ESTIMATION OF F-K-ALPHA-K(1)L(1) SATELLITE INTENSITY BASED ON THE MO SCHEME

Authors
MOCHIZUKI M YAMAMOTO T NAGASHIMA S UDA M
Citation
M. Mochizuki et al., ESTIMATION OF F-K-ALPHA-K(1)L(1) SATELLITE INTENSITY BASED ON THE MO SCHEME, Nuclear instruments & methods in physics research. Section B, Beam interactions with materials and atoms, 109, 1996, pp. 31-38
Citations number
28
Categorie Soggetti
Physics, Nuclear","Nuclear Sciences & Tecnology","Instument & Instrumentation
Journal title
Nuclear instruments & methods in physics research. Section B, Beam interactions with materials and atoms → ACNP
ISSN journal
0168583X
Volume
109
Year of publication
1996
Pages
31 - 38
Database
ISI
SICI code
0168-583X(1996)109:<31:EOFSIB>2.0.ZU;2-D
Abstract
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 orb ital scheme. This is the first estimation of the deviation in ionizati on cross sections due to differences in chemical environments. The res ults calculated here can satisfactorily explain a decreasing tendency in the relative intensities (K(1)L(1)/K(1)L(0)) for the observed FK al pha satellite spectra emitted from fluorides, MF(2)(M = Mg, Fe, Co, Ni , Zn), with a rutile structure.