Search results for "Number"

showing 10 items of 3939 documents

Lévy distributions and disorder in excitonic spectra.

2020

We study analytically the spectrum of excitons in disordered semiconductors like transition metal dichalcogenides, which are important for photovoltaic and spintronic applications. We show that ambient disorder exerts a strong influence on the exciton spectra. For example, in such a case, the wellknown degeneracy of the hydrogenic problem (related to Runge–Lenz vector conservation) is lifted so that the exciton energy starts to depend on both the principal quantum number n and orbital l. We model the disorder phenomenologically substituting the ordinary Laplacian in the corresponding Schro¨dinger equation by the fractional one with Le´vy index m, characterizing the degree of disorder. Our v…

PhysicsSpintronicsCondensed matter physicsCondensed Matter::Otherbusiness.industryExcitonGeneral Physics and Astronomy02 engineering and technologyCondensed Matter::Mesoscopic Systems and Quantum Hall Effect021001 nanoscience & nanotechnology01 natural sciencesSpectral lineSchrödinger equationCondensed Matter::Materials Sciencesymbols.namesakeSemiconductor0103 physical sciencesPrincipal quantum numbersymbolsPhysical and Theoretical Chemistry010306 general physics0210 nano-technologybusinessDegeneracy (mathematics)Laplace operatorPhysical chemistry chemical physics : PCCP
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Accurate Period Determination of an Eclipsing Binary X-Ray Source in M33

1993

We have analyzed the time variability of one of the X-ray sources in M33 observed by both the ROSAT and Einstein Observatory telescopes. The light curve of M33 X-7 exhibits a variability pattern of high and low states, suggesting an eclipsing binary X-ray source. The data suggest a binary period P=1.78572 days (very close to that of Her X-1) and an eclipse duration of ∼0.4 days. The low phase lasts about one-fourth of the period as in Cen X-3

PhysicsSpiral galaxyEinstein TelescopeSpace and Planetary ScienceBinary starROSATPhase (waves)Binary numberAstronomyAstronomy and AstrophysicsAstrophysicsLight curveEclipseThe Astrophysical Journal
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Nonstandard analysis in classical physics and quantum formal scattering

1988

After a rigorous introduction to hyperreal numbers, we give in terms of non standard analysis, (1) a Lagrangian statement of classical physics, and (2) a statement of formal quantum scattering. © 1988 Plenum Publishing Corporation.

PhysicsStatement (computer science)Physics and Astronomy (miscellaneous)General MathematicsHyperreal numberClassical physicsSchrödinger equationNon-standard analysisField Theory Elementary Particle Quantum Field Theory Standard Analysis Classical Physicsymbols.namesakeAnalytical mechanicssymbolsScattering theoryQuantumSettore MAT/07 - Fisica MatematicaMathematical physics
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Inherent structure entropy of supercooled liquids

1999

We present a quantitative description of the thermodynamics in a supercooled binary Lennard Jones liquid via the evaluation of the degeneracy of the inherent structures, i.e. of the number of potential energy basins in configuration space. We find that for supercooled states, the contribution of the inherent structures to the free energy of the liquid almost completely decouples from the vibrational contribution. An important byproduct of the presented analysis is the determination of the Kauzmann temperature for the studied system. The resulting quantitative picture of the thermodynamics of the inherent structures offers new suggestions for the description of equilibrium and out-of-equilib…

PhysicsStatistical Mechanics (cond-mat.stat-mech)FOS: Physical sciencesGeneral Physics and AstronomyThermodynamicsBinary numberDisordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksCondensed Matter::Disordered Systems and Neural NetworksPotential energyCondensed Matter::Soft Condensed MatterPotential energy landscapeConfiguration spaceSupercoolingCondensed Matter - Statistical Mechanics
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Thermodynamics of supercooled liquids in the inherent structure formalism: a case study

2000

In this article we review the thermodynamics of liquids in the framework of the inherent structure formalism. We then present calculations of the distribution of the basins in the potential energy of a binary Lennard-Jones mixture as a function of temperature. The comparison between the numerical data and the theoretical formalism allows us to evaluate the degeneracy of the inherent structures in a bulk system and to estimate the energy of the lowest energy disordered state (the Kauzmann energy). We find that, around the mode-coupling temperature, the partition function of the liquid is approximated well by the product of two loosely coupled partition functions, one depending on the inheren…

PhysicsStatistical Mechanics (cond-mat.stat-mech)Formalism (philosophy)Structure (category theory)Binary numberThermodynamicsFOS: Physical sciencesFunction (mathematics)Condensed Matter - Soft Condensed MatterPartition function (mathematics)Condensed Matter PhysicsPotential energyDistribution (mathematics)Soft Condensed Matter (cond-mat.soft)General Materials ScienceDegeneracy (mathematics)Condensed Matter - Statistical Mechanics
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Dynamical Heterogeneities Below the Glass Transition

