The hep reaction and the solar neutrino problem
arXiv:nucl-th/0009066 · doi:10.1016/S0375-9474(01)00842-9
Abstract
The results of a new calculation of the astrophysical S-factor for the proton weak capture on 3He are here reviewed. The methods used to obtain very accurate initial and final state wave functions and to construct the nuclear weak current operator are described. Finally the implications of these results for the Super-Kamiokande solar neutrino data are discussed.
arXiv comment10 pages, 1 figure, XVII European Few-Body plenary talk, Evora, September 2000