cloudy-astrophysics / bug-tracker-migration-test

Trial run for importing the nublado.org Trac tickets as GitHub issues
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collisional ionization rate coefficients (trac #277) #279

Open cloudy-bot opened 10 years ago

cloudy-bot commented 10 years ago

reported by: @CloudyLex

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.

Migrated from https://www.nublado.org/ticket/277

{
    "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"
}
cloudy-bot commented 10 years ago

@peter-van-hoof-noaccount changed milestone from "" to "no milestone"