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Processing the Signal Response of the Dulkyn Gravitational-Wave Detector

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Measurement Techniques Aims and scope

Abstract

Systems are considered for stabilizing the frequency and phase differences of the optical radiations in the resonators of the Dulkyn gravitational-wave detector laser system. Algorithms are proposed for processing the signal response of the detector to the action of gravitational radiation and these make it possible to observe a detected signal with a signal-to-noise ratio of the order of 50 when the signal-to-noise ratio at the output of the optical part of the system is lower than 10–7.

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Authors
  1. R. A. Daishev
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  2. S. F. Levin
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  3. Z. G. Murzakhanov
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  4. A. F. Skochilov
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Daishev, R.A., Levin, S.F., Murzakhanov, Z.G. et al. Processing the Signal Response of the Dulkyn Gravitational-Wave Detector. Measurement Techniques 44, 118–125 (2001). https://doi.org/10.1023/A:1010948921618

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  • DOI: https://doi.org/10.1023/A:1010948921618

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