Particle spectrum of the Reissner–Nordström black hole
Michael R. R. Good, Yen Chin Ong
Abstract
Abstract The Reissner–Nordström black hole – moving mirror correspondence is solved. The beta coefficients reveal that charge makes a black hole radiate fewer particles (neutral massless scalars) per frequency. An old Reissner–Nordström black hole emits particles in an explicit Planck distribution with temperature corresponding to the surface gravity of its outer horizon.
Topics & Concepts
PhysicsVirtual black holeBlack hole (networking)Charged black holeWhite holeExtremal black holeMassless particleRotating black holeSpin-flipHawking radiationParticle (ecology)Quantum electrodynamicsPrimordial black holeBlack-body radiationStellar black holePlanckClassical mechanicsElectron holeSonic black holeQuantum mechanicsRing singularitySchwarzschild radiusAstrophysicsMicro black holeCharge (physics)Spectrum (functional analysis)Surface gravityBinary black holeAstrophysical Phenomena and ObservationsBlack Holes and Theoretical PhysicsRelativity and Gravitational Theory