogalvanic effect mpge due to intersubband transitions in 001oriented gaas quantum wells this effect is related to the gyrotropic properties of the structures it is shown that intersubband absorption of linearly polarized radiation may lead to spinrelated as well as spin in... | [['we', 'report', 'on', 'the', 'observation', 'of', 'the', 'magnetophotogalvanic', 'effect', 'mpge', 'due', 'to', 'intersubband', 'transitions', 'in', '001oriented', 'gaas', 'quantum', 'wells', 'this', 'effect', 'is', 'related', 'to', 'the', 'gyrotropic', 'properties', 'of', 'the', 'structures', 'it', 'is', 'shown', 't... | [-0.12559397033602762, 0.1967349360539763, -0.04381046370893228, 0.041381145333184204, -0.07469046318552411, -0.12465821227562598, 0.0400073748705985, 0.45618675675121, -0.25613936540655424, -0.27821138252687383, 0.027214777028020165, -0.2708134310640639, -0.16154194173792408, 0.23904670899940014, 0.013378626399780394,... |
708.0089 | Discussion of "2004 IMS Medallion Lecture: Local Rademacher complexities
and oracle inequalities in risk minimization" by V. Koltchinskii | Discussion of "2004 IMS Medallion Lecture: Local Rademacher complexities and
oracle inequalities in risk minimization" by V. Koltchinskii [arXiv:0708.0083]
| q-fin.RM math.ST stat.TH | discussion of 2004 ims medallion lecture local rademacher complexities and oracle inequalities in risk minimization by v koltchinskii arxiv07080083 | [['discussion', 'of', '2004', 'ims', 'medallion', 'lecture', 'local', 'rademacher', 'complexities', 'and', 'oracle', 'inequalities', 'in', 'risk', 'minimization', 'by', 'v', 'koltchinskii', 'arxiv07080083']] | [-0.04620913315662428, -0.01606457386361925, -0.05329715259569256, 0.19175361194892934, -0.0260421199062349, -0.26058023275905534, 0.20598403261484285, 0.24738681237948568, -0.251077052303835, -0.3320668751471921, 0.1784132805983781, -0.32687197998166084, -0.13523328931708084, 0.12226964003945652, -0.32103299344644737,... |
708.009 | Soret Motion of a Charged Spherical Colloid | The thermophoretic motion of a charged spherical colloidal particle and its
accompanying cloud of counterions and co-ions in a temperature gradient is
studied theoretically. Using the Debye-Huckel approximation, the Soret drift
velocity of a weakly charged colloid is calculated analytically. For highly
charged colloi... | cond-mat.soft cond-mat.mtrl-sci cond-mat.stat-mech | the thermophoretic motion of a charged spherical colloidal particle and its accompanying cloud of counterions and coions in a temperature gradient is studied theoretically using the debyehuckel approximation the soret drift velocity of a weakly charged colloid is calculated analytically for highly charged colloids the ... | [['the', 'thermophoretic', 'motion', 'of', 'a', 'charged', 'spherical', 'colloidal', 'particle', 'and', 'its', 'accompanying', 'cloud', 'of', 'counterions', 'and', 'coions', 'in', 'a', 'temperature', 'gradient', 'is', 'studied', 'theoretically', 'using', 'the', 'debyehuckel', 'approximation', 'the', 'soret', 'drift', '... | [-0.11747425330035827, 0.20819536124849145, -0.05786622924839749, 0.02773695830392706, 0.0112889629405211, -0.17355936634189942, -0.032716584304238065, 0.3899589531561908, -0.22156267265843996, -0.2897804474019829, 0.012212403943104778, -0.31723010193090884, -0.12457845021477516, 0.1712207762264263, 0.00289903611204970... |
708.0091 | A useful correspondence between fluid convection and ecosystem operation | Both ecological systems and convective fluid systems are examples of open
systems which operate far-from-equilibrium. This article demonstrates that
there is a correspondence between a resource-consumer chemostat ecosystem and
the Rayleigh-Benard (RB) convective fluid system. The Lorenz dynamics of the RB
system can ... | physics.flu-dyn physics.bio-ph | both ecological systems and convective fluid systems are examples of open systems which operate farfromequilibrium this article demonstrates that there is a correspondence between a resourceconsumer chemostat ecosystem and the rayleighbenard rb convective fluid system the lorenz dynamics of the rb system can be transla... | [['both', 'ecological', 'systems', 'and', 'convective', 'fluid', 'systems', 'are', 'examples', 'of', 'open', 'systems', 'which', 'operate', 'farfromequilibrium', 'this', 'article', 'demonstrates', 'that', 'there', 'is', 'a', 'correspondence', 'between', 'a', 'resourceconsumer', 'chemostat', 'ecosystem', 'and', 'the', '... | [-0.14177401773610596, 0.1673846803407598, -0.11391597210328926, 0.11930626389981659, -0.04317160398774856, -0.15927094239678635, 0.02869854420255702, 0.28286094749598084, -0.28435899760062294, -0.27774263359606266, 0.08014629159944954, -0.23765296532420088, -0.2451963694514455, 0.19417181315093493, -0.0980400232879260... |
708.0092 | Fluctuations of a weakly interacting Bose-Einstein condensate | Fluctuations of the number of condensed atoms in a finite-size, weakly
interacting Bose gas confined in a box potential are investigated for
temperatures up to the critical region. The canonical partition functions are
evaluated using a recursive scheme for smaller systems, and a saddle-point
approximation for larger... | cond-mat.stat-mech | fluctuations of the number of condensed atoms in a finitesize weakly interacting bose gas confined in a box potential are investigated for temperatures up to the critical region the canonical partition functions are evaluated using a recursive scheme for smaller systems and a saddlepoint approximation for larger sample... | [['fluctuations', 'of', 'the', 'number', 'of', 'condensed', 'atoms', 'in', 'a', 'finitesize', 'weakly', 'interacting', 'bose', 'gas', 'confined', 'in', 'a', 'box', 'potential', 'are', 'investigated', 'for', 'temperatures', 'up', 'to', 'the', 'critical', 'region', 'the', 'canonical', 'partition', 'functions', 'are', 'ev... | [-0.12335817273387442, 0.20045240405422177, -0.054479099859091794, 0.0946378676296537, 0.06194224032492096, -0.11692773262851887, 0.0796744031351178, 0.30881004797900835, -0.21456649093075641, -0.2910034544765949, -0.0022944118522684135, -0.34484038145906415, -0.05379534828927486, 0.16930509767391616, 0.083356314606221... |
708.0093 | Note sur la d\'etermination alg\'ebrique du groupe fondamental
pro-r\'esoluble d'une courbe affine | Let X be a smooth projective algebraic curve of genus g minus $r\geq 1$
points defined over an algebraically closed field k of characteristic $p\geq
0$. The structure of the largest prime to p quotient of the \'etale fundamental
group is well known by transcendental methods : it is isomorphic to the largest
prime to ... | math.AG math.NT | let x be a smooth projective algebraic curve of genus g minus rgeq 1 points defined over an algebraically closed field k of characteristic pgeq 0 the structure of the largest prime to p quotient of the etale fundamental group is well known by transcendental methods it is isomorphic to the largest prime to p quotient of... | [['let', 'x', 'be', 'a', 'smooth', 'projective', 'algebraic', 'curve', 'of', 'genus', 'g', 'minus', 'rgeq', '1', 'points', 'defined', 'over', 'an', 'algebraically', 'closed', 'field', 'k', 'of', 'characteristic', 'pgeq', '0', 'the', 'structure', 'of', 'the', 'largest', 'prime', 'to', 'p', 'quotient', 'of', 'the', 'etal... | [-0.2517623876743268, 0.07795482008025699, -0.13091784548790505, 0.05630274625963509, -0.10857882793615795, -0.13821501112986534, -0.025712711703298346, 0.32446312048428116, -0.4010494074651173, -0.2255759649422197, 0.04799464629918691, -0.2654222125752962, -0.0880011350991914, 0.2616119858520549, -0.13663961467820973,... |
708.0094 | Discussion of ``2004 IMS Medallion Lecture: Local Rademacher
complexities and oracle inequalities in risk minimization'' by V.
Koltchinskii | Discussion of ``2004 IMS Medallion Lecture: Local Rademacher complexities and
oracle inequalities in risk minimization'' by V. Koltchinskii [arXiv:0708.0083]
| math.ST stat.TH | discussion of 2004 ims medallion lecture local rademacher complexities and oracle inequalities in risk minimization by v koltchinskii arxiv07080083 | [['discussion', 'of', '2004', 'ims', 'medallion', 'lecture', 'local', 'rademacher', 'complexities', 'and', 'oracle', 'inequalities', 'in', 'risk', 'minimization', 'by', 'v', 'koltchinskii', 'arxiv07080083']] | [-0.04620913315662428, -0.01606457386361925, -0.05329715259569256, 0.19175361194892934, -0.0260421199062349, -0.26058023275905534, 0.20598403261484285, 0.24738681237948568, -0.251077052303835, -0.3320668751471921, 0.1784132805983781, -0.32687197998166084, -0.13523328931708084, 0.12226964003945652, -0.32103299344644737,... |
708.0095 | Solving the cosmic lithium problems with primordial late-decaying
particles | We investigate the modifications to predictions for the abundances of light
elements from standard Big-Bang nucleosynthesis when exotic late-decaying
particles with lifetimes exceeding ~1 sec are prominent in the early Universe.
Utilising a model-independent analysis of the properties of these long-lived
particles, w... | astro-ph hep-ph | we investigate the modifications to predictions for the abundances of light elements from standard bigbang nucleosynthesis when exotic latedecaying particles with lifetimes exceeding 1 sec are prominent in the early universe utilising a modelindependent analysis of the properties of these longlived particles we identif... | [['we', 'investigate', 'the', 'modifications', 'to', 'predictions', 'for', 'the', 'abundances', 'of', 'light', 'elements', 'from', 'standard', 'bigbang', 'nucleosynthesis', 'when', 'exotic', 'latedecaying', 'particles', 'with', 'lifetimes', 'exceeding', '1', 'sec', 'are', 'prominent', 'in', 'the', 'early', 'universe', ... | [-0.01881189751561339, 0.20349996296786949, -0.05254413792863488, 0.1403024925507213, -0.02298581341624652, -0.11578995062307895, 0.025825938258908297, 0.35042591265549783, -0.19466699077747762, -0.35616977004285316, 0.06875162088085505, -0.33702998150042013, 0.017628042152960245, 0.17910297286059512, -0.00460432201476... |
708.0096 | Abundances on the Main Sequence of Omega Centauri | Abundance ratios of carbon, nitrogen and strontium relative to iron,
calculated using spectrum synthesis techniques, are given for a sample of main
sequence and turnoff stars that belong to the globular cluster omega Centauri.
