Search results for "visti"

showing 10 items of 759 documents

Production altitude and time delays of the terrestrial gamma flashes: Revisiting the Burst and Transient Source Experiment spectra

2008

[1] On the basis of the RHESSI results it has been suggested that terrestrial gamma flashes (TGFs) are produced at very low altitudes. On the other hand some of the Burst and Transient Source Experiment (BATSE) spectra show unabsorbed fluxes of X rays in the 25–50 keV energy range, indicating a higher production altitude. To investigate this, we have developed a Monte Carlo code for X-ray propagation through the atmosphere. The most important features seen in the modeled spectra are (1) a low-energy cutoff which moves to lower energies as TGFs are produced at higher altitudes, (2) a high-energy cutoff which moves to lower energies as TGFs are observed at larger zenith angles, and (3) time d…

PhysicsAtmospheric ScienceEcologyAstrophysics::High Energy Astrophysical PhenomenaCompton scatteringPaleontologySoil ScienceForestryAstrophysicsAquatic ScienceOceanographySpectral lineAtmosphereGeophysicsAltitudeRelativistic runaway electron avalancheSpace and Planetary ScienceGeochemistry and PetrologyPhysics::Space PhysicsEarth and Planetary Sciences (miscellaneous)Atmospheric electricityZenithEarth-Surface ProcessesWater Science and TechnologyTerrestrial gamma-ray flashJournal of Geophysical Research: Space Physics
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Theoretical study of the electron structure of superheavy elements with an open 6d shell: Sg, Bh, Hs, and Mt

2019

We use recently developed efficient versions of the configuration interaction method to perform {\em ab initio} calculations of the spectra of superheavy elements seaborgium (Sg, $Z=106$), bohrium (Bh, $Z=107$), hassium (Hs, $Z=108$) and meitnerium (Mt, $Z=109$). We calculate energy levels, ionization potentials, isotope shifts and electric dipole transition amplitudes. Comparison with lighter analogs reveals significant differences caused by strong relativistic effects in superheavy elements. Very large spin-orbit interaction distinguishes subshells containing orbitals with a definite total electron angular momentum $j$. This effect replaces Hund's rule holding for lighter elements.

PhysicsAtomic Physics (physics.atom-ph)FOS: Physical scienceschemistry.chemical_elementBohriumConfiguration interaction7. Clean energy01 natural sciencesHassiumPhysics - Atomic Physics010305 fluids & plasmasAtomic orbitalchemistryAb initio quantum chemistry methodsSeaborgium0103 physical sciencesPhysics::Atomic PhysicsAtomic physicsElectric dipole transition010306 general physicsRelativistic quantum chemistryPhysical Review A
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Relativistic Kinematics and Phase Space

2015

Here we present a list of the most important formulae needed for calculating relativistic collisions and decays. It includes one-to-two and one-to-three body decays, and the two-to-two scattering process both in the center of mass and laboratory frames. It also includes simplified general formulae of one, two and three-body Lorentz invariant phase space. No explicit calculation is performed, however the reader is highly encouraged to reproduce the results presented here.

PhysicsClassical mechanicsPhase spaceKinematicsScattering processLorentz covarianceCenter of mass (relativistic)Relativistic particle
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The nonadiabatic general-relativistic stellar oscillations

1990

We have derived the equations which govern the linear nonadiabatic general-relativistic radial oscillations. The perturbation produces a heat flux that is coupled with the geometry, through the Einstein field equations of a stellar configuration. The classical limit is recovered. The stability conditions are examined by means of a simplified one-zone model.

PhysicsComputational astrophysicsClassical mechanicsHeat fluxSpace and Planetary ScienceGeneral relativityEinstein field equationsPerturbation (astronomy)Astronomy and AstrophysicsAstrophysics::Earth and Planetary AstrophysicsRelativistic quantum chemistryClassical limitStellar pulsationAstrophysics and Space Science
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Plenty of motion at the bottom: atomically thin liquid gold membrane

2015

The discovery of graphene some ten years ago was the first proof of a free-standing two-dimensional (2D) solid phase. Here, using quantum molecular dynamics simulations of nanoscale gold patches suspended in graphene pores, we predict the existence of an atomically thin, free-standing 2D liquid phase. The liquid phase, enabled by the exceptional planar stability of gold due to relativistic effects, demonstrates extreme fluxionality of metal nanostructures and opens possibilities for a variety of nanoscale phenomena.

