Black hole mass spectrum vs spectrum of Hawking radiation
V. A. Berezin, A. M. Boyarsky, A. Yu. Neronov

TL;DR
This paper models black hole evaporation using self-gravitating shells, revealing a mismatch between the mass spectrum of the collapsing body and Hawking radiation, and proposing that including ingoing radiation explains the Bekenstein-Mukhanov spectrum for large black holes.
Contribution
It introduces a shell-based model for black hole collapse and radiation, showing the necessity of ingoing radiation to reconcile the spectra and explaining the spectrum evolution during evaporation.
Findings
Mass-energy spectra of the body and radiation do not match.
Including ingoing radiation accounts for the Bekenstein-Mukhanov spectrum.
Black hole structure changes during evaporation.
Abstract
We consider a massive selfgravitating shell as a model for collapsing body and a null selfgravitating shell as a model for quanta of Hawking radiation. It is show that the mass-energy spectra for the body and the radiation do not match. The way out of this difficulty is to consider not only out-going radiation but also the ingoing one. It means that the structure of black hole is changing during its evaporation resulting in the Bekenstein-Mukhanov spectrum for large masses.
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.
