dc.creator | Praena Rodríguez, Javier | es |
dc.creator | Sabaté Gilarte, Marta | es |
dc.creator | Porras, I. | es |
dc.creator | Quesada Molina, José Manuel | es |
dc.creator | Altstadt, Sebastian G. | es |
dc.creator | Andrzejewski, J. | es |
dc.creator | Audouin, Laurent | es |
dc.creator | Bécares, Vicente | es |
dc.creator | Cortés Giraldo, Miguel Antonio | es |
dc.creator | Guerrero Sánchez, Carlos | es |
dc.creator | Lerendegui Marco, Jorge | es |
dc.date.accessioned | 2019-06-11T10:58:23Z | |
dc.date.available | 2019-06-11T10:58:23Z | |
dc.date.issued | 2018-06-04 | |
dc.identifier.citation | Praena Rodríguez, J., Sabaté Gilarte, M., Porras, I., Quesada Molina, J.M., Altstadt, S.G., Andrzejewski, J.,...,Lerendegui Marco, J. (2018). Measurement and resonance analysis of the 33S(n,α) 30Si cross section at the CERN n_TOF facility in the energy region from 10 to 300 keV. Physical Review C, 97, 064603. | |
dc.identifier.issn | 2469-9985 | es |
dc.identifier.issn | 2469-9993 | es |
dc.identifier.uri | https://hdl.handle.net/11441/87343 | |
dc.description.abstract | The 33S(n,α)
30Si cross section has been measured at the neutron time-of-flight (n_TOF) facility at CERN in the
neutron energy range from 10 to 300 keV relative to the 10B(n,α)
7
Li cross-section standard. Both reactions were
measured simultaneously with a set of micromegas detectors. The flight path of 185 m has allowed us to obtain
the cross section with high-energy resolution. An accurate description of the resonances has been performed by
means of the multilevel multichannel R-matrix code SAMMY. The results show a significantly higher area of the
biggest resonance (13.45 keV) than the unique high-resolution (n,α) measurement. The new parametrization of
the 13.45-keV resonance is similar to that of the unique transmission measurement. This resonance is a matter of
research in neutron-capture therapy. The 33S(n,α)
30Si cross section has been studied in previous works because
of its role in the production of 36S in stars, which is currently overproduced in stellar models compared to
observations. | es |
dc.description.sponsorship | Ministerio de Economía y Competitividad de España-FPA2013- 47327-C2-1-R, FPA2016-77689-C2-1-R | es |
dc.description.sponsorship | Junta de Andalucía-P11- FQM-8229 | es |
dc.description.sponsorship | MINECO-FEDER, EU-FIS2015-69941-C2-1-P | es |
dc.description.sponsorship | Spanish Association Against Cancer (AECC)-PS16163811PORR) | es |
dc.format | application/pdf | es |
dc.language.iso | eng | es |
dc.publisher | American Physical Society | es |
dc.relation.ispartof | Physical Review C, 97, 064603. | |
dc.rights | Attribution-NonCommercial-NoDerivatives 4.0 Internacional | * |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0/ | * |
dc.title | Measurement and resonance analysis of the 33S(n,α) 30Si cross section at the CERN n_TOF facility in the energy region from 10 to 300 keV | 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 | FPA2013-47327-C2-1-R | es |
dc.relation.projectID | FPA2016-77689-C2-1-R | es |
dc.relation.projectID | P11- FQM-8229 | es |
dc.relation.projectID | FIS2015-69941-C2-1-P | es |
dc.relation.projectID | PS16163811PORR) | es |
dc.relation.publisherversion | https://journals.aps.org/prc/abstract/10.1103/PhysRevC.97.064603 | es |
dc.identifier.doi | 10.1103/PhysRevC.97.064603 | es |
idus.format.extent | 11 p. | es |
dc.journaltitle | Physical Review C | es |
dc.publication.volumen | 97 | es |
dc.publication.initialPage | 064603 | es |