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

^*この研究の対応する著者

研究成果: Article › 査読

25 被引用数 (Scopus)

抄録

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.

本文言語	English
論文番号	204020
ジャーナル	Classical and Quantum Gravity
巻	26
号	20
DOI	https://doi.org/10.1088/0264-9381/26/20/204020
出版ステータス	Published - 2009
外部発表	はい

ASJC Scopus subject areas

物理学および天文学（その他）

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10.1088/0264-9381/26/20/204020

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引用スタイル

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), 記事 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

@article{2204aca5eeda4359b166b5b310193837,

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",

year = "2009",

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

language = "English",

volume = "26",

journal = "Classical and Quantum Gravity",

issn = "0264-9381",

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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

N2 - 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.

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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SN - 0264-9381

VL - 26

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 20

M1 - 204020

ER -

Status of Japanese gravitational wave detectors

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