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dc.contributor.authorGaffney, L. P.
dc.contributor.authorHackstein, M.
dc.contributor.authorPage, R. D.
dc.contributor.authorGrahn, Tuomas
dc.contributor.authorScheck, M.
dc.contributor.authorButler, P. A.
dc.contributor.authorBertone, P. F.
dc.contributor.authorBree, N.
dc.contributor.authorCarroll, R. J.
dc.contributor.authorCarpenter, M. P.
dc.contributor.authorChiara, C. J.
dc.contributor.authorDewald, A.
dc.contributor.authorFilmer, F.
dc.contributor.authorFransen, C.
dc.contributor.authorHuyse, M.
dc.contributor.authorJanssens, R. V. F.
dc.contributor.authorJoss, D. T.
dc.contributor.authorJulin, Rauno
dc.contributor.authorKondev, F. G.
dc.contributor.authorNieminen, Päivi
dc.contributor.authorPakarinen, Janne
dc.contributor.authorRigby, S. V.
dc.contributor.authorRother, W.
dc.contributor.authorVan Duppen, P.
dc.contributor.authorWatkins, H. V.
dc.contributor.authorWrzosek-Lipska, K.
dc.contributor.authorZhu, S.
dc.date.accessioned2014-09-01T08:57:16Z
dc.date.available2014-09-01T08:57:16Z
dc.date.issued2014
dc.identifier.citationGaffney, L. P., Hackstein, M., Page, R. D., Grahn, T., Scheck, M., Butler, P. A., Bertone, P. F., Bree, N., Carroll, R. J., Carpenter, M. P., Chiara, C. J., Dewald, A., Filmer, F., Fransen, C., Huyse, M., Janssens, R. V. F., Joss, D. T., Julin, R., Kondev, F. G., . . . Zhu, S. (2014). Shape coexistence in neutron-deficient Hg isotopes studied via lifetime measurements in Hg-184,Hg-186 and two-state mixing calculations. <i>Physical Review C</i>, <i>89</i>(2), Article 024307. <a href="https://doi.org/10.1103/PhysRevC.89.024307" target="_blank">https://doi.org/10.1103/PhysRevC.89.024307</a>
dc.identifier.otherCONVID_23760293
dc.identifier.otherTUTKAID_62356
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/44160
dc.description.abstractAbstract: The neutron-deficient mercury isotopes, 184 , 186 Hg, were studied with the recoil distance Doppler-shift method using the Gammasphere array and the K ̈ oln plunger device. The differential decay curve method was employed to determine the lifetimes of the yrast states in 184 , 186 Hg. An improvement on previously measured values of yrast states up to 8 + is presented as well as first values for the 9 3 state in 184 Hg and 10 + state in 186 Hg. B ( E 2) values are calculated and compared to a two-state mixing model which utilizes the variable moment of inertia model, allowing for extraction of spin-dependent mixing strengths and amplitudes.fi
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.relation.urihttp://journals.aps.org/prc/abstract/10.1103/PhysRevC.89.024307
dc.subject.otherlight mercury isotopes
dc.subject.otherdecay curve method
dc.subject.otherhigh-spin states
dc.titleShape coexistence in neutron-deficient Hg isotopes studied via lifetime measurements in Hg-184,Hg-186 and two-state mixing calculations
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201408292687
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineFysiikkafi
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiainePhysicsen
dc.contributor.oppiaineAccelerator Laboratoryen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2014-08-29T03:30:04Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn0556-2813
dc.relation.numberinseries2
dc.relation.volume89
dc.type.versionpublishedVersion
dc.rights.copyright©2014 American Physical Society. This is an article whose final and definitive form has been published by American Physical Society.
dc.rights.accesslevelopenAccessfi
dc.rights.urlhttp://creativecommons.org/licenses/by/3.0/
dc.relation.doi10.1103/PhysRevC.89.024307
dc.type.okmA1


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©2014 American Physical Society. This is an article whose final and definitive form has been published by American Physical Society.
Ellei muuten mainita, aineiston lisenssi on ©2014 American Physical Society. This is an article whose final and definitive form has been published by American Physical Society.