The hep reaction and the solar neutrino problem

Physics – Nuclear Physics – Nuclear Theory

Scientific paper

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10 pages, 1 figure, XVII European Few-Body plenary talk, Evora, September 2000

Scientific paper

10.1016/S0375-9474(01)00842-9

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.

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