Quantum rotating black holes

Abstract

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.

arXiv commentLaTeX, 12 pages, 1 figure, final version to appear in JHEP

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• A new representation of vacuum Lovelock solutions in $d=2N+1$ dimensions: Black holes with an integrable singularity and regular black holes
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• The Quantum Model of Spinning Black Holes
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• Reissner Nordstrom black holes with integrable singularity interiors supported by string distributions
• Regular Kerr black holes: Junction conditions and the matter content across the ring