Search results for "Electron shell"

showing 8 items of 18 documents

Experimental and theoretical study of thenf-level lifetimes of potassium

2008

The theoretical and experimental values of the 5f ,6 f ,7 f, and 8f radiative lifetimes of neutral potassium are reported. The reduced matrix elements for all allowed electric-dipole nf5/2-nd5/2, nf5/2-nd3/2, and nf7/2-nd5/2 transitions with n =5–8 in K arecalculated using the relativistic linearized coupled-cluster method with single and double excitations of Dirac-Fock wave functions included to all orders in many-body perturbation theory. The resulting electric-dipole matrix elements are used to evaluate the lifetimes of the 5f ,6 f ,7 f, and 8f states in neutral K and their uncertainties. The contributions from the nf5/2-ng7/2, nf7/2-ng7/2, and nf7/2-ng9/2 transitions to the lifetimes o…

PhysicsDipoleElectric dipole momentExcited stateQuadrupoleElectron shellHartree–Fock methodAtomic physicsPerturbation theoryWave functionAtomic and Molecular Physics and OpticsPhysical Review A
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On Relativistic Disk Spectroscopy in Compact Objects with X-ray CCD Cameras

2010

X-ray charge-coupled devices (CCDs) are the workhorse detectors of modern X-ray astronomy. Typically covering the 0.3-10.0 keV energy range, CCDs are able to detect photoelectric absorption edges and K shell lines from most abundant metals. New CCDs also offer resolutions of 30-50 (E/dE), which is sufficient to detect lines in hot plasmas and to resolve many lines shaped by dynamical processes in accretion flows. The spectral capabilities of X-ray CCDs have been particularly important in detecting relativistic emission lines from the inner disks around accreting neutron stars and black holes. One drawback of X-ray CCDs is that spectra can be distorted by photon "pile-up", wherein two or mor…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhotonSpectrometerAstrophysics::High Energy Astrophysical PhenomenaElectron shellFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyRelativistic diskSpectral lineaccretion accretion disks black hole physics instrumentation spectrographs methods analytical X-rays binariesNeutron starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceEmission spectrumAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaSpectroscopyAstrophysics::Galaxy Astrophysics
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Symmetry and Electronic Structure of Noble Metal Nanoparticles and the Role of Relativity

2004

High resolution photoelectron spectra of cold mass selected Cu_n-, Ag_n- and Au_n- with n =53-58 have been measured at a photon energy of 6.42 eV. The observed electron density of states is not the expected simple electron shell structure, but seems to be strongly influenced by electron-lattice interactions. Only Cu55- and Ag55- exhibit highly degenerate states. This is a direct consequence of their icosahedral symmetry, as is confirmed by density functional theory calculations. Neighboring sizes exhibit perturbed electronic structures, as they are formed by removal or addition of atoms to the icosahedron and therefore have lower symmetries. Gold clusters in the same size range show complet…

PhysicsIcosahedral symmetryDegenerate energy levelsElectron shellGeneral Physics and AstronomyFOS: Physical sciencesElectronic structureSpectral lineCondensed Matter - Other Condensed MatterAb initio quantum chemistry methodsDensity of statesDensity functional theoryAtomic physicsOther Condensed Matter (cond-mat.other)
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Spontaneous fission instability of the neutron-deficient No and Rf isotopes: The new isotope No249

2021

In the heaviest elements, the instability of atomic nuclei against spontaneous fission leads to ever shorter nuclear half-lives. Upon falling below a timescale of ${10}^{\ensuremath{-}14}$ s, the border of existence of isotopes is crossed because this is the timescale on which the formation of atomic shells occurs. Analysis of the experimental data on the spontaneous fission half-lives of Rf isotopes in relation with their expected single-particle orbitals hint at a potentially abrupt decrease in half-lives of unknown neutron-deficient Rf isotopes with neutron numbers $l149$, which suggests that the isotopic border is already almost reached. However, this conjecture, which cannot be explain…

