LISA interferometry - art. no. 626826

被引：0
|
作者：
Mueller, Guido [1 ]
机构：
[1] Univ Florida, Dept Phys, Gainesville, FL 32611 USA
来源：
Advances in Stellar Interferometry Pts 1 and 2 | 2006年 / 6268卷
关键词：
LISA; interferometry; gravitational wave; TDI;
D O I：
10.1117/12.670353
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
The Laser Interferometer Space Antenna (LISA) is a joint NASA/ESA space mission aimed to detect gravitational waves in the 3.10(-5) to 1 Hz frequency range. Expected sources for LISA include super massive black hole mergers (SMBH), galactic neutron star and white dwarf binaries, and extreme mass ratio inspirals (EMRI). The three LISA spacecraft will travel in a heliocentric orbit trailing or leading earth by about 20 degrees. The distance between the spacecraft will be about 5 million km or 16 s light travel time. Laser interferometry will measure the distance with pm/root Hz accuracy. This report focuses on the technology for LISA interferometry.
引用
收藏
页码：26826 / 26826
页数：10
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