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Effect of Self-Interaction on Charged Black Hole Radiance | | Per Kraus
; Frank Wilczek
; | | Date: |
29 Nov 1994 | | Journal: | Nucl.Phys. B437 (1995) 231-242 | | Abstract: | 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. | | Source: | arXiv, hep-th/9411219 | | Services: | Forum | Review | PDF | Favorites | |
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