Theory-agnostic searches for non-gravitational modes in black hole ringdown

TL;DR

This paper introduces a theory-agnostic method to detect non-gravitational modes in black hole ringdown signals, which could reveal new physics beyond General Relativity with future high-sensitivity gravitational wave detectors.

Contribution

It proposes a novel, model-independent test for nongravitational modes in black hole mergers, applicable to current and future gravitational wave data, enhancing the search for new fundamental physics.

Findings

No evidence for extra modes in GW150914, GW190521, GW200129

Including extra modes affects the inferred remnant spin distribution

Future detectors can detect modes with very low amplitude ratios

Abstract

In any extension of General Relativity (GR), extra fundamental degrees of freedom couple to gravity. Besides deforming GR forecasts in a theory-dependent way, this coupling generically introduces extra modes in the gravitational-wave signal. We propose a novel theory-agnostic test of gravity to search for these nongravitational modes in black hole merger ringdown signals. To leading order in the GR deviations, their frequencies and damping times match those of a test scalar or vector field in a Kerr background, with only amplitudes and phases as free parameters. By applying this test to GW150914, GW190521, and GW200129, we find no strong evidence for an extra mode; however, its inclusion modifies the inferred distribution of the remnant spin. This test will be applicable for future detectors, which will achieve signal-to-noise ratios higher than 100 (and as high as 1000 for space-based detectors such as LISA). Such sensitivity will allow measurement of these modes with amplitude ratios as low as 0.02 for ground-based detectors (and as low as 0.003 for LISA), relative to the fundamental mode, enabling stringent agnostic constraints or detection of scalar/vector modes.