The variations of carbon, nitrogen and/or strontium show several different
abundance patter... | astro-ph | abundance ratios of carbon nitrogen and strontium relative to iron calculated using spectrum synthesis techniques are given for a sample of main sequence and turnoff stars that belong to the globular cluster omega centauri the variations of carbon nitrogen andor strontium show several different abundance patterns as a ... | [['abundance', 'ratios', 'of', 'carbon', 'nitrogen', 'and', 'strontium', 'relative', 'to', 'iron', 'calculated', 'using', 'spectrum', 'synthesis', 'techniques', 'are', 'given', 'for', 'a', 'sample', 'of', 'main', 'sequence', 'and', 'turnoff', 'stars', 'that', 'belong', 'to', 'the', 'globular', 'cluster', 'omega', 'cent... | [-0.01957656964412437, 0.20973414579093191, -0.013276961736125558, 0.07291421567633814, -0.005800766998127235, -0.06676274946420989, 0.13774825440641428, 0.44028222432310604, -0.16726876050388376, -0.4111083504574917, -0.01570313501035778, -0.2992769419339246, 0.029618233087909434, 0.15323265595155547, -0.0740136817855... |
708.0097 | SDSS J150722.30+523039.8: a CV formed directly from a detached white
dwarf/brown dwarf binary? | We present high-speed, three-colour photometry of the eclipsing cataclysmic
variable SDSS J150722.30+523039.8 (hereafter SDSS J1507). This system has an
orbital period of 66.61 minutes, placing it below the observed ``period
minimum'' for cataclysmic variables. We determine the system parameters via a
parameterised m... | astro-ph | we present highspeed threecolour photometry of the eclipsing cataclysmic variable sdss j150722305230398 hereafter sdss j1507 this system has an orbital period of 6661 minutes placing it below the observed period minimum for cataclysmic variables we determine the system parameters via a parameterised model of the eclips... | [['we', 'present', 'highspeed', 'threecolour', 'photometry', 'of', 'the', 'eclipsing', 'cataclysmic', 'variable', 'sdss', 'j150722305230398', 'hereafter', 'sdss', 'j1507', 'this', 'system', 'has', 'an', 'orbital', 'period', 'of', '6661', 'minutes', 'placing', 'it', 'below', 'the', 'observed', 'period', 'minimum', 'for'... | [-0.12583365273099836, 0.1544337808689162, -0.04698623705523023, 0.09163046160472828, -0.11753705137159003, -0.12194294115068957, 0.10658181776571608, 0.35952234337832534, -0.20047678878030326, -0.35234238359962267, 0.07705350651811924, -0.31755235333955695, -0.03684067286423814, 0.18752658228432997, -0.095683557953734... |
708.0098 | Discussion of ``2004 IMS Medallion Lecture: Local Rademacher
complexities and oracle inequalities in risk minimization'' by V.
Koltchinskii | Discussion of ``2004 IMS Medallion Lecture: Local Rademacher complexities and
oracle inequalities in risk minimization'' by V. Koltchinskii [arXiv:0708.0083]
| q-fin.RM math.ST stat.TH | discussion of 2004 ims medallion lecture local rademacher complexities and oracle inequalities in risk minimization by v koltchinskii arxiv07080083 | [['discussion', 'of', '2004', 'ims', 'medallion', 'lecture', 'local', 'rademacher', 'complexities', 'and', 'oracle', 'inequalities', 'in', 'risk', 'minimization', 'by', 'v', 'koltchinskii', 'arxiv07080083']] | [-0.04620913315662428, -0.01606457386361925, -0.05329715259569256, 0.19175361194892934, -0.0260421199062349, -0.26058023275905534, 0.20598403261484285, 0.24738681237948568, -0.251077052303835, -0.3320668751471921, 0.1784132805983781, -0.32687197998166084, -0.13523328931708084, 0.12226964003945652, -0.32103299344644737,... |
708.0099 | On the well-posedness for the Ideal MHD equations in the
Triebel-Lizorkin spaces | In this paper, we prove the local well-posedness for the Ideal MHD equations
in the Triebel-Lizorkin spaces and obtain blow-up criterion of smooth
solutions. Specially, we fill a gap in a step of the proof of the local
well-posedness part for the incompressible Euler equation in \cite{Chae1}.
| math.AP math-ph math.MP | in this paper we prove the local wellposedness for the ideal mhd equations in the triebellizorkin spaces and obtain blowup criterion of smooth solutions specially we fill a gap in a step of the proof of the local wellposedness part for the incompressible euler equation in citechae1 | [['in', 'this', 'paper', 'we', 'prove', 'the', 'local', 'wellposedness', 'for', 'the', 'ideal', 'mhd', 'equations', 'in', 'the', 'triebellizorkin', 'spaces', 'and', 'obtain', 'blowup', 'criterion', 'of', 'smooth', 'solutions', 'specially', 'we', 'fill', 'a', 'gap', 'in', 'a', 'step', 'of', 'the', 'proof', 'of', 'the', ... | [-0.17057350188817666, -0.01224298453029326, -0.12361405255353969, 0.12304611472443314, -0.03996510001952234, -0.06212133644958553, -0.03608662584219533, 0.22283311253008636, -0.32726501932610635, -0.1945339746206351, 0.14796042963659958, -0.22083335778291296, -0.0992509662527996, 0.1489148432307917, -0.076763252828918... |
708.01 | Gamma-ray and neutrino diffuse emissions of the Galaxy above the TeV | In this contribution we will discuss recent results concerning the intensity
and the angular distribution of the gamma-ray and neutrino emissions as should
be originated from the hadronic scattering of cosmic rays (CR) with the
interstellar medium (ISM). We assumed that CR sources are supernova remnants
(SNR) and est... | astro-ph | in this contribution we will discuss recent results concerning the intensity and the angular distribution of the gammaray and neutrino emissions as should be originated from the hadronic scattering of cosmic rays cr with the interstellar medium ism we assumed that cr sources are supernova remnants snr and estimated the... | [['in', 'this', 'contribution', 'we', 'will', 'discuss', 'recent', 'results', 'concerning', 'the', 'intensity', 'and', 'the', 'angular', 'distribution', 'of', 'the', 'gammaray', 'and', 'neutrino', 'emissions', 'as', 'should', 'be', 'originated', 'from', 'the', 'hadronic', 'scattering', 'of', 'cosmic', 'rays', 'cr', 'wi... | [-0.03655245767979167, 0.16361296412908807, -0.02675358793970679, 0.1348013725950617, -0.055696428275103266, -0.030447331516921115, 0.008081813260507421, 0.40749061422511224, -0.2208726624609763, -0.30543725120203036, 0.02079947277995422, -0.33836686087860945, -0.03426720398687282, 0.2149513817240237, 0.035192747435652... |
708.0101 | Radiative and interelectronic-interaction corrections to the hyperfine
splitting in highly charged B-like ions | The ground-state hyperfine splitting values of high-Z boronlike ions are
calculated. Calculation of the interelectronic-interaction contribution is
based on a combination of the 1/Z perturbation theory and the large-scale
configuration-interaction Dirac-Fock-Sturm method. The screened QED corrections
are evaluated ut... | physics.atom-ph | the groundstate hyperfine splitting values of highz boronlike ions are calculated calculation of the interelectronicinteraction contribution is based on a combination of the 1z perturbation theory and the largescale configurationinteraction diracfocksturm method the screened qed corrections are evaluated utilizing an e... | [['the', 'groundstate', 'hyperfine', 'splitting', 'values', 'of', 'highz', 'boronlike', 'ions', 'are', 'calculated', 'calculation', 'of', 'the', 'interelectronicinteraction', 'contribution', 'is', 'based', 'on', 'a', 'combination', 'of', 'the', '1z', 'perturbation', 'theory', 'and', 'the', 'largescale', 'configurationi... | [-0.05182395706919354, 0.14596132408635526, 0.024245443561210715, 0.10329972997163261, 0.029340225799094843, -0.07524881331014564, 0.02882267921044352, 0.37201488309208003, -0.15783864448660578, -0.3220623304944314, -0.024447564742174643, -0.3137589931272602, -0.018115625716745853, 0.18297864759980498, 0.10382351246073... |
708.0102 | Constraint Algorithm for Extremals in Optimal Control Problems | A geometric method is described to characterize the different kinds of
extremals in optimal control theory. This comes from the use of a presymplectic
constraint algorithm starting from the necessary conditions given by
Pontryagin's Maximum Principle. Apart from the design of this general algorithm
useful for any opt... | math.OC math-ph math.MP | a geometric method is described to characterize the different kinds of extremals in optimal control theory this comes from the use of a presymplectic constraint algorithm starting from the necessary conditions given by pontryagins maximum principle apart from the design of this general algorithm useful for any optimal ... | [['a', 'geometric', 'method', 'is', 'described', 'to', 'characterize', 'the', 'different', 'kinds', 'of', 'extremals', 'in', 'optimal', 'control', 'theory', 'this', 'comes', 'from', 'the', 'use', 'of', 'a', 'presymplectic', 'constraint', 'algorithm', 'starting', 'from', 'the', 'necessary', 'conditions', 'given', 'by', ... | [-0.11135900660883635, 0.012628979799566358, -0.10030879787657232, 0.09328075488502648, -0.09342237058860649, -0.1587573039134787, 0.07863348968731727, 0.3240471171503443, -0.32848354985582684, -0.30627292299288367, 0.1349114866821938, -0.19945887878670224, -0.20010810456283035, 0.23137409878628595, -0.1528870601850074... |
708.0103 | Time-dependent magnetotransport of a wave packet in a quantum wire with
embedded quantum dots | We consider wave packet propagation in a quantum wire with either an embedded
antidot or an embedded parallel double open quantum dot under the influence of
a uniform magnetic field. The magnetoconductance and the time evolution of an
electron wave packet are calculated based on the Lippmann-Schwinger formalism.
