Stable characteristic evolution of generic 3-dimensional single-black-hole spacetimes
arXiv:gr-qc/9801069 · doi:10.1103/PhysRevLett.80.3915
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.
4 pages, 3 figures
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Cited by in corpus (66)
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