Measurements of radiative vacancy transfer probabilities from L3 subshells to M, N and O shells and subshells in the atomic range 72≤Z≤92

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The probabilities of vacancy transfer, ηL3M, ηL 3M1, ηL3M4, ηL 3M5, ηL3N, ηL3N1, ηL3N4, ηL3N5, ηL 3O1 and ηL3O4,5 from L 3 subshell to M, N and O shells and subshells for the elements Hf, Ta, W, Re, Pt, Au, HgO, Tl, Pb, Bi, Th, U have been measured using L shell fluorescence yields and X-ray intensity ratios. These experimental values were obtained from samples excited by 59.5-keV γ-rays, which were emitted from an 241Am radioisotope source. Also K and L X-rays emitted from samples were measured by means of Si(Li) detector with a resolution of 155 at 5.9 keV. The results obtained from this study are compared with the results of other studies. © 2008 Elsevier Ltd. All rights reserved.

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AlanDeğerDil
dc.contributor.authorTuzluca, F.
dc.contributor.authorSöǧüt, Ö.
dc.contributor.authorBüyükkasap, E.
dc.contributor.authorDurdu, B.G.
dc.contributor.authorKüc-ükönder, A.
dc.date.accessioned2026-10-18T20:30:59.656462498Z
dc.date.available2026-10-18T20:30:59.656462498Z
dc.date.issued2008
dc.description.abstractThe probabilities of vacancy transfer, ηL3M, ηL 3M1, ηL3M4, ηL 3M5, ηL3N, ηL3N1, ηL3N4, ηL3N5, ηL 3O1 and ηL3O4,5 from L 3 subshell to M, N and O shells and subshells for the elements Hf, Ta, W, Re, Pt, Au, HgO, Tl, Pb, Bi, Th, U have been measured using L shell fluorescence yields and X-ray intensity ratios. These experimental values were obtained from samples excited by 59.5-keV γ-rays, which were emitted from an 241Am radioisotope source. Also K and L X-rays emitted from samples were measured by means of Si(Li) detector with a resolution of 155 at 5.9 keV. The results obtained from this study are compared with the results of other studies. © 2008 Elsevier Ltd. All rights reserved.
dc.identifier.doi10.1016/j.radphyschem.2008.05.005
dc.identifier.endpage1001
dc.identifier.issn0969-806X
dc.identifier.issue9
dc.identifier.scopus2-s2.0-54049089541
dc.identifier.startpage996
dc.identifier.urihttps://rdlopen.rawdatalibrary.net/r/ebyu/16191
dc.identifier.volume77
dc.identifier.wosWOS:000260203500002
dc.language.isoen
dc.publisherElsevier Ltd
dc.relation.ispartofRadiation Physics and Chemistry
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectFluorescence yield and radiative transition
dc.subjectIntensity ratio
dc.subjectVacancy transition
dc.subjectX-ray
dc.subjectFluorescence
dc.subjectGold
dc.subjectLead
dc.subjectUranium
dc.subjectX rays
dc.subjectamericium 241
dc.subjectbismuth
dc.subjectmercuric oxide
dc.subjectplatinum
dc.subjecttantalum
dc.subjectthallium
dc.subjectthorium
dc.subjecttungsten
dc.subjectExperimental values
dc.subjectL shell fluorescence
dc.subjectRadiative vacancy transfer
dc.subjectRadioisotope sources
dc.subjectX-ray intensity ratios
dc.subjectarticle
dc.subjectfluorescence analysis
dc.subjectgamma radiation
dc.subjectmathematical model
dc.subjectradiation scattering
dc.subjectX ray analysis
dc.subjectGamma rays
dc.titleMeasurements of radiative vacancy transfer probabilities from L3 subshells to M, N and O shells and subshells in the atomic range 72≤Z≤92
dc.typeArticle
dspace.entity.typePublication
rdl.citation.scopus16
rdl.citation.wos16
rdl.source.indexSCOPUS
rdl.source.indexWOS
rdl.wos.indexScience Citation Index Expanded (SCI-EXPANDED)