End of a black hole's evaporation

At the end of the 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 characterize its physics and introduce a technique to study it.

Automated summary

At the end of Hawking radiation, the horizon of a black hole enters a physical region where quantum gravity cannot be ignored. The physics of this region has not been thoroughly explored, but a technique to study it has been introduced.