Gravitational waves from quasi-spherical black holes

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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4 revtex pages, 2 eps figures

Scientific paper

10.1103/PhysRevD.61.101503

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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