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Gravitational waves from quasi-spherical black holes

Sean A. Hayward
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Abstract

A quasi-spherical approximation scheme, intended to apply to coalescing black holes, allows the waveforms of gravitational radiation to be computed by integrating ordinary differential equations.

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Sean A. Hayward. 2000-01-21. Gravitational waves from quasi-spherical black holes. https://doi.org/10.1103/physrevd.61.101503

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