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dc.contributor.authorBes, D.R.
dc.contributor.authorCivitarese, Osvaldo
dc.contributor.authorSuhonen, Jouni
dc.date.accessioned2016-02-18T11:07:45Z
dc.date.available2016-02-18T11:07:45Z
dc.date.issued2012
dc.identifier.citationBes, D.R., Civitarese, O., & Suhonen, J. (2012). Schematic and realistic model calculations of the isovector spin monopole excitations in 116In. <i>Physical Review C</i>, <i>86</i>(2), Article 024314. <a href="https://doi.org/10.1103/PhysRevC.86.024314" target="_blank">https://doi.org/10.1103/PhysRevC.86.024314</a>
dc.identifier.otherCONVID_22313447
dc.identifier.otherTUTKAID_55688
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/48824
dc.description.abstractThe excitation of Gamow-Teller (GT) and isovector spin monopole (IVSM) J π = 1+ modes in 116In by (p,n) and (n, p) charge-exchange reactions on 116Cd and on 116Sn, respectively, is studied within the framework of the quasiparticle random-phase approximation. The calculations have been performed both for schematic and realistic model situations. It appears that the calculated admixture of the IVSM and Gamow-Teller (GT) J π = 1+ excitations is negligible and that the contribution to the strength above 20 MeV of excitation energy, in 116In, is due to the IVSM (σr2t±) mode. This result is compared with the recent experimental work that reported a large amount of both (p,n) and (n,p) strength beyond 10 MeV of excitation energy in 116In. This measured excess strength has led to speculations about its importance for the double beta decay rate of 116Cd.
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.subject.otherteoreettinen ydinfysiikka
dc.subject.otherTheoretical nuclear physics
dc.titleSchematic and realistic model calculations of the isovector spin monopole excitations in 116In
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201601201203
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.updated2016-01-20T13:15:27Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn0556-2813
dc.relation.numberinseries2
dc.relation.volume86
dc.type.versionpublishedVersion
dc.rights.copyright© 2012 American Physical Society. Published in this repository with the kind permission of the publisher.
dc.rights.accesslevelopenAccessfi
dc.relation.doi10.1103/PhysRevC.86.024314
dc.type.okmA1


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