This... | cond-mat.mes-hall | we consider wave packet propagation in a quantum wire with either an embedded antidot or an embedded parallel double open quantum dot under the influence of a uniform magnetic field the magnetoconductance and the time evolution of an electron wave packet are calculated based on the lippmannschwinger formalism this appr... | [['we', 'consider', 'wave', 'packet', 'propagation', 'in', 'a', 'quantum', 'wire', 'with', 'either', 'an', 'embedded', 'antidot', 'or', 'an', 'embedded', 'parallel', 'double', 'open', 'quantum', 'dot', 'under', 'the', 'influence', 'of', 'a', 'uniform', 'magnetic', 'field', 'the', 'magnetoconductance', 'and', 'the', 'ti... | [-0.22821545501651821, 0.16373791951305885, -0.05587031780436757, 0.043597374255501774, 0.008457468509613002, -0.11832732929023684, 0.034494180592983106, 0.38473923342516186, -0.25949935694454146, -0.2548530108932803, 0.026068075851071626, -0.27491404085821325, -0.1294071127137658, 0.20232012293293888, 0.07240465191024... |
708.0104 | Solutions to the nonlinear Schroedinger equation carrying momentum along
a curve. Part II: proof of the existence result | We prove existence of a special class of solutions to the (elliptic)
Nonlinear Schroedinger Equation $- \epsilon^2 \Delta \psi + V(x) \psi =
|\psi|^{p-1} \psi$ on a manifold or in the Euclidean space. Here V represents
the potential, p is an exponent greater than 1 and $\epsilon$ a small parameter
corresponding to th... | math.AP | we prove existence of a special class of solutions to the elliptic nonlinear schroedinger equation epsilon2 delta psi vx psi psip1 psi on a manifold or in the euclidean space here v represents the potential p is an exponent greater than 1 and epsilon a small parameter corresponding to the planck constant as epsilon ten... | [['we', 'prove', 'existence', 'of', 'a', 'special', 'class', 'of', 'solutions', 'to', 'the', 'elliptic', 'nonlinear', 'schroedinger', 'equation', 'epsilon2', 'delta', 'psi', 'vx', 'psi', 'psip1', 'psi', 'on', 'a', 'manifold', 'or', 'in', 'the', 'euclidean', 'space', 'here', 'v', 'represents', 'the', 'potential', 'p', '... | [-0.1919036814380951, 0.08333218965595608, -0.08223516930793894, 0.041494785083441774, -0.07777107792659582, -0.13554808205587726, 0.03438442583288195, 0.28600727739454856, -0.2590649926850315, -0.22227515013695792, 0.08422787697054446, -0.3060222642179097, -0.12539108971671747, 0.18428135708030635, -0.0275514302815407... |
708.0105 | Kinematical Constraints on QCD Factorization in the Drell-Yan Process | We study factorization schemes for parton shower models in hadron-hadron
collisions. As an example, we calculate lepton pair production mediated by a
virtual photon in quark--anti-quark annihilation, and we compare factorized
cross sections obtained in the conventional $\bar{\rm MS}$ scheme with those
obtained in a f... | hep-ph | we study factorization schemes for parton shower models in hadronhadron collisions as an example we calculate lepton pair production mediated by a virtual photon in quarkantiquark annihilation and we compare factorized cross sections obtained in the conventional barrm ms scheme with those obtained in a factorization sc... | [['we', 'study', 'factorization', 'schemes', 'for', 'parton', 'shower', 'models', 'in', 'hadronhadron', 'collisions', 'as', 'an', 'example', 'we', 'calculate', 'lepton', 'pair', 'production', 'mediated', 'by', 'a', 'virtual', 'photon', 'in', 'quarkantiquark', 'annihilation', 'and', 'we', 'compare', 'factorized', 'cross... | [-0.0786093358457198, 0.1689984232740672, -0.1636530507958549, 0.20797169372364058, 0.014847455433268538, -0.06221870402120711, -0.0395957023891456, 0.418174946516314, -0.18803104718544467, -0.20659303451504776, -0.1031037421147202, -0.2818595266709214, 0.03538840722895282, 0.15063931135570302, 0.07646335537463207, 0.0... |
708.0106 | An evolutionary study of the pulsating subdwarf B eclipsing binary
PG1336-018 (NY Vir) | The formation of subdwarf B (sdB) stars is not well understood within the
current framework of stellar single and binary evolution. In this study, we
focus on the formation and evolution of the pulsating sdB star in the very
short-period eclipsing binary PG1336-018. We aim at refining the formation
scenario of this u... | astro-ph | the formation of subdwarf b sdb stars is not well understood within the current framework of stellar single and binary evolution in this study we focus on the formation and evolution of the pulsating sdb star in the very shortperiod eclipsing binary pg1336018 we aim at refining the formation scenario of this unique sys... | [['the', 'formation', 'of', 'subdwarf', 'b', 'sdb', 'stars', 'is', 'not', 'well', 'understood', 'within', 'the', 'current', 'framework', 'of', 'stellar', 'single', 'and', 'binary', 'evolution', 'in', 'this', 'study', 'we', 'focus', 'on', 'the', 'formation', 'and', 'evolution', 'of', 'the', 'pulsating', 'sdb', 'star', '... | [-0.09043590151748368, 0.16105663555596192, -0.06975823920764133, 0.11375646934807562, -0.11638450862352397, -0.062189445204197245, 0.08358981422905888, 0.35750369772001683, -0.14782977105111805, -0.3393071558235091, 0.05010818002966372, -0.25204170225884454, -0.06430355007716707, 0.18830831958689273, -0.07409947460286... |
708.0107 | Magnetized String Cosmological Model in Cylindrically Symmetric
Inhomogeneous Universe with Variable Cosmological-Term $\Lambda$ | Cylindrically symmetric inhomogeneous magnetized string cosmological model is
investigated with cosmological term $\Lambda$ varying with time. To get the
deterministic solution, it has been assumed that the expansion ($\theta$) in
the model is proportional to the eigenvalue $\sigma^{1}_{1}$ of the shear
tensor $\sigm... | gr-qc | cylindrically symmetric inhomogeneous magnetized string cosmological model is investigated with cosmological term lambda varying with time to get the deterministic solution it has been assumed that the expansion theta in the model is proportional to the eigenvalue sigma1_1 of the shear tensor sigmai_j the value of cosm... | [['cylindrically', 'symmetric', 'inhomogeneous', 'magnetized', 'string', 'cosmological', 'model', 'is', 'investigated', 'with', 'cosmological', 'term', 'lambda', 'varying', 'with', 'time', 'to', 'get', 'the', 'deterministic', 'solution', 'it', 'has', 'been', 'assumed', 'that', 'the', 'expansion', 'theta', 'in', 'the', ... | [-0.13155595806622228, 0.12825881544132392, -0.04864258920708888, 0.03344111980025678, -0.10785221150361521, -0.13606682328810527, -0.0631160788281366, 0.3460867076700683, -0.26224570459318025, -0.27950288043465726, 0.11071660051522993, -0.26055495119328764, -0.10081988400887958, 0.14732757885398906, 0.0282915346513111... |
708.0108 | Geometric construction of metaplectic covers of $\GL_{n}$ in
characteristic zero | This paper presents a new construction of the m-fold metaplectic cover of
$\GL_{n}$ over an algebraic number field k, where k contains a primitive m-th
root of unity. A 2-cocycle on $\GL_{n}(\A)$ representing this extension is
given and the splitting of the cocycle on $\GL_{n}(k)$ is found explicitly. The
cocycle is ... | math.NT | this paper presents a new construction of the mfold metaplectic cover of gl_n over an algebraic number field k where k contains a primitive mth root of unity a 2cocycle on gl_na representing this extension is given and the splitting of the cocycle on gl_nk is found explicitly the cocycle is smooth at almost all places ... | [['this', 'paper', 'presents', 'a', 'new', 'construction', 'of', 'the', 'mfold', 'metaplectic', 'cover', 'of', 'gl_n', 'over', 'an', 'algebraic', 'number', 'field', 'k', 'where', 'k', 'contains', 'a', 'primitive', 'mth', 'root', 'of', 'unity', 'a', '2cocycle', 'on', 'gl_na', 'representing', 'this', 'extension', 'is', '... | [-0.22308942969896617, 0.07538999634115291, -0.0956986535365056, 0.01335989460737134, -0.11358936882594176, -0.12516353583665923, 0.03048607482056117, 0.2544438344050656, -0.3072130331083348, -0.2563441345085729, 0.07616324210743698, -0.21525716640334985, -0.1580073577433563, 0.2547588573785074, -0.11193250837580611, -... |
708.0109 | Principal values for Riesz transforms and rectifiability | Let $E\subset R^d$ with $H^n(E)<\infty$, where H^n stands for the
$n$-dimensional Hausdorff measure. In this paper we prove that E is
n-rectifiable if and only if the limit $$\lim_{\ve\to0}\int_{y\in E:|x-y|>\ve}
\frac{x-y}{|x-y|^{n+1}} dH^n(y)$$ exists H^n-almost everywhere in E. To prove
this result we obtain preci... | math.CA math.FA | let esubset rd with hneinfty where hn stands for the ndimensional hausdorff measure in this paper we prove that e is nrectifiable if and only if the limit lim_veto0int_yin exyve fracxyxyn1 dhny exists hnalmost everywhere in e to prove this result we obtain precise estimates from above and from below for the l2 norm of ... | [['let', 'esubset', 'rd', 'with', 'hneinfty', 'where', 'hn', 'stands', 'for', 'the', 'ndimensional', 'hausdorff', 'measure', 'in', 'this', 'paper', 'we', 'prove', 'that', 'e', 'is', 'nrectifiable', 'if', 'and', 'only', 'if', 'the', 'limit', 'lim_veto0int_yin', 'exyve', 'fracxyxyn1', 'dhny', 'exists', 'hnalmost', 'every... | [-0.08919391353967888, 0.10296583764961567, -0.05572865582683429, 0.0405979857776025, -0.02557936203987177, -0.11509097434965701, 0.033014678908110565, 0.34710494505948036, -0.2976205406694448, -0.1350333663024779, 0.12533779130397557, -0.3661282331971773, -0.08535814876587869, 0.20614560062451096, -0.14704154304164493... |
708.011 | Metropolis simulations of the manipulation of DNA strands in solution | This paper has been withdrawn by the authors.
