Show simple item record

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


Files in this item

FilesSizeFormatView

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record