Solar neutrino based redetermination of the ~7Be(p,γ)~8B S-factor

摘要

The present proceeding is an abbreviated version of M. P. Takacs et al., Nuclear Physics A 970 (2018) 78-85[1], exploring the possibility to constrain the astrophysical S-factor of the ~7Be(p,γ)~8B reaction at the energies of the solar Gamow peak based on the most recent ~7Be and ~8B solar neutrino flux measurements, and the Standard Solar Model.