| cond-mat.soft cond-mat.other | this paper has been withdrawn by the authors | [['this', 'paper', 'has', 'been', 'withdrawn', 'by', 'the', 'authors']] | [-0.10261085256934166, -0.04523250472266227, -0.18098232802003622, -0.15798902076494414, -0.15956164104864, -0.009353606728836894, -0.059683346524252556, 0.36475658789277077, -0.23344220919534564, -0.37511192448437214, 0.12130584195256233, -0.35290066339075565, -0.17170235351659358, -0.01896117883734405, -0.36158941220... |
708.0111 | Fluctuating semiflexible polymer ribbon constrained to a ring | Twist stiffness and an asymmetric bending stiffness of a polymer or a polymer
bundle is captured by the elastic ribbon model. We investigate the effects a
ring geometry induces to a thermally fluctuating ribbon, finding bend-bend
coupling in addition to twist-bend coupling. Furthermore, due to the geometric
constrain... | q-bio.BM cond-mat.soft | twist stiffness and an asymmetric bending stiffness of a polymer or a polymer bundle is captured by the elastic ribbon model we investigate the effects a ring geometry induces to a thermally fluctuating ribbon finding bendbend coupling in addition to twistbend coupling furthermore due to the geometric constraint the po... | [['twist', 'stiffness', 'and', 'an', 'asymmetric', 'bending', 'stiffness', 'of', 'a', 'polymer', 'or', 'a', 'polymer', 'bundle', 'is', 'captured', 'by', 'the', 'elastic', 'ribbon', 'model', 'we', 'investigate', 'the', 'effects', 'a', 'ring', 'geometry', 'induces', 'to', 'a', 'thermally', 'fluctuating', 'ribbon', 'findi... | [-0.19465624049127578, 0.19115931998540156, -0.06931585762303005, -0.0025902453307161464, -0.07096479386289387, -0.1827462615960456, -0.021378979304845027, 0.41578001600313697, -0.30995655301562014, -0.268601831019004, 0.05191888345871121, -0.2265899229752633, -0.15495190036512832, 0.11579872261574294, -0.0104272201367... |
708.0112 | Suppressing noise-induced intensity pulsations in semiconductor lasers
by means of time-delayed feedback | We investigate the possibility to suppress noise-induced intensity pulsations
(relaxation oscillations) in semiconductor lasers by means of a time-delayed
feedback control scheme. This idea is first studied in a generic normal form
model, where we derive an analytic expression for the mean amplitude of the
oscillatio... | nlin.CD | we investigate the possibility to suppress noiseinduced intensity pulsations relaxation oscillations in semiconductor lasers by means of a timedelayed feedback control scheme this idea is first studied in a generic normal form model where we derive an analytic expression for the mean amplitude of the oscillations and d... | [['we', 'investigate', 'the', 'possibility', 'to', 'suppress', 'noiseinduced', 'intensity', 'pulsations', 'relaxation', 'oscillations', 'in', 'semiconductor', 'lasers', 'by', 'means', 'of', 'a', 'timedelayed', 'feedback', 'control', 'scheme', 'this', 'idea', 'is', 'first', 'studied', 'in', 'a', 'generic', 'normal', 'fo... | [-0.15625169462966484, 0.19099531917813595, -0.07515002765316278, 0.07258464932005773, -0.027112787128723365, -0.17999233517478755, 0.07981482907470831, 0.40193287510068176, -0.3142847330606681, -0.25510643163022206, 0.0722757151828425, -0.19724884582064214, -0.21924005997704066, 0.24866510140759118, -0.019138957152113... |
708.0113 | Constraints on Dissipative Non-Equilibrium Dark Energy Models from
Recent Supernova Data | Non-critical string cosmologies may be viewed as the analogue of
off-equilibrium models arising within string theory as a result of a cosmically
catastrophic event in the early Universe. Such models entail relaxing-to-zero
dark energies provided by a rolling dilaton field at late times. We discuss
fits of such non-cr... | astro-ph gr-qc hep-th | noncritical string cosmologies may be viewed as the analogue of offequilibrium models arising within string theory as a result of a cosmically catastrophic event in the early universe such models entail relaxingtozero dark energies provided by a rolling dilaton field at late times we discuss fits of such noncritical mo... | [['noncritical', 'string', 'cosmologies', 'may', 'be', 'viewed', 'as', 'the', 'analogue', 'of', 'offequilibrium', 'models', 'arising', 'within', 'string', 'theory', 'as', 'a', 'result', 'of', 'a', 'cosmically', 'catastrophic', 'event', 'in', 'the', 'early', 'universe', 'such', 'models', 'entail', 'relaxingtozero', 'dar... | [-0.08819176399642054, 0.16239402953206616, -0.13487071323153726, 0.1587138474206714, -0.06426125312333598, -0.14515047977294993, -0.023917754866894993, 0.27590506863506403, -0.1949186424834325, -0.33342406285159726, 0.0936950110761887, -0.2632806185523377, -0.07981839589774609, 0.1850060396389488, -0.00950433755411615... |
708.0114 | Shintani Cocycles on $\GL_{n}$ | The aim of this paper is to define an n-1-cocycle $\sigma$ on $\GL_{n}(\Q)$
with values in a certain space $\hD$ of distributions on
$\A_f^{n}\setminus\{0\}$. Here $\A_f$ denotes the ring of finite ad\`{e}les of
$\Q$, and the distributions take values in the Laurent series
$\C((z_{1},...,z_{n}))$. This cocycle can be... | math.NT | the aim of this paper is to define an n1cocycle sigma on gl_nq with values in a certain space hd of distributions on a_fnsetminus0 here a_f denotes the ring of finite adeles of q and the distributions take values in the laurent series cz_1z_n this cocycle can be used to evaluate special values of artin lfunctions on nu... | [['the', 'aim', 'of', 'this', 'paper', 'is', 'to', 'define', 'an', 'n1cocycle', 'sigma', 'on', 'gl_nq', 'with', 'values', 'in', 'a', 'certain', 'space', 'hd', 'of', 'distributions', 'on', 'a_fnsetminus0', 'here', 'a_f', 'denotes', 'the', 'ring', 'of', 'finite', 'adeles', 'of', 'q', 'and', 'the', 'distributions', 'take'... | [-0.1956772365208183, 0.08308146253548329, -0.08489928336681, 0.015958922511656835, -0.05562576704126384, -0.09869648262725345, -0.029880213083898915, 0.2894217172903674, -0.27169683742603024, -0.21367394775152207, 0.04276078272378072, -0.2408245142017092, -0.11013519949545818, 0.20484673749389393, -0.13936932025078153... |
708.0115 | Nuclear matrix elements of neutrinoless double beta decay with improved
short-range correlations | Nuclear matrix elements of the neutrinoless double beta decays of 96Zr,
100Mo, 116Cd, 128Te, 130Te and 136Xe are calculated for the light-neutrino
exchange mechanism by using the proton-neutron quasiparticle random-phase
approximation (pnQRPA) with a realistic nucleon-nucleon force. The g_pp
parameter of the pnQRPA i... | nucl-th | nuclear matrix elements of the neutrinoless double beta decays of 96zr 100mo 116cd 128te 130te and 136xe are calculated for the lightneutrino exchange mechanism by using the protonneutron quasiparticle randomphase approximation pnqrpa with a realistic nucleonnucleon force the g_pp parameter of the pnqrpa is fixed by th... | [['nuclear', 'matrix', 'elements', 'of', 'the', 'neutrinoless', 'double', 'beta', 'decays', 'of', '96zr', '100mo', '116cd', '128te', '130te', 'and', '136xe', 'are', 'calculated', 'for', 'the', 'lightneutrino', 'exchange', 'mechanism', 'by', 'using', 'the', 'protonneutron', 'quasiparticle', 'randomphase', 'approximation... | [-0.03897837607338898, 0.21467949696151273, -0.0679035784556296, 0.16492089665444176, 0.05331487722891275, -0.12859445861635768, 0.05495023851197365, 0.3181696950527681, -0.1871502986621289, -0.22573768113404005, -0.034241519082768436, -0.3328480310183728, -0.04907180853884946, 0.18066535350948978, 0.15395457127296244,... |
708.0116 | Fast computation of the Gauss hypergeometric function with all its
parameters complex with application to the Poschl-Teller-Ginocchio potential
wave functions | The fast computation of the Gauss hypergeometric function 2F1 with all its
parameters complex is a difficult task. Although the 2F1 function verifies
numerous analytical properties involving power series expansions whose
implementation is apparently immediate, their use is thwarted by instabilities
induced by cancell... | math-ph math.MP | the fast computation of the gauss hypergeometric function 2f1 with all its parameters complex is a difficult task although the 2f1 function verifies numerous analytical properties involving power series expansions whose implementation is apparently immediate their use is thwarted by instabilities induced by cancellatio... | [['the', 'fast', 'computation', 'of', 'the', 'gauss', 'hypergeometric', 'function', '2f1', 'with', 'all', 'its', 'parameters', 'complex', 'is', 'a', 'difficult', 'task', 'although', 'the', '2f1', 'function', 'verifies', 'numerous', 'analytical', 'properties', 'involving', 'power', 'series', 'expansions', 'whose', 'impl... | [-0.1561539152907711, 0.04235405969446072, -0.05940042914369622, 0.08531791547225234, -0.11710198987401216, -0.11084244970131565, 0.031880515146169915, 0.33628514859624004, -0.23450614175683743, -0.29698176504792395, 0.12374280354549252, -0.24316938017822198, -0.20965508662189383, 0.2634713346214109, -0.018641189849428... |
708.0117 | Resistance noise in Bi_2Sr_2CaCu_2O$_{8+\delta}$ | The resistance noise in a Bi_2Sr_2CaCu_2O$_{8+\delta}$ thin film is found to
increase strongly in the underdoped regime. While the increase of the raw
resistance noise with decreasing temperature appears to roughly track the
previously reported pseudogap temperature for this material, standard noise
analysis rather s... | cond-mat.supr-con cond-mat.dis-nn | the resistance noise in a bi_2sr_2cacu_2o_8delta thin film is found to increase strongly in the underdoped regime while the increase of the raw resistance noise with decreasing temperature appears to roughly track the previously reported pseudogap temperature for this material standard noise analysis rather suggests th... | [['the', 'resistance', 'noise', 'in', 'a', 'bi_2sr_2cacu_2o_8delta', 'thin', 'film', 'is', 'found', 'to', 'increase', 'strongly', 'in', 'the', 'underdoped', 'regime', 'while', 'the', 'increase', 'of', 'the', 'raw', 'resistance', 'noise', 'with', 'decreasing', 'temperature', 'appears', 'to', 'roughly', 'track', 'the', '... | [-0.14220488355573963, 0.2039686058119129, -0.043755709840837174, -0.0015260791544155297, -0.03257247262586981, -0.13979183472850817, 0.10085914132453627, 0.3342051464054039, -0.27304617438654777, -0.3179054657723439, 0.02299548972445398, -0.3601840478131327, -0.11380596758829335, 0.17622154960566658, -0.08648062004881... |
708.0118 | Interacting holographic generalized Chaplygin gas model | In this paper we consider a correspondence between the holographic dark
energy density and interacting generalized Chaplygin gas energy density in FRW
universe. Then we reconstruct the potential of the scalar field which describe
the generalized Chaplygin cosmology.
| hep-th | in this paper we consider a correspondence between the holographic dark energy density and interacting generalized chaplygin gas energy density in frw universe then we reconstruct the potential of the scalar field which describe the generalized chaplygin cosmology | [['in', 'this', 'paper', 'we', 'consider', 'a', 'correspondence', 'between', 'the', 'holographic', 'dark', 'energy', 'density', 'and', 'interacting', 'generalized', 'chaplygin', 'gas', 'energy', 'density', 'in', 'frw', 'universe', 'then', 'we', 'reconstruct', 'the', 'potential', 'of', 'the', 'scalar', 'field', 'which',... | [-0.12582519791536279, 0.12831561012487663, -0.170227067177429, 0.1445911626276364, -0.07129737739696314, -0.16898207306420723, -0.12076743659992262, 0.2536869929907353, -0.23171696713880488, -0.2796308716612035, -0.06262770902340938, -0.21104325770743584, -0.0734425586476726, 0.01473797818547801, -0.002529098039590999... |
708.0119 | Sum rules for B-->pi eta('), K eta('), eta(') eta(') decays | We provide a set of sum rules, using flavour symmetries, relating CP-averaged
ratios and CP asymmetries of different neutral and charged B mesons decaying
into an eta(') particle together with a pion, a kaon or a second eta('). These
sume rules allow us to give a prediction for the B^0-->K^0 eta branching ratio.
