Details
| Originalsprache | Englisch |
|---|---|
| Aufsatznummer | 1845001 |
| Seitenumfang | 16 |
| Fachzeitschrift | International Journal of Modern Physics D |
| Jahrgang | 28 |
| Ausgabenummer | 12 |
| Frühes Online-Datum | 4 Juni 2018 |
| Publikationsstatus | Veröffentlicht - 1 Sept. 2019 |
Abstract
DECi-hertz Interferometer Gravitational-wave Observatory (DECIGO) is a future Japanese space gravitational-wave antenna. The most important objective of DECIGO, among various sciences to be aimed at, is to detect gravitational waves coming from the inflation of the universe. DECIGO consists of four clusters of spacecraft, and each cluster consists of three spacecraft with three Fabry-Perot Michelson interferometers. As a pathfinder mission of DECIGO, B-DECIGO will be launched, hopefully in the 2020s, to demonstrate technologies necessary for DECIGO as well as to lead to fruitful multimessenger astronomy. B-DECIGO is a small-scale or simpler version of DECIGO with the sensitivity slightly worse than that of DECIGO, yet good enough to provide frequent detection of gravitational waves.
ASJC Scopus Sachgebiete
- Mathematik (insg.)
- Mathematische Physik
- Physik und Astronomie (insg.)
- Astronomie und Astrophysik
- Erdkunde und Planetologie (insg.)
- Astronomie und Planetologie
Zitieren
- Standard
- Harvard
- Apa
- Vancouver
- BibTex
- RIS
in: International Journal of Modern Physics D, Jahrgang 28, Nr. 12, 1845001, 01.09.2019.
Publikation: Beitrag in Fachzeitschrift › Übersichtsarbeit › Forschung › Peer-Review
}
TY - JOUR
T1 - Space gravitational-wave antennas DECIGO and B-DECIGO
AU - Kawamura, Seiji
AU - Nakamura, Takashi
AU - Ando, Masaki
AU - Seto, Naoki
AU - Akutsu, Tomotada
AU - Funaki, Ikkoh
AU - Ioka, Kunihito
AU - Kanda, Nobuyuki
AU - Kawano, Isao
AU - Musha, Mitsuru
AU - Nakazawa, Kazuhiro
AU - Sato, Shuichi
AU - Takashima, Takeshi
AU - Tanaka, Takahiro
AU - Tsubono, Kimio
AU - Yokoyama, Jun'ichi
AU - Agatsuma, Kazuhiro
AU - Aoyanagi, Koh Suke
AU - Arai, Koji
AU - Araya, Akito
AU - Aritomi, Naoki
AU - Asada, Hideki
AU - Aso, Yoichi
AU - Chen, Dan
AU - Chiba, Takeshi
AU - Ebisuzaki, Toshikazu
AU - Eguchi, Satoshi
AU - Ejiri, Yumiko
AU - Enoki, Motohiro
AU - Eriguchi, Yoshiharu
AU - Fujimoto, Masa Katsu
AU - Fujita, Ryuichi
AU - Fukushima, Mitsuhiro
AU - Futamase, Toshifumi
AU - Gondo, Rina
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 - Ishihara, Hideki
AU - Ishikawa, Takehiko
AU - Ishizaki, Hideharu
AU - Ito, Hiroyuki
AU - Itoh, Yousuke
AU - Izumi, Kiwamu
AU - Kanemura, Shinya
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 - Kuroyanagi, Sachiko
AU - Maeda, Kei Ichi
AU - Matsuhara, Hideo
AU - Matsumoto, Nobuyuki
AU - Michimura, Yuta
AU - Miyakawa, Osamu
AU - Miyamoto, Umpei
AU - Miyoki, Shinji
AU - Morimoto, Mutsuko Y.
