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dc.contributor.authorLv, B.F.
dc.contributor.authorPetrache, C.M.
dc.contributor.authorLawrie, E.A.
dc.contributor.authorGuo, S.
dc.contributor.authorAstier, A.
dc.contributor.authorZheng, K.K.
dc.contributor.authorOng, H.J.
dc.contributor.authorWang, J.G.
dc.contributor.authorZhou, X.H.
dc.contributor.authorSun, Z.Y.
dc.contributor.authorGreenlees, P.T.
dc.contributor.authorBadran, H.
dc.contributor.authorCalverley, T.
dc.contributor.authorCox, D.M.
dc.contributor.authorGrahn, T.
dc.contributor.authorHilton, J.
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.authorRahkila, P.
dc.contributor.authorRuotsalainen, P.
dc.contributor.authorSandzelius, M.
dc.contributor.authorSarén, J.
dc.contributor.authorScholey, C.
dc.contributor.authorSorri, J.
dc.contributor.authorStolze, S.
dc.contributor.authorUusitalo, J.
dc.contributor.authorCederwall, B.
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.accessioned2022-01-24T06:35:14Z
dc.date.available2022-01-24T06:35:14Z
dc.date.issued2022
dc.identifier.citationLv, B.F., Petrache, C.M., Lawrie, E.A., Guo, S., Astier, A., Zheng, K.K., Ong, H.J., Wang, J.G., Zhou, X.H., Sun, Z.Y., Greenlees, P.T., Badran, H., Calverley, T., Cox, D.M., Grahn, T., Hilton, J., Julin, R., Juutinen, S., Konki, J., . . . Andreoiu, C. (2022). Evidence against the wobbling nature of low-spin bands in 135Pr. <i>Physics Letters B</i>, <i>824</i>, Article 136840. <a href="https://doi.org/10.1016/j.physletb.2021.136840" target="_blank">https://doi.org/10.1016/j.physletb.2021.136840</a>
dc.identifier.otherCONVID_103956519
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/79475
dc.description.abstractThe electromagnetic character of the ΔI=1 transitions connecting the 1- to 0-phonon and the 2- to 1-phonon wobbling bands should be dominated by an E2 component, due to the collective motion of the entire nuclear charge. In the present work it is shown, based on combined angular correlation and linear polarization measurements, that the mixing ratios of all analyzed connecting transitions between low-lying bands in 135Pr interpreted as 0-, 1-, and 2-phonon wobbling bands, have absolute values smaller than one. This indicates predominant M1 magnetic character, which is incompatible with the proposed wobbling nature. All experimental observables are instead in good agreement with quasiparticle-plus-triaxial-rotor model calculations, which describe the bands as resulting from a rapid re-alignment of the total angular momentum from the short to the intermediate nuclear axis.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherElsevier BV
dc.relation.ispartofseriesPhysics Letters B
dc.rightsCC BY 4.0
dc.subject.otherγγγ-coincidences
dc.subject.otherangular correlations
dc.subject.otherparticle rotor model
dc.subject.otherwobbling bands
dc.titleEvidence against the wobbling nature of low-spin bands in 135Pr
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202201241251
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineFysiikkafi
dc.contributor.oppiaineYdin- ja kiihdytinfysiikan huippuyksikköfi
dc.contributor.oppiainePhysicsen
dc.contributor.oppiaineCentre of Excellence in Nuclear and Accelerator Based Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn0370-2693
dc.relation.volume824
dc.type.versionpublishedVersion
dc.rights.copyright© 2021 The Author(s). Published by Elsevier B.V.
dc.rights.accesslevelopenAccessfi
dc.subject.ysoydinfysiikka
dc.subject.ysospin (kvanttimekaniikka)
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p38874
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1016/j.physletb.2021.136840
jyx.fundinginformationThis work has been supported by the Special Research Assistant Project of the Chinese Academy of Sciences; by the Strategic Priority Research Program of Chinese Academy of Sciences (Grant No. XDB34000000); by the Academy of Finland under the Finnish Centre of Excellence Programme (2012-2017); by the EU 7th Framework Programme Project No. 262010 (ENSAR); by the National Research Foundation of South Africa (Grants No. 116666 and No. 109134), and by the French Ministry of Foreign Affairs and the Ministry of Higher Education and Research, France (PHC PROTEA Grant No. 42417SE); by the National Research, Development and Innovation Fund of Hungary (Project No. K128947), as well as by the European Regional Development Fund (Contract No. GINOP-2.3.3-15-2016-00034); by the Polish National Science Centre (NCN) Grant No. 2013/10/M/ST2/00427; by the Swedish Research Council under Grant No. 621-2014-5558. The use of germanium detectors from the GAMMAPOOL is acknowledged. I.K. was supported by National Research, Development and Innovation Office-NKFIH, contract number PD 124717.
dc.type.okmA1


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