Speaker
Tessa Baker
(Queen Mary University of London)
Description
Departures from General Relativity impact the propagation of gravitational waves (GW) in multiple ways. I’ll explain the theoretical underpinnings of these phenomena, and how they connect to potentially observable features of waveforms. I’ll review the current status of constraints on modified GW propagation, and outline how LISA and other detectors are expected to enhance these bounds.
Primary author
Tessa Baker
(Queen Mary University of London)
