Nonextensive statistics in stellar plasma and solar neutrinos

Details Nonextensive statistics in stellar plasma and solar neutrinos Nonextensive statistics in stellar plasma and solar neutrinos

1999-12-27

arxiv.org/abs/nucl-th/9912064v1

Nucl.Phys.Proc.Suppl. 87 (2000) 209-211

Physics

Nuclear Physics

Nuclear Theory

4 pages. Proc. of TAUP99, Sept. 6-10 1999, Paris. To appear in Nucl. Phys. B, Proc. Suppl

Scientific paper

10.1016/S0920-5632(00)00669-1

Nonextensive and quantum uncertainty effects (related to the quasiparticles composing the stellar core) have strong influence on the nuclear rates and, of course, affect solar neutrino fluxes. Both effects do coexist and are due to the frequent collisions among the ions. The weakly nonextensive nature of the solar core is confirmed. The range of predictions for the neutrino fluxes is enlarged and the solar neutrino problem becomes less dramatic.

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