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|Title:||Second-generation laser interferometry for gravitational wave detection: ACIGA progress|
|Citation:||Classical and Quantum Gravity, 2001; 18(19):4121-4126|
|Publisher:||IOP Publishing Ltd|
|D E McClelland, S M Scott, M B Gray, D A Shaddock, B J Slagmolen, A Searle, D G Blair, L Ju, J Winterflood, F Benabid, M Baker, J Munch, P J Veitch, M W Hamilton, M Ostermeyer, D Mudge, D Ottaway and C Hollitt|
|Abstract:||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.|
|Rights:||© 2001 IOP Publishing|
|Appears in Collections:||Physics publications|
Environment Institute publications
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