The Detectability of Relic (Squeezed) Gravitational Waves by Laser Interferometers

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dc.creatorGrishchuk, L. P.
dc.date1998-10-17
dc.date1999-01-15
dc.date.accessioned2026-07-07T03:32:44Z
dc.date.available2026-07-07T03:32:44Z
dc.descriptionIt is shown that the expected amplitudes and specific correlation properties of the relic (squeezed) gravitational wave background may allow the registration of the relic gravitational waves by the first generation of sensitive gravity-wave detectors.
dc.descriptionmodifications to emphasize work's independence of the existing disagreement regarding inflationary prediction of infinitely large density perturbations for spectral slope n=1; revtex, 7 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/9810055
dc.identifierhttp://arxiv.org/abs/gr-qc/9810055
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36342
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleThe Detectability of Relic (Squeezed) Gravitational Waves by Laser Interferometers
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