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From Reissner-Nordström quantum states to charged black holes mass evaporation

P. V. Moniz
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Abstract

In this report we describe quantum Reissner-Nordström (RN) black-holes interacting with a complex scalar field. Our analysis 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. A special emphasis is given to the evolution of the mass-charge rate affected by Hawking radiation. More details can be found in gr-qc/9709080.

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P. V. Moniz. 1997-09-30. From Reissner-Nordström quantum states to charged black holes mass evaporation. https://arxiv.org/abs/hep-th/9709208

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