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Wave Function for the Reissner–Nordström Black Hole
1997
Modern Physics Letters A
We study the quantum behaviour of Reissner-Nordström (RN) black-holes interacting with a complex scalar field. A Maxwell field is also present. Our analysis is based on M. Pollock's method and is characterized by solving a Wheeler-DeWitt equation in the proximity of an apparent horizon of the RN space-time. Subsequently, we obtain a wave-function Ψ_RN[M, Q] representing the RN black-hole when its charge, | Q |, is small in comparison with its mass, M. We then compare quantum-mechanically the
doi:10.1142/s0217732397001527
fatcat:yj4eukzcgzbrhiwns4g25b6qf4