Heat flux in the presence of a gravitational field in a simple dilute fluid: an approach based in general relativistic kinetic theory to first order in the gradients

Abstract

Richard C. Tolman analyzed the relation between a temperature gradient and a gravitational field in an equilibrium situation. In 2012, Tolman\textquoteright s law was generalized to a non-equilibrium situation for a simple dilute relativistic fluid. The result in that scenario, obtained by introducing the gravitational force through the molecular acceleration, couples the heat flux with the metric coefficients and the gradients of the state variables. In the present paper it is shown, by \textquotedblleft suppressing\textquotedblright{} the molecular acceleration in Boltzmann\textquoteright s equation, that a gravitational field drives a heat flux. This procedure corresponds to the description of particle motion through geodesics, in which a Newtonian limit to the Schwarzschild metric is assumed. The effect vanishes in the non-relativistic regime, as evidenced by the direct evaluation of the corresponding limit.

11 pages, no figures

References in corpus (6)

• Thermal equilibrium and statistical thermometers in special relativity
• Relativistic gas in a Schwarzschild metric
• Heat conduction in relativistic neutral gases revisited
• Tolman's law in linear irreversible thermodynamics: a kinetic theory approach
• The Boltzmann equation in special and general relativity
• Benedicks effect in a relativistic simple fluid