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Numerical Relativity in 3+1 Dimensions

Bernd Bruegmann
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Abstract

Numerical relativity is finally approaching a state where the evolution of rather general (3+1)-dimensional data sets can be computed in order to solve the Einstein equations. After a general introduction, three topics of current interest are briefly reviewed: binary black hole mergers, the evolution of strong gravitational waves, and shift conditions for neutron star binaries.

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Bernd Bruegmann. 1999-12-02. Numerical Relativity in 3+1 Dimensions. https://doi.org/10.1002/(sici)1521-3889(200005)9%3A3%2F5%3C227%3A%3Aaid-andp227%3E3.0.co%3B2-d

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