The End of a Black Hole's Evaporation -- Part II
arXiv:2105.06876 · doi:10.1103/PhysRevD.104.066015
Abstract
We derive an explicit expression for the transition amplitude from black to white hole horizon at the end of Hawking evaporation using covariant loop quantum gravity.
10 pages, 12 figures. V2: added references, corrected typos
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- Stellar collapse with pressure in effective loop quantum gravity
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- Tunneling of quantum geometries in spinfoams
- Quantum Schwarzschild-(A)dS Black Holes: Unitarity and Singularity Resolution
- Spinfoam tunneling of quantum geometries in angle variables
- Gravastar-like black hole solutions in -theory
- A spin foam framework for the black-to-white hole transition