Evolution of KL satellite of F in CaF 2 | Zendy

Uda M. | Zendy; Yamamoto T. | Zendy; Ogyu Y. | Zendy; Yamashita D. | Zendy; Perera R. C. C. | Zendy; Mukoyama T. | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Premium

Evolution of KL satellite of F in CaF 2

Author(s) -

Uda M.,

Yamamoto T.,

Ogyu Y.,

Yamashita D.,

Perera R. C. C.,

Mukoyama T.

Publication year - 2003

Publication title -

x‐ray spectrometry

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.447

H-Index - 45

eISSN - 1097-4539

pISSN - 0049-8246

DOI - 10.1002/xrs.607

Subject(s) - excitation , satellite , atomic physics , spectral line , line (geometry) , physics , monotonic function , energy (signal processing) , intensity (physics) , excitation function , chemistry , computational physics , optics , quantum mechanics , mathematics , mathematical analysis , geometry , astronomy

Photoexcited F Kα satellite spectra of CaF 2 were studied as a function of excitation energy from threshold. The observed spectra show that the intensity evolution of the KL satellite line is not a monotonic function increasing with excitation energy, in contrast to the prediction from the conventional shake model, but has a small bump. Comparison with the Hartree–Fock calculations indicates that the origin of the bump can be ascribed to resonances of multi‐electron excitation processes in photoabsorption. Copyright © 2003 John Wiley & Sons, Ltd.

This content is not available in your region!

Continue researching here.

Having issues? You can contact us here

Accelerating Research