Deep-Learning continuous gravitational waves
Christoph Dreissigacker, Rahul Sharma, Chris Messenger, Ruining Zhao, and Reinhard Prix

TL;DR
This study explores using deep neural networks as a fast alternative to traditional methods for detecting continuous gravitational waves from neutron stars, showing promising results in certain scenarios.
Contribution
It introduces a convolutional neural network approach for CW detection and compares its performance to matched filtering, demonstrating its potential and limitations.
Findings
DNN achieves ~88% detection probability in easy cases
Detection probability drops to ~13% in harder scenarios
Few trained networks can generalize across the entire frequency range
Abstract
We present a first proof-of-principle study for using deep neural networks (DNNs) as a novel search method for continuous gravitational waves (CWs) from unknown spinning neutron stars. The sensitivity of current wide-parameter-space CW searches is limited by the available computing power, which makes neural networks an interesting alternative to investigate, as they are extremely fast once trained and have recently been shown to rival the sensitivity of matched filtering for black-hole merger signals. We train a convolutional neural network with residual (short-cut) connections and compare its detection power to that of a fully-coherent matched-filtering search using the WEAVE pipeline. As test benchmarks we consider two types of all-sky searches over the frequency range from to : an `easy' search using of data, and a `harder'…
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