• Corpus ID: 100238494

Atomic Data and Nuclear Data Tables

  title={Atomic Data and Nuclear Data Tables},
  author={P. Bogdanovich and Romas Kisielius},
a b s t r a c t The ab initio quasirelativistic Hartree–Fock method developed specifically for the calculation of spectral parameters of heavy atoms and highly charged ions is used to derive transition data for a multicharged tungsten ion. The configuration interaction method is applied to include electron correlation effects. The relativistic effects are taken into account in the Breit–Pauli approximation for quasirelativistic Hartree–Fock radial orbitals. The energy level spectra, radiative… 

Figures and Tables from this paper

Extended Calculations of Energy Levels and Transition Rates for Singly Ionized Lanthanide Elements. I. Pr–Gd
Lanthanide elements play important roles as an opacity source in the ejected material from neutron star mergers. Accurate and complete atomic data are necessary to evaluate the opacities and to
Extended theoretical transition data in C i–iv
Accurate atomic data are essential for opacity calculations and for abundance analyses of the Sun and other stars. The aim of this work is to provide accurate and extensive results of energy levels
Theoretical investigation of energy levels and transition for Ce IV
Aims. We present extensive energy level and transition data for the Ce IV spectrum. By providing accurate atomic data, we evaluate the impact of atomic data on the opacity in the neutron star merger
Comprehensive calculations of energy levels, radiative transition parameters, hyperfine structure constants A$_J$-B$_J$, Land\'e g$_J$ factors and isotope shifts for Sc XX
Large scale calculations for the energy levels, transition rates, oscillator strengths, lifetimes, hyperfine interaction constants, Landé gJ factors, and isotope shift factors have been performed for
Energy Levels and Oscillator Strengths of Ca V
We report an extensive and elaborate theoretical study of excitation energies and radiative data for the lowest 148 fine-structure levels of Sulphur-like Ca using Configuration Interaction Method
Nuclear Polarization and Σ ¯ Atom Energy Levels
Based on SIC-Xα the more rigorous method of calculating the electronic states for Ry dberg exchange parameters using a self-consistent field model, taking into account the Rydberg electron and the
Diverse Trends of Electron Correlation Effects for Properties with Different Radial and Angular Factors in an Atomic System: A case study in Ca$^{+}$
Atomic properties such as field shift constants, magnetic dipole and electric quadrupole hyperfine structure constants, Land\'e $g_J$ factors, and electric quadrupole moments that are described by
Spectroscopic data of Rb-isoelectronic Zr and Nb ions for astrophysical applications
We present high-accuracy spectroscopy data of line strengths, transition probabilities and oscillator strengths for the allowed transitions among the nS1/2, nP1/2,3/2 and n ′D3/2,5/2 states with n =


The Theory of Atomic Structure and Spectra
Both the interpretation of atomic spectra and the application of atomic spectroscopy to current problems in astrophysics, laser physics, and thermonuclear plasmas require a thorough knowledge of the
  • http://www.webnucleo.org/pages/ 42 nse/0.1/
  • 2008
  • J. 511
  • 1999
  • J. 460
  • 1996
  • Astrophys. 529
  • 2011
Acta Phys
  • Polon. B 41
  • 2010
  • Astrophys. 521 28
  • 2010
  • Astrophys. 30 522
  • 2010
The art of writing a scientific article
  • J. Sci. Commun
  • 2010