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dc.date.accessioned2017-08-15T13:52:51Z
dc.date.available2017-08-15T13:52:51Z
dc.date.created2013-10-27T02:28:07Z
dc.date.issued2013
dc.identifier.citationKoehler, Paul Edward Larsen, Ann-Cecilie Guttormsen, Magne Sveen Siem, Sunniva Guber, K. H. . Extreme nonstatistical effects in γ decay of 95Mo neutron resonances. Physical Review C. Nuclear Physics. 2013, 88(4)
dc.identifier.urihttp://hdl.handle.net/10852/57061
dc.description.abstractWe demonstrate that high-quality total radiation width (Γγ) data are a virtually untapped resource for testing and improving nuclear models. To this end, we obtained unprecedentedly large sets of Γγ values for all six s- and p-wave Jπ values for 95Mo neutron resonances. We show that Γγ distributions simulated in the framework of the nuclear statistical model are in sharp disagreement with the data. Simulations modified to include doorway effects resulted in much better agreement. These results call into question the reliability of the nuclear statistical model. © 2013 American Physical Societyen_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleExtreme nonstatistical effects in γ decay of 95Mo neutron resonancesen_US
dc.typeJournal articleen_US
dc.creator.authorKoehler, Paul Edward
dc.creator.authorLarsen, Ann-Cecilie
dc.creator.authorGuttormsen, Magne Sveen
dc.creator.authorSiem, Sunniva
dc.creator.authorGuber, K. H.
cristin.unitcode185,15,4,0
cristin.unitnameFysisk institutt
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1060597
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=88&rft.spage=&rft.date=2013
dc.identifier.jtitlePhysical Review C. Nuclear Physics
dc.identifier.volume88
dc.identifier.issue4
dc.identifier.pagecount5
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevC.88.041305
dc.identifier.urnURN:NBN:no-59761
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0556-2813
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/57061/1/PhysRevC.88.041305.pdf
dc.type.versionPublishedVersion
cristin.articleid041305


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