We study quantum dynamics of spherically symmetric black holes interacting with a scalar field, by solving the Wheeler-DeWitt equation near the apparent horizon. We obtain the wave function representing the black-hole evaporation due to quantum production of scalar waves. The mass-loss rate inferred from the Hawking radiation is justified, and the final fate of the evaporation is discussed.
机构:
Inst Gravitat & Cosmos, University Pk, PA 16802 USA
Phys Dept Penn State, University Pk, PA 16802 USA
Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USAIN2P3, CNRS, INPG, UJF,Lab Phys Subatom & Cosmol, F-38026 Grenoble, France