Oscillatory null singularity inside realistic spinning black holes

Abstract

We calculate the asymptotic behavior of the curvature scalar $(Riemann{)}^2$ near the null weak singularity at the inner horizon of a generic spinning black hole, and show that this scalar oscillates infinite number of times while diverging. The dominant parallelly-propagated Riemann components oscillate in a similar manner. This oscillatory behavior, which is in a remarkable contrast to the monotonic mass-inflation singularity in spherical charged black holes, is caused by the dragging of inertial frames due to the black- hole's spin.

10 pages, Latex; This version is almost identical to the one previously published in Phys. Rev. Lett

References in corpus (2)

• Late-Time Evolution of Realistic Rotating Collapse and The No-Hair Theorem
• Late-time decay of gravitational and electromagnetic perturbations along the event horizon

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