Toward a reassessment of the 19F(p, α0)16O reaction rate at astrophysical temperatures

Toward a reassessment of the 19F(p, α0)16O reaction rate at astrophysical temperatures

The 19F(p, α0)16O reaction at low energies plays an important role in fundamental physics. In particular in nuclear astrophysics it represents, together with the 19F(p, γ)20Ne reaction, the crossing point between the CNO and the NeNa cycles in stars. Further, in hydrogen-rich stellar environments, i...

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Bibliographic Details
Main Authors: I. Lombardo, D. Dell'Aquila, A. Di Leva, I. Indelicato, M. La Cognata, M. La Commara, A. Ordine, V. Rigato, M. Romoli, E. Rosato, G. Spadaccini, C. Spitaleri, A. Tumino, M. Vigilante
Format: Article
Language:English
Published: Elsevier 2015-09-01
Series:Physics Letters B
Subjects:
Nuclear reactions
Fluorine nucleosynthesis
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269315005031

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