Optimization of Design Parameters for Gravitational Wave Detector DECIGO Including Fundamental Noises

Optimization of Design Parameters for Gravitational Wave Detector DECIGO Including Fundamental Noises

The DECi-hertz Interferometer Gravitational-Wave Observatory (DECIGO) is a space gravitational wave (GW) detector. DECIGO was originally designed to be sensitive enough to observe primordial GW background (PGW). However, due to the lowered upper limit of the PGW by the Planck observation, further im...

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Bibliographic Details
Main Authors: Yuki Kawasaki, Ryuma Shimizu, Tomohiro Ishikawa, Koji Nagano, Shoki Iwaguchi, Izumi Watanabe, Bin Wu, Shuichiro Yokoyama, Seiji Kawamura
Format: Article
Language:English
Published: MDPI AG 2022-02-01
Series:Galaxies
Subjects:
gravitational waves
DECIGO
thermal noise
quantum noise
diffraction loss
Online Access:https://www.mdpi.com/2075-4434/10/1/25

Internet

https://www.mdpi.com/2075-4434/10/1/25

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