Remnant-free Moving Mirror Model for Black Hole Radiation Field
General Relativity and Quantum Cosmology
2020-02-04 v1 High Energy Physics - Theory
Quantum Physics
Abstract
We analyze the flow of energy and entropy emitted by a class of moving mirror trajectories which provide models for the radiation fields produced by black hole evaporation. The mirror radiation fields provide natural, concrete examples of processes that follow thermal distributions for long periods, accompanied by transients which are brief and carry little net energy, yet they ultimately represent pure quantum states. A burst of negative energy flux is a generic feature of these fields, but it need not be prominent.
Cite
@article{arxiv.1909.01129,
title = {Remnant-free Moving Mirror Model for Black Hole Radiation Field},
author = {Michael R. R. Good and Eric V. Linder and Frank Wilczek},
journal= {arXiv preprint arXiv:1909.01129},
year = {2020}
}
Comments
5 pages, 5 figures