Solar reaction rates, non-extensivity and quantum uncertainty
Nuclear Theory
2009-11-07 v1 Astrophysics
Statistical Mechanics
High Energy Physics - Phenomenology
Abstract
We show that in weakly non-ideal plasmas, like the solar interior, both non-extensivity and quantum uncertainty (a' la Galitskii and Yakimets) should be taken into account to derive equilibrium ion distribution functions and to estimate nuclear reaction rates and solar neutrino fluxes.
Keywords
Cite
@article{arxiv.nucl-th/0102016,
title = {Solar reaction rates, non-extensivity and quantum uncertainty},
author = {A. Lavagno and P. Quarati},
journal= {arXiv preprint arXiv:nucl-th/0102016},
year = {2009}
}
Comments
8 pages, revtex