Causal temperature profiles in horizon-free collapse
arXiv:gr-qc/0510013
Abstract
We investigate the causal temperature profiles in a recent model of a radiating star undergoing dissipative gravitational collapse without the formation of an horizon. It is shown that this simple exact model provides a physically reasonable behaviour for the temperature profile within the framework of extended irreversible thermodynamics.
8 pages, 2 figures, submitted to Mod. Phys. Lett. A