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showing 10 items of 3931 documents

Low-energy excitations from interacting tunneling units in the mean-field approximation

1991

Abstract The low-energy excitation spectrum of dilute concentrations of interacting tunneling quadrupoles randomly distributed in a non-polar medium was studied in the mean-field approximation. In particular the case of six-orientational tunneling quadrupoles (TQs) with a r−3 (elastic) interaction was considered. Because of the random position of the TQs, the internal field in a random variable and for relatively low concentrations has a Lorenzian probability distribution. The low-energy density of states is a constant and the low-energy excitations arise from the large internal fields, i.e. strongly interacting tunneling quadrupoles. The low-energy excitations were compared with those obta…

PhysicsCondensed matter physicsField (physics)Condensed Matter PhysicsElectronic Optical and Magnetic MaterialsMean field theoryMaterials ChemistryCeramics and CompositesDensity of statesVirial expansionProbability distributionAtomic physicsRandom variableQuantum tunnellingExcitationJournal of Non-Crystalline Solids
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Interference pattern and visibility of a Mott insulator

2005

We analyze theoretically the experiment reported in [F. Gerbier et al, cond-mat/0503452], where the interference pattern produced by an expanding atomic cloud in the Mott insulator regime was observed. This interference pattern, indicative of short-range coherence in the system, could be traced back to the presence of a small amount of particle/hole pairs in the insulating phase for finite lattice depths. In this paper, we analyze the influence of these pairs on the interference pattern using a random phase approximation, and derive the corresponding visibility. We also account for the inhomogeneity inherent to atom traps in a local density approximation. The calculations reproduce the expe…

PhysicsCondensed matter physicsMott insulatorFOS: Physical sciencesInterference (wave propagation)01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmasCondensed Matter - Other Condensed MatterRadiation pressureLattice (order)[PHYS.COND.CM-GEN]Physics [physics]/Condensed Matter [cond-mat]/Other [cond-mat.other]0103 physical sciencesAtomLocal-density approximation010306 general physicsRandom phase approximationOther Condensed Matter (cond-mat.other)Coherence (physics)
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General treatment of vortical, toroidal, and compression modes

2011

The multipole vortical, toroidal, and compression modes are analyzed. Following the vorticity concept of Ravenhall and Wambach, the vortical operator is derived and related in a simple way to the toroidal and compression operators. The strength functions and velocity fields of the modes are analyzed in $^{208}$Pb within the random-phase-approximation using the Skyrme force SLy6. Both convection and magnetization nuclear currents are taken into account. It is shown that the isoscalar (isovector) vortical and toroidal modes are dominated by the convection (magnetization) nuclear current while the compression mode is fully convective. The relation between the above concept of the vorticity to …

PhysicsConvectionNuclear and High Energy PhysicsToroidNuclear Theoryta114IsovectorIsoscalarNuclear TheoryFOS: Physical sciencesVorticityNuclear Theory (nucl-th)Physics::Fluid DynamicsClassical mechanicsCondensed Matter::SuperconductivityCompression (functional analysis)Quantum electrodynamicsNuclear Experiment (nucl-ex)Multipole expansionRandom phase approximationNuclear ExperimentPhysical Review C
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A weakly random Universe?

2010

The cosmic microwave background (CMB) radiation is characterized by well-established scales, the 2.7 K temperature of the Planckian spectrum and the $10^{-5}$ amplitude of the temperature anisotropy. These features were instrumental in indicating the hot and equilibrium phases of the early history of the Universe and its large scale isotropy, respectively. We now reveal one more intrinsic scale in CMB properties. We introduce a method developed originally by Kolmogorov, that quantifies a degree of randomness (chaos) in a set of numbers, such as measurements of the CMB temperature in some region. Considering CMB as a composition of random and regular signals, we solve the inverse problem of …

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)530 Physicsmedia_common.quotation_subjectCosmic microwave backgroundIsotropyAstrophysics::Instrumentation and Methods for AstrophysicsCosmic background radiationFOS: Physical sciencesAstronomy and AstrophysicsScale (descriptive set theory)General Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGeneral Relativity and Quantum CosmologyUniverseAmplitude1912 Space and Planetary ScienceSpace and Planetary Science10231 Institute for Computational Science3103 Astronomy and AstrophysicsAnisotropyRandomnessAstrophysics - Cosmology and Nongalactic Astrophysicsmedia_common
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Modeling dark photon oscillations in our inhomogeneous Universe

2020

A dark photon may kinetically mix with the Standard Model photon, leading to observable cosmological signatures. The mixing is resonantly enhanced when the dark photon mass matches the primordial plasma frequency, which depends sensitively on the underlying spatial distribution of electrons. Crucially, inhomogeneities in this distribution can have a significant impact on the nature of resonant conversions. We develop and describe, for the first time, a general analytic formalism to treat resonant oscillations in the presence of inhomogeneities. Our formalism follows from the theory of level crossings of random fields and only requires knowledge of the one-point probability distribution func…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonRandom fieldPhoton conversion010308 nuclear & particles physicsFOS: Physical sciencesObservableProbability density functionElectronAstrophysics::Cosmology and Extragalactic AstrophysicsPlasma oscillation01 natural sciencesDark photonHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum electrodynamics0103 physical sciences010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Spurious finite-size instabilities in nuclear energy density functionals: Spin channel

