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Various collective states in the I-124 nucleus

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dc.contributor.authorChang Bum Moon-
dc.contributor.authorB. Moon-
dc.contributor.authorJooChun Park-
dc.contributor.authorDracoulis, G.D.-
dc.contributor.authorKibedi, T.-
dc.contributor.authorBark, R.A.-
dc.contributor.authorByrne, A.P.-
dc.contributor.authorDavidson, P.A.-
dc.contributor.authorLane, G.J.-
dc.contributor.authorWilson, A.N.-
dc.date.accessioned2022-07-29T08:12:49Z-
dc.date.available2022-07-29T08:12:49Z-
dc.date.created2021-05-27-
dc.date.issued2021-03-
dc.identifier.issn2469-9985-
dc.identifier.urihttps://pr.ibs.re.kr/handle/8788114/12093-
dc.description.abstractThe level structure of I-124 (Z = 53, N = 71) has been studied via the Sn-122(Li-7, (5)n) I-124 reaction with a beam energy of 54 MeV. Through in-beam and out-of-beam gamma-ray spectroscopy, the sophisticated low-lying levels including isomeric states and numerous collective states have been established for the first time. A positive-parity collective band built on the 10(+) state at 1297 keV is interpreted as being associated with the combination of a proton and a neutron in the same intruder h(11/2) orbital, namely the pi h(11/2)nu h(11/2) configuration. This band shows a typical quadrupole vibrational character. In contrast, the negative parity bands based on the pi g(7/2)nu h(11/2) configuration show a soft triaxial rotation. An isomeric 8(-) state at 689 keV with a half-life of 14 ns can be explained as a K isomer due to a proton with an Omega(p) = 9/2 in the g(9/2) orbital coupled to a neutron with an Omega n = 7/2 in the h(11/2) orbital. The excited states based on this pi g(9/2)nu h(11/2) configuration show a coupled rotational structure. Another coupled rotational band built on the 6(+) state at 714 keV is thought to be based on the pg(9/2)nu d(3/2) configuration.-
dc.language영어-
dc.publisherAMER PHYSICAL SOC-
dc.titleVarious collective states in the I-124 nucleus-
dc.typeArticle-
dc.type.rimsART-
dc.identifier.wosid000647588300004-
dc.identifier.scopusid2-s2.0-85104232187-
dc.identifier.rimsid75683-
dc.contributor.affiliatedAuthorChang Bum Moon-
dc.contributor.affiliatedAuthorB. Moon-
dc.contributor.affiliatedAuthorJooChun Park-
dc.identifier.doi10.1103/PhysRevC.103.034318-
dc.identifier.bibliographicCitationPhysical Review c, v.103, no.3, pp.1 - 11-
dc.relation.isPartOfPhysical Review c-
dc.citation.titlePhysical Review c-
dc.citation.volume103-
dc.citation.number3-
dc.citation.startPage1-
dc.citation.endPage11-
dc.description.journalClass1-
dc.description.journalClass1-
dc.description.isOpenAccessN-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalWebOfScienceCategoryPhysics, Nuclear-
dc.subject.keywordPlusEXCITED-STATES-
dc.subject.keywordPlusBANDS-
dc.subject.keywordPlusCOEXISTENCE-
Appears in Collections:
Center for Exotic Nuclear Studies(희귀 핵 연구단) > 1. Journal Papers (저널논문)
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