[논문]An arm length stabilization system for KAGRA and future gravitational-wave detectors

Akutsu, T; Ando, M; Arai, K; Arai, K; Arai, Y; Araki, S; Araya, A; Aritomi, N; Aso, Y; Bae, S; Bae, Y; Baiotti, L; Bajpai, R; Barton, M A; Cannon, K; Capocasa, E; Chan, M; Chen, C S; Chen, K; Chen, Y; Chu, H; Chu, Y-K; Doi, K; Eguchi, S; Enomoto, Y; Flaminio, R; Fujii, Y; Fukunaga, M; Fukushima, M; Ge, G-G; Hagiwara, A; Haino, S; Hasegawa, K; Hayakawa, H; Hayama, K; Himemoto, Y; Hiranuma, Y; Hirata, N; Hirose, E; Hong, Z; Hsieh, B H; Huang, G-Z; Huang, P-W; Huang, Y; Ikenoue, B; Imam, S; Inayoshi, K; Inoue, Y; Ioka, K; Itoh, Y; Izumi, K; Jung, K; Jung, P; Kajita, T; Kamiizumi, M; Kanbara, S; Kanda, N; Kang, G; Kawaguchi, K; Kawai, N; Kawasaki, T; Kim, C; 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; Kozakai, C; Kozu, R; Kumar, R; Kume, J; Kuo, C; Kuo, H-S; Kuroyanagi, S; Kusayanagi, K; Kwak, K; Lee, H K; Lee, H W; Lee, R; Leona

doi:10.1088/1361-6382/ab5c95

[해외논문] An arm length stabilization system for KAGRA and future gravitational-wave detectors 원문보기

Classical and quantum gravity, v.37 no.3, 2020년, pp.035004 -

Akutsu, T (Gravitational Wave Project Office, National Astronomical Observatory of Japan (NAOJ), Mitaka City, Tokyo 181-8588, Japan) , Ando, M (Gravitational Wave Project Office, National Astronomical Observatory of Japan (NAOJ), Mitaka City, Tokyo 181-8588, Japan) , Arai, K (California Institute of Technology, Pasadena, CA 91125, United States of America) , Arai, K (Institute for Cosmic Ray Research (ICRR), KAGRA Observatory, The University of Tokyo, Kashiwa City, Chiba 277-8582, Japan) , Arai, Y (Institute for Cosmic Ray Research (ICRR), KAGRA Observatory, The University of Tokyo, Kashiwa City, Chiba 277-8582, Japan) , Araki, S (Accelerator Laboratory, High Energy Accelerator Research Organization (KEK), Tsukuba City, Ibaraki 305-0801, Japan) , Araya, A (Earthquake Research Institute, The University of Tokyo, Bunkyo-ku, Tokyo 113-0032, Japan) , Aritomi, N (Department of Physics, The University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan) , Aso, Y (Kamioka Branch, National Astronomical Observatory of Japan (NAOJ), Kamioka-cho, Hida City, Gifu 506-1205, Japan) , Bae, S (Korea Institute of) , Bae, Y , Baiotti, L , Bajpai, R , Barton, M A , Cannon, K , Capocasa, E , Chan, M , Chen, C S , Chen, K , Chen, Y , Chu, H , Chu, Y-K , Doi, K , Eguchi, S , Enomoto, Y , Flaminio, R , Fujii, Y , Fukunaga, M , Fukushima, M , Ge, G-G , Hagiwara, A , Haino, S , Hasegawa, K , Hayakawa, H , Hayama, K , Himemoto, Y , Hiranuma, Y , Hirata, N , Hirose, E , Hong, Z , Hsieh, B H , Huang, G-Z , Huang, P-W , Huang, Y , Ikenoue, B , Imam, S , Inayoshi, K , Inoue, Y , Ioka, K , Itoh, Y , Izumi, K , Jung, K , Jung, P , Kajita, T , Kamiizumi, M , Kanbara, S , Kanda, N , Kang, G , Kawaguchi, K , Kawai, N , Kawasaki, T , Kim, C , 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 , Kozakai, C , Kozu, R , Kumar, R , Kume, J , Kuo, C , Kuo, H-S , Kuroyanagi, S , Kusayanagi, K , Kwak, K , Lee, H K , Lee, H W , Lee, R , Leona

Abstract ▼ AI-Helper

Modern ground-based gravitational wave (GW) detectors require a complex interferometer configuration with multiple coupled optical cavities. Since achieving the resonances of the arm cavities is the most challenging among the lock acquisition processes, the scheme called arm length stabilization (ALS) had been employed for lock acquisition of the arm cavities. We designed a new type of the ALS, which is compatible with the interferometers having long arms like the next generation GW detectors. The features of the new ALS are that the control configuration is simpler than those of previous ones and that it is not necessary to lay optical fibers for the ALS along the kilometer-long arms of the detector. Along with simulations of its noise performance, an experimental test of the new ALS was performed utilizing a single arm cavity of KAGRA. This paper presents the first results of the test where we demonstrated that lock acquisition of the arm cavity was achieved using the new ALS. We also demonstrated that the root mean square of residual noise was measured to be 8.2 Hz in units of frequency, which is smaller than the linewidth of the arm cavity and thus low enough to lock the full interferometer of KAGRA in a repeatable and reliable manner.

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