Asymmetric emission of gravitational waves during a compact binary coalescence results in the loss of linear momentum and a corresponding "kick" or recoil on the binary's center of mass. This leads to a direction-dependent Doppler shift of the ringdown gravitational waveform. We quantify the measurability of the kick imparted to the remnant black hole in a binary black hole merger. Future ground- and space-based gravitational-wave detectors will measure this effect to within ∼2% to ∼30% for a subset of their expected observed sources. Certain binary configurations in the LISA band may allow a sub-percent-level measurement of this effect. This direct measurement of black hole kicks can also facilitate a novel test of general relativity based on linear momentum balance. We formulate this kick consistency test via measurement of a null variable that quantifies the difference between the inferred kick (using numerical relativity) and that observed via the Doppler-shifted ringdown signal. This null variable can be constrained (at 90\% confidence) to ∼10% to 30% with Cosmic Explorer and to ∼3% to 12% with LISA.
@article{arxiv.2308.08319,
title = {Testing general relativity via direct measurement of black hole kicks},
author = {Parthapratim Mahapatra and Marc Favata and K. G. Arun},
journal= {arXiv preprint arXiv:2308.08319},
year = {2024}
}