The experimental plan of displacement- and frequency-noise free laser 
interferometer

Kokeyama, K.; Sato, S.; Nishizawa, A.; Kawamura, S.; Chen, Y.; Ward, R.; Pai, A.; Somiya, Kentaro; Sugamoto, A.

doi:10.1088/1742-6596/122/1/012022

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The experimental plan of displacement- and frequency-noise free laser interferometer

MPG-Autoren

Chen, Y.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Pai, A.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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

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Zitation

Kokeyama, K., Sato, S., Nishizawa, A., Kawamura, S., Chen, Y., Ward, R., et al. (2008). The experimental plan of displacement- and frequency-noise free laser interferometer. Journal of Physics: Conference Series, 122(1): 012022. doi:10.1088/1742-6596/122/1/012022.

Zitierlink: https://hdl.handle.net/11858/00-001M-0000-0013-1448-A

Zusammenfassung

We present the partial demonstration of displacement- and laser-noise free interferometer (DFI) and the next experimental plan to examine the complete configuration. A part of the full implementation of DFI has been demonstrated to confirm the cancellation of beamsplitter displacements. The displacements were suppressed by about two orders of magnitude. The aim of the next experiment is to operate the system and to confirm the cancellation of all displacement noises, while the gravitational wave (GW) signals survive. The optical displacements will be simulated by electro-optic modulators (EOM). To simulate the GW contribution to laser lights, we will use multiple EOMs.