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dc.contributor.authorGuadilla, V.
dc.contributor.authorAlgora, A.
dc.contributor.authorTain, J. L.
dc.contributor.authorAgramunt, J.
dc.contributor.authorÄystö, J.
dc.contributor.authorBriz, J. A.
dc.contributor.authorCucoanes, A.
dc.contributor.authorEronen, T.
dc.contributor.authorEstienne, M.
dc.contributor.authorFallot, M.
dc.contributor.authorFraile, L. M.
dc.contributor.authorGanioğlu, E.
dc.contributor.authorGelletly, W.
dc.contributor.authorGorelov, D.
dc.contributor.authorHakala, J.
dc.contributor.authorJokinen, A.
dc.contributor.authorJordan, D.
dc.contributor.authorKankainen, A.
dc.contributor.authorKolhinen, V.
dc.contributor.authorKoponen, J.
dc.contributor.authorLebois, M.
dc.contributor.authorLe Meur, L.
dc.contributor.authorMartinez, T.
dc.contributor.authorMonserrate, M.
dc.contributor.authorMontaner-Pizá, A.
dc.contributor.authorMoore, I.
dc.contributor.authorNácher, E.
dc.contributor.authorOrrigo, S. E. A.
dc.contributor.authorPenttilä, H.
dc.contributor.authorPohjalainen, I.
dc.contributor.authorPorta, A.
dc.contributor.authorReinikainen, J.
dc.contributor.authorReponen, M.
dc.contributor.authorRinta-Antila, S.
dc.contributor.authorRubio, B.
dc.contributor.authorRytkönen, K.
dc.contributor.authorSarriguren, P.
dc.contributor.authorShiba, T.
dc.contributor.authorSonnenschein, V.
dc.contributor.authorSonzogni, A. A.
dc.contributor.authorValencia, E.
dc.contributor.authorVedia, V.
dc.contributor.authorVoss, A.
dc.contributor.authorWilson, J. N.
dc.contributor.authorZakari-Issoufou, A. A.
dc.date.accessioned2019-08-23T04:37:51Z
dc.date.available2019-08-23T04:37:51Z
dc.date.issued2019
dc.identifier.citationGuadilla, V.; Algora, A.; Tain, J. L.; Agramunt, J.; Äystö, J.; Briz, J. A.; Cucoanes, A.; Eronen, T.; Estienne, M.; Fallot, M.; Fraile, L. M.; Ganioğlu, E.; Gelletly, W.; Gorelov, D.; Hakala, J. et al. (2019). Total absorption γ-ray spectroscopy of niobium isomers. Physical Review C, 100 (2), 024311. DOI: 10.1103/PhysRevC.100.024311
dc.identifier.otherCONVID_32282548
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/65276
dc.description.abstractThe β-intensity distributions of the decays of 100 gs, 100 m Nb and 102 gs, 102 m Nb have been determined using the total absorption γ-ray spectroscopy technique. The JYFLTRAP double Penning trap system was employed in a campaign of challenging measurements performed with the decay total absorption γ-ray spectrometer at the Ion Guide Isotope Separator On-Line facility in Jyväskylä. Different strategies were applied to disentangle the isomeric states involved, lying very close in energy. The low-spin component of each niobium case was populated through the decay of the zirconium parent, which was treated as a contaminant. We have applied a method to extract this contamination, and additionally we have obtained β-intensity distributions for these zirconium decays. The β-strength distributions evaluated with these results were compared with calculations in a quasiparticle random-phase approximation, suggesting a prolate configuration for the ground states of 100, 102 Zr. The footprint of the Pandemonium effect was found when comparing our results for the analyses of the niobium isotopes with previous decay data. The β-intensities of the decay of 102 m Nb, for which there were no previous data, were obtained. A careful evaluation of the uncertainties was carried out, and the consistency of our results was validated taking advantage of the segmentation of our spectrometer. The final results were used as input in reactor summation calculations. A large impact on antineutrino spectrum calculations was already reported, and here we detail the significant impact on decay heat calculations.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.rightsIn Copyright
dc.subject.otherbeta decay
dc.subject.otherisomer decays
dc.subject.othernuclear structure and decays
dc.titleTotal absorption γ-ray spectroscopy of niobium isomers
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201908233877
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries2
dc.relation.volume100
dc.type.versionpublishedVersion
dc.rights.copyright© 2019 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.subject.ysoydinfysiikka
dc.subject.ysospektroskopia
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p10176
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevC.100.024311
jyx.fundinginformationThis work has been supported by the Spanish Ministerio de Economía y Competitividad under Grants No. FPA2011- 24553, No. AIC-A-2011-0696, No. FPA2014-52823-C2-1- P, No. FPA2015-65035-P, No. FPI/BES-2014-068222, No. FPA2017-83946-C2-1-P, and the program Severo Ochoa (SEV-2014-0398), by the Spanish Ministerio de Educación under the FPU12/01527 Grant, by the European Commission under the FP7/EURATOM Contract No. 605203 and the FP7/ENSAR Contract No. 262010, and by the Junta para la Ampliación de Estudios Programme (CSIC JAE-Doc contract) co-financed by ESF. We acknowledge the support of the UK Science and Technology Facilities Council (STFC) Grant No. ST/P005314/1. This work was also supported by the Academy of Finland under the Finnish Centre of Excellence Programme (Project No. 213503, Nuclear and AcceleratorBased Physics Research at JYFL). The authors thank the IAEA for supporting and encouraging the work in this field.


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