L-SHELL AUGER AND COSTER-KRONIG SPECTRA FROM RELATIVISTIC THEORY

被引:9
作者
CHEN, MH
CRASEMANN, B
AOYAGI, M
MARK, H
机构
[1] USAF,WASHINGTON,DC 20330
[2] NASA,AMES RES CTR,MOFFETT FIELD,CA 94035
来源
PHYSICAL REVIEW A | 1979年 / 20卷 / 02期
关键词
D O I
10.1103/PhysRevA.20.385
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The intensities of L-shell Auger and Coster-Kronig transitions in heavy atoms have been calculated relativistically. A detailed comparison is made with measured Auger spectra of Pt and U. The pertinent transition energies were computed from relativistic wave functions with inclusion of the Breit interaction, self-energy, a vacuum-polarization correction, and complete atomic relaxation. Multiplet splitting is found to distribute Auger electrons from certain transitions among several lines. The analysis leads to reassignment of a number of lines in the measured spectra. Lines originally identified as L2-L3Ni in the U spectrum are shown to arise from M4,5 Auger transitions instead. The effect of relativity on L3-MM Auger-transition intensity ratios is studied; in some cases, these ratios are found to be affected by as much as 50% by the inclusion of relativity, while in others the ratios change little. This variation in response can be traced to the different factors through which relativity influences radiationless transition probabilities. © 1979 The American Physical Society.
引用
收藏
页码:385 / 393
页数:9
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