Abstract
A space gravitational-wave antenna, DECIGO (DECI-hertz interferometer Gravitational wave Observatory), will provide fruitful insights into the universe, particularly on the formation mechanism of supermassive black holes, dark energy and the inflation of the universe. In the current pre-conceptual design, DECIGO will be comprising four interferometer units; each interferometer unit will be formed by three drag-free spacecraft with 1000 km separation. Since DECIGO will be an extremely challenging mission with high-precision formation flight with long baseline, it is important to increase the technical feasibility before its planned launch in 2027. Thus, we are planning to launch two milestone missions. DECIGO pathfinder (DPF) is the first milestone mission, and key components for DPF are being tested on ground and in orbit. In this paper, we review the conceptual design and current status of DECIGO and DPF.
Original language | English |
---|---|
Article number | 084010 |
Journal | Classical and Quantum Gravity |
Volume | 27 |
Issue number | 8 |
DOIs | |
Publication status | Published - 2010 |
Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)
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DECIGO and DECIGO pathfinder. / Ando, Masaki; Kawamura, Seiji; Seto, Naoki; Sato, Shuichi; Nakamura, Takashi; Tsubono, Kimio; Takashima, Takeshi; Funaki, Ikkoh; Numata, Kenji; Kanda, Nobuyuki; Tanaka, Takahiro; Ioka, Kunihito; Agatsuma, Kazuhiro; Aoyanagi, Koh Suke; Arai, Koji; Araya, Akito; Asada, Hideki; Aso, Yoichi; Chiba, Takeshi; Ebisuzaki, Toshikazu; Ejiri, Yumiko; Enoki, Motohiro; Eriguchi, Yoshiharu; Fujimoto, Masa Katsu; Fujita, Ryuichi; Fukushima, Mitsuhiro; Futamase, Toshifumi; Harada, Tomohiro; Hashimoto, Tatsuaki; Hayama, Kazuhiro; Hikida, Wataru; Himemoto, Yoshiaki; Hirabayashi, Hisashi; Hiramatsu, Takashi; Hong, Feng Lei; Horisawa, Hideyuki; Hosokawa, Mizuhiko; Ichiki, Kiyotomo; Ikegami, Takeshi; Inoue, Kaiki T.; Ishidoshiro, Koji; Ishihara, Hideki; Ishikawa, Takehiko; Ishizaki, Hideharu; Ito, Hiroyuki; Itoh, Yousuke; Izumi, Kiwamu; Kawano, Isao; Kawashima, Nobuki; Kawazoe, Fumiko; Kishimoto, Naoko; Kiuchi, Kenta; Kobayashi, Shiho; Kohri, Kazunori; Koizumi, Hiroyuki; Kojima, Yasufumi; Kokeyama, Keiko; Kokuyama, Wataru; Kotake, Kei; Kozai, Yoshihide; Kunimori, Hiroo; Kuninaka, Hitoshi; Kuroda, Kazuaki; Maeda, Kei Ichi; Matsuhara, Hideo; Mino, Yasushi; Miyakawa, Osamu; Miyamoto, Umpei; Miyoki, Shinji; Morimoto, Mutsuko Y.; Morisawa, Toshiyuki; Moriwaki, Shigenori; Mukohyama, Shinji; Musha, Mitsuru; Nagano, Shigeo; Naito, Isao; Nakamura, Kouji; Nakamura, Masahiro; Nakano, Hiroyuki; Nakao, Kenichi; Nakasuka, Shinichi; Nakayama, Yoshinori; Nakazawa, Kazuhiro; Nishida, Erina; Nishiyama, Kazutaka; Nishizawa, Atsushi; Niwa, Yoshito; Noumi, Taiga; Obuchi, Yoshiyuki; Ohashi, Masatake; Ohishi, Naoko; Ohkawa, Masashi; Okada, Kenshi; Okada, Norio; Oohara, Kenichi; Sago, Norichika; Saijo, Motoyuki; Saito, Ryo; Sakagami, Masaaki; Sakai, Shin Ichiro; Sakata, Shihori; Sasaki, Misao; Sato, Takashi; Shibata, Masaru; Shinkai, Hisaaki; Somiya, Kentaro; Sotani, Hajime; Sugiyama, Naoshi; Suwa, Yudai; Suzuki, Rieko; Tagoshi, Hideyuki; Takahashi, Fuminobu; Takahashi, Kakeru; Takahashi, Keitaro; Takahashi, Ryutaro; Takahashi, Ryuichi; Takahashi, Tadayuki; Takahashi, Hirotaka; Akiteru, Takamori; Takano, Tadashi; Taniguchi, Keisuke; Taruya, Atsushi; Tashiro, Hiroyuki; Torii, Yasuo; Toyoshima, Morio; Tsujikawa, Shinji; Tsunesada, Yoshiki; Ueda, Akitoshi; Ueda, Ken Ichi; Utashima, Masayoshi; Wakabayashi, Yaka; Yagi, Kent; Yamakawa, Hiroshi; Yamamoto, Kazuhiro; Yamazaki, Toshitaka; Yokoyama, Jun'Ichi; Yoo, Chul Moon; Yoshida, Shijun; Yoshino, Taizoh; Sun, Ke Xun.
