Affordable Access

deepdyve-link deepdyve-link
Publisher Website

Generalized statistics and solar neutrinos

Authors
  • Kaniadakis, G.
  • Lavagno, A.
  • Quarati, P.
Publication Date
Mar 01, 1996
Identifiers
DOI: 10.1016/0370-2693(95)01535-3
OAI: oai:inspirehep.net:416960
Source
INSPIRE-HEP
Keywords
License
Unknown
External links

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 with 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.

Report this publication

Statistics

Seen <100 times