LISA interferometry:: recent developments

被引：33
|
作者：
Heinzel, G.
Braxmaier, C.
Danzmann, K.
Gath, P.
Hough, J.
Jennrich, O.
Johann, U.
Ruediger, A.
Sallusti, M.
Schulte, H.
机构：
[1] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany
[2] Leibniz Univ Hannover, D-30167 Hannover, Germany
[3] EADS Astrium GmbH, Immenstaad, Germany
[4] Univ Glasgow, Glasgow, Lanark, Scotland
[5] Estec, Noordwijk, Netherlands
来源：
CLASSICAL AND QUANTUM GRAVITY | 2006年 / 23卷 / 08期
关键词：
D O I：
10.1088/0264-9381/23/8/S16
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
LISA, the Laser Interferometer Space Antenna, will be launched by NASA and ESA in the 2014 timeframe and will be the first gravitational wave observatory for the many fascinating sources at low frequencies (down to 10(-5) Hz). One of the challenges is to perform precision laser interferometry over a distance of 5 million km. This paper describes recent developments in the interferometer design.
引用
收藏
页码：S119 / S124
页数：6
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