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dc.date.accessioned2022-03-12T18:19:53Z
dc.date.available2022-03-12T18:19:53Z
dc.date.created2022-02-09T15:39:28Z
dc.date.issued2021
dc.identifier.citationRoux, D.G. Ma, W.C. Hagemann, G.B. Elema, D.R. Fallon, P. Görgen, Andreas Herskind, B. Hübel, H. Marsh, J.C. Sletten, G. Ward, D. Wilson, J. N. . High-spin states and signature inversion in odd-odd Lu 168. Physical Review C. 2021, 103(3)
dc.identifier.urihttp://hdl.handle.net/10852/92395
dc.description.abstractHigh-spin states of the odd-odd nucleus 168Lu were populated in the 123Sb(48Ca,3n)168Lu reaction at a beam energy of 203 MeV and decay γ rays measured using the Gammasphere spectrometer array. The level scheme has been extended from spin 27 to 50 ℏ, and three new rotational bands have been added. A number of interband linking transitions were revealed, so that all but two bands could be connected with each other. High-spin band crossings, above the first νi13/2 alignment, are delineated in most bands. Significant signature inversions are identified for the first time in the bands involving both favored and unfavored signatures of the πh9/2 orbital, which are likely caused by a residual proton-neutron interaction. A signature inversion with small amplitude is also observed in the πd5/2⊗νi13/2 band. Configurations are suggested for all bands based on their experimental properties, with the help of Cranked Shell Model calculations. No evidence is found for triaxial strongly deformed structures that were predicted by the calculations.
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleHigh-spin states and signature inversion in odd-odd Lu 168
dc.typeJournal article
dc.creator.authorRoux, D.G.
dc.creator.authorMa, W.C.
dc.creator.authorHagemann, G.B.
dc.creator.authorElema, D.R.
dc.creator.authorFallon, P.
dc.creator.authorGörgen, Andreas
dc.creator.authorHerskind, B.
dc.creator.authorHübel, H.
dc.creator.authorMarsh, J.C.
dc.creator.authorSletten, G.
dc.creator.authorWard, D.
dc.creator.authorWilson, J. N.
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1999631
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=103&rft.spage=&rft.date=2021
dc.identifier.jtitlePhysical Review C
dc.identifier.volume103
dc.identifier.issue3
dc.identifier.pagecount0
dc.identifier.doihttps://doi.org/10.1103/PhysRevC.103.034326
dc.identifier.urnURN:NBN:no-94991
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn2469-9985
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/92395/1/PhysRevC.103.034326%2B%25281%2529.pdf
dc.type.versionPublishedVersion
cristin.articleid034326


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