State-of-the-art MCDF calculations plus a Lorentzian-Gaussian overlap model reproduce Cu Kα satellite intensity evolution near threshold, attributing below-edge intensity to Cu(I)/Cu(II) oxide resonances.
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Theoretical ab initio Evolution of Satellite Intensity near Threshold for Cu K-shell transitions
State-of-the-art MCDF calculations plus a Lorentzian-Gaussian overlap model reproduce Cu Kα satellite intensity evolution near threshold, attributing below-edge intensity to Cu(I)/Cu(II) oxide resonances.