We a... | hep-ph | we provide a set of sum rules using flavour symmetries relating cpaveraged ratios and cp asymmetries of different neutral and charged b mesons decaying into an eta particle together with a pion a kaon or a second eta these sume rules allow us to give a prediction for the b0k0 eta branching ratio we also predict a clear... | [['we', 'provide', 'a', 'set', 'of', 'sum', 'rules', 'using', 'flavour', 'symmetries', 'relating', 'cpaveraged', 'ratios', 'and', 'cp', 'asymmetries', 'of', 'different', 'neutral', 'and', 'charged', 'b', 'mesons', 'decaying', 'into', 'an', 'eta', 'particle', 'together', 'with', 'a', 'pion', 'a', 'kaon', 'or', 'a', 'sec... | [-0.11672498171537882, 0.22811265545478818, -0.0986021332006203, 0.12487333661410957, -0.06683345312485471, -0.18235036385594866, 0.16704834617485176, 0.30552298123948274, -0.18492601574653236, -0.22531321712303906, -0.029230223575723357, -0.3142134491179604, 0.0014039055691682733, 0.10393855723523301, 0.12183636842528... |
708.012 | A case study of the Hirsch index for 26 non-prominent physicists | The h index was introduced by Hirsch to quantify an individual's scientific
research output. It has been widely used in different fields to show the
relevance of the research work of prominent scientists. I have worked out 26
practical cases of physicists which are not so prominent. Therefore this case
study should b... | physics.soc-ph | the h index was introduced by hirsch to quantify an individuals scientific research output it has been widely used in different fields to show the relevance of the research work of prominent scientists i have worked out 26 practical cases of physicists which are not so prominent therefore this case study should be more... | [['the', 'h', 'index', 'was', 'introduced', 'by', 'hirsch', 'to', 'quantify', 'an', 'individuals', 'scientific', 'research', 'output', 'it', 'has', 'been', 'widely', 'used', 'in', 'different', 'fields', 'to', 'show', 'the', 'relevance', 'of', 'the', 'research', 'work', 'of', 'prominent', 'scientists', 'i', 'have', 'wor... | [-0.050866166654870745, 0.09122201988308613, -0.07014746935003334, 0.11365727993737286, -0.09930977390872107, -0.16783181962867577, -0.01937761190864775, 0.40680292397737505, -0.2113271100860503, -0.3418484102520678, 0.09809727763058618, -0.2796201181391047, -0.18893139460124075, 0.2104493736134221, -0.0922616973001923... |
708.0121 | Discussion of ``2004 IMS Medallion Lecture: Local Rademacher
complexities and oracle inequalities in risk minimization'' by V.
Koltchinskii | Discussion of ``2004 IMS Medallion Lecture: Local Rademacher complexities and
oracle inequalities in risk minimization'' by V. Koltchinskii [arXiv:0708.0083]
| q-fin.RM math.ST stat.TH | discussion of 2004 ims medallion lecture local rademacher complexities and oracle inequalities in risk minimization by v koltchinskii arxiv07080083 | [['discussion', 'of', '2004', 'ims', 'medallion', 'lecture', 'local', 'rademacher', 'complexities', 'and', 'oracle', 'inequalities', 'in', 'risk', 'minimization', 'by', 'v', 'koltchinskii', 'arxiv07080083']] | [-0.04620913315662428, -0.01606457386361925, -0.05329715259569256, 0.19175361194892934, -0.0260421199062349, -0.26058023275905534, 0.20598403261484285, 0.24738681237948568, -0.251077052303835, -0.3320668751471921, 0.1784132805983781, -0.32687197998166084, -0.13523328931708084, 0.12226964003945652, -0.32103299344644737,... |
708.0122 | Cosmological Constraints on Radion Evolution in the Universal Extra
Dimension Model | The constraints on the radion evolution in the Universal Extra Dimension
(UED) model from Cosmic Microwave Background (CMB) and Type Ia supernovae (SNe
Ia) data are studied. In the UED model, where both the gravity and standard
model fields can propagate in the extra dimensions, the evolution of the extra
dimensional... | astro-ph | the constraints on the radion evolution in the universal extra dimension ued model from cosmic microwave background cmb and type ia supernovae sne ia data are studied in the ued model where both the gravity and standard model fields can propagate in the extra dimensions the evolution of the extra dimensional volume the... | [['the', 'constraints', 'on', 'the', 'radion', 'evolution', 'in', 'the', 'universal', 'extra', 'dimension', 'ued', 'model', 'from', 'cosmic', 'microwave', 'background', 'cmb', 'and', 'type', 'ia', 'supernovae', 'sne', 'ia', 'data', 'are', 'studied', 'in', 'the', 'ued', 'model', 'where', 'both', 'the', 'gravity', 'and',... | [-0.09051809426552306, 0.15054212906915282, -0.004807454184629023, 0.1506584402005602, -0.09274617826255659, -0.11914331428835996, 0.03488212103645007, 0.31070728715923096, -0.20819952647822598, -0.3127886705359237, 0.0650116359170675, -0.32446061547638644, 0.021325553083119706, 0.2033050946192816, 0.000668598518718176... |
708.0123 | SuperAGILE: the hard X-ray Imager for the AGILE space mission | SuperAGILE is a coded mask experiment based on silicon microstrip detectors.
It operates in the 15-45 keV nominal energy range, providing crossed
one-dimensional images of the X-ray sky with an on-axis angular resolution of 6
arcmin, over a field of view in excess of 1 steradian. It was designed as the
hard X-ray mon... | astro-ph | superagile is a coded mask experiment based on silicon microstrip detectors it operates in the 1545 kev nominal energy range providing crossed onedimensional images of the xray sky with an onaxis angular resolution of 6 arcmin over a field of view in excess of 1 steradian it was designed as the hard xray monitor of the... | [['superagile', 'is', 'a', 'coded', 'mask', 'experiment', 'based', 'on', 'silicon', 'microstrip', 'detectors', 'it', 'operates', 'in', 'the', '1545', 'kev', 'nominal', 'energy', 'range', 'providing', 'crossed', 'onedimensional', 'images', 'of', 'the', 'xray', 'sky', 'with', 'an', 'onaxis', 'angular', 'resolution', 'of'... | [-0.08703895882280747, 0.12041712246804416, -0.06570502043459095, 0.08348497099824202, -0.07709735111620065, -0.05770428951031396, 0.048530442069848106, 0.4512312878079775, -0.17018379524209293, -0.42238503145132245, 0.11441492762107465, -0.3306661367557254, -0.009555963916751016, 0.25929867501268866, -0.08696361082535... |
708.0124 | Discussion of ``2004 IMS Medallion Lecture: Local Rademacher
complexities and oracle inequalities in risk minimization'' by V.
Koltchinskii | Discussion of ``2004 IMS Medallion Lecture: Local Rademacher complexities and
oracle inequalities in risk minimization'' by V. Koltchinskii [arXiv:0708.0083]
| q-fin.RM math.ST stat.TH | discussion of 2004 ims medallion lecture local rademacher complexities and oracle inequalities in risk minimization by v koltchinskii arxiv07080083 | [['discussion', 'of', '2004', 'ims', 'medallion', 'lecture', 'local', 'rademacher', 'complexities', 'and', 'oracle', 'inequalities', 'in', 'risk', 'minimization', 'by', 'v', 'koltchinskii', 'arxiv07080083']] | [-0.04620913315662428, -0.01606457386361925, -0.05329715259569256, 0.19175361194892934, -0.0260421199062349, -0.26058023275905534, 0.20598403261484285, 0.24738681237948568, -0.251077052303835, -0.3320668751471921, 0.1784132805983781, -0.32687197998166084, -0.13523328931708084, 0.12226964003945652, -0.32103299344644737,... |
708.0125 | Solutions to the nonlinear Schroedinger equation carrying momentum along
a curve. Part I: study of the limit set and approximate solutions | We prove existence of a special class of solutions to the (elliptic)
Nonlinear Schroeodinger Equation $- \epsilon^2 \Delta \psi + V(x) \psi =
|\psi|^{p-1} \psi$, on a manifold or in the Euclidean space. Here V represents
the potential, p an exponent greater than 1 and $\epsilon$ a small parameter
corresponding to the... | math.AP | we prove existence of a special class of solutions to the elliptic nonlinear schroeodinger equation epsilon2 delta psi vx psi psip1 psi on a manifold or in the euclidean space here v represents the potential p an exponent greater than 1 and epsilon a small parameter corresponding to the planck constant as epsilon tends... | [['we', 'prove', 'existence', 'of', 'a', 'special', 'class', 'of', 'solutions', 'to', 'the', 'elliptic', 'nonlinear', 'schroeodinger', 'equation', 'epsilon2', 'delta', 'psi', 'vx', 'psi', 'psip1', 'psi', 'on', 'a', 'manifold', 'or', 'in', 'the', 'euclidean', 'space', 'here', 'v', 'represents', 'the', 'potential', 'p', ... | [-0.1912295567257137, 0.0904649184570158, -0.0954925220588158, 0.03329745570101358, -0.07698891974287107, -0.11514904055872868, 0.016116414598895814, 0.2966681024653773, -0.2853520404997057, -0.22952992353459883, 0.10496149474658586, -0.28464803647667425, -0.12472456733310788, 0.18491718226818946, -0.03536596181963025,... |
708.0126 | Monte Carlo simulations of the L10 long-range order relaxation in
dimensionally reduced systems | Monte Carlo simulations have been performed to investigate the relaxation of
the L10 long-range order in dimensionally reduced systems. The effect of the
number of (001)-type monatomic layers and of the pair interaction energies on
these kinetics has been examined. The vacancy migration energies have been
deduced fro... | cond-mat.soft cond-mat.mtrl-sci | monte carlo simulations have been performed to investigate the relaxation of the l10 longrange order in dimensionally reduced systems the effect of the number of 001type monatomic layers and of the pair interaction energies on these kinetics has been examined the vacancy migration energies have been deduced from the ar... | [['monte', 'carlo', 'simulations', 'have', 'been', 'performed', 'to', 'investigate', 'the', 'relaxation', 'of', 'the', 'l10', 'longrange', 'order', 'in', 'dimensionally', 'reduced', 'systems', 'the', 'effect', 'of', 'the', 'number', 'of', '001type', 'monatomic', 'layers', 'and', 'of', 'the', 'pair', 'interaction', 'ene... | [-0.08792369512483737, 0.1575269000713042, -0.0455018712240163, 0.01831365633501433, 0.042018064749860314, -0.05700430379595694, 0.00972988637878971, 0.43902395406824557, -0.23817889293829023, -0.3532403309201432, 0.03657947518716588, -0.3400182406266415, -0.03963044984807629, 0.18825295474380255, 0.09361500595154804, ... |
708.0127 | Accuracy control in ultra-large-scale electronic structure calculation | Numerical aspects are investigated in ultra-large-scale electronic structure
calculation. Accuracy control methods in process (molecular-dynamics)
calculation are focused. Flexible control methods are proposed so as to control
variational freedoms, automatically at each time step, within the framework of
generalized ... | cond-mat.mtrl-sci | numerical aspects are investigated in ultralargescale electronic structure calculation accuracy control methods in process moleculardynamics calculation are focused flexible control methods are proposed so as to control variational freedoms automatically at each time step within the framework of generalized wannier sta... | [['numerical', 'aspects', 'are', 'investigated', 'in', 'ultralargescale', 'electronic', 'structure', 'calculation', 'accuracy', 'control', 'methods', 'in', 'process', 'moleculardynamics', 'calculation', 'are', 'focused', 'flexible', 'control', 'methods', 'are', 'proposed', 'so', 'as', 'to', 'control', 'variational', 'f... | [-0.05389570241095498, 0.06857071082211202, -0.08619802775663427, 0.03483445593827936, -0.013391098731921779, -0.15351772650481305, 0.020462002535673998, 0.4486047426600837, -0.27601753521917594, -0.27840303784857195, 0.037593595483081624, -0.26318926657161984, -0.17060774766206224, 0.19011768896274994, -0.011381703108... |
708.0128 | The alternating marked point process of h-slopes of the drifted Brownian
motion | We show that the slopes between h-extrema of the drifted 1D Brownian motion
form a stationary alternating marked point process, extending the result of J.
