Semiclassical Stability of the Extreme Reissner-Nordstrom Black Hole

Details Semiclassical Stability of the Extreme Reissner-Nordstrom Black Hole Semiclassical Stability of the Extreme Reissner-Nordstrom Black Hole

1995-04-13

arxiv.org/abs/gr-qc/9504019v1

Phys.Rev.Lett.74:4365-4368,1995

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

10 pages, REVTeX, 4 figures in separate uuencoded compressed file

Scientific paper

10.1103/PhysRevLett.74.4365

The stress-energy tensor of a free quantized scalar field is calculated in the extreme Reissner-Nordstr\"{o}m black hole spacetime in the zero temperature vacuum state. The stress-energy appears to be regular on the event horizon, contrary to the suggestion provided by two-dimensional calculations. An analytic calculation on the event horizon for a thermal state shows that if the temperature is nonzero then the stress-energy diverges strongly there.

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