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Cauchy-horizon singularity inside perturbed Kerr black holes
2016
Physical Review D
The Cauchy horizon inside a perturbed Kerr black hole develops an instability that transforms it into a curvature singularity. We solve for the linearized Weyl scalars ψ_0 and ψ_4 and for the curvature scalar R_αβγδR^αβγδ along outgoing null rays approaching the Cauchy horizon in the interior of perturbed Kerr black holes using the Teukolsky equation, and compare our results with those found in perturbation analysis. Our results corroborate the previous perturbation analysis result that at its
doi:10.1103/physrevd.93.041501
fatcat:zoujypwtgrhxfngwwzrm2phfpe