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Relic Gravitational Waves and Their Detection

Identifieur interne : 000A16 ( Main/Exploration ); précédent : 000A15; suivant : 000A17

Relic Gravitational Waves and Their Detection

Auteurs : P. Grishchuk [Royaume-Uni, Russie]

Source :

RBID : ISTEX:952C319CD3ACA4A3B90FB18213C916C784E639C8

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:


Links toward previous steps (curation, corpus...)


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