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Figure 10
The eigenvalue emission spectra (XES) for the Mn Kα 2s and 2p shake-off transitions. These are hypothesized to be the origin of the Kα3,4 satellite. There is not one peak for either of the 2s or 2p satellite spectra; rather, there are 28 366 discrete energy eigenvalues for the 2s satellite transition and 87 966 eigenvalues for the 2p satellite transition. The height represents the relative probability of each eigenvalue within the transition. Each energy eigenvalue experimentally yields a broadened (Lorentzian) profile with area corresponding to the amplitude. This figure details the current best and first theoretical prediction of the complex spectrum observed.

IUCrJ
Volume 11| Part 4| July 2024| Pages 620-633
ISSN: 2052-2525
https://doi.org/10.1107/S2052252524005165