Effect of Self-Interaction on Charged Black Hole Radiance

Details Effect of Self-Interaction on Charged Black Hole Radiance Effect of Self-Interaction on Charged Black Hole Radiance

1994-11-29

arxiv.org/abs/hep-th/9411219v1

Nucl.Phys.B437:231-242,1995

Physics

High Energy Physics

High Energy Physics - Theory

13 pages in Latex, no figures

Scientific paper

10.1016/0550-3213(94)00588-6

We extend our previous analysis of the modification of the spectrum of black hole radiance due to the simplest and probably most quantitatively important back-reaction effect, that is self-gravitational interaction, to the case of charged holes. As anticipated, the corrections are small for low-energy radiation when the hole is well away from extremality, butbecome qualitatively important near extremality. A notable result is that radiation which could leave the hole with mass and charge characteristic of a naked singularity, predicted in the usual approximation of fixed space-time geometry, is here suppressed. We discuss the nature of our approximations, and show how they work in a simpler electromagnetic analogue problem.

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