Grazing Collisions of Black Holes via the Excision of Singularities

Abstract

We present the first simulations of non-headon (grazing) collisions of binary black holes in which the black hole singularities have been excised from the computational domain. Initially two equal mass black holes $m$ are separated a distance $\approx 10m$ and with impact parameter $\approx 2m$. Initial data are based on superposed, boosted (velocity $\approx 0.5c$) solutions of single black holes in Kerr-Schild coordinates. Both rotating and non-rotating black holes are considered. The excised regions containing the singularities are specified by following the dynamics of apparent horizons. Evolutions of up to $t\approx 35m$ are obtained in which two initially separate apparent horizons are present for $t\approx 3.8m$. At that time a single enveloping apparent horizon forms, indicating that the holes have merged. Apparent horizon area estimates suggest gravitational radiation of about 2.6% of the total mass. The evolutions end after a moderate amount of time because of instabilities.

2 References corrected, reference to figure updated