Current status of large-scale cryogenic gravitational wave telescope

K. Kuroda; M. Ohashi; S. Miyoki; T. Uchiyama; H. Ishitsuka; K. Yamamoto; K. Kasahara; M. K. Fujimoto; S. Kawamura; R. Takahashi; T. Yamazaki; K. Arai; D. Tatsumi; A. Ueda; M. Fukushima; S. Sato; S. Nagano; Y. Tsunesada; Zong Hong Zhu; T. Shintomi; A. Yamamoto; T. Suzuki; Y. Saito; T. Haruyama; N. Sato; Y. Higashi; T. Tomaru; K. Tsubono; M. Ando; A. Takamori; K. Numata; Y. Aso; K. I. Ueda; H. Yoneda; K. Nakagawa; M. Musha; N. Mio; S. Moriwaki; K. Somiya; A. Araya; N. Kanda; S. Telada; H. Tagoshi; T. Nakamura; M. Sasaki; T. Tanaka; K. Oohara; H. Takahashi; O. Miyakawa; M. E. Tobar

doi:10.1088/0264-9381/20/17/329

Current status of large-scale cryogenic gravitational wave telescope

K. Kuroda^*, M. Ohashi, S. Miyoki, T. Uchiyama, H. Ishitsuka, K. Yamamoto, K. Kasahara, M. K. Fujimoto, S. Kawamura, R. Takahashi, T. Yamazaki, K. Arai, D. Tatsumi, A. Ueda, M. Fukushima, S. Sato, S. Nagano, Y. Tsunesada, Zong Hong Zhu, T. ShintomiA. Yamamoto, T. Suzuki, Y. Saito, T. Haruyama, N. Sato, Y. Higashi, T. Tomaru, K. Tsubono, M. Ando, A. Takamori, K. Numata, Y. Aso, K. I. Ueda, H. Yoneda, K. Nakagawa, M. Musha, N. Mio, S. Moriwaki, K. Somiya, A. Araya, N. Kanda, S. Telada, H. Tagoshi, T. Nakamura, M. Sasaki, T. Tanaka, K. Oohara, H. Takahashi, O. Miyakawa, M. E. Tobar

^*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

30 被引用数 (Scopus)

抄録

The large-scale cryogenic gravitational wave telescope (LCGT) project is the proposed advancement of TAMA, which will be able to detect the coalescences of binary neutron stars occurring in our galaxy. LCGT intends to detect the coalescence events within about 240 Mpc, the rate of which is expected to be from 0.1 to several events in a year. LCGT has Fabry-Perot cavities of 3 km baseline and the mirrors are cooled down to a cryogenic temperature of 20 K. It is planned to be built in the underground of Kamioka mine. This paper overviews the revision of the design and the current status of the R&D.

本文言語	英語
ページ（範囲）	S871-S884
ジャーナル	Classical and Quantum Gravity
巻	20
号	17
DOI	https://doi.org/10.1088/0264-9381/20/17/329
出版ステータス	出版済み - 2003/09/07

ASJC Scopus 主題領域

物理学および天文学（その他）

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10.1088/0264-9381/20/17/329

引用スタイル

Kuroda, K., Ohashi, M., Miyoki, S., Uchiyama, T., Ishitsuka, H., Yamamoto, K., Kasahara, K., Fujimoto, M. K., Kawamura, S., Takahashi, R., Yamazaki, T., Arai, K., Tatsumi, D., Ueda, A., Fukushima, M., Sato, S., Nagano, S., Tsunesada, Y., Zhu, Z. H., ... Tobar, M. E. (2003). Current status of large-scale cryogenic gravitational wave telescope. Classical and Quantum Gravity, 20(17), S871-S884. https://doi.org/10.1088/0264-9381/20/17/329

@article{c04cd735fbb642ae92ed24395ac59f4d,

title = "Current status of large-scale cryogenic gravitational wave telescope",

abstract = "The large-scale cryogenic gravitational wave telescope (LCGT) project is the proposed advancement of TAMA, which will be able to detect the coalescences of binary neutron stars occurring in our galaxy. LCGT intends to detect the coalescence events within about 240 Mpc, the rate of which is expected to be from 0.1 to several events in a year. LCGT has Fabry-Perot cavities of 3 km baseline and the mirrors are cooled down to a cryogenic temperature of 20 K. It is planned to be built in the underground of Kamioka mine. This paper overviews the revision of the design and the current status of the R&D.",

