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arXiv · 1703.01921

Inflation followed by Belinskii-Khalatnikov-Lifshitz collapse inside accreting, rotating black holes

Andrew J. S. Hamilton
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Abstract

Numerical evidence is presented that the Poisson-Israel mass inflation instability at the inner horizon of an accreting, rotating black hole is generically followed by Belinskii-Khalatnikov-Lifshitz oscillatory collapse to a spacelike singularity. The computation involves following all 6 degrees of freedom of the gravitational field. To simplify the problem, the computation takes as initial conditions the conformally separable solutions of arXiv:1010.1269, arXiv:1010.1271 just above the inner horizon of a slowly accreting, rotating black hole, and integrates the equations inward along single latitudes.

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Andrew J. S. Hamilton. 2017-03-06. Inflation followed by Belinskii-Khalatnikov-Lifshitz collapse inside accreting, rotating black holes. https://doi.org/10.1103/physrevd.96.084041

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