Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1834175 | Atomic Data and Nuclear Data Tables | 2006 | 19 Pages |
Abstract
We have calculated fine-structure energy levels, oscillator strengths and transition probabilities for transitions among the terms belonging to the 1s22s22p6ns (2S), 1s22s22p6np (2P), 1s22s22p6nd (2D) (n = 3, 4, 5), and 1s22s22p6nf (2F) (n = 4, 5) configurations. The calculations are based upon the general configuration-interaction code CIV3 of Hibbert which uses orthonormal orbitals of radial functions expressed as superpositions of normalized Slater-type orbitals. Our calculated values are compared with experimental and other theoretical results where a satisfactory agreement is found. We also report on some unpublished energy values and oscillator strengths.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
W.O. Younis, S.H. Allam, Th.M. El-Sherbini,