Japanese large-scale interferometers

K. Kuroda; M. Ohashi; S. Miyoki; H. Ishizuka; C. T. Taylor; K. Yamamoto; O. Miyakawa; M. K. Fujimoto; S. Kawamura; R. Takahashi; T. Yamazaki; K. Arai; D. Tatsumi; A. Ueda; M. Fukushima; S. Sato; T. Shintomi; A. Yamamoto; T. Suzuki; Y. Saito; T. Haruyama; N. Sato; Y. Higashi; T. Uchiyama; T. Tomaru; K. Tsubono; M. Ando; A. Takamori; K. Numata; K. I. Ueda; H. Yoneda; K. Nakagawa; M. Musha; N. Mio; S. Moriwaki; K. Somiya; A. Araya; N. Kanda; S. Telada; M. Sasaki; H. Tagoshi; T. Nakamura; T. Tanaka; K. Ohara

doi:10.1088/0264-9381/19/7/302

Japanese large-scale interferometers

K. Kuroda^*, M. Ohashi, S. Miyoki, H. Ishizuka, C. T. Taylor, K. Yamamoto, O. Miyakawa, M. K. Fujimoto, S. Kawamura, R. Takahashi, T. Yamazaki, K. Arai, D. Tatsumi, A. Ueda, M. Fukushima, S. Sato, T. Shintomi, A. Yamamoto, T. Suzuki, Y. SaitoT. Haruyama, N. Sato, Y. Higashi, T. Uchiyama, T. Tomaru, K. Tsubono, M. Ando, A. Takamori, K. Numata, K. I. Ueda, H. Yoneda, K. Nakagawa, M. Musha, N. Mio, S. Moriwaki, K. Somiya, A. Araya, N. Kanda, S. Telada, M. Sasaki, H. Tagoshi, T. Nakamura, T. Tanaka, K. Ohara

^*この論文の責任著者

物理学科

研究成果: ジャーナルへの寄稿 › 学術論文 › 査読

27 被引用数 (Scopus)

抄録

The objective of the TAMA 300 interferometer was to develop advanced technologies for kilometre scale interferometers and to observe gravitational wave events in nearby galaxies. It was designed as a power-recycled Fabry-Perot-Michelson interferometer and was intended as a step towards a final interferometer in Japan. The present successful status of TAMA is presented. TAMA forms a basis for LCGT (large-scale cryogenic gravitational wave telescope), a 3 km scale cryogenic interferometer to be built in the Kamioka mine in Japan, implementing cryogenic mirror techniques. The plan of LCGT is schematically described along with its associated R&D.

本文言語	英語
ページ（範囲）	1237-1245
ページ数	9
ジャーナル	Classical and Quantum Gravity
巻	19
号	7
DOI	https://doi.org/10.1088/0264-9381/19/7/302
出版ステータス	出版済み - 2002/04/07

ASJC Scopus 主題領域

物理学および天文学（その他）

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10.1088/0264-9381/19/7/302

引用スタイル

Kuroda, K., Ohashi, M., Miyoki, S., Ishizuka, H., Taylor, C. T., Yamamoto, K., Miyakawa, O., Fujimoto, M. K., Kawamura, S., Takahashi, R., Yamazaki, T., Arai, K., Tatsumi, D., Ueda, A., Fukushima, M., Sato, S., Shintomi, T., Yamamoto, A., Suzuki, T., ... Ohara, K. (2002). Japanese large-scale interferometers. Classical and Quantum Gravity, 19(7), 1237-1245. https://doi.org/10.1088/0264-9381/19/7/302

@article{a005071069754eeab7cc01fdf2c17910,

title = "Japanese large-scale interferometers",

abstract = "The objective of the TAMA 300 interferometer was to develop advanced technologies for kilometre scale interferometers and to observe gravitational wave events in nearby galaxies. It was designed as a power-recycled Fabry-Perot-Michelson interferometer and was intended as a step towards a final interferometer in Japan. The present successful status of TAMA is presented. TAMA forms a basis for LCGT (large-scale cryogenic gravitational wave telescope), a 3 km scale cryogenic interferometer to be built in the Kamioka mine in Japan, implementing cryogenic mirror techniques. The plan of LCGT is schematically described along with its associated R&D.",

author = "K. Kuroda and M. Ohashi and S. Miyoki and H. Ishizuka and Taylor, {C. T.} and K. Yamamoto and O. Miyakawa and Fujimoto, {M. K.} and S. Kawamura and R. Takahashi and T. Yamazaki and K. Arai and D. Tatsumi and A. Ueda and M. Fukushima and S. Sato and T. Shintomi and A. Yamamoto and T. Suzuki and Y. Saito and T. Haruyama and N. Sato and Y. Higashi and T. Uchiyama and T. Tomaru and K. Tsubono and M. Ando and A. Takamori and K. Numata and Ueda, {K. I.} and H. Yoneda and K. Nakagawa and M. Musha and N. Mio and S. Moriwaki and K. Somiya and A. Araya and N. Kanda and S. Telada and M. Sasaki and H. Tagoshi and T. Nakamura and T. Tanaka and K. Ohara",

