3D hairy rotating black holes have interiors consisting of an infinite analytically describable sequence of Kasner epochs that evolve into a curvature singularity.
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In O(d,d) symmetric gravity with curvature corrections, black brane singularities are not resolved but approach with altered Kasner exponents, while a dilaton generates negative cosmological constants at small coupling.
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Analytical studies on 3D hairy rotating black hole interiors
3D hairy rotating black holes have interiors consisting of an infinite analytically describable sequence of Kasner epochs that evolve into a curvature singularity.
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$O(d,d)$ symmetric gravity and finite coupling holography
In O(d,d) symmetric gravity with curvature corrections, black brane singularities are not resolved but approach with altered Kasner exponents, while a dilaton generates negative cosmological constants at small coupling.