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The Solar Core and Solar Neutrinos

Dallas C. Kennedy

astro-pharXiv:astro-ph/0005412

Abstract

The long-standing deficit of measured versus predicted solar neutrino fluxes is re-examined in light of possible astrophysical solutions. In the last decade, solar neutrino flux and helioseismic measurements have greatly strengthened the case for non-astrophysical solutions. But some model- independent tests remain open.

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