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dc.contributor.authorRakopoulos, V.
dc.contributor.authorLantz, M.
dc.contributor.authorSolders, A.
dc.contributor.authorAl-Adili, A.
dc.contributor.authorMattera, A.
dc.contributor.authorCanete, Laetitia
dc.contributor.authorEronen, Tommi
dc.contributor.authorGorelov, Dmitry
dc.contributor.authorJokinen, Ari
dc.contributor.authorKankainen, Anu
dc.contributor.authorKolhinen, Veli
dc.contributor.authorMoore, Iain
dc.contributor.authorNesterenko, Dmitrii
dc.contributor.authorPenttilä, Heikki
dc.contributor.authorPohjalainen, Ilkka
dc.contributor.authorRinta-Antila, Sami
dc.contributor.authorSimutkin, V.
dc.contributor.authorVilén, Markus
dc.contributor.authorVoss, Annika
dc.contributor.authorPomp, S.
dc.date.accessioned2018-08-22T10:31:40Z
dc.date.available2018-08-22T10:31:40Z
dc.date.issued2018
dc.identifier.citationRakopoulos, V., Lantz, M., Solders, A., Al-Adili, A., Mattera, A., Canete, L., Eronen, T., Gorelov, D., Jokinen, A., Kankainen, A., Kolhinen, V., Moore, I., Nesterenko, D., Penttilä, H., Pohjalainen, I., Rinta-Antila, S., Simutkin, V., Vilén, M., Voss, A., & Pomp, S. (2018). First isomeric yield ratio measurements by direct ion counting and implications for the angular momentum of the primary fission fragments. <i>Physical Review C</i>, <i>98</i>(2), Article 024612. <a href="https://doi.org/10.1103/physrevc.98.024612" target="_blank">https://doi.org/10.1103/physrevc.98.024612</a>
dc.identifier.otherCONVID_28213194
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/59308
dc.description.abstractWe report the first experimental determination of independent isomeric yield ratios using direct ion counting with a Penning trap, which offered such a high resolution in mass that isomeric states could be separated. The measurements were performed at the Ion Guide Isotope Separator On-Line (IGISOL) facility at the University of Jyväskylä. The isomer production ratios of 81Ge, 96,97Y, 128,130Sn, and 129Sb in the 25-MeV proton-induced fission of natU and 232Th were studied. Three isomeric pairs (81Ge, 96Y, and 129Sb) were measured for the first time for the natU(p,f) reaction, while all the reported yield ratios for the 232Th(p,f) reaction were determined for the first time. The comparison of the experimentally determined isomeric yield ratios with data available in the literature shows a reasonable agreement, except for the case of 130Sn for unspecified reasons. The obtained results were also compared with the gef model, where good agreement can be noticed in most cases for both reactions. Serious discrepancies can only be observed for the cases of 96,97Y for both reactions. Moreover, based on the isomeric yield ratios, the root-mean-square angular momenta (Jrms) of the fission fragments after scission were estimated using the talys code. The experimentally determined isomeric yield ratios, and consequently the deduced Jrms, for 130Sn are significantly lower compared to 128Sn for both fissioning systems. This can be attributed to the more spherical shape of the fragments that contribute to the formation of 130Sn, due to their proximity to the N=82 shell closure. The values of Jrms for 129Sb are higher than 128Sn for both reactions, despite the same neutron number of both nuclides (N=78), indicating the odd-Z effect where fission fragments with odd-Z number tend to bear larger angular momentum than even-Z fragments. The isomer production ratio for the isotopes of Sn is more enhanced in the natU(p,f) reaction than in 232Th(p,f). The opposite is observed for 96Y and 97Y. These discrepancies might be associated to different scission shapes of the fragments for the two fission reactions, indicating the impact that the different fission modes can have on the isomeric yield ratios.fi
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.rightsIn Copyright
dc.subject.otherfission
dc.subject.otherisomer decays
dc.titleFirst isomeric yield ratio measurements by direct ion counting and implications for the angular momentum of the primary fission fragments
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-201808203862
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.updated2018-08-20T06:15:19Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries2
dc.relation.volume98
dc.type.versionpublishedVersion
dc.rights.copyright© 2018 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.relation.grantnumber312544
dc.relation.grantnumber275389
dc.relation.grantnumber284516
dc.relation.grantnumber295207
dc.subject.ysofissio
dc.subject.ysoydinreaktiot
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p18705
jyx.subject.urihttp://www.yso.fi/onto/yso/p12413
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/physrevc.98.024612
dc.relation.funderSuomen Akatemiafi
dc.relation.funderSuomen Akatemiafi
dc.relation.funderSuomen Akatemiafi
dc.relation.funderSuomen Akatemiafi
dc.relation.funderResearch Council of Finlanden
dc.relation.funderResearch Council of Finlanden
dc.relation.funderResearch Council of Finlanden
dc.relation.funderResearch Council of Finlanden
jyx.fundingprogramAkatemiatutkijan tutkimuskulut, SAfi
jyx.fundingprogramAkatemiatutkija, SAfi
jyx.fundingprogramAkatemiatutkijan tutkimuskulut, SAfi
jyx.fundingprogramAkatemiatutkija, SAfi
jyx.fundingprogramResearch costs of Academy Research Fellow, AoFen
jyx.fundingprogramAcademy Research Fellow, AoFen
jyx.fundingprogramResearch costs of Academy Research Fellow, AoFen
jyx.fundingprogramAcademy Research Fellow, AoFen
jyx.fundinginformationThis work was supported by the European Commission within the Seventh Framework Programme through Fission-2013-CHANDA (Project No. 605203), the Swedish Radiation Safety Authority (SSM), the Swedish Nuclear Fuel and Waste Management Co. (SKB), and the Academy of Finland under the Finnish Centre of Excellence Programme 2012–2017 (Nuclear and Accelerator Based Physics Research at JYFL). A.K. acknowledges support from Academy of Finland under Projects No. 275389, No. 284516, and No. 312544. T.E. acknowledges support from Academy of Finland under Project No. 295207.
dc.type.okmA1


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