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Spacetime Structure of an Evaporating Black Hole in Quantum Gravity

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arxiv hep-th/0602159 v1 pith:6XEJDVAP submitted 2006-02-16 hep-th astro-ph

A.Bonanno , M.Reuter This is my paper · ORCID
classification hep-thastro-ph
keywords quantumblackevaporationgravityholehorizonprocessspacetime
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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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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Effective geometrodynamics for renormalization-group improved black-hole spacetimes in spherical symmetry

    gr-qc 2026-01 unverdicted novelty 7.0 of 10

    RG-improved black hole spacetimes with scale-dependent gravitational coupling are derived as vacuum solutions to 2D Horndeski master field equations, embedding prior works and exposing implementation discrepancies.

  2. Starobinsky-inflation in asymptotically safe shift-symmetric scalar-tensor theory

    gr-qc 2026-06 unverdicted novelty 6.0 of 10

    Starobinsky inflation rules out two of three non-Gaussian fixed points in asymptotically safe scalar-tensor theories, identifying viable RG trajectories from the remaining fixed point.

  3. Improved unimodular black holes with self-consistent renormalization scale identification

    gr-qc 2026-06 unverdicted novelty 5.0 of 10

    Renormalization group improved unimodular black holes with self-consistent radial scale identification yield non-singular metrics and associated mass gaps.

  4. Consistency in the Quantum-Improved Charged Black Holes

    gr-qc 2026-05 unverdicted novelty 5.0 of 10

    Thermodynamic consistency for quantum-improved Reissner-Nordström black holes permits arbitrary radial dependence in both Newton and electromagnetic couplings, while equation-action consistency requires an extra quant...

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