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• W2094534035 abstract "The final evolution of a binary black-hole system gives rise to a recoil velocity if an asymmetry is present in the emitted gravitational radiation. Measurements of this effect for non-spinning binaries with unequal masses have pointed out that kick velocities $sim~175$ km/s can be reached for a mass ratio $simeq 0.36$. However, a larger recoil can be obtained for equal-mass binaries if the asymmetry is provided by the spins. Using two independent methods we show that the merger of such binaries yields velocities as large as $sim 440$ km/s for black holes having unequal spins that are antialigned and parallel to the orbital angular momentum." @default.
• W2094534035 created "2016-06-24" @default.
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• W2094534035 date "2007-07-27" @default.
• W2094534035 modified "2023-10-18" @default.
• W2094534035 title "Recoil Velocities from Equal-Mass Binary-Black-Hole Mergers" @default.
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• W2094534035 doi "https://doi.org/10.1103/physrevlett.99.041102" @default.
• W2094534035 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/17678346" @default.
• W2094534035 hasPublicationYear "2007" @default.
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