Post-Newtonian Kinetic Theory
Abstract
A kinetic theory for relativistic gases in the presence of gravitational fields is developed in the second post-Newtonian approximation. The corresponding Boltzmann equation is determined from the evolution of the one-particle distribution function with respect to the proper time along the world line of the particle. From the knowledge of the equilibrium Maxwell-J\"uttner distribution function in the second post-Newtonian approximation the components of the particle four-flow and energy-momentum tensor are obtained. The Eulerian hydrodynamic equations for the mass density, mass-energy density and momentum density in the second post-Newtonian approximation are determined from the Boltzmann equation. It is shown that the combination of the hydrodynamic equations of mass and mass-energy densities leads to the hydrodynamic equation for the internal energy density in the first post-Newtonian approximation.
Cite
@article{arxiv.2010.11017,
title = {Post-Newtonian Kinetic Theory},
author = {Gilberto M. Kremer},
journal= {arXiv preprint arXiv:2010.11017},
year = {2021}
}
Comments
12 pages