Relativistic CI calculations of spectroscopic data for the 2p{sup 6} and 2p{sup 5}3l configurations in Ne-like ions between Mg III and Kr XXVII
- School of Technology, Malmö University, 20506 Malmö (Sweden)
- Department of Physics, Vilnius Pedagogical University, Studentu 39, LT-08106 Vilnius (Lithuania)
- National Institute of Standards and Technology Gaithersburg, MD 20899-8420 (United States)
- National Institute for Fusion Science, 322-6 Oroshi-cho, Toki 509-5292 (Japan)
- National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588 (Japan)
- The University of Electro-Communications, Chofu, Tokyo 182-8585 (Japan)
- Chubu University, Kasugai, Aichi 487-8501 (Japan)
Energies, E1, M1, E2, M2 transition rates, oscillator strengths, and lifetimes from relativistic configuration interaction calculations are reported for the states of the 2p{sup 6}, 2p{sup 5}3s, 2p{sup 5}3p, and 2p{sup 5}3d, configurations in all Ne-like ions between Mg III and Kr XXVII. Core–valence and core–core correlation effects are accounted for through single and double excitations to increasing sets of active orbitals. The Breit interaction and leading quantum electrodynamic effects are included as perturbations. The results are compared with experiments and other recent benchmark calculations. In Mg III, Al IV, Si V, P VI, S VII, and Ar IX, for which experimental energies are known to high accuracy, the mean error in the calculated energies is only 0.011%.
- OSTI ID:
- 22237229
- Journal Information:
- Atomic Data and Nuclear Data Tables, Vol. 100, Issue 1; Other Information: Copyright (c) 2013 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.; Country of input: International Atomic Energy Agency (IAEA); ISSN 0092-640X
- Country of Publication:
- United States
- Language:
- English
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