The impact-parameter dependence of K-vacancy production in Ta, Au, Bi and U by 4 MeV protons has been measured using a magnetic spectrometer and fast coincidence techniques. The ionization probabilities are greater than non-relativistic SCA predictions by as much as a factor of four. The inclusion of relativistic electronic wavefunctions in the SCA calculations substantially reduces the discrepancies.
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Clark et al. (1975) studied this question.
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