Semiclassical Stability of the Extreme Reissner-Nordstrom Black Hole

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dc.creatorAnderson, Paul R.
dc.creatorHiscock, William A.
dc.creatorLoranz, Daniel J.
dc.date1995-04-13
dc.date.accessioned2026-07-07T10:57:54Z
dc.date.available2026-07-07T10:57:54Z
dc.descriptionThe 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.
dc.description10 pages, REVTeX, 4 figures in separate uuencoded compressed file
dc.identifierhttps://arxiv.org/abs/gr-qc/9504019
dc.identifierhttp://arxiv.org/abs/gr-qc/9504019
dc.identifierPhys.Rev.Lett.74:4365-4368,1995
dc.identifierdoi:10.1103/PhysRevLett.74.4365
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186916
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleSemiclassical Stability of the Extreme Reissner-Nordstrom Black Hole
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