The future of gravitational wave science unlocking LIGO potential: AI-driven data analysis and exploration

TL;DR

This paper reviews how AI techniques, especially deep learning, are transforming gravitational wave data analysis by improving detection accuracy, efficiency, and enabling real-time exploration of cosmic events.

Contribution

It provides a comprehensive review of AI methods applied to gravitational wave data, highlighting recent advancements and future integration into GW detectors and analysis pipelines.

Findings

Deep learning outperforms other AI methods in detection accuracy.

Supervised learning enhances true positive rates and reduces false positives.

Unsupervised and reinforcement learning offer high efficiency for real-time applications.

Abstract

The advent of gravitational wave astronomy (GW) has revolutionized the observation of cataclysmic cosmic events, such as black hole mergers and neutron star collisions. The Laser Interferometer Gravitational-Wave Observatory (LIGO) has been at the forefront of these discoveries. However, the immense volume and complexity of gravitational wave data present significant challenges for traditional analysis methods. This paper investigates the growing synergy between artificial intelligence (AI) and GW science, emphasizing how AI enhances signal detection, noise reduction, and data interpretation. It begins with an overview of GW fundamentals and the role of machine learning in increasing detector sensitivity. Notable GW events observed by LIGO are discussed alongside persistent analytical challenges such as data quality, generalization, and computational constraints. A comprehensive performance review of AI techniques, including supervised learning, unsupervised learning, deep learning, and reinforcement learning, is presented based on data spanning 2021 to 2024. Evaluation metrics include accuracy, precision, true positive rate (TPR), false positive rate (FPR), and computational efficiency. Findings indicate that deep learning and supervised learning outperform other approaches, particularly in enhancing TPR and minimizing FPR. While unsupervised and reinforcement learning models offer less precision, they demonstrate high efficiency and potential for real-time applications. The study also explores AI integration into next-generation detectors and waveform reconstruction techniques. Overall, the integration of AI into GW research significantly improves the reliability and speed of event detection, unlocking new possibilities for exploring the dynamic universe. This paper provides a comprehensive outlook on the transformative role of AI in shaping the future of GW astronomy.