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Extended p3/2 Neutron Orbital and the N=32 Shell Closure in Ca 52

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dc.contributor.authorEnciu, M.-
dc.contributor.authorLiu, H.N.-
dc.contributor.authorObertelli, A.-
dc.contributor.authorDoornenbal, P.-
dc.contributor.authorNowacki, F.-
dc.contributor.authorOgata, K.-
dc.contributor.authorPoves, A.-
dc.contributor.authorYoshida, K.-
dc.contributor.authorAchouri, N.L.-
dc.contributor.authorBaba, H.-
dc.contributor.authorBrowne, F.-
dc.contributor.authorCalvet, D.-
dc.contributor.authorChateau, F.-
dc.contributor.authorChen, S.-
dc.contributor.authorChiga, N.-
dc.contributor.authorCorsi, A.-
dc.contributor.authorCortes, M.L.-
dc.contributor.authorDelbart, A.-
dc.contributor.authorGheller, J.-M.-
dc.contributor.authorGiganon, A.-
dc.contributor.authorGillibert, A.-
dc.contributor.authorHilaire, C.-
dc.contributor.authorIsobe, T.-
dc.contributor.authorKobayashi, T.-
dc.contributor.authorKubota, Y.-
dc.contributor.authorLapoux, V.-
dc.contributor.authorMotobayashi, T.-
dc.contributor.authorMurray, I.-
dc.contributor.authorOtsu, H.-
dc.contributor.authorPanin, V.-
dc.contributor.authorPaul, N.-
dc.contributor.authorRodriguez, W.-
dc.contributor.authorSakurai, H.-
dc.contributor.authorSasano, M.-
dc.contributor.authorSteppenbeck, D.-
dc.contributor.authorLaszlo STUHL-
dc.contributor.authorSun, Y.L.-
dc.contributor.authorTogano, Y.-
dc.contributor.authorUesaka, T.-
dc.contributor.authorWimmer, K.-
dc.contributor.authorYoneda, K.-
dc.contributor.authorAktas, O.-
dc.contributor.authorAumann, T.-
dc.contributor.authorChung, L.X.-
dc.contributor.authorFlavigny, F.-
dc.contributor.authorFranchoo, S.-
dc.contributor.authorGasparic, I.-
dc.contributor.authorGerst, R.-B.-
dc.contributor.authorGibelin, J.-
dc.contributor.authorKevin Insik Hahn-
dc.contributor.authorDa Hee KIM-
dc.contributor.authorKondo, Y.-
dc.contributor.authorKoseoglou, P.-
dc.contributor.authorLee, J.-
dc.contributor.authorLehr, C.-
dc.contributor.authorLi, P.J.-
dc.contributor.authorLinh, B.D.-
dc.contributor.authorLokotko, T.-
dc.contributor.authorMaccormick, M.-
dc.contributor.authorMoschner, K.-
dc.contributor.authorNakamura, T.-
dc.contributor.authorPark, S.Y.-
dc.contributor.authorRossi, D.-
dc.contributor.authorSahin, E.-
dc.contributor.authorSoderstrom, P.-A.-
dc.contributor.authorSohler, D.-
dc.contributor.authorTakeuchi, S.-
dc.contributor.authorToernqvist, H.-
dc.contributor.authorVaquero, V.-
dc.contributor.authorWagner, V.-
dc.contributor.authorWang, S.-
dc.contributor.authorWerner, V.-
dc.contributor.authorXu, X.-
dc.contributor.authorYamada, H.-
dc.contributor.authorYan, D.-
dc.contributor.authorYang, Z.-
dc.contributor.authorYasuda, M.-
dc.contributor.authorZanetti, L.-
dc.date.accessioned2023-01-26T02:21:27Z-
dc.date.available2023-01-26T02:21:27Z-
dc.date.created2023-01-11-
dc.date.issued2022-12-
dc.identifier.issn0031-9007-
dc.identifier.urihttps://pr.ibs.re.kr/handle/8788114/12472-
dc.description.abstractThe one-neutron knockout from Ca52 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 Ca51 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. © 2022 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the https://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.-
dc.language영어-
dc.publisherAmerican Physical Society-
dc.titleExtended p3/2 Neutron Orbital and the N=32 Shell Closure in Ca 52-
dc.typeArticle-
dc.type.rimsART-
dc.identifier.wosid000906643300003-
dc.identifier.scopusid2-s2.0-85144628362-
dc.identifier.rimsid79641-
dc.contributor.affiliatedAuthorLaszlo STUHL-
dc.contributor.affiliatedAuthorKevin Insik Hahn-
dc.contributor.affiliatedAuthorDa Hee KIM-
dc.identifier.doi10.1103/PhysRevLett.129.262501-
dc.identifier.bibliographicCitationPhysical Review Letters, v.129, no.26-
dc.relation.isPartOfPhysical Review Letters-
dc.citation.titlePhysical Review Letters-
dc.citation.volume129-
dc.citation.number26-
dc.type.docTypeArticle-
dc.description.journalClass1-
dc.description.journalClass1-
dc.description.isOpenAccessN-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaPhysics-
dc.relation.journalWebOfScienceCategoryPhysics, Multidisciplinary-
dc.subject.keywordPlusQUASI-FREE SCATTERING-
dc.subject.keywordPlusKNOCKOUT REACTIONS-
dc.subject.keywordPlusCHARGE RADII-
dc.subject.keywordPlusBETA-DECAY-
dc.subject.keywordPlusISOTOPES-
dc.subject.keywordPlusMASSES-
dc.subject.keywordPlusMINOS-
Appears in Collections:
Center for Exotic Nuclear Studies(희귀 핵 연구단) > 1. Journal Papers (저널논문)
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