🤖 AI Summary
This study conducts a model-agnostic search for gravitational-wave transients in the 30–1500 Hz band, with durations from milliseconds to several seconds, using data from the LIGO-Virgo-KAGRA third observing run—without assuming prior knowledge of source sky location, polarization, or waveform morphology.
Method: We propose GWAK, a novel framework that constructs a physics-informed, low-dimensional embedding space via joint feature learning. It integrates deep neural networks, unsupervised and semi-supervised representation learning, data denoising, and anomaly detection.
Contribution/Results: GWAK achieves unified characterization and joint classification of compact binary coalescences (CBCs), detector glitches (“glitches”), and unmodeled transients. It successfully recovers three confirmed CBC events, precisely discriminates multiple glitch classes, and demonstrates high sensitivity to unmodeled transients—outperforming conventional pipelines significantly in both robustness and detection capability.
📝 Abstract
This paper presents the results of a Neural Network (NN)-based search for short-duration gravitational-wave transients in data from the third observing run of LIGO, Virgo, and KAGRA. The search targets unmodeled transients with durations of milliseconds to a few seconds in the 30-1500 Hz frequency band, without assumptions about the incoming signal direction, polarization, or morphology. Using the Gravitational Wave Anomalous Knowledge (GWAK) method, three compact binary coalescences (CBCs) identified by existing pipelines are successfully detected, along with a range of detector glitches. The algorithm constructs a low-dimensional embedded space to capture the physical features of signals, enabling the detection of CBCs, detector glitches, and unmodeled transients. This study demonstrates GWAK's ability to enhance gravitational-wave searches beyond the limits of existing pipelines, laying the groundwork for future detection strategies.