Spacetime Structure of an Evaporating Black Hole in Quantum Gravity
arXiv:hep-th/0602159 · doi:10.1103/PhysRevD.73.083005
Abstract
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.
23 pages, BibTeX, revtex4, 7 figures
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Cited by in corpus (23)
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