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dc.contributor.authorFrauendorf, S.
dc.contributor.authorLv, B. F.
dc.contributor.authorAstier, A.
dc.contributor.authorERTOPRAK, Ayşegül
dc.contributor.authorWang, K. L.
dc.contributor.authorGreenlees, P. T.
dc.contributor.authorBadran, H.
dc.contributor.authorCox, D. M.
dc.contributor.authorGrahn, T.
dc.contributor.authorJulin, R.
dc.contributor.authorJuutinen, S.
dc.contributor.authorKonki, J.
dc.contributor.authorPakarinen, J.
dc.contributor.authorPapadakis, P.
dc.contributor.authorPartanen, J.
dc.contributor.authorSandzelius, M.
dc.contributor.authorSaren, J.
dc.contributor.authorScholey, C.
dc.contributor.authorSorri, J.
dc.contributor.authorStolze, S.
dc.contributor.authorUusitalo, J.
dc.contributor.authorCederwall, B.
dc.contributor.authorLiu, H.
dc.contributor.authorKuti, I
dc.contributor.authorTimar, J.
dc.contributor.authorTucholski, A.
dc.contributor.authorDupont, E.
dc.contributor.authorRahkila, P.
dc.contributor.authorAktaş, Özge
dc.contributor.authorGuo, S.
dc.contributor.authorLiu, M. L.
dc.contributor.authorZhou, X. H.
dc.contributor.authorSrebrny, J.
dc.contributor.authorAndreoiu, C.
dc.contributor.authorPetrache, C.
dc.date.accessioned2021-03-05T21:27:24Z
dc.date.available2021-03-05T21:27:24Z
dc.date.issued2019
dc.identifier.citationPetrache C., Frauendorf S., Lv B. F. , Astier A., Dupont E., Guo S., Liu M. L. , Zhou X. H. , Wang K. L. , Greenlees P. T. , et al., "Collective rotation of an oblate nucleus at very high spin", PHYSICAL REVIEW C, cilt.99, 2019
dc.identifier.issn2469-9985
dc.identifier.othervv_1032021
dc.identifier.otherav_d8f7e085-08d0-4b78-999e-899da4201e2c
dc.identifier.urihttp://hdl.handle.net/20.500.12627/143129
dc.identifier.urihttps://journals.aps.org/prc/pdf/10.1103/PhysRevC.99.041301
dc.identifier.urihttps://doi.org/10.1103/physrevc.99.041301
dc.description.abstractA sequence of nine almost equidistant quadrupole transitions is observed in Nd-137. The sequence represents an extremely regular rotational band that extends to a spin of about 75/2 and an excitation energy of approximate to 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.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectFizik
dc.subjectTemel Bilimler
dc.subjectFİZİK, NÜKLEER
dc.titleCollective rotation of an oblate nucleus at very high spin
dc.typeMakale
dc.relation.journalPHYSICAL REVIEW C
dc.contributor.departmentCentre National de la Recherche Scientifique (CNRS) , ,
dc.identifier.volume99
dc.identifier.issue4
dc.contributor.firstauthorID617230


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