arXiv · hep-th/0504073
Semi-classical geometry of charged black holes
Abstract
At the classical level, two-dimensional dilaton gravity coupled to an abelian gauge field has charged black hole solutions, which have much in common with four-dimensional Reissner-Nordstrom black holes, including multiple asymptotic regions, timelike curvature singularities, and Cauchy horizons. The black hole spacetime is, however, significantly modified by quantum effects, which can be systematically studied in this two-dimensional context. In particular, the back-reaction on the geometry due to pair-creation of charged fermions destabilizes the inner horizon and replaces it with a spacelike curvature singularity. The semi-classical geometry has the same global topology as an electrically neutral black hole.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Andrei V. Frolov, Kristjan R. Kristjansson, Larus Thorlacius. 2006-04-06. Semi-classical geometry of charged black holes. https://doi.org/10.1103/physrevd.72.021501
Cite the original work for its findings. Save a collection to share your selection of sources.