Physics-inspired spatiotemporal-graph AI ensemble for the detection of higher order wave mode signals of spinning binary black hole mergers
Minyang Tian, E.A. Huerta, Huihuo Zheng, Prayush Kumar

TL;DR
This paper introduces a novel AI ensemble combining dilated convolutional and graph neural networks for detecting higher order gravitational wave modes from spinning binary black hole mergers, achieving state-of-the-art performance.
Contribution
It presents a new spatiotemporal-graph AI model that effectively captures both temporal and spatial features for gravitational wave detection, trained on synthetic data and applied to real observation data.
Findings
Achieved state-of-the-art detection performance with minimal false positives.
Processed a decade of gravitational wave data in 3.5 hours using supercomputing resources.
Detected 6 gravitational waves in the O3b LIGO/Virgo data with high accuracy.
Abstract
We present a new class of AI models for the detection of quasi-circular, spinning, non-precessing binary black hole mergers whose waveforms include the higher order gravitational wave modes , and mode mixing effects in the harmonics. These AI models combine hybrid dilated convolution neural networks to accurately model both short- and long-range temporal sequential information of gravitational waves; and graph neural networks to capture spatial correlations among gravitational wave observatories to consistently describe and identify the presence of a signal in a three detector network encompassing the Advanced LIGO and Virgo detectors. We first trained these spatiotemporal-graph AI models using synthetic noise, using 1.2 million modeled waveforms to densely sample this signal manifold, within 1.7 hours using 256 A100…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Model Reduction and Neural Networks
MethodsDilated Convolution · Convolution
