Abstract
Abstract We report on the evolution of L 3 – and L 2 – M 45 M 45 Auger spectral regions in Cu and CuO as a function of photon energy used to create the initial hole states. It is shown that the satellite features in Auger spectra are completely suppressed close to the threshold; intensities of these satellites increase dramatically when photon energy is swept through deeper core level thresholds. We discuss various decay channels responsible for the spectral features in the L 23 – M 45 M 45 regions of Cu and CuO and obtain quantitative estimates for their contributions to the total spectrum.
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