Discovery reveals variable many-body effects in K beta emission spectra of manganese, suggesting new modeling approaches.
The discovery of the novel n = 2 satellite transition in the K β emission spectrum of manganese and its evolution with incident photon energy are presented. Using the XR-HERFD (extended-range high-energy-resolution fluorescence detection) technique, we conclusively demonstrate the existence of this phenomenon with a statistical significance corresponding to 652 σ se across the measured spectrum, far above the discovery threshold of 3–6 σ se . We apply principal component analysis (PCA) to the XR-HERFD data to extract advanced structural insights. The evolution of this novel spectral feature and physical process are quantified by incorporating regression, revealing the increase in intensity over a wide range of incident photon energies. We validate these findings through independent test data. These results directly challenge the conventional treatment of the many-body reduction factor S 0 2 as a constant independent of incident photon energy in the standard XAFS (X-ray absorption fine structure) equation. Thereby, these results present compelling evidence that S 0 2 should be modelled as a varying function of incident photon energy, marking the first observation of this behaviour in K β spectra. This facilitates a greater quantitative understanding of HERFD spectra and a comprehensive representation of many-body effects in condensed matter systems.
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Stephens et al. (2025) studied this question.
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