The Japanese space gravitational wave antenna - DECIGO

被引：442

作者：

Kawamura, Seiji ^{[1
]}

Nakamura, Takashi

Ando, Masaki

Seto, Naoki

Tsubono, Kimio

Numata, Kenji

Takahashi, Ryuichi

Nagano, Shigeo

Ishikawa, Takehiko

Musha, Mitsuru

Ueda, Ken-ichi

Sato, Takashi

Hosokawa, Mizuhiko

Agatsuma, Kazuhiro

Akutsu, Tomotada

Aoyanagi, Koh-suke

Arai, Koji

Araya, Akito

Asada, Hideki

Aso, Yoichi

Chiba, Takeshi

Ebisuzaki, Toshikazu

Eriguchi, Yoshiharu

Fujimoto, Masa-Katsu

Fukushima, Mitsuhiro

Futamase, Toshifumi

Ganzu, Katsuhiko

Harada, Tomohiro

Hashimoto, Tatsuaki

Hayama, Kazuhiro

Hikida, Wataru

Himemoto, Yoshiaki

Hirabayashi, Hisashi

Hiramatsu, Takashi

Ichiki, Kiyotomo

Ikegami, Takeshi

Inoue, Kaiki T.

Ioka, Kunihito

Ishidoshiro, Koji

Itoh, Yousuke

Kamagasako, Shogo

Kanda, Nobuyuki

Kawashima, Nobuki

Kirihara, Hiroyuki

Kiuchi, Kenta

Kobayashi, Shiho

Kohri, Kazunori

Kojima, Yasufumi

Kokeyama, Keiko

Kozai, Yoshihide

机构：

[1] Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan

[2] Kyoto Univ, Grad Sch Sci, Kyoto 6068502, Japan

[3] Univ Tokyo, Grad Sch Sci, Bunkyo Ku, Tokyo 1130033, Japan

[4] CALTECH, Pasadena, CA 91125 USA

[5] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[6] Natl Inst Informat & Commun Technol, Koganei, Tokyo 1848795, Japan

[7] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Tsukuba, Ibaraki 3058505, Japan

[8] Univ Electrocommun, Inst Laser Sci, Chofu, Tokyo 1828585, Japan

[9] Niigata Univ, Fac Engn, Niigata 9502181, Japan

[10] Waseda Univ, Shinjuku Ku, Tokyo 1698555, Japan

[11] Univ Tokyo, Earthquake Res Inst, Bunkyo Ku, Tokyo 1130032, Japan

[12] Hirosaki Univ, Fac Sci & Technol, Hirosaki, Aomori 0368560, Japan

[13] Nihon Univ, Coll Humanities & Sci, Setagaya Ku, Tokyo 1568550, Japan

[14] RIKEN, Wako, Saitama 3510198, Japan

[15] Univ Tokyo, Grad Sch Arts & Sci, Meguro Ku, Tokyo 1538902, Japan

[16] Tohoku Univ, Grad Sch Sci, Sendai, Miyagi 9808578, Japan

[17] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan

[18] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan

[19] Natl Inst Adv Ind Sci & Technol, Tsukuba, Ibaraki 3058563, Japan

[20] Kinki Univ, Sch Sci & Engn, Osaka 5778502, Japan

[21] Univ Wisconsin, Milwaukee, WI 53201 USA

[22] Osaka City Univ, Grad Sch Sci, Osaka 5588585, Japan

[23] Liverpool John Moores Univ, Astrophys Res Inst, Birkenhead L41 1LD, Merseyside, England

[24] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[25] Hiroshima Univ, Grad Sch Sci, Hiroshima 7398526, Japan

[26] Ochanomizu Univ, Grad Sch Humanities & Sci, Bunkyo Ku, Tokyo 1128610, Japan

[27] Gunma Astron Observ, Gunma 3770702, Japan

[28] Natl Inst Informat & Commun Technol, Bunkyo Ku, Tokyo 1130001, Japan

[29] Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan

[30] Niigata Univ, Fac Sci, Niigata 9502181, Japan

[31] Kyoto Univ, Fac Intergrated Human Studies, Kyoto 6068501, Japan

[32] Osaka Univ, Grad Sch Sci, Toyonaka, Osaka 5600043, Japan

[33] Observ Paris, Sect Meudon, F-92195 Meudon, France

[34] INAMORI Fdn, Kyoto 6008411, Japan

[35] Max Planck Inst Gravitat Phys, D-14476 Potsdam, Germany

[36] Univ Illinois, Dept Phys, Urbana, IL 61801 USA

[37] Tokyo Inst Technol, Grad Sch Sci & Engn, Meguro Ku, Tokyo 1528550, Japan

来源：

CLASSICAL AND QUANTUM GRAVITY | 2006年 / 23卷 / 08期

关键词：

D O I：

10.1088/0264-9381/23/8/S17

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. It aims at detecting various kinds of gravitational waves between 1 mHz and 100 Hz frequently enough to open a new window of observation for gravitational wave astronomy. The preconceptual design of DECIGO consists of three drag-free satellites, 1000 km apart from each other, whose relative displacements are measured by a Fabry-Perot Michelson interferometer. We plan to launch DECIGO in 2024 after a long and intense development phase, including two pathfinder missions for verification of required technologies.

引用

页码：S125 / S131

页数：7

共 4 条

[1] The gravitational wave background from cosmological compact binaries [J].

Farmer, AJ ;

Phinney, ES .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2003, 346 (04) :1197-1214

[2] Japanese large-scale interferometers [J].

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 .

CLASSICAL AND QUANTUM GRAVITY, 2002, 19 (07) :1237-1245

[3]

*LISA, SYST TECHN STUD REP

[4] Possibility of direct measurement of the acceleration of the universe using 0.1 Hz band laser interferometer gravitational wave antenna in space [J].

Seto, N ;

Kawamura, S ;

Nakamura, T .

PHYSICAL REVIEW LETTERS, 2001, 87 (22) :221103-221103

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