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dc.contributor.authorAkman, F.
dc.date.accessioned2021-04-08T12:08:30Z
dc.date.available2021-04-08T12:08:30Z
dc.date.issued2016
dc.identifier10.1016/j.apradiso.2016.07.014
dc.identifier.issn09698043
dc.identifier.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-84989285274&doi=10.1016%2fj.apradiso.2016.07.014&partnerID=40&md5=1a3e8962388b971e716de2c94e007468
dc.identifier.urihttp://acikerisim.bingol.edu.tr/handle/20.500.12898/4620
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. © 2016 Elsevier Ltd
dc.language.isoEnglish
dc.sourceApplied Radiation and Isotopes
dc.titleExperimental values of K to Li sub-shell, K to L, and K to M shell vacancy transfer probabilities for some rare earth elements


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