Evaporation of near-extremal Reissner-Nordstrom black holes
arXiv:hep-th/0004027 · doi:10.1103/PhysRevLett.85.2434
Abstract
The formation of near-extremal Reissner-Nordstrom black holes in the S-wave approximation can be described, near the event horizon, by an effective solvable model. The corresponding one-loop quantum theory remains solvable and allows to follow analytically the evaporation process which is shown to require an infinite amount of time.
LaTeX file, 4 pages, 2 figures. Final version, to appear in Phys. Rev. Lett
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