dc.creator | Tagliente, G. | es |
dc.creator | Milazzo, Paolo | es |
dc.creator | Fujii, K. | es |
dc.creator | Abbondanno, U. | es |
dc.creator | Aerts, G. | es |
dc.creator | Álvarez, H. | es |
dc.creator | Wisshak, K. | es |
dc.creator | Capote, Roberto | es |
dc.creator | Lozano Leyva, Manuel Luis | es |
dc.creator | Quesada Molina, José Manuel | es |
dc.date.accessioned | 2017-04-19T11:45:41Z | |
dc.date.available | 2017-04-19T11:45:41Z | |
dc.date.issued | 2010 | |
dc.identifier.citation | Tagliente, G., Milazzo, P., Fujii, K., Abbondanno, U., Aerts, G., Álvarez, H.,...,Quesada Molina, J.M. (2010). The 92Zr(n,γ) reaction and its implications for stellar nucleosynthesis. Physical Review C - Nuclear Physics, 81 (5), 055801-1-055801-9. | |
dc.identifier.issn | 0556-2813 | es |
dc.identifier.uri | http://hdl.handle.net/11441/57899 | |
dc.description.abstract | Because the relatively small neutron capture cross sections of the zirconium isotopes are difficult to measure, the results of previous measurements are often not adequate for a number of problems in astrophysics and nuclear technology. Therefore, the 92Zr(n,γ) cross section has been remeasured at the CERN n-TOF facility, providing a set of improved parameters for 44 resonances in the neutron energy range up to 40 keV. With this information the cross-section uncertainties in the keV region could be reduced to 5% as required for s-process nucleosynthesis studies and technological applications. | es |
dc.description.sponsorship | EC FIKW-CT-2000-00107 | es |
dc.format | application/pdf | es |
dc.language.iso | eng | es |
dc.publisher | The American Physical Society | es |
dc.relation.ispartof | Physical Review C - Nuclear Physics, 81 (5), 055801-1-055801-9. | |
dc.rights | Attribution-NonCommercial-NoDerivatives 4.0 Internacional | * |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0/ | * |
dc.title | The 92Zr(n,γ) reaction and its implications for stellar nucleosynthesis | es |
dc.type | info:eu-repo/semantics/article | es |
dcterms.identifier | https://ror.org/03yxnpp24 | |
dc.type.version | info:eu-repo/semantics/publishedVersion | es |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | es |
dc.contributor.affiliation | Universidad de Sevilla. Departamento de Física Atómica, Molecular y Nuclear | es |
dc.relation.projectID | FIKW-CT-2000-00107 | es |
dc.relation.publisherversion | 10.1103/PhysRevC.81.055801 | es |
idus.format.extent | 9 p. | es |
dc.journaltitle | Physical Review C - Nuclear Physics | es |
dc.publication.volumen | 81 | es |
dc.publication.issue | 5 | es |
dc.publication.initialPage | 055801-1 | es |
dc.publication.endPage | 055801-9 | es |
dc.contributor.funder | European Commission (EC) | |