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RESEARCH PRODUCT
Evaporation of Near-Extremal Reissner-Nordström Black Holes
José Navarro-salasD. J. NavarroAlessandro Fabbrisubject
AstrofísicaHigh Energy Physics - TheoryPhysicsEvent horizonMembrane paradigmAstronomyAstronomical PhenomenaEvaporationFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Models TheoreticalFuzzballGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics - Theory (hep-th)Nonsingular black hole modelsAstronomiaCamps Teoria quàntica deBlack hole thermodynamicsMathematical physicsdescription
The formation of near-extremal Reissner-Nordstrom black holes in the S-wave approximation can be described, near the event horizon, by an effective solvable model. The corresponding one-loop quantum theory remains solvable and allows to follow analytically the evaporation process which is shown to require an infinite amount of time.
year | journal | country | edition | language |
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2000-09-18 | Physical Review Letters |