K-shell photoionization of Nickel ions using R-matrix
M.C. Witthoeft, M.A. Bautista, J. Garcia, T.R. Kallman, C. Mendoza, P. Palmeri, P. Quinet
(Submitted on 15 Jul 2011)
We present R-matrix calculations of photoabsorption and photoionization cross sections across the K edge of the Li-like to Ca-like ions 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.
{
"status": "new",
"changetime": "2019-02-04T13:07:06Z",
"_ts": "1549285626580696",
"description": "http://arxiv.org/abs/1107.3146 \n\nK-shell photoionization of Nickel ions using R-matrix\nM.C. Witthoeft, M.A. Bautista, J. Garcia, T.R. Kallman, C. Mendoza, P. Palmeri, P. Quinet\n(Submitted on 15 Jul 2011)\n\n We present R-matrix calculations of photoabsorption and photoionization cross sections across the K edge of the Li-like to Ca-like ions 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. ",
"reporter": "gary",
"cc": "",
"resolution": "",
"time": "2011-07-20T09:48:52Z",
"component": "atomic/molecular data base",
"summary": "Ni inner shell atomic data",
"priority": "good to do",
"keywords": "",
"version": "trunk",
"milestone": "no milestone",
"owner": "nobody",
"type": "enhancement"
}
reported by: @CloudyLex
http://arxiv.org/abs/1107.3146
K-shell photoionization of Nickel ions using R-matrix M.C. Witthoeft, M.A. Bautista, J. Garcia, T.R. Kallman, C. Mendoza, P. Palmeri, P. Quinet (Submitted on 15 Jul 2011)
Migrated from https://www.nublado.org/ticket/212