Evaporation of near-extremal Reissner-Nordstrom black holes
classification
✦ hep-th
gr-qc
keywords
blackevaporationholesnear-extremalreissner-nordstromsolvableallowsamount
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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.
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Cited by 1 Pith paper
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Radiating black holes in general relativity need not be singular
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