Title:
Electron-impact Ionization of P-like Ions Forming Si-like Ions
Authors:
Kwon, D.-H.; Savin, D. W.
Affiliation:
AA(Nuclear Data Center, Korea Atomic Energy Research Institute, Daejeon 305-353, Korea hkwon@kaeri.re.kr), AB(Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA)
Publication:
The Astrophysical Journal, Volume 784, Issue 1, article id. 13, 7 pp. (2014). (ApJ Homepage)
Publication Date:
03/2014
Origin:
IOP
Astronomy Keywords:
atomic data, atomic processes
DOI:
10.1088/0004-637X/784/1/13
Bibliographic Code:
2014ApJ...784...13K
Abstract
We have calculated electron-impact ionization (EII) for P-like systems from P to
Zn15 + forming Si-like ions. The work was performed using the flexible atomic
code (FAC) which is based on a distorted-wave approximation. All 3l ? nl' (n = 3-
35) excitation-autoionization (EA) channels near the 3p direct ionization threshold
and 2l ? nl' (n = 3-10) EA channels at the higher energies are included. Close
attention has been paid to the detailed branching ratios. Our calculated total EII
cross sections are compared both with previous FAC calculations, which omitted
many of these EA channels, and with the available experimental results. Moreover,
for Fe11 +, we find that part of the remaining discrepancies between our
calculations and recent measurements can be accounted for by the inclusion of the
resonant excitation double autoionization process. Lastly, at the temperatures
where each ion is predicted to peak in abundances in collisional ionization
equilibrium, the Maxwellian rate coefficients derived from our calculations differ by
50%-7% from the previous FAC rate coefficients, with the difference decreasing with
increasing charge.
{
"status": "new",
"changetime": "2019-02-04T13:07:06Z",
"_ts": "1549285626580696",
"description": "{{{\nTitle:\t\nElectron-impact Ionization of P-like Ions Forming Si-like Ions\nAuthors:\t\nKwon, D.-H.; Savin, D. W.\nAffiliation:\t\nAA(Nuclear Data Center, Korea Atomic Energy Research Institute, Daejeon 305-353, Korea hkwon@kaeri.re.kr), AB(Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA)\nPublication:\t\nThe Astrophysical Journal, Volume 784, Issue 1, article id. 13, 7 pp. (2014). (ApJ Homepage)\nPublication Date:\t\n03/2014\nOrigin:\t\nIOP\nAstronomy Keywords:\t\natomic data, atomic processes\nDOI:\t\n10.1088/0004-637X/784/1/13\nBibliographic Code:\t\n2014ApJ...784...13K\nAbstract\n\nWe have calculated electron-impact ionization (EII) for P-like systems from P to \nZn15 + forming Si-like ions. The work was performed using the flexible atomic \ncode (FAC) which is based on a distorted-wave approximation. All 3l ? nl' (n = 3-\n35) excitation-autoionization (EA) channels near the 3p direct ionization threshold \nand 2l ? nl' (n = 3-10) EA channels at the higher energies are included. Close \nattention has been paid to the detailed branching ratios. Our calculated total EII \ncross sections are compared both with previous FAC calculations, which omitted \nmany of these EA channels, and with the available experimental results. Moreover,\nfor Fe11 +, we find that part of the remaining discrepancies between our \ncalculations and recent measurements can be accounted for by the inclusion of the\nresonant excitation double autoionization process. Lastly, at the temperatures \nwhere each ion is predicted to peak in abundances in collisional ionization \nequilibrium, the Maxwellian rate coefficients derived from our calculations differ by\n50%-7% from the previous FAC rate coefficients, with the difference decreasing with\nincreasing charge.\n}}}",
"reporter": "gary",
"cc": "",
"resolution": "",
"time": "2014-03-19T14:08:41Z",
"component": "atomic/molecular data base",
"summary": "collisional ionization rate coefficients",
"priority": "good to do",
"keywords": "",
"version": "trunk",
"milestone": "no milestone",
"owner": "nobody",
"type": "enhancement"
}
reported by: @CloudyLex
Migrated from https://www.nublado.org/ticket/277