Consistency Relations for Large Field Inflation: Non-minimal Coupling

Takeshi Chiba, Kazunori Kohri

Published 2014-11-26Version 1

We derive the consistency relations for chaotic inflation model with a non-minimal coupling to gravity. For a quadratic or quartic potential in the limit of a small non-minimal coupling parameter $\xi$, we give consistency relations among spectral index $n_s$, the tensor-to-scalar ratio $r$ and the running of the spectral index $\alpha$. We find that unlike $r$, $\alpha$ is less sensitive to $\xi$. If $r<0.1$, then $\xi$ is constrained to $\xi<0$ and $\alpha$ is predicted to be $\alpha\simeq -8\times 10^{-4}$ for a quadratic or quartic potential. For general monomial potential, $\alpha$ is constrained in the range $-2.7\times 10^{-3}<\alpha< -6\times 10^{-4}$ as long as $|\xi|\leq 10^{-3}$ if $r<0.1$.