Speaker
Eleonora Capocasa
(National Astronomical Observatory of Japan)
Description
The generation of frequency dependent squeezing with ~100 scale filter cavities is a promising technique to obtain a broadband quantum noise mitigation in 2nd generation GW detectors and its implementation is planned in their near-term upgrade. At NAOJ, we are developing a 300 m filter cavity prototype in order to demonstrate squeezing angle rotation below 100 Hz, as required for an optimal noise reduction. The update on the experiment will be presented.
Primary authors
Koji Arai
Yoichi Aso
Matteo Barsuglia
Eleonora Capocasa
(National Astronomical Observatory of Japan)
Marc Eisenmann
Flaminio Raffaele
Yuefan Guo
Matteo Leonardi
Naoki Aritomi
Pierre Prat
Roman Schnabel
Emil Schreiber
Kentaro Somiya
Matteo Tacca
Ryutaro Takahashi
Akihiro Tomura
Marco Vardaro
Yuhang Zhao
