The Japanese space gravitational wave antenna; DECIGO

S. Kawamura, M. Ando, T. Nakamura, K. Tsubono, T. Tanaka, I. Funaki, N. Seto, K. Numata, S. Sato, K. Ioka, N. Kanda, T. Takashima, K. Agatsuma, T. Akutsu, T. Akutsu, K. S. Aoyanagi, K. Arai, Y. Arase, A. Araya, H. AsadaY. Aso, T. Chiba, T. Ebisuzaki, M. Enoki, Y. Eriguchi, M. K. Fujimoto, R. Fujita, M. Fukushima, T. Futamase, K. Ganzu, T. Harada, T. Hashimoto, K. Hayama, W. Hikida, Y. Himemoto, H. Hirabayashi, T. Hiramatsu, F. L. Hong, H. Horisawa, M. Hosokawa, K. Ichiki, T. Ikegami, K. T. Inoue, K. Ishidoshiro, H. Ishihara, T. Ishikawa, H. Ishizaki, H. Ito, Y. Itoh, S. Kamagasako, N. Kawashima, F. Kawazoe, H. Kirihara, N. Kishimoto, K. Kiuchi, S. Kobayashi, K. Kohri, H. Koizumi, Y. Kojima, K. Kokeyama, W. Kokuyama, K. Kotake, Y. Kozai, H. Kudoh, H. Kunimori, H. Kuninaka, K. Kuroda, K. I. Maeda, H. Matsuhara, Y. Mino, O. Miyakawa, S. Miyoki, M. Y. Morimoto, T. Morioka, T. Morisawa, S. Moriwaki, S. Mukohyama, M. Musha, S. Nagano, I. Naito, N. Nakagawa, K. Nakamura, H. Nakano, K. Nakao, S. Nakasuka, Y. Nakayama, E. Nishida, K. Nishiyama, A. Nishizawa, Y. Niwa, M. Ohashi, N. Ohishi, M. Ohkawa, A. Okutomi, K. Onozato, K. Oohara, N. Sago, M. Saijo, M. Sakagami, S. I. Sakai, S. Sakata, M. Sasaki, T. Sato, M. Shibata, H. Shinkai, K. Somiya, H. Sotani, N. Sugiyama, Y. Suwa, H. Tagoshi, K. Takahashi, K. Takahashi, T. Takahashi, H. Takahashi, R. Takahashi, R. Takahashi, A. Takamori, T. Takano, K. Taniguchi, A. Taruya, H. Tashiro, M. Tokuda, M. Tokunari, M. Toyoshima, S. Tsujikawa, Y. Tsunesada, K. I. Ueda, M. Utashima, H. Yamakawa, K. Yamamoto, T. Yamazaki, J. Yokoyama, C. M. Yoo, S. Yoshida, T. Yoshino

Research output: Contribution to journalConference article

20 Citations (Scopus)

Abstract

DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. DECIGO is expected to open a new window of observation for gravitational wave astronomy especially between 0.1 Hz and 10 Hz, revealing various mysteries of the universe such as dark energy, formation mechanism of supermassive black holes, and inflation of the universe. The pre-conceptual design of DECIGO consists of three drag-free spacecraft, whose relative displacements are measured by a differential Fabry-Perot Michelson interferometer. We plan to launch two missions, DECIGO pathfinder and pre-DECIGO first and finally DECIGO in 2024.

Original languageEnglish
Article number032004
JournalJournal of Physics: Conference Series
Volume120
Issue numberPart 3
DOIs
Publication statusPublished - 2008 Jan 1
Event10th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2007 - Sendai , Japan
Duration: 2007 Sep 112007 Sep 15

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Fingerprint Dive into the research topics of 'The Japanese space gravitational wave antenna; DECIGO'. Together they form a unique fingerprint.

  • Cite this

    Kawamura, S., Ando, M., Nakamura, T., Tsubono, K., Tanaka, T., Funaki, I., Seto, N., Numata, K., Sato, S., Ioka, K., Kanda, N., Takashima, T., Agatsuma, K., Akutsu, T., Akutsu, T., Aoyanagi, K. S., Arai, K., Arase, Y., Araya, A., ... Yoshino, T. (2008). The Japanese space gravitational wave antenna; DECIGO. Journal of Physics: Conference Series, 120(Part 3), [032004]. https://doi.org/10.1088/1742-6596/120/3/032004