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dc.date.accessioned2023-03-13T17:43:16Z
dc.date.available2023-03-13T17:43:16Z
dc.date.created2022-12-07T09:17:27Z
dc.date.issued2022
dc.identifier.citationIngeberg, Vetle Wegner Jones, P. Msebi, L. Siem, Sunniva Wiedeking, M. Avaa, A.A. Chisapi, M.V. Lawrie, E.A. Malatji, K.L. Makhathini, L. Noncolela, S.P. Shirinda, O. . Nuclear level density and γ-ray strength function of Ni 63. Physical Review C. 2022, 106(5)
dc.identifier.urihttp://hdl.handle.net/10852/101401
dc.description.abstractThe nuclear level density (NLD) and γ-ray strength function (γSF) of 63Ni have been investigated using the Oslo method. The extracted NLD is compared with previous measurements using particle evaporation and those found from neutron resonance spacing. The γSF was found to feature a strong low-energy enhancement that could be explained as M1 strength based on large-scale shell model calculations. Comparison of γSFs measured with the Oslo method for various Ni isotopes reveals systematic changes to the strength below 5MeV with increasing mass.
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleNuclear level density and γ-ray strength function of Ni 63
dc.title.alternativeENEngelskEnglishNuclear level density and γ-ray strength function of Ni 63
dc.typeJournal article
dc.creator.authorIngeberg, Vetle Wegner
dc.creator.authorJones, P.
dc.creator.authorMsebi, L.
dc.creator.authorSiem, Sunniva
dc.creator.authorWiedeking, M.
dc.creator.authorAvaa, A.A.
dc.creator.authorChisapi, M.V.
dc.creator.authorLawrie, E.A.
dc.creator.authorMalatji, K.L.
dc.creator.authorMakhathini, L.
dc.creator.authorNoncolela, S.P.
dc.creator.authorShirinda, O.
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin2089832
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physical Review C&rft.volume=106&rft.spage=&rft.date=2022
dc.identifier.jtitlePhysical Review C
dc.identifier.volume106
dc.identifier.issue5
dc.identifier.pagecount0
dc.identifier.doihttps://doi.org/10.1103/PhysRevC.106.054315
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn2469-9985
dc.type.versionPublishedVersion
cristin.articleid054315


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