Signatures of Quantum Gravity in the Large-Scale Universe

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dc.creatorGrishchuk, L. P.
dc.date1997-08-28
dc.date.accessioned2026-07-07T03:31:44Z
dc.date.available2026-07-07T03:31:44Z
dc.descriptionThe quantum gravity processes that have taken place in the very early Universe are probably responsible for the observed large-scale cosmological perturbations. The comparison of the theory with the detected microwave background anisotropies favors the conclusion that the very early Universe was not driven by a scalar field with whichever scalar field potential. At the same time, the observations allow us to conclude that there is a good probability of a direct detection of the higher frequency relic gravitational waves with the help of the advanced laser interferometers.
dc.description20 pages; crckapb.sty; contribution based on a talk given at the 4-th Colloque Cosmologie, Paris, June 1997
dc.identifierhttps://arxiv.org/abs/gr-qc/9708070
dc.identifierhttp://arxiv.org/abs/gr-qc/9708070
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35968
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectQuantum Physics
dc.titleSignatures of Quantum Gravity in the Large-Scale Universe
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