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

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Abstract

Energy levels and oscillator strengths (transition probabilities) have been calculated for transitions among 46 fine-structure levels of the (1s2) 2s22p2, 2s2p3, 2p4, 2s22p3s, 2s22p3p and 2s22p3d 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.

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Aggarwal, K. M., Keenan, F. P., & Msezane, A. Z. (2003). Oscillator strengths for transitions in C-like ions between K XIV and MN XX. Astronomy and Astrophysics, 401(1), 377–383. https://doi.org/10.1051/0004-6361:20030117

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