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

Citation

McClelland, DE and Scott, SM and Gray, MB and Shaddock, DA and Slagmolen, BJ and Searle, A and Blair, DG and Ju, L and Winterflood, J and Benabid, F and Baker, M and Munch, J and Veitch, PJ and Hamilton, MW and Ostermeyer, M and Mudge, D and Ottaway, D and Hollitt, CP, Second-generation laser interferometry for gravitational wave detection: ACIGA progress, Classical and Quantum Gravity, 18, (19) pp. 4121-4126. ISSN 0264-9381 (2001) [Refereed Article]

DOI: doi:10.1088/0264-9381/18/19/321

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.

Item Details

Item Type:Refereed Article
Research Division:Physical Sciences
Research Group:Astronomical and Space Sciences
Research Field:Galactic Astronomy
Objective Division:Expanding Knowledge
Objective Group:Expanding Knowledge
Objective Field:Expanding Knowledge in the Physical Sciences
Author:Hollitt, CP (Mr Christopher Hollitt)
ID Code:35958
Year Published:2001
Web of Science® Times Cited:7
Deposited By:Physics
Deposited On:2005-09-21
Last Modified:2005-09-21
Downloads:0

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