Evaporation of charged black holes near extremality

Details Evaporation of charged black holes near extremality Evaporation of charged black holes near extremality

2000-12-04

arxiv.org/abs/hep-th/0012019v1

Physics

High Energy Physics

High Energy Physics - Theory

LaTeX file, 3 pages. Talk given at the Ninth Marcel Grossmann Meeting

Scientific paper

The AdS_2\timesS^2 geometry of near-extremal Reissner-Nordstrom black holes
can be described by an effective solvable model which allows to follow
analytically the evaporation process including the backreaction. We find that
an infinite amount of time is required for the black hole to decay to
extremality.

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