Theory of the detection of continuous gravitational radiation

Details Theory of the detection of continuous gravitational radiation Theory of the detection of continuous gravitational radiation

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jpsj...46..703f&link_type=abstract

Physical Society of Japan, Journal, vol. 46, Mar. 1979, p. 703-706. Research supported by the Mitsubishi Foundation.

Physics

4

Continuous Radiation, Gravitational Wave Antennas, Signal To Noise Ratios, Fourier Analysis, Q Factors, Sensitivity

Scientific paper

The sensitivity of resonant antennas for continuous gravitational radiation emitted from a coherent source is discussed. Fourier integration of the antenna output over an extended period results in a signal-to-noise ratio proportional to the quality factor of the antenna. This holds true even for an antenna with an extremely large quality factor which has an antenna decay time longer than the available observation time. The method of cold damping is useful in this connection, increasing the bandwidth of the antenna without losing its sensitivity.

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