Neveu and J. Pitman for the non drifted case. Our analysis covers the results
on the statistics of h-extrema obtained by P. Le Doussal, C. Monthus and D.
Fisher vi... | math.PR math-ph math.MP | we show that the slopes between hextrema of the drifted 1d brownian motion form a stationary alternating marked point process extending the result of j neveu and j pitman for the non drifted case our analysis covers the results on the statistics of hextrema obtained by p le doussal c monthus and d fisher via a renormal... | [['we', 'show', 'that', 'the', 'slopes', 'between', 'hextrema', 'of', 'the', 'drifted', '1d', 'brownian', 'motion', 'form', 'a', 'stationary', 'alternating', 'marked', 'point', 'process', 'extending', 'the', 'result', 'of', 'j', 'neveu', 'and', 'j', 'pitman', 'for', 'the', 'non', 'drifted', 'case', 'our', 'analysis', '... | [-0.11933968252446137, 0.07862423843536735, -0.15227440853728755, -0.0020101292318103017, -0.011519505464461413, -0.08130376415557405, 0.09289413008163945, 0.3101292146458761, -0.23926212513044978, -0.26418391481209336, 0.051822188833540075, -0.31461023736033544, -0.1458922532816114, 0.18574437752282352, -0.03922407977... |
708.0129 | Low temperature specific heat of La_{3}Pd_{4}Ge_{4} with
U_{3}Ni_{4}Si_{4}-type structure | Low temperature specific heat has been investigated in a novel ternary
superconductor La_{3}Pd_{4}Ge_{4} with an U_{3}Ni_{4}Si_{4}-type structure
consisting of the alternating BaAl_{4} (ThCr_{2}Si_{2})- and AlB$_{2}$-type
layers. A comparative study with the related ThCr_{2}Si_{2}-type superconductor
LaPd_{2}Ge_{2}, ... | cond-mat.supr-con | low temperature specific heat has been investigated in a novel ternary superconductor la_3pd_4ge_4 with an u_3ni_4si_4type structure consisting of the alternating baal_4 thcr_2si_2 and alb_2type layers a comparative study with the related thcr_2si_2type superconductor lapd_2ge_2 one of the layers in la_3pd_4ge_4 is als... | [['low', 'temperature', 'specific', 'heat', 'has', 'been', 'investigated', 'in', 'a', 'novel', 'ternary', 'superconductor', 'la_3pd_4ge_4', 'with', 'an', 'u_3ni_4si_4type', 'structure', 'consisting', 'of', 'the', 'alternating', 'baal_4', 'thcr_2si_2', 'and', 'alb_2type', 'layers', 'a', 'comparative', 'study', 'with', '... | [-0.1657674342311359, 0.18718054305568468, -0.002068577817584755, -0.014424661072553135, -0.04774758388873923, -0.17983802261931653, 0.11169508411055148, 0.32651983043461136, -0.24187953114707136, -0.289192569741951, 0.03735018601626948, -0.3959362476104588, -0.04818211653918931, 0.18901607744169957, 0.0655812030520544... |
708.013 | Lowest Weights in Cohomology of Variations of Hodge Structure | Let X be a smooth complex projective variety, let $j:U\into X$ an immersion
of a Zariski open subset, and let V be a variation of Hodge structure of weight
n over U. Then IH^k(X, j_*V) is known to carry a pure Hodge structure of weight
k+n, while H^k(U,V) carries a mixed Hodge structure of weight $\ge k+n$. In
this n... | math.AG math.CV | let x be a smooth complex projective variety let juinto x an immersion of a zariski open subset and let v be a variation of hodge structure of weight n over u then ihkx j_v is known to carry a pure hodge structure of weight kn while hkuv carries a mixed hodge structure of weight ge kn in this note it is shown that the ... | [['let', 'x', 'be', 'a', 'smooth', 'complex', 'projective', 'variety', 'let', 'juinto', 'x', 'an', 'immersion', 'of', 'a', 'zariski', 'open', 'subset', 'and', 'let', 'v', 'be', 'a', 'variation', 'of', 'hodge', 'structure', 'of', 'weight', 'n', 'over', 'u', 'then', 'ihkx', 'j_v', 'is', 'known', 'to', 'carry', 'a', 'pure... | [-0.18909640655064405, 0.05065968556118605, -0.15122836021791128, 0.019036600362266076, -0.10391816111620177, -0.14156820061907638, -0.010755983399576508, 0.3177969439420849, -0.40784566779620945, -0.19530274064428257, 0.06669399182349232, -0.20526849559973925, -0.13719861657062377, 0.1287422199013897, -0.1625398199116... |
708.0131 | On the Density Dependent Nuclear Matter Compressibility | In the present work we apply a quantum hadrodynamic effective model in the
mean-field approximation to the description of neutron stars. We consider an
adjustable derivative-coupling model and study the parameter influence on the
dynamics of the system by analyzing the full range of values they can take. We
establish... | astro-ph nucl-th | in the present work we apply a quantum hadrodynamic effective model in the meanfield approximation to the description of neutron stars we consider an adjustable derivativecoupling model and study the parameter influence on the dynamics of the system by analyzing the full range of values they can take we establish a set... | [['in', 'the', 'present', 'work', 'we', 'apply', 'a', 'quantum', 'hadrodynamic', 'effective', 'model', 'in', 'the', 'meanfield', 'approximation', 'to', 'the', 'description', 'of', 'neutron', 'stars', 'we', 'consider', 'an', 'adjustable', 'derivativecoupling', 'model', 'and', 'study', 'the', 'parameter', 'influence', 'o... | [-0.058804875709440395, 0.1344359529216055, -0.09632036488746172, 0.1066388095860653, -0.08973984933741715, -0.07332148762500805, 0.07171462165272754, 0.32735240555003936, -0.23173362881593082, -0.34209619642680755, 0.04601569938797342, -0.2691902109361051, -0.07529244000578056, 0.16350628275262272, -0.0059045743116218... |
708.0132 | Discussion of ``2004 IMS Medallion Lecture: Local Rademacher
complexities and oracle inequalities in risk minimization'' by V.
Koltchinskii | Discussion of ``2004 IMS Medallion Lecture: Local Rademacher complexities and
oracle inequalities in risk minimization'' by V. Koltchinskii [arXiv:0708.0083]
| q-fin.RM math.ST stat.TH | discussion of 2004 ims medallion lecture local rademacher complexities and oracle inequalities in risk minimization by v koltchinskii arxiv07080083 | [['discussion', 'of', '2004', 'ims', 'medallion', 'lecture', 'local', 'rademacher', 'complexities', 'and', 'oracle', 'inequalities', 'in', 'risk', 'minimization', 'by', 'v', 'koltchinskii', 'arxiv07080083']] | [-0.04620913315662428, -0.01606457386361925, -0.05329715259569256, 0.19175361194892934, -0.0260421199062349, -0.26058023275905534, 0.20598403261484285, 0.24738681237948568, -0.251077052303835, -0.3320668751471921, 0.1784132805983781, -0.32687197998166084, -0.13523328931708084, 0.12226964003945652, -0.32103299344644737,... |
708.0133 | The clumpy structure of the chemically active L1157 outflow | We present high spatial resolution maps, obtained with the Plateau de Bure
Interferometer, of the blue lobe of the L1157 outflow. We observed four lines
at 3 mm, namely CH3OH (2_K-1_K), HC3N (11-10), HCN (1-0) and OCS (7-6).
