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- W2059403908 endingPage "2317" @default.
- W2059403908 startingPage "2313" @default.
- W2059403908 abstract "Using recently calculated values of radiative, Coster-Kronig, and Auger transition rates, and the hypothesis that the satellite structure arises from doubly ionized atoms (with $L$ and $N$ holes), and an assumed incident x-ray spectrum, we calculate the relative intensities of the Ag $L$-series x-ray spectrum. The calculations are in best agreement with Parratt's measurements when Ag ${L}_{1}ensuremath{-}{L}_{3}{M}_{4,5}$ Coster-Kronig transitions are forbidden. Comparison of the calculations with the satellite components leads to unsatisfactory agreement. Reasons for this are discussed. Modified values of ${f}_{12}$, ${f}_{13}$, and ${ensuremath{omega}}_{1}$ for the Ag and Sn $L$ shells are reported." @default.
- W2059403908 created "2016-06-24" @default.
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- W2059403908 date "1972-06-01" @default.
- W2059403908 modified "2023-09-25" @default.
- W2059403908 title "Origin of the SilverL-Series X-Ray Spectrum" @default.
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- W2059403908 doi "https://doi.org/10.1103/physreva.5.2313" @default.
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