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dc.contributor.authorTurhan, Mehmet Fatih
dc.contributor.authorAkman, Ferdi
dc.contributor.authorKaçal, Mustafa Recep
dc.contributor.authorDurak, Rıdvan
dc.date.accessioned2016-12-20T05:49:09Z
dc.date.available2016-12-20T05:49:09Z
dc.date.issued2016-02-27
dc.identifier.urihttp://hdl.handle.net/11472/1069
dc.description.abstractThe radiative vacancy transfer probabilities from L3 sub-shell to M, N, O sub-shells were measured for the elements Ho, Lu and Hg. To obtain related parameters, we used 59.54 keV gamma photons of 241Am radioactive source. Emitted L X-ray photons from targets were collected by means of a Si(Li) detector with resolution of 160 eV at 5.9 keV. The present results are generally in a good agreement with theoretical calculations and the other results obtained in the literature, within their range considering experimental uncertainty.tr_TR
dc.language.isoengtr_TR
dc.publisherIPCAP 2016tr_TR
dc.titleMeasurement of L3 Sub-Shell to M, N, O Shell Radiative Vacancy Transfer Probabilities for Ho, Lu and Hg Elementstr_TR
dc.typePresentationtr_TR


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