Improvement of the Target Sensitivity in DECIGO by Optimizing its Parameters for Quantum Noise Including the Effect of Diffraction Loss

Improvement of the Target Sensitivity in DECIGO by Optimizing its Parameters for Quantum Noise Including the Effect of Diffraction Loss

The DECi-hertz Interferometer Gravitational-wave Observatory (DECIGO) is the future Japanese, outer space gravitational wave detector. We previously set the default design parameters to provide a good target sensitivity to detect the primordial gravitational waves (GWs). However, the updated upper l...

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Bibliographic Details
Main Authors: Tomohiro Ishikawa, Shoki Iwaguchi, Yuta Michimura, Masaki Ando, Rika Yamada, Izumi Watanabe, Koji Nagano, Tomotada Akutsu, Kentaro Komori, Mitsuru Musha, Takeo Naito, Taigen Morimoto, Seiji Kawamura
Format: Article
Language:English
Published: MDPI AG 2021-02-01
Series:Galaxies
Subjects:
gravitational waves
DECIGO
quantum noise
diffraction loss
Online Access:https://www.mdpi.com/2075-4434/9/1/14

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https://www.mdpi.com/2075-4434/9/1/14

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