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Aggarwal, K., Keenan, F. and Msezane, A. (2003) Oscillator Strengths for Transitions in C-Like Ions between KXIV and MnXX. The Astronomy and Astrophysical Journal, 401, 377-383.

has been cited by the following article:

• TITLE: Theoretical Study of Laser Emission for C-Like (Ar XIII), (Ti XVII) and (Fe XXI)

  AUTHORS: Wessameldin S. Abdelaziz, Th. M. El Sherbeni, Nahed H. Wahba

  KEYWORDS: XUV, Soft X-Ray, Laser Radiation, Population Inversion, Gain Coefficient

  JOURNAL NAME: Open Journal of Applied Sciences, Vol.6 No.4, April 15, 2016

  ABSTRACT: Energy levels, transition probability and oscillator strengths have been calculated for the Ar XIII, Ti XVII and Fe XXI. The configurations included in the calculations are 2s2 2p2, 2s2 2p 3l (l = s, p & d) and 4l (l = s, p, d, & f) of C-like Ar XIII, Ti XVII & Fe XXI which has 69 fine structures by using the fully relativistic flexible atomic code (FAC) program. These data are used in the determination of the reduced population and gain coefficients over a wide range of electron densities from (10+18 to 10+23) and at various plasmas temperatures. The results show that the transitions in Ar18+, Ti22+, and Fe26+ ions are the most promising laser emission lines in the XUV and soft X-ray spectral regions.