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Volumn 23, Issue 8, 2006, Pages

The Japanese space gravitational wave antenna - DECIGO

(103)  Kawamura, Seiji a   Nakamura, Takashi b   Ando, Masaki c   Seto, Naoki d   Tsubono, Kimio c   Numata, Kenji e   Takahashi, Ryuichi a   Nagano, Shigeo f   Ishikawa, Takehiko g   Musha, Mitsuru h   Ueda, Ken Ichi h   Sato, Takashi i   Hosokawa, Mizuhiko f   Agatsuma, Kazuhiro c   Akutsu, Tomotada c   Aoyanagi, Koh Suke j   Arai, Koji a   Araya, Akito c   Asada, Hideki k   Aso, Yoichi c   more..


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EID: 33645527399     PISSN: 02649381     EISSN: 13616382     Source Type: Journal    
DOI: 10.1088/0264-9381/23/8/S17     Document Type: Conference Paper
Times cited : (705)

References (4)
  • 1
    • 37649031771 scopus 로고    scopus 로고
    • Possibility of direct measurement of the acceleration of the universe using 0.1 Hz band laser interferometer gravitational wave antenna in space
    • Seto N, Kawamura S and Nakamura T 2001 Possibility of direct measurement of the acceleration of the universe using 0.1 Hz band laser interferometer gravitational wave antenna in space Phys. Rev. Lett. 87 221103
    • (2001) Phys. Rev. Lett. , vol.87 , pp. 221103
    • Seto, N.1    Kawamura, S.2    Nakamura, T.3
  • 2
    • 84894015323 scopus 로고    scopus 로고
    • LISA: System and technology study report
    • ESA-SCI
    • 2000 LISA: System and Technology Study Report ESA document ESA-SCI
    • (2000) ESA Document
  • 3
    • 0036275897 scopus 로고    scopus 로고
    • Japanese large-scale interferometers
    • Kuroda K et al 2002 Japanese large-scale interferometers Class. Quantum Grav. 19 1237-45
    • (2002) Class. Quantum Grav. , vol.19 , pp. 1237-1245
    • Kuroda, K.1
  • 4
    • 0348207662 scopus 로고    scopus 로고
    • The gravitational wave background from cosmological compact binaries
    • Farmer A J and Phinney E S 2003 The gravitational wave background from cosmological compact binaries Mon. Not. R. Astron. Sot: 346 1197
    • (2003) Mon. Not. R. Astron. Sot , vol.346 , pp. 1197
    • Farmer, A.J.1    Phinney, E.S.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.