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dc.contributor.authorDi Leva, A
dc.contributor.authorScott, D.A.
dc.contributor.authorCaciolli, A.
dc.contributor.authorFormicola, A.
dc.contributor.authorStrieder, F.
dc.contributor.authorAliotta, M.
dc.contributor.authorAnders, M.
dc.contributor.authorBemmerer, D.
dc.contributor.authorBroggini, C.
dc.contributor.authorCorvisiero, P.
dc.contributor.authorElekes, Z.
dc.contributor.authorFulop, Zs.
dc.contributor.authorGervino, G.
dc.contributor.authorGuglielmetti, G.
dc.contributor.authorGustavino, C.
dc.contributor.authorGyurky, Gy.
dc.contributor.authorImbriani, G.
dc.contributor.authorJosé Pont, Jordi
dc.contributor.authorJunker, M.
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física i Enginyeria Nuclear
dc.identifier.citationDi 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.description.abstractThe 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.
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Spain
dc.subjectÀrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.titleUnderground study of the 17O(p,alpha)18F reaction relevant for explosive hydrogen burning
dc.contributor.groupUniversitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica
dc.rights.accessOpen Access
dc.description.versionPostprint (published version)
local.citation.authorDi Leva, A.; Scott, D.; Caciolli, A.; Formicola, A.; Strieder, F.; Aliotta, M.; Anders, M.; Bemmerer, D.; Broggini, C.; Corvisiero, P.; Elekes, Z.; Fulop, Z.; Gervino, G.; Guglielmetti, G.; Gustavino, C.; Gyurky, G.; Imbriani, G.; Jose, J.; Junker, M.; et al.,
local.citation.publicationNamePhysical review C

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