Gravitational Back Reaction of Hawking modes
D. Ring

TL;DR
This paper models black hole evaporation considering gravitational back reaction, showing that such effects can prevent complete evaporation and make the black hole effectively eternal.
Contribution
It introduces a toy model using Vaidya metric to incorporate back reaction, demonstrating how it alters the black hole evaporation process.
Findings
Back reaction suppresses evaporation rate significantly.
Singularity near the horizon is softened by back reaction.
Black hole can become effectively eternal due to back reaction.
Abstract
The radiation rate of an evaporating black hole is calculated in a toy model in which the geometry outside the collapsing matter is described by a Vaidya metric. When back reaction consistency is imposed, the singularity in the blueshift factor near the horizon is softened, suppressing the evaporation rate in the Schwarzschild case by the fourth power of the external time, thus rendering the hole eternal.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Quantum Electrodynamics and Casimir Effect
