Final State of Hawking Radiation in Quantum General Relativity

Details Final State of Hawking Radiation in Quantum General Relativity Final State of Hawking Radiation in Quantum General Relativity

2005-03-18

arxiv.org/abs/hep-ph/0503189v4

Acta Phys.Polon. B37 (2006) 347-356

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, 2 figures; improved text and references; extended text

Scientific paper

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.

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