Paper
26 February 2003 Advanced interferometer configurations
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Abstract
We discuss optical methods which either enhance the signal response or reduce the quantum noise in a long baseline interferometric type detector of gravitational waves. We review current progress in the science and engineering of the different techniques and consider when they may be applicable to full scale interferometers.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David E. McClelland and Malcolm B. Gray "Advanced interferometer configurations", Proc. SPIE 4856, Gravitational-Wave Detection, (26 February 2003); https://doi.org/10.1117/12.459092
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Cited by 1 scholarly publication.
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KEYWORDS
Interferometers

Mirrors

Interference (communication)

Reflectivity

Sensors

Michelson interferometers

LIGO

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