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dc.date.accessioned2017-08-15T13:49:36Z
dc.date.available2017-08-15T13:49:36Z
dc.date.created2013-05-17T20:27:19Z
dc.date.issued2013
dc.identifier.citationLarsen, Ann-Cecilie Bürger, Alexander Goriely, Stephane Guttormsen, Magne Sveen Görgen, Andreas Hagen, Trine Wiborg Harrisopulos, Sotirios Nyhus, Hilde-Therese Renstrøm, Therese Schiller, Andreas Ulrich Siem, Sunniva Tveten, Gry Merete Voinov, Alexander Wiedeking, Mathis Ruud, Inger Eli . Transitional γ strength in Cd isotopes. Physical Review C. Nuclear Physics. 2013, 87(1)
dc.identifier.urihttp://hdl.handle.net/10852/57059
dc.description.abstractThe level densities and γ-ray strength functions of 105,106,111,112Cd have been extracted from particle-γ coincidence data using the Oslo method. The level densities are in very good agreement with known levels at low excitation energy. The γ-ray strength functions display no strong enhancement for low γ energies. However, more low-energy strength is apparent for 105,106Cd than for 111,112Cd. For γ energies above ≈4 MeV, there is evidence for some extra strength, similar to what has been previously observed for the Sn isotopes. The origin of this extra strength is unclear; it might be due to E1 and M1 transitions originating from neutron skin oscillations or the spin-flip resonance, respectively. © 2013 American Physical Societyen_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleTransitional γ strength in Cd isotopesen_US
dc.typeJournal articleen_US
dc.creator.authorLarsen, Ann-Cecilie
dc.creator.authorBürger, Alexander
dc.creator.authorGoriely, Stephane
dc.creator.authorGuttormsen, Magne Sveen
dc.creator.authorGörgen, Andreas
dc.creator.authorHagen, Trine Wiborg
dc.creator.authorHarrisopulos, Sotirios
dc.creator.authorNyhus, Hilde-Therese
dc.creator.authorRenstrøm, Therese
dc.creator.authorSchiller, Andreas Ulrich
dc.creator.authorSiem, Sunniva
dc.creator.authorTveten, Gry Merete
dc.creator.authorVoinov, Alexander
dc.creator.authorWiedeking, Mathis
dc.creator.authorRuud, Inger Eli
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1029069
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. Nuclear Physics&rft.volume=87&rft.spage=&rft.date=2013
dc.identifier.jtitlePhysical Review C. Nuclear Physics
dc.identifier.volume87
dc.identifier.issue1
dc.identifier.pagecount10
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevC.87.014319
dc.identifier.urnURN:NBN:no-59760
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0556-2813
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/57059/1/PhysRevC.87.014319.pdf
dc.type.versionPublishedVersion
cristin.articleid014319


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