Gravitational Recoil during Binary Black Hole Coalescence using the Effective One Body Approach
Thibault Damour, Achamveedu Gopakumar

TL;DR
This paper uses the Effective One Body approach to estimate the gravitational recoil velocity during binary black hole coalescence, highlighting the importance of a momentum flux burst before merger and providing a range of recoil velocities with uncertainties.
Contribution
It introduces a method to compute recoil velocities during black hole mergers using the EOB approach, including a new estimate for the maximum recoil and analysis of uncertainties.
Findings
Maximum recoil velocity ~74 km/s for certain mass ratios.
Recoil velocities range between 49 and 172 km/s depending on assumptions.
A key momentum flux burst occurs just before coalescence.
Abstract
Using the Effective One Body approach, that includes nonperturbative resummed estimates for the damping and conservative parts of the compact binary dynamics, we compute the recoil during the late inspiral and the subsequent plunge of non-spinning black holes of comparable masses moving in quasi-circular orbits. Further, using a prescription that smoothly connects the plunge phase to a perturbed single black hole, we obtain an estimate for the total recoil associated with the binary black hole coalescence. We show that the crucial physical feature which determines the magnitude of the terminal recoil is the presence of a ``burst'' of linear momentum flux emitted slightly before coalescence. When using the most natural expression for the linear momentum flux during the plunge, together with a Taylor-expanded correction factor, we find that the maximum value of the terminal…
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