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Probing the shapes of <sup>186</sup>Pb

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dc.contributor.authorPakarinen, J.en
dc.contributor.authorDarby, I. G.en
dc.contributor.authorEeckhaudt, S.en
dc.contributor.authorEnqvist, T.en
dc.contributor.authorGrahn, T.en
dc.contributor.authorGreenlees, P. T.en
dc.contributor.authorHellemans, V.en
dc.contributor.authorHeyde, K.en
dc.contributor.authorJohnston-theasby, F.en
dc.contributor.authorJones, P.en
dc.contributor.authorJulin, R.en
dc.contributor.authorJuutinen, S.en
dc.contributor.authorKettunen, H.en
dc.contributor.authorLeino, M.en
dc.contributor.authorLeppänen, A. P.en
dc.contributor.authorNieminen, P.en
dc.contributor.authorNyman, M.en
dc.contributor.authorPage, R. D.en
dc.contributor.authorRaddon, P. M.en
dc.contributor.authorRahkila, P.en
dc.contributor.authorScholey, C.en
dc.contributor.authorUusitalo, J.en
dc.contributor.authorWadsworth, R.en
dc.date.accessioned2025-12-31T22:40:51Z
dc.date.available2025-12-31T22:40:51Z
dc.date.issued2006-04-26en
dc.description.abstractRecoil-decay tagging technique has been employed in the study of non-yrast states in 186Pb. High quality γγ-coincidence data have revealed three new bands and the yrast band has been extended up to I π=20+. A low-lying non-yrast band provide evidences for an oblate structure.en
dc.description.statusPeer-revieweden
dc.format.extent3en
dc.identifier.isbn0735403236en
dc.identifier.isbn9780735403239en
dc.identifier.issn0094-243Xen
dc.identifier.scopus33845500110en
dc.identifier.urihttps://hdl.handle.net/1885/733798454
dc.language.isoenen
dc.relation.ispartofFrontiers in Nuclear Structure, Astrophysics, and Reactions - FINUSTARen
dc.relation.ispartofseriesAIP Conference Proceedingsen
dc.relation.ispartofseriesInternational Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions - FINUSTARen
dc.subjectGamma spectroscopyen
dc.subjectRecoil decay taggingen
dc.subjectShape coexistenceen
dc.titleProbing the shapes of <sup>186</sup>Pben
dc.typeConference paperen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage531en
local.bibliographicCitation.startpage529en
local.contributor.affiliationPakarinen, J.; University of Jyväskyläen
local.contributor.affiliationDarby, I. G.; University of Liverpoolen
local.contributor.affiliationEeckhaudt, S.; University of Jyväskyläen
local.contributor.affiliationEnqvist, T.; University of Jyväskyläen
local.contributor.affiliationGrahn, T.; University of Jyväskyläen
local.contributor.affiliationGreenlees, P. T.; University of Jyväskyläen
local.contributor.affiliationHellemans, V.; Ghent Universityen
local.contributor.affiliationHeyde, K.; Ghent Universityen
local.contributor.affiliationJohnston-theasby, F.; University of Yorken
local.contributor.affiliationJones, P.; University of Jyväskyläen
local.contributor.affiliationJulin, R.; University of Jyväskyläen
local.contributor.affiliationJuutinen, S.; University of Jyväskyläen
local.contributor.affiliationKettunen, H.; University of Jyväskyläen
local.contributor.affiliationLeino, M.; University of Jyväskyläen
local.contributor.affiliationLeppänen, A. P.; University of Jyväskyläen
local.contributor.affiliationNieminen, P.; Department of Nuclear Physics & Accelerator Applications, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationNyman, M.; University of Jyväskyläen
local.contributor.affiliationPage, R. D.; University of Liverpoolen
local.contributor.affiliationRaddon, P. M.; University of Yorken
local.contributor.affiliationRahkila, P.; University of Jyväskyläen
local.contributor.affiliationScholey, C.; University of Jyväskyläen
local.contributor.affiliationUusitalo, J.; University of Jyväskyläen
local.contributor.affiliationWadsworth, R.; University of Yorken
local.identifier.ariespublicationU3488905xPUB9366en
local.identifier.doi10.1063/1.2201005en
local.identifier.essn1551-7616en
local.identifier.pure842bd31d-d3dc-425c-9fc9-9afd2ac0d2eben
local.identifier.urlhttps://www.scopus.com/pages/publications/33845500110en
local.type.statusPublisheden

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