Search results for "MBD"

showing 10 items of 646 documents

Test of mode coupling theory for a supercooled liquid of diatomic molecules. II.q-dependent orientational correlators

1997

Using molecular dynamics computer simulations we study the dynamics of a molecular liquid by means of a general class of time-dependent correlators S_{ll'}^m(q,t) which explicitly involve translational (TDOF) and orientational degrees of freedom (ODOF). The system is composed of rigid, linear molecules with Lennard- Jones interactions. The q-dependence of the static correlators S_{ll'}^m(q) strongly depend on l, l' and m. The time dependent correlators are calculated for l=l'. A thorough test of the predictions of mode coupling theory (MCT) is performed for S_{ll}^m(q,t) and its self part S_{ll}^{(s)m}(q,t), for l=1,..,6. We find a clear signature for the existence of a single temperature T…

PhysicsStatistical Mechanics (cond-mat.stat-mech)Degrees of freedom (physics and chemistry)FOS: Physical sciencesLinear molecular geometryDisordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksLambdaOmegaDiatomic moleculeQuantum mechanicsMode couplingExponentSignature (topology)Condensed Matter - Statistical MechanicsPhysical Review E
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High Resolution Spectroscopy ofBΛ12by Electroproduction

2007

An experiment measuring electroproduction of hypernuclei has been performed in Hall A at Jefferson Lab on a $^{12}$C target. In order to increase counting rates and provide unambiguous kaon identification two superconducting septum magnets and a Ring Imaging CHerenkov detector (RICH) were added to the Hall A standard equipment. An unprecedented energy resolution of less than 700 keV FWHM has been achieved. Thus, the observed \lam{12}{B} spectrum shows for the first time identifiable strength in the core-excited region between the ground-state {\it s}-wave $\Lambda$ peak and the 11 MeV {\it p}-wave $\Lambda$ peak.

PhysicsSuperconductivity010308 nuclear & particles physicsResolution (electron density)General Physics and AstronomyOrder (ring theory)Lambda01 natural sciencesRing-imaging Cherenkov detectorNuclear physicsFull width at half maximum0103 physical sciencesNuclear Experiment010306 general physicsSpectroscopyEnergy (signal processing)Physical Review Letters
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A high statistics lattice calculation of the B-meson binding energy

1996

We present a high statistics lattice calculation of the B--meson binding energy $\overline{\Lambda}$ of the heavy--quark inside the pseudoscalar B--meson. Our numerical results have been obtained from several independent numerical simulations at $\beta=6.0$, $6.2$ and $6.4$, and using, for the meson correlators, the results obtained by the APE group at the same values of $\beta$. Our best estimate, obtained by combining results at different values of $\beta$, is $\overline{\Lambda}=180^{+30}_{-20}$ MeV. For the $\overline{MS}$ running mass, we obtain $\overline{m}_{b}(\overline{m}_{b})=4.15 \pm 0.05 \pm 0.20$ GeV, in reasonable agreement with previous determinations. The systematic error is…

PhysicsSystematic errorNuclear and High Energy PhysicsMesonHigh Energy Physics::LatticeBinding energyNuclear TheoryHigh Energy Physics - Lattice (hep-lat)QUARK EFFECTIVE THEORYPerturabation theoryHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaParticle Physics - LatticeLambdaPseudoscalarHigh Energy Physics - PhenomenologyHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)Lattice (order)StatisticsHeavy quark effective theoryB mesonHigh Energy Physics::ExperimentNuclear Experiment
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Cosmological Applications of Extended Electromagnetism

2013

Extended electromagnetism (EE) has been applied to cosmology in various papers. In all of them, the zero order energy density of the EE vector field plays the same role as vacuum energy. Perturbations of this field have been studied by using different approaches. Firstly, some basic equations and ideas are summarized and, then, the CMBFAST code is used to calculate the cosmic microwave background angular power spectrum for appropriate values of the EE parameters. Comparisons of the resulting spectra with a good observational one compatible with WMAP7 (Wilkinson map anisotropy probe 7 years data) seem to be promising. We are currently looking for a set of parameters leading to the best fitti…

PhysicsTheoretical physicsClassical mechanicsField (physics)Vacuum energyElectromagnetismCMBFASTMathematics::History and OverviewCosmic microwave backgroundVector fieldLambda-CDM modelAstrophysics::Cosmology and Extragalactic AstrophysicsCosmology
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Two-photon spectroscopy of mercury and velocity-selective double resonances

2009

Two-photon laser spectroscopy of the $6\text{ }{^{1}S}_{0}\ensuremath{-}7\text{ }{^{1}S}_{0}$ transition in mercury has been performed using two copropagating continuous-wave laser beams. One laser beam is at 254 nm wavelength and can be tuned to the $6\text{ }{^{1}S}_{0}\ensuremath{-}6\text{ }{^{3}P}_{1}$ resonance. The other laser beam is at 408 nm. Two very different regimes can be distinguished, one far off resonance and one near resonance with the one-photon resonance. A resonance which is not Doppler broadened has been observed for low Rabi frequencies. This velocity-selective double resonance in a three-level ladder system is analogous to the dark resonance in three-level $\ensuremat…

PhysicsWavelengthNuclear magnetic resonanceTwo-photon excitation microscopyOff resonanceResonanceAtomic physicsSpectroscopyLambdaAtomic and Molecular Physics and OpticsLaser beamsPhysical Review A
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Large-scale inhomogeneities may improve the cosmic concordance of supernovae

