Black-hole kicks: a tool to measure the accuracy of gravitational-wave models

TL;DR

This paper proposes using black-hole recoil velocities, derived from gravitational waves, as a diagnostic tool to evaluate and improve the accuracy of waveform models in gravitational-wave astronomy.

Contribution

It introduces the concept of using black-hole kicks as a new method to test and enhance the precision of gravitational waveform models.

Findings

Black-hole kicks are highly sensitive to waveform inaccuracies.

Current higher-mode waveform models show inconsistencies in kick predictions.

Improving waveform accuracy could enable extraction of meaningful kick information from future observations.

Abstract

Asymmetric binary systems radiate linear momentum through gravitational waves, leading to the recoil of the merger remnant. Black-hole kicks have attracted much attention because of their astrophysical implications. However, little information can be extracted from the observations made by LIGO and Virgo so far. In this work, we discuss how the gravitational recoil, an effect that is encoded in the gravitational signal, can be used to test the accuracy of waveform models. Gravitational-wave models of merging binary systems have become fundamental to detect potential signals and infer the parameters of observed sources. But, as the interferometers' sensitivity is enhanced in current and future detectors, gravitational waveform models will have to be further improved. We find that the kick is highly sensitive to waveform inaccuracies and can therefore be a useful diagnostic test. Furthermore, we observe that current higher-mode waveform models are not consistent in their kick predictions. For this reason, we discuss whether measuring and improving waveform accuracy can, in turn, allow us to extract meaningful information about the kick in future observations.