Search results for "IONIZATION"

showing 10 items of 1255 documents

Warm dark matter and the ionization history of the Universe

2017

In warm dark matter scenarios structure formation is suppressed on small scales with respect to the cold dark matter case, reducing the number of low-mass halos and the fraction of ionized gas at high redshifts and thus, delaying reionization. This has an impact on the ionization history of the Universe and measurements of the optical depth to reionization, of the evolution of the global fraction of ionized gas and of the thermal history of the intergalactic medium, can be used to set constraints on the mass of the dark matter particle. However, the suppression of the fraction of ionized medium in these scenarios can be partly compensated by varying other parameters, as the ionization effic…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cold dark matter010308 nuclear & particles physicsHot dark matterScalar field dark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)13. Climate action0103 physical sciencesMixed dark matterOptical depth (astrophysics)Warm dark matter010303 astronomy & astrophysicsReionizationLight dark matterAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Theory of bound polarons in oxide compounds

2001

We present a multilateral theoretical study of bound polarons in oxide compounds MgO and \alpha-Al_2O_3 (corundum). A continuum theory at arbitrary electron-phonon coupling is used for calculation of the energies of thermal dissociation, photoionization (optically induced release of an electron (hole) from the ground self-consistent state), as well as optical absorption to the non-relaxed excited states. Unlike the case of free strong-coupling polarons, where the ratio \kappa of the photoionization energy to the thermal dissociation energy was shown to be always equal to 3, here this ratio depends on the Froehlich coupling constant \alpha and the screened Coulomb interaction strength \beta.…

PhysicsCoupling constantStrongly Correlated Electrons (cond-mat.str-el)Statistical Mechanics (cond-mat.stat-mech)FOS: Physical sciencesPhotoionizationCoupling (probability)PolaronCondensed Matter - Strongly Correlated ElectronsExcited statePhysics::Atomic and Molecular ClustersAbsorption (logic)Atomic physicsContinuum hypothesisEnergy (signal processing)Condensed Matter - Statistical MechanicsPhysical review : B : condensed matter and materials physics
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Electron energy distribution in the photodetachment ofH−by two radiation fields

1993

We report on the energy distribution of the electrons emitted in two-color photodetachment of ${\mathrm{H}}^{\mathrm{\ensuremath{-}}}$ in a highly nonlinear regime, and compare these results with the ones found by averaging the cross section obtained in the presence of a static field over the values taken by the low-frequency field in a cycle. Similarities and differences are discussed.

PhysicsCross section (physics)Field (physics)IonizationElectronPhotoionizationRadiationAtomic physicsAtomic and Molecular Physics and OpticsCharged particleIonPhysical Review A
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Multicomponent density-functional theory for time-dependent systems

2007

We derive the basic formalism of density functional theory for time-dependent electron-nuclear systems. The basic variables of this theory are the electron density in body-fixed frame coordinates and the diagonal of the nuclear N-body density matrix. The body-fixed frame transformation is carried out in order to achieve an electron density that reflects the internal symmetry of the system. We discuss the implications of this body-fixed frame transformation and establish a Runge-Gross-type theorem and derive Kohn-Sham equations for the electrons and nuclei. We illustrate the formalism by performing calculations on a one-dimensional diatomic molecule for which the many-body Schrodinger equati…

PhysicsDensity matrixElectron densityNONEQUILIBRIUM PROCESSESElectronic correlationDiagonalHartreeNUCLEARDiatomic moleculeFIELDSAtomic and Molecular Physics and OpticsSchrödinger equationPOLYATOMIC-MOLECULESMODELsymbols.namesakeClassical mechanicsLASER-PULSEQuantum mechanicsMOTIONSsymbolsSCHRODINGER-EQUATIONDensity functional theoryDOUBLE-IONIZATIONELECTRON CORRELATIONPhysical Review A
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PNO-CI and CEPA studies of electron correlation effects

1974

Ab initio calculations of the potential curves of low laying electronic states of OH are performed on the basis of a variational configuration interaction wavefunction (PNO-CI) and the coupled electron pair approximation (CEPA). The latter approach yields a ground state potential curve which deviates from the RKR curve by less than 200 cm−1 in the region from 0.7 to 1.6 A. Calculated ground state constants are as follows (experimental values in parentheses): r e = 0.972 (0.971) A, B e = 18.85 (18.87) cm−1, α e = 0.727 (0.714) cm−1, ω e = 3742 (3739) cm−1, ω e χ e = 85.3 (86.4) cm−1, μ0 = 1.686 (1.66) D, D e = 4.35 (4.63) eV,IP = 12.78 (13.36?) eV, El.Aff. = 1.51 (1.83) eV, v 00(2Π↔2Σ+) = 32…

PhysicsDipoleElectron pairElectronic correlationAb initio quantum chemistry methodsIonizationElectron affinityChiropracticsPhysical and Theoretical ChemistryConfiguration interactionAtomic physicsGround stateTheoretica Chimica Acta
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Calculation of atomic spectra and transition amplitudes for superheavy element Db (Z=105)

2018

Atomic spectra and other properties of superheavy element dubnium (Db, $Z=105$) are calculated using recently developed method combining configuration interaction with perturbation theory [the CIPT method, V. A. Dzuba, J. C. Berengut, C. Harabati, and V. V. Flambaum, Phys. Rev. A 95, 012503 (2017)]. These include energy levels for low-lying states of Db and Db II, electric dipole transition amplitudes between the ground state and low-lying states of opposite parity, isotope shift for these transitions, and the ionization potential of Db. Similar calculations for Ta, which is a lighter analog of Db, are performed to control the accuracy of the calculations.

