A machine learning approach for gravitational waves searches associated with pulsar glitches
In gravitational-wave research, machine learning approaches sometimes struggle to match the sensitivities achieved in optimized pipelines. However, certain areas in gravitational-wave astrophysics pose challenges for conventional methods due to high computational costs or imprecise signal models. In these instances, machine learning emerges as promising avenue, offering a feasible approach. In this presentation, I will first explain the case of gravitational waves searches for glitching pulsars, and then I will focus into a pilot study using convolutional neural networks to analyze them. The study is built upon Albus, a machine-learning algorithm developed originally for minute-long gravitational wave burst. By showcasing this research, the poster aims to highlight the immediate prospects of machine learning as viable approach in unlocking new realms of discovery withing gravitational-wave and pulsar astrophysics.
Institutions
- Max Planck Institute for Gravitational Physics (DE)
- Fundació Universitat-Empresa de les Illes Balears (ES)
- Universitat de les Illes Balears (ES)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2025-03-13
- DOI
- https://doi.org/10.5281/zenodo.15019490
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00