Second-generation laser interferometry for gravitational wave detection: ACIGA progress

Details Second-generation laser interferometry for gravitational wave detection: ACIGA progress Second-generation laser interferometry for gravitational wave detection: ACIGA progress

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cqgra..18.4121m&link_type=abstract

Classical and Quantum Gravity, Volume 18, Issue 19, pp. 4121-4126 (2001).

Astronomy and Astrophysics

Astronomy

6

Scientific paper

Reasonable event rate gravitational wave astronomy in the audio frequency detection band will require improving the sensitivity of long-baseline interferometer-based gravitational wave detectors currently under construction by at least a factor of 10. In this summary we report research being carried out by the Australian Consortium for Interferometric Gravitational Astronomy towards this end.

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