Final State of Hawking Radiation in Quantum General Relativity
High Energy Physics - Phenomenology
2007-05-23 v4
Abstract
We use a new approach to the UV behavior of quantum general relativity, together with some recent results from the phenomenological asymptotic safety analysis of the theory, to discuss the final state of the Hawking radiation for an originally very massive black hole solution of Einstein's theory. We find that, after the black hole evaporates to the Planck mass size, its horizon is obviated by quantum loop effects, rendering the entire mass of the originally massive black hole accessible to our universe.
Cite
@article{arxiv.hep-ph/0503189,
title = {Final State of Hawking Radiation in Quantum General Relativity},
author = {B. F. L. Ward},
journal= {arXiv preprint arXiv:hep-ph/0503189},
year = {2007}
}
Comments
10 pages, 2 figures; improved text and references; extended text