Hafnium to thorium M-shell X-ray production cross sections by proton impact

被引:3
|
作者
Deghfel, B. [1 ,2 ]
Kahoul, A. [2 ,3 ,4 ]
Nekkab, M. [1 ,2 ]
机构
[1] Univ Msila, Fac Sci, Phys Dept, Msila 28000, Algeria
[2] Univ Ferhat Abbas, Fac Sci, Phys Dept, LESIMS Lab, Setif 19000, Algeria
[3] Univ Bordj Bou Arreridj, Fac Sci & Technol, Dept Mat Sci, Bordj Bou Arreridj 34000, Algeria
[4] Bordj Bou Arreridj Univ, Fac Sci & Technol, Dept Mat Sci, LPMRN Lab, Bordj Bou Arreridj 34030, Algeria
关键词
M-shell X-ray production cross sections; ECPSSR theory; Semi-empirical and empirical cross sections;
D O I
10.1016/j.jrras.2014.08.008
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Theoretical M-shell X-ray production cross sections have been calculated within the ECPSSR model. The semi-empirical cross sections are then deduced by fitting the available experimental data normalized to their corresponding theoretical values for elements with 72 <= Z <= 90 by proton in the energy range 0.1-4.0 MeV. Also, an analytical formula has been used to calculate the empirical X-ray production cross sections by direct fitting of the same experimental data, which are found to be universal, both for individual and collective fits. On the other hand, based on the individual fitting which gives the reliable cross sections, we attempt to deduce another new empirical cross sections by assuming that the ratio empirical to ECPSSR of the cross sections is roughly the same for all elements. In addition, our results are presented for selected heavy elements, namely W-74, Au-79 and Bi-83, being the most extensively studied. Finally, a comparison is made between the different procedures followed here and the experimental data. Copyright (C) 2014, The Egyptian Society of Radiation Sciences and Applications. Production and hosting by Elsevier B.V. All rights reserved.
引用
收藏
页码:512 / 518
页数:7
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