Moreover, the bright B1 clump has also been observed at better spatial
resolution in CS (2-1)... | astro-ph | we present high spatial resolution maps obtained with the plateau de bure interferometer of the blue lobe of the l1157 outflow we observed four lines at 3 mm namely ch3oh 2_k1_k hc3n 1110 hcn 10 and ocs 76 moreover the bright b1 clump has also been observed at better spatial resolution in cs 21 ch3oh 2_11_1a and 34so 3... | [['we', 'present', 'high', 'spatial', 'resolution', 'maps', 'obtained', 'with', 'the', 'plateau', 'de', 'bure', 'interferometer', 'of', 'the', 'blue', 'lobe', 'of', 'the', 'l1157', 'outflow', 'we', 'observed', 'four', 'lines', 'at', '3', 'mm', 'namely', 'ch3oh', '2_k1_k', 'hc3n', '1110', 'hcn', '10', 'and', 'ocs', '76'... | [-0.08775891852752206, 0.0965439846814531, -0.002384073245671711, 0.0493890248351298, -0.03964496291591786, -0.07419113180783045, -0.010723238542725864, 0.4859811941793721, -0.16998947245842178, -0.30436682987887514, 0.07206918855663388, -0.26728982529602946, -0.0037385261039681998, 0.0913822246359944, 0.02533065358542... |
708.0134 | LHC Physics and Cosmology | In these Lectures I review possible constraints on particle physics models,
obtained by means of combining the results of collider measurements with
astrophysical data. I emphasize the theoretical-model dependence of these
results. I discuss supersymmetric dark matter constraints at colliders (mainly
LHC) in various ... | hep-ph astro-ph hep-th | in these lectures i review possible constraints on particle physics models obtained by means of combining the results of collider measurements with astrophysical data i emphasize the theoreticalmodel dependence of these results i discuss supersymmetric dark matter constraints at colliders mainly lhc in various theoreti... | [['in', 'these', 'lectures', 'i', 'review', 'possible', 'constraints', 'on', 'particle', 'physics', 'models', 'obtained', 'by', 'means', 'of', 'combining', 'the', 'results', 'of', 'collider', 'measurements', 'with', 'astrophysical', 'data', 'i', 'emphasize', 'the', 'theoreticalmodel', 'dependence', 'of', 'these', 'resu... | [-0.054390153075354365, 0.15413726370480627, -0.08413928224131315, 0.13796614306141633, -0.11092024681751024, -0.17756068207925618, -0.036584034830218916, 0.2717319250370216, -0.23794934563715048, -0.3574346586488037, 0.08327683630032522, -0.3150669232274246, -0.01875176375045093, 0.19820198246555384, 0.054616503064718... |
708.0135 | Rejoinder: 2004 IMS Medallion Lecture: Local Rademacher complexities and
oracle inequalities in risk minimization | Rejoinder: 2004 IMS Medallion Lecture: Local Rademacher complexities and
oracle inequalities in risk minimization [arXiv:0708.0083]
| math.ST stat.TH | rejoinder 2004 ims medallion lecture local rademacher complexities and oracle inequalities in risk minimization arxiv07080083 | [['rejoinder', '2004', 'ims', 'medallion', 'lecture', 'local', 'rademacher', 'complexities', 'and', 'oracle', 'inequalities', 'in', 'risk', 'minimization', 'arxiv07080083']] | [0.01076726991062363, -0.06430117512742678, -0.11209756725778182, 0.2987693337102731, -0.04122264566831291, -0.25109252966940404, 0.2063384658967455, 0.2271235167980194, -0.25563641972839835, -0.3398139422138532, 0.2034417312204217, -0.3584949001669884, -0.16292761266231537, 0.09200651173790296, -0.3942384081582228, 0.... |
708.0136 | Harmonic morphisms from solvable Lie groups | In this paper we introduce two new methods for constructing harmonic
morphisms from solvable Lie groups. The first method yields global solutions
from any simply connected nilpotent Lie group and from any Riemannian symmetric
space of non-compact type and rank $r\ge 3$. The second method provides us with
global solut... | math.DG | in this paper we introduce two new methods for constructing harmonic morphisms from solvable lie groups the first method yields global solutions from any simply connected nilpotent lie group and from any riemannian symmetric space of noncompact type and rank rge 3 the second method provides us with global solutions fro... | [['in', 'this', 'paper', 'we', 'introduce', 'two', 'new', 'methods', 'for', 'constructing', 'harmonic', 'morphisms', 'from', 'solvable', 'lie', 'groups', 'the', 'first', 'method', 'yields', 'global', 'solutions', 'from', 'any', 'simply', 'connected', 'nilpotent', 'lie', 'group', 'and', 'from', 'any', 'riemannian', 'sym... | [-0.12002758507007434, 0.07676411599472717, -0.0674104638984082, 0.06065281425792448, -0.2007198709661118, -0.1964325826373641, -0.037308724733632934, 0.4157450791379368, -0.28288265257889844, -0.18445772446554015, 0.1405340154112006, -0.20308981405824056, -0.18435907785861214, 0.2250822442871185, -0.11785213334232937,... |
708.0137 | Viscosity in the excluded volume hadron gas model | The shear viscosity $\eta$ in the van der Waals excluded volume
hadron-resonance gas model is considered. For the shear viscosity the result of
the non-relativistic gas of hard-core particles is extended to the mixture of
particles with different masses, but equal values of hard-core radius r. The
relativistic correc... | nucl-th hep-ph | the shear viscosity eta in the van der waals excluded volume hadronresonance gas model is considered for the shear viscosity the result of the nonrelativistic gas of hardcore particles is extended to the mixture of particles with different masses but equal values of hardcore radius r the relativistic corrections to had... | [['the', 'shear', 'viscosity', 'eta', 'in', 'the', 'van', 'der', 'waals', 'excluded', 'volume', 'hadronresonance', 'gas', 'model', 'is', 'considered', 'for', 'the', 'shear', 'viscosity', 'the', 'result', 'of', 'the', 'nonrelativistic', 'gas', 'of', 'hardcore', 'particles', 'is', 'extended', 'to', 'the', 'mixture', 'of'... | [-0.1274120655453842, 0.23604123840320432, -0.09792416797906249, 0.06006859989438072, 0.053430475905770436, -0.14498297422901243, 0.0194915519179609, 0.28723892478640384, -0.20491127531925316, -0.27592659778028594, -0.03501757451724875, -0.34457437936105056, 0.1057320944574511, 0.089661422186994, 0.06303550126616603, 0... |
708.0138 | Self-similar branching Markov chains | The main purpose of this work is to study self-similar branching Markov
chains. First we will construct such a process. Then we will establish certain
Limit Theorems using the theory of self-similar Markov processes.
| math.PR | the main purpose of this work is to study selfsimilar branching markov chains first we will construct such a process then we will establish certain limit theorems using the theory of selfsimilar markov processes | [['the', 'main', 'purpose', 'of', 'this', 'work', 'is', 'to', 'study', 'selfsimilar', 'branching', 'markov', 'chains', 'first', 'we', 'will', 'construct', 'such', 'a', 'process', 'then', 'we', 'will', 'establish', 'certain', 'limit', 'theorems', 'using', 'the', 'theory', 'of', 'selfsimilar', 'markov', 'processes']] | [-0.09122302455259212, 0.16391889493474188, -0.12132965214550495, 0.12053587014628754, -0.07659630269250449, -0.04561504972276881, 0.07513289965401568, 0.3901231738683932, -0.31229006103239954, -0.13047317007337422, 0.15139856553800843, -0.21257431021727183, -0.15374712435090365, 0.16250533917370966, -0.041380238144055... |
708.0139 | Suppressed Decays of D_s^+ Mesons to Two Pseudoscalar Mesons | Using data collected near the Ds*+ Ds- peak production energy Ecm = 4170 MeV
by the CLEO-c detector, we study the decays of Ds+ mesons to two pseudoscalar
mesons. We report on searches for the singly-Cabibbo-suppressed Ds+ decay modes
K+ eta, K+ eta', pi+ K0S, K+ pi0, and the isospin-forbidden decay mode Ds+ to
pi+ p... | hep-ex | using data collected near the ds ds peak production energy ecm 4170 mev by the cleoc detector we study the decays of ds mesons to two pseudoscalar mesons we report on searches for the singlycabibbosuppressed ds decay modes k eta k eta pi k0s k pi0 and the isospinforbidden decay mode ds to pi pi0 we normalize with respe... | [['using', 'data', 'collected', 'near', 'the', 'ds', 'ds', 'peak', 'production', 'energy', 'ecm', '4170', 'mev', 'by', 'the', 'cleoc', 'detector', 'we', 'study', 'the', 'decays', 'of', 'ds', 'mesons', 'to', 'two', 'pseudoscalar', 'mesons', 'we', 'report', 'on', 'searches', 'for', 'the', 'singlycabibbosuppressed', 'ds',... | [-0.12189692393327328, 0.3081977754879684, -0.10694730078840864, 0.046426413679154406, -0.04525938826472938, -0.16899407749444667, 0.21483264713380879, 0.25225912535589345, -0.1856754139380556, -0.2342606606998999, -0.11634661324820678, -0.48932507830921196, 0.11861286301847915, 0.052387997096496254, 0.1509193461322763... |
708.014 | Optical and Near-Infrared Observations of the Highly Reddened, Rapidly
Expanding Type Ia Supernova 2006X in M100 | We present extensive optical (UBVRI), near-infrared (JK) light curves and
optical spectroscopy of the Type Ia supernova (SN) 2006X in the nearby galaxy
NGC 4321 (M100). Our observations suggest that either SN 2006X has an
intrinsically peculiar color evolution, or it is highly reddened [E(B -
V)_{host} = 1.42+/-0.04 ... | astro-ph | we present extensive optical ubvri nearinfrared jk light curves and optical spectroscopy of the type ia supernova sn 2006x in the nearby galaxy ngc 4321 m100 our observations suggest that either sn 2006x has an intrinsically peculiar color evolution or it is highly reddened eb v_host 142004 mag with r_v 148006 much low... | [['we', 'present', 'extensive', 'optical', 'ubvri', 'nearinfrared', 'jk', 'light', 'curves', 'and', 'optical', 'spectroscopy', 'of', 'the', 'type', 'ia', 'supernova', 'sn', '2006x', 'in', 'the', 'nearby', 'galaxy', 'ngc', '4321', 'm100', 'our', 'observations', 'suggest', 'that', 'either', 'sn', '2006x', 'has', 'an', 'i... | [-0.03875570922003438, 0.06679712746441105, -0.08927246574312449, 0.08871342050066838, -0.10284957183628446, -0.1766038020538097, 0.07925193101702327, 0.4820932533522999, -0.1748271340862158, -0.25051583151022594, 0.037240874841895505, -0.34395911441598503, -0.04320623975385118, 0.18430700753987939, -0.0663209248178949... |
708.0141 | Using ultra-short pulses to determine particle size and density
distributions | We analyze the time dependent response of strongly scattering media (SSM) to
ultra-short pulses of light. A random walk technique is used to model the
optical scattering of ultra-short pulses of light propagating through media
with random shapes and various packing densities. The pulse spreading was found