2001

We present molecular dynamics simulations of a binary Lennard-Jones mixture at temperatures below the kinetic glass transition. The ``mobility'' of a particle is characterized by the amplitude of its fluctuation around its average position. The 5% particles with the largest/smallest mean amplitude are thus defined as the relatively most mobile/immobile particles. We investigate for these 5% particles their spatial distribution and find them to be distributed very heterogeneously in that mobile as well as immobile particles form clusters. The reason for this dynamic heterogeneity is traced back to the fact that mobile/immobile particles are surrounded by fewer/more neighbors which form an ef…

PhysicsStatistical Mechanics (cond-mat.stat-mech)General Physics and AstronomyBinary numberFOS: Physical sciencesScale (descriptive set theory)Disordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksCondensed Matter - Soft Condensed MatterKinetic energyMolecular physicsMolecular dynamicsAmplitudePosition (vector)ParticleSoft Condensed Matter (cond-mat.soft)Physical and Theoretical ChemistryGlass transitionCondensed Matter - Statistical Mechanics
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Quantitative tests of mode-coupling theory for fragile and strong glass-formers

2001

We calculate for a binary mixture of Lennard-Jones particles the time dependence of the solution of the mode-coupling equations in which the full wave vector dependence is taken into account. In addition we also take into account the short time dynamics, which we model with a simple memory kernel. We find that the so obtained solution agrees very well with the time and wave vector dependence of the coherent and incoherent intermediate scattering functions as determined from molecular dynamics computer simulations. Furthermore we calculate the wave vector dependence of the Debye-Waller factor for a realistic model of silica and compare these results with the ones obtained from a simulation o…

PhysicsStatistical Mechanics (cond-mat.stat-mech)ScatteringBinary numberFOS: Physical sciencesFunction (mathematics)Disordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsMolecular dynamicsSimple (abstract algebra)Kernel (statistics)Mode couplingMaterials ChemistryCeramics and CompositesWave vectorStatistical physicsCondensed Matter - Statistical Mechanics
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X-ray detection of the substellar twin 2MASS J11011926-7732383 AB

2007

2MASS J11011926-7732383 AB (hereafter 2M1101AB), located in the Cha I star forming region, is a rare wide-separation brown dwarf binary. XMM-Newton and Chandra observations of 2M1101AB have allowed us to examine the influence of physical parameters (mass, bolometric luminosity and effective temperature) on X-ray emission from a coeval pair of substellar objects. The spatial resolution of XMM-Newton is not sufficient to separate contributions from the two components in the binary. The X-ray source detected with XMM-Newton has a column density compatible with the infrared extinction of component A. On the other hand, the binary is resolved with Chandra, and the bulk of the X-ray emission is c…

PhysicsStellar massInfraredAstrophysics::High Energy Astrophysical PhenomenaExtinction (astronomy)Astrophysics (astro-ph)Brown dwarfX-rayBinary numberFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEffective temperatureAstrophysicsLuminositySpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy Astrophysics
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Problems in neutrino physics

1990

The three “known” neutrinos νe νµ and ντ, as well as their postulated heavy companions, have been the subject of intense experimental and theoretical research over the last decade. And yet, all the basic questions that we raised when the first, controversial, results on the mass of electron neutrino from triton beta decay were announced and when the new generation of experiments on lepton family changing processes started, remain essentially unanswered, in spite of the impressive effort that went into neutrino research [1]. So we may just repeat some of these questions and then see what we know about them and what remains to be done.

PhysicsSterile neutrinoParticle physicsSolar neutrinoTau neutrinoMeasurements of neutrino speedNeutrinoSolar neutrino problemNeutrino oscillationLepton number
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Dynamical Density-Matrix Renormalization Group for the Mott--Hubbard insulator in high dimensions

2004

We study the Hubbard model at half band-filling on a Bethe lattice with infinite coordination number in the paramagnetic insulating phase at zero temperature. We use the dynamical mean-field theory (DMFT) mapping to a single-impurity Anderson model with a bath whose properties have to be determined self-consistently. For a controlled and systematic implementation of the self-consistency scheme we use the fixed-energy (FE) approach to the DMFT. In FE-DMFT the onset and the width of the Hubbard bands are adjusted self-consistently but the energies of the bath levels are kept fixed relatively to both band edges during the calculation of self-consistent hybridization strengths between impurity …

PhysicsStrongly Correlated Electrons (cond-mat.str-el)Condensed matter physicsBethe latticeHubbard modelDensity matrix renormalization groupCoordination numberFOS: Physical sciencesRenormalization groupCondensed Matter PhysicsParamagnetismCondensed Matter - Strongly Correlated ElectronsDensity of statesGeneral Materials ScienceCondensed Matter::Strongly Correlated ElectronsAnderson impurity model
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