A study on motion reduction for suspended platforms used in gravitational wave detectors

Author:

Koehlenbeck Sina M.ORCID,Mow-Lowry Conor M.,Bergmann Gerald,Kirchoff Robin,Koch Philip,Kühn Gerrit,Lehmann Johannes,Oppermann Patrick,Wöhler Janis,Wu David S.

Abstract

AbstractWe report a reduction in motion for suspended seismic-isolation platforms in a gravitational wave detector prototype facility. We sense the distance between two seismic-isolation platforms with a suspension platform interferometer and the angular motion with two optical levers. Feedback control loops reduce the length changes between two platforms separated by $$11.65\,\textrm{m}$$ 11.65 m to $$10\,\mathrm {pm\,Hz}^{-1/2}$$ 10 pm Hz - 1 / 2 at $$100\,\textrm{mHz}$$ 100 mHz , and the angular motion of each platform is reduced to $$1\,\mathrm {nrad\, Hz}^{-1/2}$$ 1 nrad Hz - 1 / 2 at $$100\,\textrm{mHz}$$ 100 mHz . As a result, the length fluctuations in a suspended optical resonator on top of the platforms is reduced by three orders of magnitude. This result is of direct relevance to gravitational wave detectors that use similar suspended optics and seismic isolation platforms.

Funder

Deutsche Forschungsgemeinschaft

International Max Planck Research School (IMPRS) on Gravitational Wave Astronomy

Max Planck Institute for Gravitational Physics

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

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