Effective Field Theory for Compact Object Evolution in Newtonian Non-Relativistic General Relativity

Abstract: In this talk, we review some of the tools to model compact objects with effective field theory to study their numerical evolution in the late inspiral before merging or disrupting. We show that by adding Newtonian effects such as spin, tidal and dissipative effects in addition to gravitational wave radiation, the contribution to the phase evolution in the gravitational waveform is significant in order to match the coefficients of the theory from gravitational wave observations and constrain fundamental physics.

general relativity and quantum cosmologyHEP - theory

Audience: researchers in the discipline

QGaSLAB Seminar Series

Series comments: The webinar can be joined via zoom.us/j/260447387?pwd=VnRMWVhuM0xiNCtxcEtpZjZ3ZHdYUT09

Meeting ID: 260 447 387 Password: qgas01