Key points are not available for this paper at this time.
Solar model predictions of ^8B and p-p neutrinos agree with the experimentally determined fluxes (including oscillations): (pp) ₌₄₀ₒₔₑ₄₃= (1. 0200. 020. 01) (pp) ₓ₇₄₎ₑₘ and (^8B) ₌₄₀ₒₔₑ₄₃= (0. 880. 040. 23) (^8B) ₓ₇₄₎ₑₘ, 1 experimental and theoretical uncertainties, respectively. We use improved input data for nuclear fusion reactions, the equation of state, and the chemical composition of the Sun. The solar composition is the dominant uncertainty in calculating the ^8B and CNO neutrino fluxes; the cross section for the ^3He (^4He, ) ^7Be reaction is the most important uncertainty for the calculated ^7Be neutrino flux.
Bahcall et al. (Thu,) studied this question.