Underground study of the 17O(p,alpha)18F reaction relevant for explosive hydrogen burning

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dc.contributor	Universitat Politècnica de Catalunya. Departament de Física i Enginyeria Nuclear
dc.contributor	Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica
dc.contributor.author	Di Leva, A
dc.contributor.author	Scott, D.A.
dc.contributor.author	Caciolli, A.
dc.contributor.author	Formicola, A.
dc.contributor.author	Strieder, F.
dc.contributor.author	Aliotta, M.
dc.contributor.author	Anders, M.
dc.contributor.author	Bemmerer, D.
dc.contributor.author	Broggini, C.
dc.contributor.author	Corvisiero, P.
dc.contributor.author	Elekes, Z.
dc.contributor.author	Fulop, Zs.
dc.contributor.author	Gervino, G.
dc.contributor.author	Guglielmetti, G.
dc.contributor.author	Gustavino, C.
dc.contributor.author	Gyurky, Gy.
dc.contributor.author	Imbriani, G.
dc.contributor.author	José Pont, Jordi
dc.contributor.author	Junker, M.
dc.date	2014-01
dc.identifier.citation	Di Leva, A. [et al.]. Underground study of the 17O(p,alpha)18F reaction relevant for explosive hydrogen burning. "Physical review C", Gener 2014, vol. 89, p. 015803/1-015803/15.
dc.identifier.citation	0556-2813
dc.identifier.uri	http://hdl.handle.net/2117/25055
dc.language.iso	eng
dc.rights	Attribution-NonCommercial-NoDerivs 3.0 Spain
dc.rights	info:eu-repo/semantics/openAccess
dc.rights	http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subject	Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject	Astrophysics
dc.subject	Astrofísica
dc.title	Underground study of the 17O(p,alpha)18F reaction relevant for explosive hydrogen burning
dc.type	info:eu-repo/semantics/publishedVersion
dc.type	info:eu-repo/semantics/article
dc.description.abstract	The 17O(p,γ )18F reaction affects the production of key isotopes (e.g., 18F and 18O) in the explosive hydrogen burning that powers classical novae. Under these explosive conditions, the reaction rate is dominated by contributions from a narrow resonance at Ec.m.= 183 keV and by the combined contributions of direct capture and low-energy tails of broad resonances. At present, the astrophysical reaction rate is not well constrained because of the lack of data in the energy region appropriate to classical novae.

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