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 language | English |
|---|---|
| Pages (from-to) | 4121-4126 |
| Number of pages | 6 |
| Journal | Classical and Quantum Gravity |
| Volume | 18 |
| Issue number | 19 |
| DOIs | |
| Publication status | Published - 7 Oct 2001 |