PhysicsDubniumAtomic Physics (physics.atom-ph)FOS: Physical scienceschemistry.chemical_elementConfiguration interaction7. Clean energy01 natural sciences010305 fluids & plasmasPhysics - Atomic PhysicsAmplitudechemistry0103 physical sciencesPhysics::Atomic PhysicsNuclear Experiment (nucl-ex)Atomic physicsElectric dipole transitionIonization energyPerturbation theory010306 general physicsGround stateSpectroscopyNuclear Experiment
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The effect of dynamical screening on helium (e, 3e) differential cross-sections

2005

A simplified derivation of dynamic screening in the case of three Coulomb-interacting particles in the continuum is given and applied to describe the shapes of multi-differential cross-sections for the (e, 3e) process on the helium atom in which the incident fast electron is treated in first-order Born approximation. A very good agreement with experimental multi-differential cross-sections is obtained for two slow ejected electrons (specifically both electrons have 5 eV) but the strategy appears to be breaking down at intermediate emission energies.

PhysicsDynamic screeningHelium atomchemistry.chemical_elementElectronCondensed Matter PhysicsAtomic and Molecular Physics and Opticschemistry.chemical_compoundchemistryBasso continuoAtomic physicsBorn approximationElectron ionizationHeliumJournal of Physics B: Atomic, Molecular and Optical Physics
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On the soft excess in the x-ray spectrum of circinus X-1: Revisitation of the distance to circinus X-1

2005

We report on a 300 ks BeppoSAX (0.12-200 keV) observation of Circinus X-1 (Cir X-1) at phases between 0.62 and 0.84 and on a 90 ks BeppoSAX observation of Cir X-1 at phases 0.11-0.16. Using the canonical model adopted until now to fit the energy spectrum of this source, large residuals appear below 1 keV. These are well fitted using an equivalent hydrogen column of 0.66¿1022 cm-2, adding absorption edges of O VII, O VIII, and Ne IX in the spectra extracted from the observation at phases 0.62-0.84 and adding absorption edges of O VII, O VIII, Mg XI, and Mg XII and absorption lines of O VIII and Mg XII in the spectra extracted from the observation at phases 0.11-0.16. During the observation a…

PhysicsElectron densityAccretionAbsorption spectroscopyStars: Individual: Constellation Name: Circinus X-1Stars: individual (Circinus X-1)Accretion; Accretion Disks; Stars: Individual: Constellation Name: Circinus X-1; Stars: Neutron; X-Rays: Binaries; X-Rays: StarsX-rayAstronomy and Astrophysicsindividual (Circinus X-1); Stars: neutron; X-rays: binaries; X-rays: stars; Nuclear and High Energy Physics; Space and Planetary Science [Accretion accretion disks; Stars]AstrophysicsCompact starX-rays: binarieSpectral lineStars: neutronX-Rays: BinariesAccretion accretion diskSpace and Planetary ScienceIonizationAccretion DisksX-Rays: StarsCircinusX-rays: starAbsorption (logic)Nuclear and High Energy Physic
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Plasma heating power dissipation in low temperature hydrogen plasmas

2015

A theoretical framework for power dissipation in low temperature plasmas in corona equilibrium is developed. The framework is based on fundamental conservation laws and reaction cross sections and is only weakly sensitive to plasma parameters, e.g., electron temperature and density. The theory is applied to low temperature atomic and molecular hydrogen laboratory plasmas for which the plasma heating power dissipation to photon emission, ionization, and chemical potential is calculated. The calculated photon emission is compared to recent experimental results.

PhysicsElectron densityHydrogenta114Plasma parameterslow temperature plasmaspower dissipationchemistry.chemical_elementFOS: Physical sciencesPlasmaDissipationCondensed Matter PhysicsCoronaPhysics - Plasma PhysicsPlasma Physics (physics.plasm-ph)chemistryPhysics::Plasma PhysicsIonizationPhysics::Space Physicshydrogen plasmasElectron temperatureAtomic physicsPhysics of Plasmas
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Phototransition of Na(3p3/2) into high Rydberg states and the ionization continuum

2005

A model potential method is used to investigate photoabsorption from the Na(3p3/2) state. Absorption cross sections into higher Rydberg states and photoionization cross sections are presented as an analytical function of photo electron energy. Einstein coefficients for spontaneous emissions 3p3/2 ← ns1/2, nd5/2, nd3/2 are tabulated for n up to 50. The Einstein coefficients and low-energy ionization cross sections are believed to be accurate to better than 2–3%, above 1 eV the error may increase to 4–6%.

PhysicsElectron energyContinuum (design consultancy)PhotoionizationCondensed Matter PhysicsAtomic and Molecular Physics and Opticssymbols.namesakeEinstein coefficientsIonizationPhysics::Atomic and Molecular ClustersRydberg formulasymbolsSpontaneous emissionAtomic physicsAbsorption (electromagnetic radiation)Journal of Physics B: Atomic, Molecular and Optical Physics
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