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Formation and evaporation of charged black holes
Physical Review D, Particles and fields
We investigate the dynamical formation and evaporation of a spherically symmetric charged black hole. We study the self-consistent one loop order semiclassical back-reaction problem. To this end the mass-evaporation is modeled by an expectation value of the stress-energy tensor of a neutral massless scalar field, while the charge is not radiated away. We observe the formation of an initially non extremal black hole which tends toward the extremal black hole M=Q, emitting Hawking radiation. Ifdoi:10.1103/physrevd.63.124024 fatcat:34scflryijcanfepv7o6niq6zm