K-vacancy levels in Ne, Mg, Si, S, Ar, and Ca

P. Palmeri; P. Quinet; C. Mendoza; M. A. Bautista; J. Garcia; T. R. Kallman

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arXiv · 0804.0623

K-vacancy levels in Ne, Mg, Si, S, Ar, and Ca

P. Palmeri·P. Quinet·C. Mendoza·M. A. Bautista·J. Garcia·T. R. Kallman

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Abstract

The HFR and AUTOSTRUCTURE atomic structure codes are used to compute complete data sets of level energies, wavelengths, A-values, and radiative and Auger widths for K-vacancy states of the Ne, Mg, Si, S, Ar, and Ca isonuclear sequences. Ions with electron number N>9 are treated for the first time. Detailed comparisons with previous measurements and theoretical data for ions with N<=9 are carried out in order to estimate reliable accuracy ratings.

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P. Palmeri, P. Quinet, C. Mendoza, M. A. Bautista, J. Garcia, T. R. Kallman. 2008-04-04. K-vacancy levels in Ne, Mg, Si, S, Ar, and Ca. https://arxiv.org/abs/0804.0623

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