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Detecting Gravitational Waves from Quasi-Continuous Sources: the German-British Project GEO 600
Published online by Cambridge University Press: 12 April 2016
Abstract
At five sites, laser-interferometric detectors, with armlengths ranging from 0.3 to 4 km, are being built. By using advanced optical technologies early on, the German-British project GEO 600, although only intermediate in size (600 m), has good chances for a competitive sensitivity. Particularly the use of the so-called signal recycling technique will allow a search for faint sources of only slowly varying frequency (pulsars, close binaries). First science runs of GEO 600 are expected in the year 2001.
- Type
- Part 11. The Future – Where to go?
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 733 - 734
- Copyright
- Copyright © Astronomical Society of the Pacific 2000