Gravitational Waves in Conformal Flat Spaces

The purpose of this work is to describe the exact solutions of Einstein — Klein — Gordon equations for the inflationary model of the Universe in conformal flat spaces. We determined the geometry of space–time by means of Friedman — Robertson — Walker metric. The conformal factor defines the model of cosmological inflation. Moreover, we found the key cosmological parameters in the considered model and density of energy of the relic gravitational waves.

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