K-shell photoionization of nickel ions using R-matrix

15Citations
Citations of this article
7Readers
Mendeley users who have this article in their library.

Abstract

We present R-matrix calculations of photoabsorption and photoionization cross sections across the K edge of the Li-like to Ca-like ion stages of Ni. Level-resolved, Breit-Pauli calculations were performed for the Li-like to Na-like stages. Term-resolved calculations, which include the mass-velocity and Darwin relativistic corrections, were performed for the Mg-like to Ca-like ion stages. This data set is extended up to Fe-like Ni using the distorted wave approximation as implemented by AUTOSTRUCTURE. The R-matrix calculations include the effects of radiative and Auger dampings by means of an optical potential. The damping processes affect the absorption resonances converging to the K thresholds causing them to display symmetric profiles of constant width that smear the otherwise sharp edge at the K-shell photoionization threshold. These data are important for the modeling of features found in photoionized plasmas. © 2011. The American Astronomical Society. All rights reserved.

Cite

CITATION STYLE

APA

Witthoeft, M. C., Bautista, M. A., García, J., Kallman, T. R., Mendoza, C., Palmeri, P., & Quinet, P. (2011). K-shell photoionization of nickel ions using R-matrix. Astrophysical Journal, Supplement Series, 196(1). https://doi.org/10.1088/0067-0049/196/1/7

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free