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Power recycling in the Garching 30 m prototype interferometer for gravitational-wave detection

MPS-Authors

Schnier,  D.
Max Planck Society;

Mizuno,  J.
Max Planck Society;

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

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

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Rüdiger,  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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Schrempel,  M.
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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PLA_225_1997_210.pdf
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Citation

Schnier, D., Mizuno, J., Heinzel, G., Lück, H., Rüdiger, A., Schilling, R., et al. (1997). Power recycling in the Garching 30 m prototype interferometer for gravitational-wave detection. Physics Letters. A, 225(4-6), 210-216. doi:10.1016/S0375-9601(96)00893-6.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0012-CB51-4
Abstract
Experimental realization of power recycling in an interferometer with 30 m arm-length and suspended optical components has been achieved. The power-recycling factor was about 300, corresponding to a light power of more than 100 W impinging on the beam splitter. A new concept was used to acquire simultaneous lock of the power-recycling cavity to resonance and of the Michelson phase difference to a dark fringe.