Quantum Noise in a Fabry-Perot Interferometer Including the Influence of Diffraction Loss of Light

Quantum Noise in a Fabry-Perot Interferometer Including the Influence of Diffraction Loss of Light

The DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is designed to detect gravitational waves at frequencies between 0.1 and 10 Hz. In this frequency band, one of the most important science targets is the detection of primordial gravitational waves. DECIGO plans to use a space inte...

Full description

Bibliographic Details
Main Authors: Shoki Iwaguchi, Tomohiro Ishikawa, Masaki Ando, Yuta Michimura, Kentaro Komori, Koji Nagano, Tomotada Akutsu, Mitsuru Musha, Rika Yamada, Izumi Watanabe, Takeo Naito, Taigen Morimoto, Seiji Kawamura
Format: Article
Language:English
Published: MDPI AG 2021-01-01
Series:Galaxies
Subjects:
diffraction loss
fabry-perot cavity
quantum noise
Online Access:https://www.mdpi.com/2075-4434/9/1/9

Internet

https://www.mdpi.com/2075-4434/9/1/9

Similar Items