Evolution of KL satellite of F in CaF2

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

doi:10.1002/xrs.607

Evolution of KL satellite of F in CaF₂

M. Uda^*, T. Yamamoto, Y. Ogyu, D. Yamashita, R. C.C. Perera, T. Mukoyama

^*この研究の対応する著者

基幹理工学部

研究成果: Article › 査読

4 被引用数 (Scopus)

抄録

Photoexcited F Kα satellite spectra of CaF₂ 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.

本文言語	English
ページ（範囲）	89-92
ページ数	4
ジャーナル	X-Ray Spectrometry
巻	32
号	2
DOI	https://doi.org/10.1002/xrs.607
出版ステータス	Published - 2003 3月 1

ASJC Scopus subject areas

分光学

文献へのアクセス

10.1002/xrs.607

他のファイルとリンク

引用スタイル

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abstract = "Photoexcited F Kα satellite spectra of CaF2 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.",

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AU - Ogyu, Y.

AU - Yamashita, D.

AU - Perera, R. C.C.

AU - Mukoyama, T.

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AB - Photoexcited F Kα satellite spectra of CaF2 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.

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