Heat conduction in relativistic systems: alternatives and perspectives
arXiv:1011.6628
Abstract
The non-equilibrium thermodynamics of relativistic systems have a rich phenomenology. The simplest phenomenon in the class of dissipative processes is that of heat. This letter presents a brief summary of the efforts made to tackle the problem of relativistic heat conduction. In particular, we focus on the multi-fluid approach to relativistic dissipation.
Invited article to the IoP Gravitational Physics Group newsletter, December 2010