M sub-shell fluorescence and Coster-Kronig yield data generation for elements, 57 ≤ Z ≤ 90 (computer code 'MFCKYLD')

被引:13
|
作者
Kaur, Gurpreet [1 ]
Mittal, Raj [1 ]
机构
[1] Punjabi Univ, Dept Phys, Nucl Sci Labs, Patiala 147002, Punjab, India
关键词
M sub-shells; Fluorescence yields; Coster-Kronig yields; Relativistic and non-relativistic data; Computer code; TRANSITIONS;
D O I
10.1016/j.jqsrt.2013.09.012
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
M subshell fluorescence yield (omega(Mi), i=1-5) and Coster-Kronig yield (f(Mij), i=1-4, j=2-5) values have been generated for elements with Z, 57 <= Z <= 90. Keeping in view the importance of omega(Mi) and fmu for M X-ray productions in the region Z > 56, the interpolation of non-relativistic data of McGuire [Phys. Rev. A 1972;5:1043-7] in the region Z=57-90 as well as relativistic data of Chen et al. [Phys. Rev. A 1980;21:449-53 and 1983;27:2989-94] in the region Z=67-90 was attempted. The agreement between the generated data and the actual ones supported the adopted procedure. Subsequently, a computer software code MFCKYLD was developed to generate the yield values on computer terminal or in file for both non-relativistic and relativistic data just by entering the atomic number Z of the element through keyboard or file. The precision of present procedure that relies on the deviation of fitted values from the actual ones was found far better than the earlier fitted data. (C) 2013 Elsevier Ltd. All rights reserved.
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页码:489 / 503
页数:15
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