Better early than never: A new test for superluminal gravitational wave polarizations

TL;DR

This paper introduces a novel method to detect superluminal gravitational wave polarizations that arrive before the standard modes, providing a new test for theories beyond Einstein's gravity.

Contribution

It proposes a new technique to identify superluminal, non-transverse-traceless polarizations in gravitational wave data, expanding the toolkit for testing gravity theories.

Findings

The new test can potentially detect superluminal polarizations.

Current detectors are capable of implementing this test.

Constraints can be placed if superluminal polarizations are not observed.

Abstract

In some beyond-Einstein theories of gravity, gravitational waves can contain up to six polarizations, which are allowed to propagate at different speeds faster than light. These different propagation speeds imply that polarizations generated by the same source will not arrive simultaneously at the detector. Current constraints on the speed of propagation of transverse-traceless polarizations, however, indicate that any additional polarizations must arrive with or before the transverse-traceless ones. We propose a new technique to test for the existence of superluminal, non-transverse-traceless polarizations that arrive in the data before a gravitational-wave observation of transverse-traceless modes. We discuss the circumstances in which these non-transverse-traceless polarizations would be detectable and what constraints could be placed if they are not detected. To determine whether this new test of general relativity with gravitational wave observations is practical, we outline and address many of the challenges it might face. Our arguments lead us to conclude that this new test is not only physically well-motivated but also feasible with current detectors.