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

Simple item page
dc.creatorPalmeri, P.
dc.creatorQuinet, P.
dc.creatorMendoza, C.
dc.creatorBautista, M. A.
dc.creatorGarcia, J.
dc.creatorKallman, T. R.
dc.date2008-04-04
dc.date.accessioned2026-07-07T09:30:24Z
dc.date.available2026-07-07T09:30:24Z
dc.descriptionThe 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.
dc.description31 pages, 5 figures, 2 machine-readable tables
dc.identifierhttps://arxiv.org/abs/0804.0623
dc.identifierhttp://arxiv.org/abs/0804.0623
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/158111
dc.subjectAstrophysics
dc.titleK-vacancy levels in Ne, Mg, Si, S, Ar, and Ca
dc.typetext

Files

Collections

arXiv