Stochastic gravitational waves backgrounds: a probe for inflationary and non-inflationary cosmology
arXiv:hep-ph/9912480 · doi:10.1142/9789812792129_0024
Abstract
Physical scenarios, leading to highly energetic stochastic gravitational waves backgrounds (for frequencies ranging from the Hz up to the GHz) are examined. In some cases the typical amplitude of the logarithmic energy spectrum can be even eight orders of magnitude larger than the ordinary inflationary prediction. Scaling violations in the frequency dependence of the energy density of the produced gravitons are discussed.
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