Implications of Sm-151(n,gamma) cross section at n_TOF

Marrone, S.; Abbondanno, U.; Aerts, G.; Capote del Villar, Ramón; Lozano Leyva, Manuel Luis; Quesada Molina, José Manuel; Wisshak, K.

doi:10.1063/1.2200996

Ponencia

dc.creator	Marrone, S.	es
dc.creator	Abbondanno, U.	es
dc.creator	Aerts, G.	es
dc.creator	Capote del Villar, Ramón	es
dc.creator	Lozano Leyva, Manuel Luis	es
dc.creator	Quesada Molina, José Manuel	es
dc.creator	Wisshak, K.	es
dc.date.accessioned	2020-09-18T11:30:38Z
dc.date.available	2020-09-18T11:30:38Z
dc.date.issued	2006
dc.identifier.citation	Marrone, S., Abbondanno, U., Aerts, G., Capote del Villar, R., Lozano Leyva, M.L., Quesada Molina, J.M. y Wisshak, K. (2006). Implications of Sm-151(n,gamma) cross section at n_TOF. En International Conference on Frontiers in Nuclear Structure, Astrophysics and Reactions (FINUSTAR) (502-504), Isla de Kos, (Grecia): American Institute of Physics.
dc.identifier.isbn	0-7354-0323-6	es
dc.identifier.issn	0094-243X (impreso)	es
dc.identifier.issn	1551-7616 (electrónico)	es
dc.identifier.uri	https://hdl.handle.net/11441/101301
dc.description.abstract	The accurate knowledge of the 151Sm(n,γ) cross section has important implications for the nuclear technologies as well as for fundamental studies. Due to its radioactivity, the only experimental data available on 151Sm were derived from a transmission measurement [1]. Nowadays thanks to the innovative features of neutron time-of-flight facility (n_TOF), it was possible to measure 151Sm(n,γ) cross section in a wide energy range and with good accuracy [2]. We present, here, the main experimental results together with the implications concerning the nuclear astrophysical part.	es
dc.description.sponsorship	European Commission (EC) FIKW-CT-2000-00107	es
dc.format	application/pdf	es
dc.format.extent	5 p.	es
dc.language.iso	eng	es
dc.publisher	American Institute of Physics	es
dc.relation.ispartof	International Conference on Frontiers in Nuclear Structure, Astrophysics and Reactions (FINUSTAR) (2006), pp. 502-504.
dc.rights	Attribution-NonCommercial-NoDerivatives 4.0 Internacional	*
dc.rights.uri	http://creativecommons.org/licenses/by-nc-nd/4.0/	*
dc.subject	151 Sm	es
dc.subject	Neutron capture	es
dc.subject	Level density	es
dc.subject	Neutron strength function	es
dc.subject	Nucleosynthesis	es
dc.subject	S process	es
dc.title	Implications of Sm-151(n,gamma) cross section at n_TOF	es
dc.type	info:eu-repo/semantics/conferenceObject	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	https://doi.org/10.1063/1.2200996	es
dc.identifier.doi	10.1063/1.2200996	es
dc.publication.initialPage	502	es
dc.publication.endPage	504	es
dc.eventtitle	International Conference on Frontiers in Nuclear Structure, Astrophysics and Reactions (FINUSTAR)	es
dc.eventinstitution	Isla de Kos, (Grecia)	es
dc.contributor.funder	European Commission (EC)	es

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