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Frequency response of Michelson- and Sagnac-based interferometers

MPG-Autoren
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Rüdiger,  Albrecht
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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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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372447.pdf
(Verlagsversion), 1013KB

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Zitation

Mizuno, J., Rüdiger, A., Schilling, R., Winkler, W., & Danzmann, K. (1997). Frequency response of Michelson- and Sagnac-based interferometers. Optics Communications, 138(4-6), 383-393. doi:10.1016/S0030-4018(97)00056-4.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-0013-5AA4-A
Zusammenfassung
The frequency response of Michelson- and Sagnac-based interferometers are evaluated and compared, considering the application for gravitational-wave detection. It is shown that Sagnac-based interferometers have some interesting features, but in general do not offer advantages over Michelson-based ones for the detection of gravitational waves.