Abstract
We investigate the causal temperature profiles in a recent model of a radiating star undergoing dissipative gravitational collapse without the formation of a horizon. It is shown that this simple exact model provides physically reasonable behaviour for the temperature profile within the framework of extended irreversible thermodynamics.
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Naidu, N.F., Govender, M. Causal temperature profiles in horizon-free collapse. J Astrophys Astron 28, 167–174 (2007). https://doi.org/10.1007/s12036-007-0014-6
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DOI: https://doi.org/10.1007/s12036-007-0014-6