Coherent injection of magnetic noise and its impact on gravitational-wave searches

Correlated noise sources, particularly magnetic noise, form a risk to future gravitational-wave searches aimed at detecting the gravitational-wave background. To investigate potential noise contamination, we project noise levels based on accurate measurements of how strongly the noise couples to the detector. To make these estimates, we inject, for the first time, broadband, coherent magnetic noise between two gravitational-wave detectors, LIGO Hanford and LIGO Livingston, separated by several thousands of kilometers. We describe the noise injection and its impact on the analysis pipelines, then investigate the accuracy of noise projection techniques used over the past decade. Finally, we present a proof-of-concept demonstration of noise subtraction using Wiener filtering, while also highlighting potential risks associated with this method. This unique dataset with correlated noise caused by magnetic field fluctuations in two gravitational-wave detectors, as well as in an array of witness sensors, provides an excellent testing ground for additional future studies. Ultimately, this study demonstrates that Wiener filtering is effective and can be applied in the eventual detection of the gravitational-wave background by the LIGO-Virgo-KAGRA Collaboration.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-11-12
DOI
https://doi.org/10.1103/hll9-qmtk
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
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article

Coherent injection of magnetic noise and its impact on gravitational-wave searches

T. O’Hanlon, K. Janssens, Max Lalleman, N. Van Remortel et al.
Physical review. D/Physical review. D.
Pulsars and Gravitational Waves Research
article

Coherent injection of magnetic noise and its impact on gravitational-wave searches

T. O’Hanlon, K. Janssens, Max Lalleman, N. Van Remortel, E. A. Quintero, N. Christensen, M. W. Coughlin, Jessica Lawrence, Jorge dos Reis, Adrian F. Helmling-Cornell, Joseph Betzwieser, Anamaria Effler, Jennifer C Driggers, R. M. S. Schofield
article en

Abstract

Correlated noise sources, particularly magnetic noise, form a risk to future gravitational-wave searches aimed at detecting the gravitational-wave background. To investigate potential noise contamination, we project noise levels based on accurate measurements of how strongly the noise couples to the detector. To make these estimates, we inject, for the first time, broadband, coherent magnetic noise between two gravitational-wave detectors, LIGO Hanford and LIGO Livingston, separated by several thousands of kilometers. We describe the noise injection and its impact on the analysis pipelines, then investigate the accuracy of noise projection techniques used over the past decade. Finally, we present a proof-of-concept demonstration of noise subtraction using Wiener filtering, while also highlighting potential risks associated with this method. This unique dataset with correlated noise caused by magnetic field fluctuations in two gravitational-wave detectors, as well as in an array of witness sensors, provides an excellent testing ground for additional future studies. Ultimately, this study demonstrates that Wiener filtering is effective and can be applied in the eventual detection of the gravitational-wave background by the LIGO-Virgo-KAGRA Collaboration.

Physical review. D/Physical review. D.Vol. 112(10)
Texas Tech University (US), University of Minnesota (US), University of Antwerp (BE), University of Oregon (US), Carleton College (US), Université Côte d'Azur (FR), LIGO Scientific Collaboration (US), University of Minnesota System (US), ARC Centre of Excellence for Dark Matter Particle Physics (AU), Observatoire de la Côte d’Azur (FR), The University of Adelaide (AU), Massachusetts Institute of Technology (US), Instituto Nacional de Pesquisas Espaciais (BR)
Openalex Percentile: Top 80%
Pulsars and Gravitational Waves Research
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