Extended calculations of energy levels, radiative properties, A(J), B-J hyperfine interaction constants, and Lande g(J)-factors for oxygen-like Kr XXIX

Wang, Kai (author): Malmö högskola,Fakulteten för teknik och samhälle (TS),Hebei Key Lab of Optic-electronic Information and Materials, College of Physics Science and Technology, Hebei University, Baoding, 071002, China

Jönsson, Per (author): Malmö högskola,Fakulteten för teknik och samhälle (TS)

Ekman, Jörgen (author): Malmö högskola,Fakulteten för teknik och samhälle (TS)

Si, R. (author): Shanghai EBIT Lab, Institute of Modern Physics, Department of Nuclear Science and Technology, Fudan University, Shanghai, 200433, China

Chen, Z. B. (author): College of Science, National University of Defense Technology, Changsha, 410073, China

Li, Y. G. (author): Hebei Key Lab of Optic-electronic Information and Materials, The College of Physics Science and Technology, Hebei University, Baoding, 071002, China

Chen, C. Y. (author): Shanghai EBIT Lab, Institute of Modern Physics, Department of Nuclear Science and Technology, Fudan University, Shanghai, 200433, China

Yan, J. (author): Institute of Applied Physics and Computational Mathematics, Beijing, 100088, China

(creator_code:org_t)

Elsevier, 2017
2017
English.
In: Journal of Quantitative Spectroscopy and Radiative Transfer. - : Elsevier. - 0022-4073 .- 1879-1352. ; 194, s. 108-112

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Abstract Subject headings

Using the multiconfiguration Dirac-Fock method and the second-order many-body perturbation theory method, highly accurate calculations are performed for the lowest 344 fine-structure levels arising from the 2s(2)2p(4), 2s2p(5), 2p(6), 2s(2)2p(3)3s, 2s(2)2p(3)3p, 2s(2)2p(3)3d, 2s2p(4)3s, 2s2p(4)3p, 2s2p(4)3d, 2p(5)3s, 2p(5)3p, 2p(5)3d, 2s(2)2p(3)4s, 2s(2)2p(3)4p, 2s(2)2p(3)4d, 2s(2)2p(3)4f, and 2s2p(4)4s configurations in O-like Kr XXIX. Complete and consistent atomic data, including excitation energies, lifetimes, wavelengths, hyperfine structures, Lande g(J)-factors, and E1, M1, E2, M2 transition rates, line strengths, and oscillator strengths among these 344 levels are obtained. Comparisons are made between our two different sets of results, as well as with the other available experimental and theoretical values. For O-like Kr only a few levels have been experimentally established. The accuracy of our calculated energies is however high enough to facilitate identifications of observed lines involving the n = 3,4 levels. The calculated data are also useful for modeling and diagnosing fusion plasmas. (C) 2017 Elsevier Ltd. All rights reserved.

By the author/editor: Wang, Kai; Jönsson, Per; Ekman, Jörgen; Si, R.; Chen, Z. B.; Li, Y. G.; show more...; Chen, C. Y.; Yan, J.; show less...

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