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Japanese large-scale interferometers

delete2002-03-12
delete22
PRE
AI
K
K. Kuroda *
M
M. Ohashi
S
S. Miyoki
H
Hideki Ishizuka
C
C. Taylor
K
Kazuhiro Yamamoto
V
V. P. Mitrofanov
M
M.-K. Fujimoto
S
Seiji Kawamura
R
Ryutaro Takahashi
T
Toshitaka Yamazaki
K
K. Arai
D
D Tatsumi
M
Mitsuhiro Fukushima
S
S. Sato
T
T. Shintomi
A
A. Yamamoto
T
T. Suzuki
Y
Y. Saito
T
T. Haruyama
N
N. Sato
Y
Y. Higashi
T
Takashi Uchiyama
T
T. Tomaru
K
K. Tsubono
M
Masaki Ando
K
Kenji Numata
K
K-I Ueda
H
Hitoki Yoneda
K
K. Nakagawa
M
M. Musha
N
N. Mio
S
Shigenori Moriwaki
K
K. Somiya
A
A Araya
N
Nobuyuki Kanda
S
S. Telada
M
Misao Sasaki
H
Hideyuki Tagoshi
T
T. Nakamura
T
Takahiro Tanaka
K
K Ohara
DOI:10.1088/0264-9381/19/7/302delete
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摘要

摘要

En 中文
The objective of the TAMA 300 interferometer was to develop advanced technologies for kilometre scale interferometers and to observe gravitational wave events in nearby galaxies. It was designed as a power-recycled Fabry-Perot-Michelson interferometer and was intended as a step towards a final interferometer in Japan. The present successful status of TAMA is presented. TAMA forms a basis for LCGT (large-scale cryogenic gravitational wave telescope), a 3 km scale cryogenic interferometer to be built in the Kamioka mine in Japan, implementing cryogenic mirror techniques. The plan of LCGT is schematically described along with its associated RD.
Keyword:
GRAVITATIONAL-WAVE TELESCOPE
MECHANICAL QUALITY FACTOR
LASER-INTERFEROMETER
DETECTORS
MIRROR
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期刊

Classical and Quantum Gravity 封面图
Classical and Quantum Gravity
IF:
3.7
论文数:
1.3W
被引数:
3.0W

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