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dc.contributor.authorZugec, P.
dc.contributor.authorBarbagallo, M.
dc.contributor.authorColonna, Nicola
dc.contributor.authorBosnar, D.
dc.contributor.authorAltstadt, S.
dc.contributor.authorAndrzejewski, J.
dc.contributor.authorAudouin, L.
dc.contributor.authorCalviño Tavares, Francisco
dc.contributor.authorCortés Rossell, Guillem Pere
dc.contributor.authorGómez Hornillos, María Belén
dc.contributor.authorRiego Pérez, Albert
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física i Enginyeria Nuclear
dc.date.accessioned2014-01-29T10:19:58Z
dc.date.created2014-01-09
dc.date.issued2014-01-09
dc.identifier.citationZugec, P. [et al.]. Experimental neutron capture data of 58Ni from the CERN n_TOF facility. "Physical review C", 09 Gener 2014, vol. 89, núm. 1, p. 014605-1-014605-9.
dc.identifier.issn0556-2813
dc.identifier.urihttp://hdl.handle.net/2117/21392
dc.description.abstractThe 58Ni(n,γ ) cross section has been measured at the neutron time of flight facility n_TOF at CERN, in the energy range from 27 meV up to 400 keV. In total, 51 resonances have been analyzed up to 122 keV. Maxwellian averaged cross sections (MACS) have been calculated for stellar temperatures of kT = 5–100 keV with uncertainties of less than 6%, showing fair agreement with recent experimental and evaluated data up to kT = 50 keV. The MACS extracted in the present work at 30 keV is 34.2 ± 0.6stat ± 1.8sys mb, in agreement with latest results and evaluations, but 12% lower relative to the recent KADoNIS compilation of astrophysical cross sections.When included in models of the s-process nucleosynthesis in massive stars, this change results in a 60% increase of the abundance of 58Ni, with a negligible propagation on heavier isotopes. The reason is that, using both the old or the new MACS, 58Ni is efficiently depleted by neutron captures.
dc.language.isoeng
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::Electromagnetisme
dc.subject.lcshNeutrons Capture
dc.subject.otherCross section
dc.subject.otherNeutron
dc.subject.otherTime of flight
dc.subject.othernTOF
dc.titleExperimental neutron capture data of 58Ni from the CERN n_TOF facility
dc.typeArticle
dc.subject.lemacNeutrons
dc.contributor.groupUniversitat Politècnica de Catalunya. GREENER - Grup de recerca d'estudis energètics i de les radiacions
dc.identifier.doi10.1103/PhysRevC.89.014605
dc.rights.accessRestricted access - publisher's policy
drac.iddocument12966952
dc.description.versionPostprint (published version)
dc.date.lift10000-01-01
upcommons.citation.authorZugec, P.; Barbagallo, M.; Colonna, N.; Bosnar, D.; Altstadt , S.; Andrzejewski, J.; Audouin, L.; Calviño, F.; Cortes, G.; Gómez-Hornillos, M.B.; Riego, A.
upcommons.citation.publishedtrue
upcommons.citation.publicationNamePhysical review C
upcommons.citation.volume89
upcommons.citation.number1
upcommons.citation.startingPage014605-1
upcommons.citation.endingPage014605-9


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