First Demonstration of Optical Feedback Control to Parametric Instability at Advanced LIGO

Increasing the circulating power in gravitational-wave detectors to the megawatt level is essential for future sensitivity improvement, but this is critically limited by optomechanical parametric instabilities.

Current mitigation strategies are projected to be inadequate against instabilities when circulating power reaches a megawatt.

Optical feedback offers a novel independent paradigm to mitigate parametric instability.

In this Letter, we report the first demonstration of optical feedback control in a full-scale gravitational wave detector.

We successfully suppressed an unstable mode at 10.428 kHz, reducing the parametric gain from R = 2 to R < 0.02.

This work validates optical feedback control as an effective mitigation scheme for kilometre-scale interferometric gravitational-wave detectors, providing an effective strategy to allow detectors to reach the megawatt level.