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Matrix Heater in the Gravitational Wave Observatory GEO 600

MPG-Autoren
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Wittel,  Holger
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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

/persons/resource/persons206568

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

/persons/resource/persons40456

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

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Lough,  James
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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Schreiber,  Emil
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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

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1806.01652.pdf
(Preprint), 6MB

oe-26-18-22687.pdf
(Verlagsversion), 4MB

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Zitation

Wittel, H., Affeldt, C., Bisht, A., Doravari, S., Grote, H., Lough, J., et al. (2018). Matrix Heater in the Gravitational Wave Observatory GEO 600. Optics Express, 26(18), 22687-22697. doi:10.1364/OE.26.022687.


Zitierlink: https://hdl.handle.net/21.11116/0000-0001-8E2E-D
Zusammenfassung
Large scale laser interferometric gravitational wave detectors (GWDs), such
as GEO 600 require high quality optics to reach their design sensitivity. The
inevitable surface imperfections, inhomogeneities and light-absorption induced
thermal lensing in the optics can convert laser light from the fundamental mode
to unwanted higher order modes, and pose challenges to the operation and
sensitivity of the GWDs. Here we demonstrate the practical implementation of a
thermal projection system which reduces those unwanted effects via targeted
spatial heating of the optics. The thermal projector consists of 108
individually addressable heating elements which are imaged onto the beam
splitter of GEO 600. We describe the optimization of the spatial heating
profile and obtained results.