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

D.E. Mcclelland, S.M. Scott, M.B. Gray, D.A. Shaddock, B.J. Slagmolen, A. Searle, David Blair, Li Ju, John Winterflood, Fetah Benabid, M. Baker, J. Munch, P.J. Veitch, M.W. Hamilton, M. Ostermeyer, D. Mudge, D. Ottaway, C. Hollitt

    Research output: Contribution to journalArticlepeer-review

    8 Citations (Web of Science)

    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.
    Original languageEnglish
    Pages (from-to)4121-4126
    JournalClassical and Quantum Gravity
    Volume18
    DOIs
    Publication statusPublished - 2001

    Fingerprint

    Dive into the research topics of 'Second-generation laser interferometry for gravitational wave detection: ACIGA progress'. Together they form a unique fingerprint.

    Cite this