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.
[51]Gursel, Y., Sandberg, V., Novikov, I., and Starobinsky, A.Evolution of scalar perturbations near the Cauchy horizon of a charged black hole.Phys
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
gr-qc 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
A weak null singularity forms inside generic subextremal strictly rotating black holes, with the metric continuously extendible but not Lipschitz extendible.
A technical note strengthens the linear instability of the Kerr Cauchy horizon to enable a nonlinear instability proof.
citing papers explorer
-
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.
-
The formation of a weak null singularity in the interior of generic rotating black holes
A weak null singularity forms inside generic subextremal strictly rotating black holes, with the metric continuously extendible but not Lipschitz extendible.
-
A note on the instability of the Kerr Cauchy horizon under linearised gravitational perturbations
A technical note strengthens the linear instability of the Kerr Cauchy horizon to enable a nonlinear instability proof.