Relativistic configuration interaction calculations have been performed for Mo VI 4p5 4d2 J=5/2 and nf 2F5/2 (n=4–6) wavefunctions. Level energies and E1 oscillator strengths for transitions between these states and the nd2D (n=4–6) states have been obtained. The calculated LS compositions of all 11 levels of 4p5 4d2 J=5/2 have been found to be in good agreement with other designations. While most calculated level energies agree well with the most recent experimental work, large discrepancies in a few (upper) levels do exist. The oscillator strength of all 84 transitions are computed, and 36 of the largest (f \u3e 0.001) are presented here. Most of the oscillator strengths are computed for the first time
Relativistic configuration-interaction (RCI) calculations with ∼15 000 vectors have been done for f ...
Energy levels, oscillator strengths and transition probabilities for dipole-allowed transitions amon...
A parametric study of the energy levels of the Xe I configurations 5 p5(6s + 5d) and 5p5(6p + 7p), a...
Relativistic Configuration Interaction results are obtained for the lowest 9 J = 0 even parity and t...
The bottom three J = 1 K II levels are nearly degenerate, leading to strong interactions among them,...
Relativistic Configuration Interaction calculations are reported for Zr III and Nb IV J = 0 → J = 1 ...
Relativistic Configuration Interaction calculations are reported for Zr III and Nb IV J = 0 → J = 1 ...
Energy levels and oscillator strengths (transition probabilities) have been calculated for transitio...
The spectrum of Kr VI was recorded in the 23-254-nm-wavelength range, resulting in 109 new line clas...
Aims. Accurate atomic data for Ti II are essential for abundance analyses in astronomical objects. T...
Relativistic configuration interaction hyperfine constants (HFC) have been obtained for all 5[Formul...
In this dissertation, the relativistic configuration interaction (RCI) method has been applied to so...
Excitation energies from ground state for 97 fine-structure levels as well as oscillator strengths ...
Energies, E1, M1, E2, M2 transition rates, oscillator strengths, and lifetimes from relativistic con...
The weighted oscillator strengths (gf), presented in this work, were carried out in a Multiconfigura...
Relativistic configuration-interaction (RCI) calculations with ∼15 000 vectors have been done for f ...
Energy levels, oscillator strengths and transition probabilities for dipole-allowed transitions amon...
A parametric study of the energy levels of the Xe I configurations 5 p5(6s + 5d) and 5p5(6p + 7p), a...
Relativistic Configuration Interaction results are obtained for the lowest 9 J = 0 even parity and t...
The bottom three J = 1 K II levels are nearly degenerate, leading to strong interactions among them,...
Relativistic Configuration Interaction calculations are reported for Zr III and Nb IV J = 0 → J = 1 ...
Relativistic Configuration Interaction calculations are reported for Zr III and Nb IV J = 0 → J = 1 ...
Energy levels and oscillator strengths (transition probabilities) have been calculated for transitio...
The spectrum of Kr VI was recorded in the 23-254-nm-wavelength range, resulting in 109 new line clas...
Aims. Accurate atomic data for Ti II are essential for abundance analyses in astronomical objects. T...
Relativistic configuration interaction hyperfine constants (HFC) have been obtained for all 5[Formul...
In this dissertation, the relativistic configuration interaction (RCI) method has been applied to so...
Excitation energies from ground state for 97 fine-structure levels as well as oscillator strengths ...
Energies, E1, M1, E2, M2 transition rates, oscillator strengths, and lifetimes from relativistic con...
The weighted oscillator strengths (gf), presented in this work, were carried out in a Multiconfigura...
Relativistic configuration-interaction (RCI) calculations with ∼15 000 vectors have been done for f ...
Energy levels, oscillator strengths and transition probabilities for dipole-allowed transitions amon...
A parametric study of the energy levels of the Xe I configurations 5 p5(6s + 5d) and 5p5(6p + 7p), a...