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dc.contributor.authorDomingo-Pardo, C
dc.contributor.authorAgramunt Ros, Jorge
dc.contributor.authorAlgora, A.
dc.contributor.authorCalviño Tavares, Francisco
dc.contributor.authorCortés Rossell, Guillem Pere
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física
dc.date.accessioned2016-11-03T12:35:12Z
dc.date.available2016-11-03T12:35:12Z
dc.date.issued2013
dc.identifier.citationDomingo-Pardo, C., Agramunt, J., Algora, A., Calviño, F., Cortes, G. Approaching the precursor nuclei of the third r-process peak with RIBs. A: Nuclear Physics in Astrophysics. "Journal of Physics: Conference Series, vol. 665, no. 1, January 5, 2016". Lisboa: Institute of Physics (IOP), 2013, p. 1-8.
dc.identifier.urihttp://hdl.handle.net/2117/91416
dc.description.abstractThe rapid neutron nucleosynthesis process involves an enormous amount of very exotic neutron-rich nuclei, which represent a theoretical and experimental challenge. Two of the main decay properties that affect the final abundance distribution the most are half-lives and neutron branching ratios. Using fragmentation of a primary 238U beam at GSI we were able to measure such properties for several neutron-rich nuclei from 208Hg to 218Pb. This contribution provides a short update on the status of the data analysis of this experiment, together with a compilation of the latest results published in this mass region, both experimental and theoretical. The impact of the uncertainties connected with the eta-decay rates and with beta-delayed neutron emission is illustrated on the basis of r-process network calculations. In order to obtain a reasonable reproduction of the third r-process peak, it is expected that both half-lives and neutron branching ratios are substantially smaller, than those based on FRDM+QRPA, commonly used in r-process model calculations. Further measurements around N 126 are required for a reliable modelling of the underlying nuclear structure, and for performing more realistic r-process abundance calculations.
dc.format.extent8 p.
dc.language.isoeng
dc.publisherInstitute of Physics (IOP)
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subjectÀrees temàtiques de la UPC::Energies::Energia nuclear
dc.subject.lcshNuclear energy
dc.subject.lcshNeutrons
dc.subject.otherNucleosynthesis
dc.subject.otherNeutron
dc.titleApproaching the precursor nuclei of the third r-process peak with RIBs
dc.typeConference lecture
dc.subject.lemacEnergia nuclear
dc.subject.lemacNeutrons
dc.contributor.groupUniversitat Politècnica de Catalunya. ANT - Advanced Nuclear Technologies Research Group
dc.identifier.doi10.1088/1742-6596/665/1/012045
dc.relation.publisherversionhttp://iopscience.iop.org/article/10.1088/1742-6596/665/1/012045/meta;jsessionid=9D05BBCBC424AD1511D66B514184F623.c3.iopscience.cld.iop.org
dc.rights.accessOpen Access
local.identifier.drac19070809
dc.description.versionPostprint (published version)
dc.relation.projectidinfo:eu-repo/grantAgreement/MICINN/6PN/FPA2011-28770-C03-03
local.citation.authorDomingo-Pardo, C.; Agramunt, J.; Algora, A.; Calviño, F.; Cortes, G.
local.citation.contributorNuclear Physics in Astrophysics
local.citation.pubplaceLisboa
local.citation.publicationNameJournal of Physics: Conference Series, vol. 665, no. 1, January 5, 2016
local.citation.startingPage1
local.citation.endingPage8


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