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dc.contributor.authorAkman, Ferdi
dc.date.accessioned2016-06-15T05:15:19Z
dc.date.available2016-06-15T05:15:19Z
dc.date.issued2016-05-04
dc.identifier.urihttp://www.nrcresearchpress.com/doi/abs/10.1139/cjp-2016-0097#.V18R4dKLQdU
dc.identifier.urihttp://hdl.handle.net/11472/877
dc.description.abstractThe K to L shell vacancy transfer probabilities for some elements in the atomic range 30 ≤ Z ≤ 58 were determined using the semi-empirical values of K shell fluorescence yield and the experimental values of Kβ/Kα X-ray intensity ratio. Furthermore, the KLX/KLL and KXY/KLL Auger electrons emission ratios for the same elements were obtained using the experimental values of Kβ/Kα X-ray intensity ratio. The experiments were performed using a 241Am annular radioisotope source and a high-resolution Si(Li) semiconductor detector. The experimental values of K to L shell vacancy transfer probabilities, and KLX/KLL and KXY/KLL Auger electrons emission ratios were compared with the fitted, theoretical, semi-empirical, and other available experimental values. To the best knowledge of the author, the KLX/KLL and KXY/KLL Auger electrons emission ratios of ruthenium, palladium, and tellurium have been obtained for the first time in the present work.tr_TR
dc.language.isoengtr_TR
dc.publishernrc research presstr_TR
dc.relation.isversionof10.1139/cjp-2016-0097tr_TR
dc.subjectX-ray production cross sectiontr_TR
dc.subjectX-ray intensity ratiotr_TR
dc.subjectfluorescence yieldtr_TR
dc.subjectvacancy transfer probabilitytr_TR
dc.subjectAuger electrons emission ratestr_TR
dc.titleK to L shell vacancy transfer probabilities and Auger electron emission ratios for elements in the atomic range 30 ≤ Z ≤ 58tr_TR
dc.typeArticletr_TR


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