2015

Background: It has been recently shown that some Skyrme functionals can lead to nonconverging results in the calculation of some properties of atomic nuclei. A previous study has pointed out a possible link between these convergence problems and the appearance of finite-size instabilities in symmetric nuclear matter (SNM) around saturation density. Purpose: We show that the finite-size instabilities not only affect the ground-state properties of atomic nuclei, but they can also influence the calculations of vibrational excited states in finite nuclei. Method: We perform systematic fully-self consistent random phase approximation (RPA) calculations in spherical doubly magic nuclei. We employ…

PhysicsCoupling constantNuclear and High Energy Physics[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear TheoryIsovector010308 nuclear & particles physicsIsoscalarNuclear TheoryFOS: Physical sciencesFísicaNuclear matter01 natural sciencesNuclear Theory (nucl-th)Nuclear physicsMean-fieldMean field theoryQuantum mechanics0103 physical sciencesAtomic nucleusNuclear force010306 general physicsRandom phase approximation
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Statistical analysis ofβdecays and the effective value ofgAin the proton-neutron quasiparticle random-phase approximation framework

2016

We perform a Markov chain Monte Carlo (MCMC) statistical analysis of a number of measured ground-state-to-ground-state single ${\ensuremath{\beta}}^{+}$/electron-capture and ${\ensuremath{\beta}}^{\ensuremath{-}}$ decays in the nuclear mass range of $A=62--142$. The corresponding experimental comparative half-lives ($logft$ values) are compared with the theoretical ones obtained by the use of the proton-neutron quasiparticle random-phase approximation $(pn\mathrm{QRPA})$ with $G$-matrix-based effective interactions. The MCMC analysis is performed separately for 47 isobaric triplets and 28 more extended isobaric chains of nuclei to extract values and uncertainties for the effective axial-vec…

PhysicsCoupling constantParticle physicsProton010308 nuclear & particles physicsNuclear TheoryValue (computer science)01 natural sciences0103 physical sciencesQuasiparticleIsobaric processNeutronBeta (velocity)Atomic physicsNuclear Experiment010306 general physicsRandom phase approximationPhysical Review C
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Euclidean random matrix theory: low-frequency non-analyticities and Rayleigh scattering

2011

By calculating all terms of the high-density expansion of the euclidean random matrix theory (up to second-order in the inverse density) for the vibrational spectrum of a topologically disordered system we show that the low-frequency behavior of the self energy is given by $\Sigma(k,z)\propto k^2z^{d/2}$ and not $\Sigma(k,z)\propto k^2z^{(d-2)/2}$, as claimed previously. This implies the presence of Rayleigh scattering and long-time tails of the velocity autocorrelation function of the analogous diffusion problem of the form $Z(t)\propto t^{(d+2)/2}$.

PhysicsDensity matrixStatistical Mechanics (cond-mat.stat-mech)AutocorrelationFOS: Physical sciencesInverseDisordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural Networks16. Peace & justiceCondensed Matter Physics01 natural sciences010305 fluids & plasmassymbols.namesakeSelf-energyTheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITYQuantum mechanicsPhysical Sciences0103 physical sciencesEuclidean geometrysymbolsRayleigh scatteringDiffusion (business)010306 general physicsRandom matrixCondensed Matter - Statistical MechanicsPhilosophical Magazine
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Measurement of the Dipole Polarizability of the Unstable Neutron-Rich NucleusNi68

2013

The E1 strength distribution in Ni68 has been investigated using Coulomb excitation in inverse kinematics at the RB3-LAND setup and by measuring the invariant mass in the one- and two-neutron decay channels. The giant dipole resonance and a low-lying peak (pygmy dipole resonance) have been observed at 17.1(2) and 9.55(17) MeV, respectively. The measured dipole polarizability is compared to relativistic random phase approximation calculations yielding a neutron-skin thickness of 0.17(2) fm. A method and analysis applicable to neutron-rich nuclei has been developed, allowing for a precise determination of neutron skins in nuclei as a function of neutron excess.

PhysicsDipolePolarizabilityNuclear TheoryTransition dipole momentGeneral Physics and AstronomyResonanceNeutronCoulomb excitationAtomic physicsElectric dipole transitionNuclear ExperimentRandom phase approximationPhysical Review Letters
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Spin-coupling topology in the copper hexamer compounds A2Cu3O(SO4)3 (A=Na, K)

2020

The compounds ${A}_{2}\mathrm{C}{\mathrm{u}}_{3}\mathrm{O}{(\mathrm{S}{\mathrm{O}}_{4})}_{3}$ $(A=\mathrm{Na},\phantom{\rule{0.16em}{0ex}}\mathrm{K})$ are characterized by copper hexamers that are weakly coupled to realize antiferromagnetic order below ${T}_{N}\ensuremath{\approx}3\phantom{\rule{0.16em}{0ex}}\mathrm{K}$. They constitute quantum spin systems with $S=1$ triplet ground states. We investigated the energy-level splittings of the copper hexamers by inelastic neutron scattering experiments covering the entire range of the magnetic excitation spectra. The observed transitions are governed by very unusual selection rules that we ascribe to the underlying spin-coupling topology. This…

PhysicsExcitation spectrachemistry.chemical_elementOrder (ring theory)Coupling topology02 engineering and technologyRandom hexamer021001 nanoscience & nanotechnology01 natural sciencesCopperInelastic neutron scatteringCrystallographychemistry0103 physical sciencesAntiferromagnetism010306 general physics0210 nano-technologySpin (physics)Physical Review B
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