Spacetime Structure of an Evaporating Black Hole in Quantum Gravity

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dc.creatorBonanno, A.
dc.creatorReuter, M.
dc.date2006-02-16
dc.date.accessioned2026-07-07T10:45:58Z
dc.date.available2026-07-07T10:45:58Z
dc.descriptionThe 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.
dc.description23 pages, BibTeX, revtex4, 7 figures
dc.identifierhttps://arxiv.org/abs/hep-th/0602159
dc.identifierhttp://arxiv.org/abs/hep-th/0602159
dc.identifierPhys.Rev.D73:083005,2006
dc.identifierdoi:10.1103/PhysRevD.73.083005
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183082
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.titleSpacetime Structure of an Evaporating Black Hole in Quantum Gravity
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