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arXiv · astro-ph/9603109

Generalized Statistics and Solar Neutrinos

G. Kaniadakis·A. Lavagno·P. Quarati
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Abstract

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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G. Kaniadakis, A. Lavagno, P. Quarati. 1996-03-20. Generalized Statistics and Solar Neutrinos. https://doi.org/10.1016/0370-2693(95)01535-3

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