Stochastic background detection with gravitational-wave resonant detectors

Details Stochastic background detection with gravitational-wave resonant detectors Stochastic background detection with gravitational-wave resonant detectors

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cqgra..14.1487v&link_type=abstract

Classical and Quantum Gravity, Volume 14, Issue 6, pp. 1487-1490 (1997).

Physics

3

Scientific paper

A linearized version of the standard Wiener filter theory is used to calculate the sensitivity to an isotropic stochastic gravitational-wave background of the AURIGA - NAUTILUS pair of ultra-low-temperature bar detectors, near to operating in coincidence in Italy, obtaining a sensitivity of 0264-9381/14/6/015/img7. The addition of the VIRGO interferometric detector under construction in Italy improves the figure to 0264-9381/14/6/015/img8. We also consider the pair formed by VIRGO and one large mass spherical detector located in a nearby available site in Italy and a pair of spherical detectors located at the AURIGA and NAUTILUS sites that promise to achieve sensitivities of 0264-9381/14/6/015/img9.

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