Akiyama, Y, Akutsu, T, Ando, M, Arai, K, Arai, Y, Araki, S, Araya, A, Aritomi, N, Asada, H, Aso, Y, Bae, S, Baiotti, L, Barton, M A, Cannon, K, Capocasa, E, Chen, C-S, Chiu, T-W, Cho, K, Chu, Y-K, Craig, K, Dattilo, V, Doi, K, Enomoto, Y, Flaminio, R, Fujii, Y, Fujimoto, M-K, Fukunaga, M, Fukushima, M, Furuhata, T, Haino, S, Hasegawa, K, Hashimoto, Y, Hashino, K, Hayama, K, Hirayama, T, Hirose, E, Hsieh, B H, Huang, C-Z, Ikenoue, B, Inoue, Y, Ioka, K, Itoh, Y, Izumi, K, Kaji, T, Kajita, T, Kakizaki, M, Kamiizumi, M, Kanbara, S, Kanda, N, Kanemura, S, Kang, G, Kasuya, J, Kawai, N, Kawasaki, T, Kim, C, Kim, W S, Kim, J, Kim, J C, Kimura, N, Kirii, S, Kitaoka, Y, Kitazawa, H, Kojima, Y, Kokeyama, K ![]() |
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Abstract
A vibration isolation system called the Type-Bp system used for power recycling mirrors has been developed for KAGRA, the interferometric gravitational-wave observatory in Japan. A suspension of the Type-Bp system passively isolates an optic from seismic vibration using three main pendulum stages equipped with two vertical vibration isolation systems. A compact reaction mass around each of the main stages allows for achieving sufficient damping performance with a simple feedback as well as vibration isolation ratio. Three Type-Bp systems were installed in KAGRA, and were proved to satisfy the requirements on the damping performance, and also on estimated residual displacement of the optics.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Publisher: | IOP Publishing |
ISSN: | 0264-9381 |
Date of First Compliant Deposit: | 19 March 2021 |
Date of Acceptance: | 14 March 2019 |
Last Modified: | 14 Nov 2024 13:15 |
URI: | https://orca.cardiff.ac.uk/id/eprint/139926 |
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