The Stress-Energy Tensor in Soluble Models of Spherically Symmetric Charged Black Hole Evaporation
arXiv:hep-th/0107137 · doi:10.1103/PhysRevD.65.024018
Abstract
We study the decay of a near-extremal black hole in AdS, related to the near-horizon region of 3+1-dimensional Reissner-Nordström spacetime, following Fabbri, Navarro, and Navarro-Salas. Back-reaction is included in a semiclassical approximation. Calculations of the stress-energy tensor of matter coupled to the physical spacetime for an affine null observer demonstrate that the black hole evaporation proceeds smoothly and the near-extremal black hole evolves back to an extremal ground state, until this approximation breaks down.
19 pages, 14 figures
Cited by in corpus (5)
- The causal structure of dynamical charged black holes
- Quantum Gravity Effects in Black Holes at the LHC
- Near-Extremal Black Hole Evaporation in Asymptotically Flat Spacetime
- Low-energy scattering of extremal black holes by neutral matter
- Late-time correlators in semiclassical particle-black hole scattering