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dc.contributor.authorIDS Collaboration
dc.date.accessioned2019-02-25T12:26:09Z
dc.date.available2019-02-25T12:26:09Z
dc.date.issued2019
dc.identifier.citationIDS Collaboration. (2019). β decay of 133In : γ emission from neutron-unbound states in 133Sn. <i>Physical Review C</i>, <i>99</i>(2), Article 024304. <a href="https://doi.org/10.1103/PhysRevC.99.024304" target="_blank">https://doi.org/10.1103/PhysRevC.99.024304</a>
dc.identifier.otherCONVID_28935378
dc.identifier.otherTUTKAID_80747
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/62959
dc.description.abstractExcited states in 133Sn were investigated through the β decay of 133In at the ISOLDE facility. The ISOLDE Resonance Ionization Laser Ion Source (RILIS) provided isomer-selective ionization for 133In, allowing us to study separately, and in detail, the β-decay branch of 133In Jπ = (9/2+) ground state and its Jπ = (1/2−) isomer. Thanks to the large spin difference of the two β-decaying states of 133In, it is possible to investigate separately the lower and higher spin states in the daughter, 133Sn, and thus to probe independently different single-particle and single-hole levels. We report here new γ transitions observed in the decay of 133In, including those assigned to the deexcitation of the neutron-unbound states.fi
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.rightsCC BY 4.0
dc.subject.otherbeta decay
dc.subject.otherexcited states
dc.titleβ decay of 133In : γ emission from neutron-unbound states in 133Sn
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201902221624
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiaineAccelerator Laboratoryen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2019-02-22T16:15:06Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries2
dc.relation.volume99
dc.type.versionpublishedVersion
dc.rights.copyright© 2019 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber654002
dc.relation.grantnumber654002
dc.relation.projectidinfo:eu-repo/grantAgreement/EC/H2020/654002/EU//
dc.subject.ysotina
dc.subject.ysoydinfysiikka
dc.subject.ysoindium
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15916
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p38731
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevC.99.024304
dc.relation.funderEuroopan komissiofi
dc.relation.funderEuropean Commissionen
jyx.fundingprogramResearch infrastructures, H2020fi
jyx.fundingprogramResearch infrastructures, H2020en
jyx.fundinginformationWe acknowledge the support of the ISOLDE Collaboration and technical teams. This work was supported in part by the Polish National Science Center under Contract No. UMO-2015/18/E/ST2/00217 and under Contract No. UMO-2015/18/M/ST2/00523, by the Spanish MINECO via FPA2015-65035-P project, by the Portuguese FCT via CERN/FIS-NUC/0004/2015 and CERN-FIS-PAR-0005-2017 projects. The research leading to these results has received funding from the European Union's Horizon 2020 research and innovation programme under Grant Agreement No. 654002.
dc.type.okmA1


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