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, but become 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.
Original language | English (US) |
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Pages (from-to) | 231-242 |
Number of pages | 12 |
Journal | Nuclear Physics, Section B |
Volume | 437 |
Issue number | 1 |
DOIs | |
State | Published - Mar 6 1995 |
Externally published | Yes |
ASJC Scopus subject areas
- Nuclear and High Energy Physics