A model for ultrarelativistic spherically symmetric Pre-Hawking radiating gravitational collapse
General Relativity and Quantum Cosmology
2014-06-24 v2
Abstract
In this paper we present a simple but non-simplistic model of gravitational collapse with thermal emission of pre-Hawking radiation. We apply Einstein equations to a time-dependant spherically symmetric metric and an ultrarelativistic stress-energy tensor. In our model, particles either radially approach the center of the star as collapsing matter, or radially flee from it.
Keywords
Cite
@article{arxiv.1205.0283,
title = {A model for ultrarelativistic spherically symmetric Pre-Hawking radiating gravitational collapse},
author = {Miquel Pinyol Ribas},
journal= {arXiv preprint arXiv:1205.0283},
year = {2014}
}
Comments
This paper has been withdrawn by the author due to an inadequate treatment of the stress-momentum tensor and a not well-behaved radiation law. The right development may be found at arXiv: gr-qc\1406.4189