K-shell photoionization and photoabsorption of Ne, Mg, Si, S, Ar, and Ca

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Abstract

We present extensive computations of photoabsorption and photoionization cross sections across the K-edge of Ne, Mg, Si, S, Ar, and Ca ions with less than 11 electrons. The calculations are performed using the Breit-Pauli R-matrix method and include the effects of radiative and Auger damping by means of an optical potential. The wave functions are constructed from single-electron orbital bases obtained using a Thomas-Fermi-Dirac statistical model potential. Configuration interaction is considered among all fine-structure levels within the n = 2 complex. The damping processes affect the resonances converging to the K thresholds causing them to display symmetric profiles of constant width that smear the otherwise sharp edge at the photoionization thresholds. © 2009. The American Astronomical Society. All rights reserved.

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Witthoeft, M. C., Bautista, M. A., Mendoza, C., Kallman, T. R., Palmeri, P., & Quinet, P. (2009). K-shell photoionization and photoabsorption of Ne, Mg, Si, S, Ar, and Ca. Astrophysical Journal, Supplement Series, 182(1), 127–130. https://doi.org/10.1088/0067-0049/182/1/127

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