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dc.creatorCaballero Folch, R.es
dc.creatorDomingo Pardo, Césares
dc.creatorAgramunt-Ros, J.es
dc.creatorAlgora, A.es
dc.creatorAmeil, F.es
dc.creatorAyyad, Y.es
dc.creatorGuerrero Sánchez, Carloses
dc.date.accessioned2019-06-11T10:20:34Z
dc.date.available2019-06-11T10:20:34Z
dc.date.issued2017-06-23
dc.identifier.citationCaballero Folch, R., Domingo Pardo, C., Agramunt-Ros, J., Algora, A., Ameil, F., Ayyad, Y. y Guerrero Sánchez, C. (2017). β-decay half-lives and β-delayed neutron emission probabilities for several isotopes of Au, Hg, Tl, Pb, and Bi, beyond N = 126. Physical Review C, 95, 064322.
dc.identifier.issn2469-9985es
dc.identifier.issn2469-9993es
dc.identifier.urihttps://hdl.handle.net/11441/87333
dc.description.abstractBackground: There have been measurements on roughly 230 nuclei that are β-delayed neutron emitters. They range from 8 He up to 150La. Apart from 210Tl, with a branching ratio of only 0.007%, no other neutron emitter has been measured beyond A = 150. Therefore, new data are needed, particularly in the region of heavy nuclei around N = 126, in order to guide theoretical models and help understand the formation of the third r-process peak at A ∼ 195. Purpose: To measure both β-decay half-lives and neutron branching ratios of several neutron-rich Au, Hg, Tl, Pb, and Bi isotopes beyond N = 126. Method: Ions of interest were produced by fragmentation of a 238U beam, selected and identified via the GSI-FRS fragment separator. A stack of segmented silicon detectors (SIMBA) was used to measure ion implants and β decays. An array of 30 3 He tubes embedded in a polyethylene matrix (BELEN) was used to detect neutrons with high efficiency and selectivity. A self-triggered digital system is employed to acquire data and to enable time correlations. The latter were analyzed with an analytical model and results for the half-lives and neutron-branching ratios were derived by using the binned maximum-likelihood method. Results: Twenty new β-decay half-lives are reported for 204−206Au, 208–211Hg, 211–216Tl, 215–218Pb, and 218–220Bi, nine of them for the first time. Neutron emission probabilities are reported for 210,211Hg and 211–216Tl. Conclusions: The new β-decay half-lives are in good agreement with previous measurements on nuclei in this region. The measured neutron emission probabilities are comparable to or smaller than values predicted by global models such as relativistic Hartree Bogoliubov plus the relativistic quasi-particle random phase approximation (RHB + RQRPA).es
dc.description.sponsorshipSpanish Ministerio de Economía y Competitividad-FPA2011- 28770-C03-03, FPA2008-04972-C03-3, AIC-D2011-0705, FPA2011-24553, FPA2008-6419, FPA2010-17142, FPA2014-52823-C2-1-P, FPA2014- 52823-C2-2-P, and CPAN CSD-2007-00042 (Ingenio2010)es
dc.description.sponsorshipProgram Severo Ochoa-SEV-2014-0398es
dc.description.sponsorshipGerman Helmholtz Association (Young Investigators)-VH-NG 627 (LISA-Lifetime Spectroscopy for Astrophysics)es
dc.description.sponsorshipNuclear Astrophysics Virtual Institute-VH-VI-417es
dc.description.sponsorshipGerman Bundesministerium für Bildung und Forschung-06MT7178 / 05P12WOFNFes
dc.description.sponsorshipSpanish Nuclear Security Council (CSN)-Catedra Argoses
dc.description.sponsorshipUK Science & Technology Facilities Council (STFC)-ST/F012012/1es
dc.formatapplication/pdfes
dc.language.isoenges
dc.publisherAmerican Physical Societyes
dc.relation.ispartofPhysical Review C, 95, 064322.
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.titleβ-decay half-lives and β-delayed neutron emission probabilities for several isotopes of Au, Hg, Tl, Pb, and Bi, beyond N = 126es
dc.typeinfo:eu-repo/semantics/articlees
dc.type.versioninfo:eu-repo/semantics/publishedVersiones
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses
dc.contributor.affiliationUniversidad de Sevilla. Departamento de Física Atómica, Molecular y Nucleares
dc.relation.projectIDFPA2011- 28770-C03-03es
dc.relation.projectIDFPA2008-04972-C03-3es
dc.relation.projectIDAIC-D2011-0705es
dc.relation.projectIDFPA2011-24553es
dc.relation.projectIDFPA2008-6419es
dc.relation.projectIDFPA2010-17142es
dc.relation.projectIDFPA2014-52823-C2-1-Pes
dc.relation.projectIDFPA2014- 52823-C2-2-Pes
dc.relation.projectIDCPAN CSD-2007-00042 (Ingenio2010)es
dc.relation.projectIDSEV-2014-0398es
dc.relation.projectIDVH-NG 627 (LISA-Lifetime Spectroscopy for Astrophysics)es
dc.relation.projectIDVH-VI-417es
dc.relation.projectID06MT7178 / 05P12WOFNFes
dc.relation.projectIDST/F012012/1es
dc.relation.publisherversionhttps://journals.aps.org/prc/abstract/10.1103/PhysRevC.95.064322es
dc.identifier.doi10.1103/PhysRevC.95.064322es
idus.format.extent17 p.es
dc.journaltitlePhysical Review Ces
dc.publication.volumen95es
dc.publication.initialPage064322es

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