Relic Gravitational Waves and Their Detection
Identifieur interne : 000997 ( Main/Exploration ); précédent : 000996; suivant : 000998Relic Gravitational Waves and Their Detection
Auteurs : P. Grishchuk [Royaume-Uni, Russie]Source :
- Lecture Notes in Physics [ 0075-8450 ] ; 2001.
Abstract
Abstract: The range of expected amplitudes and spectral slopes of relic (squeezed) gravitational waves, predicted by theory and partially supported by observations, is within the reach of sensitive gravity-wave detectors. In the most favorable case, the detection of relic gravitational waves can be achieved by the cross-correlation of outputs of the initial laser interferometers in LIGO, VIRGO, GEO600. In the more realistic case, the sensitivity of advanced ground-based and space-based laser interferometers will be needed. The specific statistical signature of relic gravitational waves, associated with the phenomenon of squeezing, is a potential reserve for further improvement of the signal to noise ratio.
Url:
DOI: 10.1007/3-540-40988-2_9
Affiliations:
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