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dc.contributor.authorSuhonen, Jouni
dc.date.accessioned2016-02-18T11:04:47Z
dc.date.available2016-02-18T11:04:47Z
dc.date.issued2013
dc.identifier.citationSuhonen, J. (2013). Analysis of double-beta transitions in 78^Kr. <i>Physical Review C</i>, <i>87</i>, Article 34318. <a href="https://doi.org/10.1103/PhysRevC.87.034318" target="_blank">https://doi.org/10.1103/PhysRevC.87.034318</a>
dc.identifier.otherCONVID_23219265
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/48823
dc.description.abstractIn this paper a comprehensive theoretical analysis of the two-neutrino (2ν2β) and neutrinoless (0ν2β) doublebeta decays of 78Kr is performed by evaluating the corresponding nuclear matrix elements by combining the quasiparticle random-phase approximation with the multiple-commutator model. Transitions to the ground state 0+ gs and 0+ and 2+ excited states in 78Se are investigated by using G-matrix-based nuclear forces. The channels β+β+, β+EC, and ECEC are discussed for the 2ν2β decays and the channels β+β+ and β+EC for the 0ν2β decays. The associated half-lives are computed to see if the detection of some of these transitions is experimentally feasible.
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.subject.otherteoreettinen ydinfysiikka
dc.subject.othertheoretical nuclear physics
dc.titleAnalysis of double-beta transitions in 78^Kr
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-201601201194
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineFysiikkafi
dc.contributor.oppiainePhysicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2016-01-20T13:15:05Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn0556-2813
dc.relation.volume87
dc.type.versionpublishedVersion
dc.rights.copyright© 2013 American Physical Society. Published in this repository with the kind permission of the publisher.
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.relation.doi10.1103/PhysRevC.87.034318
dc.type.okmA1


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