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The energy dependence of the cross sections for both the Kα (one-electron, one-photon) and Kαα (two-electron, one-photon) x-ray emissions for Ni-Ni collisions have been measured in the energy range 17.6-91.5 MeV. To account for these observations, we have extended the electron promotion model to the quantitative, ab initio calculation of double K-shell vacancies. The results furnish, for the first time, an independent test of both the Briggs-Macek formulation of the electron promotion model and the concept of velocity-dependent exit channels suggested by Fastrup et al. We also present, for the first time, a theory of the vacancy-sharing mechanism for double K-shell excitation in symmetric systems. The theoretical results are in quantitative agreement with experiment.
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Greenberg et al. (1977) studied this question.
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