Resonant gravitational wave antennas for stochastic background measurements

Details Resonant gravitational wave antennas for stochastic background measurements Resonant gravitational wave antennas for stochastic background measurements

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cqgra..14.2019a&link_type=abstract

Classical and Quantum Gravity, Volume 14, Issue 8, pp. 2019-2030 (1997).

Physics

16

Scientific paper

The sensitivity of a resonant gravitational wave (GW) antenna is calculated in terms of spectral density and frequency bandwidth. For a quantum-limited detector the bandwidth might reach values greater than 100 Hz, with a sensitivity to bursts of 0264-9381/14/8/005/img5. The spectral amplitude sensitivity for the Nautilus detector has been measured to be 0264-9381/14/8/005/img6 and its target value is 0264-9381/14/8/005/img7. Using two near-Nautilus detectors the GW stochastic background can be measured with a sensitivity, with respect to the critical density, of a few 0264-9381/14/8/005/img8 for an integration time of one year, as shown by simulations.

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