Oscillator strengths for transitions in C-like ions between K XIV and Mn XX


Autoria(s): Keenan, Francis; Aggarwal, Kanti; Msezane, A.Z.
Data(s)

01/04/2003

Resumo

Energy levels and oscillator strengths (transition probabilities) have been calculated for transitions among 46 fine-structure levels of the (1s(2)) 2s(2) 2p(2), 2s2p(3),2p(4), 2s(2)2p3s, 2s(2) 2p3p and 2s(2)2p3d configurations of C-like K XIV, Sc XVI, Ti XVII, V XVIII, Cr XIX and Mn XX using the GRASP code. Configuration interaction and relativistic effects have been included while generating the wavefunctions. Calculated values of energy levels agree within 3% with the experimentally compiled results, and the length and velocity forms of oscillator strengths agree within 20% for a majority of allowed transitions.

Identificador

http://pure.qub.ac.uk/portal/en/publications/oscillator-strengths-for-transitions-in-clike-ions-between-k-xiv-and-mn-xx(eb282b5d-e14b-413b-9726-c71718ecc35f).html

http://www.scopus.com/inward/record.url?scp=0037382164&partnerID=8YFLogxK

Idioma(s)

eng

Direitos

info:eu-repo/semantics/restrictedAccess

Fonte

Keenan , F , Aggarwal , K & Msezane , A Z 2003 , ' Oscillator strengths for transitions in C-like ions between K XIV and Mn XX ' Astronomy and Astrophysics , vol 401 , no. 1 , pp. 377-383 .

Palavras-Chave #/dk/atira/pure/subjectarea/asjc/1900/1912 #Space and Planetary Science
Tipo

article