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

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

2008-04-04

arxiv.org/abs/0804.0623v1

Astronomy and Astrophysics

Astrophysics

31 pages, 5 figures, 2 machine-readable tables

Scientific paper

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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