The cross-coupled interferometer for gravitational wave detection

Details The cross-coupled interferometer for gravitational wave detection The cross-coupled interferometer for gravitational wave detection

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cqgra..19.1997m&link_type=abstract

Classical and Quantum Gravity, Volume 19, Issue 7, pp. 1997-2004 (2002).

Physics

Scientific paper

The cross-coupled interferometer is a new design for interferometric gravitational wave detectors. Similar to the baseline gravitational wave detectors proposed for Advanced LIGO, it uses long-arm cavities in which the signal is generated. The signal fields are then extracted from the arm cavities with an additional cavity behind the long-arm cavities. The tuning of this signal extraction cavity and the parallel tuning of the signal recycling mirror can be used to optimize the peak frequency and the bandwidth of the detector independently. If we replace the signal recycling mirror by a small cavity, it is possible to amplify signals in two different frequency bands.

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