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Simple excision of a black hole in 3+1 numerical relativity
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Simple excision of a black hole in 3+1 numerical relativity
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We describe a simple implementation of black hole excision in 3+1 numerical relativity. We apply this technique to a Schwarzschild black hole with octant symmetry in Eddington-Finkelstein coordinates and show how one can obtain accurate, long-term stable numerical evolutions.
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Cited by 1 Pith paper
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