author = "K. Kuroda and M. Ohashi and S. Miyoki and T. Uchiyama and H. Ishitsuka and K. Yamamoto and K. Kasahara 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 S. Nagano and Y. Tsunesada and Zhu, {Zong Hong} and T. Shintomi and A. Yamamoto and T. Suzuki and Y. Saito and T. Haruyama and N. Sato and Y. Higashi and T. Tomaru and K. Tsubono and M. Ando and A. Takamori and K. Numata and Y. Aso 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 H. Tagoshi and T. Nakamura and M. Sasaki and T. Tanaka and K. Oohara and H. Takahashi and O. Miyakawa and Tobar, {M. E.}",

year = "2003",

month = sep,

day = "7",

doi = "10.1088/0264-9381/20/17/329",

language = "英語",

volume = "20",

pages = "S871--S884",

journal = "Classical and Quantum Gravity",

issn = "0264-9381",

publisher = "IOP Publishing Ltd.",

number = "17",

}

Kuroda, K, Ohashi, M, Miyoki, S, Uchiyama, T, Ishitsuka, H, Yamamoto, K, Kasahara, K, Fujimoto, MK, Kawamura, S, Takahashi, R, Yamazaki, T, Arai, K, Tatsumi, D, Ueda, A, Fukushima, M, Sato, S, Nagano, S, Tsunesada, Y, Zhu, ZH, Shintomi, T, Yamamoto, A, Suzuki, T, Saito, Y, Haruyama, T, Sato, N, Higashi, Y, Tomaru, T, Tsubono, K, Ando, M, Takamori, A, Numata, K, Aso, Y, Ueda, KI, Yoneda, H, Nakagawa, K, Musha, M, Mio, N, Moriwaki, S, Somiya, K, Araya, A, Kanda, N, Telada, S, Tagoshi, H, Nakamura, T, Sasaki, M, Tanaka, T, Oohara, K, Takahashi, H, Miyakawa, O & Tobar, ME 2003, 'Current status of large-scale cryogenic gravitational wave telescope', Classical and Quantum Gravity, vol. 20, no. 17, pp. S871-S884. https://doi.org/10.1088/0264-9381/20/17/329

TY - JOUR

T1 - Current status of large-scale cryogenic gravitational wave telescope

AU - Kuroda, K.

AU - Ohashi, M.

AU - Miyoki, S.

AU - Uchiyama, T.

AU - Ishitsuka, H.

AU - Yamamoto, K.

AU - Kasahara, K.

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 - Nagano, S.

AU - Tsunesada, Y.

AU - Zhu, Zong Hong

AU - Shintomi, T.

AU - Yamamoto, A.

AU - Suzuki, T.

AU - Saito, Y.

AU - Haruyama, T.

AU - Sato, N.

AU - Higashi, Y.

AU - Tomaru, T.

AU - Tsubono, K.

AU - Ando, M.

AU - Takamori, A.

AU - Numata, K.

AU - Aso, Y.

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 - Tagoshi, H.

AU - Nakamura, T.

AU - Sasaki, M.

AU - Tanaka, T.

AU - Oohara, K.

AU - Takahashi, H.

AU - Miyakawa, O.

AU - Tobar, M. E.

PY - 2003/9/7

Y1 - 2003/9/7

N2 - The large-scale cryogenic gravitational wave telescope (LCGT) project is the proposed advancement of TAMA, which will be able to detect the coalescences of binary neutron stars occurring in our galaxy. LCGT intends to detect the coalescence events within about 240 Mpc, the rate of which is expected to be from 0.1 to several events in a year. LCGT has Fabry-Perot cavities of 3 km baseline and the mirrors are cooled down to a cryogenic temperature of 20 K. It is planned to be built in the underground of Kamioka mine. This paper overviews the revision of the design and the current status of the R&D.

AB - The large-scale cryogenic gravitational wave telescope (LCGT) project is the proposed advancement of TAMA, which will be able to detect the coalescences of binary neutron stars occurring in our galaxy. LCGT intends to detect the coalescence events within about 240 Mpc, the rate of which is expected to be from 0.1 to several events in a year. LCGT has Fabry-Perot cavities of 3 km baseline and the mirrors are cooled down to a cryogenic temperature of 20 K. It is planned to be built in the underground of Kamioka mine. This paper overviews the revision of the design and the current status of the R&D.

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U2 - 10.1088/0264-9381/20/17/329

DO - 10.1088/0264-9381/20/17/329

M3 - 学術論文

AN - SCOPUS:0142137611

SN - 0264-9381

VL - 20

SP - S871-S884

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 17

ER -

Current status of large-scale cryogenic gravitational wave telescope

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