Background: The cross section influences a variety of astrophysical scenarios, including big-bang and stellar nucleosynthesis. In recent years, conflicting results of direct measurements have been published, reporting contradictory low-energy trends. Purpose: To shed light on the contradiction between the existing data sets, the reaction was studied using the asymptotic normalization coefficient (ANC) technique which was up-to-now never used for this reaction. Methods: To derive the ANC, the transfer reaction, studied at the Department of Physics and Astronomy of the University of Catania and at the John.
Indirect determination of the astrophysical S factor for the 6Li(p,γ)7Be reaction using the asymptotic normalization coefficient method
Cherubini S.;D'Agata G.;Guardo G. L.;Indelicato I.;Lamia L.;Lattuada M.;Rapisarda G. G.;Romano S.;Sergi M. L.;Spitaleri C.;
2021-01-01
Abstract
Background: The cross section influences a variety of astrophysical scenarios, including big-bang and stellar nucleosynthesis. In recent years, conflicting results of direct measurements have been published, reporting contradictory low-energy trends. Purpose: To shed light on the contradiction between the existing data sets, the reaction was studied using the asymptotic normalization coefficient (ANC) technique which was up-to-now never used for this reaction. Methods: To derive the ANC, the transfer reaction, studied at the Department of Physics and Astronomy of the University of Catania and at the John.File in questo prodotto:
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