Principles of calculating alignment signals in complex resonant optical interferometers

被引:36
作者
Hefetz, Y
Mavalvala, N
Sigg, D
机构
[1] MIT,DEPT PHYS,CAMBRIDGE,MA 02139
[2] MIT,CTR SPACE RES,CAMBRIDGE,MA 02139
关键词
gravitational-wave observatories; laser interferometer; misalignment of Gaussian beams; LIGO; mode decomposition; optical cavities;
D O I
10.1364/JOSAB.14.001597
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
In the long-baseline laser interferometers that are now under construction to measure gravitational waves, the alignment of the optical components with respect to the incoming laser beam is crucial for maintaining maximum phase sensitivity. We present a basic formalism to calculate the effects of misalignment and beam distortions analytically in an arbitrarily complex optical system, including coupled cavities and Michelson interferometer configurations coupled with cavities. The electromagnetic field is decomposed into a superposition of higher-order Gaussian modes, while misaligned and distorting optical components along with free-space propagators are represented by matrix operators that act on the state vectors in this basis. We show how to deduce useful alignment signals generally, in order to design angular control systems. (C) 1997 Optical Society of America.
引用
收藏
页码:1597 / 1605
页数:9
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