Search results for "Exponent"

showing 10 items of 896 documents

Level statistics and Anderson delocalization in two-dimensional granular materials

2020

Contrary to the theoretical predictions that all waves in two-dimensional disordered materials are localized, Anderson localization is observed only for sufficiently high frequencies in an isotropically jammed two-dimensional disordered granular packing of photoelastic disks. More specifically, we have performed an experiment in analyzing the level statistics of normal mode vibrations. We observe delocalized modes in the low-frequency boson-peak regime and localized modes in the high frequency regime with the crossover frequency just below the Debye frequency. We find that the level-distance distribution obeys Gaussian-Orthogonal-Ensemble (GOE) statistics, i.e. Wigner-Dyson distribution, in…

PhysicsAnderson localizationFOS: Physical sciences02 engineering and technologyCondensed Matter - Soft Condensed Matter021001 nanoscience & nanotechnologyGranular material01 natural sciencesDebye frequencyDelocalized electronNormal mode0103 physical sciencesStatisticsExponentSoft Condensed Matter (cond-mat.soft)010306 general physics0210 nano-technologyScalingAnderson impurity model
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The phase diagram of the multi-dimensional Anderson localization via analytic determination of Lyapunov exponents

2004

The method proposed by the present authors to deal analytically with the problem of Anderson localization via disorder [J.Phys.: Condens. Matter {\bf 14} (2002) 13777] is generalized for higher spatial dimensions D. In this way the generalized Lyapunov exponents for diagonal correlators of the wave function, $$, can be calculated analytically and exactly. This permits to determine the phase diagram of the system. For all dimensions $D > 2$ one finds intervals in the energy and the disorder where extended and localized states coexist: the metal-insulator transition should thus be interpreted as a first-order transition. The qualitative differences permit to group the systems into two classes…

PhysicsAnderson localizationGroup (mathematics)DiagonalFOS: Physical sciencesLyapunov exponentFunction (mathematics)Disordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksCondensed Matter PhysicsElectronic Optical and Magnetic Materialssymbols.namesakePercolationsymbolsCritical dimensionMathematical physicsPhase diagram
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The parameterisation of the atmospheric aerosol optical depth using the Ångström power law

1998

Abstract We have analysed the ability of the Angstrom power law to model the spectral aerosol optical depth, τaλ, for the 400–670 nm band, obtained from spectral direct irradiance measurements at normal incidence. The spectra were registered at ground level in Valencia, Spain, using a Li-cor 1800 spectroradiometer. The results obtained showed that the fitting method that introduces lower errors in the determination of the Angstrom power law coefficients is to adjust directly the spectral experimental data. In this way the errors obtained for the turbidity coefficient, β, were about 0.004 and for the wavelength exponent, α, 0.07. The correlation coefficient was always greater than 0.95. Thes…

PhysicsAngstrom exponentCorrelation coefficientbiologyRenewable Energy Sustainability and the Environmentbusiness.industryIrradiancebiology.organism_classificationPower lawSpectral lineWavelengthOpticsSpectroradiometerGeneral Materials SciencebusinessValenciaSolar Energy
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Blue Moon: Is This a Property of Background Aerosol?

2010

Stellar extinction measurements made at three astronomical observatories showed that on ~50% of the nights the extinction due to aerosol light scattering increased rather than decreased with increasing wavelength (anomalous extinction) for wavelengths close to 500 nm. This extinction behavior is analyzed in this paper and limits are established for the aerosol characteristics necessary for this phenomenon to exist, including geometric standard deviations, imaginary part of refractive index, mean radius, and gaseous NO(2).

PhysicsAngstrom exponentbusiness.industryMaterials Science (miscellaneous)RadiusIndustrial and Manufacturing EngineeringLight scatteringAerosolWavelengthOpticsExtinction (optical mineralogy)Quantitative Biology::Populations and EvolutionAstrophysics::Earth and Planetary AstrophysicsScattering theoryBusiness and International ManagementbusinessRefractive indexAstrophysics::Galaxy AstrophysicsApplied Optics
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Measurement of the Pseudoscalar Decay ConstantfDsUsing Charm-Tagged Events ine+e−Collisions ats=10.58  GeV

2007

Using 230.2 fb^(-1) of e+e- annihilation data collected with the BABAR detector at and near the peak of the Y(4S) resonance, 489 +/- 55 events containing the pure leptonic decay D_s^+ --> mu^+ nu_mu have been isolated in charm-tagged events. The ratio of partial widths Gamma(D_s^+ --> mu^+ nu_mu)/Gamma(D_s^+ --> phi pi^+) is measured to be 0.143 +/- 0.018 +/- 0.006 allowing a determination of the pseudoscalar decay constant f_{D_s} = (283 +/- 17 +/- 7 +/- 14) MeV. The errors are statistical, systematic, and from the D_s^+ --> phi pi^+ branching ratio, respectively.

