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Stable characteristic evolution of generic 3-dimensional single-black-hole spacetimes

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abstract

We report new results which establish that the accurate 3-dimensional numerical simulation of generic single-black-hole spacetimes has been achieved by characteristic evolution with unlimited long term stability. Our results cover a selection of distorted, moving and spinning single black holes, with evolution times up to 60,000M.

fields

gr-qc 1

years

2025 1

verdicts

CONDITIONAL 1

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