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• W2953260740 abstract "We numerically solve Einstein's equations coupled to a scalar field in the interior of Kerr black holes. We find shock waves form near the inner horizon. The shocks grow exponentially in amplitude and need not be axisymmetric. Observers who pass through the shocks experience exponentially large tidal forces and are accelerated exponentially close to the speed of light." @default.
• W2953260740 created "2019-06-27" @default.
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• W2953260740 date "2019-04-17" @default.
• W2953260740 modified "2023-09-30" @default.
• W2953260740 title "Numerical evolution of shocks in the interior of Kerr black holes" @default.
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• W2953260740 doi "https://doi.org/10.1103/physrevd.99.084033" @default.
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