Anderson-Witting transport coefficients for flows in general relativity
High Energy Astrophysical Phenomena
2017-09-26 v1 General Relativity and Quantum Cosmology
High Energy Physics - Theory
Abstract
The transport coefficients induced by the Anderson-Witting approximation of the collision term in the relativistic Boltzmann equation are derived for close to equilibrium flows in general relativity. Using the tetrad formalism, it is shown that the expression for these coefficients is the same as that obtained on flat space-time, in agreement with the generalized equivalence principle.
Cite
@article{arxiv.1608.01400,
title = {Anderson-Witting transport coefficients for flows in general relativity},
author = {Victor E. Ambrus},
journal= {arXiv preprint arXiv:1608.01400},
year = {2017}
}
Comments
6 pages, 1 figure, proceedings of TIM 15-16 conference (26-28 May 2016, Timisoara, Romania)