Näytä suppeat kuvailutiedot

dc.contributor.authorPasqualato, G.
dc.contributor.authorGottardo, A.
dc.contributor.authorMengoni, D.
dc.contributor.authorGoasduff, A.
dc.contributor.authorValiente-Dobón, J. J.
dc.contributor.authorNowacki, F.
dc.contributor.authorPéru, S.
dc.contributor.authorPillet, N.
dc.contributor.authorde Angelis, G.
dc.contributor.authorBakes, S. D.
dc.contributor.authorBayram, T.
dc.contributor.authorBazzacco, D.
dc.contributor.authorBenzoni, G.
dc.contributor.authorBrugnara, D.
dc.contributor.authorCicerchia, M.
dc.contributor.authorColovic, P.
dc.contributor.authorCortés, M. L.
dc.contributor.authorGadea, A.
dc.contributor.authorGaltarossa, F.
dc.contributor.authorGórska, M.
dc.contributor.authorGozzelino, A.
dc.contributor.authorGregor, E.
dc.contributor.authorHubbard, N.
dc.contributor.authorIllana, A.
dc.contributor.authorJurado, M.
dc.contributor.authorLenzi, S. M.
dc.contributor.authorMantovani, G.
dc.contributor.authorMarchi, T.
dc.contributor.authorMenegazzo, R.
dc.contributor.authorMontaner-Pizá, A.
dc.contributor.authorNapoli, D. R.
dc.contributor.authorRecchia, F.
dc.contributor.authorSiciliano, M.
dc.contributor.authorTestov, D.
dc.contributor.authorSzilner, S.
dc.contributor.authorZanon, I.
dc.date.accessioned2023-09-11T10:16:55Z
dc.date.available2023-09-11T10:16:55Z
dc.date.issued2023
dc.identifier.citationPasqualato, G., Gottardo, A., Mengoni, D., Goasduff, A., Valiente-Dobón, J.J., Nowacki, F., Péru, S., Pillet, N., de Angelis, G., Bakes, S. D., Bayram, T., Bazzacco, D., Benzoni, G., Brugnara, D., Cicerchia, M., Colovic, P., Cortés, M. L., Gadea, A., Galtarossa, F., . . . Zanon, I. (2023). An alternative viewpoint on the nuclear structure towards 100Sn : Lifetime measurements in 105Sn. <i>Physics Letters B</i>, <i>845</i>, Article 138148. <a href="https://doi.org/10.1016/j.physletb.2023.138148" target="_blank">https://doi.org/10.1016/j.physletb.2023.138148</a>
dc.identifier.otherCONVID_184743672
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/89020
dc.description.abstractThis work aims at presenting an alternative approach to the long standing problem of the B(E2) values in Sn isotopes in the vicinity of the N=Z double-magic nucleus 100Sn, until now predominantly measured with relativistic and intermediate-energy Coulomb excitation reactions. The direct measurement of the lifetime of low-lying excited states in odd-even Sn isotopes provides a new and precise guidance for the theoretical description of the nuclear structure in this region. Lifetime measurements have been performed in 105Sn for the first time with the coincidence Recoil Distance Doppler Shift technique. The lifetime results for the 7/2+ 1 first excited state and the 11/2+ 1 state, 2+(104Sn) ⊗ ν1g7/2 multiplet member, are discussed in comparison with state-of-the-art shell model and mean field calculations, highlighting the crucial contribution of proton excitation across the core of 100Sn. The reduced transition probability B(E2) of the 11/2+ 1 core-coupled state points out an enhanced staggering with respect to the B(E2; 2+ 1 →0+ 1 ) in the even-mass 104Sn and 106Sn isotopes.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherElsevier
dc.relation.ispartofseriesPhysics Letters B
dc.rightsCC BY 4.0
dc.subject.othernuclear structure
dc.subject.otherγ-ray spectroscopy
dc.subject.othertransition probabilities
dc.subject.otherneutron-deficient isotopes
dc.subject.otherodd-mass nuclei
dc.subject.otherlifetime measurements
dc.titleAn alternative viewpoint on the nuclear structure towards 100Sn : Lifetime measurements in 105Sn
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202309115047
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.volume845
dc.type.versionpublishedVersion
dc.rights.copyright© 2023 The Authors. Published by Elsevier B.V.
dc.rights.accesslevelopenAccessfi
dc.subject.ysospektroskopia
dc.subject.ysoydinfysiikka
dc.subject.ysoisotoopit
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p10176
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p6387
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1016/j.physletb.2023.138148
jyx.fundinginformationThe work of the author G.P. of this paper has been partly funded by the P2IO LabEx (ANR-10-LABX-0038) in the framework “Investissements d'Avenir” (ANR-11-IDEX-0003-01) managed by the French National Research Agency (ANR). M.S. acknowledge the support of the OASIS project no. ANR-17-CE31-0026 and the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under contract number DE-AC02-06CH11357. The work of A.G. was supported by MCIN/AEI/10.13039/501100011033 and Generalitat Valenciana, Spain under grants FPA2017-84756-C4, PID2020-118265GB-C4, PROMETEO 2019/005 and by the EU FEDER funds. Support for S.S. and P.C. were provided by the Croatian Science Foundation under the project IP-2018-01-1257, and by Scientific Center of Excellence for Advance Materials and Sensors in Zagreb.
dc.type.okmA1


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