dc.creator | Žugec, P. | es |
dc.creator | Barbagallo, M. | es |
dc.creator | Colonna, Nicola | es |
dc.creator | Bosnar, D. | es |
dc.creator | Altstadt, Sebastian G. | es |
dc.creator | Andrzejewski, J. | es |
dc.creator | Cortés Giraldo, Miguel Antonio | es |
dc.creator | Praena Rodríguez, Javier | es |
dc.creator | Quesada Molina, José Manuel | es |
dc.creator | Wright, T. | es |
dc.date.accessioned | 2022-03-02T09:50:02Z | |
dc.date.available | 2022-03-02T09:50:02Z | |
dc.date.issued | 2013 | |
dc.identifier.citation | Žugec, P., Barbagallo, M., Colonna, N., Bosnar, D., Altstadt, S.G., Andrzejewski, J.,...,Wright, T. (2013). Experimental neutron capture data of 58 Ni from the CERN n_TOF facility. Physics Letters C, 89, 014605. | |
dc.identifier.issn | 2469-9985 | es |
dc.identifier.issn | 2469-9993 | es |
dc.identifier.uri | https://hdl.handle.net/11441/130302 | |
dc.description.abstract | The
58
Ni(
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
k
T
=
5
–
100
keV with uncertainties of less than 6%, showing fair agreement with recent experimental and evaluated data up to
k
T
= 50 keV. The MACS extracted in the present work at 30 keV is
34.2
±
0
.
6
stat
±
1
.
8
sys
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
58
Ni, with a negligible propagation on heavier isotopes. The reason is that, using both the old or the new MACS,
58
Ni is efficiently depleted by neutron captures. | es |
dc.description.sponsorship | National Science Foundation (NSF) de los Estados Unidos. PHY 02-16783 y PHY 09-22648 | es |
dc.description.sponsorship | Joint Institute for Nuclear Astrophysics (JINA) de los Estados Unidos. EU MIRG-CT-2006-046520 | es |
dc.format | application/pdf | es |
dc.format.extent | 9 p. | es |
dc.language.iso | eng | es |
dc.publisher | American Physical Society | es |
dc.relation.ispartof | Physics Letters C, 89, 014605. | |
dc.rights | Attribution-NonCommercial-NoDerivatives 4.0 Internacional | * |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0/ | * |
dc.title | Experimental neutron capture data of 58 Ni from the CERN n_TOF facility | 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 | PHY 02-16783 | es |
dc.relation.projectID | PHY 09-22648 | es |
dc.relation.projectID | EU MIRG-CT-2006-046520 | es |
dc.relation.publisherversion | https://doi.org/10.1103/PhysRevC.89.014605 | es |
dc.identifier.doi | 10.1103/PhysRevC.89.014605 | es |
dc.journaltitle | Physics Letters C | es |
dc.publication.volumen | 89 | es |
dc.publication.initialPage | 014605 | es |
dc.contributor.funder | National Science Foundation (NSF). United States | es |
dc.contributor.funder | Joint Institute for Nuclear Astrophysics (JINA) U.S. | es |