arXiv · cond-mat/0112146
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 low-velocity part and substantially different from the Maxwellian velocity distribution in the high-velocity 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.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Jian-Miin Liu. 2001-12-09. Relativistic equilibrium velocity distribution to improve standard solar models. https://arxiv.org/abs/cond-mat/0112146
Cite the original work for its findings. Save a collection to share your selection of sources.