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How Uncertain Are Solar Neutrino Predictions?

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arxiv astro-ph/9805135 v2 pith:2KWC3H53 submitted 1998-05-12 astro-ph hep-phnucl-th

classification astro-phhep-phnucl-th
keywords neutrinosolarfluxescalculatedeffectsestimatedfusionidentified
verification ladder T0 review T1 audit T2 compute T3 formal

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Solar neutrino fluxes and sound speeds are calculated using a systematic reevaluation of nuclear fusion rates. The largest uncertainties are identified and their effects on the solar neutrino fluxes are estimated.

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Cited by 1 Pith paper

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  1. Constraints on Fermionic Dark Matter Absorption from Radiochemical Solar-Neutrino Measurements

    hep-ph 2026-02 unverdicted novelty 5.0 of 10

    Reanalysis of solar neutrino capture rates yields 90% upper limits of 0.39-0.59 SNU on fermionic dark matter induced contributions, mapping to y bounds of 4.9-7.1 x 10^{-49} cm^2 at 1 MeV dark matter mass.

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