Radiative and Auger decay data for modelling nickel K lines

Details Radiative and Auger decay data for modelling nickel K lines Radiative and Auger decay data for modelling nickel K lines

2008-06-06

arxiv.org/abs/0806.1112v1

Astronomy and Astrophysics

Astrophysics

submitted to ApJS. 42 pages. 12 figures

Scientific paper

10.1086/591965

Radiative and Auger decay data have been calculated for modelling the K lines in ions of the nickel isonuclear sequence, from Ni$^+$ up to Ni$^{27+}$. Level energies, transition wavelengths, radiative transition probabilities, and radiative and Auger widths have been determined using Cowan's Hartree--Fock with Relativistic corrections (HFR) method. Auger widths for the third-row ions (Ni$^+$--Ni$^{10+}$) have been computed using single-configuration average (SCA) compact formulae. Results are compared with data sets computed with the AUTOSTRUCTURE and MCDF atomic structure codes and with available experimental and theoretical values, mainly in highly ionized ions and in the solid state.

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