1987
DOI: 10.1088/0022-3700/20/21/029
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Electron impact excitation of rare gases: differential cross sections and angular correlation parameters for neon, argon, krypton and xenon

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Cited by 122 publications
(102 citation statements)
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“…In their model, the spin dependence results from an interplay of exchange between the projectile and ejected target electron, angular-momentum coupling and the impactinduced orientation of the residual ion. The model predicts zero spin asymmetries in the limit of negligible exchange, and in analogy to the "Fine-structure Effect" in excitation [10,11], zero spin asymmetry for the case where the individual finestructure transitions are energetically unresolved. Subsequent measurements on xenon [12,13] and later, more sophisticated calculations [14,15], while confirming a strong spin-dependence in the ionization cross sections as originally predicted, have revealed additional and significant contributions from many-body exchange effects which tend to mask the signatures for a "pure" fine-structure effect.…”
Section: Fine Structure Effectmentioning
confidence: 85%
“…In their model, the spin dependence results from an interplay of exchange between the projectile and ejected target electron, angular-momentum coupling and the impactinduced orientation of the residual ion. The model predicts zero spin asymmetries in the limit of negligible exchange, and in analogy to the "Fine-structure Effect" in excitation [10,11], zero spin asymmetry for the case where the individual finestructure transitions are energetically unresolved. Subsequent measurements on xenon [12,13] and later, more sophisticated calculations [14,15], while confirming a strong spin-dependence in the ionization cross sections as originally predicted, have revealed additional and significant contributions from many-body exchange effects which tend to mask the signatures for a "pure" fine-structure effect.…”
Section: Fine Structure Effectmentioning
confidence: 85%
“…Previous measurements cover only a small scattering regime corresponding primarily to large impact parameters. P3 data have been obtained at an impact energy of 80 eV in Ne [21] which is the only theoretical calculation available at this energy. The agreement between measured data and theoretical prediction is less satisfactory than the level of agreement between experiment and theory for the linear coherence parameters P~ and P2 at the same energy [11 ].…”
Section: Ii1 Results and Discussionmentioning
confidence: 99%
“…A semirelativistic first-order DW approximation (DWBA) was introduced by Madison and Shelton (1973) and later modified by Bartschat and Madison (1987) to treat electron collisions with heavy noble gases and also with mercury. Other variants include the first-order many-body theory (FOMBT) of the Los Alamos group Machado, Leal and Csanak (1982), the semirelativistic version developed and described by Dasgupta, Blaha and Giuliani (2000), and the relativistic distorted-wave (RDW) method of the Toronto group Zuo, McEachran and Stauffer (1991).…”
Section: The Distorted-wave (Dw) Methodsmentioning
confidence: 99%