The time evolution of the gravitational radiation radiated power per unit solid angle for a generic binary black hole configuration. The asymmetry in the radiation leads to the instantaneous gravitational radiation recoil.
Manuela Campanelli, Carlos Lousto, Yosef Zlochower
Center for Computational Relativity and Gravitation, School of Mathematical Sciences, Rochester Institute of Technology, One Lomb Memorial Drive, Rochester, New York 14623, USA Phone: (585) 475-7752 Fax: (585) 475-7340
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