On the solar neutrino problem in the relativistic field theory model of the deuteron
Oberhummer, H. · Ivanov, A. N. · Troitskaya, N. I. · Faber, M.
Original · EN
The relativistic field theory model of the deuteron suggested by us previously is applied to the calculation of the reaction rate of the low-energy two-proton fusion p + p -> D + e+ + nu. The theoretical prediction of the reaction rate obtained is 2.9 times larger than given by the potential approach. This leads to a strong suppression of the high energy solar neutrino fluxes.
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