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The M4,5NO and M4,5NN Auger spectra in Rb have been studied both experimentally and theoretically in order to understand the effect of the outermost 5s electron on the valence-shell hole states in Rb. Transition energies were obtained from extensive multiconfiguration Dirac-Fock calculations and the line intensities from our relativistic single-channel Auger-rate code. The M4,5NO transitions were reproduced by intermediate-coupling calculations quite well indicating that the initial-state correlation with the 5s electron present is weak. For the M4,5NN transitions our single-channel calculations revealed dramatic effects of the 5s electron on the configuration interaction in the final ionic states. Even the most elaborate calculations failed, however, to give a basis for complete identification of the observed spectral features.
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Aksela et al. (1990) studied this question.
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