Relativistic equilibrium velocity distribution to improve standard solar models
Abstract
The current standard solar models can be improved by substituting the relativistic equilibrium velocity distribution for the Maxwellian velocity distribution. The relativistic equilibrium velocity distribution is close fitting to the Maxwellian velocity distribution in the lowvelocity part and substantially different from the Maxwellian velocity distribution in the highvelocity part, and vanishes at the velocity of light. If adopted in standard solar models, it will lower solar neutrino fluxes, change solar neutrino energy spectra but maintain solar sound speeds.
 Publication:

arXiv eprints
 Pub Date:
 December 2001
 arXiv:
 arXiv:condmat/0112146
 Bibcode:
 2001cond.mat.12146L
 Keywords:

 Condensed Matter  Statistical Mechanics;
 Astrophysics
 EPrint:
 5 pages with no figure