Causal temperature profiles in horizon-free collapse

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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

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/95406

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/0510013
 http://arxiv.org/abs/gr-qc/0510013

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arXiv