Abstract
Aims. In this paper we report on calculations of energy levels, radiative rates, oscillator strengths, line strengths, and effective collision strengths for transitions among the lowest 362 levels of the (1s22s22p6) 3s23p5, 3s3p6, 3s23p43d, 3s3p53d, 3s23p33d2, 3s3p43d2, 3p63d,
and 3s23p44 configurations of Cr viii.
Methods. The general-purpose relativistic atomic structure package (grasp) and flexible atomic code (fac) are adopted for the
calculations.
Results. Radiative rates, oscillator strengths, and line strengths are reported for all electric dipole (E1), magnetic dipole (M1), electric
quadrupole (E2), and magnetic quadrupole (M2) transitions among the 362 levels. Comparisons are made with earlier available results
and the accuracy of the data is assessed. Additionally, lifetimes for all 362 levels are listed, although comparisons with other theoretical
results are limited to only a few levels. Our energy levels are estimated to be accurate to better than 3% (within 0.4 Ryd), whereas
results for other parameters are probably accurate to better than 20%. Finally, electron impact collision strengths and excitation rates
are computed for all transitions over a wide energy (temperature) range. For these calculations, FAC is adopted and results in the form
of effective collision strengths are reported over a wide temperature range of 105.0−106.6 K.
Original language | English |
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Pages (from-to) | 1501-1509 |
Journal | Astronomy and Astrophysics |
Volume | 506 |
DOIs | |
Publication status | Published - 02 Nov 2009 |
ASJC Scopus subject areas
- Space and Planetary Science
- Astronomy and Astrophysics