Spacetime structure of an evaporating black hole in quantum gravity
By Alfio M. Bonanno, Martin Reuter. 2006
228 citations recorded by the source corpus.
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 by 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.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/055337a3accd48d3a3db50599ada54fed7b418de
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- M. Niedermaier
- Martin Reuter
- Gianluca Calcagni
- J. W. Moffat
- A. Eichhorn
- J. Brownstein
- Frank Saueressig
- Jan M. Pawlowski
In Nuclear and High Energy Physics
- M. Niedermaier
- Martin Reuter
- Gianluca Calcagni
- A. Eichhorn
- J. W. Moffat
- J. Brownstein
- Jan M. Pawlowski
- Frank Saueressig
In Statistical and Nonlinear Physics
- M. Niedermaier
- Martin Reuter
- Gianluca Calcagni
- A. Eichhorn
- Jan M. Pawlowski
- Frank Saueressig
- E. Manrique
- Steven Carlip
Citations in the corpus
- The Asymptotic Safety Scenario in Quantum Gravity (2006, methodology): “In the literature similar arguments have been used for the “renormalization group improvement” of cosmological [37, 38, 183, 28] and black hole spacetimes [36, 35, 40] on the basis of the effective average action (see also [189, 191, 190] for a discussion of different improvement schemes).”