About this document
Black Holes and Thermal Bath Dynamics by Fajar Nugrahanto is a document available to read on EtoBox.
This document summarizes a study of evaporating black holes coupled to a thermal bath. The study finds that depending on the initial temperature of the black hole relative to the bath, the black hole can lose mass by emitting Hawking radiation, stay in equilibrium with the bath, or gain mass by absorbing thermal radiation. In all scenarios, a unitary Page curve is obtained by applying the generalized entropy prescription and identifying the quantum extremal surface. As the black hole evaporates, the quantum
- Author
- Fajar Nugrahanto
- Language
- EN