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Optical sensitivities of current gravitational wave observatories at higher kHz, MHz and GHz frequencies
Roman Schnabel, Mikhail Korobko
GEO 600, Kagra, LIGO, and Virgo were built to observe gravitational waves at frequencies in the audio band, where the highest event rates combined with the largest signal to noise…
Observation of Noise Suppression during High-Efficiency Wavelength Doubling of Intense Quasi-Monochromatic Laser Light
Julian Gurs, Mikhail Korobko, Christian Darsow-Fromm +2
Ultra-stable, quasi-monochromatic laser light forms the basis for high-precision interferometric measurements, e.g. for observing gravitational waves and for time keeping with opti…
Coherent feedback for quantum expander in gravitational wave observatories
Niels Böttner, Joe Bentley, Roman Schnabel +1
The observation of gravitational waves from binary neutron star mergers offers insights into properties of extreme nuclear matter. However, their high-frequency signals in the kHz…