학술논문

The Japanese space gravitational wave antenna-DECIGO
Document Type
Article
Author
Kawamura, SeijiNakamura, TakashiAndo, MasakiSeto, NaokiTsubono, KimioNumata, KenjiTakahashi, RyuichiNagano, ShigeoIshikawa, TakehikoMusha, MitsuruUeda, Ken-ichiSato, TakashiHosokawa, MizuhikoAgatsuma, KazuhiroAkutsu, TomotadaAoyanagi, Koh-sukeArai, KojiAraya, AkitoAsada, HidekiAso, YoichiChiba, TakeshiEbisuzaki, ToshikazuEriguchi, YoshiharuFujimoto, Masa-KatsuFukushima, MitsuhiroFutamase, ToshifumiGanzu, KatsuhikoHarada, TomohiroHashimoto, TatsuakiHayama, KazuhiroHikida, WataruHimemoto, YoshiakiHirabayashi, HisashiHiramatsu, TakashiIchiki, KiyotomoIkegami, TakeshiInoue, Kaiki TIoka, KunihitoIshidoshiro, KojiItoh, YousukeKamagasako, ShogoKanda, NobuyukiKawashima, NobukiKirihara, HiroyukiKiuchi, KentaKobayashi, ShihoKohri, KazunoriKojima, YasufumiKokeyama, KeikoKozai, YoshihideKudoh, HideakiKunimori, HirooKuroda, KazuakiMaeda, Kei-ichiMatsuhara, HideoMino, YasushiMiyakawa, OsamuMiyoki, ShinjiMizusawa, HiromiMorisawa, ToshiyukiMukohyama, ShinjiNaito, IsaoNakagawa, NoriyasuNakamura, KoujiNakano, HiroyukiNakao, KenichiNishizawa, AtsushiNiwa, YoshitoNozawa, ChoetsuOhashi, MasatakeOhishi, NaokoOhkawa, MasashiOkutomi, AkiraOohara, KenichiSago, NorichikaSaijo, MotoyukiSakagami, MasaakiSakata, ShihoriSasaki, MisaoSato, ShuichiShibata, MasaruShinkai, HisaakiSomiya, KentaroSotani, HajimeSugiyama, NaoshiTagoshi, HideyukiTakahashi, TadayukiTakahashi, HirotakaTakahashi, RyutaroTakano, TadashiTanaka, TakahiroTaniguchi, KeisukeTaruya, AtsushiTashiro, HiroyukiTokunari, MasaoTsujikawa, ShinjiTsunesada, YoshikiYamamoto, KazuhiroYamazaki, ToshitakaYokoyama, Jun'ichiYoo, Chul-MoonYoshida, ShijunYoshino, Taizoh
Source
Classical and Quantum Gravity; April 2006, Vol. 23 Issue: 8 pS125-S131, 7p
Subject
Language
ISSN
02649381; 13616382
Abstract
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 pre-conceptual 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.