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• W2064664821 abstract "We present the first simulations of non-head-on (grazing) collisions of binary black holes in which the singularities are excised from the simulation. Initially equal mass m black holes (spinning or not) are separated by approximately 10m and with impact parameter approximately 2m. Evolutions to t approximately 35m are obtained where two separate horizons are present for t approximately 3.8m; then a single enveloping horizon forms indicating that the holes merged. Apparent horizon area estimates suggest gravitational radiation of about 2%-3% of the total mass. The evolutions end after a moderate amount of time because of instabilities." @default.
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• W2064664821 date "2000-12-25" @default.
• W2064664821 modified "2023-09-26" @default.
• W2064664821 title "Grazing Collisions of Black Holes via the Excision of Singularities" @default.
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• W2064664821 doi "https://doi.org/10.1103/physrevlett.85.5496" @default.
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