Boundary Conditions at Infinity are those of computational electromagnetics (CEM)
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Not those familiar from CFD
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One needs to look for wave solutions and these waves are precisely what LIGO experiment will detect
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Curiously I see that methods used in CEM such as method of moments are not being used in Numerical Relativity
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NR solves evolution equations and identifies oscillatory wave solution
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Waves very sensitive to numerics -- small numerical errors can be amplified as wave propagates
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Numerical approximation can introduce an effective dissipative term which has small coefficient but enhanced by large propagation distance
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