Modeling black hole evaporative mass evolution via radiation from moving mirrors

Abstract

We investigate the evaporation of an uncharged and non-rotating black hole (BH) in vacuum, by taking into account the effects given by the shrinking of the horizon area. These include the back-reaction on the metric and other smaller contributions arising from quantum fields in curved spacetime. Our approach is facilitated by the use of an analog accelerating moving mirror. We study the consequences of this modified evaporation on the BH entropy. Insights are provided on the amount of information obtained from a BH by considering non-equilibrium thermodynamics and the non-thermal part of Hawking radiation.

arXiv comment13 pages, 5 figures

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Cited by in corpus (6)

• Optomechanical Backreaction of Quantum Field Processes in Dynamical Casimir Effect
• Moving mirrors and event horizons in non-flat background geometry
• A numerical approach to particle creation in accelerating toy models
• Vacuum-purified Hawking radiation from evaporating black holes: Lessons from moving mirrors
• Time-dependent accelerated Unruh-DeWitt detector without event horizon
• Searching for the classical version of Hawking radiation and screening of Coulomb field by the horizon