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

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 ${\Psi }_{RN}[M,Q]$ 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 gr-qc/9709080.

3 pages, LaTeX, requires mprocl.sty available at http://shemesh.fiz.huji.ac.il/MG8/submission.html, talk given in the Quantum Gravity session at the MG8 conference, minor correction in the abstract

References in corpus (1)

• Wave Function for the Reissner-Nordström Black-Hole