AU - Morisawa, Toshiyuki
AU - Moriwaki, Shigenori
AU - Mukohyama, Shinji
AU - Nagano, Shigeo
AU - Nakamura, Kouji
AU - Nakano, Hiroyuki
AU - Nakao, Kenichi
AU - Nakasuka, Shinichi
AU - Nakayama, Yoshinori
AU - Nishida, Erina
AU - Nishizawa, Atsushi
AU - Niwa, Yoshito
AU - Noumi, Taiga
AU - Obuchi, Yoshiyuki
AU - Ohishi, Naoko
AU - Ohkawa, Masashi
AU - Okada, Kenshi
AU - Okada, Norio
AU - Okutomi, Koki
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 - Shibata, Kazunori
AU - Shimo-Oku, Ayumi
AU - Shinkai, Hisaaki
AU - Shoda, Ayaka
AU - Somiya, Kentaro
AU - Sotani, Hajime
AU - Suemasa, Aru
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, Hirotaka
AU - Akiteru, Takamori
AU - Takano, Tadashi
AU - Tanaka, Nobuyuki
AU - Taniguchi, Keisuke
AU - Taruya, Atsushi
AU - Tashiro, Hiroyuki
AU - Torii, Yasuo
AU - Toyoshima, Morio
AU - Tsujikawa, Shinji
AU - Ueda, Akitoshi
AU - Ueda, Ken Ichi
AU - Ushiba, Takafumi
AU - Utashima, Masayoshi
AU - Wakabayashi, Yaka
AU - Yagi, Kent
AU - Yamamoto, Kazuhiro
AU - Yamazaki, Toshitaka
AU - Yoo, Chul Moon
AU - Yoshida, Shijun
AU - Yoshino, Taizoh
N1 - Funding information: This research was supported by the Japan Aerospace Exploration Agency (JAXA), the Japan Society for the Promotion of Science (JSPS) and by the Research Center for the Early Universe (RESCEU) at the University of Tokyo.
PY - 2019/9/1
Y1 - 2019/9/1
N2 - DECi-hertz Interferometer Gravitational-wave Observatory (DECIGO) is a future Japanese space gravitational-wave antenna. The most important objective of DECIGO, among various sciences to be aimed at, is to detect gravitational waves coming from the inflation of the universe. DECIGO consists of four clusters of spacecraft, and each cluster consists of three spacecraft with three Fabry-Perot Michelson interferometers. As a pathfinder mission of DECIGO, B-DECIGO will be launched, hopefully in the 2020s, to demonstrate technologies necessary for DECIGO as well as to lead to fruitful multimessenger astronomy. B-DECIGO is a small-scale or simpler version of DECIGO with the sensitivity slightly worse than that of DECIGO, yet good enough to provide frequent detection of gravitational waves.
AB - DECi-hertz Interferometer Gravitational-wave Observatory (DECIGO) is a future Japanese space gravitational-wave antenna. The most important objective of DECIGO, among various sciences to be aimed at, is to detect gravitational waves coming from the inflation of the universe. DECIGO consists of four clusters of spacecraft, and each cluster consists of three spacecraft with three Fabry-Perot Michelson interferometers. As a pathfinder mission of DECIGO, B-DECIGO will be launched, hopefully in the 2020s, to demonstrate technologies necessary for DECIGO as well as to lead to fruitful multimessenger astronomy. B-DECIGO is a small-scale or simpler version of DECIGO with the sensitivity slightly worse than that of DECIGO, yet good enough to provide frequent detection of gravitational waves.
KW - Fabry-Perot Michelson interferometer
KW - Gravitational-wave
KW - inflation
KW - multimessenger astronomy
UR - http://www.scopus.com/inward/record.url?scp=85047964579&partnerID=8YFLogxK
U2 - 10.1142/S0218271818450013
DO - 10.1142/S0218271818450013
M3 - Review article
AN - SCOPUS:85047964579
VL - 28
JO - International Journal of Modern Physics D
JF - International Journal of Modern Physics D
SN - 0218-2718
IS - 12
M1 - 1845001
ER -