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Quantum Theory of Black Holes

J. Gegenberg·G. Kunstatter
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Abstract

A solvable 2-dimensional conformally invariant midi-superspace model for black holes is obtained by imposing spherical symmetry in 4-dimensional conformally invariant Einstein gravity. The Wheeler-DeWitt equation for the theory is solved exactly to obtain the unique quantum wave functional for an isolated black hole with fixed mass. By suitably relaxing the boundary conditions, a non-perturbative ansatz is obtained for the wave functional of a black hole interacting with its surroundings.

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J. Gegenberg, G. Kunstatter. 1993-02-05. Quantum Theory of Black Holes. https://doi.org/10.1103/physrevd.47.r4192

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