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dc.date.accessioned2019-02-19T12:36:49Z
dc.date.available2019-02-19T12:36:49Z
dc.date.created2018-12-18T14:05:57Z
dc.date.issued2018
dc.identifier.citationLarsen, Ann-Cecilie Midtbø, Jørgen E. Guttormsen, Magne Sveen Renstrøm, Therese Liddick, Sean N. Spyrou, Artemis Karampagia, Sofia Brown, Alex Achakovskiy, Oleg Kamerdzhiev, Sergei Bleuel, Darren L. Couture, Aaron J. Crespo Campo, Lucia Crider, Benjamin P. Dombos, Alexander C. Lewis, Rebecca Mosby, Shea M. Naqvi, Farheen Perdikakis, Georgios Prokop, Christopher J. Quinn, Stephen Siem, Sunniva . Enhanced low-energy γ-decay strength of 70Ni and its robustness within the shell model. Physical Review C. 2018, 97(5), 1-9
dc.identifier.urihttp://hdl.handle.net/10852/66645
dc.description.abstractNeutron-capture reactions on very neutron-rich nuclei are essential for heavy-element nucleosynthesis through the rapid neutron-capture process, now shown to take place in neutron-star merger events. For these exotic nuclei, radiative neutron capture is extremely sensitive to their γ -emission probability at very low γ energies. In this work, we present measurements of the γ -decay strength of 70Ni over the wide range 1.3 Eγ 8 MeV. A significant enhancement is found in the γ -decay strength for transitions with Eγ < 3 MeV. At present, this is the most neutron-rich nucleus displaying this feature, proving that this phenomenon is not restricted to stable nuclei. We have performed E1-strength calculations within the quasiparticle time-blocking approximation, which describe our data above Eγ 5 MeV very well. Moreover, large-scale shell-model calculations indicate an M1 nature of the low-energy γ strength. This turns out to be remarkably robust with respect to the choice of interaction, truncation, and model space, and we predict its presence in the whole isotopic chain, in particular the neutron-rich 72,74,76Ni.en_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.relation.ispartofMidtbø, Jørgen E. (2019) The low-energy enhancement. An experimental and theoretical study of nuclear level densities and γ-ray strength functions. Doctoral thesis http://hdl.handle.net/10852/76787
dc.relation.urihttp://hdl.handle.net/10852/76787
dc.titleEnhanced low-energy γ-decay strength of 70Ni and its robustness within the shell modelen_US
dc.typeJournal articleen_US
dc.creator.authorLarsen, Ann-Cecilie
dc.creator.authorMidtbø, Jørgen E.
dc.creator.authorGuttormsen, Magne Sveen
dc.creator.authorRenstrøm, Therese
dc.creator.authorLiddick, Sean N.
dc.creator.authorSpyrou, Artemis
dc.creator.authorKarampagia, Sofia
dc.creator.authorBrown, Alex
dc.creator.authorAchakovskiy, Oleg
dc.creator.authorKamerdzhiev, Sergei
dc.creator.authorBleuel, Darren L.
dc.creator.authorCouture, Aaron J.
dc.creator.authorCrespo Campo, Lucia
dc.creator.authorCrider, Benjamin P.
dc.creator.authorDombos, Alexander C.
dc.creator.authorLewis, Rebecca
dc.creator.authorMosby, Shea M.
dc.creator.authorNaqvi, Farheen
dc.creator.authorPerdikakis, Georgios
dc.creator.authorProkop, Christopher J.
dc.creator.authorQuinn, Stephen
dc.creator.authorSiem, Sunniva
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1644960
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=1&rft.date=2018
dc.identifier.jtitlePhysical Review C
dc.identifier.volume97
dc.identifier.issue5
dc.identifier.startpage1
dc.identifier.endpage9
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevC.97.054329
dc.identifier.urnURN:NBN:no-69824
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn2469-9985
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/66645/1/Larsen_Midtboe_PhysRevC.97.054329.pdf
dc.type.versionPublishedVersion
cristin.articleid054329
dc.relation.projectCOST/CA16117
dc.relation.projectNOTUR/NORSTORE/NN9464K
dc.relation.projectNFR/210007
dc.relation.projectEC/H2020/637686


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