Generalized Statistics and Solar Neutrinos

Details Generalized Statistics and Solar Neutrinos Generalized Statistics and Solar Neutrinos

1996-03-20

arxiv.org/abs/astro-ph/9603109v1

Phys.Lett. B369 (1996) 308-312

Astronomy and Astrophysics

Astrophysics

4 pages, RevTex

Scientific paper

10.1016/0370-2693(95)01535-3

The generalized Tsallis statistics produces a distribution function appropriate to describe the interior solar plasma, thought as a stellar polytrope, showing a tail depleted respect to the Maxwell-Boltzmann distribution and reduces to zero at energies greater than about $20 \, k_{_B} T$. The Tsallis statistics can theoretically support the distribution suggested in the past by Clayton and collaborators, which shows also a depleted tail, to explain the solar neutrino counting rate.

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