Velocity distribution of high-energy particles and the solar neutrino problem
Astrophysics
2007-05-23 v1
Abstract
High energy infers high velocity and high velocity is a concept of special relativity. The Maxwellian velocity distribution is corrected to be consistent with special relativity. The corrected distribution reduces to the Maxwellian distribution for small velocities, contains a relatively depleted high-energy tail and vanishes at the velocity of light. This corrected distribution will lower solar neutrino fluxes and change solar neutrino energy spectra but keep solar sound speeds.
Keywords
Cite
@article{arxiv.astro-ph/0108304,
title = {Velocity distribution of high-energy particles and the solar neutrino problem},
author = {Jian-Miin Liu},
journal= {arXiv preprint arXiv:astro-ph/0108304},
year = {2007}
}
Comments
5 pages, no figures