Semiclassical Stability of the Extreme Reissner-Nordström Black Hole
- 29 May 1995
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 74 (22) , 4365-4368
- https://doi.org/10.1103/physrevlett.74.4365
Abstract
The stress-energy tensor of a free quantized scalar field is calculated in the extreme Reissner-Nordström 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
All Related Versions
This publication has 12 references indexed in Scilit:
- Entropy, area, and black hole pairsPhysical Review D, 1995
- Massive string states as extreme black holesPhysics Letters B, 1995
- Semiclassical extremal black holesPhysical Review D, 1993
- Stress-energy tensor of quantized scalar fields in static black hole spacetimesPhysical Review Letters, 1993
- Black holes as elementary particlesNuclear Physics B, 1992
- Killing approximation for vacuum and thermal stress-energy tensor in static space-timesPhysical Review D, 1987
- Magnetic Monopoles and Evaporating Black HolesPhysical Review Letters, 1983
- Stress-tensor trace anomaly in a gravitational metric: General theory, Maxwell fieldPhysical Review D, 1977
- Stress-energy tensor near a charged, rotating, evaporating black holePhysical Review D, 1977
- Uniform Electromagnetic Field in the Theory of General RelativityPhysical Review B, 1959