Solar reaction rates, non-extensivity and quantum uncertainty
arXiv:nucl-th/0102016 · doi:10.1016/S0370-2693(00)01370-8
Abstract
We show that in weakly non-ideal plasmas, like the solar interior, both non-extensivity and quantum uncertainty (a' la Galitskii and Yakimets) should be taken into account to derive equilibrium ion distribution functions and to estimate nuclear reaction rates and solar neutrino fluxes.
8 pages, revtex
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