# Real-Time Detection of Gravitational Waves from Binary Neutron Stars   using Artificial Neural Networks

**Authors:** Plamen G. Krastev (Harvard University)

arXiv: 1908.03151 · 2021-07-08

## TL;DR

This paper demonstrates that deep convolution neural networks can rapidly detect gravitational waves from binary neutron star mergers in noisy data, enabling real-time alerts for multi-messenger astrophysics.

## Contribution

It introduces a deep learning method trained on extensive data to identify neutron star merger signals in real-time, improving detection speed and accuracy over traditional techniques.

## Key findings

- Neural network achieves rapid detection in noisy data
- Distinguishes neutron star mergers from black hole signals
- Enables prompt multi-messenger follow-up observations

## Abstract

The groundbreaking discoveries of gravitational waves from binary black-hole mergers and, most recently, coalescing neutron stars started a new era of Multi-Messenger Astrophysics and revolutionized our understanding of the Cosmos. Machine learning techniques such as artificial neural networks are already transforming many technological fields and have also proven successful in gravitational-wave astrophysics for detection and characterization of gravitational-wave signals from binary black holes. Here we use a deep-learning approach to rapidly identify transient gravitational-wave signals from binary neutron star mergers in noisy time series representative of typical gravitational-wave detector data. Specifically, we show that a deep convolution neural network trained on 100,000 data samples can rapidly identify binary neutron star gravitational-wave signals and distinguish them from noise and signals from merging black hole binaries. These results demonstrate the potential of artificial neural networks for real-time detection of gravitational-wave signals from binary neutron star mergers, which is critical for a prompt follow-up and detailed observation of the electromagnetic and astro-particle counterparts accompanying these important transients.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1908.03151/full.md

## References

33 references — full list in the complete paper: https://tomesphere.com/paper/1908.03151/full.md

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Source: https://tomesphere.com/paper/1908.03151