| Name: | Description: | Size: | Format: | |
|---|---|---|---|---|
| 1.6 MB | Adobe PDF |
Authors
Advisor(s)
Abstract(s)
The purpose of this paper is to analyse the back reaction problem, between Hawking radiation and the black hole, in a simplified model for the black hole evaporation in the quantum geometrodynamics context. The idea is to transcribe the most important characteristics of the Wheeler-DeWitt equation into a Schrödinger’s type of equation. Subsequently, we consider Hawking radiation and black hole quantum states evolution under the influence of a potential that includes back reaction. Finally, entropy is estimated as a measure of the entanglement between the black hole and Hawking radiation states in this model.
Description
Keywords
Quantum gravity Hawking radiation Entanglement entropy