학술논문

Input optics systems of the KAGRA detector during O3GK
Document Type
Academic Journal
Author
Akutsu, T.Ando, M.Arai, K.Arai, Y.Araki, S.Araya, A.Aritomi, N.Asada, H.Aso, Y.Bae, S.Bae, Y.Baiotti, L.Bajpai, R.Barton, M.A.Cannon, K.Cao, Z.Capocasa, E.Chan, M.Chen, C.Chen, K.Chen, Y.Chiang, C-I.Chu, H.Chu, Y-K.Eguchi, S.Enomoto, Y.Flaminio, R.Fujii, Y.Fujikawa, Y.Fukunaga, M.Fukushima, M.Furuhata, T.Gao, D.Ge, G.-G.Ha, S.Hagiwara, A.Haino, S.Han, W.-B.Hasegawa, K.Hattori, K.Hayakawa, H.Hayama, K.Himemoto, Y.Hiranuma, Y.Hirata, N.Hirose, E.Hong, Z.Hsieh, B-H.Huang, G-Z.Huang, H-Y.Huang, P.Huang, Y-C.Huang, Y.-J.Hui, D.C.Y.Ide, S.Ikenoue, B.Imam, S.Inayoshi, K.Inoue, Y.Ioka, K.Ito, K.Itoh, Y.Izumi, K.Jeon, C.Jin, H.-B.Jung, K.Jung, P.Kaihotsu, K.Kajita, T.Kakizaki, M.Kamiizumi, M.Kanbara, S.Kanda, N.Kang, G.Kataoka, Y.Kawaguchi, K.Kawai, N.Kawasaki, T.Kim, C.Kim, J.Kim, J.C.Kim, W.S.Kim, Y.-M.Kimura, N.Kita, N.Kitazawa, H.Kojima, Y.Kokeyama, K.Komori, K.Kong, A.K.H.Kotake, K.Kozaka, C.Kozu, R.Kumar, R.Kume, J.Kuo, C.Kuo, H-S.Kuromiya, Y.Kuroyanagi, S.Kusayanagi, K.Kwak, K.Lee, H.K.Lee, H.W.Lee, R.Leonardi, M.Li, K.L.Lin, L.C.-C.Lin, C-Y.Lin, F-K.Lin, F-L.Lin, H.L.Liu, G.C.Luo, L.-W.Majorana, E.Marchio, M.Michimura, Y.Mio, N.Miyakawa, O.Miyamoto, A.Miyazaki, Y.Miyo, K.Miyoki, S.Mori, Y.Morisaki, S.Moriwaki, Y.Nagano, K.Nagano, S.Nakamura, K.Nakano, H.Nakano, M.Nakashima, R.Nakayama, Y.Narikawa, T.Naticchioni, L.Negishi, R.Quynh, L. NguyenNi, W.-T.Nishizawa, A.Nozaki, S.Obuchi, Y.Ogaki, W.Oh, J.J.Oh, K.Oh, S.H.Ohashi, M.Ohishi, N.Ohkawa, M.Ohta, H.Okutani, Y.Okutomi, K.Oohara, K.Ooi, C.Oshino, S.Otabe, S.Pan, K.-C.Pang, H.Parisi, A.Park, J.Arellano, F.E. PenaPinto, I.Sago, N.Saito, S.Saito, Y.Sakai, K.Sakai, Y.Sakuno, Y.Sato, S.Sato, T.Sawada, T.Sekiguchi, T.Sekiguchi, Y.Shao, L.Shibagaki, S.Shimizu, R.Shimoda, T.Shimode, K.Shinkai, H.Shishido, T.Shoda, A.Somiya, K.Son, E.J.Sotani, H.Sugimoto, R.Suresh, J.Suzuki, T.Tagoshi, H.Takahashi, H.Takahashi, R.Takamori, A.Takano, S.Takeda, H.Takeda, M.Tanaka, H.Tanaka, K.Tanaka, T.Tanioka, S.Martin, E.N. Tapia SanTelada, S.Tomaru, T.Tomigami, Y.Tomura, T.Travasso, F.Trozzo, L.Tsang, T.Tsao, J-S.Tsubono, K.Tsuchida, S.Tsutsui, T.Tsuzuki, T.Tuyenbayev, D.Uchikata, N.Uchiyama, T.Ueda, A.Uehara, T.Ueno, K.Ueshima, G.Uraguchi, F.Ushiba, T.Putten, M.H.P.M. vanVocca, H.Wang, J.Washimi, T.Wu, C.Wu, H.Wu, S.Xu, W-R.Yamada, T.Yamamoto, K.Yamamoto, T.Yamashita, K.Yamazaki, R.Yang, Y.Yano, K.Yokogawa, K.Yokoyama, J.Yokozawa, T.Yoshioka, T.Yuzurihara, H.Zeidler, S.Zhan, M.Zhang, H.Zhao, Y.Zhu, Z.-H.Goetz, R.Heintze, M.Liu, J.Muller, C.Savage, R.L.Tanner, D.B.
Source
Progress of Theoretical and Experimental Physics. February, 2023, Vol. 2023 Issue 2, p1c, 20 p.
Subject
Taiwan
South Korea
Japan
China
Language
English
Abstract
KAGRA, the underground and cryogenic gravitational-wave detector, was operated for its solo observation from February 25 to March 10, 2020, and its first joint observation with the GEO 600 detector from April 7 to April 21, 2020 (O3GK). This study presents an overview of the input optics systems of the KAGRA detector, which consist of various optical systems, such as a laser source, its intensity and frequency stabilization systems, modulators, a Faraday isolator, mode-matching telescopes, and a high-power beam dump. These optics were successfully delivered to the KAGRA interferometer and operated stably during the observations. The laser frequency noise was observed to limit the detector sensitivity above a few kilohertz, whereas the laser intensity did not significantly limit the detector sensitivity. Subject Index F30
1. Introduction Approximately 100 years after Einstein predicted gravitational waves (GWs) as a consequence of general relativity, two advanced laser interferometer gravitational-wave observatory (aLIGO) detectors observed a binary black hole [...]