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arXiv · hep-th/0202005

Near-Extremal Black Hole Evaporation in Asymptotically Flat Spacetime

Kamran Diba·David A. Lowe
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Abstract

We study black hole evaporation of near-extremal black holes in spherically reduced models with asymptotically Minkowskian spacetime, with the effects of the back-reaction on the geometry included semi-classically. The stress-energy tensor is calculated for null in-falling observers. It is shown that the evaporation proceeds smoothly and there are no instabilities of the outer or inner apparent horizon before the endpoint of evaporation.

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Kamran Diba, David A. Lowe. 2002-02-01. Near-Extremal Black Hole Evaporation in Asymptotically Flat Spacetime. https://doi.org/10.1103/physrevd.66.024039

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