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Calculation of M x-ray production cross sections from 1-1500 keV in the atomic region 70 <= Z <= 92

机译:在原子区70 <= Z <= 92中从1-1500 keV计算M x射线产生的横截面

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M x-ray production cross sections from 1 to 1500 keV were obtained for elements with 70 less than or equal to Z less than or equal to 92. Obtained values were tabulated and plotted against the atomic number and energy. In the calculation process, published sources were used. The radiative transition rates and photoionization cross sections of the elements were taken from the relativistic Hartree-Slater model of Scofield (At. Data Nucl. Data Tab. 14, 121 (1974), UCRL-51376 (1973)), the nonradiative transition rates were taken from the Dirac-Hartree-Slater model of Chen et al. (At. Data. Nucl. Data Tab. 24, 14(1979)) and average M shell fluorescence yield values were obtained from Hubbell et al. (J. Phys. Chem. Ref. Data 23, 339 (1994)). Copyright (C) 2004 John Wiley Sons, Ltd.
机译:对于70个小于或等于Z小于或等于92的元素,获得了1至1500 keV的M X射线产生截面。将获得的值制成表格并针对原子序数和能量作图。在计算过程中,使用了已发布的资源。元素的辐射跃迁速率和光电离截面取自Scofield的相对论Hartree-Slater模型(At。Data Nucl。Data Tab。14,121(1974),UCRL-51376(1973)),非辐射跃迁速率摘自Chen等人的Dirac-Hartree-Slater模型。 (At.Data.Nucl.Data Tab.24,14(1979))和平均M壳荧光产率值是从Hubbell等人获得的。 (J.Phys.Chem.Ref.Data 23,339(1994))。版权所有(C)2004 John Wiley Sons,Ltd.

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