The Stress-Energy Tensor in Soluble Models of Spherically Symmetric Charged Black Hole Evaporation

Details The Stress-Energy Tensor in Soluble Models of Spherically Symmetric Charged Black Hole Evaporation The Stress-Energy Tensor in Soluble Models of Spherically Symmetric Charged Black Hole Evaporation

2001-07-17

arxiv.org/abs/hep-th/0107137v1

Phys.Rev. D65 (2002) 024018

Physics

High Energy Physics

High Energy Physics - Theory

19 pages, 14 figures

Scientific paper

10.1103/PhysRevD.65.024018

We study the decay of a near-extremal black hole in AdS$_2$, related to the near-horizon region of 3+1-dimensional Reissner-Nordstr\"om 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.

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