Abstract

The L-shell X-ray intensity ratios, the production cross-sections, the average L-shell fluorescence yields, the L 3 sub-shell fluorescence yields and the radiative vacancy transfer probabilities from the L 3 sub-shell to the M, N and O sub-shells for heavy elements and their compounds from Ta to Pt were measured. The samples were excited by 59.5 keV γ-rays from a 241Am annular radioactive source. The L X-rays emitted by the samples were counted by an Ultra-LEGe detector with a resolution of 150 eV at 5.9 keV. The experimental values were compared with the theoretical and other experimental values for pure elements.

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