In: Classical and Quantum Gravity, Vol. 27, No. 8, 084010, 2010.Research output: Contribution to journal › Article › peer-review
}
TY - JOUR
T1 - DECIGO and DECIGO pathfinder
AU - Ando, Masaki
AU - Kawamura, Seiji
AU - Seto, Naoki
AU - Sato, Shuichi
AU - Nakamura, Takashi
AU - Tsubono, Kimio
AU - Takashima, Takeshi
AU - Funaki, Ikkoh
AU - Numata, Kenji
AU - Kanda, Nobuyuki
AU - Tanaka, Takahiro
AU - Ioka, Kunihito
AU - Agatsuma, Kazuhiro
AU - Aoyanagi, Koh Suke
AU - Arai, Koji
AU - Araya, Akito
AU - Asada, Hideki
AU - Aso, Yoichi
AU - Chiba, Takeshi
AU - Ebisuzaki, Toshikazu
AU - Ejiri, Yumiko
AU - Enoki, Motohiro
AU - Eriguchi, Yoshiharu
AU - Fujimoto, Masa Katsu
AU - Fujita, Ryuichi
AU - Fukushima, Mitsuhiro
AU - Futamase, Toshifumi
AU - Harada, Tomohiro
AU - Hashimoto, Tatsuaki
AU - Hayama, Kazuhiro
AU - Hikida, Wataru
AU - Himemoto, Yoshiaki
AU - Hirabayashi, Hisashi
AU - Hiramatsu, Takashi
AU - Hong, Feng Lei
AU - Horisawa, Hideyuki
AU - Hosokawa, Mizuhiko
AU - Ichiki, Kiyotomo
AU - Ikegami, Takeshi
AU - Inoue, Kaiki T.
AU - Ishidoshiro, Koji
AU - Ishihara, Hideki
AU - Ishikawa, Takehiko
AU - Ishizaki, Hideharu
AU - Ito, Hiroyuki
AU - Itoh, Yousuke
AU - Izumi, Kiwamu
AU - Kawano, Isao
AU - Kawashima, Nobuki
AU - Kawazoe, Fumiko
AU - Kishimoto, Naoko
AU - Kiuchi, Kenta
AU - Kobayashi, Shiho
AU - Kohri, Kazunori
AU - Koizumi, Hiroyuki
AU - Kojima, Yasufumi
AU - Kokeyama, Keiko
AU - Kokuyama, Wataru
AU - Kotake, Kei
AU - Kozai, Yoshihide
AU - Kunimori, Hiroo
AU - Kuninaka, Hitoshi
AU - Kuroda, Kazuaki
AU - Maeda, Kei Ichi
AU - Matsuhara, Hideo
AU - Mino, Yasushi
AU - Miyakawa, Osamu
AU - Miyamoto, Umpei
AU - Miyoki, Shinji
AU - Morimoto, Mutsuko Y.
