Generalizes ⟨Φ̂²⟩_ren and flux computations to non-minimal ξ near Kerr inner horizon along axis, finding per-mode ringdown (frequencies twice classical QNMs) then r_*^{-2ℓ-3} tails approaching finite value.
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Quantum fluxes and $\langle\hat{\Phi}^2\rangle$ for a non-minimally coupled scalar field: ringdown and tail on approaching the polar Kerr inner horizon
Generalizes ⟨Φ̂²⟩_ren and flux computations to non-minimal ξ near Kerr inner horizon along axis, finding per-mode ringdown (frequencies twice classical QNMs) then r_*^{-2ℓ-3} tails approaching finite value.