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Black holes modeled by the Kerr metric are not semiclassically self-consistent at or below the inner horizon.
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G. O. Papadopoulos and K. D. Kokkotas, Preserving Kerr symmetries in deformed spacetimes, Classical and Quantum Gravity 35
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J. Baines and M. Visser, Killing horizons and surface gravities for a well-behaved three-function generalization of the Kerr spacetime, Universe 9
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C. Klein, M. Soltani, M. Casals, and S. Hollands, Infinite quantum twisting at the Cauchy horizon of rotating black holes, Phys. Rev. Lett. 132
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