Gravitational-Wave Geodesy: A New Tool for Validating Detection of the Stochastic Gravitational-Wave Background

TL;DR

This paper introduces gravitational-wave geodesy, a novel method to validate the detection of the stochastic gravitational-wave background by ensuring observed signals align with detector geometry, helping to distinguish true signals from terrestrial noise.

Contribution

The paper presents a new technique called gravitational-wave geodesy that uses background observations to verify detector signals match known geometries, reducing false positives.

Findings

Successfully validated true gravitational-wave background observations.

Effectively rejected terrestrial and spurious correlated signals.

Demonstrated method's potential for improving detection confidence.

Abstract

A valuable target for advanced gravitational-wave detectors is the stochastic gravitational-wave background. The stochastic background imparts a weak correlated signal into networks of gravitational-wave detectors, and so standard searches for the gravitational-wave background rely on measuring cross-correlations between pairs of widely-separated detectors. Stochastic searches, however, can be affected by any other correlated effects which may also be present, including correlated frequency combs and magnetic Schumann resonances. As stochastic searches become sensitive to ever-weaker signals, it is increasingly important to develop methods to separate a true astrophysical signal from other spurious and/or terrestrial signals. Here, we describe a novel method to achieve this goal -- gravitational-wave geodesy. Just as radio geodesy allows for the localization of radio telescopes, so too can observations of the gravitational-wave background be used to infer the positions and orientations of gravitational-wave detectors. By demanding that a true observation of the gravitational-wave background yield constraints consistent with the baseline's known geometry, we demonstrate that we can successfully validate true observations of the gravitational-wave background while rejecting spurious signals due to correlated terrestrial effects.