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dc.contributor.authorPetrache, C. M.
dc.contributor.authorFrauendorf, S.
dc.contributor.authorLv, B. F.
dc.contributor.authorAstier, A.
dc.contributor.authorDupont, E.
dc.contributor.authorGuo, S.
dc.contributor.authorLiu, M. L.
dc.contributor.authorZhou, X. H.
dc.contributor.authorWang, K. L.
dc.contributor.authorGreenlees, Paul
dc.contributor.authorBadran, Hussam
dc.contributor.authorCox, Daniel
dc.contributor.authorGrahn, Tuomas
dc.contributor.authorJulin, Rauno
dc.contributor.authorJuutinen, Sakari
dc.contributor.authorKonki, Joonas
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.authorCederwall, B.
dc.contributor.authorAktas, Ö.
dc.contributor.authorErtoprak, A.
dc.contributor.authorLiu, H.
dc.contributor.authorKuti, I.
dc.contributor.authorTimár, J.
dc.contributor.authorTucholski, A.
dc.contributor.authorSrebrny, J.
dc.contributor.authorAndreoiu, C.
dc.date.accessioned2019-04-04T05:37:23Z
dc.date.available2019-04-04T05:37:23Z
dc.date.issued2019fi
dc.identifier.citationPetrache, C. M., Frauendorf, S., Lv, B. F., Astier, A., Dupont, E., Guo, S., . . . Andreoiu, C. (2019). Collective rotation of an oblate nucleus at very high spin. <em>Physical Review C</em>, 99 (4), 041301(R). <a href="https://doi.org/10.1103/PhysRevC.99.041301">doi:10.1103/PhysRevC.99.041301</a>fi
dc.identifier.otherTUTKAID_81102
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/63375
dc.description.abstractA sequence of nine almost equidistant quadrupole transitions is observed in 137Nd. The sequence represents an extremely regular rotational band that extends to a spin of about 75/2 and an excitation energy of ≈4.5 MeV above yrast. Cranked mean-field calculations of the Nilsson-Strutinsky type suggest an oblate shape for the band. They reproduce the observed I(I + 1) dependence of the rotational energy whereas predicting a pronounced decrease in the deformation, which is the hallmark of antimagnetic rotation.fi
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.rightsIn Copyright
dc.subject.othercollective levelsfi
dc.subject.othercollective modelsfi
dc.subject.otherelectromagnetic transitionsfi
dc.titleCollective rotation of an oblate nucleus at very high spinfi
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201904032065
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2019-04-03T12:15:22Z
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries4
dc.relation.volume99
dc.type.versionpublishedVersion
dc.rights.copyright© 2019 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.format.contentfulltext
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevC.99.041301


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