Black Hole Paradoxes
Abstract
We propose here that the wellknown black hole paradoxes such as the information loss and teleological nature of the event horizon are restricted to a particular idealized case, which is the homogeneous dust collapse model. In this case, the event horizon, which defines the boundary of the black hole, forms initially, and the singularity in the interior of the black hole at a later time. We show that, in contrast, gravitational collapse from physically more realistic initial conditions typically leads to the scenario in which the event horizon and spacetime singularity form simultaneously. We point out that this apparently simple modification can mitigate the causality and teleological paradoxes, and also lends support to two recently suggested solutions to the information paradox, namely, the `firewall' and `classical chaos' proposals.
 Publication:

arXiv eprints
 Pub Date:
 February 2014
 DOI:
 10.48550/arXiv.1402.3055
 arXiv:
 arXiv:1402.3055
 Bibcode:
 2014arXiv1402.3055J
 Keywords:

 High Energy Physics  Theory;
 Astrophysics  High Energy Astrophysical Phenomena;
 General Relativity and Quantum Cosmology
 EPrint:
 Revised version