The status of DECIGO
Creators
- Sato, Shuichi1
- Kawamura, Seiji2
- Ando, Masaki3
- Tsubono, Kimio3
- Nakazawa, Kazuhiro3
- Agatsuma, Kazuhiro3
- Nakamura, Takashi4
- Araya, Akito5
- Funaki, Ikkoh6
- Sakai, Shin-ichiro6
- Takashima, Takeshi6
- Ioka, Kunihito7
- Kanda, Nobuyuki8
- Moriwaki, Shigenori9
- Musha, Mitsuru10
- Numata, Kenji11
- Seto, Naoki12
- Arai, Koji12
- Tanaka, Takahiro13
- Aoyanagi, Koh-suke14
- and others
- 1. Faculty of Science and Engineering, Hosei University, kajinocho, Tokyo 184-8584 (Japan)
- 2. Institute for Cosmic Ray Research, The University of Tokyo, Chiba 277-8582 (Japan)
- 3. Department of Physics, The University of Tokyo, Tokyo 113-0033 (Japan)
- 4. Department of Physics, Kyoto University, Kyoto 606-8502 (Japan)
- 5. Earthquake Research Institute, The University of Tokyo, Tokyo 113-0032 (Japan)
- 6. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), Kanagawa 229-8510 (Japan)
- 7. Institute of Particle and Nuclear Studies, High Energy Accelerator Research Organization (KEK), Ibaraki 305-0801 (Japan)
- 8. Department of Physics, Osaka City University, Osaka 558-8585 (Japan)
- 9. Department of Advanced Materials Science, The University of Tokyo, Chiba 277-8561 (Japan)
- 10. Institute for Laser Science, The University of Electro-Communications, Tokyo 182-8585 (Japan)
- 11. NASA Goddard Space Flight Center, Code 663, 8800 Greenbelt Rd., Greenbelt, MD20771 (United States)
- 12. National Astronomical Observatory Japan, Osawa 2-21-1, Tokyo 181-8588 (Japan)
- 13. Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502 (Japan)
- 14. Department of Physics, Waseda University, Tokyo, 169-8555 (Japan)
Description
DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) is the planned Japanese space gravitational wave antenna, aiming to detect gravitational waves from astrophysically and cosmologically significant sources mainly between 0.1 Hz and 10 Hz and thus to open a new window for gravitational wave astronomy and for the universe. DECIGO will consists of three drag-free spacecraft arranged in an equilateral triangle with 1000 km arm lengths whose relative displacements are measured by a differential Fabry-Perot interferometer, and four units of triangular Fabry-Perot interferometers are arranged on heliocentric orbit around the sun. DECIGO is vary ambitious mission, we plan to launch DECIGO in era of 2030s after precursor satellite mission, B-DECIGO. B-DECIGO is essentially smaller version of DECIGO: B-DECIGO consists of three spacecraft arranged in an triangle with 100 km arm lengths orbiting 2000 km above the surface of the earth. It is hoped that the launch date will be late 2020s for the present.. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1742-6596/840/1/012010Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 840
- Journal Issue
- 1
- Journal Page Range
- [8 p.]
- ISSN
- 1742-6596
Conference
- Title
- 11. international LISA symposium
- Dates
- 5-9 Sep 2016
- Place
- Zurich (Switzerland)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 49019318
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ANTENNAS; ASTRONOMY; ASTROPHYSICS; DRAG; FABRY-PEROT INTERFEROMETER; GRAVITATIONAL WAVE DETECTORS; GRAVITATIONAL WAVES; LENGTH; ORBITS; PRECURSOR; SATELLITES; SPACE; SPACE VEHICLES; SUN; UNIVERSE
- Descriptors DEC
- DIMENSIONS; ELECTRICAL EQUIPMENT; EQUIPMENT; INTERFEROMETERS; MAIN SEQUENCE STARS; MEASURING INSTRUMENTS; PHYSICS; RADIATION DETECTORS; STARS; VEHICLES