Radiative and Auger Decay of K‐Vacancy Levels in the Ne, Mg, Si, S, Ar, and Ca Isonuclear Sequences | Zendy

P. Palmeri | Zendy; P. Quinet | Zendy; C. Mendoza | Zendy; M. A. Bautista | Zendy; Javier A. García | Zendy; T. R. Kallman | Zendy

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Radiative and Auger Decay of K‐Vacancy Levels in the Ne, Mg, Si, S, Ar, and Ca Isonuclear Sequences

Author(s) -

P. Palmeri,

P. Quinet,

C. Mendoza,

M. A. Bautista,

Javier A. García,

T. R. Kallman

Publication year - 2008

Publication title -

the astrophysical journal supplement series

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 3.546

H-Index - 277

eISSN - 1538-4365

pISSN - 0067-0049

DOI - 10.1086/587804

Subject(s) - auger , vacancy defect , atomic physics , ion , auger effect , radiative transfer , physics , wavelength , auger electron spectroscopy , nuclear physics , optics , nuclear magnetic resonance , quantum mechanics

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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