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dc.contributor.authorKostensalo, Joel
dc.contributor.authorSuhonen, Jouni
dc.date.accessioned2017-09-04T10:53:29Z
dc.date.available2017-09-04T10:53:29Z
dc.date.issued2017
dc.identifier.citationKostensalo, J., & Suhonen, J. (2017). gA-driven shapes of electron spectra of forbidden β decays in the nuclear shell model. <i>Physical Review C</i>, <i>96</i>(2), Article 024317. <a href="https://doi.org/10.1103/PhysRevC.96.024317" target="_blank">https://doi.org/10.1103/PhysRevC.96.024317</a>
dc.identifier.otherCONVID_27175511
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/55268
dc.description.abstractThe evolution of the shape of the electron spectra of 16 forbidden β− decays as a function of gA was studied using the nuclear shell model in appropriate single-particle model spaces with established, well-tested nuclear Hamiltonians. The β spectra of 94Nb(6+)→94Mo(4+) and 98Tc(6+)→98Ru(4+) were found to depend strongly on gA, which makes them excellent candidates for the determination of the effective value of gA with the spectrum-shape method (SSM). A strong gA dependence is also seen in the spectrum of 96Zr(0+)→96Nb(6+). This decay could be used for determining the quenching of gA in sixth-forbidden decays in the future, when the measurement of the spectrum becomes experimentally feasible. The calculated shell-model electron spectra of the ground-state-to-ground-state decays of 87Rb, 99Tc, and 137Cs and the decay of 137Cs to the isomeric 11/2− state in 137Ba were found to be in excellent agreement with the spectra previously calculated using the microscopic quasiparticle-phonon model. This is further evidence of the robust nature of the SSM observed in the previous studies.
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.subject.othernuclear shell model
dc.titlegA-driven shapes of electron spectra of forbidden β decays in the nuclear shell model
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-201709013643
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2017-09-01T12:15:18Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries2
dc.relation.volume96
dc.type.versionpublishedVersion
dc.rights.copyright© 2017 American Physical Society. Published in this repository with the kind permission of the publisher.
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.subject.ysoelektronit
dc.subject.ysoydinfysiikka
dc.subject.ysospektrit
jyx.subject.urihttp://www.yso.fi/onto/yso/p4030
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p6086
dc.relation.doi10.1103/PhysRevC.96.024317
dc.type.okmA1


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