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arXiv · 2003.13202

Optimization of quantum noise by completing the square of multiple interferometer outputs in quantum locking for gravitational wave detectors

Rika Yamada·Yutaro Enomoto·Atsushi Nishizawa·Koji Nagano·Sachiko Kuroyanagi·Keiko Kokeyama·Kentaro Komori·Yuta Michimura·Takeo Naito·Izumi Watanabe·Taigen Morimoto·Masaki Ando·Akira Furusawa·Seiji Kawamura
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Abstract

The quantum locking technique, which uses additional short low-loss sub-cavities, is effective in reducing quantum noise in space gravitational wave antenna DECIGO. However, the quantum noise of the main interferometer depends on the control systems in the sub-cavities. Here we demonstrate a new method to optimize the quantum noise independently of the feedback gain by completing the square in the quantum locking system. We successfully demonstrate in simulations that this method is effective in optimizing the homodyne angle to the best quantum-noise-limited sensitivity.

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Rika Yamada, Yutaro Enomoto, Atsushi Nishizawa, Koji Nagano, Sachiko Kuroyanagi, Keiko Kokeyama, Kentaro Komori, Yuta Michimura, Takeo Naito, Izumi Watanabe, Taigen Morimoto, Masaki Ando, Akira Furusawa, Seiji Kawamura. 2020-12-21. Optimization of quantum noise by completing the square of multiple interferometer outputs in quantum locking for gravitational wave detectors. https://doi.org/10.1016/j.physleta.2020.126626

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