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Examination of the Low-Energy Enhancement of the gamma-ray Strength Function of 56Fe

dc.date.accessioned2019-02-18T15:12:11Z
dc.date.available2019-02-18T15:12:11Z
dc.date.created2018-12-17T16:08:15Z
dc.date.issued2018
dc.identifier.citationJones, M.D. Macchiavelli, Augusto Oswaldo Wiedeking, Mathis Bernstein, Lee A. Crawford, Heather L. Campbell, C.M. Clark, Rod M. Cromaz, Mario Fallon, Paul Lee, I-Yang Salathe, M. Wiens, Andreas Ayangeakaa, A.D. Bleuel, Darren L. Bottoni, S. Carpenter, M.P. Davids, H.M. Elson, J. Görgen, Andreas Guttormsen, Magne Sveen Janssens, R.V.F. Kinnison, J.E. Kirsch, Leo Larsen, Ann-Cecilie Lauritsen, Torben Reviol, Walter Sarantites, Demetrios G. Siem, Sunniva Voinov, A.V. Zhu, S. . Examination of the Low-Energy Enhancement of the gamma-ray Strength Function of 56Fe. Physical Review C. 2018, 97(2)
dc.identifier.urihttp://hdl.handle.net/10852/66608
dc.description.abstractA model-independent technique was used to determine the γ -ray strength function ( γ SF ) of 56 Fe down to γ -ray energies less than 1 MeV for the first time with GRETINA using the (p,p′ ) reaction at 16 MeV. No difference was observed in the energy dependence of the γ SF built on 2+ and 4+ final states, supporting the Brink hypothesis. In addition, angular distribution and polarization measurements were performed. The angular distributions are consistent with dipole radiation. The polarization results show a small bias towards magnetic character in the region of the enhancement.en_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleExamination of the Low-Energy Enhancement of the gamma-ray Strength Function of 56Feen_US
dc.typeJournal articleen_US
dc.creator.authorJones, M.D.
dc.creator.authorMacchiavelli, Augusto Oswaldo
dc.creator.authorWiedeking, Mathis
dc.creator.authorBernstein, Lee A.
dc.creator.authorCrawford, Heather L.
dc.creator.authorCampbell, C.M.
dc.creator.authorClark, Rod M.
dc.creator.authorCromaz, Mario
dc.creator.authorFallon, Paul
dc.creator.authorLee, I-Yang
dc.creator.authorSalathe, M.
dc.creator.authorWiens, Andreas
dc.creator.authorAyangeakaa, A.D.
dc.creator.authorBleuel, Darren L.
dc.creator.authorBottoni, S.
dc.creator.authorCarpenter, M.P.
dc.creator.authorDavids, H.M.
dc.creator.authorElson, J.
dc.creator.authorGörgen, Andreas
dc.creator.authorGuttormsen, Magne Sveen
dc.creator.authorJanssens, R.V.F.
dc.creator.authorKinnison, J.E.
dc.creator.authorKirsch, Leo
dc.creator.authorLarsen, Ann-Cecilie
dc.creator.authorLauritsen, Torben
dc.creator.authorReviol, Walter
dc.creator.authorSarantites, Demetrios G.
dc.creator.authorSiem, Sunniva
dc.creator.authorVoinov, A.V.
dc.creator.authorZhu, S.
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1644454
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=97&rft.spage=&rft.date=2018
dc.identifier.jtitlePhysical Review C
dc.identifier.volume97
dc.identifier.issue2
dc.identifier.pagecount6
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevC.97.024327
dc.identifier.urnURN:NBN:no-69816
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn2469-9985
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/66608/2/PhysRevC.97.024327.pdf
dc.type.versionPublishedVersion
cristin.articleid024327
dc.relation.projectEC/H2020/637686


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