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dc.date.accessioned2021-03-16T20:45:27Z
dc.date.available2021-03-16T20:45:27Z
dc.date.created2021-02-10T12:00:31Z
dc.date.issued2020
dc.identifier.citationWu, J. Nishimura, S. Möller, P. Mumpower, M.r. Lozeva, R. Moon, C.B. Odahara, A. Baba, H. Browne, F. Daido, R. Doornenbal, P. Fang, Y. F. Haroon, M. Isobe, T. Jung, H. S. Lorusso, G. Moon, B. Patel, Z. Rice, S. Sakurai, H. Shimizu, Y Sinclair, L. Söderström, P.-A. Sumikama, T. Watanabe, H. Xu, Z. Y. Yagi, A. Yokoyama, R. Ahn, D. S. Bello Garrote, Frank Leonel Daugas, J.M. Didierjean, F. Fukuda, N. Inabe, N. Ishigaki, T. Kameda, T. Kojouharov, I. Komatsubara, T. Kubo, T. Kurz, N. Kwon, K. Y. Morimoto, S. Murai, D. Nishibata, H. Schaffner, H. Sprouse, T. M. Suzuki, H. Takeda, H. Tanaka, M. Tshoo, K. Wakabayashi, Y. . β-decay half-lives of 55 neutron-rich isotopes beyond the N = 82 shell gap. Physical Review C. 2020, 101
dc.identifier.urihttp://hdl.handle.net/10852/84135
dc.description.abstractThe β-decay half-lives of 55 neutron-rich nuclei 134−139Sn, 134−142Sb, 137−144Te, 140−146I, 142−148Xe, 145−151Cs, 148−153Ba, and 151−155La were measured at the Radioactive Isotope Beam Factory employing the projectile fission fragments of 238U. The nuclear level structure, which relates to deformation, has a large effect on the half-lives. The impact of newly measured half-lives on modeling the astrophysical origin of the heavy elements is studied in the context of r process nucleosynthesis. For a wide variety of astrophysical conditions, including those in which fission recycling occurs, the half-lives have an important local impact on the second (A ≈ 130) peak.
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleβ-decay half-lives of 55 neutron-rich isotopes beyond the N = 82 shell gap
dc.typeJournal article
dc.creator.authorWu, J.
dc.creator.authorNishimura, S.
dc.creator.authorMöller, P.
dc.creator.authorMumpower, M.r.
dc.creator.authorLozeva, R.
dc.creator.authorMoon, C.B.
dc.creator.authorOdahara, A.
dc.creator.authorBaba, H.
dc.creator.authorBrowne, F.
dc.creator.authorDaido, R.
dc.creator.authorDoornenbal, P.
dc.creator.authorFang, Y. F.
dc.creator.authorHaroon, M.
dc.creator.authorIsobe, T.
dc.creator.authorJung, H. S.
dc.creator.authorLorusso, G.
dc.creator.authorMoon, B.
dc.creator.authorPatel, Z.
dc.creator.authorRice, S.
dc.creator.authorSakurai, H.
dc.creator.authorShimizu, Y
dc.creator.authorSinclair, L.
dc.creator.authorSöderström, P.-A.
dc.creator.authorSumikama, T.
dc.creator.authorWatanabe, H.
dc.creator.authorXu, Z. Y.
dc.creator.authorYagi, A.
dc.creator.authorYokoyama, R.
dc.creator.authorAhn, D. S.
dc.creator.authorBello Garrote, Frank Leonel
dc.creator.authorDaugas, J.M.
dc.creator.authorDidierjean, F.
dc.creator.authorFukuda, N.
dc.creator.authorInabe, N.
dc.creator.authorIshigaki, T.
dc.creator.authorKameda, T.
dc.creator.authorKojouharov, I.
dc.creator.authorKomatsubara, T.
dc.creator.authorKubo, T.
dc.creator.authorKurz, N.
dc.creator.authorKwon, K. Y.
dc.creator.authorMorimoto, S.
dc.creator.authorMurai, D.
dc.creator.authorNishibata, H.
dc.creator.authorSchaffner, H.
dc.creator.authorSprouse, T. M.
dc.creator.authorSuzuki, H.
dc.creator.authorTakeda, H.
dc.creator.authorTanaka, M.
dc.creator.authorTshoo, K.
dc.creator.authorWakabayashi, Y.
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1888464
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=101&rft.spage=&rft.date=2020
dc.identifier.jtitlePhysical Review C
dc.identifier.volume101
dc.identifier.issue4
dc.identifier.doihttps://doi.org/10.1103/PhysRevC.101.042801
dc.identifier.urnURN:NBN:no-86870
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn2469-9985
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/84135/2/PhysRevC.101.042801.pdf
dc.type.versionPublishedVersion
cristin.articleid042801


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