The End of a Black Hole's Evaporation -- Part I
arXiv:2009.05016 · doi:10.1103/PhysRevD.103.106014
Abstract
At the end of Hawking evaporation, the horizon of a black hole enters a physical region where quantum gravity cannot be neglected. The physics of this region has not been much explored. We characterise its physics and introduce a technique to study it.
11 pages, 10 figures