Astrophysical S-factors for the p+16O and n+16O captures from the analysis of 16O(d,n)17F and 16O(d,p)17O transfer reactions

Assunção, M.; Lichtenthäler, R.; Guimarães, V.; Lépine-Szily, A.; Moro Muñoz, Antonio Matías

doi:10.1063/1.2710573

Ponencia

dc.creator	Assunção, M.	es
dc.creator	Lichtenthäler, R.	es
dc.creator	Guimarães, V.	es
dc.creator	Lépine-Szily, A.	es
dc.creator	Moro Muñoz, Antonio Matías	es
dc.date.accessioned	2021-05-04T10:32:56Z
dc.date.available	2021-05-04T10:32:56Z
dc.date.issued	2007
dc.identifier.citation	Assunção, M., Lichtenthäler, R., Guimarães, V., Lépine-Szily, A. y Moro Muñoz, A.M. (2007). Astrophysical S-factors for the p+16O and n+16O captures from the analysis of 16O(d,n)17F and 16O(d,p)17O transfer reactions. En 6th Latin American Symposium on Nuclear Physics and Applications (158-162), Iguazú, Argentina: American Institute of Physics.
dc.identifier.issn	0094-243X (impreso)	es
dc.identifier.issn	1551-7616 (electrónico)	es
dc.identifier.uri	https://hdl.handle.net/11441/108423
dc.description.abstract	Coupled reaction channels calculations were performed for the 16O(d,n)17F and 16O(d,p)17O transfer reactions for the ground and first excited states at several energies from Elab=2.29 MeV up to 3.27 MeV. A strong polarization effect between the entrance channel and the transfer, 16O(d,n)17F (1/2+,0.495) and 16O(d,n)17O (1/2+,0.87), channels was observed. This polarization effect had to be taken into account to all orders for obtaining realistic spectroscopic factors from these reactions. The 16O(p,γ) 17F and 16O(n,γ) 17O direct captures were calculated using the Asymptotic Normalization Coefficients (ANC) values from these transfer reactions analysis. The astrophysical S-factors were compared to measurements. The Maxwellian-averaged neutron capture cross section at kT=30 keV was 22(3)μbarn.	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	6th Latin American Symposium on Nuclear Physics and Applications (2007), pp. 158-162.
dc.rights	Attribution-NonCommercial-NoDerivatives 4.0 Internacional	*
dc.rights.uri	http://creativecommons.org/licenses/by-nc-nd/4.0/	*
dc.subject	Direct reaction	es
dc.subject	Coupled-channel	es
dc.subject	Distorted-wave model	es
dc.subject	Capture cross section	es
dc.subject	Astrophysical S-factor	es
dc.title	Astrophysical S-factors for the p+16O and n+16O captures from the analysis of 16O(d,n)17F and 16O(d,p)17O transfer reactions	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.publisherversion	http://dx.doi.org/10.1063/1.2710573	es
dc.identifier.doi	10.1063/1.2710573	es
dc.publication.initialPage	158	es
dc.publication.endPage	162	es
dc.eventtitle	6th Latin American Symposium on Nuclear Physics and Applications	es
dc.eventinstitution	Iguazú, Argentina	es

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