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dc.contributor.authorWimmer, K.
dc.contributor.authorRuotsalainen, P.
dc.contributor.authorLenzi, S.M.
dc.contributor.authorPoves, A.
dc.contributor.authorHüyük, T.
dc.contributor.authorBrowne, F.
dc.contributor.authorDoornenbal, P.
dc.contributor.authorKoiwai, T.
dc.contributor.authorArici, T.
dc.contributor.authorAuranen, K.
dc.contributor.authorBentley, M.A.
dc.contributor.authorCortés, M.L.
dc.contributor.authorDelafosse, C.
dc.contributor.authorEronen, T.
dc.contributor.authorGe, Z.
dc.contributor.authorGrahn, T.
dc.contributor.authorGreenlees, P.T.
dc.contributor.authorIllana, A.
dc.contributor.authorImai, N.
dc.contributor.authorJoukainen, H.
dc.contributor.authorJulin, R.
dc.contributor.authorJungclaus, A.
dc.contributor.authorJutila, H.
dc.contributor.authorKankainen, A.
dc.contributor.authorKitamura, N.
dc.contributor.authorLongfellow, B.
dc.contributor.authorLouko, J.
dc.contributor.authorLozeva, R.
dc.contributor.authorLuoma, M.
dc.contributor.authorMauss, B.
dc.contributor.authorNapoli, D.R.
dc.contributor.authorNiikura, M.
dc.contributor.authorOjala, J.
dc.contributor.authorPakarinen, J.
dc.contributor.authorPereira-Lopez, X.
dc.contributor.authorRahkila, P.
dc.contributor.authorRecchia, F.
dc.contributor.authorSandzelius, M.
dc.contributor.authorSarén, J.
dc.contributor.authorTaniuchi, R.
dc.contributor.authorTann, H.
dc.contributor.authorUthayakumaar, S.
dc.contributor.authorUusitalo, J.
dc.contributor.authorVaquero, V.
dc.contributor.authorWadsworth, R.
dc.contributor.authorZimba, G.
dc.contributor.authorYajzey, R.
dc.date.accessioned2023-11-16T12:03:46Z
dc.date.available2023-11-16T12:03:46Z
dc.date.issued2023
dc.identifier.citationWimmer, K., Ruotsalainen, P., Lenzi, S.M., Poves, A., Hüyük, T., Browne, F., Doornenbal, P., Koiwai, T., Arici, T., Auranen, K., Bentley, M.A., Cortés, M.L., Delafosse, C., Eronen, T., Ge, Z., Grahn, T., Greenlees, P.T., Illana, A., Imai, N., . . . Yajzey, R. (2023). Isospin symmetry in the T = 1, A = 62 triplet. <i>Physics Letters B</i>, <i>847</i>, Article 138249. <a href="https://doi.org/10.1016/j.physletb.2023.138249" target="_blank">https://doi.org/10.1016/j.physletb.2023.138249</a>
dc.identifier.otherCONVID_194195815
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/91939
dc.description.abstractExcited states in the Tz = 0, −1 nuclei 62Ga and 62Ge were populated in direct reactions of relativistic radioactive ion beams at the RIBF. Coincident γ rays were measured with the DALI2+ array and uniquely assigned to the A = 62 isobars. In addition, 62Ge was also studied independently at JYFL-ACCLAB using the 24Mg(40Ca,2n) 62Ge fusion-evaporation reaction. The first excited T = 1, Jπ = 2+ states in 62Ga and 62Ge were identified at 979(1) and 965(1) keV, respectively, resolving discrepant interpretations in the literature. States beyond the first 2 + state in 62Ge were also identified for the first time in the present work. The results are compared with shell-model calculations in the f p model space. Mirror and triplet energy differences are analyzed in terms of individual charge-symmetry and charge-independence breaking contributions. The MED results confirm the shrinkage of the p-orbits’ radii when they are occupied by at least one nucleon on average.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherElsevier
dc.relation.ispartofseriesPhysics Letters B
dc.rightsCC BY 4.0
dc.titleIsospin symmetry in the T = 1, A = 62 triplet
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202311167955
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiaineAccelerator Laboratoryen
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.volume847
dc.type.versionpublishedVersion
dc.rights.copyright© 2023 the Authors
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.doi10.1016/j.physletb.2023.138249
jyx.fundinginformationK. W. acknowledges the support from the Spanish Ministerio de Ciencia, Innovación y Universidades grant RYC2017-22007 and the European Research Council through the ERC Grant No. 101001561-LISA. A. P. is supported in part by grants CEX2020-001007-S funded by MCIN/AEI (Spain) /10.13039/501100011033 and PID2021-127890NBI00. The work is further supported by the UK STFC under Grants Nos. ST/L005727/1, ST/P003885/1, ST/V001035/1
dc.type.okmA1


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