Quantum corrections for (anti)-evaporating black hole
arXiv:hep-th/0007172 · doi:10.1103/PhysRevD.63.044020
Abstract
In this paper we analyse the quantum correction for Schwarzschild black hole in the Unruh state in the framework of spherically symmetric gravity (SSG) model. SSG is a two-dimensional dilaton model which is obtained by spherically symmetric reduction from the four-dimensional theory. We find the one-loop geometry of the (anti)-evaporating black hole and corrections for mass, entropy and apparent horizon.
16 pages, Latex, no figures
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Cited by in corpus (9)
- Dilaton Gravity in Two Dimensions
- Vacuum polarization in the Schwarzschild spacetime and dimensional reduction
- Anti-Evaporation of Bardeen de-Sitter Black Holes
- Vacuum polarization in two-dimensional static spacetimes and dimensional reduction
- Islands in Non-Minimal Dilaton Gravity: Exploring Effective Theories for Black Hole Evaporation
- Quantum corrections for BTZ black hole via 2D reduced model
- Unveiling horizons in quantum critical collapse
- Anti-Evaporation/Evaporation of -dimensional Reissner-Nordström Black Hole
- Quantum Critical Collapse Abhors a Naked Singularity