The Advanced Virgo plus status

The gravitational wave detector Advanced Virgo+ is currently in the commissioning phase in view of the fourth Observing Run (O4). The major upgrades with respect to the Advanced Virgo configuration are the implementation of an additional recycling cavity, the Signal Recycling cavity (SRC), at the output of the interferometer to broaden the sensitivity band and the Frequency Dependent Squeezing (FDS) to reduce quantum noise at all frequencies. The main difference of the Advanced Virgo + detector with respect to the LIGO detectors is the presence of marginally stable recycling cavities, with respect to the stable recycling cavities present in the LIGO detectors, which increases the difficulties in controlling the interferometer in presence of defects (both thermal and cold defects). This work will focus on the interferometer commissioning, highlighting the control challenges to maintain the detector in the working point which maximizes the sensitivity and the duty cycle for scientific data taking.

Automated summary

The gravitational wave detector Advanced Virgo+ is currently in the commissioning phase for the fourth Observing Run (O4). It includes major upgrades such as the addition of a Signal Recycling cavity (SRC) to broaden sensitivity band and the implementation of Frequency Dependent Squeezing (FDS) to reduce quantum noise at all frequencies. The Advanced Virgo+ detector has marginally stable recycling cavities, which differs from the stable recycling cavities in the LIGO detectors, leading to increased difficulties in controlling the interferometer in the presence of defects. This work focuses on the challenges in commissioning the interferometer to maximize sensitivity and duty cycle for scientific data taking.