AU - Morisawa, Toshiyuki
AU - Moriwaki, Shigenori
AU - Mukohyama, Shinji
AU - Musha, Mitsuru
AU - Nagano, Shigeo
AU - Naito, Isao
AU - Nakamura, Kouji
AU - Nakamura, Masahiro
AU - Nakano, Hiroyuki
AU - Nakao, Kenichi
AU - Nakasuka, Shinichi
AU - Nakayama, Yoshinori
AU - Nakazawa, Kazuhiro
AU - Nishida, Erina
AU - Nishiyama, Kazutaka
AU - Nishizawa, Atsushi
AU - Niwa, Yoshito
AU - Noumi, Taiga
AU - Obuchi, Yoshiyuki
AU - Ohashi, Masatake
AU - Ohishi, Naoko
AU - Ohkawa, Masashi
AU - Okada, Kenshi
AU - Okada, Norio
AU - Oohara, Kenichi
AU - Sago, Norichika
AU - Saijo, Motoyuki
AU - Saito, Ryo
AU - Sakagami, Masaaki
AU - Sakai, Shin Ichiro
AU - Sakata, Shihori
AU - Sasaki, Misao
AU - Sato, Takashi
AU - Shibata, Masaru
AU - Shinkai, Hisaaki
AU - Somiya, Kentaro
AU - Sotani, Hajime
AU - Sugiyama, Naoshi
AU - Suwa, Yudai
AU - Suzuki, Rieko
AU - Tagoshi, Hideyuki
AU - Takahashi, Fuminobu
AU - Takahashi, Kakeru
AU - Takahashi, Keitaro
AU - Takahashi, Ryutaro
AU - Takahashi, Ryuichi
AU - Takahashi, Tadayuki
AU - Takahashi, Hirotaka
AU - Akiteru, Takamori
AU - Takano, Tadashi
AU - Taniguchi, Keisuke
AU - Taruya, Atsushi
AU - Tashiro, Hiroyuki
AU - Torii, Yasuo
AU - Toyoshima, Morio
AU - Tsujikawa, Shinji
AU - Tsunesada, Yoshiki
AU - Ueda, Akitoshi
AU - Ueda, Ken Ichi
AU - Utashima, Masayoshi
AU - Wakabayashi, Yaka
AU - Yagi, Kent
AU - Yamakawa, Hiroshi
AU - Yamamoto, Kazuhiro
AU - Yamazaki, Toshitaka
AU - Yokoyama, Jun'Ichi
AU - Yoo, Chul Moon
AU - Yoshida, Shijun
AU - Yoshino, Taizoh
AU - Sun, Ke Xun
PY - 2010
Y1 - 2010
N2 - A space gravitational-wave antenna, DECIGO (DECI-hertz interferometer Gravitational wave Observatory), will provide fruitful insights into the universe, particularly on the formation mechanism of supermassive black holes, dark energy and the inflation of the universe. In the current pre-conceptual design, DECIGO will be comprising four interferometer units; each interferometer unit will be formed by three drag-free spacecraft with 1000 km separation. Since DECIGO will be an extremely challenging mission with high-precision formation flight with long baseline, it is important to increase the technical feasibility before its planned launch in 2027. Thus, we are planning to launch two milestone missions. DECIGO pathfinder (DPF) is the first milestone mission, and key components for DPF are being tested on ground and in orbit. In this paper, we review the conceptual design and current status of DECIGO and DPF.
AB - A space gravitational-wave antenna, DECIGO (DECI-hertz interferometer Gravitational wave Observatory), will provide fruitful insights into the universe, particularly on the formation mechanism of supermassive black holes, dark energy and the inflation of the universe. In the current pre-conceptual design, DECIGO will be comprising four interferometer units; each interferometer unit will be formed by three drag-free spacecraft with 1000 km separation. Since DECIGO will be an extremely challenging mission with high-precision formation flight with long baseline, it is important to increase the technical feasibility before its planned launch in 2027. Thus, we are planning to launch two milestone missions. DECIGO pathfinder (DPF) is the first milestone mission, and key components for DPF are being tested on ground and in orbit. In this paper, we review the conceptual design and current status of DECIGO and DPF.
UR - http://www.scopus.com/inward/record.url?scp=77950840284&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=77950840284&partnerID=8YFLogxK
U2 - 10.1088/0264-9381/27/8/084010
DO - 10.1088/0264-9381/27/8/084010
M3 - Article
AN - SCOPUS:77950840284
VL - 27
JO - Classical and Quantum Gravity
JF - Classical and Quantum Gravity
SN - 0264-9381
IS - 8
M1 - 084010
ER -