In this talk, we will study the effect of gravitational waves (GWs) on the geodesic deviation of test masses in uniform circular motion. Using this as a detection principle, we will estimate the capacity of such a detector to detect and constrain astrophysical GW events. This includes analyzing the detector response signal, sensitivity curve, observational range, and parameter estimation capabilities. This talk is based on papers by Rao et al. - Phys. Rev. D 102, 122006 (2020) and arXiv:2301.08331 (2023).
Join the meeting here: Zoom link
Meeting ID: 921 1801 0804
Passcode: 68144845