2010

We reanalyze the supernovae data from the Union Compilation including the weak lensing effects caused by inhomogeneities. We compute the lensing probability distribution function for each background solution described by the parameters Omega_M, Omega_L and w in the presence of inhomogeneities, approximately modeled with a single-mass population of halos. We then perform a likelihood analysis in the space of FLRW-parameters and compare our results with the standard approach. We find that the inclusion of lensing can move the best-fit model significantly towards the cosmic concordance of the flat LCDM model, improving the agreement with the constraints coming from the cosmic microwave backgro…

Physicseducation.field_of_studyCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsCosmic microwave backgroundPopulationDark matterGeneral Physics and AstronomyFOS: Physical sciencesLambda-CDM modelAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyObservational cosmology0103 physical sciencesDark energyBaryon acoustic oscillationseducation010303 astronomy & astrophysicsWeak gravitational lensingAstrophysics - Cosmology and Nongalactic Astrophysics
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Topology of adiabatic passage

2002

We examine the topology of eigenenergy surfaces characterizing the population transfer processes based on adiabatic passage. We show that this topology is the essential feature for the analysis of the population transfers and the prediction of its final result. We reinterpret diverse known processes, such as stimulated Raman adiabatic passage (STIRAP), frequency-chirped adiabatic passage and Stark-chirped rapid adiabatic passage. Moreover, using this picture, we display new related possibilities of transfer. In particular, we show that we can selectively control the level that will be populated in STIRAP process in $\ensuremath{\Lambda}$ or V systems by the choice of the peak amplitudes or …

Physicseducation.field_of_studyPopulationStimulated Raman adiabatic passagePulse sequenceLambdaAdiabatic quantum computationTopologyAtomic and Molecular Physics and OpticsAmplitudeQuantum mechanicsPhysics::Atomic and Molecular ClustersAdiabatic processeducationTopology (chemistry)Physical Review A
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Photo-z optimization for measurements of the BAO radial scale

2009

ArXiv pre-print avaible at:http://arxiv.org/abs/0812.3414

PopulationAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicspower spectrumLambda01 natural sciencesComputer Science::Digital LibrariesSpectral lineComputer Science::Computational Engineering Finance and Science0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicseducation010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhotometric redshiftPhysicseducation.field_of_study010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsShot noiseAstronomy and Astrophysicssuveys of galaxiesRedshiftGalaxyAstronomiaAstrophysics::Earth and Planetary AstrophysicsBaryon acoustic oscillations
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The behavior of solutions of a parametric weighted (p, q)-laplacian equation

2021

<abstract><p>We study the behavior of solutions for the parametric equation</p> <p><disp-formula> <label/> <tex-math id="FE1"> \begin{document}$ -\Delta_{p}^{a_1} u(z)-\Delta_{q}^{a_2} u(z) = \lambda |u(z)|^{q-2} u(z)+f(z,u(z)) \quad \mbox{in } \Omega,\, \lambda >0, $\end{document} </tex-math></disp-formula></p> <p>under Dirichlet condition, where $ \Omega \subseteq \mathbb{R}^N $ is a bounded domain with a $ C^2 $-boundary $ \partial \Omega $, $ a_1, a_2 \in L^\infty(\Omega) $ with $ a_1(z), a_2(z) > 0 $ for a.a. $ z \in \Omega $, $ p, q \in (1, \infty) $ and $ \Delta_{p}^{a_1}, \Delta_{q}^{a_2} $ are weighted …

Positive and negative solutionsGeneral MathematicsNodal solutionsLambdaOmegaCombinatoricssymbols.namesakeMathematics - Analysis of PDEsSettore MAT/05 - Analisi MatematicaQA1-939FOS: Mathematicspositive and negative solutionsResonant Carathéodory functionudc:517.956Physics35J20 35J60Spectrum (functional analysis)weighted (pWeighted (p q)-LaplacianDifferential operatorresonant Carathéodory functionweighted (pq)-LaplacianDirichlet boundary conditionBounded functionq)-laplacianDomain (ring theory)symbolsnodal solutionsParametric power termLaplace operatorMathematicsparametric power termAnalysis of PDEs (math.AP)
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Statistical properties of the site-frequency spectrum associated with lambda-coalescents.

2013

Abstract Statistical properties of the site-frequency spectrum associated with Λ-coalescents are our objects of study. In particular, we derive recursions for the expected value, variance, and covariance of the spectrum, extending earlier results of Fu (1995) for the classical Kingman coalescent. Estimating coalescent parameters introduced by certain Λ-coalescents for data sets too large for full-likelihood methods is our focus. The recursions for the expected values we obtain can be used to find the parameter values that give the best fit to the observed frequency spectrum. The expected values are also used to approximate the probability a (derived) mutation arises on a branch subtending a…

PseudolikelihoodMaleAquatic OrganismsInferenceExpected valueBiologyInvestigationsLambdaDNA MitochondrialCoalescent theoryGeneticsQuantitative Biology::Populations and EvolutionAnimalsComputer SimulationGeneticsPopulation DensityLikelihood FunctionsModels StatisticalModels GeneticReproductionCovarianceFrequency spectrumFertilityGenetics PopulationGadus morhuaSample size determinationMutationFemaleGenetics
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