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; Mitsuhiro 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, Mitsuhiro 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

^*Corresponding author for this work

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

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.

Original language	English
Journal	Classical and Quantum Gravity
Volume	20
Issue number	17
DOIs	https://doi.org/10.1088/0264-9381/20/17/329
Publication status	Published - 2003 Sept 7
Externally published	Yes

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

Access to Document

10.1088/0264-9381/20/17/329

Cite this

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). https://doi.org/10.1088/0264-9381/20/17/329

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. https://doi.org/10.1088/0264-9381/20/17/329

@article{2fca4d844a804205b5c6bc081679784f,

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 Mitsuhiro 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 = "English",

volume = "20",

journal = "Classical and Quantum Gravity",

issn = "0264-9381",

publisher = "IOP Publishing Ltd.",

number = "17",

}

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, Mitsuhiro

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.

UR - http://www.scopus.com/inward/record.url?scp=0142137611&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0142137611&partnerID=8YFLogxK

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

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

M3 - Article

AN - SCOPUS:0142137611

SN - 0264-9381

VL - 20

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 17

ER -

Current status of large-scale cryogenic gravitational wave telescope

Abstract

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this