Self-Interaction Correction to Black Hole Radiance

Details Self-Interaction Correction to Black Hole Radiance Self-Interaction Correction to Black Hole Radiance

1994-08-02

arxiv.org/abs/gr-qc/9408003v1

Nucl.Phys.B433:403-420,1995

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

20 pages, no figures, uses Phyzzx, IASSNS-HEP 94/61

Scientific paper

10.1016/0550-3213(94)00411-7

We consider the modification of the formulas for black hole radiation, due to the self-gravitation of the radiation. This is done by truncating the coupled particle-hole system to a small set of modes, that are plausibly the most significant ones, and quantizing the reduced system. In this way we find that the particles no longer move along geodesics, nor is the action along the rays zero for a massless particle. The radiation is no longer thermal, but is corrected in a definite way that we calculate. Our methods can be extended in a straightforward manner to discuss correlations in the radiation, or between incoming particles and the radiation.

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