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dc.date.accessioned2021-03-16T21:26:10Z
dc.date.available2021-03-16T21:26:10Z
dc.date.created2020-12-15T12:10:55Z
dc.date.issued2020
dc.identifier.citationKibédi, T. Alshahrani, B. Stuchbery, A.E. Larsen, Ann-Cecilie Görgen, Andreas Siem, Sunniva Guttormsen, Magne Sveen Giacoppo, Francesca Morales, A.I. Sahin, Eda Tveten, Gry Merete Bello Garrote, Frank Leonel Crespo Campo, Lucia Eriksen, Tomas Kvalheim Klintefjord, Malin Maharramova, Sabina Nyhus, Hilde-Therese Tornyi, Tamas Gabor Renstrøm, Therese Paulsen, Wanja . Radiative Width of the Hoyle State from γ -Ray Spectroscopy. Physical Review Letters. 2020, 125(18)
dc.identifier.urihttp://hdl.handle.net/10852/84149
dc.description.abstractThe cascading 3.21 and 4.44 MeV electric quadrupole transitions have been observed from the Hoyle state at 7.65 MeV excitation energy in 12C, excited by the 12C(p,p′) reaction at 10.7 MeV proton energy. From the proton-γ−γ triple coincidence data, a value of Γrad/Γ=6.2(6)×10−4 was obtained for the radiative branching ratio. Using our results, together with ΓE0π/Γ from Eriksen et al. [Phys. Rev. C 102, 024320 (2020)] and the currently adopted Γπ(E0) values, the radiative width of the Hoyle state is determined as Γrad=5.1(6)×10−3  eV. This value is about 34% higher than the currently adopted value and will impact models of stellar evolution and nucleosynthesis.
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleRadiative Width of the Hoyle State from γ -Ray Spectroscopy
dc.typeJournal article
dc.creator.authorKibédi, T.
dc.creator.authorAlshahrani, B.
dc.creator.authorStuchbery, A.E.
dc.creator.authorLarsen, Ann-Cecilie
dc.creator.authorGörgen, Andreas
dc.creator.authorSiem, Sunniva
dc.creator.authorGuttormsen, Magne Sveen
dc.creator.authorGiacoppo, Francesca
dc.creator.authorMorales, A.I.
dc.creator.authorSahin, Eda
dc.creator.authorTveten, Gry Merete
dc.creator.authorBello Garrote, Frank Leonel
dc.creator.authorCrespo Campo, Lucia
dc.creator.authorEriksen, Tomas Kvalheim
dc.creator.authorKlintefjord, Malin
dc.creator.authorMaharramova, Sabina
dc.creator.authorNyhus, Hilde-Therese
dc.creator.authorTornyi, Tamas Gabor
dc.creator.authorRenstrøm, Therese
dc.creator.authorPaulsen, Wanja
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin1859976
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 Letters&rft.volume=125&rft.spage=&rft.date=2020
dc.identifier.jtitlePhysical Review Letters
dc.identifier.volume125
dc.identifier.issue18
dc.identifier.pagecount6
dc.identifier.doihttps://doi.org/10.1103/PhysRevLett.125.182701
dc.identifier.urnURN:NBN:no-86881
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0031-9007
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/84149/1/Kibedi_Hoylestate_PhysRevLett.125.182701.pdf
dc.type.versionPublishedVersion
cristin.articleid182701
dc.relation.projectNFR/263030
dc.relation.projectEC/H2020/637686


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