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dc.date.accessioned2019-02-25T11:57:07Z
dc.date.available2019-02-25T11:57:07Z
dc.date.created2015-04-30T23:20:22Z
dc.date.issued2015
dc.identifier.citationLarsen, Ann-Cecilie Goriely, Stephane Bernstein, L. A. Bleuel, D. L. Bracco, A. Brown, B. A. Camera, F. Eriksen, Tomas Kvalheim Frauendorf, Stefan Giacoppo, Francesca Guttormsen, Magne Sveen Görgen, Andreas Harrisopulos, Sotirios Leoni, S. Liddick, S. N. Naqvi, F. Nyhus, Hilde-Therese Rose, Sunniva Johanne Renstrøm, Therese Schwengner, Ronald Siem, Sunniva Spyrou, A. Tveten, Gry Merete Voinov, Alexander Wiedeking, Mathis . Upbend and M1 scissors mode in neutron-rich nuclei — consequences for r-process (n,gamma) reaction rates. Acta Physica Polonica B. 2015, 46(3), 509-512
dc.identifier.urihttp://hdl.handle.net/10852/66809
dc.description.abstractAn enhanced probability for low-energy γ-emission (upbend, Eγ < 3 MeV) at high excitation energies has been observed for several light and medium-mass nuclei close to the valley of stability. Also the M1 scissors mode seen in deformed nuclei increases the γ-decay probability for low-energy γ-rays (Eγ ≈ 2–3 MeV). These phenomena, if present in neutron-rich nuclei, have the potential to increase radiative neutron-capture rates relevant for the r-process. The experimental and theoretical status of the upbend is discussed, and preliminary calculations of (n,γ) reaction rates for neutron-rich, mid-mass nuclei including the scissors mode are shown.en_US
dc.languageEN
dc.publisherJagellonian University
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleUpbend and M1 scissors mode in neutron-rich nuclei — consequences for r-process (n,gamma) reaction ratesen_US
dc.typeJournal articleen_US
dc.creator.authorLarsen, Ann-Cecilie
dc.creator.authorGoriely, Stephane
dc.creator.authorBernstein, L. A.
dc.creator.authorBleuel, D. L.
dc.creator.authorBracco, A.
dc.creator.authorBrown, B. A.
dc.creator.authorCamera, F.
dc.creator.authorEriksen, Tomas Kvalheim
dc.creator.authorFrauendorf, Stefan
dc.creator.authorGiacoppo, Francesca
dc.creator.authorGuttormsen, Magne Sveen
dc.creator.authorGörgen, Andreas
dc.creator.authorHarrisopulos, Sotirios
dc.creator.authorLeoni, S.
dc.creator.authorLiddick, S. N.
dc.creator.authorNaqvi, F.
dc.creator.authorNyhus, Hilde-Therese
dc.creator.authorRose, Sunniva Johanne
dc.creator.authorRenstrøm, Therese
dc.creator.authorSchwengner, Ronald
dc.creator.authorSiem, Sunniva
dc.creator.authorSpyrou, A.
dc.creator.authorTveten, Gry Merete
dc.creator.authorVoinov, Alexander
dc.creator.authorWiedeking, Mathis
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1240108
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Acta Physica Polonica B&rft.volume=46&rft.spage=509&rft.date=2015
dc.identifier.jtitleActa Physica Polonica B
dc.identifier.volume46
dc.identifier.issue3
dc.identifier.startpage509
dc.identifier.endpage512
dc.identifier.doihttp://dx.doi.org/10.5506/APhysPolB.46.509
dc.identifier.urnURN:NBN:no-69997
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0587-4254
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/66809/2/Larsen_v46p0509.pdf
dc.type.versionPublishedVersion


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