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Detailed spectroscopy of doubly magic Sn-132

dc.contributor.authorBenito García, Jaime
dc.contributor.authorFraile Prieto, Luis Mario
dc.contributor.authorCarmona, M.
dc.contributor.authorGalve Lahoz, Pablo
dc.contributor.authorGarcía Díez, Miguel
dc.contributor.authorIbañez, P.
dc.contributor.authorLópez Montes, Alejandro
dc.contributor.authorMartínez, M. C.
dc.contributor.authorSánchez Parcerisa, Daniel
dc.contributor.authorSánchez Tembleque Verbo, Víctor
dc.contributor.authorUdías Moinelo, José Manuel
dc.contributor.authorVedia Fernández, María Victoria
dc.contributor.authorVilla Abaunza, Amaia
dc.date.accessioned2023-06-16T15:22:36Z
dc.date.available2023-06-16T15:22:36Z
dc.date.issued2020-07-29
dc.description© Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Artículo firmado por 88 autores. We acknowledge the support of the ISOLDE Collaboration and the ISOLDE technical teams, and by the European Union Horizon 2020 research and innovation programme under Grant Agreement No. 654002. This work was partially funded by the Spanish government via Projects No. FPA201565035-P, No. FPA-64969-P, No. FPA2017-87568-P, and No. RTI2018-098868-B-I00; the Polish National Science Center under Contracts No. UMO-2015/18/E/ST2/00217, No. UMO-2015/18/M/ST2/00523, and No. UMO2019/33/N/ST2/03023; the Portuguese FCT via CERN/FIS-NUC/0004/2015 project; the German BMBF under Contract No. 05P18PKCIA; the Romanian IFA Grant CERN/ISOLDE; and by grants from the U.K. Science and Technology Facilities Council, the Research Foundation Flanders (FWO, Belgium), the Excellence of Science program (EOS, FWO-FNRS, Belgium), and the GOA/2015/010 (BOF KU Leuven). J.B. acknowledges support from the Universidad Complutense de Madrid under the Predoctoral Grant No. CT27/16-CT28/16.
dc.description.abstractThe structure of the doubly magic Sn-132(50)82 has been investigated at the ISOLDE facility at CERN, populated both by the beta(-) decay of In-132 and beta(-)-delayed neutron emission of In-133. The level scheme of Sn-13(2) is greatly expanded with the addition of 68 gamma transitions and 17 levels observed for the first time in the beta decay. The information on the excited structure is completed by new gamma transitions and states populated in the beta-n decay of In-133. Improved delayed neutron emission probabilities are obtained both for In-132 and In-133. Level lifetimes are measured via the advanced time-delayed beta gamma gamma(t) fast-timing method. An interpretation of the level structure is given based on the experimental findings and the particle-hole configurations arising from core excitations both from the N = 82 and Z = 50 shells, leading to positive- and negative-parity particle-hole multiplets. The experimental information provides new data to challenge the theoretical description of Sn-132.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipUnión Europea. Horizonte 2020
dc.description.sponsorshipMinisterio de Economía y Competitividad (MINECO)
dc.description.sponsorshipPolish National Science Center
dc.description.sponsorshipISOLDE
dc.description.sponsorshipPortuguese FCT Portuguese Foundation for Science and Technology
dc.description.sponsorshipGerman BMBF Federal Ministry of Education & Research (BMBF)
dc.description.sponsorshipRomanian IFA Grant CERN/ISOLDE
dc.description.sponsorshipU.K. Science and Technology Facilities Council
dc.description.sponsorshipResearch Foundation Flanders (FWO, Belgium)
dc.description.sponsorshipExcellence of Science program (EOS, FWO-FNRS, Belgium) Fonds de la Recherche Scientifique - FNRS
dc.description.sponsorshipBOF KU LeuvenKU Leuven
dc.description.sponsorshipUniversidad Complutense de Madrid
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/62100
dc.identifier.doi10.1103/PhysRevC.102.014328
dc.identifier.issn0556-2813
dc.identifier.officialurlhttps://doi.org/10.1103/PhysRevC.102.014328
dc.identifier.relatedurlhttps://journals.aps.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/6522
dc.issue.number1
dc.journal.titlePhysical Review C
dc.language.isoeng
dc.publisherAmer Physical Soc
dc.relation.projectIDENSAR2 (654002)
dc.relation.projectID(FPA201565035-P; FPA-64969-P; FPA2017-87568-P; RTI2018-098868-B-I00)
dc.relation.projectID(UMO-2015/18/E/ST2/00217; UMO-2015/18/M/ST2/00523; UMO2019/33/N/ST2/03023)
dc.relation.projectIDCERN/FIS-NUC/0004/2015
dc.relation.projectID05P18PKCIA
dc.relation.projectIDGOA/2015/010
dc.relation.projectIDCT27/16-CT28/16
dc.rightsAtribución 3.0 España
dc.rights.accessRightsopen access
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/es/
dc.subject.cdu539.1
dc.subject.keywordShell nucleus sn-132
dc.subject.keywordPicosecond lifetime measurements
dc.subject.keywordNeutron-rich nuclei
dc.subject.keywordBeta-decay
dc.subject.keywordStates
dc.subject.keywordFission
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleDetailed spectroscopy of doubly magic Sn-132
dc.typejournal article
dc.volume.number102
dspace.entity.typePublication
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