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dc.date.accessioned2020-05-12T19:40:27Z
dc.date.available2020-05-12T19:40:27Z
dc.date.created2019-06-03T21:36:57Z
dc.date.issued2019
dc.identifier.citationNaqvi, F. Simon, Anna Guttormsen, Magne Sveen Schwengner, R Frauendorf, S Reingold, C. S. Burke, J. T. Cooper, N Hughes, R.O. Ota, S Saastamoinen, A . Nuclear level densities and γ-ray strength functions in samarium isotopes. Physical Review C. 2019, 99(5)
dc.identifier.urihttp://hdl.handle.net/10852/75515
dc.description.abstractThe γ -strength functions and level densities in the quasicontinuum of 147 , 149 Sm isotopes have been extracted from particle- γ coincidences using the Oslo method. The nuclei of interest were populated via (p,d) reactions on pure 148 , 150 Sm targets and the reaction products were recorded by the Hyperion array. An upbend in the low-energy region of the γ SF has been observed. The systematic analysis of the γ SF for a range of Sm isotopes highlights the interplay between scissors mode and the upbend. Shell-model calculations show reasonable agreement with the experimental γ SFs and confirm the correspondence between the upbend and scissors mode.en_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleNuclear level densities and γ-ray strength functions in samarium isotopesen_US
dc.typeJournal articleen_US
dc.creator.authorNaqvi, F.
dc.creator.authorSimon, Anna
dc.creator.authorGuttormsen, Magne Sveen
dc.creator.authorSchwengner, R
dc.creator.authorFrauendorf, S
dc.creator.authorReingold, C. S.
dc.creator.authorBurke, J. T.
dc.creator.authorCooper, N
dc.creator.authorHughes, R.O.
dc.creator.authorOta, S
dc.creator.authorSaastamoinen, A
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1702427
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=99&rft.spage=&rft.date=2019
dc.identifier.jtitlePhysical Review C
dc.identifier.volume99
dc.identifier.issue5
dc.identifier.pagecount8
dc.identifier.doihttps://doi.org/10.1103/PhysRevC.99.054331
dc.identifier.urnURN:NBN:no-78623
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn2469-9985
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/75515/1/PhysRevC.99.054331.pdf
dc.type.versionPublishedVersion
cristin.articleid054331


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