Laser interferometry for the Big Bang Observer

被引：305
|
作者：
Harry, Gregory M.
Fritschel, Peter
Shaddock, Daniel A.
Folkner, William
Phinney, E. Sterl
机构：
[1] MIT, LIGO Lab, Cambridge, MA 02139 USA
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[3] CALTECH, Pasadena, CA 91125 USA
来源：
CLASSICAL AND QUANTUM GRAVITY | 2006年 / 23卷 / 15期
关键词：
D O I：
10.1088/0264-9381/23/15/008
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Big Bang Observer is a proposed space-based gravitational-wave detector intended as a follow on mission to the Laser Interferometer Space Antenna ( LISA). It is designed to detect the stochastic background of gravitational waves from the early universe. We discuss how the interferometry can be arranged between three spacecraft for this mission and what research and development on key technologies are necessary to realize this scheme.
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页码：4887 / 4894
页数：8
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