Advances in Machine and Deep Learning for Modeling and Real-time Detection of Multi-Messenger Sources
E. A. Huerta, Zhizhen Zhao

TL;DR
This paper reviews recent advances in machine and deep learning techniques applied to multi-messenger astrophysics, highlighting their role in real-time detection and modeling of cosmic sources across various messengers.
Contribution
It provides a comprehensive overview of the evolution and integration of AI algorithms in multi-messenger astrophysics, emphasizing recent innovations and their impact.
Findings
Deep learning algorithms have significantly improved detection capabilities.
Integration of domain expertise enhances model performance.
Advancements enable real-time analysis of multi-messenger data.
Abstract
We live in momentous times. The science community is empowered with an arsenal of cosmic messengers to study the Universe in unprecedented detail. Gravitational waves, electromagnetic waves, neutrinos and cosmic rays cover a wide range of wavelengths and time scales. Combining and processing these datasets that vary in volume, speed and dimensionality requires new modes of instrument coordination, funding and international collaboration with a specialized human and technological infrastructure. In tandem with the advent of large-scale scientific facilities, the last decade has experienced an unprecedented transformation in computing and signal processing algorithms. The combination of graphics processing units, deep learning, and the availability of open source, high-quality datasets, have powered the rise of artificial intelligence. This digital revolution now powers a multi-billion…
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