K-vacancy levels in Ne, Mg, Si, S, Ar, and Ca
Astrophysics
2008-04-07 v1
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.
Cite
@article{arxiv.0804.0623,
title = {K-vacancy levels in Ne, Mg, Si, S, Ar, and Ca},
author = {P. Palmeri and P. Quinet and C. Mendoza and M. A. Bautista and J. Garcia and T. R. Kallman},
journal= {arXiv preprint arXiv:0804.0623},
year = {2008}
}
Comments
31 pages, 5 figures, 2 machine-readable tables