Hide metadata

dc.date.accessioned2021-03-15T21:33:17Z
dc.date.available2021-03-15T21:33:17Z
dc.date.created2021-02-10T11:24:05Z
dc.date.issued2020
dc.identifier.citationGottardo, A. De Angelis, G. Doornenbal, P. Coraggio, L. Gargano, A. Itaco, N. Kaneko, K. Van Isacker, P Furumoto, T. Benzoni, G. Lee, J. Liu, H. Matsushita, M. Mengoni, D. Modamio, Victor Momiyama, S. Motobayashi, T. Napoli, D. Niikura, M. Sahin, Eda Shiga, Y. Sakurai, H. Taniuchi, R. Takeuchi, S. Wang, H. Valiente-Dobón, J.J. Avigo, R. Baba, H. Blasi, N. Bello Garrote, Frank Leonel Browne, F. Crespi, F.C.L. Ceruti, S. Daido, R. Delattre, M.-C. Fang, D. Dombradi, Zs. Isobe, T. Kuti, I. Lorusso, G. Matsui, K. Melon, B. Miyazaki, T. Nishimura, S. Orlandi, R. Patel, Z. Rice, S. Sinclair, L. Söderström, P.-A. Sohler, D. Sumikama, T. Taprogge, J. Vajta, Zs. Watanabe, H. Wieland, O. Wu, J. Xu, Z. Y. Yalcinkaya, M. Yokoyama, R. . Transition strengths in the neutron-rich 73,74,75Ni isotopes. Physical Review C. Nuclear Physics. 2020, 102
dc.identifier.urihttp://hdl.handle.net/10852/84117
dc.description.abstractReduced transition probabilities have been measured for the neutron-rich 73,74,75Ni nuclei with relativistic Coulomb excitation performed at the RIKEN Nishina Center. For the even-even Ni isotope the determined B(E2;0+→2+) value is compatible within errors with the result of a previous intermediate energy Coulomb excitation experiment, although being somewhat larger. For the odd Ni isotopes B(E2) values have been determined for the first time. In the middle νg9/2 shell nucleus 73Ni three peak candidates have been observed and tentatively assigned to the (5/2+), (13/2+), and (11/2+) excitations. Two peak candidates have been observed in 75Ni and tentatively assigned to the (13/2+) and (11/2+) levels. The measured B(E2) values are in line with the large B(E2) reported in 70Ni and at variance with the small strength measured in 72Ni. Excitation energies compare well with the result of large-scale shell-model calculations, while B(E2) values are larger than predicted. This could indicate an increasing contribution of proton excitations across the Z=28 shell closure when approaching 78Ni.
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleTransition strengths in the neutron-rich 73,74,75Ni isotopes
dc.typeJournal article
dc.creator.authorGottardo, A.
dc.creator.authorDe Angelis, G.
dc.creator.authorDoornenbal, P.
dc.creator.authorCoraggio, L.
dc.creator.authorGargano, A.
dc.creator.authorItaco, N.
dc.creator.authorKaneko, K.
dc.creator.authorVan Isacker, P
dc.creator.authorFurumoto, T.
dc.creator.authorBenzoni, G.
dc.creator.authorLee, J.
dc.creator.authorLiu, H.
dc.creator.authorMatsushita, M.
dc.creator.authorMengoni, D.
dc.creator.authorModamio, Victor
dc.creator.authorMomiyama, S.
dc.creator.authorMotobayashi, T.
dc.creator.authorNapoli, D.
dc.creator.authorNiikura, M.
dc.creator.authorSahin, Eda
dc.creator.authorShiga, Y.
dc.creator.authorSakurai, H.
dc.creator.authorTaniuchi, R.
dc.creator.authorTakeuchi, S.
dc.creator.authorWang, H.
dc.creator.authorValiente-Dobón, J.J.
dc.creator.authorAvigo, R.
dc.creator.authorBaba, H.
dc.creator.authorBlasi, N.
dc.creator.authorBello Garrote, Frank Leonel
dc.creator.authorBrowne, F.
dc.creator.authorCrespi, F.C.L.
dc.creator.authorCeruti, S.
dc.creator.authorDaido, R.
dc.creator.authorDelattre, M.-C.
dc.creator.authorFang, D.
dc.creator.authorDombradi, Zs.
dc.creator.authorIsobe, T.
dc.creator.authorKuti, I.
dc.creator.authorLorusso, G.
dc.creator.authorMatsui, K.
dc.creator.authorMelon, B.
dc.creator.authorMiyazaki, T.
dc.creator.authorNishimura, S.
dc.creator.authorOrlandi, R.
dc.creator.authorPatel, Z.
dc.creator.authorRice, S.
dc.creator.authorSinclair, L.
dc.creator.authorSöderström, P.-A.
dc.creator.authorSohler, D.
dc.creator.authorSumikama, T.
dc.creator.authorTaprogge, J.
dc.creator.authorVajta, Zs.
dc.creator.authorWatanabe, H.
dc.creator.authorWieland, O.
dc.creator.authorWu, J.
dc.creator.authorXu, Z. Y.
dc.creator.authorYalcinkaya, M.
dc.creator.authorYokoyama, R.
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode0
dc.identifier.cristin1888426
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=102&rft.spage=&rft.date=2020
dc.identifier.jtitlePhysical Review C. Nuclear Physics
dc.identifier.volume102
dc.identifier.issue1
dc.identifier.doihttps://doi.org/10.1103/PhysRevC.102.014323
dc.identifier.urnURN:NBN:no-86826
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0556-2813
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/84117/1/PhysRevC.102.014323.pdf
dc.type.versionPublishedVersion
cristin.articleid014323


Files in this item

Appears in the following Collection

Hide metadata