An adaptive sequential detector of gravitational radiation

Details An adaptive sequential detector of gravitational radiation An adaptive sequential detector of gravitational radiation

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990prib...33...14t&link_type=abstract

Priborostroenie (ISSN 0021-3454), vol. 33, Nov. 1990, p. 14-17. In Russian.

Physics

Gravitational Wave Antennas, Gravitational Waves, Radiation Sources, White Noise, Adaptive Control, Correlation Coefficients, Signal Processing

Scientific paper

The parameters of gravitational waves emitted by continuous sources of gravitational radiation, such as binaries and pulsars, remain practically constant for the earth observer. Long-term observation of gravitational waves against a noisy background is therefore possible using heterodyne detection techniques. Here, a hardware implementation is proposed for the adaptive sequential processing of the output signal of a heterodyne gravitational antenna. Error probabilities are determined.

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