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dc.contributor.authorLehnert, B.
dc.contributor.authorHult, M.
dc.contributor.authorLutter, G.
dc.contributor.authorMarissens, G.
dc.contributor.authorOberstedt, S.
dc.contributor.authorStroh, H.
dc.contributor.authorKotila, J.
dc.contributor.authorOberstedt, A.
dc.contributor.authorZuber, K.
dc.date.accessioned2022-06-16T10:21:23Z
dc.date.available2022-06-16T10:21:23Z
dc.date.issued2022
dc.identifier.citationLehnert, B., Hult, M., Lutter, G., Marissens, G., Oberstedt, S., Stroh, H., Kotila, J., Oberstedt, A., & Zuber, K. (2022). Constraints on partial half-lives of 136Ce and 138Ce double electron captures. <i>Physical Review C</i>, <i>105</i>(4), Article 045801. <a href="https://doi.org/10.1103/PhysRevC.105.045801" target="_blank">https://doi.org/10.1103/PhysRevC.105.045801</a>
dc.identifier.otherCONVID_146538756
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/81804
dc.description.abstractThe γ-ray emissions from a radiopure cerium-bromide crystal with a mass of 4381 g were measured for a total of 497.4 d by means of high-resolution γ-ray spectrometry in the HADES underground laboratory at a depth of 500 m.w.e. A search for 0/2νεε and 0/2νεβ+ double beta decay transitions of 136Ce and 138Ce was performed using Bayesian analysis techniques. No signals were observed for a total of 35 investigated decay modes. 90% credibility limits were set in the order of 1018–1019 yr. Existing constraints from a cerium oxide powder measurement were tested with a different cerium compound and half-life limits could be improved for most of the decay modes. The most likely accessible decay mode of the 136Ce 2νεε transition into the 0+1 state of 136Ba results in a new best 90% credibility limit of 5.0×1018 yr.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review C
dc.rightsCC BY 4.0
dc.titleConstraints on partial half-lives of 136Ce and 138Ce double electron captures
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202206163413
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosKoulutuksen tutkimuslaitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.laitosFinnish Institute for Educational Researchen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries4
dc.relation.volume105
dc.type.versionpublishedVersion
dc.rights.copyright©2022 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber314733
dc.relation.grantnumber320062
dc.subject.ysoydinfysiikka
dc.subject.ysopuoliintumisaika
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p12173
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevC.105.045801
dc.relation.funderResearch Council of Finlanden
dc.relation.funderResearch Council of Finlanden
dc.relation.funderSuomen Akatemiafi
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramAcademy Research Fellow, AoFen
jyx.fundingprogramResearch costs of Academy Research Fellow, AoFen
jyx.fundingprogramAkatemiatutkija, SAfi
jyx.fundingprogramAkatemiatutkijan tutkimuskulut, SAfi
jyx.fundinginformationThis work received support from the EC-JRC open access scheme EUFRAT under Horizon-2020, Project No. 35375-1. EIG EURIDICE and the staff of HADES are gratefully acknowledged for their work. One of the authors (A.O.) acknowledges support from the Extreme Light Infrastructure Nuclear Physics (ELI-NP) Phase II, a project cofinanced by the Romanian Government and the European Union through the European Regional Development Fund, the Competitiveness Operational Programme (1/07.07.2016, COP, ID 1334). Another author (J.K.) acknowledges support from the Academy of Finland, Grants No. 314733 and No. 320062. The work of B.L. is supported by Lawrence Berkeley National Laboratory under the U.S. Department of Energy Federal Prime Agreement No. DE-AC02-05CH11231.
dc.type.okmA1


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