2006/02/16 by A. Bonanno, M. Reuter · 1 citation
Physics and Astronomy · #hep-th #astro-ph
paper · pdf · doi:10.1103/physrevd.73.083005
published as Phys.Rev.D73:083005,2006 · 23 pages, BibTeX, revtex4, 7 figures
arxiv created 2006/02/16 · arxiv updated 2009/12/01
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.