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Energies and E1, M1, E2, and M2 transition rates for states of the 2s22p4, 2s2p5, and 2p6configurations in oxygen-like ions between F II and Kr XXIX.

Published

Author(s)

P. Rynkun, P. Jonsson, G. Gaigalas, Charlotte F. Fischer

Abstract

Based on relativistic wave functions from multiconfiguration Dirac-Hartree-Fock and configuration interaction calculations, E1, M1, E2, M2 transition rates, weighted oscillator strengths, and lifetimes are evaluated for the states of the (1s2)2s22p4; 2s2p5, and 2p6 configurations in all oxygen-like ions between F II and Kr XXIX. Valence, core-valence, and core-core correlation e ects were accounted for through single-double multireference (SD-MR) expansions to increasing sets of active orbitals. Computed energies are compared with the NIST recommended values, generally di ering by less than 600 cm..1. For some spectra, significantly larger di erences are found and our results are in better agreement with Edlén values. For levels where experimental lifetimes are available, the agreement is within experimental uncertainty for all but a few lowly ionized spectra. Complete Online tables of energy levels and transition data are available.
Citation
Astronomy & Astrophysics
Volume
557

Keywords

O-like ions, energies, lifetimes, transition rates, weighted oscillator strengths

Citation

Rynkun, P. , Jonsson, P. , Gaigalas, G. and Fischer, C. (2013), Energies and E1, M1, E2, and M2 transition rates for states of the 2s22p4, 2s2p5, and 2p6configurations in oxygen-like ions between F II and Kr XXIX., Astronomy & Astrophysics, [online], https://doi.org/10.1051/0004-6361/201321992 (Accessed June 16, 2024)

Issues

If you have any questions about this publication or are having problems accessing it, please contact reflib@nist.gov.

Created September 24, 2013, Updated July 3, 2023