End of a black hole’s evaporation
Fabio D’Ambrosio, Marios Christodoulou, Pierre Martin-Dussaud, Carlo Rovelli, Farshid Soltani
Abstract
At the end of the Hawking evaporation the horizon of a black hole enters a physical region where quantum gravity cannot be neglected. The physics of this region has not been much explored. We characterize its physics and introduce a technique to study it.
Topics & Concepts
Black hole (networking)HawkingPhysicsEvaporationHorizonHawking radiationBlack hole thermodynamicsSonic black holeQuantum gravityMicro black holeTheoretical physicsQuantumQuantum electrodynamicsQuantum mechanicsAstronomyThermodynamicsComputer scienceRouting (electronic design automation)Routing protocolComputer networkLink-state routing protocolNoncommutative and Quantum Gravity TheoriesQuantum Electrodynamics and Casimir EffectBlack Holes and Theoretical Physics