Spacetime Structure of an Evaporating Black Hole in Quantum Gravity

Details Spacetime Structure of an Evaporating Black Hole in Quantum Gravity Spacetime Structure of an Evaporating Black Hole in Quantum Gravity

2006-02-16

arxiv.org/abs/hep-th/0602159v1

Phys.Rev.D73:083005,2006

Physics

High Energy Physics

High Energy Physics - Theory

23 pages, BibTeX, revtex4, 7 figures

Scientific paper

10.1103/PhysRevD.73.083005

The impact of the leading quantum gravity effects on the dynamics of the Hawking evaporation process of a black hole is investigated. Its spacetime structure is described by a renormalization group improved Vaidya metric. Its event horizon, apparent horizon, and timelike limit surface are obtained taking the scale dependence of Newton's constant into account. The emergence of a quantum ergosphere is discussed. The final state of the evaporation process is a cold, Planck size remnant.

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