Speculation about the black hole final state: resolving singularity by quantum gravity
arXiv:2105.00066 · doi:10.31526/ACP.BSM-2021.37
Abstract
The interior of the black hole can be described by anisotropic cosmology. By quantizing the metric function, we can obtain the Wheeler-DeWitt equation for inside the horizon. In order to interpret the wave function consistently, one needs to impose a boundary condition. In this paper, we introduce a prescription for the Euclidean analytic continuation inside the horizon and the corresponding wave function solution.
4 pages, 1 figure; Proceedings of Beyond Standard Model: From Theory to Experiment. Talk on March 29, 2021, Giza, Egypt