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On the solar neutrino problem in the relativistic field theory model of the deuteron

H. Oberhummer·A. N. Ivanov·N. I. Troitskaya·M. Faber
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Abstract

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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H. Oberhummer, A. N. Ivanov, N. I. Troitskaya, M. Faber. 1997-05-16. On the solar neutrino problem in the relativistic field theory model of the deuteron. https://arxiv.org/abs/astro-ph/9705119

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