1983
DOI: 10.1088/0022-3700/16/17/008
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Shake theory predictions of excited-state populations following 1s ionisation in argon

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Cited by 47 publications
(32 citation statements)
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“…The results show that in the asymptotic limit the shakeoff channel prevails over the shakeup. This is consistent with the previous result of Armen [14] and is in contrast with the theoretical prediction by Dyall [20]. The ½1s3p shakeoff threshold energy was found at 3236:3 AE 0:7 eV and ½1s3p4p; 5p shakeup edges at 3228:56 AE 0:04 eV and 3233:43 AE 0:08 eV, respectively.…”
Section: Fig 1 (Color Online)supporting
confidence: 90%
“…The results show that in the asymptotic limit the shakeoff channel prevails over the shakeup. This is consistent with the previous result of Armen [14] and is in contrast with the theoretical prediction by Dyall [20]. The ½1s3p shakeoff threshold energy was found at 3236:3 AE 0:7 eV and ½1s3p4p; 5p shakeup edges at 3228:56 AE 0:04 eV and 3233:43 AE 0:08 eV, respectively.…”
Section: Fig 1 (Color Online)supporting
confidence: 90%
“…The continuous rise of the curve from zero at threshold is an indication that the satellites originate in a SO, rather than SU, process, since the later results in an intensity jump at the threshold (Å berg, 1972;Armen et al, 1985;Deutsch et al, 1996;Fritsch et al, 1998;Heiser et al, 1994). This is in full accord with the predicted intensity contribution of p1% (Deutsch et al, 1996;Fritsch et al, 1998) for SU in our case, as extrapolated from RMCDF calculations for Ar (Dyall, 1983;Mukoyama and Ito, 1994) and Kr (Wark et al, 1991). Note, however, that a KO process, the crosssection of which also rises continuously from zero, could also be a possible contributor.…”
Section: Article In Presssupporting
confidence: 89%
“…There have been dozens of experimental and theoretical investigations into the shake processes [17][18][19][20][21][22][23][24][25][26][27][28][29], and several advanced relativistic quantum mechanical techniques have been applied to characteristic diagram lines [30] or fewelectron scattering [31,32], though only Mukoyama [22] and Kochur [24] have performed ab initio calculations for the difficult transition metals. Due to both the experimental and computational difficulties involved in identifying satellite intensities empirically, there has been little comparison with experimental results in open-shell atoms.…”
mentioning
confidence: 99%