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LISA interferometry:: recent developments
DOI:10.1088/0264-9381/23/8/S16.png)
Abstract
En 中文
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.
Keywords:
GRAVITATIONAL-WAVE MEASUREMENTS
LASER FREQUENCY STABILIZATION
ESA CORNERSTONE MISSION
SPACE ANTENNA
PHASE-LOCKING
ARM-LOCKING
PROGRESS
DELAY
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3.7
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1.3W
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3.0W
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