Searching for gravitational waves with LIGO
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,...
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| Published in | Journal of physics. Conference series Vol. 110; no. 6; p. 062024 |
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| Main Author | |
| Format | Journal Article |
| Language | English |
| Published |
Bristol
IOP Publishing
01.05.2008
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| Subjects | |
| Online Access | Get full text |
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| 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. |
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| AbstractList | 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. |
| ArticleNumber | 062024 |
| Author | Sutton, P J |
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| Cites_doi | 10.1086/382155 10.1103/PhysRevLett.98.111101 10.1103/PhysRevD.76.042001 10.1086/511329 |
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| DOI | 10.1088/1742-6596/110/6/062024 |
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| References | 12 14 Abbott B (9) 2007 Abbott B (13) 2007; 659 Abbott B (15) 2007 1 2 Abbott B (7) 2007 3 Abbott B (8) 2007 4 Abbott B (6) 2007 Abbott B (11) 2007 Kalogera (5) 2004; 601 10 |
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| SubjectTerms | Binary stars Black holes Gamma ray bursts Gamma rays Gravitational waves LIGO (observatory) Neutron stars Physics Searching Supernovae |
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| Title | Searching for gravitational waves with LIGO |
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