From reissner-nordstrom quantum states to charged black holes mass evaporation

摘要

In this report we describe quantum Reissner-Nordstrom (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 #PSI#_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 ref. ~12.