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Q: Fachverband Quantenoptik und Photonik
Q 39: Posters: Quantum Optics and Photonics III
Q 39.14: Poster
Mittwoch, 11. März 2020, 16:30–18:30, Empore Lichthof
High-Q monolithic inertial sensors for seismic control in gravitational wave detectors — Sina Maria Köhlenbeck1,2, •Jonathan Carter1,2, Gerhard Heinzel1,2, and Oliver Gerberding3 — 1MPI für Gravitationsphysik, Callinstr. 38, 30167 Hannover — 2Institut für Gravitationsphysik, Leibniz Universität Hannover, Callinstr. 38, 30167 Hannover — 3Institut für Experimentalphysik, Universität Hamburg, Luruper Chaussee 149, 22761 Hamburg
Seismic noise is one of the noise sources limiting the performance of earth-bound interferometric gravitational wave detectors. To enhance the operation time of future detectors, new sensors for active stabilization of the mirror displacement are required. Commercial sensors are heavy, bulky and not vacuum compatible, where our design, based on an all-glass opto-mechanic oscillator with an interferometric read-out, resolves these constraints. The concept, design and first tests of the oscillators will be presented.