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• W2040808323 endingPage "1169" @default.
• W2040808323 startingPage "1165" @default.
• W2040808323 abstract "Partial $L$-shell fluorescence yields of 23 heavy elements have been measured using an x-ray coincidence counting method. Vacancies in the $K$ shell of the target atoms are created by photoelectric absorption of 122- and 136-keV gamma rays emitted by a ${mathrm{Co}}^{57}$ source. A known fraction of these $K$-shell vacancies are filled by $L$ electrons. The $L$-shell vacancies created in this way are then occupied by electrons from higher shells, causing emission of $L$ x rays and Auger electrons. The coincidence rate between the $L$ and $K$ x rays determines the fluorescence yield ${ensuremath{omega}}_{mathrm{KL}}$, which is defined as the partial $L$-shell fluorescence yield following the emission of ${K}_{ensuremath{alpha}}$ x rays. ${ensuremath{omega}}_{mathrm{KL}}$ is a linear combination of the fluorescence yields of the ${L}_{mathrm{II}}$ and ${L}_{mathrm{III}}$ subshells. A comprehensive comparison with previous measurements is given." @default.
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• W2040808323 date "1963-08-01" @default.
• W2040808323 modified "2023-10-17" @default.
• W2040808323 title "<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mi>L</mml:mi></mml:math>-Shell Fluorescence Yields in Heavy Elements" @default.
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• W2040808323 doi "https://doi.org/10.1103/physrev.131.1165" @default.
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