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Part of the book series: NATO ASI Series ((ASIC,volume 511))

Abstract

The 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.

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Grishchuk, L.P. (1998). Signatures of Quantum Gravity in the Large-Scale Universe. In: Sánchez, N., Zichichi, A. (eds) Current Topics in Astrofundamental Physics: Primordial Cosmology. NATO ASI Series, vol 511. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5046-0_17

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  • DOI: https://doi.org/10.1007/978-94-011-5046-0_17

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6119-3

  • Online ISBN: 978-94-011-5046-0

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