Semiclassical Stability of the Extreme Reissner-Nordstrom Black Hole

Preprint

13 April 1995

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.gr-qc/9504019

Abstract

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.

Keywords

SEMICLASSICAL STABILITY
REISSNER NORDSTROM
EXTREME REISSNER
STRESS ENERGY
TEMPERATURE
BLACK HOLE
QUANTIZED

All Related Versions

Version 1, 1995-04-13, ArXiv
Published version: Physical Review Letters, 74 (22), 4365.

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