Solar models with Solar Fusion III reaction rates show slight improvement in helioseismic agreement but lower predicted beryllium, boron, and CNO neutrino fluxes, with rate uncertainties insufficient to match observations.
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Investigating the impact of Solar Fusion III reaction rates on helioseismic constraints and solar neutrino fluxes
Solar models with Solar Fusion III reaction rates show slight improvement in helioseismic agreement but lower predicted beryllium, boron, and CNO neutrino fluxes, with rate uncertainties insufficient to match observations.