Gorczyca, T. W. and Dumitriu, I. and Hasoglu, M.F. and Korista, K.T. and Badnell, N.R. and Savin, D.W. and Manson, S.T. (2006) Importance of configuration interaction for accurate atomic data : Fluorescence yields of K-shell vacancy, lithium-like ions. Astrophysical Journal, 638 (2). L121-L124. ISSN 0004-637XFull text not available in this repository. (Request a copy from the Strathclyde author)
We demonstrate that the inclusion of configuration interaction (CI) results in significant values for the K-shell fluorescence yields of Li-like ions, which are zero in a single-configuration approach. Modeling codes for simulating supernova remnants under nonequilibrium ionization conditions or photoionized plasmas such as active galactic nuclei or X-ray binaries need to be updated accordingly. A two-parameter fitting formula for the fluorescence yields has been developed. The generality of important CI effects on atomic calculations is pointed out.
|Keywords:||atomic data, atomic processes, line : formation, X-rays , dielectronic satellite spectra, resonant transfer excitation, X-ray emission, cross sections, recombination, photoionization, ionization, photoabsorption, plasma, lines, Physics, Astronomy and Astrophysics, Space and Planetary Science|
|Subjects:||Science > Physics|
|Department:||Faculty of Science > Physics|
|Depositing user:||Pure Administrator|
|Date Deposited:||17 Nov 2011 09:41|
|Last modified:||27 Apr 2016 16:47|