作者: H. Enkisch , C. Sternemann , M. Paulus , M. Volmer , W. Schülke
DOI: 10.1103/PHYSREVA.70.022508
关键词:
摘要: The intensity evolution of the Cu K{beta}{sub 1,3} and 2,5} emission spectra is measured as a function excitation energy using resonant inelastic x-ray scattering spectroscopy. contribution 1s3d lowbar shake satellites to well spectrum extracted. Both indicate an additional 1s3p satellites. from threshold saturation compared Thomas model shows similar behavior found for K{alpha}{sub 1,2} satellites, stating that process independent reemission shell. These rapidly reach their limit in contrast 1s2p 1s1s Furthermore, KMN KNN radiative Auger obtained, respectively. satellite shown play important role interpretation valence fluorescence spectra.