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Gravitational wave extraction and outer boundary conditions by perturbative matching

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abstract

We present a method for extracting gravitational radiation from a three-dimensional numerical relativity simulation and, using the extracted data, to provide outer boundary conditions. The method treats dynamical gravitational variables as nonspherical perturbations of Schwarzschild geometry. We discuss a code which implements this method and present results of tests which have been performed with a three dimensional numerical relativity code.

fields

gr-qc 1

years

2024 1

verdicts

CONDITIONAL 1

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