PhysicsCondensed Matter - Mesoscale and Nanoscale Physicsta114free-standing 2D liquidGraphenePhysics::OpticsFOS: Physical sciencesNanotechnologygold membranelaw.inventionMembranePlanarquantum molecular dynamics simulationslawPhase (matter)Mesoscale and Nanoscale Physics (cond-mat.mes-hall)Nanoscale PhenomenaGeneral Materials ScienceMetal nanostructuresRelativistic quantum chemistryNanoscopic scaleNanoscale
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Ionization of atoms by slow heavy particles, including dark matter

2016

Atoms and molecules can become ionized during the scattering of a slow, heavy particle off a bound electron. Such an interaction involving leptophilic weakly interacting massive particles (WIMPs) is a promising possible explanation for the anomalous 9 sigma annual modulation in the DAMA dark matter direct detection experiment [R. Bernabei et al., Eur. Phys. J. C 73, 2648 (2013)]. We demonstrate the applicability of the Born approximation for such an interaction by showing its equivalence to the semiclassical adiabatic treatment of atomic ionization by slow-moving WIMPs. Conventional wisdom has it that the ionization probability for such a process should be exponentially small. We show, howe…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)010308 nuclear & particles physicsScatteringDark matterAtoms in moleculesFOS: Physical sciencesGeneral Physics and AstronomyElectron01 natural sciencesAstrophysics - Astrophysics of GalaxiesPhysics - Atomic PhysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics of Galaxies (astro-ph.GA)IonizationWeakly interacting massive particles0103 physical sciencesBorn approximationAtomic physics010306 general physicsRelativistic quantum chemistryAstrophysics - Cosmology and Nongalactic Astrophysics
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Dark matter scattering on electrons: Accurate calculations of atomic excitations and implications for the DAMA signal

2016

We revisit the WIMP-type dark matter scattering on electrons that results in atomic ionization and can manifest itself in a variety of existing direct-detection experiments. Unlike the WIMP-nucleon scattering, where current experiments probe typical interaction strengths much smaller than the Fermi constant, the scattering on electrons requires a much stronger interaction to be detectable, which in turn requires new light force carriers. We account for such new forces explicitly, by introducing a mediator particle with scalar or vector couplings to dark matter and to electrons. We then perform state-of-the-art numerical calculations of atomic ionization relevant to the existing experiments.…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)010308 nuclear & particles physicsScatteringPhysics beyond the Standard ModelDark matterScalar (mathematics)FOS: Physical sciencesElectron01 natural sciencesHigh Energy Physics - ExperimentPhysics - Atomic PhysicsComputational physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Ionization0103 physical sciencesAtomic physics010306 general physicsRelativistic quantum chemistryAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space TelescopePhysical Review D
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Perturbative treatment of scalar-relativistic effects in coupled-cluster calculations of equilibrium geometries and harmonic vibrational frequencies …

2007

An analytic scheme for the computation of scalar-relativistic corrections to nuclear forces is presented. Relativistic corrections are included via a perturbative treatment involving the mass-velocity and the one-electron and two-electron Darwin terms. Such a scheme requires mixed second derivatives of the nonrelativistic energy with respect to the relativistic perturbation and the nuclear coordinates and can be implemented using available second-derivative techniques. Our implementation for Hartree-Fock self-consistent field, second-order Moller-Plesset perturbation theory, as well as the coupled-cluster level is used to investigate the relativistic effects on the geometrical parameters an…

PhysicsCoupled clusterElectronic correlationQuantum electrodynamicsComputationNuclear TheoryGeneral Physics and AstronomyPerturbation (astronomy)Nuclear forcePerturbation theory (quantum mechanics)Physical and Theoretical ChemistryRelativistic quantum chemistrySecond derivativeThe Journal of Chemical Physics
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Relativistic corrections to electrical first-order properties using direct perturbation theory.

2008

Direct perturbation theory (DPT) is applied to compute relativistic corrections to electrical properties such as dipole moment, quadrupole moment, and electric-field gradient. The corrections are obtained as second derivatives of the energy and are given via method-independent expressions that involve the first derivative of the density matrix with respect to the relativistic perturbation as well as property integrals with additional momentum operators. Computational results obtained using Hartree-Fock (HF), second-order Moller-Plesset (MP2) perturbation theory, and the coupled-cluster singles and doubles approach augmented by a perturbative treatment of triple excitations are presented for…

PhysicsDensity matrixDipoleQuantum electrodynamicsQuantum mechanicsQuadrupoleGeneral Physics and AstronomyPerturbation (astronomy)Perturbation theory (quantum mechanics)Physical and Theoretical ChemistryRelativistic quantum chemistryElectron electric dipole momentSecond derivativeThe Journal of chemical physics
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Relativistic corrections in quasi-free electro-disintegration of the deuteron

1992

The role of relativistic effects in deuteron break-up by electrons is investigated for quasi-free kinematics by including the lowest-order relativistic corrections beyond the nonrelativistic limit to electromagnetic operators and by wave-function boost. In particular, the dependence of form factors and structure functions on the frame in which they are calculated is studied. It is found that the inclusion of these corrections leads to observables that are less frame-dependent than for a pure nonrelativistic description. The boost contributions show a decisive influence even though they are small in absolute size. Furthermore, the dependence on the parametrization of the nucleon current in t…

PhysicsDeuteriumQuantum electrodynamicsNuclear TheoryForm factor (quantum field theory)ObservableElectronLimit (mathematics)NucleonRelativistic quantum chemistryParametrizationAtomic and Molecular Physics and OpticsFew-Body Systems
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