Self-interaction correction to black hole radiance

1994/08/02 by Per Kraus, Frank Wilczek · 16 citations
Mathematics · Physics and Astronomy · #Action (physics) #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Black hole (networking) #Black-body radiation #Charged particle #Classical mechanics #Computer science #Geodesic #Geometry #Gravitation #Massless particle #Mathematics #Optics #Particle (ecology) #Particle radiation #Physics #Quantum Electrodynamics and Casimir Effect #Quantum electrodynamics #Quantum mechanics #Radiance #Radiation #Thermal radiation #gr-qc #hep-th

paper · pdf · doi:10.1016/0550-3213(94)00411-7

published as Nucl.Phys.B433:403-420,1995 · 20 pages, no figures, uses Phyzzx, IASSNS-HEP 94/61

arxiv created 1994/08/02 · openalex publication_date 1995/01/01 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

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.

Citations

• Quantum Fields in Curved Space
• Particle creation by black holes
• The black hole interpretation of string theory

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