1997/06/28 by Paulo Vargas Moniz, P. V. Moniz · 1 citation
Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Charge (physics) #Cosmology and Gravitation Theories #Field (mathematics) #Function (biology) #Geometry #Gravitational wave #Hawking radiation #Horizon #Mathematical physics #Physics #Quantum #Quantum Electrodynamics and Casimir Effect #Quantum electrodynamics #Quantum mechanics #Scalar (mathematics) #Scalar field #Wave equation #Wave function #gr-qc #hep-th
paper · pdf · doi:10.1142/s0217732397001527
published as Mod.Phys.Lett. A12 (1997) 1491-1505 · 13 pages, LaTeX
openalex publication_date 1997/06/28 · arxiv created 1997/09/30 · arxiv updated 2015/06/25 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We study the quantum behavior 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 1 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 cases of (i) Q=0 and (ii) M≥|Q|≠0. A special emphasis is given to the evolution of the mass-charge rate affected by Hawking radiation.