year = "2002",

month = apr,

day = "7",

doi = "10.1088/0264-9381/19/7/302",

language = "英語",

volume = "19",

pages = "1237--1245",

journal = "Classical and Quantum Gravity",

issn = "0264-9381",

publisher = "IOP Publishing Ltd.",

number = "7",

}

Kuroda, K, Ohashi, M, Miyoki, S, Ishizuka, H, Taylor, CT, Yamamoto, K, Miyakawa, O, Fujimoto, MK, Kawamura, S, Takahashi, R, Yamazaki, T, Arai, K, Tatsumi, D, Ueda, A, Fukushima, M, Sato, S, Shintomi, T, Yamamoto, A, Suzuki, T, Saito, Y, Haruyama, T, Sato, N, Higashi, Y, Uchiyama, T, Tomaru, T, Tsubono, K, Ando, M, Takamori, A, Numata, K, Ueda, KI, Yoneda, H, Nakagawa, K, Musha, M, Mio, N, Moriwaki, S, Somiya, K, Araya, A, Kanda, N, Telada, S, Sasaki, M, Tagoshi, H, Nakamura, T, Tanaka, T & Ohara, K 2002, 'Japanese large-scale interferometers', Classical and Quantum Gravity, vol. 19, no. 7, pp. 1237-1245. https://doi.org/10.1088/0264-9381/19/7/302

TY - JOUR

T1 - Japanese large-scale interferometers

AU - Kuroda, K.

AU - Ohashi, M.

AU - Miyoki, S.

AU - Ishizuka, H.

AU - Taylor, C. T.

AU - Yamamoto, K.

AU - Miyakawa, O.

AU - Fujimoto, M. K.

AU - Kawamura, S.

AU - Takahashi, R.

AU - Yamazaki, T.

AU - Arai, K.

AU - Tatsumi, D.

AU - Ueda, A.

AU - Fukushima, M.

AU - Sato, S.

AU - Shintomi, T.

AU - Yamamoto, A.

AU - Suzuki, T.

AU - Saito, Y.

AU - Haruyama, T.

AU - Sato, N.

AU - Higashi, Y.

AU - Uchiyama, T.

AU - Tomaru, T.

AU - Tsubono, K.

AU - Ando, M.

AU - Takamori, A.

AU - Numata, K.

AU - Ueda, K. I.

AU - Yoneda, H.

AU - Nakagawa, K.

AU - Musha, M.

AU - Mio, N.

AU - Moriwaki, S.

AU - Somiya, K.

AU - Araya, A.

AU - Kanda, N.

AU - Telada, S.

AU - Sasaki, M.

AU - Tagoshi, H.

AU - Nakamura, T.

AU - Tanaka, T.

AU - Ohara, K.

PY - 2002/4/7

Y1 - 2002/4/7

N2 - The objective of the TAMA 300 interferometer was to develop advanced technologies for kilometre scale interferometers and to observe gravitational wave events in nearby galaxies. It was designed as a power-recycled Fabry-Perot-Michelson interferometer and was intended as a step towards a final interferometer in Japan. The present successful status of TAMA is presented. TAMA forms a basis for LCGT (large-scale cryogenic gravitational wave telescope), a 3 km scale cryogenic interferometer to be built in the Kamioka mine in Japan, implementing cryogenic mirror techniques. The plan of LCGT is schematically described along with its associated R&D.

AB - The objective of the TAMA 300 interferometer was to develop advanced technologies for kilometre scale interferometers and to observe gravitational wave events in nearby galaxies. It was designed as a power-recycled Fabry-Perot-Michelson interferometer and was intended as a step towards a final interferometer in Japan. The present successful status of TAMA is presented. TAMA forms a basis for LCGT (large-scale cryogenic gravitational wave telescope), a 3 km scale cryogenic interferometer to be built in the Kamioka mine in Japan, implementing cryogenic mirror techniques. The plan of LCGT is schematically described along with its associated R&D.

UR - http://www.scopus.com/inward/record.url?scp=0036275897&partnerID=8YFLogxK

U2 - 10.1088/0264-9381/19/7/302

DO - 10.1088/0264-9381/19/7/302

M3 - 学術論文

AN - SCOPUS:0036275897

SN - 0264-9381

VL - 19

SP - 1237

EP - 1245

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 7

ER -

Japanese large-scale interferometers

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