2019
DOI: 10.1016/j.cplett.2018.11.058
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Study the effect of crystal structure on radiative vacancy transfer probabilities from L3 to Mi, Ni and Oi subshells

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Cited by 7 publications
(4 citation statements)
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“…Consequently, the Coster-Kronig transition probabilities would modify the intensities of L X-ray photons. For such situations, the expressions for L X-ray intensities are given by Equations 12 in Equations (17), (19) and (20), the L subshell fluorescence yield ratios (ω 2 /ω 3, ω 1 /ω 3 , ω 1 /ω 2) have been determined and they are given in Table 3. The derivation of L subshell fluorescence yield ratios (ω 2 /ω 3, ω 1 /ω 3, ω 1 /ω 2 ) from intensity ratios mainly come from L α , L β , L γ groups.…”
Section: Resultsmentioning
confidence: 99%
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“…Consequently, the Coster-Kronig transition probabilities would modify the intensities of L X-ray photons. For such situations, the expressions for L X-ray intensities are given by Equations 12 in Equations (17), (19) and (20), the L subshell fluorescence yield ratios (ω 2 /ω 3, ω 1 /ω 3 , ω 1 /ω 2) have been determined and they are given in Table 3. The derivation of L subshell fluorescence yield ratios (ω 2 /ω 3, ω 1 /ω 3, ω 1 /ω 2 ) from intensity ratios mainly come from L α , L β , L γ groups.…”
Section: Resultsmentioning
confidence: 99%
“…The L β group originates from vacancies in L 3 , L 2 and L 1 subshell, and L γ group originates from vacancies in L 2 and L 1 subshell. The intensities of L α L β , L γ are used to determine the L subshell fluorescence yield ratios (ω 2 /ω 3, ω 1 /ω 3, ω 1 /ω 2 ) in accordance with Equations (17), (19) and (20). In Table 3, and ratios of L subshell fluorescence yield (ω 2 /ω 3, ω 1 /ω 3, ω 1 /ω 2 ) are 2.4-3.4% and 4-7%, respectively.…”
Section: Resultsmentioning
confidence: 99%
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