Status of Japanese gravitational wave detectors

K. Arai; R. Takahashi; D. Tatsumi; K. Izumi; Y. Wakabayashi; H. Ishizaki; Mitsuhiro Fukushima; T. Yamazaki; M. K. Fujimoto; A. Takamori; K. Tsubono; R. Desalvo; A. Bertolini; S. Mrka; V. Sannibale; T. Uchiyama; O. Miyakawa; S. Miyoki; K. Agatsuma; T. Saito; M. Ohashi; K. Kuroda; I. Nakatani; S. Telada; K. Yamamoto; T. Tomaru; T. Suzuki; T. Haruyama; N. Sato; A. Yamamoto; T. Shintomi

doi:10.1088/0264-9381/26/20/204020

Status of Japanese gravitational wave detectors

K. Arai^*, R. Takahashi, D. Tatsumi, K. Izumi, Y. Wakabayashi, H. Ishizaki, Mitsuhiro Fukushima, T. Yamazaki, M. K. Fujimoto, A. Takamori, K. Tsubono, R. Desalvo, A. Bertolini, S. Mrka, V. Sannibale, T. Uchiyama, O. Miyakawa, S. Miyoki, K. Agatsuma, T. SaitoM. Ohashi, K. Kuroda, I. Nakatani, S. Telada, K. Yamamoto, T. Tomaru, T. Suzuki, T. Haruyama, N. Sato, A. Yamamoto, T. Shintomi

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

25 Citations (Scopus)

Abstract

The Large-scale Cryogenic Gravitational wave Telescope (LCGT) is planned as a future Japanese project for gravitational wave detection. A 3 km interferometer will be built in an underground mine at Kamioka. Cryogenic sapphire mirrors are going to be employed for the test masses. For the demonstration of LCGT technologies, two prototype interferometers, TAMA300 and CLIO, are being developed. This paper describes the current status of the LCGT project and the two prototype interferometers.

Original language	English
Article number	204020
Journal	Classical and Quantum Gravity
Volume	26
Issue number	20
DOIs	https://doi.org/10.1088/0264-9381/26/20/204020
Publication status	Published - 2009
Externally published	Yes

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

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10.1088/0264-9381/26/20/204020

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Arai, K., Takahashi, R., Tatsumi, D., Izumi, K., Wakabayashi, Y., Ishizaki, H., Fukushima, M., Yamazaki, T., Fujimoto, M. K., Takamori, A., Tsubono, K., Desalvo, R., Bertolini, A., Mrka, S., Sannibale, V., Uchiyama, T., Miyakawa, O., Miyoki, S., Agatsuma, K., ... Shintomi, T. (2009). Status of Japanese gravitational wave detectors. Classical and Quantum Gravity, 26(20), Article 204020. https://doi.org/10.1088/0264-9381/26/20/204020

Arai, K, Takahashi, R, Tatsumi, D, Izumi, K, Wakabayashi, Y, Ishizaki, H, Fukushima, M, Yamazaki, T, Fujimoto, MK, Takamori, A, Tsubono, K, Desalvo, R, Bertolini, A, Mrka, S, Sannibale, V, Uchiyama, T, Miyakawa, O, Miyoki, S, Agatsuma, K, Saito, T, Ohashi, M, Kuroda, K, Nakatani, I, Telada, S, Yamamoto, K, Tomaru, T, Suzuki, T, Haruyama, T, Sato, N, Yamamoto, A & Shintomi, T 2009, 'Status of Japanese gravitational wave detectors', Classical and Quantum Gravity, vol. 26, no. 20, 204020. https://doi.org/10.1088/0264-9381/26/20/204020

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title = "Status of Japanese gravitational wave detectors",

abstract = "The Large-scale Cryogenic Gravitational wave Telescope (LCGT) is planned as a future Japanese project for gravitational wave detection. A 3 km interferometer will be built in an underground mine at Kamioka. Cryogenic sapphire mirrors are going to be employed for the test masses. For the demonstration of LCGT technologies, two prototype interferometers, TAMA300 and CLIO, are being developed. This paper describes the current status of the LCGT project and the two prototype interferometers.",

author = "K. Arai and R. Takahashi and D. Tatsumi and K. Izumi and Y. Wakabayashi and H. Ishizaki and Mitsuhiro Fukushima and T. Yamazaki and Fujimoto, {M. K.} and A. Takamori and K. Tsubono and R. Desalvo and A. Bertolini and S. Mrka and V. Sannibale and T. Uchiyama and O. Miyakawa and S. Miyoki and K. Agatsuma and T. Saito and M. Ohashi and K. Kuroda and I. Nakatani and S. Telada and K. Yamamoto and T. Tomaru and T. Suzuki and T. Haruyama and N. Sato and A. Yamamoto and T. Shintomi",

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doi = "10.1088/0264-9381/26/20/204020",

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AU - Arai, K.

AU - Takahashi, R.

AU - Tatsumi, D.

AU - Izumi, K.

AU - Wakabayashi, Y.

AU - Ishizaki, H.

AU - Fukushima, Mitsuhiro

AU - Yamazaki, T.

AU - Fujimoto, M. K.

AU - Takamori, A.

AU - Tsubono, K.

AU - Desalvo, R.

AU - Bertolini, A.

AU - Mrka, S.

AU - Sannibale, V.

AU - Uchiyama, T.

AU - Miyakawa, O.

AU - Miyoki, S.

AU - Agatsuma, K.

AU - Saito, T.

AU - Ohashi, M.

AU - Kuroda, K.

AU - Nakatani, I.

AU - Telada, S.

AU - Yamamoto, K.

AU - Tomaru, T.

AU - Suzuki, T.

AU - Haruyama, T.

AU - Sato, N.

AU - Yamamoto, A.

AU - Shintomi, T.

PY - 2009

Y1 - 2009

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AB - The Large-scale Cryogenic Gravitational wave Telescope (LCGT) is planned as a future Japanese project for gravitational wave detection. A 3 km interferometer will be built in an underground mine at Kamioka. Cryogenic sapphire mirrors are going to be employed for the test masses. For the demonstration of LCGT technologies, two prototype interferometers, TAMA300 and CLIO, are being developed. This paper describes the current status of the LCGT project and the two prototype interferometers.

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JF - Classical and Quantum Gravity

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Status of Japanese gravitational wave detectors

Abstract

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