Estimation of FKαKLl1 satellite intensity based on the MO scheme

M. Mochizuki; Tomoyuki Yamamoto; S. Nagashima; M. Uda

doi:10.1016/0168-583X(95)00883-7

Estimation of FKαK^Ll¹ satellite intensity based on the MO scheme

M. Mochizuki, Tomoyuki Yamamoto, S. Nagashima, M. Uda

研究成果: Article

5 引用（Scopus）

抜粋

We expanded the theory for the Semi Classical Approximation, which is used for estimating an ionization cross section for an isolated atom, to a form applicable to condensed matters in view of the molecular orbital scheme. This is the first estimation of the deviation in ionization cross sections due to differences in chemical environments. The results calculated here can satisfactorily explain a decreasing tendency in the relative intensities (K¹L¹/K¹L⁰) for the observed FKα satellite spectra emitted from fluorides, MF₂(M = Mg, Fe, Co, Ni, Zn), with a rutile structure.

元の言語	English
ページ（範囲）	31-38
ページ数	8
ジャーナル	Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms
巻	109-110
DOI	https://doi.org/10.1016/0168-583X(95)00883-7
出版物ステータス	Published - 1996 4

フィンガープリント

ASJC Scopus subject areas

Surfaces, Coatings and Films
Instrumentation
Surfaces and Interfaces

これを引用

Mochizuki, M., Yamamoto, T., Nagashima, S., & Uda, M. (1996). Estimation of FKαK^Ll¹ satellite intensity based on the MO scheme. Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms, 109-110, 31-38. https://doi.org/10.1016/0168-583X(95)00883-7

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AU - Nagashima, S.

AU - Uda, M.

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文献にアクセス

10.1016/0168-583X(95)00883-7