Abstract: The era of gravitational wave science began in spectacular fashion with several detections already reported by the LIGO-Virgo-KAGRA collaboration, and many more yet to come with the future planned observatories such as LISA and the Einstein Telescope. Motivated by these initial experimental breakthroughs and the expected scientific output, a community effort has been established toward constructing high-accurate waveform models for the emission of gravitational waves from binary systems. In this talk I review how ideas and techniques from particle physics — such as effective field theory methods and modern integration techniques from collider physics — have impacted the state-of-the-art in our analytic understanding of the two-body problem in general relativity.
Precision Gravity: From the LHC to LISA and ET
Perex