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dc.date.accessioned2023-03-14T17:32:46Z
dc.date.available2023-03-14T17:32:46Z
dc.date.created2023-01-10T13:24:02Z
dc.date.issued2022
dc.identifier.citationEnciu, M. Liu, H.N. Obertelli, A. Doornenbal, P. Nowacki, F. Ogata, K. Poves, A. Yoshida, K. Achouri, N.L. Baba, H. Browne, F. Calvet, D. Château, F. Chen, S. Chiga, N. Corsi, A. Cortés, M.L. Delbart, A. Gheller, J.-M. Giganon, A. Gillibert, A. Hilaire, C. Isobe, T. Kobayashi, T. Kubota, Y. Lapoux, V. Motobayashi, T. Murray, I. Otsu, H. Panin, V. Paul, N. Rodriguez, W. Sakurai, H. Sasano, M. Steppenbeck, D. Stuhl, L. Sun, Y.L. Togano, Y. Uesaka, T. Wimmer, K. Yoneda, K. Aktas, O. Aumann, T. Chung, L.X. Flavigny, F. Franchoo, S. Gasparic, I. Gerst, R.-B. Gibelin, J. Hahn, K.I. Kim, D. Kondo, Y. Koseoglou, P. Lee, J. Lehr, C. Li, P.J. Linh, B.D. Lokotko, T. Maccormick, M. Moschner, K. Nakamura, T. Park, S.Y. Rossi, D. Sahin, Eda Söderström, P.-A. Sohler, D. Takeuchi, S. Toernqvist, H. Vaquero, V. Wagner, V. Wang, S. Werner, V. Xu, X. Yamada, H. Yan, D. Yang, Z. Yasuda, M. Zanetti, L. . Extended p3/2 Neutron Orbital and the N=32 Shell Closure in Ca 52. Physical Review Letters. 2022, 129(26)
dc.identifier.urihttp://hdl.handle.net/10852/101438
dc.description.abstractThe one-neutron knockout from 52Ca in inverse kinematics onto a proton target was performed at ∼230  MeV/nucleon combined with prompt γ spectroscopy. Exclusive quasifree scattering cross sections to bound states in 51Ca and the momentum distributions corresponding to the removal of 1f7/2 and 2p3/2 neutrons were measured. The cross sections, interpreted within the distorted-wave impulse approximation reaction framework, are consistent with a shell closure at the neutron number N=32, found as strong as at N=28 and N=34 in Ca isotopes from the same observables. The analysis of the momentum distributions leads to a difference of the root-mean-square radii of the neutron 1f7/2 and 2p3/2 orbitals of 0.61(23) fm, in agreement with the modified-shell-model prediction of 0.7 fm suggesting that the large root-mean-square radius of the 2p3/2 orbital in neutron-rich Ca isotopes is responsible for the unexpected linear increase of the charge radius with the neutron number.
dc.languageEN
dc.publisherAmerican Physical Society
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleExtended p3/2 Neutron Orbital and the N=32 Shell Closure in Ca 52
dc.title.alternativeENEngelskEnglishExtended p3/2 Neutron Orbital and the N=32 Shell Closure in Ca 52
dc.typeJournal article
dc.creator.authorEnciu, M.
dc.creator.authorLiu, H.N.
dc.creator.authorObertelli, A.
dc.creator.authorDoornenbal, P.
dc.creator.authorNowacki, F.
dc.creator.authorOgata, K.
dc.creator.authorPoves, A.
dc.creator.authorYoshida, K.
dc.creator.authorAchouri, N.L.
dc.creator.authorBaba, H.
dc.creator.authorBrowne, F.
dc.creator.authorCalvet, D.
dc.creator.authorChâteau, F.
dc.creator.authorChen, S.
dc.creator.authorChiga, N.
dc.creator.authorCorsi, A.
dc.creator.authorCortés, M.L.
dc.creator.authorDelbart, A.
dc.creator.authorGheller, J.-M.
dc.creator.authorGiganon, A.
dc.creator.authorGillibert, A.
dc.creator.authorHilaire, C.
dc.creator.authorIsobe, T.
dc.creator.authorKobayashi, T.
dc.creator.authorKubota, Y.
dc.creator.authorLapoux, V.
dc.creator.authorMotobayashi, T.
dc.creator.authorMurray, I.
dc.creator.authorOtsu, H.
dc.creator.authorPanin, V.
dc.creator.authorPaul, N.
dc.creator.authorRodriguez, W.
dc.creator.authorSakurai, H.
dc.creator.authorSasano, M.
dc.creator.authorSteppenbeck, D.
dc.creator.authorStuhl, L.
dc.creator.authorSun, Y.L.
dc.creator.authorTogano, Y.
dc.creator.authorUesaka, T.
dc.creator.authorWimmer, K.
dc.creator.authorYoneda, K.
dc.creator.authorAktas, O.
dc.creator.authorAumann, T.
dc.creator.authorChung, L.X.
dc.creator.authorFlavigny, F.
dc.creator.authorFranchoo, S.
dc.creator.authorGasparic, I.
dc.creator.authorGerst, R.-B.
dc.creator.authorGibelin, J.
dc.creator.authorHahn, K.I.
dc.creator.authorKim, D.
dc.creator.authorKondo, Y.
dc.creator.authorKoseoglou, P.
dc.creator.authorLee, J.
dc.creator.authorLehr, C.
dc.creator.authorLi, P.J.
dc.creator.authorLinh, B.D.
dc.creator.authorLokotko, T.
dc.creator.authorMaccormick, M.
dc.creator.authorMoschner, K.
dc.creator.authorNakamura, T.
dc.creator.authorPark, S.Y.
dc.creator.authorRossi, D.
dc.creator.authorSahin, Eda
dc.creator.authorSöderström, P.-A.
dc.creator.authorSohler, D.
dc.creator.authorTakeuchi, S.
dc.creator.authorToernqvist, H.
dc.creator.authorVaquero, V.
dc.creator.authorWagner, V.
dc.creator.authorWang, S.
dc.creator.authorWerner, V.
dc.creator.authorXu, X.
dc.creator.authorYamada, H.
dc.creator.authorYan, D.
dc.creator.authorYang, Z.
dc.creator.authorYasuda, M.
dc.creator.authorZanetti, L.
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin2104153
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=129&rft.spage=&rft.date=2022
dc.identifier.jtitlePhysical Review Letters
dc.identifier.volume129
dc.identifier.issue26
dc.identifier.pagecount0
dc.identifier.doihttps://doi.org/10.1103/PhysRevLett.129.262501
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0031-9007
dc.type.versionPublishedVersion
cristin.articleid262501


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