Universal Lyapunov bounds for rotating higher-dimensional black holes
Determine whether the dimension-dependent Lyapunov-exponent bounds derived for static, spherically symmetric higher-dimensional black holes extend to rotating higher-dimensional black holes, where null trapping is described by a photon region rather than a single photon sphere.
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Whether the same substitution disposes of the charged-particle violations above is an open question rather than a settled one, since no T_{\rm ind} has been constructed for those orbits.
A more challenging extension concerns rotating higher-dimensional black holes. Once spherical symmetry is lost, null trapping is generally described by a photon region rather than a single photon sphere, making the construction of a universal instability bound considerably more involved. Investigating these extensions would help determine whether the bounds derived here reflect a more general property of black-hole spacetimes or are specific to the static, spherically symmetric setting considered in this work.