Deep Residual Networks for Gravitational Wave Detection
Paraskevi Nousi, Alexandra E. Koloniari, Nikolaos Passalis, Panagiotis, Iosif, Nikolaos Stergioulas, Anastasios Tefas

TL;DR
This paper introduces a deep residual neural network approach for gravitational wave detection that outperforms traditional methods in sensitivity and computational efficiency, especially for complex black hole binary signals.
Contribution
The paper presents a novel deep residual network architecture combined with normalization, data augmentation, and curriculum learning for improved gravitational wave detection.
Findings
Surpasses traditional detection sensitivity in specific scenarios.
Reduces computational cost significantly compared to matched filtering.
Effective in real LIGO O3a noise samples.
Abstract
Traditionally, gravitational waves are detected with techniques such as matched filtering or unmodeled searches based on wavelets. However, in the case of generic black hole binaries with non-aligned spins, if one wants to explore the whole parameter space, matched filtering can become impractical, which sets severe restrictions on the sensitivity and computational efficiency of gravitational-wave searches. Here, we use a novel combination of machine-learning algorithms and arrive at sensitive distances that surpass traditional techniques in a specific setting. Moreover, the computational cost is only a small fraction of the computational cost of matched filtering. The main ingredients are a 54-layer deep residual network (ResNet), a Deep Adaptive Input Normalization (DAIN), a dynamic dataset augmentation, and curriculum learning, based on an empirical relation for the signal-to-noise…
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Taxonomy
TopicsPulsars and Gravitational Waves Research
