A Machine Learning Application in Multi-Messenger Astrophysics
Offered By: Institute for Pure & Applied Mathematics (IPAM) via YouTube
Course Description
Overview
Explore a 45-minute conference talk on machine learning applications in multi-messenger astrophysics, presented by Irene Di Palma from Sapienza University of Rome. Delve into the challenges of detecting gravitational waves from core-collapse supernova explosions and learn about a novel method using machine learning techniques. Discover how this approach was tested by injecting signals into real noise data from the Advanced LIGO-Virgo network during the O2 observation run. Gain insights into the improved efficiency of signal classification and detection, with the potential to identify events up to 14 kpc away. Understand the importance of connecting multiple messengers, including neutrinos and electromagnetic signals, in advancing our understanding of these cosmic phenomena.
Syllabus
Irene Di Palma - A Machine Learning Application in Multi-Messenger Astrophysics - IPAM at UCLA
Taught by
Institute for Pure & Applied Mathematics (IPAM)
Related Courses
LIGO - Virgo & the Promise of Multi-Messenger ObservationsAPS Physics via YouTube Global Cyberinfrastructure for LIGO, Virgo, Kagra, IceCube, and Others
Institute for Pure & Applied Mathematics (IPAM) via YouTube Low-Latency Noise Mitigation Techniques in Gravitational-Wave Detector Data Using Auxiliary Sensor Information
Institute for Pure & Applied Mathematics (IPAM) via YouTube Computational Challenges in Gravitational Wave Parameter Estimation - IPAM at UCLA
Institute for Pure & Applied Mathematics (IPAM) via YouTube Rapidly Searching for Continuous Gravitational Waves
Institute for Pure & Applied Mathematics (IPAM) via YouTube