Quantum rotating black holes
Roberto Casadio, Andrea Giusti, Jorge Ovalle
Abstract
A bstract We consider black holes generically sourced by quantum matter described by regular wavefunctions. This allows for integrable effective energy densities and the removal of Cauchy horizons in spherically symmetric configurations. Moreover, we identify the ultrarigid rotation of the Kerr spacetime as causing the existence of an inner horizon in rotating systems, and describe general properties for quantum matter cores at the centre of rotating black holes with integrable singularities and no Cauchy horizon.
Topics & Concepts
PhysicsGravitational singularityHorizonIntegrable systemBlack hole (networking)QuantumMathematical physicsRotating black holeWave functionQuantum mechanicsClassical mechanicsRouting protocolAstronomyLink-state routing protocolRouting (electronic design automation)Computer networkComputer scienceBlack Holes and Theoretical PhysicsNonlinear Waves and SolitonsCosmology and Gravitation Theories