to be stron... | physics.optics | we analyze the time dependent response of strongly scattering media ssm to ultrashort pulses of light a random walk technique is used to model the optical scattering of ultrashort pulses of light propagating through media with random shapes and various packing densities the pulse spreading was found to be strongly depe... | [['we', 'analyze', 'the', 'time', 'dependent', 'response', 'of', 'strongly', 'scattering', 'media', 'ssm', 'to', 'ultrashort', 'pulses', 'of', 'light', 'a', 'random', 'walk', 'technique', 'is', 'used', 'to', 'model', 'the', 'optical', 'scattering', 'of', 'ultrashort', 'pulses', 'of', 'light', 'propagating', 'through', ... | [-0.07035887687293402, 0.22681858652824796, -0.12802132897836677, 0.028008617994462345, -0.02742004546463111, -0.09208642634152735, 0.036456635284979465, 0.48570115952673604, -0.28277409296103956, -0.3098229573471314, 0.06237699524341625, -0.29280959010731933, -0.10087441158149454, 0.1744506461417571, -0.00426484042802... |
708.0142 | The 4th Concept Detector for the International Linear Collider | The 4th Concept detector presently being designed for the International
Linear Collider introduces several innovations in order to achieve the
necessary experimental goal of a detecter that is 2-to-10 times better than the
already excellent SLC and LEP detectors. We introduce a dual-readout
calorimeter system, a clus... | hep-ex | the 4th concept detector presently being designed for the international linear collider introduces several innovations in order to achieve the necessary experimental goal of a detecter that is 2to10 times better than the already excellent slc and lep detectors we introduce a dualreadout calorimeter system a cluster cou... | [['the', '4th', 'concept', 'detector', 'presently', 'being', 'designed', 'for', 'the', 'international', 'linear', 'collider', 'introduces', 'several', 'innovations', 'in', 'order', 'to', 'achieve', 'the', 'necessary', 'experimental', 'goal', 'of', 'a', 'detecter', 'that', 'is', '2to10', 'times', 'better', 'than', 'the'... | [-0.08117030688233419, 0.1369350540282374, -0.07677199367158623, 0.0828152913243023, -0.07459902621551671, -0.14174800654555755, -0.021310885274777484, 0.3720229376551949, -0.18739616811878726, -0.36374769355593756, 0.07737837605236564, -0.32110279332846403, 0.02312289527617395, 0.21136725227353798, -0.0046569355657662... |
708.0143 | Nonparametric quasi-maximum likelihood estimation for Gaussian locally
stationary processes | This paper deals with nonparametric maximum likelihood estimation for
Gaussian locally stationary processes. Our nonparametric MLE is constructed by
minimizing a frequency domain likelihood over a class of functions. The
asymptotic behavior of the resulting estimator is studied. The results depend
on the richness of ... | math.ST stat.TH | this paper deals with nonparametric maximum likelihood estimation for gaussian locally stationary processes our nonparametric mle is constructed by minimizing a frequency domain likelihood over a class of functions the asymptotic behavior of the resulting estimator is studied the results depend on the richness of the c... | [['this', 'paper', 'deals', 'with', 'nonparametric', 'maximum', 'likelihood', 'estimation', 'for', 'gaussian', 'locally', 'stationary', 'processes', 'our', 'nonparametric', 'mle', 'is', 'constructed', 'by', 'minimizing', 'a', 'frequency', 'domain', 'likelihood', 'over', 'a', 'class', 'of', 'functions', 'the', 'asymptot... | [-0.05298907310152274, 0.03239238929477249, -0.11228503277677981, 0.10565774277016377, -0.048373599697026565, -0.12536814774493457, 0.02994355183384824, 0.390153741677765, -0.2392127706409722, -0.26103468367936794, 0.1656399809423315, -0.23085975936675046, -0.16010506612202915, 0.23568789356032227, -0.11470544066845027... |
708.0144 | Magnetic Field Structure in the Parsec Scale Jet of 3C273 from
Multifrequency VLBA Observations | We present first results from a multifrequency VLBA observations of 3C273 in
2003. The source was observed simultaneously at 5.0, 8.4, 15.3, 22.2, 43.2 and
86.2 GHz, and from this multifrequency data set, spectra of 16 emission
features in the parsec scale jet were carefully constructed by using a new
model-fitting b... | astro-ph | we present first results from a multifrequency vlba observations of 3c273 in 2003 the source was observed simultaneously at 50 84 153 222 432 and 862 ghz and from this multifrequency data set spectra of 16 emission features in the parsec scale jet were carefully constructed by using a new modelfitting based method the ... | [['we', 'present', 'first', 'results', 'from', 'a', 'multifrequency', 'vlba', 'observations', 'of', '3c273', 'in', '2003', 'the', 'source', 'was', 'observed', 'simultaneously', 'at', '50', '84', '153', '222', '432', 'and', '862', 'ghz', 'and', 'from', 'this', 'multifrequency', 'data', 'set', 'spectra', 'of', '16', 'emi... | [-0.10123273995643678, 0.13141305715743282, -0.06650096317263025, 0.05518670261188067, -0.04504721207593224, -0.033973355929514296, -0.006383467195547909, 0.3982797390536258, -0.20659878156883152, -0.37836420173315627, 0.06348612878630919, -0.2618137793419392, 0.04382507986830254, 0.1850229410209546, 0.0580828224736155... |
708.0145 | Programmable Quantum State Transfer | A programmable quantum networks model is used in this paper for development
of methods of control of a quantum state transport. These methods may be
applied for a wide variety of patterns of controlled state transmission and
spreading in quantum systems. The programmable perfect state transfer and
quantum walk, mobil... | quant-ph | a programmable quantum networks model is used in this paper for development of methods of control of a quantum state transport these methods may be applied for a wide variety of patterns of controlled state transmission and spreading in quantum systems the programmable perfect state transfer and quantum walk mobile qua... | [['a', 'programmable', 'quantum', 'networks', 'model', 'is', 'used', 'in', 'this', 'paper', 'for', 'development', 'of', 'methods', 'of', 'control', 'of', 'a', 'quantum', 'state', 'transport', 'these', 'methods', 'may', 'be', 'applied', 'for', 'a', 'wide', 'variety', 'of', 'patterns', 'of', 'controlled', 'state', 'trans... | [-0.1413202589780737, 0.17896028761393748, -0.09741075540391299, -0.015837653876783757, -0.0028281628798979977, -0.22642906109730784, 0.04455229059184113, 0.39507048084185675, -0.3057621050196198, -0.27821867216665014, 0.06372486042360273, -0.1936319790279063, -0.1910091411931297, 0.25061752606684773, -0.06275087902322... |
708.0146 | A Side of Mercury Not Seen By Mariner 10 | More than 60,000 images of Mercury were taken at ~29 deg elevation during two
sunrises, at 820 nm, and through a 1.35 m diameter off-axis aperture on the
SOAR telescope. The sharpest resolve 0.2" (140 km) and cover 190-300 deg
longitude -- a swath unseen by the Mariner 10 spacecraft -- at complementary
phase angles t... | astro-ph | more than 60000 images of mercury were taken at 29 deg elevation during two sunrises at 820 nm and through a 135 m diameter offaxis aperture on the soar telescope the sharpest resolve 02 140 km and cover 190300 deg longitude a swath unseen by the mariner 10 spacecraft at complementary phase angles to previous groundbas... | [['more', 'than', '60000', 'images', 'of', 'mercury', 'were', 'taken', 'at', '29', 'deg', 'elevation', 'during', 'two', 'sunrises', 'at', '820', 'nm', 'and', 'through', 'a', '135', 'm', 'diameter', 'offaxis', 'aperture', 'on', 'the', 'soar', 'telescope', 'the', 'sharpest', 'resolve', '02', '140', 'km', 'and', 'cover', ... | [-0.08490468609292125, 0.1755063477499852, -0.049485697769499355, 0.045997384176562635, -0.08722048251878879, -0.09102161382082742, 0.045184924977836924, 0.38747536147691614, -0.20536057385373752, -0.3584752144571932, 0.11780247891206036, -0.3263615618508331, -0.07966572283820997, 0.24355188739954392, -0.12780906493786... |
708.0147 | Control of unstable steady states by extended time-delayed feedback | Time-delayed feedback methods can be used to control unstable periodic orbits
as well as unstable steady states. We present an application of extended time
delay autosynchronization introduced by Socolar et al. to an unstable focus.
This system represents a generic model of an unstable steady state which can be
found... | nlin.CD | timedelayed feedback methods can be used to control unstable periodic orbits as well as unstable steady states we present an application of extended time delay autosynchronization introduced by socolar et al to an unstable focus this system represents a generic model of an unstable steady state which can be found for i... | [['timedelayed', 'feedback', 'methods', 'can', 'be', 'used', 'to', 'control', 'unstable', 'periodic', 'orbits', 'as', 'well', 'as', 'unstable', 'steady', 'states', 'we', 'present', 'an', 'application', 'of', 'extended', 'time', 'delay', 'autosynchronization', 'introduced', 'by', 'socolar', 'et', 'al', 'to', 'an', 'unst... | [-0.18513766348016739, 0.0880447310191812, -0.09307283075558472, 0.0067719278389443485, -0.047078990530029965, -0.14533413099205314, 0.07015085428880913, 0.35734560033145907, -0.2877390484229244, -0.27286600505387215, 0.1498828802402292, -0.18129972491317012, -0.17637483203976317, 0.20699717079546173, -0.08092976668207... |
708.0148 | Modelling the behaviour of accretion flows in X-ray binaries | (abridged) We review how the recent increase in X-ray and radio data from
black hole and neutron star binaries can be merged together with theoretical
advances to give a coherent picture of the physics of the accretion flow in
strong gravity. Both long term X-ray light curves, X-ray spectra, the rapid
X-ray variabili... | astro-ph | abridged we review how the recent increase in xray and radio data from black hole and neutron star binaries can be merged together with theoretical advances to give a coherent picture of the physics of the accretion flow in strong gravity both long term xray light curves xray spectra the rapid xray variability and the ... | [['abridged', 'we', 'review', 'how', 'the', 'recent', 'increase', 'in', 'xray', 'and', 'radio', 'data', 'from', 'black', 'hole', 'and', 'neutron', 'star', 'binaries', 'can', 'be', 'merged', 'together', 'with', 'theoretical', 'advances', 'to', 'give', 'a', 'coherent', 'picture', 'of', 'the', 'physics', 'of', 'the', 'acc... | [-0.08117372305483289, 0.14181770717974135, -0.06912714198601674, 0.13795164813868038, -0.08501119564577606, -0.0913249968410763, -0.0024248532387140934, 0.4069789960965066, -0.20096027136984448, -0.3202790796680197, 0.12949596883646175, -0.30528113694880665, -0.022936858846973437, 0.24007748771532222, -0.0414119692812... |
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