End of a black hole’s evaporation. II.
Farshid Soltani, Carlo Rovelli, Pierre Martin-Dussaud
Abstract
We derive an explicit expression for the transition amplitude from black to white hole horizon at the end of Hawking evaporation using covariant loop quantum gravity.
Topics & Concepts
PhysicsBlack hole (networking)Covariant transformationHorizonMathematical physicsCosmologyHawking radiationWhite holeBlack hole thermodynamicsHawkingAstrophysicsEvaporationTheoretical physicsAstronomyThermodynamicsComputer scienceComputer networkLink-state routing protocolRouting (electronic design automation)Routing protocolNoncommutative and Quantum Gravity TheoriesBlack Holes and Theoretical PhysicsCosmology and Gravitation Theories