학술논문

The status of KAGRA underground cryogenic gravitational wave telescope
Document Type
Working Paper
Author
KAGRA CollaborationAkutsu, T.Ando, M.Araya, A.Aritomi, N.Asada, H.Aso, Y.Atsuta, S.Awai, K.Barton, M. A.Cannon, K.Craig, K.Creus, W.Doi, K.Eda, K.Enomoto, Y.Flaminio, R.Fujii, Y.Fujimoto, M. -K.Furuhata, T.Haino, S.Hasegawa, K.Hashino, K.Hayama, K.Hirobayashi, S.Hirose, E.Hsieh, B. H.Inoue, Y.Ioka, K.Itoh, Y.Kaji, T.Kajita, T.Kakizaki, M.Kamiizumi, M.Kambara, S.Kanda, N.Kanemura, S.Kaneyama, M.Kang, G.Kasuya, J.Kataoka, Y.Kawai, N.Kawamura, S.Kim, C.Kim, H.Kim, J.Kim, Y.Kimura, N.Kinugawa, T.Kirii, S.Kitaoka, Y.Kojima, Y.Kokeyama, K.Komori, K.Kotake, K.Kumar, R.Lee, H.Liu, Y.Luca, N.Majorana, E.Mano, S.Marchio, M.Matsui, T.Matsushima, F.Michimura, Y.Miyakawa, O.Miyamoto, T.Miyamoto, A.Miyo, K.Miyoki, S.Morii, W.Morisaki, S.Moriwaki, Y.Morozumi, T.Musha, M.Nagano, S.Nagano, K.Nakamura, K.Nakamura, T.Nakano, H.Nakano, M.Nakao, K.Narikawa, T.Quynh, L. NguyenNi, W. -T.Ochi, T.Oh, J.Oh, S.Ohashi, M.Ohishi, N.Ohkawa, M.Okutomi, K.Oohara, K.Alleano, F. E. PeñaPinto, I.Sago, N.Saijo, M.Saito, Y.Sakai, K.Sakai, Y.Sasaki, Y.Sasaki, M.Sato, S.Sato, T.Sekiguchi, Y.Seto, N.Shibata, M.Shimoda, T.Shinkai, H.Shoda, A.Somiya, K.Son, E.Suemasa, A.Suzuki, T.Tagoshi, H.Takahashi, H.Takahashi, R.Takamori, A.Takeda, H.Tanaka, H.Tanaka, K.Tanaka, T.Tatsumi, D.Tomaru, T.Tomura, T.Travasso, F.Tsubono, K.Tsuchida, S.Uchikata, N.Uchiyama, T.Uehara, T.Ueki, S.Ueno, K.Ushiba, T.van Putten, M. H. P. M.Vocca, H.Wada, S.Wakamatsu, T.Yamada, T.Yamamoto, S.Yamamoto, T.Yamamoto, K.Yamamoto, A.Yokoyama, J.Yokozawa, T.Yoon, T. H.Yuzurihara, H.Zeidler, S.Zhu, Z. -H.
Source
J. Phys.: Conf. Ser. 1342, 012014 (2020)
Subject
General Relativity and Quantum Cosmology
Astrophysics - Instrumentation and Methods for Astrophysics
Physics - Instrumentation and Detectors
Language
Abstract
KAGRA is a 3-km interferometric gravitational wave telescope located in the Kamioka mine in Japan. It is the first km-class gravitational wave telescope constructed underground to reduce seismic noise, and the first km-class telescope to use cryogenic cooling of test masses to reduce thermal noise. The construction of the infrastructure to house the interferometer in the tunnel, and the initial phase operation of the interferometer with a simple 3-km Michelson configuration have been completed. The first cryogenic operation is expected in 2018, and the observing runs with a full interferometer are expected in 2020s. The basic interferometer configuration and the current status of KAGRA are described.
Comment: 7 pages, 2 figures. Proceedings for XV International Conference on Topics in Astroparticle and Underground Physics (TAUP2017), Sudbury, July 24-28, 2017