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• W2077490622 abstract "All first-generation large-scale gravitational wave detectors are operated at the dark fringe and use a heterodyne readout employing radio frequency (RF) modulation–demodulation techniques. However, the experience in the currently running interferometers reveals several problems connected with a heterodyne readout, of which phase noise of the RF modulation is the most serious one. A homodyne detection scheme (DC-readout), using the highly stabilized and filtered carrier light as a local oscillator for the readout, is considered to be a favourable alternative. Recently a DC-readout scheme has been implemented on the GEO 600 detector. We describe the results of first measurements and give a comparison of the performance achieved with homodyne and heterodyne readout. The implications of the combined use of DC-readout and signal recycling are considered." @default.
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• W2077490622 date "2009-02-17" @default.
• W2077490622 modified "2023-10-01" @default.
• W2077490622 title "DC-readout of a signal-recycled gravitational wave detector" @default.
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• W2077490622 doi "https://doi.org/10.1088/0264-9381/26/5/055012" @default.
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