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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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Uloženo v:
Hlavní autoři: 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
Médium: Artigo
Jazyk:Inglês
Vydáno: MDPI AG 2021-02-01
Edice:Galaxies
Témata:
gravitational waves
DECIGO
quantum noise
diffraction loss
On-line přístup:https://www.mdpi.com/2075-4434/9/1/14
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