Predictions of quantum gravity in inflationary cosmology: effects of the Weyl-squared term

摘要

A bstract We derive the predictions of quantum gravity with fakeons on the amplitudes and spectral indices of the scalar and tensor fluctuations in inflationary cosmology. The action is R + R ~(2)plus the Weyl-squared term. The ghost is eliminated by turning it into a fakeon, that is to say a purely virtual particle. We work to the next-to-leading order of the expansion around the de Sitter background. The consistency of the approach puts a lower bound ( m _(χ)> m _( ? )/4) on the mass m _(χ)of the fakeon with respect to the mass m _( ? )of the inflaton. The tensor-to-scalar ratio r is predicted within less than an order of magnitude (4/2 < N ~(2) r <12 to the leading order in the number of e -foldings N ). Moreover, the relation r ? –8 n _( T )is not affected by the Weyl-squared term. No vector and no other scalar/tensor degree of freedom is present.