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The discrete energy method in numerical relativity: towards long-term stability

Luis Lehner1, David Neilsen1,2, Oscar Reula3 and Manuel Tiglio1,4,5

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The energy method can be used to identify well-posed initial boundary value problems for quasi-linear, symmetric hyperbolic partial differential equations with maximally dissipative boundary conditions. A similar analysis of the discrete system can be used to construct stable finite difference equations for these problems at the linear level. In this paper we apply these techniques to some test problems commonly used in numerical relativity and observe that while we obtain convergent schemes, fast growing modes, or 'artificial instabilities', contaminate the solution. We find that these growing modes can partially arise from the lack of a Leibnitz rule for discrete derivatives and discuss ways to limit this spurious growth.


PACS

04.25.D- Numerical relativity

02.60.Lj Ordinary and partial differential equations; boundary value problems

04.70.-s Physics of black holes

MSC

65M12 Stability and convergence of numerical methods

83C57 Black holes

83C27 Lattice gravity, Regge calculus and other discrete methods

Subjects

Computational physics

Gravitation and cosmology

Dates

Issue 24 (21 December 2004)

Received 29 July 2004, in final form 19 October 2004

Published 25 November 2004



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