Phys. Rev. D 63, 104006 (2001) [6 pages]Simple excision of a black hole in 3+1 numerical relativity
Miguel Alcubierre and Bernd Brügmann Received 6 September 2000; published 5 April 2001 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. ©2001 The American Physical Society
URL: http://link.aps.org/abstract/PRD/v63/e104006 [ Abstract | Previous article | Next article | Issue 10 ] |
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