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dc.contributor.authorAkman, Ferdi
dc.date.accessioned2016-12-20T05:49:52Z
dc.date.available2016-12-20T05:49:52Z
dc.date.issued2016-09-01
dc.identifier.urihttp://www.sciencedirect.com/science/article/pii/S0969804316303803
dc.identifier.urihttp://hdl.handle.net/11472/1073
dc.description.abstractThe K to Li (i=2,3), K to L, and K to M shell vacancy transfer probabilities for La, Ce, Pr, Nd, Sm, Eu, Gd, Tb, Dy and Er were determined at 59.54 keV using a reflection geometry. The measurements were performed using an 241Am annular radioactive source and a high resolution Si(Li) detector. The experimental results were compared with the theoretical values of Hartree-Slater and Hartree-Fock theories, semi-empirical and other available experimental results in the literature. Reasonable agreement is observed between the measured and theoretical results.tr_TR
dc.language.isoengtr_TR
dc.publisherElseviertr_TR
dc.relation.isversionof10.1016/j.apradiso.2016.07.014tr_TR
dc.subjectX-ray production cross section; X-ray intensity ratio; Fluorescence yield; Vacancy transfer probabilitytr_TR
dc.titleExperimental values of K to Li sub-shell, K to L, and K to M shell vacancy transfer probabilities for some rare earth elementstr_TR
dc.typeArticletr_TR


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