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dc.contributor.authorBarbagallo, Massimo
dc.contributor.authorAberle, O.
dc.contributor.authorAlcayne, V.
dc.contributor.authorCalviño Tavares, Francisco
dc.contributor.authorCasanovas Hoste, Adrià
dc.contributor.authorCortés Rossell, Guillem Pere
dc.contributor.authorTarifeño Saldivia, Ariel Esteban
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física
dc.contributor.otherUniversitat Politècnica de Catalunya. Institut de Tècniques Energètiques
dc.date.accessioned2019-05-30T11:02:20Z
dc.date.available2019-05-30T11:02:20Z
dc.date.issued2019
dc.identifier.citationBarbagallo, M. [et al.]. (n,cp) reactions study at the n_TOF facilitty at CERN: results for the cosmological lithium problem. A: International Conference on Nuclear Reaction Mechanisms. "Proceedings of the 15th International Conference on Nuclear Reaction Mechanisms: Varenna, Italy: June 11-15, 2019". Meyrin: European Organization for Nuclear Research (CERN), 2019, p. 259-264.
dc.identifier.isbn9789290835202
dc.identifier.otherhttps://cds.cern.ch/record/2669963?ln=ca
dc.identifier.urihttp://hdl.handle.net/2117/133707
dc.description.abstractThe Big Bang Nucleosynthesis describes the production of the lightest nuclides from deuterium to Li at the early stages of the Universe. While a general good agreement is found for most of the isotopes involved in the synthesis, a serious discrepancy between the predicted abundance of 7Li and the related experimental observations is still present. This discrepancy has been referred since several decades as Cosmological Lithium Problem. In one last attempt to find nuclear solutions to this longstanding conundrum, the 7Be(n,alpha)4He and 7Be(n,p)7Li reactions, that affect predominantly the production of 7Li via the destruction of his parent nucleus 7Be, have been studied. Here we present the 7Be(n,a)4He and 7Be(n,p)7Li reaction crosssection measurements performed at the high-resolution n_TOF facility using the time-of-flight technique and high purity samples. The result of the experiments definitely rules out neutron induced reactions as a solution to the puzzle, thus indicating that explanations have to be sought out in other Physics scenarios.
dc.format.extent6 p.
dc.language.isoeng
dc.publisherEuropean Organization for Nuclear Research (CERN)
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Spain
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subjectÀrees temàtiques de la UPC::Física
dc.subjectÀrees temàtiques de la UPC::Energies::Energia nuclear
dc.subject.lcshNeutrons
dc.subject.lcshNucleosynthesis
dc.subject.lcshNuclear physics
dc.title(n,cp) reactions study at the n_TOF facilitty at CERN: results for the cosmological lithium problem
dc.typeConference lecture
dc.subject.lemacNeutrons
dc.subject.lemacNucleosíntesi
dc.subject.lemacFísica nuclear
dc.contributor.groupUniversitat Politècnica de Catalunya. ANT - Advanced Nuclear Technologies Research Group
dc.rights.accessOpen Access
local.identifier.drac24475642
dc.description.versionPostprint (published version)
dc.relation.projectidinfo:eu-repo/grantAgreement/MICINN//FPA2011-28770-C03-03/ES/DATOS NUCLEARES PARA FISICA NUCLEAR E INGENIERIA NUCLEAR/
local.citation.authorBarbagallo, M.; Aberle, O.; Alcayne, V.; Calviño, F.; Casanovas, A.; Cortes, G.; Tarifeño, A.
local.citation.contributorInternational Conference on Nuclear Reaction Mechanisms
local.citation.pubplaceMeyrin
local.citation.publicationNameProceedings of the 15th International Conference on Nuclear Reaction Mechanisms: Varenna, Italy: June 11-15, 2019
local.citation.startingPage259
local.citation.endingPage264


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