PhysicsIsotopeAtomic orbitalFissionAtomic nucleusElectron shellNeutronAtomic physicsNuclear ExperimentSpontaneous fissionLine (formation)Physical Review C
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Positron Production In Heavy-Ion Collisions

1985

Atomic systems with a nuclear charge Z much greater than 100 exhibit a number of unique features not otherwise found in nature. Two characteristic properties are illustrated in Figs. 1 and 2. In Fig. 1 we have plotted the binding energy of a K-shell electron around hypothetical nuclei up to Z ≈ 200. For Z > 150 the binding energy exceeds the rest energy m e c 2 of the electron; i.e., adding the electron to the nucleus actually diminishes the total mass of the system. At the critical charge Z c ≈ 170–175 the binding energy reaches twice the electron rest mass, the threshold for spontaneous creation of an electron-positron pair. As has been discussed extensively in the literature (Pieper and …

PhysicsPhase transitionBinding energyElectron rest massElectron shellCharge (physics)ElectronAtomic physicsGround stateEffective nuclear charge
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Determination of ion-induced K-shell ionization cross sections by comparison with nuclear Coulomb excitation

1979

Abstract A new method for the determination of cross sections for K-shell ionization of heavy atoms by charged particles is proposed. The method is based on a comparison of photon lines due to K X-rays and low-energy γ-rays, the latter ones being produced in nuclear Coulomb excitation with accurately known cross sections. This procedure applies within a limited energy range to the study of targets comprising deformed even nuclei, but can also be extended to other targets having Z≳30. A test of the new technique has been carried out for Gd, W, Th and U natural targets irradiated by 4.75 MeV protons. For Th, also energies of 6.80–10.10 MeV were used. The results are briefly discussed with ref…

PhysicsRange (particle radiation)PhotonIonizationElectron shellNuclear cross sectionGeneral MedicineCoulomb excitationAtomic physicsCharged particleIonNuclear Instruments and Methods
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Superheavy element flerovium (element 114) is a volatile metal.

2014

The electron shell structure of superheavy elements, i.e., elements with atomic number Z ≥ 104, is influenced by strong relativistic effects caused by the high Z. Early atomic calculations on element 112 (copernicium, Cn) and element 114 (flerovium, Fl) having closed and quasi-closed electron shell configurations of 6d(10)7s(2) and 6d(10)7s(2)7p1/2(2), respectively, predicted them to be noble-gas-like due to very strong relativistic effects on the 7s and 7p1/2 valence orbitals. Recent fully relativistic calculations studying Cn and Fl in different environments suggest them to be less reactive compared to their lighter homologues in the groups, but still exhibiting a metallic character. Expe…

Physicsgas chemistryValence (chemistry)ta114Electron shellchemistry.chemical_elementelement 114Inorganic ChemistryFleroviumsuperheavy elementsPhysisorptionchemistryAtomic orbitalChemical physicsSubatomic PhysicsAtomic numberPhysical and Theoretical ChemistryAtomic physicsRelativistic quantum chemistryCoperniciumInorganic chemistry
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Electronic structure and properties of MAu and MOH, where M = Tl and Nh: New data

2018

Abstract Properties of the MAu and MOH (M = Tl and element 113, Nh) molecules were calculated using the 2c-DFT method. The obtained data are needed for evaluation of reactivity of Nh studied by gas-phase chromatography experiments. Results show that Nh should be less reactive (or more volatile) than Tl, both with respect to gold and the hydroxyl group. The reason for that are strong relativistic effects on the valence 7s and 7p electron shells. In difference to the atoms, NhOH may be less volatile than TlOH due to its larger both dipole moment and anisotropic polarizability.

Valence (chemistry)010304 chemical physicsChemistryElectron shellAnalytical chemistryGeneral Physics and AstronomyElectronic structure010402 general chemistry01 natural sciences0104 chemical sciencesDipolePolarizability0103 physical sciencesMoleculePhysical and Theoretical ChemistryAnisotropyRelativistic quantum chemistryChemical Physics Letters
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