Resonant sideband extraction: a new configuration for interferometric 
gravitational wave detectors

Mizuno, J.; Strain, Kenneth A.; Nelson, P. G.; Chen, J. M.; Schilling, Roland; Rüdiger, Albrecht; Winkler, Walter; Danzmann, Karsten

doi:10.1016/0375-9601(93)90620-F

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Resonant sideband extraction: a new configuration for interferometric gravitational wave detectors

MPS-Authors

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Strain, Kenneth A.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Schilling, Roland
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Rüdiger, Albrecht
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Winkler, Walter
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Danzmann, Karsten
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Citation

Mizuno, J., Strain, K. A., Nelson, P. G., Chen, J. M., Schilling, R., Rüdiger, A., et al. (1993). Resonant sideband extraction: a new configuration for interferometric gravitational wave detectors. Physics Letters A, 175(5), 273-276. doi:10.1016/0375-9601(93)90620-F.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0013-5C42-5

Abstract

We introduce a new Fabry-Perot based interferometric gravitational wave detector that, compared with previous designs, greatly decreases the amount of power that must be transmitted through optical substrates to obtain a given light power in its arms. This significantly reduces the effects of wavefront distortions caused by heating due to absorption in the optics, and allows an improved broadband sensitivity to be achieved.