Speaker
Eleonora Capocasa
(APC)
Description
Detectors of the post-O5 era, as Virgo_nEXT and third generation detectors, as Einstein Telescope aim to achieve squeezing levels of the order of 10 dB. This implies a drastic reduction in optical losses, down to a level of a few percent. In this presentation, we will describe the study to reach these squeezing levels in the context of the Virgo_nEXT concept study, and the possible synergies with third-generation detectors, which aim at the same goals. In particular, we will illustrate possible avenues to reduce input and output losses, phase noise losses, filter cavity losses and interferometer losses.
Primary author
Eleonora Capocasa
(APC)
