Anderson-Witting transport coefficients for flows in general relativity
classification
🌌 astro-ph.HE
gr-qchep-th
keywords
coefficientsanderson-wittingflowsgeneralrelativitytransportagreementapproximation
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.