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Energy levels and t...
Energy levels and transition rates for the boron isoelectronic sequence : Si X, Ti XVIII – Cu XXV
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- Jönsson, Per (author)
- Malmö högskola,Teknik och samhälle (TS)
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- Ekman, Jörgen (author)
- Malmö högskola,Teknik och samhälle (TS)
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- Gustafsson, Stefan (author)
- Malmö högskola,Teknik och samhälle (TS)
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- Hartman, Henrik (author)
- Malmö högskola,Teknik och samhälle (TS)
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- Karlsson, Lennart (author)
- Malmö högskola,Teknik och samhälle (TS)
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- du Rietz, Rickard (author)
- Malmö högskola,Teknik och samhälle (TS)
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Gaigalas, Gediminas (author)
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Godefroid, Michel (author)
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Froese Fischer, Charlotte (author)
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(creator_code:org_t)
- 2013-11-21
- 2013
- English.
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In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 559
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https://urn.kb.se/re...
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https://doi.org/10.1...
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Abstract
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- Relativistic configuration interaction (RCI) calculations are performed for 291 states belonging to the configurations 1s22s22p, 1s22s2p2, 1s22p3, 1s22s23l, 1s22s2p3l, 1s22p23l, 1s22s24l , 1s22s2p4l , and 1s22p24l (l = 0, 1,2 and l = 0, 1, 2, 3) in boron-like ions Si X and Ti XVIII to Cu XXV. Electron correlation effects are represented in the wave functions by large configuration state function (CSF) expansions. States are transformed from j j-coupling to LS -coupling, and the LS -percentage compositions are used for labeling the levels. Radiative electric dipole transition rates are given for all ions, leading to massive data sets. Calculated energy levels are compared with other theoretical predictions and crosschecked against the Chianti database, NIST recommended values, and other observations. The accuracy of the calculations are high enough to facilitate the identification of observed spectral lines.
Publication and Content Type
- ref (subject category)
- art (subject category)
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