Inflation is studied in the context of induced gravity (IG) $\gamma {\sigma }^{2}R$, where $R$ is the Ricci scalar, $\sigma$ a scalar field and $\gamma$ a dimensionless constant, and diverse symmetry-breaking potentials $V(\sigma )$ are considered. In particular we compared the predictions for Landau-Ginzburg and Coleman-Weinberg type potentials and their possible generalizations with the most recent data. We find that large field inflation generally leads to fewer constraints on the parameters and the shape of the potential whereas small field inflation is more problematic and, if viable, implies more constraints, in particular, on the parameter $\gamma$. We also examined the reheating phase and obtained an accurate analytical solution for the dynamics of the inflaton and the Hubble parameter by using a multiple scale analysis. The solutions were then used to study the average expansion of the Universe, the average equation of state for the scalar field and both the perturbative and resonant decays of the inflaton field.

• Received 10 February 2010

DOI:https://doi.org/10.1103/PhysRevD.81.123505