First cryogenic test operation of underground km-scale gravitational-wave observatory KAGRA

T Akutsu, M Ando, K Arai, Y Arai, S Araki, A Araya, N Aritomi, H Asada, Y Aso, S Atsuta, K Awai, S Bae, L Baiotti, M A Barton, K Cannon, E Capocasa, C-S Chen, T-W Chiu, K Cho, Y-K Chu, K Craig, W Creus, K Doi, K Eda, Y Enomoto, R Flaminio, Y Fujii, M-K Fujimoto, M Fukunaga, M Fukushima, T Furuhata, A Hagiwara, S Haino, K Hasegawa, K Hashino, K Hayama, S Hirobayashi, E Hirose, B H Hsieh, C-Z Huang, B Ikenoue, Y Inoue, K Ioka, Y Itoh, K Izumi, T Kaji, T Kajita, M Kakizaki, M Kamiizumi, S Kanbara, N Kanda, S Kanemura, M Kaneyama, G Kang, J Kasuya, Y Kataoka, N Kawai, S Kawamura, T Kawasaki, C Kim, J Kim, J C Kim, W S Kim, Y-M Kim, N Kimura, T Kinugawa, S Kirii, Y Kitaoka, H Kitazawa, Y Kojima, K Kokeyama, K Komori, A K H Kong, K Kotake, R Kozu, R Kumar, H-S Kuo, S Kuroyanagi, H K Lee, H M Lee, H W Lee, M Leonardi, C-Y Lin, F-L Lin, G C Liu, Y Liu, E Majorana, S Mano, M Marchio, T Matsui, F Matsushima, Y Michimura, N Mio, O Miyakawa, A Miyamoto, T Miyamoto, K Miyo, S Miyoki, W Morii, S Morisaki, Y Moriwaki, T Morozumi, I Murakami, M Musha, K Nagano, S Nagano, K Nakamura, T Nakamura, H Nakano, M Nakano, K Nakao, Y Namai, T Narikawa, L Naticchioni, L Nguyen Quynh, W-T Ni, A Nishizawa, Y Obuchi, T Ochi, J J Oh, S H Oh, M Ohashi, N Ohishi, M Ohkawa, K Okutomi, K Ono, K Oohara, C P Ooi, S-S Pan, J Park, F E Peña Arellano, I Pinto, N Sago, M Saijo, Y Saito, S Saitou, K Sakai, Y Sakai, M Sasai, M Sasaki, Y Sasaki, N Sato, S Sato, T Sato, Y Sekiguchi, N Seto, M Shibata, T Shimoda, H Shinkai, T Shishido, A Shoda, K Somiya, E J Son, A Suemasa, T Suzuki, H Tagoshi, H Tahara, H Takahashi, R Takahashi, A Takamori, H Takeda, H Tanaka, K Tanaka, T Tanaka, S Tanioka, E N Tapia San Martin, D Tatsumi, S Terashima, T Tomaru, T Tomura, F Travasso, K Tsubono, S Tsuchida, N Uchikata, T Uchiyama, A Ueda, T Uehara, S Ueki, K Ueno, F Uraguchi, T Ushiba, M H P M van Putten, H Vocca, S Wada, T Wakamatsu, Y Watanabe, W-R Xu, T Yamada, A Yamamoto, K Yamamoto, S Yamamoto, T Yamamoto, K Yokogawa, J Yokoyama, T Yokozawa, T H Yoon, T Yoshioka, H Yuzurihara, S Zeidler, Z-H Zhu

doi:10.48550/arxiv.1901.03569

書誌事項

公開日: 2019-07-23

資源種別: journal article

権利情報

https://publishingsupport.iopscience.iop.org/iop-standard/v1
https://iopscience.iop.org/info/page/text-and-data-mining

DOI

10.1088/1361-6382/ab28a9
10.48550/arxiv.1901.03569

公開者: IOP Publishing

説明

<jats:title>Abstract</jats:title> <jats:p> KAGRA is a second-generation interferometric gravitational-wave detector with 3 km arms constructed at Kamioka, Gifu, Japan. It is now in its final installation phase, which we call <jats:italic>bKAGRA</jats:italic> (baseline KAGRA), with scientific observations expected to begin in late 2019. One of the advantages of KAGRA is its underground location of at least 200 m below the ground surface, which reduces seismic motion at low frequencies and increases the stability of the detector. Another advantage is that it cools down the sapphire test mass mirrors to cryogenic temperatures to reduce thermal noise. In April–May 2018, we operated a 3 km Michelson interferometer with a cryogenic test mass for 10 d, which was the first time that km-scale interferometer was operated at cryogenic temperatures. In this article, we report the results of this ‘bKAGRA Phase 1’ operation. We have demonstrated the feasibility of 3 km interferometer alignment and control with cryogenic mirrors. </jats:p>

収録刊行物

Classical and Quantum Gravity

Classical and Quantum Gravity 36 (16), 165008-, 2019-07-23

IOP Publishing

キーワード

詳細情報詳細情報について

書き出し

問題の指摘

First cryogenic test operation of underground km-scale gravitational-wave observatory KAGRA

書誌事項

この論文をさがす

説明

収録刊行物

被引用文献 (26)*注記

参考文献 (33)*注記

関連プロジェクト

関連未分類成果物

キーワード

詳細情報詳細情報について

書き出し

問題の指摘

First cryogenic test operation of underground km-scale gravitational-wave observatory KAGRA

書誌事項

この論文をさがす

説明

収録刊行物

被引用文献 (26)*注記

参考文献 (33)*注記

関連プロジェクト

関連未分類成果物

キーワード

詳細情報 詳細情報について

書き出し

問題の指摘

詳細情報詳細情報について