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Evolution from γ-soft to stable triaxiality in 136Nd as a prerequisite of chirality

dc.contributor.authorLv, B. F.
dc.contributor.authorPetrache, C. M.
dc.contributor.authorAstier, A.
dc.contributor.authorDupont, E.
dc.contributor.authorLopez-Martens, A.
dc.contributor.authorGreenlees, Paul
dc.contributor.authorBadran, Hussam
dc.contributor.authorCalverley, Tom
dc.contributor.authorCox, Daniel
dc.contributor.authorGrahn, Tuomas
dc.contributor.authorHilton, Joshua
dc.contributor.authorJulin, Rauno
dc.contributor.authorJuutinen, Sakari
dc.contributor.authorKonki, Joonas
dc.contributor.authorLeino, Matti
dc.contributor.authorPakarinen, Janne
dc.contributor.authorPapadakis, Philippos
dc.contributor.authorPartanen, Jari
dc.contributor.authorRahkila, Panu
dc.contributor.authorSandzelius, Mikael
dc.contributor.authorSarén, Jan
dc.contributor.authorScholey, Catherine
dc.contributor.authorSorri, Juha
dc.contributor.authorStolze, Sanna
dc.contributor.authorUusitalo, Juha
dc.contributor.authorHerzán, A.
dc.contributor.authorCederwall, B.
dc.contributor.authorErtoprak, A.
dc.contributor.authorLiu, H.
dc.contributor.authorGuo, S.
dc.contributor.authorLiu, M. L.
dc.contributor.authorQiang, Y. H.
dc.contributor.authorWang, J. G.
dc.contributor.authorZhou, X. H.
dc.contributor.authorKuti, I.
dc.contributor.authorTimár, J.
dc.contributor.authorTucholski, A.
dc.contributor.authorSrebrny, J.
dc.contributor.authorAndreoiu, C.
dc.date.accessioned2018-10-30T11:19:26Z
dc.date.available2018-10-30T11:19:26Z
dc.date.issued2018
dc.identifier.citationLv, B. F., Petrache, C. M., Astier, A., Dupont, E., Lopez-Martens, A., Greenlees, P., Badran, H., Calverley, T., Cox, D., Grahn, T., Hilton, J., Julin, R., Juutinen, S., Konki, J., Leino, M., Pakarinen, J., Papadakis, P., Partanen, J., Rahkila, P., . . . Andreoiu, C. (2018). Evolution from γ-soft to stable triaxiality in 136Nd as a prerequisite of chirality. <i>Physical Review C</i>, <i>98</i>(4), Article 044304. <a href="https://doi.org/10.1103/physrevc.98.044304" target="_blank">https://doi.org/10.1103/physrevc.98.044304</a>
dc.identifier.otherCONVID_28671767
dc.identifier.otherTUTKAID_79212
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/60029
dc.description.abstractThe level structure of 136Nd has been investigated using the 100Mo(40Ar, 4n) reaction and the JUROGAM II+RITU+GREAT setup. The level scheme has been extended significantly. Many new bands have been identified both at low and high spin, among which are five nearly degenerate bands interpreted as chiral partners. Excitation energies, spins, and parities of the previously known bands are revised and firmly established, and some previously known bands have been revised. Configurations are assigned to the observed bands based on cranked Nilsson-Strutinsky calculations. The band structure of 136Nd is now clarified and the various types of single-particle and collective excitations are well understood.fi
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.rightsCC BY 4.0
dc.subject.otherdeformed nuclei
dc.subject.othertriaxiality
dc.subject.otherchirality
dc.titleEvolution from γ-soft to stable triaxiality in 136Nd as a prerequisite of chirality
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201810224470
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineFysiikkafi
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiainePhysicsen
dc.contributor.oppiaineAccelerator Laboratoryen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2018-10-22T06:15:20Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries4
dc.relation.volume98
dc.type.versionpublishedVersion
dc.rights.copyright© the Authors, 2018. Published by the American Physical Society.
dc.rights.accesslevelopenAccessfi
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/physrevc.98.044304
dc.type.okmA1


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