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dc.contributor.authorLv, B. F.
dc.contributor.authorPetrache, C. M.
dc.contributor.authorLawrie, E. A.
dc.contributor.authorAstier, A.
dc.contributor.authorDupont, E.
dc.contributor.authorZheng, K. K.
dc.contributor.authorGreenlees, P.
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.authorSaren, 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.authorGuo, S.
dc.contributor.authorWang, J. G.
dc.contributor.authorOng, H. J.
dc.contributor.authorZhou, X. H.
dc.contributor.authorSun, Z. Y.
dc.contributor.authorKuti, I.
dc.contributor.authorTimár, J.
dc.contributor.authorTucholski, A.
dc.contributor.authorSrebrny, J.
dc.contributor.authorAndreoiu, C.
dc.date.accessioned2021-04-14T12:28:01Z
dc.date.available2021-04-14T12:28:01Z
dc.date.issued2021
dc.identifier.citationLv, B. F., Petrache, C. M., Lawrie, E. A., Astier, A., Dupont, E., Zheng, K.K., Greenlees, P., Badran, H., Calverley, T., Cox, D. M., Grahn, T., Hilton, J., Julin, R., Juutinen, S., Konki, J., Pakarinen, J., Papadakis, P., Partanen, J., Rahkila, P., . . . Andreoiu, C. (2021). Tilted precession bands in 135Nd. <i>Physical Review C</i>, <i>103</i>(4), Article 044308. <a href="https://doi.org/10.1103/PhysRevC.103.044308" target="_blank">https://doi.org/10.1103/PhysRevC.103.044308</a>
dc.identifier.otherCONVID_66365022
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/75058
dc.description.abstractTwo new excited bands built on the πh11/2 configuration have been identified in 135Nd in addition to the known πh11/2 band. The energy spectra of the excited bands and the available electromagnetic transition probabilities are in good agreement with theoretical results obtained using quasiparticle-plus-triaxial-rotor model calculations. The properties of the bands identify them as tilted precession bands instead of wobbling bands. Our results give a new insight into the interpretation of the low-lying bands in odd-A mass nuclei, and can stimulate future studies to address the nuclear triaxiality.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review C
dc.rightsIn Copyright
dc.titleTilted precession bands in 135Nd
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202104142370
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineYdin- ja kiihdytinfysiikan huippuyksikköfi
dc.contributor.oppiaineFysiikkafi
dc.contributor.oppiaineCentre of Excellence in Nuclear and Accelerator Based Physicsen
dc.contributor.oppiainePhysicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries4
dc.relation.volume103
dc.type.versionpublishedVersion
dc.rights.copyright© 2021 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevC.103.044308
jyx.fundinginformationThis work has been supported by the Academy of Finland under the Finnish Centre of Excellence Programme (2012–2017); by the Special Research Assistant Project of the Chinese Academy of Sciences; 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; and by the National Natural Science Foundation of China (Grants No. 11505242, No. 11305220, No. U1732139, No. 11775274, and No. 11575255). The use of germanium detectors from the GAMMAPOOL is acknowledged. I.K. was supported by National Research, Development and Innovation Office-NKFIH, contract No. PD 124717.
dc.type.okmA1


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