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dc.contributor.authorRice, S.
dc.contributor.authorCakirli, Rabia Burcu
dc.contributor.authorPerez Cerdan, A.
dc.contributor.authorVedia, V.
dc.contributor.authorValencia, E.
dc.contributor.authorAlgora, A.
dc.contributor.authorGANİOĞLU NUTKU, Ela
dc.contributor.authorSarriguren, P.
dc.contributor.authorGuadilla, V.
dc.contributor.authorFraile, L.M.
dc.contributor.authorNácher, E.
dc.contributor.authorRubio, B.
dc.contributor.authorTain, J.L.
dc.contributor.authorAgramunt, J.
dc.contributor.authorGelletly, W.
dc.contributor.authorBriz, J.A.
dc.contributor.authorFallot, M.
dc.contributor.authorJordán, D.
dc.contributor.authorHalász, Z.
dc.contributor.authorKuti, I.
dc.contributor.authorMontaner, A.
dc.contributor.authorOnillon, A.
dc.contributor.authorOrrigo, S.E.A.
dc.date.accessioned2021-12-10T10:15:22Z
dc.date.available2021-12-10T10:15:22Z
dc.identifier.citationAlgora A., GANİOĞLU NUTKU E., Sarriguren P., Guadilla V., Fraile L., Nácher E., Rubio B., Tain J., Agramunt J., Gelletly W., et al., "Total absorption gamma-ray spectroscopy study of the beta-decay of Hg-186", PHYSICS LETTERS B, cilt.819, 2021
dc.identifier.issn0370-2693
dc.identifier.othervv_1032021
dc.identifier.otherav_344eeab5-68ef-4e8e-8c28-a05050563d71
dc.identifier.urihttp://hdl.handle.net/20.500.12627/169528
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85107816908&origin=inward
dc.identifier.urihttps://doi.org/10.1016/j.physletb.2021.136438
dc.description.abstractThe Gamow-Teller strength distribution of the decay of Hg-186 into Au-186 has been determined for the first time using the total absorption gamma spectroscopy technique and has been compared with theoretical QRPA calculations using the SLy4 Skyrme force. The measured Gamow-Teller strength distribution and the half-life are described by mixing oblate and prolate configurations independently in the parent and daughter nuclei. In this theoretical framework the best description of the experimental beta strength is obtained with dominantly prolate components for both parent Hg-186 and daughter Au-186. The approach also allowed us to determine an upper limit of the oblate component in the parent state. The complexity of the analysis required the development of a new approach in the analysis of the X-ray gated total absorption spectrum. (C) 2021 The Authors. Published by Elsevier B.V.
dc.language.isoeng
dc.subjectTemel Bilimler
dc.subjectPhysics and Astronomy (miscellaneous)
dc.subjectGeneral Physics and Astronomy
dc.subjectSpace and Planetary Science
dc.subjectNuclear and High Energy Physics
dc.subjectAstronomy and Astrophysics
dc.subjectPhysical Sciences
dc.subjectFİZİK, PARTİKLER VE ALANLAR
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Parçacıklar ve Alanlar
dc.subjectFizik
dc.subjectFİZİK, NÜKLEER
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleTotal absorption gamma-ray spectroscopy study of the beta-decay of Hg-186
dc.typeMakale
dc.relation.journalPHYSICS LETTERS B
dc.contributor.departmentUniversitat de València , ,
dc.identifier.volume819
dc.contributor.firstauthorID2685573


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