Simple excision of a black hole in 3+1 numerical relativity

Preprint

28 August 2000

preprint
Published by arXiv in arXiv

Abstract

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.

Keywords

SIMPLE IMPLEMENTATION
NUMERICAL RELATIVITY
SCHWARZSCHILD BLACK
SIMPLE EXCISION
HOLE EXCISION
BLACK HOLE
EVOLUTIONS
STABLE
OCTANT

All Related Versions

Version 1, 2000-08-28, ArXiv
Version 2, 2001-03-23, ArXiv
Published version: Physical Review D, 63 (10).

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