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Searching for gravitational waves with LIGO

Patrick J. Sutton*, Kirk McKenzie, Karl Wette, David McClelland, Susan Scott, Malcolm Gray, Ping Lam

*Corresponding author for this work

    Research output: Contribution to journalConference articlepeer-review

    6 Citations (Scopus)

    Abstract

    The Laser Interferometer Gravitational-wave Observatory (LIGO) detectors have reached their design sensitivity, and searches for gravitational waves are ongoing. We highlight current attempts to detect various classes of signals. These include unmodelled sub-second bursts of gravitational radiation, such as from core-collapse supernovae and gamma-ray burst engines. Gravitational waves from isolated neutron stars and from the inspiral/merger of compact binary systems carry information about the bulk properties of black holes and neutron stars. A stochastic background of gravitational waves of cosmological origin would provide a unique view of conditions in the very early universe. We discuss current attempts to detect gravitational waves from these sources and comment on future prospects for these searches.

    Original languageEnglish
    Article number062024
    JournalJournal of Physics: Conference Series
    Volume110
    Issue number6
    DOIs
    Publication statusPublished - 30 Jun 2008
    EventEPS High Energy Particle Physics Conference, HEPP 2007 - Manchester, United Kingdom
    Duration: 19 Jul 200726 Jul 2007

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