PhysicsAnnihilation010308 nuclear & particles physicsBranching fractionElectron–positron annihilationGeneral Physics and AstronomyResonanceElectron01 natural sciencesNuclear physicsPseudoscalarPositron0103 physical sciencesExponential decay010306 general physicsPhysical Review Letters
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The relaxation dynamics of a viscous silica melt: II The intermediate scattering functions

2001

We use molecular dynamics computer simulations to study the relaxation dynamics of a viscous melt of silica. The coherent and incoherent intermediate scattering functions, F_d(q,t) and F_s(q,t), show a crossover from a nearly exponential decay at high temperatures to a two-step relaxation at low temperatures. Close to the critical temperature of mode-coupling theory (MCT) the correlators obey in the alpha-regime the time temperature superposition principle (TTSP) and show a weak stretching. We determine the wave-vector dependence of the stretching parameter and find that for F_d(q,t) it shows oscillations which are in phase with the static structure factor. The temperature dependence of the…

PhysicsArrhenius equationCondensed matter physicsStatistical Mechanics (cond-mat.stat-mech)ScatteringThermodynamicsFOS: Physical sciencesDisordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksFick's laws of diffusionPower lawsymbols.namesakeTime–temperature superpositionsymbolsRelaxation (physics)Exponential decayStructure factorCondensed Matter - Statistical Mechanics
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Order in the Chaos: Spin-up and Spin-down during the 2002 Outburst of SAX J1808.4-3658

2006

We present a timing analysis of the 2002 outburst of the accreting millisecond pulsar SAX J1808.4-3658. A study of the phase delays of the entire pulse profile shows a behavior that is surprising and difficult to interpret: superposed to a general trend, a big jump by about 0.2 in phase is visible, starting at day 14 after the beginning of the outburst. An analysis of the pulse profile indicates the presence of a significant first harmonic. Studying the fundamental and the first harmonic separately, we find that the phase delays of the first harmonic are more regular, with no sign of the jump observed in the fundamental. The fitting of the phase delays of the first harmonic with a model whi…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Phase (waves)X-ray binaryFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsPulse (physics)Neutron starPulsarSpace and Planetary ScienceMillisecond pulsarAstrophysics::Solar and Stellar AstrophysicsStars: Pulsars: General Stars: Pulsars: Individual: SAX J1808.4-3658 Stars: Magnetic Fields Stars: Neutron X-Rays: BinariesExponential decaySpin-½
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Visibility forecast in the phase of pre-condensation

1969

The effect on visibility of the swelling of aerosol particles due to increasing humidity is studied. The swelling can be described by r(f)/r (0) = (1 - f ) ?1/? where r ( f ) = particle radius at relative humidity f and ? = const ? 4 on the average. The visibility variation is expressed as V(f)/V(f 0 ) = [(1 - f )/(1 - f 0 )] V * ? 1)/? where V * = exponent of the aerosol size distribution ? 3 on the average. The last formula allows to compute the standard visual range V(f) at relative humidity f from the present standard visual range V(f 0 ) at present relative humidity f 0 . DOI: 10.1111/j.2153-3490.1969.tb00469.x

PhysicsAtmospheric Science010504 meteorology & atmospheric sciencesbusiness.industryCondensationVisibility (geometry)Phase (waves)Analytical chemistryHumidityGeneral MedicineOceanography01 natural sciencesAerosolOpticsVisual rangeExponentRelative humiditybusiness0105 earth and related environmental sciencesTellus A: Dynamic Meteorology and Oceanography
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Calculations and measurements of the spectral radiance of the solar aureole

1968

The application of the theory of primary scattering to describe and interpret the spectral distribution of the sky radiance is discussed. It is shown that within the solar aureole the influence of the scattering of higher order can be neglected. Theoretical calculations of the spectral distribution of the sky radiance, carried out by Bullrich et al . (1965) based on an exponential aerosol size distribution with an upper limiting particle radius r = 10 ?, have been extended to r = 150 ?. The detailed study of the influence of these “giant” particles revealed that aerosol particles of r >30 ? have no effect on the sky radiation any more. Representative measurements taken at Mainz, Germany, at…

PhysicsAtmospheric ScienceAngstrom exponent010504 meteorology & atmospheric sciencesSpectral power distributionMeteorologyScatteringmedia_common.quotation_subjectSubsidence (atmosphere)General MedicineOceanography01 natural sciencesComputational physicsAerosolAtmosphereSkyRadiancePhysics::Atmospheric and Oceanic Physics0105 earth and related environmental sciencesmedia_commonTellus A
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Lifetime measurements of highly excited Rydberg states of strontium I

1993

Lifetimes of Rydberg states of the triplet-series 5s ns3S1 withn = 19–23, 35 and 5s nd3D3 withn = 18–20, 23–28 in the spectrum of neutral strontium have been determined. Observation of the exponential decay after excitation by a pulsed laser in a fast atomic beam and subsequent state-selective field ionization was employed. The lifetimes of the states of the3S1-series show the expectedn*3 dependence on the effective principal quantum number, while the3D3-series is disturbed by configuration mixing. Furthermore, state re-populations induced by black-body radiation have been observed.

PhysicsAtomic and Molecular Physics and Opticssymbols.namesakeIonizationExcited stateField desorptionPrincipal quantum numberRydberg formulasymbolsPhysics::Atomic PhysicsRydberg stateExponential decayAtomic physicsExcitationZeitschrift f�r Physik D Atoms, Molecules and Clusters
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