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• W1976662389 abstract "We consider the effect of backreaction of quantized massive fields on the metric of extreme black holes (EBH). We find the analytical approximate expression for the stress-energy tensor for a scalar (with an arbitrary coupling), spinor and vector fields near an event horizon. We show that, independent of a concrete type of EBH, the energy measured by a freely falling observer is finite on the horizon, so that quantum backreaction is consistent with the existence of EBH. For the Reissner-Nordstrom EBH with a total mass M_{tot} and charge Q we show that for all cases of physical interest M_{tot}< Q. We also discuss different types of quantum-corrected Bertotti-Robinson spacetimes, find for them exact self-consistent solutions and consider situations in which tiny quantum corrections lead to the qualitative change of the classical geometry and topology. In all cases one should start not from a classical background with further adding quantum corrections but from the quantum-corrected self-consistent geometries from the very beginning." @default.
• W1976662389 created "2016-06-24" @default.
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• W1976662389 date "2001-10-26" @default.
• W1976662389 modified "2023-09-23" @default.
• W1976662389 title "Quantum back reaction of massive fields and self-consistent semiclassical extreme black holes and acceleration horizons" @default.
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• W1976662389 doi "https://doi.org/10.1103/physrevd.64.104018" @default.
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