Active controls in interferometric detectors of gravitational waves: inertial damping of the VIRGO superattenuator

TL;DR

This paper discusses the implementation of inertial damping control in the VIRGO gravitational wave detector's superattenuator to reduce mirror motion and improve interferometer stability.

Contribution

It introduces the inertial damping control technique for the VIRGO superattenuator, highlighting its role in stabilizing the suspended mirrors for gravitational wave detection.

Findings

Inertial damping effectively reduces mirror residual motion.

Improved control enhances interferometer locking stability.

The method is crucial for gravitational wave detection sensitivity.

Abstract

The operation of an interferometer for gravitational waves detection requires sophisticated feedback controls in many parts of the apparatus. The aim of this lecture is to introduce the types of problems to be faced in this line of research. The attention is focused on the "inertial damping" of the test mass suspension of the VIRGO interferometer (the superattenuator): it is a multidimensional local control aimed to reduce the residual motion of the suspended mirror associated to the normal modes of the suspension. Its performance is very important for the locking of the interferometer.