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Construction of KAGRA: an underground gravitational-wave observatory

Authors
Akutsu, T.Ando, M.Araki, S.Araya, A.Arima, T.Aritomi, N.Asada, H.Aso, Y.Atsuta, S.Awai, K.Baiotti, L.Barton, M. A.Chen, D.Cho, K.Craig, K.DeSalvo, R.Doi, K.Eda, K.Enomoto, Y.Flaminio, R.Fujibayashi, S.Fujii, Y.Fujimoto, M. -K.Fukushima, M.Furuhata, T.Hagiwara, A.Haino, S.Harita, S.Hasegawa, K.Hasegawa, M.Hashino, K.Hayama, K.Hirata, N.Hirose, E.Ikenoue, B.Inoue, Y.Ioka, K.Ishizaki, H.Itoh, Y.Jia, D.Kagawa, T.Kaji, T.Kajita, T.Kakizaki, M.Kakuhata, H.Kamiizumi, M.Kanbara, S.Kanda, N.Kanemura, S.Kaneyama, M.Kasuya, J.Kataoka, Y.Kawaguchi, K.Kawai, N.Kawamura, S.Kawazoe, F.Kim, C.Kim, J.Kim, J. C.Kim, W.Kimura, N.Kitaoka, Y.Kobayashi, K.Kojima, Y.Kokeyama, K.Komori, K.Kotake, K.Kubo, K.Kumar, R.Kume, T.Kuroda, K.Kuwahara, Y.Lee, H. -K.Lee, H. -W.Lin, C. -Y.Liu, Y.Majorana, E.Mano, S.Marchio, M.Matsui, T.Matsumoto, N.Matsushima, F.Michimura, Y.Mio, N.Miyakawa, O.Miyake, K.Miyamoto, A.Miyamoto, T.Miyo, K.Miyoki, S.Morii, W.Morisaki, S.Moriwaki, Y.Muraki, Y.Murakoshi, M.Musha, M.Nagano, K.Nagano, S.Nakamura, K.Nakamura, T.Nakano, H.Nakano, M.Nakano, M.Nakao, H.Nakao, K.Narikawa, T.Ni, W. -T.Nonomura, T.Obuchi, Y.Oh, J. J.Oh, S. -H.Ohashi, M.Ohishi, N.Ohkawa, M.Ohmae, N.Okino, K.Okutomi, K.Ono, K.Ono, Y.Oohara, K.Ota, S.Park, J.Pena Arellano, F. E.Pinto, I. M.Principe, M.Sago, N.Saijo, M.Saito, T.Saito, Y.Saitou, S.Sakai, K.Sakakibara, Y.Sasaki, Y.Sato, S.Sato, T.Sato, Y.Sekiguchi, T.Sekiguchi, Y.Shibata, M.Shiga, K.Shikano, Y.Shimoda, T.Shinkai, H.Shoda, A.Someya, N.Somiya, K.Son, E. J.Starecki, T.Suemasa, A.Sugimoto, Y.Susa, Y.Suwabe, H.Suzuki, T.Tachibana, Y.Tagoshi, H.Takada, S.Takahashi, H.Takahashi, R.Takamori, A.Takeda, H.Tanaka, H.Tanaka, K.Tanaka, T.Tatsumi, D.Telada, S.Tomaru, T.Tsubono, K.Tsuchida, S.Tsukada, L.Tsuzuki, T.Uchikata, N.Uchiyama, T.Uehara, T.Ueki, S.Ueno, K.Uraguchi, F.Ushiba, T.van Putten, M. H. P. M.Wada, S.Wakamatsu, T.Yaginuma, T.Yamamoto, K.Yamamoto, S.Yamamoto, T.Yano, K.Yokoyama, J.Yokozawa, T.Yoon, T. H.Yuzurihara, H.Zeidler, S.Zhao, Y.Zheng, L.Agatsuma, K.Akiyama, Y.Arai, N.Asano, M.Bertolini, A.Fujisawa, M.Goetz, R.Guscott, J.Hashimoto, Y.Hayashida, Y.Hennes, E.Hirai, K.Hirayama, T.Ishitsuka, H.Kato, J.Khalaidovski, A.Koike, S.Kumeta, A.Miener, T.Morioka, M.Mueller, C. L.Narita, T.Oda, Y.Ogawa, T.Sekiguchi, T.Tamura, H.Tanner, D. B.Tokoku, C.Toritani, M.Utsuki, T.Uyeshima, M.van den Brand, J. F. J.van Heijningen, J. V.Yamaguchi, S.Yanagida, A.
Issue Date
1월-2018
Publisher
OXFORD UNIV PRESS INC
Citation
PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS, v.2018, no.1
Indexed
SCIE
SCOPUS
Journal Title
PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS
Volume
2018
Number
1
URI
https://scholar.korea.ac.kr/handle/2021.sw.korea/131816
DOI
10.1093/ptep/ptx180
ISSN
2050-3911
Abstract
The major construction and initial-phase operation of a second-generation gravitational-wave detector, KAGRA, has been completed. The entire 3 km detector is installed underground in a mine in order to be isolated from background seismic vibrations on the surface. This allows us to achieve a good sensitivity at low frequencies and high stability of the detector. Bare-bones equipment for the interferometer operation has been installed and the first test run was accomplished in March and April of 2016 with a rather simple configuration. The initial configuration of KAGRA is called iKAGRA. In this paper, we summarize the construction of KAGRA, including a study of the advantages and challenges of building an underground detector, and the operation of the iKAGRA interferometer together with the geophysics interferometer that has been constructed in the same tunnel.
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