You only thermoelastically deform once: point absorber detection in LIGO test masses with YOLO

Current and future gravitational-wave observatories rely on large-scale, precision interferometers to detect the gravitational-wave signals. However, microscopic imperfections on the main interferometer mirrors, known as <i>point absorbers</i>, cause problematic heating of the optic via absorption of the high-power laser beam, which results in diminished sensitivity, loss of interferometer lock, or even permanent damage. Consistent monitoring of these mirrors is crucial for detecting, characterizing, and ultimately removing point absorbers. We present a machine-learning algorithm for detecting point absorbers based on the object-detection algorithm You Only Look Once (YOLO). The algorithm can perform this task in situ while the detector is in operation. We validate our algorithm by comparing it with past reports of point absorbers identified by humans at LIGO. The algorithm confidently identifies the same point absorbers as humans with minimal false positives. It also identifies some point absorbers previously not identified by humans, which we confirm with human follow-up. We highlight the potential of machine learning in detector commissioning efforts.

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Publication Details

Journal
Optics Express
Published
2025-04-03
DOI
https://doi.org/10.1364/oe.554989
Citations
1
Primary Topic
Geophysics and Gravity Measurements
Type
article
Field-Weighted Citation Impact
1.79
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article

You only thermoelastically deform once: point absorber detection in LIGO test masses with YOLO

P. D. Lasky, Daniel B. Brown, Simon Goode, M. G. Schiworski et al.
1 citations
Optics Express
Geophysics and Gravity Measurements
1.79
article

You only thermoelastically deform once: point absorber detection in LIGO test masses with YOLO

P. D. Lasky, Daniel B. Brown, Simon Goode, M. G. Schiworski, E. Thrane
article en
1 citations

Abstract

Current and future gravitational-wave observatories rely on large-scale, precision interferometers to detect the gravitational-wave signals. However, microscopic imperfections on the main interferometer mirrors, known as <i>point absorbers</i>, cause problematic heating of the optic via absorption of the high-power laser beam, which results in diminished sensitivity, loss of interferometer lock, or even permanent damage. Consistent monitoring of these mirrors is crucial for detecting, characterizing, and ultimately removing point absorbers. We present a machine-learning algorithm for detecting point absorbers based on the object-detection algorithm You Only Look Once (YOLO). The algorithm can perform this task in situ while the detector is in operation. We validate our algorithm by comparing it with past reports of point absorbers identified by humans at LIGO. The algorithm confidently identifies the same point absorbers as humans with minimal false positives. It also identifies some point absorbers previously not identified by humans, which we confirm with human follow-up. We highlight the potential of machine learning in detector commissioning efforts.

Optics ExpressVol. 33(8)
ARC Centre of Excellence for Gravitational Wave Discovery (AU), The University of Adelaide (AU), Syracuse University (US)
Openalex Percentile: Top 19%
Geophysics and Gravity Measurements
1.79
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You only thermoelastically deform once: point absorber detection in LIGO test masses with YOLO — P. D. Lasky, Daniel B. Brown, et al. · Optics Express (2025) | TGRS Research Map | TGRS