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SCATTERED LIGHT CONTROL IN ADVANCED LIGO
https://doi.org/10.1142/9789814374552_0312Cited by:0 (Source: Crossref)
Abstract: 
The phase shift of the light field scattered into the interferometer (IFO) optical mode from baffles, beam dumps, optical elements, or from the vacuum enclosure walls that have horizontal motion, will cause an apparent differential arm signal (noise) defined by the following expression1:
